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Opening / Closing Ceremony


Mon-31 Jul | 4:50 – 7:00 | Level 3 Nicoll Room
Opening & General Assembly

Fri-04 Aug | 4:15 – 6:00 | Level 3 Summit 1
Closing & Awards


Key Lectures


Mon-31 Jul | 8:15 - 10:00 | MR331
AS Distinguished Lecture

Speaker(s): Steven SHERWOOD, Climate Change Research Centre, The University of New South Wales

How can we Understand Small-Scale Atmospheric Processes Better?
Mon-31 Jul | 8:15 - 10:00 | MR331
AS Kamide Lecture

Speaker(s): Yan YU, Department of Atmospheric and Oceanic Sciences School of Physics, Peking University

Land-Atmosphere Feedbacks through Dust and Wildfire Processes
Mon-31 Jul | 8:15 - 10:00 | MR332
SE Distinguished Lecture

Speaker(s): Chong XU, National Institute of Natural Hazards, Ministry of Emergency Management

Probability Hazard Assessment of Earthquake-Triggered Landslides in China
Mon-31 Jul | 8:15 - 10:00 | MR333
IG Distinguished Lecture

Speaker(s): Yuei-An LIOU, National Central University

Hydrological Hazards and Environmental Issues by using Remote Sensing and Artificial Intelligence Techniques
Mon-31 Jul | 8:15 - 10:00 | MR333
IG Kamide Lecture

Speaker(s): Annie LAU, Geomorphic and Sedimentary Signatures of Storms and Tsunamis on Tropical Coastlines

Geomorphic and Sedimentary Signatures of Storms and Tsunamis on Tropical Coastlines
Mon-31 Jul | 8:15 - 10:00 | MR334
PS Distinguished Lecture

Speaker(s): Joseph MICHALSKI, University of Hong Kong

Geological Diversity and Strategic Exploration Potential of Lakes and Seas on Mars
Mon-31 Jul | 8:15 - 10:00 | MR334
PS Kamide Lecture

Speaker(s): William DUNN, University College London

X-ray Emissions from Magnetospheric Processes at Jupiter and Uranus
Mon-31 Jul | 12:20PM – 1:10PM | MR332
SE Distinguished Lecture

Speaker(s): Emma HILL, Nanyang Technological University

Approaching the 20th Anniversary of the Great 2004 Aceh-Andaman Earthquake and Tsunami: Lessons Learned on Tectonics, Hazards, and Resilience along the Sumatran Subduction Zone
Mon-31 Jul | 3:30 – 5:15 | Level 3 Nicoll
Axford Lecture

Speaker(s): John C. H. CHIANG, University of California, Berkeley

A Role of Orbital Eccentricity in Earth’s Seasonal Climate

Speaker(s): Mark John COSTELLO, Faculty of Biosciences and Aquaculture, Nord University

Global Ocean Biogeography - Latitude, Depth, Climate Change, 20°C Effect
Tue-01 Aug | 8:15 - 10:00 | MR308
OS Distinguished Lecture

Speaker(s): Hidekatsu YAMAZAKI, Shanghai Ocean University

How Planktonic Organisms Adapted to Turbulent Environments?
Tue-01 Aug | 8:15 - 10:00 | MR308
OS Kamide Lecture

Speaker(s): Yoko YAMAGAMI, Japan Agency for Marine-Earth Science and Technology

Arctic Sea-Ice Reduction and Gulf Stream Warming under Global Warming: Implication for the Further Development of GCMs
Tue-01 Aug | 8:15 - 10:00 | MR309
ST Distinguished Lecture

Speaker(s): Peng-Fei CHEN, Nanjing University

Diagnosis of the Coronal Magnetic Field Based on Imaging Observations
Tue-01 Aug | 8:15 - 10:00 | MR309
ST Kamide Lecture

Speaker(s): Kornyanat HOZUMI, National Institute of Information and Communications Technology (NICT), Catholic University of America, National Aeronautics and Space Administration (NASA)

Review of R&D on Ionosphere and Radio Propagation to Support a Stable Operation of Radio Infrastructure
Tue-01 Aug | 8:15 - 10:00 | MR310
BG Distinguished Lecture

Speaker(s): Prabir K. PATRA, Research Institute of Humanity and Nature

Co-Benefits of Reduction in Regional Emissions of Greenhouse Gases and Air Pollutants
Tue-01 Aug | 8:15 - 10:00 | MR310
BG Kamide Lecture

Speaker(s): Fiona Seh-Lin KENG, Universiti Malaya

Tropical Marine Algae: Halocarbon Emissions under Changing Environment
Tue-01 Aug | 8:15 - 10:00 | MR311
HS Distinguished Lecture

Speaker(s): Ashish SHARMA, University of New South Wales

The Implications of Global Warming on Dams, Reservoirs, the Probable Maximum Precipitation, and the Probable Maximum Flood
Tue-01 Aug | 8:15 - 10:00 | MR311
HS Kamide Lecture

Speaker(s): Xia WEI, National University of Singapore

Advances in Surrogate-Assistant Methods and Parallel Computing Techniques for Efficient Water Resources and Environmental Model Management
Wed-02 Aug | 8:30 - 10:00 | MR331
Axford Medal Lecture

Speaker(s): John CHURCH, University of New South Wales

What do we really know about 20th and 21st Century Sea-Level Change?
Wed-02 Aug | 8:30 - 10:00 | MR331
Wing Ip Medal Lecture

Speaker(s): Shigeo YODEN, Institute for Liveral Arts and Sciences, Kyoto University

Stratosphere-Troposphere Dynamical Coupling
Fri-04 Aug | 3:30 – 4:15 | Level 3 Summit 1
Axford Lecture

Speaker(s): Masato NAKAMURA, Japan Aerospace Exploration Agency

The Beginning of Venus Climate Orbiter AKATSUKI

Panels, Special Sessions & Workshops


Tue-01 Aug | 1:10 - 3:10 | MR335
Interdisciplinary Panel Session: Costal Issues - SOS (Support Ocean Sustainability)

Walk-in, Free of Charge

Invited Speakers: Htar Sandi NAING, Young Insurance
Thant Sin HAN, Young Insurance
Hsiao-Wen WANG, National Cheng-Kung University
Punyasloke BHADURY, Indian Institute of Science Education and Research Kolkata
Phaik Eem LIM, University of Malaya

Our geosciences affect our communities in many ways, especially the coastal communities. Our coastal environment has been degrading through beach erosion, plastic waste and other pollutants. Along with bleaching of reefs, these conditions have negatively impacted and sometimes endangered marine wildlife and coastal communities. Sea level changes are also affecting the coasts and coastal communities. Typically, scientists work in isolation, with little interaction with non-scientists. This panel will bring coastal scientists together with non-scientists (i.e. economists, engineers, public policy makers, insurers) working in industries affected by climate change in order to bridge this gap. We hope that this will lead to future collaborations and data exchanges for everyone’s benefits.

Tue-01 Aug | 3:30 - 5:15 | MR335
Interdisciplinary Panel Session: Climate Change Impact

Walk-in, Free of Charge

Invited Speakers: Htar Sandi NAING, Young Insurance
Thant Sin HAN, Young Insurance
Adam SWITZER, Nanyang Technological University
John CHURCH, Climate Change Research Centre; University of New South Wales
Steven SHERWOOD, Climate Change Research Centre; University of New South Wales

Recently climate change has been resulting in disastrous ways, impacting communities globally, through stronger storms, stronger cyclones, higher sea level, floods, droughts, wildfires, and other events. Typically, scientists work in isolation, with little interaction with non-scientists. This panel will bring climate scientists together with non-scientists (i.e. economists, engineers, public policy makers, insurers) working in industries affected by climate change in order to bridge this gap. We hope that this will lead to future collaborations and data exchanges for everyone’s benefits.

Wed-02 Aug | 10:20 - 12:20 | MR335
SS01 - Space Agency Perspectives on the Remote Sensing of the Earth

Walk-in, Free of Charge

The world’s space and/or environment agencies are making unprecedented contributions to studies of the Earth as an integrated system through a combination of new and existing observations that are providing an ever-expanding set of observations about the Earth’s interacting atmosphere, oceans, cryosphere, land surface, and interior. Advances in both operational and research satellites are making a significant impact on both scientific understanding and forecasting, thus contributing to societal benefits in many areas. In this session, a summary of status, accomplishments, and plans of several of the space agencies engaged in using the vantage point of space to study the Earth system and to turn the resulting knowledge into scientifically and societally useful products.

Conveners: * Richard ECKMAN, National Aeronautics and Space Administration
Yasuko KASAI, Tokyo Institute of Technology
Takehiko SATOH, Japan Aerospace Exploration Agency
Fee: Walk-in, Free of Charge
Invited Talks:

NASA EARTH SCIENCE DIVISION PROGRAM
Jack KAYE, Associate Director for Research National Aeronautics and Space Administration

FENGYUN METEOROLOGICAL SATELLITE PROGRAMS AND APPLICATIONS
Na XU, Director for National Satellite Meteorological Center

JAXA’S EARTH OBSERVATION MISSION
Shinichi SOBUE, ALOS-2 Project Manager Japan Aerospace Exploration Agency

Space-borne Atmospheric Environment Monitoring Program of Korea: GEMS and Beyond
Jhoon KIM, GEMS Principal Investigator Professor of Atmospheric Science Yonsei University

NOAA REMOTE SENSING SATELLITE OBSERVATIONS OF THE EARTH: DATA AND INFORMATION FOR SOCIETAL BENEFIT
Douglas HOWARD, Director of the Center for Satellite Applications and Research National Oceanic & Atmospheric Administration

Wed-02 Aug | 3:30 - 5:15 | MR335
SS02 - 20th Anniversary Special: AOGS Founders Session

Walk-in, Free of Charge

The development of the Asia Oceania Geosciences Society (AOGS) was initiated 20 years ago by a small group of broad-minded Earth and space scientists who felt the necessity of promoting scientific cooperation and dialogue in the Asia-Oceania region. From a fruitful partnership with Meeting Matters International (Meet Matt), the membership of our Singapore-based organization has grown from a modest beginning of 983 members made up of 48 nationalities to 11,367 members comprising 79 nationalities. Together with AGU and EGU, AOGS is now one of the three major international societies dedicated to geosciences, and the one with both the widest geographical distribution and the largest scientific population. The bottom-up approach in structure and scientific program is fundamental to the growth of our Society. The annual meetings in different Asia-Pacific cities outside Singapore are important in furthering capacity building and scientific networking. With the emergence of a new generation of geoscientists who have established lasting friendships and continue to cultivate the cooperative spirit of AOGS, we look forward to the next twenty years. Please join us for this colloquium, which will reflect back fondly on our Society's past achievements and discuss our ambitions ahead.

Conveners: * Chun-Chieh WU, National Taiwan University
Robin ROBERTSON, Xiamen University Malaysia
James TERRY, Zayed University
Fee: Walk-in, Free of Charge
Keynote Speakers: Wing-Huen IP, AOGS Founding President
National Central University

David HIGGITT, AOGS Vice-President (2020 to 2024)
Beijing Jiatong University (Lancaster University College)

Michel BLANC, Astronomer
Institute for Research in Astrophysics and Planetology
Thu-03 Aug | 8:15 - 12:20 | MR335
Workshop 1 - NASA's PACE Mission: Observation, Data and Opportunities for Ocean and Atmospheric Sciences

Register & Pay by 18 May 2023
SGD10 per person

Conveners: Laura LORENZONI, NASA Headquarters Science Mission Directorate (SMD)
Jeremy WERDELL, NASA Goddard Space Flight center (GSFC)
Participation: Up to 50 Pax
Fee: SGD10/person
Associated Sections: AS, BG, OS, PS, ST

The Plankton, Aerosol, Cloud, ocean Ecosystem (PACE) mission will continue NASA’s multi-decade record of satellite ocean color, cloud, and aerosol particle observations. Anticipated to launch in early 2024, PACE is a strategic climate continuity mission that will enable new insight into oceanographic and atmospheric responses to Earth's changing climate. PACE’s primary instrument is a global spectrometer that spans the ultraviolet to near-infrared region in 2.5 nm steps and also includes seven discrete shortwave infrared bands from 940 to 2260 nm. This leap in technology will enable improved understanding of aquatic ecosystems and biogeochemistry, as well as provide new information on phytoplankton community composition and improved detection of algal blooms. This, in combination with its aerosol and cloud measurements, will enable improved assessment of aerosol impacts on ocean biology and chemistry. PACE data is anticipated to provide new and improved applications such as better quantification of Earth’s energy budget, more accurate forecasting of harmful algal blooms, aid fisheries management and monitor ocean health. To ensure that PACE data is of the quality needed for its different applications, there are a number of validation activities planned post-launch. This session will discuss the scientific and technological advances that the PACE mission brings to the community, the opportunities that exist to support calibration/validation, including synergistic in situ and satellite measurements, and the breadth of applications that will be enabled by PACE data, in particular focused on the AOGS region. It is anticipated that the PACE instrument suite will substantially advance studies of global biogeochemistry, carbon cycle, and aerosols/clouds in the ocean-atmosphere system.

Interested parties may sign up via MARS Registration Form from 21 March 2023 onwards. Sign-ups will close when maximum participant capacity is reached.

Fri-04 Aug | 8:15 - 12:20 | MR335
Workshop 2 – Introduction to Satellite Validation using Worldwide AERONET Measurements

Register & Pay by 18 May 2023
SGD10 per person
Bring Own Computer

Conveners: Pawan GUPTA, NASA Goddard Space Flight Center (GSFC)
Robert LEVY, NASA Goddard Space Flight Center (GSFC)
Participation: 15 - 25 Pax
Participants are required to bring their own laptops
Fee: SGD10/person
Associated Sections: AS, PS, ST

The Moderate Resolution Imaging Spectroradiometer (MODIS) sensors aboard NASA’s Earth Observing Satellites (EOS) have been observing the earth-atmosphere system for more than two decades. Atmospheric aerosols (particulate matter) play an important role in the earth radiation budget and contribute to air pollution. Since its launch, the “dark-target” (DT) aerosol retrieval algorithm has been applied to MODIS to retrieve aerosol optical depth (AOD) and other aerosol properties on a global scale. The AOD data product has been extensively used for climate and air quality applications. The DT algorithm has been applied to a new generation of sensors such as Visible Infrared Imaging Radiometer Suite (VIIRS) on Suomi-NPP, and the Advanced Himawari and Baseline Imagers (AHI and ABI) on Himawari-8 and GOES-R. The application of a consistent algorithm on multiple Low Earth Orbiting (LEO) and GEOstationary (GEO) sensors is key for observing aerosols with high temporal and spatial resolution.

The AERONET (AErosol RObotic NETwork) project is a federation of ground-based remote sensing aerosol networks established by NASA and PHOTONS (PHOtométrie pour le Traitement Opérationnel de Normalisation Satellitaire; Univ. of Lille 1, CNES, and CNRS-INSU) and is greatly expanded by networks (e.g., RIMA, AeroSpan, AEROCAN, NEON, and CARSNET) and collaborators from national agencies, institutes, universities, individual scientists, and partners. For more than 25 years, the project has provided long-term, continuous, and readily accessible public domain database of aerosol optical, microphysical and radiative properties for aerosol research and characterization, validation of satellite retrievals, and synergism with other databases. The network imposes standardization of instruments, calibration, processing, and distribution.

The workshop will provide lectures and hands-on exercises. Lectures will be about fundamentals of satellite atmospheric aerosol datasets, introduction to AERONET datasets, and best research practices on spatiotemporal collocation of space and ground datasets for validation studies. Hands-on exercises will be geared towards accessing data, spatiotemporal collocation, and validating against ground measurements.
All activities will use free or open-source software tools such as Python.

Interested parties may sign up via MARS Registration Form from 21 March 2023 onwards. Sign-ups will close when maximum participant capacity is reached.


Field Trip


Wed-02 Aug | 1:30 - 5:00
Visit to Satellite Research Centre (SaRC)
Group Size: Maximum of 20 persons
Cost: SGD35/person (Covers 2-way transportation costs)
Tour Leader: Wee Seng LIM, Executive Director of Satellite Research Centre

Description
Come along with us to visit the birthplace of Singapore Designed Satellites at the Satellite Research Centre (SaRC). Since the 1st launch of XSAT microsatellite in 2011, SaRC has designed, built, tested and operated 10 satellites. Another 3x satellite will be launched in 2Q 2023 (you may witness the mission operation room of these 3x satellites lives). These satellites which range from 1U size (10cm x 10cm x 10cm) nanosatellite till 100+ kg microsatellite, will be communicating with NTU UHF/VHF, & S/X Band ground mission room automatically. In this lab visit, participants will get the exclusive opportunity to visit the 2 labs in SaRC:

  1. SaRC-II-Mission Room – This is where satellite will be operated in full automation. In here, NTU satellite and space program will be shared and presented in the mission room.
  2. SaRC-I-Satellite Integration Clean Room and Lab – This is where visitors can view SaRC’s satellites and the testing environment. A walkabout in the lab shall also introduce the various space science and technology research work from different NTU experts.

For more information on SaRC, you may visit:
https://www.ntu.edu.sg/sarc
https://www.ntu.edu.sg/sarc/research-capabilities/programmes

Timetable
1:30PM Assemble at SUNTEC Singapore Convention Centre (in front of Big Screen, Level 1)
2:00PM Arrive at Satellite Research Centre
2:00 – 4:30PM Lab Tour at Satellite Research Centre
4:30PM Transportation back to SUNTEC Singapore
Thu-03 Aug | 6:00 - 8:30
Visit to Centre of Climate Research Singapore (CCRS)
Group Size: Maximum of 20 persons
Cost: SGD35/person (Covers 2-way transportation costs)
Tour Leader: Thea TURKINGTON, Senior Research Scientist at the Centre for Climate Research Singapore

Description
The Centre for Climate Research Singapore (CCRS), part of the Meteorological Service Singapore, is celebrating its tenth anniversary in 2023. As a research center, CCRS aims to advance scientific understanding of how the tropical climate variability and change and its associated weather systems affects Singapore and the wider Southeast Asia Region.

During this visit, participants will get a chance to tour CCRS, learn about CCRS’ research, as well as watch the weather balloon launch (weather permitting). There will be a series of short presentations where participants will learn more about the Centre, including the latest developments of the in house SINGV model, used for weather forecasting up to climate change projections. The tour will end in the Upper Air Observatory, to check the progress (and information gathered from) the weather balloon.

This visit is targeted towards those who have a general interest in weather and/or climate and are interested to learn what is happening at CCRS.

For more information on SaRC, you may visit: http://ccrs.weather.gov.sg/

Timetable
6:00PM Assemble at SUNTEC Singapore Convention Centre (in front of Big Screen, Level 1)
6:30PM Arrive at the Centre for Climate Research Singapore
6:30 – 8:00PM Tour of the Centre for Climate Research Singapore
8:00PM Transportation back to SUNTEC Singapore
Fri-04 Aug | 8:30 - 12:00
Visit to Earth Observatory of Singapore (EOS)
Group Size: Maximum of 20 persons
Cost: SGD35/person (Covers 2-way transportation costs)
Tour Leader: Adam SWITZER, Principal Investigator at Earth Observatory of Singapore

Description
The Earth Observatory of Singapore (EOS) was created in 2008 with the mission to conduct fundamental research on earthquakes, volcanic eruptions, tsunamis and climate in and around Southeast Asia, toward safer and more sustainable societies. The research done at EOS allows for better understanding of the Earth so that more accurate predictions made can allow nations to adapt in order to minimize the impact. In this visit, participants will get a chance to have a tour of EOS and sit in a presentation to learn more about the different areas of research that EOS is heavily involved in.

For more information on SaRC, you may visit: https://earthobservatory.sg/

Timetable
8:30AM Assemble at SUNTEC Singapore Convention Centre (in front of Big Screen, Level 1)
9:00AM Arrive at Earth Observatory of Singapore
9:00 – 11:30AM Tour at Earth Observatory of Singapore
11:30AM Transportation back to SUNTEC Singapore
Sat-05 Aug | 5:30 - 1:30
Exploration of Coral Microatolls on St. John’s Island and Lazarus Island
Group Size: Maximum of 20 persons
Cost: SGD120/person
(Covers 2-way bus transportation, 2-way ferry and lunch)
Tour Leader: Aron MELTZNER, Principal Investigator of Earth Observatory of Singapore

Description
In a highly urbanized island state like Singapore, one can still find diverse marine biodiversity. One of such is the unique coral microatoll field sites present at the Southern Islands of Singapore – St. John’s Island and Lazarus Island. Coral microatolls are renowned for the precision of tracking relative sea level. These coral colonies grow near the base of the intertidal zone and are characterized by living outer perimeters with dead upper surfaces. The best microatolls have multiple concentric rings on their upper surfaces. Each ring that is produced follows a coral ‘die-down’ due to prolonged exposure at extreme low water. Differences in elevation of successive rings reflect changes in sea level as the coral grows. Field trip participants will get to visit fields of living and fossil microatolls that provide unique insights into Singapore relative sea level since the 20th century and in the mid-Holocene. Do come prepared for heavy rain and wet feet, but also bring along a sun hat.

Participants are advised to bring along the following for this trip:

  • Water Bottle (At least 2L)
  • Light Clothes
  • Rain Gear
  • Sunscreen
  • Sunglasses
  • Wide-brimmed hat/cap
  • Insect Repellent Comfortable Walking Shoes
  • Closed-Toed Water Shoes
Timetable*
05:00 AM Assemble at SUNTEC Singapore Convention Centre (in front of Big Screen, Level 1)
05:30 AM Arrive at Marina South Pier
06:00 AM Chartered boat to St. John’s Island
06:30 AM Arrival at Island and Walk to Microatoll Site
06:45 AM Introduction to Microatolls
07:00 AM Self-Exploration of Coral Microatoll Site & St. John’s Site
07:30 AM Scenic Walk to Lazarus Island Site
08:30 AM Intro to Lazarus West and Lazarus Bay Sites
09:00 AM Self-Exploration of Lazarus Microatoll site
10:00 AM Walk to Seringat Jetty/Lazarus Beach
10:45 AM Scenic meal by the beach (dry weather) or at Seringat Jetty (wet weather)
12:00 PM Walk Back to Jetty
12:30 PM Chartered Boat back to Mainland
01:00 PM Transport Back to SUNTEC Singapore Convention Centre

*Schedule subject to change depending on weather conditions

Tioman Island Scuba Dive Trip     ← Click Here
For more information, please email Robin Robertson: robin.robertson@xmu.edu.my

Atmospheric Sciences


Mon-31 Jul | 10:20 - 12:20 | MR309
AS04 - Impact of Fires on Air Quality and Climate: Processes, Field and Modeling Studies

Session Chair(s): Abdelwahid MELLOUKI, ICARE-CNRS/OSUC

AS04-A009 | Invited
Secondary Organic Aerosol Formation from Biomass Burning Derived Compounds

Lin DU#+
Shandong University

Biomass burning processes emit substantial amounts of compounds into the atmosphere, such as phenolic compounds and furans. These compounds have been recognized as potential precursors for secondary organic aerosols (SOA). Here, the kinetics of phenolic compounds and furans with hydroxyl radical (OH) were characterized in the gas phase and aqueous phase, and corresponding SOA formation mechanisms were determined. Phenolic compound with high water solubility can be involved in aqueous-phase reactions. Bimolecular aqueous-phase reaction rate constants of phenolic compounds with OH range from (3.8 ± 0.7) × 109 to (1.1 ± 0.3) × 1010 M−1 s−1. Aqueous-phase OH oxidation of phenolic compounds can form high-molecular-weight compounds, which are important SOA components. Hydroxylation of benzene ring occurs through OH addition, which could increase SOA oxidation degree. Furans are mainly oxidized by gas-phase OH to form SOA, and oxidation processes are influenced by different factors. Specifically, we observed a positive relationship between the furan SOA yields and NOx concentration, which is attributed to the production of low-volatility hydroxyl nitrates and dihydroxyl dinitrates. Increasing RH results in high OH concentration and enhances carbonyl-rich products condensation, thereby promoting furan SOA formation. In addition, changing SO2 level in the range of 0–80 ppb cause furan SOA yield to increase by 3.8%, while the presence of ∼50 ppb NH3 increased furan SOA yield by 3.3%. SO2 can lead to three C5-organosulfate formation, which may be precursors for the atmospheric C5-organosulfate. NH3 has a substantial promotion effect on the formation of light-absorbing nitrogen-containing products, which may be important brown carbon constituents. Our work provided mechanism insights about SOA formation from biomass burning-derived compounds, which is helpful for refining the representation of biomass burning-related SOA formation in models.


AS04-A012
Photochemical Air Pollution in Highly Urbanized Subtropical Regions: From Micro Environments to Urban-terrestrial-oceanic Interactions

Tao WANG#+
The Hong Kong Polytechnic University

Photochemical air pollution is a pressing environmental problem in the world’s urban and industrialized regions, including Hong Kong. Ozone and fine particulate are major air pollutants. In 2018, the Hong Kong Research Grants Council funded a comprehensive research project on the sources, atmospheric processes, and control strategy of photochemical pollution. This talk will give an overview of the project’s scope and key findings in the past 5 years. The major scientific achievements made thus far include the discoveries of the important roles of halogen atoms in air quality of polluted regions, the new source/production pathway of organic particulate matter from urban and biomass-burning emissions, and the complex responses of secondary air pollutants to emission controls. Based on the findings, the project has recommended additional measures to mitigate winter haze in north China and photochemical smog in south China.


AS04-A008
Saccharide in PM2.5 at the Remote Sites of Southwest China

Zhenzhen WANG, Di WU, Qing LI, Jianmin CHEN#+
Fudan University

Biomass burning (BB) and biogenic emissions of saccharides were investigated in 3 rural sites at Lincang, in the southwest border of China. PM2.5 samples were simultaneously collected on three mountaintop sites in Lincang: Datian, Dashu, and Yakoutian, which are located ∼ 300 km west of Kunming (the capital of Yunnan Province in China) and ∼ 120 km east from the Burma border. Five saccharide alcohols (glycerol, erythritol, inositol, arabitol, and mannitol) and five primary saccharides (fructose, glucose, mannose, sucrose, and trehalose), together with three anhydrosugars (levoglucosan, mannosan, and galactosan), were quantified by an improved high-performance anion-exchange chromatograph coupled with a pulsed amperometric detector. The total saccharides accounted for 1.6 ± 0.6 % in PM2.5. The anhydrosugars accounted for 48.5 % of total saccharides, among which levoglucosan was the most dominant species. The high level of levoglucosan was both attributed to the local BB activities and biomass combustion smoke transported from the neighboring regions of Southeast Asia (Myanmar) and the northern Indian subcontinent. The mono- or di-saccharides and sugar alcohols accounted for 24.9 ± 8.3 % and 26.6 ± 9.9 % of the total saccharides, respectively, and both proved to be mostly emitted by direct biogenic volatilization from plant material or surface soils rather than byproducts of polysaccharide breakdown during BB processes. Five sources of saccharides were resolved by non-negative matrix factorization (NMF) analysis, including BB, soil microbiota, plant senescence, airborne pollen, and plant detritus with contributions of 34.0 %, 16.0 %, 21.0 %, 23.7 %, and 5.3 %, respectively. The results provide information on the magnitude of levoglucosan and contributions of BB, as well as the characteristic of biogenic saccharides, at the remote sites of southwest China, which can be further applied to regional source apportionment models and global climate models.


AS04-A028
Ammonia Enhancement from Wildfire

Le KUAI1#+, Olga KALASHNIKOVA2, Karen CADY-PERERIA3, William PORTER4
1Jet Propulsion Laboratory - California Institute of Technology, 2California Institute of Technology, 3Atmospheric and Environmental Reserch, 4University of California, Riverside

Global ammonia is increasingly recognized as a significant contributor to fine particulate matter with a diameter smaller than 2.5 microns (PM2.5) due to the lack of mitigation policies for this species. Apart from agriculture fields, feedlots, and dairy farms, the more frequent wildfires during the dry season are contributing to rising emissions. Airborne and satellite instruments, such as Hyperspectral Thermal Emission Spectrometer (HyTES) and Cross-track Infrared Sounder (CrIS), have both detected and observed the ammonia plumes and enhancement from wildfires. Quantitative retrievals of HyTES observations at Gulch Fire in Arizona on July 3rd, 2014, suggest that the enhancement level is about 5 ppb, which is lower than both the emission from power plants (~10 ppb) and feedlots (~50 ppb) but ineligible. A further study with CrIS observations showed an unusual high level of ammonia at the Los Angeles area during the Bobcat fire in September 2020. A similar abnormal peak during the same month over Imperial Valley, a remote region southeast of Los Angeles basin. This may suggest the remote impact of wildfire emissions. Further modeling studies will help us to understand the process and contribution of wildfires in addition to local anthropogenic sources.


AS04-A003
Atmospheric Reactivity of VOCs Emitted from Fires: Kinetics and Degradation Mechanisms

Yangang REN1,2#+, Abdelwahid MELLOUKI3,4
1Research Center for Eco-Environmental Sciences, Chinese Academy of Sciences, 2University of Chinese Academy of Sciences, 3Mohammed VI Polytechnic University, Morocco, 4Shandong University

Volatile organic compounds (VOCs) are important species in the atmosphere which affect air quality and climate. Fire burning, including wildfires, agricultural fires, prescribed burning, and residential wood combustion, is the largest combustion-related source of VOCs to the atmosphere 1–3. In addition to CO, CO2 and CH4 hundreds or even thousands of VOCs are emitted from fire burning 4. Such emissions are likely to increase in the future, with the spatial extent, number, and severity of wildfires having increased markedly at the global scale in recent decades 5,6, this is predicted to continue as the climate warms 7,8. In general, VOCs from fire burning include non-methane hydrocarbons (NMHC, C2-C12), aromatics, oxygenated hydrocarbons, nitrogen containing compounds. In the atmosphere, the emitted VOCs could be oxidized by OH radical, NO3 radical and O3 to form photochemical oxidants (e.g. O3) and fine particles, which can cause severe air pollutions and damage human health. In this presentation, we review the knowledge about VOCs emissions from fires and discuss their atmospheric impacts on air quality and climate using the recent data from laboratory and fields studies. Reference:(1) Reid, J. S.; et al., Atmospheric Chem. Phys. 2005, 5 (3), 799–825. (2) Chen, J.; et al., Sci. Total Environ. 2017, 579, 1000–1034. (3) Granier, C.; et al., Clim. Change 2011, 109 (1–2), 163–190. (4) Koppmann, R.; von Czapiewski, K.; Reid, J. S. Atmospheric Chem. Phys. preprint; 2005. (5) Jolly, W. M.; Cochrane, M. A.; Freeborn, P. H.; et al., Nat. Commun. 2015, 6 (1), 7537. (6) Harvey, B. J. Proc. Natl. Acad. Sci. 2016, 113 (42), 11649–11650. (7) Krikken, F.; Lehner, F.; Haustein, K.; et al., Nat. Hazards Earth Syst. Sci. 2021, 21 (7), 2169–2179. (8) Lohmander, P. Cent. Asian J. Environ. Sci. Technol. Innov. 2020, 1 (5).


AS04-A010
The Gaseous Nitro-phenolic Compounds in the Background Air of South China: Source, Formation and Impacts on Air Quality

Zhe WANG#+
The Hong Kong University of Science and Technology

Nitro-phenolic compounds (NPs) have attracted increasing attention because of their health risks and impacts on visibility, climate and atmospheric chemistry. Both primary emission and secondary formation of NPs have been reported in recent studies, despite increasing research, the knowledge of the abundances, sources, atmospheric fates, and impacts remains incomplete, especially the gaseous species. In the present work, we conducted continuous measurement of eighteen gaseous NPs with a chemical ionization mass spectrometer at a background site in South China. Abundant NPs were observed in the continental outflows, with a total concentration of up to 122.1 pptv. A tracer method estimation showed that besides the direct emission from biomass burning, the secondary formation from the transported precursors contributed significantly to the observed NPs, with mono-NPs exhibiting photochemical daytime peaks and nighttime enrichments of di-NPs and Cl-substitute NPs. The budget analysis with a photochemical box model indicates that besides the ŸOH oxidations of aromatics, the NO3Ÿ oxidation also contributed significantly to the daytime mono-NPs, and was more dominant for the nocturnal formation of di-NPs. Photolysis was the main daytime sink of NPs, producing substantial HONO, and thus would largely influence atmospheric oxidation capacity in downwind and background regions. This study provides quantitative insights on the characteristics, formation and impacts of gaseous NPs in the continental outflow, and highlights the role of NO3Ÿ chemistry in the nitro-aromatics production that may facilitate regional pollution.


AS04-A017
Elemental Characterization of Atmospheric Fine Particles Released from Urban Fires in Hong Kong

Tao LI+, Hanzhe CHEN, Jianzhen YU#
The Hong Kong University of Science and Technology

Urban fires in densely populated areas can burn large amounts of manmade structures and synthetic materials, which potentially have different chemical characteristics to wildfire smoke. Realworld chemical composition data of urban fire plumes are vital for evaluating health impacts; however, they are rarely available. Online monitoring of trace elements in ambient PM2.5 at five sites throughout Hong Kong in 2021 provided unprecedented opportunities to observe the highly transient urban fire plumes. We observed sharp spikes for bromine (up to 0.65 µg m-3), chlorine (7.0 µg m-3), and certain metals such as lead (0.97 µg m-3), zinc (8.3 µg m-3), and copper (0.32 µg m-3) during four urban fires, which showed ~10–6,000 times higher concentrations than pre-fire periods. These elements behaved decreased concentrations with increased distance from the fire location due to transport and dilution, but their concentration ratios remained relatively constant. During fire-influenced hours, these elements exhibited 3–101 times enrichment relative to iron, an element that had no discernable increase in concentration. It was distinct to one monitored hill fire that was characterized of remarkably high enrichment of tracers for biomass burning, i.e., Rb (11.6) and K (6.5). Our results represent the first observation of the co-emissions of Br and certain metals from urban fires. Reactive bromine released from burning of the wide-spread brominated synthetic chemicals was suggested to facilitate the mobilization of toxic metals into the atmosphere. This mechanistic knowledge will help us understand the emissions and impacts of fires occurring in wildland urban interface zones. The work also calls attention to previously overlooked influence of urban fires-mobilized metals on human health and of bromine on atmospheric oxidizing capacity in megacities.


AS04-A005
Shedding Light on Ionic Strength Effects on Multiphase Reactions of Atmospheric Oxidants with Methoxyphenols as Proxies for Wood Smoke Pollution

Sasho GLIGOROVSKI#+
Chinese Academy of Sciences

Methoxyphenols represent one of the most abundant biomarker tracers for atmospheric wood smoke pollution. The reactions of atmospheric oxidants (ozone, OH, and NO2) with methoxyphenols can contribute to the formation of secondary organic aerosols (SOA). The ionic strength effect can affect the kinetics and products distribution within the aerosol deliquescent particles. However, the ionic strength effects on aqueous phase reactions of atmospheric relevance have been barely studied in the past. In this work, we have leveraged our knowledge on ionic strength (I) effects on the reactive uptakes of gas-phase oxidants ozone (O3) and nitrogen dioxide (NO2) on methoxyphenols by the well-known wetted wall flow tube technique. The obtained results highlight the importance of the ionic strength effect and suggest a much faster oxidation kinetics of methoxyphenols in aerosol deliquescent particles, compared to that in the dilute aqueous phase of cloud droplets; hence, the oxidative power of O3 and NO2 could be enhanced by one order of magnitude at elevated ionic strength, compared to a dilute aqueous phase. Considering the high concentrations of inorganic salts occurring in aerosol deliquescent particles during haze events, the oxidative power of different atmospheric oxidants might become considerably higher than that predicted for oxidation reactions in cloud droplets. The addition of SO42- typical for the liquid core of aerosol deliquescent particles increase the formation of condensed aromatics but also organosulfates (-OSO3H) arose upon ozone reactions with methoxyphemols. The addition of NO3- ions, substantially favors the formation of multi-core aromatic compounds through heterogeneous ozone processing of methoxyphenols. More importantly, the addition of NO3- ions favors the formation of nitrooxy (-ONO2) or oxygenated nitrooxy group of organonitrates, which are potential components of poorly characterized light absorbing organic matter (“brown carbon”) which in turn can affect the climate and air quality.


Mon-31 Jul | 10:20 - 12:20 | MR328
AS09 - The Science and Prediction of Heavy Precipitation and Floods

Session Chair(s): Yali LUO, Nanjing University of Information Science & Technology

AS09-A005 | Invited
Extreme Rainfall in Northern China in September 2021 Tied to Air–sea Multi-factors

Jianping LI#+, Yue SUN, Hao WANG, Ruize LI, Xinxin TANG
Ocean University of China

The September rainfall over Northern China (NC) in 2021 was the heaviest since 1961 and had unprecedented socioeconomic impacts. Holding the hypothesis that the drivers of extreme climate events usually contain extreme factors, we firstly propose the Ranking Attribution Method (RAM) to find the possible air–sea multi-factors responsible for this rainfall event. Via the atmospheric bridges of zonal-vertical circulation and Rossby wave energy propagation, the remote factors of warm sea surface temperature anomalies (SSTA) over the tropical Atlantic, cold SSTA over the tropical Pacific, Southern Annular Mode-like pattern in the Southern Hemisphere and North Pacific Oscillation-like pattern in the Northern Hemisphere jointly strengthened the Maritime Continent (MC) convection and Indian monsoon (IM). Through meridional-vertical circulation, the intensified MC convection enhanced the subtropical high over southern China and induced ascending motion over NC. The local factor of extreme air acceleration in the east Asian upper-level jet entrance region further anchored the location of the southwest-northeast rain belt. The strengthened IM and subtropical high over southern China induced considerable moisture transport to the rain belt via two moisture channels. The combined effect of these extreme dynamic and moisture conditions formed this unprecedented rainfall event. This study suggests that the RAM can effectively reveal the factors that contributed to this extreme rainfall event, which could provide a new pathway for a better understanding of extreme climate events.


AS09-A002
Real-time Nowcasting of Sudden Heavy Rainfall at Meso-γ-scale Using Neural Network and Dense 3D Observations by Precipitation Radar

Philippe BARON1#+, Kohei KAWASHIMA2, Hanado HIROSHI1, Seiji KAWAMURA1, Takeshi MAESAKA3, Shinsuke SATOH1, Tomoo USHIO2
1National Institute of Information and Communications Technology, 2Osaka University, 3National Research Institute for Earth Science and Disaster Resilience

Sudden heavy rainfalls occur more and more frequently in Japan during the summer. They are concentrated in restricted areas (typically of 5x5 km2) and can cause severe damage to infrastructure, often with casualties. The extrapolation of precipitation measured by radars is the conventional method for carrying out their nowcast in real time, i.e., short-term prediction on small spatial scales. However, the limit of predictability of such storms with current operational nowcasts is less than 10 minutes. This is due to the short lifetime (<15 minutes) of the individual convective cells causing the precipitation, as well as the limitations of nowcast models to properly account for the 3D nonlinear evolution of the cells. This presentation is about AI based real-time nowcasts of heavy precipitation on meso-γ-scale (2-20 km). The X-band Multi-Parameter Phased-Array Weather Radar (MP-PAWR) operating in Saitama prefecture (Japan) provides 3D observations of individual convective cells with a time resolution of 30 sec. A recurrent neural network is trained to detect the cells aloft and extrapolate them up to 10 minutes ahead. The neural network uses conventional Long Short-Term Memory (LSTM) units enhanced with 3D spatial convolutions and a training method developed for Generative Adversarial Network (GAN). It exploits high spatio-temporal resolution of the measurement up to an altitude of 8 km and the dual polarization. The model is trained with observations of 2020 and successfully predicts the onsets of sudden storms that occurred in 2018 and 2019. Its high prediction skills are illustrated with examples of typical storms where the operational system of Japan Meteorological Agency (JMA) or a conventional approach fails. A real-time system has been prepared to continuously analyze the observations of summer 2023 and we will present the first results.


AS09-A001
Merits of Ocean Prediction for Predicting Summer Heavy Rainfall in Japan

Yuya BABA#+
Japan Agency for Marine-Earth Science and Technology

Because of the progress of global warming, heavy rainfall intensity and the total amount are increasing in Japan. The heavy rainfall in Japan is frequently observed especially during summertime and occurred by various causes. One of the causes of the heavy rainfall is stagnated pressure pattern around Japan which guides the moisture transport from southwest toward Japan. With the pressure pattern as a background field, extratropical cyclone, front activity, and tropical cyclone induce the heavy rainfall. Since the air-sea interaction has influence on the formation of the pressure pattern, ocean prediction has a possibility to increase the prediction skill for heavy rainfall, and may extend the prediction lead time. Using regional atmospheric and coupled models, the impact of ocean prediction on summer heavy rainfall in Japan was examined for four events. It was found that the ocean prediction could extend the prediction lead time, when the heavy rainfall was caused by atmospheric rivers. Also, it increased prediction skill in the case of front-derived heavy rainfall. Further investigations showed that ocean prediction can provide better air-sea coupling regarding the Pacific high locating southeast of Japan, leading to provide better moisture transport from southwest of Japan. Analysis on reanalysis data indicates that the air-sea coupling around Japan is atmospheric feedback dominant region. Thus, the ocean prediction is necessary to consider the feedback from the atmosphere. Otherwise, the atmospheric feedback is neglected, and sea surface temperature prevails the atmospheric feedback as seen in tropics, then it causes unrealistic air-sea coupling and deteriorates the prediction. It is concluded that the ocean prediction contributes to increase prediction skill and can extend the lead time of heavy rainfall prediction.


AS09-A019
Numerical Investigation of the Effects of Boundary Layer Parameterization Schemes on Typhoon Meranti (1614) Landing Process

Yehong WANG#+, Yuchun ZHAO1,1
Xiamen Meteorological Bureau

To study the effects of different boundary layer schemes on the simulation of landing attenuation stage of typhoon Meranti (1614), a series of high-resolution (1.33 km) numerical tests were carried out using seven boundary layer parameterization schemes in the mesoscale numerical model WRF v3.8, namely, YSU, MYJ, QNSE, ACM2, UW, GBM, and Boulac, in terms of movement track, intensity, structure, rainfall, and near-surface physical variables. The results indicate the following. First, boundary layer schemes significantly influenced the simulation of typhoon Meranti’s track, intensity, and rainfall during its landing attenuation stage. Second, in the overall simulation of track, intensity, and precipitation of the typhoon, Boulac and MYJ schemes showed optimal results, in which the Boulac scheme was superior in simulating the typhoon track and precipitation and the MYJ scheme was superior in simulating typhoon intensity. The YSU and GBM schemes had the second best simulation results, whereas QNSE, UW, and ACM2 schemes had worse simulation performance. Moreover, the boundary layer schemes significantly differed in calculating the latent heat flux and sensible heat flux of near-surface layer, thereby affecting the simulation of typhoon track, intensity, and rainfall, leading to significantly different simulation results. The QNSE scheme resulted in an abnormally high latent heat flux, the MYJ and Boulac schemes resulted in the most modest values, and other schemes resulted in slightly smaller values. On the other hand, the QNSE scheme had a slightly higher sensible heat flux, the MYJ scheme showed the most modest one, and other schemes resulted in significantly smaller values. Finally, the boundary layer schemes significantly differed in the simulated thermal and dynamical structure of boundary layer, and Boulac scheme had the obvious advantages, particularly for the structure of boundary layer in daytime.


AS09-A020
Applying Optical Flow to Nowcasting Heavy Rainfall Over the Maritime Continent

Joseph SMITH#+
University of Leeds

The Maritime Continent (MC) regularly experiences powerful convective storms that produce intense rainfall. Often the intense rainfall leads to flooding and landslides and thus to widespread destruction. At short lead times (0-12 hours), numerical weather prediction (NWP) models show low skill in the MC for forecasting convective activity. Nowcasting aims to solve this issue by using alternative methods to NWP models to make more accurate and reliable predictions of convective activity from observations over this key timescale. Optical flow algorithms are one of the most effective nowcasting methods as they are able to accurately track clouds across observed image series and predict forward trajectories. Optical flow is generally applied to weather radar observations, however, the radar network over the MC is sparse and cannot penetrate the high mountainous regions. In this research, we present the results of applying the Lukas-Kanade optical flow algorithm to infrared satellite imagery to generate 1 – 6 hour lead time nowcasts of heavy-precipitation-producing storms over the MC. For evaluation of the nowcasts, we present a novel adaption of the fractional skill score to quantify how nowcast skill varies spatially and temporally across the MC domain. Overall, the results show that the Lukas-Kanade algorithm has good skill, outperforming a persistence forecast for all lead times and showing skill up to 6 hours on a 50 km spatial scale. Low skill is observed over the mountainous regions in the early afternoon due to the algorithm’s inability to predict convection initiation. Overnight, however, high skill is seen over the sea as the model is able to accurately predict the offshore propagation of storms. These results show that the Lukas-Kanade algorithm can effectively nowcast mature storms and, when analysed alongside the skill maps, has potential to be used in an operational nowcasting system for the MC.


AS09-A022
Development of the Geo-KOMPSAT Image Analysis in Detecting Precursors of Developing Heavy Rain Cloud in Summer Season

Kim DONG SU1#+, Ok Hee KIM1, Byunghyun SONG2, Hee Jung KANG2
1Korea Meteorological Administration, 2Researcher

The major precursor phenomena were derived for detecting torrential rain clouds by intuitively analyzing satellite images. There were 17 cases of torrential rains in 2020-2021 in South Korea. The precursor phenomena were derived for satellite images such as water vapor, RGB composite, and secondary outputs from the Geo-KOMPSAT. We summarized major 12 possible check lists of key precursors that could become torrential rain clouds.
1. Updraft zone in front of the boundary of the upper dry area of North pacific High
2. Updraft zone in front of the dry area due to the Low pressure trough
3. Compressed wet zone between the North-South dry zones
4. Warm advection accompanied by Low pressure in warm conveyor belt
5. Lower cumulus clouds from strong southwesterly flow
6. Cirrus cloud as divergent in the upper strong wind zone
7. Upper layer cold core
8. Low-pressure rotating clouds of upper, middle, and lower layers on the stationary front
9. Periodic upper-level wave inflow on the stationary front
10. The cooling rate of the developing convective cloud lasts less than -3℃/10minutes
11. Clouds thickness of 10 km or more
12. Heavy rainfall critical index of 30 mm/hr or higher
If six or more phenomena among the above 12 conditions are present, the clouds would be developed to cause heavy rainfall. In addition, more than 60 mm/hr of possible precipitation, a strong instability index, the speed of movement of the developed clouds, and terrain factors should be considered. It is necessary to prepare for intense rainfall in summer by considering a combination of topographical factors. Several dominant cases with satellite images and checklists were introduced. 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] (KMA2020-00120).


AS09-A023
Short-range Precipitation Forecasts from SINGV with a New Science Configuration

Boon Chong Peter HENG1#+, Jeff LO2
1Meteorological Service Singapore, 2Centre for Climate Research Singapore

The Meteorological Service Singapore (MSS) maintains and runs a convection-permitting tropical configuration of the Met Office Unified Model (UM) known as SINGV for weather forecasts and climate projections over the Western Maritime Continent. A new Regional Atmosphere and Land (RAL) science configuration that includes, among other changes, a multi-moment cloud microphysics scheme has been proposed for kilometre-scale UM simulations in the mid-latitudes as well as in the tropics. Short-range forecast experiments with SINGV show that, compared to the operational configuration, the new science configuration produces more coherent storm structures with broader stratiform regions and reduces the tendency to over-forecast (under-forecast) precipitation over land (sea). An objective evaluation of the precipitation forecasts reveals significant improvements in Fractions Skill Scores (FSS) across forecast lead times and rainfall thresholds. The new RAL science configuration is a significant step towards better precipitation forecasts in this region.


AS09-A026
Implementing Double Moment Microphysics Into the Met Office Unified Model for Operational Use

Paul FIELD1#, Kalli FURTADO2+, Adrian HILL1, Ben SHIPWAY1, Jonathan WILKINSON1, Annette MILTENBERGER3, Hamish GORDON4, Daniel GROSVENOR1, Kwinten VAN WEVERBERG5
1Met Office, 2Centre for Climate Research Singapore, 3Johannes Gutenberg University Mainz, 4University of Leeds, 5Ghent University

The Cloud AeroSol Interacting Microphysics (“CASIM”) is the new double moment cloud microphysics scheme that will be introduced into the Met Office operational regional model next year. Results will be shown for performance in the Tropics and the UK. We show comparisons against the currently operational single moment cloud microphysics and investigate the effects of different aerosol activation protocols for activating droplets from the environmental aerosols. In the Tropics, CASIM outperforms the single-moment microphysics as evident from improved comparison with radar derived precipitation rates. We demonstrate that these improvements derive, in part of improved representation of rain evaporation and sedimentation when two prognostic moments are used. CASIM is also used for regional climate projections, and we will show results from dynamical downscaling over China with a particular emphasis on temperature and precipitation extremes. 


Mon-31 Jul | 10:20 - 12:20 | MR329
AS02 - Climate Change and Tropical Climatic Hazards in Asia Oceania

Session Chair(s): Yuriy KULESHOV, Bureau of Meteorology

AS02-A015
WMO GPC LRFs Support for "Climate Information Services for Resilient Development Planning in Vanuatu"

Yuriy KULESHOV1,2#+
1Bureau of Meteorology, 2Royal Melbourne Institute of Technology University

Vanuatu is one of the world's most vulnerable countries to natural disasters. The main climate hazards for Vanuatu include tropical cyclones, heavy rainfall resulting in flooding, extended periods without rain causing drought, rising sea levels threatening coastal environments and property, as well as sea temperature increase and ocean acidification impacting highly valuable coastal ecosystems and resources (including coral reefs, seagrass and fisheries). Recognising urgency to assist Vanuatu with climate change adaptation, the Green Climate Fund provided support for "Climate Information Services for Resilient Development Planning in Vanuatu (Van-CIS-RDP)" project, which is named Van-KIRAP (Vanuatu Klaemet Infomesen blong Redy, Adapt mo Protekt) in local language. Van-KIRAP project helps to address the needs to strengthen Climate Information Services (CIS) in Vanuatu delivering climate science to support decision makers and communities in Vanuatu to prepare for and adapt to climate variability and change. World Meteorological Organization's Global Producing Centre for Long-Range Forecasts (WMO GPC LRFs) Melbourne hosted by the Australian Bureau of Meteorology disseminates sub-seasonal to seasonal (S2S) climate information from the Australian Community Climate Earth-System Simulator – Seasonal (ACCESS-S) on global, regional and national scales, including climate forecast products for Vanuatu. This presentation provides an overview of products for climate monitoring and ACCESS-S S2S products for climate prediction disseminated via WMO GPC LRFs, with emphasis on utilising them under Van-KIRAP project for production of Climate Outlook Bulletins for tourism, agriculture, and fisheries sectors.


AS02-A007
Record-breaking Rainfall Accumulations in Eastern China Produced by Typhoon In-fa (2021)

Xin HUANG1#+, Johnny CHAN2,3, Ruifen ZHAN4, Zifeng YU5,2, Rijin WAN6
1Shanghai Typhoon Institute, China Meteorological Administration, 2Asia-Pacific Typhoon Collaborative Research Center, 3City University of Hong Kong, 4Fudan University, 5Shanghai Typhoon Institute/China Meteorological Administration, 6China Meteorological Administration

Persistent heavy rainfall produced by western North Pacific (WNP) tropical cyclones (TCs) can lead to widespread flooding and landslides in Asian countries. On July 2021, unprecedent rainfall amount occurred when Typhoon Infa passed through the highly populated eastern China. While the associated synoptic features have been analyzed, the extreme characteristics and return periods of rainfall induced by In-fa remain unexplored. Analyses of rainfall data from a WNP TC database of the China Meteorological Administration (CMA) show that Typhoon In-fa not only produces record-breaking rainfall accumulations at individual surface stations, but generates unprecedent rainfall amounts for the whole area of eastern China. Quantitatively, 2, 4, 11, 24 and 55 stations are exposed to once in 200-, 100-, 50-, 20- and 10-year extreme TC rainfall accumulations, respectively, and total rainfall at 75 stations reaches a record high since 1980. Overall, the return period is up to 481 years for the total rainfall amount accumulated in eastern China during the 1980–2019 baseline. The extremely long rainfall duration is identified as key to the torrential rains in the Yangtze River Delta before In-fa changes its direction of movement from northwestward to northeastward, while the extreme rain rate plays a dominant role in the northern areas afterwards. Probabilities of occurrence of such an unprecedented TC rainfall event have increased in most (75%) of the eastern China during the period of 2000–2019 compared with those during 1980–1999. Our study highlights the likely increase in risk of extreme TC-induced rainfall accumulations which should be considered in disaster risk mitigation.


AS02-A011
Impact of the North Atlantic Sea Surface Temperature Tripole on the Northwestern Pacific Weak Tropical Cyclone Frequency

Rui JIN#+, Hui YU
Shanghai Typhoon Institute of China Meteorological Administration

Previous studies focused on the intense TCs in the central-southeastern western North Pacific (WNP), whose variability is intimately linked to El Niño-Southern Oscillation and extratropical sea surface temperature anomaly (SSTA) in the Pacific. Compared with them, weak TCs (WTCs) are more numerous and form further northwestward. The great number of WTCs and thereby the landfall cases may also cause huge damage to countries in Southeast Asia. However, their modulators are far from fully understood. Our research emphasizes the delayed impact of the early spring North Atlantic tripole SSTA (NAT) on the WTC formation frequency through the “capacitor” effect of sea ice (SIC) and SST in the Barents Sea. Detailed analysis indicates that a positive NAT may modulate an anomalous high in the Barents Sea-North Europe and decrease the local low cloud cover. Thus, more downward solar radiation tends to heat the local SST and decrease the SIC. This warmer Barents Sea could maintain through the typhoon season and excite a significant southeastward wave train, with several centers in the Arctic, Central Asia, and East Asia. The abnormal easterly to the south of the anticyclone in East Asia facilitates the cyclonic anomaly in the South China Sea, the Philippines, and the subtropical WNP, which reinforces the monsoon trough and favors the WTC formation there. A physical-based empirical model is developed for the WTC frequency, and hindcast is performed from 1979 to 2018. It shows the early spring NAT effectively improves the prediction skill for the WTC frequency, which can be considered as a crucial source of predictability for WTCs.


AS02-A008
Reversal of Tropical Cyclone Genesis Frequency Anomaly Over the Western North Pacific from Boreal Summer to Autumn

Yuhao CAI+, Song YANG#
Sun Yat-sen University

Tropical cyclones (TCs) over the western North Pacific (WNP) mainly occur in boreal summer and autumn. Using three best track datasets for 1979-2021, this study finds a significant inverse relationship between the relative TC genesis frequency (TCGF) during summer and that during autumn. This strong relationship is characterized with TC activity transitions from active (inactive) season in summer to inactive (active) season in autumn. That is, positive (negative) anomaly of TCGF in summer is followed negative (positive) anomaly in autumn. Such a reversal of TCGF anomaly is generally supported by the changes in large-scale environmental fields over the WNP from summer to autumn. Based on diagnostic analyses of TC genesis potential index, it is suggested that the mid-level relative humidity and vertical motions play major roles for the phase-transition of TCGF anomalies, followed by the secondary roles of low-level vorticity and mid-level meridional shear of zonal wind. Moist static energy budget analyses demonstrate that the phase reversal of climatological moist enthalpy advection by anomalous winds contributes to the phase transitions of anomalous vertical motion and relative humidity over the WNP. Seasonal evolution in sea surface temperature over the Indian Ocean is hypothesized to be associated with the phase transition of TCGF anomaly and corresponding large-scale environmental factors over the WNP.


AS02-A009
Arctic Sea Ice Promoting Seasonal Prediction Capability of the Early Autumn Tropical Cyclone Formation Frequency Over the Western North Pacific

Peng ZHANG#+
Fudan University

Seasonal prediction of tropical cyclone (TC) activity has been a hot research theme in the past decades. Usually, the tropical sea surface temperatures (SSTs) provide considerable predictability sources for the western North Pacific (WNP) TC activity. Here, we emphasized that the Chukchi-Beaufort (C-B) and Greenland (GL) sea ice variability is closely linked to the year-to-year variations of the early autumn WNP TC formation frequency (TCF). Observational and numerical evidence proved that the excessive C-B and GL sea ice sustains from August to the following early autumn and triggers the southeastward propagation of the Rossby wave trains originating from the Arctic across Western Eurasia (Okhotsk Sea) to the WNP. The resultant anomalous low pressure over WNP provides suitable environmental conditions for TC formation—the enhancement of the lower-level relative vorticity and water moisture, and the decrease of vertical wind shear. For the reduced sea ice, an opposite situation tends to emerge. The persistent combined sea ice signal makes it a physically meaningful precursor for TCF prediction. The cross-validated hindcast and independent forecast based on both the tropical SST and the Arctic sea ice precursors present that the TCF index is predicted with much higher correlation coefficients than those of the empirical models with only the tropical SST predictors. The results demonstrate that the Arctic sea ice truly promotes the seasonal prediction capability of the WNP TCF.


AS02-A003
Convection-permitting Simulations Reveal Robust Intensification of Tropical Cyclone Extreme Precipitation Due to Anthropogenic Warming

Minkyu LEE1#+, Seung-Ki MIN2, Dong-Hyun CHA3
1Korea Institute of Energy Research, 2Pohang University of Science and Technology, 3Ulsan National Institute of Science and Technology

Understanding how global warming affects tropical cyclone (TC) intensity and precipitation for target regions is essential to preparing for associated damages but detailed processes remain uncertain. This study provides a first quantification of anthropogenic influences on TC characteristics affecting South Korea using convection-permitting model (CPM) simulations (3 km resolution). For the observed four recent TCs that strongly affected South Korea, CPM simulations were performed under current (ALL) and pre-industrial conditions (NAT). The observed sea surface temperature and lateral boundary conditions were used for ALL while changes attributable to human influences (estimated using CMIP6 multimodel simulations) were removed from observed boundary conditions for NAT runs. ALL experiments captured the observed TC intensity and precipitation reasonably. After removing human influences, TC intensity and precipitation were reduced in NAT experiments. Importantly, areas with extreme precipitation (i.e., having precipitation larger than 150 mm) were found to expand by 16~37% in ALL compared to NAT, which was induced by an enhanced upward motion near the TC core and an increase of background water vapor in line with warming. Further, the role of increased moisture was found to become important as TC moves to mid-latitudes. This study provides new insights into how greenhouse warming can intensify TC-induced extreme precipitation over East Asia.


AS02-A013
Changes to Tropical Cyclone Tracks Over Southeast Asia in a Warming Climate

Andra GARNER1#+, Dhrubajyoti SAMANTA2, Mackenzie WEAVER1, Benjamin HORTON2,3
1Rowan University, 2Nanyang Technological University, 3Rutgers University

Tropical cyclone (TC) track characteristics in a changing climate remain uncertain. Here, we use downscaled simulations from nine Coupled Model Intercomparison Project Phase 6 (CMIP6) models to investigate the genesis, tracks, and termination of >64,000 synthetic TCs traveling within the Southeast Asia region from the historical era (1881-1900 CE) to the modern era (1991-2000 CE) to the future (2081-2100 CE). Under both a moderate emissions scenario (SSP2-4.5) and a high-emissions scenario (SSP5-8.5), TCs are more likely to form closer to major land masses, terminate farther inland, and move most slowly while over mainland Southeast Asia or in the Bay of Bengal from the historical era to future. Furthermore, TCs become more likely to intensify most quickly in locations near mainland Southeast Asia in the future compared to the historical era, and the rate at which TC maximum winds increase is amplified in the future under both of our modeled scenarios. Additionally, results suggest a northern shift in TC track locations in the northwest Pacific basin, as well as an increased tendency for TC tracks to traverse mainland Southeast Asia in the future compared to the historical era.


AS02-A018
Long-term Trends in Cyclogenesis Over North Indian Ocean and the Role of Equatorial Waves and MJO

Kiranmayi LANDU#+, Lokendar TIRUNAHARI
Indian Institute of Technology Bhubaneswar

Convectively coupled equatorial waves and Madden and Jullian Oscillations (MJO) are known to significantly impact cyclogenesis throughout the tropical ocean basins. Studies show that these waves can modulate cyclogenesis potential index, thus affecting the genesis frequency. Recent studies show that the frequency and intensity of cyclones forming over Arabian Sea and Bay of Bengal have undergone significant trends over the recent decades. In this study we explore the role of tropical intraseasonal oscillations and their long term variabiliity on the observed trends of cyclogenesis over Bay of Bengal and Arabian Sea for a period of 40 years from 1981 till 2020. Long term trends in the factors that determine genesis potential index are analyzed along with their relation to equatorial waves and MJO. The study shows that the trends in the wave modulated of the genesis parameters, namely, relative humidity at mid troposphere, vorticity, vertical wind shear and potential intensity, each play a different role in the observed trends in cyclogenesis for the two basins during pre and post monsoon seasons. The results give an insight into the importance of these subseasonal processes in modulating the long term changes in extreme events in addition to background climate change.


Mon-31 Jul | 10:20 - 12:20 | MR330
AS46 - Aviation Meteorology

Session Chair(s): Jung-Hoon KIM, Seoul National University

AS46-A011
Determining the Spatial Distribution of Turbulence Near Thunderstorms

Todd LANE1,2#+, Stacey HITCHCOCK1, Robert SHARMAN3, Stanley TRIER3, Wiebke DEIERLING3, Cameron HOMEYER4
1The University of Melbourne, 2ARC Centre of Excellence for Climate Extremes, 3National Center for Atmospheric Research, 4University of Oklahoma

Severe turbulence encounters can result in serious injuries and millions of dollars of operational costs to airlines. In addition to the turbulence generated within the storm, thunderstorms can induce turbulence in the surrounding clear air, which can extend large distances from the storm boundary due to gravity waves and other circulations. Using relatively limited datasets, past studies have indicated that severe turbulence can extend beyond the current federal guidelines for avoidance (20 mi/~32 km), but many questions remain. For example, 1) What is the spatial distribution of convection induced turbulence relative to individual storms? 2) What dynamical factors determine the spatial distribution? Now, extensive archives of operational radar data and automated eddy dissipation rate (EDR) reports from commercial aircraft present an opportunity for more detailed analysis. To address the above questions, we objectively identify thunderstorms in the GridRad hourly radar archive over the contiguous USA and compare them to automated turbulence reports over a period of 9 years (2009-2017). This analysis, based on millions of turbulence data points, is used to diagnose the risk of turbulence relative to storms.


AS46-A004
Using High Resolution Global Climate Models to Project Trends in Clear Air Turbulence Over the North Atlantic

Isabel SMITH1#+, Paul WILLIAMS1, Reinhard SCHIEMANN2,1
1University of Reading, 2National Centre for Atmospheric Science

Clear-air turbulence (CAT) has a large impact on the aviation sector. Our current understanding of how CAT may increase with climate change in future is largely based on simulations from CMIP3 and CMIP5 global climate models (GCMs). However, these models have now been superseded by high-resolution CMIP6 GCMs, which have grid lengths at which median individual turbulence patches may start to be resolved. Using a CMIP6 multi-model approach, projected CAT changes over the North Atlantic have been quantified. Twenty-one CAT diagnostics are used, to represent the uncertainties in CAT production mechanisms. Each diagnostic responds differently in time, but the majority display an increase in CAT between 1950 and 2050. These results refer to Northern Hemisphere (NH) CAT changes, particularly over the North Atlantic basin. Although NH winter is historically the most turbulent season, there is strong multi-model agreement that autumn and summer will have the greatest overall percentage increase in CAT frequency. Future NH summers are projected to become as turbulent as 1950 winters. Using the global-mean seasonal near-surface temperature as a comparative metric, with every of global near-surface warming, NH autumn, winter, spring, and summer are projected to have an average of 14%, 9%, 9%, and 14% more moderate CAT, respectively.


AS46-A006
Atmospheric Turbulence Estimated from High-resolution Operational Radiosonde Data and Comparison with In-situ Flight Observations

Han-Chang KO1+, Hye-Yeong CHUN1#, Jung-Hoon KIM2, Robert SHARMAN3
1Yonsei University, 2Seoul National University, 3National Center for Atmospheric Research

The one-third power of the energy dissipation rate (EDR) is calculated based on the Thorpe method using high vertical-resolution radiosonde data (HVRRD) at 68 operational stations in the United States for six years (2012–2017) observed at 00 and 12 UTC. The spatiotemporal distributions of HVRRD-derived EDR (HVRRD-EDR) are compared with those of in-situ flight EDR (flight-EDR) observed along main flight routes of commercial airlines over z=20–45 kft and within ±1 h centered at 00 and 12 UTC. Both datasets show similar seasonal variations, with the largest total occurrences in June–August (JJA) and the smallest in December–February (DJF). Vertically, both ratios of light-or-greater (LOG) and moderate-or-greater (MOG) intensity turbulence events to the total turbulence events of HVRRD-EDR reveal two local peaks at z=20–23 kft and 41–44 kft, while those of flight-EDR at z=20–23 kft and 35–38 kft. The LOG and MOG ratios of HVRRD-EDR show clear seasonal variations with large values in JJA and small values in DJF, while those of flight-EDR show somewhat different variations: large values in DJF and small values in JJA at z=20–30 kft, large values in March–May and small values in September–November at z=30–45 kft. Consequently, correlation coefficients between HVRRD-EDR and flight-EDR are negative at z=20–30 kft and positive at z=30–45 kft. Horizontally, the MOG ratio of HVRRD-EDR is large primarily over the Rocky Mountains which is consistent with the flight-EDR. The discrepancies in the spatiotemporal distributions between the two datasets likely stem from, at least, two reasons: (i) turbulence observed from the two datasets cannot be the same events, and (ii) HVRRD-EDR associated exclusively with static instability cannot include shear instability under stable atmospheric condition that is related to the Kelvin-Helmholtz instability of which most of flight-EDR is involved.


AS46-A016
Comparison of Different Estimation Techniques of Turbulent Energy Dissipation Rate from Doppler Lidar Measurements

SeungWon BAEK1+, Kwonil KIM2, Jung-Hoon KIM3, Gyu Won LEE1#
1Kyungpook National University, 2Stony Brook University, 3Seoul National University

Turbulence is one of the most significant physical processes in aviation meteorology. Rapid changes in a headwind in the vicinity of an aircraft can lead to aviation accidents. Although many efforts have been made to detect such turbulence in advance, difficulties have been encountered due to its small spatial (1 mm ~ 1 km) and temporal (1 s ~ 1 hr) scales, and unpredictable behavior. By utilizing Doppler lidar to observe turbulence with a high spatiotemporal resolution continuously, it is possible to overcome the limitations of in situ observation and detect turbulence in advance. Energy dissipation rate (EDR) is a valuable measure that can quantitatively represent the intensity of turbulence. Various techniques have been proposed to estimate EDR using Doppler lidar. In this study, we will compare the performance of three inertial range EDR estimation techniques (power spectrum, second-order structure function, variance). They are applied to Doppler lidar measurements operating in the vertically fixed-pointing mode. The accuracy of the estimated EDR was evaluated by the one from in-situ sonic anemometer. The results show that the data sampling rate greatly affected the EDR estimation using the power spectrum. The variance technique produces the most accurate estimation when compared to the value calculated from the sonic anemometer. This study will examine the benefits and weaknesses of each technique, taking into account the instrumental characteristics and scanning strategy of Doppler lidar.

ACKNOWLEDGEMENT
This work was supported by the National Research Foundation of Korea (NRF) grant funded by the Korea government (MSIT) (No. 2021R1A4A1032646). This work was funded by the Korea Meteorological Administration Research and Development Program "Developing Technology for High-Resolution Urban Weather Information Services” under Grant (KMA2018-00627).


AS46-A010
Performance Comparison of Probabilistic Turbulence Forecasts Using the Two Operational NWP Models of KMA

Dan-Bi LEE1+, Jung-Hoon KIM1#, Hye-Yeong CHUN2
1Seoul National University, 2Yonsei University

The current aviation turbulence forecast systems worldwide, including in South Korea, are mostly based on deterministic forecasts that provide the turbulence potential fields predicted by calculating turbulence diagnostics using the single numerical weather prediction (NWP) model output. Given that both the turbulence diagnostics and NWP model have inherent uncertainties, the need for probabilistic forecasts that can take such uncertainties into account and provide confidence in the forecasting is increasing. In this study, we perform probabilistic turbulence forecasts using the two operational Global Data Assimilation and Prediction System (GDAPS) outputs based on the Unified Model (UM) and the Korean Integrated Model (KIM) of the Korea Meteorological Administration (KMA), and evaluate the performance of the two GDAPS-based probabilistic turbulence forecasts against available turbulence observation data for one year (2022.01–2022.12). Although the UM- and KIM-based GDAPS have a similar horizontal resolution (~10 km for UM; ~12km for KIM), the KIM-based GDAPS has a higher vertical resolution than the UM-based GDAPS (70 levels below 80 km for UM; 91 levels below 80 km for KIM). To perform a single NWP model-based probabilistic turbulence forecast, two probabilistic forecasting approaches are considered, which are a forecast time-lagged ensemble and a multi-diagnostic ensemble. The UM-based deterministic turbulence forecast with a higher horizontal resolution predicts wider and stronger turbulence regions than the KIM-based deterministic turbulence forecast, regardless of the higher vertical resolution of KIM-GDAPS, although the predicted turbulence regions are overall similar. Detailed comparison results of performance validation of two GDAPS-based probabilistic turbulence forecasts will be presented in the conference. Acknowledgment: This work was funded by the Korea Meteorological Administration Research and Development Program under Grant KMI2022-00410.


AS46-A014
Stochastic Ensemble System for Airport Probabilistic Forecasting

Ui-Yong BYUN1#+, Eun-Chul CHANG1, Sang-Hun PARK2, Hye-Yeong CHUN2, Jung-Hoon KIM3
1Kongju National University, 2Yonsei University, 3Seoul National University

As global air traffic has steadily increased over the past few decades, the need for more accurate flight time compliance and safe and efficient air operations has arisen. To this end, the ICAO (International Civil Aviation Organization) established a global navigation plan and urged each country to implement it. Accordingly, Korea also launched the National Aviation Plan (NARAE) to realize a safe and efficient air traffic system. To successfully carry out the NARAE, it is necessary to provide detailed and three-dimensional aircraft weather information to support optimal operation for each flight stage in preparation for environmental changes in future air operations. In particular, at airport points, it is essential to provide probabilistic forecasts for decision-making of aircraft operations for factors such as visibility, ceiling, and wind shear, which significantly affect the takeoff and landing of aircraft. In this study, we configured the ensemble system to produce probabilistic forecasts of aircraft meteorological factors. An ensemble system is configured based on the Korea Meteorological Administration's KLAPS (Korea Local Analysis and Prediction System) and employs the stochastic ensemble methods; SPPT (stochastically perturbed physics tendencies) and SKEBS (stochastic kinetic-energy backscatter scheme). We conducted experiments on low visibility and wind shear cases at Incheon Airport. We confirmed the ensemble spread of each experiment by comparing the results of experiments with the different numbers of ensemble members. This work was funded by the Korea Meteorological Administration Research and Development Program under Grant KMI2022-00410. And the main calculations in this study were performed using supercomputing resources provided by the Korea Meteorological Administration (National Center for Meteorological Supercomputing).


AS46-A001
Influence of Bohai Sea-effect on Fog Formation in Western Coastal Zone Under the Background of Cold Back-flow in Northeast China

Tian MENG1+, Bingui WU2#
1Tianjin Institute of Meteorological Sciences, 2Tianjin Institute of Meteorological Science

The sea-effect generally refers to the process of air mass denaturation after the cold air flows above the warm sea surface. This type of fog is often observed in the western coastal zone of Bohai Sea and has an important impact on the local aviation. There is little research on the heavy fog in this area due to the influence of the "sea effect". This study investigates the mechanism of a typical sea-effect fog case in the morning of October 17, 2007 using WRF model over western coastal zone of Bohai Sea. Results indicated that: contrary to the most analyses of sea-effect snowstorm and precipitation studies that generally emphasize the role of oceanic heating, evaporation of Bohai Sea and accompanying advective vapor transport are shown to play more important roles in the formation of fog. The moisture budget reveals that the evaporation of the Bohai Sea at night is ten times greater than in the western coast. The water vapor transport guided by the back-flow in Northeast China contributes the most to the fog water. The vapor flux in this direction fluctuates and increases from 16:00, Oct 16 to 03:00, Oct 17 (LST), and vertical integral corresponding to the tendency of liquid water reaches a maximum at 03:00, Oct 17. In contrast, the temperature advection is weak. Sensitivity tests further show that the changes of the SST field only cause a shift in the location of the fog, while the humidity change triggered by the Bohai Sea effect plays a decisive role on fog formation in western coastal zone. The sensitivity test of evaporation shows that: with the decrease of evaporation in Bohai Sea, the advective vapor transport will be significantly weakened, and the simulated fog on the western coast of the Bohai Sea will disappear completely.


AS46-A002
Sensitivity of YSU Modified Scheme to Fog Simulation Under Different Physical Parameterized Combinations

Bingui WU1+, Tian MENG2#
1Tianjin Institute of Meteorological Science, 2Tianjin Institute of Meteorological Sciences

A modified algorithm which represents additional top-down turbulent mixing driven by cloud/fog-top radiative cooling was provided by Wilson and Fovell in 2018. The algorithm is appended to the Yonsei University (YSU) planetary boundary layer (PBL) parameterization scheme to improve turbulent mixing within the cloud/fog. Considering the modified YSU (YSU_mod) simulation may be affected by different combined parameterizations, three different combinations of parameterization schemes, including the schemes by formula provider recommended (WF), the schemes using by operational numerical prediction of North China Plain (NCP), and the land surface process parameterization in WF schemes being substituted by that in NCP (WF_1), are selected to evaluated fog cases over North China Plain using the Weather Research and Forecasting (WRF) model in order to promote the application of YSU_mod in NCP operational forecast system. The results show that the influence of the additional top-down turbulent mixing in fog is mainly shown as, (1) it significantly increases PBL temperature while the slight and uncertain effect on specific humidity, which lead to less fog layer liquid water and fog cover, and later formation and early dissipation of fog. (2) Under different combinations of parameterization schemes, the influence is that the warmer bottom of the PBL in WF schemes which promotes fog layer lifting, while the warmer upper of the PBL in NCP schemes which lowers fog layer. (3) The warmer fog layer don’t always correspond to the truth, the negative temperature deviation is modified successfully in WF schemes, while the temperature and humidity deviations are larger than observations in NCP schemes. In addition, an appropriate land surface parameterization greatly affects fog simulation which can be concluded from the significant fog simulation improvement in WF_1 comparing to the WF.


Mon-31 Jul | 10:20 - 12:20 | MR331
AS18 - The Science and Prediction of Tropical Cyclones

Session Chair(s): Chun-Chieh WU, National Taiwan University, Kelvin T. F. CHAN, Sun Yat-sen University

AS18-A030 | Invited
Near-shore Rapid Intensification of Tropical Cyclones

Johnny CHAN1,2#+, Charlie C. F. LOK2, Ralf TOUMI3
1Asia-Pacific Typhoon Collaborative Research Center, 2City University of Hong Kong, 3Imperial College London

It has been observed that some tropical cyclones (TCs) rapidly intensify within 24-48 hours of landfall along the South China coast, which poses a great challenge in terms of intensity forecasts and subsequent disaster preparedness. Some case studies have shown that an increase in sea-surface temperature (SST) might be responsible for such rapid intensification. In this paper, we show that the SST increase is likely due to solar heating of the ocean over a shallow continental shelf, which can occur for a TC with a small cloud cover. Numerical simulations of TCs with small and extensive cloud cover demonstrate that this is indeed the case. Further studies based on a large number of cases illustrate further that a combination of a high TC translation speed and a small cloud cover has the highest chance of causing a TC to intensify rapidly just before landfall.


AS18-A001 | Invited
The Dependence of Tropical Cyclone Pressure Tendency on Size

Ralf TOUMI#+, Nathan SPARKS
Imperial College London

Current theories of tropical cyclone (TC) intensification give little direct indication of the role of the TC size in intensity changes, although there are observations showing a relationship. We develop a new model of TC central pressure tendency where the pressure change can be expressed as exponential with a time constant determined by the ratio of radius maximum wind (Rmax) and the column inflow or outflow speed. An analysis of observations confirms the relationship which becomes more important for a larger pressure tendency and suggests an upper bound on pressure tendency for a given Rmax. The dependence of the pressure tendency on size poses a challenging constraint on the accurate forecasting of TCs in numerical weather prediction and climate models.


AS18-A022 | Invited
Uncertainties in Tropical Cyclone Landfall Decay

Kelvin T. F. CHAN1#+, Johnny CHAN2,3, Kailin ZHANG1, Yue WU1
1Sun Yat-sen University, 2Asia-Pacific Typhoon Collaborative Research Center, 3City University of Hong Kong

Understanding the responses of landfalling tropical cyclones to a changing climate has been a topic of great interest and research. Among them, the recently reported slowdown of tropical cyclone landfall decay in a warming climate engenders controversy. Here, the global climatology of landfall decay, based on the tropical cyclone best-track data available, reveals that the reported trends are uncertain and not universal, but spatial, temporal, data, and methodology dependent such that any claim of a climate trend could be misleading at present. The effective area of moisture supply from the ocean, most likely determined by the landfalling track modes, is demonstrated to be an important factor for the decay. This study provides timely essential clarifications of the current contentious understanding.


AS18-A056
Quantifying the Environmental Effects on Tropical Cyclone Intensity Change Using a Simple Dynamically Based Dynamical System Model

Jing XU1#+, Yuqing WANG1, Chi YANG2
1Chinese Academy of Meteorological Sciences, 2Beijing Normal University

Accurately prediction of tropical cyclone (TC) intensity is quite challenging due to multiple competing processes among the TC internal dynamics and the environment. Most previous studies have evaluated the environmental effects on TC intensity change based on TC best-track data which results from both internal dynamics and external influence. This study quantifies the environmental effects on TC intensity change using a simple dynamically based dynamical system (DBDS) model recently developed. In this simple model, the environmental effects are uniquely represented by a ventilation parameter B, which can be expressed as multiplicative of individual ventilation parameters of the corresponding environmental effects. Their individual ventilation parameters imply their relative importance to the bulk environmental ventilation effect and thus to the TC intensity change. Six environmental factors known to affect TC intensity change are evaluated in the DBDS model using machine learning approaches with the best-track data for TCs over the North Atlantic, central, eastern and western North Pacific and the statistical hurricane intensity prediction scheme (SHIPS) dataset during 1982–2021. Results show that the deep-layer vertical wind shear is the dominant ventilation factor to reduce the intrinsic TC intensification rate or to drive the TC weakening, with its ventilation parameter ranging between 0.5–0.8. Other environmental factors are generally secondary, with their respective ventilation parameters over 0.8. An interesting result is the strong dependence of the environmental effects on the stage of TC development. Finally, applications of the DBDS model to real TC intensity prediction are briefly discussed.


AS18-A035
Statistical Analysis of Near-landfall Intensified Typhoons and Their Dynamic and Thermal Conditions

Xiang CHUNYI1,2#+, Hironori FUDEYASU2
1China Meteorological Administration, 2Yokohama National University

Unlike most tropical cyclones (TCs) that begin to weaken when approaching the land, there are some TCs that intensified near-landfall on the contrary. Those TCs bring a great challenge to typhoon forecasts and disaster prevention. Based on three best track datasets JMA, CMA and JTWC from 1980 to 2021, the intensity variation characteristics of tropical cyclones in the Western Pacific within 48 hours before landfall were studied, and 11 common typical near-landfall intensified typhoon cases in the three datasets were selected for composite analysis. The environmental wind vertical shear, relative eddy flux convergence and local radiation flux during landings were calculated using ERA5 reanalysis. The intensity changes of 24hr, 12hr and 6hr before landfall were documented. According to statistical analysis, tropical cyclones whose intensity changes of 24hr before landfall exceeded 20kt and did not weaken within 48hr before landfall were defined as near-landfall intensification cases. Statistics show that those TCs have northwestward prevailing tracks. The high activated period is from July to September, and the probability during nighttime is significantly higher than that of daytime. Composite analysis of selected typical near-landfall intensified TCs shows that the vertical wind shear, which has no significant decreasing before landfall. Further analysis find out that the decreasing of local vertical wind shear and the increase of relative eddy flux convergence can favor the development of inner-core convection. The asymmetric distribution of latent heat, sensible heat flux and long-wave radiation on the underlying surface around the typhoon before landfall is further analyzed. It is found that the asymmetric distribution of local non-adiabatic typhoon circulation is conducive to the development of offshore intensity. Under favorable dynamic and thermal processes. Statistical analysis of such typhoons reveals common characteristics and possible influential factors.


AS18-A064
Kinetic Energy Budget Associated with Movement of Maximum Wind During the Rapid Intensification of Tropical Cyclone Khanun (2017)

Yishe SHI#+
Zhejiang University

Using validated Weather Research and Forecasting (WRF) model simulation data, kinetic energy (KE) budgets were analyzed to study the dynamic processes associated with the radial movement of maximum wind in the lower troposphere during the rapid intensification (RI) of tropical cyclone (TC) Khanun (2017). In this study, the radial movement of the maximum symmetric rotational KE is computed to measure the movement of the maximum wind. RI is divided into four stages: before RI, the radial distance decreases inward rapidly (stage 1); during RI, the radial distance undergoes a slowly inward decrease (stage 2), barely unchanged (stage 3) and a slowly inward decrease again (stage 4). The comparison between the radii of maximum symmetric rotational KE and its maximum tendency reveals that the radius of maximum symmetric rotational KE generally is larger than that of maximum tendency of symmetric rotational KE in all stages except in stage 3 when maximum symmetric rotational KE and its maximum tendency are nearly collocated. The analysis of symmetric rotational KE budgets shows that flux convergence of KE always is an important term determines maximum tendency in all stages. The conversion from asymmetric rotational KE to symmetric rotational KE, and the conversions from environmental KE to symmetric rotational KE and from symmetric divergent KE to symmetric rotational KE contribute to the maximum tendency, respectively, in stage1 and stages 3 and 4. The important terms in determining maximum tendency are further partitioned and the results will be reported in the conference. Keywords: tropical cyclone, rapid intensification, kinetic energy budget, symmetric and asymmetric circulations, divergent and rotational circulations.


AS18-A008
On Tropical Cyclone Genesis Types and Their Intensification Rate

Ming-Han CHUNG#+, Chun-Chieh WU
National Taiwan University

Higher tropical cyclone (TC) intensification rates are affected by smaller radius of maximum wind (RMW) while continuing convection within the RMW can cause RMW contraction. Therefore, understanding the factors affecting convection distribution and RMW is crucial for characterizing TC intensification rates. Previous studies have shown that convection distribution is affected by TC genesis type, but subjective classification of TC genesis doesn’t rely on data distribution. Hence, this study develops a new objective method to classify TC genesis type based on a K-means cluster analysis of critical environmental parameters available in ECMWF Reanalysis v5 (ERA5) data. For a proportionate comparison between intensification rate and RMW, the lifetime maximum intensification rate (LMIR) in each case is estimated in this study. The K-means cluster analysis shows four TC genesis types: (i) monsoon confluence (MC), (ii) easterly wave or north of monsoon trough (EW), (iii) monsoon shear (MS), and (iv) monsoon depression (MD). The positive vorticity area in MC and MS indicates the monsoon trough. MC forms at the east of the monsoon trough while MS forms inside the monsoon trough. EW has a small RMW and a small high positive vorticity area. In contrast, MD has a larger RMW and a larger high positive vorticity area. Each genesis type has different convection distribution compared to previous objective method. Owing to larger circulation and scattered convection, MD has a significantly larger RMW and lower LMIR than EW based on Conover's test. In contrast, EW cases have high specific humidity only around the center. Although MC and MS have medium RMW sizes between those of EW and MD, their LMIR is as high as that in EW due to the aggregated convection.


AS18-A050
Investigating the Definition of Rapid Intensification in Typhoons: A Process-based Approach

Cheng-Hsiang CHIH+, Chun-Chieh WU#, Yi-Hsuan HUANG
National Taiwan University

The occurrence of rapid intensification (RI) of a tropical cyclone (TC) involves multi-scale processes and complex interactions, posing a major challenge in operational forecasting. RI is also a well-trodden path for TCs reaching high storm intensity. The most widely-applied RI threshold is 30 kt intensity change in 24 hours, which is the 95th percentile of the overwater intensity changes based on National Hurricane Center best-track database in Atlantic and eastern North Pacific basins during 1995-2012. The statistics of the 95th percentile of intensity change can vary for TCs in other basins or during a different time period. To conduct a process-based study, this work attempts to identify a better RI definition that can most representatively identify the storm structure difference between RI and non-RI periods for TCs in the western North Pacific. Results based on 40-year (1979-2020) TC best-track data from JMA and JTWC are presented. This study explores the differences in storm structure and TC-environment conditions between RI and non-RI periods. It is shown that an RI threshold of 50 (40) kt intensity change in 36 (24) h based on JMA (JTWC) yields the most distinct warm-core structure difference between RI and non-RI periods.


Mon-31 Jul | 1:10 - 3:10 | MR309
AS04 - Impact of Fires on Air Quality and Climate: Processes, Field and Modeling Studies

Session Chair(s): Jianmin CHEN, Fudan University, Abdelwahid MELLOUKI, ICARE-CNRS/OSUC

AS04-A016 | Invited
Prolonged Lifetime of Particulate-bound Polycyclic Aromatic Hydrocarbons with Coating of Secondary Aerosols During Photochemical Aging of Biomass Burning Plumes

Xinming WANG1#+, Wei DENG1, Tengyu LIU2, Zheng FANG3, Yanli ZHANG4, Wei SONG1, Yinon RUDICH3, Jianmin CHEN5, Abdelwahid MELLOUKI6,7, Christian GEORGE8
1Chinese Academy of Sciences, 2Nanjing University, 3Weizmann Institute of Science, 4Guangzhou Institute of Geochemistry, Chinese Academy of Sciences, 5Fudan University, 6Mohammed VI Polytechnic University, Morocco, 7Shandong University, 8National Center for Scientific Research - Catalysis and Environmental Research Institute

Polycyclic aromatic hydrocarbons (PAHs), one class of most toxic compounds in atmosphere, showed much longer than predicted lifetimes in ambient air due to heterogeneous scavenging by ozone (O3) according to previously studies. Here we show heterogeneous reactions with hydroxyl (OH) radical dominates far more over that with O3 in the degradation of particle-bound PAHs based on chamber simulation on the evolution of plumes from biomass burning, the largest emitter of PAHs on a global scale. The evolution of crop straw burning fumes in a 30 m3 smog chamber revealed that for heterogeneous reactions of PAHs with OH, their second order degradation rate constants were estimated to be 4.4~8.6×10-12 cm3 molecule-1 s-1 at the initial stage of photo-oxidation, and they dropped 4-5 times to to 1.1~1.7×10-12 cm3 molecule-1 s-1 after 1~5×1011 molecule cm-3 s OH radical exposure, corresponding to a decrease of uptake coefficients of OH (γOH) from 2.2±0.9 to 0.5±0.1. The decrease of second order rate constants and γOH were mainly caused by the reduction in secondary chemistry and the burial effect of coatings by secondary organic/inorganic aerosols during the atmospheric oxidation. Moreover, the OH oxidation pathway (1.1~1.7×10-6 s-1) dominates over ozonolysis pathway (1.7~12.7×10-7 s-1) in heterogeneous degradation of PAHs. The lifetimes of particulate PAHs were estimated to be 93.5~219 h, approximately 120 times that obtained previously by exposing pure PAHs to oxidants, implying their stronger long-range transport and more persistent health risks.


AS04-A024
Analysis of Open Bio-mass Burning in China and its Impacts on Air Quality Forecasting

Sunling GONG#+
China Meteorological Administration

A better understanding of spatial-temporal variations of open bio-mass burning in China is required to assess its impacts on the air quality and especially on the heavy haze pollution. The MODIS fire spots data and the calculated burned areas were used in this research, which shows the varying number of fire spots in China from 2013 to 2017, with the highest in 2014 and the lowest in 2016. Meanwhile, the fire spots were found mainly concentrated in three key periods (March-April, June and October-November) and two zones with inter-annual variations of burned areas. In addition, the contribution of major vegetation types burning was studied, the cropland occupied the largest proportion of burned area of more than 70 % in any period time, followed by forest. Finally, from the perspective of climate and human activities, the causes of inter-annual variations were discussed. By comparing the average temperature and precipitation in the two zones from 2013 to 2017, it was found that the burned forest area is positively correlated with the average temperature of the zones and negatively correlated with the average precipitation. Meanwhile, the relationship between the El Niño events and the bio-mass burning was discussed. Finally, by using the datasets of MODIS fire spot, land cover, vegetation cover, bio-mass loading and emission factors, a bio-mass emission model is developed, which is then embedded as an on-line module to an air quality model (WRF-CUACE) to quantitatively assess the impacts of bio-mass burning on surface PM2.5 concentration in China.


AS04-A027
Open Biomass Burning Emissions and Their Contribution to Ambient Formaldehyde in Guangdong Province, China

Chunlin ZHANG, Jiangyong LI, Wenlong ZHAO, Qian YAO, Hao WANG#+, Boguang WANG
Jinan University

Formaldehyde (HCHO) plays a vital role in atmospheric chemistry and O3 formation. Open biomass burning (OBB) is considered to be an important source of HCHO; however, its quantitative contribution to ambient HCHO remains poorly understood due to the lack of reliable high-resolution emission inventories. In this study, a satellite-based method coupled with local emission factors was developed to estimate the hourly primary emissions of HCHO and volatile organic compound (VOC) precursors from OBB in Guangdong (GD) Province of southern China. Furthermore, the contribution of OBB to ambient HCHO was quantified using the Community Multi-scale Air Quality model. The results suggested that in average OBB emissions contributed 5293 tons of primary HCHO per year, accounting for ~14% of the total anthropogenic HCHO emissions in GD. The ambient HCHO concentration ranged from 0.3 ppbv to 8.7 ppbv during normal days, and from 8 ppbv to 45 ppbv in downwind area during OBB impacted days. The monthly contribution of OBB to local HCHO levels reached up to 50% at locations with frequent fires and over 70% during a forest fire event. Ambient HCHO was heavily affected by primary OBB emissions near the source region and by the oxidation of OBB-emitted VOCs in the downwind area. Secondary HCHO formation from OBB emissions was enhanced during photochemical pollution episodes, especially under conditions of high O3 and low NOx. OBB-emitted ethene was identified as the most important VOC precursor of HCHO and contributed to the formation of ~50% of the secondary HCHO. The HCHO formation potential of cropland fires was 26% higher than that of forest fires. Our results suggest that OBB can elevate ambient HCHO levels significantly. Thus, strict control policies on OBB should be implemented, especially for open-burning agricultural residues in upwind areas on serious photochemical pollution days.


AS04-A013
Worldwide Pyrocumulonimbus Inventory Reveals the Frequency, Variability, and Stratospheric Impact of Smoke-Infused Storms During 2013-2021

David PETERSON1#+, Melinda BERMAN2, Michael FROMM1, William JULSTROM3, René SERVRANCKX4, Edward HYER1, James CAMPBELL1, Theodore MCHARDY5
1Naval Research Laboratory, 2University of Illinois Urbana-Champaign, 3University of Iowa, 4PyroCb Community Member, 5American Society for Engineering Education

This study provides the first comprehensive inventory of all known pyrocumulonimbus (pyroCb) events observed worldwide (546 confirmed events) over the nine-year period 2013-2021. PyroCbs are a dangerous and severe type of fire weather, which present many hazards to firefighting efforts and communities along the wildland-urban interface. These unique storms also serve as a vertical transport pathway (large chimney) facilitating rapid injection of smoke into the upper troposphere and lower stratosphere (UTLS). This inventory provides insight into basic questions on inter-annual, seasonal, sub-daily, and regional variability of pyroCb, along with potential controlling factors. Development of this inventory has included detailed analysis of the distribution and variability of pyroCb smoke injection altitudes, quantitative estimation of the aerosol mass associated with each stratospheric plume, and examination of the impact of pyroCb activity on stratospheric aerosol loading worldwide. This pyroCb inventory provides the means to address a wide range of significant open questions about the nature, behavior, and impact of this phenomenon. Answers to these questions are critical for advancing pyroCb prediction capabilities to mitigate aviation hazards and aid firefighting efforts. This new multi-year inventory dataset also sets a foundation for an official Earth System Data Record that can be maintained into the future and extended back in time to identify longer-term trends in pyroCb activity and ensuing impacts on the climate system.


AS04-A011
Pyrocumulonimbus and its Role in the Climate System: What is Known and Unknown?

David PETERSON1#+, Edward HYER1, James CAMPBELL1, Melinda BERMAN2, William JULSTROM3, Ghassan TAHA4, Christopher CAMACHO1, Laura THAPA5, Theodore MCHARDY6, Pablo SAIDE5
1Naval Research Laboratory, 2University of Illinois Urbana-Champaign, 3University of Iowa, 4NASA Goddard Space Flight Center, 5University of California, Los Angeles, 6American Society for Engineering Education

Pyrocumulonimbus (pyroCb) are fire-induced and smoke-infused thunderstorms that serve as the primary pathway for smoke to reach the upper troposphere and lower stratosphere (UTLS).The magnitude of smoke plumes observed in the UTLS has increased significantly in recent years, rivaling or exceeding the impact from all volcanic eruptions observed over the last decade, with the potential for significant climate feedbacks on seasonal and hemispheric scales. The Black Summer fire season of 2019-2020 in southeastern Australia contributed to an unprecedented pyroCb ‘super outbreak’ that took place over 51 non-consecutive hours. More than half of the 38 observed pyroCb updraft pulses injected smoke particles directly into the stratosphere, producing two of the three largest smoke plumes observed at such altitudes to date. Over the course of three months, these plumes encircled a large swath of the Southern Hemisphere while continuing to rise, in a manner consistent with existing nuclear winter theory. Fewer than three years earlier, a large pyroCb outbreak in Canada produced a persistent smoke plume that encircled a portion of the Northern Hemisphere. We summarize what the community has learned from these extreme events and identify science questions that remain unanswered. A recently-developed pyroCb inventory for 2013-2021 facilitates the first analysis of regional, seasonal, monthly, and inter-annual variability worldwide. Unique in-situ and remotely-sensed measurements of pyroCb activity observed during the 2019 FIREX-AQ field experiment identify the fire characteristics, cloud microphysical properties, and smoke plume chemistry associated with this extreme fire-weather phenomenon.


AS04-A007
A Study on Forest Fire Emissions in South of Orléans, France

Chaoyang XUE1#, Yangang REN2,3+, Abdelwahid MELLOUKI4, Valery CATOIRE5
1Max Planck Institute for Chemistry, 2Research Center for Eco-Environmental Sciences, Chinese Academy of Sciences, 3University of Chinese Academy of Sciences, 4ICARE-CNRS/OSUC, 5Université d'Orléans

Wildfire events are increasing globally which may be partly associated with climate change, resulting in significant adverse impacts on local, regional air quality and global climate. In September 2020, a wildfire event occurred in Souesmes (Loir-et-Cher, Sologne, France), and its plume spread out over 200 km on the following day as observed by the MODIS satellite. Based on measurements at a suburban site (~50 km northwest of the fire location) in Orléans, young wildfire plumes were characterized. Significant increases in gaseous pollutants (CO, CH4, N2O, VOCs, etc.) and particles (including black carbon) were found within the wildfire plumes. Emission factors, defined as EF (X) = ∆X/∆CO (where X represents the target species), of various trace gases and black carbon within the young wildfire plumes were determined accordingly and compared with previous studies. Changes in the ambient ions (such as ammonium, sulfate, nitrate, chloride, and nitrite in the particle- and gas- phase) and aerosol properties (e.g., aerosol water content, aerosol pH) were also quantified and discussed. Moreover, we estimated the total carbon and other gas (e.g., CO) emissions that were compared with fire emission inventories. We found that the Global Fire Assimilation System (GFAS) may underestimate emissions (e.g., CO) of this small wildfire while other inventories (GFED, FINN) showed significant overestimation. Considering that few wildfires are recorded in this region, related atmospheric implications are presented and discussed. More details can be found in Xue, Chaoyang, et al. "A study on wildfire impacts on greenhouse gas emissions and regional air quality in South of Orléans, France." Journal of Environmental Sciences (2022).


Mon-31 Jul | 1:10 - 3:10 | MR327
AS12 - Passive and Active Sensing of the Chemistry and Dynamics of the Middle and Upper Atmosphere

Session Chair(s): Patrick ESPY, Norwegian University of Science and Technology

AS12-A001
Abrupt Change in the Lower Thermospheric Mean Meridional Circulation During Sudden Stratospheric Warmings

Yvan ORSOLINI1#+, Varavut LIMPASUVAN2, Jiarong ZHANG2
1Norwegian Institute for Air Research, 2Coastal Carolina University

Our understanding of the vertical coupling between the lower atmosphere and the upper atmosphere has significantly advanced in recent years, spurred by the large amount of new space-borne and ground-based observations and the extension of atmospheric models into the mesosphere and thermosphere. Observational and model studies have revealed that the mesosphere-lower thermosphere (MLT) region is the nexus where the forcings by gravity waves (GWs), atmospheric tides and planetary waves (PWs) contribute to driving the mean meridional circulation (MMC). Sandwiched between the two summer-to-winter overturning circulations in the mesosphere and the upper thermosphere, the climatological lower thermosphere mean meridional circulation is a narrow gyre that is characterized by upwelling in the middle winter latitudes, equatorward flow near 120 km, and downwelling in the middle and high summer latitudes. Based on the hourly output from the 2000–2014 simulations of the National Center for Atmospheric Research’s vertically extended version of the Whole Atmosphere Community Climate Model (WACCM-X) in specified dynamics configuration, we examine the roles of PWs, GWs and atmospheric tides in driving the mean meridional circulation in the lower thermosphere and its response to the sudden stratospheric warming phenomenon with an elevated stratopause in the northern hemisphere. Following the onset of the sudden stratospheric warmings, this gyre reverses its climatological direction, resulting in a “chimney-like” feature of un-interrupted polar descent from the altitude of 150 km down to the upper mesosphere. This reversal is driven by the westward-propagating planetary waves, which exert a brief but significant westward forcing between 70 and 125 km, exceeding gravity wave and tidal forcings. We present evidence of this circulation in observational data and the observational needs to improve our understanding of its variability.


AS12-A016 | Invited
Interhemispheric Coupling Study by Observations and Modelling (ICSOM)

Kaoru SATO1#+, Yoshihiro TOMIKAWA2,3, Masashi KOHMA1, Ryosuke YASUI4, Dai KOSHIN1, Haruka OKUI1, Shingo WATANABE5, Kazuyuki MIYAZAKI6, Masaki TSUTSUMI2, Damian MURPHY7, Chris MEEK8, Yufang TIAN9,10, Manfred ERN11, Gerd BAUMGARTEN12, Jorge L. CHAU12, Xinzhao CHU13, Richard COLLINS14, Patrick ESPY15,16, Hiroyuki HASHIGUCHI17, Andrew KAVANAGH18, Ralph LATTECK12, Franz-Josef LUEBKEN19, Marco MILLA20, Satonori NOZAWA21, Yasunobu OGAWA2, Kazuo SHIOKAWA21, M Joan ALEXANDER22, Takuji NAKAMURA2, William WARD23
1The University of Tokyo, 2National Institute of Polar Research, 3Graduate University for Advanced Studies, 4Japan Meteorological Agency, 5Japan Agency for Marine-Earth Science and Technology, 6California Institute of Technology, 7Australian Antarctic Division, 8University of Saskatchewan, 9Chinese Academy of Sciences, 10University of Chinese Academy of Sciences, 11Forschungszentrum Jülich, 12University of Rostock, 13University of Colorado at Boulder, 14University of Alaska, 15Norwegian University of Science and Technology, 16University of Bergen, 17Kyoto University, 18British Antarctic Survey, 19Leibniz Institute of Atmospheric Physics, 20Instituto Geofísico del Perú, 21Nagoya University, 22NorthWest Research Associates, 23University of New Brunswick

An international joint research project, entitled Interhemispheric Coupling Study by Observations and Modelling (ICSOM), is ongoing. 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-art GW-permitting general circulation model using 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 planned. This paper provides an overview of ICSOM, but even initial results suggest that not only gravity waves but also large-scale waves are important for the mechanism of the IHC.


AS12-A004
Dual VHF Radar Measurements of Aspect Sensitivity, Winds, and Momentum Flux in the Troposphere and Lower Stratosphere

Iain REID1,2#+, Ruediger RUESTER3, Peter CZECHOWSKY3
1ATRAD Pty. Ltd., 2University of Adelaide, 3Max Planck Institute for Solar System Research

Radar observations of the troposphere and lower stratosphere made in northern Germany with two VHF MST radars separated by about 30 km in quite different topography over a period of one week are presented. One of the radars, the SOUSY MST radar, was located in the Harz Mountains; the other radar, the Mobile SOUSY MST radar, was operated in a limited form and provides an interesting and rare example of a small beam swinging Doppler radar operating in the lower VHF band (53.5 MHz). Wind results are consistent between the radars, but there are some differences in the measured upward fluxes of horizontal momentum. Wave activity associated with the passage the jet stream over the location of the larger radar in the Harz Mountains is quite evident in the measured winds at the two locations. Stratospheric and tropospheric measurements of aspect sensitivity, mean winds and wave fluxes measured at the two sites from this campaign are presented and discussed.


AS12-A009
Energetic Particle Precipitation Signal Found in the Bromine Nitrate Observation

Jia JIA1,2#+, Monika SZELAG3, Michael HÖPFNER4, Pekka VERRONEN3, Patrick ESPY1,5
1Norwegian University of Science and Technology, 2Birkeland Centre for Space Science, 3Finnish Meteorological Institute, 4Karlsruhe Institute of Technology, 5University of Bergen

Bromine nitrate (BrONO2) is a major reservoir of the active bromine radicals that contribute to the formation of ozone hole. Energetic particle precipitation (EPP) generated NOx enhancement is known to lead to ozone loss in the mesosphere and upper stratosphere. In the lower stratosphere, however, this NOx enhancement is believed to restrain ozone depletion by deactive chlorine and bromine species to the reservoir forms (HCl/HBr and ClONO2/BrONO2). In this study we report BrONO2 response to EPP for the first time, using the latest BrONO2 measurement data from the Michelson Interferometer for Passive Atmospheric Sounding (MIPAS) on Envisat. We report a positive and significant correlation between BrONO2 and EPP Ap index above 30km in Arctic. In addition, the Whole Atmosphere Community Climate Model with D-region ion chemistry (WACCM-D) was used to characterize the EPP contribution to BrONO2 formation.


AS12-A006
Long‐term Trends of the Meteor Altitude Distribution, Mesospheric Density and Gravity Wave Momentum Flux Observed by the High-latitude Meteor Radars

Wen YI1+, Iain REID2,3, Xianghui XUE1#, Jie ZENG1, Damian MURPHY4, Masaki TSUTSUMI5, Njål GULBRANDSEN6, Xiankang DOU1
1University of Science and Technology of China, 2ATRAD Pty. Ltd., 3University of Adelaide, 4Australian Antarctic Division, 5National Institute of Polar Research, 6UiT The Arctic University of Norway

The mesosphere and lower thermosphere (MLT) region is strongly modulated by gravity wave (GW) perturbations, and the momentum flux of GW is essential in quantitatively understanding and modeling atmospheric structure at all altitudes. In this study, we present the seasonal variations, long-trend of mesospheric density and GW momentum flux observed by the meteor radars at Davis Station (68.6°S, 77.9°E), in Antarctica, Svalbard (78.3°N, 16°E), Tromsø (69.6°N, 19.2°E) in the Arctic. In general, u’w’ decreases and v’w’ increases as altitude increasing, and westward maximum of u’w’ and northward maximum of v’w’ in spring and autumn at upper altitude. the momentum flux u’w’ and v’w’ is anti-correlated with the background winds (u/v). The seasonal variations in the Davis Station meteor radar relative densities in the southern polar mesopause are mainly dominated by an annual oscillation (AO). The mesopause relative densities observed by the Tromsø meteor radars at high latitudes in the Northern Hemisphere show mainly an AO and a relatively weak semiannual oscillation (SAO).


AS12-A013 | Invited
Dynamics of Thermospheric Nitric Oxide During Geomagnetic Storms and Solar Flares

Yongliang ZHANG#+, Larry PAXTON, Robert SCHAEFER
Johns Hopkins University Applied Physics Laboratory

Thermospheric nitric oxide (NO) is a minor species that not only cools the thermosphere through 5.3 µm radiation but also changes significantly during geomagnetic storms. NO column densities derived from TIMED/GUVI data reveal a number of features: (1) NO enhancement is very sensitive to energy input in high latitudes; (2) NO column density and O/N2 column density ratio are anti-correlated on a global scale but show a noticeable shift between the boundaries of NO enhancement and O/N2 depletion regions during geomagnetic storms; (3) Flare time NO enhancement. The features (1) and (2) are likely caused by storm-time meridian circulation that bring high latitude NO enhancement and O/N2 depletion to mid and low latitudes. The feature (3) is caused by increased production of NO. TIMED/GUVI observations of NO serve as a way to monitor the storm-time dynamics and state of the thermosphere for space weather research and operation.


AS12-A005
A New Dual-frequency Atmospheric Radar System and its First Results

Qingchen XU1#+, Iain REID2,3
1National Space Science Center of the Chinese Academy of Sciences, 2ATRAD Pty. Ltd., 3University of Adelaide

A new dual-frequency atmospheric radar system is built and installed in Langfang Observatory, north China. It utilizes 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. In dedicated meteor mode, the daily meteor count rate reaches over 40,000 and allow wind estimation of finer time resolutions, such as 15-min and 30-min interval, better than the 1-hour typical of most meteor radars. The uncertainty of the ST wind measurements is better than 2 m/s when estimating the line of best fit with radiosonde winds. Preliminary observation results of typical winter gravity waves (GWs) momentum fluxes in the mesosphere, lower stratosphere and troposphere are also presented.


Mon-31 Jul | 1:10 - 3:10 | MR328
AS09 - The Science and Prediction of Heavy Precipitation and Floods

Session Chair(s): Jung-Eun CHU, City University of Hong Kong

AS09-A028 | Invited
An Review of Research on the Record-breaking Precipitation Event in Henan Province of China, July 2021

Qinghong ZHANG1#+, Juanzhen SUN2, Rumeng LI1
1Peking University, 2National Center for Atmospheric Research

A record-breaking precipitation event caused 398 deaths and 20.06 billion RMB economic losses in Henan Province of China in July 2021. A maximum 24-h (1-h) precipitation of 624 mm (201.9mm) was observed at the Zhengzhou weather station. However, all global operational forecast models failed to predict the intensity and location of maximum precipitation for the event. This high social impact event has drawn much attention from the research community. This presentation provides a high-level review of the event and its research from the perspectives of observations, analysis, dynamics, predictability, and the connection with climate warming and urbanization. Global reanalysis revealed obvious abnormality in large-scale circulation patterns that resulted in abundant moisture supplies in the region of interest. Recent studies of this event also revealed, via high-resolution model simulation and data assimilation, that three mesoscale systems (a mesoscale low pressure system, a barrier jet and downslope gravity current) contributed to the local intensification of the rainstorm. Further, observational analysis suggested that an abrupt increase of graupel through microphysical processes contributed to the record-breaking precipitation. Although these findings aided in our understanding of the extreme rainfall event, preliminary analysis indicated that the practical predictability of the extreme rainfall for this event was rather low. The contrary influences of climate warming and urbanization on precipitation extremes as revealed by two studies could add further challenges to the predictability. We concluded by emphasizing that data sharing and collaboration between meteorological and hydrological researchers would be crucial in the future research on high-impact weather events.


AS09-A008 | Invited
An Unprecedented Compound Extreme of South-rainstorm and North-heatwave in Eastern China During Early Summer 2022

Zhicong YIN#+, Xiaoqing MA, Yijia ZHANG, Tianbao XU, Botao ZHOU, Huijun WANG
Nanjing University of Information Science & Technology

Climate risks from compound extremes are much greater than the sum of their sub-components. In early summer 2022, record-breaking rainstorm and heatwave were respectively observed in the south and north of eastern China and they formed an unprecedented compound extreme (hereafter referred to as SRNH). However, most of seasonal predictions failed to capture the SRNH and the behind mechanisms are still unclear. Here we show that the wavier mid-latitude westerlies and the ridge of the western Pacific subtropical high stabilized at 20 °N were the main causes in the atmosphere and the ultra-strong 2022 SRNH event could be well reproduced. The February-March sea surface temperature anomalies in the North Atlantic concurrently promoted the 2022 SRNH extreme, which was successfully verified by numerical experiment. Main physical mechanism is the warmer sea surface excited a Rossby wave train to enhance the contrast between hot North China and wet South China.


AS09-A027
The Roles of Low-level Jets in “21·7” Henan Extremely Persistent Heavy Rainfall Event

Yuhan LUO#+, Yu DU
Sun Yat-sen University

An extremely heavy rainfall event lasting from 17 to 22 July 2021 occurred in Henan Province of China, with accumulated precipitation of more than 1000 mm over a 6-day period that exceeded its mean annual precipitation. The present study examines the roles of persistent low-level jets (LLJs) in maintaining the precipitation using surface station observations and reanalysis datasets. The LLJs triggered strong ascending motions and carried moisture mainly from the outflow of Typhoon In-fa (2021). The varying directions of the LLJs well corresponded to the meridional shifts of the rainfall. The precipitation rate reached a maximum during 20−21 July as the LLJs strengthened and expanded vertically into double LLJs, including synoptic-weather-system-related LLJs (SLLJs) at 850–700 hPa and boundary-layer jets (BLJs) at ~950 hPa. The coupling of the SLLJ and BLJ provided strong mid- and low-level convergence on 20 July, whereas the SLLJ produced mid-level divergence at its entrance that coupled with low-level convergence at the terminus of the BLJ on 21 July. The formation mechanisms of the two types of LLJs are further examined. The SLLJs and the low-pressure vortex (or inverted trough) varied synchronously as a whole and were affected by the southwestward movement of the WPSH in the rainiest period. The persistent large total pressure gradient force at low levels also maintained the strength of low-level geostrophic winds, thus sustaining the BLJs on the synoptic scale. The results based on a Du-Rotunno 1D model show that the Blackadar and Holton mechanisms jointly governed the BLJ dynamics on the diurnal scale.


AS09-A007
On the Influences of Urbanization on the Extreme Rainfall Over Zhengzhou on 20 July 2021: A Convection-permitting Ensemble Modeling Study

Yali LUO1#+, Jiahua ZHANG2, Miao YU3
1Nanjing University of Information Science & Technology, 2Chengdu University of Information Technology, 3Chinese Academy of Meteorological Sciences

This study investigates the influences of urban land cover on the extreme rainfall event over the Zhengzhou city in central China on 20 July 2021 using the Weather Research and Forecasting model at a convection-permitting scale [1-km resolution in the innermost domain (d3)]. Two ensembles of simulation (CTRL, NURB), each consisting of 11 members with a multi-layer urban canopy model and various combinations of physics schemes, were conducted using different land cover scenarios: (i) the real urban land cover, (ii) all cities in d3 being replaced with natural land cover. The results suggest that CTRL reasonably reproduces the spatiotemporal evolution of rainstorms and the 24-h rainfall accumulation over the key region, although the maximum hourly rainfall is underestimated and displaced to the west or southwest by most members. The ensemble mean 24-h rainfall accumulation over the key region of heavy rainfall is reduced by 13%, and the maximum hourly rainfall simulated by each member is reduced by 15–70 mm in CTRL relative to NURB. The reduction in the simulated rainfall by urbanization is closely associated with numerous cities/towns to the south, southeast, and east of Zhengzhou. Their heating effects jointly lead to formation of anomalous upward motions in and above the planetary boundary layer (PBL), which exaggerates the PBL drying effect due to reduced evapotranspiration and also enhances the wind stilling effect due to increased surface friction in urban areas. As a result, the lateral inflows of moisture and high-θe (equivalent potential temperature) air from south and east to Zhengzhou are reduced.


AS09-A012
Moisture Sources for the Weather Pattern Classified Extreme Precipitation in the First Rainy Season Over South China

Dongdong PENG#+
Institute of Tropical and Marine Meteorology, Guangzhou, China Meteorological Administration

Moisture transport, associated with moisture sources and synoptic-scale weather conditions, is a key dynamic process of precipitation events. Using the K-means clustering method and the FLEXPART Lagrangian particle dispersion model, this paper investigates moisture contributions from different source regions to extreme precipitation in the first rainy season (hereafter FRS) over South China. In average, land regions contribute more to the FRS extreme precipitation over South China than the ocean regions. The main source regions are Southeast Asia (22.7%), South China (17.2%), the South China Sea (14.3%), and the Bay of Bengal (8.3%). Extreme precipitation events are classified into three types by the K-means clustering based on 850 hPa geopotential height, which are all characterized by an anomalous low-pressure system over South China with varying intensity and locations. The distribution of geopotential height anomaly for Type I (30.3%) is characterized the low trough extending from Japan to South China, while Type II (42.5%) and Type III (27.2%) are characterized by “west negative–east positive” and “north positive–south negative” patterns over East Asia with anomalous cyclone over South China, respectively. The much larger contribution of land sources than ocean regions are mainly concentrated in Type I and Type III, of which the contribution from each source region is similar. Ocean sources play a more important role in Type II and are mainly from the Indian Ocean (16.2%) associated with the onset of South China Sea summer monsoon.


AS09-A018
Future Changes in Coastal Warm-sector Flood-producing MCS in Southern China

Murong ZHANG1#+, Zhiyong MENG2, Yipeng HUANG3
1Xiamen University, 2Peking University, 3Xiamen Meteorological Bureau

During the pre-summer rainy season in southern China, MCS-associated heavy rainfall frequently occurs in the warm sector hundreds of kilometers to the south of a front or without any front, which is one of the major contributors for coastal flooding events during this period. The intensity and frequency of strong convective storms are expected to rise with warming climate, posing a greater threat of extreme rainfall in the future. This study aims at revealing the future changes of coastal warm-sector MCS in southern China on its related precipitation features and essential mesoscale process associated based on quasi-idealized WRF simulations and pseudo global warming (PGW) approach. Typical warm-sector heavy rainfall events are selected to produce composite environments that force the quasi-idealized simulation in current climate (CTRL). After that, the climate sensitivity experiment (PGW) is conducted with the same configurations except that it is forced by reanalysis data plus a climate thermodynamic perturbation derived from a 32-model CMIP5 ensemble climate change signal for SSP5-8.5 scenario. Comparisons between PGW and CTRL reveal that 12-h accumulated area-averaged rainfall increases 51% by the end of 21st century, with the maximum rising from 333.1 mm to 703.4 mm. As for convection population, the frequency of convection weaker (stronger) than 20dBZ increases (decreases). The rainfall distribution and rainfall maximum are characterized by a north shift, which is largely due to stronger southerly LLJ in warming climate. Moreover, the MCS is initiated ~1h earlier in PGW, with more unstable inflow and stronger back building process leading to larger rainfall accumulation. Notably, although dynamic climate change signal is not included in the current experiment, the LLJ is significantly enhanced by increasing latent heating. The LLJ, latent heating, and deep moist convection may therefore link as a positive feedback in warming climate and eventually lead to extreme rainfall.


AS09-A025
Changes of Global Spatiotemporally Continuous Precipitation Events Under Past and Future Climate Warming

Xiaoyu WANG1+, Ming LUO1,2#
1Sun Yat-sen University, 2The Chinese University of Hong Kong

Extreme precipitation events cause damage to the natural environment and human society, but their jointly evolution behaviors in both time and space dimensions have not been extensively studied. By introducing a spatiotemporally contiguous events tracking (SCET) method, here we examine the climatologies and trends of the 3D (latitude×longitude×time) characteristics of spatiotemporally contiguous extreme precipitation events across the globe under the past and future climate warming during 1980 and 2020. The results show that the SCET can well demonstrate the jointly dynamic evolution patterns of contiguous precipitation events in time and space dimensions. Spatially, large contiguous precipitation events tend to be concentrated southeastern Asia, Europe and central Africa. Temporally, the frequency of contiguous precipitation events shows an overall increasing trend, but their affected area, intensity, duration and movement showed different characteristics. The future changes of spatiotemporally contiguous precipitation are further investigated based on a set of CMIP6 model simulations. In the coming decades (e.g., 2020–2100), the affected area, intensity and moving speed of contiguous precipitation events will increase. These trends are especially more prominent under high greenhouse gasses emission scenarios (e.g., SSP585). It is expected that extreme precipitation events that are more intense, affect larger areas, and move faster will cause even more harm to human society. Our results provide new insight to understand the spatiotemporal evolutions and future changes of precipitation extremes.


AS09-A024
Long-term Variability of Temperature and Precipitation in Eastern China and the Underlying Mechanisms

Wen ZHOU#+, Yue ZHANG
Fudan University

This study explores the coupled variability of temperature and precipitation in eastern China during summer using multivariate EOF analysis. Two leading modes are identified and analyzed, with the first mode showing a robust increasing trend in temperature and a robust drying trend in precipitation in the region north of the Yangtze River; the second mode suggests a systematic decadal variability in temperature and precipitation. The underlying mechanisms for these leading modes are revealed through correlation and composite analysis. A negative Pacific-Japan teleconnection pattern in the lower troposphere and a stationary Rossby wave train across Eurasia in the upper troposphere are contributing factors to the trend mode. The trend component is closely tied to global warming, and also to increased sea surface temperature anomalies over the western Atlantic Ocean, which amplify the wave train teleconnection across Eurasia. The decadal variability is found to be associated with internal decadal change in interannual variability in the atmosphere, specifically, the decadal alternation of active oscillations above the North Atlantic and Pacific, which are likely related to the North Atlantic Oscillation (NAO) and Pacific Decadal Oscillation (PDO) modes, respectively. Further analysis illustrates that the NAO has a stronger impact during its active periods, while the PDO tends to have an opposite influence to the NAO when the NAO is inactive.


Mon-31 Jul | 1:10 - 3:10 | MR329
AS02 - Climate Change and Tropical Climatic Hazards in Asia Oceania

Session Chair(s): Johnny CHAN, Asia-Pacific Typhoon Collaborative Research Center

AS02-A019 | Invited
Reprocessing of Global Satellite Mapping of Precipitation (GSMaP) Product

Takuji KUBOTA#+, Munehisa YAMAMOTO, Moeka YAMAJI
Japan Aerospace Exploration Agency

The Global Satellite Mapping for Precipitation (GSMaP) produces high-resolution and high-frequent global rainfall map based on multi-satellite passive microwave radiometer observations with information from the Geostationary InfraRed (IR) instruments (Kubota et al. 2020). Outputproduct of GSMaP algorithm is 0.1-degree grid for horizontal resolution and 1-hour for temporal resolution. Images and data of the GSMaP are available at JAXA GSMaP website (http://sharaku.eorc.jaxa.jp/GSMaP/). The GSMaP has been developed by the Japan Aerospace Exploration Agency (JAXA). The JAXA has participated in the World Meteorological Organization (WMO) has been initiated the Space-based Weather and Climate Extremes Monitoring (SWCEM) (Kuleshov et al. 2020) and provided 22-yr GSMaP data. Currently, the gauge-adjusted near-real-time version 6 (GNRT6) of the GSMaP (Tashima et al. 2020) has been distributed to the SWCEM.In December 2021, the GSMaP algorithm was updated to version 8 by implementing various improvements to better estimate precipitation (Kubota et al. 2022). We plan the reprocessing of the GSMaP version 8 in a period during the past 24 years ”since Jan. 1998” using JAXA super computer system (JSS3). Past GSMaP products did not cover the first 2 years of TRMM era (1998-Mar. 2000) due to lack of NOAA CPC-4km Global IR dataset. There is a possibility that GridSat-B1 data (Knapp et al. 2011) enables to fill the lack of period. In order to extend the period of the GSMaP before 2000, the validity of GridSat-B1 data is investigated in this study.


AS02-A020
A Machine-learning Aided Quantile-mapping Method for Calibration of Satellite Rainfall Estimates

Wee Leng TAN#+, Thea TURKINGTON
Centre for Climate Research Singapore

Satellite rainfall estimates provide valuable spatial information of precipitation, although biases in the estimate need to be corrected, especially for regions near the equator with large spatial and temporal variability in precipitation. It was found that the large variability in the bias can significantly reduce the benefit of quantile-mapping methods for the calibration of the satellite rainfall estimates with gauge measurements. Further investigations found that the bias is possibly related to the type of weather system and this bias can be sub-divided into different categories accordingly. In this presentation, the results of the calibration of weekly and sub-weekly rainfall from the SWCEM-EAWP (Space-based Weather and Climate Extremes Monitoring - East Asia West Pacific) products (CMROPH-CRT and GSMaP_GNRTv6) using rainfall measurements from subset of gauges over Singapore will be presented. The categorization of the rainfall to the respective bias group is first trained using machine learning methods and followed by quantile-mapping for calibration. The improvement in the performance in the machine-learning aided quantile mapping is then evaluated with the full set of rain gauges in Singapore, and compared to the satellite rainfall estimates before calibration and with just quantile mapping calibration applied.


AS02-A012 | Invited
Seasonal Tropical Cyclone Landfall Forecasts Along the East Asia Coast

Johnny CHAN1,2#+
1Asia-Pacific Typhoon Collaborative Research Center, 2City University of Hong Kong

Quite a few real-time forecasts of the annual frequency of tropical cyclones (TCs) have been made in recent years, using statistical and dynamical approaches. However, such forecasts are not very useful for disaster preparedness. Since 2015, we have been making seasonal forecasts of the number of TCs making landfall in different regions along the East Asia coast using a regional climate model with boundary conditions from the Climate Forecast System (CFS). In this paper, how such forecasts are made will be presented together with verification statistics for the last six years. A possible extension of this approach to forecast the intensity of these landfalling TCs will also be discussed.


AS02-A017
Monitoring and Predicting Marine Heatwaves in Vanuatu

Jessica BHARDWAJ#+
Bureau of Meteorology

Marine Heatwaves (MHWs) have dire impacts on aquatic ecosystems and the communities that rely on them for livelihood, recreation, and cultural identity. In Vanuatu, a MHW event in 2016 led to record high sea surface temperatures with widespread reports of fish mortality. Given the severity of impacts, monitoring and predicting MHW events is critical in allowing communities and key sectors to effectively manage (and where possible) mitigate the impacts of MHW events. In this study, we use in situ data, satellite data and dynamical forecasts to derive MHW climatologies and investigate key MHW events. Results for the common period of overlap between all examined datasets (1981-2018) will be presented.


AS02-A016
Pairing Monitoring Datasets with Probabilistic Forecasts to Provide Early Warning of Drought in Australia

Jessica BHARDWAJ#+
Bureau of Meteorology

Droughts are a cyclical feature of Australia's climate and have compounding effects on agricultural productivity and wellbeing. Understanding future conditions in context of antecedent observations is critical to providing informed early warning of drought. In this study we pair probabilistic seasonal forecasts with monitoring datasets to provide early warning of drought. Hindcasts from the Bureau of Meteorology's sub seasonal to seasonal forecast model, ACCESS-S2, are paired with MSWEP satellite blended precipitation data and AWRA-L water balance modelled soil moisture and evapotranspiration. Principal Component Analysis (PCA) is used to derive objective weightings to combine precipitation, soil moisture and evapotranspiration percentiles in a multivariate manner similar to the U.S. Drought Monitor. The final DEWS maps overlay forecasting information with PCA-weighted antecedent conditions. We produce 1-, 3- and 6-month maps and analyse drought concern over the common period of overlap between our datasets (1981-2018) and conduct case studies for the 1982-1983 Ash Wednesday tinder drought and the 1997-2001 Millennium drought. We validate PCA-weighted maps with satellite vegetation data and find performance is strongest over the Murray Darling Basin region (R = 0.63, p= 0.009) and poorest over Central interior Australia (insignificant correlations). We also validated PCA-weighted maps using agricultural commodity data from ABARES. Significant negative correlations at 95%, 99% and 99.9% confidence intervals were found between %-Area in drought category and crop cultivation area; export volume/value; crop yield; and rural debt. Our findings indicate that early warning of drought can be categorised by concern – wherein dry antecedent conditions and dry forecasted conditions are of highest concern. Our proof-of-concept drought early warning system contributes to the growing body of proactive drought research. In a drought vulnerable future, operationalising and communicating drought early warnings will be critical to reducing the harmful impacts of drought on economies, environments, and people.


AS02-A001
Top Ten Reasons for the Necessity of Global Adaptation to Climate Change

Menachem LURIA#+
The Hebrew University of Jerusalem

There is a near consensus among scientists that the average global temperature will increase in the next several decades. Many international organizations are taking steps to reduce this anticipated phenomenon by as much as possible. However, there are many forces, social and economic interests that make this goal almost impossible to achieve. Significant climate changes will occur and the world must be prepared. The talk will discuss the top ten reasons why the efforts taken by certain governments and motivated people are not going to be enough. The USA supreme court decision from June 2022; Increased world population; Rapid increase in GDP mainly in developing countries; Increased global demand for electric power; The coal oil and Gas Industry; Increased demand for air and ocean transportation and the tourism Industry; The increased demand for food, mainly but not only from live stock; Increased demand for raw materials mainly steel and cement; The Garment industry and Production of solar panels and storage devices and 


AS02-A022
Uncertainty in Multidecadal and Future Changes of Tropical Pacific SST Zonal Gradient: Internal Variability and Model Spread

Lu DONG#+
Ocean University of China

The zonal sea surface temperature (SST) gradient over tropical Pacific is important for global climate and known to be a pacemaker of global warming. During recent decades, observations show a “La Niña-like” strengthening of the zonal SST gradient, whereas most climate models produce an “El Niño-like” weakening of this gradient. There is also large model uncertainty in the future projection of this gradient change under global warming. Quantifying the sources and understanding the mechanisms for the uncertainty is needed to reconcile the discrepancy between observations and models and reduce model uncertainty of future projections. Here we use a total of 342 simulations, including six large ensembles, 36 CMIP5 and 36 CMIP6 models, to quantify the relative contribution of internal variability and model spread to the uncertainty in this gradient change on multidecadal timescales and future projections. On multidecadal timescales, the uncertainty of zonal SST gradient change over the tropical Pacific is dominated by internal variability. Although external forcing is increasing under global warming, the ratio of internal uncertainty is decreasing but still >80% at the end of the 21st century. The Pacific Decadal Oscillation (PDO) is revealed as the key internal mode influencing the uncertainty of the multidecadal changes. The PDO-related SST pattern exhibits a pronounced zonal gradient over the tropical Pacific. For future projection, the uncertainty of zonal SST gradient change over the tropical Pacific is mainly from the model spread in response to external forcing. Based on future change between 2070-2099 and 1961-1990, model spread accounts for ~70% of the total uncertainty. The SST change in the western and eastern tropical Pacific dominates the total uncertainty of the zonal SST gradient for CMIP5 and CMIP6 models, respectively. That is mainly due to the stronger low cloud positive feedback over the southeastern Pacific among CMIP6 models.


AS02-A014
Optimising Satellite Altimetry Data for Studying the Interaction of Ocean and Atmosphere

Noor Nabilah ABDULLAH#+, Dudy Darmawan WIJAYA, Fathin NURZAMAN, Meilano IRWAN, Wedyanto KUNTJORO
Bandung Institute of Technology

Satellite altimetry is a matured technology that provides accurate measurements of ocean geophysical information of sea surface heights (SSHs), significant wave heights (SWHs), and wind speed. It was designed specifically for observing ocean’s geo-physicality and dynamics. Furthermore, these technologies also have the potential to be developed to study the ocean and atmosphere, simultaneously. It is well known that satellite altimetry is also equipped with sensors to measure atmospheric components to provide corrections for the range measurement. On-board microwave radiometer measures atmospheric water vapour to provide wet path delay correction for the main altimeter range measurement. This perspective develops a new potential for satellite altimetry to also be exploited to observe the atmosphere. It has been proven that the interaction of ocean and atmosphere have a significant role on influencing climate phenomena and their variations through its complex process. Several studies also found that the uncommon reactions between anomalies in atmosphere and ocean hydrological cycle occurred due to rapid climate changes resulting in hydro-meteorological catastrophe. These situations make a thorough study about the interaction between ocean and atmospheric component are necessary. Thus, this study is performed to leverage satellite altimetry sea level anomaly and water vapour measurement to analyse the complex interactions between the ocean and atmosphere to determine the nature and characteristics of these interactions. Using both ocean and atmosphere measurement from satellite altimetry not only present a new potential of the satellite itself, but also a way to overcome the drawback of previous ocean-atmosphere studies, which has temporal and spatial disparities as each parameter were observed using different platforms at different time and locations. Moreover, by multi-missions observations, spatial and temporal resolution are enhanced, making it reliable enough to monitor long periodic phenomena, such as El Niño–Southern Oscillation (ENSO), Indian Ocean Dipole (IOD), Madden-Julian Oscillation (MJO), and monsoons.


Mon-31 Jul | 1:10 - 3:10 | MR331
AS18 - The Science and Prediction of Tropical Cyclones

Session Chair(s): Qinglan LI, Chinese Academy of Sciences, Masashi MINAMIDE, The University of Tokyo

AS18-A057 | Invited
Multi-scale Interaction and Predictability of the Onset of Tropical Cyclone Rapid Intensification

Masashi MINAMIDE1,2#+, Derek POSSELT2
1The University of Tokyo, 2Jet Propulsion Laboratory

Predicting tropical cyclone intensity changes, especially rapid intensification (RI), has been a more challenging topic than tropical cyclone tracking because of its multi-scale physical process with significant contributions from convective-scale phenomena. Before intensification, tropical cyclones experience precession process, in which tilted vortices rotate counterclockwise around the center of circulation, and develop an axisymmetric structure. The forecast uncertainty in precession process limits the predictability of early-stage intensification of TCs. In this study, we have explored the contribution of moist convective activity to the variability of TC precession process using a simple toy-model of the vortex precession process, together with fully dynamic ensemble-based sensitivity experiments using convection-permitting Weather Research and Forecasting model (WRF-ARW) simulations. The results indicate the potential existence of a threshold in vortex strength and structure that governs whether it completes precession and initiates RI. Given the strong nonlinearity of the onset process of RI, the advancement of our understanding of the uncertainty sources will provide an insight about the observation network that may effectively constrain the TC forecasting.


AS18-A005
Tropical Cyclones Intensity Prediction in the Western North Pacific Using Gradient Boosted Regression Tree Model

Qinglan LI#+, Gangya ZHU
Chinese Academy of Sciences

As an artificial intelligence method, machine learning (ML) has been widely used in prediction models of high-dimensional datasets. This study proposes an ML method, the Gradient Boosted Regression Tree (GBRT), to predict the intensity changes of tropical cyclones (TCs) in the Western North Pacific at 12-, 24-, 36-, 48-, 60-, and 72-h (hr) forecasting lead time and the model is optimized by the Bayesian Optimization algorithm. The model predictands are the TCs intensity changes at different forecasting lead times, obtained from the best track data of the Shanghai Typhoon Institute (STI) and the Joint Typhoon Warning Center (JTWC) from 2000 to 2019. The model predictors are the synoptic variables, climatological and persistent variables derived from the reanalysis data obtained from the National Centers for Environmental Prediction (NCEP), and the sea surface temperature (SST) data obtained from the National Oceanic and Atmospheric Administration (NOAA). The results show that the GBRT model can capture the TCs intensity changes well for the succeeding 12-h, 24-h, 36-h, and 72-h. Compared with the traditional multiple linear regression (MLR) model, the GBRT model has better performance in predicting TCs intensity changes. Compared with the MLR model, R2 of the GBRT model for TCs intensity forecast increases by an average of 8.47% and 4.45% for STI data and JTWC data. MAE (RMSE) drops by 26.24% (25.14%) and 10.51% (4.68%) for the two datasets, respectively. The potential future intensity change (POT), the intensity changes during the previous 12 h (Dvmax), Initial storm maximum wind speed (Vmax), SST, and the Sea-Land ratio are the most significant predictors for the GBRT model in predicting TCs intensity change over the Western North Pacific.


AS18-A051
Intensification Study of Tropical Cyclone Batsirai (2022) Using High-resolution Mesoscale Numerical Model

Keunok LEE1#+, Soline BIELLI2
1CNRS - Université de La Réunion - Météo-France, 2Université de La Réunion - CNRS

The aim of this study is to enhance our understanding about the intensification phase of tropical cyclones that occurred in the southwest Indian Ocean. Tropical cyclone (TC) Batsirai (2022) which unexpectedly and rapidly intensified into a Saffir-Simpson Category 4 cyclone (lowest sea level pressure of 934 hPa) after undergoing an eyewall replacement cycle was selected in this study. During the passage of the intensified tropical cyclone (1−4 February 2022), Mascarenes Islands (i.e. Rodrigue, Mauritius, Réunion) were heavily impacted though the effects were relatively minor; the major devastating hazards were reported in Madagascar (121 deaths). The French cloud-resolving mesoscale model, Meso-NH, successfully reproduced the lifecycle of TC Batsirai. In this study, the intensification phase of TC Batsirai has been focused to understand the physical and thermodynamical processes responsible for the intensity change of the tropical cyclone. In addition, the impact of the orography of Mascarenes Islands on localized heavy rainfall and strong winds has been studied. The detailed analysis using the numerical simulation results with fine horizontal grid spacings (250 m) has been done. The key results will be presented at the conference.


AS18-A066
A Comparison Study of Kinetic and Potential Energy Budgets of Typhoon Mujigae (2015) Between the Slow and Rapid Intensification

Chi ZHANG#+
Zhejiang University

In this study, kinetic and potential energy budgets of Typhoon Mujigae (2015) are compared in slow (SI) and rapid (RI) intensification periods. The high-resolution numerical simulation data of Mujigae are validated with observations and are used for comparison analysis. The analysis of kinetic energy budgets reveals that the conversion between asymmetric rotational kinetic energy and symmetric rotational kinetic energy play a key role in determining the differences in the tendencies of symmetric and asymmetric rotational kinetic energy between RI and SI in the lower troposphere. Asymmetric rotational kinetic energy is converted to symmetric kinetic energy in RI, whereas symmetric rotational kinetic energy is converted to asymmetric kinetic energy in SI. This can explain why the symmetric rotational kinetic energy tendency is larger in RI than in SI, but asymmetric rotational kinetic energy tendency is smaller in RI than in SI. In both RI and SI, both conversions from symmetric divergent and environmental kinetic energy to symmetric rotational kinetic energy contributed to the increase in symmetric rotational kinetic energy. The analysis of symmetric divergent kinetic energy budget shows that conversion from symmetric divergent kinetic energy to symmetric rotational kinetic energy is nearly balanced out by the work done by symmetric divergent winds against pressure gradient, which is further related to the conversion from potential energy mainly due to the latent heat release. The detailed results will be presented in the conference.


AS18-A059
Impact of Soil Moisture Initialization on Poleward-moving Tropical Cyclone Forecasts

Jinyoung PARK+, Dong-Hyun CHA#
Ulsan National Institute of Science and Technology

Tropical cyclones (TCs) moving poleward to mid-latitudes in the western North Pacific basin are complex to forecast their track since their tracks are largely influenced by the upper-level synoptic fields in subtropical and mid-latitude regions (i.e., western North Pacific subtropical high, mid-latitude trough, and jet stream). Thus, forecast performances are especially poor when TCs approach the East Asian region. It is known that soil moisture (SM) modulates the total available energy into sensible heat fluxes (SHF) and latent heat fluxes (LHF) at the land surface. It can affect the atmospheric temperature, clouds, and even precipitation through land-atmosphere interaction. Thus, those land surface processes are necessary for accurate weather forecasts or climate predictions. Therefore, we prescribed two types of SM data for the initial condition of the Weather Research and Forecasting (WRF) model to investigate the sensitivity of the SM initialization on the TC forecasts. The Global Land Data Assimilation System (GLDAS) Version 2.1 and the European Centre for Medium-Range Weather Forecasts (ECMWF) Reanalysis v5 (ERA5) were selected in this study. The result showed that ERA5 SM data had more wet biases than GLDAS data over the whole simulations except for some areas located south of Mongolia. Also, TC intensity forecast performances were similar in both runs, while TC track forecast performances were improved in the experiments with GLDAS data. The differences in track forecasts between the two runs were more considerable during the landfall period. In addition, in the experiments with ERA5 data, simulated TCs tended to move westward compared to the experiments with GLDAS data due to the strengthened interaction between simulated TCs and the mid-latitude trough. This study showed that it is important to provide realistic SM data to improve the TC track forecast performances during the TC landfall period.


AS18-A009
Prediction of Tropical Cyclogenesis Based on Machine Learning Methods and its Shap Interpretation

Chi Lok LOI#+, Chun-Chieh WU, Yu-Chiao LIANG
National Taiwan University

Predicting Tropical Cyclogenesis has long been a challenging research task. Machine learning methods recently have been shown to withhold a high prediction skill for forecasting tropical cyclogenesis. In this study, we first use Kalman filters applied on the Gaussian-smoothed 850-hPa vorticity field to label tropical disturbances. Dynamic and thermodynamic variables, such as wind shear and sea surface temperature, are extracted following the disturbance center in a Lagrangian sense. Three machine learning models with varying complexity: a random forest, a support vector machine and a neural network, are trained to classify developing and non-developing tropical disturbances at a forecast lead time of 24 hours. All of the three models have displayed consistently good performance, with the neural network having the highest f1-scores of 0.79. SHAPley values analysis shows that the mid-level vorticity at 500 hPa is the most essential feature in deciding if a tropical disturbance is developing or non-developing for all the models. Wind shear and tilting are found to possess a certain level of importance as well. Our results suggest that rich mid-level cyclonic vorticity in a mesoscale convective vortex is instrumental in the subsequent low-level spin-up of the disturbance and is an essential sign for the prediction of Tropical Cyclogenesis.


AS18-A031
Influence of Region-dependent Error Growth on Predictability of Tropical Cyclone Track and Intensity in High-resolution HWRF Ensembles

Jie FENG#+
Fudan University

The prediction of tropical cyclones (TCs) has progressively improved in the past few decades. How long can we further extend skillful TC prediction? The answer to this question relies on in-depth studies about TC intrinsic predictability. In this study, the HWRF-based convection-resolving ensemble forecasts were adopted with perturbed initial conditions to study the error growth and intrinsic predictability of TCs. The new aspect of our study is the focus on the sensitivity of TC track and intensity predictability on region-dependent initial errors. The main conclusions include: (1) the most sensitive region for TC track forecasts is case-dependent, for TC intensity forecasts, however, consistently locates within the TC vortex. (2) The 0-2 wave number structures of the TC inherent vortex flow can be predicted for more than 4 days, which is primarily determined by the predictability of the synoptic-scale environment. In contrast, the remaining components (wave numbers >2) are only predictable for a few hours. These finer scales, despite much less variance than larger scales, saturate rapidly and intensively limit the predictability of TC intensity which is generally defined by the maximum surface wind at a certain point in time and space rather than the azimuthal mean wind.


AS18-A021
Effect of the Initial Vortex Vertical Structure on Early Development of an Axisymmetric Tropical Cyclone

Ke PENG1#+, Juan FANG2
1Nanjing University of Information Science & Technology, 2Nanjing University

With the nonhydrostatic axisymmetric cloud-resolving model CM1, two sets of ensemble runs are conducted to study the influence of initial vortex depth on the early development of an idealized tropical cyclone (TC). It is found that with the shallow initial vortex, the intensification rate (IR) is smaller and the TC takes a longer time to reach a state of slantwise moist neutrality. These behaviors are primarily ascribed to the less active convection in the shallow case. In contrast to the deep initial vortex, the shallow initial vortex is characterized by a more stable stratification in the lower troposphere and a smaller gradient of angular momentum (M) in the mid-to-upper troposphere. The former tends to hinder the occurrence of deep convection in the TC while the latter makes it difficult to intensify the mid-toupper level vortex and to establish a deep vortex. Thus, deep convection bursts intermittently in the early developing stage of the TC originating from the shallow vortex. During the periods of inactive convection, the TC weakens by the decline of M source associated with reduced horizontal advection, which is overwhelmed by sinks of M from moderately decreased vertical advection and nearly-constant dissipation term. Therefore, the IR of the TC is smaller in the early developing stage and the development of TC from the shallow vortex usually needs a longer time to build the steady deep secondary circulation favorable for more rapid intensification.


Tue-01 Aug | 8:15 - 10:00 | MR323
AS18 - The Science and Prediction of Tropical Cyclones

Session Chair(s): Tsung-Lin HSIEH, Princeton University, Kosuke ITO, Kyoto University

AS18-A011
Maintenance Mechanisms of the Long-lived Concentric Eyewall Structure of Typhoon Lekima (2019): Axisymmetric Perspective

Shang-En LI#+, Ming-Jen YANG, Hung-Chi KUO
National Taiwan University

This study examines the long-lived concentric eyewall structure of Typhoon Lekima (2019) from an axisymmetric perspective. Possible maintenance mechanisms for the concentric eyewalls are investigated using a high-resolution WRF simulation (nested down to 1-km horizontal grid size). The secondary-circulation responses to the latent heating in the inner eyewall, moat and outer eyewall are diagnosed by solving the Sawyer-Eliassen equation individually to examine the corresponding contribution to the moat downdraft. By calculating the dynamic efficiency factor (DEF), the conversion of latent heating to kinetic energy is evaluated in the moisture-restricted inner eyewall. The Sawyer-Eliassen diagnoses show that the moat downdraft was contributed mainly by latent heating in the inner and outer eyewall, with a secondary contribution from latent cooling in the moat after concentric eyewall formation. DEF diagnoses show that the conversion of latent heating to kinetic energy in the inner eyewall was more efficient than in the outer eyewall. Although tangential wind within the boundary layer was weakened by friction, the compensative tangential wind in the inner eyewall was larger than in the outer eyewall. The compensative tangential wind indirectly accumulated moisture from the sea surface in the moat, aiding the moisture supply to the inner eyewall and enhancing the amount of kinetic energy converted from latent heating. Although the inner eyewall of Typhoon Lekima eventually weakens due to the moisture cut off from the outer eyewall, the inner eyewall can still be maintained for tens of hours by the high DEF from latent heating.


AS18-A020
On the Role of Cloud Radiative Effect in Tropical Cyclogenesis

Chun-Kai HSU#+, Chun-Chieh WU
National Taiwan University

Idealized model simulations have shown that cloud radiative effect (CRE) can accelerate early development of tropical cyclones (TCs). Deep convective region near TC inner cores receives more energy than surrounding environment, and this spatial radiative heating difference can further drive a secondary circulation, transporting angular momentum and water vapor into TC center, thus favoring the TC intensification. However, the quantitative contribution of radiation to TC genesis in observation has not been well documented and need further investigation. In this study, tropical cloud clusters are identified according to their brightness temperature, then classified into developing and non-developing systems based on IBTrACS data. Satellite observations from CloudSat are used to composite vertical structure of radiative heating and atmospheric cloud radiative effect (ACRE), and to verify the differences between these two groups. Preliminary results show that, for developing systems, the upper troposphere absorbs more shortwave but lose more longwave from clouds. While at mid-level, more longwave energy is trapped but less shortwave energy can be transmitted through deep clouds to these layers. Overall, shortwave ACRE drives anomalous upper-level upward motion, and longwave ACRE promotes mid-level upward motion. Both of these effects enhance the secondary circulation between the convective region and their environment. As for non-developing systems, the general characteristics are similar to those in developing systems, except for smaller deep cloud extent and less radiative heating in surrounding area, implying that the deep convection structure, the cloud canopy extent, the associated cloud radiative effect, and the responded vertical motion could be related to the cyclogenesis process. More quantitative analyses, such as Sawyer-Eliassen equation, are still undergoing to further evaluate how secondary circulation and TC genesis process would respond to the radiative heating difference between developing and non-developing systems.


AS18-A053
Super Typhoon Hinnamnor (2022) with a Record-breaking Lifespan Over the Western North Pacific

Qian WANG1+, Dajun ZHAO2#, Yihong DUAN3, Shoude GUAN4
1Fudan University, 2Chinese Academy of Meteorological Sciences, 3China Meteorological Administration, 4Ocean University of China

Super Typhoon Hinnamnor (2022) was rare and unique in the record over the western North Pacific as throughout its lifespan it featured all of the major frontier issues in typhoon research currently. Specifically, in different stages of its lifespan, it had a sudden change of track, underwent rapid intensification, interacted and merged with another vortex, expanded in size, underwent rapid weakening and had a strong cold wake, eyewall replacement, and extratropical transition. Therefore, a timely identification and review of these typical features of Hinnamnor (2022), as reported in this article, will help update and enrich the case sets for each of these scientific issues and provide a background for more in-depth mechanistic studies of typhoon track, intensity, and structural changes in the future. We believe that Hinnamnor (2022) can serve as an excellent benchmark to quickly evaluate the overall performance of different typhoon numerical models in predicting its track, intensity, and structural changes.


AS18-A055 | Invited
Changes in the Structure and Intensity of Tropical Cyclones Associated with Diurnal Pulsing

Weixin XU#+, Xinyan ZHANG
Sun Yat-sen University

One of the most prominent diurnal cycle features in tropical cyclones (TCs) is the radially outward propagation of a cooling signal in the upper-level clouds, the so-called diurnal pulse (DP). Previous studies suggested that some of the DPs occur in the deeper convective layer and therefore may impact the TC structure and intensity. This study investigates how the internal structures and intensity will change associated with DPs in global TCs using 18 years of multi-source satellite observations. Over 3000 DP events are identified based on objective method using satellite infrared data. Satellite microwave observations and spaceborne radar measurements are used to examine the changes of the TC convective structures related to DP events. Results show that the precipitation, microwave ice scattering, radar-echo top height, and lightning in the TC inner core are all markedly enhanced on DP days compared to non-DP days. Spaceborne radar observations further indicate that convection becomes deeper in the upshear quadrants with the presence of DPs and convective depths remain similar in the downshear quadrants. These changes in the TC internal structures are consistent to changes in rapidly intensifying TCs reported in the literature. In fact, this study shows that rapidly intensifying TCs have a higher frequency of the long-duration DP event and significantly longer DP duration than steady-state and gradually intensifying TCs. In short, DP implies a coherent pattern of the convective structure in the TC’s evolution and provides important implications for TC intensity change.


AS18-A048
Cloud-radiation Feedback Prevents Tropical Cyclones from Reaching Higher Intensities

Bolei YANG1#+, Xi GUO2, Jian-Feng GU3, Ji NIE1
1Peking University, 2Jiangsu Meteorological Observatory, 3University of Reading

The prediction of tropical cyclone (TC) intensity remains a major scientific challenge. Recent studies indicate that cloud-radiation feedback (CRF) plays a positive role in the intensification of TCs during their genesis. However, little attention has been given to how CRF affects TC intensity after genesis. This study shows that CRF may prevents TCs from attaining higher maximum intensities. The ascending motion induced by the anomalous radiative heating of TC promotes more latent heating on the outer side of the upper eyewall, resulting in a more tilted eyewall. A more tilted eyewall leads to a larger inner-core size and less inward flux of absolute vertical vorticity within the inner core, thus preventing the TC from reaching higher intensity. This work highlights that CRF may affect TC intensity by modulating the structure of the inner-core convection, and further advances our understanding of the interaction between radiation effect and TC dynamics


AS18-A058
Characteristics of Deep Convective Clouds, Precipitation, and Cloud Properties of Rapidly Intensifying Tropical Cyclones in the Western North Pacific

Jason Pajimola PUNAY1#+, Chian-Yi LIU2, Chun-Chieh WU3, Kaoshen CHUNG4, Putu ARYASTANA5
1Bicol University, 2Academia Sinica, 3National Taiwan University, 4National Central University, 5Warmadewa University

Toward the understanding of rapid intensification (RI) of tropical cyclones (TCs) in the western North Pacific, the TC's deep convective cloud (DCC), precipitation, and cloud properties in terms of cloud effective radius, optical thickness, and top height from satellite observations are investigated. Mean and radial distributions of the variables at different intensity stages and intensification categories are examined. The relationship indicates that the DCC percentage and temperature, especially their radial distributions, could be used to identify an impending RI regardless of TC intensity. Meanwhile, the mean and radial distribution of precipitation may discriminate RI from non-RI in tropical depression (TD) and tropical storm (TS). The radial distribution of the cloud properties in rapidly intensifying TD and TS also suggest that most of the clouds near the center of the storm has deepened already while those that are far from the center are generally in developing or dissipating stage. Moreover, rapidly intensifying TCs, regardless of their intensities, manifest common DCC, precipitation, and cloud properties characteristics near the TC center. It is to be noted that the different mean and radial distribution characteristics of the variables between initial and continuing stages of RI are inferred to be artifacts of their intensities and RI rates (or radius of maximum wind sizes) rather than whether the TCs are at the onset or 24 hr of RI.


AS18-A065
Uncertainty in Tropical Cyclone Frequency Projection Linked to Uncertainty in Western North Pacific Cloud Feedback

Tsung-Lin HSIEH#+
Princeton University

The Western North Pacific basin has large uncertainty in future tropical cyclone (TC) frequency projection across climate models, but the underlying reason has been unclear. We show that uncertainty in TC frequency projection is highly correlated with uncertainty in the response of clouds to sea surface warming. Based on the previously developed seed propensity index and gross moist stability theory, we hypothesize that the pattern of cloud response influences TC frequency through its radiative effect on the atmospheric column energy budget. Cloud radiative heating over the Western North Pacific drives anomalous vertical ascent in the large-scale circulation, generating more precursory vortices and seeding more TCs. This hypothesis is supported by numerical experiments with perturbed radiative heating rates and sea surface temperature using global atmospheric models developed at the Geophysical Fluid Dynamics Laboratory. We show that uncertainty in Western North Pacific TC response is reduced when controlling for the radiative heating rate. We further show that cloud and TC response in the Western North Pacific has global impact on the top-of-atmosphere energy budget, using simulations with localized sea surface temperature perturbations. The results suggest that Western North Pacific TC frequency tends to decrease in a scenario with more positive cloud feedback; while the frequency tends to increase in a scenario with more negative cloud feedback.


Tue-01 Aug | 8:15 - 10:00 | MR327
AS23 - Observations, Remote Sensing, and Modeling of Tropospheric Composition and Air Quality in Asia and the Transpacific Region

Session Chair(s): Richard ECKMAN, National Aeronautics and Space Administration

AS23-A066 | Invited
An Update on Plans for the Airborne and Satellite Investigation of Asian Air Quality (ASIA-AQ)

James CRAWFORD1#+, Barry LEFER2, Limseok CHANG3, Gangwoong LEE4, Jhoon KIM5, Rokjin J. PARK6, Chang-Keun SONG7, Laura JUDD8,1, Katherine TRAVIS8,1
1NASA Langley Research Center, 2National Aeronautics and Space Administration, 3National Institute of Environmental Research, 4Hankuk University of Foreign Studies, 5Yonsei University, 6Seoul National University, 7Ulsan National Institute of Science and Technology, 8National Center for Atmospheric Research

The Airborne and Satellite Investigation of Asian Air Quality is a multi-perspective field study (aircraft, ground, satellite) planned to take place in early 2024. It is jointly sponsored by NIER (Korea) and NASA (United States) with flights over South Korea as a definite part of the plan and flights over a second partner country still under negotiation at the time of this abstract. The project will make an important contribution to science-based validation of the Geostationary Environment Monitoring Spectrometer (GEMS) which serves to provide an important catalyst for increased dialogue and cooperation among Asian countries to address air quality. In combination with satellite and ground observations, data will support analyses for assessment of emissions, model evaluation, process-level understanding of secondary pollutants (i.e., fine particles and ozone), and satellite validation and interpretation. Aircraft observations can provide invaluable context to the satellite and ground-based perspectives that are used more routinely to inform air quality models used for both forecasting and attribution. Important information from aircraft includes measuring detailed composition for source fingerprinting, vertical profiling of composition for satellite validation and model assessment, observing chemical and dynamical processes affecting secondary pollution (i.e., fine particles and ozone), relating specific VOC mixtures to satellite HCHO, providing fine scale pollution mapping with remote sensors, etc. Such information is critical for understanding the local factors influencing air quality for a specific location, quantifying emission sources, and assessing potential mitigation strategies for decision makers. This presentation will provide an important update on final decisions for deployment locations and planned observing strategies.


AS23-A054
GEMS - Two Years of Operation

Jhoon KIM1#+, Dongwon LEE2, Myoung Hwan AHN3, Jae KIM4, Rokjin J. PARK5, Hanlim LEE6, Chul Han SONG7, Yong-Sang CHOI3, Kwon Ho LEE8, Jung-Moon YOO3, Seon Ki PARK3, Kwang-Mog LEE9, Chang-Keun SONG10, Sang-Woo KIM5, Si-Wan KIM1, Jongmin YOON2, Won-Jin LEE2, Hyunkee HONG2, Chang-Seok LEE2, Won-Jun CHOI2, Yuha KIM2, Kyung-Jung MOON2, Dai Ho KO11, Seung-Hoon LEE11, Yeseul CHO1, Sangseo PARK10, Heesung CHONG12, Sujung GO13, Hana LEE1, Mina KANG3, Mijin EO3, Junsung PARK6, Kanghyun BAEK14,4, Gyuyeon KIM3, Xiong LIU12, Kelly CHANCE12, Pepijn VEEFKIND15, Jassim AL-SAADI13, Ben VEIHEMLANN16, GEMS SCIENCE TEAM17
1Yonsei University, 2National Institute of Environmental Research, 3Ewha Womans University, 4Pusan National University, 5Seoul National University, 6Pukyong National University, 7Gwangju Institute of Science and Technology, 8Gangneung-Wonju National University, 9Kyungpook National University, 10Ulsan National Institute of Science and Technology, 11Korea Aerospace Research Institute, 12Center for Astrophysics | Harvard & Smithsonian, 13NASA Goddard Space Flight Center, 14National Center for Atmospheric Research, 15Royal Netherlands Meteorological Institute, 16European Space Research and Technology Centre, 17GEMS.Science.Team

Hourly observations of air quality (AQ) over Asia have been available by the Geostationary Environment Monitoring Spectrometer (GEMS) for the first time from a geostationary Earth orbit (GEO) since its launch in February 2020. After 8-month in-orbit tests, GEMS has observed column amounts of atmospheric pollutants (O3, NO2, SO2, HCHO, CHOCHO, and aerosols) to capture their diurnal variations with the UV–visible spectrometer at 0.6 nm spectral resolution and sophisticated retrieval algorithms. Details of the GEMS mission are presented, including calibrations, results, validations, and case studies including volcanic eruption, dusts, and urban pollution. L2 algorithms have been updated for version 2 and the products were released on November 30, 2022. In version 2, there are noticeable improvements in trace gases from updated AMF and the separation of stratospheric/tropospheric components. Ongoing calibration/validation activities including the 2022 GMAP/SIJAQ campaign and international CAL/VAL team works are critical to diagnose and improve the overall data quality. The GEMS retrievals indicate good agreements from the validation campaign, but still require further improvement in L1 processing. We start testing improvements for L1 processing including BTDF correction. Faster sampling rates at higher spatial resolution increase the probability of finding cloud-free pixels, leading to more observations of aerosols and trace gases than has been possible from LEO. GEMS will be joined by NASA’s Tropospheric Emissions: Monitoring of Pollution (TEMPO) this year and ESA’s Sentinel-4 to form a GEO AQ satellite constellation in late 2024, respectively, as recognized by the Committee on Earth Observation Satellites (CEOS).


AS23-A001
Impacts of Geostationary Environment Monitoring Spectrometer Measurements on NOx Emission Estimates: Observation System Simulation Experiments with GEOS-Chem Adjoint Data Assimilation System

Yi WANG1#+, Xiaodong JIANG2, Minghui TAO3
1China University of Geosciences, Wuhan, 2China University of Geosciences, 3The Aerospace Information Research Institute of the Chinese Academy of Sciences

Although polar-orbit satellite NO2 Vertical Column Density (VCD) observations have been widely used for inverse modeling of the NOx emission inventory, the relative low temporal resolution of polar-orbit satellite data restricts the improvement of the temporal resolution and accuracy of posterior emission inventory. Geostationary Environment Monitoring Spectrometer (GEMS) will provide NO2 VCD observations with unprecedented spatial and temporal resolution, and it is critical to investigate their impacts on NOx emission estimates. In this study, Observing System Simulation Experiments (OSSEs) are performed to quantify the improvements of using GEMS high spatiotemporal NO2 VCD observations to constrain anthropogenic NOx emission over China in relation to the widely used polar-orbit TROPOspheric Monitoring Instrument (TROPOMI) measurements. Our OSSEs use NO2 data from WRF-Chem simulations as the “true” atmosphere and sample it with a configuration designed to represent TROPOMI and GEMS. These TROPOMI and GEMS NO2 “observations” are assimilated through GEOS-Chem adjoint model with the perturbed prior anthropogenic NOx emissions to obtain posterior monthly and daily emission inventories the corresponding diurnal NOx emission profiles. The posterior results based on GEMS “observations” are in better agreement with the “true” anthropogenic NOx emissions used in the WRF-Chem simulations than TROPOMI “observations”.


AS23-A006
High-resolution Optical Depth for Coastal Areas—Near-real-time Production and Assimilation in a Global Aerosol Model

Edward HYER1#+, Christopher CAMACHO1, Andrew LAMBERT2, Chengzhe LI3, Jun WANG3
1Naval Research Laboratory, 2General Dynamics Information Technology, 3The University of Iowa

A novel method developed at the University of Iowa for retrieving aerosol optical depth at high resolution over coastal areas has been implemented using data from the NASA MODIS instrument. This algorithm leverages the spatial autocorrelation of atmospheric properties and the temporal autocorrelation of near-coastal areas to obtain high-resolution retrieved AOD even in areas with significant water-leaving radiance. This code uses MODIS top-of-atmosphere reflectance data and numerous ancillary data sources, and produces retrievals of 550nm aerosol optical depth at the native pixel resolution of MODIS (1km at nadir). This retrieval is applied specifically in coastal areas that are rejected for processing by other MODIS-based algorithms including the Dark Target retrieval. The retrieval code has been ported for near-real-time production by the Naval Research Laboratory. The data have been post-processed to provide the cleanest possible set of observations for data assimilation and incorporate estimated uncertainties required for use in data assimilation. This paper briefly summarizes the novel algorithm, and the skill evaluations that establish its usefulness for characterizing coastal aerosol. The steps taken for near-real-time production are described, including code optimization and linking of near-real-time ancillary data. Post-processing is described, including discussion of the tradeoffs between data coverage and data quality mediated by filtering and aggregation decisions. Estimation of per-observation uncertainties for data assimilation is described. Finally, results from including these observations in the initialization of aerosol forecasts using the Navy Aerosol Analysis and Prediction System are shown, including discussion of the regional, seasonal, and diurnal impacts of this new dataset. The potential for operational use of this product, and more broadly the potential of multi-sensor and hybrid products using both remote sensing and modeling inputs is discussed. 


AS23-A061
Improved Ensemble Kalman Filter Aerosol Data Assimilation by Prognostic Variable Perturbation and Multiphysics

Myong-In LEE#+, Seunghee LEE
Ulsan National Institute of Science and Technology

This study developed an aerosol data assimilation system with the Weather Research and Forecasting model coupled with Chemistry (WRF-Chem) model and Ensemble Kalman Filter (EnKF) approach to improve PM2.5 forecast skill over East Asia. Unlike the variational assimilation method, the advantages of EnKF are flow-dependent background error covariance which is important in a fast-developing air quality system. In spite of considering flow-dependent BEC, the baseline run analysis exhibits poor performance, primarily due to small ensemble spread. This study conducted new two effective methods for increasing ensemble spread: one considering the uncertainty of model physics and the other considering the uncertainty in the prognostic variables. Both methods improved the quality of surface PM analysis substantially, compared with baseline run. And the DA_all experiment which incorporates both uncertainty in model physics and prognostic variables, demonstrates the best performance. The physical perturbation and multiplicative perturbation have a non-linear relationship. The forecast skill is also improved over South Korea and Jing-Jin-Ji area. With the substantial increase of BEC, the revised EnKF system has significantly improved the PM2.5 forecast skills.


AS23-A041
Aerosol Retrieval from MERSI Onboard Chinese Fengyun-3: Performance Over Dark Target and Preliminary Test Over Bright Surface

Leiku YANG#+, Xin PEI, Weiqian JI, Xinyao TIAN, Huan LIU
Henan Polytechnic University

Fengyun-3(FY-3) is the second generation of polar orbit series meteorological satellite built by China, with the capability of global observation. The Medium-Resolution Spectral Imager (MERSI) is one of the main loads of the FY-3 series satellites, belonging to the visible infrared band scanning imager. MERSI and MODIS belong to the same type of sensors. Most of the channel designs are similar and have the ability of aerosol retrieval. Based on the principle of MODIS dark target (DT) algorithm, we build a globally applicable land aerosol retrieval algorithm for the new generation of MERSI-II carried by the newly launched FY-3D to test its quantitative capability. Compared with the DT algorithm of MODIS, the algorithm has been improved mainly in two aspects: MERSI's own surface estimation model and inland-water mask method for haze extraction. We have carried out aerosol retrieval tests on global data in 2019 and 2020, and the validation results using the ground-based observation data of AERONET have reached a high overall accuracy close to MODIS aerosol product. We also used the DT algorithm to conduct aerosol retrieval for MERSI over ocean. The global retrieval and validation test in 2019 shows that the validation results have reached an acceptable accuracy. Recently, we plan to develop a new aerosol retrieval algorithm for the bright surface for MERSI, extending the DT algorithm to the bright target. The algorithm has been preliminarily tested in Northwest China as a research area. The results and validation of two years show that this algorithm can realize the retrieval of aerosol optical thickness over the bright surface by MERSI, and the validation accuracy of the retrieval results for the research area is slightly better than MODIS DB and MAIAC aerosol products. 


AS23-A070
Scale Height of NO2 and its Associations with Meteorological Conditions Using GEMS Measurements

Changqing LIN#+
The Hong Kong University of Science and Technology

Atmospheric boundary layer structure plays a critical role in controlling the occurrence and evolution of extreme air pollution episodes. Our knowledge on the boundary layer structure of Nitrogen dioxides (NO2) is still limited. Satellite remote sensing technique measures vertical column density of NO2 with an extensive spatial and temporal coverage. Recent developments in geostationary satellites (e.g., GEMS) offer new opportunities to observe air pollution with a high resolution of 1 hour. In this study, we applied the GEMS measurements together with various ground measurements to evaluate the variations of the scale height of NO2, which is an important indicator of the vertical structure of NO2. The monthly and diurnal variations of the scale height of NO2 were explored. In particular, the association between the scale height of NO2 and various meteorological factors (e.g., temperature, wind, humidity, air pressure) were evaluated. Our results show that the variations of the vertical structure of NO2 were highly related to the meteorological conditions. For instance, with the subsidence effect of tropical cyclone, the scale height of NO2 were extremely low because most NO2 were accumulated near the ground. We then used random forest regression to estimate the scale height of NO2 based on the meteorological values. Good results with a R2 value of >0.9 were obtained. These analyses enhance our understanding of the vertical structure of NO2 and the relationships between column and surface NO2.


Tue-01 Aug | 8:15 - 10:00 | MR328
AS06 - Assimilation of Space- and Ground-based Water Vapor Observations for Weather Forecasting and GNSS Applications

Session Chair(s): Kefei ZHANG, China University of Mining and Technology, George Zhizhao LIU, The Hong Kong Polytechnic University, Jonathan JONES, Met Office

AS06-A007
Improving Afternoon Thunderstorm Prediction Over Northern Taiwan with the Assimilation of Ground-based Observation

Yi-Pin CHANG1+, Shu-Chih YANG1#, Hsiang-Wen CHENG1, Ya-Ting TSAY2, Jing-Shan HONG2, Yu-Chi LI2
1National Central University, 2Central Weather Bureau

This study investigates the impact of assimilating densely distributed GNSS zenith total delay (ZTD) and surface station data on very short-term heavy rainfall prediction associated with afternoon thunderstorms. A series of sensitivity experiments are applied to multiple cases characterized by intense rainfall rates within 2 hours in the Taipei Basin to identify key assimilation strategies for initializing afternoon thunderstorms. Data assimilation experiments are conducted with a convective-scale WRF-LETKF system, which assimilates the ZTD data and surface station data every 30 min. The results suggest that ZTD assimilation provides effective low-level moisture adjustments. The model generates strong convections due to the large amount of moisture flux over northern Taiwan, and thus heavy precipitation takes place in a short time. When station data is additionally assimilated, the location of the strongest convection is better predicted. Adopting variable- and scale-dependent covariance localization is crucial for optimizing the impact of ZTD assimilation. While the large-scale moisture correction from ZTD assimilation provides the essential thermodynamic precondition of convection development, the small-scale wind correction from surface station assimilation gives the ability to capture the wind direction over the complex terrain, which is decisive for the heavy rainfall location. Increasing the assimilation frequency gives the strongest near-surface convergence in the Taipei Basin. The well-coupled dynamic and thermodynamic conditions trigger extreme convection development in Taipei Basin and lead to a rainfall intensity that best agrees with the observations.


AS06-A001
Investigating the Optimal Spatial Resolution for Assimilating Ground-based GNSS Tropospheric Products to Improve Atmospheric Humidity Field

Haobo LI1#+, Suelynn CHOY1, Safoora ZAMINPARDAZ1, Brett CARTER1, Kefei ZHANG2, Xiaoming WANG3
1Royal Melbourne Institute of Technology University, 2China University of Mining and Technology, 3Chinese Academy of Sciences

Water vapor (WV) is generally recognized as an essential climate variable and one of the most active components in the atmosphere. Being a typical type of greenhouse gas, the content and migration of WV are greatly associated with the intensity, time and extent of various types of severe weather events, e.g., rainstorm, typhoon and drought. Therefore, it is significant to further refine the existing methods to conduct continuous, timely and accurate monitoring of atmospheric humidity fields. Over the past few decades, on account of the benefits including high spatiotemporal resolution, long-term stability and all-weather capability, the emerging ground-based Global Navigation Satellite Systems (GNSS) atmospheric sounding technique has been widely used to sense WV content in the atmosphere. The GNSS-derived products of zenith total delay and precipitable water vapor have also advanced their usages in improving the accuracy of atmospheric WV fields simulated by numerical weather prediction models. In this paper, a comprehensive investigation on the optimal spatial resolution for assimilating GNSS-derived tropospheric products in the Weather Research and Forecasting (WRF) model to improve atmospheric humidity field is conducted in the context of Australia. By using the strategy of data thinning, the optimal spatial resolution for data assimilation was proved to be 46.4 km. By using the reanalysis data over the study period as the reference, it was found that, with the variational assimilation of GNSS-derived products, both the accuracy of initial field and that of final predictions were greatly improved. Therefore, the research findings not only further corroborate the effectiveness of using ground-based GNSS tropospheric products to improve model performance, but could provide some clues/insights in the development of more robust forecasting models.


AS06-A003
Investigating the Impact of Assimilation of MODIS Calibrated PWV on Numerical Weather Prediction

Yangzhao GONG1+, George Zhizhao LIU1#, K.K. HON2, P.W. CHAN2
1The Hong Kong Polytechnic University, 2Hong Kong Observatory

The impact of assimilation of Moderate Resolution Imaging Spectroradiometer (MODIS) near infrared (NIR) water vapor data on the weather forecasting performance of mesoscale Numerical Weather Prediction (NWP) model, i.e., the Weather Research and Forecasting (WRF) model, is investigated in this study. Three WRF schemes including a no data assimilation scheme and two data assimilation schemes are performed over the South China area for February 2020 and July 2020, respectively. The no data assimilation scheme dose not assimilate any data and is treated as the background run. For the first data assimilation scheme, Precipitable Water Vapor (PWV) data from the MODIS onboard Terra satellite are assimilated into the WRF model. For the second data assimilation scheme, a Back Propagation Neural Network (BPNN) model with assistance of Global Navigation Satellite System (GNSS) PWV is adopted to calibrate the MODIS PWV data. Then, the MODIS calibrated PWV are assimilated into the WRF model. The performance of three WRF schemes are comprehensively assessed by actual observations from the GNSS, radiosonde, and meteorological stations. The results show that: (1) Within the first 12 h after data assimilation, assimilation of MODIS calibrated PWV gains an average PWV forecasting accuracy improvement of 7.6% for February period and 3.3% for July period, while the corresponding improvements of assimilation of MODIS raw (uncalibrated) PWV are 3.6% and 4.1% for February period and July period, respectively. (2) Both assimilation of MODIS raw PWV and calibrated PWV improve the humidity and temperature profile forecasting accuracy, particularly for July period. (3) For July period, after assimilating MODIS raw PWV and calibrated PWV, the accumulated rainfall forecasting success rate for the first 12 h after data assimilation increases from 62.7% to 63.1% and 62.9%, respectively.


AS06-A005
A Study on Humidity Information Application to Enhance the GNSS-RO Quality Control in the KIM Data Assimilation System

Jeon-Ho KANG#+, In-Hyuk KWON
Korea Institute of Atmospheric Prediction Systems

Global positioning system (GPS) radio occultation (RO) data has been playing an important role in the new Korea Meteorological Administration (KMA) operational weather prediction system. The Korea Institute of Atmospheric Prediction Systems (KIAPS) delivered the global atmosphere NWP model - named the Korean Integrated Model (KIM) - to the KMA. GPS-RO provides a promising data set with a combination of global coverage, high vertical resolution, and all-weather capability. However, the accuracy of the observation operator in the lower atmosphere (troposphere) - particularly in the subtropical moist marine area - limits the effectiveness of assimilating RO data in these regions. We are currently using the standard Abel transform, which gives the minimum refractivity solution of the continuum consistent with a given RO bending angle (BA) profile, but this is known to give rise to large negative biases in the lower troposphere. As for this issue, we guessed two strategies could relieve the enormous gap of the refractivity (or bending angle) between the observation and the background field over the moist region. The first is to modify the observation operator directly to get more reliable simulation results based on a better understanding of the GNSS-RO features according to the atmospheric structure. And the other is enhancing the quality control (QC) process allows it could more sophisticatedly eliminate the observations that seem highly affected by the moisture.
In this study, we tried to strengthen the impacts of the GNSS-RO, especially over the lower atmosphere, by enhancing the QC process using the humidity information of the background field. And the new QC process was tested in conjunction with applying dynamical observation errors varying with the observation point. Preliminary results from the latest KIAPS DA cycle experiments with these GNSS-RO data processing modifications will be presented.


AS06-A004
Fusing the ERA5 and MODIS Products to Generate Daily 1 km Seamless Precipitable Water Vapor Across the Continental Europe Based on the Generative Adversarial Network

Jinhua WU+, Linyuan XIA#, Ting On CHAN
Sun Yat-sen University

Precipitable water vapor (PWV), as the medium of land surface-atmosphere energy exchange, plays a crucial role in Earth radiative balance and global climate. However, the applicability of mainstream satellite PWV products is limited by the tradeoff between spatial and temporal resolution and spatiotemporal discontinuity caused by cloud contamination. In this study, we fused the reanalysis-based ERA5 and satellite-derived MODIS PWV to generate accurate and seamless PWV of high spatio-temporal resolution (0.01°, daily) across the continental Europe from 2015 to 2018 based on the generative adversarial network (GAN) model. Firstly, the optimal clear-sky ERA5- MOD05 image pairs are selected based on the image similarity as inputs to raise the fusion performance. Secondly, a flexible multiscale feature extraction architecture is used to capture spatio-temporal variations which primely addresses the non-stationarity of PWV. Finally, the attention-based GAN architecture is used to recover the high-resolution and seamless PWV based on the extracted multiscale features. The results indicate that the fused PWV has great consistency with the GPS retrievals (r = 0.88–0.95 and Bias = -0.89–3.13 mm), showing an improvement in the accuracy and continuity compared to the original MODIS PWV. The fused accurate and spatiotemporal continuous PWV has great potential for meteorological and hydrological analyses.


AS06-A002
Enhancing the Observation Accuracy of Sentinel-3 OLCI Water Vapor Estimates Based on Ground-based GPS Measurements

Jiafei XU1+, George Zhizhao LIU2#
1Hong Kong Polytechnic University, 2The Hong Kong Polytechnic University

High-quality satellite remotely sensed water vapor observations present a vital role in Earth’s weather and climate. The Ocean and Land Color Instrument (OLCI) sensor, on-board Sentinel-3A and Sentinel-3B satellite platforms, can observe atmospheric water vapor data records at near-infrared (NIR) measurements. Yet the measurement performance of satellite-sensed OLCI water vapor estimates is generally inferior to that of ground-based and reanalysis-based water vapor observations. In our research, we develop a novel Back Propagation Neural Network (BPNN) based calibration approach to adjust the observation performance of official Sentinel-3 OLCI NIR water vapor products, which considers multiple influence factors that are correlated with the performance of satellite-based NIR water vapor measurements. The in-situ water vapor data records, measured from Global Positioning System (GPS) stations, are used as the desired resulting water vapor estimates. The model is validated based on ground-based water vapor data from GPS and radiosonde instruments. The results show that the BPNN-based adjustment approach can significantly improve the measurement quality of official Sentinel-3 OLCI NIR water vapor data records. Our model can reduce the root-mean-square error (RMSE) of official OLCI NIR water vapor by 24.52% from 3.10 mm to 2.34 mm for Sentinel-3A and 25.00% from 3.44 mm to 2.58 mm when compared to GPS-measured reference water vapor. When compared to radiosonde-observed reference water vapor, the RMSE reduces 21.01% from 4.57 to 3.61 mm and 20.81% from 5.19 to 4.11 mm for Sentinel-3A and Sentinel-3B, respectively. The BPNN-based calibration model exhibits a higher accuracy enhancement on OLCI/Sentinel-3 NIR water vapor observations, compared with other existing previous methods in previous studies. This could be because we have considered multiple dependence parameters in association with the measurement performance of OLCI-retrieved NIR water vapor, while the previous research did not do so.


AS06-A006
Detection of Tropical Cyclone Seroja Based on Precipitable Water Vapor from Indonesian CORS Data

Nabila PUTRI1#+, Dudy WIJAYA1, Muhammad Rais ABDILLAH1, Sidik WIBOWO2
1Institut Teknologi Bandung, 2Badan Informasi Geospasial

Tropical cyclones are low pressure systems created by a local heating of the sea surface, which triggers an intense convective activity involving large amounts of water vapor. A deadly tropical cyclone was formed in the early April 2021 over the Savu Sea and was given the name Seroja. This study aims to understand the characteristics of Seroja based on the precipitable water vapor (PWV) as derived from the Global Navigation Satellite Systems (GNSS) data. Observations at 22 permanent GNSS stations, as well as in situ meteorological sensors, in the Nusa Tenggara region from 1 March 2021 until 30 April 2021 were used for this purpose. Surface pressure values dropped significantly by more than 20 hPa, while relative humidity increased and temperature was reduced. Furthermore, during the formation of Seroja, PWV values gradually increased, reaching its peak around the time of when the cyclone was at its closest. After the cyclone had passed, PWV values decreased rapidly, dropping from around 70 mm to below 20 mm at CKUP. PWV pre-Seroja tends to be larger than post-Seroja, whereas post-Seroja PWV was more variable.


Tue-01 Aug | 8:15 - 10:00 | MR329
AS11 - Atmospheric Chemistry in Highly Polluted Environments: Emissions, Fate, and Impacts

Session Chair(s): Jianlin HU, Nanjing University of Information Science & Technology, Hongliang ZHANG, Fudan University

AS11-A003
Diurnal Variation, Chemical Fingerprint, and Source Resolution of Marine PM2.5 at the Dongsha Islands Based on Three-Year Field Measurement Data

Zi-You HUANG#+, Chung-Shin YUAN
National Sun Yat-sen University

This study aims to clarify the spatiotemporal variation, chemical fingerprint, transport routes, and source apportionment of marine fine particles (PM2.5) at a remote island in the South China Sea (SCS). Field sampling and receptor modeling of PM2.5 were conducted from September, 2020 to July, 2023. Twenty-four hour marine PM2.5 was collected at the Dongsha Islands for continuous seven days in each season. Chemical composition of PM2.5 was analyzed for water-soluble ions (WSIs), metallic content, carbonaceous content, anhydrosugars, and organic acids. Moreover, the potential sources of PM2.5 and their contribution were further resolved by backward trajectory simulation and chemical mass balance (CMB) receptor model. Three-year field sampling results indicated that high concentrations of PM2.5 were commonly observed in winter and spring. In terms of chemical composition of PM2.5, secondary inorganic aerosols (SIAs; SO42-, NO3-, and NH4+) accounted for 53.0-64.1% of WSIs which dominated PM2.5. Crustal elements (Ca, K, Mg, Fe, and Al) dominated metallic content of PM2.5, while trace elements (V, Ni, and Cu) were originated from anthropogenic sources. The concentrations of organic carbon (OC) in PM2.5 were generally higher than those of elemental carbon (EC). The highest concentrations of levoglucosan were 20.94 ng/m3 at the Dongsha Islands in winter, while galactosan and mannosan were non-detectable (MDL). Major sources of PM2.5 resolved by CMB receptor modeling were sea salts (16.6-24.7%), fugitive dust (15.8-23.0%), industrial boilers (6.6-12.0%), secondary sulfate (7-10.9%), mobile sources (4.7-9.6%), waste incinerators (2.4-5.2%), and biomass burning (2.8-5.3%). Keywords: marine fine particles, chemical fingerprints, spatiotemporal variation, transport routes, source apportionment.


AS11-A005
Impacts of Chlorine Chemistry and Anthropogenic Emissions on Secondary Pollutants in the Yangtze River Delta Region

Jingyi LI1#+, Peng WANG2, Qi YING3, Song GUO4, Keding LU4, Xionghui QIU5, Jianlin HU1
1Nanjing University of Information Science & Technology, 2The Hong Kong Polytechnic University, 3Texas A&M University, 4Peking University, 5North China Electric Power University

Multiphase chemistry of chlorine is coupled into a 3D regional air quality model (CMAQv5.0.1) to investigate the impacts on the atmospheric oxidation capacity, ozone (O3), as well as fine particulate matter (PM2.5) and its major components over the Yangtze River Delta (YRD) region. By including the chlorine chemistry, the model performances in simulating hydrochloric acid (HCl), particulate chloride (PCl), and hydroxyl (OH) and hydroperoxyl (HO2) radicals are significantly improved. O3 is enhanced in the high chlorine emission regions by up to 4% and depleted in the rest of the region. PM2.5 is enhanced by 2~6%, mostly due to the increases in PCl, ammonium, organic aerosols, and sulfate. Nitrate exhibits inhomogeneous variations, by up to 8% increase in Shanghai and 2~5% decrease in most of the domain. Radicals show different responses to the chlorine chemistry during the daytime and nighttime. Both OH and HO2 are increased throughout the day, while nitrate radicals (NO3) and organic peroxy radicals (RO2) show an opposite trend during the daytime and nighttime. Higher HCl and PCl emissions can further enhance the atmospheric oxidation capacity, O3, and PM2.5 so that the anthropogenic chlorine emission inventory must be carefully evaluated and constrained.


AS11-A007
Global and East Asian Tropospheric Ozone Trends in the Recent Two Decades

Xiao LU#+, Haolin WANG
Sun Yat-sen University

Tropospheric ozone is an important greenhouse gas and is central to atmospheric oxidation capacity. We examine observed tropospheric ozone trends, their attributions, and radiative impacts from 1995–2017 using aircraft observations from the In-Service Aircraft for a Global Observing System database (IAGOS), ozonesondes, and a multi-decadal GEOS-Chem chemical model simulation. IAGOS observations above 11 regions in the Northern Hemisphere and 19 of 27 global ozonesonde sites have measured increases in tropospheric ozone (950-250hPa) by 2.7 ± 1.7 and 1.9 ± 1.7 ppbv decade-1 on average, respectively, with particularly large increases in the lower troposphere (950-800 hPa) above East Asia, Persian Gulf, India, northern South America, Gulf of Guinea, and Malaysia/Indonesia by 2.8 to 10.6 ppbv decade-1. The GEOS-Chem simulation, driven by reanalysis meteorological fields and the most up-to-date year-specific anthropogenic emission inventory, reproduces the overall pattern of observed tropospheric ozone trends with an increasing trend of 0.4 Tg year-1 of the tropospheric ozone burden in 1995–2017. Sensitivity simulations show that changes in global anthropogenic emission patterns, including the equatorward redistribution of surface emissions and the rapid increases in aircraft emissions, are the dominant factors contributing to tropospheric ozone trends by 0.5 Tg year-1. In particular, we highlight the disproportionately large contribution of aircraft which emitting NOx in the mid- and upper troposphere where ozone production efficiency is high. Regionally, the Chinese nationwide ozone monitoring network has observed rapid increases in warm-season surface ozone in cities during 2013−2019 by about 2.4 ppbv per year, among the fastest urban ozone trends in the recent decade reported in the Tropospheric Ozone Assessment Report (TOAR). Our model simulations reveal that the presence of soil NOx emissions in the North China Plain, mainly driven by agricultural fertilizer applications, present as an underappreciated challenge for ozone mitigation there.


AS11-A009
Fast Spreading of Surface Ozone in Both Temporal and Spatial Scale in Pearl River Delta

Tianhui CAO+, Haichao WANG#, Shaojia FAN
Sun Yat-sen University

Surface ozone (O3) is a major air pollutant and draw increasing attention in the Pearl River Delta (PRD), China. Here, we characterize the spatial-temporal variability of ozone based on a dataset obtained from 57 national monitoring sites during 2013-2019. Our results show that: (1) the seasonal difference of ozone distribution in the inland and coastal areas was significant, which was largely affected by the wind pattern reversals related to the East Asian monsoon, and local ozone production and destruction; (2) the daily maximum 8hr average (MDA8 O3) showed an overall upward trend by 1.11 ppbv/year. While the trends in the nine cities varied differently by ranging from -0.12 to 2.51 ppbv/year. The hot spots of ozone were spreading to southwestern areas from the central areas since 2016. And ozone is becoming a year-round air pollution problem with the pollution season extending to winter and spring in PRD region. (3) At the central and southwestern PRD cities, the percentage of exceedance days from the continuous type (defined as ≥ 3 days) was increasing. Furthermore, the ozone concentration of continuous type was much higher than that of scattered exceedance type (< 3 days). In addition, although the occurrence of continuous type starts to decline since 2017, the total number of exceedance days during the continuous type is increasing. These results indicate that it is more difficult to eliminate the continuous exceedance than the scatter pollution days and highlight the great challenge in mitigation of O3 pollution in these cities.


AS11-A012
Age-resolved Source and Region Contributions to Fine Particulate Matter During an Extreme Haze Episode in China

Xiaodong XIE#+, Jianlin HU
Nanjing University of Information Science & Technology

A Source- and Age-Resolved Algorithm (SARA) was developed in the CMAQ model and applied to study the sources and ages of primary fine particulate matter (PPM) and secondary inorganic aerosols (SNA) in China during January 2013. Residential and industry are the major contributors to PPM and sulfate, especially for fresh particles. The contributions of power increase with age, accounting for 25% and 51% of aged sulfate and nitrate (> 48 h), respectively. Local emissions and intra-regional transport with younger age contribute to over 70% of PPM and SNA in Beijing, while long-range transport from northern China with older age becomes more significant in Shanghai. On pollution days, the ages of PPM and SNA consistently increase, suggesting enhanced contributions from regional transport. This study highlights that the age-specific particle source and region information produced by our SARA algorithm can help design cost-effective emission control strategies to reduce extreme haze pollution.


AS11-A013 | Invited
Quantification and Characterization of Fine Plastic Particles as Considerable Components in Atmospheric Fine Particle

Yunqian CHEN1#+, Siyuan JING2, Yanting WANG3, Jianmin CHEN1
1Fudan University, 2Westlake University, 3Zhejiang University

Fine plastic particles (particle diameter < 2.5 μm, hereafter FPP) have made considerable contributions to human health, aerosol pollution, climate effects, and many aspects of the ecosystem. However, the direct characteristics and high-time resolution (hourly) quantitative detection of atmospheric FPP were limited. We investigated the composition and probable sources of FPP in PM2.5 in this study. Dual-hour-resolution was obtained for the quantitative study of FPP in PM2.5 using the Versatile Aerosol Concentration Enrichment System (VACES) and Thermal Desorption/Pyrolysis-Gas Chromatography-Mass Spectrometry (TD/Py-GC-MS). The FPP in PM2.5 accounted for an expected value of 5.57 μg/m³ (from 0 to 24.73 μg/m³) while a ratio of FPP to PM2.5 was 13.2 % (from 4.1 to 42.6 %) in most PM2.5 samples during the campaign. FPP are not significantly correlated with PM2.5 yet accounted for in PM2.5 concentrations, and PAEs are not part of atmospheric particulate matter yet are highly correlated with PM2.5. Additionally, a comprehensive chemical analysis of the FPP in PM2.5 has revealed the abundant presence of plastic particles, as opposed to other particles such as soot and tar balls. Heavy pollution of FPP was closely related to local human activities. This work implied that FPP in the air are a growing threat and atmospheric stocks of FPP were strongly related to human activity.


AS11-A039
An Approach Towards Preparation of a National Emission Inventory for the Food Service Industry in India: A Case Study for Megacity Delhi

Medhavi GUPTA#+, Sri KOTA
Indian Institute of Technology Delhi

Increasing air pollution levels and associated detrimental health and environmental impacts is a rising concern for citizens of India. National policies and action plans have been sporadically implemented by the government along with various mitigation pathways suggested for further control of air pollution. To effectively combat air pollution, a detailed emission inventory is vital taking into account every sector. The Indian food service industry is one sector that is neglected. The food industry in India is a growing sector, and the unexpected rise due to the high demand in the service delivery market indicates the expected increase in cooking oil fumes. The cooking oil fumes produced as a result of high temperature processes are a major health hazards to human. However, there are limited studies addressing the issue and lack of data related to the sector for construction of a national emission inventory for the food service industry. To develop an inventory for India, firstly the structure of food/restaurant industries in the capital region of the country, megacity Delhi was studied by conducting a survey campaign. Based on the data collected, the emissions from the sector were calculated for Delhi. This study helps understand the pollutant emissions from the food service industry for megacity Delhi which is the hub for the largest number of restaurants in the country. This information can further be extrapolated across all states of India to help construct national emission inventory in future studies.


Tue-01 Aug | 8:15 - 10:00 | MR330
AS21 - Past and Future Irreversible and Abrupt Climate Changes: Hysteresis and Resilience

Session Chair(s): Seung-Ki MIN, Pohang University of Science and Technology, Seungmok PAIK, Yonsei University, Chao LIU, Yonsei University

AS21-A001
Hysteresis of the El Niño-southern Oscillation Characteristics to CO2 Forcing Linked to the ITCZ

Chao LIU1+, Soon-Il AN1#, Fei-Fei JIN2, Jongsoo SHIN3, Jong-Seong KUG3, Wenjun ZHANG4, Malte STUECKER5, Xinyi YUAN6, Aoyun XUE3, Xin GENG4, Soong-Ki KIM1
1Yonsei University, 2University of Hawaii, 3Pohang University of Science and Technology, 4Nanjing University of Information Science & Technology, 5University of Hawaii at Manoa, 6China Meteorological Administration

Underpinned by large-scale air-sea coupled dynamics in the equatorial Pacific, the El Niño-Southern Oscillation (ENSO) makes it the strongest natural interannual variability on Earth with far-reaching socio-economical influences across the globe. Compared to its extensively studied changes in warming scenarios, ENSO responses to anthropogenic forcing removal or reduction, however, remain less explored so far. Based on the 1% per year CO2 changing for ramp-up and ramp-down experimental scenarios and climate models that capture key ENSO dynamics, here we show two major ENSO sea surface temperature (SST) statistics of variance and skewness exhibit prominent hysteresis responses in a CO2 changing pathway. In contrast to largely uncertain responses in the ramp-up period, eastern Pacific SST variance and central Pacific SST skewness during the ramp-down period display exaggerated increases and decreases changes, respectively. Such ENSO hysteresis owing to corresponding SST feedback changes is closely associated with a continuously strengthening and eastward-propagating of the El Niño action center until the middle of the ramp-down period. The El Niño action center changes are further linked with similar hysteresis background changes manifested in the intertropical convergence zone, which increase the eastern Pacific atmosphere sensitivity to local SST anomalies during the El Niño initial stage. We also suggest that the presence of El Niño hysteresis would possibly exacerbate its amplified consequential global impacts in a warming world.


AS21-A002
Hysteresis and Irreversibility of Global Extreme Precipitation to Anthropogenic CO2 Emission

Sanjit Kumar MONDAL1#+, Soon-Il AN1, Seung-Ki MIN2, Soong-Ki KIM1, Jongsoo SHIN2, Seungmok PAIK1, Nari IM1, Chao LIU1
1Yonsei University, 2Pohang University of Science and Technology

 In this study, a comprehensive analysis is conducted to explore the response of global precipitation extremes to CO2 in terms of hysteresis and reversibility effect and associated population exposure. In this regard, climate outputs under two idealized CO2 scenarios such as ramp-up (RU; about +1% annually until quadrupling of present level) and ramp-down (RD; around -1% annually set back to present level) from Community Earth System Model version 1.2, and the projected population data from the five shared Socioeconomic Pathways (SSPs) are used. Precipitation extremes are evaluated using the number of heavy precipitation days, maximum consecutive 5-day precipitation, and the precipitation of very wet days indices. Results show that the magnitude of extreme precipitation change and associated population exposure is higher in the CO2 reduction period (RD) than in RU. All the indices show substantial irreversible and hysteresis effects, ~69% of the global land is expected to experience irreversible changes in precipitation extreme. Further, the hotspots of irreversibility (the region with irreversible change and a large hysteresis) will emerge in >20% of the global area. Spatially, strong hysteresis and irreversibility are particularly concentrated over global land monsoon regions. The leading exposure is estimated under SSP3 combined with both RU and RD periods. Under the SSP3-RD combination, the highest population exposure is estimated at ~67.1% (globally averaged), and ~72% (averaged over hotspots) higher than that of the present day. The exposed population is prominent in South Africa and Asia. Notably, the population change effect is the principal factor in global exposure change, while it is the climate change effect over the hotspots of irreversibility. These findings provide new insight into policymaking that only CO2 mitigation effort is not enough to cope with precipitation extremes, rather advanced adaptation planning is a must to have more socio-economic benefits.


AS21-A006
Roles of Two Hemispheres for Changes in the Global Mean Temperature Under the Zero Emission Commitment (CESM2) Scenario

Seung-Hwon HYUN#+, Soon-Il AN, Ho-Jeong SHIN
Yonsei University

For investigation in the change of global temperature after the cessation of COemissions, Zero Emissions Commitment (ZEC) scenario has been proposed. In our four ensemble members of CESM2 ZEC experiment, CO2 emissions are linearly increased and symmetrically decreased till zero, then this net zero condition is maintained over longer than 100 years. During this net zero emission period, authors found that the ensemble spread of global mean surface temperature (GMST) increases drastically and the ensemble mean also increases again, without increasing CO2 emissions. The ensemble spread, especially over the northern or subpolar Atlantic Ocean, is associated with differences in the reconstruction of Atlantic Meridional Overturning Circulation (AMOC) within ensembles. This could be explained by AMOC–Salt–Advection positive feedback that a stronger surface salinity derives a weaker stratification of the northern Atlantic Ocean and a stronger AMOC. This raises the stronger meridional warm and salt advection in faster warming ensemble members than slower warming members during the net zero emission period. On the other hand, the positive trend of surface temperature over Southern Ocean (SO) persists during the entire ZEC scenario, thus this plays an important role in the increasing ensemble mean GMST during the net zero period. In contrast, it is noteworthy that the ensemble spread is not as large as the northern Atlantic Ocean or Arctic regions. Authors further found that this positive trend over SO is associated with changes of surface heat budget by the intensified downwelling radiation. From these results, present study argues that the roles of both Northern and Southern hemisphere in ZEC scenario is distinguished in the ensemble spread and mean of GMST, respectively.


AS21-A007
Hysteretic Behavior of Global to Regional Monsoon Area Under CO2 Ramp-up and Ramp-down

Seungmok PAIK1+, Soon-Il AN1#, Seung-Ki MIN2, Andrew KING3, Jongsoo SHIN2
1Yonsei University, 2Pohang University of Science and Technology, 3The University of Melbourne

When projecting future monsoon changes by carbon dioxide (CO2) pathway, most studies have analyzed precipitation responses without considering monsoon area (MA) variations. Further, how MA responds to CO2 removal remains uncertain. This study evaluates MA variations and impacts in idealized CO2 ramp-up (toward CO2 quadrupling), ramp-down, and stabilized simulations using the Community Earth System Model version 1. Global MA negatively overshoots (i.e., recovery with decreasing tendency beyond the original MA) during the ramp-down period due to reduced or rapidly recovered MA in several regional monsoons, including Northern and Southern Africa, South and East Asia, and South America, showing hysteresis when comparing ramp-up and -down periods despite similar global warming levels. These non-linear regional MA variations come from distinct regional summer and winter precipitation variations, which are found to be associated with Intertropical Convergence Zone movements and El Niño-like response. Further, regional monsoon precipitation characteristics also vary through ramp-up and ramp-down periods consistently with overall hysteresis. Changes in total monsoon precipitation resemble the distinct responses of MA. Our results suggest that regions characterized by a monsoonal climate may experience reduced seasonal rainfall variations under net-negative CO2 emissions.


AS21-A009 | Invited
Asymmetrical Response of Summer Rainfall in East Asia to CO2 Forcing

Sang-Wook YEH#+, Se-Yong SONG
Hanyang University

Understanding the regional hydrological response to varying CO2 concentration is critical for cost-benefit analysis of mitigation and adaptation polices in the near future. To characterize summer monsoon rainfall change in East Asia due to a change in the CO2 pathway, we used the Community Earth System Model (CESM) with 28 ensemble members in which the CO2 concentration increases at a rate of 1% per year until its quadrupling peak, i.e., 1,468 ppm (ramp-up period), followed by a decrease of 1% per year until the present-day climate conditions, i.e., 367 ppm (ramp-down period). Although the CO2 concentration change is symmetric in time, the rainfall response is not symmetric. The amount of summer rainfall anomaly in East Asia is increased 42% during a ramp-down period than that during a ramp-up period when the two periods of the same CO2 concentration are compared. This asymmetrical rainfall response is mainly due to an enhanced El Niño-like warming pattern as well as its associated increase in the sea surface temperature in the western North Pacific during a ramp-down period. These sea surface temperature patterns enhance the atmospheric teleconnections to East Asia and the local meridional circulations around East Asia, resulting in more rainfall over East Asia during the ramp-down period. This result implies that the removal of CO2 does not guarantee the return of regional rainfall to the previous climate state with the same CO2 concentration.


AS21-A010
Hemispherically Asymmetric Hadley-cell Response to CO2 Removal

Seo-Yeon KIM1+, Seok-Woo SON1#, Yeong-Ju CHOI1, Paul William STATEN2, Kevin M GRISE3, Soon-Il AN4, Jong-Seong KUG5, Sang-Wook YEH6, Seung-Ki MIN5, Jongsoo SHIN7
1Seoul National University, 2Indiana University, 3University of Virginia, 4Yonsei University, 5Pohang University of Science and Technology, 6Hanyang University, 7Woods Hole Oceanographic Institution

A poleward shift of the Hadley cell (HC) edge in a warming climate has been widely documented. However, its possible change to CO2 removal has not been explored. By conducting large ensemble experiments where CO2concentrations are systematically increased and then decreased to the present-day level, we show that the poleward-shifted HC edges in a warming climate do not return to the present-day state when CO2 concentrations are reduced to the present-day climate. While the Southern-Hemisphere HC edge remains poleward of its present-day state, the Northern-Hemisphere HC edge returns and remains farther equatorward. Such hemispherically asymmetric HC-edge changes, which contribute to drought-prone subtropical regions, are closely associated with the changes in the vertical wind shear. We attribute the vertical wind shear change to the hysteresis in the oceanic response to a changing CO2 pathway.


AS21-A013
Asymmetric Response of South Asian Summer Monsoon Rainfall in a Carbon Dioxide Removal Scenario

Suqin ZHANG#+
Chinese Academy of Sciences

The reversibility of South Asian summer monsoon (SASM) precipitation under the CO2 removal scenario is critical for climate mitigation and adaptation. In the idealized CO2 ramp-up (from 284.7 to 1138.8 ppm) and symmetric ramp-down experiments, SASM precipitation is largely reversible while exhibiting strong asymmetry: it may overshoot the unperturbed level when CO2 recovers. Such asymmetric response is mainly due to the enhanced El Niño-like and Indian Ocean dipole-like warming during the ramp-down period. The uneven sea surface warming weakens Walker circulation, with anomalous sinking over the SASM region; meanwhile, the warming also affects the rainfall over the Maritime Continent and tropical western Indian Ocean. The suppressed rainfall over the Maritime Continent triggers the equatorial Rossby wave, which weakens the ascent over the SASM region. The increased rainfall over the tropical western Indian Ocean excites the equatorial Kelvin wave, which reduces moisture transport. Additionally, tropic-wide warming reduces the land-sea thermal contrast and weakens monsoonal circulation. Consequently, the combined effects of the weakened ascent and moisture transport lead to the overshooting of SASM rainfall. Our results suggest that symmetric CO2 removal, although unlikely in the foreseeable future, may result in a risk of local drought over the SASM region.


Tue-01 Aug | 8:15 - 10:00 | MR331
AS01 - The Asian Monsoon, Extremes and Climate Change

Session Chair(s): Renguang WU, Zhejiang University, Kyung-Ja HA, Pusan National University, Ramesh KRIPALANI, Indian Institute of Tropical Meteorology

AS01-A012
Extremely Hot East Asia and Flooding Western South Asia in the Summer of 2022 Tied to Reversed Flow Over Tibetan Plateau

Chao HE1#+, Lixia ZHANG2, Xiaolong CHEN2, Tianjun ZHOU2, Wenxia ZHANG2
1Jinan University, 2Chinese Academy of Sciences

In the summer (July and August) of 2022, unprecedented heat wave occurred along the Yangtze River Valley (YRV) over East Asia while unprecedented flood occurred over western South Asia (WSA), which are located on the eastern and western sides of Tibetan Plateau (TP). Here, by analyzing the interannual variability based on observational and reanalysis data, we show evidences that the anomalous zonal flow over subtropical Tibetan Plateau (TP) explains a major fraction the extreme events occurred in 2022. As isentropic surfaces incline eastward (westward) with altitude on the eastern (western) side of the warm center over TP in summer, anomalous easterly (westerly) flow in upper troposphere generates anomalous descent (ascent) on the eastern side of TP and anomalous ascent (descent) on the western side of TP via isentropic gliding. The anomalous easterly flow is extremely strong to reverse the climatological westerly flow over subtropical TP in 1994, 2006, 2013 and 2022. The easterly flow in 2022 is the strongest since 1979, and it generates unprecedented descent (ascent) anomaly on the eastern (western) side of TP, leading to extreme heat wave over YRV and extreme flood over WSA in 2022. The anomalously strong easterly flow over subtropical TP in 2022 is dominated by atmospheric internal variability related to mid-latitude wave train, while the cold sea surface temperature anomaly over the tropical Indian Ocean increases the probability of a reversed zonal flow over TP by reducing the meridional gradient of tropospheric temperature.


AS01-A052
Summer Precipitation Extremes Over the Yellow River Loop Valley and its Link to European Blocking

Yina DIAO1#+, Kan XU2, Peng HUANG3
1Ocean University of China, 2Naval Aviation University, 391954 PLA

Characteristics of extreme precipitation over Yellow River Loop Valley (YRLV) and links to European blocking are investigated in this study. Spatial and temporal analysis of extreme precipitation shows that it contributes more than 30% of the total summer precipitation in the YRLV and is characterized by a strong and short period of local rainfall. Most of the extreme rains in the YRLV occur in July and August. Two typical circulation patterns were identified using a k-means clustering method. The extreme precipitation results from the combined actions of intensified high pressure over northeast China (NECH) and the westward extension of the western Pacific subtropical high (WPSH). The intensified southerly flow of the amplified NECH strengthens the water vapor transport induced by the westward extension of the WPSH from the northwest Pacific or Bay of Bengal into the YRLV. The NECH is amplified by the wave energy propagating from European blocking via the Silk Road pattern (SRP). This is the subseasonal cause of extreme precipitation over the YRLV. The composited July and August mean 500 hPa geopotential anomaly pattern for extreme precipitation years shows a high-pressure anomaly over the European continent and a negative phase of the SRP. The former provides a background for the occurrence of European blocking, and the latter explains the preexistence of the NECH and provides a linkage between the activity of European blocking and the subseasonal evolution of the NECH. Thus, the interannual variation in the extreme precipitation over the YRLV is mainly reflected by the phase of the SRP and the stationary waves over Europe.


AS01-A094
Excessive Southern China Spring Rainfall Promoted by Multi-year El Niño Events

Wenxiu ZHONG1#+, Yuting WU1, Song YANG1, Tianjiao MA2, Qingyu CAI3, Qian LIU1
1Sun Yat-sen University, 2Yunnan University, 3Chinese Academy of Sciences

Southern China spring rainfall (SCSR) is significant for agricultural sowing and soil moisture accumulation before the rainy summer. A better prediction of the rainfall improves our ability to risk response to natural disasters. It is found that the SCSR can be promoted by multi-year El Niño events through the high-latitude pathway (HP) and low-latitude pathway (LP). The long-lasting El Niño warming heats the tropical troposphere persistently until the decaying spring, which strengthens the Arctic polar vortex and the mid-latitude blockings. This HP is in favor of more southward transport of Rossby wave energy and cold air, resulting in strong ascending motions over southern China in spring. The multi-year El Niño also induces an enhanced western North Pacific anticyclone and a secondary circulation transporting moisture to southern China through the LP. The HP is more important in the early spring, while the LP dominates the heavy SCSR in the late spring.


AS01-A001
Zonal Extension of the Middle East Jet Stream and its Influence on the Asian Monsoon

Wei WEI#+
Sun Yat-sen University

Investigation into the interannual variation of the Middle East jet stream (MEJS) and its influence on the Asian monsoon indicates that the eastward extension of MEJS is closely related with a wetter and colder winter in southern China and a later onset of the subsequent Asian summer monsoon, compared with normal conditions. When the MEJS extends eastward, a significant barotropic anomalous anticyclone is located over the Arabian Sea (AS), associated with the southeastward propagating wave train from Europe. Intense divergence in the southwest of the AS anomalous anticyclone favors more convection over the western tropical Indian Ocean, which excites an anomalous upper-level anticyclone to the north as a Rossby wave response, further intensifying the AS anticyclonic anomaly. This positive feedback loop maintains the AS anomalous anticyclone and results in the eastward extension of the MEJS. Accordingly, intense northeasterly anomalies over the Mediterranean Sea and the subtropical westerly anomalies bring abundant cold air from the middle-higher latitudes to subtropical regions, resulting in a widespread cooling in subtropical Eurasia including southern China. Barotropic anomalous westerlies occur around the Tibetan Plateau in the south and deepen the India-Burma trough, favoring more water vapor transport from the Bay of Bengal to southern China. This wetter and colder conditions in subtropical Eurasia can persist from winter to spring, leading to the much later onset of the Asian summer monsoon. Therefore, the winter MEJS variability can be considered as an important indicator for the Asian monsoon.


AS01-A059
Characteristics of Precipitation and Atmospheric Environment During the Heavy Rain Event Observed on June 14-16, 2022 in the Southern Meghalaya Plateau

Fumie MURATA1#+, Toru TERAO2, Hiambok J. SYIEMLIEH3, Laitpharlang CAJEE3, Shyam S. KUNDU4, Sayeed Ahmed CHOUDHURY5, Shameem Hassan BHUIYAN5, Fatima AKTER6, Raju GOGOI7
1Kochi University, 2Kagawa University, 3North-Eastern Hill University, 4North Eastern Space Applications Centre, 5Bangladesh Meteorological Department, 6University of Dhaka, 7Diphu Government College

The towns of Cherrapunji and Mawsynram, located on the southern slopes of the Meghalaya Plateau in the northeastern part of the Indian subcontinent, are known to have the heaviest rainfall in the world. The Indian Meteorological Department announced that 972 mm of rain was recorded in the 24 hours ending 03 UTC on 17 June 2022. This was the third rain in the last 122 years. Severe flash floods occurred downstream in Sylhet, Bangladesh. Such case studies of heavy rain events must be useful in understanding the mechanism of heavy rain and in considering countermeasures against flash floods. An automatic weather station installed at Cherrapunji and an optical disdrometer installed at Sylhet recorded rain for the heavy rain event. The rainfall for the three days from the 14th to the 16th was 2412 mm, and it was 43% of the monthly rainfall in June 2022. Precipitation showed a distinct diurnal variation and increases from midnight to early morning. On the other hand, in Sylhet, which is located in the plains 40 km southeast of Cherrapunji, the precipitation variability was completely different and the diurnal variation of precipitation was unclear. The precipitation system was characterized by the images of Bangladesh Air Force (BAF) C-band radar at Jessore, Bangladesh, and the Global Satellite Mapping of Precipitation (GSMaP) product. The precipitation system was a topographical system localized in southern Meghalaya. The precipitation system on the 15th was not sufficiently detected by the BAF radar, suggesting that the echo top height was relatively low. While the GSMaP showed some agreement with the BAF radar, on the 14th it was not possible to properly detect the onset of the nocturnal rain around 12UTC. This was because the data from the satellite-borne microwave radiometer observations used to create the GSMaP were not available within 3 hours.


AS01-A086
Different Mechanisms for Daytime, Nighttime, and Compound Heatwaves: A Study in Southern China

Ming LUO1,2#+, Gabriel LAU2, Zhen LIU3
1Sun Yat-sen University, 2The Chinese University of Hong Kong, 3IBS Center for Climate Physics

Heatwaves often cause immense stress on human society and the natural environment. While heatwaves can be classified into daytime, nighttime, and compound daytime-nighttime types, the specific processes associated with different heatwave types remain poorly understood. In this paper, we identify different mechanisms operating in compound (i.e., extreme heat during both day and night) and independent daytime and nighttime heatwaves in southern China. Compound heatwaves generally exhibit stronger temperature increases than either daytime or nighttime types. Daytime heatwaves are accompanied by increased downward shortwave radiation under a clear sky with reduced cloud cover and moisture. Nighttime heatwaves are characterized by more cloudy and moist conditions, and increased downward longwave radiation at the surface at night. A combination of these conditions for daytime and nighttime heatwaves prevail during compound heatwaves. All heatwaves are associated with strengthening and eastward extension of the South Asian high (SAH) in the upper troposphere, and strengthening and westward extension of the western North Pacific subtropical high (WNPSH) in the lower and middle troposphere. Further examinations suggest that compound heatwaves are accompanied by the strongest intensification of SAH and WNPSH. Compared with daytime heatwaves, nighttime events are associated with a stronger amplitude of SAH and WNPSH, and both highs tend to extend more southward when nighttime heatwaves occur. This southward extension induces an anomalous lower-level anticyclone that drives a southwesterly wind anomaly over southeastern China. This circulation feature transports warmer and more humid air towards southern China. The enhanced concentration of water vapor leads to increased absorption of outgoing longwave radiation, and increased re-emission of longwave radiation to the surface, thus resulting in surface warming at night.


AS01-A007
The Concurrent Record-breaking Rainfall Over Northwest India and North China in September 2021

Ying NA1#+, Riyu LU2
1Beijing Municipal Climate Center, 2Chinese Academy of Sciences

Extremely heavy rainfall occurred over both Northwest India and North China in September 2021. The precipitation anomalies were 4.1 and 6.2 times interannual standard deviation over the two regions, respectively, and broke the record since the observational data were available, i.e., 1901 for India and 1951 for China. In this month, the Asian upper-tropospheric westerly jet was greatly displaced poleward over West Asia, and correspondingly, an anomalous cyclone appeared over India. The anomalous cyclone transported abundant water vapor into Northwest India, leading to the heavy rainfall there. In addition, the Silk Road pattern, a teleconnection pattern of upper-level meridional wind over the Eurasian continent and fueled by the heavy rainfall in Northwest India, contributed to the heavy rainfall in North China. Our study emphasizes the roles of atmospheric teleconnection patterns in concurrent rainfall extremes in the two regions far away from each other, and the occurrence of rainfall extremes during the post- or pre-monsoon period in the northern margins of monsoon regions.


Tue-01 Aug | 8:15 - 10:00 | MR332
AS55 - Environmental Impacts of Biomass Burning Pollution Over Southeast Asia

Session Chair(s): Shantanu Kumar PANI, National Central University, Maggie Chel Gee OOI, Universiti Kebangsaan Malaysia

AS55-A003
Retrieving Rapid-evolving Smoke Absorption Using Critical Reflectance Methods with Geostationary Observations

Yingxi SHI1#+, Roshan MISHRA1, Zhibo ZHANG1, Robert LEVY2, Lorraine REMER1,3, J. Vanderlei MARTINS1
1University of Maryland, Baltimore County, 2NASA Goddard Space Flight Center, 3Airphoton LLC

Emissions from biomass burnings, cause large impacts on our society and environment and cause local to global scale issues. The properties of smoke particles from these emissions rapidly evolve at seconds to minutes scales. Being able to accurately measure the smoke absorption properties is essential when quantifying the aerosol impacts on radiation budgets and mesoscale dynamics and help improving the forecast as well as facilitate risk management. In-situ measurements can provide accurate measurements of aerosol properties but have limited sample size. From satellites, which have much wider temporal and spatial coverage, the fast-changing absorbing properties of smoke plumes are very challenging to retrieve. Utilizing the very fine temporal resolution observations from geostationary satellites and the powerful critical reflectance (CR) methods, we now have a pathway to retrieve wavelength dependent absorption at 10 minutes intervals. CR is a surface reflectance at which increasing or decreasing aerosol loading does not change the TOA reflectance. This reflectance value is highly associated with the absorption of the aerosol layer and not related to lower boundary conditions, which makes it suitable to apply over heterogeneous land surfaces. Using Advanced Base Imager onboard GOES-17, we demonstrated the power of CR technique by retrieving aerosol single scattering albedo on two fire events, following the track of freshly emitted smoke plumes, and compared with nearby ground-based observations. The uncertainty of the CR method is also tested using sensitivity studies. This method will be applied to all suitable fire events and the temporal and spatial variation of retrieved SSA for each case will be analyzed and compared to other aerosol absorption products. 


AS55-A004
Future Biomass Burning Activities in Malaysia and Indonesia Based on the CORDEX-SEA Projections

Aulia NISA'UL KHOIR1#+, Maggie Chel Gee OOI1, Liew JUNENG1, Jing Xiang CHUNG2, Alif AKBAR SYAFRIANNO3, Imron ADE RANGGA3
1Universiti Kebangsaan Malaysia, 2Universiti Malaysia Terengganu, 3Indonesian Agency for Meteorology, Climatology, and Geophysics

In the context of climate change, fire danger conditions are expected to increase in many regions of the world due to the projected changes in climate as the occurrences of biomass burning are events highly dependent on the meteorological driver. The threat from biomass haze in Malaysia and Indonesia will not only be about frequency but also intensity. There is a possibility that biomass burning will become more severe in the future. However, while the study of the near-real-time predictions of burning hotspots in Malaysia and Indonesia has been developed widely, the study of its projection has not been assessed. This study aims to project burning hotspots that are represented by FWI (Fire Weather Index), a fire danger system that relies upon the daily weather readings during the previous day, including temperature, relative humidity, wind speed, and rain. The projection is performed based on the future climate condition (2041 – 2070) under RCP4.5 and RCP8.5 scenarios using the downscaled simulations of the Southeast Asia Regional Climate Downscaling/Coordinated Regional Climate Downscaling Experiment—Southeast Asia (SEACLID/CORDEX-SEA). The result of the projection of trends of the fire hotspots by applying the FWI shows an overall significant increase in fire activities under the RCP4.5 and RCP8.5 scenarios in the future. The average FWI reached 9.6 and 11.1 under RCP4.5 and RCP8.5 scenarios, respectively. The average percentage increase of FWI in the future under the RCP8.5 scenario is 43.9%, higher than under the RCP4.5 scenario, which is 39.7%. In short, the result of this study provides an understanding of how fire events condition in the future as the efforts to control the forest and land fire disasters which affect the biomass burning haze.


AS55-A006
Systematic Long-term Analyses of Simultaneous Multipoint Wood-log and Biomass Burning Caused by Holikadahan: Regional Comparison of West, Central, and East Indo-gangetic Plains

Bharat Ji MEHROTRA1#+, Shivam SINGH1, Atul K. SRIVASTAVA2, Abhay Kumar SINGH1, Sudhir SHARMA3, Manoj Kumar SRIVASTAVA1
1Banaras Hindu University, 2Indian Institute of Tropical Meteorology, 3CSIR- National Physical Laboratory

Research has shown that short term events, such as forest-fires, agricultural-burning, dust-storms, fireworks, etc., significantly contribute to air-pollution, and impact the climate, air-quality, visibility, human-health, etc. Festivals that are marked by firework displays and wood-log fires are among these transient events that severely alter the local air-quality. In India, two major festivals, Diwali and Holi, are celebrated throughout the country, and are dominated by fireworks and wood-log/ biomass burning, respectively. As per the religious belief, Holi is preceded by Holikadahan, when wood-log/ biomass is burned in the last evening. The burning results in the emission of huge amounts of gaseous and particulate pollutants. Innumerable point sources Holikadahan in the vicinity make Holikadahan a huge polluter on a regional basis.The study, spanning six years (2017-2022), was conducted using data collected from 12 cities, extending from west to east in the Indo-Gangetic plains (IGP) to examine the impact of Holikadahan by comparing the period of background levels, pre-Holikadahan, and Holikadahan of PM2.5, PM10 and aerosol optical depth (AOD). As a general observation, the highest spike in pollutant concentrations, including PM2.5, PM10 were observed during the Holikadahan and immediately after the Holikadahan, followed by a decreasing trend, back to background levels, typically after 24-hours.In the western IGP, the maximum impact of Holikadahan on air-quality was observed in 2021, showing 71%, 63% and 82% increase in PM2.5, Pm10, and AOD values, respectively, between pre-Holika and Holika. Similar increases in central IGP, observed in 2021, were 80%, 25% and 55%, respectively. In the eastern IGP, however, the maximum impact was observed in 2020, with 74% and 75% increase in PM2.5 and PM10 concentration, respectively. This increase in primary data is expected to change the localized air-quality index (AQI), aerosol radiative forcing efficiency, and atmospheric heating-rate.


Tue-01 Aug | 8:15 - 10:00 | MR333
AS27 - From Weather Predictability to Controllability

Session Chair(s): Takemasa MIYOSHI, RIKEN Center for Computational Science, Tetsuo NAKAZAWA, The University of Tokyo

AS27-A004
Quantifying Weather Controllability and Mitigatable Flood Damage Based on Ensemble Weather Forecast

Shunji KOTSUKI#+
Chiba University

For realizing a weather-controlled society, we need to discuss the way to maximize the effect of manipulations to the atmosphere. For that purpose, this project aims at developing methods that quantify weather controllability and mitigatable flood damage based on ensemble weather forecasts. To quantify weather controllability, this project investigates meteorological landscapes that separate disaster and non-disaster regimes which may be controllable with small manipulations. We also estimate economic damages under non-controlled/controlled scenarios, in order to quantify avoidable damage by weather control. We have started illustrating directed graphs as the first step in understanding the meteorological landscape. Typhoon Prapiroon in 2018 was used for the case study. Singular value decomposition (SVD) is employed for Japan Meteorological Agency’s operational meso-scale ensemble prediction data to extract principle components of atmospheric states, followed by a clustering using density-based spatial clustering of applications with noise known as DBSCAN. The illustrated graph succeeded in detecting separated two clusters that correspond to faster and slower movements of predicted Parapiroon. The developed algorithm is currently applied to other disastrous events as well as further investigations on non-linear data compression methods beyond SVD. This presentation includes the most recent achievements up to the time of the conference.


AS27-A001
A New Interpretation of Ensemble Sensitivity and its Potential Applications in Weather Controllability

Le DUC#+, Yohei SAWADA
The University of Tokyo

Ensemble sensitivity has been proved to be a very useful sensitivity measure in practice. In this study, we show the relevance of ensemble sensitivity in another important problem. Instead of estimating how each state element will change a forecast response, we now examine which analysis perturbation among all possible ones with the same magnitudes will yield the largest change in the forecast response. We have proved that changes of the forecast response are maximized along the direction of the vector consisting of ensemble sensitivities which forms the most sensitive perturbation. This fact is found to be applicable in the field of weather controllability. In the simplest problem of weather controllability, we concern the optimal perturbation that minimizes a damage cost over a critical area. This optimization problem can be solved with variational data assimilation techniques by including the damage cost into the cost function. However, the problem becomes more complicated if we consider two important factors: (1) the power of optimal perturbation is limited by our technology so that it is impossible to realize the optimal perturbation in reality; and more importantly (2) we need to control the damage not just over an area but over several areas and it is possible that the damage only redirected from an area to another area under modification. We will demonstrate how the new understanding on ensemble sensitivities can qualitatively give potential solutions for such complicated issues.


AS27-A005
Applying ESV to Identify the Sensitivity of Heavy Rainfall Prediction

Peng-Xiang LAI1#+, Shu-Chih YANG1, Kevin LUPO2, Ryan TORN2
1National Central University, 2University at Albany, State University of New York

Forecast sensitivity has been formulated to identify fast-growing perturbations in ensemble forecast. The ensemble singular vector (ESV), which doesn't require the tangent-linear and adjoint models, is derived in this study to obtain the critical initial condition that affects the ensemble forecast of high-impact events. While past researches mainly use this method in large-scale systems, this research examines the feasibility of ESV for long-lived heavy rainfall associated with synoptic-mesoscale fronts prediction. All of three cases show large rainfall forecast uncertainty in targeted area at validation time. The ESV is calculated using the metric of rainfall accumulation in the target area to evaluate the final forecast. To validate the evolution of ESV, the leading ESV is compared with the post forecast sensitivity defined by the difference between the members with high- and low-performance rainfall forecast in each case. In addition, the leading ESV is used to perturb the initial condition of the ensemble forecast to investigate the impact of ESV on rainfall forecasts. The preliminary result with a Mei-Yu front associated heavy rainfall event shows that the rainband can be effectively adjusted with the perturbed forecasts. Furthermore, , we confirm that the final ESV agrees with the evolution of the ESV-based initial perturbations under the non-linear model dynamic to a great extent. Finally, the effectiveness and challenges of applying ESV will be shown and discussed in this presentation. 


AS27-A003
Why Did Weather Modification Research in Japan and the United States Rapidly Decline in 1971?

Mirai ABE#+, Hironori FUDEYASU, Manami SASAOKA
Yokohama National University

The national project in Japan, the Moonshot Research and Development Program sets ambitious goals, and Goal 8 is “Realization of a society safe from the threat of extreme winds and rains by controlling and modifying the weather by 2050”. It is expected to develop weather control technology that is technically, ethically, legally and socially feasible. Between 1962 and 1983, research in hurricane modification centered on an ambitious experimental program, Project STORMFURY in the USA. In Japan, research on weather modification became active under the influence of Project STORMFURY. In this study, we investigated the weather modification research in 1960s and 1970s in Japan and the USA by looking through all the references and interviewing people. The main purpose of the project STORMFURY was to conduct cloud-seeding experiments within hurricanes. Unfortunately, during the Project, the project team didn not take good opportunities and was only able to conduct cloud-seeding experiments three cases. To increase experimental opportunities, the USA government proposed to Japan and other countries over the northwestern Pacific Ocean. The possibility of experimenting in the Pacific was considered, but it did not materialize. In Japan, weather modification research had been active for 7 years, but rapidly declined in 1971. In this presentation, we will report the reasons why the experimental relocation did not materialize and why the weather modification research declined in Japan. The USA had discussed the experimental relocation with countries concerned, but the results were not satisfactory and the deadline for reporting to the Navy was not met. In Japan, declining of weather modification research can be attributed to the 1971 Kawasaki accident, 15 people died in landslide experiments on artificially slopes. The members leading weather modification research at the time were involved in that accident. This research was supported by JST Moonshot R&D Grant Number JPMJMS2282.


AS27-A002
Impacts of Drag Coefficient on Typhoon Intensity Using the Numerical Simulations

Hiroaki YOSHIOKA1#+, Hironori FUDEYASU1, Ryuji YOSHIDA1, Junshi ITO2, Takeshi HORINOUCHI3
1Yokohama National University, 2Tohoku University, 3Hokkaido University

A project ”Moonshot Goal 8” supported by Japan Science and Technology Agency was established to study the possible weakening of typhoon intensity due to artificial interventions. One such measure is to increase the sea surface drag by using obstacles such as large ships. The maximum potential intensity theory suggests that the equilibrium intensity decreases as the surface drag coefficient increases if the surface enthalpy exchange is unaffected, but numerical studies to test it are limited. Previous fine-resolution simulations (e.g., with a sub-kilometer grid) tend to agree with the theoretical indication, but the number of cases is limited. 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 tropical cyclones would react to surface drag change over limited regions that can be set in various ways. As a first step, we conducted preliminary numerical simulations of Typhoon FAXAI in 2019 by changing the drag coefficient (CD) over the whole simulation area. Here we ran the Scalable Computing for Advanced Library and Environment (SCALE) at a coarse resolution of 5 km. The resultant minimum central pressure was nearly insensitive to CD, but the maximum winds were weakened by about 60 % of the control run (CTL) when CD was set to 1.5 to 3.5 times that in CTL. Also, the radii of average winds of 15ms-1 were decreased by about 20 %. We will conduct further studies until the meeting. This research was supported by JST Moonshot R&D Grant Number JPMJMS2282.


AS27-A006
Impacts of Decrease in Sea Surface Temperature Through the Released Deep Sea Water on Typhoon Intensity

Hironori FUDEYASU1#+, Takafumi HOSOGI1, Yasutomo KIYOHARA1, Hiroaki YOSHIOKA1, Kosuke ITO2, Koji INOUE3, Katsumi TAKAYAMA4, Kazuhiro TAKEUCHI4
1Yokohama National University, 2Kyoto University, 3NPO The Society of Ocean Romantics, 4IDEA Consultants, Inc.

A project of Moonshot Goal 8 supported by Japan Science and Technology Agency is to study the possibility to reduce typhoon intensity by artificial interventions. Ocean thermal energy conversion (OTEC) which is planned to be established in the ocean near Okinawa islands is considered one of artificial interventions. The OTEC technology collects cold deep sea water at a depth of 800m and warm sea water at a depth of 20m, and discharges this mixed water to a depth of 20m. Namely an OTEC decreases the sea surface temperature (SST). When a typhoon passes over the ocean where the SSTs are decreased by OTEC, it is considered that the typhoon intensity is lower than without an OTEC. The purpose of this study is to conduct a numerical simulation of real typhoons using an atmospheric model with a SST distribution simulated by ocean model including the effects of OTECs (OTEC experiment), and to evaluate the impact of a SST forcing in the OTEC (sensitivity experiment). In the case of 2020, Typhoon HAISHEN passed through the OTEC influence zone, and the central pressures of HAISHEN were 930hPa by the Best Track data created by the Regional Specialized Meteorological Center Tokyo-Typhoon Center, 924.4hPa by our experiment without OTECs effect, and 924.6hPa by the OTEC experiment with the cooled SST (from -0.05 to -0.02℃) spread from each point of OTECs to the north for 50 to 70 km (OTEC influence zone). In the sensitivity experiment, the central pressures of Haishen increased by 0.57hPa and 1.00hPa at SST forcing with -0.5℃ and -1.0 in the OTEC influence zone, respectively. The sensitivity experiment of the OTEC or SST forcing that effectively affects the other cases of typhoons will be investigated. This research was supported by JST Moonshot R&D Grant Number JPMJMS2282.


Tue-01 Aug | 10:20 - 12:20 | MR323
AS18 - The Science and Prediction of Tropical Cyclones

Session Chair(s): Satoki TSUJINO, Meteorological Research Institute, Di TIAN, Second Institute of Oceanography, Ministry of Natural Resources

AS18-A052 | Invited
Sea Surface Wind Structure in the Outer Region of Tropical Cyclones Observed by Wave Gliders

Di TIAN#, Han ZHANG+
Second Institute of Oceanography, Ministry of Natural Resources

Understanding the sea surface wind structure during tropical cyclones (TCs) is the key for study of ocean response and parameterization of air-sea surface in numerical simulation. However, field observations are scarce. In 2019, three wave gliders were deployed in the South China Sea and the adjacent Western Pacific region, which acquired sea surface wind structure of eight TCs. Analysis of the field data suggests that the wave glider-observed surface winds are consistent with most analysis/reanalysis data (i.e., ERA5, CCMP and NCEP-GDAS) and SMAP. Both wave glider observations and analysis/reanalysis data indicate that TC wind fields induce an obvious increase in speed toward the sea surface together with a sharp change in direction, showing an asymmetric wind structure which is sensitive to TC translation speed and intensity. Larger mean values of wind speed and inflow angle are located on the right side along TC tracks. The inflow angle shows a highly dynamic dependence on the radial distance from the TC center, the TC intensity, as well as the TC-relative azimuth. Comparisons between field observations and theoretical models indicate that the most widely used, ideal TC wind profile models can largely represent the observed sea surface wind structure, but generally underestimate the wind speed due to lack of consideration of background wind. Moreover, simple ideal models (e.g., the modified Rankine vortex model) may outperform complex models when accurate information of TCs is limited. Wave glider observations have potential for better understanding of air-sea exchanges and for improvements of the corresponding parameterization schemes.


AS18-A004 | Invited
Formation Mechanism of TC Secondary Eyewall by Numerical Experiments: Role of Dry Air Inflow from the Middle and Upper Troposphere and Cooling by Evaporation and Sublimation

Kyohei KASAMI, Masaki SATOH#+
The University of Tokyo

Eyewall Replacement Cycle (ERC) is often seen in TCs. ERC occurs when secondary eyewall forms outside the inner eyewall, and the inner eyewall disappears. ERC significantly impacts TC intensity, so revealing the mechanism is an important issue both scientifically and socially. Several mechanisms of secondary eyewall formation have been proposed. According to Huang et al. (2012), tangential wind enhancement associated with lower-level inflow causes secondary eyewall formation. The relationship between the mesoscale descending inflow (MDI) formed by diabatic cooling of stratiform precipitation areas and secondary eyewall formation has also been pointed out (Didlake et al. 2018). However, the detailed processes by which dry air inflow and diabatic cooling affect secondary eyewall formation through MDI are not yet well understood. Therefore, in this study, the role of dry air inflow from the middle and upper troposphere and diabatic cooling in secondary eyewall formation is investigated using numerical experiments. Idealized numerical experiments were conducted using the plane version of the nonhydrostatic icosahedral atmospheric model, NICAM. Control experiments confirmed the existence of dry air inflow in the middle and upper troposphere and the formation of downdrafts due to diabatic cooling. It was also confirmed that the mechanism of secondary eyewall formation by agradient force was working, as pointed out in previous studies. In a sensitivity experiment, we conducted an experiment to increase water vapor in the middle and upper troposphere outside the TCs. The results showed that the secondary eyewall formation was hindered and slowed down as the water vapor increased. We further conducted a realistic case study for Typhoon Haishen in 2020 and confirmed the above mechanism works for the ERC of Haishen.


AS18-A047
A New Method to Estimate Circulations in Tropical Cyclones from Single-Doppler Radar Observations

Satoki TSUJINO1#+, Takeshi HORINOUCHI2, Udai SHIMADA3
1Meteorological Research Institute, 2Hokkaido University, 3Japan Meteorological Agency

Doppler weather radars are a powerful tool for investigating the inner-core structure of tropical cyclones (TCs). The Doppler velocity from a single radar has no information on the wind component normal to the radar beam. Therefore, closure assumptions are needed to estimate the circulations of the TCs from single-Doppler radar observations. The Generalized Velocity Track Display (GVTD) technique used to estimate the TC circulations adopts the closure assumption of no asymmetric radial winds in the TC vortex.
The present study proposes a new closure assumption introducing asymmetric radial winds to improve the axisymmetric-circulations estimation in TCs with asymmetric structure in the GVTD retrieval formula. Our new method can consider the asymmetric radial winds by using streamfunction based on the Helmholtz decomposition theorem of horizontal winds. As with GVTD, the new method retrieves TC circulations based on the Fourier decomposition of winds in the azimuthal direction and the least-square fit of the Doppler velocity from the single radar observation. The new method and GVTD are applied to analytical vortices and a real typhoon. For the analytical vortices with asymmetric winds in wavenumber-2 vortex Rossby waves, the axisymmetric tangential wind of VT0 retrieved by the new method (GVTD) has a relative error of less than 2% (10%) near the radius of maximum wind speed. For the real typhoon, the GVTD-estimated VT0 has periodical fluctuations with an amplitude of about 5 m/s near the elliptical eyewall. The period of the fluctuations is approximately synchronized with the counterclockwise rotating period of the elliptical shape of the eyewall, suggesting pseudo-signals due to the closure assumption in GVTD. The periodical fluctuations are largely reduced in the estimated VT0 from the new method. We find that the new method can reduce the pseudo-signals of the GVTD-retrieved axisymmetric circulation in cases of asymmetric vortices.


AS18-A032
Consistent Pattern of Rainfall Asymmetry in Binary Tropical Cyclones

Jian-Feng GU1+, Hao-Yan LIU2#, Yuqing WANG3
1Nanjing University, 2Hohai University, 3Chinese Academy of Meteorological Sciences

Accurate prediction of rainfall distribution associated with tropical cyclone (TC) is very important for risk management but remains challenging due to complicated multi-scale interactions. Previous studies mostly focus on the precipitation associated with a single TC but little attention has been paid to the features of precipitation in binary tropical cyclone system. In this study, based on the satellite observations, a novel approach with rotated coordinate system is proposed to examine the binary TC interactions over the western North Pacific and the associated asymmetry of rainfall distributions. The results show that the asymmetric component of TC rainfalls strengthened with the decreasing of the separation distance between the two TCs. The results show that the asymmetric component of TC rainfalls enhances with the decreasing of the separation distance between the two TCs. A critical separation distance at about 2050 km for binary TCs could naturally emerge based on the relationship between the asymmetric rainfall component and the separation distance. This can be an observational reference for estimating the strength of binary-TC interaction and identifying binary TCs from two coexisting TCs. When two TCs become nearby, the asymmetric component of rainfall shows an increasing trend with rainfall significantly suppressed in Quadrant IV of the TC located to the west when orienting the two TCs in the west-east direction. The suppression becomes remarkable once the separation distance between the two TCs is within about 2,050 km. It is found that the convective activity in one TC is related to the deep-layer vertical wind shear (VWS) from its companion. Rainfall is enhanced downshear-left in a TC, consistent with a single TC embedded in an environmental VWS as found in previous studies. Our study suggests that the evolution of rainfall distribution under the binary-TC conditions could be potentially predictable at vortex scale.


AS18-A012
Diurnal Variations in Tropical Cyclone Intensification and Size Growth

Qiaoyan WU#+
Second Institute of Oceanography

Various aspects of tropical cyclones (TCs) fluctuate with the diurnal cycle. In this paper, diurnal variations in TC intensification and the growth of the radius of gale-force winds (34 kt; R34) over the Ocean for in global TCs were investigated using best-track data. Statistically significant diurnal variations were found for global TCs, with a maximum intensification over the period 03–09 local solar time (LST). No diurnal signals are detected for TC decay. Statistically significant diurnal variations are found for global TCs which experienced rapid intensification (RI, ≥30 knots within 24 h), with a maximum 6-h growth rate occurring at 03–09 LST. The highest rate of intensification and R34 growth rates at 03–09 LST for TCs were associated with the greatest coverage of very deep convective clouds with infrared brightness temperatures < 208 K at 03–06 LST. R34 growth is favored at the same time as TC intensification. This study suggests that nocturnal radiative cooling affects the intensity and outer region sizes.


AS18-A025
Tropical Cyclone Size Asymmetry Index and Climatology

Lifeng XU+, Kelvin T. F. CHAN#, Kailin ZHANG
Sun Yat-sen University

Size of tropical cyclone (TC) is often asymmetric in nature. Yet, there is a lack of clean and intuitive definition/expression to specify the asymmetry of TC size. Here, we introduce a novel index, TC size asymmetry index (SAI), which indexes both the degree and pattern of the asymmetry systematically. In particular, the symbolic form of SAI is vividly designated for identifying the latter. The SAI proposes 1 quasi-symmetric pattern and 28 asymmetric patterns in total. The 41-yr (1979–2019) global climatology of SAI shows that the distribution of the degree of TC size asymmetry is trimodal. Elementarily, the degree and pattern of TC size are found to be TC intensity, TC movement, time, and space dependent. The introduction of SAI does not only give an insight into the subject of TC size asymmetry but also lays important foundation for future applications and research. Furthermore, besides meteorology, it could inspire other fields to index the geometric asymmetries of other kinds.


AS18-A045
High-resolution Simulation of Tropical Cyclone Debbie (2017): The Current and Future Changes in the Inner-core Structure and Evolution During Offshore Rapid Intensification

Difei DENG1#+, Elizabeth A. RITCHIE2
1UNSW Canberra, 2Monash University

Tropical Cyclone Debbie (2017) made landfall near Airlie Beach on 28 March 2017 causing 14 fatalities and an estimated US$2.67B economic loss and was ranked as the most dangerous cyclone to hit Australia since TC Tracy in 1974. In addition to the extreme flooding as TC Debbie moved onshore and down the east coast of Australia, it intensified rapidly just offshore from Category 2 to Category 4 in approximately 18 hours and finally made landfall as a Category 4 TC, causing widespread and disastrous damage. A high-resolution WRF simulation (1-km horizontal, and 10-min temporal resolution) is used to analyze the inner-core structure and evolution during the offshore rapid intensification period in the current conditions and potential future change. In current condition, Debbie’s a rapid intensification (RI) stage is characterized by three rounds of eyewall breakdown into mesovortices and re-development events. Each round of breakdown and re-establishment brings high potential vorticity and equivalent potential temperature air back into the eyewall, re-invigorating eyewall convection activity and driving intensification. The potential future changes in the inner-core structure and eyewall evolution will also be discussed using WRF with the Coupled Model Intercomparison Project Phase 6 (CMIP6) perturbed conditions to better assess the possible TC intensity change under different climate change scenarios. 


AS18-A070
Evolution of Background Circulation and Thermodynamic Conditions Before and After the Onset of Typhoon Rapid Intensification

Shuanzhu GAO#+, Xinyan LYU
National Meteorological Center

Using the tropical cyclone best track data from Shanghai Typhoon Institute of CMA of 1949-2020 and the reanalysis data of the European Centre for Medium-Range Weather Forecasts of 1991-2020, and the joint EOF analysis of u and v components of the wind field on the 200 and 850 hPa, the characteristics of the larger-scale circulation at onset of the rapid-intensification typhoon are summarized, and the evolutions of environmental dynamic and thermal conditions during the ±12 h period at the onset of typhoon rapid intensification are further analyzed. The results indicate that the lower level of the main circulation of EOF decomposition is the convergence pattern of monsoon trough at the onset of the typhoon rapid intensification, and the circulation is conducive to the low-level water vapor transport of typhoon. The upper-level circulation has obvious typhoon outflow channels, and the characteristic can be used as a typical circulation for the rapid intensification forecast. The thermal conditions such as sea surface temperature, water vapor and convective instability, as well as dynamic conditions such as environmental vertical wind shear and the strength of upper-level outflow all can generally reach the fitness range of conditions that are favorable for typhoon intensification. However, the values of above environmental factors have not changed significantly or suddenly during the transition from the slow intensification process to rapid intensification process. Even some extreme cases show that the change tend of environmental factors towards to the unfavorable conditions. These research results provide a reference for the prediction of rapid intensification and further study of typhoon in the future. As for the unfavorable conditions in RI some cases, whether there are other favorable factors to offset the negative effects of these conditions and what are the corresponding physical processes, these issues need to be further studied in the future.


Tue-01 Aug | 10:20 - 12:20 | MR327
AS23 - Observations, Remote Sensing, and Modeling of Tropospheric Composition and Air Quality in Asia and the Transpacific Region

Session Chair(s): Minghui TAO, Chinese Academy of Sciences

AS23-A068 | Invited
Three Decades of Atmospheric Aerosols Column Measurements from AERONET

Pawan GUPTA1#+, Elena LIND1, Brent HOLBEN1, Thomas ECK1, David GILES2,1, Alexander SMIRNOV3,1, Joel SCHAFER2, Aliaksandr SINYUK1, Ilya SLUTSKER3,1, Mikhail SOROKIN1, Jason KRAFT1, Arsenio MENENDEZ2, Zane MCBRIDGE2, Hal MARING4, Sheng-Hsiang WANG5, Huizheng CHE6, Neng-Huei LIN5, Jhoon KIM7, Itaru SANO8
1NASA Goddard Space Flight Center, 2Science Systems and Applications, Inc., 3Sigma Space Corporation, 4NASA Headquarters, 5National Central University, 6Chinese Academy of Meteorological Sciences, 7Yonsei University, 8Kindai University

The AERONET program is a federation of ground-based sun-photometer networks and operates in partnership with various national and international agencies, universities, institutions, research groups, and individual scientists and stakeholders. It provides worldwide observations of spectral aerosol optical depth, inversion products (microphysical and radiative properties), and precipitable water across diverse aerosol regimes. In addition, other network components enable measurements of normalized water-leaving radiance, solar flux, and marine aerosols. For the past three decades, AERONET has been providing long-term, continuous, and readily accessible public-domain datasets. The network has been growing steadily, with currently about 600 active sites. The program also supports research and application field campaigns around the world. The program continues to refine instrumentation, measurement techniques, and algorithms through research and development. AERONET has recently started making nighttime aerosol measurements using direct moon observations. The program's biggest strength is its imposition of standardized of instruments, calibration, quality control, processing, and data distribution. This presentation will provide an overview of the program with examples of available datasets, current research, and applications. We will also highlight important upcoming satellite missions, field campaigns, and new research results from the AERONET team at NASA Goddard. The presentation will highlight ongoing data analysis focused on the Asia-Pacific region by the GSFC team.


AS23-A065
GEMS Validation Campaign-GMAP 2021

Limseok CHANG1#+, Hyunkee HONG1, Donghee KIM1, Soi AHN2
1National Institute of Environmental Research, 2National Institute of Environmental Research(NIER)

The GEMS validation campaign was conducted in the Seoul Metropolitan Area (SMA) from October to November, 2021. Twenty-four research teams participated in four platforms: ground remote sensing, chemical sonde, ground and airborne in situ chemical analysis, and chemical transport modeling. In particular, 5 Pandora and 5 MAX-DOAS were deployed within SMA, and 3 Car-DOAS were operated throughout SMA. Preliminary results showed that diurnal variations in the NO2 and HCHO columns in ground remote sensing matched well with those in GEMS. Car-DOAS yielded pollution maps in detail, which were used for subgrid variability analysis. The various shapes in the vertical profile of NO2 retrieved from MAX-DOAS and directly measured from the airborne NO2 monitor demonstrate the importance of A prior in GEMS VCD calculation.


AS23-A073
Characterization of the PBL Structure and PM2.5 in Taiwan: T-POMDA Field Campaign and Modeling

Fang-Yi CHENG#+, Sheng-Hsiang WANG, Shu-Chih YANG, Yi-Cheng LIN, Chih-Kuan WANG
National Central University

The intensive field observations were conducted in central to southwestern Taiwan to clarify the physical and chemical processes and emission sources that lead to the serious PM2.5 problem. The deployment of the atmospheric observations included the wind profiler, radiosonde, unmanned aerial vehicle (UAV), lidar, and surface datasets. These observations provide the wind fields, temperature, humidity, and aerosol information with high temporal and vertical resolutions in the planetary boundary layer (PBL). In addition, the PBL ensemble data assimilation system was developed based on the Weather Research and Forecasting Local Ensemble Transform Kalman Filter (WRF-LETKF) framework coupled with the Community Multiscale Air Quality (CMAQ) model. We applied WRF and CMAQ models, and observations, to characterize the PBL vertical structures, evolutions, and air pollutants transport and dispersion processes. The preliminary analysis of the observation and model results demonstrate that the development of the PBL depth was limited due to the enhanced atmospheric stability in the PBL and the strong subsidence process from the layer above. The coastal sites revealed a shallow PBL depth; yet, the inland sites revealed a well-mixing PBL structure during the day. The lidar and radiosonde revealed distinct layer structures of the PM2.5 concentrations. The model can reproduce the observed features and assist in discussing the air pollution transport processes.


AS23-A034
Extensive Characterization of Aerosol Optical Properties and Chemical Component Concentrations: Application of the GRASP/component Approach to Long-term AERONET Measurements

Xindan ZHANG1#+, Lei LI1, Cheng CHEN2, Oleg DUBOVIK3, Huizheng CHE1, Yu ZHENG1
1Chinese Academy of Meteorological Sciences, 2UMR 8518 – Laboratoire d’Optique Atmosphérique, 3University of Lille

A recently developed GRASP/Component approach (GRASP: Generalized Retrieval of Atmosphere and Surface Properties) was applied to AERONET (Aeronet Robotic Network) sun photometer measurements in this study. Unlike traditional aerosol component retrieval, this approach allows the inference of some information about aerosol composition directly from measured radiance, rather than indirectly through the inversion of optical parameters, and has been integrated into the GRASP algorithm. The newly developed GRASP/Component approach was applied to 13 AERONET sites for different aerosol types under the assumption of aerosol internal mixing rules to analyze the characteristics of aerosol components and their distribution patterns. The results indicate that the retrievals can characterize well the spatial and temporal variability of the component concentration for different aerosol types. A reasonable agreement between GRASP BC retrievals and MERRA-2 BC products is found for all different aerosol types. In addition, the relationships between aerosol component content and aerosol optical parameters such as aerosol optical depth (AOD), fine-mode fraction (FMF), absorption Ångström exponent (AAE), scattering Ångström exponent (SAE), and single scattering albedo (SSA) are also analyzed for indirect verifying the reliability of the component retrieval. It was demonstrated the GRASP/Component optical retrievals are in good agreement with AERONET standard products [e.g., correlation coefficient (R) of 0.93 – 1.0 for AOD, fine-mode AOD (AODF), coarse-mode AOD (AODC) and Ångström exponent (AE); R = ~ 0.8 for absorption AOD (AAOD) and SSA; RMSE (root mean square error) < 0.03 for AOD, AODF, AODC, AAOD and SSA]. Thus, it is demonstrated the GRASP/Component approach can provide aerosol optical products with comparable accuracy as the AERONET standard products from the ground-based sun photometer measurements as well as some additional important inside on aerosol composition.


AS23-A003
New Top-down Spatially Distributed Daily Emissions Inventory for Black Carbon Driven by OMI and AERONET Observations

Jian LIU1+, Jason COHEN2#, Steve YIM1
1Nanyang Technological University, 2China University of Mining and Technology

Changes in urbanization, industry, and biomass burning in South, Southeast, and East Asia, have led to rapidly changing emissions of gasses and aerosols. These changes are due to missing and misrepresented sources, extreme events, and time-varying sources. Due to few ground stations outside urban areas in China, Korea, Japan, Singapore, and Thailand, this work uses a new, model-free approach in combination with daily OMI measurements of NO2 and UV, to identify and quantify emissions where measurements are available. An emphasis is made in regions that have undergone rapid or significant change. Using observations from the same platform takes advantage of consistent spatial and temporal coverage while taking advantage of the fact that NO2 and BC are co-emitted from the same processes and under the same thermodynamic conditions. The BC mass, size, and number loadings are all computed using AERONET SSA and a core/shell-constrained MIE model. Through the application of the mass-conserving model-free approach constrained by first-order approximations of wet and dry deposition, chemical aging, and dynamic transport, the computed number, size, and mass emissions profiles are computed. Differences between existing a priori emissions from FINN and EDGAR are compared with the top-down emissions database and the ranges of allowable physical, chemical, and dynamical terms. All products and analyses are done grid-by-grid in both space and time, with an emphasis on extreme events previously identified from OMI NO2 columns in 2016.The results demonstrate a significant underestimation in rural areas in Myanmar, Northern Thailand, Laos, and Northeast India, as well as in suburban areas around cities in Southeast Asia. However, some highly developed areas have overestimated emissions, likely due to more strict environmental enforcement, including Shanghai, Singapore, and Taibei. The uncertainty and day-to-day variability are examined in further detail, supporting that the inversion results are statistically significant in the regions mentioned.


AS23-A045
Towards Continuous Cargo Ship-based Observations of Greenhouse Gases and Air Pollutants by a Novel Semi-automatic FTIR - UV Spectrometer

Astrid MUELLER1#+, Hiroshi TANIMOTO1, Takafumi SUGITA1, Prabir K. PATRA2,3, Matthias FREY1, Ralph KLEINSCHEK4, André BUTZ4, Isamu MORINO1, Vincent ENDERS4, Karolin VOSS4, Shin-ichiro NAKAOKA1, T. MACHIDA1
1National Institute for Environmental Studies, 2Japan Agency for Marine-Earth Science and Technology, 3Tohoku University, 4Heidelberg University

Simultaneous observations of carbon dioxide (CO2), the major greenhouse gas (GHG), and nitrogen dioxide (NO2), a tracer for fossil fuel combustion, help to identify and quantify anthropogenic CO2 sources. Ship-, aircraft-, and ground-based observations together with satellite observations of GHG and other trace gases aim to better understand changes in their atmospheric concentrations. To achieve this goal, the global coverage of in situ observations by public and private networks is expanding, and new satellite missions are scheduled like that of GOSAT-GW. By using an approach to integrate ship data of the Ship-of-Opportunity program and aircraft data of the Comprehensive Observation Network for Trace gases by Airliner, we set up a framework to evaluate satellite observations of the column-averaged dry-air mole fractions of, for example, CO2 (XCO2) over the ocean. Although the applicability to CH4 is currently limited due to the sparseness of in-situ data, we explore the potential of this approach for the future when the observation networks are expanded. Complementary to this approach to constrain anthropogenic CO2 emissions and to validate CO2 and NO2 data of the GOSAT-GW mission, we are aiming to make continuous cargo ship-based observations of XCO2, XCH4, and XCO using a semi-automatic Fourier transform infrared (FTIR) spectrometer, combined with a UV spectrometer to measure the vertical column densities of NO2 (VCDNO2). The setup, developed by the Heidelberg University, consisted initially only of the mobile semi-automatic FTIR, and was tested for the first time on a cargo ship in the summer 2022. Currently, the Heidelberg University is integrating the UV spectrometer. Scheduled for end of this year, the novel setup will be deployed on a cargo ship operating along major anthropogenic emission sources of the Japanese East Coast. We will present the concepts, challenges, and perspectives for validating future satellite missions and monitoring anthropogenic emissions.


AS23-A005
POMINO-GEMS: A Research Product for Tropospheric NO2 Columns from Geostationary Environment Monitoring Spectrometer

Yuhang ZHANG1+, Jintai LIN1#, Jhoon KIM2, Hanlim LEE3, Junsung PARK3, Hyunkee HONG4, Van Roozendael MICHEL5, Francois HENDRICK5, Ting WANG6, Pucai WANG6, Qin HE7, Kai QIN7, Yongjoo CHOI8, Yugo KANAYA9, Jin XU6, Pinhua XIE6, Xin TIAN10, Sanbao ZHANG11, Shanshan WANG11, Robert SPURR12, Lulu CHEN1, Hao KONG1, Mengyao LIU13
1Peking University, 2Yonsei University, 3Pukyong National University, 4National Institute of Environmental Research, 5Royal Belgian Institute for Space Aeronomy, 6Chinese Academy of Sciences, 7China University of Mining and Technology, 8Hankuk University of Foreign Studies, 9Japan Agency for Marine-Earth Science and Technology, 10Anhui University, 11Fudan University, 12RT Solutions, 13Royal Netherlands Meteorological Institute

Nitrogen dioxide (NO2) is a major air pollutant. Tropospheric NO2 vertical column densities (VCDs) retrieved from sun-synchronous satellite instruments have provided abundant NO2 data for environmental studies, but such data are limited by insufficient temporal sampling (e.g., once a day). The Geostationary Environment Monitoring Spectrometer (GEMS) launched in February 2020 will retrieve NO­2 at an unprecedented high temporal resolution. Here we present a research product for tropospheric NO2 VCDs, referred to as POMINO-GEMS. We develop a hybrid retrieval technique combining GEMS and TROPOMI observations as well as GEOS-Chem simulations to generate hourly tropospheric NO2 slant column densities (SCDs). We then derive tropospheric NO2 air mass factors (AMFs) with explicit corrections for the anisotropy of surface reflectance and aerosol optical effects, through pixel-by-pixel radiative transfer calculations. Prerequisite cloud parameters are retrieved with O2-O2-based cloud algorithm by using ancillary parameters consistent with those used in NO2 AMF calculations. Initial retrieval of POMINO-GEMS tropospheric NO2 VCDs for June–August 2021 exhibit strong hotspot signals over megacities and distinctive diurnal variations over polluted and clean areas. POMINO-GEMS NO2 VCDs agree well with our POMINO-TROPOMI v1.2.2 product (R = 0.96, and NMB = 6.9%). Comparison with MAX-DOAS VCD data at five sites shows a small bias of POMINO-GEMS (NMB = –12.2%); however, the correlation for diurnal variation varies from -0.57 to 0.86, suggesting strong location-dependent performance. Surface NO2 concentrations estimated from POMINO-GEMS VCDs are consistent with measurements from the Ministry of Ecology and Environment of China at 855 sites (NMB = – 5.6%, and R = 0.96 for diurnal correlation averaged over all sites). POMINO-GEMS will be made freely available for users to study the spatiotemporal variations, sources and impacts of NO2.


AS23-A046
Synergistic Use of Atmospheric Dispersion Modelling and Satellite Products to Study Smoke Haze Emissions in Southeast Asia

Efthymia PAVLIDOU1#+, Chee-Kiat TEO2, Boon Ning CHEW2, Zhong Yi CHIA2, Phoebe JULIAN1,3, Peng YUAN SNG4
1Meteorological Service Singapore, 2Centre for Climate Research Singapore, 3Nanyang Technological University, 4National University of Singapore

Local environmental conditions in Southeast Asia, especially high humidity and frequent cloud cover, pose challenges in atmospheric monitoring both via modelling and when using satellite observations. We explore opportunities to address such challenges in the case of smoke haze dispersion, with the synergistic use of model outputs and satellite products. The Numerical Atmospheric-dispersion Modelling Environment (NAME) is an atmospheric pollution dispersal modelling tool capable of simulating and forecasting many atmospheric dispersion phenomena and associated physical and chemical processes. Himawari is a geostationary satellite providing high frequency multispectral observations. We use Himawari Aerosol Optical Depth (AOD) and Fire Radiative Power (FRP) products. We focus on 2019 and explore use of Himawari FRP, instead of the MODIS FRP assimilated by CAMS GFAS which is currently used as input to NAME. The aim is to evaluate the impact of the higher observation frequency of Himawari and the differences in saturation limit between the two instruments on the emission outputs of the model. We further compare model-derived AOD with Himawari AOD data, to get a view of the uncertainties of AOD estimation. Finally, we train a Machine Learning algorithm to translate AOD to column-integrated Particulate Matter emissions using NAME model simulations. This translation is traditionally done using smoke mass extinction coefficients measured in laboratory experiments or field expeditions. However, there is limited availability of such data in Southeast Asia, and their accuracy is further impacted by high levels of humidity in the region and plume aging. Use of model outputs in the ML algorithm could complement the lack of data and cover a wider range of local conditions. Based on our findings, we discuss potential synergistic use of satellite products and NAME outputs, for research regarding deriving smoke haze emissions in the region as well as for operational monitoring and forecasting of haze dispersion.


Tue-01 Aug | 10:20 - 12:20 | MR329
AS11 - Atmospheric Chemistry in Highly Polluted Environments: Emissions, Fate, and Impacts

Session Chair(s): Sri KOTA, Indian Institute of Technology Delhi

AS11-A015 | Invited
Unaccounted Anthropogenic and Natural Emissions of Nitrogen Oxides in China Over 2012–2022 Revealed from OMI and TROPOMI

Jintai LIN1#+, Hao KONG1, Yuhang ZHANG1, Mengyao LIU2
1Peking University, 2Royal Netherlands Meteorological Institute

NOx (NOx = NO + NO2) is a major component of air pollution with substantial spatiotemporal variations. Current emission inventories lag in time for several years and can hardly capture the fine-scale spatial pattern of NOx emissions. Here we develop a novel 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. We apply the algorithm to obtain NOx emissions for China at 5 km resolution in summer (JJA) 2012–2022 based on POMINO NO2 VCD data for OMI and TROPOMI instruments. Our PHLET data reveal many fine-scale emission details and considerable small-to-medium-scale sources missing in current anthropogenic inventories. Those missing sources are associated with human activities reflected in road network and Tencent user location data. Our PHLET data also show substantial inter-regional differences in interannual variations and trends of NOx emissions over the past decade, which are also absent in current inventories. Although the total NOx emission in China has been decreasing, the contribution of emissions from the western provinces to the national total has been growing and has exceeded the contribution of the eastern coastal provinces. Besides the anthropogenic sources, our PHLET retrieval discovers large NOx emissions from natural lakes on the Tibet Plateau that are previously unknown. Such emissions are likely a result of the anammox process under rapid warming over the plateau as an unaccounted feedback between climate change, lake ecology and nitrogen emissions. Overall, our NOx emission retrieval serves as a crucial tool to detect and quantify anthropogenic and natural emissions at fine scales, in support of air quality and climate modeling and targeted emission mitigation.


AS11-A019
Molecular Characterization of Atmospheric Particulate Organosulfates from the Port Environment Using Ultrahigh Resolution Mass Spectrometry: Identification of Ship Emissions

Lijuan QI1#+, Huan LIU2
1Qinghai University, 2Tsinghua University

Organosulfates (OSs) as important constituents of atmospheric organic aerosol (OA) are widespread in ambient environments. Although the sources, formation process, and chemical composition of OSs have been diversely studied, OSs formed by anthropogenic emissions are still little known. In this study, the molecular compositions of OSs in atmospheric PM2.5 samples collected from a winter measurement campaign (SEISO-Bohai) at Jingtang Harbor, a typical traffic environment, are characterized by ultra-performance liquid chromatography (UHPLC) coupled to electrospray ionization ultrahigh resolution mass spectrometer (UHRMS) Orbitrap. The changing trends of the port OS chemical compositions are observed from one complete haze pollution episode, which happened in this campaign. Along with the increased degree of haze pollution, the relative abundances of OSs have been apparently added and the molecule structures have become more complex. The processes of oxidation and fragmentation drive the OS formations in the haze environment. Then, the potential precursors from ship emissions are identified based on the “OS precursor map” created by previous study. The high molecular weight and low degree of unsaturation and oxidization of OSs are suggested to be mainly derived from ship intermediate/semi-volatile organic compound (I/SVOC) emissions. These OSs have appeared the wide range of molecule weight and good chemical homogeneity in the clean aerosol samples. In addition, our study also finds that ship emissions should further facilitate the production of OSs under the haze pollution condition. 


AS11-A020
Long-term Variations of Air Quality in India: A Study Using WRF-CMAQ Models

Mengyuan ZHANG1#+, Sri KOTA2, Peng WANG1, Hongliang ZHANG1
1Fudan University, 2Indian Institute of Technology Delhi

Air pollution in India is a growing concern, which has significant adverse effects on human health and ecosystems. However, there are very limited observations of air pollutants, and assessments of specific effects of air pollution are hindered. This study aims to simulate air pollutants in India from 2015 to 2019 using the Community Multi-scale Air Quality (CMAQ) model at the resolution of 36 × 36 km2. 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) and the MIX Asian emission inventory. Emissions are adjusted to simulation years with different adjustment coefficients for different sectors and states. Biogenic and wildfire emissions are also provided to CMAQ. After the model results are validation, the levels, health and ecosystem effects are analyzed. The study would reveal the importance of controlling particulate matters and ozone in India and provide information for designing effective control strategies.


AS11-A024
Biogenic Volatile Organic Compounds Enhance Ozone Production and Complicate Control Efforts: Insights from Long-term Observations in Hong Kong

Yingnan ZHANG1+, Tao WANG1#, Likun XUE2
1The Hong Kong Polytechnic University, 2Shandong University

With decreases in anthropogenic precursors, natural precursors may become more important in O3 pollution. However, the biogenic volatile organic compounds (BVOCs) change and its impact remain unclear due to the lack of long-term measurements of VOCs. In this study, we emphasize the increasingly important role of BVOCs in O3 pollution by analyzing the long-term measurements in Hong Kong obtained during 2013–2019. Driven by the warming temperature, biogenic isoprene at a suburban site in Hong Kong increased 0.05 ± 0.02 ppbv/yr (9%/yr), which is in sharp contrast to the decreases in anthropogenic precursors during study period. Detailed chemical modeling shows that increased BVOCs enhanced local O3 production by 25%, and the most obvious effect was shown in summer. Increased BVOCs also affected the non-linear relationships between O3 and anthropogenic precursors, i.e., increasing the O3 sensitivity to nitrogen oxides (NOx) and decreasing the O3 sensitivity to anthropogenic VOCs (AVOCs). Despite changes in precursors, the O3 formation remains in VOC-limited regimes at Tung Chung. Joint control of AVOCs and NOx (at a ratio greater than 1.2) would help avoid exacerbation of O3 pollution and reduce NO2 pollution. Our findings also suggest the BVOCs increase likely have occurred in the larger Pearl River Delta (PRD) region, and thus the results from our study in Hong Kong may have implications for developing AVOCs/NOx reduction measures in the PRD region and beyond.


AS11-A025
Ambient Measurements of Heterogeneous Ozone Oxidation Rates of Oleic, Elaidic, and Linoleic Acid Using a Relative Rate Constant Approach in an Urban Environment

Qiongqiong WANG1#+, Jian Zhen YU2
1China University of Geosciences, 2The Hong Kong University of Science and Technology

Long-chain unsaturated fatty acids (uFAs), such as oleic acid, undergo rapid degradation via heterogeneous reactions with atmospheric oxidants upon emission. The oxidation mechanism and kinetics have been extensively studied in laboratory experiments. However, quantitative knowledge of degradation rates under real-world atmospheric conditions is scarce. We obtained the nighttime decay rates of three cooking-related uFAs using a relative rate approach applied to bihourly measured data in urban Shanghai. The estimated lifetime of oleic acid was 6 h under conditions of ∼12 ppb ozone and 60%–100% relative humidity encountered at our urban location or an inferred ∼2 h at a higher ozone level of ∼40 ppb. The decay rates of elaidic and linoleic acid are determined to be 0.62 and 1.37 that of oleic acid, respectively. This work provides the first kinetic data pertaining to real-world conditions. They are valuable for constraining the modeling of heterogeneous aging of ambient organic aerosols.


AS11-A026
Implication for Polycyclic Aromatic Hydrocarbons: From the Present-day to the Future

Sijia LOU1#+, Manish SHRIVASTAVA2
1Nanjing University, 2Pacific Northwest National Laboratory

Polycyclic aromatic hydrocarbons (PAHs) are unavoidably derived from combustion processes, and are contaminants of global concern because they increase the risk of lung cancer and are detrimental to human health and the ecosystem. While high concentrations of PAHs were already measured in 2008, future changes in energy use, land use, and climate policy may alter the PAHs concentrations. Integrating a global atmospheric chemistry model, a lung cancer risk model, and plausible future emissions trajectories of PAHs, we assess how global PAHs and their associated lung cancer risk will likely change in the future. Benzo(a)pyrene (BaP) is used as an indicator of cancer risk from PAH mixtures. From 2008 to 2050, the population-weighted global average BaP concentrations under all RCPs consistently exceeded the WHO-recommended limits, primarily attributed to residential biofuel use. Peaks in PAH-associated incremental lifetime cancer risk shift from East Asia (4×10-5) in 2008 to South Asia (mostly India, 2-4×10-5) and Africa (1-2×10-5) by 2050. In developing regions of Africa and South Asia, PAH-associated lung-cancer risk increased by 30-64% from 2008 to 2050, due to increasing residential energy demand in households for cooking, heating, and lighting as the rapid population growth, as well as the continued use of traditional biomass use, increases in agricultural waste burning, and forest fires. With the stringent air quality policy, PAH lung-cancer risk substantially decreases by ~80% in developed countries. Climate change is likely to have minor effects on PAH lung-cancer risk compared with the impact of emissions. Future policies, therefore, need to consider efficient combustion technologies that reduce air pollutant emissions, including incomplete combustion products such as PAH.


AS11-A028
Seasonal and Spatial Heterogeneities of PM, Chemical Constituents and Sources Contribution at Vijayawada City, Andhra Pradesh India

Manuj SHARMA1#+, Suresh JAIN2,1
1Indian Institute of Technology Tirupati, 2Indian Institute of Technology Delhi

Aiming to control the rising Particulate Matter (PM) emissions, many researchers highlighted the importance of identifying PM sources within and transboundary of the city. This study investigates the seasonal and spatial heterogeneity of PM concentration and chemical characteristics. The source apportionment technique was performed to identify the potential sources' contribution in Vijayawada city. Based on the land use land cover (LULC) pattern, the atmospheric PM10 and PM2.5 samples were collected at multiple monitoring sites with Traffic, Commercial, Industrial, Residential, and Background characteristics during winter and summer. The highest average PM concentration (PM10: 154±42 µg/m3, PM2.5: 82±21 µg/m3) was measured at the industrial site in winter followed by traffic, commercial, background, and residential sites with an estimated difference of (20%, 14%), (31%, 30%), (36%, 34%) and (36%, 25%), respectively. A similar trend was observed in the summer season, with the highest concentrations at the industrial site (PM10: 86±24 µg/m3, PM2.5: 52±15 µg/m3) followed by traffic, commercial, background and residential sites. Secondary Inorganic Aerosols (SIA) (7-35%, 6-24%) and crustal elements (4-35%, 11-18%) were observed to be the significant components in PM10 and PM2.5 mass size fraction, respectively. Low OC/EC ratio values ranging from 0.98-2.95 indicate a high proportion of gasoline and diesel emissions in the urban atmosphere. Chemical Mass Balance (USEPA CMBV5.0) model identified vehicular, industrial, construction, road dust, SIA, biomass burning, and coal combustion sources, respectively, with a significant variation in seasonal and spatial contributions. Vehicular emission is one of the primary sources, contributing 47-16% in PM10 and 51-22% in PM2.5, followed by the combined contribution of biomass and coal combustion, which varies from 35-13% and 31-20% in PM10 and PM2.5, respectively. High biomass and coal combustion emissions were attributed to several industrial units which use coal, wood, briquettes, etc., for fuel requirements.


AS11-A029
Diagnosing Drivers of Modeling Bias in Fine Particulate Matter Simulations: An Efficient Machine Learning Based Method

Shuai WANG+, Peng WANG, Hongliang ZHANG#
Fudan University

Accurate modeling of PM2.5 is essential for effective air quality management and mitigation. Chemical transport models (CTMs) like the Community Multiscale Air Quality (CMAQ) model, are widely used for PM2.5 simulation through atmospheric processes of dispersion, deposition, and chemical reactions. However, CMAQ often suffers from biases due to limitations in model structure, uncertainties in initial and boundary conditions, and insufficient representation of meteorological conditions and source contributions. Traditional methods for model bias diagnosis usually rely on empirical and priori assumptions and require extensive sensitivity tests with high demands on computational resources, such as Monte Carlo methods or Latin hypercube sampling. Recently machine learning (ML) methods have been widely used in environmental science researches due to their simple structure, fast speed and ability to deal with no-linear relationships. ML also provides a new perspective on the identification of simulation biases. However, as a complex multi-phase mixture, it is still challenging to diagnose biases in PM2.5 simulations using ML methods. In this study, we plan to diagnose the drivers of the model bias in simulating surface PM2.5 concentrations based on the lightGBM model, an efficient ensemble ML method. The individual components of PM2.5 will be simulated using CMAQ and the sectoral sources of PM2.5 will be tracked using source apportionment methods. CMAQ simulation bias will be diagnosed from multiple perspectives, including meteorology, PM components, and sectoral sources. The results of this study can provide new ideas for CTMs model biases diagnosis, deepen the understanding of CMAQ simulation biases, and provide information for model improvement.


Tue-01 Aug | 10:20 - 12:20 | MR331
AS01 - The Asian Monsoon, Extremes and Climate Change

Session Chair(s): Kyung-Ja HA, Pusan National University, Ramesh KRIPALANI, Indian Institute of Tropical Meteorology, Renguang WU, Zhejiang University

AS01-A084
Monsoon Planet: Competing Effect of Global Warming and Aerosol Concentration

Anja KATZENBERGER1,2#+, Anders LEVERMANN1
1Potsdam Institute of Climate Impact Research, 2University of Potsdam

Monsoon systems are transporting water vapour and energy across the globe, making them a central component of the global circulation system. Changes in different forcing parameters have the potential to fundamentally change the monsoon characteristics as indicated in various paleoclimatic records and as projected by the latest generation of general circulation models in the context of the Coupled Model Intercomparison Project Phase 6 (CMIP6). Here, we use 32 CMIP6 models to analyze the model projections for the Indian summer monsoon with particular focus on the seasonal summer monsoon rainfall, its interannual variability and the occurrence of extremes. Besides, we use the Atmosphere Model version 2 developed at the Geophysical Fluid Dynamics Laboratory (GFDL-AM2) and couple it with a slab ocean to analyse the monsoon's sensitivity to changes in different forcing parameters on a planet with idealized topography. This Monsoon Planet concept of an Aquaplanet with a broad zonal land stripe allows to reduce the influence of topography and to access elementary meridional monsoon dynamics behind the competing effects of different forcings.


AS01-A013
Modelling the Effect of Aerosol and Greenhouse Gas Forcing on the Asian Monsoons with an Intermediate Complexity Climate Model

Lucy RECCHIA1#+, Valerio LUCARINI2
1University of Colorado Boulder, 2University of Reading

The Asian summer monsoons are globally significant meteorological features, creating a strongly seasonal pattern of precipitation. The stability of this hydrological cycle is of extreme importance for ecosystems and the livelihoods of a large share of the world’s population. Simulations are performed with an intermediate complexity climate model, PLASIM, to assess the future response of the Asian monsoons to changing concentrations of aerosols and greenhouse gases. The radiative forcing associated with aerosol loading consists of a mid-tropospheric warming and compensating surface cooling, which is applied to India, Southeast Asia and East China, both concurrently and independently. The primary effect of increased aerosol loading is a decrease in summer precipitation in the vicinity of the applied forcing, although the regional responses vary significantly. The decrease in precipitation is only partially ascribable to a decrease in the precipitable water, and instead derives from a reduction of the precipitation efficiency, due to changes in the stratification of the atmosphere. When the aerosol loading is added in all regions simultaneously, precipitation in East China is most strongly affected, with a quite distinct transition to a low precipitation regime as the radiative forcing increases beyond 60 W/m2. The response is less abrupt as we move westward, with precipitation in South India being least affected. By applying the aerosol loading to each region individually, we are able to explain the mechanism behind the lower sensitivity observed in India, and attribute it to aerosol forcing over East China. Additionally, we note that the effect on precipitation is approximately linear with the forcing. Doubling carbon dioxide levels acts to increase precipitation and weakening the circulation over the region. When the carbon dioxide and aerosol forcings are applied simultaneously, the carbon dioxide forcing partially offsets the surface cooling and reduction in precipitation associated with the aerosol response.


AS01-A066
Higher Sensitivity of Northern Hemisphere Monsoon to Anthropogenic Aerosol Than Greenhouse Gases

Jian CAO#+
Nanjing University of Information Science & Technology

Because increased greenhouse gas emissions considerably warm and moisten the Earth's atmosphere, one may expect an increase in monsoon precipitation during the historical period. However, we find the observed Northern Hemisphere land summer monsoon (NHLM) precipitation has significantly decreased since 1901. Simulations from Coupled Model Intercomparison Project Phase 6 (CMIP6) well reproduce global warming and the drying of NHLM since the industrial revolution when forced by observed external forcings. Result from single forcing experiment shows that the anthropogenic aerosol (AA) dominates the Northern Hemisphere (NH) monsoon precipitation drying, while the greenhouse gases (GHG) largely control surface warming. Thus, the NH monsoon precipitation responds to AA more sensitively than the GHG. The AA can more effectively modulate downward solar radiation reaching the surface, decreasing evaporation and weakening monsoon circulations by reducing the interhemispheric temperature difference and land-ocean thermal contrast, albeit with the same efficiency of the thermodynamic effect in the two forcings. Our result indicates the future intensive reduction of aerosol emission may rapidly recover the NH monsoon precipitation.


AS01-A023
Emission Sources of the Black Carbon Aerosols Over the Indian Ocean During the Monsoon Season

Krishnakant BUDHAVANT1,2#+, August ANDERSSON3, Henry HOLMSTRAND3, S.K. SATHEESH2, Orjan GUSTAFSSON3
1Maldives Meteorological Services, 2Indian Institute of Science, 3Stockholm University

The Indian Ocean summer aerosol regime is of greater relevance to the regionally-important monsoon system of South Asia. The effects of aerosols such as black carbon (BC) on climate and buildup of the monsoon over the Indian Ocean are poorly constrained. Uncertain contributions from various natural and anthropogenic sources impede our understanding. Here, we use multi-year (2012-2017) observations of BC and its isotope fingerprint at a remote island observatory in the northern Indian Ocean to constrain loadings and sources during the little-studied monsoon season. Carbon-14 data pin down a largely fossil (65±15%) BC source domain. Occasional plumes from African savanna fire contribute up to (50 ± 5%) of the loadings over the summertime Indian Ocean. We estimate that the mass-absorption cross-section for this region is 7.6 ± 2.5 (m2/g), with a tendency to increase with savanna fire input. Simultaneous measurement of air and rain allow us to calculate washout ratios of BC and other chemical species. The washout rates are much lower for BC than OC and inorganic ions such as sulfate, implying a longer atmospheric lifetime for BC. The wet deposition flux for BC during the high-loading winter was three times higher than during the wet summer, despite much less precipitation in the winter. Taken together, the combustion sources, longevity, and optical properties of BC aerosols over the summertime Indian Ocean are different from the more-studied winter aerosol, with implications for chemical transport and climate model simulations of the Indian monsoon.


AS01-A060
Modeling the Impacts of the Urban Land-use Effects on the Heavy Precipitation Events During the Indian Summer Monsoon

Renaud FALGA1#+, Chien WANG2
1Toulouse III - Paul Sabatier University, 2National Center for Scientific Research/ Université Toulouse III

The rise of the trends of extreme rainfall events across all the major regions of India since 1901 has been revealed in our recent study. This machine-learning driven data analysis also suggested several potential drivers including urbanization and other land-use changes behind the observed trends. However, their causal relations need to be carefully examined by using, e.g., advanced models. Specifically, it has been indicated that urbanization can modify the water cycle and precipitations, either through the modification of land-use, or through effects induced by the emissions of anthropogenic aerosols. The thermodynamical perturbations induced by the presence of urban land-use, including the urban heat island effect, are known to induce rainfall modification due to perturbation of the flow and enhancement of the convective activity. However, this impact has yet to be clarified in a large scale, highly energetic system like the Asian Monsoon system. Using the high resolution meso-scale atmospheric model Meso-NH coupled with an urban-module, we have investigated the impact of urban land use on the heavy precipitation events during the Indian Summer Monsoon. The results of this study will be presented and discussed.


AS01-A055
Strengthening Effect of Maritime Continent Deforestation on the Precipitation Decline Over Southern China During Late Winter and Early Spring

Shengbiao WEI1#+, Xin WANG2, Qiang XIE2
1South China Sea Institute of Oceanology, Chinese Academy of Sciences, 2Chinese Academy of Sciences

A high rate of deforestation has occurred in the Maritime Continent (MC) during recent decades due to the rapid growth of the local economy. MC deforestation is known to have a considerable influence on the local climate. However, its possible teleconnections to other regions are less understood. In this study, the influence of MC deforestation on precipitation over southern China is investigated using both reanalysis data and state-of-the-art climate models. The results show that MC deforestation could strengthen the late winter and early spring precipitation decline over southern China during 1979–2019. The enhanced regional convection due to MC deforestation leads to anomalous northward shifting of the tropical meridional circulation, with the ascending branch at 0°–10° N and descending at 20°–30° N compared with climatological ascending (10° S–0°) and descending (10°–20° N) branches. Such circulation change suppresses the moisture convergence and the development of convection over southern China. Our results suggest that, in addition to the local effects of deforestation, a further investigation of the remote impacts is essential for a thorough understanding of the climate influences of ongoing MC deforestation.


AS01-A050
Universal Definition of Local Monsoon Onset

Elena SUROVYATKINA1,2#+
1Potsdam Institute for Climate Impact Research, 2The Space Research Institute of the Russian Academy of Sciences

The classical understanding of monsoon onset implies a sudden increase in precipitation and sustainable rains. However, initial rain often gets stalled after monsoon onset for a week or even longer, causing disaster for farming. Here, I show that there are two types of critical transitions to monsoon: a direct transition, with a sudden increase in precipitation, and a two/multiple-step transition, with a dry spell after the initial rain. I present evidence that 70% of the last 47 years show a two/multiple-step transition, which went overlooked. Significantly, the second type of transition prevails under climate change. I uncover that the cause of rainfall cessation is the hidden phenomenon of intermittence emerging between two successive phase transitions. The new theoretical finding opens a door for the universal definition of local monsoon onset. I show how to evaluate the effect of climate change on the transition to monsoon in every state of the Indian subcontinent. 


Tue-01 Aug | 1:00 - 5:15 | Summit
AS - Atmospheric Sciences Poster Session 1

AS03-A002
Cloud Water Resource in North China in 2017 Simulated by the CMA-CPEFS Cloud Resolving Model: Validation and Quantification

Chao TAN1,2+, Yuquan ZHOU3#
1The University of Hong Kong, Hong Kong SAR, 2The University of Hong Kong, Hong Kong SAR, 3China Meteorological Administration Weather Modification Center, China

Based on the concept of cloud water resource (CWR) and the cloud microphysical scheme developed by the Chinese Academy of Meteorological Sciences (CAMS), a coupled mesoscale and cloud-resolving model system is developed in the study for CWR numerical quantification (CWR-NQ) in North China for 2017. The results show that (1) the model system is stable and capable for performing 1-yr continuous simulation with a water budget error of less than 0.2%, which indicates a good water balance. (2) Compared with the observational data, it is confirmed that the simulating capability of the CWR-NQ approach is decent for the spatial distribution of yearly cumulative precipitation, daily precipitation intensity, yearly average spatial distribution of water vapor. (3) Compared with the CWR diagnostic quantification (CWR-DQ), the results from the CWR-NQ differ mainly in cloud condensation and cloud evaporation. However, the deviation of the net condensation (condensation minus evaporation) between the two methods is less than 1%. For other composition variables, such as water vapor advection, surface evaporation, precipitation, cloud condensation, and total atmospheric water substances, the relative differences between the CWR-NQ and the CWR-DQ are less than 5%. (4) The spatiotemporal features of the CWR in North China are also studied. The positive correlation between water vapor convergence and precipitation on monthly and seasonal scales, and the lag of precipitation relative to water vapor convergence on hourly and daily scales are analyzed in detail, indicating the significance of the state term on hourly and daily scales. The effects of different spatial scales on the state term, ad- vection term, source–sink term, and total amount are analyzed. It is shown that the advective term varies greatly at different spatiotemporal scales, which leads to differences at different spatiotemporal scales in CWR and related characteristic quantities.


AS03-A005
Aerosol Susceptibilities on the Wintertime Stratocumulus Clouds Over the Northwest Pacific Ocean

Chung-Kai WU+, Jen-Ping CHEN#
National Taiwan University, Taiwan

Aerosol indirect effects, including the Twomey and Albrecht effects, remain a major uncertainty in current weather and climate studies. Such effects are found to vary with cloud types, and the vulnerability is often evaluated with a metric called susceptibility -- the derivatives of the measured variable to aerosol concentration. In this research, the Weather Research and Forecasting model v4.3.1 combined with the NTU microphysical scheme is used to investigate the aerosol susceptibility of marine boundary-layer clouds over the NW Pacific Ocean during cold-air outbreak events. These clouds are often found in mixed-phase upstream and liquid-phase downstream of the cold air trajectory. We found distinctive features of aerosol susceptibility in both cloud types. In the liquid-phase stratocumulus clouds, most cloud properties (e.g., liquid water path, optical depth, and cloud albedo) have positive susceptibilities to the aerosol effects, consistent with earlier studies. However, the cloud fraction showed a negative susceptibility when drizzle is active. In the mixed-phase stratocumulus clouds, on the other hand, the cloud and ice water paths, as well as cloud fraction, are found to increase in the low-end and high-end aerosol concentrations but decrease when the aerosol concentration is between 102 and 104 cm-3. Such a nonlinearity is likely associated with the transition of precipitation formation from drizzle-dominated in low aerosol concentrations to ice-dominated at high aerosol concentrations.


AS03-A006
Role of Cloud Subgrid-scale Structure in Modulating Clouds Viewed by ISCCP, MODIS, and MISR Simulators

Xiaocong WANG#+
Chinese Academy of Sciences, China

The role of cloud subgrid-scale structure in modulating satellite views of clouds was investigated. This was realized by implementing a stochastic cloud generator into the CFMIP (Cloud Feedback Model Intercomparison Project) Observation Simulator Package together with surrogate clouds produced by a cloud- resolving model (CRM). The subgrid-scale structural parameters are decorrelation length for overlapping cloud fraction (Lcf), decorrelation length for overlapping cloud condensate (Lcw), and the shape parameter v for measuring cloud inhomogeneity. With the use of median values of Lcf, Lcw, and v derived from CRM, the simulated satellite views bear close resemblance to those using CRM-inherent clouds. Varying these parameters in the range of lower and upper quartiles leads to differences that are about one-fifth of those caused by changing cloud microphysics in CRM. While Lcf influences clouds throughout the whole troposphere, Lcw and
v result in changes mostly within the upper layers. Increasing (decreasing) cloud inhomogeneity or overlapping degree leads to decreased (increased) occurrence of clouds, except for high-topped clouds viewed by Multiangle Imaging Spectroradiometer. Care must then be exercised when interpreting model biases in comparison with different instruments. Sensitivity tests show changing condensate distribution from gamma to lognormal makes little impact on final results. Although the differences induced by any of the parameters alone are much limited, they are getting comparable to those seen between models and observations when all parameters are synergistically altered. This brings encouraging results to the modeling community that simulator-diagnosed clouds can be potentially improved by tuning cloud subgrid-scale parameters.


AS03-A012
A Critical Evaluation of Top-hat Approximation in Shallow Convection 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 in the mass flux type convection, is verified at different horizontal scales, especially those at the limit of vanishing cloud fraction, with the aid of large eddy model simulations (LES). Three shallow convection cases in the Global Energy and Water Cycle Experiment (GEWEX) Cloud System Study (GCSS) programs are conducted, including BOMEX, RICO and ATEX. Results show that convective cloud fraction increases with the increase of horizontal resolution, consequently resulting in errors of cloud component in the decomposition of scalar flux increase. These errors are however largely compensated by the decrease of errors in the environment, leading to the error of top-hat approximation almost unchanged. For either cloud or environment component, there exists an inversed relationship between convective fraction and the covariance between vertical velocity and conserved tracer. This brings encouraging results to the modeling community that the mass-flux method in parameterizing convection still works at high resolutions. However, the closure remains a big problem at the limit of vanishing cloud fraction, which is not covered in this study.


AS03-A014
Comparison of ERA-5, JRA-55 and MERRA-2 on Diurnal Cycle of Precipitation and Associated Physical Processes

Yanjie LIU1#+, Xiaocong WANG2, Yimin LIU2
1University of Chinese Academy of Sciences, China, 2Chinese Academy of Sciences, China

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). In this study, the behaviors of the phase and amplitude of DCP in China in three commonly used reanalysis products, including ERA-5, JRA-55 and MERRA-2, are compared against GPM (Global Precipitation Measurement) and CMORPH (Climate Prediction Center Morphing Technique). Results show while JRA-55 and ERA-5 produce DCP that are closely consistent with observation, MERRA-2 shows 1- to 3-hour shifts in phase and significantly underestimates the amplitude. Further analysis is performed by comparing 3-D cloud fraction, apparent heating (Q1) and apparent moisture sink (Q2) against cloud-resolving model (CRM) simulations. Only ERA-5 captures the evolution of clouds in association with convective precipitation as in CRM simulations, while the other two fail to reproduce such characteristics. This implies the need to link DCP with subgrid-scale processes besides convection and to treat physical parameterizations as an integrated system.


AS03-A015
Effect of the Low-level Jets on the Movement of the Mei-yu Front

Mu-Qun HUANG#+, Pay-Liam LIN
National Central University, Taiwan

The Mei-Yu front heavy rainfall event occurred in northern Taiwan on 2 June 2017. The largest daily accumulated rainfall was 645.5 mm at the north tip of Taiwan. The frontal system becomes quasi-stationary in northern Taiwan, and it lasts for 10 hours. A strong barrier jet over the northwest coast of Taiwan is present when the Mei-Yu front approaches northern Taiwan. The strong low-level jet brings abundant moisture to Taiwan and causes strong convergence along the frontal zone. The strong convection produces more than 600 mm of rainfall when the system becomes stationary. In order to examine how the barrier jet over northwestern Taiwan affects the movement of the Mei-Yu front, this study uses the WRF model to reproduce this heavy rain event. Meanwhile, three sensitivity tests are conducted in the numerical experiment. In the removing Taiwan terrain test, the front moves southward quickly. The accumulated rainfall was only 200 mm and the barrier jet is much weaker than the CTRL, showing that the orographic can obstruct the frontal movement. In the replacing southern Taiwan mountain test, northern Taiwan terrain provides part of the blocking effect, but the front still moves southward quickly without a strong barrier jet. In the enhanced barrier jet test with the same topography as CTRL, the barrier jet is slightly stronger than CTRL. The position of the stationary Mei-Yu front is further north than the CTRL. The strong southerly wind also enhanced the convergence, resulting in more rainfall, however, the rainfall did not fall over the land. The results show that the orographic effect contributed to part of the blocking effect for the frontal movement in northern Taiwan, and caused the barrier jet to form in northwestern Taiwan. The slow movement of the Mei-Yu front is significantly influenced by the barrier jet.


AS05-A009
Synoptic Control and Surface Condition of Hail Events Over the Beijing Metropolitan Region During the Warm Seasons of 2011–2021

Mingxin LI#+
Chinese Academy of Meteorological Sciences, China

The fine spatial characteristics of hail events over Beijing metropolitan region (BMR) is performed using direct observation from quality-controlled disaster information dataset during the year of 2011-2021. Hail is concentrated in urban and northeast mountain region which is highly related with both synoptic circulations and the underlying surface. Four synoptic circulation patterns: the northwest flow in front of ridge (NWP), straight westerly flow (SWP), cold vortex (CV), and pre-trough (PT) are investigated and the hail generation is found differs under these patterns. SWP favors local hail events with the largest convective available potential energy and PT favors systematic hail events with the highest vertical wind shear. With weak low level background flows under NWP and CV, hail events concentrate over the BMR’s plains with obvious surface warm center and wind convergence near urban region which favor storm initiation and enhancement. When the low-level background flow is larger in SWP and PT, the more dominated mountain-plain circulations lead to the hail events center changing to the BMR’s northeast mountains rather than the urban region. These results suggest the potential influences of urban environment and mountain-plain circulations on the distribution of hail events under different synoptic circulation patterns.


AS07-A005
Objective Climate Predictions of Summer Temperatures in South Korea Based on CNN and GNN

Jinyoung RHEE#+, Uran CHUNG, Kyoungwon PARK, Soo-Jin SOHN
APEC Climate Center, Korea, South

We explored the use of modern deep learning models of Convolutional Neural Networks (CNN) and Graph Neural Networks (GNN) for objective climate predictions of summertime air temperatures in South Korea. In order to design deep learning models more appropriate for climate predictions, the CUTMIX data augmentation technique was modified and applied to climate observations and APCC Multi-Model Ensemble (MME) data. The 3-dimensional CNN model performed much better with data augmentation for validation (accuracy > 0.6 for all summer months and folds) as well as test data for June (LT1) and July (LT2). Class activation maps were examined and the contributions of the data augmentation could be observed in some cases of the test data, e.g., in July 2018 and July 2021, when the northern Pacific are and northern polar region are activated and improved the predictions respectively. Graph Convolution Network models were developed for node classification (years as nodes) and graph classification (geographical grids as nodes and years as multiple graphs). Predictions for July (LT2) of the node classification model were improved with the month-agnostic approach, where all months of data are used for training. Predictions for June (LT1) of the graph classification model were improved with the month-agnostic approach (Heidke Skill Score > 0.35 for all folds) and predictions for July (LT2) were also improved with the aforementioned data augmentation. ※ This research was supported by APEC Climate Center.


AS07-A010
A Wind-dependent Parameterization for Ocean Sea Surface Albedo in FIO-ESM V2.0 Simulations

Xueyi JING1#+, Lanning WANG2, Zhenya SONG3
1College of Global Change and Earth System Science, Beijing Normal University, China, 2Beijing Normal University, China, 3Ministry of Natural Resources, China

Ocean surface albedo (OSA) is essential to the ocean and climate energy balance. It is usually considered as the constant or just a simple function of the solar zenith angle (SZA) in the climate model. However recent research suggests that the OSA can be significantly affected by low-level wind, and play an important role in climate simulation, especially in high-resolution simulation. In this work, we incorporated an improved OSA parameterization scheme into the First Institute of Oceanography-Earth System Model (FIO-ESM) V2.0. The revised parameterization scheme takes into account the sea surface roughness and whitecaps induced by surface wind and simplified water volume scattering. Numerical experiments indicate that the improved scheme leads to an increase in OSA of roughly 40% at the global scale. It is remarkable that the effects of foams or whitecaps are noticeable in areas with strong winds, such as the Southern Hemisphere westerly zone. The model bias in sea surface net shortwave radiation has been reduced by an average of 3 W/m2, and over the subtropical and Antarctic oceans by up to 8 W/m2 and 14 W/m2. The enhanced OSA parameterization also reduces the global annual mean error of sea surface temperature by up to 0.87°C.


AS07-A012
Optimization of Air Mass Factor Calculation for GOSAT-GW Satellite NO2 Observation

Ayano NAKAMURA1#+, Tomohiro SATO1, Tamaki FUJINAWA2, Yasuko KASAI3
1National Institute of Information and Communications Technology, Japan, 2National Institute for Environmental Studies, Japan, 3Tokyo Instutute of Technology, Japan

The Global Observing Satellite for Greenhouse gases and Water cycle(GOSAT-GW) satellite is planned to be launched in 2024 as the successor to the GOSAT-1 and GOSAT-2 greenhouse gas observation missions. The GOSAT-GW satellite challenges to simultaneously observe greenhouse gases and nitrogen dioxides (NO2), major air pollutants. The grating spectrometer is equipped, and more than three million points are observed per day.
The air mass factor (AMF) is used to convert from the NO2 slant column density to the vertical column density, and is one of the largest error sources in retrieving NO2 vertical column from the observation spectrum. High speed calculation of AMF is required because of large number of observation points of GOSAT-GW. The AMF values for all observation cases are pre-calculated by radiative transfer model and saved in the look-up table (LUT).
This study discusses the optimization of LUT, i.e, how to select the nodes of input variables in LUT. We used SCIATRAN version 4.6.1 for radiative transfer calculation. The node of each input variable, such as solar zenith angle, viewing zenith angle, albedo, and terrain height, are selected by AMF gradients for the variables. Our algorithm showed 45% lower error than conventionally-made LUT. In this presentation, we show the results of all LUTs used in the NO2 retrieval data processing of the GOSAT-GW.


AS07-A013
Predicting Ambient NH3 Concentrations Based on the Extra Trees with Time Lag and Parcel Tracking Functions

Chin Yu HSU#+
Ming Chi University of Technology, Taiwan

Ambient NH3 plays an important role in forming particulate matter (PMs), and therefore, it is crucial to comprehend NH3's properties in order to reduce PMs. However, it is not easy to achieve this goal due to the lack of monitoring data on ambient NH3 concentrations in typical air quality stations. Nor are we aware of any study that has looked into NH3 predictions as of yet. This study thus offers the first inquiry into applying machine learning and an auto hyperparameter optimization approach to estimate NH3 concentrations. To obtain more crucial data about NH3 concentration, we additionally created time lag and parcel tracking routines. To analyze feature importance, we applied the SHAP (SHapley Additive exPlanations) function. From 2016 to 2018, Taichung's hourly average NH3 values were about 16.9 ppb. Such NH3 concentrations were predicted using an optimized extra trees model that has the potential to account for up to 96% of the total variance. Agriculture activity was the most significant factor (main source) to affect NH3 concentrations in Taichung among all the characteristics.


AS07-A016
Role of the Spring Southeastern Indian Ocean Warming in Bridging the Indian Ocean Dipole and Subsequent ENSO

Yue ZHONG+, Wenshi LIN, Tuantuan ZHANG#, Shuyan WU
Sun Yat-sen University, China

A significant relationship between the Indian Ocean Dipole (IOD) and the following year’ s El Niño-Southern Oscillation (ENSO) has been reported in recent decades. Nevertheless, uncertainty exists regarding the associated mechanisms. Based on the statistical analysis and numerical experiments, our study proposes that the spring southeastern Indian Ocean warming (SEIOW) plays a bridging role in the teleconnections of the IOD and subsequent ENSO. A positive IOD could induce a positive tendency of sea surface temperature (SST) in the southeastern Indian Ocean from autumn to winter, primarily through the cloud-radiation-SST feedback, forming an anomalous SEIOW in the subsequent spring. As a Gill-model response to this SEIOW, an anomalous anticyclone appears over the western North Pacific, accompanied by easterly wind anomalies in the western equatorial Pacific which generate eastward propagating upwelling Kelvin waves. As a result, anomalous cooling appears over central-eastern tropical Pacific in the following seasons, manifesting as a La Niña mode. The process is vice versa for the teleconnections of the negative IOD and following year’s El Niño. Additionally, role of the ocean channel (i.e., the Indonesian Throughflow) in connecting the spring southeastern Indian Ocean and the subsequent winter eastern Pacific SSTs is also discussed.


AS07-A020
Major Factors Governing the Trends and Interannual Variability in the Occurrences of Mixed Rossby-Gravity Wave Events

Mehak N.A.#+, Shreya KESHRI, Suhas ETTAMMAL
Indian Institute of Science Education and Research Pune, India

Mixed Rossby-Gravity (MRG) waves are westward propagating synoptic scale equatorial disturbances, which play a crucial role in the formation of tropical cyclones and tropical depressions. They constitute a significant part of various modes of tropical variability, like Madden-Julian Oscillation (MJO) and Quasi-Biennial Oscillation. This study investigates the trends and Inter Annual Variability (IAV) in the occurrence of upper tropospheric MRG events using ERA-I reanalysis data for the period 1979-2018. The MRG events are identified by projecting the 200hpa meridional winds onto the theoretical spatial structure of MRG waves. A steady increasing trend is observed in the MRG events, which is contributed by the MRG events associated with intrusion of extratropical disturbances. Possible factors governing the observed trend and IAV in MRG events are El-Nino Southern Oscillation (ENSO), MJO and extratropical forcing. The MRG events over the central and eastern Pacific contribute maximum to IAV. ENSO explains about 25% of IAV and exhibits a positive correlation with non-intrusion MRG events and a negative correlation with intrusion MRG events. These observations have been investigated by exploring the properties of the westerly duct at 200hPa and Outgoing Longwave Radiation during El-Nino and La-Nina years over the central-eastern Pacific. The convectively active state of MJO over the western Pacific explains 20% of IAV. The antisymmetric heating with respect to the equator, associated with MJO, enhances non-intrusion MRG events by forbidding the intrusion of extratropical disturbances through subtropical easterlies. The increasing trend in the intrusion of extratropical disturbances explains the observed trend in MRG events.


AS07-A025
Diagnosis of Data Assimilation Effect on East Asian Forecast of the Global NWP Model Through OSSE

Hyerim KIM+, Kyung-Hee SEOL#, In-Hyuk KWON, Hui-Nae KWON, Hyun-Jun HAN
Korea Institute of Atmospheric Prediction Systems, Korea, South

The global atmosphere NWP system – named the Korean Integrated Model (KIM) – developed by the Korea Institute of Atmospheric Prediction Systems (KIAPS) was made operational at the Korea Meteorological Administration (KMA) in April 2020. The global data assimilation (DA) system is based on a hybrid-4DEnVar system consisting of KVAR (KIM VARiational data assimilation) and LETKF (Local Ensemble Transform Kalman Filter). Although it provides a good forecast skill within the performance range of the world’s leading NWP centers, the prediction has some systematic bias over East Asia. Forecast skill of the forecast system including DA system is sensitive to initial data and assimilated observation data. Thus, improving the model itself is important, but the performance of observation data used for DA is also important in order to improve forecast skill. An Observing System Simulation Experiment (OSSE) has been conducted to understand the model prediction sensitivity according to DA. If we consider a global gridded virtual Sonde observation network and assume that the ERA5 analysis is true of the OSSE system, simulated observations with globally 1-degree intervals can be generated from ERA5. In this study, the difference between forecasts fields assimilated with the existing observation data and the virtual Sonde data is examined for cases chosen when KIM’s East Asia forecast skills are significantly low. Through these experiments and analysis, we would like to examine the following two. First, this system will be used to investigate the effect of the initial condition and the virtual Sonde data as the observation data on the 5-day prediction accuracy of the East Asia. Second, we plan to conduct sensitivity experiments for diagnosing regions where affect the improvement of East Asia’s forecast performance to improve 5-day forecast skill.


AS07-A027
Development of Global Observing System Simulation Experiment (OSSE) System Using Korean Integrated Model (KIM) : Description and Preliminary Result

Hyun-Jun HAN#+, Jeon-Ho KANG, In-Hyuk KWON
Korea Institute of Atmospheric Prediction Systems, Korea, South

Observing system simulation experiment (OSSE) provide a rigorous, cost-effective approach to evaluating the potential impact of new observing systems and alternate deployments of existing systems and to optimizing observing strategies (Hoffman and Atlas, 2016). One of most advantageous thing in OSSE is that researcher can verify the result of Numerical Weather Prediction (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, appling 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 (OSSE is generally consist of the NR, simulated observation, DA and forecast, and calibration and verification), KIM forecast system, and what i done to develop the OSSE system used KIM, briefly. Finally, to verify the OSSE system used KIM, we performed the denial experiments for aircraft, not only in OSSE but also performed in OSE. In comparison result between OSE and OSSE aircraft denial experiments, OSE/OSSE showed similar performance in most atmospheric variables of analysis field. So, we evaluated the OSSE system used KIM is well made enough to simulate the real case.


AS07-A034
Estimation of Planetary Boundary Layer Height Based on Radiosonde Data

Junsik KIM+, Junshik UM#
Pusan National University, Korea, South

The planetary boundary layer (PBL) is the lowest part of the atmosphere and interacts directly with the Earth's surface, playing an important role in weather, climate, and air quality. It also plays an important role in the exchange of aerosols, heat, humidity, and other atmospheric gases. Therefore, it is vital to understand the spatial and temporal variations of the PBL height (PBLH). Radiosonde launching has been used to determine the vertical profile of the PBL. The Korea Meteorological Administration(KMA) has been launching radiosondes twice a day (00 and 12 UTC or 9 and 21 LST) at ten different stations in Korea. In this study, the PBLH was calculated using the bulk-Richardson method with the KMA radiosonde data. The bulk Richardson method calculated the PBLH using the ratio of thermally generated turbulence generated by the vertical shear. The used variables were virtual potential temperature, wind speed, gravity, altitude, and humidity. When the bulk Richardson method reached the threshold, two types of thresholds, 0.25 and 0.5, were commonly used. In this study, 0.25 was used as the threshold. The altitude when the threshold of the bulk Richardson method calculated from the ground exceeded 0.25 was determined as the PBLH. The calculated PBLH was also compared with those determined based on the ceilometer measurements.


AS07-A035
A 4DIAU Scheme for the KIM Data Assimilation System

Wonho KIM#+, Adam CLAYTON, In-Hyuk KWON
Korea Institute of Atmospheric Prediction Systems, Korea, South

Currently, the operational Korean Integrated Model (KIM) Numerical Weather Prediction system at the Korea Meteorological Administration (KMA) uses 3DIAU to add deterministic analysis increments to the model. The weights are based on a Dolph filter, but with the first and last weights modified to remove discontinuities, producing a “modified Dolph filter”. Hybrid-4DEnVar scheme used for deterministic analyses produces a total of 7 analysis increments – one every hour within data assimilation window. Thus, it is possible to replace the 3DIAU scheme with a 4DIAU scheme that makes use of the hourly analysis increments. We have experimented with a 4DIAU scheme that adds each analysis increment over a 2-hour period, again using modified Dolph weights. For increments that are, the response is determined by the weighting function used for the individual increments, giving relatively light time-filtering. For increments that are not, such as the stationary increments related to the static covariance, the response is determined by the sum of the weights across all increments, giving relatively heavy time-filtering similar to that obtained with the 3DIAU scheme. Thus, for balanced increments that are consistent in time, such as increments associated with rapidly-moving features like tropical cyclones, 4DIAU should be better than 3DIAU at retaining the increments. We compared analysis and forecast performance of the new 4DIAU scheme with the original 3DIAU scheme. In analyses, there was relatively little impact on T and Q, but U and V were improved. In the Northern Hemisphere, overall forecast performance was improved, and the performance improvement of geopotential height was significant. The performance improvement in the Northern Hemisphere is particularly noticeable in Asia. In a tropical cyclone case experiment, the 4DIAU scheme gave a slightly deeper central pressure than the 3DIAU scheme, and expressed the change in tropical cyclone position over time better than 3DIAU.


AS07-A036
Introduction of Research Performance During 2017-2021 in NIMS/KMA

Youngmi KIM#+, Jinyoung KO, Heon Woo KIM, Ha-Kwom LIM
National Institute of Meteorological Research/Korea Meterological Research, Korea, South

NIMS works for meteorological science research and policy support for people’s safety and happiness and has been doing lots of research under the research project, called the “Research and Development for KMA Weather, Climate, and Earth System Services”.
NIMS has developed technologies needed to improve forecasting for KMA such as a medium-term forecast guideline and marine weather forecasting system. Initialization and ensembles of climate prediction system were improved for more accurate and reliable climate predictions. Due to climate change, damages caused by heavy rains in summer have increased and rainfall forecasting has become difficult. So, NIMS has developed diagnostic factors for heavy rainfall through synoptic analysis of severe weather.
There was challenged study using advanced observation equipment meteorological observation vehicles, meteorological aircraft, and meteorological drones. For understanding and analyzing of a meteorological phenomenon, NIMS observed heavy rainfall, black ice, and so on. These data are used to understand the mechanisms of severe weather. Black ice prediction based on these data has been developed to decrease winter traffic accidents. The technologies of weather modification are constantly evolving using advanced equipment. Also, Korea Cloud Physics Experimental Chamber (K-CPEC) was conducted in 2021. We expect to develop better technology and understand cloud physics.
To support national climate change response policy, NIMS produced new future projections based on New Green House Gases (GHG) and published climate change reports. Also, NIMS continuously monitors GHG. For expanding renewable energy, NIMS provides high-resolution meteorological resource maps.
In addition, NIMS has been producing convergence weather information such as airport weather prediction, health weather, and agricultural weather. More detailed results will be shown at the conference.


AS07-A037
Hydrothermal Factors Influence on Spatial-temporal Variation of Evapotranspiration-precipitation Coupling Over Climate Transition Zone of North China

Ze Su YANG#+
Chengdu University of Information Technology, China

As a land-atmosphere coupling “hot spot”, the northern China climate transition zone has a sharp spatial gradient of hydrothermal conditions, which plays an essential role in shaping the spatial and temporal pattern of evapotranspiration-precipitation coupling, but whose mechanisms still remain unclear. This study analyzes the spatial and temporal variation of land-atmosphere coupling strength (CS) in the climate transitional zone of northern China and its relationship with soil moisture and air temperature. Results show that CS gradually transitions from strong positive in the northwest to negative in the southeast and northeast corners. The spatial distribution of CS is closely related to climatic hydrothermal conditions, where soil moisture plays a more dominant role: CS increases first, and then decreases with increasing soil moisture, with the threshold of soil moisture at 0.2; CS gradually transitions from positive to negative at soil moisture between 0.25 and 0.35; CS shows an exponential decreasing trend with increasing temperature. In terms of temporal variation, CS is strongest in spring and weakens sequentially in summer, autumn, and winter, and has significant interdecadal fluctuations. The trend of CS shifts gradually from significantly negative in the west to a non-significant positive in the east. Soil moisture variability dominates the intra-annual variability of CS in the study regions, and determines the interannual variation of CS in arid and semi-arid areas. Moreover, the main reason for the positive and negative spatial differences in CS in the study area is the different driving regime of evapotranspiration (ET). ET is energy-limited in the southern part of the study area, leading to a positive correlation between ET and lifting condensation level (LCL), while in most of the northern part, ET is water-limited and is negatively correlated with LCL.


AS07-A039
Evaluation of High-resolution Crop Model Meteorological Forcing Datasets at Regional Scale: Air Temperature and Precipitation Over Major Land Areas of China

Qiuling WANG1+, Wei LI2#, Chan XIAO2, Wanxiu AI2
1National Climate Center, China Meteorological Administration, China, 2China Meteorological Administration, China

Air temperature and precipitation are two important meteorological factors affecting the earth’s energy exchange and hydrological process. High quality temperature and precipitation forcing datasets are of great significance to agro-meteorology and disaster monitoring. In this study, the accuracy of air temperature and precipitation of the fifth generation of atmospheric reanalysis produced by the European Centre for Medium-Range Weather Forecasts (ERA5) and High-Resolution China Meteorological Administration Land Data Assimilation System (HRCLDAS) datasets are compared and evaluated from multiple spatial–temporal perspectives based on the ground meteorological station observations over major land areas of China in 2018. Concurrently, the applicability to the monitoring of high temperatures and rainstorms is also distinguished. The results show that (1) although both forcing datasets can capture the broad features of spatial distribution and seasonal variation in air temperature and precipitation, HRCLDAS shows more detailed features, especially in areas with complex underlying surfaces; (2) compared with the ground observations, it can be found that the air temperature and precipitation of HRCLDAS perform better than ERA5. The root-mean-square error (RMSE) of mean air temperature are 1.3 ◦C for HRCLDAS and 2.3 ◦C for ERA5, and the RMSE of precipitation are 2.4 mm for HRCLDAS and 5.4 mm for ERA5; (3) in the monitoring of important weather processes, the two forcing datasets can well reproduce the high temperature, rainstorm and heavy rainstorm events from June to August in 2018. HRCLDAS is more accurate in the area and magnitude of high temperature and rainstorm due to its high spatial and temporal resolution. The evaluation results can help researchers to understand the superiority and drawbacks of these two forcing datasets and select datasets reasonably in the study of climate change, agro-meteorological modeling, extreme weather research, hydrological processes and sustainable development.


AS07-A040
The Effect on the Wind of Coastal Urban Buildings Using LES Model

Jiseon KIM1#+, Soon-Hwan LEE1, Soon-Young PARK2, JungWoo YOO1
1Pusan National University, Korea, South, 2Daegu National University of Education, Korea, South

Due to concentrated buildings, low vegetation, and road paving materials, cities are likely vulnerable to weather environments such as heat waves and floods. In addition, in complex urban structures, it is difficult to predict wind changes caused by high-rise buildings, making it challenging to analyze the thermal environment and pedestrians' thermal comfort in the city.
This study attempts to simulate and analyze wind changes in complex urban environments using a PALM(Parallelized Large-Eddy Simulation Model). Haeundae Marine City in Busan, Korea, located on the coast, was selected as the study target area. This area is where concentrated high-rise residential and commercial buildings are and where light reflection by the outer walls of the building glass and damage by strong winds occur.
Simulate the actual urban structure of Marine City with a large-eddy simulation (LES)-based PALM model to identify changes in surrounding winds due to the height difference of the high-rise buildings inside the city and compare environmental changes such as pedestrian thermal comfort.


AS07-A042
Predictability of the Western Pacific Pattern in the APCC Multi-model Ensemble

Joong-Bae AHN1#+, Eung-Sup KIM2, Vladimir KRYJOV3
1Pusan National University, Korea, South, 2National Institute of Agricultural Sciences, Korea, South, 3Hydrometcenter of Russia, Russian Federation

In this study, the predictability of the Western Pacific (WP) pattern is evaluated using five seasonal prediction models the Asia-Pacific Economic Cooperation (APEC) Climate Center (APCC) multi-model ensemble (MME) for the winters from 1982/1983 to 2021/2022. The temporal correlation coefficient (TCC) between the observed and MME-predicted WP indices was 0.61 (0.37–0.54 for individual models) for the entire series. However, when only three Super El Niño (SEN) years (Niño3.4 ≥ 2.0) out of the 40-year series were excluded, the TCC dropped down to 0.54 (0.27–0.42). During the SEN years, the WP was strongly affected by the SEN-excited anomalies via the PNA. In observations from non-SEN years, the WP pattern was strongly related to the dipole pattern in Northwestern Pacific SST (TCC = 0.8), for the description of which we suggested a Northwestern Pacific (NWP) index, and it was significantly weakly related to the ENSO and IOD, whereas in the model simulations, the main role was played by the ENSO (TCC = 0.6). The NWP index was well predictable in MME (TCC = 0.73) and individual models (0.56–0.71). We showed that the prediction of the WP index polarity is reliable when both predicted WP and NWP anomalies are significant and indicate the same WP sign that has implications for the seasonal forecasting. Acknowledgment: This work was carried out with the support of the Research Fund of Research Institute for Basic Sciences, Pusan National University, Korea.


AS07-A045
A Survey of Mixed Rossby-gravity Waves and Quantification of Their Association with Extratropical Disturbances

Shreya KESHRI#+, Suhas ETTAMMAL
Indian Institute of Science Education and Research Pune, India

In this study we have conducted a survey of Mixed Rossby-Gravity (MRG) wave events in the upper troposphere and quantified their association with the intrusions of extratropical disturbances for the period 1979-2019. MRG events are identified by projecting the equatorial meridional winds at 200 hPa onto the meridional structure of theoretical MRG waves. 2390 MRG events are identified and majority (61%) of them occurred during May-October months, and 65% of the total MRG events occurred over the central-east Pacific and Atlantic Ocean domains. Not only the frequency of occurrence but also the amplitude, wavenumber and trapping scale of the MRG events are found to exhibit a clear seasonality. MRG events associated with intrusions of extratropical disturbances are identified as when the potential vorticity on the 350K isentropic surface at 15° latitude exceeded 1 PVU in the vicinity of the MRG events. We find that 37% of the MRG events are intrusion MRG events and a large majority (88%) of such events occurred over the central-east Pacific and Atlantic Ocean domains. It is also noteworthy that nearly 70% of such intrusions occurred in the winter Hemisphere where the westerly wind ducts are well developed. Over the central-east Pacific during Northern Hemispheric (NH) winter, it is observed that the amplitude of intrusion MRG events are larger and have a larger meridional extent compared to non-intrusion MRG events. They also exhibit a similar spatial scale as the extratropical disturbances implying that resonant interactions may be a primary mechanism for the genesis of MRG events. During NH summer, on the other hand, MRG events are primarily triggered by convective processes and the extratropical disturbances may be instrumental in amplifying their amplitude.


AS07-A053
Impact of Changes in Ice Microphysical Processes on Predictability of the Korean Integrated Model

Jeong-Ock LIM#+, Jeong-Hyun PARK, Hyun-Joo CHOI, Seonghoon CHEONG
Numerical Modeling Center/Korea Meteorological Administration, Korea, South

Korean Integrated Model (KIM), developed by Korea Institute of Atmospheric Prediction System (KIAPS), has been in operation at Korea Meteorological Administration (KMA) since April 2020. It has been continuously improved its performance through five updates (v3.5a (2020.06), v3.6a (2021.4), and v3.7 (2021.12), v3.8 (2023.2)) including data assimilation and physics.
One of the major systematic errors of the KIM is the cold biases in the lower Arctic atmosphere in summer, which degrades KIM’s prediction performance in the northern hemisphere. The radiative cooling effect by clouds, especially, over-estimated cloud ice, is analyzed as one of the main factors.
In this study, we will examine the possibility of improving the above-mentioned systematic errors through sensitivity test to changes in parameters related to ice crystals of WSM5, cloud microphysics scheme adopted by KIM.


AS08-A005
Size Distribution of Atmospheric Aerosols Considerably Impacts Radiative Effects Over the Himalayas by Modulating Aerosol Single-scattering Albedo

Zeren YU#+, Pengfei TIAN, Lei ZHANG, Jiening LIANG
Lanzhou University, China

The single-scattering albedo (SSA) of atmospheric aerosols is a key parameter that controls aerosol radiative effects. The variation of SSA is thought to be mainly regulated by aerosol absorption in the Himalayas and South Asia, but observations contradict this idea. In situ field campaigns conducted over two Himalayan sites revealed that SSA was strongly dependent on scattering but weakly correlated with absorption. Observational results combined with the Mie theory further illustrated that SSA was primarily modulated by size distribution rather than absorption. Aerosol Robotic Network (AERONET) data showed similar impacts of size distribution on SSA and that aerosol radiative forcing efficiencies were significantly dependent on SSA. Aerosol size distribution therefore considerably affects radiative forcing by modulating aerosol SSA over the Himalayas. This study highlighted the influence of aerosol size distribution on radiative forcing over the Himalayas, which has important implications for understanding aerosol radiative effects globally.


AS08-A006
Polarized Adding Method of Discrete Ordinate Approximation for Visible and Near-infrared Radiative Transfer

Kun WU1#+, Feng ZHANG2, Wenwen LI2
1Nanjing University of Information Science & Technology, China, 2Fudan University, China

Polarization characteristics of the atmospheric scattering is important and not to be ignored in radiative transfer simulation. A new polarized radiative transfer method is developed for visible and near-infrared spectra, which is suited for use in remote sensing applications and can calculate the polarized radiation emerging from an atmosphere. The single-layer polarized radiative transfer equation and inhomogeneous multi-layer connection are solved by the discrete ordinates method and adding method, respectively. Monte Carlo model (MYSTIC, as the benchmark) and PolRadtran/RT3 are used to evaluate the new method in both accuracy and computational efficiency under different atmospheric conditions and view angles. Judging from the results, the accuracy of Stokes vector (I-, Q-, U-, V-component) calculated by the new method is a good agreement with the results by PolRadtran/RT3 except where near solar incident zenith angle and anti-incident zenith angle. The relative root mean square errors (RMSE) of Stokes vector for test cases between MYSTIC and the new method or RT3 can also prove the good accuracy of new method. Meanwhile, the new method has a higher computational efficiency compared to RT3, especially for the atmosphere with large scattering optical depth. As differ from RT3, the computing time of the new method cannot increase with increasing optical depth.


AS08-A007
A Study on Changes in Particle Characteristics Depending on Relative Humidity Using LiDAR Data

Sohee JOO1+, Youngmin NOH1#, Dukhyeon KIM2, Juseon SHIN1, Naghmeh DEHKHODA1, Juhyeon SIM1, Jaewon KIM1, Yuseon LEE1, Gahyeon PARK1, Jihyeon YUN1
1Pukyong National University, Korea, South, 2Hanbat National University, Korea, South

In this study, the Extinction coefficient(α) was calculated using lidar data installed at Seoul National University and divided by the mass concentration of fine particles to confirm the Mass Extinction Efficiency(MEE). This study used lidar data from January 2015 to June 2020 for analysis and compared the mass concentration of fine particle at the AirKorea Gwanak-gu station and relative humidity data(RH) at the Metropolitan Meteorological Administration. RH was divided into 7 sections, and we checked the change in the particle's characteristics. As a result, as the RH increased, MEE tended to increase, and it was confirmed that the PM2.5/PM10 ratio also increased. However, the α ratio observed by lidar appears different from the mass concentration. The α Fine/Total ratio rather decreased as the RH increased. Conversely, the α Coarse/Total Ratio showed an increase. We thought to be caused by differences between observation equipment. Airkorea's station method is a Beta-radiation attenuation monitor method that uses a heater to remove some moisture to lower the RH. However, in the case of LiDAR, the effect of RH is not removed by directly observing particles distributed in the atmosphere. Particles corresponding to PM2.5 in a dry atmosphere can increase to a particle size larger than PM2.5 as the RH increases, so they can be classified as coarse particles in LiDAR. However, in mass concentration measurement, the effect of humidity is partially removed, and It is classified as PM2.5. 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-2023-01-02-084).


AS08-A012
Real-time LiDAR Ratio Calculation Using Nighttime Camera and Laser

Juhyeon SIM1+, Dukhyeon KIM2, Juseon SHIN1, Sohee JOO1, Jaewon KIM1, Yuseon LEE1, Gahyeon PARK1, Jihyeon YUN1, Youngmin NOH1#
1Pukyong National University, Korea, South, 2Hanbat National University, Korea, South

When atmospheric information is analyzed through LiDAR, backscattering coefficients and extinction coefficients are calculated through LiDAR signals. The LiDAR ratio represents the ratio of the extinction coefficient and the backscattering coefficient. The LiDAR ratio is a variable that varies depending on the size distribution of particles in the air, the refractive index of particles, etc. Still, in most studies, it is fixed as a constant, and the extinction coefficient is calculated from the backscattering coefficient, or the backscattering coefficient is calculated from the extinction coefficient. In this study, LiDAR using a 532 nm wavelength laser and a camera attached to the lidar were utilized. The relationship between the extinction coefficient and the backscattered signal was examined by calculating the backscattered signal proportional to the backscattered coefficient with the pixel value of the laser taken in the picture while obtaining the extinction coefficient by LiDAR. Using these two variables, it was confirmed that the optimized lidar ratio could be calculated according to each atmospheric condition. In addition, in the case of LIDAR, because of the field of view (FOV), a short-range signal of about 0.5 km cannot be calculated. However, since the camera can also obtain pixel values at a short distance, the near-field extinction coefficient can also be restored by using the previously obtained LiDAR ratio and the backscattered signal received from the photograph. Through this study, it was confirmed that if the pixel signal of the camera is used, it is possible to calculate the extinction coefficient more accurately by using the LiDAR ratio optimized for each atmospheric situation, and the overlapping LiDAR short-range signal can be restored.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-2023-01-02-084).


AS08-A013
Geometric Factor Correction in the Horizontal Scanning LIDAR System

Juseon SHIN1#, Gahyeon PARK1+, Dukhyeon KIM2, Youngmin NOH1
1Pukyong National University, Korea, South, 2Hanbat National University, Korea, South

We tried to use scanning Light Detection and Range (LIDAR) to measure PM mass concentration as a three-dimension. The scanning Lidar system can detect PM mass concentration in an area with a radius of 5 km using 1064 nm and 532 nm wavelengths. Furthermore, the time resolution of the scanning LIDAR is as short as 10 sec, so it can apply to the timely monitoring of specific aerosol emissions. In the experiment for emissions of aerosols, we faced some problems; the laser was blocked at 2500 m by mountain, and the overlap distance of the 1064 nm laser was longer than that of the 532 nm laser. For the former problem, we neglected the signal from blocking and found the reference extinction coefficient through measured signals over 10 min to increase SNR. In the case of the overlap problem, the range-corrected signal contributed to increasing the slope, which made the reference signal overestimated. Therefore, we need to correct the LIDAR signal by the geometric factor in blind-zone, in which the backscattered signal cannot reach the field of view on telescope. For those reasons, 1) we have theoretically calculated geometric factor from experimental system parameters, such as laser beam divergence, FOV, distance between laser and telescope, and others. 2) We also experimentally considered the relationship signals between 1064 nm and 532 nm lasers to find the signal loss with the assumption of constant Angstrom Exponent. 3) We have corrected geometric factors iteratively from theory to experiment. 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-2023-01-02-084).


AS08-A014
Determined Spatial and Temporal Variability of Mixing Layer Height Using Aerosol Backscatter Data of Ceilometer

Hyunkyoung KIM1+, Heejung JUNG1, ChangHoon JUNG2, Junshik UM1#
1Pusan National University, Korea, South, 2Kyungin Women's University, Korea, South

A mixing layer height (MLH) is an important factor that controls air pollution concentrations. Thus, it is necessary to determine MLH accurately and to understand its spatial and temporal variability. One of the common methods for determining MLH is to calculate MLH using the vertical profiles of aerosol backscatter measured by a ceilometer. Originally, a ceilometer has been developed to detect the cloud base height. However, its measurement has also been used to determine the MLH, and several ceilometer measurement networks have been emerged across the world. The Korea Meteorological Administration (KMA) has installed ceilometers to observe cloud amount and cloud base height, and two different types of ceilometers, Vaisala CL31 and Eliasson CBME80B have been operating at 64 stations in Korea. Since 23 December 2022, the National Institute of Environmental Research (NIER) in Korea also has deployed nine Lufft CHM 15k ceilometers to determine the MLH and they are in operation now.
In this study, the MLH was determined based on a gradient method using the aerosol backscatter data measured by KMA and NIER ceilometers, and the spatial and temporal variability of MLH were quantified. The spatial and temporal variability of MLH was further examined as a function of the distance between ceilometers. All correlation analyses were also separated for daytime (06:00 LST to 18:00 LST) and night-time (18:00 LST to 06:00 LST), which had also compared each other. Based on these analyses, the impacts of temporal and spatial variability of MLH on the determined MLH were examined.


AS08-A016
Prediction Algorithms for the Rapid Changes of Visibility According to the Radiation Fog Events

Jaewon KIM1+, Dukhyeon KIM2#, Youngmin NOH1, Juseon SHIN1, Sohee JOO1, Juhyeon SIM1, Yuseon LEE1
1Pukyong National University, Korea, South, 2Hanbat National University, Korea, South

Fog is defined as a case where the visibility distance is less than 1 km by atmospheric water droplet, and it is known that fog is difficult to predict because it is caused by various causes depending on the seasons and locations. However, the extinction coefficient of water droplet at a given wavelength of 550 nm is exactly determined by the product of the volume concentration of a water droplet with a given refractive index of 1.33 and the volume extinction efficiency defined at the given size and wavelength. So the rapid change of visibility can be simply explained only by the rapid changes of the volume extinction efficiency by particle size or the rapid changes of water droplet concentration. The volume extinction efficiency sequentially reaches the maximum value following the wavelength for the constantly increasing particle size. In this study, we developed the algorithms on how to predict the occurrence of radiation fog by measuring the growth rate of particles using the relative change in extinction coefficient that occurs sequentially at the three wavelengths of RGB (449nm, 534nm, 597nm). Based on the particle growth theory, when particles grow in various ways, how the extinction coefficient changes at three wavelengths was studied, and how the relative value of the extinction coefficient at each wavelength changes with the growth of the particle size. Based on these theoretical results, we checked the changes of the extinction coefficient obtained from the 3 wavelengths at the radiation fog events and predicted the fog disappearing in the Daecheong area around Daecheong Lake where actual radiation fog often occurs. This work was supported by the “Graduate school of Particulate matter specialization.” of Korea Environment Industry & Technology Institute grant funded by the Ministry of Environment, Republic of Korea.


AS10-A003
Impact of Tropical Intraseasonal Oscillation on the 2015 Indian Heatwave

Tukaram ZORE#+, Kiranmayi LANDU
Indian Institute of Technology Bhubaneswar, India

It is well known that tropical intraseasonal oscillation (ISO) modulates the weather in the tropics. The ISO’s importance in cyclogenesis, extreme precipitation events, and heatwave events is established in the literature. Hence understanding and simulating these oscillations can tremendously improve the extended-range predictions of weather extremes. With changing climate, the frequency and intensity of heatwaves are known to be increasing and becoming one of the primary weather catastrophes. In May 2015 southeastern states of India faced the deadliest heatwave in its history which claims to take 2500 lives. The atmospheric circulation and role of surface fluxes in forming this heatwave were studied in the recent past but the underlying physical mechanism is not known. In this study, we investigated the impact of the tropical intraseasonal oscillation (ISO) in forming the May 2015 heatwave over the southeastern regions of India. The observations show that the occurrence of a heatwave is attributed to north-eastward propagating ISO circulation which results in persistent high-pressure anomaly with anomalous downward motion favoring clear skies, adiabatic heating, and horizontal warm advection. The 2m maximum temperature anomaly shows that 60% to 75% contribution in maximum surface air temperature (SAT) during heatwave period is from ISO-related temperature anomalies. Further numerical analysis using the WRF model confirms that this heatwave event was caused by Propagating ISO. The model output shows a difference of 1.5 to 2 ℃ in maximum SAT between the control and sensitive experiment. Indicating the substantial role of ISO in the development and intensification of the heatwave. This analysis emphasizes that improving the forecasting skills of ISO may facilitate the sub-seasonal forecast of local heatwave events.


AS10-A016
Comparison and Application of Gap-filling Algorithm for Extreme Climate Analysis of Vanuatu Observation Data

Imgook JUNG+, Kyungwon PARK, Jong Ahn CHUN#
APEC Climate Center, Korea, South

The weather observation data collected over a long period of time can be used as important data as the basis for showing the long-term climate characteristics and extreme weather of an area. Meanwhile, in the case of developing countries, it is difficult to collect high-quality weather observation data due to the lack of installation and management system of weather observation equipment. Through the Van-KIRAP (Vanuatu Klaemet Informesen blong Redy, Adapt mo Protekt, in Bislama) project, APCC (APEC Climate Center) wanted to provide observational data that could be useful in the Vanuatu region by adding the gap-filling of observational data to the OSCAR (tailored System of Climate services for AgRiculture) system. Through a comparative analysis conducted by applying various existing gap-filling algorithms to observation data, an algorithm technique suitable for precipitation and temperature, which are the target variables of this study, was selected. The performance of the gap-filling algorithm was compared using the standard statistical indicator CC (Correlation Coefficient) and RMSE (Root Mean Squared Error), and an algorithm that shows compliance performance was selected. It is expected to be used in various applied studies, including long-term climate analysis and extreme climate analysis, through correction observation data through the OSCAR system.


AS10-A017
Development of Long-term Climate Products Using Remote Sensing Data

Kyungwon PARK#+, Imgook JUNG, Jong Ahn CHUN
APEC Climate Center, Korea, South

Long-term climate data is one of the main data used for climate analysis, but in developing countries, the development of observation data is insufficient compared to developed countries. We tried to build observation data for long-term climate analysis using satellite remote sensing as the data needed for climate analysis. Precipitation datasets were constructed using GridSat and GPM-IMERGE, and the temperature was constructed based on AQUA, TERRA on installed MODIS sensor and AIRS satellite products. The results of the 10km spatial resolution of the satellite output were developed using the IGISRM technique to construct the entire Vanuatu area with high-resolution grid datasets of 5km. It is expected that climate analysis of high-resolution grid data produced in this project will be used as data for agriculture and various applications.


AS10-A019
The Latitudinal Position of the Westerly Jet Stream Modulated by the Tropics-Extratropics Boundary and Sea Surface Temperature Fronts

Mari MUTO#+, Tsubasa KOHYAMA
Ochanomizu University, Japan

Large-scale dynamics in the tropics and midlatitudes are governed by two 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, 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-extratropics boundary in the Northern Hemisphere.
The 5800 meter height line at 500 hPa is defined as the tropics-extratropics 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. Then, we investigate the positional relationship between the jet stream and the tropical mid-latitude boundary.
By measuring the mean latitudinal distance between the jet stream and the boundary, it is shown that the jet stream flows near tropics-extratropics boundary in most seasons. However, only in seasons when a sea surface temperature (SST) front exists near the boundary, the westerly jet stream is anchored by the SST front and temporarily leaves tropics-extratropics boundary. In boreal spring and autumn, when the westerly jet stream is trapped above the SST front, the existence of mesoscale phenomena such as the Meiyu-Baiu front may be required to connect the tropical and midlatitude solutions in place of the westerly jet stream.


AS10-A023
Development of Composite Hydrological Drought Index for Northern Thailand Watershed

Duangnapha LAPYAI1#+, Chakrit CHOTAMONSAK1, Somporn CHANTARA1, Atsamon LIMSAKUL2
1Chiang Mai University, Thailand, 2Environmental Research and Training Center, Thailand

This research aims to assess the effectiveness of hydrological drought indicators in describing characteristics of drought events and to develop a composite hydrological drought index (CHDI) to better characterize the drought conditions in the northern watershed of Thailand, where hydrological droughts frequently occur as a result of climate change and land use. The study utilizes the WRF-CESM climate model and land cover data from MODIS (IGBP) as inputs for the VIC hydrological model to analyze the drought indicators. The VIC model includes surface soil moisture, runoff, precipitation, baseflow, first-layer soil moisture, evaporation, and second-layer soil moisture. The results showed that all parameters have moderate to high correlations with runoff gauge station data, respectively. The CHDI was further developed by combining the indicators using weights derived from the principal component analysis (PCA) technique. The CHDI showed a better correlation (r= 0.45-0.73) with the observed data and was closest to the low-volume water events declared by the Upper Northern Region Irrigation Hydrology Center.


AS10-A026
Footprints of Atlantic Multidecadal Oscillation in the Low-frequency Variation of Extreme High Temperature in the Northern Hemisphere

Miaoni GAO#+
Nanjing University of Information Science & Technology, China

The frequency and intensity of extreme high temperature (EHT) in the Northern Hemisphere exhibit remarkable low-frequency (LF) variations (longer than 10 years) in summer during 1951–2017. Five hotspots featuring large LF variations in EHT were identified, including western North America–Mexico, eastern Siberia, Europe, central Asia, and the Mongolian Plateau. The probability density functions show that the higher EHT occurrences over these hotspots in recent decades is consistent with the shifted average and increased variances in daily mean temperature. The common features of the LF variation in EHT frequency over all domains are the remarkable increasing trends and evident decadal to multidecadal variations. The component of decadal to multidecadal variations is the main contribution to the LF variations of temperature in the last century. Further analysis shows that the coherent variability of decadal to multidecadal temperature variations over western North America–Mexico, eastern Siberia, Europe, and the Mongolian Plateau are the footprints of a dominant natural internal signal: the Atlantic multidecadal oscillation. It contributes to the variations in temperature over these hotspots via barotropic circumglobal teleconnection, which imposes striking anomalous pressure over these regions. This study implies that natural internal variability plays an important role in making hotspots more vulnerable to EHT.


AS10-A029
Recent Changes and Related Factors of Tropical Night in the South Korea Metropolitan Area

TaeHun KANG1#+, Donghyuck YOON2, Junseo PARK1, Dong-Hyun CHA1
1Ulsan National Institute of Science and Technology, Korea, South, 2Princeton University, Korea, South

To investigate the recent change of tropical night in South Korea, we analyzed the duration and intensity of tropical nights (daily minimum temperature, Korea Meteorological Administration; KMA) for 40 years (1979-2018) quantitatively. Spatiotemporal analysis showed that the tropical nights in the Seoul metropolitan area were more intense and longer-lasting as compared to other South Korean regions. Specifically, the tropical nights over this region increased more prominently in intensity, frequency, and duration. The tropical night event in the metropolitan area was classified into pure-TN (no heatwave prior to tropical night) and HWTN (tropical night following heatwave). The composite analysis was conducted for two types of tropical night events, pure-TN, and HWTN, based on 40-year ERA5 reanalysis data. Pure-TN mostly occurred when the edge of western North Pacific subtropical high (WNPSH) was present over the Korean Peninsula with the southwesterly wind, leading to a positive temperature advection anomaly in the metropolitan area. Furthermore, a positive low cloud cover anomaly with enhanced downward longwave radiation also prevailed. On the other hand, HWTN mainly occurred when the WNPSH expanded northwestward until its center was located over the Korean Peninsula with a positive downward shortwave radiation anomaly. Moreover, a descending motion anomaly induced adiabatic heating over the metropolitan area was presented. The significant increasing trends in tropical night events (pure-TN: 0.143 day/year, HWTN: 0.077 day/year) were observed at 95% confidence level. To investigate these trends, the regression analysis was performed on the synoptic factors for three sub-analysis periods with 10 days (21-31 July;P1, 1-10 August;P2, 11-20 August;P3). As a result, the favorable atmospheric conditions for HWTN (pure-TN) have been frequently constructed during P2 (P1 and P3).


AS10-A034
Examining Taiwan's Extreme Rainfall Changes from an Event Perspective

Pin-Yu CHAO+, Cheng-Ta CHEN#
National Taiwan Normal University, Taiwan

Understanding the changes in extreme rainfall has raised a lot of attention since it is one of the major exposures in terms of climate risk. In Taiwan, extreme rainfall usually occurs with the unique environmental condition such as tropical cyclone or Mei-yu front. While Extreme indices has been widely used for analyzing extreme rainfall, the data sample is based on each grid instead of the extreme rainfall event itself. Therefore, investigating the extreme rainfall from the event perspective can provide a new insight for the changing extremes. Here we apply the event-tracking method by using Depth-First Search algorithm on high-resolution gridded observation data to track the extreme rainfall events from 1980 to 2019 in Taiwan. Two different thresholds (80mm and 200mm) are then selected for analysis due to their potential threats to river flood and flash flood. Our results show that the extreme rainfall events have increased significantly in both frequency and intensity. Frequency changes in extreme rainfall events indicate a 16.84% increase for 200mm-event and a 10.95% increase for 80mm-event. Mean changes of total rainfall volume also show a larger increase for 75.40% in 200mm-event than 33.03% in 80mm-event. Within all the contributors to the change of total rainfall volume, mean affected area contributes the most even without the effect of increasing rainfall intensity to the threshold. Furthermore, the increasing frequency of extreme rainfall events is larger in southern Taiwan than in northern Taiwan.


AS10-A037
Intense Western Disturbance Associated Extreme Precipitation Events Over Western Himalayas as Simulated by WRF Model

Nischal SHARMA+, Raju ATTADA#
Indian Institute of Science Education and Research Mohali, India

Extreme precipitation events (EPEs) associated with intense extratropical cyclonic storms (Western Disturbances; WDs) during the winter season (December through March) have the potential to induce catastrophic damages to life, infrastructure, environment and agricultural sustainability over the western Himalayas (WH). However, a sparse in-situ observational network in this region conjugated with complex topography highlights the uncertainties in available coarse resolution precipitation products and emphasizes the necessity of finer grid scaled regional climate models for accurate simulation of precipitation variability, specifically EPEs with highly localized characteristics as well as underlying synoptic dynamics. The present study is an effort to investigate the performance of a ultra-resolution Weather Research and Forecasting (WRF) model through the evaluation of its sensitivity to various microphysical schemes and their ensemble for the simulation of intense episodes of WDs and associated extreme precipitation events over the WH. The sensitivity of precipitation extremes (identified using percentile approach) to different microphysics (~3 km resolution), in the WRF model configured on two two-way nested domains (9km and 3km), has been validated using multi-source rainfall datasets including gauge-based (IMD) and satellite (IMERG) observations as well as with the latest regional reanalysis dataset, IMDAA. Different rainfall skill scores (CSI, ETS, BSS, HSS, POD and FAR) provided insight into how well WRF mimicked intense WDs and the accompanying rainfall. Furthermore, the corresponding dynamics and physical processes in the model has been elucidated through a composite analysis for the simulated EPEs using the reanalyses, IMDAA and ERA5. Our findings underpin the sensitivity of model-simulated winter precipitation extremes associated with intense WDs over WH to different microphysical parameterizations. Detailed results will be discussed.


AS13-A003
Historical Fidelity and Future Change of Amundsen Sea Low Under 1.5°C-4°C Global Warming in CMIP6

Miaoni GAO#+
Nanjing University of Information Science & Technology, China

The realistic simulation and projection of the Amundsen Sea Low (ASL) are essential for understanding the Antarctic climate and global climate change. Using 14 models that participated in phase 6 of the Coupled Model Intercomparison Project (CMIP6), this study evaluates the climatological characteristics of ASL with comparison to the ERA5 reanalysis and their CMIP5 versions and assesses the future change of ASL under 1.5℃-4℃ global warming. The climatological spatial distribution of ASL is captured reasonably but with underestimated intensity by CMIP6 multi-model ensemble (MME). Among the CMIP6 models, EC-Earth3 has most accurate representation of ASL according to the pattern correlation and biases. The seasonal variation of the ASL depth and location are found to be reasonably reproduced by the CMIP6 models. Compared with CMIP5, CMIP6 MME exhibit evident reduced uncertainties and overall improvement in simulating absolute depth and location of the ASL center, which might be attributed to models’ capability of representing westerlies, while the biases in relative depth become even large in CMIP6 MME. In response to future warming from 1.5℃ to 4℃ above pre-industrial levels, the absolute depth of ASL will very likely deepen with larger amplitude in all seasons, while the relative depth might enhance only under high-level warmer world in austral autumn to winter. The CMIP6 MME also projects that the ASL will shift poleward constantly in austral summer and migrate southwestward during austral autumn with the rising global mean temperature. The enhancement and poleward movement of ASL could also be identified during the Ross Sea ice advance season under 1.5℃-4℃ global warming. The results reveal the potential of CMIP6 models in the ASL study and the impact of ASL on Antarctic climate under different global warming levels.


AS13-A005
Two-way Interactions Between Storm Tracks and Sea Ice in the Southern Hemisphere

Xihui MAO#+, Li ZHANG
Ocean University of China, China

Using the lagged maximum covariance analysis (MCA), the present study investigates the interannual variability of the storm track in the Southern Hemisphere and the Antarctic sea ice throughout the year. The results show that the two are most tightly coupled in the austral cold seasons. Specifically, storm track anomalies in June and July are associated with a zonal dipole structure of the sea ice concentration (SIC) anomalies in the western Hemisphere, with centers in the Antarctic Peninsula and the Amundsen-Bellingshausen Seas. The storm track can modulate the large-scale atmospheric circulations, which induces anomalous meridional heat transport, downward longwave radiation, and mechanical forcing to further influence the SIC anomalies. The resultant SIC anomalies can last for several months and have the potential to feed back to the storm track. According to the MCA, the influence of the SIC anomalies to the storm track is most evident in August. The SIC dipole along with the SIC anomalies in the Indian Ocean sector have large impact on the storm track activities downstream. The SIC anomalies alters the near-surface temperature gradient and subsequently atmospheric baroclinicity. Further energetic analysis suggests that the enhanced atmospheric baroclinicity facilitates the baroclinic energy conversion from mean available potential energy to eddy available potential energy, and then to eddy kinetic energy, strengthening the storm track activities over the midlatitude Indian Ocean.


AS13-A010
Seasonal and Interannual Variations of Poleward Moisture Transport by Atmospheric Rivers in the Southern Hemisphere

Kyu-Myong KIM1#+, Alexa HENNY1,2
1NASA Goddard Space Flight Center, United States, 2NASA Postdoctoral Program, 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 seasonal and interannual variations of the poleward moisture transport by AR using 43-year MERRA-2 reanalysis data. 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. 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. In this talk, 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 will be discussed on intraseasonal, seasonal, and interannual timescales.


AS13-A011
Cause of the Extreme Warming Event on February 9, 2020, in Seymour Island, Antarctic Peninsula

Hyo-Jun BAE1+, Seong-Joong KIM2,3#, Baek Min KIM1, Ha-Taek KWON4
1Pukyong National University, Korea, South, 2Korea Polar Research Institute, Korea, South, 3University of Science and Technology, Korea, South, 4Seoul National University, Korea, South

In early February 2020, two consecutive extreme warming events occurred within three days of each other at the same location in the Antarctic Peninsula (AP). The second event on February 9, 2020, saw the temperature reach 15.5°C at Marambio station on Seymour Island, northeast of the AP, the second-highest recorded temperature. To understand the cause of the extreme warming event, observational data from Marambio station and the European Center for Medium-Range Weather Forecasts Reanalysis v5 (ERA5) data were analyzed to examine extreme warming events that had occurred on Seymour Island during February over the past 40 years. The analysis revealed that the extreme warming event on February 9, 2020 was caused by foehn winds and large-scale horizontal advection, which are associated with a strong blocking high in the upper and lower atmosphere. Unlike typical extreme warming events in February over the past 40 years, the event in 2020 occurred not only in the AP but also throughout the entire West Antarctica.


AS13-A014
Teleconnection of the El Niño-southern Oscillation Impacts on the Antarctic Sea Ice Under the Near Future Condition

Jihae KIM1+, Daehyun KANG2, Myong-In LEE1#
1Ulsan National Institute of Science and Technology, Korea, South, 2Korea Institute of Science and Technology, Korea, South

The El Niño–Southern Oscillation (ENSO) is well-known climate variability in the tropics that has the potential to affect the Antarctic sea ice. The sea ice concentration pattern induced by ENSO is primarily linked with an anticyclonic circulation anomaly in the Amundsen-Bellingshausen Sea (ABS) that modulates atmospheric poleward temperature advection and longwave radiation forcing via poleward moisture advection. In the current climate, the remote influences between the tropics and the Antarctic are strongest during Austral spring (September-October-November, SON). However, this seasonality can change in future conditions. Comparing the remote influences from the tropics to the Antarctic between the present (1982-2014) and the near future (2015-2050) using the CMIP6 historical and SSP585 experiments, the positive geopotential heights at 500 hPa in the ABS regressed onto the ENSO index becomes stronger in Austral winter (June-July-August, JJA). This results in a more extended melting period of sea ice by the remote forcing from the tropics. The stronger response in the upper-level geopotential height anomalies in JJA is suggested by the increased forcing in the tropics and strengthened jet stream. The global model experiments with a dynamical core only support well these changes in the dynamical mechanisms related to the Antarctic sea ice condition in the future.


AS14-A005
Subseasonal Forecasts of Precipitation Over Maritime Continent in Boreal Summer and the Sources of Predictability

Yang LYU#+, Xiefei ZHI, Yan JI
Nanjing University of Information Science & Technology, China

The current paper investigates the weekly forecasts skills on precipitation in boreal summer over Maritime Continent (MC), which is an area featured by complex topography, warmest oceans, and characterized by great vulnerabilities to high-impact precipitation events, for the models of European Centre for Medium-Range Weather Forecasts (ECMWF) and China Meteorological Administration (CMA) derived from the S2S Project. Results indicate that the ECMWF model shows generally superior forecast performances than CMA, which is characterized by lower errors and higher correlations compared with the observations. Meanwhile, ECMWF tends to produce wet biases with increasing lead times, while the mean errors of CMA are revealed to be approximately constant throughout lead times of 2–4 weeks over most areas. Besides, the temporal correlations between model outputs and observations obviously decrease with growing lead times, with a high-low distribution presented from north to south. In order to detect the sources of predictability, the roles of large-scale drivers like ENSO and BSISO in modulating subseasonal precipitation forecast skills are also assessed in the models. Both ECMWF and CMA can reasonably capture the ENSO related precipitation anomalies for all lead times, while their capabilities of capturing BSISO related precipitation anomalies decrease with growing lead times, which is more obvious in CMA. The enhanced subseasonal precipitation forecast skills mainly respond to the BSISO associated precipitation variability. For most MC areas such as southern Indochina, western Indonesia, Philippines and the eastern ocean, the forecast skills of both ECMWF and CMA can be improved to a great extent by enhancing the capture of BSISO related precipitation anomalies, with the temporal correlations for both ECMWF and CMA increased by about 0.15 for lead times of 3–4 weeks. It provides an opportunity window for the models to improve precipitation forecasts on the subseasonal timescale.


AS14-A006
Improved MJO Prediction Using a Multi-member Subseasonal to Seasonal Forecast System of NUIST (NUIST CFS 1.1)

Jiye WU1,2#+, Yue LI3, Jing-jia LUO1, Xianan JIANG4, Takeshi DOI2, Toshio YAMAGATA2
1Nanjing University of Information Science & Technology, China, 2Japan Agency for Marine-Earth Science and Technology, Japan, 3New South Wales Government, Australia, 4University of California, Los Angeles, United States

The Madden-Julian Oscillation (MJO) provides an important source of global subseasonal-to-seasonal (S2S) predictability, while its prediction remains great challenges. Based on an atmosphere-ocean coupled model and the widely-used nudging method, suitable initialization and ensemble schemes are explored toward an improved MJO prediction. It is found that strong but not excessive relaxation strength for the divergence and vorticity, and a mild relaxation for the air temperature are appropriate to generate good atmospheric initial conditions. Additionally, the ensemble strategy with perturbed atmospheric nudging coefficients conduces to adequate ensemble spread and hence improves the prediction skill.Here, an 18-member ensemble subseasonal prediction system called NUIST CFS1.1 is developed. Skill evaluation indicates that the NUIST CFS1.1 can extend the MJO prediction to 24 days lead, which outperforms a majority of current models in the S2S project but is far from the estimated potential predictability (~47 days). The limited skill at longer lead times corresponds to forecast errors exhibiting slower propagation and weaker intensity, which are largely owing to the model’s shortcoming in representing MJO-related physical processes. The model underestimates the diabatic heating of enhanced convection and fails to reproduce the suppressed convection within the MJO structure, collaboratively weakening the Kelvin/Rossby waves. This causes weaker horizontal winds and ultimately reduces the horizontal moisture advection on the two flanks of MJO convection. Furthermore, the underestimated Kelvin wave induces insufficient planetary boundary layer (PBL) convergence and thereby results in poor simulation of PBL premoistening ahead of MJO convection. These biases limit the MJO prediction in the NUIST CFS1.1, prompting further efforts to improve the model physics.


AS14-A008
Predictability Limit of Monsoon Intraseasonal Precipitation and its Prediction in S2S Models: An Implication of Central Indian Ocean Mode

Jianhuang QIN1#+, Lei ZHOU2, Baosheng LI3
1Hohai University, China, 2Shanghai Jiao Tong University, China, 3Second Insititute of Oceanography, China

The prediction of monsoonal precipitation during Indian summer monsoon (ISM) remains difficult. Due to the high correlation between the Central Indian Ocean (CIO) mode index and the ISM precipitation variability, the predictability limit of the CIO mode index is investigated by the non-linear local Lyapunov exponent (NLLE) method in observations. Results show that the predictability limit of the CIO mode index can reach 38 days during boreal summer (from June to September), which is close to the upper predictability limit of intraseasonal precipitation (up to 40 days), and higher than the predictability limits of dynamical monsoon indices (under 3 weeks) and boreal summer intraseasonal oscillation (BSISO) indices (around 30 days). Such high predictability limit of the CIO mode index is mainly attributable to the long predictability limits from the intraseasonal sea surface temperature (SST) and intraseasonal zonal wind, which are the components of the CIO mode. However, the prediction skill of the CIO mode in the subseasonal-to-seasonal (S2S) air–sea coupled models is still an issue. The ECMWF and UKMO models display significantly higher skills for up to about 2 and 3 weeks, respectively, which are longer than other S2S models. The decline of the CIO mode prediction skill is due to the reduced signal of subseasonal zonal winds at 850 hPa over the tropical central Indian Ocean (especially along the equator; 5°S–5°N, 70°E–85°E). Therefore, a better simulation of tropical subseasonal zonal winds is required to improve the CIO mode prediction in models, and the improvement will benefit a better MISO simulation and a higher prediction skill during the ISM.


AS14-A010
Machine Learning Based Subseasonal to Seasonal (S2S) Forecasts for Warm Season Predictability

Venkatesh BUDAMALA+, Rajarshi DAS BHOWMIK#
Indian Institute of Science, India

S2S forecast has significant potential to aid decision-makers in mitigating extreme weather risks. Efficient S2S forecasts employ a central component between Weather and Climate predictions (for two weeks to less than a season). S2S models can yield adequate information based on the probability of the occurrence of extreme events within sufficiently larger areas through the prediction of complex, large-scale predictors. However, one of the significant challenges for S2S forecast is to develop a robust relationship for warm season predictability. A warming climate amplifies extreme events, making them a greater societal threat. Therefore, the current study develops an adaptive machine learning approach to predict the weekly frequency of intense warm days and 14-day standardized precipitation index (SPI) during the warm season for the Mahanadi River basin, India. The framework incorporates the multiple S2S global forecast models and ensembles across a continuum of S2S timescales to characterize the deterministic predictability of warm season atmospheric teleconnection patterns. The current skillful S2S forecasts of extreme heat and precipitation in warm season greatly benefit multiple sectors, including water management, public health, and agriculture, in mitigating the impact of extreme events.


AS14-A012
Key Regions in the Modulation of Seasonal GMST Variability by Analyzing the Two Hottest Years: 2016 vs. 2020

Kexin LI1+, Fei ZHENG2#, Deyang LUO2, Cheng SUN3, Jiang ZHU2
1Institute of Atmospheric Physics, Chinese Academy of Sciences, China, 2Chinese Academy of Sciences, China, 3Beijing Normal University, China

As an important parameter to measure the exchange of surface fluxes and climate sensitivity, the surface temperature is used to reflect specific responses to climate changes. The global mean surface temperature (GMST) justifiably became a primary indicator of climate volatility on a global scale to evaluate the intensity of climate change. However, the GMST peaked in 2020 under the background of moderate La Niña and even beat the highest record of GMST in 2016 when a strong El Niño occurred. The phenomenon overturned the conventional idea that the highest GMST occurs with strong El Niño. Our work used several datasets of surface temperature and adopted the ensemble empirical mode decomposition (EEMD) algorithm to distinguish the sources of direct contribution to the highest GMST of 2016 and 2020 at different timescales, especially focusing on the subseasonal-to-interannual variations. The results show that high GMST in 2016 was controlled by secular trend (SCT) and annual variability (ANV). However, the dominator of the sharp GMST rise in 2020 was SCT alone because the ANVs in different seasons canceled each other out in 2020, contributing little to the annual mean GMST. We further revealed two prominent patterns of seasonally varying ANVs, one is induced by atmospheric internal variability and the other is related to ENSO. The two patterns mainly located in Eurasia, North America, the Arctic Ocean, and the tropical eastern Pacific Ocean. Dominance by surface temperatures over the four crucial regions on the subseasonal-to-seasonal (S2S) GMST variations was also observed in nearly 80% of the years during 1982-2021, indicating a potential opportunity to improve the S2S GMST forecast by ameliorating the forecast in the four areas. Whether the contribution of ANV will become weaker and weaker in a warmer future world will be the concern of follow-up work.


AS14-A013
PISSARO: A Collaborative and User-oriented Project on the Monthly Forecasting of Extreme Events in the Southwest Indian Ocean

Sylvie MALARDEL1#+, Helene VEREMES1, Francois BONNARDOT2, Keunok LEE3
1Université de La Réunion - CNRS, France, 2Meteo-France, Reunion, 3CNRS - Université de La Réunion - Météo-France, Reunion

The PISSARO project focuses on atmospheric and oceanic forecasting at the subseasonal scale for applications over the southwest Indian Ocean basin. It is a collaborative academic research project, developed and conducted in partnership with stakeholders from Reunion and Seychelles and a panel of scientific experts in tropical forecasting. We have exploited the IFS monthly forecast ensemble for the development of future S2S-derived forecast products to provide probabilities of tropical cyclone trajectory scenarios, rainfall anomalies and to follow the ITCZ migration in the southwest Indian Ocean. The products which have been designed and calibrated with the S2S data are now tested in real time during the 2023 austral summer by the forecasters of the Seychelles Meteorological Authority and at the Regional Specialised Meteorological Centre - Tropical Cyclones of La Réunion. A co-creation approach between scientists, forecasters and humanitarian stakeholders has also enabled the development of products to anticipate the cyclone hazard in the southwest Indian Ocean region to support the tropical cyclone disaster risk management. The PIROI is testing this product under operational conditions for the 2022-2023 cyclone season. At the end of the TC season, all these prototypes will be evaluated and the best products will be selected for an operational implementation. We will provide an overview of these products at the workshop.


AS14-A015
The Role of Sea Surface Temperature Anomalies in Latent Heat Transport in the Northern Hemisphere

Kyungmin KWAK1+, Hajoon SONG1#, Myung-Seo KOO2, Eunjeong LEE2, JunSeong PARK2
1Yonsei University, Korea, South, 2Korea Institute of Atmospheric Prediction Systems, Korea, South

The heat transfer through atmospheric circulation is vital in determining local weather patterns. In the boreal summer, latent heat transport is the main contributor to the moist static energy transport from the equator to high latitudes. Using a global coupled atmosphere-ocean model (KIM-NEMO), we analyze the impact of ocean coupling on the subseasonal-to-seasonal (S2S) prediction of latent heat transport. The results showed that the highest latent heat transport in the boreal summer was along the eastern part of the continent. The simulations in July 2017 revealed the significant differences between KIM and KIM-NEMO, particularly over the Western North Pacific Ocean. These changes were triggered by the cold SST anomalies (SSTA) in KIM. The improvement of cold SSTA through ocean coupling influenced the regional wind patterns, leading to modifications in moisture transport. Consequently, latent heat transport is simulated more realistically, when considering air-sea interactions.


AS14-A019
Comparison of Monthly Rainfall Predictions Over Singapore for Improved Climate Services

Thea TURKINGTON#+, Wee Leng TAN, Chen SCHWARTZ, Shipra JAIN
Centre for Climate Research Singapore, Singapore

Situated in the deep tropics, Singapore experiences considerable intra- and interannual variability of rainfall. Therefore, improving rainfall predictions, including the 1-month rainfall outlook, is an important component of improving climate services for Singapore. Traditionally, seasonal prediction models were used as the basis for predicting rainfall for the next month and next season. These seasonal predictions were also combined with additional information, such as the status and outlook of climate drivers such as ENSO (El Nino Southern Oscillation) and MJO (Madden Julian Oscillation) to produce an expert-based outlook. However, for users who do not require outlooks prior to the end of the month, S2S predictions can be used instead, with S2S predictions issued towards the end of the month showing improved skill compared to the seasonal predictions for the 1-month rainfall outlook. This work compares the 1-month rainfall outlook for Singapore from various sources including seasonal models (single models and multi-model ensemble), the ECWMF extended range model as well as along with expert judgment for the period 2020 – 2022. The benefits of the various types of outlooks will also briefly be discussed as part of improving climate services for the country.


AS14-A020
The Winter North Pacific Teleconnection in Response to ENSO and the MJO in Operational Subseasonal Forecasting Models is Too Weak

Chen SCHWARTZ1+, Chaim GARFINKEL2#, Wen CHEN3, Yanjie LI4, Daniela I.V. DOMEISEN5
1Centre for Climate Research Singapore, Singapore, 2Hebrew University of Jerusalem, Israel, 3Yunnan University, China, 4Chinese Academy of Sciences, China, 5ETH Zurich, Switzerland

Teleconnection patterns associated with the Madden–Julian oscillation (MJO) and El Niño–Southern Oscillation (ENSO) impact weather and climate phenomena in the Pacific–North American region and beyond, and therefore accurately simulating these teleconnections is of importance for seasonal and subseasonal forecasts. Systematic biases in boreal midwinter ENSO and MJO teleconnections are found in eight subseasonal to seasonal (S2S) forecast models over the Pacific–North America region. All models simulate an anomalous 500-hPa geopotential height response that is too weak. This overly weak response is associated with overly weak subtropical upper-level convergence and a too-weak Rossby wave source in most models, and in several models there is also a biased subtropical Pacific jet, which affects the propagation of Rossby waves. In addition to this overly weak response, all models also simulate ENSO teleconnections that reach too far poleward toward Alaska and northeastern Russia. The net effect is that these models likely underestimate the impacts associated with the MJO and ENSO over western North America, and suffer from a reduction in skill from what could be achieved.


AS14-A021
Evaluation of a Spatial Approach to the Verification of Gridded S2S Wind Forecasts for Southeast Asia

Wee Leng TAN#+, Thea TURKINGTON, Shipra JAIN, Chen SCHWARTZ
Centre for Climate Research Singapore, Singapore

Weather and climate in Southeast Asia are heavily influenced by the Monsoon, with the Monsoon traditionally characterised by the seasonal change in wind directions along with seasonal changes in precipitation. Wind observations or reanalysis data are commonly used for defining the Monsoon period and therefore having wind forecast for the region can provide information on the upcoming onset and cessation of the Monsoon. A spatial approach to the verification of gridded S2S wind forecasts for Southeast Asia is investigated and analysed. The approach uses the fractional skill score (FSS), a neighbourhood spatial verification method commonly used for verifying high resolution precipitation forecast. This spatial approach verification method avoids the problems of conventional local grid-based verification metrics, such as double-penalty when predicting the correct pattern of wind but at the wrong position, and can highlight the spatial displacement of the wind patterns in the forecast. The score for the ECMWF Extended Range wind forecast for Southeast Asia region will be evaluated and compared with the conventional local grid-based verification metrics for the added information using the spatial approach. The possibility of the usage of sub-seasonal wind forecast for the Monsoon onset and cessation forecast in the region will also be discussed.


AS14-A022
MJO-related Rainfall in Southeast Asia: How Well is it Represented by Subseasonal Operational Forecasting Models?

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. Southeast Asia (SEA) is 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 assess the representation of MJO-related rainfall in subseasonal forecasting models. Specifically, we will explore how well the commonly used MJO monitoring indices can represent rainfall associated with MJO in SEA, both in observations and the models. The skill of the models to simulate MJO-related rainfall in sub-regions in SEA where different MJO phases show the largest subseasonal variability will be examined, as well as the seasonality in prediction skill of MJO-related rainfall in these sub-regions.


AS14-A023
Influence of Compound Zonal Displacements of the South Asia High and the Western Pacific High on Meiyu Subseasonal Variation

Zhiwei ZHU#+, Shanshan FU
Nanjing University of Information Science & Technology, China

Meiyu shows substantial subseasonal variation at periods of 10–30 days and 30–60 days, which often leads to extreme precipitation and disastrous flooding over the Yangtze River Basin. Monitoring and prediction of the subseasonal variation of Meiyu is crucial for disaster prevention and mitigation. Here, we proposed two sets of novel indices for Meiyu real-time monitoring and prediction based on the compound zonal displacements of the South Asia high (SAH) and the western Pacific high (WPH) at 10–30-day and 30–60-day period. For the 10–30-day period of Meiyu, the zonal displacement of the SAH is associated with a mid-latitude Rossby wave train, whereas the WPH is related to the second mode of the boreal summer intraseasonal oscillation. On the 30–60-day timescale, the zonal displacement of the SAH and the WPH are both associated with the first mode of the boreal summer intraseasonal oscillation. The subtle differences in zonal displacement of the SAH and the WPH determine eight type configurations, corresponding to distinct influences on Meiyu. Meiyu subseasonal variation can be well reconstructed by using the relationship between these two indices and rainfall anomalies pattern over China. Given that the ECMWF S2S model is more skillful in forecasting upper- and lower-level circulation than that in directly forecasting precipitation, a hybrid dynamical–statistical model is conducted to predict the Meiyu subseasonal variation with the ECMWF model forecast indices. The hybrid model outperforms the ECMWF model in predicting the Meiyu subseasonal variation at 17–40-day lead times.


AS15-A009
Assimilation of Aerosol Optical Depth from Geostationary Environmental Monitoring Spectrometer to Improve a Prediction of Asian Dust Storm

Ebony LEE1+, Milija ZUPANSKI2, Seon Ki PARK1#
1Ewha Womans University, Korea, South, 2Colorado State University, United States

In the spring season, Korea suffers from the Asian dust storms (ADSs) sometimes originated from the Gobi Desert and Inner Mongolia. Since the ADSs are known to deteriorate respiratory or eye health as well as visibility, it is important to predict the occurrence and the intensity of ADSs through numerical prediction and satellite observations. In this study, we assimilate aerosol optical depth (AOD) retrieved from Geostationary Environmental Monitoring Spectrometer (GEMS) observing East Asia. The ADSs are affected by various atmospheric (e.g., wind, temperature, planetary boundary layer, etc.) and land surface conditions (e.g., land use, soil temperature, soil moisture, etc.). Therefore, we employ a coupled meteorology-chemistry model --- the Weather Research and Forecasting model coupled with Chemistry (WRF-Chem) --- in order to consider the complex interactions among the atmospheric and land surface variables simultaneously. The Maximum Likelihood Ensemble Filter (MLEF) is adopted to assimilate AOD. For an ADS case in March 2021, it is shown that the GEMS AOD assimilation improves the analysis and prediction of AOD and is useful for ADS prediction in the East Asia region.


AS15-A012
Identifying Sensitive Areas for Targeted Observations to Improve Numerical Prediction of Asian Dust Storms Over South Korea

Seungyeon LEE1+, Xiaohao QIN2, Seon Ki PARK1#
1Ewha Womans University, Korea, South, 2Chinese Academy of Sciences, China

In air quality prediction, initial conditions are essentially required for a coupled atmosphere-chemistry model which is based on both atmospheric and aerosol/chemistry observations. In general, a higher amount and quality of observations produce more accurate model results; however, forecast errors in a region of interest may grow from an initial error in a specific upstream region, primarily due to the lack of observations therein. Therefore, it is a milestone to find the upstream areas from which a small initial error can grow into large forecast errors in the region of interest. The conditional nonlinear optimal perturbation for initial conditions (CNOP-I) is a suitable tool for adaptive (targeted) observations. To calculate the CNOP-I, several variables are included in defining multiple energy equations (e.g., kinetic energy, dry energy, moist energy, etc.). In particular, the previous studies on improving the Asian dust storms (ADSs) prediction mainly considered the kinetic energy calculation, which included only two variables (u-wind and v-wind). The goal of this study is twofold: finding variables that strongly affect the ADSs and identifying sensitive areas for the adaptive observations. We collected and examined the ADS events that occurred during the last 32 years (1990—2021) over South Korea. Through the principal component analysis, we first recognized top variables—temperature, vertical velocity, divergence, specific humidity, ozone mass mixing ratio, and eastward wind—which affect origination and translocation of the ADSs; for example, strong downdraft and divergence make ADSs finally land on the Korean Peninsula. We are applying the CNOP-I to identify the sensitive areas for adaptive observations in air quality prediction. We expect to improve air quality forecasts by classifying the synoptic situations that brings about severe ADS outbreaks in South Korea and by identifying the upstream areas for adaptive observations to which we can enhance observations, potentially through international collaborations.


AS16-A001
Changes in the SST-precipitation Relationship Over the Indo-pacific Warm Pool Under a Warming Climate

Hye-Ryeom KIM+, Kyung-Ja HA#
Pusan National University, Korea, South

The Indo-Pacific warm pool (IPWP) is a region with one of the strongest atmospheric convections on Earth and deep convection over the IPWP plays a key role in global climate. In recent decades, it has experienced human-induced warming. In addition, it has been observed to have a non-linear relationship between Sea Surface Temperature (SST) and precipitation. Even though SST is increasing, the increase in precipitation is limited up to a specific SST, defined as saturation threshold SST (STT). Existing STT indicates that a completely different state occurs before and after STT showing a non-linear response of precipitation to SST. However, how warmer climates affect changes in the SST-precipitation relationship as well as STT is yet to be unexplored. To investigate future changes in the relationship between SST and precipitation, we used a joint distribution of the two variables with the historical data as well as three Shared Socioeconomic Pathway (SSP) scenarios (SSP2-4.5, SSP3-7.0, and SSP5-8.5) during the near future (2041-2060), and far future (2081- 2100). The results demonstrate that with the shift of mean state, the STT rises due to the involvement of atmospheric stratification in all three scenarios in both future periods, but the largest increase is observed in the SSP5-8.5 scenario during the far future. In the warming climate, greater warming in the upper troposphere compared to the surface leads to stabilization of the troposphere, supporting an increase in STT through Moist-Adiabatic Lapse Rate (MALR) adjustment. This study suggests a change in the SST-precipitation relationship and a possible mechanism for a limited increase in precipitation, and thus provides a background for a better understanding of a non-monotonic precipitation response to SST in the context of climate change.


AS16-A004
Convectively-coupled Kelvin Waves: Moist Static Energy and Gross Moist Stability Analyses

Yi-Bin HORNG+, Jia-Yuh YU#
National Central University, Taiwan

Convectively-coupled Kelvin wave (CCKW) is one of the important large-scale oscillations in the equatorial area. It is an eastward-propagating mode that constantly causes fluctuations in pressure and winds, and thus, CCKW takes part in shaping the weather and climate through bringing countless rainfall events to countries in tropics. CCKW is relatively active in the Pacific and the Indian basins due to the absence of obstruction from topography, and yet it shows distinct properties over these two regions, including the intensity, active season, symmetry, and propagation speed. The vertical profiles also suggest the differences in tilting angle and the extent of low-level pre-moistening at the leading edge of the convection. It is hypothesized that the differences arise from the mechanisms in triggering the convection associated with CCKW. We conduct a detailed moist static energy (MSE) budget analysis to uncover the dominant factors in driving the energy recharge-discharge process of CCKW. The results indicate that the key factors might lie in the horizontal advection and moisture profile, especially within the boundary layer. The gross moist stability, a measure of development of moist convection, is also tested over the two regions. It is speculated that the background environmental conditions play a major role in determining the structures of CCKW.


AS16-A011
Climatology and Environmental Conditions of Two Types of Quasi-linear Convective Systems with Extremely Intense Weather in North China

Jie SHENG#+
National Meteorological Center of China, China

In this work, the spatial and temporal distribution characteristics of 171 QLCS cases in North China identified by an objective identification method for the period 2013—2018 are analyzed. According to the statistics of intense weather produced by them, at least two types of QLCSs exist: one type with strong thunderstorm wind gusts and the other with extreme heavy rainfall. Furthermore, the characteristics of circulation pattern, environmental condition, terrain effect, and surface cold pool as a key type of mesoscale system are given for the two types of QLCSs. The findings are presented as follows. The spatial distribution of QLCSs in North China. There are significant differences in the month of occurrence, the spatial scale, the moving speed, the formation time and maintenance period between the two types of QLCSs. The circulation background, environmental conditions and cold pool are also obviously different. The atmospheric baroclinicity is relatively obvious for QLCSs with strong thunderstorm wind gusts. The large value area of BCAPE and DCAPE caused by the dry middle layer and large temperature reduction rate are important environmental conditions for the generation of strong convective wind gusts. The strong cold pool and vertical wind shear within the layer of 0—3 km altitude play an important role in the forward propagation of the QLCSs. Extreme precipitation caused by QLCSs with heavy rainfall is more prominent for this type of QLCSs than that for the previous type. The second type of QLCSs usually occur in weak synoptic-scale forcing systems with sufficient water vapor supply. The back propagation maintained by the interaction between the weak cold pool or the windward slope and the low level southerlies is the main mechanism for the development and slow movement of the QLCS, which is also directly responsible for extreme heavy rainfall.


AS17-A011
Validation, Analysis, and Comparison of MISR V23 Aerosol Optical Depth Products with MODIS and AERONET Observations

Ruonan FAN+, Yingying MA, Shikuan JIN#
Wuhan University, China

The latest Multi-angle Imaging Spectro Radiometer (MISR) V23 aerosol optical depth (AOD) products were released, with an improved spatial resolution of 4.4 km, providing an unprecedented opportunity for the refined regional application. To ensure the reliability of their applications and build a scientific reference for the further optimization, it is imperative to conduct a comprehensive evaluation, especially for the unique size-resolved AOD products: small-size AOD (AODS, representing the contribution of fine-mode aerosols), medium-size AOD (AODM), and large-size AOD (AODL), and AODM+L represents the AOD part of coarse-mode aerosols. AErosol RObotic NETwork (AERONET) and MODerate-resolution Imaging Spectroradiometer (MODIS) C6.1 aerosol products from 2001 to 2020 are utilized for the validation, analysis, and inter-comparison, considering three spatial scales and four key factors. In general, MISR V23 aerosol products show a good accuracy compared with AERONET. The best performance for all AOD products appears in forest units (the highest R ~ 0.93, data percentage within Expected Error bounds, %EE > 93), related to the inactive human activity and dark underlying surface. Dependences of retrieval deviations illustrate that the performance of MISR AOD deteriorates as aerosol loading increases. Namely, with the increase of aerosols, total AOD (AODT) and AODS show increasing negative deviations, while increasing positive deviations are observed for AODM+L. This suggests that the Empirical Orthogonal Functions do not perform well in this situation, since numerous aerosol particles can obstruct the underlying reflection and reduce the surface spectral contrast. In addition, AODT and AODS often exhibit anomalous positive deviations in areas with low vegetation cover, such as deserts, revealing that MISR will overestimate aerosol content over bright surfaces and in environments dominated by coarse-mode particles. The above findings not only deepen the understanding of MISR aerosols products from multiple perspectives, but also provide useful information for the product improvement.


AS17-A012
Toward a Versatile Spaceborne Architecture for Immediate Monitoring of the Global Methane Pledge

Pengfei LI#+
Hebei Agricultural University, China

The global methane pledge paves a fresh, critical way toward Carbon Neutrality. However, it remains largely invisible and highly controversial due to the fact that planet-scale and plant-level methane retrievals have rarely been coordinated. This has never been more essential within a narrow window to reach the Paris target. Here we present a two-tiered spaceborne architecture to address this issue. Using this framework, we patrol the world, like the United States, China, the Middle East, and North Africa, and simultaneously uncover methane-abundant regions and plumes. These include new super-emitters, potential leakages, and unprecedented multiple plumes in a single source. More importantly, this framework is shown to challenge official emission reports that possibly mislead estimates from global, regional, to site scales, particularly by missing super-emitters. Our results show that, in principle, the above framework can be extended to be multi-tiered by adding upcoming stereoscopic measurements and suitable artificial intelligence, thus versatile for immediate and future monitoring of the global methane pledge.


AS17-A017
A Case Study of Extreme Precipitation Forecast Based on Satellite Data Assimilation in North China

Jiexia WU#+, Jiawen CUI, Xiangze JIN, Fangyuan PING, Shiyu ZHUANG
PIESAT, China

This study used Weather Research and Forecasting model (WRF) 4.4 and Weather Research and Forecasting model data assimilation system (WRFDA) 3D-var assimilation system to analyze and predict two extreme precipitation events in North China during summer 2022. Based on the system, different satellite data were assimilated in the initial field to improve the accuracy of the model forecast. The satellite data used in this study are NOAA AMSU-A/B, FY-3D MWHS-II/MWTS-II, FY-4A AGRI and Himawari-8 AHI. Artificial intelligence algorithm was applied to these satellite data to retrieve atmospheric temperature and moisture profiles, and these results were used for data assimilation in the system. In this study we have designed three experiments: 1 control run and 2 experiments. The control run only assimilated conventional data to the initial field. Besides the conventional data, the first experiment assimilated AI retrieved atmospheric temperature and moisture profiles and the second experiment assimilated brightness temperature from these sensors. We conducted 72 hours forecast for all the experiments and evaluated the precipitation amount and area with observed data. The results showed that the AI algorithm that we have developed in this study performed well in atmospheric temperature and moisture profile retrieval and the temperature and moisture profiles had positive contributions to precipitation forecast. According to TS, FAR and POD sores, the second experiments showed high accuracy in 0-6 hour precipitation forecast.


AS17-A020
Retrieval of Total Precipitable Water from Gk2A/AMI Data Using Machine Learning Approach Over Korea

Hyejin MOON1#+, Jae-Young BYON2, Myoung-Hee LEE1
1Korea Meteorological Administration, Korea, South, 2National Institute of Meteorological Research, 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. Traditionally TPW has been calculated from using vertical profiles of temperature and humidity. But operational TPW derived from GK2A provides under only clear sky conditions and TPW calculated from radiosonde observations provides in several stations at 4 times in a day. To overcome temporal and spatial limitation of these TPW, this study proposes a retrieval algorithm based on convolutional neural network (CNN) model to retrieve TPW from geostationary Korea multi-purpose satellite 2A (GEO-KOMPSAT 2A, GK2A) equipped with the Advanced Meteorological Imager (AMI). The TPW is prepared by integrating the water vapor profiles from radiosonde observations over Korea. The algorithm performances are assessed using radiosonde observations for other period as the reference data. Through statistical verification, the results show that the CNN model performs with a root mean square error (RMSE) of 9.42 (5.32) mm, a bias of 0.02 (-0.76) mm, and a correlation coefficient of 0.88 (0.94) under all (clear) sky conditions. This study addressed the availability of satellite-derived TPW to resolve the limitations of in situ measurements and cloudy sky conditions. Both the quantity and the quality of data are important in machine learning approach. We will expand training data like as GNSS and numerical weather forecast model to improve retrieval of TPW.


AS17-A022
Development of Atmospheric Profile Retrieval Algorithm for FY-4A/B GIIRS

Hye-In PARK#+, Byung-il LEE, Junhyung HEO, Myoung-Hee LEE
Korea Meteorological Administration, Korea, South

The National Meteorological Satellite Center of the Korea Meteorological Administration has developed an algorithm to retrieve the atmospheric profiles for Geostationary Interferometric Infrared Sounder (GIIRS) onboard FengYun-4A/B (FY-4A/B). Hyperspectral infrared sounder with thousands of channels has a high vertical resolution, so it can estimate more accurate atmospheric temperature and humidity profiles and is useful for monitoring severe weather such as typhoons and heavy rainfall because it highly depends on atmospheric instability and water vapor information. To develop the algorithm for GIIRS of FY-4A/B, channel selection, and systematic bias correction were performed. The channel was chosen to consider the vertical distribution of the weighting function, except for the channel with strong trace gas absorption and channels with large observation error among 1650 channels of FY-4A GIIRS and 1682 channels of FY-4B GIIRS. The retrieved temperature and humidity profiles with GIIRS/FY-4 for the summer of 2022 were compared with radiosonde and the profiles of the GK2A AMI. The validated results of GIIRS/FY-4 were similar to the GK2A even though more channels were used. So it is needed various sensitivity tests to get more accurate temperature and humidity profiles using hyperspectral infrared sounder such as the number of channels and wavelength selection used by the algorithm. The detailed results and plans are presented at the conference. 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 (KMA2020-00120)


AS17-A024
Radial Distribution of Deep Convective Clouds Preceding Rapid Intensification of the Tropical Cyclones in the Western North Pacific

Chian-Yi LIU1#+, Jason Pajimola PUNAY2
1Academia Sinica, Taiwan, 2Bicol University, Philippines

This study investigates the radial distribution of deep convective clouds 24 hr prior to the rapid intensification (RI) of the tropical cyclones (TCs) in the Western North Pacific. TCs are categorized according to the 24 hr future intensity (Vmax) change (ΔVmax), as follows: non-RI (ΔVmax < 30 kt), short RI (RI-S, ΔVmax > 30 kt for less than a day), and long RI (RI-L, ΔVmax > 30 kt continuously for at least 1 day). RI-S TCs have the strongest intensity and shortest RMW within 24 hr prior to RI, whereas non-RI TCs have the weakest intensity and longest RMW within 24 hr prior to its lifetime maximum Vmax. In all categories, highest DCC percentage (DCC-P) and coldest temperature (DCC-T) are found within 3 RMW from the storm’s center. Non-RI has the lowest DCC-P and warmest DCC-T anywhere within 10 RMW, whereas RI-L has the highest DCC-P and coldest DCC-T within 2 RMW especially at the onset of RI. DCC-P starts to increase 12 hr prior to RI with sharpest 3-hr increase of 17% at 2-3 RMW in RI-L. DCC-T within RMW is always colder than that within 2-3 RMW, 9 hr prior to RI. Sharpest DCC-T difference of 3oC is found in RI-L, at least 3 hr prior to RI. Results in the study can be used to identify the TCs that are more likely to undergo prolonged RI even before the RI onset.


AS17-A025
Update of Global Maps of Alisov's Climate Classification Using an Unsupervised Machine-learning Algorithm

Ryu SHIMABUKURO1#+, Tomohiko TOMITA1, Ken-ichi FUKUI2
1Kumamoto University, Japan, 2Osaka University, Japan

Alisov's climate classification was proposed in 1954, and it focuses on the January–July changes in large-scale air mass zones and their fronts. In this study, data clustering by machine learning was applied to global reanalysis data assimilated from some satellite data to quantitatively and objectively determine air mass zones, which were then used to classify the global climate. The differences in air mass zones between two half-year seasons were used to determine climatic zones, which were then subdivided into continental or maritime climatic regions or according to east–west climatic differences. This study began by questioning whether the global climate can be divided into four air mass zones as Alisov did in the 1950s. The results showed that Alisov's four air mass zones from the 1950s were supported from a modern data-driven perspective using high-quality global reanalysis data. In addition, the clustering technique accurately captured frontal precipitation between air mass zones in the mid-and high latitudes. This study, thus, renews Alisov's climate classification for the first time in almost 70 years and applies data-driven machine learning to establish a standard for air-mass-based climate classification. This paper has been peer-reviewed once in Progress in Earth and Planetary Science (PEPS) and a revised manuscript is in preparation.


AS19-A001
Statistical Post-processing of Week 3-4 Precipitation Forecasts Over Taiwan

Joyce JUANG1#+, Hui-Ling CHANG2,3, Shih-Chun CHOU4, Chih-Yung Feng FENG5, Han-Fang LIN5, Jing-Shan HONG2
1Central Weather Administration, Taiwan, 2Central Weather Bureau, Taiwan, 3National Central University, Taiwan, 4International Integrated Systems, Inc., Taiwan, 5Manysplended Infotech Ltd, Taiwan

Numerical prediction models cannot correctly predict the extended-range (10-30-day) precipitation amount and pattern over Taiwan due to the low predictability. However, demand for extended-range precipitation forecasts by users in different sectors has grown significantly. In this study, a statistical post-processing technique combining Analog Post-processing (AP) and Probability-Matched mean (PM), called APPM, is used to perform bias correction and downscaling for week 3-4 precipitation forecasts in Taiwan. The purpose is to provide users with more accurate Quantitative Precipitation Forecasts (QPF) and more reliable Probabilistic Quantitative Precipitation Forecasts (PQPF). Previous study shows that 1-14-day post-processed precipitation forecasts using APPM, including QPF and PQPF, are promising. Here we want to confirm that the APPM method also works for the week 3-4 forecast range, which was thought to be a “predictability desert” with little forecast skill. Forecast evaluation shows that the raw ensemble is under-dispersive, while the calibrated ensemble distribution well represents the observation variability. Compared to the raw forecasts, the AP-based probabilistic forecasts have better reliability and higher skill in discrimination. Users with a much wider spectrum of cost/loss ratio can benefit more from the calibrated forecasts in decision making as compared to the raw forecast. In addition, the calibrated QPF removes most bias and displays obviously higher correlation and reduced error.


AS19-A003
Precipitation Characteristics of Tropical Cyclones During Summer Monsoon Season in the North Indian Ocean

Surya Pramod JALAKAM1+, Pay-Liam LIN1#, Wei-Yu CHANG1, Balaji Kumar SEELA1,2, Jayalakshmi JANAPATI1
1National Central University, Taiwan, 2Academia Sinica, Taiwan

This study examines the environmental conditions that influences the tropical cyclone (TC) occurrence frequency (TCOF) as well as the rain microphysics of TCs over the North Indian Ocean (NIO) during major monsoon stages (pre-monsoon, monsoon, and post-monsoon) in 2014-2021. Two regions in NIO domain are a particular focus, namely, the Arabian Sea (AS) and the Bay of Bengal (BOB). TCs that formed within the NIO domain and reached at least the tropical storm stage were selected. High TCOF is attributed to the combined presence of warm sea surface temperature and cyclonic wind or positive 850-hPa relative vorticity. Moreover, high reflectivity and heavy rainfall are found within the 50 km radius from the storm’s center. Monsoon season TC Vayu (2019) have the heaviest rainfall and highest reflectivity within the inner band region, as compared to pre-monsoon TC Fani (2019) and post-monsoon TC Kyaar (2019). The probability density functions of the rain microphysics parameters vary with the season (pre-monsoon, monsoon, and post-monsoon) and the mode of rain (total, stratiform, and convective). In all season, the breakup process is found to be dominant in total and stratiform precipitating clouds, whereas the break-up and coalescence processes are comparable in convective precipitating clouds.


AS19-A010
A Study on Microphysical Characteristics of Mei-yu Season Rainfall Over Taiwan

Jayalakshmi JANAPATI1+, Balaji Kumar SEELA1,2, Pay-Liam LIN1#
1National Central University, Taiwan, 2Academia Sinica, Taiwan

The Mei-yu season over Taiwan, mainly associated with frontal systems, is a transition period (May and June) between the winter and summer seasons. The interactions of Mei-yu season frontal systems with the complex topography of Taiwan lead to heavy precipitations across the island. The present study investigates rain and microphysical attributes of the Mei-yu season over Taiwan using Global precipitation measurement mission dual-frequency precipitation radar (GPM DPR). To analyze the regional and intra-seasonal characteristics of the Mei-yu season, May and June are segregated into pre-Mei-Yu (5/15-5/31), mid-Mei-Yu (6/1-6/15), post-Mei-Yu (6/16-6/30). There are clear distinctions in the raindrop size distributions among pre-, mid-, and post-Mei-yu seasons, with abundant large drops in the post-Mei-yu. Furthermore, raindrop size distributions also showed apparent differences among four regions (north, south, central, and eastern part) of Taiwan, with relatively bigger drops in central Taiwan. The contoured frequency by altitude diagrams of rain rate, radar reflectivity, mass-weighted mean diameter, and normalized intercept parameters are used to understand the microphysical processes responsible for the regional and intra-seasonal variations. 


AS19-A012
Roles of Marine Boundary Layer Jet on Heavy Rainfall Over Taiwan During Early Summer Rainy Season

Chuan-Chi TU1#+, Chung-Hsiung SUI2, Mong-Ming LU2, Pay-Liam LIN1, Ching-Hsuan WU2
1National Central University, Taiwan, 2National Taiwan University, Taiwan

From the climatological views, 20-yr (1999-2018) June CFSR Dongsha wind vertical profiles are used to define the MBLJ days. It is found that when MBLJ occurs at Dongsha, the above 90/95-percentile extreme rainfall occurrence frequency over low land (< 1km) of western Taiwan and northern Taiwan is larger than that of NoTC days, with the peak values occur over southwestern slope of the Snow Mountains and the Central Mountain Range, and southwestern Taiwan. It is similar that the above 90/95-percentile extreme rainfall occurrence frequency over high land (> 1 km) of Taiwan is larger during MBLJ days than NoTC days, with peak values occur over southwestern slope of the Snow Mountains and the Central Mountain Range. During early summer rainy season (June) over the South China Sea, there are six CMBLJs (Coastal MBLJs) with occurrence frequency peaks (> 35 %). Their formation mechanisms are related to terrain. (1) and (2) BLJ-East and BLJ-West (East and West of Hainan Island over South China); (3) and (4) Orographic enhanced southwesterly (southwesterly flow impinging on southeastern tip of Vietnam and Taiwan); (5) Barrier jet off the northwestern Taiwan; (6) Gap wind flow through mountain gap over central eastern Vietnam.


AS19-A013
The Interdecadal Change of Relationship Between Ocean-atmospheric Thermal Environment and Typhoon Intensity in the Northwest Pacific Ocean

Chieh CHANG#+, Pay-Liam LIN
National Central University, Taiwan

Under climate change, the number of typhoons in the Northwest Pacific region will decrease and the proportion of strong typhoons will increase. In order to understand whether the interdecadal changes in the ocean and atmospheric environment affect the development of typhoon intensity. This study compares the changes in the ocean and atmospheric environment from June to November in the past two decades (1980-1999) and the current twenty years (2000-2019), and discusses the relationship between changes in the ocean and atmospheric environment and the typhoon intensity. Compared with the past, the sea surface temperature has increased by an average of 0.42°C, the ocean mixed layer depth has deepened by an average of 2.7 meters, and the ocean heat content (OHC) has increased by 9.89 kJ/cm2. The results show that under climate change, the thermal environment of the upper ocean will be more conducive to the development of typhoon intensity. In terms of atmospheric environment, the Pacific subtropical high strengthened and extended westward, and the monsoon trough also tended to retreat westward compared with the past. Under climate change, atmospheric environment has both positive and negative contributions to the development of typhoon intensity, and changes in the Pacific subtropical high, monsoon trough, and vertical wind shear will be unfavorable for the formation of typhoons. Using the observed maximum wind speed of typhoon and potential intensity to analyze the relationship between ocean and atmospheric environment and typhoon intensity. The results show that compared with the atmospheric environment, the ocean environment has a more direct relationship with typhoon intensity. Compared with sea surface temperature, OHC has a higher relationship with typhoon intensity. Moreover, the correlation between OHC and stronger typhoon is even more higher than that of weak typhoon. In conclusion, among all variables, OHC has highest correlation with typhoon intensity.


AS19-A014
Influence of COVID-19 Pandemic on Rain Microphysics Over Taiwan

Balaji Kumar SEELA1,2+, Jayalakshmi JANAPATI1, Pay-Liam LIN1#
1National Central University, Taiwan, 2Academia Sinica, Taiwan

The coronavirus disease 2019 (COVID-19) is responsible for the worldwide disorder in livelihood and enormous loss of human lives. To curtail the COVID-19 spread, the government of China imposed a lockdown over most of its provinces from 23 January to 25 March 2020. The effects of the COVID-19 lockdown on public health, transport, aviation, and meteorological parameters were well documented globally; however, its influence on rain microphysics is not fully understood. In the present study, we tried to report the distinction in precipitation microphysics, especially the raindrop size distribution between the COVID-19 lockdown (23 January to 25 March 2020) and non-lockdown (23 January to 25 March: 2015- 2029) periods over Taiwan. The raindrop size distributions between the lockdown and non-lockdown periods showed clear distinctions, with more mid- and large-size drops during the lockdown periods. Furthermore, possible microphysical differences between the lockdown and non-lockdown periods are explored using reanalysis and remote-sensing data sets.


AS19-A017
Using ISCA GCM with Dry Dynamical Core Examine to Simulate the Glacial Climate in Taiwan

Pin-Hsiu KUO1#+, Yu-Hsiang HUANG1, Po-Yu CHUANG1, Chien-Chung KE1, Kai-Chih TSENG2
1Sinotech Engineering Consultants, Inc., Taiwan, 2National Taiwan University, Taiwan

Studying the glacial climate provides opportunities to examine the change in climate systems in response to external forcing, e.g., solar radiation, greenhouse gases and the abrupt change in cryosphere. In addition, the climate is one of its external conditions which impacts the development of safety assessment scenarios, such as glacial and interglacial conditions causing sea level variations and the surface system changes. For example, the change in sea level in glacial and interglacial periods strongly determines the groundwater system and the ecosystem. The groundwater system dominates the flow rate which influences the hydrogeological condition in the near field and the potential release path from underground facility to the ecosystem in the far field. Also, the landform controls the release location of radioactive and how it will influence the biosphere. To have a better picture for the processes above and the potential risks, we leverage a GCM for simulating the glacial climate and downscale to the regional states of Taiwan. Specifically, we use ISCA, an idealized global circulation modelling framework, to simulate the glacial climate since 12,000 B.P. (last glacial maximum, LGM) until the present day. Following the standard of Held–Suarez experiment, we modulate the global energy budget through changing TOA radiation, solar zenith angle and proxy surface temperature (due to changed terrain in Taiwan and adjacent region) to mimic different climate states. Our study demonstrates the potential for safety assessment of spent nuclear fuel disposal repository based on model outputs from the idealized GCM along with the regional model downscaling.


AS19-A020
Analysis of Microphysics Process of Afternoon Thunderstorm Using Raindrop Size Distribution Retrieval from Polarimetric Radar Measurements

Chen-Hau LAN#+, Pay-Liam LIN
National Central University, Taiwan

The afternoon thunderstorm event is the common nature disaster in Taiwan area. Because of the short life cycle and high variety, it is difficult to observe the microphysics feature for whole system, especially the Drop Size Distribution (DSD), one of the fundamental microphysical parameters. Using dual-polarimetric radar to retrieve DSD is useful to obtain the variation of microphysical processes for the entire weather system. In general, the retrieved method is based on gamma distribution to reduce the degree of freedom and get the DSD parameter, such as shape parameter (µ), slope parameter (Λ), and intercept parameter (N0). However, the shape of DSD is incompatible with the gamma distribution if the specific microphysical processes are dominated. There is a new method with the moment-based operator to convert the dual-polarimetric variables to the moments of DSD which can avoid the model error. In this study, the new retrieved method is used to study DSD during different life period of the afternoon thunderstorm in Taipei area. Moreover, we try to categorize the feature of DSD under the influence of collisional coalescence, breakup, or drop settling processes. Base on the results of retrieved DSD, the evaporation and coalescence are the main microphysics processes in initial stage and mature stage respectively.


AS19-A023
Evaluation of Probabilistic Forecasts of Consecutive 5 Days Without Measurable Rainfall Over Taiwan

Shih-Chun CHOU1#+, Hui-Ling CHANG2,3, Tsun-Wen LO2, Chih-Yung Feng FENG4, Han-Fang LIN4
1International Integrated Systems, Inc., Taiwan, 2Central Weather Bureau, Taiwan, 3National Central University, Taiwan, 4Manysplended Infotech Ltd, Taiwan

In Summer, high temperatures and humidity are suitable for forage planting, but long days of sunshine are needed for hay preparation in this period to cope with the lack of fresh forage in autumn and winter over Taiwan. Therefore, the livestock industry has a demand for probabilistic forecasts of consecutive days without rainfall. However, due to the complex topographic distribution in Taiwan, rainfall forecast has high uncertainty in space and time and it is very difficult to capture the fine information from model output with low resolution. The purpose of this study is to provide users with reliable and skillful forecasts, which help users obtain more economic benefits in decision making. In this study, Analog post-processing (AP) is applied in 20-year re-forecasts of the National Centers for Environmental Prediction (NCEP) Global Ensemble Forecast System version 12 (GEFS v12) to produce calibrated and downscaled probabilistic forecasts of consecutive 5 days without measurable rainfall over Taiwan. The evaluation results show that (1) The under-dispersion of the raw forecasts is effectively improved through the AP method. (2) The probabilistic forecasts calibrated by AP method have better reliability, brier skill score and discrimination (potential usefulness) than raw forecasts. (3) The calibrated probabilistic forecasts can provide higher relative economic values compared to the raw forecasts, and it indicates the enhancement of forecast value.


AS19-A025
The Application of 3D Motion Fields in Radar Extrapolation Nowcasting: Case Study of Meiyu Front and Autumn Precipitation

Yu Chiao HSU#+, Kaoshen CHUNG, Yi-Hao ZHOU
National Central University, Taiwan

Radar echo extrapolation utilizes the observed composite reflectivity to estimate the motion fields of radar echoes and provide advection and rotation information for extrapolation. The uncertainty of motion fields is one of the major error in radar extrapolation. In addition, the weather system may have different moving directions at different heights. In this study, 3-Dimension motion fields is estimated by the entire volume scanned data and applied to MAPLE (McGill Algorithm for Precipitation nowcasting using Lagrangian Extrapolation) nowcasting system. With autumn precipitation events in the Yilan area and the Meiyu front events in Taiwan, the characteristic of 3D motion fields in space and time are analyzed. The results show that u-velocity changes a lot in both time and vertical levels in Mei-yu front event. As for autumn precipitation, the standard deviation and mean of u-velocity are similar to v-velocity. Then, the added value of 3D motion fields for the nowcasting is evaluated by continuous and categorical verification. It is found that when applying 3D motion fields in radar extrapolation nowcasting, it can capture more complete advection and rotation due to orographic effect over Taiwan area. Overall, the improvement of the nowcasting with 3D motion fields can be up to 3-h.


AS19-A027
Use Wind Profiler and Disdrometer to Analyze the Circulation and Rainfall Microphysics of Typhoons

Jun-Yan LI#+, Pay-Liam LIN, Chuan-Chi TU, Siang-Yu ZHAN, Chen-Hau LAN
National Central University, Taiwan

This study mainly discusses the synoptic environment, observed wind speed, wind direction and raindrop size distribution (DSD) when typhoon Maria (2018) and Lekima (2019) approach Taiwan. When typhoon Maria moves westward approaching northern Taiwan coastal ocean, the near surface wind speed strengthens to > 17 m/s which is observed by wind profiler at National Central University (NCU) over northwestern Taiwan. In addition, the observed wind direction using profiler gradually changes from northwesterly to southwesterly. The mass-weighted mean diameter in millimeters (Dm), observed by NCU impact-type Joss-Waldvogel disdrometer (JWD), gradually decrease to ~ 1.5 mm. On the other hand, typhoon Lekima moves northwestward from east of Taiwan. The NCU wind profiler observed near surface wind speed is smaller than 17 m/s and wind direction changes gradually from northeasterly to southwesterly. The Dm observed by NCU JWD changes irregularly as time processes. Research results show that wind speed and wind direction have impacts on DSD. Moreover, observed radar reflectivities show that the principal rainband of typhoon Maria passes northern Taiwan. At that time, the NCU JWD observations show that Dm is large (~ 2.5 mm) and the continuous rainfall > 12 hr. On the other hand, only the distant rainband of typhoon Lekima passes northern Taiwan and the observed Dm is small. The rainfall maintains less than 4 hr. Research results show that if principal rainband passes Taiwan or not influences DSD and the duration of rainfall.


AS19-A028
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, Taiwan, 2University of Hawaii at Manoa, United States

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.


AS20-A010
Global Cloud-resolving Simulations with NICAM on the Supercomputer Fugaku

Chihiro KODAMA1#+, Hisashi YASHIRO2, Tamaki SUEMATSU3, Daisuke TAKASUKA1, Yuki TAKANO1, Ryusuke MASUNAGA1, Yohei YAMADA1, Shuhei MATSUGISHI4, Takashi ARAKAWA4, Masuo NAKANO1, Hiroaki MIURA4, Tatsuya SEIKI1, Akira NODA1, Masaki SATOH4, Tomoki OHNO5, Tomoe NASUNO1, Tomoki MIYAKAWA4
1Japan Agency for Marine-Earth Science and Technology, Japan, 2National Institute for Environmental Studies, Japan, 3RIKEN, Japan, 4The University of Tokyo, Japan, 5Meteorological Research Institute, Japan

Global cloud-resolving climate simulation is believed to promote our understandings of the atmospheric phenomena with multi-scale nature and also improve reliability of their climate projections such as tropical cyclones and cloud feedback. With this background, the Nonhydrostatic ICosahedral Atmospheric Model (NICAM) has been developed and used for more than two decades. The first realistic global cloud-resolving (here, 3.5 km mesh) simulation was published in 2007, and its extension toward climate scale is now in sight with the supercomputer Fugaku, the latest flagship machine of Japan. The value of such climate simulation is guaranteed by a series of recent model improvements to better simulate both mean state and disturbances. We are also revealing the climatological performance of the ocean-coupled version of NICAM through a series of seasonal to decadal simulations. Other important challenges include a global O(103) ensemble prediction experiments with 14 km mesh and a global 220 m experiments toward an era of global large-eddy simulation. The above challenges on the supercomputer Fugaku would be harder without an effective co-design activity with the application developers. In terms of post-processing, we recently modified our MPI-based remapping tool and confirm its applicability to a global 870 m mesh data.


AS20-A016
Mesoscale Convective Systems Simulated by a High-resolution Global Nonhydrostatic Model Over the United States and China

Ying NA1#+, Qiang FU2, L. Ruby LEUNG3, Chihiro KODAMA4, Riyu LU5
1Beijing Municipal Climate Center, China, 2University of Washington, United States, 3Pacific Northwest National Laboratory, United States, 4Japan Agency for Marine-Earth Science and Technology, Japan, 5Chinese Academy of Sciences, China

Mesoscale convective systems (MCSs) contribute a large fraction of warm-season precipitation and generate hazardous weather with substantial socio-economic impacts. Uncertainties in convection parameterizations in climate models limit our understanding of MCS characteristics and reliability of future projection. We examine MCSs simulated by the global 14-km Nonhydrostatic ICosahedral Atmospheric Model (NICAM) without cumulus parameterization against satellite observation from Global Precipitation Measurement (GPM) during 2001-2008. We focus on MCSs over the central U.S. and eastern China where MCSs are prevalent from March to August. A process-oriented tracking method incorporating both cloud and precipitation criteria is used to identify and track MCSs. About 140/100 MCSs initiate in the central U.S./eastern China per warm season and most of them initiate east of high mountains and in coastal regions. The frequency distribution of MCS lifetime is well captured by NICAM. However the simulated MCSs have stronger precipitation, smaller precipitation area, and larger cold cloud system than observed in both regions, which may be caused by weak entrainment as it is not well resolved at 14 km resolution. The simulated MCS number is also underestimated in summer. By examining the climatological and MCS large-scale environments, the significant underestimation of MCS number in summer over the central U.S. may be attributed to the large climatological dry bias in the atmosphere. For China, mean moisture in summer is well simulated but deficiency in capturing the dynamic condition related to the coastal topography for triggering convection may have contributed to underestimation of MCS even in a sufficiently moist environment.


AS20-A020
On-the-fly Data Streaming from Climate Simulations for Training the Data-driven Surrogated Models

Hisashi YASHIRO1#+, Takashi ARAKAWA2, Kengo NAKAJIMA2
1National Institute for Environmental Studies, Japan, 2The University of Tokyo, Japan

Machine learning technology has recently been applied to weather and climate simulations. Compared to atmospheric models that include various algorithms, data-driven models can reduce the amount of computation (= elapsed time) and achieve significant speedups. A data-driven model for weather forecasting is being developed using datasets such as weather reanalysis (e.g., ERA5) and multi-model intercomparison (e.g., CMIP6). However, for meteorological/climate researchers who want to elucidate processes and mechanisms, data-driven models shouldn't be used as complete black boxes. We need high-speed, on-demand "surrogate models" to imitate the physical models that algorithms are based on understanding processes and continuously developed.
We developed a coupling library h3-Open-UTIL/MP (Arakawa et al., 2022) to bridge legacy weather/climate models and modern machine learning tools. This library was initially designed to connect each component of the earth system model. We extract the necessary training data from the part of the model code written in Fortran and pass it to ML frameworks in Python on-the-fly. The proposed system enables the creation of the necessary surrogate models step-by-step using a large amount of simulation data. We will present an overview of the library and initial experimental results.


AS20-A022
Application of Deep Learning with Physical Constraints in Precipitation Nowcasting

Hongxu ZHU#+, Ji CHEN
The University of Hong Kong, Hong Kong SAR

Nowadays, extreme precipitation has brought very serious losses. How to timely and accurately forecast precipitation has become the top priority of disaster prevention. The emergence of deep learning technology has provided a new idea for the precipitation nowcasting, and achieved good results in the short forecast period, but there is still a problem that as the forecast period becomes longer, the forecast effect becomes worse. On the basis of deep learning technology, this study attempts to introduce additional physical information and simulate the future information of numerical model forecast to improve the accuracy of precipitation nowcasting. This study uses precipitation data, and two-dimensional water vapor flux data in the input and forecast stages respectively. Because there are errors in the real forecast, random errors are introduced when additional future data is added into the forecast stage. The results show that, compared with the simple application of precipitation data, the introduction of more physical information in the input stage can improve the prediction effect by 4.75%, while the introduction of predicted future physical information in the forecast stage can improve the effect by 16.69%, showing a strong application prospect.


AS22-A003
Does the Expansion of Urban Areas Aggravate Air Pollution in North China Plain (NCP)?

Qian JIANG#+, Guohui LI
Chinese Academy of Sciences, China

Urban expansion has been rapid in North China Plain (NCP) since 2000, and the metropolitan area of 2015 increased by 4.92% compared with 2000. The change in Land-Use and Land-Cover (LULC) directly affects the meteorological conditions, impacting the atmospheric pollutant concentrations. Therefore, based on the MERIS300 LULC product of 2015, this study simulates a continuous heavy pollution incident from 05 December 2015 to 02 January 2016 in NCP, to explore whether the urban expansion causes LULC changes that will worsen the atmospheric environment. The T2 increases by 0.19 ℃ while the relative humidity (RH) decreases by 1.28%. Urbanization aggravates the pollution of O3 but reduces the other four concentrations of pollutants. The concentration of PM2.5 increased significantly. In addition, the trends of PM2.5 and O3 are significantly negatively correlated in vertical distribution. Therefore, it is necessary for PM2.5 and O3 to cooperate in emission reduction.


AS22-A004
Impacts of Changes in Land Use and Land Cover Between 2001 and 2018 on Summertime O3 Formation in North China Plain and Surrounding Areas - A Case Study

Jiaoyang YU1+, Weijian ZHOU2, Guohui LI2#, Qian JIANG2, Xuexi TIE2, Suixin LIU2, Xia LI2,3, Guohui LI2, Ruonan WANG2, Lang LIU2
1Institute of Earth Environment,Chinese Academy of Sciences, China, 2Chinese Academy of Sciences, China, 3University of Chinese Academy of Sciences, China

Changes in land use and land cover (LULC) influence meteorological fields and biogenic emissions, further affecting the atmospheric chemistry and air quality. Combing the satellite measurements and WRF-Chem model simulations, we evaluate impacts of the LULC change between 2001 and 2018 on the summertime ozone (O3) formation in North China Plain and surrounding areas (NCPs). Satellite measurements have revealed that from Taihang to Yanshan Mountain, the fraction of broadleaf and needle forest coverage has increased by 5%-20% and the urban area has increased by up to 25% in the NCP. Additionally, the vegetation density has increased significantly in the NCPs except for urban areas. The LULC change generally enhances biogenic volatile compounds emissions in the NCPs, particularly over Taihang and Yanshan mountain, but the O3 variation is divergent. The maximum daily 8-hours average (MDA8) O3 concentrations are reduced by 1%-7% over Taihang and Yanshan Mountain because the raised vegetation density increases O3 dry deposition velocity to accelerate the O3 loss. The raised vegetation density enhances the evapotranspiration to decrease the near-surface temperature by 0.1 ℃ ~ 1.5 ℃, which also generates a divergence in the low-level atmosphere in the NCPs, causing secondary northerly or easterly winds in the NCP. The O3 enhancement along the coastal areas of the NCP is attributed to the perturbation of wind fields and photolysis induced by the LULC change. The divergent variation of the MDA8 O3 concentrations in the NCP is generally caused by the variations of biogenic emissions and photolysis.


AS22-A005
Understanding How Solar Farms Modify Radiation Budget and Regional Climate Based on Satellite-observation Constrained Climate Modeling

Chongxing FAN#+, Xianglei HUANG
University of Michigan, United States

Solar farms consist of arrays of solar panels to convert solar energy to electricity. Building solar farms has become an acknowledged approach to mitigate global climate change. Meanwhile, solar farm deployments change the surface radiative properties and, thus, can impact the local surface radiation budget and climate. So far, global modeling studies have primarily focused on simulating the impact caused by surface albedo changes due to large-scale solar farm deployments. Such modeling studies lack long-term observational constraints and do not consider complex atmosphere-panel-surface interactions. Using Moderate Resolution Imaging Spectroradiometers (MODIS) aboard the NASA Aqua satellite, we have quantified the change of surface spectral reflectances, spectral emissivities, and land surface temperature over six solar farms commissioned in the southwestern U.S. Results suggest a 20-25% reduction of surface reflectance over the seven MODIS shortwave bands due to the solar panel installation, leading to a ~23% decrease in the surface upward shortwave broadband flux and a ~14-18% decrease in the clear-sky reflected shortwave flux at the top of the atmosphere. Despite the uncertainty and disagreement in current surface retrieval algorithms, results show that the outgoing longwave radiances over the MODIS infrared window channels are reduced. Based on these observations, we will implement a more realistic representation of solar farms in global climate models. Specifically, we will put a translational layer in the Community Terrestrial System Model, the land component in CESM. This layer will modify the radiative and momentum fluxes given solar panels’ geometrical and radiative properties on top of the natural surfaces. The new scheme can output panel temperature to be compared to and explain in-situ and satellite observations. It will help us understand the potential impact on the climate system if an increasing number of solar farms are deployed in the future.


AS22-A006
Effects of Irrigation on the Local and Regional Climate with a New Groundwater Scheme Using Couple Model Simulations

Ren-Jie WU1#+, Min-Hui LO1, Yadu POKHREL2, Agnès DUCHARNE3
1National Taiwan University, Taiwan, 2Michigan State University, United States, 3Institut Pierre-Simon Laplace, France

The critical zone (CZ), extending from the bottom of groundwater to the top of the lower atmosphere, plays a crucial role in shaping the environment and human well-being (Brantley 2007). The CZ and climate systems are affected by various natural and human-driven processes. In this study, we utilized a modified version of CESM2 that incorporated data on groundwater, irrigation, and human water use. The groundwater scheme has also been enhanced to simulate lateral flow and aquifer pumping. To assess the impact of irrigation on climate, we conducted two experiments spanning from 1901 to 2014: one with a fixed irrigation demand in 1901, and the other with a changing irrigation demand (Sibert 2015). Our results indicate that irrigation is concentrated in India, China, and North America. In India, the irrigation effect leads to increased soil moisture, latent heat, and decreased sensible heat, resulting in a cooling effect. Rainfall is also seen to increase, particularly in the Ganges river region. Conversely, the west coast of the USA experiences contrasting feedback with decreased rainfall and soil moisture. References: Brantley SL, Goldhaber MB, Ragnarsdottir KV. (2007). Crossing disciplines and scales to understand the Critical Zone. Elements 3: 307-314. Siebert S, Kummu M, Porkka M, et al. A global data set of the extent of irrigated land from 1900 to 2005[J]. Hydrology and Earth System Sciences, 2015, 19(3): 1521-1545.


AS22-A009
The Impact of Regional and Global Groundwater Pumping on Sea Level Changes

Ren-Jie WU1+, Min-Hui LO1, Yuwen FAN2, Eun-Soon IM3#
1National Taiwan University, Taiwan, 2The Hong Kong University of Science and Technology, Hong Kong SAR, 3HKUST, Hong Kong SAR

Severe groundwater depletion due to intensive irrigation has begun to emerge and has been clearly detected by satellite-based estimates in major agricultural areas, particularly the North China Plain. The effects of groundwater overexploitation are not restricted locally, but an incursion of dormant groundwater into the active hydrological cycle can critically affect the hydroclimatology of remote places and the global water budget, which eventually leads to terrestrial contributions to rising sea levels. This study explores how much groundwater depletion as a result of intensive irrigation will contribute to accelerating global sea level rise. For this, the long-term simulations with/without groundwater pumping are performed using the fully coupled configuration in Community Earth System Model (CESM). The groundwater-fed irrigation is activated in the North China Plain, the entire China, and global scale to discern different responses to the locations of the irrigation forcing. A comparative analysis of a suite of sensitivity experiments can facilitate identifying the obscure effect of groundwater pumping from the background climates. In particular, the quantification of the contributions of groundwater pumping to sea level changes will be focused, which will strengthen our understanding of the nonlinear climate processes that occur when the atmosphere, land surface, and subsurface are perturbed by groundwater pumping. [Acknowledgements]This research was supported by project GRF16309719, which was funded by the Research Grants Council (RGC) of Hong Kong. 


AS22-A010
Relationship of Land-use Changes with Wildfire Risks Under Global Warming Based on CMIP6 Multi-model Projections

Yan HE1+, Subin HA1, Eun-Soon IM2#
1The Hong Kong University of Science and Technology, Hong Kong SAR, 2HKUST, Hong Kong SAR

Wildfire hazards have witnessed a substantial increase in frequency, extent, and severity globally. While wildfire outbreaks and spread are strongly affected by non-climatic factors such as campfires, forest management, and monitoring capacity, there is a growing scientific consensus that increasing temperatures and resultant dryness may be responsible for a favorable environment for wildfires. A potential escalation of wildfires under global warming could result in changes to the land cover and carbon emissions, which may in turn have an impact on regional climate. However, complex climate-soil-vegetation-interacting processes leave numerous uncertainties in wildfire projections and their impacts under the acceleration of global warming. In this study, Forest Fire Danger Index (FFDI) and Fire Weather Index are calculated based on the Coupled Model Intercomparison Project (CMIP) multi-model projections in order to investigate future changes in fire weather danger under different emission pathways. The regional hotspots which are expected to face a heightened risk of fire weather are then focused on to further comprehend the wildfire and land cover feedback. (Acknowledgements: This study was supported by the Special Research Support Scheme from the Hong Kong University of Science and Technology (R9055), which was funded with the donation from the Chau Hoi Shuen Foundation.)


AS25-A003
Fast Response of East Asian Precipitation to Local and Remote Aerosol Emission Reductions During COVID-19

Weiyi WANG1+, Xiaohong LIU2#, Chenglai WU3, Guangxing LIN3, Yong WANG4, Zheng LU2, Xi ZHAO2, Linyi WEI4
1Institute of Atmospheric Physics, Chinese Academy of Sciences, China, 2Texas A&M University, United States, 3Chinese Academy of Sciences, China, 4Tsinghua University, China

In this study, the fast response of East Asian summer precipitation to COVID-induced aerosol emission reductions is examined using the Community Earth System Model version 2.2 (CESM2.2). The emission reductions decreased aerosol optical depth and cloud cover over northern China in June 2020. The troposphere became warmer, strengthening the land-sea thermal contrast and anomalous southerly winds. The subtropical westerly jet accelerated and shifted southwards, favoring the low-level convergence, upward air motions, and subsequent condensational heating over the Yangtze River Basin (YRB). The feedback of condensational heating in return strengthened the convergence and ascent. The western North Pacific Subtropical High was intensified, which further enhanced the moisture advection and convergence over the YRB. Both the enhanced moisture convergence and ascent increased precipitation over the YRB during June 2020. Furthermore, local and remote emission reductions show different impacts on convection and moisture transport over the YRB. The emission reductions over China caused stronger convective precipitation (1.15 mm/day versus 0.63 mm/day), but weaker larger-scale precipitation (1.17 mm/day versus 2.24 mm/day) than the emission reductions outside China did.


AS25-A006
Correlation Between the Number of Patients with Allergic Rhinitis and the Concentrations of Airborne Particles in Northern Beijing, China

Sun AIZHI1#+, Sun XIAOLI2, Zhang HAIHONG2, Li XUEYIN1, Wu SHUANGSHUANG1
1University of Chinese Academy of Sciences, China, 2Beijing Huairou Hospital, China

The presence of biological (airborne pollen) and non-biological (PM2.5, PM10, O3, CO, NO2, SO2, etc.) particles in the atmosphere is associated with the incidence of adverse allergenic reactions affecting human health. Considering all the probable effects of air pollutants and airborne pollen on allergic reactions, the present study mainly examines the relationship between the daily concentrations of airborne pollen, PM2.5, PM10, O3, CO, NO2, SO2, and the number of patients with allergic rhinitis (AR) at the same time in northern Beijing, China by statistical analysis. The results showed that the daily visiting number of AR patients was positively associated with the concentration of airborne pollen, as well as the pollutants NO2 and PM10 particles, while, it was negatively associated with the concentrations of O3 and CO. Airborne pollen and part air particles (e.g., NO2, PM10) had a significant impact on the morbidity of AR patients. Thus, public health and clinical approaches are needed to anticipate and reduce the morbidity of allergic disease caused by airborne pollen and non-biological particles.


AS25-A007
Effects of Different Types of Aerosols on Deep Convective Clouds and Anvil Cirrus

Jinming ZHANG1+, Bin ZHAO2, Xiaohong LIU3#
1Chinese Academy of Sciences, China, 2Tsinghua University, China, 3Texas A&M University, United States

Deep convective clouds and associated anvils exert opposite radiative effects. The impact of different aerosol types on these two categories of clouds remains a major challenge in understanding aerosol-cloud interactions. Using 11-year satellite retrievals, we find that cloud top height (CTH) and ice cloud fraction of deep convective clouds and anvil cirrus identified by Cloud-Aerosol Lidar with Orthogonal Polarization increase with small aerosol loadings and level off or even decrease with further aerosol increase. Compared with continental aerosols, CTH affected by marine aerosols starts to decrease at smaller aerosol loadings. Moreover, cloud optical depth (COD) of deep convective clouds decreases with aerosol loadings. COD of anvil cirrus increases with increased loadings of most aerosol types but decreases with smoke aerosol. These relationships are mainly attributed to the aerosol effect rather than the meteorological effects. Our findings contribute to the development of models and better assessment of aerosol-cloud radiative forcing.


AS25-A015
The Effect of Aerosols on Surface Ozone Through Meteorology Feedbacks Over China

Yawei QU#+
Jinling Institute of Technology, China

Interactions between aerosols and gases in the atmosphere have been the focus of an increasing number of studies in recent years. Here, we focus on aerosol effects on tropospheric ozone that involve meteorological feedbacks induced by aerosol–radiation interactions. Specifically, we study the effects that involve aerosol influences on the transport of gaseous pollutants and on atmospheric moisture, both of which can impact ozone chemistry. For this purpose, we use the UK Earth System Model (UKESM1), with which we performed sensitivity simulations including and excluding the aerosol direct radiative effect (ADE) on atmospheric chemistry, and focused our analysis on an area with a high aerosol presence, namely China. By comparing the simulations, we found that ADE reduced shortwave radiation by 11 % in China and consequently led to lower turbulent kinetic energy, weaker horizontal winds and a shallower boundary layer (with a maximum of 102.28 m reduction in north China). On the one hand, the suppressed boundary layer limited the export and diffusion of pollutants and increased the concentration of CO, SO2, NO, NO2, PM2.5 and PM10 in the aerosol-rich regions. The NO/NOratio generally increased and led to more ozone depletion. On the other hand, the boundary layer top acted as a barrier that trapped moisture at lower altitudes and reduced the moisture at higher altitudes (the specific humidity was reduced by 1.69 % at 1493 m on average in China). Due to reduced water vapour, fewer clouds were formed and more sunlight reached the surface, so the photochemical production of ozone increased. Under the combined effect of the two meteorology feedback methods, the annual average ozone concentration in China declined by 2.01 ppb (6.2 %), which was found to bring the model into closer agreement with surface ozone measurements from different parts of China.


AS25-A019
Spatiotemporal Variation of the Burned Area and its Relationship with Climatic Factors in Central Kazakhstan

Yongfang XU1#+, Zhaohui LIN2, Chenglai WU2
1National Meteorological Information Centre, China Meteorological Administration, China, 2Chinese Academy of Sciences, China

Central Asia is prone to wildfires, but the relationship between wildfires and climatic factors in this area is still not clear. In this study, the spatiotemporal variation in wildfire activities across Central Asia during 1997–2016 in terms of the burned area (BA) was investigated with Global Fire Emission Database version 4s (GFED4s). The relationship between BA and climatic factors in the region was also analyzed. The results reveal that more than 90% of the BA across Central Asia is located in Kazakhstan. The peak BA occurs from June to September, and remarkable interannual variation in wildfire activities occurs in western central Kazakhstan (WCKZ). At the interannual scale, the BA is negatively correlated with precipitation (correlation coefficient r = –0.66), soil moisture (r = –0.68), and relative humidity (r = –0.65), while it is positively correlated with the frequency of hot days (r = 0.37) during the burning season (from June to September). Composite analysis suggests that the years in which the BA is higher are generally associated with positive geopotential height anomalies at 500 hPa over the WCKZ region, which lead to the strengthening of the downdraft at 500 hPa and the weakening of westerlies at 850 hPa over the region. The weakened westerlies suppress the transport of water vapor from the Atlantic Ocean to the WCKZ region, resulting in decreased precipitation, soil moisture, and relative humidity in the lower atmosphere over the WCKZ region; these conditions promote an increase in BA throughout the region. Moreover, the westerly circulation index is positively correlated (r = 0.53) with precipitation anomalies and negatively correlated (r = –0.37) with BA anomalies in the WCKZ region during the burning season, which further underscores that wildfires associated with atmospheric circulation systems are becoming an increasingly important component of the relationship between climate and wildfire.


AS25-A021
Seasonal and Diurnal Variations of Carbon Dioxide and Energy Fluxes Over Three Land Cover Types of Nepal

Bharat JOSHI1#+, Yaoming MA2
1Kathmandu Centre for Research Education, CAS-TU, Nepal, 2Chinese Academy of Sciences, China

This study examines the seasonal and diurnal variations of carbon dioxide and energy fluxes over three land cover types of Nepal by using the eddy covariance method from March to November 2016. The surface energy balance closures were moderate with the values of about 56%, 61%, and 64% closure at Kirtipur, Simara, and Tarahara sites respectively. The monthly average values of net radiation flux and latent heat flux peaked in August at Kirtipur and Tarahara sites whereas in June at the Simara site respectively. The maximum monthly average measured sensible heat flux was 37 W m⁻², 43.6 W m⁻², and 36.3 W m⁻² in April for all the sites whereas soil heat flux was 5.1 W m⁻² and 2.9 W m⁻² in April for Kirtipur and Simara sites and 6.2 W m⁻² in June for the Tarahara site. The magnitude of diurnal peak of net ecosystem CO2 exchange (NEE) reached up to 11.04 μmol m⁻² s⁻¹ at Kirtipur, 15.04 μmol m⁻² s⁻¹ at Simara, and 10.44 μmol m⁻² s⁻¹ at Tarahara sites respectively. Among the three study sites, the ecosystem at the Kirtipur site was a good carbon source; the ecosystems at Simara and Tarahara sites were low and good carbon sink in the growing season. In addition, all three different land cover ecosystem were carbon source when accounted for the measurement period.


AS25-A022
A Study on the Spatial Difference of PM2.5 Concentration in Similar Synoptic Fields

DaEun CHAE1+, Soon-Hwan LEE1#, EunJi KIM2
1Pusan National University, Korea, South, 2Pusan University, Korea, South

In this study, we performed a synoptic analysis to investigate the reason for the spatial difference in PM2.5 concentration despite a similar synoptic pattern. Synoptic pressure patterns associated with high PM2.5 episodes (greater than 35 ㎍/㎥) were classified into three sub-groups related to high concentrations occurring only in Busan and Seoul metropolitan areas using K-means cluster analysis, based on the 900 hPa geopotential height of NCEP FNL data. Although the synoptic patterns of high PM2.5 episodes that occur independently in Busan and Seoul metropolitan areas were similar, there was a difference in the intensity of pressure gradient and its direction, which tends to be an important factor determining the movement time of pollutants. The spatial difference in PM2.5 concentration in the Korean Peninsula is due to the difference and direction of the atmospheric pressure gradient that develops from southwest to northeast direction.


AS25-A027
Environmental Impacts of Haze Pollution and Urbanization and Their Interactions Over the Beijing-Tianjin-Hebei City Cluster

Zilin WANG#+, Xin HUANG, Aijun DING
Nanjing University, China

With fast economic development, urban expansion and haze pollution are two main eco-environmental challenges confronting China. Though their individual impacts on urban climate and environment are investigated by multiple studies, the synthetic effect and intricate interaction of these two effects have not been fully understood. Here, based on in-situ measurements and numerical simulations at the densely populated and heavily polluted Beijing-Tianjin-Hebei (BTH) city cluster, the respective impact of aerosol and urbanization is quantitatively identified. Under polluted conditions, the aerosol radiative effect dominates with 3 oC cooling at ground surface and 1 oC warming in the upper boundary layer. In contrast, urban heat island (UHI) effect is more prominent during clean days, leading to over 1 oC warming in the lower atmosphere. Furthermore, aerosols are found to enhance UHI via confining the dispersion of anthropogenic heat and perturbing longwave radiation budget. Since the implement of China’s Clean Air Action in 2013, aerosol reduction contributes to a decreasing trend of both aerosol radiative effect and UHI intensity in BTH city cluster. The study highlights a comprehensive understanding of air pollution and urbanization as well as their interactions over megacities.


AS25-A029
The Global Environmental Measurement and Monitoring Initiative: Driving Global to Local Solutions

Mark SHIMAMOTO1#+, David LANG2, Daniel KLINGENBERG2, Janice LACHANCE1
1American Geophysical Union, United States, 2Optica, United States

The Global Environmental Measurement and Monitoring (GEMM) Initiative is an international project of Optica and the American Geophysical Union seeking to provide precise and usable environmental data for local impact. The Initiative brings together science, technology, and policy stakeholders to address critical environmental challenges and provide solutions to inform policy decisions on greenhouse gases (GHGs) and air and water quality. GEMM Centers are currently established in Scotland, Canada, New Zealand, and the United States. These Centers represent partnerships with leading institutions that are actively working toward developing or deploying new measurement technology and improved climate models. Additional Centers are under development in India and Australia with plans to expand to Asia and Africa. In addition to establishing monitoring centers worldwide, GEMM actively engages with other sectors (including industry, standards organizations, and regional or national governments) to support the incorporation or adoption of these evidence-based approaches into decision making processes. For example, Glasgow, Scotland is piloting the GEMM Urban Air Project, deploying a low-cost, real-time, ground-based network of devices that continuously monitors GHGs and air pollutants at a neighborhood scale. The sensor network in Glasgow is increasing the precision of local models that can provide the city with information to assess current policies and support future action. Here we will share the progress and outputs of the GEMM Initiative to date and highlight paths forward to grow the network.


AS26-A003
Influence of Tropical Atlantic Meridional Dipole of Sea Surface Temperature Anomalies on Antarctic Autumn Sea Ice

Xuya REN1+, Li ZHANG1#, Wenju CAI2,3, Xichen LI4, Chuan-Yang WANG1, Yishuai JIN1, Lixin WU1
1Ocean University of China, China, 2Ocean University of China and Qingdao National Laboratory for Marine Science and Technology, China, 3Commonwealth Scientific and Industrial Research Organisation, Australia, 4Chinese Academy of Sciences, China

Antarctic sea ice plays an important role in polar ecosystems and global climate, while its variability is affected by many factors. Teleconnections between the tropical and high latitudes have profound impacts on Antarctic climate changes through the stationary Rossby wave mechanism. Recent studies have connected long-term Antarctic sea ice changes to multidecadal variabilities of the tropical ocean, including the Atlantic Multidecadal Oscillation and the Interdecadal Pacific Oscillation. On interannual timescales, whether an impact exists from teleconnection of the tropical Atlantic is not clear. Here we find an impact of sea surface temperature (SST) variability of the tropical Atlantic meridional dipole mode on Antarctic sea ice that is most prominent in austral autumn. The meridional dipole SST anomalies in the tropical Atlantic force deep convection anomalies locally and over the tropical Pacific, generating stationary Rossby wave trains propagating eastward and poleward, which induce atmospheric circulation anomalies affecting sea ice. Specifically, convective anomalies over the equatorial Atlantic and Pacific are opposite-signed, accompanied by anomalous wave sources over the subtropical Southern Hemisphere. The planetary-scale atmospheric response has significant impacts on sea ice concentration anomalies in the Ross Sea, near the Antarctic Peninsula, and east of the Weddell Sea.


AS26-A009
The Delayed Impact of ENSO on Generation of the Amundsen Sea Low (ASL) Anomaly

Hyunju LEE#+, Emilia Kyung JIN
Korea Polar Research Institute, Korea, South

The El Niño-Southern Oscillation (ENSO) influences West Antarctica via atmospheric teleconnection, but it is delayed by one season because the Amundsen Sea Low (ASL) response to the ENSO has the strongest intensity in May. However, the mechanism related to the delay has not been fully discovered yet. This study investigates the formation mechanism of the ENSO-driven teleconnection in each month by examining the kinetic energy conversion (CK), total wavenumber, and wave activity flux. The perturbation induced by the ENSO gains energy from the basic state as the ENSO appears, however it does reach high latitudes only in May. Although the ENSO becomes weak in May, the developed subtropical jet makes waves to move further south, resulting in the strong ASL anomaly. Numerical experiments considering the decay of the ENSO forcing also show that the ENSO-related teleconnection is the strongest in May. The results demonstrate that the basic state is essential for the ENSO teleconnection to extend to West Antarctica.


AS29-A008
Study on the Movable Rain Belt in Lanyang Plain Under the Strong Northeast Monsoon

Jou-Ping HOU#+, Chih-Yi CHEN
National Defense University, Taiwan

In November 2020, Taiwan implemented a 5-day intensive observation experiment on the Lanyang Plain in the northeast, which we call the Yilan Experiment for Severe Rainfall (YESRain). The reason for this project is that according to the statistics of the Taiwan Central Meteorological Bureau over the years, when the northeast monsoon occurs, the Lanyang Plain often receives the most precipitation in Taiwan, and this precipitation is even higher than the Keelung area on the windward side.In order to analyze the reasons for the rainfall in the Lanyang Plain under the strong northeast monsoon, this study analyzed and simulated the moveable rain belt, rainfall time and rainfall intensity caused by the strong northeast monsoon on November 23, 2020. In addition, various observation tools such as laser wind profiler are used to analyze the relationship between the wind field and the rain belt after the interaction between the bell mouth terrain in Yilan area and the wind field at different heights, and to verify each other with the WRF numerical simulation results. It was found that the northeastern part of Taiwan was affected by the strong northeast monsoon on the 23rd, and the severe rainfall in the Yilan area not only appeared on the south windward side, but also occurred in the Lanyang Plain and the outer sea. The precipitation distribution is highly related to the direction and speed of the wind field, while The surface flux has a considerable contribution to the severe rainfall in Yilan.


AS29-A012
The Spatial and Temporal Character Analysis of Complex Terrain Rainfall in Northeastern Taiwan with Northeasterly Condition in 1961-2020

Chin-Hsiang WU, Wen-Wei TSENG, Shih-Hao SU#+
Chinese Culture University, Taiwan

There are typical spatial rainfall patterns in the northeast Taiwan area (Yi-Lan) under the northeasterly in wintertime. Such rainfall features are related to the interaction of large-scale background mean flow and complex topography. According to the climatology of rainfall, most precipitation hot spots occur on the windward side of the terrain and decrease toward the plain area. However, the difference in large-scale environmental conditions can lead the variations in spatial rainfall characteristics. By analyzing the gridded rainfall data in the Yilan area in the past 60 years, we noticed that the average rainfall has an increasing trend. The increasing trend was more significant in the southern mountain region on the windward side. The rainfall increase in winter was more extensive than in autumn and spread to the plains in coastal areas. We have also noticed that there will still be heavy rain (HR, >80mm/day) events in the Yilan area in autumn and winter when Taiwan has less rainfall. The probability of HR events has increased significantly in the past 30 years, and HR events also occurred in plain areas. On the other hand, although the probability of occurrence was low, there still were torrential rain (TR, >200mm/day) events in the mountainous areas of Yilan. The frequency and extent of occurrence of these types of extreme rainfall events have significantly increased during 2016-2020 compared with 1961-2015. According to the reanalysis data, the background large-scale circulation field has also changed in the past 60 years. The change in the background circulation led to changes in the frequency of occurrence and hot-spot locations of convection initiation, which also caused variations in the spatial distribution of rainfall.


AS29-A013
Characteristics of Mountain-wave Occurrence in the Taebaek Mountain Range Based on GK-2A

Dabin YEOM+, Jinyeong KIM, Myoung Hwan AHN#
Ewha Womans University, Korea, South

Mountain-waves, also known as Lee wave, can generate strong rotational forces or up and down air currents that can affect aircraft operations. If mountain-wave clouds exist during the calculation of atmospheric motion vectors using satellite data, the vector may become inaccurate. Therefore, it is important to analyze the atmospheric flow characteristics and generation mechanisms of mountain-wave formation. In this study, we present a satellite-based characteristics of mountain-wave events in the Taebaek Mountain range in Gangwon-do, Korea. Our analysis was based on detailed visual inspection of infrared satellite imagery in the ch13 (10.5㎛) of the GK-2A satellite during 2020-2022. Two analysts independently inspecting the same satellite images using visual inspection methods, and cross-verifying the results. If there are enough moisture in the incoming airstream, mountain-wave clouds are generated parallel to the mountain range from the ridge of mountain-wave that have the characteristics of normal waves. Therefore, we detected clouds whose positions did not change over time and observed the duration of their occurrence. Previous research used visible satellite imagery in 15-min intervals during daylight hours. This had limitations as it could not identify mountain-wave cloud that occurred or lasted at nighttime hours and the 15-min interval was too long to detect the exact duration. But, using the infrared imagery from the GK-2A satellite with 2-min intervals, we were able to overcome these limitations and achieve more accurate observations. The maximum number of mountain-wave events occurred in winter season, with the largest number in February. Conversely, the minimum number of mountain-wave events occurred in summer season, with the fewest number in July. The average duration of mountain-wave events was longest in October and shortest in June. The maximum duration is 2268-min, while the minimum is 48-min.


AS29-A018
Numerical Simulation of Boundary Layer Characteristics in the Taipei Basin and Yilan Region Under Northeast Monsoon Conditions

Pei-Di JENG#+, Jou-Ping HOU
National Defense University, Taiwan

As the latitude of the continental cold high-pressure center was higher and gradually moves eastward to the sea, the environmental wind field in northern Taiwan was mostly northeasterly or easterly winds introduced by continental high-pressure peripheral circulation. Though the distance between the Taipei Basin and the Yilan of northern Taiwan were closed, the local wind fields were quite different. In order to understand the relationship between the environmental wind field (northeast monsoon), local circulation, and complex terrain effects, this study applied the Weather Research and Forecasting Model, simulating the change of local circulation in the Taipei Basin and Yilan under the northeast monsoon on October 25 and November 26, 2022.It was found that when the wind field in the Taipei Basin is weak northeasterly, local circulation will be generated after noon due to the influence of the terrain, and the wind field will gradually change to easterly or southeasterly easterly. With such airflow characteristics, and the weather tended to be stable. When the wind field of the same environment passed through the Lanyang Plain, it was affected by the terrain effect, and the area where the wind field convergence zone was formed in the Lanyang Plain has Nimbostratus and indirect precipitation. In addition, a northwest-southeast trending wind direction convergence zone was formed in the vicinity of Sansing. As the terrain blocking and local circulation became more obvious, the wind direction gradually turned to westerly and went out to ocean. When the northeast monsoon was strong, the large-scale ambient wind field would directly change the boundary layer structure of the Taipei Basin and the Lanyang Plain. However, under the same northeast monsoon environment, there would still be obvious differences in the boundary layer wind field characteristics between the Taipei Basin and the Lanyang Plain.


AS29-A021
Preliminary Analysis of the Autumntime Heavy Rainfall Event Over Northeastern Taiwan Related to the Typhoon Nesat and Northeasterly Wind

Siang-Yu ZHAN#+, Pay-Liam LIN, Chen-Hau LAN
National Central University, Taiwan

The rain gauges over Yilan observed the heavy rainfall during 15 Oct 2022 to 17 Oct 2022 with maximum accumulated rainfall is 972.5 mm within 40 hours. During 14 Oct 2022 to 18 Oct 2022, typhoon Nesat carrying abundant moisture moved westward, passing through the sea south of Taiwan. After Nesat moved into South China Sea, the northeasterly wind enhanced. In this case, the maximum moisture flux exceeded 300 g kg-1 m s-1 near 950-hPa level. Typhoon Nesat provided abundant moisture when it was on southeast and south of Taiwan. The northeasterly wind played an important role in moisture transport after Nesat passed by Taiwan. The wind profile radar at Dongshan observed that during 1600 UTC 15 Oct to 0800 UTC 16 Oct, the low-level wind over Yilan was consistent easterly wind with the maximum wind speed ~20 m s-1. After 2000 UTC 16 Oct, the northeasterly wind advanced into Yilan, and the thickness of northeasterly wind was ~3 km. The maximum wind speed of northeasterly wind was near 1 km height, and the wind speed exceeded 20 m s-1. After 1600 UTC 17 Oct, the northeasterly wind weakened, and the westerly winds were present in the planetary boundary layer. In this case, the characteristics of drop size distribution over southern Yilan plain showed two different types. One was affect by typhoon circulation mainly (during 1200 UTC 15 Oct to 1200 UTC 16 Oct), the rain rate was stronger with larger diameter (Dm) and smaller number concentration (Nw). The other type was under northeasterly wind, and the rain rate was smaller with smaller Dm and larger Nw.


AS29-A022
Statistical Characteristics of Sounding-derived Parameters of Mesoscale Convective Systems Over South Korea

Si-Hyeon SON1+, Kwonil KIM2, Kyuhee SHIN1, Gyu Won LEE1#
1Kyungpook National University, Korea, South, 2Stony Brook University, United States

The heavy rainfall caused by Mesoscale Convective Systems (MCS) has been increasing recently. As a result, there is a growing emphasis on studying MCS. The formation and development of MCS are associated with the thermodynamic and dynamical environment, which has been mostly investigated using a numerical model. There have been limited attempts to utilize in situ rawinsonde measurements, which provide an accurate and high-resolution thermodynamic and dynamic profile, to characterize the MCS over South Korea. In this study, the sounding-derived parameters of the MCS occurring on the Korean Peninsula were presented using the data obtained 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). The results show that CC was generated by thermal instability and had the largest convective potential available energy at 470.8 m2 s-2. The total Richardson number had 27.0, exhibiting a distinctly large value compared to other types, but mechanical instability was the smallest in the MCS types. MCC had a considerable convective inhibitory energy of 174.5 m2 s-2 and a large low-layer shear of 7.8 m s-1. SLD and SLP had a large vertical wind shear, with mechanical instability contributing to formation and development. Sounding-derived parameters during the formation, development, and extinction cycles of MCS suggested that the thermodynamic values gradually increased until they reached their highest values at the peak of convective system development, followed by decreasing trend during the dissipating stage. This study will present the favorable environmental condition for each MCS type to identify the key parameters in determining the MCS type and the development stage.

ACKNOWLEDGEMENT
This work was supported by the National Research Foundation of Korea grant funded by the Korea government (MSIT) (No. 2021R1A4A1032646).


AS29-A024
Radar-based Precipitation Growth and Decay Patterns During the Summer Season in South Korea

Kwonil KIM1+, Chia-Lun TSAI2, Gyu Won LEE3#
1Stony Brook University, United States, 2Chinese Culture University, Taiwan, 3Kyungpook National University, Korea, South

Improving the predictability of precipitation requires a comprehensive understanding of precipitation growth and decay (GD). Investigating the precipitation GD has mostly relied on the Eulerian approach, which examines the physical characteristics in a fixed coordinate. On the other hand, Lagrangian approach follows the precipitation system motion and enables capturing its temporal evolution. This study quantitatively retrieves radar-based GD of precipitation in South Korea in a framework of semi-Lagrangian advection. This study is followed by the investigation of the dependence of GD on the following factors: flow direction, flow speed, and relative geographical location to the topography and land–ocean boundary. The results indicate that the flow direction determines the spatial distribution of GD. The growth generally tends to occur on the windward side of the mountain range and vice versa on the lee side. The flow speed affects the intensity of GD. The study further explores the diurnal variability of the GD. Under the strong orographic forcing on the diurnal variation, unique geographical features of South Korea created interesting diurnal patterns near Seoul by land–ocean breeze circulation and on the windward side of the mountain ranges (inland) by solar heating. The GD in South Korea shows two diurnal peaks of growth: the early morning peak over the ocean and the afternoon peak in the land areas. In addition, the GD in South Korea exhibits a monthly variation with the most intense growth occurring in August.

ACKNOWLEDGMENT
This work was supported by the National Research Foundation of Korea (NRF) grant funded by the Korea government (MSIT) (No. 2021R1A4A1032646).


AS29-A025
Snow Cover Change in Mountain Regions

Manuel Tobias BLAU1,2#+, Pratik KAD2, Kyung-Ja HA2
1IBS Center for Climate Physics, Korea, South, 2Pusan National University, Korea, South

The mountains have been getting warmer in recent years. Special interest was put on mountain snow cover change as their environment was accounted to the cooler alpine climate zone. Snow cover is expected to reduce in response to global warming and is most evident in mountainous regions. Using available reanalysis and observation data, a decline in snow cover and snow depth was detected over the last 43 years. Our study considers the relationship between global warming and changes in snow persistence. We found that the mean global warming rate is higher than mountain warming. In addition, polar amplification and global warming do not play a significant role in snow cover changes on individual snow persistence mountains. However, local processes can influence snow cover, and long-term changes in these radiation budgets are significant drivers of the changes being observed. We conclude that regional radiation imbalance is a major contributor to the decline in snow cover. The results reveal new insights into the course of snow cover changes and their implication on the mountain climate. Understanding the impact of changing snow cover patterns is critical for informing sustainable development and preparing for the potential consequences of these changes.


AS30-A008
Analysis of Phase Change in Solid Precipitation in the Yeongdong Region of Korea: Episode Analysis of Ice Pellet and Graupel

Ji Yun KIM1+, Younggil CHOI1, Han JINHEON1, Kim TAE YEON1, Byung-Gon KIM1#, Kwonil KIM2, Gyu Won LEE3
1Gangneung-Wonju National University, Korea, South, 2Stony Brook University, United States, 3Kyungpook National University, Korea, South

The Yeongdong region (the eastern mountainous region of Korea) is frequently vulnerable to heavy snowfall. By virtue of a lot of previous efforts on the snowfall study, snowfall forecast has been significantly improved, but the phase change of solid precipitation is still hard to predict since its time scale is very short (a couple of hours) and spatial dimension is very limited, which is largely attributable to Taeback mountains and East Sea effect. For instance, two ice pellet (IP) episode (1 March 2021 & 14 March 2018) occurred along with a rapid cooling by strong cold advection during the transition period of winter to spring, when a reversed S profile of temperature was identified in both rawinsonde soundings and model reanalysis. Another episode of phase change was observed on 19 March 2022 when dramatic change of precipitation occurred in the process of rain to snow. Precipitation started on 17 March in the rain phase and persisted 3 days when the Low-pressure system passed over the Korean peninsula. Phase changed from rain to aggregate of dendrites in the morning of 19 March, and melting snow and graupel around noon in the condition of low-level cooling together with surface warming explained by thermodynamic soundings. Later, the habit of snow crystal returned to aggregates. The dramatic change of phase and habit occurred within several hours, which was observed by multi-angle snowflake camera and PARSIVEL together. The results emphasize that cold air intrusion with barrier wind plays an important role in phase change of solid precipitation such as ice pellet (or freezing rain) with a help of cold air blocking by the mountains during the transition period of winter to spring. It is necessary to examine other phase change episodes, and to understand the various roles of cold air advection along the mountains in precipitation.


AS30-A009
Observed Kinematics and Microphysics of Orographic Precipitation Associated with a Landfalling Typhoon Rainband

Tsubaki HOSOKAWA#+, Cheng-Ku YU
National Taiwan University, Taiwan

This study used Doppler radar observations, a dense rain gauge network, and disdrometers to investigate the kinematic and microphysical characteristics of orographic precipitation over Da-Tun (DT) Mountain of northern Taiwan associated with an outer rainband of Typhoon Chanthu (2021). The outer rainband, located about 100 km from the typhoon center, approached and made landfall on DT and brought a maximum rainfall of 57 mm h-1 at 0600 UTC on 12 September. A significant precipitation enhancement of 25 mm h-1 over DT was confirmed as compared to rain gauge observations over coastal and plain areas. The rainband was characterized by a broad area of strong reflectivities (> 40 dBZ) with a vertically extending feature, and its echo patterns were less organized with weak bright-band signatures. The upward motions (~1.5 m s-1) and near-zero vertical motions existed at mid-levels and lower levels, respectively. The low-level horizontal winds impinging on the DT barrier intensified with time and could reach about 20 m s-1, causing upslope lifting (~2.0 m s-1) and a corresponding local reflectivity maximum over mountain slopes. Averaged polarimetric vertical profiles calculated over the DT area indicated a significant increase in ZHH, ZDR, and KDP toward the ground below 3 km MSL, implying that the microphysical process contributing to the rainfall enhancement was primarily related to the collision-coalescence. These results were also supported by disdrometer observations, showing an increase in mass-weighted mean diameter and liquid water content during the passage of the rainband. In addition, as evident from the drop-size distribution (DSD) analysis, the observed heavy rainfall was mostly due to the presence of a numerous number concentration of midsize drops. This study demonstrated the important roles of orographic effects in modulating kinematic and microphysical characteristics and contributing to the heavy precipitation over DT.


AS30-A021
Assessment of Wind and PM2.5 Prediction with Lidar Data Assimilation in Taiwan

Fang-Yi CHENG#+, Cheng-Pei YANG, Shu-Chih YANG, Sheng-Hsiang WANG, Chia-Hua HSU, Lian-Jie WANG
National Central University, Taiwan

A lidar data assimilation system was developed based on the Weather Research and Forecasting-Local Ensemble Transform Kalman Filter (WRF-LETKF) framework coupled with the Community Multiscale Air Quality (CMAQ) model. The objective was to investigate the impact of lidar data assimilation on PBL prediction and the subsequent influence on PM2.5 prediction for a high-air-pollution event. The fine particulate matter (PM2.5) profiles retrieved from two micropulse lidar observations were assimilated in the WRF-LETKF system. Three numerical experiments, BASE (with a nudging strategy), CTRL (with an ensemble framework), and LDA (with assimilation of lidar-retrieved PM2.5 profiles), were conducted for a high-air-pollution episode. The BASE simulation overestimates the wind speed, leading to PM2.5 underestimation. The CTRL and LDA simulations can improve the wind fields and enhance the PM2.5 accumulation. With a strong error correlation between the lidar-retrieved PM2.5 concentration and the wind fields, the LDA simulation effectively corrects the wind flow from the surface to the PBL top, further adjusting the PM2.5 transport processes.


AS30-A022
Evaluation of Precipitation Type Based on Spectral Bin Model and LDAPS

Wonbae BANG1+, Kwonil KIM2, Carlin JACOB3,4, Alexander RYZHKOV3,4, Sanghun LIM1, Gyu Won LEE1#
1Kyungpook National University, Korea, South, 2Stony Brook University, United States, 3NOAA Oceanic and Atmospheric Research, United States, 4NOAA National Severe Storms Laboratory, United States

The Spectral Bin Model (SBM) is a 1-dimensional microphysics model that includes various thermodynamic processes such as melting, freezing, evaporation, and sublimation. The SBM determines precipitation type (PT) based on the simulated rainfall rate (RR), snowfall rate (SR), and input environmental profile. When the sounding observation is used as the input environmental profile, it has been shown that the PT produced by the SBM have relatively higher accuracy compared to different traditional prediction methods. The sounding, however, suffers from limited spatiotemporal resolution. The question that arises is whether the high-resolution thermodynamic fields of the operational numerical weather prediction model yield satisfactory results in determining the spatial distribution of PT. Local Data Assimilation and Prediction System (LDAPS) has been developed by the Korean Meteorological Administration (KMA) and has meteorological variables (Temperature [T], Relative humidity [RH], Pressure [P]) with a 1.5 km horizontal resolution and 70-71 layers. Prior to the joint utilization of SBM and LDAPS, we need to understand the impacts of errors in LDAPS on the performance of the SBM. The T, RH, and wet-bulb T (Tw) profiles of LDAPS will be compared with those of the sounding. Additionally, we will compare the accuracy of PT produced by the SBM when the input is either sounding or LDAPS.

Acknowledgment
This work was supported by the National Research Foundation of Korea (NRF) grant funded by the Korea government (MSIT) (No. 2021R1A4A1032646). This work was funded by the Korea Meteorological Administration Research and Development Program under Grant KMI2022-00310.


AS30-A023
The Study of Overall Physical Characteristics for Precipitation Types Using Observation Datasets

Choeng-Lyong LEE1+, Wonbae BANG1, Chia-Lun TSAI2, Ji-Hye JUNG1, Gyu Won LEE1#
1Kyungpook National University, Korea, South, 2Chinese Culture University, Taiwan

Different rainfall systems such as stratiform and convection evolve in different developing mechanisms. The characteristics study of precipitation types are important in order to understand their differences in terms of physical, dynamic, thermodynamical and micro-physical processes. Therefore, we investigated the whole properties of various rainfall systems after identifying precipitation types using newly developed classification algorithm. Categorization of precipitation types is performed using the combined algorithms composed of 1) the SL3D (storm labeling in three dimensions) and 2) classification algorithm based on feature parameters. The feature parameters are derived from VIL (vertical integrated liquid water contents) and mean reflectivity. The precipitation types are divided into 8 categories (precipitation stratiform, non-precipitation stratiform, convection, updraft, deep system, shallow system, low cloud and anvil). The vertical structures of different precipitation types are explored to compare the physical (dynamic) peculiarities using dual-polarization radar observation (WISSDOM attributes). In the addition, the generalized microphysical parameters (N0’, Dm) and the latent heat (LH) acquired directly from GPM product are also investigate to analyze the microphysical and thermodynamical characteristics respectively. The N0’ and Dm are obtained using polynomial regressions consisting of ZDR and reflectivity. The bright band appeared at 4.5~5.5 km altitude in stratiform and deep system as shown in the vertical profiles of reflectivity and ZDR. The convergence (divergence) patterns, one of WISSDOM attributes, are distinctive in lower (higher) atmospheric layers for convection and updraft regions. Both Dm and log (N0’) of updraft are relatively higher than those of stratiform. Similar to several previous studies, the mean LH profile of convection is higher than one of stratiform at all heights. 

Acknowledgment: This work was supported by the National Research Foundation of Korea (NRF) grant funded by the Korea government (MSIT) (No. 2021R1A4A1032646).


AS32-A003
Relationship Between Strength of the Walker Circulation and Dominant Equatorial Waves

Ryoko ARAI1#+, Tamaki SUEMATSU2, Tsubasa KOHYAMA1
1Ochanomizu University, Japan, 2RIKEN, Japan

The Walker circulation is the most prominent tropical zonal circulation on a planetary scale, which is influenced by sea Surface temperature fluctuations at a time scale longer than the intraseasonal time scale. Previous studies have theoretically suggested that equatorial waves accelerate or decelerate the large-scale zonal flow of the upper troposphere in the tropics. Therefore, this study investigates the relationship between the Walker circulation and equatorial waves to clarify which equatorial waves are dominant depending on the strength of the Walker circulation. By sorting the strength of the downward branch of the Walker Circulation above the western Indian Ocean, we make composite maps of outgoing longwave radiation. The results imply that prominent equatorial waves vary depending upon the seasonality. In boreal winter when the Walker circulation is strong, some signals presumably associated with mixed Rossby-gravity waves are hinted, whereas in boreal spring when the Walker circulation is weak, Kelvin wave-like features are exhibited. Interannual variability of the aforementioned relationship will also be discussed.


AS32-A006
Contrasting the Convective Energy Recharge-discharge Cycle Between Propagating and Eastward-decaying Madden-Julian Oscillation Events

Jia-Yuh YU#, Yu-Cian TSAI+
National Central University, Taiwan

In this study, we contrast the distinct energy recharge-discharge cycle between propagating and eastward-decaying Madden-Julian Oscillation (MJO) events during the boreal winter season (November – April) from 1979 to 2018 using the moist static energy (MSE) budget and gross moist stability (GMS) plane analyses. A total of 41 MJO events are selected during the 40-year period, including 16 strong propagating (SP), 13 weak propagating (WP) and 12 eastward-decaying (ED) types of MJOs. The column-integrated MSE budget shows that, depending on the phases, vertical and horizontal advection terms take turns leading the role in discharging or recharging the MSE. In the phase when the net flux heating reaches the maximum, vertical advection plays the lead role in discharging the MSE. In the subsequent phases when the net flux heating gradually weakens, horizontal advection becomes the dominant factor in discharging the MSE. A similar situation occurs during the recharge phases to balance the net flux cooling. The SP MJO exhibits a stronger energy recharge-discharge cycle compared to the WP and ED MJOs, and the contrast significantly enlarges from the Indian Ocean to the Maritime Continent. The GMS plane analysis further reveals that four different types of convection attribute to the recharge-discharge process. During the wet phases, the top-heavy ascending motion and negative shallow convection jointly stabilize the atmosphere by exporting the MSE; while during the dry phases, the top-heavy descending motion and the positive shallow convection together destabilize the atmosphere through importing the MSE. Moreover, the recharge (discharge) phase leads the amplifying (decaying) phase by a quarter cycle is essential to maintain a robust energy recharge-discharge cycle to drive the eastward propagating MJOs.


AS32-A008
Machine Learning Parameterization of the Multi-scale Kain-Fritsch (MSKF) Convection Scheme in Grey-zone

Xing YU1+, Xiaohui ZHONG2#
1Shenzhen Institute of Artificial Intelligence and Robotics for Society, China, 2Fudan University, China

Numerical weather prediction (NWP) models are running at finer grid spacings from 1 to 10 km with increasing computational resources. However, as the grid spacing becomes comparable to the length scales of convection, known as the grey zone, the turbulent eddies in the atmospheric boundary layer are partially resolved and parameterized. Whether a convection parameterization (CP) should be used in the grey zone remains controversial. Scale-aware CP schemes are designed to improve the representation of convective transport within the grey zone. For example, the multi-scale Kain-Fritsch (MSKF) scheme introduces modifications, such as tuning convective adjustment time scale and adding linear mixing of updraft vertical velocity with grid-scale vertical velocity so that it can be implemented successfully at grid resolution as high as 2 km. However, the scale awareness is empirical and, to some extent, remains tunable. In recent years, more and more machine learning (ML) models have been applied to different domains of atmospheric sciences, including using ML models as substitutions for physical parameterizations. In this work, we proposed to use bidirectional long short-term memory (Bi-LSTM) models to replace the scale-aware MSKF CP scheme. The Weather Research and Forecast (WRF) model is used to generate training and testing data over South China at a horizontal resolution of 4 km. Torrential rainfall often occurs along the coast of South China, with the background of a frontal rain band over northern South China or the Yangtze River basin. It is called warm sector heavy rainfall and is usually associated with convective, localized, torrential, and long-lasting; thus is challenging to predict. In addition, the Bi-LSTM based CP scheme is coupled with the WRF model. The preliminary results demonstrate that the Bi-LSTM model is able to achieve good accuracy, showing the potential substitution of the MSKF scheme by ML models in grey zone.


AS32-A009
Surface Thermodynamic Gradients and ITCZ Properties in Idealised Simulations Over an Aquapatch

Maxime COLIN#+, Jan O. HAERTER
Leibniz Centre for Tropical Marine Research, Germany

Monsoons are often considered as ITCZ migrations into the land. Monsoon theories also consider the main control on precipitation properties to be the moist static energy near the surface. This study attempts to further clarify the role of surface thermodynamic gradients in determining precipitation outcome.
We run a series of idealised ITCZ simulations at 30-km grid spacing with the WRF model, in an aquapatch domain from 63S to 63N. The model is forced by a meridional contrast of surface temperature, with comprehensive physics, rotation, and symmetric boundary conditions at the North and South boundaries.
Summer solstice equilibrium simulations capture the main general circulation features and the main spatial organisation of convection. Turning on or off the convective parameterization does not impact the mean precipitation latitudinal distribution, but it does impact the eddies at smaller spatiotemporal scales, which shows a non-negligible but limited influence of convection on the summer ITCZ properties. By varying the forcing, we show that monsoon intensity follows a highly non-linear (logarithmic) relationship with surface temperature gradient, and that a finite temperature contrast is necessary to generate any cross-equatorial flow.
Simulations with an additional seasonal cycle forcing capture the abrupt and delayed monsoon onset. We also compare seasonal cycle simulations over ocean and over an idealised land to tell apart the influence of land in the delayed ITCZ migration.


AS33-A002
Real-time, Online Monitoring of Ammonia and Greenhouse Gas Emissions in Livestock with Cavity Ring-down Spectroscopy

Jinshu YAN1#+, Thomas GOTTSCHALK1, Xiaojing ZHANG2, Ryan QIN3, Magdalena E. G. HOFMANN1
1Picarro Incorporated, United States, 2Picarro Incorporated, China, 3No organization, China

Agricultural activities and processes emit greenhouse gases like CO2, CH4 and N2O, as well as NH3. While greenhouse gas emissions affect the global climate, ammonia can be a toxic pollutant to human health and biosphere environments. To reduce the impact of livestock production and fertilizer on the environment, it is vital to quantify greenhouse gases as well as ammonia emissions. However, accurate monitoring of NH3 emissions from barns, livestock, fertilization, and industry can be challenging at low levels (ppb to ppm) due to the high reactivity of ammonia and its tendency to adsorb to surfaces. Here, we present the new Picarro G2509 Cavity Ring-Down Spectroscopy (CRDS) analyzer that is optimized for continuous measurement of ammonia, while also reporting concentrations of greenhouse gases CO2, CH4 and N2O. The measurement response time of NH3 is sped up with low-reactivity internal materials and a high flow rate. The CH4 concentration range of the analyzer has been extended to 800 ppm to account for large variations in barns. The G2509 analyzer adapts the excellence of the G2508 that is commonly used to study greenhouse gas fluxes from soils by implementing key design of the G2103 analyzer which is dedicated to low level ammonia monitoring at air quality stations. Researchers studied ammonia production from livestock in cattle barns using G2103, and G2509 has been proved to be optimized for ammonia abatement measurement at dairy barns. Methane and nitrous oxide emissions have great influence on crops production and impacts of temperature and moisture on carbon and nitrogen cycling has been investigated by G2508. The effect of nitrogen and carbon modification on soil and plants has also been widely studied among Asia regions. Therefore, it is worthwhile to understand the emissions, transport, fate, and impact of greenhouse gas and ammonia pollutants via continuous gas monitoring techniques.


AS33-A004
Establishment of National Soil Nitrous Acid Emissions Network in China: Parameterization and its Application in Model

Yanan WANG1#+, Xiao FU2, Tao WANG1
1The Hong Kong Polytechnic University, Hong Kong SAR, 2Tsinghua University, China

Nitrous acid (HONO) is a key precursor of the highly reactive hydroxyl radical (OH). OH is a major oxidant to remove many gases emitted into the atmosphere and produces secondary air pollutants. Previous studies have revealed that the HONO emitted from soil is an important source of atmospheric HONO. As an agricultural country with a huge amount of fertilizer application, the effects of N fertilizers on HONO emissions have not been studied. In addition to HONO emissions introduced by fertilizers, emissions from unfertilized soils also accounted for a large part of total soil emissions due to their long duration. However, there has been limited research to quantify the HONO emissions for different soil types, thus lacking corresponding parameterization schemes to assess their impact on air quality. Here, we measured background (unfertilized) HONO and NO emission fluxes of soil samples collected from diverse soil types across China, and observed post-fertilization soil HONO emissions after applying three common fertilizers. The results show much higher emissions of HONO than those of NO, especially for samples from northern China. In terms of the fertilization effects, high HONO emissions from soils at 75%–95% WHC were founded, which contrasts with previous lower predictions at high soil moisture. Based on the results of laboratory experiments, the parameterization schemes for HONO emissions from fertilized and unfertilized soils were developed and implemented in a chemistry transport model. The inclusion of the soil HONO emissions improved simulations of atmospheric HONO and revealed a significant impact of this HONO source on air quality.


AS33-A005
Wet Deposition and Long Range Transport of Total Nitrogen and Total Organic Carbon at Two Sites in Mithila Region of Bihar (India)

Akanksha ROY+, U.C. KULSHRESTHA#
Jawaharlal Nehru University, India

Wet deposition of reactive nitrogen in the form of NH4+ and NO3- has become a major concern for scientists. The excess amount of such nitrogen species poses a threat to the environment and human health. NH3 and NO3- which primarily represent a major fraction of Total Nitrogen (TN) are contributed from the emissions from transport, agricultural and industrial sectors. N containing fertilisers, N fixation and livestock are the major sources of NH3 in the atmosphere while vehicular emissions and biomass burning contribute NO2 and further NO3in the atmosphere. This study reports the measurements of Total Nitrogen (TN), Dissolved Organic Carbon (DOC) and Inorganic Carbon (IC) in the wet deposition at a sub-urban site (Saharsa) and a rural site (Purnia) during July 2018 - September 2019 in the Mithila region of highly enriched alluvial plains of Bihar. Total 63 samples were collected from Saharsa and 29 samples were collected from Purnia using a polypropylene bottle-fennel assembly placed at a height of 20m from the surface of ground. The concentration of TN was determined by using Shimadzu TOC-TN analyser (Shimadzu model-TOC-LCPH E200 ROHS) The volume weighted mean of TN was comparatively high at the sub-urban site (1.72 mg/L) than the rural site (1.32mg/L) suggesting a greater contribution of NOx and NH3 at the sub-urban site. The annual wet deposition fluxes of TN were calculated as 13.45 kg N ha−1 yr−1 at the sub-urban site and 5.73 kg N ha−1 yr−1 at the rural site. The airmass trajectory analysis carried out using NOAA data suggested that part from local sources, both the sites also had an influence of trans-boundary and long-range transport of air pollution. Keywords: Reactive Nitrogen, Total N, Wet deposition flux, Airmass trajectory.


AS34-A002
The Characteristics of the Equatorial Waves Caused a Record Torrential Rain Event Over Sumatra Island

Pei-Ming WU1#+, Yoshiki FUKUTOMI2, Kazuyoshi KIKUCHI3
1Japan Agency for Marine-Earth Science and Technology, Japan, 2Nagoya University, Japan, 3University of Hawaii at Manoa, United States

This study examined the cause of a record torrential rain event over the western coast of Sumatra Island in March 2016. The influence of atmospheric equatorial waves (EWs) and the characteristics of the EWs were investigated. Analysis of the Japanese 55-year Reanalysis data (JRA-55) and precipitation data from the Global Precipitation Measurement (GPM) satellite showed that the event was caused by the combined effects of Kelvin waves, equatorial Rossby waves, and westward inertio-gravity (WIG) waves. An examination of the characteristics of the EWs revealed that the Kelvin waves had longitudinal scales of ~6,000 km, with a period of ~6 days and phase speed of ~12 m s-1, which was typical of the convectively coupled Kelvin waves in this region. The WIG waves had a scale of ~2,500 km, with a period of 2.5 days and a relatively fast phase speed of 12~13 m s-1. Heavy precipitation occurred when an eastward Kelvin wave from the Indian Ocean encountered a westward inertio-gravity (WIG) over Sumatra Island. It was concluded that along with the Kelvin and equatorial Rossby waves, the WIG waves might have played a major role in the formation of the extreme precipitation event.


AS34-A006
Indian Ocean Dipole Variations During the Last Millennium in PMIP3 Simulations

Charan Teja TEJAVATH1#+, Karumuri ASHOK2, Supriyo CHAKRABORTY3, Sreenivas PENTAKOTA2
1National Center for Earth Science Studies, India, 2University of Hyderabad, India, 3Indian Institute of Tropical Meteorology, India

Proxy-observational studies, and a sole model study, suggest that the Indian Ocean Dipole (IOD), an important global climate driver, exhibited multi-scale temporal variability during the Last Millennium (LM; CE 0851-1849, with relatively high number of strong positive IOD events during the Little Ice Age (LIA; CE 1550-1749), and strong negative IOD events during the Medieval Warm Period (MWP; CE 1000-1199). Using nine model simulations from the PMIP3, we study the IOD variability during the Last Millennium after due validation of the simulated current day (CE 1850-2005) IOD variability. Majority of the models simulate relatively higher number of positive IOD events during the MWP, and negative IOD events in the LIA, commensurate with simulated background conditions. However, higher number of strong positive IOD events are simulated relative to the negative IODs during the LIA, in agreement with proxy-observations, apparently owing to increased coupled feedback during positive IODs.


AS35-A011
A Regime-based Investigation Into the Errors of CMIP6 Simulated Cloud Radiative Effects Using Satellite Observations

Hao MIAO1#+, Xiaocong WANG2, Yimin LIU2, Guoxiong WU2
1Nanjing Joint Institute for Atmospheric Sciences, China, 2Chinese Academy of Sciences, China

Using a variety of CloudSat/CALIPSO products, this study synergistically examines the performance of clouds and their radiative effects (CRE) for models participating in CMIP6. Results show virtually all models overestimate the net cooling effect of clouds, which is caused by the overestimation of shortwave CRE and the underestimation of longwave CRE. By dividing clouds into regimes jointly sorted by cloud water path and cloud cover, we found models commonly underestimate the relative frequency of occurrence (RFO) for clouds that are geometrically thick, and the bias of RFO is dominant over that of within-regime CRE in an error decomposition of total CRE. This results in underestimations of CRE in geometrically thick clouds, which are partially offset by overestimations in the remaining cloud regimes, leading to the globally averaged CRE being less biased. The consideration of regime-based CRE gives important information that could be used for correction of cloud parameterization in models.


AS35-A014
Exploring Aerosol-cloud Interactions Over Eastern China and its Adjacent Ocean Using the WRF-SBM-MOSAIC Model

Jianqi ZHAO1+, Xiaoyan MA1#, Johannes QUAAS2, Hailing JIA2
1Nanjing University of Information Science & Technology, China, 2Leipzig University, Germany

This study aims to explore aerosol-cloud interaction over eastern China (EC) and its adjacent ocean (ECO) in boreal winter by coupling of a spectral-bin cloud microphysics (SBM) and an online aerosol module (MOSAIC) in WRF-Chem, with the support of four-dimensional data assimilation. The evaluation shows that assimilation has an overall positive impact on the simulation, and the coupling system reproduces the satellite-retrieved cloud parameters while exhibiting significantly improved simulation ability compared to the original SBM scheme as well as the bulk microphysical and MOSAIC coupling system. Differences in aerosol composition and physical processes lead to clear discrepancies in the aerosol-cloud interactions of EC and ECO during the simulation period. In EC with the gradual increase of aerosol number concentration (Naero), cloud droplet number concentration (Nd) first increases then decreases and fluctuates around 800 cm-3, while Nd in ECO increases faster initially, but soon its activation is suppressed by aerosol hygroscopicity and high activation threshold of numerous small particles, and almost no additional cloud droplets are produced. In terms of rapid adjustments, more bursty atmospheric supersaturation and lack of subsequent water cause cloud liquid water content (CLWC) in EC to increase explosively with Nd when there are few cloud droplets, but only maintains a low increase rate with further increasing Nd. ECO exhibits a fast increase in CLWC with Nd at high proportion of naturally emitted large aerosol particles, but its CLWC increase gradually stagnates as Nd increases. For non-precipitating clouds with less water content, CLWC in EC increases slowly with Nd, but can maintain a stable trend. While ECO, which relies mainly on large scale water and temperature variations to reach supersaturation, the increase in Nd leads to a decrease in CLWC.


AS35-A015
Effect of Aerosols in an Extreme-rain Producing Convective Storm in Eastern China

Yuxing YUN1#+, Da-Lin ZHANG2, Jinfang YIN1, Wenhua GAO1, Chun ZHAO3, Jiawei LI4, Hongli LIU1, Jianping GUO1
1Chinese Academy of Meteorological Sciences, China, 2University of Maryland, United States, 3University of Science and Technology of China, China, 4Chinese Academy of Sciences, China

We use the WRF-Chem model to simulate the extreme precipitation event in Guangzhou on May 7th, 2017, and investigate the effect of aerosols during this event. It is found that under polluted conditions, more latent heat is released through the condensational growth of droplets, which increases the updraft speed and ice-phase hydrometers. Precipitation is increased due to the melting of snow and graupel. However, in the latter stages of MCS development, the instantaneous extreme rain rate is lower in the polluted experiment, while the accumulated precipitation is higher. This study explains the evolution of extreme precipitation in the MCS and how the different microphysics, dynamics, and thermodynamics processes contribute to the evolution.


AS35-A016
Cloud Removal Using Machine Learning for BRDF/albedo Retrievals in the Arctic

Vikas HANASOGE NATARAJA#+
University of Colorado Boulder, United States

Since the late 1990s, NASA’s Earth Observing System constellation of satellites has provided continuous, long-term observations of atmospheric and surface processes on Earth, which has advanced our knowledge of our planet’s radiation budget. Imagery-based surface properties such as surface albedo and Bidirectional Reflectance Distribution Function (BRDF) are generated as an operational product using cloud-cleared, multi-angle surface reflectances from multiple overpasses over several days. The BRDF is central to imagery-based cloud and aerosol retrievals, while the surface albedo is a fundamental Earth energy budget parameter. Yet, this product is currently unavailable at higher latitudes such as the Arctic where (1) the low contrast between clouds and snow/ice poses a challenge for cloud detection and clearing, and (2) ice floes are drifting over time, which is currently not accounted for in the operational products. As a result, there is a significant gap in our understanding of the Arctic radiation budget and the influence of melt events on the ice-albedo feedback, cloud-radiative effects, etc. To address this gap, we propose the development of a BRDF/albedo product for moving sea ice floes and snow called the Sea Ice Floe and Snow Albedo Tracker (SIF-SAT). By leveraging multi-overpass, multi-angular satellite data, SIF-SAT will retrieve BRDF and albedo under low contrast and moving surface conditions. We combine existing cloud masks with machine learning (ML) models to produce cloud-cleared scenes in the Arctic. These scenes are then fed to a segmentation algorithm to identify individual moving sea ice floes and their reflectances are tracked over time to obtain BRDF and albedo. The focus of this presentation will be on the cloud-clearing model which has implications for radiation science in polar regions. SIF-SAT will enhance our capabilities in the challenging conditions of the Arctic and enable more accurate estimates of the cloud-radiative effect and ice-albedo feedback.


AS35-A017
Determined Characteristics of Particulate Matters and Precipitations and the Impacts of Wet Removal Based on Long-term Surface Measurements in Seoul, Korea

Suji HAN1+, Junshik UM1#, 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 modulates the water cycle and also contributes to controlling the concentration of atmospheric pollutants by washing out particulate matters (PMs) (i.e., wet removal or below-cloud scavenging). Previous studies showed the spatial and temporal characteristics of the concentration of PMs or precipitation. Although several studies attempted to quantify the impact of the wet-removal mechanism on the concentration of surface PMs, they were limited to a few events-based case studies. Thus, this study determined the impact of the wet-removal mechanism on the concentration of surface PMs (i.e., PM2.5 and PM10) by many events (over 10 thousand) based on long-term measurements in Seoul, Korea. Twenty-one years (2001-2021) surface measurements of precipitation and PM10 made at 25 stations in Seoul were used, while PM2.5 measurements were only available for seven years (2015-2021). All measurements were made with a one-hour resolution. The statistical analyses (i.e., monthly, seasonal, and yearly averages) for the variability of precipitation and mass concentrations of PMs were performed. The precipitation events were identified when the threshold time interval (i.e., 2 hours) existed between hourly precipitation data. The characteristics of precipitation events were quantified based on the precipitation duration, precipitation intensity, and accumulated amount of precipitation. The variation in PM concentrations during the precipitation events and the rate of wet removal were calculated as functions of the characteristics of precipitation events. The optimal duration, intensity, and accumulated amount of precipitation for the maximum wet removal were determined and the influence of precipitation properties on the wet-removal mechanism was also evaluated.


AS35-A018
Impact of Aerosols on Clouds with Different Weather Patterns in Northwestern Pacific

Keying LI1#+, Tianyi FAN1, Chuanfeng ZHAO2, Xin YANG1
1Beijing Normal University, China, 2Peking University, China

Aerosols are one of the crucial factors that impact regional and global climate. Dust and anthropogenic aerosol from East Asia contribute to the change of radiative fluxes and climate by modifying the cloud regimes in Northwestern Pacific (NWP). In this study, we attempt to find the role of aerosols on cloud properties in various cloud regimes under the control of differential weather systems in NWP. Using the cloud products obtained from Himawari-8 satellite combined with the Moderate Resolution Imaging Spectroradiometer (MODIS) retrievals for comparison, we classified the cloud regimes in NWP using the "k-means" clustering algorithm. The characters of the cloud regimes are described by analyzing their spatio-temporal distributions of the occurrences. Using the principal component analysis in T mode (T-PCA) for classifying weather patterns, we discussed the association between cloud formation and weather systems. We assessed the sensitivity of cloud properties to the perturbation of aerosols of different types in the main cloud regimes under the dominant weather patterns. This study helps to improve our understanding of the aerosol-cloud-radiation interactions in NWP.


AS35-A020
Vertical Distribution and Source Apportionment of Aerosol in Typical Areas of China

Dongyang PU#+, Hao WU
Chengdu University of Information Technology, China

The typical areas of aerosol distribution in China include three mega-city regions (BTH, YRD, PRD) and the background area of the Qinghai-Tibet Plateau. To compare the distribution and source of aerosol particles in these regions which have large differences in natural conditions and population density. In this research, we observed the aerosol particle number concentration continuously from July 2017 to September 2020. The conclusions can be deduced: 1. Aerosol-sounding observations conducted on the Qinghai-Tibet Plateau from June to September 2020 found that there is a high concentration level ( > 165 #/cm3) of fine particle layer (N < 300nm) near 15km in the upper air. 2. Due to the Northwest airflow in the upper air on the Qinghai-Tibet Plateau in September, the concentration is the lowest value of the four times observations. 3. The Hybrid Single-Particle Lagrangian Integrated Trajectory (HYSPLIT) model is used to analyze the 96h back trajectories of particles on the Qinghai-Tibet Plateau. It is found that in the late summer and early autumn, there are 29.3%~57.3% of the aerosols were transported from the southwest of the observation site. 4. According to the analysis of aerosol trajectories and particle size distribution characteristics, the source of aerosol in megacities is mainly attributable to human activities. We first investigate the aerosol differences under the influence of natural atmospheric conditions and human activities. But there are some deficiencies in the current research: further research is needed on the vertical distribution of aerosols and their climatic effects in megacities and the remote background region.


AS35-A022
Contrasting Influence of Nitrogen Oxides on the Cloud Condensation Nuclei Activity of Monoterpene-derived Secondary Organic Aerosol in Daytime and Nighttime Oxidation

Chenqi ZHANG1+, Yindong GUO1, Hongru SHEN1, Hao LUO1, Iida PULLINEN2, Sebastian SCHMITT2, Mingjin WANG3, Hendrik FUCHS2, Astrid KIENDLER-SCHARR2, Andreas WAHNER2, Thomas MENTEL2, Defeng ZHAO1#
1Fudan University, China, 2Forschungszentrum Jülich, Germany, 3Hefei University of Technology, China

Anthropogenic nitrogen oxides may influence the cloud condensation nuclei (CCN) activity of biogenic secondary organic aerosols (SOA) in both daytime photooxidation and nighttime NO3 oxidation, which has significant implications for the climatic impact of SOA. However, the influence remains unclear. In this study, we investigated the CCN activity of monoterpene-derived SOA formed from photo-oxidation of two monoterpenes (α-pinene and limonene) at different NOx levels, as well as BSOA generated in the dark by reaction of limonene and NO3. And we use the hygroscopicity parameter κ to characterize the CCN activity of MT-SOA. In daytime OH oxidation, NOx had little influences on the CCN activity of MT-SOA. In nighttime NO3 oxidation, MT-SOA had much lower CCN activity compared with those formed via OH or O3 oxidation. And we report the κ of monoterpene-derived organic nitrates (0.029-0.052) for the first time to our knowledge, which may be used to improve model simulations of CCN concentrations.


AS35-A023
Air Pollution Characteristics and Source Tracking in Megacity Chengdu Based on Cruise Observation

Hancheng HU#+
Chengdu University of Information Technology, China

This study researched the distribution characteristics of air pollution in Shuangliu District, Chengdu, the main persistent aerosol pollutants and ozone concentration in Shuangliu District from December 21, 2022 to February 5, 2023 were comprehensively analyzed by using the results of cruse observations. The sources of pollutants were analyzed by combining the meteorological data provided by Shuangliu Meteorological administration The Portable Optical Particle Profiler (POPS), ozone detector, hand-held weather station and wind lidar were integrated on the vehicle and made the cruse observation around the Baihe Park site, Yong'an Primary School site and their surrounding area in Shuangliu District. Three-dimensional spatial and temporal changes of areosol size distribution and ozone were obtained. The results showed that the average daily total particle number concentration was 5000~18000 #/m3/15000~18000#/m3 in haze weather, 5000~8000#/m3 after rain, respectively. coarse particles (272nm~473nm) accounted for 45%~60% in the whole observation period. Results showed that pollution was more likely to form the north wind, mainly due to industrial emissions and human activities in the upper wind direction region. The total particle number concentration decreased by 3%~8% when arriving at the park, but increased significantly, around 3%~10%, when passing by construction sites and driving close to trucks. Results of the cruse observation provide a scientific basis for particle and ozone control in Shuangliu District, which is conducive to the subsequent targeted pollution prevention and control of relevant departments, and can also provide reference for other urban areas.


AS35-A032
North Atlantic Oscillation Associated Variation in Cloud Phase and Cloud Radiative Forcing Over the Greenland Ice Sheet

Haotian ZHANG1#+, Chuanfeng ZHAO2, Jie YANG1, Yikun YANG2
1Beijing Normal University, China, 2Peking University, China

The Greenland ice sheet (GrIS) has been losing mass at an accelerating rate in recent decades due to warming, and understanding the underlying mechanisms, such as the impacts of clouds, is essential. Using space-borne data, this study investigates the spatial distribution of ice clouds and liquid-bearing clouds (LBCs) over the GrIS and their surface radiative forcing effects during summer daytime from 2006 to 2017, along with their characteristics during the North Atlantic Oscillation (NAO) events. Due to the perennial high-albedo surface, both ice and LBCs have a less important shortwave radiative cooling effect than in other environments. Based on the spatial variation pattern of clouds with the NAO index, the GrIS can be divided into three regions: the western, central, and eastern GrIS. During the positive NAO, the westerly wind strengthens in the western region, which causes the fraction of both ice clouds and LBCs to increase, and the cloud radiative effect at the surface increases by 2.07 W/m2; the temperature decreases in the central region, the fraction of ice clouds increases, the fraction of LBCs decreases, and the net radiative forcing is −2.05 W/m2; and sinking airflow is generated in the eastern region, both ice cloud and LBCs decrease, and the net cloud radiative effect at the surface is −1.34 W/m2. 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.


AS35-A033
Impacts of Dust on the Cloud Formation Time Over the Badain Jaran Desert Region

Xin ZHAO1+, Chuanfeng ZHAO2#, Yikun YANG2, Yulei CHI1, Yue SUN1
1Beijing Normal University, China, 2Peking University, China

To explore the influence of dust aerosols on cloud formation via radiative effect, this study takes the Badain Jaran desert area as the research area where cloud formation is less disturbed by human activities compared to other densely populated areas such as the North China Plain. We first identify 469 cases with cloud formation after 03:00 UTC (11:00 Beijing time) by manual method (checking every cloud image to identify the temporal evolution of clouds) using the high temporal resolution Himawari-8 satellite data. Through the analysis of individual cases, we find that the cloud formation time is mainly dependent on the low tropospheric stability (LTS) when the total precipitable water (TPW) is less than about 18.5 kg/m2, and greatly affected by the TPW when it is larger than 18.5 kg/m2. Dust aerosols near the ground absorb shortwave solar radiation, making the atmospheric structure unstable (decreased LTS) and conducive to cloud formation. Statistically, for every 0.1 increase in AOD, the cloud formation time is advanced about 138 minutes. Further analysis shows that dust aerosols actually inhibit the formation of convective clouds through microphysical processes when the TPW is small, while promote the formation of convective clouds through radiative processes when the TPW is large. This study reveals the effects of dust aerosols on the time of cloud formation along with the underlying mechanisms, which provides observational support for improving cloud parameterization in numerical models.


AS36-A001
Future Changes in Monsoon Precipitation Over the Indonesian Region Obtained by Bias Correction and Statistical Downscaling Methods: Including the Differences Between CMIP5 and CMIP6 GCMs

Motoki NISHIMORI1#+, Michihiko TONOUCHI2, Hiroshi SATODA2, Kadarsah 3, Agus SABANA HADI3, Dodo GUNAWAN3
1National Agriculture and Food Research Organization, Japan, 2Japan Meteorological Business Support Center, Japan, 3Indonesian Agency for Meteorology, Climatology and Geophysics, Indonesia

The climate of Indonesia located under the equator is predominated by the monsoon of both the northern and southern hemispheres. Climate changes in Indonesia would affect agricultural production and the whole economy. The future climate changes were projected by GCM simulation, but the geographical features of Indonesia are very complicated. Therefore, various downscaling methods involving RCM simulations are necessary to find detailed changes in the monsoon climate over Indonesia. Our previous work showed that precipitation over Java Island generally decreased in the onset season and increased in the dry season deduced by the bias-corrected CMIP5-GCMs output. In this study, CMIP6-GCMs are added as boundary conditions, the time scale of the analysis is varied from daily, 10-day, and monthly scales, and a downscaling method is also applied to account for the monsoonal atmospheric field and its changes. Preliminary analysis results using two CMIP6 GCMs (MIROC6 and MRI-ESM2) indicated that in each model group (MIROC5:MIROC6 and MRI-CGCM3: MRI-ESM2-0) seasonal monsoonal precipitation shift and wind system of historical runs (1995-2014) is similar. That is the onset of the monsoon is relatively postponed and the total amount of precipitation is small in MRI-ESM2-0. Future precipitation changes in the onset season would also decrease in MRI-ESM2-0. Multiple bias correction and statistical-downscaling methods are also being applied to the CMIP6 dataset to further analyze the seasonality and model dependence of future changes in precipitation in Indonesia.


AS36-A002
Climate Change Projection Over Mainland Southeast Asia and the Lancang-Mekong River Basin Based on a Set of RegCM4 Simulations

Yuanhai FU1#+, Xuejie GAO2, Ying XU3, Filippo GIORGI4
1Institute of Atmospheric Physics, Chinese Academy of Sciences, China, 2Chinese Academy of Sciences, China, 3National Climate Center, China, 4The Abdus Salam International Centre for Theoretical Physics, Italy

We investigate the projected climate change over Mainland Southeast Asia (also known as the Indochina Peninsula) and the Lancang-Mekong River basin, a region with complex topography and unique weather and climate systems, but limited availability of published high-resolution regional climate model (RCM) studies. The study is based on an unprecedented ensemble of 21st century projections with the RegCM4 RCM driven by five different general circulation models (GCMs) at a grid spacing of 25 km under the representative concentration pathways RCP4.5 and RCP8.5. We focus on mean temperature and precipitation in the dry season November–March (NDJFM), the wet season May–September (MJJAS), and the whole year. Intercomparison between the RegCM4 simulations with the driving GCMs is provided to illustrate the added value of the RegCM4 experiments. RegCM4 reproduces greater and more realistic spatial detail of the present day temperature and precipitation distribution compared to the driving GCMs, but some biases are found, such as an overestimation of precipitation over high topography regions. The spatial pattern of biases shows some consistencies across the GCMs and, for NDJFM the RegCM4, although weak correlation is found between the GCM and nested RegCM4 biases. A generally lower warming is projected in the future by the RegCM4 in different seasons and the whole year. For precipitation, while prevailing increases are found in the GCM projections, large areas of decrease occur in the RegCM ones, in particular during the wet season, possibly due to the more detailed topographical representation. The change patterns of precipitation show consistencies across the GCMs and the RegCM4, especially in MJJAS. The projected changes of extreme indices indicate a general decrease/increase of extreme cold/warm events. Drought events are projected to be more frequent over southwestern, while a general increase of heavy rain events prevails over most parts of the region.


AS36-A006
Projection of Future Photovoltaic Potential in South Korea Based on High-resolution SSP Scenarios

Jinuk KIM#+, Do-Hyun KIM, Tae Jun KIM, Young-Hwa BYUN
National Institute of Meteorological Sciences, Korea, South

Policies for carbon neutrality are being implemented around the world. To achieve carbon neutrality, renewable energy production must be increased. Solar energy is a representative renewable energy and is known to be significantly affected by climate change. In this study, based on high-resolution climate change scenarios, future Photovoltaics potential (PVpot) changes in South Korea was predicted. According to the four SSP scenarios (SSP1-2.6, SSP2-4.5, SSP3-7.0, SSP5-8.5), at the late 21st century, surface down-welling shortwave radiation, which has a major impact on PVpot, is expected to increase (by about +0.8 ~ +3.6 W/m2) compared to the present. However, PVpot is expected to increase (by about +1.3%) in the low-emissions scenario (SSP1-2.6) and decrease (by about -0.7 ~ -2.0%) in the high-emissions scenarios (SSP3-7.0, SSP5-8.5) at the end of the 21st century compared to the present. Because as the temperature increases significantly, the temperature of the solar cell panels increase, and performance ratio of PVpot decreases. Seasonally, PVpot is expected to increase (by about +2.3 ~ +4.0%) in summer and decrease (by about -3.6 ~ -7.1%) in winter.


AS36-A012
Assessing the Feasibility of Wind Energy Development in South Asia Through an Analysis of Land Surface Wind Speed Trends Using Reanalysis and In Situ Observations

Muhammad Abid KHAN#+, Koji DAIRAKU, Saurabh KELKAR
University of Tsukuba, Japan

Reanalysis metadata are a critical resource for examining meteorological changes and evaluating wind energy potential. Observed wind speed studies reveal a global decline in land surface wind speed since the 1960s, known as terrestrial stilling, but with a reversal around 2010. The extent to which the decline in trend and turning point of land surface wind speed has been captured by reanalysis products is currently unknown. To address the research gap, a systematic evaluation of climatological winds and trends in three reanalysis products (ERA5, JRA-55, and NCEP/NCAR) was conducted by comparing 10-m wind speed time series from grid cells with observational data from 32 in situ meteorological stations for the period 1973-2005. To measure the accuracy of the reanalysis products, a range of statistical metrics were employed, including standard deviation (STD), mean absolute error (MAE), percent bias (PBIAS), correlation coefficient (R), M-K test and Sens slope estimation. Based on the evaluation of climatological winds, JRA55 proves to be the most accurate reanalysis product compared to the observations. Despite this, considerable deviations were discovered between the simulated wind speeds and the observations. The JRA55 reanalysis product was found to reflect changes observed in the Subcontinent, with the NCEP/NCAR product following closely behind. The JRA55 reanalysis demonstrated agreement with observations m/s, with a high R of 0.93, a PBIAS of -10.70, and a low MAE of 0.28. further, NCEP/NCAR showed lower standard deviation levels of 0.54. The Subcontinent's wind energy industry is experiencing growth and expansion, with opportunities for the development of offshore wind farms and the expansion of existing land wind farms. This study aims to highlight the discrepancy between observed and simulated land surface wind speeds, emphasizing the importance of careful use of reanalysis products for wind assessment and forecasting in the subcontinent region.


AS36-A013
Dynamical Downscaling Over Southeast Asia: Perfect vs Imperfect Boundary Conditions

Venkatraman PRASANNA1#+, Xin Rong CHUA2, Chen CHEN2, Gerald LIM1, Sandeep SAHANY2, Muhammad Eeqmal HASSIM2,1, Aurel MOISE2
1Meteorological Service Singapore, Singapore, 2Centre for Climate Research Singapore, Singapore

In dynamical downscaling, biases in lateral boundary conditions obtained from coarser models can play an important role in the dynamically downscaled simulations. As a part of Singapore’s Third National Climate Change Study, dynamical downscaling has been carried out over Southeast Asia (SEA; 79E-160E;16S-24N), using the Singapore Regional Climate Model (SINGV-RCM; an adapted version of Singapore’s operational NWP model) using perfect boundary conditions (ERA-5) and four CMIP6 GCM (ACCESS, EC-Earth, MPI & UKESM) at 8km horizontal resolution. The SINGV-RCM is forced with ERA-5 reanalyses data for a 36-year period (1979-2014) at 8km resolution over SEA with regular update of the sea surface temperature at 6-hr interval; further, a similar simulation is carried out using four CMIP6 GCM (ACCESS, EC-Earth, MPI & UKESM) forcing data for a 60-year period (1955-2014). The last 20-year period (1995-2014) from the five simulations with reliable high-resolution observation (merged in-situ and satellite) is selected for evaluation. Rainfall characteristics including the diurnal cycle and extremes from the five simulations evaluated against observations will be presented.


AS36-A021
Future Projections of Bioclimatic Indicators on Korean Peninsula Using SSP Scenarios

Chansung OH1+, Jina HUR2, Sera JO2, Seung Beom SEO3, Jaepil CHO1#
1Integrated Watershed Management Institute, Korea, South, 2National Institute of Agricultural Sciences, Korea, South, 3University of Seoul, Korea, South

Climate change due to global warming affects various areas such as agriculture, ecosystem, water resources, and forest in different ways. Climate change scenarios have been used as a scientific basis for establishing climate change adaptation policies to preemptively minimize damage by assessing future impacts due to climate change. In this study, downscaled data with 1 km resolution for the Korean Peninsula was produced using the SSP (Shared Socioeconomic Pathways) scenario used in the AR6 report. In order to consider the uncertainty of the future outlook that may occur depending on the selection of a specific Global Climate Model (GCM) when using only a single climate model, a total of 18 climate model data were used to analyze the future projections based on multiple model ensemble (MME). First, the downscaled data was produced using a non-parametric quartile mapping (QM) technique that does not use a distribution formula in estimating the bias between the observed data and the GCM data. Then, the characteristics of future fluctuations of 19 bioclimatic indicators were analyzed. The future projections were analyzed for each of the 30-year periods of the near-future (2011-2040), mid-future (2041-2070), and far-future (2071-2100) compared to the past 30-year period (1981-2010). In the case of annual precipitation and annual average temperature, the rate of change tended to be higher during the far-future compared to the near-future period. Within the same future period, SSP5-8.5 showed the highest change rate while SSP1-2.6 showed the lowest change rate. In the case of bioclimatic indicators, bio4 and bio15, which represent seasonal variability in precipitation and temperature, also showed the highest increase rates in the far-future and SSP5-8.5 scenarios.


AS36-A024
Domain Shift Problem in Deep Learning-based Downscaling Models: Daily Precipitation

Hae Soo JUNG+, Sungmin O, Seon Ki PARK#
Ewha Womans University, Korea, South

Extreme precipitation events, causing tremendous socio-economic damage, are among the most disastrous phenomena. Nowadays, many studies address the localization of extreme events and their intensification throughout climate change; thus, the demand for high-resolution and reliable atmospheric data is increasing. Downscaling of model output is one of the efficient ways to produce detailed data, and it simultaneously draws attempts to increase its efficiency through deep learning (DL) methods. Although DL methods have the advantages of less demand for long-term observation data and lower calculation costs, there are limitations, too: in particular, the performance of downscaling through DL methods heavily depends on the amount of the training data set. The enormous amount of atmospheric data is suitable for training DL-based downscaling models; however, high-quality atmospheric data with appropriate resolution and reliability are restricted. Considering various features of regional climate, investigation of the domain-shifting problem is crucial in order to apply the learned DL model to other regions excluded from the training data. Accordingly, the performance differences among the DL-based downscaling models, trained with differently distributed data, are investigated by comparing the cross-applying results. In addition, the DL model with integrated learning data is also investigated. This study lays the foundation for the smooth application of a deep-learning model for detailed daily precipitation.


AS37-A003
Cold Surge Impacts on the South China Sea Boundary Layer

Chung-Hsiung SUI#+, Kuan-Yun WANG, Mong-Ming LU
National Taiwan University, Taiwan

Episodic cold surges associated with the East Asia (EA) winter monsoon can penetrate deep into the South China Sea (SCS), enhance consequent tropical rainfall, and further strengthen the EA meridional overturning circulation (MOC). These cold surges can promote strong surface fluxes and lead to a deeper marine planetary boundary layer (PBL). In this study, we use high resolution radiosonde data of temperature and humidity profiles over Dongsha Island to identify the PBL height (PBLH), mixed layer height (MLH), cloud base, and cloud top for the period of December-January-February (DJF) from 2010 to 2020. We combined ERA-5 meteorological variables and surface fluxes, MERRA-2 cloud radiation data, and radiosonde-derived PBL parameters to perform an energy budget analysis and turbulent diagnostics from the mixed-layer model from Nicholls (1984). Here we show a strong turbulent flux convergence of both heat and moisture over the SCS during cold surges, which leads to a lifting of the MLH to ~1.0 km and PBLH to ~2.0 km and associated cloud development over Dongsha Island (116.69E, 20.70N). The cold and dry horizontal advection is balanced by this vertical turbulent flux convergence in the energy budget. Overall, at post-surge the PBL is stable but mixed layer is unstable, which contrasts with the pre-surge stage that features a stable mixed layer and a conditionally unstable PBL.


AS37-A004
Intraseasonal Oscillations and the Subseasonal Peak Rainfall Event in the Eastern Philippines During 2017/18 Winter and S2S Prediction Evaluation

Wayne Yuan-huai TSAI#+, Mong-Ming LU, Yin-Min CHO, Chung-Hsiung SUI
National Taiwan University, Taiwan

From December 13, 2017 to January 2, 2018, three tropical cyclones (TCs) successively made landfall in Mindanao and led to the most extreme wintertime (December - February) subseasonal peak rainfall event (SPRE) over the eastern Philippines (9°-14°N, 122°-127°E). The SPRE is defined by the maximum 15-day accumulated rainfall amount within the region during a time span of 90 days. The 15-day rainfall extremes over the eastern Philippines are associated with the environmental low-level cyclonic vorticity, which can be contributed to La Niña condition, Madden-Julian Oscillation (MJO), and equatorial Rossby (ER) waves. During the 15-day period of 2017/18 winter SPRE, the cyclonic vorticity phase of the westward propagation ER waves from the North Pacific occurred twice and the second episode occurred simultaneously with an MJO from the Indian Ocean across the Maritime Continent to the western Pacific. Favored by anomalous cyclonic vorticity and humidity produced by La Niña and MJO, the two ER waves enhanced and resulted in two TCs and led to the extreme SPRE. Based on the hindcast data in the S2S database, the 2017/18 SPRE and associated MJO and ER waves in ECMWF and NCEP models show skillful forecasts up to the extended range (11-day lead). For the SPRE in 2017/18 winter, the ECMWF model performs better than the model’s hindcast skill, whereas the NCEP model performs worse. The model with a better representation of SPRE timing and intensity has smaller phase and amplitude biases of tropical waves in the medium (5-10-day lead) and extended ranges. The forecast skill of the MJO and ER linked to ENSO phases will be discussed. The analysis procedure proposed in this study can be applied to monitor and predict the SPREs and their associated large-scale drivers in other regions.


AS37-A005
The Impact of Scale-aware Parameterization on the Next-generation Global Prediction System in Taiwan for Front Predictions

Chang-Hung LIN1#+, Ming-Jen YANG2, Ling-Feng HSIAO1, Jen-Her CHEN1
1Central Weather Bureau, Taiwan, 2National Taiwan University, Taiwan

In order to improve the precipitation forecast of the next-generation Global Prediction System with the Finite-Volume Cubed-Sphere Dynamical Core in Taiwan’s Central Weather Bureau (TFV3), this study modified the convective processes in New Simplified Arakawa-Schubert scheme (NSAS) based on the methodology of scale-aware parameterization developed in Kwon and Hong (2017) and investigated its impacts on a front event, which propagated across Taiwan and produced heavy rainfall in late May of 2020. Results show that the modified scale-aware parameterization has significantly improved the intensity and the spatial distribution of frontal precipitation forecasts due to the proper definition of convective updraft fraction. However, the synoptic-scale features perform a larger warm bias with the modified scale-aware parameterization. To understand the reason for the warm bias, the vertical profiles of zonal mean temperature, cloud cover and the heating rate from each physical parameterization were investigated to reduce the biases. The result of verification shows that the occurrence of a larger warm bias in low-to-mid levels is attributed to the decrease in subgrid-scale water vapor consumption by the deep convection process and the increase in grid-scale condensation heating resulting from the consumption of environmental instability by microphysical processes. Therefore, further modification of the scale-aware capability of convective cloud water detrainment is proposed to reduce the heating from microphysical processes and result in a better overall performance for the medium-range weather forecasts.


AS37-A006
Weather and Climate Analysis of Tropical Cyclone Genesis Clustering Events in Western North Pacific Extended-weather Analysis

Jian-Hung LIAO1#+, Chung-Hsiung SUI1, Jau-Ming CHEN2, Hsu-Feng TENG3
1National Taiwan University, Taiwan, 2National Kaohsiung University of Science and Technology, Taiwan, 3National Center for Atmospheric Research, United States

In the boreal warm season (May-September), tropical cyclone genesis (TCG) is active in the West North Pacific (WNP) region. TCG occurs in WNP monsoon trough that are influenced by active weather and climate oscillations. In addition, TCG tends to cluster in a short period and absent at other times. In this study, we investigate the weather (or extended weather) disturbances responsible for the extreme TCG clustering and how the weather disturbances are influenced by low-frequency climate oscillations including QBWO, ISO, and ENSO. We first calculate the maximum number of TCG per 10 days in each JJASO season from 1990 to 2019 to determine the most extreme TCG cases. Four cases with 5 TCGs in 10-days are selected. By analyzing the extended weather disturbances of the four periods, we find that 15 out of 20 TCs occurred in positive vorticity phase of QBWO and 4 TCs formed following a preexisting mature TC suggesting Rossby wave energy dispersion within positive vorticity region of QBWO. A further analysis of the climate conditions shows that, three of the four extreme TCG-clustering events occurred in late July-August during La Niña developing summer with inactive BSISO, while the other occurred in El Niño developing July with active BSISO in WNP.


AS37-A007
Characteristics of the South Asian High Intraseasonal Variability and its Influence on the Precipitation Over the South China Sea and Surrounding Region

Po-Chia CHEN#+, Mong-Ming LU
National Taiwan University, Taiwan

The South Asian High (SAH) is the most important upper tropospheric summer system over Asia as its intensity and shape variation are closely linked with Indian and East Asian summer monsoon rainfall variability. However, SAH intraseasonal variability and its impacts on precipitation has not been fully untangled. In this study, we used the empirical orthogonal function (EOF) to analyze the 200-hPa daily geopotential height (GPH) during June-August in 1979-2020 over 20°-120°E, 10°-50°N. The first three leading modes are all significant at the intraseasonal time-scale. The regression patterns of 200hPa wind and GPH in the Northern Hemisphere show the first two modes are associated with different types of midlatitude circumglobal teleconnection patterns. The spatial pattern of EOF3 shows a negative sign over the Black Sea, a positive sign over the North China and another negative sign over the north of Indian and Indochina Peninsula, suggesting a possible north-south shift of the SAH center location. The regressed precipitation on PC3 shows negative correlation with the precipitation over the Yangtze River and Japan and positive correlation with the precipitation over the South China Sea (SCS) and Philippine. The PV tendency equation is used to diagnose how the SAH variations influence the precipitation anomalies over the SCS. The extreme cases in June and July 1998 are selected for detailed analysis. In June and July 1998, the SAH was extended eastward to the South China, and the Western Pacific subtropical high (WPSH) was extended westward to the SCS. Due to the anomalous descending motions associated with the WPSH, the rainfall over the SCS (110°–120°E, 10°–20°N) was the fewest during 1979-2020. The process of how the upper tropospheric circulation affects the lower tropospheric circulation and precipitation will be discussed.


AS37-A013
Sub-seasonal Rainfall Extremes and Extended-range Forecast Opportunity in Taiwan and the Philippines Revealed in the S2S Database

Mong-Ming LU1#+, Wayne Yuan-huai TSAI1, Sheng-Fong HUANG1, Yin-Min CHO1, Chung-Hsiung SUI1, Ana Liza Solmoro SOLIS2, Meng-Shih CHEN3
1National Taiwan University, Taiwan, 2Philippine Atmospheric, Geophysical and Astronomical Services Administration, Philippines, 3Central Weather Bureau, Taiwan

During the first half month of April 2022 the Philippines experienced severe disasters associated with the weak but deadly tropical storm Megi that caused 214 deaths and the sinking of two ships. This prompted us to investigate the predictability of the springtime Philippine sub-seasonal scale rainfall extremes and to identify the forecast opportunity in the S2S prediction database. The results suggest that ENSO is the most influential climate driver for the sub-seasonal scale springtime (February-April) rainfall variability in the Philippines. MJO and equatorial Rossby (ER) waves can modulate the sub-seasonal rainfall extremes. The 15-day accumulated rainfall amount of the sub-seasonal peak rainfall events (SPRE) is higher during a La Niña spring, so is the occurrence probability of a extremely wet event. The wet extremes can be enhanced by strong MJO or equatorial Rossby (ER). For the April 2022 case, the S2S multi-model ensemble mean (MMEM) can successfully predict the extremity of the SPRE at least 10 days ahead, although both MJO and ER were weak during the occurrence period of the deadly SPRE. Thus the successful prediction was interpreted as a result of the predictability rooted in the rainfall variability driven by the La Niña event. Since the S2S prediction is built on the ENSO foundation, it is proposed to include the SPRE in the real-time extended-range forecast items to exploit the benefits of S2S prediction and applications.


AS38-A008
LSM Perturbation Experiment and Impact on Afternoon Thunderstorm Ensemble Forecast

YuTze HONG#+, Jen-Ping CHEN
National Taiwan University, Taiwan

This study examines the sensibility of WRF simulation to different options of the Noah land surface model (LSM) with multiple parameterization options (Noah-MP) and the feasibility of using LSM perturbation for the ensemble forecast of afternoon thunderstorms over the Taiwan area. Five land surface processes in Noah-MP were tested, and the results showed that the sensitivity of the processes in descending order are: surface layer exchange coefficient, canopy radiation geometry, canopy stomatal resistance, surface resistance to evaporation, and soil moisture factor for stomatal resistance. Based on the sensitivity analysis, we designed an LSM perturbation method for WRF based ensemble system by applying various Noah-MP configurations and land surface initial conditions. Two ensemble experiments, each with 24 members, were conducted to assess the impact of LSM perturbation on afternoon thunderstorm rainfall simulations. One applied perturbation on initial atmospheric conditions and the other with additional LSM perturbations. The preliminary results from the 24-hour forecast of five afternoon thunderstorm cases showed that the LSM perturbation scheme could effectively improve the spread-skill performance of atmospheric variables near the surface, and the probability match of precipitation is also improved. Further details of the probability forecast analysis will be presented.


AS38-A010
Evaluation of Multi-scale Sampling Performance of Ensemble Perturbations in the NCEP Global Ensemble Forecast System and Mechanisms

Li MA#+, Jie FENG
Fudan University, China

The key to ensemble forecasting is the generation of initial ensemble perturbations which is aimed at sampling the probability distribution of analysis errors. Most studies assess the prediction skill of the ensemble forecasts, which, however, is simply an indirect reflection of the quality of initial ensemble conditions. This study will evaluate the performance of ensemble perturbations in sampling forecast errors at multiple spatial scales through the entire forecast lead times. The projection of ensemble perturbations onto forecast errors at multi-scales and different lead times is the major metric used in this study. The variations of the projection as a function of spatial scale, lead time, and vertical levels will be carefully investigated. How these perturbation-error relationships can influence the control and perturbed forecast skill will also be explored.


AS38-A019
Spatiotemporal Estimation of Analysis Errors in the Operational Global Data Assimilation System at the China Meteorological Administration Using a Modified Safe Method

Jie FENG#+
Fudan University, China

Quantification of the uncertainties in initial analyses against the real atmosphere (“reality”) provides a fundamental reference for the evaluation and development of operational data assimilation (DA) systems. Due to the unknown reality, most existing methods for analysis error estimation use reanalysis datasets or observations as a proxy for reality, which are empirical, nonobjective, and biased. Unlike these methods, our study adopted a modified Statistical Analysis and Forecast Error (SAFE) estimation method to objectively and directly quantify spatiotemporal errors in analyses compared to reality based on unbiased assumptions. In the present study, the SAFE method was first applied to estimate the annual variation and spatial distribution of analysis errors in the Global Forecast System of Global/Regional Assimilation and PrEdiction System (GRAPES_GFS) at the China Meteorological Administration since the beginning of its operational implementation (i.e., 2016–2021). Qualitative comparison to analysis error estimations in previous studies showed that SAFE can provide more reasonable spatial-mean analysis error profiles than can the estimation with the ERA-5 reanalysis as a reference (the approach hereafter called “ERAv”). Moreover, ERAv overestimates (underestimates) the spatial-mean analysis error below (above) ~500 hPa compared to SAFE because it neglects the uncertainties inherent in reanalysis. Overall, the SAFE estimation reveals that relative reductions of about 12.5%, 29%, and 24.5% were achieved for the spatial-mean analysis errors of wind, temperature, and geopotential height, respectively, in the GRAPES_GFS throughout the six-year study period. These results can largely be attributed to the DA scheme being upgraded from 3D-Var to 4D-Var. SAFE can also provide more reasonable and accurate point-wise analysis errors than ERAv can.


AS38-A023
Status and Plan of Ensemble Forecast System in Korea Meteorological Administration

Eun-Jung KIM#+, Sora PARK, Hyun-Cheol SHIN, Jong Im PARK, Jong-Chul HA, Young-Cheol KWON
Korea Meteorological Administration, Korea, South

The ensemble forecast system based on the Korea Integrated Model (KIM), which is developed for Korea’s own numerical weather prediction (NWP) model, has been in operation at Korean Meteorological Administration (KMA) since October 2021. KMA ensemble forecast system consists of 50 perturbation members (25 members for long-range forecast) and 1 control simulation. Four-dimensional LETKF (Local Ensemble Transform Kalman Filter) with additive and RTPS inflation scheme is used to make initial perturbation.
Evaluation of forecast scores shows that our operational ensemble forecast system is generally more skillful compared to the deterministic simulation as forecast time is longer. We also tested ensemble forecast with increased ensemble size which is planned to be operated this summer. Increased ensemble size produces better representation of atmospheric fields especially in higher latitudes. Details of results from operational ensemble system and impacts of increased ensemble size will be discussed with introducing a brief overview of our ensemble forecast system and development plan in future.


AS39-A005
The Tables of Aerosol Optics (TAO) Project

Greg SCHUSTER1#+, Bastiaan VAN DIEDENHOVEN2, Richard MOORE3, Elisabeth ANDREWS4,5, Joshua SCHWARZ4, Masanori SAITO6, Ping YANG6, Snorre STAMNES3, Benjamin JOHNSON7, Arlindo DA SILVA8, Mian CHIN9
1NASA Langley Research Center, United States, 2SRON Netherlands Institute for Space Studies, Netherlands, 3National Aeronautics and Space Administration, United States, 4National Oceanic and Atmospheric Administration, United States, 5University of Colorado Boulder, United States, 6Texas A&M University, United States, 7University Corporation for Atmospheric Research, United States, 8NASA Goddard Space Flight Center, United States, 9NASA GSFC, United States

The Table of Aerosol Optics (TAO) project is a community repository of optics computations (extinction, absorption, single-scatter albedo, lidar ratio, etc) that are useful for global models and remote sensing applications. TAO expands upon historical efforts (e.g., Hess et al., 1998) by building an open database that uses recent measurements and new computational techniques for non-spherical particles. The ‘open’ aspect of TAO is important, since the size distributions, hygroscopicities, refractive indices, and morphological recommendations of today will undoubtedly yield to different values in the future; the open framework of TAO allows scientists to keep adding new computations to the database as the science evolves.
TAO is meant to be a community repository where specialists can put their computations for other scientists to use. So for instance, some groups are advancing new techniques that can accommodate complex fractal aggregates of black carbon, other groups are working on realistic irregular shapes for mineral dust, and different groups are updating the hygroscopicity of various aerosol types using new techniques. The TAO database gives these scientists a place to distribute their products. As TAO grows, modelers and remote sensing specialists will look to TAO as a place to find a wide variety of choices for testing. Meanwhile, global modelers can also use TAO to lobby for new tables that accommodate their needs.
Eventually, TAO will provide mass extinction coefficients, mass absorption coefficients, lidar ratios, etc., at popular remote sensing and global modeling wavelengths (0.25-40 µm) for all pertinent species (sulfate, sea salt, BC, OC, BrC, dust, etc.). Multiple tables may be created for each species or type to account for the multiple valid size distributions, hygroscopicities, complex refractive indices, and shapes that can be found in the literature.
Hess, M., P. Koepke, and I. Schult (1998), Bull. Am. Meteorol. Soc.


AS39-A010
Comparison of GOCI 6km-AOD and 500m-AOD in Estimating Ground-level PM2.5 Concentrations Over Metropolitan City Busan in South Korea Using Machine Learning Method

Juhee LEE1+, Yeseul CHO1, Seoyoung LEE1, Kwang-min MYUNG2, Young-doh KIM3, Ja-Ho KOO1#
1Yonsei University, Korea, South, 2Data Intelligence Lab, Inc., Korea, South, 3Weatheri, Inc., Korea, South

Since the airborne particulate matter (PM) affects the respiratory health of human significantly, the monitoring of its quantity in a high spatial resolution is requested. But it is not an easy task because the installation of qualified surface monitoring station is expensive. The satellite monitoring can be an alternative but its spatial resolution is still sparse. To get over these limitations, we can estimate of PM2.5 (PM having a diameter < 2.5 μm) based on the machine-learning system with the consideration of both surface in-situ and satellite measurements. In this study, we develop the PM2.5 estimation platform based on the random forest (RF) algorithm using the Geostationary Ocean Color Imager (GOCI) 6km-AOD products and 500m-AOD products with surface PM2.5 measured by KT company cheap sensor networks from June 2018 to December 2019. Our target region is Busan in South Korea. In addition to AOD, we use other 11 physical values such as the meteorological parameters (e.g., temperature, wind speed, etc.) from the ERA5 reanalysis dataset of the European Centre for Medium-Range Weather Forecasts. For the validation, we use two methods, which are the 10-fold cross validation and the comparison with the surface PM2.5 observed by the Korean government monitoring system. In conclusion, the quality of our RF-based PM estimation is reliable, showing R2 = 0.45 for the case to use AOD at 6 x 6 km2, and R2 = 0.71 for the case to use AOD at 0.5 x 0.5 km2, showing that the usage of high resolution AOD enables us to have better PM2.5 estimation. Our study clearly shows the advantage of high AOD resolution for the regional air quality monitoring, related to the machine-learning system. This work was supported by the National Research Foundation of Korea(NRF) grant funded by the Korea government(MSIT) (No. 2020R1C1C1011624).


AS39-A011
Comparison of PM2.5 Concentration Between the Surface Measurement and MERRA-2 Reanalysis Dataset in South Korea

Dayeong LEE, Juhee LEE+, Ja-Ho KOO#
Yonsei University, Korea, South

Reanalysis data prepared by the aerosol data assimilation was developed to compensate for the limitations of ground observation data, satellite data, and modeling. Since The second version of Modern-Era Retrospective analysis for Research and Applications (MERRA-2) reanalysis data including AOD assimilation provides the gridded PM2.5 for the long-term period, it can be widely used for the analysis of regional aerosol pollution. To do this work, the validation of MERRA-2 PM2.5 is strongly required. In South Korea, however, this evaluation research is still insufficient. In this study, from 2015 to 2021, the PM2.5 concentration of MERRA-2 is evaluated by surface PM2.5 observed by the Korean national intensive monitoring sites (NIMSs). We found some difference between the MERRA-2 and NIMSs PM2.5. First, the monthly variation is different. While NIMSs PM2.5 is highest in winter but lowest in summer, MERRA-2 PM2.5 shows a maximum in April and minimum in winter. In other words, MERRA-2 PM2.5 is largely overestimated in summer but underestimated in winter generally. Among the components used in the MERRA-2 PM2.5, sulfate, black carbon, dust, and sea salt is overestimated but organic carbon is underestimated compared to the aerosol component of NIMSs. However, total MERRA-2 PM2.5 is much lower than the PM2.5 of NIMSs, especially in the urban area. This feature seems due to the absence of nitrate component in the MERRA-2 data. When we consider the amount of nitrate based on the empirical estimation suggested by some previous studies, we confirm that the quantity of MERRA-2 PM2.5 becomes much closer to the NIMSs PM2.5. Understanding of MERRA-2 PM2.5 characteristics for each region is still required in future studies. This work was supported by the National Research Foundation of Korea(NRF) grant funded by the Korea government(MSIT) (No. 2020R1C1C1011624).


AS39-A013
Satellite-assisted Particulate Matter (SAPM) for the Models, In Situ, and Remote Sensing of Aerosols (MIRA) Working Group

Travis TOTH1#+, Greg SCHUSTER1, Alexander MATUS2, Mian CHIN3, Meloë KACENELENBOGEN4, Edward NOWOTTNICK2, Melanie FOLLETTE-COOK2
1NASA Langley Research Center, United States, 2NASA Goddard Space Flight Center, United States, 3NASA GSFC, United States, 4NASA Ames Research Center, United States

Particulate matter with aerodynamic diameters smaller than 2.5 microns (PM2.5) is a major contributor to air pollution worldwide and negatively impacts human health. For the past few decades, researchers have developed a variety of approaches to estimate surface PM2.5 from satellite observations, due to a lack of ground station in situ PM2.5 coverage in many regions globally. A well-documented technique is the use of column-integrated aerosol optical depth (AOD) retrievals from passive sensors to obtain surface PM2.5 proxies. Active sensors, like lidars, provide aerosol vertical distribution, and thus can be used to scale column AOD to the surface to improve the proxies. In addition to this synergistic passive/active sensor approach, near-surface aerosol extinction retrievals from lidar measurements can also be used independently to derive PM2.5 concentrations. Furthermore, researchers have used aerosol models to convert satellite AOD to surface PM2.5, and data assimilation methods can be employed to improve forecast PM2.5 model simulations. Benefits of space-based/model-assisted PM2.5 estimates include helping to approximate PM2.5 concentration levels for those areas lacking in situ ground station coverage, providing nighttime characterization of air quality, and assessing spatial and temporal variations of PM2.5 pollution on both regional and global scales. For this Models, In situ, and Remote sensing of Aerosols (MIRA) Topic, we aim to provide inter-comparisons of various methods and techniques for retrieving surface PM2.5 assisted by satellite remote sensors, global aerosol models, and in situ aerosol measurements. These comprehensive PM2.5 estimates can be useful for current and future efforts in air quality research, modeling, forecasting, and applications. We seek international in situ datasets (e.g., mass scattering/absorption coefficients and aerosol hygroscopic properties) for various aerosol species to develop more robust PM2.5 estimates. We also seek international ground-based in situ PM2.5 datasets to validate the PM2.5 concentration estimates.


AS39-A017
Characteristics of PM2.5 at the Ground-level and Top of POSCO Tower, Incheon, Korea

Yongjoo CHOI1#+, Jeonghoon LEE2, Saehee LIM3, Jiyoung KIM4, Yong Jae LIM4, Jongbyeok JUN1, Giyeol LEE1, Ilkwon NAM4, Sumin KIM4
1Hankuk University of Foreign Studies, Korea, South, 2Korea University of Technology and Education, Korea, South, 3Chungnam National University, Korea, South, 4National Institute of Environmental Research, Korea, South

Since 2019, the Korean government has been implementing a PM2.5 Seasonal Management Policy during wintertime (December to March in next year) to protect public health by mitigating the frequency and concentration of high PM2.5 events. To investigate the difference in the chemical composition of PM2.5 at ground-level and mid-upper planetary boundary layer (PBL) during winter (January to March) in 2023, 24-h PM2.5 filter samplings were conducted at both the ground-level and top of POSCO Tower (37.39°, 126.64°, 305 m a.s.l) along with co-located air quality monitoring stations (AQMS) which provide hourly concentrations of PM10, PM2.5, CO, NO2, SO2, and O3. POSCO Tower is the sixth-highest building in Korea thus the Korean first AQMS at high altitude was established in 2023. Using low volume sampler (16.7 LPM), filter samples were collected on the 47 mm Teflon filter (PTFE Filter with support ring, 2.0 μm; MTL) for mass and trace metal concentration, and the quartz fiber filter (Tissuquartz™ 2500QAT-UP, Pall Pallflex) for water-soluble ions and carbonaceous concentration. The concentration of chemical components (ion, trace metal, and carbon) will be analyzed to utilize the input into a positive matrix factorization (PMF) analysis, which will allow us to identify different emission sources between two vertical sites by combining the backward trajectory analysis. We believe that this study will be contributed to not only identifying the major emission sources at two vertical sites, but also enhancing the accuracy of vertical PM2.5 prediction in the chemical transport models and remote sensing techniques.


AS39-A021
Retrieval of Aerosol Optical Depth from Geostationary Environment Monitoring Spectrometer (GEMS) Using Machine Learning Approaches

Hyunyoung CHOI+, Seohui PARK, Jungho IM#, Audrieauna BEATTY
Ulsan National Institute of Science and Technology, Korea, South

Aerosols are not only air pollutants that are linked to human health, but also an important factor in understanding earth radiation and climate change. As aerosol optical depth (AOD) is a quantitative estimate of aerosols present in the atmosphere, it can be used as a proxy of air quality. Satellite-based AOD is mainly obtained through a radiative transfer model, demanding heavy computation and having uncertainties. To overcome these challenges, this study proposed a machine learning-based model to estimate hourly AOD from the Geostationary Environment Monitoring Spectrometer (GEMS) over Asia-Pacific regions (5°S–45°N, 75°E–145°E). The model was constructed using light gradient boosting machine, which has top-of-atmosphere (TOA) reflectance and observation angle data obtained by the GEMS satellite sensor, meteorological variables from the numerical model, and other auxiliary variables as independent variables. Aerosol Robotic Network (AERONET)-measured AOD data were used as a dependent variable. The proposed model was evaluated using random, spatial, and temporal 10-fold cross-validation (CV) with in-situ data to examine the spatiotemporal generalization possibility. The results of the random and temporal CV showed good agreement with the reference data, resulting in the determination of coefficient (R2) of 0.87–0.90 and root-mean-square-error (RMSE) of 0.11–0.12. However, the spatial CV results yielded slightly lower accuracy, with an R2 of 0.67 and an RMSE of 0.19. This explains the low spatial transferability in areas where ground stations are rare or in low-latitude regions where input data for modeling are often unavailable due to frequent precipitation. However, it is confirmed that the accuracy of AOD estimation is comparable to or even better than the operational GEMS AOD product. Our results indicate that the proposed approach using TOA reflectance data from geostationary satellite sensors has great potential for estimating AOD for operational purposes.


AS40-A004
Impact of the Pacific Sector Sea Ice Loss on the Sudden Stratospheric Warming Characteristics

Yvan ORSOLINI1#+, Jiarong ZHANG2, Varavut LIMPASUVAN2, Jinro UKITA3
1Norwegian Institute for Air Research, Norway, 2Coastal Carolina University, United States, 3Niigata University, Japan

The extent of sea ice coverage over the Arctic Ocean has dramatically declined over the past few decades. The anomalously warm Arctic surface associated with the Arctic sea ice loss has been linked to the mid-latitude surface cooling in the subsequent boreal winter. Several studies have suggested that this linkage could involve the wintertime stratospheric circulation by enhancing the upward planetary wave (PW) activity and weakening the polar vortex. Temperature anomalies induced by the vortex weakening could subsequently descend into the troposphere on time scales of weeks to months, potentially leading to cold air outbreaks (CAOs) over the continents. Cases studies based on observations or model simulations even suggested that the enhanced wave flux could be strong enough to cause the demise of the polar vortex associated with the sudden stratospheric warming (SSW) phenomenon. The atmospheric response to Arctic sea ice loss remains however a subject of much debate. Most studies have focused on the sea ice retreat in the Barents-Kara Seas and its troposphere-stratosphere influence. Here [1], we investigate the impact of large sea ice loss over the Chukchi-Bering Seas on the sudden stratospheric warming (SSW) phenomenon during the easterly phase of the Quasi-Biennial Oscillation through idealized large-ensemble experiments based on a global atmospheric model with a well-resolved stratosphere. Although culminating in autumn, the prescribed sea ice loss induces a near-surface warming that persists into winter and deepens as the SSW develops. The resulting temperature contrasts foster a deep cyclonic circulation over the North Pacific, which elicits a strong upward wavenumber-2 activity into the stratosphere, reinforcing the climatological planetary wave pattern. While not affecting the SSW occurrence frequency, the amplified wave forcing in the stratosphere significantly increases the SSW duration and intensity, enhancing cold air outbreaks over the continents afterward. 


AS40-A006
Contributions of Equatorial Planetary and Small-scale Gravity Wave Modes to the 2015/16 QBO Disruption Revealed in ERA5

Hyun-Kyu LEE+, Hye-Yeong CHUN#
Yonsei University, Korea, South

Contributions of the equatorial planetary waves (Rossby wave (RW), mixed Rossby-gravity wave (MRGW), Kelvin wave (KW), Inertio-gravity wave (IGW)) and small-scale gravity wave (SSGW) to the 2015/16 QBO disruption are examined using the ERA5 data, which have finer horizontal and vertical resolutions than some other global reanalysis data sets used in previous studies. Each wave mode is selected by frequency and horizontal wavenumber criteria, based on theoretical studies, in each month for 1 year from July 2015 to June 2016. The contributions of planetary wave modes are evaluated by calculating Eliassen-Palm flux divergence (EPFD), while those of SSGW are evaluated by considering both the EPFD of IGW with horizontal wavenumbers larger than 20 and parameterized gravity waves (PGWs) calculated from an offline convective GW parameterization. It shows that RWs contribute mostly to decelerating the westerly winds at 40 hPa during the disruption, with stronger contribution by meridional-propagating components than vertical-propagating ones. MRGWs weaken the center of the westerly jet, which leads to a favorable condition for RW breaking. The negative forcing by IGWs is gradually increased since November 2016, and it is larger than RW forcing after March 2016. The negative forcing by IGWs is mostly from small scale waves with horizontal wavenumber larger than 20, which is much larger than that from some coarse-resolution reanalysis data. The PGW forcing using ERA5 is smaller than that using coarse-resolution reanalysis data in some previous studies, as more IGWs are resolved from ERA5. Accordingly, forcing by SSGWs including both small-scale IGWs and PGWs in the present study is similar to that using coarse-resolution reanalysis data. The positive forcing by KWs is prominent nearly all month and altitude, except that SSGWs provide stronger positive forcing in March 2016 at 20 hPa where strong westerlies sustain by additional support from the vertical advection.


AS40-A009
Cloud Radiative Effects on the Stratospheric Brewer-Dobson Circulation

Kai-Wei CHANG1#+, Tristan L'ECUYER2, David HENDERSON2, Yun HANG3
1Chinese Culture University, Taiwan, 2University of Wisconsin-Madison, United States, 3Emory University, United States

The Brewer-Dobson circulation (BDC) is driven by dynamics and balanced by diabatic heating, which is dominated by radiative heating above the tropopause. Clouds interact with radiation and cause radiative heating perturbations which in turn can influence the BDC. This study evaluates how the ERA5 and MERRA-2reanalyses and satellite data represent the effects of cloud-induced radiative heating perturbations on the BDC. The stratospheric residual circulation is diagnosed using all-sky and clear-sky radiative heating, and the difference between the two solutions is interpreted to be the cloud effect on the BDC. Above 70 hPa, clouds in reanalyses induce positive upward velocity anomalies near the summer hemispheric poles, suggesting that clouds tend to dampen the high-latitude subsiding branch of the BDC. Below 80 hPa, the three separate estimates show little agreement, with ERA5depicting weak cloud effects while the MERRA-2 and satellite-based results are larger in impact but opposing signs. Satellite-based estimates show that tropical cirrus strengthen equatorial upwelling as well as tropics-to-subtropics meridional transport, while the MERRA-2 solutions suggest the opposite. This discrepancy is attributed to significantly larger tropical tropopause-level cloud ice water content in MERRA-2 compared to satellite radar/lidar retrievals, suggesting that unrealistically thick high-altitude clouds result in unrealistic cloud effects on the BDC. Results suggest that the properties and frequency of tropopause-level clouds strongly influence representation of the cloud effects on the shallow branch of the BDC.


AS40-A019
Atmospheric Gravity Wave Derived from the Neutral Wind with 5-min Resolution Routinely Retrieved by the Meteor Radar at Mohe

Chi LONG1#+, Tao YU2, Yang-Yi SUN2, Jian ZHANG2, Jin WANG1, Na YANG2, Xiangxiang YANG2, Hailun YE3
1China University of Geosciences (Wuhan), China, 2China University of Geosciences, China, 3University of Science and Technology of China, China

Atmospheric gravity waves (GWs) in the mesosphere-lower thermosphere (MLT) are crucial for the understanding of general circulation. However, their dynamical characteristics are hardly retrieved due to the difficulty in the high-resolution observation of wind. Therefore, this paper uses eight years (2013–2020) of meteor radar measurements in the MLT region at Mohe station (53.5°N, 122.3°E), China, to retrieve high temporal-resolution mesospheric wind data and further evaluate the temporal variation of GW kinetic energy. As the detected meteor trails exceed 6, the wind velocity is recalculated using the least square algorithm method, significantly increasing the temporal resolution of wind from 1 h up to 5 min. This resolution is sufficiently high for the investigation of GW kinetic energy, which exhibits a high spatial-temporal variability. For instance, it is enhanced in the winter season during the period of 0200 1400 UT and in the spring season during the period of 0800–1300 UT. The similarity between the climatological characteristics of GWs in MLT and the seasonal variation of GW total energy in the troposphere, determined from high-resolution radiosondes near to Mohe station, suggests that the meteorology in the lower atmosphere could be an important source of GWs in the MLT region.


AS40-A021
Disentangling the Drivers of the Brewer-Dobson Circulation Long-term Changes

Petr SACHA1#, Petr PISOFT1+, Radek ZAJICEK1, Roland EICHINGER1, Ales KUCHAR2
1Charles University, Czech Republic, 2Universität Leipzig, Germany

The meridional overturning mass circulation in the middle atmosphere, i.e. the Brewer- Dobson circulation (BDC), was first discovered before decades based on the distribution of trace gases and a basic analytical concept of BDC has been derived using the transformed Eulerian mean equations. Since then, BDC is usually defined as consisting of a diffusive part, and an advective, residual mean circulation. Climate model simulations robustly show that the advective BDC part accelerates in connection to the greenhouse gas induced climate change and this acceleration dominates the middle atmospheric changes in climate model projections. A prominent quantity that is being studied as a proxy for advective BDC changes is the net tropical upwelling, which measures the amount of mass advected by residual circulation across a given level (the tropopause, the stratopause, 70 hPa, 100 hPa isobar) and upwards. Another robust aspect of the changes in greenhouse gas concentrations is the changing structure of the atmosphere across layers. Particularly, it was debated whether the increasing BDC is not driven by the vertical shift of the circulation. We developed an analytical method that allows us to attribute the changes in tropical upwelling to kinematic causative factors such as the accelerating residual mean circulation, changing density of air, vertical shift of the circulation and for the first time, changes in width and geometry of the upwelling region. Here we demonstrate that this is the complete set of kinematic factors influencing the net upwelling and that all these factors are important contributions to the net upwelling trend depending on the level, where the upwelling is analyzed. In our presentation we describe the method and show its utilization on ERA5 and CMIP6 data for the shallow BDC branch and on CCMI models for the deep BDC branch and the transport between the stratosphere and mesosphere.


AS41-A004
A NASA GEO Imager Research Algorithm Dataset for Cloud Optical Properties, Part I: GEO Algorithm Description

Steven PLATNICK1#+, Kerry MEYER1, Robert HOLZ2, Galina WIND3, Nandana AMARASINGHE3, Steve DUTCHER2, Andrew HEIDINGER4
1NASA Goddard Space Flight Center, United States, 2University of Wisconsin, United States, 3Science Systems and Applications, Inc., United States, 4National Oceanic and Atmospheric Administration, United States

As the NASA Earth Observing System (EOS) program ages, the new generation of advanced operational weather satellites are natural successors for extending important imager cloud climate data records begun by MODIS. In addition, many of these low-Earth orbit (LEO) observations are expected to be coupled with like observations from the new generation of advanced geostationary (GEO) imagers (e.g., ABI, AHI, etc.), allowing for the possibility of a consistent LEO/GEO cloud product Program of Record (PoR) that can enable enhanced climate and process studies by NASA investigators and the broader research community. Note that a cloud product PoR is desired to provide critical synergy with the NASA Atmosphere Observing System (AOS), which is currently in formulation and designed to address the Aerosols, Clouds, Convection, and Precipitation Designated Observables identified by the 2018 NASA Earth Science Decadal Survey. Here, we give an overview of a NASA research cloud optical property algorithm for GEO imagers that was developed to be consistent, to the extent possible, with NASA cloud continuity products from LEO imagers (Aqua MODIS MYD06, VIIRS CLDPROP for Suomi NPP and NOAA-20). Challenges and approaches the team has taken to-date to best allow for GEO/LEO continuity will be summarized (e.g., the need for common geophysical algorithms across the sensor records to account for instrument differences along with forward radiative models, ancillary data sources, and inversion approaches). We will also discuss the need for a flexible computational infrastructure that that can provide a robust and flexible science algorithm testing and intersensory evaluation tools (including colocation and combined inter-sensor match files for on-orbit evaluation).


AS41-A007
Aerosol Products from the Pandora Asia Network

Ukkyo JEONG1#+, Limseok CHANG2, Hyunkee HONG2, Hanlim LEE1, Si-Chee TSAY3
1Pukyong National University, Korea, South, 2National Institute of Environmental Research, Korea, South, 3NASA Goddard Space Flight Center, United States

For validation of the recently launched GEMS (Geostationary Environment Monitoring Spectrometer), the Korean government has supported expanding the Pandonia Global Network (PGN) over the GEMS field of view by donating over 20 instruments to Asian Countries. Currently, over 8 instruments were deployed in Thailand, Mongolia, Indonesia, and Cambodia and we are aiming to install the rest of the units by the end of 2023. As one of Asia's top air quality priorities is aerosols, the NIER (National Institute of Environmental Research) is developing an additional aerosol inversion algorithm that can be used for various types of Pandora measurements. This presentation aims to share recent updates of the PAN (Pandora Asia Network) including aerosol retrievals which will be publicly available on the NIER website. Merits of simultaneous retrievals of trace gases and aerosols will also be presented.


AS41-A008
Spatial Gap-filling of Geostationary Satellite-derived PM10 and PM2.5 Concentrations by Combining Real-time Learning and Hybrid-random Forest and Regression Kriging

Seohui PARK, Jungho IM#, Hyunyoung CHOI, Dongjin CHO+
Ulsan National Institute of Science and Technology, Korea, South

Particulate matter (PM) is one of the most harmful atmospheric aerosols which have influenced adverse human health such as respiratory and cardiovascular disease. Rapid industrial and economic growth has resulted in a significant increase in PM10 and PM2.5 in East Asia. The aerosol optical depth (AOD) from the geostationary satellite is actively used to estimate ground-level PM10 and PM2.5 concentrations due to their high temporal resolution. Since satellite-derived AOD, however, is provided under high-quality conditions, there are spatially missing values due to the bright surface, cloud contaminations, and shadows. In this study, I proposed a machine learning-based hybrid-random forest and regression kriging (Hybrid-RFK) approach for filling gaps in the geostationary satellite-based ground-level PM10 and PM2.5 concentrations over East Asia. The AOD from the Geostationary Ocean Color Imager (GOCI) was mainly used to estimate satellite-based PM concentrations by real-time learning (RTL) model, while the hybrid-RFK was developed using the meteorological and land-based products without GOCI AOD to represent full-coverage PM distributions. The estimated PM concentrations by hybrid-RFK and the RTL-based PM models have been combined with each other for better performance in the AOD available region through gaussian filtering (i.e., combined RFK-RTL). In the clear sky, in which the AOD product is available, the RTL models (R2=0.91, rRMSE=20.79% for PM10 and R2=0.90, rRMSE=26.56% for PM2.5) show more improved performance than hybrid-RFK (R2=0.56, rRMSE=45.89% for PM10 and R2=0.83, rRMSE=32.22% for PM2.5) during the cases study period (i.e., 23 May 2015). One of the main reasons is whether the AOD values were used or not. Although the hybrid-RFK is comparatively low performed than RTL-models, the hybrid-RFK also shows good agreement with observed PM concentration for all sky conditions (R2=0.77, rRMSE =44.52% for PM10 and R2=0.81, rRMSE=36.60% for PM2.5) during the same cases study period.


AS41-A010 | Invited
Clouds Induced Modulations of the Atmospheric Processes

Som Kumar SHARMA#+, Dharmendra KAMAT
Physical Research Laboratory, India

Clouds are a vital part of the hydrological cycle and play an important role in the weather and climate of the earth-atmosphere system and play a crucial role in the modulation of the Earth’s radiation balance, dynamics, and thermal balance of the atmosphere. The impact of clouds on the radiation budget of the atmosphere depends on the cloud properties, such as their frequency of occurrence, the number of cloud layers, cloud base height, cloud thickness, spatial distribution, and water/ice content. An excess surface radiative heating produces instability in the atmosphere, resulting in convection and transfer of energy from the surface and its subsequent cooling and it affects the atmospheric circulation pattern which initiates several processes and affects the meteorology of the regions. Understanding the vertical distribution of clouds, their properties, and temporal evolution is essential for understanding the origin and impact of clouds and their feedback on the above-mentioned processes and their parameterization in weather and climate models for improving forecasts. This is correspondingly essential for investigating the cloud-aerosol interaction, heterogeneous chemistry in the atmosphere, and other associated processes. Cloud properties can be investigated using in-situ observations, ground-based lidar and radar remote sensing, airborne detectors, and space-borne payloads (onboard satellites). These techniques and observing platforms are having their advantages and limitations. Lidar and Radar-based observations are having very good temporal and vertical resolution but have limited spatial coverage. Satellite observations have the advantage of providing global distribution of clouds. In this talk investigation of the atmospheric processes which are modulated due to clouds will be presented. Furthermore, the observation of clouds using various techniques and the implication of the advanced techniques in improving the understanding of atmospheric clouds will also be discussed and presented.


AS41-A012
Working Towards Dark Target Aerosol Product Synergy Among Geo and Leo Sensors

Yingxi SHI1#+, Shana MATTOO2,3, Pawan GUPTA3, Lorraine REMER1,4, Virginia SAWYER3, Yaping ZHOU1
1University of Maryland, Baltimore County, United States, 2NASA Science Systems and Applications, Inc., United States, 3NASA Goddard Space Flight Center, United States, 4Airphoton LLC, United States

Aerosols are one of the major components that affects climate and air quality. Being able to measure global aerosol comprehensively has been a major goal for the last several decades. Now with the increasing number of sensors that are capable of retrieving aerosols on both geostationary orbit (GEO) and low-Earth orbit (LEO), getting a complete picture of global aerosol distribution is more achievable than ever. However, how to use these data with various temporal and spatial resolution synergistically is one of the urgent questions that needs to be answered before combining products. Using a consistent Dark Target algorithm on three GEO sensors (two Advanced Baseline Imagers (ABI) on GOES-E and GOES-W and Advanced Himawari Imager (AHI) on Himawari-8) and three LEO sensors (Moderate resolution Imaging Spectrometers (MODIS) on Terra and Aqua and the Visible Near-Infrared Imaging (VIIRS) on Suomi-NPP), we evaluate six level 2 DT aerosol optical depth (AOD) products against Aerosol Robotic Network (AERONET) as well as Marine Aerosol Network (MAN) and investigated the similarity and differences among the products with a special focus on the two GEO and LEO common regions, namingly North America and East Asia. The error statistics of these products are generated against observing conditions with major uncertainty sources identified. Our results provide baseline evaluation results before synergy of DT aerosol products can be pursued.


AS42-A005
The Capability of X-band Radar for Diagnosing the Trigger and Developing Convective Rainbands in the Gap Area of a C-band and S-band Radar Network

Yabin GOU1#+, Haonan CHEN2
1Hangzhou Meteorological Observatory, China, 2Colorado State University, United States

It is cost-effective to use X-band polarimetric radar to fill the large gap between C-band or S-band radar networks for severe weather monitoring and nowcasting; however, X-band radar suffers more attenuation than C- and S-band due to its short-wavelength characteristics, particularly in convective situations. In this work, a combined utilization of a radar network, which includes a C-band radar in Hangzhou located on the top of a western mountain (1512 m), an S-band radar in Ningno near the East Sea (454 m), as well as an X-band radar (816 m) located in their vertical gap, is used to demonstrate the capability of X-band radar in analyzing the developing convective rainstorms, after the attenuation correction for horizontal reflectivity (ZH) of all three radar. The result shows that (i) after the significant attenuation on ZH is corrected based on the self-consistency approach, X-band radar exhibits finer and even larger ZH than S- and C-band radar when it captures the lowest part of the convective rainbands relative to the other two radars. (ii) The trigger and developing convective rainbands occurred on the lower atmospheric layers, which are insignificant in the view of S- and C-band radar because of longer distances, are all well captured by the X-band radar in their gap area. (iii) Benefiting from the nearest distance, S-band radar afterward captured the lowest developing part of another convective rainband with the most significant ZH, which is different from but similar to that captured by X-band radar. In these senses, the X-band radar effectively favors diagnosing the trigger and developing of convective rainstorms in the gap area of this S- and C-band radar network.


AS42-A007
Precipitation Microphysical Processes in the Tropical Cyclone Inner Rainband and Tropical Squall Line Revealed by Polarimetric Radar

Hepeng ZHENG#+, Yanqiong XIE, Yun ZHANG, Zuhang WU
National University of Defense Technology, China

Polarimetric radars provide new insights into the precipitation microphysical processes and characteristics in a tropical cyclone (TC, Kajiki 2019) inner rainband and a tropical squall line in the South China Sea. The precipitation of Kajiki is dominated by high concentrations and small (< 3 mm) raindrops, which contribute more than 98% to the total precipitation. The formation of precipitation in the inner rainband of Kajiki is dominated by warm-rain processes, and accretion and coalescence play a critical role in the formation of heavy rainfall. At the same time, the melting of different particles generated by the ice process has a great influence on the initial raindrop size distribution (DSD). The aloft DSD above heavy rain with the effect of graupel has a wider spectral width compared with the region affected by dry snow. A tropical squall line was also documented. The ZH is similar for both convective systems, while the ZDR (KDP) is higher (lower) at the front of the squall line, indicating a low concentration of large drops; the peak values of ZH, KDP, and ZDR in the inner rainband are all concentrated in the convention center. The trend of liquid water content toward the ground within the squall line is consistent with that of the inner rainband, while the mean value is lower, and is more affected by ice processes. This work may contribute to our understanding on cloud microphysics of tropical convective systems using polarimetric radars.


AS42-A011
Precipitation Structures and Convective Characteristics of MCSs Associated with Different Large-scale Circulations Over Southern China

Hao CHEN1#+, Weixin XU1, Jiaolan FU2, Nana LIU3, Jianhua SUN4, Lejian ZHANG5
1Sun Yat-sen University, China, 2National Meteorological Center of China Meteorological Administration, China, 3University of California, United States, 4Chinese Academy of Sciences, China, 5Meteorological Detection Center of China Meteorological Administration, China

Mesoscale convective systems (MCSs) are frequent in Southern China (SCH) during warming season and can result in severe weathers. While the large-scale circulations and precipitation patterns of MCSs over SCH have been well studied, studies on finer-scale (meso- and micro-) structures of MCSs are still limited, especially changes in MCS structures associated with different large-scale circulations. In this study, we first identify and track nearly three warm seasons of MCSs over SCH using operational radar network data in China. Multi-source observations are then collocated into MCSs to examine the precipitation intensity, horizontal organization, vertical structure, and ensemble microphysics of MCSs. MCSs are stratified by six types of large-scale circulations, including front (7%), southwest vortex (SW-Vortex, 15%), trough (10%), tropical cyclone (TC, 18%), South China Sea vortex (SCS-Vortex, 10%), and other (40%). Our results reveal significant variations in the precipitation structures and convective characteristics of MCSs developed under various large-scale circulations. For example, MCSs of SW-Vortex and trough types exhibit the strongest and deepest convection as indicated by radar and IR observations, but the trough-type MCSs have a much smaller precipitation area and a shallower column of ice particles (microwave-based) likely due to a drier troposphere. Interestingly, MCSs associated with TCs and SCS-Vortex have the weakest convective intensity and the least lightning density, although they produce heavier precipitation at the surface. Mechanisms responsible for the variations in meso- and micro-scale structures among MCSs produced by various types of large-scale circulations will be further investigated.


AS42-A017
Beam Blocking Mitigation of X-band Radar Data and its Application for QPE Improvement of S-band Radar Network

Daehyung LEE1, Choeng-Lyong LEE1, SeungWon BAEK1#+, Geunsu LYU1, Wonbae BANG1, Park HONG-MOK1, Alexander RYZHKOV2, Gyu Won LEE1
1Kyungpook National University, Korea, South, 2NOAA/OAR/National Severe Storms Laboratory, United States

Two X-band dual polarimetric radars were installed in the Seoul metropolitan area to supplement the limitation of low-level observation of the S-band radar network. High spatiotemporal resolution data of the X-band radar can be useful for flash flood monitoring and forecasting. However, there were unexpected beam blocking areas caused by artificial buildings, trees and terrain which cannot be detected using DEM (Digital Elevation Model) based on beam blocking simulation results and the real time beam blocking detection (consisting of the standard deviation of radar variables and co-polar cross-correlation coefficient). The frequency of occurrence of dual-polarization parameters (FOD) technique, an extended method of the frequency of occurrence of reflectivity technique (FOR, Chang et al. 2009) was used in this research to improve the beam blocking detection. This method is applied to the beam blocking detection and identifies ground clutter using feature parameters consisting of dual-polarization parameters (ZDR, ρHV), proxy quantity dubbed depolarization ratio (DR) and their statistical variation (horizontal and vertical standard deviation, average, texture, etc.). The blockage areas are categorized using fuzzy logic based on FOD parameters. Different types of HSR masks (beam blocking simulation with DEM, real time beam blocking, FOR and FOD) were applied to Hybrid Surface Rainfall (HSR, Lyu et al. 2015) estimation with various methods (R(ZH), R(ZH, ZDR), R(ZH, KDP), R(ZH, KDP_P) and R(ZH, AH)) to validate effect of FOD. QPE accuracy of the X and S-band radar was validated with rain gauges and compared with the QPE of S-band radar.

Acknowledgment
This work was supported by the National Research Foundation of Korea (NRF) grant funded by the Korea government (MSIT) (No. 2021R1A4A1032646). This work was funded by the KMA Research and Development Program “Observing Severe Weather in Seoul Metropolitan Area and Developing Its Application Technology for Forecasts” under Grant (KMA2018-00125).


AS42-A018
Improved Combination of Different Disdrometers Data for Complete Drop Size Distribution

Sanghun LIM1+, Wonbae BANG1, Kyuhee SHIN1, Kwonil KIM2, Viswanathan BRINGI3, Merhala THURAI3, Gyu Won LEE1#
1Kyungpook National University, Korea, South, 2Stony Brook University, United States, 3Colorado State University, United States

Raindrop Size Distribution (DSD) has been studied since the late 19th century by observing different disdrometers. Especially, the 2D-video disdrometer (2DVD) was widely used in many studies because the 2DVD has relatively high accuracy for the measurement of physical variables of drop by using two orthogonal optical cameras with high performance. However, the 2DVD data tends to underestimate the concentration of small raindrops, especially drop diameters below 0.7 mm. Against the underestimation issue, recent studies have tried to combine 2DVD data with Meteorological Particle Spectrometer (MPS) data showing a more realistic number concentration of small drops. Simply, the complete DSD is adding 2DVD DSD above 1.125 mm channel and MPS DSD less than 1.125 mm. Meanwhile, the complete DSD can be discontinuous when the number concentration difference between 2DVD and MPS nearby the binding point is too large. In this study, we propose an improved combination method based on the weighting factor. The new complete DSD was produced by applying the distance weighting factor between 2DVD and MPS about a specific drop channel range 1 mm to 1.25 mm. We compare the rainfall rate between the original complete DSD and the new complete DSD as a reference to Pluvio data. The comparison for summer rainfall events in 2022 in Incheon, South Korea shows the new complete DSD has relatively higher skill scores. We will also compare radar reflectivity between the two methods as a reference to Precipitation Occurrence Sensor System (POSS) data.

ACKNOWLEDGEMENT
This work was supported by the National Research Foundation of Korea (NRF) grant funded by the Korea government (MSIT) (No. 2021R1A4A1032646).


AS42-A019
Investigating the Potential Interaction Between Updraft and Microphysical Processes Near the Dendritic Growth Layer

Ji-Hye JUNG1+, Kwonil KIM2, Kyuhee SHIN1, Gyu Won LEE1#
1Kyungpook National University, Korea, South, 2Stony Brook University, United States

The dendritic growth layer (DGL) at an altitude of about -15 °C plays an important role in the production and growth of snowfall. In the DGL, the difference in saturated vapor pressure between ice and water is maximized, resulting in the rapid growth of dendritic ice particles and increasing ground precipitation. Despite the research efforts in previous studies, the microphysical characteristics of snowfall in the DGL and its role in the dynamical and thermodynamical processes are not yet fully understood. In particular, noticeable updrafts and bimodal particle size distribution in the vicinity of DGL are often observed, but their underlying mechanism remains unknown. Recently, Ye and Lee (2021) established a hypothesis that the generation of new small particles is favorable due to the supersaturation associated with the updrafts below.In this study, we will try to reveal the interaction between updrafts and snowfall microphysics in the DGL by using data from intensive observations during the ICE-POP 2018 (International Collaborative Experiments for Pyeongchang 2018 Olympic & Paralympic winter games). We analyzed the vertical profiles of polarimetric radar variables from surveillance radar, the Doppler spectrum of vertically pointing radar, and the 3-hr rawinsonde data. Furthermore, the vertical air velocity estimation technique was applied to the vertically pointing radar to quantify the updraft in the DGL. The three analyzed cases revealed the presence of the updraft around -15℃. There was an increase in reflectivity, a maximum value of differential reflectivity and specific differential phase, and a decrease in the cross-correlation coefficient in the region where the updraft was at its maximum intensity. We will suggest the possible mechanisms of the generation of small particles and updraft.

ACKNOWLEDGEMENT
This work was supported by the National Research Foundation of Korea (NRF) grant funded by the Korea government (MSIT) (No. 2021R1A4A1032646).


AS43-A001
Retrieving the Atmospheric Motion Vectors from the Geostationary Satellite Images by Using the Convolutional Neural Network

Renge ZHOU#+, Keyi CHEN
Chengdu University of Information Technology, China

Atmospheric motion vectors (AMVs) are of great significance for constructing initial fields of the numerical weather prediction and analyzing damaging weather processes such as typhoons and heavy precipitation. Based on the convolutional neural network (CNN) architecture, this study uses transfer learning in deep learning strategy to retrieve the AMVs from the infrared and water vapor images of the geostationary satellites Himawari and FY-4A respectively, and finally the output of the neural network model is stitched and merged to obtain the AMVs within the same observation area of the two satellites. The results show that CNN can effectively acquire the information from the satellite images and convert it into vector wind fields at various height layers. Compared with the traditional algorithms, AMVs retrievals with machine learning algorithms have the features of no requirements for the height assignment, the ability to display the complete atmospheric circulations at different height layers and the uniform AMVs distribution in the vertical direction.


AS43-A004
Enhancing Typhoon Precipitation Nowcasting via Spatial and Temporal Difference in Deep Learning

Hongyi YAO#+, Ji CHEN
The University of Hong Kong, Hong Kong SAR

Tropical cyclones (TCs) always bring torrential rains triggering loss of property, even lives. Nowcasting heavy rainfall from TCs within 2 hours is thus an important topic in meteorology and hydrology. Traditional numerical weather forecasting fails to provide accurate results due to spin up in such short lead time while deep learning-based extrapolation has proven its potential. In this work, we proposed a multi-tasking learning framework to forecast the rotating features of TCs. Spatial and temporal difference (STD) are coupled with structural similarity (SSIM) to better predict periphery rainfall bands and rotation. The framework adopted two different backbones namely convolutional long short-term memory (ConvLSTM) and U-Net neural network with fed of radar reflectivity composite. The results showed that: (1) the coupling of STD and SSIM could significantly increase performance matrix compared to traditional deep learning with SSIM loss function only. The average improvement of critical success index (CSI) of 30 dbZ are 84% and 8.9% in ConvLSTM and U-Net, respectively, and the decreasing of mean absolute error (MAE) are 7.1% and 4.6%. (2) The movement of TCs, including transformation and rotation are observed in our proposed framework, indicating the effectiveness of spatial and temporal difference. However, the blur issue exists, especially with lead time over 1 hour, which calls for physical driving coupled in deep learning.


AS43-A006
Application of ConvLSTM and Optical Flow Method Integration in Extreme Precipitation Nowcasting

Hongxu ZHU#+, Ji CHEN
The University of Hong Kong, Hong Kong SAR

In recent years, extreme precipitation has brought serious losses, accurate and timely forecasting of extreme precipitation has become more and more important. This study analyzes the radar echo data of some extreme precipitation in Shenzhen using Convolutional Long Short-Term Memory (ConvLSTM) network. Based on the radar echo data, our study calculates the optical flow field by variational echo tracking (VET) method, which is added to model input and prediction respectively. This study also explores why optical flow field can improve the performance of the model. The outcome shows that the total loss is reduced by approximately 7% compared with pure ConvLSTM when the optical flow field is added to model input, and 12% when it is also added to model prediction. It is also shown that the ConvLSTM model with optical flow field as additional input is equal to a more complex ConvLSTM model since optical flow field calculated by radar echo data can’t provide more real-world information. Meanwhile, when optical flow field is also added to model prediction, the model performs better because additional information is considered, which also provides the basis for combining with numerical weather forecast results.


AS43-A007
Hybrid Hydrodynamic-machine Learning Modeling-based Flood Susceptibility Analysis Under Climate Change

Weifeng WU+, Chia-Jeng CHEN#
National Chung Hsing University, Taiwan

Climate change will induce more extreme rainfall events, leading to less reliable flood susceptibility analysis based on the existing hydrological handbook. To better distinguish flood-prone areas in a more variable environment, this study aims to propose a hybrid assessment framework that uses a hydrodynamic model referred to as the Two-dimensional Runoff Inundation Toolkit for Operational Needs (TRITON) and three machine learning models, namely Convolutional Neural Networks (CNN), Random Forest (RF), and Support Vector Machine (SVM), for flood susceptibility analysis in Changhua county, Taiwan. TRITON, which makes use of graphics processing units to achieve high-performance computing, simulates Probable Maximum Precipitation (PMP) and Probable Maximum Flood (PMF) in various scenarios to identify flood susceptible sites that are adopted as the training and validation points for the machine learning models to develop flood susceptibility mapping. Preliminary results show that the “very high” flood susceptibility category accounts for 13% to 20% under the SSP5-8.5 scenario, suggesting a 6% increase compared to the baseline analysis. It is expected that the hybrid modeling framework can not only deal with data scarcity regarding historical flood susceptible sites but also produce flood susceptibility maps for disaster preparedness.


AS43-A008
A Comparative Study on Rainfall Nowcasting Using Deep Learning Methods

Xianqi JIANG+, Ji CHEN#
The University of Hong Kong, Hong Kong SAR

With the requirement of high accuracy and short responding time, rainfall nowcasting has become a significant challenge for weather authorities to provide timely and accurate alerts of floods to the public. Hence, three state-of-the-art deep learning models, the Convolutional Long Short-Term Memory (ConvLSTM), the Trajectory Gated Recurrent Unit (TrajGRU), and the Predictive Recurrent Neural Network (PredRNN), are trained and tested for rainfall nowcasting with a newly collected radar echo maps dataset provided by the Meteorological Bureau of Shenzhen Municipality in China. All three deep learning models outperform the traditional optical flow-based extrapolation method in all performance metrics, improving the performance by up to 63%. Performances of those models are further compared and discussed with three typical cases of different rainfall intensities in South China, showing the prediction accuracy for 0-2 hours nowcasting using deep learning. Data fusion between different cities in the same area is also tested for the building of high-quality rainfall dataset for nowcasting tasks. The difference is less than 5% when the model has multiple data sources which proves the robustness of the deep learning models. Analysis are carried out regarding the effectiveness of deep learning techniques on rainfall nowcasting, suggesting ways of improvement in the future.


AS43-A016
Whether Raises the Embankment is Enough for Future Climate Change - A Study to Predict River Water Level in Coastal Basins Using a Hybrid Machine Learning Model Framework

Shaoxu ZHENG1,2#+, Zhan TIAN1, Yingping ZHAO3, Qian KE4
1Southern University of Science and Technology, China, 2Southern University of Science and Technology, China, 3Pengcheng Laboratory, China, 4Erasmus University Rotterdam, Netherlands

Making sure of the safety of embankments, which are powerful measures to prevent river from flooding thus safeguarding people’s lives and property, is crucial, especially when human society is under rapid development and the impacts of climate change are becoming bigger and bigger. However, engineering measures previously constructed may not meet the risk resistance requirements at the time of embankments construction. This study evaluates the resilience of embankments against future risks of Maozhou River as a case study, which is a cross-border river connecting to the Pearl River Estuary. The modelling of water dynamics in coastal basins is very complex and challenging, for flood events in estuary areas are often compounded by extreme rainfall and tidal patterns. To overcome this challenge, this study uses the water level data of Maozhou River in Shenzhen, China and employs wavelet transform method to decompose the water level data into two time series parts: direct runoff related part and base flow related water level part, which correspond to the part influenced by precipitation and the part by tidal events, respectively. These two parts time series data are modelled separately using a hybrid machine learning model framework, and then combined together for the final composite water level analysis. This method preprocesses water level based on the rainfall-runoff process and can significantly improves model’s prediction performance when compared with models that simply uses rainfall and tidal events as covariates. Finally, with our method, using the rainfall data predicted from IPCC6, this study forecasts the future changes in water level with better accuracy, providing a scientific evaluation method for embankment safety.


AS44-A001
Atmospheric Contributions of Water-soluble and Water-insoluble Nitrogen and Phosphorus Species to the Southern East China Sea

Hung-Yu CHEN#+, Meng-Lun CHEN
National Taiwan Ocean University, Taiwan

From Oct-2019 to Sep-2020, a high-volume sampler was used to monitor atmospheric dry deposition over Mazu Island which is located at the southern end of the East China Sea. The collected samples were divided into coarse particles and fine particles using a six-stage particle size separator, and the nitrogen (N) and phosphorus (P) species were categorized as either water-soluble (WS) or water-insoluble (WI). In this study, WS-TN and WI-TN accounted for 74% and 26% of TN, while WS-TP and WI-TP accounted for 47% and 53% of TP, respectively. According to the historical literature, the proportions of WI-TN and WI-TP in TN and TP are 39-51% and 95% in inland areas, which are significantly higher than 8-26% and 53-63% observed in coastal atmospheres. Correlation analysis results showed that there was a high correlation between WS-TN and WI-TN (r = 0.79, p < 0.01) and a moderate correlation was noted among nss-K+, nss-Ca2+, and nss-SO42-. The results show that WS-TP and WI-TP may be derived from fossil fuel combustion and biomass combustion, respectively. In terms of particle size distribution, the ratios of the concentrations of WS-TN, WI-TN and WS-TP within fine particles are 72%, 93% and 72%, respectively. However, WI-TP displays the opposite pattern since the proportion of fine particles is only 37%. Flux calculation results show that the annual fluxes of TN and TP are 48.4 and 0.29 mmol m-2 yr-1, respectively. Both TN and TP had the highest average daily flux during winter; of these, up to 88% of the annual N flux consisted of WS species. On the other hand, approximately 69% of P was dominated by WI species. The above results show that N has a higher bioavailability than P in the areas, which may cause nutrient imbalances in adjacent ecology. 


AS44-A008
Abundant Nitrogenous Secondary Organic Aerosol Formation Accelerated by Cloud Processing

Zhe LIU#+, Jianmin CHEN
Fudan University, China

Nitrogenous organics (CHONs) are one of the most important components of secondary organic aerosol (SOA). However, the formation mechanism of CHONs in clouds has rarely been studied. Here, we observed the evolution of CHONs during cloud processes (CPs) and found that CPs significantly enrich the diversity of CHONs, specifically generating CHONs with O numbers of 1–10 and double bond equivalent (DBE) values of 2–10, which can be described by the formula CnH(2n-16)–(2n)O1–10N1–4. We proposed that the CHONs formed during CPs are likely formed through aqueous phase reactions with CHO compound precursors via nucleophilic attacks by NH3. Nearly 77% of the CHONs in cloud water can be accounted for by this scheme, and 66% of all CHONs are formed through reactions between NH3 and carbonyl-containing biogenic volatile organic compound (BVOC) ozonolysis intermediates. This study provides the first insights into the evolution of CHONs during CPs and reveals the significant roles of CPs in the formation of CHONs.


AS44-A010
The Impact of Clean Heating Reform on the Size Distribution of Nitrated Phenols and its Association with Biomarkers of Homemakers in the Fenwei Plain, China

Rong FENG+, Hongmei XU#
Xi'an Jiaotong University, China

The clean heating renovation has been executed for improving particulate matter (PM) pollution in northern China since 2017. This study determined particle size distributions of nitrated phenols (NPs) in personal exposure (PE) samples and its associations with biomarkers in saliva and urine from homemakers in rural households of the Fenwei Plain, China. Remarkable reductions of 28.6–66.3% and 52.2–82.4% on PMs and total quantified NPs were found with the substitutions of raw coal chunk and biomass by advanced clean coal. 4-Nitroguaiacol (4NG) showed the largest reductions of 81.2% among individual NP. In addition, the clean coal efficiently reduced interleukin-6 (IL-6) and 8-hydrox-2'-deoxyguanosine (8-OHdG) in the urine and saliva by 12–72%. Furthermore, significant positive correlations between urinary 8-OHdG with most of NPs in all particle sizes, urinary IL-6 with 4NG for particles with Dp > 2.5 µm and Dp = 0.25–1.0 µm, salivary IL-6 with 4-nitrocatechol (4NC) and 4-methyl-5-nitrocatechol (4M5NC) for particles with Dp > 2.5 µm, Dp = 0.5–1.0 µm, and Dp < 0.25 µm were observed, but not for salivary 8-OHdG or PMs. The results provide scientific support for the clean energy reformation and demonstrate the strong particle size dependence between NPs and biomarkers.


AS44-A011
Modeling the Regional Nitrogen Cycle in the Atmosphere and its Response to the Future Emission Control Strategy

Qi FAN#+
Sun Yat-sen University, China

The characteristics of the regional nitrogen cycle have not been fully understood and its response to the future emissions control strategy is warranted. Here, we used the WRF-CMAQ model to reveal the regional nitrogen cycle (emissions, concentrations, and depositions) in the atmosphere in January (winter) and July (summer) 2015 and anticipate its changes under emissions control by 2030 in YRD. The model has reasonable simulations for the meteorological factors, chemical concentrations, and depositions in 2015. The results show that the nitrogen concentration (deposition) is generally higher (lower) in January than in July due to higher precipitation and dry deposition velocity in summer. Local emissions of YRD are the major contributors to the concentration in this region. For the deposition, HNO3, NH3, NO3-, and NH4+ are the major species. The depositions of oxidated nitrogen and reduced nitrogen account for 62% and 38% of the total nitrogen deposition in January, while their proportions are 51% and 49% in July. To achieve the carbon peak emission in 2030, the NOx and NH3 emission is projected to reduce by ~51% and ~22%, respectively. The concentration and deposition of oxidated nitrogen will decrease by ~50%, generally in consist with the reduction of NOx. However, the NO3- concentration is less responsive to the emission reduction in January because the contribution of NOx reduction will be offset by the increase of atmospheric oxidation capacity during nighttime. The lower reduction of NOx than NH3 results in a higher proportion of reduced nitrogen than oxidated nitrogen in deposition. In addition, the smaller reduction of reduced nitrogen wet deposition than sulfur wet deposition and oxidated nitrogen wet deposition can raise the pH of precipitation and help alleviate the acid rain problem, especially in July.


AS47-A001
Changes to the IMERG Algorithm from V06 to V07

George J. HUFFMAN1, David BOLVIN2, Eric NELKIN2, Robert JOYCE2, Jackson TAN3,1#+
1NASA Goddard Space Flight Center, United States, 2Science Systems and Applications, Inc., United States, 3University of Maryland, Baltimore County, United States

The Integrated Multi-satellitE Retrievals for GPM (IMERG) product from the U.S. Science Team of the Global Precipitation Measurement (GPM) mission provides estimates of surface precipitation rate at 0.1° every half-hour globally, with three different Runs to cater to various latency requirements. The latest version (V07) of IMERG, which involves a uniform reprocessing of the full 20+ years of record spanning the TRMM and GPM projects, includes numerous changes to the algorithm that are expected to improve the precipitation estimates in different ways. This poster will describe the major changes in the algorithm from the previous V06 to latest V07 and show examples of the associated improvements. One prominent issue with IMERG V06 is an overestimation of the satellite-only precipitation estimates, especially during the TRMM era; this poster will summarize the cause and the solution adopted in V07. Another issue that was identified in the development of V07 is a 0.1°-eastward spatial offset in the gridded microwave estimates and hence most of the inputs; this poster will demonstrate the improvement resulting from the correction. As well, changes to the Kalman filter in IMERG are expected to improve the distribution of estimated precipitation rates and mitigate the differences arising from the use of diverse types of sensors. Other changes in V07 include a modification of the motion vector source to address deficiencies in the precipitation propagation near orography, a modernized infrared precipitation algorithm, an update to the precipitation phase parametrization for improved consistency, and a renewed effort to implement climatological gauge adjustment to the near-real-time Runs. These enhancements in IMERG V07 are focused on the goal of providing the community with a long record of reliable high-resolution precipitation observations.


AS47-A004
GPCP Version 3.2 Products and Results

George J. HUFFMAN1#+, Ali BEHRANGI2, Robert ADLER3, David BOLVIN4, Eric NELKIN4, Guojun GU3, Mohammad Reza EHSANI2
1NASA Goddard Space Flight Center, United States, 2University of Arizona, United States, 3University of Maryland, United States, 4Science Systems and Applications, Inc., United States

The Global Precipitation Climatology Project (GPCP) products address the need for long-term precipitation products that emphasize homogeneity, following Climate Data Record (CDR) principles.  The new-generation Version 3.2 provides key improvements over the operational Version 2.3 such as: finer spatial resolution of 0.5°x0.5°; wider geosynchronous infrared estimation (58°N-S) upgraded with the PERSIANN-CDR algorithm; upgraded retrievals from selected passive microwave sensors (GPROF algorithm) that calibrate the IR input; revised intercalibrations of TOVS and AIRS data (used at high latitudes); climatologies based on CloudSat, TRMM, and GPM to provide overall calibration by modern satellite estimates; the latest Global Precipitation Climatology Centre (GPCC) precipitation gauge analyses over land areas; regional modifications to the gauge undercatch correction; and IMERG half-hourly data input to the Daily V3.2 product. We will show sample analyses that demonstrate aspects of the Version 3.2 precipitation record, such as the global climatology, the time series for global land and ocean total precipitation and snowfall, and the time series of tropical land and ocean daily precipitation rate histograms.  For selected analyses we will show improvements in both the Monthly and Daily products in Version 3.2 compared to the operational Version 2.3.  In particular, the climatological zonal profile of precipitation in the Southern Ocean, extending south of 40°S, improves a suspected artifact in V2.3.  Similarly, the Daily histograms over ocean in Version 3.2 lack the jump in the predecessor Version 1.3 Daily over ocean at the start of 2009, although a smaller jump is introduced in June 2014. The presentation will conclude with a prospectus for the future satellites/sensors and community datasets necessary to continue computation of a consistent CDR product on the one hand, while also potentially contributing to improvements in the historical record.


AS47-A005
Quantitative Evaluation of Graupel Shape Observed by Particle Imaging Radiosonde "Rainscope" in Baiu Convective Cloud

Yurika HARA1+, Kenji SUZUKI1#, Tetsuya KAWANO2
1Yamaguchi University, Japan, 2Kyushu University, Japan

A new balloon-borne precipitation particle imaging radiosonde named "Rainscope" has been developed. The decisive difference between the Rainscope from the ground-based disdrometer is that it can know the vertical distribution of microphysical parameters. In other words, from the liquid phase to the ice phase such as graupel and snowflakes that exist above the freezing level, their types, shapes, sizes, spatial concentrations, etc. in clouds are provided. It is a powerful tool for the ground validation of remote sensing techniques. For example, it can provide observational data useful for the validation of GPM DPR products such a "binHeavyIcePrecipTop", which was newly released in 2021 and shows the upper end elevation of strong solid precipitation in clouds below -10ºC. The Rainscope was first deployed in the intensive observation campaign, which was conducted in Kyushu region during the Baiu rainy season in 2022. It was launched into convective clouds with active lightning and gust on 25 June 2022. It transmitted images of ice particle in the process of melting just below 0ºC, and frozen particles with semi-transparent and smooth outlines around 0ºC. And white and irregularly shaped graupel were observed across all layers up to -30ºC level. The clear particle images captured by the Rainscope enable us to get more detailed information of particle shapes, surface conditions, and contours, making it easier to evaluate their shapes quantitatively. The circularity of graupel was smaller in upper layer. It has a longer circumference and more irregular shapes, suggesting an active riming process originated from ice crystals. On the other hand, graupel in lower layer with larger circularity was suggested to be originated from a frozen particle. The different graupel formation processes was considered to exist in convective clouds.


AS47-A009
Investigation of Moving Vector Calculation at High Latitudes Using NEXRA Data for Polar Extension of the GSMaP PMW-IR Combined Algorithm

Munehisa YAMAMOTO1#+, Takuji KUBOTA1, Ying-Wen CHEN2
1Japan Aerospace Exploration Agency, Japan, 2The University of Tokyo, Japan

The Global Precipitation Measurement (GPM) project leads the global distribution of precipitation by combining observations from multiple microwave radiometers (PMWs) onboard low Earth orbit satellite. Since temporal resolutions shorter than 3 hours cause sampling gaps only by PMW observations, a combined PMW-infrared (IR) combined algorithm has been developed to interpolate precipitation areas based on cloud areas and their moving vectors using IR images from geostationary meteorological satellites. It is difficult to accurately capture cloud areas at high latitudes due to radiometric effect at large zenith angle from the geostationary Earth orbits. Therefore, the coverage of major PMW-IR combined satellite precipitation map products has been limited to the equatorial region below 60 degrees latitude. The Global Satellite Mapping of Precipitation (GSMaP) product version 05 (algorithm version 8), released in December 2021, provides precipitation estimation up to the poles only in the PMW observation area. However, a polar extension of the PMW-IR combined algorithm has been expected to fill the remaining PMWs sampling gaps. This study examined the derivation of moving vectors using Nonhydrostatic Icosahedral Atmospheric Model-Local Ensemble Transform Kalman Filter (NICAM-LETKF) Japan Aerospace Exploration Agency (JAXA) Research Analysis (NEXRA), which is in regular operation together with GSMaP to extend the PMW-IR combined algorithm to the polar regions. The moving vectors of column water vapor and precipitation were calculated by modifying the current version of GSMaP moving vector calculation program to extend poleward and to allow the use of geophysical quantities other than IR. In this presentation, we will compare the results with other numerical weather forecast data used in previous studies and discuss issues for their use.


AS47-A011
Analysis of the Environment and Precipitation Characteristics of Widespread Extreme Rainfall Events During the Akisame Season

Yukari TAKAYABU#+, Aiko NARITA
The University of Tokyo, Japan

Akisame season is the autumn rainy season in Japan, with heavy rainfalls particularly recorded in eastern Japan. However, research on heavy rainfalls in the Akisame season is not as sufficient as those for the Baiu season. The objective of this study is to clarify the environment and precipitation characteristics of widespread heavy rainfalls during the Akisame season. We utilized gauge data collected by the Automated Meteorological Data Acquisition System (AMeDAS) stations for 1979-2020 to define the widespread heavy rainfalls. Japanese 55-year Reanalysis (JRA-55) and rainfall data from the Global Satellite Mapping of Precipitation (GSMaP) are utilized to analyze the environments and rainfall distributions. GPM/DPR data are utilized to examine the characteristics of rainfall events embedded in the widespread heavy rainfall events in Akisame season. Widespread extreme precipitation event cases in western Japan in Baiu season and in eastern Japan in Akisame season are compared. A northwest-southeast dipole structure in the geopotential height anomalies is found from the lower to upper level for the Baiu case, while a northeast-southwest dipole structure is found in the Akisame case. These different structures of anomalous field tend to enhance the water vapor flux associated with the different mean large-scale circulations in the two rainy seasons, preparing large precipitable water field. Next, three-dimensional rainfall characteristics are examined with the GPM/DPR overpasses for four representative cases of widespread extreme precipitation events in Akisame/Eastern Japan cases. Two of the four representative cases are associated with precipitation systems with strong convective precipitation. Other two cases are characterized as organized precipitation systems with very intense precipitation, but with moderate heights. The latter cases are similar to the precipitation system observed in the record-breaking extreme rainfall event in July 2018.


AS47-A013
What Do the Latest Global Oceanic Precipitation Estimates from GPM V7 and GPCP V3.2 Products Tell Us?

Ali BEHRANGI1#+, Yang SONG2
1University of Arizona, United States, 2Hohai University, China

Satellite observations have brought opportunities to quantify the amount and distribution of precipitation over the globe, critical to understand how the Earth system works. The amount and spatial distribution of oceanic precipitation from the latest versions (V7 and the previous version) of the Global Precipitation Measurement (GPM) core-instruments and the constellation of passive microwave sensors are quantified and compared with other products such as the Global Precipitation Climatology Project (GPCP V3.2), the Merged CloudSat, TRMM and GPM (MCTG), and ERA5. Results show that GPM V7 products have higher precipitation rate than the previous version, except for the radar-only product. For the ~ 65oS-N region, covered by all of the instruments, this increase ranges from about 9% for the combined radar-radiometer to about 16% for radiometer-only product. While GPM precipitation products still show lower values than MCTG (except over the tropics and Arctic Ocean), the V7 products (except radar-only) are generally more consistent with MCTG and GPCP V3.2 than V5. Precipitation products are found to be least consistent over the Southern Oceans, displaying the largest spread in mean precipitation rate and location of latitudinal peak precipitation. Over the tropics, (25°S-25°N) passive microwave sounders show the highest precipitation rate, and the highest increase (~19%) compared to their previous version, among all of the studied precipitation products. Furthermore, analysis showed that precipitation products are generally less consistent (larger spread) over lower and higher values of sea surface temperature and total precipitable water. Analysis of mean monthly precipitation variation (MPV) showed that MPV is relatively small when averaged over 90°S-90°N and 65°S-65°N (e.g., ~4-6% of the annual mean precipitation rate), but is large over the tropics (e.g., 9-11%) and high latitudes (~26-55%). 


AS47-A015
Precipitation Characteristics of the Tropical Cyclone Over the Arabian Sea

Amit KUMAR1#+, Atul Kumar SRIVASTAVA1, Manoj K. SRIVASTAVA2
1Indian Institute of Tropical Meteorology, India, 2Banaras Hindu University, India

Over the Arabian Sea, the tropical cyclone (TC) formed during the post-monsoon season is investigated through the Global Precipitation Measurement (GPM) satellite level 2 observation. The precipitation characteristics of the TC developed between 2014 and 2021 are analyzed to understand the cyclonic rainfall's precipitation characteristics. 2-D distribution between the liquid water content (LWC) and non-liquid water content (IWC) shows considerable variations in the different precipitating cloud. In the convective cloud, the LWC is 0-800 g/m2, and IWC is about 0-300 g/m2. The amount of LWC is low, and IWC is higher in the stratiform cloud than in the convective cloud. In the stratiform (convective) cloud of the TC, the mean of normalized intercept parameter (Nw) and mass-weighted mean diameter (Dm) is 34.0 (35.54) mm-3m-1 and 1.27 (1.31) mm, respectively. Moving from the smaller to the bigger rain droplets, the value of Nw decreases, as observed in the 2-D distribution between Dm and Nw. The concentration of the bigger rain droplets is high in the convective cloud, and stratiform cloud is dominated by the smaller rain droplets. The contoured frequency altitude diagram (CFAD) of the Dm and reflectivity (Ze) for the stratiform and convective cloud of the TC indicate significant variation in the droplet's state above and below the melting layer. Ice particles and droplets in the supercooled liquid state dominate above the melting layer, and below it, a high concentration of rain droplets in the liquid form observed. Below the melting layer, the contribution of the various microphysical processes (size-sorting, evaporation, breaking-up and collision-coalescence process) in the rain droplets formation is different for the stratiform and convective cloud. The breaking-up process acts as the primary microphysical process in the stratiform cloud, and the collision-coalescence process is predominating in the convective of the TC.


AS51-A010
Numerical Simulation of Heavy Rainfall Events Over the Korean Peninsula During Summer of 2022

Sujeong CHO#+, Eun-Hee LEE, Keon-Hee CHO, Ji-Young HAN
Korea Institute of Atmospheric Prediction Systems, Korea, South

The Korean Integrated Model (KIM) is a global NWP model, which was developed in 2020 for the operational medium-range forecast at Korean Meteorological Administration. The Korea Institute Atmospheric Prediction Systems has a mission to improve KIM predictability for high-impact weather especially over the Korean Peninsula with an approach to increase resolution and advance physics parameterization. In this study, we evaluate heavy rainfall events simulated by KIM during summer 2022 by using both in-situ and remote sensing measurements. It is found that KIM simulates overall synoptic conditions for summer heavy rainfall events, which are characterized with upper level trough, low level jet, and migratory cyclones with North Pacific High located in the east of the Korean Peninsula. However, it also shows that precipitation prediction performance can be significantly affected by the simulated thermodynamic conditions by the model. Meanwhile, the model shows strong sensitivity to the cumulus parameterization scheme especially in events with an east-west rain belt passing from the West sea to the central part of Korea. The characteristics of the vertical structures of simulated rainfall events are further evaluated using remote sensing measurements to give comprehensive understanding to improve model predictability.


AS51-A011
Evaluation of the SMoothed Hybrid Sigma-pressure (SMH) Coordinate in KIM

Hae-Jin KONG1#+, Ja-Rin PARK1, Suk-Jin CHOI2, Hyun NAM1
1Korea Institute of Atmospheric Prediction Systems, Korea, South, 2Gangneung-Wonju National University, Korea, South

Various terrain-following vertical coordinates have been developed to mitigate the influence of the terrain structure in atmospheric numerical models. However, it still remains the problems in computing horizontal pressure gradients and advection along steep terrain surfaces. These small-scale structures can further promote artificial circulations as the model resolution increases. Choi and Klemp (2021) proposed the smoothed hybrid sigma-pressure (SMH) coordinate to reduce small-scale components more rapidly with height than basic sigma or hybrid sigma coordinates. The SHM coordinate is designed to flexibly control smaller scale of terrain influences with height by separating a reference surface pressure to smoothed and deviated parts. The performance of SMH coordinate was demonstrated in two-dimensional slice version of KIM through several idealized tests. Compared to the hybrid sigma coordinate, the SMH coordinate showed significant improvement in reduction of topographic features. This study examines the impact of the SMH coordinate in a full version of KIM. The SMH coordinate has potential to well control smaller scale of terrain features so that the model can be allowed to have less smoothing of the terrain in high resolution. With testing idealized experiments and real forecasts, the SMH performance will be discussed in terms of model stability and accuracy. Reference: Choi, S.-J., and Klemp, J. B., MWR, Vol. 149 (2021), 4077-4089. Acknowledgement: One of the authors, Suk-Jin Choi, wishes to acknowledge this study was supported by 2023 Academic Research Support Program in Gangneung-Wonju National University.


AS51-A012
Correcting Sub-daily Satellite Precipitation Based on GRU and TrajGRU in Taiwan

Hsiang-En TSOU+, Chia-Jeng CHEN#
National Chung Hsing University, Taiwan

The uneven spatiotemporal distribution of rain gauge data in Taiwan demands a need for a comprehensive gridded product that can be obtained from satellite observations, such as the Integrated Multi-satellitE Retrievals for Global satellite precipitation measurement (IMERG) product. However, IMERG still poses known biases and can sometimes be erroneous. In order to enhance the accuracy of satellite rainfall estimates, this study aims at applying two deep learning (DL) models, namely the Gated Recurrent Unit (GRU) model and the Trajectory Gated Recurrent Unit (TrajGRU) model, to correct IMERG Early and Final Run data in Taiwan at different sub-daily scales. Compared to traditional recurrent neural networks, GRU exhibits better model efficiency with a low memory usage, while TrajGRU incorporates a deformable convolution kernel able to effectively capture spatiotemporal features and improve predictive capabilities. Gauge data from Taiwan’s Central Weather Bureau are adopted as ground truth in the training and validation of DL models. Relative performance in the corrected IMERG products will determine the capabilities of the DL models as well as the limitation of time scales for such correction scheme.


AS51-A015
Pseudo Seeder-feeder Mechanism in Orographic Precipitation in a Typhoon Environment and its Response to Global Warming

Jianan CHEN#+, Xiaoming SHI
The Hong Kong University of Science and Technology, Hong Kong SAR

The intense winds in a Typhoon environment over mountainous regions can trigger strong convections and produce enhanced precipitation, yet few previous studies have been done in understanding how the orographic precipitation in a TC environment might respond to global warming. Here, we focus on this problem and use large-eddy simulation (LES) to estimate the global warming-induced response of precipitation over and near an idealized mountain with 10km half width and 1km height. Pseudo-global warming experiments are further conducted by adding mean thermodynamic structure changes predicted by a CMIP6 climate simulation. Two regions exhibit locally enhanced precipitation. One is over the mountain with rainfall maximum on the lee slope; the other is in the downstream region 30 to 50 km away from the mountain. Regression analysis suggests the enhanced precipitation in both regions are related to the seeder-feeder mechanism. Though the enhancement in the downstream regions differs from the conventional definition. Mountain waves generate an intense cloud formation center in the upper troposphere above the mountain, resulting snow and graupel drift downstream which intensify downstream convection when they fall into a proper height. This precipitation enhancement mechanism in the downstream region is called as Pseudo Seeder-Feeder Mechanism (PSF). Under global warming, the downstream enhanced region exhibits mean precipitation sensitivity ~18%/K which is significantly higher than the Clausius–Clapeyron (CC) scaling of ~7%/K of surface warming. This super-CC scaling in the downstream region is induced by both the precipitation efficiency and thermodynamic enhancement, of which the precipitation efficiency is the dominant factor. Additionally, the larger sensitivity in the downstream region is partially due to the upwind shift of the enhanced precipitation, which in turn is attributed to changes in the mountain wave patterns.


AS51-A017
Super-Clausius–Clapeyron Scaling of Tropical Cyclone Rainfall at Urban Scales

Xiaoming SHI#+
The Hong Kong University of Science and Technology, Hong Kong SAR

Accurate quantification of future extreme tropical precipitation is challenging because global climate models have insufficient resolutions to resolve convection. Yet reliable estimation is needed to prepare our society for the increasing risks of flooding and landslide as extreme rainfall is expected to intensify generally as the climate warms. Here, we combine deep learning (DL) and convection-permitting simulations to provide reliable estimations of the future change in extreme precipitation in South China. The DL model was trained to statistically downscale low-resolution climate model data and proved more effective in identifying extreme precipitation events than simply using global climate model rainfall. High-resolution (1km) downscaling simulations are conducted for DL-selected cases so as to verify DL prediction and provide a more accurate, physical modeling-based prediction of precipitation. We found that the sensitivity of extreme rainfall at the grid-point scale is close to the Clausius-Clapeyron (CC) scaling, around 7%/K. However, for large spatial scales and temporal accumulation, the sensitivity can be as high as 17%/K. Such accelerated response of extreme precipitation in the urban-relevant scales is found to result from more compact organizations of convective cores in tropical cyclones. Such super-CC scaling has important implications for future urban flooding and slope safety.


AS51-A021
Using Machine Learning to Analyze the Changes in Summer Extreme Precipitation in Southern China

Bojun WANG+, Wei WEI#, Zejiang YIN
Sun Yat-sen University, China

Convolutional neural network (CNN) is applied to identify the extreme precipitation in southern China in summer and the physical contributions are quantified for the interdecadal changes in the extreme precipitation. The CNN correctly identifies 93% of the observed extreme precipitation events based on the given large-scale atmospheric circulation through hyper-parameter optimization and model training. The discrimination made by the neural network is revealed by using the layer-wise relevance propagation method. The CNN is inclined to classify the circulation pattern as an extreme precipitation circulation pattern (EPCP) when the low pressure anomalies of sea level pressure and 500-hPa geopotential height appear in southern China. Both the extreme precipitation amount and the frequency of EPCP show significant interdecadal changes around the early-1990s. Result of the partition analyze indicates that the interdecadal increase in the extreme precipitation in the last three decades is mainly attributed to the dynamic influence of the increasing frequency of the EPCP. The thermodynamic effect of the increasing watervapor also plays an important role in the increase of both the extreme and non-extreme precipitation after the early-1990s.


AS52-A007
A Novel Hybrid Deep Learning Model for Predicting Ionospheric TEC Under Different Geomagnetic Conditions

Han WU1+, Ling HUANG1#, Hongping ZHANG2, Dezhong CHEN2, Yidong LOU2, Bin MA1, Xu LIU1
1Guilin University of Technology, China, 2Wuhan University, China

Aiming at the characteristics of high noise, nonlinearity and non-smoothness of ionospheric Total Electron Content (TEC) time series, this study constructs a combined short-term ionospheric TEC prediction model based on long short-term memory (LSTM) neural network model, incorporating singular spectrum analysis (SSA). The data of geomagnetic storm periods in high solar activity year and geomagnetic calm periods in low solar activity year are selected, and the trend component, period component and noise residual component of TEC time series are firstly extracted using SSA, and then the LSTM model is used to implement TEC prediction at different geomagnetic conditions and geographic latitudes. The results show that the relative accuracy of SSA-LSTM model is 91.17% and 95.46% respectively, which is 4.92% and 3.17% higher than that of single LSTM model, during the period of geomagnetic storm periods and geomagnetic calm periods.


AS52-A011
A Comparison of NmF2 Derived from Nighttime OI 135.6nm Emission to Ionosonde Measurements

Shixiang XUE, Chunhua JIANG#+
Wuhan University, China

It is well known that there is a strong correlation between the intensity of nighttime OI 135.6nm emission and the critical frequency of ionospheric F2 region (foF2). However, the relationship depends on the different longitudes and latitudes. In this study, an improved algorithm was developed to estimate foF2 from nighttime OI 135.6nm emission. The proposed method is suitable for different longitude, latitude, local time, season and solar activity. This study estimated foF2 from OI 135.6nm emission observed by the Special Sensor Ultraviolet Spectrographic Imager (SSUSI) instrument on board the Defense Meteorological Satellite Program (DMSP), and then the estimated results were compared with the results of ground-based ionosonde. Results show that the data with relative error less than or equal to 20% accounted for 92.99%, and the average relative error was about 7.08% during the high-solar activity year (2013). During the low-solar activity years (2017), the data with relative error less than or equal to 20% accounted for 80.76%, and the average relative error was about 12.64%. Furthermore, we discussed the possible reasons about the difference of retrieval accuracy of the algorithm during the high and low solar activity years.


AS52-A018
Estimation Model of Global Ionospheric Irregularities: An Artificial Intelligence Approach

Penghao TIAN#+, Jianfei WU
University of Science and Technology of China, China

The ionospheric sporadic E layer, the ionospheric irregularities of enhanced electron density, appears in the Earth’s ionosphere at altitudes between 90 and 120 km, which supports the real-world radio communication needs of many sectors reliant on ionosphere-dependent decision-making. The prediction of the occurrence of sporadic E layers has been extremely difficult due to the highly complex behavior. Conventional numerical methods are limited because of the inability to extract high-level information from data. Deep learning is a powerful tool for mining latent features from data, which can theoretically avoid assumptions constraining physical methods. Inspired by feature extraction, we applied deep learning to explore latent relationships between mapping observable lower atmospheric data and ionospheric data from limited observations. The proposed model was trained with high-resolution ERA5 data during Jan. 1, 2007-Aug. 30, 2018 as input and corresponding ionospheric sporadic E data collected from COSMIC RO measurements as output. The results show that the model can learn complex relevance as bridges connecting the input and the desired output and obtain excellent performance and generalization capability by applying multiple evaluation criteria. Additionally, we established several model architecture training methods to explore the performance of the model with different input data. The statistic results show that model inference performance is proportional to the abundance of input information and is impacted by intraseasonal variability. The inference capability of the model achieves the best performance in the Jun.-Aug. (JJA) and Dec.-Feb. (DJF) seasons, which is the exact period of sporadic E layer significant occurrence, although different models are evaluated.


AS56-A001
Impacts of Land Cover Changes on Biogenic Emission and its Contribution to Ozone and Secondary Organic Aerosol in China

Ma JINLONG1#+, Hongliang ZHANG1, Peng WANG2
1Fudan University, China, 2The Hong Kong Polytechnic University, China

The increase in vegetated areas in China led to increased biogenic volatile organic compounds (BVOC) emissions. As the important precursor for ozone (O3) and secondary organic aerosol (SOA), an increase in BVOC emissions will impact the formation of O3 and SOA. Thus, accurate estimation of BVOC emissions is critical to understanding their impacts on air quality. In this study, Model of Emissions of Gases and Aerosols from Nature (MEGAN) v2.1 was used to investigate the impact of different leaf area index (LAI) and land cover (LC) datasets on BVOC emissions in China in 2016 and the effects on O3 and SOA were evaluated based on the Community Multiscale Air Quality Modelling System (CMAQ). Three LAI satellite datasets of the Global LAnd Surface Satellite (GLASS), the Moderate Resolution Imaging Spectroradiometer (MODIS) MOD15A2H version 6 (MOD15), and the Copernicus Global Land Service (CGLS), as well as three LC satellite datasets of the MODIS MCD12Q1 LC products, the Copernicus Climate Change Service (C3S) LC products, and the CGLS LC products were used in five parallel experiments (cases: C1-C5). Results show that changing LAI and LC datasets of the model input has an impact on BVOC estimations. BVOC emissions in China range from 25.42 to 37.39 Tg in 2016. Changing the LC inputs for the MEGAN model has a more significant difference in BVOC estimates than using different LAI datasets. Besides the impact on BVOC emissions, changing the MEGAN inputs further impacts the concentrations of O3 and SOA. The highest O3 and biogenic SOA (BSOA) concentrations appear in the C1 (using GLASS and MCD12Q1 LC) simulation, which can reach 12 ppb and 9.8 μg m-3, respectively. Due to the effect of BVOC emissions, the relative differences between C1 and C4 are over 52% and 140% in O3 and BSOA in central China.


AS56-A007
Effects of Temperature on Biogenic VOCs Emissions and its Contributions to Ozone Formation in Pearl River Delta

Hao GUO1#+, Yanli ZHANG1, Xinming WANG2
1Guangzhou Institute of Geochemistry, Chinese Academy of Sciences, China, 2Chinese Academy of Sciences, China

Ozone (O3) pollution is influenced by a combination of NOx and VOCs emissions. The biogenic volatile organic compounds (BVOC) emitted from plants could be an important source and the production is significantly impacted by temperature changes. This study will investigate the effects of temperature on Biogenic VOCs emissions and its contributions to ozone formation in Pearl River Delta in summer, 2022 using Model of Emissions of Gases and Aerosols from Nature (MEGAN) and the Community Multi-scale Air Quality (CMAQ) model. The meteorology will be generated using Weather Research and Forecasting (WRF) model version 3.9.1 and biogenic emissions will be generated based on MEGAN version 2.4 with two scenarios: base case and temperature increased 2K case. The differences in spatial variations of biogenic emissions, ozone concentrations and SOA concentrations between two scenarios will be analyzed. The results show a significant increase in BVOC emission (24%) and ozone concentrations (~2 ppb) with 2K increase of temperature in Pearl River Delta in summer, 2022. BVOC emissions are highly sensitive to the temperature changes, and we need to adjust our air pollution control strategy based on temperature effects especially in Pearl River Delta.


AS56-A011
Molecular Composition of Secondary Organic Aerosol from α-pinene Ozonolysis Affected by Relative Humidity

Hao LUO+, Yindong GUO, Hongru SHEN, Defeng ZHAO#
Fudan University, China

Biogenic volatile organic compounds (BVOC) can contribute a significant fraction to secondary organic aerosols (SOA) through atmospheric oxidation, which plays a critical role in climate change and human health. The ozonolysis of α-pinene, one of the most important BVOCs, is a canonical SOA system. At present, the effects of relative humidity (RH) on SOA composition from α-pinene+O3 reaction are still unclear. In this study, we report the SOA composition on molecular level formed in α-pinene+O3 reaction under various RH. The SOA components were measured by an Extractive ElectroSpray Ionization inlet coupled with a long Time-of-Flight Mass Spectrometer (EESI-TOF-MS). We observed RH-dependent SOA chemical composition, including larger contribution of monomer products with increasing RH, although the total O:C remained largely unchanged. The effect of RH may be attributed to the particle-phase reactions of SOA components. This study highlights the necessity of characterizing SOA composition on molecular level and of considering RH dependence of SOA chemical composition and it physicochemical properties in atmospheric models.


AS56-A013
Unexpected Significance of a Minor Reaction Pathway in Daytime Formation of Biogenic Highly Oxygenated Organic Compounds

Hongru SHEN1+, Luc VEREECKEN2, Sungah KANG2, Iida PULLINEN2, Hendrik FUCHS2, Defeng ZHAO1#, Thomas MENTEL2
1Fudan University, China, 2Forschungszentrum Jülich, Germany

Secondary organic aerosol (SOA), formed by oxidation of volatile organic compounds, significantly influence air quality and climate. Highly oxygenated organic molecules (HOM), particularly those formed from biogenic monoterpenes, play a key role in their formation and growth. As the most important daytime oxidant, hydroxyl radical (OH) initiated HOM from monoterpenes is believed to be mainly formed via the OH addition channel. However, for α-pinene, the most abundant atmospheric monoterpene, we found that the minor hydrogen abstraction channel is underappreciated in the HOM formation. We will present our observations and theoretical calculations, showing the role of hydrogen-abstraction and alkoxy radicals for fast autoxidation leading to HOM. We also provide a mechanism and yield, suggesting the non-negligible contribution of the hydrogen abstraction channel to ambient SOA, particularly in OH rich areas.


AS57-A002
A Method to Retrieve the Refractive Indices and Mineral Components of Dust Aerosols from Satellite Infrared Hyperspectral Data

Senyi KONG#+, Lei BI
Zhejiang University, China

Dust aerosols exert an enormous influence on human health, global weather, and climate due to their large mass loading and wide spatial distribution. A large uncertainty still exists in quantitatively assessing the impact of dust aerosols on radiative transfer and climate simulation, which can partly be attributed to the complex refractive indices of dust. The complex refractive indices of dust are related to mineral composition. However, the mineral composition of dust is manifold and varies with dust origins, which results in sampling limitations in the experimental measurement of the complex refractive indices of dust and the contents of mineral components. In response to this problem, this study has obtained the complex refractive indices and the contents of the mineral composition of dust aerosols from satellite data by utilizing the mineral composition characteristics in the infrared band. The results showed that the retrieved complex refractive indices were higher than the experimental reference values, while the retrieved contents of mineral components were in good agreement with the experimental measurements.


AS57-A004
Assessment of the Inhomogeneity and Nonsphericity Effect of Internally Mixed Aerosols in the Chemical Weather Prediction Model

Xuan WANG+, Lei BI#
Zhejiang University, China

In order to represent aerosols for radiative transfer simulations in the atmospheric model, we developed an internally-mixed aerosol scheme in which both particle nonsphericity and inhomogeneity effect were considered. In this scheme, black carbon was assumed to be fractal and soil dust was modeled as super-spheroid. These two insoluble aerosols (black carbon and soil dust) were partially coated with hygroscopic aerosols such as sulfate, nitrate, and aerosol water. The aerosol hygroscopic growth and composition variations were parameterized. Then, we built a database of the optical properties for the aforementioned models using the Invariant Imbedding T-Matrix Method(IITM). In addition, deep neural networks (DNN) were trained based on the database. We found that the DNN can predict the optical properties of aerosols efficiently and accurately. With these efforts, the aerosol-optics scheme was implemented into the Global/Regional Assimilation and Prediction System with Chinese Unified Atmospheric Chemistry Environment (GRAPES/CUACE). Two case studies were performed in East Asia on the summer and winter of 2020. Compared to the uniform and spherical aerosol scheme, the inhomogeneity and nonsphericity effect caused negative radiative forcing on the surface and positive radiative forcing on the top of atmosphere (TOA), enhancing the solar heating rate. The surface was cooler and the air beyond the boundary layer was warmer. Thus, the boundary layer was found to be more stable, leading to less precipitation and lower boundary layer heights. Finally, the meteorological and optical profiles computed from the GRAPES/CUACE were implemented in the RTTOV (Radiative Transfer for TOVS). The simulated solar reflectance on the TOA was compared with observations from the FY-4A satellite. We found that the comparisons were improved when the inhomogeneity and nonsphericity effect of aerosols were incorporated.


AS57-A005
Hourly Assimilation of Himawari-8 Cloud Optical Depth Using Four-dimensional Local Ensemble Transform Kalman Filter Over the Tibetan Plateau

Tianyu ZHANG#+
Aerospace Information Research Institute,Chinese Academy of Sciences, China

It is a challenge for improving the simulation effect of thick clouds over the Tibetan Plateau due to the rapidly and deeply cloud convection occurs frequently in summer. A cloud optical thickness assimilation system is developed by introducing Four-Dimensional Ensemble Kalman Filter theory (4D-LETKF) which establishing the covariance relationship between 2D cloud optical thickness and 3D cloud water content and taking advantage of the high spatial and temporal resolution of the next generation of geostationary satellites. A typical simulation case of convective clouds in summer is carried out over the Tibetan Plateau using the new assimilation system. The cloud optical thickness is assimilated hourly from the next generation data of Himawari-8 satellite to correct the cloud water mixing ratio in the WRF model. The assimilation significantly improves the simulation accuracy of cloud optical depth on thick clouds which solves the problem that the assimilation effect is weak on thick clouds in the existing cloud assimilation system. Using Himawari-8 satellite data as the true value for effect evaluation, the new assimilation scheme can improve the accuracy of cloud optical thickness correlation coefficient by 34% after the assimilation.


AS57-A006
A Machine-learning-based Cloud Top Pressure Retrieval by Synergistically Using Polarized and O2 A-band Measurements from GF-5 and PARASOL

Lesi WEI#+, Huazhe SHANG, Husi LETU
Chinese Academy of Sciences, China

Cloud top pressure (CTP) is a critical cloud property that significantly affects cloud radiation. Multi-angle polarization-based sensors can employ polarized bands (490 nm) or O2 A-bands (763 and 765 nm) to retrieve the CTP. However, the CTP retrieved by the two methods shows inconsistent results in certain cases, and large uncertainties in low and thin cloud retrievals may negatively affect subsequent applications. This study proposes a synergistic algorithm that appends both O2 A-bands and polarized bands using a random forest (RF) model. LiDAR CTP data are used as the sample true values, and polarized and non-polarized measurements are concatenated to train the RF model of CTP. Additionally, through analysis, we discovered that the polarized signal is saturated with increasing cloud optical thickness (COT), thus necessitating a special treatment for COT intervals <10 to improve the stability of the algorithm. We then applied the synergistic method to directional polarized camera (DPC) and Polarized and Directionality of the Earth’s Reflectance (POLDER) measurements for evaluation, and the validation accuracy and retrieval accuracy of the POLDER-based measurements (RMSE=121.431 hPa, R2=0.827 and RMSE=30.611 hPa, R=0.470, respectively) were higher than that of the MODIS and POLDER Rayleigh pressure measurements. Moreover, POLDER also showed good performance relative to DPC. This algorithm is expected to provide data support for atmosphere-related fields as an atmospheric remote sensing algorithm in the Cloud Application for Remote Sensing, Atmospheric Radiation and Updating Energy (CARE) platform.


AS57-A008
Characterization of the Size-resolved Morphology for Black Carbon Particles During Atmospheric Aging

Yan PENG#+, Xiaofeng HUANG, Jing WEI, Ling-Yan HE
Peking University Shenzhen Graduate School, China

The morphology of black carbon (BC) plays an important role in the determination of its aging scale and constraining its radiation effect. Therefore, it is urgent to characterize the distribution and evolution of observational-based morphology of BC-containing particles during atmospheric aging. In this study, a tandem differential mobility analyzer–single-particle soot photometer (DMA–SP2) system was used to estimate the size-resolved effective density (ρeff) of atmospheric BC-containing particles. The results show that there are differences in the morphology evolution with different BC core diameters (Dc) during the emitted-to-age process. With less coating materials, the small Dc particles (100-120 nm) tend to be spherical (ρeff = 1.31-1.33 g cm-3) while the large Dc particles (280-300 nm) are fractal (ρeff = 0.95-1.08 g cm-3). During atmospheric aging, the non-BC materials dominate the ideal growth of particle diameter for small Dc particles, while used to fill the void for large Dc particles and cause the collapse of the fractal branches. Furthermore, this study classified the BC-containing particles into two groups, i.e., near-spherical and non-spherical particles. For the first time, we calculated and parameterized the coating-to-BC mass ratio (MR) of the shape transition points as a function of Dc and the mean aging state of BC-containing particles. After considering this parameterization, compared with the core-shell prediction, there are ~ 18% reductions for calculated absorption cross section over the entire population. This study highlights that the strong dependence of the ρeff and shape transition MR point of atmospheric BC-containing particles on Dc can improve the representation of its morphology in the global climate model and reduce uncertainty in the evaluation of BC climate effects.


AS57-A014
A Precipitation Estimation Method by Considering Clouds Microphysical Parameters Based on Observations from Geostationary Satellite

Dabin JI1#+, Husi LETU2, Jiancheng SHI2
1Aerospace Information Research Institute, Chinese Academy of Sciences, China, 2Chinese Academy of Sciences, China

Real time precipitation is an important parameter in flood forecast. Geostationary satellites which have real time observations at visible and infrared bands with high spatial and temporal resolution provide a good way to estimate precipitation. A lots of precipitation estimation algorithms have been developed for geostationary satellites. Cloud top information which includes cloud top reflectivity, cloud top brightness temperature, gradient of cloud top brightness temperature and motion vectors of cloud top was usually used to retrieve precipitation in these precipitation estimation algorithms. However, it is hard to accurately select precipitation pixels from non-precipitation clouds only based on cloud top information. In this study, a new real-time precipitation estimation method for geostationary meteorological satellite Himawari-8 considering cloud microphysical parameters was proposed. Besides the cloud top information, the cloud microphysical parameters including cloud effective radius and cloud optical depth in both day and night were used in the new precipitation recognition method to improve the accuracy of precipitation identification. Based on the identified precipitation area, the cloud top brightness temperature and cloud liquid water path which was calculated from cloud effective radius and cloud optical depth were used to build a dynamic calibrating model to estimate the rainfall rate by taking the GPM-IMERG early run precipitation product as reference. The estimated rainfall rate was further calibrated using rain gauge observations on hourly scale. According to the validation using independent hourly rain gauges observations over Chinese mainland in summer, the probability of detection (POD) of the real-time estimated precipitation can reach up to 0.7, and the false alarm ratio (FAR) is lower than 0.6. From the aspect of precipitation identification, the accuracy of the newly developed precipitation algorithm has a obvious improvement compared with that of the GSMaP_NOW over Chinese mainland.


AS59-A003
Characteristics of Intracloud Lightning to Cloud-to-ground Lightning Ratio in Thunderstorms Over China

Yushu REN#+, Weixin XU
Sun Yat-sen University, China

The intracloud (IC) to cloud-to-ground (CG) lightning ratio (IC:CG ratio) provides not only essential information for extrapolating IC flashes from the continuously monitored CG activities but also important implications for the kinematic and microphysical structures of thunderstorms. This study examines the IC:CG ratio climatologies in China and seeks the underlying reasons responsible for regional variations on IC:CG ratios. Analyses are based on both grid-scale (2 degree) and thunderstorm-scale (convective feature), using coincident observations from TRMM LIS (total flash) and the China Lightning Detection Network (CG lightning) during 2009-2014. National mean IC:CG ratios in China are about 3-5, consistent to those reported in other regions around the world. However, Guangxi Province (GXP) and Sichuan Basin (SCB) have exceptionally high (> 10) and lower-than-average (< 2) IC:CG values, respectively. While the IC:CG in GXP significantly maximizes in the spring season and diurnally peaks in the morning, SCB exhibits virtually no seasonal nor diurnal variation on IC:CG. The contrasting IC:CG ratios between GXP (~7.5) and SCB (~2.5) are also found on the storm scale. Thunderstorms in GXP have a much lower CG flash rates than those in SCB, even though they share a similar total flash rate, resulting in a far higher IC:CG in GXP. All convective proxies indicate that SCB has a higher likelihood in producing CG flash than GXP under the same convective intensity. In addition, the CG flash rate in SCB increases much more rapidly with the increase of total flash rate or convective intensity. The underlying mechanisms for regional variations on IC:CG may be associated with storm morphology, microphysical property, and/or convective environments, which will be further investigated.


AS59-A004
A High-resolution Numerical Simulation of the “7.19” Extraordinary Heavy Rainfall in Henan Province Under Topographic Effect

Xinmin WANG#+
Xiamen Key Laboratory of Straits Meteorology, China

In this study, based on the ERA5 dataset, the orographic precipitation characteristics during an extraordinary heavy rainfall event in Henan Province on July 19, 2016 are analyzed. Besides, by using WRF, a high-resolution numerical simulation is carried out, including a series of sensitivity experiments on the Taihang Mountains, the Yunmeng Mountain and low-altitude areas. The distribution of observed precipitation shows that the precipitation over the Taihang Mountains in northern Henan during the daytime of July 19 is significantly enhanced due to the topographic effect compared with that over the plain on the east. The simulation results demonstrate that the distribution of simulated precipitation over the steep terrains on the east side of the Taihang Mountains is closer to the observational precipitation when SRTM-90m is introduced to the WRF model. When the altitude of the Taihang Mountains is lowered by 50%, the accumulated precipitation along the Taihang Mountains in the daytime of the 19th decreases by 26%, accompanied with the northward movement of the heavy precipitation center over the northern Taihang Mountains. Besides, the Yunmeng Mountain plays an important role in blocking or diverting the easterly and southeasterly low-level jet. When the terrain elevation of the Yunmeng Mountain is reduced, the convergence zone of the wind field in the low-level moves to the areas along the Taihang Mountains, which leads to the expansion of the area with heavy rainfall, with the average accumulated precipitation in mountain areas increasing by 7%. Besides, When the low-altitude terrain in the study region is reduced by 50%, the center of heavy precipitation moves westward obviously. Combined with the diagnostic analysis of the topographical forced vertical velocity, the results show that the uplift of low-level jet caused by the low-altitude terrain is one of the reasons that affect the location of heavy rainfall center.


AS59-A010
Analysis of Environmental Field Characteristics of Convective Initiation Triggered by Thunderstorm Gust Fronts in Beijing Area

Na HE1#+, Xiaoding YU2, Qinglan DING3, Xian XIAO2, Nan XING4, Ke LIU5
1Beijing Weather Forecast Center,Beijing Meteorological Service, China, 2China Meteorological Administration, China, 3Beijing Weather Forecast Center, China, 4Beijing Meteorological Service, China, 5North China Aviation Administration, China

In order to enhance the understanding of the environmental field characteristics of the convective regeneration triggered by thunderstorm gust fronts. Based on Beijing sounding observation, automatic stations, S-band Doppler radar and new detection data to analysis environmental field characteristics of two typical cases in which convection initiation triggered by thunderstorm gust fronts. The results show that: (1) One type is convection triggered by collision of multiple gust fronts or the encounter of gust fronts with other boundary layer convergence lines in the region with high Convective Available Potential Energy (CAPE) and sufficient water vapor (collision triggering). In this type, the vertical velocity of two collision gust fronts is much larger than that of a single gust front. Strong upward movement is easy to provide good lifting conditions for the triggering of convection, and convection is easy to trigger. (2)The other type is the gust front triggers convection in the unstable region (non-collision trigger). In this type, the low-level wind direction is perpendicular to the gust front, which is conducive to the strong convergence between the ambient wind near the ground and the gust front. Meanwhile, the updraft of the convection triggered by the gust front tends to be vertical, which is beneficial to convective initiation. (3)By comparing the environmental field of gust fronts trigger and non-trigger Convective Initiation (CI) cases, the results show that there are deep wet convection potential with high CAPE and low Convective Inhibition (CIN) of the environment field in these cases which CI are triggered by gust fronts. There are cold dry advection at the upper level and warm wet advection at the lower level in most cases CI triggered by the gust fronts, which also happened at the wind speed or wind direction convergence areas with high CAPE. 


AS59-A013
Impact of Boundary Layer Jets on Cold Pool Characteristics During the Pre-summer Rainy Season in South China

Dong FU#+, Yu DU
Sun Yat-sen University, China

The South China Sea frequently experiences boundary layer jet (BLJ) events, which are closely related to the coastal rainfall of South China during the pre-summer rainy season. The gust front associated with the cold pool can interact with the low-level vertical wind shear, potentially affecting convection. The BLJ with a unique vertical wind shear may also interact with the cold pool, but the nature of this interaction is yet to be fully understood. The present study uses data from 356-m high Shenzhen Met-Tower to analyze the statistical characteristics of cold pools and investigate how these characteristics vary between BLJ- and nonBLJ- related cold pools. A total of 54 cold pools were observed by Shenzhen Met-Tower from April to June during 2018-2020, which included 26 BLJ-related cold pools and 28 nonBLJ-related cold pools. Results showed that the BLJ-related cold pools had a weaker temperature drop and less pressure increase compared to the nonBLJ-related cold pools, but their structure were deeper, greater specific humidity decrease and recovery was faster. The BLJ-related cold pools caused the decreases of relative humidity in the upper levels but increases in the lower levels. In contrast, both the upper and lower layers of the nonBLJ-related cold pools showed an increase in relative humidity. It is found that BLJ-related cold pools moved faster and were affected by the type of convective systems. The BLJ-related cold pools associated with mesoscale convective systems are deeper, longer-lasting, and had less pressure increase and more specific humidity reduction than those associated with convective cells.


AS59-A014
Using Polarimetric Radar Observations to Characterize First Echoes of Thunderstorms and Nonthunderstorms: A Comparative Study

Chuanhong ZHAO1#+, Yijun ZHANG2
1Chengdu University of Information Technology, China, 2Fudan University, China

This work compares the characteristics of the first echoes of thunderstorms and nonthunderstorms retrieved from S-band polarimetric radar observations. Observations of 57 (39) isolated thunderstorm (nonthunderstorm) cells with roughly equivalent aerosol and water vapor conditions but different convective available potential energy were obtained with a S-band polarimetric radar and three independent lightning location systems during 2016/2017 in southern China. Storms with the first echoes were divided into three types based on echo top heights, namely, type 1 (below 0°C layer), type 2 (0°C to −10°C), and type 3 (above −10°C layer). Our observations show median values of radar reflectivity (ZH) and differential reflectivity (ZDR) of type 1 and type 2 in warm phase layer (below 0°C layer) are obviously greater in nonthunderstorms than in thunderstorms, but this feature is not significant in type 3 storms. In the mixed 1 phase layer (0°C to −10°C), median ZH in type 2 is greater in nonthunderstorms while median ZDR in type 3 is slightly smaller. In the mixed 2 phase layer (−10°C to −38°C), median ZH is greater in thunderstorms while median ZDR is smaller, and ZDR values in nonthunderstorms are closer to zero. Although results of ZDR comparisons in the mixed phase are likely affected by random errors and/or residual bias errors, these different signatures suggest different characteristics of liquid or ice particles between thunderstorms and nonthunderstorms. This study is expected to advance our understanding of physical processes responsible for the generation of the first flash.


AS59-A016
Climatic Interactions Between Cold Surges and North Pacific Extratropical Cyclones—in the Perspective of Cold Surges

Lan XIA#+, JIalin ZHANG, Yao HU
Yunnan University, China

Cold surge events are divided into four types depending on their correlation with North Pacific extratropical cyclones. Climatologic relationships between the two phenomena reveal that 92% (39%) of all cold surges are accompanied by extratropical cyclones (explosive extratropical cyclones), while 31% of extratropical cyclones are accompanied by cold surges. The occurrence and development of extratropical cyclones favor eruptions of cold air from higher latitudes, which in turn produce conditions conducive to cold surges. In the North Pacific, extratropical cyclones travel in a northeastward direction, ultimately contributing to the Aleutian low. Meanwhile, the westerly jet is observed to strengthen following cold surge events. Both actions drive further extratropical cyclone activity, which in turn facilitates subsequent cold surges. Therefore, when extratropical cyclones occur before and after cold surges, the cold surge event itself tends to be relatively strong and long-lived. The transmission of energy by extratropical cyclones is a primary link between the high and middle latitudes, and contributes to the impact of cold surges on low latitudes. This study also explores the respective influences of the Siberia High and Aleutian Low on cold surges.


AS59-A022
Machine Learning Approach for Prediction of Lightning Probability in the Warm Season

Kyuhee SHIN1+, Kwonil KIM2, Si-Hyeon SON1, Gyu Won LEE1#
1Kyungpook National University, Korea, South, 2Stony Brook University, United States

Lightning affects significant hazards to society directly or indirectly, such as by striking individuals, causing damage to electrical infrastructure, and disrupting transportation systems. Accurate prediction of lightning is crucial for forecasters to respond effectively to its imminent occurrence. Lightning usually occurs in convective storms, which develop rapidly and occurs in a narrow area. This causes difficulties in predicting their location using numerical weather prediction (NWP). Lightning occurrence is often predicted by utilizing thermodynamic parameters (K index, CAPE, Lifted index, etc.). A high-resolution NWP model provides a prediction of thermodynamic variables at high spatiotemporal resolution with high accuracy for a few hours. However, a complicated algorithm is required to handle all the useful high-resolution variables from the NWP model. Recently emerging machine learning (ML) technique can solve this issue because it properly handles these “big data” without any model distributional assumption.
In this study, we have examined the capability of the use of “random forest” (RF) in the prediction of lightning probability for 3 years (2020–2022) of the warm season (June to August). The RF was trained by a lightning occurrence as a predictand and characteristic parameters from the NWP as predictors. The precision of RF was higher than 0.9 for lightning and higher than 0.85 for non-lightning, respectively. The trained RF was applied to the independent analysis and forecast fields and showed high agreement with the observation, suggesting that the trained model had the potential to assist forecasters in improving their lightning forecasting skills using real-time probabilistic forecasts from the trained model.

ACKNOWLEDGEMENT
This work was funded by the KMA Research and Development Program “Observing Severe Weather in Seoul Metropolitan Area and Developing Its Application Technology for Forecasts” under Grant (KMA2018-00125). This work was supported by the NRF of Korea grant funded by the Korea government (MSIT) (No. 2021R1A4A1032646).


Tue-01 Aug | 1:10 - 3:10 | MR323
AS18 - The Science and Prediction of Tropical Cyclones

Session Chair(s): Haikun ZHAO, Nanjing University of Information Science & Technology, Hisayuki KUBOTA, Hokkaido University

AS18-A041 | Invited
Counterbalancing Impacts from Historical Anthropogenic Aerosols and Greenhouse Gases on Global-scale Tropical Cyclone Genesis Potential

Haikun ZHAO1#+, Jian CAO1, Bin WANG2, Liguang WU3
1Nanjing University of Information Science & Technology, 2University of Hawaii, 3Fudan University

How anthropogenic forcing could change tropical cyclones (TCs) is a keen societal concern owing to its significant socio-economic impacts. However, a global picture of the anthropogenic aerosol and greenhouse gas effect on TCs has not yet emerged. Here we show that anthropogenic aerosol emission can reduce northern hemisphere (NH) TCs, represented by genesis potential index (GPI), but increase southern hemisphere (SH) TCs primarily through altering vertical wind shear and mid-tropospheric upward motion in the TC formation zones using the single anthropogenic forcing experiments from the 14 Coupled Model Intercomparison Project phase 6 (CMIP6) models. These circulation changes are driven by anthropogenic aerosol-induced NH-cooler-than-SH and NH-increased versus SH-decreased meridional (equator to mid-latitudes) temperature gradients. The cooler NH produces a low-level southward cross-equatorial transport of moist static energy, weakening the NH ascent in the TC formation zones; meanwhile, the increased meridional temperature gradients strengthen vertical wind shear, reducing NH TC genesis. The opposite is true for the SH. The results may help to constrain the models’ uncertainty in the future TC projection. Reduction of anthropogenic aerosol emission may increase the NH TCs threat. Further, we quantify the relative contributions of anthropogenic aerosol and greenhouse gas (GHG) to global TCF. We find that the two forcings have comparable but opposite impacts on GPIs due to their influences on the TC environment, leading to an insignificant change in GPIs in the historical period (1850-2014). Notably, the aerosol radiative forcing’s intensity is only about one-third of that of GHG, suggesting a more effective modulation of aerosol forcing on GPIs. The stable global TC frequency during the past decades could be attributable to the similar pace of the two anthropogenic emissions. The results highlight that a reliable global TC projection depends on both the aerosol and GHG emission policies.


AS18-A072 | Invited
Tropical Cyclone Events Observed by Naval Ships Along Japan Waters During the 1850s and 1860s

Hisayuki KUBOTA1#+, Togo TSUKAHARA2, Junpei HIRANO3, Jun MATSUMOTO4,5, Masumi ZAIKI6, Takehiko MIKAMI4, Rob ALLAN7, Clive WILKINSON8, Sally WILKINSON8, Alice DE JONG9
1Hokkaido University, 2Kobe University, 3Teikyo University, 4Tokyo Metropolitan University, 5Japan Agency for Marine-Earth Science and Technology, 6Seikei University, 7International ACRE Project, 8CSW Associates Data Services, 9Leiden University

Long-term historical meteorological observations are necessary for understanding climate variability. European and US ships sailed in the vicinity of Japan waters before the weather station network was established in Japan during the late Edo period in the eighteenth and nineteenth centuries. Many historical meteorological observation records are stored in libraries and repositories around the world and are slowly being recovered and used in weather and climate research. Such historical weather observations are being recovered worldwide through “Data Rescue” activities under the international ACRE (Atmospheric Circulation Reconstruction over the Earth) initiative. However, the spatial range of these weather data can be limited. In this study, we focus on the ship log weather records made on vessels sailing along Japan waters during this period. The oldest weather records in the vicinity of Japan were found to be recorded on the ship of the third expedition of James (Caption) Cook in 1779. During the eighteenth-century weather records came mostly from the Expedition cruises. In the nineteenth century, weather records were found from the US Navy and other ships came to Japan to open the country to the wider world. We focus on three tropical cyclone (TC) events in the vicinity of Japan during the period from 21 to 25 July 1853 observed by seven US Naval Japan Expedition of Perry’s fleet, on 23 and 24 September 1856 observed by Medusa of Dutch Navy ship, and on 15 and 16 August 1863 during the bombardment of Kagoshima in Japan observed by eleven UK Navy ships. Tracks of TCs are analyzed based on the ship log weather records.


AS18-A007
Rapid Growth of Outer Size of Tropical Cyclones: A New Perspective on Their Destructive Potential

Yi LI1+, Youmin TANG1#, Shuai WANG2
1Hohai University, 2Princeton University

The destructive potential of a tropical cyclone (TC) is primarily determined by its intensity and outer size. Although TC intensification has been researched extensively, the growth rate of its outer size remains obscure. This prompts us to develop the concept of rapid growth of outer size (RG) of TCs. RG is defined as an increase of at least 75 km in the gale-force wind radius within 24 hr using an objective anomaly detection algorithm. RG is intrinsically linked to the life cycle of the outer size and comprises most of the peak for large TCs (>300 km) in the distribution of lifetime maximum size. Compared with rapid intensification, RG is a more dangerous change in the TC structure, leveling up the destructive potential more rapidly. This is the first attempt to reveal the importance of RG to the outer size climatology, life cycle, and destructive potential of TCs.


AS18-A010
A Seesaw Variability in Tropical Cyclone Genesis Between the Western North Pacific and the North Atlantic Shaped by Atlantic Multidecadal Variability

Liguang WU1, Chao WANG2#+, Bin WANG3
1Fudan University, 2Nanjing University of Information Science & Technology, 3University of Hawaii

Variabilities in tropical cyclone (TC) activity are commonly interpreted in individual TC basins. We identify an antiphase decadal variation in TC genesis between the western North Pacific (WNP) and North Atlantic (NA). An inactive (active) WNP TC genesis concurs with an enhanced (suppressed) NA TC genesis. We propose that the transbasin TC connection results from a subtropical east–west “relay” teleconnection triggered by Atlantic multidecadal oscillation (AMO), involving a chain atmosphere–ocean interaction in the North Pacific. During a negative AMO phase, the tropical NA cooling suppresses local convective heating that further stimulates a descending low-level anticyclonic circulation in the tropical NA and eastern North Pacific as a Rossby wave response, inhibiting the NA TC genesis. Meanwhile, the anomalous southwesterly to the western flank of the anomalous anticyclonic circulation tends to weaken the surface evaporation and warm the SST over the subtropical eastern North Pacific (southwest–northeast-oriented zone from the tropical central Pacific to the subtropical west coast of North America). The SST warming further sustains a cyclonic circulation anomaly over the WNP by local atmosphere–ocean interaction and the Bjerknes feedback, promoting the WNP TC genesis. This transbasin linkage helps us interpret the moderate amplitude of variations in TC genesis frequency in the Northern Hemisphere.


AS18-A019
Impact of Tropical Cyclones Over the Eastern North Pacific on El Niño–southern Oscillation Intensity

Qiuyun WANG1+, Zhe-Min TAN2#
1Ocean University of China, 2Nanjing University

Most tropical cyclones (TCs) generated over the eastern North Pacific (ENP) do not make landfall. Consequently, TCs in this basin have received less attention, especially those that occur away from the mainland. Furthermore, there have been few studies of the climatic effects of ENP TCs. This study explores the feedback relationship between ENP TCs and the intensity of the El Niño–Southern Oscillation (ENSO), including El Niño and La Niña events, from the perspective of accumulated cyclone energy (ACE). Observational and modeling results indicate that the ENP ACE 3 months earlier can still affect the intensity of El Niño and La Niña events, although the SST persistence is main contributor. Thereinto, the impact of ENP TCs on El Niño appears to be approximately equal to that on La Niña. Moreover, this impact is independent of the persistence of the sea surface temperature (SST) in the Niño 3.4 region and the Madden–Julian Oscillation. Generally, the greater the ENP ACE, the stronger the El Niño, and the smaller the ENP ACE, the stronger the La Niña, this is especially the case for those TCs that develop over the July‒September period. In addition, results show that the ENP TCs modulate ENSO intensity by changing anomalous zonal wind at the low-level atmospheric layer. And the joint impacts of the low-level zonal wind anomalies on the Walker circulation and the east-west thermocline gradient lead to the time characteristics that ENP TCs lead ENSO intensity by about 3 months.


AS18-A036
Long-term Analysis of Tropical Cyclone Intensity Using MPI Theory Based on HighResMIP Projections

Shun ITO#+, Nobuhito MORI, Tomoya SHIMURA, Takuya MIYASHITA
Kyoto University

In addition to sea level rise, other effects of global warming have already been observed. The intensification of tropical cyclones (TC) is also no exception. This study shows how TCs will change in the future using MPI (Maximum Potential Intensity) theory, which estimates the maximum development of TCs for given climatological environmental conditions. This study presents future changes in TCs based on HighResMIP (High-Resolution Model Intercomparison Project). This projection focuses on the intercomparison of TC intensities, providing high-resolution data and estimating the effect of atmosphere-ocean coupling. The scenario-based projections show intensified TC trends in the monthly mean MPI in the Western North Pacific, although each mode of HighResMIP has different characteristics. There is also likely to be a spatial error between MPI and the maximum development value of TCs from track data of HighResMIP. MPI mostly depends on SST (Sea Surface Temperature). Therefore, it is important to reveal the north-south difference. By clearly quantifying this difference, we can accurately estimate TC intensity in each area over the long term and significantly contribute to predicting future changes in maximum storm surge risk. The detail of the results will be presented at the conference.


AS18-A034
Effect of Model Resolution on Simulation of Tropical Cyclone Landfall in East Asia Based on a Comparison of 25- and 50-km HiRAMs

Kuan-Chieh CHEN1#+, Chihhua TSOU2, Chi-Cherng HONG1, Huang-Hsiung HSU3, Chia-Ying TU3
1University of Taipei, 2National Taiwan Normal University, 3Academia Sinica

The effect of model resolution on the simulation of tropical cyclone (TC) landfall frequency in East Asia [including the South China Sea (SCS), Taiwan and coastal areas of East China (TWCN) and Japan (JP)] was investigated by comparing Atmospheric Model Intercomparison Project (AMIP) type simulations on the basis of 50-km High Resolution Atmospheric Models (HiRAMs) and 25-km HiRAM. The number of TC landfalls in the TWCN region was realistically simulated by the 50-km HiRAM ensemble model. However, fewer (more) TCs were steered westward (northward) toward the SCS (JP) because of an overestimation of the monsoon trough in the western North Pacific (WNP). The overestimation created a low-level cyclonic circulation anomaly in the WNP, which substantially modified steering flow. Consequently, more (less) TC made landfall in JP (SCS). The overestimation of the monsoon trough in model was primarily resulted from compounding factors, including the AMIP type simulation, upscale feedback of TCs to mean flow and the monsoon flow–topography interaction in the Indochina Peninsula Mountains and Philippine. First, the SST was negatively correlated with precipitation in the WNP during the typhoon season for the observation. Conversely, the SST–precipitation relationship was positive in the AMIP run. Second, the upscale feedback of TCs to mean flow (monsoon trough) was overestimated, which in term contributed to the overestimation of monsoon trough. Third, the model underestimated the mountain lifting effect in the Indochina Peninsula and Philippine. Overall, the aforementioned biases were substantially improved by increasing model’s horizontal resolution from 50-km to 25-km HiRAM.


AS18-A049
Rainfall Strength and Area from Landfalling Tropical Cyclones Over the North Indian and Western North Pacific Oceans Under Greenhouse Warming

Mincheol MOON1+, Kyung-Ja HA2#
1Pohang University of Science and Technology, 2Pusan National University

Climate change due to greenhouse gases has fueled more powerful tropical cyclones (TCs). However, their characteristics and future changes of rainfall strength (RS) and rainfall area (RA) of TCs in regional scales are not fully revealed yet. Here, using ultra-high-resolution coupled simulations, we investigate the dominant factor in rainfall characteristics due to landfalling TCs in the North Indian Ocean (NIO) and western-North Pacific (WNP) and their future change in response to doubling and quadrupling atmospheric CO2 concentrations. As CO2 increases, RS increases more than RA in the NIO, but the opposite changes indicate in the WNP. We demonstrate that RS is highly related to the lifetime maximum intensity, landfall intensity, and latent heat flux (LHFLX), while RA mainly depends on LHFLX, relative humidity at 600 hPa, and vertical wind shear over the WNP. Our results suggest the need to establish regional-scale adaptation strategies for future rainfall change in landfalling TCs.


Tue-01 Aug | 1:10 - 3:10 | MR327
AS23 - Observations, Remote Sensing, and Modeling of Tropospheric Composition and Air Quality in Asia and the Transpacific Region

Session Chair(s): Jason COHEN, China University of Mining and Technology, Meiying Melissa MARTIN, NASA

AS23-A026 | Invited
Tracking Air Pollution in China from Space Using Artificial Intelligence

Jing WEI1#, Zhanqing LI1,2+
1University of Maryland, 2Beijing Normal University

Exposure to ambient air pollution, including fine particulate matter (PM2.5) and trace gases like ozone (O3) and nitrogen dioxide (NO2) at the ground level, poses serious threats to environmental quality and public health, significantly increasing the risk of death. Satellite remote sensing allows for generating spatially continuous PM2.5 data, but current datasets have overall low accuracies with coarse spatial resolutions limited by data sources and models. Air pollution levels in developing countries like China have experienced dramatic changes over the past couple of decades. To reveal the spatiotemporal variations, artificial intelligence, including machine and deep learning, is extended by considering the spatiotemporal heterogeneity of air pollution to generate long-term and high spatiotemporal-resolution outdoor air pollutants from big data that integrate ground-based measurements, satellite remote sensing products, atmospheric reanalysis, and model simulations. The application and fidelity of the dataset are demonstrated by analyzing their spatial distributions and temporal variations of surface air pollution, exposure risk to the public, and the COVID-19 pandemic. These novel products have been widely employed to address a variety of atmospheric, environmental, ecological, and public health issues.


AS23-A047
Emissions of Nitrous Acid (HONO) and Nitric Oxide (NO) from Soils and its Impact O3 Pollution

Tong SHA#+
Shaanxi University of Science and Technology

Reactive nitrogen gases including NOx and HONO strongly affect the atmospheric oxidization capacity through the contribution to the hydroxyl radicals (OH) and ozone (O3). Although stringent anthropogenic NOx emission controls policies have been implemented in past years, observations show that the surface O3 concentrations in China are still increasing. Soils are important sources of emissions of NO and HONO that have been overlooked in previous studies; however, there is still a lack of research on the quantitative effects of soil nitrogen emissions on O3 pollution in China. Since atmospheric HONO sources are not well understood, and the default HONO formation mechanism (NO + OH → HONO) always severely underestimates HONO observations and atmospheric oxidation capacity as a result, we first added HONO source from soil bacteria and other four potential sources (traffic emissions, NO2 heterogeneous reactions on ground and aerosol surfaces, and inorganic nitrate photolysis in the atmosphere) in the WRF-Chem model. Soil NOx emissions are also estimated by a new mechanistic parameterization, the Berkeley Dalhousie Iowa Soil NO Parameterization (BDISNP).In this study, the improved WRF-Chem model coupled with a new soil reactive nitrogen emissions (SoilNr) scheme is applied to quantitatively assess of the effects of soil NOx and HONO on ozone formation separately, and their combined effect on ozone formation in the North China Plain. The results of this study highlight the previously underappreciated important role of SoilNr on O3 pollution and provide scientific basis for designing ozone pollution regulation strategies.


AS23-A039
The Exploration of 2015-2019 Surface Background Ozone Over China: A Model Study by GEOS-Chem High Performance (GCHP)

Xingpei YE1#+, Lin ZHANG1, Xiaolin WANG1, Danyang LI1, Jiayu XU1, Ni LU1, Xiao LU2
1Peking University, 2Sun Yat-sen University

Here we apply a state-of-art global chemical transport model GEOS-Chem High Performance (GCHP) to understand the sources contributing to Chinese background (CNB) daily maximum 8 h average (MDA8) ozone, and to identify the driving factor of its interannual variability from 2015 to 2019. The five-year-mean CNB ozone is estimated as 37.8 ppbv, showing a general west-to-east downward spatial gradient. The national-mean CNB ozone is the largest in summer (42.5 ppbv), but distinct seasonality can be seen at different regions. Using the tagged ozone technique, we show that the high background levels in western China are due to abundant transport from the free troposphere and adjacent foreign regions, while in eastern China, domestic ozone formation near the surface from natural precursors is also important and exhibits intensive seasonal variation. We find the greater importance of biogenic volatile organic compounds (VOCs) over soil NOx to ozone as reported in previous studies is reversed when domestic anthropogenic emissions are turned off, reflecting a more NOx-sensitive ozone chemical regime in a “clean” atmosphere. The interannual variability (IAV) of CNB ozone shows the peak in summer, with standard deviation values during five years of ~5 ppbv over Qinghai-Tibet Plateau (QTP) and >3.5 ppbv over vast eastern China. CNB levels in QTP are found to be well correlated with horizontal circulation anomalies at 500 hPa, while in the east, year-to-year changes in soil NOx emissions dominate the IAV of CNB ozone. We also explore the role of El Nino-Southern Oscillation (ENSO) in modulating the IAV of CNB ozone over southern China in spring, and find that the El Nino (La Nina) event has opposite effects on Southeast China and Southwest China.


AS23-A014
Observational Evidence of Aerosol Radiation Modifying Photochemical Ozone Profiles in the Lower Troposphere

Bin ZHU1#+, Shuangshuang SHI1, Yan CAI2
1Nanjing University of Information Science & Technology, 2Nanjing University of Post & Telecommunications

Aerosol optical effects can trigger complex changes in solar shortwave radiation in the atmosphere, resulting in significant impacts on the photochemistry and vertical structure of ozone. This study provides observational evidence of aerosol absorbing and scattering effects on modifying the shortwave radiation and ozone profiles in the low troposphere. Using field vertical measurements and observation-based model simulations, we demonstrated that absorbing aerosols decreased shortwave radiation, resulting in substantial inhibition of ozone production throughout the boundary layer (BL). A similar inhibition effect occurred within the lower BL under sufficient scattering aerosols. However, the scattering augmentation effect played an additional role in enhancing the photolysis rate and promoting ozone generation in the upper BL. Hence, the observational evidence as well as our model simulations disentangled the radiative effects of different types of aerosols on the vertical structures of ozone.


AS23-A038
A Spatial Interpretable Deep Learning Model for Satellite-based O3 Estimation in China

Nana LUO1#+, Jiawei ZHANG1, Mingyi DU1, Wenji ZHAO2, Xing YAN3
1Beijing University of Civil Engineering and Architecture, 2Capital Normal University, 3Beijing Normal University

Surface ozone (O3) pollution has become a major public health concern in China. To accurately estimate the spatial-coverage O3 from sparse ground-truth data, we propose a two-stage deep learning model that combines convolutional neural networks (CNN), deep neural network (DNN), and integrated gradients (IG). This model is able to monitor large-scale O3 dynamics with greater temporal and spatial accuracy than that achieved by current models (R2 = 0.78 and RMSE = 18.35 μg/m3). Using the integrated IG, we are also capable of interpreting the contribution of nearby cities to O3 in a targeted site (i.e., Beijing) even under dust storms conditions, which traditionally limits model accuracy. In clean days, especially during summer when O3 concentrations are often high, the surroundings have positive scores ranging from 0.05 to 0.11, indicating that these areas enhance O3 formation. Conversely, during dust storms, the surrounding dust cells have negative IG scores, ranging from -1.43 to - 0.01, indicating that these areas inhibit the formation of O3. This study provides a novel strategy to extract spatial dependence among predictors to estimate O3 with high accuracy while obtaining spatial-coverage interpretation. It also contributes to further our understanding of O3 pollution dynamics, and is applicable to the monitoring of other noxious air pollutants.


AS23-A028
Ozone in the Lower Boundary Layer and its Influence on Surface Ozone: Insights from 3-year Tower-based Observations in South China and Regional Air Quality Modeling

Guowen HE#+, Xiao LU, Shaojia FAN
Sun Yat-sen University

We present 3-year (2017-2019) tower-based measurement of lower boundary layer (up to 500m) ozone and examine its interaction with surface ozone from the Canton Tower in Guangzhou, the core megacity in South China with severe ozone pollution. Measurements of ozone, CO, NO2, and meteorological parameters are available at 10m, 118m, 168m, 488m. We find that ozone concentrations increase with altitude, with ozone concentration higher by 1.8-3.3 times at 488m level than that at the surface. The diurnal cycle of ozone is consistent throughout the lower boundary layer, Regional air quality model (CMAQ) simulations show that chemical loss and dry deposition are the main sinks of surface ozone contributing to 55 ppbv·hr−1, shaping the strong ozone vertical gradients. On ozone polluted days, the average ozone is higher by 1.5~2.2 times at 488m level than that on clean days. The ratio of nighttime to daytime ozone range from 69%~90% at 488m level, suggesting that a large proportion of daytime ozone can be stored in the nighttime residual layer. We also find significant positive correlation coefficients between 488m nighttime ozone and the following day surface MDA8 ozone, indicating nighttime ozone in the residual layer is a critical ozone factor in forecasting surface ozone in the following day. The tower-based measurements capture the ozone decreases at the 488m level with increases at lower altitude during the nocturnal ozone enhancement (NOE) event (defined as nighttime ozone concentration increases by more than 5ppbv in one of any two adjacent hours), supporting that the enhanced vertical mixing between the surface and the residual layer is an important contributing factor to NOE events. Our study highlights the value of long-term tower-based measurements for understanding the coupling between air pollution and boundary dynamics.


AS23-A074
Impact of Aerosol Radiative Effects on Surface Ozone in Megacity Delhi, India

Lakhima CHUTIA, Jun WANG#+
The University of Iowa

Atmospheric aerosols can influence ozone (O3) by modulating photolysis rates (aerosol–photolysis interaction, API) and through meteorological feedback (aerosol–radiation feedback, ARF). This study attempts to assess the impact of API and ARF on surface O3 and fine particulate matter (PM2.5, aerodynamic diameter ≤2.5 µm) during a pollution episode in November-December 2018 in megacity Delhi, India using the Unified Inputs (initial/boundary conditions) for WRF-Chem (UI-WRF-Chem) model. The UI-WRF-Chem uses MERRA-2 data to provide both meteorological and chemical initial and boundary conditions for the regional WRF-Chem model. Our model reasonably well captured the observed diurnal variations of surface O3 and PM2.5 with a good correlation (r = 0.52–0.90) in megacity Delhi. API considerably lowers the surface photolysis rates (18–20%) and reduced surface O3 concentration by 6% over the study region. The ARF shows a small increase in O3 concentration (2%) and as a result, the combination of ARF and API contributes to an overall reduction in surface O3. Aerosol-induced solar dimming (50 Wm-2) due to ARF led to cooling (1 K) at the surface, suppresses the development of the planetary boundary layer (180 m), and further hinders the PM2.5 dispersion, resulting in an enhancement in surface PM2.5 concentration by 24% in megacity Delhi. Contrarily, the lower abundances of atmospheric oxidants caused by the API constrain the secondary aerosol formation, thereby lessening the ARF effects on PM2.5. The combined effect of API and ARF results in a net increase (16%) of surface PM2.5. The API and ARF have important implications on the mitigation of higher pollution loading in Delhi, particularly during the post-monsoon and winter seasons.


AS23-A009
Implementation of Modified Halogen Chemistry Over South Korea

Kiyeon KIM1+, Chul Han SONG1#, Kyung Man HAN1, Greg YARWOOD2, Beardsley ROSS2, Bonyoung KOO3, Minchan KIM4
1Gwangju Institute of Science and Technology, 2Ramboll, 3Bay Area Air Quality Management District, 4Cheju National Univeristy

Halogen radicals (Cl, Br, and I) can strongly affect oxidation capacity as a product of photochemical reactions in atmosphere. Several Studies from 3-D chemical transport models and field observations have discovered the formation of nitrogen oxides and ozone through halogen radicals over a variety of regions and weather conditions. In addition, during KORUS-AQ campaign from 08 May to 12 June 2016, many studies measured not only nitrogen oxides and ozone but halogen species of nitryl chloride (ClNO2) and chloride (Cl2) as a precursor of chlorine radicals. However, current knowledge of halogen chemistries has not been fully understood due to insufficient study in South Korea. Therefore, this study aims to facilitate halogen chemistry including chlorine, bromine, and iodine species and evaluate the impacts of halogen chemistry on the atmospheric species during the KORUS-AQ campaign for the first time in South Korea. The modification was incorporated into the CMAQ modeling system as follows: i) preparing emissions (Cl2, HCl, HBr, and Br2 for anthropogenic source; BR2, I2, and HOI and other inorganic species from GOCI chlorophyll-a for natural source;) and ii) modifying/adding 139 gaseous, 7 aqueous, 18 heterogeneous reactions. In conclusion, impact of chlorine emission (5990Mg of HCl and 451Mg of Cl2 in EXP1) enhances ozone (~1.6%) and OH mixing ratios (~5.4%), and reduces nitrate concentrations (~6.2%) in South Korea. The newly updated chlorine chemistry can capture ClNO2 and Cl2 mixing ratios (EXP2). Furthermore, ozone destruction and formation mechanisms exhibited by bromine and iodine chemistry in the ocean (~2.3% in EXP3) and updated bromine chemistry over land (~0.3% in EXP4), respectively. Collectively in this study, halogen emissions and modified halogen chemistry reproduced the levels of ClNO2, nitrate, and ozone in the Korean peninsula and can help further understand halogen radicals in the CMAQ model simulation.


Tue-01 Aug | 1:10 - 3:10 | MR328
AS24 - Machine Learning applications in the field of atmospheric pollution

Session Chair(s): Shovan Kumar SAHU, Centre for Climate Research Singapore, Ge SONG, Wuhan University, Jia XING, George Mason University

AS24-A001
Ensemble Surface Ozone Forecast Using Deep Learning and Implications for Surface Ozone Predictability

Aoxing ZHANG1#+, Tzung-May FU1, Xu FENG2, Jianfeng GUO3, Chanfang LIU3, Jiongkai CHEN1, Jiajia MO1, Xiao ZHANG4, Xiaolin WANG5, Wenlu WU1, Yue HOU1, Honglong YANG6, Chao LU6
1Southern University of Science and Technology, 2Harvard University, 3Shenzhen Ecology and Environment Monitoring Centre of Guangdong Province, 4Tsinghua University, 5Peking University, 6Shenzhen National Climate Observatory

Surface ozone forecast accuracy is limited by weather forecast uncertainties, which are not quantitatively represented in current air quality forecast systems. We developed an ensemble surface ozone forecast (2DCNN-ESOF) system using 2-D convolutional neural network and ensemble weather forecasts, and we applied the system to 216-h ozone forecasts in Shenzhen, China. The 2DCNN-ESOF’s skills were comparable to or better than other current operational systems and fulfilled the Chinese mandate for air quality level forecast accuracies up to 144-h lead time. Additionally, the 2DCNN-ESOF enabled an “ozone exceedance probability” forecast given the range of possible weather outcomes. Half of the ozone forecast errors were due to weather forecast uncertainties, which would induce a 7.4 ± 1.4 μg m-3 uncertainty in forecasted ozone concentrations at 24-h lead time even with perfect emission estimates and chemical mechanisms. Our ensemble forecast framework can be applied to the operational forecasts of other meteorology-dependent environmental risks.


AS24-A007
Deep Neural Network with Improved Features Suitable for Adjacent Sites is Introduced to Predict Future PM2.5 Concentration

Siwei LI#+, Mengfan TENG
Wuhan University

Machine learning has become a powerful tool to establish models for predicting the future PM2.5 concentration, which can help the policy makers to take control measures to protect on human health and promote sustainable urban development. The spatial information of adjacent sites can well reflect the regional pollution pattern, however it has not been widely investigated in most existing prediction models. In this study, a novel hybrid model is used to select appropriate adjacent site information and add it into the deep learning prediction model as additional features. This hybrid model combined long and short-term memory neural network (LSTM) and a convolutional neural network (CNN) of 1 * 1 specific convolution kernel to solve the challenges of time series data prediction and discrete data aggregation. The experimental results showed that the novel hybrid model presented the highest prediction accuracy and the lowest error (R2=0.92-0.94, RMSE=8.54-8.93μg/m3, MAE=5.76-6.52μg/m3) compared with single models (R2=0.81-0.92, RMSE=9.01-13.24μg/m3, MAE=6.79-9.34μg/m3). The comparison with other similar research sets shows that the deep learning model significantly improves the ability to capture peak PM2.5 concentration by adding information from appropriate adjacent sites.


AS24-A015 | Invited
Predicting PM2.5 Levels in Delhi Using Long Short-term Memory

Sanchit BEDI#+, N.M. Anoop KRISHNAN, Sri KOTA, Arpit KATIYAR
Indian Institute of Technology Delhi

The study utilized a Recurrent Neural Network architecture with Long short-term memory to predict PM2.5 levels in Delhi. Four different models were developed, each incorporating different combinations of data inputs. The models that utilized PM2.5 data alone or in conjunction with gaseous pollutants exhibited the best performance in predicting PM2.5 concentrations during both hourly and daily forecasts. The models were also evaluated for their performance during specific events characterized by a drastic increase in PM2.5 concentrations. The evaluation revealed that the models that incorporated gaseous pollutants displayed superior performance compared to others during such episodes. The results demonstrated that the models were effective in providing accurate predictions, but only for forecast windows limited to twelve hours for hourly forecasts or seven days for daily forecasts. Due to the difficulty in predicting gaseous pollutants, it is more practical to employ models that only utilize PM 2.5 data or PM 2.5 and meteorological information. The outcomes of this research can serve as decision-making tools for regulators seeking to implement timely interventions in heavily polluted cities, thus imparting a sense of assurance in the potential of these models.


AS24-A016
Improving Air Quality Forecasting Using a Physics-based Machine Learning Approach

Sanchit BEDI#+, N.M. Anoop KRISHNAN, Sri KOTA
Indian Institute of Technology Delhi

Air quality is a pressing issue worldwide, with 90% of people exposed to unhealthy air. Chemical transport models are frequently used in the absence of dependable monitoring networks. These models integrate meteorology, emissions inventory, and atmospheric chemistry to forecast air quality. However, due to the high computational power necessary for each operation, such systems may not be the most efficient or effective early warning systems. An alternative to traditional modeling is Machine Learning models, which require little time and computational resources after being trained. Physics-based machine learning is a developing field that combines Partial Differential Equations, simulated data, and models in a data-driven approach that penalizes physically inconsistent results. Another way to utilize Machine Learning is by parameterizing a physical model. In our study, we utilized 4 years of simulated WRF-Chem data over the Indian subcontinent to apply a physics-based machine learning approach to improve upon the existing model. Our findings reveal that the trained model is efficient and performs well.


Tue-01 Aug | 1:10 - 3:10 | MR329
AS11 - Atmospheric Chemistry in Highly Polluted Environments: Emissions, Fate, and Impacts

Session Chair(s): Sri KOTA, Indian Institute of Technology Delhi

AS11-A021 | Invited
Absorption Enhancement of Black Carbon Aerosols Constrained by Mixing-state Heterogeneity

Jinghao ZHAI1#+, Xin YANG1, Ling LI2, Bin BAI3, Pengfei LIU3, Yuanlong HUANG4, Tzung-May FU1, Lei ZHU1, Zhenzhong ZENG1, Shu TAO1, Xiaohui LU2, Xingnan YE2, Xiaofei WANG2, Lin WANG2, Jianmin CHEN2, Huizhong SHEN1, Jianhuai YE1, Chen WANG1
1Southern University of Science and Technology, 2Fudan University, 3Georgia Institute of Technology, 4California Institute of Technology

Atmospheric black carbon (BC) has a large yet highly uncertain contribution to global warming. When mixed with non-BC/coating material during atmospheric aging, the BC light absorption can be enhanced through the lensing effect. Laboratory and modeling studies have consistently found strong BC absorption enhancement, while the results in ambient measurements are conflicting, with some reporting weak absorption enhancement even for particles with large bulk coating amounts. Here, from our direct field observations, we report both large and minor absorption enhancement factors for different BC-containing particle populations with large bulk non-BC-to-BC mass ratios. By taking insights into the measured coating material distribution across each particle population, we find the level of absorption enhancement is strongly dependent on the particle-resolved mixing state. Our study shows that the greater mixing-state heterogeneity results in the larger difference between observed and predicted absorption enhancement. We demonstrate that by considering the variability in coating material thickness into the optical model, the previously observed model-measurement discrepancy of absorption enhancement can be reconciled. The observations and improved optical models performed here highlight the importance of mixing-state heterogeneity on BC’s radiative forcing, which should be better resolved in large-scale models to increase confidence when estimating the aerosol radiation effect.


AS11-A033
Underestimation of Summertime Urban Ammonia Emissions in Beijing, China : lmplications for Air Quality

Jiayu XU1#+, Lin ZHANG1, Mengran LU1, Yixin GUO2
1Peking University, 2The Hong Kong University of Science and Technology

Ammonia (NH3) emission reduction has been advocated for its potential to mitigate PM2.5 air pollution, yet emission quantifications at city levels are limited. Here we develop high-resolution (3 km) bottom-up emission inventories of agricultural NH3 in the Beijing-Tianjin-Hebei (BTH) region and traffic NH3 in Beijing for the year 2016. Then the WRF-Chem model is used to evaluate the NH3 and PM2.5 concentrations against ground-based and satellite observations. Our estimated annual BTH agricultural NH3 emissions (625 Gg) and Beijing’s traffic emissions (7.8 Gg) are within the ranges of published inventories. However, simulated NH3 concentrations are significantly lower than observations during August in urban Beijing, nevertheless wintertime underestimations are much more moderate. Further evaluation and sensitivity experiments show that biases in meteorology or regional transport cannot explain such discrepancies. Using measurements as constraints, our inversed NH3 inventory indicates both agricultural and non-agricultural NH3 emissions in Beijing during August should increase by ~5 times to match NHand PM2.5 observations. Current underestimations may stem from the missing power sector, urban green space emissions, the lack of representation of industrial hotspots, and uncertainties in traffic emissions. Our study highlights that denser and more frequent urban NH3 observations are urgently needed to constrain and validate bottom-up inventories.


AS11-A035
Identification of Influencing Parameters from Agriculture Sector for Developing Region-specific Emission Inventory

Thirunagari BABY KEERTHI1#+, Sri KOTA1, Rajesh KUMAR2
1Indian Institute of Technology Delhi, 2University Corporation for Atmospheric Research

Air pollution constitutes one of the major global threats to both the environment and human health. Pollutant emissions from various agricultural activities cause significant environmental impacts are highly understudied and call for the preparation of a detailed emission inventory. Emission inventories are a useful tool for comprehending the sources of pollutant emissions and their overall effects on the environment. Most nations and regions do not include entire agricultural operations during the process of developing an emission inventory (EI) for their agricultural sector. Additionally, there hasn't been enough work done to improve our understanding of agricultural emissions’ effects on the ecosystem. Listing emissions by source and quantity for each tracked pollutant enables defining their primary emission sources. However, comprehensive datasets associated with emissions and agricultural activities are often missing. The lack of data is mainly because of the false perception that the agriculture sector emits much smaller pollutant(s) quantities compared to other sources. Data non-availability impedes the ability to develop appropriate policies (that could lower the emissions), leading to decreased interest for collecting relevant data by pertinent authorities which consequently results in less research on agricultural emissions. Instead of using models based on laboratory research, gathering activity data (such as fertilizer application, crop burning, equipment usage, pesticides, livestock management, tillage, etc.) from field operating conditions helps in determining the actual real-world agricultural emissions and their significant sources. Large deficits in activity data causes high degrees of uncertainty in the results of EI. This article identifies and delineates the influencing parameters to develop an EI for the agriculture sector of a region. The requirement for the collection of apposite data, types of influencing data, data sources, the parametric format in which data must be collected, and how each parameter is attributable to the emissions are elucidated in detail.


AS11-A040
Influence of Land Use and Meteorology on Concentrations of Short Lived Climate Pollutants Over India

Diljit NAYAK#+, Gazala Habib HABIB, Sri KOTA
Indian Institute of Technology Delhi

To address the issue of poor air quality in India, a number of emission reduction scenarios were devised, each specific to a certain source. However, many of these scenario-based model simulations overlooked the impact of changes in Land Use Land Cover (LULC) and meteorology on air quality. The study endeavors to assess the influence of these two factors on concentrations of Short-Lived Climate Pollutants (PM2.5, OC, and BC). The simulations were performed using the WRF-Chem V3.8.1 model for the years 2019 and 2024, with emissions remaining constant (2019 emissions) for both years, and only the LULC and meteorology being altered. The results indicate that greater emission reductions are necessary in light of the effect of LULC and meteorology, to achieve the clean air goals set forth in India's national action plan.


AS11-A045
Factors Contributing to Changes in PM2.5 Concentration in South Korea During the Recent Winter Season

Jaein JEONG1#+, Rokjin J. PARK1, Chang-Keun SONG2, Sang-Wook YEH3, Jung-Hun WOO1
1Seoul National University, 2Ulsan National Institute of Science and Technology, 3Hanyang University

This study aims to quantify the contributing factors to changes in winter PM2.5 concentrations in South Korea from 2019 to 2021. We consider various factors, such as meteorological variability, reduced anthropogenic emissions in China, and South Korea's Seasonal Particulate matter Management (SPM) plan. To determine the individual impact of these factors on PM2.5 concentrations, we used nested versions of GEOS-Chem and updated the anthropogenic emissions with observational data. Our simulations captured well the spatial distribution of observed surface PM2.5 concentrations in China and South Korea. Our findings indicate that meteorological variability was the most significant factor affecting PM2.5 concentrations over the past three winters, despite its high level of monthly variability. Furthermore, reductions in anthropogenic emissions in China and the implementation of South Korea's SPM also contributed to changes in PM2.5 concentrations. Since various factors have a complex effect on changes in winter PM2.5 concentration in South Korea, the methodology used in this study will contribute to establishing effective environmental policies in the future.


AS11-A047
Seasonal Variation and Source Identification of Ambient PM2.5 and Associated Water-soluble Inorganic Ions (WSII): A Diurnal Field and Comparative Study of Two Indian Cities

Yash JAIN#+, Sri KOTA, Vivek KUMAR
Indian Institute of Technology Delhi

The air quality in the Indian subcontinent has been a growing concern in recent years, with particulate matter (PM) being one of the major pollutants. PM2.5, in particular, has a significant impact on human health and the environment as it can penetrate deep into the respiratory system. PM2.5 has been linked to several health issues including respiratory and cardiovascular disease, while Water-Soluble inorganic Ions (WSII) contribute to the acidity and salinity of the air. In this study, we aim to investigate the seasonal variation and contributing sources of PM2.5 and 13 associated WSII (Na+, NH4+, K+, Mg2+, Ca2+, Li+, F-, Cl, Br-, NO2-, PO43-, NO3 and SO42−) in two non-attainment Indian cities, Alwar and Amritsar. The study regions are selected owing to the unique meteorological conditions, population density and industrial activities. The study employs a combination of field measurements and comparative analysis to understand the sources and seasonal patterns of PM2.5 and WSII in these cities. Initial analysis of PM2.5 winter samples shows Nitrate (22.078 μg/m3) and Sulphate (17.408 μg/m3) to be the dominant anionic species and Ammonium (13.046 μg/m3) and Sodium (5.452 μg/m3) to be dominant cationic species for both day and night respectively in Alwar city. The total average day anionic concentrations for the same period were observed to be 31.37 μg/m3 and night concentrations to be 52.52 μg/mwith total observed average day cationic concentrations to be 15.23 μg/m3 and night concentrations to be 23.29μg/m3.


AS11-A054
Impact of Improved Representation of VOC Emissions and Photochemistry on Regional Ozone Production During Korus-AQ

Katherine TRAVIS1,2#+, James CRAWFORD2, Benjamin NAULT3
1National Center for Atmospheric Research, 2NASA Langley Research Center, 3Aerodyne, Inc.

Models underestimated ozone, formaldehyde, peroxyacetyl nitrate (PAN) and alkyl nitrate (AN) concentrations in Seoul during the 2016 joint NIER/NASA Korea United States-Air Quality (KORUS-AQ) field study. This indicates needed improvements in emissions and chemistry of volatile organic compounds (VOCs) in a region where photochemistry is radical-limited. Total peroxynitrates (PNs) were twice as large as PAN during the campaign, in contrast to previous studies where missing PNs were <20%. Observations of speciated ANs could only explain 3% of total ANs. This points to the need to evaluate model VOC emissions and chemical mechanisms producing ANs and PNs. We find that model emissions severely underestimate PAN-precursors such as ethanol and methyl ethyl ketone, which contribute approximately 30% and 10% to the PAN budget, respectively. These species may be underestimated from vehicles, or from non-combustion sources such as solvents or cooking. We use the GEOS-Chem chemical transport model to investigate the impacts of improvements in VOC emissions and chemistry on ozone. Scaling emissions of individual VOC species based on KORUS-AQ observations increases surface ozone by ~10 ppb in Seoul, while addition of chemistry to produce missing ANs and PNs reduces ozone in Seoul by ~1 ppb but results in transport of ozone precursors to downwind regions.


AS11-A051 | Invited
Quantifying Nonlinear Chemical Effects of Emission Reductions on PM2.5 Pollution in Beijing Using the Adjoint Method

Ni LU#+, Lin ZHANG, Xiaolin WANG
Peking University

The relationships between emissions and PM2.5 pollution are governed by nonlinear chemistry. Therefore, understanding the role of nonlinear chemistry in the PM2.5 formation pathways is critical for policy-making. Here we analyze the sensitivity of PM2.5 in Beijing to emissions from different precursor species and different regions using the adjoint of the GEOS-Chem chemical transport model, with a focus on the changes in sensitivity in response to precursor emission changes of COVID-19 lockdown and 2013-2017 control policies. This allows us to diagnose the direct effects versus nonlinear chemical effects and analyze the differences and commonalities between long-term and short-term emission reductions. We find significant changes in the sensitivities for secondary inorganic aerosols in response to emission reductions. In the absence of such nonlinear chemical effects, the emission reductions of COVID-19 lockdown and 2013-2017 control policies would reduce the February mean PM2.5 by 10.7 μg/m3 and 63.6 μg/mrespectively in Beijing. However, an increase of 6.3 μg/m3 occurred for each emission reduction scenario due to the increased sensitivities of nitrate to NOx and NH3 emissions, reflecting changes in atmospheric oxidation capacity and gas-particle partitioning. These chemical effects accelerate aerosol formation and offset the effectiveness of emission reductions. Overall, our study highlights the importance of considering nonlinear chemical effects when assessing the effectiveness of emission reduction measures for highly polluted areas.


Tue-01 Aug | 1:10 - 3:10 | MR331
AS01 - The Asian Monsoon, Extremes and Climate Change

Session Chair(s): Namyoung KANG, Kyungpook National University, Jun MATSUMOTO, Tokyo Metropolitan University, Hirokazu ENDO, Meteorological Research Institute

AS01-A014
Role of the intraseasonal IPCO in the Absence of Typhoons in July 2020

Jianping LI#+, Fei LI, Yina DIAO, Hao WANG
Ocean University of China

The influence of the intraseasonal Indo-western Pacific convection oscillation (IPCO) on the absence of typhoons in July 2020 over the western North Pacific (WNP) was explored. While observation analysis shows that necessary conditions such as sea surface temperature (SST) and vertical wind shear in July 2020 meet the basic requirement of or even are conducive to the formation of typhoon, the unprecedented absence of typhoon over the WNP occurred in July 2020, and it is the first time that no typhoon in July since 1951. Additionally, significant differences were found in the number of typhoons in July between the different phases of the intraseasonal IPCO, and the number in the positive phase of the intraseasonal IPCO was significantly higher than that in the negative phase of the intraseasonal IPCO. In July 2020, the intraseasonal IPCO was in a strong negative phase, with the third lowest index in history and had the strongest inhibition effect on convection over the WNP on record, leading to large-scale circulation anomalies. The strongest descending movement on record inhibited the upward transport of water vapor and the development of cumulus convection, thereby reducing the release of latent heat of condensation and making it difficult to form a typhoon warm-core structure. In addition, the geopotential height increased over the WNP, and the western Pacific subtropical high moved southerly, which inhibited typhoon formation. Simultaneously, the South China Sea monsoon trough weakened significantly, with increased negative vorticity anomaly in the response scale, which hindered disturbance generation. The lowest genesis potential index confirmed that the large-scale circulation anomaly caused by the intraseasonal IPCO had an unprecedented restraining effect on typhoon generation, leading to the absence of typhoons over the WNP in July 2020.


AS01-A020
Application of Linear Inverse Modelling to Tropical Interbasin Interaction

Shoichiro KIDO1#+, Ingo RICHTER1, Tomoki TOZUKA2, Ping CHANG3
1Japan Agency for Marine-Earth Science and Technology, 2The University of Tokyo, 3Texas A&M University

A large body of observational and modelling studies has pointed out that two-way interaction of the Pacific Ocean (PO) with regions outside of the PO, such as the tropical Atlantic (AO) and Indian Ocean (IO), plays an important role in tropical climate variability and predictability, and multiple interactions among the three basins are now known as tropical interbasin interaction (TBI). Here, the impact of TBI upon characteristics and predictability of sea surface temperature (SST) in the tropics are assessed by applying a linear inverse modelling (LIM) framework that uses SST and sea surface height anomalies in the tropical Pacific (PO), Atlantic (AO), and Indian Ocean (IO). The TBI pathways are shown to be successfully isolated in stochastically-forced simulations that modify off-diagonal elements of the linear operators. The removal of TBI leads to a substantial increase in the amplitude of El Niño-Southern Oscillation (ENSO) and related variability. Partial decoupling experiments that eliminate specific coupling components reveal that PO-IO interaction is the dominant contributor, whereas PO-AO and AO-IO interactions play a minor role. A series of retrospective forecast experiments with different operators shows that decoupling leads to a substantial decrease in ENSO prediction skill especially at longer lead times. The relative contributions of individual pathways to forecast skill are generally consistent with the results from the stochastically-forced experiments. We will also discuss some typical examples that highlight the importance of TBI on regional SST variability.


AS01-A003
Diverse Impacts of ENSO on Summertime Synoptic-scale Disturbance Intensity Over the Tropical Western North Pacific

Qinlu GU+, Renguang WU#
Zhejiang University

Synoptic-scale disturbances are prominent over the tropical western North Pacific during boreal summer and they play an important role in the weather and climate of East and Southeast Asia through causing extremely heavy rainfall events, seeding tropical cyclone genesis and interacting with low-frequency activities. Those disturbances are generated over the equatorial western-central Pacific and propagate northwestward to the tropical western North Pacific. Thus, understanding the changes and factors of synoptic-scale disturbance intensity over the tropical WNP is an important topic. The intensity of synoptic-scale disturbance is closely related to the El Niño–Southern Oscillation that modulates the seasonal atmospheric fields over the source regions, along the propagation paths, and over the impact regions of the synoptic-scale disturbances. In this talk, we will present analysis of interannual variations of synoptic-scale disturbance intensity over the tropical western North Pacific during boreal summer and the associated factors. Evidences for the asymmetric and nonlinear response of synoptic-scale disturbance intensity to El Niño and La Niña events will be presented along with physical explanations based on observational analysis and numerical model experiments.


AS01-A027
Trans-basin Influence of Southwest Tropical Indian Ocean Warming During Early Boreal Summer

Zesheng CHEN1+, Zhenning LI2, Yan DU1#, Zhiping WEN3, Renguang WU4
1Chinese Academy of Sciences, 2The Hong Kong University of Science and Technology, 3Fudan University, 4Zhejiang University

This study examines the climate response to a sea surface temperature (SST) warming imposed over the southwest Tropical Indian Ocean (TIO) in a coupled ocean-atmosphere model. The results indicate that the southwest TIO SST warming can remotely modulate the atmospheric circulation over the western North Pacific (WNP) via inter-basin air-sea interaction during early boreal summer. The southwest TIO SST warming induces a “C-shaped” wind response with northeasterly and northwesterly anomalies over the north and south TIO, respectively. The northeasterly wind anomalies contribute to the north TIO SST warming via a positive Wind-Evaporation-SST(WES) feedback after the Asian summer monsoon onset. In June, the easterly wind response extends into the WNP, inducing an SST cooling by WES feedback on the background trade winds. Both the north TIO SST warming and the WNP SST cooling contribute to an anomalous anticyclonic circulation (AAC) over the WNP. The north TIO SST warming, WNP SST cooling, and AAC constitute an inter-basin coupled mode called the Indo-western Pacific ocean capacitor (IPOC), and the southwest TIO SST warming could be a trigger for IPOC. While the summertime southwest TIO SST warming is often associated with antecedent El Niño, the warming in 2020 seems to be related to extreme Indian Ocean Dipole in 2019 fall. The strong southwest TIO SST warming seems to partly explain the strong summer AAC of 2020 over the WNP even without a strong antecedent El Niño.


AS01-A011
Effects of Indian Ocean Dipole Initialization on the Forecasting of La Niña One Year in Advance

Jing WANG1, Shouwen ZHANG2#+, Hua JIANG3, Dongliang YUAN1
1Chinese Academy of Sciences, 2Southern Marine Science and Engineering Guangdong Laboratory, 3National Marine Environmental Forecasting Center

The climate systems over the Indian and Pacific oceans interact with each other at the interannual time scales. The Dipole Mode Index(DMI) is found to lead the Niño3 index by more than one year. Traditional understanding of this precursory relationship is thought through the atmospheric bridges, a.k.a. the Walker Cell variability. Latest studies suggest that the oceanic channel process, i.e. the Indonesian Throughflow (ITF) variability, plays a dominant role in the inter-basin interactions, which quickly emerges as a hot research topic. However, due to the concurrent ENSO and Indian Ocean Dipole (IOD) events in history, the effects of an IOD on the evolution of ENSO are contaminated by the repercussions of the ENSO. In 2019, a strong IOD took place in the Indian Ocean, with the tropical Pacific in a neutral state throughout that year, which provides an opportunity to test the effectiveness of the oceanic channel dynamics. A strong La Niña event indeed took place at the end of 2020, the dynamics of which are investigated using the China National Marine Environmental Forecasting Center (NMEFC) operational seasonal forecasting system. The strong subsurface cooling in the Indian Ocean is found to propagate to the eastern equatorial Pacific Ocean through the Indonesian seas and induce a strong La Niña event at the end of 2020, suggesting the dominance of the oceanic channel in the inter-basin forcing leading to the outburst of the 2020/2021 La Niña. In comparison, experiments initialized with only surface temperature anomalies over the tropical Indian Ocean show that the atmospheric bridge alone is unable to induce the onset of the 2020/2021 La Niña. Forecasting experiments of historical ENSO events with and without the IOD initializations suggest that both the delayed feedback of ENSO and the Indo-Pacific oceanic channel dynamics are important in forecasting the ENSO.


AS01-A010
Narrowing Region for Tropical Convections in the Western North Pacific

Namyoung KANG1#+, Sanghyeon YUN1, Chan Joo JANG2
1Kyungpook National University, 2Korea Institute of Ocean Science and Technology

Considering that the subtropical highs and tropical convections are observed as negative and positive vorticities respectively, the large-scale features of the atmospheric environment can be effectively represented using streamfunctions as defined by the Laplacian. By investigating the geographical patterns of streamfunctions from different modes of environmental variability, this study conceptualizes how the subtropical high expands and the region for tropical convections migrates in the western North Pacific. It is confirmed that, owing to the expansion of the subtropical high, the limited ocean area for tropical convections even bounded by the equator becomes narrower in the “La Niña mode” than that in the “El Niño mode”. This study finds that a warmer environment is likely to further expand the subtropical high to the west, and then the westernmost shift in the region for tropical convections appears in the “warmer La Niña mode”. A linear perspective suggests that every warmer La Niña environment could be one that people have scarcely experienced before.


AS01-A063
Physical Processes Driving Mean-state Biases in MetUM Simulations of the Summer West Pacific Subtropical High

Jose M. RODRIGUEZ#+, Mike CULLEN
Met Office

In this work we examine a methodology to study the origin of systematic circulation biases associated to the mean-state West Pacific subtropical high (WPSH) in the Met Office Unified Model (MetUM). MetUM exhibits robust biases, including a weakening of the anticyclone and a location too far east, which leads to an underestimation of the southwesterly monsoon flow over East Asia and contribute to seasonal precipitation errors in the area. We study the development of the errors in an ensemble of equivalent NWP hindcasts and, using a semigeotriptic (SGT) balance model, we link the circulation errors to physical processes. With this tool we show that most of the circulation errors in the WPSH are corrected when tropical convection occurs in the right location. We then examine how MetUM deep convection biases in the region arise and find a large drying of the boundary layer by convection that is balanced mainly by local surface fluxes. In places with low exchange coefficient (places with light surface winds), the surface fluxes are not able to support deep convection over a long time and the convection error is established.


AS01-A089
Roles of the North Indian Ocean SST and Tropical North Atlantic SST in the Latitudinal Extension of the Anomalous Western North Pacific Anticyclone During the El Niño Decaying Summer

Juan FENG#+
Chinese Academy of Sciences

The El Niño-related anomalous western North Pacific anticyclone (WNPAC) shows different latitudinal extensions during the El Niño decaying summer, which determines the moisture transport to different regions and leads to distinct climate impacts over East Asia. It is known that both the north Indian Ocean (NIO) sea surface temperature (SST) and the tropical North Atlantic (TNA) SST can generate a WNPAC in summer. However, the difference between the NIO SST-forced WNPAC and the TNA SST-forced WNPAC has hardly been noted before now. This study shows that the NIO SST warming makes the WNPAC contract southward, whereas the TNA SST warming makes the WNPAC extend northward. The NIO SST warming generates the WNPAC via a Kelvin wave response. Owing to the limited domain of Kelvin wave activity, the Kelvin wave-induced suppressed convection over the western Pacific is confined south of 20°N, resulting in the WNPAC being concentrated in the low latitudes. In contrast, the TNA SST warming generates the WNPAC via a Rossby wave-induced divergence/convergence chain response over the Pacific. The Rossby wave-induced suppressed convection over the central-eastern Pacific north of the Equator leads to enhanced convection on its southwest side, which further generates the low-level anomalous divergent winds over the western North Pacific and suppresses convection there. In this process, the suppressed convection over the western North Pacific is pushed more northward, thus producing a WNPAC extending northward. Further study finds that there are good precursors for predicting the WNPAC latitudinal extension based on the El Niño spatial pattern and the NIO/TNA SST intensity in the previous winter and spring.


Tue-01 Aug | 1:10 - 3:10 | MR332
AS45 - Interaction of Atmospheric Composition and the Asian Monsoon

Session Chair(s): James CRAWFORD, NASA Langley Research Center

AS45-A009 | Invited
The Asian Summer Monsoon Chemical and Climate Impacts Project (ACCLIP)

Laura L. PAN1#+, Paul A. NEWMAN2, Elliot ATLAS3, Troy THORNBERRY4, Bill RANDEL1, Brian TOON5
1National Center for Atmospheric Research, 2NASA Goddard Space Flight Center, 3University of Miami, 4NOAA Chemical Sciences Laboratory, 5University of Colorado at Boulder

The Asian summer monsoon has been recognized in recent decades for its importance in modifying atmospheric composition based on data from modern Earth observing satellites. To understand the influence of Asian monsoon convection on the gas phase chemistry and aerosol loading in the upper troposphere and lower stratosphere (UTLS), a layer of significant climate sensitivity, airborne in-situ measurements are necessary. The ACCLIP campaign was motivated by these needs and was designed to obtain a large suite of trace gas and aerosol measurements in the Asian summer monsoon UTLS outflow over the Western Pacific. After a two-year postponement due to the COVID-19 pandemic, the campaign was successfully carried out during the summer of 2022, with operations based in Osan, South Korea. The campaign used two research aircraft, the NCAR Gulfstream V and the NASA WB-57, and it conducted 29 research flights with measurements ranging from 100 m above sea level to ~19 km altitude across a broad area of the western Pacific (15°N-43°N, 125°E-155°). The US led project received strong international collaboration, particularly from Asia, with multiple regional teams participating with airborne, balloon-borne, and ground-based measurements. This overview will focus on the trace gas measurements, highlighting the novel UTLS observations of species impacting ozone chemistry in the UT, very short-lived substances (VSLS) relevant for stratospheric ozone, and the species contributing to aerosol formation.


AS45-A010
Aerosol Perturbation in the UTLS Region Over the Tibetan Plateau

Dan LI1#+, Janchun BIAN2, Zhixuan BAI2
1Institute of Atmospheric Physics, Chinese Academy of Sciences, 2Chinese Academy of Sciences

The Asian tropopause aerosol layer (ATAL) was thicker than other regions at the same latitude due to the strong confinement effect of the Asian summer monsoon anticyclone. The size distribution of the particles requires further measurements. Aerosol profiles were measured by balloon-borne sensors (Cobald, POPS) launched from Lhasa (29.66 °N, 91.14 °E), Golmud (36.48 °N, 94.93 °E), Kunming (25.01 °N, 102.65 °E) China, from 2019 to 2022 over the Tibetan Plateau at the part of the SWOP (Sounding Water vapor, Ozone, and Particle) campaign. The measurements combined with backward trajectories show that the volcano Raikoke (48°N, 153°E) in June 2019 and the dust storm in March 2021 over the Taklamakan desert have significantly impacted on the aerosol layer in the upper troposphere and lower stratosphere (UTLS). The backscatter ratio at wavelength 455 nm of the volcanic plume and dust storm was 0.1 higher than the ATAL. The particle number density in the volcanic plume is 30 cm-3, higher than the ATAL and dust storm (10 cm-3) in the lower stratosphere, with particle diameters centered around 0.42-3.4 μm. In contrast, the dust storm has a high density of up to 100 cm-3 in the upper troposphere with particle diameters less than 0.42 μm.


AS45-A004
Intraseasonal and Interannual Variability of the Asian Summer Monsoon Transport of CO and Aerosols to the Upper Troposphere and Implications for Global Atmospheric Composition

Mian CHIN1#+, Huisheng BIAN2, Qian TAN3, Ghassan TAHA4, Peter COLARCO5, Paul A. NEWMAN6
1NASA GSFC, 2University of Maryland, Baltimore County, 3Bay Area Environmental Research Institute, 4Morgan State University, 5National Aeronautics and Space Administration, 6NASA Goddard Space Flight Center

We present our study on the intraseasonal and interannual variability of CO and aerosols in the upper troposphere (UT) that are the results induced by the variability of the Asian summer monsoon dynamics. We use the NASA global model GEOS simulations that incorporates emissions from anthropogenic, biomass burning, volcanic, and other natural sources to simulate CO and aerosols from 2000 to 2022 that are evaluated with satellite and aircraft observations. Model experiments separating source types (anthropogenic, biomass burning, volcanic) and source locations (East Asia, South Asia, and Southeast Asia) are used to identify the origin, trends, transport pathways, and spatial/temporal variabilities of CO and aerosols in the UT, and the meteorological data from NASA MERRA-2 reanalysis are used to assess the Asian summer monsoon anticyclone intensity and size associated with climate variability to understand the response of atmospheric composition to the ASM dynamics.


AS45-A005
Tropospheric Ozone Responses to Reductions in Aviation NOx Emissions During COVID-19 Lockdowns

Qi RAN1#+, Shao-Yi LEE2, Wenjie DONG1
1Sun Yat-sen University, 2Kyoto University

Global tight restrictions of the movement have severely affected civil aviation during COVID-19 lockdowns, resulting in noticeable reductions in aviation-related nitrogen oxides (NOx) emissions worldwide. As the formation and depletion of ozone (O3) are mainly driven by its precursors volatile organic compounds (VOCs) and NOx, the emission reductions of NOx from aircrafts are expected to affect ozone concentrations at both the surface and upper troposphere. Given the different effects of tropospheric and stratospheric ozone on human health and climate, the potential changes in ozone concentrations at the surface and upper troposphere are of interest to us. In this study, we quantified the location- and time-resolved emission reductions of aviation-related NOx due to the COVID-19 lockdowns based on open-access air traffic activity data. The Single Column Atmospheric Model Version 6 (SCAM6) was used to simulate the responses of tropospheric ozone to abrupt changes in aviation NOx emissions in 2020. We shall discuss what these simulations reveal about the role of aviation emissions in atmospheric composition and global climate change.


AS45-A008
Atmospheric Ozone and CO Measurements by FTIR at Koror, Palau (7.34°N, 134.47°E)

Xiaoyu SUN1#+, Mathias PALM2, Justus NOTHOLT2, Katrin MUELLER3
1University of Bremen, Institute of Environmental Physics, 2University of Bremen, 3Helmholtz Centre for Polar and Marine Research

This study aims to explore the impact of the Asian Monsoon on atmospheric ozone (O3) and Carbon monoxide (CO) in the Western Pacific (WP) region, using measurements collected from August 2022 at the site of Koror, Palau (7.34°N, 134.47°E). The measurements of O3 and CO are conducted using a solar absorption Fourier transform infrared (FTIR) spectrometer. O3 and CO concentrations in WP are simulated by the GEOS-Chem global 3-D chemistry transport model. Balloon sondes of O3 were launched two to four times per month in Koror to get the O3 profiles from the surface to around 30 km. CO and O3 measurements from different instruments and model simulation results are compared. The results will provide a deeper understanding of the relationship between the Asian Monsoon and atmospheric O3 and CO in the WP region, using data from a specific time period. Comparing the measurements with simulations of the GEOS-Chem model offers insights into the dynamics of atmospheric composition and tests how well the current model’s understanding of WP is. Furthermore, this study provides an evaluation of the emission processes and source regions of O3 and CO pollution in the WP region.


AS45-A016
The Decline of the Winter Cloudy Days Over China Under Global Warming

Hui TAN#+, Zhiwei ZHU
Nanjing University of Information Science & Technology

Winter cloudy days (CDs) in China exhibits strong spatiotemporal variability which has a large impact on agriculture, transportation and solar photovoltaic power industry. While the physical mechanism of CDs variability over China remains unclear, it is unknown what are the future changes of CDs under global warming. Here we reveal the spatiotemporal feature of the leading mode of winter CDs in China and its two independent formation mechanisms. The future changes of winter CDs under global warming are further projected using the optimal state-of-the-art models which are capable in simulation the two formation mechanisms in historical period. Results show that 1) the leading mode of winter CDs presents a homogeneous pattern over China. The positive CDs anomaly is related to the anomalous southerly wind over the western flank of the lower level North Pacific anomalous anticyclone and the southeastern flank of lower level Asian anomalous cyclone, which is related to the Eurasian Rossby wave train and the convection over Maritime Continent; 2) the optimal models projects a significant decrease of CDs in Tibetan Plateau and southern China, and nearly unchanged CDs over northern China under global warming; 3) The warming trend of surface air temperature in Arctic (around Barents Sea) is the possible reason for the decreasing winter CDs in Tibetan Plateau and southern China in the future.


AS45-A006
Footprints of El Niño and La Niña on the Particulate Matter Evolution Over Subtropical Island Taiwan

Yen-Ta FU1+, Ming-Cheng YEN1#, Neng-Huei LIN1, Hai BUI-MANH1, Cheng-Chih LIN2, Jia-Yuh YU1, Chi-Ming PENG3, Duc-Tu DINH4
1National Central University, 2Air Force Institute of Technology, 3WeatherRisk Explore Inc., 4Vietnam Meteorological and Hydrological Administration

Particulate matter (PM), which causes severe problems in human health, has become an important global issue in recent years. However, the climatology of annual variations and the interannual variations in PM level are still not fully evaluated. In our research, we find that the vertical motions of the East Asian monsoon system can affect the development of boundary layer height and then regulate the annual variation in PM over Taiwan. By understanding the annual variation in PM climatologically, the PM pollution season in Taiwan, from October to the following April, can be delineated. Then, we further define five phases of the PM pollution lifecycle that are similar to the well-defined East Asian summer monsoon lifecycle: onset (PM10 onset date, PMOD), active (November to January, NDJ), break (between the end of January and early February), revival (February to April, FMA) and retreat (PM10 retreat date, PMRD). After the precise definition of the PM pollution lifecycle, the interannual variation in PM level is clearer. Both the starting (PMODs) and ending (PMRDs) dates of PM pollution seasons are earlier during El Niño episodes than during La Niña episodes, in particular a significant 20-day difference between their starting dates. For the active phase (NDJ), climatological PM pollution development does not show distinct features under the two different El Niño-Southern Oscillation (ENSO) episodes. On the other hand, the influence of El Niño and La Niña on PM pollution during the revival phase (FMA) is significant. In summary, the climatology of PM pollution in wintertime is dominated by the annual seasonal cycle, but in the seasonal transition periods, October and March are significantly modulated by ENSO.


AS45-A017
Anthropogenic vs. Biogenic Secondary Organic Aerosols in a Warm and Humid Tropical Urban Environment

Hyoungmook PAK1#+, Bao Ngoc THAI1, Santo V. SALINAS1, Simon O'MEARA2, Liya YU1
1National University of Singapore, 2National Centre for Atmospheric Science

Secondary organic aerosols (SOAs) comprise a substantial portion of urban PM2.5 concentrations, and can be formed through gaseous reactions of volatile organic compounds (VOCs). To mitigate urban PM2.5 by reducing SOAs, this study investigates VOC-borne SOAs and explores the associated emission sources via a box chemical reaction model (PyCHAM), incorporating >110 measured VOCs. The VOC-borne SOAs (173.2±146.7 ng/m3) on average account for approximately >20% of total SOAs in PM2.5. Anthropogenic (AVOCs) and biogenic VOCs (BVOCs) account for ~85% and ~7% of the total VOC-borne SOAs, respectively. Synergistic effects of both AVOCs and BVOCs lead to ~10% of the formed SOAs. We investigated the potential overestimation of biogenic SOAs (BSOAs) due to the inclusion of VOCs that are likely emitting from volatile chemical products (VCPs), such as fragrance chemicals in household cleaning products. Excluding six potential VCP-borne VOCs decreases the BSOAs by more than 60%. This indicates anthropogenic SOAs (ASOAs) could account for >85% of total VOC-borne SOAs with lesser contribution from BVOCs in the warm humid tropical urban environments.


Tue-01 Aug | 3:30 - 5:15 | MR323
AS18 - The Science and Prediction of Tropical Cyclones

Session Chair(s): Kosuke ITO, Kyoto University, Yi-Hsuan HUANG, National Taiwan University

AS18-A062
Tropical Cyclone Motion Under Global Warming –Track Cluster Analysis

Yi-Hsuan HUANG1+, Yi-Chen LI1, Chun-Chieh WU1#, Huang-Hsiung HSU2, Hsin-Chien LIANG2
1National Taiwan University, 2Academia Sinica

Tropical cyclone (TC) motion determines areas affected by the TC, and has a consequential effect on the severity of TC impacts. This is because TC motion modulates TC characteristics by exposing it to environments that regulate the subsequent TC behaviors, including TC intensity and structure. In the existing literatures, the impact of global warming on TC translation speed (TCTS) has mixed signals and receives different opinions. Studies have shown that the change in TC frequency by latitudes, in addition to TC’s steering flow, influences the mean TCTS. Analysis of historical observation data indicated that multi-decadal variability can substantially contribute to slow down the mean TCTS. In this study, TC motion is assessed through the track-cluster analysis of four ensemble projections from the High-Resolution Atmospheric Model during a historical period and late 21st century under RCP 8.5 scenario at 25-km resolution. The two analysis periods share the same year-to-year variability of sea surface temperatures. Changes identified herein are solely attributed to the global warming trend. The impact of varying interannual variabilities under global warming on TC activity is beyond the scope of this study. For TCs in the western North Pacific, this study presents results of six clusters, stratified by TC genesis zones and moving patterns. The analysis better allows exploration of the intra-cluster environmental favorability for TC formation and TC steering flow pattern(s). In a warmer future, most of the projected results (19 of 24 outcomes, composed of the analysis of six clusters and projections under four SST warming patterns) show faster intra-cluster mean TCTS, but only four out of these 19 incidents report a statistically meaningful increase (0.4 – 0.75 m s-1). The analysis suggests a faster TC-moving trend under global warming, however, with limited statistical significance. The meeting presentation will include discussions on relevant physical causes.


AS18-A027
Quantifying the Contribution of Track Changes to Interannual Variations of North Atlantic Intense Hurricanes

Liguang WU#+
Fudan University

Previous studies have linked interannual variability of tropical cyclone (TC) intensity in the North Atlantic basin (NA) to Sahelian rainfall, vertical shear of the environmental flow, and relative sea surface temperature (SST). In this study, the contribution of TC track changes to the interannual variations of intense hurricane activity in the North Atlantic basin is assessed through numerical experiments. It is found that that observed interannual variations of the frequency of intense hurricanes during the period 1958–2017 are dynamically in agreement with changes in the large-scale ocean/atmosphere environment. Track changes can account for ~50% of the interannual variability of intense hurricanes, while there is no significant difference in individual environmental parameters between active and inactive years. The only significant difference between active and inactive years is in the duration of TC intensification in the region east of 60°W. The duration increase is not accounted for by the slow-down of TC translation. In active years, a southeastward shift of the formation location in the region east of 60°W leads TCs to take a westward prevailing track, which allows TCs to have a longer opportunity for intensification. On the other hand, most TCs in inactive years take a recurving track, decreasing the duration of intensification. This study suggests that the influence of track changes should be considered to understand the basin-wide intensity changes in the North Atlantic basin on the interannual time scale.


AS18-A015
Influence of Synoptic-Scale Waves on the Interdecadal Change of Tropical Cyclone Activity Over the Northwestern Pacific in the Early-2010s

Jingliang HUANGFU#+, Yulian TANG, Ronghui HUANG
Chinese Academy of Sciences

This study investigated the interdecadal change of tropical cyclone (TC) activity over the Northwestern Pacific (NWP) in the early-2010s. On the western boundary of the NWP, the interdecadal change of TC activity exhibited a meridional tripole pattern. In contrast to depressed activity over the northern South China Sea (SCS) and Taiwan, TC activity became active over the southern SCS and to the north of Shanghai after the early-2010s. This study focus on the northern NWP, in the recent decade, frequent TC occurrence has brought devastating disasters to East China, Korea and Japan. This work examined the influence of SSWs on the interdecadal change in TC activity. During the 2011–2021 period, SSWs tended to propagate northward, which lead to more TC tracks turning to affect the northern NWP and the surrounding countries. In contrast, the westward-propagating SSWs before the early-2010s were more likely to favor westward moving TCs.


AS18-A002
Three-dimensional Fujiwhara Effect in the Western North Pacific

Kosuke ITO1#+, Soichiro HIRANO2, Jaedeok LEE3, Johnny CHAN4,5
1Kyoto University, 2University of the Ryukyus, 3Kongju National University, 4Asia-Pacific Typhoon Collaborative Research Center, 5City University of Hong Kong

Recent idealized simulations have shown that a system of binary tropical cyclones (TCs) induces vertical wind shear (VWS) in each TC, which can subsequently modify the tracks of these TCs through asymmetric diabatic heating. This study investigates these three-dimensional effects in the western North Pacific using the best track and ERA5 reanalysis data. The TC motion was found to deviate systematically from the steering flow. The direction of deviation is clockwise and repelling with respect to the midpoint of the binary TCs with a separation distance of more than 1000 km. The large-scale upper-level anticyclonic and lower-level cyclonic circulations serve as the VWS for each TC in a manner consistent with the idealized simulations. The VWS of a TC tends to be directed to the rear-left quadrant from the direction of the counterpart TC, where the maxima of rainfall and diabatic heating are observed. The potential vorticity budget analysis shows that the actual TC motion is modulated by the diabatic heating asymmetry that offsets the counterclockwise and approaching motion owing to horizontal advection when the separation distance of the binary TCs is 1000–2000 km. With a small separation distance (<1000 km), horizontal advection becomes significant, but the impact of diabatic heating asymmetry is not negligible. The above-mentioned features are robust, while there are some dependencies on the TC intensities, size, circulation, duration, and geographical location. This research sheds light on the motion of binary TCs from the three-dimensional perspective that has not been previously explained by a two-dimensional barotropic framework.


AS18-A013
Detection of Typhoons with Complex Tracks Using Their Steering Angles

Kyoko TAMURA#+, Tsubasa KOHYAMA
Ochanomizu University

Forecasting typhoon tracks is important from the viewpoint of disaster prevention, because the damage area of a typhoon depends greatly on the typhoon track. Although the accuracy of typhoon track forecast is improving year by year on average, it is often difficult to forecast typhoons with complex track patterns (hereafter “stray typhoons”). It may be possible to improve forecast accuracy for stray typhoons by identifying the conditions that cause their complex movements and understanding their effect on typhoon tracks. However, there is no established quantitative definition of a stray typhoon, making statistical analysis difficult. In this study, we aim to quantitatively define and extract stray typhoons to statistically analyze the environmental conditions required for stray typhoons to exist. To extract stray typhoons, a numerical value called steering angle is introduced. Steering angle represents how much the steering wheel is turned from the perspective of the “driver” of a typhoon. When the typhoon passes through coordinates P(n), P(n+1), and P(n+2) every 6 hours, the steering angle is defined as the angle changed from path P(n) → P(n+1) to path P(n+1) → (n+2). Next, we extract stray typhoons using this steering angle based on observations. We identify 31 stray typhoons, whose absolute value of the steering angle is in the top 1%, the maximum wind speed exceeds 25 m/s, and the velocity of movement exceeds 5 kt. We will also discuss the usage of these indices to determine the large-scale field preferable for the existence of stray typhoons.


AS18-A016
The Slowdown Tends to Be Greater for Stronger Tropical Cyclones

Yuan SUN#+, Wei ZHONG, Yao YAO, Hongrang HE
National University of Defense Technology

Understanding the impact of climate change on tropical cyclones (TCs) has become a hot topic. The slowdown of TC translation speed contributes greatly to the locally accumulated TC damage. While the recent observational evidence shows that TC translation speed has decreased globally by 10% since the mid-twentieth century, the robustness of the trend is questioned by other studies as effects of changes in observational capability can strongly affect the global trend. Moreover, none of the published studies considered dependence of TC slowdown on TC intensity. This is the caveat of these analyses as the effect of TC slowdown is closely related to TC intensity. Here, we investigate the relationship between TC translation speed trend and TC intensity, and reveal possible reasons for the trend. We show that the global slowing trend without weak TC moments (≤ 17 m s-1) is about double of that with weak TC moments in a recent study. This is because the slowing trend is dominated by strong TCs’ trend. Stronger (weaker) TCs tend to be controlled more by upper-level (lower-level) steering flow, and the calculated trend of upper-level steering flow is much larger than that of lower-level steering flow. This may be an important reason for the large difference between the slowing trend without weak TC moments and that with weak TC moments. Furthermore, the changes of TC tracks (including inter-basin trend and latitudinal shift), which are partly attributed to data inhomogeneity, make a much larger contribution to the slowing trend, compared with the weakening of tropical circulation, which is related to anthropogenic warming.


AS18-A044
Multidecadal Variability of Tropical Cyclone Translation Speed Over the Western North Pacific

Yi-Peng GUO#+
Nanjing University

Tropical cyclone (TC) translation speed (TCS) is closely related to TC disasters. Recently, the long-term changes in TCS are extensively studied. To date, however, little is known about the multidecadal variability of TCS over the western North Pacific (WNP). By using multiple observational and reanalysis datasets, this study investigated the multidecadal variability of the WNP TCS and the underlying physical mechanisms. The results show that the mean TCS over the WNP presents robust multidecadal variability during the past seven decades. The multidecadal variability of the basin mean TCS is dominated by the TCS over the extratropics. Further analysis shows that the Atlantic multidecadal oscillation (AMO) is mainly responsible for the WNP TCS multidecadal variability. For the tropical mean TCS, AMO induced steering flow anomalies are responsible for the TCS multidecadal variability. In contrast, for the extratropics, AMO positive (negative) phases lead to favorable (unfavorable) large-scale environmental conditions for maintaining TCs, which results in longer (shorter) action time of the mid-latitude steering flow on TCs and leads to higher (lower) TCS. The shift from negative to positive phases of the TCS anomalies during the recent three decades strongly offsets the long-term slowdown trend of TCS, leading to the inconsistent TCS trends before and after the 1980s. Our results help to complete the physical picture for how TCS responds to internal and external forcings, and also provide new evidence for the recent controversial slowdown of TCS.


Tue-01 Aug | 3:30 - 5:15 | MR327
AS23 - Observations, Remote Sensing, and Modeling of Tropospheric Composition and Air Quality in Asia and the Transpacific Region

Session Chair(s): Huizheng CHE, Chinese Academy of Meteorological Sciences, Jhoon KIM, Yonsei University

AS23-A011 | Invited
Satellite Aerosol Retrieval Algorithm for Multi-angle Polarimetric Measurements Over East Asia

Minghui TAO1#+, Liangfu CHEN2, Yi WANG3, Lan FENG4
1The Aerospace Information Research Institute of the Chinese Academy of Sciences, 2Chinese Academy of Sciences, 3China University of Geosciences, Wuhan, 4China University of Geosciences

The simultaneous retrieval of aerosol optical/microphysical and surface parameters have been a challenging work due to the limited information of satellite observations. The common optimized methods with iterative Radiative Transfer (RT) calculations are usually time-consuming and have to retrieve all the unknowns with different information content. In this study, we developed a flexible aerosol algorithm framework for satellite measurements based on physical-based deep learning (PDL) method. By pre-training of RT simulations, all the unknown aerosol parameters can be retrieved independently by modeling their respective function with the whole satellite observations. Moreover, our method can utilize the abundant priori information such as existing surface and aerosol products, which can also provide an effective constraint for 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 a high efficiency in both computation and information utilization, the PDL algorithm with flexible framework gives a competitive selection for operational aerosol retrieval with various satellite measurements.


AS23-A025
New Global Land Aerosol Fine-mode Fraction Dataset (2001–2020) Retrieved from Modis

Xing YAN1#+, Zhanqing LI2,1
1Beijing Normal University, 2University of Maryland

The aerosol fine-mode fraction (FMF) is valuable for discriminating natural aerosols from anthropogenic ones. However, most current satellite-based FMF products are highly unreliable over land. Here, we developed a new satellite-based global land daily FMF dataset (Phy-DL FMF) by synergizing the advantages of physical and deep learning methods (Figure 1) at a 1° spatial resolution covering the period from 2001 to 2020. It was extensively evaluated against AERONET FMF retrievals, revealing its higher accuracy (RMSE= 0.136) based on 361089 validation samples; 79.15% of the data fell within the ±20%EE envelope) and generally good agreement with AERONET FMF with respect to its values, trends, and frequencies. Phy-DL FMF showed superior performance over alternative deep learning or physical approaches (such as the spectral deconvolution algorithm presented in our previous studies), particularly for forests, grasslands, croplands, and urban and barren land types. By examining Phy-DL FMFs from 2001 to 2020, we found a general decreasing trend around the globe, which was not revealed by AERONET point-scale measurements. However, both Phy-DL and AERONET FMFs showed significant increasing trends in FMF over the western USA and India. The new dataset captured high-level FMFs (> 0.80) over southern China, South Asia, eastern Europe, and the eastern USA. The FMFs were consistently < 0.3 in Northwest China, the Saharan region, and southern South America, indicating coarse-particle desert emissions. The findings of various evaluations, especially the attempted explanations of the spatiotemporal variations and long-term trend changes, suggest that this newly developed dataset is sound, more accurate and thus useful for investigating the impact of fine-mode and coarse-mode aerosols on the atmospheric environment and climate, especially in gaining a deeper insight into fine-mode aerosols. The datasets can be downloaded from https://doi.org/10.5281/zenodo.5105617.


AS23-A052
Optimal Estimation Retrieval of Aerosol Optical Properties from the GEMS Onboard GK-2B Satellite

Yeseul CHO1#+, Sujung GO2, Mijin KIM2, Hyunkee HONG3, Dongwon LEE3, Omar TORRES2
1Yonsei University, 2NASA Goddard Space Flight Center, 3National Institute of Environmental Research

Atmospheric aerosols play a crucial role in the Earth's climate system by affecting radiative forcing, cloud formation, and precipitation patterns. Air quality in Asia is a growing concern due to the region's rapid industrialization and urbanization. Anthropogenic activities such as burning fossil fuels and deforestation can release large amounts of aerosols into the atmosphere, which can have negative impacts on air quality and human health. The Geostationary Environment Monitoring Spectrometer (GEMS), onboard GEO-KOMPSAT-2B (GK-2B) satellite, is the first air quality monitoring sensor in geostationary earth orbit launched in 2020. GEMS measures the hyperspectral radiances with 0.6 nm spectral resolution in ultraviolet and visible ranges over the Asia region during the daytime to provide hourly air quality information. We have updated the aerosol retrieval algorithm based on the optimal estimation method for GEMS. The aerosol retrieval algorithm for GEMS uses 6 channels in ultraviolet and visible wavelengths, which have the advantage of measuring aerosol absorption and height information. We present GEMS aerosol retrieval results for high aerosol loading cases over Asia. The results show that the GEMS AOD has the advantage of allowing retrieving of aerosol over bright surfaces due to dark surface reflectance in UV. The GEMS AOD and SSA are validated against ground-based AERONET. The GEMS ALH is compared to data from the Cloud-Aerosol Lidar with Orthogonal Polarization (CALIOP). The GEMS aerosol product is in good overall agreement with ground measurement and satellite data products. In addition, we conducted an error analysis of GEMS aerosol optical properties. The retrieval can have errors associated with various factors. Sun–earth–satellite geometry, and assumed aerosol model, clouds, and other atmospheric effects. Conducting an error analysis of aerosol optical properties is essential to identify the major contributors to errors and to improve the accuracy of the retrieval algorithms.


AS23-A055
Improved Inversion of Aerosol Components in the Atmospheric Column from Remote Sensing Data

Ying ZHANG#+
Chinese Academy of Sciences

This study develops an improved algorithm for retrieving atmospheric columnar aerosol components from optical remote sensing data. This is achieved by using the complex refractive index (CRI) of a multi-component liquid system in the forward model and minimizing the differences with observations. The aerosol components in this algorithm comprise five species combining eight sub-components including black carbon, water-soluble and water-insoluble organic matter, inorganic salt (ammonium nitrate, AN), sea salt (sodium chloride, SC), dust-like (DU), and aerosol water content in fine and coarse modes (AWf and AWc). The calculation of the complex refractive index (CRI) in the multi-component liquid system allows the separation of the water soluble components (AN, WSOM and AWf) in the fine mode and the sea salt (SC) and water content (AWc) in the coarse mode. The uncertainty in the retrieval results is analysed based on the simulation of typical models, showing that the complex refractive index (CRI) obtained from instantaneous optical-physical inversion compares well with that obtained from chemical estimation. The algorithm is not only used for ground-based remote sensing, but is also transferred to satellite inversion algorithms to obtain larger area-wide observations. Based on the POLDER observations, the study inverted the spatial distribution of aerosol optical, microphysical and chemical parameters in the North China region and made a preliminary comparison with ground-based observations. The comparison shows that the column mass concentration of aerosol black carbon mass concentration is consistent with that observed on the ground, and the MAE is 0.38. The mass ratios of black carbon, inorganic salt and organic aerosol (8%, 49%, 43%) are in good agreement with the mass ratios of the ground chemical sampling analysis results (11%, 49%, 40%).


AS23-A071
Remote Sensing of Carbonaceous Aerosols from Himawari-8 Satellite Using Critical Reflectance Algorithm

Ying LI1,2#+, Fangwen BAO1, Jinhui GAO3
1Southern University of Science and Technology, 2Southern Marine Science and Engineering Guangdong Laboratory, 3Chengdu University of Information Technology

Current aerosol remote sensing without using multi-view satellite sensors still fails to retrieve aerosol components directly, such as black carbon (BC) and organic carbon (OC) simultaneously due to the limitations on available observations. In this study, A new general carbonaceous aerosol retrieval strategy for geostationary single-view satellite observations is implemented based on a method of critical reflectance, to retrieve the parameters of BC and extra OC concentration from measured radiance without prior quantification of Aerosol Optical Thickness (AOT). Random sampling consensus (RANSAC) is also used in the strategy to reduce the influence of clouds and anomalous pixels on the retrievals. An initial validation and application applied to Himawari images over the North China Plain (NCP) show that the carbonaceous aerosol retrievals are highly consistent with the expectations in terms of spatial and temporal patterns. The retrievals of BC and OC concentration follow the daily fluctuations of the Aethalometers observations and feature small differences in mean values throughout the month. Additionally, the AOTs at 0.55 µm can be also satisfactorily reproduced based on the carbonaceous aerosol retrievals, resulting in a mean absolute error of 0.089 and a correlation coefficient of 0.870. The main errors in the method arise from shell model assumptions, RANSAC fitting bias, inconsistent clear reference AOT in LUT, and geometric inconsistency between the clear reference and hazy images. This work indicates that the BC and OC concentration in high resolution can be acquired through the geostationary single-view remote sensing for further air quality and climate studies.


AS23-A002
AOD Fusion Based on Pixel-level Uncertainty Using Geostationary Satellite Instruments: GEMS, AMI, and GOCI-II

Minseok KIM1#+, Jhoon KIM1, Hyunkwang LIM2, Seoyoung LEE1, Yeseul CHO1
1Yonsei University, 2National Institute for Environmental Studies

For the last few years, South Korea has launched two geostationary earth orbit satellites, Geo-Kompsat-2A (GK-2A) and Geo-Kompsat-2B (GK-2B). GK-2A carries a single sensor named Advanced Meteorological Imager (AMI), which has spectral bands from visible to infrared for observations of weather variables such as clouds. GK-2B carries two sensors. One of them is an ultraviolet-visible hyperspectral spectrometer named Geostationary Environment Monitoring Spectrometer (GEMS), and the other is a band (visible-shortwave infrared) observing ocean color imager named the 2nd Geostationary Ocean Color Imager (GOCI-II). In the aspect of aerosol optical properties products, each geostationary instrument has its own instrument specification. The visible radiance capability of AMI and GOCI-II is sensitive to the size of the airborne aerosols, while ultraviolet observation by GEMS is sensitive to the light-absorption of aerosols. Moreover, a dark surface in the ultraviolet spectrum enables aerosol retrievals over arid regions. In this study, we present a statistically fused product of three aerosol optical depth (AOD) from AMI, GEMS, and GOCI-II that are retrieved by individually optimized algorithms. Because of the algorithm characteristics such as surface reflectance estimation and observation geometry, each AOD product has its own systematic retrieval bias according to surface vegetation and observation time. Therefore, we proceed with a bias correction based on comparison with Aerosol Robotic Network (AERONET) measurements before the AOD fusion. Statistical fusion uses Maximum Likelihood Estimation (MLE) method for the sake of weighting based on retrieval errors evaluated with AERONET measurements. We analyzed satellite and AERONET data of 2021 to calculate bias and retrieval error. AOD fusion algorithm was applied to the individual AOD products in 2022, and validation result showed that individual error characteristics were much improved by statistical aerosol fusion.


AS23-A012
Hypothetical RGB Bands Generation of Geostationary Environment Monitoring Spectrometer Using Data-to-data Translation

Han-Sol RYU1+, Jeong-Eun PARK1, Jaehoon JEONG2, Goo KIM2, Sungwook HONG1#
1Sejong University, 2National Institute of Environmental Research

Recently, air pollution has been worsening globally and, in particular, more severe in Asia. South Korea launched and has been operating the first geostationary environmental satellite, Geostationary Korea Multi-Purpose Satellite (GK)-2B, to monitor the atmospheric environment since February 2020. The Geostationary Environment Monitoring Spectrometer (GEMS) onboard the GK-2B has spectral bands within 300~500nm from ultraviolet (UV) to visible (VIS) wavelength ranges specialized in observing micropollutants in the atmosphere. Like human eyes, the three red-green-blue (RGB) bands are helpful for monitoring and intuitively understanding the atmospheric environment, including the movement, diffusion, and extinction of clouds and aerosols. However, the GEMS cannot provide RGB true-color images because the GEMS has hyperspectral bands within only the blue band range. Notably, the central wavelength of the Advanced Meteorological Imager (AMI) blue band corresponds to the GEMS blue band. Thus, this study presents a deep-learning-based method to simulate virtual radiances at the virtual GEMS RGB bands similar to the neighboring AMI sensor with the real RGB bands onboard the GK-2A satellite. We adopted the data-to-data translation method using the AMI three RGB bands as training and test datasets. This study used AMI data from 2020 to 2021 for model development and validation. The GEMS data during 2021 were used for model application as input data. As a result, the proposed model showed excellent results with a high correlation coefficient of over 0.95 in all AMI RGB bands, in addition to qualitative agreements between the observed AMI RGB and model-generated GEMS RGB data. This study can significantly contribute forecasters to monitoring and intuitively understanding the atmospheric environment in Asia.


Tue-01 Aug | 3:30 - 5:15 | MR328
AS24 - Machine Learning applications in the field of atmospheric pollution

Session Chair(s): Siwei LI, Wuhan University, Jie YANG, Wuhan University

AS24-A017
Global Hourly and Daily PM2.5 Estimations: A Data Fusion Approach

Pawan GUPTA1#+, Alqamah SAYEED2, Robert LEVY1, Sundar CHRISTOPHER3
1NASA Goddard Space Flight Center, 2Universities Space Research Association, 3The University of Alabama in Huntsville

Air quality has become a pressing public health issue globally due to increased urbanization and industrialization over the past several decades. One of the major contributors to poor air quality in urban areas is particulate matter (PM or aerosols). PM2.5, with an aerodynamic diameter of less than 2.5 μm, can cause respiratory and lung diseases and even premature death. It also plays a crucial role in atmospheric processes and is linked to climate change. Environmental agencies monitor and regulate particulate emissions by measuring PM2.5 concentrations on a hourly and daily basis. However, limited ground monitors are available, and recent advancements in satellite remote sensing and global numerical models offer the possibility of filling in measurement gaps. In this study, we plan to implement machine learning (ML) and deep learning (DL) methods to estimate surface PM2.5 at hourly and daily scales globally. We will combine data from ground networks, satellite platforms, and model outputs to develop an ML/DL algorithm that produces high-quality records over 22-years. Our initial analysis used one year of data and employed random forest and deep neural network algorithms. The results showed a mean bias close to zero, with a slope of 1.02 and an RMSE of 6.4 μgm-3 globally. This study will present an analysis based on three years of data, and we will also test more advanced ML/DL algorithms (including CNN) to determine the best way to estimate PM2.5 at hourly and daily scales.


AS24-A008
Promoting the Estimation of Surface Ozone Concentration by Combining Machine Learning and Photochemistry

Ge SONG+, Siwei LI#
Wuhan University

In recent years, surface ozone has observed an ascending trend in China despite of tremendous effort in reduction of emission, thus monitoring the surface ozone concentration with high accuracy and wide coverage is highly demanded. Previous studies have indicated that satellite observations can be used to retrieval the surface ozone estimation. However, the accuracy of the model estimations have not met the requirement to evaluate the spatial and temporal variations. This study proposes a machine-learning based model combining photochemical mechanisms of surface ozone aiming to better depict the patterns of surface ozone concentrations. Particularly, the incorporation of photochemical features including surface ultraviolet irradiance and nitrogen dioxide, which are among the feasible indicators and precursors of surface ozone formation, significantly enhances the model accuracy of surface ozone estimation. The proposed model achieves high accuracy (R2=0.853 and RMSE =17.09 μg/m3) with spatial continuity. Moreover, the model have overcome the critical challenges of the current model applications by promoting the effect of surface ozone estimation in regions with sparse distribution of surface monitoring sites.


AS24-A018 | Invited
Development of a Multi-scale Modeling Framework for Urban High-resolution NO2 Pollution Mapping

Huan LIU#+
Tsinghua University

Vehicle emissions have become a major source of air pollution in urban areas, especially for near-road environments, where the pollution characteristics are difficult to capture by a single-scale air quality model due to the complex composition of the underlying surface. This study promoted the capability of the emissions calculation and the air quality simulation to fine scales such as urban areas and street canyons. We developed a multi-scale coupling model (CMAQ-RLINE_URBAN) based on a street canyon flow scheme using Computational Fluid Dynamic and two machine learning methods. To estimate the influence of various street canyons on the dispersion of air pollutants, a machine-learning-based street canyon flow (MLSCF) scheme was established. It enables quantitative analysis on the effects of vehicle emissions on urban roadside NO2 concentrations at a high spatial resolution of 50m_50 m. The results indicated that compared with the Community Multiscale Air Quality (CMAQ) model, the hybrid model improved the underestimation of NO2 concentration at near-road sites with the mean bias (MB) changing from -10 to 6.3 μgm􀀀3. The MLSCF scheme obviously increased upwind concentrations within deep street canyons due to changes in the wind environment caused by the vortex. In summer, the relative contribution of vehicles to NO2 concentrations in Beijing urban areas was 39% on average, similar to results from the CMAQ-ISAM (Integrated Source Apportionment Method) model, but it increased significantly with the decreased distance to the road centerline, especially on urban freeways, where it reached 75%.


AS24-A013
How Important the Wetlands are in Curbing the PM2.5 Level; Simulation Results from Indian Cities

Prasenjit ACHARYA1#+, Bijoy Krishna GAYEN1, Dipanwita DUTTA1, S. SREEKESH2, U.C. KULSHRESTHA2, Nachiketa ACHARYA3,4
1Vidyasagar University, 2Jawaharlal Nehru University, 3University of Colorado Boulder, 4NOAA Physical Sciences Laboratory

The moisture in the air is vital for reducing the PM2.5 concentration. We performed simulations using the random forest regression model to account for the effect of wetlands in lowering the PM2.5 level over some of the selected Indian cities in the north Indian plain which are known to be some of the most highly polluted cities in the world. The meteorological factors, such as 2 m air temperature, surface pressure, AOD, relative humidity, wind speed, boundary layer height, vertical airflow, and precipitation, in combination with surface greenness feature, i.e., NDVI, and proximity to wetlands were considered as potential covariates to model the PM2.5. The simulations, at an annual scale, suggest wetland proximity is more important than precipitation, surface pressure and wind speed, and even relative humidity. However, we found variability of the influence of wetland’s proximity at the seasonal scale, with the highest influence noted in the pre-monsoon season when thermal conditions are high as well as in the winter season when vapor pressure remains lower. We also found that above a PM level of 300 µg m-3, the explanation of the regression model reduces to 57% (R2 = 0.57), including an RMSE and MAE of 42.83 µg m-3 and 29.45 µg m-3, respectively. However, below 300 µg m-3, the explanation increases to more than 60% (R2 = 0.61), with an RMSE and MAE of 34.96 µg m-3 and 25.84 µg m-3. The modeling suggested a differential rate of increment around the wetlands. It follows a limited area influence (~ 3 km) within which the PM2.5 remains low. The findings, indeed, suggest that restoration of wetlands within and surrounding the cities could be one of the effective nature-based solutions to curb the PM2.5 level while putting other pollution regulatory measures in place.


AS24-A003
Elucidate the Impacts of Meteorology and Emission Changes on Concentrations of Major Air Pollutants in Major Cities in the Yangtze River Delta Region Using a Machine Learning De-weather Method

Wenxing FU+, Jianlin HU#
Nanjing University of Information Science & Technology

Since the implementation of various air pollution control policies, the concentrations of major air pollutants in the Yangtze River Delta (YRD) region have changed significantly, but the contributions of emissions and meteorological factors are unclear. Therefore, it is essential to decouple the effects of meteorology and emissions changes to air quality. This study applied a de-weather method based on machine learning technique to quantify the contribution of meteorology and emission changes to air quality from 2015 to 2021 in four cities in the YRD region. The results show that the significant reductions in PM2.5, NO2, and SO2 emissions (57.2%-68.2%,80.7%-94.6%,81.6%-96.1%) offset the adverse effects of meteorological conditions, resulting in lower pollutant concentrations. The meteorological contribution of maximum daily 8-h average O3 (MDA8_O3) shows a stronger effect than others (23.5%-42.1%) , and meteorological factors promote the increase of MDA8_O3 concentrations (4.7%) but emission changes overall result a decrease of MDA8_O3 concentrations (−3.2%) in the four cities on average. NO2 and MDA8_O3 decreases more rapidly from 2019 to 2021, mainly because the emissions play a stronger role to reduce pollutant concentrations than 2015 to 2018. However, emissions changes have weaker reduction effects on PM2.5 and SO2 from 2019 to 2021 than 2015 to 2018. De-weather methods can effectively separate the effects of meteorology and emissions changes on pollutant trends, which helps to evaluate the real effects of emission control policies on pollutant concentrations.


Tue-01 Aug | 3:30 - 5:15 | MR329
AS11 - Atmospheric Chemistry in Highly Polluted Environments: Emissions, Fate, and Impacts

Session Chair(s): Sri KOTA, Indian Institute of Technology Delhi

AS11-A023 | Invited
Optimization of Protocol for Detection of Dicarboxylic Acids (DCAs) in Ambient Aerosol and its Analysis in Northeast Region of India Using GC-MS

Pratibha VISHWAKARMA+, Poonam NIGAM, Tarun GUPTA#
Indian Institute of Technology Kanpur

Increasing levels of hygroscopic aerosols are one of the major reasons behind irregular rainfall and changed radiative forcing which plays a significant role in climate change. Dicarboxylic acids, which are known for their deliquescence and hygroscopic nature, can act as cloud condensation nuclei (CCN) and ice nuclei (IN), due to which rainfall patterns can be disturbed. Also, the importance of DCAs analysis can be linked to its ability to act as potential organic molecular markers for various anthropogenic and biogenic sources. Despite its significance, very few studies deal with the optimization of the protocol for qualitative and quantitative analysis of DCAs using Gas Chromatography-Mass Spectrometry (GC-MS). In the present study, we have optimized the extraction of DCAs from aerosol samples collected on a quartz filter, by employing several organic solvents with differing relative polarities. Extraction efficiencies of organic solvents were evaluated at different temperatures and pressures using an advanced energized dispersive extractor (EDGE, CEM Corporation, USA). The high polarity and low levels of dicarboxylic acids demand a derivatization step prior to GC analysis to reduce the polarity of the compounds. BSTFA (N, O-bis-(trimethylsilyl)trifluoroacetamide) + TMCS (trimethylchlorosilane) was chosen as the derivatizing reagent, and reaction conditions (temperature, amount of BSTFA, conc. of TMCS) were optimized to give maximum conversions. Separation of compounds was done on HP-5 column with Helium as the carrier gas. Protocol was finalized by selecting the operating parameters of GC-MS in selected Ion monitoring (SIM) mode that reduces the total run time while maintaining a good resolution of peaks. Aerosol samples from northeast region of India have been analyzed using proposed method and DCAs were detected. The average concentration of total DCAs was found 103.75 ng/m3 in the northeast region of India where Pimelic and Suberic acids were found dominant among all the DCAs.


AS11-A055
Production and Loss of Atmospheric Formaldehyde at a Suburban Site of Shanghai in Summertime

Yizhen WU1, Juntao HUO2, Gan YANG1, Yuwei WANG1, Lihong WANG1, Shijian WU2, Lei YAO1, Qingyan FU2, Lin WANG1#+
1Fudan University, 2Shanghai Environmental Monitoring Center

Formaldehyde (HCHO) is an important trace gas that affects the abundance of HO2 radicals and ozone, leads to complex photochemical processes, and yields a variety of secondary atmospheric pollutants. In a 2021 summer campaign at the Dianshan Lake (DSL) Air Quality Monitoring Supersite in a suburban area of Shanghai, China, we measured atmospheric HCHO by a commercial Aero-Laser formaldehyde monitor, methane, and a range of non-methane hydrocarbons (NMHCs). Ambient HCHO showed a significant diurnal cycle with an average concentration of 2.2 ppbv. During the time period with the most intensive photochemistry (10:00-16:00 LT), secondary production of HCHO was estimated to account for approximately 69.6% according to a multi-linear regression method based on ambient measurements on HCHO, acetylene (C2H2), and ozone (O3). Average secondary HCHO production rate was estimated to be 0.73 ppbv h-1 during the whole campaign, with a dominant contribution from reactions between alkenes and OH radicals (66.3%), followed by OH radical-initiated reactions with alkanes and aromatics (together 19.0%), OH radical-initiated reactions with OVOCs (8.7%), and ozonolysis of alkenes (6.0%). An overall HCHO loss, including HCHO photolysis, reactions with OH radicals, and dry deposition, was estimated to be 0.49 ppbv h-1. Calculated net HCHO production rates were in relatively good agreements with the observed rates of HCHO concentration change throughout the sunny days, indicating that HCHO was approximately produced by oxidation of the 24 hydrocarbons we considered at the DSL site during the campaign, whereas calculated net HCHO production rates prevailed over the observed rates of HCHO concentration change in the morning/midday hours in the cloudy and rainy days, indicating a missing loss term, most likely due to HCHO wet deposition. Our results suggest the important role of secondary pollution at the suburb of Shanghai, where alkenes are likely key precursors for HCHO.


AS11-A056
The Impacts of Marine-emitted Halogens on Atmospheric Oxidation in Guangdong-Hongkong-Macau Great Bay Area (GBA) of China During Summer

Ying LI1,2#+, Shidong FAN1
1Southern University of Science and Technology, 2Southern Marine Science and Engineering Guangdong Laboratory

A better understanding of marine halogen emission on atmospheric oxidation is crucial for air chemistry and environment of GBA. The OH radical and O3 are the two key species to indicate the atmospheric oxidation in atmospheric chemistry. In the marine atmosphere, OH levels could be significantly affected by the halogen species emitted from the ocean. However, due to the complicated interactions of halogens with OH through different pathways, it is not well understood how halogens influence OH and even what the sign of the net effect is. In addition, whether oceanic emissions can affect the O3 level notably has not been fully understood. Therefore, in this study, we aim to quantify the impact of marine-emitted halogens (including Cl, Br, and I) through different pathways on OH and Ozone in the summer by using WRF-CMAQ model with process analysis and state-of-the-art halogen chemistry in GBA. Results show that the net change of POH is controlled by the competitions of three main pathways (OH from O3 photolysis, OH from HO2 conversion, and OH from HOX, X=Cl, Br, I) through different halogen species. Sea spray aerosols (SSA) and inorganic iodine gases are the major species to influence the strengths of these three pathways and therefore have the most significant impacts on POH. In terms of O3, we found an unexpected hourly and MDA8 O3 increase on polluted days, because the activation of particulate chloride (Cl) in sea salt aerosol (SSA) is effective due to the high level of dinitrogen pentoxide (N2O5) that is formed from the reactions of O3 and nitrogen dioxide (NO2). Our results show that marine-emitted halogen species have notable impacts over the ocean and potential impact on coastal atmospheric oxidation by species (SSA, inorganic iodine, and halocarbons), processes (chemistry, radiation, and deposition) and main pathways.


AS11-A058
Nocturnal Nitrogen Chemistry is Gaining Increasing Importance in Haze Formation

Chao YAN1#+, Yee Jun THAM2, Wei NIE1
1Nanjing University, 2Sun Yat-sen University

The largest fraction of PM2.5 in China during severe haze is composed of nitrate, which has led to strict control of nitrogen oxide (NOx) emissions believed to be an effective measure to combat air pollution. However, this notion was challenged by the persistent severe haze pollution observed during the COVID-19 lockdown, when NOx levels decreased significantly. This study provides direct field evidence that reduced nitrogen oxides (NO) during the shutdown activated nighttime nitrogen chemistry, driving severe haze formation. Dinitrogen pentoxide (N2O5) heterogeneous reactions dominate particulate nitrate (pNO3-) formation during severe pollution, explaining the higher-than-normal pNO3- fraction in PM2.5 despite substantial NOx reductions. Nocturnal nitrogen chemistry during the lockdown period was completely different from normal conditions in Beijing, but it may vividly depict future scenarios if NOx emissions are strictly controlled without simultaneous control of O3. Therefore, our results suggest that nocturnal nitrogen chemistry is becoming increasingly important in urban and suburban areas worldwide. More attention needs to be paid to the complex influence of NO, NO2, VOC, and O3 on nighttime chemistry when formulating future emission control strategies.


AS11-A063
Photo-oxidation Pathway as a Potential CS2 Sink in the Atmosphere

Yuanzhe LI1#+, Kazuki KAMEZAKI2, Sebastian DANIELACHE1
1Sophia University, 2National Institute of Advanced Industrial Science and Technology

CS2 is the main precursor of COS in the atmosphere, with about 30-75% coming from CS2 oxidation. The highly regional distribution and fast vertical concentration attenuation characteristics indicate CS2 has strong surface removal pathways. Current understanding suggests CS2 converts to COS through OH oxidation while the photochemistry pathway is neglected in previous model studies. Nevertheless, the CS2 photo-excitation reaction, which is the initial reaction of the photo-oxidation pathway, has sufficient absorption cross-section in the band range 280-380 nm, implying that the photo-oxidation pathway may also play an active role even at the surface. In this study, we constructed a 1D model of the revised CS2 reaction network with the addition of the photo-oxidation pathway and extended it to a sulfur cycle. The daytime-weighted zenith angle and solar constant are applied to counteract the spatial-temporal variation and simulate the global average solar radiation. All sulfides concentration in the model reproduced the field measurements or other model estimations. The sulfur budget of the sulfur cycle is determined and the addition of the new pathway has a relatively minor change (1.5%) on the product ratio between COS and SO2. However, the flux analysis reveals the photo-oxidation pathway and the OH-oxidation pathway contain near-magnitude sulfur fluxes in the CS2 reaction network and that 15.8% of sulfur flux passes through the photo-oxidation pathway under global average solar irradiance condition. This proportion ranges from 8.1% to 18% depending on the local solar radiation intensity, demonstrating that the photo-oxidation pathway could be a sink for CS2 in the atmosphere.


AS11-A064
Evaluation of Key Factors Influencing Urban Ozone Pollution in the Pearl River Delta and its Atmospheric Implications

Xiaoyu LIN1#+, Ling-Yan HE2, Shiyong XIA2, Yao LUO2, Hengxiao HAN2
1Peking University, 2Peking University Shenzhen Graduate School

In recent years, the concentration of ozone (O3) in typical urban agglomerations in China has generally increased. This study carries out a three-year observation in the active photochemical reaction period (August-November) in Shenzhen, a megacity in the Pearl River Delta (PRD). Our study selects the photolysis reaction rate constant of NO2 (j[NO2]) and O3 (j[O1D]) as representative factor of photolysis rate. Principal coordinate analysis (PCoA) is first applied to identify the major factors influencing daily maximum 8-h average O3 (MDA8-O3) concentration. Then, the MDA8-O3 concentration fitting equation is established by a stepwise multiple linear regression (MLR). In result, sensitivity test based on the fitting equation shows that temperature (+35.8%), photolysis rate of j[NO2] (+11.1%), relative humidity (-10.4%) and photolysis rate of j[O1D] (-9.5%) have more effect on the concentration of MDA8-O3 with per factor perturbation (25% change), while increments of △CO (6.9%) and NO2 (2.7%) have less effect. The insignificant effect produced by NO2 suggests that Shenzhen is in a transition regime for the O3-VOC-NOx sensitivity and thus the reduction of both VOC and NOx will be effective for O3 control. In addition, it is found that PM2.5 promoted O3 formation by scattering light with wavelength dependence to increase △P (5.87×103j[NO2]-2.17×106j[O1D], indicating the net effect on flux of actinic radiation), which provides a new explanation for the synergistic formation of PM2.5 and O3 usually observed in the PRD region. Finally, the method establishes here is based on parameters easily available (e.g., without VOC) and can be widely applied in other regions. The results of this study will help better understand the current ozone formation mechanisms in Shenzhen and promote forecasting ozone pollution more accurately in PRD and similar regions.


AS11-A061 | Invited
Preparation of Gridded Emission Inventory for Particulate Matter Using Ground-based Activity Data and its comparison with the Other Emission Inventories: A Study of Seven Non-attainment Cities of an Urban Airshed, Punjab India

Arpit KATIYAR#+
Indian Institute of Technology Delhi

The first step towards reducing the particulate matter (PM) load is its quantification scientifically, thereby highlighting the importance of source apportionment. Of the various ways, the emission inventory developed using the ground-based activity data is highly accurate. Developing such emission inventories is challenging because it takes a lot of resources and time. In this study, we focus on developing a gridded emission inventory for PM10 and PM2.5 at 300m × 300m resolution using ground-based activity data for the seven non-attainment cities (Jalandhar, Patiala, Mandi Gobindgarh, Khanna, Naya Nangal, Dera Bassi, and Dera Baba Nanak) of Punjab, a state in India. Further, a comparison with other databases (two global and one regional) EDGARv5, ECLIPSEv6b, and SMoGv1 emission inventories has been performed to highlight the inconsistencies or gaps that have not been accounted for in the other databases. It is observed that out of the seven cities, Jalandhar was the highest contributor to the total PM10 and PM2.5 emissions which is estimated to be 9307 and 4296 tons/year respectively whereas Dera Baba Nanak was the least contributor with total PM10 and PM2.5 emissions of 136 and 92 tons/year respectively. The primary contributing sources are mainly vehicular, road dust, and industrial emissions for all the cities. The inferences of the study will help the policy-makers to make better-informed decisions on reducing emissions and protecting public health.


AS11-A002
Spatiotemporal Variation and Inter-transport of Atmospheric Speciated Mercury Between Harbor and Urban Areas: A Case Study of Kaohsiung, Taiwan

I-Chieh TU#+, Chung-Shin YUAN
National Sun Yat-sen University

This study investigated the inte-transport of atmospheric speciated mercury (ASM) between harbor and urban areas in Kaohsiung, Taiwan. Gaseous elemental mercury (GEM), gaseous oxidized mercury (GOM), and particle-bound mercury (PBM) were sampled at four selected sites in harbor and urban areas in four seasons. The spatiotemporal variation, transport routs, and potential sources of ASM were further resolved. Field measurement results indicated that the seasonal average concentration of ASM was ordered as: winter>fall>spring>summer. The concentrations of GEM in harbor and urban areas were 7.36±2.14 and 6.07±1.70 ng/m3, those of GOM in harbor and urban areas were 360±258 and 286±198 pg/m3; and those of PBM in harbor and urban areas were 584±386 and 448±275 pg/m3, respectively. In addition, gas-solid partition of ASM indicated that GEM was the main species at four sites and GOM accounted for only 2.6-6.0% of total atmospheric mercury (TAM). We found that the urban area of Kaohsiung was frequently affected by mercury species emitted from the harbor area. Backward trajectories and wind roses showed that polluted air mainly came from the north in winter. Poor atmospheric dispersion conditions led to the accumulation of local and oversea pollutants and the increase of ASM concentrations. In spring, polluted air transported mainly from the northwest. It was presumed that they were attributed from ocean evaporation and ship exhausts. In summer, clean air transported mainly from industrial complex in the southeast.


Tue-01 Aug | 3:30 - 5:15 | MR331
AS01 - The Asian Monsoon, Extremes and Climate Change

Session Chair(s): Shoichiro KIDO, Japan Agency for Marine-Earth Science and Technology, Lakshmi Kumar T.V., SRM Institute of Science and Technology, Yina DIAO, Ocean University of China

AS01-A061
Indian Ocean Dipole and Enso’s Mechanistic Importance in Modulating the Ensuing-summer Precipitation Over Eastern China

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.


AS01-A062
Limited Signatures of ENSO on Future Precipitation Over Asia

Thanh LE#+
Sejong University

There is uncertainty in the future connection between ENSO and regional precipitation. Here we assessed the causal effects of ENSO on precipitation over Asia in the 2015-2100 period, using data from Coupled Modeling Intercomparison Project Phase 6 (CMIP6) models. Our results show that ENSO impacts on precipitation are mainly observed over parts of Southeast Asia and parts of central and western Asia, while these impacts are not significant over East Asia and South Asia.


AS01-A068
Different Influences of Southeastern Indian Ocean and Western Indian Ocean SST Anomalies on Eastern China Rainfall During the Decaying Summer of 2015/16 Extreme El Niño

Jiepeng CHEN1#+, Jin-Yi YU2, Xin WANG1, Tao LIAN3
1Chinese Academy of Sciences, 2University of California, Irvine, 3Second Institute of Oceanography

Previous studies linked the increase of middle and low reaches of Yangtze River (MLRYR) rainfall to tropical Indian Ocean warming during extreme El Niño’s (e.g. 1982/83 and 1997/98 extreme El Niños) decaying summer. The present study finds the linkage to be different for the recent 2015/16 extreme El Niño’s decaying summer, during which the above-normal rainfall over MLRYR and northern China are respectively linked to southeastern Indian Ocean warming and western tropical Indian Ocean cooling in sea surface temperatures (SSTs). The southeastern Indian Ocean warming helps to maintain the El Niño-induced anomalous lower-level anticyclone over western north Pacific and southern China, which enhances moisture transport to increase rainfall over MLRYR. The western tropical Indian Ocean cooling first enhances the rainfall over the central-northern India through a regional atmospheric circulation, whose latent heating further excites a mid-latitude Asian teleconnection pattern (part of circumglobal teleconnection) that results in an above-normal rainfall over the northern China. The western tropical Indian Ocean cooling during the 2015/16 extreme El Niño is contributed by the increased upward latent heat flux (LHF) anomalies associated with enhanced surface wind speeds, opposite to the earlier two extreme El Niños.


AS01-A083
Quantifying Characteristics of Intraseasonal Summer Rainfall in Thailand and Associated Moisture Transport During Active MJO and ENSO Warm Phase

Pattarapoom PEANGTA+, Kritanai TORSRI#, Apiwat FAIKRUA, Rati SAWANGWATTANAPHAIBUN , Thippawan THODSAN, Kanoksri SARINNAPAKORN
Ministry of Higher Education, Science, Research and Innovation

Previous studies revealed that intraseasonal global climate variation is exerted by Madden-Julian Oscillation (MJO); meanwhile its year-to-year variability is strongly controlled by El Niño-Southern Oscillation (ENSO). In Thailand, previous studies indicated that rainfall deficit in summer season is interannually significantly linked to variation of ENSO warm phase (aka, El Niño). However, a compound effect between the MJO and the El Niño on the regional rainfall has not yet been understood. In this study, we, therefore, aimed at quantifying aspects of 20-60-day summer rainfall variation in Thailand in association with active MJO and El Niño. Daily rainfall data covering 1979-2019 were collected from the Thai Meteorological Department, whereas MJO (Oceanic Niño Index; ONI) was provided by the Bureau of Meteorology (National Centers for Environmental Prediction). Additionally, ERA-5 reanalysis is used for considering large-scale moisture transport. The result shows that the combined effect between MJO and the warm episode on Thailand’s rainfall is spatially varying depending on different MJO phases by which the 20-60-day rainfall anomalies in upper Thailand are above (below) normal at MJO phases 3-4 (6-7). For southern Thailand, above normal rainfall is also profound at MJO phase 3-4, while below normal rainfall lasts slightly longer than in the upper sub-region (phases 5-7). The intraseasonal variation of rainfall in the upper Thailand is strongly associated with moisture transport from Bay of Bengal, Gulf of Thailand, and South China Sea, while moisture coming from easterly, and westerly is a major control of the rainfall anomalies in the South. Hence, this study provides a fundamental understanding and characteristics of the combined effect between the climate drivers on intraseasonal rainfall variation and is useful for further development of sub-seasonal to seasonal (S2S) prediction in Thailand.


AS01-A040
Interdecadal Variations of the Scandinavian Pattern

Bo PANG1#+, Adam SCAIFE2,3, Riyu LU1, Rongcai REN1, Xiaoxuan ZHAO1
1Chinese Academy of Sciences, 2Met Office, 3University of Exeter

This study investigates the interdecadal variation of the Scandinavian (SCA) pattern and corresponding drivers during the boreal winter. It is found that the SCA pattern experiences a prominent regime shift from its negative to positive phase in the early 2000s based on several reanalyses. This interdecadal change contributes to an extensive cooling over Siberia after the early 2000s, revealing its importance for recent variation of climate over Eurasia. The outputs from 35 couple models within the Coupled Model Intercomparison Projection Phase 6 (CMIP6) are also analyzed. The results show that the interdecadal change of SCA is weak in response to external forcings but can be largely explained by internal variability associated with a change of precipitation over the tropical Atlantic. Further analysis indicates that the enhanced tropical convection induces poleward propagation of Rossby waves and further results in an intensification of geopotential height over the Scandinavian Peninsula during the transition to positive SCA phases. These findings imply a contribution of tropical forcing to the observed interdecadal strengthening of SCA around the early 2000s and offer an insight into the understanding of future climate change over the Eurasian continent.


AS01-A095
Interdecadal Variation in Available Potential Energy of Stationary Eddies in the Midlatitude Northern Hemisphere in Response to the North Pacific Gyre Oscillation

Marco Yu Ting LEUNG1#+, Dongxiao WANG1, Wen ZHOU2
1Sun Yat-sen University, 2Fudan University

This study investigates the variation in available potential energy of stationary eddies in the mid-troposphere over the midlatitude Northern Hemisphere (30˚ to 60˚N) from 1950 to 2021, based on the ERA5 reanalysis and its preliminary back extension. The variation is attributed mainly to change in the wavenumber-1 eddy. It is also noted that potential energy conversion from the zonal mean flow in early winter plays an important role in the 20-year variation. In addition, statistical analysis and numerical simulation of an ICTP model demonstrate that the potential energy conversion is controlled by the North Pacific Gyre Oscillation (NPGO), which induces anomalous meridional temperature advection in the mid-troposphere over Northeast Asia.


AS01-A113
Can Tibetan Plateau Snow Depth Influence the Interannual Association Between Tropical Indian Ocean Sea Surface Temperatures and Rapidly Intensifying Typhoons?

Haikun ZHAO#+
Nanjing University of Information Science & Technology

This study finds that the observed decrease in winter-spring Tibetan Plateau snow depth since 2000 has played an important role in weakening the correlation between rapidly-intensifying tropical cyclones over the western North Pacific and tropical Indian Ocean sea surface temperatures (SSTs). Tibetan Plateau snow depth modulates convective activity through changes in the South Asian High. Increased Tibetan Plateau snow depth promotes basin-wide tropical Indian Ocean cooling in spring through a Gill-type response. In the following seasons, downward latent heat flux anomalies associated with a weaker monsoon circulation contributes to warm SST anomalies over the western tropical Indian Ocean, thus favoring a positive phase of the Indian Ocean Dipole. This evolution of tropical Indian Ocean SST associated with anomalously high Tibetan Plateau snow depth potentially weakens the relationship between rapidly-intensifying tropical cyclone frequency and spring tropical Indian Ocean SST. When the effect of Tibetan Plateau snow depth is removed via partial correlation analysis, we find a significant relationship between spring tropical Indian Ocean SST and rapidly-intensifying tropical cyclones as well as corresponding large-scale environmental factors. The results of this study enhance understanding of changes in tropical cyclone intensity and have implications for seasonal forecasting of tropical cyclone intensity over the western North Pacific basin. This study also emphasizes the importance of Tibetan Plateau thermal forcing in atmosphere-ocean coupling.


Tue-01 Aug | 3:30 - 5:15 | MR332
AS45 - Interaction of Atmospheric Composition and the Asian Monsoon

Session Chair(s): Mian CHIN, NASA GSFC, Liya YU, National University of Singapore

AS45-A018
The GOSAT-GW Satellite Mission: Potential Roles in the Asia-Oceania Region

Hiroshi TANIMOTO1#+, Tsuneo MATSUNAGA1, Takafumi SUGITA1, Hisashi YASHIRO1, Isamu MORINO1, Makoto SAITO1, Hirofumi OHYAMA1, Satoshi INOMATA1, Kohei IKEDA1, Yu SOMEYA1, Tamaki FUJINAWA1, Yukio YOSHIDA1, Yosuke YAMASHITA1, Astrid MUELLER1, Matthias FREY1, Hyunkwang LIM1, Hao XU1, Tazu SAEKI1, Nobuko SAIGUSA1, Yugo KANAYA2, Takashi SEKIYA2, Prabir K. PATRA2,3, Masayuki TAKIGAWA2, Masahiro YAMAGUCHI2, Jagat S. H. BISHT2, Yasuko KASAI4, Tomohiro SATO5, Ayano NAKAMURA5
1National Institute for Environmental Studies, 2Japan Agency for Marine-Earth Science and Technology, 3Tohoku University, 4Tokyo Instutute of Technology, 5National Institute of Information and Communications Technology

Complementing the bottom-up methods, the emissions inventories of greenhouse gases (GHGs) can be derived using atmospheric inverse models, providing integrated constraints on surface fluxes from all sectors/processes. For these models a variety of observations are used, including those from ground-based, ship, aircraft and satellite platforms. In particular, recent improvements in the capability of satellite observations of atmospheric composition are providing great advances on spatial resolutions. Among several plans to launch GHG and air quality (AQ) observing satellites in near future, a plan is in progress in Japan to launch the “Global Observing SATellite for Greenhouse gases and Water cycle (GOSAT-GW)”, that will make observations of carbon dioxide (CO2), methane (CH4), and nitrogen dioxide (NO2) at a horizontal resolution of 3 km or less. The missions of GOSAT-GW include (1) monitoring of whole atmosphere-mean concentrations of GHGs, (2) validation of nationwide anthropogenic emissions of GHGs, and (3) detection of GHGs emissions from large sources, such as megacities and power plants. We will provide an overview of the mission/project and some highlights on the potential role in the Asia-Oceania region, in particular, how we can support the mitigation policies on climate change as well as air quality at both international and national levels.


AS45-A011
Using a Ground-based Spectrometer, Satellite Data, and Atmospheric Model to Understand Biases in Southeast Asia Air Quality

Fernando SANTOS1#+, Santo V. SALINAS1, Li TAN1, Peng YUAN SNG1, Efthymia PAVLIDOU2, K. Emma KNOWLAND3
1National University of Singapore, 2Meteorological Service Singapore, 3Universities Space Research Association

Global emissions from industrial and transport activity, in addition to land change for intensive agriculture, have continuously increased since the pre-industrial era, driven mainly by economic and population growth. Such activity has generated immediate and long-term impacts on the local and regional atmospheric environments, especially on air quality in Southeast Asia (SEA). For instance, over Singapore, air pollution levels are strongly affected by atmospheric circulation, and Its variability is controlled by meteorological conditions and large-scale circulation patterns, including monsoon dynamics and the occurrence of biomass burning over the SEA. Therefore, accurate daily observations of NO2 and O3 made from satellites (OMPS, OMI, and TROPOMI) are critical to our ability to quantify and understand the local and regional air quality environment, particularly from the Geostationary Environment Monitoring Spectrometer (GEMS); the first instrument in the geostationary constellation (GEMS, TEMPO, and Sentinel-4) to produce hourly dataset measurements. Nevertheless, the SEA is especially challenging for satellite observations since: the sensitivity of retrievals at near-surface levels can be reduced in environments with a high degree of cloud cover, heavy particle pollution, changes in the O3 profile within the boundary layer, viewing geometry angle, biomass burning and stratospheric intrusion events. To better understand and reduce the biases between ground-based (Pandora spectrometer) and gridded (satellite and atmospheric models) trace gas datasets, we performed an exploratory data analysis using preliminary NO2 and O3 products from the Pandora spectrophotometer, GEMS instrument, and GEOS-CF numerical model. The analysis will focus on: (a) Identifying NO2 and O3 diurnal spatiotemporal biases using remote sensing data, (b) characterizing meteorological patterns at SEA, and (c) evaluating uncertainties in air quality numerical models. The outcomes of this study will significantly reduce uncertainties of NO2 and O3 algorithm retrievals from GEMS.


AS45-A014
Trend and Sources of Atmospheric Fine Particulate Matter in Recent Years in China

Mei ZHENG#+, Xiaomeng LIU, Yaxin XIANG, Yue LIU, Tianle ZHANG
Peking University

Atmospheric fine particulate matter (PM2.5) in many megacities in Asia have been of great concern due to high emission intensity and frequent pollution episodes. In recent years, a few database of PM2.5 concentration and its composition have been developed, such as Tracking Air Pollution in China (TAP), China High Air Pollutants (CHAP), and High-resolution Air Quality Reanalysis Dataset over China (CAQRA-aerosol). Based on these database, the concentration of PM2.5 and its main chemical components (e.g., sulfate, nitrate, ammonium, organic carbon, and black carbon) in China have shown a decreasing trend, but the rates vary by species and regions. In this study, concentrations of chemical species from these database are compared with the monitoring data at an urban site in Beijing during 2016-2019.Besides the trend analysis, sources of PM2.5 were investigated based on online measurements and receptor model in Beijing. With high-resolution (1h) measurement of multiple components of PM2.5 in Beijing from 2016 to 2019, positive matrix factorization was applied to quantify the contribution of different sources to PM2.5 to examine what sources contributed to the decrease of PM2.5 concentration. Our results showed that the decrease of coal combustion to PM2.5 was the most significant one for primary sources, from 9.85 μg/m3 in 2016 to 1.57 μg/m3 in 2019. Although all contributing sources of PM2.5 exhibited a decreasing trend, the relative importance of secondary source increased significantly (from 37% in 2016 to 46% in 2019). During the past decade, many studies about air quality have been conducted in China, with abundant and valuable data available. An on-going project supported by the National Natural Science Foundation of China aims to compile all air quality related data into a database. In this presentation, this project, to be completed by the end of 2023, will be also briefly introduced.


AS45-A001
Aerosol Compositions in Three Urban Areas in Taiwan During 2016-2021

Shih-Chun Candice LUNG1#+, Tzu-Yao Julia WEN1, Chia-Wei LEE2, Li-Te CHANG3
1Academia Sinica, 2National Kaohsiung University of Science and Technology, 3Feng Chia University

The objective of this study is to assess the spatiotemporal variability of the important compositions and organic markers in three urban areas in Taiwan during 2016-2021. Hi-Vol sampling of PM2.5 for 7-10 days in summer and winter has been conducted in Taipei, Taichung, and Kaohsiung, the three largest cities in Taiwan. After pre-treatments, filters were analyzed for important compositions and organic markers. Ionic species, sugars, and sugar alcohols were analyzed by Dionex ICS3000 and Thermo ICS5000. Elemental carbon (EC) and organic carbon (OC) were analyzed by a Semi-Continuous OC-EC Field Analyzer. Water-soluble organic carbon (WSOC) was analyzed by Total Organic Carbon Analyzer. Polyaromatic hydrocarbons (PAHs), nitro-PAHs, and important organic markers for cooking, biomass burning, biogenic emission, and secondary organic aerosols were analyzed by Ultra Performance Liquid Chromatography (UPLC, Sciex/Shimadzu) and a triple quadrupole mass spectrometer (MS/MS, Sciex, API5500 Plus). UPLC-MS/MS methods were optimized for the best performance. It was found that PM2.5 were 13.5 ± 5.7, 17.3 ± 7.0, and 26.0 ± 8.0 µg/m3 in Taipei, Taichung, and Kaohsiung, respectively, during 2016-2021. Ionic species accounted for 48% on average in all three cities, with 6.3 ± 3.7, 8.6 ± 5.0, and 12.9 ± 6.0 µg/m3, respectively. OC accounted for 20-23%, with 2.3 ± 1.2, 3.5 ± 1.1, and 4.2 ± 1.1 µg/m3, respectively. EC accounted for 5-7%, with 0.63 ± 0.34, 0.93 ± 0.42, and 1.31 ± 0.44 µg/m3, respectively. For biomass burning markers, levoglucosan were 11.7 ± 9.2, 35.4 ± 24.4, and 37.0 ± 21.5 ng/m3, and galactosan 16.6 ± 21.7, 4.9 ± 3.5, and 8.6 ± 7.1 ng/m3, respectively. The levoglucosan/OC values were higher in winter compared to those in summer. Source apportionment in different cities/seasons and the COVID-19 impacts will be discussed in the presentation.


Wed-02 Aug | 10:20 - 12:20 | MR327
AS16 - The Organization Processes of Atmospheric Moist Convection

Session Chair(s): Bolei YANG, Peking University

AS16-A002 | Invited
A Theory of Self-maintenance for the Madden-Julian Oscillation

Guosen CHEN1#+, Bin WANG2
1Nanjing University of Information Science & Technology, 2University of Hawaii

The Madden–Julian oscillation (MJO) is a planetary-scale convective-coupled system that amplifies over the Indo-Pacific warm pool. How the MJO is amplified and maintained and why the MJO has planetary scale are the key issues for understanding the MJO dynamics. Using a theoretical model, this study shows that the boundary layer moisture convergence feedback (BLMCF) and the cloud-radiative feedback (CRF) are major sources for the amplification of MJO. The destabilizing effect of the BLMCF is augmented over the warm ocean due to higher background moisture content there, explaining why the MJO amplifies (decays) over the warm (cold) ocean. Moreover, it is found that only the BLMCF favors the growth of the MJO over planetary scales. Due to a small Coriolis force in tropics, theoretical studies of Madden–Julian oscillation (MJO) often assume weak temperature gradient (WTG) balance, which neglects the temperature feedback (manifested in the temperature tendency). Using the scale analysis, this study further indicates that the rotation effect is strong at the MJO scales, so that the temperature feedback (TF) is as important as the moisture feedback (manifested in the moisture tendency) that is often considered to be critical for MJO. The TF is shown to be critical for the maintenance of MJO over the warm pool. This is because the TF could boost the energy generation for the system, favoring the self-maintenance of the MJO. With the interaction between BLMCF and TF, more moist available energy is generated on planetary scales, explaining the planetary-scale selection of the MJO.


AS16-A007
Pressure Drag for Shallow Cumulus Clouds: From Thermals to the Cloud Ensemble

Jian-Feng GU1#+, Robert PLANT2, Chris HOLLOWAY2, Mark MUETZELFELDT2
1Nanjing University, 2University of Reading

Shallow cumulus clouds play a crucial role in the Earth's energy budget by vertically redistributing momentum, heat, and moisture from the surface to the free atmosphere, but they cannot be explicitly resolved in current numerical models. Recent studies suggest that these clouds are composed of sticky rising thermals whose vertical velocity is mainly controlled by the buoyancy source and the drag due to the pressure perturbation. However, little is known about how the pressure drag of thermals can be related to that of a large ensemble of clouds, which is the focus of convection parameterization in climate models. This study takes the first step to bridge the gap between the pressure drag of a shallow cloud ensemble and that of an individual cloud composed of rising thermals. It is found that the pressure drag for a cloud ensemble is primarily controlled by the dynamical component. The dominance of dynamical pressure drag and its increased magnitude with height are independent of cloud lifetime and are common features of individual clouds except that the total drag of a single cloud over life cycle presents vertical oscillations. These oscillations are associated with successive rising thermals but are further complicated by the evaporation-driven downdrafts outside the cloud. The horizontal vorticity associated with the vortical structure is amplified as the thermals rise to higher altitudes due to continuous baroclinic vorticity generation. This leads to the increased magnitude of local minima of dynamical pressure perturbation with height and consequently to increased dynamical pressure drag. These findings could provide useful insights for a reasonable representation of pressure drag for shallow cumulus clouds in the convection parameterization to improve weather forecast and climate projection.


AS16-A006
Instabilities and Evolution of Radiative-convective Equilibrium

Bolei YANG1#+, Zhe-Min TAN2, Ji NIE1
1Peking University, 2Nanjing University

Radiative-convective equilibrium (RCE) is considered as the first approximation of the tropical atmosphere, which is often used as a fundamental framework to understanding climate change. With the same external forcing, numerical simulations indicate that RCE possesses multiple stable states. One is the ordinary RCE state with convection occurs randomly, and the other one is the state with bifurcation of dry and wet areas. In this study, we show that the ordinary RCE state could transfer to the other state through two phases. The first phase builds the secondary circulation and leads to the rapid intensification of dry areas, which is related to a fast and local instability revealed in previous studies. The second phase is a slow and global phase, during which dry areas expand and wet areas get wetter. A theoretical model is built to understand the mechanisms of the second phase. Based on this model, a new instability is proposed to explain the expansion of dry areas at the early period of the second phase. This work explains how two kinds of instabilities with different scales drives the ordinary RCE state to a new stable state, providing a novel pathway to understanding the evolution of RCE state and climate change in the real atmosphere.


AS16-A003
Warming Climate Intensifies Mesoscale Convective Systems During the Record-breaking Rainfall Event in July 2021 in Henan Province, China

Zhongxi LIN1#+, Ji NIE1, Jun WANG2
1Peking University, 2Chinese Academy of Sciences

Mesoscale convective systems (MCS) merged and sustained in the record-breaking heavy rainfall event during 19-21 July 2021 in Henan Province, China. Whether warming climate enhances the intensity or area of MCS is crucial for understanding the changing risk of extreme rainfall events under global warming. Ensemble simulations based on the Weather Research and Forecasting (WRF) is adopted and the human-induced temperature and humidity changes in the initial and boundary condition is estimated by ‘pseudo global warming’ approach which compares ALL-forcing and NAT-forcing in global climate model. An MCS-tracking algorithm indicates that the total rainfall volume and maximum rainfall intensity in the MCS region both enhance by ~10%. The spatial area of developing MCSs are 10%~40% larger in a warmer condition, but developed MCSs are in same sizes or smaller. Probability distributions of extreme rainfall grids inside MCS (larger than 100 mm/h) increase up to 50% in warming climate, which greatly aggravate the threat of flood. Furthermore, vertical velocity is enhanced by 10% and the cloud top is raised by 0.5 km, while the snow and ice expand horizontally and upward near the top of MCSs. Thus, the flood risk managements should take the changes of MCSs characteristics due to warming climate into account in reply to the future threat of extreme rainfall event.


AS16-A008
The Role of Diabatic Heating in the Transition from Mixed Rossby-gravity Waves to Tropical-depression-type Disturbances : A Case Study

Xianpu JI+, Tao FENG#
Hohai University

The transition from mixed Rossby-gravity (MRG) waves to tropical depression (TD)-type disturbances is commonly observed over the western North Pacific (WNP). This study aims to understand the role of diabatic heating in the wave conversion process. Using the potential vorticity (PV) diagnostic equation, it is found that diabatic heating plays a crucial role in the growth of the wave through the release of latent heat from convection. In the MRG wave stage, it is affected by both advection of the background airflow and diabatic heating, while in the TD-type disturbance stage, it is mainly affected by diabatic heating. Further sensitivity numerical experiments suggest that both thermodynamic and dynamic processes are equally significant in the MRG-TD transition process, and that the process cannot be completed if either factor is absent. The key influences and pathways of diabatic heating on MRG-TD conversion are concluded, and the physical mechanisms affecting the wave conversion are supplemented.


AS16-A012
On the Evolution of Tropopause Layer Cooling Over Tropical Cyclone

Kekuan CHU1#+, Jiayue YIN1, Zhe-Min TAN1, Jian-Feng GU1, Hao-Yan LIU2
1Nanjing University, 2Hohai University

Observations and numerical simulations show that there is typically a cold anomaly above the TC warm core. This cooling can work with the warm core to reduce the upper-tropospheric stability and affect the water vapor and momentum transport between the TC and the stratosphere. However, little is known about how the cold anomaly evolves during the life cycle of a TC and how it can be related to changes in TC intensity. This study examines the evolution of the cold anomaly throughout the lifetime of a TC with an idealized TC simulation. The cold anomaly emerges at the TC center before rapid intensification starts and continues to enhance during TC development. It moves radially and forms a cold ring around the TC until the mature stage. The advection, specifically the vertical mean motion, dominates the generation of the TLC, but the advection due to eddy motions is responsible for the cold anomaly near the center. Our findings demonstrate the importance of tropopause layer cooling on TC structure and intensity changes and indicate the necessity of additional observations of this cold anomaly to improve TC predictions.


Wed-02 Aug | 10:20 - 12:20 | MR328
AS29 - The Physical Processes Over Complex Topography: the Interactions Among Meteorology, Boundary Layer Turbulence, Clouds, Tracer Transport, and Chemistry

Session Chair(s): Wei-Ting CHEN, National Taiwan University

AS29-A010
Observing Heavily-precipitating Stratocumulus Over Complex Topography: The Yilan Experiment of Severe Rainfall (YESR)

Wei-Ting CHEN1, Shih-Hao SU2, Ching-Hwang LIU2, Hung-Chi KUO1#+
1National Taiwan University, 2Chinese Culture University

The northeasterly wind under the active East Asian winter monsoon often results in the formation of stratocumulus cloud decks in the northeastern Yilan plain area and adjacent mountains in Taiwan. It is interesting to note that Yilan’s surface wind is southwesterly even though the prevailing large-scale wind is northeasterly. In some local areas in YiLan near the mountain, the stratocumulus cloud resulted in a 200 mm/day very large rainfall. To study the evolution of precipitation patterns, planet boundary layer (PBL) turbulence, and three-dimensional circulation characteristics during these conditions, the Yilan Experiment of Severe Rainfall (YESR) was conducted in November 2020, 2021, and 2022. The study utilized a rich collection of sounding observations made with the innovative and accurately calibrated Storm Tracker (ST) mini-radiosonde, using a flexible mobile strategy to understand the evolution of PBL structure during precipitating stratocumulus events, to capture the three-dimensional structure of the planetary boundary layer wind field. The continuous meteorological data collected during two northeasterly episodes during YESR2020 revealed the variability of local-scale wind patterns and the severe rainfall characteristics induced by stratocumulus clouds. Results showed the potential for a local-scale convergence line to form over the plain area of Yilan during Northeasterly conditions, with the precipitation hotspot located in the southern mountain region of Yilan where local winds displayed turbulence features. The severe rainfall of the two northeasterly episodes highlighted the presence of shallow cumulus under the stratus with pure warm rain processes. It highlights the importance of PBL structure over complex topography. Ongoing analyses of the interplay between the cooling/moistening of the sub-cloud layer, raindrop evaporation, and local circulation patterns will be presented.


AS29-A014
Investigating the Heavy Precipitation Over Complex Topography in the Stratocumulus-dominated Environment Using Idealized Large-eddy Simulations

Jun-Jie CHANG, Wei-Ting CHEN#+, Chien-Ming WU
National Taiwan University

This study investigates the heavily precipitating stratocumulus at the windward mountains and plains, focusing on the interaction between the terrain and the moist cloud-topped boundary layer. Such a phenomenon has been observed in the northeast of Taiwan, where rainfalls can be greater than 10 mm hr-1 at some hotspots near the mountain under the stratocumulus-dominated environment with prevailing northeasterly in wintertime. To understand the related physical processes, we carried out large eddy simulations by the vector vorticity equation model (VVM) with idealized terrain configuration. The initial condition of the CONTROL simulation is the simplified Ishigaki Island sounding with a well-mixed boundary layer and homogeneous easterly below 1 km. The CONTROL indicates the heavy precipitation on the plain is related to the cold pool developed in the mountain region. The precipitation occurs mostly near the mountaintop, and the cold pool initiates in the foothill owing to evaporative cooling. When the cold pool intensifies, it moves upstream toward the plain, and the precipitation hotspot propagates with the cold pool. In the experiment with weaker low-level wind speed (WEAK), the cold pool develops much earlier and propagates upstream more easily. Inspired by the simulation results, field observations have been designed and carried out in November 2022 over Yilan to examine the evolution of the boundary layer structures of the precipitating stratocumulus and the signal of evaporative cooling in the sub-cloud layer. Our results highlight the significant role of the cold pool and its interaction with the background wind in the occurrence and propagation of heavy precipitation at the terrain and its nearby plain.


AS29-A011
The Long-term Spatial Variation of Complex Terrain Rainfall Features in Northeastern Taiwan Under the East Asian Winter Monsoon

Shih-Hao SU#+, Wen-Wei TSENG, Chin-Hsiang WU
Chinese Culture University

There are specific spatial rainfall patterns in northeast Taiwan (Yi-Lan area) under the East Asian Winter Monsoon condition. The large-scale wind field feature and the spatial distribution of water vapor flux with time can change such spatial rainfall characteristics. We analyzed the Yi-Lan area rainfall pattern variations in the past 60 years and noticed that there were obvious characteristics of terrain-locked precipitation patterns. The hot spot of rainfall occurred on the windward side of the background northeasterly flow and was decreasing toward the plain area. The average rainfall has an increasing trend, and it was more significant in the southern mountain region. We also used the reanalysis data (ERA5) to diagonalize the long-term variation of large-scale wind field features and water vapor distribution in different time periods. We noticed a significant increase in the water vapor content in the terrain's upper stream over the past 60 years. The background wind field has shifted from northerly-northeasterly to northeasterly-easterly in the past 30 years. Such changes led to a significant increase in the water vapor flux on the windward side of the terrain, which also increased the rainfall amount over the southern mountain area of Yi-Lan. However, there was not only an increasing trend in time but also showed an interdecadal oscillation signal. This decadal oscillation signal represented the background northeasterly wind speed variations. Based on the concept, we can estimate the long-term climate changes of winter rainfall in the Yi-Lan area for future climate projections by analyzing large-scale environmental variations.


AS29-A017
Investigation of Yi-Lan Low Levels Circulation and Precipitation by WISSDOM Retrieval and Ensemble Simulations

Kai-I LIN#+, Kaoshen CHUNG, Yu-Chieng LIOU, Wei-Yu CHANG
National Central University

Yi-Lan has a unique delta plain surrounded by mountains higher than 2000 m on three sides, and another side faces the Pacific Ocean. With a case study on 26 November 2021, this study attempts to investigate the local circulations at low levels of Yi-Lan area. With four-radar observations, Wind Synthesis System using Doppler Measurements (WISSDOM) is used to retrieve 3D wind fields. By illustrating wind structure below 1-km, different mechanisms of precipitation development can be examined. This study depicts different wind directions of the inflow to Yi-Lan causing different types of convergence and rainfall distributions. Furthermore, the inter-comparison between retrieved wind fields and ensemble simulations is conducted.


AS29-A003
A Physical Storyline for the Response of Orographically Locked Diurnal Convection in a Warming Scenario

Yu-Hung CHANG#+, Wei-Ting CHEN, Chien-Ming WU
National Taiwan University

This study investigates the impact of global warming on the orographically locked diurnal convection in the summer season in Taiwan. We utilize the storyline approach to provide physically self-consistent narratives of possible future projections. The orographically-locked diurnal convection involves interactions between local circulation and the thermodynamic environment of convection, which are appropriately captured by an ensemble of TaiwanVVM large-eddy simulations. The 30 ensemble simulations are forced by a set of radiosonde observations covering the variability of the background environment. The relationships of convective updraft structures over orographic precipitation hotspots and their upstream environment are analyzed. The results reveal that strong convective updraft columns within the heavily precipitating, organized systems exhibit a mass flux profile that gradually increases with height through a deep lower-tropospheric inflow layer. Enhanced convective development is associated with higher upstream moist static energy (MSE) transport through this deep-inflow layer via local circulation, augmenting the rain rate by 35% in precipitation hotspots. In the pseudo global warming experiment set, the initial temperature profiles of all ensemble members are evenly elevated by 3 K, while the relative humidity profiles remain unchanged. The enhancement of mean precipitation intensity with respect to temperature is 6.53 %·K-1, close to the Clausius–Clapeyron relation. Over the orographically-locked hotspots, the frequency of extreme rainfall increases by 65%, and their location expands toward the foothills and plains. The responses in the lifetime, structures, and propagation of the diurnal organized convection systems will be analyzed using the object-based tracking algorithm. The changes in buoyancy profiles and the MSE transport via local circulation will also be investigated to provide a comprehensive understanding of the physical processes influencing the orographically locked diurnal convection under climate change.


AS29-A009
Deep-inflow Mixing Features of Diurnal Convection Under VVM Simulations with Idealized Terrain

Wei-Ting CHEN#, Yu-Hsiu WANG+
National Taiwan University

The objective of this study is to provide a conceptual framework to understand the diurnal convection over topography dominated by local circulation. The results are analyzed from the perspective of deep-inflow mixing of convection, focusing on relating convection strength with the moist static energy from the boundary layer inflow. We used the Vector Vorticity equation cloud resolving Model (VVM) to simulate the diurnal convection over an idealized terrain of a mountain island. The simulation is initialized with a simplified sounding representing typical summer weak synoptic conditions near Taiwan. We carried out two sets of sensitivity experiments by changing the mid-troposphere relative humidity and cloud condensation nuclei (CCN) concentration, respectively. In all simulations, the diurnal precipitation time series exhibits multiple peaks in time, the first two peaks, in which the developments are closely related to the evolution of sea-valley breeze circulations, show the deep-inflow mixing features, especially in the 2nd peak with stronger local circulation and upstream energy transport. The sensitivity experiment with changing the mid-troposphere relative humidity shows that the convection in the 1st precipitation peak reduces the environmental moisture difference, while the convection strength is more influenced by the boundary layer energy in the 2nd peak. The environmental moisture determines the precipitation initiation time, duration of local circulation development, and the hydrometer contents in the atmosphere, which affect the low-level energy content, wind speed, and the amount of energy transport, further affecting the precipitation and convection intensity. The sensitivity experiment with changing CCN concentration confirms the effects of local circulation development prolonged by the delayed precipitation development on increasing energy transport and convection intensity. We concluded that the earlier precipitation peaks will modulate the environmental moisture, enhancing the influence of the boundary layer energy while reducing the influence of the mid-troposphere entrainment on estimating the convection strength.


AS29-A007
Machine Learning Detection of Fog/Low Cloud Over Eastern Taiwan Mountains from Himawari-8 Satellite True-color Images

Peng-Jen CHEN+, Wei-Ting CHEN#, Chien-Ming WU, Shih-Wen TSOU
National Taiwan University

The fog/low cloud during the cold season frequently blanket the eastern Taiwan mountains areas, known for the montane cloud forest. These fog/low clouds can provide significant water supplies to local areas and support the biodiversity of the montane cloud forest. However, it remains challenging to identify the appropriate temporal and spatial scales of these fog/low clouds due to limited ground observations in the complex topography. To address this issue, satellite remote sensing is involved to provide continuous, topography-unlimited temporal and spatial observations. In the view of the satellite from the top of the atmosphere, the mountain fog top can form a clear edge closely following the topographic features to represent the maximum height of the fog-occurring area. The objective of this work is to detect these mountain fog edges from the Himawari-8 satellite true-color image by applying the machine learning technique (U-net). The training data consist of the three visible bands observed at 8 am local time, with the fog edges in the fog-occurring cases serving as the training labels. The model performance is tested using true-color images at the same and different local times. The result shows that the model can capture the climatology of the fog edge hot spots at specific elevations, with an accuracy of over 93% for predicting fog-occurring cases at the same local time and nearly 70% for different local times. One of the characteristics of the current model is that the prediction has no false positive situations. The detection results using MODIS true-color images as input data will also be compared and discussed in this presentation. In the future, the images at different local times will be included in the model training, allowing for further investigation of the diurnal and inter-annual variations of fog/low cloud.


AS29-A005
A Study of Extreme Precipitation Events in Taiwan During the Autumn of 2022 Employing a Machine Learning-based Weather Typing Method

Li-Huan HSU#+, Kuan-Ling LIN, Chou-Chun CHIANG, Jung-Lien CHU, Yi-Chao WU, An-Hsiang WANG, Shao-Chin HUANG, Yu-Chun CHEN, Yi-Chiang YU
National Science and Technology Center for Disaster Reduction

During the autumn of 2022, a record-breaking rainfall of over 7000mm was recorded at the Ximao Shan rain gauge in Yilan. The rainfall and average daily rainfall intensity were 2 to 3 times higher than the climatology in the region. To identify the daily synoptic weather types that contributed to the heavy rainfall, a machine learning-based weather typing method was utilized. The method successfully detected multiple weather types as the synoptic systems evolved. Ten days were identified as associated with remote rainfall events, caused by the interaction between the northeasterly monsoon flow and typhoons. These 10 days contributed to approximately 40% and 60% of the autumn rainfall in eastern Taiwan and the mountainous area of Yilan, respectively. The convergence of the northeasterly monsoon flow and the outer circulation of tropical storms passing through the northern South China Sea also led to enhanced rainfall in the mountainous area of Yilan. In the La Niña year of 2022, the environment may have been favorable for such weather types. Our research shows northern Taiwan's average autumn rainfall is 1.3 times higher in La Niña years compared to the climatology. Furthermore, the rainfall from remote rainfall events in 2022 was 1.6 times higher than the average of such events in other La Niña years, but the rain intensity was similar. The 10 days of remote rainfall events in 2022 were significantly more than the average of 3 event days during other La Niña years, resulting in record-breaking rainfall.


AS29-A023
The Intercomparisons Between Various Sounding Systems Launching at Jeju Island in Summer Experiment 2021

Chia-Lun TSAI1#+, Hung-Chi KUO2, Shih-Hao SU2, Geunsu LYU3, Gyu Won LEE3
1Chinese Culture University, 2National Taiwan University, 3Kyungpook National University

The compact, low-cost Storm Tracker was co-launched with commercial sounding systems at Jeju Island, South Korea, in the summer of 2021. The Storm Tracker collected high temporospatial profiles of temperature, pressure, humidity, wind directions, and wind speed. The performance of these observational metrics will be evaluated and compared with Vaisala RS-41 and GRAW DFM-09. There were 32 launches, and the quality of Storm tracker data has been controlled by AIQC algorisms, which are developed by training huge amounts of launches in advance at subtropical regions. The main objective of this study is not only to check Strom Tracker's performance but also to understand potential variances when launched in mid-latitude areas. The average pressure bias between RS-41 and DFM-09 sounding systems is ~0.75 hPa and ~3hPa with the Strom Tracker. For temperature, the average bias is 0.57oC between RS-41 and DFM-09, with ~2oC (0.6oC) differences in the daytime (nighttime) compared with the Strom Tracker. The dew point reveals ~5oC (2oC) variances between the Strom Tracker and RS-41 (DFM-09), and ~2oC between RS-41 and DFM-09. The wind speed and direction discrepancies observed from the Storm Tracker are ~2 m s-1 and from 10 to 20o compared with the other two sounding systems. Generally, the results show good agreement between these three sounding systems. However, a significant bias of temperature in the daytime should be paid more attention to with the Strom Tracker.


Wed-02 Aug | 10:20 - 12:20 | MR329
AS41 - Atmospheric Composition and Cloud Observations from Next Generation of Satellites- Breaking the Temporal Barriers

Session Chair(s): Pawan GUPTA, NASA Goddard Space Flight Center, Robert LEVY, NASA Goddard Space Flight Center, Ukkyo JEONG, Pukyong National University

AS41-A003
A NASA GEO Imager Research Algorithm Dataset for Cloud Optical Properties, Part II: Evaluation Against NASA LEO Products

Kerry MEYER1#+, Steven PLATNICK1, Robert HOLZ2, Galina WIND3, Nandana AMARASINGHE3, Steve DUTCHER2, Andrew HEIDINGER4
1NASA Goddard Space Flight Center, 2University of Wisconsin, 3Science Systems and Applications, Inc., 4National Oceanic and Atmospheric Administration

The advanced capabilities of the new generation of operational weather satellite imagers in low-Earth orbit (LEO; e.g., VIIRS) and geostationary (GEO; e.g., ABI, AHI, etc.), having spectral and spatial capabilities analogous to the NASA Earth Observing System (EOS) MODIS, offer the opportunity to extend the high impact EOS MODIS dataset for clouds into the next decade and into the time domain. Such a merged, and consistent, LEO/GEO cloud product Program of Record (PoR) can enable enhanced climate and process studies by NASA investigators and the broader research community. In addition, this PoR is desired to provide critical synergy with the NASA Atmosphere Observing System (AOS), which is currently in formulation and is designed to address the Aerosols, Clouds, Convection, and Precipitation Designated Observables identified by the 2018 NASA Earth Science Decadal Survey. In a companion presentation (Platnick et al., also submitted to this session), we give an overview of a NASA research cloud optical property algorithm for the new GEO imagers that was developed to provide consistency with the NASA MODIS/VIIRS cloud continuity products CLDPROP. Here, we show results of our efforts to evaluate the consistency of this new GEO cloud dataset against the MODIS/VIIRS continuity dataset. We also will discuss ongoing challenges towards achieving LEO/GEO product consistency, including the impacts of fundamental differences in sensor specifications and/or orbits (e.g., spectral channel differences, spatial resolution/swath, viewing/solar geometries), differences in relative radiometric calibration, and forward radiative model issues.


AS41-A002
Cloud and Aerosol Detection Using Spectral, Spatial and Temporal Information from Passive Satellite Instruments

Chenxi WANG1,2#+, Yingxi SHI3, Yihan FANG4, Clark ZHANG5, Ryan SONG6, Kerry MEYER2, Steven PLATNICK2
1Goddard Earth Sciences Technology and Research (GESTAR) II, 2NASA Goddard Space Flight Center, 3University of Maryland, Baltimore County, 4University of Maryland, College Park, 5Vanderbilt University, 6Carnegie Mellon University

Detection of atmospheric constituents such as cloud and aerosols with satellite observations is often a critical initial step in many remote sensing algorithms. Many traditional algorithms were developed based on underlying physics and hand tuned thresholds. Weakness of these methods is that it is challenging and time-consuming to develop algorithms across multiple instruments and locations. To overcome this weakness, we designed and trained a couple of Machine Learning (ML) based models for cloud and aerosol detection. Specifically, a Random Forest (RF) model, a Convolutional based Encoder-Decoder Neural Network, and a Recurrent Neural Network (RNN) are designed and trained with spectral, spectral/spatial, and spectral/spatial/temporal input, respectively. The first two models that require spectral and spatial input are designed for passive spectrometers such as VIIRS and MODIS; while the third model is designed for geostationary instruments, such as GOES-16/17 ABI. A hybrid training database is generated based on years of collocated satellite-satellite (e.g., CALIPSO/VIIRS and CALIPSO/ABI) and satellite-ground station (e.g., ABI/AERONET) data, and manually picked events with labels. In this presentation, we will introduce of the training database and compare the three different models.


AS41-A009
Investigation of Atmospheric Cloud Characteristics Over Western-Indian Region Using Ground-based Lidar, Satellite, and Reanalysis Datasets

Som Kumar SHARMA1#+, Dharmendra KAMAT1, Prashant KUMAR2, Sourita SAHA3
1Physical Research Laboratory, 2Space Application Center, 3University of California

Clouds cover most of the Earth, and a slight variation in their properties disturbs the radiation budget, modulates weather, and impacts climate change. Due to the strong interaction with shortwave and longwave radiation, any slight changes in the clouds have a potent effect on the climate system. Clouds are highly dynamic in space and time, and their proper representation in climate models remains challenging. Cloud properties such as cloud base height (CBH), cloud top height (CTH), cloud fraction, and vertical layer structure significantly affect the radiative balance, atmospheric circulations, and other meteorological processes. Therefore, monitoring and investigating these cloud parameters is essential for climate diagnosis and predicting future climate. This study deals with the investigation of cloud properties over two locations: Udaipur (24.6°N, 73.7°E) and Mount Abu (24.5°N, 72.7°E) in the Aravalli ranges of Western India using a ground-based Lidar (ceilometer), satellite, and reanalysis datasets. Over these regions, the average cloud base height for layers 1 and 2 (CBH1 and CBH2) follows the same seasonal pattern: low during monsoon and high during pre and post-monsoon. The cloud top height (CTH) information is obtained for the same period using Moderate Resolution Imaging Spectroradiometer (MODIS) instrument onboard Terra and Aqua satellites. The observed CTH ranges from about 0.2km to 19km. Furthermore, the classification of these observed clouds is performed using cloud top pressure and cloud optical thickness values as per the International Satellite Cloud Climatology Project (ISCCP) cloud classification. Over Udaipur, cirrostratus clouds were found to have a maximum occurrence (~ 36%) during the study period. ERA5 and MODIS-derived CBH doesn’t correlate well with the observed CBH from the ceilometer, indicating the limitation of reanalysis and satellite observations of cloud base height over the complex orographic region.


AS41-A011
Automatic Smoke Plume and Wildfire Instance Tracking Across Scenes from Multiple Sensors

Michael GARAY1#+, Olga KALASHNIKOVA1, Nicholas LAHAYE1, Kyongsik YUN1, Hugo LEE2
1California Institute of Technology, 2Jet Propulsion Laboratory, California Institute of Technology

Earth observing instruments from multiple organizations, including NASA and NOAA in the United States, continue to provide multiple observations of aerosol plumes from wildfires. The Segmentation, Instance Tracking, and data Fusion Using multi-SEnsor imagery (SIT-FUSE) project at the Jet Propulsion Laboratory has developed an unsupervised machine learning framework that allows users to segment instances of objects like wildfires and smoke plumes in single and multi-sensor scenes from satellite instruments with minimal human intervention in low and no label environments. This is an important step toward allowing automatic smoke plume and wildfire instance tracking through time from multiple instruments. We will demonstrate this system with examples from the NASA/NOAA FIREX-AQ field campaign that took place in 2019. In addition, we will describe ongoing work to allow automatic feature identification and tracking using deep learning - specifically contrastive learning (CL) enhanced by the topological features of the object instances detected.


AS41-A006
Spectral Replacement Using Machine Learning Methods for Continuous Mapping of GEMS

Yeeun LEE1+, Myoung Hwan AHN1#, Mina KANG1, Mijin EO1, Kyung-Jung MOON2
1Ewha Womans University, 2National Institute of Environmental Research

For environmental monitoring, the Geostationary Environment Monitoring Spectrometer (GEMS) measures backscattered radiances in the ultraviolet and visible spectral region (300-500 nm) over the Asia-Pacific region to retrieve key atmospheric constituents and aerosol properties eight times a day. The measured radiances and retrieved properties of GEMS have been collected in about two years of operation after completion of the in-orbit test in October 2020. There have been substantial efforts to calibrate the GEMS Level 1B data and here we briefly introduce the updates of calibration processes along with one of the studies regarding bad pixels of GEMS. Bad pixels occurred on the detector array could cause consistent information gaps and the issue becomes more problematic for hyperspectral measurements because only a few defective radiances in a spectrum can induce erroneous spectral features. To efficiently resolve the spatial discontinuity caused by bad pixels in the measured radiances and further in the retrieved properties of GEMS, we apply spectral replacement on the radiance level with machine learning models using multivariate linear regression and artificial neural network (ANN). Because the key information for the retrieval is originated from subtle spectral features, we more focus on whether the features can be successfully reproduced with the models trained with large datasets, the GEMS defect-free measurements. The results and conclusions can be found in the paper published with the identical title, and briefly said, the spectral replacement can be quite effective for retrievals (i.e., cloud centroid pressure) with some conditions such as input and output ranges or instrument artifacts. However, limitation still remains for the approach especially for low signals or very strong absorption features such as ozone. It indicates additional information would be needed to improve the methods if one pursues very high retrieval accuracy with the synthetic spectra.


AS41-A013
The NASA TEMPO Mission: Revolutionary Air Pollution Observations Over North America from Geostationary Orbit

Aaron NAEGER1,2#+, Michael NEWCHURCH3, Xiong LIU4, Kelly CHANCE4
1NASA / University of Alabama in Huntsville, 2National Aeronautics and Space Administration, 3University of Alabama in Huntsville, 4Center for Astrophysics | Harvard & Smithsonian

NASA is preparing to launch the Tropospheric Emissions: Monitoring of POllution (TEMPO) mission into Geostationary Earth Orbit (GEO) in April 2023. TEMPO will provide hourly and sub-hourly daytime observations of aerosols and trace gases, including nitrogen dioxide, formaldehyde, sulfur dioxide, and ozone, at high spatial resolution (~2.0 x 4.75 km2) across a Field of Regard (FoR) covering greater North America. The hyperspectral ultraviolet-to-visible measurements from the TEMPO grating spectrometer will permit an ozone profile retrieval capable of monitoring the diurnal evolution of ozone in the planetary boundary layer. The non-standard or special scan operations of TEMPO at sub-hourly frequency (e.g., 2-10 minutes) over selected slices of the FoR will further enhance monitoring capabilities during air quality disasters, such as wildfires, volcanic eruptions, and dust storms. During the pre-launch phase of this mission, a large diversity of stakeholders and end-users have been engaged in the TEMPO Early Adopters Program, supported by the NASA Applied Sciences Program, which aims to maximize the societal benefit of TEMPO data after launch. Key objectives of the Early Adopters Program include preparing the user community for operational TEMPO data through early application of proxy products and designing products, tools, and mission planning activities to better meet user needs. This presentation will provide a TEMPO mission status update, details on data product developments, an Early Adopters Program overview, demonstrations of science applications enabled through TEMPO data, and insight into the special operations component of the mission.


AS41-A001
Decadal Characterization of Satellite-based Aerosol Types Over Arabian Peninsula: Comprehensive Insight and General Performance

Alaa MHAWISH1#+, Zakiah ALHAJJI2, Jumaan ALQAHTANI2
1Sand and Dust Storm Warning Regional Center, National Center for Meteorology, Jeddah, KSA, 2National Center for Meteorology

Retrieving aerosol characteristics such as particle size, shape, and absorption properties is a big challenge in satellite-based remote sensing, mainly for the single-viewing-angle instrument. Multi-angle instruments such as Multi-angle Imaging Spectroradiometer (MISR) measures the reflected radiation from nine viewing angles, allowing the retrieval algorithm to accurately distinguish different aerosol microphysical and optical properties along with total aerosol loading in the atmospheric column. Recently, MISR upgraded the aerosol retrieval algorithm version 23 (V23) and enhanced the spatial resolution of the aerosol products to 4.4km, enabling the study of the aerosol characteristics at a finer scale. This study uses 20 years of MISR V23 aerosol products to comprehensively investigate aerosol optical and microphysical properties and their performance over Gulf Cooperation Council (GCC) countries using two decades of aerosol products from the MISR algorithm. The assessment of MISR AOD showed good agreement with ground-truth AOD from AERONET, with ~75% of retrieval falling within the expected error (0.05±0.2AOD) and a high Pearson’s correlation coefficient (R = 0.86). However, MISR relatively underestimates AOD at higher aerosol loading conditions (AOD>0.6) while overestimating coarse-dominated aerosol mixture (Angstrom Exponent <0.7). The 20 years mean MISR AOD showed higher aerosol loading dominated by coarse aerosol types over the Eastern province of Saudi Arabia and Rub’al Khali. Seasonally, the size-fractionated AOD showed that GCC countries dominated by coarse AOD (cAOD) and non-spherical aerosol particles mainly in Spring, while the contribution of small AOD (sAOD) to the total range from 42-45% for Winter and Autumn. Overall, the high spatial resolution of MISR aerosol data products has a great potential to identify an aerosol hot spot and constrain the aerosol types, mainly dust, across the highly polluted region in the Middle East.


AS41-A005
The Dark Target Aerosol Project: Combining LEO and GEO Satellites for Monitoring Rapid Aerosol Changes on a Global Scale

Robert LEVY1#+, Shana MATTOO2,1, Pawan GUPTA1, Yingxi SHI3, Virginia SAWYER1, Robert HOLZ4, Jennifer WEI1, Lorraine REMER3,5, Zhaohui ZHANG6,7, Bhaskar RAMACHANDRAN2
1NASA Goddard Space Flight Center, 2NASA Science Systems and Applications, Inc., 3University of Maryland, Baltimore County, 4University of Wisconsin, 5Airphoton LLC, 6Adnet Inc., 7NASA Goddard Earth Sciences Data and Information Services Center

The Dark Target (DT) retrieval algorithm was developed for Moderate-resolution Imaging Spectroradiometer (MODIS) to derive aerosol optical depth (AOD) over global land and ocean. Because of its relative simplicity and flexibility, it can be implemented on the Visible Infrared Imaging Radiometer Suite (VIIRS), or any imager with MODIS-like wavelength information. We are retrieving on VIIRS Suomi-NPP and NOAA-20 which are also in sun-synchronous low-earth orbit (LEO) to stitch together a long-term data record (now at 22 years and counting). More recently, DT has been ported to Full Disk imagery from sensors in Geostationary orbit (GEO), including Advanced Baseline Imager (ABI) on GOES-R series (East and West) and Advanced Himawari Imager (AHI) on the Himawari series. With these GEO sensors, we observe much of the globe every 10 minutes, thus providing the opportunity to characterize rapid aerosol changes and the aerosol diurnal cycle. Overall, the new GEO products look good, and compare reasonably well to existing LEO and to ground-based sunphotometer data. We discuss remaining challenges regarding relative sampling of GEO versus LEO as well as calibration. Considering the period when all 6 sensors are operating, we are imminently releasing a combined 4-year GEO / LEO dataset at 0.25°x0.25° resolution and 30-minute time intervals. Here, we introduce the new dataset including details about the product, expected accuracies, steps to acquire, and intended use. 


Wed-02 Aug | 10:20 - 12:20 | MR331
AS01 - The Asian Monsoon, Extremes and Climate Change

Session Chair(s): A. P. DIMRI, Jawaharlal Nehru University, Jianping LI, Ocean University of China, Kritanai TORSRI, Ministry of Higher Education, Science, Research and Innovation

AS01-A043
Long-term Precipitation Changes in the Baiu and Akisame Seasons in Japan Over the Past 120 Years (1901–2020)

Hirokazu ENDO#+
Meteorological Research Institute

Long-term variations in precipitation during the major rainy period in Japan—the Baiu (June–July) and Akisame (September–October) seasons—are investigated using precipitation records from 44 weather stations in western to eastern Japan over the past 120 years (1901–2020). The total amount of Baiu precipitation has increased over the 1901–2020 period, mainly during the mid–late stages of the season (late June–July) over regions on the Sea of Japan side of the country. In contrast, the precipitation amount during the Akisame season has decreased, mainly during the mid-stage (late September–early October) over all regions. The frequency and intensity of heavy precipitation have generally increased in both seasons, but the trends are much stronger for the Baiu season compared to those for the Akisame season. A prominent positive trend, 23.5% per 100 years (18.1% per ℃), which is much higher than the Clausius–Clapeyron rate (approximately 7% per ℃), is observed for the Sea of Japan side of western Japan for the seasonal maximum 1-day precipitation total during the Baiu season. It may be noteworthy that the observed long-term trends differ greatly between the Baiu and Akisame seasons even though the statistical significances of the trends are not so high, because similar differences between the two rainy seasons are found in results of global warming simulations.


AS01-A004
Intraseasonal Variability of Global Land Monsoon Precipitation and its Recent Trend

Fei LIU1#+, Bin WANG2
1Sun Yat-sen University, 2University of Hawaii

Accurate prediction of global land monsoon rainfall on a sub-seasonal (2-8 weeks) time scale has become a worldwide demand. Current forecasts of weekly-mean rainfall in most monsoon regions, however, have limited skills beyond two weeks, calling for a more profound understanding of monsoon intraseasonal variability (ISV). We show that the high-frequency (HF; 8-20 days) ISV, crucial for the Week 2 and Week 3 predictions, accounts for about 53-70% of the total (8-70 days) ISV, generally dominating the sub-seasonal predictability of various land monsoons, while the low-frequency (LF; 20-70 days)’s contribution is comparable to HF only over Australia (AU; 47%), South Asia (SA; 43%), and South America (SAM; 40%). The leading modes of HFISVs in Northern Hemisphere (NH) monsoons primarily originate from different convectively coupled equatorial waves, while from mid-latitude wave trains for Southern Hemisphere (SH) monsoons and East Asian (EA) monsoon. The Madden-Julian Oscillation (MJO) directly regulates LFISVs in Asian-Australian monsoon and affects American and African monsoons by exciting Kelvin waves and mid-latitude teleconnections. During the past four decades, the HF (LF) ISVs have considerably intensified over Asian (Asian-Australian) monsoon but weakened over American (SAM) monsoon. Sub-seasonal to seasonal (S2S) prediction models exhibit higher sub-seasonal prediction skills over AU, SA, and SAM monsoons that have larger LFISV contributions than other monsoons. These results suggest an urgent need to improve the simulation of convectively coupled equatorial waves and two-way interactions between regional monsoon ISVs and mid-latitude processes and between MJO and regional monsoons, especially under the global warming scenarios.


AS01-A005
Long-term Trends and Variations of Southwesterly Flow Around Taiwan During Mei-yu Season Over 44 Recent Years

Yen-Chao CHIU#+, Fang-Ching CHIEN
National Taiwan Normal University

This study investigates the characteristics and long-term trends of southwesterly flow around southern Taiwan (hereafter, SWs) during mei-yu seasons (15 May - 15 June) from 1979 to 2022. The results show that the occurrence number of SWs had in general an increasing trend over this 44-year period, with a decadal oscillation by starting from a relatively small number in the 1980s and reaching a relative peak in the 2000s. The 4-year and 10-year periods show more power according to wavelet analysis. While the 4-year power period was more evident from 1995 to 2005, the 10-year power period was more evident before 2000. This posts a potential threat to Taiwan due to the increasing trend of heavy rainfall associated with the longer duration and higher moisture flux of the SWs events. The SWs activity was influenced by the long-term increasing trend of geopotential height and its decadal variability near Taiwan. When the intra-seasonal oscillation was evident, the weather system that mainly affected the occurrence of SWs was the low pressure system to the north of Taiwan, while when it was weak, the location of the western North Pacific subtropical high to the south of Taiwan was more important. In addition, the SWs index which was highly correlated with the precipitation during mei-yu seasons can effectively reflect the interannual variability of precipitation in Taiwan in periods of different lengths. These findings indicate that the SWs index can be used as a monsoonal precipitation index for Taiwan, especially southern Taiwan.


AS01-A077
Analysis of Long-term Trends of Water Vapor Transport in the Major Water Vapor Channel on the Southeastern Qinghai-Tibet Plateau

Dengxu ZHANG#+
Lanzhou University

As the main water vapor channel entrance of the plateau, the water vapor flux convergence and precipitation in the Yarlung Tsangpo River Canyon region have been decreasing continuously since 1979, which has an important impact on the water storage of the plateau. Since the Lagrangian method is more responsive to the spatial and temporal variability of water vapor transport than the Eulerian method, this study uses the Lagrangian trajectory tracking model LAGRANTO to drive the ERA5 reanalysis data to track the water vapor transport in the canyon region for the past 40 years and obtain specific water vapor transport trajectories, and by analyzing the changes in the spatial and temporal distribution of the trajectories including trajectory location and trajectory height changes, as well as the interannual variability of water vapor flux on the trajectories By analyzing the interannual variation of water vapor flux on the trajectory and the interannual trend of water vapor flux on the trajectory, the main factors affecting the variation of water vapor transport in the southern part of the plateau are identified by combining the large-scale circulation such as monsoon and the interdecadal oscillation index for correlation analysis. At this stage, by comparing the differences in water vapor transport in typical wet and dry years, it is found that in addition to the source water vapor contribution and the influence of monsoon, the precipitation loss-related processes along the water vapor transport play a decisive role in the water vapor balance of the Yarlung Tsangpo River region, so the trend of water vapor transport changes in the past 40 years will be further analyzed and the main factors affecting water vapor loss will be studied, aiming to clarify the influence mechanism of water vapor transport changes in the southern plateau.


AS01-A080
Increasing Trend in the Duration of the Indian Monsoon Season

Aneesh SUNDARESAN1#+, Tamas BODAI2, Sijikumar S3
1IBS Center for Climate Physics, Pusan National University, 2IBS Center for Climate Physics, 3Indian Space Research Organisation

The mean Indian summer monsoon (ISM) rainfall as well as its duration have a profound impact on the agriculture practice in the country. Due to the recent increase in the surface temperature, global circulation patterns exhibit considerable changes which also affects the characteristics of ISM. The present study aims to find out any long-term changes in the monsoon onset and withdrawal times and the length of the monsoon rainy season that exists over different parts of India and the possible mechanisms behind it. During the last four decades, the trend analysis of ISM over south India and North-West (NW) India shows an early onset in both regions. However, the trends are statistically less significant. The monsoon withdrawal dates over NW India and south India show a statistically significant delay of about 6 days/decade and 3.25 days/decade, respectively. As a result, the monsoon season over NW India and south India shows a lengthening of about 7.8 days/decade and 3.5 days/decade, respectively. During the withdrawal phase of the ISM, a stronger monsoon low-level jet and an enhancement of the ISM rainfall have been observed in recent decades. The role played by factors such as Eurasian temperature, Indian ocean warming, Atlantic Multidecadal Oscillation (AMO) and Pacific Decadal Oscillation (PDO) on the ISM withdrawal is examined. The AMO has changed its phase from negative to positive in recent decades, particularly after about 1998, which might have played a key role in enhancing the meridional tropospheric temperature gradient. The stronger meridional tropospheric temperature gradient and the Eurasian surface warming observed in recent decades might played a key role in the delayed monsoon withdrawal over NW India. The delayed ISM withdrawal over the south of India is mainly attributed to the AMO phase change and the changes in the Indian Ocean.


AS01-A024
Decadal Background for Active Extreme Drought Episodes in the Decade of 2010–19 Over Southeastern Mainland Asia

Lin WANG1#+, Gang HUANG1, Wen CHEN1, Ting WANG1, Chakrit CHOTAMONSAK2, Atsamon LIMSAKUL3
1Chinese Academy of Sciences, 2Chiang Mai University, 3Environmental Research and Training Center

Severe and extreme drought in southeastern mainland Asia (SEMA) had worsened drastically in 2010–2019, more than twice as frequently in the preceding decade. It is found that the spring rainfall has undergone a concordant positive-to-negative transition with the turning point occurred at the 2010, and can explain 43% of the overall regime shift towards exaggerated severely dry condition. Associated with the decadal precipitation change, the anomalous northeasterlies prevail over SEMA, resulting in weakened eastward moisture propagation from Indian Ocean as well as enhanced divergence. Meanwhile, there is a downward motion over SEMA. Such circulation pattern is remotely forced by teleconnection from the Tropical Western Indian (TWI) SST. TWI SST is negatively correlated with SEMA precipitation and highlights a regime shift around 2010, after which the TWI have persistent warm SST helping to maintain deficient SEMA precipitation. In terms of the physical mechanism, the heating in TWI warms the troposphere aloft and emanates wedge-shaped Kelvin wave with northeast flank traversing SEMA, where friction-driven northeasterly low-level wind and divergence emerge to block moisture penetration from the Indian Ocean. The low-level divergence is followed by descending motion in SEMA, suppressing convection and rainfall. Further, the simulated structure forced by TWI SST alone bears a close resemblance to the observed evidence, confirming the critical role of TWI. Finally, it is illustrated that ENSO and its diversity have modulating effect on SEMA precipitation as well as the coupling between TWI SST and SEMA precipitation, during the previous winter and the concurrent spring.


AS01-A075
Decadal-scale Changes in the Seasonal Transition Patterns of the Asian Summer Monsoon and the South China Sea Tropical Cyclone Frequency During May

Yin-Min CHO#+, Mong-Ming LU, Chung-Hsiung SUI
National Taiwan University

In this study, we used 40 years (1981–2020) of TC data and reanalysis data to investigate the relationship between the SCS TC activity frequency in May and the spring-to-summer transition of Asian monsoon systems. The results show clear decadal-scale variations of TC frequency with two active decades during the 1980s and 2000s, and two inactive decades during the 1990s and 2010s. The period of 2011–2020 was identified as a decade of the minimum TC genesis frequency over the SCS in May since 1981. The circulation and surface air temperature contrast during the earlier two decades is drastically different from the contrast during the later two decades. The difference can be understood as decadal-scale variations of two leading modes of the 40-yr March-June precipitation in the Asian-Australian-Pacific monsoon region. For the two earlier decades, the contrast of active and inactive SCS TC frequency in May can be explained by the difference in EOF2. The positive EOF2 corresponds to a wet and dry dipole pattern of the concurrent anomalies with enhanced convection over the eastern Indian Ocean and suppressed convection over the western Pacific warm pool. For the two later decades, the contrast can be explained by the difference in EOF1, which shows a meridional dipole pattern over the eastern Indian Ocean reflecting the northward movement of the ITCZ. Among four decades, the decade of 2001-2010 shows the earliest northward transition of the ITCZ and the most active SCS TC frequency in May.


AS01-A032
Recent Extreme Events: A Glimpse of Climate Change?

Ramesh KRIPALANI1,2#+, Preethi BHASKAR1, Kyung-Ja HA3, Jai-Ho OH4, Milind MUJUMDAR1
1Indian Institute of Tropical Meteorology, 2Pukyong and Pusan National Universities, 3Pusan National University, 4Nano C&W

During the last couple of years extreme climate-related events appear to have increased in devastating proportions in particular droughts and heatwaves. Major Rivers around the world are drying up as record breaking heatwaves take their toll. Europe recorded its worst drought in 500 years, drying up Rivers and bringing up archeological wonders and historic horrors, Roman Ruins to the surface, exposing World War II ships. Half of China hit by drought and worst heatwave in summer 2022. Siberia heating was unprecedented during the last several millennia. On the other hand, Pakistan recorded devastating and fatal floods during summer 2022. Heaviest rains in more than a century hit South Korea – worst in 115 years. While the summer monsoon rainfall during 2020 witnessed heavy rains over South Asia (in particular West-Central India) as well as over East Asia (in particular China’s Yangzte River Valley). On the other hand, summer 2022 witnessed severe floods over South Asia (Pakistan) and severe drought prevailed over East Asia (Yangzte River Valley). Possible factors leading to the contrasting behavior of Summer Monsoons 2020 and 2022 will be discussed at the AOGS2023 Conference.


Wed-02 Aug | 1:00 - 5:15 | Summit
AS - Atmospheric Sciences Poster Session 2

AS01-A002
Intraseasonal Oscillation and the Taiwan Climate

Chih-Wen HUNG#+
National Taiwan Normal University, Taiwan

It is known that the eastward moving Tropical Intraseasonal Oscillation (TISO) has impact on the climate over the Asian-Australian monsoon region. This study summarizes that the TISO can have the impact on the Taiwan climate in the onset of the Meiyu season and the summer and winter monsoon rainfall. For the onset of the Meiyu in Taiwan, it is found that for almost half of the cases, the first transition of the Asian summer monsoon can be classified as a sharp onset, which is occurred with an eastward-propagating TISO from eastern Africa and the western Indian Ocean to the Maritime Continent. This efficient and persistent transport of moisture presumably provides a favorable condition for the maintenance of the Meiyu front and marks the onset of the Taiwan Meiyu season. Following the Meiyu, during the summer, the TISO can be represented by the boreal summer intraseasonal oscillation (BSISO) better. Our results found that the BSISO and the associated horizontal patterns of the western North Pacific typhoon frequency are closely related. Taiwan has larger rainfall when the major BSISO convection moves northwestward from the Philippine Sea to the Taiwan area. The anomalous low-level cyclonic flow and the increased typhoon frequency directly result in the larger rainfall in Taiwan. The enhanced low-level southwesterly flow which transports the moisture to Taiwan is responsible for more summer rainfall in Taiwan. On the other hand, during the winter season, the rainfall in Taiwan is also related to the TISO. The results show that Taiwan has larger rainfall when TISO reaching the Indian Ocean and the western part of the Maritime Continent, and less rainfall when it moves to the western Pacific warm pool area. The mechanisms suggested by this work are: (1) Tropics to mid-latitude wave train and (2) Increase of moisture supply from South China Sea.


AS01-A019
Influences of Tropical Pacific and North Atlantic SST Anomalies on Summer Drought Over Asia

Jianmin ZHANG+, Renguang WU#
Zhejiang University, China

Droughts can cause enormous damage to agriculture, ecosystems and socio-economics because of their longevity and widespread spatial extent. As a densely populated region in the world and with a large area of arid and semi-arid regions, Asia is largely affected by droughts, especially in summer. The drought variations are determined by precipitation that affects water supply and temperature that affects water depletion through surface evaporation. In this talk, we will present an analysis of contributions of precipitation and temperature to the spatial patterns and temporal variations of summer drought over Asia measured by 3-month Standard Precipitation Evaporation Index (SPEI03) in July and the factors for year-to-year variations of summer drought. We will perform numerical experiments with the Community Earth System Model (CESM) to explore the influences of different regional SST anomalies on summer drought in Asia. Our results show that the July SPEI03 displays a north-south dipole distribution across approximately 30°N, which is dominated by interannual component. Precipitation and temperature both contribute to the summer drought variations over Asia. Asian drought in summer is associated with both the tropical Pacific and North Atlantic SST anomalies. Preceding tropical Pacific SST anomalies influence the summer Asian drought via the large-scale divergent fows and soil moisture-evaporation feedback. The North Atlantic SST anomalies influence the Asian drought through atmospheric wave trains over the North Atlantic-Eurasia. 


AS01-A029
Increase in Intraseasonal Rainfall Driven by the Arabian Sea Warming in Recent Decades

Baosheng LI1#+, Lei ZHOU2, Jianhuang QIN3
1Second Insititute of Oceanography, China, 2Shanghai Jiao Tong University, China, 3Hohai University, China

The changes in the spatial distribution of Indian summer monsoon (ISM) rainfall pose significant risks of extreme weather events in the Indian subcontinent and Arabian Peninsula. Monsoon intraseasonal oscillation (MISO) plays a key role in the intraseasonal distribution of the ISM rainfall, and changes in MISO determine the ISM rainfall patterns in the warming climate as well. However, the trend in MISO remains unclear in recent decades. Here, we find that the variance of MISO has an increasing trend from 1982 to 2017 over the northeastern Arabian Sea (AS), accompanied by increasing intraseasonal rainfall. The enhancement in rainfall is mainly nourished by the increasing moisture supply. Accordingly, the intraseasonal moisture budget diagnosis suggests that the changes in vertical moisture advection dominate the increasing amount of moisture over the northeastern AS. In contrast, the horizontal moisture advection and moisture processes associated with condensational heating exhibit a decreasing trend. By further decomposing the timescales, the upward advection of background moisture by intraseasonal vertical wind velocity is the main contributor. Given sufficient moisture availability, the changes in the intraseasonal vertical velocity are more important than the background moisture, which is a response to the strengthening of intraseasonal convergence in the PBL. Moreover, the faster warming of the AS and the increasing cyclonic vorticity associated with the poleward movement of the summer mean low-level jet are responsible for the increasing trend in PBL convergence. Thus, the MISO accompanying the intraseasonal rainfall displays an increasing trend over the northeastern AS. This recent intensified intraseasonal rainfall has contributed to the trend in the mean and extremes over the central-western parts of the Indian subcontinent. The results could assist the understanding and better projections of spatial pattern of rainfall during the ISM.


AS01-A030
Connections Between ENSO and Tibetan Plateau Snow Cover

Zhibiao WANG#+
Chinese Academy of Sciences, China

El Niño–Southern Oscillation (ENSO) and the Tibetan Plateau snow cover are important factors in interannual climate variability. The relationship between ENSO and the Tibetan Plateau snow variation is still undetermined. While some studies suggested that ENSO is a key factor of changes in snow cover over the Tibetan Plateau, other studies noted independence between the two. The present study revealed a prominent interdecadal change in the relationship between ENSO and the spring Tibetan Plateau snow-cover variation in the early 2000s. There is a significant positive correlation between ENSO and the spring Tibetan Plateau snow-cover variation in the period 1988–2003, but an obvious negative relationship is detected in the period 2004–19. The interdecadal change in the ENSO–snow relationship is related to the distinct pathway of ENSO influence on the spring Tibetan Plateau snow-cover variation during the two periods. In the period 1988–2003, ENSO induces anomalous convection over the tropical western North Pacific that in turn causes atmospheric circulation and moisture anomalies over the Tibetan Plateau. The resultant winter snow anomalies over the central-eastern Tibetan Plateau persist to the following spring. In the period 2004–19, ENSO induces North Atlantic sea surface temperature (SST) anomalies in winter that are maintained to the following spring. The North Atlantic SST anomalies then stimulate the atmospheric circulation anomalies extending to the Tibetan Plateau that induce snow-cover anomalies there in spring. The different processes of ENSO influence lead to opposite anomalies of spring snow cover over the Tibetan Plateau in the two periods.


AS01-A033
The Role of C-shape Tropical Land in Forming Asian Summer Monsoon

Xinyu WEN#+, Junyu MEI
Peking University, China

The topographic effect of lands on monsoonal climate variability is one of the key topics in monsoon dynamics studies. Here, we re-visit the topographic effect of varying-shaped lands on Asian monsoon formation using a fast AGCM with a large number of experiments. It is found that the C-shaped continent located over the tropics and subtropics favors a distinct Asian summer monsoon pattern most. The preliminary results show that the C-shape land creates more evident monsoonal responses than other shape lands through three key processes, including intensified cross-equatorial winds, water vapor convergence along with subtropical monsoonal troughs, and one significant low-pressure departure near the southeast corner of the NH land. We would like to show more detailed results derived from our numerical experiments, which help to improve our understanding of monsoon formation and variability.


AS01-A038
Low-level Jet Observed Over the East China Sea During the Bai-u Season

Megumi NOGUCHI1, Noriyuki NISHI2#+, Atsuyoshi MANDA3
1Japan Meteorological Agency, Japan, 2Fukuoka University, Japan, 3Mie University, Japan

Water vapor flux in the lower troposphere controls the occurrence of heavy rain in the Bai-u season. The strong wind as well as enough humidity is essential to enhance the flux. We analyzed the remarkable south-westerly strong wind zones whose maxima are present below 900 hPa over the central East China Sea during the Bai-u season. Our definition of a “strong wind zone” is that the maximum wind speed within the layer below 900 hPa is greater than 15 ms-1 and the wind speed decrease is larger than 3 ms-1 from the 900-hPa level up to the 700-hPa level. The zones have a maximum occurrence rate from the end of June to the beginning of July over the central Eastern China Sea. We focused on the events in which the geostrophic component has remarkable shear above the wind speed peak below 900-hPa. Most of them are detected far from low-pressure systems and Bai-u front and are not directly included in them. We showed that warm air advected by the rather strong westerly inherent to this season over the heated Asian continent and cold air above the ocean made the steep zonal temperature gradient, which strengthens vertical shear through the thermal wind relation. The mechanism is similar to the coastal jet resulting from the land-sea thermal contrast (e.g. Tu et al. 2018) except for the large distance (several hundred kilometers) from the continent. The occurrence rate of the strong wind zone has a maximum (minimum) at 02LT (20LT); this diurnal cycle was synchronized with the strength of the southerly ageostrophic wind near the surface reported in some previous studies. The combination of the geostrophic component produced through thermal wind relation and ageostrophic one inherent to the East China Sea produces a very strong jet structure.


AS01-A039
Impact of Ural Blocking on Sub‑seasonal Siberian Cold Anomalies Modulated by the Winter East Asian Trough

Yuanyuan SONG1#+, Dehai LUO2, Fei ZHENG2, Yao YAO2
1Institute of Oceanology, Chinese Academy of Sciences, China, 2Chinese Academy of Sciences, China

This paper examines the impact of Ural blocking (UB) on winter sub-seasonal Siberian cold anomalies under the different background conditions of the winter East Asian trough (EAT). It is found that the meridional displacement and the strength of the winter EAT possibly modulate the persistence or lifetime of UB and associated sub-seasonal cold anomalies over Siberia through changing background circulation conditions. Statistical analysis reveals that UB events tend to occur more frequently in strong or southward EAT winters than in weak or northward EAT winters. A composite analysis of UB events further shows that UB has larger amplitude and longer lifetime in strong or southward EAT winters (especially the latter) than in weak or northward EAT winters, thus more likely leading to stronger sub-seasonal cold anomalies over Siberia. Moreover, the possible physical cause of why a strong or southward EAT favors UB is further investigated. It is found that winter zonal wind and meridional gradient of potential vorticity (PVy) tend to be weakened on the upstream side of Siberia near the Ural Mountains when the EAT is stronger or located more southward, favoring the maintenance of UB due to the strengthening (weakening) of the nonlinearity (energy dispersion) of UB. In contrast, when the EAT is weak or northward-displaced, a strengthening of winter zonal wind and PVy is more likely seen over the Ural Mountains and adjacent regions, which may suppress UB through enhancing its energy dispersion and reducing its nonlinearity.


AS01-A048
Characteristics of Atmospheric Circulation Patterns Associated with the Long-duration of Heat Waves in South Korea

Minjeong CHO+, Ha-Rim KIM, Yong-Sang CHOI#
Ewha Womans University, Korea, South

Global warming has contributed to the recent increase in heat waves, which have become more intense, frequent, and longer lasting. Furthermore, heat waves that last for a longer period of duration are more likely to cause socioeconomic damage. Therefore, to understand how heat waves are sustained, it is imperative to identify and predict their mechanisms. In this study, we categorized the summer heat waves in South Korea into two categories based on their duration: short-duration events (5-7 days) and long-duration events (≥16 days). Following that, we examined the associated atmospheric circulation patterns pertaining to the persistence of summer heat waves (June through August from 1973 to 2022) using local and synoptic atmospheric variables obtained from the JRA-55 dataset. During both events, South Korea’s upper and lower atmospheres are dominated by high-pressure anomalies, with weakened jet streams, sinking motion, and suppressed convection. In short-duration events, there is a predominant meridional wave propagation with low-pressure anomalies in the Russian region of Siberia. Compared to short-duration events, long-duration events are related to strong and zonally extended high-pressure anomalies in the southern region of the Kamchatka Peninsula, which have suppressed the movement of anticyclones, thereby prolonging the duration of heat waves. Long-duration of heat waves in South Korea may be linked with persistent anomalies in mid-latitude induced by changes in stationary waves with global warming. As a result of this study, we will be able to improve our understanding of how summer heat waves persist, as well as be able to diagnose and predict heat waves in the future.


AS01-A056
Synergistic Roles of La Niña and Tibetan Plateau Warming in the Extreme Southeast China Drought in Winter 2020/21

Zhuoyu ZENG+, Ziqian WANG#, Song YANG
Sun Yat-sen University, China

In the winter of 2020/21, an extreme and long-lasting drought affected Southeast China (SEC), exerting significant social and economic impacts. In this study, the synergistic effects of La Niña and Tibetan Plateau (TP) warming on the drought are emphasized. Moisture budget analysis reveals that the drought was mainly attributed to the negative anomalies in horizontal and vertical moisture advections, namely the weakened atmospheric dynamic processes. The negative anomalies in horizontal moisture advection were previously claimed to be caused by La Niña events, as noticed by previous studies; however, the La Niña in 2020/21 presented as a cold tongue mode that induced more westward-extended Walker circulation and significant convection suppression over the western equatorial Pacific. Compared to the canonical La Niña events, warmer sea surface and stronger cyclonic anomaly occurred in the western North Pacific, inducing stronger northeasterlies and negative horizontal moisture advection anomalies over the SEC region. On the other hand, significant warming appeared over the TP in winter 2020/21, and it consequently enhanced the tropospheric meridional temperature gradient and further accelerated the westerly jet stream. The accelerated westerlies over the TP led to air accumulation and sinking motions in the downstream region, weakening the vertical moisture advection and being unfavorable for heavy precipitation in the SEC region. We highlight that, besides the La Niña event, the abnormal TP warming played a synergistic role in the extreme SEC drought in winter 2020/21. This multifactorial mechanism deepens our understanding of the drought formation and potentially improves the prediction of extremes in SEC.


AS01-A069
Impacts of Regional SST Warming on the Western North Pacific Under Global Warming

Chao-An CHEN1#+, Huang-Hsiung HSU2, Hsin-Chien LIANG2, Yu-Len CHEN2, Ping-Gin CHIU3, Chia-Ying TU2
1National Science and Technology Center for Disaster Reduction, Taiwan, 2Academia Sinica, Taiwan, 3University of Bergen, Norway

The Western North Pacific (WNP) area is the main precipitation region with energetic typhoon activity in the boreal summer. A decreased precipitation and anomalous anticyclonic circulation in the WNP region are shown in the high-resolution atmospheric model (HiRAM) global warming simulation (RCP8.5_Ens). This study conducts a series of sensitivity experiments with various patterns of regional sea surface temperature warming (SST’spa) to explore the causes of the projected changes in the WNP in HiRAM. A slightly decreased precipitation and enhanced anticyclonic circulation in the WNP can be reproduced in experiments with 2-degree uniform warming, the spatial pattern of SST warming, warming over the Tropics, and the warming from greenhouse gases emission. More identifiable changes are shown in cases with Tropical Atlantic warming, the Tropical Indian Ocean, and the Pacific meridional mode-like pattern. These experiments, to some extent, reproduce the WNP response in HiRAM RCP8.5_Ens, indicating that most SST’spa can lead to decreased precipitation and enhanced WNP subtropical high. That might be because SST’spa reduces the spatial contrast of SST climatological distribution. On the contrary, the SST warming in WNP shows the opposite response to RCP8.5_Ens, revealing more precipitation and anomalous cyclonic circulation in the WNP. Contrasted responses are also detected in typhoon activity changes. The warming over the tropical eastern Pacific also generates an anomalous cyclonic circulation. These findings indicate that the forcing from remote SST warming has a more decisive influence in the WNP region than in situ warming, implying a high probability of decreased precipitation and enhanced subtropical high in WNP in the warmer future.


AS01-A070
Tropical Stratospheric Forcings Weaken the Response of the East Asian Winter Temperature to ENSO

Ruhua ZHANG1+, Wen ZHOU1#, Wenshou TIAN2, Yue ZHANG1
1Fudan University, China, 2Lanzhou University, China

The El Niño–Southern Oscillation (ENSO) plays a critical role in predicting the winter surface temperature over East Asia. Numerous studies have attempted to improve the seasonal forecasting skill in view of the combined effects of ENSO and oceanic–tropospheric factors. However, high uncertainty and notable challenges still exist in using the ENSO to predict the surface temperature. Here, we showed that tropical stratospheric forcings (Quasi-Biennial Oscillation, QBO) could disrupt the response of the surface temperature to ENSO. The response of the East Asian surface temperature to El Niño/La Niña events evidently weakened in winter during the westerly/easterly phase of the QBO. This disruption has shown an increasing trend in recent decades, limiting the usefulness of ENSO alone as a seasonal predictor of the surface temperature. The modulation of the QBO on the East Asian surface temperature is achieved mainly by affecting subtropical zonal winds and North Pacific wave activity. Our analyses suggest that the QBO is a nonnegligible predictor in improving seasonal forecasts of the East Asian surface temperature.


AS01-A071
Influence of Scandinavian Teleconnection Pattern on Summer Precipitation Over the Eastern Side of the Tibetan Plateau

Quan-Liang CHEN#+
Chengdu University of Information Technology, China

This study analyzes the relationship between the Scandinavian (SCA) teleconnection pattern and summer precipitation over the eastern side of the Tibetan Plateau (ESTP) between 1960 and 2020 and further studies the underlying physical mechanism. Statistical analysis showed that there is a significant and high negative correlation coefficient (around −0.59) between ESTP summer precipitation and the SCA teleconnection pattern over the period 1960–2020. When the SCA teleconnection pattern is in its negative phase, there is a significant increase in precipitation over most of the ESTP, and vice versa. Moisture budget analysis showed that vertical moisture advection makes a larger contribution to precipitation changes related to the SCA teleconnection pattern than evaporation and horizontal moisture advection. Specifically, positive precipitation anomalies related to the SCA teleconnection pattern are dominated by the enhanced dynamic component of vertical moisture advection, which is induced mainly by the significant ascending motion over almost the whole of the ESTP region. In summer, under the effect of SCA teleconnection pattern, the abnormal westerly wind transports the mean warm air from TP to ESTP and forms an abnormal warm advection over the ESTP, resulting in a significant vertical upward motion and more summer precipitation over the ESTP. This study reveals the possible physical mechanism of the impacts of SCA teleconnection pattern on summer precipitation over the ESTP region and provides a scientific basis for ecological protection and disaster mitigation measures associated with major projects such as the Sichuan–Tibet railway and the Chengdu–Chongqing Economic Circle.


AS01-A074
Analysis of Rainfall Generation Process in East Asia by Summer Cold Wave

Kwang-Hee HAN1+, Ho-Young KU1, Hayeon NOH1, Jee-Hoon JEONG2, Baek Min KIM1#
1Pukyong National University, Korea, South, 2Chonnam National University, Korea, South

On August 8th, 2022, Seoul experienced unprecedented rainfall with a record-breaking total of 381.5 mm/day, the highest amount in 115 years. Heavy rain is a prevalent and dangerous weather phenomenon in Korea, leading to many investigations and studies on its mechanism of occurrence. However, In the Summer of 2022, the pressure system surrounding the Korean Peninsula exhibited an atypical summer pressure pattern. Therefore, this study analyzed the specifics of the pressure system in the Korean Peninsula and the Eurasian continent to uncover the factors and mechanisms behind the heavy rain in August 2022. At the surface level, high pressure increased significantly near the Ural Mountains and Lake Baikal in Siberia during the beginning of August. In terms of temperature, the analysis focused on the advection of cold air with a temperature anomaly of below -5°C from high latitudes to the northwest of the Korean Peninsula via Siberia along the flow of the high-pressure system in the lower atmosphere. And at 500 hPa, blocking was evident in the Ural. The blocking over the Eurasian continent hindered the zonal flow and amplified the meridional flow, resulting in the transport of cold air from high latitudes to East Asia through the strengthened meridional flow. The movement of cold air towards East Asia encountered the rim of the North Pacific high pressure and established a stationary front, leading to heavy rainfall. This study defined the development of a summertime cold continental high pressure affecting the mid-latitude region as a "Summer Cold Wave" (SCW) and the formation of the front caused by the SCW as a "Summer Cold Front" (SCF). Furthermore, by examining previous instances of SCW, it was discovered that the formation of Ural blocking in summer played a role in the emergence of SCW.


AS01-A078
Evaluation of Performance of Atmospheric Simulations Using Community Atmospheric General Circulation Model Over Summer Monsoon Regions

Venkatraman PRASANNA1#+, Preethi BHASKAR2, Jai-Ho OH3, Inwon KIM4
1Meteorological Service Singapore, Singapore, 2Indian Institute of Tropical Meteorology, India, 3Nano C&W, Korea, South, 4Pukyong National University, Korea, South

This study evaluates the performance of the high-resolution atmosphere general circulation model (AGCM), namely the Community Atmospheric Model (CAM) in its representation of seasonal mean, interannual variability and global teleconnections over the south Asian summer monsoon region (SAM), Western North Pacific (WNP), Equatorial Indian Ocean (EIO), Maritime Continent (MC), and West & East Pacific Ocean basin (W-PAC & E-PAC). Based on the AGCM experiment conducted for CAM model with observed SST (similar to AMIP type experiment), the model’s skill in simulating summer monsoon rainfall over different domains (SAM, WNP, EIO, MC, W-PAC & E-PAC) is low for the climate period (1981–2008). The decreased skill of the model over the south Asian monsoon region is evident, when the model is compared with the tropical mid-Pacific regions (W-PAC & E-PAC) and MC, which indicates that the impact of atmospheric dynamics is more important than SST forcing alone over the Asian monsoon regions (SAM, WNP & EIO). Our result shows that the AGCM simulation over south Asia exhibit large uncertainty in capturing the anomalies associated with the large global forcing like El Niño and La Niña. The analysis clearly brings out the presence of large systematic biases in the model simulation. The lack of air-sea interaction processes limits the skill of the model forced with SST alone over the Asian summer monsoon regions (SAM, WNP & EIO). The improved skill over the tropical mid-Pacific regions (W-PAC & E-PAC) and MC may be attributed to the strong SST forcing over the Pacific and the better representation of upward and downward limb of walker cells. While reduced skills over the Asian summer monsoon regions (SAM, WNP, EIO) may be attributed to the lack of Air-Sea Interaction and lack of dynamical feed backs from the local effects.


AS01-A088
Unprecedented Extreme Temperature Variability of Inter-/intra-monthly Timescales in East Asia During the 2022/23 Winter Season

Ho-Young KU+, Hayeon NOH, Baek Min KIM#
Pukyong National University, Korea, South

During the winter of 2022/23, East Asia experienced extreme temperature fluctuations on both inter- and intra-monthly timescales. November 2022 was warmer than normal, while December was colder than normal, with the second-highest difference in monthly temperature anomaly between the two months over the past 44 years. This regime shift in monthly time-scale can be explained by the alteration of month-long dominance of warmer air from south and cold air from north-west. The long-lasting La Niña condition over three years contributed to near record-high sea surface temperatures in the western Pacific region, affecting the warm East Asian climate until November. In December, the WACE pattern emerged over Eurasia due to the amplified warming especially in the Barents-Kara Sea causing the East Asian region to be cold climate. In January 2023, East Asia experienced abrupt regime shift from warm to cold climate within in just a few days. This event was unprecedentedly largest temperature fluctuations, dropping 12.34℃ in 12 days, observed on an intra-monthly timescale during the winter. In early to mid-January, warm and moist air intruded into East Asia from the south driven by expansion of the North Pacific High leading to above normal warm climate in East Asia. Later in mid-January, blocking occurred in the Ural region, and the meandering of the jet stream caused cold air to flow into East Asia from the north, resulting in a cold wave at the end of January. The extreme temperature fluctuations in East Asia this winter on both inter- and intra-monthly timescales are attributed to the tug-of-war between tropical and polar air masses manifested by such as WACE patterns due to arctic amplification and equatorial warm and moist air intrusion partly explained by the long-lasting La Niña condition which contributes to the intermittent expansion of North Pacific warm High.


AS01-A093
Risk Assessments of Indian Summer Monsoon Rainfall Extremes Using a Max-stable Process Based Modelling Framework

Athira K1#+, Sarmistha SINGH1, Ash ABEBE2
1Indian Institute of Technology Palakkad, India, 2Auburn University, United States

The frequent incidence of extreme precipitation in India during the Indian Summer Monsoon (ISM) season has resulted in various devastating consequences such as flash flooding, crop destruction, loss of life, and damage to infrastructure. To mitigate the potential effects of extreme rainfall, it is essential to understand its impacts across the country. In this study a Maxstable process-based model has been used to model the Spatio-temporal variability of ISM rainfall extremes and the risk associated with various return levels. In addition to the spatial factors, the impact of large-scale climatic drivers, such as the El Niño Southern Oscillation (ENSO), has also been incorporated to demonstrate its influence on the extreme precipitation field. Due to the complexity of terrain across the country, spatial clustering has been implemented. The computational efficiency was substantially improved by the implementation of parallel computing on clusters. Twenty models with different combination of spatial and temporal covariates for location, scale and shape parameters have been selected and the best fit model was identified based on Takeuchi Information Criterion (TIC) values. Results indicates that the regions have noticeable spatial variabilities extreme precipitation and around 75% of the land area in India is under the risk of heavy rainfall for more than 50-year return period. Compared to the spatial extreme models, inclusion of climatic oscillations information (ENSO) in a model framework greatly improves the suitability of the model. The results of this investigation hold significant scientific and practical implications for monitoring and managing the risks associated with extreme rainfall. They can aid in the development of appropriate mitigation strategies and inform planning efforts for potential adverse effects caused by such extreme weather events.


AS01-A100
Oxygen Isotope Variability of Rainwater, Dripwater, and Modern Calcite Respond to ENSO Based on 11 Years’ Monitoring in Yuhua Cave, Southeast China

Wanyin QIU1,2+, Xiuyang JIANG2#, Xianfeng WANG1
1Nanyang Technological University, Singapore, 2Fujian Normal University, China

The scientific explanation of speleothem δ18O in the East Asian summer monsoon (EASM) domain is a crucial issue restricting stalagmite-inferred paleoclimate research. Long-term cave monitoring is an effective solution to deal with this issue. Here, we investigate the transfer mechanism of oxygen isotopic signals from rainfall to dripwater and modern calcite, using 11-year-long cave monitoring data from Yuhua Cave, southeast China, located in the frontal zone affected by the EASM. The δ18O in the precipitation (δ18Op) shows a high response to EASM activities associated with the intertropical convergence zone (ITCZ) migrations and the activities of West Pacific Subtropical High (WPSH) affected by El Niño Southern Oscillation (ENSO) activities. Upstream convection and rainout process play a crucial role during the transmission of the ENSO signal to the δ18Op in southeastern China. Affected by the mixing effect of the epikarst reservoir, the amplitude of δ18O in dripwater (δ18Od) is much smaller than δ18Op, and there is no obvious seasonal variation. The δ18Od reflected ENSO-related δ18Op during monitoring periods, with greater amplitude. The modern calcite δ18O (δ18Oc) series show significant seasonal variations controlled by the fractionation coefficient varied with cave temperature. At the interannual scale, the δ18Oc series can inherit the δ18Od ENSO-related variations. Our results suggest that high‐resolution stalagmite δ18O reconstructions from Yuhua Cave could characterize past ENSO‐related variability in the EASM on the annual-decade scale.


AS01-A101
The Spatio-temporal Pattern of Asian Summer Monsoon During Termination II Recorded by the Chinese Stalagmite δ18O

Wei JIA1#+, Pingzhong ZHANG2, Xianfeng WANG1, Shaoneng HE1, Shufang YUAN1, Guangxin LIU3
1Nanyang Technological University, Singapore, 2Lanzhou University, China, 3Yunnan University, China

The difficulty in constraining the large-scale Asian summer monsoon (ASM) variability in the Chinese monsoon region (CMR) during Termination II lies in our poor knowledge of the western part of the CMR largely due to the sparsity of the paleoclimate records. To get a better picture of the ASM during Termination II, we examined a precisely dated stalagmite δ18O record between 133.1 and 127.0 kyr B.P. from Wanxiang Cave in western China. In combination with published δ18O data from this cave, we have identified the ‘Weak Monsoon Interval’ (WMI) in the Wanxiang δ18O record and confirmed that the severe cold event in the North Atlantic caused the weakened ASM over the CMR via reorganization of the large-scale ocean-atmospheric circulation. However, the post-WMI change in δ18O is gradual, in contrast with the abrupt shift shown in the other cave records. The rapid northward migration of the westerly jet relative to the Qinghai-Tibet Plateau is probably responsible for such discrepancy. This northward migration prevents the more 18O-depleted moisture from reaching the study site and also causes the earlier northward movement of the East Asian summer monsoon (EASM) rainband that carries positive precipitation δ18O to obscure the possible abrupt decrease in our δ18O record. After the last interglacial onset, no obvious Younger Dryas (YD)-like event was recorded in Wanxiang Cave, which suggests a minimal impact of the YD-like event on the ASM variabilities. The relatively large amplitude of δ18O variation observed in Wanxiang Cave between the late penultimate glacial and the last interglacial corresponds to a dominant control of the Indian summer monsoon (ISM), whereas smaller δ18O amplitudes were recorded in those cave sites mainly under the influence of both ISM and EASM. Therefore, the hydroclimate change over the CMR during Termination II has resulted from a combination of multiple processes.


AS01-A112
Western Himalayan Extreme Precipitation Events in High Asia Refined Analysis: Climatology and Variability

Rohtash SAINI#+, Raju ATTADA
Indian Institute of Science Education and Research Mohali, India

The hydro-meteorological climate of the Himalayas is the lifeline for the most densely populated region in South Asia. Annual floods in the Himalayan rivers often occur during the monsoon season, affecting millions of people in the Himalayas and downstream regions. The Himalayan region is extremely vulnerable to the ramifications of extreme precipitation events (EPEs), such as flash floods, landslides, and agricultural and infrastructural damages during the Indian summer monsoon (ISM). Complex terrain, high meteorological diversity and uncertainty in observations over this region make it challenging to comprehend the precipitation disparities and predict the EPEs across the Western Himalayas (WH). Therefore, a better representation of EPEs characteristics over the WH using high-resolution data is crucial for precisely understanding the precipitation variability and mechanisms of climate-triggered localised natural disasters. This study investigates EPEs using Asia's first highest resolution (10 km), a regional atmospheric reanalysis, High Asia Refined analysis version 2 (HAR v2), during ISM. HAR v2 precipitation dataset has been generated by dynamically downscaling global ERA5 reanalysis data using Weather Research and Forecasting model (WRF). Majorly, heavy rainfall over the region during the ISM occurs by convection followed by orographically locked system. The intricate interaction of regional topography with moist airflow and temperature gradient accentuates the EPEs. The present study will investigate the dynamic and thermodynamic processes associated with EPEs over the study region. Overall, this study aims to provide scientific insights to investigate the potential impacts of climate change on extreme events, which in turn could help mitigate disasters in the Himalayan region. Detailed results of precipitation variability over the Himalayas, and mechanisms altering the atmospheric conditions attributed to the EPEs will be discussed.


AS01-A114
The Importance of the Orbital Parameters for the Indian Summer Monsoon During the Mid-holocene, as Deciphered from Atmospheric Model Experiments

Charan Teja TEJAVATH1#+, Karumuri ASHOK2, Supriyo CHAKRABORTY3
1National Center for Earth Science Studies, India, 2University of Hyderabad, India, 3Indian Institute of Tropical Meteorology, India

Proxy and model-based studies suggest multi-scale temporal variability in the Indian summer monsoon (ISM). In this study, using the CESM1 atmospheric general circulation model, we carried out multiple ensemble AGCM simulations for the Mid-Holocene (MH; ≈ 6 kyr BP), Medieval Warm Period (MWP; ≈ 1 kyr BP), Little Ice Age (LIA; ≈ 0.35 kyr BP), and Historical (HS; ≈ CE 2000) periods. We used the PMIP3/CMIP5 boundary conditions for this purpose. Our simulations indicate that the ISM during the MH was stronger compared to HS and the rainfall higher, in agreement with several proxy studies. The experiments also suggest that the ISM rainfall (ISMR) was higher during MWP relative to the LIA in agreement with our earlier results from the PMIP3 models. A relatively northward migration of the ITCZ over the Indian region and strengthening of the neighboring subtropical high over the northwestern Pacific, both associated with stronger insolation associated with the obliquity and precision during the MH, seem to be important reason Indian summer monsoon during the MH.


AS01-A116
Future Indian Ocean Warming Patterns

Sahil SHARMA1,2#+, Kyung-Ja HA2, Ryohei YAMAGUCHI3, Keith RODGERS2, Axel TIMMERMANN2, Eui-Seok CHUNG4
1IBS Center for Climate Physics, Korea, South, 2Pusan National University, Korea, South, 3Japan Agency for Marine-Earth Science and Technology, Japan, 4Korea Polar Research Institute, Korea, South

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). Although the corresponding spatial temperature gradients are associated with large-scale atmospheric circulation anomalies and rainfall trends with far-reaching societal implications, little is known about the underlying physical drivers. Here, we analyze a suite of large ensemble simulations conducted with the Community Earth System Model 2 to elucidate the causes of non-uniform Indian Ocean warming. Strong negative climatological air-sea interactions in the Eastern Indian Ocean are responsible for a future weakening of the zonal equatorial sea surface temperature gradient, resulting in a slowdown of the Indian Ocean Walker circulation and the generation of southeasterly wind anomalies over the AS. These contribute to anomalous northward ocean heat transport, reduced evaporative cooling, a weakening in upper ocean vertical mixing and an enhanced AS future warming. In contrast, the projected warming in the SEIO is related to a reduction of low-cloud cover and an associated increase in shortwave radiation. Therefore, the regional character of air-sea interactions plays a key role in promoting future large-scale tropical atmospheric circulation anomalies with implications for society and ecosystems far outside the Indian Ocean realm.


AS01-A117
Can Volcanos be Linked to Extreme Monsoons in Asian Countries?

Alvin WONG1, Amitava ROY2, Wyss YIM3, Indrani ROY4#+
1Volcanoes Study Group, Hong Kong SAR, 2SmartFlow Pneumatics, United Kingdom, 3The University of Hong Kong, Hong Kong SAR, 4University College London, United Kingdom

In recent years, extreme weather events have increased and in this work, we explore whether volcanic eruptions- subaerial, submarine or mixed, may have a role in or trigger, any of these extreme events. Volcanic materials (sulphur dioxide, water vapour and aerosols) released by volcanic eruptions can be carried by the wind and transported to a long distance and can affect the regions far away from the eruption sites. Based on location, the strength of eruptions and seasonal timings, volcanos have the potential to influence and alter atmospheric and oceanic circulation too. Hence, the impact of each volcanic eruption is different. Apart from circulation fields, related mechanisms that can modulate rainfall are the reduction of solar radiation, acting as condensation nuclei and complex interaction involving clouds among others. Strong volcanic eruptions can even alter ozone distribution in the stratosphere and hence can influence stratosphere-troposphere coupling. This study using observation from satellite data and rainfall records from Hong Kong Observatory revealed that volcanic eruptions have contributed to several extreme rainfall records in Hong Kong since 1963. The 1963 Agung eruption and the 1991 Pinatubo eruption can be linked to the driest year and 11th driest year of Hong Kong respectively. On the other hand, the 1982 El Chichón eruption and the 2008 Chaitén eruption could be linked to much excess precipitation in Hong Kong, the second and sixth wettest years on record respectively. Analyses of the recent strong submarine volcanic eruption Hunga Tonga in 2021 (December) that reached its peak in 2022 January is also explored in connection to the recent extreme monsoon rainfall in some east Asian countries. Such analyses and in-depth understandings of the impact of volcanic eruptions on climate will not only provide a useful direction for volcanic risk assessment but also lead to improved regional climate prediction.


AS02-A005
The Intensification of Consecutive Three Tropical Cyclones Passing Over a Warm Ocean Eddy in the South China Sea

Xi LUO1+, Wei YANG2, Lei YANG3, Dongxiao WANG1#
1Sun Yat-sen University, China, 2Key Laboratory of South China Sea Meteorological Disaster Prevention and Mitigation of Hainan Province, China, 3Chinese Academy of Sciences, China

An extremely strong and long-lasting (more than 8 months) oceanic warm core eddy existed in the South China Sea (SCS) from February–October 2010. From July–August 2010, three tropical cyclones (TCs; TC Conson, Chanthu, and Mindulle) consecutively passed over this eddy and sustained at least 21 h. The intensity change of all three TCs reached 20 kt within 24 h when they encountered this eddy. In mid-late July, tropical cyclone heat potential (TCHP) is overall stronger in the eddy region than in its surrounding region, thus TCHP plays an important role in the intensification of TC Conson and Chanthu. It is also found that the intraseasonal oscillation (ISO) and the quasi-biweekly oscillation (QBWO) can be important in favor of the further enhancement of TCs. The TCHP is too low to favor the intensity increase of TC Mindulle in late August, 2010, but weak vertical wind shear, ISO and QBWO act as key roles in the intensification of TC Mindulle.


AS02-A021
Long-term Trend of Tropical Cyclone Rapid Intensification Over the Western North Pacific

Haeun JO#+
Ulsan National Institute of Science and Technology, Korea, South

Most strong typhoons undergo rapid intensification (RI), and it is difficult to predict them. In that sense, the analysis was conducted to understand better the trends and characteristics of the rapid intensification of tropical cyclones (RITCs) that can cause significant damage. Although it is difficult to explicitly define the rapid intensification of typhoons, generally defined as a period during which the intensification rate is greater than 15.4 m/s within 24 hours. This study used JTWC best-track data from 1982 to 2020 for the northwest Pacific. As a first result, the time series of RITCs ratio and LMI intensity shows a clear trend of increase in the autumn TC period than in the summer. In addition, the longitude of occurrence and strongest point of tropical cyclones also showed a tendency to move westward, which was evident in the autumn, especially in September. Secondly, an analysis was conducted to find the reason for the tendency of occurrence and the LMI location to be biased toward the west. When the correlations between RI genesis and LMI longitude and the various oscillation indices in the autumn period were calculated, the possibility that PDO was most likely to have an effect was found. In addition, values of sea surface temperature and tropical cyclone heat potential increased in the recent RI increase zone during the autumn TC period. This may have influenced the recent increase in the RI ratio, and further analysis of several synoptic variables will be conducted. 


AS04-A002
Aerosol High Water Content and Moderate Acidity Favorite Sulfate and Secondary Organic Aerosol Formation in Combustion-derived Soot-containing Particles

Xiaojuan HUANG#+
Fudan University, China

Fine particles pollution associated with high sulfate and secondary organic aerosol (SOA) still often occur in winter, despite efficient pollutants mitigation has been achieved in China. The fast SO2 oxidation mechanisms revealed recently are controversial but consistently recognized associating with aerosol water. Here we report that both multiphase oxidation of SO2 by N(Ⅲ) involving aged soot-containing/iron-rich particles, and aqueous hydroxymethanesulfonate formation dominated high sulfate yield in wet particles with pH of 4.0~4.5 under relative humidity >85% in wintertime of northern China. We also provide a new evidence in terms of single particles for enhanced SOA generated from combustion-derived primary organic aerosol (POA) under high humidity. High humidity benefits the water uptake of particles, and aerosol high water content buffers aerosol acidity, favorites sulfate formation and the aging of soot-containing particles, particularly facilitates the conversion of combustion-derived POA to SOA. This study highlights a co-reduction on reactive gases and particles those directly emitted from solid fuels combustion for mitigating sulfate and SOA under high humidity.


AS04-A015
Secondary Organic Aerosol Formation from Wood Burning Emissions: Contribution and Chemical Evolution

Kun LI#+, Lin DU
Shandong University, China

Organic vapors 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.


AS04-A021
Evolution of Indoor Cooking Emissions Captured by SESI-HRMS

Xue LI1#+, Sasho GLIGOROVSKI2, Jiafa ZENG3, Majda MEKIC4
1Jinan University, China, 2Chinese Academy of Sciences, China, 3University Children's Hospital Basel, China, 4Leibniz Institute for Tropospheric Research, Slovenia

Cooking emissions represent a major source of air pollution in the indoor environment and exhibit adverse health effects caused by particulate matter together with volatile organic compounds (VOCs). A multitude of unknown compounds are released during cooking, some of which play important roles as precursors of more hazardous secondary organic aerosols in indoor air. Here, we applied secondary electrospray ionization high-resolution mass spectrometry for real-time measurements of VOCs and particles from cooking peanut oil in the presence of 300 ppbv nitrogen oxides (NOx) generated by a gas stove in an indoor environment. More than 600 compounds have been found during and after cooking, including N-heterocyclic compounds, Oheterocyclic compounds, aldehydes, fatty acids, and oxidation products. Approximately 200 compounds appeared after cooking and were hence secondarily formed products. The most abundant compound was 9-oxononanoic acid (C9H16O3), which is likely the product formed during the heterogeneous hydroxyl (OH) radical oxidation of oleic acid (C18H34O2) or linoleic acid (C18H32O2). Real-time detection of an important number of organic compounds in indoor air poses a challenge to indoor air quality and models, which do not account for this extremely large range of compounds.


AS04-A022
The Combustion Conversion Coefficient for Constructing Open Biomass Burning Emission Inventory Based on Satellite FRE

Jian WU#+
China University of Geosciences, China

It is necessary to convert fire radiant energy (FRE) to biomass burning consumption by the combustion conversion coefficient, when adopting the satellite FRE to estimate the open biomass burning emission. To date, the combustion conversion coefficients are considered to be scalar constants, which ignores the influence of multiple factors during the combustion process and regional differences. This project aims to conduct a systematic analysis of combustion conversion coefficients, by the view of ground experiment measurement, satellite data verification and emission inventory improvement. Firstly, the combustion conversion coefficients of typical biomass sources in China are obtained and the effects of fuels type, combustion state, combustion scale and combustion temperature on the combustion conversion coefficient are revealed, based on the ground experiment. Then, the satellite data are used to estimate the regional combustion conversion coefficient, so as to verify the reliability of the ground experimental measurement results on the regional scale. Finally, the verified combustion conversion coefficients are applied to improve the accuracy of the emission inventory. The uncertainty of the emission inventory caused by the combustion conversion coefficient has been estimated. The research results provide a new parametric scheme for correcting the uncertainty caused by the combustion conversion coefficient and improving the accuracy of the open biomass burning emission inventory in China. 


AS04-A023
Contribution of Household Stoves to Atmospheric Ammonia and Nitrous Acid: Insights from Isotopes

Yang ZENG#+
Shandong University, China

Household stoves are widely used in developing regions for cooking and heating purposes, but they also represent a significant primary emission source of gaseous pollutants. To investigate their impact on air pollution, we collected samples of ammonia (NH3) and nitrous acid (HONO), two important reactive nitrogenous gases, from various sources including the flue gas of typical household stoves. We measured their stable nitrogen and oxygen isotopic signatures (δ15N and δ18O) to identify their sources. In a year-long case study, we found that during autumn and winter, the stable isotopic compositions of atmospheric NH3 and HONO closely matched those of stove flue gas. This suggests that household stoves play an important role in the local budgets of NH3 and HONO. These findings underscore the need for targeted interventions to address the use of household stoves in developing regions as part of broader efforts to reduce air pollution and its associated health impacts.


AS04-A025
Cases Study of 2009 Australian Black Saturday and 2003 Siberian Taiga Fires as Seen by MIPAS Instrument

Alexandra LAENG#+
Karlsruhe Institute of Technology, Germany

We investigate the effect of forest fires on aerosol and gaze composition of the stratosphere, using the interferometric measurements of MIPAS instrument, that monitored the atmosphere from to 2002 to 2012 from ENVISAT platform. Two events are analyzed: 2009 Australian Black Saturday fires and 2003 Siberian Taiga fires. The impact on the composition of CO, aerosols, H2O, ozone and temperature are analyzed and the 3-dimensional plume trajectory is reconstructed, using the data of MIPAS scientific Processor run at IMK-ASF/IAA.


AS06-A008
Towards the Next Generation Real-time Retrieval of Precipitable Water Vapor – Algorithm and Performance Evaluation

Peng SUN1#+, Kefei ZHANG1, Suqin WU1, Moufeng WAN1, Dantong ZHU2, Longjiang LI1, Minghao ZHANG1
1China University of Mining and Technology, China, 2North China University of Water Resources and Electric Power, China

As is well known, water vapor is an important greenhouse gas in the atmosphere that plays a critical role in atmospheric dynamics process. It is closely related to weather and climate phenomena that affects our daily life. Therefore, precisely determining, mapping and monitoring water vapor contents has been a vital research concentration in deepening our understanding of atmosphere and our earth’s environment. Precipitable water vapor (PWV), which measures the contents of the water vapor in the atmosphere, is an essential parameter in climate and meteorological research. Among the PWV sensing methods, Global Navigation Satellite Systems (GNSS) is characterized by its remarkable accuracy, super capacity to operate under diverse weather conditions, and high ability to deliver real-time products. This contribution focuses on the algorithm, software development, and accuracy evaluation of the real-time PWV retrievals based on GNSS precise point positioning (PPP) algorithm. First, some advanced models were developed to determine high-accuracy zenith hydrostatic delay (ZHD) and weighted mean temperature (Tm). Then, an enhanced multi-GNSS real-time PPP software was developed to calculate the zenith tropospheric delay (ZTD) over the GNSS station. Finally, an exhaustive analysis was undertaken to assess the accuracy of real-time PWVs derived from the PPP-based ZTDs. The high-accuracy real-time PWV obtained is promising for time-critical meteorological applications. Additionally, our 20-years efforts towards GNSS meteorology were also summarized in this contribution.


AS09-A003
Convective and Microphysical Characteristics of Extreme Precipitation Over the Pearl River Delta at Monsoon Coast

Yali LUO1#+, Shuting YU2, Chong WU3, Yanyu GAO4, Mingxin LI3, Dong ZHENG3, Weixin XU5
1Nanjing University of Information Science & Technology, China, 2 Ji'nan Meteorological Bureau, China, 3Chinese Academy of Meteorological Sciences, China, 4Xiong'an Atmospheric Boundary Layer Key Laboratory, China Meteorological Administration, China, 5Sun Yat-sen University, China

Using multisource data including 5-yr dual-polarization radar observations, convective and microphysical characteristics of extreme precipitation features (EPFs) over a monsoon coastal region in South China are investigated including dependence on rainfall extremity and subseasonal variations. The EPFs are sorted into three groups according to the extreme rainfall intensity: 84 – 126 mm hr-1 (ER1), 126 – 186 mm hr-1 (ER2), ≥186 mm hr-1 (ER3). The more extreme rainfall shows a notable increase and decrease in the fractions of “intense” convection (7.6%, 20.6%, 31.6%) and “weak” convection (41.3%, 22.9%, 18.9%), respectively, while that of the “moderate” convection remain about 50%. The higher rainfall extremity is accompanied by statistically significant increases in ice and liquid water contents and a slight decrease in the fraction of coalescence in liquid-phase processes. While the raindrop size distributions (RSDs) of ER1 to ER3 similarly feature a mean size larger than “maritime-like” droplets and a concentration much higher than “continental-like” raindrops, the mean size and concentration of raindrops tend to increase with the increasing rainfall extremity. During the pre-monsoon period, precipitation systems are the largest in area but their EPFs are the least frequent and have the lowest raindrop concentration, likely due to the colder, drier environment with large vertical wind shear (VWS). Onset of the summer monsoon increases the frequency and convective intensity of EPFs, leading to an increase in raindrop size, consistent with the substantial increases of CAPE and moisture during the active-monsoon period. EPFs share similar convective intensity and RSD between the post-monsoon and active-monsoon periods, although the post-monsoon EPFs are slightly less frequent and have a smaller horizontal scale related to the reduced 0–6-km VWS. EPFs associated with tropical cyclones have the weakest convective intensity but the most active warm-rain processes with the RSD being closer to the maritime regime.


AS09-A004
Synergistic Effect of El Niño and Negative Phase of North Atlantic Oscillation on Winter Precipitation in the Southeastern United States

Xinxin TANG1+, Jianping LI1#, Yazhou ZHANG1, Yanjie LI2, Sen ZHAO3
1Ocean University of China, China, 2Chinese Academy of Sciences, China, 3University of Hawaii at Manoa, United States

This study reveals that the significant increase of winter precipitation over the southeastern United States (SEUS) is associated with El Niño and negative phase of North Atlantic Oscillation (NAO-). Diagnosis of large-scale dynamics shows that El Niño and NAO- have a synergistic effect on the enhancement of transient eddies and stationary waves in the eastern Pacific, southern United States, and North Atlantic. These enhanced transient eddies are associated with subtropical jet stream acceleration and maintenance of subtropical low from the eastern Pacific to the Atlantic, influencing stronger stationary waves propagation from tropical Pacific to the SEUS and North Atlantic, and from the northwestern Atlantic to the SEUS and Pacific. This favors a positive phase of meridional dipole in geopotential height anomalies between the tropics and subtropics in the Western Hemisphere (WTSD) during the co-occurrence of El Niño and NAO-. The strong positive WTSD-like pattern, accompanied by a zonally extended and southerly shifted subtropical westerly jet, induces a northward tilted secondary circulation with ascending motion over the SEUS and Gulf of Mexico. Simultaneously, intensified trough over the SEUS promotes moisture and warm advection from the subtropical and tropical Pacific converging with cold advection from the northwestern North Atlantic in the adjacent Gulf of Mexico, which is beneficial for front and cyclone generation, and induces heavy precipitation in the SEUS. This study suggests that the synergistic effects of El Niño and NAO- help to understand the variability of winter SEUS precipitation.


AS09-A006
Differences in Hourly Heavy Rainfall Over the Southeastern Extension of the Tibetan Plateau Under the Topographic Impacts

Weihua YUAN#+
Institute of Atmospheric Physics, Chinese Academy of Sciences, China

The southeastern extension of the Tibetan Plateau (SETP) is distributed by the typical longitudinal mountains and has unique climate characteristics and significant regional differences. The diurnal cycles of rainfall amount, frequency, and intensity over the SETP in the warm seasons (May to September) were investigated using high-density hourly station rainfall data and the possible mechanisms were discussed by analyzing the ERA5 reanalysis and satellite data. The largest amounts of rainfall appeared on the southern and western margins of the SETP. Located at the southern margins of the SETP, the adjacent western (Reg_W) and eastern (Reg_E) regions presented a similar rainfall amount, frequency, and intensity, but the diurnal features of the two regions were quite different. The rainfall amount, frequency, and intensity had dominant peaks in the late afternoon in Reg_W, while in the early morning in Reg_E. A secondary peak in the early morning can be found in Reg_W. The diurnal features of the two regions were closely related with the low-level atmospheric conditions and the distribution of clouds. The enhanced convergence of the anomalous southerly winds and sufficient water vapor after midnight contributed to the nocturnal rainfall at the southern edge of the SETP. In the afternoon, the lower surface air temperature and more stable stratification in Reg_E, as compared with Reg_W, were relatively unfavorable for the occurrence of afternoon convection.


AS09-A009
Impact of the Prognostic Snow and Graupel Number Concentrations on the Simulated Precipitation

Juhee KWON+, Sun Young PARK, Kyo-Sun LIM#
Kyungpook National University, Korea, South

The Weather Research and Forecasting (WRF) Double-Moment 6-class (WDM6) microphysics scheme only predicts the number concentrations for liquid-phase hydrometeors. Even though Park and Lim (2023) recently revised the WDM6 scheme by implementing the prognostic number concentration of cloud ice, the precipitating solid-phase hydrometeors such as snow and graupel are still treated as the single-moment approach, in which only mixing ratio is prognosed. In this study, the new version of WDM6 microphysics scheme is introduced by adding the prognostic number concentrations of snow and graupel to the WDM6 (Park and Lim, 2023). Therefore, the new WDM6 scheme predicts the number concentrations of all hydrometeors. By introducing the double-moment approach for snow and graupel, several microphysical processes related to them are modified and added. The newly added processes include the processes of accretion of rain by snow, self-collection of snow, sublimation of snow and graupel, and evaporation of snow and graupel. The new scheme has been tested for four summer-precipitating (Kim et al., 2019) and seven winter-precipitating convection cases (Ko et al., 2022). The mixing ratio of snow tends to increase and that of graupel decreases in the new scheme. Both mixing ratio and number concentration of rain reduces. The new scheme improves the equitable threat score (ETS) and false alarm ratio (FAR) for eight cases and probability of detection (POD) for seven cases among 11 total cases. *This work was supported by the National Research Foundation of Korea(NRF) grant funded by the Korea government. (MSIT) (RS-2023-00208394)


AS09-A010
The New Version of Weather Research and Forecasting (WRF) Double-moment 6-class (WDM6) with the Revised Ice Microphysics

Sun Young PARK+, Kyo-Sun LIM#
Kyungpook National University, Korea, South

The Weather Research and Forecasting (WRF)-Double-Moment 6-class (WDM6) microphysics scheme treats the solid-phase hydrometeors as the single-moment approach. The scheme only predicts the mixing ratio of graupel, snow and cloud ice. In addition, each category of solid-phase hydrometeors is characterized by static parameters defining pre-defining density, diameter-mass relationship, and diameter-fall speed relationship. Previous studies have reported a considerable sensitivity of simulated precipitation systems according to these static parameters. This study revises the ice microphysics in the WDM6 scheme through the implementation of prognostic graupel density and cloud ice number concentration. The new version of WDM6 has been tested in the idealized squall line and winter-time snowfall cases. the simulations with the new WDM6 show better statistical skill scores such as Root Mean Square Error (RMSE) and Equitable Treat Score (ETS), relative to the ones with the original WDM6. It is also confirmed that the new WDM6 simulates a similar fall velocity-density relationship of graupel to the observation. More detailed analysis will be presented in the conference.* This work has been supported by the South Korean Ministry of Science and ICT (MSIT) and the National Research Foundation of Korea (NRF) (grant no.2021R1A4A1032646).


AS09-A013
A Convection‐permitting Numerical Study of Diurnal Cycles of Pre‐summer Rainfall Over Southern China

Xi LU#+
Sun Yat-sen University, China

In this study, the convection-permitting model (CPM) with 3-km horizontal resolution has been used to investigate the simulated ability on diurnal cycles of pre-summer rainfall over southern China with various subregions and rainfall systems. Compared with the observations, the model captures the peak time of nocturnal rainfall in the western inland related to the eastward-propagating rainfall system over the eastern slope of the Yungui Plateau. The simulated eastward-propagating rainfall system moves a short distance and has a short lifetime due to the weaker westerly-steering flow and southerly winds in the late night bringing less warm and moist air with the weaker upward flow of the mountain–plain solenoid circulation that is unfavorable for convection instability. Over the eastern inland, the model shows good performance on simulating the quasi-stationary rainfall system in the morning because of the high resolution of topography. However, the model cannot simulate the climatology of the secondary morning rainfall peak due to overestimation of the rainfall from noon to evening. On the other hand, the weaker simulated southwesterly winds especially on the north side of the Nanling Mountains with decreased upward movement and moisture convergence and the more stable atmospheric condition lead to the disadvantage of convective rainfall. The CPM reproduces the afternoon rainfall peak but with a lead of 2–3 hr and still cannot simulate the morning peak well over the coastal region. The main source of mode bias is the over estimation of the onshore winds in the boundary layer over the land with the reduced temperature difference between land and sea resulting in insufficient convergence in the coastal region.


AS09-A014
Characteristics and Origins of the Intraseasonal Precipitation in the Wintertime North Pacific

Jing HUANG1+, Yang ZHANG2#, Xin WANG3, Xiu-Qun YANG2, Xuejuan REN2
1South China Sea Institute of Oceanology, Chinese Academy of Sciences, China, 2Nanjing University, China, 3Chinese Academy of Sciences, China

High-resolution observations show that the intraseasonal precipitation variance accounts for 20-50% and 40-70% of the total daily precipitation variance in the wintertime western and eastern North Pacific, respectively, implying the indispensable ingredient of the intraseasonal precipitation for the hydrological cycle over the East Asia-North Pacific-North American region. In this study, using daily observational data, characteristics and origins of the intraseasonal precipitation in the wintertime western and eastern North Pacific are investigated. The changes of the intraseasonal precipitation in the western and eastern North Pacific are featured by the anomalous precipitation in the Kuroshio-Oyashio Extension (KOE) and eastern North Pacific along 30°N, respectively. The intraseasonal precipitation in the western North Pacific is associated with the migratory weather systems with anomalous anticyclone originating from Japan and the cyclone originating from Northwest Asia, accompanied with the upward draft in the KOE region. The instability conditions are different in the north and south of the KOE. The unstable static and baroclinic conditions are both responsible for the enhanced precipitation in the south of the KOE. The anomalous precipitation is mainly determined by the atmospheric baroclinic instability in the north of the KOE. The anomalous atmospheric circulations associated with the intraseasonal precipitation in the eastern North Pacific are characterized by a dipolar structure, in which the anomalous quasi-stationary cyclone in the eastern North Pacific plays a major role. The upward draft associated with the anomalous cyclone and atmospheric static instability induced by the anomalous southeasterly wind provide dynamic and instability conditions for the anomalous precipitation. Furthermore, the moisture sources of the intraseasonal precipitation in western and eastern North Pacific are both dominated by the anomalous water vapor transport by the atmospheric circulation and the change of the precipitable water.


AS09-A016
A Comparison of Precipitation Forecasts with Different Scale-aware Cumulus Parameterizations Over South Korea

Ji-Young HAN#+
Korea Institute of Atmospheric Prediction Systems, Korea, South

Scale-aware cumulus parameterizations and their precipitation forecast skill over South Korea are compared at different horizontal resolutions. A series of single-domain experiments are conducted at 3-, 9-, and 27-km spatial resolution with three different scale-aware cumulus parameterization schemes available in the Weather Research and Forecasting (WRF) Model, that is, the multiscale Kain-Fritsch scheme, the Grell-Freitas scheme, and a revised version of the simplified Arakawa-Schubert scheme developed by the KIAPS (KSAS). The results from the experiments are compared with each other and with those obtained with the cumulus parameterization scheme switched off and using conventional cumulus parameterization schemes with no scale-aware capability, particularly focusing on the contribution of parameterized convection, which is determined by the convective updraft fraction or scale-dependent parameter as a function of horizontal resolution in the scale-aware cumulus parameterization, and the short-range precipitation forecast skill over South Korea against automatic weather station rain gauge observations. Based on the results, the method of defining convective updraft fraction in the KSAS is revised to use a more physically-based method and its effect on the precipitation forecast skill at each spatial resolution is examined.


AS09-A017
Impact of Vertical Movement of Soil Liquid Water on an Extreme Precipitation Event in South China

Youyong XIE+, Huiling YUAN#
Nanjing University, China

Soil liquid water (SLW) has an important impact on near-surface soil hydro-thermodynamics and surface energy budget. A new term about vertical movement of SLW (VMSLW) was added to the soil heat conservation equation in Noah-MP coupled with WRF, and the effects of the local and upstream VMSLW on a heavy summer rainfall event during June 15-25, 2010 in South China were investigated. Results show that when precipitation intensity is ≥ 2 mm/day, the magnitude of the VMSLW term in the soil heat conservation equation is comparable to that of the original term due to soil thermal conduction. Local VMSLW (contribution rate: 5.88%) leads to high pressure anomalies in South China, which weakens precipitation and reduces the positive bias of precipitation. The upstream VMSLW (contribution rate: 9.24%) decreases water vapor transport in Indo-China Peninsula, causing reduced precipitation in South China. The modified soil heat conservation equation with the new VMSLW term improves the precipitation simulation in the coupled WRF-Noah-MP model and deepens the understanding of interactions between SLW and precipitation. 


AS11-A004
Thermal Effects on Dispersion of Secondary Inorganic Aerosols in an Urban Street Canyon

Minjoong KIM1#+, Seungyeon LEE1, Seon-Young PARK1, Jae-Jin KIM2
1Myongji University, Korea, South, 2Pukyong National University, Korea, South

The surface heating in complex urban areas affects concentration of secondary inorganic aerosol (SIA) via flow and chemical environment changes. Previous studies on heating effects on pollutants have focused on effect of dispersion change. However, the heating of buildings also affects SIA concentration via chemical environmental changes, such as reaction rate and thermodynamic equilibrium changes. Accordingly, we investigated the effect of heating, by not only flow changes but also chemical environment changes, on SIA using a coupled chemistry-computational fluid dynamics (CFD) model. We investigated the change of temperature and wind in each scenario to separately identify the effects caused by the chemistry and dynamics of thermal heating on reactive aerosols. We found that both the chemical and dynamical effects reduce SIA concentration. The effect of heating caused by chemical environment changes on SIA was 49.4% larger than that of flow changes, suggesting the importance of chemical reactions in aerosol calculations in urban microscale aerosol simulations, which are not considered in most CFD-based models. We conclude that chemical speciation and detailed aerosol chemistry calculations, including an inorganic aerosol thermodynamic equilibrium model, should be considered for accurately accounting for the effect of heating on urban areas. This work was funded by the Korea Meteorological Administration Research and Development Program under Grant KMI2021-03312.


AS11-A008
Comparison of Emission Characteristics and Treatment Technologies of VOCs in Typical Pharmaceutical Enterprises

Wang XIUYAN#+
Nankai University, China

In order to obtain VOCs emission characteristics of different products in corresponding processes of pharmaceutical industry, and evaluate the impact of different treatment technologies on VOCs emission, this study took 11 typical pharmaceutical enterprises in Zibo City, Shandong Province as the research object, collected and analyzed VOCs samples of different processes and treatment technologies. The VOCs source spectra of different emission stages were compared using the coefficient of divergences (CD) method. The total non-methane hydrocarbon (NMHC) was used to characterize the overall emission of VOCs. The emission factors of pharmaceutical industry were calculated using the measurement method. The effects of different waste gas treatment technologies on VOCs emissions were evaluated according to the purification efficiency. The results show that the average VOCs emission factor of typical enterprises A and B in Zibo pharmaceutical industry is 7.97 ± 8.21 g/kg-product, which was 1/54 of the recommended value (430 g∙kg-1) provided by literature (Ministry of Ecology and Environment of the People's Republic of China, 2014). There are significant differences in VOCs emission characteristics among different processes. After RTO treatment, the proportion of aromatic hydrocarbon species increased from 49% to 58%, while the proportion of other species decreased. However, after water spraying +UV photo-oxygenation treatment, the proportion of alkane species decreased from 75% to 69%, and the proportion of other species increased. The VOCs discharged by chemical synthesis enterprises are mainly alkanes, and the proportion of each species has almost no change after the treatment of condensation, spraying and activated carbon adsorption (CSA). Different treatment technologies have different purification efficiency for different kinds of PAMs. UV photo-oxygenation + water spray is more suitable for the removal of VOCs and odor in sewage stations, and RTO is more suitable for the removal of VOCs with higher concentration.


AS11-A010
Aqueous Aging of Secondary Organic Aerosol Coating Onto Black Carbon at an Urban Site in Southern China

Liming CAO#+, Xiaohe LI
Peking University Shenzhen Graduate School, China

Secondary organic aerosol (SOA) in the atmosphere can be formed from the gas phase precursors and evolve in the particle phase. Compared to numerous studies on gas phase oxidation of volatile organic compounds (VOCs), the evolution of OA and corresponding mechanisms in the particle phase are still unclear. In this study, a thermodenuder (TD) was coupled with both a long time-of-flight aerosol mass spectrometer (L-ToF-AMS) and a soot particle aerosol mass spectrometer (SP-AMS) at an urban site in southern China during wintertime of 2018, to explore whether there is significant difference for OA evolution on black carbon (BC) aerosols. The average mass concentration of PM1 during the sampling period was 19.5±9.5 μg m-3, with OA as the most abundant chemical components. The OA measured by L-ToF-AMS and SP-AMS both were resolved into different primary and secondary factors, with the OA factors on BC particles showed different volatilities to that on the bulk aerosol. The BC-containing organics was more aged with a higher fraction of SOA contribution (83.3%) and higher O/C (0.63) compared with bulk OA. During the aging process of OA on BC particles, the fraction of BC-containing OA in total mass increased with the decreasing of volatility and correlation with BC. The more-oxidized oxygenated OA (MO-OOA, an agent of aged SOA) exhibited a unique preference on BC particles compared to other OA components. The abundant transition metals detected on BC particles was possibly the catalyser for the transformation from less oxidized OOA (LO-OOA, an agent of fresh SOA) to MO-OOA in aerosol aqueous-phase on BC particles and thus facilitates SOA formation. More studies are needed to further explore the potential role of BC and transition metals as catalysers for OA aging and the co-benefit of BC and transition metals pollution control on SOA reduction in the atmosphere.


AS11-A014
Fine Mode Atmospheric Arsenic Concentrations Over a Semi-urban Atmosphere in Eastern Indo Gangetic Plain: Very High Exceedance Over Indian Standard

Sauryadeep MUKHERJEE1#+, Adnan QADRI2, Tarun GUPTA2, Abhijit CHATTERJEE1
1Bose Institute, India, 2Indian Institute of Technology Kanpur, India

Arsenic (As) exposure is a worldwide public health issue. Inhalation of atmospheric particulate matter enriched with As is an important exposure route. Little research has been conducted for atmospheric As, especially in Indian context. This study has been conducted over Shyamnagar (22°50’N, 88°23’E, 8masl) a semi-urban station situated in the eastern part of IGP near Kolkata metropolis for an entire year (2019). 24hr samples of fine mode aerosols (PM2.5) were collected using a 5-channel aerosol sampler on every alternate day covering all the seasons. The Energy Dispersive X-ray Fluorescence technique was used to determine As concentrations along with other trace elements in PM2.5. The major elements observed were Chlorine, Sulphur, Potassium, Silicon, Aluminum, Zinc, Iron, Sodium, Calcium, Barium, and Lead along with Arsenic. The annual mean concentration of As was found to be 381.8 ngm-3 which is more than 60 times the Indian Standard (NAAQS; 6 ngm-3). The concentrations were highest during winter (~800 ngm-3) followed by postmonsoon (~ 630 ngm-3), premonsoon (~ 160 ngm-3), and monsoon (~ 80 ngm-3). This implies the constant emission of atmospheric As throughout the year. As showed very strong correlations with Lead (Pb) throughout the year (R2 = 0.99) suggesting some continuous stationary emission sources, e.g. battery industry. Low-grade coal containing arsenates (AsO43-) can also be a source of Arsenic as they are used in local eateries and domestic cooking purposes as easily affordable fuel. Irrespective of the source, this kind of high concentration of As in the atmosphere can be of huge adverse impact from the perspective of human health for the local residents. This study draws the serious attention of the scientific community as well as policymakers for regular surveillance and action plans for such overlooked semi-urban stations.


AS11-A016
Increases of Atmospheric Oxidation Capacity and Shifts of Formation Regimes Led to Ozone Increase in China from 2016 to 2019

Shengqiang ZHU1#+, Jinlong MA1, Peng WANG2, Hongliang ZHANG1
1Fudan University, China, 2The Hong Kong Polytechnic University, China

China is infronting severe ozone (O3) pollution although particulate matter reduced significantly, causing damages to public health and ecological systems. Here we utilized the comprehensive methods of ground-level observations, satellite data, and source-oriented chemical transport model to interpret O3 variations throughout China from 2016 to 2019. A remarkably worsened trend of O3 levels has been found both by observation and simulation in these years. Our results showed that the remarkable O3 elevation was found in the NCP and YRD (maximum daily 8h average O3 ~60 ppb) with an annual increasing rate of 10%. In addition, O3 formation regimes also changes obviously in the NCP, which shifted from VOC-limited to transition regimes (4.9%) and transition to NOx-limited regimes (9.6%). The elevation of MDA8 O3 was mainly attributed to the enhanced atmospheric oxidation capacity (AOC) in above regions. Particularly, the increasing ratios of OH and HO2 radicals (major oxidants) in NCP and YRD reached to ~15% and ~5%, respectively. The comprehensive study of long-term O3 changes, formation regimes, and AOC based on a multimethod approach should be considered when designing O3 control policies.


AS11-A017
Simulation of Global Aerosol Particle Number Concentration Considering the Volatility Distribution of Organic Aerosols

Xueshun CHEN#+
Chinese Academy of Sciences, China

The contribution of organic aerosol (OA) to particle formation, mass, and number concentration is one of the major uncertainties in current climate and air quality models. In this study, a global aerosol model considering the volatility distribution of organic components was developed to simulate detailed microphysical processes of organic species and other components. The model calculates the kinetic condensation of low-volatility organic compounds and equilibrium partitioning of semi-volatile organic compounds. Using this model, the response of particle number concentration to emission change was investigated. The model results strongly suggest the important role of OA volatility distribution in particle formation and the impacts of emission change on particle number concentration over the whole globe, especially over the areas influenced by anthropogenic sources.


AS11-A018
A Numerical Study on the Impact of Air Filter Equipped in the Vehicle on the Air Quality by Using WRF-CHEM with CAPSS Dataset

Chang KIM+, Yun Haeng JOE#, Hyun-Goo KIM
Korea Institute of Energy Research, Korea, South

The relationship between air quality and the pollutants generated by vehicles is of great concern in many cities around the world. In this research, we aim to understand the interaction between these two factors and the role of air filters in mitigating air pollution. To do so, we have used a combination of the Weather Research and Forecast model with a chemistry version 3.7.1 to study the impact of anthropogenic emissions from vehicles on air quality. In our study, we have used the CAPSS, Clean Air Policy Support System dataset as the source of anthropogenic emissions. The WRF-Chem model is used to the dispersion of these pollutants in the atmosphere and then predict the impact of these emissions on air quality. The simulation was executed from April 28 00 UTC, 2020 to May 30 00 UTC, 2020. Analysis data was made by the results 7 days after simulation began. This study prescribes that the mitigation of air pollutant emissions is valid only for the road emissions. i.e., line sources. Our results show that the use of air filters in vehicles can significantly reduce the concentration of air pollutants in the atmosphere by 5%. In conclusion, our study highlights the importance of considering the interaction between air quality and air pollutants generated by vehicles when developing air quality management strategies. The results of our research demonstrate the potential benefits of using air filters in vehicles to mitigate air pollution, and provide a basis for further investigation into the impact of air pollution on public health and the environment.


AS11-A022
Quantifying the Inter-city Transport of PM2.5 Using the Michaelis-Menten Equation in the Yangtze River Delta, China

Kangjia GONG#+, Jianlin HU
Nanjing University of Information Science & Technology, China

China began implementing the Air Pollution Prevention and Control Action Plan (APPCAP) in 2013 to improve air quality. Although the concentration of particulate matter in most areas has decreased significantly, some regions have yet to reach the second-level standard of China Environmental Air Quality Standards (CAAQS), such as Beijing-Tianjin-Hebei (BTH) and Yangtze River Delta (YRD). In this study, we used a source-oriented chemical transport model to quantitatively estimate the effects of inter-city transport on fine particulate matter (PM2.5) among the 41 cities in the YRD. And use the Michaelis-Menten equation to quantify the relationship between the cumulative contribution rate and the distance between cities in the YRD region. The results show that it is more appropriate to use the Michaelis-Menten equation to indicate the relationship between the cumulative contribution rate and distance, 71% of R2 values are greater than 0.9 in six regions and four seasons. The maximum contribution of regional transport (K1) and the distance where the regional transport contribution is half of the maximum contribution (K2) are different in different regions. The average value of K1 is 73.6, which is smaller in the northern part of the YRD and higher in central Jiangsu. K2 is larger in northern Jiangsu and central and southern Zhejiang. Primary PM2.5 and secondary organic aerosols (SOA) contribute more within the YRD, with 82.9% and 88.6%. The local contribution in autumn and winter in the northern part of the YRD is lower than that in spring and summer, especially in northern Jiangsu, where it is 90.4% in summer and 53.0% in autumn and winter. K2 is larger on polluted days, which means that it will be affected by a larger range on polluted days. The results can provide a scientific basis for regional joint prevention and control in the YRD region.


AS11-A027
On the Impact of Vertical Diffusion on Mesoscale Chemistry Transport Modeling

Lei JIANG#+
Nanjing University of Information Science & Technology, China

In this study, firstly, three first-order local closure vertical diffusion schemes used in multiple mesoscale chemical transport models (CTM) were embedded in the CHIMERE CTM model and tested over a one-year simulation covering the whole of France. Three model configurations present a fair reproduction of pollutant concentrations both in urban and rural areas, indicating it is an effective way to reproduce the dispersion of pollutants in chemistry transport modeling. However, it cannot be expected to significantly improve the vertical mixing under the first-order closure scheme. Secondly, a 1.5-order turbulence kinetic energy-based eddy diffusivity closure scheme called the new eddy diffusion (NED) is implemented in CHIMERE to describe more realistic diffusion processes near the surface. A fifteen-day simulation encompassing a winter pollution episode was performed for three major cities with a horizontal resolution of 1.67 km and the first layer height at 12 m, respectively. The NED scheme improved NO2 simulations at most urban sites compared to the initial Kz diffusion scheme (IKD). Taking the root mean square error as evaluation criteria, the average improvements are 18.8%, 24.5% and 9.5% for NO2 simulation in Paris, Lyon and Bordeaux respectively. For the model performance of PM2.5 and PM10 simulations in the urban areas of Paris, the improvements are 13.5% and 19.1%, respectively. Overall, preliminary outcomes of this study are encouraging. The simulation with more sophisticated and realistic eddy viscosities are better than for IKD that is widely used in CTMs, but we need to realize that this is only a fifteen-day simulation for three cities, for further research, longer periods are needed with a greater variety of meteorological situations to prove the universality of the NED scheme.


AS11-A032
Effects of Chemical Mechanism and Meteorological Factors on the Concentration of Atmospheric Pollutants in the Megacity Beijing, China

Li YUJIE#+
Beijing Normal University, China

In order to distinguishe effects of chemical mechanism and meteorological factors in the megacity Beijing, the sensitively experiments with the third-Generation Air Quality Modelling System is designed. The modelling system consists of the meteorological model (WRF), the emissions process model (SMOKE) and the air quality model CMAQ, and the experiments focus on the megacity Beijing for one year simulation in 2018. The baseline group experiment, named CB05_AER05 experiment, choses the gas-phase chemistry module CB05 and the aerosol mechanism AERO5, while the NOOP group experiment deactivates gas-phase chemistry module and the aerosol mechanism, and standing for the only meteorological factor without the chemical mechanism in the simulation. The results indicates that: 1) the modelling system plays well performance in the megacity Beijing in 2018. The correlation coefficient(R) of the simulated PM2.5 concentration and the observation value reaches to 0.7, which the normal mean bias (NMB) is -14%~32% in the 12 National Standard Air Quality (NSAQ) observation stations in Beijing. 2) The chemical mechanism has an effect on the concentration of PM2.5 up to 135% compared to the NOOP group results, while the PM2.5 concentration in NOOP group is 43.3 ug/m3, which stands for the influencing of the meteorological factor. The influencing factors of the pollutant concentration are complex, which also proves that the atmosphere is a complex system. 3) For the photochemical species, the peak frequency of NO2 concentration in the baseline group (CB05_AER05) and the NOOP group experiments are 26.9 ppbV and 2.2 ppbV, respectively. The numerical model is a good tool to quantify the effects of chemical mechanism and meteorological factors.


AS11-A038
Evaluation of Widely Utilized Emission Inventories in India Using the WRF-Chem Model and MODIS AOD Data

Diljit NAYAK#+, Gazala Habib HABIB, Sri KOTA
Indian Institute of Technology Delhi, India

To ameliorate the substandard air quality, a comprehensive national emission database is crucial for determining the aggregate emission reductions that are necessary to conform to air quality standards. Thus, it is imperative to assess the uncertainties associated with these emission inventories. This study endeavors to evaluate the accuracy of emission inventories in replicating the satellite-observed AOD for the Indian region, and to identify the most suitable emission inventory among the available options for the common baseline year of 2015. The study contrasts four databases (three global and one regional) that furnish emission estimates for air pollutants in India, which include EDGARv5, REASv3.2, and SMoGv1. Simulations were conducted for different seasons using WRF-Chem V3.8.1. The key finding of the study is that EDGAR emerged as the best performing emission inventory among all the databases across all seasons, with an average Root Mean Square Error (RMSE) of 0.38 for the entire year.


AS11-A041
Atmospheric Chlorine Chemistry in Urban Environment

Yee Jun THAM1#+, Shichun ZOU1, Lei YAO2
1Sun Yat-sen University, China, 2Fudan University, China

Chlorine chemistry play essential roles in tropospheric physicochemical processes, such as affecting the ozone (O3) level and secondary aerosol formation. Tropospheric chlorine chemistry was initially known to be important in the marine and polar atmosphere; however, more and more recent studies have indicated that chlorine chemistry was also active in inland areas. Various of gaseous chlorine species, such as nitryl chloride (ClNO2), molecular chlorine (Cl2), hydrochloric acid (HCl) and others, have been observed to be ubiquitous in the urban atmosphere, and were linked to the influence from anthropogenic sources like coal combustion and biomass burning activities. Upon photolysis, these chlorine species can release chlorine atom, which can react with O3 rapidly. The chlorine atom can also oxidize volatile organic compounds (VOC) with a reaction rate up to two order of magnitude faster than the reaction of hydroxyl radical (OH) with VOC. Despite the importance, a full understanding of the chlorine cycling and its impacts in the atmosphere remains unclear, particularly in urban environment. Our recent findings have shown that the presence of reactive halogen compounds (such as bromine and iodine) can change our understanding on the chlorine cycling in the atmosphere. Here, we will present the vital chlorine species observations and current understanding of reactive chlorine cycling in the urban atmosphere of China, and further discuss on the future challenges of reactive chlorine chemistry.


AS11-A044
Estimation of Tail Pipe and Non-tailpipe Emissions for Seven Non-attainment Cities in the Indian State of Punjab from the Ground-based Activity Data and their Comparison with the Existing Global Emission Inventories EDGAR and ECLIPSE

Arpit KATIYAR#+, Sri KOTA
Indian Institute of Technology Delhi, India

The global emission inventories of Emission Data Base for Global Atmospheric research (EDGAR) and Evaluating the Climate and Air Quality Impacts of Short-Lived Pollutants (ECLIPSE) uses top-down approach considers the total fuel consumed or the number of vehicles registered, to estimate vehicular emissions in India. However, this might not represent the actual traffic emissions in a city. Therefore, the following study aims to estimate the vehicular emissions for the year 2019 using bottom-up approach for seven cities in Punjab, India viz. Jalandhar, Patiala, Mandi Gobindgarh, Khanna, Dera Baba Nanak, Naya Nangal and Dera Bassi. The traffic volume data for two wheelers, three wheelers, four wheelers, light commercial vehicles, heavy commercial vehicles, buses, and others (tractors etc.) were calculated at twenty-five pre-identified locations in all the cities. Jalandhar which had the maximum traffic volume data, contributes to 8.02 kt/day PM10 and 3.54 kt/day PM2.5 vehicular emissions (tail pipe and non-tail pipe emissions combined) respectively. The silt loading value observed for the seven cities lie in the range of 0.89 to 9.86 g/m2. The study also compares the total estimated vehicular emissions with EDGAR and ECLIPSE global emission inventories. This study signifies the importance of bottom-up approach for the combined vehicular emissions. It is expected to provide an insight in the scientific community on the need for developing local emission inventories to devise city specific action plans for combating the air pollution.


AS11-A048
Seasonal Variation and Health Risk Assessment of PM2.5 Bound Heavy Metals: A Field and Comparative Study of Two Indian Cities

Yash JAIN#+, Sri KOTA, Vivek KUMAR
Indian Institute of Technology Delhi, India

Air pollution, especially PM2.5, is a significant environmental health concern globally, particularly in the Indian subcontinent. A minor proportion of PM2.5 is comprised of heavy metals, that can be toxic even at low concentrations, such as Cr, Cd, As, Pb, and Ni. Scientific evidence has illustrated that these metals can accumulate in adipose tissue and the circulatory system of the human body, leading to potential adverse effects on the digestive, cardiovascular, and central nervous systems, and may also act as a co-factor in the development of other diseases. This study focuses on the seasonal variation and health risk assessment of PM2.5 bound heavy metals in two north Indian cities, Alwar and Amritsar in the states of Rajasthan and Punjab respectively. The study was conducted through a combination of field measurements and comparative analysis. PM2.5 samples were collected during summer and winter seasons in both cities and analyzed for the presence of heavy metals using ICP-MS. The health risk assessment was carried out to understand the risk associated from the exposure to PM2.5 and heavy metals to the population, particularly in terms of respiratory and cardiovascular diseases.


AS11-A049
Atmospheric Assimilation Capacity of Non-attainment City in Southern India

Manuj SHARMA1+, Suresh JAIN2,1#
1Indian Institute of Technology Tirupati, India, 2Indian Institute of Technology Delhi, India

This study evaluated the Atmospheric Assimilation Capacity (AAC) of Vijayawada city in Andhra Pradesh, India. Emission inventory of 1 × 1 km2 resolution was used to estimate the emission load of PM10, PM2.5, SO2 and NOx under the Business as Usual (BAU) and Alternative (ALT) scenarios for the year 2030 compared to the reference year 2021. Subsequently, the emission load was fed into the AERMOD view v9.7.0 dispersion model to simulate the concentration of the pollutants in various scenarios for the city sources. The study reported the city's overall emission load of PM10~5648 tonnes/day, PM2.5~2131 tonnes/day, SO2~1378 tonnes/day and highest for NOx~8912 tonnes/day. PM10, PM2.5 and SO2 emissions were projected to increase by 36%, 22% and 11%, respectively, compared to a 14% decline in NOx emission load between the reference year and BAU 2030. For ALT 2030, the simulation of control and abetment measures resulted in a 16% decline in PM10 and a 23% decline in PM2.5. Implementing progressive measures in the transportation and industrial sectors also projected a significant decrease in gaseous emission load. Annual city average projected PM10 and PM2.5 concentrations reported the exceedance of Indian National Ambient Air Quality Standards (NAAQS) that resulted in reduced AAC due to an increase of 24% and 15% concentrations under the BAU 2030 scenario. However, the stringent implementation of ALT scenarios reported a high AAC with 16%, 24% and 38% decline in PM10, PM2.5 and NOx concentration, respectively. Among urban sources, construction and road dust were the prominent contributors to the city's PM10 emission load, whereas transportation and coal-burning industries contributed significantly to PM2.5, NOx and SO2, respectively. Such measures will help improve the air quality and livability of the city.


AS11-A050
Assessment of the Impact of Meteorological and Emission Variations on Winter PM2.5 Over the North China Plain in 2018-2020

Huiyun DU#+, Xueshun CHEN, Jie LI
Chinese Academy of Sciences, China

Air quality in Beijing-Tianjin-Hebei and its surrounding regions has been significantly improved during the Three-Year Action Plan for Winning the Battle Against Air Pollution from 2018 to 2020. The effectiveness of anthropogenic emissions reduction on PM2.5 over the North China Plain remains unclear. In this study, the Nested Air Quality Model System and observations were used to quantitatively examine the contribution of meteorological and emission variations to autumn-winter (November to February) PM2.5 concentrations in Beijing and its surrounding regions from 2018 to 2020. The model reproduced the temporal evolution of atmospheric pollutants and components well. The results showed that the observed mean PM2.5 concentrations during the winter were reduced by 15% and 29% in 2019 and 2020, respectively, compared with that in 2018. In 2019, the meteorological conditions over the Beijing-Tianjin-Hebei (BTH) region were poor, causing an increase of PM2.5 by 7.6% in BTH and 11% in Beijing; therefore, the control of air pollutant emission compensated for the unfavorable influence of meteorology and emission reduction was the decisive factor for PM2.5 reduction; In 2020, the meteorological conditions were relatively favorable, and the changes in meteorological factors and emission reduction led to a decrease in PM2.5 concentration by 18.6% and 10.5%, respectively, compared to 2018. Emission reduction also contributed to decrease in nitrate, ammonium, organic matter, element carbon and precursors. This work confirmed the obvious environmental benefit of pollution control measures from 2018 to 2020.


AS11-A052
Probabilistic Assessment of Spatiotemporal Air Quality in Taiwan Using Multivariate Indicator Kriging

Cheng-Shin JANG#+
Kainan University, Taiwan

Recently, because the fine particulate matter (PM2.5) concentrations monitored in Taiwan have substantially decreased due to less long-range transport of air pollutants in East Asia and the COVID-19 pandemic outbreak, many environmental groups have suggested that Taiwan’s Environmental Protection Administration should adjust the current regulatory standard for PM2.5 to an annual average of 12 μg/m3, which would accord with that of the United States. Thus, to determine whether such a regulatory adjustment is needed, assessing air quality on the basis of spatiotemporal PM2.5 distributions is critical for establishing risk maps and maintaining human health. This study spatiotemporally characterized the air quality in Taiwan by using multivariate indicator kriging (MVIK) according to current Taiwanese and US regulatory standards for annual average PM2.5 concentrations (i.e., 15 and 12 μg/m3, respectively). First, long-term PM2.5 concentrations were statistically analyzed to determine recent stable temporal PM2.5 data. Multivariate integration was implemented using the 2019-2021 and 2020-2022 PM2.5 data. MVIK was then adopted for modeling probabilities according to the two standards. Finally, compared with PM2.5 observations, quantile estimates based on the probabilities were employed to determine the optimal classifications for establishing risk maps of different PM2.5 standards. Suitable regulatory standards for PM2.5 are discussed according to risk classification maps. The results indicated that the multivariate integration of temporal PM2.5 data used in MVIK can effectively streamline the analytic process. The multivariate integration of 3-year PM2.5 data was suitable for the assessment of adjusting a regulatory standard for annual average PM2.5. The air quality in the Central, Yunchianan, and Kaoping air quality regions was found to pose high risks to human health due to long durations of high levels of PM2.5 concentrations. Adjusting the regulatory standard of annual average PM2.5 in Taiwan to 12 μg/m3 would be inappropriate at this time.


AS11-A053
The Optical Properties and CCN Activities of Black Carbon by Mixed Atmospheric Secondary Pollutants Coating

Cheng YUAN#+, Yan MA
Nanjing University of Information Science & Technology, China

Previous lab studies have suggested that other non-BC pollutants can promote the aging of black carbon (BC). However, most of the experiments were carried out with a single component mixed with BC, and the results obtained in previous studies under simple laboratory conditions may not be applicable to atmospheric relevant conditions. Here we will use a robust experimental system to perform a laboratory simulation of the internal mixing of flame-generated BC aggregates with atmospheric-relevant secondary pollutants in a smoke chamber. The impact on BC optical properties and CCN activities from the concentration of pollutants, coating sequence, as well as relative humidity, will be investigated. Variations in particle size, mass, coating thickness, effective density, dynamic-shape-factor, chemical composition, optical properties and CCN activities were determined online by a suite of instruments. Accordingly, this study will help to attain a comprehensive and clear understanding of the effects of coatings on the morphology, optical properties and CCN activities of BC and provide a foundation for accurately predicting the radiative forcing of BC as well as its role in air pollution control and climate change.


AS11-A057
Estimations of Indirect and Direct Anthropogenic Dust Emission at the Global Scale

Junyan CHEN#+, Siyu CHEN, Jianping HUANG
Lanzhou University, China

Dust emission acts as a crucial part in the dust cycle that determines dust related processes at both regional and global scale, such as long-range transport, dry/wet deposition, and radiation forcing. However, most dust emission simulations utilizing dust emission scheme merely investigate natural dust, neglecting the contributions of anthropogenic dust induced by direct or indirect anthropogenic activities, resulting in great uncertainties in estimating dust emissions by previous numerical modelling. To comprehensively reproduce the anthropogenic dust emissions process, both “indirect” and “direct” anthropogenic dust emission schemes were constructed to simulate anthropogenic dust emissions originated from diverse kinds of source regions in the study. Results showed that using both indirect and direct anthropogenic dust emission schemes show good performance on reproducing the spatio-temporal distributions of anthropogenic dust at the global scale during 2007–2010. The natural dust sources contributed 81.0%(6.34 ± 0.31 μg m−2 s−1) of the global dust emissions and the anthropogenic contributed 19.0%(1.01 ± 0.07 μg m−2 s−1) of the residual. The anthropogenic dust emissions concentrate in semi-arid, semi-humid and humid regions and generally fluctuated between 0.1 and 10 μg m2 s−1. Anthropogenic dust accounted for about 42.99% of the total dust emission in the semi-arid areas. In semi-humid and humid areas, represented by cities, direct anthropogenic dust emissions are much higher in developing regions than in developed regions. This study provides a basis for accurately estimating dust emissions, further studying the radiation forcing and climate effects of dust.


AS11-A059
The Nord Stream Pipeline Gas Leaks Released Approximately 220,000 Tonnes of Methane Into the Atmosphere

Mengwei JIA#+, Fei JIANG, Fei LI
Nanjing University, China

Sudden mega natural gas leaks of two Nord Stream pipelines in the Baltic Sea (Denmark) occurred from late September to early October 2022, releasing large amounts of methane into the atmosphere. We inferred the methane emissions of this event based on surface in situ observations using two inversion methods and two meteorological reanalysis datasets, supplemented with satellite-based observations. We concluded that approximately 220 ± 30 Gg of methane was released from September 26 to October 1, 2022. This figure is about 0.08% and 85% of global and Danish annual anthropogenic methane emissions, respectively, and comparable to the annual anthropogenic methane emission in Austria. It surpasses the Aliso Canyon gas leak (100 Gg) that occurred in California in 2015, making the Nord Stream leak the largest gas leak ever reported.


AS11-A060
Observations of NOx, O3, CO, VOCs, and PM in an Urban Region in Taiwan During the Chinese New Year

Jonalyn MADRIAGA1,2#+, Charles CHOU1, Tse-Tsung HO1
1Academia Sinica, Taiwan, 2National Central University, Taiwan

Air quality especially in urban regions is known to be highly influenced by anthropogenic activities (e.g. vehicle engine combustion, industrial processes, solvent use, etc.). The Chinese New Year (CNY) is a well-celebrated festivity in Taiwan and anthropogenic behavior in the region changes during this time - people are on holiday vacation, there is a probable decrease in manufacturing operations, and some people celebrate it with fireworks and firecrackers. In this study, we investigated the effect of CNY on the air quality in the region particularly in terms of VOCs, PM, NOx, CO, and O3. The hourly ambient measurements were done at Urban Air Pollution Research Station, Taichung City, Central Taiwan from January 9 to February 8, 2023. The sampling period was subdivided into three periods, the pre-CNY (Jan 9-19), the CNY (Jan 20-29), and the post-CNY (Jan 30- Feb 8). Results showed a significant decrease in the concentrations of the measured CO and VOCs particularly of benzene, toluene, xylene/ethylbenzene, and trimethylbenzene during the CNY period. In particular, the sum of BTX average concentrations was 11.83 ppbv, 2.60 ppbv, and 10.97 ppbv for pre-CNY, CNY, and post-CNY, respectively. PM 2.5 concentrations also showed a huge decrease during the CNY period (20.46±3.48 µg/m3) as compared to pre-CNY (27.68±14.18 µg/m3) and post-CNY (25.70±5.58 µg/m3). NOx is also found to be lowest during the CNY period (6.28±2.56 ppbv), as compared to pre-CNY (15.26 ±7.32 ppbv) and post-CNY (15.38±9.12 ppbv). CO, BTX, and NOx are known to be tracers of vehicle emissions hence the decrease can be mainly attributed to the low traffic in the area during the CNY holiday. Meanwhile, ozone concentration did not vary that much which is subject to further analysis. Diurnal variations during each period will also be investigated to further understand the observed measurements.


AS11-A062
Atmospheric Dry Deposition of N-alkanes at an Urban Site in Indo-Gangetic Plain

Shweta SINGH+, Monika J. KULSHRESTHA #
CSIR-National Physical Laboratory, India

The present study investigated the seasonal trend and source attribution of n-alkanes in dry deposition during 2021 at an urban site in Indo-Gangetic Plain i.e., Delhi. Dry deposition samples (n=30) were collected weekly on 24 hourly basis (except COVID lockdown). The samples were extracted in methanol and analyzed for n-alkanes (C21-C40) using Gas Chromatograph-Mass Spectrometer. However, only C21-C31 n-alkane homologues could be quantified in the samples. The annual average dry deposition flux of total n-alkanes was 51.5±4.5 µg/m2/day following the seasonal trend as winter (75.6, n=9) > post-monsoon (61.8, n=7) > summer (34.3, n=6) > monsoon (28.4, n=8). The seasonal variability in deposition fluxes of total n-alkanes was more pronounced during winter and post-monsoon due to higher emissions arising from burning of woods for domestic heating and biomass burning respectively. The micrometeorology of the region also aids to the formation of shallow planetary boundary layer resulting in accumulation of the pollutants during this period. The drastic decline in the average dry deposition flux of total n-alkanes during summer could be due to volatilization of the n-alkanes at high temperature during summer season. The minimum deposition flux of total n-alkanes during monsoon provides the insights on the wet scavenging of the atmospheric pollutants. The molecular distribution of ≤C25 n-alkane homologues with maxima at C23 and C25 indicates the signature for vehicular emissions while the odd-even predominance of the >C27 n-alkanes homologues with maxima at C29 suggests the prevalence of biogenic sources. The annual CPI value (1.9±0.1) confirms the presence of mixed emission sources coming from fossil fuel burning and biogenic emissions at the sampling site. Concentration Weighted Trajectory (CWT) showed the prevalence of long-range transport from Arabian, Gulf, Myanmar and Indo-Gangetic Plains during summer and monsoon while prominent local and regional sources during winter and post-monsoon seasons.


AS12-A002
Eastward Propagating Planetary Waves Observed Using the SuperDARN Meteor Radar Network

Patrick ESPY1,2#+, Tina MIRZAAMIN1, Yvan ORSOLINI3, Christian RHODES4
1Norwegian University of Science and Technology, Norway, 2University of Bergen, Norway, 3Norwegian Institute for Air Research, Norway, 4Naval Research Laboratory, Space Science Division, United States

The SuperDARN network of meteor radars near 60o N have been used in a number of studies to characterize the climatology of planetary waves (PW) in the mesosphere and lower thermosphere (MLT). Classically, planetary waves are considered to propagate westward relative to the background flow due to planetary vorticity. However, instabilities in the zonal-mean flow produce vorticity gradients that provide a rich spectrum of PWs generated in-situ in stratosphere and mesosphere, including eastward propagating PW. Such instabilities are generally associated with sudden stratospheric warming (SSW) events, and eastward propagating planetary waves (EPW) have typically been associated with SSW. Here we present both super-posed epoch analyses of EPW during SSW as well as an extensive climatology of EPW during winter seasons from 2007 to 2019 using the SuperDARN meteor network. The details of the analysis to extract the EPW will be presented as well as the results showing that while EPW do occur during SSW events, their presence in the MLT is ubiquitous throughout the winter season.


AS12-A008
Particle Precipitation Effects on the Global Secondary Ozone Distribution

Lise E. MURBERG1, Tiril LØVSET2, Yvan ORSOLINI1, Jia JIA2,3#+, Patrick ESPY2,4, Cornelius Csar Jude SALINAS5,6, Jae LEE5, Dong WU5, Jiarong ZHANG7
1Norwegian Institute for Air Research, Norway, 2Norwegian University of Science and Technology, Norway, 3Birkeland Centre for Space Science, Norway, 4University of Bergen, Norway, 5NASA Goddard Space Flight Center, United States, 6University of Maryland, Baltimore County, United States, 7Coastal Carolina University, United States

The secondary ozone layer is a global peak in ozone abundance in the upper mesosphere-lower thermosphere (UMLT) around 90-95 km. The effect of energetic particle precipitation (EPP) from geomagnetic processes on this UMLT ozone has not been well studied. In this research we investigated how the secondary ozone response to EPP from the Microwave Limb Sounder (MLS) and the Sounding of the Atmosphere using Broadband Emission Radiometry (SABER) instrument on the Aura and TIMED satellites, respectively. In addition, the Whole Atmosphere Community Climate Model with thermosphere and ionosphere extension and specified dynamics (SD-WACCM-X) was used to characterize the residual circulation during EPP events. By comparing ozone and circulation changes under High- and low-Ap conditions, we report regions of secondary ozone enhancement or deficit across low, mid and high latitudes as a result of circulation and transport changes induced by EPP.


AS12-A010
The “Keystone" Mission Concept for an Upper Atmosphere Explorer

Daniel GERBER1,2#+, John PLANE3, Franz-Josef LUEBKEN4, Patrick ESPY5,6, Christian VON SAVIGNY7, Dan MARSH3, David JACKSON8, Donal MURTAGH9, Ladislav REZAC10, Brian ELLISON1,2, Alexander VALAVANIS3, Neil BOWLES11
1UK Research and Innovation, United Kingdom, 2The Science and Technology Facilities Council-RAL Space, United Kingdom, 3University of Leeds, United Kingdom, 4Leibniz Institute of Atmospheric Physics, Germany, 5Norwegian University of Science and Technology, Norway, 6University of Bergen, Norway, 7University of Greifswald, Germany, 8Met Office, United Kingdom, 9Chalmers University of Technology, Sweden, 10Max Planck Institute for Solar System Research, Germany, 11University of Oxford, United Kingdom

Keystone is a mission concept for a limb sounding satellite to explore the upper mesosphere and lower thermosphere, as well as the ionosphere. Keystone was a candidate missions for the ESA Earth Explorer 11 Call (EE-11). It’s a maturation of the EE-10 and EE-9 mission concept LOCUS. In its present form Keystone comprises of three instruments: A Supra-THz radiometer, an infrared radiometer, and a UVIS spectrometer.The infrared radiometer has four channels at 15um (CO2), 9.6um (O3), 5.3um (NO), and 4.3um (CO2). The UVIS spectrometer ranges from 230nm-780nm (O, O2, O3, O+, M/Mg+, Fe/Fe+, and Temperature). These two instruments are a continuation of upper atmospheric measurements such as MIPAS, HiRDLS or SABER, and OSIRIS, SCIAMACHY or ICON/GOLD, respectively. Keystone addresses the looming gap in upper atmospheric measurements at these wavelengths. The novelty of the Keystone mission is the heterodyne Supra-THz sounder with frequencies of 770GHz (O2), 1.1THz (NO,CO), 2THz (O), 3.5THz (OH), and 4.7THz (O). The THz instrument - made possible at these very high frequencies by novel quantum cascade laser (QCL) local oscillators - will provide vertical profiles of its target species. Prime among these is the elusive atomic oxygen (O), which is the kingpin of upper atmospheric chemistry and energy balance. Atomic oxygen is the missing keystone in the interpretation of both infrared and UVIS measurements. The unique combination of the three Keystone instruments presents a strong and novel synergy. By resolving age old questions - e.g., the conundrum of the quenching rate of CO2 with O - Keystone will significantly improve our understanding of the upper mesosphere and thermosphere, the least well-known region of the atmosphere, maybe the entire planet.


AS18-A003
On the Alleged Tropical Cyclogenesis Induced by a Pre-existing Tropical Cyclone

Kenji YAMAUCHI1, Kosuke ITO2#+
1University of the Ryukyus, Japan, 2Kyoto University, Japan

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.


AS18-A006
Are You Typhoon Ready? - Typhoon Ready System -

Woo-Sik JUNG#+, Hana NA
Inje University, Korea, South

Analysing the intensity of typhoons that have affected Korea over the past ten years revealed that half of them were very strong typhoons (with a maximum wind speed of 44 m or more per second). In particular, one of the four typhoons had a maximum wind speed of more than 55 m/s, which is the superpower level newly established in 2021. As such, the typhoons affecting Korea are gradually getting stronger. The World Meteorological Organization (2021) has highlighted that the world will be exposed to risks from complex weather disasters rather than single weather disasters. In particular, weather disasters caused by typhoons are not a single phenomenon, such as strong winds, heavy rains, and tsunamis, but natural disasters that can have simultaneous adverse effects on air quality; therefore, preparation and evaluation are required. Accordingly, the National Weather Service (NWS) declared a paradigm shift for Weather-Ready Nation (WRN), an influence-based weather information service to support decision-making. This is a national strategic plan to minimise damage by acting in advance against the effects of extreme weather events (such as heavy snow, tornadoes, hurricanes, floods, and droughts). Researchers have established partnerships with the NWS WRN and AMBASSADOR and are conducting research to predict the impact of typhoons in Korea. In line with this, this study intends to establish and introduce the Typhoon-Ready System (TRS), which produces pre-disaster information (risk) on complex weather disasters associated with typhoons across Korea and in each detailed area. We believe that this system can be used as a countermeasure to the typhoon climate crisis on the Korean Peninsula. This work was supported by the National Research Foundation of Korea(NRF) grant funded by the Korea government(MSIT) (No. 2020R1F1A1068738)


AS18-A014
Increase in Tropical Cyclone Rain Rate with Translation Speed

Shifei TU1#+, Johnny CHAN2,3, Jianjun XU1, Quanjia ZHONG4, Wen ZHOU5, Yu ZHANG1
1Guangdong Ocean University, China, 2Asia-Pacific Typhoon Collaborative Research Center, China, 3City University of Hong Kong, Hong Kong SAR, 4Chinese Academy of Sciences, China, 5Fudan University, China

In general, tropical cyclone (TC) rainfall accumulation usually decreases with faster TC translation speed but increases with heavier rain rate. However, how the TC rain rate changes with translation speed is unclear. Here we show that, in all TC basins, the average TC rain rate significantly increases with translation speed. On average, the rain rate in a fast-moving TC is 24% higher than in a slow one. This difference increases with TC intensity, with category 3–5 TCs having a 42% increase while tropical depressions exhibit only a 9% increase. The increase in the average TC rain rate with translation speed is mainly caused by the TC net inflow in the lower troposphere, as well as vertical wind shear. These findings have important implications not only for a deeper understanding of rain rate changes in a translating TC but also for short-term forecasts of TC rainfall and disaster preparedness.


AS18-A018
Simulation and Projection of Tropical Cyclone Activities Over the Western North Pacific by CMIP6 HighResMIP

Yulian TANG+, Jingliang HUANGFU#, Ronghui HUANG
Chinese Academy of Sciences, China

This study assesses the relative impacts of model resolutions, tropical cyclone (TC) trackers, and ocean coupling on simulating TC climatology over the western North Pacific (WNP) based on six Coupled Model Intercomparison Project phase 6 (CMIP6) High-Resolution Model Intercomparison Project (HighResMIP) models from 1979 to 2014. The HighResMIP multimodel ensemble (MME) analysis shows that the high resolution has a higher Taylor skill score II (S2) in both temporal and spatial patterns of TC genesis frequency and accumulated cyclone energy (ACE) than the low resolution. In contrast, the TempestExtremes tracker (coupled run) results in a higher S2 in temporal patterns but a lower S2 in spatial patterns than the TRACK tracker (uncoupled run). Among the three factors, increased resolution leads to the greatest improvement in S2 in both temporal and spatial patterns. Furthermore, this study investigates the projections of future TC activity over the WNP by HighResMIP under the SSP5–8.5 scenario. Overall, HighResMIP MMEs project a decrease in the genesis frequency, track density, and ACE of all TCs, with the high-resolution, TRACK tracker, and uncoupled run showing greater magnitude. The high-resolution MMEs, using both trackers, project an increase in the genesis frequency and ACE of intense TCs in the coupled run. Moreover, TC track density and ACE show a larger poleward migration in the coupled run than in the uncoupled run, consistent with the significant surface warming in the northern WNP.


AS18-A028
Effects of Megacities on Tropical Cyclone Precipitation Over Pearl River Delta, China

Yukun YANG#+
Nanjing University, China

Land cover changes and anthropogenic emissions cause by megacities can modulate convection and precipitation of the landfalling storms. In this study, we investigate the influence of megacity (the Pearl River Delta) on Typhoon Nida (2016) using the Weather Research and Forecasting model coupling with Chemistry (WRF-Chem). By changing the landuse type and initial anthropogenic emissions, the results suggest that megacity significantly enhances rainfall in outer-rainband in downstream area of the Pearl River Delta (PRD), with the land effect more significant than anthropogenic emissions. Urban land modifies the convection in the downstream area of PRD by enhancing vertical velocity, generating more sensible heat fluxes, and further promoting ice phase microphysical processes. The effect of anthropogenic emissions becomes evident after intensifying vertical convection, accelerating the conversion of hydrometeors into precipitation and further increasing precipitation in this region.


AS18-A029
An Observational Study of Quasi-Periodic Lightning Activity in the Inner Core of Super Typhoon Hato (2017) Before Landfall

Yuanyuan XU1#+, Hao HUANG1, Qingqing LI2
1Nanjing University, China, 2Nanjing University of Information Science & Technology, China

In 2017, Super Typhoon Hato was characterized by pronounced convective asymmetries in its inner core immediately before landfall in China. Together with the asymmetric convection, quasi-periodic lightning activities occurred concurrently, with a period of approximately 3 hours. This study discussed the characteristics of short-cycle lightning activity and corresponding polarimetric quantities in the inner core of Super Typhoon Hato (2017) before its landfall. Although the strongest inner-core convection was located persistently in the downshear and downshear-left quadrants, the lightning bursts behaved quasi-periodically with a cycle of about 3 hours. The analysis revealed that wavenumber-2 vortex Rossby waves (VRWs) were present in the inner core, propagating cyclonically and intensifying downshear left. When the positive perturbation of the VRWs was coupled with the VWS-forced convective enhancement, the local convection was significantly reinforced. Moreover, the slanted updrafts intensified by the phase-locking between VRW activity and convection strengthened by VWS can invigorate the growth of graupel, probably through riming processes, and further enhance the charge separation and lightning production immediately outside the eyewall. The invigorated graupel growth accompanied by lightning outbreaks can enhance surface precipitation and more efficient warm-rain growth below the melting layer. The radar observations demonstrated that when other VRWs were excited and propagated to the left side of the shear, the abovementioned phase-locking occurred again, leading to increased volumes of graupel and updrafts near the eyewall and short-cycle lightning bursts.


AS18-A033
Track Deflection of a Tropical Cyclone Past a Mountain Range as Explored by Idealized Simulations

Po-Chen LIN#+, Ching-Yuang HUANG
National Central University, Taiwan

An idealized WRF model is used to investigate the track evolution of a tropical cyclone approaching westward at different departure positions toward an elongated mesoscale mountain (mimicking Taiwan) at different orientation angles (denoted by A0 and A90 for south-north and east-west orientations herein). The track deflection is primarily controlled by the meridional departure position as well as the ratio of the vortex size and effective terrain length (the aspect ratio, or the nondimensional vortex size). For a lengthy mountain range (A0) with the smallest aspect ratio, the cyclone track will be significantly deflected counterclockwise (northward) when the cyclone is closing to the terrain. The counterclockwise deflection ahead of the mountain is much enhanced as the aspect ratio is much larger as in A90 (a shallow mountain range). However, the counterclockwise deflection is stronger as the mountain range of A0 is rotated by 45 degrees counterclockwise rather than clockwise despite the same aspect ratio. Due to such counterclockwise paths, the tracks at later times may turn southward to the leeside of the terrain and thus clutter near the same location. When departing south of the terrain, the upstream cyclone may somewhat be deflected southward before taking a counterclockwise path (thus northward). The degree of the track deflection is also reduced by increased meridional departure and basic flow intensity. Only when the terrain blocking becomes significant as in A0, the cyclone can be deflected northward but then rapidly southward near landfall, due to the channeling effect of the induced strong northerly jet along the mountain base. The wavenumber-1 vortex flow and potential vorticity (PV) budget analysis has helped explain the track deflection that is dominated by horizontal PV advection in comparison to both vertical PV advection and differential diabatic heating that somewhat modulate the tracks in the vicinity of the mountain.


AS18-A038
Statistical Seasonal Forecasting of Tropical Cyclone Utilizing Preseason Predictors

Chak Wai LO1+, Kelvin T. F. CHAN1#, Oscar Y. W. ZHANG2, Minglin ZHENG3, Lifeng XU1
1Sun Yat-sen University, China, 2The Hong Kong University of Science and Technology, Hong Kong SAR, 3National University of Defense Technology, China

Predicting tropical cyclone activities has been a topic of great interest and research. Nonetheless, most of the existing forecast models are closed-source, and the prediction performance is fair, especially the early prediction. Therefore, we employ statistical methods to develop “simpler, more open and accurate” (compared with the existing) seasonal forecast models and build an open-source operational platform for providing seasonal forecasting service, focusing on the western North Pacific (including South China Sea, East Asia and Southeast Asia). In this conference, we will promote 3 statistical seasonal forecasting models (namely SYSU models) to predict the number of tropical storms over the western North Pacific, and number of tropical storms that could make landfall on South China and East China by every mid of May using preseason factors as the predictors.


AS18-A039
Future Changes in Tropical Cyclone Activity Over the Western North Pacific by Chlorophyll Under Global Warming

Han-Kyoung KIM1+, Jong-Yeon PARK1#, Doosun PARK2, Sang-Wook YEH3, Jong-Seong KUG4, Jun-Hyuk SON5
1Jeonbuk National University, Korea, South, 2Kyungpook National University, Korea, South, 3Hanyang University, Korea, South, 4Pohang University of Science and Technology, Korea, South, 5Korea Power Exchange, Korea, South

Chlorophyll can significantly affect climate systems through changes in atmospheric and oceanic circulation, and therefore could impact tropical cyclone (TC) activity. Here, we use future ensemble simulations performed by an Earth system model to investigate the biological feedback by future chlorophyll change on the large-scale environmental conditions that affect TCs over the western North Pacific (WNP). For this investigation, two sets of global warming simulations are conducted with activated and inactivated marine ecosystem models. Compared to the inactivated simulation, the increased chlorophyll concentration over the tropical eastern Pacific is a crucial feature in the activated simulation. The increased chlorophyll concentration over the tropical eastern Pacific strengthens the upper ocean’s stratification, inducing shoaling of the mixed layer and intensification of the equatorial upwelling. These changes lead to a La Niña-like SST warming pattern, hence intensifying Walker and local Hadley circulations. The intensified local Hadley circulation derives upper-level westerly and lower-level easterly wind anomalies in the southeastern part of the WNP (SE-WNP), resulting in a significant decrease in the vertical wind shear and a significant increase in the genesis potential index (GPI) in that region. The enhanced GPI in the SE-WNP and further TC properties are reproduced using a high-resolution atmospheric model simulation, which supports our Earth system model results. Our results can contribute to the understanding of the projection of TC activity in other basins because the tropical Pacific SST variability can influence the climate conditions in other basins. Acknowledgments: This work was supported by a National Research Foundation of Korea (NRF) grant funded by the Korean government (No. 2020R1A4A3079510).


AS18-A040
Estimation of Tropical Cyclone Intensity Based on Deep Learning Using Two Geostationary Satellite Data

Hye-Yoon JUNG1+, Il-Ju MOON2#, Dong-Hoon KIM2
1Interdisciplinary Postgraduate Program in Marine Meteorology, Korea, South, 2Jeju National University, Korea, South

One of nature's most violent and destructive occurrences, tropical cyclones (TCs) have a significant negative influence on society and the economy. Reducing TC damages requires precise TC intensity estimation and forecasting. The Geo-KOMPSAT-2A (GK2A) satellite images are used in this study to create the Convolutional Neural Network (CNN) model, which estimates the TC intensity in the western North Pacific (NWP). Given the insufficient GK2A data, the present study adapts a transfer learning technique, which uses information learned from available Communication, Ocean, and Meteorological Satellite (COMS) satellite images, to develop the model. When the two data are similar, the transfer learning technique performs well because it can enhance learning a new task by transferring knowledge from a task that has already been trained. The present CNN model based on transfer learning approaches lowered mean absolute error (MAE) by up to 27% compared to GK2A-only learning because COMS and GK2A satellite data use similar infrared channels. Our findings imply that transfer learning, combined with additional satellite data or artificial intelligence methods, will represent a significant advance in the estimation of TC intensity. Acknowledgement. This research was supported by Korea Institute of Marine Science & Technology Promotion(KIMST) funded by the Ministry of Oceans and Fisheries, Korea (20180447, Improvements of ocean prediction accuracy using numerical modeling and artificial intelligence technology) and the National Research Foundation of Korea(NRF) grant funded by the Korea government(Ministry of Science and ICT)(No. RS-2022-00144325)


AS18-A042
Utilizing a Causal Discovery to Identify Robust Tropical Cyclone Predictors Across the North Indian Ocean

Akshay kumar SAGAR1#+, Arun CHAKRABORTY1, Swadhin BEHERA2, Abhishek KUMAR1, Pankaj KUMAR1
1Indian Institute of Technology Kharagpur, India, 2Japan Agency for Marine-Earth Science and Technology, Japan

Each year, there are significant variations in both the activity of tropical cyclones (TC) and the damage they do. The reduction of wear and human loss brought on by tropical cyclones (TCs) depends heavily on the longer-term forecasting of TCs. In this study, the primary development regions and precursors responsible for the genesis and intensification of TC were identified using a Causal-network-based approach. However, there are numerous worldwide links that connect all of the severe occurrences. Therefore, using this Causal Effect Network (CEN) based algorithm, it is examined how tropical cyclone teleconnection and correlation with El Nino Southern Oscillation (ENSO), Indian Ocean Dipole (IOD), and North Atlantic Oscillation (NAO) during the satellite era (1980-2020) over the North Indian Ocean (NIO) basins. The most appropriate metric for cyclone energy is Accumulated Cyclone Energy (ACE); its correlation with the various factors is investigated. We examined the variation in TCs activity during all three phases (positive, negative, and neutral phases). The findings indicate an upward trend in ACE over the NIO region during that particular time period. The most intense cyclones last longer at this time, but they are less frequent overall. After 1997, ACE begins to change, and it continues to climb sharply. Analysis of the sea surface temperature (SST), and vertical wind shear (VWS) between 850 and 250 hPa is conducted, and it demonstrates ACE's positive changes and variability. Causal graphs show the contributing regions with a good significance level. These findings could lead to a better understanding of the teleconnections between the events in the atmosphere or the ocean, and better tropical cyclone forecasting could lessen the damage brought on by TCs and shows how other phenomena affect the different parameters.


AS18-A043
Diurnal Variations on the Initiation Time and Intensification Rate of Rapidly Intensifying Tropical Cyclones

Xinyan ZHANG#+, Weixin XU
Sun Yat-sen University, China

The outbreak of intense convection in the inner core of tropical cyclones (TCs) may promote the rapid intensification of TCs. It is well known that TC inner-core convection varies diurnally and usually peaks in the early morning. Recent studies found that TC intensification rate (INTRATE) also exhibits a diurnal cycle that is in phase with the inner-core deep convection. These studies further proposed that the nocturnally enhanced inner-core convection may simultaneously promote the TC INTRATE. However, the previously reported diurnal amplitude of INTRATE is just marginal (5-10%). It is unknown whether and how the diurnal cycle of the INTRATE varies among different TC intensifying periods. Also, whether the initial time of the TC intensification exhibits an evident diurnal signal? Based on the analysis of 30-year TC track data, this study investigates whether and how the INTRATE and initiation time of intensifying TCs vary diurnally. TC intensifying periods are classified into slowly intensifying (SI) and rapidly intensifying (RI) events. RI events last ~42 h on average, much longer than SI events. Interestingly, TC intensification including RI is the most likely to initiate at 00-06 LT. The INTRATE shows limited diurnal variations, especially for SI and RI events (amplitude of 6-8%), and the peak INTRATE time shifts from the morning in non-RI events to the late afternoon for RI events. Inner-core convection of all intensifying events maximizes in the early morning, in phase with the peak initiation time. However, the INTRATE and inner-core convection in RI TCs are diurnally out of phase, suggesting that the nocturnally enhanced inner-core convection may play a role in triggering TC intensification (e.g., RI), but not maximizing the INTRATE.


AS18-A046
Validation of Typhoon Forecasts Simulated by the Numerical Weather Prediction Models and Analysis of its Biases

Kyeong-Chan SHIN1#+, Hyun-Mi KIM2, Jung-Rim LEE1, Seong-Hee WON1, Hyun-Soo LEE1
1Korea Meteorological Administration, Korea, South, 2Korea Meteorological Administration , Korea, South

Typhoons are one of the deadliest natural disasters causing damage to human life and property so accurate forecasts of typhoons are crucial to reducing the risks. For the prediction of typhoons, forecasts from numerical weather prediction models (NWPs) are fundamental, and operational centers largely rely on NWPs. In the meantime, NWP techniques for the course and intensity of typhoons have been developed over many years, but prediction errors still exist so it is necessary to verify errors and analyze biases of the NWPs.
In this presentation, the prediction errors of the typhoon information from various kinds of NWPs were calculated compared to RSMC Tokyo's best track, and the tendencies of each NWP were analyzed for recent four years. The NWP used in the analysis were the global and ensemble models of KMA, NCEP, US Navy, ECMWF, and JMA.
As a result, DPEs show different validation scores every year due to the characteristics of typhoon phenomena. For example, there are many typhoons with unusual paths in 2021, so the accuracy is relatively low in all models. In this case, it is hard to predict both tracks and intensity so the model consensus didn't agree well. Also, the spatial distribution of biases such as along-track biases (ATBs), cross-track biases (CTBs), and biases of maximum wind speed are analyzed. NWPs tend to simulate typhoons' track leftward and slower, and intensity weaker. Moreover, some distinct biases are shown for the different regions in the western North Pacific area.


AS18-A060
The Effect of Low Salinity Water on Interaction Between Ocean and Typhoon Chaba (2016) Passing Over East China Sea

Woojin CHO#+, Jinyoung PARK, Dong-Hyun CHA
Ulsan National Institute of Science and Technology, Korea, South

The decreasing sea surface temperature with increasing latitude is one of the causes of the weakening of the intensity of typhoons moving to mid-latitudes. In 2016, the track of Typhoon Chaba passed over the East China Sea where the sea surface temperature (SST) was abnormally high; hence, Chaba maintained a relatively high intensity. The Changiang River discharge peaked in early July and gradually decreased before typhoon Chaba approached. Conversely, the salinity in the East China Sea was minimal in early August and increased. Moreover, the positive anomaly area of sea surface temperature in the East China Sea matched the negative anomaly area of sea surface salinity related to Changiang river discharge. Changiang freshwater inflow and sea surface temperature in the East China Sea had 30 days lagged positive correlation. Therefore, based on these, we determined that the increase in the East China Sea's sea surface temperature is associated with the outflow of the Changiang River. In this study, we investigated the sea surface temperature warming due to ocean stratification caused by Changiang diluted water and following typhoon-ocean interaction after warming and ocean stratification using a coupled atmosphere-ocean modeling system. The freshwater inflow caused ocean stratification in the East China Sea and formed a barrier layer, and this barrier layer inhibited the vertical mixing and energy transport between the surface and the thermocline and led to sea surface warming. As a result, the stabilized ocean structure restricted sea surface cooling induced by typhoon-forced upwelling and turbulent mixing. In conclusion, this study discovered the mechanism that maintains the intensity of TCs moving northward using ocean-atmosphere couple modeling, which may be used to improve the performance of ocean-atmosphere couple modeling in predicting the intensity of TCs.


AS18-A071
Multi-scale Characteristics of an Extreme Rain Event in Shandong Province Produced by Typhoon Lekima (2019)

Yi ZHANG#+
Nanjing University, China

Super typhoon Lekima (2019) is the 5th strongest typhoon to make landfall in mainland China since 1949. After its landfall, typhoon Lekima moved northward along the coastline, resulting in an extreme rain event in Shandong Province that makes the largest precipitation within the available meteorological records. A WRF model simulation that well produces the track and intensity of typhoon Lekima and the spatio-temporal evolution of the rainfall is used to analyze the multi-scale characteristics of the extreme rain event. Different from the typhoon precipitation occurred at low latitudes, the extreme rain event occurred in midlatitudes were influenced by the interactions of midlatitude synoptic systems and typhoon circulation, especially with five mesoscale rainbands. The midlatitude synoptic systems, mainly including the upper-tropospheric jet, the Western North Pacific Subtropical High, the mid-latitude trough, the low-level jets and typhoon Krosa (2019), allow typhoon Lekima to maintain its intensity after landfall and provide favorable kinematic, thermodynamic and moisture conditions for the heavy rainfall in Shandong. Based on the evolution of the mesoscale rainbands, the extreme rain event can be divided into three stages. The first stage can be classified as a distant rainfall, which was affected by two convective rainbands associated with boundary layer processes. The second stage had the largest precipitation, featured the formation of a frontal zone in Shandong interacting with typhoon Lekima. The third stage had weakened rainfall and was directly influenced by the spiral rainband of typhoon Lekima.


AS21-A003
Rate-dependent Hysteresis of Atlantic Meridional Overturning Circulation

Soon-Il AN1#, Hyo-Jeong KIM2, Soong-Ki KIM1+
1Yonsei University, Korea, South, 2City University of Hong Kong, Hong Kong SAR

AMOC is a typical density-driven thermocline circulation, featuring a clockwise basin-scale meridional overturning in the present climate. A freshwater hosing over a north Atlantic leads to slowing down or even collapse of AMOC, while in order to recover the typical state of AMOC, over-reduction of freshwater than that used for a collapse of AMOC is required. This indicates an existence of multiple equilibria state, which can be visualized by a hysteresis diagram showing a relationship between freshwater forcing (FWF) and AMOC intensity. Here, we explored AMOC hysteresis dependency on a frequency of FWF using a Stommel’s box model. Results showed that the abrupt transitions between typical state and collapse state were lagged as FWF changes faster. Furthermore, as the complexity of system increases, the detailed hysteresis feature was modified. Especially, the abruptness in transition during decreasing FWF phase was more distinct than that during increasing FWF phase. This asymmetric hysteresis response to FWF was attributed to nonlinear salt-advection feedback, which is mainly operating on a typical state but does not on a collapse state of AMOC.


AS21-A004
Hysteresis of ENSO Teleconnection in CO2 Removal Experiment

Su-Hyeon SHIN1#+, Soon-Il AN1, Jae-Heung PARK2, Jongsoo SHIN3, Chao LIU1
1Yonsei University, Korea, South, 2Seoul National University, Korea, South, 3Pohang University of Science and Technology, Korea, South

ENSO (El Nino – Southern Oscillation) is the most dominant mode on Earth, having tremendous impacts on nature and human society. Since the Earth’s climate is changing continuously by anthropogenic greenhouse gas emissions, understanding of the ENSO teleconnection in changing climate is needed. In this study, based on an idealized CO2 ramp-up and ramp-down climate model experiment, which increases CO2 concentration by 1% per year (ramp-up) and decreases symmetrically (ramp-down), we show how the ENSO teleconnection responds in the CO2 removal experiment and what factors induce the changes in ENSO teleconnection. ENSO teleconnection patterns in midlatitude 500hPa geopotential height anomalies show the systematic eastward-shift tendency during both the ramp-up and -down periods, and thus the ENSO teleconnection change shows significant hysteresis behavior. To investigate main cause of this hysteresis, we analyze the correlation between the changes in ENSO characteristics including standard deviation, skewness, phase shift, and its convection center, and the NINO3.4-500hPa geopotential height regression. The results reveal that the change in ENSO teleconnection in each region was correlated with the different factors. Especially, the ENSO skewness change was related to changes in ENSO teleconnections near North and South America, and the phase change in ENSO induces the change of ENSO teleconnection near Africa, the Aleutian region, and Australia. Through this study, it is expected that we could predict changes in ENSO teleconnection in each region according to changes in ENSO characteristics due to climate change.


AS21-A005
Future Projection of Arctic Sea Ice Constrained by Observed Sea Ice

Hyeonui CHOE+, Soon-Il AN#
Yonsei University, Korea, South

Arctic amplification refers the fastest warming of Arctic region due to Anthropogenic increase of greenhouse gases. The main cause of this fast warming is known as so-call ‘ice-albedo feedback’ especially associated with the reducing sea ice area over the Arctic. Therefore, in near future, the emergence of seasonal sea ice free would be expected. The prediction of sea ice free timing is challenging because of complexity in atmosphere-ocean-ice system. In particular, it is known that the fast disappearing of Arctic sea ice in early 21 centaury was not well simulated in most of the advanced climate models. Therefore, the correction of the future projection in Arctic sea ice using observations is necessary. Here, using 1979-2020 analysis data, we calibrate the present-day melting rate of Arctic sea ice of climate models participating CMIP6 and apply for the future projection. Results show that the sea ice free year obtained from this calibration is earlier than that without calibration. This study may provide more accurate information in future Arctic sea ice change.


AS21-A008
Hiatus of Near-surface Wind Speed in March Over China

Huishuang YUAN1+, Zhibo LI2, Youli CHANG1#
1Yunnan University, China, 2Peking University, China

Variability in near-surface wind speed (NSWS) has significant impact for understanding the hydrological cycle, environmental governance, and renewable energy development. Global NSWS shows the stilling and reversal phenomenon before and after 2011, but lacks the attention on the discrepancy of monthly NSWS annual changes. Our study employed daily observational data from the China Meteorological Administration to investigate changes in monthly NSWS across China. We found a consistent decline in NSWS before 2011, after which March was marked by a hiatus in increasing wind. The hiatus phenomenon was mostly attributed to the southern displacement and weakening of the East Asian subtropical jet in March, which weakened the meridional temperature gradient and decreased transient eddy activity at mid-latitudes over China. Furthermore, the decline in atmospheric baroclinity suppressed anticyclonic anomalies, leading to a breakdown in NSWS. 


AS21-A011
Hysteresis of Southern Ocean Temperature in a Carbon Dioxide Removal Scenario Through Warm Water Upwelling and Sea Ice-albedo Feedback

Jongsoo SHIN1#+, Jong-Seong KUG2, Soon-Il AN3, Jae-Heung PARK4
1Woods Hole Oceanographic Institution, United States, 2Pohang University of Science and Technology, Korea, South, 3Yonsei University, Korea, South, 4Seoul National University, Korea, South

The Southern Ocean plays a crucial role in regulating global temperature through its interactions with the atmosphere, ocean, and sea ice. However, its thermostatic impact on greenhouse gas forcing is not well understood. This study conducted idealized CO2 ramp-up and -down experiments and found that the hysteretic behavior of the air-sea interaction through declining sea ice has a substantial impact on the hysteresis of the Southern Ocean temperature. The reduced sea ice due to increased CO2 supplies heat to the ocean through the sea-ice albedo feedback. In the Weddell Sea, where a large amount of sea ice exists, the reduction in sea ice makes open water, which leads to continuous heat release from the ocean to the atmosphere, thereby raising the temperature of the atmosphere. The loss of heat at the ocean surface is supplemented by accumulated heat in the ocean subsurface during the period of increased CO2, thus inhibiting the formation of sea ice. These feedback processes keep the Southern Ocean warm for a prolonged period, suggesting that once human-induced warming starts, it may take a long time for the Southern Ocean to return to its initial state, or irreversible changes may occur. Acknowledgments: This work was supported by the National Research Foundation of Korea (NRF) grant funded by the Korea government (MSIT) (NRF-2018R1A5A1024958). The CESM simulation was carried out on the supercomputer supported by the National Center for Meteorological Supercomputer of Korea Meteorological Administration (KMA), the National Supercomputing center with supercomputing resources, associated technical support (KSC-2021-CHA-0030), and the Korea Research Environment Open NETwork (KREONET).


AS21-A012
The Relationship Between the Mass Term of Atmospheric Angular Momentum and Water Vapor Mass

Wirid BIRASTRI1,2#+, Tri Wahyu HADI1, Nining Sari NINGSIH1
1Bandung Institute of Technology, Indonesia, 2Institut Teknologi Sumatera, Indonesia

In this study, the relationship between atmospheric angular momentum's mass term (MΩ) and water vapor has been investigated using four reanalysis datasets for the years 1950–2020: ERA5, ERA-20C, JRA55, and NCEP/NCAR. The four reanalysis datasets revealed a consistent positive long-term trend in global MΩ anomalies, while also identified shifts in the trend from negative to more positive around 1970s. Meanwhile, analysis of global water vapor trends shows that there is an additional mass of water vapor, which results in variations in water vapor surface pressure (pw) of about ~0.3 mbar. Changes in the contribution of water vapor to MΩ after the 1970s were calculated based on the anomaly of MΩw (estimated from pw) relative to the climatology value of 1970-1979. It can be shown that the MΩw anomalies tend to be positive after the 1970s period. In addition, the ratio of the MΩw anomalies relative to MΩ suggests a change in the pattern of the contribution of water vapor to MΩ, which is indicated by the fluctuation of this percentage every ten years. The highest contribution of water vapor to MΩ occurred in the equatorial region during 2010-2020, with a ratio of MΩw to the global MΩ at 25-50%. The stability of the relationship between MΩ and water vapor is examined using the 20 year shifting window correlation. The relationship between MΩ and water vapor is more consistent on annual and interannual scales, especially in the equatorial region, but there are inconsistencies for longer time scales. Inconsistency in the interdecadal scale is characterized by a lower statistical coherence from the mid-1980s to the 2000s, which indicates a decrease in the contribution of water vapor to MΩ. These results suggest that water vapor alone is insufficient to account for the increase in MΩ over the period.


AS23-A013
Development of High-resolution Chemical Reanalysis System Over Northeast Asia and South Korea Based on the Korean Air Chemistry Modeling System (K_ACheMS RA)

Dogyeong LEE+, Chul Han SONG#
Gwangju Institute of Science and Technology, Korea, South

Chemical reanalysis data, produced by assimilating observations into numerical model backgrounds, can provide systematically best-estimated and spatiotemporally continuous information on atmospheric chemical components. Nowadays, the chemical reanalysis data have been actively released by several institutes such as Copernicus Atmospheric Modeling and Monitoring Service (CAMS) reanalysis from European Centre for Medium-Range Weather Forecasts (ECMWF) and Modern-Era Retrospective Analysis for Research and Applications Aerosol Reanalysis (MERRAero) from National Aeronautics and Space Administration Global Modeling and Assimilation Office (NASA-GMAO). However, because such datasets are produced by using global chemistry transport models (e.g., C-IFS and GEOS-5/GOCART), they could not be suitable for air quality studies on a regional scale due to low spatial resolutions and poor parameterizations for regional atmospheric environments. Therefore, in this study, a chemical reanalysis system has been developed based on the Korean Air Chemistry Modeling system (hereafter ‘K_ACheMS RA’) for regional air quality study over northeast Asia and South Korea with high resolutions of 15×15 km2 and 5×5 km2, respectively. The K_ACheMS RA mainly consists of the following: i) the Community Multi-scale Air Quality version 5.2.1 (CMAQ v5.2.1) model updated for atmospheric conditions over northeast Asia by Gwangju Institute of Science and Technology (GIST) science team (i.e., CMAQ vG model); ii) the Weather Research and Forecasting (WRF) model with high resolutions of topography, land cover, and forest type datasets over South Korea; and iii) an advanced data assimilation system based on an ensemble Kalman Filter (EnKF). Ground-based observations, such as PM2.5, CO, O3, NO2, and SO2 in South Korea, China, and Japan, are assimilated into the CMAQ vG model every 3 hours. The evaluations of the produced reanalysis data by comparison with AIR KOREA observations in South Korea will be shown in this presentation.


AS23-A020
Total Column Water Vapor Retrieval Over Asia From Geostationary Environment Monitoring Spectrometer (GEMS) Visible Spectra

Hyeji CHA1+, Jhoon KIM1#, Heesung CHONG2, Gonzalo GONZÁLEZ ABAD2, Dha Hyun AHN1, Sangseo PARK3, Ja-Ho KOO1, Won-Jin LEE4, Deok-Rae KIM4
1Yonsei University, Korea, South, 2Center for Astrophysics | Harvard & Smithsonian, United States, 3Ulsan National Institute of Science and Technology, Korea, South, 4National Institute of Environmental Research, Korea, South

Water vapor is one of the greenhouse gases which has strong impacts on the weather and climate. Despite of long-term observation by meteorological satellites, the physical/chemical process related to water vapor is not well understood. Therefore, continuous, accurate monitoring of atmospheric water vapor is essential for understanding its interaction with weather and climate. From this purpose, water vapor retrieval algorithm is newly developed in the visible channels (435.0 – 467.0 nm) for the Geostationary Environment Monitoring Spectrometer (GEMS) onboard the GEO-KOMPSAT 2B satellite. The algorithm is based on the direct fitting method, which is originally developed by Smithsonian Astrophysical Observatory (SAO). The GEMS Total Column Water Vapor (TCWV) algorithm conducts the two-step approach, which are comprised of spectral fitting of slant column densities (SCDs), and conversion of the retrieved SCDs to vertical column densities (VCDs) using air mass factors (AMFs). The TCWV retrieval algorithm is applied to GEMS observations for all months in 2021. The retrieval results show not only the monthly variations of water vapor but also its diurnal cycle over Asia. TCWV derived from GEMS observations are validated by comparing with AERONET precipitable water data. The results agree well with the reference data and the linear regression parameters tend to vary with time. If high quality water vapor product can be produced from this study, it is expected to improve our understanding of water vapor-related chemical and physical processes.


AS23-A021
Near-real-time PM2.5 Prediction Over East Asia Using Geostationary Aerosol Monitors of GOCI-II and Machine Learning

Jeewoo LEE#+, Jhoon KIM
Yonsei University, Korea, South

Air-suspended particulate matter under the size of 2.5 μm (PM2.5) has been known to be a potential cause of asthma and increase of mortality even when exposed in the short-term (U.S. EPA, 2019). East Asian countries, where concerns on PM2.5 has been high, have provided ground-based PM2.5 observation data, but is spatially confined to the monitoring site. To overcome this limitation, aerosol optical properties (AOPs) derived from space-borne satellites have been used to estimate PM2.5 concentrations over a broad area. In this study, we used a near-real-time random forest model with AOPs from a geostationary satellite, GEO-KOMPSAT-2B, to nowcast the ground-level PM2.5 in East Asia. Hourly AOPs of the second generation Geostationary Ocean Color Imager-II (GOCI-II) retrieved by Yonsei aerosol retrieval algorithm were used as a major input, while meteorological and atmospheric chemical composition data from numerical models, and spatially and temporally inverse-weighted PM2.5 were used as ancillary variables. AOPs of GOCI-II are provided in 2.5 km spatial resolution and 10 times hourly in the daytime, for which ancillary variables were collocated in terms of time and space. The synthetic minority over-sampling technique (SMOTE) was adopted to compensate for the low occurrences of high-PM2.5 cases. Validation against ground-based PM2.5 networks has shown a good model performance in terms of R2 and RMSE. Hourly validation yielded a high R2 in the daytime, and a higher R2 in the winter. The predicted hourly PM2.5 of this study can be used as an real-time indicator for outdoor air quality and public health.


AS23-A022
Estimating Emissions from Crop Residue Open Burning in Central China Using Statistical Models Combined with Satellite Observations

Rong LI#+
Hubei University, China

Crop residues open burning has significant adverse effects on regional air quality, climate change and human health. Accurate crop residues open burning emission inventory can provide an important basis for objective and comprehensive analysis of biomass combustion, strengthening biomass combustion control and improving air quality. In this study, based on the VIIRS 375 m thermal anomaly products, land use data and high-resolution remote sensing images of sky maps, the spatiotemporal characteristics of crop residues open burning in central China were extracted and analyzed. Based on statistical models and satellite data, the high-resolution emission inventory in central China was estimated. The results showed that the number of crop residues open burning points showed a significant downward trend from 2012 to 2020, and the number of fire points remained at a low level after 2015. The peak period of straw burning is mainly concentrated during the harvest season. However, under strict control measures, staggered burning in some areas has led to several scattered small peaks of straw burning in spring and winter. The black carbon (BC), organic carbon (OC), sulfur dioxide (SO2), nitric oxide (NOX), carbon monoxide (CO), carbon dioxide (CO2), fine particulate matter (PM2.5), coarse particulate matter (PM10), ammonia-ammonia (NH3), methane (CH4) and non-methane volatile organic compounds (NMVOC) emitted by crop residues open burning were 34.84, 149.72, 41.06, 90.11, 2640.97, 78094.91, respectively. 485.17, 481.05, 35.21, 246.38 and 499.59 Gg. Among them, the largest contributor was rice, followed by wheat, rapeseed and maize, with a contribution rate of 35.34–64.07%, 15.78–34.71%, 9.12–25.56% and 5.69–14.06%, respectively.


AS23-A023
Distribution and Trend of Surface Ozone Pollution in the South Korea

Taegyung LEE1, Ja-Ho KOO1#, Junsu GIL2, Donghee LEE1+
1Yonsei University, Korea, South, 2Korea University, Korea, South

Recently, we found that the ozone concentration in the South Korea is increasing rapidly. To examine the general pattern of this ozone increasing trend in South Korea, we conducted the Mann-Kendall trend analysis using the monthly 10th, 50th, and 90th percentile of ozone level for all monitoring sites in South Korea for the purpose to see the tendency of background, mean, and polluted cases. We used the long-term (2003-2021) observation of ozone provided from the Korea Air Quality Network Program of the National Institute of Environmental Research. There are numerous monitoring stations > 400 in South Korea, but here we only use ozone data at 122 stations, which have the large number of data enough (In case that 75% days in a year have a daily representative ozone value). As a result, we found that some spatiotemporal differences. First, ozone level in the coastal region is higher than the inland region. Second, surface ozone is highest in spring (March to May). Third, ozone peak occurs in the afternoon (14-16 local time). Fourth, all trends of 10th, 50th, and 90th percentile of ozone in whole South Korea show large increasing pattern: 0.11, 0.71, and 0.75 ppbv per year, respectively. The increasing trend of 50th and 90th percentile is significant in most of the stations. The reason of large ozone increase in coastal region will be more investigated in the future. This work was supported by the National Research Foundation of Korea(NRF) grant funded by the Korea government(MSIT) (No. 2020R1C1C1011624).


AS23-A024
The COVID-19 Lockdowns Improved Air Quality in Asia as Revealed by Observations and Model Simulations

Claire YU1#+, Mian CHIN2, Huisheng BIAN3, Qian TAN4, Peter COLARCO5, Hongbin YU6
1Richard Montgomery High School, United States, 2NASA GSFC, United States, 3University of Maryland, Baltimore County, United States, 4Bay Area Environmental Research Institute, United States, 5National Aeronautics and Space Administration, United States, 6NASA Goddard Space Flight Center, United States

When the COVID-19 pandemic emerged in 2020, numerous countries across the world went into shutdowns, which caused an absence of frequent transportation, manufacturing, and other factors considered anthropogenic, or man-made, sources of aerosol emissions. Some cities in China, notably Shanghai, went through additional shutdowns from April to June 2022. This study investigates the hypothesis that the COVID-19 lockdowns in Asia resulted in large reductions in anthropogenic emissions, which may have improved air quality. We collected both satellite and ground-based observations to examine and compare levels of aerosol optical depth (AOD) and PM2.5 during pre-pandemic climatology and in the pandemic years; AOD data was taken from the MODIS Aqua satellite and PM2.5 data of nine sites from the US Embassies and Consulates in China and India. In comparison to the pre-pandemic climatology, MODIS data clearly demonstrated significant reductions of AOD, corresponding to their individual lockdown periods. Time series of PM2.5 data revealed that PM2.5 per lockdown period reached a record low. The level of PM2.5 during the lockdown was lower than the pre-pandemic average of the same period by 30-50%, depending on location. We also used AOD and PM2.5 data from NASA GEOS model to analyze simulations of pre-pandemic climatology (2010-2019), plus two simulations in 2020: the business as usual (BAU) run with 2019 anthropogenic emissions, and the COVID run with adjusted anthropogenic emissions accounting for COVID lockdowns. The relative differences in GEOS AOD and PM2.5 between the 2020 COVID run and pre-pandemic climatology were consistent with the observations but at a smaller magnitude, suggesting that the model may have underestimated lockdown-related emission reductions. These findings show strong indication that the effects of the COVID-19 lockdowns likely have left their mark in the atmosphere, improving the air quality. 


AS23-A030
Interpretation of Daytime and Nighttime Difference in AOD Over China Based on CALIOP Observations and GEOS-Chem Simulation

Xiaodong JIANG1#+, Yi WANG2, Minghui TAO3, Lu GUI1
1China University of Geosciences, China, 2China University of Geosciences, Wuhan, China, 3The Aerospace Information Research Institute of the Chinese Academy of Sciences, China

Aerosols play a crucial role in climate change by absorbing and scattering radiation. The Cloud-Aerosol Lidar with Orthogonal Polarization (CALIOP) satellite sensor can provide aerosol extinction coefficient profile observations during daytime as well as nighttime, which helps us understand the horizontal and vertical distribution of aerosols throughout the day and night. CALIOP observes that nighttime AOD is up to ~0.2 larger than daytime during 2007-2019 over the populated North China Plain, Central China, Sichuan Basin and South China. CALIOP AOD at nighttime is significantly larger than daytime below 4 km, while the difference is much smaller above 4 km. We then use the GEOS-Chem chemical transport model to simulate aerosol distribution in 2019, the year with the largest relative CALIOP AOD difference between daytime and nighttime. The simulation results also show that nighttime AOD is greater than daytime. However, from the perspective of vertical distribution, nighttime AOD is greater than daytime only below 1 km, and nighttime and daytime AOD profiles almost coincide above 1 km. Meanwhile, the results of three sensitivity experiments show that higher relative humidity due to lower temperature at nighttime than daytime leads to hygroscopic growth enhancement, which plays a decisive role in the difference between daytime and nighttime AOD compared with the emission, chemical processes, and transport factors.


AS23-A042
Dust Emission Changes in Northern China from 2016-2029 Under SSP2-4.5 Scenario

Jianqi ZHAO+, Xiaoyan MA#, Rong TIAN
Nanjing University of Information Science & Technology, China

In this study, the WRF-Chem model is used to simulate the dust emission change in northern China from 2016-2029. We first evaluated the ability of the five dust emission parameterization schemes in WRF-Chem to simulate dust processes in the study area through real-case simulations. The evaluation indicates that among the five schemes, the Shao01 scheme performs better than the others in simulating the emission flux, the spatial pattern of source region and the spatiotemporal variation of dust mass concentration, while the Shao11 scheme fails to simulate the dust process on soils of types loam and clay loam since it omits the importance of the fully disturbed particle size distribution. Simulation based on the Shao01 scheme shows that from 2016 to 2029, the amount of dust emission in the northwestern dust source region is higher than that in the northern dust source region. In addition, differences in topography and climate lead to differences in dust emission processes and their seasonal variations in the two regions. Seasonal mean dust emission fluxes in the northwestern and northern dust source regions from 2016 to 2029 show general decreasing trends, whereas some seasons show increasing trends. The dust emission flux in the northwestern dust region shows a weak increasing trend in spring and decreasing trends in summer, autumn, and winter. The dust emission flux in the northern dust source region shows decreasing trends in spring, summer, and winter and a weak increasing trend in autumn. Variation trends of dust emission fluxes in the two regions are dominated by the near-surface wind speed, whereas the vegetation fraction, precipitation, and surface temperature have important effects on the interannual fluctuation of dust emission fluxes.


AS23-A057
Air Pollution Monitoring in Singapore Using Ground-based Observations and Satellite Data

Peng YUAN SNG1, Efthymia PAVLIDOU2#+, Santo V. SALINAS1, Fernando SANTOS1, Boon Ning CHEW3
1National University of Singapore, Singapore, 2Meteorological Service Singapore, Singapore, 3Centre for Climate Research Singapore, Singapore

Air quality in Singapore is regularly monitored by the ground-based network of NEA and reflected in a composite air quality index derived by the concentrations of PM2.5, PM10, O3, NO2, and SO2. We focus on O3, NO2, and SO2 and study emissions on days within the period 2020-2023 when high levels of these pollutants were recorded. We use ground-based observations and data from satellite instruments to assess estimates of pollutant concentration, their spatiotemporal distribution, and potential indications of interactions. Finally, we discuss on complementary use of different sources of information to support diurnal air quality monitoring and better understand the local dynamics of air pollution.


AS23-A058
Greenhouse Gases Monitoring Over the East Asia by Satellite-based Observation

Byung-il LEE1#+, Junhyung HEO1, Myoung-Hee LEE1, Yoonjae KIM2, Young-Suk OH2, Sangwon JOO2
1Korea Meteorological Administration, Korea, South, 2National Institute of Meteorological Sciences, Korea, South

Greenhouse gases emitted by humans are a major cause of global warming. The concentration of GHGs has increased rapidly compared to pre-industrial times. The world is making efforts to reduce greenhouse gases, the Korean government has also declared carbon Net-zero, and has enacted and enforced the Zero Carbon Act to achieve this. The National Meteorological Satellite Center, Korea Meteorological Administration has analyzed satellite-based greenhouse gases to monitor climate change and support government’s achievement of Net-Zero, because objectively monitoring the spatio-temporal variability of greenhouse gases is so important.
NMSC/KMA validated the accuracy of satellite-based greenhouse gas within situ and TCCON retrieved CO2 from 2014 to 2021 in Anmyeon, the South Korea which is a GAW site. Both ground- and satellite-based CO2 showed a good agreement in their increasing trends with seasonal variations. However, satellite-based CO2 observed total column appear smaller than in situ observations affected by local sources due to observe near the surface, but agree well with TCCON observed the total column. The RMSD of GOSAT, and OCO2 with in situ and TCCON is estimated about 9.78, 10.47 and 2.40, 2.11 ppmv for a 1.0 degree × 1.0 degree spatial resolution on a daily time scale from January 2014 to December 2021. The results show that satellite-based products could be used greenhouse gases monitoring, but it needs to be verified with other sites data. We will present the detailed methods and results in the conference.
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 (KMA2020-00120).


AS23-A059
Pandora Asia Network (PAN) of Status and Future Plan

Soi AHN1#+, Limseok CHANG2, Donghee KIM2
1National Institute of Environmental Research(NIER), Korea, South, 2National Institute of Environmental Research, Korea, South

 A continuous collaboration is required to combat air pollution and natural disasters in Asia. The UN General Assembly adopted resolution A/RES/74/212 on “International Day of Clean Air for blue skies” in 2019 to strengthen international cooperation at the global, regional and subregional levels in various areas related to improving air quality. In accordance with the UN resolution, the project of PAPGAPi (PAN-Asia partnership for Geospatial Air Pollution information) was launched in 2020 by Ministry of Foreign Affairs of Korea in order to establish a joint-utilization platform of environmental data through the Pandora Asia Network(PAN) and environmental satellite(GEMS) data utilization system. At present, 5 countries (Thailand, Indonesia, Mongol, Laos, Cambodia) have signed a record of discussion with KOICA to join the PAN officially, and 3 countries (Vietnam, Philippines, Bangladeshi) are awaiting government approval. In addition, it will trying to negotiate with Asian countries (Singapore, Nepal, Bhutan, India) within the GEMS area. The PAN will complete to install 20 Pandora sites until 2023 and enter into regular operation in 2023. A robust PAN operation system is essential for seamless data production and active utilization which follows. The ESC of NIER will provide an opportunity for member organizations to share PAN progress to date and discuss future directions for long-term operations and PAN groups establishment. Also, it will operate and maintain the Pandora instruments in Asia and facilitate the application of GEMS data on air pollution.


AS23-A062
Top-down Derivation of Biomass Burning Particulate Matter Emissions from Different Biomes Using Himawari Fire Radiative Power Observations in ASEAN

Phoebe JULIAN1,2#+, Efthymia PAVLIDOU1, Boon Ning CHEW3, Chee-Kiat TEO3, Zhong Yi CHIA3, Hannah NGUYEN4, Martin WOOSTER4
1Meteorological Service Singapore, Singapore, 2Nanyang Technological University, Singapore, 3Centre for Climate Research Singapore, Singapore, 4King's College London, United Kingdom

Forest fires are a common occurrence throughout the ASEAN nations, often resulting in transboundary haze incidents and degraded air quality. Emissions from fires can be retrospectively estimated following bottom-up approaches, which require information on biomass density, fraction of above-ground biomass and burnt area estimates. Top-down alternative methodologies have been developed to bypass the uncertainty of such estimates and allow for near real-time monitoring. They utilise satellite-based Fire Radiative Power (FRP) and Aerosol Optical Depth (AOD) to calculate biome-specific smoke emissions coefficients (Ce) linking FRP directly to Total Particulate Matter (TPM) emissions. We apply a Top-down methodology on Himawari-based products to utilise the high frequency and the spatial resolution of the sensor; namely, the FRP product available from EUMETSAT’s Land Surface Satellite Applications Facility, and for the first time the AOD L2 product available from JAXA. We compare the coefficients we extract with those obtained from published literature and from available global datasets. We present emission estimates for fire locations across the North and South of ASEAN during 2019-2020 and use model-derived TPM as reference to evaluate our findings. We further compare emission estimates of different biomes, in order to get insights on the impact of different fire types on haze. Finally, we discuss on the challenges and the advantages of utilising geostationary satellite products for retrospective studies and operational monitoring in the local context of Southeast Asia.


AS23-A072
Estimating the Columnar Concentrations of Black Carbon Aerosols in China Using MODIS Products

Fangwen BAO1+, Ying LI1,2#
1Southern University of Science and Technology, China, 2Southern Marine Science and Engineering Guangdong Laboratory, China

Black carbon (BC), the strongest light-absorbing particle, is believed to play substantial roles in regional air quality and global climate change. In this study, taking advantage of the high quality of Moderate Resolution Imaging Spectroradiometer (MODIS) products, we developed a new algorithm to estimate the BC columnar concentrations over China by simulating the BC and non-BC aerosol mixing states in detail. The results show that our new algorithm produces a reliable estimation of BC aerosols, in which BC columnar concentrations and their related parameters (aerosol absorption and BC surface concentration) show reasonable agreements and low biases compared with ground-based measurements. The uncertainties of BC retrievals are mainly associated with the surface and aerosol assumptions used in the algorithm, ranging from -14% to 44% at higher aerosol optical depth (AOD>0.5). The proposed algorithm can improve the capability of space-borne aerosol remote sensing by successfully distinguishing BC from other aerosols. The acquired BC columnar concentrations enable the spatial pattern of serious BC aerosol pollution over East China to be characterized, showing that it exhibits higher levels in winter. These nationwide results are beneficial for estimating BC emissions, proposing mitigation strategies for air pollution, and potentially reducing the uncertainties of climate change studies.


AS24-A002
Improving the Accuracy of O3 Prediction of CMAQ with a Random Forest Model in the Yangtze River Delta Region, China

Kaili XIONG#+, Xiaodong XIE, Jianjiong MAO, Lin HUANG, Jingyi LI, Jianlin HU
Nanjing University of Information Science & Technology, China

Due to inherent errors in the chemical transport models, inaccuracies in the input data, and simplified chemical mechanisms, ozone (O3) predictions are often biased from observations. Accurate O3 predictions can better help assess its impacts on public health and facilitate the development of effective prevention and control measures. In this study, we used a random forest (RF) model to construct a bias-correction model to correct the bias in the predictions of hourly O3 (O3-1h), daily maximum 8-h O3 (O3-Max8h), and daily maximum 1-h O3 (O3-Max1h) concentrations from the Community Multi-Scale Air Quality (CMAQ) model in the Yangtze River Delta region. The results show that the RF model successfully captures the nonlinear response relationship between O3 and its influence factors, and has an outstanding performance in correcting the bias of O3 predictions. The normalized mean biases (NMBs) of O3-1h, O3-Max8h, and O3-Max1h decrease from 15.8%, 20.0%, and 17.0.% to 0.5%, −0.8%, and 0.1%, respectively; correlation coefficients increase from 0.78, 0.90, and 0.89 to 0.94, 0.95, and 0.94, respectively. For O3-1h and O3-Max8h, the original CMAQ model shows an obvious bias in the central and southern Zhejiang region, while the RF model decreases the NMB values from 54% to −1% and 34% to −4%, respectively. The O3-1h bias is mainly caused by the bias of nitrogen dioxide (NO2). Relative humidity and temperature (T) are also important factors that lead to the bias of O3. For high O3 concentrations, the T bias and O3 observations are the major reasons for the discrepancy between the model and the observations.


AS24-A004
Clustering Analysis of 24-hour Indoor Air Quality According to Facility Types in South Korea

Sun-Kyong HUR#+, KyongTae KIM, Ju-Won LEE, Soo Joeng JOEN, Boo-Hun CHOI
Kweather, Korea, South

This study attempts to classify the timeseries pattern of indoor air quality levels which tends to be different according to facility types. Indoor air quality data are obtained from Kweather, which company uses its self-developed air quality monitors installed nationwide to collect real-time observation data. Using this data, K-mean clustering analysis derive four distinct patterns (Group A, B, C, and D) based on 24-hour timeseries of PM10, PM2.5, CO2, noise and temperature from 186 monitors located in 11 facilities (apartment, school, childcare, hospital, sports center, senior center, senior care, office, library, study café, government building) for the year 2021. Group A shows relatively low concentration of PM10 up to 18 ㎍/㎥ while other groups show higher values of PM10 up to 23 ㎍/㎥. In addition, PM10 in Group B and D shows only one positive peak during 10-11 am while Group C show two PM peaks during 10-11 am and 20-21 am. While CO2 show one peak during 15-17 am for both Group B and D, the peak level of CO2 is higher for Group B (843 ppm) than Group D (570 ppm). Similarly, temperature, and noise show different levels for each four groups. Interestingly, Group A include large portions of air quality data from senior cares (49%), libraries (44%), sports centers (59%), apartments (44%), schools (66%) and childcares (38%). Meanwhile, Group B consists of only small portions of data from all facilities (~34%). Group C are mostly from hospitals (51%). Group D show common air quality patterns in senior center (45%), government buildings (47%), offices (40%), and study cafés (42%). This work was supported by Korea Environment Industry & Technology Institute (KEITI) through Prospective green technology innovation project, funded by Korea Ministry of Environment (MOE) (RE2022011054).


AS24-A005
Prediction of PM2.5 Concentration in 24 Hours Based on Hybrid Depth Neural Network

Mengfan TENG#+, Siwei LI
Wuhan University, China

Accurate prediction of the future PM2.5 concentration is basis for human health and ecological environmental protection. In recent years, deep neural network models show advantages in the prediction of PM2.5 concentration, but few of the studies can be able to achieve a credible prediction of future longer term PM2.5 concentration(6~24 hours). To solve this problem, this study constructs a novel hybrid prediction model by combining the empirical mode decomposition (EMD) method, sample entropy (SE) index and bidirectional long and short-term memory neural network (BiLSTM) to reliably predict PM2.5 concentration at 24 future consecutive moment. The results show that the hybrid model has better performance on PM2.5 prediction in the future, with R2=0.987, RMSE=2.77μg/m3 at next hour and R2=0.904, RMSE=7.51μg/m3 in the sixth hours. Compared with other deep learning models, this model can improve the prediction accuracy of PM2.5 concentration in the short term (within 6 hours) by at least 50%, and better capture the change trend of PM2.5 concentration in 6 to 24 hours. It can be used as an effective tool for long-term prediction of PM2.5 concentration.


AS24-A006
The Impact of Air Pollution Control on Inter-provincial Trade-associated Environmental Inequality

Jiaxin DONG+, Siwei LI#
Wuhan University, China

Inter-provincial trade may cause transfer of air pollutants and associated health risks, contributing to the issue of environmental inequality. Strengthened air pollution control in China over the past years has gained considerable benefits in reducing the air pollution and related health damage, while its effect in modulating the trade-associated environmental inequality is still unknown. Here we explore the inter-provincial environmental inequality in China and analyze the impact of air pollution control on the inequality, not only by traditional emissions-based index, but also based on the perspectives of premature deaths and economic losses. Although the inter-provincial transfer of pollutant emissions were substantially reduced due to air pollution control, the imbalance in distribution of pollutant emissions and value added in different provinces existed and even further aggravated from 2012 to 2017. In particular, Shanxi, Ningxia, Guizhou and other provinces contributed more to emissions than to GDP. Moreover, the exposure-based index suggested that air pollution control reduced the absolute and relative environmental inequality associated with human health risks due to inter-provincial transfer. The provincial 100 million RMB value added came at the cost of 5.46 premature deaths in 2012, which fell to 3.91 deaths in 2017. The average proportion of economic losses to value added of all transfers was 5% in 2012 and dropped to 3.6% in 2017. This study can provide a reference for inter-regional economic cooperation and joint air pollution control, making accurate inter-provincial compensation possible.


AS24-A009
Quantify the Responses of Nitrogen and Sulphur Deposition on NH3 Control by Machine Learning

Zhaoxin DONG#+, Jia XING, Shuxiao WANG, Dian DING
Tsinghua University, China

NH3 emission control is proved of great importance in reducing PM2.5 concentrations in China, while how it affects nitrogen/sulphur (N/S) deposition is still unclear. The fast development of machine learning provides a new method for understanding the effect of NH3 on N/S deposition by the imitation of 3-D model. This study develops a new response surface model by using the machine learning technique to quantify the responses of N/S deposition to NH3 emission control in the Yangtze River Delta, China. It is found that NH3 control has higher efficiency in reducing the N/S deposition than NOx and SO2 alone. The reduced N deposition response to NH3 emission abatement is higher in the north part of the YRD region whereas oxidized N deposition decreases sharply in the region with low N critical load. An unexpected co-benefit is found in reducing N deposition when we control the NH3 and NOx emission simultaneously. Compared with the sum effect of individual NH3 and NOx emission abatement, the extra benefits from the synergy controls account for 4.4% (1.23 kg N·ha-1·yr-1) of the total N deposition, of which 81% comes from the oxidized N deposition. The YRD region could receive the largest co-benefits with a 1:1 ratio of NOx: NH3 emission reduction. The NH3 emission control also changes the ratio of wet S deposition to dry S deposition and mitigates the wet S deposition. These findings highlight the effectiveness of NH3 emission control and suggest a multiple pollutant control strategy for reducing N/S deposition, which may be also appropriate for other regions in China and other countries.


AS24-A010
Estimating Carbon Dioxide Emissions on Roads Based on Deep Learning

Myeong-Gyun KIM#+, Hyo-Jong SONG
Myongji University, Korea, South

Greenhouse gases(GHGs), a major factor in climate change, are emitted from various sectors. Among them, GHGs emitted from the transportation sector account for the third-highest proportion of the energy. In 2018, GHG emissions in the transportation sector in Korea were about 98 million tons, accounting for 13.5% of the total emissions. Therefore, it is urgent to reduce GHGs in the transportation sector to achieve the national carbon neutral goal. In order to efficiently reduce GHGs in the transportation sector, emissions by region/road must be accurately calculated. However, currently, emissions are only measuring at the national level, so calculating emissions for each road remains a problem. This study aims to estimate traffic volume through deep learning and develop a model obtaining road carbon dioxide emission. Seoul, which has good data provision, was selected as a pilot destination. First, the traffic volume missing link is estimated, and the model used for this uses the measured traffic volume as a dependent variable, and the traffic volume of the measured link, which is a dependent variable, and the traffic speed and road characteristics, which are explanatory variables, are composed of the data of the estimation model. These data are provided by the Seoul TOPIS and ITS. Traffic volume estimation is implemented using the LSTM+DNN model, and MAE and MSE are used for verification. As a result, MAE is 205, which shows that it is quite good performance even though there is no traffic volume data in the explanatory variable. Then, the traffic volume estimated through this model is used to calculate carbon dioxide emissions by road. Although it is an initial level result, it is expected that efficient carbon emission reduction can be supported if a better emission calculation algorithm is developed by upgrading deep learning technology in the future.


AS24-A011
Particulate Matter Prediction and Shapley Value Interpretation Through a Deep Learning Model

Youngchae KWON#+
Myongji University, Korea, South

The adverse effects of particulate matter (PM) on public health are well known and the public are cautious of exposure to these air pollutants. This has led to the need for accurate particulate matter predictions and clear explanations of the mechanisms involved. This study collected and analyzed data to predict particulate matter concentrations at regular intervals in Korea. Automated synoptic observation system data (ASOS), real-time atmospheric observation data from Airkorea (Air), and GEO-KOMPSAT-2A (GK-2A) data were used. We also used deep learning which is useful for particulate matter predictions. The deep learning model used a neural network to predict PM with diameter less than 2.5 µm (PM2.5) and PM with diameter less than 10 µm (PM10) concentrations. To illustrate the results of the nonlinear model, we calculated the Shapley value using eXplanable Artificial Intelligence (XAI) in the SHapley Additive exPlanations (SHAP) library. The difference in analysis according to the diameter of aerosols was explained. was most affected by the previous day's value, and was most affected by sea level pressure (SLP). Furthermore, to analyze the contribution of features for each grid, Shapley values were normalized. Normalized Shapley values (NSV) were clustered and represented visually. was classified into three clusters and was classified into four clusters. when predicting each grid, we also confirmed whether the data on the adjacent grid points had high feature importance. Overall, the study summarizes how much SHAP analysis fits with the characteristics of generally known PM mechanisms.


AS24-A012
Development of PM2.5 and PM10 Prediction Models Using Artificial Intelligence, CMAQ, and Meteorology

Seong-il LEE#+, Hyo-Jong SONG
Myongji University, Korea, South

Air pollution is a big problem all over the world. It is important not only to reduce air pollutants, which are the causes, but also to predict them because they can be prepared for and prevented by making accurate predictions. Therefore, research on air pollutants continues to be conducted. Among them, we developed a model that predicts PM2.5 and PM10, studied how to continuously improve performance, and compared and analyzed with previous models. For the data, calculated values and meteorological data obtained through CMAQ were used as input data, and observation values were used as target data. The prepared data were applied to the grid model to make predictions, and compared and analyzed with observations using the previous model and CMAQ. In order to improve predictive performance, appropriate data from meteorological data were selected, preprocessed, and applied together with the data obtained from CMAQ. These activities have improved performance.


AS45-A003
Long-term Effects of Siberian Wildfire on Vertical Distributions of Hydrocarbons in UTLS Over East-Asia

Donghee LEE1+, Ja-Ho KOO1#, Patrick SHEESE2, Kaley WALKER2
1Yonsei University, Korea, South, 2University of Toronto, Canada

In this study, we examined the seasonal vertical pattern of six hydrocarbons (C2H2, C2H6, CH3OH, HCOOH, HCN, and HCHO) and carbon monoxide (CO) in the East Asian upper troposphere and lower stratosphere (UTLS) from 2004 to 2020. We used satellite data from Atmospheric Chemistry Experiments (ACE) – FTS version 4.1 to investigate seasonal hydrocarbons vertical pattern over East-Asia, and MODIS Level 2 active fire data (MOD14 and MYD14, and MCD64A1) and land cover product (MCD12C1) to analyze fire information along with land cover type over Siberia: fire count (FC), fire radiative power (FRP) and Burned Area (BA). we divided forest regions into 3 parts based on the MODIS land cover percentage. Since East-Asia often suffered from Siberia wildfire plume for summer, it is likely to see the large enhancement of hydrocarbon in summer (June to August). As expected, we found the summertime enhancement of hydrocarbons and CO volume mixing ratio at 8.5 to 13.5km. Around 10-13 km altitude, FC and BA in Siberia shows the highest correlation coefficients with HCN and CO in Northern China (R = ~0.5 to 0.6). Moreover, BA and HCN, CO vertical correlation indicate also significant. (R = ~ 0.5 at 10.5 km to 12.5km of altitude), meaning that the wildfire effect is almost reaching to the northern hemispheric tropopause. Since the lifetime of HCN and CO is rather long (at least a month), the atmospheric chemistry in the upper troposphere is largely affected by the plume of Siberian wildfire. If the Sibrian wildfire becomes more frequent related to the global warming trend, this connection may be more intensified in the future, where the necessity of further research lies. This work was supported by the National Research Foundation of Korea(NRF) grant funded by the Korea government(MSIT) (No. 2020R1C1C1011624).


AS46-A003
Statistical Analysis of Aviation Turbulence in Middle-upper Troposphere Over Japan

Yoshiaki MIYAMOTO1#+, Ayako MATSUMOTO2, Soshi ITO1
1Keio University, Japan, 2ANA HOLDINGS, Japan

This study examined the statistics of aviation turbulence that occurred in Japan between 2006 and 2018 by analyzing the Pilot Report (PIREP). In total, 81,639 turbulence events, with moderate or greater intensity, were reported over this period. The monthly number of turbulence has an annual periodical variation as observed in different regions by previous studies. The number of turbulence cases is high from March to June and low in July and August. Higher number of turbulence cases are experienced along the major flight routes in Japan, especially around Tokyo, for the active period between 9:00 and 20:00 local time. The number of cases of turbulence peaks when the flight reaches an altitude of 33000 ft (FL330), while it reduces when the flight altitude is less above FL380 and below FL280. The statistical features are not largely different among the four seasons; however, there are some exceptions. For instance, the number of turbulence is large in high altitudes in summer and small in low altitudes in winter. Considering the number of flights, it is evident that the frequency of turbulence is higher in altitudes between FL200 and FL350, whereas the flight number is high below FL200 and above FL350. The number of convectively induced turbulence is relatively large during the daytime in summer compared with the other seasons. Large number of mountain wave turbulence is observed around the mountainous region in fall and winter when the jet stream flows over Japan.


AS46-A005
Multi-model-based In-flight Icing Forecast Based on the Simplified Forecast Icing Potential (SFIP) Algorithm

Eun-Tae KIM#+, Jung-Hoon KIM
Seoul National University, Korea, South

Multi-model-based in-flight icing forecast based on the Simplified Forecast Icing Potential (SFIP) algorithm has been developed using two operating global Numerical Weather Prediction (NWP) models: the Unified Model-Global Data Assimilation and Data Prediction System (UM-GDAPS) from the Korean Meteorological Administration (KMA) and the Global Forecast System (GFS) from the National Centers for Environmental Prediction (NCEP). The SFIP is a fuzzy-logic algorithm calculating icing potential from temperature, relative humidity, vertical velocity, and cloud water content (liquid + ice) predicted directly by NWP model. The most important components of the SFIP algorithm are the membership functions and weight combinations, which have been optimized using icing pilot reports (PIREPs) from Oct 2015 to Jul 2018 for the two NWP models. The time-lagged ensemble (TLE) method is applied to combine the two NWP model-based SFIPs with five forecast lead times from 12 to 36 hours (6-hourly). The multi-model-based TLE prediction system provides two types of forecasts: deterministic and probabilistic. The deterministic icing forecasts provide an ensemble mean of SFIPs from the 10 ensemble forecast members. The probabilistic forecasts provide the relative frequency of the number of ensemble members among total members that exceed a specific threshold of severe icing potential at given grid point. All single- or multi-model-based systems are evaluated using the icing PIREPs and several icing cases observed by the Nara (meaning a nation in a native Korean) research aircraft operated by the KMA/National Institute of Meteorological Sciences (NIMS) in South Korea.


AS46-A007
Numerical Study of Near-cloud Turbulence Encounters Associated with Convective Clouds Over East Asia

Soo-Hyun KIM+, Jung-Hoon KIM#
Seoul National University, Korea, South

Turbulence associated with convective clouds is termed convectively induced turbulence (CIT). The CIT occurs within the cloud as well as in cloud-free air above or near convective clouds (near-cloud turbulence, NCT). Because in-cloud CIT can be detected from a visible cloud boundary, predicting NCT in advance is more significant for a safe air travel. Although there have been investigated generation mechanisms of NCT using numerical simulations and observations in the world, further studies on NCT frequently occurred over East Asia have been required. In this regard, current study examines two clusters of moderate-or-greater (MOG)-level turbulence occurred over East Asia using convection-permitting scale simulation. On 2 December 2019, a commercial aircraft traveling across the northern Pacific Ocean encountered MOG-level turbulence near convective clouds developed along well-organized surface front. The numerical simulation is conducted using the Advanced Research Weather Research and Forecasting model v4.3.3 with five domains with horizontal grid spacings from 9 to 0.11 km. It is found that there are convectively induced modifications in large-scale flow near turbulence incident regions: 1) strong bulk vertical wind shear is evident near downstream regions of deep convection and 2) areas of moist static instability. In vertical cross sections, it is found that strong vertical wind shear and flow deformation below and above enhanced jet due to deep convection exist. The current simulated results indicate that a combination of vertical wind shear, flow deformation, and convective gravity waves and their breaking can be related to the southern cluster of NCT cases. On the other hand, shear instability due to strong vertical wind shear mainly induced by enhanced upper-level jet may be associated with the northern cluster of NCT cases. The additional nesting with the fifth domain is conducted for detailed analyses and results will be presented in the conference. 


AS46-A008
Regional Real-time Weather Prediction System Over Incheon International Airport Using WRF Model

Yujeong DO+, Hyeon-Ji LEE, Kyo-Sun LIM#
Kyungpook National University, Korea, South

This study introduces the regional real-time weather prediction system using Weather Research and Forecasting (WRF) model to support the aviation safety and investigates the impact of initial/boundary conditions and horizontal resolutions on the model simulations, especially on the low-level weather variables such as 2-m temperature, relative humidity, and 10-m wind speed and direction. The 6-hour interval forecast fields, that are generated by National Centers for Environmental Prediction (NCEP) Global Forecast System (GFS) and Korea Meteorological Administration (KMA) Korean Integrated Model (KIM), are utilized for the real-time model simulations. For the Sea Surface Temperature (SST), National Oceanic and Atmospheric Administration (NOAA) daily Optimum Interpolation SST (OISST) climatology data are incorporated. Three nested domains are constructed centering on Incheon international airport and horizontal resolutions are set as 10-km, 1-km, and 100-m grid spacing. The numerical experiments are carried out during a period of 24 hours starting at 00 UTC on each day of April 2021 when the monthly averaged wind speed was strongest through the year. With the introduced configuration, we can provide the climatological evaluation results of the real-time weather prediction system based on WRF model. From the comparison of model simulations with available observations at the selected weather observation stations over Yeong-Jong island where Incheon international airport is located and adjacent areas, we figure out that the simulation with the finer horizontal resolution captures the diurnal variability of temperature better than the one with the coarser horizontal resolution. In addition, the simulated wind speed under the finer resolution shows better agreement with the observations. More detailed results will be presented at the conference. This work was funded by the Korea Meteorological Administration Research and Development Program under Grant KMI2022-00410 and the National Research Foundation of Korea (NRF) grant funded by the Korea government (MSIT) (RS-2023-00208394).


AS46-A009
Seasonal Variation of Environmental Fields of Aviation Turbulence in the Upper Level Around Japan

Soshi ITO1#+, Yoshiaki MIYAMOTO1, Yoshiyuki KAJIKAWA2
1Keio University, Japan, 2RIKEN Advanced Institute for Computational Science, Japan

Turbulence is a major factor that hinders the safe navigation of aircraft. Various organizations and researchers attempt to predict turbulence, but it is difficult to accurately predict the location and time of turbulence. This is because the mechanism of turbulence generation and the environmental field at the time of generation are not fully understood. Because environmental fields vary depending on where they occur, regionally focused studies are needed. In this study around Japan, which has not been done very often, the objective was to determine the environmental fields during the occurrence of clear-air turbulence of moderate intensity in the upper levels by season. In addition, to clarify the relationship with the Baiu front, the analysis will be conducted in five seasonal divisions, with summer and June as independent months. We used the Pilot Report (PIREP), which is data reported by pilots on meteorological phenomena they encountered in flight, and Japan Meteorological Agency Mesoscale Reanalysis data (MANAL). The analysis period was 8 years, from 2010 - 2017. Based on stellar and topographic data, the cases of mountain wave turbulence and convective induced turbulence were excluded from PIREP. The analysis showed that the environmental field at the time of the outbreak differed depending on the season. Especially, in winter, it occurs in a field with a weaker-than-average jet stream and smaller trough curvature. It was also a field of enhanced vertical wind shear rather than deformational motion. In June, there is a strong moist convergence field to the south in the lower troposphere, and the north-south gradient of the equivalent potential temperature suggests the presence of the Baiu front. It is also suggested that the field is prone to intensify deformation motions associated with the Baiu front.


AS46-A012
Development of Model Output Statistics to Support Flight Operations Around the Airports in South Korea

Jeonghoe KIM+, Jung-Hoon KIM#
Seoul National University, Korea, South

Weather phenomena such as low-level wind shear, icing, low ceiling and visibility can be potential weather hazards for flight operations around the airports. To support safe flight operations against these aviation weather hazards, especially around the airports, weather forecast offices around the world produce terminal aerodrome forecasts (TAFs) in which meteorological information related to the weather hazards is included. One way to produce weather forecasts is to use model output statistics (MOS). In the MOS method, relationships between meteorological variables from observations and numerical weather prediction (NWP) model outputs are established from long-term data archives using statistical models. Currently, Korea Meteorological Administration (KMA) operates a MOS system that is based on multilinear regression applied to global NWP models. However, this MOS system suffers from limitations since (1) the weather forecasts produced by the MOS system is not directly focused on the airport locations with high resolution of regional model and (2) a relatively “simple” statistical model was used in the development. In this study, MOS systems were developed for weather forecasts around the airports in South Korea using Local Data Assimilation and Prediction System (LDAPS), which is a regional NWP model operated by KMA. First, a MOS system was developed using multilinear regression with forward feature selection as a baseline model. Then, the new MOS systems are developed further using both linear (e.g. LASSO regression) and nonlinear (e.g. random forest regression) statistical models. Performance skills of the developed MOS systems are compared by scoring metrics including mean absolute error (MAE) and bias against observations at the airports in South Korea. Acknowledgement: This work was funded by the Korea Meteorological Administration Research and Development Program under Grant KMI2022-00310.


AS46-A013
Evaluation of Aviation Convective Index for Deep Convective Area Using the Global Unified Model of the Korean Meteorological Administration

Yi June PARK+, Jung-Hoon KIM#
Seoul National University, Korea, South

 This study developed a new index for predicting deep convective area, the Aviation Convective Index (ACI), using the operational global Unified Model of the Korea Meteorological Administration (KMA). ACI was developed by the fuzzy-logic algorithm in Korea, which was validated and optimized by using the 1-yr period of radar data. The yearly optimized ACI (ACIYrOpt) based on the optimized weight coefficients for 1-yr period shows a better skill than the original one with the uniform weights. But, in winter with the lowest number of the deep convective events, performance skill was deteriorated significantly, resulting in the decrease of seasonal averaged value of Area Under the ROC Curve (AUC) and True Skill Statistics (TSS) by 0.358 % and 6.143 %, respectively. To consider the seasonal variability in the background conditions conducive to deep convections, membership function (MF) and weight combination in the fuzzy-logic algorithms were optimized in each season. Finally, seasonally optimized ACI (ACISnOpt) showed a better skill with the significant improvements in AUC and TSS by 0.931 % and 25.62 %, respectively, compared with those from the . We also conducted several case studies for confirming the improvements. The representative cases were selected in each season with observed CIT events from the aircraft data. In all cases, the ACISnOpt predicted a better spatial distribution and intensity of the convection. Enhancements in the forecast fields from the ACIYrOpt to the ACISnOpt in the selected cases explained well the changes in overall performance skills of the probability of detection for both “yes” and “no” events during 1-yr period of the data. These results imply that the ACI forecast should be optimized seasonally to take into account the variabilities in the background conditions for deep convections in Korea. Acknowledgement: This work was funded by the Korea Meteorological Administration Research and Development Program under Grant KMI2022-00410.


AS46-A015
Statistical Analysis on the Estimations of Solid Hydrometeors Growth Zones and Their Weather Conditions Using Radar Spectrum Width

Sung-Ho SUH1#+, Woonseon JUNG2, Hong-il KIM1, Eun-Ho CHOI1, Jung-Hoon KIM3
1Korea Aerospace Research Institute, Korea, South, 2National Institute of Meteorological Sciences, Korea, South, 3Seoul National University, Korea, South

This is a follow-up study to analyze the correlation between hydrometeor type and the radar spectrum width (σv) according to atmospheric disturbances such as turbulence and wind shear. The statistical analysis was performed for eight precipitation cases under various conditions (precipitation type, season) focusing on Dendrite Growth Zone (DGZ) and Needle Growth Zone (NGZ), where Dendrite (DN) and Needle (NE) type snowflakes are dominant, respectively. The Growth Zone Determination Algorithm (GZDA) was proposed to determine them quantitatively. The σv zone was identified only in stratiform precipitation, and the intensity of the σv zone in DGZ has inverse-proportional to their altitude (i.e., winter). The strong σv-the differential radar reflectivity (ZDR) negative relationship in DGZ for all cases is consistent with the aerodynamic properties of DN. In addition, as the range of SW was larger than that of ZDR, it was confirmed that the dependence of σv according to atmospheric conditions is significant. On the other hand, NGZ had a weak σv-ZDR negative relationship with a narrow range of SW, which is consistent with the aerodynamic properties of NE. The lower cross-correlation coefficient (ρhv) in DGZ than that in NGZ implied that the irregularities (particle shape and aerodynamics features) of DN were more pronounced than those of NE. Furthermore, the possibility of sub-zero air temperature estimation based on weather radar from GZDA was confirmed.


AS46-A017
A Study of Sea Fog Event Over the Yellow Sea Using the High-resolution Modeling with Improved Initial Surface Conditions

Jae-Sik MIN#+, Jung-Hoon KIM
Seoul National University, Korea, South

The west coast of Korea is composed of many islands and tideland, and the coastline is changing due to reclamation projects that began in the 1960s. Incheon International Airport (ICN) on Yeongjong Island in the Yellow Sea is a representative artificial structure built through land reclamation. Due to land reclamation and the construction of artificial structures, the surface conditions change, and the ocean-atmosphere interaction changes, resulting in changes in meteorological phenomena. This study aims to analyze the influence of meteorological phenomena according to changes in surface conditions, focusing on ICN. In particular, on November 16, 2019, the case was analyzed using the WRF for low visibility, which is a representative weather hazard around airports. Through a control experiment (CTL) using geographical information (topography and land-use type) before the past reclamation and an improved experiment (EXP) using the latest geographical information, the effect on the NWP simulations was examined. For geographic information, a topography with a 5 m resolution (NGII, 2022) and a land-use type (ME, 2021) with a 5 m resolution were used as initial conditions for the WRF. On November 16, 2019, low visibility was a case in which a migratory high in autumn was located on the Korean Peninsula, and radiation fog generated inland at night affected ICN by a land breeze. The minimum visibility distance was 150 m. In EXP, the low visibility phenomenon was well simulated. However, using past geographical information in CTL, an advection of radiative fog appeared inland, whereas fog due to radiative cooling did not occur because ICN was composed of the ocean. This study confirms the change in radiation fog distribution due to land reclamation, and details will be mentioned in this presentation. Acknowledgment: This research is supported by the Korean Meteorological Administration Research and Development Program (KMI2022-00310).


Wed-02 Aug | 1:10 - 3:10 | MR311
AS19 - Extreme Weather Resiliency: Prediction and Response Strategies

Session Chair(s): Huang-Hsiung HSU, Academia Sinica

AS19-A007 | Invited
Cloud Radiative Effects on the Development of Tropical Cyclones: Role of Cloud Vertical Structure

Enwang LUO1#+, Guoxing CHEN1, Wei-Chyung WANG2
1Fudan University, 2University at Albany - State University of New York

Clouds affect the life cycle of tropical cyclones (TCs) greatly via the cloud radiative effects, which may accelerate the TC genesis by enhancing the mid-level circulation but prevent TCs from attaining higher intensities by reducing the inward vorticity flux. Therein, the role of cloud vertical structure, which is crucial to the cloud radiative effects, is still unclear due to the model deficiencies in cloud-fraction parameterization. In this study, we equipped the WRF model with a neural network-based scale-adaptive (NSA) cloud-fraction scheme that was developed using the CloudSat data, and simulated the record-breaking TC ‘In-Fa’ (2021) using the NSA scheme and the conventional Xu-Randall scheme. Results show that the TC track simulated by NSA is closer to the JTWC best-track data than that by Xu-Randall both spatially and temporally. The landing point by the NSA scheme is almost the same as the observation. Meanwhile, the cloud vertical structure in NSA is more compact than that in Xu-Randall, yielding cloud radiative effects closer to the observation. Further analyses will be presented within the context of physical associations between the cloud vertical structure and the TC development.


AS19-A011
Investigating the Weather Effects of Smoke Aerosols in the Unified Forecast System: A Study of 2020 Summer North America Wildfires

Sarah LU1#+, Shih-Wei WEI1, Dustin GROGAN1, Anning CHENG2, Partha BHATTACHARJEE2, Jeffery MCQUEEN2
1University at Albany, State University of New York, 2National Oceanic and Atmospheric Administration

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. The 2020 fire season was a record setting season for the western United States, with more than 8 million acres burned. Previous studies have projected significant increases in boreal forest fire occurrence, area burned, and fire intensity for a changing climate. In this study, we adopted the NOAA community model, the Unified Forecast System (UFS), to investigate the impact of smoke aerosols from wild fires on medium range weather forecasts. The UFS was modified to include the option to frequently update the aerosol distributions during the forecast (i.e., rapid refresh of the aerosol loading). We conducted a series of 7-day UFS forecasts, initialized from 00Z of NOAA analysis, during Aug 22nd -Sep 18th, 2020. The control UFS run considers climatological aerosol loading while the rapid refresh UFS run updates aerosol fields every 6 hour. Only direct aerosol-radiative effects are considered in both UFS runs. We will report aerosol-induced changes in UFS results, including 1) the impact of smoke aerosols on radiation, 2) the sensitivity in the thermodynamic fields, and 3) the weather effects of smoke aerosols. The UFS and its flexible aerosol configuration provides a useful scientific tool for the community to understand the fate and impact of wildfire events.


AS19-A026
Sensitivity of Extreme Rainfall in Taiwan to SST Over the South China Sea Through Modulation of Marine Boundary Layer Jet

Kuan-Jen LIN1+, Shu-Chih YANG1#, Shuyi CHEN2
1National Central University, 2University of Washington

Water vapor transport from the South China Sea (SCS) by the marine boundary layer jet (MBLJ) can be an important moisture source for heavy rainfall events in Taiwan during the mei-yu season. However, the variability of MBLJ due to the sea surface temperature (SST) changes and its impact on extreme rainfall events in Taiwan has not been well understood. This study aims to better understand this problem by conducting numerical experiments varying the SST over the SCS. Results show that increasing the SST over the SCS leads to stronger vertical mixing in the boundary layer and weakened MBLJ. With the weaker MBLJ, the mei-yu front can push further south, which shifted the heavy rainfall over Taiwan southward for a hundred kilometers. The opposite effect is observed when the SST is decreased over the SCS but with a relatively smaller impact.


AS19-A002
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

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 characteristized by stronger vorticity, circulation, ascent, total precipitiable 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.


AS19-A005
Impact of Global Warming on the Characteristics of Tropical Depression in Southwest Indian Ocean Investigating by ARPEGE Simulations

Chia-Lun TSAI1#+, Olivier BOUSQUET2, Sylvie MALARDEL3, Julien CATTIAUX4, Fabrice CHAUVIN4
1Chinese Culture University, 2Meteo-France, 3Université de La Réunion - CNRS, 4Université de Toulouse - CNRS

The globe numerical weather prediction model ARPEGE (Action de Recherche Petitle Echelle Grande Echelle) was adopted in this study to investigate the characteristics of tropical depression (TD) activity in the Southwest Indian Ocean (SWIO). Three main metrics of the TD frequency, intensity, and precipitation were documented for future changes under significant global warming in a significant scenario (RCP 8.5) and will discuss their possible causes. The TD tracks can be efficiently detected using “JPD scheme” on two ARPEGE experiments as present-day and future simulations during 1946-2013 and 2046-2093, respectively. The results indicate that the frequency of the TD initiation (TDI) will decrease, and its decreasing rate is ~25% during austral summer (i.e., from November to April). The locations of reducing TDI are more concentrated in the eastern SWIO (~10°S-15°S, 75°E-85°E) and possibly related to the more substantial vertical wind share, weaker low-level horizontal wind shear/vorticity, and dryer mid-level relative humidity. Very intense TD (i.e., ITD-44; the intensity of the TD can have reached 44 m s-1) will become more vital as their maximum lifetime intensity (LMI) increases ~3 m s-1 in the future. Warmer sea-surface temperature (SST) would be a critical factor in dominating the ITD-44 intensity changes in the SWIO. In the future, plentiful precipitation of precipitation will explore surrounding the centers in 1° radius distance with a significantly increased rate of ~11%. The ITD precipitation changes are linked to the increasing specific humidity associated with warmer SST.


AS19-A019
Potential Changes of Westward-typhoon Near Taiwan Under a Global Warming Climate

Chen-Hau LAN1+, Pay-Liam LIN1#, Wei-Chyung WANG2, Sarah LU3
1National Central University, 2University at Albany - State University of New York, 3University at Albany, State University of New York

Under global warming, the potential change of intensity, occurrence probability, and tracks for Tropical cyclones (TCs) is one of the important scientistic issues. In Taiwan, there are many TCs landing in Taiwan from the west pacific along the easterly flow. To discuss the effects of climate-changing, General circulation models (GCMs) have played a significant role in projecting changes in the frequency, track, and occurrence location of future TCs. However, the coarse resolution of GCMs will be a problem to discuss the interaction between TCs and topography. Considering the disasters by TCs, in addition to the interaction between typhoons and the environment, the location of typhoons relative to the terrain, moving speed, and intensity of the typhoon are also important factors to affect the precipitation distribution of Taiwan. In this study, the tracks simulations are conducted dynamical downscaling experiments with 5km WRF models from Hiram models by the National Science and Technology Center for Disaster Reduction (NCDR). The results indicated that not only intensities are increased by warming sea surface temperature but also have a faster motion for westward TCs. Because of the change in intensity and translation speed, the cyclone damage potential (CDP) is decreased in north-eastern Taiwan and increased in western Taiwan. On the other hand, the orographic effect still plays a significant role for the typhoon intensity and movement in the future. The duration time of TCs is symmetric between the north and south part of Taiwan under global warming. To discuss the translation speed when the TC passes through Taiwan, the westward TCs in north Taiwan will accelerate before landing since the typhoon intensity is stronger in the future.


AS19-A006
An Investigation on the Regional Characteristics of Summer Season Rainfall Over Taiwan Using GPM DPR Measurements

Jayalakshmi JANAPATI1+, Balaji Kumar SEELA1,2, Pay-Liam LIN1#
1National Central University, 2Academia Sinica

Taiwan, an island located in the northwest Pacific region is influenced by heavy rainfall events during warm seasons, more particularly during June to August months. These heavy rainfall events in summer are chiefly caused by the precipitating clouds of monsoons and tropical cyclones. Interaction of precipitating clouds with the complex topography results in inhomogeneous and intense rainfall throughout this island. Even though there were reports on the rainfall characteristics for Taiwan, the raindrop size distributions/cloud microphysical attributions responsible for the regional changes in summer rainfall are yet to be documented. The dual-frequency capability of the Global Precipitation Measurement dual-frequency precipitation radar (GPM DPR) can offer the opportunity not only to measure the vertical profile of rainfall but also the precipitation drop size information. Hence, the present study investigates the regional variations in the microphysical characteristics of summer season rainfall over Taiwan using nine years (2014-2022) of GPM DPR measurement. The results showed clear distinctions in the precipitation and raindrop size distributions over the north, south, east, and central part of Taiwan. Among four regions, central (north) Taiwan is dominated by large-size (small) drops. The possible microphysical attributions are revealed with the aid of contour frequency by altitude diagrams (CFAD) of radar reflectivity, rainfall rate, mass-weighted mean diameter, and normalized intercept parameter.


AS19-A008 | Invited
Causes of the Record-breaking Drought in Taiwan in 2020-2021

Huang-Hsiung HSU1#, Ming-Ying LEE2, Hao-Jhe HONG1+, Chao-An CHEN3
1Academia Sinica, 2Central Weather Bureau, 3National Science and Technology Center for Disaster Reduction

During 2020, an earlier-ended Mei-Yu season combined with a typhoon-absent summer, followed by notably low rainfall from following autumn to spring in 2021, Taiwan’s accumulated rainfall during June 2020 to May 2021 broke the lowest record since 1910. The duration and strength of subtropical height over the Western North Pacific in Jun to September were the longest and strongest since 1949. The abnormal subtropical height maybe caused by the compounding effects from cool sea surface temperature (SST) over the central to eastern equatorial Pacific associated with La Niña, and warm SST in the northern Indian Ocean and the tropical Atlantic. The warmest SST appeared in the Philippine Sea through October 2020 to Marth 2021, concurrent with La Niña, generated the dry the condition near Taiwan. The less spring rainfall in Taiwan in 2021 could be directly attributed to the warmest SST in the Philippine Sea and indirectly to the weakening La Niña , whereas negative phase of the Pacific Decadal Oscillation seemed to have little effect. An anomalous cyclone usually appeared in the western side of the warm Philippine Sea and brought dry northeasterly anomaly to the East Asian coast, resulting in less spring rainfall in Taiwan, and the La Niña would favor and maintain this atmosphere-ocean coupled system. In April-May 2021, active tropical intra-seasonal oscillation caused weaker moist southeasterly in middle to end of April, and also resulted in dry condition before the end of May. In conclusion, the most serious drought event in 2020-2021 since 1910 was caused by the compounding effect from various influencing factors that occurred concurrently and sequentially. How much of these abnormal conditions were caused by the warming trend in recent decades, which is not investigated in this study, warrants further studies.


Wed-02 Aug | 1:10 - 3:10 | MR323
AS35 - Aerosols, Clouds, Radiation, Precipitation, and Their Interactions

Session Chair(s): Xiquan DONG, University of Arizona

AS35-A007
Aerosol Impacts on the Precipitation of Squall Lines: A Case Study in South China

Hui XIAO#+
Guangzhou Institute of Tropical and Marine Meteorology, China Meteorological Administration

It remains unclear to what extent squall lines respond to aerosol particles serving as cloud condensation nuclei (CCN). To solve this problem, dozens of simulated cases formed by adding balanced perturbations to initial meteorological fields have been conducted to quantify the effect of the aerosol on hydrometeors, precipitation, and their related microphysical processes in this study. The results showed that the changes in total surface precipitation of squall lines to aerosol perturbations ranged from −14% to 4% in South China. Even if there was no significant change in total precipitation in some cases, the precipitation over partial area still showed obvious changes. Through cluster analysis, the sign of the precipitation response to increasing aerosol loading depended on whether the increase in graupel growth compensated for the loss of snow and rain growth under polluted conditions. With increased aerosol loading, more cloud droplets suppressed rain formation and subsequently rain growth due to lower collision-coalescence efficiency, and the snow growth was also suppressed by the decrease in the riming process. However, there was more graupel melting into rainwater due to an increase in graupel growth by accreting cloud droplets. Through composite analysis of meteorological fields, surface precipitation suppressed by aerosols was shown to be more likely to appear in poor water vapor conditions and weak convective intensities, and vice versa.


AS35-A008 | Invited
Rethinking of Aerosol-cloud-interaction and Aerosol-radiation-interaction by Accounting for Cloud-PBL-coupling

Zhanqing LI1,2#+
1University of Maryland, 2Beijing Normal University

Aerosol-cloud-interaction (ACI) has been extensively studies using a variety of observation data, but aerosol data are often limited to either ground-based and satellite measurements due to a severe lack of in-situ measurements. The bulk of aerosol is situated in the planetary-boundary-layer (PBL) with a non-uniform distribution. This implies that neither column or surface aerosol measurements do not denote the true loading and properties of aerosol that interact with cloud through both ACI and aerosol-radiation-interaction (ARI). Whether and how much ground-based aerosol measurements can represent the aerosol that do interact with cloud and PBL depend on the coupling between cloud and PBL (also surface). To resolve these fundamental problems, we have conducted systematic investigations concerning the ACI and ARI by accounting for the cloud-PBL-coupling (CPC) as the later plays an important role in affecting atmospheric thermodynamics. Using comprehensive field observations made in China and US, we gain insight into the response of the PBL process to aerosols, especially entrainment. We found that high aerosol loading can significantly suppress the entrainment rate, breaking the conventional linear relationship between sensible heat fluxes and entrainment fluxes. Related to aerosol vertical distributions, aerosol heating effects can alter vertical heat fluxes, leading to a strong interaction between aerosols and the entrainment process in the upper boundary layer. Such aerosol-entrainment coupling can inhibit boundary layer development and explains the great sensitivity of observed entrainment rates to aerosols than can traditional calculations. Likewise, we have sorted out clouds according to the CPC and noted drastic different responses of the ACI to aerosol loading under different states of the CPC. Under coupled conditions, the ACI is a lot stronger than without accounting for it. This implies that many of the previous studies tend to underestimate the ACI.


AS35-A025
What are the Similarities and Differences in Marine Boundary Layer Cloud and Drizzle Microphysical Properties During ACE-ENA and Marcus Field Campaigns?

Baike XI1#+, Alexa MARCOVECCHIO2, Xiaojian ZHENG2, Peng WU3, Xiquan DONG2, Ali BEHRANGI2
1The University of Arizona, 2University of Arizona, 3Pacific Northwest National Laboratory

This study compares macrophysical and microphysical properties of single-layered, liquid-dominant MBL clouds from the Measurements of Aerosols, Radiation, and Clouds over the Southern Ocean (MARCUS) (above 60°S) and the ARM East North Atlantic (ENA) site during the Aerosol and Cloud Experiments in Eastern North Atlantic (ACE-ENA) field campaigns. A total of 1,136 (16.5% of clouds) and 6,034 5-min cloud samples are selected from MARCUS and ARM ENA in this study. MARCUS clouds have higher cloud-top heights, thicker cloud layers, larger liquid water path, and colder cloud temperatures than ENA. Thinner, warmer MBL clouds at ENA can hold a higher liquid water content due to higher cloud and ocean surface temperatures along with greater precipitable water vapor (PWV). MARCUS has a higher drizzle frequency rate (71.8%) than ENA (45.1%), but MARCUS drizzling clouds are drier and thinner. Retrieved cloud and drizzle microphysical properties from each field campaign show key differences. MARCUS clouds feature smaller cloud droplets, whereas ENA clouds have larger cloud droplets, especially at the upper region of the cloud. From cloud top to cloud base, drizzle drop sizes increase while number concentrations decrease. Drizzle drop radius and number concentration decrease from cloud base to drizzle base from net evaporation, and these decrease much faster under MARCUS’ drier environment. The broader surface pressure and lower tropospheric stability (LTS) distributions during MARCUS have demonstrated that there are different synoptic patterns for the selected cases during MARCUS with less PWV, while ENA is dominated by high pressure systems with nearly doubled PWV.


AS35-A024
Numerical Simulations of Cloud Number Concentration and Ice Nuclei Influence on Cloud Processes and Seeding Effects

Xiaofeng LOU#+
China Meteorological Administration

Aerosols, through cloud condensation nuclei (CCN) or ice nuclei (IN), affect cloud microphysics. With increasing concentrations of aerosols, it is important to consider the impact of IN along with CCN on clouds and precipitation in numerical simulations; further, aerosols may also affect the weather-modification seeding effect. On the basis of the observation of natural IN concentration and cloud-drop number concentrations, numerical sensitivity experiments for a snowfall case were designed to study the effects of parameters of IN and cloud number concentrations at the cloud base to consider the CCN effects on clouds and precipitation as well as weather-modification seeding effects. Generally, with smaller cloud-drop number concentration, the mass contents were much lower. With more ice nuclei, more ice crystals were able to nucleate, and additional snow particles were generated through ice crystals. Cloud-drop number concentrations heavily affected the location and amount of snowfall. During the 1e9 test, 2.4 mm was the highest reduction in the amount of snowfall; additionally, the amount of snowfall from the combined impacts of increased IN and cloud-drop number decreased in wide areas, and its maximum precipitation reduction exceeded
2.7 mm as well as up to 15% of the daily amount of snowfall. More IN reduced the artificial seeding effect, lowered the increase in snowfall in the center of the seeding, and lowered the reduction of snowfall in the reduction center of the seeding. With more IN, the seeding effect was able to shift approximately 0.6% from the 3.9% seeding effect of the control simulation.


AS35-A010
Global Precipitation System Scale Increased from 2001 to 2020

Yan ZHANG1#+, Kaicun WANG2
1Beijing Normal University, 2Peking University

How precipitation responds to global warming has drawn much interest from the scientific community. However, as one of the important properties of precipitation, changes in the precipitation system scale have rarely been studied. The latest retrospective merged satellite precipitation product has provided a great opportunity to investigate quasi-global precipitation system scale changes. This study uses the Integrated Multi-satellitE Retrievals for Global Precipitation Measurement (IMERG) data during 2001-2020 to investigate quasi-global precipitation system scale changes. Our results indicate that, generally, quasi-global precipitation system scales exhibit a significant increasing trend, which is more significant in winter and spring than that in summer and autumn over both hemispheres. The scale of nearly all precipitation systems over land regions has increased over the last two decades. In oceanic regions, precipitation system scales increase over tropical oceans but decrease over subtropical oceans. Medium-scale precipitation systems (100–1000 km) significantly increase in scale and decrease in frequency, while large-scale precipitation systems significantly increase in frequency, which both lead to a quasi-global increase in the precipitation system scale. Diagnostic investigation based on atmospheric analysis reveals that an increase in atmospheric stability tends to suppress local convective precipitation, while an increase in the total column water vapor could help maintain and enhance precipitation system scale, which jointly contribute to quasi-global precipitation system scale increase.


AS35-A003
Model Simulation of the Aerosol Perturbation on the Tibetan Plateau Convective Precipitation

Mengjiao JIANG1,2+, Yaoting LI3, Weiji HU1, Yinshan YANG4, Guy BRASSEUR2#
1Chengdu University of Information Technology, 2Max Planck Institute for Meteorology, 3Civil Aviation Flight University of China, 4Beijing Normal University

The Tibetan Plateau (TP) is important for weather and climate. Relatively clean aerosol conditions over the Plateau makes the study on the aerosol-cloud-precipitation interactions in this region distinctive. A convective event with precipitation observed on 24 July 2014 in Naqu was selected to explore the influence of aerosols on the onset and intensity of precipitation. We use the Modern-Era Retrospective analysis for Research and Applications Version 2 (MERRA-2) reanalysis to derive the cloud condensation nuclei (CCN), which can be regarded as the real-time background. These values are adopted to initialize the regional WRF 4.0 meteorological model and to simulate the onset of convective events and the formation of precipitation. Four sets of experiments were adopted for our simulations. A detailed analysis of microphysical processes shows that, with the increase in the aerosol number concentration, the conversion rate of cloud water to rain in clouds is enhanced at first. Under polluted situation, the conversion process of cloud water to rain is suppressed; however, the transformation of cloud water to graupel and the development of convective clouds are favored. As a result, the onset of the precipitation is delayed and cold-rain intensity increases.


AS35-A004
Spatial Heterogeneity of Aerosol Effect on Liquid Cloud Microphysical Properties in the Warm Season Over Tibetan Plateau

Pengguo ZHAO#+
Chengdu University of Information Technology

The effect of aerosol on liquid cloud microphysical properties over the Tibetan Plateau during the warm season is investigated by using aerosol index and cloud property parameters data. Distinct differences in aerosol effect on liquid cloud microphysical properties have been found between the northern TP (NTP) and southern TP (STP). The composite liquid cloud droplet effective radius (LREF) anomalies for positive aerosol index (AI) events are positive in the NTP and negative in the STP. In both NTP and STP, when the AI anomalies are positive, the LREF anomalies are also positive, which suggests that the increased aerosol loading reduces the solar radiation reaching the ground and thus enhances the atmospheric stability, which reduces the cloud base height and makes the liquid cloud area thicker, which gives cloud droplets more space to grow by collision-coalescence. This indicates that the aerosol radiative effect is not likely the reason causing the distinct differences of aerosol effects on liquid cloud properties between NTP and STP. Further analysis shows that in the STP, the LREF first increases and then decreases with the increase of AI, while in the NTP, the LREF always increases with the increase of AI, suggesting a spatial difference in aerosol microphysical effect. In the STP, the influence of aerosol on liquid clouds is mainly dependent on liquid water path (LWP) and convective available potential energy (CAPE), while in the NTP, the influence of aerosol on liquid cloud is more likely related to large aerosol particles.


Wed-02 Aug | 1:10 - 3:10 | MR327
AS03 - Application of Cloud-resolving Model Simulations for Studying Cloud and Related Physical Processes in Climate

Session Chair(s): Xiaowen LI, Morgan State University, Chien-Ming WU, National Taiwan University

AS03-A009
CRM and LES Estimates of Tangent Linear Convective Responses

Steven SHERWOOD1,2#+, Timothy RAUPACH1, Chimene DALEU3, Robert PLANT3, Yi-Ling HWONG4
1University of New South Wales, 2ARC Centre of Excellence for Climate System Science, 3Reading University, 4Institute of Science and Technology Austria

One way of measuring the impact of atmospheric small-scale processes on larger scales is via the tangent linear sensitivity of an atmospheric column to vertically localized perturbations, most straightforwardly starting from (i.e. tangent to) a radiative convective equilibrium (RCE) state. This can be encoded into an n x m response matrix given n vertical perturbation and m response layers. Recent studies with single-column versions of atmospheric models (SCMs) have reported substantial differences across SCMs, particularly in moisture sensitivities. and implausible discontinuities in responses with height. They have also shown that if radiative cooling and surface exchange coefficients are held fixed during perturbations, the SCM responses are determined mainly by the convective scheme. Although such responses appear informative, there is no observation available to tell us the true response matrix, so we need a reference CRM or LES calculation of these such as the one originally performed by Kuang (2010). Here we present calculations from two numerical models (WRF and MONC) run in a mesoscale box with periodic boundaries, at grid resolutions ranging from 100 to 4000m. WRF results are relatively insensitive to domain size (from 20-100km) and microphysical scheme. Results differ somewhat between the WRF and MONC models, however, for reasons that are still under exploration and could be due to microphysics. Results also differ with resolution, with the 4km-grid results differing notably from those at 1 km or 200m. This suggests that current global CRM resolutions of around 4 km may not reliably resolve the coupling of convection with large scale motions, but that a 1km grid may offer significant improvement. Results also confirm that numerical models of O(1 km) resolution, though inexact, should be able to provide reference estimates of tangent linear responses that are useful for identifying systematic errors in the behavior of traditional convective schemes.


AS03-A003
Superparameterization Improves Simulations of Mesoscale Convective Systems in E3SM

Guangxing LIN1#+, L. Ruby LEUNG2
1Chinese Academy of Sciences, 2Pacific Northwest National Laboratory

Mesoscale convective systems (MCSs) are significant contributors to heavy precipitation and flooding worldwide. Accurately representing MCSs is crucial for simulating the water and energy cycles in global climate models (GCMs). However, MCSs pose a great challenge for GCMs in no small part due to the multiscale nature of the physics and dynamics, confounding conventional convection parameterizations used in traditional GCMs. As a result, traditional GCMs have a common long-standing issue of being unable to simulate midlatitude warm-season MCSs. Usually, they show a persistent summer warm and dry bias over mid-latitudes. Here, we use a super-parameterized GCM (SP-E3SM) to simulate the MCSs in the central US. Different from the traditional GCM (E3SM), SP-E3SM uses a cloud-resolving model at 1km grid spacing within each E3SM grid column (approximately 25km horizontal grids) to simulate deep convection explicitly. Using a novel detection and tracking algorithm to characterize MCS features, we find that the SP-E3SM, compared to E3SM, better simulates MCS number and MCS precipitation amount, diurnal cycle, propagation, and the probability distribution of precipitation rate in both spring and summer. The improvement from SP is partly contributed by improvement in simulating the large-scale environments, featuring enhanced atmospheric low-level moisture and larger moisture transport to the central US relative to E3SM. Our results suggest that SP improves MCS simulation by improving the modeling of the large-scale environments and convection initiation, which are both major limiting factors in E3SM even at 25 km grid spacing where deep convection is represented by a cumulus parameterization.


AS03-A008
The Role of Convection on Troposphere-stratosphere Interactions in Radiative-convective Equilibrium Simulations

Chien-Ming WU1#+, Tzung-Yu TSAI1, Jin-De HUANG1, Shih-Hao SU2
1National Taiwan University, 2Chinese Culture University

The study investigates the role of convectively generated gravity waves in the lower stratosphere in the idealized Radiative-Convective Equilibrium (RCE) simulation using the Vector Vorticity cloud-resolving Model (VVM). The high-resolution RCE simulation was used to research the evolution and properties of convection in the tropics within fewer than 100 days. However, if the simulation time is extended, the impacts of convectively generated gravity waves on the lower stratosphere become more pronounced. We conduct a long-term RCE simulation with a long domain size and high resolution to investigate interactions between convection and the lower stratosphere. The simulation runs for approximately two years (755 days), allowing for a comprehensive analysis of the relationship between zonal wind oscillations and different convective structures. The results show that the zonal wind oscillation in the lower stratosphere is affected by the interaction between gravity waves and different structures of convection. The oscillation is observed to be asymmetric, with extremely strong westerly phases in the first two cycles and symmetric in the last two cycles. The differences in convection structures during asymmetric oscillations are found: upstream-evolving convection and aggregated convection. The difference in the environment and convection between the two types results in asymmetric oscillation in the simulation. The aggregated convection creates more convective core clouds than upstream-evolving convection, leading to a faster transition of the zonal wind oscillation. In conclusion, this study provides new insight into the impact of convective-induced gravity waves on the lower stratosphere and the relationship between zonal wind oscillations and convective structures.


AS03-A001
Response of Convection to Forcing That Creates a Cold Pool

Masaki SATOH#+, Shunnosuke NAKAI , Jun HIRAIWA
The University of Tokyo

It is known that the dynamics of cold pools generated by the evaporation of raindrops in the mixed layer play an important role in the excitation of convection in the atmosphere. In this study, assuming non-adiabatic cooling due to the evaporation of raindrops, we investigate the convection response when a cooling source is forced into the mixed layer by numerical simulations. The numerical model SCALE is used to drive a radiative-convective equilibrium state with a horizontal grid spacing of 1 km in a 96 km × 96 km double-period domain, with a uniform forcing near the center in the x-direction and the y-direction. The forcing provides a constant cooling source - 1 K/h in the region below 1 km height. The results show that for a forcing width of 2 km or more, convection is localized at both ends of the region in the x-direction, indicating that the effect of the forcing extends over the entire region. When the forcing width is 1 km, the convective suppression area is generally limited to half of the region. The case of a circular forcing in the region's center was also examined. The temperature drop at the lowest level in the forcing region is a few degrees. The balance between the strength of the mass flux and the heat supply from the sea surface determines the area of expansion of the cold pool. A similar forcing was applied to Typhoon Nanmadol in 2022 using the stretch-NICAM. A circular region of force is applied to a fixed position. The nature of the forcing that effectively affects the eyewalls and the spiral bands will be investigated. This research was supported by JST Moonshot R&D Grant Number JPMJMS2282.


AS03-A010
Effects of Diurnal Ocean Mixing on Convective Aggregation Under Different Wind Regimes in VVM with KPP

Jin-De HUANG#+, Chien-Ming WU
National Taiwan University

This study investigates the dependency of competition between the nighttime mixing and daytime heating on the wind regimes. We couple the Vector Vorticity cloud-resolving Model (VVM) with a pencil ocean model using K-profile parameterization to represent the ocean mixing. During the daytime, the shortwave radiation shallows and heats the ocean's mixed layer, which triggers convection in the dry region and delays the development of convective aggregation. The development of convective clouds in the dry area can reduce the longwave cooling in the nighttime through their moistening effect, which also prohibits aggregation development. On the other hand, the mixing due to longwave radiative cooling in the nighttime reduces SST. It enhances the dry region development, and the dry region expansion can strengthen radiative cooling. We perform two simulations with the perpetual and diurnal insolation to investigate the competition between the above feedbacks. With the diurnal cycle, the nighttime cooling feedback dominates and leads to faster development of convective aggregation compared to the simulation with perpetual insolation. The effect of nighttime mixing in convective aggregation is dependent on the wind regime. We hypothesize that increased wind speed accelerates the formation of convective aggregation. Further experiments will be conducted to validate this hypothesis.


AS03-A011
A Convective Cell Database for Cloud Process Study

Xiaowen LI1#+, Monir SHARKER1, MD Rafsan JANI1, Wei-Kuo TAO2
1Morgan State University, 2NASA Goddard Space Flight Center

We build a convective cell database using cloud-resolving model simulation data and three-dimensional image segmentation and machine learning techniques. The convective cells are the basic building blocks of atmospheric convection and convective systems. They are crucial in understanding precipitation formation and latent heat release, especially in the tropics. Understanding the full lifecycle of convective cells and their associated mass fluxes can potentially improve convection parametrization schemes in GCMs. The Goddard Cumulus Ensemble (GCE) model with the Hebrew University Cloud Model (HUCM) Spectral Bin microphysical scheme was used to simulate two convective events near Darwin, Australia during the monsoonal period of the TWP-ICE field campaign. These simulations are constrained by largescale forcing calculated from sounding observations. The horizontal resolution of the GCE model is 1km with a varying vertical resolution. The model outputs are saved every 10 minutes to be able to resolve the lifecycle of convective cells. Three-dimensional image segmentation adapted from the open source “pyclesperanto_prototype” on github is applied to the simulated vertical velocity fields. Each identified convective cell is inspected by human eyes and corrected if necessary. These cells are then tracked through time to build a database of convective cell life cycles. In this presentation, we describe characteristics of the simulated convective cells, their mean behavior, and their associated vertical mass flow, latent heating release, hydrometeor distributions, and cloud coverage.


AS03-A016
The Model Predictability of Consecutive ENSO Events: The Implication on Extreme Weather Prediction

Hann-MIng JUANG#+, Pay-Liam LIN
National Central University

The observed data show that more yearly consecutive ENSO events has been occurred since 2012, which may have links to more extreme weather events in recent years. The comparison from the model results between Taiwan CWB one-tier seasonal forecast system (TCWB1T) and NCEP CFS shows the similar performance/skill-score for hindcast year before 2012, but different scores for forecast years after 2012. TCWB1T has higher skill scores than NCEP CFS after 2012 in the forecast years, but similar skill score during the hindcast years. It implies that TCWB1T has better predictability to predict well of consecutive ENSO events. We found that the consistent time-lag in one month of ensemble member as initial conditions provide the key to have better predictability on consecutive ENSO events. Results and more findings will show.


Wed-02 Aug | 1:10 - 3:10 | MR328
AS29 - The Physical Processes Over Complex Topography: the Interactions Among Meteorology, Boundary Layer Turbulence, Clouds, Tracer Transport, and Chemistry

Session Chair(s): Wei-Ting CHEN, National Taiwan University, Shih-Hao SU, National Taiwan University

AS29-A016
Investigating Impacts of Local Circulation on Coastal Ozone Problem in the New York Metropolitan Area: A Modeling and Observational Study

Sarah LU1#+, Chin-An LIN2, Huiying LUO2
1University at Albany, State University of New York, 2University at Albany - State University of New York

Elevated surface ozone levels are often detected during hot summer days in the New York metropolitan area, including New York City (NYC), Long Island (LI), the south shore of Connecticut (CT), and the northeast corner of New Jersey (NJ), due to the rich sources of local anthropogenic and natural ozone precursor emissions. Moreover, surface ozone in this region exhibits extensive horizontal and vertical gradients and distinctive diurnal cycles when coupled with transport by complex boundary layer circulation induced by the intricate coastal geometry throughout the domain. This study first examines the spatial and temporal ozone characteristics under different cluster-based local circulation scenarios during summertime in the pre-COVID era of 2017-2019, utilizing observations from various surface networks, New York State Mesonet (NYSM) Profilers, and 2018 Long Island Sound Tropospheric Ozone Study (LISTOS), as well as composites from the High-Resolution Rapid Refresh (HRRR) reanalysis fields. The most polluted days are closely associated with classic sea breeze days with weak large-scale flow. Meteorological characteristics, such as sea breeze onset time and strength, most critical to ozone exceedances and high peaks are identified and analyzed for future improvement in coastal ozone simulation and prediction. This study then conducts regional air quality model experiments to characterize an ozone episode during the LISTOS.


AS29-A019
Characterization of the Boundary Layer Mean and Turbulence Structures Over the Heterogeneous Land Surface in Taiwan

Fang-Yi CHENG#+, Yu-Tzu WANG, Yi-Cheng LIN
National Central University

The distributions of the heterogeneous land surface and topography lead to the complexity of the atmospheric structures. To understand the interplay of the atmospheric processes over the heterogeneous areas in Taiwan, a field campaign (2013/9/3~2013/9/10) was conducted over the Puli basin, which is located in central Taiwan and surrounded by the complex topography. The characteristics of the turbulence structures were investigated over the heterogeneous areas in Taiwan, using the radial wind profiler (RWP), microwave radiometer profiler (MRP), and WINDCUBE in several places in Taiwan. To enhance the understanding of spatial variability, the numerical weather simulation with the high spatial resolution was conducted to provide the three-dimensional turbulence structures. The objectives are to characterize the mean and turbulence variations and to investigate the turbulence structures using high-resolution weather simulation and measurement. The preliminary analysis indicates a daytime well-mixed boundary layer structure in the Puli basin and a steady westerly flow prevailed in the planetary boundary layer (PBL) during the day. The interaction of the synoptic flow, sea breeze flow, and valley winds was identified from the WRF simulation at 600-m resolution. The estimation of the turbulence kinetic energy based on the observations revealed the PBL evolution process.


AS29-A020
Assimilation of the High Vertical-resolution PBL Observations During the TPOMDA Field Campaign and its Impact on Meteorological Analysis and Air-quality Simulation

Shu-Chih YANG#+, Chih-Kuan WANG, Sheng-Hsiang WANG, Fang-Yi CHENG
National Central University

This study investigates the impact of assimilating the high vertical-resolution observations on the Planetary Boundary Layer (PBL) analysis, forecast, and air quality prediction during the Taiwan Air Pollution Modeling and Data assimilation (T-POMDA) experiment. The observations include wind profilers, unmanned aerial vehicles (UAV), and Aerosond collected from 16 to 17 March 2021. The assimilation is conducted with the Weather Research and Forecasting model-Local Ensemble Transform Kalman Filter (WRF-LETKF) with rapid update cycles. Assimilation strategies with variable localization and adaptive observation error variance inflation (AOEI) are adopted to highlight the impact of assimilating the PBL observations with a high vertical resolution.
Our results suggest that assimilating the wind observations of wind profilers and Aerosond can improve the PBL dynamic structure over central Taiwan. Applying variable error covariance localization is crucial to maintain the impact of wind assimilation and avoid the negative impact on the thermodynamic structure. Due to the significant temperature variation and cold bias, the large innovation occurred easily in the PBL. Assimilating the UAV temperature observation using AOEI alleviates the overly large temperature increment and prevents the unrealistic flow in the analysis, further improving the thermal-direct land-sea breeze simulation.
The WRF-LETKF analysis is used to drive the Community Multiscale Air Quality Model (CMAQ) to obtain the air quality simulation. The assimilation of wind data with high vertical resolution corrects the structure of vertical circulation near the terrain and thus better represents the vertical transportation of the pollutants. In addition, the assimilation of UAV temperature corrects the model overcooling at night, which help to suppress the unrealistic strong land breeze and prevent the pollutants from diffusing offshore. In summary, assimilating the PBL observation with the high vertical resolution is beneficial for improving the air-quality simulation related to local emission issues.


AS29-A004
Significant Impacts of Atmospheric Boundary Layer Dynamics and Photochemistry on Fine Particulate Pollution Revealed by Intensive Vertical Observations

Min ZHANG#+, Pengfei TIAN, Lei ZHANG, Jiening LIANG, Jiayun LI
Lanzhou University

Surface fine particulate matter (PM2.5, particulate matter with aerodynamic diameters less than 2.5 μm) pollution in winter is still a vital issue of air pollution and human health, and its pollution mechanisms can be understood deeply by combining the vertical distribution of aerosols. The vertical direction dynamics and chemical processes in the planetary boundary layer (PBL) are the most significant factors affecting the above problems. However, the PBL dynamic-chemistry coupled effects lack further studies, especially the observational evidence. In this article, comprehensive observations were collected in a semi-arid city in western China in winter, including the vertical distribution of PBL dynamics, aerosol optical properties, and PM2.5 chemical composition. We found large differences in particulate pollution levels under the comparable columnar aerosol loadings due to the contrast of aerosol vertical distributions. The different Richardson number (Ri) profiles under different pollution levels, reflecting the vertical structure of the boundary layer stability, were the main reason for the differences in aerosol vertical distributions. Photochemistry is the major process for secondary aerosol formation in the semi-arid region due to the lower relative humidity (RH), which is different from humid areas. The strongest photochemistry occurred in the upper boundary layer (0.42 km) due to influences of solar irradiance and the vertical exchange of precursors. This paper provides observational evidence for the significant influence of the coupled atmospheric physical and chemical processes on the vertical distribution of aerosol and particulate pollution levels at the surface.


AS29-A006
Response of Surface Ozone to Atmospheric Aerosol Absorption is More Sensitive Than to Scattering

Xin SONG#+, Pengfei TIAN, Lei ZHANG, Jiening LIANG
Lanzhou University

Interactions between atmospheric aerosols and ozone have a significant impact on air pollution and the climate. However, the relative importance of the response of surface ozone to aerosol scattering and absorption has been poorly quantified from in situ observations. Results derived from a one-year in situ observational study conducted in a semi-arid region showed that the response of ozone to aerosol absorption was more sensitive than to scattering. Specifically, the change in surface ozone from low to high absorption coefficients was approximately five times that from low to high scattering coefficients. The mass scattering and absorption efficiencies, rather than the single-scattering albedo, which are commonly applied in numerical simulations, were able to clearly distinguish surface ozone. The positive correlation between aerosol and ozone in summer showed the promotion of secondary aerosols by ozone. This study provides robust observational evidence of the response of surface ozone to aerosol scattering and absorption.


AS29-A001
Impacts of Boundary-layer Structure and Turbulence on the Variations of PM2.5 During Fog–haze Episodes

Tingting JU1+, Bingui WU2#
1Dalian Maritime University, 2Tianjin Institute of Meteorological Science

The precise cause of PM2.5 (fine particular matter with a diameter smaller than 2.5 µm) explosive growth and the contribution of intermittent turbulence to the dispersion of PM2.5 are uncertain. Thus, the impact of boundary-layer structure and turbulence on the variations of surface PM2.5 during fog–haze episodes, especially during explosive growth and dispersion episodes, are investigated using turbulence data collected at a 255-m high meteorological tower in Tianjin from 2016 to 2018. Results suggest that the explosive growth of surface PM2.5 during fog–haze episodes is closely related to weak turbulent mixing, nocturnal inversions, or anomalous inversions, and the barrier effect of strong turbulent intermittency. Turbulent intermittency acts as a lid for hindering pollutant dispersion and is favourable for the fast accumulation of surface PM2.5. Apart from the potential causes mentioned above, the persistent moderate south-westerly flow is also a contributing factor for the explosive growth of surface PM2.5 during fog–haze episodes associated with regional transport. In addition, we demonstrate a possible mechanism of how intermittent turbulence affects the dispersion of PM2.5. Results verify that intermittent turbulence induced by the nocturnal low-level jet (LLJ) indeed plays an important role in the dispersion of PM2.5. However, the contribution of intermittent turbulence generated by the nocturnal LLJ to the dispersion of PM2.5 strongly relies on the intensity of the nocturnal LLJ.


AS29-A002
Effects of the Atmospheric Turbulence on the Vertical Transport of Dust Aerosols During Strong Sandstorm Period

Lu ZHANG#+, Hongsheng ZHANG
Peking University

An extreme sand storm hit North China from March 14 to 16, 2021. With the enhanced observations in Beijing, the effects of atmospheric turbulence on the vertical transport of dust aerosols are investigated. By effectively quantifying the turbulent dust flux and turbulence intermittency, the evolution of turbulence and its role in dust dispersion is clearly illustrated on March 15, 2021, in Beijing. Initially, turbulence was more quiescent and the turbulent exchange was suppressed significantly. Thus, despite the dust mass was advected to 300–800 m above Beijing, the dust mass concentration near the surface was negligibly increased. Then, a short turbulence burst occurred, and subsequently the elevated dust aerosols were mixed downward intensely, leading to a sharp increase in the near-surface dust mass concentration. Finally, continuous turbulence dominated and diffused dust upward, dust aerosols was gradually dissipated in the lower atmosphere. Furthermore, it is also found that the dissimilarity between the turbulent transport of dust and momentum-heat depends on the presence of dust sources. When dust sources exist, the transport of dust and momentum-heat is similar. In contrast, when there is no dust source, dust particles exhibit strong random movements, which leads to low dust transport efficiency, showing the transport dissimilarity between dust and momentum-heat.


Wed-02 Aug | 1:10 - 3:10 | MR329
AS20 - Weather and Climate Studies with High Performance Computing

Session Chair(s): Yi ZHANG, PIESAT Information Technology Co., Ltd., Chihiro KODAMA, Japan Agency for Marine-Earth Science and Technology

AS20-A011 | Invited
Impact of Ocean Layer Thickness in Storm-and-eddy-rich Global Coupled Simulations on the Climate State and ENSO Variability

Dian PUTRASAHAN1#+, Dietmar DOMMENGET2, Daniel KLOCKE1, Jin-Song VON STORCH1
1Max Planck Institute for Meteorology, 2Monash University

CMIP-type models have been widely used to make significant progress in our understanding of the climate state and variability. However, they are based on the assumption that the ocean mesoscales do not play an essential role, a necessary assumption due to insufficient computational resources. Yet, studies with coupled simulations that resolve the ocean mesoscale have revealed their implications on air-sea heat exchange, atmospheric circulation and coupling variability, counteracting the long-held notion of a passive ocean to the atmosphere. As such, quite some attention has been given to increasing horizontal resolution to resolve said processes, with critical implications on the climate state and variability. However, little attention has been given to the impact that arises from vertical resolution at the ocean surface. Here, we evaluate the influence of surface ocean layer thickness on the climate mean state and ENSO variability in simulations that resolve the ocean mesoscales and atmospheric convection. More specifically, we analyse outputs from two 30-year coupled R2B8 (10km) ICON simulations, the first multi-decadal global coupled storm-and-eddy-rich climate simulations. These simulations differ only in the thickness of the upper 20m ocean, namely the thin case has ~2m layers while the thick case has ~10m layers. Preliminary results showed that in both simulations, warm biases over the tropical east Pacific is ameliorated compared to CMIP-type simulations. Interestingly, SST variability over tropical Pacific is larger in the thick case compared to the thin case, with implications on ENSO variability. SST variability through its response to winds, has a large impact on thermocline variability in both cases. However, the two-way coupling whereby thermocline variability in turn feeds back to SST variability only occurs in the thick case. Indeed, ENSO has no interannual variability in the thin case, while a strong 3-year oscillation is seen in the thick case.


AS20-A001
An Overview of the Development of a Unified Weather-climate Model System (GRIST) in China

Yi ZHANG1#+, Jian LI2, Xiaohan LI1, Zhuang LIU3, Yihui ZHOU2, Xindong PENG2,4, Xinyao RONG5, Yiming WANG1, Rucong YU2
1PIESAT Information Technology Co., Ltd., 2Chinese Academy of Meteorological Sciences, 3Tsinghua University, 4CMA Earth System Modeling and Prediction Centre, 5CMA Earth System Modeling and Prediction Center

GRIST is a unified weather–climate model system. It was created in response to the requirement for, and calls to develop, unified weather and climate modeling in China. This “unification” process was pursued following two routes: (i) maximizing the possibility of constructing weather and climate models using a single model framework and dynamical core; (ii) maximizing the possibility of using a unified model formulation which requires minimal application-specific changes for weather-to-climate forecast applications that are relevant to most operational business demands. This talks gives a review on the general features of the model framework, its dynamical core and physics-dynamics couping. Model applications from typical global AMIP climate simulations, operational numerical weather prediction, and high-resolution experimental global storm-resolving simulations are presented and discussed. Future model development and application efforts will be briefly outlined.


AS20-A008
Improved Climate Simulation by Using a Double-plume Convection Scheme in a Global Model

Xiaohan LI1#+, Zhou BAIQUAN2
1PIESAT Information Technology Co., Ltd., China, 2Chinese Academy of Meteorological Sciences

Convective parameterization can drastically regulate the mean climate and tropical transient activity of a general circulation model. In this study, the physics suite of the NCAR Community Atmosphere Model, version 5 (CAM5) was first ported to the GRIST (Global-to-Regional Integrated Forecast System) model. Then, the original convective parameterization of CAM5—with a separate representation of deep convection (Zhang–Mcfarlane; ZM) and shallow convection (University of Washington; UW)—was replaced by a double-plume (DP) scheme. This DP scheme adopts a quasi-unified representation of shallow and deep convection within a single framework. Results demonstrate that the new scheme brings about several improvements in the modeled climate. The differences in the trigger and closure assumptions, lateral mixing rate, and cloud model for the deep convection result in systematic regional differences in the simulated precipitation pattern, cloud vertical structure, and the associated radiative forcing. Compared with ZM-UW, DP reduces the biases in precipitation over the Indian Ocean, ameliorates the “high-frequency and low-intensity” problem of tropical precipitation, and leads to an improved representation of tropical variability, including the Madden–Julian Oscillation. DP reduces low clouds and increases high clouds in the tropics, due to its internal parallel-split convective processes and smaller cumulus cloud fraction. Discussions related to parametric tuning of convective parameterization are also presented.


AS20-A021
Progress and Challenges of Kilometer-scale Atmospheric Climate Simulations with NICAM

Daisuke TAKASUKA1#+, Chihiro KODAMA2, Tamaki SUEMATSU3, Tomoki OHNO4, Yohei YAMADA2, Tatsuya SEIKI2, Hisashi YASHIRO5, Masuo NAKANO2, Hiroaki MIURA1, Akira NODA2, Tomoe NASUNO2, Tomoki MIYAKAWA1, Ryusuke MASUNAGA2
1The University of Tokyo, 2Japan Agency for Marine-Earth Science and Technology, 3RIKEN, 4Meteorological Research Institute, 5National Institute for Environmental Studies

A global kilometer-scale (K-scale) “convection-resolving” model (GCRM) simulation on the climate time scale is expected to be advantageous to the seamless representation of various kinds of phenomena related to cloud processes. Meanwhile, we have also known that the good reproducibility of both climatological statistics and weather disturbances is not straightforward, and that there exist resolution-independent model errors at least for O(1–10)-km grid spacing. Considering that this situation partly comes from the poor constraint of a moisture-convection relation depending on model physics even on a K-scale, we have revised the settings of cloud microphysics, turbulent diffusion, and vertical resolutions in the Nonhydrostatic ICosahedral Atmospheric Model (NICAM) for a K-scale climate simulation. After this revision, we are now performing a 10-year AMIP-type simulation at 3.5-km horizontal mesh on a Japanese flagship supercomputer “Fugaku”. A preliminary analysis of about 5-year integration reveals that both the model revisions and K-scale horizontal resolution can improve the reproducibility of many atmospheric aspects over a wide range of spatio-temporal scales (e.g., mean precipitation and OLR distributions, mid-latitude westerly jets, monsoon, MJO, tropical cyclone intensity, and precipitation diurnal cycle). However, it is still non-trivial how low clouds are appropriately simulated in the K-scale GCRM framework, which should be resolved in the ocean-coupled climate run in which the energy balance is important. This work can be a clue for understanding the merits and limitations of a K-scale GCRM climate simulation and providing a strategy for the future model development.


AS20-A014 | Invited
High-resolution Weather and Climate Modelling at CCRS: Current Status and Future Priorities

Hugh ZHANG1#+, Dale BARKER2, Aurel MOISE3, Joshua LEE3, Song CHEN3, Rajesh KUMAR3
1CCRS, 2Centre for Climate Research Singapore (CCRS), 3Centre for Climate Research Singapore

The Centre for Climate Research Singapore (CCRS) is a research centre and part of the Meteorological Service Singapore (MSS). This presentation is used to give a brief overview of the current high-resolution modelling system being developed at CCRS. In recent years, enhanced supercomputing power has enabled us develop the high-resolution regional ‘SINGV’ Numerical Weather Prediction (NWP) system at 1.5km resolution with advanced data assimilation of ground- and space-based weather observations. We have further developed a seamless weather and climate modelling approach by configuring the SINGV NWP model for use as a regional climate model (SINGV-RCM) in the Third Singapore National Climate Change Study [V3], with a model resolution down to 2km in our region.
The weather and climate of Southeast Asia are heavily influenced by strong feedbacks between the atmosphere, ocean, waves and land. Thus, one of our current priorities is to develop a unified ‘cSINGV’ coupled environmental prediction system at 1.5km resolution, which helps improve the accuracy of very short-term weather forecasts and long-term climate change projections, and allows us to provide consistent weather, climate and marine forecasts for all users. At the same time, we are focused on developing urban (~100m) ‘uSINGV’ prediction system that provides improved representation of key processes governing local weather and allows us to provide more specific local and/or regional weather and climate information. We welcome collaborations with regional and global partners to improve our modelling capability in tropical Southeast Asia which, as the “engine room“ of the global climate system, has far-reaching impacts for other regions of the world.


AS20-A003
Global-regional-unified Modeling of Atmospheric Phenomena on the Yin-yang Grid

Xindong PENG1,2#+, Siyuan CHEN1, Yifan ZHAO1, Xiaohan LI3
1Chinese Academy of Meteorological Sciences, 2CMA Earth System Modeling and Prediction Centre, 3PIESAT Information Technology Co., Ltd.

A global-reginal-unified atmospheric model, Yin-Yang-grid Unified Model for the Atmosphere (YUNMA), is developed for flexible weather simulation using a semi-implicit semi-Lagrangian solver. With the help of arbitrary coordinate rotation and convenient switch between global and regional choices, easy configuration of model domains is possible for either global or regional run with nesting-grid refinement. Numerical performance of the dynamical core was confirmed using a series of numerical benchmark tests on sphere. An average convergence rate of the dynamical core reached 2.43 in the balanced flow test, and rotation of the Yin-Yang grid showed positive impact on the simulation even though generally did not affect the basic flow pattern and average numerical error, as shown in the balanced flow test and the terminator chemical reaction test. Local refinement and limited-area high-resolution simulation improved the numerical results in the baroclinic wave test, and achieved similar development of baroclinic waves as the global high-resolution run with significantly low cost. Transport of vortices in the colliding modons test showed unique features in comparison with existing simulations. Travel distance and vorticity amplitude varied with model resolution and time step explicitly in the global model, which is consistent with published results. In a nested model, however, the vortex enhanced just the same as in the global high-resolution model, but traveled a distance the same as in the low-resolution global (parent) model, which illustrates the impact of lateral boundary condition on the modons propagation. With terrain data introduced, the development of topographic gravity wave and topographic Rossby wave was proved very well in the YUNMA dynamic core, which confirms the correctness of the global-regional-unified model development. Global 10-km- and regional 3-km-resolution results of a real case simulation will be shown in this presentation.


AS20-A005
A Revised Gaussian Filter Technique for Stabilizing Explicit Atmospheric Model on the Latitude-longitude Grid

Li DONG#+
Chinese Academy of Sciences

The pole problem has been hindering the horizontal resolution increment of the global atmospheric models on the latitude-longitude grids due to the stringent limit on the time step size. Some implicit or semi-implicit methods were designed to increase the stability of the models, but the algorithms used to solve the large matrix systems are very complex and unfriendly to massive parallel computers. This study tried to solve this problem by devising an effective Gaussian filter so that the explicit time step can be large enough and the numerical accuracy is preserved as much as possible. The filter is applied in the zonal direction, and its kernel width is decreased smoothly according to the zonal Courant-Friedrichs-Lewy (shortly as CFL) condition from the pole to the equator. The tendencies are filtered so that the zonal spatial scale is enlarged to improve the numerical stability in the polar region. Meanwhile, the 2D horizontal decomposition parallel implementation is optimized so that only filtered arrays have large zonal halo width. Several test cases are applied to demonstrated the efficacy of this new technique.


AS20-A018
An Assessment of the Simulation of East‐Asia Precipitation in the High‐resolution Community Earth System Model

Mingkui LI#+, Guang YANG, Shaoqing ZHANG
Ocean University of China

Data analyses of long-term historical experiments using version 1.3 of the Community Earth System Model with 100 km resolution for both atmosphere and ocean (low-resolution, LR), and 25 km resolution for atmosphere and 10 km resolution for ocean (high-resolution, HR), were conducted to study the impact of model horizontal resolution on the simulation of East Asian precipitation. The features analyzed here include long-time mean spatial distribution, intra-seasonal variabilities, and probability of frequency and intensity. Due to the finer grid resolution, the better simulation of convection and water vapor transport conditions, the long-time mean spatial pattern of precipitation in the HR is much closer to the observation compared to the LR simulation, especially the rain belt along the south edge of the Tibetan Plateau associated with complex topography. Although the HR slightly improves the intra-seasonal evolution of East Asian precipitation, on the whole, the inaccurate simulation of circulation characteristics in the middle and upper troposphere amplifies the simulation bias of the rain belt position. The daily time scale precipitation was evaluated by intensity-frequency structure, indicating that the finer resolution makes the simulation more reasonable, especially in monsoon regions. Although there are aspects that need to be further improved in the HR simulation, the HR model bias in East Asian precipitation is overall smaller compared to that of the LR.


Wed-02 Aug | 1:10 - 3:10 | MR331
AS23 - Observations, Remote Sensing, and Modeling of Tropospheric Composition and Air Quality in Asia and the Transpacific Region

Session Chair(s): Hongbin YU, NASA Goddard Space Flight Center, Meiying Melissa MARTIN, NASA

AS23-A063 | Invited
WMO Vegetation Fire and Smoke Pollution Warning Advisory and Assessment System (VFSP-WAS) - Supporting Sustainability Efforts in Southeast Asia

Boon Ning CHEW1#+, Alexander BAKLANOV 2, Sara BASART2, Mikhail SOFIEV3, Bambang H. SAHARJO4, Goldammer JOHANN GEORG5
1Centre for Climate Research Singapore, 2World Meteorological Organization, 3Finnish Meteorological Institute, 4Regional Fire Management Resource Center - South East Asia, 5Global Fire Monitoring Center

Vegetation fires, including the applications of fire in land use, land-use change and uncontrolled wild fires, are sources of severe smoke pollution, and impact the environment and public health. WMO has responded to urgent requests from smoke-impacted regions by initiating the Vegetation Fire and Smoke Pollution Warning Advisory and Assessment System (VFSP-WAS). In Southeast Asia, VFSP-WAS is hosted by the ASEAN Specialised Meteorological Centre (ASMC), and partners with the Regional Fire Management Resource Center (RFMRC) - a regional branch of the Global Fire Monitoring Center (GFMC) - to provide guidance to address smoke and fire dangers. The VFSP-WAS smoke forecasts for the region are given as an ensemble product combined from 5 global models (ECMWF-CAMS, JMA MASINGAR, NASA GEOS-5, NOAA GEFS-Aerosols, FMI SILAM) and a regional model (MSS-UKMO NAME). Here, we introduce VFSP-WAS and its mission, and discuss how these ensemble forecasts, together with other ASMC's data products and RFMRC's work with the stakeholders on the ground, can be used to assess and forecast population exposure to smoke, mitigate fires, and enable more sustainable developments in the fire-impacted regions.


AS23-A048 | Invited
Top-down Model-free Estimation of Emissions of BC, CH4, CO, and NOx in Tandem: Increased Emissions and Radiative Forcing in Rural Areas Overwhelm Reductions in Emissions and Radiative Forcing Variability in Urban Areas

Jason COHEN#+
China University of Mining and Technology

Black carbon (BC), NO2, CO and CH4 tend to be underestimated by models in rapidly developing and changing areas of Asia, which is at odds with regulations and incentives employed to improve air quality and reduce climate altering species. Recent advances in analyzing large datasets, and the ability to merge multiple overlapping measurements in space, time, and across the radiative spectrum, have led to new methods to detect signals and quantify patterns which were not previously realized. This work does this by merging mass conservation, number conservation, first order thermodynamics and chemistry, core/shell MIE modeling, and remotely sensed measurements across the UV, VIS, and NIR in tandem. Thermodynamics of combustion, driven by the type of fuel and energy usage, constrain the ratios between co-emitted species. First order in-situ chemistry and advection generate temporally and spatially varying fields. Core-Shell MIE models and inverse solutions across many possible outcomes are used to constrain physically realistic solutions across all measurements. Uncertainty bounds are harmonized across unique retrievals of all species. Total errors are explored and are found to generally be smaller than day-to-day and grid-to-grid variability. A few conclusions are discussed. First, regulations effectively reduce emissions in urban centers, powerplants, steel-plants, and concrete-plants. Second, new sources and increased existing sources in suburban/rural areas lead to increased emissions in these regions. Third, biomass burning is identified and attributed, and found to be impactful over a much wider region than previously identified, including the megacities of Hong Kong, New Delhi, and Shanghai. Fourth, there are additional significant impacts attributed to changes in UV radiation and atmospheric transport. Fifth, there are significant biases observed in the TOA radiative forcing, with the aerosol effects resulting in a generally less negative TOA.


AS23-A049 | Invited
The Diurnal Variation of Pollutant Distributions Over Asia Using Observations from the Geostationary Environment Monitoring Spectrometer (GEMS)

David EDWARDS1#+, Sara MARTINEZ-ALONSO1, Duseong JO1, Ivan ORTEGA1, Louisa EMMONS1, Helen WORDEN1, Jhoon KIM2
1National Center for Atmospheric Research, 2Yonsei University

The new-generation geostationary (GEO) satellite perspective, with high spatial resolution and hourly measurements, represents a major step forward in capability for understanding how air quality processes change diurnally at the local scale. South Korea's Geostationary Environment Monitoring Spectrometer (GEMS) was launched in February 2020 over Asia and is the first member of the GEO constellation that will eventually include the Tropospheric Emissions: Monitoring Pollution (TEMPO) mission over North America, and Sentinal-4 over Europe. The measurement hourly time resolution is truly the new perspective that the GEO platform provides, and in this presentation, we use a combination of satellite observations from GEMS and chemical transport model simulations to investigate the diurnal variation of pollution over several Asian regions. For a reactive gas such as nitrogen dioxide (NO2), the magnitude of the diurnal change is often very large as are the hour-by-hour changes in the spatial distribution. To help understand daily differences in diurnal patterns at regional and local scales, we use the Multi-Scale Infrastructure for Chemistry and Aerosols (MUSICA-V0). This uses a global modeling framework with regional grid refinement to resolve chemistry at emission and exposure relevant scales. The model also allows the drivers of variability due to emissions, meteorology, and photochemistry to be considered separately. Comparing with LEO observations of carbon monoxide (CO) from MOPITT (morning overpass) and CrIS and TROPOMI (afternoon overpass) also allows helps differentiate combustion sources. The results of this analysis are further compared with the NO2 diurnal variability observed by PANDORA sun spectrometer measurements at polluted and less-polluted Korean and other Asian sites. We investigate spatial scale, including the city-scale within Seoul, at which GEMS captures the differences in diurnal variability between the PANDORAs.


AS23-A015
Characteristics of Spatiotemporal Distribution of OMI NO2 VCDs in Southeast Asia (2005-2019)

Ja-Ho KOO#+, Nahyun LEE, Donghee LEE
Yonsei University

NO2 is one of representative trace gases strongly affecting the local air pollution. Compared to other trace gases, satellite can observe the NO2 density with a reliable quality, enabling us to see the spatiotemporal pattern of NO2 for a long-term period in a continental scale. In this context, we tried to investigate the spatiotemporal distribution of NO2 vertical column density (VCD) using the Ozone Monitoring Instrument (OMI) dataset, which is the well-known polar orbit satellite observation. At first, we examined the long-term (from 2005 to 2019) trend of NO2 VCDs in 10 Association of Southeast Asian Nations (ASEAN) countries in Southeast Asia. As a result, countries in the Indochinese Peninsula show the increasing trend (e.g., 1.93 %/year in Laos and 2.24 %/year in Vietnam), but countries in the tropical region show the decreasing trend (e.g., -0.66 %/year in Malaysia and -0.88 %/year in Indonesia). We also found that NO2 enhancement in Laos and northern Vietnam is strongly related to the high number of fire count measured by another satellite sensor, the Moderate Resolution Imaging Spectroradiometer (MODIS), indicating the significant contribution of wildfire to the local NO2 concentration. One more interesting characteristic is that this region (Laos and northern Vietnam) mostly show the higher NO2 after the COVID-19 outbreak, which is much different from previous findings addressing the NO2 decrease resulted from the weakened anthropogenic emission after the COVID-19 outbreak. This feature implies that the wildfire plays a dominant role of NO2 emission here, different from the large contribution of anthropogenic emission of other industrial regions. Acknowledgement: 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).


AS23-A064
Investigating Transport and Environmental Impacts of the Strongest Asian Dust Event Over the Past Decade in China

Tianle ZHANG1+, Mei ZHENG1#, Xiaoguang SUN2, Huanhuan CHEN3, Yuntao WANG4, Xuehua FAN2, Yubing PAN5, Jiannong QUAN6, Junyi LIU1, Yinan WANG2, Daren LYU2,7, Shuangling CHEN3, Tong ZHU1, Fei CHAI3
1Peking University, 2Chinese Academy of Sciences, 3Ministry of Natural Resources, 4State Oceanic Administration, 5Institute of Urban Meteorology, 6Institute of Urban Meteorology, 7University of Chinese Academy of Sciences

In March 2021, China experienced three dust events (Dust-1, 2, 3), especially the first of which was reported as the strongest one in recent ten years, covering an area of >3.80 million km2 (about 40% of land area of China). Multiple advanced measurements, including satellite, ground-based lidar, online aerosol speciation instrument, and biogeochemical Argo float, were applied to examine the transport paths, optical and chemical properties, and impacts on urban air quality and marine ecosystem. Our results showed that Dust-1 exhibited the largest impact on urban area, increasing PM10 concentration to 7525 μg/m3 in Beijing, and the absorbing aerosol index retrieved from satellite was as high as 3.3. In addition, during these events, particles were enriched with crustal elements while the concentration of pollution elements was low, and the depolarization ratio of these particles measured by lidar was 0.3-0.4. The transport paths of dust were also examined. Although Dust-1 was the strongest among three, due to fast movement of the Mongolian low-pressure cyclone, most dust retained on the land and cannot be transported to the northwestern Pacific, resulting in limited impact on the ocean. Dust-2 and Dust-3, though weaker in intensity, were transported directly to the sea, leading to a substantial increase in chlorophyll-a concentration (up to 3 times) in the northwestern Pacific, comparing to its climatological value. We find that the impacts of dust events on ocean was not necessarily and positively correlated to their impacts on land. Based on the integrated analyses of land-ocean-space monitoring data and synoptic systems, this study quantitatively assessed the overall impacts of super Asian dust storms both on land and ocean. The methodology developed in this study could also serve as a reference for future research on strong aerosol emission events such as wildfire and volcanic eruption.


AS23-A010
Sub-grid Variability of Column NO2 at Industrial Point Sources in Korea Inferred from Airborne Hyperspectral Observations

Jong-Uk PARK1#+, Sang-Woo KIM1, Jin-Soo PARK2, Hyunjae KIM2, Jin-Soo CHOI2, Sangseo PARK3
1Seoul National University, 2National Institute of Environmental Research, 3Ulsan National Institute of Science and Technology

Nitrogen oxides (NOx) are one of the key atmospheric pollutants in the urban atmosphere from its innate health effect and enrollment in the atmospheric photochemistry forming ozone (O3) and secondary aerosols. Various hyperspectral satellite sensors have successfully captured NOx emission hot-spots worldwide by retrieving NO2 concentrations from spectral fitting (i.e., DOAS), but not in sufficient spatial resolution considering the highly variable character of NOx in the polluted atmosphere. In this study, high-resolution NO2 vertical column densities (VCD) were obtained from the airborne low-cost hyperspectral imaging sensor (HIS) observations at two major industrial source regions (i.e., coastal area in Chungnam-province and Pohang) in Korea to examine the NO2 spatial variability in the scale below the resolution of the state-of-art satellite observations (i.e., TROPOMI) near the emission hot-spots. NO2 VCDs from the airborne HIS observations were retrieved using the modified wavelength-pair method to overcome the instrumental defects in the spectral resolution and the precision of calibration, and spatial kriging was applied to achieve full spatial coverage based on the variogram representing spatial continuity along and across the wind at the time of observation. Kriged NO2 VCD field well captured the localized NO2 plume and the dispersion-advection pattern with the high concentration on its center (> 1.1 DU) and sharp gradient on its lateral peripheries, whereas the collocated TROPOMI swath exhibited relatively lower peak values (< 1.0 DU) from the spatial averaging effect of the pixel footprint area and failed to resolve exact plume structure. Although the current study is based on a limited number of observations, further HIS airborne observations over major source regions in Korea (i.e., megacities such as Seoul Metropolitan Area) will enable quantifying the sub-grid inhomogeneity of NO2 VCD in the polluted region in East Asia and elucidate the inherent uncertainties of satellite observations from its limited spatial resolution.


AS23-A004
Top-down Nitrogen Oxide Emissions Based on TROPOMI Observations

Yi-Chun CHEN#+, Charles CHOU, Chian-Yi LIU, Szu-Yu CHI, Ming-Tung CHUANG
Academia Sinica

To compensate for the emissions missed or underestimated in the national bottom-up emission inventories, we apply the high spatial resolution satellite data from TROPOspheric Monitoring Instrument (TROPOMI) to estimate the top-down nitrogen oxide (NOx) emissions in regional scales. The NOx chemical lifetime is derived based on ground-based measurements of ozone photolysis rate, ultra-violet index, and temperature. For western Taiwan, the derived lifetime is about 1 to 2 h in summer and 2 to 4 h in winter. The retrieved emissions for regions near major pollution sources (e.g., Taichung thermal power plant and Mailiao Industrial Zone) are comparable with the emission from the Continuous Emission Monitoring System. After validating the data and methods, the NOx emissions for different regions of western Taiwan are derived and applied to evaluate the bottom-up inventories. For northern and southern Taiwan, the top-down emissions agree well with emission inventories. The top-down emissions are 12%-23% higher than emission inventories for north-central to south-central Taiwan, indicating that the bottom-up inventories are underestimated, which may be associated with the uncertainties from traffic sources. Given the various complex pollution sources, deriving NOx emissions from space allows us to acquire a better understanding of emissions on urban scales and improve the bottom-up emission inventories.


AS23-A037
Global Temperature Dependency of Satellite Formaldehyde (HCHO) Columns: Implications to Isoprene Emissions

Xicheng LI1+, Lei ZHU1#, Isabelle DE SMEDT2, Wenfu SUN3, Lei SHU4, Dakang WANG5, Song LIU1, Yuyang CHEN1, Dongchuan PU1, Juan LI1, Shuai SUN1, Xiaoxing ZUO1, Weitao FU1, Xin YANG1, Tzung-May FU1
1Southern University of Science and Technology, 2Belgian Institute for Space Aeronomy, Federal Space Pole, 3Royal Belgian Institute for Space Aeronomy, 4Fujian Normal University, 5Guangzhou University

Temperature is the most influential driver of biogenic isoprene emissions and its oxidation production HCHO. We revisit such a temperature (T-) dependency here in a global manner using HCHO columns retrieved from the TROPOspheric Monitoring Instrument (TROPOMI) satellite. We find T-dependency of HCHO columns varies significantly among PFTs, with the highest for Broadleaf Evergreen Tropical Trees (HCHO columns double every 6.0 K ± 4.0 K) and the lowest for Broadleaf Deciduous Temperate Tree (double every 27.6 K ± 3.5 K). T-dependency of TROPOMI HCHO columns is inconsistent with that of isoprene emissions estimated by the Model of Emissions of Gases and Aerosols from Nature (MEGAN), likely due to MEGAN lacking PFT-specified T-dependency parameters.


Wed-02 Aug | 1:10 - 3:10 | MR332
AS30 - Mesoscale and Orographic Effects on Airflow, Precipitation and Weather Systems

Session Chair(s): Cheng-Ku YU, National Taiwan University, Tetsuya TAKEMI, Kyoto University

AS30-A019 | Invited
High-resolution Numerical Simulation of the Record-breaking 2018 Kauai Flooding

Pao-Shin CHU1#+, Xiao LUO1, Cheng-Ku YU2
1University of Hawaii, 2National Taiwan University

On April 13-15, 2018, Kaua‘i of the Hawaiian Islands received record-breaking rainfall, setting a new U.S. 24-h record. During this 24-hour extreme rainfall event, Waipā Garden, which is located in the northern coast of Kauai, has experienced three torrential rainfall episodes. During the 2nd and 3rd episodes, the storm moves eastward and expands southward over Kauai. The WRF simulation can realistically reproduce the spatial pattern of the 24-hour accumulated rainfall, the evolution feature of the storm, and the observed record-breaking rainfall intensity. Simulation results indicate that the rainfall drives the low-level circulation response. The rainfall-related downdraft forms a cold pool in the rear of the thunderstorm, and the associated surface high anomaly leads to anomalous northerly wind intruding into the northern coast of Kauai. Correspondingly, the enhanced low-level convergence results in intensified rainfall at Waipā Garden. The sensitivity experiment further suggests that the terrain in Kauai plays an important role in enhancing storm-related rainfall over Kauai. When the terrain height over Kauai is reduced by 80%, the simulation shows that the rainfall over Kauai is largely reduced.


AS30-A004
Orographic-induced Winds Seen from WISSDOM Under the Clear-air Condition: A Case Study on 14 February 2018

Chia-Lun TSAI1#+, Kwonil KIM2, Yu-Chieng LIOU3, Gyu Won LEE4
1Chinese Culture University, 2Stony Brook University, 3National Central University, 4Kyungpook National University

The WISSDOM (Wind Synthesis System using Doppler Measurements) synthesis scheme was developed to derive high-resolution 3-dimensional (3D) winds over complex terrain under clear-air conditions. A strong wind case associated with a low-pressure system (LPS) was selected to evaluate its performance and document the possible mechanisms in Pyeongchang, South Korea. The size of the test domain is 12 × 12 km2 extended up to 3 km height mean sea level (MSL) with a remarkably high horizontal and vertical resolution of 50 m. The results indicate that the derived winds reveal good patterns with a control run, similar to the sounding observations. A series of sensitivity tests with different weighting coefficients, the radius of influence (RI) in interpolation, and various combinations of different datasets were also performed. The current setting of the control run is the optimal reference to WISSDOM synthesis in this case. The evolution of surface winds shows quite different patterns, exhibiting intensification of strong winds in the lee side and periodically persistent strong winds in upstream mountainous areas with the approaching LPS. The surface wind speed was significantly intensified at a lee side surface station. The pressure gradient force (PGF) contributed from adiabatic warming, and the passage of LPS was the main factor in accelerating the surface wind on the leeward side of the mountains. The PGF also modulated the background winds at the mountainous station, which caused persistent strong and periodic winds related to the channeling effect. The evidence showed that under the same synoptic condition of a LPS, different mechanisms are essential for strong winds in determining the strength and persistence of orographic-induced strong winds under clear-air conditions.


AS30-A015
Development of a Seeder-feeder Orographic Precipitation Model in the Typhoon Environment

Lin-Wen CHENG#+, Cheng-Ku YU, Syuan-Ping CHEN
National Taiwan University

Recent studies of tropical cyclones (TCs) have suggested that the seeder-feeder process is one of the important mechanisms contributing to the orographically enhanced precipitation as TC’s circulation and precipitation approach and interact with mountain barriers. In an effort to provide a theoretical quantification on the seeder-feeder process in the typhoon environment, this study develops an idealized seeder-feeder orographic precipitation model and uses the model to simulate the precipitation distribution over Da-Tun Mountain (DT) under the influence of Typhoon Meari (2011). The high spatial and temporal resolution radar data and dense rain gauge observations available over DT (~1 km MSL) are used for the model verification. The observational analyses show that the accumulated rainfall over DT can exceed 280 mm within 10 h as Meari brought strong north-northwesterly flow impinging on this mountain barrier. The rainfall maximum was found near the northwestern (i.e., windward) ridge of DT and its leeward side. In this model, the upper-level seeder cloud is hypothetically originated from and approximated by the background precipitation valid at the 4-km MSL seen from radar observations, whereas the lower-level feeder cloud is assumed to be generated exclusively by the condensation due to upslope lifting. The growth of the seeder cloud as it falls into the layer of the feeder cloud is based on the warm-rain collision-coalescence process. It is found that the spatial distributions and accumulations of modeling rainfall are similar to those of the observations. The time series analysis of precipitation intensity also indicates that the model can provide an evolving trend generally consistent with the actual observations. However, some minor but important differences in rainfall distribution and intensity between the modeling and observational results are also noted. These aspects and their underlying reasons will be further discussed in the presentation.


AS30-A001
Effect of Boundary Layer Process on Snowfall in Beijing Under Complex Terrain

Bo YU#+
Beijing Meteorological Service

Snowfall is a complex weather process, and the internal changes of the shallow boundary layer play a vital role in the occurrence and development of snow. At present, the limited understanding of the winter boundary layer process has become an important reason for restricting the accuracy of snow forecast in Beijing. In recent years, the failure of the snow air report shows that the water vapor transport and dynamic convergence effects caused by the internal changes of the boundary layer play a key role in the snow weather in Beijing, regardless of the influence of the obvious synoptic scale system. Based on the difficulties of winter snowfall forecast in Beijing, The formation mechanism of snow dominated by the shallow boundary layer process, which is difficult to predict under complex terrain conditions, is revealed, and a physical conceptual model is established. Beijing is surrounded by mountains on three sides and close to the Bohai Sea, resulting in winter snowfall is often affected by the easterly wind in the boundary layer. The easterly wind in the boundary layer itself has the role of water vapor transport and dynamic uplift, which has an important impact on the formation and development of snowfall. It is clearly pointed out that the easterly wind in the boundary layer during the snowfall process in Beijing is not entirely caused by the return cold air, and the influence of the easterly wind in the boundary layer with different thermal and humidity characteristics on the snowfall is different. This study systematically reveals the difference of contribution of different types of boundary layer easterly in different weather background snowfall, and qualitatively describes the impact of boundary layer easterly wind and synoptic scale system on snowfall.


AS30-A024
Simulation of Flow Around a Flat Obstacle Placed in a Rotating Stratified Flow

Reina ORITA#+, Tetuya KAWAMURA, Tsubasa KOHYAMA
Ochanomizu University

In this study, assuming a situation in which a flat obstacle is placed in a rotating stratified flow, numerical simulations were carried out to investigate the structure of the flow when the flow passes through the obstacle. An interesting example of such a flow is the Karman vortex observed behind Jeju Island in Korea. The existence of the Karman vortex street has been confirmed by satellite images of clouds, which form well above the island. This indicates that the influence of the island extends far above the island. Therefore, the effects of Earth rotation and stratification are thought to play an important role. The incompressible Navier-Stokes equation with the Coriolis force as an external force and the equation of continuity (the advection equation for density that expresses the incompressibility condition) were used as the basic equations. These basic equations were solved using the fractional step method. At this time, the advection term was approximated by the upstream finite difference method with third-order accuracy so that calculations can be stably performed even at high Reynolds numbers. A turbulence model was not used. As described above, the flow is considered to be affected by the flow velocity, the magnitude of the Coriolis force, and the strength of the density stratification. Therefore, we systematically changed these parameters and examined their effects on the flow.


AS30-A018
Convective Characteristics of Outer Tropical Cyclone Rainbands and Their Similarity with Squall Lines

Brian JENG#+, Cheng-Ku YU, Che-Yu LIN
National Taiwan University

Tropical cyclone rainbands (TCRs) are a complex precipitation system with a lot of possible causes and uncertainties which trigger heated discussion among researchers. TCRs can be divided into inner and outer rainbands based on the degree to which convection is influenced by the inner-core vortex circulation. Previous research suggests that outer TCRs (OTCRs) develop in an environment with relatively larger convective available potential energy (CAPE) and frequently exhibit structural and surface characteristics similar to ordinary convective systems such as squall lines. In this study, radar measurements and high temporal resolution surface observations are used to further explore the degree of similarity between OTCRs and squall lines from a comprehensive OTCR dataset. A convective intensity index (CII) and squall-line similarity index (SSI) are developed based on fuzzy logic. CII quantifies the convective intensity of OTCRs and SSI determines the degree of similarity between OTCRs and squall lines, both of which range from 0 and 1. A total of 216 OTCR cases associated with 97 TCs as they approached Taiwan are identified during 2002-2019, together with six squall line cases and 24 surface station passages that are chosen for the analysis. Most of the OTCRs exhibit a certain degree of similarity with squall lines, with only about 30% of the analyzed OTCRs possessing a higher similarity with squall lines (i.e., SSI > 0.5). These results suggest that the convective characteristics associated with OTCRs are more complicated and diverse compared to typical squall -lines.


AS30-A003
Influence of Complex Terrain on the 21.7 Zhengzhou Extreme Rainfall

Peng WEI#+, Xin XU
Nanjing University

On 20 July 2021, an extremely heavy rainfall event occurred in Zhengzhou, North China (hereafter, the 21.7 extreme rainfall event). The 24-hr rainfall reached up to 682.5 mm, with an extreme hourly rainfall rate of 201.9 mm that broke the record in mainland China. This extreme rainfall event was poorly predicted by even the state-of-the-art global numerical weather prediction (NWP) models. Specifically, the predicted rainfall by the ECMWF and NCEP models was biased to the west of observation. Moreover, the amount of predicted rainfall was much lower than in reality. The possible influence of unresolved orography in global NWP models on the 21.7 extreme rainfall event was studied using the MPAS model with a resolution of 15 km. Two numerical experiments were conducted with and without the parameterization of subgrid-scale orographic drag (SOD), respectively. Results showed that the extreme rainfall was closely related to a low-level mesoscale vortex. The SOD induced a high pressure over the mountains to the west of Zhengzhou which prevented the westward movement of the low-level vortex. The SOD also weakened the vortex by decelerating the horizontal winds. However, the water vapor flux convergence was enhanced in Zhengzhou. Therefore, the rainfall was enhanced compared to no SOD. We further investigated the key dynamical processes that supported the hourly extreme rainfall using a convection-permitting WRF simulation. The extreme-rain-producing storm was maintained by the dynamic lifting of three-way converging flows. The low-level northerly flow originated from a mesoscale barrier jet on eastern slope of the Taihang Mountain due to terrain blocking, which reached an overall balance with the southerly winds associated with a low-level meso-β-scale vortex. The large-scale easterly inflows that fed the deep convection prevented the eastward propagation of the cold pool. The convective storm was nearly stationary over Zhengzhou, resulting in the record-breaking hourly rainfall.


AS30-A006
Characteristics of Cold Air Damming and its Effect on Snowfall in the Yeongdong Region of Korea

Younggil CHOI1, Ji Yun KIM1+, Han JINHEON1, Kim TAE YEON1, Byung-Gon KIM1#, Byunghwan LIM2, Gyu Won LEE3
1Gangneung-Wonju National University, 2National Institute of Meteorological Sciences, 3Kyungpook National University

The Yeongdong region has lots of snowfall in winter because of the Taeback mountain range and adjacent East Sea. Severe snowfall generally tends to be accompanied with strong cold air outbreak of northerly and northeasterly.
We investigate characteristics of cold air damming and its effect on snowfall by using rawinsonde soundings and model reanalysis data in the Yeongdong region. Two strong CAD events (14 February 2019 and 6 February 2020) were observed when the snowfall forecast was wrong specifically in its location and timing. For two CAD events, lower-level temperature below ~ 2 km ranged to lowest limit in comparisons to those of the previous years (2014 – 2021) rawinsonde soundings, along with the stronger inversion strength (>2.0℃) and thicker inversion depth (>700m). Further, the cold northwesterly was predominant within the CAD layer, whereas the thin easterly wind was exhibited above the CAD layer. Meanwhile, during two weak CAD events (14 March 2018 and 1 March 2021), ice pellets of solid precipitation were observed when strong cold advection was prevalent below around 2 km as accompanied with stronger inversion strength (4.7 ~ 9.3 ℃) above the cold clouds. Cold air accumulation along the eastern side of the mountains appeared to significantly decrease low level temperature (850 hPa) up to -4.7 ~ -3.4 ℃, which was lower than long-term averages (-9.5 ℃). Rawinsonde observation and LDAPS reanalysis identify that extreme cold air intrusion with barrier wind to Yeongdong plays an important role in modulating snowfall intensity and location in terms of snow clouds moving and convergence, and weak CAD during the transition period of winter to spring is vulnerable to phase change of solid precipitation such as ice pellet (or freezing rain) with a help of cold air blocking by the mountains.


Wed-02 Aug | 1:10 - 3:10 | MR335
AS56 - Biogenic VOCs: Emissions, Atmospheric Oxidation, and Impacts

Session Chair(s): Yanli ZHANG, Guangzhou Institute of Geochemistry, Chinese Academy of Sciences

AS56-A002 | Invited
Biogenic VOC Emissions from Urban and Agricultural Landscapes

Alex GUENTHER#+, Jesus CAMPOS, Bee KITTITANANUVONG, Saewung KIM
University of California, Irvine

Accurate estimates of the reactive gas emissions driving atmospheric composition is required to make effective policy decisions on local to global scales. The biosphere is the dominant source of the reactive organic gases in the atmosphere that interact with anthropogenic pollution to form ozone and secondary aerosol and play an important role in air quality and climate. Biogenic volatile organic compound (BVOC) emission studies have primarily focused on the natural ecosystems that are the globally dominant sources. The widescale reductions in anthropogenic VOC emissions in recent decades have increased the relative contribution of BVOC emissions to total urban VOC emissions to the point where BVOC emissions now dominate in some urban areas. Estimating BVOC emissions in managed (e.g., urban and agricultural) landscapes is more challenging than for natural ecosystems due to the spatial heterogeneity, rapid temporal changes, and the lack of observations. An approach for quantifying BVOC emissions from urban and agricultural landscapes, using the MEGAN model, will be presented through case studies. The approach utilizes ultra high-resolution imagery and virtual surveys to characterize tree, shrub, grass and crop cover fractions and species composition and a multi-modal emission approach to assign emission factors. Landcover classification approaches tend to substantially underestimate tree cover in both urban and agricultural landscapes due to the challenges in detecting isolated trees in these heterogeneous landscapes. Urban and agricultural landscapes with relatively low BVOC emissions may require greater BVOC emission factor accuracy due to the greater VOC sensitivity of ozone formation in VOC limited regions. Assigning a constant low BVOC emission to these landscapes is not sufficient. Urban and agricultural BVOC responses to climate and landcover change and potential for emission mitigation will be discussed and gaps and priorities for future progress identified.


AS56-A009
Formation of 2-methyltetrol and 2-methylglyceric Acid in the Northern Hemisphere from Marine Isoprene Emission

Jie ZHANG1, Junyi LIU2, Minsu CHOI1, Xiang DING3, Mei ZHENG2, Qi YING1#+
1Texas A&M University, 2Peking University, 3Chinese Academy of Sciences

Field measurements have shown that isoprene emitted from ocean surfaces are significant. However, their contributes to secondary organic aerosol (SOA) formation in the polluted and remote marine troposphere have not been accurately quantified. In this study, we used a modified hemi-spheric community multiscale air quality model (hemisphere CMAQ) to study the formation of 2-methyltetrols (2-MT) and 2-methylglyceric acid (2-MG) due to isoprene emissions originated from chlorophyll-a and marine and sea surface microlayer in the northern hemisphere. The modified hemi-sphere CMAQ model considers the formation of 2-MT and 2-MG from the acid-driven reactive surface uptake of isoprene epoxide (IEPOX), methacrylic acid epoxide (MAE), and hydroxymethyl-methyl-α-lactone (HMML). In addition, it considers the photochemical decay of 2-MT and 2-MG in gas and aerosol aqueous phase, and the gas-aqueous-organic phase partitioning. The emissions of isoprene and other biogenic VOCs from on-land sources are also considered in the model using the estimations from the Model of Emissions of Gases and Aerosols from Nature (MEGAN), and anthropogenic emissions are based on the EDGAR emission inventory. Our simulations will reveal the concentrations of the marine-originated isoprene tracers and total SOA in various parts of the marine boundary layer in the northern hemisphere and their contributions to total SOA loading.


AS56-A004
Biogenic Volatile Organic Compounds Emission Characterization and its Contribution to Ozone Formation in the Subtropical Region in South China

Yanli ZHANG1#+, Xinming WANG2
1Guangzhou Institute of Geochemistry, Chinese Academy of Sciences, 2Chinese Academy of Sciences

With the accumulation of data about biogenic volatile organic compounds (BVOCs) emissions from plants based on branch-scale enclosure measurements worldwide, it is vital to assure that measurements are conducted using well-characterized dynamic chambers with good transfer efficiencies and less disturbance on natural growing microenvironments. A self-made cylindrical semi-open dynamic chamber with Teflon-coated inner surface was characterized both in the lab with standard BVOC mixtures and in the field with typical broad-leaf and coniferous trees. BVOC emissions from twenty mature trees (15 evergreen broad-leaved and 5 evergreen needle-leaved) were measured using dynamic chambers in situ. The emitted BVOCs were collected using sorbent tubes and speciated with a thermal desorption-gas chromatography/mass spectrometry system (TD-GC/MS). Twenty BVOC compounds, including isoprene, 14 monoterpene species, and 9 sesquiterpene species, were quantified to calculate their emission factors. The emissions of BVOCs in the Pearl River Delta region were estimated by using the localized emission factor database, and their contributions to ozone formation were also estimated. Furthermore, field campaigns were also conducted to investigate the atmospheric chemistry of BVOC during ozone pollution episodes. These results can help us better understand the BVOC’s roles in ozone formation and can guide a reasonable control of anthropogenic emissions.


AS56-A008
Comprehensive Chemical Characterization of Gaseous I/SVOC Emissions from Heavy-duty Diesel Vehicles Using Two-dimensional Gas Chromatography Time-of-flight Mass Spectrometry

Xiao HE#+
Shenzhen Univerisithy

Intermediate-volatility and semi-volatile organic compounds (I/SVOCs) are key precursors of secondary organic aerosol (SOA). However, the comprehensive characterization of I/SVOCs has long been an analytical challenge. Here, we develop a novel method of speciating and quantifying I/SVOCs using two-dimensional gas chromatography time-of-flight mass spectrometry (GC×GC-ToF-MS) by constructing class-screening programs based on their characteristic fragments and mass spectrum patterns. Using this new approach, we then present a comprehensive analysis of gaseous I/SVOC emissions from heavy-duty diesel vehicles (HDDVs). Over three thousand compounds are identified and classified into 21 categories. The dominant compound groups of emitted I/SVOCs are alkanes (normal + branched alkanes), benzylic alcohols, alkenes, cycloalkanes, and benzylic ketones. Oxygenated I/SVOCs (O-I/SVOCs, e.g., benzylic alcohols and ketones) are first quantified and account for > 20% of the total I/SVOC mass. Advanced aftertreatment devices largely reduce the total I/SVOC emissions but increase the proportion of O-I/SVOCs. With the speciation data, we successfully map the I/SVOCs into the two-dimensional volatility basis set space, which facilitates a better estimation of SOA.


AS56-A006
Rethink BVOC Emissions and Their Contributions to Air Quality in South China

Peng WANG#+
Fudan University

The biogenic volatile organic compounds (BVOCs), dominantly emitted from the terrestrial ecosystem, significantly contribute to ozone (O3) and secondary organic aerosol (SOA) formation in the troposphere due to their high reactivity with oxidants such as hydroxyl radicals. It is important to get an accurate estimation of the BVOC emissions from vegetated surfaces to evaluate their impacts on air quality and climate change. The Model of Emissions of Gases and Aerosols from Nature (MEGAN) has been widely used to estimate BVOC emissions from local to global scales. However, previous studies have shown large uncertainties existed in estimating BVOC emissions in China via MEGAN. In this study, a localized emission factors (EFs) database was developed for MEGAN in south China, which is fronting high BVOC emissions. This EFs database was derived based on a recent field measurement, covering all major BVOCs (isoprene, monoterpenes, and sesquiterpenes). The Community Multiscale Air Quality (CMAQ) model was then applied to investigate the impacts on air quality of different EFs. Results show that using new EFs (NEF case) reduces BVOC emissions compared to that of default EFs (BASE case). The most remarkable decrease is found in sesquiterpene with an average reduction rate of ~40%. In addition, the NEF case improves CMAQ O3 predictions in all seasons. Through south China, the lower BVOC emissions of the NEF case decrease concentrations of O3 and SOA by -1 ppb and -0.8 µg m-3, respectively, although the enhanced atmospheric oxidation capacity levels are found in some locations. Further efforts including field measurements, lab experiments, and modeling studies should be made to better evaluate BVOC effects in south China.


AS56-A010
Highly Oxygenated Organic Molecules Formation in the Oxidation of Limonene by OH Radical: Significant Contribution of Hydrogen Abstraction Pathway

Hao LUO1+, Luc VEREECKEN2, Hongru SHEN1, Sungah KANG2, Iida PULLINEN2, Mattias HALLQUIST3, Hendrik FUCHS2, Andreas WAHNER2, Astrid KIENDLER-SCHARR2, Thomas MENTEL2, Defeng ZHAO1#
1Fudan University, 2Forschungszentrum Jülich, 3University of Gothenburg

Highly oxygenated organic molecules (HOM) play a pivotal role in the formation and growth of secondary organic aerosol particles. The distribution, formation mechanism and yield of HOM from the oxidation of atmospheric VOC are key information to understand SOA and their effect on climate and health. As an important biogenic monoterpene with the fourth largest emission strength and a common component in volatile chemical products, limonene and its oxidation derived HOM have a potentially important role in SOA formation in both forested and urban regions. In this study, we report HOM formation in the oxidation of limonene by OH radical in the SAPHIR chamber (Simulation of Atmospheric PHotochemistry In a large Reaction chamber) measured by a high-resolution time-of-flight chemical ionization mass spectrometer with nitrate reagent ion (NO3-CIMS). We performed analysis of the complex mass spectra acquired and identified the distribution of HOM, including major monomers (C9-10) and dimers (C17-20), to classify them into various series. Numerous HOM, both closed-shell products and open-shell peroxy radicals (RO2), were identified in low and high NO condition (0.06-0.2 ppb, 17 ppb). C10 monomers are the most abundant HOM products, accounting for over 80% of total HOM. The HOM formation pathways were proposed on the basis of observed RO2 and known mechanisms. Particularly, the role of hydrogen abstraction by OH is highlighted, which is quantitatively compared against the OH addition pathway. The molar yields of HOM were estimated at low and high NO conditions, respectively.


AS56-A012
The Impact of Biogenic VOCs on Atmospheric Oxidation Capacity

Hongliang ZHANG, Wenxuan YU#+
Fudan University

With the background of global climate change, extreme weather events are occurring with increasing frequency and intensity, which not only threaten human health and ecological environment, but also have a significant impact on biogenic volatile organic compounds (BVOCs). BVOCs are emitted from plants and are important precursors to the formation of secondary pollutants such as ozone, particulate matter, and other pollutants. Atmospheric oxidation capacity (AOC) is used to measure the rate of secondary pollutant generation. Understanding the impacts of BVOCs on AOC is important for designing effective control strategies. This study aims to simulate summer vegetation emissions and secondary pollutant concentrations in China based on the Model of Emissions of Gases and Aerosols from Nature (MEGAN) and the Community Multi-scale Air Quality (CMAQ) model with the resolution of 36 km × 36 km. The meteorological fields are generated by the Weather Research and Forecasting (WRF) model. The anthropogenic emissions are generated from Multi-resolution Emission Inventory for China (MEIC). The study investigates the changes in the concentrations of BVOCs and secondary pollutant in China and analyzes the causes of ozone increase in Yangtze River Delta. The results show that this might be related to the rise in BVOCs caused by warming. The study also revealed the process and formation of compound air pollution and provides an important reference for improving our air quality assessment methods.


Wed-02 Aug | 3:30 - 5:15 | MR311
AS19 - Extreme Weather Resiliency: Prediction and Response Strategies

Session Chair(s): Kaoshen CHUNG, National Central University, Pay-Liam LIN, National Central University

AS19-A009 | Invited
High-resolution Time-lagged Rainfall Forecasts for Typhoons and Predetermination of Their Qualities Through Machine Learning

Chung-Chieh WANG#+, Shin-Hau CHEN
National Taiwan Normal University

As high-resolution is necessary for high-quality quantitative precipitation forecasts (QPFs) over terrain (Wang, 2015), it is not ideal to split computational resources as in multi-member ensembles. Thus, the use of a single member (or a few members) with a larger fine domain, longer range, and the time-lagged strategy to obtain ensemble information has been explored (Wang et al., 2016). So far, case studies with one run every 6 h and a range of eight days indicate that this approach takes advantages of realistic QPFs both within the short range (72 h) and beyond (Wang et al., 2023). Because forecast uncertainty is high at early stages when the typhoon is far away, the spread of tracks tends to be large and this better ensures the appearance of the worst-case scenario (typically from a direct hit) for early preparation. In some cases that this scenario did occur, the system predicted a high-quality QPF almost one week before landfall. Later when the uncertainty reduces, model tracks converge and the most-likely scenario emerges to allow for adjustments, and this typically occurs about 2-3 days before landfall. To learn about the quality of the QPFs in each run and hence the likelihood of the particular scenario to happen, machine learning is used to predict the similarly skill score (SSS), which measures how similar is the QPF to observation, shortly after each run is completed. Encouraging results are obtained (Chen and Wang, 2022), as after training, the model from machine learning can capture the tendency of the actual SSS computed using observed rainfall for most cases, thereby informing the forecasters/users which QPFs are more trustworthy and which ones less likely to occur prior to the event. Such guidance is especially valuable at longer lead times, when the forecast uncertainty is relatively high.


AS19-A021 | Invited
Improved Extended-range Probabilistic Forecasts of Extreme Precipitation Events Over Taiwan Using Analog Post-processing

Hui-Ling CHANG1,2#+, Shih-Chun CHOU3, Pay-Liam LIN2, Jing-Shan HONG1
1Central Weather Bureau, 2National Central University, 3International Integrated Systems, Inc.

The predictability of precipitation is limited due to the important role finer-scale processes play. However, demand for extended-range precipitation forecasts by users has grown significantly, especially for extreme events. Therefore, the goal of this study is to predict the conditional climatology of precipitation given the forecast of the large-scale circulation conditions, which still retain predictability in the extended range. In this study, we focus on week 2-3 extreme precipitation forecasts over Taiwan. Most ensemble prediction systems are characterized by under-dispersion that limits the utility of predictions for extreme events. Here we use Analog Post-processing (AP) to produce calibrated posterior ensembles with reasonable spread to effectively mitigate the problem of under-dispersion. The AP forecast ensembles are derived from the observationally based precipitation analysis corresponding to the historical forecast analogs that most resemble the current precipitation forecast. Therefore, the forecast is also effectively downscaled to 1 km in the AP procedure. Frequency counting is then applied to the AP ensembles to produce week 2-3 probabilistic precipitation forecasts. Forecast evaluation confirms that the raw ensemble is under-dispersive with an obvious wet bias. In contrast, the AP ensemble distribution is well calibrated with most of the bias removed. Frequency distribution of rain rate shows that the AP ensemble is much closer to the observation than the raw ensemble, while the raw ensemble displays over-forecasting for most of the samples and under-forecasting for extra extreme precipitation. Extreme precipitation cases show that the probabilistic forecast from the AP ensemble is well consistent with the observation in precipitation pattern, while the raw ensemble severely deviates from the observation. Evaluation of potential economic value demonstrates that users with a much wider spectrum of cost/loss ratio can benefit from the calibrated forecasts as compared to the raw forecast, with a significantly higher gain in decision-making.


AS19-A004
An Insight Into the Microphysical Attributes of Northwest Pacific Tropical Cyclones

Balaji Kumar SEELA1,2+, Jayalakshmi JANAPATI1, Pay-Liam LIN1#, Meng-Tze LEE3
1National Central University, 2Academia Sinica, 3McGill University

Northwestern Pacific (NWP) tropical cyclones (TCs) impose a severe threat to the life and economy of the people living in East Asian countries. The microphysical features, mainly the raindrop size distributions (RSD) of TCs that improve the modeling simulation and rainfall estimation algorithms, are limited to case studies, and an extensive understanding of TCs’ RSD is still scarce over the northwest Pacific. Here, we examine a comprehensive outlook on disparities in microphysical attributes of NWP TCs with radial distance and storm type, using sixteen years of disdrometer, ground-based radar, and reanalysis datasets in north Taiwan. We find that dominant stratiform precipitation in the inner rainbands leads to the occurrence of more bigger drops in the inner rainbands than the inner core and outer rainbands. Moreover, a decrease in mass-weighted mean diameter and rainfall rate with radial distance is associated with a reduction in moisture availability for various circumstances, and this association is deceptive in intense storms. Our findings give an insight into crucial processes governing microphysical inequalities in different regions of NWP TCs, with implications for the ground-based and remote-sensing rainfall estimation algorithms.


AS19-A015
Simulation of the Diurnal Forcing in the Heavy Rainfall Event Produced by the Prefrontal MCS During Mei-yu Season

Siang-Yu ZHAN#+, Pay-Liam LIN
National Central University

The heavy rainfall event with the maximum accumulated rainfall ~340 mm/6h occurred over northwestern Taiwan coastal region on 17 May 2019. In this case, Taiwan was under the unstable prefrontal warm sector with southwesterly wind prevailing. The marine boundary layer jet (MBLJ) transports moisture from low latitudes to Taiwan Strait. A mesoscale convection system (MCS) initiated over northern Taiwan Strait in nocturnal time, extending eastward to northwestern Taiwan coastal region, resulting in the heavy rainfall event. The Weather Research and Forecasting (WRF) model was used to analyze the mechanisms of the development of the MCS and the diurnal forcing in this case. The results showed that the prefrontal MCS was produced by the low-level convergence combining with upper level divergence under the unstable warm, moist atmospheric condition. The low-level convergence played an important role on rainfall distribution. The low-level convergence was between the terrain induced barrier jets (BJ) and the weak westerly winds from southeastern China costal region. In the daytime initiation run (DI run), the westerly wind over northern Taiwan Strait near southeastern China costal region in control run were replaced by southwesterly wind. As a result, there were little low-level convergence, and there was little rainfall over northern Taiwan.


AS19-A018
Evaluation of One-day-ahead Probabilistic 100-meter Wind Speed Forecasts Produced by the WRF Ensemble Prediction System in Taiwan

Shih-Chun CHOU1#+, Hui-Ling CHANG2,3, Chung Ho HORNG2, Chih-Yung Feng FENG4, Han-Fang LIN4, Pay-Liam LIN3
1International Integrated Systems, Inc., 2Central Weather Bureau, 3National Central University, 4Manysplended Infotech Ltd

The use of renewable energy for power generation is gradually increasing in many developed countries. Due to the intermittent nature and current limits to the prediction of renewable energy, grid connection and power dispatch are important challenges to renewable energy management. High-quality and calibrated meteorological forecasts play a critical role to provide valuable information for applications. This study evaluates both the quality and performance of probabilistic 100-meter wind speed forecasts based on the Weather Research and Forecasting model Ensemble Prediction System (WEPS). Moreover, the relative economic analysis can quantify the economic benefit for users with different cost-loss ratio, and assist users in optimizing their decision making for specific situations users concerning. The results indicate that (1) Probabilistic forecasts of 100-m wind speed from WEPS exhibited greater over-forecasting during northeast than southwest monsoon periods and over northern Taiwan than other areas. (2) Through the statistical post-processing (SPP) technique for bias correction, both reliability and potential usefulness of probabilistic forecasts are significantly improved. (3) Almost all users, regardless of their cost-loss ratio, can obtain more economic benefit if they make decisions based on the calibrated probabilistic forecasts produced by WEPS.


AS19-A024
Investigating the Warm Rain Process by Assimilating Dual-polarimetric Radar Data in Wintertime: A Case Study of Shallow Convection Event in Northeastern Taiwan

Chin-Chuan CHANG#+, Kaoshen CHUNG, Bing-Xue ZHUANG
National Central University

In this study, the dual-polarimetric radar data are assimilated into the model to investigate the shallow rainfall event over Yi-Lan area. In addition, two experiments are conducted to examine the added value of assimilating dual-polarimetric radar data. The observations of radar illustrated that the rainfall event is dominated by different numbers of small raindrops with a medium ZH value and a uniform low ZDR value structure. Results of assimilating ZDR show that the over-estimate of the ZDR value can be modified toward observations although the bias of the microphysics scheme remains. Overall, assimilating ZDR from the shallow convection system can improve the analysis of microphysics structure, and have a better illustration of the small-raindrop-dominant warm rain structure in the wintertime rainfall event. Further analysis of dynamic and cloud physics could be proceeded after data assimilation.


AS19-A022
Low Level Jets and Heavy Rainfall Events Over Taiwan Revealed from Wind Profiler Radars

Pay-Liam LIN#+, Yen-LIng LIOU
National Central University

The 499 MHz wind profiler is used to study the relationship between low-level jet (LLJ) and heavy rainfall over Taiwan and Dongsha island during the mei-yu season of 2018~2020. The LLJ day is defined as LLJ that occurs more than 6 hours in a day. On the LLJ day of northern Taiwan, the low layer wind speed extreme appears on the northwest side of Taiwan, and Taiwan locates at the front edge of the frontal system. On the LLJ day of Dongsha island, the extreme low layer wind speed appears on the southeast side of Taiwan and the South China Sea, and the frontal system locates over Taiwan. The boundary layer jet (BLJ) is defined as LLJ occurs below 1000 m, and the synoptic system-related low-level jet (SLLJ) is defined as LLJ occurs above 1000 m. On the SLLJ day of northern Taiwan and SLLJ day of Dongsha island, water vapor transportation mainly comes from the coastal South China to the South China Sea in the boundary layer. On the BLJ day of northern Taiwan and BLJ day of Dongsha island, water vapor transportation mainly comes from the coastal South China and the South China Sea in the boundary layer, respectively. When the strong BLJ events occurred in northern Taiwan, the average hourly extreme rainfall happened in the southern mountains and the northwest coast from Hsinchu to Taichung. When the strong SLLJ events occurred in northern Taiwan, the average hourly extreme rainfall happened on the northwest coast from Taoyuan to Hsinchu. When the strong BLJ events occurred on Dongsha island, the average hourly extreme rainfall happened on the southwest coast to the mountains and the northwest coast of Miaoli to the mountains. When the strong SLLJ events occurred on Dongsha island, there was no significant precipitation in Taiwan.


Wed-02 Aug | 3:30 - 5:15 | MR323
AS35 - Aerosols, Clouds, Radiation, Precipitation, and Their Interactions

Session Chair(s): Chuanfeng ZHAO, Peking University, Jingyu WANG, Nanyang Technological University

AS35-A029 | Invited
21st Century Global and Regional Surface Temperature Projections and Uncertainties Due to Cloud and Aerosol Forcing and Feedbacks

Jonathan JIANG#+
California Institute of Technology

Recent studies have been sparking concerns about the impending arrival of “tipping points” later in the 21st century. This study analyzes observed global surface temperature trends in three target latitudinal regions: the Arctic Circle, Tropics, and the Antarctic Circle. We show that global warming is accelerating unevenly across the planet, with the Arctic warming at more than three times the average rate of our world. We also analyzed the reliability of latitude-dependent surface temperature simulations from a suite of Coupled Model Intercomparison Project Phase 6 (CMIP6) models and their multi-model mean (MMM) by comparing their outputs to observational data sets. We selected the best-performing models based on their statistical abilities to reproduce historical, latitude-dependent values adapted from these data sets. The surface temperature projections were calculated from ensemble simulations of the Shared Socioeconomic Pathway 2–4.5 (SSP2–4.5) by the selected CMIP6 models. We estimate the calendar years of when surface temperatures will increase by 1.5, 2.0, and 2.5°C relative to the preindustrial period, both globally and in the three target regions. Our results also indicate large uncertainties in surface temperature projections due to differences in cloud and aerosol forcings used in climate models. Further studies are necessary to determine the most efficient solutions to reduce these uncertainties in surface temperature projections both globally and regionally.


AS35-A028
Emergent Constraint on Extratropical Marine Low Cloud Feedback

Hui SU1#+, Xianan JIANG2, Jonathan JIANG3, J. David NEELIN2, Longtao WU4, Yoko TSUSHIMA5
1The Hong Kong University of Science and Technology, 2University of California, Los Angeles, 3California Institute of Technology, 4Jet Propulsion Laboratory, California Institute of Technology, 5Met Office

It has been shown that low cloud amount feedback contributes significantly to the uncertainty in equilibrium climate sensitivity (ECS). In the models that participated in the Coupled Model Intercomparison Project Phase 6 (CMIP6), we found that the inter-model spread in the extratropical marine low cloud fraction (LCFe) feedback under long-term warming is highly correlated with the seasonal variation of LCFe per degree of sea surface temperature change. The models with ECS greater than 4.5 K (termed high ECS models) tend to have a stronger seasonal cycle in LCFe than the models with ECS lower than 3.3 K (termed low ECS models). Further analysis of cloud vertical structures reveal that the strong seasonal cycle of LCFe in the high ECS models is primarily driven by the variability of low-to-middle clouds associated with midlatitude storm tracks, while the seasonal variability of LCFe in the low ECS models is decoupled from the storm track activity. The new emergent constraint on ECS based on the seasonal variability of LCFe indicates that the high ECS models are more consistent with the satellite observations than the low ECS models.


AS35-A031
Including Ice-cloud Longwave Scattering and Surface Spectral Emissivities in Climate Models Leads to More Impacts on Mean-state Climate Than Climate Feedbacks

Chongxing FAN1#+, Yi-Hsuan CHEN2, Xiuhong CHEN1, Wuyin LIN3, Xianglei HUANG1, Ping YANG4
1University of Michigan, 2Academia Sinica, 3Brookhaven National Laboratory, 4Texas A&M University

Climate models often ignore cloud scattering and surface emissivity in the longwave (LW) for computational efficiency. Such approximations can cause biases in radiative fluxes and affect simulated climate, especially in the Arctic because of its large sensitivity to perturbations. We implemented treatments to both physics into the Energy Exascale Earth System Model (E3SM) version 2 by DoE and assessed their impacts on the simulated mean-state global climate as well as climate feedback and sensitivity. By turning on and off the switches in the modified E3SMv2 model, we studied the changes in mean-state climate due to cloud LW scattering and surface emissivity effects by comparing four 35-year fully-coupled simulations. Cloud LW scattering warms the entire global troposphere by ~0.4 K on average; the warming is stronger in the Arctic (~0.8 K) than in the tropics, which is a manifestation of the polar amplification phenomenon. When realistic emissivity is incorporated into the model, the surface skin temperature increases by 0.36 K instantaneously on a global average, especially in the Sahara Desert (~0.7 K) where the surface emissivity is low. Surface temperature further increases by 0.19 K due to the inclusion of surface spectral emissivity. The mean-state climate changes due to both effects are linearly additive. We also carried out four 35-year simulations under the abrupt 4xCO2 scenario, with cloud LW scattering and/or surface emissivity effects on and off. Based on radiative kernel analysis, we found that total global-mean climate feedback does not change significantly after including either or both physics. Nevertheless, lapse rate feedback, water vapor feedback, and cloud feedback in the tropics have changed by up to 10%. They are primarily associated with high cloud fraction response in the upper troposphere. Our study highlights the importance of both processes in climate models.


AS35-A021
Do Aerosols Increase or Decrease Precipitation?

Kalli FURTADO1#+, Paul FIELD2
1Centre for Climate Research Singapore, 2Met Office

Do aerosols increase or decrease precipitation? The observed variety of aerosol effects on precipitation at different spatial and time scales means that no simple answer to this question has so far been discovered. However, although aerosol effects are many, it remains possible that there are universal constraints on the number of degrees of freedom needed to represent them. We use convective-scale simulations to reveal a self-similar probability density function that underpins surface rainfall statistics. This function is independent of cloud-droplet number concentration and is unchanged by aerosol perturbations. It therefore represents an invariant property of our model with respect to cloud–aerosol interactions. For a given aerosol concentration, if at least one moment of the rainfall distribution on cloud-droplet number is a known input parameter, then this can be combined with the self-similar function to reconstruct the entire rainfall distribution to a useful degree of accuracy. We will demonstrate this using simulations from convective permitting, aerosol interacting simulations over China.


AS35-A005
Diagnostic Cloud Fraction Scheme Based on Cloud Hydrometeors

Raeseol PARK1#+, Jung-Yoon KANG1, Soo Ya BAE1, Suk-Jin CHOI2
1Korea Institute of Atmospheric Prediction Systems, 2Gangneung-Wonju National University

Atmospheric clouds play important roles in redistribution of energy budgets via scattering solar radiative fluxes and absorbing/reemitting terrestrial radiative fluxes in atmospheric models and then consequently affect change of atmospheric temperature and precipitation. Therefore, parameterizations of cloud physical processes are tightly related to predictability of atmospheric models. Cloud physical processes in the atmospheric models involve cumulus convection, cloud microphysics, and cloud macrophysics which produce cloud information such as resolved/subgrid cloud hydrometeors, effective radius of cloud droplet, cloud fraction, and so on. The model-predicted cloud information is utilized in radiative process in order to estimate cloud radiative forcing. Quantification of cloud fraction among cloud properties simulated form the atmospheric models is relatively uncertain because its concept is somewhat ambiguous, so amount of cloud fraction has a large deviation depending on the cloud fraction schemes. The cloud fraction in the Korean Integrated Model (KIM) has been calculated via a prognostic scheme proposed by Park et al. (2016), which reported that the prognosed cloud fraction shows a better similarity to satellite observation compared to diagnosed cloud fraction. However, recently, inconsistency between the prognosed cloud fraction and KIM-simulated cloud hydrometeors was found and a new diagnostic cloud fraction scheme was proposed to reduce the inconsistency. The newly-proposed diagnostic cloud fraction scheme was designed assuming a proportional relation between cloud hydrometeor and cloud fraction considering its variation due to altitude and latitude. The diagnostic cloud fraction scheme was optimized via comparison to ERA5 data and its impact on the KIM performance was analyzed. In this talk, details of the diagnostic cloud fraction scheme based on the cloud hydrometeors will be presented and better approaches for estimation of cloud fraction could be discussed.


AS35-A009
Smoke-weather Interaction Affects Cloud, Precipitation and Extreme Wildfires in Southeast Asia

Ke DING1#+, Aijun DING1, Xin HUANG1, Yafang CHENG2
1Nanjing University, 2Max Planck Institute for Chemistry

The biomass burning in Indo-China Peninsula, caused by agricultural activities, has a significant impact on human lives, air quality, ecosystems, and weather systems. However, it is not fully clear how wildfire can affect weather processes, especially clouds and precipitation formation, which are important for wildfire behaviours. Here we show that biomass burning aerosols aloft strongly increase the low cloud coverage over both land and ocean in subtropical southeastern Asia. The degree of this enhancement and its spatial extent is comparable to that in the Southeast Atlantic, even though Southeast Asia's total biomass burning emissions are only one-fifth of those in Southern Africa. We find that a synergetic effect of aerosol-cloud-boundary layer interaction with the monsoon is the main reason for the strong semi-direct effect and enhanced low cloud formation in southeastern Asia. Moreover, the interactions between smoke and weather can reduce rainfall on Indo-China Peninsula, thus worsening air pollution by enhancing fire emissions and weakening dispersion. The intricate interactions among wildfires, smoke, and weather form a positive feedback loop that substantially increases air pollution exposure.


Wed-02 Aug | 3:30 - 5:15 | MR327
AS32 - Frameworks, Modelling, and Observations to Understand Moist Convective Processes for Weather and Climate

Session Chair(s): Maxime COLIN, Leibniz Centre for Tropical Marine Research, Ji NIE, Peking University, Chien-Ming WU, National Taiwan University

AS32-A012 | Invited
Towards a Stochastic Parameterization of Unresolved MCS Impacts on Large Scales

Robert PLANT1#+, Hannah CHRISTENSEN2, Mark MUETZELFELDT1, Tim WOOLLINGS2, Zhixiao ZHANG2
1University of Reading, 2University of Oxford

The treatment of MCS is a long-standing challenge for global numerical weather prediction and climate models. The model dynamics, convection scheme, microphysics, radiation and turbulence are all relevant, and upscale transports necessary to modulate phenomena such as the MJO and ITCZ may be removed, artificially damped, or even artificially stimulated because the parameterizations incorrectly couple to the model dynamics. Traditional convection schemes assume convection to be disorganized, and do not explicitly treat the coherent mesoscale overturning circulation. Recently, however, Moncrieff and collaborators proposed a parameterization of MCS effects which can be coupled to a traditional convection parameterization, making the hearting profile more top-heavy and providing additional momentum transports. The method improved precipitation across the ITCZ and Maritime Continent in CAM and E3SM.Our project aims to build on the Moncrieff approach by developing a stochastic parameterization of unresolved MCS impacts. While the traditional convection scheme assumes all deep convection to be disorganized and the original Moncrieff method assumed all deep convection to be MCS-like, we aim to develop a stochastic formulation of the likelihood of developing an MCS for a given model profile. We also intend to reformulate the missing tendencies imposed in an MCS situation based on an analysis of DA increments. We are working in the Met Office Unified Model, coupling our MCS approach to its new CoMorph convection parameterization. In this talk we will describe our experiences with the Moncrieff MCS parameterization so far, and the steps being taken towards its extension and generalization.


AS32-A007
The Nonlocal Response of Convective Updraft to Buoyancy and Dynamic Pressure Perturbation

Yi-Hung KUO1#+, J. David NEELIN2, Ming ZHAO3, Zhihong TAN1
1Princeton University, 2University of California, Los Angeles, 3NOAA's Geophysical Fluid Dynamics Laboratory

In many of the existing convective schemes, the updraft is modeled based on assumptions including: (i) a steady state in quasi-equilibrium with the environment; (ii) the updraft kinetic energy variation balanced by buoyancy work; (iii) the buoyancy and dynamic pressure perturbation gradient approximated by damping or turbulent mixing. Recent analyses of radar wind profiler observations point to the importance of dynamic entrainment, i.e., a deep layer of horizontal inflow in the lower troposphere associated with updraft mass flux divergence in the vertical. The nonlocal effects of the pressure perturbations have been adapted to explain the observed deep-inflow structure. For a vertically restricted buoyancy feature, the theoretical updraft response can, under suitable conditions, extend below and above the buoyant layer. For features containing horizontal scales comparable to a significant fraction of the tropospheric depth, the nonlocal response can contribute to inflow that extends through the lower troposphere. The updraft evolution tends to be robust to inhomogeneities arising from imperfectly turbulent mixing---due to the nonlocal dynamics averaging over smaller-scale buoyancy anomalies. In this work, an idealized, 1-dimensional time-dependent cloud model is proposed to include dynamic entrainment (and detrainment) and nonlocal pressure perturbation gradient. In a conditionally unstable environment, the inclusion of nonlocal response to buoyancy permits deep convection to develop even in the presence of a CIN layer---no trigger required. For conserved tracers the budget is primarily dominated by updraft advection, entrainment mixing, and the inflow/outflow associated with dynamic entrainment/detrainment. For the updraft mass flux, on the other hand, the nonlocal dynamic pressure perturbation gradient substantially offsets the advection and dynamic-entrainment mixing of vertical momentum flux. This suggests that the conventional balance involving the updraft kinetic energy variation and buoyancy used in existing schemes is likely an artifact of inadequate approximation of the dynamic pressure perturbation gradient.


AS32-A002
Parameterizing Convection and Clouds with an Ensemble of Neural Networks

Yilun HAN1#+, Guang ZHANG2, Yong WANG1
1Tsinghua University, 2 University of California San Diego

Current moist physics parameterization schemes in general circulation models (GCMs) are the main source of biases in simulated precipitation and atmospheric circulation. With the recent advances in data science, machine learning has been increasingly applied to convection and cloud parameterizations in GCMs. This study uses an ensemble of 32-layer deep convolutional residual neural networks, referred to as ResCu-en, to emulate the convection and cloud processes simulated by a super parameterized GCM, SPCAM. ResCu-en uses the current environmental states and advections plus the past history of convection and clouds to predict the GCM grid-scale temperature and moisture tendencies, cloud liquid and ice water contents from moist physics processes. The surface rainfall is derived diagnostically from the column-integrated moisture tendency. The prediction uncertainty inherent in deep learning algorithms in emulating the moist physics is reduced by ensemble averaging. In an independent offline validation, it is found that ResCu-en has extremely high prediction accuracy for all output variables considered. In addition, ResCu-en trained with data in the current climate can generalize well to a warmer climate with +4K sea surface temperature, with high prediction accuracy as well.


AS32-A005
“Relay-race” Propagation of Super Clusters in a Cloud-permitting Simulation of the Madden-Julian Oscillation

Yan LIU1#+, Zhe-Min TAN1, Zhaohua WU2
1Nanjing University, 2Florida State University

Eastward-propagating super clusters comprise the major convective body of the Madden-Julian Oscillation (MJO) envelope. They have significant effects on the propagation speed of the MJO. The dynamical processes underlying the eastward propagation of super clusters are investigated using a month-long cloud-permitting simulation of an MJO event over the tropical Indian Ocean. The analysis shows that the propagation of super clusters resembles a “relay-race”, which can be divided into four stages: i) the super cluster accompanied by low surface pressure to its east moves eastward slowly, while in front of it there are westward-propagating waves approaching rapidly; ii) the superposition of moisture convergence associated with westward-propagating waves and the moisture convergence induced by the low surface pressure promotes the formation of a new cloud cluster, which blocks the eastward propagation of the former cloud cluster; iii) the newly formed cluster continues to grow and consume moisture, while the former cluster gradually matures and eventually dissipates; iv) the new super cluster to the east replaces the old one and then propagates further eastward. Moisture convergence extends zonally and stays stagnant in a period of stages ii and iii. The non-instantaneous convection-convergence feedback determines the total duration of the stagnant period. Repeated occurrences of “relay-race” propagation result in the slow eastward propagation of super clusters in the MJO. Shallow convection is critical in the “relay-race” propagation, as cloud clusters are anchored at the same location when shallow convection dominates.


AS32-A004
Observed and Projected Changes of Large-scale Environments Conducive to Spring MCS Initiation Over the U.S. Great Plains

Fengfei SONG1#+, L. Ruby LEUNG2, Zhe FENG2, Qiu YANG2, Xingchao CHEN3
1Ocean University of China, 2Pacific Northwest National Laboratory, 3The Pennsylvania State University

Mesoscale convective systems (MCSs) are frequent over the U.S. Great Plains during spring. The link between large-scale environments and spring MCS initiation were well established. Here, historical and future changes of spring large-scale environments favorable for MCS initiation are investigated using an MCS tracking dataset, ERA5 reanalysis, and 20 CMIP6models. The frequency of Great Plains low-level jet (GPLLJ)-related MCS environments is found to have increased by ~41% from 1979 to 2019, consistent with the enhanced GPLLJ and more frequent MCSs. Comparing CMIP6 AMIP and historical experiments, we find that the observed GPLLJ strengthening and more frequent MCS environments are mainly due to the decadal sea-surface temperature variations rather than external forcings. Under a high emission scenario, the frequency of GPLLJ-related environments favorable for MCS initiation will increase by ~65% during 2015-2100, along with a stronger GPLLJ, suggesting more frequent MCSs over the U.S. Great Plains in a warming world.


AS32-A001
Bridging the Gap Between Implementing and Understanding the Weak Temperature Gradient Approximation in Cloud Resolving Models

Nathanael WONG#+, Zhiming KUANG
Harvard University

The weak-temperature gradient (WTG) approximation is a popular method used to couple convection in small-domain simulations to the large-scale climatology. Two major implementations that use the WTG approximation have gained popular use over the past two decades - the Temperature Gradient Relaxation (TGR) implementation and the Damped Gravity Wave (DGW) implementation. Our comparison of these different WTG implementations in an idealised framework result in different model behaviour, with implications on the nature of convective self-aggregation in similarly idealised setups. A further investigation shows that the different model behaviour is caused by the different treatment of the baroclinic modes by the different WTG implementations. More specifically, we hypothesise that the ratio of the strengths of the baroclinic modes in relation to the 2-day wave behaviour is important in determining if multiple-equilibria states are obtained under different WTG implementations. By varying the strengths of these two baroclinic modes, we are thus able to understand the major difference between two major WTG schemes and therefore bridge the gap between them.


AS32-A011
Stratospheric Influence on Tropical Convective Systems in a Minimal Model Framework of QBO-like Oscillations

Shigeo YODEN#+
Kyoto University

Self-sustained oscillations dynamically analogous to the equatorial QBO have been obtained as a radiative and moist-convective quasi-equilibrium state in a minimal model framework of the stratosphere-troposphere coupled system (e.g., Yoden et al. 2014). It is a two- or three-dimensional cloud-system-resolving non-hydrostatic model with a periodic lateral boundary condition. The obtained QBO-like oscillation influences organized features of moist-convective systems characterized as squall-line- or back-building-type precipitation patterns. A couple of nudging experiments to control the vertical shear of the mean zonal wind show its opposite role near the surface and the tropopause controlling the longevity and intensity of the moist-convective systems and precipitation. Possible future numerical experiments to investigate the fundamental role of internal dynamics to modulate the moist-convective systems and their larger-scale organizations interacting with the environmental zonal mean state will be discussed, in association with the international collaborative research activity of the stratospheric and tropospheric influences on tropical convective systems (SATIO-TCS) under WCRP/SPARC.


Wed-02 Aug | 3:30 - 5:15 | MR328
AS43 - Application of Data-driven and Machine Learning Approaches in Disaster Risk Reduction and Mitigation

Session Chair(s): Kelvin NG, University of Birmingham, Zhan TIAN, Southern University of Science and Technology

AS43-A015
Revolutionizing Earth Science with Generalized AI Models

Rahul RAMACHANDRAN1#+, Tsengdar LEE2, Raghu GANTI3
1NASA Marshall Space Flight Center, 2NASA Headquarters, 3IBM Research

Foundation Models (FM) are generalized Artificial Intelligence (AI) models that are designed to replace a task or an application-specific model and can be used for many downstream applications. These FM can be built on any sequence data and are trained utilizing self-supervised approaches. The obstacle of creating a sizable labeled dataset for training is removed by using self-supervised learning. Most FM employ transformer design that takes advantage of the idea of self-attention, allowing the network to represent the impact of distant data points on one another in space and time. The FM models show emergent qualities that are induced from the data.
FM can become a valuable tool for Earth science researchers. Due to the size of these models, downstream applications built fine-tuning these FM perform better and exhibit greater accuracy than models created from scratch. FM significantly lowers the entry barrier in terms of both the time and effort required to develop various downstream applications. For some scientific datasets, such as optical remote sensing data, FM can speed up processes like classification, object detection and prediction. By eliminating the training data bottleneck and maximizing the usage of science data, FM can make it simpler to integrate AI into scientific research. Initial results for three different FMs will be presented.


AS43-A012
Variation Characteristics and Attribution Analysis of Tropical Cyclone Compound Floods Derived from Observations in Shenzhen, China

Jingru LIU1,2#+, Zhan TIAN2, Steven DOBBIE3, Andrew ROSS3, Laixiang SUN4, Qinghua YE5
1University of Leeds; Southern University of Science and Technology, 2Southern University of Science and Technology, 3University of Leeds, 4University of Maryland, 5Deltares

The hazard of compound floods is much higher than that of univariate flood drivers due to the non-linear effects of multiple factors. The severe tropical cyclone (TC) compound floods that have occurred frequently in recent years have caused huge economic losses to China's coastal cities. A clearer understanding of TC compound flooding is essential for flood risk assessment, mitigation and management in coastal cities under global warming and urbanization. This study applies the machine learning (ML) models and multi-statistical methods for exploring the variations and characteristics of TC compound flooding events in western Shenzhen. The current indicator of compound floods is by a threshold that was determined by a ML approach. The results show an increase in the frequency of TC compound floods between 1964-2019, which is considered to be related to a decrease in the distance of TC maximum intensity to land. Besides, there has been a significant increase in compound flood events occurring with extreme high sea level. This study also found a higher risk of extreme TC compound flooding during the ENSO neutral phase. Flood predictions based on a 'rainfall-sea level' threshold obtained in this study enable decision makers to make high-level evaluations of TC compound flood risks in a short period of time. The findings will help the subsequent research on the atmospheric-hydrological processes and variability mechanisms of TC compound flooding.


AS43-A010
On the Prediction of Water Level in the Urban Waterlogging Area Using Deep Learning Approach

Xiefei ZHI#+
Nanjing University of Information Science & Technology

With the continuous intensification of global climate change and the rapid development of urbanization, urban waterlogging disasters caused by extreme rainfall process have become increasingly serious, which has become a serious challenge for numerous cities around the world. Based on the rainfall data of 75 national automatic meteorological observation stations in Zhuji City, Zhejiang Province, from May to August 2021, and the water level data of 2 typical water level stations, the relationship between rainfall and water level was investigated using the deep learning model long short-term memory (LSTM) to provide the water level prediction in the urban waterlogging areas for the future 2 hours at an interval of 15 minutes. The results show that the forecast skill of the deep learning model decreases with the increase of the forecast time. The forecast performance is quite good to use the water level and rainfall data in the previous 4 hours to predict the water level in the next 2 hours. For the high-value water level prediction, the root-mean-square error (RMSE) of the prediction at the two water level stations using the previous 4h data is less than 5.5 cm, the correlation coefficient (CC) is more than 0.92, and the Nash–Sutcliffe model efficiency coefficient (NSE) is more than 0.85, indicating that the constructed deep learning model for waterlogging prediction has good prediction skill.


AS43-A009
Application of Machine Learning in Predicting Current and Future Climate Extremes in China

Kelvin NG1#+, Gregor C. LECKEBUSCH1, Kevin HODGES2
1University of Birmingham, 2University of Reading

Climate extremes pose a significant risk to society due to their potential regional negative socioeconomic impacts. In order to develop optimal strategies to mitigate the impact of climate extremes on society, it is necessary to strengthen our ability to predict climate extremes on different timescales. While the performance of dynamical models has improved substantially over the past few decades, predicting extreme events remains an open challenge. This is partially due to limited climate model simulation periods and observations so that the full intensity distributions are not sampled sufficiently for the tail of the distributions. It is also due to current coarse model spatial resolutions which are therefore not being able to represent all the characteristics of extreme events as well as their inability to fully represent all necessary processes on relevant scales for extreme event generation, from small to synoptic and hemispheric scales. However, hemispheric scales can provide important driving information via scale interactions and are generally seen as being better captured by dynamical models. Yet, the accuracy of extreme event prediction might be improved by combining usable information from dynamical models and data-driven, machine learning methods.
In this presentation, we provide an overview of the PRE-CAX project, which aims to develop suitable tools for climate services to predict extreme regional rainfall over China in the future climate. This is achieved by combining large scale climate modes, which are relatively well-represented in dynamical models and machine learning approaches, such as the causal network discovery algorithm. We further show the performance of our approach in improving the prediction of extreme Mei-yu front related precipitation over China using data from the CMIP6 simulations. Application of our approach on different timescales and the potential development of the methodology are also discussed.


AS43-A005
Data-driven Machine Learning Model for the Prediction of Pacific Sea Surface Temperature Prediction

John Chien-Han TSENG1#+, Bo-An TSAI2, Kaoshen CHUNG2
1Central Weather Bureau, 2National Central University

Most numerical weather models are difficult to proceed the long-term prediction. Some reasons are from the uncertainty of the proper initial condition and those unresolved physical processes. Part reasons are from the incomplete governing equation calculation and numerical scheme errors becoming increasingly over time. Traditionally the operational weather centers will consider the ensemble members forecasts or modify the data assimilation cycle to response the unknown future. However, this kind of numerical model calculation cost is very high especially in long-term predictions. For saving the computational cost, Brunton et al. (2020) suggest the computational fluid dynamics problems can be solved by dimensional reduction data-driven model instead of numerical schemes in an original high dimensional space. Tseng (2022) found that Pacific sea surface temperature (SST) leading principal components (PC) of isometric feature mapping (ISOMAP) showed meaningful trajectories. These leading PCs forms a set of low-dimensional trajectories for machine learning algorithms to simulate and to do the forecasts. In this study, we used support vector regression (SVR) and feedforward neural network (NN) to train the data of leading 20 SST ISOMAP PCs. The SVR and NN models can predict the future variation of these 20 leading PCs. Combining these prediction PCs and the residual PCs from former historical PCs multiplied by spatial empirical orthogonal functions (EOF) enables the prediction of SST. The root mean square error (RMSE) and anomaly correlation coefficient (ACC) were checked. The NN prediction could get the pretty small RMSE and high ACC score in recent 5 cases 10 lead months prediction. Moreover, the computing cost was more economic than traditional NWP models.


AS43-A017
Verification of Improved Analog Ensemble Methods for Forecasting Extreme Temperature and Wind Speed in Beijing

Cui HAO#+
Beijing Meteorological Observatory, Beijing

Upon the current requirement of the extreme weather forecast and service, we developed two improved prediction schemes (that is, scheme I and scheme II) based on the ECMWF-IFS model (EC model) and the model output statistics (MOS) method on the basis of the Analog Ensemble (AnEn) method. First, taking the EC model forecasts from 2016 to 2018 and their corresponding observations as the training dataset, the overall performance of scheme I, scheme II, and AnEn for the extreme temperature and wind speed in Beijingfrom January 1 to December 31 in 2019 is tested and evaluated against the observations at 364 stations. The results show that the prediction accuracy of scheme I and scheme II is better than that of AnEn for both extreme temperature (T) and wind speed (VM), particularly for scheme II. Second, according to the 2nd and 98th percentiles, the thresholds of extreme low temperature (Tm) and extreme high temperature (TM) at the different stations in Beijing are -22.3 ℃ and 38.8 ℃, respectively. The overall prediction results of scheme I and scheme II for T in this region show that the two schemes are significantly improved compared to AnEn, and their mean absolute errors (EMA) are reduced by 11.90% and 21.43%, respectively. Similarly, according to the 98th percentile, the VM threshold of each station in Beijing is set at 20.3 m·s-1, and the EMA of VM forecast with scheme I and scheme II is reduced by 23.08% and 26.52%, respectively, compared with AnEn. Finally, the prediction results of Tm, TM and VM at each station in Beijing show that scheme I and scheme II have improved in T and VM on the basis of AnEn, and more than 94% of stations show that scheme II has better performance. In addition, the spatial distributions of prediction accuracy of T and VM show that the two improved schemes have better performance on the prediction of T and VM in the mountainous areas than in the plain areas.


Wed-02 Aug | 3:30 - 5:15 | MR329
AS20 - Weather and Climate Studies with High Performance Computing

Session Chair(s): Anurag DIPANKAR, ETH Zurich

AS20-A012 | Invited
GPU Development of Km-scale AGCMs to Drive Earth Digital Twins

Stanley POSEY#+
NVIDIA Corporation

Efforts are underway in the climate modeling community towards refining the horizontal resolution of atmosphere GCMs from today’s 25–50 km to about 1 km, in order to explicitly resolve some of the small-scale convective cloud processes and provide more realistic local information on climate change. At the same time, Exascale HPC systems have finally arrived and in most cases are powered by GPU accelerator technology that offers opportunities in reasonable simulation turn-around times balanced with efficiency in energy consumption. High-resolution model projects such as the European nextGEMS and the global DYAMOND initiative have motivated NVIDIA collaboration in GPU development of Exascale-ready AGCMs for use in storm-resolving Earth system models. This work will be presented in three parts: (i) describe the challenges and expectations for the directions of programing methods, GPU strong-scaling experiences, and post-processing requirements; (ii) present the state-of-play and expectations for km-scale AGCMs such as ICON, IFS, and MPAS; and (iii) how the km-scale model data will be applied to provide the synthetic data for large-scale training of AL/ML surrogate ESMs. A particular challenge addressed relates to the enormous growth in output volumes of high-resolution simulations that can make it impractical or impossible to store data, and require in-situ post-processing and ML model training as the data is generated. Ultimately the km-scale model data will become the essential baseline behind the vision in the development of Earth digital twins from programs like the EU Destination Earth and NVIDIA Earth-2.


AS20-A002
EXCLAIM: Extreme Scale Computing and Data Platform for Cloud-resolving Weather and Climate Modelling

Anurag DIPANKAR1#+, Mauro BIANCO2
1ETH Zurich, 2Swiss National Supercomputing Centre

EXCLAIM aims at developing a modeling infrastructure that can allow the climate models to simulate the Earth’s climate at a substantially higher resolution. Explicit representation of key climate processes (e.g. moist convection) at such high resolution should allow for reduced uncertainty in the future climate projection simulated by these models. The climate model used for this exercise is ICON based that is developed jointly by the Max Planck Institute for Meteorology in Hamburg, Germany, and the German weather service. The approach taken by EXCLAIM to reach the performance target is to re-write the currently Fortran-based monolithic codes into a descriptive user code based on Python, which is then translated into standard imperative language (e.g., C++) for specific architectures using a toolchain based on GT4Py (GridTools for Python). However, performance gain alone doesn’t ensure sustainable software development for a code that is already too complex. A modularized code structure is therefore envisioned. Modularization is performed down to the smallest reasonable part of the code- termed granules- that can be tested in isolation, and in combination with other granules. Status of these developments and how they address the needs of ultra-high-resolution modeling while allowing for further innovation will be presented.


AS20-A017
A Heterogeneous Coupling Library h3-Open-UTIL/MP

Takashi ARAKAWA1#+, Shinji SUMIMOTO1, Hisashi YASHIRO2, Kengo NAKAJIMA1
1The University of Tokyo, 2National Institute for Environmental Studies

"Heterogeniety" is one of the key words of recent years in high-performance computing. In fact, the majority of the systems at the top of the TOP500 list are heterogeneous system composed of CPUs and GPUs. This heterogeneity can be classified into two categories. The one is Intra node heterogeneity, such as GPU machine and VE machine. And the other is internode heterogeneity, such as CPU node + GPU node, or CPU node + VE node. Our presentation will focus on the later system. The reason for the development of such a system is that role of HPC has expanded beyond not only simple simulation but also to large-scale data analysis and machine learning. Therefore, software that allows to interact simulation programs with Data analysis/AI programs on heterogeneous systems is required. Based on these backgrounds, we are developing a heterogeneous coupling library h3-Open-UTIL/MP, as a part of the h3-Open-BDEC project.H3-Open-UTIL/MP is a general-purpose coupling library which can couple any simulation models and applications that meet the following two conditions: 1) it has uniquely numbered and time-invariant grid points, and 2) the time interval of data exchange does not change in time. In addition, it can couple on heterogeneous environment by collaborating with a communication library h3-Open-SYS/WaitIO. In out presentation, we will describe the structure and function of h3-Open-UTIL/MP and discuss the results of performance measurements and application examples


AS20-A015 | Invited
Establishing a Non-hydrostatic Global Atmospheric Modeling System at 3-km Horizontal Resolution with Aerosol Feedbacks on the Sunway Supercomputer of China

Chun ZHAO#+
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.


AS20-A019
Evaluating the Relationship Between Tropical Cyclone Genesis Frequency and Environmental Conditions by Using a NICAM Large Ensemble Simulation

Yohei YAMADA1#+, Masuo NAKANO1, Tomoki MIYAKAWA2, Chihiro KODAMA1, Akira YAMAZAKI1, Daisuke TAKASUKA2, Tomoe NASUNO1, Hisashi YASHIRO3, Masato SUGI4, Masaki SATOH2
1Japan Agency for Marine-Earth Science and Technology, 2The University of Tokyo, 3National Institute for Environmental Studies, 4Japan Meteorological Agency

Previous studies reported environmental parameters associated with tropical cyclone genesis (TCG): the Coriolis parameter, low-level relative vorticity, ocean thermal energy, relative humidity in the mid-troposphere, atmospheric static stability and vertical wind shear. Although various definitions were proposed by previous studies, a Genesis Potential Index (GPI) is obtained by combining these parameters. The GPI well captures seasonal cycles of TCG frequency on each ocean basin. However, reproducibility of its interannual variability seems to be less than that of seasonal cycles. According to ensemble simulation with explicitly representing tropical cyclones, the number of TCG frequencies varied among ensemble members. This may suggest that ensemble simulation is required for accurately evaluating a relationship between TCG frequency and environmental conditions (GPI). To evaluate the relationship, a large ensemble simulation (64 members) was performed for the boreal summer (June-September) during 2009-2019 by using Nonhydrostatic Icosahedral Atmospheric Model, NICAM with a horizontal grid spacing of 14 kilometers. In the ensemble mean, the correlation coefficient R between TCG frequency and environmental conditions (GPI) is 0.59 for the western North Pacific, 0.92 for the eastern North Pacific and 0.91 for the North Atlantic, respectively. These were higher than those of each ensemble member for the three ocean basins. The result indicates ensemble simulation is possibly useful to evaluate the relation of TCG to the environmental conditions.


AS20-A006
Convolutional Long and Short Term Memory Network (ConvLSTM) for Extreme Precipitation Nowcasting Technique

Chao TAN1,2+, Ji CHEN1#
1The University of Hong Kong, 2The University of Hong Kong

Accurate nowcasting of precipitation is 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. In order to improve the forecast capability of extreme precipitation, this study establishes two forecast schedules based on the convolutional long short-term memory neural networks (ConvLSTM) trained with 10-year precipitation dataset from National Oceanic and Atmospheric Administration Climate Prediction Center MORPHing technique (NOAA-CMORPH) in the Guangdong-Hong Kong-Macao Great Bay Area. The results show that, the time-jump forecasting schedule could yield better performance from the third forecast time step, although the difference between the traditional hour-by-hour forecast (the original scheme) and the time-jump forecast (the improved scheme) is not significant at the beginning. In terms of performance metrics, the root mean squared error (RMSE) of the improved scheme is generally smaller than that of the original scheme at about precipitation, and the correlation coefficient is generally higher than that of the original scheme at about precipitation. Both training set and testing set show good alignment. The experiments proves that ConvLSTM is an effective in forecasting near precipitation, specially in the first two times, but coupling with improved schedule can advance the forecast of near precipitation by at least 6 hours, and its RMSE is less than 0.02 and the correlation coefficient is not less than 0.6 compared to the observation results.


AS20-A013
A Neural Network-based Scale-adaptive Cloud-fraction Scheme for GCMs: Offline Evaluation Based on the ERA-Interim Reanalysis

Guoxing CHEN1#+, Wei-Chyung WANG2
1Fudan University, 2University at Albany - State University of New York

Cloud fraction significantly affects the short- and long-wave radiation. However, its realistic representation in GCMs has been difficult due to inadequate understanding of the sub-grid scale cloud macro- and micro-physical properties. Recently, we turned to the data-driven approach by developing a neural network-based scale-adaptive (NSA) cloud-fraction scheme using CloudSat data. Preliminary findings indicate the significant potential of correcting the known GCMs’ biases in cloud spatial distribution and the associated cloud radiative forcing. In this study, we present further evaluations of the NSA cloud fraction scheme by employing the ERA-Interim reanalysis in which the cloud condensates were simulated based on the assimilated temperature and humidity. Characteristics of the simulated cloud fraction and the associated cloud radiative forcing will be presented and discussed versus the observations and simulations using other cloud fraction schemes, e.g., the Tiedtke scheme (embedded in the ERA model) and the Xu-Randall scheme.


Wed-02 Aug | 3:30 - 5:15 | MR331
AS23 - Observations, Remote Sensing, and Modeling of Tropospheric Composition and Air Quality in Asia and the Transpacific Region

Session Chair(s): Richard ECKMAN, National Aeronautics and Space Administration

AS23-A017 | Invited
The Deadly Toll of Heavy Air Pollution in Asia: An Estimate of Mortality Attributable to the Long-term PM2.5 Exposure Based on NASA MERRA-2 Reanalysis

Hongbin YU1#+, Alexander YANG1, Qian TAN2, Chamara RAJAPAKSHE1, Mian CHIN3
1NASA Goddard Space Flight Center, 2Bay Area Environmental Research Institute, 3NASA GSFC

Densely populated Asia has been experiencing heavy air pollution in recent decades due to increased human activities and wind blowing dust, raising grave concerns of detrimental impacts on human health. Ambient PM2.5 concentrations often exceed the unhealthy level in broad regions of China and India, the two most populous countries in the world. This study quantifies premature deaths attributable to long-term exposure of ambient PM2.5, or PM2.5-attributable mortality, by dust and pollution sources. We use NASA’s Modern-Era Retrospective Analysis for Research and Applications, Version 2 (MERRA-2) aerosol reanalysis product for PM2.5 validated by observations from the United States Diplomatic Posts to estimate the PM2.5-attributable mortality for five causes of deaths. The estimated yearly global PM2.5-attributable mortality in 2019 amounts to 2.89 (1.38 ~ 4.48) millions, of which about 22% are caused by desert dust. The mortality counts vary with geopolitical regions substantially, with more than 75% of the global mortality occurring in Asia. China and India take the highest mortality tolls, accounting for 43% and 23% of the global PM2.5-attributable deaths, respectively. Other Asian countries among the top ten PM2.5-attributable death tolls are Pakistan, Bangladesh, Indonesia, and Nepal. Enforcing air pollution regulations to transfer areas from PM2.5 nonattainment to PM2.5 attainment can have great health benefits. However, regulations should go beyond what are currently implemented in China and India. Being attainable with the U.S. air quality standard globally would have avoided nearly 40% or 1.2 million deaths, mostly over Asia. Our study manifests the importance of distinguishing aerodynamic size from geometric size in defining PM2.5 and accurately assessing the health burden. A use of geometric size in diagnosing dust PM2.5 from the model simulation overestimates the PM2.5 level in the dust belt by 40-170%, leading to an overestimate of global mortality by 32%. 


AS23-A036 | Invited
The Significant Contribution of Small-sized and Spherical Aerosol Particles to the Decreasing Trend in Total Aerosol Optical Depth Over Land from 2003 to 2018

Huizheng CHE#+, Ke GUI
Chinese Academy of Meteorological Sciences

The optical and microphysical properties of aerosols remain one of the greatest uncertainties associated with evaluating the climate forcing attributed to aerosols. Although the trends in aerosol optical depth (AOD) at global and regional scales have been widely examined, little attention has been paid to the trends in type-dependent AODs related to aerosol particle properties. Here, using the aerosol optical component dataset from the Multi-angle Imaging Spectro Radiometer (MISR) instrument, we investigate decadal-scale trends in total aerosol loading as well as AODs for five aerosol components by particle size and morphology during 2003–2018 over land. The relative contribution of each type-dependent AOD to the overall TAOD trends was quantified. By dividing the TAOD values into four different aerosol pollution levels (APLs) with splits at 0.15, 0.40, and 0.80, we further explored the relationships between TAOD changes and interannual variations in the frequency-of-occurrences (FoOs) of these APLs. Long-term trends in FoOs in the different APLs show that there was a significant improvement in air quality between 2003 and 2018 in most land areas, except South Asia, corresponding to a shift from lightly polluted to clean conditions. However, the effects of different APLs on TAOD changes are regionally dependent and their extent of correlation varied spatially. Moreover, we observed that the annual mean TAOD has decreased by 0.47%·a-1 over land since 2003 (P < 0.05). This significant reduction was mainly attributed to the continued reduction in small-sized (< 0.7mm diameter) AOD (SAOD) and spherical AOD (SPAOD). Statistical analysis shows that SAOD and SPAOD respectively accounted for 57.5% and 89.6% of the TAOD, but contributed 82.6% and 90.4% of the trend in TAOD. Our study suggests that small-sized and spherical aerosols composed of sulfate, organic matter, and black carbon play a dominant role in determining interannual variability in land TAOD.


AS23-A032
Changes in Aerosol Loading Before, During and After the COVID-19 Pandemic Outbreak in China: Effects of Anthropogenic and Natural Aerosol

Yuanxin LIANG+, Huizheng CHE#, Ke GUI
Chinese Academy of Meteorological Sciences

Anthropogenic emissions reduced sharply in the short-term during the coronavirus disease pandemic (COVID-19). As COVID-19 is still ongoing, changes in atmospheric aerosol loading over China and the factors of their variations remain unclear. In this study, we used multi-source satellite observations and reanalysis datasets to synergistically analyze the spring (February–May) evolution of aerosol optical depth (AOD) for multiple aerosol types over Eastern China (EC) before, during and after the COVID-19 lockdown period. Regional meteorological effects and the radiative response were also quantitatively assessed. Compared to the same period before COVID-19 (i.e., in 2019), a total decrease of −14.6% in tropospheric TROPOMI nitrogen dioxide (NO2) and a decrease of−6.8% in MODIS AOD were observed over EC during the lockdown period (i.e., in 2020). After the lockdown period (i.e., in 2021), anthropogenic emissions returned to previous levels and there was a slight increase (+2.3%) in AOD over EC. Moreover, changes in aerosol loading have spatial differences. AOD decreased significantly in the North China Plain (−14.0%, NCP) and Yangtze River Delta (−9.4%) regions, where anthropogenic aerosol dominated the aerosol loading. Impacted by strong wildfires in Southeast Asia during the lockdown period, carbonaceous AOD increased by +9.1% in South China, which partially offset the emission reductions. Extreme dust storms swept through the northern region in the period after COVID-19, with an increase of +23.5% in NCP and +42.9% in Northeast China (NEC) for dust AOD. However, unfavorable meteorological conditions overwhelmed the benefits of emission reductions, resulting in a +20.1% increase in AOD in NEC during the lockdown period. This study highlights that we can benefit from short-term controls for the improvement of air pollution, but we also need to seriously considered the cross-regional transport of natural aerosol and meteorological drivers.


AS23-A035
Seasonal Cycles and Long-term Trends of Arctic Tropospheric Aerosols Based on Calipso Lidar Observations

Wenrui YAO+, Ke GUI, Yu ZHENG#, Lei LI, Yaqiang WANG, Huizheng CHE, Xiaoye ZHANG
Chinese Academy of Meteorological Sciences

Notable warming trends have been observed in the Arctic, with tropospheric aerosols being one of the key drivers. Here the seasonal cycles of three-dimensional distributions of aerosol extinction coefficients (AECs) and frequency of occurrences (FoOs) for different aerosol subtypes in the troposphere over the Arctic from 2007 to 2019 are characterized capitalizing on Cloud–Aerosol Lidar with Orthogonal Polarization (CALIOP) Level-3 gridded aerosol profile product. Seasonal contributions of total and type-dependent aerosols through their partitioning within the planetary boundary layer (PBL) and free troposphere (FT) are also quantified utilizing the Modern-Era Retrospective Analysis for Research and Applications, version 2 (MERRA-2) PBL height data. The results show substantial seasonal and geographical dependence in the distribution of aerosols over the Arctic. Sulfate, black carbon (BC), and organic carbon (OC) contribute most of the total AEC, with Eurasia being the largest contributor. The vertical structure of AECs and FoOs over the Arctic demonstrates that the vertical influence of aerosols is higher in eastern Siberia and North America than in northern Eurasia and its coasts. When the total aerosol optical depth (TAOD) is partitioned into the PBL and FT, results indicate that the contributions of TAOD within the FT tend to be more significant, especially in summer, with the FT contributes 64.2% and 69.2% of TAOD over the lower (i.e., 60° N–70° N) and high (i.e., north of 70° N) Arctic, respectively. Additionally, seasonal trend analyses suggest Arctic TAOD exhibits a multi-year negative trend in winter, spring, and autumn and a positive trend in summer during 2007–2019, due to an overall decrease in sulfate from weakened anthropogenic emissions and a significant increase in BC and OC from enhanced biomass burning activities. Overall, this study has potential implications for understanding the seasonal cycles and trends in Arctic aerosols.


AS23-A060
Evaluating Long Range Transport of Aerosols in Reanalysis and Climate Model Simulations: A Synergistic Approach Using Remote Sensing Observations and Modeling

V. VINOJ1#+, Sanatan BINISIA1, Indra Sekar SEN2
1Indian Institute of Technology Bhubaneswar, 2Indian Institute of Technology Kanpur

The long range transport is known to modulate aerosol loading over regions separated by large distances. However, their simulations in either reanalysis or chemical transport or climate models depend on multiple factors such as emissions, transport, wet and dry removal mechanisms and secondary aerosol production. Due to such dependence on multiple factors, they are also prone to significant errors that are difficult to evaluate. Current evaluation methods compare observed and simulated loading conditions and provide some insights. However, such evaluation/validation exercises using only aerosol loading are prone to significant errors due to modulations associated with long range transport, either towards or away from the regions of concern. Here, a method is developed by merging the conventional concentration weighted trajectories and MODIS satellite observations along with reanalysis to understand long range transport over the south Asian region simulated by MERRA-2. The method is able to capture most of the distinct emission sources (both natural and anthropogenic) over the South Asian region such as the Indo-Gangetic Plains, Thar Desert, Middle East deserts etc. Arabian Sea and North-East Indian regions are shown to be an evolving virtual aerosol source region in addition to the known sources such as the middle east, Thar desert, Indo-Gangetic Plains etc. The fidelity of the method is qualitatively evaluated using natural mineral dust and sea-salt aerosols simulated by MERRA-2 which shows reasonable agreement with known sources over the middle east, Talkamakan and south Asia. However, it appears that MERRA-2 transports dust aerosols further than that estimated using MODIS-Terra indicating limitations in model physics and hence reflected in limitations in the long-range transport of aerosols. Analysis such as these will allow an understanding of model capability/limitations in the long-range transport of aerosols allowing future improvements in aerosol modeling and impact studies.


AS23-A056
Evaluation of Chemical Mechanisms in WRF-Chem for Aerosol Formation and Chemical Evolution Over the Tropics

Santo V. SALINAS#+, Li TAN, Fernando SANTOS, Soo Chin LIEW
National University of Singapore

Singapore and the South-East Asia (SEA) are regularly affected by mild to severe episodes of large scale biomass burning due to regional forest fires that occur during the region’s season of drought and dryness. During such events, satellite and in-situ observations are first hand tools for monitoring smoke spatial and temporal evolution. However, understanding aerosol formation and evolution during biomass burning events requires understanding the role of gas-phase precursors in aerosol processes and PM2.5 formation specially over the tropics where deep convection, high temperature and humidity play an important role. To investigate the effect of gas-phase chemical schemes and aerosol formation mechanisms on the reconstruction of MP2.5 concentrations and optical properties of aerosols we perform simulation experiments using the mesoscale Weather Research and Forecasting (WRF) meteorological model with chemistry (WRF-Chem). We evaluate WRF-Chem 4.2 newly added MOZCART-T1 scheme (MOZART gas-phase chemistry with 142 species and GOCART bulk aerosol scheme) and the standard MOZART gas-phase chemistry chemical mechanism (81 gas phase species) with MOSAIC 4-bin sectional aerosol module that includes aqueous phase chemistry. We perform detailed calculations of aerosol composition and properties over periods of stagnancy (no transported biomass emissions) and during biomass burning periods during year 2019 and contrasted by aerosol optical depth and PM2.5 ground measurements. Finally, we discuss the suitability of the T1/MOZART-MOSAIC implementation to better represent aerosol formation and processes over the tropics.


Wed-02 Aug | 3:30 - 5:15 | MR332
AS30 - Mesoscale and Orographic Effects on Airflow, Precipitation and Weather Systems

Session Chair(s): Fang-Yi CHENG, National Central University

AS30-A005
A Trigger of Small-scale Terrain to Generate Stationary Precipitating Systems Under Extremely Humid Conditions

Tetsuya TAKEMI#+, Nanami NAKA
Kyoto University

During the rainy season in Japan (i.e., Baiu season), the environmental conditions are generally very humid, with a large amount of precipitable water vapor and high relative humidity. Stationary precipitating systems sometimes develop during the rainy season, which will spawn an extreme amount of rainfall, flooding, landslides, and so on. Recent studies have investigated climatological characteristics of stationary precipitating systems over the Japanese islands by using long-term datasets. During the warm season including the rainy season, a humid condition not only at low levels but also at middle levels is commonly seen. A condition that host moist absolutely unstable layers (MAULs) is sometimes seen in cases with heavy rainfalls. This study investigates the environmental conditions for the generation of extreme-rain-producing, stationary precipitating systems that recently occurred in northern Kyushu Island, Japan. It is indicated that precipitable water vapor content is extremely large as compared with the climatology of stationary precipitating systems, which is due to very humid conditions close to be saturated. Under this humid situation, MAULs appear in the lower to middle troposphere, adjacent to or as a part of stationary precipitating systems. It is also found that the volume of MAULs has a correlation with the amount of heavy rainfalls. A moist absolutely unstable condition is a state that indicates a potential for the development of convective motion. Therefore, a certain triggering mechanism is required. In the case of the July 2017 heavy rainfall case in northern Kyushu, small-scale terrain induces a convergence locally, which serves as a triggering in a moist absolutely unstable condition.


AS30-A011
Persistent Rainbows Induced by the East Asian Winter Monsoon and Mesoscale Mountains in Northern Taiwan

Kun-Hsuan CHOU#+
Chinese Culture University

Rainbows appeared in the sky above Taiwan’s Chinese Culture University (CCU) for nearly nine hours continuously on 30 November 2017. This had been confirmed the world's longest-lasting rainbow which was visible from 6:57 a.m. to 3:55 p.m. by Guinness World Records. Three main reasons contributed to the occurrence of this rainbow of record-setting duration at CCU on Yangmingshan mountain range, namely geographical location, topographical features, and suitable weather conditions. Taiwan is located in a subtropical region, which is frequently affected by winter monsoons during autumn and winter. The relevant topographical features represent there are several mountains located over the northern side of Taipei Basin. Last, the campus was located over one peak of Yangminshan mountain area, which helps the observers could see the rainbow with elevation angles below the horizon during the noon time. This special phenomena of rainbow have been studied by observation and forecast approaches since autumn 2018. First, rainbow monitoring mainly uses several cameras to capture images over the northern sky. Five-year statistics show that, on average, there were 36 rainbow days from October to next January, with an average of once every 3.4 days. Compared with the frequency of occurrence in years, the frequency is the highest during the autumn and winter of 2020, with as many as 51 days. In terms of monthly occurrence frequency, November had the highest average of 11 days, followed by December with an average of 10 days. Besides, rainbow forecasting has been developed in autumn 2019. The rainbow weather index (RWI) and rainbow probability (RP) are formulated based on WRF 1.1-km resolution forecast data. In terms of the forecast performance of RP forecast in 2019-20 and 2020-21, the accuracy rate is 77%, the detection rate is 83%, and the Heidke Skii Score is 0.59 for 215 verification days.


AS30-A013
Taiwan Rainbands Formed in the Outer Region of Tropical Cyclones

Che-Yu LIN#+, Cheng-Ku YU
National Taiwan University

This study used Doppler radar data, surface observations, and National Centers for Environmental Prediction reanalysis data to explore the statistical characteristics of Taiwan rainbands (TRs) that formed in the outer region of tropical cyclones (TCs). A comprehensive examination of the available radar measurements from 2002–2017 identified a total of 103 TRs from 44 TC events and showed that approximately 47% of all TCs influencing Taiwan could develop TRs. The spatial distribution of TR formation exhibited a substantial offshore extent, with the highest frequency observed ~25–100 km offshore. The TRs tended to be initiated when the northwestward-moving typhoons passed over the oceanic area northeast of Luzon Island (122°–127° E and 16°–20° N), the Philippines. This track characteristic brought stronger easterly onshore flow to the eastern coast of Taiwan and favored the development of a pronounced coastal pressure ridge. In particular, the offshore convergence caused by upstream deceleration of the onshore flow due to orographic blocking was found to be a primary contributor to the initiation of the TRs. The strength of the observed coastal pressure ridge and its high correlation with the intensity of environmental onshore flow associated with outer circulations of TCs were consistent with the theoretical prediction of pressure distributions generated as incident flow interacted dynamically with the Taiwan topography. Results from the study suggest that the typhoon location relative to the Taiwan landmass is a critical factor determining TR initiation.


AS30-A002
Impact of Parameterized Topographic Drag on a Simulated Northeast China Cold Vortex

Mingshan LI1#, Xin XU1+, Shuixin ZHONG2, Yuan WANG1
1Nanjing University, 2China Meteorological Administration

Northeast China cold vortex (NECV) is the major influencing weather system in northern China. This work studies the influence of subgrid orographic drag (SOD) on a heavy-rain-producing NECV occurred in July 2011 using the Weather Research and Forecasting (WRF) model. A series of numerical experiments are conducted with different parameterizations of SOD including turbulent orographic form drag (TOFD), flow blocking drag (FBD) and mountain wave drag (MWD). Results show that the NECV intensity is overestimated in the absence of SOD parameterization, accompanied with too-low geopotential height (GPH) and too-strong horizontal winds. The parameterization of TOFD can significantly decelerate the 10-m winds, whereas the FBD and MWD play a minor role. However, the influence of TOFD is overwhelmed by FBD and MWD in the troposphere, especially the latter. The lower-tropospheric MWD directly weakens the convergence and ascent motion of the NECV, producing an anti-cyclonic circulation that uplifts the GPH. This MWD-induced circulation indirectly weakens the NECV in the mid-upper troposphere by producing a warm advection difference. 


AS30-A017
Characteristics and Processes of Orographic Precipitation Over Da-Tun Mountain Associated with Typhoon Saola (2012)

Ming-Jen HSU#+, Cheng-Ku YU, Lin-Wen CHENG
National Taiwan University

This study uses high-resolution rain gauge data, Doppler radar observations, and an orographic precipitation diagnostic model to identify the detailed characteristics and intensity of orographic precipitation over Da-Tun Mountain associated with Typhoon Saola (2012). The occurrence of heavy precipitation for this typhoon event was concentrated over Da-Tun Mountain as Saola moved northwestward, approached Taiwan and brought strong northeasterly/eastly flow (18-36 m s-1) impinging on the northern coast of Taiwan. Da-Tun Mountain, is a three-dimensional, isolated mountain barrier located at the northern coast of Taiwan with peaks of approximately 1 km MSL. More than 450 mm of rainfall during the 13-h study period was observed over the mountain crest, and two rainfall enhancement stages were identified. For the first stage at the earlier time, the typhoon background precipitation was mostly characterized by stratiform precipitation with relatively stronger upstream winds (30~36 m s-1), whereas the second stage was characterized by more convective background precipitation and relatively weaker upstream winds (20~28 m s-1). The simulations of the diagnostic model revealed that the seeder-feeder process can better quantify the rainfall enhancement during the first stage with stratiform background rainfall. Under convective background rainfall during the second stage, orographic lifting of low-level oncoming winds might modulate the convective cells’ circulation and precipitation, further complicating the microphysical processes of orographically enhanced precipitation.


AS30-A012
The Study of the Lightning Distribution and its Formation Mechanism Over the Strait of Malacca

Kai-Chun WANG1#+, Kun-Hsuan CHOU2, Chun-Ming YEH1
1Graduate Institute of Earth Science, Chinese Culture University, 2Department of Atmosphere Sciences, Chinese Culture University

This study mainly analyzed the lightning distribution characteristics of the Strait of Malacca area in Southeast Asia from 2005 to 2019 and explored the physical mechanisms of lightning formation therein. The lightning data used in this study were obtained from the WWLLN developed by University of Washington; the data mainly comprise frequencies of cloud-to-ground lightning. Reanalysis data of the ECMWF were also used as meteorological data for analysis. In addition, variables pertaining to the surface wind field, CAPE, and OLR were examined to explore the thermodynamic and dynamic conditions when lightning occurs. Analysis of the average lightning frequencies over 15 years revealed that the area with the most frequent lightning activities in Southeast Asia was near the Strait of Malacca. By contrast, lightning frequencies were lower on land. Both land and sea areas presented notable diurnal cycles. Lightning at sea mostly occurred at night and lasted until the next morning, whereas lightning on land frequently occurred between afternoon and night. Further analysis of yearly, seasonal, monthly, and hourly changes in lightning distributions also revealed notable diurnal cycles. In addition, seasonal differences were observed in lightning frequencies. The ITCZ near the equator exhibited a northward or southward movement during different seasons, which in turn induced the relatively high frequencies of lightning in Southeast Asia in spring and autumn. Moreover, lightning that occurred in the terrestrial area on the eastern side of the strait led the lightning on the western terrestrial area of the strait by approximately 2 hours. This phenomenon might be attributable to the topography and airflow directions of the strait. Finally, the study results revealed that lightning frequencies exhibited a strong correlation with the convergence of surface airflows, indicating the diurnal cycle of land–sea breeze as the main mechanism for lightning formation at the Strait of Malacca.


AS30-A007
Clustering of Distinct “Wind-precipitation” Regimes Over the West Coast of India During Asian Summer Monsoon

Prajwal K.1#+, Ajil KOTTAYIL1, Prince XAVIER2
1Cochin University of Science and Technology, 2Met Office Hadley Centre

The Asian Summer Monsoon is a seasonal reversal of wind direction that brings heavy rainfall to the Indian Subcontinent. The variability within the season has been of key interest to researchers for decades. Wind and precipitation are closely linked, as winds help in distributing moisture. In this study we show that large scale variability within the monsoon season over the west coast of India is embedded within five different unique wind-precipitation clusters. Five different wind-precipitation clusters have been identified using the k-means algorithm. The core speed of low level jet obtained from wind profiler radar data and India Meteorological Department gridded rainfall are used for clustering. This study attempts to understand the large-scale dynamics of the variability within each wind-precipitation cluster. We also use ERA-5 (Specific Humidity, Mean Sea Level Pressure, vertical, zonal and meridional velocity profiles, and 850 hPa Divergence), NOAA OISST (Daily Optimum Interpolation Sea Surface Temperature) and CERES top of the atmosphere (toa) radiative flux data to study the large scale features. The different wind-precipitation clusters observed over the west coast are influenced by synoptic scale background conditions such as active-break cycle of the monsoon, monsoon depressions, tropical cyclones, mid-tropospheric moisture intrusion, Madden Julian Oscillation etc.


Thu-03 Aug | 8:15 - 10:00 | MR311
AS15 - 16th Sasaki Symposium on Data Assimilation for Atmospheric, Oceanic and Hydrologic Applications

Session Chair(s): In-Hyuk KWON, Korea Institute of Atmospheric Prediction Systems, Wei KANG, Naval Postgraduate School

AS15-A013 | Invited
Current Status of the KIAPS Data Assimilation System, and Plans for Hydrometeor Analysis

In-Hyuk KWON1#+, Adam CLAYTON1, Jeon-Ho KANG1, Sihye LEE1, Han-Byeol JEONG1,2, Dayoung CHOI1
1Korea Institute of Atmospheric Prediction Systems, 2Ewha Womans University

The renewed Korea Institute of Atmospheric Prediction Systems (KIAPS) 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. 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 based on a cubed-sphere grid, utilizing 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 a LETKF for ensemble perturbation updates, and is already giving good performance. Many types of observations, including conventional data, GPS-RO, AMSR2, AMSU-A, MHS, ATMS, MWHS2, IASI, CrIS, AMV, Scatwind, and clear sky radiances from GK-2A, MSG and Himawari are quality controlled and prepared for assimilation by the KIM Package for Observation Processing (KPOP). Recently, we added support for the assimilation of ALADIN wind data and Ground GNSS, and we are testing support for MODE-S aircraft, AWS, GMI, GIIRS, and clear sky radiances from GOES. All-sky radiance for MHS is also developed and tested.
During the next few years, a further model will be developed to support high-resolution DA and forecasting over East Asia. DA focused on radar and other observations that can provide useful information on the additional small scales supported within the grid-refined region. We have tested radar reflectivity assimilation with LETKF for the WRF model. Cloud hydrometeor will be analyzed by LETKF using radar observation and all-sky radiance from geostationary satellites.


AS15-A016
How Does the Ensemble Benefit Ensemble-variational Data Assimilation in the Tropics?

Joshua LEE1#+, Ross BANNISTER2, Javier AMEZCUA3
1Centre for Climate Research Singapore, 2University of Reading, 3Tecnológico de Monterrey, Campus Ciudad de México

Hybrid ensemble-variational data assimilation methods have been tested in several global and regional numerical weather prediction systems. Such methods usually employ a combination of climatological and ensemble-derived background error statistics in the variational algorithm. Most studies report a benefit from hybrid ensemble-variational data assimilation, attributing it broadly to the flow-dependency introduced by the ensemble-derived background error statistics. However, it is still unclear whether the overall benefit of flow-dependency originates from (i) the time-appropriateness of the background error statistics, (ii) the flow-consistency of the univariate autocorrelations, and/or (iii) the flow-consistency of the multivariate cross-correlations. For the tropics, factor (iii) may be particularly important as the typical climatological background error covariance model (often using geostrophic and hydrostatic balances) becomes less relevant. In this study, we use a simplified fluid dynamics model within a tropical framework to disentangle the benefits of the ensemble for ensemble-variational data assimilation. We compare pure ensemble-variational methods with traditional variational methods to distinguish the relative importance of using time-appropriate training data, and using an ensemble background error covariance model via the alpha control variable transform. We also test the impact of new univariate and multivariate localisation approaches (e.g. variable-dependent spatial localisation and selective multi-variate localisation) to optimise the ensemble background error covariance model. These results may highlight key focus areas to further improve data assimilation in the tropics.


AS15-A017
Combining Data Assimilation and Data-driven Sparse Sensing Placement Method for Designing Better Observation Locations

Shunji KOTSUKI#+, Takumi SAITO, Mao OUYANG, Daiya SHIOJIRI
Chiba University

Data assimilation (DA) plays an important role in numerical weather prediction (NWP) to provide optimal initial conditions by combining forecasted state and observation data. For accurately estimating initial conditions over the ocean, the effective use of mobile radiosonde observations by aircraft and ships would be useful. However, there have been few studies yet that try to optimize the placement of mobile observations for NWP. This study aims at designing better observation networks using the data-driven sparse sensor placement (SSP) method explored in informatics science. This method determines the optimal sensor locations so that the selected sensors effectively determine coefficients of proper orthogonal decomposition (POD) modes. The original SSP method reconstructs the spatial patterns of data from the selected sensors by solving a linear inverse problem using the POD modes. This study combined the SSP and DA so that we can accurately estimate the spatial patterns owing to Tikhonov regularization. We applied the combined approach to two problems: statics and mobile observations. Firstly, the proposed method was applied for the placements of rain-gauge observations over Hokkaido Island in Japan. The optimized rain-gauge locations by the SSP reconstruct more accurate spatial patterns of precipitation than the fields reconstructed by operational stations known as AMeDAS. The second problem aims to optimize the locations of additional mobile stations for NWP. We implemented the SSP into an intermediate global atmospheric model coupled with the local ensemble Kalman filter (a.k.a. SPEEDY-LETKF) to optimize observing placement over the ocean. Our preliminary experiment was promising, showing that the SSP-based placement provides more accurate analyses than an ensemble spread-based placement.


AS15-A010
Non-gaussian Based Kalman Filters

Steven FLETCHER1#+, Senne VAN LOON2
1Colorado, 2Colorado State University

With the advancement of non-Gaussian based variational techniques the need to extend this to hybrid ensemble-variational techniques is the next step towards operational viability. However, there is a problem with the Gaussian assumptions that are made in the derivation of the Kalman filter. In this presentation we shall present a new approach that enables the Kalman filter theory to be applied with: a lognormal, a reverse-lognormal, a Gaussian-lognormal, and a Gaussian-reverse-lognormal distribution. All of there filters are then applied to the Lorenz 1963 model where the z component is known to be have non-Gaussian based errors. All of the filters are compared these against the Extended Kalman Filter to assess improvement over a Gaussian-fits-all approach.


AS15-A011
Nongaussian Ensemble Data Assimilation

Senne VAN LOON1#+, Steven FLETCHER2, Milija ZUPANSKI1
1Colorado State University, 2Colorado

Most standard data assimilation methods are based on the assumption that the background and observational errors are drawn from a gaussian distribution. However, this is rarely the case. To improve the forecasting skill, one can replace the gaussian assumption by allowing some errors to follow lognormal and reverse lognormal distributions. This idea has already been successfully applied to variational data assimilation [1,2], and allowed for the development of a lognormal Kalman filter [3]. We can then extend these concepts to ensemble methods, based on the maximum likelihood ensemble filter [4].
We compare the ensemble data assimilation schemes with mixed gaussian, lognormal, and reverse lognormal distributions to the standard gaussian assumption. Moreover, we allow the underlying error distribution at each assimilation time to change dynamically, and present a machine learning technique that can decide on the optimal distribution to use within the Lorenz-63 model [5].
[1] Steven J. Fletcher, and Milija Zupanski (2006). "A hybrid multivariate normal and lognormal distribution for data assimilation." Atmospheric Science Letters 7(2), 43-46.
[2] Steven J. Fletcher (2010). "Mixed Gaussian-lognormal four-dimensional data assimilation." Tellus A: Dynamic Meteorology and Oceanography 62(3), 266-287.
[3] Steven J. Fletcher, Milija Zupanski, Michael R. Goodliff, Anton J. Kliewer, Andrew S. Jones, John M. Forsythe, Ting-Chi Wu, Md Jakir Hossen, and Senne Van Loon (2023). "Lognormal and Mixed Gaussian-Lognormal Kalman Filters." Monthly Weather Review.
[4] Milija Zupanski (2005). "Maximum likelihood ensemble filter: Theoretical aspects." Monthly Weather Review, 133(6), 1710-1726.
[5] Michael R. Goodliff, Steven Fletcher, Anton Kliewer, John Forsythe, and Andrew Jones (2020). "Detection of Non‐Gaussian Behavior Using Machine Learning Techniques: A Case Study on the Lorenz 63 Model." Journal of Geophysical Research: Atmospheres 125(2), e2019JD031551.


AS15-A002
Some Computational Issues in Machine Learning for Partial State Estimation

Wei KANG1#+, Liang XU2
1Naval Postgraduate School, 2Naval Research Laboratory

The estimation of atmospheric and oceanography dynamics involves both online and offline computation. In data assimilation, such as 4D-Var and EnKF, a large portion of the online computation in each cycle is used to propagate the numerical model multiple times along trajectories. Such algorithms demand high computational capacity. In this project, we explore innovative machine learning methods for data assimilation and forecasting to reduce online computational burden by transferring computationally intensive tasks offline. In machine learning, generating data and training neural networks involve offline computation only. After a neural network is trained, the main task of online computation is to evaluate a network of neurons, which is computationally cheap and efficient. We apply machine learning to partial state estimation, i.e., estimating the state variables inside a local region using local observational information. The first question is how much data is adequate for neural networks to provide an accurate estimation. The study reveals that an error upper bound can be computed based on constrained optimization theory. The effectiveness of machine learning for partial state estimation is demonstrated using examples of Burger’s equation and shallow water equations. It is shown that neural networks can facilitate a reasonable estimate of state variables in a given region using local observations. The neural network input is the observational data, and the output is the estimation. The online computational load is low because the neural network does not require propagating trajectories of the system model. An interesting fact revealed in the examples is that the neural network trained using zero boundary conditions can be successfully applied to data sets generated using different boundary conditions. This property is significant because it implies a good generalizability of the neural network.


AS15-A018
A Hybrid Ensemble Biogeochemical Data Assimilation System for the Red Sea: Development, Implementation and Evaluation

Mohamad EL GHARAMTI1, Siva Reddy SANIKOMMU2#+, Yixin WANG2, Matthew MAZLOFF3, Ariane VERDY4, Georgios KROKOS2, Rui SUN3, Aneesh SUBRAMANIAN5, Benjamin K. JOHNSON6, Angela Kuhn CORDOVA6, Bruce CORNUELLE3, Ibrahim HOTEIT2
1National Center for Atmospheric Research, 2King Abdullah University of Science and Technology, 3University of California San Diego, 4Scripps institution of Oceanography, 5University of Colorado Boulder, 6Scripps Institution of Oceanography

A Hybrid ensemble system is implemented for data assimilation (DA) into coupled physical-biogeochemical ocean model of the Red Sea. The system comprises 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 4km 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. Two different assimilation experimental settings are tested: (1) Weakly coupled DA in which the physical and biological observations only update their respective states, and (2) Strongly coupled DA in which both the physical and biological observations are used to update both physical and biological states. Sensitivity experiments are conducted to assess the relative impact of assimilating physical and biological observations. The state estimates are evaluated against independent in situ Glider observations of temperature, salinity, chlorophyll, and oxygen. The results indicate that the strongly coupled DA generally performs better than the weakly coupled DA. The improvements are significant, particularly in the subsurface layers. We further conducted identical twin experiments using strongly coupled DA with and without assimilating satellite chlorophyll observations to confirm the positive impact of assimilating chlorophyll observations on the estimation of biogeochemical fields.


Thu-03 Aug | 8:15 - 10:00 | MR323
AS35 - Aerosols, Clouds, Radiation, Precipitation, and Their Interactions

Session Chair(s):

AS35-A002
Evaluation and Attribution of Shortwave Feedbacks to ENSO in CMIP6 Models

Huang JUNJIE1+, Lijuan LI2#, Ran HAIYAN2, Liu JUAN3, Bin WANG2, Feng TAO4, Youli CHANG4
1IAP, Chinese Academy of Sciences, 2Chinese Academy of Sciences, 3Beijing Institute of Applied Meteorology, 4Yunnan University

The shortwave (SW) feedback to El Niño–Southern Oscillation (ENSO) is one of the largest biases in climate models, as the feedback includes atmosphere–ocean interactions and cloud processes. In this study, the performance of SW feedback in 19 models from the 6th Coupled Model Intercomparison Project (CMIP6) is evaluated and the biases are attributed using the historical and Atmospheric Model Intercomparison Project (AMIP) runs. The results demonstrate that while superior to CMIP5 counterparts, most CMIP6 models still underestimate the strength of SW feedback. The underestimates of SW feedback arise mainly from the biased feedbacks to El Niño in the four models with relatively better skills, while from both underestimated negative feedbacks to El Niño and overestimated positive feedbacks to La Niña in other models, which reproduce better seasonal variations than corresponding CMIP5 models. Furthermore, the SW feedback bias is connected to weak convective/stratiform rainfall feedback, which is sensitive/insensitive to sea surface temperature (SST) biases during El Niño/La Niña. The total rainfall feedbacks and dynamical feedbacks are underestimated in the historical runs, deteriorating relative to those CMIP5 ones, and the causes and relationships between feedbacks and mean states are investigated.


AS35-A026
A Climatology of Mid-latitude Cloud Fraction and Radiative Effect Over the Land and Ocean

Xiquan DONG1#+, Baike XI2, Xiaojian ZHENG1, Shaocheng XIE3
1University of Arizona, 2The University of Arizona, 3Lawrence Livermore National Laboratory

More than four years of ground-based measurements taken at the ARM Eastern North Atlantic (ENA) site between July 2015 and September 2019 have been collected and processed in this study. Monthly and hourly means of clear-sky, all-sky, total cloud fraction (CFT), and single-layered low (CFL) and high (CFH) clouds, the impacts of all scene types on the surface radiation budget (SRB), and their cloud radiative effects (CREs) have been examined. The annual averages of CFT, CFL, and CFH are 0.785, 0.342, and 0.123, respectively. The annual averages of the SW (LW) CREs for all sky, total, low, and high clouds are 256.7 (37.7), 276.6 (48.5), 273.7 (51.4), and 226.8 (13.9) W m-2, respectively, resulting in the NET CREs of 219.0, 228.0, 222.2, and 212.9 W m-2 W m-2. Comparing the cloud properties and CREs at both ARM ENA and Southern Great Plains (SGP) sites, we found that the clear-sky downwelling SW and LW fluxes at the two sites are similar to each other due to their similar atmospheric background. With different low cloud microphysical properties and cloud condensation nuclei at the two sites, much higher cloud optical depth at SGP plays an important role in determining its lower SW flux, while Tb and PWV are important for downwelling LW flux at the surface. A sensitivity study has shown that the all-sky SW CREs at SGP are more sensitive to CFT (21.07 W m22 %-1 ) than at ENA (20.689 W m22 %-1), with the same conclusion for all-sky LW CREs (0.735 W m22 %-1 at SGP vs 0.318 W m22 %-1 at ENA). The results over the two sites shed new light on the impacts of clouds on the midlatitude surface radiation budgets, over both ocean and land.


AS35-A030
Evaluation of Cloudy-sky Radiative Flux Datasets Derived from MODIS Aqua and MODIS-VIIRS Cloud Products Against Satellite- and Ground-based Clouds and Radiation Observations

Colten PETERSON#+, Kerry MEYER, Steven PLATNICK
NASA Goddard Space Flight Center

Clouds are a critical component of the global radiation budget, and cloud radiative effects at the top-of atmosphere (TOA) and surface can significantly depend on the optical properties of the cloud. Passive spaceborne imagers can be used to simultaneously retrieve cloud optical properties and directly observe SW and LW radiation at the top-of-the-atmosphere. However, radiative fluxes calculated directly from satellite-retrieved cloud properties can provide insight into the radiative implications of the retrieved cloud properties. Furthermore, such flux calculations can provide surface fluxes on a global scale. Given that there are limited direct measurements of surface radiative fluxes globally, especially in remote regions like the Arctic, surface radiative fluxes derived from passive spaceborne imagers can play a critical role in understanding the global surface radiation budget. Newly developed pixel-level SW and LW surface and TOA radiative flux datasets calculated directly from two MODIS/VIIRS Science Team cloud products, the MOD06 and MYD06 standard cloud products for Terra and Aqua, respectively (collectively referred to as MOD06) and the MODIS/VIIRS CLDPROP product for cloud climate data record continuity, are intercompared and evaluated globally against collocated ground- and satellite-based (i.e., CERES) radiation measurements. Future work and evaluation plans will be discussed, as well as efforts to understand the extent to which errors in MODIS/VIIRS-retrieved cloud optical properties (e.g., phase, cloud ice water path, cloud liquid water path) lead to radiation biases at the TOA and surface.


AS35-A013
Radiative Forcing Bias Calculation Based on Core-shell Mie Model Optimization of AERONET Data

Pravash TIWARI1+, Jason COHEN1#, Xinying WANG2, Shuo WANG3
1China University of Mining and Technology, 2Sun Yat-sen University, 3Chengdu University of Information Technology

Aerosol concentration, mass, size, shape, and mixing state contribute to direct radiative forcing (DRF), which has been identified as one of the major remaining uncertainties in constraining climate change. Absorbing aerosols (AA) simultaneously cool the surface and heat the atmosphere spatially and temporally in a very heterogenous manner, with local DRF as much as 100 times CO2. Current models consistently underestimate AA loading in the ultraviolet and visible wavebands. For these reasons, this work introduces a new approach to quantify the mixing state and size of AA using AERONET observations in two rapidly changing parts of the world: Lumbini and Taihu, in connection with an inversely applied Core-Shell Mie model. The constrained AA size, mixing state, and optical properties, are used to compute DRF changes at the top of the atmosphere (TOA) and the atmosphere itself (ATM).We obtain four conclusions. First, DRF covers a broader range than AERONET, ranging from [0.1,212]W/m2 in Lumbini and [0.4,158]W/m2 in Taihu. Second, ATM is less negative than AERONET, while at the same time the TOA is has a wider spread, from [-95.2,37.1]W/m2 in Lumbini and [-146,5.0]W/m2 in Taihu. Results demonstrate less cooling than AERONET overall, while in some cases even displaying a net positive TOA. Third, TOA and ATM are analyzed for different sizes of BC and demonstrate that DRF is not strongly dependent on AOD, especially so under large BC size, in which up to 1.9% of solutions have TOA>0. Fourth, TOA shows a multi-modal solution space in the fine mode which is not lognormally distributed, leading to the solution space for DRF that is not a linear function of AOD, as current models assume. This results demonstrate current methods may lead to biases and offers a new way to quantify non-linearities in DRF.


AS35-A006
Cloud Vertical Overlap for Radiation Processes in the Korean Integrated Model

So-Young KIM#+
Korea Institute of Atmospheric Prediction Systems

For cloud vertical structure in radiation processes in the Korean Integrated Model (KIM), maximum-random vertical overlap of clouds has been assumed. To improve the cloud-radiation interaction considering environmental conditions, exponential-random (generalized) cloud vertical overlap assumption is applied in KIM. Then, calculation of the cloud decorrelation length, which is used to determine the cloud overlap parameter and commonly assumed to be constant, is modified to include a dependence on latitude and the vertical shear of horizontal wind, based on previous observational studies. Impact of cloud vertical overlap is examined in seasonal simulations during boreal summer and winter. Cloud radiative forcing increases overall by using the exponential-random overlap assumption of clouds. Cloud radiative forcing enhances more, especially in the mid-to-high latitudes, by introducing the latitudinal dependency representing more maximal vertical cloud overlap in the lower latitudes. This alleviates underestimation of cloud radiative forcing and resultant warm bias in KIM, especially over land in the summer hemisphere. In the winter hemisphere, modified cloud vertical overlap results in warming near the surface by changing longwave cloud forcing. In the tropical region, interaction between radiative and convective processes plays an important role in changing the distribution of the cloud radiative forcing.


AS35-A001
Quantifying Particle-to-particle Heterogeneity in Aerosol Hygroscopicity

Liang YUAN1+, Chunsheng ZHAO2#
1Chengdu University of Information Technology, 2Peking University

The particle-to-particle heterogeneity in aerosol hygroscopicity is crucial for understanding aerosol climatic and environmental effects. The hygroscopic parameter κ, widely applied to describe aerosol hygroscopicity for aerosol populations both in models and observations, is a probability distribution highly related to aerosol heterogeneity due to the complex sources and aging processes. However, the heterogeneity in aerosol hygroscopicity is not represented in observations and model simulations, leading to challenges in accurately estimating aerosol climatic and environmental effects. Here, we propose an algorithm for quantifying particle-to-particle heterogeneity in aerosol hygroscopicity, based on information-theoretic entropy measures, by using the data that comes only from the in-situ measurement of the hygroscopicity tandem differential mobility analyzer (H-TDMA). Aerosol populations in this algorithm are assumed to be simple binary systems consisting of the less hygroscopic and more hygroscopic components, which are commonly used in H-TDMA measurement. Three indices, including the average per-particle species diversity Dα, the bulk population species diversity Dγ, and their affine ratio χ, are calculated from the probability distribution of κ to describe aerosol heterogeneity. This algorithm can efficiently characterize the evolution of aerosol heterogeneity with time in the real atmosphere. Our results show that the heterogeneity varies much with aerosol particle size and large discrepancies exist in the width and peak value of particle number size distribution (PNSD) with varied heterogeneity after hygroscopic growth, especially for conditions with high relative humidity. This reveals a vital role of the heterogeneity in ambient PNSD and significant uncertainties in calculating the climate-relevant properties if the population-averaged hygroscopicity is applied by neglecting its heterogeneity. This work points the way toward a better understanding of the role of hygroscopicity in evaluating aerosol climatic and environmental impacts.


AS35-A027
Vertical Profiles of Cloud Condensation Nuclei Number Concentration and its Empirical Estimate from Aerosol Optical Properties Over the North China Plain

Yuying WANG1#+, Rui ZHANG1, Zhaniqng LI2
1Nanjing University of Information Science & Technology, 2University of Maryland

To better understand the characteristics of aerosol activation ability and optical properties, a comprehensive airborne campaign was conducted over the North China Plain (NCP) from May 8 to June 11, 2016. Vertical profiles of cloud condensation nuclei (CCN) number concentration (NCCN) and aerosol optical properties were measured simultaneously. Seventy-two-hour air mass back trajectories show that during the campaign the measurement region was mainly influenced by air masses from the northwest and southeast. Air mass sources, temperature structure, anthropogenic emissions, and terrain distribution are factors influencing NCCN profiles. CCN spectra suggest that the ability of aerosol to activate into CCN is stronger in southeasterly air masses than in northwesterly air masses and stronger in the free atmosphere than near the surface. Vertical distributions of aerosol scattering Ångström exponent (SAE) indicate that aerosols near the surface mainly originate from primary emissions consisting of more fine particles. The long-distance transport increases SAE and makes it vary more in the free troposphere than near the surface. To parameterize NCCN, the equation NCCN=10βσγ is used to fit the relationship between NCCN and the aerosol scattering coefficient (σ) at 450 nm. The fitting parameters β and γ have linear relationships with the SAE. Empirical estimates of NCCN at 0.7% water vapor supersaturation (SS) from aerosol optical properties are thus retrieved for the two air masses: NCCN=10-0.22*SAE+2.39σ0.30*SAE+0.29 for northwesterly air masses and NCCN=10-0.07*SAE+2.29σ0.14*SAE+0.28 for southeasterly air masses. The estimated NCCN at 0.7% SS agrees with that measured, although the performance differs between low and high concentrations in the two air masses. The results highlight the important impact of aerosol sources on the empirical estimate of NCCN from aerosol optical properties.


Thu-03 Aug | 8:15 - 10:00 | MR327
AS38 - Ensemble Modeling and Prediction of High-impact, Multi-scale Weather to Decadal Events

Session Chair(s): Huiling YUAN, Nanjing University

AS38-A002
Research on the Influence of Uncertainty from Background Field and Lateral Boundary Conditions and Improvement of Large-scale Perturbation in Convection-permitting Ensemble Prediction System

Hanbin ZHANG#+
Institute of Urban Meteorology,China Meteorological Administration

Large-scale uncertainty in convective scale numerical prediction mainly comes from the background condition(BC) and lateral boundary conditions(LBCs). The BC and LBCs perturbation can significantly affect the overall perturbation amplitude of convection permitting ensemble prediction system (CPEPS). In this study, the Ensemble Sensitivity Analysis (ESA) is carried out based on the key factors affecting the uncertainty of large-scale prediction, therefore to explore the influence of BC uncertainty and LBC uncertainty in regional high-resolution model on disaster weather forecast, the spatiotemporal evolution characteristics of BC perturbation and LBCs perturbation are analyzed, with a reconstruction scheme of BC and LBCs perturbation designed to improve the quality of large-scale perturbation in CPEPS. Results indicate that the time effect of BC perturbation is short, and the LBCs perturbation mainly acts on the long time range of prediction; Reconstruct the BC and LBCs of each member of the CPEPS using the high-quality ECMWF deterministic forecast field combined with the NCEPS-GEFS global ensemble forecast perturbation field to form the BC and LBC adjustment scheme, namely EC-center, can improve the quality of large-scale information in the CPEPS.


AS38-A021
High-resolution Forecasting of Warm Season Rainstorms in Shanghai Using WRF: Role of Convection Representation Across the Gray Zone

Fengxue QIAO1#+, Rui WANG2, Xinzhong LIANG3, Yiting ZHU4
1East China Normal University, 2Shanghai Central Meteorological Observatory, 3University of Maryland, 4Fudan University

The representation of convection has always been a major source of model biases. Particularly in the “gray zone” with horizontal grid spacing between 1-10 km, the convection treatment remains an open question in high-resolution modeling community. There is still no consensus on whether to use parameterized or explicit convection for regional climate simulations between 5-10 km, and systematic biases are identified in convection-permitting predictions at 3-5 km. Multi-grid nesting simulations downscaled to 1-km grid with typical ratio of approximately 1:3 have been widely conducted, but their predictive skills are highly affected by the convection treatment in the outer two grids (3 km and 9 km), which reside in the gray zone and have large uncertainty. This study investigates the role of convection treatment across the gray zone and explores the feasibility of avoiding the gray zone in the multigrid nesting simulations for the innermost 1-km grid. Triple nesting (15-5-1 km, 9-3-1 km) experiments are compared to double nesting (15-1 km, 9-1 km) with the intermediate grids removed, considering different convection treatments in the outermost grids. Two heavy rainfall events occurred in warm season over Shanghai involving complex multiscale interactions are selected. Main results show that nesting a midsize domain within the gray zone (5 km and 3 km) may degrade the innermost 1-km forecast, and double nestings with larger ratio (such as 15 or 9) are more effective for extreme rainfall forecasting. Especially the double nesting using the Kain-Fritsch scheme in the outermost grids outperform that using other convection treatments and the traditional triple nesting. The predictive skills of this double nesting with larger grid ratios can be further improved by examining the effect of Planetary boundary layer, and using the MYNN scheme most realistically reproduces the rainfall distribution and hourly variation of extreme rainfall intensity.


AS38-A001
Atlantic-forced Pacific Decadal Prediction: Observations and Model Simulations

Jun-Chao YANG#, Zhen LV+, Yu ZHANG, Xiaopei LIN
Ocean University of China

Recent studies showed that the Atlantic Multidecadal Oscillation (AMO) exhibits strong modulations on Pacific decadal variability, but its effect on Pacific decadal prediction remains unclear. Here, we use linear inverse model (LIM) to assess this trans-basin effect based on observations and climate models. LIM is a useful tool for decadal prediction which shows comparable prediction skills to model ensemble hindcast.
In observations, AMO effect is isolated by using North Atlantic pacemaker experiments. AMO effect substantially modulates decadal prediction skills in the North Pacific, especially in its western and central parts. The reason is because the AMO modulates both global mean surface temperature and the Pacific Decadal Oscillation. In climate models, the commonly underestimated AMO strength significantly lower pan-Pacific decadal prediction skills, especially in the North Pacific. Our study highlights the necessity to improve model simulation on AMO trans-basin effect to gain better Pacific decadal prediction.


AS38-A022
Testing the IMPROVER Post-processing Suite in Singapore

Robert HUVA1#+, Boon Chong Peter HENG2, Jeff LO1, Hugh ZHANG3
1Centre for Climate Research Singapore, 2Meteorological Service Singapore, 3CCRS

The IMPROVER (Integrate Model post-PROcessing and VERification) suite developed by the Met Office, UK, and with contribution from the Bureau, Australia, is an open-source toolbox for post-processing NWP output. The IMPROVER suite has several functions (including neighbourhooding, calibration and multi-model blending) that allow the user to increase forecast skill and provide probabilistic information around events. In Singapore we experience rapidly developing convection and the uncertainty in our forecasts can be quite high as a result. Our region is therefore ideally suited to probabilistic output and implementation of the IMPROVER suite is a key focus for Meteorological Service Singapore. In this talk I will outline some initial testing of the IMPROVER suite that utilises our inhouse NWP (SINGV deterministic and ensemble) and ECMWF (deterministic and ensemble) model output. Over a 2.5 month period in 2022 a comparison between output from various stages of the IMPROVER suite with the raw model will be conducted to outline the impact of each step in the post-processing chain. The focus of this work will be on rainfall at various hourly accumulation thresholds as this is a key variable of concern for our region.


Thu-03 Aug | 8:15 - 10:00 | MR328
AS10 - Extreme Events: Observations and Modeling

Session Chair(s): Sridhara NAYAK, Japan Meteorological Corporation, Mohan Kumar DAS, National Oceanographic and Maritime Institute (NOAMI), Shiori SUGIMOTO, Japan Agency for Marine-Earth Science and Technology

AS10-A020
Future Changes in Synoptic-scale Conditions Inducing Wide-spread Heavy Precipitation in Japan

Shiori SUGIMOTO1#+, Rui ITO1,2, Chieko SUZUKI1, Sachiho ADACHI3
1Japan Agency for Marine-Earth Science and Technology, 2Meteorological Research Institute, 3RIKEN Center for Computational Science

Widely spreading extreme precipitation events have been observed in Japan associated with disturbance passage and/or stationary front, which can cause severe landslide and flooding over various regions. To understand future characteristic change in such kind of precipitation events, annual maximum of daily and 5-days accumulated precipitation averaged over land in Japan are compared between current and future climate conditions. Dynamical downscaling with 5-km horizontal resolution was conducted using the nonhydrostatic regional climate model (NHRCM; Sasaki et al. 2008) based on the Database for Policy Decision-Making for Future Climate Change (d4PDF; Mizuta et al. 2017, Fujita et al. 2018). We use 720-years ensembles both for historical climate condition and 4K warming condition relative to the preindustrial level, respectively. Daily and 5-days accumulated precipitation were calculated over each grid and were averaged over land in Japan. Then, their annual maximums are detected as Rx1d and Rx5d in each year. Note that one year is defined as from September 1 of a year to August 31 of next year. Increases in Rx1d and Rx5d were shown in almost all regions of Japan under the warmer climate condition. Cluster analysis was performed to examine the spatial pattern of precipitation when Rx1d and Rx5d was simulated. Approximately 90 % of Rx1d and Rx5d occurred from disturbance passage such as typhoons in the historical climate, and a remaining 10% was from stationary front, i.e., Baiu. In the 4K warming climate, the ratio of Rx1d and Rx5d caused by stationary front increased to approximately 20% atmospheric moistening in spite of frequency covered by rainband associated with stationary front decreased over Japan. The increase in Rx1d (Rx5d) was significant in April and May (July); then, future changes in seasonality of atmospheric conditions when Rx1d and Rx5d occurred will also be investigated in more detail.


AS10-A006
Recurring Latitudinal Shifts of the 2020 Extreme Meiyu Rainfall Around Yangtse: Potential Role of MJO

Yuntao WEI1#+, Hong-Li REN2,3, Yuwen WANG1
1Fudan University, 2Chinese Academy of Meteorological Sciences, 3China University of Geosciences

Considering the unprecedented extremity of the Meiyu episodes in early summer of 2020, here the authors perform a comprehensive study of the intraseasonal evolution characteristics of the observed rainfall round Yangtse as well as the potential modulating effect of Madden-Julian Oscillation (MJO). Results suggest that the Meiyu rainfall manifests as recurring latitudinal shifts around Yangtse during June–July of 2020, corresponding well to the continued swings of MJO circulation and convection between Phase 1 and Phase 2. The MJO affects the meridional migration of the 2020 Meiyu rainfall mainly through regulating the westward extended ridge line and southwesterly of the anomalous anticyclone over the western North Pacific (WNP). Specifically, the northeastward propagation of boreal summer MJO from Phase 1 to 2 shifts the ridge line of the anomalous WNP anticyclone northeastward. Consequently, the associated southwesterly anomaly over the southeastern China penetrates to the north of Yangtse and enhances the lower-tropospheric moisture flux convergence, supporting heavy precipitation there. However, when the MJO swings back to Phase 1, the anomalous southwesterly and moisture flux convergence retreat southward, so does the Meiyu rain band. The present results advanced our understanding of the interactions between the latitudinal shifts of extreme Meiyu rainfall episodes and MJO Phase swings.


AS10-A024
The Effect of Initial and Boundary Conditions on Heavy Rainfall Forecast Over the Yellow Sea: Verification Using Dropsonde Measurements

Jiwon HWANG+, Dong-Hyun CHA#
Ulsan National Institute of Science and Technology

This study aimed to investigate the impact of initial and boundary conditions on heavy rainfall forecast over the Yellow Sea and Korean Peninsula using the Weather Research and Forecasting (WRF) model initialized with two operational global model analyses from NCEP and ECWMF. Before employing the two analysis fields as initial and lateral boundary conditions for the WRF model, they were compared to dropsonde data. When comparing temperature and humidity, it was found that, the NCEP analysis showed overall lower and drier conditions compared to the ECMWF analysis. This difference was particularly robust in the lower atmosphere, below 850 hPa. Through numerical experiments, it was found that the performance of the heavy rainfall forecast over the Yellow Sea was better when using ECMWF analysis data as the initial and lateral boundary conditions. Based on these findings, it is proposed that the use of accurate analysis data will attribute to a more accurate simulation of unstable and rapidly developing convection systems. These results indicate that the quality of the initial field can play a critical role in the performance of numerical weather forecasting models.


AS10-A004
Moisture Sources of the Record-breaking Heavy Rainfalls Over Tohoku Region in August 2022

Ning ZHAO1#+, Pei-Ming WU1, Atsuyoshi MANDA2, Xiaojun GUO3, Bin WANG4
1Japan Agency for Marine-Earth Science and Technology, 2Mie University, 3University of Hawaiʻi at Mānoa, 4Jiangsu University of Science and Technology

Tohoku region (Aomori-ken, Akita-ken, and Iwate-ken) suffered record-breaking heavy rainfalls in early August 2022. Based on observations, three major events occurred on August 3rd, 8th~9th, and 11th. According to the early reports from the JMA, the major forcing of these events was the stationary front, and there were large amount of moisture transported from the East China Sea (ECS). However, it remains unclear whether the relatively small ECS could supply enough moisture for the continuous heavy rainfalls. On the other hand, unlike the summer Meiyu-Baiu front, this stationary front located at higher latitude, and therefore could unlikely be affected by the regular moisture-rich regions reported in previous studies, such as the Kuroshio and the subtropical western Pacific (WP) due to the blocking of the Japanese Archipelago. Thus, this study was motivated to identify and evaluate the moisture contributions and transport routes during the heavy rainfalls over Tohoku region. In this study, moisture sources and transport routes were based on the Lagrangian air parcels that were backward traced 3 days. According to our results, moisture of the first event was transported mainly from the southern part of the Sea of Japan (JS) and the subtropical WP region south of Japan carried by the TS/Trases and the following migratory anticyclone. In the second event, the stationary front created a relatively stable moisture transport route which allowed moisture from the ECS and the southeast China mainland entering the JS. During the last event on August 11th, due to the approaching tropical storm, the stationary front was disturbed and so was the moisture transport route from the ECS. As the front moved southward, moisture from the Kuroshio region and the oceans south of Japan was allowed to be transported across the Japanese Archipelago.


AS10-A021
Climate Change Impact on Precipitation and Temperature Extremes Over Japan

Sridhara NAYAK1#+, Tetsuya TAKEMI2
1Japan Meteorological Corporation, 2Kyoto University

This study investigates the climate change pattern and their impact on the extreme events over Japanese regions from 140 ensemble climate simulation results conducted over Japan for the past 50 years (1961-2010) and the future 60 years (2051-2110). To do this, we specifically focused on the precipitation and temperature extremes (exceeding 30 mm/d and 25°C respectively and top 10% events) over Japan and their response to the climate change. We noticed slightly positive trends in the precipitation amounts and the frequencies and a significant positive trend in temperature over the entire Japan. The frequencies of precipitation intensities are also expected to increase over some regions of Japan. It is noticed that intensity of the precipitation extremes (averaged of top 10% precipitation days’ intensity) in the future climate is likely to increase by up to 5mm/d over northern Japan, 10mm/d over eastern Japan and 15mm/d over western and southern Japan. The temperature extremes (mean of top 10% hot days) are also expected to be much hotter in entire Japan.


Thu-03 Aug | 8:15 - 10:00 | MR329
AS05 - Cities, Extreme Weather, and Climate Change

Session Chair(s): Fei CHEN, National Center for Atmospheric Research

AS05-A023
Characteristics of WRF Coupled Urban Canopy Model Using Local Climate Zone-based Urban Classifications

Cheng-Pei YANG1+, Fang-Yi CHENG1#, Yu-Cheng CHEN2, Tzu-Ping LIN3
1National Central University, 2Nanhua University, 3National Cheng Kung University

Many studies have used different urban canopy models(UCM) and land use classifications to improve the descriptions of urban in meteorological models. World Urban Database and Access Portal Tools (WUDAPT) provides seventeen land use types based on the Local Climate Zone (LCZ) classifications for properties of surface structures. The Weather Research Forecasting (WRF) coupled with Building Energy Parameterization (BEP) and Building Energy Model (BEM) was applied to explore the characteristics of UCM in Taiwan. In addition, WRF-UCM simulation with detailed 10-LCZ urban classifications was conducted to assess its impact on fine-scale meteorological simulation in urban areas. The WRF-BEP simulation shows lower temperatures in urban areas than the simulation without UCM during nighttime. Due to consideration of the percentage of previous regions and the existence of urban vegetation for urban grids in UCM, less surface heat fluxes were simulated. Further consideration of the anthropogenic heat release in WRF-BEP+BEM improves the nighttime simulations. UCM simulates lower wind speed due to the blocking effect of buildings and the increase in roughness, which effectively improves the overestimation of wind field without UCM. Incorporating the LCZ urban classifications into UCM, the main dense residential, commercial, and industrial areas in the northern metropolitan area show higher temperatures in the daytime. The compact high-rise buildings show higher temperatures at nighttime due to the higher density and height of buildings. With poor ventilation and a stronger blocking effect, the urban types with higher density and height of buildings simulate lower wind speeds. The comparisons between using three urban types and LCZ data show significant differences in the daytime. The areas with lower urban fractions are mostly consistent with lower surface temperatures simulated by using LCZ data. The different settings in urban parameters between the two urban data are factors resulting in lower temperatures simulated using LCZ.


AS05-A002
Effect of Green-blue Space on Urban Thermal Environment and Outdoor Comfort: A Field Study in Hong Kong

Xuan CHEN+, Han WANG, Jiachuan YANG#
The Hong Kong University of Science and Technology

A two-year field measurement focusing on the urban parks and seafront promenade parks during hot and humid periods in Hong Kong was conducted with handheld mobile devices. In total, we carried out 180 rounds of the measurements for 10 places, obtaining more than twenty-five thousand records. The effect of green-blue spaces on the urban thermal environment is evaluated based on collected data. Green-blue spaces are cooler than surrounding urban areas, especially during the nighttime period in Hong Kong. The air temperature among most of the green-blue spaces is below the quarter value of the surrounding environment in the evening on average. The mean nighttime WBGT is about 0.24 °C and 0.09 °C lower than nearby urban for all studied green and blue spaces. The cooling effect of green-blue spaces would be varied depending on background climates, synoptic conditions, and local landscapes. In the sub-tropical area, the daytime cooling process is highly related to the shading effect. And the humid environment constrains evaporation and evapotranspiration cooling. The nighttime cooling effect is mainly due to less outgoing longwave radiation and stronger air movement over the open spaces compared to building canyons. Citizens who do daily exercise in the promenade park should pay more attention to the heat stress. The findings not only provide comprehensive results of the cooling performance of green-blue space but also provide insights into heat mitigation in the sub-tropical area. The measurement data could further support future numerical studies for validation.


AS05-A004
Energy Changes During Urban Heatwaves and the Impact on Human Comfort

Yizhao WEI+, Han CHEN, Jeanne Jinhui HUANG#
Nankai University

Heatwaves have increased in intensity and frequency under enhanced global warming. The response of the energy change and human discomfort to heatwave is unclear. This study combines the discomfort index (DI) and the Excess Heat Factor (EHF) to estimate the Excess Discomfort Factor (EDF), which represents the level of human comfort during the heatwave. The daily energy balance components before and after the heatwave events in a mega city: Shenzhen, China was reconstructed using a modified urban four-source model (MFSU model) during the period 1980-2019. The effects of heatwaves on the energy change of different urban surface (soil, vegetation, impervious surface, and water body) were analyzed. The response of human comfort to energy changes during the heatwaves was revealed. The results suggest that it is not drought but suppression of plant stomatal conductance that causes the reduction of latent heat of vegetation during heatwaves in Shenzhen. With the rapid urbanization, the capacity of vegetation in regulating human comfort has been decreased during heatwaves. The change of energy before and after the heatwave in impervious surface best reflects the degree of human comfort during the heatwave. This study improves the understanding of energy changes in unban heatwaves and their relationship with human comfort.


AS05-A016
Human-perceived Urban Heat Islands (UHIs) in China: A Comparison with Surface and Canopy UHIs

Hui ZHANG+, Ming LUO#
Sun Yat-sen University

Heat stress that human beings actually perceive is not only related to air temperature, but also jointly influenced by other climatic factors such as humidity. In the current study, we propose to use human-perceived temperature (HPT) to measure human-perceived urban heat island (HUHI), which remains much less understood than surface urban heat island (SUHI) measured by land surface temperature (LST) and canopy urban heat island (CUHI) quantified by near-surface air temperature (SAT). In particular, we present a thorough investigation of the spatiotemporal variations of HUHI and the comparison among SUHI, CUHI, and HUHI respectively based on LST, SAT, and HiTIC-Monthly (A monthly high spatial resolution human thermal index collection) datasets with a spatial resolution of 1 km over China from 2003 to 2020. Temporally, the mean intensities of three UHIs across China exhibit significant increasing trends during 2003–2020, and the increasing trend of HUHI (0.09 °C/decade) is faster than CUHI (0.08 °C/decade) and slower than SUHI (0.13 °C/decade). Spatially, the intensity of HUHI is around 1 °C lower than SUHI in most cities of the southeastern humid region of China, northeast China and North China Plain, and ~1 °C higher than SUHI in the northwestern arid region of China. The spatial patterns to trends of the annually-averaged intensity of SUHI, CUHI, and HUHI are similar, with the faster increase in UHI intensity concentrated in rapidly urbanizing and populated areas such as the North China Plain. By probing into the characteristics of three different types of UHI, our study is of critical importance for assessing urban climate change, developing appropriate mitigation strategies and policies on mitigating the heat island effect, and reducing the risk to public health.


AS05-A017
Impact of Urbanization and Regional Effects of Climate Change on the Temperature Changes Over an Eastern Indian Tropical City: A Modeling Perspective

Nandini G#+, V. VINOJ
Indian Institute of Technology Bhubaneswar

Climate change due to enhanced greenhouse gas emissions has led to increased temperatures globally. Over urban areas, on top of the regional effects of climate change, there is additional warming due to urbanization. Since both the anthropogenic influences of enhanced emissions and urbanization lead to warming, it is often difficult to separate and quantify their impacts on the temperature changes observed in a city. Our study uses a regional climate model to simulate the wintertime surface temperatures over a tropical city and quantifies the effects of urbanization and regional effects of climate change in the observed warming over Bhubaneswar, one of the fastest-growing tier II cities in India. During the period 2004-2015, a rise of ~1.4°C was observed in air temperature. It was found that the effect of urbanization on temperature is dominant during the nighttime, with more than half of the warming attributed to local urbanization effects. Almost 60% of the observed increase in the nighttime temperature is due to local impacts, and the remaining 40% is due to regional effects. Such quantifications are essential for cities for proper urban planning and the design of mitigation techniques.


AS05-A012
Performance Evaluation of a Land-surface-physics-based Downscaling Approach for Urban Thermal Environment Prediction

Lingbo XUE1+, Quang-Van DOAN1#, Hiroyuki KUSAKA1, Cenlin HE2, Fei CHEN2
1University of Tsukuba, 2National Center for Atmospheric Research

Urban areas are expected to have more extreme weather events (heat waves etc.) in the future because of global climate change. To help policymakers better formulate policies to address urban climate change, a fine-resolution urban climate prediction is needed. Unfortunately, there is a big gap between the need for fine-resolution information and current climate prediction technology which requires too many computational resources and is not usually available anywhere. Therefore, we propose a downscaling approach based on the land surface modelling system (High Resolution Land Data Assimilation, HRLDAS), which can directly predict urban thermal environment from GCM outputs or reanalysis data instead of direct dynamical downscaling which uses regional climate models. The new downscaling approach is effective, standardized, easy to apply and requires fewer computational resources to deal with thermal environments. This is not limited to future climate prediction, it can also be used for city-scale weather forecasts in thermal environments. A case study of Tokyo is done to assess the land-surface-model-based downscaling approach, using ERA5 data. Here we present the primary results in comparison with in-situ observations. We also discuss the advantages and disadvantages of the approach to guide potential users in using this approach for urban climate downscaling.


AS05-A013
Fine-scale Climate Change Information to Assist Decision Making: The CORDEX SEA Urban Climate Initiative

Quang-Van DOAN1#+, Fredolin TANGANG2, Faye Abigail CRUZ3, Julie Mae DADO3, Liew JUNENG2, Jing Xiang CHUNG4, Phan VAN-TAN5, Thanh NGO-DUC6, Thanh NGUYEN-XUAN6, Dang-An TRAN7, Ngoc-Dang TRAN8, Jerasron SANTISIRISOMBOON9, Patama SINGHRUCK10, Jaruthat SANTISIRISOMBOON9, Edvin ALDRIAN11, Dodo GUNAWAN12, Donaldi PERMANA12, Srivatsan VIJAYARAGHAVAN13, Matthias ROTH13, Dung PHUNG14, John MCGREGOR15, Hiroyuki KUSAKA1, Masaru INATSU16, Tetsuya TAKEMI17, Lingbo XUE1, Anurag DIPANKAR18, Rafiq HAMDI19, Dev NIYOGI20, Cenlin HE21, Fei CHEN21
1University of Tsukuba, 2Universiti Kebangsaan Malaysia, 3Manila Observatory, 4Universiti Malaysia Terengganu, 5Vietnam National University, 6University of Science and Technology of Hanoi, 7Thuyloi University, 8Ho Chi Minh City Medicine and Pharmacy University, 9Ramkhamhaeng University, 10Chulalongkorn University, 11Agency for Assessment and Application of Technology, 12Indonesian Agency for Meteorology, Climatology and Geophysics, 13National University of Singapore, 14The University of Queensland, 15Commonwealth Scientific and Industrial Research Organisation, 16Hokkaido University, 17Kyoto University, 18ETH Zurich, 19Royal Meteorological Institute of Belgium, 20The University of Texas at Austin, 21National Center for Atmospheric Research

Global climate change presents a major threat to humanity, with variable impacts across regions leading to varying patterns in extreme weather and climate changes worldwide. Local geographical factors such as terrain and land cover characteristics play a significant role in local climate and diversifying its response to global change forcing. Southeast Asia, a region with a diverse array of geophysical, economic, and social conditions, is the home to thriving metropolises like Bangkok, Manila, Jakarta, Kuala Lumpur, Singapore, and Ho Chi Minh City. The region is also a major player in the production of rice crops, with Vietnam and Thailand among the top three rice-exporting countries in the world. However, human activities like industrialization, urbanization, and deforestation are modifying local climate conditions and leading to unprecedented and hazardous changes for those who live there. The Urban Climate Initiative is established within the CORDEX SEA (Coordinated Regional climate Downscaling experiment Southeast Asia). It is aimed at providing a framework for researchers (both inside and outside the region) to work together, sharing knowledge and know-how, promoting international (bilateral & multilateral) research cooperations, and building capacity in fine-resolution climate modeling with a focus on (but not limited to) land-air interactions, urban physics. As a part of the CORDEX SEA urban climate initiative, we introduce a recent research activity related to urban climate downscaling. We introduce the potential of applying a cutting-edge land surface modeling framework based on the High-Resolution Land Data Assimilation System (HRLDAS), developed at the National Center for Atmospheric Research (NCAR), to estimate the local thermal climate in Southeast Asia's megacities. Furthermore, we will discuss the advantages and disadvantages of the land-surface-physics-based downscaling approach by comparing it with existing methods, including statistical and direct dynamical downscaling. Also, the potential use of downscaling outcomes for further risk assessment is also presented. 


Thu-03 Aug | 8:15 - 10:00 | MR331
AS01 - The Asian Monsoon, Extremes and Climate Change

Session Chair(s): Suvarna FADNAVIS, Indian Institute of Tropical Meteorology, Pune, India, Anja KATZENBERGER, Potsdam Institute of Climate Impact Research, Kritanai TORSRI, Ministry of Higher Education, Science, Research and Innovation, Elena SUROVYATKINA, Potsdam Institute for Climate Impact Research

AS01-A036
The Contribution of Non-tropical Cyclone Vortices to the Rainfall and Rainfall Extremes During Summer and Winter Monsoon Seasons in the Philippines

Jun MATSUMOTO1,2#+, Lyndon Mark OLAGUERA3, John MANALO1,4
1Tokyo Metropolitan University, 2Japan Agency for Marine-Earth Science and Technology, 3Manila Observatory, 4Philippine Atmospheric Geophysical and Astronomical Services Administration

Weaker disturbances than tropical cyclones (TCs) such as tropical depressions and cold surges sometimes induce heavy rainfall and flooding events over the Philippines. However, these disturbances including their rainfall contributions during summer or winter monsoon season in the Philippines are not well documented in previous studies. To address this research gap, this study investigates the rainfall contribution of non-TC vortices over the Philippines during both monsoon seasons from 1979 to 2020.Only those rainfall-producing non-TC vortices that formed and appeared within a 500-km radius from the Philippine coastline were examined. A total of 7686 non-TC vortex days were identified. The mean rainfall contribution of these non-TC vortices was found to be highest over the northeastern Mindanao Island (80-90% of the mean daily rainfall) and lowest over the central and western regions of Luzon Island (50-60%). Seasonal analysis of the occurrence frequency of these vortices show that they are most frequent during the winter monsoon season from December to February (DJF) season. In this season, the rainfall contribution may increase to 50-80% of the mean daily rainfall over the whole country, while in the other seasons, the rainfall contribution may only increase to as much as 60%. Higher frequency of extreme rainfall days associated with these non-TC vortices were also found during the DJF season. The occurrence frequency and percentage rainfall contribution of these non-TC vortices in relation to the different phases of the Boreal Summer Intraseasonal Oscillation (BSISO) during boreal summer or the Madden Julian Oscillation (MJO) during boreal winter were also examined. Higher frequency and percentage rainfall contribution over the country were found during Phases 4 to 6 of both the BSISO and MJO, when their respective active convections transit from the Maritime Continent to the western North Pacific.


AS01-A028
Impacts of the East Asian Winter Monsoon on Precipitation Variability Over East Asia-western North Pacific

Renguang WU#+, Zhenzhen WANG
Zhejiang University

The boreal winter precipitation variability over East Asia and the western North Pacific is often attributed to the El Niño-Southern Oscillation (ENSO). The present study investigates the independent impacts of the East Asian winter monsoon (EAWM) on winter precipitation anomalies over East Asia and the western North Pacific. It is revealed that anomalous EAWM is accompanied by a south-north dipole pattern of precipitation anomalies in the above regions. During strong EAWM years, the enhanced northeasterly winds induce anomalous convergence and divergence over the tropical and subtropical regions, respectively, leading to anomalous ascent and above-normal precipitation over the southern South China Sea-Philippine Sea and anomalous descent and below-normal precipitation over eastern China-subtropical western North Pacific. Opposite convergence, vertical motion and precipitation anomalies are induced in the above regions during weak EAWM years. In the observations, both ENSO and EAWM contribute to the south-north dipole precipitation anomaly pattern with a larger contribution from ENSO and EAWM for the tropical and subtropical precipitation anomalies, respectively. Atmospheric model experiments with climatological annually varying sea surface temperature forcing confirm the independent role of the EAWM in the formation of the south-north dipole precipitation anomaly pattern. A moisture budget diagnosis shows that the dynamic effect associated with vertical motion is dominant in the formation of the above precipitation anomaly pattern in both the observations and model simulations. The horizontal moisture transport has an additional contribution to the formation of subtropical precipitation anomalies.


AS01-A082
On the Use of an Upper-level Vorticity for Trough Prediction Over Indochina Peninsula (IP) Sub-region with a Coupled WRF-ROMS Model

Kritanai TORSRI#+, Rati SAWANGWATTANAPHAIBUN , Apiwat FAIKRUA, Pattarapoom PEANGTA, Thippawan THODSAN, Kanoksri SARINNAPAKORN
Ministry of Higher Education, Science, Research and Innovation

During rainy season, displacement of monsoon trough plays an important role in controlling an environment favorable for extreme rainfall events in tropical region. Thailand is situated in the tropic and regularly exposed to severe flood events caused by trough-induced heavy rainfall. Knowing trough displacement days or weeks in advance can yield benefit for early disaster preparedness and warning. This study aimed at validating a coupled WRF-ROMS model in capturing the monsoon trough. Upper-level vorticity computed from hourly ERA-5 winds at 300-hPa was used for determining the trough. Four heavy rainfall events in Thailand associated with trough during May-August 2022 were selected, as the observed rain band was relatively consistent with an elongated upper-level vorticity for all events. It was therefore reasonable to use the 300-hPa vorticity as an indicative variable for model comparison. The model was forced by 3-hr GFS for WRF and initiated ocean states with HYCOM for ROMS, and afterward momentum and heat fluxes were concurrently exchanged between the models. Prognostic upper-level vorticity maps estimated from predicted winds were depicted. For basis of comparison, 6-hr average of the observation and prediction were plotted along with forecasted high- and low-pressure system at sea level (SLP), then a visual comparison was made. The model well captured trough displacement in May and June, which was located over northern Thailand and contributed to heavy rainfall (up to 150 mm/day). It also showed good agreement with observation in the following months, when trough moved more southward and caused heavy rainfall in northeast and eastern sub-regions. Therefore, this study is valuable in pointing out the potential of the predicted vorticity and SLP for trough prediction over IP sub-region and is fundamental to further validating the model for longer time scale, especially week-to-week change of the trough.


AS01-A021
Link Between the Land–sea Thermal Contrast and the Asian Summer Monsoon

Zhiyan ZUO#, Kaiwen ZHANG+
Fudan University

The land–sea thermal contrast is the foundation of the occurrences of the Asian summer monsoon (ASM). Using multiobservational datasets and model simulations covering the period 1960–2018, this study investigates the relationship that links the thermal contrast between the Asian landmass and the Indian Ocean (TCAI) to the ASM and evaluates the effects of the various driving factors that influence the TCAI in the climate models. The tropospheric TCAI is highly consistent with the ASM circulation, with a stronger ASM circulation and larger tropospheric TCAI before the 1970s and after the late 1990s than those seen from the 1970s to the late 1990s. The tropospheric TCAI is also closely related to rainfall over the Indian landmass and the south-flood–north-drought pattern over eastern China. Thus, the tropospheric TCAI reliably reflects the state of the ASM system and could be used as a new ASM index that directly describes the land–sea thermal contrast. The variation of the surface TCAI is highly consistent with that of the tropospheric TCAI. The model simulation suggests that the main drivers of the surface TCAI are anthropogenic forcing and the Atlantic multidecadal oscillation (AMO). Anthropogenic forcing dominates SAT variations over the Indian Ocean, whereas the AMO plays a major role in SAT variations over the Asian landmass, which introduces a large uncertainty into the projections of the ASM.


AS01-A065
Does the Indian Monsoon Have Subseasonal Features?

Lun DAI1#+, Bin WANG1, Mengqian LU2, Fandy Tat Fan CHENG2
1University of Hawaii, 2The Hong Kong University of Science and Technology

The Indian monsoon (IM) is one of the most energetic and influential components of the Earth’s climate systems on earth. Understanding its characteristics is critical for ensuring the prosperity and livelihoods of billions of people in South Asia. As a tropical monsoon system, it features a distinctive seasonal reversal of winds and a sharp contrast between wet summer and dry winter. Tremendous efforts have been made in analyzing the Indian summer monsoon. However, there is a limited understanding of the climatological subseasonal features. In this study, an unsupervised machine learning technique was utilized to objectively classify the 850-hPa wind fields. The results reveal six subseasonal stages in the IM annual cycle, each spanning from 23 to 90 days. The summer season includes three substages, the onset, peak, and withdrawal periods of southwest monsoon from mid-May to early October, receiving over 80% of annual land precipitation. More interestingly, three distinct stages are identified in the rest of the annual cycle, which are distinguishable by the Arabian Sea high pressure ridge and feature varied hydrological conditions. In line with these findings, we provide a comprehensive picture of stage-wise hydrological hazards, including the extreme temperatures, precipitation, and frequency of tropical cyclones. Furthermore, to aid in the operational monitoring of the IM annual cycle, we present the year-to-year variations of the critical start or end dates of each stage. It is cross-validated by comparing the available onset and withdrawal dates in the literature. This study offers a fresh perspective on the IM annual cycle and is beneficial for weather diagnosis and the optimization of weather regimes and water resources management on the subseasonal to seasonal time scale.


AS01-A042
Tropical Anomalies Associated with the Interannual Variability of the Cross-equatorial Flows Over the Maritime Continent in Boreal Summer

Xiaoxuan ZHAO1+, Riyu LU1#, Buwen DONG2, Xiaowei HONG1, Junqi LIU1, Jianqi SUN3
1Chinese Academy of Sciences, 2University of Reading, 3Nansen-Zhu International Research Centre

In this study, we investigate circulation, convection and sea surface temperature (SST) anomalies associated with interannual variability of the cross-equatorial flows over the Maritime Continent (MC) in boreal summer. Observational diagnostics show that strengthened CEF is associated with large-scale circulation anomalies featured by upper-level northeasterly anomalies across MC, weakened Walker circulation and lower-level cyclonic anomalies over the tropical Western North Pacific (WNP). Correspondingly, convection is enhanced over WNP and suppressed over MC, and La Niña-like SST anomalies appear in the preceding seasons and El Niño-like SST anomalies in the simultaneous summer. Results by a linear baroclinic model further indicate that both the WNP heating and MC cooling can induce the strengthened CEF. Furthermore, the relationship between CEF and SST anomalies in the simultaneous summer is stable, but that between CEF and the preceding winter El Niño-Southern Oscillation (ENSO) experienced a decadal strengthening around 1997/98. After 1998, the preceding winter ENSO is followed by strong summer SST anomalies in MC and thus significantly affect CEF via modulating local convection. However, this ENSO-summer MC SST relationship is weak before 1997, failing to establish the relationship between the preceding ENSO and CEF.


Thu-03 Aug | 8:15 - 10:00 | MR332
AS25 - Air Pollution-Weather-Climate Interactions

Session Chair(s): Yang GAO, Ocean University of China, Jingyu WANG, Nanyang Technological University, Guangxing LIN, Chinese Academy of Sciences

AS25-A005 | Invited
Aerosol Impacts on Local Scale Convective Precipitation

Chuanfeng ZHAO1#+, Yue SUN2
1Peking University, 2Beijing Normal University

Aerosol particles in the atmosphere can alter precipitation efficiency and modulate the hydrological cycle, while their impacts on the cloud and precipitation formation time and vertical profiles remain poorly understood. Using multi-source observation data along with reanalysis meteorology, we find that different types of aerosols exert distinct effects on precipitation rate at different layers and precipitation start time. The observations show that aerosols enhance precipitation-top height first and then suppress it under various dynamics and thermodynamics conditions, with a turning point at medium aerosol amount. In contrast, the response of near surface precipitation rate to aerosol perturbation is complex due to varying evaporation efficiency. This finding challenges the previous studies that suggested that the characteristics of cloud and precipitation at high altitude are closely correlated with precipitation rate near the surface. Observations also show that absorbing aerosols near surface could advance precipitation start time while scattering aerosols near surface delay the precipitation start time, with the results illustrated with the precipitation events over the three typical regions in east China. This finding is useful for better understanding of aerosol-precipitation interaction and further improvement of model precipitation simulation and prediction.


AS25-A023
Anthropogenic Influences on Trends of Spring Rainfall Over East Asia: Synergic Effects of Greenhouse Warming and Aerosols on Decreasing Trends of Rainfall in Low-latitude East Asia

Young-Hee RYU1#+, Seung-Ki MIN2
1Yonsei University, 2Pohang University of Science and Technology

Low-latitude East Asia, particularly southern China, has shown markedly decreasing trends of springtime rainfall during recent years; however, rainfall trends are weak in mid-latitude East Asia. Details of human influences on this contrasting feature remain uncertain. This study quantifies the relative roles of greenhouse warming and aerosols in the observed spring rainfall trends over East Asia using the Weather Research and Forecasting model with chemistry (WRF-Chem model). As a result of greenhouse warming, high-latitude East Asia shows more rapid temperature increases potentially associated with reduced spring snow than the western North Pacific. These uneven temperature rises induce an anomalous anticyclone over the East China Sea. This circulation change results in a northwestward extension of the western North Pacific subtropical high, which reduces rainfall at low latitudes but moderately increases rainfall at mid-latitudes. In contrast, anthropogenic aerosols reduce rainfall in both low- and mid-latitude East Asia. Hence, the two anthropogenic factors synergistically reduce rainfall at low latitudes, with a stronger contribution of greenhouse warming (~34%) than aerosols (~17%). In mid-latitude East Asia, their contributions are offset, resulting in weak rainfall trends. Further, the anthropogenic influences are found to be relatively larger under drier conditions, suggesting that a more severe drought can occur in low-latitude East Asia under future drought-conducive conditions.


AS25-A004
Climate Impacts of Aerosol Reductions in China Due to Clean Air Actions and COVID-19

Yang YANG1#+, Jiyuan GAO2, Lili REN2, Chao LIU2, Hailong WANG3, Hong LIAO2
1Nanjing University of Information Science and Technology, 2Nanjing University of Information Science & Technology, 3Pacific Northwest National Laboratory

China has implemented a sequence of policies for clean air since year 2013 and the aerosol pollution has been substantially improved, but ozone (O3) related issues arose. Meanwhile, aerosol emissions in South Asia have continued to increase. Here, based on chemistry-climate model simulations, we found that the overall decreases in aerosols produced an anomalous warming of 0.09 ℃ in eastern China, which is further intensified by the increase in O3 in the lower troposphere, resulting in an enhanced warming of 0.16 °C in eastern China. The reductions in aerosol emissions from East Asia alone increased the East Asian summer monsoon (EASM) strength by almost 5%. The dipole pattern of aerosol emissions between South Asia and East Asia together increased the EASM by 5–15% during 2013–2017, revealing an important role of South Asian aerosols in changing the East Asian climate. Record rainfall and severe flooding struck eastern China in the summer of 2020. The extreme summer rainfall occurred during the COVID-19 pandemic, which started in China in early 2020 and spread rapidly across the globe. By disrupting human activities, substantial reductions in anthropogenic emissions of greenhouse gases and aerosols might have affected regional precipitation in many ways. Here, we investigate such connections and show that the abrupt emissions reductions during the pandemic strengthened the summer atmospheric convection over eastern China, resulting in a positive sea level pressure anomaly over northwestern Pacific Ocean. The latter enhanced moisture convergence to eastern China and further intensified rainfall in that region. Modeling experiments show that the reduction in aerosols had a stronger impact on precipitation than the decrease of greenhouse gases. We conclude that through abrupt emissions reductions, the COVID-19 pandemic contributed importantly to the 2020 extreme summer rainfall in eastern China.


AS25-A009
Decreasing Dust Over the Middle East Partly Caused by Irrigation Expansion

Yong WANG1#, Wenwen XIA1+, Bin WANG2
1Tsinghua University, 2Chinese Academy of Sciences

The importance of the effects of anthropogenic activities on modulating the global dust cycle has been increasingly recognized. Over the Middle East, we find in observations that there has been a significant decrease in dust optical depth from 2007 to 2019 during which global irrigated areas especially in the Middle East and South Asia have rapidly expanded. Whether irrigation expansion contributes to the decrease of dust in the Middle East is investigated based on observations/reanalyses and global climate model simulations with and without irrigation. Results show that irrigation over the northeast Middle East and Pakistan supplements water to the soil. By increasing local evaporation and moisture advection, irrigation enhances precipitation over the whole Middle East and the northwest Indian subcontinent. As a result, dust wet deposition by precipitation is elevated. Owing to irrigation-induced land surface cooling, surface wind speed decreases as the planetary boundary layer becomes stable. Along with increased soil moisture, reduced surface wind speed suppresses local dust emissions. Enhanced dust wet deposition and suppressed dust emissions cause atmospheric dust reduction over the Middle East. Vegetation greening in the Middle East as the climate warms has no contribution because there is no obvious trend found in observations.


AS25-A020
Attribution of the Aerosol Simulation Biases Over China in the AerChemMIP Models

Tianyi FAN1#+, Xiaohong LIU2, Chenglai WU3, Yi GAO3, Chuanfeng ZHAO4, Xin YANG1, Keying LI1
1Beijing Normal University, 2Texas A&M University, 3Chinese Academy of Sciences, 4Peking University

Biases of aerosol simulation by nine models participating the Aerosol and Chemistry Model Intercomparison Project (AerChemMIP) were identified over China. The AerChemMIP ensemble mean aerosol optical depth (AOD) is high biased over Yangtze River Basin, Sichuan Basin, Yungui Plateau, and Loess Plateau in winter compared with the MODIS satellite retrievals due to a few model outliners. AOD underestimation in North China Plain can be found all year along in most models. These patterns of model biases were persistent over multiple years from 2002 to 2015. The AOD biases cause errors in the aerosol radiative forcing estimations. We attribute the AOD biases to the biases of meteorological factors and aerosol/precursor gas emissions in the models. The results show that it is necessary for climate models to perform reasonably well in simulating the dynamical, physical and chemical processes on regional scale in order to estimate the aerosol radiative forcing. 


AS25-A010
Evaluation and Improvement of Simulated Absorption of Brown Carbon in Eastern China

Lulu XU1#+, Guangxing LIN1, Xiaohong LIU2
1Chinese Academy of Sciences, 2Texas A&M University

Recent studies have shown that components of organic aerosols, known as brown carbon (BrC), can have strong absorption of UV and short visible light in the atmosphere. According to laboratory and field studies, the optical properties of BrC, such as the imaginary part of refractive index can vary hundreds of times, which brings great challenges to the estimation of the climate effect of BrC. Primary emissions of BrC in China are particularly high and the main sources of BrC in China (residential heating, cooking and fossil fuel combustion) are quite different from American and European countries. However, the current research on the modeling of brown carbon in China is relatively few and has large biases from observation. In this study, BrC was added to the Modal Aerosol Module (MAM4) in CAM5.4, and the BrC tracer was separated from organic carbon in the model. We considered two sets of different BrC emissions and suitable optical properties were chosen for different combustion sources in China for model input. Then we simulated absorption coefficients (Babs, BrC), aerosol absorption optical depth (AAOD) and absorption Angstrom exponent (AAE) of BrC over eastern China and evaluated those values using ground-based remote sensing, satellite remote sensing and ground site observations. Our research showed that adding BrC into the climate model can improve the underestimation of absorption coefficients, aerosol absorption optical depth and absorption Angstrom exponent of brown carbon in autumn and winter seasons in eastern China. However, the simulated values are still severely underestimated. The Measurement-Model Fusion method can be considered to reduce the bias between the simulated and observed values of aerosol optical absorption.


AS25-A013
Which Aerosol Type Dominate the Impact of Aerosols on Ozone via Changing Photolysis Rates?

Jinhui GAO#+
Chengdu University of Information Technology

The impact of aerosols on ozone via influencing photolysis rates is a combined effect of absorbing aerosols (AA) and scattering aerosols (SA). However, AA and SA show different optical properties and influence photolysis rates differently, which then cause different impacts on ozone. Till now, the dominate factor is disconfirmed, which is largely due to the impact of SA on ozone not reaching to a consistent conclusion. In this study, the WRF-Chem model was implemented to simulate the air pollutants over the North China Plain (NCP). The impacts of AA and SA on ozone via influencing photolysis rates were quantitatively isolated and analyzed. Our results also demonstrated the decreasing effect of AA on ozone within planet boundary layer (PBL) which is consistent with the conclusions of previous studies. But for SA, it decreased the ozone chemical contribution (CHEM) near surface but increased which in the upper layers of PBL, that enlarge the ozone vertical gradients. In this case, more vertical exchanges of ozone would occur with the effect of vertical mixing motion of atmosphere, then the opposite CHEM variations were counteracted with each other and finally led to very slight changes in ozone within PBL. Thus, it can be summarized that AA dominate this impact of aerosols on ozone. Reducing AA could cause a general increase in ozone (ΔO3) over the NCP. Based on the aerosol levels of this case, ΔO3 would be seen over 86 % of the areas in the NCP when reducing AA by 3/4 and ΔO3 was more significant in the megacities. Our study highlights the different relationships between ozone and aerosol types, which suggests that more attentions should be paid on aerosol types, especially AA, when making the synergetic control strategy of aerosols and ozone in China.


Thu-03 Aug | 10:20 - 12:20 | MR311
AS15 - 16th Sasaki Symposium on Data Assimilation for Atmospheric, Oceanic and Hydrologic Applications

Session Chair(s): Yanhui XIE, Beijing Research Center for Urban Meteorological Engineering and Technology, Takemasa MIYOSHI, RIKEN Center for Computational Science

AS15-A005
PREVENIR: Japan-Argentina Cooperation Project for Heavy Rain and Urban Flood Disaster Prevention

Takemasa MIYOSHI1,2#+, Celeste SAULO3, Shigenori OTSUKA1, Juan RUIZ4, Yanina SKABAR3, Arata AMEMIYA1, Tomoo USHIO5, Hirofumi TOMITA6, Tomoki USHIYAMA7, Masaya KONISHI8
1RIKEN Center for Computational Science, 2University of Maryland, 3National Meteorological Service Argentina, 4University of Buenos Aires, 5Osaka University, 6RIKEN Advanced Institute for Computational Science, 7International Center for Water Hazards and Risk Management, 8Japan Meteorological Agency

This presentation provides an overall summary of the project PREVENIR and recent activities about data assimilation and numerical weather prediction (NWP) research. 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 designed for two highly vulnerable urban basins in Argentina: one located in Buenos Aires Province and the other in Córdoba Province. PREVENIR takes advantage of leading research on simulations and 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, quantitative precipitation estimates (QPE), nowcasting, BDA and NWP, hydrological model prediction, warning communications, public education, and capacity building. Here, the Japanese leading institutions in the scientific research and operational services, i.e., RIKEN, Osaka University, the International Centre for Water Hazard and Risk Management (ICHARM), and the Japan Meteorological Agency (JMA) closely work with the Argentinian counterparts, i.e., the National Meteorological Service, the National Water Institute, and the National Research Council of Argentina under the strong support of JICA, JST, and Argentinian Foreign Affairs Ministry. Heavy rains and urban floods are important global issues under the changing climate. 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.


AS15-A014
Estimation of AMSU-A Radiance Observation Impacts in an AGCM-LETKF Data Assimilation System: Comparison with EFSO and OSEs

Akira YAMAZAKI1#+, Koji TERASAKI2, Takemasa MIYOSHI3,4, Shunsuke NOGUCHI5
1Japan Agency for Marine-Earth Science and Technology, 2Meteorological Research Institute, 3RIKEN Center for Computational Science, 4University of Maryland, 5Kyushu University

The impacts of assimilating AMSU-A satellite radiances with sensitive channels to the upper troposphere and the lower stratosphere were evaluated using an AGCM–local ensemble transform Kalman filter (LETKF) data assimilation system. Two streams of data-denial experiments for the AMSU-A observations have been performed for about a month in the Northern and Southern Hemisphere (SH) winters. Accumulating observation impact (OI) effects by cycling (repeating) data denials were quantified through the data assimilation system's tropospheric and stratospheric general circulation. It was discovered that adding the AMSU-A observations aided in reducing total OI by all observations of each data assimilation cycle; this is the opposite of the estimation of AMSU-A OI by the ensemble-based forecast sensitivity to observations (EFSO); however, such contributions could stabilize the data assimilation cycles. In both experiments, the accumulated AMSU-A OI was most evident in the upper troposphere, particularly in the SH midlatitudes where the westerly jets exist, and observations of the other types are sparse. The estimated AMSU-A OI by EFSO was also the most valuable (beneficial) in a similar space. Results demonstrated that AMSU-A OI tended to accumulate just downstream where EFSO estimated beneficial OI signals and that the accumulation of AMSU-A OI was tied to dynamic processes in the upper-tropospheric and general stratospheric circulation. Therefore, EFSO helps estimate the beneficial distributions of accumulated AMSU-A OI by considering their dynamical propagation.


AS15-A008
Impact of SMAP Soil Moisture Retrievals in the Coupled Atmosphere-land Surface Data Assimilation System with WRF-Noah LSM

Sujeong LIM1+, Seon Ki PARK1#, Milija ZUPANSKI2
1Ewha Womans University, 2Colorado State University

Soil moisture is important in a coupled atmosphere-land surface model because it propagates to atmospheric variables such as temperature and water vapor mixing ratio in the planetary boundary layer through the latent and sensible heat fluxes. Therefore, soil moisture observations in a coupled atmosphere-land surface data assimilation system can provide useful information for both the land surface and atmospheric systems. In this study, we assimilate the National Aeronautics and Space Administration’s Soil Moisture Active Passive (SMAP) soil moisture retrievals, which observe the top 5 cm soil moisture with a global coverage every 2-3 days and a 1000 km swath width. We interface the Maximum Likelihood Ensemble Filter (MLEF) — a hybrid ensemble-variational data assimilation system — with the Noah land surface model (Noah LSM or simply Noah) coupled with the Weather Research and Forecasting (WRF), i.e., developing the WRF-Noah-MLEF system. As a strongly coupled data assimilation system, MLEF assimilates both atmospheric and soil moisture observations — the National Centre for Environmental Prediction (NCEP) Prepared Binary Universal Form for the Representation of meteorological data (PrepBUFR) and the SMAP soil moisture retrievals — and simultaneously corrects the atmospheric and land surface variables. Our results indicate that the WRF-Noah-MLEF system improves the soil moisture prediction that provides additional information to the atmospheric variables, especially in the planetary boundary layer, through cross-covariances between land and atmosphere.


AS15-A006
Improving Air Quality Forecasting Through an Intelligent Optimization System: Sequential Optimization of Physical Parameterization Schemes and Parameters in WRF-Chem

Ji Won YOON+, Ebony LEE, Seon Ki PARK#
Ewha Womans University

Air pollution has brought about environmental problems progressively in East Asia, mainly due to the rapid economic growth and high energy consumption. To deal with the air pollution problem, it is vital to enhance the air quality forecast skill using a numerical model. In particular, the performance of numerical air quality prediction considerably depends on the planetary boundary layer (PBL) and the land surface processes in a coupled atmosphere-chemistry model, such as the Weather Research and Forecasting (WRF) model coupled with Chemistry (WRF-Chem). 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 an optimal combination of the physical parameterization schemes and parameters sequentially in WRF-Chem to improve air quality forecasting. For optimization, we selected several cases based on the sources and transport routes of the Asian dust storm (ADS) that affected South Korea (SK). Overall, the WRF-Chem with the optimized set of parameterization schemes and parameter values outperforms that with non-optimized ones in forecasting the ADS events in SK.


AS15-A003
Data Assimilation and the Precipitation Forecast Inconsistency

Yidi XUE1, Xiang-Yu HUANG2#+, Yu XIA1, Bing LU1, Min CHEN1
1China Meteorological Administration, 2Institute of Urban Meteorology, CMA

The rapid update cycle numerical weather prediction systems (such as CMA-BJ system) assimilate multiple observation data at high frequency and have advantages for predicting precipitation events with small horizontal scale and short life history. However, the high frequency assimilation of various observation data often produces significantly different forecasts from different data assimilation cycles. The jumpiness, i.e., inconsistency in forecasts, particularly those related to precipitation, usually brings uncertainty to the forecasting operations and often seriously interferes with the judgment of duty forecasters. In this study, we investigate the inconsistent CMA-BJ precipitation forecast issue and attempt to identify the factors that may affect the consistency of subsequent cycling forecasts. In addition to subjective comparisons between consecutive precipitation forecasts, an FSS-based jumpiness index is proposed to quantify the precipitation forecast inconsistency. Numerical experiments demonstrate that the data assimilation configurations and cycling strategy would have a significant impact on the consistency of the precipitation forecast. Results from ongoing work on reducing the precipitation forecast inconsistency while maintaining performance scores will be presented at the meeting.


AS15-A015
Performances of All-sky Satellite Radiance Assimilations for the Prediction of Recent Northwest Pacific Super-typhoons

Masashi MINAMIDE1,2#+
1The University of Tokyo, 2Jet Propulsion Laboratory

Predictions of the early stage of tropical cyclones are challenging given its strong nonlinear processes with multi-scale interaction and the lack of dense observation network. Because most of super-typhoons are born and develop over tropical Pacific oceans far away from the coverage of land-based observation networks, the geostationary satellites observations are often the only available observations to capture the lifecycle of TCs. To investigate the full potential of such geostationary satellite for TC forecasting, we have developed and been investigating the impacts of assimilating all-sky satellite radiances from Himawari-8, together with the set of conventional observations, on the prediction of the rapid intensification process of TCs using convection-permitting ensemble Kalman filter data assimilation system originally developed at Penn State University with WRF and CRTM. In this study, we will introduce the forecast performances of recent super-typhoon cases, such as Mindulle (2021) and Nanmadol (2022), both of which were the target of aircraft dropsondes observations under the TPARC-II field campaign. We found that the all-sky satellite radiance assimilations helped to better capture the rapid intensification of TCs in their early stages, but also sometimes had difficulty in reproducing the detailed TC inner-core structures under the coverage of high clouds in their matured stages due the limitation of infrared observations. This research will have implications for the potential benefits of combining various sources of observations to better initialize and forecast developing typhoons.


AS15-A019
Including Observation Error Correlation for Ensemble Radar Data Assimilation and its Impact on Heavy Rainfall Prediction

Hao-Lun YEH1+, Shu-Chih YANG1#, Takemasa MIYOSHI2,3, Koji TERASAKI4
1National Central University, 2RIKEN Center for Computational Science, 3University of Maryland, 4Meteorological Research Institute

An assumption of uncorrelated observation errors is commonly adopted in conventional data assimilation. For this reason, high-resolution data are usually resampled with superobbing or data-thinning strategies. These strategies diminish the advantages of high temporal and spatial resolutions that can provide essential details in convection development. However, assimilating high-resolution data, such as radar radial wind, without considering observation error correlations can lead to overfitting and thus degrade the performance of data assimilation and forecasts. This study uses a radar ensemble data assimilation system that combines the Weather Research and Forecasting model and Local Ensemble Transform Kalman Filter (WRF-LETKF) to assimilate radar radial wind and reflectivity data. We further include the error correlation of the Doppler radar radial wind and reflectivity in the WRF-LETKF radar assimilation system. We examine the impact on the accuracy of convective-scale analysis and short-term precipitation prediction in Taiwan, for heavy rainfall events with different characteristics. The horizontal error correlation scale of radial wind and reflectivity ranges from 15 to 25 km, depending on the type of precipitation events. The introduction of observation error correlation for radar radial data assimilation produces more small-scale features in wind and hydrometer analysis corrections compared to the experiment using an independent observation assumption. Consequently, the modification of wind corrections leads to stronger convergence accompanied by higher water vapor content, which enhances local convections. The additional small-scale hydrometer corrections improve the location and intensity of the reflectivity. This results in more accurate forecasts of short-term precipitation. For local convections, including the reflectivity observation error correlation additionally can better capture the rapid changing convection.


AS15-A001 | Invited
Impact of Assimilating FY-4A Atmospheric Motion Vectors on Henan 7.20 Rainstorm Forecast in 2021

Yanhui XIE#+
Beijing Research Center for Urban Meteorological Engineering and Technology

Fengyun-4A (FY-4A) is the new-generation geostationary meteorological satellite of China. Atmospheric motion vectors (AMVs) derived from images of FY-4A can provide high-spatiotemporal-resolution wind observations in the atmospheric middle and upper levels. To explore the potential benefits of these data for the numerical forecasting of severe weather events, the impacts of assimilating FY-4A AMVs on forecasts of the rainstorm happened in Henan province of China on July 20, 2021, were investigated based on the Weather Research and Forecasting (WRF) model. Three groups of assimilation experiments were conducted and evaluated against observations. The results show that FY-4A AMVs with a higher quality indicator (QI) exhibit a lower error characteristic at the cost of a reduced sample size. Assimilation of FY-4A AMVs reduces the error of upper-level wind fields in the 24-h forecasts. A positive impact can be also obtained for 10-meter wind of 24-h forecasts, with the improvement up to 9.74% for the mean bias and 3.0% for the root-mean-square error due to the including of FY-4A AMVs with QI > 70. Assimilating the AMVs with QI > 80, there is an overall positive impact on the CSI score skills of 6-h accumulated precipitation above 1.0 mm in the 24-h forecast. A significant improvement can be found in the forecast skill of the heavy rainfall above 25.0 mm after 6 h of the forecast. The spatial distribution of 24-h accumulated heavy rainfall zone is closer to the observations with the assimilation of FY-4A AMVs. The adjustment of the initial wind fields resulting from FY-4A AMVs brings a clear benefit to quantitative precipitation forecasting skills for the event of Henan 7.20 rainstorm. However, AMVs data assimilation still has difficulty in capturing the hourly maximum rainfall and intensity well.


Thu-03 Aug | 10:20 - 12:20 | MR327
AS38 - Ensemble Modeling and Prediction of High-impact, Multi-scale Weather to Decadal Events

Session Chair(s): Jie FENG, Fudan University

AS38-A017
The Backward Nonlinear Local Lyapunov Exponent and its Application to Quantifying the Local Predictability of Extreme High‑temperature Events

Xuan LI1#+, Ruiqiang DING2
1Fudan University, 2Beijing Normal University

The backward nonlinear local Lyapunov exponent (BNLLE) was developed based on the NLLE method to quantitatively investigate the local predictability of extreme events. By studying the dynamical characteristics of error growth preceding extreme events, the local predictability limits of these events can be determined. In this study, the BNLLE method is used to quantify the local predictability limits of two extreme high-temperature events (EHTEs) that occurred in Europe during the summer of 2019. The results show that the error dynamics are dependent on the geographical location. During the early forecast period, positive error-growth rates are mainly located in southern regions, whereas negative error-growth rates are mainly located in northern regions. However, the variations in the error growth rates exhibit regional differences with the forecast time. As such, the relative growth of initial errors (RGIEs) also depends on the geographical location. From the RGIEs, the local predictability limits of the two EHTEs are determined to be 11 and 9 days, respectively. By measuring the forecast skill, the local predictability limits (11 and 9 days) are verified to be reasonable and realistic. Therefore, the BNLLE method can quantify the local predictability of EHTEs, and is an effective technique for studying the predictability of future extreme weather and climate events.


AS38-A015
Ensemble-based Sensitivity Analysis of the Track Forecasts of Typhoon In-fa in ECMWF, NCEP, and CMA Ensemble Prediction Systems

Liangying LIU#+, Jie FENG
Fudan University

Intense Typhoon In-fa in July 2021 struck eastern China and caused disastrous damage to human lives and properties. Due to the interaction of complex synoptic systems, the official track forecasts of Typhoon In-fa in most operational centers show large forecast errors, especially in the veer and landfall of In-fa. The goal of this study is to investigate the major factors that caused the track forecast uncertainties of In-fa and relevant mechanisms. A fast and feasible method, the ensemble-based sensitivity technique, is adopted using the ensemble forecast members in the operational ensemble prediction systems at ECMWF, NCEP, and CMA. In virtue of the time-lagged covariance of ensemble forecasts, the sensitivity of typhoon track forecast errors to various factors, such as variables and regions associated with specific synoptic systems, are identified and analyzed in detail. The results suggested that the environmental steering winds related to the variability of two critical systems, Pacific subtropical high (SH) and monsoon trough (MT) near the typhoon positions, were the main causes for the track forecast uncertainties of “In-fa” in the both two cases. However, the results have obvious model dependence. Although effects of MT are similar in different models, the influence mechanism of subtropical high is diverse due to the combination of morphology, location and intensity. Meanwhile, we innovatively propose an ensemble-based sensitivity technique considering the model bias, revealing the influence of the model bias on the sensitivity calculation results. 


AS38-A007
Integral Correction of Initial and Model Errors in System of Multigrid NLS-4DVar Data Assimilation for Numerical Weather Prediction (SNAP)

Hongqin ZHANG#+, Xiangjun TIAN
Chinese Academy of Sciences

Model error has a marked influence on forecast error, and integral correction of the initial and model errors in a novel four-dimensional variational data assimilation (4DVar) method (i4DVar) has recently been developed. Unlike traditional 4DVar, in which the analysis increment focuses only on the initial time point, i4DVar introduces an averaged integral correction term to correct the error evolution at multiple times with the same time interval in the assimilation window; that is, the assimilation window is divided into several sub-windows. In this study, we incorporated i4DVar into the System of Multigrid Nonlinear Least-squares-4DVar Data Assimilation for Numerical Weather Prediction (NWP) (SNAP), hereafter referred to as SN-i4DVar, and explored its impacts on NWP. The effectiveness and performance of SN-i4DVar were evaluated using two extreme rainstorm cases assimilating conventional and satellite observations, respectively. The results indicated that integral correction of the initial and model errors reduced analysis error and forecast error growth rates. SN-i4DVar performed better in precipitation forecasting than the original SNAP and exhibited generally better forecasting capability in terms of the horizontal wind speed (u and v), temperature, and humidity variables, indicating that SN-i4DVar simultaneously countered initial model errors to improve NWP capability. Meanwhile, the 4DEnVar method, which considers the optimal analysis in the ensemble space, benefits from the improved ensemble space generated according to the formulas of i4DVar, and the observation information can be more effectively absorbed and a more accurate analysis can be obtained by SN-i4DVar.


AS38-A006
A Rapid Intensification Warning Index for Tropical Cyclones Based on the Analog Method

Deyu LU#+, Quanjia ZHONG
Chinese Academy of Sciences

Prediction of the rapid intensification (RI) of tropical cyclones (TCs) remains challenging. In this paper, by using information from the early period following TC formation, the Rapid Intensification Warning Index (RIWI) is developed based on the analog method. 10-year cross-validation and data from Hurricane Ida (2021) are used to verify its potential application. Results show that the RIWI can efficiently discriminate between RI and non-RI storms and has a significant positive correlation with the lifetime maximum intensity (LMI) of the TCs. By using this index, an early warning can be issued ~30 hours before the onset of RI, which is much earlier than the predictions made using the probabilistic Statistical Hurricane Intensity Prediction System (SHIPS) RI index. In addition, by using the RIWI as a predictor, the prediction of LMI provides an early estimate of TC severity.


AS38-A005
Multidecadal Variation in the Seasonal Predictability of Winter PNA and its Sources

Xiaoqin YAN#+, Youmin TANG, Wangjie YAO
Hohai University

Based on reanalysis and ensemble hindcasts data, this work investigates the multidecadal variation in the seasonal predictability of the Pacific-North American (PNA) teleconnection pattern during the winter and its sources. The results show that at the two ends of the 20th century, the PNA is mostly driven by the El Niño-Southern Oscillation (ENSO), and a good seasonal prediction of the PNA is expected if models can accurately predict the PNA-ENSO relationship. During the middle 20th century, the PNA is not only driven by ENSO but also closely linked to the Pacific Decadal Oscillation through the air-sea coupling process in the extratropical North Pacific. Improvements in the seasonal prediction of the PNA require models to accurately predict both the PNA-ENSO relationship and the air-sea coupling in the northern extratropical Pacific.


Thu-03 Aug | 10:20 - 12:20 | MR328
AS10 - Extreme Events: Observations and Modeling

Session Chair(s): Yeon-Hee KIM, Pohang University of Science and Technology, Sridhara NAYAK, Japan Meteorological Corporation, Raju ATTADA, Indian Institute of Science Education and Research Mohali

AS10-A012
Attribution of the Unprecedented 2021 October Heatwave in South Korea

Yeon-Hee KIM1#+, Seung-Ki MIN1, Dong-Hyun CHA2, Young-Hwa BYUN3, Fraser LOTT 4, Peter STOTT4
1Pohang University of Science and Technology, 2Ulsan National Institute of Science and Technology, 3National Institute of Meteorological Sciences, 4Met Office Hadley Centre

In the first half of October 2021, an anomalously high temperature similar to summer was observed. The temperature in the first half of October was 19.9°C, which was 3.9°C higher than the average (1991-2020) and recorded the highest temperature since 1973. During the first half of October, a wide and strong circulation is maintained from the Philippines to the tropical central Pacific Ocean, resulting in strong high-pressure anomalies in South Korea and the central Pacific Ocean. The high-pressure anomaly in the upper atmosphere of the Korean Peninsula brings in warm southerly winds continuously and the central Pacific high-pressure system played a blocking role, preventing the eastward movement of the system and maintaining the downward airflow in the Korean Peninsula. This study compares probabilities of 2021-like extremely warm October in South Korea between real counterfactual world conditions using the datasets from CMIP6 (Coupled Model Intercomparison Project Phase 6) multi-model simulation and HadGEM3-A high-resolution large ensemble simulations. Results from both GCM ensembles indicate that the exceptionally strong October 2021 heatwave was extremely unlikely to occur without human influences. It should be noted, however, that the sample size and extreme nature of the event make it difficult to draw concrete conclusions from the model simulations. When based on weaker observed thresholds, robust human influences are found to have made such warm events at least 4 times more likely. Future analysis warns that October will be merged into summer in the near future, resulting in serious socioeconomic damage in health, agriculture, energy, etc. Under the high-emission SSP5-8.5 scenario, this unseasonal warmth is expected to become the new normal, occurring every 2 years after the mid-twenty-first century, which can be avoided when carbon neutrality is achieved around 2075 following the SSP1-2.6 scenario.


AS10-A002
Arctic and Pacific Ocean Conditions Were Favourable for Cold Extremes Over Eurasia and North America During Winter 2020/21

Ruonan ZHANG#+
Fudan University

A sequence of extreme cold events occurred across Eurasia and North America during winter 2020/2021. Here, we explore the causes and associated mechanisms for the extremely cold temperatures using both observations and large-ensemble simulations. Experiments were conducted with observed ocean surface boundary conditions prescribed globally, and regionally to discern the specific influence of Arctic, tropical Pacific and North Pacific drivers. Increased likelihood of daily cold extremes in mid December to mid January are found in Eurasian midlatitudes in response to reduced Arctic sea ice. Tropical sea surface temperature anomalies, more specifically the La Niña pattern, increased probability of extreme cold over high-latitude Eurasia in early January to early February. Both reduced Arctic sea ice and La Niña increased the probability of daily cold extremes over western North America in late January to late February. We conclude that a combination of reduced Arctic sea ice, La Niña, and a sudden stratospheric warming in January 2021 were factors in the February 2021 extreme cold-wave that caused huge societal disruptions in Texas and the Southern Great Plains. Although the magnitude of the simulated cold extremes are relatively small when compared with observed anomalies, the Arctic and Pacific Ocean surface conditions in winter 2020/21 increased the probability of cold days as cold or colder than observed by approximately 17%~43%.


AS10-A013
The Spatiotemporal Distribution of Extreme Precipitation and Related Near Surface Atmospheric Conditions During Summer of 2014-2019 Over the Tibetan Plateau Derived from GPM Observations and Reanalysis Datasets

Rui WANG#+, Wenshou TIAN
Lanzhou University

In this study, the characteristics of extreme precipitation events and related near surface atmospheric conditions (near surface temperature, pressure, specific humidity and CAPE) during summer of 2014-2019 over Tibetan Plateau are explored based on GPM satellite observations and multi-source reanalysis datasets (ERA5, ERA-Interim and CFSv2). The result shows significant differences in extreme precipitation between the hinterland of Tibetan Plateau and the south slope of the Himalayas. That is, the frequency and intensity of extreme precipitation are smaller in the hinterland of Tibetan Plateau than those in the south slope of the Himalayas, whereas the storm top height is higher. A small proportion of extreme precipitation develops vigorously (17 km) but does not mean that the extreme precipitation intensity is large at the same time. The peak frequency, intensity and storm top height of extreme precipitation tend to occur in the afternoon and midnight. Furthermore, the most favorable near surface temperature, pressure and specific humidity for the occurrence of extreme precipitation are 285-290 K (11.85°C-16.85°C) and 295-300 K (21.85°C-26.85°C), 550 hPa and 950 hPa, 10 g/kg and 18 g/kg over the hinterland of Tibetan Plateau and the south slope of the Himalayas, respectively. The extreme precipitation intensity could be large even if CAPE is not strong over the Tibetan Plateau. Besides, the anomalies of near surface atmospheric conditions related to extreme precipitation exhibit obvious abrupt changes within 6 hours before and after the occurrence of extreme precipitation. This work illuminates the spatiotemporal distribution of extreme precipitation and the changes of near surface atmospheric conditions before and after extreme precipitation over the Tibetan Plateau from the perspective of GPM remote sensing and reanalysis datasets, which could be considered into forecast of extreme precipitation over the Tibetan Plateau in the future.


AS10-A011
3D DBSCAN Detection and Parameter Sensitivity of the 2022 Yangtze River Summertime Heatwave and Drought

Zhenchen LIU#+, Wen ZHOU
Fudan University

Spatially and temporally accurate event detection is a precondition for exploring the mechanisms of climate extremes. To achieve this, a classical unsupervised machine learning method, the DBSCAN (Density-Based Spatial Clustering of Applications with Noise) clustering algorithm, was employed in the present study. Furthermore, we developed a 3D (longitude–latitude–time) DBSCAN-based workflow for event detection of targeted climate extremes and associated analysis of parameter sensitivity. We applied this 3D DBSCAN-based workflow in the detection of the 2022 summertime Yangtze extreme heatwave and drought based on the ERA5 reanalysis dataset. The heatwave and drought were found to have different development and migration patterns. Synoptic-scale heatwave extremes appeared over the northern Pacific Ocean at the end of June, extended southwestwards, and covered almost the entire Yangtze River Basin in mid-August. By contrast, a seasonal-scale drought occurred in mid-July over the continental area adjacent to the Bay of Bengal, moved northeastwards, and occupied the entire Yangtze River Basin in mid-September. Event detection can provide new insight into climate mechanisms while considering patterns of occurrence, development, and migration. In addition, we also performed a detailed parameter sensitivity analysis for better understanding of the algorithm application and result uncertainties. The DOI-based linkage is https://doi.org/10.1016/j.aosl.2022.100324.


AS10-A010
Winter Warming and its Trend in India

Anil KUMAR#+, Netrananda SAHU
University of Delhi

Winters around the world are changing, in some cases, faster than any other season. Natural events and human activities are believed to be contributing to an increase in average global temperature. There are many studies on global warming but most of them are focused on the summer season and winter warming is neglected. The effect of global warming can also be seen during winters. Since 1990s, the warmer winters have drawn much attention world over and India is no exception. There is an increasing trend in winter temperature in India especially during the last three decades. Due to the rising of winter temperature, the duration of winter is decreasing. Long-term changes (1971-2021) in monthly mean temperature are examined by studying trends in maximum and minimum temperature for the winter period (DJF). The trend of temperature during the winter season has been analysed using Mann-Kendall and Sen’s slope test. We get the increasing trend of temperature but this increase in temperature during winter is not uniform throughout the country. It is increasing more rapidly in the northern region as compared to the southern region. The temperature in the east India region is showing a decreasing trend.


AS10-A032
Future Changes in the Joint Probability of Compound Hot and Dry Extremes in China

Ziwei ZHU1+, Liying QIU2, Eun-Soon IM3#
1The Hong Kong University of Science and Technology, Hong Kong SAR, 2The Hong Kong University of Science and Technology, 3HKUST

The severity and frequency of compound extremes are expected to increase with the acceleration of global warming. In particular, southeastern China has already witnessed concurrent hot and dry extremes increasing over the few decades. Although there have been estimates of the likelihood of compound extremes based on Coupled Model Intercomparison Project Phase 5 (CMIP5), the recent release of the CMIP6 datasets provides a good opportunity to update their assessments. In this regard, this study investigates the changes in the joint return period of hot and dry extremes in China using multiple climate projections based on the statical downscaling of CMIP6 global models. While the wet bulb temperature is analyzed for hot extremes, the Palmer Drought Severity Index is considered to measure the meteorological drought. A bivariate copula function is then applied to comprehend the joint dependency of concurrent hot and dry extremes. The focus is placed on the comparative analysis of the changes in the joint return period under low and high emission scenarios, which may help to illustrate the benefits of climate change mitigation. In addition, our analysis attempts to discover the emergent constraints of how this relationship is likely to modulate the co-occurrence of extreme heat and dryness in response to the different levels of warming. [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.


AS10-A027
Longer- and Slower-moving Contiguous Heatwaves Linked to El Niño

Sijia WU+, Ming LUO#
Sun Yat-sen University

Although it is known that the frequency and duration of heatwaves are affected by the El Niño–Southern Oscillation (ENSO) at an interannual scale, the ENSO modulations on the moving properties (e.g., moving distance and speed) of spatiotemporally contiguous heatwaves that occur simultaneously in adjacent regions or neighboring days and exhibit 3D (latitude×longitude×time) spatiotemporal connectivity, are unknown. Here, we present the first assessment of the multi-dimensional characteristics of spatiotemporally contiguous heatwaves in relation to ENSO events by introducing a spatiotemporally contiguous event tracking (SCET) method. We show that the SCET method can well capture the dynamic evolution of contiguous heatwaves across space and time. It is also found that contiguous heatwaves during El Niño years tend to be more frequent, more persistent, and longer-traveling, but slower-moving than during La Niña episodes, and these modulations are seen on both global (particularly in the tropical regions) and continental scales. These differences in contiguous heatwaves over the tropical regions between El Niño and La Niña episodes are modulated by the maintenance of high-pressure anomalies. Further composite examinations indicate that, during the following summers El Niño induces anomalous atmospheric circulation, which is characterized by an intensified subsidence over the western North Pacific and ascending motion over the Indian and Pacific Oceans. These features provide favorable conditions for the occurrence and maintenance of contiguous heatwaves.


AS10-A009
Circum-western Canada Pattern in Boreal Summer Caused by the Boundary Current Synchronization

Akane HARA1#+, Tsubasa KOHYAMA1, Yoko YAMAGAMI2, Hiroaki TATEBE2
1Ochanomizu University, 2Japan Agency for Marine-Earth Science and Technology

The Kuroshio Current and the Gulf Stream are separated by about 10,000 km across the continent. However, the sea surface temperatures along the Kuroshio Current and the Gulf Stream synchronize via the westerly jet stream, called the Boundary Current Synchronization (BCS). BCS brings extreme heat waves and other extreme weather events to metropolitan areas in the mid-latitudes of the Northern Hemisphere, including Japan. However, the mechanism has not been investigated in detail. In this study, we define the “Circum-Western Canada (CWC) pattern” as an atmospheric variability closely related to the BCS index to examine the impact of the BCS on extreme weather in the mid-latitudes of the Northern Hemisphere. We define the CWC index using a reference region with a large regression and correlation coefficients of geopotential height at 200hPa on the BCS index. The Empirical Orthogonal Function analysis shows that the CWC pattern is the predominant mode in the western half of the Northern Hemisphere. The regression map of geopotential height at 200hPa on the Arctic Oscillation (AO) index and that on the CWC index exhibit similar features, which suggests that the CWC index is also in close relation to the AO index defined by the surface pressure. The regression map of precipitation and 2m-air temperature on the CWC index indicate that CWC explains 2m-air temperature pattern in July 1994, July 2018 and July 2022 and precipitation pattern in July 1994 and July 2018. The results of a pacemaker experiment, in which sea surface temperatures in the Kuroshio Current and the Gulf Stream is relaxed to a different control run, indicate that whether BCS excites CWC pattern is sensitive to stochasticity.


Thu-03 Aug | 10:20 - 12:20 | MR329
AS05 - Cities, Extreme Weather, and Climate Change

Session Chair(s): Quang-Van DOAN, University of Tsukuba

AS05-A001
Investigate Extreme Precipitation in Multiple Urban Systems

Fei CHEN1#+, Cenlin HE1, Quang-Van DOAN2, Dev NIYOGI3,4, Liping DI5
1National Center for Atmospheric Research, 2University of Tsukuba, 3The University of Texas at Austin, 4Purdue University, 5George Mason University

Cities are increasingly vulnerable to the effects of flooding due to changes in heavy precipitation patterns as a result of climate warming and rapid urbanization. Under the support of the NASA Interdisciplinary Research in Earth Science Program, we undertake various research activities to explore the impact of urban physical processes on extreme precipitation, especially sub-daily extremes, in multiple urban areas (Tokyo, Singapore, Lagos, Houston, etc.) in different geographical and climate regimes. These research activities were performed by integrating remote-sensing and in-situ observations and high-resolution long-term convection-permitting WRF simulations to tease out the relationship between extreme precipitation evolution and larger-scale climate warming and regional urbanization. We will present and discuss the research approach and main scientific findings. For instance, the study focusing on the Tokyo and Singapore pointed out enhanced hourly extreme precipitation by global-warming. The extreme part of heavy precipitation intensifies, and its intensification rate is at a super Clausius-Clapeyron rate. This has important implications to urban flooding prevention and mitigation and to urban planners, because the precipitation response to future climate warming is not linear, and skewed toward more increased extremes. As a team, we also conduct a coordinated study of the impact of urbanization over the Lagos, Nigeria, region, and examine the evolution of urban heat islands and precipitation as a result of Lagos rapid urbanization in the last two decades. To translate scientific findings into actionable science, we initiated dialogues with several university groups in Nigeria to discuss possible pathways for sharing data and connecting with local stakeholders. Our Nigerian colleagues have been addressing various urban environmental issues along the line of the World Climate Research Programme (WCRP) My Climate Risk (MCR) activities. One proposed idea is to help Nigerian colleagues establish a MCR Urban Regional Hub in Lagos. We will report the progress on these activities. 


AS05-A014
Representation of the Urban Boundary Layer Over Singapore in 100m uSINGV

Song CHEN1#+, Pratiman PATEL2, Anurag DIPANKAR3, Matthias ROTH2, Humphrey LEAN4, Hugh ZHANG5, Aurel MOISE1
1Centre for Climate Research Singapore, 2National University of Singapore, 3ETH Zurich, 4Met Office, 5CCRS

Singapore is a highly urbanized coastal city in the tropics, but its atmospheric boundary layer is not well modelled and understood. To address this challenge, we employed a high-resolution model, which offers a better representation of urban surfaces and turbulence processes. The numerical simulations were conducted using the urban version of Singapore Meteorological Service’s numerical weather prediction system, with a horizontal grid length of 100 m (100 m uSINGV). Results showed that the 100 m uSINGV effectively captured chaotic turbulent structures within the convective boundary layer, and a turbulent kinetic energy spectrum analysis revealed that these chaotic structures aligned with the -5/3 slope of the Kolmogorov spectrum in the inertial subrange. By comparing the model simulations using the urban slab model and the single-layer urban canopy model MORUSES (Met Office–Reading Urban Surface Exchange Scheme), it was found that the grid length played a significant role in the chaotic turbulent structures. Cloud patterns, boundary layer profiles, and near-surface meteorological parameters are also compared to models using coarser grid lengths (i.e., 1500 m and 300 m) and observations from sources such as satellite image, radiosonde, and weather stations. Our results highlight the valuable contribution of the high-resolution 100 m uSINGV model in modelling the urban boundary layer over Singapore.


AS05-A018
Evolving Urban Heat Island in the Era of Climate Change: A Study Over a Tropical Twin City Region in Eastern India

Soumya Satyakanta SETHI#+, V. VINOJ
Indian Institute of Technology Bhubaneswar

Urbanization and subsequent change to surface characteristics are known as the Surface urban heat island (SUHI) effect. SUHI is well-reported worldwide, however, studies on tier-2 growing cities in the global south are limited. Further, high-resolution long-term spatio-temporal observations with good-quality data have been publicly available since the start of this millennium. The current study explores the spatial distribution and temporal evolution pattern of SUHI for rapidly growing tropical coastal twin cities—Bhubaneswar and Cuttack—in eastern India during the last two decades (2001–2020). Our study reveals a clear discernible annual nighttime SUHI for both Bhubaneswar and Cuttack (0.75 ± 0.08 and 1.22 ± 0.07 °C) with a decadal growth rate of 0.18 ± 0.07 and 0.13 ± 0.07 °C/decade, respectively. Daytime SUHI lacked a clear urban-rural dichotomy like nighttime cases. Irrespective of the time, SUHI (both intensity and trend) was found to be very much dependent on the selection of the rural domain. A linear rise in SUHI parameters was observed for more distant rural domains indicating urban effects beyond local boundaries. We will further discuss spatial climatology and trend patterns with seasonality in detail.


AS05-A020
The Importance of Land Cover in O(100 m) Grid Length Numerical Weather Prediction – A Pearl River Delta Urban Mega-conglomeration Heat Wave Case Study

Lewis BLUNN1#, Kalli FURTADO2+, Jon SHONK1, Yali LUO3, Andrew HARTLEY1, Mathew LIPSON4
1Met Office, 2Centre for Climate Research Singapore, 3Nanjing University of Information Science & Technology, 4Bureau of Meteorology

High-fidelity spatially-detailed land cover is crucial in Numerical Weather Prediction (NWP) and climate projections when they are used to predict street-level urban processes. A global 300 m resolution land cover dataset (CCIv2) is included in the Met Office Unified Model (MetUM). Unlike the original CCI land cover dataset in the MetUM, CCIv2 has continuously varying urban fraction based on the Global Human Settlement Layer. The MetUM is run at 1.5 km, 300 m, and 100 m horizontal grid lengths for a heat wave case study (May 2018) over the Pearl River Delta urban mega-conglomeration, China. The predicted spatial variation of air temperature and relative humidity is evaluated using a high-density automatic weather station network. It is found that the spatial variation is more realistic with CCIv2 than CCI. A method is presented for calculating the indoor and outdoor Wet Bulb Globe Temperature (WBGT) heat stress index, and the benefits of mapping human extreme heat exposure using O(100 m) horizontal grid length versus typical O(1 km) horizontal grid length NWP are assessed.


AS05-A003
Quantifying the Benefits of BIPV Windows in Urban Environment Under Climate Change: A Comparison of Three Chinese Cities

Liutao CHEN#+, Jiachuan YANG
The Hong Kong University of Science and Technology

To increase renewable energy capacity, China has promoted solar technologies with a 14% annual growth rate and kept the solar PV market leadership in 2021. In the urban environment, the building-integrated photovoltaic (BIPV) window is an effective way to increase distributed PV capacity. Due to the lack of modelling tools, the impact of the BIPV windows in the street canyon is poorly understood. To fill the gap, we developed a new parameterization scheme for the BIPV window and incorporated it into building energy simulations coupled with a single-layer urban canyon model. Model evaluation suggests that the coupled model can reasonably capture the diurnal profiles of BIPV window temperature and power generation, building cooling load, and outdoor microclimate. Canyon aspect ratio, window coverage, façade orientation, and power generation efficiency are the most critical factors in maximizing the power generation of BIPV windows. Simulation results of an office floor in three Chinese cities under different climate backgrounds show that Beijing has the greatest solar potential in the south orientation for annual power generation (i.e., 44.7 kWh/(m2·yr)), which is 1.5 times the power generation in Shenzhen and Nanjing. Compared to the clear windows, the BIPV windows have positive benefits when window coverage is greater than 50% in the open canyon. The highest electricity saving ratios are all greater than 23% when southwest-facing façade is 100% covered by BIPV windows. The benefit of BIPV windows is larger in Beijing, followed by Shenzhen and Nanjing. Under the future climate forcing of the year 2050, compared to clear windows, the energy saving potentials of BIPV windows increase slightly in Nanjing, and remain relatively stable in Shenzhen and Beijing. The findings in this study provide guidance for BIPV application in the built environment and cast light on the construction of sustainable and low-carbon neighbourhoods


AS05-A021
WRF-Chem Modelling of CO2 Transport in St. Petersburg Megacity

Georgy NEROBELOV1#+, Yuri TIMOFEEV2, Sergei SMYSHLYAEV3, Stephany FOKA2
1O3Lab, Saint-Petersburg State University, 2Saint-Petersburg State University, 3Russian State Hydrometeorological University

An increase of CO2 content in the atmosphere, caused by anthropogenic emissions from the territories of large cities (~70%), determines the topicality of accurate emission estimation. Advanced experiment-based methods of the CO2 anthropogenic emission estimation are based on the solution of an inverse problem using highly-accurate measurements of CO2 content and numerical models of atmospheric transport and chemistry. The accuracy of such models greatly determines errors of the emission estimations. The aim of the current study is to adapt numerical weather prediction and atmospheric chemistry model WRF-Chem and validate its capability to simulate atmospheric CO2 over the Russian megacity of St. Petersburg. The research has demonstrated that the WRF-Chem model simulates well seasonal and diurnal cycles of CO2 content which are due to CO2 emission and absorption by plants. Correlation between the modelled and measured CO2 content time serieses is high both in a surface layer (correlation coefficient or CC is ~0.73) and in total atmospheric column up to ~75 km (XCO2, CC is ~0.95). Error of XCO2 modelling in relation to ground-based Bruker EM27/SUN measurements in St. Petersburg constitutes about 0.3% and probably is related to inaccuracies in chemical boundary conditions and atmospheric transport simulation during specific meteorological conditions (low wind speed and weak turbulent mixing). According to the results of the research, WRF-Chem model can be used to estimate anthropogenic CO2 emissions from the territory of St. Petersburg. The study was performed at the 'Laboratory for the Research of the Ozone Layer and the Upper Atmosphere' of Saint Petersburg State University and was funded by the Government of the Russian Federation under an agreement [075-15-2021-583].


AS05-A022
Estimation of Anthropogenic CO2 Emissions of St. Petersburg Megacity by Different Methods

Yuri TIMOFEEV1, Georgy NEROBELOV2#+, Anatolii POBEROVSKII1
1Saint-Petersburg State University, 2O3Lab, Saint-Petersburg State University

Increase of greenhouse gases (GHGs) content in the Earth atmosphere changes the planet`s radiation balance and causes climate changes. Anthropogenic emissions of such GHG as CO2 from the territories of large cities play an important role in the climate changes since the cities contribute up to 70% to the total CO2 anthropogenic emissions. Different methods of CO2 emissions estimation have been developed which are based on proxy data (fossil fuel consumption, locations of power plants, nighttime lights, etc.) and observations of CO2 atmospheric content (ground-based, satellite, aircraft, etc.). Lately, authorities of many countries have made a commitment to reduce anthropogenic emissions of CO2 and other GHGs. Therefore, it is important to control undertaken agreements by carrying out independent monitoring of anthropogenic emissions using state-of-the art methods. For instance, there are several working and scheduled satellite observation programmes which were developed specifically to monitor GHGs emissions with relatively high spatial resolution (several km). In addition, today CO2 emission estimation techniques based on inversion modelling are actively investigated and improved. In the last years CO2 anthropogenic emissions of Russian megacity St. Petersburg have been estimated by inventory and experimental methods. In the current study CO2 anthropogenic emissions of St.Petersburg by different methods are compared and results of the comparison will be presented. The study was performed at the 'Laboratory for the Research of the Ozone Layer and the Upper Atmosphere' of Saint Petersburg State University and was funded by the Government of the Russian
Federation under agreement [075-15-2021-583]


AS05-A008
An Ethical Framework for Climate Intervention Research and Potential Scaling

Mark SHIMAMOTO#+, Billy WILLIAMS, Janice LACHANCE, Brooks HANSON
American Geophysical Union

Geosciences in Asia and Oceania are on the frontlines of the climate crisis. While governments and organizations race to organize actions, scientific organizations and technology ventures are taking matters in their own hands, devoting attention and resources to climate intervention research often being proposed with large scale testing in the Asia and Oceania region. This presentation will present the preliminary efforts of the American Geophysical Union (AGU) and a proposed Ethical Framework for Climate Intervention. The Framework is designed to guide governments, researchers, NGOs, and the private sector. The presentation will discuss an understanding of the benefits and impacts of climate intervention measures, including carbon dioxide removal and solar radiation management, and the need for global transparency, ethical and inclusion practices and robust governance and oversight structures. 


Thu-03 Aug | 10:20 - 12:20 | MR331
AS01 - The Asian Monsoon, Extremes and Climate Change

Session Chair(s): Renguang WU, Zhejiang University, Kyung-Ja HA, Pusan National University, Ramesh KRIPALANI, Indian Institute of Tropical Meteorology

AS01-A051
Dynamics and Characteristics of Dry and Moist Heatwaves Over East Asia

Ye-Won SEO1+, Kyung-Ja HA2#, Ji-Hye YEO2, Axel TIMMERMANN2, Eui-Seok CHUNG3, Christian FRANZKE2, Johnny CHAN4,5, Sang-Wook YEH6, Mingfang TING7
1IBS Center for Climate Physics, 2Pusan National University, 3Korea Polar Research Institute, 4Asia-Pacific Typhoon Collaborative Research Center, 5City University of Hong Kong, 6Hanyang University, 7Columbia University

The increasing frequency of heatwaves over East Asia (EA) is impacting agriculture, water management, and people’s livelihood. Recently, record-breaking extreme heat events occurred corresponding to severe drought. However, the effect of humidity on high-temperature events has not yet been fully explored. Thus, distinguishing the compound heatwave associated with humidity conditions is needed to understand the fundamental features of compound extreme heat events and their physical mechanisms and to assess future projections. Using observations and future climate change projections conducted with the latest generation of Earth System models, we examine the mechanisms of dry and moist heatwaves over EA. Compound heatwaves are described by simultaneously with relative humidity conditions over East Asia. Dry heatwaves have been increased over northern East Asia adjacent to the desert regions. In the dry heatwave region, anticyclonic circulation has been amplified after the onset of heatwaves under the influence of the convergence of anomalous wave activity flux over northern EA, resulting in surface warming via adiabatic processes. In contrast, the moist heatwaves are triggered by the locally generated anticyclonic anomalies, with the surface warming amplified by cloud and water vapor feedback. Model simulations from phase six of the Coupled Model Intercomparison Project projected display intensification of dry heatwaves and increased moist heatwave days in response to projected increases in greenhouse gas concentrations.


AS01-A104
Impact of Heat Stress on the People Working in the Coastal Cities of India Due to Climate Change

Lakshmi Kumar T.V.1#+, Bharath J1, Walter LEAL2, Humberto BARBOSA3, Koteswararao KUNDETI4
1SRM Institute of Science and Technology, 2Hamburg University of Applied Sciences, 3Universidade Federal da Alagoes, 4National Center of Meteorology

The physiological stress in the working environment due to the increased levels of heat stress during climate change is an important point of research in the Indian scenario. The increase in heat stress obtained from the Steadman Heat Stress Index (SHSI) and its associated decline in work performance (DWP) are reported in this study using: a) the reanalysis data sets of the Indian Monsoon Data Assimilation and Analysis (IMDAA) for the period 1981 to 2020; and b) the high resolution, bias-corrected simulations of the Indian Institute of Tropical Meteorology (IITM) – Earth System Model (ESM) (source: NEX GDDP) for the period 1981 to 2014 (historical) and 2015 to 2050 (Shared Socioeconomic Pathway (SSP) 2.4.5 & 5.8.5) for the coastal cities of India. A lookup table has been prepared with the SHSI values for the equivalent Wet Bulb Globe Temperature (WBGT), which recommend different rest/work ratios for all the study locations. The results show that the rising heat stress is mainly dependent on the changes in relative humidity in the cities of the west coast, while it is dependent on temperature changes in the cities of the east coast. The cities of Chennai, Nellore, Puducherry and Kochi showed a higher decline in work performance in the SSP2.4.5 scenario, while Mangalore and Thiruvananthapuram have been added in the SSP5.8.5 scenario during the decade of 2041 to 2050. People working without thermal neutralities in Chennai, Nellore, Puducherry and Kochi were recommended a 25% increase of more rest per hour in the light, medium, heavy and very heavy work conditions during the future climate scenarios of 2021 to 2050.


AS01-A085
Prediction Skill of WRF-ROMS in Ensemble Forecasting with Different Microphysics Parametrizations: A Sensitivity Analysis of Rainfall Prediction in Thailand Related to Tropical Storm Events in 2020

Apiwat FAIKRUA+, Kritanai TORSRI#, Pattarapoom PEANGTA, Rati SAWANGWATTANAPHAIBUN , Thippawan THODSAN, Kanoksri SARINNAPAKORN
Ministry of Higher Education, Science, Research and Innovation

Tropical storm (TS) usually brings heavy rainfall in Thailand, especially during rainy season, which can cause significant damage to coastal areas, cities, and communities in the region. Improving rainfall forecasting during TS occurrence is, therefore, critical to reducing the negative impacts of TS and increasing community safety. Many studies indicated that rainfall prediction skill of a numerical weather prediction model was strongly dependent on cumulus (CU) and microphysics (MP) parameterizations. Because microphysical processes play a crucial role in formation and development of rainfall, accurately representing these processes is important for accurate weather forecasting. In this study, a sensitivity analysis of rainfall forecasts from an ensemble method using a coupled WRF-ROMS model with three different MPs (i.e., Eta, Lin, and WRF Single Moment 3) was conducted. Here, we focused on the impact of MP on rainfall forecasts, hence only a CU scheme was used. Seven extreme rainfall events in Thailand associated with TS in 2020 were selected for a three-day model integration, then the probability of detection (POD) was estimated by comparing the forecasted outputs with daily observations of the National Hydroinformatics Data Center. Overall, employing the ensemble method could yield better POD in capturing moderate (10.1-35.0 mm) and heavy (35.1-90.0 mm) rainfall by up to 8% and 15% (in relative to a single MP run). This work is a preliminary study to show the potential of an ensemble method on rainfall forecast in Thailand. However, the CU selected in WRF can have a significant impact on accuracy and realism of the weather forecast. Therefore, careful consideration of CU and MP combination is subject to further investigation to ensure that the model provides the best possible representation of atmospheric processes and similar rainfall pattern over Thailand.


AS01-A099
Interannual Variation and Prediction of Wintertime Precipitation in Central Asia

Xinhai CHEN#+, Xiaojing JIA
Zhejiang University

In this study, the interannual variations of winter precipitation over central Asia (CA) are investigated over the period 1948–2018 using both observational analysis and a linear baroclinic model (LBM). The focus is on the characteristics and factors of the leading empirical orthogonal function mode (EOF1) of winter precipitation over CA. The results show that the key circulation anomalies associated with the positive phase of EOF1 feature a tripole pattern that is responsible for transporting moisture from the subtropical North Atlantic region to CA. An examination of the lower boundary conditions indicates that anomalous North Atlantic sea surface temperature (SST), Kara Sea ice in the preceding autumn, and simultaneous snow cover in central Asia can promote large-scale atmospheric waves that contribute to the EOF1-related anomalous tripole pattern. This result is verified by an analysis of the apparent heat source (Q1) in the atmosphere and the LBM experiments. Linear regression (LR) models were constructed using the precursors revealed by the above observational analyses to perform hindcasts for EOF1 over the period 1950–2018. The North Atlantic SST and the Kara Sea ice in the preceding autumn are shown to be effective predictors in the LR model that can capture the variation in EOF1 during this period. The seasonal forecasts of winter precipitation over CA for the 2011–18 period based on the LR models outperform those of the Climate Forecast System version 2 (CFSv2) over central and northern CA.


AS01-A106
Intraseasonal Variability of the East Asian Subtropical Westerly Jet: Characteristics, Mechanisms and Impacts on Extremes

Jiacan YUAN#+
Fudan University

The East Asian subtropical westerly jet (EASWJ) is one of the most crucial subtropical circulation systems affecting the precipitation over East Asia. Here we investigate the dominant modes of the intraseasonal variability of the EASWJ in early (May and June) and late (July and August) summer, respectively, through the EOF analysis. The EOF1 in early summer is characterized by the anomalous westerlies centered over the North China and anomalous easterlies centered over the south of Japan. This mode is led by the south-eastward propagating wave train initiating from the Barents Sea, where the ridge of the wave train coincides with an anomalous warm advection in the low level, due to the negative phase of Arctic Dipole (AD). The EOF1 in late summer is characterized by the anomalous westerlies centered over the south of Baikal and anomalous easterlies centered over the Central China, which is affected by the two wave trains along different directions. One propagates zonally across Eurasia initiated from North Atlantic, where significant signal of East Atlantic (EA) teleconnection is found as a precursor. When the wave train disperses downstream to Eurasia, the EAWR play a dominant role on the growth and persistence of the EASWJ variability. The other one is similar to the East Asia–Pacific (EAP) teleconnection propagating poleward from the Southern Asia and Western North Pacific, where the active convection anomalies may be a key driver. In addition, the different patterns of the EASWJ from early to late summer may cause different patterns of weather extremes of China through driving the anomalous vertical motion and water vapor transport over the corresponding areas.


AS01-A110
Dynamical Processes Controlling the Evolution of Early‐summer Cut‐off Lows in Northeast Asia

Yang ZHANG1#+, Yu NIE2
1Nanjing University, 2China Meteorological Administration

The Northeast Asian cut-off low is one of the important extratropical circulations in East Asian monsoon systems that can bring weather extremes over large areas, but the mechanism responsible for the life cycle of cut-off lows remains elusive. From a perspective of regional eddy-mean flow interaction, this study investigates the dynamical processes controlling the evolution of early-summer cut-off lows over Northeast Asia using the 6-hourly reanalysis data. Through the diagnostic of local wave activity (LWA) budget, we show that the cut-off low is initialized by a Rossby wave train originated from the subpolar North Atlantic, and then reinforced rapidly by zonal LWA flux convergence and local baroclinic eddy generation, and eventually decayed through energy dispersion by zonal wave activity advection. Furthermore, we show that the evolutions of the above dynamical processes are strongly modulated by the changes of background flow. In early summer, Northeast Asia is located at the eastern exit of the midlatitude jet to the north of the sub- tropical jet and exhibits a weak meridional gradient of potential vorticity, which favors frequent formation of cyclonic anomaly and energy accumulation. Prior to the onset of cut-off lows by several days, a Rossby wave train propagates along the Eurasian midlatitude jet, which initializes a cyclonic anomaly over Northeast Asia. With the aid of mean flow advection of anomalous zonal momentum, the zonal winds are then decelerated at the midlatitude jet exit and accelerated at the subtropical jet center. The former obstructs the wave packet proceeding downstream and the latter favors stronger baroclinic eddy generation below the subtropical jet. The two processes together maintain and strengthen the cyclonic anomaly in Northeast Asia rapidly.


AS01-A107
Changes in the Frequency of Extreme Summer Temperatures Over India in Current and Future Climate Scenarios

China Satyanarayana GUBBALA#+, V. SAMBASIVARAO, Dodla V. B. RAO
K L Deemed to be University

In the 21st century, climate change is considered to impose the greatest environmental threats to the world. Associated changes in climate extremes are hypothesized to have greater negative impacts on human society and the natural environment than the changes in mean climate. In this context, an assessment of temperature extremes is made for the Indian subcontinent to identify the changes since 1951 to 2022, and for the future climate periods till 2100. The frequencies of the days having thresholds of 40C, 42C and 45C for the maximum temperature over India during the pre-monsoon are evaluated using the grid‐point maximum temperature data of India Meteorological Department [IMD] for the period 1951–2022. Corresponding temperature predictions from Coupled Model Intercomparison Projects Phase 6 (CMIP-6 ) model outputs and statistical downscaling model (SDSM) methodology were compared with the IMD gridded maximum temperature data for validation. Statistical metrics of BIAS, RMSE and MAE have indicated low BIAS, high correlation and high IOA (Index of Agreement) validating CMIP-6 climate simulations. Similarly, the model projected maximum temperatures from the future climate projections using the same model for the climate periods of 2021-2050 and 2070-2099 are calculated. The data for the period from 1 March to 31 May, for the each of the two climate periods, are used to characterise the heat waves in future climates. Specifically, the characteristics of heat waves in terms of intensity, duration and area extent are calculated and compared to heat waves of the current climate. An increase in the heat waves duration mean maximum temperatures and frequencies of heat wave days in future climate periods have been identified.


AS01-A081
Recent Changes in Indian Summer Monsoon Core Region’s Precipitation Extremes

Raju ATTADA1#+, Bajrang C1, B. N. GOSWAMI2
1Indian Institute of Science Education and Research Mohali, 2Cotton University

Understanding and predicting the behavior of precipitation extremes in the tropics have often been associated with uncertainty. The responses of precipitation extremes to climate change are largely thought to be codirectional, especially in the Indian Summer Monsoon region. In this work, we show the short-term declination of temporal frequency of monsoonal precipitation extremes over Central India, for the last 15 years starting from 2005 to 2020, with the low and moderate events showing increments. The possible dynamical factors for the observed decline in precipitation extremes include the weakening of the regional Hadley Cell, along with depletion in moisture transport to Central India via the low-level Somali jet, caused by reduced evaporation from the regional moisture sources. In addition, the vertical gradient of the moist static energy exhibits favorable conditions for increased lower atmospheric stability, supporting the declining trends. Lastly, the Atlantic Zonal Mode seems to be a potential large-scale climate driver for the less frequent central Indian extreme rainfall events during 2005-2015.


Thu-03 Aug | 10:20 - 12:20 | MR332
AS25 - Air Pollution-Weather-Climate Interactions

Session Chair(s): Chenglai WU, Chinese Academy of Sciences, Yang YANG, Nanjing University of Information Science and Technology, Guangxing LIN, Chinese Academy of Sciences

AS25-A026
Evolution of Ozone Production Sensitivity Over the Greater Bay Area of China Under the Backdrop of Climate Change

Zibing YUAN1#+, Alexis LAU2, Yi DU1
1South China University of Technology, 2The Hong Kong University of Science and Technology

China is experiencing worsening tropospheric ozone pollution in the past decade, and the ozone pollution may continue deteriorating under the backdrop of climate change. Ozone Production Sensitivity (OPS) provides essential information for developing ozone control strategy. In this regard, it is crucial to understand the evolution of OPS under different climate change scenarios. Given that there is a large gap between representative concentration pathways (RCP) scenarios and the actual pollutants emission for China during 2010-2020, this study proposed an adjustment method based on the latest 2020 Multi-resolution Emissions Inventory for China (MEIC) emission inventory to constrain the climate scenarios. Based on the emissions from the four adjusted RCP scenarios data and the meteorology data from Community Earth System Model (CESM) output, we investigated the long-term evolution of OPS over the Greater Bay Area (GBA) of China each decade from 2030 to 2050. We found that ozone concentration showed a gradual decline trend under RCP2.6, RCP4.5, and RCP8.5 scenarios, while it continued to rise under RCP6.0 scenario. The close relationship between OPS and the atmospheric oxidative capacity based HO2/OH indicator can more accurately depict OPS and its variations. A VOCs-limited regime is expected to extend under RCP6.0, while NOx-limited regime was gradually expanded under RCP2.6, RCP4.5, and RCP8.5 scenarios. Under the ‘dual-carbon’ mission, the future emission trend in China is closer to RCP4.5 scenario. Without further strengthening of control measures, ozone concentration in the GBA will steadily drop in 2030. In addition, the OPS transferred to a NOx-limited regime in most parts of the GBA. Overall, this study highlights the importance of NOx deep emission reduction in achieving the ozone pollution standards in the GBA, which provides useful information in the long-term ozone pollution control policy making.


AS25-A017
The Effect of Compound Factors of Meteorology and Emissions on Ozone Pollution

Yang GAO1#+, Mingchen MA1, Feifan YAN1, Wenbin KOU1, Junxi ZHANG2
1Ocean University of China, 2Zhejiang University

Ozone pollution has long been a major concern considering its large impact on human health. The ozone concentrations are substantially affected by both meteorology and emissions. Whereas there are extensive studies investigating the individual role of meteorology and emissions on ozone concentrations, a few major issues remain unclear. For instance, temperature usually plays a positive role on ozone formation, however, water vapor may act as both a stimulator and sink of ozone. The compound effect of temperature and water vapor will be discussed. Considering the nonlinearity of emission precursors on ozone and along with the decrease of anthropogenic emissions, the increase of biogenic emissions in future may play a much larger role in governing the ozone concentrations. The synergic effect of anthropogenic emissions and biogenic emissions will be investigated based on hundreds of numerical experiments. The findings in this study potentially play great roles in understanding the spatial heterogeneity of ozone formation mechanism in various regions.


AS25-A012
Global Trends and Drivers of Biogenic Volatile Organic Compound Emissions Over the Last 2 Decades

Hao WANG1+, Xiaohong LIU2#, Chenglai WU1, Guangxing LIN1
1Chinese Academy of Sciences, 2Texas A&M University

Biogenic volatile organic compounds (BVOCs) are important for producing tropospheric ozone and secondary organic aerosols. The contribution of various factors to the trend in BVOC emissions in different regions over the last 2 decades remains unclear. Here, global changes in BVOC emissions during 2001-2020 are calculated using the latest Model of Emission of Gases and Aerosols from Nature (MEGANv3.2) driven by time-varying satellite-retrieved vegetation and reanalysis meteorology data. We find that an increase in CO2 concentrations has a stronger effect on the trend in global total isoprene emissions (-0.20 % yr-1) than changes in vegetation (-0.03 % yr-1) and meteorological factors (0.15 % yr-1), but with large regional disparities. Isoprene emissions are rising rapidly in Europe, East Asia, and South Asia (0.37-0.66% yr-1), and vegetation growth contributes to about half of these trends. Changes in meteorological factors accounts for remaining half, with elevated temperature dominating in Europe and increased soil moisture dominating in East and South Asia. In South America and Southeast Asia, shifts in vegetation type associated with the BVOC emission capacity, partly resulting from the deforestation and agricultural expansion, lead to a decrease in BVOC emission and offset half of the emission increase caused by meteorological factors. The overall increase in isoprene emission in these regions is 0.35% yr-1 and 0.25% yr-1. In Central Africa, decreasing temperature dominates the negative emission trend (-0.74% yr-1). Global monoterpene emissions show a significant increase (0.34% yr-1, 0.6 Tg yr-1) compared to isoprene (-0.07% yr-1, -0.2 Tg yr-1), especially in strong greening hotspots, mainly due to greater sensitivity to changes in LAI and lack of CO2 inhibition effect. These findings highlight the important roles of vegetation, temperature, and soil moisture in shaping the temporal variations of global BVOC emissions over the last 2 decades.


AS25-A028
Subseasonal Reversal of Haze Pollution Over the North China Plain

Lian XUE#+, Sijia LOU, Xin HUANG, Aijun DING
Nanjing University

China has been frequently suffering from haze pollution in the past several decades. As one of the most emission- intensive regions, the North China Plain (NCP) features severe haze pollution with multiscale variations. Using more than 30 years of visibility measurements and PM2.5 observations, a subseasonal seesaw phenomenon of haze in autumn and early winter over the NCP is revealed in this study. It is found that when September and October are less (more) polluted than the climatology, haze tends to be enhanced (reduced) in November and December. The abrupt turn of anomalous haze is found to be associated with the circulation reversal of regional and large-scale atmospheric circulations. Months with poor air quality exhibit higher relative humidity, lower boundary layer height, lower near-surface wind speed, and southerly anomalies of low-level winds, which are all unfavorable for the vertical and horizontal dispersion and transport of air pollutants, thus leading to enhanced haze pollution over the NCP region on the subseasonal scale. Further exploration indicates that the reversal of circulation patterns is closely connected to the propagation of midlatitude wave trains active on the subseasonal time scale, which is plausibly associated with the East Atlantic/West Russia teleconnection synchronizing with the transition of the North Atlantic SST. The seesaw relation discussed in this paper provides greater insight into the prediction of the multiscale variability of haze, as well as the possibility of efficient short-term mitigation of haze to meet annual air quality targets in North China.


AS25-A016
More Frequent Strong Surface Solar Radiation Conducive to Persistent Ozone Pollution in a Warming Climate

Wenbin KOU#+, Yang GAO, Shaoqing ZHANG
Ocean University of China

Elevated near-surface ozone pollutes many parts of the world, exerting consequential impacts on human health in ozone-prone regions, including eastern China, eastern United States, and Europe. Key meteorological conditions, such as high temperature and downwards surface shortwave radiation (DSSR), intensify ozone pollution, yet how these meteorological conditions or associated mechanisms respond to global warming remains unknown. Taking advantage of 5-year-long daily observations in eastern China over the 2015-2019 period, with an extraordinarily ozone increase in fall 2019 over the Pearl River Delta (PRD), here we show that the 2019 strong DSSR induces extra biogenic emissions that trigger a threefold increase in long-lasting (i.e., five or more days) ozone events; consequently, mean ozone enhancement due to biogenic emissions reaches an average of 20 ppbv, highlighting the dominant role of DSSR. Furthermore, using outputs from a multimodel ensemble and a high-resolution community earth system model, we show an increased frequency of high DSSR under greenhouse warming in ozone-prone regions. Our results indicate that meteorological conditions conducive to high ozone pollution in ozone-prone regions are likely to occur more often under greenhouse warming.


AS25-A001
Impact of Weather Conditions on PM2.5 Variations in Taiwan During the Winter Season 2018-2021

Hsiao-Chen CHIEN+, Fang-Yi CHENG#
National Central University

In addition to anthropogenic emissions, meteorological conditions also play an important role affecting air pollutant dispersion processes. This study focused on the impact of mesoscale to large-scale atmospheric conditions during the winter-spring season (DJFM) of 2018-2020 on PM2.5 concentrations in Taiwan. The analysis of the observation data and WRF-CMAQ modeling was conducted. The objectives are to gain a deeper understanding of the connections between the meteorological conditions and air quality. The analysis of the surface observed PM2.5 revealed a degraded PM2.5 condition in February and March of 2021. The winter-spring seasons in 2018/19, 2019/20, and 2020/21 were affected by El Nino, neutral and La Nina, respectively. In February and March of 2021, the cyclonic anomaly was found in area of Taiwan which leads to the frequent occurrence of the easterly prevailing wind. The weaker wind speed, cooler temperature and enhanced atmospheric stability, lead to the accumulation of PM2.5 in western Taiwan due to the influence of the La Nina conditions. Besides, the enhanced long-range transported PM2.5 contributed from other countries in East Asia can increase the background concentration.


AS25-A014
Co-benefits of China’s ‘Dual-Carbon’ Policies on Ozone Pollution Mitigation in the Guangdong-Hong Kong-Macao Greater Bay Area: A Multi-model Simulation Study

Danyang LI#+, Lin ZHANG, Xiaorui LIU, Chaoyi GUO, Kai WU, Hancheng DAI
Peking University

As the leading region in air pollution prevention and control initiatives in China, the Guangdong-Hong Kong-Macao Greater Bay Area (GBA) has witnessed marked decrease in PM2.5 pollution. Despite this progress, surface ozone levels continue to increase, highlighting the limitation of current emission reduction measures in ozone pollution control and the complexity of ozone pollution changes under emission reduction scenarios. To address this challenge, this study projects the evolutions of anthropogenic emissions and regional ozone pollution from 2015 (base year) to 2050 over GBA in the context of China’s "dual-carbon" target, by softly coupling an energy-economy model IMED|CGE (Integrated Model of Energy, Environment, and Economy for Sustainable Development, Computable General Equilibrium) with an atmospheric chemistry transport model WRF-Chem. We consider low-carbon policies and different levels of end-of-pipe control policies and obtain three emission reduction pathways under different scenarios for the GBA, according to which, ozone concentration pathways are simulated, with a specific focus on ozone pollution in October when surface ozone concentrations exhibit a seasonal peak. The results demonstrate that the implementation of deep emission reductions, driven by a combination of climate mitigation policies and local clean air policies, could significantly reduce MDA8 surface ozone levels to below 90 μg m-3 by 2050. Our findings also suggest that while low-carbon policies will bring substantial air quality co-benefits, strict end-of-pipe control policies are essential for rapidly reducing ozone pollution prior to 2030 and achieving national ozone level standards in the long term. As indicated by the H2O2/HNO3 concentration ratios, ozone production will become increasingly sensitive to NOx levels, primarily due to sharp reductions in anthropogenic NOx emissions. In conclusion, controlling NMVOCs emissions in the short term and NOx emissions in the long term are imperative for effectively mitigating surface ozone air pollution in the GBA.


Thu-03 Aug | 1:10 - 3:10 | MR311
AS40 - Middle Atmosphere

Session Chair(s): Hye-Yeong CHUN, Yonsei University, Shigeo YODEN, Kyoto University

AS40-A013 | Invited
Role of Tropical Lower Stratosphere Winds in Quasi-biennial Oscillation Disruptions and its Implications for Future Climate

Min-Jee KANG1#+, Seok-Woo SON1, Rolando GARCIA2, Soon-Il AN3, Sang-Hun PARK3
1Seoul National University, 2National Center for Atmospheric Research, 3Yonsei University

In winter 2015/16, the westerly quasi-biennial oscillation (WQBO) in the equatorial stratosphere was unprecedentedly disrupted by westward forcing near 40 hPa; this was followed by another disruption in 2019/20. Strong extratropical Rossby waves propagating toward the tropics were considered the main cause of the disruptions. However, it remains unclear why the zonal wind is reversed only in the middle of the WQBO. Here, we show that strong westerly winds in the equatorial lower stratosphere (70 to 100 hPa) help to disrupt the WQBO by preventing the wind reversal at its base. These winds also help equatorial westward waves propagate further upward, increasing the negative forcing at around 40 hPa that drives the QBO disruptions. Tropical westerly winds have been increasing and are projected to increase in a warmer climate. These background wind changes may allow more frequent QBO disruptions in the future, leading to less predictability in atmospheric weather and climate systems related to the QBO. They may also induce a faster propagation rate of a typical QBO due to the enhanced westward wave flux entering the stratosphere. Therefore, a comprehensive understanding of the future behavior of the QBO will require consideration of the strengthened westerlies in the lowermost stratosphere in addition to the changes in wave sources and tropical upwelling in the stratosphere.


AS40-A014
A Comparison of Stratospheric Gravity Waves in a High-resolution General Circulation Model with 3-D Satellite Observations

Haruka OKUI1#+, Corwin WRIGHT2, Neil HINDLEY2, Emily LEAR2, Kaoru SATO1
1The University of Tokyo, 2University of Bath

Atmospheric gravity waves (GWs) play a key role in determining the thermodynamical structure of the Earth’s middle atmosphere. Despite the small spatial and temporal scales of these waves, a few high-top general circulation models (GCMs) that can resolve them explicitly have recently become available. This study compares global GW characteristics simulated in one such GCM, the Japanese Atmospheric GCM for Upper-Atmosphere Research (JAGUAR), with those derived from three-dimensional (3-D) temperatures observed by the Atmospheric Infrared Sounder (AIRS) aboard NASA’s Aqua satellite. The target period is from 15 December 2018 to 8 January 2019, including the onset of a major sudden stratospheric warming (SSW). The 3-D Stockwell transform method is used for GW spectral analysis. The amplitudes and momentum fluxes of GWs in JAGUAR are generally in good quantitative agreement with those in the AIRS observations in both magnitude and distribution. As the SSW event progressed, the GW amplitudes and eastward momentum flux increased at low latitudes in the summer hemisphere in both the model and observation datasets. Case studies demonstrate that the model is able to reproduce comparable wave events to those in the AIRS observations with some differences, especially noticeable at low latitudes in the summer hemisphere. Through a comparison between the model results with and without the AIRS observational filter applied, it is suggested that the amplitudes of GWs near the exits of the winter jet are underestimated in AIRS observations.


AS40-A016
Numerical Simulation of Changes in the General Circulation of the Middle and Upper Atmosphere During Transitional QBO Phases

Andrey KOVAL#+, Tatiana ERMAKOVA, Kseniia DIDENKO, Nikolai GAVRILOV
St Petersburg University

Three-dimensional numerical nonlinear model of general circulation of the middle and upper atmosphere (MUAM) is used to investigate reactions of the atmospheric dynamic and thermal regimes on changes in four phases of equatorial stratospheric quasi-biennial oscillation (QBO). In addition to conventional westerly and easterly QBO phases, transitional westerly-shear and easterly-shear QBO phases are added into consideration. The MUAM model allows simulating atmospheric circulation from the Earth's surface to a height of 300 km. This made it possible to consider the dynamic response of the thermosphere to the change in the QBO phase. To interpret the obtained results, the residual meridional circulation, Eliassen-Palm fluxes and meridional thermal gradients are calculated. For this purpose, four 12-members ensembles of MUAM simulations have been obtained corresponding to the mentioned four QBO phases. It is shown in particularly, that at the middle and high latitudes, the strongest changes in thermal and dynamical characteristics of the stratosphere and mesosphere occur during easterly-shear QBO phase. The formation of the temperature regime in the winter extratropical stratosphere is predominantly influenced by the residual meridional circulation during easterly and westerly-shear QBO phases and by planetary waves during westerly and easterly-shear QBO phases. The research is supported by the Ministry of Science and Higher Education of the Russian Federation (Agreement 075-15-2021-583).


AS40-A007
Sea-land-breeze Bidirectional Gravity Waves Robustizing Stratospheric QBO: JRA-55 Data Analysis

Manabu D. YAMANAKA1,2#+, Shin-Ya OGINO3
1Research Institute for Humanity and Nature, 2Kobe University, 3Japan Agency for Marine-Earth Science and Technology

The quasi-biennial oscillation (QBO) appearing robustly in the equatorial stratosphere has been explained by the wave-mean flow interaction. However, requested bidirectional (east/westward propagating) waves generated in the troposphere have not been ascertained yet. The strongest thermal forcing on the equatorial lands with diurnal cycle (DC) drives the sea-land breeze circulations (SLBCs) centered at the Indonesian maritime continent (IMC) with the longest coastline, next at African and South-American continents, which organize convective clouds making atmospheric energy equilibrium and water cold trap. Here we analyze objective re-analysis data (JRA-55), and reveal that SLBCs are the bidirectional (land- and sea-ward) waves maintaining QBO. The pressure coordinate and velocity data are converted to quasi-vertical (log-pressure) ones, and zonal and vertical wind deviations from each diurnal means are regarded as diurnal wave components, based on comparisons with some radiosonde data over IMC. The global diurnal tides, which make ocean-side variations much weaker than land-side ones, are omitted by a longitudinally 30°-high passed filter. For resulting bidirectional gravity waves, the zonal-mean vertical flux of zonal momentum are calculated, which should be conserved vertically without nonlinear and dissipation effects. We obtain that the zonal momentum associated with components propagating in the same direction as the stratospheric mean flow is selectively absorbed to produce directly about 30% of the mean zonal acceleration of QBO. The momentum absorbed locally may generate also longer waves contributing to the remainder of zonal acceleration. Because of “pair production” the bidirectional wave momenta are equi-amplitude, determined with land-sea contrast, and their zonal components are dependent on the angle between a coastline and the meridian. Therefore, QBO is dependent on the distribution of coastline as the triple boundary among land, sea and air, which are changed with tectonics and climate.


AS40-A003 | Invited
Strengthened Impact of the Equatorial Quasi-biennial Oscillation on the Extratropics in Both Hemispheres

Jian RAO1#+, Chaim GARFINKEL2, Tongwen WU3, Rongcai REN4
1Nanjing University of Information Science & Technology, 2Hebrew University of Jerusalem, 3China Meteorological Administration, 4Chinese Academy of Sciences

Using state-of-the-art models with a spontaneous quasi-biennial oscillation (QBO) from the Coupled Model Intercomparison Project Phases 5 and 6 (CMIP5/6), this study explores projected changes in the Holton-Tan (HT) relationship and the near surface response to the QBO. Most models project an enhanced surface response to the QBO via a strengthened HT relationship in the future for both hemispheres. In the Northern Hemisphere, the North Atlantic Oscillation-like response is projected to double and shift eastward in the future in the high-end emissions scenarios compared with the historical simulation. This strengthening occurs even as the amplitude of the QBO in the tropical stratosphere weakens from the historical simulation to the future projections. The seemingly contradictory projections of future changes in the QBO and the HT relationship might imply that the HT relationship changes nonlinearly with the QBO intensity, and the coherent changes in the background circulation structure should also be highlighted. In the Southern Hemisphere, The maximum wind anomaly center in high latitudes is projected to expand to midlatitudes in future scenarios. The climatological subtropical jet is projected to strengthen, while tropical easterlies are projected to weaken. As a consequence, upward wave activity in the future appears to become more sensitive to the QBO phase. Enhanced upward propagation of waves in mid-to-high latitudes during EQBO are much stronger in future scenarios than in historical simulations. In future scenarios, the reduction in OLR during EQBO over the Maritime Continent grows in extent and becomes stronger. The enhancement and spatial shift in the stratospheric vortex pathway and tropical convection pathway subsequently lead to changes in the tropospheric QBO signal. An annular mode like response forms in the troposphere and near surface in the present climate, whereas this pattern shifts further equatorward in future projections with circulation anomalies in the tropical Indian Ocean amplifying.


AS40-A018
Influences of the Equatorial Quasi-Biennial Oscillation on Regional Monsoon Systems in the Northern Subtropics in Summer and Winter

Shigeo YODEN1#+, Vinay KUMAR2, Matthew HITCHMAN3
1Kyoto University, 2University of Delhi, 3University of Wisconsin-Madison

Recently it has been observationally studied that the equatorial QBO in the stratosphere influences tropospheric variations in the form of organized moist convective systems associated with the MJO and the ENSO in sub-seasonal and inter-annual time scales, respectively. In addition, QBO modulation of the global monsoon systems, i.e., annual cycle response of land-ocean systems in low-latitudes to the periodic solar forcing, was reported recently in specific phases of the QBO, in the equator and subtropics (Yoden et al. 2023). By analyzing only neutral ENSO periods of 42 years of ERA-5 data, we further investigate the QBO modulations of boreal summer or winter circulations in synoptic scales with organized precipitation systems. We apply the composite difference analysis introduced by Kumar et al. (2021) using eight QBO phases based on the EOF method of Wallace et al. (1993): The composite difference between Phase 1 – Phase 5 has the largest difference of the equatorial zonally symmetric wind at 20 hPa, whereas that between Phase 4 – Phase 8 has a local maximum difference of the zonally symmetric wind at 50 hPa. In boreal summer, precipitation, its proxy data of OLR and specific humidity, and the lower tropospheric circulation fields show statistically significant composite differences between Phase 4 – Phase 8 QBO phases in the Western Pacific northern subtropics, with an intensification of the west side of Ogasawara high with less precipitation in Phase 8. In boreal winter, on the other hand, statistically significant composite differences are observed in such quantities between Phase 4 – Phase 8 with an intensification of Atlantic low in North Atlantic in Phase 8. There are also statistically significant composite differences between Phase 1 – Phase 5 over the Eastern Pacific northern subtropics. The relative importance of the subtropical and extratropical pathways is studied for these two areas with different QBO phases.


AS40-A011
Troposphere-stratosphere Interaction During Different ENSO and PDO Phases in Idealized Model Experiments

Yulia ZYULYAEVA1#+, Daria SOBAEVA2
1Shirshov Institute of Oceanology, 2Moscow Institute of Physics and Technology

Large-scale sea surface temperature anomalies (SSTA) 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 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. 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.


AS40-A012
Dynamical Response of Arctic Stratospheric Polar Vortex to ENSO and PDO Sea Surface Temperature Anomalies in Idealized Modeling

Daria SOBAEVA1#+, Yulia ZYULYAEVA2
1Moscow Institute of Physics and Technology, 2Shirshov Institute of Oceanology

Currently, the intensity of the stratospheric polar vortex (iSPV) is predicted no more 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 (PDO), extend the period of stratospheric dynamics’ prediction. In this work, the response of iSPV anomalies to large-scale SSTAs is estimated using idealized modeling on ISCA platform. In these experiments SSTAs corresponding to ENSO and PDO modes were increased compared to the observed values. It is shown that SSTAs in the mid-latitudes of the Pacific Ocean on their own do not significantly influence the formation of iSPV. With positive SST anomalies in the Niño-3 region (CEN), a weakening of the polar vortex by 40% is observed compared to the control experiment. The weakening of the vortex with positive SSTAs in the central part of the tropical Pacific Ocean (ENM) is comparable to the effect of the CEN, the difference is observed during late autumn and early spring. Negative SSTAs which represent La Niña (LN) phase correspond to a weakening of the vortex by no more than 20%. The positive PDO phase significantly increases the weakening of iSPV during El Niño events, while the negative phase of the PDO decreases the effect of CEN. The LN effect is weakened by both PDO phases. An analysis of the large-scale pressure field structure in the middle troposphere showed that CEN leads to increased PNA pattern, and during LN, the spatial structure of pressure anomalies corresponds to an increase in the AO. In contrast to some recent studies, it is shown that the pressure field response in the middle troposphere to ENM is similar to the response to CEN. This study proposes the mechanisms for the formation of these observed anomalies.


Thu-03 Aug | 1:10 - 3:10 | MR323
AS42 - Weather Radar Networks And Their Applications For High-Impact Weather Observations and Warnings

Session Chair(s): Ben Jong-Dao JOU, National Taiwan University, Taro SHINODA, Nagoya University

AS42-A023
Airborne Phased Array Radar (APAR): The Next Generation of Airborne Polarimetric Doppler Weather Radar

Everette JOSEPH1, Wen-Chau LEE2#+, Scott MCINTOSH1, Krista LAURSEN1, Angela RICHARDSON1
1National Center for Atmospheric Research, 2UCAR

This paper presents a configuration of a novel, airborne phased array radar (APAR) motivated by major advances in cellular technology, component miniaturization, and radar antenna simulation software. This has paved the way for a next-generation radar being designed by NCAR/EOL to be installed on the NSF/NCAR C-130 aircraft. 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. Polarimetric measurements are not available from current airborne tail Doppler radars. However, APAR, with dual-Doppler and dual polarization diversity at a lesser attenuating C-band wavelength, will further advance the understanding of the microphysical processes within a variety of precipitation systems. Such unprecedented observations, in conjunction with the advanced radar data assimilation schema, will be able to address the key science questions to improve understanding and predictability of significant weather.A Mid-scale Research Infrastructure proposal is submitted to the National Science Foundation to request the implementation cost. The development is expected to take ~5 years after the funding is in place. It adopts a phased approach as an active risk assessment and mitigation strategy. At the present time, both the National Science Foundation and the NOAA are funding the APAR project for risk reduction activities. 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 review the overall design and current progress of APAR and outline ambitious future development work needed to bring this exceptional tool into full operation.


AS42-A020
The Airborne Phased Array Radar (APAR) Observing Simulator (AOS)

Wen-Chau LEE1#+, Bradley KLOTZ2, Jothiram VIVEKANANDAN2
1UCAR, 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. Given the technological advancements that have occurred recently, the creation of end-to-end observing system simulators provides an opportunity to investigate the observing capabilities and limitations of instruments and reduce some of the risks associated with the performance of instrument development. This work aims to describe such a scenario for the Airborne Phased Array Radar (APAR). 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 current work is the first of a two-part paper, where the first part describes the prototype version of AOS, including its design and functionality along with some initial APAR performance metrics related to a 3-D wind analysis. The second paper will focus on a more detailed analysis of the 3-D winds and dual-polarization products to showcase the usefulness of the AOS for generating reliable scientific products. The contents herein are presented in such a way as to provide insight into simulating APAR and to present a methodology for future simulation of radar observations.


AS42-A001
Explainable AI for Polarimetric Radar Rainfall Mapping

Haonan CHEN#+
Colorado State University

Polarimetric radar-based rainfall estimates are typically derived through empirical parametric relations obtained from nonlinear regression between measured rain rates and simulated radar observables from disdrometer data. The performance of such empirical relations is highly dependent on the sample size and representativeness of the measured raindrop size distribution, which vary in different precipitation regimes or even within a single storm system. Even if one can eliminate all the random errors associated with polarimetric radar measurements, the parameterization error inherent in the empirical relations used to estimate rainfall rate from polarimetric radar measurements is hard to reduce. In addition, it is difficult to estimate surface rain rates with the radar measurements aloft, especially during the precipitation events characterized by varying precipitation microphysics with height. Recent studies have shown that artificial intelligence (AI) is effective in reducing these parameterization errors and improving the accuracy of radar-based precipitation estimation. However, it is challenging to train a deep learning AI model that is applicable to a variety of locations or precipitation regimes. Often, local rain gauge data would be required to retrain the model developed in a domain with different precipitation characteristics. To this end, this research uses a deep convolutional neural network (CNN) as benchmark to design a transfer learning framework to incorporate the knowledge learned at one location to the other locations which feature different precipitation characteristics. Saliency maps are used to interpret the underlying model physics and quantify the impacts of input features on the performance of precipitation estimation. Extensive experiments are performed to explain the transfer learning model by investigating the saliency maps on the activation of a specific neuron and different groups of neurons. The results demonstrate that this explainable machine learning framework can significantly improve precipitation estimation accuracy compared to conventional fixed-parameter rainfall algorithms.


AS42-A013
Variation Characteristics of Radar Parameters Based on Three X-band Dual-polarization Phased Array Radars During Hail Suppression Experiment in Southwestern China

Hui WANG#+
Chinese Academy of Meteorological Sciences

In order to study the effect mechanism of hail suppression by artillery, the national hail suppression experiment is jointly organized by the Weather Modification Center of the China Meteorological Administration and the Guizhou Meteorological Bureau in July to September 2021 and 2022. The experiment region is located in Weining country, Bijie City, Guizhou province, which belongs to Wumeng Mountains of Yunnan-Guizhou Plateau in southwestern China, where the hailstorms occur frequently in summer. Three X-band dual-polarization phased array radars distributed as approximate equilateral triangle with no more than 20 km distances are used to obtain the variation of hailstorms during hail suppression by artillery. Some preliminary results on hail cloud characteristics and effect of hail suppression have been achieved as follows. (1)The hail cloud characteristics include that the time from birth to hail fall down is 10-20 minutes, the hail duration is about 2-5 minutes, and the hailstorm size is mainly 5-10 mm. (2) By analyzing the variation of radar parameters of some hail clouds operated by artillery based on high time resolution observations of RHI and fan sweep, it can be all found that the intensity of radar echo suddenly weakens, the top height of strong echo suddenly decreases and the radial wind direction turns in about 1 minute in the explosion region caused by artillery in hail cloud. Such a rapid change in the structure of the hail cloud probably has more to do with the dynamic effect of artillery. It can be seen that the vortex and sinking air flow generated by the explosion based on analyzing the three-dimensional wind field, which is consistent with explosion simulation results on the dynamic effect of explosion by predecessors. These results provide an important observational basis for the mechanism study of hail suppression by artillery.


AS42-A015
Application of Polarimetric Variables as Leading Indicators for Heavy Rain with Apparent Rotational Signature

Chi-June JUNG+, Ben Jong-Dao JOU#
National Taiwan University

The appearance of extreme volumes of differential reflectivity (ZDR) and specific differential phase (KDP) above the environmental 0 °C level was proposed to be a leading indicator of heavy rain on the ground (Jung and Jou, 2023). Its applicability was explored in several summer severe rain events in the Taipei Basin (Jung and Jou, 2022), and the results showed that the integrated amount of ZDR and KDP from 1 to 3 kilometers above the ground has a better correlation with surface rainfall and the lead time is about 10 minutes. If the variation of KDP above the melting layer is considered, the lead time can be extended to 20 minutes. However, the polarimetric variables did not correlate with rainfall for some analyzed events, including typhoons and local eddies on the terrain. This study presents the possibilities of the abovementioned situation, including weak convection and cyclonic circulation in these rainstorm systems. The improved leading indicator using polarimetric radar for heavy rain with apparent rotational signature is under investigation. Reference: Jung, C.-J. and B. J.-D. Jou, 2022: Application of Polarimetric Variables as Leading Indicators for Severe Rainfall [Poster presentation]. 30th Conference on Severe Local Storms, Santa Fe, NM, United States. Jung, C.-J. and B. J.-D. Jou, 2023: Bulk microphysical characteristics of a heavy rain complex thunderstorm system in the Taipei Basin. Mon. Wea. Rev., accepted.


Thu-03 Aug | 1:10 - 3:10 | MR327
AS39 - Models, in Situ, and Remote Sensing of Aerosols (MIRA)

Session Chair(s): Sang-Woo KIM, Seoul National University, Greg SCHUSTER, NASA Langley Research Center

AS39-A008 | Invited
Models, in Situ, and Remote Sensing of Aerosols (MIRA) International Working Group

Charles TREPTE1#+, Sang-Woo KIM2, Greg SCHUSTER1, Oleg DUBOVIK3, Mian CHIN4, Maria Obmininda CAMBALIZA5
1NASA Langley Research Center, 2Seoul National University, 3University of Lille, 4NASA GSFC, 5Ateneo de Manila University and Manila Observatory

There is a natural partitioning of scientific interest amongst three focus areas of aerosol research: modeling, in situ measurements, and remote sensing observations. The community benefits when these groups interact, with overall benefits towards advancing our understanding of climate, weather, and air quality. To this end, MIRA seeks to foster international collaborations across disciplines and regional boundaries and offers a complementary association with established international working groups. Within the present framework, MIRA has identified four initial focus areas, with opportunities to add more by the working group. One effort advances knowledge of the aerosol lidar ratio for different aerosol compositions and locations to improve backscatter lidar retrievals from satellites and ground-based instruments. Another effort seeks to improve aerosol optical parameters used by climate and radiative transfer models. A third effort focuses on harmonizing aerosol assimilation models with satellite measurement retrievals, and a fourth interest seeks to develop retrievals of aerosol Particulate Matter from remote sensing measurements. The presentation will provide an overview of MIRA and ways for the community to engage.


AS39-A015 | Invited
Toward a Synergistic Use of GEO-LEO Satellite Observations, Atmospheric Measurements, and Models for Air Quality Research and Applications

Mian CHIN1#+, Huisheng BIAN2, Qian TAN3, Tianle YUAN4,2, Hongbin YU4, Gao CHEN5
1NASA GSFC, 2University of Maryland, Baltimore County, 3Bay Area Environmental Research Institute, 4NASA Goddard Space Flight Center, 5NASA Langley Research Center

In this study, we explore how to use the aerosol optical depth (AOD) data from both low earth orbiting (LEO) and geostationary (GEO) satellites for air quality research and applications. Using results from the atmospheric chemistry and transport model together with measurements from ground-based networks, we will address the following questions:(1) What are key factors modulating the relationship between column aerosol optical depth (AOD) and surface PM2.5 over different spatial and temporal scales, including aerosol vertical distributions, composition/size, and meteorological conditions? (2) What are the most scientifically robust and logistically feasible ways to convert satellite observations of aerosols to surface PM2.5 for air quality applications? We will use the simulation of AOD and PM2.5 from the NASA GEOS/GOCART model and the meteorological fields from the MERRA-2 reanalysis to analyze the relationship between AOD and PM2.5 on different time scales and in different aerosol regimes/environment to identify the most important factors that should be included in converting column AOD to surface PM2.5. We will test these parameters with observations from co-located AOD and PM2.5 measurements to verify the results. At the end, we will recommend the practical use of the GEO-LEO satellite data for air quality study.


AS39-A016 | Invited
A Fractionation of Asian Dust and Locally Generated Dust Layers in Japan Using Depolarization Ratio Obtained by AD-net Lidars

Atsushi SHIMIZU#+, Tomoaki NISHIZAWA, Yoshitaka JIN, Nobuo SUGIMOTO
National Institute for Environmental Studies

An elastic backscatter lidar is a relatively simple, but robust equipment which can measure the vertical distribution of aerosols. Especially the depolarization ratio, a measure of non-sphericity of scatterers, is useful to identify the existence of mineral dust particles. The Asian dust and aerosol lidar observation network (AD-Net) is dedicated to the continuous monitoring of both of anthropogenic and natural particles in the East Asia region. Although AD-Net supplies dust extinction coefficient, both of long-range transported Asian dust and locally generated dust are treated in same manner without differentiation. In this study a method to fractionate them separately is proposed.
In spring season wider area in Japan receives long-range transported Asian dust which is originally generated in inner Eurasian continent and transported eastward. Also, wind-blown local dust are generated in Kanto area (around Tokyo metropolitan) of Japan in early spring. To compare the optical properties of these two kinds of dust, February 2017 and May 2017 were selected as typical months for Asian dust and local dust, respectively. The frequency distribution of depolarizaiton ratio at 532 nm for dust layer detected by AD-Net lidar in Tsukuba showed a clear difference in two months, and 40% of the particulate depolarization ratio was identified as the threshold.
Statistical analysis of depolarization ratio during February and May at four AD-Net stations indicated that the local dust was dominant in February and March at Tsukuba, and in other months/places the Asian dust was dominant. Lower depolarizaiton ratio found in Nagasaki (western Japan) suggests an external mixture of Asian dust and anthropogenic (spherical) particles which were also transported from Eurasian continent.


AS39-A018 | Invited
Long-term Monitoring of Aerosol Optical Properties by Sky Radiometer

Kazuma AOKI1#+, Masahiro MOMOI2, Toshihiko TAKEMURA3
1University of Toyama, 2Generalized Retrieval of Atmosphere and Surface Properties, 3Kyushu University

We investigated the long-term monitoring of aerosol and cloud optical properties at ground-based and maritime measurements since 1990's by using the Sky radiometer (POM-01, 02: PREDE Co. Ltd., Tokyo, Japan.). Our objectives were to understand the effect on climate change, and the other was to validate satellite (e.g., GCOM-C/SGLI, JAXA) and numerical models (e.g., SPRINTRAS). Solar radiation measurements have been employed for aerosol optical properties (Aerosol optical thickness and Single scattering albedo at each wavelength, Ångström exponent, etc.), size distribution of volume and so on. These data have revealed various events (anthropogenic and/or natural aerosols), seasonal and long-term trends. However, there are still some things to consider in different observation environments and different climatic conditions, such as changes in some parameters (surface albedo and atmospheric conditions), which are also related to spatial and temporal representation. Based on the validation of satellite and numerical model, we are conducting different research (atmosphere, Ocean, Cryosphere, Land) to proposals for next validation and analysis, focusing on the wavelength dependence of optical properties. We provide the possibility to the comparison of remote sensing and model, in this presentation, on the aerosol optical properties measurements with temporal and spatial variability in the long-term record.


AS39-A014
Optical Properties of Boundary Layer Aerosols from High Spectral Resolution Lidar Measurements in a Polluted Urban Environment (Seoul, Korea)

Soojin PARK1#+, Sang-Woo KIM1, Man-Hae KIM1, Robert HOLZ2, Ralph KUEHN2
1Seoul National University, 2University of Wisconsin

The vertical distribution of aerosols and its evolution over time is important for accurately simulating near-surface air quality since the chemical and transport processes of aerosols vary by altitude. Understanding the optical properties of aerosols by altitude is also important when accounting for aerosol radiative and climate effects. We investigated the temporal variation of aerosol optical properties in Seoul, Korea, using 2-year (2016–2018) High Spectral Resolution Lidar (HSRL) measurements. The HSRL offers accurate AOD measurements without the need for a predefined lidar ratio due to its capability to separately measure backscattered signals by molecules and particles. Continuous measurements of aerosol extinction coefficient from the HSRL were used to investigate the diurnal variation of AOD. Nighttime AOD displayed a larger mean and standard deviation (0.45 ± 0.46) than daytime (0.40 ± 0.31). Hygroscopic growth of aerosols under humid conditions was a key factor in the relative enhancement of nighttime AOD. Taking advantage of the HSRL’s vertically-resolved measurements, the contribution of aerosols within the boundary layer (BL) and the free troposphere (FT) to AOD were investigated. Unlike the diurnal AOD variation, AOD within the BL (AODBL) showed similar diurnal variations with the mixing layer height (MLH), displaying lower nighttime values with a peak around 14–15 local standard time. Using HSRL and surface PM10 measurements, the mass extinction efficiency (MEE) of aerosols in Seoul was estimated. The PM10 MEE showed a mean of 5.40 g m-2 and displayed significant variability by PM2.5 to PM10 ratio, season, and ambient relative humidity (RH). The uncertainty of estimated surface PM10 concentrations was minimized when the seasonality and humidity factor in MEE were considered. We additionally investigated the lidar ratio values dependent on aerosol type using HSRL measurements that can be used to improve aerosol extinction coefficient retrievals from elastic lidar measurements.


Thu-03 Aug | 1:10 - 3:10 | MR328
AS10 - Extreme Events: Observations and Modeling

Session Chair(s): Rajasekhar MEKA, Indian Space Research Organisation, Sridhara NAYAK, Japan Meteorological Corporation

AS10-A036
The Evaluation of Skill of Global Extended Range Ensemble Predictions for Predicting the Genesis of Tropical Cyclone Over Bay of Bengal

Rajasekhar MEKA1#+, Yesubabu VISWANADHAPALLI2
1Indian Space Research Organisation, 2National Atmospheric Research Laboratory

Accurate prediction of tropical cyclone (TC) genesis, movement, intensification and landfall locate are extremely crucial for successful and effective cyclone disaster prevention and mitigation plan for Indian Coasts. Particularly, the genesis and intensification of TC are mainly depends the underlying features of upper ocean surface, the wind shear between lower and upper troposphere. In this study, we analysed the skill of ensemble forecasts from multiple forecast centres including the European Centre for Medium Range Weather Forecasting (ECMWF) and the Global Ensemble Forecast System (GEFS) extended range probabilistic forecasts for predicting the genesis and intensification of TCs over Bay of Bengal by considering a 15-day lead period. Out of these two ensemble forecasts, ECMWF provides forecasts with 51-members while the GEFS produces ensembles forecast with 21-member to compute the track probability and density compositions. Our comparison of results with the observed estimates of TC best track data clearly suggests that the both ensemble predictions (ECMWF and GEFS) have demonstrated the good skill in predicting the tropical cyclogenesis over Bay of Bengal with lead of 7 to 10 days for the three TC cases (Asani, Sitarang and Mandous) of 2022. Further, our detailed analysis and validation of extended predictions for three TCs of 2022 with best track datasets clearly suggests that the tropical cyclogenesis outlook provided by ECMWF with 51 ensemble members forecast is extremely useful and highly valid for prior prediction of TC genesis over Bay of Bengal.


AS10-A005
Organized Convective Systems Yielding Tornadoes Far from Typhoon

Koji SASSA1#+, Sora ISHIDO2
1Kochi University, 2Japan Meterological Agency

When the Typhoon Trami (2018) moved northeastward in the Pacific Ocean south of the Kyushu Island at 6:30JST on 30 September 2018, a tornado occurred and caused damages in Kochi city. A funnel cloud also appeared two hour later. Their parent convective system is the array of slender rainbands formed more than 500 km apart from the typhoon center. The present study aims to clarify the characteristics and environment of the parent convective systems. The results of radar analysis show that the rainbands are 30km in length and 4 km in width are arranged parallel to the radial axis of the typhoon and move north-northwestward. Their principal axis is northeast and is almost same with the direction of shear vector of the environment wind. The parent convetive systems have a mesocyclone at its southwest end, but their arrangement is different from the ordinary mini supercells. Then, the mesocyclone repeats alteration of generation. The environment indices, MUCAPE and SReH of in this case are found to be larger and smaller than those of a mini supercell in outer rainband, respectively.


AS10-A008
Fitting Parametric Tropical Cyclone-induced Rainfall Model for Tropical Cyclones Landfalling onto the Northern Vietnam Coast

Warinthorn ANGKANASIRIKUL1#+, Wei JIAN2, Edmond LO1
1Nanyang Technological University, 2Institute of Catastrophe Risk Management, Nanyang Technological University

Tropical cyclones (TCs) can cause major flooding individually or collectively due to wind, storm surges and rainfall. This study applies the parametric rainfall climatology and persistence (R-CLIPER) model to analyse the axisymmetric component of 14 TC rainfall events in Northern Vietnam with the observed rainfall dataset from the Global Precipitation Mission from 2001 to 2021.The R-CLIPER model uses two inputs from TC track information: the maximum wind speed and radial distance from the TC centre. Four parameters represent the axisymmetric profile of rainfall rates: To, Tm, rm, and re. To and Tdescribe the rainfall intensity at the TC centre, and the maximum intensity which is located at radial distance rfrom the centre, respectively. The fall-off from the maximum is exponential with a characteristic distance re. The R-CLIPER model generally assumes linear relationships between the four parameters and a normalised maximum wind speed (U). We adopt the operational coefficients by the National Hurricane Center (NHC) for the Western Pacific region as the initial setting. The observed TC rainfall profiles are further used to fit the parameters using the least-square method. Performance of the R-CLIPER with the initial and fitted settings for predicting the observed 14 rainfall profiles is assessed. Tand Tm are found to be better represented by logarithm relationships with U, and rm by exponential relationship, based on their improved Rvalues over the R-CLIPER with NHC coefficients for the 14 historical TC events. At 0.1-degree resolution, the equitable threat score demonstrated significant improvement, almost six times at the 100 mm rainfall threshold. Improved root mean square error and bias are also seen for the cumulative rainfall volume and the averaged rainfall intensity. For instance, the bias has been reduced by around 50% with the new relationships of the parameters and U in most cases. 


AS10-A007
Active Influence of the Boundary Current Synchronization on the Northern Annular Mode

Tsubasa KOHYAMA1#+, Yoko YAMAGAMI2, Shoichiro KIDO2, Fumiaki OGAWA3, Hiroaki MIURA4, Hiroaki TATEBE2
1Ochanomizu University, 2Japan Agency for Marine-Earth Science and Technology, 3Hokkaido University, 4The University of Tokyo

Synchronized variability between two Northern Hemispheric western boundary currents, which is referred to as the Boundary Current Synchronization (BCS), is associated with meridional migrations of the atmospheric jet stream. Based on observational evidence, BCS exhibits covariability with the Northern Annular Mode (NAM), the most prominent internal atmospheric variability that controls the latitudinal position of the jet stream in Northern Hemispheric winter. Therefore, in this study, we have performed a set of high-resolution pacemaker experiments where sea surface temperatures in the two boundary current regions are strongly relaxed to a preindustrial control run. These eddy-permitting pacemaker runs show that BCS actively supports the existence of extreme NAM events, which in turn affects the abnormal weather events in winter. The extent to which boundary currents affect the NAM phase varies among different ensemble members, so the BCS influence on NAM is sensitive to stochasticity.


AS10-A028
The Indonesia Numerical Weather Prediction (InaNWP): Development, Progress, and Preliminary Results

Jaka PASKI1#+, Erwin MAKMUR2, Urip HARYOKO2, Danang Eko NURYANTO2, Dwikorita KARNAWATI2, Wido HANGGORO2, Supriyanto ROHADI2, Fatkhuroyan FATKHUROYAN2, Nelly Florida RIAMA2, Donaldi PERMANA2
1Tohoku University, 2Indonesian Agency for Meteorology, Climatology and Geophysics

In 2021, the Indonesian Agency for Meteorology, Climatology and Geophysics (BMKG) developed the Indonesia Numerical Weather Prediction (InaNWP) using weather research and forecasting (WRF) model with data assimilation. The model was developed using WRF model package and WRF Data Assimilation (WRFDA) version 4.2 with a three-dimensional variational (3DVAR) data assimilation system. The domain of InaNWP covered Indonesia region with 9 km of spatial resolution and nesting to a 3 km spatial resolution over Java Island. InaNWP assimilates data from in-situ, remotely sensed, and radiance observations. The in-situ data assimilation includes at least 137 synop data and 19 sounding data collected by BMKG stations at 00 and 12 UTC. In addition, InaNWP has also assimilated the radiance data from the new generation of Himawari satellite and the remotely sensed data from at least 25 out of 42 weather radar stations throughout Indonesia. Due to limited computing resources, InaNWP produces 3-hourly weather forecast for up to 72 hours. After one year of testing, InaNWP was able to predict extreme weather events such as Tropical Cyclone Seroja on April 3, 2021. Model verification from about 150 BMKG stations during the period of February–August 2021 indicates InaNWP has good performance in predicting mean sea level pressure, temperature, and relative humidity, followed by dewpoint temperature, winds, and precipitation.


AS10-A042
Statistical Analysis on Direction of Tornado Motions and its Relationship with the Large-scale Wind Field

Yuri MITA#+, Tsubasa KOHYAMA
Ochanomizu University

A tornado is a violent updraft vortex that occurs in association with a cumulonimbus cloud. Tornadoes are generated when atmospheric conditions are extremely unstable, and can cause extensive damage over a narrow band-like area in a short period of time. Forecasting genesis and tracks of tornadoes is essential to minimize damage to people and structures. According to Niino et al. (1997), more than half of tornadoes moved into the northeast quadrant. However, since this data was based on visual observations, the reported directions of tornado motions were biased toward 8 directions out of 16. Therefore, by collecting directional data of tornado motions in an objective way, this study investigates the relationship between directions of tornado motions and the large-scale wind field, assuming that cumulonimbus clouds accompanied by tornadoes are carried by large-scale winds. First, the direction of tornado movement is calculated from the latitude and longitude of the point of genesis and extinction to obtain more accurate statistics than the eyewitness testimony used in previous studies. These calculations show that approximately 70% of tornadoes moved into the northeast quadrant. The northeastward bias is presumably not a sampling bias because the qualitative results are the same for two independent periods. Regardless of the year or region of occurrence, 60 to 80% of tornadoes moved toward the northeast quadrant. In particular, the eastward bias suggests that the cumulonimbus clouds are being carried by the westerly jet stream overhead. In addition to this eastward bias, in boreal summer and autumn, the directional distribution of tornado motions exhibits a northward bias, which is due to tornadoes associated with typhoons. The correlation between the direction of tornado motions and the large-scale wind direction is consistent with a hypothesis that tornadoes are transported by winds along with cumulonimbus clouds.


AS10-A041
Maintenance Mechanism of Cutoff Lows as Vortex–Vortex Interactions (The 2nd Report)

Koryu YAMAMOTO1#+, Keita IGA1, Akira YAMAZAKI2
1The University of Tokyo, 2Japan Agency for Marine-Earth Science and Technology

A cutoff low that covered Central Europe in the middle of July 2021 brought heavy rainfall and severe flooding, resulting in more than 200 fatalities. This low was formed by a trough on 11 July and merged with another cutoff low from 12 to 14 July. An energetic analysis suggests the main cutoff low was maintained through a vortex–vortex interaction between the two cutoff lows, as well as downstream development from an upstream ridge as a baroclinic eddy; these conclusions are confirmed by Lagrangian backward trajectory analysis. A forward trajectory analysis then shows that parcels move into the main cutoff low and exhibit cyclonic circulation. As some previous studies have pointed out that diabatic processes can strengthen or weaken cutoff lows, the processes along the parcels that move into the main cutoff low from the other low are diagnosed. It is suggested that radiative effects act mainly to strengthen the interaction inside the main cutoff low, whereas latent heat release contributes a negative potential vorticity tendency in the latter period of analyses. These results demonstrate that cutoff lows can be maintained through vortex–vortex interactions and underline the need to also take diabatic processes into account, which no previous studies have discussed in detail. In the presentation, results by sensitivity experiments focused on the interaction will be shown.


Thu-03 Aug | 1:10 - 3:10 | MR329
AS44 - Atmospheric Nitrogen-containing Organic Compounds: Sources, Processes, and Impacts

Session Chair(s): HWA JIN KIM, Seoul National University, Tzung-May FU, Southern University of Science and Technology, Qi CHEN, Peking University

AS44-A018
Organic Nitrates and Their Contribution to Secondary Aerosol Formation Over China’s Megacites

Wei NIE#+, Chao YAN, Yuliang LIU, Aijun DING
Nanjing University

Organic nitrates (ONs) are potentially important contributors to secondary aerosol formation, especially those with low volatility. However, the direct measurement of the gaseous condensable ONs poses a great challenge due to their diversity and low concentration. Here we present coordinated measurements of gaseous ONs in the urbanized regions of China and determine their likely precursors, enabling us to connect them to secondary organic aerosol (SOA) formation. We found ONs dominated the organic condensable vapors and contributed significantly to the SOA formation over China’s megacities. In particular, ONs accounted for more than 80% of the observed organic condensable vapors, which originated from the oxidation of the aliphatics (most likely dominated by alkanes). The reaction of peroxy radicals (RO2) with NO controlled the daytime formation of ONs, while the oxidation of alkenes (e.g., isoprene and monoterpenes) by NO3 plays a non-negligible role during the night.


AS44-A017
Molecular Characteristics and Formation Pathways of Particulate Organic Nitrates During Winter and Summer in Urban Beijing

Yan ZHENG+, Qi CHEN#, Yanli GE, Xi CHENG, Theodore K. KOENIG, Gaoyuan WEI, Xiaodi SHI, Zhen CHENG, Xinghua QIU, Shiyi CHEN
Peking University

Particulate organic nitrates (ONs) can account for a major mass fraction of secondary organic aerosol (SOA) in urban environments with large emissions of organic precursors and nitrogen oxides (NOx). Limited by current measuring techniques, molecular characteristics and formation pathways of ONs have still remained less investigated. In this study, we obtained the molecular compositions and sources of SOA during winter and summer in urban Beijing based on online and offline measurements by high-mass-resolution mass spectrometry, including a long time-of-flight aerosol mass spectrometer (LTOF-AMS) and an iodide-adduct time-of-flight chemical ionization mass spectrometer (I--TOF-CIMS) coupled with a filter inlet for gases and aerosols (FIGAERO). We found that aqueous processing plausibly played an important role in forming multifunctional organic nitrates during strong humid haze in winter, which contributed to a major mass fraction of enhanced SOA. Oxidation of monoterpenes by NO3 radicals was the major formation pathway of particulate organic nitrates in summer. High NOx concentrations during daytime might hinder the gas-to-particle partitioning of organic nitrates in urban environments. Compared to winter, oxidation products of biogenic organic precursors (i.e., monoterpenes and isoprene) accounted for a larger mass fraction of particulate ONs in summer, while the oxidation of long-chain alkanes and alkenes contributed less. Aromatics are important precursors of ONs in both winter and summer. Our results highlight the complexity of reducing nitrogen oxides and nitrate for SOA reduction in the future.


AS44-A016
Source Apportionment of Atmospheric Organic Nitrogen Aerosols at a Suburban Site in Hong Kong

Jinjian LI1+, Xu YU2, Shan WANG2, Yuk Ying CHENG2, Hanzhe CHEN2, Jianzhen YU2#
1Guangzhou HKUST Fok Ying Tung Research Institute, 2The Hong Kong University of Science and Technology

Organic nitrogen (ON) compounds constitute an important fraction of atmospheric nitrogenous aerosols. They are relevant to ecosystem evolution, secondary aerosol formation, and biotoxicity. Due to the absence of a direct analytical method for bulk aerosol ON quantification, our understanding regarding the sources, formation pathways of ON remains largely qualitative, let alone the assessment of the environmental and health impacts. In this study, we applied the first online instrumental method for simultaneous determination of bulk aerosol inorganic nitrogen (IN) and ON to quantify the atmospheric abundances of nitrogenous aerosols at a suburban site in Hong Kong in the winter of 2020–2021. The ON measurements, together with a suite of molecular and elemental aerosol source markers, were used for source apportionment analysis through positive matrix factorization receptor modeling. At our site, primary sources such as biomass burning and soil dust contributed significantly to bulk aerosol ON (19.3% and 12.5%, respectively). Secondary processes, including α-pinene-related SOA formation (22.5%) and secondary sulfate and nitrate formation processes (20.8%), also played important roles in ON production. Furthermore, the bihourly time resolution of the ON measurement allows capturing the rapid changes of nitrogenous aerosol concentrations and investigating the diurnal-scale dynamics of ON sources. For example, the ON/TN ratio generally increased with ambient relative humidity and temperature, likely a result of that these meteorological factors mediate aqueous-phase formation of secondary ON and the gas-particle partitioning of IN. Additionally, nighttime ON showed a notable increase under high NOx levels, indicating the importance of NO3 radical chemistry in secondary ON formation. This work presents the first source apportionment of bulk aerosol ON and provides measurement-based insights to secondary aerosol ON formation chemistry.


AS44-A012
Saturated Nitrogenated Organics Observed in Wintertime Beijing Aerosol

Theodore K. KOENIG#+, Yanli GE, Xi CHENG, Gaoyuan WEI, Yan ZHENG, Chong ZHANG, Zhen CHENG, Sihua LU, Limin ZENG, Chunxiang YE, Jing SHANG, Qi CHEN
Peking University

In the course of wintertime measurements Beijing, we have consistently observed the diurnal photochemical production of saturated nitrogenated organics CnH2n+1NO4,5,6 (n = 5 – 10) and monounsaturated nitrogenated organics CnH2n-1NO4,5,6 (n = 5 – 10) in the gas-phase utilizing NO3-- and I--Chemical Ionization Mass Spectrometry (CIMS), both separately and simultaneously over several years. Using Oxidation Flow Reactor (OFR) experiments we confirm that the observed signals are consistent with hydroxy- and peroxy- alkyl nitrates produced by OH-initiated oxidation of select alkanes under high NOx conditions and bound the production of the same products from select common unsaturated precursors. Unexpectedly, we further observe these same chemical formulas in the particle phase at highly significant levels using Filter Inlet of Gas and AEROsol (FIGAERO) I--CIMS in parallel to the gas-phase I--CIMS measurements during wintertime haze, which we do not reproduce in OFR experiments. This is particularly notable for the lightest formulas e.g. C5H11NO4, C6H13NO4 which are expected to have high vapor pressures not conducive to condensation to particles and for which plausible alternative chemical structure, especially those amenable to detection by I--CIMS are highly limited. Previous studies have found negligible SOA production from the photochemical processing of light alkanes as well. We use auxiliary measurements, and data analysis methods such as Positive Matrix Factorization (PMF) to investigate the possible sources and drivers of these signals in the particle phase.


AS44-A020
Formation and Photochemical Aging of Secondary Organic Aerosols from NO3 Oxidation of Phenolic Compounds

Hongru SHEN1+, Rongrong WU2, Quanfu HE2, Hui WANG2, Yarê BAKER2, Sören ZORN2, Hendrik FUCHS2, Thomas MENTEL2, Defeng ZHAO1#
1Fudan University, 2Forschungszentrum Jülich

Phenolic compounds containing at least one hydroxyl functional group on the aromatic ring constitute a significant fraction of volatile organic compounds precursors in urban cities, representing a wide range of environmental, climate, and health effects. Daytime OH oxidation and nighttime NO3 oxidation reactions are their main loss pathways. However, compared to OH oxidation, although NO3 reactions demonstrate higher chemical reactivities and potentially higher SOA yields, less is known about SOA formation from NO3 oxidation of phenolic compounds and their roles in next daytime OH oxidation aging. Here, we conducted NO3 oxidation experiments of phenol and o-cresol in SAPHIR-STAR (Simulation of Atmospheric PHotochemistry In a large Reaction Chamber-Stirred Atmospheric flow Reactor) and photochemical aging experiments in SAPHIR (Simulation of Atmospheric PHotochemistry In a large Reaction Chamber). In both chamber experiments, an online EESI-ToF-MS (Extractive ElectroSpray Ionization Time-of-Flight Mass Spectrometer) was used for direct measurement of SOA composition on near-molecular level. Combining gas measurement using NO3- CI-ToF-MS (Chemical Ionization Time-of-Flight Mass Spectrometer), we showed a full picture of gas-phase products formation, their partitioning to particle phase, and photochemical aging of particle phase products. In contrast to OH oxidation reactions, highly oxygenated organic molecules (O≥6) contribute a small fraction of both gas (<1%) and of particle (<10%) phase products. The main particle-phase products (monomers and accretion products) show different time series during OH oxidation aging process. Overall, our experiments help understand SOA formation and photochemical aging from NO3 oxidation of phenolic compounds and provide fundamental data support for accurate assessment of their roles in urban air quality, climate, and health effects.


AS44-A007
Remote Sensing of Trace Gases with Chinese Satellite Instruments

Cheng LIU1#+, Chengxin ZHANG1, Wenjing SU1, Qihou HU2, Haoran LIU3
1University of Science and Technology of China, 2Chinese Academy of Sciences, 3Anhui University

Remote sensing from hyperspectral satellite instruments, such as OMI, TROPOMI and OMPS, can simultaneously obtain the spatio-temporal distribution of several species of trace gases, which has been widely used to study the emissions, regional transport and physical and chemical evolution of trace gases. Nevertheless, there were very few relevant studies using Chinese satellite instruments, because the poor spectral quality makes it extremely difficult to retrieve data from the spectra of the Environmental Trace Gases Monitoring Instrument (EMI), the first Chinese satellite-based ultraviolet–visible spectrometer monitoring air pollutants. In this study, we performed on-orbit wavelength calibration to calculate daily instrumental spectral response functions (ISRFs) and wavelength shifts to diminish the fitting residuals. For the retrieval under the low signal-to-noise ratio (SNR) of EMI, an adaptive iterative retrieval algorithm is set up to select the retrieval setting best with minimum uncertainty. Besides, we used simulated irradiance instead of measured irradiance to obtain the requisite daily solar spectrum for the following retrieval algorithm, because EMI only provides the solar spectrum once every six months. Through these algorithm updates, several trace gases, such as Ozone (O3), nitrogen dioxide (NO2), sulfur dioxide (SO2) and formaldehyde (HCHO), were retrieved from EMI with comparable accuracy of OMI and TROPOMI. The retrieval results from EMI were used to locate emission sources, evaluate regional transport and trace the change of air quality due to important events, such as COVID-19 pandemic, China International Import Expo and Beijing Winter Olympic Games.


AS44-A014
Highly Oxygenated Organic Molecules Produced by Photooxidation of Aromatic Compounds Under Various NOx Conditions

Xi CHENG1+, Qi CHEN1#, Yong Jie LI2, Yan ZHENG1, Keren LIAO1
1Peking University, 2University of Macau

Oxidation of aromatic volatile organic compounds (VOCs) leads to the formation of tropospheric ozone and secondary organic aerosol, for which gaseous oxygenated products are important intermediates. In urban environments, NOx are rich and compete with HO2 and RO2 for the termination of RO2 radicals. Despite of recent progresses, the dependence of oxygenated products distribution on NOx conditions (e.g., [NOx]:[VOC] or [NO2]:[NO] ratios) remains largely unclear. We show herein the experimental results of highly oxygenated organic molecules (HOMs) produced by the oxidation of six aromatic VOCs, including four monocyclic (benzene, toluene, m-xylene, and, 1,3,5-trimethylbenzene) and two double-ring (naphthalene and 1-methylnaphthalene) ones in a wide range of NOx conditions, based on the nitrate-adduct time-of-flight chemical ionization mass spectrometer. The detected HOMs are categorized into fragmented products, open-shell monomeric products, closed-shell monomeric products, and dimeric products, as well as nitrogen-containing products when NOx is present. Fragmented products are suppressed for more substituted aromatic VOCs, and multi-generation OH oxidation diversifies the hydrogen number in both monomers and dimers, which is more prominent for double-ring aromatic VOCs. Under high-NOx conditions, nitrated phenols are the most abundant nitrogen-containing products. The highly oxygenated nitrogen-containing products, especially products with two nitrogen atoms, become more important as the NOx level increases. With high [NO2]:[NO] ratios of tens to hundreds, further investigations find that these compounds might be peroxyacyl nitrates, which can be formed through the reaction of RC(O)OO with NO2.


Thu-03 Aug | 1:10 - 3:10 | MR330
AS59 - Mesoscale Meteorology and High-impact Weather

Session Chair(s): Yipeng HUANG, Xiamen Meteorological Bureau

AS59-A005 | Invited
Processes of Colliding Cold Pools Derived from a 356-m High Shenzhen Met-Tower During an Extremely Heavy Rainfall Event

Yu DU#+, Chuying MAI
Sun Yat-sen University

Convectively generated cold pools are key for convection initiation and development, but observations of their vertical structure are insufficient. In this study, quantitative vertical evolutions of cold pools during a high-impact heavy rainfall event near the south coast of China were examined using observations on a 356-m high Shenzhen Met-Tower, and their possible impacts on heavy rainfall were further discussed with high-resolution surface station network and radar observations. On 11 April 2019, precipitation was enhanced near metropolitan Shenzhen and lasted for 50 min at its southern downtown, resulting in 11 deaths. During this event, a shallow cold pool was first observed by the tower and yielded a long-lasting cooling of 2.6 K. Approximately one hour later, another deeper cold pool accompanied by a squall line was added from the west. This addition led to a more abrupt and intense surface temperature deficit (-5.1 K) and stronger gusty winds (23 m/s). When the two cold pools collided near Shenzhen, the low-level winds converged at their intersection, dynamically enhancing the heavy-rain-producing squall line. Furthermore, the collision of the two cold pools decreased the temperature gradient at the northern edge of the merged cold pool, which could inhibit development of the squall line. The area south of the squall line became a relatively preferred environment for triggering convection under the warm and moist oceanic environment. Consequently, the squall line turned northeast‒southwest and formed a training line mode in which the orientation was almost parallel to the eastward movement. The training line mode prolonged the precipitation duration in the southern downtown area.


AS59-A020 | Invited
Characteristics of Different Intensity Hourly Heavy Rainfall Events and Forecasting Indices Thresholds in Beijing Metropolitan Region of 2010-2019

Lei LEI1#+, Yanyan KANG2, Nan XING3, Jisong SUN4, Mingxuan CHEN4, Xuan ZHOU2, Yuanyuan WANG2
1Beijing Weather Forecast Center, Beijing Meteorological Service, 2Beijing Weather Forecast Center, 3Beijing Meteorological Service, 4China Meteorological Administration

Using the AWS data 2010-2019, the Hourly Heavy Rainfall events (HHR) over Beijing metropolitan region was divided into four levels: 20~40, 40~60, 60~80 mm/h and more than 80 mm/h. The statistical spatiotemporal characteristics and the key thermal dynamical and vaporous forecasting indices thresholds was extracted. The results showed: (1) The distribution of different levels HHR was slightly different, the common high frequency (HF) areas were located in the northeast, the western of the central urban city, and the southwest area nearby the plain. In addition to these three HF areas, 40~60 mm/h HHR also occurs more frequently in the southeast plain. Since 2015, the distribution has changed, the extreme HHR (above 60mm/h) near the Miyun Reservoir and the eastern urban area have shown an increasing trend. (2) There are three main synoptic patterns (SP) of extreme HHR: the westerly trough (WT) pattern, Mongolia low vortex (MV) pattern, and northeast low vortex (or northwest flow)pattern. The WT and MV patterns have more occurrences of HHR. When the northwest Pacific subtropical high was coupled with the WT pattern, 86% of the HHR exceeded 80mm/h. In the MV pattern, HHR is generally 60~80 mm/h. (3) The analysis of environmental forecasting indices have shown that most are not of significance for HHR intensity forecasting if the SP is not distinguished. Only the 850~925hPa wind speed (W), 2 meters dew point (2m-td) and specific humidity (q) have significance. Studying the indices thresholds under different SP make more sense. The CA pattern is the most different from other pattern with the indices thresholds, and the key indices under this pattern is mainly the stability of the layer. The WT pattern is with stronger thermal dynamical and moisture conditions.


AS59-A011
The Influence of Land–sea Contrast and Topography on the Diurnal Cycle of Precipitation in the Bay of Bengal

Zijian CHEN+, Yu DU#
Sun Yat-sen University

An offshore propagating diurnal signal of rainfall is observed from the eastern coast of India to the eastern Bay of Bengal from satellite data. A series of numerical model experiments reveal that this is closely related to the diurnal land-sea thermal contrast between India and the Bay of Bengal. The experiments show that the inertia-gravity waves driven by the land-sea thermal contrast play a significant role in the initiation and offshore propagation of mesoscale convective systems (MCSs) in the bay, and their phase speed well match the propagation speed of rainfall. The offshore propagating signal remains even after removing the topography in India or turning off latent heating from MCSs over the land of India. This implies that terrain and latent heating have secondary but not dominant effects on the offshore propagation of rainfall. The diurnal boundary layer heating depth is modulated by topography and diurnal MCS’s latent heating over land areas, and thus affect the amplitude, phase and speed of the inertia-gravity waves. Higher mountains or stronger latent heating in convection over land result in stronger and faster propagating gravity waves, leading to faster rainfall propagation.


AS59-A019
Prediction Skill of WRF Cycling 3DVAR on Summer Extreme Rainfall Events in Thailand: A Case Study in Chi and Mun Basins During a Tropical Storm Event

Thippawan THODSAN+, Kritanai TORSRI#, Rati SAWANGWATTANAPHAIBUN , Thakolpat KHAMPUENGSON, Pattarapoom PEANGTA, Apiwat FAIKRUA, Kanoksri SARINNAPAKORN
Ministry of Higher Education, Science, Research and Innovation

Initial conditions are factors that affect short-term weather forecast, which is useful for planning daily activities and making short-term decisions. Fundamentally, blending observations from various sources with a numerical weather model can produce a more accurate depiction of the initial atmospheric state, which could allow a more accurate forecast to be generated. This study was conducted to quantify the impacts of data assimilation on heavy rainfall prediction in Thailand using a three-dimension variation of the WRFDA-3DVAR. In this case, 24-hr model integration was employed with the finest horizontal resolution of 3-km grid spacing for two heavy rainfall events occurring in Chi and Mun basins, which were regularly affected by tropical cyclones during summer season. Three assimilation experiments with different data sources were conducted consisting of (1) Global Weather Surface (GWS), (2) Automatic Weather Data (AWD) from the National Hydroinformatics Data Center (NHC), Thailand, and (3) the combination of GWS and AWD. As a basis of comparison, 3-hr accumulated rainfall forecasts were computed considering three different types of rainfall intensity (i.e., 1 mm, 5 mm, and 10 mm) and compared with in-situ observations. Overall, the model yielded higher skill in predicting the 3-hr accumulated rain intensity in all categories compared to without data assimilation. Obviously, the better improvement of the model was seen for the accumulated rainfall of the 5-mm category over 15 hours lead time with the highest fraction skill score of about 0.65 when both GWS and AWD were integrated into the model. The study suggested a potential of implementing the WRF cycling 3DVAR and the use of the NHC’s AWD combined with GWS to reduce errors in the initial conditions used by the model, which can improve the accuracy of the short-term weather forecast in Thailand, particularly during the high-impact weather situations.


AS59-A015
Convection Initiation During the Meiyu Environment in the Yangtze-Huai River Basin of China

Fan ZHANG#+
Chinese Academy of Meteorological Sciences

Convection is the main contributor to heavy rainfall over China’s Yangtze-Huai River Basin (YHRB) during Meiyu season; however, the mechanisms of convection initiation (CI) associated with the Meiyu front are still not well understood. In this study, a large set of 86,099 CI events, identified from composite reflectivity data in YHRB over six Meiyu seasons, were used to investigate the characteristics of the spatiotemporal distribution of CI in YHRB. The result showed that the overwhelming majority of CI events (~90%) occurred in the region of existing stratiform clouds. Meanwhile, CI tended to concentrate in mountainous areas and exhibit two triggering modes. By relating the CI events with an objective analysis of ERA5 reanalysis data, it was also revealed that the characteristics of CI occurrence varied with patterns of Meiyu circulation and their interactions with local topography, and the warm air advection pattern dominated the Meiyu CI. We further illustrated that the CI on plains occurred with a morning peak corresponding to environments of high 0-3 km shear (SHR3) and low MUCAPE (most unstable convective available potential energy), while the CI near or over mountains had an afternoon peak corresponding to low SHR3 and high MUCAPE environments.


Thu-03 Aug | 1:10 - 3:10 | MR331
AS01 - The Asian Monsoon, Extremes and Climate Change

Session Chair(s): Kyung-Ja HA, Pusan National University, Ramesh KRIPALANI, Indian Institute of Tropical Meteorology, Renguang WU, Zhejiang University

AS01-A009
Monsoon During Past Millennium and Present

Akanksha SHARMA#+, A. P. DIMRI
Jawaharlal Nehru University

In the India, monsoon season is vital to existence it continues to be a seasonal phenomenon and impact society, human existence, civilization. It has been looked from many perspectives and various sculptures like Vedas, sastras and many poets’ explicitly mentioned monsoon. It is a strong subject for multi-dimensional involvement. Over time, it helped humans to settle lives based on agriculture and many civilizations have relied on the monsoon for their survival. In the present study, an attempt has been made to draw connections between Indian Summer Monsoon (ISM) and its historical development in order to comprehend internal variability and perhaps get insight into ISM's future course. Extensive multi-proxy records from archaeology, ancient literature, settlement patterns, chronology with available palaeoclimate proxies from terrestrial and marine data from the Indian subcontinent and a few nearby regions are used to study evolution of monsoon and its linkage with agriculture and human settlement.


AS01-A073
On Interpreting Modern Precipitation-δ18O from South Korea: Implications to Paleoclimate Reconstruction

Nitesh SINHA1#+, Timmermann AXEL2, Hyuna KIM3
1Pusan National University, 2Center for Climate Physics, Institute for Basic Science, 3IBS Center for Climate Physics

Stable isotopes in precipitation (e.g., δ18Op) act as tracers for rainfall amount, moisture's origins, and transport pathways (Dansgaard, 1964). In turn, underlying climate-isotope correlations lead to the paleoclimate records’ (e.g., speleothem-δ18O) dependency on precipitation isotopes. It has been reported in earlier studies that the southeast Asia precipitation isotope compositions have influence from various air masses (e.g., Araguás-Araguás et al., 1998). The Korean peninsula location is complex in terms of changes in moisture sources on monthly to seasonal timescales. This makes use of the isotopic signatures challenging to understand precipitation variability over the Korean peninsula. Korea is known to be strongly affected by the East Asian Summer Monsoon (EASM) system. However, the Korean speleothem-δ18O records generally do not show local precipitation signals even during severe drought or extreme events (Jo et al., 2010). We investigate the relationship between δ18Op and rainfall using Busan monthly rainwater isotopes (2019-2022) and data from the Global Network of Isotopes in Precipitation (GNIP) over Korea. We exploit trajectory analysis to track back moisture sources on a monthly scale. We proposed that the moisture source changes, contrary to the local precipitation amount, mainly control δ18Op over the Korean peninsula. In addition, the spatial correlation between rainfall and Korea δ18Op in the isotope-enabled Community Earth System Model (iCESM1.2) provides further insights into EASM and Korea δ18Op relationship. Our results may help interpret δ18O from speleothems from the Korean peninsula. References: 1. Araguás-Araguás et al, 1998. Stable isotope composition of precipitation over Southeast Asia. Journal of Geophysical Research 103: 28721–28742. 2. Dansgaard W. 1964. Stable isotopes in precipitation. Tellus 16: 436–468. 3. Jo et al., 2010. Rainfall and hydrological controls on speleothem geochemistry during climatic events (droughts and typhoons): An example from Seopdong Cave, Republic of Korea. Earth and Planetary Science Letters 295(3–4): 441–450.


AS01-A008
The Synergistic Effect of the Summer NAO and Northwest Pacific SST on Extreme Heat Events in the Central–eastern China

Hao WANG1+, Jianping LI1#, Fei ZHENG2
1Ocean University of China, 2Sun Yat-sen University

The synergistic effect of the summer positive North Atlantic Oscillation (pNAO) and positive northwest Pacific (pNWP) sea surface temperature anomaly (SSTA) on the interannual variability of the extreme heat events in the central–eastern China (CEC) is investigated in this study. The two factors act synergistically in strengthening the extreme heat events in the CEC, and the CEC is likely to experience a hotter summer when both the summer pNAO and pNWP SSTA occur. The two factors influence the extreme heat events in the CEC via a series of atmospheric bridges. The pNWP SSTA increases the strength of pNAO via the eastward propagating Rossby wave from the western Pacific. The enhanced pNAO induces a stronger eastward Rossby wave propagation across the Eurasian continent, and leads to a strong anomalous anticyclone over the CEC. The significantly increased atmosphere thickness increases the air temperature of the layer, and favors the extreme heat events in the CEC. Besides, the anomalous southerlies on the west side of the anomalous anticyclone are also favorable for the increase in air temperature. Furthermore, the pNWP SSTA also has adjacent effect on the atmospheric circulation over the CEC, which could lead to a positive geopotential height anomaly. Therefore, the summer pNAO and pNWP SSTA act synergistically in influencing the atmospheric circulation over the CEC, and thereby significantly increase the extreme heat events in the CEC. Compared with the cooccurrence of the summer pNAO and pNWP SSTA, the magnitude of the extreme heat events decreases greatly when only one factor happens, which highlights the synergistic effect of the two factors.


AS01-A076
Detection and Attribution of Changes in the Mean and Peak Near-surface Wind Speed over Various Regions of China

Hairong LI#+, Kaiqiang DENG, Song YANG
Sun Yat-sen University

The variations of wind speed at 10 m (WS10) play a key role in influencing the natural environment and human society, but the differences in WS10 changes between specific regions of China in a warming climate and their associated causes remain unclear. This study evaluates the WS10 changes in seven subregions of China, based on station observations and a method involving the analysis of rotated empirical orthogonal function and hierarchical clustering. The results show that high WS10 is more likely to occur in the northwestern, eastern, and northern regions of China, where the WS10 has experienced rapidly decreasing trends in the recent decades. In contrast, lower WS10 and smaller WS10 trends are observed in the southern and central regions. Moreover, the peak WS10 (above 3 m s-1) exhibits more significant decreasing trends in various regions than the mean WS10 and the peak WS10 becomes less frequent in a warmer climate. This study further investigates the effects of land use and cover change (LUCC) on the WS10 in different regions by comparing observation and the ERA5 reanalysis, since the ERA5 reanalysis data does not incorporate surface roughness information into its data assimilation system. It is revealed that the impact of LUCC on the mean WS10 exhibits an east-west dipole pattern, with decreased mean WS10 in most areas east of 105°E but increased WS10 in the western regions. In addition, the LUCC could also have contributed to a large decreasing trend in the peak WS10 over most of China, with a particularly significant reduction of -6.8% decade1 in eastern China. This study improves our understanding of the changes in the mean and peak WS10 across China as well as their causes.


AS01-A105
Insights Into Monsoonal Orographic Rainfall in the Eastern Himalayas: Unraveling Dynamics Through Interannual Variability

Pratik KAD#+, Kyung-Ja HA
Pusan National University

The Himalayas are crucial for driving the monsoon and climate system, but the annual river flooding during the monsoon impacts the densely populated downstream of its regions. Previous studies have reported changes in the Himalayas, such as warming, rainfall changes, ice-sheet melting, and extremes. However, due to the complicated orography, quantitatively understanding Himalayan precipitation dynamics on a spatial scale is limited compared to other monsoon regions. Recent studies highlight how melting glaciers and snow, along with monsoonal rains causing recurrent floods, play a significant role in the context of climate change. This study emphasizes interannual variability by examining the last 43 years from the available rainfall observed dataset and illustrated using reanalysis data. We found a robust interannual variability signal in the Eastern Himalayas, where the orographic features and processes dominate. Further analysis indicates that Monsoonal rainfall, rather than melting snow, is the primary factor for these unusually extreme years. The local moist process controls the variability of Himalayan monsoonal rainfall via regional Hadley circulation, connected to walker circulation. Our findings illustrate the wet (dry) response coupled with strong (weak) dynamical circulation in the Eastern Himalayas. Understanding the dynamics and variability of Himalayan monsoon floods will be crucial for predicting and mitigating their impact.


AS01-A103
Projected Changes in Temperature and Rainfall Extremes Over India Using Bias-corrected CMIP6 Simulations

Koteswararao KUNDETI1#+, Vinod Kumar BURI2, Lakshmi Kumar T.V.3, Jasti CHOWARY4, Srinivas DESAMSETTI5
1National Center of Meteorology, 2National Institute of Technology Rourkela, 3SRM Institute of Science and Technology, 4Indian Institute of Tropical Meteorology, 5Ministry of Earth Sciences

Global warming can profoundly impact the mean climate over the Indian subcontinent, which may significantly affect both natural and human systems. This study used thirteen statistically downscaled, bias-corrected, high-resolution data derived from Coupled Model Intercomparison Project Phase 6 (CMIP6) under the Shared Socioeconomic Pathways (SSP) of SSP2-4.5 & SSP5-8.5 scenarios. This study assesses the projected changes in rainfall and along its extremes (rainy days and simple daily intensity) for both the southwest (SW) and northeast (NE) monsoon seasons in the near (2021-2050) and far future (2071-2100) relative to the baseline period (1985-2014). Further, the maximum, minimum, and mean temperature changes and their extremes (highest values in maximum and lowest values in minimum temperatures) for the summer and winter seasons are also studied. Overall, the Multi-Model Mean (MMM) slightly underestimated (overestimated) the SW (NE) monsoon rainfall compared to the observed rainfall in the baseline period, and the biases are statistically not significant. A considerable increase in future rainfall is noticed in most parts of central India, the Himalayan region, and a more than 80% increase in the northwestern parts of India during the SW monsoon season. In the NE monsoon season, south peninsular India is getting more rainfall under SSP5-8.5 than SSP2-4.5. However, both emission scenarios show that rainfall may increase from the mid-future onwards. Interestingly, the number of rainy days is reducing, and rainfall intensity over all the areas of India drastically increases by the end of the 21st century. An increase in maximum temperature of around 4.5°C, and in minimum temperatures is about 5°C in northern parts of India in the 21st century. Overall, the results show a significant contribution of global warming in increasing the frequency and intensity of extreme events, which may have severe implications for the future agricultural, health, and power sectors.


AS01-A018
Quantitative Attribution of Vertical Motions Responsible for the Early Spring Drought Conditions Over Southeastern China

Zejiang YIN+, Song YANG, Wei WEI#
Sun Yat-sen University

The interannual variability and long-term trend of the drought conditions over southeastern China during early spring (from February to April) are investigated by analyzing the standardized precipitation evapotranspiration index in 1979–2020. Results from an attribution analysis show that precipitation deficiency and atmospheric water demand contributes about 96.5% and 6.7% to the drought conditions on interannual time scale, and about 72.8% and 22.3% to the long-term trend, respectively. The precipitation deficiency is primarily contributed by moisture divergence via the descending anomalies throughout the troposphere over southeastern China. A further diagnosis with the omega equation reveals that the descending anomalies are dominated by the strong negative zonal vorticity advection in the upper troposphere and the enhanced meridional cold advection throughout the troposphere. They are controlled by a barotropic anomalous anticyclone over the eastern Tibetan Plateau and an anomalous cyclone over the western North Pacific. Non-negligibly, the contribution of potential evapotranspiration to the drying trend in early spring over southeastern China is about four times larger than that to the interannual variability. Given that potential evapotranspiration may increase in a warming climate, it may be critical for the change in drought conditions in future. This study serves as a basis for fully understanding the severity of recent droughts and for model simulation of the drought conditions over southeastern China.


AS01-A064
Unprecedented Rainfall Intensification Over Western India During the 2019 Summer Monsoon

Sumit K. MUKHERJEE1,2#+, Ayantika DEY CHOUDHURY1, Krishnan RAGHAVAN1, Ramesh VELLORE1, Pulak GUHATHAKURTA3
1Indian Institute of Tropical Meteorology, 2Savitribai Phule Pune University, 3India Meteorological Department

In 2019, large areas of Western India (WI) recorded the highest summer monsoon (June–September) precipitation for over a century, resulting in disastrous floods claiming hundreds of human lives. Our analysis illustrates that widespread heavy rainfall in this region markedly came from three intense rain episodes (IREs), viz. 1) 28 June – 12 July, 2) 24 July – 11 August, and 3) 1 – 14 September, in the backdrop of intense positive Indian Ocean Dipole (pIOD) conditions evolving at the equatorial Indian Ocean. The IREs favorably stemmed from large-scale bands of organized monsoon convection embedded with stratiform precipitating systems. Analysis of GPM satellite swaths brings out the prevalence of stratiform precipitation and elevated latent heating in the precipitating systems. Diagnostic analyses of various ERA5 atmospheric fields were performed to understand the dominant spatial structures during the IRE days. The continual top-heavy stratiform latent heating, in synergy with the pIOD-generated equatorial heating anomalies, forced a Rossby-wave pattern of high mid-tropospheric potential vorticity with the maximum over WI and an associated sizeable cyclonic vortex stretching across South and Southeast Asia (SSEA). Results show that as the east-west gradient of sea surface temperature strengthened at the equatorial Indian Ocean, it induced anomalous equatorial easterlies, in turn enhancing cross-equatorial moisture transport. It fostered large-scale moisture convergence and deep convective ascent, thereby leading to extensive heavy rainfall over much of SSEA. This study highlights the ramifications of intense pIOD manifestations and their potential role in increasing the occurrence of hydrological extremes in WI as well as SSEA in the 21st century.


Thu-03 Aug | 1:10 - 3:10 | MR332
AS36 - Regional Climate Downscaling and Cordex: Challenges and Prospects

Session Chair(s):

AS36-A003 | Invited
Bias Correction of Temperature and Precipitation Over China for RCM Simulations Using the QM and QDM Methods

Xuejie GAO1#+, Yao TONG1, Zhenyu HAN2, Filippo GIORGI3
1Chinese Academy of Sciences, 2China Meteorological Administration, 3The Abdus Salam International Centre for Theoretical Physics

Two different bias correction methods, the quantile mapping (QM) and quantile delta mapping (QDM), are applied to simulated daily temperature and precipitation over China from a set of 21st century regional climate model (the ICTP RegCM4) projections. The RegCM4 is driven by 5 different general circulation models (GCMs) under the representative concentration pathway RCP4.5 at a grid spacing of 25 km using the CORDEX East Asia domain. The focus is on mean temperature and precipitation in December-January-February (DJF) and June-July-August (JJA). The impacts of the two methods on the present day biases and future change signals are investigated. Results show that both the QM and QDM methods are effective in removing the systematic model biases during the validation period. For the future changes, the QDM preserves the temperature change signals well, in both magnitude and spatial distribution, while the QM artificially modifies the change signal by decreasing the warming and modifying the patterns of change. For precipitation, both methods preserve the change signals well but they produce greater magnitude of the projected increase, especially the QDM. We also show that the effects of bias correction are variable- and season-dependent. Our results show that different bias correction methods can affect in different way the simulated change signals, and therefore care has to be taken in carrying out the bias correction process.


AS36-A010
Correcting Multivariate Bias in RCM Boundary Conditions for Improved Simulation of Extremes

Youngil KIM1#+, Jason EVANS1, Ashish SHARMA2
1University of New South Wales, 2UNSW Sydney

The Accuracy of hydro-climatological simulations at fine resolution is 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, their application is hindered by the inherent systematic biases in input boundary conditions, which can be amplified further within the RCM domain. Although recent studies have employed univariate bias corrections on the RCM boundary conditions to reduce the bias, the increasing complexity of these techniques can be limited in simulating extreme events due to a lack of consideration with regard to the physical relationships between the atmospheric variables. Hence, this study evaluates the multivariate bias correction of the RCM boundary conditions on extreme events. The results are compared to RCMs with three univariate bias-corrected boundary conditions, which have been widely used in previous studies. For RCM, the Weather Research and Forecasting model (WRF) with dynamical core (ARW), version 4.2.1, was used. ERA5 reanalysis of the global climate from the European Centre for Medium-range Weather Forecasts (ECMWF) was also used as a reference for bias correction. The downscaling was performed over the Australasian Coordinated Regional Climate Downscaling Experiment (CORDEX) domain. To evaluate the impact of bias correction, two quantitative measures were used: mean absolute errors (MAE) and bias. It is clear from the results that RCM with multivariate bias-corrected boundary conditions represents a generally better simulation of extremes when compared to RCMs with univariate bias-corrected boundary conditions in reducing MAE and bias in the RCM outputs. In contrast, the RCM with uncorrected boundary conditions produces a considerable bias, showing different wet- and dry biases in the tropics.


AS36-A018
Reproducibility Evaluation on High-resolution Downscaled Climate Data Estimated by IGISRM

Chansung OH1+, Jaeyong CHOI2, Jaepil CHO1#
1Integrated Watershed Management Institute, 2Chungnam National University

The main purpose of this study is to prepare countermeasures that can reduce the damage caused by the forest-related disasters. To achieve these objectives, ERA5 reanalysis data are first collected, and high-resolution gridded data (100m interval) are produced using the statistical downscaling scheme model of IGISRM (Improved GIS-based Regression Model). The produced data are projected through a series of daily-based bias correction using the ASOS (Automated Surface Observing System), and then a series of reproducibility evaluations has performed using the AWS (Automated Weather Station) and on-site PT (precise temperature) 9 monitoring data. The results of the reproducibility evaluation using AWS data show that the precipitation have a low reproducibility as it shows a tendency to underestimate the observed temporal fluctuations and rainfall amounts. However, The Correlation Coefficients and scatter plot of Slope of maximum and minimum temperature are close to 1 with an NRMSE near 0, showing the excellent estimation performance of the produced high-resolution gridded climate data. On the other hand, the evaluation results using temperature monitoring data show that the statistical efficiency of min. temperature was somewhat less compared to that of max. temperature even though it has a value under 0.5 of NRMSE. In addition, according to the comparison of temperature between the points and downscaled gridded points during the measurement period (May 2021 ~ April 2022), the max. temperature is slightly underestimated overall, while the min. temperature shows overestimated compared to the actual measured value in the winter season (after November) when the temperature drops sharply.


AS36-A023
Improvement of a 1-month Prediction in South Korea Using Dynamical Downscaling and a Time-lagged Ensemble Method

Subin HA1+, Eun-Soon IM2#, Jina HUR3, Sera JO3, Kyo-Moon SHIM3
1The Hong Kong University of Science and Technology, 2HKUST, 3National Institute of Agricultural Sciences

Dynamical downscaling has been well recognized as a useful tool to improve simulations of global climate models (GCMs) by better resolving geographical details and fine-scale climate processes. Meanwhile, a time-lagged ensemble is a common approach to improve forecasts, providing a range of possible future meteorological conditions and reflecting the uncertainty arising from a single deterministic forecast. In this regard, this study aims to construct an optimal time-lagged ensemble with an adequate number of members for 1-month prediction in South Korea using NCEP Climate Forecast System version 2 (CFSv2) operational forecasts initialized at different times. Systematically selected members that can represent the ensemble spread are then downscaled using the Weather Research and Forecasting (WRF) modeling system customized over Korea. Various quantitative metrics are used to compare the performance of between deterministic and ensemble predictions derived from CFSv2 and WRF-based downscaling products. The results of this comparative assessment can illustrate the effectiveness of dynamical downscaling and a time-lagged ensemble when it comes to improving prediction accuracy. 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. [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.


AS36-A026
A Study on the Synoptic and Mesoscale Changes of Upward motion Affecting Future Precipitation Changes on the Korean Peninsula

Tae-Min KIM#+, Eun-Chul CHANG, Namgu YEO, Jaedeok LEE, Ui-Yong BYUN, Joowan KIM
Kongju National University

According to the IPCC AR6, global temperature and precipitation increase under global warming caused by the release of greenhouse gases. In particular, gradual increase of precipitation over East Asia is expected in the future climate change scenarios. For rainfall formation, water vapor condensation which induced by adiabatic cooling with vertical updraft is required. Therefore, examining the change of vertical motion is necessary to analyze precipitation change in future climate. This study investigates the downscaled regional climate change information from the Coordinated Regional Climate Downscaling Experiment (CORDEX) East Asia (EA) to figure out changes in summer precipitation over the Korean Peninsula. The Global/Regional Integrated Model system (GRIMs) Regional Model Program (RMP) is used for the dynamical downscaling of global climate model output from coupled model intercomparison project phase 6 (CMIP6) in shared socioeconomic pathway (SSP) scenarios. In the extreme warming scenarios, more increased EA summer precipitation is simulated compared to the current climate. Through spatial filtering, vertical motion is separated into mesoscale and synoptic scales. Three forcing terms (i.e., the vorticity advection, the temperature advection, and the diabatic heating) for the quasi-geostrophic omega equation are analyzed to explain contributions to the synoptic-scale vertical motion. In both mesoscale and synoptic-scale, vertical movement increased in areas where precipitation increased. In the synoptic scale, the contribution of the diabatic heating term on vertical motion is the largest and in the order of vorticity advection forcing and temperature advection forcing. This work was funded by the Korea Meteorological Administration Research and Development Program under Grant KMI2022-00410. And the main calculations in this study were performed using supercomputing resources provided by the Korea Meteorological Administration (National Center for Meteorological Supercomputing).


AS36-A020
A Study on Global Warming Impact on Extreme East Asian Summer Monsoon in 2020 Using Regional Climate Model

Tae Ho MUN#+, Dong-Hyun CHA
Ulsan National Institute of Science and Technology

The East Asian summer monsoon (EASM) recorded extremely high precipitation in 2020, causing enormous human and property damage to Korea, China, and Japan. Therefore, understanding the factors which influence in the variability of the EASM and investigating the potential causes of the extreme 2020 EASM event is important. This study analyzed the effects of global warming on synoptic-scale circulation, which is the cause of the extraordinary EASM in 2020, using regional climate model experiments. The control experiment simulated precipitation patterns such as those of the EASM and the Western North Pacific summer monsoon during summer reasonably. In sea surface temperature (SST) sensitivity experiments, which added or subtracted the trend of increasing SST due to global warming, a positive correlation was confirmed between SST and precipitation change in the tropics. In contrast, the EASM region showed a negative correlation, and its magnitude was smaller than that of the tropics. The pattern of increasing SST due to global warming provided sufficient moisture to the tropical region and strengthened the convection. This increased the SST gradient between the Indian Ocean and Northwest Pacific, causing westerly wind anomalies and resulting in strong convection activity in the South China Sea. This mechanism refers to strengthening the local Hadley cell, thereby dynamically inhibiting convection in East Asia, and vice versa. Through this study, it is possible to investigate the changes in synoptic fields and the regional effects of increased SST due to global warming that can affect the East Asian summer monsoon.


AS36-A027
Simulation of Extreme Hydrometeorological Events Over Southern China by a Regional Climate Model

Michael SANDERSON1#, Kalli FURTADO2+, Nicholas SAVAGE1, Grace REDMOND1, Erasmo BUONOMO1
1Met Office, 2Centre for Climate Research Singapore

China has experienced rapid urbanization over the past few decades, especially in the Pearl River delta located in Guangdong province in the south of China. This has placed significant strains on water and energy resources, particular in the wake of climate extremes. For example, in 2022 a severe heat wave affected this region, meaning energy production was reduced whilst energy demand soared. Evaluating the ability of climate models to predict such regional hydrometeorological extremes is therefore a pressing concern. Currently, however, it is unclear whether current models are adequate for such a purpose, or that their predictions can support better services or decisions in the region. Here, we evaluate a regional climate model (RCM) simulation over Guangdong province, focusing on simulations of heat waves and droughts.
The RCM was executed with a horizontal resolution of 12 km using a domain that included all of China and the nearby ocean. RCM data for Guangdong province were compared with a gridded dataset (CN05.1) containing daily values of temperature and precipitation. Heat waves were studied using daily maximum temperatures averaged over Guangdong province. In both the modelled and observed data, heat waves have appeared earlier and later in the year from 1975 to 2010. The modelled heat wave durations were similar to those observed, although the model did not capture the positive trends in numbers and lengths of heat waves.
Droughts were studied by applying run theory to monthly precipitation anomalies from the observations and RCM. The numbers and durations of droughts were similar in the modelled and observed data, although the RCM did not capture the observed spatial pattern in durations. The intensities (related to the rainfall deficits) were also similar. Overall, the RCM has some skill in simulating climate extremes over Guangdong province.


Thu-03 Aug | 1:10 - 3:10 | MR335
AS52 - Ionospheric Space Weather Monitoring and Forecasting

Session Chair(s): Haixia LYU, Wuhan University

AS52-A002 | Invited
Structure of Post-midnight Enhancements in Ionospheric Electron Density at Low Latitudes

Libo LIU#+
Institute of Geology and Geophysics, Chinese Academy of Sciences

Night-time enhancement in the ionosphere is a fantastic feature of the diurnal variation of the ionosphere. It is a challenging issue to answer the spatial coverage of the enhancement in the ionosphere will appear during an event. We conduct a case study to explore the spatial presence of the post-midnight enhancements of electron density (Ne) in the low latitude ionosphere. The total electron content (TEC) data are retrieved from the Beidou Geostationary Earth Orbit (GEO) satellite signals recorded by a network of Global Navigation Satellite System (GNSS) receivers in Asia-Australia, and the F2-layer peak parameters and the altitudinal profiles of Ne are measured by the ionosonde and incoherent scatter radar at Sanya (109.6° E, 18.3° N). At Sanya, when the F2-layer peak Ne (NmF2) rises in the post-midnight hours, common features occur, including a descent of the peak height (hmF2) and the Ne increase on the bottom side and reduction at topside altitudes, respectively. However, GEO-TEC does not always consistently follow the enhancement of NmF2 case by case. Further, the enhancement is present in a limited area. The GEO-TEC enhancements may peak roughly simultaneously in an event or with significant time shifts in the west-east direction; it is possible that the enhancement is not present in all GEO-TECs. In some studied cases, the low latitude enhancements show a hemispheric asymmetry. They are clustered mainly in the northern hemisphere and usually have no corresponding magnetic conjugate features in the southern hemisphere. It implies that the physical drivers, not only the electric field, are responsible for the limited spatial presence of post-midnight enhancements in the low latitude ionosphere.


AS52-A014
On the Contribution of Plasmasphere to the TEC on the Ground

Shigeto WATANABE#+
Hokkaido University

Is the plasmaspheric plasma essential to the improvement of positioning accuracy by GNSS? How much plasma in the plasmasphere contributes to the TEC on the ground? To investigate the plasma in the plasmasphere and to understand the physical processes of various phenomena occurring in the ionosphere and plasmasphere of the earth, we have constructed three ionosphere/plasmasphere models: an empirical model, a physical model, and a deep learning model. From the electron densities at altitudes below 30,000km from the upper-hybrid resonance (UHR) emissions obtained by the plasma wave experiments on Akebono, Arase, and Hinotori satellites, which consist of more than 4 million datasets in the ionosphere and plasmasphere regions, the empirical model of electron density distribution in the topside ionosphere and the plasmasphere has been constructed using simple base functions with the parameters of longitude, latitude, local time, season, and solar/magnetic activities. The empirical model is also used as the assimilation data of the physical model of the Plasmasphere Thermosphere Model (PTM), which calculates the densities, velocities, and temperatures of O+, He+, and H+ at altitudes from 100 km to 10 Re. We have also applied to make a model with deep learning because the amount of the observation data in space is still insufficient to construct the earth’s ionosphere and plasmasphere. The model includes the memory effects of plasmasphere structure and dynamics affected by geomagnetic disturbance. We will present the comparisons of the ionosphere and plasmasphere electron densities estimated from our models with the total electron content (TEC) on the ground and the 2020 International Reference Ionosphere (IRI) model.


AS52-A003
An Additional Plasma Density Peak at Poleward of the Equatorial Ionization Anomaly Crests Observed by Swarm

Chao XIONG#+, Yuyang HUANG
Wuhan University

The equatorial ionization anomaly (EIA) is one of the most important phenomena at equatorial and low latitudes, which is caused by the daytime eastward electric field via E×B effect. The well-developed EIA at dayside is thought to be a quite large structure with two crests extending to ±15° magnetic latitude, and the plasma density distributes quite smooth along the magnetic fluxtube. However, an additional density peak at poleward of the EIA crests is sometimes observed from the high-resolution plasma density measurements of Swarm. The additional peak is observed at the poleward of EIA crest only in the summer hemisphere, and shows a local time preference between 09:00 and 24:00. From a global view, the additional peak has relatively large occurrence at the norther hemisphere in the pacific longitudes. From the perspective of constellation, the Swarm B can revisit the same longitude of Swarm A/C, though with a certain time day. The delay time gradually increases from a few minutes to a few hours. By comparing the location of the additional peak observed by Swarm B and Swarm A/C, we found the peak keeps at a rather constant latitude irrespective of the delay time between Swarm satellites. Possible drivers for causing such additional peak have been further discussed.


AS52-A010
An Investigation of the Tonga Volcanic Eruption Effects on GNSS Precise Point Positioning

Xiaomin LUO1+, Zichun XIE1, Dezhong CHEN2#
1China University of Geosciences, 2Wuhan University

On 15 January 2022, a great volcanic eruption at Hunga Tonga-Hunga Ha’apai produced various waves propagating globally, disturbing the background atmosphere and ionosphere. Using more than 1100 GNSS stations datasets collected at Asia-Pacific region, this study investigates the Tonga volcanic eruption effects on GNSS measurements and precise point positioning (PPP). During the Tonga volcanic eruption, the positioning results of GNSS kinematic PPP vary significantly and the range can reach several meters in the east, north, and up directions. The Rate of Total Electron Content (TEC) Index (ROTI) maps and scintillation indexes indicate that the ionospheric anomalies during this volcanic eruption should include not only the ionospheric disturbances but also the ionospheric irregularities. It is found that these ionospheric anomalies did not cause large fluctuations of the C/N0 and multipath values, but the number of cycle slips increased obviously. Statistical results indicate that the mean value of the cycle slip occurrence rate on volcanic day is 17.2%, while that on ionospheric quiet day is only 10.4%. By expanding the cycle slip detection thresholds in PPP solution, it is found that the PPP results of several stations can be improved under the Tonga volcanic eruption conditions. However, based on 357 stations data, the PPP performance with the expanded thresholds and the default thresholds are generally comparable. Statistics indicate that the average RMS values of PPP with the expanded (default) thresholds are 0.030 m (0.026) and 0.052 m (0.053 m) in the horizontal and vertical directions, respectively. That means only expanding the cycle slip thresholds cannot fundamentally improve PPP performance under the Tonga volcanic eruption conditions.


AS52-A016
Seismo-ionospheric Anomalies Before Assam Earthquakes (Mw = 6.0) Detected by GIMs and GPS-TEC

Uma PANDEY#+, Javed MALIK, Onkar DIKSHIT, B. NAGARAJAN
Indian Institute of Technology Kanpur

Ionospheric and atmospheric anomalies registered around the time of earthquakes in low-latitude regions are reported now regularly. Majority of these reports have the character of case studies without clear physical mechanism proposed. In this paper, we analyze the TEC data for April 2021 observed at ground station, Dibrugarh University, Assam to examine the effect of earthquake of magnitude Mw = 6.0 which occurred on 28 April 2021 at Assam. We process the TEC data. The anomalous enhancements and depletions are found in TEC data on 1–15 days before the occurrence of event. The aims of this study understand atmospheric system during earthquake preparatory processes through features of Total Electron Content (TEC) taken by GNSS-GPS. An anomaly crests station. The impact on pre-earthquake TEC variations over Dibrugarh the low-latitude ones show their imprints on TEC even when their epicenters lie at 500–600 km longitudinal separation. This paper discusses how electric field generated in the earthquake preparatory processes works in a complex manner at the equatorial anomaly zone in a way similar to electro jet current system, leading to changes in ionospheric parameters. Finally attempts are made to understand the situation prior to and during a seismic event by assigning parameters with special reference to IRI model, for obtaining the observed results. 


AS52-A006
Ionospheric Irregularities Monitoring and its Impacts on Precise Point Positioning

Wei LI1,2+, Shuli SONG1#
1Shanghai Astronomical Observatory, Chinese Academy and Sciences, 2State Grid Siji Location Service Co., Ltd., State Grid Communication Industry Group Co., Ltd

The ionosphere is an important part of the upper atmosphere. Its activities directly affect the state of the space weather and the related applications that rely on radio communications, e.g., Global Positioning System (GPS) or Global Navigation Satellite System (GNSS). Ionospheric irregularities within the ionosphere cause GPS/GNSS signals scintillation, loss lock, and cycle slip and thus further degrade the performance of GPS/GNSS applications, e.g., Precise Point Positioning (PPP). Thus, it is of significant interest to monitor ionospheric scintillation and further study the influence mechanism of ionospheric irregularities on PPP for space environment monitoring and GPS/GNSS applications. In this contribution, we summarized the limitations of ROTI (Rate of change of TEC Index) in monitoring ionospheric scintillation and evaluated the performance of ROTI in monitoring ionospheric scintillation in the aspect of correlation, integrity, and reliability. In addition, we investigated the impacts of ionospheric irregularities on the performance of kinematic PPP in China. The results show that the sampling rate of observations is the key to the performance of ROTI in monitoring ionospheric scintillation. ROTI calculated from 1s-data (1s/sample) has better performance (integrity of 90%, correlation with S4 of 0.8-0.9, reliability of 88%) than that from 30s-data (30s/sample) (integrity of 60%, correlation with S4 of 0.7-0.8, reliability of 80%). The results of the kinematic PPP show that the ionospheric irregularities caused increased positioning errors (decimeter- to meter-level), enlarged phase residuals (decimeter-level), and increased cycle slips in PPP processing in low latitude regions of China. By proposing a novel strategy, we present direct evidence of the falsely detected cycle slips in 30s-data by the traditional cycle slip detection threshold in PPP processing. We reveal that the falsely detected cycle slips are dominantly responsible for the degradation of kinematic PPP solutions during the period of ionospheric irregularities.


Thu-03 Aug | 3:30 - 5:15 | MR311
AS40 - Middle Atmosphere

Session Chair(s): Shigeo YODEN, Kyoto University, Hye-Yeong CHUN, Yonsei University

AS40-A001 | Invited
Atmospheric-dynamical Impacts of the 2022 Hunga Tonga Volcanic Eruption

Corwin WRIGHT#+
University of Bath

The January 2022 Hunga Tonga–Hunga Ha’apai eruption was one of the most explosive volcanic events of the modern era, producing a vertical plume that peaked more than 50 km above the Earth. The initial explosion and subsequent plume triggered atmospheric waves that propagated around the world multiple times, attracting significant media and public attention. In addition to the initial explosion, latent heat release from the plume remained the most significant individual atmospheric wave source worldwide for more than 12 h, producing circular wavefronts visible across the Pacific basin in satellite observations. In this talk, I will describe and discuss these waves and the observations made of them using a diverse range of satellite and ground-based datasets from the surface to the edge of space, highlighting the ability of the modern international satellite constellation and ground-based instrumentation to make rapid measurements of unique extreme events such as this. I will also quantify just how unique this event was relative to our multi-decade record of the atmospheric wave climatology, and describe how the eruption represents a key natural experiment in how the atmosphere responds to a sudden point-source-driven state change, which will be of use for improving weather model physics.


AS40-A005
Examining the Sudden Stratospheric Warming Events in High-top and Low-top Climate Model Large Ensembles

Yu-Chiao LIANG1#+, Yih WANG1, Young-Oh KWON2, Claude FRANKIGNOUL3, Lorenzo POLVANI4, Lingling SUO5
1National Taiwan University, 2Woods Hole Oceanographic Institution, 3Sorbonne University, 4Columbia University, 5Nansen Environmental and Remote Sensing Center and Bjerknes Center for Climate Research

Sudden stratospheric warming (SSW) events, followed by a characteristic circulation regime in the lower troposphere, are crucial for the subseasonal weather prediction. One issue remains controversial is whether or not increase in the height of top layer and vertical resolution in the stratosphere in a climate model improves the representation of SSW events and the subsequent influences on the near-surface climate. This study compares the SSW events simulated by a high-top climate model (the Whole Atmosphere Community Climate Model version 6, WACCM6) and those from the corresponding low-top model (Community Atmosphere Model version 6, CAM6) with large ensembles. The two sets of 30 member ensemble simulations are forced by identical observational sea-surface temperature and sea-ice concentration, and radiative forcings, during the 1979-2013 period. We find that WACCM6 produces about two times more SSWs than CAM6. In terms of occurrence frequency, SSWs in WACCM6 happen about 7 times per decade, consistent with the frequency in reanalysis datasets. Analyses on the dynamical indicators of SSWs, including the sea-level pressure precursor, the preceding Eliassen-Palm fluxes into the stratosphere, and the associated downward impacts on the troposphere, reveal that WACCM6 compares more favorably with reanalysis datasets, and that CAM6 overestimates them. This is likely due to the more realistic stratospheric background circulation in WACCM6. We also find that the differences between WACCM6 and CAM6 can be amplified during the years with El Niño and La Niña events. Finally, we perform the vortex moment diagnostics to gain insights into the vortex structure and to separate the SSWs into splitting and displacement types. The diagnostics show that the geometry and the centroids of WACCM6 polar vortex are much closer to those from reanalysis data. Overall, our results suggest that the high-top configuration leads to more realistic SSWs and the subsequent near-surface impacts than the low-top configuration.


AS40-A015
Precursory Analysis Ensemble Spread Signals That Foreshadow Stratospheric Sudden Warmings

Akira YAMAZAKI1#+, Shunsuke NOGUCHI2
1Japan Agency for Marine-Earth Science and Technology, 2Kyushu University

Behaviors of analysis ensemble spreads were investigated during stratospheric sudden warming (SSW) events in an atmospheric general circulation model–ensemble Kalman filter (LETKF; the local ensemble transform Kalman filter) reanalysis system, in which the model resolves the stratospheric circulations. Precursory signals of the increased spreads in the reanalysis system were found a week to a few days prior to stratospheric sudden warming events occurred during December 2018 and August–September 2019 in both hemispheres. The signals did appear in upper and middle stratosphere and did not below the lower stratosphere. When the signals appeared analysis increments became substantial against forecast updates in the forecast-analysis cycles; it is found that the precursory signals help to reproduce SSWs accordingly. An empirical orthogonal function analysis showed that the dominant structures of the precursory signals were equivalent barotropic and were 90-degree out of phase with the analysis ensemble-mean field. In the same timing the meridional gradients of absolute or potential vorticity in the middle stratosphere became temporally reversed. Hence, the spread signals can be equivalent to barotropic instability modes in the ensemble perturbation fields associated with SSWs.


AS40-A017
Interactions of Stationary Planetary Waves During Sudden Stratospheric Warmings

Kseniia DIDENKO#+, Andrey KOVAL, Tatiana ERMAKOVA
St Petersburg University

Planetary-scale waves, in particular, stationary planetary waves (SPW) are one of the main objects of stratosphere dynamic researches. Interacting with the mean flow, the SPW lead to the deceleration (sometimes even reversal) of the stratospheric jet stream during winter on one side and the conditions of their propagation depend on the mean flow on the other. As a result, so-called stratospheric vacillations occur, i.e., irregular amplitude variations of the SPW and the intensity of the mean flow. Such effects are mainly due to nonlinear wave-wave and wave-mean flow interactions in the stratosphere. Nonlinear interactions are most clearly exerted during sudden stratospheric warming (SSW) – strong thermodynamic phenomena in the winter polar stratosphere that affects the middle atmosphere and also causes significant changes in the troposphere, mesosphere, and lower thermosphere. The emergence of SSW is associated with the propagation of planetary waves from the troposphere to the stratosphere and their further interaction with the zonal circulation. An analysis of wave-wave and wave-mean flow interactions during winter 2008-2009 and 2018-2019 sudden stratospheric warmings was made using the equation of perturbed potential enstrophy. It is shown that wave-wave interactions make the least contribution to the wave activity variation during the 2008-2009 SSW, the contribution of all interactions is comparable during the 2018-2019 SSW. The research is supported by the Ministry of Science and Higher Education of the Russian Federation (Agreement 075-15-2021-583).


AS40-A008
Studying Global Ozone Variability and Long-term Trends with Suomi NPP OMPS Measurements

Natalya KRAMAROVA1#+, Stacey FRITH1,2, Jerald ZIEMKE1
1NASA Goddard Space Flight Center, 2NASA Science Systems and Applications, Inc.

The Ozone Mapping and Profiler Suite (OMPS) includes three ozone sensors – Nadir Mapper (NM), Nadir Profiler (NP) and Limb Profiler (LP) - to measure total and vertical ozone distributions globally. The combination of limb stratospheric profile and nadir total column observations also enable measurements of tropospheric ozone columns. The first OMPS instrumental suite was launched on board of Suomi National Polar Partnership (SNPP) satellite in October 2011, followed by two more OMPS suites launched on boards of NOAA-20 (with two nadir sensors only) and NOAA-21 satellites in November 2017 and November 2022, respectively. Observations from OMPS are aimed to extend the NASA long-term ozone climate records from TOMS, OMI, SBUV, MLS and SAGE instruments. In this presentation, we will analyze the decadal record from the SNPP OMPS sensors. The combination of OMPS ozone measurements can be used to trace changes in the atmospheric circulation associated for example with the polar vortex, Quasi-Biennial Oscillation (QBO), El Nino Southern Oscillation (ENSO). We will demonstrate the OMPS capability to accurately measure ozone distribution over polar latitudes during ozone depletion seasons using a combination of profile and column sensors. During the SNPP lifetime, we observed several large and deep polar ozone depletion events (e.g. 2019-2020 over the Arctic and 2020, 2021, and 2022 in the Antarctic), driven by weaker than average planetary wave activity. In the last decade, we also observed a number of major sudden stratospheric warming events (e.g. 2019 over Antarctica). Ozone profile observation with the OMPS LP allows to accurately determine the layer with the maximum ozone depletion, while total ozone from OMPS nadir sensors can determine the spatial extend of the depletion. Finally, we will discuss long-term trends in ozone profile and tropospheric and total columns as observed by OMPS sensors.


AS40-A002
Study of the Ozone Layer Evolution in the Past and Future with ESM SOCOLv4

Eugene ROZANOV1,2#+, Timofei SUKHODOLOV1, Tatiana EGOROVA1, Jan SEDLACEK1, Arseniy DOYENNEL3
1World Radiation Center, 2ETH Zürich, 3Vrije Universiteit Amsterdam

The ozone layer was damaged by halogen containing ozone-depleting substances (hODS) of anthropogenic origin. The majority of the chemistry-climate models projected the recovery of the ozone layer around 2040 due to the regulations introduced by the Montreal Protocol and its Amendments. In this paper, we discuss the ozone behavior from 1980 to 2100 simulated with the Earth system model SOCOLv4. We demonstrate and explain past ozone layer trends in the atmosphere elucidating the role of greenhouse gases and hODS. We also present the future behavior of the ozone layer taking into consideration very-short lived species, newly discovered ozone-depleting substances, solar and volcanic activity, two IPCC scenarios of anthropogenic activity (SSP2-4.5 and SSP5-8.5), as well as possible climate interventions. In both scenarios, the model projects a decline in tropospheric ozone in the future due to a decrease in ozone precursors. The ozone also increases in the mesosphere, upper and middle stratosphere, however in the lower stratosphere it is observed only over high latitudes. Under SSP5-8.5, the ozone increase in the stratosphere is larger due to stronger cooling and suppression of catalytic ozone destruction cycles.
In contrast, in the tropical lower stratosphere ozone concentration decreases in both experiments while increasing over extratropic due to the intensification of meridional transport, which is stronger in SSP5-8.5. The future total column ozone exceeds present values in mid-to-high latitudes but declines in the tropics. Thus, the stratospheric ozone evolution in the 21st century is strongly governed not only by a decrease in hODS but also by future greenhouse forcing. The tropospheric ozone changes due to the changes in ozone precursors, also have a strong impact on the total column. Therefore, even though the anthropogenic halogen loading problem is resolved, the future ozone column changes are unclear and largely depend on diverse future human activities.


AS40-A020
Study of Factors Influencing Polar Ozone in the Southern Hemisphere Using CCM SOCOL-3: Solution of the Problem with Satellite Data

Andrey MIRONOV1#, Eugene ROZANOV2,3+, Vladimir ZUBOV4
1St Petersburg University, 2World Radiation Center, 3ETH Zürich, 4Voeikov Main Geophysical Observatory

Comparison of the results of numerical modeling of atmospheric ozone using the chemistry-climate model (CCM) SOCOL-3 with the corresponding measurements from the IASI (Infrared Atmospheric Sounder Interferometer) satellite instrument shows significant differences in total ozone for the polar regions of the Southern Hemisphere. This problem is common for chemical-climatic modeling of the Earth ozone layer. To resolve this problem and to assess the role of the main physical and photochemical processes affecting the annual cycle of polar ozone in the Southern Hemisphere, we carried out a number of numerical experiments, changing the following model parameters: 1) the rate of ozone photodissociation at large zenith angles of the Sun; 2) the rates of stratospheric heterogeneous reactions under polar night conditions; and 3) the intensity of meridional mixing on the sub-grid scales of the model in the region of the circumpolar vortex. Comparison of the results of these experiments with the corresponding IASI measurement data showed that the most important characteristics for improving ozone modeling are the rate of ozone photolysis at high zenith angles and the intensity of horizontal mixing at subgrid scales. A reasonable adjustment of these factors has made it possible to significantly improve the model representation of the annual ozone cycle over the polar region in the southern hemisphere. The work was carried out at the St. Petersburg State University "Laboratory for the Study of the Ozone Layer and Upper Atmosphere" under contract 075-15-2021-583.


Thu-03 Aug | 3:30 - 5:15 | MR323
AS42 - Weather Radar Networks And Their Applications For High-Impact Weather Observations and Warnings

Session Chair(s): Wen-Chau LEE, UCAR, Haonan CHEN, Colorado State University

AS42-A016
Microphysics of Heavy Rainfall Observed During the Prediction of Rainfall Extremes Campaign In the Pacific (PRECIP) 2022

Michael BELL#+
Colorado State University

The Prediction of Rainfall Extremes Campaign In the Pacific (PRECIP) collected novel observations in East Asia during the 2022 spring and summer to improve our understanding of the multi-scale dynamic, thermodynamic, and microphysical processes that produce extreme precipitation. The campaign was designed to maximize the chances of observing a variety of heavy rainfall events in the moisture-rich natural laboratory of the western North Pacific in order to find the commonalities across different weather phenomena. The U.S. instrumentation included the Colorado State University SEA-POL radar, radiosondes, disdrometers, and the National Center for Atmospheric Research S-Pol radar and three MicroPulse Differential Absorption LIDARs (DIALs). PRECIP was conducted in from May to August 2022 in partnership with the Taiwan TAHOPE and Japan T-PARCII experiments, which included research X-band radars and the operational Central Weather Bureau and Japan Meteorological Agency radar networks. An overview of the project and analysis of the new radar observations will be presented. Composites of microphysical characteristics retrieved from range-height vertical scans across a wide spectrum of precipitation events are combined with thermodynamic measurements from the radiosonde and DIALs over the 3-month project. The presentation will highlight the new field observations obtained from the field campaign radar network and the implications for improving our understanding of heavy rainfall.


AS42-A014
Different Types of Coastal Barrier Jet Associated with Landfalling Typhoon

Yucheng KAO1+, Ben Jong-Dao JOU2#
1Central Weather Bureau, Taiwan, 2National Taiwan University

The typhoon induced coastal barrier jet (CBJ) is a unique mesoscale phenomenon in mountainous Taiwan island. Kao et al. (2019) conducted a case study to great detail document the structural features and evolutions of CBJ, explored the CBJ formation mechanism by using Doppler radar and surface mesonet observations. Kao and Jou (2022) further suggested the CBJ is key factor that caused the inner core structural and intensity dramatic change of a landfalling typhoon between 3 hours period. In this study, the CBJ associated with six westbound landfalling typhoons with different track, intensity and size in Taiwan are examined to further clarify the control factor of CBJ structure and evolution. The analysis results show that the incident angle of onshore flow determines the CBJ location, the mountain height, windward slope and onshore flow speed determine the strength of CBJ, the typhoon size determines the duration of CBJ. The CBJ features are also affected by passing rainbands. Systematic collecting and analyzing CBJ in different typhoon environment provide an important information to better understand the behavior of landfalling typhoon in Taiwan area. Reference: Kao, Y.-C. and B. J.-D. Jou, 2022: Mesoscale Circulation and Intensity Changes of a Landfalling Typhoon: Role of the Coastal Barrier Jet. Mon. Wea. Rev. 150, 3325-3346. Kao, Y.-C., B. J.-D. Jou, J. C.-L. Chan and W.-C. Lee, 2019: An observational study of a coastal barrier jet induced by a landfalling typhoon. Mon. Wea. Rev., 147, 4589-4609.


AS42-A021
Improving Short-term High-impact Weather Prediction by Assimilating Reflectivity Mosaics of China Next Generation Weather Radar Network

Sheng CHEN1#+, Junjun HU2, Jinkai TAN3
1Northwest Institute of Eco-Environment and Resources, Chinese Academy of Sciences, Lanzhou 730000, China, 2Chinese Academy of Sciences, 3Sun Yat-sen University

Hight-impact weather occurs more and more frequently as the climate changes, and usually causes severe losses of properties and lives. Accurately prediction of high-impact weather can provide the governments of different levels with reference for decision-making of risk management, and helps common people take corresponding actions for their regular daily life plans. The technology of numerical weather prediction (NWP) develops rapidly as the advancement of remote sensing and computer science, which can give people better and better prediction of high-impact weather with different lead time lengths from hourly scale to daily and monthly scales. Observations of weather radar network are the most important data sources to improve the skills of NWP models such as Weather Research and Forecast (WRF). In China, common people and most of researchers are hard to access the weather radar base data due to the restriction of data policy. In order to investigate the predictability of high-impact weather over China, in this study, we assimilate the reflectivity mosaics of China Next Generation Weather Radar (CINRAD) Network with WRF to predict high-impact weathers over China. Results show that the assimilation of CINRAD reflectivity mosaics can significantly improve prediction skills of high-impact weathers, including local strong convection storms, squall lines and typhoons.


AS42-A022
Microphysical Responses of Snow Clouds to Kelvin-Helmholtz Wave During ICE-POP 2018

Kwonil KIM1, Chia-Lun TSAI2, Gyu Won LEE3#+
1Stony Brook University, 2Chinese Culture University, 3Kyungpook National University

An environment of strong wind shear and weak static stability is a favorable condition for the Kelvin-Helmholtz (KH) wave development. Advanced high-resolution measurements from microphysical instruments (radar and airborne instruments) suggested that the KH wave influences the microphysical processes and contributes to the increased precipitation at the surface. In mixed-phase clouds, in particular, snow growth by additional microphysical processes such as riming, aggregation, or secondary ice production has been revealed. The major processes are primarily determined by the environmental condition of the areas where the KH wave exhibits. Due to limited observations, the microphysical processes associated with the KH wave have yet to be fully investigated. This study will add to the existing knowledge base by presenting new observational evidence of the microphysical impact of the KH wave under two contrasting environments: a speed shear environment with a colder temperature (SKH) and a directional shear environment with a warmer temperature (DKH).
This study uses comprehensive in-situ and remote-sensing measurements collected during the ICE-POP 2018 (International Collaborative Experiments for Pyeongchang 2018 Olympic and Paralympic winter games) field campaign. Vertical velocity fluctuations within the identified KH wave modulated radar moments (e.g., Z, ZDR, and ρHV) and Doppler spectrum characteristics within and beneath the KH wave. The polarimetric variables, Doppler spectrum, and particle size distribution at the surface imply that the KH wave in SKH contributes to secondary ice production (SIP) by ice-ice collision. The KH wave in DKH exhibited persistent waves with much stronger amplitude due to the sustained directional shear environment. The KH wave in DKH suggested the additional SIP by sublimation and activation of ice-nucleating particles.

ACKNOWLEDGMENT
This work was supported by the National Research Foundation of Korea (NRF) grant funded by the Korea government (MSIT) (No. 2021R1A4A1032646).


AS42-A012
Early Detection of Rapidly Developing Convective Echoes Using a Ka-band Radar

Rie NAKAZAWA1, Taro SHINODA1#+, Tadayasu OHIGASHI2, Kosei YAMAGUCHI3, Haruya MINDA1, Moeto KYUSHIMA1, Kazuhisa TSUBOKI1
1Nagoya University, 2National Research Institute for Earth Science and Disaster Resilience, 3Kyoto University

Rapidly developing convective precipitation clouds are brought about flash floods, thus early detection of those is one of important goals for the radar meteorology. A Ka-band radar enable us to detect early development of precipitating clouds by utilizing shorter wavelength radio wave (about 8.6 mm) in comparison with typical meteorological radars. We installed a Ka-band radar at Kobe City in summer season in 2018. The Ka-band radar can detect -17 dBZ as the minimum reflectivity. Continuous sector PPI observations by 90 deg. azimuthal scan with 8 elevation angles were conducted every 2 min. Reflectivity values obtained by the Ka-band radar are projected on the horizontal plane and vertically averaged reflectivity (VAR) is calculated at each grid (horizontally 50 m times 50 m size). We define the developing convective echo as the maximum rainfall intensity exceeds 20 mm/h in an isolated convective precipitation region obtained every 1 min by the X-band radar network. Total 12 convective echoes are analyzed by time series of VAR on August 6 and 16, 2018. Two echoes are evaluated as the developing convective ones. We cannot recognize the significant difference of time series of VAR between 2 developing echoes and other 10 non-developing ones. However, time series of the area of VAR of developing echoes are clearly larger than those of non-developing ones. By confirming time series of VAR, the developing echoes tend to merge the surrounding small/weak echoes and rapidly increase their area. As the increasing rate of the VAR area tends to exceed 4 km2 in 2 min, the convective echoes develop as the developing precipitation cell detected by an X-band radar. As a result, using high sensitivity and frequent continuous PPI observations, we have possibility to conduct early detection of rapidly developing convective echoes.


AS42-A009
Comparison of Microphysical Characteristics of Warm-sector and Frontal Heavy Rainfall During Pre-summer Rainy Season in South China

Xiantong LIU#+
Guangzhou Institute of Tropical and Marine Meteorology, China Meteorological Administration

Warm-sector heavy rainfall (WR), frontal heavy rainfall (FR) and shear-line heavy rainfall (SR) are three types of rainfall that often occur during the pre-summer rainy season in South China. In this study, based on the merged observations from 11 S-band polarimetric radars in South China, differences in microphysical characteristics are investigated for the heavy rainfall event during 10-15 May, 2022. The conclusions are as follows: (1) WR has the highest radar echo top height, the strongest radar echo at all heights, the highest lightning density, and the most active ice-phase process, which indicate that the convection in the WR is the most vigorous, the convection in the FR is moderate, and the SR is the weakest. (2) Three types of rainfall are all marine type precipitation, the equivalent raindrop diameter Dm and the intercept parameter Nw of the WR are the largest. (3) The WR has the highest proportion of graupel compared with the FR and SR, stronger updrafts and more abundant water vapor supply may lead to larger raindrops during the melting and collision coalescence processes. (4) Over the all heights, liquid and ice water content in the WR are higher than those in the SR and FR. The ratio of ice to liquid water content in the WR is as high as 27% when ZH exceeds 50 dBZ, obviously higher than that in the SR and FR, indicating that the active ice-phase process existing in the WR is conducive to the formation of heavy rainfall.


Thu-03 Aug | 3:30 - 5:15 | MR327
AS39 - Models, in Situ, and Remote Sensing of Aerosols (MIRA)

Session Chair(s): Atsushi SHIMIZU, National Institute for Environmental Studies

AS39-A004 | Invited
Mapping Aerosol Lidar Ratios for CALIPSO Version 5

Greg SCHUSTER1#+, Travis TOTH2, Jayanta KAR3, Marian CLAYTON3, Zhujun LI3, David PAINEMAL3, Sharon RODIER3, Richard FERRARE1, Charles TREPTE1, Mian CHIN4, Dongchul KIM5, Ellsworth WELTON2, Huisheng BIAN5
1NASA Langley Research Center, 2National Aeronautics and Space Administration, 3NASA Science Systems and Applications, Inc., 4NASA GSFC, 5NASA Goddard Space Flight Center

The joint NASA/CNES CALIPSO* satellite mission hosts a lidar that has been providing nearly continuous backscatter profiles of aerosols and clouds since June 2006. The CALIPSO aerosol retrieval algorithm converts integrated attenuated backscatter profiles into extinction profiles as part of its tropospheric data products, but this requires ab initio assumptions in the aerosol lidar ratio (Sa) selection process. The selection process has been guided by observables and includes information from the linear depolarization ratio, signal strength, aerosol layer height, and surface type (ocean/land/desert). The information content is limited, however, so the number of Sa values employed by the algorithm is simplified to seven representative aerosol types that are applied uniformly worldwide (clean marine, dust, dusty marine, polluted dust, smoke, polluted and clean continental). The CALIPSO team is improving the selection process by incorporating newly-observed Sa values into the algorithm and enabling an approach that includes geographical and seasonal variations of Sa. Here, we report on an investigation that uses 12 years of collocated MODIS aerosol optical depth observations with CALIPSO backscatter measurements to infer constrained Sa for each of the CALIPSO aerosol types around the globe. The purpose is to obtain seasonal maps with spatially variable Sa for each of the seven aerosol types, effectively allowing the existing CALIPSO aerosol types to contain unspecified mixtures of dissimilar aerosols. This approach allows for smoother Sa transitions at coastlines and dust Sa values that can indicate mineral properties from different regions. We also use the GEOS-GOCART climate-chemical transport model to inform our maps in regions where data are sparse. In this presentation, we report seasonal lidar ratio maps for dust and sea salt and discuss the implications that these new maps may have on the CALIPSO Version 5 aerosol extinction products. ∗Cloud-Aerosol Lidar and Infrared Pathfinder Satellite Observation


AS39-A003 | Invited
Lidar Ratios Determined from Ground-based Lidars Using AODs from Sky Radiometers as a Constraint in East Asia

Man-Hae KIM1#+, Sang-Woo KIM1, Soojin PARK1, Tomoaki NISHIZAWA2, Atsushi SHIMIZU2
1Seoul National University, 2National Institute for Environmental Studies

The lidar ratio is an essential parameter to produce vertical profiles of aerosol extinction coefficient from elastic lidar measurements. In this study, aerosol lidar ratios are retrieved from a synergetic use of ground-based lidars and collocated sun-sky radiometers (AERONET or SKYNET) for six observatories in East Asia (Korea and Japan). There were tens of thousands collocated data pairs of lidar and sun/sky radiometer for each observatory, and 15~40% of the collocated data pairs were successfully retrieved. The mean retrieved lidar ratios are 58.4±18.0 sr, 50.9±20.3 sr, 47.2±26.7 sr, 61.1±25.1 sr, 57.6±22.1 sr, and 48.0±23.7 sr for Seoul, Osaka, Chiba, Gosan, Fukue, and Hedo, respectively. It is clearly seen that the lidar ratio is relatively high in Seoul and Gosan where are close to the Asian continent and decreases with an increase in the distance from the continent. Higher lidar ratios in Seoul and Gosan are related with anthropogenic pollutant aerosols. In coastal areas with a distance from the Asian continent such as Chiba and Hedo, lidar ratio is relatively low due to an influence of maritime aerosols. Lidar ratio increases as AOD increases for most observatories. It is thought that anthropogenic pollutant aerosols are more dominant for high AOD cases whereas clean marine aerosols are dominant for low AOD cases. The relation between lidar ratio and depolarization ratio is rarely recognizable for all observatories, which indicates the influence of dust aerosol on lidar ratio is not significant for long-term and column averaged lidar ratio in East Asia, especially in Korea and Japan.


AS39-A006 | Invited
Constraints on Spectral Mass Extinction Efficiency for a Global Aerosol Model

Edward HYER1#+, Christopher CAMACHO1, James CAMPBELL1, Peng XIAN1, James CHEN2, Andrew LAMBERT3, Lari MCDERMID3
1Naval Research Laboratory, 2Kirby School, 3General Dynamics Information Technology

Numerical models of atmospheric aerosol require extreme reduction of the complexity in particle composition and distribution in the real atmosphere. Translation from the particle mass quantities acted on by the model physics to the optical characteristics important to prediction of visibility embeds additional assumptions, but can also be an opportunity to introduce additional information to improve the model prediction. The Navy Aerosol Analysis and Prediction System (NAAPS) uses a limited number of tracers to represent the extremely heterogeneous particles encountered in the global atmosphere. The NAAPS model solves the 3-dimensional distribution of mass for each tracer type by simulating advection, sedimentation, wet and dry scavenging, and particle sources. These mass values are translated into extinction for prediction of atmospheric transmission and visibility. The conversion from physical to optical properties hinges on a mass extinction efficiency, which in the current operational NAAPS is a pair of values (scattering and absorbing) for each tracer type for each wavelength. By comparison of NAAPS and spectrally resolved AERONET measurements of scattering and absorbing optical depth, we examine the question of how well the mass information carried by the model could predict the atmospheric transmission with varying degrees of knowledge of the scattering and absorbing mass extinction efficiency. This analysis will be used to evaluate different schemes of computing extinction as well as potential deficiencies in the sets of tracers used in NAAPS.


AS39-A019
Improving Brown Carbon Evolution Processes in the WRF-Chem Model with DSCOVR EPIC Products

Olga KALASHNIKOVA1#+, Yuan WANG1, Michael GARAY1, Chenchong ZHANG2, James COY3
1California Institute of Technology, 2Purdue University, 3Texas A&M University

The fire-emitted particle-phase compounds of smoke exert significant atmospheric impacts on climate, air quality, and health, especially in downwind urban areas. Brown carbon (BrC), emitted mainly by smoldering fires and other biomass combustion, is one of the most important light-absorbing substances in the atmospheric aerosol. However, the extent of absorption by BrC particles for different types of fires and the effects of BrC on the radiation budget are still largely unknown. Observational techniques alone do not provide enough constraints on the global BrC direct radiative forcing, and the current representation of BrC in climate and regional chemical transport models is either absent or overly simplistic. For example, in majority of chemical transport models BrC optical properties are invariant with atmospheric processing or aging. DSCOVR EPIC UV observations provide comprehensive coverage and sufficient spatial and temporal resolutions for improving our understanding of BrC processes. EPIC MAIAC aerosol products combined with the regional-scale WRF-Chem model provide a unique opportunity for determining the impacts of BrC-emitting smoldering fire phases on air quality and climate in globally distributed target areas. We will discuss the roles of BrC processes in climate-relevant and air-quality relevant properties of smoke, focusing on understanding large-scale BrC evolution in the Western US and Canada. An approach to evaluate BrC evolution with a newly developed WRF-Chem parametrization that incorporates BrC time-resolved photobleaching will be introduced and evaluated. We will also assess the assumptions used to derive EPIC MAIAC BrC products with other collocated satellite datasets. In particular, we will discuss the importance of smoke plume vertical distributions for a set of fire cases where the smoke plume could be tracked through multiple DSCOVR images when collocated with CALIPSO and MISR products.


AS39-A012
Impacts of the COVID-19 Lockdown in China on New Particle Formation and Particle Number Size Distribution in Three Regional Background Sites in Asian Continental Outflow

Do-Hyeon PARK1+, Jeongeun KIM2,3, Jin-Soo PARK4, Jin-Soo CHOI4, Sang-Woo KIM1#
1Seoul National University, 2Korea Meteorological Administration, 3National Institute of Meteorological Sciences, 4National Institute of Environmental Research

This study examined the impact of emission reduction during the Chinese lockdown (LD) period on the new particle formation (NPF) frequency and corresponding particle number size distribution (PNSD) at three regional background atmospheric monitoring sites in western coastal areas of the Korea. During this period, the number concentrations of the nucleation- (<25 nm) and accumulation-mode (>90 nm) particles significantly decreased in Baengryeong (BRY), by 34% and 29% respectively. However, the PNSD in Anmyeon (AMY), which is influenced by nearby industrial emissions, showed only a slight decrease in nucleation- and accumulation-mode particles during the LD period, possibly because the reduction in industrial emissions was not significant during the social distancing period enforced by Korea. Bongseong (BOS) showed a similar variation to that of BRY, but the magnitude of the reduction was weaker due to its higher altitude. The cyclostationary empirical orthogonal function (CSEOF) technique was applied to the measured PNSDs at the three sites to objectively distinguish NPF events. The NPF frequency decreased by 7%, 1%, and 7% in BRY, AMY, and BOS, respectively, despite favorable meteorological conditions such as increased temperature and insolation during the LD period. The diurnal variation in the sulfuric acid (H2SO4) proxy implied that the H2SO4 proxy acted as a limitation factor for NPF events during the NPF occurrence time (8-12 local hours) in AMY and BOS; however, NPF occurrence in BRY was not connected with the H2SO4 proxy level. This suggests that BRY was more likely to be influenced by the reduction in organic species in the continental upwind regions, while the occurrence of NPF events in AMY and BOS can be suppressed in association with the distinct reduction in inorganic compounds represented by the H2SO4 proxy during the LD period.


AS39-A007 | Invited
Transboundary Transport Pattern Related to the Aerosol Pollution in South Korea

Ja-Ho KOO#+, Donghee LEE, Taegyung LEE
Yonsei University

While back-trajectory analyses have been widely used for the diagnosis of transboundary transport effect to the aerosol pollution in the receptor region in South Korea, those were limited to the Seoul metropolitan area or specific field campaign period. Thus, this study would derive more generalized pattern of transboundary transport influence with considering the 5-year (2015-2019) measurement of PM2.5 (particulate mass density having the diameter > 2.5 μm) at 5 cities: Seoul, Gwangju, Busan, Gangneung, and Daejeon. At first, we calculate 48-hour back-trajectories for every hour using the NOAA HYSPLIT4 model, then categorize those into 3 cases related to the extent of PM2.5: low, middle, and high aerosol pollution cases. If a back-trajectory passes over the box region in the Yellow Sea that we designate, that case is regarded as a transboundary transport. As a result, we can see high transboundary transport frequency (TTF) for the case of high aerosol pollution for all 5 cities. This pattern is seasonally consistent, implying that the serious haze is mostly resulted from the inflow of external air pollutants and this influence is not occasional but very constant through the whole year. Also we find that the altitude of back-trajectories is lower in the case of high aerosol pollution in Korea, meaning the large contribution of surface emission. At last, our analysis illustrates shorter straight travel distance of air flow when the high aerosol pollution happens in Korea. This well describes the weakened ventilation results in more serious air pollution. Acknowledgement: 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).


AS39-A009
Exacerbation of PM2.5 Concentration Due to Unpredictable Weak Asian Dust Storm: A Case Study of an Extraordinarily Long-lasting Spring Haze Episode in Seoul, Korea

Kyuseok SHIM1+, Man-Hae KIM1, Hyo-Jung LEE2, Tomoaki NISHIZAWA3, Atsushi SHIMIZU3, Hiroshi KOBAYASHI4, Cheol-Hee KIM2, Sang-Woo KIM1#
1Seoul National University, 2Pusan National University, 3National Institute for Environmental Studies, 4University of Yamanashi

Severe haze episodes have become a frequent occurrence in East Asian megacities, particularly during winter and early spring. Despite advancements in understanding the factors behind haze formation, the impact of weak Asian dust particles on PM2.5 concentrations has not been thoroughly investigated. Our study aimed to examine the role of Asian dust in PM2.5 concentrations during a prolonged high PM2.5 episode in Seoul, Korea in early spring 2019. The results showed that PM2.5 concentrations exceeding national standards (PM2.5 > 35 g m-3) were sustained from February 27 to March 7, 2019 and were largely due to transboundary transport of aerosols from the Asian continent under slow-moving anticyclones. High frequency of PM10-2.5 (PM10-2.5 > 30 μg m-3) and PM2.5 (PM2.5 > 80 μg m-3) mass concentrations in the high concentration range indicated the presence of Asian dust particles, which contributed to elevated PM2.5 Levels. Lidar and optical particle counter measurements revealed elevated depolarization ratios (532: 0.06–0.13) and aerosol volume concentrations in both coarse and fine modes, indicative of non-spherical dust particles. Despite advancements in air quality forecasting model, one of the latest models was unable to accurately predict the low Asian dust particle concentrations during high PM2.5 haze episodes, suggesting the difficulty of simulating dust particles from weak Asian dust events. Our findings highlight the need to incorporate dust emission and transport processes in air quality models to better predict PM2.5 levels during winter-spring high PM2.5 episodes.


Thu-03 Aug | 3:30 - 5:15 | MR328
AS33 - Reactive Nitrogen and Atmosphere-biosphere Interactions

Session Chair(s):

AS33-A009 | Invited
Mitigating Reactive Nitrogen Loss and Associated Environmental Damages: Opportunities from Changes in Food Production, Consumption and Supply Chains

Yixin GUO1#+, Lin ZHANG2, Denise MAUZERALL3, Tim SEARCHINGER3, Gang LIU2, Pan HE4, Mi ZHOU3
1The Hong Kong University of Science and Technology, 2Peking University, 3Princeton University, 4Cardiff University

Low nitrogen (N) use efficiency of food production and dietary shifts towards more N-intensive meats have caused substantial losses of reactive nitrogen (ammonia (NH3) and N2O to air and nitrate to water), contributing to health-damaging PM2.5 formation, climate warming and excess nitrogen deposition adverse to ecosystem biodiversity. Food-sector strategies may mitigate abovementioned inter-connected damages, yet comprehensive evaluation has been limited owing to gaps among disciplines. Here we explore reactive nitrogen reductions from management improvements and dietary shifts in China, and global food loss and waste (FLW) reductions. We combine agronomic field experiments, meta-analyses, atmospheric chemistry modeling, life-cycle assessments and epidemiological models. From the production perspective, improving Chinese agricultural management (including reduced N fertilizer use, machine fertilizer deep placement, enhanced-efficiency fertilizer and improved manure handling) can reduce NH3 emissions by ~6%-35%, PM2.5 by 0-8 microgram/m3 locally, cropland nitrate-leaching and runoff by 14-38%, N loss to water from animal farms by 20%, and increase grain yield by 7-9%. Total benefits (US$30 billion/a) exceed costs (US$ 18 billion/a). From the consumption perspective, replacing red meat by soy or shifting from the 2011 baseline Chinese diet towards the EAT-Lancet guidelines would decrease NH3 emissions by ~40% and ~20% respectively and decrease PM2.5 by up to 8microgram/m3 locally. Greater soybean intake and less red meat intakes also improve dietary health. In contrast, shifting to China’s dietary guidelines or a typical US diet increase NH3 emissions by ~100% and ~200% respectively, and increase PM2.5 by 2-10microgram/m3 locally. From the supply chain perspective, eliminating global FLW in 2015 would have mitigated agricultural NH3 emissions by 14% thus PM2.5 formation and N deposition. This avoids 1.5 million Years of Life Lost (YLL) from PM2.5 exposure and reduces N critical load exceedances at biodiversity hotspots.


AS33-A007 | Invited
Reducing Ammonia Volatilization and Improving Nitrogen Use Efficiency Using Coated Fertilizer

Arti BHATIA1#+, Vinod KUMAR2, Ritu TOMER2, Shikha SHARMA2, Ankita PAUL2, Sandeep KUMAR2, Niveta JAIN3, Mark A. SUTTON4
1ICAR-Indian Agricultural Research Institute, 2ICAR- Indian Agricultural Institute, 3ICAR- Indian Agricultural Research Institute (PUSA), 4Centre for Ecology and Hydrology

Quantification of ammonia volatilization (NH3) losses from agricultural soils is essential for identifying strategies for reducing direct and indirect nitrous oxide emissions and improving air quality. This study was carried out at the experimental fields of ICAR-Indian Agricultural Research Institute, New Delhi, India growing maize (PEHM) under four nitrogen fertilizer treatments to evaluate the impact on emissions of NH3 and nitrogen use efficiency from cropped soil. The treatments were Prilled urea (PU), Limus coated urea (LCU), Neem oil coated urea (NCU), and no fertilizer (Control). The volatilized NH3 was quantified by trapping in boric acid using Force draft method followed by acid titration and also by Gray Wolfpack multigas analyser equipped with an NH3 sensor. The cumulative NH3 volatilization loss in the different treatments varied from 0.27 to 12.78 kg N ha-1 by Force draft method and from 5.8 to 20.5 kg N ha-1 using the gas analyser. The NH3 loss varied from 1.7 to 10.65 % of applied N in the different treatments using the boric acid method, whereas it varied from 6.36 to 17.08% using the ammonia sensor. During the two-year study in the Limus treatment, wherein a urease inhibitor was coated on to urea reduced the NH3 loss by 62 to 71%, increased the maize yield by 17.5 to 21.2% as compared to PU and by 6.3 to 11.4 % as compared to NCU. No significant difference was observed in the % N content in maize grain in any of the treatments, however, the N uptake by plant (grain + straw) was significantly higher in NCU than PU and NCU. Therefore, the use of such enhanced efficiency fertilizers should be promoted for improving the crop productivity while safeguarding the environment. Acknowledgements: This study was supported by the UKRI GCRF South Asian Nitrogen Hub (Grant Number NE/S009019/1).


AS33-A003
Leaching Losses of Nutrients in Wetland Paddy Fields Under Different Nitrogen Management

Md. Mizanur RAHMAN1#+, Majharul ISLAM1, Mohammad Saiful ALAM1, Robert Martin REES2, GKM Mustafizur RAHMAN1, Md. Giashuddin MIAH1, Arti BHATIA3, Tapan Kumar ADHYA4, Mark A. SUTTON5
1Bangabandhu Sheikh Mujibur Rahman Agricultural University, 2Scotland's Rural College, 3ICAR-Indian Agricultural Research Institute, 4Kalinga Institute of Industrial Technology, 5Centre for Ecology and Hydrology

A significant amount of reactive nitrogen (N) and other nutrients applied to crop fields are lost through leaching which caused environmental pollution. This study aimed to determine the leaching loss of reactive N, phosphorus (P), potassium (K) and sulfur (S) from wetland rice culture under different N fertilizer practices. The experiment comprised of seven treatments viz., zero N as control, recommended dose of N (RDN) from prilled urea (PU), RDN + 25% N, RDN-25% N, cowdung 2 t ha-1 + supplemented N as PU, RDN + biochar 2 t ha-1, and deep placement of urea supper granules (USG). The study was conducted in four consecutive seasons of boro (dry season) and transplanted aman (wet season) rice. Findings revealed that leaching losses of NH4+-N, NO3--N, N, P, K and S in boro season ranged from 3.9 to 20.65, 4.26 to 25.97, 8.16 to 46.62, 0.23 to 0.28, 4.97 to 6.62, and 5.22 to 7.03 kg ha-1, respectively, while in the aman season, losses were 2.6 to 14.71, 2.35 to 10.72, 4.95 to 25.43, 0.14 to 0.17, 2.90 to 4.22, and 3.32 to 4.27 kg ha-1, respectively. The higher rates of N fertilizer application resulted in greater N, P, K and S losses. Compared to RDN, biochar and USG treatments reduced leaching losses of N by 48.07% and 30.29%, P 11.22% and 17.22%, K 23.02% and 19.72% and S 22.90% and 18.28% in boro season, while in aman season losses were 48.88% and 39.61%, 10.34% and 14.10%, 27.83% and 23.11%, and 13.97% and 19.59%, respectively. Biochar and USG deep placement might be effective in reducing leaching losses of N, P, K and S from wetland rice fields. Acknowledgements: This study was supported by the UKRI GCRF South Asian Nitrogen Hub (Grant Number NE/S009019/1).


AS33-A006
Long-range Transport of Atmospheric Inorganic Reactive Nitrogen (Nr) and Other Ionic Species at a Nr Emission Hotspot of Northern India

U.C. KULSHRESTHA#+, Moh NASEEM
Jawaharlal Nehru University

The anthropogenically induced acute reactive nitrogen (Nr) pollution is chronically eroding the biospheric integrity and undermining the earth system’s resilience to be in an accommodatable state by contributing to the disruption of critical biospheric and planetary processes. The present study comprehensively attempts to decipher the dry depositions of atmospheric inorganic Nr along with other major ions through dust fall fluxes. Authentic atmospheric dust samples were collected over a year-long temporal scale from October 2017 to September 2018 by incorporating a surrogate-surface approach. The sequentially descending orders of annual mean (± SE) NH4+-N, NO3-N - and Total Inorganic Nitrogen (TIN: NH4+-N+NO3-N -) fluxes (unit: kg ha-1 yr-1) across all sites were observed as MTL (0.41 ± 0.09) > BRT (0.20 ± 0.05) > LNI (0.12 ± 0.06), BRT (8.58 ± 2.30) > MTL (6.51 ± 1.58) > LNI (4.90 ± 0.66) and BRT (8.70 ± 2.30) > MTL (6.92 ± 1.57) > LNI (4.96 ± 0.65), respectively. Ionic deposition fluxes showed that SO42- was the dominant ionic species among all analyte ions in dustfall across all sites, which show a quite good congruence with the occurrence of higher surface mass concentrations of its gaseous precursor SO2 and the occurrence of a thick column of SO42- aerosol production from gaseous SO2 oxidation over sampling sites during the entire sampling period. All the dustfall samples exhibited alkaline nature (pH > 7.0) across all sites, and the annual mean pH of the dustfall samples across all sites was found to be ≥ 7.37. The 72 hrs back trajectory analysis suggested that the airmasses arrived from the west had significant influence on the deposition. Conversely, during the monsoon season, the prevailing direction of air masses arriving at all the sampling sites was South-West followed by South-East.


AS33-A010
Kinetics of the Nitrate-mediated Photooxidation of Monocarboxylic Acids in the Aqueous Phase

Yuting LYU+, Jany Ting Chun CHOW, Theodora NAH#
City University of Hong Kong

The photooxidation of organic compounds by hydroxyl radicals (·OH) in atmospheric aqueous phases contribute to the formation and evolution of secondary organic aerosols, which have significant impacts on visibility, health, and climate. Inorganic nitrate is an important ·OH source and its formation is increased with development of industry and agriculture. Low molecular-weight carboxylic acids (LMWCA) are ubiquitous components in urban, rural, and remote environments. The pH is an important factor in atmospheric aqueous phases that not only controls the dissociation of carboxylic acids and their ·OH reactivities, but also the production of ·OH and other reactive species from nitrate photolysis. Given ubiquitous nature of LMWCA and nitrate, it is crucial to understand their photochemical reactivities at different pH conditions. We studied the pH-dependent (pH 2 to 7) aqueous photooxidation of formic acid (FA), glycolic acid (GA), and pyruvic acid (PA) initiated by NH4NO3 photolysis. Their decay rates were controlled by the [NH4NO3]/[carboxylic acid] concentration ratios. Higher ratios lead to faster photodegradation rates, which were attributed to the higher concentrations of ·OH produced from higher concentrations of NH4NO3. The photodegradation rates of three carboxylic acids strongly depended on the pH. The highest photodegradation rate was observed at pH 4 for FA, whereas the rates were consistently higher at lower pH for GA and PA. The pH-dependent photodegradation of FA and GA were due to combined effects of the pH-dependent ·OH formation from NH4NO3 photolysis and the differences in ·OH reactivities of dissociated vs. undissociated forms. In contrast, the pH dependence in PA was due primarily to the pH-dependent decarboxylation of PA. These results highlight how pH and nitrate photolysis can combine to influence the degradation of carboxylic acids, which have significant implications for how the atmospheric fates of organic species are modeled for regions with substantial emission of inorganic nitrate. 


AS33-A011
Reducing Leaching Losses of Mineral Nitrogen from Paddy Fields with Different Nitrogen and Water Managements Practices

Niveta JAIN1#+, Om KUMAR2, Archana SHARMA2, Helen MARY ROSE3, Arti BHATIA4, Julia DREWER5, Mark A. SUTTON5
1ICAR- Indian Agricultural Research Institute (PUSA), 2ICAR- Indian Agricultural Institute, 3ICAR- Indian Agricultural Research Institute, 4ICAR-Indian Agricultural Research Institute, 5Centre for Ecology and Hydrology

The fertilizer nitrogen applied to agricultural fields is lost to the environment as N2O/NH3/NOx to the atmosphere and is also leached to ground water as nitrate and ammonium ions. An experiment was carried out at the experimental farm of ICAR-IARI, Delhi growing rice (Pusa 44) to quantify the leaching losses of nitrogen under different nitrogen and water management practices to device strategies for reducing N loses. Five N treatments under two water management practices (continuously flooding and Intermittent flooding) were unfertilized control, Prilled urea, Neem coated urea (NCU), LCC based NCU application, and 50:50% N through FYM and NCU+ biofetilizer. The percolation water was collected by porous suction cups made of clay materials embedded in a PVC pipe placed at 70cm depth. Total amount of percolation varied between 169 m3ha-1 and 250 mha-1 among the treatments. The NO32- and NH4+-N concentrations in different treatments varied from 0.01 to 4.53 mgL-1 and 0.01 to 12.81 mg L-1, respectively. The total NH4+-N in percolation water was high in CF treatment compared to IF, whereas NO32--N concentrations was lower by 33.7% compared to IF treatment under the same N treatment during the rice season. In case of different N treatments, the NO32--N ranged from 1.32 to 3.08 kg Nha-1 and NH4+-N concentration varied between 7.0 and 11.26 kg Nha-1. The LCC based NCU performed best amongst the different N treatments where both NO32--N and NH4+-N concentrations in percolation water were lowest. Total mineral N leached during the rice growing season ranged from 4.94 to 17.83 kg Nha-1 in different treatments. Loss of applied N was 9.23 to 12.53% in water management practices and 9.96 to 11.76% in different N treatments.


Thu-03 Aug | 3:30 - 5:15 | MR329
AS44 - Atmospheric Nitrogen-containing Organic Compounds: Sources, Processes, and Impacts

Session Chair(s): HWA JIN KIM, Seoul National University, Qi ZHANG, University of California, Davis, Tzung-May FU, Southern University of Science and Technology

AS44-A002
How Does the Chemistry at Environmental Surfaces Affect the Formation of Nitrogen Containing Organic Compounds?

Sasho GLIGOROVSKI#+
Chinese Academy of Sciences

Building surfaces are a boundary between the indoor and outdoor environment. Myriad of pollutants which are emitted into the air by automobiles, factories and a host of other sources present in the cities where we live, can settle on the building surfaces in form of a grime. Sunlight acting on urban grime very rapidly releases gas phase nitrogen oxides (NO) and nitrous acid (HONO) back into the atmosphere, by the light-induced heterogeneous reactions of nitrogen dioxide (NO2) with organic compounds such as polycyclic aromatic hydrocarbons (PAHs) trapped in the grime. HONO is very important player in urban atmospheric chemistry as represents the main primary source of hydroxyl radicals (OH) in urban air. Some of the released N-containing organic compounds by this chemistry make a part of the still poorly characterized light-absorbing organic compounds known as “brown carbon” indicating the importance of heterogeneous NO2 conversion processing on urban grime. Water surface microlayer (SML) is ubiquitous in the environment and provides a unique medium for interfacial processing. We present real-time measurements of volatile organic compounds (VOCs) produced by interfacial oxidation chemistry of gaseous ozone with an authentic SML collected at three different places located at upper, middle and lower reaches of East Pearl River within urban area of Guangzhou, China 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 SML of the river can lead to a large suite of unsaturated and saturated CHO organic compounds including nitrogen containing organic compounds. 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.


AS44-A019
Optical Properties and Potential Sources of Brown Carbon in the Seoul Metropolitan Area

Yanfang CHEN, Hwajin KIM#+
Seoul National University

The light-absorbing organic aerosol (OA), known as brown carbon (BrC), has significant impact on both air quality and climate. However, the sources and formation processes of BrC in the atmosphere are not well characterized. There are only limited studies have quantified the contributions of specific sources to BrC absorption in different environments, hindering the quantification of the impact of these sources on climate. In this study, a multiple-wavelength Aethalometer coupled with a High-Resolution Time-of Flight Aerosol Mass Spectrometer (HR-ToF-AMS) was deployed to investigate the relationship between the chemical composition and optical properties of BrC at a typical urban environment in Seoul, Korea from October to December in 2018. The results showed that BrC contributed 25.04 % to the total aerosol absorption at 370 nm. Sources of OA were divided into six different factors (HOA, BBOA, COA, MO-OOA, LO-OOA1 and LO-OOA2) by performing the positive matrix factorization (PMF) analysis. The multi-linear regression analysis on the PMF factors indicated the OA from biomass burning emission contributed to 38.9 % of BrC absorption. Consistently, clear correlations between nitrogen-containing OA and BrC absorption were observed and these nitrogen-containing compounds were likely produced during the biomass burning emission. Moreover, the two less oxygenated OA (LO-OOA1 and LO-OOA2) were found to contribute dominantly to the light absorption of BrC (56.7 %). Finally, the specific cases were investigated to further elucidate the photobleaching and photo-enhancement process of BrC.


AS44-A015
Optical Properties, Chemical Composition and Photooxidation of Atmospheric Nitrogen-containing Organic Aerosols

Ru-Jin HUANG#+
Chinese Academy of Sciences

Nitrogen-containing organic compounds (NOC) are a group of key chromophores in brown carbon (BrC, or light-absorbing organic carbon) aerosol, which affects atmospheric photochemical processes and radiative forcing. The optical properties, chemical composition, sources and aging processes of NOC, however, are still not well understood. In this study, we report the optical properties, chemical composition, and sources of NOC in urban atmospheric PM2.5. Nitrated aromatic compounds are the main light-absorbing NOC quantified in urban atmospheric PM2.5, and the seasonal variations of its chromophore composition, sources and contribution to light absorption of BrC are discussed. Nitrate-mediated photooxidation of NOC (including 4-nitrocatechol, 3-nitrosalicylic acid and 3,4-dinitrophenol) in atmospheric aqueous phase under different pH and temperature conditions are also studied. The dynamic changes in light absorption of NOC during photolysis are measured, and the photolysis rates and products of NOC are further characterized. The photolysis rate of NOC generally increases with the increase of temperature. The photooxidation of NOC begin with the addition of -OH or/and –NO (–NO2) groups to aromatic ring, and further ring-opening of aromatic ring with formation of smaller, highly oxygenated molecules.


AS44-A003
Particulate Amines and the Large Contributions from Anthropogenic Sources at a Coastal Area in Northern China in Winter

Xinfeng WANG1#+, Zhiyi LIU1, Min LI1, Yiheng LIANG2, Yueru JIANG1, Jing CHEN1, Jiangshan MU1, Yujiao ZHU1, Likun XUE1
1Shandong University, 2ETH Zürich

Particulate amines constitute a significant fraction of secondary organic aerosols and have adverse effects on air quality and human health. To understand the chemical composition, variation characteristics, and potential sources of particulate amines in the coastal area in northern China, field sampling and chemical analysis were conducted in coastal Qingdao in the winter of 2018 and 2019. A total of 15 major amines were identified and quantified by using an ultra-high-performance liquid chromatography with a hydrophilic interaction column in combination with a mass spectrometer. The average concentration of total amines in PM2.5 samples was approximately 130 ng m−3. Dimethylamine was the most abundant species among the quantified amines, followed by triethylamine and methylamine. The particulate amines usually exhibited elevated concentrations in the presence of high levels of SO2 and NOx or in the condition of high relative humidity. Moderately high correlations were recognized between amines and the SO2 and NOx. A receptor model of positive matrix factorization was employed and seven major sources were identified, including coal combustion, industrial production, vehicle exhaust, biomass burning, agricultural activities, secondary formation, and marine emission. Surprisingly, most particulate amines primarily originated from the primary emissions of anthropogenic activities particularly related to coal combustion and industrial productions, which should be given close concern to address the amine pollution. Further laboratory and field studies are required to evaluate the anthropogenic emissions of amines.


AS44-A006
Nitrogen-containing Compounds Enhance Light Absorption of Aromatic-derived Brown Carbon

Zhaomin YANG+, Lin DU#
Shandong University

The formation of secondary brown carbon (BrC) is chemically complex, leading to an unclear relationship between its molecular composition and optical properties. Here, we present an in-depth investigation of molecular -specific optical properties and aging of secondary BrC produced from the photooxidation of ethylbenzene at varied NOx levels for the first time. Due to the pronounced formation of unsaturated products, the mass absorption coefficient (MAC) of ethylbenzene secondary organic aerosols (ESOA) at 365 nm was higher than that of biogenic SOA by a factor of 10. A high NOx level ([ethylbenzene]0/[NOx]0 < 10 ppbC ppb−1) was found to significantly increase the average MAC300−700 nm of ESOA by 0.29 m2 g−1. The data from two complementary high -resolution mass spectrometers and quantum chemical calculations showed that nitrogen-containing compounds were largely responsible for the enhanced light absorption of high-NOx ESOA, and multifunctional nitroaromatic compounds (such as C8H9NO3 and C8H9NO4) were identified as important BrC chromophores. High-NOx ESOA underwent photobleaching upon direct exposure to ultraviolet light. Photolysis did not lead to the significant decomposition of C8H9NO3 and C8H9NO4, indicating that nitroaromatic compounds may serve as relatively stable nitrogen reservoirs and would effectively absorb solar radiation during the daytime.


AS44-A004
Dissecting the Contributions of Organic Nitrogen Aerosols to Global Atmospheric Nitrogen Deposition and Implications for Ecosystems

Yumin LI1,2+, Tzung-May FU1#, Jian Zhen YU2, Xu YU2, Qi CHEN3, Ruqian MIAO3, Yang ZHOU 4, Aoxing ZHANG1, Jianhuai YE1, Xin YANG1, Shu TAO1, Hongbin LIU2, Weiqi YAO1
1Southern University of Science and Technology, 2The Hong Kong University of Science and Technology, 3Peking University, 4Ocean University of China

Atmospheric deposition of particulate organic nitrogen (ONp) is a significant process in the global nitrogen cycle and may be pivotally important for N-limited ecosystems. However, past models largely overlooked the spatial and chemical inhomogeneity of atmospheric ONp and were severely deficient in assessing global ONp impacts. We constructed a comprehensive global model of atmospheric gaseous and particulate organic nitrogen (ON), including latest knowledge on emissions and secondary formations, and successfully simulated global atmospheric ONp. Our estimated global atmospheric ON deposition was 26 Tg N yr-1, predominantly in the form of ONp (23 Tg N yr-1) and mostly from wildfires (37%), oceans (22%), and aqueous productions (17%). Globally, ONp contributed as high as 40% to 80% of the total N deposition downwind of biomass burning regions. Atmospheric ONp deposition thus constituted the dominant external N supply to the N-limited boreal forests, tundras, and the Arctic Ocean, and its importance may amplify in a future warming climate.


Thu-03 Aug | 3:30 - 5:15 | MR330
AS59 - Mesoscale Meteorology and High-impact Weather

Session Chair(s): Yu DU, Sun Yat-sen University

AS59-A008 | Invited
Contrasting Mesoscale Convective System Features of Two Successive Warm-sector Rainfall Episodes in Southeastern China: A Satellite Perspective

Yipeng HUANG1+, Murong ZHANG2#
1Xiamen Meteorological Bureau, 2Xiamen University

As a typical rainfall type over South China, warm-sector rainfall is often attributed to Mesoscale Convective Systems (MCSs). However, the MCS contribution to warm-sector rainfall is rarely well-quantified, and the potential distinction of MCS behaviors in different warm-sector rainfall events remains unexplored. On 6–7 May 2018, two warm-sector rainfall episodes (EP1 and EP2) occurred in succession over southeastern China, with EP2 breaking historical rainfall records and producing a maximum rainfall total over four times that of EP1. The purpose of the present study was to elucidate how MCSs behaved in these two back-to-back but distinct warm-sector episodes, and thus explore the distinct role of MCSs in warm-sector rainfall. MCSs were identified, tracked, and characterized based on Himawari-8 infrared images. Results showed that MCSs played a dominant role in EP2, but not in EP1, by contributing over 80% of the extreme rainfall total and all the 10-min rainfalls over 20 mm. MCS occurrences were more frequent in EP2 than EP1, especially in the coastal rainfall hotspots, along with more frequent merging processes. Overall, the MCS samples in EP2 were larger in size, more intense, and moved slower and more in parallel to their orientation, which facilitated local rainfall accumulation. Two new indices are proposed—the overlap index (OLI) and merging potential index (MPI)—to evaluate two MCS processes vital for rainfall production: the repeated passage of an individual MCS over given areas and the merging between MCSs, respectively. Both OLI and MPI in EP2 were significantly larger than in EP1, which tended to produce larger maximum rainfall amount and stronger 10-min rain rates in the following hour. These results demonstrate the potential value of satellite-based MCS information for heavy rainfall nowcasting, which is particularly significant for warm-sector rainfall with its limited predictability.


AS59-A018 | Invited
Simulation and Diagnosis of Interactions Across Scales in Frontal Convective Vortices During the Mei-yu Season in Taiwan

Chung-Chieh WANG#+, Shin-Yi HUANG
National Taiwan Normal University

This study examines the contributions in vorticity from processes at different scales in two cases of mesoscale convective vortex (MCV) on the Mei-yu front. Case 1 occurred in 6-7 June 2003 and the MCVs were larger in size, while case 2 formed from isolated storms during 19-20 May 2014. The Cloud-Resolving Storm Simulator (CReSS) was used to reproduce the two events, and processes in the output data were separated into large-scale, mesoscale, and convective scales using the band-pass filtering method. The analysis of vorticity budget after scale separation shows that the positive vorticity contribution of case 1 is the vorticity divergence term and tilting term, and the convective scale is the most important, followed by the mesoscale. The positive vorticity contribution in the northern region (over northern Taiwan Strait) of case 2 is the vorticity divergence and tilting terms, which are dominated by meso- to convective scales. Especially in the development period of MCV, the convective scale in the vorticity divergence term and the horizontal advection term can be equivalent to the mesoscale. It can be seen that although the proportion of deep convection cells in the spatial distribution is small, the positive vorticity provided by them cannot be ignored. The analysis of the southern region shows that the positive vorticity contribution is the vorticity divergence term and the vorticity vertical advection term. The vorticity divergence term is the convective scale synergistic the large scale, and the vorticity vertical advection term is the large scale synergistic the mesoscale, which shows that the large-scale environment has a considerable degree of background vorticity value, and the latent heat release of deep convection enhances the low-level convergence and vertical upward movement, which can feedback the vorticity to the large-scale.


AS59-A012
Climatology of Wavelike Banded Convective Activities in South China

Xuan ZHOU+, Yu DU#, Junhong WEI
Sun Yat-sen University

Multiple parallel convective systems in form of wavelike banded convective activity have been observed in South China. A total of 114 cases were recorded from 2013 to 2021 by using the radar mosaic. This type of convective activity is most likely to occur in spring, summer and winter, with the least probability in autumn. Summer is the season with the greatest probability of large-scale bands. The wavelength range is between 50-400 km, with an average wavelength of 150 km. There are several possible causes of this phenomenon, including cold pools and gravity waves. Our focus is on the type of banded convective activities coupled with gravity waves, which has been identified as accounting for 47% of cases (54 cases) based on the presence of wave ducting. This type of banded convective activity is most likely to occur in spring and winter, and almost nonexistent in summer. There are two major types in terms of the orientation of wave front, including the northeast-southwest one and the northwest-southeast one.


AS59-A007
Impacts of Moisture on the Organizational Modes of Mesoscale Convective Systems Associated with Warm-sector Heavy Rainfall

Sa LI1, Zhiyong MENG2#+
1Huaneng Clean Energy Research Institute, 2Peking University

This work examines sensitivities of organizational modes of warm-sector heavy-rainfall-associated mesoscale convective systems (MCSs) in South China to relative humidity based on an MCS event with a typical linear organizational mode of trailing stratiform precipitation (TS). This TS system with two arc-shaped structures in its convective region induced by two pairs of bookend vortices was simulated as the control experiment (CTRL), based on which sensitivity experiments were performed by perturbing relative humidities in different layers. Results showed that sensitivities of organizational modes of the MCS to moisture decrease with height, with the highest sensitivity to lower-level moisture. Increasing lower-level moisture produces a bow echo (BE) mode with more stratiform precipitation than that in CTRL. Increasing lower-level moisture results in the increase of CAPE (convective available potential energy) and the decrease of LCL (lifting condensation level) thus favoring convection enhancement with strong cold pool and cold-pool-outflow-associated convergence, which lead to faster movements and larger rearward storm-relative winds that produce more stratiform precipitation. The occurrence of the BE mode is owning to the strengthening of rear inflows resulting from the merging of bookend vortices. Conversely, decreasing lower-level moisture produces no stratiform precipitation (NS) mode, possibly resulting from the lack of rearward storm-relative winds owning to the weak convection, the lack of cold pool and slow movements as a result of the decrease of CAPE and the increase of LCL. In addition, decreasing midlevel moisture may increase stratiform rainfall and the curvature of the convective line owning to the cold pool intensification resulting from the strong midlevel evaporation.


AS59-A006
The Role of Gravity Waves in the Asymmetric Development of Squall Lines

Hongpei YANG+, Yu DU#
Sun Yat-sen University

Squall lines, one of the most frequent mesoscale convective systems, are featured by asymmetric development, which is mainly explained by the interaction between cold pool and low-level wind shear. This study sheds further light on the role of gravity waves in shaping the asymmetry of squall lines through a combination of moist and dry numerical simulations. The moist simulations successfully capture the asymmetric and cyclical evolution of squall lines. In the initial stage, new cells are organized in both two sides of the parent system, but occur higher in the downshear side and persist longer in the upshear side. The mature stage is characterized by the cyclical growth of the parent system, the expansion and contraction of cloud anvil, and the cyclical generation of forward new cells. Although most new cells are short-lived, one develops into discrete propagation later.
These asymmetric features are closely linked to the convectively generated gravity waves, with n=1 waves stabilizing the environment while n=2 waves promote convective organization through uplifting, enhancing moisture, and favorable thermal conditions in the low-level. The cyclical generation of multiple n=1 and n=2 waves lead to the cyclical asymmetric development of squall lines. The idealized dry simulations further examine the impact of low-level vertical wind shear on the wave asymmetry. The low-level shear results in faster wave speed, larger wave amplitude, and lower the height of wave nodes in the upshear side, and thus jointly contribute to the asymmetric development of squall lines.


AS59-A021
Initiations of Mesoscale Convective Systems in the Middle Reaches of the Yangtze River Basin Based on FY-4A Satellite Data: Statistical Characteristics and Environmental Conditions

Ya-Nan FU1+, Jianhua SUN1#, Shenming FU2, Yuanchun ZHANG1, Zheng MA1
1Chinese Academy of Sciences, 2Institute of Atmospheric Physics, Chinese Academy of Sciences

Based on the brightness temperature observed by the Fengyun-4A satellite, eight hundred mesoscale convective systems (MCSs) are identified in the middle reaches of the Yangtze River Basin during the warm seasons (April–September) of 2018–2021, which are categorized into the quasistationary (QS) type and the outward-moving (OM; i.e., vacating the source region) type. Afterward, the initiations of the MCSs are backward tracked using a hybrid method of areal overlapping and optical flow. Then, the main features of QS and OM MCSs and their respective synoptic circulations and environmental parameters are analyzed. The QS MCSs primarily occur in July and August and are mainly initiated in the afternoon. The OM MCSs mostly occur in June and July with two initiation peaks appeared at noon and late night, respectively. The QS MCSs are mainly initiated in mountainous areas, and they are primarily caused by local thermal effects. In contrast, the OM MCSs are mainly initiated in plain areas under synoptic forcings. Circulations of a total of 285 days (without direct influencings from tropical cyclones) are objectively classified into three patterns by using the k-means algorithm. Pattern-I (128 days) which is closely related to low-level jets, shows the most similar features to those of typical Mei-yu fronts, and it acts as the most favorable circulation type for MCSs’ initiations. Pattern-II (66 days) is dominated by northwesterlies, with a relatively stable layer in the low-level troposphere. Pattern-III (91 days) features a dry-adiabatic or even a superadiabatic layer that contributes to lowering the layer stability.


AS59-A017
Linear Stability Analysis of a Tornado-like Vortex with Double Helical Structure Produce in a Vortex Simulator of National Defense Academy

Toshihisa ITANO#+
National Defense Academy

Linear stability of a tornado-like vortex with double helical structure produced in a vortex simulator of National Defense Academy is investigated. The simulator has cylindrical structure with 1.8 m in diameter and 0.95 m in height, and consists of a blower at the top, which sucks the air inside and generates mainstream passing through the devise, and 50 guide vanes arranged point-symmetrically at the bottom, which give angular momentum, necessary for the formation of tornado-like vortex, to the inflow. Various kinds of tornado-like vortices, from axi-symmetric one or two cell’s ones to asymmetric ones embedding secondary vortices within them, can be generated in the simulator. A vortex with double helical structure, which contains two secondary vortices intertwining with each other like DNA, is formed when the inflow angle of the 50 guide vanes is around 30 – 50 deg. In this study, we focused on such a vortex which emerges when the inflow angle is 37.5 deg, where two secondary vortices are rather tightly intertwined with each other. The vortex is measured by sonic anemometer-thermometer (SAT) developed for laboratory use, whose probe has a base line of 3 cm. Three components of wind speed are measured with the spatial interval of 3 cm and 5 cm in the radial and vertical directions, respectively. Each run is set to 4 min with 10 Hz. The radial wind profile, which becomes a basic state of the linear stability analysis, is obtained by averaging the data. A sextic equation is used to approximate and smooth the profile. Linear stability of the axisymmetric parent vortex thus obtained is investigated with a non-divergent barotropic vorticity equation following the method proposed by Staley and Gall (1979). Fortunately, the preliminary result shows instability against a wave number-2 perturbation. Detailed considerations will be introduced at the conference.


Thu-03 Aug | 3:30 - 5:15 | MR331
AS01 - The Asian Monsoon, Extremes and Climate Change

Session Chair(s): Renguang WU, Zhejiang University, Ramesh KRIPALANI, Indian Institute of Tropical Meteorology

AS01-A026
More Than Six Billion People Encountering More Exposure to Climate Extremes with 1.5 ◦c and 2.0 ◦c Global Warming

Peihua QIN#+
Chinese Academy of Sciences

The Paris Agreement established the aims for global warming in the 21st Century relative to preindustrial times, with 1.5 ◦C as ideal object and 2.0 ◦C as upper boundary. Compound population exposure to climate extremes under different global warming levels, which is determined both by changes in climate and the amount and distribution of population, is not well known. Here, we investigate changes in population exposure to wet, dry, heat and cold extremes with 1.5 and 2.0 ◦C global warming. Results show that population exposure to wet, dry and heat extremes over middle Africa, Arabian Peninsula and South Asia is generally found to increase at 1.5 and 2.0 ◦C warming levels, whereas that over eastern Asia largely decreases from 1.5 to 2.0 ◦C warming due to a population reduction by 107 million. Then we adopt a 4-bit binary number as a compound index to represent the size of the exposure increase to different extremes under different warming levels. Total population with exposure increases to wet, dry, heat and cold extremes is 2358, 1900 and 1569 million persons at 1.5 ◦C warming, 2.0 ◦C warming and from 1.5 to 2.0 ◦C warming, respectively. Furthermore, there are 7242, 6574 and 6299 million persons faced with increased exposure to all four extremes but the cold extreme during the above periods, which is more than two-thirds of total population. Therefore, we should do more to confront possible climate risks under global warming.


AS01-A035
Quasi-biweekly Oscillation in Tropical Asian Monsoon Rainfall Variations During Boreal Summer: Propagation and Maintenance

Weizhen CHEN+, Song YANG, Wei WEI#
Sun Yat-sen University

The quasi-biweekly oscillation (QBWO) is an important component of tropical monsoon variations. The first two leading modes of the empirical orthogonal function analysis of rainfall variations over the tropical monsoon region show that the western North Pacific QBWO and the Indian Ocean QBWO propagate northwestward and encounter in the Bay of Bengal. They further propagate westward toward the Arabian Sea. Enhanced (suppressed) rainfall activity is closely related to significant positive (negative) specific humidity anomalies. Results from a moisture budget analysis indicate that the successive westward movement of moisture precursor is primarily due to the interaction between the perturbation zonal wind (vertical motions) and the mean zonal (vertical) gradient of moisture at the lower level (middle level), with two anomalous cyclone circulations alternately presenting over the South China Sea and the Bay of Bengal. This research reveals the connection of the two branches of QBWO rainfall anomalies over the western North Pacific and the Indian Ocean in the view of moisture dynamics.


AS01-A090
Climate Responses to Tambora-size Volcanic Eruption and the Impact of Warming Climate

Linshan YANG1+, Chaochao GAO1#, Fei LIU2
1Zhejiang University, 2Sun Yat-sen University

The climatic consequences to large volcanic eruptions depend on direct radiative perturbation and climate variability that amplifies or dampens the initial perturbation. Potential climate responses to future eruptions, however, have been rarely studied. Here we show perturbation of Tambora- size causes significant but no inter-scenario different global average climate responses, by using CESM simulations under preindustrial and RCP8.5 scenarios. Regionally we find severe reduction in African and Asian-Australian monsoon rainfall and emerge of El Niño-like responses, largely due to the land-ocean thermal contrast mechanism. Global warming significantly amplifies such El Niño-like responses, which feed on the enhanced climatology atmospheric moisture and cause higher sensitivity of monsoon circulation to radiative forcing in the tropics. We also find prolonged Asian-Australian monsoon suppression that enhances the westerly anomalies through Kalvin wave response over the Pacific, suggesting the complexity of climate responses and feedbacks to external forcing under future climate.


AS01-A091
Weakening of Decadal Variation of Northern Hemisphere Land Monsoon Rainfall Under Global Warming

Yeyan JIANG1#+, Juan LI1, Zhiwei ZHU1, Bin WANG2
1Nanjing University of Information Science & Technology, 2University of Hawaii

Over the past century, Northern Hemisphere (NH) land monsoon rainfall (NHLMR) experienced significant decadal to multidecadal variations, mainly driven by an east–west sea surface temperature (SST) contrast over the Pacific (EWPC) and an interhemispheric North Atlantic–South Indian Ocean SST dipole (NAID). However, how the NHLMR’s decadal variation would vary and whether the oceanic forcing could continue to drive it in a warming world remain unexplored. Here, by analyzing 24 CMIP6 (Coupled Model Intercomparison Project Phase 6) models’ historical simulations and future projections, we show that the leading mode of decadal NHLMR would remain its nearly-uniform spatial pattern and representation of the NHLMR’s intensity. However, the intensity of decadal NHLMR variation will experience a comprehensive decline under various emission scenarios. In the future, EWPC will remain a primary driver, but NAID is no longer. The significant historical correlation between NAID and NHLMR is mainly attributed to the influence of high anthropogenic aerosols emission. However, the NAID-NHLMR linkage would no longer exist owing to the reduced anthropogenic aerosol emission in the future.


AS01-A096
The Accelerating Increase of Dangerous Compound Heatwaves in China Under Different Warming Levels

Wei DONG#+, Xiaojing JIA
Zhejiang University

Extreme heat waves have attracted much attention in recent decades in China due to the great threat they pose to human and ecology. Defining meteorological compound events that pose a direct threat to human health is urgently needed, and accurately capturing the rate of increase in such events is a direct reflection of the increasing risks of climate change. Thus, detecting the increasing rate and future changes under different warming levels is an important topic. The increase in such events is primarily a response to the level of global warming. In this talk, the latest CMIP6 Universal Thermal Climate Index datasets are first evaluated and corrected by a robust empirical quantiles method. We then define dangerous compound heatwaves based on different risk levels. Finally, we show the evolution of the change rate and spatial extent of dangerous compound heatwaves in China based on different levels of global warming. Therefore, our study reveals the urgency of mitigating climate warming and resisting the risk of dangerous compound heatwaves.


Thu-03 Aug | 3:30 - 5:15 | MR332
AS36 - Regional Climate Downscaling and Cordex: Challenges and Prospects

Session Chair(s): Dong-Hyun CHA, Ulsan National Institute of Science and Technology

AS36-A007 | Invited
Uncertainty Analysis of Future Summer Monsoon Duration and Area Over East Asia Using a Multi-GCM Multi-RCM Ensemble

Seung-Ki MIN1#+, Donghyun LEE2, Joong-Bae AHN3, Dong-Hyun CHA4, Seok-Woo SHIN4, Eun-Chul CHANG5, Myoung-Seok SUH5, Young-Hwa BYUN6, Jin-Uk KIM7
1Pohang University of Science and Technology, 2University of Oxford, 3Pusan National University, 4Ulsan National Institute of Science and Technology, 5Kongju National University, 6National Institute of Meteorological Sciences, 7Korea Meteorological Administration

This study examines spatio-temporal characteristics of the summer monsoon rainy season over East Asia (EA) using six regional climate models (RCMs) participating in the CORDEX EA Phase II project. The combination of multiple GCMs × RCMs framework produces a larger spread in summer monsoon characteristics than those from driving GCMs only, enabling a better quantification of uncertainty factors. The RCM simulations reproduce the observed summer monsoon duration and area with overall improved performances compared to their corresponding boundary GCM outputs, representing the added values of RCMs. Both area and duration of the EA summer monsoon are projected to increase by the late 21st century, more strongly in the high emission scenarios than in the low emission ones, particularly in China. Warming mitigation benefits estimated from different responses between scenarios tend to be larger in area than in duration across EA. ANOVA results show that uncertainty in future EA monsoon area and duration is generally larger between boundary GCMs than between RCMs. A strong inter-simulation relationship between RCMs and GCMs supports that the boundary GCMs substantially diversify downscaled RCM projections through different climate sensitivities. Further, the distinct sub-regional responses in future monsoon area and duration emphasize the importance of fine-resolution projections with appropriate uncertainty measures for better preparing region-specific adaptation plans.


AS36-A004
Future Projection of Precipitation Over the Korean Peninsula Under Global Warming Levels of 1.5℃ and 2.0℃, Using Large Ensemble of RCMs in CORDEX-EA Phase 2

DoHyun KIM1#+, Jin-Uk KIM2, Young-Hwa BYUN1, Tae Jun KIM1
1National Institute of Meteorological Sciences, 2Korea Meteorological Administration

This study conducted analysis about future projection of precipitation (PR) over the Korean Peninsula (KP) under global warming levels of 1.5℃ and 2.0℃ (GWL 1.5℃ and 2.0℃). Large ensemble of state-of-the-art regional climate model (RCM) in CORDEX-EA Phase 2 was used and bias correction was performed on the ensemble. Under GWL 1.5℃ (2.0℃), RCM multi-model ensemble (MME) predicted that mean PR will increase slightly by 4.69% (5.08%) with larger increase of northern KP (NKP) and southern KP (SKP). This spatial pattern was expected to be similar for extreme PR, but the response was expected to be intensified with increase by 10.14% (12.05%). RCM MME also predicted that distribution of extreme PR will shift to the right and then extreme event occur once in 20 years will change the event with reoccurrence of 12.56 years (10.88 years) over SKP and 10.04 years (9.96 years) over NKP. Mechanism was investigated for cases when extreme PR occur during June to September. It was expected that increase of extreme PR per warming will be close to Clausis-Clapeyron scale, which will be 5.64% ℃-1 (5.52% ℃-1) over SKP and 8.37% ℃-1 (6.54% ℃-1) over NKP. This meant that increased moisture capability by warming will affect extreme PR rather than mean PR. However, expected ratio over CKP was 3.39% ℃-1 (2.03% ℃-1), which implied that there will be other factors affecting extreme PR. Accordingly, some possible factors were investigated and RCM MME predicted vertical instability over East Asia to continue and moisture flux and convergence around KP to be intensified under GWLs.


AS36-A019
Future Changes in Extreme Precipitation Over CORDEX East Asia

Ana JUZBASIC1#+, Dong-Hyun CHA1, Joong-Bae AHN2, Seung-Ki MIN3, Eun-Chul CHANG4, Myoung-Seok SUH4, Young-Hwa BYUN5, Jin-Uk KIM6
1Ulsan National Institute of Science and Technology, 2Pusan National University, 3Pohang University of Science and Technology, 4Kongju National University, 5National Institute of Meteorological Sciences, 6Korea Meteorological Administration

The present study used daily precipitation data from a total of 10 GCM-RCM chains using four GCM (GFDL_ESM2, HadGEM2_AO, MPI_ESM_LR, and UKESM) and four RCMs (WRF, RegCM, MM5, and CCLM), to address the future changes in extreme precipitation during boreal summer (June-July-August, JJA). Model performance has been evaluated by comparing model simulation with APHRODITE data, using Expert Team on Climate Change Detection and Indices (ETCCDI) indices related to extreme precipitation. Due to systematic biases apparent in the initial analysis, bias correction was deemed to be necessary, and was performed using quantile mapping. After the correction, all of the models simulated the current climate sufficiently, especially for the average daily precipitation, maximum 1- and 5-day precipitation (Rx1Day and Rx5day), and the number of days with precipitation over 20mm (R20mm), while the number of the continuous wet and dry days was still overestimated or underestimated after bias correction. In both RCP8.5 and SSP5-8.5 scenarios, average daily precipitation during summer was not projected to have significant changes by the end of the century over the whole domain. However, the extreme precipitation indices, that is, Rx1Day, Rx5Day, and R20mm were projected to increase, with the largest increases being over the coastal areas. This change was projected to be larger in the SSP5-8.5 scenario than in the RCP8.5 scenario, most likely as a consequence of both slightly higher emissions, as well as increased climate sensitivity of the models in the SSP5-8.5 scenario.


AS36-A025
Present Day Bias and Future Change Signal of Temperature Over China in a Series of Multi-GCM Driven RCM Simulations

Jia WU1#+, Xuejie GAO2
1National Climate Center of China, 2Chinese Academy of Sciences

Simulation of surface air temperature over China from a set of regional climate model (RCM) climate change experiments over the East Asia domain of CORDEX phase II are analyzed with the focus on bias and change signal of the RCM and driving general circulation models (GCMs). The set consists of 4 simulations by the RCM of RegCM4 driven by 4 different GCMs for the period of 1979-2099 under the mid-range RCP4.5 (Representative Concentration Pathway) scenario. Results show that for present day conditions, the RCM provides with more spatial details of the distribution and in general reduces the biases of GCM, in particular in DJF (December-January-February) and over areas with complex topography. Bias patterns show some correlation between the RCM and driving GCM in DJF but not in JJA (June-July-August). In JJA, the biases in RCM simulations show similar pattern and low sensitivity to the driving GCM, which can be attributed to the large effect of internal model physics in the season. For change signals, dominant forcings from the driving GCM are evident in the RCM simulations as shown by the magnitude, large scale spatial distribution, as well as interannual variation of the changes. The added value of RCM projection is characterized by the finer spatial detail in sub-regional (river basins) and local scale. In DJF, profound warming over the Tibetan Plateau is simulated by RCM but not GCMs. In general no clear relationships are found between the model bias and change signal, either for the driving GCMs or nested RCM.


AS36-A017
Projection of Extreme Heatwaves Over the CORDEX-East Asia Phase 2 Domain Under RCP and SCP Scenarios

Young Hyun KIM1#+, Joong-Bae AHN2, Dong-Hyun CHA1, Myoung-Seok SUH3, Eun-Chul CHANG3, Seung-Ki MIN4, Young-Hwa BYUN5, Jin-Uk KIM6
1Ulsan National Institute of Science and Technology, 2Pusan National University, 3Kongju National University, 4Pohang University of Science and Technology, 5National Institute of Meteorological Sciences, 6Korea Meteorological Administration

This study accesses the future changes in an extreme heatwave, in terms of intensity and duration, over the CORDEX-East Asia Phase 2 domain. An extreme heatwave is defined as one in which the heatwave magnitude (HWM), which is the accumulated daily intensity of a heatwave during the heatwave period, is higher than the 95th percentile of the HWM for the reference period. In the Historical simulations (1981–2005), heatwaves have occurred mainly from April to June in India, in April and May in Indochina, from June to August in China and Mongolia, and in July and August in the Korean Peninsula and Japan. Most heatwaves in East Asia last three to four days, but long-lasting and intense heatwaves occur more often in India and Indochina than elsewhere. In the end of the 21st century (2071-2100), heatwave intensity will increase, the average duration of heatwaves will be approximately two to three weeks, and the heatwave season will be lengthened. Therefore, extreme heatwaves will occur more frequently and strongly. Under two representative concentration pathway scenarios (RCP2.6 and RCP8.5) and two shared socioeconomic pathway scenarios (SSP1-2.6 and SSP5-8.5), the proportion of extreme heatwaves to all heatwave events will increase from 5.0% (historical) to 8.0%, 20.8%, 19.3%, and 36.3%, and the HWM of the extreme heatwave will be 1.4, 3.5, 3.0, and 9.0 times stronger, respectively. The main reason for the increase in the HWM of extreme heatwaves is the increased duration rather than the daily intensity of the heatwaves. In East Asia, the temporal and regional disparities of heatwave damage will be much more prominent as extreme heatwaves become stronger and more frequent in these regions and during the periods that are more affected by heatwaves in the present day.


AS36-A016
Changes in Wind Energy Potential Over East Asia Using the CORDEX-East Asia High-resolution Multiple Regional Climate Models

Changyong PARK#+, Dong-Hyun CHA, Seok-Woo SHIN
Ulsan National Institute of Science and Technology

Renewable energy generation, such as photovoltaic or wind power, is directly affected by weather and climate. This study investigated recent changes in Wind Energy Potential (Wpot) over sub-regions for East Asia and projected them for the future period using the CORDEX-East Asia phase Ⅱ high-resolution multiple regional climate models. Since the wind has high variability over time, we applied 3-hourly data, which is the shortest time interval in the regional climate models produced. In addition, since the amount of power generated in a wind turbine varies depending on the wind speed, the Wpot was estimated in detail according to the wind speed intervals. The averaged Wpot over the past 40 years (1979-2018) was high in Northeast China and Northwest China across all seasons, and recent East Asia averaged Wpot generally increased in spring, autumn, and winter, and decreased in summer, but had large inter-regional variability. In particular, the recent increase in Korea and Inner Mongolia was the largest in spring. Moreover, in inner Mongolia, wind speeds from 12 m s-1 or higher to less than 25 m s-1, which are the highest efficiency sections, were the most frequent and had the highest rate of increase. In the case of the RCP2.6 scenario, Wpot will increase considerably in Korea and Japan in all seasons from 2041 to 2065, and will increase, and the autumn from 2075 to 2099 will increase more than during the period from 2041 to 2065 in all sub-regions except Southern China. In the RCP8.5 scenario, the difference between regions is larger than that of the RCP2.6 scenario, and it is predicted that the decrease in Wpot will be significantly greater in the autumn during the two future periods.


AS36-A022
Future Activities of Tropical Cyclone Under the SSP Scenarios Using Multi-RCMs

Eunji KIM1+, Taehyung KIM1, Tae Ho MUN1, Seok-Woo SHIN1, Minkyu LEE2, Dong-Hyun CHA1#, Eun-Chul CHANG3, Joong-Bae AHN4, Seung-Ki MIN5, Jin-Uk KIM6, Young-Hwa BYUN7
1Ulsan National Institute of Science and Technology, 2Korea Institute of Energy Research, 3Kongju National University, 4Pusan National University, 5Pohang University of Science and Technology, 6Korea Meteorological Administration, 7National Institute of Meteorological Sciences

Tropical cyclones (TCs) are often generated over the western North Pacific (WNP). They result in destructive damages in East Asian countries including South Korea. In this study, we investigated future activities of TCs using five regional climate models (RCMs) (e.g., RegCM4, GRIMs, WRF, CCLM, HadGEM3-RA) are forced by UK Earth System Model (UKESM) under the historical and two Shared Socioeconomic Pathways (SSP) scenarios (SSP1-2.6 and SSP5-8.5). The simulation experiments are conducted at 25-km horizontal resolution over Coordinated Regional Climate Downscaling Experiment (CORDEX) East Asia domain. The performance based-ensemble mean method is applied to reduce the uncertainty of a single RCMs. In the historical (1985-2014) period, the ensembled models captured the number of TC genesis of observation data but simulated the intensity weakly. Comparing the historical and the near-future (2031-2060) and far-future (2071-2100) periods, the RCMs show the same feature that the core region of TCs genesis migrates northwards. As the migration of genesis region, activities of TCs also moved northward. It is related to several synoptic fields; increasing of relative vorticity and specific humidity of 850 hPa, and weakening of vertical wind shear over the mid-latitudes, due to higher sea level pressure than in the historical period.


Thu-03 Aug | 3:30 - 5:15 | MR335
AS52 - Ionospheric Space Weather Monitoring and Forecasting

Session Chair(s): Haixia LYU, Wuhan University, Sampad Kumar PANDA, Koneru Lakshmaiah Education Foundation

AS52-A013 | Invited
New Insights on the Equatorial Plasma Bubble(EPB) Morphology and Geomagnetic Storm Effects on EPBs Using GOLD Data

Deepak KARAN1#+, Richard EASTES1, Carlos MARTINIS2, Robert DANIELL3, Stanley SOLOMON4, William MCCLINTOCK1
1University of Colorado Boulder, 2Boston University, 3Ionospheric Physics, 4National Center for Atmospheric Research

The Equatorial Plasma Bubble (EPB) morphology depends on several factors, such as the alignment of the dusk terminator with the magnetic field lines, thermospheric winds, waves, and electric fields, etc. The multifactor dependency makes the EPB morphology complex. In 2-D airglow images, sometimes the EPBs appear to be straight (aligned along the magnetic field lines) and at other times the poleward extensions can be tilted eastward or westward from the magnetic field line resembling either a C-shape or reversed C-shape structures, respectively. All these different structured EPBs have never been observed together. NASA’s Global-scale Observations of the Limb and Disk (GOLD) mission observed these differently shaped EPBs within ~12o and 6o longitudes on 12 October 2020 and 26 December 2021, which is very rare, probably the first of the kind. These EPBs were inside the GOLD imager’s field-of-view for ~3 hours. This allowed us to compute their zonal drift velocities. To investigate the role of latitudinal variations of EPB’s drifts in their different shapes, the zonal drifts at the magnetic equator and at both EIA crests are calculated. Observed differences in the EPBs’ shape can be explained by the calculated latitudinal differences in their zonal drift velocities. Such occurrences of opposite EPB morphologies in a narrow longitude during a geomagnetic quiet time may indicate the strong longitudinal differences in the neutral winds and/or electric fields, responsible for the EPBs motion. The enhancement of equatorial electric fields due to the geomagnetic storm makes the ionosphere conducive to more EPBs. Coincidence electric field and neutral wind measurements by ICON (Ionospheric Connection Explorer) and EPB locations from GOLD have brought capabilities to forecast the EPB occurrence. These aspects will be discussed in this presentation.


AS52-A001
Driver of the Positive Ionospheric Storm Over South American Sector During 4 November 2021

Changzhi ZHAI#+
Hohai University

During geomagnetic storms, ionospheric storms can be driven by several mechanisms. Observations from ground- and space-based instruments are used to reveal the driver of the positive ionospheric storm over South American sector during 4 November 2021 geomagnetic storm. The positive storm appeared from ~10:30 UT to 18:00 UT and covered the region from 40°S to 20°N. The maximum magnitude of TEC (Total Electron Content) enhancement and relative TEC enhancement were about 20 TECU and 100%, respectively. Defense Meteorological Satellite Program (DMSP) also observed significant electron density increase over South America and east of Pacific Ocean. In the meantime, about 50% ∑O/N2 enhancement was observed by the Global‐scale Observations of the Limb and Disk (GOLD) satellite at low latitudes. Ionosonde observations (AS00Q, CAJ2M) registered ~80 km uplift of F2 peak height (HmF2) and a prominent F2 peak electron density (NmF2) increase ~3 hour after the uplift. Prominent enhancement of Cross-Polar Cap Potential (CPCP) in the southern hemisphere was also observed by Super Dual Auroral Radar Network (SuperDARN), which was one hour earlier than the HmF2 uplift. Measurements from Ionospheric Connection Explorer satellite (ICON) showed that the outward E×B drift enhanced significantly and the horizontal ion drift was poleward. According to the ICON ion drift observations, the HmF2 uplift was caused by electric field rather than equatorward neutral wind. We propose that the enhanced eastward electric field dominated the positive ionospheric storm and the thermospheric composition variation may also contributed.


AS52-A008
Analysis of the BDGIM Performance in BDS Single Point Positioning

Guangxing WANG1#+, Zhihao YIN2, Zhigang HU3
1China University of Geosciences, 2Mengxin Technology, 3Wuhan University

As a novel broadcast ionospheric model for BDS-3, BeiDou global ionospheric delay correction model (BDGIM) was analyzed through single point positioning (SPP) in this study. Since the broadcast ionospheric model is mainly used to correct the ionospheric delay error for single-frequency users, a series of stations simultaneously receiving B1C, B2a, B1I and B3I signals were selected from the International GNSS Service (IGS) and the International GNSS Monitoring and Assessment System (iGMAS) tracking networks for the SPP experiments. The differential code bias (DCB) parameters were used to correct the hardware delays in the signals of B1C and B2a. The results showed that the BDGIM performs the best in high-latitude areas, and can effectively improve the positioning accuracy compared with the Klobuchar model. The average 3D positioning accuracy of the four civil signals can reach 3.58 m in high-latitude areas. The positioning accuracies with the BDGIM in the northern hemisphere are better than those in the southern hemisphere, and the global average 3D positioning accuracy of the four civil signals is 4.60 m. The performance of the BDGIM also shows some seasonal differences. The BDGIM performs better than the Klobuchar model on the days of spring equinox and winter solstice, while the opposite is true on the days of summer solstice and autumn equinox. Although the SPP accuracies are to some extent affected by the geomagnetic storm, the BDGIM generally performs better and are more resistant to the geomagnetic storm than the Klobuchar model.


AS52-A004
Regional Ionospheric Tec Prediction Based on Multi-factor Neuralprophet Model Under Disturbed Conditions

Han WU1+, Ling HUANG1#, Hongping ZHANG2, Dezhong CHEN2, Yidong LOU2, Bin MA1, Xu LIU1
1Guilin University of Technology, 2Wuhan University

In this study, a novel multi-factor regional ionospheric TEC prediction model (multi-factor NeuralProphet model, MF-NPM) considering multiple factors was constructed based on the NeuralProphet hybrid prediction framework by taking solar activity index, geomagnetic activity index, geographic coordinates, and IGS GIM data as input parameters. The prediction performance of MF-NPM, trained using the dataset from 2009 to 2013, was evaluated using test dataset (2014) by sliding 1 day. Furthermore, MF-NPM was validated with the LSTMNN model, IGS GIM, and CODE 1-day predicted GIM products (C1PG) from the spatiotemporal perspective during the solar maximum phase (2014) and geomagnetic storm. The results show that the MF-NPM achieves good prediction performance effectively. In terms of temporal perspective, MF-NPM achieves the best performance with RMSE and relative accuracy (RA) of 2.33 TECU and 93.75%, outperforming LSTMNN and C1PG, which are (3.10 TECU, 91.84%) and C1PG (4.20 TECU, 87.07%), respectively, in solar maximum (2014). Additionally, during geomagnetic storms, the results suggest that RMSE and RA of MF-NPM are 3.12 TECU and 92.86% which are better than LSTMNN and C1PG, which lead to RMSE value of (4.37,5.42) TECU, RA as (90.48, 85.62)%, respectively. From the spatial perspective, the RMSE and RA of MF-NPM are 3.24 TECU and 93.33% which are superior to LSTMNN (4.32 TECU, 91.21%) and C1PG (5.29 TECU, 89.13%) in low-latitudes, respectively. In addition, MF-NPM also achieves better performance than LSTMNN and C1PG in the mid-latitude region with respect to the RMSE and RA, which are improved by (0.52 TECU, 1.73%) and (2.20 TECU, 8.59%), respectively. All the results prove that the proposed model can capture the variations of ionospheric TEC more accurately than LSTMNN and C1PG under high solar activity and geomagnetic storms conditions over China.


AS52-A015
Global IGS-3D Electron Density Model by Deep Learning

Eun-Young JI1#+, Yong-Jae MOON2, Young-Sil KWAK3, Kangwoo YI1, JeongHeon KIM3
1Kyung Hee University, 2School of Space Research, Kyung Hee University, 3Korea Astronomy and Space Science Institute

We develop a global IGS-3D Ne model that generates global 3-D electron density (Ne) from International Global Navigation Satellite Systems (GNSS) Service (IGS) total electron content (TEC) data through deep learning. As a first step towards this, we construct a model to generate a vertical electron density profile from a TEC value using Multi-Layer Perceptron (MLP). In this process, the vertical electron density profiles (100 km ~ 700 km altitude, ~25 km altitude interval) and the corresponding TEC values of the IRI-2016 model from 2001 to 2013 with resolutions of 2 hours in time, 2.5° in latitude, and 5° in longitude are used. We use the IRI vertical density profiles (approximately 4.2 million) from 2001 to 2008 for training, 2009 for validation, and 2010 to 2013 for a test. The next step is to generate global IGS electron density profiles using the global IGS TECs as input data for the model, which is called the global IGS-3D Ne model. We evaluate the IGS-3D Ne model by comparing the electron density profiles from the incoherent scatter radars (ISRs) at three stations (low, middle, and high latitudes) with the IGS-3D Ne model from 2010 to 2013. The evaluation shows that the electron density profiles from the IGS-3D Ne model are closer to the ISR data than those of the IRI model, especially at high latitudes. The IGS-3D Ne model shows that the averaged RMSE values between IGS and ISR electron density profiles are 0.37 log(m-3), 0.22 log(m-3), and 0.34 log(m-3) for all test datasets at Jicamarca, Millstone Hill, and EISCAT stations, respectively. These results suggest that our IGS-3D Ne model has sufficient potential to enhance the ability to predict global electron density profiles.


Fri-04 Aug | 8:15 - 10:00 | MR311
AS08 - Atmospheric Light Scattering and Remote Sensing

Session Chair(s):

AS08-A004 | Invited
Aerosol Direct Radiative Effects at the ARM SGP Site Based on Raman Lidar Observations

Qiang FU#+
University of Washington

Atmospheric aerosols exert a large influence on Earth’s climate. Both natural and anthropogenic aerosols are important since the formal is a prerequisite for an accurate assessment of impacts of the latter on the climate change. For the role of aerosols both natural and anthropogenic in the climate system, the most fundamental understanding starts with the knowledge of aerosol direct radiative effects. In this talk, I will present our efforts to quantify all-sky aerosol direct radiative effect (DRE) with uncertainty estimates at the Atmospheric Radiation Measurement (ARM) Southern Great Plains (SGP) site by using multiyear ground-based observations including aerosol and cloud vertical extinction profile from Raman lidar; spectral aerosol optical depth, single-scattering albedo, and asymmetry factor from Aerosol Robotic Network; cloud water content profiles from cloud radars; temperature and water vapor profiles from radiosondes; and surface shortwave spectral albedo from radiometers. We find that at the ARM SGP site where the cloud occurrence frequency is 0.62, the annual mean all-sky aerosol DRE at the top of the atmosphere is −2.13 ± 0.54 W m−2, compared to −3.00 ± 0.58 W m−2 for clear-skies.


AS08-A011
Advancing Aerosol Remote Sensing Over Ocean Using PACE Multi-angle Polarimetric Measurements

Meng GAO1#+, Kirk KNOBELSPIESSE2, Bryan FRANZ2, Pengwang ZHAI3, Brian CAIRNS4, Jeremy WERDELL2
1SSAI, NASA GSFC, 2NASA Goddard Space Flight Center, 3University of Maryland, Baltimore County, 4NASA Goddard Institute for Space Studies

The NASA Plankton, Aerosol, Cloud, ocean Ecosystem (PACE) mission has been designed with the goal of studying the global ocean and atmosphere, with a focus on improving data records of ocean ecology, biogeochemistry, atmospheric aerosols, and clouds. The mission is equipped with state-of-the-art instruments, including the Ocean Color Instrument (OCI), a hyperspectral scanning radiometer, and two Multi-Angle Polarimeters (MAPs), namely the UMBC Hyper-Angular Rainbow Polarimeter (HARP2) and the SRON Spectro-Polarimeter for Planetary EXploration one (SPEXone). These MAP measurements hold a wealth of information that can be used to enhance aerosol and ocean color observations simultaneously, and the PACE mission plans to produce a suite of advanced data products with high accuracy. To achieve these goals, we have developed a highly efficient aerosol and ocean color retrieval algorithm, FastMAPOL, which is based on neural network forward models and Jacobians. This presentation will explore ways to further improve retrieval performance through multi-angle cloud masking, adaptive data quality control, and uncertainty model analysis considering uncertainty correlations. These methods provide a mechanism to evaluate the forward and uncertainty models, thereby improving our understanding of MAP data and guiding algorithm developments. The effectiveness of our algorithm has been demonstrated through retrieval studies on both synthetic HARP2 and real AirHARP measurements. The algorithm and associated experience will be valuable for efficiently processing the large volume of MAP data that will be acquired by the PACE mission and similar future Earth observing satellite missions.


AS08-A003
Aerosol Microphysical Properties Retrieved from Dual-polarization Lidar Measurements

Qingqing DONG#+, Zhongwei HUANG, Xintai SHEN, Jianrong BI, Tian ZHOU, Shuang ZHANG
Lanzhou University

Aerosol properties such as particle size distribution, shape and optical properties are important parameters to accurately evaluate its radiative forcing. Single scattering albedo (SSA) can characterize the proportion of aerosol absorption and scattering, and is a vital optical parameter to measure the aerosol absorption. However, its vertical distribution still cannot be obtained by remote sensing currently. Here we proposed a novel method for retrieving profile of aerosols SSA from observation of dual-polarization lidar system developed by Lanzhou University, which can simultaneously detect polarization measurements at 355 nm and 532 nm. The results show that lidar-retrieved aerosols SSA are reliable, validated by field observation by collocated radiosonde balloon. The correlation coefficient (R2) between lidar SSA and in situ results reaches up to 0.7. Our study firstly provides a new way for obtaining range-resolved aerosol SSA with high spatial-temporal resolution, which can be widely used and further improve assessment ability of aerosol climatic effect.


AS08-A010
A Potential Feedback Mechanism of Springtime Arctic Snow/ice Algae, Biological Aerosols and Arctic Clouds

Yongxiang HU1#+, Patricia LUCKER2, Wenbo SUN2
1NASA Langley Research Center, 2Science Systems and Applications, Inc.

Water cloud droplet number density (Nd) can be accurately estimated from CALIPSO lidar measurements (Hu et al., 2021, https://www.frontiersin.org/articles/10.3389/frsen.2021.724615/full). One interesting findings from the new droplet number density statistics is the huge Nd values of boundary layer clouds in the springtime Arctic (Figure attached). Comparing Nd with chlorophyll biomass of snow/ice algae calculated from high resolution Arctic models, we found excellent spatial/temporal correlations between the two. I will introduce the lidar measurements of water cloud microphysical properties and a hypothesis of a positive feedback mechanism of springtime Arctic snow/ice algae, biological aerosols and Arctic clouds. I will also introduce the ongoingICESAT-2 data analysis of snow properties (Hu et al., 2022, https://www.frontiersin.org/articles/10.3389/frsen.2022.855159/abstract) that may help evaluate the feedback mechanisms. Figure 1. Left panel: droplet number concentration of Arctic boundary layer clouds in April derived from CALIPSO lidar measurements; Right Panel: Snow algae biomass of the same time period. 


AS08-A008
Forward and Inverse Models for Satellite Remote Sensors Using Principal Component Analysis

Xu LIU#+
NASA Langley Research Center

Satellite remote sensors such as AIRS on Aqua, CrIS on S-NPP, NOAA20 and JPSS-2, IASI on Metop A, B, and C make millions of observations each day with thousands of spectral channels for each observation; this poses challenges for efficiently inversion of the inherently large dataset as needed to retrieve atmospheric and surface properties. This presentation will illustrate the use of Principal Component Analysis (PCA) to speed up radiative transfer forward model calculations and to stabilize the inversion algorithms. A Principal Component-based radiative transfer model (PCRTM) developed at NASA Langley Research Center can simulate top of atmosphere (TOA) radiance or reflectance spectra from 50 cm-1 to 50000 cm-1 (200 mm to 0.20 mm quickly and accurately. PCRTM demonstrated very high accuracy relative to reference line-by-line radiative transfer models and it saves orders of magnitude computational time. Examples of the PCRTM model developed for hyperspectral sensors such as AIRS, CrIS, IASI, NAST-I, SHIS, CPF, TEMPO, SBG, OMI, and SCIAMACHY will be presented. In addition to using the PCRTM as forward model, the NASA Langley developed inversion algorithm also uses PCA to compress the state vector into a compressed dimension to speed up and stabilize the inversion process. Examples of retrieved atmospheric temperature, water vapor, CO2, CO, CH4, N2O, and O3 profiles, cloud properties (optical depth, size, phase, and height), and surface properties (surface emissivity spectra and skin temperatures) will be presented. This algorithm is being transitioned to the NASA Sounder SIPS and NASA's Goddard Earth Sciences Data and Information Services Center (GES DISC).


Fri-04 Aug | 8:15 - 10:00 | MR323
AS37 - Monitoring, Analysis, and Prediction of Typhoon and Climate Affecting Taiwan and the Philippines

Session Chair(s): Mong-Ming LU, National Taiwan University, Ana Liza Solmoro SOLIS, Philippine Atmospheric, Geophysical and Astronomical Services Administration

AS37-A014
The Development of User-oriented Sub-seasonal to Seasonal Forecast Products for Water Resource Management in Taiwan

Tzu-Ting LO1#+, Ching-Teng LEE2, YunChing LIN2, SzuYing LEE2, Jui-ling KUO2, Yun-Jing CHEN2, Meng-Shih CHEN2, Hsiao-Chung TSAI3
1National Taiwan University, 2Central Weather Bureau, 3Tamkang University

From 2020 to 2021, an unprecedented drought event happened in Taiwan. In the face of water shortage, sub-seasonal to seasonal forecast products were developed to facilitate decision-making for water resource management. For monitoring the evolution of drought condition, high resolution (~1km) drought indices of SPI and SPEI were calculated to provide early warning information and decrease the risks of crop and food loss. This real-time drought monitor system with 1-km grid rainfall observation data all over Taiwan proved to be very useful for water resource management and agriculture. Meanwhile, high-resolution space-time rainfall seasonal forecast products were developed with a statistical downscaling method using ECMWF's fifth generation seasonal forecast system (SEAS5) forecast products. Moreover, for the wet season from May to October, an extended-range TC forecast product has been developed to provide extreme rainfall information from CWB TC Tracker system (https://tctracker.cwb.gov.tw). The system provides the TC tracking results obtained from multiple global ensemble models, such as the NCEP GEFS (GEFSv12; FV3-based), CFSv2 (Climate Forecast System version 2), ECMWF extend-range forecast system and the CWB 1-tier climate forecast model. The CWB TC Tracker also has been utilized by the forecasters at CWB, NCEP CPC (Climate Prediction Center), and PAGASA (Philippine Atmospheric, Geophysical and Astronomical Services Administration) to monitor extended-range TC formations and subsequent tracks. Further details about real-time extended-range TC forecast applications with large-scale factor will be presented in the meeting.


AS37-A002
Interannual Processes Suppressing Tropical Cyclone Activity Around Taiwan During October

Jau-Ming CHEN1#+, Wei-Teh LI2
1National Kaohsiung University of Science and Technology, 2National Sun Yat-sen University

In October, TCs originating in the WNP and later affecting Taiwan are very few. For the period 1970-2019, zero TCs affected Taiwan in 32 out of 50 years with the other 18 years only experiencing one TC per year. For the 32 years with zero TCs in Taiwan, suppressed TC activity results from different modulating processes imposed by various climatic features. During October of El Niño years, TC genesis in the WNP tends to shift eastward with a decrease in the western WNP to the southeast of Taiwan. An anomalous anticyclone across the SCS and Taiwan prevents TCs from moving toward Taiwan. In La Niña years, TC genesis features are largely opposite to those of El Niño years. Increased TC genesis occurs in the region southeast of Taiwan. These TC are guided by an anomalous cyclone centering in the SCS to result in major TC tracks to the southwest of Taiwan toward the SCS. A year with a September-November value of Ocean Niño Index (ONI) between 0o-0.5oC (-0.5o-0oC) is categorized as a positive (negative) Normal year. During the positive Normal years, an anomalous cyclone over the WNP causes more TC genesis in its southern section and guides these TCs northward along the regions east of Taiwan toward its central zone. An accompanying anomalous anticyclone over the SCS and Taiwan also hinders TC movement toward Taiwan. During the negative Normal years, a westward elongation of warm sea surface temperature anomalies from the WNP into the Maritime Continent forces an anomalous anticyclone to extend westward from the WNP toward the SCS. TC genesis in the southern section of this anomalous anticyclone thus decreases and consequent TC movement is also blocked from moving northward/northwestward toward Taiwan. Under the above modulating processes, TC activity is suppressed in Taiwan during October.


AS37-A001
Large-scale Processes Modulating the Frequency of Typhoons Affecting Taiwan During 1900–1945

Pei-Hua TAN1#+, Jien-Yi TU2, Pen-Yuan CHEN1
1National Chiayi University, 2National Changhua University of Education

The typhoons affecting Taiwan during 1900–1945 are defined as those with a low-pressure center making a landfall in Taiwan or moving near Taiwan and included in disaster reports. The annual and monthly numbers of typhoons were lower during 1900–1945 than during 1970–2015, which might be attributed to the colder environ­ment, a weakened western North Pacific subtropical high with the eastward retreat and lack of satellite detection techniques during 1900–1945. However, the monthly percentages of typhoons were comparable in the high-frequency months of July–Sep­tember during the two periods. In contrast to the warm period, the cold period had fewer total typhoon numbers but more concentrated occurrence during May–Octo­ber. During 1900–1945, an interannual variability of the typhoon frequency affecting Taiwan was observed. During the typhoon-more (typhoon-less) years, the significant sea surface temperature patterns were dominated by warm (cold) anomalies elongat­ing the tropical central-eastern Pacific with a maximum center in the central Pacific and cold (warm) anomalies over the tropical western Pacific. The anticyclonic (cy­clonic) circulation around Taiwan that responds to a divergent (convergent) center in the Maritime Continents tended to provide a favorable (unfavorable) steering flow to force typhoons over the east of the Philippines moving westward/northwestward (eastward) toward (away from) Taiwan. The modulations of intraseasonal oscilla­tions on typhoon movements under the westward/northwestward and northward tracks of typhoons affecting Taiwan exerted a positive but different effect on steering the typhoon toward or near Taiwan.


AS37-A012
The Development and Improvements of Global Ensemble Prediction System in Center Weather Bureau (CWBGEPS)

Jia-Ying WU1#+, Pei-Hsuan KUO2, Pang-Yen LIU1, Jen-Her CHEN1, Ting-Huai CHANG1
1Central Weather Bureau, 2National Central University

The new version of Global Ensemble Prediction System in Center Weather Bureau (CWBGEPS v2.0) is for extended weather prediction that generates one deterministic and 20 ensemble members forecasts for 45 days. This new model system uses octahedral reduced Gaussian grid (Malardel et al. 2016) coordinate at a base horizontal resolution of ~28km(TCo383) and 72 layers in vertical with Non-iteration Dimensional-split Semi-Lagrangian (NDSL, Juang 2007& Juang 2008) two-time levels dynamical core. The initial fields of prediction system for both deterministic model and ensemble members are come from our own FV3GFS(Finite-Volume Cubed-Sphere Global Forecast System) data assimilation system. The CWBGEPS v2.0 is going to operational in June 2023, and initialized at 00UTC each day for producing 45 days forecasts. Since the lower resolution prediction system is hard to well simulate the interaction between complex terrain over Taiwan and the weather system; besides, considering the limit of the computing resources, the upcoming version of CWBGEPS v2.1 will couple the high-resolution regional spectral model(RSM, Juang and Kanamitsu 1991) for dynamical down scaling instead of increasing the resolution of the global model. The RSM model had been nested into CWB climate model via Multi-Program Multiple-Data (MPMD) technique in 2018 for dynamic downscaling of short-term climate forecast in Taiwan (Chen et al. 2018). In CWBGEPS v2.1, we adopt the same MPMD technique to couple CWBGFS and RSM. This research will introduce the structure, development, and improvements of CWBGEPS v2.1.


AS37-A017
The Taiwan WRF Ensemble Prediction System: Enhancement of Initial Perturbation via Integration with a Global Ensemble Prediction System

Chih-Hsin LI#+, Guo-Yuan LIEN, Wen-Hsin TENG, Yi-Jui SU
Central Weather Bureau

A Weather Research and Forecast (WRF) model based regional ensemble prediction system (WEPS) has been developed and operationally maintained by the Central Weather Bureau of Taiwan since 2011. The WEPS employs ensemble initial conditions from a regional Ensemble Adjustment Kalman Filter (EAKF) system, lateral boundary conditions from NCEP global ensemble forecast system (GEFS), multi-physics ensemble, and stochastic physics. For performance consideration, the ensemble initial conditions are further blended with analysis from CWB’s WRF-based deterministic prediction system, taking the large-scale information from the latter. Though the WEPS has achieved satisfactory forecast skill with the current design, an issue of insufficient ensemble spread in early forecast time has been noted. In this study, a new approach for initializing the WEPS members is proposed. Inspired by the partial cycle and blending strategy that has been successfully implemented in the regional deterministic system at CWB, the new approach separately initializes regional ensemble members as individual partial cycles. Therefore, the regional ensemble system is now closely integrated with a global ensemble prediction system, while the mesoscale observation information can still be utilized by the partial cycling with 3DVAR data assimilation. Results show that this new method is superior to the current operational WEPS in terms of most ensemble forecast verification metrics, including a significant improvement in the spread-error relationship, especially in early forecast time. The typhoon track forecasts are also benefited from the new method. Overall, this new regional ensemble initialization method has shown good potential for use in the next version of the WEPS at CWB.


AS37-A018
The Next-generation Global Prediction System Development and Operational Implementation at Taiwan’s Central Weather Bureau

Ling-Feng HSIAO#+, Guo-Yuan LIEN, Jen-Her CHEN, Jing-Shan HONG, Chin-Tzu FONG
Central Weather Bureau

Central Weather Bureau (CWB) has cultivated the technique for numerical weather prediction (NWP) from 1983. The NWP provides accurate weather forecasts and extreme weather forecasts for Taiwan. In recent years, CWB has developed a new generation global NWP system based on the Finite-Volume Cubed-Sphere dynamical core (FV3) used at the U.S. National Centers for Environmental Prediction (NCEP). The next-generation Global Prediction System with the FV3 dynamical core (FV3GFS) at CWB includes the horizontal resolution of C384 (~25 km) and a hybrid 4D ensemble–variational data assimilation (4DEnVar). In addition, a nested domain (4.8 km resolution) around Taiwan is also implemented to examine the extreme precipitation. The model has 64 vertical levels with the model top at 0.2 hPa and the NCEP GFS physics package. The important difference of physics upgrades is the replacing of the Zhao–Carr cloud microphysics scheme with the GFDL cloud microphysics scheme. Regarding the data assimilation research and development, the stochastic physics methods have been enabled in the ensemble Kalman filter (EnKF) system to optimize the ensemble spread. The time-lagged ensemble method for the hybrid 4DEnVar assimilation has been implemented and tested to increase the usable ensemble size. Results from statistics in 2022 show that the CWB FV3GFS is superior to the operational CWBGFS, which significantly improves synoptic-scale features and the typhoon track forecasts. This system is expected to be used in operation in this year. The detailed results will be presented in the conference.


AS37-A021
Sensitivity Analysis on WRF-generated Models for Tropical Cyclones During Winter La Nina

Ana Liza Solmoro SOLIS1#+, Esperanza CAYANAN1, Joseph BASCONCILLO1, Mong-Ming LU2
1Philippine Atmospheric, Geophysical and Astronomical Services Administration, 2National Taiwan University

This study aims to determine predictability in simulating tropical cyclones for weeks 3-4 and compare the performance of two configurations: the CMA Scheme (Di et al., 2019) and the Tropical Suite scheme (UCAR, 2022) with a benchmark. Because re-analyses are usually not available in real-time, the CFSv2 model was used as the lateral boundary forcing of the Weather and Research Forecasting (WRF) model. Three tropical storms, Washi, Melor and Nockten during the December-January-February season or winter La Nina with active phases of MJO were simulated and tested the effect of domain resolution and adjusted the initialization times using three nested domains. We adopted the vortex following nesting option in tracking the center of low pressure in a tropical cyclone. We determine the initial moment when the storm hit a 35-knot mark. A clear advantage of using this vortex-following grid is that the tropical cyclone will always be centered in the highest resolution and in all moving nests. Fine-tuning was done by setting grid ratios and downscaling. Analyses show that the two tropical suite experiments with different initialization times had similar levels of accuracy in terms of direct position error, with mean errors of around 80 and 90 kilometers, respectively. Additionally, the tropical suite run which was initialized 12 hours after Day zero had the lowest direct positional error, with a mean error of less than 100km. Therefore, the Tropical Suite Scheme performed better in terms of central pressure, with more consistency and the lowest error according to both the MAE and RMSE measures suggesting reliability in predicting both typhoon positions and central pressures.


Fri-04 Aug | 8:15 - 10:00 | MR327
AS51 - Understanding and Predicting Precipitation Extremes Through Integrative Analyses of Observation, Numerical Models, and Deep Learning

Session Chair(s): Xiaoming SHI, The Hong Kong University of Science and Technology, Ji NIE, Peking University

AS51-A002
Constraining Global to Continental Future Extreme Precipitation Intensification

Seungmok PAIK1+, Soon-Il AN1#, Seung-Ki MIN2, Andrew KING3, Soong-Ki KIM1
1Yonsei University, 2Pohang University of Science and Technology, 3The University of Melbourne

Extreme precipitation (annual maximum daily precipitation, Rx1day) intensification under global warming have received attention, but large uncertainties still exist how much Rx1day will increase in future even under same emission pathway. Based on scaling analysis, dynamics (i.e., atmospheric circulation changes) are found to cause regional deviation of future Rx1day variations as well as inter-model spread in each region (grid) under relatively homogeneous thermodynamic contributions (i.e., atmospheric humidity increases). In contrast, over broader regions average, thermodynamics have greater to comparable influence on uncertainty of Rx1day projections with dynamic contributions. From global to individual continent averages, climate models historical warming trends present strong inter-model correlations with magnitudes of future Rx1day intensification, which mostly be related to thermodynamic contributions. CMIP6 models generally overestimate observed global to continental historical warming, resulting smaller Rx1day increases than raw model projections when it is constrained based on observed historical warming trends with strongly reduced uncertainties (e.g., mean and spread of Rx1day intensification is decreased to 25% and 27%, respectively, in global average under high-emission scenario). Our results suggest that future Rx1day increase will be weaker than raw model projections. Nevertheless, strong Rx1day increases will evidently occur, supporting demand of strong adaptation and mitigation strategies. We will also present model-simulated, constrained future projection with considering diverse precipitation intensities, time-scales with comprehensive understanding dependence of the results from different precipitation characteristics.


AS51-A004
Evaluation of a Scale-similarity Subgrid-scale Closure in Idealized Squall Line Simulations at Kilometer-scale Resolutions

Shiwei SUN1,2#+, Bowen ZHOU3, Kefeng ZHU4, Ming XUE5
1Nanjing Joint Institute for Atmospheric Sciences, Chinese Academy of Meteorological Sciences, 2China Meteorological Administration, 3Nanjing University, 4Chinese Academy of Meteorological Sciences, 5The University of Oklahoma

The subgrid-scale (SGS) turbulent mixing plays an important role in severe weather simulations at kilometer-scale resolutions. Sun 2021 JAS introduced a scale-similarity-based nonlinear SGS closure (Hgrad closure hereafter) in supercell simulations, which is 3D, scale-aware, and could produce counter-gradient SGS fluxes. Here we expanded the work to idealized squall line simulations. A large-eddy simulation (LES) with 50-m grid spacing was conducted and the outputs were filtered horizontally to 250 m, 500 m, 1 km, 2 km, and 4 km grid spacings to get the benchmarks at kilometer-scale resolutions. Significant counter-gradient SGS fluxes were observed within the convective region in both horizontal and vertical directions for heat, water vapor, and water contents. These SGS transports were generally from bottom to top in the vertical direction, and from head (towards the moving direction) to tail in the horizontal direction. The filtered LES variables were substituted into two SGS closures to evaluate the offline behavior: the Hgrad closure and the well-used 1.5-order turbulent kinetic energy closure (TKE closure). TKE closure could not generate counter-gradient fluxes so produced SGS fluxes with wrong directions in many regions of the convective core. The Hgrad model reproduced the counter-gradient SGS transports well and the distribution and magnitudes of the SGS fluxes were similar to that of the results from LES. The Hgrad and TKE closures were further evaluated in the online simulations in which the SGS parameterizations could be chosen differently in horizontal and vertical directions. Simulations with the 3D Hgrad scheme performed better than the 3D TKE scheme in the strength of the updraft motion, the depth of the cold pool, and the precipitation. Simulations with horizontal Hgrad and vertical TKE performed better than the cases with horizontal TKE and vertical Hgrad, hinting at the significant contribution of horizontal mixing in severe weather simulations.


AS51-A005 | Invited
The Impact of Marine Boundary Layer Jet on Extreme Rainfall in South China

Yu DU#+
Sun Yat-sen University

The characteristics of boundary layer jets (BLJs) over South China Sea (SCS) and their impacts on extreme rainfall are examined using scientific-research-ship observations and reanalysis. Typically, the BLJs exhibit a maximum intensity at night and reach their peak at 950 hPa. They are formed by the large-scale diurnal land-sea thermal contrasts under the background of the monsoon flow. The emergence of the BLJs leads to increased rainfall in South China, particularly in areas downstream of each BLJ. The strengthened BLJs drive mesoscale ascent on their northwestern edge and terminus, creating enhanced convergence zones and promoting convection initiation and upscale convective growth dynamically. From a thermodynamic perspective, the BLJ-driven mesoscale ascent combined with high sea surface temperature strengthens the warm moist tongue over the SCS, allowing it to farther extend northward and reach the coast of South China. The study also investigates the sensitivity of the simulated BLJ and associated precipitation in South China to different planetary boundary layer parameterization schemes. Results show that both too strong or too weak BLJs are unfavorable for extreme rainfall in South China.


AS51-A006 | Invited
Improvement of a Cloud Microphysics Scheme and its Advantage in the Precipitation Simulation Along the Sichuan-Tibet Railway

Chunsong LU1#+, Xiaoqi XU2, Zhiwei HENG3
1Nanjing University of Information Science & Technology, 2Nanjing Joint Institute for Atmospheric Sciences, 3Chengdu Institute of Plateau Meteorology

The Sichuan-Tibet Railway is an important part of railway network in China. The topography along the railway leads to frequent geological disasters such as mountain torrents and landslides in this area, and precipitation is the main cause of these disasters. Therefore, accurate simulation of precipitation in this area is crucial. The Weather Research and Forecasting Model is used to simulate multiple precipitation events in the area along the Sichuan-Tibet Railway during the flood-season of 2021. Several liquid-phase cloud microphysical processes in Morrison scheme are improved, including activation of cloud droplets, autoconversion, accretion, and entrainment-mixing. The advantages of improving these processes for precipitation simulation along the Sichuan-Tibet Railway are explored. Comparison of precipitation and cloud with observations shows that the improvement of these microphysical processes has positive effects on the simulation of precipitation and clouds. Compared to the default microphysics scheme, the improved scheme obviously alleviates the overestimation of precipitation intensity and distribution range. The improved scheme also has more reasonable cloud physical quantities than the default scheme. Especially, adding the cloud droplet activation process to the microphysics scheme and updating the cloud droplet number concentration instantaneously has the most significant impact on cloud microphysics and precipitation processes. When the concentration of cloud droplet number is fixed in the default scheme, unreasonable large cloud droplet size could be produced, which further affects physical processes (such as autoconversion) and leads to bias in cloud microphysics and precipitation simulations. The simulation of multiple precipitation events shows that the improvement is not limited to a certain case but is generally effective. The results obtained in this study can provide a reference for further improving simulation/forecast of precipitation and disaster prevention in this area in the future.


AS51-A003
Is the 2021 Peninsular Malaysia Flood Truly a ‘Once-in-a-century’ Event?

Jingyu WANG#+, Luojie DONG, Edward PARK, Xianfeng WANG
Nanyang Technological University

Super typhoon Rai swept over the South Philippines and East Malaysia in December 2021, which has caused nearly 400 deaths and enormous financial loss. While these regions were being ravaged by Rai, 1,500 km west to the typhoon path, a catastrophic flooding event hit Peninsular Malaysia, resulting in socioeconomic impacts comparable to that of Rai. During December 16-18, Peninsular Malaysia received record-breaking 3-day precipitation. Based on a storm tracking algorithm with the inputs of satellite observations, two mesoscale convective systems (MCSs) are identified most conductive to the flooding event, and their characteristics are revealed in this study. Regarding the key synoptic factors that drive the heavy precipitating MCSs, a long-range easterly water vapor corridor is found to continuously provide moisture supply to the tropical depression over the peninsula, making the two MCSs explosive. Frequency analyses of key drivers show the return period of such strong precipitation is truly ‘once-in-a-century’.


AS51-A018 | Invited
Convection-permitting Simulation of Precipitation Over Asia with Global Variable-resolution Model

Chun ZHAO#+
University of Science and Technology of China

To simulate simultaneously the small-scale and large-scale processes of the rainfall system and their interactions, non-hydrostatic global variable-resolution models with regional refinement at convection-permitting scale may provide a more effective way compared to non-hydrostatic global uniform high-resolution modeling and limited-area regional modeling at convection-permitting scale. This talk will present some studies using a global variable-resolution model to conduct the experiments with regional refinement at convection permitting resolution over some key areas of Asia such as East Asia and the Tibetan Plateau. These areas have active convective systems in summer and are also with complex topography that may affect regional weather and climate systems. The modeling results are evaluated and analyzed with the focus on the spatial and temporal characteristics of precipitation in summer over these areas. The mechanisms driving the variation of precipitation revealed by the experiments are also examined.


AS51-A016
Role of Aerosol Ice-nucleation Effect in the Development of the ‘21 7 Henan Extreme Precipitation

Weishan WANG#+, Guoxing CHEN, Yijun ZHANG
Fudan University

Aerosols can affect clouds and precipitation by serving as cloud condensation nuclei and ice nuclei (IN). However, these effects are seldom considered in the operational numerical weather forecast. This study investigates the role of aerosol ice nucleation effect in the ’21 7’ extreme precipitation event that occurred to Henan, China in July 2021 using an aerosol-aware WRF Model. The control simulation prescribed spatio-temporal varying IN concentration estimated using the dust fields in the MERRA2 aerosol reanalysis, while the sensitivity simulation prescribed spatially uniform and temporally constant IN concentration. Results show that the control simulation yields more ice crystals than the sensitivity simulation as the precipitation initiates. This leads to more latent-heat release and larger vertical velocity, and subsequently shifts the precipitation center to Zhengzhou. Overall, the 24-hour precipitation in 7/20 from the control simulation is closer to the observation results in both intensity and spatial distribution than that in the sensitivity simulation. More analyses will be presented within the context of detailed mechanisms between the ice nucleation and the shifting of precipitation location.


Fri-04 Aug | 8:15 - 10:00 | MR328
AS13 - Polar Atmospheric Processes and Their Interactions with the Surface

Session Chair(s): Myong-In LEE, Ulsan National Institute of Science and Technology, Yuekui YANG, NASA Goddard Space Flight Center

AS13-A018 | Invited
Investigate the Feedback Mechanisms of Arctic Clouds and Radiation on Sea Ice Changes

Xiquan DONG1#+, Baike XI2, Yiyi HUANG1
1University of Arizona, 2The University of Arizona

Since the dawn of the satellite era, Arctic summer sea ice coverage has declined by nearly 50% and this decline has accelerated in the early 21st century. The Arctic sea-ice variations are caused by different dynamic and thermodynamic processes. The surface energy budget anomaly is one of the most important thermodynamic forces associated with Arctic sea-ice changes. Clouds impact the long-term trend and year-to-year variability of Arctic sea ice due to their strong modulation of radiative energy fluxes at the surface. In this study, we have investigated the role of cloud-radiation feedback in modulating Arctic sea ice changes from weekly to interannual time scales through an integrative analysis of satellite observations, global reanalysis products and model simulations. Through this study, we want to tentatively answer the following three scientific questions: How do the radiative effects of clouds and water vapor modulate the melt onset of Arctic sea ice in spring? How do the melt season cloud and radiation properties have an impact on the September sea ice concentration decline?


AS13-A006
Effects of Large-scale Changes in Environmental Factors on the Genesis of Arctic Super Cyclones

Yujun LIU+, Yijun HE#
Nanjing University of Information Science & Technology

The Arctic cyclone is an active weather system in the Arctic, and the Arctic extreme cyclone (AEC) strongly influences polar weather. Thus, many studies have focused on the activity of AEC and its relationship with large-scale circulation in the Arctic. In this study, Arctic cyclones were detected using the ERA5 Reanalysis data from 1979 to 2020, and the AECs of cold and warm semesters were defined using the 5th percentile of sea level pressure. An Arctic cyclone genesis index, GPIArctic, is established by using the least square fitting of absolute vorticity, omega, wind shear, and long-wave radiation with Eady growth rate. Our findings show that wind shear and long-wave radiation strongly influence AECs. In the cold semester, the high value of GPIArctic mainly occurs in the south of Greenland, while in the warm semester, the high value of GPIArctic also occurs in northeast Eurasia. The results of the multi-model integration of CMIP6 show that more AECs will be formed in the Arctic in the future (2021–2050), and their seasonal contrast will be stronger in northeast Eurasia.


AS13-A008
Warming in the Arctic Due to Ocean Dynamics from Northern Extratropical Radiative Cooling

Ruomei RUAN1+, Sarah KANG2#, Lei ZHOU1, Xiao-Tong ZHENG3, Hai WANG3, Fukai LIU3
1Shanghai Jiao Tong University, 2Ulsan National Institute of Science and Technology, 3Ocean University of China

Greenhouse-induced warming causes a pronounced warming amplification and sea ice decline over the Arctic. However, it is yet unclear how anthropogenic aerosol-induced radiative cooling affects the Arctic climate. Using the idealized experiments with a hierarchy of the Geophysical Fluid Dynamics Laboratory model, here we investigate the Arctic climate response to radiative cooling prescribed over major aerosol emission areas in the northern extratropics. In a slab ocean configuration, the Arctic cools regardless of the position of prescribed radiative cooling. By contrast, in a fully-coupled configuration, unlike a radiative cooling over North America and North Asia, a radiative cooling over Europe causes the Norwegian and Barents Seas to warm via the intensified Norwegian Atlantic Current associated with the large-scale low-pressure anomaly west of the prescribed cooling. Our results suggest that better knowledge about the spatial distribution of aerosol forcing will help improve the ability to simulate and predict the Arctic climate.


AS13-A012
Observed Contribution of Barents-Kara Sea Ice Loss to Warm Arctic-cold Eurasia Anomalies by Submonthly Processes in Winter

Li YANQIN1+, Li ZHANG1, Bolan GAN1#, Hong WANG1, Xichen LI2, Lixin WU1
1Ocean University of China, 2Chinese Academy of Sciences

The warm Arctic-cold Eurasia (WACE) pattern of surface air temperature anomalies is a prominent feature of the Eurasian climate variations during boreal winter. The interannual WACE anomalies are accompanied by sea ice loss in the Barents-Kara (BK) seas, however, the causality between them remains controversial because of large internal atmospheric variability over subarctic Eurasia in winter. Here we disentangle the contribution of BK sea ice loss to the WACE anomalies based on a statistical decomposition approach. An anticyclonic circulation anomaly over subarctic Eurasia that forces the WACE anomalies is found to reach its peak 3 days prior to BK sea ice loss. After excluding this prior atmospheric forcing signature, the East Asian cooling matures about 15 days later as a result of the weakened moisture transport associated with the enhanced BK downstream ridge and East Asian trough due to BK sea ice loss. The results suggest that BK sea ice loss contributes ~65% and ~81% of the WACE-related East Asian cooling and Arctic warming at interannual timescale, respectively, whereas the WACE-related cooling over central Eurasia primarily results from internal atmospheric variability. Such submonthly lagged East Asia cooling caused by BK sea ice loss could be helpful in predicting winter extreme cold events over East Asia.


AS13-A016
Jet Response to Arctic Warming in Idealized GCM

Gun-Hwan YANG+, Baek-Min KIM#, Woosok MOON, Hayeon NOH
Pukyong National University

To examine the impact of Arctic amplification on mid-latitude extreme weather event, we investigated the local and remote circulation response to the pan-Arctic and the regional thermal forcing confined to the Arctic. An idealized atmospheric GCM (General Circulation Model) coupled with a slab mixed layer ocean is used for the experiment. With the increasing thermal forcing in the pan-Arctic, the mid-latitude jet moves toward the equator due to the southward shift of the eddy-heat and eddy-momentum flux convergence zone. Impose the regional thermal forcing in the polar region, zonal mean response is similar to the response from the pan-Arctic configuration. The non-zonal response is characterized by an enhanced wavy jet in the mid-latitude, due to the 300-hPa circumpolar zonal wind of wavenumber 1 structure. In regional warming simulation, the residual heat flux increased due to a dipole pattern in the polar region, leading to enhanced heat advection to the mid-latitude.


AS13-A004
Antarctic Blowing Snow Diagnosis with MERRA-2 Reanalysis Using a Machine Learning Model

Yuekui YANG#+
NASA Goddard Space Flight Center

Over Antarctica, snow is frequently lifted by wind and forms blowing snow, which can extend hundreds of thousands of square kilometers in area and reach hundreds of meters in height. Blowing snow affects ice sheet mass balance and hydrological processes by redistributing surface mass and driving spatial and temporal variations in snow accumulation. It also affects the Antarctic water vapor and radiation fields; hence it is desirable for earth system models such as the Goddard Earth Observing System (GEOS) system to have a blowing snow product. This paper presents the work on using a machine learning model to diagnose blowing snow properties with the Modern Era Retrospective analysis for Research and Applications v2 (MERRA-2) data. We adopt the random forest classifier for blowing snow identification and the random forest regressor for blowing snow optical depth and height diagnosis. Blowing snow observations from CALIPSO are used as the truth for training the machine learning model. Results show that with the MERRA-2 fields such as, snow age, surface elevation and pressure, temperature, specific humidity, and temperature gradient at the 2m level, and wind speed at the 10m level as input, promising results can be achieved. With this method, we can produce hourly blowing snow property diagnostics, which can serve an additional important resource for Antarctic surface mass balance studies.


Fri-04 Aug | 8:15 - 10:00 | MR329
AS14 - Subseasonal to Seasonal Forecasts and Applications

Session Chair(s): Thea TURKINGTON, Centre for Climate Research Singapore

AS14-A011 | Invited
The Impact of Intraseasonal Oscillation and Equatorial Waves on Rainfall Extremes in Indonesia

Donaldi PERMANA1#+, Jaka PASKI2, Danang Eko NURYANTO1, Nurdeka HIDAYANTO1, Erwin MAKMUR1, Supari SUPARI1, Supriyanto ROHADI1, Dwikorita KARNAWATI1
1Indonesian Agency for Meteorology, Climatology and Geophysics, 2Tohoku University

Intraseasonal Tropical Oscillation (ISO) is an atmospheric phenomena as a result of ocean-atmosphere interaction which has a periodicity of 20 to 100 days. The Madden-Julian Oscillation (MJO) is the dominant mode of intraseasonal variability of rainfall in Indonesia during boreal winter (November - April), but its signal is often obscured in individual station data, where effects are most directly felt at the local level. While, the Boreal Summer Intraseasonal Oscillation (BSISO) is the dominant mode of intraseasonal variability of summer rainfall (May - October) in Indonesia. BSISO has quasi-oscillating periods of 30-60-days (BSISO1) and biweekly (BSISO2) time scale with northward/northwestward propagation. It has been affecting monsoon onsets, active/break phases of monsoon and monsoon seasonal mean. The general impacts of MJO/BSISO on rainfall anomalies in Indonesia has been investigated using in-situ data from 86 stations during 1983 - 2012 (30 years) and remote sensing data using GPM IMERGV06 from 2001 - 2020 (20 years). Along with MJO, equatorial waves (Kelvin and Rossby) and their interactions have been triggering extreme rainfall and floods in Indonesia. Several case studies have been investigated to understand the interaction of equatorial waves with regional scale atmospheric drivers and its impact to rainfall extremes. For example, the 22 January 2019 floods in Southwest Sulawesi, the 1 January 2020 disastrous flooding which associated with record-breaking rainfall in Jakarta, and the 2017 extreme rainfall in Padang, Sumatra have been investigated. Recently, the role of tropical waves in the genesis of Tropical Cyclone Seroja in April 2021 was discussed. TC Seroja was one of the first tropical cyclones to significantly impact Indonesian land.


AS14-A002
Post-correcting of Multi-model Ensemble Sub-seasonal Forecast of Precipitation Based on Deep Learning

Uran CHUNG#+, Jinyoung RHEE, Soo-Jin SOHN
APEC Climate Center

This study was conducted to improve the prediction skills of precipitation amount and occurrence from the sub-seasonal (S2S) multi-model ensemble (MME), focusing on week 3-4 for the East Asian region, through deep learning based post-processing. To train the model for post-processing, S2S MME prediction data was first generated using the simple composite method, considering several climate models from the S2S database at once. Due to the heterogeneous S2S data of prediction frequency and lead time during hindcast period for the models considered, the MME calculation is based on the common prediction frequency once a week and lead time up to 30 days. ECMWF Reanalysis v5 (ERA5) was used as observations, which is the labeled data to train the deep learning model. To define the precipitation occurrence, the data exceeding 0.1 mm/hr was converted to 1, and otherwise 0. U-net architecture, the deep learning model most used in climate prediction, is adopted for the training, and the convolutional layer in U-net is wrapped by TimeDistributed to consider temporal continuity in this study. In order to evaluate the improvement effect of post-correction, the improvement ratio (e.g., skill score), for example, the amount of changes in evaluation index such as PCC of precipitation with and without the training model, was calculated by lead time (e.g., week 1 to 4). In result, the skill scores of MME precipitation were 0.1, 0.3, 0.4, and 0.2 at each lead time, and the skill score of MME precipitation occurrence showed -0.1, 0.2, 0.0, and -0.1 at each lead time. Although there was no improvement in MME precipitation occurrence, it was indicated that it was possible to improve the prediction of MME precipitation according to a deep learning based-post correcting since the skill score of target week 3-4 was higher than the before the training.


AS14-A009
Forecast of Subseasonal Indian Monsoon Precipitation Using Central Indian Ocean Mode and Machine Learning

Lei ZHOU1#+, Yanwei YU2, Bingqi YAN2, Jianhuang QIN3, Wei TAN4, Youmin TANG5,6, Xiaofeng LI7, Xiaojing LI8, Junyu DONG2, Raghu MURTUGUDDE9, Dake CHEN10
1Shanghai Jiao Tong University, 2Ocean University of China, 3Hohai University, 4Shandong University of Science and Technology, 5State Oceanic Administration, 6University of Northern British, 7Chinese Academy of Sciences, 8Second Institute of Oceanography, MNR, 9University of Maryland, 10Second Insititute of Oceanography

The monsoonal precipitation is dominated by intraseasonal variabilities, whose period is between 20-90 days. The skillful prediction lead time for subseasonal Indian monsoon rainfall is currently less than 5 days and remains a grand challenge. A central Indian Ocean (CIO) mode was established, and it was found to have a close dynamic relation with the intraseasonal rainfall during summer monsoon. Here we show that an intrinsic variability in the Indian Ocean, the CIO mode, when combined with a machine learning (ML) algorithm, can produce skillful predictions of precipitation over the monsoon region with a lead time of over 15 days, which is close to the theoretical predictability limit. This remarkable skill improvement stems from the fact that the CIO mode is dynamically related to the intraseasonal monsoon rainfall, while the data-driven ML algorithm suppresses unwanted high-frequency noises. Using the CIO mode and the ML algorithm, the forecast system hybridizes physical fundamentals and the versatility of data-driven algorithm. The identification of the CIO mode and the verification of its significant contribution to intraseasonal prediction advance our understanding of the coupled monsoon system and also demonstrate the great potential of ML techniques in weather forecast and climate prediction.


AS14-A017
Indian Ocean Dipole and its Impact on Southeast Asia: A Climate Service Perspective

Shipra JAIN#+, Thea TURKINGTON, Wee Leng TAN, Chen SCHWARTZ
Centre for Climate Research Singapore

Indian Ocean Dipole (IOD) is one of the key climate drivers influencing the interannual variability in climate over Southeast Asia. The recent 2019 IOD event, which was the strongest positive IOD (pIOD) event in the last 60 years at least, coincided with a severe drought in Indonesia and heavy rainfall in East Africa. Though there has been a growing interest from the climate community in the IOD for more than two decades, this event has attracted more interest, particularly from the users due to its widespread impact on the socio-economy. In this work, we present key results from the operational IOD climate watch system for the Southeast Asian region, which is currently under development. We started with a stock take exercise on existing IOD-related climate service products, including how the start and end time of the event are defined in real-time outlooks and historical observations, and the criterion for defining an IOD event in the historical record. We then used a suite of observations to examine the sensitivity of the Dipole Mode Index (DMI) – an indicator of the IOD – to the climatological base period, diagnostic variable (i.e., monthly mean or 3-month running mean), and SST observational dataset. We find that the DMI is most sensitive to the SST data and relatively less to the base period used and the diagnostic. We also find that the latest seasonal prediction models (available through C3S) are skillful for the DMI from June-December (the period when IOD is usually observed), and a combination of different observations and models show similar skill scores for this period. However, for the Northern Hemispheric winter and spring, the skill score becomes sensitive to the observations used, suggesting a potential role of observational uncertainty in the SST data for the apparent low DMI skill during winter/spring.


AS14-A024
Seasonal Climate and Crop Prediction for Agricultural Decision Support

Xinzhong LIANG#+, Chao SUN, Sanghoon SHIN
University of Maryland

Local water availability/quality and soil health/productivity are inextricably linked to climate variations and agricultural practices both regionally and in teleconnected areas. Effective farm and water planning must consider not only local crop yields and socioeconomic drivers, but also competing resource needs and multi-scale climate feedbacks, all of which impact regional water availability, quality, and usability. These concerns have created an urgent need for predictive earth system models that can support multiscale agricultural decisions while explicitly simulating interactions between the climate and agrohydrosystem. Such models need to be capable of forecasting the occurrence and agricultural impact of climate anomalies and extreme events such as heatwaves, droughts, and floods. We therefore develop a predictive regional earth system model-based decision support Dashboard for Agricultural Water use and Nutrient management (DAWN) to sustain food and energy crop production. Our goal is to create infrastructure that combines advanced science and innovative technology to provide credible, usable information for agricultural producers and water managers in order to improve land, water, and fertilizer use synergies across multiple systems and scales. This talk will present the development and application of the DAWN system, focusing on its current ability to predict seasonal climate variation, crop growth, water demand, and annual yield over the United States. Initial analysis shows that the DAWN system improves NOAA operational forecasts of U.S. seasonal climate anomalies and provide useful predictions of crop production and terrestrial hydrology conditions. We will elaborate the integration of regional climate-crop coupled downscaling, multi-physics or multi-models ensemble optimization, more realistic surface initialization, and machine learning to maximize probabilistic seasonal forecast skills. 


AS14-A026
Subseasonal to Seasonal (S2S) Forecast and Applications in Indonesia : Operational and Research Development

Nurdeka HIDAYANTO+, Robi MUHARSYAH, Donaldi PERMANA#, Kharisma APRILINA, Supari SUPARI, Ummu MA'RUFAH, Danang Eko NURYANTO, Amsari Mudzakir SETIAWAN, Adi RIPALDI, Novi FITRIANTI, Adyaksa RAHARJA, Dodo GUNAWAN, Ardhasena SOPAHELUWAKAN, Supriyanto ROHADI, Dwikorita KARNAWATI
Indonesian Agency for Meteorology, Climatology and Geophysics

Subseasonal to seasonal (S2S) predictions have been developing in Indonesia and have become an interesting discussion in recent years. This is because of particular concern about the increasing accuracy of the S2S prediction and its application. Since 2015, Indonesia Agency for Meteorology, Climatology, and Geophysics (BMKG) has been using the European Center for Medium Range Forecast (ECMWF) S2S model raw output for operational S2S prediction services, particularly rainfall forecast at 10-days time scale (decad). Regularly, BMKG produces rainfall predictions for 3 to 4 decads both in deterministic prediction (rainfall accumulation) and probabilistic prediction (probability of rainfall exceeding a certain threshold). These S2S products are used as input for early warning of extreme climates. Since 2020, after the availability of national observational rainfall gridded data at 5 km spatial resolution (land only), a Linear-Scaling bias correction was implemented to the ECMWF S2S model output. As a result, the S2S prediction skill has increased by 10-15%. In the research mode, the accuracy of S2S prediction can be improved by applying model output statistics (MOS) and state-of-the-art of machine learning. Recently, PyCPT and Xcast are used to resolve these problems in research mode. These tools are powerful in producing, analyzing, and visualizing the results from the combined dynamical model with model output statistic (MOS) and also machine learning models using a python-based approach. We conducted a case study of deterministic and probabilistic predictions of rainfall in the Indonesian domain using several methods in PyCPT and Xcast. The results show that there is a significant reduction in the mean error of the rainfall forecast. Furthermore, these tools can also enhance model performance. Therefore, PyCPT and Xcast have great potential to be applied as tools for enhancing S2S model performance.


Fri-04 Aug | 8:15 - 10:00 | MR331
AS17 - Application of Satellite Data to Weather, Climate and Environmental Study

Session Chair(s): Jun LI, National Satellite Meteorological Center, Kozo OKAMOTO, Japan Meteorological Agency

AS17-A001 | Invited
The Insights from Twenty Years of AIRS Radiances and an Outlook for the Incoming Decade: A Climate Perspective

Xianglei HUANG1#, Xiuhong CHEN1, Larrabee STROW2, Chongxing FAN1+, Norman LOEB3, Seiji KATO3, Qing YUE4
1University of Michigan, 2University of Maryland, Baltimore County, 3NASA Langley Research Center, 4California Institute of Technology

Atmospheric Infrared Sounder (AIRS) aboard the NASA Aqua satellite has been operating since September 2002. Its information content, superb instrument performance, and dense sampling pattern make the AIRS radiances an unprecedentedly invaluable data set for climate studies. We use two studies here to illustrate its merit in climate studies. First, the trends of global-mean, nadir-view, and clear-sky radiances from two decades of AIRS observations are studied, together with the counterparts of synthetic radiances based on two reanalyses, ECMWF ERA5 and NASA GEOS V5.4.1. The AIRS observation shows statistically significant negative trends in most of its CO2 channels, positive but non-significant trends in the channels over the window regions, and statistically significant positive trends in some of its H2O channels. The best agreements between observed and reanalysis radiance trends are seen over the CO2 tropospheric channels, while the trends over the CO2 stratospheric channels are opposite between the observations and reanalyses. ERA5 results largely agree with the AIRS observation over the H2O channels, but this is not the case for GEOS V5.4.1. Second, using ERA5 reanalysis data, other A-Train observations, and greenhouse gas measurements from NOAA, we derived the spectral radiative forcing due to greenhouse gas increases in the last 20 years, and short-term spectral radiative feedbacks of lapse rate, water vapor, and cloud over the same period. The combined spectral radiative forcings and radiative feedbacks agree well with the spectral flux trend derived from the AIRS L3 spectral OLR product. The most significant discrepancies happened in the far-IR region, a spectral region with no actual AIRS coverage (so its spectral flux has to be estimated using the mid-IR spectral flux directly inferred from AIRS radiance observations). The implications of two forthcoming far-IR missions, PREFIRE by NASA and FORUM by ESA, for resolving such far-IR discrepancies are then discussed.


AS17-A008
Monitoring of NOAA Satellite Land Surface Products and Their Anomalies

Peng YU1,2#+, Yunyue YU2, Jingjing PENG1,2, Yuling LIU1, Heshun WANG2, Zhangyan JIANG3, Corinne CARTER3, Lei JI1,2, Yuan ZHOU3
1University of Maryland, 2National Oceanic and Atmospheric Administration, 3National Oceanic and Atmospheric Administration STAR

The Land Product Development Team at NOAA STAR is responsible for the development, maintenance, and quality assurance of multiple land parameters from two satellite missions, the Joint Polar-orbiting Satellite System (JPSS) and the Geostationary Environmental Satellite R-Series (GOES-R). The involved land products are about essential radiation and vegetation parameters, which are the Land surface temperature (LST), the land surface albedo (LSA), the surface reflectance (SR), the land surface bidirectional reflectance factor (BRF), and the vegetation product suite, including the green vegetation fraction (GVF), the top-of-atmosphere (TOA) normalized difference vegetation index (NDVI), the top-of-canopy (TOC) NDVI, and the TOA enhanced vegetation index (EVI). To understand the product quality and ensure their successful production, a comprehensive monitoring system was developed for their visualization and their evaluation with measurements from in-situ observation sites and/or various other satellites as reference. The LST product was the first parameter being monitored and has accumulated the longest data record. The LST product performance summary, including retrieval anomaly detection, is routinely conducted and delivered to corresponding team members weekly for their review and further analysis. Moreover, the system is being gradually extended to other land parameters. This presentation will walk through the main functionality and logic flow of the system and brief the quality of these products. One highlight in the presentation is a newly developed analysis component, the monitoring of extreme weather events. It focuses on the LST anomaly and refers to the change of other related variables when needed. The analyses are released to the public as a series of routine monthly anomaly reports. Twenty monthly summaries have been accumulated along with multiple event-driven analyses. This presentation gives various examples, including their connection to certain climate patterns, e.g., ENSO.


AS17-A030
Time Series Analysis of Monthly Averaged Insolation Across Metro Cities of India

Srinivasa Ramanujam KANNAN#+
Indian Institute of Technology Bhubaneswar

Renewable energy sources are becoming more and more critical, as it neither contributes to the increasing level of greenhouse gases nor imposes. The surface solar short-wave radiation (SSSR) information is essential for solar energy systems. In the present study, a time-series analysis of monthly averaged insolation over major cities of India is carried out. The analysis is based on the remote sensed observation from geostationary platform in visible and infrared sensor from INSAT between 2014 and 2020. The daily averaged insolation data available from the mosdac server maintained by the Indian Space Research Organisation (ISRO) is converted to monthly averaged insolation data. Data pertinent to the major metro cities are interpolated from the monthly averaged data to generate the time series in monthly scale. Statistical and machine learning algorithms are proposed to be develop in order to predict the monthly averaged insolation with greater accuracy. Using the time series data, the dynamic aspect of insolation will also be characterized and cross compared across multiple sites to study the insolation behaviour.


AS17-A035
Surface Short-wave Radiation Estimation and Spatiotemporal Variation Analysis in China Based on the New Generation Geostationary Satellite

Gegen TANA1#+, Jian XU2, Chong SHI3, Jiancheng SHI2
1National Space Science Center, Chinese Academy of Sciences, 2Chinese Academy of Sciences, 3Aerospace Information Research Institute, Chinese Academy of Sciences

Downward Surface Shortwave Radiation (DSSR) concentrates most of the energy of solar radiation on the earth's surface, and its accurate estimation plays an important role in climate change research and surface solar energy estimation. The successful launch of a new generation of stationary meteorological Himawari-8 and FY-4 and the integration of remote sensing technology and machine learning methods have made the estimation of DSSR based on satellite remote sensing significantly improved in terms of spatial and temporal resolution and calculation accuracy. Based on the ground-based measurements and satellite observation data, this study establishes the surface solar short-wave radiation database, and uses the base station point data as the training data of random forest and deep learning. Combining the model optimal selection method, the DSSR fast estimation model is developed and applied to geostationary measurements in China. Taking advantage of the high frequency of the satellite measurements, the DSSR estimation results are visualized to analyze the seasonal and spatial distribution of DSSR in China, which can compensate for the shortcomings of ground station monitoring on the spatial scale.


AS17-A029
Construction of Rooftop Albedo Database from Open Satellite Images: Application of Super Resolution Algorithm

Makoto NAKAYOSHI1#+, Kosho IDO1, Shiho ONOMURA1, Yuya TAKANE2, Benjamin CRAWFORD3, Ryo KANEKO4, Yuta WATANABE1, Masuo NAKANO5
1Tokyo University of Science, 2National Institute of Advanced Industrial Science and Technology, 3University of Colorado Denver, 4The University of Tokyo, 5Japan Agency for Marine-Earth Science and Technology

Severe summer heat is becoming problematic in many cities; the incidence of heat stroke steadily is increasing, and electricity demand is also souring due to the use of air conditioning. Cool Roof Strategy, which increases the reflectivity of rooftops, is considered a promising technique for urban heat mitigation. Previous studies simulated the effect of Cool Roof installation with mesoscale meteorological models and reported that the reduction of the near-surface air temperature (Ta) reached to 0.5 to 2 K. On the other hand, the lack of city-scale actual rooftop albedo data may undermine their findings. We developed a methodology to construct the city-to-country scale rooftop albedo database with a deep learning technique; applying a super-resolution algorithm to surface albedo images computed with non-commercial satellite images, or Sentinel-2 with 10 m spatial resolution yields 8 times upscaled images of 1.25 m spatial resolution, then averaging them by every building for rooftop albedos. The training was done with surface albedo images identified with commercial satellite data, or worldview3 data with 1.25 spatial resolution. Our method successfully reproduced rooftop albedos better than ordinary image interpolation methods, such as bicubic and nearest neighbor. Sentinel-2 images taken at different date and time resulted in different albedo images and that difference showed the clear dependence on solar altitude. The simple regression formula between surface albedo and solar altitude resolved solar altitude dependency on surface albedo calculation. With the proposed method and the regression formula, the rooftop albedo database over Japan for meso-scale simulations was constructed with 1 km spatial resolution.


AS17-A036
Rainfall Intercomparison of Grid Satellite Rainfall Products and Gauge Station Dataset Over Complex Terrain in Bali Province, Indonesia

Putu ARYASTANA1#+, Chian-Yi LIU2
1Warmadewa University, 2Academia Sinica

Rain gauge measurements have limitations in spatial coverage for remote areas and high terrain. Recently, remote sensing platforms are capable to present global grid satellite rainfall products at high spatial and temporal resolution. Reliable validation of rainfall data is key for justifying the ability of grid satellite rainfall products so that they are feasibly used in various applications. The main contribution of this study is the intercomparison of the abilities of three grid satellite rainfall products (GSMaP: Global Satellite Mapping of Precipitation, IMERG: Integrated Multi-satellitE Retrievals for Global Precipitation Measurement, CHIRPS: Climate Hazards Group Infrared Precipitations with Stations) concerning gauge station dataset at different time scales (hourly, daily, penta-day, decadal, monthly, and seasonal), elevations, and rainfall intensities. The continuous and volumetric quantitative statistical index methods were performed to compare the ability of each grid satellite rainfall product by using a grid-point-based approach. The intercomparison results exhibited that the IMERG dataset reaches the best abilities on hourly, daily, penta-day, and seasonal scales, while CHIRPS has better performance on the monthly scale compared to other datasets. In addition, IMERG performed better in different elevations. All grid satellite rainfall products are inclined to overestimate the moderate rainfall events but underestimate both the light and heavy rainfall events. The result of the present study suggests that indeed adjustments in the rainfall estimate algorithm are needed when investigating complex terrain on the small island.


Fri-04 Aug | 8:15 - 10:00 | MR332
AS07 - General Session for Atmospheric Sciences

Session Chair(s): Joong-Bae AHN, Pusan National University

AS07-A043
Enhanced Impact of Vegetation on Evapotranspiration in the Northern Drought-prone Belt of China

Jian ZENG#+
Chengdu University of Information Technology

Evapotranspiration (ET) is an essential component of the land–atmosphere water cycle. In this work, the trend of ET and its dominant factors during 1982 to 2011 are investigated in the northern drought-prone belt of China (NDPB) based on five datasets, including the gridded FLUXNET, using the Pearson correlation and linear regression methods. Specially, we focus on the increasing contribution of vegetation in the change of ET. During 1982–2011, summer ET significantly increased at the rate of 0.33 mm/year (p < 0.05) in the NDPB. However, similar to global-mean ET, the ET in NDPB also experienced a pronounced fluctuation during 1999 and 2002. The role of water supply differed remarkably before and after the fluctuation while the atmospheric demand maintained weak constraint on ET. Before the fluctuation (during 1982–2000), ET correlated significantly (p < 0.01) and positively with soil moisture, indicating ET was primarily limited by water supply. However, their correlation weakened remarkably after the fluctuation when soil moisture decreased to the lowest level for the past thirty years, indicating that neither moisture supply nor atmospheric demand dominated the ET during this period. In contrast, vegetation leaf area index (LAI) maintained consistent significant (p < 0.01) and positive correlation with ET before and after the fluctuation in the NDPB, and it reflected over 60% of the change in ET. Moreover, the LAI in NDPB increased by 19.6% which was more than double of the global-mean increase. The ET increase due to rising LAI offset the ET decrease due to reduction of soil moisture, and vegetation became the primary constraint on ET during 2001–2011. The expansion of vegetation may intensify the risk of drought and cause conflicting demands for water between the ecosystem and humans in the NDPB, especially in the case of weak summer monsoon.


AS07-A044
Impacts of Floods on Indoor and Outdoor Air Quality: A Comparative Analysis Between the Flooded and Non-flooded Residential Houses

Akila MUTHALAGU1#+, Yang LIAN2, Rekha RAVINDRAN3, Asif QURESHI1
1Indian Institute of Technology Hyderabad, 2Indian Institute of Tropical Meteorology, 3State Health Systems Resource Centre

Floods are common in India. The frequency of disease outbreaks followed by floods has been steadily increasing. We found indoor and outdoor air of flood-affected houses had a significantly higher concentration of microbes than the non-flooded (control) houses. Microbial concentration was significantly three times higher in flooded houses than in the control houses. Bacterial genera Pantoea, Acinetobacter, fungal genera Aspergillus, and Penicillium were found dominant in the indoor air of flooded houses. Concentrations of many pathogenic bacteria were found higher in the indoor air of flooded houses. Results suggested that indoor air microbial burden was significantly and positively associated with outdoor air and outdoor soil, highlighting the potential importance of flooded soil and outdoor air as sources of microbes to indoor air. Here, we show a case of the prevalence of antibiotic-resistant bacteria (ARB) in indoor air of flooded houses and their corresponding sources. Bacteria were resistant to common antibiotics such as penicillin and ciprofloxacin. Our results indicate remediation after the floods does not improve indoor and outdoor air quality, posing various health risks to the inhabitants.


AS07-A011
Offshore Wind Resource Assessment by Characterizing Weather Regimes Based on Self-organizing Map

Shangshang YANG1, Huiling YUAN1#+, Li DONG2
1Nanjing University, 2Southern University of Science and Technology

As offshore wind power is continuously integrated into the electric power systems in China, it is critical to understand its variability. Weather regimes (WRs) can provide meteorological explanations for fluctuations in wind power. Instead of relying on traditional large-scale circulation WRs, this study focuses on assessing the dependency of wind resources on WRs in the tailored region clustered based on the finer spatial scale. For this purpose, we have clustered atmospheric circulations over the South China Sea (SCS) using self-organizing map algorithm (SOM) and characterized wind resources for the classified WRs. Results show that WRs at mesoscale can effectively capture weather systems driving wind power production variability, especially on multi-day timescale. Capacity factor reconstruction during four seasons illustrates that WRs highly influence most areas in winter and southern part of SCS in summer, and WRs can serve as a critical source of predicting the potential of wind resources. In addition, we further qualify the wind power intermittency and complementarity under different WRs, which have not been assessed associated with WRs. During WRs with changeable atmosphere conditions, the high complementarity over coastal areas can reduce the impact of intermittency on wind power generation. The proposed approach is able to be implemented in any region and may benefit wind resource evaluation and characterization.


AS07-A015
Wind and Stability in the Lower Troposphere Revealed in High-resolution Radiosonde Data in South Korea

Ye-Seul LEE#, Hye-Yeong CHUN+
Yonsei University

Using 1-second high resolution operational radiosonde data observed at 5 stations in South Korea for 4 years (July 2016-June 2020), seasonal and spatial variations of wind and stability in the lower troposphere below 1500 m are investigated, analyzing four variables: horizontal wind speed (HWS), vertical wind shear (VWS), squared Brunt-Väisälä frequency (N2), and Richardson number (Ri). Remarkable seasonal variations are identified in those variables, affected by geographical locations. VWS is high in spring and summer at two island stations on the west of Korean Peninsula, Bangnyengdo and Heuksando, while that is in winter at National Typhoon Center, N. Gangneung and Pohang. Below z=1000 m, static stability is lower in winter than in summer at all stations, which is associated with the inflow of marine boundary layer. This difference is likely influenced by local topography (coastal region and inland), which is consistent with the results at 5 stations in USA. The microstructures of the lower tropospheric instabilities revealed in the current radiosonde observations are found not to be properly represented from the high resolution local numerical weather prediction and analysis system, named Local Data Assimilation and Prediction System (LDAPS) of Korean Meteorological Administration (KMA). The synoptic patterns favorable for the convective instability (Ri<0) and Kelvin-Helmholtz instability (KHI) (0<Ri<1/4) cases are found based on a Self-Organizing Map (SOM) clustering algorithm: (1) west-high and east-low patterns with extended Siberian high in winter, (2) strong low-pressure systems susceptible for KHI from spring to fall, (3) weak high-pressure systems with potential convective instability. For all synoptic pattern, northerly or north-westerly flows are dominant with cold advection at 925 hPa.


Fri-04 Aug | 10:20 - 12:20 | MR311
AS08 - Atmospheric Light Scattering and Remote Sensing

Session Chair(s): Meng GAO, SSAI, NASA GSFC

AS08-A001 | Invited
Remote Sensing of Atmospheric Winds, Boundary Layer Heights, and Snow Depth

Xubin ZENG#+
The University of Arizona

Three-dimensional (3D) atmospheric winds, atmospheric boundary layer (ABL) heights, and snow depth are all outstanding science and technology issues. For instance, 3D winds and snow depth (and snow water equivalent) are two of the seven observables for the NASA Earth Science Explorer competition (with a cost cap of $310M), while ABL (including its height) is one of the two observables for incubation studies in the next few years. In this invited presentation, I will overview our recent efforts on these topics, including: (1) Retrieval, for the first time, of global 3D atmospheric winds from 60N to 60S by tracking water vapor from the hyper-spectral Cross-track Infrared Sounder (CrIS) aboard two polar-orbiting satellites (NOAA-20 and Suomi-NPP) that have overlapped tracks separated by 50 minutes (Ouyed et al. 2023). (2) Evaluation and retrieval of marine ABL heights using the airborne HSRL-2 lidar during the NASA Earth Venture Suborbital Mission (ACTIVATE) (Xu et al. 2023; Ouyed et al. 2023; Cutler et al. 2023) and ABL height over land using Global Positioning System radio occultation (Wang et al. 2022).(3) Evaluation of snow depth retrieval from ICESat-2 (Hu et al. 2022; Lu et al. 2022) using a variety of surface-based and satellite data (Mitchell et al. 2023).


AS08-A009
Partially Melting Droplets Strongly Enhance Lidar Backscatter

Wenbo SUN1#+, Yongxiang HU2
1Science Systems and Applications, Inc., 2NASA Langley Research Center

There has been a long-standing problem in discrepancy between theoretical and observed backscatter by water clouds. Lidar ratios from water clouds are often much lower than what calculated out by Mie theory. In this study, we find the low lidar ratios of water clouds in CALIPSO lidar observations can be explained if we assume some large droplets with liquid spherical shells and ice cores. Using a light scattering model for layered spherical particles, we can produce lidar ratios similar to those from the CALIPSO data while assuming large droplets with ice cores in clouds. This study explains the reason of low lidar ratios for water clouds and provides a method for remotely sensing partially melting droplets.


AS08-A018
Approximating the Backscatter Efficiency Factor of Preferentially Oriented Snow Particles

Kwo-Sen KUO1,2#+, Ines FENNI3, Robert SCHROM4, William OLSON4, Ian ADAMS4
1University of Maryland-College Park, 2Bayesics, LLC, 3NASA Jet Propulsion Laboratory, 4NASA Goddard Space Flight Center

We have evaluated the approximations of orientation-averaged efficiency factors (scattering, extinction, and backscatter) of realistic solid hydrometeors, assuming they are uniformly randomly oriented in space, using different quadrature schemes, i.e., Lebedev (lb), spherical design (sd), and adaptive quadrature (aq) and have shown that much fewer quadrature orientations (those aligned with the quadrature node directions) are needed with lb and sd than aq to achieve a similar level of precision (Fenni et al 2021). We have then tried to approximate the efficiency factors at non-quadrature orientations through interpolation using the ones obtained at the quadrature orientations. We found that, while the interpolation is generally accurate for scattering and extinction efficiency factors, it leads to large and unacceptable uncertainties for backscatter. We later realize that, since the hydrometeors in an ensemble illuminated by the radar beam are never oriented in the same direction, the quantity we must approximate well for remote sensing purposes is not the backscatter efficiency factor at a specific orientation but that with some underlying orientation distribution. The aforementioned orientation averages that we are able to approximate well using quadrature orientations assume a uniform orientation distribution, which radiometer polarization signals have shown to be unrealistic as well. We thus, in this presentation, examine and report the effectiveness of approximating the efficiency factors resulting from preferentially random orientation distribution using those calculated at the quadrature orientations.
Fenni, I., K.-S. Kuo, M. S. Haynes, Z. S. Haddad, and H. Roussel, 2021: Evaluation of Higher-Order Quadrature Schemes in Improving Computational Efficiency for Orientation-Averaged Single-Scattering Properties of Nonspherical Ice Particles. Journal of Geophysical Research: Atmospheres, 126, e2020JD034172, https://doi.org/10/gj3jr8.


AS08-A015
Improved Aerosol Characterization Using Spectral Sorting and Machine Learning

Vijay NATRAJ1#+, Sihe CHEN2, Yuk YUNG2
1Jet Propulsion Laboratory, California Institute of Technology, 2California Institute of Technology

Atmospheric aerosols represent a significant part of the anthropogenic forcing responsible for climate change. However, uncertainties in the origin and composition of aerosol particles, their size distribution, concentration, spatial and temporal variability, make it difficult to model their radiative effects. In order to quantify the influence of aerosols on Earth’s climate and to better validate climate models, information about their global abundance, properties and height distribution are needed. It is well known that spectrally resolved measurements of gaseous absorption contain information about the vertical distribution of scattering. We utilize O2 A-band measurements made by the Orbiting Carbon Observatory-2 (OCO-2), in conjunction with spectral sorting and machine learning approaches, to retrieve aerosol optical depth and layer height. We show results for the Saudi Arabian desert and the Sahel region in Africa. The retrievals compare well with collocated lidar measurements. This approach also has the potential to reduce biases in greenhouse gas retrievals. © 2023 California Institute of Technology. US Government sponsorship acknowledged.


AS08-A019
Aerosol Scattering and Composition at an Urban Site in Melbourne, Australia

Robyn SCHOFIELD1,2#+
1The University of Melbourne, 2The Centre of Excellence for Climate Extremes

Since August 2022 a Spartan network (a global particulate matter network) observational site has been established in Melbourne, Australia - on the roof within the urban centre. A comparison of nephelometer scattering properties, composition as well as miniMPL back-scatter aerosol profiles is presented. Melbourne, on the coast enjoys clean Southern Ocean air, but also hot central Australian air with alternating regularity. With some of the worst fuel standards for petrol in the OECD and minimal controls on domestic wood burning, the Australian urban environment is complex and relies heavily on sufficient ventilation to disperse pollution. Along with controlled biomass burning to reduce fuel loads, aiming to avoid extreme fire events, the city's air pollution is often compromised, and citizens have some of the highest asthma rates in the world. Here we present observations aiming to ground truth satellite observations of particulate matter, in order to utilize satellites to improve air pollution predictions for the region.


Fri-04 Aug | 10:20 - 12:20 | MR323
AS37 - Monitoring, Analysis, and Prediction of Typhoon and Climate Affecting Taiwan and the Philippines

Session Chair(s): Chung-Hsiung SUI, National Taiwan University

AS37-A019 | Invited
Mesoscale Analysis of Typhoons Near Landfall

Ben Jong-Dao JOU1#+, Chi-June JUNG1, Yucheng KAO2
1National Taiwan University, 2Central Weather Bureau, Taiwan

Mesoscale analysis of typhoons near landfall observed by mesonet weather stations and radar network in Taiwan is presented. Single radar analysis algorithm developed to retrieve primary and secondary circulations of typhoons near landfall is briefly reviewed (Jou et al. 2008; Lee et al. 1999). Orographic effects on landfalling typhoon intensity and precipitation changes are especially emphasized. Studies include the effect of coastal barrier jet (CBJ) on the intensity and track changes of landfalling typhoons (Haitang 0505); bulk microphysical properties of near-center secondary rainbands of landfalling typhoon (Soudelor 1513). Leeside meso-low and localized strong winds of typhoon near landfall is also investigated (Meranti 1614). The results are important for emergency response when typhoons are approaching land. Reference: Jou, B. J.-D., W.-C. Lee, S.-P. Liu, and Y.-C. Kao, 2008a: Generalized VTD retrieved of atmospheric vortex kinematic structure. Part I: Formulation and error analysis. Mon. Wea. Rev., 128, 1925-1936. Lee, W.-C., B. J.-D. Jou, P.-L. Chang, and S.-M. Deng, 1999: Tropical cyclone kinematic structure retrieved from single-Doppler radar observations. Part I: Interpretation of Doppler velocity patterns and the GBVTD technique. Mon. Wea. Rev., 127, 2419-2439.


AS37-A016
The Recent Development of Yhe Official Storm Surge Forecast System in Taiwan

Tso-Ren WU1#+, Jun-Wei LIN1, Chuen-Teyr TERNG2
1National Central University, 2Central Weather Bureau

During the typhoon warning period, in order to quickly and accurately warn the potential damage caused by the storm surge, the Taiwan government and related units have been actively developing the technology of the storm surge forecasting system. This research develops COMCOT-SS, the multi-scale storm surge forecasting system in Taiwan's coastal waters, based on the nonlinear multi-grid tsunami model COMCOT (Cornel Multi-grid Coupled Tsunami Model). COMCOT-SS uses nonlinear shallow water wave equations with dynamic nested grids to analyze the transmission of long waves at different scales, uses the moving boundary scheme to calculate the overflow area, and uses Open-Multi-Processing (OpenMP) for multi-execution parallel thread modification to meet forecast timeliness. The model can take advantage of the large computational domain to cover the full cycle of storm surge propagation, while also incorporating coastal inundation simulation. In addition to importing the ideal TC model, the model can be coupled with the 2D meteorological field to reflect changes in the typhoon structure and the TPXO model to describe the astronomical tide components. However, the forecast is directly affected by uncertain factors such as typhoon intensity and track, and the forecast results may differ significantly from the actual observations. To account for the uncertainties in the metrological conditions, the Central Weather Bureau constructs the ensemble forecast system based on the existing storm surge model kernel. The ensemble forecast system provides flexible options for generating ensemble members, such as track, intensity, and ideal wind field structure, and provides related probability forecast products with detailed and accurate storm surge forecast information for people in coastal areas to achieve the purpose of disaster preparedness and prevention, and reduce the loss of life and property.


AS37-A008
An Observational Study on Rapid Intensification of Typhoon Chanthu (2021) Near Taiwan

Wei-Ting FANG1+, Pao-Liang CHANG2#, Ming-Jen YANG3
1Central Weather Administration, 2Central Weather Bureau, 3National Taiwan University

As Typhoon Chanthu (2021) moved along the eastern coast of Taiwan, a noticeable intensification with the eyewall convection asymmetry highly dominated by wavenumber-1 features was observed by the dense radar network in Taiwan. In this study, the data from multiple radars were integrated to analyze the evolution of the inner-core structure and kinematic features. The radar-retrieved maximum wind speed at an altitude of 3 km rapidly increased by ~18 m s-1 within 11 hours in the intensifying stages and significantly decreased by ~19 m s-1 in 8 hours in the weakening stage, which are features of rapid intensification (RI) and rapid weakening (RW), respectively. Namely, Chanthu experienced both RI and RW within the 24-h analyzed period, which was challenging for intensity forecasts. During Chanthu’s intensifying stages, the maximum region of eyewall convection asymmetry suddenly rotated from the eastern to the northern semicircle cyclonically immediately after a terrain-induced boundary inflow from south of the typhoon was initiated. This sudden rotation of eyewall asymmetry showed a better consistency with the radar-derived vertical wind shear (VWS) than that from global reanalysis data. Collocated with surface observations, it is found that the intensification was associated with 1) terrain blocking-induced boundary inflow south of the typhoon, 2) upshear-left pointing low-level flow, and 3) weak upper-level VWS.


AS37-A015
Analyzing Tropical Cyclone Wind Structure by Satellite Imagery Utilizing Convolutional Neural Networks

Chun-Min HSIAO1#+, Buo-Fu CHEN2, Yung-Lan LIN1, Kuan-Liang LAI1, Treng-Shi HUANG1, Guo-Chen LU1
1Central Weather Bureau, 2National Taiwan University

Tropical cyclone (TC) structure analysis is crucial for TC research and disaster prevention. However, observational limitations can make it difficult to accurately analyze TC structure. To address this issue, we developed a deep learning model using the convolutional neural network (CNN). This model uses satellite observations to estimate TC structure and provides objective, globally consistent results. Our model is expected to improve the temporal and spatial resolution of typhoon structure observations, making it a valuable tool for TC research and disaster prevention. To train the CNN, labeling data is required to compute the loss function during the training process. In this study, the structural parameters of the best track data and a physically-based parametric wind model were used to estimate the axisymmetric wind speed structure of TCs. However, the wind profiles are not accurate enough, so we used ERA5 reanalysis data to correct the maximum wind and the wind speed at the outer radii. The model was trained on data from 2004 to 2016 and showed good performance. The intensity RMSE and 9.9 kt and the storm wind radius MAE of 43.6 km. Independent verification of the 2017-2018 TCs using ASCAT and SAR sea surface wind observations showed the model's ability to reasonably estimate TC structure. Using the objective method of this study, we can convert the one-dimensional axisymmetric wind profile into a two-dimensional wind field and compare it with actual observations. The results showed that the method could generally estimate the asymmetric wind speed structure of TCs. In addition, this new technology is integrated into CWB TAFIS (Typhoon Analysis and Forecast Integration System), providing intensity and asymmetric storm radius for 4 quadrants.


AS37-A010
Adopting Predicted Typhoon Inner Core Winds for WRF FDDA to Improve Typhoon Initial Structure of TWRF

Hua HSU1#+, Der-Song CHEN2, Jia-Hong XIE2, Chun-Teng CHENG2, Ling-Feng HSIAO2, Pao-Liang CHANG2, Jing-Shan HONG2
1International Integrated Systems, Inc. (IISI), 2Central Weather Bureau

Typhoon WRF (TWRF) model based on the Advanced Research Weather Research and Forecasting Model (WRF-ARW) is the operational tropical cyclone (TC) prediction system at the Central Weather Bureau (CWB). The forecast performances of track and intensity in 2016~2021 were found competitive with that of two leading global models, EC and NCEP. But there is not yet using TC initialization process in TWRF, which has the potential to improve TC intensity forecast significantly. Therefore, this study focuses on further improving the initial TC intensity and position of TWRF. Reasonable initial TC structure could not only reduce model spin-up time, but also improve the performance of TC forecast. This study adopted FDDA in TWRF model to assimilate the forecast TC structure. We assimilated hourly forecast winds into FDDA as objective analyses and apply it to TWRF with partial cycle assimilation. We choose 9 TCs in western North Pacific to evaluate the improvement of TC initial intensity and position in TWRF with FDDA initialization process. All cases show better results of TC initial positions, and most of cases shows better results of TC initial intensity. We discussed more in forecast results of Typhoon Chanthu (2020). Typhoon Chanthu was closed to Taiwan during 9/11 00~9/12 00 UTC when radar system in Taiwan could provide observation wind compared to forecast wind we used in FDDA. The results pointed out that adopt FDDA with the forecast TC inner core winds or observation wind not only improved the representativeness of the initial TC location and intensity, but also advanced the prediction on the typhoon track and intensity of TWRF. The improvements were comparable with the result of nudging observation wind.


AS37-A009
Impact of Combination of Inflation Schemes in an Operational Local Ensemble Transform Kalman Filter (LETKF)

Chin-Cheng TSAI1#+, Craig SCHWARTZ2, Guo-Yuan LIEN1, Siou-Ying JIANG1,3, Pao-Liang CHANG1, Jing-Shan HONG1, Chun-Chieh WU3
1Central Weather Bureau, 2National Center for Atmospheric Research, 3National Taiwan University

Covariance inflation schemes are often implemented in ensemble-based data assimilation systems to mitigate underestimation of forecast errors due to small ensemble sizes. Insufficient ensemble spread was noted in the operational hourly-cycling, 2-km, 32-member Local Ensemble Transform Kalman Filter (LETKF) system at Taiwan’s Central Weather Bureau (CWB), which degraded forecast quality of convective-scale weather systems. To enhance the ensemble spread during LETKF forecast-analysis cycles, two kinds of covariance inflation schemes are evaluated in this study, including relaxation-to-prior spread (RTPS) (Whitaker and Hamill, 2012) and random additive noise (Dowell and Wicker, 2009; Caya et al. 2005). Their impacts are evaluated with an afternoon thunderstorm case in 2018 and a Meiyu front case in June 2022 over Taiwan. When incorporating both covariance inflation schemes into LETKF cycles, the prior spread-error relationship was improved relative to a control LETKF where neither RTPS nor additive inflation was applied. The spread-error relation was improved after about 10 hourly forecast-analysis cycles for the afternoon thunderstorm case but was enhanced within the first 2 hourly data assimilation cycles in the Meiyu front case. As measured by the fractions skill score (FSS), deterministic quantitative precipitation forecasts (QPFs) initialized from LETKF mean analyses were improved in both the afternoon thunderstorm and Meiyu cases when applying both covariance inflation schemes. In addition, verification against surface observations indicated that humidity, temperature, and wind speed were improved in the Meiyu case but only humidity in the first 3 forecast hours was improved in the afternoon thunderstorm case. Nonetheless, overall, the combination of RTPS and random additive noise in an hourly updated convective-scale LETKF data assimilation system can provide suitable ensemble spread to represent model forecast error and improve short range QPF performance. More studies about the proposed inflation schemes in a typhoon event will be demonstrated in the presentation.


AS37-A011
Investigate the Sensitivity of Updating Sea Surface Temperatures on TWRF Typhoon Predictions Over the Western North Pacific

Der-Song CHEN1#+, Ling-Feng HSIAO1, Kang-Ning HUANG1, Chun-Teng CHENG1, Hua HSU2, Jing-Shan HONG1, Chin-Tzu FONG1
1Central Weather Bureau, 2International Integrated Systems, Inc. (IISI)

The ocean plays a major role in modulating the TC intensity changes. It is well known that strong winds of a TC can induce significant upwelling in the ocean, bring down the SST and affect TC intensity for slow-moving storms. Without coupling ocean model, the TC intensity prediction skill of atmospheric-only models suffers from this shortcoming. However, for computational limitation, most operational TC models are uncoupled. The TC model, TWRF of Central Weather Bureau uses the forecast fields from the NCEPFV3 for the boundary conditions. Due to the lack of ocean-coupling, TWRF suffers over-prediction of TC intensity when storm move slowly. A new strategy is designed for this remedy using the predicted SST from ECMWF coupled IFS instead of a fixed SST from NCEPFV3.
Typhoon In-Fa is selected for its over-intensified prediction and slow speed. In the operation run where the SST is fixed, the over forecast intensity error is 35 hPa in the 3km domain at 120h. When the SST is updated with ECMWF IFS, the intensity errors are improved by 20 hPa. Meanwhile, the track error has increased slightly in the 3km domain. We speculate the that the slight degradation is by the inconsistent between the bottom boundary condition from the ECMWF and the lateral boundary condition from NCEP. We tested a combination strategy using NCEP and EC as the boundary conditions for TWRF. The hybrid strategy, mixing the EC and NCEP forecast fields as the lateral boundary condition and ECMWF SST as the bottom boundary condition, performs the best in In-Fa. The hybrid strategy consistently beats the operation version of TWRF on the intensity prediction with 85 cases/8 typhoons. This hybrid method with updating SST posts as a workable strategy for uncoupled models to account for the feedback from the ocean in a computationally efficient way.


Fri-04 Aug | 10:20 - 12:20 | MR327
AS51 - Understanding and Predicting Precipitation Extremes Through Integrative Analyses of Observation, Numerical Models, and Deep Learning

Session Chair(s): Jingyu WANG, Nanyang Technological University, Yixin WEN, University of Florida

AS51-A009
Effects of Upshear Lifted Convection on Vortex Alignment of Super Typhoon Rammasun (2014) Under Sheared Environment

Yecheng FENG+, Liguang WU#
Fudan University

A vertically-aligned circulation of tropical cyclones (TCs) is widely acknowledged as a key structure to drive rapid intensification (RI). Currently, no agreement has been reached on the mechanisms for maintaining alignment although several pathways have been proposed. In this study, a high-resolution simulation of Rammasun (2014), a moderately sheared super typhoon that underwent offshore RI, is utilized to investigate key physical processes on vortex tilt reduction, with a focus on the vortex motion at different vertical layers. Based on the potential vorticity tendency (PVT) diagnosis, it is found that the vortex alignment cannot be simply attributed to the steering flow hypothesized by some previous pathways, while the diabatic heating process plays a dominated role in reducing vortex tilt. The contribution of diabatic heating is closely related to the upper-level lifted convection at the upshear quadrant, which acts to shift the upper-level vortex centers toward the low-level centers through generating the positive PV tendency. The convergence of low-entropy air from upper-level environmental ventilation flow and high-entropy air from inner-core is conducive to instability in the upper-level of upshear quadrant, leading to the earlier occurrence of convection at upper-levels than the lower-levels before RI onset. This study suggests that TCs can maintain vortex alignment through diabatic modulation by shear-induced convective asymmetry.


AS51-A007 | Invited
Evolution of Precipitation Triple Oxygen Isotopes During Monsoon Cold Surges in Singapore: Implications for Evaluating Tropical Convection

Yilin ZHANG#+, Shaoneng HE, Bernie WEE, Xianfeng WANG
Nanyang Technological University

Precipitation stable isotopes (δ18O, δ2H and d-excess) have been successfully used to investigate microphysical processes during tropical convection. Recently, 17O-excess has been developed as a new tracer of hydrological processes. However, it has not yet been used to understand rain event microphysics. In combination with other parameters, 17O-excess may provide more insights into tropical convection. In this study, we collected precipitation samples at minute interval from multiple cold surge events during the Northeast monsoon season in Singapore in 2017 and 2022. Their triple oxygen isotopes were analyzed to study how tropical mesoscale convective systems affect precipitation isotopes. 𝛿18O was found to decrease in the convective zones and then gradually increase in the stratiform zones, while d-excess exhibited inverse trends. This reveals that raindrop re-evaporation is important in shaping precipitation isotopes. For rain events with more vigorous convection and higher integrated rainout amount, the relative humidity estimated from precipitation 17O-excess was lower than that in the moisture source area. The moisture recycling from reevaporated vapor may increase 17O-excess during transport. This is further exemplified by those events with higher integrated rainout generally having a lower 𝛿18O but a higher 17O-excess. Additionally, d-excess and 17O-excess are mostly positively correlated, inconsistent with their negative correlation observed in monthly precipitation. This implies that stronger regional convection may attenuate the positive correlation between d-excess and 17O-excess, even switching to a negative correlation for the cumulative monthly signal. Tropical convection has largely modified 17O-excess in precipitation; thus, 17O-excess does not purely record the moisture source humidity. Understanding the various control mechanisms of precipitation isotopes at different timescales will help interpret paleoclimate records and improve the parameterization of climate models.


AS51-A001
Robust Expansion of Extreme Midlatitude Storms Under Global Warming

Ji NIE1#+, Panxi DAI2
1Peking University, 2Zhejiang University

Extreme extratropical storms are among the most impact-relevant weather events in the midlatitudes. Under global warming, extreme storms are expected to intensify; however, little is known about the response of their spatial structure. Here, we show that with warming, extreme storms not only become stronger, but also grow larger. By employing multi-model projections from the sixth Coupled Model Intercomparison Project and an idealized aquaplanet simulation, we demonstrate that global warming leads to a robust increase in extreme storm size that is relatively spatially uniform in the midlatitudes and consistent among the models. The physical mechanism for the size increase is the increase in the Rossby deformation radius due to the increase in low-level dry static stability with warming. The storm expansion adds a substantial contribution (2.6%/K), along with the increase in precipitation intensity (3.2%/K), to the increase in storm total precipitation. The results improve our understanding and have significant implications for climate mitigation.


AS51-A013 | Invited
The Tibetan Plateau Bridge: Influence of Tropic Convection on Extreme Precipitation Events in Eastern Asia

Yimin LIU#+, Jilan JIANG, Tingting MA, Guoxiong WU
Chinese Academy of Sciences

The special geographical location of the TP makes it plays a unique role in the Asian summer precipitation, particularly in extreme precipitation. This talk will present recent studies on the bridge roles of the Tibetan Plateau (TP) in the link of tropic convections anomalies and extreme precipitation events in eastern Asia in intraseasonal and interannual time scales. Excessive precipitation was observed throughout the Yangtze River Valley during the record-breaking Meiyu season in 2020. The persistent Indian Ocean warming in 2020 is responsible for the record-breaking Meiyu rainfall over eastern China. But there is no significant correction between this SSTA and the extreme precipitation over the upper reaches of Yangtze River. Our results show that the activities of high potentia­l vorticity (PV) systems during their eastward propagation over the eastern TP should be responsible for the above-normal rainfall in the intraseasonal time scale. The activity of high-PV systems is characterized by a prominent diurnal cycle, and their formation is closely related to the thermal contrast between the near-surface and lower atmosphere. Compared with the climatology, an excessive water vapor supply from the anomalous anticyclone over the northern Bay of Bengal, forced by the strengthened convection over western Indian Ocean and increased surface sensible heating over the Bay of Bengal, contributes to a stronger thermal contrast and enhances activity of high-PV systems over the TP. In late summer in 2019, TP bridge influence exists in the connection from the suppressed convection over the Maritime Continent to the heavy drought over Southeast China through enhancing northly winds and providing a stable circulation patter in eastern Asia and western Pacific. Such TP bridge influence has been identified and verified in the interannual time scale by the partial correlation analysis and AGCM sensitivity experiments with and without the TP.


AS51-A014 | Invited
Impacts of the Topographical Factors on Hourly Extreme Precipitation – A Study in the Yangtze River Delta

Yanhong GAO1#+, Li ZENG2, Zhaoyang LIU1
1Fudan University, 2Chinese Academy of Sciences

Under global warming, centered with Shanghai, the Yangtze River Delta (YRD) of China has experienced an extreme precipitation increasing, in which the short-duration heavy precipitation increases significantly. Topography as well as its attributions are fundamental factors during precipitation generation. In this study, the relations between hourly extreme precipitation and five topographical factors with 12 km grid cell were explored using the Multi-scale Geographically Weighted Regression model established on observed precipitation records at CMA stations and topography. The extreme hourly precipitation events were divided into single-peak and double-peak according to the diurnal variation, which are corresponding to the weather background of Non-ENSO and ENSO year. Both types of extreme events capture the dominant role of the topographic relief. But the secondary topographical factors differ. In single-peak event, afternoon convections occur at the southeastern side of the Zhejiang-Fujian Mountains with larger slopes. However, in double-peak event, another peak occurs due to the moisture transfer in the morning. Therefore, the distance from the coastline becomes the secondary role. Two dynamic downscaling simulated precipitation at the horizontal resolution of the traditional quarter degree and convection-permitting scale are evaluated compared to the observed relationship between topographical factors and hourly extreme precipitation. Discrepancies of the coarse resolution simulation were revealed. This research highlights the key role of underground sub-grid variations on the precipitation in eastern China, which implies a potential way forward for precipitation simulation improvements.


AS51-A008 | Invited
Impacts of Coastal Terrain on Warm-sector Heavy-rain-producing MCSs in Southern China

Murong ZHANG1, Kristen RASMUSSEN2, Zhiyong MENG1#+, Yipeng HUANG3
1Peking University, 2Colorado State University, 3Xiamen Meteorological Bureau

Warm-sector heavy rainfall in southern China refers to the heavy rainfall that occurs within a weakly forced synoptic environment under the influence of monsoonal airflows. It is usually located near the southern coast and is characterized by poor predictability and a close relationship with coastal terrain. This study investigates the impacts of coastal terrain on the initiation, organization, and heavy rainfall potential of MCSs in warm-sector heavy rainfall over southern China using quasi-idealized WRF simulations and terrain-modification experiments. Typical warm-sector heavy rainfall events were selected to produce composite environments that forced the simulations. MCSs in these events all initiated in the early morning and developed into quasi-linear convective systems along the coast with a prominent back-building process. When the small coastal terrain is removed, the maximum 12-h rainfall accumulation decreases by ∼46%. The convection initiation is advanced ∼2 h with the help of orographic lifting associated with flow interaction with the coastal hills in the control experiment. Moreover, the coastal terrain weakens near-surface winds and thus decreases the deep-layer vertical wind shear component perpendicular to the coast and increases the component parallel to the coast; the coastal terrain also concentrates the moisture and instability over the coastal region by weakening the boundary layer jet. These modifications lead to faster upscale growth of convection and eventually a well-organized MCS. The coastal terrain is beneficial for back-building convection and thus persistent rainfall by providing orographic lifting for new cells on the western end of the MCS, and by facilitating a stronger and more stagnant cold pool, which stimulates new cells near its rear edge.


AS51-A019 | Invited
Microphysical and Dynamical Characteristics of Convection in the 21·7 Henan Extremely Heavy Rainfall Event

Kun ZHAO1#+, Gang CHEN2, Lu YINGHUI1, Zhe-Min TAN1, Ming XUE3
1Nanjing University, 2Nanjing Joint Institute for Atmospheric Sciences, 3The University of Oklahoma

In this study, significant rainfall microphysical variability is revealed for the extremely heavy rainfall event over Henan Province in July 2021 (the “21.7” Henan EHR event) using a dense network of disdrometers and two polarimetric radars. The broad distributions of specific drop size distribution (DSD) parameters are identified in heavy rainfall from disdrometers, indicating obvious microphysical variability on the surface. Combined with the supporting precipitation structures obtained through radar observations, distinct microphysical features of five DSD groups are derived. An extreme rainfall group is dominantly formed in the deep convection over the plain regions, where the high number of concentrations and large mean sizes of surface raindrops are underpinned by both active ice-phase processes and efficient warm-rain collision–coalescence processes in the vertical direction. Convection located near orographic regions is characterized by restricted ice-phase processes and high coalescence efficiency of liquid hydrometeors, causing the dominant DSD group to comprise negligible large raindrops. Moreover, the microphysical processes accompanying convective-scale and mesoscale dynamics of the convective cell causing the record-breaking hourly rainfall (201.9 mm) are investigated using the Variational Doppler Radar Analysis System. Clearly, the interaction between convective-scale and mesoscale dynamics and microphysical processes within favorable synoptic conditions led to the extremely heavy rainfall.


AS51-A022
The Evaluation of Precipitation Estimates and Simulations from the Remote Sensing Technologies and WRG Modeling Over the Peruvian Andes Region

Mengye CHEN1#+, Yang HONG1, Yongjie HUANG1, Hector Mayol NOVOA2
1The University of Oklahoma, 2Universidad Nacional de San Agustín de Arequipa

Peruvian Andes region has been proven in multiple studies to be one of a few regions have poor performance of many global precipitation estimations, due to its complex terrain and extreme interruption of atmospheric movement by the Andes mountain. This study provides an evaluation over two Peruvian local precipitation products PISCO and RAIN4PE, along with a regional dynamic downscaled WRF model simulation, and GPM-IMERG. The precipitation products were evaluated against local rain gauge data and used as the forcing data for CREST-VEC model to test the uncertainties of the precipitation products in a extremely dry region in Peru. This study readdress the accuracy issue of precipitation products in the Peruvian Andes region, and highlights the importance of using WRF modeling simulation to ‘fill-the-blank’ of heterogenous rain gauge distribution, when remote-sensing technologies fail to perform in this area.


Fri-04 Aug | 10:20 - 12:20 | MR328
AS13 - Polar Atmospheric Processes and Their Interactions with the Surface

Session Chair(s): Yuekui YANG, NASA Goddard Space Flight Center

AS13-A001 | Invited
Polar Climate Change and its Global Impact

Seong-Joong KIM1,2#+, Joo-Hong KIM1, Sang-Yoon JUN1, Sang-Jong PARK1, Eui-Seok CHUNG1, Yonghan CHOI1, Hye Sun CHOI1
1Korea Polar Research Institute, 2University of Science and Technology

In response to the increase in greenhouse gases, the Arctic is warming nearly four times as fast as the global average. The rapid Arctic warming, associated with the rapid ice melting over the Arctic Ocean and Greenland, has been reported to have an impact on extreme weathers in midlatitudes by modulating polar vortices, though the linking mechanism remains controversial. In Antarctica, climate changes are different regionally with little warming or even cooling in the eastern part and large warming in western part. In order to understand the polar climate change and its impact on polar regions and lower latitudes, we have participated the year of polar prediction (YOPP) program in both the Arctic and Antarctica for the past several years including the observation campaigns of Special Observing Period in 2018-2019 and Targeted Observing Period in 2022 from the Antarctic Jangbogo and King Sejong Stations and in the Arctic Ocean during the IBRV Araon’s summer Arctic research expedition. In the Arctic, we have measured the summertime characteristics of sea ice and atmosphere by the IBRV Araon, while in the Dasan research station in Svalbard, we have observed cloud droplets and boundary layer wind characteristics for the entire year. In addition, we have deployed a buoy over the Bering Sea to figure out the role of subarctic on the heatwaves over the Korean Peninsula.


AS13-A002
The Arctic-siberian Plain Warming Causes the East Asian Heat Waves

Jeong-Hun KIM1,2+, Seong-Joong KIM3,4, Joo-Hong KIM3, Michiya HAYASHI5, Maeng-Ki KIM1#
1Kongju National University, 2Kongju National University, 3Korea Polar Research Institute, 4University of Science and Technology, 5National Institute for Environmental Studies

As global warming accelerates, it is reported that the frequency and intensity of heat waves and their associated socioeconomic damages have been increasing in East Asia. Hence, many studies have attempted to identify their causes and mechanism. Typically, the East Asian heat waves are mainly influenced by the Pacific-Japan (P-J) pattern and the circum-global teleconnection (CGT) pattern. In addition to the P-J and CGT patterns, recent studies suggested that various remote forcings also can contribute to the East Asian heat waves (e.g., Scandinavian pattern, North Atlantic Oscillation, Arctic Oscillation, Arctic Sea ice concentration, etc.). However, the teleconnection between the Arctic-Siberian Plain (ASP) warming and East Asian heat waves has not been considered. This study investigates the teleconnection mechanism between East Asian heatwaves and the warming over the ASP for the last 42 years (1979-2020). The results show that the anticyclonic anomaly over the ASP region, mainly affected by vorticity advection, increases the air temperature and surface evaporation. Enhanced surface radiative heating and specific humidity amplify the thermal high pressure through positive water vapor feedback. The Rossby wave, amplified by land-atmosphere interaction in the ASP, propagates to East Asia through the upper troposphere, causing favorable atmospheric patterns for the occurrence of the East Asian heatwaves.


AS13-A007
Asymmetric Arctic and Antarctic Warmings and Their Inter-model Spread in CMIP6

Yihan ZHANG#+
Sun Yat-sen University

Under the background of global warming, the Arctic region has warmed faster than the Antarctic, which is referred to as asymmetric Arctic and Antarctic warming. The new generation of model simulations from CMIP6 offers an opportunity to identify the major factors contributing to asymmetric warming and its inter-model spread. In this study, the pre-industrial and abrupt-4xCO2 experiments from 18 CMIP6 models are examined to extract the asymmetric warming and its inter-model spread. The climate feedback-response analysis method is applied to decompose the total warming into partial temperature changes caused by individual factors, which allows quantifying individual contributions of feedback processes to the asymmetric warming and its inter-model spread. It is found that the seasonal energy transfer mechanism (SETM), namely, the temporal storage of the extra solar energy absorption by the ocean in summer due to sea ice melting and then release in cold months via sensible and latent heat fluxes, plays an important role for stronger warming in winter than summer in both polar regions. The key factor for the inter-model spread in asymmetric warming is the difference in the strength of SETM. The poleward atmospheric transport and water vapor feedback also contribute to the inter-model spread in asymmetric warming.


AS13-A009
Wildfire Activities in Northeast Siberia: Implications on Arctic Climate

Yeonsoo CHO1#+, Sang-Woo KIM1, Baek Min KIM2, Jinho YOON3, Jee-Hoon JEONG4
1Seoul National University, 2Pukyong National University, 3Gwangju Institute of Science and Technology, 4Chonnam National University

Wildfires in carbon-rich northern high latitudes are a crucial phenomenon due to their potential to worsen the air quality and accelerate warming in the Pan-Arctic regions. Here, we investigate the changes of wildfire activities in northern high latitudes during 2003 – 2022 using Moderate Resolution Imaging Spectroradiometer (MODIS) active fire data. Northeast Siberia is experiencing a significant increase in the number of wildfires (+11.04 % year-1) and an extension of the fire season (+3 days year-1), especially during 2017 – 2021. Strong and long-lasting warm and dry conditions and related strengthened anomalous anti-cyclonic circulation in Northeast Siberia under the Pan-Arctic warming are responsible for the ignition and persistence of wildfire. However, wildfire activities in 2022 declined rapidly despite persistent warming, which is analyzed in this study. Furthermore, extreme wildfire events in Northeast Siberia show biomass-burning aerosols and gases are transported into the Arctic Ocean, contributing to the rapid melting of sea ice and snow by altering the surface radiation budget. These results emphasize the importance of changing wildfire activities over Northeast Siberia in predicting the future Arctic climate.


AS13-A013
Changes in Tropics-SAM Relationship and its Impacts on the Antarctic Sea Ice Long-term Variability

Jihae KIM, Myong-In LEE#+, Joonlee LEE
Ulsan National Institute of Science and Technology

Antarctic sea ice extent has shown a significant increase in interannual variability in recent years, but the mechanisms of sea ice variability over a long time scale are in veil due to short observation data. This study examines the changed relationship between tropical forcing and the variability of Antarctic atmospheric circulations dominated by the southern annular mode (SAM) throughout 1982-2022. According to the EOF analysis using sea ice concentration, the first mode is related to the decadal variation and represents the entire variability of Antarctic sea ice. On the other hand, the second mode is characterized by the interannual time scale with a high correlation with the SAM index (r = -0.68). The positive SAM drives a dipole pattern of sea ice in the West Antarctic, which provides a favorable condition for sea ice melting in the Antarctic peninsula and growing in the Amundsen-Bellingshausen Sea. After the late 1990s, the dipole pattern of sea ice in the West Antarctic has become more robust compared with the past period, in which the changes in tropical forcing are likely to influence remotely. The increased precipitation in the central tropics has enhanced the convection, which signal propagates to the Antarctic through the Rossby wave, thereby forming strong negative anomalies in the West Antarctic (Weddell sea). The global model experiments with dynamical core support this teleconnection mechanism, and reveal that the recent change in tropical forcing is more closely linked to the Antarctic atmospheric patterns and sea ice.


Fri-04 Aug | 10:20 - 12:20 | MR329
AS14 - Subseasonal to Seasonal Forecasts and Applications

Session Chair(s): Chen SCHWARTZ, Centre for Climate Research Singapore

AS14-A016
The Subseasonal Prediction of Springtime Near-surface Temperature Evolution Over Indochina

Mien-Tze KUEH#+, Chuan-Yao LIN
Academia Sinica

The transition to rainy season in the Indochina Peninsula usually occurs in May, accompanying the decrease in near-surface temperatures over the region. The advancing southwest monsoon flow provides dynamic settings for the transition period, during which a negative relationship between the temperature and precipitation can be found on a daily basis. Therefore, the skillful subseasonal prediction of the near-surface temperature evolution over Indochina relies largely on the development of summer monsoon. We examine the subseasonal prediction of springtime near-surface temperatures in Indochina for two contrasting years: dry and hot 2016 and wet and cool 2022, based on their average conditions in April and May. The real-time forecasts from the ECMWF subseasonal-to-seasonal (S2S) forecasting system provide reasonable week-3 predictions of the tendency of hot conditions in May of 2016, but unsatisfying predictions for the cool May of 2022. The large-scale monsoon circulations are well predicted for both years. The forecast system can also capture the rainy spells in both years. We find that the local thermodynamic responses in the prediction system may provide hints for the performance of temperature predictions. For the higher temperature regime (approximately above 27.5 °C), the forecast values reveal a negative relationship between temperatures and precipitations, and the relationship remains valid with the precipitations in the preceding week. A similar pattern is also found between the temperatures and soil moistures, where such relationship is valid for a relatively longer period, even with the soil moistures in the preceding two weeks. We do not find any relationships between the lower temperature regime (below 27 °C) and precipitation or soil moisture. This may imply large uncertainty in the prediction of cool conditions.


AS14-A014
Tropospheric Precursor and Predictability of the 2021 Sudden Stratospheric Warming

Min-Jee KANG+, Hyeong-Oh CHO, Seok-Woo SON#
Seoul National University

The role of North Pacific bomb cyclones and the associated upper-level trough on the onset of January 2021 sudden stratospheric warming (SSW) is examined by conducting a set of numerical model experiments. The control simulation, initialized 10 days before the SSW onset, successfully reproduces the SSW. As this event is preceded by the bomb cyclones in the North Pacific, their impact is tested by initializing the model without them. This sensitivity experiment shows much weaker polar-vortex deceleration than the control simulation, resulting in no distinct SSW onset. This difference is attributable to the dampened constructive linear interference between the climatological wave and the cyclone-related wavenumber-one anomaly in the sensitivity experiment. It weakens the vertical propagation of wavenumber-one wave into the stratosphere, thereby reducing wave breaking in the polar stratosphere. This result suggests that bomb cyclones and the associated upper-level trough can be an important factor for improving SSW predictability. The predictability of the 2021 SSW in subseasonal-to-seasonal (S2S) prediction models is also examined. Particularly, ECMWF and JMA models, initialized 15 days and 13 days before the onset date, respectively, are used to investigate the key factors in the SSW onset. By comparing 10 ensembles with successful SSW and those without SSW, it is found that the upward-propagating planetary-scale wave at 60°-200°E from the upper troposphere (~300 hPa) is a crucial factor for the successful SSW prediction. This result suggests that the upper-level trough over East Eurasia to North Pacific is important in predicting successful SSW in S2S models.


AS14-A018
Study on Snow Data Assimilation Using Satellite Data Into the Jules Land Surface Model Based on LETKF

Joonlee LEE+, Myong-In LEE#
Ulsan National Institute of Science and Technology

Land initial states such as snow and soil moisture are crucial factors in season-to-sub-seasonal (S2S) time-scale predictions due to their climatic memory lasting 1-2 months. To improve the S2S prediction skills, this study aims to develop a land data assimilation system with the remote observation of snow water equivalent (SWE) and snow cover (SC) from a satellite based on the Joint U.K. Land Environment Simulator (JULES) land surface model (LSM) using the Local Ensemble Transform Kalman Filter (LETKF). The system assimilates SWE using Advanced Microwave Scanning Radiometer 2 (AMSR2) and the SC from Information Service Interactive Multisensor Snow and Ice Mapping System (IMS). The background field produced by the JULES land model was comparable to the snow distribution of JRA-55 reanalysis data used for boundary forcing. The climatological analysis field produced through the LETKF data assimilation showed a distribution similar to that of the background field, while the temporal variance of the analysis field has a superior performance compared to it. In particular, the performance improvement is notable in the mid-latitude snow transition region, where having SWE ranges from 0.001 to 20 mm climatologically. High values of the Kalman gain are also shown in the transition region, indicating that the effect of data assimilation is significant in the transition region. In this regard, we expect that data assimilation with satellite data will contribute to improving the S2S prediction skills in climate models.


AS14-A025
The Transition of Stratospheric Polar Vortex Intensity and it Subseasonal Climate Predictability: A Case Study of Winter 1987/88

Ke FAN#+
Sun Yat-sen University

The stratospheric polar vortex (SPV), an important factor in subseasonal-to-seasonal climate variability and climate prediction, exhibited a remarkable transition from weak in early winter to strong in late winter in 1987/88 (the most significant in inter-annual timescale during 1979–2019). Therefore, we selected winter 1987/88 as an extreme case to analyze its stratosphere-troposphere interaction processes and its subseasonal predictability. Results indicate that the positive transition of SPV intensity was probably caused by the negative transition of upward planetary wave intensity entering the stratosphere, especially planetary wave-1. It is found that the anomalous strong (weak) upward planetary wave-1 in the stratosphere originates from the increased (reduced) generation of planetary wave-1 in the lower troposphere. Accompanied by anomalous SPV intensity, the positive (negative) stratospheric zonal wind anomalies were able to propagate downwards into the troposphere during strong (weak) SPV stages. And these out-of-phase downward propagating anomalies contributed to the out-of-phase tropospheric zonal wind anomalies between these two stages, which appeared as North Atlantic Oscillation (NAO)-like zonal wind anomalies in the North Atlantic region and similar dipole-like anomaly mode but in the Asia-Arctic region at 500 hPa. Then, the subseasonal predictability of this transition SPV case in 1987/1988 was investigated using the hindcasts from Subseasonal-to-Seasonal Prediction project. Results indicated that the predictability of both weak and strong SPV stages in winter 1987/88, especially near their peak dates, exhibited large sensitivity to the initial condition, which derived mainly from the sensitivity in capturing the 100-hPa eddy heat flux anomalies. The Eurasian teleconnection wave trains might be a key precursor for the weak SPV stage.


AS14-A004
A Novel Application of the Initial Stratospheric Polar Vortex State to the East Asian Spring Rainfall Prediction from Seasonal Forecast Models

Jian RAO1#+, Chaim GARFINKEL2, Tongwen WU3, Jing-Jia LUO1
1Nanjing University of Information Science & Technology, 2Hebrew University of Jerusalem, 3China Meteorological Administration

The possible impact of the stratospheric polar vortex on East Asian spring rainfall and the representation of this effect in seasonal forecast models are assessed. A strong stratospheric polar vortex is typically associated with dry conditions across Southeastern China and wet conditions across Korea and Japan in spring. Seasonal forecast models have a decent skill of forecasting the stratospheric polar vortex strength in March. However, they show a wide spread in the predictability of East Asian spring rainfall, possibly due to the underrepresentation of the linkage between the stratospheric polar vortex and East Asian rainfall. The dry impact of strong polar vortex on Southeastern China is forecasted, but the wet impact on Korea and Japan is missing. Tropospheric positive height anomalies over Lake Baikal extend farther equatorward in East Asia during a strong vortex, corresponding to an anomalous anticyclone and less rainfall across Southeastern China. In contrast, the observed anomalous cyclonic shear at 200 hPa and the observed anomalous cyclone at 850 hPa in spring are not realistically forecasted over Northeast Asia, explaining the low skill of producing the wet anomalies in Korea and Japan by models.
Seasonal forecasting models have a harder time accurately predicting regional precipitation anomalies in East Asia than the large-scale drivers of these precipitation anomalies. A maximum covariance analysis is used to isolate the SST and stratospheric patterns most associated with anomalous East Asian precipitation, which are employed to correct seasonal forecasts by projecting the forecasted stratospheric circulation and SST onto the observed combined modes. The nonuniform predictability of East Asian rainfall in seasonal forecast models is improved after error correction with the observed linkage between the stratosphere–tropical ocean modes and East Asian rainfall. This method should be helpful for improving rainfall forecasts in other regions as well.


AS14-A003
Forecast Skill of the Large MJO Case in March 2015

Tetsuo NAKAZAWA1#+, Mio MATSUEDA2
1The University of Tokyo, 2University of Tsukuba

To understand MJO better, we first picked up the “top five largest” MJO cases by selecting the large amplitudes of the multivariate MJO index. The largest one in March 2015, when the devastating tropical cyclone Pam hit Vanuatu over the South Pacific ocean. The ensemble forecast data in ECMWF shows that the forecast skill is low during the week stage of MJO, but the time goes on, it is getting better both before/after the peak amplitude a week in advance. The peak amplitude would be related with the planetary-scale tropical divergence maximum, which lags about two weeks after the equatorial large-scale convection peak. 


AS14-A027
Oceanic Rossby Wave Predictability in ECMWF’s S2S Model

Jonathan CHRISTOPHERSEN#+, Adam RYDBECK, Maria FLATAU, Matthew JANIGA, Carolyn REYNOLDS, Tommy JENSEN, Travis SMITH
Naval Research Laboratory

In recent years, studies have put forth various theories and findings on the role of oceanic equatorial Rossby waves (OERW) in the subseasonal-to-seasonal (S2S) predictability of the Indian Ocean (IO). While much of the scientific literature uses data from in-situ, satellite, and/or reanalysis datasets, this study focuses on reforecast fields from the European Centre for Medium-Range Weather Forecasting’s (ECMWF) S2S dataset. Evaluation of the model’s predictive skill in representing OERWs and the associated variations in sub-surface-to-surface interaction and air-sea coupling are discussed. This work provides a unique methodology to calculate and evaluate the predictability of OERWs from model forecast data, which, to the author’s knowledge, is the first of its kind to do so. Our results indicate that the model forecasts OERWs with relatively high skill (anomaly correlation > 0.5 out to 40 days), indicating they are a key source of oceanic subseasonal predictability at extended lead times. Analysis of the wavenumber-frequency spectra for the IO indicates a reduction in power throughout the model forecast time period in the oceanic equatorial Kelvin wave (OEKW) regime, indicating the potential misrepresentation of the zonal winds. This erroneous weakening of the OEKWs are attributed to the weakening of the reflected oceanic equatorial Rossby waves (OERWs). This results in weaker transport of the associated westward advection of warm ocean heat content (OHC) anomalies via the OERWs, which has numerous implications for air-sea and sub-surface-to-surface coupling as will be discussed. In general, the atmospheric response to the waning westward transport of OHC anomalies in the western IO is associated with the weakening of precipitation anomalies related to the diminishing intraseasonal oscillation.


Fri-04 Aug | 10:20 - 12:20 | MR331
AS17 - Application of Satellite Data to Weather, Climate and Environmental Study

Session Chair(s): Myoung Hwan AHN, Ewha Womans University

AS17-A003 | Invited
Using Satellite Microwave Sounder to Observe Strong Storms at the Pre-convection Stage

Min MIN1#+, Xiaocheng WEI2
1Sun Yat-sen University, 2National Satellite Meteorological Center

High-temporal-resolution geostationary satellite infrared measurements are always used to capture and predict typical characteristics at the cloud top of rapidly developing strong storms at the pre-convection or convection initiation (CI) stage. However, the large false alarm rate of CI nowcasting is difficult to avoid due to the complex and unpredictable trigger factors. Although the microwave measurement technique can observe thick clouds and even the precipitation within clouds due to the weaker atmospheric extinction effect on microwave, microwave data from polar-orbiting satellites are rarely used to observe the CI due to their relatively low temporal resolution. In this study, we analyze several previously unknown CI characteristics over the East Asia region from 2016 to 2019 based on spatially and temporally matched Advanced Technology Microwave Sounder data. These typical CI samples are initially identified by using continuous infrared images from the Himawari-8 geostationary satellite. The results show that there is a distinct cloud optical depth at the pre-convection stage in the western (deep cloud clusters) and eastern (shallow cloud clusters) Tibetan Plateau (TP). The shallow precipitating cloud clusters of the CI over the eastern TP are possibly attributed to the favorable local dynamic and thermal conditions stem from the Asian monsoon. Another notable finding shows that the fast-developing CI over the ocean has thick clouds compared with the samples over the land. Overall, the unique CI characteristics found from microwave observations in this study indicate that the future geostationary microwave sounder technologies will almost certainly provide some new findings and enhance early warning capabilities about convection.


AS17-A019
Cloud Identification and Properties Retrieval of the Fengyun-4A Satellite Using a Resunet Model

Feng ZHANG1#+, Zhijun ZHAO1, Qiong WU2, Zhengqiang LI3, Xuan TONG1, Jingwei LI4, Wei HAN5
1Fudan University, 2Shanghai Central Meteorological Observatory, 3Chinese Academy of Sciences, 4Shanghai Qi Zhi Institute, 5Chinese Meteorological Administration

The Advanced Geostationary Radiation Imager (AGRI) onboard the Fengyun-4A (FY4A) satellite has good cloud observation ability, but it still absents all-weather and high-precision official cloud products. This study develops a deep-learning ResUnet model for all-weather retrieval of cloud phase (CLP) and cloud properties using the brightness temperature from water vapor and longwave infrared channels of AGRI. The ResUnet model is trained with the Himawari-8 satellite Level-2 (H8-L2) cloud products as true targets, and adopts image-by-image way to learn the spatial structure information of clouds, which compensates for the difficulty of retrieving thick clouds by thermal infrared radiation at night to some extent. On an independent testing dataset, the model has an overall accuracy of 90.64% for CLP identification and performs well at retrieving cloud top height (CTH). Even without using visible and near-infrared radiation, the root mean square error of cloud effective radius (CER) and cloud optical thickness (COT) estimations still reaches 7.14 µm and 9.01 in the range of 0−60. To further illustrate the reliability and applicability, CLP and cloud properties provided by the CALIPSO and MODIS are used as benchmarks to assess the quality of cloud products from FY4A satellite Level-2 (FY4A-L2), H8-L2 and ResUnet model retrieval. The ResUnet model provides a significant improvement over FY4A-L2 for the accuracy of cloud identification and in the quality of CTH products. In the range of 0−40 µm (0−60), the CER (COT) product of ResUnet model retrieval has a reliable and higher precision that is comparable with H8-L2.


AS17-A037
Cloud Properties and Surface Solar Radiations Observed from Global New Geostationary Satellites

Husi LETU#+, Huazhe SHANG, Liangfu CHEN
Chinese Academy of Sciences

In this study, we developed an algorithm to retrieve global cloud properties and solar radiations from four geostationary satellites. These cloud properties and solar radiations include cloud mask, cloud phase, cloud optical thickness, cloud effective radius, cloud top temperature/pressure/height, as well as shortwave radiation (SWR), photosynthetically active radiation (PAR), ultraviolet-A (UVA), and ultraviolet-B (UVB), as well as their direct and diffuse components. Our algorithm combines the high accuracy of radiative transfer model (RSTAR) and machine learning techniques, and effects of cloud phases, aerosol types, gas components are considered. Validation with ground-based data shows that the accuracy of the SWR and PAR compositions are better than those of state-of-the-art products, while the accuracy of UVA and UVB measurements is comparable with CERES. We analyzed the characteristics of aerosols, clouds, gases, and their impacts on SSRC before, during and after COVID-19. In particular, significant SSRC variations due to the reduction of aerosols and increase of ozone are identified in the Chinese central and eastern areas during that period. The spatial–temporal resolution of data products (up to 0.05°/10 min for the full-disk region and 0.02°/10 min for specific areas) is one of the most important advantages. Our SSRC products can be downloaded from the CARE website: http://www.slrss.cn/care/sp/pc/.


AS17-A006
NDWI and Near-Infrared Bands based Cloud Detection Method Using CALIPSO Satellite for GEO-KOMPSAT-2A Satellite

Yunjeong CHOI+, Sungwook HONG#
Sejong University

Cloud detection is a fundamental step required for estimating secondary satellite products. Many previous cloud detection studies have used reflectance and brightness temperature in various approaches. This study proposes a unique and simple cloud detection method using two visible (VIS) and two near-infrared (NIR) bands. This study used the Advanced Meteorological Imager (AMI) observation data of GEO-KOMPSAT-2A (GK2A) for the cloud detection algorithm, which was validated with the Lidar Level 2 Vertical Feature Mask (VFM) data of the CALIPSO satellite. The East Asia region within 15° to 45° in latitude and 100° to 150° in longitude was chosen as the study area for the GK2A satellite zenith angle to be less than 65°. Methodologically, first, thick clouds were detected using the Normalized Difference Water Index (NDWI) and a relationship between NDWI and the AMI green band. Second, cirrus clouds and thin clouds were detected using 1.38 μm and 1.64 μm bands, which are sensitive to cirrus and cloud ice particles, respectively. We added the Normalized Difference Snow Index (NDSI) as an intermediate step to the proposed cloud detection algorithm over land. The thresholding coefficients of the proposed algorithm were determined from a comparison with the CALIPSO VFM data using 135 cases in 2020 and 128 cases in 2021. As a result, the proposed cloud detection method and CALIPSO VFM showed the probability of detection POD=0.88, false alarm ratio FAR=0.08, and percent correct PC=0.87 in the cases of 2020, and POD=0.84, FAR=0.10, PC=0.83 in the cases of 2021. Additionally, the proposed cloud detection algorithm showed an advantage in distinguishing between sea ice and clouds different from other existent cloud detection algorithms. Consequently, this study can be applied as a cloud detection algorithm to numerous low-orbit and geostationary-orbit satellites with VIS and NIR bands.


AS17-A039
Estimating Carbon Dioxide Emissions with the Orbiting Carbon Observatory-2

Chunlin JIN+, Yong XUE#, Tao YUAN, Liang ZHAO
China University of Mining and Technology

In order to cope with the climate crisis caused by massive emissions of greenhouse gases, mainly carbon dioxide (CO2), many countries participating in the Paris Agreement have made commitments to reduce CO2 emissions, hoping to achieve the goal of limiting global temperature rise within 2℃ in this century. Estimation of CO2 emissions through satellite observations provides a way to assist in more transparent verification of each partner country's contribution to reducing emissions. In this study, we used XCO2 (the column-average dry-air mole fraction of atmospheric) enhancement observed by Orbiting Carbon Observatory-2 (OCO-2) to retrieve regional CO2 emissions. Assuming that the Ratio of grid CO2 emissions provided by the Anthropogenic CO2 Open Data Inventory (ODIAC) to actual emissions in the 1°×1° region is linear, we used an improved Gaussian plume model to simulate the XCO2 enhancement caused by ODIAC emission sources and obtained the true regional carbon emissions by minimizing the difference between the simulated XCO2 enhancement (ODIAC×Ratio) and the OCO-2 detected XCO2 enhancement. From September 2014 to December 2021, the global estimated average emissions of OCO-2 are 6.66 times higher than those reported by ODIAC. At the same time, we found that in China, the difference between the OCO-2 results and Multi-resolution Emission Inventory for China (MEIC) was small and the average emission from OCO-2 was 1.88 times that reported by MEIC. All evidence indicates an overall underestimation of the ODIAC and MEIC inventories.


AS17-A005
Virtual RGB Bands of Advanced Meteorological Imager Onboard Geo-KOMSAT-2A Through Data-to-data Translation

Kyung-Hoon HAN1+, Sumin RYU2, Eunha SOHN3, Jae-Cheol JANG3, Sungwook HONG1#
1Sejong University, 2Korea Aerospace Research Institute, 3Korea Meteorological Administration

The red-green-blue (RGB) true-color images based on satellite observations at visible bands provide various atmospheric and surface information and are crucial for intuitive understanding and visualization. This study presents a data-to-data (D2D) translation method based on the combination of a conditional generative adversarial network (CGAN) and data normalization to generate virtual daytime and nighttime RGB images of the advanced meteorological imager (AMI) sensor onboard GEO-KOMPSAT-2A (GK-2A) satellite. The D2D model used pre/post-processed AMI brightness temperature (BT) and albedo data. In detail, the D2D model was trained and tested using the datasets of the BT at AMI infrared (IR) bands, the BT difference between the two AMI IR bands, and the albedo at the AMI three visible bands. For the daytime, the D2D model compared to the observed AMI visible bands showed statistically excellent results, including correlation coefficient (CC) = 0.941, root mean square error (RMSE) = 0.047, and bias = -0.006 in albedo for the blue band; CC = 0.939, RMSE = 0.050, and bias = -0.007 in albedo for the green band; CC = 0.917, RMSE = 0.061, and bias = -0.010 in albedo for the red band. The D2D model demonstrated excellent results in simulating virtual AMI VIS bands for both day and night while showing limitations in simulating desert areas with high-temperature contrast during day and night. The Korea Meteorological Administration provides the proposed D2D model RGB products in official service to the public. Consequently, this study contributes significantly to the monitoring and understanding global meteorological phenomena by complementing present GK-2A observation.


Fri-04 Aug | 10:20 - 12:20 | MR332
AS07 - General Session for Atmospheric Sciences

Session Chair(s): Masaki SATOH, The University of Tokyo

AS07-A047
Doppler Lidar Based Observation Nudging Towards Improving the Model Accuracy in Predicting Major Weather Variables

Sridhara NAYAK#+, Isao KANDA
Japan Meteorological Corporation

In this study an attempt is made to improve the major weather variables in the weather research and forecasting (WRF) model by using the Doppler Lidar based observation nudging over the Osaka region of Japan. We performed various simulations with different model configurations and domain setups at different horizontal resolutions (100-500m) with and without observation nudging. The results indicated that the major weather variables such as temperature, precipitation, wind etc. are better captured in the simulations with Lidar based nudging compared to those simulations without nudging. The root mean square error (RMSE) in reproducing these weather variables decreased and correlation coefficient (R) is increased after using the nudging not only at Lidar location but also at the locations far from the Lidar location (e.g. AMeDAS observation stations). Our overall analysis emphasized an improvement of the profiles of weather variables by considering the Lidar based observation nudging in the WRF simulation.


AS07-A050
Regional and Seasonal Variations of the Double-ITCZ Bias in CMIP6 Models

Baijun TIAN1,2#+
1Jet Propulsion Laboratory, California Institute of Technology, 2University of California, Los Angeles

The double-intertropical convergence zone (ITCZ) bias is one of the most persistent and outstanding biases in fully coupled global climate models. Based on the annual mean tropical precipitation distributions and indices, Tian and Dong (2020) found that the double-ITCZ bias and its big inter-model spread persist in the latest fully coupled global climate models that participated in the Coupled Model Intercomparison Project (CMIP) Phase 6 (CMIP6) although the double-ITCZ bias is slightly decreased in CMIP6 models in comparison to CMIP Phase 3 (CMIP3) and CMIP Phase 5 (CMIP5) models. In this study, we examine the regional and seasonal variations of the double-ITCZ bias as well as the difference of the double-ITCZ biases between the fully coupled and atmosphere-only models in CMIP6 models to better understand the origin of the double-ITCZ bias in CMIP6 models. The NASA satellite data, such as TRMM, GPCP and AIRS will be used in this study.


AS07-A028
Methods to Evaluate Dipolar Climate Patterns

Sandro F. VEIGA#+, Huiling YUAN
Nanjing University

In climate studies, one of the most widely used metrics to evaluate spatial patterns simulated by climate models is the Taylor skill score (TS score). However, this metric may fail to accurately assess the ability of climate models to simulate the similarity of dipolar or multipolar climate patterns with observation because the TS score compares the spatial variances of model and observation patterns (through their ratio) but ignores their spatial variances' distributions. In light of this, we compare three metrics to evaluate dipolar (East Asian summer monsoon) and multipolar (Pacific-North American pattern) climate patterns simulated by six CMIP6 state-of-the-art models. The metrics that are evaluated are the TS score, an adjusted Taylor skill score (TSadj score) that relies on the normalized root-mean-square error, and the Arcsin-Mielke skill score. As a reference for this comparison, we adapt the Contiguous Rain Areas to estimate the baseline error of the model's simulation.


AS07-A052
Responses of East Asian Climate to SST Anomalies in the Kuroshio Extension Region During Boreal Autumn

Yu GENG1+, Hong-Li REN1,2#
1Chinese Academy of Meteorological Sciences, 2China University of Geosciences

Sea surface temperature anomalies (SSTAs) in the Kuroshio Extension (KE) region play a key role in influencing midlatitude climate variations. This study investigates the impacts of SSTAs in the KE region (KE-SSTA) on East Asian climate during boreal autumn. The results reveal that positive KE-SSTA, changing the meridional temperature gradient in the lower troposphere, contributes to the formation of an anomalous quasi-barotropic anticyclonic circulation (AC) over the KE region. Such a configuration tends to be affected by wind through thermal wind adjustment. Simultaneously, it is also impacted by eddy activity related to the strengthened atmospheric baroclinicity through transient eddy feedback. By both means, obvious descending motion and warm advection are generated, which increases tropospheric temperature through adiabatic heating and further maintains the abnormal AC over the KE region. This anomalous circulation changes wind in the east of the East Asian trough, which favors the transportation of warm and wet air from the midlatitude northwest Pacific and further causes the increase of temperature in northeastern East Asia. Moreover, it also leads to the convergence and divergence of water vapor fluxes in Northeast Asia and eastern North China, favoring the increase and decrease of precipitation in the two regions, respectively. The above responsive characteristics of the midlatitude atmospheric circulation to positive KE-SSTA can be confirmed by numerical experiments. These results suggest that anomalous SST in the KE region can be used as a potentially effective predictability source for autumn climate variations in the mid to high latitudes of East Asia.


AS07-A048
Remote Tropical Central Pacific Influence on Driving Sea Surface Temperature Variability in the Northeast Pacific

Hao-Jhe HONG+, Huang-Hsiung HSU#
Academia Sinica

The Northeast Pacific (NEP) had two record-breaking marine heatwave events (MHWs) in the winters of 2013–2015 and summer of 2019, which had a detrimental impact on the fisheries, marine ecosystems, and climate in North America. Here, we investigated the cause of sea surface temperature (SST) variability in NEP during late spring–summer of 1981–2020. The regression circulation anomalies to the principal component of leading EOF mode suggested that the warm NEP SST were characterized by a cyclonic circulation anomaly in the midlatitude North Pacific and a warming SST center in the Gulf of Alaska. We noted that this cyclonic circulation anomaly, attributable to a barotropic atmospheric wave originating from the tropical central Pacific (CP) in the preceding spring, reduced the surface heat flux loss from the ocean to the atmosphere in the NEP and led to the warm SST anomalies in summer. This finding was confirmed by not only empirical diagnosis but also long-term numerical simulations forced by the observed SST perturbations in the tropical CP. Our results highlight the role of the tropical CP SST in driving the summertime North Pacific SST variability through the atmospheric bridge in recent decades.


AS07-A049
Interdecadal Variation in Winter Precipitation Over Non-monsoonal Eurasian Regions

Xinhai CHEN#+, Xiaojing JIA
Zhejiang University

The interannual variations of winter precipitation over central Asia (CA) are investigated over the period 1948–2018 using both observational analysis and a linear baroclinic model (LBM). The focus is on the characteristics and factors of the leading empirical orthogonal function mode (EOF1) of winter precipitation over CA. The results show that the key circulation anomalies associated with the positive phase of EOF1 feature a tripole pattern that is responsible for transporting moisture from the subtropical North Atlantic region to CA. An examination of the lower boundary conditions indicates that anomalous North Atlantic sea surface temperature (SST), Kara Sea ice in the preceding autumn, and simultaneous snow cover in central Asia can promote large-scale atmospheric waves that contribute to the EOF1-related anomalous tripole pattern. This result is verified by an analysis of the apparent heat source (Q1) in the atmosphere and the LBM experiments. Linear regression (LR) models were constructed using the precursors revealed by the above observational analyses to perform hindcasts for EOF1 over the period 1950–2018. The North Atlantic SST and the Kara Sea ice in the preceding autumn are shown to be effective predictors in the LR model that can capture the variation in EOF1 during this period. The seasonal forecasts of winter precipitation over CA for the 2011–18 period based on the LR models outperform those of the Climate Forecast System version 2 (CFSv2) over central and northern CA.


Fri-04 Aug | 1:10 - 3:10 | MR311
AS57 - Progress and Challenge in Light Scattering and Radiative Transfer About Clouds and Aerosols

Session Chair(s): Takashi NAKAJIMA, Tokai University, Husi LETU, Chinese Academy of Sciences

AS57-A003 | Invited
Sounding the Atmosphere from Space for Weather Applications – Progress and Challenges

Jun LI#+
National Satellite Meteorological Center

Since the first Tiros-N Vertical Operational Sounder (TOVS) satellite was launched in 1979, sounding the atmosphere from space becomes the main approach for obtaining global atmospheric temperature and moisture vertical information for weather applications such as situation awareness, data assimilation for improving Numerical Weather Prediction (NWP), etc. Since 2002, measurements from the hyperspectral infrared sounders, together with the advanced microwave sounders, have become main sources of data needed for NWP, they also provide critical information for nowcasting applications. Despite those advancement in satellite sounding applications, the information used for weather applications are still very limited due to challenges including complex radiative transfer computations and the computational cost due to the large number of channels as well as establishing adequate error characteristics. With hyperspectral IR sounder onboard the geostationary orbit, rapid extraction of sounding information with high accuracy and low latency becomes the main challenges for real-time or near real-time applications. This presentation will overview the progress and challenges in the applications of atmospheric soundings from satellite for weather nowcasting and forecasting, with focus on addressing the needs on radiative transfer model that enables integration of spectral, spatial, and temporal information from hyperspectral IR sounder measurements, especially under all-weather conditions, for real-time or near real-time weather applications.


AS57-A011 | Invited
Derivation of Aerosol Parameters from Newly-launched Spaceborne Sensors

Jian XU1#+, Lanlan RAO1, Adrian DOICU2, Zhuo ZHANG1, Chong SHI3, Husi LETU1, Yongmei WANG4, Entao SHI1
1Chinese Academy of Sciences, 2German Aerospace Center, 3Aerospace Information Research Institute, Chinese Academy of Sciences, 4National Space Science Center, CAS

Aerosols have an impact on Earth’s radiation budget by scattering and absorbing solar radiation (direct effect) and by influencing the cloud formation processes (indirect effect). Highly-absorbing aerosols also affects the atmosphere causing the evaporation of cloud particles, which can decrease the size of the cloud cover (semi-direct effect). Reliable observations of aerosol parameters like layer height, optical depth, and UV aerosol index, are essential for a better understanding of aerosol effects on air pollution and climate. A number of new-generation passive spaceborne instruments have been recently launched and are monitoring aerosol properties using different spectral ranges. Measurements in the UV, visible, and near infrared spectral bands from Tropospheric Monitoring Instrument (TROPOMI) onboard Sentinel-5P, Ozone Monitoring Suite (OMS) onboard FengYun-3F, and Absorbing Aerosol Sensor (AAS) onboard GaoFen-5B are used to derive aerosol absorbing index, optical depth, and height information. The goal of this study is to incorporate an improved cloud detection and radiative transfer calculation into the adopted aerosol retrieval algorithms and to analyze the retrieval results from the above-mentioned spaceborne instruments.


AS57-A001
Measurement of the Cloud Properties and the Cloud Evolution Process from Novel Satellites, the GCOM-C and the EarthCARE

Takashi NAKAJIMA#+, Minrui WANG, Yu MATSUMOTO, Kanta SHIMIZU
Tokai University

The IPCC/AR6 pointed out that the prediction of the future climate still has some uncertainties. Our lack of knowledge about the aerosol-cloud interaction, in terms of the cloud evolution process, is one of the sources of such uncertainties. Therefore, it is very important to study cloud distributions on the Earth, and the mechanisms of the cloud evolution process in nature, from observations and modeling. In this paper, we are going to show validation results of cloud flag products obtained from the GCOM-C (launched 2017). For this study, we obtained cloud amount data using ground-based whole-skycamera images and compare them against the GCOM-C cloud flags. A simple threshold technique and a machine learning technique have been applied for detecting cloud area from the whole-skycamera images. Also, we are going to show some candidate observation products that will be obtained from the EarthCARE (will be launched in 2024, by corroborative mission of JAXA, ESA, an NICT). Indeed, we performed a statistical analysis of the CloudSat/CPR and the Aqua/MODIS data, as a preparatory stage of the EarthCARE, to depict cloud evolution process as global scale and regional scale. This statistical method is called, Contoured Frequency by Optical Depth Diagram (CFODD). In the CFODD, we can confirm clear contrast between the CFODDs obtained at e.g. East Asia, Californian, and Peruvian. This means that the cloud evolution features are different in such three regions.


AS57-A010
Ice Cloud Synergy Retrieval Using Joint Passive Infrared and Microwave Instruments

Chenxi WANG1,2#+, Jie GONG3, Kerry MEYER2, Steven PLATNICK2, Dong WU2, Zhibo ZHANG4
1Goddard Earth Sciences Technology and Research (GESTAR) II, 2NASA Goddard Space Flight Center, 3Universities Space Research Association, 4University of Maryland, Baltimore County

Previous comparisons of satellite ice cloud products have demonstrated that, although yield similar spatial/zonal patterns, ice cloud properties such as ice water path (IWP) and cloud optical thickness (COT) from different instruments can vary by a factor of 10. The large discrepancy arises because of observational differences from multi-instruments such as spectral channels, solar/viewing geometries, and footprint sizes. The present study aims at exploring a feasible retrieval approach to leveraging the advantages of two passive spectrally independent (IR and MW) instruments while minimizing the systematic biases from their large field of view (FOV) differences. As a pioneer study, we focus on IWP and cloud-top height (CTH) retrievals using IR narrow bands and high-frequency MW bands (>165 GHz) from VIIRS and ATMS, respectively. Similar approaches can be applied to many other instruments that are largely different in FOV sizes (e.g., VNIR/SWIR spectrometer and high-spectral resolution IR Sounder.


AS57-A015
Particle and Single Scattering Database for Cross-mission Support of Particulate Matter Retrievals

Ian ADAMS1#, Kwo-Sen KUO2,3+, Ines FENNI4, Robert SCHROM1, William OLSON1, George J. HUFFMAN1, Scott BRAUN1
1NASA Goddard Space Flight Center, 2University of Maryland-College Park, 3Bayesics, LLC, 4NASA Jet Propulsion Laboratory

All physics-based algorithms for particulate matter retrievals start with the single-scattering properties (SSPs) of the constituent particles, e.g., aerosols, cloud and precipitation hydrometeors, phytoplankton, etc. We numerically solve the electromagnetic scattering (EMS) problem of the individual particles for the SSPs, which are in turn used by the retrieval algorithms. For spherical particles or those with symmetries to exploit, the EMS problem is efficiently solved using methods such as Mie and T-matrix. Due to the symmetries, the storage requirement for the solutions is relatively modest. Unfortunately, a large portion of the naturally occurring particles is irregular, without symmetry to be exploited by these efficient solution methods. In their 2-part papers, Kuo et al. (2016, https://doi.org/10/f8h83f) and Olson et al. (2016, https://doi.org/10/f8h9qw) have shown the importance of realistic shapes to consistent active-and-passive combined retrievals of solid-phase precipitation. Thus, to better the retrieval, more sophisticated methods are required to solve the more general problem. These methods are accordingly more computationally demanding, requiring considerable high-performance computing resources. Because of the lack of symmetry in the particles, the solutions are more voluminous as well, necessitating much greater storage capacity. It is wasteful and often impossible for researchers to repeat such calculations and procure the needed storage. We have thus proposed a Particle and Single Scattering Database (PaSS DB) to collect, warehouse, and disseminate the particle structures and corresponding SSPs in cross-mission support of particulate matter retrievals. We outline the rationale and roadmap of PaSS DB development in this presentation.


AS57-A007
Establishment of an Analytical Model for Remote Sensing of Typical Stratocumulus Cloud Profiles Under Various Precipitation and Entrainment Conditions

Huazhe SHANG#+
Chinese Academy of Sciences

Structural patterns of cloud effective radius (ER) and liquid water content (LWC) profiles are essential variables of cloud lifecycle and precipitation processes, while observing cloud profiles from passive remote sensing sensors remains highly challenging. Understanding whether there exist typical structural patterns of ER and LWC profiles in liquid clouds and how they link with cloud entrainment or precipitating status is critical in developing algorithms to derive cloud profiles from passive satellite sensors. This study aims to address these questions and provide a preliminary foundation for the development of liquid cloud profile retrievals for the Multi-viewing, Multi-channel and Multi-polarization Imaging (3MI) sensor aboard the European Organization for the Exploitation of Meteorological Satellites (EUMETSAT) Polar System-Second Generation (EPS-SG) satellite, which is scheduled to be launched in 2025. Firstly, we simulate a large ensemble of stratocumulus cloud profiles using the Colorado State University (CSU) Regional Atmospheric Modeling System (RAMS). The empirical orthogonal function (EOF) analysis is adopted to describe the shape of simulated profiles with a limited number of elemental profile variations. Our results indicate that the first three EOFs of LWC and ER profiles can explain >90% of LWC and ER profiles. The profiles are classified into four prominent patterns and all of these patterns can be simplified as triangle-shaped polylines. The frequency of these four patterns is found to relate to intensities of the cloud-top entrainment and precipitation. Based on these analyses, we propose a simplified triangle-shape cloud profile parameterization scheme allowing to represent these main patterns of LWC and ER. This simple yet physically realistic analytical model of cloud profiles is expected to facilitate the representation of cloud properties in advanced retrieval algorithms such as those developed for the 3MI/EPS-SG.


AS57-A017
Recent Updates and Applications of the UNL-VRTM Remote Sensing Testbed

Xiaoguang XU1#+, Jun WANG2
1University of Maryland, Baltimore County, 2The University of Iowa

The Unified Linearized Vector Radiative Transfer Model (UNL-VRTM) was specifically designed as a testbed for remote sensing of Earth atmosphere and surface, especially for aerosols. It is freely available to the community to promote open science and collaboration in the fields of atmospheric science. Since its debut in 2014, UNL-VRTM has been applied to various studies in remote sensing of aerosols, clouds, trace gas, and ground surface. The model itself has also gained many important updates. In this presentation, we aim to provide a review of its physics, philosophy, capabilities, and recent updates. Moreover, we will showcase a few interesting applications of this model in the information content analysis for atmospheric aerosols and clouds from recent and upcoming satellite sensors.


AS57-A018
Linearization of Light Scattering Properties Using the Invar-iant-imbedding T-matrix and Physical-geometric Optics Methods

Bingqiang SUN#+, Chenxu GAO, Dongbin LIANG
Fudan University

Linearization of light scattering properties is significant for the physical retrievals of particle microphysical parameters. Light scattering properties of a single particle include its differential scattering properties represented by a scattering phase matrix and its integrated scattering properties such as extinction, absorption, and scattering cross-sections, and asymmetry factor. The scattering properties can be efficiently obtained using the invariant imbedding T-matrix method (IITM) for small particles and the physical-geometric optics method (PGOM) for large particles. In this study, the linearization with respect to the refractive indices, size parameters, and shape factors is obtained using the IITM and the PGOM [1-2]. The linearization is verified using the extended-boundary condition method for the IITM linearization and the finite-difference method for both linearization. The capability and convergence for the two algorithms are discussed based on the linearized scattering properties [3]. The sensitivities associated with linearized parameters are shown and discussed. A linearized scattering database only for the regular hexagonal prisms from 0.4 to 15 microns is also established and discussed for demonstration [4]. References [1] Sun, C. Gao, L. Bi, and R. Spurr (2021). Analytical Jacobians of single scattering optical properties using the invariant imbedding T-matrix method. Opt. Express 29, 9635-9669. [2] Liang and B. Sun (2022). Linearization of light scattering properties based on the physical-geometric optics method. Opt. Express 30, 22178-22199. Sun, C. Gao, D. Liang, Z. Liu, and J. Liu (2022). [3] Convergence and applicability of linearized invariant-imbedding T-matrix and physical-geometric optics methods. Opt. Express 30, 37769-37785. Gao, D. Liang, B. Sun, J. Liu and Z. Liu (2022). [4] Linearized single-scattering property database for hexagonal prism ice particles. Remote Sensing 14, 6138.


AS57-A013
Retrieval of Cloud Microphysical Properties from Himawari-8/AHI Infrared Channels and its Application in Surface Shortwave Downward Radiation Estimation in the Sunglint Region

Gegen TANA1, Xu RI2, Chong SHI3#+, Run MA2, Husi LETU2, Jian XU2, Jiancheng SHI2
1National Space Science Center, Chinese Academy of Sciences, 2Chinese Academy of Sciences, 3Aerospace Information Research Institute, Chinese Academy of Sciences

Satellite remote sensing of cloud property retrieval and shortwave downward radiation (SWDR) estimation is essential for global radiation budget and climate change studies. Sun glint areas remain a challenge for the existing cloud and SWDR algorithms based on the visible channel since surface specular reflection has a significant impact on satellite retrieval. In this study, a set of algorithms for cloud detection and cloud microphysical parameter estimation were developed using infrared multichannel data from the new generation geostationary satellite Himawari-8 based on the random forest method. The results indicated that the cloud retrieval algorithm exhibited better performance in the sun glint areas where the official Himawari-8 products (cloud detection and cloud optical thickness) were overestimated. We developed a new SWDR estimation algorithm combining the radiative transfer model and machine learning techniques by considering the cloud properties from the cloud retrieval algorithm. The results indicated that the SWDR and cloud radiative forcing derived by the new algorithm were more consistent with those of the well-known radiation products Cloud and the Earth’s Radiant Energy System than those estimated using the official-based cloud product, with decreases in the root mean square error of approximately 22% and 41%, respectively. The new algorithms effectively addressed sun glint contamination by providing more data coverage and exhibiting stable performance on a spatiotemporal scale.


Fri-04 Aug | 1:10 - 3:10 | MR323
AS47 - Global Precipitation Measurement and Future Missions

Session Chair(s): Yukari TAKAYABU, The University of Tokyo, George J. HUFFMAN, NASA Goddard Space Flight Center

AS47-A003
NASA GPM Status and Future Activities

George J. HUFFMAN1#+, Mircea GRECU2,1, Christian KUMMEROW3, Stephen LANG1, Adrian LOFTUS1, William OLSON4,1, Erich STOCKER1
1NASA Goddard Space Flight Center, 2Morgan State University, 3Colorado State University, 4University of Maryland, Baltimore County

The joint U.S.-Japan Global Precipitation Measurement (GPM) mission is approaching a decade of operations, and continues to pursue research, dataset production, and outreach related to precipitation. One key activity over the last year was the release of an improved “Version 07” of all GPM precipitation and latent heating products. This talk summarizes key improvements to the GPM products for which NASA has lead responsibility and provides some examples of the changes between Versions 06 and 07 in algorithm performance. One important operational change that affected Version 07 is that the scanning strategy for the Ka-band radar channel changed in May 2018; all products that depend on Ka were revised to accommodate this change. For example, in Version 07 the Goddard Profiling (GPROF) algorithm has implemented improvements in regions where orographic enhancement and suppression take place and where the surface is snowy/icy, and again covers radiometers reaching back to 1987. The Combined Radar Radiometer Algorithm (CORRA) now incorporates modified drop-size distribution constraints that substantially reduce bias. Revisions to the Convective-Stratiform Heating (CSH) algorithm employ new radiative transfer retrievals. Each algorithm was adjusted to ensure continuity for each product across the boundary in 2014 between the predecessor Tropical Rainfall Measuring Mission (TRMM) and the GPM Core Observatory. The U.S. Science Team’s Integrated Multi-satellitE Retrievals for GPM (IMERG) was upgraded to account for distortions in the probability density function of regional precipitation rates due to weighted averaging in the Kalman filter used for “morphing” the passive microwave data. The talk will conclude by considering major issues that require continued attention, including the use of machine learning algorithms, the operational challenge of swarms of “small”, perhaps short-lived satellites, and estimates of the remaining lifespan of the Core Observatory.


AS47-A008
Global Precipitation Measurement (GPM) Mission in Japan and Future Japanese Precipitation Measuring Mission (PMM)

Takuji KUBOTA1#+, Moeka YAMAJI1, Kosuke YAMAMOTO1, Nobuhiro TAKAHASHI2, Yukari TAKAYABU3
1Japan Aerospace Exploration Agency, 2Nagoya University, 3The University of Tokyo

The Japan Aerospace Exploration Agency (JAXA) has operated spaceborne precipitation radars since 1997 through Tropical Rainfall Measuring Mission (TRMM) Precipitation Radar (PR) and the Global Precipitation Measurement (GPM) Dual-Frequency Precipitation Radar (DPR). The GPM mission is an international collaboration to achieve highly accurate and highly frequent global precipitation observations. The GPM mission consists of the GPM Core Observatory jointly developed by U.S. and Japan and Constellation Satellites that carry microwave radiometers and provided by the GPM partner agencies. The GPM Core Observatory, launched on February 2014, carries the DPR by the JAXA and the National Institute of Information and Communications Technology (NICT). Japanese science community has discussed future precipitation observation mission from space based on the achievements from the TRMM and the GPM and expecting achievements from the Earth Clouds, Aerosols and Radiation Explorer (EarthCARE)and a mission of “Precipitation Measuring Mission (PMM)” was proposed. According to user requirements, the JAXA has studied a feasibility of a higher sensitivity precipitation radar with the doppler capability in the PMM. The JAXA has participated in NASA’s Atmosphere Observing System (AOS) mission Pre-Phase A activities. In January 2022, the PMM Pre-Project Team was established in the JAXA for the JAXA Spacecraft carrying the Ku-band Doppler Precipitation Radar with the displaced phase center antenna (DPCA) approach. As the Ku-band Radar enables us retrievals in heavy precipitation, it is expected to provide unique information, in particular, over vigorously convective regions. Observations of the precipitation vertical motion will contribute to improvements of microphysics schemes in weather models. This paper provides recent status of the GPM mission in Japan and an introduction of the future mission, PMM, studied in the JAXA.


AS47-A002
Early Results from IMERG V07

Jackson TAN1,2#+, George J. HUFFMAN2, David BOLVIN3, Eric NELKIN3, Robert JOYCE3
1University of Maryland, Baltimore County, 2NASA Goddard Space Flight Center, 3Science Systems and Applications, Inc.

The Integrated Multi-satellitE Retrievals for GPM (IMERG) product from the Global Precipitation Measurement (GPM) mission’s U.S. Science Team provides precipitation rate estimates at 0.1° every half-hour globally, with three Runs to cater to various applications with different latency requirements. With a reprocessing of the entire record spanning the TRMM and GPM eras, the latest version—IMERG V07—contains numerous algorithmic changes that are anticipated to improve the precipitation estimates. This presentation will show some early results from the IMERG V07 data. These results will quantify and demonstrate the expected improvements, not just from the individual changes in the algorithm but their combined effect on the final estimates. In particular, we will focus on the overestimation issue in V06, the longstanding problem of intersensor differences, and the biased distribution of morphed estimates, which has implications for the estimations of extremes. Above all, an evaluation against ground reference will quantify the difference in overall performance between V06 and V07. As well, we will highlight aspects of IMERG that have room for further improvement in V08. These early results on IMERG V07 demonstrate the status of our goal of providing the community with a long record of reliable high-resolution precipitation observations.


AS47-A007
Validation of the GPM/DPR Instantaneous Rain Rate Estimates by Using High-temporal-resolution Rain Gauge Dataset

Shinta SETO1#+, Nobuyuki UTSUMI2
1Nagasaki University, 2Kyoto University of Advanced Science

The precipitation rate estimates by the Dual-frequency Precipitation Radar (DPR) on the core satellite of the Global Precipitation Measurement mission are validated by means of every-1-minute and every-10-second rain gauge data of the Japan Meteorological Agency. As the resolution of tipping bucket is 0.5 mm, a simple calculation converts 1-minute rain amount to rain rate with a step of 30 mm/h, which is not accurate enough for the validation purpose. Every-10-second rain gauge data store not only rain amount but the time of tipping in second. Assuming that the rain rate is constant between two successive tipping, rain rates are estimated for every 1 second and are averaged for every 1 minute. It is called gauge-based rain rate data. Next, the gauge-based rain rate data are compared with eXtended Radar Information Network (XRAIN) dataset for July 2018. Correlation coefficient between the gauge-based rain rate data and XRAIN rain rate data is 0.791 at Nagasaki, while it is 0.585 if the rain rate is simply calculated from 1-minute rain amount. Finally, the gauge-based rain rate data are used for the validation of DPR precipitation rate estimates. Surface precipitation rate estimates (precipRateESurface) of the KuPR algorithm and the Dual-frequency algorithm of DPR Version 07 are validated with the gauge-based rain rate data for the whole year of 2019. The correlation coefficients are 0.804 and 0.832 for KuPR and Dual-frequency algorithms respectively, when the time lag is set to 4 minutes considering the height difference between the clutter free bottom and the land surface. For DPR algorithms Version 06, they are 0.573 (KuPR algorithm) and 0.570 (Dual-frequency algorithm). The results suggest the advantages of the Dual-frequency algorithm and the latest version against the KuPR algorithm and the previous version respectively.


AS47-A006
Advances and Applications of Satellite Data Assimilation of Clouds, Precipitation, and the Ocean

Takemasa MIYOSHI1,2#+, Shun OHISHI1, Jianyu LIANG1, Rakesh Teja KONDURU1, Shigenori OTSUKA1, Shunji KOTSUKI3, Koji TERASAKI4, Atsushi OKAZAKI5, Hirofumi TOMITA6, Ying-Wen CHEN7, Kaya KANEMARU8, Masaki SATOH7, Hisashi YASHIRO9, Kozo OKAMOTO10, Eugenia KALNAY2, Takuji KUBOTA11, Misako KACHI11
1RIKEN Center for Computational Science, 2University of Maryland, 3Chiba University, 4Meteorological Research Institute, 5Hirosaki University, 6RIKEN Advanced Institute for Computational Science, 7The University of Tokyo, 8National Institute of Information and Communications Technology, 9National Institute for Environmental Studies, 10Japan Meteorological Agency, 11Japan Aerospace Exploration Agency

This presentation summarizes progress of a research project started in FY2022. This research aims to advance data assimilation, analysis and prediction of clouds, precipitation and the ocean, based on the achievements from the previous projects since 2013, i.e., “ensemble data assimilation of TRMM/GPM precipitation observations” (2013-2016), “advancing data assimilation of GPM observations” (2016-2019), “advancing precipitation prediction algorithm by data assimilation of GPM observations” (2019-2022), “development of a satellite ocean data assimilation system with the JAXA Supercomputer System Generation 2” (2017-2020), and “satellite data assimilation using an ocean model” (2020-2022). We developed the global atmospheric ensemble data assimilation system called NICAM-LETKF, where NICAM stands for the Nonhydrostatic ICosahedral Atmospheric Model and the LETKF for the Local Ensemble Transform Kalman Filter. We also developed a precipitation nowcasting system called GSMaP RIKEN Nowcast (GSMaP_RNC) using the satellite-analyzed Global Mapping of Precipitation (GSMaP) dataset. We developed real-time precipitation prediction system by seamlessly merging data from the NICAM-LETKF numerical weather prediction and GSMaP_RNC and have been operating it continuously for public data dissemination. In addition, we have been operating JAXA’s real-time atmospheric analysis system called NEXRA (NICAM-LETKF JAXA Research Analysis) and have been disseminating real-time level-4 analysis products using satellite data, with proven data quality by analyzing past high-impact weather events such as typhoons and heavy rainfalls. Moreover, we implemented the LETKF with an ocean model called sbPOM and developed daily-update ocean data assimilation system using dense and frequent SST data from the Himawari-8 geostationary satellite. This research will integrate these atmospheric and oceanic data assimilation projects with significant extension. Through the research, we aim to deepen our integrated understanding of the earth system on clouds, precipitation and the ocean and to advance analysis and prediction, and their real-life applications.


AS47-A012
Event-based Extreme Precipitation Characteristics in the Tropics

Yaping ZHOU1#+, Kuan-Man XU2
1University of Maryland, Baltimore County, 2NASA Langley Research Center

Extreme precipitation (EP) has become increasingly frequent and is causing more devastating impacts on society in recent years. EP is traditionally measured by the maximum or threshold-exceeding gridded precipitation of a given duration. We have developed an extreme precipitation event (EPE) algorithm that tracks entire precipitation life cycle across space and time, which enables us to characterize properties of the entire EPE, such as duration (from sub-daily to multi-day), areal coverage, and total rain volume of the event. These EPE characteristics are critical in understanding precipitation development and their interaction with large-scale meteorology, in addition, providing more comprehensive matrix for disaster management. This study examines the EPE characteristics from the tropics derived from high-resolution Integrated Multi-satellitE Retrievals fro GPM (IMERG) product. The difference between EPE characteristics between tropical land and ocean will be discussed. Large-scale meteorological control as well as convective aggregation will be studied on the impact of EPE characteristics in tropics.


AS47-A014
Intercomparisons of the Latest Precipitation Estimates from Satellite, Reanalysis and Merged Products Over the Alaska

Yang SONG1,2#+, Ali BEHRANGI2, Bin YONG1,3
1Hohai University, 2University of Arizona, 3State Key Laboratory of Hydrology-Water Resources and Hydraulic Engineering

Accurate precipitation retrieval is challenging in high-latitudes due to difficulties in collecting sufficient ground measurements. Satellite products provide global coverage that complement scattered surface observations. This study intercompares precipitation estimates over all of Alaska from the most recent versions of multiple precipitation products, including satellite-based infrared (AIRS), passive microwave (PMW; SSMIS, METOPB, NOAA19, AMSR2, ATMS and GMI in V05 and V07), radar (GPM DPR in V06 and V07), and combined sensor (DPR/GMI in V06 and V07); reanalysis (NCEP Stage IV, ERA5, MERRA2) and merged products (GPCP V2.3 and V3.2). Results show that the mean annual precipitation increases from the North Slope (1.0mm/day) to the Gulf of Alaska (10.0mm/day). Performance indicators of the Correlation Coefficient (CC), the Root Mean Square Error (RMSE), the Relative Bias (RB) and the Heidke Skill Score (HSS) show that for mean annual precipitation: ERA5 and MERRA2, PMW, AIRS and GPCP (CC: 0.40-0.90) outperform radar and combined products (CC: 0.10-0.50) over the mountainous and snow-covered regions. Underestimations (RB: 0.30) and overestimations (RB: 1.50-3.00) are found in old and new versions respectively in PMW, radar and combined in comparison to Stage IV. Similar upward trend of HSS is identified when precipitation intensity ranges from 0 to 6.0mm/day, with ERA5 showing the highest value. CC, RMSE and RB range from 0.30-0.80, 7.50-16.50mm/day and 0.25-1.10 for rain; 0.15-0.70, 6.00-13.50mm/day and 0.25-1.25 for mixed phase; and 0.10-0.65, <5.00mm/day and 0.20-1.40 for snow on snow-covered surface. Radar and combined products in V07 presented better performance in mixed phase than in V06 over snow-free surface. However, it is still unclear how the radar behaviors over this region and further analysis are required. The study highlights the performance of different precipitation products over the cold regions of Alaska, which may provide guidance for future high-latitude precipitation development.


Fri-04 Aug | 1:10 - 3:10 | MR327
AS22 - Understanding and Modeling Climate Impacts of Anthropogenic Land Use Change

Session Chair(s): Eun-Soon IM, HKUST, Min-Hui LO, National Taiwan University

AS22-A001 | Invited
Urban Heat and Mitigation in the Kansas City Metropolitan Area: An Integrated Regional Modeling and Heat Mapping Campaign Study

Fengpeng SUN#+, Kyle REED
University of Missouri - Kansas City

An urban heat island (UHI) is a phenomenon where the temperatures within cities are greater than those of surrounding rural and suburban areas due to human activity and the physical properties of urban land surfaces. It is one aspect of anthropogenic impacts on regional climate due to land use change. One method that has been investigated as a way to mitigate the UHI phenomenon is to increase the surface albedo in cities, which reflects a greater amount of solar radiation away from these surfaces compared to conventional materials (e.g., dark asphalt shingles). In this study, we utilize the Weather Research and Forecasting (WRF) model to investigate the UHI under different scenarios during a heat wave event in the Kansas City metropolitan area (KCMA). Two cool roof simulations are implemented to determine the effectiveness of this mitigation strategy on reducing temperatures within the KCMA. The first scenario represents “newly installed” cool roofs with an albedo of 0.8 and the second with “aged” cool roofs with an albedo of 0.5. Results indicate that cool roof materials were able to mitigate the surface UHI effect by up to 0.64 °C during the evening, causing the onset of the UHI effect to be delayed until later in the day. The cooling effects of cool roofs on the surface skin temperature have been shown more evident. Cool roofs were also shown to have important impacts on the surface energy balance, affecting both sensible and ground storage heat fluxes, and the planetary boundary layer. Leveraged by the numerical modeling studies, an urban heat mapping campaign in Kansas City was launched to further study the urban heat distribution and better understand the adverse UHI effect.


AS22-A002 | Invited
Combinatory Impact of Soil Texture and Land Use/cover Change on Hydroclimate Modeling Over Central Taiwan

Chia-Jeng CHEN#+, Min-Hung CHI
National Chung Hsing University

Previous studies have revealed the individual impact of the difference in soil texture or land use/cover change (LUCC) on the simulation of land-atmosphere interactions in Taiwan; however, an assessment of the “combinatory” impact is still pending. We thus aim at designing a numerical modeling experiment to assess such combinatory impact on regional hydroclimate. We acquire and adopt Taiwan’s survey-based soil data (stationary) as well as land use data (in 1995 and 2015) as different land surface conditions to separately drive the Weather Research and Forecasting (WRF) model, coupled with the WRF Hydrological modeling system (WRF-Hydro). For each combination of land surface conditions (i.e., default soil or Taiwan’s soil plus land use in 1995 or 2015), we conduct a simulation of 10 selected rainy events under weak synoptic forcings in July and August over the past 20 years, and then derive the mean fields of assorted atmospheric and surface variables (e.g., sensible and latent heat, temperature, specific humidity, precipitation, and soil moisture) for comparison. In addition to addressing whether the difference in soil texture or LUCC can yield more significant impact on hydroclimate modeling, we will compare the relative importance of land surface conditions with the completeness of terrestrial hydrological processes (i.e., coupling with WRF-Hydro or not) in the modeling environment.


AS22-A008
Forestation Induced Greening in South China Favours Carbon Neutrality and Ozone Air Pollution Abatement

Zehui LIU+, Lin ZHANG#
Peking University

Forestation-induced greening in South China has been known to increase carbon sinks and help carbon neutrality, while how forestation would affect ozone air quality is still unknown due to the complexity of atmospheric chemistry-biosphere interactions. Here we use an improved regional atmospheric chemistry model coupled with a forest canopy turbulence scheme to quantify the effects of past and future greening in South China on ozone air quality. Model results are evaluated by measurements of near-surface ozone vertical gradient at a forest station. We show that the 2005-2019 greening effects on ozone dry deposition and vertical transport far outweigh biogenic volatile organic compounds emissions, alleviating mean surface maximum daily 8-hour average (MDA8) ozone over South China by 1.4 ppb in the growing season. In addition, greening also assuages ozone damage to vegetation over South China 15%-41% depending on different vegetation ozone metrics. Future forestation could further boost Chinses forest carbon storage by 4.3 Pg C and abate 1.4 ppb of ozone pollution over South China by 2050. Our findings indicate that forestation could benefit both carbon neutrality and ozone pollution, and highlight the pivotal role of interaction between the biosphere and air pollution.


AS22-A012
Growing Food and Biomass Crops on Arable and Marginal Lands Affects Regional Climate and Feedback Processes

Xinzhong LIANG1#+, Chao SUN1, Yufeng HE2
1University of Maryland, 2University of Illinois

Climate change and population growth at alarming rates are crippling global food, energy, and water (FEW) systems, projected to increase global demand for food by 70%, water by 55%, and energy by 50% in 2050. While the FEW systems are already under stress in meeting the current need, the projected doubling or more demand is a grand challenge facing humanity. A FEW modeling framework that couples regional climate-agrohydrosystems and bio-hydro-economic systems (MFEW) has been developed to gain new insights on climate adaptation/mitigation, land use strategies, food/bioenergy productions, and sustainability managements that may address the impeding challenge. Here we conduct MFEW experiments to evaluate feedbacks between climate and agricultural land use change, focusing on scenarios that expand production of Miscanthus and Energycane onto marginal land, together with the existing staple crops on arable land, in and across the Belts. Initial analysis shows that growing biomass crops on marginal land would improve climatic conditions for production of both these perennial grasses and the arable food/fodder crops currently cultivated across the heartland of U.S. agriculture. It would also provide a significant offset to regional climate changes expected with global warming, including cooler temperature, more precipitation, and less vapor pressure deficit. This marginal land use could not only offset carbon emissions and provide feedstock for renewable products, but also ameliorate adverse climate change impacts on the food production in the heartland. As a result, it represents a promising mitigation strategy to sustain U.S. agriculture. This talk will elaborate understanding of the physical processes and underlying mechanisms on the FEW system teleconnected impacts and feedbacks under the present and future climate conditions.


AS22-A014
Quantifying the Contributions of Vegetation Restoration and Climate Change to Energy Budget in the Loess Plateau of China

Linjing QIU#+
Xi'an Jiaotong University

Anthropogenic land cover change (ALCC) can modify energy exchanges and further alter the regional climate. Due to the complexity of land-atmosphere energy exchange processes and limited observation networks, the influence of ALCC on the energy balance remains unclear. The Loess Plateau (LP) of China has experienced evident land surface change due to the implementation of the Grain for Green vegetation restoration program. Under this program, a large amount of cropland has been converted to grassland and forestland, which will inevitably result in surface energy balance changes. However, due to their complexity and lack of in situ observations, it is a challenge to quantify the spatial-temporal dynamics of energy balance changes associated with the GFGP. Here we first investigated the changes in surface energy partitioning in the LP region during the period of 1980–2018. Then we modified the land cover characteristics for each plant functional type in the LP based on multiple sources of observations to improve the representations of historical vegetation in the model. Finally, we performed a series of sensitivity simulation experiments to quantitatively identify the contribution of vegetation restoration and climate change to energy balance component changes.


AS22-A007
Investigating the Climate's Reaction to Varying Levels of Deforestation in the Maritime Continent

Chun-Hung LI#+, Min-Hui LO
National Taiwan University

This study aimed to understand the climate's response to varying levels of deforestation in the MC. Using the Community Earth System Model (CESM), we simulated five cases of deforestation with different magnitudes and investigated the nonlinear effects on mean state climate conditions. Results showed that surface temperature and sensible heat flux increased with increasing deforestation while latent heat fluxes decreased. Precipitation patterns were also found to have nonlinear characteristics, with a slight increase initially, followed by a more significant increase as deforestation progressed. However, nonlinearities may vary depending on the distribution and terrain of the islands. For example, Borneo showed a tipping point, while the Guinea region did not. The study also explored the alteration of land-atmosphere interactions after deforestation using the concept of critical soil moisture and segmented regression. Results indicated that the interactions changed and soil moisture feedback may play a role in extreme temperature events.


AS22-A011
Quantifying the Regional Climate Response to Groundwater-fed Irrigation in North China Plain Based on WRF Simulations

Yuwen FAN1+, Eun-Soon IM2#, Min-Hui LO3
1The Hong Kong University of Science and Technology, 2HKUST, 3National Taiwan University

Irrigation is a common anthropogenic activity that changes land-use and land-cover, which leads to considerable alteration in land-atmosphere interaction and hydrological cycle. As one of the most intensively irrigated regions in the world, agriculture in the North China Plain (NCP) heavily depends on groundwater due to its deficit precipitation and scarce water. Irrigation is already claimed to have a notable climate impact in the NCP. Moreover, groundwater-dependent irrigation can reduce water storage, but it can also be affected by groundwater exploitation because the declining soil water may exaggerate the irrigation, forming a positive feedback loop. The groundwater depletion is clearly identified from the observation and satellite data, but it is not well implemented with irrigation processes in the climate models. For example, the current Noah-MP in WRF cannot represent the potential feedback loop between groundwater storage and irrigation usage, since the groundwater module is not directly connected with the irrigation scheme. Also, the crop module is not compatible with the dynamic vegetation scheme for non-crop plants. Thus, the current land scheme is inapplicable to a large-extent agricultural area that contains both cropland and non-cropland, such as the NCP. This study aims to simulate groundwater-fed irrigation in the NCP and its surrounding area in eastern China by integrating the existing vegetation, crop, irrigation, and groundwater modules in Noah-MP. The modified model should be able to (1) generate seasonal dynamic patterns of crop growth under different soil conditions, (2) calculate the irrigation amount with varied soil moisture and crop growth, and (3) simulate the soil-groundwater interaction considering the irrigation-induced extraction. The results will help us better comprehend the interactions between the atmosphere, land surface, and subsurface that can modulate climate patterns both locally and remotely. This research was supported by project GRF16309719 and funded by the Research Grants Council of Hong Kong.


Fri-04 Aug | 1:10 - 3:10 | MR328
AS26 - Tropical Polar Teleconnections

Session Chair(s): Seong-Joong KIM, Korea Polar Research Institute, Sheeba Nettukandy CHENOLI, University of Malaya

AS26-A004
A Distinct Impact of Multi-year La Niña on Antarctic Sea Ice Concentration

Jin-Yi YU#+, Tingting ZHU
University of California, Irvine

La Niña events are characterized by abnormal cooling of sea surface water over the tropical Pacific Ocean that typically last for one year. Recently, more La Niña events can persist more than two years. In this study, we analyze a long-term CESM1 simulation to show that multi-year La Niña events produce a different impact on Antarctic sea ice concentration (SIC) from the single-year La Niña. We find that the typical SIC impact produced by single-year La Niñas appears only during the second austral winter of the multi-year La Niña, but is shifted westward during its first winter to exhibit a distinct tripolar pattern with anomaly centers over the Ross, Bellingshausen, Weddle Seas. The shifted impact pattern is caused by the different atmospheric wave trains excited by the different Indian Ocean conditions between the first and second winters of the multi-year events. The distinct impact and impact mechanism revealed from the climate model can be verified in the observations. Four out of the six multi-year La Niña events observed during 1979-2020 exhibit this zonally-shifting SIC anomaly pattern from its first to second winters. This study suggests that the increasing occurrence of multi-year La Niña events may affect Antarctic sea ice patterns in a new way.


AS26-A006
Interdecadal Changes of Dominant Modes of Antarctic Sea Ice Variability in the Austral Warm Season and Associated Sea-air-ice Interactions

Qigang WU#+
Fudan University

The “Antarctic Dipole” (ADP), characterized by an out-of-phase relationship between sea ice anomalies in the Pacific and Atlantic sectors of the Antarctic, is the dominant mode of Antarctic sea ice concentration (SIC) variability and is strongly affected by tropical El Niño–Southern Oscillation (ENSO) variations. Since the 2000s, the ENSO regime and associated tropical-Antarctic connections have significantly changed with more central Pacific El Niño events occurring. This study shows that the first leading empirical orthogonal function (EOF1) mode of the Antarctic SIC from austral summer to early winter shifted from the ADP during 1979-1999 to an in-phase relationship between SIC anomalies in the Ross and Weddell Seas during 2000-2021, accompanied by interdecadal changes of sea surface temperature (SST) and atmospheric circulations. During 1979-1999, the ADP was triggered by ENSO forcing and associated Pacific-South American (PSA) atmospheric forcing, but also forced by SST anomalies over the Tasman Sea and the tropical-subtropical South Atlantic. During 2000-2021, the EOF1 mode was associated with Southern Annular Mode (SAM)-like and zonal wave 3 (ZW3)-like atmospheric forcing, and forced by SST anomalies over the subtropical South Pacific and high-latitude South Atlantic. The EOF1 modes of the Antarctic SIC from austral summer to autumn were significantly related to the autumn-early winter negative SAM-like atmospheric circulation during 1979-1999, but weakly related to a zonal wave 2 pattern around 60°S during 2000-2021. Our results indicate that an interdecadal shift of dominant modes of Antarctic sea ice and associated sea-air-ice interactions occurred around 2000 in the austral warm season.


AS26-A001
The Influence of Pacific‑north American Teleconnection on the North Pacific SST Anomalies in Wintertime Under the Global Warming

Zheng CHEN#+
Ocean University of China

The impact of the enhancing Pacific-North American teleconnection (PNA) on the intensity of the first mode of SST anomalies (SSTa) in wintertime North Pacific [known as the Pacific decadal oscillation (PDO)-like SST pattern] under global warming is studied using reanalysis datasets and 12 selected CMIP5 models. The robust observational result of the PNA one month ahead of the PDO shows that the PNA has a great effect on the PDO-like SSTa. The intensities of PNA and PDO are defined with elimination of the ENSO signals to evaluate the direct impact of PNA on the PDO in the North Pacific under global warming. By comparing RCP8.5 and historical scenario of selected multi-models (PNA enhanced models), future projection illustrates that the PDO intensity will intensify 2.2 times its internal variability. Approximately 67% of the increase in PDO variations is contributed by the PNA-induced SSTa in the future warming scenario of multi-models ensemble mean. Models with stronger intensification of PNA variability tends to have larger magnitude of SSTa response in the North Pacific, which has more contributions to the enhancement of PDO intensity change in a warmer climate. This may shed some light on the projection of PDO variability and the relative role of PNA forcing under the global warming.


AS26-A005
Climatic Effects of the Indian Ocean Tripole on the Western United States in Boreal Summer

Yazhou ZHANG#+
Ocean University of China

The Indian Ocean tripole (IOT) is an independent mode of ocean–atmosphere circulation centered on the tropical Indian Ocean. This study explores the physical mechanisms of the IOT affecting the western United States climate variation during the boreal summer. We find that the IOT is significantly correlated with both western United States summer surface temperature and precipitation anomalies. During positive IOT events, the westerly wind anomalies over the northern Indian Ocean are intensified by two cross-equator airflows over the tropical eastern Indian Ocean and the east coast of Africa. The resulting convergence of air over the northern Bay of Bengal–Indochina Peninsula–northern South China Sea (NBB–IP–NSCS) region (80°–125°E, 15°–25°N) exacerbates the surplus precipitation there. Serving as a heat source, these NBB–IP–NSCS precipitation anomalies can excite a circum-global teleconnection-like (CGT–like) pattern that propagates eastward from west-central Asia towards North America along the Asia subtropical westerly jet, further influencing local circulation anomalies. Development of strong anticyclonic circulation over the western United States enhances descending motion and divergence there, resulting in negative precipitation anomalies. This circulation anomaly also induces the diabatic heating anomalies through allowing more solar radiation to reach the ground surface, further increasing the surface temperature anomalies. Meanwhile, the increased tropospheric temperature also raises local surface temperatures by modulating the adiabatic air expansion and compression. Ultimately, the CGT-like pattern associated with NBB–IP–NSCS precipitation anomalies sets up an atmospheric bridge by which the IOT can impact summer climate in the western United States.


AS26-A010
North American Extreme Winter Weather and the Polar Vortex

Muyin WANG1,2#+
1University of Washington, 2PMEL/NOAA

Extreme cold-air outbreaks (CAOs) during winter in North America can cause huge damages in society’s infrastructure and people’s daily life. A strong link exists between stratospheric variability and anomalous weather patterns at the earth’s surface. Specifically, during extreme variability of the Arctic polar weak vortex event, anomalies can descend from the upper stratosphere to the surface on time scales of weeks. Subsequently, the outbreak of cold-air events has been noted in high northern latitudes. In this study we document the recently observed extreme cold events and its connection with Polar Vortex strength and displacement. Because of the importance of stratosphere–troposphere coupling for seasonal climate predictability, identifying the type of stratospheric variability to capture the correct surface response will be necessary.


AS26-A007
The Mechanism Linking the Variability of the Antarctic Sea Ice Extent to Indian Summer Monsoon Rainfall

Sheeba Nettukandy CHENOLI1#+, Azizan Abu SAMAH1, Seong-Joong KIM2,3, Nuncio MURUKESH4,5
1University of Malaya, 2Korea Polar Research Institute, 3University of Science and Technology, 4National Centre for Polar and Ocean Research, 5Ministry of Earth Sciences, Government of India

The study investigates the mechanism of teleconnection between the variability of sea ice extent (SIE) in the Indian Ocean sector of the Southern Ocean and the variability of Indian summer monsoon rainfall. We utilized reanalysis, satellite, and in-situ observation data, from 1979 to 2013. The empirical orthogonal function (EOF) and correlation analysis show that the first and third modes of principal component (PC1 and PC3) of SIE in the Indian Ocean sector during April–May–June (AMJ) are significantly correlated with the second mode of principal component (PC2) of Indian summer monsoon rainfall. The reanalysis data revealed that the changes in the SIE in the Indian Ocean sector excite meridional wave train responses along the Indian Ocean for both principal component modes. Positive (negative) SIE anomalies based on first and third EOFs (EOF1 and EOF3) contribute to the strengthening (weakening) of the Polar, Ferrel, and Hadley cells, inducing stronger (weaker) convective activity over the Indian latitudes. The stronger (weaker) convective activity over the Indian region leads to more (less) rainfall over the region during high (low) ice phase years. Furthermore, a stronger (weaker) polar jet during the high (low) ice phase is also noted.


Fri-04 Aug | 1:10 - 3:10 | MR329
AS34 - Climate Drivers of Rainfall Variability Over the Maritime Continent

Session Chair(s): Muhammad Eeqmal HASSIM, Centre for Climate Research Singapore, Hui SU, The Hong Kong University of Science and Technology

AS34-A004
Shipborne Doppler Radar Observations of Daily and Subdaily Wind and Divergence Variations Off the Southwestern Coast of Sumatra

Biao GENG#+
Japan Agency for Marine-Earth Science and Technology

This study investigated the daily cycle of the wind and divergence fields off the southwestern coast of Sumatra for the period from 0000 UTC November 24 to 0000 UTC December 13, 2015. Doppler radar data obtained aboard the research vessel Mirai during the field campaign of the Years of the Maritime Continent (YMC) pilot study (Pre-YMC) were used. The observed daily cycles of the wind and divergence fields consisted of diurnal, semidiurnal, and short-term variations. Diurnal wind variation was characterized by deep and three-dimensional circulation. There was an approximate phase locking of the semidiurnal variation to the diurnal variation, both in the wind and divergence fields. The short-term wind variation occurred at a time scale of ~1–3 h, and this pattern was associated with density currents or mesoscale gravity waves. Our results suggest that diurnal and semidiurnal wind variations dominate the daily evolution of precipitation, whereas density currents and mesoscale gravity waves control offshore propagation. It appears that the daily precipitation cycle is modulated by multiple timescale wind variabilities of less than a day, which is also responsible for the development of strong nocturnal convection off the southwestern coast of Sumatra.


AS34-A001
Modelling the Climatology of Tropical Islands of Different Sizes Using the Weak Temperature Gradient Approximation

Nathanael WONG#+, Zhiming KUANG
Harvard University

The climatology of small tropical islands has always been difficult to reproduce in models as high spatial resolutions that have high computational costs are necessary to resolve them. In this study, we bypass this computational cost limitation by coupling small-domain model runs to a large-scale reference climatology using the Weak Temperature Gradient (WTG) approximation. We believe that adjusting the strength of the WTG implementation is an analogue to modelling the climatology of tropical islands of different sizes. This is best shown in the diurnal cycle of precipitation, which tends to initiate and peak earlier in the day the stronger the WTG implementation (i.e. the smaller the island size, or closer to the coast/ocean). We also compare our model results to GPM IMERG observations of the offshore - and inland -propagation of precipitation, and believe that our results encourage further study.


AS34-A007
Physical Mechanisms of Offshore Propagation of Convection in the Maritime Continent

Simon PEATMAN1#+, Cathryn BIRCH1, Juliane SCHWENDIKE1, John MARSHAM1, Chris DEARDEN1, Stuart WEBSTER2, Emma HOWARD3, Steve WOOLNOUGH4, Ryan NEELY1, Adrian MATTHEWS5
1University of Leeds, 2Met Office, 3Bureau of Meteorology, 4University of Reading, 5University of East Anglia

The spatio-temporal variability of Maritime Continent convection, its organisation and the offshore propagation of diurnal convection overnight all depend on many factors including the topography of island coastlines and mountains, and large-scale weather phenomena such as the MJO, ENSO and equatorial waves. Here we consider the physical mechanisms of offshore propagation and how they relate to large-scale forcings. The literature proposes numerous mechanisms for this propagation but a consensus remains elusive. Greater understanding is needed to reduce the considerable model biases which exist in the Maritime Continent region. Proposed physical mechanisms of the offshore propagation include convective triggering due to gravity waves, or low-level convergence between environmental winds and either the offshore land breeze or convective cold pools. Using convection-permitting simulations of selected case studies of convection propagating offshore from Sumatra, we find a squall line propagating slowly (~3 m s-1) overnight due to low-level convergence between the land breeze and the environmental winds, within around 150–300 km of the coast. This is reinforced by cold pools, which we diagnose using model tracers. Gravity waves play a role further from the coast, triggering localized (non-organized) convection which does not itself propagate, but can appear as faster (~16 m s-1) propagation along wave trajectories when compositing the diurnal cycle over many days. The investigation is extended to other coastlines in the Maritime Continent, using convection-permitting simulations for 900 days during boreal winters, to demonstrate broader evidence for these physical mechanisms; to understand why the offshore propagation occurs on some days but not others; and to show how the strength, timing and causes of offshore propagation vary for different Maritime Continent islands, caused by variations in the large-scale winds due to large-scale climate forcings, as well as the shape of the orography and the topography of coastlines.


AS34-A003
Relationship Between Convectively Coupled Equatorial Waves and Sumatra Squalls Affecting Singapore

Hanh NGUYEN1#+, Matthew WHEELER1, Muhammad Eeqmal HASSIM2,3, Sandeep SAHANY2, Xin Rong CHUA2, Aurel MOISE2
1Bureau of Meteorology, 2Centre for Climate Research Singapore, 3Meteorological Service Singapore

The weather and climate of the Maritime Continent, including Singapore, is influenced by a wide range of tropical climate drivers including the El-Niño Southern Oscillation (ENSO), the Indian Ocean Dipole (IOD), the Madden-Julian Oscillation (MJO), and equatorial wave activity. In Singapore the rainfall pattern is often characterised by episodes of short strong rainfall bursts which are dominated by mesoscale convective systems such as Sumatra squall lines, and often lead to local flash floods and strong wind bursts. Here we investigate the impact of equatorial tropical waves on the Sumatra squalls over Singapore. The Precipitation Estimation from Remotely Sensed Information using Artificial Neural Networks (PERSIANN) high-resolution precipitation dataset (0.04o horizontal x daily resolution) spanning from 1983-2020 is used to extract equatorial waves by filtering for the Wheeler and Kiladis (1999) wavenumber-frequency domains. Then, archives of the Sumatra squalls dataset will be assessed against the passage of equatorial waves over the region in order to identify their potential co-occurrence and interaction.


AS34-A009
Future Projections of Cold Surges Over the Maritime Continent from CMIP6 GCMs

Xin Rong CHUA1#+, Sandeep SAHANY1, Aurel MOISE1, Chen CHEN1, Muhammad Eeqmal HASSIM1,2, Gerald LIM2, Venkatraman PRASANNA2
1Centre for Climate Research Singapore, 2Meteorological Service Singapore

Cold surges are a key synoptic phenomenon over the Maritime Continent during boreal winter, and can contribute significantly to extreme rainfall events. It is therefore important to know how the behaviour of surge winds and rainfall might change in a warmer climate. Historical and SSP585 simulations from the CMIP6 archive do not indicate much change in surge frequency. However, there is a robust increase in surge rainfall over parts of Sumatra and Borneo under warming, alongside a slight weakening of surge winds over the South China Sea. This suggests that the increase in surge rainfall could be thermodynamically driven.


AS34-A005
The Indo-Pacific Warm Pool Expansion May Be Slower Than Expected Under Greenhouse Warming – From the View of its Role in the Climate System

Jeremy Cheuk-Hin LEUNG1+, Banglin ZHANG2#, Qiuying GAN3, Lei WANG3, Zeng-Zhen HU4
1Guangzhou Institute of Tropical and Marine Meteorology/Guangdong Provincial Key Laboratory of Regional Numerical Weather Prediction, China Meteorological Administration, 2China Meteorological Administration, 3Guangdong Ocean University, 4National Oceanic and Atmospheric Administration

The Indo-Pacific warm pool (IPWP) acts as the heat engine of global climate system by consistently supporting and maintaining atmospheric deep convection throughout the year. For this reason, researchers have been defining the IPWP as the region with sea surface temperature (SST) exceeding a pre-condition necessary to favor deep convection (e.g., 28°C). Based on this definition, recent studies reported that the IPWP has expanded quickly due to anthropogenic greenhouse warming and will further expand in the future. However, these conclusions were obtained by neglecting the change in SST threshold favoring deep convection (σconv) under climate change, although this has been documented a decade ago. In other words, the widely-used traditional definition of IPWP may not hold under global warming. In this study, we show that the estimation of IPWP expansion is sensitive to the σconv change. The expansion speed of the traditionally defined IPWP (denoted as oceanic warm pool, OWP28, defined by a static σconv=28°C) overestimates the region that favors deep convection (denoted as deep convection favoring pool, DCFP, defined by considering the time-varied σconv). Because of the long-term increase in σconv, the DCFP expands slowly, at a rate 2.6 times smaller than the OWP28 from 1979 to 2020. The difference reaches 12–27 times from 2015–2100 under different emission scenarios, based on 20 CMIP6 models’ simulations. While the OWP28 expands to the eastern Pacific, the DCFP will not expand to a large extent, and will remain within the Indian Ocean and western Pacific Ocean regardless of the anthropogenic emission level. Given the IPWP’s role in the global climate system, this study emphasizes the necessity of considering the response of the relationship between deep convection and SST to climate change when studying the long-term variability of the IPWP and its impacts on the climate system.


AS34-A008
Linking Rainfall Changes Over Maritime Continent to Walker Circulation Shifts Under Warming

Chen CHEN1#+, Sandeep SAHANY1, Aurel MOISE1, Xin Rong CHUA1, Muhammad Eeqmal HASSIM1,2, Gerald LIM2, Venkatraman PRASANNA2
1Centre for Climate Research Singapore, 2Meteorological Service Singapore

The Maritime Continent (MC), located in the heart of the Indo-Pacific warm pool, is a small yet heavily populated region with a fast-growing economy. The state-of-art CMIP6 models disagree on the sign of change in the MC summer rainfall, which could have huge socio-economic impacts. Here we trace back the reasons for the diverging projections across models. We show that rainfall changes over the Maritime Continent are closely governed by changes in the Walker Circulation. Models projecting a smaller eastward shift of the Indo-Pacific rainfall center are models projecting a smaller rainfall increase over the Tropical Pacific (TP) but a wetter MC. On the other hand, Models projecting a larger eastward shift of the Indo-Pacific rainfall center are models projecting a larger rainfall increase over the TP but a drier MC. Moreover, models predicting a larger rainfall shift are models showing a larger reduction in the zonal sea surface temperature gradient across the TP with a larger warming sensitivity. These results suggest that narrowing down the uncertainty in the MC rainfall projection relies on a better constraint and understanding of the modeled circulation changes.


Fri-04 Aug | 1:10 - 3:10 | MR331
AS17 - Application of Satellite Data to Weather, Climate and Environmental Study

Session Chair(s): Min MIN, Sun Yat-sen University, Feng ZHANG, Fudan University

AS17-A004 | Invited
Extension of the Global All-sky Infrared Radiance Assimilation of Himawari

Kozo OKAMOTO#+, Toshiyuki ISHIBASHI, Izumi OKABE
Japan Meteorological Agency

Infrared all-sky radiance (ASR) assimilation is believed to be more beneficial than traditional clear-sky radiance (CSR) assimilation because it enhances the observation coverage, reduces dry bias due to a sampling error, and extracts more observation information in meteorologically sensitive regions. Despite many challenges, we successfully developed ASR assimilation for Himawari-8 in a global data assimilation system. Essential assimilation procedures are cloud-dependent quality control (QC), bias correction (BC), and observation error (OE) models. The ASR assimilation brought better forecast skills than CSR assimilation by modestly utilizing cloud-affected radiances in low and thin ice cloud conditions in addition to CSRs. We also separately assessed the impacts of several settings of the assimilation procedures using data assimilation cycle experiments. Important findings are as follows: (1) Single-band ASR assimilation that was often employed in previous studies is inferior to multiband CSR assimilation, not to mention multi-band ASR assimilation (2) OE correlation and cloud-dependent OE standard deviation are important, but cloud-dependency of OE correlation structure is not so much, (3) cloud-dependent BC predictors are essential in the presence of (negative) biases in observation-minus-simulation. We started extending the development to other satellites such as GOES and MSG. The results of assimilating these new developments will also be presented.


AS17-A009
Applying GPM Satellite Observations to Evaluate and Improve the Forecast of Landfalling Tropical Cyclones

Zuhang WU#+, Yun ZHANG, Yanqiong XIE, Hepeng ZHENG
National University of Defense Technology

Observations from microwave satellites such as the advanced Global Precipitation Mission (GPM) satellite permit the testing of cloud microphysical assumptions in numerical model with unprecedented capabilities. We proposed a method to improve the model forecast of landfalling tropical cyclones (LTCs) by constraining the “cloud physics” with GPM satellite observations. Eight typical LTCs that are well observed by GPM satellite in the Asia-Pacific region from 2015 to 2021 are selected to verify the feasibility of this method. Using a cloud-resolving model, the LTCs are simulated for three days with both the original and modified microphysics scheme for comparison. The improvement of LTC forecasts is evaluated in terms of structure, amplitude, and location. Most notably, the structure forecast of condensed water improved up to 32% on average for all LTCs. The location forecast and amplitude forecast of condensed water also improved to varying degrees.


AS17-A023
A Pre-processing Method for Better Assimilation of Microwave Sounding Observations Over Sea Ice for Numerical Weather Prediction

Ji-Soo KIM1+, Myoung Hwan AHN2#
1Seoul National University, 2Ewha Womans University

Observations from microwave sounders have been assimilated into Numerical Weather Prediction systems and have contributed to reducing forecast errors. However, the assimilation of microwave sea ice observations sensitive to surface is limited due to uncertainties in estimating surface radiation. This study presents a pre-processing method to assimilate near-surface microwave sounding observations (e.g. 53.6, 54 GHz) over sea ice. The method involves a better estimation of surface emissivity and a bias correction for surface radiation. Here, the sea ice emissivity is dynamically calculated using Advanced Technology Microwave Sounder (ATMS) observations and the auxiliary data from Korean Integrated Model (KIM). The observation counterparts simulated using the dynamic emissivity exhibit a high correlation with the ATMS observations. However, the simulated brightness temperatures in winter sea ice show a negative bias of 0.6-0.8 K at 53.6 GHz. This bias is caused by using the skin temperature instead of emitting layer temperature to estimate surface radiation. It is found that this bias can be effectively corrected by applying multi-linear regression with predictors related to the surface radiation, such as dynamic emissivity, skin temperature and atmospheric transmittance. Furthermore, a dynamic emissivity and bias correction scheme has been implemented to assimilate the 53.6 and 54 GHz sea ice observations into the KIM system. The assimilation experiment was run in July 2021 together with a control run. As a result, the number of ATMS observations used for data assimilation has increased by 5% compared to the control run. The newly assimilated observations have increased the model temperatures in the winter sea ice by up to 2 K from the surface to 700 hPa, reducing the temperature errors by 1.2 K. The results of this study suggest that a new approach for pre-processing of ATMS sea ice observations is effective and contributes to better utilization of microwave observations.


AS17-A002
Impacts of All-sky Assimilation of FY-3C and FY-3D MWHS-2 Radiances on the Analysis and Forecasts of Typhoon Hagupit

Keyi CHEN1#+, Zhenxuan CHEN1, Zhipeng XIAN2
1Chengdu University of Information Technology, 2Institute of Atmospheric Physics Chinese Academy of Sciences

With the Microwave Humidity Sounder-2 (MWHS-2)/Fengyun (FY)-3D in operation, it is the first time to evaluate the impact of a joint assimilation of MWHS-2 radiances in all-sky conditions from both the FY-3C and FY-3D satellites on the forecast of typhoons within regional areas. In this study, Typhoon Hagupit in 2020 was chosen to investigate the impact; the forecast performances of the joint assimilation were slightly better than the experiments assimilating MWHS-2 observations from FY-3C and FY-3D, respectively, whose results were comparable, especially for the landfall location of Hagupit. With extra cloud- and precipitated-affected MWHS-2 observations assimilated, better forecasts of track and intensity as well as precipitation caused by Hagupit were achieved due to the improvement of the analysis of relative humidity, temperature and wind fields around Hagupit, as compared with the clear-sky assimilation experiments. In addition, the channel selection scheme affects the forecast performances evidently, that is, the radiances from the MWHS-2 118 GHz and 183 GHz channels made an opposite results of the track of Hagupit.


AS17-A031
Evaluation of the Ground-based Microwave Radiometer Data and Its Unified Application with Satellite-based Sounder Observations

Yan-An LIU1#+, Meng LIU1, Jiong SHU1, Jun LI2
1East China Normal University, 2National Satellite Meteorological Center

Ground-based microwave radiometers (MWRs) can continuously detect atmospheric temperature and humidity profiles in the tropospheric atmosphere. Thus, MWR can supplement radiosonde and satellite observations in monitoring the thermodynamic evolution of the atmosphere and improving numerical weather prediction (NWP) through data assimilation. The analysis of product characteristics of MWR is the basis for applying data to real-time monitoring and assimilation. In this research, observations from the ground-based multi-channel MWR are compared with the radiosonde observations (RAOB) and ERA5 reanalysis data. The detection performance, brightness temperature characteristics of various channels, and the accuracy of the retrieval profile products of the MWR are comprehensively evaluated during various weather conditions. On this basis, further research on the collaborative retrieval of ground-based microwave data and satellite observation is carried out to lay a foundation for space-based and gound-based  unified application.


AS17-A026
Cloud Properties of Hot Towers During Slow and Rapid Intensification of Tropical Cyclones in the Western North Pacific

Jason Pajimola PUNAY1#+, Chian-Yi LIU2
1Bicol University, 2Academia Sinica

This study investigates the cloud properties of hot towers (HTs) during slow intensification (SI) and rapid intensification (RI) of tropical cyclones (TCs) in the Western North Pacific. The wide abundance of deep convective clouds (DCCs) during RI is investigated by examining the cloud microphysical properties of the HTs nested in DCCs. In a matured HT, the vertical profiles of liquid water content (LWC) and ice water content (IWC) reveal that condensates [1] mostly form at upper levels; and [2] have strong correlations with vertical velocity. Higher concentration of cloud ice in the HTs of rapidly intensifying TCs as compared with that in slowly intensifying TCs is found and may be used to delineate the onset of RI from SI.


AS17-A014
Tracking Atmospheric Moisture Motion for Three-dimensional Horizontal Winds from Geostationary Hyperspectral Infrared Measurements

Jun LI1#+, Wei HAN2, Di DI3, Zheng MA4, Ruoying YIN5, Zhenglong LI6, W. Paul MENZEL6
1National Satellite Meteorological Center, 2Chinese Meteorological Administration, 3Nanjing University of Information Science & Technology, 4Chinese Academy of Sciences, 5CMA Earth System Modeling and Prediction Centre (CEMC), China Meteorological Administration, 6University of Wisconsin-Madison

Radiance measurements from a geostationary hyperspectral infrared sounder with high temporal resolution not only provide a continuous weather cube of atmospheric temperature and moisture information at different pressure levels, but also enable derivation of three‐dimensional (3D) horizontal winds by tracking atmospheric moisture features. Both thermodynamic and dynamic information is critical for monitoring and predicting the evolution of atmospheric mesoscale events. Using targeted observations from the Geosynchronous Interferometric Infrared Sounders (GIIRS) onboard Fengyun-4A (or FengYun-4B) with 15-minute temporal resolution, three-dimensional horizontal winds are derived by tracking moisture features depicted in radiances or profile retrievals at different atmospheric pressure levels. The derived 3D horizontal winds are evaluated against different reference sources including atmospheric reanalysis and radiosonde/dropsonde observations. The 3D horizontal winds are assimilated together with the GIIRS radiance measurements in the China Meteorological Administration Global Forecast System (CMA-GFS) with a 4Dvar approach; the added value of 3D horizontal winds to the numerical weather prediction based high impact weather forecast will be presented and discussed.


Fri-04 Aug | 1:10 - 3:10 | MR332
AS07 - General Session for Atmospheric Sciences

Session Chair(s):


Biogeosciences


Mon-31 Jul | 8:15 - 10:00 | MR305
BG07 - Biogeochemical Cycling of C and N Through Nexus of Land, Freshwater and Coastal Ocean

Session Chair(s): Punyasloke BHADURY, Indian Institute of Science Education and Research Kolkata

BG07-A020
Sulfur Cycle Research Activities within SCOR Working Groups DMS-PRO and CIce2Clouds

Hakase HAYASHIDA1#+, Martí GALÍ2, Daniela DEL VALLE3, Stephen ARCHER4, Hermann BANGE5, Eva BUCCIARELLI6, Elisabeth DESCHASEAUX7, José GONZÁLEZ8, Frances HOPKINS9, Sohiko KAMEYAMA10, Erin MCPARLAND11, Ki-Tae PARK12,13, Damodar SHENOY14, Jacqueline STEFELS15, Jonathan TODD16, Philippe TORTELL17, Lenny WINKEL18,19, Gui-Peng YANG20, Marcos ZÁRATE21, Miming ZHANG22, Sakiko ISHINO23, Hélène ANGOT24, Antoine HADDON25, Sankirna JOGE26, Hyung-Gyu LIM27, Anoop MAHAJAN26, Ilka PEEKEN28, Nadja STEINER29, Jennie THOMAS24, Megan WILLIS30
1Japan Agency for Marine-Earth Science and Technology, 2Institut de Ciències del Mar (ICM, CSIC), 3Mar del Plata; and Consejo Nacional de Investigaciones Científicas y Técnicas (CONICET), 4Bigelow Laboratory for Ocean Sciences, 5GEOMAR Helmholtz Centre for Oceanic Research Kiel, 6Université de Bretagne Occidentale, 7Southern Cross University, 8University of La Laguna, 9Plymouth Marine Laboratory, 10Hokkaido University, 11Woods Hole Oceanographic Institution, 12Korea Polar Research Institute, 13University of Science and Technology, 14National Institute of Oceanography, 15University of Groningen, 16University of East Anglia, 17University of British Columbia, 18ETH Zurich, 19Swiss Federal Institute of Aquatic Science and Technology, 20Ocean University of China, 21Centro para el Estudio de Sistemas Marinos, Consejo Nacional de Investigaciones Científicas y Técnicas (CESIMAR-CONICET), 22Third Institute of Oceanography, Ministry of Natural Resources, 23Kanazawa University, 24Université Grenoble Alpes, 25University of Victoria, 26CSIR-National Institute of Oceanography, 27University of California San Diego, 28Alfred Wegener Institute Helmholtz-Zentrum für Polar- und Meeresforschung, Bremerhaven, 29Institute of Ocean Sciences, Fisheries and Oceans, 30Colorado State University

Organic methylated sulfur compounds (MSCs) play key roles in planktonic food webs as important carbon and sulfur substrates and also as infochemicals that facilitate biological interactions. In addition, the oceanic emission of biogenic volatile MSCs (dimethylsulfide and methanethiol) to the atmosphere acts as a source of aerosols, which impact cloud formation and properties, and hence climate. Understanding the role of MSCs in the Earth system requires accurate rate measurements to capture the rapid biotic and abiotic cycling processes responsible for the turnover of MSCs in the surface ocean. However, we currently lack both standardized protocols for the analytical determination, and a quality-controlled database for process rate measurements of MSCs. The recently formed DMS-PRO (SCOR working group #166) will address these knowledge gaps by (i) compiling a comprehensive, open-access database of quality-controlled, existing and future MSC cycling rates; and (ii) publishing standardized operating practices on analytical procedures involved in the determination of MSCs rates. CIce2Clouds is another recently-established SCOR working group (#163) that aims to better understand the coupled processes in the ocean–sea-ice–snow–atmosphere system involving sulfur. An overarching aspiration of DMS-PRO and CIce2Clouds is to stimulate research, build capacity, and establish an international, multidisciplinary community of practice on the global sulfur cycle that can share knowledge and skills with the broader oceanographic and Earth system science communities.


BG07-A006
Nitrogen Budget Losses at Present and Future from Aquaculture on a National Scale: A Case Study for India

Shiva SHANKAR Y#+, Asif QURESHI
Indian Institute of Technology Hyderabad

The share of aquaculture in global fisheries production has increased from 4% in the 1950s to 49% in 2020. Destruction of mangroves, biodiversity loss, nutrient and toxic chemical accumulation, soil acidification, greenhouse gas emissions, and interference with natural water courses are outcomes of this expansion. Asian subcontinent contributes to 91.6% of global aquaculture production, predominated by China, followed by Indonesia and India. The sector's growth with intensified nitrogenous inputs is a significant ecological concern. Quantitative assessment of reactive nitrogen (NR) species combining the causative factors and fate of released species on a national scale is lacking for India. Present work attempts to address these gaps by adopting material flow analysis with coupled human and natural systems (CHANS) approach. Results of the study point out an increase in NR from inputs with 66.8 Gg in 1980 to 686.7 Gg in 2020. The relative increase in feed input from 30.8% in 1980 to 68.5% in 2020 has been the guiding factor for NR inflows. Cultivators adopting nutritionally imbalanced and unstable farm-made mash feeds for financial gains enriched pond NR. Nitrogen-use index was reduced by 50% in four decades resulting in a rise of NR accumulation from 13.2 Gg in 1980 to 102.4 Gg in 2020. Release of gases such as NH3, CH4, and N2O from the accumulated uneaten feed and excretions combined with other organic/ inorganic fractions are of significant concern. The atmospheric subsystem receives 49% of NR outflows, followed by the 44% towards the human subsystem with the fish harvest. Research also projects futuristic scenarios for 2050 with possible strategies for optimizing the Nrelease. Considering the sector's importance in enhancing food security, work emphasizes the immediate need for an integrated-climate resilient framework for facing the impacts of climate change to support global aquaculture production.


BG07-A010
Elucidating the Sedimentary Carbon Dynamics of North-east Coastal Bay of Bengal Using Benthic Foraminifera Biocoenosis

Arkaprava MANDAL#+, Punyasloke BHADURY
Indian Institute of Science Education and Research Kolkata

Coastal ecosystems are recognized by their multifaceted ecological functions, including providing resources for food security, livelihood, and protection of coastal shorelines and represent a key part of achieving UN SDG Goals, including SDG14. The northeast coastal Bay of Bengal (BoB) in South Asia is interspersed with several coastal biotopes influenced by the Ganga-Brahmaputra-Meghna delta, among others and it contributes immensely to the sustainable blue economy. Over the last decade, anthropogenic climate change, including cyclonic storms, depressions, coastal erosions, reduced freshwater flow, relative sea level rise, and altered riverine course, has become a primary driver toward changing environmental conditions in the northeast coastal BoB. The coastal BoB was increasingly reeling from numerous anthropogenic stressors, and the scales of anthropogenic disturbances were characterized through benthic foraminifera coenosis over the seasons along with robust measurement of organic carbon in sediment. Extensive sampling of the significantly different microhabitats highlighted the overwhelming abundance of opportunity calcareous taxa Ammonia spp., Quinqueloculina spp. The present study classified the ecosystem quality of the coastal Bay of Bengal based on sedimentary total organic carbon and benthic foraminifera abundance. The values of total organic carbon of sediment indicated the “Good” ecological status of coastal BoB, although the total organic carbon content exhibited the influence of anthropogenic forcings in closer proximity to human influences. Evidence of anaerobic degradation of sediment organic matter resulted in changes in sediment pH and taphonomic alteration of benthic foraminifera tests. Overall, this study has provided much-needed baseline information on tracking the biogeochemical status of the north-east coastal Bay of Bengal in link with anthropogenic stressors.


Mon-31 Jul | 10:20 - 12:20 | MR305
BG07 - Biogeochemical Cycling of C and N Through Nexus of Land, Freshwater and Coastal Ocean

Session Chair(s): Anwesha GHOSH, Indian Institute of Science Education and Research Kolkata

BG07-A008
Mangrove Leaf Litter Dynamics in Aquaculture Ponds of Indian Sundarbans – Exploring Carbon and Nitrogen Dynamics for Sustainable Blue Economy

Yash YASH#+, Punyasloke BHADURY
Indian Institute of Science Education and Research Kolkata

Mangroves serve various ecological and socio-economic functions including in blue economy; hence crucial to achieving United Nations Sustainable Development Goals (SDGs). Sundarbans, the world’s largest contiguous mangrove forest, an UNESCO World Heritage Site and a RAMSAR site formed on the delta of Ganga-Brahmaputra-Meghna, faces the northeast coastal Bay of Bengal (BoB). This ecosystem is key to sustenance of blue economy in the Bay of Bengal including BoB rim countries. The coastal Indian Sundarbans is intensively used for aquaculture practices leading to continuous anthropogenic stressors including release of pollutants. Moreover, such aquaculture practices are considered to unsustainable and can cause irreversible damage to health of coastal oceans. In the present study, efficacy of mangrove vegetation planted along the boundaries of aquaculture ponds in Sundarbans (integrated mangrove aquaculture-IMA) has been evaluated by investigating role of mangrove leaf-derived phenolic groups (tannic and gallic acids) that can contribute significantly to carbon and nitrogen pools leading to better coastal bioresources yield. The values of inorganic nitrogen (50-300µM), o-phosphate (0.5-10µM), silicate (10-80 µM), dissolved organic carbon (37 mg/L – 80 mg/L) exhibited wide variation, indicating a strong influence of anthropogenic forcings in recent years, and that the ecological stoichiometry was favoured by breakdown of mangrove leaf litter. The observed higher concentration of tannic acid encountered during the studied period highlighted alteration in nitrogen cycle and also showed that tannic and gallic acids-maintained water quality and may have ultimately led to improved yield of coastal bioresources in the IMA pond. The current study provides a new approach to nature-based solutions (NbS) and for improving the income of aquaculture practitioners through sustainable blue economy.


BG07-A013
Role of Microplastics in Effecting the Carbon Dynamics of Coastal Bay of Bengal

Nirupama SAINI#+, Punyasloke BHADURY
Indian Institute of Science Education and Research Kolkata

The mangrove ecosystem provides multifarious ecosystem services and is critical to a sustainable blue carbon economy. Mangrove vegetation slows down water flow and thus allows particles to deposit or settle down and has been identified as a potential sink of microplastics. The Sundarbans mangrove ecosystem, one of the largest contiguous mangrove ecosystems and a UNESCO world heritage site, is facing an increasing immense threat of plastic pollution. The Sundarbans lies on the deltaic region formed by three major rivers named Ganges, Brahmaputra and Meghna that converge into the Bay of Bengal and form the world’s third largest freshwater discharge outlet to oceans. These rivers are among the top ten global plastic waste-carrying rivers. The mean microplastic concentration observed in the surface water of Indian Sundarbans is 24.36±12.19 in monsoon, 14.41±7.39 in post-monsoon and 13.85±7.55 (Particles/ Liter)in pre-monsoon. All four forms of microplastics, including fiber, fragment, foam, and microbead, have been detected in the surface water of Sundarbans with the highest contribution of fibers and fragments, respectively. Further, chemical characterization of microplastics confirmed around 20 types of polymeric composition. These microplastics in the water column thrive as micro-niche and thus can affect the carbon pool. Plastisphere community is explored using bright field microscopy and the FESEM approach, which showed bacterial and algal community association with the surface of plastics. Moreover, the visible physical changes in the plastic surface confirm the signs of biodegradation. Metagenomic profiling of the surface water microbial community revealed the presence of potential genes associated with the degradation of plastic polymers such as PET, LDPE. Overall, the presence of microplastics in surface water, its colonization and the possible plastic degrading potential of the microbial community indicates the disruption of biogeochemical cycling, which can have cascading effects throughout the ecosystem.


BG07-A009
Biological Tracking of Nitrogen Pollution in Mangroves- The Importance of 'omics' Based Approach

Punyasloke BHADURY#+
Indian Institute of Science Education and Research Kolkata

Mangroves represent a unique ecotone between land and ocean boundary systems, drive ecosystem processes and contribute to blue economy across South Asia. The mangroves surrounding the Bay of Bengal receives nitrogen inputs from multiple sources including from continuous anthropogenic activities with effects on structure and functioning of resident biological communities. The main objective of this study was to track the effect of dissolved inorganic nitrogen (DIN) pool influenced by anthropogenic nitrogen on resident bacterioplankton communities in Sundarbans, world’s largest contiguous mangrove wetland. Using ‘omics’ based high-throughput sequencing of bacterioplankton communities based on sequencing of V3-V4 region of 16S rRNA (32777527 pair-end reads) and robust DIN pool quantification, a large number of stations representing from west to east of Sundarbans were classified as low DIN (>45μM) and high DIN (<40 μM) stations. Proteobacteria, Bacteroidetes, and Firmicutes were the dominant bacterioplankton phyla across all stations. Nitrogen-fixing groups such as Nitrospirae, Lentisphaerae, Chloroflexi, and Planctomycetes were found to make up about1% of the bacterioplankton communities. Abundances of Spirochaetes and Tenericutes showed a positive correlation with DIN. Pseudomonadales, Alteromonadales, and Desulfovibrionales were found to distinctly vary in abundance between Low and High DIN stations. Predicted metagenomic profiles from taxonomically derived community structures indicated bacterial nitrate-nitrite reductase to be negatively correlated with prevalent DIN concentration in High DIN stations but positively correlated in Low DIN stations. This trend was also consistent for genes encoding for nitrate/nitrite response regulators and transporter proteins. The identified high DIN stations incidentally also exhibited signs reeling from nitrogen pollution including loss of biodiversity. The new DIN approach coupled with ‘omics’ based biomonitoring provides a new mechanistic classification of mangroves reeling from nitrogen pollution and can form the basis for targeted ecosystem restoration as well as to improve the concept of sustainable blue economy.


Tue-01 Aug | 10:20 - 12:20 | MR310
BG01 - Climate Change and the Biogeochemical Cycles of Elements and Contaminants

Session Chair(s): Jagannath BISWAKARMA, University of Bristol, Asif QURESHI, Indian Institute of Technology Hyderabad

BG01-A003
Impact of Different Bulk Density Estimation Methods on Soil Organic Carbon Storage Prediction

May Thi Tuyet DO+, Minho YEON, YoungHun KIM, Giha LEE#
Kyungpook National University

Evaluating soil organic carbon stock (SOCS) is critical in controlling carbon dioxide (CO2) emissions to the atmosphere to mitigate the effect of climate change and global warming. Bulk density (BD) is a significant factor that affects uncertainty in the national estimate of soil organic carbon stock. This study estimated bulk density data in the Korea Rural Development Administration soil dataset (n=391 soil series) at depths 0 to 30 cm using a variety of methodologies. Regression analysis (i.e., pedotransfer function) and machine learning (i.e., Artificial Neural Network (ANN)) approaches were mainly used to predict BD parameters. The predicted BD established the SOCS density for 0-30 cm depth in South Korea. The results reveal that the SOCS density differs greatly depending on the specific BD prediction method employed. With the coefficient of determination (R2) and root mean squared error (RMSE) 0.68 and 0.158, respectively, constructing BD based on regression analysis provided the most outstanding results. The established SOCS content differed significantly between the regression-based BD and machine-learning approaches. The longitudinal distribution of SOCS changed with temperature and precipitation. Where annual rainfall was above 1300 mm and the average yearly temperature was cold, the SOCS concentration in Korea was exceptionally high.


BG01-A002
Changing Bioaccumulation of Organic Contaminants in Food-webs Under a Changing Climate

Asif QURESHI#+
Indian Institute of Technology Hyderabad

Oceans (including open oceans and coastal zones) are a major source of protein and sustenance for a large portion of earth’s populations. Seafood is a staple diet in many regions, and fishes are an important source of proteins and essential acids. However, anthropogenic emissions have introduced a large suite of contaminants into the oceans. These contaminants, particularly mercury and persistent organic pollutants bioaccumulate and biomagnify in the food chains. Concentrations in top predators are up to a million times those in water. Climate change stresses the fish residing in ocean ecosystems. How these stress further increase or decrease bioaccumulation has not been sufficiently studied. Previous works including that from my group has shown the temperature increase of 1 degree Celsius and the correspondingly increased metabolic rates increase mercury bioaccumulation in top predators by 20 to 80%. How temperature affects organic chemicals is unclear, and requires model development and parameterization. Here, I am going to present the development of a food-web bioaccumulation model that is constructed on first principles, similar to mercury bioaccumulation model, but differs in the description of chemicals (as organic chemicals are different to mercury). In short, uptake, metabolic and accumulation rates will be parameterized along with contaminant uptake rates. Bioaccumulation effects in different climate change (temperature increase) scenarios will be presented on chemicals such as DDT, HCH, and organochlorine pesticides such as lindane, and many others. Results are of global significance as climate change is already impacting oceans and the dependent communities.


BG01-A013
Assessing the Influence of Climate Variability on the PCBs Dynamics Using Two Different Global Models BETR-Global and MIT-GCM

Vikas Kumar MEENA#+, Priyanka ., Asif QURESHI
Indian Institute of Technology Hyderabad

Toxic pollutants such as polychlorinated biphenyls (PCBs) are ubiquitous in the environment, and are of concern because of their persistence, long range transport and bioaccumulation. Oceans are an important component of their biogeochemical cycle. Oceans act as their long-time reservoirs and also as the base of marine food-webs which are consumed by humans. Two classes of global model exist to understand PCBs behaviour: multimedia models that simplify the physics and chemistry of global circulation and focus on the chemical; and the complex global circulation models that contain chemicals as tracers. BETR (Berkeley-Trent)-Global is a global-scale multimedia contaminant fate model widely used to model organics. However, their treatment of oceans is limited to a top layer. The global circulation model MIT-GCM has detailed parameterization of parameters such as concentrations of plankton and mixed layer depths, and contains deep ocean layers. How these differences in model descriptions change the predictions of PCBs concentrations and the impacts of climate shifts have been largely unexplored. Here, we will use both BETR-Global and MIT-GCM models to understand the global fate and distribution of PCBs, and the impact of changes in parameters such as temperature and primary productivity in the volatilization, transport or sinking of PCBs in the oceans. BETR-Global runs from years 1930 to 2018 for two congeners PCB-28 and PCB-153. There is a net air-to-ocean flux of 6.03x10-05 ng/m2/hr for PCB-28 and 3.11x10-04 ng/m2/hr for PCB-153. For 1° increase in global oceanic temperature, net air-to-ocean flux of PCB-28 is decreased by 4.62% and PCB-153 by 0.15%. Overall, oceans become a net sink, but sinking is decreasing with increase in oceanic temperature. Further simulations are planned to extract trans-basin flows in BETR, and the use of MIT-GCM for PCBs fate and transport.


BG01-A014
Impact of Seasonal and Climate Variability on the Global Fate and Transport of PAHs

Priyanka .#+, Vikas Kumar MEENA, Asif QURESHI
Indian Institute of Technology Hyderabad

Polycyclic aromatic hydrocarbons (PAHs) are highly toxic and persistent pollutants known to undergo long range transport and bioaccumulate in food chains. Atmospheric transport of PAHs has been shown to be dependent on regional meteorology in regional-scale simulations, such as in China. In the presented work, we will take advantage of the newly available inventory of global emissions of PAHs in EDGAR (Emissions Database for Global Atmospheric Research) for the period 1970-2018 to understand the global transport of PAHs and its seasonal variability across the world. We will use the widely used BETR-Global model for organic contaminants to assess the impacts of changes in variables such as wind, temperature and precipitation will be assessed for their impacts on seasonal trans-regional/trans-boundary flows of PAHs. Model runs for the PAH benzo(a)pyrene reveal the yearly average concentrations of BaP in northern hemisphere to be 1.29 x 10-14 kg/m3 in air, 1.42 x 10-7 kg/m3 in vegetation, 6.86 x 10-12 kg/m3 in oceans and 1.23 x 10-9 kg/m3 in soil. Concentrations in the southern hemisphere are lower in air by 21%, vegetation by 23%, ocean by 48% and soil by 17%. These differences are largely a result of BaP sources being in the northern hemisphere. We are now extracting seasonal flows of BaPs across regions such as Asia to Europe, Europe to Arctic, North America to Arctic, Africa to Europe. We will use these seasonal variations to understand how changes in climate, such as increased El-Nino or La-Nina events, may contribute to increased or decreased transport of BaP across the globe.


BG01-A012
Deforestation in the Amazonian Basin Increases Anthropogenic Mercury Pollution

Aryeh FEINBERG1, Martin JISKRA2, Pasquale BORRELLI3, Jagannath BISWAKARMA4#+, Noelle E. SELIN1
1Massachusetts Institute of Technology, 2University of Basel, 3Roma Tre University, 4University of Bristol

Mercury (Hg) is a global pollutant causing adverse effects on human and environmental health. Several studies showed that terrestrial ecosystems are a significant sink for atmospheric Hg. Anthropogenic changes such as land-use change, including deforestation, can severely impact global Hg cycling. In contrast to carbon dioxide, Hg (re)emission due to land-use change is not included in any national or international Hg emission inventories, including Minamata Convention on Mercury. In this study, we quantified the effect of deforestation on the terrestrial-atmosphere net exchange of Hg and on Hg transfer to the aquatic ecosystem in the Amazon basin. To determine the Hg fluxes under different scenarios, global mechanistic models GEOS-Chem and GloSEM were used for the atmosphere and soil erosion, respectively. Our results showed that if deforestation continues to occur at a similar rate, Amazon can only take up 94 Mg yr-1 in 2050 compared to 268 Mg yr-1 in 2003. Thus the business-as-usual scenario highlights that the Amazon sink will be 65% weakened by 2050 compared to 2003 forest conditions. This study presents substantial evidence to land-use-change-induced impacts on Hg cycling and, thereby, the urgent necessity of including land-use-change as a driver of anthropogenic Hg pollution in the policy.


BG01-A010
Geogenic Arsenic Contamination in Soil-water-plant System and its Possible Mitigation

GKM Mustafizur RAHMAN#+, Md. Humayun KABIR, Mohammad Saiful ALAM, Md. Mizanur RAHMAN
Bangabandhu Sheikh Mujibur Rahman Agricultural University

Arsenic (As) toxicity in soil-water-plant system is a serious concern in Bangladesh and west Bengal of India. It’s transfer from soil to food chain causes serious health hazards of hundreds of thousands of people living in this region. Arsenic in irrigated paddy soils have been continuously accumulating (20-80 mg kg-1) because of irrigating with contaminated shallow tube well (STW) water (50-400 μg L-1). The south west part of Bangladesh i.e., the Ganges Flood Plain soils is heavily contaminated through STW irrigation water driven from shallow aquifer (60 to 120 feet depth) where As bearing minerals from the Himalayas deposited with geogenic processes. Thus, higher concentration of As were observed in different crops grown in the As contaminated soils. The technologies for As remediation in agriculture have already been discovered from the findings of the different research project activities. It was found that As buildup in soil through contaminated irrigation could be reduced up to 30-40% through water management practices like raised bed and alternate wetting and drying (AWD) methods. Besides, an arsenic tolerant rice (BRRI dhan47) was discovered for the first time in Bangladesh. On the other hand, biochar has also been appeared as a potential organic material of reducing As uptake in food chain significantly.


BG01-A011
Role of Mixed-valent Iron Phases on Arsenic Mobilization

Molly MATTHEWS, Jagannath BISWAKARMA#+, Harry FORRESTER, James BYRNE
University of Bristol

Arsenic (As) contamination in groundwater is a global health crisis. Due to the abundance of geogenic As, southeast Asia and south America are acutely affected regions of the globe. Many studies have shown that As can be eliminated from groundwater when treated with iron (Fe) phases. For example, zero-valent Fe has removed As from groundwaters in Bangladesh and Burkina Faso. However, other Fe phases are under-explored for their potential uses in As treatment. Mixed-valent Fe phases, such as Fe-rich clay and minerals, are ubiquitous in terrestrial and aquatic environments and can be investigated for their potential to treat As-containing groundwater. In this study, we considered two mixed-valent Fe minerals- nontronite (NAu2) and green rust sulphate, and investigated: 1. As (III) sorption onto the mineral surfaces; and 2. As mobilization due to organic ligands such as citrate or EDTA. We conducted experiments under anoxic conditions at neutral pH with two mineral concentrations (0.1 and 1 g/L) combined with five As (III) concentrations ranging from 0 to 500 µg/L. We used ICP-OES to quantify the dissolved concentrations of Fe and As. The results were used to identify the sorption mechanism. We also determined the kinetics of As mobilization in the presence of 50 µM citrate or 200 µM EDTA. This presentation will highlight the role of mixed-valent Fe minerals on As sorption and As mobilization in the presence of organic ligands.


BG01-A009
Quantifying the Benefits of Environmental and Sustainability Measures Undertaken by NMDC

Abhas JAIN1,2#+, M. Jayapal REDDY1, Dilip Kumar MOHANTY1
1NMDC Limited, 2Indian Institute of Technology Hyderabad

About: NMDC Limited is a public Sector company and is the single largest producer of iron ore in India with its operations in Chhattisgarh and Karnatakas and a fully mechanized open cast Diamond Mine in Panna, Madhya Pradesh. Background: Mining activities have associated carbon emissions. To mitigate the same, NMDC has been proactively undertaking activities to restore the natural environment during and post mining viz. massive plantation drives, reclamation of land by plantation of saplings, native species, grass and shrubs. The total area covered till date is more than 2300 Ha. These mitigation methods help capture and sequester carbon in vegetation and below-ground biomass and the fluxes of greenhouse gases are also mitigated. The research is being taken up to quantify the environmental benefits of sustainability initiatives undertaken at NMDC. Quantifying the benefits of plantation activities, in terms of calculating the total carbon stock is not a requirement and hence not popular in India and is not being taken up by companies. Objective of this paper is to have a better accounting of the carbon sequestered by the afforestation drives of NMDC over the past seven decades. Methods: The aboveground and belowground carbon stocks will be estimated by calculating the tree volume and biomass (based on the species-specific regional volume equations from the Forest Survey of India) and equivalent carbon stocks (as per methods listed in Forest Survey of India (FSI 2017), UNFCC manual for estimation of for projects under the Clean Development Mechanisms (UNFCCC 2015)). The results will be validated by experimental work to obtain a total carbon account of soil (by using total carbon analyzer). Results: The research will help to have a better accounting mechanism of the total carbon sequestered will help to plan systematic mine closure and reclamation of mine-site during and post mining.


Tue-01 Aug | 1:10 - 3:10 | MR305
BG09 - Role of Biogeosciences in a Sustainable and Circular Society

Session Chair(s): Bhoopesh MISHRA, Illinois Institute of Technology, Punyasloke BHADURY, Indian Institute of Science Education and Research Kolkata

BG09-A011
Low Cost Sustainable Solutions for Wastewater Treatment

Bhoopesh MISHRA#+
Illinois Institute of Technology

Converting biomass waste to sustainable carbon-negative materials via hydrothermal and thermochemical process conditions has emerged as an economically viable pathway for a regenerative circular economy by recapturing resources after disposal. Driven by multidisciplinary research integrating basic sciences and engineering, we have successfully designed hierarchical porous carbon materials from lignocellulosic biomass waste residues. Further, we have used these scalable and affordable porous carbon-materials to design a range of products including nanomaterial functionalized carbon composites and biopolymer-based crosslinked hydrogels for enhanced decontamination and water purification. This presentation will highlight the design and properties of sustainable materials for water/wastewater treatment.


BG09-A006
Assessment of Air Pollutant Emission Reduction Potential for Sustainable Bioenergy

Yifan XU+, Zhangcai QIN#
Sun Yat-sen University

Compared with traditional fossil fuels, bioenergy has obvious advantages due to its renewability and sustainability, and plays a vital role in maintaining energy security. However, the comprehensive life-cycle assessments of air pollutions from bioenergy are still insufficient in China. In this study, by analyzing biomass availability and bioenergy conversion pathways in China, we estimated the air pollution emissions reduction potential (including CO, NOX, SO2, PM10, and NMHC) of sustainable bioenergy resources compared with the coal-based emissions. Results show that the emission reduction potential of air pollutants varies by biomass conversion pathways. Biomass direct-fired cogeneration could reduce the emissions of all these five air pollutions. Biomass gasification cogeneration and integrated gasification combined cycle (IGCC) could also reduce a large amount of SO2 and NOX emissions, but may contribute to more NMHC emissions. Our results provide critical insights into bioenergy production and deployment in China from the perspective of air-quality benefits.


Tue-01 Aug | 3:30 - 5:15 | MR305
BG10 - Biogeosciences General Session

Session Chair(s): Punyasloke BHADURY, Indian Institute of Science Education and Research Kolkata

BG10-A003
Biogeochemical Factors Driving Mercury Methylation in a Subtropical Mangrove Wetland

Shaoyi WANG, Martin TSUI#+
The Chinese University of Hong Kong

Wetland ecosystems serve important functions for coastal environments. Most tropical and subtropical wetland areas, about 60-75%, is mangrove forest. However, sediments in mangroves with strong reducing conditions may play a significant role in producing highly toxic methylmercury (MeHg). In Hong Kong, Mai Po Nature Reserve has one of the largest mangrove forests along the south China coastline. At Mai Po, multiple 15-cm deep sediment cores were collected along a transect from within mangrove stands (Kandelia obovata), water and sediment interface, middle of the water channel to open water area in Gei Wei, enclosed ponds featured in Mai Po. Sediment cores were sectioned into every centimeter, and total mercury, methylmercury, organic matter content were analyzed, while in-situ water quality were measured for site. The concentrations of total mercury (THg) were relatively similar among depth and transect locations (139.2-179.9 ng/g dry wt.). In general, both THg and loss on ignition (LOI) were consistent along the vertical profiles of each sediment core but the vertical and spatial distribution of MeHg varied substantially. For spatial distribution, MeHg concentrations within mangrove forests were relatively high (0.26 – 2.07 ng/g) compared to those in the pond sediments (0.10-0.17 ng/g). At the forest-pond interface, the MeHg concentrations were intermediate (0.01-0.30 ng/g). We also found that the THg to MeHg ratio within mangrove roots is about seven times higher than that in other sites. This could be a direct indication that mangrove trees have influence on mercury methylation. And LOI was found to have a significant correlation with methylmercury concentration (r = 0.602), which means organic matter in sediment could play an important role in controlling MeHg distribution.


BG10-A002
Mercury Bioaccumulation and Biomagnification in Subtropical Forest Ecosystems of Hong Kong

Matthew CHENG, Martin TSUI#+, Jack CHEUNG, Ken YAU
The Chinese University of Hong Kong

Mercury (Hg) is a global pollutant and Hg can be converted by certain microbial communities to a highly toxic organic form called methylmercury (MeHg). Relatively, there are very few investigations on the sources and the transfer of MeHg in terrestrial ecosystems compared to the extensive research on aquatic ecosystems in the past 4-5 decades. Energy flow and trophic structure is investigated in this study on three subtropic forest floor food webs by using stable carbon (δ13C) and nitrogen (δ15N) isotope ratios, respectively. Total mercury (THg) and MeHg concentrations in basal resources and terrestrial invertebrates would be measured. THg in foliage and litter in these subtropical forests in Hong Kong are found to be higher than that in the temperate region (e.g., the U.S.), potentially implying higher atmospheric deposition. For the data on invertebrate samples obtained so far, THg and MeHg levels would increase along the trophic levels, indicating the biomagnification of Hg in these subtropical food webs. The study will provide a better understanding on whether MeHg would pose a threat to the ecosystem health in subtropical forests without point source pollution.


BG10-A014
Assessment of Heavy Metals Contamination and its Sources Using Stable Isotope in Ennore Estuary, South-east Coast of India

Pavitra C. MIRJANKAR1#+, Krushna VUDAMALA2, Sarang DEEP 2, Sanny Kumar KASHYAP1, Aaron SCHULTZ3, Tanveer ADYEL3, Asif QURESHI1
1Indian Institute of Technology Hyderabad, 2CSIR-National Institute of Oceanography, 3Deakin University

Estuaries are vital ecosystems that support diverse flora and fauna, and act as a major source of food and economic activities. Industrialization near coastal habitats has led to increased presence of pollutants in coastal ecosystems. Ennore estuary located on the South- East coast of India, is one such important aquatic ecosystems which supports major industrial and residential settlements. But at the same time, receives effluent discharges from these industrialized and urban settlements. In the presented study, the concentration of heavy metals lead, mercury, arsenic, cadmium, chromium and selenium are being investigated from collected sediment and shrimp samples from the Ennore estuary. Samples are taken from a transect starting from estuary mouth to locations receiving industrial discharge, to upstream low impacted locations that act as a local background. Mercury analysis has already revealed the highest value of mercury in sediments, 127.13 μg/kg, is from the zone receiving a direct industrial discharge and is much lower 2.4 μg/kg in a farther point 9 km away. Pollution indices such as Contamination Factor (CF) and Geo- accumulation Index (Igeo) will be further used to assess the degree of heavy metal contamination in the sediment of the estuarine system. Stable isotopes of nitrogen and carbon will be utilized to understand the trophic status of shrimps and the source of their diet. Carbon stable isotope analysis further used to reveal if carbon isotopes measured in shrimps are similar to sediments and collected fly ash. We expect the similarity to be to be high in the industrially impacted zones and lower in uncontaminated zones. The study will help to assess heavy metal distribution and its sources. Results of this study will provide information for the protection of the Ennore estuary and the ecosystems it supports and highlight the utility of stable isotopes in source attribution.


BG10-A006
Comparative Analysis of Climate-driven Carbon Cycle Extremes Using Observations and CMIP6 Earth System Models

Bharat SHARMA1#+, Forrest HOFFMAN1,2, Jitendra KUMAR1, Auroop R. GANGULY3
1Oak Ridge National Laboratory, 2University of Tennessee, Knoxville, 3Northeastern University

Terrestrial ecosystems and their diversity are affected by extreme events related to the carbon cycle (e.g., gross primary productivity, GPP) driven by anomalies in the climate drivers. The impact of these events is expected to increase in the future due to increasing frequency and compound climate drivers. The variability in carbon cycle anomalies and their climate drivers are key to determining the future trajectory of the land carbon sink and its capacity. This study analyzes the interannual variability and extremes of the carbon cycle in observations and CMIP6 Earth System Models. We also compare the change in the characteristics of carbon cycle extremes between historical and various future shared socioeconomic pathways. Results show that the interannual variability and extremes in GPP anomalies are much higher in CMIP6 models compared to observationally derived GPP datasets. Multiple models suggest that the relative increase in negative carbon cycle extremes is expected to be higher than the increase in plant productivity. The largest driver of these extremes is precipitation anomalies, followed by surface air temperature anomalies. Uncertainties in carbon uptake must be addressed to achieve carbon emissions reduction goals while meeting the growing demand for infrastructure and consumer goods.


Wed-02 Aug | 1:00 - 5:15 | Summit
BG - Biogeosciences Poster Session

BG01-A004
A Potential Solution in the Removal of Copper in Mine Wastewater

Kung Ming LEUNG1#+, Richard XU2, Grace LAI1, Simon GRIFFIN1
1The ISF Academy, Hong Kong SAR, 2Melbourne Grammar School, Australia

Mine tailings and wastewater are often toxic and acidic. Heavy metal ions in the tailings can easily dissolve into wastewater and run-off to contaminate both surface water and groundwater, resulting in serious toxicity to humans and ecosystems, representing a long-term environmental hazard. Waste containment and chemical remediation are expensive options, so that bioremediation may present a more viable alternative. Serratia is a bacterial genus with a wide geographical distribution, known to survive harsh conditions such as acidic environments and high concentrations of heavy metal ions. This project has investigated two copper-tolerant isolates of Serratia sp. to explore their potential application to heavy metal remediation. 
Two isolates of Serratia sp., isolated from a disused tungsten mine (KML.E1) and from countryside soil (RX11.2), showed tolerance to high levels of Cu2+. Upon incubation in Luria broth containing up to 90 mM CuSO4 or copper(II) tartrate, red-brown precipitates were observed indicating reduction of copper(II) ions to the metal. Subsequently, the activites of the bacterial strains immobilised in the form of calcium alginate beads has been investigated, since this would allow the bacteria to be localised and protected from competing microbes; it also minimises the risk of biocontamination of the surroundings.
While this work helps to support the use of bioremediation for the removal of Cu2+ from wastewater, the reductive mechanism of Serratia sp. strains ML.E1 and RX11.2 might also be applied to the recovery of other metals with suitable electrode potentials such as Ag and Au.


BG01-A006
Mercury Methylation in Sediment Influenced by Permafrost Thawing in the East Siberian Sea and Beaufort Sea, Arctic Ocean

Hakwon JEONG1#+, Jihee KIM2, Sangwoo EOM1, Juhyeong CHAE1, Seunghee HAN1
1Gwangju Institute of Science and Technology, Korea, South, 2Korea Institute of Science and Technology, Korea, South

The extent of submarine permafrost on the Arctic shelves has been declining in recent decades due to climate change, however, the influence of submarine permafrost thawing on methylmercury (MeHg) production in sediment has been understudied. The total Hg (THg) and MeHg concentrations and sediment properties in the shelf and slope sites of the East Siberian Sea (ESS) were observed to identify the seasonal permafrost thawing effect on the methylation of Hg(II) in sediment overlying permafrost zone. Top (0–2 cm) sediment was collected from the 12 sites on the ESS Shelf and Slope on the icebreaker R/V Araon in August 2019. THg in sediment was higher in the slope than in shelf sites due to the hydrodynamic sorting of fine particles enriched with Mn/Fe oxides. In contrast, the highest MeHg/THg ratio in sediment was noted at 50–60 m isobaths of the shelf sites, identified as a continuous-discontinuous transition zone. The same sediment also showed greater fractions of photoreactive humic and organic sulfur than in the surrounding sites. This suggests that a copious supply of dissolved organic matter in the active layer of the between transition zone may promote the in situ methylation rate. To confirm this hypothesis in the Beaufort Sea, thirteen 50 cm sediment cores were collected in August to September 2022 on R/V Araon. Like ESS, THg in surface sediment tends to increase towards the slope. The highest MeHg/THg ratio in surface sediment was noted at 50-60 m isobaths, presumed to be a transition zone. This transition zone was confirmed by the observation of pingos, formed through processes of freezing and thawing of sediment porewater. We are currently analyzing methylation rate constant values in each sediment cores to identify if the MeHg production rate increases in the sediment overlying transition zone.


BG01-A007
Productivity-induced Redox Oscillation Control the Nitrogen Isotope Offsets Between Bulk Sediment and Foraminifera-bound Nitrogen in the South China Sea Over the Past 500ky

Li-Wei ZHENG1#+, Yao LAI2, Xiaodong DING3, Ehui TAN1, Xufeng ZHENG1, Zhixiong HUANG1, Zhenzhen ZHENG1, Shuh Ji KAO2
1Hainan University, China, 2Xiamen University, China, 3North Minzu University, China

In oligotrophic South China Sea (SCS), the isotopic compositions of planktonic foraminifera tests (δ15NFB) and bulk nitrogen (δ15NTN), which are both considered as recorders of nitrogen dynamic in the upper ocean of SCS, showing inconsistent temporal patterns (variable offsets (Δδ15NTN-FB) through time) with debatable causes. Since the δ15NFB was protected from degradation, the multi-sources contribution and diagenetic alteration of δ15NTN was thought to be responsible for the offsets, which need further verified. Here we determine the different speciation of nitrogen isotope of a sediment core MD972142 in Southeastern SCS and synthesizes the modern observations of sinking particles (PN%, δ15Nsinking) over the SCS basin from export to burial modern to explore the temporal variation of Δδ15NTN-FB. Results show that the Δδ15NTN-FB changed from -3 to 3‰ over the past 500ky, with negative values in glacial and positive in interglacial period, which was controlled by the productivity-induced bottom water redox oscillation, while both the contribution of terrigenous ON and clay-fixed inorganic nitrogen to δ15NTN was ignorable.


BG01-A008
Biogeochemical Paleoceanography of Ulleung Basin, East Sea for the Last 600 Kyr

Jeongwon KANG#, Sangmin HYUN, Jin Hyung CHO, Yunji KIM+
Korea Institute of Ocean Science and Technology, Korea, South

GPC-2B sediment core, collected in Ulleung Basin, was analyzed to reconstruct the variation of paleoceanographic conditions of southern East Sea. Two tephra layers, Aso-4 (88 kyr) and Aso-3 (133 kyr), were observed and alkenone concentrations and lightness (L*) indicated that GPC- 2B covered 600 kyr (MIS 16). Similar to other sediment cores collected in East Sea, foliation and bioturbation were observed in GPC-2B suggesting GPC-2B would have well recorded surface primary production and paleoceanographic conditions. This study aims to reconstruct the history of terrigenous organic matter input and qualitative paleoclimate changes based on biogeochemical properties. The range of TOC content and δ13C were 1 ~ 4% and -21 ~ -25‰, respectively. Based on stable isotope and alkenone-derived SST of GPC-2B suggested that the sediment core reflected the orbital-scale variation for the last 600 kyr. N-alkane also showed orbital-scale alterations; N-alkane content generally increased during glacial stages and decreased during interglacial stages. It suggested that East Asian paleoclimate changes were in association with glacial-interglacial cycle. In addition to biogeochemistry, inorganic geochemical characteristics would be investigated to obtain more reliable paleoclimate and paleoceanographic reconstructions such as relative sea surface temperature and strength of influx East China Coastal Water.


BG02-A001
Applications of Geochronology in Mesozoic Evolutionary Events

Su-Chin CHANG1#+, Daran ZHENG2, Yangyang XIA1, Jun WANG3, Rui PEI2, Yuling LI1
1The University of Hong Kong, Hong Kong SAR, 2Chinese Academy of Sciences, China, 3Yunnan University, China

Geochronology is a foundational approach to understanding Earth’s history. Significant developments in the past 30 years in both U–Pb and 40Ar/39Ar datings, two of the most widely used geochronological methods, allow for unprecedented levels of precision and re-interpretation of geological, climatic, and biological events. Since 2011, our research team based at the University of Hong Kong has applied U–Pb and 40Ar/39Ar radio-isotopic dating techniques to refine the dates and durations of several key Mesozoic evolutionary events. Our age data, for example, provide robust ages to calibrate the terrestrial and marine recoveries after the Permo-Triassic mass extinction event, the origin and diversification of flowering plants, the radiation and migration of the famous Jehol Biota, and the fossil-rich amber discovered from China and Myanmar. In this study, we summarize our contributions which have improved our understanding of the Mesozoic world. We also review the limitations of applying geochronology to evolutionary events and discuss the solutions to these issues.


BG06-A001
Will Nature Do its Trick to Limit Warming Below 1.5°C?

Zhangcai QIN#+
Sun Yat-sen University, China

Significant reduction of greenhouse gas (GHG) emissions is urgently required in order to limit global temperature rise with a reasonable possibility. Under current and even more ambitious climate policies, emissions mitigation from energy and industrial sectors alone do not seem to be able to achieve the Paris climate target of 1.5 °C. The natural climate solutions, by reducing emissions and/or increasing carbon sinks in natural ecosystems, could provide additional efforts to mitigate GHG emissions. However, the role of nature has always been underappreciated in mitigating climate change, will nature do its trick to significantly limit warming? This talk hopes to present recent updates on this topic and discuss the role of nature in climate change from a broader perspective.


BG06-A003
Sensitivity of Land Surface Processes to Surface and Boundary Forcing: A Regional Application of Community Land Model Version 5 for Pearl River Basin

Deng JINLING#+, Liuqian YU
The Hong Kong University of Science and Technology (Guangzhou), China

Knowledge of land surface processes is essential to understanding and predicting the response of terrestrial ecosystems to human activities and climate change. A valuable tool to obtain the required knowledge is land surface models (LSM) that simulate a wide range of Earth’s surface processes, such as exchange fluxes of energy and water and cycling of carbon and nutrients. However, land surface simulations can have significant uncertainties and errors stemming from the imperfect representation of processes, inaccurate forcing, and uncertain initial and boundary conditions, among others. Sensitivity analysis of land surface models is thus an indispensable step for interpreting and improving model results to advance our knowledge of land surface processes. In this study, we implement the Community Land Model version 5.0 (CLM5.0) to Pearl River Basin, an expansive watershed in Southern China with complex heterogeneous landscapes. We assess how the simulated land surface processes respond to three variants of the model grid with high (0.01° × 0.01°), medium (0.05° × 0.05°) and coarse (0.1° × 0.1°) horizontal resolution, and to a suit of atmospheric forcing datasets with various spatial-temporal resolutions. Model simulations for 2010-2015 are validated against remote sensing products and tower-based flux measurements to identify the model configuration that best reproduces observations. Through these analyses, we gain insight into the key factors affecting the performance of land model simulations and improve our understanding of surface energy fluxes, and hydrological and biogeochemical processes in the Pearl River Basin.


BG06-A004
Forest Carbon Sequestration Potential in China Under Different SSP-RCP Scenarios

Yidan HAO#+, Jieming CHOU
Beijing Normal University, China

Forests are major components of terrestrial ecosystems, the estimation of forest carbon sequestration and its economic value as a carbon sink is an important element of global carbon cycle research. In this study, based on the prediction of forestland changes under the future shared socioeconomic pathways SSP1-RCP2.6, SSP2-RCP4.5, and SSP5-RCP8.5, the growth equations of different tree species were fitted using forest inventory data, and the biomass conversion factor continuum function method was used to estimate forest vegetation carbon fixation at the national-scale. The carbon sink potential of the forest ecosystems in 2020-2100 was estimated under the three scenarios, and the carbon fixation potential of forest ecosystems in China and its spatial pattern were discussed.


BG06-A005
Quantifying the Climate and Carbon Cycle Response to Negative CO2 Emissions Over Multi-centennial Timescales

K. U. JAYAKRISHNAN#+, G. BALA
Indian Institute of Science, India

Anthropogenic emissions of carbon dioxide during the industrial period (1750-present) has led to an increase in global mean surface temperature by approximately 1°C. Previous studies show that the increase in frequency of natural disasters such as extreme rainfall, floods and heatwaves is attributed to human induced climate change. The Paris agreement targets to keep global mean warming below 2°C above the preindustrial state, while pursuing efforts to limit the increase to 1.5°C. To achieve the targets set by the Paris agreement, artificially removing large amounts of atmospheric carbon dioxide might be necessary in the 2nd half of this century. Therefore, understanding the response of climate system towards negative atmospheric CO2 emissions is important. In this study, using a coupled climate and carbon cycle model, we simulate the response of the climate system to net negative emissions in 9 idealized simulations. Each simulation has a positive emission phase followed by a negative emission phase such that the cumulative emission since the preindustrial period is zero in each simulation. Three sets of simulations are performed with cumulative emissions of 1000PgC, 2000PgC and 5000PgC in the positive phase. For each value of cumulative emission during the positive phase, three different simulations are performed by varying the total duration (300, 500 and 1000 years) over which the positive and negative emissions occur. The above idealized simulations are designed to address the following two questions: 1) For the same total emissions in the positive phase, does the timescale of emissions have any impact on the long-term response of the climate system? 2) If the timescale of emissions is the same, what is the sensitivity to the magnitude of total emissions in the positive phase? The results from our nine climate-carbon model simulations will be discussed at the meeting.


BG06-A006
Towards Improved Accuracy and Efficiency of Ecohydrologic Processes Using Artificial Intelligence

Elias MASSOUD1#+, Forrest HOFFMAN1,2, Nathan COLLIER1
1Oak Ridge National Laboratory, United States, 2University of Tennessee, Knoxville, United States

Ecohydrology research sits at the intersection of ecosystem ecology and water cycle science, and it incorporates land surface processes and atmospheric and watershed science in addressing ecophysiological responses and feedbacks to the hydrologic cycle. Understanding interactions among important ecohydrologic mechanisms is challenging, and constraining models of ecohydrology is limited by mechanistic knowledge gaps and by observations that are available at only a few of the scales of interest. Artificial intelligence (AI) and machine learning (ML) approaches are likely to provide new avenues for extracting mechanistic understanding from the diversity of data available at different scales. In this work, we aim to apply AI/ML methods to improve computational accuracy and efficiency in estimations of vegetation processes relevant to ecohydrology by utilizing datasets that are rich with observational as well as model simulated information. Beyond improved skill and reduced computational cost, this work explores potential mechanistic process understanding that can be achieved by combining AI/ML methods with available libraries of data.


BG06-A009
Evaluating Land Carbon Cycle Processes in Earth System Models: Have Models Improved Over Time?

Forrest HOFFMAN1,2#+, Mingquan MU3, Min XU1, Gretchen KEPPEL-ALEKS4, Dave LAWRENCE5, Charles KOVEN6, Weiwei FU7, Bill RILEY6, James RANDERSON7
1Oak Ridge National Laboratory, United States, 2University of Tennessee, Knoxville, United States, 3University of California Irvine, United States, 4University of Michigan, United States, 5National Center for Atmospheric Research, United States, 6Lawrence Berkeley National Laboratory, United States, 7University of California, Irvine, United States

Better representations of biogeochemistry–climate feedbacks and ecosystem processes in Earth system models (ESMs) are essential for reducing uncertainties associated with projections of climate change during the remainder of the 21st century and beyond. Model–data intercomparison and integration activities are required to inform improvement of land carbon cycle models and the design of new measurement campaigns aimed at reducing uncertainties associated with key land surface processes. The International Land Model Benchmarking (ILAMB) Package was designed to facilitate systematic and comprehensive model–data intercomparison and improve understanding of factors influencing model fidelity. We used ILAMB to benchmark and intercompare terrestrial carbon cycle models coupled within ESMs used to conduct historical simulations for the Fifth and Sixth Phases of the Coupled Model Intercomparison Project (CMIP5 and CMIP6). Results indicate that the suite of CMIP6 land models exhibits better performance than the suite of CMIP5 land models in comparison with observations for a variety of biogeochemical, hydrological, and energy-related variables. To test the hypothesis that the multi-model range of climate–carbon cycle feedback strengths from more realistic models would diverge less over time, we calculated and compared the ranges of concentration–carbon and climate–carbon sensitivity parameters and the trajectories of land carbon uptake from CMIP5 and CMIP6 models. Since the multi-model means of both the CMIP5 and CMIP6 land models performed better across most variables than any single model that contributed to the means, we also calculated the CMIP5 and CMIP6 multi-model mean feedback sensitivities and uptake trajectories. In an attempt to further reduce uncertainties in carbon cycle projections, we used the ILAMB benchmark performance scores to weight model contributions to the CMIP5 and CMIP6 multi-model means for land carbon uptake and related variables and compared them with observationally constrained estimates for the historical period.


BG06-A010
Autumn Cooling Paused Increased CO2 Release in Central Eurasia

Masayuki KONDO#+
Hiroshima University, Japan

Recent autumn warming in northern latitudes has facilitated an increase in terrestrial ecosystem respiration (TER) more than that in gross primary productivity (GPP), leading to a net loss of CO2 from the land to the atmosphere in autumn. Conversely, autumn cooling is expected to induce a greater decrease in TER than in GPP, thus leading to a net increase in autumn CO2 uptake. However, a recent study reported an increase in net CO2 release in northern autumn cooling from 2004 to 20183, indicating that both the autumn warming and cooling result in net CO2 release. Here, we show that the conclusion regarding net CO2 release under autumn cooling was flawed owing to the inappropriate choice of the autumn period, which resulted in overlooking regions such as central Eurasia, where the 2004–2018 autumn cooling most affected CO2 fluxes. Empirical upscaling of eddy flux observations (FLUXCOM) and atmospheric CO2 measurements from seven towers suggested that the increased net CO2 release paused during the 2004–2018 autumn cooling in central Eurasia. The results reported by the recent study are likely biased toward CO2 release as their assessment involves regions including North America where the 2004–2018 autumn cooling had little effect (rather, the autumn warming effect was more profound) on CO2 fluxes.


BG06-A011
Global C4 Distribution Estimate Constrained by Observations and Optimality Theory

Xiangzhong LUO#+
National University of Singapore, Singapore

Photosynthesis of C4 plants responds to climate change differently than the more common C3 plants, due to their unique anatomic and biochemical characteristics. The different response is expected to cause a change in global C4 distribution, however, current C4 distribution models are inadequate to predict that as they are based on a temperature-only hypothesis and lack observational constraints. Here, we used a global database of photosynthetic pathways, satellite observations and a photosynthetic optimality theory to produce a new observation-constrained estimate of C4 distribution. We found that global C4 coverage stabilized at 11.2% of the vegetated land surface during 1992 to 2016, as a net effect of C4 grass decrease due to elevated CO2 and C4 crop increase, mainly from maize expansion. Using an emergent constraint approach, we estimated that C4 contributed 12.5% of global photosynthetic carbon assimilation, a value much lower than previous estimates (~20%) but more in line with the mean of an ensemble of dynamic global vegetation models (14 ± 13%). By improving the understanding of recent global C4 dynamics, our study sheds insight on the critical and previously underappreciated role of C4 plants in modulating the global carbon cycle in recent history.


BG06-A013
Peatland Loss in Southeast Asia Contributing to U.S. Biofuel’s Greenhouse Gas Emissions

Yakun ZHU+, Zhangcai QIN#
Sun Yat-sen University, China

Land use change (LUC) induced by biofuel production could lead to greenhouse gas (GHG) emissions, which potentially increase biofuel’s carbon intensity. Among the sources of LUC-related emissions for soy biodiesel, the contribution from peatland loss to agricultural plantations in Southeast Asia remains uncertain. Here, we analyzed LUC in Malaysia and Indonesia and modeled its impacts on the GHG emissions of soy biodiesel produced in the United States. It shows that oil palm plantations have more than doubled over 2001-2016 and the area of palm-on-peatlands (PoP) has expanded 3.7 times. Over new palm plantations, the share of PoP is about 19% regardless of time and location and the emission factor (EF) for peatland-to-palm conversion is estimated to be 41.5 Mg CO2 ha-1 yr-1. With these updates on PoP and EF, the contribution of peatland loss (0.7-5.1 g CO2e MJ-1) to biodiesel emissions is only 40- 65% of previous estimates, which reduces discrepancies among model simulations used by different agencies. Based on emerging evidence on LUC and related carbon changes, our analysis reexamines regional peatland loss and its impacts on LUC emissions modeling and provides new insights into the estimation of LUC impacts on biofuels’ carbon intensity.


BG07-A001
Trophic Base and Basal Resources of Northeast Asian Stream Food Webs Pre- and Post-monsoon

Hee Yoon KANG#+
Chonnam National University, Korea, South

Identifying variability in the trophic base and the role of aquatic and terrestrial sources for food webs is a challenge in understanding the dynamics and stability of aquatic ecosystems. Although a large amount of terrestrial detritus transported into the stream continuum during the East Asian summer monsoon would be expected to change the food web base from the pre- to post-monsoon period, further geographically and regionally specific case studies are needed due to the systematic differences in trophic pathways of organic matter supporting aquatic food webs. Here, we examined the δ13C and δ15N values of consumers (invertebrates and fish) across the upstream channel and lacustrine habitats during the pre- and post-monsoon periods in the stream system of Korea compared with those of their potential sources of organic matter. The isotope signatures of potential organic matter sources differentiated allochthonous sources (leaf litter and riparian vegetation) from autochthonous sources (algal biofilm and phytoplankton). The resultant trophic niche indicated a spatiotemporal consistency of the trophic structure at the community level. In addition, the isotope mixing model estimates revealed the trophic attribute of instream production as the primary source of organic matter. These results highlight a consistent dominance of autochthonous trophic bases in aquatic food webs pre- to post-monsoon. Our findings may provide insights into food web dynamics and processes in association with the availability of nutrient sources across the potential links between terrestrial and aquatic ecosystems in the East Asian monsoon climate zone.


BG07-A002
Assessing Carbon Sequestration Capacity of Shellfish Aquaculture Using a Coupled Bioenergetic and Biogeochemical Model

Ye LIU1#+, Liuqian YU2
1The Hong Kong University of Science and Technology, China, 2The Hong Kong University of Science and Technology (Guangzhou), China

Shellfish aquaculture has been rapidly expanding worldwide to meet the accelerating global seafood demand. Recent years have also witnessed a growing interest in including the cultivated shellfish in carbon trading systems. However, significant uncertainty remains in assessing shellfish's carbon sequestration capacity primarily because of the complex interaction between the shellfish and carbon and nutrient cycling in the aquatic environment as well as the atmosphere-water and sediment-water interfaces. Shellfish growth associated with shell formation can directly affect carbon flow through respiration, shell calcium carbonate production, and carbon dioxide (CO2) release from biogenic calcification. Shellfish can also indirectly regulate the ecosystem’s carbon sink capacity by exerting top-down control over carbon-sequestering phytoplankton populations through filter feeding and by accelerating the carbon sedimentation rate via bio-deposition. Therefore, a rigorous assessment of shellfish aquaculture’s carbon sink potential requires thoroughly accounting for the direct and feedback effects of shellfish on the carbon cycle. To conduct such assessment, we propose to build a coupled bioenergetic and biogeochemical modeling framework that can explicitly track the CO2 fluxes from respiration and shell calcification, the carbon flow through the planktonic food webs, and the deposition, remineralization and burial of particulate organic carbon at the aquatic-benthic interface. We will present initial results from the coupled model configured for a eutrophic bay with sizeable oyster farms. The potential of applying the modelling framework to assess shellfish aquaculture’s carbon sequestration capacity over a larger ecosystem scale will also be discussed.


BG07-A004
The Activity and Composition of Methanogens in Constructed Wetland Soils by DNA Stable Isotope Probing

Wen Ting HUANG+, Yo-Jin SHIAU#
National Taiwan University, Taiwan

Constructed wetlands provide various ecosystem services and are important in regulating the global C and N cycles, but they are also important sources for methane (CH4) emissions. Because CH4 is estimated to have a global warming potential of 27-30 over 100 years, it is important to know how the emissions are regulated by soil physiochemical properties in wetland ecosystems. Thus, in this study, we tried to determine the compositions of active methanogens in three constructed wetlands with different ages in Taiwan using a DNA-based stable isotope (DNA-SIP) technology. By incubated the field collected soil samples with 13C-methanol and sequenced the mcrA genes in the heavy layers of the isopycnic density gradient centrifugation, we were able to determine the changes of active methanogens after wetlands were constructed. The results showed the potential CH4 fluxes were respectively 0.02-0.40, 0-0.10 and 0.04-0.17 μg CH4 g-1 soil hr-1 with incubated with methanol, glucose and CO2. In addition, mcrA genes were between 3.12-6.24×108 copies and 0.81-8.88×108 copies in the fresh and incubated wetlands soils, respectively. Furthermore, the dominant methanogens were Methanosarcinales, Methanomicrobiales and Methanomassiliicoccales in the constructed wetlands across different ages. This observation showed that compositions of methanogens were temporal varied in the constructed wetlands. Future study may need to further determine the environmental factors that may decrease the activities of methanotrophs under different wetlands’ ages to maximize the C sequestration potential that wetlands may provide.


BG07-A005
DNA Stable Isotope Probing Reveals Temporal and Spatial Variations of Active Methanotrophs in Subtropical Constructed Wetlands in Taiwan

Ting-Kai CHEN+, Yo-Jin SHIAU#
National Taiwan University, Taiwan

Constructed wetlands, as ecological engineering technologies, are similar in function to natural wetlands in sequestrating carbon and are recognized as nature-based solutions (NBS) in reducing the global greenhouse gas concentrations. However, the anaerobic soil conditions that wetlands provide also make them considerable sources for methane (CH4) emissions. Fortunately, approximately 50 to 90 percent of the CH4 produced from deep wetland soils can be oxidized into carbon dioxide (CO2) by methanotrophs in the aerobic soil layer and mitigate the overall methane emissions from wetlands. Previous studies on methanotrophs have mainly focused on rice paddy and natural wetlands, with limited data on constructed wetlands, particularly in tropical and subtropical areas. This study analyzed the changes of active methanotrophs in three constructed wetlands with different ages and seasons in Taiwan. With using DNA stable isotope probing (DNA-SIP) and next-generation sequencing (NGS) techniques, we revealed the temporal and spatial variations of active methanotrophic compositions in the constructed wetlands. The results of 16S rRNA and pmoA genes in the field soil showed that the highest relative abundance of type II Methylocystis in the wetlands with the lowest sulfate (SO42-) concentration (8.10 ± 1.44 ppm). While the type I methanotrophs were mostly found in the wetlands with high SO42- concentrations. Furthermore, the DNA-SIP experiments revealed active type I methanotrophs were dominated all the studied constructed wetlands. In young wetlands during winter, the increased abundance of type Ib methanotrophs may have a positive impact on methane oxidation. These results demonstrate the ecological niche differentiation of methanotrophs in constructed wetlands under different conditions and the active community structure changes in response to methane concentration. Future management in constructed wetlands will be needed to enhance their carbon sequestration value.


BG07-A012
Seasonal Dynamicity of Environmental Variables, Water Quality Index and Unusual Abundance of Bloom-forming Aulacoseira Spp. Diatom Populations in the Lower Stretch of the River Ganga

Chakresh KUMAR#+, Anwesha GHOSH, Punyasloke BHADURY
Indian Institute of Science Education and Research Kolkata, India

Untreated sewage and other pollutants are being released on a daily basis into major rivers globally including the Ganga in India. Increasing human pressure and resulting anthropogenic pollutants pose numerous challenges to health of Ganga, in particular at the lower stretch which culminates into Bay of Bengal which also receives significant freshwater influx during monsoon season. In this study, the effect of monsoonal precipitation on environmental variables and the Water Quality Index (WQI) was studied at nine sites represented by 59 stations along the lower stretch of Ganga during 2019. Both pH and DO were strongly influenced by monsoon and affected WQI. Seasonal variations in dissolved nutrients, such as nitrate and o-phosphate concentrations were influenced by monsoonal precipitation. Higher concentrations of dissolved nutrients at point-source stations in the study area reflected the effect of direct discharge of untreated urban and industrial sewage on the river. During monsoon, the effects of precipitation and accompanying environmental factors were clearly visible on a key biological variable (concentration of Chl-a), with measured values in PS stations being lower than the SW stations. The WQI values determined for lower stretch of the Ganga revealed very poor water quality in majority of the stations and monsoonal precipitation did not show any influence on the observed trends. Besides, there was evidence of an algal bloom-like scenario, dominated by the centric diatom Aulacoseira spp. in one of the studied sites of the lower stretch of Ganga. This event highlighted the deteriorating water quality with implications for key ecosystem processes such as carbon cycling and the River Ganga's overall health.


BG07-A014
Removal of Arsenic from Groundwater by Natural Polymer-based Hydrogel in the Bengal Delta Plains- Linking Arsenic Biogeochemical Cycling with Carbon Cycling

Meghna BISWAS1#+, Punyasloke BHADURY2
1Vellore Institute of Technology, India, 2Indian Institute of Science Education and Research Kolkata, India

In the Bengal Delta Plains (BDP) encompassing parts of India along with Bangladesh, arsenic in groundwater, agricultural lands and in staple food such as rice, pose serious health challenges to millions of people on a daily basis. The prevailing biogeochemistry of arsenic cycling is influenced by nature and forms of organic carbon present in the BDP. Surface modified iron doped cellulose, a type of polymeric scaffold of biological origin, has been prepared in the laboratory and the efficacy of this polymeric scaffold for removal of forms of As has been evaluated using groundwater and agricultural soils collected from BDP. Based on ICP-MS analysis, the synthesized hydrogel showed ability to remove up to 11 ppb As from groundwater of BDP which exhibited initial concentration of almost 13 ppb As. Besides, the germination efficiency of a cultivar of rice grown in BDP was evaluated by spiking 10-100 mg/kg of As (arsenate salt) and 0.025 g polymeric scaffold. Under all the As spiked conditions, there was germination of the rice cultivar and the physiological mechanisms of this polymeric scaffold in stopping entry of As is being evaluated. As part of ongoing experiment, two cultivars of paddy grown under laboratory conditions but spiked with 100 ppb As and polymeric scaffold (1-2.5 g per 6 kg of soil) seems to be growing and did not exhibit observable physiological abnormalities. The ongoing study with spiked As along with different forms and concentrations of organic carbon in groundwater as well as agricultural soil are being evaluated to assess the efficacy ranges of the synthesized polymeric scaffold of biological origin. The study can form the basis for developing cost-effective and sustainable polymeric scaffold which can render As free groundwater and staple food.


BG07-A016
Harmonizing Satellite and Species Modeling to Explore Mangrove Suitable Area in Timor-Leste

Hyeon-Kwon AHN1#+, Chul-Hee LIM1, Wonhee CHO1, Byungwoo CHANG1, Sue Kyoung LEE2, Ohjung KWON2
1Kookmin University, Korea, South, 2SK Forest, Korea, South

Recently, various measures have been implemented to achieve carbon neutrality, among them, nature-based solutions such as planting tree species are emerging. Mangroves, representative high carbon absorption species, play an important role in minimizing negative impact while mitigating climate change, sea level rising, salt water intrusion, and tidal surges. This study aims to predict the habitat suitable area of mangroves in East Timor (Timor-Leste) based on machine learning ensemble approach. Mangrove presence data were extracted from the Sentinel-2 satellite data using deep learning based classification. The climate information used downscaled data for long-term averages globally. Habitat suitability was evaluated by ensemble the results of machine learning-based species distribution models. Currently, the area of mangrove habitat is about 0.19% of East Timor, and the area with significant mangrove habitat suitability is about 1.7% of East Timor, accounting for more area than the existing area. In addition, only areas with high habitat suitability for mangroves were extracted from shrubland, grassland, and agricultural land to extract areas suitable for additional mangroves. Areas with high habitat suitability for mangroves in shrubland, grassland, and agricultural land were evaluated to be capable of afforestation by 2,732.9ha in Pante Macassar and 1,452.1ha in Uato-Lari. Our results predict that carbon absorption and storage through additional mangrove afforestation can be expected.


BG07-A019
Microcosm Study to Simulate Effects of Ocean Acidification and Fertilizer Runoff on the Methylmercury Uptake by Marine Copepods

JuHyeong CHAE#+, Seunghee HAN
Gwangju Institute of Science and Technology, Korea, South

Ocean is the largest environmental medium absorbs CO2 released into the atmosphere. The COdissolution causes ocean acidification, resulting in significant impacts on ecosystems. Before the Industrial Revolution, the CO2 concentration in the atmosphere was 280 ppm; this has increased to 420 ppm as of 2022. If the current trend continues, the concentration is likely to become 1,000 ppm by 2100, which corresponds to seawater pH of 7.6. A large proportion of agricultural land is bordered by Yellow Sea, and, freshwater with high nutrients is discharged into the sea, particularly during the monsoon. To determine the combined effect of seawater acidification and fertilizer runoff on the MeHg accumulation in copepods, we constructed microcosm with varying pCO2. The seawater was collected from the Yellow Sea and filtered through 150 um membrane to remove large particles and to contain the natural communities of bacteria, protozoa, and phytoplankton. Copepods were purchased and added to the microcosm along with 5 pM MeHg, to observe: 1) how the microbial food web structures, and the MeHg accumulation in copepods respond to the lower pH of seawater than current pH induced by COdissolution; and 2) the effect of an increase in inorganic nutrients on the food-web structure, and the MeHg accumulation in copepods under the lower pH than current pH. We expect to detect less MeHg accumulation in the copepods due to the dominance of the conventional over the microbial food web under the high-CO2 and high-nutrition conditions. there is a possibility a higher accumulation of MeHg occurs in the copepods under the high-CO2 and high-nutrient condition, caused by copious release of dissolved organic matter from primary producers followed by additional Hg(II) methylation in the seawater. The microcosm simulation for understanding, is currently being carried out to verify whether the hypothesis stated above is valid.


BG07-A021
Spatiotemporal Variations of Organic Carbon and Sterols as Indicators of Primary Production and Ocean Sewage Dumping in the Sediments in the Southwestern Part of the East Sea (Japan Sea)

Minkyoung KIM1+, Jeomshik HWANG2#, Daniel B. MONTLUÇON3, Negar HAGHIPOUR3, Dongyoung KIM4, Chang-Keun KANG4, Young-Il KIM5, Timothy I. EGLINTON3
1Kyungpook National University, Korea, South, 2Seoul National University, Korea, South, 3Swiss Federal Institute of Technology Zürich, Switzerland, 4Gwangju Institute of Science and Technology, Korea, South, 5Korea Institute of Ocean Science & Technology, Korea, South

We examined sedimentary records in the UB (Ulleung Basin), located in the southwestern part of the East Sea and nearby shelf sites to investigate spatiotemporal variations in the depositional environment with a special focus on the various sterols. Sedimentary Organic carbon (SOC) accumulation rate and abundances of planktonic sterols (brassicasterol, cholesterol, and dinosterol) were obtained from 25-cm depth sediment samples. Spatiotemporal variation of coprostanol, a tracer of ocean waste dumping, was also examined to understand the dispersal and preservation of organic matter in this region. This study aims to provide new insights on SOC accumulation in the context of the biological carbon pump and behavior of the sewage in the water and sediments.


BG09-A001
Hand Sanitizers, Disinfectant Washes and Bacterial Cross-resistance to Antibiotics in Environmental Water Sources

S. Q. ZHANG+, Kung Ming LEUNG, Grace LAI, Simon GRIFFIN#
The ISF Academy, Hong Kong SAR

While the WHO has identified increasing antimicrobial resistance (AMR) as a global concern, this is a ‘slow emergency’ and a problem easily neglected in favour of more acute events [1]. In the meantime, of course, levels of AMR may even be unwittingly exacerbated: during the recent COVID epidemic, for example, the liberal use of sanitizers and disinfectants intended to neutralise the SARS-CoV-2 virus is likely to have encouraged bacterial cross-resistance to antibiotics [2], with resistant strains especially prevalent in sewage, grey water, and wastewater recycling facilities. 
In order to track the possible effects of biocides on the levels and spread of AMR, this work comprises two stages. First, the isolation of antibiotic-resistant bacteria from beneath fingernails of a large cohort of subjects has been correlated with individual use of antibacterial agents and, at the same time, DNA extraction and sequencing of these bacterial isolates has allowed the identification of common AMR genes. Second, after the design of relevant primers, PCR testing is used to screen water samples recovered from a variety of sources and locations to understand their distribution and frequency of these AMR genes in the environment. In isolates recovered so far, the dominant resistance to ampicillin and augmentin points to an extended spectrum beta-lactamase, often accompanied by co-resistance to tetracycline. In some isolates, the relevant AMR genes co-occur with qac-family genes for quaternary ammonium salt resistance and plasmid- and transposase-mediated gene transfer allows their rapid dissemination. References
[1] D. Dominey-Howes, Geosci. Lett., 5: 7 (2018) [2] K. R. Harrison, A. D. Kappell, P. J. McNamara, Environ. Pollut., 257: 113472 (2020).


BG09-A002
An Investigation Into the Effects of Glyphosate on the Soil Microbiome

Rosalyn TANG+, Anya N. K. CHAN, Kung Ming LEUNG, Grace LAI, Simon GRIFFIN#
The ISF Academy, Hong Kong SAR

N-(phosphonomethyl)glycerine (glyphosate) is a popular broad-spectrum herbicide that is especially relevant in the Asia-Pacific region, its largest market. Despite concerns over possible human toxicity and its environmental impact, the global market for glyphosate in 2020 was estimated at US$7.6 billion and projected to grow to US$9.3 billion by 2027. Residue levels exceeding 0.5 mg.kg–1 have been reported in soils, large streams and groundwater in both Europe and the USA, and soil conditions and crop mix suggest that USA, Brazil and China are likely to see the highest exposure rates to glyphosate and its persistent breakdown product aminomethyl-phosphonic acid (AMPA) [1].
While human health and the emergence of resistant weeds are often identified as potential problems with glyphosate, as a potent inhibitor of the shikimate pathway for the biosynthesis of aromatic amino acids, the undoubted effects of the compound on the soil microbiome are poorly understood. Given that soil bacteria and fungi perform are key to the cycling of carbon and other nutrients and for sustaining plant growth, this lack of knowledge would seem to represent a major oversight.
This project investigates the effects of glyphosate on the soil microbiome in two ways. First, using soil samples recovered from a 1.5 x 1.5 m test square before and after treatment (on days 0, 3, 7, 14, 28 and monthly thereafter), 16S and ITS1 microbiome profiling of glyphosate-treated soil examines the immediate effects of glyphosate and estimates a recovery time under local conditions. Second, given some controversy about possible antimicrobial co-resistance, glyphosate-resistant bacteria have been identified in a number of soil extracts in order to gain an insight into characteristics that treatment is likely to favour. References: [1] F. Maggi, D. la Cecilia, F. H. M. Tang, A. McBratney, Sci. Total Environ., 717: 137167 (2020).


BG09-A003
Exploring Coffee Suitable Land Based on Socio-environmental Geo-criteria in Timor-Leste

Wonhee CHO1#, Byungwoo CHANG1+, Chul-Hee LIM1, Sue Kyoung LEE2, Ohjung KWON2, Hyeon-Kwon AHN1
1Kookmin University, Korea, South, 2SK Forest, Korea, South

The coffee industry is the largest non-oil export in Timor-Leste. Coffee was introduced by the Portuguese in the 1800s, and it became a major source of income for local communities. The Eremera, Ainaro, Aileu, and Liquica are known as the major municipality for the coffee industry in Timor-Leste. However, the coffee industry is vulnerable to global price fluctuations, lack of capital, and deficient infrastructure. Therefore, this study assesses the land suitability for coffee production, especially Coffea arabica L., in order to estimate the potential area for coffee plantations to support their sustainable industry. For this purpose, a suitability modeler in ArcGIS pro (version 3.0) was used for potential area estimation. Our model integrated 18 spatial inputs categorized as climatological (6), Edaphological (5), Physiographic (3), and Socio-economic (4). Our results confirm that Tatamailau mountainous area in Ermera and Ainaro, and Alieu are suitable for coffee plantations. Also, the results represent the mountainous area in Manatuto and Bobonaro, and the eastern part of Baucau is suitable for coffee plantations. This study can support local communities and governments in Timor-Leste to implement new strategies for coffee plantations and management to increase coffee production and their income. In addition, it can support the development of the local industry models, and afforestation (or reforestation) of the land by the coffee and shade tree can contribute to carbon absorption ability in Timor-Leste.


BG09-A008
Development of the Peptide-detecting Method for On-site Analysis

Miyamoto AI#+, Hajime MITA
Fukuoka Institute of Technology, Japan

One of the mysterious subjects is the origin of life. In 1969, approximately 100 amino acids were found in a meteorite that fell to Murchison, Australia, and glycylglycine was the only peptide found in the meteorite. It is essential to investigate whether peptides are synthesized in space to clarify life’s birthplace. In the Tanpopo, amino acids were exposed to the space environment on the International Space Station (ISS), and dipeptides were synthesized in space under vacuum ultraviolet light. The new space station, Gateway, is starting to construct in lunar orbit. Cosmic radiation at Gateway is stronger than those at ISS by shielding of the Van Allen belts. Therefore, the exposure experiments of peptide syntheses at Gateway are essential for studying peptide synthesis in deep space. It is necessary to analyze samples on-site since there is little opportunity to bring them back to Earth at the Gateway. Therefore, we will develop a simple method to analyze amino acid decrease, and dipeptide formation in space orbit on a cubic sat scale. Amino acid monomers and dipeptides were analyzed by FT-IR spectroscopy and biuret color reactions. FT-IR is acceptable, but a high-resolution one is required. In the biuret reaction, alanine (Ala) did not color, but alanylalanine (Ala-Ala) slightly colored blue. In general, the biuret reaction is a detection method for polypeptides that are longer than tripeptides, and the reaction causes a reddish-purple to bluish-purple color. Since amino acids and dipeptides have been used, this reaction should not normally occur. However, in this experiment, the dipeptides did not turn reddish purple to bluish purple but changed to blue that they could be distinguished from amino acids. In addition, a blue shift was observed depending on the ratio of Ala-Ala to Ala. The details of the biuret reaction are then studied.


BG09-A009
Nucleic Acid Adsorption on Proteinoid Microspheres

Sayaka TAKAHASHI#+, Hajime MITA
Fukuoka Institute of Technology, Japan

As one of the hypotheses for the origin of life, Oparin proposed chemical evolution. Fox and Harada et al. heated monoammonium malate to produce a polyamino acid called proteinoid. They also found that micron-sized spherical particles called microspheres were formed by dissolving proteinoids in hot water. This corresponds to the third stage of the chemical evolution theory, that specific structures such as coacervates are formed by the molecular assembly. The combination of proteins and nucleic acids is thought necessary for the proteinoid microspheres to express a function that leads to the emergence of life as the fourth step in chemical evolution. This study, therefore, investigated the adsorption and uptake of nucleic acids onto the proteinoid microspheres. Sheared salmon sperm DNA was added to a dispersion of proteinoid microspheres. The microspheres were then observed using an electron probe microanalyzer (EPMA). The distribution pattern of phosphorus was consistent with that of the spherical carbon and nitrogen, which were identified as proteinoid microspheres in the SEM images. This confirms that nucleic acids were either uptake into the microspheres or adsorption on the microsphere surface. A reconstitution experiment was also performed. After microspheres with nucleic acids were heated to dissolve and then cooled to reconstitute the microspheres. The EPMA observation confirmed the adsorption or uptake of nucleic acids onto the microspheres. It found that under both different timings of microsphere formation and nucleic acid addition, nucleic acids were adsorbed or taken up by the microspheres. In the future, we will confirm whether nucleic acids are taken up inside the proteinoid microspheres or only adsorbed on the surface. In addition, the functional expression of adsorbed nucleic acids, such as transcription and translation, will be clarified. 


BG09-A010
Synthesisynthesis of Peptides by UV Irradiation and Synthesis of Authentic Peptides

Yoshiki BANZONO1#+, Koyo MIZUNO1, Kaori NAKASHIMA1, Kazumichi NAKAGAWA2, Hajime MITA1
1Fukuoka Institute of Technology, Japan, 2Kobe University, Japan

There are many organisms on Earth today. However, the origin of life on Earth remains unknown. About 100 amino acids and many organic compounds were found in the meteorites. Amino acids, the minimum unit to sustain living organisms, exist in the universe. Still, no peptides have been detected in meteorites, except for glycylglycine. have been reported for the existence of peptides. Studying whether peptides can be synthesized from amino acids in the space environment is essential. It has been reported that alanylalanine is synthesized by vacuum ultraviolet (VUV) irradiation, which is the most common and chemically reactive in the space environment. We, therefore, decided to study the synthesis of peptides from amino acids other than alanine and the formation of co-peptides from mixtures of amino acids. In the first step, thin films prepared by vapor deposition of two amino acids were irradiated with VUV rays. After irradiation, the products were extracted with water, and the extracts were analyzed by liquid chromatography combined with mass spectrometry. It is necessary to examine the authentic samples of peptides for chromatographic analysis. Some peptides were synthesized using DMATMM as a condensation reagent. In addition to the dimers, trimers were synthesized in the peptide synthesis experiments. Using the L-form for the N-terminal amino acids and racemic amino acids for the C-terminal, two peptides were obtained as diastereomers in the dimer and four in the trimer, and their retention times could be determined by chromatography. Using these authentics, it has been shown that the VUV irradiation of a composite thin film of alanine and serine produced co-peptides Ser-Ala. Further analysis of other combinations of amino acids is in progress. The exposure experiment is now underway to expose thin films of mixed amino acids in the natural space environment at the exposed facility on the ISS.


BG10-A007
The Climate Sensitivity of Vegetation in Tropical Asia

Tin SATRIAWAN#+, Jiaqi TIAN, Xiangzhong LUO
National University of Singapore, Singapore

Changes in global climate have been known to alter the productivity of tropical forest vegetation. To better understand the response of tropical forests to climate change, it is important to study the driving factors of vegetation dynamics. Temperature, precipitation, and solar radiation are potential drivers of vegetation dynamics in the tropics, however, their relative contributions vary between regions due to differences in soil type and community composition across tropical forests. The spatial heterogeneity is particularly high in tropical Asia, therefore, it is important to investigate the influence of climate on vegetation dynamics in the region. In this study, we aim to analyze the climate sensitivity of tropical Asia’s vegetation by answering: (1) what are the main climatic drivers influencing tropical Asia’s vegetation? (2) how does the impact of these drivers vary spatially? This study uses multiple satellite products (e.g., GIMMS NDVI and GLASS LAI) as proxies of vegetation seasonality. We use various statistical methods (i.e., multiple linear regression, machine learning) to infer the changes in vegetation seasonality in response to interannual climatic fluctuations (e.g., gridded temperature, precipitation, and solar radiation from CRU JRA, soil moisture from ESA CCI, and vapor pressure deficit). We expect to see larger anomalies of vegetation when climatic fluctuations are the most pronounced, e.g., during El Nino and La Nina years. We also hypothesize that different regions (e.g., continental vs maritime) would have different resistance to interannual climatic variabilities. Ultimately, our findings will help improve our understanding of the vegetation-climate interaction mechanisms and how different regions may respond to climatic changes in the future.


BG10-A013
Observation Site Coordinated to Eddy Covariance and Remote Sensing Techniques to Verify the Ecological and Productive Functions on Rice Paddy in Naju, South Korea

Bo-Kyeong KIM1#+, Jong-Min YEOM2, Jong-Sung HA2, Hyunki KIM3,1, Hyun-Dong MOON1, Euni JO1, Jaeil CHO1
1Chonnam National University, Korea, South, 2Korea Aerospace Research Institute, Korea, South, 3National Institute of Crop Science, Korea, South

Rice is the major staple food, particularly in Asia region. The flooded condition in rice paddy field will affect not only the agricultural productivity but also the surface energy, water, and carbon exchanges compared to other non-flooding crops. In this study, the Naju observation site on the rice paddy field of Jeollanamdo Agricultural Research and Extension Services, Naju, Jeollanam-do Province, Republic of Korea (N 35.026950°, E 126.82195°) was established in 2020. The simultaneous observation system of H2O/CO2/CH4 gases flux and hyperspectral reflectance and chlorophyll fluorescence on vegetated surface could be valuable for extension from the observed phenomenon in ground-scale monitoring to space-based estimation in upper-scale region. Fluxes, such as net ecosystem exchange, methane emission, and evapotranspiration, was observed with an open-path gas analyzer (LI-7500A & LI-7700; LICOR Inc., USA) and three-dimensional sonic anemometer (CSAT3; Campbell Scientific Inc., USA). The GPP could be derived from eddy covariance method and estimated by observing solar-induced chlorophyll fluorescence (SiF) using hyperspectral instrument (FLOX; JB Hyperspectral Devices, Germany), which is also produce the vegetation indices within visible and near infra-red wavelengths. In addition, the drone monitoring installed with 10 multispectral bands and thermal cameras is performed regularly for the ground-based observation area. The various scaled and instrumental data achieved from the Naju observation site will be helpful for comprehensive understanding of rice paddy ecosystem and validation for satellite-based model.


BG10-A015
Understanding the Fine-scale Space Use and Habitat Selection of Invasive Species: Applying Core Habitat Estimation to Improve Management Strategy

Byungwoo CHANG1+, Wonhee CHO1, Chanwoo KO1, Hyemin KIM1, Yongsu PARK2, Dongwook W. KO 1#
1Kookmin University, Korea, South, 2National Institute of Ecology, Korea, South

In order to eradicate invasive species, spatio-temporal analysis information on the behavioral characteristics of wildlife is important. In previous invasive species management studies, GPS collars were attached to track their movement and the traditional home range estimation technique was used to estimate their home range area. However, for the intensive management of invasive species, new analysis methods are required to consider the behavioral and ecological characteristics of target species in terms of activity patterns at core habitats. Nutria (Myocastor coypus) is a representative invasive species that destroys native ecosystems worldwide. It was introduced to South Korea in 1985 for their economic value (fur farming and food resources), but quickly settled after illegal release. Nutria, a semi-aquatic mammal, mainly lives along the banks of lakes and rivers, building burrows for shelter. Therefore, by analyzing their activity patterns in their critical habitats, it may be possible to obtain information at the particular location of nutria burrows. In this study, we applied the method of analyzing intensity of use within the range of movement to analyze the activity patterns of nutria inhabiting the Upo wetland in Changnyeong-gun, South Korea. We used GPS tracking data of nutria (n=3) to identify the core habitat areas and calculate the revisitation rate of these areas along the movement path. In addition, we analyzed the concentration of specific space use by period and individual, created density map, and identified the particular locations at the core habitats. The results of this study are expected to contribute to the effective control and management of nutria by providing fundamental data for understanding the behavioral characteristics related to their use of burrows.


Thu-03 Aug | 1:10 - 3:10 | MR305
BG06 - Integrated Understanding of Global Carbon and Other Biogeochemical Cycles and Their Feedbacks

Session Chair(s): Bharat SHARMA, Oak Ridge National Laboratory, Forrest HOFFMAN, Oak Ridge National Laboratory, Masayuki KONDO, Hiroshima University

BG06-A018
CO2 Budget Assessment of Southeast Asia for the 1980s−2010s and State Toward Realizing Carbon Neutrality

Masayuki KONDO1#+, Prabir K. PATRA2,3
1Hiroshima University, 2Japan Agency for Marine-Earth Science and Technology, 3Tohoku University

Southeast Asia is a complex geographical and geopolitical region. It has mainland and insular regions dominated by tropical rainforests and croplands, with savanna woodlands in the northern part. Forest cover constitutes 236 mha, corresponding to approximately 15% of the world’s tropical forests. A large part of Southeast Asia is considered a biodiversity hotspot because it harbors a high number of endemic species, especially the greatest diversity of mangrove species in the world. On top of the complexity and diversity of ecosystems, two major factors controlling the dynamics of carbon uptake and release makes Southeast Asia a region challenging to assess the carbon budget (a net exchange of carbon in and out of the territorial boundaries of a certain region): (1) the large inter-annual climate variability due to El Niño Southern Oscillation (ENSO) cycles, and (2) the forest loss due to land-use and land-cover changes (LULCC). Notably, synergies between ENSO-driven droughts and rapid LULCC have resulted in a number of extreme episodes of carbon emissions into the atmosphere, particularly when fire plays a role. For being a region characterized by the key factors that exacerbate carbon emissions, attention has been paid to whether carbon neutrality can be achieved in Southeast Asia. As a part of the RECCAP2 activities, this study establishes (1) the recent four decadal budgets (the 1980s to 2010s) of carbon dioxide (CO2) of Southeast Asia, (2) its inter-decadal variability, and (3) the natural and human-driven attributions to the CO2 budgets. We achieve the four objectives by analyzing three independent approaches for CO2 budget estimation: top-down estimates of the net CO2 flux from atmospheric inversions, bottom-up estimates integrating components of the CO2 budget, and carbon stock change estimates from microwave remote sensing.


BG06-A008
Enhanced India-Africa Carbon Uptake and Asia-Pacific Carbon Release Associated with the 2019 Extreme Positive Indian Ocean Dipole

Jun WANG#+, Fei JIANG
Nanjing University

The 2019 extreme positive Indian Ocean dipole drove climate extremes over Indian Ocean rim countries with unclear carbon-cycle responses. We investigated its impact on net biome productivity (NBP) and its constituent fluxes, using the Global Carbon Assimilation System (GCASv2) product, process-based model simulations from TRENDYv9, and satellite-based gross primary productivity (GPP). By distinguishing two separate regions, the India–Africa and Asia–Pacific, GCASv2 indicated enhanced terrestrial carbon uptake of 0.23±0.20 PgC and release of 0.38±0.15 PgC, respectively, during September–December 2019. These NBP anomalies had comparable magnitudes to those following the 2015 extreme El Niño which, however, caused the consistent carbon release in both regions. The TRENDYv9 model ensemble confirmed these NBP responses, albeit with smaller magnitudes. These regional NBP anomalies were related to soil moisture variations with a dominant role of GPP. Understanding the impact of IOD provides new insights into mechanisms driving interannual variations in regional carbon cycling.


BG06-A016
Characterizing the Variability of XCO2 and Fluxes Over Global Tropics Using OCO-2 Satellite Observations and Model Simulations

Ravi Kumar KUNCHALA1#+, Chiranjit DAS1, Prabir K. PATRA2,3, Naveen CHANDRA2
1Indian Institute of Technology Delhi, 2Japan Agency for Marine-Earth Science and Technology, 3Tohoku University

Developing and implementing mitigation strategies for greenhouse gas emissions and related climate change require an understanding of the sources and sinks of CO2. Carbon dioxide (CO2) is the most significant anthropogenic greenhouse gas in the atmosphere, contributes to climate change and global warming. The recent significant increase in anthropogenic CO2 emissions mostly attributable to the burning of fossil fuels, the production of cement, and changes in land use (Canadell et al., 2021; Friedlingstein et al., 2022). The underlying uptake and release of CO2 by surface processes and atmospheric transport are represented in the spatiotemporal variations in atmospheric CO2. With developments in the space based observations of column averaged atmospheric CO2 (XCO2) we obtain wider and denser spatial coverage to constrain the fluxes at both global and regional scales, compared to the existing high quality in-situ observation network. This study is aimed to understand the regional scale CO2 concentration and flux variability in the region of climate-sensitive tropical land region, which is facilitated by OCO-2 observations and the global chemistry-transport model MIROC4-ACTM. The difference in model-OCO-2 has shown more than ±1 ppm bias in global tropics, especially over Amazon rainforest and South Asia. In addition, we will focus to use of the aircraft observations to further examine the differences in the vertical distribution of CO2 together with the model simulations. This will provide an opportunity to understand deficiency in the model simulating CO2 variability at different altitudes, if any, as well as to examine the impact of underlying flux signals and transport in different temporal scale and discuss possible uncertainties or regional biases in OCO-2 retrievals.


BG06-A017
The Impact of Hydroxyl Radical (OH) on the Trend and Variability of Global and Regional Methane Budget

Dmitry BELIKOV1#, Prabir K. PATRA2,3+, Naoko SAITOH1
1Chiba University, 2Japan Agency for Marine-Earth Science and Technology, 3Tohoku University

The rise in methane (CH4) levels in the Earth's atmosphere has more than doubled since pre-industrial times, contributing to the greenhouse effect and increasing radiative forcing by 0.62 W/m2 from 1750 to 2011. While total global CH4 emissions are well-constrained by atmospheric data, estimates of emissions from different sources or at the regional level can vary. Interannual variations of CH4 levels are not well understood due to uncertainties in the CH4 sink, which is caused mainly (up to 90%) by the reaction with the hydroxyl radical (OH). There are differences between OH levels estimated using bottom-up and top-down methods, leading to varying CH4 sink estimates (Patra et al., JGR, 2021; Spoza et al., IPCC AR6 WG1, Chapter 6). Improving the understanding of CH4 emissions and their impact on the atmosphere requires better incorporation of 3D simulations from atmospheric chemistry models in atmospheric inversions. In this study, the impact of OH on CH4 emissions was quantified during 2001-2021 using an atmospheric chemistry-transport model (i.e., MIROC4-ACTM) and atmospheric measurements from 60 sites. The study aimed to better understand OH production and loss processes and assess their impact on the CH4 lifetime and the global CH4 budget on a decadal scale. The results showed that anthropogenic emissions were better estimated in regions dominated by human activities and that the magnitude of interannual variations varied due to natural climate events such as the El Nino Southern Oscillation. Further sensitivity experiments by changing anthropogenic emission trends were performed to assess our ability to derive regional emission trends by the inverse modeling system. The study contributes to a better understanding of CH4 emissions and their impact on the atmosphere and highlights the importance of incorporating 3D simulations in atmospheric inversions to improve CH4 emission estimates.


BG06-A019
Magnitude and Trajectory of Carbon Emissions Induced by Land Use and Land Cover Changes in Southeast Asia in the Twenty-first Century

Ruiying ZHAO#+, Xiangzhong LUO
National University of Singapore

Southeast Asia is a global hotspot of land use and land cover changes (LULCC), which has substantially impacted the regional carbon budget. However, the magnitude and trend of LULCC-induced carbon emissions vary substantially across current Bookkeeping or DGVM models, highlighting a lack of constraint of LULCC-relevant carbon processes. To obtain an accurate quantification of carbon uptake and emissions caused by LULCC and identify dominate changes of carbon processes, we used a diagnostic terrestrial biosphere model (BEPS) to simulate the relevant processes. We use multiple fine-resolution (500 m) state-of-the-art satellite-derived biophysical and biochemical variables to constrain the carbon uptake process in the models. We test five existing LULCC datasets (ESACCI, MCD12Q1, GLCC, GlobalLand30, HANSEN product) when quantifying LUCC-drive CO2 fluxes. To further explore the impacts of LULCC on C turnover processes, we further disentangled the relative impact of LULCC on C-pool and C-flux components based on the Lindeman-Merenda-Gold (LMG) approach. Our findings were also compared with outputs from an ensemble of Dynamic Global Vegetation Models and Bookkeeping models. Our study provided a new quantification of C emissions associated with LULCC in Southeastern Asia, which can better support global carbon budget accounting.


BG06-A015
Evolution of Uncertainty in Terrestrial Carbon Storage in Earth System Models from CMIP5 to CMIP6

Ning WEI1+, Jianyang XIA1#, Jian ZHOU2, Lifen JIANG3, Erqian CUI1, Jiaye PING1, Yiqi LUO2
1East China Normal University, 2Cornell University, 3Northern Arizona University

The contemporary terrestrial carbon storage is key to predicting future climate change due to the significant biogeochemical feedbacks between the land and atmosphere. However, Earth system models (ESMs), which fully coupled climate-carbon cycle feedbacks, have great uncertainty on quantifying the global terrestrial carbon storage. Based on multiple global datasets and a traceability analysis, we diagnose the uncertainty source of terrestrial carbon storage in 22 ESMs that participate in the 5th and 6th phases of the Coupled Model Intercomparison Project (CMIP5 and CMIP6). We detect that the modeled global terrestrial carbon storage is converging among ESMs from CMIP5 (1936.9 ± 739.3 PgC) to CMIP6 (1774.4 ± 439.0 PgC), but is persistently lower than the observation-based estimates (2285 ± 669 PgC). By further decomposing terrestrial carbon storage into net primary production and ecosystem carbon residence time. We find that the decreased inter-model spread in land carbon storage primarily results from more accurate simulations on terrestrial productivity among ESMs from CMIP5 to CMIP6. The persistent underestimation of land carbon storage is caused by the biased ecosystem carbon residence time in both CMIPs, which is far shorter than the observation-based estimates. Moreover, the modeled ecosystem carbon residence time becomes the key driver for the inter-model spread in global land carbon storage in CMIP6. Overall, this study indicates that CMIP6 models have greatly improved in the terrestrial carbon cycle, with a decreased model spread in global terrestrial carbon storage and less uncertain productivity. However, more efforts are urgently in need to improve model performance in terrestrial carbon residence time.


Thu-03 Aug | 3:30 - 5:15 | MR305
BG02 - The Mesozoic World: Knowns and Unknowns

Session Chair(s): Su-Chin CHANG, The University of Hong Kong, Daran ZHENG, Chinese Academy of Sciences

BG02-A006 | Invited
Divergent Orbital Forcing in Early Jurassic Climate and Carbon Cycle Revealed by the High-latitude Continental Junggar Basin

Yanan FANG#+
Chinese Academy of Sciences

Orbital-pacing cyclic insolation variations are the primary external forcing on the Earth’s climate system. However, their effect on the climate and carbon cycle (the key component of the climate feedback system) remains unclear in the greenhouse worlds, especially those before the Cenozoic, due to the lack of long and continuous geological records. The Early Jurassic is a typical greenhouse period characterized by extremely high levels of atmospheric Pco2 (partial pressure of CO2). Here, we present high-resolution analysis of relative lake levels based on depth rank data (a series of numerical facies), total organic carbon (TOC) and stable carbon isotope (δ13CTOC) datasets from the thick, continuous, lacustrine sequences of the paleo-high-latitude Junggar Basin of northwestern China. Our results indicate that climate/hydrological variability in the Early Jurassic high latitudes was dominated by the 405 kyr eccentricity cycle, which is consistent with the contemporaneous low latitudes. However, the dominant pacemaker in the carbon isotope values of bulk organic matter (δ13CTOC) is the ~1.2 Myr inclination cycle. The δ13CTOC shifts are related to the atmospheric carbon pool fluctuations supported by the consistent shifts from wood particles (δ13Cwood) and long-chain n-alkanes (δ13Calk). Our results for the first time point to divergent orbital forcing on the global climatic/hydrological changes and carbon cycle in the Early Jurassic. Our findings not only highlight the sensitivity of high-latitude carbon reservoirs to the inclination and obliquity pacing insolation changes and their decisive control on the global carbon cycle, but also contribute to our understanding of the complex climate systems at orbital scale in greenhouse worlds.


BG02-A002
Seed Ferns from the Triassic Karamay Formation in the Junggar Basin, Northwestern China, and Their Implications

Yangyang XIA1#+, Su-Chin CHANG1, Daran ZHENG2
1The University of Hong Kong, 2Chinese Academy of Sciences

Seed ferns discovered from the Upper Permian to the Upper Triassic strata worldwide provide important clues to the global Triassic stratigraphic correlations. Despite their abundance, the epidermal anatomical characteristics of pteridosperm remain poorly understood due to the rare occurrence of compression specimens. Understanding the detailed characteristics of this type of plant will allow the reconstruction of the paleoenvironment and paleoclimate. Since joining HKU in the fall of 2021, I have conducted fieldwork in the Junggar Basin of NW China, which preserves one of the most complete Permian-Triassic terrestrial sediments worldwide. I aim to systematically study the epidermal anatomy of key pteridosperm fossils. Furthermore, I will reconstruct the paleo atmospheric carbon dioxide concentration based on a statistical analysis of stomatal density (SD) and stomatal index (SI) from the plant fossils. This study will improve our understanding of the terrestrial recovery after the most severe mass extinction events in the Earth’s history and will provide significant information on the environmental circumstances that may impact the Triassic ecosystems.


BG02-A003
Age for the Fossil-rich Reshuitang Beds in NE China and its Implications

Yuling LI1+, Su-Chin CHANG1#, Haichun ZHANG2, Jun WANG3, Daran ZHENG2, Yan FANG2
1The University of Hong Kong, 2Chinese Academy of Sciences, 3Yunnan University

The Jurassic Reshuitang beds of northeastern China contain various terrestrial invertebrate and vertebrate fossils, especially including well-preserved larval and adult salamander specimens. Since the beginning of the 21st century, these discoveries have allowed the understanding of salamander body outlines, gill rakers and external gill filaments, caudal fins, eyes, and other organs. Thus, the Reshuitang fossils provide a rare opportunity to conduct a multifaceted study of phylogeny, life-history features, and paleoecology of early salamanders. Fossil-rich beds of the Reshiutang, however, lack adequate stratigraphic and geochronological constraints. Here we report robust 40Ar/39Ar ages of 161.4 ± 0.8 Ma and 161.6 ± 0.6 Ma for two tuff layers lying directly above salamander fossil-bearing beds in Reshuitang Village, Lingyuan City, Liaoning, China. Our new age data indicate that the Reshuitang fossil beds were deposited contemporaneously with the well-known Daohugou fossil beds, ~15 km apart. Given interpretations that the Daohugou beds host the oldest known crown-group salamanders, we propose that the correlative Reshuitang beds also host the earliest crown-group salamanders. This work provides accurate chronostratigraphic constraints on early salamander evolution and diversification.


BG02-A005
Calibrating the Early Jehol Biota in Luanping, Northeastern China

Daran ZHENG#+
Chinese Academy of Sciences

The Jehol Biota sensu stricto consists of numerous exceptionally well preserved fossils typically found in the Yixian and Jiufotang formations of northeastern China. These respectively record the middle and late evolutionary stages of the Jehol Biota. The Dabeigou Formation appears in outcrop in Luanping, Chengde, northern Hebei and hosts the early Jehol Biota as documented by the presence of representative Ephemeropsis trisetalis (insect) and Peipiaosteus (fish) fossils. Although biostratigraphic constraints have been established for this formation, uncertainties persist regarding its exact age range and especially its time of inception. The present study describes U-Pb geochronological results which date the Zhangjiakou and Dabeigou formations found in the Yushuxia outcrop of Luanping. Results indicate an upper age constraint of 134.8 Ma for the Zhangjiakou Formation and an overall age range of 134.5-129.3 Ma for the Dabeigou Formation. Integrated analysis of biostratigraphy and geochronology indicate that the Dabeigou Formation and the Sichakou Sedimentary Member of the Huajiying Formation in Fengning, Chengde, northern Hebei, generally correlate with Members 2 and 3 of the Dabeigou Formation in Luanping. Previous studies do not reach in consistent of which formation contains the early evolutionary stages of the Jehol Biota. This study supports that the Dabeigou Formation in Luanping bears the early Jehol Biota.



Hydrological Sciences


Mon-31 Jul | 8:15 - 10:00 | MR307
HS12 - Climate Change Impacts on Regional Hydrological Issues: Projections and Adaptations Strategies

Session Chair(s): Shuichi KURE, Toyama Prefectural University

HS12-A008
Effective Flooding Modelling Under the Characteristics of Construction and Management of Cities in China

Chun-Yao HOU#+, Yan WANG, Shuwei WANG
Suzhou Yuhong Water Tech. Ltd.

In recent years, cities in China have been constantly affected by extreme weather, and extreme rainfall has also caused significant economic and life losses. Therefore, the demand for efficient urban flood models in China is constantly increasing for disaster prevention and management purposes. However, due to the different construction characteristics and management methods of cities in China compared to other countries, the simulation experience commonly used in other cities cannot be directly applied in Chinese cities. The largest feature of city construction in China is that each plot will have a wall at the boundary, blocking the connection between plots, and only the entrance and exit can be entered and exited, which also means that the surface runoff in the plot can only flow out through the plot stormwater pipe and the entrance and exit of the plot. In terms of management, information related to drainage and flood prevention is held by different government departments and units, and the content, accuracy, and timeliness of the information is also insufficient. In addition, most Chinese cities currently lack relevant hydrological monitoring data for model calibration and validation work. Therefore, the principle of building an efficient urban flooding model in China is to outline the plot walls as subcatchments and block lines, and the outfall of the subcatchment is set near the plot exit by the manhole of the municipal stormwater pipe. The road section is divided into the catchment area of each manhole of municipal stormwater pipe using the Thiessen polygon method. With this principle, the actual surface runoff behavior in Chinese cities can be better reflected and simulation errors caused by various factors can be reduced.


HS12-A014
New Flood Hazard Information Based on Risk Assessment of Levees of Rivers in Toyama Prefecture, Japan

Shintaro MATSUMOTO#+, Shuichi KURE
Toyama Prefectural University

This study presents new flood hazard information for the entire Toyama Prefecture in order to clearly identify truly high-risk areas for the selection of flood damage prevention zones, which is one of the measures for flood control in river basins. Specifically, we calculated the inundation probability, floor inundation probability, and horizontal evacuation probability at each point of the target area, based on an evaluation of levee erosion risk. 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. The flood inundation analysis was conducted for the Oyabe River, Sho River, Joganji River, and Kurobe River in Toyama Prefecture, Japan. The results obtained from the flood inundation analysis were used to calculate the probability of inundation, inundation above floor level, and horizontal evacuation probabilities by classifying the "risk of the ground" according to the magnitude of the inundation depth and flow velocity. The risk assessment of levees was also taken into account during the calculation of each probability. The risk assessment of levees using the erosion potential assessment of Ishikawa et al. was used in this study. From the results of the analysis in this study, the importance of considering the levee erosion risk for the flood hazard information was confirmed.


HS12-A004
Probable Maximum Precipitation Projection Using CORDEX-EA in Soyang Dam, South Korea

Ju-Young SHIN1#+, Ji-Hye KWON2, Sunghun KIM3, Jun-Haeng HEO3
1Kookmin University, 2SISTECH, 3Yonsei University

The climate change has altered characteristics of heavy rainfall events in various regions. This change will lead to increases or decreases in rainfall depth. To mitigate the impacts of climate change on adverse risks from changes in rainfall events, the possible scenarios of rainfall events induced by climate change should be adopted. The probable maximum precipitation (PMP) has been frequently employed for design criteria of mega hydraulic infrastructure like dam and spillway. PMP may be changed by the climate change, and changes in PMP eventually lead to reinforce the design of these infrastructure facilities. Hence, this study investigated the possible scenarios of PMP change induced by climate change using climate change scenarios. The PMP should have sub-daily duration. Thus, climate change scenarios have high temporal resolution. In this study, CORDEX-EA phase 2 that simulated by output of CMIP6 earth system model was used for projecting the future PMP. To correct biases, precipitation observations in 615 stations were employed. There are large spatial variations in changes in PMP in South Korea. For example, the PMP in some stations largely increases while the PMP decreases in some stations. Overall, the amount of PMP may be increased in the future.


HS12-A021
Basin-scale Trend Analysis of Hydro-climatic Variables from Historical to Projected CMIP5 Future

Sushree Swagatika SWAIN1#+, Ashok MISHRA2, Chandranath CHATTERJEE2
1Research Scholar, 2Indian Institute of Technology Kharagpur

In almost all water resources management projects, there is an implicit assumption of ‘stationarity’, which denotes the time-invariant statistical properties of hydro-climatic variables under consideration. In light of global climate change due to increased greenhouse gases, such assumptions cannot be reliable. Considering these assumptions result in inefficiencies in regional water resources management. Thus it is necessary to study the temporal trends of climate change at a regional scale. To address the above concerns, this work attempts to study the temporal trends of rainfall, temperature and streamflow of the Brahmani-Baitarani river basins, neighbouring basins of eastern India. The study of historical trends is shown in the observed rainfall and temperature data using India Meteorological Department (IMD), Pune. Using the observed discharge data from the Central Water Commission (CWC), Bhubaneswar, the trends of streamflow are presented. To observe the future trends of hydro-climatic variables, the rainfall, temperature and streamflow are obtained from the Coordinated Regional Downscaling Experiment (CORDEX) simulations. These are the coordinated climate change experiments of the fifth phase of the Coupled Model Intercomparison Project (CMIP5) family. Usually, the CORDEX data provides detailed information about climate change and its impact on a regional scale. With the advantage of modest data requirement and simple concept, a Linear Scaling (LS) concept is employed to adjust the biases in projected climate models. A widely used linear regression-based trend analysis approach is fitted to observed and projected hydro-climatic variables using a generalized least-square regression function to study the temporal correlation and variations. The future trends analysis is performed for two Representative Concentration Pathways (RCPs) 4.5 and 8.5. With the decreasing rainfall and increasing temperature patterns, the decline in future streamflow is observed from the trend analysis. The depletion of river basin streamflow is a potential risk to existing as well as long-term water management policies.


HS12-A015
Assessment of Impact of 1.5-degree Celsius Increase Due to Global Warming on Flood and Erosion Risk in Rivers in Toyama Prefecture, Japan

Ryuto FUJISHITA#+, Shuichi KURE
Toyama Prefectural University

In Japan, floods caused by typhoons and frontal rains occur every year, causing massive damage to human lives and property. Although multiple hazard and risk assessments have been conducted for Japanese rivers, hazard assessments considering the climate change impact are inadequate. In addition, since the recent target is to keep the global temperature increase within 1.5°C, it has become important to assess the impact of flooding under the situation of a 1.5°C increase. Therefore, in this study, rainfall-runoff simulations were conducted for all rivers in Toyama Prefecture, Japan considering the climate change impact to evaluate the potential increase in river flood and erosion risks. Also, the effects of lowering water levels by removing vegetation from river channels and applying paddy dams as global warming adaptation measures when the temperature rises by 1.5°C were evaluated. Rainfall data from the d4PDF dataset was used to project future climate situations. The erosion potential assessment indicated that there is a risk of erosion in bends and high gradients of the target river. The global warming adaptation assessment showed that all adaptation measures are effective in the Oyabe River. This may be due to the fact that the Oyabe River has a large amount of vegetation in the river channel and a higher ratio of paddy land use in the watershed compared to other rivers.


Mon-31 Jul | 8:15 - 10:00 | MR323
HS01 - Challenges in Hydrologic Modeling

Session Chair(s): Deepthi B, Indian Institute of Technology Bombay

HS01-A016
Challenges in Modelling Soil Water, Heat and Salt Dynamics with Crop Growth in Arid Regions

Xiaomin MAO#+
China Agricultural University

Water shortage and soil salinization are two restricting factors for agricultural development in Northwest China. Drip irrigation under film mulching is widely used to enhance the crop water productivity, meanwhile producing more soil salinization problems potentially. Modelling the soil water, heat and salt dynamics and their interactions with crop growth is essential for scientific agricultural management in order to save water, control salinization and ensure crop yield. We reviewed the current advancements and challenges in this process modelling, which include the soil-water-salt interactions, the hydrogeochemical reactions, the heat budget and partition with canopy cover and film mulch, and the heterogeneity caused by the partial film mulching in the common row seeding farmland. In particular, we introduced our work of a recently finished National Scientific Fund of China (NSFC) key project which aimed to dealing with quantification of soil water and salt dynamics in farmland, and our ongoing work supported by National key research and development program for dealing with soil water, heat and salt dynamics in both crop growing and fallow (with soil thawing and freezing) seasons.


HS01-A003
Development of an AI Model for Extreme Flood Event Prediction

Haneul LEE#+, Seonuk BAEK, Joonhak LEE, Seongcheol SHIN, Hung Soo KIM, Soojun KIM
Inha University

Global warming has accelerated since the Industrial Revolution, and the increase in surface temperature caused by global warming has increased the frequency and scale of rainfall. As a result, flood damage is occurring all over the world, and the scale of flood damage has gradually increased, and the term "climate disaster" has recently been mentioned. In the case of South Korea, floods in 2020 caused huge loss of KRW 1.2 trillion, and heavy rainfall accounted for 60% of the damage caused by natural disasters in 2021. In order to reduce flood damage, the water level of rivers is predicted using a hydrological model, and flood warnings are performed based on the river water level. However, in the case of a hydrologic model, many parameter values are required, and since the parameters must be changed according to rainfall events, it takes a long time to perform a flood warning. In the case of an AI model, if the model is trained in advance, it can estimate the runoff without estimating parameters. However, in the case of South Korea, there is not enough data on extreme flood events, so when learning AI models, the learning weight is biased low runoff. Therefore, there is a limit to predicting the peak of the flood. Therefore, in this study, we tried to develop an AI model to predict extreme flood events. In order to construct dependent variables of the AI model, extreme flood events were extracted from water level observation data. In addition, extreme flood events was generated using a hydrological model for getting sufficient data of AI model. Ai model for predicting the peak time and volume of an extreme flood events was developed and evaluated.


HS01-A034
Complex Networks for Hydrologic Modeling: Progress and Future

Bellie SIVAKUMAR1,2#+
1Indian Institute of Technology Bombay, 2Tsinghua University

Hydrologic systems are complex nonlinear dynamically-evolving systems, made up of a large number of interconnected components that change both in space and in time. In recent years, the concepts of complex networks have been gaining significant attention in studying the various types of connections in hydrologic systems. The purpose of the present study is to discuss the progress in the applications of the concepts of complex networks to hydrologic systems and offer some potential directions for the future. First, some key concepts of complex networks and their relevance to address problems associated with hydrologic systems are presented. Next, various applications of complex networks-based concepts to hydrologic systems are reviewed, including those for representing connections (spatial, temporal and spatio-temporal), prediction, identification of optimal monitoring networks, ranking of global climate models, and development of a catchment classification framework, among others. Finally, some specific directions to address future grand challenges associated with hydrologic systems are highlighted.


HS01-A015
Physics-informed Neural Networks for 1D Shallow Water Equations

Van Giang NGUYEN+, Xuan-Hien LE, Sungho JUNG, Giha LEE#
Kyungpook National University

Understanding the characteristics of water flow regimes is essential for river engineers. In this study, we focus on the study of 1D Shallow Water Equations (SWEs) that are utilized for describing the moving of water in the channels or rivers. Solving SWEs by traditional numerical produces such as finite differences and finite volume methods is generally challenging because of the non-linearity behaviors of SWEs. In addition, these methods could be computationally expensive in certain situations. To overcome these challenges, a Physics-Informed Neural Network (PINNs) approach to solving SWEs has been investigated. PINNs, which integrates both neural networks and the physics laws in the training process, can eliminate the notoriously data-hungry traditional neural network. The core idea of this approach is adding physic constraints to the loss function of the neural network. The accuracy and efficiency of PINNs were evaluated for unsteady flow in a trapezoidal channel. Furthermore, the results achieved from PINNs were also compared directly with high-fidelity simulation results from the numerical model. The results showed that PINNs be able to produce similar numerical model. Moreover, by leveraging the power of neural networks and integrating physical knowledge, PINNs could output effective solutions in solving problems in hydrology and water resources.


HS01-A007
Influence of the Temporal Resolution on the Ranking of General Circulation Models: A Complex Networks-based Approach

Deepthi B1#+, Bellie SIVAKUMAR1,2
1Indian Institute of Technology Bombay, 2Tsinghua University

Selection of suitable General Circulation Models (GCMs) reduces the uncertainty associated with their outputs while assessing the impact of climate change in a region. The present study uses the concepts of complex networks to evaluate the ability of 15 GCMs from the Coupled Model Intercomparison Project phase 6 (CMIP6). They are evaluated based on their ability to simulate the precipitation in India, across 288 grids, for the period 1961-2014. We have considered two different temporal resolutions; Daily; and Monthly, to identify whether the temporal resolution has any influence on the ranking of GCMs. The shortest path is employed as the network measure to evaluate the performance of GCMs. In the present study, each grid is considered as a network, and the scalar rainfall time series is represented in higher-dimensional space using the phase-space reconstruction concept. Each reconstructed vector is considered as a node in the network, and the connections between the vectors serve as the links. The false nearest neighbor method is used to determine the optimum embedding dimension for phase-space reconstruction. The GCMs are ranked at each grid based on the difference in the average shortest path length between the observed rainfall network and the GCM-simulated rainfall network. Finally, the group decision-making (GDM) methodology is used to rank the GCMs for the entire study area, considering all 288 grids. The results suggest that the models GFDL-ESM4, TaiESM1, ACCESS-ESM-1-5, EC-EARTH3, and CMCC-ESM2 are, in order, the five best-performing models for daily resolution. For monthly resolution, the models EC-EARTH3, GFDL-ESM4, MIROC6, TaiESM1, and NorESM2-LM are, in order, the five best-performing models. The models ACCESS-ESM-1-5, NorESM2-LM and MIROC6 occupies the 3rd (14th), 11th (5th) and 10th(3rd) position for daily(monthly) resolution, respectively. Hence, the ranking of GCMs varies according to the temporal resolution of the simulated data.


HS01-A039
Sub-basin Scale Simulation of Profile Soil Moisture by Assimilating Multi-source Information Into a Conceptual Hydrological Model

Qiaoling LI#+, Xingwen LIU, Zhijia LI
Hohai University

The profile soil moisture (PSM) in a conceptual hydrological model is generally derived from measured rainfall, evaporation and other data, which often causes the accumulation of PSM errors. While coupling satellite remotely sensed soil moisture products with hydrological models can lead to more realistic PSMs, coarse resolution and high hysteresis limit their further applications. The objective of this study is to employ both multi-sources remote sensed data and in-situ real-time soil moisture stations in the calculation of spatial PSM, which is essential for hydrological modeling and real-time flood forecasting.2D Triple-Collocation (2D-TC) method and machine learning models were selected for the evaluation, fusion and downscaling of SMAP, ASCAT, and CLDAS soil moisture products. Several machine learning models were built based on the downscaling spatial soil moisture (1×1km2, daily) and in-situ real-time soil moisture data. The models were used to transfer the point station data into the sub-basin scale as the corrected PSM. The conceptual Xinanjiang model with three-layer (WU, WL, WD) soil moisture was applied to the Wuqiangxi Reservior of China. The basin was divided into a set of sub-basins for the soil moisture and flood simulation at daily scale. The corrected PSM data was subsequently assimilated into the Xinanjiang model for updating WU, WL and W based on an autoregression error model and a water balance equation. The comparison analyses show that the corrected PSM matched well with the W and WL simulated by the Xianjiang model, and the R value was increased by 3.9% and 4.2% respectively compared with only using in-situ real-time soil moisture data. The accuracy was improved in terms of Nash Efficiency coefficient by using the assimilation data, particularly for the rising limb on a flood hydrograph. The corrected PSM data and related techniques are useful for real-time flood forecasting at basin scale.


Mon-31 Jul | 8:15 - 10:00 | MR330
HS07 - Impact, Risk, and Predictability of Compound Hydroclimatic Extremes in a Changing Environment

Session Chair(s): Jonghun KAM, Pohang University of Science and Technology

HS07-A001 | Invited
Mechanism and Prediction of the 2022 Compound Hot Drought Over Southern China

Xing YUAN#+, Yumiao WANG
Nanjing University of Information Science & Technology

A mega hot drought occurred in the summer of 2022 in southern China, and affected 2.85 million hectares of crops and water supply for 4.73 million people. With the strongest rainfall deficit and hottest temperature since 1961, the hot drought developed from less than 20% of the Yangtze River basin at the beginning of July to more than 80% of the basin in the mid-August, which is unprecedent due to its rapid intensification and wide coverage. Here, we investigate multi-scale causes of the mega-hot drought including the land-atmospheric dry coupling at sub-seasonal time scale, the link with La Niña and PDO at interannual to decadal scales, and the effect of anthropogenic climate change. The subseasonal-to-seasonal (S2S) climate forecast models and the NMME seasonal prediction models will be used to assess the forecast skill of the drought onset, and a copula-based method will be implemented to predict the probability of drought recovery. Lastly, the future risk of the mega-hot drought will also be investigated by using CMIP6 models.


HS07-A003
Intensifying Response of Global Ecosystem Productivity to Flash Droughts Under Climate Warming

Miao ZHANG+, Xing YUAN#
Nanjing University of Information Science & Technology

The increasing occurrence of flash droughts with rapid onsets poses a great threat to ecosystem productivity. More evidence shows that the global terrestrial ecosystem is more vulnerable to short-term climate extremes, yet little is known about how the response of ecosystem productivity to flash drought at the global scale and whether it evolves over time. Here we propose a flash drought response framework to analyze the resistance of ecosystem gross primary productivity (GPP) to flash droughts, in conjunction with satellite-derived solar-induced chlorophyll fluorescence (SIF) and GPP around the globe. We found that ecosystem productivity over wetter regions shows higher resistance to flash drought, whereas GPP over drier regions shows quicker and more intensive response to flash drought. Surprisingly, the resistance shows a significant declining trend especially for forests, which may relate to intensifying atmospheric dryness and soil moisture drought.


HS07-A005
Risk Assessments of Compound Droughts and Hot Events at the Global Scale

Yitong ZHANG+, Zengchao HAO#, Qian MA
Beijing Normal University

Compound dry and hot events or extremes (CDHEs), which are commonly defined as the concurrent or consecutive occurrences of droughts and hot extremes, have caused severe impacts on human and ecological systems. These events can lower water levels, reduce crop yields, or escalate wildfires. Moreover, recent studies show an increased frequency of CDHEs across most global land areas in the future with continued global warming. This calls for improved efforts in the risk assessments of these extremes to provide useful insights for mitigation. In this study, we explored the risk of CDHEs at the global scale for the future periods based on observations and simulations from CMIP6 models. The changes in different risk components were first assessed to understand their variations under global warming. We then constructed the risk assessment model for the CDHEs across the globe. Results showed an increased risk of CDHEs in large regions across global land areas. This study can be useful for developing adaptation measures under a changing climate. 


HS07-A010
Spatially Synchronized Occurrence of Global Droughts and Floods Revealed by Multi-layer Complex Networks

Hui-Min WANG+, Xiaogang HE#
National University of Singapore

Large-scale droughts and floods are among the most devastating natural disasters, with profound impacts on water, energy, food, and infrastructure sectors. Existing studies largely focus on single types of events in isolated regions. Spatial compound events deserve more attention, as synchronized droughts and/or floods across remote regions amplify the risk, cascade the impacts, strain the shared resources, and disproportionately burden local communities. Here we develop a novel data-driven framework based on multi-layer complex networks and event coincidence analysis to identify the global hotspots of concomitant occurrences of multiple hydroclimatic extremes. We apply this framework to gridded Standardized Precipitation Index (SPI) data over 1950-2016 to investigate the global synchronization links of extreme droughts and/or floods. Coincidence analysis of 0.7 trillion node pairs in a two-layer setting illustrates a similar spatial network structure of remote links (>2500 km) among the three subnetworks (i.e., drought–drought, pluvial–pluvial, and drought-pluvial). To understand how spatial compound extremes lead to potential disruptions to global crop production, we also quantify prevailing hotspots in the teleconnection patterns of drought and flood cooccurrences among 14 major cropland regions. Regional bundle analysis based on kernel density estimation reveals a highly synchronized bundle of extreme floods between southeastern Australia and southern Africa, and a bundle of extreme drought synchronization between northern India and eastern Africa. A synchronized bundle also emerges between western American droughts and Mexican floods. Globally coordinated efforts must target these hotspot regions to mitigate potential shocks to international food trade caused by synchronized hydroclimatic extremes, which are likely to increase in a warming climate.


HS07-A012
Land-atmosphere Coupling Accelerates the Onset Speed of Flash Drought Over China

Yumiao WANG#+, Xing YUAN
Nanjing University of Information Science & Technology

Flash drought is a special drought phenomenon characterized by rapid onset. In the context of climate warming, flash drought occurs frequently around the world, which poses a serious threat to water and ecological security without sufficient early warning. However, the causes of the rapid onset and underlying mechanisms are still unclear. Considering that the land-atmosphere coupling can influence the energy distribution and water exchange, and further affect hydro-meteorological extreme events, here we investigate the coupling characteristics during the onset process of flash droughts over China. Compared with the conventional dry conditions, the sensible heat transfer from the land surface to the atmosphere during the onset stage of flash drought is more significant, which can raise the lifting condensation level, promote the drying of the atmosphere, and effectively suppress the convective precipitation. Meanwhile, the drying of the atmosphere increases the demand for atmospheric evaporation, which can further consume the soil moisture and accelerate the onset speed of flash drought. With the contribution of evapotranspiration increased by about 26%, the flash drought onset speed over China almost doubled, which is important for distinguishing flash drought from conventional drought. Furthermore, concentrated on the hotspots of flash drought over China, the long-term evolution characteristics of land-atmosphere coupling were studied, and its impacts on the evolution characteristics of flash drought were revealed. This study highlights the importance of land-atmosphere coupling for speeding up flash drought onset in the changing climate and provides insights for flash drought diagnosis and prediction.


HS07-A002
Low-cost Future Estimation Method of Flood Quantiles for Large Climate Projection Ensembles

Jiachao CHEN#+, Takahiro SAYAMA
Kyoto University

The impact of climate change on flood frequency is a hot topic. The combination of General Circulation Models (GCMs) and hydrologic models is one of the most important ways to understand future flood changes with non-stationary problems. For detailed planning and adaptation measures, the application of hydrodynamic model simulations becomes crucial. However, a large number of climate projection ensembles and the high computational cost of solving the dynamic equation limit their application. To reduce the computational cost, this study performs the Flood Frequency Analysis (FFA) by regionalizing multiple basins and expanding the block size of the Block Maximum (BM) method and rising the threshold of the Peak Over Threshold (POT) method, respectively. The study is conducted on Shikoku Island using a 5km resolution climate ensemble called SI-CAT DDS5TK (a total of 31*12-year-data for each scenario) and the Rainfall-Runoff-Inundation (RRI) model is used. The assessment results show that a threshold of 10% of the Annual Maximum Series (AMS) for POT or a block size of 2 years for BM is the optimal choice. The statistical results of the eight major basins under three scenarios (current, 2k, and 4k warming) show that the vast majority of the Relative Root Mean Square (RRMSE) are <20%, which is mainly caused by the spatio-temporal variability of precipitation. Based on the above method, we can effectively reduce the computational effort and obtain similar conclusions on the frequency variation as the basin-by-basin simulation results.


HS07-A013
Upwind Flash Droughts Speed Up Heat Waves Over East China

Shiyu ZHOU#+, Xing YUAN
Nanjing University of Information Science & Technology

Compared to an individual heat wave or drought event, their concurrence often causes a greater impact, such as the extreme temperature and large-scale drought that sweep across the Northern Hemisphere in the summer of 2022. Previous studies have found that droughts can enhance heat waves by heating the land surface, but how the droughts affect the onset speed of heat waves remains unclear, especially for the drought with a rapid onset, i.e., flash drought. Here, we show that upwind droughts enhance 21% of the heat waves over East China by using a Lagrangian model to track the air mass trajectory, and the upwind flash droughts have a greater impact on heat waves than slow droughts. The negative soil moisture anomaly caused by upwind flash droughts increases total sensible heat and atmospheric boundary layer height over East China. Meanwhile, the rapid onset speed of flash drought is accompanied by the rapid accumulation of advected sensible heat which increases the onset speed of heat waves. Compared with the upwind slow droughts, the upwind flash droughts significantly accelerate the onset speed of heat waves by 43%. It indicates the important role of flash drought in the heat wave in the downwind region, and suggests a precursor for a sudden heat wave over East China.


Mon-31 Jul | 8:15 - 10:00 | MR335
HS13 - Hydrology of Data-scarce Mountainous Basins

Session Chair(s): Sanjeev Kumar JHA, Indian Institute of Science Education and Research Bhopal

HS13-A004
Sustainable Water Resources Management Using Soil and Water Assessment Tool (SWAT) and Analytical Hierarchy Process (AHP) for Water-scarce Northern Afghanistan

Wahidullah HUSSAINZADA1, Han Soo LEE1#, Jonathan CABRERA2,3+, Ahmad Tamim SAMIM1,4
1Hiroshima University, 2Hiroshima University / Davao Oriental State University, 3Davao Oriental State University, 4Balkh University

Water scarcity is a global issue nowadays, especially in arid and semi-arid regions with scarce precipitation and limited water resources. The current study represents a multidisciplinary approach to the management of water resources for irrigation, water supply, energy production, and flood protection using a hydrological model coupled with multi-criteria decision analysis (MCDA). This study focused on a semi-arid region in northern Afghanistan. Soil and Water Assessment Tool (SWAT) was used for the hydrological modelling. The model was calibrated (2013-2015) and validated (2016-2018) using monthly streamflow. The irrigation scheme of the watershed was revised based on the existing land area and crop water requirements to address water shortages. An engineering-based solution (dam construction) to regulate and control the streamflow, especially during winter and flood season is proposed and further analyses were made. Analytical hierarchy process (AHP) was used to determine suitable dam site locations. Then, the impact of the dam was analysed using SWAT. The dam reservoir capacity (197,900,938 m3), dam storage area (748 ha), dam height (69 m), electricity generation (Ave = 25.4 MW, Min =16.23 MW, Max = 66.5 MW), and flood protection ability were estimated. Finally, cost–benefit analysis (CBA) was conducted to ensure the project’s feasibility. The CBA proves the feasibility and applicability of the proposal. The surplus water can address the water shortages with an extra capacity of irrigating 17,180.5 ha or provision of water supply for the Mazar-i-Sharif City. These findings can be used by decision-makers for developing future development policies and overcoming with water scarcity issue in the region. This study represents a primary set of studies for water resources management in the less-managed watershed with the water-shortage problem in a less developed country.


HS13-A006
Assessing Total Water Storage and Associated Hydrological Processes in Indian Himalayan River Basins

Mohit YADAV1#+, A. P. DIMRI1, Suraj MAL2, Pyarimohan MAHARANA2
1Jawaharlal Nehru University, 2Delhi University

Water budget over the Himalayan river basins has become critical for management of water resource, flood risk, etc. In recent decades, the shifting pattern of precipitation phenomenon like Indian Summer Monsoon and Western Disturbance, and changing agricultural practices makes hydrological budget over Himalayan rivers basin an important aspect. In this study, assessment of Total Water Storage (TWS) for the period 2002 to 2020 in the three river basins viz. Indus River Basin (IRB), Ganga River Basin (GRB) and Brahmaputra River Basin (BRB) is evaluated in terms of spatial and temporal changes, along with other variables such as precipitation, snow water equivalent, runoff, evaporation, turbulent heat fluxes. This particular study uses TWS products available from GRACE mission and other variables from ERA5 except precipitation which was taken from GPM. The TWS anomaly and corresponding seasonal trends are calculated using the Mann Kendall test and Theil Sen estimator. Our preliminary results show that the predominant form of monsoon precipitation over GRB and BRB, and winter precipitation over IRB contribute to replenishing TWS with a lag of about a month. The TWS shows highest variability, being highest in summer and lowest in winter. Among other variables, precipitation show the highest intraseasonal variability, followed by runoff, whereas the evaporation is the least variable. Among all the three basins, a highest negative trend in TWS is observed during monsoon with most negative trend observed in GRB at rate of 6.16 (*10 -2 cm/year). Furthermore, during monsoon season, most parts of all the basins under study are drying though slower. However, during winter and post monsoon seasons, partitioning of turbulent heat fluxes in GRB and IRB basins indicates more humid and arid regions, respectively. Finally, in future, the results from the present work will be of great importance for policy makers in decision making.


HS13-A001
A Statistical Approach to Gap Filling of Precipitation Data Over the Indian Himalayan Region

Nibedita SAMAL#+, Sanjeev Kumar JHA
Indian Institute of Science Education and Research Bhopal

Avalanches and rainfall-induced landslides are common hazards in the Indian Himalayan region. The mitigation of these hazards needs early warnings which is obtained from models using real-time meteorological data such as precipitation. Samal et. al., (2022) have shown gaps in the datasets obtained from the automatic weather stations established in the Himalayan region. The gaps incur due to the complexity involved in acquiring data due to the complex terrain and extreme weather conditions of the Himalayas. In this study, we have used the Multiple Point Statistics (MPS) model to fill the gaps in the hourly precipitation data. As there is limited access to the observed precipitation data for most of the avalanche sites of the Himalayas, we have extracted reanalysis data for 20 avalanche and landslide sites of Uttarakhand and Himachal Pradesh. The reanalysis data is obtained from High Asia Refined Analysis version 2 (HARV2) at 10×10 km spatial resolution for the monsoon season (June, July, August, and September) of 2000 to 2020 years. For the analysis, we have created synthetic gaps of up to 50% in the time series at definite intervals. Using daily precipitation as the conditioning data and nearest station data as covariates, we have tried to fill the gaps in the precipitation data at those sites. The Direct Sampling (DS) algorithm available in the MPS model uses optimization of DS parameters and data patterns from the nearest station predictor variables to produce reliable simulations. The study is significant in its ability to produce multiple simulations of hourly precipitation with no gaps for various avalanche sites of the Himalayas, which can be helpful in monitoring of the sites. The results will be presented at the conference.


HS13-A008
Stream Flow Modelling in Kabul River Basin Using Soil and Water Assessment Tool (SWAT)

Usman SHEHZAD#+
Hiroshima University

Water resource management requires effective stream flow modelling which is critical to predict the impact of changes in land use and land cover (LULC) and climate change on river discharge. Kabul River Basin, an international river basin between Pakistan and Afghanistan with a total drainage area of around 87,000 km², comprises high mountains with some steep slopes and plain low-lying areas. This study aims to simulate the stream flow in Kabul River Basin at four different locations, Chitral, Chakdra, Bara River and Nowshera in Pakistan, using Soil and Water Assessment Tool (SWAT) by considering the physical aspects of the hydrological process. Modern-Era Retrospective analysis for Research and Applications, version 2 (MERRA-2) reanalysis data is used to input meteorological parameters in the SWAT model, while Global Food Security Support Analysis Data (GFSAD) is used to find the crop dominance to estimate the irrigated water requirements based on the crop calendar. Two years (2006-2007) warm-up period is considered, whereas the model is calibrated for 2008-2012 and validated for 2013-2017. The calibration results showed Nash Sutcliffe Efficiency (NSE) values of 0.89, 0.77,0.39 and 0.72 and NSE values of 0.77, 0.36, -1.51 and 0.44 for validation at Chitral, Chakdra, Bara River and Nowshera respectively. Sensitivity analysis showed that temperature lapse rate (TLAPS) and precipitation lapse rate (PLAPS) along with snow parameters are highly sensitive to resulting river discharge. The study addresses the issues of data scarcity in a large international river basin in developing countries and its impact on watershed modelling. The study can also be helpful to assist decision-makers in allocating water resources in an efficient way by keeping in view the possible extreme future climate events. 


HS13-A009
A Time-space Varying Distributed Unit Hydrograph (TS-DUH) for Operative Flash Flood Forecast Using Publicly-available-only Data

Ying HU1#+, Huan WU1, Weitian CHEN1, Chaoqun LI1, Wei WU2, Zequn HUANG3, Lulu JIANG1, Zhijun HUANG1
1Sun Yat-sen University, 2Ministry of Emergency Management, 3Key Laboratory for Meteorological Prevention and Mitigation of Disasters in Hunan Province

Increasing threats of Flash flood call for effective and operative ways to offer accurate forecasting and warning. In this study, a Time-Space varying Distributed Unit Hydrograph (TS-DUH) based on publicly-available-only data is proposed for efficient flash flood forecasting in un-gauged catchments. As in the traditional spatially distributed unit hydrograph (SDUH) method, TS-DUH initially estimates the runoff travel time (and flow velocity) from each location within a catchment to the outlet based on its static topographic and hydroclimate characteristics, i.e., DEM, land use and land cover. The runoff-drainage process is then adjusted by further considering the heterogeneous and dynamic runoff contribution caused by rainfall and soil moisture variations. The excess rainfall is estimated by a modified CN value from the Soil Conservation Service's (SCS) curve number method. An alternative net rainfall input is taken from the widely used Global Flood Monitoring System (GFMS) which provides long-term (2000-present) well-archived and real-time operative global runoff datasets from a state-of-the-art hydrological model, with persistent validation efforts. The performance of the TS-GUH method is evaluated using 2,804 flash flood events of 136 small-to-medium-sized catchments in the CONUS, with 816 events used for calibration. The validation results show that 92% and 56% of events have KGE values greater than 0 and 0.5, respectively, with a mean KGE value of 0.46. The probability of detection (POD) of flood events is 0.87. More importantly, the uncalibrated results show 84% and 49% of KGE values greater than 0 and 0.5, respectively, with a mean of 0.36, indicating the great potential value of the TS-DUH method in ungauged areas. In addition, this study also facilitates the analysis of the interaction and variation of land cover and rainfall in the flash flood formation process.


HS13-A005
Inter-comparison of Thirteen Gridded Global Precipitation Dataset for Natural Resources Management

Ahmad Tamim SAMIM1,2+, Han Soo LEE1#, Farhad NAYYER1, Wahidullah HUSSAINZADA1
1Hiroshima University, 2Balkh University

Gridded Global Precipitation (GGP) datasets with the high temporal and spatial resolution are reliable sources for water-related studies in regions with sparse observation. In this study, 13 GGPs were compared to observations at 75 stations from 2009 to 2020 in Afghanistan. Statistics, such as Pearson’s correlation coefficient (R), RMSE, and bias, were calculated to quantitatively and qualitatively assess GGPs versus observations. Precipitation data from GGPs were extracted on the same coordinates with stations for daily and monthly analysis. For annual analysis, the observations were changed to spatial data using inverse distance weighting (IDW). Then, the differences between the observed and GGPs were measured. Findings show a good correlation between the observed and CFSR, GPCC, MERRA-2, CPC, and CHIRPS dataset with mean daily correlation coefficients over 75 stations of 0.46, 0.44, 0.42, 0.40, and 0.39 respectively. In monthly analysis, CHIRPS, CFSR, GPCC, MERRA-2, and CPC shows mean R values of 0.74, 0.71, 0.71, 0.60, and 0.59, respectively. The lowest monthly mean bias of 75 stations was found in PERSIANN [6.1], TRMM [-6.7], PERSIANN-CDR [-9.6], and CHIRPS [-9.8] datasets. Daily minimum and maximum bias in the 75 stations range between 1.3 to -3.5 mm and 41 to -102 mm for monthly analysis. Furthermore, the daily minimum and maximum RMSE ranges from 0.8 to 9.3 and from 4.9 to 126 for monthly minimum and maximum values. Analysis results show that GPCC, CFSR, and MERRA-2 are more reliable than others considering the statistics. Considering monthly analysis, CHIRPS also agrees better with observations than the other nine datasets. These findings could help other researchers in the selection of the GGPs according to their applications and purposes. GGPs can also fill the gap of data scarcity in terms of temporal and spatial frequency, where a short period of observations is available.


HS13-A003
Smaller Sets of Training Data Can Effectively Generate Fine-scale Weather Data Over the Northwest Himalayas

Sanjeev Kumar JHA#+, Nibedita SAMAL, Akshay SINGHAL
Indian Institute of Science Education and Research Bhopal

The hydrological and glaciological responses of the Himalayan region are highly sensitive to changes in climate. In the detailed studies of such crucial responses, fine-resolution weather data is essential. However, the Himalayan region, due to its complex topography and harsh climate, has very few ground observatories. As a result, researchers look for alternative data sources, one of which is to set up a Weather Research and Forecasting (WRF) model. One of the problems with setting up a WRF model over the Himalayan region is that the model has to incorporate a variety of factors that determine the weather of the region, such as the local climate physics, complex terrain, and orography. The other problem is the high computational cost involved. In this study, we set up a Multiple-Point Statistics (MPS) based statistical model using available hindcast data (HARC and HARF) to generate precipitation and temperature (HARF) in the future. We also investigate into the adequate length of hindcast data required for developing the model. The success of MPS simulation depends on the Training Image (TI). We generate five sets of TIs, each succeeding set larger than the previous one. The largest TI set acts as the benchmark for the evaluation of smaller sets. Results indicate that smaller TIs can produce reasonably good results up to a certain threshold. Overall, the study shows that MPS can adequately predict fine-scale weather data even for highly complicated regions such as the Western Himalayas. Also, simulations using smaller TIs provide an avenue for using limited available historical data in MPS modeling, thus making way for more hydroclimatic studies in data-limited regions. The results from the study will be presented at the conference.


Mon-31 Jul | 8:15 - 10:00 | MR336
HS11 - Urban Water-related Problems

Session Chair(s): Kei NAKAGAWA, Nagasaki University, Hitoshi MIYAMOTO, Shibaura Institute of Technology, Kenichiro KOBAYASHI, Kobe University, Channa RAJANAYAKA, National Institute of Water and Atmospheric Research, Detchphol CHITWATKULSIRI, Faculty of Engineering, Kasetsart University

HS11-A028
A Study on Measures to Prevent Flooding at Seoul National University's Gwanak Campus

Hyeonju KIM#+, Soohyun YANG, Young-Oh KIM
Seoul National University

Seoul National University’s Gwanak Campus in Seoul is prone to flash flooding during concentrated heavy rainfall due to its location on the hillside of Mt. Gwanak. To prevent damage by extreme rainfall, the largest storage facility with 20,000 tons was constructed at the campus in 2015. Nonetheless, the campus experienced unprecedented flood damage in August 2022 when a record-breaking downpour occurred over the megacity of Seoul. This study aims to unravel major causes of the flood damage at the campus and propose feasible solutions, as localized heavy rain is expected to be more frequent and intense in urban areas. To this end, we conducted a frequency analysis of the annual maximum hourly precipitation data gauged at the Gwanak Radar observatory from 1997 to 2022. We also simulated the Storm Water Management Model with 10-minute interval rainfall data for August 8th to 9th, 2022 when the damage-causing downpour occurred. With the simulated results, we estimated the amount of flooding, compared the effects of the storage facility’s opening conditions on flood magnitude, and established a vulnerability map of the drainage networks. The frequency analysis resulted the heavy rainfall in 2022 with a return period of 36.5 years had a shorter return period than the design standard of the storage facilities. The simulated peak discharge from the upstream sub-catchment of the storage facility and the sub-catchment where storage facility is located were 17.86m3/s and 0.43m3/s, respectively. Testing different opening conditions of the storage facility highlighted no flooding occurred when the release was full. Furthermore, the vulnerability map of drainage systems showed specific areas getting vulnerable to extreme rainfall at the campus. To prevent future flood damage at the campus, we suggest to implement real-time management of the storage facility, and improve drainage systems by enlarging pipes in vulnerable areas.


HS11-A005 | Invited
Improving a Unit-hydrograph Model for Flood Early Warning System

James GRIFFITHS#+
National Institute of Water and Atmospheric Research

Samoa’s geographic location makes it susceptible to storm surges and heavy rainfall during the cyclone season. The Vaisigano catchment on Samoa’s north coast is at particular of flash flooding due to its steep and narrow, funnel-shaped catchment. Flood incidence has been exacerbated in recent years by increased urbanisation in the lower reaches of the catchment. The catchment has a relatively short time of concentration (just 2 hours) making the development of short-response flood warning systems difficult. Intermittent historic river flow and rainfall data, and limited mapping of soil and land use cover, also hinder reliable parameterisation and validation of runoff models. In this study we assess the cumulative impact of data uncertainty on parameterisation of parsimonious unit hydrograph model. Performance of the model with respect to forecast rainfall data is then assessed, and recommendations made for its future use as part of a real time early warning system. Options identified for model improvement included use of a dynamic rainfall loss factor (based on antecedent conditions) and different methods for representing mean rainfall from multiple guage data, depending on the direction of incident rainfall.


HS11-A008 | Invited
The Effects of Forecast Rainfall and Sewerage Water Level Information for Early Evacuation in Urban Areas

Naoki KOYAMA#+, Shiori TERAI, Tadashi YAMADA
Chuo University

The number of localized torrential rainfall events is increase in Japan, and flooding and accidents due to internal flooding from sewers are common in urban areas. To prevent these floods, it is important to provide information on early evacuation. In this study, the effectiveness of rainfall forecasting and sewer water level information for early evacuation of internal flooding was therefore investigated. The study basin is Nishi-word, Yokohama, Kanagawa Prefecture, and catchment area is approx. 7 km. First, forecast rainfall information which is provided by JMA examined accuracy verification. As a validation index with precipitation, the accuracy rate, miss rate and false alarm rate of forecasts were evaluated for each forecast time (1h~15h ahead). The results showed that miss rate was 2-3% and false alarm rate was 1-6% at any given time. On the other hand, the accuracy rate was about 60% for forecasts up to six hours ahead, but about 40% for forecasts beyond that time. A model was constructed from all sewer data in the target area and the response of rainfall and sewer water levels was analyzed by sewer simulation. The results showed that the sewer water level has a flood arrival time of 5~30 minutes. These results show that precipitation forecast information is valuable for making evacuation decisions, and the sewer simulation results show that it is effective in providing early evacuation.


HS11-A002
ML-RAINCAST: Application of Data-driven Models for Rainfall Radar Nowcasting in a Real-time Urban Flood Prediction System

Detchphol CHITWATKULSIRI1#+, Hitoshi MIYAMOTO2
1Faculty of Engineering, Kasetsart University, 2Shibaura Institute of Technology

Short to mid-term rainfall nowcasting is a significant component for the various aspects of urban flood management, such as drainage system monitoring and inundation risk management. Existing data-driven approaches, e.g., deep learning models, have shown significant reliable output by using rainfall radar images as inputs. However, real-time urban flood prediction requires continuous rainfall radar images in their dynamic time series. To examine whether using a dynamic AI model approach such as long short-term memory (LSTM) for image-to-image translation, this research has tried to train a deep learning model of rainfall radar images with their reflectivity for improving the continuity of prediction. The trained model called herewith ML-RAINCAST: a Machine Learning-based methodology for radar Images nowcasting was developed based on an LSTM architecture. Here, the LSTM encoder-decoder framework provided a general framework for sequence-to-sequence learning problems. This research implemented a convolutional LSTM encoder-decoder network for weather prediction, with the sequences being image maps of radar reflectivity. The ML-RAINCAST was compared to a previous development based on a storm-tracking model. This research outperformed by 9.14% of RMSE, and the SSIM values are approximately unity. The ML-RAINCAST's performance was evaluated for moderate and higher rainfall events for forecasts at 5 min in frequency and 60 min in rainfall duration. The results showed that the ML-RAINCAST performed higher accuracy from 70% for the previous storm-tracking-based model to 83.5% for an hour of rainfall duration. Furthermore, merging the ML-RAINCAST with a real-time flood forecasting system indicated to stabilize the continuous rainfall process nowcasting and enabled significant improvement in the difficult-to-predict dynamic time series of flood mapping.


HS11-A030
Multi-objective Uncertainty Assessment of High-resolution Urban Flood Modeling Using Heterogeneous Information

Seong Jin NOH1#+, Bomi KIM1, Hyeonjin CHOI1, Garim LEE1, Seungsoo LEE2, Seongsim YOON3, Wonkook KIM4
1Kumoh National Institute of Technology, 2Korea Environment Institute, 3Korea Institute of Civil Engineering and Building Technology, 4Pusan National University

Urban flood prediction is affected by a variety of factors including topography, land cover, storm drain network, and the capacity of infrastructure. Furthermore, a combination of pluvial and fluvial flooding in dual drainage systems makes it more difficult to obtain a holistic understanding of physical processes and associated uncertainties. Meanwhile, the amount of high-resolution hydrologic data and heterogeneous flood information such as streamflow measurement, flood marks, and, images from social media and remote sensing is sharply increasing. Thus, various types of flood information are expected to help improve the accuracy of urban flood predictions. However, methods for effectively minimizing uncertainty in high-resolution urban flood modeling using heterogeneous information have not been thoroughly studied. In this study, we investigate the effects of different types of flood information on the uncertainty of urban inundation prediction. Multiple numerical experiments are implemented in the Oncheon-cheon catchment in Busan, South Korea using a high-resolution 1D-2D inundation model forced by the radar rainfall estimates. The discussion will focus on how to quantify the uncertainty of urban inundation modeling using different combinations of flood information.


HS11-A031
Multi-objective Stormwater Management in Industrial Land Developments

Ranjan SARUKKALIGE#+
Curtin University

The impacts of urban land developments, changing from natural to artificial impervious surface limits the infiltration into the ground and lead to increase surface runoff. Increase in impervious surface is expected to lead to a greater risk of flooding, especially in combination with the more frequent and intense extreme precipitation events caused by climate change. Managing the urban stormwater in rapidly developing areas is critical, specially in industrial developments, where most of the areas are covered with impervious layers. Infiltration is one of the best operational and sustainable methods to manage urban stormwater. Until recently, in stormwater management designs and selection of best stormwater management strategies, infiltration capacity of different soils were not been considered as a major factor. Therefore stormwater management strategies have failed to adequately consider the criticality of spatially varying soil permeability and their implications on stormwater runoff. Due to the increasing housing density, local land development authorities requires stormwater runoff from developing lots to be retained/detained within the property. Due to lack of information on local soil properties, specifically permeability within the predominant soils in land development areas, it is difficult to assess stormwater retention/detention requirement. This study was carried out in new industrial development areas in Western Australia, focusing on identification of soil properties and development of a typology of suitable stormwater management strategies with respect to manage both quality and quantity of urban stormwater. Different scales; lot scale, street scale and precinct scale stormwater strategies have been developed to manage the stormwater in the land development. Recommendations are developed for future stormwater management, taking expansion of the industrial zone into account to cater the additional runoff generation.


HS11-A035
Analysis of Influencing Factors and LID Optimization Design of Sponge City Construction in Typical Coastal Area

Qian ZHANG#+, Yingwei YUAN, Chen FEIWU, Yang YU
Tianjin Agricultural University

Sponge urban construction is an important measure for slowing down urban waterlogging, improving usage of rainwater resources, and optimizing the ecological environment. The buried conditions of groundwater often have some constraints on the construction of sponge city, so it is necessary to clarify the response mechanism and constraints of groundwater in the area to sponge city construction. Based on data collection, actual investigation, indoor experiments and computer simulation techniques, this research aims to clarify the dynamic process of groundwater in the region, and to conduct a qualitative analysis of the hydrological cycle process in sponge city from the perspective of water equilibrium. The response mechanism and control conditions of groundwater to sponge city construction are put forward. In response to potential problems such as high water table congestion and particulate matter blocking sponge in rainwater during the rain flood supply process, a new compound function LID(Low Impact Development) facility that is conducive to the efficient use of rainwater is designed and physical simulation and optimization is carried out. It provides theoretical basis, technical means and practical basis for the construction of sponge city.


Mon-31 Jul | 10:20 - 12:20 | MR307
HS12 - Climate Change Impacts on Regional Hydrological Issues: Projections and Adaptations Strategies

Session Chair(s): Shuichi KURE, Toyama Prefectural University

HS12-A007
Projection and Mitigation to the Hydrological Drought Over the Upper Yellow River Basin Under Climate Change, Land Cover Change and Reservoir Operation

Peng JI+, Xing YUAN#
Nanjing University of Information Science & Technology

The upper Yellow River basin (UYRB) provides about half of the total annual discharge of the entire Yellow River basin in northern China, and influences more than one hundred million people over downstream regions. In a changing environment, climate change and water resources managements are influencing the streamflow regime over UYRB significantly. In addition, a warming future favors the vegetation greening over UYRB, inevitably impacting the hydrological process and extremes. Yet, future hydrological drought changes over UYRB remain unclear due to complex interactions between climate change, land cover change and reservoir operations. In this study, we coupled the Conjunctive Surface-Subsurface Process version 2 (CSSPv2) land surface model with a reservoir module, and used the new CSSPv2+Reservoir model to perform future projections driven by bias-corrected meteorological forcings from 11 Coupled Model Intercomparison Project Phase 6 (CMIP6) models. Evaluations show the model well captures the monthly streamflow over the UYRB with a Kling-Gupta efficiency of 0.75. The increasing precipitation during dry seasons reduces hydrological drought duration, while its impact on drought severity is limited. The dramatic increase of leaf area index at the 4.0℃ warming level robustly exacerbates hydrological drought severity by intensifying evapotranspiration. The reservoir operation, designed to reduce seasonality in monthly releases to ensure stable hydropower generation, further decreases drought duration, but increases drought frequency and severity. A mitigated operation rule which stores less water during wet seasons, however, can reduce hydrological drought severity and duration significantly. Our results highlight that impacts of climate change, land cover change and reservoir operation on future hydrological change are not synergistic, and emphasize that future reservoir operation should consider the trade-off between hydropower generation and hydrological drought mitigation.


HS12-A001
Functional Assessment of Off-channel Storage Using Existing Facilities and Topography

Sora MARUTA+, Seiki KAWAGOE#
Fukushima University

It is concerned that extreme precipitation events and increase flood inundation damage have increased due to climate change. Basin flood control is being promoted to reduce damage, in which flood control measures are considered from the catchment area to the inundation area as a whole. In this study, we focused on the effect of off-channel storage and estimated the reduction effect of precipitation due to storage in Japan.
We focused on paddy fields, parks and schools as land structures with potential storage effects. In addition, we considered the topographic effect of hollows as a new option. Hollows are a natural resource that can provide a storage function due to differences in elevation independent of land use and facilities. We analyzed a selection of depressions in Japan to quantify their storage function. The extraction of hollows gives utility not only to the storage effect but also to the derivation of flooding high risk area. The paddy field was classified into flat, sloping, and fan-shaped areas, and the waterlogging depth was set for each. For hollows, a DEM with a spatial resolution of 10 m was used as the dataset. The possible storage volume using hollows was calculated based on the difference in elevation from the smoothed topography.
The paddy field reservoirs were located in the northern Japan, while the park and school reservoirs were located in the metropolitan area. For hollow storage, large reservoirs were scattered throughout Japan, and many reservoirs existed in areas where lakes existed. It was confirmed that the decrease in precipitation due to storage was greater in northern Japan and lower in mountainous areas or in watersheds with low storage. It has been determined the distribution of off-channel storage in Japan, and the areas where the reduction of rainfall due to storage is vulnerable were derived.


HS12-A002
Relationship Between Frequent Flood, People Perception, and Countermeasures in Cases of the 2022 Floods in Japan

So KAZAMA#+
Tohoku University

In 2022, seven flood damages occurred in Japan. Each of the seven floods has different characteristics and impacts depending on the region. Among them, the floods of the Nabuta River in Miyagi Prefecture in July and the Mogami River in Yamagata Prefecture in August occurred in areas that had frequently breached and flooded in the past. Residents in both areas did not relocate despite they had frequent floods, but residents in the Aterazawa area relocate this time. On the other hand, residents in the Nabuta river area did not relocate by the 2022 flood. The reason of different reaction is due to the depth of inundation and the structure of local industries. The Aterazawa district had mainly the tertiary industry, and many houses were flooded more than 50 cm deep. On the other hand, the Nabuta River was mainly used for agriculture, and the flood depth of many houses was less than 50 cm. The government decided to build embankments in both districts, but the scale is larger in the Aterazawa district. This is due to cost benefit. In both areas, where depopulation is expanded in the future, the construction of levees instead of urban planning measures remained concerns about future maintenance. The national government is promoting river basin management, but administrative sectionalism prevents the river department and city planning department from working together. Watershed management is really desired, but it is still limited to some areas.


HS12-A016
Assessing Rainwater Storage Facilities for Flood Prevention in Urban Areas: A Case Study of Seoul's Gangnam Area

Sujin KIM#+, Jonguk KIM, Kwangwon YOON, Hyeonseok CHOI, Sunkwon YOON
Seoul Institute of Technology

Seoul experienced record-breaking heavy rainfall(116mm/hr) in August 2022, causing significant flooding and casualties in the Gangnam area. Conventional flood prevention projects, such as deep rainwater tunnels, are no longer sufficient to handle the increasingly frequent and intense guerrilla torrential rains. This study suggests the installation of rainwater storage facilities as a solution to reduce flooding in the concentrated infrastructure of the Gangnam area. Three installation methods were considered: underground installation along arterial roads, installation in publicly available sites such as schools and parks, and underground rainwater storage facilities (OSD, On Site Detention). Combining these methods could shorten installation time by two years and reduce costs compared to large-scale drainage systems. To address the flooding problem in the Gangnam area, short- and long-term measures need to be applied together through cooperation and institutional improvement of the government and local agencies responsible for the area. Acknowledgements: This research was supported by the Seoul Institute of Technology (SIT) (2022-BA-020, Establishment of comprehensive measures for local flood safety through the evaluation of the response capability for flood disaster prevention facilities in Seoul).


HS12-A020
Examining the Method of Pre-discharge from Dam Reservoirs for Flood Damage Mitigation in Central Vietnam

Tadashi YAMADA, Naoki KOYAMA, Kei KOURA#+
Chuo University

In Vietnam, flood occurs almost every year, inundating low-lying coastal areas. There was one which was considered one of the worst flood in the past decade. It occurred in October 2020, causing many victims and damage to homes in Quang Nam province and Thua Tien Hue province in central Vietnam. In addition, the annual number of floods is increasing, and rainfall is estimated to increase with climate change in the future. In other words, vulnerability to flood is raised. On the other hand, in the river basins of central Vietnam, there are dam reservoirs serve the purposes of not only for flood control purposes but also for hydropower generation and agricultural use, which could be used to reduce flood damage. However, actual flood operations confirmed that the reservoir water level reached the surcharge level in the early stages of the flood and that flood control is not done well during the peak of the flood. Therefore, this study took a numerical approach to the effect of discharge from dam reservoir on river water levels and inundation depths with the aim of reducing flood damage in a river basin in Central Vietnam. As a result, the main findings of this study are as follows. Firstly, the application of the pre-discharge method using observed rainfall information upstream of the dam reservoir can reduce the river water level and inundation depth downstream while maintaining water storage capacity for power generation and agricultural use. Secondly, if all rainfall upstream of the dam reservoir could be stored in the dam reservoir, there would be a greater decline in river water level and inundation depth. Finally, even in that case, inundation in downstream could not be completely prevented.


Mon-31 Jul | 10:20 - 12:20 | MR323
HS01 - Challenges in Hydrologic Modeling

Session Chair(s): Deepthi B, Indian Institute of Technology Bombay

HS01-A001
Simulating the Impact of Reservoir Operation on its Inflow Flood

Yangbo CHEN#+
Sun Yat-sen University

Reservoirs formed by a dam in a river can provide many benefits but can also negatively impact the reservoir inflow flood responses. In this study, the impact of reservoirs on inflow flood responses is regarded to be caused by three effects induced by reservoir operation: the runoff routing acceleration effect, the water volume increasing effect and the runoff routing deceleration effect. Three indices are proposed to quantitatively describe these effects, namely, the peak flow concentration time effect index, peak flow effect index, and runoff coefficient effect index. A general methodology is proposed for quantitatively assessing the impact of reservoirs on inflow flood responses. This method employs a physically based distributed hydrological model, the Liuxihe Model, to simulate the reservoir inflow flood processes with or without a reservoir and then quantitate reservoir impact based on the simulated hydrological processes. The impact of several reservoirs, including large, medium and small-size in China has been studied, and the results suggests that the impact of the reservoirs on the inflow flood responses is significant, and the peak flow concentration times are shortened and the peak flows and runoff coefficients are increased. The larger the scale of the flood event is, the stronger these impacts. If the precipitation is heavily concentrated in the reservoir impoundment area and its adjacent area, the peak flow effect will be strengthened.


HS01-A002
Bivariate Frequency Analysis of Storm Events for Estimating Design Floods in a Watershed

Min Ji KIM+, Seok Woo KIM, Kyung Woon PARK, Jae Hee RYU, Tae-Woong KIM#
Hanyang University

Recently, a bivariate frequency analysis has been introduced in hydrological design to consider the characteristics of storm events, i.e., rainfall amount and duration of the storm event, which have a great influence on design hydrograph, rather than the existing univariate analysis. We proposed a practical method to calculate design floods based on bivariate rainfall frequency analysis (DF_BRFA) to consider properties of storm events, and compared the design floods with those calculated by the existing method design flood based on univariate rainfall frequency analysis (DF_URFA) and the design flood based on flood frequency analysis (DF_FFA). To evaluate the validity of DF_BRFA proposed in this study, DF_FFA was calculated for gauged watersheds with sufficient observed flood data, and DF_BRFA and DF_URFA were compared based on the accuracy measures. We collected independent and isolated storm events based on the inter-event time definition, and selected two annual maximum storm events among the events, one of which has the largest return period and the other has maximum rainfall amount, respectively. A bivariate frequency analysis was performed for annual maximum storm events using copula functions, and design storm events were determined corresponding to the median and 95% upper and lower limits values. The overall results for the 80-year frequency showed that DF_FFA was calculated as 3485 m³/s, and DF_URFA was overcalculated as 5710 m³/s. When calculating the maximum annual rainfall event and median, DF_BRFA was calculated 3511 m³/s, which was close to the DF_FFA. When using the proposed method in this study, it is possible to solve the problem of over-estimation of design floods by the existing design practice based on univariate rainfall frequency analysis.


HS01-A005
Spatial, Temporal & Spatiotemporal Streamflow Dynamics Using Network Theory: Application to Australia

Vishakha REGULWAR1#+, Bellie SIVAKUMAR1,2
1Indian Institute of Technology Bombay, 2Tsinghua University

There is now an increasing interest in the applications of network theory, especially complex network concepts, to study streamflow (and other hydrologic) processes. This study aims to apply concepts from complex networks to study the connections in streamflow dynamics, with a focus on spatial, temporal, and spatiotemporal connections. The monthly streamflow data from 218 stations in Australia over a 26-year (1981–2006) period is considered. The spatial network is formed based on linear correlation, with different threshold values used to examine the influence on the clustering coefficient. The temporal network is developed using phase space reconstruction and the False Nearest Neighbour algorithm to identify the optimum embedding dimension, and the Euclidean distance is used to identify connections between the reconstructed vectors. The spatiotemporal network for streamflow is constructed by considering spatial connections and temporal connections jointly, rather than separately. To form the spatiotemporal network, a nonlinear phase space embedding procedure was employed to jointly reconstruct multiple time series in a multi-dimensional phase space. The resulting spatiotemporal streamflow network was constructed based on the reconstructed vectors. The study shows that a small proportion of stations has considerable influence on the network, and the stations connected with a station are not all geographic neighbors. The study is limited by its single variable approach and the need to consider actual influencing variables in future studies. The results of this study provide valuable information for water resource management and planning.


HS01-A011
Analysis of Soil Loss Using a Physics-based Erosion Model: A Case Study of Uiam Basin in South Korea

Mingeun SONG+, Minho YEON, Giha LEE#
Kyungpook National University

Soil Erosion causes various problems such as loss of agricultural land, increase dead storage area due to soil flowing into dams, and deterioration of water quality. Soil erosion is caused by water or wind, but in South Korea it is mainly caused by water (rainfall). High rainfall intensity and short-term heavy rain are the main cause of soil erosion, and the frequency of these heavy rains is increasing due to climate change. The Universal Soil Loss Equation (USLE) is limited in its ability to model erosion caused by heavy rain events with short-term rainfall periods and high rainfall intensity. To address this, the SSEM model is proposed as a physically based model that can consider short-term rainfall. The SSEM model calculates the soil erosion process through a physically based approach, such as numerical analysis of the motion wave equation, in order to more accurately estimate soil erosion caused by Heavy rains, which are becoming more frequent in Korea. In order to estimate and calibrate the parameters of the SSEM model, data on water level-discharge data, soil characteristics, DEM, and land use were collected in the Uiam Dam basin in South Korea, which was the research basin. As a result, much erosion occurred in agricultural land and bare land, and sediment was deposited in the urban area.


HS01-A033
Regional Flood Frequency Analysis Considering L-moment and LH-moment Based Framework for Krishna River Basin

Amit SINGH#+, Sagar CHAVAN
Indian Institute of Technology Ropar

Design flood estimation at an ungauged location is an essential aspect of planning and designing any hydrological structure. Regional flood frequency analysis (RFFA) helps in estimating the design flood at ungauged locations within a hydrologically homogeneous region. The RFFA involves the determination of appropriate regional frequency distribution through L-moment based regional goodness of fit test. The parameters of the regional distribution are generally obtained by using various approaches such as the method of moments, methods of maximum likelihood, and L-moment approach. The generalization of L-moment based on the linear combination of higher order statistics, famously known as LH-moment can be considered for parameter estimation. In this study, three probability distributions namely generalized extreme value (GEV), generalized logistic (GLO), and generalized Pareto (GPA) are considered for performing RFFA for estimating ungauged flood quantiles corresponding to various return periods (e.g., 50, 100, and, 200 years) in the Krishna River basin. The discordancy measure, heterogeneity measure, and goodness of fit test have been performed for different orders of LH-moment. The suitability of GEV, GLO, and GPA distribution is judged through the LH-moment ratio diagram and the |Z|-statistic criteria. The performance of LH-moment based RFFA is evaluated through Leave One Out Cross Validation (LOOCV). Results indicate that the LH-moment based RFFA yields more reliable estimates of flood quantiles.


HS01-A006
Temporal Dynamics Study of Suspended Sediment Concentration with Network Theory

Swetalina NATH1#+, Bellie SIVAKUMAR1,2
1Indian Institute of Technology Bombay, 2Tsinghua University

Suspended sediment transport helps to study water quality, landscape evolution, and geomorphic development of river basins. The present study uses complex networks' concepts to study suspended sediment concentration's temporal dynamics. The daily suspended sediment concentration is collected over a period of 52 years (October 1969-September 2021) from the Rio Grande River basin at Albuquerque, Bernalillo County, New Mexico, USA. The daily suspended sediment concentration data is used to construct an annual suspended sedimentation network by considering each year as a node in the network. Each node has a time series of daily suspended sedimentation data and the connection between the nodes is identified based on the linear correlation. If the correlation between any pair of nodes is greater than the threshold, there exists a connection, otherwise is not. The influence of the threshold on the properties of the network is also examined. The clustering coefficient and degree centrality are used as the network measures. The clustering coefficient quantifies the tendency of the network to cluster whereas degree centrality helps to identify the significant node in the network. This study’s results will help us identify the type of network (random, small world, or scale-free network) based on the value of the clustering coefficient. The degree centrality result will help us to identify the significance (years) in the annual suspended sediment concentration network.


HS01-A031
Selection of Suitable Sites for Flood Buffer Zone Based on Nature-based Solutions: A Case Study of the Han River in Republic of Korea

Seonuk BAEK#+, Joonhak LEE, Seongcheol SHIN, Haneul LEE, Soojun KIM, Hung Soo KIM
Inha University

In recent years,. various flood patterns such as local heavy rainfall event and extraordinary floods are occurring due to the influence of climate change. However, the flood management method based on flood control structure is difficult to efficiently cope with various flood patterns. Also, it is difficult to efficiently operate the stream in terms of socio-economic and ecological aspects through the method. Therefore, it is essential to create the 'flood buffer zone' based on nature-based solutions that can actively cope with various flood patterns and minimize damage to the aquatic environment. Consequently, in this study, site-suitability analysis was performed for the 'flood buffer zone'(candidate site) for the riparian zone(park, farmland, and so on) located in the Han River area. First, various evaluation index using meteorological, topographical, and socio-economic factors were constructed. Next, based on the evaluation index, the optimal candidate site ('flood buffer zone') was identified to reduce flood damage and improve the water environment. As a result, the area most needed a flood buffer zone for flood management in the Han River was selected. The results of this study are expected to be used as basic research data in the course of a project to create a 'flood buffer zone' in the Han River area in the future.


Mon-31 Jul | 10:20 - 12:20 | MR336
HS11 - Urban Water-related Problems

Session Chair(s): Kenichiro KOBAYASHI, Kobe University, Kei NAKAGAWA, Nagasaki University, Hitoshi MIYAMOTO, Shibaura Institute of Technology, Detchphol CHITWATKULSIRI, Faculty of Engineering, Kasetsart University, Channa RAJANAYAKA, National Institute of Water and Atmospheric Research

HS11-A036
Evaluation of Two Low Impact Development Technologies: Permeable Pavement and Exfiltration Storage

James LI#+
Toronto Metropolitan University

This field assessment study evaluated the hydrologic response of a concrete laneway in Toronto, Ontario, Canada retrofitted with (1) a new street-level low impact development system called Cupolex®, an arcade of concrete-covered plastic domes stormwater detention system which forms part of the concrete pavement; and (2) a permeable interlocking concrete pavers (PICP). A special monitoring protocol was developed for the study based on local recommended guidelines. Based on eight rainfall events between May to July in 2020, it was found that a % runoff depth and peak runoff rate reductions between 90.6% to 100%, and 94% to 100% respectively for Cupolex®. The results for PICP revealed a % runoff depth and peak runoff rate reductions between 35% to 67%, and 4% to 85% respectively. The performance for PICP may be attributed to the low permeability soil conditions and design features such as absence of a underdrain system. Overall, the runoff control of Cupolex® was excellent under the events observed and provided a baseline understanding of its performance for future implementation. Further research should focus on long-term monitoring and further development of stormwater management models for performance prediction under different design conditions.


HS11-A032
Future Proofing Green Infrastructure

James GRIFFITHS#+
National Institute of Water and Atmospheric Research

Future climate change will lead to an increased incidence of both heavy rainfall and heat stress in many urban environments. The resulting increased risk of floods and heatwaves will necessitate an equivalent increase in resilience. Green infrastructure and nature-based solutions can be utilised to increase urban resilience to climate related hazards (UNEP, 2022), but their designs also need to be future-proofed against changing climate.The Budyko curve (1974) can be used to represent the timing and magnitude of shifts in the water-energy balance predicted by global climate models in a way that can be easily understood and utilised by engineers and stakeholders. For example, the relationship between evaporation and dryness indices for rainfall and potential evapotranspiration (PET) ranging from 300 to 950 mm/year can be used to illustrate relative differences between hot and cold, or wet and dry environments. This information can be used to optimise green infrastructure design and performance by representing the trade-offs between temperature reduction and water retention that would result from different land-cover types. Using examples from New Zealand, the study illustrates how the Budyko curve can be used to represent the potential impact of climate change in urban areas, and how that information can be used to formulate climate resilient, nature-based mitigation techniques


HS11-A033
Impact of Climate Change on the Implementation of Green Roof on a Micro-urban Watershed

Amrutha SURESH#+, Sreeja PEKKAT, Senthilmurugan SUBBIAH
Indian Institute of Technology Guwahati

In recent years, cities have become increasingly vulnerable to frequent flooding due to increased imperviousness caused by urbanization and frequent extreme rainfall caused by climate change. One widely adopted mitigation strategy to reduce flood damage is Low-Impact Developments (LIDs), a stormwater management technology. Notably, LIDs have been gaining popularity recently due to their affordability, sustainability, and minimal space requirement. Though LIDs are growing in popularity, arguments exist regarding their installation location, hydrologic processes, parameter settings, and so on. Given the space restrictions in urban areas, green roofs have significant potential in urban catchments. Therefore, this study analyses the effectiveness of green roofs in managing stormwater in an urban micro-watershed. Sensitivity analysis of various parameters of the green roofs was performed using the Morris coefficient. In addition, the impact of climate change on green roof's effectiveness in managing runoff was studied using the Storm Water Management Model (SWMM). The ensemble average of various Coupled Model Intercomparison Project Phase 5 (CMIP5) models and Representative Concentration Pathway (RCPs) were considered for predicting future precipitation intensities. Rainfall intensity-duration-frequency (IDF) curves were developed to determine the design rainfall. The future climate was divided into three periods, and the IDF curves were generated for each period. Simulation results indicate that green roofs can reduce flooding, but the increased rainfall intensity due to climate change could affect the performance of green roofs.


HS11-A014
The Applicability of LSTM, XGBoost, and LightGBM for Water Level Prediction in Rivers and Reservoirs

Zheng Kun WANG+, Yu LI#
Nankai University

Water level prediction is a crucial reference in water resources regulation and flood control for most cities along rivers and reservoirs. In the field of massive hydrological data processing, machine learning methods have unique advantages over the physical models. In this study, 12-year observed data of water level and precipitation of Katsuragawa river and Xiaolangdi dam were obtained from Ministry of Land, Infrastructure, Transport and Tourism and Yellow River Conservancy Commission of the Ministry of Water Resources. These data were analyzed by Long Short-Term Memory (LSTM) , Extreme Gradient Boosting (XGBoost) and Light Gradient Boosting Machine (LightGBM) models, while evaluated by R2, mean absolute error (MAE) , mean squared error (MSE) , and root mean square error (RMSE) to explore the optimal water level prediction model in the river and reservoir condition. The results show that LSTM is more effective and accurate than the other two methods in the Katsuragawa river water level prediction, while LightGBM makes a good performance in the Xiaolangdi dam water level prediction. Both of LSTM and LightGBM have a high R2 score over 0.99 in the whole validation set and have good performance even during the flood season, which receives 50% more precipitation than average, providing a practical water level prediction method for cities along rivers and reservoirs.


HS11-A017 | Invited
Impact of a Number of Ensemble Members in Numerical Weather Prediction Models on Flood Prediction

Tsutao OIZUMI1#+, Takuya KAWABATA1, Le DUC2, Kenichiro KOBAYASHI3, Kazuo SAITO2, Takuma OTA1
1Meteorological Research Institute, 2The University of Tokyo, 3Kobe University

This study investigates the impact of different numbers of ensemble members on the accuracy of flood forecasting. In numerical weather forecasting, many studies have been carried out a large ensemble forecasting, such as 1000-member ensemble forecasting experiments. Those researchers have reported that more accurate probabilistic information can be obtained by increasing the number of members. However, these studies still need to sufficiently investigate the impact of the number of ensemble members on the probability of disasters. This study investigated the impact of different ensemble numbers on the accuracy of flood forecasting. The ensemble numbers used are 1000, 100, and 21 members. Experimental results show that 1000-member forecasts are more accurate in predicting flood peaks than 100-member forecasts. On the other hand, the 21-member ensemble could not predict the flood peaks but could predict the risk of floods occurring.


HS11-A015
Ensemble Rainfall–runoff and Inundation Simulations Including Kalman Filter Application Using 1000 Member Rainfalls by 4D LETKF on the Kumagawa River Flooding 2020

Kenichiro KOBAYASHI#+
Kobe University

This presentation deals with the 1000 ensemble flood simulations using ensemble rainfalls simulated by 4D LETKF. The number of ensemble rainfall members is large as 1000 compared to the operational rainfall products of two-digit numbers to avoid sampling errors in the three-dimensional meteorological simulation based on chaotic theory. Using the large data set, 1000 ensemble rainfall–runoff simulation for dam catchments and high-resolution inundation simulation of large area are carried out focusing on the Kumagawa river catchment. As a result, the possibility was indicated that the number of ensembles could be reduced in flood simulation unlike the meteorological simulation due to the topography and soil characteristics of the catchment. The presentation also shows the application of a Kalman filter for short range flood simulation. The presentation is to be the summary of the paper in the following: Kobayashi, K., Duc, L., Kawabata, T. et al. Ensemble rainfall–runoff and inundation simulations using 100 and 1000 member rainfalls by 4D LETKF on the Kumagawa River flooding 2020. Prog Earth Planet Sci 10, 5 (2023). https://doi.org/10.1186/s40645-023-00537-3


Mon-31 Jul | 1:10 - 3:10 | MR310
HS10 - Hydrometeorology

Session Chair(s): Jingyu WANG, Nanyang Technological University

HS10-A010
Unlocking the Future of Rainfall: Enhancing Interannual Forecasts with Spectral Transformations of CMIP Decadal Predictions

Ze JIANG1#+, Dipayan CHOUDHURY 2, Ashish SHARMA1
1UNSW Sydney, 2NSW Department of Planning and Environment

In recent years, Australia has faced drastic variations in rainfall, including severe drought and widespread bushfires followed by two consecutive years of heavy rainfall in the east. This study aims to explore the possibility of predicting such anomalies years in advance. We present a prediction framework that combines empirical and physically-based approaches, utilizing the novel technique of spectral transformations of sea surface temperature anomaly (SSTA) indices from CMIP6 decadal experiments. SSTA indices, representative of large-scale modes of climate variability, are spectrally transformed using the Wavelet System Prediction (WASP) method to enhance the prediction of rainfall at specific locations. These transformed SSTA indices are then used as inputs into a hierarchical linear combination (HLC) model to forecast interannual rainfall across Australia. Our hindcast experiment results demonstrate remarkable prediction accuracy for rainfall up to five years in all regions and climate zones over Australia, using the HLC-WASP hybrid framework. The framework was then validated for the forecast period of 2020-2029, showcasing its potential for predicting wetter or drier conditions in the future, providing valuable insights for managing water resources, prioritizing demands, protecting vulnerable systems, and reducing uncertainty in hydrological decision-making.


HS10-A012
Three Factors to Explain the Spatial Distribution in Surface Humidity: Application to South Korea

Jisoo LEE+, Dongwoon KANG, Kyungrock PAIK#
Korea University

The relative humidity over terrestrial surface exhibits characteristic spatial distributions, and its explanation is important in understanding local climate and water-related disasters. South Korea is a great example, showing a wide range of spatial variability in surface relative humidity. In this nation, the Yeongdong and Yeongnam region show relatively lower humidity than the rest, the difference particularly apparent during winter. We suggest three key factors of the surface temperature, precipitation, and external contribution to explain the spatial variability in surface humidity. Each of them is developed as a quantitative measure, and the relative humidity is expressed as multi-regression model of the three factors. This idea is going to be applied to 66 stations across South Korea. Quantitatively evaluation of how much variation is explained by each factor will be presented.


HS10-A005 | Invited
Analysis of the Characteristics of the Low-level Jets and Its Relationship Between Precipitation During the Mei-yu Season

C.G. CUI#+
Institue of Heavy Rain,China Meteorological Administration

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.


HS10-A006
Long-term Changes, Synoptic Behaviors, and Future Projections of Large-scale Anomalous Precipitation Events in China Detected by a Deep Learning Autoencoder

Zeqin HUANG#+, Xuezhi TAN
Sun Yat-sen University

The frequency of large-scale anomalous precipitation events over China has increased during 1961-2018. However, it remains challenging to understand the mechanisms associated with these anomalous events showing different spatial patterns. Here, we applied an autoencoder technique to identify large-scale anomalous precipitation events for both observations and model simulations, which were then classified into several patterns through a self-organizing map method. The synoptic behavior and atmospheric circulation background of different anomalous patterns were also analyzed using simultaneous composite analyses. Results show that occurrences of different anomalous precipitation patterns have increased significantly, except those centered in North China, Northeast China, and the Yangtze River Basin. The anomalous precipitation patterns manifest various intraseasonal distributions, which are linked to zonal oscillations of the western North Pacific subtropical high (WNPSH) and meridional displacements of East Asia westerly jet (EAJ). Accompanied by the westward movement of WNPSH, anticyclonic systems transport warm moist air from the Indian Ocean and the South China Sea to converge with the cold air caused by anomalous cyclones over the northwest flank of the WNPSH, leading to large-scale anomalous precipitation in these regions. Besides WNPSH, the northward and southward displacements of EAJ also favor the occurrence of anomalous precipitation events in northern and southern China, respectively. Our study also illustrates that the occurrence frequency of anomalous precipitation events is projected to increase remarkably under the SSP585 scenario by rates of 2~4 folds.


HS10-A002
Competing Aerosol Effects in Convections During Mei-yu Season Over the Yangtze–Huai River Valley in China

Lin LIU#+
China Meteorological Administration

Aerosol effects on convective clouds remain an important open-ended question in climate research. This paper reports on the effects of anthropogenic aerosols on the convections during Mei-yu season by means of long-term simulations with the Weather Research and Forecasting with Chemistry (WRF/Chem) model. Sensitivity experiments indicate that increased aerosols reduce the total rainfall and convection occurrences by 9.00% and 7.17% over the Yangtze–Huai River Valley during Mei-yu season due to the suppression of shallow convections with cloud geometrical thickness (CGT) less than 4 km. Aerosol radiation effect plays a dominant role in shallow convections suppression by cooling the surface air and increasing regional atmospheric stability. On the contrary, deep convections are invigorated under polluted conditions with a stronger updraft and more latent heating release, which can be explained by the interactions between aerosol-induced microphysical effects and the dynamical response. Due to the shorter distances that the downdrafts accelerate to the surface in shallow convections, the interaction between dynamics and microphysics is reduced comparing to the deep convections, leading to suppression of shallow convections at high aerosols. In addition, relative humidity which controls the balance between the net generation and loss of condensate mass is an important meteorological factor in regulating the net influence of aerosols on convections. These findings provide us insight into the competing mechanism between aerosol radiative and microphysical effects on convections during Mei-yu season, which can aid in better parameterizing aerosol effects in climate models.


HS10-A009
Application of Lightning Data to High-resolution Rapid Refresh

Anwei LAI#+
China Meteorological Administration

For a further study on the usage of ADTD lightning data in rapid refresh assimilation system, we develop a new relationship between lightning activity and radar echo characteristics in Central China to calculate lightning-proxy reflectivity and conducts three sets of numerical experiments to analyze a strong weather process occurred in Hubei Province on 1 June 2015. By utilizing the Severe Weather Automatic Nowcast System (SWAN) 3D mosaic products and lightning locating data from 2014 to 2018, a new S-shape curve relationship between lightning activity and radar echo characteristics in Central China is investigated and their functional fits under two different terrains of plains and mountains are established for calculating lightning-proxy reflectivity. By using S-shape curve fitting formulas and the Grid point Statistical Interpolation (GSI) empirical formulas to estimate radar echo, the lightning-proxy reflectivity derived by S-shape curve fitting is very corresponding to the high frequency region of lightning flashes and the strong radar echo field. The influence of assimilation of lightning data from this new S-shape curve relationship on radar reflectivity, cloud microphysical variables and precipitation forecast calculated by rapid refresh assimilation system was mainly analyzed and compared with assimilation of lightning data from GSI empirical formulas and the direct assimilation of radar reflectivity. Results are as follows. The assimilation of lightning-proxy reflectivity of this new S-shape curve relationship can improve the precipitation forecast skill by adjusting the cloud microphysical variables. By comparing the results of precipitation, it can be concluded that after adding lightning-proxy reflectivity obtained by the new relationship, the missing report rate can be effectively reduced, and the model can respond to the precipitation forecast that is more closely to the observation in a short time scale. Finally, the accuracy of short-term prediction is improved and achieves similar results as the direct assimilation of radar reflectivity.


HS10-A015
Higher Temperature Enhances Spatio-temporal Concentration of Rainfall

Dagang WANG#+
Sun Yat-sen University

The relationship between extreme precipitation intensity and temperature has been comprehensively studied over different regions worldwide. However, the effect of temperature on the spatio-temporal organization of precipitation, which can have a significant impact on precipitation intensity, has not been adequately studied or understood. In this study, we propose a novel approach to quantifying the spatial and temporal concentration of precipitation at the event level and study how the concentration varies with temperature. The results based on rain gauge data from 843 stations in the Ganzhou county, a humid region in south China, show that rain events tend to be more concentrated both temporally and spatially at higher temperature, and this increase in concentration qualitatively holds for events of different precipitation amounts and durations. The effects of temperature on precipitation organization in space and in time differ at high temperatures. The temporal concentration increases with temperature up to a threshold (approximately 24°C) beyond which it plateaus, whereas the spatial concentration keeps rising with temperature. More concentrated precipitation, in addition to a projected increase of extreme precipitation, would intensify flooding in a warming world, causing more detrimental effects.


HS10-A004
Statistical Characteristics and Drivers of Heavy Precipitation Events Under Different Synoptic Circulation Patterns in the Middle and Lower Reaches of the Yangtze River in Summer

Tao PENG#+
China Meteorological Administration

Aiming at the hourly heavy rainfall of rainstorm days (≥50 mm/d) in the middle and lower reaches of the Yangtze River during 2010–2020, the obliquely rotated Principal Component in T-mode (PCT) method is used to classify the daily mean 850 hPa geopotential height, including Type1 (southwest vortex/shear line), Type2 (shear line), Type2 (frontal surface), Type3 (warm shear line), Type4 (warm inverse trough line), Type5 (typhoon-westerly trough) and Type6 (easterly wave). We studied the weather system configurations of different synoptic circulation patterns, their long-term trends and impacts on diurnal variations of heavy precipitation, and drew the following conclusions: Type1, Type2 or Type3 shows balanced double-peak frequencies of the start time of heavy precipitation during 06:00–08:00 BT and around 17:00 BT, respectively. For Type1, the dynamical lifting and thermal lifting play balanced roles, while for Type2 and Type3, the dynamical lifting plays a key role. The number of rainstorm stations for Type1 shows a slight increasing trend, while that for Type2 or Type3 shows a significant increasing trend. Type4, Type5 or Type6 shows a significant single peak frequency of the start time during 15:00–16:00. Type5 and Type6 are mainly affected by dynamical lifting along with favourable cape values, which can trigger rainstorms. The number of rainstorm stations for Type4 or Type6 shows a decreasing trend (that for Type4 is more significant), while that for Type5 shows a slight increasing trend.


HS10-A003
Bayesian Model Averaging with Stratified Sampling for Probabilistic Quantitative Precipitation Forecasting

Haixia QI#+
China Meteorological Administration

To study the impact of training sample heterogeneity on the performance of Bayesian model averaging (BMA), two BMA experiments were performed on probabilistic quantitative precipitation forecasts for the middle and lower reaches of the Yangtze River in summer 2016 using TIGGE (THORPEX Interactive Grand Global Ensemble) multi-model and multi-member precipitation forecast data. The first experiment, conventional Bayesian model averaging (CBMA), pools the subsamples together in training and forecasting without categorisation. The second experiment stratified sampling BMA (SBMA), divides all available training samples into three subsets according to their ensemble spread. The results show that spread is a good indicator to divide the ensemble precipitation samples into subsets, especially for heavy rainfall. Moreover, the optimal training period for BMA is about 50 days. The CBMA often filters out most information on the high spread cases and produces ill-fitted parameters for them. Additionally, CBMA deterministic forecast and percentile forecast are often underestimated. In contrast to CBMA, parameters estimated using SBMA with stratified samples of different properties are much more reasonable. The mean absolute error, continuous ranked probability scores and Brier scores of the two BMA experiments were examined for all available forecast cases. Although CBMA was slightly superior to the raw ensemble prediction system (REPS) forecasts in low-threshold forecasts, SBMA outperformed REPS, probability matching ensemble mean, and CBMA in all evaluations.


Mon-31 Jul | 1:10 - 3:10 | MR323
HS01 - Challenges in Hydrologic Modeling

Session Chair(s):

HS01-A008
Evaluation of Numerous Kinetic Energy-rainfall Intensity Equations Using Disdrometer Data

Linh NGUYEN+, Minho YEON, Mingeun SONG, Giha LEE#
Kyungpook National University

Calculating rainfall erosivity, which is the capacity of rainfall to dislodge soil particles and cause erosion, requires the measurement of the rainfall kinetic energy (KE). Direct measurement of KE has its own challenges, owing to the high cost and complexity of the measuring instruments involved. Consequently, the KE is often approximated using empirical equations derived from rainfall intensity (Ir) inputs in the absence of such instruments. However, the KE-Ir equations strongly depend on local climate patterns and measurement methods. Therefore, this study aims to compare and evaluate the efficacy of 27 KE-Ir equations with observed data. Based on a re-analysis, we also propose an exponential KE-Ir equation for the entire Korean site, and the spatial distribution of its parameter in the equation is also discussed. In this investigation, we used an optical disdrometer (OTT Parsivel 2) to gather data in Sangju City (Korea) between June 2020 and December 2021. The outputs of this study are shown as follows: (1) The statistically most accurate estimates of KE expenditure and KE content in Sangju City are obtained using power-law equations given by Sanchez-Moreno et al. and exponential equations published by Lee and Won, respectively. (2) The suggested KE-Ir equation applied to the entire Korean site exhibits a comparable general correlation with the observed data. The parameter maps indicate a high variance in geography.


HS01-A004
The Impact of Bedrock Surface Geometry on the Matrix Flow Component of Subsurface Stormflow

Tongbi TU1#+, Levent KAVVAS2, Ali ERCAN3, Z.Q CHEN4
1Sun Yat-sen University, 2University of California, Davis, 3Middle East Technical University, 4California Department of Water Resources

Subsurface flow is a critical component in the hydrological cycle since it controls the quantity and timing of surface runoff and groundwater flow. Field studies have shown the fundamental influence of the bedrock surface geometry on subsurface stormflow (SSSF) and that the SSSF process consists of at least two major components: the matrix flow component and the macropore flow component that are in dynamical interaction toward forming the SSSF. Furthermore, field studies have shown that the bedrock surface that underlies the SSSF has essentially a two-dimensional (2D) geometry, where not only the longitudinal profile along the hillslope but also the profile in the transverse direction influence the subsurface stormflow over the bedrock. The macropore flow itself being a multidimensional flow process requires a multidimensional matrix flow component in order to quantify realistic dynamical interactions between these components within the subsurface stormflow module of a watershed hydrology model. Within this framework, the critical research question is how to extend the existing 2D Boussinesq model for the matrix flow over an inclined flat 2D surface in the longitudinal hillslope direction by developing the governing equations of matrix flow at hillslope scale over various 2D bedrock surface geometries that are reported in the field studies of SSSF. Then, numerical experiments are performed by applying the developed governing equations to various bedrock surface geometries. The results of the numerical simulations show 1) the proposed governing equations can simulate various two-dimensional bedrock surface geometries, and are capable of incorporating the upward or downward concavity of bedrock surface in longitudinal and transverse directions into SSSF by modulating the timing and magnitude of the flows; and 2) the proposed governing equations for matrix flow provide an appropriate setting for the dynamical interaction of the matrix flows with the macropore flows, creating a promising modeling framework for SSSF. 


HS01-A010
Analysis of Evapotranspiration Using Complex Networks and Chaos Theory

Vamsi Krishna GUNTURU1#+, V. JOTHIPRAKASH1, Bellie SIVAKUMAR1,2
1Indian Institute of Technology Bombay, 2Tsinghua University

Terrestrial evapotranspiration (ET) is the second largest component in the hydrological cycle and accounts up to 60 to 70% of annual rainfall over land. Estimation/prediction of ET is challenging due to its nonlinear interactions with several hydro-meteorological variables. This study uses network and chaos theory to examine the nonlinearity in the ET time series. The analysis of ET is carried out using the Visibility Graphs (a networks approach) and the False Nearest Neighbor (chaotic approach) methods. Firstly, the time series is converted into nodes (temporal instances) and links (relation between nodes) based on the horizontal visibility criteria. Secondly, the number of links (degree) extracted from the network is fitted to an exponential form to analyze the dynamics of the evapotranspiration series. The fitted exponent value is compared to the theoretical value (ln(3/2)) to identify the underlying dynamics (as a dimension). The dimension information obtained from the network approach is compared with the result of the False Nearest Neighbor (FNN) method. The FNN method involves 1) a reconstruction procedure based on delay embedding and 2) the identification of “false” neighbors in the reconstructed phase space. The dimensionality approach (FNN) is a quantitative approach for analyzing the time series, which complements the qualitative dimension inferred from complex networks. These methods are applied to daily evapotranspiration data extracted from Global Land Evaporation Amsterdam Model from 1980 to 2020. The analysis is carried out across India for 4642 grids; results from the complex networks suggest that the exponent value is less than 0.405. This indicates that evapotranspiration is showing chaotic behavior using networks approach, and the dimensionality approach (FNN) suggests that the evapotranspiration is indeed chaotic with dimensions varying between 3 to 18. The present study has important implications for evapotranspiration modelling and for analyzing spatial variability.


HS01-A026
Development of Hybrid Model for Flood Damage Prediction

Joonhak LEE#+, Haneul LEE, Seonuk BAEK, Seongcheol SHIN, Soojun KIM, Hung Soo KIM
Inha University

In order to reduce damage from disasters such as heavy rainfall, urban and non-urban flooding, it is important to identify in advance the occurrence of these natural disasters. Recently, flood forecasting are mainly based on actual measured data, making the possible damage information caused by future floods to be insufficient. However, the United Kingdom and the United States flood forecast information system can provided for up to 9 days flood forecasting lead time. 3-day lead time flood forecasting information per administrative district can help to prepare and respond to flood damage even before it occurs. This study focused on Cheongmicheon basin where floods are frequent and damages are high. In addition, long short-term memory(LSTM) and deep neural network(DNN) models were used as the models for prediction. Results show that the DNN model have better predictive performance than the LSTM model with an NRMSE of 0.002. Each design flood was calculated by applying the predicted rainfall and observed rainfall values ​​through the DNN model as an input to the HEC-HMS model. Each calculated design flood was applied to HEC-RAS to calculate the design flood level. Finally, two flood maps were produced and the results were compared. As a result, the technique developed through this study excellently predicted the occurrence of damage. Thus, the developed methodology culd potentially have a great contribution in reducing the damages caused by floods.


HS01-A041
Catchment Classification Using Network Theory

Dineshkumar MUTHUVEL1#+, Bellie SIVAKUMAR1,2
1Indian Institute of Technology Bombay, 2Tsinghua University

Records of streamflow data are essential in monitoring water availability and designing hydraulic structures across the river. However, the installation and maintenance of the streamflow gauge stations are costly and cumbersome, especially during extreme flood events leading either to missing data or the worst-case of abandonment of the station altogether. With only a few gauge stations available with continuous and adequate data length, catchment classification becomes pertinent to interpolate missing data and check the sufficiency of the number of gauging stations in the basin. In recent times, complex network concepts have widely been used to analyze the spatial relationship in hydrology. Streamflow networks are built by considering the stations as nodes, and the links are established on the basis of streamflow correlation between node pairs. Three different undirected networks are formed by eliminating the weak links of correlations below 0.6, 0.7, and 0.8. The centrality measures of closeness, betweenness, and degree, along with the clustering coefficient, are determined to find the significant gauging stations in the basins. Some of the gauging stations continue to have high centrality values for all the correlation thresholds. Using these network measures, communities of gauging stations are detected for each network. The communities of each network are compared using Normalized Mutual Information (NMI) values. The narrow distribution of elevation and streamflow of each community reveals that the partitions made are appropriate. It proves that the network concepts could inherit such topographic details. The communities formed could be used for data imputation and to check the sufficiency of gauge stations in the basin.


HS01-A020
Pollution Accident Analysis Using a Hybrid Hydrologic-hydraulic Model(K-river & K-drum)

Yonghyeon LEE1+, Hyunuk AN1#, Jungmin AHN2, Youngteck HUR3
1Chungnam National University, 2National Institute of Environmental Research, 3K-water Institute

In this study, the transport of pollutants was analyzed using the K-River and K-DRUM coupling model for water pollution accidents that occurred in the Nakdong River water system. In Korea, the necessity of a distribution model that accommodates the water circulation process and the importance of nonpoint pollution sources were emphasized in water quality management after the introduction of the total amount of water pollution. Therefore, in order to reflect the runoff characteristics of nonpoint sources, the K-DRUM distribution model, which can analyze pollution in the basin, was used. And the reproducibility of the model was improved by applying the operating rules of dams operating in the Nakdong River system. In addition, in order to analyze the movement of pollutants in the river, only the advection part of the advection-dispersion equation was applied to the 1D hydraulic model K-River to perform pollutant tracking. As a result of water pollution analysis, the peak concentration of the pollutant was underestimated, but the arrival time and the trend of the overall pollutant concentration were well reproduced. Water pollution concentration is a value estimated through water pollution accident investigations, and there may be limitations in accurate analysis. However, it will be possible to establish countermeasures for water pollution accidents in a short period of time if accurate measurement data are secured and the reliability of the model is increased. This work was supported by the National Research Foundation of Korea (NRF) grant funded by the Korea government (MSIT) (No. 2021R1A2C200553012).


HS01-A009
A Developed Method for Quantifying Various Sources of Data Errors in the Calibration of Water Quality Models: Bayesian Error Analysis with Reordering (BEAR)

Xia WU1#+, Lucy MARSHALL2, Ashish SHARMA2, Qingyun DUAN1
1Hohai University, 2UNSW Sydney

Water quality and hydrologic variables inevitably suffer from data errors, such as the streamflow error arising from the use of a river stage in place of a streamflow measurement via a rating curve and the proxy error of a pollutant load or concentration introduced by using turbidity data as a surrogate. These data errors will negatively affect the water quality model predictions. Accurately identifying them during the model parameter estimation can promote model calibration and prediction. However, it is challenging due to the interactions between the data errors and parameter errors and the simultaneous identification of multiple sources of data errors makes this approach more complicated. This study explores these issues in the case of total suspended solids (TSS) simulated via a conceptual water quality model, build-up/wash-off model, whose input is streamflow and output is TSS concentration. A new method called Bayesian error analysis with reordering (BEAR) has been developed to identify the errors in both input and output data during the model calibration. Rather than identifying these data errors directly via the traditional methods, the BEAR method samples the data errors from the prior error distribution, reorders their ranks with the secant method, and removes the reordered error sequences to modify the data and improve the model calibration. The results demonstrate that 1) Based on an accurate error distribution of one source of data error, the BEAR method can estimate the error distribution of another source of data error and improve the parameter estimation; 2) Quantifying errors in both input and output data can provide a more accurate characterization of model parameters and data errors, than just one source of data error; 3) The accuracy of the prior information used for the data error model is a significant factor in the success of the BEAR algorithm.


Mon-31 Jul | 1:10 - 3:10 | MR330
HS07 - Impact, Risk, and Predictability of Compound Hydroclimatic Extremes in a Changing Environment

Session Chair(s): Xing YUAN, Nanjing University of Information Science & Technology, Baoqing ZHANG, Lanzhou University

HS07-A017 | Invited
Variability of Australian Compound Hot & Dry Events and Their Large-scale Drivers

S SHARMILA1#+, Acacia PEPLER1, Jyoteeshkumar PAPARI2, Ulrike BENDE-MICHL1, Wendy SHARPLES1, Irina RUDEVA1, Mitchell BLACK1
1Bureau of Meteorology, 2Commonwealth Scientific and Industrial Research

Australia is a global hotspot of compound drought and heatwaves (CDHWs), and such concurrent hot and dry events provide an ideal backdrop for bushfire risk as well as pose detrimental socio-economic and ecological impacts. Recent studies have identified increased likelihood of such events in Australia in a warmer climate (Ridder et al. 2022, Reddy et al. 2022), however, the spatio-temporal variability of such CDHW events in the historical period and their physical mechanisms are yet to be well understood. In this study, we investigate the observed variability in CDHW events in Australia during extended austral summer (November to March) using the latest high resolution (~5km) daily Australian Gridded Climate Data and daily ERA5 reanalysis dataset for the recent 40 years. We have used daily Excess Heat Factor and 3-month Standard Precipitation Index to identify heatwaves and meteorological drought conditions respectively and have employed a grid-by-grid joint peak-over-threshold-based approach to identify CDHW events. We have detected the preferred geographic locations of such events and quantified their interannual spatial extents across Australia. We have also identified the dominant CDHW variability and their relationship with the large-scale drivers, crucial for their predictability. Furthermore, the CDHWs followed by heavy rainfall over south-eastern Australia are investigated and the interconnectivity between climate and hydrological processes are illuminated. The emerging results will provide new insight on the physical processes involved in CDHW events, which could serve as a blueprint for compound event analysis across disciplines and sectors.


HS07-A015 | Invited
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.


HS07-A021
Evaluation and Multi-model Projection of Seasonal Precipitation Extremes Over Central Asia Based on CMIP6 Simulations

Victor DIKE#+, Zhaohui LIN
Chinese Academy of Sciences

Central Asia faces an increasing challenge related to water resources arising from severe droughts and floods that have impacted the region in the past decades. Using a comprehensive set of extreme precipitation indices, we assess the performance of CMIP6 models in representing observed precipitation extremes and investigate future responses of these extremes to greenhouse gas emissions under four shared socioeconomic pathways (SSP). Particularly, this study identifies robust signals of projected changes in spring and summer precipitation extremes over central Asia. Results show that the CMIP6 models reasonably reproduced the spatial distribution and variability of precipitation extremes over southern central Asia (SCA) and northern central Asia (NCA) during the spring and summer seasons, respectively. Across the SSPs, the CMIP6 models project a decrease in total spring wet-day precipitation amount (PRCPTOT) over SCA and a significant increase in PRCPTOT over the NCA. The projected changes are characterized by a significant increase in maximum consecutive 5-day precipitation (RX5day), wet-day intensity (SDII), and the number of heavy precipitation days (R10mm); these suggest that the spring will be characterized by intense precipitation extremes. Moreover, no significant change is projected for consecutive wet days (CWD) and dry spells (CDD) over SCA. Nonetheless, the CMIP6 models project a significant increase in summer PRCPTOT over SCA and a decrease in summer PRCPTOT, RX5day, R10mm, SDII, and CWD over NCA while projecting a significant and robust increase in dry spells. It is also found that the severity of the projected dry spell deepens across the SSP spectra and gets more pronounced towards the end of the 21st century. Notably, the inter-model spread of the precipitation extremes is smaller during the spring over SCA, larger during the summer season over NCA, and more probable in the warmer future.


HS07-A004
Evaluating the Effects of Climate Change and Human Activities on Watershed Runoff Variation: Focusing on the Geum River Basin

Miju OH1+, Baesung LEE1, Joo Heon LEE2, Tae-Woong KIM1#
1Hanyang University, 2Joongbu University

Watershed runoff is a very important component of water resources management. Recently, however, climate change and human activity have significantly influenced the changes of watershed runoff. Climate change represents natural impacts due to precipitation and temperature increases, whereas human activity includes dam and embankment construction, urbanization, deforestation, and land use change that can affect runoff either directly or indirectly by disrupting hydrologic processes. This study quantitatively evaluated the effects of climate change and human activity on the watershed runoff in the Geum River basin, Korea, using observed and synthesized runoff sequences from 1966 to 2099. Using the Mann-Kendall test, the trend of runoff was analyzed, and using the climate elasticity approach and Buduko framework, the effects of climate change and human activity on past and future runoff were quantitatively evaluated. In the Gapcheon watershed, the amount of runoff variation in the past was accounted for 76.7% by climate change and 23.3% by human activity. In addition, when comparing future period of S1 (2024-2061) and S2 (2062-2099) with the past, the contributions of climate change (RCP 8.5) accounted for 56.8% and 65.5%, respectively. Therefore, evaluating the relative contribution of climate change and human activity to changes in watershed runoff is expected to play important role in water resource management in future. Acknowledgement: This research was supported by a grant(2022-MOIS63-001) of Cooperative Research Method and Safety Management Technology in National Disaster funded by Ministry of Interior and Safety (MOIS, Korea).


HS07-A011
A Knowledge-informed Deep Generative Model for Spatially Compound Risk Assessment

Xinyue LIU1,2+, Dongxiao ZHANG2, Xiaogang HE1#
1National University of Singapore, 2Southern University of Science and Technology

Climate change is causing an increase in the frequency and severity of weather and climate extremes. The combination of multiple hazards can result in impacts that are far greater than the sum of each individual event. Studying these compound extremes, however, is more challenging as they occupy only a small corner of the multi-dimensional probability space, requiring a large amount of data for accurate assessment. Unfortunately, the rare nature of compound events limits the available observational records, making it difficult for robust analysis of the occurrence probability and cascaded impacts. Existing studies, such as weather generators, can produce stochastic realizations of observed climate, yet they only maintain the essential statistical properties of climate variables. Meanwhile, deep generative models such as generative adversarial networks (GANs) have demonstrated their ability to estimate complex distributions and generate visually indistinguishable samples. Only a few studies have explored the power of deep generative models in extreme events, yet they lack the consideration of the spatial extremal dependence structure, which is crucial in spatially compound events. Here, we develop a knowledge-informed deep generative framework to advance the simulation of spatially compound extremes for the sake of data augmentation and stress tests. Specifically, we utilize a metric to consider the spatio-temporal coupling with the spatial extremal dependence structure embedded into the GAN framework. The incorporation of extreme value theory further improves the generated spatially compound events and enables the user to control the level of extremeness. These synthetic samples can be employed in climatic stress tests to anticipate the response of highly-managed and nonlinear systems. By extending the framework to nonstationary cases, we can assess the risk of compound events in a changing climate.


HS07-A026
Future Hydrological Projection for Flood Management of the LCRR

Taesam LEE1#+, TBMJ OUARDA2
1Gyeongsang National University, 2National Institute for Scientific Research

The record-breaking floods of 2011 in the Lake Champlain-Richelieu River (LCRR) basin led to interest to improve flood forecasting and mitigation plans. To evaluate the adequacy of the flood risk mitigation measures and management strategies, synthetic Net Basin Supply (NBS) series for the LCRR including the 2011 flood must be properly modelled and stochastically simulated according to the characteristics of the records. From a previous Great Lakes study, it has been found that the series presents stochastically nonstationary and the application of Shifting Mean Level (SML) process can be a possible alternative as a stochastic simulation model of the NBS series for the Great Lakes. In the current study, the interest is in checking whether the SML model is feasible to simulate the NBS for the LCRR basin and to provide an alternative model if any. Additionally, the nonstationary behaviors of the NBS were also considered as trend and oscillations. Therefore, three different approaches were suggested to deal with the stochastically nonstationary behavior especially in the long-term variability: as overall trend, shifting mean, or as a long-term oscillation. To represent these three different options, the Autoregressive (AR) model with an overall trend, SML, and Empirical Mode Decomposition and Nonstationary Oscillation Resampling (EMD-NSOR) were tested, respectively. In addition, AR for a traditional time series modeling and LSTM for recent deep learning developments were further tested. The results show that the SML and EMD-NSOR models reproduced the observed drought and surplus statistics as well as the key statistics. The detailed results indicate that the EMD-NSOR model outperforms the SML model especially for the long-term variability of the observed NBS shown with the Hurst coefficient. The overall results conclude that the record can be considered as oscillations and modelled as the EMD-NSOR to simulate the mean annual NBS series of the LCRR basin.


HS07-A007
Risk Assessment of Flood Disaster in Land Subsidence Areas: The Case of Choushui Alluvial Fan

Rong-Yu CHEN#+, Hong Ru LIN, Jet-Chau WEN
National Yunlin University of Science and Technology

For a long time since the industrial revolution, humans have burned enormous amounts of fossil fuels, causing an increase in the concentration of greenhouse gases in the atmosphere, leading to global warming after a long period of accumulation. In addition, changes in atmospheric gas concentrations cause changes in rainfall patterns. As a result, climate change increases the frequency of extreme climate events, such as heavy rains, droughts, and forest fires. In recent years, many abnormal climate events have occurred in Taiwan, including the massive flooding caused by typhoon Fanapi (6-hour cumulative rainfall over 600 mm) in 2010 and the most extensive drought in Taiwan in 2021, both of which caused enormous damage. Many studies have been conducted to assess the risk of abnormal rainfall and drought events, but few studies have been conducted on land subsidence. Therefore, in this study, the land subsidence area of the Choushui alluvial fan was used as the study area, the hazard and vulnerability factors that may affect the area were collected and analyzed. The risk assessment method was established by combining the hazard and vulnerability factors in a risk matrix approach to investigate the disaster risk of the study area when the stratigraphic subsidence area was exposed to an abnormal rainfall event. The above findings can help government agencies to develop area-specific disaster prevention strategies and contingency, enhancing disaster response capabilities in the future.


HS07-A023
Snow Risk Assessment and Snow Damage Prediction Model Development by Region in South Korea

Hyeong-Joo LEE+, Jae-Hyeong HAN, Gunhui CHUNG#
Hoseo University

Recently, heavy snow damage, which has fewer damages than other natural disasters, is becoming more and more severe due to global climate change. Looking at the current status of heavy snow damage in Korea for the past 10 years, about 160 billion won of damage occurred over the past 10 years, showing the third largest amount of damage among natural disasters that occurred. Therefore, in this study, we tried to develop a heavy snow damage prediction model that reflects the regional characteristics of administrative districts in Korea. DPSIR risk assessment technique was used to classify into 4 risk levels, and heavy snow damage prediction models for each level were developed using multiple regression models. As a result of comparing the predictive power of the existing heavy snow damage prediction model and the heavy snow damage prediction model by grade, the graded prediction model developed using the DPSIR technique showed excellent predictive power. If a model predicting the extent of damage is developed through the results of this study in the future, it will be possible to take preemptive and effective measures against heavy snow damage. 


Mon-31 Jul | 1:10 - 3:10 | MR336
HS11 - Urban Water-related Problems

Session Chair(s): Hitoshi MIYAMOTO, Shibaura Institute of Technology, Kei NAKAGAWA, Nagasaki University, Channa RAJANAYAKA, National Institute of Water and Atmospheric Research, Kenichiro KOBAYASHI, Kobe University, Detchphol CHITWATKULSIRI, Faculty of Engineering, Kasetsart University

HS11-A023
A hp Adaptive Discontinuous Galerkin Hydrodynamic Model for 2D Shallow Water Equations

Tsubasa IWASAKI+, Tetsuya SHINTANI#
Tokyo Metropolitan University

Discontinuous Galerkin (DG) method is suitable for reproducing shock waves which often appear in the front of the Tsunami waves. Although the DG method can obtain higher-order solution in each element independently, it requires high computational costs. To reduce these costs, the hp adaptation is proposed to adjust the grid resolution (h) and the order of the solution (p) locally and dynamically. However, the implementation of h and p adaptations tend to be complicated so that the further extensions of the Tsunami propagation model such as combination of different element shapes cannot be straightforward. Therefore, in this study, we proposed an extensive hp adaptive DG model based on Object-Oriented Design. The present model is constructed on the computational grid system (called “Systematic Grid”). The Systematic Grid is composed of three object layers of parallel computation (Domain object), spatial resolution (Block object) and computational element (Element object). The size and the order of the Element object are adjusted in each Block object independently. The Block objects of different spatial resolution and order of the solution are connected with Connector object which interpolate numerical fluxes between them. Applicability of the present hp adaptive DG method is examined with the problems of the Rossby wave propagation and symmetric shock-on-shock interaction. The result of the Rossby wave shows the hp adaptive DG method suppresses the numerical diffusion with low computational cost compared to that without the hp adaptation. It also suggests that the rectangular element keeps better symmetricity than that of the triangular element. The result of the latter problem shows the hp adaptive DG method can maintain the sharpness of the shock waves such as the Tsunami front.


HS11-A024
Enhancing Equitable Distribution and Network Resilience in Intermittent Water Supply Systems

Vasan ARUNACHALAM#+, M. Naveen NAIDU, Murari RR VARMA
Birla Institute of Technology and Science, Pilani

Water supply systems are essential for urban infrastructure systems, as they deliver water from water sources to domestic, commercial, and industrial water users to maintain their daily activities. Water supply system design, construction, operation and maintenance are a huge challenge for engineers worldwide. Design optimization of water distribution networks has been thoroughly researched over the past few decades due to its computational and engineering complexity. In developing countries, intermittent water supply is followed in which the water is supplied only for a fixed duration of a week. One of the major challenges associated with intermittent water supply systems is maintaining equitable water distribution. Several researchers have explored designing of intermittent water supply system as a single objective in terms of minimizing network cost. However, designing an intermittent water supply system is a multiobjective problem keeping in mind the several challenges faced by the field engineers. In view of this, the present study proposes to design the intermittent water supply system in a multiobjective scenario considering network cost (minimizing), network resilience (maximizing) and equitable water supply (maximizing). Particle swarm optimization technique has been used to solve the multiobjective mathematical model, while EPANET is used for hydraulic simulation. The proposed methodology is tested on two benchmark problems: Two loop network and Hanoi network. The results from the analysis infer the trade-off between network cost, network resilience and equity for both networks. It is observed that a moderate increase in the network cost yields better equity as well as network resilience.


HS11-A004
Source Identification of Nitrate Pollution in Groundwater Using Fecal Sterol Markers of an Urban Area in Japan

Kei NAKAGAWA1#+, Zhuolin LI1, M. Shahidal ISLAM1, Taito AIHARA2, Takahiro HOSONO2, Yuji TAKAO1
1Nagasaki University, 2Kumamoto University

Nitrate pollution threatens groundwater in many areas of the world. Meanwhile, nitrate pollution sources can be assumed to be the situation but are difficult to identify. Therefore, investigating the source of nitrate pollution is essential to controlling groundwater pollution. We have proposed to use fecal sterols to identify the sources of nitrate pollution. In the present study, we measured coprostanol (5β), cholestanol (5α) as well as sterol ratio (5β/(5β+5α)) and NO3- concentration to predict the sources of nitrate pollution of groundwater in Kumamoto city area, Japan. Deep groundwater samples were collected from 13 locations from June 2022 to January 2023 and analyzed. The laboratory finding of coprostanol concentration ranged from 115.2 ng L-1 to 756.1 ng L-1 and was found nearer the urban area. In the summer, four sampling stations were found of relatively high coprostanol concentrations accompanied by low nitrate content. The ORP and DO results confirmed the denitrification of nitrate occurred in these study locations. The high content of coprostanol indicated that nitrate contamination originated from livestock farming. Thus, the fecal indicators may be a useful tool for source identification of nitrate pollution in study areas and can be more effective.


HS11-A006 | Invited
Patch Size Effect on Dissolved Inorganic Carbon Absorption by Submerged Aquatic Vegetation

Keisuke NAKAYAMA1#+, Keita MATSUMURA1, Hiroki MATSUMOTO2, Tetsuya SHINTANI3
1Kobe University, 2Port and Airport Research Institute, 3Tokyo Metropolitan University

Global warming has accelerated the occurrence of natural disasters such as floods and droughts, which are considered to be due to climate change. Nellemann (2009) showed that 55% of the earth's total carbon storage is due to photosynthesis by seagrass meadows and kelp systems, called "Blue carbon", and there is a considerable possibility that blue carbon ecosystem can capture and store carbon dioxide from the atmosphere. Submerged aquatic vegetation (SAV), such as seagrass meadows, grow in patches, suggesting a complex interaction between currents and the flexibility of SAVs, meaning that the carbon absorption rate is affected by the complex interactions. Therefore, enhancing carbon capture and storage using aquatic vegetation is urgent, and it is necessary to approve submerged aquatic vegetation efficiently absorbs carbon dioxide from the atmosphere. This study thus aims to investigate the patch size effect on carbon absorption by SAVs using numerical simulations. As a result, the extent to which the patch occupies the water area was found to be the most substantial factor in controlling carbon capture, and deflection was found to be another significant factor. Additionally, we successfully proposed an equation to estimate carbon sequestration using these two factors.


HS11-A025
Impacts of Multiple Water Sources on Water Quality of Urban Rivers

Shurong ZHANG#+, Ling BAI, Yijuan BAI
Beijing Normal University

For urban rivers with water shortages and degradation, water supplies from multiple sources play important roles for improving river ecological status. However, the impact of different water sources on the water quality of the rivers are still not clarified yet. In this study, inorganic ions, dissolved organic carbon and optical spectrum characteristics of organic matter of the urban rivers in Beijing, China were investigated and the impacts of different water sources (reclaimed water, diverted natural water, etc.) were analyzed. Our study suggests the importance of understanding the impact of different water sources on the river water quality for the sustainable river management in the water shortage regions.


HS11-A027
Fundamental Study on Accurate Prediction of River Temperature Using Deep Learning

Daichi FUKUMARU+, Yoshihisa AKAMATSU#
Yamaguchi University

There have been concerns about the effects of climate changes on river water quality and ecosystems due to the increased river temperature. Thus, it is necessary to predict basin-wide river temperature based on the data from future climate models such as d4PDF. In this study, we developed a basin-wide river temperature prediction model using deep learning and implemented a fundamental study for accurate prediction of water temperature for the Takatsu River in Japan. We developed two models (Case1 and Case2) with different input data using LSTM, which had high ability of learning time-series data. On both cases, the inputs were past 7 days data at multiple points in each river basin and the outputs were hourly river temperature at the current time. However, in the input layer, Case1 had air temperature, while Case2 had the air temperatures and precipitation. We observed continuous river temperature at 13 points over the Takatsu River. The observed hourly river temperature, air temperature from The Agro-Meteorological Grid Square Data, and precipitation from Rader-AMeDAS composite precipitation were used for the analyses. The model was trained based on the correlation between input and output data from 12/3/2016 to 12/31/2019, and the model prediction was implemented by inputting the data from 1/1/2020 to 12/31/2020. Case1 overestimated the observed value during the June-October flood season, whereas Case2 reduced the overestimation. The Nash-Sutcliff coefficient (the goodness of fit between predicted and observed values) of Case2 exceeded that of Case1 at most points. In particular, the Nash-Sutcliff coefficient for Case1 was about 0.65 at the middle and lower reaches, while that for Case2 was 0.75, showing significant difference in accuracy. These results suggest that using precipitation data for the inputs can improve the prediction accuracy on flood season at the middle and lower reaches with large catchment area.


HS11-A016
Comparative Analysis of Stream Water Temperatures in River Basins with Different Degrees of Urbanization

Hitoshi MIYAMOTO#+, Shuji IDEI
Shibaura Institute of Technology

This study analyzed the characteristics of stream water temperature fluctuations in rivers with different degrees of urbanization by comparing rivers with significant urbanization and rivers with many forests in their river basins. This study calculated the theoretical equilibrium water temperature, and its deviation from the observed water temperature was used to examine the effects of urbanization. The Tama River, an urban river, has a basin area of 1,240 km2, and approximately 3.8 million people live in the middle and lower reaches. Eight water reclamation centres are located along the river from midstream to downstream. On the other hand, the Ibo River, a rural river, has a basin area of 810 km2, and the population is 700,000. The Ibo River has little treated water inflow. Meteorological data from meteorological observatories near the observation points were used to calculate the equilibrium water temperature. Analysis of water temperatures in both rivers indicated that the correlation between the observed and equilibrium water temperatures was smaller in the Tama River. Its deviation was more significant in low-temperature circumstances. The seasonality of water temperature fluctuations showed substantial differences in spring and winter. In particular, the river water temperature in the Tama River showed characteristic large fluctuations along with the downstream direction. It could be attributed to the rapid temperature rise due to the inflow of high-temperature treated water from the water reclamation centres and the rapid temperature decrease due to the influx of low-temperature water from the tributaries. These results revealed that the Tama River's river temperatures in the urban river basin were significantly altered compared to those of the Ibo River in the rural river basin. Such rapid changes in stream water temperature could have significantly impacted the fluvial ecological environment in the urban river.


Tue-01 Aug | 10:20 - 12:20 | MR311
HS03 - The Third Pole Environment and High Mountains of Central Asia - Hydrometeorological Processes and Human Dimension

Session Chair(s): Yaoming MA, Chinese Academy of Sciences, Petrus (Peter) VAN OEVELEN, George Mason University

HS03-A007
Comprehensive Study of Energy and Water Exchange Process and its Climatic Effects Over the Third Pole

Yaoming MA#+
Chinese Academy of Sciences

Containing elevated topography, the Tibetan Plateau (TP) has significant thermodynamic effects for regional environment and climate change, where understanding energy and water exchange process (EWEP) is an important prerequisite. However, estimation of the exact spatiotemporal variability of the land-atmosphere energy and water exchange 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 EWEP via observation, remote sensing, and numerical simulation. Based on the three main approaches, the major advances on EWEP over the past 25 years are systematically summarized in this work. Observations reveal distinct characteristics of the energy balance components and micrometeorological parameters. Moreover, multisource (multispectral, thermal, and microwave) satellite data have been successfully used to retrieve key land–atmosphere properties, which offers a feasible way to monitor EWEP at different spatiotemporal scales. In addition, different numerical models have been evaluated and improved to study EWEP over heterogeneous land surfaces. All these results advanced the understanding of different aspects of EWEP over the TP by using in situ measurements, multisource satellite data and numerical modeling. 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 EWEP on weather and climate changes over the TP and surrounding regions.


HS03-A002
Future Changes in Drought Over Central Asia Under CMIP6 Forcing Scenarios

Lijuan HUA1#+, Linhao ZHONG2, Tianbao ZHAO3
1University of Chinese Academy of Sciences, 2National Institute of Natural Hazards, Ministry of Emergency Management of China, 3Chinese Academy of Sciences

New hydrological insights for the region: Corresponding to the spatially consistent warming in Central Asia, an asymmetrical west–east-orientated dipole precipitation pattern, i.e., a decrease in the west but an increase in the east, is found in the warm-season (April to September) precipitation of future projections. A similar but even stronger west–east or northwest–southeast contrast is found in the changes in total runoff and surface soil moisture in response to future warming. Most of Central Asia shows an increase in drought frequency and duration by the end of the current century, mainly caused by the consistently enhanced evaporation that roughly balances the precipitation growth after 2030. When the effect of temperature is considered, the drought area of Central Asia displays a significant upward trend under both the moderate and high emissions pathway. However, in the east of the region, including Northwest China and western Mongolia, warming and wetting tendencies under the future warming climate are apparent, regardless of the drought definition.


HS03-A003
Quantifying the Spatial Characteristics of the Moisture Transport Affecting Precipitation Seasonality and Recycling Variability in Central Asia

Linhao ZHONG1#+, Lijuan HUA2
1National Institute of Natural Hazards, Ministry of Emergency Management of China, 2University of Chinese Academy of Sciences

Moisture contribution and transport pathways for Central Asia (CA) are quantitatively examined using the Lagrangian water cycle model based on reanalysis and observational data to explain the precipitation seasonality and the moisture transport variation during 1979–2015. Westerly-related (northwesterly and westerly) transport explains 42% of CA precipitation and dominates in southwest CA, where precipitation is greatest in the cold season. Southeast CA, including part of Northwest China, experiences its maximum precipitation in the warm season and is solely dominated by southerly transport, which explains about 48% of CA precipitation. The remaining 10% of CA precipitation is explained by northerly transport, which steadily impacts north CA and causes a maximum in precipitation in the warm season. Most CA areas are exposed to seasonally varying moisture transport, except for southeast and north CA, which are impacted by southerly and northerly transport year-round. In general, the midlatitude westerlies-driven transport and the Indian monsoon-driven southerly-related transport explain most of the spatial differences in precipitation seasonality over CA. Moreover, the contribution ratio of local evaporation in CA to precipitation exhibits significant interdecadal variability and a meridionally oriented tripole of moisture transport anomalies. Since the early 2000s, CA has experienced a decade of anomalously low local moisture contribution, which seems jointly determined by the weakened moisture contribution from midlatitudes (the Atlantic, Europe, and CA itself) and the enhanced contribution from high latitudes (West Siberia and the Arctic) and tropical areas (South Asia and the Indian Ocean).


HS03-A004
Increasing Lake Water Storage on the Inner Tibetan Plateau Under Climate Change

Binghao JIA#+, Longhuan WANG, Zhenghui XIE
Chinese Academy of Sciences

The Inner Tibetan Plateau (TP) is an endorheic basin with densely distributed lakes that serve as 'sentinels' of climate change. The accurate estimation of lake water storage (LWS) changes on the Inner TP is vital for studying lake ecosystems and water resources. Owing to the cold environment and oxygen deprivation on the TP and the complex natural conditions, a significant amount of human and material resources are required to estimate the LWS using in situ measurements. Using Gravity Recovery and Climate Experiment (GRACE) data and land surface model simulations, we estimated the LWS for 18 lakes (>300 km2) on the Inner TP from 2002 to 2018. The estimated LWS agreed with the multi-source satellite altimetry data. The LWS of the 18 lakes on the Inner TP expanded rapidly with an increasing rate of 26.92 mm year-1. The increasing rate of LWS by the mid-twenty-first century for an intermediate scenario is predicted to decrease to 40% of that in recent decades based on an artificial neural network model. This prediction is supported by the terrestrial water storage and glacial runoff projections on the Inner TP. The results of this study highlight the importance of water resource mitigation and adaptation to avoid flood threats from increased LWS on the Inner TP. The LWS estimations based on GRACE data and land surface model can be used to identify regional changes in lakes for areas with limited available data, which is a helpful tool for monitoring lake water resource changes.


HS03-A006
Modeling the Impact of Climate Change on Water Availability in the Snow-Glacier-fed River Basin of the Central Himalayas

Insaf ARYAL1#+, Navraj DHAKAL2, Piyush DAHAL2
1Central Department of Hydrology and Meteorology, 2Recham Consult Pvt. Ltd

The Himalayas play a critical role in the water availability of South Asia. A SWAT hydrological model was developed for the Madi River Basin, the Snow-Glacier-fed basin in Nepal of the Central Himalayas, to evaluate the impact of climate change on water availability. The model was calibrated for ten years (1986-1995) and validated for 20 years (1996-2015) using daily flow data. The performance of the model was rated "very good." To assess the impact of climate change on river discharge, the projected daily minimum and maximum temperature and precipitation data (1980-2100) from five bias-corrected and downscaled climate models (ACCESS-ESMI-5, BCC-CM2-MR, CNRM-ESM2-1, GFDL-ESM4, INM-CM5-0) were incorporate the calibrated SWAT model for SSP245 and SSP585 scenarios. The model was rerun to determine the effect of climate change on river flow in the basin. The results indicate that there will be a significant change in water availability in the basin in the future compared to the historical record. The future discharge will increase with increased precipitation and temperature, while the snowmelt contribution will also increase significantly due to climate change. The result shows that the highest increase in flow in the basin will occur during the monsoon (JJAS) season, while during the other seasons the flow decreases. This study will provide valuable information for future hydropower, irrigation, and infrastructure planning in the basin and downstream.


HS03-A010
Development of a High-resolution Tibetan Plateau Climate System Model and its Application in Developing Precipitation Product

Kun YANG1#+, Xu ZHOU2, Yaozhi JIANG1, Xin LI2
1Tsinghua University, 2Chinese Academy of Sciences

The Tibetan Plateau is a region with strong land-atmosphere interactions, and it is urgent to develop a climate system model that can present the interactions in order to improve climate simulation capabilities and deepen the understanding of climate change processes and impacts. Current climate models generally simulate too wet, too cold and too windy climate in the Tibetan Plateau. To improve climate modeling capacities for this region, a joint team was established to develop a high-resolution Tibetan Plateau climate system model (TPCSM) based on WRF4.0. So far, the team has implemented parameterization schemes of turbulent drag, hydrological process and snow cover fraction associated with complex terrain, with which the TPCSM much reduces the above-mentioned modeling errors. Further improvements of land surface process schemes also contribute to reducing the above errors. Short-term high-resolution (3km) atmospheric simulation with the TPCSM obtains the fine-scale spatial distribution of precipitation. The short-term simulation precipitation result is used to downscale ERA5 precipitation data through a machine-learning statistical method and the downscaling data can show the variations of precipitation on large spatial and temporal scales; finally, by fusion the downscaling data with data from high-density rain gauges (over 9000), a long-term (1979-2020) high-resolution (1/30°) precipitation dataset for the Tibetan Plateau is generated. The data accuracy is significantly better than widely used global/quasi-global datasets.


HS03-A012
Response of Surface Energy Fluxes and Hydrothermal Characteristics to Precipitation Changes in the Southeastern Tibetan Plateau

Qingxue DONG#+, Siqiong LUO
Chinese Academy of Sciences

This study assessed the simulation applicability of the land-surface model CLM 4.5 in the southeastern Tibetan Plateau with field observation data of Kabu and Pailong, and used the model to study the impact of precipitation changes on surface radiation, energy fluxes, and soil hydrothermal characteristics in this region. It is found that the CLM 4.5 simulates radiation, energy fluxes and soil temperature credibly in this region. The deviation of the simulation for soil moisture is mainly manifested in the small fluctuation of the simulated value during precipitation, so the simulation effect is worse in the period of heavy rainfall than in the period of less rainfall, which is reflected in the failure to simulate the rapid change of latent heat flux and soil moisture during heavy precipitation. The sensitivity test concluded that precipitation plays an important role in surface radiation, energy cycle and soil hydrothermal process, and each element changes significantly with the change of precipitation. The elements were more sensitive to decreases than increases in precipitation, and changes in precipitation had a more pronounced effect on relatively dry areas and seasons and less on already extremely wet areas and seasons. Our results highlight the non-negligible influence of precipitation on surface hydrothermal characteristics and energy cycle in Southeastern Tibetan Plateau.


Tue-01 Aug | 10:20 - 12:20 | MR333
HS08 - Drought Characterizing and Modelling Hydroclimatological Processes in a Changing Environment

Session Chair(s): Jun NIU, China Agricultural University

HS08-A015 | Invited
How Climate and Vegetation Changes Impact Water Availability and Ecosystem Conditions in the Yellow River Basin

Fubo ZHAO#+
Xi'an Jiaotong University

Terrestrial ecosystems provide crucial ecosystem services to human beings, and their functions are largely dependent on soil moisture availability. Although many studies have evaluated the effects of vegetation and climate changes on soil moisture at the ecosystem scale, changes in ecosystem water limitation remain poorly understood. This study evaluated the spatiotemporal changes of ecosystem water limitation in the Yellow River Basin (YRB)—the second largest river basin of China—during 1982–2016 and identified the major drivers by establishing ecosystem limitation index (ELI) using soil moisture, transpiration, net radiation, and air temperature. The results show a significant and widespread spatiotemporal increase in the water limitation of ecosystems in YRB during the 35-year study period. Temporally, areas with positive ELI (water-limited regime) exhibited a significant upward trend (p < 0.01). Spatially, above 75.0% of the total areas showed upward trend in ELI Almost all ecosystems showed significant upward trends in water limitation over this period. Further analysis using two different but comparable methods, partial correlation (PC) and Lindeman-Merenda-Gold (LMG), show that vegetation change was the major driver of changes in water limitation, with contributions of more than 35.0%. Air temperature and atmospheric CO2 changes contributed comparably to changes in positive ELI, followed by precipitation changes. These findings improve the understanding of the spatiotemporal pattern and underlying mechanisms of ecosystem water limitation in the greening and warming YRB.


HS08-A020
Impacts of Land Use Change in the Water Quality and Sediment Transport in the Sambunotan Watershed, Dinagat Island, Philippines

Nichole Anthony PACLE#+, Michelle JAPITANA, Riva Karyl VARELA, Marjunelyn LLESIS, Jahn Rey BAUTISTA, Stephanie Mae SALCEDO-ALBORES, Jojene SANTILLAN, Meriam MAKINANO-SANTILLAN
Caraga State University

The Sambunotan Watershed in the Dinagat Islands, Philippines is a relatively pristine watershed that supplies water to two municipalities (i.e., Tubajon and Loreto) in northern Mindanao. This watershed is on the verge of rapid development by virtue of cropland conversion and nickel laterite exploration. This projected drastic land use change in the area will have an impact on the water quality and sediment transport, hence possibly affecting the water availability and flooding mitigation measures in the local communities. Water quality data collection of samples were done during May and November for the dry and wet seasons, respectively. Total dissolved solids (TDS), dissolved oxygen (DO), pH, surface water temperature were obtained alongside the acquisition of suspended sediment concentration (SSC), and the riverbed sediments for sediment transport analyses. Grain size analysis was performed for the riverbed sediments in order to determine the erodibility index, while the SSC was utilized to calculate the sediment yield and sediment budget in the fluvial system. The land use- land cover distribution of the sampling points was analyzed to better understand and describe the Sambunotan Watershed employing the “Contributing area" concept. Correlation and regression analyses were conducted to evaluate the relationship between land use to water quality and soil erodibility in the watershed. The results from the study imply that human activities within the watershed can indeed affect the quality of the surface waters, as well as the erodibility in the area. The statistical analysis confirmed the importance of trees in the watershed and the impacts of the practices within the cropland and built-up areas. ​Per assessment, the sampling sites passed the Class AA government standards in the majority of the sampling sites. The local government needs to intensify their watershed protection programs especially with regard to land use planning.


HS08-A013
Increased Sensitivity of Vegetation to Soil Moisture and Its Key Mechanisms in the Loess Plateau, China

Xi WANG+, Yiping WU, Fubo ZHAO#
Xi'an Jiaotong University

Soil moisture (SM) plays a crucial role in connecting various ecological processes in terrestrial ecosystems, as vegetation growth heavily relies on soil moisture availability. Despite many studies evaluating the impacts of SM on vegetation activity, changes in vegetation sensitivity to SM are still poorly understood. In this study, we evaluated the spatiotemporal changes of vegetation sensitivity to SM across the Loess Plateau region from 1982 to 2010 using satellite-based normalized difference vegetation index (NDVI) and reanalysis SM data. Our results showed a significant increase in NDVI (slope = 0.0015/yr, p < 0.001) and a slight decrease in SM (slope = -0.0001m3/m3/yr, p = 0.7) over the past 29 years, indicating a greening trend in the Loess Plateau. By establishing a multiple linear model, we found that the sensitivity of vegetation dynamics to SM has significantly increased during the same period (slope = 0.029, p < 0.05). Spatially, vegetation in over half (51.2%) of the total areas showed enhanced sensitivity to SM. Further analysis using the Lindeman-Merenda-Gold method showed that atmospheric CO2 was the major contributor (27.2%) to the sensitivity changes, followed by nitrogen deposition (23.70%) and air temperature (20.11%). Changes in ecosystem structure (represented by non-tree cover land fraction areas) and precipitation contributed comparably to the sensitivity change (16.13% and 12.83%). These findings provide a better understanding of the spatiotemporal pattern and underlying mechanisms of ecosystem sensitivity to SM in the greening and warming Loess Plateau.


HS08-A009
A Hierarchy of Drought Projections for Australia

Anna UKKOLA1#+, Steven THOMAS2, Elisabeth VOGEL1, Ulrike BENDE-MICHL2
1UNSW Sydney, 2Bureau of Meteorology

Australia suffers from frequent droughts but future projections of drought have remained stubbornly uncertain over the continent. Here we explore future changes in drought over Australia using a hierarchy of projections from coupled global and regional climate models and several offline hydrological models that are widely employed in Australia. We analyse changes in hydrological (runoff) and agricultural (soil moisture) droughts across the different modelling methods using a consistent definition of drought. Our study aims to better quantify uncertainties in future hydrological projections over Australia and explore the causes behind the uncertainties arising from different modelling methods.


HS08-A011
Global Patterns of Drought Propagation Under Future Warming

Shulei ZHANG#+
Sun Yat-sen University

Quantifying the changes and propagation of drought is of great importance for regional eco-environmental safety and water-related disaster management under global warming. In this study, phase 6 of the Coupled Model Intercomparison Project was employed to examine future meteorological (Standardized Precipitation Index, SPI, and Standardized Precipitation–Evapotranspiration Index, SPEI), hydrological (Standardized Runoff Index, SRI), and agricultural (Standardized Soil moisture Index, SSI) drought under two warming scenarios (SSP2-4.5 and SSP5-8.5). The results show that, across the globe, different types of drought events generally exhibit a larger spatial extent, longer duration, and greater severity from 1901 to 2100, with SPEI drought experiencing the greatest increases. Although SRI and SSI drought are expected to be more intensifying than SPI drought, the models show higher consistency in projections of SPI changes. Regions with robust drying trends include the southwestern United States, Amazon Basin, Mediterranean, southern Africa, southern Asia, and Australia. It is also found that meteorological drought shows a higher correlation with hydrological drought than with agricultural drought, especially in warm and humid regions. Additionally, the maximum correlation between meteorological and hydrological drought tends to be achieved at a short time scale. These findings have important implications for drought monitoring and policy interventions for water resource management under a changing climate.


HS08-A002
Evaluating the Hydrologic Risk of Drought in Nakdong River Basin Using a Dynamic Naïve Bayesian Classifier-based Composite Drought Index

Hyeok KIM1+, Seungho HONG1, Hyun-Han KWON2, Tae-Woong KIM1#
1Hanyang University, 2Sejong University

The frequency and intensity of natural disaster have recently increased due to climate change. Especially, drought is resulted from various factors and results in extensive hydrological and agricultural impacts. To develop effective drought mitigations, it is necessary to use a composite drought index to consider various factors and to evaluate future drought comprehensively. Thus, this study evaluated hydrologic risk of future drought in Nakdong River basin based on the DNBC(Dynamic Naïve Bayesian Classification)-based composite drought index. The DNBC-based composite drought index was calculated by SPI, SDI, ESI and WSCI. The individual indices were calculated according to the climate change scenarios as well as observed data. Hydrologic risk of drought was calculated based on the return period of drought events estimated by bivariate frequency analysis of drought severity and duration. The result showed that the hydrologic risk increased for the future period(2021-2040)(on average, and Miryang River basin (#2021) had the highest hydrologic risk( . For the far future(2040-2099), the hydrologic risk decreased in the northern basins of Nakdong River basin and increased in the southern basins. It showed that the future drought of Nakdong River basin will move from northern basins to southern to basins. The results of this study are useful for decision makers to respond future drought effectively and strategically. 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)(No.2022003610001).


HS08-A003
Extreme Drought Event Susceptible to Groundwater Recharge Zonation: A Case Study from Western Odisha, India

Madhusmita OJHA1#+, Chandrakanta OJHA2, Ipsita NAYAK3, Shreerup GOSWAMI4, Pramod Chandra SAHU1
1Maharaja Sriram Chandra Bhanja Deo University, 2Indian Institute of Science Education and Research Mohali, 3Odisha Space Application Centre, 4Ravenshaw University

Extreme droughts are responsible for causing serious underground water crises in many parts of the world. According to the Drought and famine in India, 1870–2016 report of Mishra, V. et al (2019) drought onset in the Indian subcontinent was observed during the 1876-78 great famine. In the eastern part of India, i.e., in particular, the northern region of Nuapada district of Odisha state has been affected by continuous drought for decades, causing the decline in groundwater level. However, less precipitation, high evapotranspiration, geological settings, consolidated hard rock terrains such as quartzite, granite gneiss, and khondalite, changes in the vegetation cover and land use pattern combinedly resulting further depletion of the water table. However, it is difficult to replenish all aquifer systems naturally and cumbersome to identify or map the potential groundwater (GW) zones in a region. In that context, an attempt has been made through this research study to locate the potential groundwater recharge zones in the drought-prone hilly terrain of the projected study area using geospatial techniques. Here, we considered a weighted probabilistic approach integrating various hydrogeological parameters as different thematic layers include lithology, slope, contour, geomorphology, drainage, Lineaments, NDVI and Land Use Land Cover over a geospatial platform to investigate suitable sites for recharge over the region. Further the groundwater prospective zones over the study region has been categorized into five major categories includes; excellent, good, moderate, moderate to poor and poor zones respectively. The result shows that the areas of suitable zones for recharge are 734.77, 250.272, and 718.548 Km² respectively lie in the west and few patches in the eastern side of the entire study area. Comparatively most part of Komna block lies in the poor zone whereas most of Nuapada block of the study area lies in the good to moderate zone category.


Tue-01 Aug | 10:20 - 12:20 | MR336
HS04 - Characterizing and Modelling Ecohydrological Processes in a Changing Environment

Session Chair(s): Huimin LEI, Tsinghua University

HS04-A011 | Invited
Impacts of Compound Droughts and Hot Extremes on Vegetation

Zengchao HAO#+, Yitong ZHANG
Beijing Normal University

Droughts and heat waves can pose severe threats to vegetation growth. Moreover, these extreme stresses can co-occur (e.g., compound droughts and hot extremes, CDHEs), leading to larger impacts than individual components. In this study, based on meteorological data and Normalized Difference Vegetation Index (NDVI), we evaluate the impacts of CDHEs on vegetation from a probabilistic perspective. This is achieved by constructing conditional models, in which the conditional distribution of vegetation response under different extreme stresses is evaluated. Our results indicate that compared with individual extremes (i.e., droughts, hot extremes), CDHEs can amplify the impact on vegetation in arid and semi-arid regions. Besides, for different vegetation types, vegetation decline for temperate grassland was remarkable under combined dry-hot conditions. This study provides useful insights for understanding vegetation response to compound droughts and hot extremes under global warming.


HS04-A001
Potential Evaporation and the Complementary Relationship

Zhuoyi TU1+, Yuting YANG1#, Michael RODERICK2, Tim MCVICAR3
1Tsinghua University, 2The Australian National University, 3Commonwealth Scientific and Industrial Research Organisation

The complementary relationship (CR) provides a framework for estimating land surface evaporation with basic meteorological observations by acknowledging the relationship between actual evaporation, apparent potential evaporation and potential evaporation (Epo). As a key variable in the CR, Epo estimates by conventional models have a long-standing problem in practical applications. That is, the meteorological forcings (i.e., radiation and temperature) employed in conventional Epo models are observed under actual conditions that are generally not saturated. Hence conventional Epo models do not conform to the original definition of Epo (i.e., the evaporation that would occur with an unlimited water supply). Here, we estimate Epo using the maximum evaporation approach (Epo_max) that does follow the original Epo definition. We find that adopting Epo_max considerably reduces the asymmetry of the complementary relationship compared to when the conventional Priestley-Taylor Epo is used. We then employ Epo_max and develop a new physically-based, calibration-free CR model, which shows an overall good performance in estimating actual evaporation in 705 catchments at the mean annual scale and 64 flux sites at monthly and mean annual scales (R2 ranges from 0.73 to 0.75 and root-mean-squared error ranges from 9.8 to 18.8 W m-2). More importantly, the use of Epo_max leads to a new physical interpretation of the CR.


HS04-A002
Development of an Evapotranspiration Data Assimilation Framework for Improving the Simulation of Crop Growth and Water Consumption

Cheng YANG+, Huimin LEI#
Tsinghua University

Data assimilation has been attracting considerable interest owing to the rapid development of remote sensing and field observation techniques. Integration of data assimilation approaches and crop models could diminish uncertainties of crop models and promote the precision of model simulation. While extensive studies have been focused on assimilating leaf area index (LAI) or soil moisture (SM), the feasibility and effectiveness of assimilating evapotranspiration (ET) has been rarely explored. In this study, we propose a novel framework of ET assimilation. Then, together with commonly used LAI and SM, we evaluate the performance of this new method in simulating the key indicators at daily and interannual scales based on the long-term eddy covariance field observation and a well calibrated and validated crop model. Data assimilation strategies designed in this study consist of different combinations of two approaches (i.e., Ensemble Kalman filter (EnKF) and EnKF with simultaneous state-parameter estimation (SSPE)) and three assimilated variables (i.e., LAI, SM, and ET). Our results demonstrate that assimilation of LAI and ET plays a dominant role in improving the model performance for wheat and maize, respectively. For interannual variation of LAI that is mainly controlled by agricultural managements (e.g., wheat), assimilating LAI is more effective. For daily ET with stronger variation (e.g., maize), assimilating ET is more informative. Assimilating average SM from 0-80cm only provides inaccurate information, whereas a joint assimilation of SM and ET performs the best in maize modeling where SM and ET or photosynthesis processes are tightly coupled. EnKF-SSPE outperforms EnKF and is more preferable for its potential to obtain the parameter evolution in long-term crop modeling when cultivars are regularly renewed. This study appraises different variables and approaches of data assimilation based on a newly proposed sequential ET assimilation framework, which may be illuminating in future work of data assimilation.


HS04-A005
Aerodynamic Effects Explain Higher Forest Evapotranspiration After Wildfires

Naika MEILI1#+, Jason BERINGER2, Jiacheng ZHAO3, Simone FATICHI4
1Singapore-ETH Centre, 2The University of Western Australia, 3Beijing Normal University, 4National University of Singapore

Wildfire extent, intensity and frequency is increasing in many parts of the world due to climate change. The destruction of forests by fire and the subsequent regrowth of young vegetation can lead to changes in evapotranspiration and downstream water resources availability. However, past research is still inconclusive on even the sign of these hydrological changes after fire as both decrease and increase in evapotranspiration or runoff have been reported post-fire. In this study, we combine mechanistic ecohydrological modelling, eddy-covariance measurements, and remote sensing over 18 years including both pre- and post-fire periods to quantify the effects of forest destruction and subsequent regrowth on evapotranspiration and runoff in an old-growth mountain ash forest (Eucalyptus regnans) in Australia. Eddy-covariance measurements, remote sensing and ecohydrological modelling show a fast recovery of evapotranspiration, which reaches and exceeds pre-fire magnitudes as fast as two years after the fire. A similar fast evapotranspiration recovery post-fire is found with remote sensing across multiple fires in eucalypt forests in south-eastern Australia and hence, is likely generalizable in this forest type. After removing climate variability effects, ecohydrological modelling simulates a peak increase of +20% evapotranspiration three years after the fire originating from the young recovering forest and as a result, a substantial runoff reduction is also simulated. Model results show that the evapotranspiration increase is mostly caused by aerodynamic land-surface warming due to a shorter forest stature post-fire, which leads to higher humidity gradients between leaf interior and air and therefore enhanced transpiration. Such an increase in evapotranspiration caused by the aerodynamic effects of converting tall into shorter forests could also influence the hydrological response after wildfires in other regions of the world.


Tue-01 Aug | 1:10 - 3:10 | MR311
HS03 - The Third Pole Environment and High Mountains of Central Asia - Hydrometeorological Processes and Human Dimension

Session Chair(s): Toru TERAO, Kagawa University, Petrus (Peter) VAN OEVELEN, George Mason University

HS03-A018
Impact of the Initial Soil Conditions on Soil Hydrothermal and Surface Energy Fluxes in the Permafrost Region on the Tibetan Plateau

Siqiong LUO#+, Zihang CHEN
Chinese Academy of Sciences

The accurate initial soil state is important for soil hydrothermal and surface energy fluxes in land surface process modeling. In this paper, using different initial soil conditions, the performance of the Community Land Model 5.0 (CLM5.0) for simulating soil temperature (ST), soil moisture (SM) and surface energy fluxes in the permafrost region on the Tibetan Plateau (TP) was assessed. Results showed the initial field of ST, soil liquid water (SLW) and soil ice (SI) obtained by the spin-up method was limited. Three modified initial soil conditions improved the ST and SM simulation effectively by reducing the root mean square error (RMSE) and mean bias error (MBE), and improving Nash–Sutcliffe efficiency (NSE), especially in permafrost layers. The average MBE of ST was reduced by 64%, 88 % and 77% while it was only reduced by 11% in two spin-up experiments. The average RMSE of SLW was reduced by 13%, 21% and 19% in these two modified experiments while it was only reduced by 5% in the two spin-up experiments. Modified initial soil condition experiments could simulate the characteristics of ST and SM profiles in permafrost. The estimations of net radiation and ground heat flux were much improved by the modified initial soil conditions. The average MBE of net radiation was reduced by 7%, 22% and 21%, respectively, and the average MBE of ground heat flux was reduced from -1.78 W m-2 to -1.64 W m-2.


HS03-A019
Effects of Precipitation on Soil Hydrothermal Characteristics and Freeze-thaw Process on the Seasonally Frozen Ground

Jingyuan WANG#+
Chinese Academy of Sciences

The variations on precipitation were analyzed at Madoi and Maqu sites in 2014-2018 on the seasonally frozen ground of the source region of the Yellow River. In addition, the effects of precipitation on soil hydrothermal characteristics and freeze-thaw process of frozen ground at two sites were also investigated. The results showed that the precipitation of Madoi site was the least in 2015, while the precipitation in 2018 was the most. The annual precipitation of Maqu site was higher than that of Madoi site, and the precipitation of Maqu site in 2016, 2017 and 2018 were higher than that of 2014 and 2015. Due to the sufficient precipitation in September and October of 2014 and 2017 at Madoi site, soil moisture in 2014 and 2017 were higher before soil freezing, more liquid water frozen into ice, the greater latent heat released by soil freezing, the slower the cool rate of soil was. As a result, the beginning of freezing in the two years were later than that of other years, but the ice content of soil in the complete freezing stage were higher than that of other years. From 2014 to 2018, the precipitation in April of 2016 was the lowest. During the soil melting stage, the temperature of precipitation was higher than temperature of soil in the spring and summer, so the increase in precipitation would lead to the acceleration of soil thawing, and the end of thawing in 2016 was later than other years. Similar conditions existed on Maqu sites in October and February 2018.


HS03-A023
Parameterization of Pasture and Toxic Weeds in Community Land Model (CLM5) Over the Three River Source Region on the Tibetan Plateau

Yaqiong LU#+, Bintao LIU, Yan YANG, Hui YU
Chinese Academy of Sciences

The Three River Source Region is the source of Yangtze, Yellow, and Lancang (Mekong) river, which played a fundamental role for water security in Asia. Historically, the region has experienced severe ecological degradation due to human activities. Since the dramatic stream flow reduction of the Yellow River in the 1990s, a series of ecological restoration and protection projects have been carried out in the Three River Source Region that increased grassland coverage and water supply capacity. Our field survey in 2008 and 2018 at 36 alpine grassland sites showed that the aboveground biomass increased for legumes and forbs (toxic weeds), but decreased for grasses and sedges (pasture). The pasture and toxic weeds showed quite different role in altering surface energy and water cycles, and their response to climate changes are not the same. Many advanced land surface models incorporated vegetation growth modules to simulate vegetation growth, however, seldom current land surface models considered the different growth of pasture and toxic weeds. To better represent the different growth for pasture and toxic weeds, we developed a global parameter parametrization method for CLM5 based on eFAST algorithm to understanding the key parameters that affecting grass growth. Then we calibrated two sets of parameters representing pasture and toxic weeds growth and performed future scenario simulations to understand the pasture and toxic weed biomass changes. Our primary results showed the toxic weeds biomass may continue increase from 2030 to 2050, while the pasture biomass changes showed large uncertainties across different SSP scenarios.


HS03-A036
Lightning Climatology and Extreme Lightning Event Analysis in Northeast India Using TRMM LIS and WRF Model: Implications for Hazard Mitigation

Unashish MONDAL1,2#+, Subrat Kumar PANDA1, S. DAS1, Toru TERAO3, Fumie MURATA4
1Central University of Rajasthan, 2Ministry of Earth Sciences, 3Kagawa University, 4Kochi University

The aim of the study is to investigate the lightning climatology over mountainous region over the northeast part of India by using Tropical Rainfall Measuring Mission (TRMM) Lightning Imaging Sensor (LIS) at 0.1 degree resolution datasets from 1998-2013. The study identified lightning hotspots in the region where the frequency of lightning strikes exceeded 50 flashes/km2/yr. This information is crucial for mitigating the potential hazards associated with lightning in the region. According to the latest report by the Indian Meteorological Department (IMD) and Down to Earth, the northeastern region experienced a staggering 68 days of extreme lightning events in 2022, which unfortunately resulted in over 810 fatalities. This study also examines the intense lightning event that occurred in the northeast part of India on June 17 and 18, 2022, and its association with hydrometeors and precipitation. The use of the WRF model with the Morrison double moment scheme 6-class microphysics and lightning parameterization scheme (PR92) to simulate the cloud to ground and inter cloud (CG:IC) lightning and precipitation. The NASA Gridded rainfall estimates from GPM Combined Radar-Radiometer provides the most accurate, high-resolution surface rainfall rate and precipitation vertical distribution estimations from satellite with 0.25-degree resolution used for validation of the model simulated precipitation and hydrometeors. The cross-calibrating radiometer estimates is crucial for obtaining a reliable precipitation record for climate science and model prediction validation. In conclusion, this study provides valuable insights into lightning climatology in the northeast region of India and the potential hazards associated with lightning strikes. The use of advanced modeling techniques and data sources can help in better predicting and managing the impacts of extreme weather events, which can potentially save lives and reduce the damage caused by such event.


HS03-A017
Collaborative Observational and Modeling Initiative Toward Understanding of Asian Hydroclimatological System

Toru TERAO1#+, Shinjiro KANAE2, Jun MATSUMOTO3,4, Hatsuki FUJINAMI5
1Kagawa University, 2Tokyo Institute of Technology, 3Tokyo Metropolitan University, 4Japan Agency for Marine-Earth Science and Technology, 5Nagoya University

We launched new Asian hydroclimatological research project, Asian Precipitation Experiment (AsiaPEX) in 2019. AsiaPEX is a successor of GAME and MAHASRI, Asian Regional Hydroclimatological Projects (RHPs) in recent decades. AsiaPEX aims to understand Asian terrestrial precipitation over diverse hydroclimatologial conditions for improvement of prediction, disaster reduction, and sustainable development over this region. AsiaPEX adopt six approaches 1) observation and estimation of precipitation, 2) process studies focusing on the land-atmosphere coupling, 3) interactions among systems in different spatio-temporal scales, 4) high-resolution hydrological modeling that includes humanosphere and cryosphere, 5) initiative for collaborative observation and modeling, and 6) climate projection under the warming climate.Based on the achievement of previous RHPs and recent development of our research activities after the kick-off conference in 2019, in the present paper, we will review these research status, and will propose expected next steps of science on Asian hydroclimatological system; 1) the observational platform focusing on a sub-regional process-oriented studies, and 2) integrated analysis using global modeling, reanalysis and remote sensing dataset. They will be performed through a Asia scale collaborative observational and modeling initiative, Asian Monsoon Year (AMY)-II. AMY-II will be planned in the latter half of 2020's, from 2025. We will discuss implementation plan of AMY-II. In the Asian hydroclimatological system, interaction between Tibetan Plateau and surrounding landmass plays important role. Therefore, we will further suggest key research targets that should be tackled under the collaboration of TPE and AsiaPEX.


HS03-A013
A Soil Temperature Dataset Based on Random Forest Model in Three River Source Region

Xiaoqing TAN#+, Siqiong LUO
Chinese Academy of Sciences

Soil temperature is an important physical variable that characterises geothermal conditions and influences geophysical, biological and chemical processes in the earth sciences. Soil temperature is not only influenced by climatic and geographical factors, it is also regulated by local factors of soil properties. In this paper, we use the random forest regression method to model the soil temperature observations from 0-320 cm at 23 stations in the Three River Source Region (TRSR) and combine the climate reanalysis data (the China Meteorological Forcing Dataset, CMFD), soil properties dataset (Dataset of Soil Properties for Land Surface Modelling over China), the snow cover (China 5 km Cloud-gap-filled Advanced Very High Resolution Radiometer Snow Cover Extent product dataset, CGF-AVHRR SCE) and vegetation remote sensing data (Global Inventory Monitoring and Modelling System, GIMMS NDVI3g v1) to simulate a new soil temperature set for the Sanjiangyuan region from 1982-2015. Site validation of the dataset showed Nash-Sutcliffe efficiency coefficient (NSE) of 0.97, 0.93, 0.92, 0.72, 0.7, root-mean-square error (RMSE) of 1.72 ℃, 2.19 ℃, 2.1 ℃, 2.1 ℃, 2.34 ℃ and Bias of 0.10 ℃, 0.71 ℃, 0.80 ℃, 1.14 ℃, 0.48℃ for soil temperature at 0 cm, 10 cm, 20 cm, 80 cm and 160 cm, respectively, and the results were better than the commonly used global land surface reanalysis dataset (ERA5-Land) and the latest land surface reanalysis dataset in China (CRA40-Land). In the new dataset, the average temperatures at 0cm,10cm,20cm,40cm80cm,160cm, 320cm in the multi-year permafrost zone of Sanjiangyuan are -0.02 ℃, 0.83 ℃, 0.83 ℃, 1.13 ℃, 1.24 ℃, 0.99 ℃ and 0.81 ℃, respectively, and 2.31 ℃, 2.85 ℃, 2.81 ℃, 2.90 ℃, 2.93 ℃, 2.80 ℃, and 2.70 ℃ in the seasonal permafrost zone.


Tue-01 Aug | 1:10 - 3:10 | MR336
HS04 - Characterizing and Modelling Ecohydrological Processes in a Changing Environment

Session Chair(s): Yuting YANG, Tsinghua University

HS04-A021 | Invited
Slower Changes in Vegetation Phenology than Precipitation Seasonality in the Dry Tropics

Jiaqi TIAN#+, Xiangzhong LUO
National University of Singapore

The dry tropics occupy forty percent of tropical land surface and play a dominant role in the trend and interannual variability of global carbon cycle. While several studies have reported considerable changes in dry tropical precipitation seasonality, the accompanied changes in vegetation growing season have not been examined. Here, we used long-term satellite observations with in-situ flux measurements to investigate phenological changes in the dry tropics over the past 40 years. We found that 54.4% of the area showed increases in the length of the growing season (LGS) and 45.6% showed decreases. The direction of LGS change depended jointly on precipitation seasonality and vegetation water use strategy, meanwhile the rate of LGS change was 23% slower than that of precipitation seasonality, likely caused by a buffering effect from soil moisture. Our study uncovers the potential mechanisms for dry tropical phenology changes, providing guidance to regional vegetation and carbon cycle studies.


HS04-A010
The Impact of Flood Regime on River Floodplain Vegetation Coverage: Insights from 30-year Landsat Record

Sheng HUANG1,2#+, Jiarui LEI2, Jun XIA1, Gangsheng WANG1
1Wuhan University, 2National University of Singapore

The impact of flood regimes on river floodplain vegetation within banks remains poorly understood. In this study, we examined the monthly variation of river floodplain vegetation coverage (RFVC) at a typical reach of the Yangtze River with a 30-year Landsat record. We evaluated its relationships with 13 hydrodynamic characteristic indices. Our results showed that flow regime alteration associated with dam construction could increase the downstream RFVC throughout the year. The maximum specific energy, reflecting both physical and physiological damage effects to riparian plants, was most related to the RFVC after floods (i.e., September-October) in the whole study period (Adj.R2 = 0.64, p < 0.05), and flood duration with water levels above floodplain vegetation had the most significant correlation with RFVC in the post-dam period (Adj.R2 = 0.84, p < 0.05). The change of riparian vegetation area in different elevation zones before and after floods mainly depended on the combined effect of vegetation distribution and flood intensity. Our findings further understand river floodplain vegetation dynamics and provide scientific support to riparian vegetation modelling.


HS04-A013
Multi-scale Ecological Operation Model of Reservoir Group Coupled with Ecological Infiltration Irrigation

Tao BAI#, Dong LIU+
Xi'an University of Technology

Aiming at the extensive management problems in ecological operation and ecological irrigation, this paper proposed a novel ecological irrigation method—ecological infiltration irrigation (EII), and established a multi-scale ecological operation model of reservoir group coupled with EII for the irrigation and restoration of river valley grasslands. Firstly, the ecological available water supplies in ecological periods were obtained by long-term ecological operation. Then, reservoirs on mainstream and tributaries gathered flood peaks through real-time ecological operation to create artificial ecological flood processes. Finally, by the joint operation of EII projects, the water level of artificial flood was raised, and the artificial flood was controllably introduced into irrigation districts for the precision irrigation of river valley grasslands. The rationality of ecological operation model and the feasibility of EII technology were then verified through case analysis. Results indicate that: (1) through the 5-9-13 division of ecological irrigation districts, analysis of the ecological water demand, multi-scale ecological operation, EII technology and projects, and other measures, suitable artificial floods can be created and fully introduced into ecological irrigation districts to realize the timely and appropriate irrigation of river valley grasslands; (2) in the critical ecological period in 2018, the core protected area was basically fully irrigated through EII, with an effective irrigation rate of 82.4% and a vegetation coverage of 74.8%, which basically met the ecological water demand of river valley forests and grasses; and (3) for animal husbandry, after using EII technology for grassland irrigation, the average forage yield of river valley grasslands has an increase of 25%, and the direct economic benefit has an average increase of 18.9 million yuan per year, effectively improving the economic income of local herdsmen. The research results have important theoretical and practical significance for the ecological protection and restoration of river valley vegetation.


HS04-A015
Temporal Variability in the Surface Energy Partitioning Over Vegetation Types

Kwanghun CHOI, Kyungrock PAIK#+
Korea University

The density and vigor of vegetation play important roles in the surface energy partitioning, i.e., how the incoming Solar radiation is distributed to three (ground, sensible, and latent) heat fluxes and the energy storage. We investigated the time series of all energy terms for several sites with distinct biome and climate, provided from Fluxnet, and discussed how vegetation status influences the energy variability of each site. We address the clear seasonality in the energy partitioning using monthly analysis. It is found that the sum of latent and sensible heat fluxes occupies a major fraction in the energy balance. Further the sum remains fairly steady regardless of vegetation types and seasons. Nevertheless, each of latent and sensible heat fluxes exhibits wide seasonal variability. It is argued that any increase or decrease in the latent heat flux is compensated by the decrease or increase in the sensible heat flux, making the sum fairly uniform.


HS04-A017
Analyzing the Water Budget and Responses to Land Use in a Small Catchment Use Using SWAT Model: A Case Study of Sha Lo Tung in Hong Kong

Xiao FENG+, Ji CHEN#
The University of Hong Kong

Sha Lo Tung was an ecologically rich valley consisting of abandoned agricultural lands, clear streams, and extensive wetlands with a small area of 56 ha. In the past 20 years, with the impacts of anthropogenic activities, the lands are drying out and the biodiversity of the place has been degrading. There is an urgent need to conserve and restore the ecosystem by bringing back the agricultural land use in this catchment. To evaluate the water balance and study the water abundance for agriculture, a hydrological model was set up using Soil and Water Assessment Tool (SWAT). Applying the SWAT model in small catchments is challenging as it is designed for large and complex basins. The performance of the SWAT model was evaluated using monthly streamflow with R2 = 0.93 and NSE = 0.92 in the calibration period (2002 – 2009) and R2 = 0.81 and NSE = 0.79 in the validation period (2010 – 2017). The key hydrological features were analyzed based on the model simulations and the hydrological impacts of the change in land use from forest to agriculture were characterized, which could benefit the sustainable water resource management and conservation plan of Sha Lo Tung catchment.


HS04-A006
Impact of Groundwater Extraction on Hydrological Process Over the Beijing-Tianjin-Hebei Region, China

Longhuan WANG+, Binghao JIA#, Zhenghui XIE
Chinese Academy of Sciences

Groundwater extraction influences water redistribution and hydrothermal processes, which significantly affect the water cycle and the sustainable development of the economy and environment. In this study, a high resolution (~1 km) land surface model that considered groundwater lateral flow and groundwater extraction was used to investigate the impacts of groundwater extraction on hydrological process. Simulations with and without groundwater extraction were conducted for the Beijing-Tianjin-Hebei (BTH) region for the period 2000−2012. The comparison of the simulated results and measurements from water wells, automatic weather stations, and satellite observations demonstrated the good performance of the model. Our results showed that groundwater extraction deepened the groundwater table depth by approximately 0.5−2 m across the plains and rapidly reduced terrestrial water storage (TWS; exceeding 24 cm per unit area) from 2000 to 2012. Both surface (2cm) and deep (100cm) soil moisture showed an increase of 0.01−0.02 m3 m-3 due to groundwater extraction used for irrigation. Groundwater extraction changed the water and energy budgets, leading to a significant cooling effect in the irrigated areas of BTH. The latent heat flux showed an increase of 30 W m-2 across the plains caused by the long-term exploitation. The surface soil moisture and latent heat flux increased mainly within the growing season due to farmland irrigation. The reduction in TWS was mainly due to the combined effects of over-exploitation and climate, while the contribution of extraction could not be ignored across the BTH region.


HS04-A008
Ecohydrological Response to Transient and Long-term Changes in Solar Radiation

Yiran WANG1#+, Naika MEILI2, Simone FATICHI1
1National University of Singapore, 2Singapore-ETH Centre

Geoengineering solutions aim to mitigate the adverse effects of global warming by modifying solar radiation, but the ecohydrological changes associated with these variations in solar radiation are often poorly known. Previous research mostly evaluated the long-term (slow) response of hydrological variables to solar radiation changes where it is difficult to untangle the sensitivity of hydrological variables to temperature changes from the sensitivity to radiation changes. In this study we aim to analyze the combined effects of short and long-term changes in solar radiation and hydroclimatic variables on the ecohydrological response of vegetation in multiple biomes. At a global scale, results from six CMIP6 climate models under five experimental conditions were utilized to calculate the instantaneous and long-term sensitivity of precipitation, surface temperature, specific humidity, and wind speed to top-of-atmosphere (TOA) and surface solar radiation changes. As expected, long-term changes lead to a higher sensitivity of precipitation, temperature and specific humidity to variations in solar radiation compared to short-term scenarios. The derived sensitivities of the hydro-climatic variables to solar radiation changes obtained from CMIP6 were used to force a mechanistic ecohydrological model in 118 sites characterized by different climates and vegetation types. Simulations results are used to quantify the ecohydrological response expected due to the changes of solar radiation and associated hydroclimatic variables as a result of geoengineering projects.


Tue-01 Aug | 3:30 - 5:15 | MR311
HS21 - Water-carbon Cycles in Agricultural Lands Under Changing Climate

Session Chair(s): Jun NIU, China Agricultural University

HS21-A005 | Invited
Remote Sensing-based Assessment of Crop Water Productivity in a Large Irrigation District

Songhao SHANG#+, Bing YU
Tsinghua University

Quantitative assessment of crop water productivity is crucial for agricultural water management in irrigation district. We proposed an approach to assess the regional crop water productivity using remote sensing-based models for regional evapotranspiration, crop identification, and yield estimation. A crop planting suitability index is further developed from the probability distribution of crop water productivity. This method was applied in Hetao Irrigation District (HID), the largest irrigation district in arid region of China. Spatial distributions of evapotranspiration, cropping pattern, crop yield, crop water productivity, and crop planting suitability from 2009 to 2015 were obtained. Results show that maize is more suitable to be planted in the western HID, while sunflower in middle and eastern HID.


HS21-A001
Irrigation Benefits of Maize Gross Primary Productivity in China

Dehai LIAO+, Jun NIU#
China Agricultural University

Irrigation is the most important water use sector accounting for about 70% of the global freshwater withdrawals and contributing 75% of China's total grain production. Application of irrigation water significantly alters agroecosystem water cycle, energy cycle and carbon cycle. In this study, we simulated irrigation benefits for maize gross primary productivity (GPP) using land surface models and satellite observations. The effects of climate interactions on the irrigation benefits were untangled using an explainable machine learning framework (XGB-SHAP). Reinforcing anthropogenic activities such as irrigation water management and planting structure adjustment are strongly required to improve crop resilience to climate variability.


HS21-A013
Assessment of Water Retention Variation and Risk Warning Under Climate Change in an Inner Headwater Basin in the 21st Century

Guangchuang ZHANG+, Yiping WU#, Huiwen LI
Xi'an Jiaotong University

Identifying the dynamics of water retention (WR) is critical for developing adaptive strategies for effective water resources management under climate change. However, our understanding about the responses of WR to climate change is still limited, which hinders risk assessment and warning of WR under future climate trajectories. In this study, we used the Soil and Water Assessment Tool (SWAT) to quantify the impact of climate change on WR in the upper Heihe River Basin (UHRB), a typical inner headwater basin, and predicted the future trends and potential degradation risks of WR based on climate scenarios under three Representative Concentration Pathways (RCP2.6, RCP4.5, and RCP8.5). Our results showed that the historical (1971-2020) average WR in the UHRB was approximately 91.1 mm, with high WR occurring in the middle and west of the basin and low WR in the north and southeast. Our prediction suggested that the WR may remain stable during the near future (near future, 2021-2060) under the RCP2.6 scenario; however, WR may decrease by 23% and 32% during this period under the RCP4.5 and RCP8.5, respectively. By the end of this century (far future, 2061-2099), the WR may decrease by 10%, 40%, and 69% under the RCP2.6, RCP4.5, and RCP8.5 scenarios, respectively, due to the substantially enhanced evapotranspiration in the warming context, though a slight increase in precipitation may partly offset this negative impact. In brief, this study provides a paradigm for assessing the dynamics and future degradation risk of water retention at watershed scale, and this can be valuable and applicable for other areas.


HS21-A008
Response of Evapotranspiration (ET) to Climate Change and Human Activities in the Shiyang River Basin, Northwestern China

Xueyi YANG#+, Fei TIAN
China Agricultural University

Evapotranspiration (ET) is an essential part of energy flow between the surface and the atmosphere, simultaneously involved in water, carbon, and energy cycles. ET is mainly determined by climate change, land use and land cover changes, and elevated atmospheric carbon dioxide concentrations. Climate change is expected to intensify the hydrological cycle and alter evapotranspiration. Land use affects ET within regional ecosystems mainly through vegetation changes, agricultural activities such as farmland reclamation, crop cultivation, and agricultural management. However, there still needs to be a quantitative characterization of the impacts of climate change and human activities on ET and regional water resources benefits. Based on Landsat-8 remote sensing images and combined with land use data, this paper inverted the planting structures of Liangzhou District in the middle reaches of the Shiyang River from 2019 to 2020 with a multi-band and multi-time combination method. On this basis, we quantitatively characterized the response of ET for wheat and corn in Liangzhou District to climate and human activity factors within two years. We clarified the impact of planting structure optimization on water resource benefits. Results showed that the multi-temporal Green and SWIR-1 band combination is the optimal band combination for extraction of planting structure. Compared with 2019, the wheat area decreased by 23.27%, and the corn increased by 5.96 % in 2020. ET in the two crops showed apparent heterogeneity: wheat's daily ET range was 0.4~7.2mm/d, and corn was 1.5~4.0mm/d. The spatiotemporal changes of ET have a more significant relationship with crop types and areas than climate change. Optimizing the agricultural planting structure is still an essential task for the sustainable development of water resources in the basin.


HS21-A004
Spatial Optimization of Cropping Pattern for Maximizing Crop Water Productivity, Economic Water Productivity and Nutrient Water Productivity

Jun NIU#+, Qi LIU
China Agricultural University

The optimization takes the maximum of crop water productivity (CWP), the maximum economic water productivity (EWP) and the maximum nutrient water productivity (NWP) as the objective function. The model optimizes the spatial distribution of six crops including corn, spring wheat, spring barley, spring canola-Polish, alfalfa and upland cotton. Results show that under the premise of considering food security, the maximization of water productivity for CWP, EWP, and NWP, leads to the reduction of corn planting area and the eastward shift of corn planting region.


Tue-01 Aug | 3:30 - 5:15 | MR336
HS04 - Characterizing and Modelling Ecohydrological Processes in a Changing Environment

Session Chair(s): Anna UKKOLA, UNSW Sydney

HS04-A025
Rainfall Induced Changes in the Soil Effluxes of Chir-Pine and Banj-Oak Dominated Ecosystems of Central Himalaya

Priyanka LOHANI1,2#+, Sandipan MUKHERJEE1, K. Chandra SEKAR1, Pooja MEHTA1, Sumit PUNDIR3
1Govind Ballabh Pant 'National Institute of Himalayan Environment', 2Graphic Era University, 3Graphic Era University, Dehradun

Soil efflux is one of the major contributors of CO2 to the atmosphere, and natural drying and rewetting of the soil through rainfall can significantly modulate the efflux amount of an ecosystem. Although the central Himalayan region is occupied with two dominant ecosystems, Chir-Pine (Pinus roxburghii) and Banj-Oak (Quercus leucotrichophora), differences in their soil efflux dynamics and responses of effluxes to varying rainfall are not examined in detail. Therefore, this study presents a comparative assessment of seasonal variation of the soil efflux of Chir-Pine and Banj-Oak dominated ecosystems. Efforts are made to quantify the changes in soil effluxes from these ecosystems due to varying rainfall spells. Data used in this study were collected from eosense carbon dioxide forced diffusion chamber (eosFD-CO2) sensors installed under a Chir-Pine dominated ecosystem (29°3'N, 79°3'E), at Kosi-Katarmal, Almora, India and a Banj-Oak dominated ecosystem (29o34'N, 79o3'E), at Shitlakhet, Almora, India for a total of 275 days of pre-monsoon (March-May), monsoon (June-September) and post-monsoon (October-November) seasons during 2021. The mean soil effluxes of Chir-Pine and Banj-Oak dominated ecosystems were found to be 4.57(±2.21) μmol.m-2.s-1 and 3.69(±1.92) μmol.m-2.s-1 during the period of observation, respectively. Moreover, both Chir-Pine and Banj-Oak dominated ecosystems have notably high soil effluxes (6.49±1.28 and 4.90±1.11 μmol.m-2.s-1) during monsoon season. Our initial observation further shows a systematic enhancement in the soil efflux of the Chir-Pine dominated ecosystem with successive rainy days of pre-monsoon season; however, no such increment was observed for Banj-Oak dominated ecosystem. The general inference of the study indicates that rainfall can be attributed as one of the major determinant factors for soil efflux variability in Chir-Pine dominated ecosystem.


HS04-A026
Bimodal Boreal Summer Soil Moisture: Satellite Observation and Analytical Land-vegetation-atmosphere Model

Abhinav DENGRI#+, Tomohito J. YAMADA
Hokkaido University

Soil moisture plays a critical role in the land-atmosphere coupling, particularly in transitional climate regions. This study employs satellite data and a simple coupled analytical land-vegetation-atmosphere model to detect global soil moisture bimodality hotspots during boreal summer and investigate the relationship between vegetation type and soil moisture bimodality. Soil moisture bimodality is characterized by two distinct peaks of wetness in long-term soil moisture distribution over one season. To detect bimodal distribution in the satellite dataset, a two-component Gaussian mixture model is first fitted, followed by the application of three bimodal statistical tests. The analytical model includes three vegetation landcover types: barren land, cropland, and forests, where croplands have dynamic Leaf Area Index (LAI), while barren land and forest land have fixed LAI. Additionally, evapotranspiration is partitioned into evaporation and transpiration. Satellite observations reveal that most bimodal regions occur over boreal summer land-atmosphere interaction hotspots, such as northern India, western Sahel, and the central great plains of northern America, where the primary land use is agriculture croplands. Similarly, the analytical model suggests that bimodality occurs over croplands, while it is absent in forests and barren land. Notably, forest vegetation maintains wet climate conditions, whereas barren lands maintain dry conditions, while croplands, depending on initial soil moisture wetness, may have dry or wet climates. Given the large-scale conversion of forests into cultivable land, the study examines its impact on boreal summer climate using a simple coupled land-atmosphere model.


HS04-A028
Simulating the Impacts of Numerous Reservoirs on Streamflow and its Extremes in the Yellow River Basin

Yang JIAO#+, Xing YUAN, Peng JI
Nanjing University of Information Science & Technology

Numerous reservoirs have been constructed over large basins in China, and have influenced both water and energy cycles by changing the underlying surface, altering local flow regimes, and redistributing regional water resources. The impact of reservoirs on direct streamflow regulations has received much attention, while actual water demand for irrigation is usually not considered from a water balance perspective, and the influence on streamflow and its extremes is not clear either. Here we focus on the Yellow River basin where numerous reservoirs have been built and irrigation is extremely important to agriculture. A reservoir operation scheme considering regional irrigation and other water requirements was developed and will be coupled to a land surface hydrological model with channel flow explicitly simulated and energy-water fully balanced. After model validation considering reservoir operations, hydrological extreme events will be identified with their frequency analyzed. By considering actual water demands, this study would facilitate the understanding of the impacts of reservoirs on streamflow and provide adaptation advice on reservoir operations during extremes.


HS04-A029
Biological and Hydraulic Controls on Soil Water Dynamics and Its Implication for Arizona Grassland Carbon Cycle Under Changing Hydroclimate

Yang SONG1#+, Tianyi HU1, Joel BIEDERMAN2, Xubin ZENG1
1The University of Arizona, 2U.S. Department of Agriculture

 The US Southwest dryland is experiencing fewer and more dense precipitation events. This changing hydroclimate drives physiological and phenological responses of dryland vegetation with unknown feedback to dryland soil water status and atmospheric CO2. It remains unclear what are the key mechanisms of Arizona grassland feedback to changing hydroclimate; and how this vegetation feedback to hydroclimate, together with unique dryland hydraulic properties, regulate soil water dynamics. Finally, how does coupled vegetation-soils-hydroclimate feedback contribute to Arizona grassland's carbon budget? To address these questions, we integrated the observations from a rainfall manipulation experiment site in the Santa Rita Experimental Range of Southeast Arizona, US, into the Community Land Model (CLM5). Vegetative observations under different precipitation operations were incorporated into the CLM5 to parameterize distinct phenological, root dynamics, and carbon allocation feedbacks of annual and perennial grasses in response to changing hydroclimate. Observed soil water content (SWC) and soil water potential (SWP) were assimilated into CLM5.0 using the data assimilation research testbed (DART) to improve the parameterization of soil hydraulic effect on soil moisture dynamics. Our results indicated that the soil water status of Arizona grassland is mainly regulated by soil hydraulic processes. In contrast, vegetation composition and their distinct feedback to changing hydroclimate affect the seasonal fluctuation of soil water. Less frequent and more dense precipitation alters vegetation community composition. Parameterizing specific drought tolerance, carbon allocation, and root dynamics of annual grass and perennial grass better captured the seasonal fluctuation of evapotranspiration and GPP with precipitation events. Assimilating observed SWC and SWP better captured distinct magnitudes of carbon and water fluxes under different precipitation frequencies and intensities. Our findings highlighted that the feedback of the dryland carbon cycle to changing hydroclimate depends on soil hydraulic regulation on the water cycle and the resultant impact on vegetation dynamics.


Wed-02 Aug | 10:20 - 12:20 | MR311
HS14 - Water-related Hazards and Their Forecasting and Warning

Session Chair(s): Gwo-Fong LIN, National Taiwan University, Jui-Yi HO, National Science and Technology Center for Disaster Reduction

HS14-A007
The Application of FORMOSAT-7/COSMIC-2 Radio Occultation Observation in Hazardous Weather

Yu-Chun CHEN#+, Chih-Chien TSAI, Yi-Chao WU, An-Hsiang WANG, Chieh-Ju WANG, Hsin-Hung LIN, Yi-Chiang YU
National Science and Technology Center for Disaster Reduction

The monitoring of monsoon moisture and the prediction of severe weather play a crucial role in disaster prevention and water resource management. The Global Navigation Satellite System (GNSS) radio occultation (RO) technique provides global coverage of temperature and moisture vertical profiles, which are not affected by weather conditions or land-sea distributions. This study utilizes COSMIC-2/FORMOSAT-7 RO observations to establish a monsoon moisture indicator and to enhance numerical weather forecasts through data assimilation techniques. The quality of the RO observations is validated by comparing the in situ radiosonde profiles in the vicinity of Taiwan with the collocated RO profiles. The proposed moisture indicator effectively captures the daily variations of the monsoon moisture source from the South China Sea. The results of this study indicate that incorporating RO observations into severe weather predictions in Taiwan has a neutral to positive impact on precipitation forecasts during the monsoon period. Furthermore, the assimilated RO observations also demonstrate a reduction in the forecast error of typhoon tracks, which is a significant advantage in typhoon prediction.


HS14-A016
Pre-processing of Rainfall Forecasts to Improve the Predictive Skill of the Real-time Flood Forecasting System for the Chao Phraya River Basin

Theerpol CHAROENSUK1,2#+, Jakob LUCHNER3, Nicola BALBARINI3, Piyamarn SISOMPHON4, Peter BAUER-GOTTWEIN 1
1Technical University of Denmark, 2Hydro Informatics Institute, 3DHI A/S, 4Ministry of Higher Education, Science, Research and Innovation

Currently, the effects of climate change are becoming more pronounced. To monitor and forecast floods, many nations and agencies have developed decision support (DSS) and flood forecasting systems. The Chao Phraya River basin, in particular, Thailand’s most important river basin, is subject to frequent flooding because of the combined effects of precipitation, river floods and ocean storm surges. Thailand has established the operational Chao Phraya's flood forecasting model and DSS developed by Hydro-Informatics Institute (HII) in collaboration with DHI A/S for monitoring, warning, and assisting the Thai government in decision-making. The flood forecasting system consists of 3 components: 1) A numerical weather model (WRF-ROMS) coupling an atmospheric model, the Weather Research and Forecast (WRF) model with the Regional Oceanic Model System (ROMS) developed by HII 2) A hydrological model simulating runoff using real-time rainfall from situ stations and rainfall forecasts from WRF-ROMS 3) A 1D/2D hydrodynamic model that is forced with runoff produced by the rainfall-runoff model and includes real-time structure operation to simulate water level, discharge, and flood inundation. The quality of rainfall predictions, which have a tendency to underestimate rainfall peaks but overestimate total rainfall, most significantly limits system performance. For this reason, we explored pre-processing techniques applied to the rainfall forecast before ingestion into rainfall-runoff model. In this study, quantile mapping bias correction and random forest regression are used as pre-processing techniques to improve the accuracy of rainfall prediction. Forecast skill was assessed at key stations using RMSE and CSI, evaluated using re-forecasting experiments over a 6-year historical period with and without pre-processing techniques. The evaluation of flood forecast performance using pre-processing techniques shows a significant improvement in prediction skill compared the baseline scenario. Our study demonstrates that the pre-processing techniques can improve the accuracy of rainfall prediction and the skill of the operational system.


HS14-A023
Near Real Time (NRT) Flood Forecasting Model on 10 Sub-basins in the Greater Chao Phraya River Basin, Thailand

Pongsit POLSOMBOON1#+, Anurak SRIARIYAWAT2, Piyatida RUANGRASSAMEE2
1Faculty of Engineering, Chulalongkorn University, 2Chulalongkorn University

Flood is a major natural disaster that causes severe problems and extensive damage to socio-economic and ecological systems. The flood inundation estimation is crucial for early warning, flood mitigation and adaptation measures to manage risk and mitigate damage from flood. The study aims to develop the Near Real Time (NRT) flood forecasting model using Rainfall-Runoff-Inundation (RRI) model for the Greater Chao Phraya River Basin, Thailand, and the forecasted rainfall data from the Thai Meteorological Department (TMD). The Greater Chao Phraya River Basin has a total area of 158,500 km2 and consists of eight sub basins including Ping, Wang, Yom, Nan, Sakae Krang, Pasak, Tha Chin, and Lower Chao Phraya River Basins. For the calibration of the RRI model, the Greater Chao Phraya River Basin was delineated into 10 sub-basins to address diverse topography and land use. The performance of the RRI model was evaluated using the observed daily discharge from the Royal Irrigation Department (RID) and the inundated area from satellite images from The Geo-Informatics and Space Technology Development Agency (GISTDA) during flood events. The calibrated RRI model and the 10-day forecasted rainfall from TMD was used to simulate flood forecasting during typhoon Noru in September 2022 and its performance was evaluated to quantify uncertainty for an early warning system.


HS14-A014
Prediction of River Level by Neural Network Model and Ensemble Learning Model

Siyan LIU+, Yu LI#
Nankai University

Flood prediction can give early warning to the rapid rise of water level and the arrival time of flood, which has important research value to protect people's life and property safety. Affected by many factors such as rainfall, temperature, evaporation and historical water level, the rainfall-river level model is a complex, nonlinear and multi-dimensional dynamic process. The discover of internal correlations and relationships between above factors may help in the predication of water level. In this study, the long-term (12 years) data of 4 gauges in the Katsuragawa river basin in Japan were obtained, including the historical water level data and the rainfall data. Long and short term neural networks (LSTM) and two ensemble learning algorithm (XGboost and LightGBM) were established to predict the water level of Katsura gauge. Moreover, Statistical indicators, such as R2, MAE, MSE, RMSE, were used to evaluate performance of these models. All three models can effectively predict the hourly water level in the next 72 hours. Compared with Xgboost and LightGBM, LSTM model has the highest goodness of fit (R2=0.985), which provides an effective guarantee for the precise control of flood control and storage.


HS14-A009
Challenges in Monitoring and Forecasting Flood Hazards in Developing Countries

Mohamed RASMY1,2#+, Tomoki USHIYAMA1,2, Katsunori TAMAKAWA1, Kentaro AIDA1, Keijiro KUBOTA1, Toshio KOIKE1
1Public Works Research Institute, 2National Graduate Institute for Policy Studies

Floods due to unprecedented extreme rainfall events have caused devastating damage worldwide, particularly in developing countries. Severe flood damage can be attributed to slow progress in implementing flood monitoring, forecasting and early warning and other countermeasures in developing regions mainly due to the unavailability of reliable and timely observations, thus hindering their commitments to achieve the Sustainable Development Goals (SDGs) by 2030. However, recent advancements in satellite rainfall observation, ensemble rainfall forecasting, and flood simulation modelling can significantly help to improve these unfavourable circumstances and enhance flood monitoring, early warning, and disaster mitigation activities in these regions. This research investigated the performance of real-time and near-real-time satellite precipitation products (SPPs) and quantitative ensemble rainfall forecasts for recent extreme floods in two river basins (i.e., the 2017 and 2018 floods in the Kalu River basin of Sri Lanka and the 2018 flood in the Periyar River basin of India). In general, SPPs underestimated the rainfall amount and showed significant errors in the locations of heavy rainfall that may have arisen when microwave data were interpolated for unobserved regions using geostationary satellite cloud top temperature data. The rainfall products, which were bias-corrected using limited ground gauges improved the simulations of peak river discharges and inundation extents. The ensemble rainfall forecasts in both basins produced a good performance in forecasting flood alarming signals with uncertainties in the peak amounts. The storm location shifts and/or poor rainfall forecasting skills over non-mountainous regions were found to be the reasons for the low performance of the ensemble streamflow forecasts.


HS14-A020
The Behavior of Landslide-induced Sediment Pulse Evolution in Channel Network: Theory and Simulation

Cheng WEI#+
DPRI, Kyoto University

In previous studies, researchers endeavored to investigate reach-scale sediment wave dynamics. However, few studies emphasized a comprehensive investigation of tributary interaction between the evolution of sediment pulses and the response of the fluvial system. This study aims to develop a 1D model to describe the sediment pulse evolution in the form of a dispersion-advection equation to capture the physical wave motion of sediment pulses in a single channel and the channel network structure. For the model establishment, the St. Venant equations, the Exner equation, and the Meyer–Peter–Mueller (MPM) bed load equation are utilized to simulate the water flow condition, the changes in river bed elevation, and sediment pulse evolution. Meanwhile, the Peclet number is adopted as an effective indicator to quantify the extent of wave translation and dispersion on sediment pulse evolution. The simulation results reveal that the translation direction of sediment pulses would depend on positive or negative values of the Froude number. The translation impacts dominated the evolution process when flow velocity increased under the same discharge, while the sediment pulse tended to disperse in place when flow discharge increased and under lower flow velocity. In the channel network, there would be an extra increase of sediment supply in confluence, and sediment pulses would also move in a combination of translation and dispersion at the same time with the decay of the apex gradually translating downstream to the estuary. Finally, the model is applied to simulate the landslide-induced sediment pulses in Nanshih and Hsintien catchments, Taiwan, after Typhoon Soudelor in 2015, which was a significant natural disaster with many landslides left in the catchments. The evolution process of the landslide-induced sediment pulses is described as wave motion translating downstream to the estuary.


HS14-A021
Investigation of Downstream Geomorphology and Biological Environment Influenced by the Sediment Bypass Tunnel Operation of the Koshibu Dam

Yixuan LIU#+, Tetsuya SUMI, Yasuhiro TAKEMON, Sameh KANTOUSH
Kyoto University

Dams built artificially can disrupt the natural flow and obstruct ongoing sediment transport. Changes in riverbed morphology and ecosystems downstream may result as a result of this. While economic activity, the hydropower sector, and the worldwide population continue to rise rapidly, global reservoir storage capacity is decreasing year after year. The sediment siltation issue in reservoirs is the main cause of the decrease in reservoir storage capacity. Therefore, sustainable management of reservoirs and water resource infrastructure is necessary to ensure the expected usable life of the reservoirs. Sediment bypass tunnels (SBTs) are one of the sediment management techniques that move sediment downstream of the reservoir, preventing reservoir siltation. In the meantime, SBTs can support the reconnection of upstream and downstream sediments. The sediment will change riverbed morphology, with previously degraded reaches re-trending toward deposition, which can help with downstream ecological restoration. However, it is unclear what morphological changes are brought about downstream by the release of sediment through SBTs. Moreover, the downstream dynamics are complicated by the sediment-laden water being imported. Different sediment grain sizes may have different effects on changes in downstream morphology. Reach-scale channel configuration (RSCC), a riverbed geomorphology feature, can be used to connect hydraulic disturbance and ecological function. Because changes in RSCC may be predicted using knowledge of hydraulic and geomorphic conditions, it could be utilised to combine ecology and hydraulics through geomorphology. This study aims to investigate the interrelationships between RSCC, habitat structure and biodiversity downstream of the Koshibu River under the influence of SBT operations. Through this approach, trends in downstream surface morphology and sediment movement patterns can be analysed. Thereby determining how the application of SBTs can best contribute to downstream ecological restoration.


HS14-A001
Modeling Storm Surge and Wave Induced Sea Dike Breaking and Overflow

Wei-Che HUANG#+, Wen-Cheng LIU
National United University

Due to the limitation of land area and topography, Taiwan's population is mainly concentrated along the rivers or coastal areas, and typhoons often hit Taiwan every summer. In this study, a breaking mechanism of concrete sea dike is established and combined with tide-surge-wave model to simulate the storm surge and wave height caused by typhoons along the coast of Taiwan, calculate the impact force, uplift height, and wave-induced overtopping flow, and then evaluate whether the sea dike is damaged by the breaking mechanism; if the dike is damaged, the breaking overflow can be calculated according to storm surge height, current, and breaking width. Four historical typhoon events were used to validate the tide-surge-wave model. The results showed that the root-mean-square error (RMSE) of the simulated and measured wave heights ranged from 0.43 m to 2.43 m, and the skill score (SS) ranged from 0.53 to 0.96. The RMSE of the simulated and measured water levels ranged from 0.08 m to 0.42 m and the SS ranged from 0.90 to 0.99. Then, the validated model was utilized to simulate the possible damage to the sea dike for different surge and wave heights generated by different typhoon intensities, exploring the limits of sea dike damage and the breaking overflow.


Wed-02 Aug | 10:20 - 12:20 | MR330
HS16 - Applying Novel Technologies to Assess the Impacts of Flood-induced Disasters Over the Watershed

Session Chair(s): Dong-Sin SHIH, National Yang Ming Chiao Tung University, Jian-Ping SUEN, National Cheng Kung University

HS16-A004
An Investigation on Spatiotemporal Characteristics of River Sediment Using Time Series InSAR

Shih-Yuan LIN1#+, Shih-Teng CHANG1, Ching-Fang LEE2
1National Chengchi University, 2Sinotech Engineering Consultants Inc.

For the purpose of investigating spatiotemporal characteristics of river sediment behavior, we applied the PS-InSAR technique capable of estimating time series displacement over wide area to estimate the surface deformation along the target section in Daan River in Taiwan. In order to reduce the effect of unfavorable atmospheric condition and wide water coverage in the river way in wet seasons, only the Sentinel-1 SAR images taken in dry seasons were input in the PS-InSAR processing. In the monitoring period from 2017/11 to 2021/04, even though the image number introduced to PS-InSAR was half reduced, the deformation difference was estimated with the accuracy up to 2.8 mm compared against GPS observation data. In addition, the long-term deformation trend derived from GPS and PS-InSAR also agreed with each other. Since the PS-InSAR results was proved reliable, we took the advantage of its long-term and wide-extent observation to investigate the sediment behavior over sequential wet/dry seasons and relatively long hydrological seasons. As a result, the season when the most serious erosion occurred was identified and the corresponding erosion volume was estimated. Moreover, through the deformation maps, the regions prone to suffer from erosion was also identified. As the strategy for understanding river sediment behavior was proved feasible, we were able to perform detailed spatial- and temporal-wise investigation along the river way.


HS16-A008
Sediment Estimation Using Machine Learning Approaches in Wu River, Taiwan

Chia-Hsuan CHUNG, Yu-Cheng CHEN, Chun-Ju CHENG, Yuan-Fong SU#+
National Taiwan Ocean University

Sediment transportation is a highly nonlinear process and which is very difficult to model with a simple and linear regression method. To address on this, we aimed at exploring the relationship between suspended sediment and hydrologic and topographic characteristics of Wu River in Taiwan. In Wu River catchment, we collected discharge, water depth, flow velocity, cross-section area, river width, sediment concentration at 6 gauges from 2014 to 2019. With this dataset, we compared the performance of simple regression and machine learning approaches such as support vector machine and random forests in terms of root mean square error and mean absolute percentage error. The results revealed that machine learning approaches are better than traditional regression model.


HS16-A005
Estimation of Pier Scours by Incorporating Hydraulic Parameters and Triaxial Accelerometer

Hsuan-Yu PENG#+, Dong-Sin SHIH
National Yang Ming Chiao Tung University

Due to the effects of climate change in recent years, river flow has often surged in Taiwan during the rainy season. To prevent scour damage to piers caused by floods, estimating scour depth of bridge piers is crucial for disaster early warning. However, only using the physical hydraulic parameters to estimate pier scour tended to miscalculate because the field flow situation is highly complicated. The vibration monitoring technology that has emerged in recent years provides a new direction for estimating the scouring depth of bridge piers. This study tried incorporating the hydraulic information and vibration signal into a formula for estimating bridge scour. We used dimensionless analysis to derive a formula and designed a series of laboratory experiments to determine the coefficients of the proposed formula. A tri-axial accelerometer is provided to measure the vibration of the bridge stand and uses the fast Fourier transform to convert the signal from amplitude to the frequency domain. Theoretically, the scouring of the riverbed leads to a decrease in the loading capacity of the pier foundation and structural stiffness. As a result, the vibration response of the overall structure tends to be changed. This study explores pier models of different stiffness and applies various confinement forces on top of the piers. The relationship between the vibration frequency and the flowing current is studied. This study tries to provide a way to estimate the scour depth of bridge piers and bridge early warning benchmarks.


HS16-A002
River Stage Forecasting Based on the Coupling of Support Vector Regression and Runge–Kutta Schemes

Jiun-Huei JANG#, Kun-Fang LEE, Hsuan Yeh SHIH+
National Cheng Kung University

For river stage prediction, numerical models are highly accurate but take much time for building and calculating; in contrast, machine learning models require less computation time but lack physical theorems. To combine the advantages of the two methods, we proposed a hybrid model based on the coupling of support vector regression (SVR) machine learning method and Runge Kutta (RK) numerical method in this study. A total of 13 typhoon events from 2015 to 2019 in Tamsui River, Taiwan, were adopted for model training and validation. In comparison with the original SVR (without coupling with RK method), the hybrid model increased the accuracy in river stage forecast with average root mean square error (RMSE) and error of peak stage (EPS) decreased at most by 19 % and 93 %, respectively. Meanwhile, the hybrid model had higher accuracy and lower fluctuation as the lead time increased. In application, the hybrid model is more efficient than individual models because it takes less training time than the original SVR and less computation time than the numerical model.


HS16-A009
Evaluating the Effectiveness of a Convolutional Autoencoder for Bias-corrected Satellite Precipitation Product in Hydrological Modeling

Oudom Satia HUONG#+, Xuan-Hien LE, Van Giang NGUYEN, Giha LEE
Kyungpook National University

Precipitation plays a critical role in the hydrological cycle, but it can also lead to natural disasters, such as floods. Although satellite-based precipitation products (SPPs) have been used to estimate precipitation with spatiotemporal variability, it suffers from lots of uncertainties and coarse spatial resolution. In order to overcome this challenge and obtain more accurate precipitation estimates, this study employed a convolutional neural network (CNN) - based model to generate pixel-by-pixel bias-corrected daily precipitation product. In this study, two gridded precipitation products, APHRODITE and PERSIANN-CDR, with spatial resolutions of 0.25° were used as observed- and satellite-based datasets, respectively. These precipitation datasets (satellite-based and corrected-based) are then utilized as the input for Rainfall-Runoff-Inundation (RRI) model to simulate river discharge, flood depth, and flood extent for Cambodia's Prek Thnot River Basin (PTRB). The results of this study demonstrated the effectiveness of the CNN-based model in correcting bias in precipitation estimates. The bias-corrected dataset has shown superiority to the original SPP in both spatial and temporal correlations. Besides, the simulation results of the rainfall-runoff process for the PTRB using the above data also showed the same trend. The corrected precipitation product has improved the accuracy of the RRI model in inundation simulation as well as providing river discharge information. The findings of this study suggest that the CNN-based model could be a promising tool for correcting the bias of SPPs in hydrological modeling, providing significant implications for flood risk management and disaster preparedness in the region.


HS16-A001
Flood Depth Estimation for Urban Area Using Google Earth Engine and Digital Elevation Based Hydroprocessing Models

Lifan CHEN#+, Tsun Hua YANG
National Yang Ming Chiao Tung University

Extreme rainfall weather can cause flooding. As the level of damage is usually proportional to the inundation extents and depth of flooding. For most of the time, ground observations are limited and in consequence the size, or magnitude of flood events is hardly estimated. Images collected by satellites orbiting the planet can be used to extract the extent from floods. Among the various available satellites and sensors, Synthetic Aperture Radar (SAR) is distinguished in the context of flood management by its ability to penetrate cloud cover and its robust images during night-time. However, satellite images can only provide two-dimensional information such as the extent of flooding. The third-dimensional information which is flood depth cannot be directly obtained from the images. Only a very few studies have studied this issue and none of them focuses on urban area. This study proposed a rapid approach integrating Google Earth Engine (GEE), an open-source software FwDET_GEE, and a flood inundation model SPM_GEE to produce detailed flood risk maps with extent and depth. SPM_GEE model is a customized model which is based on digital elevation model and developed by this study. At first, the approach is to use the images from Sentinel-2 satellite from GEE to extract the flood extent, and then to apply FwDET_GEE tool to roughly estimate flood depths along flood extent boundaries. These flood depths are then used as inputs to SPM_GEE model to produce detailed flood depths for urban area. The study used a historical flood event in Chiayi County, Taiwan to evaluate the approach and the results show that the root mean square error in comparison with observation data is 0.25 m. This proposed approach has demonstrated its potential to provide detailed floodwater depths for urban area while satellite images are available.


HS16-A012
Hydrodynamic Features of Undular Flow Induced by a Submerged Channel-span Cylinder

WuRong SHIH#+, Yi-Ze ZHANG
National Chung Hsing University

Undular flow is characterized by a wavy free-surface, or termed undulation of flow, appearing immediately downstream of a weak hydraulic jump. Such post-jump undulation is ubiquitous in natural rough-bed rivers, particularly in those mountain streams where hydraulic jump is easy to develop over cobbles and boulders. Despites its prevalence, undular flow has drawn less attention from the scientists mainly because this phenomenon is not as intense and apparent as is hydraulic jump itself. However, most recent studies have shown that undular flow can play an important role in determining near-bed flow properties, including seepage effects and hyporheic exchange. A better understanding of undular flow, therefore, provides implications for the improvements on river management and pollutant control as these efforts are affected by the surface-subsurface exchange. Having that purpose in mind, in this study we used a channel-span circular cylinder to create weak hydraulic jump in a laboratory flume for examining the post-jump undulation. To ensure an optimal observation, upstream flow conditions were set at a lower range of supercritical flow, having a Froude number of 1.2 to 1.5, to attain a clear undulation after jump. Observation of flow field was made through a non-intrusive, laser-based particle tracking velocimetry (PTV) system. The sampling rate of velocity measurement was up to 500 Hz, sufficiently high for fully resolving pertinent turbulent properties, such as turbulence intensity, transport of turbulence kinetic energy, instantaneous velocity quadrant sequences, hydrodynamic pressure distribution, and vortex identification. These analyses were applied to a variety of undulation scenarios controlled by the relative submergence of the cylinder used. The results helped us to examine important properties of undular flow and identify the driving mechanism of flow undulation.


HS16-A013
Innovative Use of Unmanned Surface Vehicle Technology for Muskingum Flood Routing Parameter Derivation

Yeo LIM#+
University of North Dakota

Flood modeling and forecasting are essential in managing water resources and reducing the loss of life and property damage caused by floods. One important aspect of flood modeling is the use of flood routing methods, such as the Muskingum Routing method, to route flood water through river reaches and predict the flood levels of downstream reaches during a flood event. The critical aspect of using the Muskingum Routing method is the characterization of the parameters K and x. Accurate discharge measurements to define observed hydrographs at two locations are required to calibrate the routing parameters. However, collecting such data can be difficult and time-consuming, leading to modelers making assumptions about the parameters. The objective of this study was to derive Muskingum flood routing parameters for one site during a major flood period using an autonomous surface vehicle (USV) equipped with acoustic Doppler current profilers (ADCP) technology. In the process, we have developed an innovative method for deriving Muskingum parameters. The method involves selecting a river reach with an existing streamflow measurement site, selecting a study section upstream or downstream of the site, and deploying UAS with ADCP to measure discharge during the rising flood level and continue until sufficient points are collected on the receding flood to allow a well-defined flood hydrograph. The calibration of Muskingum routing for K and x is then performed, followed by a plausibility check. The method has proven to be efficient and safe to use, allowing for deriving accurate hydrographs for major flood events that could take years to collect using traditional methods. The use of USV with ADCP technology is a game changer for flood modeling and water resource management, providing accurate routing parameters in flood modeling, forecasting, and response efforts, resulting in significant benefits.


Wed-02 Aug | 10:20 - 12:20 | MR336
HS15 - Satellite Remote Sensing for Water and Carbon Cycle Studies

Session Chair(s): Chang-Hwan PARK, Ajou University, Xiwu ZHAN, National Oceanic and Atmospheric Administration

HS15-A002
Nasa Soil Moisture Active Passive Mission Status, Products and Applications

Simon YUEH1#+, Dara ENTEKHABI2, Rajat BINDLISH3, Jared ENTIN4
1Jet Propulsion Laboratory, California Institute of Technology, 2Massachusetts Institute of Technology, 3NASA Goddard Space Flight Center, 4National Aeronautics and Space Administration

The NASA Soil Moisture Active Passive (SMAP) Mission was launched in January 2015, and its L-band radiometer has been operational since April 2015. The key science requirements of the SMAP mission are to provide accurate soil moisture for hydrology and carbon cycle studies. The radiometer calibration has been very stable with less than 0.2 K rms variation over eight years. The quality of baseline soil moisture products based on the Dual Channel Algorithm (DCA) has reached 0.036 m3/m3 unbiased RMSE and better than 0.8 correlation in comparison with the in-situ data from Cal/Val sites. The DCA algorithm can also produce the Vegetation Optical Depth (VOD). There is clear linearity between SMAP VOD and tree height spatially for values of tree height less than 20 m and the relationship remains fairly linear up to tree heights of ~ 35 m with a strong correlation of 0.81. Validation studies in the US corn belt have also found significant correlation of the SMAP VOD with the crop water content. Since 2020, the SMAP soil moisture on a polar EASE-2 grid has been developed to achieve more uniform zonal and meridional sampling in the polar regions. We have also updated the water mask derived from NASA Terra MODIS Land Water Mask version 6 (2015-2019) record. The benefit is greater in the Northern Hemisphere high latitudes where the updated water mask is more effective in resolving the abundance of smaller water bodies in boreal and tundra wetlands, and many anomalous soil moisture retrievals (overly wet) near the coastlines have been eliminated. SMAP’s data has been found useful for many scientific applications, including depictions of water and carbon cycles, improvement to parameterization of hydrologic processes over land surfaces, flood forecasting, and ocean surface salinity mapping. Highlights of the future plan will be provided.


HS15-A015
Improving Soil Moisture Retrieval by Synergistic Update of Vegetation Index and Surface Roughness

Jianxiu QIU#+
Sun Yat-sen University

Satellite-based soil moisture (SM) retrieval within agricultural regions is challenging due to pronounced vegetation and land cover variations during the growing season. Vegetation water content (VWC)–used to describe vegetation opacity in both the Soil Moisture Active Passive (SMAP) Dual Channel Algorithm (DCA) and V-polarization Single Channel Algorithm (SCA-V)–is approximated using a climatological Normalized Difference Vegetation Index (NDVI) time series. To understand the impact of VWC algorithms on SMAP SM retrievals, we investigated optimal vegetation indices for VWC estimation, and further evaluated the impact of VWC uncertainty on DCA and SCA-V SM retrievals. Besides NDVI from Moderate Resolution Imaging Spectroradiometer (MODIS), we applied dynamic vegetation indices (VIs) acquired from Visible Infrared Imaging Radiometer Suite (VIIRS) to estimate growing-season VWC and the impact of different empirical relationships on VWC estimates. We find that climatological NDVI from MODIS significantly underestimates VWC, and therefore underestimates SM over croplands during the growing season, whereas dynamic VIs can improve the accuracy of VWC and SM retrievals. In addition, the influence of VWC uncertainty on SM accuracy is shown to be higher in SCA-V than in DCA. The results of this study provide insight into preferred approaches for the accurate estimation of VWC and associated improvement in passive microwave algorithms for SM retrieval.


HS15-A001
Soil Mositure Estimation from SMAP Brightness Temperature with Variational Scattering Albedo in Dense Vegetation

Chang-Hwan PARK1#+, Andreas COLLIANDER2, Thomas JAGDHUBER3, Aaron BERG4, Michael COSH5
1Ajou University, 2Jet Propulsion Laboratory, California Institute of Technology, 3German Aerospace Center, 4University of Guelph, 5United States Department of Agriculture

Calculating soil moisture from microwave brightness temperature is a big challenge in areas with dense vegetation. The soil moisture retrieved by SMAP is usually overestimated and can even exceed the saturation of mineral soils. This means that current remote sensing of soil moisture cannot detect or track climate extremes such as floods and droughts in these areas which are important for forest and natural resources management and climate change research. In this study, it is assumed that the primary cause of the overestimation is the scattering coefficient (ω) which is taken as a fixed value in conventional microwave radiative transfer models (RTMs). To solve the issue of overestimation, a unified (𝜏-ω) radiative transfer model is presented which adjusts w based on the measured vegetation optical depth VOD (or 𝜏). When retrieving soil moisture using operational RTM, increasing the Volume of Depolarized Light (VOD) with fixed omega (ω) produces unrealistic high Brightness Temperature (Tb). Introducing the change in omega in the Tb simulated by the unified RTM has helped to minimize this issue. It is found that the physical connection between tau and omega in RTM is a major factor in reducing the bias in soil moisture estimation in forested areas.


HS15-A004
Long-term Evaluation of the AMSR2 L2 Soil Moisture Product of JAXA on the Mongolian Plateau for Ten Years from 2012 to 2021

Ichirow KAIHOTSU1#+, Jun ASANUMA2, Kentaro AIDA3, Dambaravjaa OYUNBAATAR4, Nozomu HIROSE5
1Hiroshima University, 2The University of Tsukuba, 3Public Works Research Institute, 4Institute of Meteorology, Hydrology and Environment, 5National Institute of Technology, Matsue College

This study evaluated the Advanced Microwave Scanning Radiometer 2 (AMSR2) L2 soil moisture product (ver. 3.0) of the Japan Aerospace Exploration Agency (JAXA) using in situ hydrological observational data for ten years from 2009 to 2021 in a 50 × 50 km flat study area of the Mongolian Plateau covered with pasture and shrubs. Although AMSR2 slightly underestimated soil moisture content at 3-cm depth, satisfactory timing was observed in both the response patterns and the in situ soil moisture data, and the differences between these factors were not large. In terms of the relationship between AMSR2 soil moisture from descending orbits and in situ measured soil moisture at 3-cm depth, the values of the RMSE (m3/m3) and the bias (m3/m3) varied from 0.025 to 0.063 and from 0.011 to − 0.051 m3/m3, respectively. The values of the RMSE and the bias depended on rainfall condition. Comparison of the Soil Moisture and Ocean Salinity (SMOS) soil moisture product (V700) with the AMSR2 L2 soil moisture product showed that AMSR2 could observe surface soil moisture with nearly same accuracy and stability. However, the bias of the AMSR2 soil moisture measurement was worse than that of SMOS which measured deeper soil moisture. It implicates that AMSR2 cannot effectively measure soil moisture at 3-cm depth. In situ soil temperature and vegetation did not affect the underestimation of AMSR2 soil moisture measurements. These results suggest that underestimation of AMSR2 soil moisture measurements is possibly caused by the difference between the depth of the AMSR2 observations and in situ soil moisture measurements. Overall, the AMSR2 L2 soil moisture product has been useful for monitoring daily surface soil moisture over large grassland areas and the high-performance capability of AMSR2 since 2012 was clearly proved in this study.


HS15-A012
Evaluating Drydown Patterns from SMAP L3 Using a Bivariate Recursive Filter

Jhilam SINHA#+, Ashish SHARMA, Lucy MARSHALL
UNSW Sydney

Appropriate representation of soil drying characteristics in satellite soil moisture (SM) retrievals is crucial for conducting environmental studies. Following the advent of remote sensing technology, satellite derived SM products have provided a viable alternative to ground measurements of SM that are sparse at spatio-temporal scale, for conducting investigations at a larger spatial scale. Soil Moisture Active Passive (SMAP) mission is one of the prominent L-band missions, which is intensively used in environmental research. However, previous studies have highlighted systematic deviation of drying rates of SMAP L3 product compared to in-situ stations and surface model estimates. SMAP L3 SM, during drying phases, generally dry faster. This can be attributed to differing measurement depths of soil wetness and spatial scale mismatches. Here, a recursive filtering approach is introduced that attempts to modify drying rates of SMAP drydowns to be comparable to in-situ drydowns. The idea is to preserve the drying characteristics, as they define partitioning of precipitation and energy, thus, acting as hydrological signatures. The approach maintains the interdependence structure of initial wetness condition and drying coefficient for SMAP drydown events to be in consistent to in-situ. The study is conducted over the United States region that has dense and well distributed ground SM networks. Considerable improvement is achieved in correcting the drying rates of SMAP drydown events. The performance is found to be acceptable across spatial heterogeneity, assessed by sand and clay fraction and dryness index. Incorporating modified satellite derived drying characteristics to hydrological models has the potential to derive more accurate runoff estimations.


HS15-A014
Reprocessing Satellite Data Products of Soil Moisture and Evapotranspiration Using Machine Learning Approaches for NOAA Weather and Climate Prediction and Societal Applications

Xiwu ZHAN1#+, Jifu YIN1, Li FANG1, Jicheng LIU2,1, Chengquan HUANG2
1National Oceanic and Atmospheric Administration, 2University of Maryland

Soil moisture and evapotranspiration (ET) are among the major components of global water and energy cycle. They are among the critical variables of NOAA numerical water, weather and climate prediction models. Temporarily and spatial continuous observations are required for the verification, validation and calibration of these models. NOAA NESDIS has developed a global soil moisture operational product system (SMOPS) and a GOES ET and Drought (GET-D) product system for providing satellite soil moisture and ET data products primarily for NOAA users. SMOPS ingests and blends soil moisture observations from NASA Aqua AMSR-E, JAXA GCOM-W AMSR2, EUMETSAT MetOp ASCATS, NASA SMAP, NASA GPM Microwave Imager and ESA SMOS. For ET retrievals, GET-D uses data from GOES-13/15 Imagers and GOES-16/17/18 Advanced Baseline Imagers for clear skies and integrates data from GOES and AMSR-E/AMSR2 for all-skies. Although these satellites provide collectively continuous observational data, the availability and characteristics of the data are not consistent among different sensors along the past decades. The evaporative stress index (ESI) based on daily ET retrievals and used as a useful independent drought data product requires long term consistent climatology of the ET data from GET-D. Therefore, NESDIS is refining algorithms for long term time series of soil moisture and ET retrievals using the various satellite observations. Various machine learning algorithms are used to calibrate different satellite data, retrieve soil moisture and ET, and blend the all available soil moisture retrievals when the individual satellite data are available on a same day. This paper will present some details of the machine learning algorithms for the reprocessing of the long-term soil moisture and ET data products obtained thus far. Preliminary validation and application results will be demonstrated. Generation of even longer term data products of the satellite soil moisture, ET and ESI will be discussed.


HS15-A008
Hydrologic Predictions Using Surrogate River Discharge Derived from L-band Microwave and Hydrologic Signatures

Hae Na YOON1#+, Ashish SHARMA2, Lucy MARSHALL2
1Macquarie University, 2UNSW Sydney

Predicting hydrologic events, such as floods, is of utmost importance for mitigating their potential impacts and making informed decisions for society. To overcome limitations in collecting data through ground-based in-situ methods, researchers have increasingly paid attention to remote sensing to measure hydroclimatic variables. New methods have been developed in recent years, including surrogate river discharge (SR), to enhance hydrologic predictions in ungauged catchments. This study introduces the surrogate river discharge model (SRM), a novel approach that solely relies on remotely sensed data and climatic variables. The SRM infers river discharge using the ratio of target and reference reflectance from a satellite signal but requires a hydrologic signature for physical realism. Here the Budyko relationship, which derives the mean river discharge using precipitation and potential evapotranspiration data, is incorporated into SRM to estimate the signature in ungauged basins. A synthetic study is conducted to evaluate the impact of the hydrologic signature on the model’s predictions, demonstrating that estimates within a range of -40% to 20% of the true mean flow value are suitable for calibrating the SRM. Despite being influenced by the quality of SR and the accuracy of the mean flow, using the Budyko relationship in SRM results in robust predictions. In conclusion, the SRM provides a promising approach for predicting hydrologic events using only remotely sensed data and climate information. Furthermore, its fast and straightforward calibration process makes the SRM a potentially widely-adopted tool for forecasting extreme hydrologic events in ungauged catchments.


Wed-02 Aug | 1:10 - 3:10 | MR330
HS02 - Artificial Intelligence for Model and Data Integration in Hydrology

Session Chair(s): Haiyun SHI, Southern University of Science and Technology, Suning LIU, Southern University of Science and Technology

HS02-A002
Application of Machine Learning Models in Improving the Meteorological Data Quality for Accurate Evapotranspiration Estimation

Satyajit DWIVEDI+, Mazhuvanchery Avarachen SHERLY#, Arun KANSAL
TERI-School of Advanced Studies

Several physical and mechanistical models, such as the FAO-56 Penman-Monteith equation and the ASCE Penman-Monteith (ASCEPM) equation, are used to estimate ET0 (reference evapotranspiration). These models require multiple meteorological inputs, including temperature, relative humidity, solar radiation, wind speed, and others that may not be available in gridded data format. Also, there are gaps in the observed data from the weather stations although all relevant parameters are recorded. Therefore, this study attempts daily ET0 estimation using machine learning at the regional level using limited weather parameters. For this, it is necessary to combine data from multiple sources, including resampled gridded data and autonomous weather station data available with IMD (India Meteorological Department) along with remote sensing data. However, the missing data, outliers, and anomalies pose data quality issues due to which data conditioning becomes a pre-requisite for ET0 model building. The identification and management of outliers and anomalies must take agroecological homogeneity into account and consider the temporal, spatial, and spatiotemporal behaviours. Machine learning models have demonstrated considerable potential in data quality event detection and appropriate treatment. In order to improve the quality of the meteorological data, a structured hierarchical process has been proposed based on machine learning models. Using the time-series clustering method, Dynamic Time Warping on daily data, homogenous zones are identified, while the LSTM autoencoder has been used to detect temporal anomalies. Using both temporal and spatiotemporal machine learning techniques like ANN, Gradient Boosting, KNN Input, and MICE approach, the anomalous events and missing values are identified, and a comparative analysis has been carried out. The proposed framework has been demonstrated for Tamil Nadu State in India using both gridded (temperature and rainfall) and observed weather station data (temperature, rainfall, and humidity).


HS02-A003
Hypothetical Ground Radar-like Rainfall Generation of Geostationary Weather Satellite Using Data-to-data Translation

Kim YEONJUN+, Sungwook HONG#
Sejong University

This study presents a deep-learning-based data-to-data (D2D) translation to simulate radar-like rainfall in order to take the benefits of the spatial coverage and temporal resolution of geostationary (GEO) satellite. The D2D method includes normalization and de-normalization in the pre-processing and post-processing stages to preserve the original data. The D2D method employs an adversarial learning structure for conversion between physical values such as albedo and brightness temperature (BT). This study selected the source and target domains covering the Korean Peninsula for training and testing the D2D model using the GEO-KOMPSAT-2A (GK-2A) and hybrid surface rainfall (HSR). This study used a dataset of 4,000 HSR and satellite data from September 2019 to September 2021. The D2D model was trained for three representative rain types in the Korean Peninsula: non-rain, stratiform rain, and convective rain, based on rainfall rate (RR). This study selected the three visible bands using the R-squared values with the strongest correlation with the radar HSR data. This study assumed the independence of infrared (IR) bands and also included the traditional BT and BT difference (BTD) in the GK-2A IR bands associated with precipitation. The developed D2D model for radar-like rainfall generation was tested and validated using radar-observed RR data. In addition, the D2D-simulated RR was compared to GK-2A RR, the Precipitation Estimation from Remotely Sensed Information using Artificial Neural Networks-Cloud Classification System (PERSIANN-CCS) RR, and the Integrated Multi-satellite Retrievals for Global Precipitation Measurement (IMERG) RR products. As a result, the D2D model showed outstanding performance for various rainfall types compared to GK-2A, PERSIANN-CCS, and IMERG RRs. Consequently, the D2D RR model can contribute valuable and virtual ground radar-like rainfall distribution and intensity with a GK-2A temporal resolution beyond the radar coverage over the Korean Peninsula, including the East Asia region.


HS02-A004
A Review of Computer Vision Techniques Adopted to Tackle Problems in Water Resource Engineering

Hyewoon JANG+, Donghwi JUNG#
Korea University

Computer vision (CV) techniques analyze and process visual data (e.g. image, video) to extract meaningful information and to recognize the pattern of objects from them. Due to the advances in the related technologies (e.g., cameras, artificial intelligence) and growth of big data, CV techniques are applied to a wide range of fields such as automation, robotics, security, manufacturing, etc. During the last decade, CV techniques began to be widely adopted even in the water resource engineering(WRE) domain: from real-time river flow discharge estimation and fault detection in sewer pipes to identification of microplastic particles in water. However, few studies have been devoted to comprehensively and systematically analyzing the current trend of CV techniques applied in WRE. In this study, a state-of-the-art review has been matched between WRE problems and CV techniques to identify the general characteristics. To that end, we first (1) classified the WRE problems for which CV techniques were applied into research topics (e.g., fault detection, water quality and contamination, water level and velocity), (2) identified the CV technique’s type used (e.g., image segmentation, objective detection, objective tracking), and (3) analyzed the level and trend of each CV techniques applied. Through this, connectivity is identified from the type of CV techniques used for each WRE problem, input data used, and what processing methods are mainly used. For example, a problem called Fault detection in Sewer pipes uses CV technique for objective detection. Due to, detecting defects based on videos obtained using a single camera. To this end, analysis is mainly used by applying CNN-based models such as R-CNN, Fast R-CNN, etc. Based on the methodology proposed in this paper, future research directions of expansion and applicability of CV techniques in WRE are suggested.


HS02-A005
Influence of Predictor Aggregation on Performance of Machine Learning Metamodels for Predicting Transit Time

Reed MAXWELL, Mario SORIANO#+
Princeton University

Water transit time, referring to the time it takes for a parcel of water to travel across a catchment, has broad implications for water quality, quantity, and sustainability. Physically based numerical modeling has been shown to accurately describe transit time distributions but often requires high computational costs. In this study, we study the potential of machine learning approaches for computationally efficient prediction of key transit time metrics. Specifically, we employ a continental scale, three-dimensional, integrated hydrologic model coupled with Lagrangian particle tracking to quantify transit time to stream discharge in the Upper Colorado River Basin, USA. Particles are initialized at streams and tracked backwards to their entry points on the land surface. We use the particle tracking results to train machine learning metamodels for predicting the mean and variance of transit time at different levels of aggregation: point (no aggregation), upstream watershed, and hydrologic unit. Upstream watersheds are delineated for each point in the stream network, while hydrologic units are extracted from a standardized national scale dataset. Input predictors for the metamodels include descriptors of topography, climate, and geology. Functional input-output relationships are evaluated through model-agnostic explainability techniques and compared to theoretical physically based relationships. Results from the analysis help elucidate the effects of aggregation scale on machine learning metamodel performance and provide guidelines on the appropriate use of such models for water management decisions.


HS02-A006
An Automatic Evaluation Mechanism of Acoustic-induced Rainfall Technology

Linhao FAN1#+, Ji CHEN1, Tiejian LI2, Hongwei XIE3, Jiaye LI4, Mengyao WANG1, Jinzhao WANG3
1The University of Hong Kong, 2Tsinghua University, 3Qinghai University, 4Dongguan University of Technology

Acoustic-induced rainfall technology as a new type of artificial rainfall enhancement technology has received a lot of attention in recent years. On the one hand, laboratory experiments have proved the reliability of the effect of acoustic waves on particle agglomeration from the mechanism; on the other hand, field experiments have proved the authenticity of the effect of acoustic waves on precipitation. However, there has been few quantitative assessments of the mechanism of acoustic-induced rainfall technology so far. In this study, a fully automatic evaluation platform for acoustic-stimulated precipitation technology based on the air-modulated fluidic acoustic system that could accurately determine the actual acoustic effective area in precipitable clouds is demonstrated through large-scale field acoustic atmospheric attenuation experiments. Besides, a specially designed cluster acoustic generation system was used to achieve the directional propagation of acoustic waves, which effectively slowed down the acoustic attenuation, thereby retaining more high-intensity acoustic waves reaching the target cloud layer. Our research is of great value for further assessment of the overall efficiency of acoustic precipitation and ultimately the full application of acoustic-induced rainfall technology.


HS02-A010
Deep Learning Framework for Correcting Satellite-based Precipitation Products in Mekong River Basin with Discontinuous Observed Data

Xuan-Hien LE+, Van Giang NGUYEN, Sungho JUNG, Giha LEE#
Kyungpook National University

The Mekong River Basin (MRB) is one of the largest watersheds in the world, spanning six developing nations in Asia and impacting over 60 million people. However, studies on reducing the bias of satellite-based precipitation products (SPPs) in this region have been limited due to the lack of up-to-date ground-based rainfall data sources. The most widely used reference data source for MRB studies is the APHRODITE product, which has not been updated since 2015. This study proposes a novel deep learning-based approach to address this challenge by combining convolutional neural networks and the benefit of encoder-decoder architecture to eliminate pixel-by-pixel bias and enhance the accuracy of SPPs. The model was applied to five gridded precipitation products, including four SPPs (TRMM, CMORPH, CHIRPS, and PERSIANN-CDR) and one gauge-based product (APHRODITE), and was evaluated in the MRB. According to the results of the analyses, the TRMM product exhibited the best performance among the four SPPs analyzed, and the deep learning model effectively reduced the spatial-temporal gap between the SPPs and the gauge-based product. The ADJ-TRMM product performed the best among the four corrected products, followed by ADJ-CDR and ADJ-CHIRPS. This study highlights the advantages and disadvantages of each SPP in the MRB, indicating that different SPPs may perform better in different regions. Moreover, the deep learning framework is a powerful and flexible tool for bias correction in the MRB and other regions, as it can capture complex patterns and learn from the data to make adjustments. The proposed model is a promising solution for generating a more up-to-date and reliable dataset for MRB research, especially after the discontinuation of the APHRODITE product. Overall, this study demonstrates the potential of deep learning-based approaches for improving the accuracy of SPPs and reducing bias in hydrological and watershed management applications.


Wed-02 Aug | 1:10 - 3:10 | MR333
HS17 - Climate Variability and Its Impact on River Hydrology: Observational and Model Based Studies

Session Chair(s): Subashisa DUTTA, Indian Institute of Technology Guwahati

HS17-A002 | Invited
Comparison of Rainfall-runfoff in the Mekong River Basin Using Grid-based Precipitation Products(GPPs)

YoungHun KIM+, Xuan-Hien LE, Sungho JUNG, Alena GONZALEZ BEVACQUA, Giha LEE#
Kyungpook National University

Rainfall-runoff analysis is an important process in water resource management and planning, such as flood forecasting and warning. Rainfall data collected from a dense rainfall observation network is the most important data for accurate rainfall-runoff analysis. The Mekong River Basin, which is the target area of this study, is a nationally shared river. It is difficult to collect data with high reliability because the data collected by country is different and the density of observation stations is low. Recently, with the development of remote sensing technology, it has become easy to obtain grid-based precipitation products(GPPs), and various hydrological analysis studies have been conducted in unmeasured or large basins using GPPs. In this study, three satellite GPPs (TRMM, GSMaP, PERSIANN-CDR) and two GPPs (APHRODITE, GPCC) were used to evaluate the applicability of GPPs in the hydrologic analysis of an unmeasured large basin. In addition, it was conducted using the SWAT model to simulate rainfall-runoff for the Mekong River basin. Spatio-temporal correction of satellite GPPs was performed using the ConvAE algorithm, a convolutional neural network model, with APHRODITE as an observation value. In addition, four water level stations, Luang Prabang, Pakse, Stung Treng, and Kratie, which are the major outlets of the Mekong River, were selected to calibrate the parameters of the SWAT model (2004-2011) and compare and analyze the results of the rainfall-runoff simulation (2012-2013) before and after correction of the GPPs. As a result, GPPs before calibration was under or overestimated compared to APHRODITE, but it was analyzed that the spatio-temporal correlation was improved at all points in the case of GPPs after calibration using ConvAE. Therefore, it is expected that the correction technique using ConvAE can be used in the hydrographic analysis of the unmeasured basin using various satellite precipitation data in the future.


HS17-A005
Impact of Climate Change on Hydrological Extremes in Brahmaputra River Under 2o and 3o C Global Warming Level

Rishi GUPTA#+
Indian Institute of Technology Jammu

The present study investigates effects of anthropogenic climate change on hydrological extremes within 2o and 3o global-warming in the Brahmaputra River basin, India. An ensemble mean of 13 different climate models under CMIP6 projections has been simulated under two different Shared Socioeconomic Pathways (SSP2-4.5 and SSP5-8.5). A widely used hydrological model, SWAT (Soil Water Assessment Tool) was used to systematically assess the changes in discharge pattern and flood wave characteristics in the river basin. The analysis indicated a significant increase in annual rainfall of 30% by the end of this century from the baseline period (year 1990-2020), which corresponds to almost 6oC warmer climate under SSP5-8.5 scenario. Annual high flow (Q05) has also been observed to be increasing by 25% and 60% respectively in the early future, EF (year 2021-2050) and far future, FF (year 2071-2100), while it increased by 24% and 38% under 2oC and 3oC warming. Annual low flow (Q95) increased by 8% in the FF, whereas it decreased by 4.5%, 7.5%, and 6.7% in 2oC, 3oC and EF scenarios, respectively. Number of consecutive wet days (CWD) were decreasing in the pre-monsoon by 7% which was increased by 4% in monsoon period. The monsoonal high flow was also increased by 30% and 40% under the SSP5-8.5 scenario for 2oC and 3oC warming periods whereas the pre-monsoon high flow was increased by 48% and 65%, respectively. There was a decrease in pre-monsoon low flow by 15 % while a minor rise of 2-3% in monsoon low flow. The study predicts warmer and dryer pre-monsoon periods with concentrated rainfall over a shorter span under 3oC warming whereas a wetter monsoon period under 2oC and 3oC warming. The results of analysis can be helpful for understanding the future hydrological response of catchment that influences hydrological designs and planning of river basin management.


HS17-A007
High-resolution Satellite Imaging for Characterizing the Braided Morphology of the Brahmaputra River

Ketan Kumar NANDI1#+, Chandan PRADHAN1, Subashisa DUTTA1, Kishanjit KHATUA2
1Indian Institute of Technology Guwahati, 2National Institute of Technology Rourkela

This study examines the highly braided Brahmaputra River, which poses a major challenge due to its complex and non-uniform processes and high energy dissipation. The role of in-stream vegetation in energy dissipation adds to the difficulty in understanding the system. The study aims to conceptualize the hierarchical energy dissipation process in the river. Using Google Earth Engine (GEE) cloud computing, the study analyzed historical satellite products from 1990 to 2019 to develop an ecosystem-based approach. The Modified Normalized Differenced Water Index (MNDWI) and the Normalized Differenced Vegetation Index (NDVI) were used to determine the sand-bar area and vegetation cover. The results showed that the braided belt of the river has dissipated a significant amount of energy, resulting in multiple geomorphic stages. The bar assemblage and confluence-bifurcation nodes also trigger mechanisms for the mega-channel formation and channel-in-channel physiography. Additionally, the vegetation cover operates as a filter for the system and its bio-morphological properties contribute to geomorphic unit stabilization. This study provides valuable information for river restoration or rejuvenation planning and design for researchers and river managers. It highlights the important role of vegetation in energy dissipation and geomorphic stability in the highly braided Brahmaputra River.


HS17-A006
Evaluating the Influence of Hydrological Changes on the Process-based River Recovery Trajectory in Asian River Systems

Chandan PRADHAN#, Suman Kumar PADHEE, Ketan Kumar NANDI, Subashisa DUTTA+, Rishikesh BHARTI
Indian Institute of Technology Guwahati

Large Asian Rivers are known for their high flow-sediment variability resulting in a non-uniform spatio-temporal distribution of geomorphic units. The interplay of local topography and periodic fluvial disturbances leads to frequent morphological changes such as bar formation, migration, and sculpting. To assess the past and future fluvial status of these dynamic river systems (the Brahmaputra and the Brahmani), the concept of river recovery (RR) is essential. RR is defined as the fluvial system's capacity to adapt to changes in boundary conditions, including those caused by climate variability and its impact on river hydrology. The present study has used the Google Earth Engine Clod Computing (GEE) platform for assessing the river recovery trajectories in the Brahmaputra and Brahmani Rivers. The results from this study reveal the inherent resilience of large Asian Rivers and presence of mega channel strips of 3-4 km and < 1km in the Brahmaputra and Brahmani River, respectively. Additionally, this study takes an observational and model-based approach to investigate the influence of climate variability on river hydrology. Finally, the RR model developed for Asian Rivers integrates a multi-disciplinary approach, incorporating both natural and engineered solutions, long-term morphological status, and societal feedback.


HS17-A008
Climate Change Impact on Spring Water Discharge in the Himalayas Region

Netrananda SAHU#+
University of Delhi

Climate change’s impact on hydrological regime in the Himalayan region is become a significant issue in Indian context. Springs are the major sources of surface water for the Himalayan people. Recent observation has been reported that the spring-water discharge has been decreased year after year. Resulted into, disappearance is now a common issue in the Himalayan region especially in the upper part of Himachal Pradesh due to both climate change and anthropogenic activities. But in this study, we focused on the reduction of spring-water discharge in response to climatic data from 1981 to 2021. Therefore, the multi-linear correlation plot was used to identify which parameter has the strong association. The value was denoted that the rainfall has the strong association (=0.94) with the spring-water discharge. So, we used rainfall-runoff model using MIKE 11 NAM hydrological model to estimate and assess the discharge trends of spring-water in response to daily average rainfall data. After model calibration and simulation, it explicated that spring-water runoff both observed and simulated were decreased tremendously almost 29% within past 40 years. The validation results (NSE=0.79, R2=0.944, RMSE=0.23, and PBIAS=32%) showed that the model was well performed and executed the model simulation results. However, reduced spring-water discharge was made sensitive the hydrological (groundwater stress, base flow, and stream water flow) and environmental entities (drinking water, evaporation, soil moisture, and evapotranspiration). So, either preserve the rainwater in shorter reservoir during the rainy season is the prerequisite or being a resilient people adjusted with the situation. This study will help the researcher or policy maker to think and work about spring disappearances and its consequences in the Himalayan region.


HS17-A014
Assessing the Hydro-geomorphological Impacts of Manas-Sankosh-Teesta-Ganga River Interlinking Project

Saikat DAS#+, Subashisa DUTTA
Indian Institute of Technology Guwahati

India is a diverse country with a broad range of natural resources and socioeconomic conditions. In addition, the distribution of water resources in India is characterized by an uneven spatiotemporal pattern. India faces acute water scarcity due to the uneven distribution of water resources, and river interlinking is being explored as a potential solution to transfer water from surplus rivers to deficient ones. The Manas-Sankosh-Teesta-Ganga (MSTG) River Interlinking project aims to address water scarcity and improve irrigation in the northeast region of India. However, this large-scale intervention has the potential to impact the hydrological regime of interconnected rivers, with both positive and negative consequences. A comprehensive surface and groundwater modeling study is conducted to understand the effects of the interlinking project on water resources. The results suggest that the interlinking project could lead to increased surface water availability in deficit river basins while reducing the average flow in surplus river basins. The study also confirms that interlinking could lead to changes in groundwater recharge, with potential impacts on groundwater quality and quantity. The project may have ecological impacts, including changes in water quality and loss of habitats for aquatic species. It is important to consider both surface and groundwater impacts when evaluating the effects of river interlinking projects, and this study provides essential information for informed decision-making and risk management in the implementation of the MSTG interlinking project.


Wed-02 Aug | 1:10 - 3:10 | MR336
HS15 - Satellite Remote Sensing for Water and Carbon Cycle Studies

Session Chair(s): Jinhu BIAN, Institute of Mountain Hazards and Environment, CAS

HS15-A010
Spatially Gap-filling and Downscaling of Visual/NIR Derived Flood Inundation

Ying HU1#+, Wenjiang ZHANG2, Huan WU1
1Sun Yat-sen University, 2Sichuan University

Visual/near-infrared (NIR) remote sensing is widely adopted in flood monitoring because of high resampling frequency, but it has weakness of coarse spatial resolution and missing coverage in cloudy weather. Previous gap-filling and downscaling algorithms highly depending on terrain information tend to cause failure in downstream river reaches because of the low variation in terrain elevation and the complex flood defense system. In this study, we propose an improved downscaling algorithm for fast inundation mapping at high resolution by taking full advantage of multi-scale hydrological connectivity and accounting levee effects. The original visual/NIR data is preprocessed to remove false water grid cells which are related to DEM outliers and levees, while missing water grid cells are recovered through a grid spreading algorithm based on flow direction and surrounding elevation distribution. The adjusted coarse-resolution (360m) water mapping is then downscaled to a high resolution (10m) by matching the water fractions between the fine and coarse resolutions. Water fraction of a coarse grid cell at water-land boundary is spatially distributed to the fine grid cells filtered by elevation sorting, while the hydrological connectivity is preserved at the fine resolution. The algorithm is applied to four scenes of NOAA VIIRS for Dongting Lake, China acquired in July, 2020 when a major flooding event lasted more than six weeks. The validation is performed by comparing the downscaled results with ESA Sentinel-1 imageries acquired at the similar times. The comparison shows significantly increased monitoring accuracy of the original visual/NIR product from 57.5% to 75.2%, and decreased missing rate from 42.7% to 24.8% with only minor increase in false rate from 17.0% to 23.1%. The evaluation also shows a very good gap-filling efficiency of the new method, which is highly appealing for real-time flood mapping as heavy clouds often occur during the flooding.


HS15-A020
Estimation of Actual Evapotranspiration and Its Components by Integrating the Shuttleworth-Wallace and Surface Temperature-vegetation Index Schemes

Yaokui CUI#+
Peking University

Daily actual evapotranspiration (ET) and its components –soil evaporation (E) and vegetation transpiration (T) –play a key role in water resource management of irrigated areas. Nevertheless, due to large uncertainties in the parameterization of the resistances, traditional ET models do not always provide accurate ET estimates, especially for its components. This uncertainty is mainly due to the difficulty of determining the empirical parameters accurately of soil and canopy resistances which is debated for a long time and the error in input variables. This paper proposed an optimized Shuttleworth-Wallace model (SW) using the particle swarm optimization (PSO) algorithm to integrate the original SW with the surface temperature-vegetation index (Ts-VI) triangle models (named Shuttleworth & Wallace_Temperature Vegetation Index model, SW_TVI).The performance of the SW_TVI model was significantly improved by optimizing the soil and canopy resistances in the original SW model using discontinuous regional ET estimates from the Ts-VI model under clear-sky conditions. Compared with the original SW model, the root mean squared error (RMSE) and mean absolute deviation (MAD) of the SW_TVI model were reduced by more than 30%, against in situ measurements in the Heihe River Basin. The Bias of the T/ET ratio was also significantly reduced from -22.3% for the original SW model to -5.5% for the SW_TVI model. The annual contributions of E and T to ET were about 20% and 80%, respectively, and had a strong seasonal variation in the typical irrigated area of China. In summary, the SW_TVI model shows three outstanding advantages: (1) it estimates daily continuous E, T, and total ET with high accuracy; (2) it is very robust and insensitive or slightly sensitive to most input variables and empirical parameters; (3) it is independent from ground data. This new SW_TVI model will benefit water resources management.


HS15-A021
Partitioning of Evapotranspiration Based on Flux Variance Similarity Theory for an Urban Forest Land

Han LI+, Han CHEN, Jeanne Jinhui HUANG#
Nankai University

Partitioning of evapotranspiration(ET) of urban forest land is important for guiding precise irrigation decisions in urban areas and assessing the impact of urbanization on the urban hydrological cycle. Although ET partitioning has been extensively studied in natural ecosystems, there have been relatively few studies in urban ecosystems. For the first time, the flux variance similarity (FVS) theory was used to partition urban forest ET into soil evaporation (E) and vegetation transpiration (T). The performance of daily T/ET based on five leaf-water use efficiency(WUE) algorithms was verified using two years stable oxygen isotope observations. The driving factors affecting the T/ET were investigated. The simulation results indicated that the T/ET ranged from 0.38 to 0.96, with a mean value of 0.62. The validation results suggested that the constant value WUE algorithms performed very good agreement when the leaf area index (LAI) varied between 3.85-6.02, with the lowest root mean square error (0.14), bias(0.21), and mean absolute percentage differences (17%). Although the optimized-WUE algorithm has proved the reliability of the FVS theory in urban forest land, only 15% of the eddy correlation(EC) data was available to partition successfully. Furthermore, correlation analysis showed that T/ET was mainly controlled by air carbon dioxide(CO2) concentration, air temperature(Ta) and LAI throughout the growing season. Compared to natural ecosystems, the urban forest T/ET is about 10% higher due to the existence of higher air CO2 concentration, Ta, and higher tree planting densities. This study successfully partitioned urban forest ET using high frequency EC observations and the FVS theory. The results of the study gained insight into the effects of urbanization and enhanced our understanding of urban the hydrological cycle.


Wed-02 Aug | 3:30 - 5:15 | MR330
HS02 - Artificial Intelligence for Model and Data Integration in Hydrology

Session Chair(s): Suning LIU, Southern University of Science and Technology, Haiyun SHI, Southern University of Science and Technology

HS02-A011
Bias Correction of Satellite Precipitation Products (SPPs) Using Machine Learning in the Amazon River Basin

Alena GONZALEZ BEVACQUA+, Xuan-Hien LE, Giha LEE#
Kyungpook National University

The Amazon River basin is the biggest basin in the world spanning several countries. Its ecosystem is essential for food production, biodiversity, hydrology, and climate regulation. Therefore, understanding the hydrometeorological process in the Amazon River basin is fundamental to its maintenance. Yet, monitoring the Amazon River basin is still challenging due to its size, remote areas, and low density of the monitoring gauge network. Remote sensing products are a way to tackle those issues, and they have been largely used since it allows to have spatial-temporal homogeneous and continuous datasets. However, those products still have high uncertainty. Therefore, in this study, we aim to improve the accuracy of Satellite Precipitation Products (SPPs) in the Amazon River basin through bias correction using a machine learning approach. Thus, we used the convolution neural networks combined with an autoencoder architecture, known as convolution autoencoder (ConvAE), to correct the bias in each pixel of the SPPs. We use three daily precipitation gridded datasets (CHIRPS, PERSIANN-CDR, TRMM). For the observed data, 331 rainfall gauges were utilized. The period of analysis goes from January 1st of 1990 to December 31st of 2010 due to the limitation of the observed data. The performance of the bias correction method was evaluated using several statistical indicators (NSE, RMSE, MAD).


HS02-A012
A Platform for Extreme Rainfall Nowcast Using Deep Learning Methods and a Regional Climate Model

Ji CHEN#+, Xianqi JIANG, Hongyi YAO, Chao TAN1,1, Hongxu ZHU
The University of Hong Kong

Capability of nowcasting extreme rainfall plays an imperative part in the forecasting and warning of geohazards in urban areas. With the development of artificial intelligence, deep learning techniques have the ability to process enormous amount of meteorological data and identify underlying physical characteristics which has the potential for accurate and timely extreme rainfall forecasting. Our study focuses on the extreme rainfall nowcasts using radar echo maps based on several state-of-the-art deep learning models. In the study, we develop a new platform to improving nowcasting skill, and the platform includes a regional climate model, WRF, and several deep learning methods. Using the radar echo map dataset provided by the Meteorological Bureau of Shenzhen Municipality in China, we will provide nowcasting results.


HS02-A015
Application of Machine Learning in Predicting Turbidity in the Mountainous River, a Case Study in Lai Chi Wo Catchment, Hong Kong

Yi LU1,2#+, Ji CHEN2, Hongxu ZHU2, Hongyi YAO2, Zhaofeng HAN3, Qian XU2
1Hong Kong Chu Hai College, 2The University of Hong Kong, 3THE UNIVERSITY OF HONG KONG

In the mountainous catchment area, the intensity of sediment movement has a great impact on the quality of water resources. Excess suspended sediments in the water system can be harmful to aquatic life. Continuous suspended solids records cannot be easily obtained accurately with the current techniques, while turbidity is usually seen as the surrogate for presenting sediment movement. To strengthen the water quality management in the watershed, this study attempts to use Machine Learning (ML) to set up a prediction model for turbidity in the catchment. A monitored dataset of the water quality parameters and hydrological parameters obtained from the Lai Chi Wo (LCW) catchment in Hong Kong was adopted in this study. In exploring the application of ML methods in the hydrology field, some types of Artificial Neural Networks (ANN) were constructed to realize the turbidity prediction model in the current study. It was found by the investigation that the Long Short-Term Memory neural network (LSTM) showed high efficiency in predicting turbidity. In addition, combinations of various associated hydrological factors can improve the prediction accuracy of the model. The improvement of the data resolution per unit of time can also enhance the predictive performance of the model. The current study was devoted to providing more innovative technologies and modern working ideas in establishing an intelligent water-safety-early-warning platform to prevent or reduce the impact of human activities and natural disasters on environmental sustainability.


HS02-A016
Large-scale Precipitation Nowcasting Based on a Novel Deep Learning Model

Jinkai TAN#+
Sun Yat-sen University

There are two inevitable problems in most deep learning (DL)-based models for precipitation forecasting: the smoothing effect of precipitation area and the degenerate effect of precipitation intensity. Therefore, this talk proposes a novel DL framework named “time series residual convolution (TSRC)” for large-scale precipitation nowcasting for up to 3 hours. The main idea of TSRC is it compensates the current local cues with previous local cues during convolution processes, so more contextual information and less uncertain features would remain in deep networks. Four years’ radar echo reflectivity data from 2017 to 2021 are used for model training and testing. in addition, two commonly used nowcasting models: optical flow model (OF) and UNet are used to compare the findings. Results show that TSRC obtains better forecasting performances than OF and UNet with a relatively high probability of detection (POD), low false alarm rate (FAR), small mean absolute error (MAE) and high structural similarity index (SSIM), especially at longer lead times. Meanwhile, the results of two case studies suggest that TSRC still introduces smoothing effects and slightly outperforms UNet at longer lead times. The most considerable result is that TSRC can forecast high-intensity radar echoes even for typhoon rainfall systems, suggesting that the degenerate effect of forecasting precipitation intensity can be improved by the model.


HS02-A017
Monitoring the Spatio-temporal Evolution of Supraglacial Lakes in Polar Regions Based on Multi-source Remote Sensing Using Deep Learning

Jiahui QIU+, Jiangjun RAN#, Ruigang HU
Southern University of Science and Technology

Ephemerally stored liquid water on the surface of vast polar continent (i.e., Antarctica and Greenland Ice Sheet), namely supraglacial lakes (SGLs), may trigger ice discharge and modulate surface meltwater runoff thus causing mass imbalance, makes it a dynamic proxy of the cryospherical hydrology cycle. To automatically map the extent of SGLs, we present a novel method for extracting SGLs from satellite imagery using deep learning techniques. Based on Landsat 8 and Sentinel-2 data, specifically, we proposed a Convolutional Neural Network (CNN) architecture for SGLs extraction during the melting season of 2017-2022. Our results demonstrate the effectiveness, robustness, and transferability of CNN method for SGLs feature retrieving at local or regional scales compared to traditional methods (e.g., adaptive thresholding and various widely used machine learning algorithms). Several scenes of ultra-high resolution commercial satellite imagery were adopted for validation. It is apparent that the accuracy of lake detection was improved by incorporating multi-source data and utilizing both spatial and spectral features. We also employed empirical approach to calculate the depth of SGLs then further estimate the volume, which is critical for assessing the potential impact of lake drainage on ice dynamics. To better understand the mechanisms behind SGLs evolution, we conducted a detailed analysis of environmental factors that contribute to SGLs variation, including temperature, topography, and modelled surface meltwater runoff. We found that temperature had the strongest correlation with SGLs distribution, indicating that warming climate is a major driver of SGLs formation. In addition, we have identified key topographic features, such as slope and elevation, which can impact the distribution of SGLs as well as the retention capacity of meltwater. Our analysis provides valuable insights into better understanding the dynamics of cryospherical hydrology under future climate scenarios.


HS02-A018
Recent Rapid Changes in Tibetan Lake Areas Driven by Precipitation Anomaly Patterns

Ruigang HU+, Jiangjun RAN#, Jiahui QIU
Southern University of Science and Technology

The limited anthropogenic activities on the Tibetan Plateau make this an ideal natural laboratory to elucidate how climate change impacts lake changes. Previous studies have mainly focused on long-term lake area changes, yet their exact monthly and seasonal evolutions and the associated atmospheric origins remain elusive. By combining radar and optical images, we extract improved lake area changes at monthly sampling over 2015−2020. Our deep-learning-based estimates achieve an accuracy of 1–2 pixels, as evidenced by in-situ GPS field survey validations of representative lake shorelines. We conclude that evident contrasting patterns in rapid area changes: deaccelerating in north and accelerating in south, are likely caused by recent precipitation anomalies. Significant summer area expansion started in north and moved southwards, which was possibly associated with oscillations in atmospheric circulation. Our study highlights the importance of investigating short-term area change as a climate proxy to study their rapid responses to intra-annual climate variability.


Wed-02 Aug | 3:30 - 5:15 | MR333
HS29 - Water Resources Management Under Changing Environment in Asia

Session Chair(s): Xiaojun WANG, Nanjing Hydraulic Research Institute, Ministry of Water Resources, Young-Oh KIM, Seoul National University

HS29-A002
Transboundary Water Management in the Ganges-Brahmaputra-Meghna Basin Between Bangladesh, Bhutan, China, India, and Nepal

Sonia Binte MURSHED1#+, Jagath KALUARACHCHI2
1Bangladesh University of Engineering and Technology, 2Utah State University

Managing shared river systems is challenging due to increased agricultural water needs, population growth, urbanization, and existing socio-economic conflicts. Climate change is another critical factor influencing freshwater availability. In addition, the non-equitable distribution and competition for freshwater resources and varying economic and technological development among countries produce disputes and have been a source of tension in many Asian countries. As a result, the increasing and conflicting demand for freshwater necessitates transboundary water management. This study critically reviewed the existing rules, water-sharing agreements, policies, and practices for managing shared water resources in the Ganges-Brahmaputra-Meghna (GBM) river system shared between Bangladesh, Bhutan, China, India, and Nepal and compared with other water-sharing agreements, national and international laws across the world. We also proposed possible solutions to ensure water security in the GBM basin. The study found no common water-sharing framework among the five sharing countries. Existing bilateral water-sharing agreements such as the Ganges Water Treaty and Mahakhali Treaty could be more effective if a basin-wide focus was incorporated, involving all the countries at the treaty formulation stage. Segregated country-specific water management plans produce complex and conflicting issues and affect good relationships among transboundary countries. Moreover, socio-political factors, historical disputes, and lack of sufficient technical capacity affect water security. We found informal data-sharing agreements are making effective water management difficult. This study explores the possibility of focusing on common goals, such as preserving the Sundarbans Ecosystem for India and Bangladesh, which may lead to initiating a better understanding and engagement for transboundary river management. These findings demonstrate an urgent need for a comprehensive and holistic basin-wide approach that addresses these complex issues with effective involvement of all GBM countries.


HS29-A006
Does Prioritizing Environmental Flows Compromise Demand Satisfaction and Hydropower Production in the Nagarjuna Sagar Reservoir?

Akshay SUNIL#+, Riddhi SINGH
Indian Institute of Technology Bombay

Multi-purpose reservoirs present a particularly challenging decision context where multi-sectoral water and energy demands have to be balanced, while also considering the instream water requirements downstream. Although releasing adequate water to support downstream riverine ecosystem should be an essential consideration for reservoir operations, the legislative and socio-economic context may not always prioritize the maintenance of minimum environmental flows downstream over demand satisfaction and/or hydropower production. Thus, a systematic framework to evaluate the trade-offs between demand satisfaction, hydropower production and satisfaction of minimum environmental flows (MEFs) would help reservoir operators better understand the consequences of various operational choices. We designed two formulations of a multi-purpose reservoir operation problem; one that prioritized MEF (PF_MEF) releases over demand satisfaction and another that did not (PF_nMEF). We identified Pareto approximate strategies for each formulation using the Borg multi-objective evolutionary algorithm considering multiple objectives related to water demand satisfaction, hydropower production, prevention of flood exceedance thresholds and satisfaction of MEF. We applied the framework to the Nagarjuna Sagar (NS) reservoir in southern India. Reservoir operation strategies were modelled using direct policy search (DPS), where radial basis functions (RBFs) are used to condition decisions, releases for hydropower in this case, on reservoir storage states. Results show that the Pareto approximate strategies resulting from optimizing for PF_MEF and PF_nMEF attain MEF - MEF in ranges 86-98% and 56- 79%, respectively. However, the ensuing compromises in water demand satisfaction and hydropower production are not considerably higher. Mean demand deficits and mean annual hydropower production ranged from 99.9 -818.1 Mm3 (48.13-818.8 Mm3) and 3252-3900 Gwh (3394- 3910 Gwh) for PF_MEF (PF_nMEF). We were able to identify strategies from PF_MEF that attained low values of volumetric demand deficits and high values of hydropower production, indicating that prioritizing MEFs may not necessarily yield compromises for human-related objectives in this case.


HS29-A007
Tightly Couple Short-term Reservoir Dynamics with Long-term Energy Expansion Decisions to Maximize Hydropower’s Role in the Clean Energy Transition

Zhanwei LIU+, Xiaogang HE#
National University of Singapore

Reservoir hydropower plays a critical role in the clean energy transition by providing flexible, low-carbon electricity to balance variable renewable energy (e.g., solar and wind power) through changes in water head and turbined flow dynamics. Fully accounting for hydropower flexibility requires explicit representation of short-term reservoir operation processes in long-term energy capacity expansion models. However, due to the high computational complexity of multi-scale, constrained optimization problems, traditional coupling strategies typically simplify the spatio-temporal dynamics, by modelling only a few representative days for a discrete set of planning years. This fails to capture the seasonality and interannual variability of natural reservoir inflows, which can lead to suboptimal energy expansion decisions and overinvestment. To address this, we apply two linear programming decomposition algorithms, Benders decomposition and Dantzig-Wolfe decomposition, to a recently developed energy capacity expansion model, Pathways for Renewable Energy Planning coupling Short-term Hydropower OperaTion (PREP-SHOT), to jointly optimize short-term reservoir operation and long-term energy expansion decisions. Our proposed framework first decomposes the sequential multi-year investment decisions into annual decisions and then decomposes the full-year optimal operation into optimization problems for several sub-periods within the year. This allows us to run a continuous simulation that captures the full-year hourly operational details (e.g., dispatch processes) for each planning year, with guaranteed optimal solutions in finite iterations that can dramatically reduce runtime. We apply PREP-SHOT to a regional power system in China, including 46 large hydropower reservoirs (each with an installed capacity of at least 300 MW), to identify optimal decarbonization pathways from 2020 to 2050. Improved computational efficiency from this regional case study demonstrates the potential to scale PREP-SHOT even globally to fully understand the role of hydropower in the global clean energy transition.


HS29-A010
Quantifying the Sensitivity and Stability of a Multi-purpose Reservoir's Performance to Model, Inflow, and Operational Uncertainties

Manvitha MOLAKALA#+, Riddhi SINGH
Indian Institute of Technology Bombay

Performance metrics within a simulation-optimization framework are frequently used to identify and evaluate water resource management strategies. These metrics are likely to be sensitive to different levels of input variables like inflows, model-related choices, and strategy implementation errors. The ability to quantify the sensitivity of performance metrics to the aforementioned uncertain factors may thus help decision-makers understand the relative importance of these factors and their interactions. Furthermore, the total variation in performance measures caused by uncertain factors may be useful in quantifying the stability of a performance measure. We quantify the performance metrics' first, second, and total order sensitivity to uncertain factors using Sobol's variance-based sensitivity analysis. The sensitivity and stability indices are then applied to four performance metrics of the multi-purpose Nagarjuna Sagar reservoir in the Krishna river basin of southern India. To identify the Pareto approximate set of reservoir operation strategies, we use evolutionary multi-objective direct policy search (EMODPS), which employs a state-aware operating rule based on radial basis functions. We identify the stability and sensitivity of the performance measures against the following uncertain factors: i) the planning horizon (ranging from 1 to 15 years), (ii) the model timestep (daily, 15-day, and monthly timesteps), (iii) imperfect operations while employing optimized strategies, and (iv) stochastic and deep uncertainties associated with inflows. Our results show that the hydropower generation goal is the most sensitive to model choices. On the other hand, high flow non-exceedance reliability, demand deficits, and minimum environmental flow reliability objectives are particularly sensitive to deep uncertainties in inflows. We find that the flood reliability objective is the most stable and the demand deficits objective is the least stable. Our framework can be applied to any water management problem to determine the relative importance of the uncertain factors and the stability of the performance measures.


HS29-A024
Development of Discharge Estimation Using 1D Numerical Model in the Confluence of the Seomjin River

Hansol KANG1+, Joonwoo NOH2, Yeonsu KIM2, Jisun BYUN2, Hyunuk AN1#
1Chungnam National University, 2K-water Research Institute

Reliable discharge data is of paramount importance during this time of frequent floods and droughts. Typically, the discharge is derived from water level measurements using a rating curve (RC), which is established based on the correlation between water level and flow. However, uncertainties can arise during the calculation of RC parameters. This study proposes a method for estimating discharge data that accounts for both the uncertainty in RC and the uncertainty of the roughness coefficient that affects flow. This is achieved through random number combinations using the Monte Carlo (MC) method. The water level was simulated using K-RIVER, a one-dimensional model, for a set of discharge data to which the methodology was applied. The discharge data for the relevant region was then estimated based on the high reproducibility of the flood season water level, as indicated by the Nash-Sutcliffe Efficiency (NSE). This approach allows for the temporary creation of RCs at points where they have not been established, and it is believed that time series discharge estimation can be performed even in areas where discharge observations are difficult to obtain. This work was supported by the National Research Foundation of Korea (NRF) grant funded by the Korea government (MSIT) (No. 2021R1A2C200553012).


HS29-A025
Delineation of Sustainable Groundwater Extraction and Recharge Potential Zones in Agricultural Micro-watersheds Using an Integrated RS-GIS-AHP Approach

Kartick GM1#+, Meenu RAMADAS1, Suraj JENA2
1Indian Institute of Technology Bhubaneswar, 2Oregon State University

Sustainable groundwater development of region necessitates the delineation of safe yield potential zones. Such zones are identified by synchronal mapping of groundwater storage and recharge potential zones. This paper presents an approach using remote sensing (RS), geographical information systems (GIS), and analytical hierarchical process (AHP), an integrated groundwater tool for quantification the safe yield, to extend the cropping pattern of rainfed farming to irrigated farming which significantly leads to both sustainable as well as social development of the micro-watershed. This study is conducted in a micro-watershed in the state of Odisha, India. The thematic layers used in this study were soil, land use/ land cover, geomorphology, lithology, aquifer properties, drainage density, lineament density, and slope. Each thematic layer undergoes sensitivity analysis that depicts the responsive percentage changes in potential zones by defining the relative importance of the thematic layers under consideration. Moreover, the percentage overlap of storage and potential zones was found to be very insightful for the quantification of safe yield which subsequently enhanced the scope for rabi cultivation in the micro-watershed. These generated groundwater storage and recharge potential maps were helpful in finding the best extraction and artificial recharge locations respectively, which certainly augments the water resources in the region.


Wed-02 Aug | 3:30 - 5:15 | MR336
HS15 - Satellite Remote Sensing for Water and Carbon Cycle Studies

Session Chair(s): Ainong LI, Institute of Mountain Hazards and Environment, CAS

HS15-A017
Progress and Perspective of the Stereoscopic Observation and High Spatial Resolution Products Development of Key Global Change Parameters for Mountain Ecosystem

Ainong LI#+, Jinhu BIAN
Institute of Mountain Hazards and Environment, CAS

Mountains are the sentinels of climate change from the perspective of the Future Earth prospect. Remote sensing provides the key data sources for the global climate change research. However, most of the existing remote sensing products at global scale have a spatial resolution of kilometer level, which is difficult to accurately characterize the strong temporal and spatial heterogeneity of mountain land surface. Remote sensing products with higher spatial resolution, continuous temporal resolution, seamless space and reliable precision are urgently needed for scientific cognition of response and adaptation process of mountain ecosystems to climate change. This presentation systematically introduces the research progress of the Chinese key R&D project named "stereoscopic observation and high spatial resolution products development of key global change parameters for mountain ecosystem" conducted by the author team in recent years. By constructing a satellite-space-ground based stereoscopic observation experimental technology system for mountain ecosystems, the author's team carried out networked three-dimensional observations at typical mountain ecosystem observation stations in China, and obtained stereoscopic observation data sets covering key parameters of global change such as carbon/water cycle and energy balance. On this basis, by developing spatio-temporal scale expansion and inversion models for the parameters in mountain area, the author's team has carried out trial production of “reference true" products with high spatio-temporal resolution for key parameters, and has launched the production of product covering global mountains, long time series, high spatio-temporal resolution and reliable accuracy. The product will achieve important innovations in global change data sets, fill the gap in high-resolution satellite data in mountain regions, and serve the study of global change in mountain ecosystems in the near future.


HS15-A016
Global High-resolution Mapping of UN SDG Indicator Mountain Green Cover Index

Jinhu BIAN#+, Ainong LI
Institute of Mountain Hazards and Environment, CAS

Mountains provide essential ecosystem services to billions of people and are home to the majority of global biodiversity hotspots. However, the mountain ecosystem is particularly sensitive to climate and environmental change. Ensuring the protection of mountain ecosystems has been listed as the target (Target 15.4) in the United Nations (UN) 2030 Agenda for Sustainable Development. The Mountain green cover index (MGCI), one of the key SDG indicators (SDG 15.4.2) for monitoring the status of the conservation of mountain environments, is defined as the area ratio of all green plants in the mountain, including the area of forests, shrubs, woodlands, pastures, farmland with the total area of mountain. However, as a country indicator, the current MGCI data is challenging to quantify the spatial details of mountain vegetation change within each country and correspondingly hard to support the decision-making of sustainable development and protection strategy at regional scale. In this paper, a new global high resolution gridded-MGCI calculation method that depicts the varying details in the MGCI from both the spatial and temporal domains was proposed based on 30-m Landsat-8 images and the Google Earth Engine. A grid-based MGCI calculation model was firstly proposed by that considers the true surface area instead of the planimetric area of each mountain pixel. The global green vegetation cover was then extracted using all available 30-m Landsat-8 satellite observations within the calendar year on the GEE platform. The mountain true surface area was finally calculated and introduced into the MGCI calculation model for global MGCI mapping. The method has great potential for getting the spatio-temporal continuous MGCI with a high spatial resolution for characterizing explicit mountain vegetation dynamics and vegetation-climate change interactions to advance our understanding of global mountain changes.


HS15-A011
Aboveground Carbon Sequestration Variation by Forest in the Western Sichuan of China

Shiyu DENG+, Mingfang ZHANG#, Zipei LIU
University of Electronic Science and Technology of China

Spatiotemporal variation of forest aboveground carbon sequestration (ACS) at large-scale is crucial for assessing the carbon storage and time of carbon-emission peaking. Unfortunately, a systematic assessment of accurate ACS and its change is not yet developed, especially at a large scale. Here, to contribute to the national goal in the ACS assessment, we evaluate the spatiotemporal ACS trend based on the LANDIS PRO and PnET-II models, and the Mann-Kendall trend test from 2000 to 2020 in Western Sichuan, China, where various vegetation species exist. Key findings are: (1) the total ACS increased from 344.62 to 466.99 Tg due to large-scale reforestation programs from 2000 to 2020. To be specific, the ACS is statistically significant in the forested areas, especially in evergreen coniferous forests (ECF). They are mainly spruce and fir and are distributed in subalpine areas with elevations ranging from 2500 to 4000 m. In contrast, the lower carbon sequestration is located on the ranges of dry valleys with less precipitation and higher temperature than other regions. (2)Primary species fir (abies fabri), spruce (picea asperata), China fir (cunninghamia lanceolate), and cedar (cryptomeria japonica) contributed the most ACS (85.28%). Contributions of the evergreen broad-leaved forest (EBF) and deciduous broad-leaved forest (DBF) to the ACS were 7.84% and 6.21%. The ECF’s contribution per unit area is the highest. Thus, planting and increasing evergreen coniferous trees should have the maximum return in reducing the atmospheric carbon concentration. The developed methodology can be applied to analyzing the ACS at the watershed and regional level timely and helping decision-makers and managers develop effective forest management measures.


HS15-A019
A Hybrid Method of D8 and Deep Learning for Extraction of Drainage Networks from Digital Elevation Models

Jian GAO1+, Tiejian LI1, Lujie HAN1, Xin MAO2#
1Tsinghua University, 2The Hong Kong University of Science and Technology

Topographic maps rely on the precise representation of drainage networks, which is essential for a variety of research and applications. While deep learning techniques have been used to address these issues, different challenges remain. Traditional extraction method is of less efficiency, low accuracy toward flat regions, of difficulty detecting channel heads. The purpose of this analysis is to focus on high-quality data analysis, optimize and reduce management costs, and achieve better planning. Therefore, we introduced aspect features distributed representation to facilitate the calculation of process directions in deep learning models; semantic segmentation model U-Net to improve the accuracy and efficiency of predicting flow directions and pixel classifications, followed by post-processing to compartmentalize the flowlines. However, it is hard for researchers to collect real-world data from some remote regions, which is indispensable for training deep learning models. We adopt non-depression-filling method to generate ground truth and deal with the incontinuity due to our segmentation model. Our proposed framework achieved state-of-the-art results compared with the traditional methods and the published deep-learning-based methods. The case study demonstrates that the framework can extract drainage networks of different width rivers under different topography. The precise, efficient and scalable framework does not require any parameters from the user and can also generate waterbody polygons and allow the use of cyclic graphs in drainage network.


HS15-A018
Integration of Fine and Moderate Resolution Land Cover Products for Improved Global Surface Water Mapping

Chengquan HUANG1#+, Xiwu ZHAN2
1University of Maryland, 2National Oceanic and Atmospheric Administration

The distribution of surface water can affect many Earth system processes, and therefore needs to be represented properly in weather forecast and hydroclimate models. Although water has been mapped in many global land cover products, each product has its own limitations. For example, partly due to limitations of their pixel sizes, moderate resolution products derived based on MODIS or VIIRS cannot represent small water bodies and narrow water channels. While fine resolution products can provide more spatial details, most of them do not provide a complete coverage of the entire globe. In this study, we first examine the differences and complementarity of available fine and moderate resolution land cover products for surface water mapping. Based on this analysis, a global water surface fraction dataset is developed by harmonizing the existing products. A statistically based accuracy assessment will be conducted to quantify improvements of the derived product over the existing land cover products in representing surface water distribution across the globe.


HS15-A003
Looking Beyond the Grace Era: A Novel Index Based on Reconstructed Daily Grace Data for Water Extremes During 1961-2015

Abhishek ABHISHEK1#+, Jinghua XIONG2, Shenglian GUO2, Jun LI3, Jiabo YIN2
1Indian Institute of Technology Roorkee, 2Wuhan University, 3South China University of Technology

Since its launch in 2002, Gravity Recovery and Climate Experiment (GRACE) based terrestrial water storage (TWS) has been widely used for a variety of applications including, quantification of water extremes, climate change impacts, sea level changes, and water budget, among others. Despite its huge success in several interconnected applications, one of the major shortcomings is its short period of ~20 years with a coarse spatial resolution of ~one month. Here (Journal of Hydrometeorology, 23, 1419–1438, https://doi.org/10.1175/JHM-D-22-0011.1), taking the Yangtze River basin of China as an example, we reconstructed daily GRACE-like TWS during 1961-2015 using a random forest model and subsequently, proposed a conceptually improved standardized drought and flood potential index (SDFPI) by incorporating the inherent land decay mechanisms. Through comparison with the traditional indices (e.g., PDSI and SPEI) and validation with the in-situ discharge data, we demonstrate the improvements of SDFPI in capturing the spatiotemporal propagation of the hydrological extremes (i.e., floods and droughts) of varying intensities. Our results of the conceptually improved SDFPI and reconstructed long-term daily GRACE-like TWS data provide inferences for water managers and stakeholders to effectively and efficiently monitor and mitigate the extreme events in the study basin and beyond.


Thu-03 Aug | 8:15 - 10:00 | MR330
HS27 - Flash Floods: How to Forecast Potential Magnitude and Mitigate Risks?

Session Chair(s): Van-Thanh-Van NGUYEN, McGill University, Philippe GOURBESVILLE, Institute of Water Resources and Hydropower Research & University of Nice Sophia Antipolis

HS27-A005
What are the Most Useful Solutions for Flash Floods Forecast and Management?

Philippe GOURBESVILLE1#+, Qiang MA2
1Institute of Water Resources and Hydropower Research & University of Nice Sophia Antipolis, 2China Institute of Water Resources and Hydropower Research

Within the context of climate change and global warming, the flash floods are some the most serious threats for human communities. The rapid urban development combined with economic growth in many Asian countries has exacerbated the risks by increasing vulnerability of populations located in catchments where extreme flash flood events can take place. The rainfall events generating the floods are frequently related to complex conditions such as convective situations. The forecast of those events is now a priority for many communities. The challenge of flash flood forecasting requests to mobilize various resources such as regional meteorological forecasts, field data and results from real-time hydrological models. The speed of the processes involved is a major constraint as the intensity that is frequently challenging the efficiency of the classical measurement approaches. This particular context, reinforced by the high level of expectation of the exposed populations and the crisis managers, requests to review the frequently used solutions and to select only those that can provide a real added value. The presentation will review the various challenges, the implemented tools, and their efficiency. It will also underline the needs and the gaps for an efficient forecast of the extreme events and the definition of relevant mitigation actions. From various examples related to recent events, the presentation will demonstrate the efficiency and the limits of currently used solutions and the needed improvements.


HS27-A013
Flash Flood Management Strategy in Indonesia

Firdaus ALI#+, Marsya Dyasthi PUTRI, Dwi LESTARI, Khalidah AZMI
Indonesia Water Institute

The floods and landslide disaster happening in Indonesia is closely related with the heightened rainfall intensity caused by the extreme weather conditions as an impact of climate change. Environmental factors such as poor river and drainage infrastructure, deforestation, and other environmental factors that surely impacts a lot. The case study in this paper is the big flooding that happened early 2020 in Jakarta, the high rainfall intensity (377 mm/day recorded at Halim BMKG Station, East Jakarta) caused the Ciliwung River runoff and leading to floods in a number of areas in Jakarta and its surrounding areas (BNPB, 2020). An idea to mitigate the negative impacts of the Jakarta flooding is then adopted through the introduction of multipurpose deep tunnel (MPDT) to reduce the flood disaster risk of Ciliwung River. Integration of flood control by utilizing a flood control system as a means of collecting or utilizing excess water together with a system for collecting and distributing domestic wastewater for an alternative source of raw water for urban clean water supply systems while at the same time linked to efforts to improve environmental sanitation as well as efforts restoration of the quality of surface water and groundwater is an understatement for Jakarta.


HS27-A020
Climate Change Projections for Impact and Adaptation Studies in Urban Areas

Van-Thanh-Van NGUYEN#+
McGill University

Urban water infrastructures have reduced the vulnerability of the cities, but at the same time could make them more vulnerable to climate extremes, due to the lack of consideration of what might occur when the design criteria are exceeded. Furthermore, recent climate change assessment reports have indicated for the late 20th century a worldwide increase in the frequency of extreme weather events because of global warming, and this trend would be very likely to continue in the 21st century. Consequently, research on developing innovative approaches for limiting and adapting climate change impacts on urban water infrastructures is highly critical due to the substantial investments involved. However, it has been widely recognized that the main difficulty in dealing with climate change impacts for urban areas is “how to estimate accurately the changes in the hydrologic processes at the urban basin scale projected by climate models because these models do not contain an adequate description of the hydrologic governing processes at relevant high temporal and spatial resolutions as required by impact and adaptation studies”. This necessitates some form of downscaling of the climate model simulations from a coarse spatial resolution down to much finer spatial grids, and even point values if changes in local hydrologic processes are to be assessed. In addition, the required time scales for assessing the climate change impacts on the urban hydrologic processes are usually less than one day. Consequently, different downscaling methods have been developed to establish the linkage between large-scale climate variability to the historical observations at a location of interest. The overall objective of this article is to provide a critical review of the adequacy of these downscaling techniques in order to enhance our understanding of the reliability of climate change projections for improving the planning and design of our urban water systems.


HS27-A018
Improving Efficiency of Flash Flood Forecasting System in Thailand Based on the Antecedent Moisture Condition-III (AMCIII) and WRF-ROMS's Rainfall Forecast

Apimook MOOKTAREE#+, Ticha LOLUPIMAN, Sathit CHANTHIP, Piyamarn SISOMPHON
Ministry of Higher Education, Science, Research and Innovation

In the past two decades, Thailand has experienced frequent Flash floods every year. In some years, the number of affected villages has increased significantly due to heavy rainfall that occurs more frequently, caused by changes in climate conditions and land use. Flash floods usually occur in areas with high slopes, mainly in the northern and southern regions of Thailand. The severity of Flash floods depends on the amount of rainfall and the physical characteristics of the area. The flash floods cause severe damage to life and property. Therefore, the development of a flash flood warning system is very important to reduce the damage and losses. A simple Flash Flood Forecasting System (FFFS) using multi-criteria analysis and data overlaying technique was developed using 3 simple concepts consist of 1) the selecting high potential flash flood areas using the Flash Flood Potential Index (FFPI) which depends on physical properties of catchment, 2) the updating soil moisture state from AMC classes were calculated by 5-days accumulated rainfall from satellite, and 3) the forecasting of flash flood risk-areas using 24 hrs predicted rainfall from WRF-ROMS. At present, the system uses fix AMC for soil moisture criteria and 12UTC WRF-ROMS for the predicted rainfall criteria. To improve the efficiency of flash flood forecasting, the dynamic-AMC and 18UTC WRF-ROMS were evaluated and re-analyzed for each storm event. Statistical analysis such as POD, FAR and CSI were made to evaluate the forecasting performance. It was found that with the improved the AMC threshold and initial WRF-ROMS, the overall accuracy is also improved. Especially for probability of detection, POD is increase significantly. The warning areas can be narrowed down with improvement of accuracy and reliability in the warning areas.


HS27-A004
An Area-orientated Analysis of the Temporal Variation of Extreme Daily Rainfall in Great Britain and Australia

Han WANG1#+, Yunqing XUAN2
1China Institute of Water Resources and Hydropower Research, 2Swansea University Bay Campus

We present an analysis of the temporary variation of the area-orientated annual maximum daily rainfall (AMDR) with respect to the three spatial properties: location, size and shape of the region-of-interest (ROI) in Great Britain and Australia using two century-long datasets. The Maximum Likelihood and Bayesian Markov-Chain-Monte-Carlo methods are employed to quantify the time-varying frequency of AMDR, where a large proportion of the ROIs shows a non-decreasing level of most frequent AMDR. While the most frequent AMDR values generally decrease with larger-sized ROIs, their temporal variation that can be attributed to the climate change impact does not show the same dependency on the size. Climate change impact on ROI-orientated extreme rainfall is seen higher for rounded shapes although the ROI shape is not as significant as the other two spatial properties. Comparison of the AMDR at different return levels shows an underestimation by conventionally used stationary models in regions where a nonstationary (i.e., time-varying) model is preferred. The findings suggest an overhaul of the current storm design procedure in view of the impact of not only climate change but also spatial variation in natural processes.


HS27-A026
Managing Residual Flood Risk: Lessons Learned from Experiences in Taiwan

Hsiao-Wen WANG#+, Daniel DANIEL CASTILLO CASTRO, Rex CHEN
National Cheng Kung University

Risk of flooding has dramatically increased over the decades, and is complicated by climate change, such as rising sea level, more extreme rainfall, etc. Nevertheless, the residual risk of flooding still remains scarcely addressed in practice and in theory. This paper is to document the lessons learned from management actions taken to address residual risk in Taiwan. Through a semi-structured interview process, fourteen stakeholders from the flood management system in academia, government, and local communities shared their perspectives on residual risk covering various aspects, including flood risk mapping, social representations, and other management strategies. Land use reorganization and autonomous disaster prevention community initiatives were highlighted as preparedness measures and were recognized in their effectiveness to mitigate flood residual risk. However, there is still an insufficient consideration of the risk of flooding for a given building design or the urban space design yet. Besides, almost all the interviewed stakeholders agreed that marginal flood risk awareness limits the recognition and discussion of residual risk as a problem of its own. Misconceptions and the lack of communications between stakeholders have been identified as the main barriers. Interviewees pointed out that citizens are unaware of risks mainly either due to their inexperience or overtrust the safety of flood protection structures, such as levees. Overall, this work may serve useful for residual flood risk management for Taiwan and to other nations enduring similar extreme floods.


HS27-A021
Flash Flood Cases and Application of Digital Water Management Technologies in Korea

Dongwoo JANG1#+, Hyoseon PARK2
1Incheon National University, 2The Society of Korean Smart Water Grid

While abnormal weather phenomena occur frequently around the world, the frequency and intensity of large-scale natural disasters are also increasing. Extreme weather events have recently appeared in various forms such as record-high heat waves, droughts, and heavy rains all over the world, causing enormous human and material damage. Recently, the concept of digitalization has been introduced in water management systems, including smart metering, digital twin, and artificial intelligence (AI) concepts. The effects of digital water management include innovative water management, quality of life improvement, stable water resource securing, flood and drought response, integrated water management and water treatment system advancement, information transparency, tap water reliability improvement, flood and water accident prediction and maintenance efficiency. In this study, trends in flash flood in Korea were analyzed, and technological trends in smart water grid and digital water management, which are the latest water management systems in response to climate change, were identified. For this purpose, cases of natural disasters at home and abroad and trends in digital water management research were investigated. 


Thu-03 Aug | 8:15 - 10:00 | MR336
HS30 - Hydro-meteorological Forecasting: Methods and Applications

Session Chair(s): Durga Lal SHRESTHA, Commonwealth Scientific and Industrial Research Organisation

HS30-A003
Challenges in Forecasting Heavy Rainfall During 2018 and 2019 Floods in Kerala, India

Tomoki USHIYAMA1,2#+, Mohamed RASMY1, Ralph ACIERTO1, Katsunori TAMAKAWA1, Keijiro KUBOTA1, Toshio KOIKE1
1Public Works Research Institute, 2National Graduate Institute for Policy Studies

The Kerala Flood, the South India in 2018 is known as an unprecedented flood disaster resulted in more than 400 casualties, caused by abnormal rainfall in August. To mitigate the flood disaster, rainfall prediction is one of the most important nonstructural measures. We have investigated the possibility on reproducing the heavy rainfall diagnostically (boundary condition of ERA5) and prognostically (boundary condition of GFS and GEFS) via Weather Research and Forecasting (WRF) model. The target area is Chalakudy River subbasin of Periyar River in the central Kerala state. The abnormal rainfall is supported by large moisture flux from the Arabian See west of Kerala, maintained by an axis of low level jet originated by a cyclonic vortex in Bay of Bengal to the central India. As a result, heavy rainfall was developed along the windward side of the mountain range. However, the simulated rainfall underestimated two raingauge observations (Upper Sholayar Dam and Lower Sholayar Dam). Those raingauges are located between the foothill and top of the mountain range, but they are outside of our simulated heavy rainfall core area. When we tried finer resolution of model grid intervals from 5km to 1.66km, there was some improvement. An ensemble forecasting with the lateral boundary condition of GEFS forecast showed heavy rainfall core in the windward of the mountains as well, but it still has underestimation at the raingauge sites. Radar observation images showed rainbands transported from western ocean to the river basin, and provided heavy rainfall from coastal to mountainous area. Some ensemble members showed more rainfall in the foothill area than other members. The ensemble forecast could show the possibility of rainfall area in the foothill to the mountain range.


HS30-A008
A Bayesian Joint Probability Approach to Improve the Skill of Medium-range Precipitation Forecasts in Five Indian River Basins

Nibedita SAMAL1#+, Ashwin RAMAN1, Akshay SINGHAL1, Sanjeev Kumar JHA1, David ROBERTSON2
1Indian Institute of Science Education and Research Bhopal, 2Commonwealth Scientific and Industrial Research Organisation

Reliable precipitation forecast(s) is an essential component of hydrological forecasting systems. The quantitative precipitation forecasts (QPFs) obtained from Numerical Weather Prediction (NWP) models are often biased, and thus not reliable due to technical limitations in the models. Hence, the raw QPFs need to be post-processed before using it for operational purposes. This study attempts to improve the skill of raw deterministic daily annual and seasonal (summer monsoon) QPFs obtained from the National Center for Medium-Range Weather Forecasting (NCMRWF), India. A Bayesian joint probability (BJP) based rainfall post-processing (RPP) approach is implemented by modeling the relationship of joint distribution between the raw QPFs and the observation. The study is performed over 177 sub-basins in five major river basins of India located across diverse geographical extents. The post-processing approach subsequently generates 300 statistical ensemble members of calibrated QPFs with improved reliability and reduced bias. To assess the efficacy, we run the model with two temporal lengths, i.e., annual and seasonal. For the annual run, we use continuous daily data from August 2017 to December 2020, while for the seasonal run, we consider only the wet season, i.e., three consecutive monsoon seasons from 2018 to 2020. Results show that the approach successfully produces less biased, more skillful, and more reliable calibrated QPFs. We observe that the seasonal calibrated QPF (SCQ) performs better than the annual calibrated QPF (ACQ) in terms of reliability. Overall, the post-processing approach is successfully able to produce reliable calibrated QPFs over the sub-basins, which is essential for operational forecasting purposes.


HS30-A009
Sub-seasonal Prediction of Regional Drought Over India Using the Statistical-dynamical Framework

Sidhan V. V.#+, Sarmistha SINGH, Abdul RAHOOF
Indian Institute of Technology Palakkad

Drought, an extreme meteorological phenomenon, has significant impacts on a country's social, economic, and environmental stability. Early prediction of drought is crucial to provide warning and preparedness measures. Sub-seasonal prediction, which encompasses a few weeks to a few months ahead, is a critical timescale with limited memory of initial conditions, and not significantly controlled by boundary conditions. Presently, dynamical models have drawn much attention in the sub-seasonal precipitation forecast, however, the accuracy in drought prediction remains low. Statistical models using climate oscillation indices as predictors are superior to dynamic models for drought prediction. Sophisticated post-processing techniques like wavelet decomposition have shown the potential to enhance drought predictions significantly. This study explores the sub-seasonal predictability of regional drought events over India using a combination of statistical and dynamic model frameworks. Results suggest that prediction accuracy can be improved through combined statistical-dynamic framework, but significant improvements are dependent on the regions.


HS30-A004
Application of AI Technique for Bias-correction and Forecast of Near-real-time Satellite Precipitation Products

Sungho JUNG+, Xuan-Hien LE, Van Giang NGUYEN, Giha LEE#
Kyungpook National University

With advancements in space technology, high-resolution precipitation data is being produced using multiple sensors, and various studies are ongoing. Each satellite precipitation products (SPPs) has a different spatial resolution, and global SPPs are utilized highly when the hydrological data in a specific target basin is lacking or of poor quality. In addition, Climate change has led to an increase in the frequency of short-term, high-intensity localized torrential rainfall. This study generates an ensemble machine learning-based near-real-time (NRT) merged precipitation data over South Korea and uses it for short-term prediction. The model's input data includes three NRT SPPs (GSMaP-NRT, IMERG-Early, PERSIANN-CCS) and temperature, humidity, and precipitation data from gauge stations. Precipitation observation data was collected from 480 gauges and was randomly divided into 80% training data and 20% validation data, taking spatiality into account. The Kling-Gupta efficiency (KGE), Mean Absolute Error (MAE), and Root Mean Square Error (RMSE) were used as quantitative evaluation indicators. The Probability of Detection (POD), Success Ratio (SR), Bias Score (BS), and Critical Success Index (CSI) were selected from the Rain Contingency Table as qualitative evaluation indicators. The machine learning merge technique showed higher accuracy than raw NRT SPPs and other precipitation merging techniques and provided spatially stable results. Short-term precipitation prediction (1, 3, 6 hours) was performed using the merged precipitation data and demonstrated stable prediction performance in simulating the spatial pattern of precipitation. And the accuracy of the 1-hour prediction was high, but as the lead time increased, the prediction performance decreased. But it can be solved through real-time updating of the observed and produced input data. Therefore, AI techniques can be effectively used for not only bias correction of NRT SPPs but also prediction, providing high-reliability precipitation data for flood forecasting.


HS30-A005
Predicting Flood Inundation Extent Using Machine Learning Techniques

Durga Lal SHRESTHA#+, David ROBERTSON, Warren JIN, Catherine TICEHURST
Commonwealth Scientific and Industrial Research Organisation

Flood inundation modelling and mapping are critical for managing river systems to minimize loss of life and property. Hydrodynamic models are widely used to model floods but can be complex and computationally intensive, limiting their applications. Remote sensing techniques have been utilized to provide efficient and inexpensive flood inundation mappings. However, these techniques are limited in predicting real-time inundation or assessing changes under different climate scenarios. Recently, machine learning (ML) techniques have been employed for flood inundation modelling, mostly as surrogate models for hydrodynamic models. This study develops a method that combines ML and remote sensing to predict flood inundation extent. To begin, the method is applied to a set of randomly selected pixels in the Macintyre River catchment in Australia. Sub-monthly Landsat-derived raster images mapping the inundation extent from 1988 to 2020 are used. The daily concurrent and lagged streamflow data from nearby gauges and recent flood inundation are used as predictors. A range of ML techniques, including logistic regression, support vector machines, random forest (RF), multi-layer perceptron (MLP), and convolutional neural networks (CNN) are employed. Three performance metrics namely accuracy, Heidke skill, and the area under the receiver operating characteristics curve are used to evaluate the performance of the ML models. The results show that the performance of the ML models varies across the pixels, with RF generally outperforming the other models. Pixels with balanced classes (similar proportions of inundated and non-inundated cases) have accuracy well above 90%, while performance for the highly imbalanced class is worse than climatology. Future work will extend the method to simultaneously predict multiple pixels by using a model that can produce multiple outputs or by incorporating spatial information in the model predictors. This has the potential to assess the impact of climate change and various climate adaptation options on flood inundation extent.


HS30-A007
IMERG Run Deep: Can We Produce a Low-latency IMERG Final Run Product with a Deep Learning Based Prediction Model?

Ho TIn HUNG#+, Li-Pen WANG
National Taiwan University

IMERG is a global satellite-based precipitation dataset, produced by NASA. It has provided valuable rainfall information to facilitate the design or the operation of the disaster and risk management worldwide. In operation, NASA offers three types of IMERG Level 3 (L3) products, with different levels of trade-offs in terms of time latency and accuracy. These are Early run (4-hour latency), Late run (14-hour latency) and Final run(3.5-month latency). The final-run product integrates multi- sensor retrievals and provides the highest-quality precipitation estimates among three IMERG products. It however suffers from a long processing latency, which hinders its applicability to near real-time applications. In the past 10 years, deep learning techniques have made significant breakthroughs in various scientific fields, including short-term rainfall forecasting. Deep learning models have shown to have the potential to learn the complex variations in weather systems and to outperform the Numerical Weather Prediction (NWP) in terms of short lead-time predictability and the required computational resources for operation. In this research, we would like to explore the potential of deep learning (DL) in generating high-quality satellite-based precipitation product with low latency. More specifically, we investigate if DL models can learn the difference between Final- and Early-run products, and thus predict a Final- run-like product using Early-run product as input. Low-latency yet high-quality IMERG precipitation product can be therefore obtained. Various DL techniques are being tested in this work, including Auto-Encoder(AE), ConvLSTM and Deep Generative model. IMERG data between 2018 and 2020 over a rectangular area centred in the UK is used for model training and testing, and ground rain gauge records will be used to evaluate the performance of the original and predicted products. The proposed work is of great potential to improve the applicability of IMERG products in an operational context.


Thu-03 Aug | 10:20 - 12:20 | MR330
HS27 - Flash Floods: How to Forecast Potential Magnitude and Mitigate Risks?

Session Chair(s): Philippe GOURBESVILLE, Institute of Water Resources and Hydropower Research & University of Nice Sophia Antipolis

HS27-A006
Added Value of Deterministic Hydrological Models for Flash Floods

Philippe GOURBESVILLE1#+, Qiang MA2
1Institute of Water Resources and Hydropower Research & University of Nice Sophia Antipolis, 2China Institute of Water Resources and Hydropower Research

Extreme floods events have been recorded over the last five years in various regions of the world and have demonstrated the vulnerability of modern built environments regarding those specific situations. ln most the cases, the extreme flood events and the associated inundations are generated by specific meteorological conditions that combine warm and wet air masses in convective events. Under the climate change conditions and the gradual increase the temperature, the possibility to generate conditions for the development of convective and intense events is increasing. Over the last two decades, several events have been recorded along the Mediterranean coastline: Algeria, Spain, ltaly and France are some of the recurrent locations for those disasters. The recorded events have generated massive losses that frequently exceed € 1 billion for the direct damages. Similar cases are also recorded in Asian regions. This type of situation requests from the managing authorities the capacity to forecast impacts and to define mitigation plans based on the resilience approach. Within this context, a reasonable approach is to develop modelling tools that can produce a meaningful and trustable estimation of the processes. The deterministic hydrological models offer this possibility and can be deployed within decision support systems that are used for flood forecasting and real-time management. The approach is currently more and more widely implemented in different regions of the word and results are promising despite the remaining technical issues that are frequently related to computation resources to produce on time assessments. The presentation will address the most recent developments regarding distributed deterministic hydrological modelling and report successful applications including extremes cases recorded in Europe (Alex storm in France, 2020 ) and in China.


HS27-A009
Challenges & Solutions in Flash Flood Risk Analysis Using MIKE1D, Mike21FM, and Image-based Method. Application to the Lower Paillons River, Nice, France

Paguedame GAME#+, Philippe GOURBESVILLE, Philippe AUDRA, Mingyan WANG
Universite Cote d'Azur

Nice Côte d’Azur metropolis is exposed to flooding and droughts. Few existing gauging stations provide runoff data in the Paillons river which flows through the city centre of Nice. The last two kilometres of the river is channelized into a combination of open channels and closed channels. Downstream, seven closed channels merging into five at sea exist in the river bed. One of them is used as road tunnel and can be flooded during extreme rainfall events. Estimating flow discharge and water depths at the entrance of these channels and the risk of overflow is important to operational management of the road tunnel and urban flood. In addition, a set of video images was recorded during some events. However, there are limitations in the understanding of flash floods. Gaps and errors are present in monitoring data. Modelling and novel methods are used to complete discharge information for flood assessment. When runoff information is not available, hydrological models like DHI Mike SHE provide boundary conditions to hydraulic models. Thus, this study applies DHI Mike21FM, MIKE1D and image-based methods to assess river discharge during flood events. Some flood events are described. Image analysis technics like direct visual measurements and particle image velocimetry are applied to some major events. Modelling results are compared with measurements data. The performance of each approach is discussed. The results obtained are satisfactory and highlights the challenges to reproduce flow processes during flash floods in the Paillon lower river. Combining these methods provide useful insights to decision makers involved in management and mitigation of flash floods.


HS27-A008
Applications of Agent-based Modelling for Non-structural Measures Against Flooding: A Case Study of Nice, France

Hao-Ming HSU1#+, Philippe GOURBESVILLE2
1University of Cote d Azur, 2University of Nice Sophia Antipolis

Extreme rainfall events and floods can cause severe damage and fatality, and thus flood disaster management is essential to lower the risk. In order to evaluate non-structural measures of disaster management during a flood event, this study employs an agent-based model (ABM) to analyses the interaction between disaster response strategies and the environment. A historical flood event in Magnan area in Nice was selected as a study case. The study first used Mike 1D-2D coupled hydraulic model to simulate the historical flood event, and then an ABM, Netlego, was utilised to run agent simulations for representing possible human behaviours of the non-structural measures according to the result of the Mike model. The rudimentary model outputs showed the capability of describing plausible outcomes of the non-structural measures. The model can be further enhanced and extended. The aim of the study is to investigate and to improve the existing disaster management.


HS27-A010
Machine Learning and Hydrological Modeling for Flood Inundation Prediction: Case Study of Vu Gia-Thu Bon Basin in Vietnam

Mohamed SABER1#+, Sameh KANTOUSH1, Tetsuya SUMI1, Tayeb BOULMAIZ2, Karim ABDRABO1, Hamouda BOUTAGHANE3, Quang Binh NGUYEN4, Emad MABROUK5
1Kyoto University, 2University of Ghardaia, 3Badji Mokhtar-Annaba University, 4The University of Danang, 5Assiut University

Flash flood risk mitigation requires precise and accurate flood monitoring measures to support hazard management. Many machine learning techniques, have been recently used to improve the predictive accuracies of natural hazards. Therefore, the objective of this study is to use machine learning approaches and hydrological modeling for predicting flood depth in Vu Gia-Thu Bon basin in Vietnam. Ten independent factors that influence the FSMs in the study area, namely, aspect, rainfall, curvature, DEM, horizontal proximity to the river, hillshade, geology land use, slope, and stream power index, are assessed. An inventory map with approximately 850 flooding sites is based on several post-flood surveys after the typhoons in 1999, 2006, 2007, 2009, 2013, and 2020. The inventory dataset is randomly split between training (70%) and testing (30%). The AUC-ROC results are 97.9%, 99.5%, 99.5% for CatBoost, LightGBM, and RF, respectively. The FSMs developed by the ML methods show good agreement in terms of an extension with flood inundation maps developed using the rainfall-runoff model. The FSMs show that downstream areas (both urbanized and agricultural) are under high and very high levels of susceptibility. Decision-makers and planners in Vietnam can use the developed FSMs for such typhoon-prone regions to propose effective mitigation measures for community resilience and development.


HS27-A019
Monitoring and Early Warning of Wadi Flash Flood Using Image-based Techniques in the Arid Region, Oman

Mahmood AL-MAMARI1#+, Sameh KANTOUSH2, Tetsuya SUMI2, Mohamed SABER2
1Disaster Prevention Research Institute, Kyoto University, 2Kyoto University

Flash floods are a major natural hazard in a dry environment that pose a significant threat to human life, infrastructure, and properties. In arid regions, flash floods often occur in wadi channels (ephemeral streams), where a sharp hydrograph of water from a dry channel can rapidly and unexpectedly flood the channel, causing significant damage. Monitoring and forecasting flash floods in wadi channels is a critical component of disaster risk reduction and mitigation. The conventional method to monitor flash floods in the wadi system includes in-situ monitoring techniques such as water level gauges, which are inaccessible data during an extreme flood. Therefore, monitoring and quantifying these events with new technologies will provide real-time streamflow data, enabling more accurate and timely flash flood warnings. In this study, we establish a network of fixed cameras to monitor flash floods in the Wadi Samail catchment in Oman. Additionally, image-based methods used to measure surface flow velocities during a wadi flash flood to test the applicability of large-scale particle image velocimetry (LSPIV) and space–time image velocimetry (STIV) techniques for the estimation of wadi discharge and calculate the time of concentration between upstream and downstream camera locations. As a result, applying LSPIV and STIV techniques has a reliable outcome for obtaining surface flow velocity in the wadi system. Finally, these techniques will support the early warning systems, and emergency response plans to help mitigate the impacts of these events and reduce the risk and vulnerability of communities and infrastructure in wadi channels.


HS27-A014
A Novel Water Level Recognition Method in Complex Scenes

Zhong LI1, Yanwei ZHANG1#+, Xiaolong WANG1, Guocheng AN1, Qiang MA2, Philippe GOURBESVILLE 2
1Artificial Intelligence Research Institute of Shanghai Huaxun Network System Co., LTD., 2China Institute of Water Resources and Hydropower Research

Due to the diversity of climate and environment in China, the frequent occurrence of extreme rainfall events has brought great challenges to flood prevention. Water level measurement is one of the important research topics of flood prevention. Recently, the image-based water gauge water level recognition method has become an important part of water level measurement research due to its advantages of easy installation, low cost, and no need for manual reading. However, the existing image-based water level recognition methods mainly have two shortcomings: (1) serious interference from light intensity and (2) low accuracy of water level recognition for stained water gauges. To solve these two problems, this paper proposes a water gauge water level recognition method in complex scenarios. This method first uses a semantic segmentation convolutional neural network to extract the water gauge mask, and then uses the YOLOv5 object detection network to extract the letter "E" on the water gauge in the water gauge area. Based on the letter sequence inspection strategy, the algorithm dynamically compensates for the character recognition defects caused by stained water gauges. Through a large number of experiments, the algorithm can dynamically recognize water levels in complex scenarios, meeting the needs of mountain flood defense.


HS27-A001
Managing Flood Risk During Building Construction Process: A Case Study of Taichung International Convention and Exhibition Center

Ihsin WU#+, Tsun Hua YANG
National Yang Ming Chiao Tung University

Short-term impacts are visible during extreme weather events such as flash floods and typhoons. The damage can include death; injuries; loss of infrastructure; damage to businesses; and interruption of the progress of the construction. Identification of areas at high risk of flooding can help decision makers take proactive measures accordingly to decrease the damage. For example, floods can have a big impact on construction facilities located in basements and first floors. It would put construction projects behind planned schedule and increase the total cost of the projects. Given early warning information, portable power generators can be removed in advance to prevent a power outage. To the best of our knowledge, no study has yet examined the flood risk specifically for construction sites and discussed preventive measures for different stages of building construction. This study is a first attempt to address the abovementioned issues and Taichung International Convention and Exhibition Center currently under construction was chosen as the study area. The idea is to divide the building construction process into different stages. For example, this study identified five stages which are false work, excavation, foundation, basement, and ground surface. Given rainfall events for different return periods, this study applied TUFLOW, a fully-dynamic hydraulic model, to produce various flood risk maps of each stage. Recommended response measures were also provided along with the flood risk maps. It is expected that the site managers can respond to the threats with these maps and associated measures while receiving weather warning information in practice. As a result, the damage to the construction site can be decreased and the works can proceed without further delay.


HS27-A002
Deep Learning-based Solver for Dynamical Systems of Shallow Water Equations

Shunyu YAO#+
China Institute of Water Resources and Hydropower Research

Landslides, debris flow, collapses, and other geological disasters are common in mountainous areas in China. Researchers often use shallow water equations as the control equation for simulating the movement of these disasters. Solving partial differential equations with traditional methods requires a detailed understanding of the basic physics of the system and the mathematical techniques used to solve PDEs. This can pose difficulties for modelers responsible for solving large-scale complex systems. This paper aims to provide a new approach to constructing solvers for shallow water equations. Here, we construct a deep learning-based spatial discretization format, build a flux prediction model, use an explicit format for time step advancement, use a central difference format for the source term differentiation, and handle the dry-wet boundary to prevent false momentum from causing the solution process to converge. We evaluate the performance of the deep learning-based solver in simulating landslides on real terrain and compare it with the mainstream simulation software Massflow. Our results demonstrate that deep learning modeling is a viable approach to constructing solvers for shallow water equations and greatly reduces the modeler's requirements for understanding basic physics and mathematical theory used to solve partial differential equations.


HS27-A027
Application of Nature-based Solutions for Coastal Protection

Wei-Cheng CHEN#+, Cheng-Hui LIAO, Dong-Jiing DOONG
National Cheng Kung University

Climate change is a global challenge that is leading to a variety of serious disasters. In Taiwan, coastal erosion is leading to the loss of coastal recreational areas and biological habitats. To address these societal challenges, many coastal protection measures have been proposed that incorporate nature-based solutions (NbS). NbS have received considerable attention as a means of addressing societal challenges such as climate change and promoting enormous benefits such as human well-being, ecological diversity, and socio-economic benefits. However, the concept of NbS is diverse and complex, and there is a lack of clear evaluation criteria and implementation processes. In this study, we have developed an integrated framework for evaluating NbS measures to ensure consistency with the international consensus on NbS. The framework includes an initial pre-selection, evaluation indicators, and ranking analysis. The evaluation process initially pre-selects with 8 filters to exclude inappropriate measures and considers 12 utility aspects of NbS implementation, including quantitative criteria and stakeholder indicators. This study applies the framework to the evaluation of coastal protection measures and highlights the need for the concept of co-implementation, with more discussion and co-design with stakeholders to avoid controversy in different aspects and to establish a process that meets international standards. Overall, this study contributes to the development of a comprehensive NbS framework focusing on coastal erosion, providing transparency and more direct ways to assess NbS and enhance its credibility.


Thu-03 Aug | 10:20 - 12:20 | MR336
HS25 - Sustainable Water Resource Management in a Changing Climate

Session Chair(s): Van-Thanh-Van NGUYEN, McGill University, Pingping LUO, Chang'an University, Shie-Yui LIONG, NA

HS25-A012
Development of Extreme Rainfall Intensity-duration-frequency Relations for Climate Change Impact and Adaptation Studies in Urban Areas

Van-Thanh-Van NGUYEN#+
McGill University

There exists an urgent need to assess the possible impacts of climate change on the design storm for improving the design of urban water infrastructures in the context of a changing climate. This design storm is commonly estimated from the intensity-duration-frequency (IDF) relations at the location of interest. Consequently, the derivation of IDF relations in the climate change context for a given location has been recognized as one of the most challenging tasks in current engineering practice. The main challenge is how to establish the linkages between the climate projections given by Global/Regional Climate Models at global/regional scales and the observed extreme rainfalls at a given local site or at many sites concurrently over an urban catchment area. If these linkages could be established, then the projected climate change conditions given by climate models could be used to predict the resulting changes of local extreme rainfalls and related runoff characteristics. Hence, innovative downscaling approaches are needed in the modeling of extreme rainfall processes over a wide range of temporal and spatial scales and given the high uncertainty in climate projections by different climate models. Therefore, the overall objective of the present paper is to provide an overview of some recent progress and shortcomings in the modeling of extreme rainfall processes in a changing climate from both theoretical and practical viewpoints. In particular, the main focus of this paper is on the development of some guidance to water professionals on how to consider the climate change information in the design of urban water infrastructures.


HS25-A011
Future Projection of Extreme Climate Events Over Different Homogenous Meteorological Regions of India: Insights from CMIP6 Multi-model Ensemble

Ravi KESHARWANI#+, Netrananda SAHU
University of Delhi

The simulation of extreme climatic events is very important to be able to understand and prepare for the potential impacts of climate change. By modelling the effects of extreme weather events such as heatwaves, floods, and droughts under different scenarios, we can better anticipate and mitigate their impact on infrastructure, agriculture, ecosystems, and human health. The study focuses on forecasting extreme climatic events in the homogenous meteorological regions (HMRs) of India using Global Climate Models (GCMs) from the CMIP6. The rainfall and temperature data are obtained from the India Meteorological Department (IMD). The spatiotemporal trend analysis of rainfall and temperature data has been analyzed using M-K Test, and Sen’s Slope Analysis. The GCMs are evaluated on their ability to estimate extreme events in the past, and the top-performing models are then employed to forecast extreme occurrences in future scenarios. The multi-model ensemble technique has been utilized for the near (2024-2050), middle (2051-2075), and far (2075-2100) future projections of extreme climatic events under different shared socioeconomic pathways 126 (SSP126), SSP245, SSP370, and SSP585 scenarios. The study concludes that in many parts of the study area, the CMIP6 predicts a rise in the frequency and intensity of extreme climate events, including heatwaves, droughts, and heavy precipitation events which can be incorporated into the planning for infrastructure and development of climate resilient strategies. The study underlines the need for action to mitigate the effects of catastrophic climate events on both natural and human systems.


HS25-A006
A Framework for Assessing the Impact of Climate Change, Water Management Practice and Land-use Change on Streamflow in a Highly Managed River Basin

Maochuan HU1#+, Takahiro SAYAMA2, Pingping LUO3, Bingjun LIU1, Xuezhi TAN1
1Sun Yat-sen University, 2Kyoto University, 3Chang’an University

The effects of climate change, water management practice, and land use change on the hydrological process are complicated, particularly in highly managed river basins. It is generally difficult to separate each factor in a basin without records of a non-interference period. In this study, a framework was developed to solve this issue based on hydrological simulation and water budget analysis. The current study demonstrated and used this framework to simulate the hydrological process and quantify the effects of each driving factor in two basins located in China and Japan, which have more than 50-year’s history of modern water management. The results indicate that the proposed framework is useful to distinguish the effects of climate change, water management practices and land-use change on streamflow. The results also provide useful information for local water resource management.


HS25-A013
AquaVar: DSS System for Surface and Groundwater Management

Lian Guey LER1, Philippe GOURBESVILLE2#, Guillaume MASSELIS3, Felix BILLAUD3, Hao-Ming HSU4, Mingyan WANG5+
1Eau d'Azur / University Cote d'Azur, 2Institute of Water Resources and Hydropower Research & University of Nice Sophia Antipolis, 3Eau d'Azur, 4University of Cote d Azur, 5Universite Cote d'Azur

AquaVar system is a DSS based on deterministic modeling tools that are capable of representing the full hydrological behavior of the Var catchment (about 3000 km2) located in the French Riviera. The architecture of the AquaVar system is based on the coupling of 3 models (hydrology, free surface flows and underground resources) that are operating in real time to produce a 3 days forecast of the conditions for all the 3 models. To ensure that the AquaVar system is able to produce the forecast in real-time efficiently, the computing architecture is run on a system consisting of 38 VCPUs and 128GB RAM and a GPU performance in the range of the NVIDIA A and V GPU series. Access to the AquaVar resources and forecasts is through a WEB service where the models’ results and field data can be access through a WEB GUI. This approach has demonstrated the efficiency of the high-performance solution and the interest to invest within deterministic approaches that were, up to now, not so frequently used within the DSS dedicated to the water management. This added value of the GPU approach is clear and represent a major axis for the development of DSS in the water management field.


HS25-A007
Modelling Strategy for Water Resources Management in a Karstic Catchment

Mingyan WANG#+, Philippe GOURBESVILLE, Paguedame GAME
Universite Cote d'Azur

Effective management of underground water resources is crucial for numerous coastal Mediterranean catchments that are frequently characterized by karstic conditions. The threats of the climate change with the evolution of spatial and temporal rainfall patterns combined with the competition among various uses related to urban development and tourisms request a fine tuning within the resources’ allocation and management. To achieve this complex task, a good knowledge of the hydrological processes within the catchment is deeply needed. The hydrogeological tool FEFLOW was used to model the groundwater system in the Cagne catchment and assess its response to different hydrological scenarios. The model was set up with a resolution of 5m in the river area and 100m in the other areas to provide a detailed representation of the hydrological processes involved, and 5 layers were created in the underground part based on geological data. The model was calibrated using data from the 2020 October to December event, which was chosen as a representative period of high groundwater recharge. The calibrated model was then validated using data from the 2021-2022 one-year event, which covered a full annual cycle of recharge and discharge. The results showed that the model was able to accurately predict the behaviour of the groundwater system in the Cagne catchment, both in terms of the distribution of water resources and the impact of changing hydrological conditions. Overall, this study provides a valuable contribution to the understanding of groundwater management in the Cagne catchment and demonstrates the potential of hydrogeological model as a decision-support tool for water resource managers. By providing a comprehensive and accurate representation of the groundwater system, this study can inform future management decisions and help to ensure the long-term sustainability of the region's water resources.


HS25-A005
Multi-objective Operation- Decision-making-risk Propagation Analysis for Cascade Reservoirs Affected by Future Streamflow Process Variations

Zhe YANG#+
Northwest A&F University

Significant climate variations have decreased the stability of water resource systems, leading to multiple uncertainties in streamflow response, reservoir operation optimization, decision-making, and adaptive adjustments for water resource scheduling. Understanding the impact of climate change on reginal streamflow is necessary and crucial to identifying reservoir operation strategies and decision-making responses. In this study, we created an integrated systematic “uncertain streamflow responses”– “reservoir operation”– “optimization”– “decision-making risk analysis” chain. Three bias-corrected and downscaled general circulation models (GCMs) were used to analyze the inter-model uncertainties under three representative concentration pathways (RCPs). The streamflow responses and uncertainty in the future were determined using a distributed hydrological model and the fuzzy extension principle under predefined scenarios and uncertainty levels. Then, a stochastic simulation model and modified stochastic multi-criteria decision-making model were applied to identify the effects of climate change projections and streamflow responses on reservoir multi-objective operation and decision-making. Moreover, risk quantification indices were used to determine the uncertainty propagation and potential risks accumulated in the chain. We applied this framework to cascade reservoirs in the Qing River Basin. The results indicate that the mean annual streamflow projected using selected GCMs will increase, enhancing the hydropower response and weakening the ecological benefit response. The Pareto non-dominated solutions optimized based on the streamflow projections obtained using the GCMs (under the same RCP) and hydrological model are more distinct than those based on different RCPs and the same GCM. Moreover, a high emission scenario may increase the uncertainty of the streamflow projections and reservoir operation responses, which is consistent with the finding that the decision-making process becomes more variable and sensitive with increasing streamflow uncertainty. Finally, we identified the preferred solutions for reservoir operation under different uncertainties, the respective expected values, and the 95% confidence interval bands to enhance the adaptability of future reservoir operation.


HS25-A001
Evolving Efficiency of Inter-basin Water Transfers in Regional Water Stress Alleviation

Kai DUAN#+
Sun Yat-sen University

Inter-basin water transfer (IBT) is widely used to mitigate water shortage at the cost of compromising water availability in water-exporting regions. However, it is unclear how the IBTs’ role evolves with the dynamic hydroclimatic and socioeconomic circumstances. Here, we report the efficiency of 50 active IBTs across the conterminous United States in alleviating regional water stress through the period of 1986-2015. The IBTs vastly reduced the coverage of highly stressed land area (8.7×104 km2) and population (4.3 million people). The widespread (74%-80% of the IBTs) increasing IBT efficiency suggest that regional water supply is increasingly dependent on water transfers in a drying climate. However, the complex combinations of changes in climate, water use behaviors in energy and food production, population, and transfer magnitudes have caused divergent changes in IBT efficiency, revealing the challenges posed by streamflow depletion and spatial migration of water demand. Adaptive management strategies from both water supply and demand aspects will be critical for planning and renewing these grand water infrastructures in a changing environment, and upland transfers should be dealt with particular caution for their uncertain and potentially amplified downstream influences.


Thu-03 Aug | 1:00 - 5:15 | Summit
HS - Hydrological Sciences Poster Session

HS01-A012
Uncertainty Analysis and High-resolution Prediction of Soil Moisture and Streamflow Using WRF-Hydro, PEST, and Deep Learning for Digital Twins

Bomi KIM+, Garim LEE, Sohyeon KIM, Yaewon LEE, Seong Jin NOH#
Kumoh National Institute of Technology, Korea, South

Reliable hydrologic modeling is a key to mitigate climate-related disasters in uncertain environments. However, it is widely known that hydrological models are subject to various uncertainties stemming from the input data, parameters, and model structure. As high-resolution is preferred and required in the era of digital twins and metaverse, challenges for calibrating hydrologic models with limited information are rather increasing. In this study, we will discuss challenges and solutions for sensitivity and uncertainty analysis to calibrate distributed hydrologic models with high-resolution land use and soil information using WRF-Hydro and PEST, model-independent parameter estimation. Then, we will discuss how deep learning approaches such as convolutional neural networks can be combined with physical modeling for high-resolution predictions with computational efficiency. The numerical experiments are conducted in the Kumho River basin in South Korea. The discussion will focus on the feasibility and limitations of the current physical and machine learning approaches for high-resolution digital twins.


HS01-A013
Multivariate Chaotic Analysis of Daily Runoff Series in Savitri River Basin, India

Namitha Elza SAJI1#+, V. JOTHIPRAKASH1, Bellie SIVAKUMAR1,2
1Indian Institute of Technology Bombay, India, 2Tsinghua University, China

The identification of the complexity of runoff is of great use in the water resources assessment and management in a region. It has more importance in today’s world, especially with the occurrence of more frequent and greater intensity of flood events due to climate change. The nonlinear dynamic approach can identify the nature of hydrologic variables with good accuracy. Although the single-variable phase space reconstruction approach has been found to yield useful results for characterization and prediction, more reliable outcomes can be achieved using multiple variables, if data are available. The present study aims to propose a multi-variable phase space reconstruction approach for chaos identification and prediction of daily runoff time series. Eight daily hydro-meteorologic variables namely runoff, rainfall, minimum temperature, maximum temperature, pan evaporation, relative humidity, sunshine duration, and wind speed collected for Savitri basin, India will be considered for phase space reconstruction. The influence of these variables on chaos identification will be investigated by applying False Nearest Neighbour (FNN) algorithm. The FNN is a dimension-based method that identifies the dimension. Here, hydro-meteorological variables observed during 2000–2011 at Birwadi station in the Savitri basin are used to develop the phase space. Initially, the complexity of hydrometeorological variables under consideration is identified individually. The daily hydro-meteorological variables at Birwadi are identified as low-dimensional chaotic systems with dimensions varying from 4 to 7. The phase space for the runoff series using the multivariate concept is reconstructed by using different combinations of runoff with rainfall, minimum temperature, maximum temperature, pan evaporation, relative humidity, sunshine duration, and wind speed.


HS01-A021
Integrated Modeling of Distributed Hydrological Model and 1D River Model on Nakdong River Basin

Hyeonseung KU1+, Hyunuk AN1#, Youngteck HUR2, Ahn JUNG MIN3
1Chungnam National University, Korea, South, 2K-water Institute, Korea, South, 3National Institute of Environmental Research , Korea, South

In the water system of South Korea, since several multi-function weirs have been built as a part of the four major river development projects, the water circulation has changed significantly. It has led to changes in quantity and water ecosystems and has had a significant impact on changes in water quality in rivers. Therefore, it is necessary to analyze and predict the quality and ecosystems of the river due to the influence of multi-functional weirs. In hydrological model, the routing analysis is usually performed by downstream traces such as kinematic waves by assuming a rectangular cross-section; therefore, reliable results cannot be obtained in large watersheds such as four major rivers where hydraulic structures are installed. To overcome this limitation, a distributed hydrology-hydraulic model, K-DRUM, and one-dimensional hydraulic river model, K-River, are integrated and applied on a Nakdong river basin in this study. The K-DRUM can perform detailed hydrologic analysis such as flow velocity, flow rate, and water level at any point in the basin by applying various physical characteristics. K-River can perform hydraulic analysis considering various hydraulic structures such as bridges, weirs. A series of water circulation processes were simulated by integrating K-DRUM and K-River to reflect weir operation. The model built through this study was compared and verified with the inflow amount for dam inflow points in the Nakdong River basin and the water level at several water level points in the mainstream of the Nakdong River for flood season in Repulic of Korea. As a result of the simulation, it was confirmed that the water level, the inflow, and the arrival time were successfully simulated at a meaningful level. This work was supported by the National Research Foundation of Korea (NRF) grant funded by the Korea government (MSIT) (No. 2021R1A2C200553012).


HS01-A023
Ensemble Streamflow Prediction Using Ensemble Meteorological Forecast and Dynamic Water Resources Assessment Tool (DWAT)

Jeonghyeon CHOI#+, Cheol Hee JANG, Deokhwan KIM, Hyeonjun KIM
Korea Institute of Civil Engineering and Building Technology, Korea, South

In Korea, weather and climate forecasts have mainly focused on meteorological and climatological aspects. However, it is necessary to prepare ways to utilize weather and climate forecasts that consider the spatial and temporal scale, accuracy, and evaluation scheme for short- and medium-term water resource assessment and analysis. This study predicted the streamflow for the Gyeongan Stream basin to prepare a method for future water resources assessment and analysis. To this end, we first applied the Dynamic Water resources Assessment Tool (DWAT) for the Gyeongan Stream basin, and calibrate it using daily observed rainfall, weather, and streamflow information from 2015 to 2021. A correlation analysis between global climate patterns and domestic meteorological characteristics was performed for the ensemble meteorological forecasts. After that, the climate indices that showed high correlations for each month were selected as predictors to construct the multiple regression model and the artificial neural network model for monthly rainfall and temperature forecasting for 2022. One thousand daily ensemble time series datasets were produced for meteorological stations that affect the targeted study area by downscaling the predicted monthly rainfall and temperature. The generated rainfall and temperature forecast information was used as input data for DWAT. The predicted daily streamflow differs from the one observed, which stems from errors in the predicted ensemble rainfall and temperature information. The result reaffirms the limitation that the error of the hydrologic model results is significantly affected by the error of forcing data sets. Therefore, it is necessary to consider analyzing monthly statistics by converting short- and mid-term water resources assessment and analysis into monthly streamflow. Acknowledgments: This work was supported by the Korea Environment Industry & Technology Institute (KEITI) through the Water Management Program for Drought Project, funded by the Korea Ministry of Environment (MOE), (2022003610002).


HS01-A024
Water Scarcity Risk Assessment in Four Major Basin Areas Using Dynamic Water Resources Assessment Tool

Deokhwan KIM1#+, Jeonghyeon CHOI1, Cheol Hee JANG1, Hyeonjun KIM1, Hyoungsub SHIN2
1Korea Institute of Civil Engineering and Building Technology, Korea, South, 2ERI Co., Korea, South

The complex water use system, such as the intake and drainage of river and groundwater, discharge of sewage and wastewater, and water reuse, significantly affects the availability of water resources in a catchment area during a drought. However, existing assessments for water resource availability during drought do not consider such a complex water usage arrangement, so it is difficult to predict water resource availability with high reliability. Therefore, it is necessary to develop a reliable technique to assess water scarcity risk and resource availability by investigating the interrelation between the detailed water use scheme and hydrological and environmental factors in watersheds during drought. This study used the Dynamic Water resources Assessment Tool (DWAT) to measure the water shortage risk and water resource availability during drought, reflecting the comprehensive water use system and hydrological and environmental factors within the basin area by simulating the four major medium-sized basins (Han River, Nakdong River, Geum River, and Yeongsan-Seomjin River). The results are expected to provide reliable evidence, such as primary data and software for preparing drought response measures. Acknowledgments: This work was supported by the Korea Environment Industry & Technology Institute (KEITI) through the Water Management Program for Drought Project, funded by the Korea Ministry of Environment (MOE), (2022003610002).


HS01-A025
Development and Global Extension of Dynamic Water Resources Assessment Tool (DWAT) Considering Interaction of Surface Water and Groundwater

Cheol Hee JANG#+, Hyeonjun KIM, Deokhwan KIM, Jeonghyeon CHOI
Korea Institute of Civil Engineering and Building Technology, Korea, South

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. In particular, DWAT is loaded with a module capable of simulating the runoff process of rice paddies, coupled with a snow-melting module that could reflect the hydrological characteristics of high latitudes and alpine regions, and a parameter optimization function. As of December 2022, WMO is pushing ahead with the "global Hydrological Status and Outlook System (HYDROSOS)" project, one of the major initiatives in the water resources sector. This project utilizes the global climate forecasts to perform the status assessment and outlook of natural streamflow at major points and consists of the following three modules: - A status module that collects and presents hydrological observation data, - A climate forecast module that collects global climate forecasts and converts them into the scale for the required basin, and - A hydrological forecasting module that converts climate forecasts into streamflow. The 18th WMO Congress held in June 2019 decided that DWAT would support the pilot project of HYDROSOS, a major initiative in the field of water resources. As a result, it is expected that Korea's water resource assessment technique will be continuously extended to WMO member countries with the utilization of DWAT. 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).


HS01-A040
Simulation of Precipitation Induced Flood Flow in Arid Region

Jennifer DUAN#+
University of Arizona, United States

In arid region, high-intensity and short duration monsoon rainfall can induce severe flash flood in the arid region. The HMS model developed by the US Army Corps Hydrologic Engineering Center has been widely applied in predicting precipitation induced flood flow. However, the traditional CN number approach was challenged by its original definition, and difficulty in taking account of various vegetation species and densities. The CN values were available from the tables in National Engineering Handbook Section 4: Hydrology (NEH-4) are based on two factors: one is the hydrologic soil group, and the other is land use and land cover including the type of landuse, and the type and density of vegetation cover. These CN values were obtained primarily from the small rain-fed agricultural watersheds. The CN method works well for the agricultural watersheds, but it’s less successful for the arid and semi-arid regions where vegetation is typically sparsely distributed with desert shrubs and perennial grass at low elevation, but forest at the higher elevation. The unique vegetation types and spatial distributions limit the applicability of the original CN table (Table 2-2d in TR-55) in the arid and semi-arid region. This paper reports an application of HEC-HMS model to simulate flash flood and sediment transport in an arid watershed in the southern Arizona. The model was used to simulate several largest precipitation events observed from 1970 to 2015. This paper discusses various methods for simulating the rainfall loss, surface and channel flow routing, and soil erosion. Results showed HEC-HMS model can achieve a high accuracy of flow and sediment yield prediction. The threshold value for watershed delineation is critical for HEC-HMS model to converge to accurate results.


HS02-A008
Development of a Surrogate Model to Improve the Efficiency of Groundwater Level Fluctuation Pattern-based Hydrologic Properties Evaluation

Jiho JEONG+, Jina JEONG#
Kyungpook National University, Korea, South

In this study, a method of aquifer hydrologic property estimation incorporating the deep learning method was developed to improve the estimation efficiency of a process-based model based on groundwater level fluctuation (GLF) patterns. As a reference study, a data-driven method suggested by Jeong et al. (2020) was considered; the uncertainty of the GLF patterns resulting from different yearly patterns of precipitation, which were considered as noise in the previous study, was effectively discarded using the newly proposed method of applying the conditional variational autoencoder (CVAE). The CVAE was used to acquire the specific GLF patterns under certain identical precipitation patterns for all the monitoring stations. The data-driven hydrologic property estimation model was developed to predict two hydrologic parameters ( and ) of the process-based model using the generated GLF patterns from the CVAE network as the input variables. The actual GLF and precipitation data that were acquired from nationwide groundwater monitoring stations in South Korea were applied to validate the developed method. It was found that the estimated and target hydrologic properties were highly correlated (correlation coefficients [CC]: 0.9833 and 0.9589 for and, respectively), which significantly improved the results when compared to the previous study (CC: 0.7207 and 0.8663 for and, respectively). Consequently, the developed model can contribute to a more accurate hydrologic property estimation of aquifers. Additionally, it can facilitate efficient groundwater development planning since the manual fitting of the process-based model by an expert is not required.


HS02-A009
Investigation of Influencing Factors of Acoustic Attenuation in the Atmosphere

Linhao FAN#+, Ji CHEN
The University of Hong Kong, Hong Kong SAR

With more research on new artificial rainfall technology in recent years, the concept of guiding the re-distribution of cloud water resources through acoustic waves has begun to gain more attention. Therefore, it is essential to study how acoustic waves attenuate and finally affect the layers of precipitation clouds. However, research on actual atmospheric acoustic attenuation in the outdoor field is not particularly extensive because of the high operating expenses, high requirements of equipment and energy consumption, and complicated environmental environment. Here, we design various case studies based on the existing typical theory of acoustic wave propagation to investigate the main characteristic parameters of the atmospheric acoustic attenuation. To promote the transmission efficiency of acoustic intensity more economically, we choose three characteristic frequencies to evaluate the optimized design of a multi-acoustic source combination layout. This study is of guiding significance for the efficiency improvement of future implementations of the emerging technology of acoustic-induced precipitation.


HS03-A001
Impacts of Meridional Wind and Water Vapor Flux on Regional Long-term and Short-term Precipitation Over Yarlung Zangbo River Basin

Xinzheng TANG#+, Ji CHEN, Dawei WANG
The University of Hong Kong, Hong Kong SAR

The Tibetan Plateau (TP), the third pole of the Earth, is the highest land in the world. Yarlung Zangbo river (YR) basin, located in the southern TP, is the world's highest great river, providing water resources for more than billions of people through several large Asian rivers. Under the control of the interaction between the westerlies and the Indian Summer Monsoon (ISM), the YR basin has undergone significant surface warming during the past five decades. ISM has exported huge atmospheric water vapor to TP, which experienced a weakening trend during the same period. However, to what extent the ISM influences the local precipitation in the YR basin remains uncertain. In this context, it is significant to investigate the regional climate change over the YR basin and the relationship between precipitation here and ISM. In this study, we conduct both long-term climate and short-term weather simulations using the Weather Research Forecasting model to quantify the impacts of the meridional wind on regional precipitation. Besides, we investigate the net water vapor input into three YR basin reaches through four boundaries to reveal the source of the precipitation. The results indicate the critical role of the meridional wind in the precipitation amount and location over the YR basin, especially in the lower reaches. The study would provide a unique insight for climate research and contribute to understanding the precipitation evolution over the TP.


HS03-A005
The Performance of CMIP6 Surface Water and Energy Balance Predictions and its Influence in Pan Third Pole

Zhu LIU#+, Bohan HUANG, Su LIU, Tao SU, Qingyun DUAN
Hohai University, China

The Pan Third Pole (PTP) contains Tibet Plateau and its surrounding regions such as Hindu Kush, Karakoram and Pamirs and it is one of the highest and most fragile as well as rapidly developing regions of the Earth. The water balance and energy balance not only regulate the fundamental water supply and demand as well as thermal conditions on earth but also control various atmosphere and land surface processes. In this study, predictions of water balance components including precipitation, evapotranspiration, runoff and surface energy balance components including net radiation, latent heat and sensible heat from 20 CMIP6 models are evaluated with ERA5 reanalysis data during 1981-2014 over PTP region and its three subregions. Specifically, the annual and seasonal relative bias of different components as well as water and energy imbalance are evaluated. Besides, considering the significantly large difference of CMIP6 multi-year mean air temperature predictions over Tibet Plateau, we investigate its influence on snow depth, frozen soil and runoff predictions. Results show that the spatial patterns of relative bias of water and energy components are quite different among models and significant bias exist for seasonal model predictions. Runoff has relative larger bias compared with precipitation and evapotranspiration for PTP region. Additionally, CMCC-HR4, CMCC-SR5 and CMCC-ESM2 have significant water imbalance because of runoff overestimation and water and energy imbalance are not negligible for seasonal predictions in PTP. The snow depth predictions are not always consistent with temperature bias. CNRM-ESM2-1 overestimates snow depth to 25m with its temperature only underestimated about 3.5 degree Celsius, which might be related to the maximum snow depth restrictions of model structure.


HS03-A008
Spatial and Temporal Analysis of Precipitation Extremities of Eastern Nepal in the Last Two Decades (1997–2016)

Sunil SUBBA1#+, Yaoming MA2, Weiqiang MA2
1University of Chinese Academy of Sciences, China, 2Chinese Academy of Sciences, China

In recent days there have been discussions regarding the impact of climate change and its vagaries of the weather, particularly concerning extreme events. Nepal, being a mountainous country, is more susceptible to precipitation extreme events and related hazards which hinders the socio-economic development of the nation. In this regard, this study aimed to address this phenomenon for one of the most naturally and socio-economically important regions of Nepal, namely, Eastern Nepal. The data were collected for the period of 1997 to 2016. The inter-decadal comparison for two periods (1997–2006 and 2007–2016) was maintained for the calculation of extreme precipitation indices as per recommended by Expert Team on Climate Change Detection and Indices (ETCCDI). Linear trends were calculated by using Mann-Kendall and Sen’s Slope estimator. The average annual precipitation was found to be decreasing at an alarming rate of -20 mm/year in the last two decades’ tenure. In case of extreme precipitation events, Consecutive Dry Days (CDD), one of the frequency indices, showed a solo increase in its trend (mostly significant). Meanwhile, all the intensity indices of extreme precipitation showed decreasing trends (mostly insignificant). Thus, it can be concluded that Eastern Nepal has witnessed some significant drier days in the last two decades, as the events of heavy, very heavy, extremely heavy precipitation events, and annual wet day precipitation (PRCPTOT) were found to be decreasing. The same phenomena were also seen in the Tropical Rainfall Measuring Mission (TRMM) 3B42 V7 satellite precipitation product for whole Nepal.


HS03-A009
Variation of Surface Air Temperature Induced by Enhanced Land–atmosphere Coupling During 1981−2020 in Xinjiang, Northwest China

Yang YANG1+, Zhaohui LIN2, Lifeng LUO3, Linhao ZHONG1, Dabang JIANG2#
1National Institute of Natural Hazards, Ministry of Emergency Management of China, China, 2Chinese Academy of Sciences, China, 3Michigan State University, United States

Land–atmosphere coupling (LAC) is a critical process in the climate system and has great effects on surface air temperature over the humid–dry transition zones. Using ERA5/ERA5-land reanalysis data, we show that summer temperature anomalies over Northwest China (NWC), known as one of the most important LAC hotpots in China, are significantly correlated with the LAC strength during 1981−2020. The stronger the coupling strength between air temperature and land surface, the more pronounced decrease in air temperature and extreme hot days over NWC. Among different pathways of LAC processes, soil moisture–latent heat flux–air temperature pathway contributes the most to the overall temperature changes in summer (> 30−40%). By analyzing the possible local and non-local physical links in this relationship, we show that wave-trains from Arctic Oscillation–East Atlantic/West Russia-like circulation patterns stimulate a meridional fluctuation of westerly airflow over mid-high latitudes of Eurasia, manifested by the intensification of Ural ridge and Central–Asia trough. Large moisture, therefore, converges into NWC, leading to excessive precipitation and deficient incident solar radiation reaching the land surface. In such cases, wetter and cooler soil states accelerate the cooling of the environment through a series of feedbacks between lands, land–atmosphere exchanging fluxes, and air temperature locally, significantly enhancing the LAC strength. Our study provides insight into the physical processes causing variations in summer temperature over a typical LAC hotspot and suggests that the role of land surface–atmosphere interactions need to be considered when studying temperature extremes under climate change.


HS03-A014
Implementation of the Calculating Soil Freezing and Thawing Fronts Parameterization in the Earth System Model CAS-ESM

Ruichao LI#+, Zhenghui XIE
Chinese Academy of Sciences, China

Permafrost and seasonally frozen ground are an important part of the cryosphere. it is widely distributed and the cycle of freezing and thawing of frozen ground has important influence on energy and water exchanges between the land surface and the atmosphere. In this study, the calculating soil freezing and thawing fronts parameterization was implemented into the earth system model of Chinese Academy of Sciences (CAS-ESM) and its land component the Common Land Model (CoLM) to investigate dynamic change of soil freezing and thawing fronts and the effects of soil freezing and thawing fronts on soil temperature and soil moisture. Our results showed that the developed models could reproduce the soil freezing and thawing process and the dynamic change of soil freezing and thawing fronts. We also evaluated the effects of soil freezing and thawing fronts on soil temperature and soil moisture. These results would be constructive to a better understanding of the freeze and thaw cycle process.


HS03-A016
The GEWEX Regional Hydroclimate Activities in Asia

Petrus (Peter) VAN OEVELEN#+
George Mason University, United States

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.


HS03-A029
The Impacts of Third Pole Snow Assimilation on Seasonal Meteorology Predictions

Lu LI1#+, Wei LI2, Jie CHEN2, Yvan ORSOLINI3, Retish SENAN4, Patricia DE ROSNAY4
1NORCE Norwegian Research Center, Norway, 2Wuhan University, China, 3Norwegian Institute for Air Research, Norway, 4European Centre for Medium-Range Weather Forecasts, United Kingdom

The Third Pole (TP) contains the largest amount of snow outside the Antarctic and Arctic regions, and is the source of many major rivers in Asia. An accurate seasonal hydrometeorological forecast is of great importance for this region. The fifth-generation seasonal forecast system of the European Centre for Medium-Range Weather Forecasts (SEAS5) provides global long-range meteorological forecasts including over the TP. However, SEAS5 uses land initial conditions produced by assimilating Interactive Multi-sensor Snow and Ice Mapping System (IMS) snow data only below 1500 m altitude, which may affect the forecast skill of SEAS5 over mountainous regions like the TP. In this study, we used twin ensemble reforecasts, which are initialized with and without snow assimilation above 1500 m altitude over the TP for spring and summer 2018, to investigate the impacts of snow assimilation on the forecasts of meteorological variables (e.g., snow, temperature, precipitation, and streamflow). We found that significant changes occur in the springtime. The reforecasts, which is without snow assimilation, overestimate snow cover and snow depth while underestimating daily temperature. Precipitation reforecasts perform better in the west TP than in the east TP compared with satellite-based data. Besides, the snow assimilated reforecasts of snow cover, snow depth and temperature are improved in the spring over TP. The snow assimilation experiment significantly increases temperature and precipitation for the east TP comparing with that of experiment without snow assimilation. The higher temperature after snow assimilation, in particular the cold bias reduction after initialization, can be attributed to the effects of a more realistic, decreased snowpack, providing favourable conditions for generating more precipitation. Overall, snow assimilation can improve seasonal forecasts through the interaction between land and atmosphere.


HS04-A003
Flow Characteristics of the Hornad River and the Anthropogenic Impact of the Ruzin Dam

Maria HLINKOVA#+, Martina ZELENAKOVA
Technical University of Kosice, Slovakia (Slovak Republic)

The aim of the study is to analyse the seasonal and term variability of the flow of the Hornad River. The annual RBI and Cv values ​​show an even distribution of values ​​over the analysed period 1973–2020 at the hydrological stations Spisska Nova Ves and Margecany. Higher annual amplitudes of RBI values ​​were recorded at the Kysak post below the Ruzin II water reservoir, while lower amplitudes of RBI values ​​at the posts located above the reservoir. The analysis of monthly mean RBI values ​​showed that in the period from 1973–2020 the RBI values ​​ranged from 0 to 0.49 at the hydrological stations Spisska Nova Ves and Margecany, while at the Kysak station, the RBI indicator ranged from 0 to 0.57, which indicated large changes in short-term flows. The maximum value of the RBI index occurred in June 1973 (0.57) at the Kysak station and in July 2008 (0.49) at the Margecany station (0.49) and the Spisska Nova Ves station (0.48), which was the result of very high precipitation (over 170 mm in a month). The correlation coefficient r between the RBI index and the monthly sum of rainfall shows that the highest correlation was in October, November, and December (r> 0.8) at the hydrological stations Spisska Nova Ves and Margecany, while at the Kysak hydro-logical station the highest value of r was recorded in October (r = 0.73). The lowest r values were recorded in February and March at all stations, and they ranged from 0.28 to 0.39 and were related to thaws, which could cause fluctuations in flows. The possibilities of water retention in the Ruzin reservoir are limited, which is visible in the case of very high precipitation.


HS04-A004
Using Integrated Flow Modeling to Understand Complex River-aquifer-sea Interactions in the Guangdong-Hong Kong-Macao Greater Bay Area

Xiaoli WANG+, Ji CHEN#
The University of Hong Kong, Hong Kong SAR

Hydrological processes in mega deltas are generally complex due to river-aquifer-sea interactions, especially under the joint influences of intensifying climate change and human activities. Systematic and quantitative understanding of the river-aquifer-sea interactions and their response to natural and anthropogenic disturbances is a prerequisite for the effective management of water resources and ecosystem health. In this study, we developed a high-resolution integrated hydrological model for the Guangdong-Hong Kong-Macao Greater Bay Area, one of the four largest city-clusters in the world with dense population and intensive socioeconomic development. The study was intended to quantify the watershed hydrological cycle and land-ocean interactions to support sustainable water management in the region. After being calibrated and cross-checked based on observations at gauging stations and independent remote-sensing products, the flow model was used to explore the influences of inland and ocean processes on river-aquifer-sea interactions at different time scales. The pivotal role of ocean tides in shaping the coastal groundwater system was closely examined and analyzed. Moreover, the total flux of the fresh submarine groundwater discharge of the terrestrial source was computed by the flow model, together with its spatial and temporal variations.


HS04-A007
Calibrate Tropical Forest Coexistence in Ecosystem Demography Models Using Multi-objective Optimization

Yanyan CHENG#+, Christine SHOEMAKER
National University of Singapore, Singapore

Tropical forest diversity governs forest structures and compositions and consequently responses and feedbacks of tropical forests to environmental changes. Better representation of forest diversity in ecosystem demography (ED) models within Earth system models is thus necessary to accurately capture and project how tropical forests affect Earth system dynamics subject to climate changes. However, achieving forest coexistence in ED models is still an ongoing research challenge. This study applies an advanced Multi-Objective Population-based Parallel Local Surrogate-assisted search (MOPLS) optimization algorithm to simultaneously calibrate ecosystem fluxes and coexistence for two physiologically-distinct tropical forest species in a size- and age-structured ED model with realistic representation of wood harvest. MOPLS exhibits satisfactory model performance in capturing hydrological and biogeochemical dynamics (both calibrated and non-calibrated variables) that observed in Barro Colorado Island, Panama, as well as robustly achieves coexistence for the two representative tree species. Given the same ensemble size, MOPLS results in much more simulations with stable coexistence than a random sampling strategy, demonstrating its effectiveness in calibrating coexistence for tropical trees. The optimal solution is applied to investigate the recovery trajectories of forest biomass after various intensities of clear-cut deforestation. We find that a 20% selective logging can take approximately 40 years for aboveground biomass to return to the initial level, due to the slow recovery rate of late successional trees. This study lays the foundation to calibrate coexistence in ED models. MOPLS can be an effective tool to help better represent tropical forest diversity in ESMs and guide forest management practices.


HS04-A009
Habitat Suitability Analysis Considering Low-flow and High-flow Periods – A Case Study in Shuangxi River of Taiwan

Kwan Tun LEE#+, Huan-Yuan CHEN, Cho-Min YANG, Jing-Zong YANG, Nai-Kuang CHEN, Ta-Chun CHIEH, Pin-Chun HUANG, Yu-Han HSU, Yu-Hsun LIAO, Yi-Ting LIN, Ching-Wen HSU, Chiao-Ju LEE, Han-Chung LIN, Kuo-Feng TSENG
National Taiwan Ocean University, Taiwan

This research analyzes the physical characteristics of the habitat in the Shuangxi River Basin of Taiwan. Due to the lack of flow records in the study watershed, geomorphologically-based models suitable for ungauged watershed analysis were developed for hydrological analysis. In-site water level and flow velocity measurements were used to calibrate the parameters of the hydrological models. Using the aforementioned hydrological analysis results and substituting them into a two-dimensional hydraulic model, we can simulate the spatial distribution of water depth and flow velocity in the study channel reach. Acrossocheilus paradoxus and Candidia barbata were selected as the target fishes for habitat evaluation. Two specified flow values, the low and the high flows, were chosen to assess the habitat suitability. The low flow (Q95%) indicates 95 percent time flow equaled or exceeded the flow value, and the high flow indicates a flood corresponding to the 5-yr return period flow (Q5) condition. Considering the low-flow period, a minimum required water depth of 15 cm was set for the target fishes to assess the habitat suitability. The result shows that the upstream inflow of Q95% can provide continuous water paths for the movement and survival of the target fishes. A fish-preferred-swimming path can then be delineated in the study channel reach during the low-flow period. In considering high flow velocity during the flood period, the prolonged-swimming speeds of the target fishes were used to assess the habitat suitability. The result shows that the low-velocity areas, where suitable for the target fish, were only 11.16% in the channel reach and mainly distributed in the riparian areas near the river bank. Therefore, the shoal areas can provide safe habitats to avoid fish being washed downstream during the flood.


HS04-A014
Changes of River Channel and Habitat Conditions by Vegetation Density

Mikyoung CHOI1#+, Hyunuk AN1, Chang Lae JANG2
1Chungnam National University, Korea, South, 2Korea National University of Transportation, Korea, South

Reduction of sediment flow and control of flow rate due to dam operation accelerates vegetation growth and succession, and then these vegetation affect changes in riverbed and biological habitats. In this study, we simulate how the vegetation affects river channel change using a numerical model (Nays2D), and try to identify fish habitat changes using the physical habtiat suitability Model (PHABSIM). Nays2D model was conducted according to 8 scenario by 2 types of flow (dam outflow, 2-year frequency flow rate) and 4 types of vegetation density (no vegetation, current vegetation density, density decrease, density increase) for 2 km the Geum River in Korea. The result of riverbed change (elevation, water depth and velocity) simulated by Nays2D were used as input data for PHABSIM model. The target fish species is Zacco platypus, and the Weighted Usable Area (WUA) for each scenario was calculated and analyzed. As a result, WUA value was the highest when the riverbed change not reflecting the vegetation, and the WUA value was the lowest riverbed change with increased vegetation density both of 2 flow conditions. This work was supported by the National Research Foundation of Korea (NRF) grant funded by the Korea government (MSIT) (No. 2021R1A2C200553012) and Korea Environment Industry & Technology Institute(KEITI) through the Water Management Project for Drought, funded by Korea Ministry of Environment(MOE) (2022003610004)


HS04-A016
Exploring the Effects of Environmental Factors on Macroinvertebrates in Mountainous Rivers: Lai Chi Wo River in Hong Kong, China

Zhaofeng HAN1#+, Ji CHEN2, Yi LU3,2, Qian XU2
1THE UNIVERSITY OF HONG KONG, Hong Kong SAR, 2The University of Hong Kong, Hong Kong SAR, 3Hong Kong Chu Hai College, Hong Kong SAR

Rivers have always been the foundation of human survival and development, and an important source of fresh water and food. However, with the rapid economic development, the pressure on the river system have increased dramatically, threatening and deteriorating the environmental and ecological conditions. Society needs to clarify the various interactions among water movement, pollutant transport, and biological organisms in aquatic environment to protect and restore riverine ecologies. According to the research focus, this study explores the interrelationships between macroinvertebrates and environmental factors with structural equation modeling. This study indicated that PLS-SEM would provide more precise understanding of the direct and indirect effects of environmental factors on macroinvertebrates than linear fitting and principal component analysis methods.


HS04-A018
Comprehensive Analysis of Flow Characteristics in Stepped Fishway with Experimental and Numerical Approaches

Chanjin JEONG1+, Hyung-Ju YOO1, Hyungsuk KIM2, Seungoh LEE1#
1Hongik University, Korea, South, 2Kunsan National University, Korea, South

General purpose of fishway in streams is to minimize the negative impact of the river ecosystem due to streamwise discontinuation induced by transversal structures such as barriers, weirs and dams. When constructing a fishway, the ecological characteristics of the fish community such as the ascending capacity of migratory fish should be considered. Therefore, it is necessary to know the hydraulic characteristics near a fishway whether it works properly or not for fish passing. The maximum flow velocity within the fishway should be less than possible swimming speed of a fish at each step, and the flow characteristics within the fishway could be appropriate for the easy and safe ascending. In this study, the flow characteristics near a stepped fishway were measured using the LDV(Laser Doppler Velocimeter). In the hydraulic experiment, the velocity fields at the downstream for each step were measured and turbulent productions were calculated. Experimental results using LDV were also compared with those calculated with FLOW-3D, a three-dimensional numerical model. A total of four turbulence models, (k-epsilon), renormalized group (RNG), (k-omega), and large eddy simulation (LES), inside the FLOW-3D were used to select the most suitable turbulence model for a stepped fishway. In addition, the results of this study are expected to contribute as fundamental data for the fishway design to archive its purpose considering flow characteristics.


HS04-A019
Annual Precipitation Explains Variability in Dryland Vegetation Greenness Globally But Not Locally

Anna UKKOLA1#+, Martin DE KAUWE2, Michael RODERICK3, Arden BURRELL4, Peter LEHMANN5, Andy PITMAN1
1UNSW Sydney, Australia, 2University of Bristol, United Kingdom, 3The Australian National University, Australia, 4Woodwell Climate Research Center, United States, 5ETH Zurich, Switzerland

Dryland vegetation productivity is strongly modulated by water availability. As precipitation patterns and variability are altered by climate change, there is a pressing need to better understand vegetation responses to precipitation variability in these ecologically fragile regions. We present a global analysis of dryland sensitivity to annual precipitation variations using long-term records of Normalised Difference Vegetation Index (NDVI). We show that while precipitation largely explains spatial gradients in NDVI across dryland regions, precipitation only accounts for <26% of temporal NDVI variability over most dryland regions. This suggests that drylands are highly resistant to annual precipitation variability despite water availability playing a major role in determining vegetation greenness across dryland regions. Earth system models (ESMs) from the latest Coupled Model Intercomparison Project overestimate the observed vegetation sensitivity to precipitation variability up to three-fold, particularly during dry years. With projections of increasing meteorological drought, ESMs are likely to overestimate the impacts of future drought on dryland vegetation with observations suggesting that dryland vegetation is more resistant to increasing precipitation variations than ESMs project.


HS04-A023
Identification of a Function to Fit the Flow Duration Curve and Parameterization of a Semi-arid Region in North China

Dengfeng LIU1#, Lan MA1+, Qiang HUANG1, Fengnian GUO1, Xudong ZHENG1, 静 赵2, Jinkai LUAN3, Jingjing FAN4, Guanghui MING5
1Xi'an University of Technology, China, 2西安理工大学, China, 3Chinese Academy of Sciences, China, 4Hebei University of Engineering, China, 5Yellow River Engineering Consulting Co., Ltd., China

The discharge process has undergone major changes in many river basins throughout the world as a result of the simultaneous influences of global climate change and human activity. Flow duration curves (FDCs) are crucial indicators of river basin's hydrological processes. However, it is challenging to compare FDCs in a quantitative way. This study will identify the best function with which to fit the flow duration curve in a semi-arid region of North China, so as to quantify the FDC, and parameterize the function of the FDC of the region in order to describe the FDCs of ungauged basins. In this work, six small- and medium-sized catchments in North China are selected as the study area, and three functions, i.e., Log Normal, Generalized Pareto and H2018 function, were chosen to fit the FDC at nineteen hydrological stations. The relationship between the parameters of the FDC and the basin characteristics, such as the climatic factor and geographical features, were analyzed. A regression formula of the parameters of the FDC function was established, and its spatial and temporal distributions were examined. Based on the evaluation of four indicators, the Nash-Sutcliffe efficiency, the root mean square relative error, the Logarithmic Nash efficiency coefficient and the coefficient of determination, the results demonstrate that the H2018 function can match FDCs the best. Through the annual runoff, annual precipitation, precipitation in summer, potential evapotranspiration, catchment area, mean elevation, length of the main channel and maximum flow frequency, the parameters of a, b, and k in the H2018 function can be formulated. The regression formula constructed in this study can obtain a regional flow duration curve with satisfactory performance, which provides a reference for the validation of remote sensing based runoff data in ungauged regions.


HS04-A024
Soil Hydraulic Parameters Inversion Based on HYDRUS-2D Model

Xinmei HAO#+
China Agricultural University, China

Although many studies have been conducted to investigate soil water movement parameters by the inversion of the HYDRUS model, studies on the spatial and temporal variability of soil hydraulic parameters on an agricultural land, especially under intensive irrigation, are still lacking. In this study, soil hydrological parameters at different depths at different growth stages were estimated using HYDRUS-2D model inversion based on soil water content data measured in a vineyard. The performance of the estimated parameters in predicting soil water content for an independent validation period were evaluated, and the temporal variability of those parameters were analyzed. The results showed that the parameters from the inversion performed better than the predicted parameters of Rosetta model for most cases. The inversion simulations were best in the split layer case during fruit expansion and color change without irrigation. Soil hydraulic parameters from the inversion were only applicable to predicting soil water content under similar conditions as used in the inversion, and the simulation accuracy became significantly lower when the conditions varied greatly with the conditions for the inversion. The three parameters Ks, α, and n derived from the inversion showed spatial and temporal variability with different magnitudes, with Ks and n showing smaller spatial and temporal variability, and α having the largest spatial and temporal variability. The results of the study are of great scientific significance for accurately predicting the variability of soil water content in agricultural fields, so as to develop reasonable irrigation schemes and improve water use efficiency in the areas.


HS07-A006
Global-scale Interpretable Reconstruction of Compound Drought and Heatwaves Utilizing Anomalies of Atmospheric Dynamics

Zhenchen LIU#+, Wen ZHOU
Fudan University, China

Droughts and associated near-surface temperature anomalies can be attributed to amplified vertical subsidence and anomalous anticyclonic circulations from dynamic perspectives. However, two open and interesting issues remain unknown: 1) whether hydrometeorological situations under droughts can be reproduced directly utilizing variability of atmospheric dynamics, and 2) what specific roles atmospheric dynamics play in drought reconstruction. To explore them, this study employs three kinds of dynamical features (i.e., vertical velocity, relative vorticity, and horizontal divergence) for hydrometeorological reconstruction (e.g., soil moisture, and evaporation) under drought situations through an ensemble learning method. Regarding the 2010 European summer mega hot drought and 2015/2016 tropical South America hot drought, reconstruction of spatial patterns and intensities on the interannual scale performs relatively well, seemingly regardless of seasonality and drought-inducing mechanisms. More importantly, from interpretable perspectives, global-scale analysis on dynamical contributions help discover unexpected dynamically drought-inducing roles and associated latitudinal modulation. That is, low-level cyclonic/anticyclonic anomalies contribute to drought development in the northern middle and high latitudes, while upper-level vertical subsidence contributes a lot to tropical near-surface temperature anomalies concurrent with droughts. These achievements could provide potential guidance for conceptual models of drought monitoring and prediction in different geographic regions. The DOI-based linkage is https://doi.org/10.1175/JHM-D-22-0006.1.


HS07-A008
Development of the China Meteorological Administration Land Surface Data Assimilation System (CLDAS-Prcp) Multi-source Precipitation Fusion Dataset and Its Evaluation of Soil Moisture and Snow Simulation Effects

Shuai SUN1+, Chunxiang SHI2#, Shuai HAN2, Junxia GU2, Bin XU2
1National Meteorological Information Center, China, 2China Meteorological Administration, China

Precipitation plays a role in climate change, agricultural development, water use and management. Howerver, there are no long-term, high spatiotemporal resolution, high-quality precipitation datasets in China. To address these issues, in the China Meteorological Administration (CMA) Land Data Assimilation System (CLDAS), we blended the Climate Prediction Center (CPC) morphing technique (CMORPH) and Modern-Era Retrospective analysis for Research and Applications version 2 (MERRA2) precipitation datasets with more than 60,000 CMA precipitation in-situ data using multigrid variational analysis and temporal downscaling to produce a multi-source precipitation fusion dataset for China (CLDAS-Prcp). This dataset covers all of China at a resolution of 6.25 km at hourly intervals from 1998 to 2022. We evaluated the CLDAS-Prcp dataset using CMA and Ministry of Water Resources (MWR) precipitation in-situ data separately. Our results show that the CLDAS-Prcp dataset represents reasonably the spatial distribution of precipitation in China. Using the CMA stations to evaluate CLDAS-Prcp indicates that the CLDAS-Prcp performs better than the MERRA2 precipitation, CMORPH precipitation, GLDAS-V2.1 precipitation, and CLDAS-V2.0 winter precipitation, as compared to the meteorological observational precipitation. Using the MWR stations to evaluate CLDAS-Prcp indicates that the CLDAS-Prcp dataset performs better than the IMERGE precipitation dataset and is similar to the CLDAS-V2.0 summer precipitation dataset. To further validate the simulation effect of CLDAS in soil moisture and snow depth, we used CLDAS-Prcp as well as CLDAS temperature, pressure, humidity, wind, and solar radiation to drive the Noah-MP land surface model for the simulation of soil moisture and snow depth in China. The results showed that the simulated soil moisture and snow depth driven by CLDAS-Prcp are better than the GLDAS-2.1 soil moisture and snow depth. Overall, the CLDAS-Prcp can meet the needs of the land surface models and hydrological research in China.


HS07-A009
Increasing Global Precipitation Whiplash Due to Anthropogenic Greenhouse Gas Emissions

Xinxin WU+, Xuezhi TAN#
Sun Yat-sen University, China

Precipitation whiplash including abrupt shifts between wet and dry extremes can cause large adverse impacts to human and natural systems. Observed and projected changes in occurrences of sub-seasonal precipitation whiplash remain not quantified, and response of precipitation whiplash to anthropogenic forcings remains unknown. We detect historical and projected future changes in whiplash and investigate the role of individual anthropogenic influences on these changes. Results show that the occurrence frequency of global (land) precipitation whiplash is expected to be 2.6 (3.5) times higher than that in the current period by the end of the 21st Century, with increasingly rapid and intense transitions between the two extremes. The most dramatic increases of whiplash show in the polar and monsoon regions. Changes in precipitation whiplash are concurrent with changes in precipitation totals with a much greater rate of change. Anthropogenic greenhouse gas (GHG) and aerosol (AER) emissions have increased and decreased precipitation whiplash, respectively. Anthropogenic GHG emissions are projected to increase ~40% occurrences of precipitation whiplash (mean of dry-to-wet and wet-to-dry extremes), given GHG are projected to sharply outpace of AER after the 2020s. The precipitation whiplash between dry and wet extremes is driven by shifts in circulation patterns conducive to precipitation extremes. Changes in precipitation regimes and circulation patterns will potentially challenge the current actions to water resources management and disaster prevention.


HS07-A014
Increased Risk of Compound Flood-heat Extremes in a Warming Climate

Jun ZHOU1+, Chuanhao WU1#, Pat YEH2, Jiali JU3, Lulu ZHONG1, Saisai WANG1, Junlong ZHANG4
1Jinan University, China, 2Monash University, Malaysia, 3China University of Geosciences, China, 4Shandong Normal University, China

Compound flood-heat extreme (CFHE) is a successive extreme event that threatens human health, economy, and building environment security that has attracted extensive research attention recently. However, the risk of global CFHE in a warming climate is unclear given the large uncertainties in climate change projections. Here, we present a global-scale evaluation of the projected changes and uncertainty in CFHE characteristics within the ISIMIP 2b framework based on the multi-model ensemble of 20 members (5 global water models × 4 global climate models) under two representative concentration pathway (RCP) scenarios (RCP2.6 and RCP6.0). The results show that CFHE frequency is projected to increase nearly globally especially in tropical (e.g., north South America, central Africa, and southeast Asia), and some temperate (e.g., eastern and southern Asia) regions. Furthermore, the higher projected CFHE frequency is generally accompanied by larger model uncertainty. Relative to the 1970-1999 baseline period, the CFHE land exposure is expected to increase by 10% (20%) by the end of this century under RCP2.6 (RCP6.0). The interval between flood and heatwave in CFHE tends to decrease (by up to 3 days) in most global regions under both RCPs, implying more intermittent CFHE occurrence under future warming. Attribution analyses suggest that the change of flood frequency contributes more to the change of CFHE frequency than that of heatwave in most global regions.


HS07-A016
Projecting Spatial and Temporal Changes of Rainfall Events Using CMIP6 Scenarios in Ca River Basin, Vietnam

Ju-Young SHIN1, Pham Van CHIEN2, Vo Cong HOANG2, YeonJi CHUNG3+, Myoung-Jin UM3#
1Kookmin University, Korea, South, 2Thuyloi University, Viet Nam, 3Kyonggi University, Korea, South

Climate change is causing significant change in the intensity, frequency and amount of rainfall in Vietnam. To attenuate the adverse effects of the rainfall changes on people’s life, the future projection of the rainfall changes induced by climate change in Vietnam is essential. Some studies have investigated the changes of rainfall events using CMIP5 climate change scenarios in Vietnam. Recently, CMIP6 climate change scenarios released and some studies have shown that the climate change scenarios from CMIP6 would be more reliable than those from CMIP5. Thus, spatial and temporal changes of rainfall events in Vietnam should be projected using climate change scenarios from CMIP6 and these projections should be analyzed. Hence, this study aimed to investigate spatial and temporal changes of rainfall events in Ca river basin in Vietnam using the climate change scenarios from CMIP6. Climate change scenarios from 26 CMIP6 models were used for monthly precipitation projections. Precipitation observations in eight ground weather stations near Ca river basin were employed to correct biases in monthly precipitation projections. There are large spatial variations in annual and seasonal precipitation within the eight stations. Overall, the total annual precipitation is increased. The autumn precipitation increases while the winter and spring precipitation decreases. Hence, there are possibility to increase magnitude of floods and severity of drought in Ca river basin in Vietnam.


HS07-A018
Projection of Future Drought Characteristics Using the Multiple Drought Indices Under SSP Scenarios in South Korea

Songhyun KIM+, Won-Ho NAM#
Hankyong National University, Korea, South

Recently, climate change has caused abnormal weather worldwide. Europe experienced a record heat wave and drought in 500 years, a severe drought in 1,200 years in the southwestern United States, and China experienced a heat wave in 60 years. Drought can have a serious social and economic impact on the entire agricultural system because of its wide range, and it is expected that the intensity and frequency of natural disasters such as drought will increase due to climate change. The trend of drought in South Korea has been increasing rapidly since 2000, and in 2015 and 2017, there was an unusual extreme drought, showing a different trend from before 2000. Therefore, in order to prepare for the occurrence of drought due to future climate change, it is required to establish a long-term drought outlook and adaptation strategy. In the Intergovernmental Panel on Climate Change (IPCC) 6th evaluation report, a Shared Socioeconomic Pathways (SSPs) scenario considering future socioeconomic changes and climate change mitigation efforts was developed through Coupled Model Intercomparison Project 6 (CMIP6). The SSP includes various factors of change, such as demographics, economic development, ecosystem, institutional, technological development, and policy development. Various drought indices were calculated based on the SSP scenarios calculated through 18 global climate models provided by CMIP6. The SSP5-8.5 scenario was used for the climate change scenario, and the Standardized Precipitation Index (SPI), Effective Drought Index (EDI), and Standardized Precipitation Evapotranspiration Index (SPEI) were applied to analyze the prediction and variability of each future drought index in South Korea.


HS07-A019
Dynamic Prediction and Early Warning Model of Urban Flood Ponding Process Based on Data-driven

Huiliang WANG, Yihong ZHOU#+, Zening WU
Zhengzhou University, China

Frequent urban floods disasters have become a major threat to cities, causing huge loss of life and property. To reduce the potential losses, it is important to improve the prediction ability of urban flood disasters. Previous studies have confirmed that the data-driven urban flood model can mine the nonlinear relationship between the driving factors and the target variables. However, few studies systematically describe how to use urban flood disaster data to realize dynamic prediction and early warning of ponding process. Therefore, this research seeks to propose a set of methods for dynamic prediction and early warning of urban flood from the perspective of data-driven to improve the accuracy and timeliness of urban flood prediction. Firstly, by using the spatial autocorrelation analysis and logical regression method to screen the sensitive index combination of urban flood prediction, the optimal index combination scheme suitable for the urban flood prediction was proposed. Secondly, three classical machine learning models were used to construct the prediction model of urban flood ponding process. On this basis, the improved Bayesian model average (BMA) method was used to dynamically couple the prediction results of the three models, and the integrated urban flood prediction model with dynamic weight was constructed. Finally, the modified rainfall forecast data was used to drive the integrated model to dynamically forecast the ponding process, realizing the rolling forecast and early warning of the urban flood. The results show that the Nash-Sutcliffe efficiency coefficient (NSE) of the integrated model was 0.986, the prediction accuracy of the integrated model was 11.4% - 50.4% higher than that of single model, which indicates that the proposed integrated prediction model based on data-driven has significant advantages in correcting the prediction bias, and can provide guidance for accurate and rapid urban flood ponding process prediction.


HS07-A020
Evaluation of the Stability of River Embankments Considering Climate Change

Sungho LEE1#+, Ingi YOO1, Jung Soo KIM2
1C&I Tech., Korea, South, 2University of Bucheon, Korea, South

Due to heavy localized rains and typhoons, which are caused by abnormal weather patterns, there is continued human loss of life and property damage in disaster-prone areas. In Korea, most rainfall occurs in summer, and runoff is concentrated in rivers in a short period of time, causing rapid fluctuations in river water levels. These sudden changes in water level can damage river levees and make them less stable, increasing the risk of flooding and causing loss of life in cities located near the levees. Therefore, it is important to regularly evaluate and maintain the stability of riverbanks to minimize the impact of natural disasters. In this study, the Levee Flood Vulnerability Index(LFVI) developed by referring to the Flood Vulnerability Index(FVI) was applied to evaluate the stability of river embankments when rainfall was applied considering climate change. The LFVI is a new technique developed by borrowing the format of the FVI and composing factors suitable for river embankments. It is a method of calculating the vulnerability index by calculating weights using an entropy technique based on the values of 7 factors. The study applied a climate change scenario to analyze the LFVI of river embankments along the Namhan River under rainfall scenarios in 2016, 2040 and 2070. The results of the analysis revealed a range of grades from 1 to 6, with the LFVI decreasing as climate change progressed, indicating potential concerns about stability. Acknowledgement: This work was supported by Institute of Information and communications Technology Planning and Evaluation (IITP) grant funded by the Korea government(MSIT) (No. 2022-0-00035, Development of Safety Management System for Deteriorated Reservoirs and River Embankment using Converged-Distributed Architecture with Composite IOT Sensors and AI Techniques).


HS07-A022
Assessing Human Contribution of a Drought via CMIP6 Models: A Case Study of the 2021 Iran Drought

Jonghun KAM#+
Pohang University of Science and Technology, Korea, South

In 2021, 4.9 million people over Iran, particularly rural areas, were at medium and high risk of drought impacts. The 2012 annual precipitation over Iran was lowest since 1979 while the level of public awareness of the ongoing drought was low, possibly due to the antecedent wet condition in 2020. The Arabian Subtropical High (ASH) expanded and was strong over 2020/21. The understanding of this event remains limited from the following perspectives: 1) How unusual the Iran drought in 2021 was? and 2) Was it attributable anthropogenic forcings? In this study, an extreme event is the unprecedented Iran drought in the calendar year 2021, defined by the 12-month standardized precipitation index (SPI12) calculated from the regional averages over Iran, excluding desert areas. Firstly, we evaluate the performance of the 13 CMIP6 models for the precipitation seasonality. Secondly, we use the CMIP6 models that capture well the precipitation seasonality and then construct the SPI12 distributions of the CMIP6 models for individual experiment forcing ensemble runs (historical, greenhouse gas-only, aerosol-only, and natural-only) and their SPI12 distributions over 2002–2021. Lastly, we compute the attributable probability ratio of the 2021-like drought to anthropogenic forcings in terms of drought intensity, persistence, and severity. Results show that the 2020/21-like severe and long-lasting Iran droughts have become more probable by at least 50% due mainly to anthropogenic greenhouse gas increases. In closing, the need for climate change adaptation for long-lasting Iran drought is discussed.


HS07-A025
Changes in Sediment Discharge Due to Climate Change Considering Sediment Production Factors

Riho KIDO1#+, Takuya INOUE1, Misako HATONO1, Kazuki YAMANOI2
1Hiroshima University, Japan, 2Kyoto University, Japan

Global climate change will have a significant impact on sediment discharge due to heavy rainfalls associated with climate change. Increase in sediment discharge will affect downstream riverbed form and channel conveyance capacity, causing damage such as levee breaks, overflows, and bridge failures. Climate change predictions require a large ensemble calculation to account for uncertainties. As a result, the calculation results of sediment discharge using the climate change predictions are also bigdata. However, there is no established method for evaluating the results of these large sediment discharge predictions. In this study, we investigate changes in sediment discharge based on changes in the factors of sediment production due to climate change using a physics-based model that can account for slope failure, channel erosion, and mixed grain-size sediment. Our study site is the upper reaches of the Pekerebetsu River in Hokkaido, Japan. Heavy rainfall in this basin was recorded during the heavy rainfall in Hokkaido in August 2016. We evaluate extreme events that are statistically infrequent using a large ensemble data for climate change in Japan called d4PDF and analyze the changes in return period using the abundant calculation results of sediment discharge. Our results show that the rate of increase in sediment discharge is larger than that in rainfall. Increase in heavy rainfall increases the supply of fine sediment from slope failures. When fine sediments are supplied into armored beds, the friction angle between bed materials decreases and the critical Shields number for incipient sediment motion decreases. Thus, the sediment on the riverbed will move more easily. Our results will contribute to the understanding of future landform changes and the planning of disaster prevention against climate change.


HS08-A001
Estimation of Water Demand Considering Natural, Social, and Environmental Variability

Tae-Woong KIM#+, Min Ji KIM, Jiyoung KIM, Ji-Young YOO
Hanyang University, Korea, South

Water shortage is a big challenge in the future because the global average temperature continues to increase, the drought occurrence due to climate change increases, and the availability of clean water decreases due to water pollution. To reduce future water shortage risk, it is necessary to estimate water demand in consideration of nature, social, and environmental factors. Thus, this study performed basic survey and analyses of change trends for the past water usage, and evaluated the variability and uncertainty of the water demand. We performed correlation analyses among water usage (domestic/industrial/agricultural), average temperature, precipitation, population, and water supply area (including residential, commercial, and industrial areas) in 19 districts within the Geum River basin from 1965 to 2019. Considering the correlations, enumeration models were proposed of which natural factors (precipitation, average temperature) consider non-linear relationship and social and environmental factors (water use, population, water supply area) represent a linear relationship. Based on the coefficient of determination, the enumeration models indicated that the water for industrial use accounted for 70.9%, and the water for agriculture accounted for 48.4%. 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) (No.2022003610001).


HS08-A005
Flash Droughts Identification Based on an Improved Framework and Their Contrasting Impacts on Vegetation Over the Loess Plateau, China

Shengzhi HUANG#, Xudong ZHENG+, Qiang HUANG, Lin YE, Beibei HOU, Xiaojuan ZHAO, Yifei LI
Xi'an University of Technology, China

Flash drought occurs in a short timescale and has more adverse impacts on society and ecosystems than regular drought. Considering flash drought as a special type of regular drought and identifying it by the rate of the first intensification period might ignore posterior intensification periods. To this end, we introduced the combinatorial decomposable flash drought identification framework (CDFDI) to identify flash drought from the perspective of regarding it as the subphase of drought and explore the characteristics and vegetation response of flash drought in the Loess Plateau (LP), China, where is prone to drought and its ecological environment is very fragile. The effectiveness of the framework is evaluated through the comparison analysis with a preexisting identification method proposed by Liu et al. (2020, https://doi.org/10.1175/jhm-d-19-0088.1). Results indicate that: (a) the CDFDI framework can better capture flash drought events than the Liu's method in terms of time series and spatial patterns, its rationality was further demonstrated by the obvious latitudinal pattern of correlation between flash drought and normalized difference vegetation index (NDVI); (b) the correlation shows an southeast (positive) and northwest (negative) contrasting pattern in the LP; (c) such contrasting pattern was also found in the response time of GPP, which suggests a more rapid impact on vegetation of flash drought in the arid northwestern LP; and (d) flash drought shows an exacerbating trend across the LP under the background of climate warming and mainly concentrated in the southern part. In general, this study provides new insights on flash drought connotations in a changing environment.


HS08-A007
The Decadal Changes in Drought Indicators in Indonesia from 1981 - 2020

Amalia Nafisah Rahmani IRAWAN#+, Daisuke KOMORI
Tohoku University, Japan

According to the Intergovernmental Panel on Climate Change (IPCC), the global temperature is projected to rise by around 1.5°C by 2030. This increase in temperature will result in an uneven distribution of rainfall patterns and amounts, leading to increased risk of drought disasters in certain regions. Droughts have a significant impact on water availability, both surface and groundwater, which in turn affects human activities that heavily rely on water such as domestic, industrial, and agricultural purposes. To assess droughts, numerous drought indexes have been developed, including the Standardized Precipitation Index (SPI) introduced by McKee et al. in 1993.  One of the benefits of using SPI, it only requires long-term precipitation data as input and uses probability distribution and normalization to evaluate wet and dry conditions. This research used SPI-3, which is often used by many researchers to represent agricultural drought conditions, to assess various drought indicators including frequency, duration, severity, and intensity in Indonesia from 1981 – 2020. This research also focused on the change of agricultural drought indicators under changing climate that could also affect the agricultural activities. The precipitation dataset was obtained from the Multi-Source Weighted-Ensemble Precipitation (MSWEP) which provides monthly precipitation with 0.1° resolution from 1979 – present date. Based on the assessment, the drought frequency, duration, severity, and intensity tend to increase in the recent decade especially in South Sumatra and Java Island which is known as the main producer of crops. However, the worst drought event occurred in 1991 – 2000 where the precipitation was recorded as the lowest compared to the other decades. This study will be beneficial to assess the hotspot region to consider the appropriate drought mitigation and preparedness.


HS08-A008
Study on Multi-scale Drought Propagation and Its Impact on Grain Yield in the Yellow River Basin

Wenjing MAO+, Jun NIU#
China Agricultural University, China

The transition of drought signal from one type of drought to another is referred to as drought propagation. Exploring the propagation among meteorological, agricultural and hydrological drought and its potential influence factors is crucial for early warning of drought. As a case study in the Yellow River Basin (YRB), the Standardized Precipitation Index (SPI), Standardized Soil Moisture Index(SSMI) and Standardized Runoff Index (SRI) were used to represent meteorological, agricultural and hydrological drought, respectively. The Pearson correlation coefficient was used to explore the propagation time of meteorological to agricultural and hydrological drought. The run theory is applied to identify drought events and match both types of drought events. The copula-based conditional probability distribution and Bayesian network probabilistic model were used to constructs drought propagation index. Then, an integrated risk assessment framework based on drought propagation characteristics and socio-economic impact was established to assess drought propagation risk. And the drought-induced yield loss rate was analyzed.


HS08-A012
A Multimodel Assessment of Climate Change Impacts on Hydrological Drought Over Hanjiang River Basin, China

CHAO DAI#+, Zhu HAORAN
Sun Yat-sen University, China

Drought has become one of the natural disasters affecting the water ecosystems in many basins around the world, and the situation may become more severe under the impact of climate change. For better adaptation planning, this study proposes a drought assessment framework integrating downscaling method, hydrological model, drought index and statistic frequency analysis, and applies it to explore the changes in drought characteristics from the past to the future in the Hanjiang River basin of South China. First, a hydrological model of this basin was constructed and the hydrological parameters were calibrated. Then, the standardized runoff index (SRI) was used to define the hydrological drought based on the runoff data simulated by the hydrological simulation. Then, the spatial and temporal distributions of drought duration and severity are calculated. To address the effect of climate change, similar calculation process was applied to the future climate data, which was downscaled using delta change method from 10 general circulation models (GCMs) of Coupled Model Intercomparison Project Phase 6 (CMIP6). The results of the study provide useful information for water resource authorities interested in developing effective long-term drought management adaptation strategies.


HS08-A014
Assessment of Groundwater Recharge and Ternary Mixing in a Small Watershed Using Natural Tracers in Daejeon, Korea

Hanna CHOI1+, Chung-Mo LEE2, Shim BYOUNG OHAN1#
1Korea Institute of Geoscience and Mineral Resources, Korea, South, 2Pusan National University, Korea, South

The estimation of groundwater recharge and hydrochemical changes is necessary to long-term management of water resource and the understanding of hydrologic water balance. We investigated the hydrochemical mixing among rainwater, groundwater, and surface water under the given hydrological condition in a watershed boundary of Yuseong region, Daejeon in South Korea. To identify the mixing ratio among different water bodies of the catchment, hydrochemical analysis with tracers of chloride and stable isotope were performed. Ion composition indicates this watershed is mainly influenced by precipitation recharge in the mountain areas. The groundwater recharge rate in this site was calculated as about 20% of total precipitation by the GIS application with the water budget method. According to the calculated mixing ratios from tracer analysis, the groundwater hydrochemistry in this site is affected by water-rock interaction but it is also reflected the impact on small amount of untreated domestic effluent. Comprehensive interpretations of the recharge rate and surface water-groundwater mixing will be useful for estimating hydrological water balance in small mountainous catchments.


HS08-A016
Comprehensive Evaluation of Hydrological Models for Climate Change Impact Assessment

Shanshan WEN#+
Anhui Normal University, China

Climate change has substantial impacts on regional hydrology in the major river basins. To figure out such latent hydrological impacts of changing climate, more reliable hydrological simulations are imperative. In this study, we evaluated the impacts of climate change on the hydrological regime in the Upper Yangtze River Basin based on four downscaled and bias-corrected Global Climate Model outputs from Coupled Model Intercomparison Project Phase 5 under four Representative Concentration Pathways (RCP2.6, RCP4.5, RCP6.0, and RCP8.5) driving three hydrological models. Two model evaluation approaches were applied: simple and comprehensive. The comprehensive approach was used to evaluate models in the historical period, optimizing objective function at four gauges, and hydrological models were weighted for impact assessment based on their performance. In such a way, projected streamflow time series are obtained under different emission scenarios. Results show that the annual average discharge is projected to increase by 4.1–10.5% under the RCP scenarios at the end of twenty-first century relative to the reference period (1970–1999). Moreover, the high flow is projected to increase and the low flow to decrease indicating a higher probability of flood and drought occurrence in the basin. The severity of floods and droughts may increase. In comparison with the simple one-site model evaluation approach, the comprehensive method reveals that the anticipated extreme flow events would be less severe, and annual mean discharge slightly lower. The projected results imply that the application of the comprehensive model evaluation approach could narrow the simulated spreads of projections significantly, and might provide more credible results.


HS08-A017
Influence of Agricultural Irrigation on the Regional Groundwater System

Yi Hsuan HUANG#+, Ko Li LIU, Kai Wen LIN, Ray Shyan WU
National Central University, Taiwan

Agricultural water accounts for more than 70% of Taiwan's total water consumption, so there are often doubts about excessive water consumption. In recent years, studies have mentioned that about 40% of irrigation water will return to groundwater, and groundwater resources have gradually become an important water supply. The Tainan area has a relatively mature irrigation system. The irrigation system in the Kaohsiung area is rather incomplete. During the dry season, agricultural water is often unable to provide enough water due to insufficient water, resulting in an imbalance between the supply and demand of water resources, leading some areas to supplement water demand and over-extract groundwater. In this study, the system dynamics model - VENSIM is used to establish the correlation model between the reservoir river system and groundwater. The hydrological data of several years are used to analyze the adequate rainfall and irrigation water demand, and to explore the impact of agricultural water use on the groundwater level, to understand the agricultural water consumption. The amount available for dispatch and the best reasonable use amount.


HS08-A018
The Hydrological Impact of Climate Variability and Forest Disturbance in Stellako Watershed of Canada

Zipei LIU+, Mingfang ZHANG#, Shiyu DENG
University of Electronic Science and Technology of China, China

Climate variability and forest disturbance are commonly recognized as critical driving factors significantly affect the regional hydrology in large-scale forested watersheds. Yet, due to the watershed landscape heterogeneities (e.g., topography, soil characteristics, climate conditions, and vegetation types), hydrological responses to climate and forest changes and associated mechanisms have not been fully understood. In addition, distinguishing the hydrological effects of forest change, climate variability and other factors in a large watershed efficiently and accurately, remains a challenge. In this study, we combined the modified double mass curve (MDMC), Autoregressive Integrated Moving Average (ARIMA) intervention, and multivariate ARIMA to assess the annual streamflow affected by climate variability and forest disturbance in the forested Stellako watershed, a typical forest-disturbed area in Canada. The study period was from 1951 to 2018. The key findings are: (1) the hydrological environment was significant influence by cumulative external disturbances after 1980, referring to the 1951-1979 period the annual runoff decreased by 38.65 mm, (2) from 1980 to 2018, the streamflow decreased by 14.69 and 24.75 mm due to climate and forest changes, respectively, (3) the annual runoff variation was mainly attributed to forest disturbances contributing 42.42% of the total variations. The developed methodology can be applied to quantify the disturbance effects at a watershed or regional scale and develop watershed and forest management strategies under future climate and forest changes.


HS10-A007
Comparative Analysis of One Parameter Hydrological Model on Watershed in Republic of Korea

Heemin KO1+, Hyunuk AN1#, Seungjun LEE2, Jiyoung JUNG3
1Chungnam National University, Korea, South, 2Korea Institute of Geoscience and Mineral Resources, Korea, South, 3K-water, Korea, South

Agricultural reservoirs supply water for various purposes such as irrigation, maintenance, and living. Since agricultural reservoirs respond sensitively to seasonal and climate changes, it is essential to estimate supply and inflow for efficient operation, and water management should be done based on these data. However, in the case of agricultural reservoirs, the measurement of supply and inflow is relatively insufficient compared to multi-purpose dams, and inflow-supply analysis in agricultural reservoirs through water balance analysis is necessary for efficient water management. Therefore, rainfall-runoff analysis models such as ONE model and Tank model have been developed and used for reservoir water balance analysis, but the applicability analysis for ungauged watersheds is insufficient. The ONE model is designed for daily runoff calculation, and the model has one parameter, which is advantageous for calibration and ungauged watershed analysis. In this study, the water balance was analyzed through the ONE model and the Tank model for 15 watersheds upstream of dams, and R2 and NSE were used to quantitatively compare the performance of the two models. The simulation results show that the ONE model is suitable for predicting the inflow of agricultural reservoirs with the ungauged watershed. This work was supported by Korea Institute of Planning and Evaluation for Technology in Food, Agriculture and Forestry(IPET) through Agricultural Foundation and Disaster Response Technology Development Program (or Project), funded by Ministry of Agriculture, Food and Rural Affairs(MAFRA)(321071-3).


HS10-A008
Impact of Acoustic Waves on Rainfall Distribution in Acoustics-induced Artificial Rainfall Technology

Mengyao WANG1#+, Ji CHEN1, Jiaye LI2, Jinzhao WANG3
1The University of Hong Kong, Hong Kong SAR, 2Dongguan University of Technology, China, 3Qinghai University, China

As a potentially effective method for increasing water resources, the acoustics-induced artificial technology has attracted wide attention for the characteristics of eco-friendly and low-cost. In this study, a non-randomized acoustic rainfall field test was carried out in the Tibetan Plateau from May 18, 2020, to June 19, 2020. The rainfall data were collected by ground-based tipping bucket rain gauges. Various classification criteria were applied to these rain gauges to analyze the acoustic impact on rainfall distribution. The results showed that the natural rainfall distribution in the experimental base is highly related to the cloud condition and terrain. The overall rainfall was more concentrated in the east. While with the influence of acoustic waves, the rainfall center has shifted to the west region during the rainfall events with the acoustic operation. This phenomenon may be caused by the combined effect of acoustic field and near-surface convection. Compared with the natural rainfall process, the long-duration rainfall process under acoustic fields has an apparent two-stage pattern. The rainfall intensity is much heavier in the central region (near the acoustic operation point) than on either side during the first stage, lasting less than one hour. This phenomenon may be attributed to the trigger effect of acoustic waves, which has accelerated the forming process of large droplets. While rainfall in the second stage usually lasts for hours with random distribution. The impact of acoustic waves on the growth of relatively small particles may not be reflected in the rainfall distribution due to the complex cloud dynamics.


HS10-A011
Analysis of the Effect of Design Rainfall Overrun Duration on Drainage System

Seok Hwan HWANG#+, Jungsoo YOON, Narae KANG
Korea Institute of Civil Engineering and Building Technology, Korea, South

On August 8, 2022, torrential rain of more than 100 to 300 mm per day fell in the Seoul, Incheon, and Gyeonggi metropolitan areas and Gangwon of KOREA, causing flooding of roads, houses, and vehicles in various places. Overall, the southern area of Seoul recorded more than 90 mm of precipitation per hour. At around 9:00 pm on the 8th, the maximum one-hour precipitation of 141.5mm was recorded at the Korea Meteorological Administration branch. The maximum daily rainfall also recorded 435.0mm/day (2022. 8. 9, 12:17) at the operating point, exceeding the all-time high of 354.7mm (1920. 8. 2.). It exceeded 350 mm in most of the Gangnam area of Seoul. And Gangnam, Seocho, and Korea Meteorological Administration (Sindaebang) points where precipitation was concentrated exceeded the 200-year frequency for up to 6 hours of rainfall duration. However, it is insufficient to judge the magnitude of the heavy rain that caused flood damage this time only by the frequency of rainfall. Compared to large-scale inundation and heavy rain events that have occurred since 2000, the instantaneous rainfall intensity was not record-breaking. However, it is characterized by the fact that the rain of strong rainfall intensity exceeding the design capacity continued continuously for 3 hours. Therefore, in this study, considering the duration exceeding the frequency as well as the frequency of precipitation, we analyzed the degree of effect on the performance of the drainage system according to the duration compared to the past cases. Acknowledgment: This research was supported by a grant(2022-MOIS61-002) of ‘Development Risk Prediction Technology of Storm and Flood for Climate Change based on Artificial Intelligence’ funded by Ministry of Interior and Safety(MOIS, Korea).


HS11-A001
Development of Observational Data Collecting System for Urban Flood Analysis

GyeongHyeon KIM+, BonHyun KOO, TaeYoung HAM, KyuCheoul SHIM#
JBT Corporation, Korea, South

This study presents various observational data collecting module to use collected data as input data in urban flood analysis model. Various institutions provide various formats of data such as XML, JSON, CSV, SHP, etc. We established different collection processes according to the format. Urban flood data collecting module is a web platform which automatically collecting 33 kinds of data for analyze rivers from K-water, Korea Meteorological Administration, Han River Flood Control Office, etc. using representational state transfer application programming interface and Linux crontab. Urban flood data collecting module provides quasi-real-time data collection and collection status information. Development of urban flood data collecting module is first part of 5 years research urban flood meta-solution. Based on the urban flood data collecting module, we are planning to import urban flood analysis model on the meta-solution platform and use collected data for input data. 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) (2022003470001).


HS11-A007
Characteristic of Regional Groundwater Flow System: Case Modeling Study in Longzici Karst Spring Area, North China

Xiaojuan QIAO1,2#+, Yu CHENG1, Dawei WANG1
1University of Chinese Academy of Sciences, China, 2Chinese Academy of Sciences, China

Karst spring water dynamic characteristics and its response to atmospheric precipitation are of great significance for water resources utilization under the background of climate change. This paper selects Longzici spring area, North China, as the study area. Based on a long series of spring water flow and precipitation data, the dynamic characteristics of spring flow was analyzed and the numerical simulation of the groundwater flow model was established. The results shows that the groundwater kept the sustained decline over the past decades which is in a negative equilibrium state, with a storage variable of -2.26 million m³/year. The sensitivity of spring flow to precipitation under different precipitation scenarios shows that the water level changes in the recharge and drainage areas are similar about (3-5cm) and slightly larger than that in the runoff area(1.5cm) when minimum rainfall (287.24 mm) happens. When the precipitation is at its maximum (867.66 mm), the water level change in the runoff area can reach 95 cm which is much larger than those in the recharge and discharge areas. The results indicates that Longzici karst spring has a relatively good regulation water resource capacity and the runoff area is more sensitive which plays an important role in response to climate change.


HS11-A013
Isolation and Characterisation of Bacterial Species for the Bioremediation of Synthetic Dyes in Wastewater

Priscilla S. K. LEUNG+, Kung Ming LEUNG, Grace LAI, Simon GRIFFIN#
The ISF Academy, Hong Kong SAR

Discharged effluent from textile dyeing is a major pollution concern for urban surface water as well as groundwater. While persistence and chemical stability may be desirable qualities for dyeing, the same properties make for a detrimental and unsustainable environmental impact. As the world’s predominant supplier of textiles, pollution from dyeing and finishing is especially acute in Asia, with annual discharges of textile wastewater in China alone exceeding 1.84 billion tonnes [1, 2]. 
This project has sought to isolate and characterise versatile dye-degrading bacteria that might offer an energy-efficient method of remediation of textile wastewater. Samples from a stormwater drain were used to inoculate a high salt content medium (CAV) and the resulting colonies transferred to separate agar plates containing azure B, methylene blue and malachite green. After isolation, DNA extraction by Qiagen DNeasy PowerSoil Pro Kit and sequencing via Illumina and Nanopore platform, the complete genomes of three isolates with vigorous dye-decolorizing activity were established by hybrid assembly (Unicycler v0.4.8). They were identified and annotated via PATRIC-BRC as Aeromonas hydrophila subs. hydrophila strain PSKL.DP, Aeromonas dhakensis strain PSKL.DM and Pseudomonas putida strain PSKL.D1, with genome sizes 4.78, 4.82 and 5.88 Mbp respectively. Whilst all three isolates possess genes explaining their dye-decolorization activity (up to 2.5 mg/L Azure B and 1.25 mg/L methylene blue in 24hr), the presence of potential virulence and antibiotic resistance genes in PSKL.DP would preclude its use for wide scale remediation. PSKL.DM and PSKL.D1, on the other hand, appear more promising. References:
[1] R. Al-Tohamy, S. S. Ali, F. Li, et al.. Ecotoxicol. Environ. Saf., 231: 113160 (2022). [2] H. Chen, X. Yu, X. Wang, Y. He, J. Clean. Prod., 326: 129353 (2021).


HS11-A022
Patch Size Effect on a Flow Field Due to Submerged Aquatic Vegetation

Keita MATSUMURA1+, Keisuke NAKAYAMA1#, Tetsuya SHINTANI2, Hiroki MATSUMOTO3
1Kobe University, Japan, 2Tokyo Metropolitan University, Japan, 3Port and Airport Research Institute, Japan

Natural disasters have become more frequent and severe worldwide, so it is urgent to adapt and mitigate climate change. In contrast, the carbon absorbed and sequestered by ecosystems, called "Blue carbon", has attracted attention as a means of mitigating climate change. Nellemann (2009) revealed that blue carbon ecosystems, such as coastal seagrass beds, absorb atmospheric carbon dioxide. Therefore, effective carbon dioxide reduction through accurate assessment and management of the blue carbon ecosystem is desired. However, submerged aquatic vegetation (SAV) often exists in patches, creating complex flow regimes through mutual interference with the current. As a result, the carbon absorption rate is significantly affected, making accurate estimates of sequestration by blue carbon ecosystems difficult. Therefore, it is necessary to understand mass transport under such a complex flow field. Thus, this study aims to clarify the patch size and deflection effect on the hydrodynamics around SAVs using numerical simulations. The SAV numerical model was successfully used to analyze the flow around an SAV patch, with results in good agreement with laboratory experiments. Numerical results showed that when the SAV bended significantly, the higher velocities occurred above the SAV meadow, with the lower velocities at the bottom of the SAV. Additionally, when the SAV did not bend significantly, the water flow was found to go significantly around the SAV patch than in the low-elastic modulus case. As a result, it was found that the proportion of the channel width occupied by the patch was the most critical factor in controlling the flow conditions and mass transport. Additionally, deflection was also an essential factor.


HS11-A037
Rainfall-runoff-inundation Simulation Using a 1m Resolution Elevation Data Focusing on Sannomiya, Japan

Nanako INOKAWA#+, Kenichiro KOBAYASHI
Kobe University, Japan

Due to climate change, the risk of flooding is increasing also in areas where previously the risk was low. It is very important to estimate the flooding risk accurately by using high accuracy inundation model against large-scale flooding and to take measures for such as large-scale flooding. There are several inundation models developed such as Rainfall-Runoff-Inundation (RRI) model and many researchers have been considered its accuracy. Input data especially elevation data is one of the most important factors for accurate inundation analysis. In Japan, 5m high-resolution elevation data by geospatial information Authority of Japan has been widely used for inundation analysis. In this study, we examined the accuracy of inundation analysis by using the inundation model based on two-dimensional shallow water equation in Kobe, Japan using 1m resolution elevation data that is firstly published by Hyogo prefecture in Japan. As a result, inundation analysis using 1m resolution elevation data is highly accurate compared using 5m resolution elevation and accurately reflects topography also in steep areas.


HS12-A005
Evaluation the Carbon Dioxide Control Effect of Hydropower Generation Using Irrigation Reservoirs Targeting Pre-discharged Water

Atsuya IKEMOTO1#+, So KAZAMA1, Takeo YOSHIDA2
1Tohoku University, Japan, 2National Agriculture and Food Research Organization, Japan

The ultimate objective of this study is to evaluate the effectiveness of hydropower generation by irrigation reservoirs. To achieve the ultimate objective, as a first step, this paper examines factors that influences electric-generating capacity by prior releasing at irrigation reservoirs. This study also attempted to discuss effect of control on the discharge of carbon dioxide. As a result, it was estimated that a 3-day pre-discharge to reduce the reservoir storage volume to zero would reduce carbon dioxide emissions by 156 t-CO2. In addition, electric-generating capacity which is generated prior releasing discharge at irrigation reservoirs set in this study throughout Japan is estimated about 0.2%. Each electric-generating capacity is thought of as depends not storage of irrigation reservoirs but also reservoirs height. So this study focuses on storage capacity and reservoirs height, and attempts to examine the relationship between irrigation reservoir’s storage or height and electric-generating capacity by prior releasing by prefectures. The higher the storage capacity per reservoir, the higher the power output. The higher the height per reservoir, the higher the power output.


HS12-A006
Relationship Between Population Change and Regional Characteristics Caused by Flood Damage

Ayaka OKAMOTO#+, So KAZAMA, Hayata YANAGIHARA, Yusuke HIRAGA
Tohoku University, Japan

Relationship between population change and population density was investigated in term of the occurrences of flooding. The target areas for the study were municipalities in which the proportion of damaged buildings to the total number of buildings was 10% or greater between the years 2011 and 2020. The flood damage was defined as the damage caused by the breakage of embankments, overflow of embankments and non-embankment areas, pluvial flooding, and water storage water in depressions. The population change resulting from flood disasters was calculated utilizing actual population data obtained from the Basic Resident Register. The rate of population change due to flood disasters was estimated by subtracting the estimated population in the non-flooding from the actual population. The estimated population in the non-flooding was determined based on the actual population data obtained in the six years after the flood event. The findings revealed a correlation between the rate of population loss due to flooding and low population density, as well as a correlation between the rate of population growth and high population density. Additionally, the impact of different types of building damage on population loss was evaluated in small cities (population less than 100,000), medium cities (population between 100,000 and 500,000), and large cities (population over 500,000). The results showed that in small cities, even in cases where a significant number of houses were inundated or partially and totally destroyed, there was no tendency for population changes. However, in medium-sized cities, people tended to migrate to areas with building damage in cases of both inundation and partial/total destruction. In contrast, in large cities, the damage to buildings had a limited effect on population migration.


HS12-A009
Consideration of the Best Way of Desalination of Salinity Accumulation Soil in Mekong Delta

Aoi TAKAHASHI#+
Sendai Nika Junior & Senior High School, Japan

Salt damage is currently occurring in Mekong Delta, which causes failure of the cultivation of crop and thus resulting in a heavy economic damage. In general, it takes about three months for rain to wash away the salt in the soil. My objective was to find the best way of desalting which can shorten the time to reduce the salt. Small-scale industrial farmers cannot afford neither purchasing an expensive drainage equipment nor using a large amount of water, which is the standard way of desalting. Therefore, developing less expensive way to reduce the salt is required. Based on previous studies, the three different methods were considered the practical alternatives; mixing compost which contains Haemophiles in the salted soil, disseminating calcareous materials, using phytoremediation of salt tolerant plants. First, the salt-damaged soil was made by sprinkling 3 wt. % of brine. Next, the soil was put into 10 flowerpots and divide each two of them into the following five groups; (1) mix halophilic bacteria contained compost, (2) disseminate calcareous materials, (3) implant sorghum, (4) implant chard, and (5) do nothing special. The water, which amount was determined with reference to precipitation of Cà Mau province, were given to these pots, and the salinity was measured once a week. The average salinity of soil in Group 1 and Group 2 was significantly reduced than that of Group 5. Sorghum in Group 3 and chard in Group 4 were withered. The approximate period until the salinity of the soil reaches 0% was about 60 days in Group 1 and 58 days in Group 2, while 76 days in Group 5. These results suggest that contained compost and disseminate calcareous materials were effective to desalt the salinity accumulation soil and that those desalting ways would be helpful as less expensive option in Mekong delta.


HS12-A010
Algorithm Development for Precipitation Estimation by Image Segmentation Model Using Meteorological Satellite Images

Kansei FUJIMOTO#+, Taichi TEBAKARI
Chuo University, Japan

With climate change becoming more severe in recent years due to global warming and other factors, accurate precipitation data from meteorological satellites is expected to play an important role in disaster prevention and agriculture in regions where ground rain gauges and radar rain gauges are not fully deployed. Recently, many deep learning models have been developed, among which image segmentation models are useful for precipitation estimation from meteorological satellite images. This study aims to develop an algorithm that can estimate precipitation more accurately from weather satellite IR bands using multiple image segmentation models. Many image segmentation models for deep learning CNNs have been developed from around 2015 to the present. Among them, we select a model that excels in precisely discriminating rainfall areas and estimating precipitation intensity using IR band brightness temperature information, latitude and longitude, and elevation data. We also extract features from the IR band as training data, aiming for a model with high generalization performance. The satellite data used was the Himawari elevation data. In addition to the brightness temperature information, latitude, longitude, and elevation data were provided for the training data. The National Synthetic Radar GPV was used as the teacher data. The spatial resolution of the Sunflower standard data is 2 km. The satellite observations used for the training data and the radar images used for the teacher data have different observation targets: cloud particles and raindrops, respectively. Therefore, the observed brightness temperatures and precipitation intensities do not always agree with the peak positions. The training and teacher data are varied from 2 km to 10 km at 2 km intervals to see which estimation results are more reasonable. The results showed an improvement in the accuracy of precipitation estimation compared to nonparametric regression.


HS12-A011
Applicability of Excess Probable Rainfall Using Radar Rainfall for Watershed Management

Shihori OHASHI#+, Taichi TEBAKARI
Chuo University, Japan

Although Japan's meteorological radar systems are currently well equipped in both space and time, the data are rarely used for analysis of past phenomena other than disaster investigation. Considering the cost of operating ground rain gauges in the future, it is necessary to consider the possibility of replacing radar rainfall observation with ground. In this study, we examined the applicability of radar rainfall to watershed management by comparing excess probable rainfall between radar and ground rainfall data. The radar rainfall is used from Synthetic Radar GPV (2006-2022), and the ground rainfall is from Water Information System (MLIT) and AMeDAS (JMA) (1976-2022). The target area was the upstream from each reference point of the Tone, Watarase, Kinu, Kokai, Ara, Tama, Tsurumi, Sagami, Naka and Kuji Rivers flowing through the metropolitan area of Japan. We calculated the annual maximum basin average rainfall per planned rainfall duration (2 or 3 days) and the probability rainfall using Gumbel and GEV distributions of both radar and ground rainfall for the period 2006-2022 (Pattern A) and of radar rainfall for the period 2006-2022 and ground rainfall for 1976-2022 (Pattern B). We compared the rainfall probabilities calculated from radar and ground rainfall. As a result, the comparison of rainfall probabilities calculated from radar and ground rainfall using the GEV distribution showed that in Pattern A, the difference between radar and ground rainfall was generally within a range of ±20% for all basins except the Tama River. On the other hand, in Pattern B, the larger probability rainfall, the more the ground rainfall tended to be underestimated to radar. By adjusting the sample sizes of radar and ground rainfall, the calculated probability rainfall was found to have a generally similar trend. Consequently, radar rainfall may be applicable to using for watershed management.


HS12-A013
Projections of Future Flood Damage Cost and Evaluation of Adaptation Measures in River Basins of Toyama Prefecture, Japan

Shuichi KURE#+, Daichi KIKUCHI, Ryuto FUJISHITA
Toyama Prefectural University, Japan

In recent years, water disasters have become more frequent due to global warming, and basin flood control has been promoted to mitigate the damage, and several adaptation measures have been considered for flood damage reduction. However, the comparison of adaptation measures in different river basins and the feasibility of adaptation measures with mitigation effects to achieve a decarbonized society is not discussed. Therefore, this study proposes the most appropriate adaptation measures for five rivers in Toyama Prefecture, Japan by projecting the amount of future flood damage cost and conducting a quantitative evaluation of several adaptation measures. Therefore, flood damages are estimated from rainfall-runoff and flood inundation simulations under changing climates. For adaptation measures, vegetation management in rivers, rice paddy field dams, a concrete dam reservoir, green infrastructure, and forest conservation management were evaluated in this study. From the results of the analysis, the potential for paddy field dams, vegetation management, and green infrastructure shows a greater effect than a grey infrastructure at the Oyabe River.


HS12-A018
Regional Scale Water Footprint Based Agricultural Water Security Assessment

T. R. SREESHNA#+, Athira P
Indian Institute of Technology Palakkad, India

Climate change causes a significant impact on water availability and crop yield, which in turn are governing factors for ensuring water security in an agrarian region. The current study analyses the impact of climate change on water security in the command area of a multipurpose reservoir in Kerala, India. An integrated modelling framework considering SWAT hydrological model and DSSAT CERES rice model has been utilized for quantifying the water footprint and analyzing the water security on a regional scale for kharif and rabi season. The study considers the major role of reservoirs and the relevance of management practices in the region for water security assessment. The green water and blue water use in the study area has been estimated using the SWAT hydrological model, while the crop yield has been estimated for the short-span rice cultivar, Jyothi, using the DSSAT CERES rice model. The climate change signals are accounted in the study by considering three CMIP6 GCMs under two scenarios of shared socioeconomic pathways, SSP245 and SSP585. The regional agricultural water security under the changing climate is accounted by the green and blue water footprints as an indicator. An increasing trend of water footprint was observed towards the future, thus paving a path to a water insecure future. The study indicates the importance of developing adaptation policies on a regional scale.


HS12-A019
Evaluation of the Impact of Changes in Domestic Wastewater Treatment Methods on the Nitrogen Load Discharged from the Kurobe River to Toyama Bay

Matsuura TAKUYA1#+, Taichi TEBAKARI2
1University of Yamanashi, Japan, 2Chuo University, Japan

In Japan, the nitrogen load in closed sea areas such as Tokyo Bay, Ise Bay, and the Seto Inland Sea has been decreasing year by year, and the decrease in fish catches and the discoloration of cultivated algae such as seaweed and wakame (seaweed) are emerging as social and economic problems. In Toyama Bay, the target area of this study, it has been reported that the nitrogen load is decreasing year by year due to the improvement of wastewater treatment capacity as a result of changes in the domestic wastewater treatment system. The purpose of this study is to clarify the effect of changes in domestic wastewater treatment on the nitrogen load discharged from the Kurobe River to Toyama Bay. The precipitation, temperature, and solar radiation used in this study are the Japanese bias-corrected climate scenario data set based on the CMIP6 CDFDM method. In this study, the analysis was conducted for the period 1987-2014, when observation and scenario data are available. The spatial and temporal resolutions are 1 km and 1 day, respectively. The tank model was used as the effluent model, and the intensity method was used to calculate the total nitrogen (TN) emission load. In this study, TN sources were divided into areal and point sources. As a result, the pollution load from public sewage systems has increased, while the use of stand-alone septic tanks has decreased. As a result of a 76% increase in the sewage treatment population coverage from 1987 to 2014, the nitrogen load discharged from the Kurobe River watershed into Toyama Bay decreased by 8 % (76 kg/day) over a 30-year period.


HS13-A002
Effect of Land Use Land Cover Changes on the Water Balance Components of the Glacier-fed Mountainous Watershed: Assessment Using Fully Distributed Hydrological Model

Kavya M#, Sanjeev Kumar JHA+, Ankit SINGH
Indian Institute of Science Education and Research Bhopal, India

Land use and land cover patterns have a significant impact on the hydrology of a watershed. The mountainous watersheds have varying land classes with changes in elevation. The increasing anthropogenic activities also lead to changes in the aerial extent of different land classes. The highly variable topography, intricate river networks, and occasionally the presence of snow and glaciers limit the semi-distributed hydrological models to capture the physical processes in the Himalayan region fully. This study aims to quantify the hydrological response of a glacier-fed mountainous region with changes in land use and land cover. The fully distributed hydrological model WATFLOOD is used for stimulating the hydrological processes at the Alakananda River basin in the Western Himalayan region. Considering the data scarcity in the Himalayan region, the model is calibrated using reanalysis data from ERA-5. The land use land cover maps from 2005 to 2015 are used to set up the model. The entire basin is divided into seven sub-basins based on the discharge sites and land use types. The rainfall and temperature data from ERA-5 are used as input to WATFLOOD to calculate the runoff at the outlet of each sub-basins. The water balance components are evaluated across eleven land-use classes at multiple locations in the study area. The results show that the WATFLOOD model can accurately simulate the water balance in the Himalayan region. The developed hydrological model can be a potential tool for the management of mountainous watersheds.


HS14-A002
Delineation of Saltwater Intrusion to Exploit Freshwater in the Coastal Vietnamese Mekong Delta: Empirical Evidences in Co Chien Estuary

Duc Dung TRAN1,2#+, Thuc PHAM THI BICH3, Edward PARK2, Nam NGUYEN TRUNG4, Vu TRUONG NGUYEN3, Man DUONG BA3
1National Institute of Education and Earth Observatory of Singapore, Singapore, 2Nanyang Technological University, Singapore, 3Vietnam Academy of Science and Technology, Viet Nam, 4Ministry of Agriculture and Rural Development, Viet Nam

In the Vietnamese Mekong Delta, saltwater intrusion reduces freshwater resources for agricultural and domestic use in coastal areas, causing difficulties in multi-scale socio-economic development. Our study analyses salinity monitoring data from 1996-2020 and applied a 1-dimensional coupled with 3-dimensional model to determine saline-intrusion boundaries along the Co Chien river of Ben Tre province under the severe salinity year of 2016 and forecast to 2030. The findings show that the freshwater exploitability at 0.3g/l salinity is complicated along the Co Chien river, particularly for 3 to 6 months in the dry season at 28km to 5.29km from the river mouth. For the freshwater at 4g/l salinity, the exploitation time is sufficient at 25-28km; however, the difficulty from 1 to 3 months is found at the location 17km to the river mouth. Generally, the salinity pattern is stratified at the beginning and the end of the dry season but evenly mixed in the middle. Cross-sectional analysis shows freshwater layering when the tide recedes to a depth of 3m. Freshwater resources decrease with the frequencies of 50%, 75%, 85%, and 95% along the river, causing high salinity intrusion and deep water intrusion, while the salinity 0.3g/l does not occur in the case of super-depleted water of 85% and 95% probability) and 4g/l salinity penetrates 90% of Ben Tre province. The future forecast shows that salinity will intrude 10-15km further than that in the current condition. We propose active water storage reservoirs along the main rivers, consistent operation of water infrastructure systems and effective water distribution and exploitation, crop pattern change, and people awareness raising to exploit freshwater resources to adapt to saline intrusion driven by climate change. Our findings provide a lesson learned for similar worldwide deltas where freshwater is scarce due to salinity intrusion.


HS14-A003
The Integration Technology of Wind Warning and Application During Typhoons Affecting Taiwan

Chieh-Ju WANG#+, Dan Rong CHEN, Hsin-Hung LIN, Yi-Chiang YU
National Science and Technology Center for Disaster Reduction, Taiwan

Taiwan is threatened by typhoons in summer and autumn, and there is a high risk of wind disasters. However, the wind speed simulated by the model is overestimated for the average wind and underestimated for the peak gust. Therefore, it is necessary to correct the error of the model before using the modeled wind data for wind warning. In order to improve the accuracy of wind forecasting, this study applies lots research results from academic community, such as feature analysis for observation and forecasting, and also further establishes statistical models and dynamic statistical correction methods, etc. At last, it integrates all technologies and develops a wind warning system for typhoon disaster response. In order to understand the climate characteristics of wind observations, feature classification and statistical analysis were carried out for the historical wind direction and wind speed of each station in Taiwan. Also, a gust factor database was built for 503 stations in Taiwan by using the characteristic statistical method of gust factor. This database is used as the calculation index of forecast wind speed conversion and forecast gust. In addition, the past ensemble forecast wind data database is also analyzed to understand the error distribution and systematic error causes of numerical weather prediction models in wind speed forecasting, and try to carry out regression correction and effect evaluation of different methods. Finally, technologies such as gust factor, ensemble forecast, regression correction method and typhoon path correction method are integrated, and are applied to the wind warning during typhoons affecting Taiwan.


HS14-A004
Risk Assessment and Real-time Warning System Development of Hillslope Disaster in Mountainous Indigenous Villages

Jui-Yi HO#+, YuTing WANG, Che-Hsin LIU, Wei-Bo CHEN, Chih-Hsin CHANG
National Science and Technology Center for Disaster Reduction, Taiwan

This study proposes the risk assessment method for hill tribes by field disaster environmental survey. The field investigation of 558 indigenous tribes in Taiwan was based on four items that include indigenous village potential (IVP), indigenous village symptom (IVS), Indigenous village magnitude (IVM), and Indigenous village traffic (IVT). The Nature Break method is used to classify the risk of the hillslope disaster. There are 27 high-potential hillslope disaster areas were selected as the demonstrated areas to develop the real-time warning system. To increase the disaster lead time, this study combined Shallow landslide prediction based on the Infinite slope Model and TOPMODEL (SIMTOP) with the Precipitation Ensemble forecasts to construct a comprehensive real-time shallow landslide warning system for study areas. The results of this study reveal excellent predictive performance in terms of the time of occurrence landslides in all study areas. The proposed model has the potential for application in landslide early warning systems to reduce loss of life and property.


HS14-A005
Analysis on Large-scale Landslide Occurrence - A Case Study for Hu-Hu-Lun Area

Yu-Ching LIN+, Jui-Yi HO#, Chiao-Yin LU, Che-Hsin LIU, Shih-Chiang LEE, Chih-Hsin CHANG
National Science and Technology Center for Disaster Reduction, Taiwan

Taiwan is prone to hillslope disaster in mountain areas because of its special topographical, geological, and hydrological conditions. Up to 9,848 large-scale landslides potential areas had been delineated based on the landslide micro-topography. Consequently, Soil and Water Conservation Bureau in Taiwan make a large-scale landslide prevention and response operation plan. The 269 large-scale landslide potential areas in Taiwan with high risk and protected objects had been selected to predict the large-scale landslide occurrence. Although the large-scale landslide is the rare event, one of large-scale landslide potential areas, namely Hu-Hu-Lun area (number: D003), occurred deep-seated landslide caused by the heavy rainfall during Typhoon NESAT in October 2022.In this study, the airborne Lidar with unmanned aircraft system was used to generate the digital elevation model (DEM) to provide the surface information such as the scope of the landslide, the historical cliff, and the old forest road. The results indicated the maximum elevation change of the landslide and the accumulation area are decreasing 26.1 m and increasing 22 m respectively. In addition, 180 frames (from 2019 to 2021) of down-orbit synthetic aperture radar images (SAR) were analyzed by permanent scatterer radar interferometry (PSInSAR). The long-term submersible phenomenon in the landslide crown and the landslide area has obvious deformation in the second half of 2021 from the monitoring results. The analysis results are good agreement with in situ monitoring. It is promising to apply the proposed method for subsequent disaster response research and application.


HS14-A006
Exploring the Use of Single Image Super-resolution Techniques for Enhancing GCM Rainfall Data in Taiwan

Chou-Chun CHIANG1+, Li-Huan HSU1#, Jung-Lien CHU1, Kuan-Ling LIN1, Li-Rung HWANG1, Hsin-Hung LIN1, Chieh-Ju WANG1, Yi-Chiang YU1, Chin-Shyurng FAHN2
1National Science and Technology Center for Disaster Reduction, Taiwan, 2National Taiwan University of Science and Technology, Taiwan

This study develops a downscaling technique for global circulation model (GCM) rainfall data using the Multi-Scale Residual Network (MSRN) algorithm, which is a deep learning algorithm for image super-resolution problems. The GCM rainfall data with a resolution of 0.25 degrees is increased 20 times to 0.0125-degree high-resolution grid rainfall data covering Taiwan. The technique consists of two MSRN modules that increase the resolution by 4 times and 5 times, respectively, in a hierarchical concatenation. The results of the verification of the test data show that the MSRN module can modify the rainfall distribution towards higher values and outperforms the linear interpolation method for daily rainfall thresholds less than 500 mm. Four sets of global model daily rainfall forecast downscaling products were tested from August 28th to November 30th, 2022, including the ECMWF deterministic forecast, the ECMWF ensemble forecast with 51 ensemble members, the MPAS deterministic forecast, and the JMA deterministic forecast. The verification results show that MSRN improves the rainfall forecast results for the four different model datasets, with significant improvement in the threat score and true positive rate for rainfall thresholds from 40 to 200 mm. However, the results also indicate that MSRN tends to overestimate higher rainfall thresholds and leads to higher false positive rates.


HS14-A008
Inundation Analysis of Farmlands Area Using 2D Inundation Model K-flood

Inhyoek SONG+, Hyunuk AN#, Hee Sung LIM
Chungnam National University, Korea, South

The frequency of heavy rains is increasing due to climate change. In Republic of Korea, the average annual rainfall has increased over the past 30 years, while the number of rainy days decreased, which means increasing rainfall intensity. In particular, despite of its importance for food production, farmland areas suffer great damage every year due to relatively insufficient preparedness and mitigation measures compared to urban areas or residential areas. In Korea, because the maintenance for main river is relatively well established, and farmland inundation is often caused by insufficient drainage capacity. However, flood analysis on farmland is still insufficient. In this study, flood analysis was conducted using K-Flood to analyze the causes of flooding in farmland areas and to reduce flood damage. K-Flood is a two-dimensional flood inundation analysis model developed by this research team that can simulate flooding in two dimensions in the target area to be analyzed. Farmland near the Shindae drainage plant in Mihocheon, Cheongju-si, Chungcheongbuk-do was selected as the target site, and the flood that occurred on July 14-16, 2017 was selected as the target event. Rainfall data and DEM data from Cheongju and Ochang were used for flood analysis. The flooded area simulated by K-Flood and the reported flooded area were compared, and the cause and progress of the flood were analyzed. This work was supported by Korea Institute of Planning and Evaluation for Technology in Food, Agriculture and Forestry (IPET) through Agricultural Foundation and Disaster Response Technology Development Program (or Project), funded by Ministry of Agriculture, Food and Rural Affairs (MAFRA) (321071-3)


HS14-A011
Improvement and Uncertainty Analysis of Streamflow Prediction Using Lumped-hydrologic Modeling and Ensemble-based Data Assimilation

Garim LEE+, Bomi KIM, Songhee LEE, Seong Jin NOH#
Kumoh National Institute of Technology, Korea, South

Accurate prediction of streamflow is essential for water resource management and disaster mitigation. However, under changing climate and environment, the conventional optimization schemes have become more uncertain and vulnerable since stationary features or parameters of a catchment might change over time. Hydrological data assimilation (DA) is a method that can improve predictive accuracy by considering the uncertainty of hydrological models, updating the states or parameters of a hydrologic model to produce more reliable estimates of the initial conditions and parameters. In this study, the two ensemble-based sequential DA techniques, ensemble Kalman filter and particle filter were analyzed for the streamflow predictions by a lumped hydrologic model using airGRdatassim. In addition, we assessed the effect of DA-related hyper-parameters on the simulation performance. Multiple numerical experiments were implemented for the Yongdam Dam catchment in South Korea. As expected, the accuracy of the daily streamflow simulation was improved by ensemble-based sequential DA while limited performance was found for high-flow simulation. We discuss the impacts of and hyper-parameters such as input forcings uncertainty and updating schemes on the performance and ensemble distributions. Also, feasibility of further improving DA such as increasing temporal resolution and adding new post-processing schemes will be discussed.


HS14-A012
Effects of Sample Volume on Microplastics Occurrence in Groundwater: A Case Study in Haean, Korea

Jihye CHA+, Jin-Yong LEE#
Kangwon National University, Korea, South

Microplastics, defined as particles less than 5 mm in size, have become a global environmental concern due to their widespread presence in the environment and potential harmful impacts on humans. Accurate quantification of microplastics is crucial to understand the extent of the problem and to evaluate the effectiveness of managing strategies. Sample volume is one of the key factors that can affect the detection and quantification of microplastics, and therefore should be carefully considered. This study examined the effects of sample volume on microplastics, including how it can affect their abundance, size, shape, and polymer type. To this end, we collected 30 microplastics samples using five different groundwater sample volumes of 100, 200, 300, 400, and 500 L from three groundwater wells located in the Haean agricultural basin of Korea, in the wet and dry seasons of 2022. The results showed that the sample volume may impact the conclusions about the distribution and abundance of microplastics, but larger sample volumes required more resources and time. Overall, the sample volume is a crucial consideration in the microplastics investigation and must be carefully evaluated in order to accurately understand the occurrence and impact of microplastics in groundwater. This research was supported by Korea Environment Industry & Technology Institute (KEITI) through Measurement and Risk assessment Program for Management of Microplastics Program, funded by Korea Ministry of Environment (MOE) (2020003110010).  This work was supported by the National Research Foundation of Korea (NRF) grant funded by the Korea government (MSIT, Ministry of Science and ICT) (No. NRF-2021R1F1A1064027).


HS14-A015
Using Three-dimensional Numerical Simulation Technology for Delineation of the Impact Area Caused by Large-scale Landslide

YuTing WANG, Jui-Yi HO#, Chih-Hsin CHANG, Yu-Ching LIN+
National Science and Technology Center for Disaster Reduction, Taiwan

The Three-Dimensional Distinct Element Code (3DEC) belonging to the Distinct Element Method (DEM) was adopted to generate the three-dimensional model for deep-seated landslide simulation in this study. This study simulates the deep-seated landslide by 3D numerical simulation to explore the sliding process and its impact area. The analyze results determine the unstable block and impact potential area caused by large-scale landslides. Two study areas of Xin-Zhuang settlement in Shan-Lin District, Kaohsiung City (District-D021) and the landslide area at 3.1k on National Highway No. 3 in Taiwan, were adopted to evaluate the performance of 3DEC model. The results indicated that good landslide simulation in both study areas for subsequent disaster prevention.


HS14-A017
Use UAS to Track Coastal Changes in Northern Area in Taiwan

Ting-Yu LIANG+, Hung-Ju SHIH, Shih-Chiang LEE, Yu-Ching LIN#, Jui-Yi HO, Chih-Hsin CHANG
National Science and Technology Center for Disaster Reduction, Taiwan

The erosion and deposition of coastal areas are greatly affected by wave, storm surge, and sea level rise especially during typhoon periods. The range or altitude changes in coastal area will affect the safety of coastal settlements in both short and long term time period. That highlights the importance of long-term records of coastal terrain change. Started from 2020, we use unmanned aircraft systems (UAS) to take multi-period images at 3 locations (Lao Mei, Yong Xing, and Zhong Jiao) of northern coast area in Taiwan. And transfer these images into digital surface model (DSM), which can show high resolution surface elevation. Through this multi-period DSM data, we can analysis the elevation changes between different seasons and notify the inter-annual variability of chosen locations. We can also analysis the efficacy of coastal facilities, as a reference for future facility construction.


HS14-A018
Prediction of Sewer Pipe Water Level Using Machine Learning Algorithm

Hyojin LEE1+, Hyunuk AN1#, Hee Sung LIM1, Seungsoo LEE2
1Chungnam National University, Korea, South, 2Korea Environment Institute, Korea, South

In highly impervious urban areas, the frequency of inundation and its damage is increasing due to the lack of drainage capacity and sewage outflow. Urban flooding causes enormous property damage and loss of life. Flooding countermeasures include expansion of drainage capacity and flood forecasting. In general, flood forecasting is practiced using river water level prediction. In the past, studies on river level prediction have been conducted using various methods. However, since urban inundation is caused by insufficient rainwater drainage capacity and sewage outflow, urban inundation is related to sewer pipe water level rather than river level. Currently, measuring sewer pipe water levels is being carried out as part of flood forecasting and damage prevention in Seoul, South Korea. However, the research on predicting sewer pipe water levels is insufficient and necessary. Therefore, this study predicted the sewer pipe water levels using the LSTM algorithm widely used in water level prediction research. We collected data on sewer pipe water levels from 25 points in Seoul. Since LSTM requires big data to perform deep learning, this study analyzed the Gangdong area where the least missing data among 25 points. We construct 5-, 10-, and 30-minute interval data through data in 1-minute intervals. We selected a week with significant sewer level fluctuations for accuracy analysis. In addition, the water level was predicted by adding rainfall data affecting sewer pipe water level. And the model performance was validated using an R square. This work was supported by the National Research Foundation of Korea (NRF) grant funded by the Korea government (MSIT) (No. 2021R1A2C200553012).


HS14-A019
Development of Rapid Flood Image Recognition Using Deep Learning Algorithm

Yuan-Fu ZENG#+, Gwo-Fong LIN, Cheng-Lin YANG
National Taiwan University, Taiwan

In recent years, the increased frequency of short-term, high-intensity rainfall events, caused by the intensification of climate change, has placed significant stress on urban and drainage facilities. Accurately predicting, detecting, measuring, and locating water volume and bodies can serve as the foundation for decision-making, enabling appropriate actions to minimize risk and loss. Therefore, developing an automatic and efficient flood image recognition system has become essential. Recent advances in deep learning have overcome the shortcomings of traditional technologies, particularly in the field of computer vision. Image segmentation technology has also gained significant attention in areas such as medical imaging, object tracking, image reconstruction, and intelligent transportation. In this study, we propose a deep learning-based flooded image recognition system, utilizing two widely-used image recognition models: DeepLabv3+ and Mask R-CNN. The accuracy of both models in detecting water bodies is compared, and the actual flooded area in the imagery is calculated. To prove the model's practicality, we applied it to intersection monitoring imagery in Taiwan, successfully identifying the flooded area and location with high accuracy and reliability. The proposed model can provide relevant emergency response units with an effective reference for flood management. This study highlights the significance of developing advanced flood image recognition systems, which can significantly contribute to reducing flood risk and loss.


HS14-A022
Semantic Standardization and Automatic Alert Application of Taiwan's Tangible Cultural Heritage Under the Flood Situation

Yu-Hua CHEN#+
National Science and Technology Center Disaster Reduction, Taiwan

With the rapid development of science and technology, the software and hardware of computer science are constantly innovating, the development of three-dimensional space is becoming more and more mature, and the concept of four-dimensional time series is also gradually emerging. Domestic and foreign are committed to formulating standards and regulations. Tangible cultural heritages are an important witness to the history of the country. It is located on the west side of the Pacific Ocean. And Taiwan, which is located in the volcanic and seismic belt around the Pacific Ocean, is one of the hot spots of natural disasters in the world. However, once the tangible cultural heritages are damaged, it will cause irreversible damage. This study refers to OGC (Open Geospatial Consortium, OGC) and OSM (Open Street Map, OSM) to formulate the three-dimensional semantic framework of tangible cultural heritages in the context of flooding disasters. It tries to filter through historical disaster data and flooding potential, cooperate with the Water Conservancy Department to announce the warning value of township flooding, and then use the system automation method to proactively Publish flood warning E-mail, string API, and system platform presentation, and provide diversified warning information, so that the competent authority can obtain the priority list of tangible cultural heritages before and during the disaster, so as to shorten the response decision-making time and achieve optimization management to reduce the risk of disasters to tangible cultural heritages.


HS14-A024
A Study on the Establishment of Flood Criteria for Vehicle Using a Survey

Cheonkyu CHOI#+, Hui-Seong NOH
Korea Institute of Civil Engineering and Building Technology, Korea, South

Recently, localized heavy rains have occurred due to the influence of climate change. When a flood occurs, it causes a lot of damage to property and human life located in the flood damaged area. In addition, traffic control and vehicle damage may occur on roads located in flooded areas. In this study, establishment of flood risk levels about vehicle according to the depth of flooding. First, selection of vehicle type for establishment of flood risk levels. And, In order to evaluate the risk according to the depth of flooding, the vehicle height calculates from the ground for each vehicle type. And, Conduct a survey of vehicle experts. This study has experience in repairing vehicles that suffered actual flood damage, and we conducted a survey of vehicle-related experts. The vehicle is divided into chassis, body, power train, interior, and electronic unit, and the degree of damage is evaluated according to the flood depth. In the future, it is considered that the flood criteria for vehicle can be used by determining the expected area of vehicle damage due to flooding.

ACKNOWLEDGEMENT
Research for this paper was carried out under the KICT Research Program (project no. 20230174-001, Development of Prediction and Monitoring Technology for Road Inundation based on Artificial Intelligence) funded by the Ministry of Science and ICT.


HS15-A005
Deep Learning-based Multi-source Soil Moisture Merging and Downscaling in Central Taiwan

Yu-Ru CHIOU+, Chia-Jeng CHEN#
National Chung Hsing University, Taiwan

Soil moisture (SM) is a critical component of the hydroclimate system, yet obtaining an accurate estimate of SM at high spatiotemporal resolution is still challenging. Three primary sources of SM information, namely satellite sensors, land surface models, and in-situ measurements, exhibit their own strengths and weaknesses in accuracy and spatiotemporal coverage. This study aims at conducting multi-source SM merging and downscaling based on Quadruple Collocation (QC) analysis and the Trajectory Gate Recurrent Unit (TrajGRU) model, respectively. QC method is used to merge SM data from Soil Moisture Active Passive (SMAP), Soil Moisture and Ocean Salinity (SMOS), Climate Change Initiative (CCI), and High Resolution Land Data Assimilation System (HRLDAS). TrajGRU is used to downscale the merged SM data from ~0.36° to 0.01° (~1 km) resolution based on the relationship between the SM data and auxiliary environmental variables (e.g., land surface temperature, land cover, elevation, and slope). Our analysis will be carried out in central Taiwan, and the merged and downscaled SM product is expected to not only resolve the issue of data scarcity but also support hydrological applications in this region.


HS15-A006
Global Snow and Ice Cover Dataset and Climatology Derived from 35 Years of Multi-satellite Observations

Peter ROMANOV#+
City University of New York, United States

Since 2006 NOAA has been using Global Multisensor Automated Snow and Ice Mapping System (GMASI) for operational monitoring of the Earth’s cryosphere. The GMASI system implements an automated algorithm which processes observations in the visible and infrared bands from the AVHRR sensor onboard NOAA and METOP satellites and observations in the microwave from SSMI and SSMIS sensors onboard DMSP satellites. The primary output of the system is a daily spatially-continuous (gap-free) maps of snow and ice cover at the spatial resolution of 4 km. The GMASI algorithm has been applied to process historical satellite data back to 1987 and to generate a high-resolution 30+ year-long daily dataset of global snow and ice cover. Daily data have been further used to produce monthly and yearly statistics of the snow and ice cover occurrence and to estimate long-term trends in the snow and ice extent. In the presentation we provide details on the data processing algorithm focusing on efforts to ensure consistency of retrievals across the 30+ year-long time period. Estimates of the snow and ice extent and corresponding long-term trends derived from the GMASI-reprocessed data are compared with the available coarse resolution snow cover climatology based on NOAA interactive snow and ice charts. The output of the GMASI system is shown to closely match the accuracy of snow maps produced within NOAA Interactive Multisensor Snow and Ice Mapping System (IMS) and to over-perform the existing coarse, 190 km, resolution, NOAA Snow Climate Data Record (CDR). The analysis of the Northern Hemisphere snow area extent changes over time estimated from the GMASI dataset supports earlier findings of a generally decreasing snow cover extent in late spring, and in summer and of its small increase in winter months.


HS15-A022
Estimation of Actual Evapotranspiration by Using Soil Moisture Data

Harshita Rani AHIRWAR#+, Anupam Kumar NEMA, Prashant K. SRIVASTAVA
Banaras Hindu University, India

The great importance of water is well-known worldwide. Also, its various forms are present on Earth. Alternation of any natural activity distress the life on the planet proving the importance of the water cycle. Hence, it becomes vital to understand every form of water, therefore, the moisture loss from the agricultural field and vegetation. The research work attempts to illuminate the process of actual evapotranspiration via soil characteristics (soil moisture, field capacity, and wilting point). The experiment was done for a single field considering the two extreme conditions of crop coefficient (fully vegetative and bear soil) to reach the results of actual evapotranspiration from potential evapotranspiration. From various combinations created, it was found that soil moisture data at a depth of 20cm gives a better result compared to the others like 5 cm and 50 cm depths and satellite data. Further, from standard and experimental values of field capacity and wilting point, the RMSE value of both was almost alike but standard values perform better. The research delivers that actual evapotranspiration can be calculated with minimum data generated in the field and has a lot more scope for the future to develop better algorithms.


HS15-A023
Examining the Extreme and Long-term 2022 Drought Event in the Southern Region of South Korea Using Remote Sensing-based Drought Index

Gwangsu PARK+, Won-Ho NAM#
Hankyong National University, Korea, South

Drought is a disaster that causes great social, economic, and environmental damage worldwide, and its occurrence frequency and magnitude are increasing due to recent abnormal climate. In the case of domestic drought monitoring, research is being conducted using satellite images that can provide periodic as a drought monitoring in ungauged areas. The drought index is used to quantitatively analyze and respond to drought damage, and representative drought indices include the probability distribution based Standard Precipitation Index (SPI) using ground precipitation data, the Standard Precipitation Evaporation Index (SPEI) including variability in precipitation and temperature, and Evaporation Stress Index (ESI) that predicts drought using satellite image data. The average temperature in spring 2022 (March to May) was the highest since 1973 weather observation, and May precipitation was the lowest ever, and as of June 6, cumulative rainfall was a national average of 193.6 mm, which was only 55% of the average year, resulting in an extreme drought. From July to August, the southern regions except the metropolitan area showed less precipitation compared to the average year, so the drought was not resolved even by the rainy season. Even, the drought duration has been reported to be the longest ever since 1974. In this study, the time series changes by individual indicators were analyzed for the spring drought in 2022 and the occurrence period of drought in the southern region using the drought index. In the case of SPI and SPEI, the temperature and precipitation in the weather station point data were utilized, and the ESI utilized satellite image data provided by the Terra MODIS (Moderate Resolution Imaging Spectroradiometer). Accordingly, there are compared drought indices and analyze spatio-temporal variability with respect to the overall cycle (preparation, occurrence, diffusion, deepening, and resolution) of extreme drought events due to continuous lack of precipitation in 2022.


HS16-A003
Inundation Risk and Its Impact Assessment on Groundnuts Under Climate Change in Yunlin County, Taiwan

Yi-Hua HSIAO1#+, Chun-Che CHEN1, Xing-Yu LIU1, Chih-Tsung HSU2, Dong-Sin SHIH3
1National Science and Technology Center for Disaster Reduction, Taiwan, 2National Center for High-Performance Computing, Taiwan, 3National Yang Ming Chiao Tung University, Taiwan

According to the 110-year agricultural land area statistics, the total area of Yunlin County is about 307.64 mi2, accounting for 61.73% of the total area of the county. It is mainly rich in rice, groundnuts. According to the statistics of typhoon and water damage losses in the past 20 years, the largest losses in one year are $440 million (typhoon) and $350 million (water damage), and the frequency of water damage is increasing. The types of disasters that groundnuts will be damaged are mainly typhoons and heavy rains. In addition to strong winds that cause dryness and affect the development of flower buds, inundation is more likely to cause losses. Therefore, this study uses typhoon event data under climate change scenarios to simulate future inundation disasters, and conduct risk assessment for groundnuts. The climate change data used is RCP8.5 dynamic downscaling HiRAM-WRF typhoon events, with a total of 149 in the base period (1979 to 2008), 450 in the middle of the 21st century (2040 to 2065) and 214 in the end of the 21st century (2075 to 2099). The SOBEK model was used to simulate the above typhoon events, and calculate the proportion of the worst inundation distribution above 0.3m within the groundnut planting range in Yunlin County in each period. The analysis results show that the average inundation occurrence probability is about 17.3% in the base period, about 15.0% in the middle of the 21st century, and about 22.5% in the end of the 21st century in the area where groundnuts are distributed. Overall, the increase in the scope and frequency of inundation is more likely to cause losses. The follow-up disaster reduction and adaptation assessment can be carried out early by the results of this study.


HS16-A006
Measuring Flow Field of Scouring Hole Using Laser Doppler Velocimetry

Wei-Feng TAI#+, Dong-Sin SHIH
National Yang Ming Chiao Tung University, Taiwan

Taiwan is located at the junction of the Eurasian plate and the Philippine Sea plate, pushing out a series of north-south mountains. The rivers primarily run east-west and have steep slopes in the flow channel. The bridges connect the towns and are essential for Taiwan's economy and population communication. In addition, many reservoirs or hydrological structures in Taiwan, such as sand check dams, fishways, and groundsill works...etc., are built upstream of the river, resulting in insufficient sand sources for bridge piers. Therefore, the scouring around the bridge pier of Taiwan is getting severe under extreme floods. In recent years, the global climate has intensified. The intensity of rainfall, the shortening of rainfall delay, and other factors have made sediment around the foundation of bridge piers more prone to local erosion. The traditional measurement of flow velocity and turbulence is mostly an invasive device that interferes with the flow field and may cause some measurement errors. This study tried using the open channel flume experiment to measure the flowing current of equivalent scour by the non-invasive Laser Doppler Velocimetry. The study also explores the relationship between the flow field and the scouring pit, then tries to identify the significance of turbulent flow intensity and maximum scouring. From measurements, the deepest erosion area is at the front of the horseshoe-shaped fossa flow area from the observed position. Furthermore, the area with the most significant turbulence intensity was about 1.2 times the diameter of the pier behind the pier.


HS16-A007
Analysis of Compound Flood Risk Using Trivariate Copulas

Jiun-Huei JANG#, Jun-Hao LIN+
National Cheng Kung University, Taiwan

For flooding triggered by multiple factors, flood risks are greatly influenced by the correlations of the triggering factors. In this study, trivariate copulas were used to describe the joint probability of rainfall (R), storm surge (T), and river discharge (Q) based on 28 historical events for a coastal area in Daan River, Taiwan. The model parameters were estimated using the maximum likelihood method, and the best-fit marginal and copula functions were selected using the Akaike Information Criterion and Bayesian Information Criterion. The results showed that R, T, and Q fitted Log-Normal, Gumbel, Gamma distributions, and the joint probability fitted Joe copulas the best. To estimate the compound flood risk simultaneously influenced by the R, T, and Q, Monte Carlo simulations were employed to generate numerous sets of (R, T, Q) based on the determined copula and served as boundary conditions for flood simulation. The simulated flood depths were used to establish a statistical model for calculating the return period for any set of (R, T, Q). The proposed method can be applied to different regions to enhance flood risk assessment and disaster management under the impact of compound flooding.


HS16-A011
Urban Restoration Priority Assessment Against Urban Flood Damage with Resilience

HyungJun PARK+, Chanjin JEONG, Hyun Jung LEE, Seungoh LEE#
Hongik University, Korea, South

Flood forecasting technology has been developing because the frequency and scale of damage of floods become increased due to globalized climate variability. At the same time, researches related to the evaluation of resilience, the ability to resist and restore after specific flood damage, are emerging as an important field. However, separate factors and methods were studied and presented for each case, and most of them focused on measuring only the resilience of facilities. Therefore, this study developed the blanket evaluation methodology for resilience degree that is able to consider additionally social and economic factors as well as facility one. Also, to reflect the temporal variation, it is subdivided into a dynamic factor that is affected by the time and a static factor that is less affected by the time. Facilities factor includes both buildings and infrastructures, and damage costs were quantified through the depth-damage functions in the literature. The resident characteristics and distribution, which were quantified through the ratio of the population affected by flooding and the flooded area ratio are considered in social factor. Lastly, economic factor related to recovery and resilience speed includes the regional income and resident income level, which were used as weighting factors for facilities and social factors. The time-damage graph for each zone was created using QGIS, one of popular GIS softwares, and resilience was calculated through it. Finally, after applying to the pilot urban area, the priority of urban restoration was visualized. By comparing and analyzing with the flood risk map, the areas that need to prepare for floods was listed. If further studies for additional factors such as industrial and policy factors will be conducted in the next time, it would be expected to be used as more precise reference materials to improve urban flood resilience.


HS17-A001
Flood Susceptibility Mapping Using Frequency Ratio and Weights of Evidence Models: A Study on Brahmaputra River Basin

Pritiranjan DAS#+, Netrananda SAHU
University of Delhi, India

Flood is one of the most devastating natural disasters worldwide and having great influence in the Indian sub-continent. Therefore, thorough flood control is required to mitigate the effects of flooding on human lives and livelihoods. The main aim of this study to examine the application of the frequency ratio (FR) and weights-of-evidence (WoE) models for flood susceptibility mapping in the Brahmaputra River basin. At first, a flood point data was prepared using Google Earth Engine (GEE) using global dataset and locations were identified in the study area. The flood point database was split as training data and testing dataset, 70% as training and 30% as testing dataset. Training database were used for model calibration and testing database used for the validation purposes. In the next step, flood influencing factors such as rainfall, elevation, slope, lithology, geology, land-use, distance from rivers, soil texture, slope angle, slope aspect, plan curvature, topographic wetness index (TWI). Each conditioning factor was used for flooding mapping using bivariate statistical analysis for flood susceptibility study. Following that, the receiver operating characteristic (ROC) curves for the obtained flood susceptibility maps were constructed, and the area under the curves (AUCs) were computed. The final results showed that the FR and WoE models produced nearly identical and fair outcomes. As a result, these flood susceptibility maps can help academics and planners in developing flood mitigation plans.


HS17-A003
River Sediment Prediction Based on Coupling WRF with GSSHA Models

Wen Yi LU+, Chia-Jeng CHEN#
National Chung Hsing University, Taiwan

Rainfall and runoff are responsible to the inception and transport of sediment over a catchment, respectively. New rainfall datasets available from satellite products (e.g., the Integrated Multi-satellitE Retrievals for Global precipitation measurement, IMERG) and numerical weather prediction models (e.g., Weather Research and Forecasting model, WRF) can provide more real-time information for river sediment analysis. In this study, rainfall data from IMERG and WRF are used to drive the Gridded Surface Subsurface Hydrologic Analysis model (GSSHA) to investigate the inception mechanisms of sediment motion and simulate the amount of sediment discharge in the Shimen Reservoir watershed in Taiwan. GSSHA is first calibrated with gauge-based rainfall and sediment discharge derived from rating curves to ensure a reasonable simulation of river runoff and sediment discharge at catchment outlets. Afterwards, by replacing gauge-based rainfall with IMERG or WRF rainfall, we are able to assess the predictability and physical mechanisms of sediment initiation and transportation. Preliminary results indicate that, as expected, the accuracy and spatiotemporal patterns of precipitation estimates are the determinant of the predictability of sediment discharge. The coupled modeling framework can indeed disclose the dynamics of sediment motion, pinning down the hotspots of soil erosion for further attention.


HS17-A004
Assessment of River Morphological Changes Based on Coupling WRF-Hydro with SRH-2D Models

Yi Yun LU+, Chia-Jeng CHEN#
National Chung Hsing University, Taiwan

Characteristics associated with surface runoff and sediment transport in a catchment can change drastically in response to extreme rainfall events, accelerating the evolution of river morphology. Modeling techniques can provide a means to assess transient changes in river morphology. This study aims at coupling the Weather Research and Forecasting model-Hydrological modeling system (WRF-Hydro) with a two-dimensional river hydraulic mobile-bed model referred to as the Sedimentation and River Hydraulics-2D (SRH-2D) to simulate rainfall-runoff and river bed changes in the Yousheng Creek in northern Taiwan. WRF-Hydro is able to simulate multi-scale land-atmosphere interactions and streamflow, while SRH-2D uses the hybrid mesh of quadrilateral and triangular cells to simulate various flow-related mechanisms, including river hydraulics, sediment transport, and river bed changes. WRF-Hydro is first calibrated to ensure a reasonable simulation of runoff at the downstream station to the Yousheng Creek, and then the simulated upstream runoff is used to drive SRH-2D to simulate multiple large flow events in a semi-consecutive fashion. It is found that simulated changes in the river bed over different cross sections mimic the survey data, suggesting the capability of such coupled modeling framework in predicting morphological changes. Under this framework, locations of channel erosion and deposition, found to be dependent upon the simulated flow velocity, can also be identified in great detail.


HS17-A010
Seasonal Variability of River Discharge and Profile Analysis Using Acoustic Doppler Current Profiler (ADCP): Monitoring the Agno River in San Carlos City, Pangasinan, Philippines

Kim Bryan CABRERA1#+, Decibel FAUSTINO-ESLAVA1, Juan Miguel GUOTANA2, Loucel CUI1, Jenielyn PADRONES1, Richard WILLIAMS3, Emma BILES4, Laura QUICK3, Patrick BYRNE4, Ylam Shalev MATBA1, Kennethjer ALEJO1, Francis GONZALVO1, Maria Regina REGALADO1
1University of the Philippines Los Baños, Philippines, 2University of the Philippines Diliman, Philippines, 3University of Glasgow, United Kingdom, 4Liverpool John Moores University, United Kingdom

Rivers provide insights into a watershed’s health and potential future trajectories. One of the crucial watersheds in the Philippines is the Agno Catchment. The Agno River is the most significant river within this catchment and provides food, sanitation, irrigation and livelihoods for local communities. Monitoring river discharge, paired with the analysis of water quality samples, can create contaminant flux estimations - which are valuable for estimating total pollution loads within rivers, particularly for highly modified (by agriculture, mining, and other land uses) regions. Estimating river discharge in wide and deep rivers, like the Agno River, requires a more advanced approach than handheld flow gauging used for smaller rivers. This study utilized a remote-controlled Acoustic Doppler Current Profiler (ADCP). Discharge data were collected from one representative site at the downstream section of the Agno River, using an ADCP. Monitorings were done during the wet and the dry seasons - representing the two pronounced seasons in the area. Data were collected for one month during each season with an average of six (6) transects per day. Data were then post-processed to achieve a ≤0.03 covariance for the discharge (Q). Average monthly wet and dry season discharges were 119.33 m3/s and 41.907 m3/s respectively. A transverse profile of the riverbed was also ascertained by recording depth values throughout each transect. Maximum and average river depth were also recorded for wet (8.01m, 3.36m) and dry (6.56m, 3.17m) seasons. Results from the study showed that the use of ADCP improved the monitoring of river discharge, making seasonal morphological changes more identifiable. Discharge data can be used as a baseline for planning activities of local government units for disaster risk reduction management. River discharge measurement results can then be correlated with water quality parameters for estimating contaminant fluxes.


HS19-A003
Performance Evaluation and Improvement of CMFD-based Precipitation Products Over Shanghai City, China

Nuo LEI#+, Zhengzheng ZHOU, Shuguang LIU, Guihui ZHONG, Sha LOU, Qi ZHUANG
Tongji University, China

Precipitation products with high resolution for urban areas remain an important and challenging issue. The main purposes of this study are to evaluate the accuracy of the China Meteorological Forcing Dataset (CMFD) in the Shanghai megacity and to improve the accuracy of the CMFD precipitation. With the rain gauge observations for the 2013-2018 period, we evaluate the error and detection ability of CMFD at the sub-daily, daily, monthly, and yearly scales, and examine the spatial variation of CMFD performance over the region. The Geographic Differential Analysis (GDA) method is used to calibrate the CMFD precipitation dataset. The results show that the performance of CMFD precipitation varies from sub-daily to annual time scales with better accuracy at the monthly scale in the study region. The CMFD can capture the spatial variability over the region with less error in the north and outliers in the center. The GDA-based calibration framework can significantly improve the capability of CMFD products, especially at the sub-daily and daily scales. The calibrated CMFD can provide reliable precipitation estimates and capture more extreme precipitation events. The improved CMFD products can provide a key basis for applications related to hydrological and meteorological hazard monitoring and assessment in the Shanghai area. The overall framework is scalable and could be readily generalized to other regions, and the calibrated product can be used in the research of urban natural disaster risks and other studies.


HS19-A008
Bivariate Rainfall Frequency Analysis in an Urban Watershed: Combining Copula Theory with Stochastic Storm Transposition

Qi ZHUANG#, Shuguang LIU, Zhengzheng ZHOU, Yuting JIN+
Tongji University, China

Extreme rainfall is a critical “agent” driving flash floods in urban areas. In rainfall frequency analysis (RFA), however, storms are usually assumed to be uniform in space and fixed in time. Spatially and temporally uniform design storms and area reduction factors are oftentimes used in conjunction with RFA results in engineering practice for infrastructure design and planning. The consequences of such assumptions are poorly understood. This study examines how spatiotemporal rainfall heterogeneity impacts RFA, using a newly-introduced bivariate framework consisting of copula theory and stochastic storm transposition (SST). A large number of regionally extreme storms with specific features—rainfall depth, duration, intensity, and level of intra-storm spatial organization—were collected. Rainfall intensity-duration-frequency (IDF) estimates exhibiting these bivariate features were then generated by synthesizing long records of rainfall via SST. The results show that dependencies exist among spatiotemporal storm characteristics. Bivariate frequency results exhibit smaller uncertainties but more complex physical meanings that the results from conventional methods. In particular, the highly spatially organized storms play a leading role in frequency estimates.


HS20-A009
Energy Distribution Within the Canopy Column

Kwanghun CHOI, Kyungrock PAIK#+
Korea University, Korea, South

Incoming Solar radiation on the terrestrial surface is distributed into various fluxes. The widely used surface energy balance equation treats the surface as 2-d entity. However, the Earth’s terrestrial surface is mostly covered by vegetation, rather than bare land. Energy distribution within the canopy column is complex: in addition to three (ground, sensible, latent) heat fluxes, redistribution within the canopy, photosynthesis, and heat captured within the vegetation body and canopy air needs to be considered. In this sense, 2-d assumption is limited and terrestrial surface should be seen as 3-d entity. Here we suggest the 3-d canopy column structure consisting of the hypothetical canopy column for the space of vegetation on the ground surface. Energy distribution within the 3-d canopy column using data from Fluxnet sites of different biome and climate will be carefully examined and presented with discussions.


HS21-A002
Safe Alternative Wet and Dry Irrigation to Increase Water Use Efficiency in Dry-season Rice Cultivation, Case Study: Cambodia

Chan Arun PHOEURN#+
Institute of Technology of Cambodia, Cambodia

Improving water use efficiency is considered globally as a key adaptive strategy for responding to climate change and for sustainable development to countries such as Cambodia where rice growing is the main source of income. The objective of the study is to evaluate the effectiveness of alternative wet and dry (AWD) compared to conventional flooding method in terms of water use efficiency and growth responses, and (2) to assess the tolerance level of rice toward different AWD severities. During AWD cycle, the field was re-irrigated whenever the water level in the field drops below -15 and -20 centimeters for AWD15 and AWD20, respectively. The field experiment was conducted at Cambodia Agricultural Research and Development Institute (CARDI) in 2021 and in Kampong Province in 2022. The Annova Test reveals that the yield, water productivity and the majority of phenological indicators such canopy cover, percentage of filled kernels, harvest index, and biomass of rice grown in AWD15 were not significantly different from those in CF condition. In terms of AWD application, CARDI could save the highest amount of water in AWD15 treatment equal to 34%, which is 12% and 11% higher than KTM 1 and KTM 2. Grain yield and WUE were not significantly different. Average yield was 3.59 t ha−1 in AWD15, 3.29 t ha−1 in AWD20, and 3.61 t ha−1 in CF, respectively. Average WUE was 0.52 kg m-3 in AWD15, 0.44 kg m-3 in AWD 20, and 0.40 kg -3 in CF, respectively. From this study, we can conclude that AWD could potentially be an adaptive measure for climate change to help farmers who grow rice in the dry season to save more input water.


HS21-A003
Study on the Multi-scale Regional Climate-vegetation-evaporation-runoff Relationship Based on Wavelet-Budyko Coupling Model

Wenting WEI+, Jun NIU#
China Agricultural University, China

This research provides a new method that combines wavelet analysis and the Budyko framework to study the multi-scale regional climate-vegetation-evaporation-runoff relationship. Based on this method, the driving mechanisms of regional climate change on hydrological processes are comprehensively analyzed, the factors that can be included in Budyko parameter estimation at different scales are determined, the contribution of climate change and human activities to regional hydrological water resources is quantitatively recognized, and the multi-scale relationship between regional climate-vegetation-evaporation-runoff is clarified, providing reference for the protection of the ecological environment, rational development and utilization of agriculture, and configuration and management of water resources in the Shiyang River Basin.


HS21-A007
Spatial-temporal Dynamics of Cropland Ecosystem Water-use Efficiency and Its Response to Climate Change and Human Activities in the Shiyang River Basin, Northwestern China

Fei TIAN#+
China Agricultural University, China

To deal with serious water resources crisis, the Shiyang River Basin (SRB) of Hexi Corridor in Northwestern China has been experiencing rehabilitation for water-saving since 2006. Water-use efficiency in cropland (WUEc) is a critical indicator to understand the response of carbon-water interactions. Because we currently lack a clear picture of how WUEc responds to climate and human activities factors in the SRB, here we applied Moderate Resolution Imaging Spectroradiometer (MODIS) satellite images to obtain a regional estimation of gross primary productivity in cropland (GPPc) and actual evapotranspiration in cropland (ETc), and analyzed the variations in WUEc and climate and human activities factors, then we evaluated the annual WUEc responses to climate and human activity factors and discussed major driving factors underlying the interannual variability (IAV) of WUEc from 2000 to 2014 in the SRB. Finally, we clarified the implications of the water saving project (WSP) on the water cycle. Results indicated that increased WUEc covered 97.25 % of the cropland area, with a trend of 0.017 g C kg−1 H2O yr-1. ETc decreased at 0.41 mm yr-1. ETc decreasing pixel mainly occurred in the irrigation districts of WSP completed by 2010. The IAV of WUEc was mainly determined by ETc (68 %) rather than GPPc (6%). The relative contribution of human activities factors in the WSP to ETc was 77.5 %, while that of climate factors was 22.5 %. Which further proved water availability increase was mainly artificially controlled, an effect of the WSP rather than that of climate factors.


HS21-A010
Optimal Cropping Patterns Can Be Conducive to Sustainable Irrigation: Evidence from the Drylands of Northwest China

Yunfei FAN+, Sufen WANG#
China Agricultural University, China

The pressures of frequent extreme weather, water shortages and increasing food demand pose a continued challenge of maintaining the sustainable development of irrigated agricultural systems. Although rational arable land management is fundamental to alleviating these pressures, the relationship between cropping patterns and irrigation sustainability is understudied. Using the Hexi Corridor as an example, a maximum entropy machine learning model was used to determine the optimal cropping pattern based on crop suitability and to explore the impact mechanism of the optimal cropping pattern on the irrigation sustainability index (SI) from the perspective of reliability, resilience, and vulnerability. An optimal cropping pattern was conducive to sustainable irrigation and reduced irrigation water use by 21.03% from 1960s–2010s with no continued agricultural expansion. Thus, the challenges of food security and sustainability for similar regions, and globally, can be met but will require major changes in cropping planning and management.


HS21-A011
Reallocating Crop Spatial Pattern Improves Agricultural Productivity and Irrigation Benefits Without Reducing Yields

Sufen WANG#+
China Agricultural University, China

The allocation of crop spatial pattern has an appreciable impact on achieving sustainable agricultural development. Crop spatial pattern should be adjusted in accordance with the agricultural environment factors and climate change so that we make full use of agricultural resources to produce more food. However, crop suitability has not been adequately considered in crop patterns, ignoring the fact that the fundamental solution to agricultural water scarcity is to promote crop water productivity (CWP). This study aims to reallocate crop spatial patterns while synergistically improving irrigation benefits and water productivity. To achieve this, we developed a minimum cumulative resistance (MCR) model based on ecological movement processes to simulate crop suitability distribution and thus determine crop spatial patterns. The results show that the adjusted crop pattern could increase the regional water productivity by 1.35 times and the net benefits of unit water by 0.94%, and maintained crop yields. Under future climate scenarios, this approach can still ensure irrigation benefits and food security. Therefore, the MCR model provides effective crop patterns and solutions for sustainable agricultural development when facing a complex agricultural environment.


HS21-A012
Surface Soil Moisture Assimilation Improves Subsurface Soil Moisture Estimation

Dehai LIAO+, Jun NIU#
China Agricultural University, China

Surface soil moisture is widely available from remotely sensed imagery, however, estimation of subsurface moisture has long been a common challenge for the scientific community. Here, we assimilate surface soil moisture into a physical hydrological model and use a dual state-parameter filtering method to jointly update the model parameters to better represent the physical processes of the model, ultimately achieving a better estimate of subsurface soil moisture.


HS21-A014
Analytical Modelling of Water Retention Across the Ecological Indexes and Hydrological Process Mechanism

Guangchuang ZHANG+, Yiping WU#
Xi'an Jiaotong University, China

Land water cycle and water resources health are important prerequisites to ensure regional sustainable development and ecosystem security. As an important part of ecosystem services, water retention function plays a vital role in the stability and sustainability of regional ecosystems. The weakening of its function will directly lead to the decrease of biodiversity, the aggravation of land desertification, and even the deterioration of local regional weather, etc., which will lead to the imbalance of the watershed ecosystem that was originally in dynamic balance, and then affect the landscape structure and ecological functions of the watershed ecosystem. In recent decades, scholars at home and abroad have done a lot of research on the service function of watershed ecosystem, especially the water retention function, with various research methods and perspectives. At present, the methods for calculating the water retention function mostly focus on discussing the variation law and its influencing factors of single or few hydrological factors (such as surface runoff, soil water, runoff yield), or only pay attention to the change and influence of vegetation growth, and some studies have been carried out on site scale through field sampling for local analysis and discussion. Most of the work often ignores the integrity of watershed ecosystem, and lacks the theoretical research on the water retention function of hydrological process and multi-factors of ecological system elements. The purpose of the present study is to provide a quantitative diagnosis method and system of water retention function integrating hydrological and ecological elements, so as to solve the problem in the existing methods, which only discusses watershed water retention quantity, but is difficult to reflect the function of vegetation conservation.


HS22-A002
Soil-moisture Derived Spatial Drought Prediction Using Long Short-term Memory (LSTM) Model in India

Vaibhav KUMAR#+, Hone-Jay CHU, Sumriti Ranjan PATRA
National Cheng Kung University, Taiwan

Drought is one of the costliest hydro-meteorological hazards, which poses a fundamental challenge to predict spatially and temporally. The severity and frequency of drought events have increased under the warming climate. It has sophisticated physical mechanics characterized by precipitation deficiency, having a ripple effect on agricultural and hydrological systems, which causes severe socio-economic damage, particularly in emerging countries like India. However, developing accurate and more reliable drought prediction models is challenging but essential for mitigation strategies and enhancing early warning systems. Even though the deep learning approach can enhance our comprehensive understanding of drought features, specifically spatial variations, intensity, and frequency, they have not been thoroughly explored. Therefore, this study proposes a deep learning method, specifically the Long Short-Term Memory (LSTM), to predict standardized soil-moisture index (SSI) at short-term time scales (SSI-06) over India region. This region has experienced severe droughts during this spanning period. The LSTM model utilizes soil-moisture and other hydro-meteorological variables (herein precipitation, potential evapotranspiration, and surface air temperature) as predictors acquired from the Global Land Evaporation Amsterdam Model (GLEAM), India Meteorological Department (IMD), and Climate Research Unit (CRU) datasets continuous from 1981 to 2020. The observed and predicted results were compared during monsoon season ((June to September) in the 2009 and 2015 severe drought years. Moreover, LSTM improves soil-moisture drought features and focuses on spatial variations, intensity, and frequency. Albeit having these drought characteristics, the model needs to tightly constrain to enhance forecasting accuracy and more reliable simulations over India. Further, the present study will strengthen soil-moisture drought conditions through a data-driven prediction model. It will be helpful for drought mitigation purposes.


HS22-A004
Multi-objective Extraction-injection Optimization Modeling for Saltwater Intrusion Control Using Machine Learning Models

Jina YIN#+, Ning WANG, Zhu LIU
Hohai University, China

Data-driven machine learning surrogates are used to substitute complex groundwater numerical simulation models within optimization algorithms to reduce computational burden for large-scale aquifer management. The traditional surrogate-assisted simulation-optimization modeling has been limited due to uncertainty persisting in surrogate model predictions. More advanced methods are imperative to reduce impact of uncertainties from surrogate models on solution optimality. In this regard, we propose an ensemble surrogate-based simulation-optimization methodology for optimal saltwater intrusion (SWI) control through accounting for uncertainty induced by surrogate models. The optimization model includes two conflicting objectives: minimizing total groundwater pumping and injection rate from an extraction-injection horizontal well system while reducing chloride concentration at monitoring locations below a certain level as much as possible. Three types of machine learning surrogates including artificial neural network, random forest and support vector machine were established to replace a high-fidelity physically based saltwater intrusion model. Optimal Latin hypercube design combined with parallel computing on high performance computing (HPC) was performed to generate input-output data of pumping and injection schedules and resulting salinity levels. An innovative Bayesian model averaging approach was presented to derive posterior model weights by considering big training and testing data. The newly constructed individual and ensemble machine learning surrogates were then coupled with a multi-objective optimization model to obtain Pareto-optimal extraction-injection strategies, where the optimization was solved using NSGA-II. Results showed that individual and ensemble surrogate models were accurate enough for salinity prediction. Through comparing the Pareto-optimal solutions, the ensemble surrogate-based modeling was confirmed to provide more reliable and conservative strategies for alleviating saltwater intrusion threat while considerably reducing computational cost.


HS22-A007
A Method of Solving Data Imbalance Problem to Improve the Performance of Data-driven Model for Estimating High-concentration Occurrence Probability for the Naturally Occurring Radioactive Materials in Groundwater

Hyeongmok LEE+, Jina JEONG#
Kyungpook National University, Korea, South

Groundwater can be easily contaminated by naturally occurring radioactive materials (NORMs) as it interacts with surrounding geological elements while moving through the primary and secondary pores of the underground medium for a long time. Therefore, it is necessary to efficiently evaluate groundwater contamination vulnerability to NORMs. In this study, a classification model to assess a high-concentration occurrence probability for NORMs in groundwater was developed based on the in-situ groundwater quality monitoring data and geological information, and its practical applicability was evaluated. For model implementation, random forest (RF), an ensemble machine learning model, was applied to develop the proposed model; the actual in-situ monitoring data (pH, temperature, Eh, EC, DOE, HCO3-) and the concentration of NORMs (238U and 222Rn) acquired from 201 locations were applied in this study. In particular, this study used data sampling techniques to solve the data imbalance problem and improve the performance of the developed model. The sampling techniques applied in this study are as follows: (1) under-sampling, (2) SMOTE (synthetic minority over-sampling technique), (3) complex sampling that comprehensively utilizes techniques of (1) and (2). The classification results showed that the accuracy of the model applying the sampling techniques was higher than the model without using the sampling techniques. In particular, techniques (3) and (2) showed superior performance for estimating the high-concentration occurrence probability of uranium (238U) and radon (222Rn), respectively. Data imbalance problem frequently occurs in developing data-driven geological estimation model. In this aspect, this study might be practical in suggesting a method to improve the performance of the estimation model. In addition, the developed model can contribute to the safety of the groundwater user by informing the risk of the NORMs in groundwater in real-time.


HS22-A011
A Hybrid Approach for Forecasting Flood Runoff by Combining a Rainfall-runoff Simulation Model and Deep Learning Networks

Kyung Soo JUN#, Kyung Soo JUN+
Sungkyunkwan University, Korea, South

Accurate prediction of flood runoff during storm events is essential for mitigating flood damages. Deep learning model is a powerful tool to address various practical problems, and it is extensively used for forecasting in diverse areas. However, as the forecast lead time increases, it shows poor performance because the output variable has less correlation with the input variables. In this study, hybrid models which integrate the outputs of physically based rainfall-runoff simulation model into data-driven deep learning models are proposed to predict hourly flood runoff from Yongdam Dam Basin in South Korea. Two types of hybrid models were established. One is the deep learning model that includes the runoff forecasted by a physically based simulation model as input variable. The other adopts error correction modeling that attempts to analyze the potential nonlinear relationships between the previous rainfall and runoff data and errors of runoff forecasted by the simulation model. Artificial neural networks (ANN) and HEC-HMS models were used for machine learning model and physically based simulation model, respectively. To assess the hybrid forecasting approach, performances of the physically based model, ANN based pure machine learning model, and the hybrid models were compared. Sixteen flood events were used for model calibration (or training) and validation. Various statistical indices were employed to assess prediction performance. The hybrid models showed better performance in prediction accuracy compared with the physically based rainfall-runoff simulation model or pure machine learning model especially as the forecasting lead time increases. This suggests that the hybrid models can take advantage of complementary strengths of both the simulation model and the deep learning model. Hence, the physically based simulation model coupled with deep learning model can be used for accurate forecasting of flood runoff. This study was supported by the Korea Environmental Industry and Technology Institute (KEITI) (Grant number: 2022003460001).


HS22-A012
Combining CNN and Transformer for Enhanced Daily Streamflow Forecasting: A Study on Lanyang Stream Basin

Wei Jin WANG#+, Weicheng LO
National Cheng Kung University, Taiwan

Flood disasters often result in significant losses of life and property and are considered one of the most devastating natural hazards. In recent years, the frequency and intensity of extreme rainfall events have increased significantly. As a result, reliable and accurate streamflow forecasting is of vital importance. Rainfall-runoff modeling is a complex and nonlinear time series process. In data-driven methods, numerous studies have demonstrated their promising performance in streamflow prediction by using deep learning approaches such as Long Short-Term Memory (LSTM), Convolutional Neural Network (CNN) and Transformer. This study proposes a deep learning framework that combines CNN and Transformer for rainfall-runoff modeling. The framework extracts precipitation and meteorological features of meteorological stations through self-attention mechanisms and aggregates these features and the streamflow data through cross-attention mechanisms. In this study, the proposed model is applied to the Lanyang Stream basin to validate its applicability to the task of streamflow forecasting by predicting the 5-day-ahead runoff. The results show that the proposed model significantly outperforms LSTM, CNN and traditional Transformer models in terms of the Root Mean Squared Error (RMSE) and the Nash–Sutcliffe Efficiency (NSE) for 1-day-ahead runoff predictions. Additionally, the results also indicate that the model has better performance for multiple-step-ahead runoff predictions.


HS22-A016
Development and Application of a High-resolution Urban Flood Model Based on Cellular Automata

Hyeonjin CHOI#+, Songhee LEE, Hyuna WOO, Seong Jin NOH
Kumoh National Institute of Technology, Korea, South

In this work, we propose and evaluate a high-resolution urban flood model based on cellular automata. Cellular Automata (CA), a rule-based machine learning model, has advantages over conventional physics-based flood models, especially in terms of computational efficiency in high-resolution predictions. Instead of solving the entire St. Venant equation, CA can relax computational limits without losing computational accuracy. However, user-defined rules in CA-based models can be a source of uncertainty leading to unstable predictions such as numerical oscillations. By reviewing several existing CA algorithms, we will discuss what conditions are needed for stable urban flood modeling, especially with high-resolution data. We will also show the performance of urban flood modeling with additional features such as adaptive time steps and GPU parallel computation. Finally, we will discuss how CA-based approaches can be efficiently integrated with physical and deep learning-based models to improve flood and hydrological predictions in urban areas.


HS22-A020
A Novel Approach for Image-based Rainfall Estimation with GAN and VAE: Focusing on Rainstreak Detection, Removal, and Generation

Jongyun BYUN, Hyeon-Joon KIM, Jinwook LEE, Jongjin BAIK, Ki-Hong PARK, Changhyun JUN#+
Chung-Ang University, Korea, South

In this study, a novel approach is proposed to estimate rainfall amounts from actual rainfall image datasets obtained by surveillance cameras. Here, basic characteristics of rainstreaks in a CCTV video are mainly investigated to find how to deal with rainstreaks’ information in terms of rainfall estimation with high accuracy. We selected two observation sites (i.e., Seoul and Jincheon) in Republic of Korea and used datasets obtained by rain gauges, disdrometers, and CCTVs from 1st March to 31th December 2022. At first, background subtractor algorithms (e.g. K-nearest neighbors (KNN), Gaussian Mixture-based Background/Foreground Segmentation Algorithm (MOG2)) were exploited to extract the rainsteak from CCTV raw data. Secondly, generative adversarial networks (GAN) and variational autoencoders (VAE) were applied to generate rainstreak datasets based on the extracted actual rainstreak data at the prior stage. The generated rainstreaks’ information were analyzed and compared under different experimental conditions such as initial values in the considered CCTV device (e.g., shutter speed, depth of field), rainfall parameter (e.g., drop size distribution, fall speed), and image background subtraction methods (e.g., KNN, MOG2). As results, it indicates that the GAN model has the advantage of being able to generate more realistic images and the VAE model has the advantage of learning in structural and effective latent space which enables the encoding of meaningful transformation in image data. It is also expected that the proposed approach with a generative model can be a fresh alternative in the field of rainfall estimation from characteristics of rainstreaks in image datasets. [Acknowledgement] This work was funded by the Korea Meteorological Administration Research and Development Program under Grant KMI2022-01910 and this work was supported by the National Research Foundation of Korea(NRF) grant funded by the Korea government(MSIT) (No. NRF-2022R1A4A3032838) and this work was funded by the Korea Meteorological Administration Research and Development Program under Grant RS-2023-00243008. 


HS25-A002
Environmental Issues in the Mekong Delta: Drivers, Consequences, and Management Outlooks

Edward PARK1#+, Duc Dung TRAN2,1, Huu Loc HO3
1Nanyang Technological University, Singapore, 2National Institute of Education and Earth Observatory of Singapore, Singapore, 3Asian Institute of Technology, Thailand

The flow of the Mekong is contributing to the delta’s richness and diversity of ecosystem services. Besides providing obvious ecosystem services such as water provision and natural soil fertilisation, the Mekong Delta (MD) also provides less obvious, but nonetheless, important services including protection against storm surges and carbon sequestration. However, the MD, like many mega deltas worldwide, has been constantly threatened by human activity on multiple geographical scales: (i) local: sand mining and groundwater extraction; (ii) trans-boundary: dam construction; and (iii) regional to global: climate change-induced salinity intrusion and sea-level rise. These environmental stressors have rendered critical threats toward various important ecosystem services of the MD, greatly affecting agricultural productivity and the livelihood of millions of inhabitants. In this article, we provide an overview of the current environmental issues plaguing the MD. Among the many issues (Arias et al., 2019), we focus on four of the most critical environmental challenges in the MD (sand mining, land subsidence, dam construction, and sea-level rise), and provide a review of their causes and environmental consequences. Management implications for the delta include transboundary water diplomacy, halting the sinking delta, and promoting sustainable agricultural practices.


HS25-A003
Uncertainty in Projected Agricultural Water Demand in the Ganges Delta of Bangladesh

Sonia Binte MURSHED1#+, Homin KIM2, Jagath KALUARACHCHI3
1Bangladesh University of Engineering and Technology, Bangladesh, 2Freeport-McMoRan, United States, 3Utah State University, United States

Understanding the climate change effects on agricultural water demand is crucial for the Ganges Delta of Bangladesh, which is an agriculture-dominated region. Evidence shows a decrease in agricultural land and loss of soil fertility in the region due to water scarcity, floods, droughts, and salinity intrusion. These concerns are the basis for this study to understand the potential impacts on future agricultural water demand under climate change. We used projected climate data (2020-2100) of three regional climate models along with their eight driving global climate models with moderate and high carbon emission scenarios (RCP 4.5 and 8.5). The analysis is used to assess the changes in climatic parameters, water loss, crop water requirement, irrigation water need, and freshwater availability. Random forest algorithm is used to predict future land cover data, and a complementary relationship model is used to estimate actual evapotranspiration. Crop water requirement is estimated and compared with freshwater availability to assess agricultural sustainability. We found high uncertainty among different climate model scenarios. A mean increase of 2 to 3°C temperature during the dry season is expected while rainfall shows a fluctuation pattern over time Although we found the possibility of decreased wet season rainfall up to 500 mm, there is also the possibility for opposite scenarios. In essence, the results suggest a wide uncertainty of rainfall and associated impacts. Therefore, irrigation water need is expected to increase by 18% to 60% from the historical (2001-2015) mean. Such an increase can seriously affect other water uses such as domestic, industries and in-stream. Quantifying uncertainty is therefore essential to develop adaptation plans to combat climate change effects. The findings of this study are helpful to develop economically feasible agricultural water management plans.


HS25-A009
Identification of Agricultural Drought-flood Abrupt Alternation Events in the Middle and Lower Reaches of the Yangtze River

Si CHEN#+, Peng HAN
Hubei University, China

The drought-flood abrupt alternation (DFAA), as an extreme event that coexist with drought and flood, is a serious natural disaster that poses a great threat to water resources and food security. At present, there are no unified definitions for DFAA, and its evolution characteristics are under study. In order to investigate the agricultural DFAA events and figure out the monitoring method, this study proposed the standardized soil moisture index (SSMI) based on the root zone soil moisture data from the Global Land Data Assimilation System from 1951 to 2020, and was used as the index to detect the onset/determination and turning point of the DFAA events in the middle and lower reaches of the Yangtze River. The detection accuracy was verified with historical recorded disaster data and the spatial and temporal evolution characteristics of agricultural DFAA events were analyzed. Results indicated that the SSMI exhibited an accuracy of 50%-62% in full detection of agricultural DFAA events in the study area. The observed events have gradually expanded and shifted southward since the 1950s. The frequency of DFAA events showed an increasing trend, with drought-to-flood events occurred mostly in the north-central part while flood-to-drought events occurred mostly in the south-central part. It was found that most of the moderate and severe DFAA events were concentrated in Anhui, Hubei and Zhejiang Province. The historical DFAA events mainly occurred during May to August, while drought-to-flood events occurred more frequently in June and July, and flood-to-drought events occurred more frequently in May and August. This study focused on the monitoring of DFAA events based on agricultural conditions and is expected to provide scientifical decision support for local water resources management.


HS25-A014
Study on Economic Game Logic of Groundwater Overexploitation

Chunfeng HAO#+
China Institute of Water Resources and Hydropower Research, China

To deal with significant decline of groundwater table along with eco-environment degradation in most regions of North China in past decades, China government has carried out a series of countermeasures on comprehensive treatment of groundwater overexploitation. The paper studies on the economic game logic of groundwater overexploitation by quantitatively analysis the actual benefits and losses with overall consideration of eco-environment and socio-economic systems to illustrate the institutional defect accounting for continuous ecological damage and the necessity of eco-environment value assessment in the check-up system of local government. Taking Fenhe river basin as an example, the second large sub-basin of the Yellow river in North China, the direct economic benefit of groundwater overexploitation is 12.0 billion yuan, the direct socio-economic loss is 846 million yuan, the indirect socio-economic loss is 116 million to 491 million yuan, and the ecological service value loss is 15.3 billion to 38.3 billion yuan. The net socio-economic benefit of groundwater overexploitation is as high as over 10 billion yuan, that’s why people prefer more groundwater exploitation in the past. However, by considering the eco-environmental impacts, the overall benefit becomes negative for local eco-environment and socio-economic systems. The loss of groundwater overexploitation is 27.6~164.6 yuan per cubic meter, over twice of the apparent socio-economic benefit. The efforts for effective treatment of groundwater overexploitation should be made from both administrative and market sides for a long-term mechanism by comprehensive assessment of local water resources management.


HS27-A007
Anthropogenic Activity Forcing Has Significantly Influenced Snowfall Changes in Eurasia

Wenqing LIN#, Han WANG+, Weiqi WANG, Dawei ZHANG, Fan WANG, Wuxia BI
China Institute of Water Resources and Hydropower Research, China

This study investigates the influence of external forcings on the various grades of snowfall (including light snowfall (<2.5 mm/day) and instense snowfall (>5mm/day)) over the Eurasian continent. Based on the phase 6 of the Coupled Model Intercomparison Project (CMIP6) multi-forcing dataset and regularized optimal fingerprint method, the detection and attribution of snowfall changes in Eurasia were carried out. Results show that All-forcing (ALL), anthropogenic activity forcing (ANT) and greenhouse gas forcing (GHG) well reproduced the spatial-temporal characteristics of snowfall. The influence of ANT on the changes in annual snowfall, light snowfall and its days over the Eurasian continent could be detected at the 90% confidence level. Moreover, the decreases of snowfall days and light snowfall also could be detected in GHG at the 90% confidence level. Thus, anthropogenic activities may considerably account for the decreases of snowfall days and light snowfall, wherein the GHG plays a dominant role. However, GHG underestimated the changes in snowfall days and light snowfall. Compared with observation, ALL, ANT and GHG significantly overestimated intense snowfall and its days, and couldn’t detected changes in them, which may be related to the low capability of models in simulating high levels of snowfall; thus, further improvement is needed.


HS27-A012
Complex Large-Scale Global Optimization based on Sea Anemone Optimization Algorithm

Xiaolong WANG1#, Guocheng AN1+, Dan WANG1, Qiang MA2, Philippe GOURBESVILLE 2
1Artificial Intelligence Research Institute of Shanghai Huaxun Network System Co., LTD., China, 2China Institute of Water Resources and Hydropower Research, China

Intelligent bionic optimization algorithms can effectively solve complex multimodal optimization problems compared with traditional optimization algorithms. In the paper, based on the anemone algorithm, the principle and effect of its application in complex optimization-seeking problems are investigated; it simulates anemone competition processes: covering, reproduction, convergence, exploration and elite processes. Its process and theory are discussed in detail, and the convergence process of the algorithm is explored. Based on the complex optimization problem test, the effectiveness of the anemone algorithm in solving complex optimization problems is verified. Thus its can be effectively applied in the optimization of parameters of hydrological model, etc., and it also has a wide range of application prospects in the remaining fields.


HS27-A016
Development of Flash Flood (Road Inundation) Real-time Monitoring and Response Technology Using AI

Hui-Seong NOH#+, Cheonkyu CHOI
Korea Institute of Civil Engineering and Building Technology, Korea, South

Flood damage is increasing as the frequency and intensity of torrential rains and typhoons increase due to global warming. In particular, in terms of road flooding, it is necessary to shift away from the post-processing system centered on 'recovery-compensation' to a proactive disaster response system through 'prevention-response-management'. This study aims to solve local issues related to flood damage targeting Jinju-si, Korea, with 'real-time road flood prediction, monitoring and operation technology', which can be the foundation technology for road flood-related disaster policies. It consists of empirical studies that combine various technologies such as flood analysis using rainfall prediction data, AI-based real-time monitoring using CCTV images, flood information based on spatial big data, and e-SOP.
ACKNOWLEDGEMENT
Research for this paper was carried out under the KICT Research Program (project no. 20230174-001, Development of Prediction and Monitoring Technology for Road Inundation based on Artificial Intelligence) funded by the Ministry of Science and ICT.


HS27-A022
Study on the Outburst Flood of Mazbach Ice Lake Based on Remote Sensing

Wei QU1#, Shuai LI2, Yuan YAO3, Tingting ZHANG2, Juan LU1, Changjun LIU1, WenlOng SONG4, Wenjing LU5+
1China Intstitue of Water Resources and Hydropower Research, China, 2Shenyang Agricultural University, China, 3North China University of Water Resources and Electric Power, China, 4China Institute of Water Resources and Hydropower Research, China, 5IAHR, China

In order to reveal the characteristics of the outburst flood of Mazbach Lake, the bottom topography of Mazbach lake was extracted based on the cartographic satellite data, and the water area changes before and after the ice lake outburst were extracted using the GF satellites and Sentinel-2 satellites. At the same time, combined with the water area - ice lake storage curve drawn based on the lake topographic data, the burst flood volume of the Mazbach Lake was calculated. Based on the flood volume, the HEC-RAS model is used to simulate the evolution process of the ice lake outburst flood, and the characteristics of the Mazbach lake outburst flood are analyzed.


HS27-A025
Assessment of Wave Runup on Seawalls in Southwestern Taiwan

Yun-Ta WU#+, Hsiao-Chu HUNG
National Cheng Kung University, Taiwan

Understanding wave runup process has been an important issue in designing coastal structures since it is highly related to coastal flooding. Taiwan is vulnerable to the pathways of typhoons from the Western North Pacific. To withstand the impacts from typhoon-induced long waves, more than half of Taiwan’s coastline has been protected by artificial structures, such as seawalls, indicating the urgent need for efficient and accurate estimates of wave runup on structures. In Taiwan empirical runup formulas developed by the US or European countries are frequently used to estimate the runup height levels. Since these runup formulas are not specifically designed for the coasts in Taiwan, additional correlation parameters should be applied. Having said that, these correction values are in general manually tuned for different locations. In this study, the main aim is to develop an integrated framework for estimating runup heights in the southwestern coasts of Taiwan. A new empirical runup formula has been developed which unifies the runup prediction capability for solitary waves, regular waves and irregular waves on uniform slopes. This new runup formula is then used to compare with those of field observed runup data during typhoon events on three seawalls in Southwestern Taiwan. Existing empirical runup formulas which have been frequently used are also used to compare with the present estimates and in-situ runup measurements. The comparisons indicate that the present runup model shows a higher value of index of agreement than the other empirical formulas. Since the present framework is essentially based on empirical formulas, it can serve as a quick estimation of wave runup and can be then utilized and optimized for nationwide applications in Taiwan.


HS28-A001
Research on Combining Mixed Reality Technology and Fracture Propagation Process by the Hybrid Domain Finite Element Model in Fractured Rocks

Chuen-Fa NI, I-Hsien LEE#+
National Central University, Taiwan

Fracture is the dominant pathway for groundwater flow and solute transport in fractured rock, and it plays an important role in the field of geology and engineering. Hydraulic fracturing is one of the methods for increasing the fractures and has been well-developed in these decades, however, it still has a serious of challenges to realize the fracture propagation mechanism by numerical method. Fracture tip displacement is one the mechanism for fracture propagation which influences the strength and hydraulic conductivity of geological medium and it is a critical issue for engineering. Mixed Reality helmets and the metaverse concept will be utilized to achieve synchronous/asynchronous operation and display by sharing virtual reality. The aim of this research is to review important issues such as fracture propagation, derivation of hydraulic-mechanical coupled numerical model, development of grid generation for fracture propagation unstructured, hybrid domain groundwater flow and transport simulation in fractured rocks, and combine with multi-person mixed reality technology and other important topics.


HS28-A002
Feasibility Study of Floodplain Dredging Using SRH-2D

Tzu Chieh SU#+, Weicheng LO
National Cheng Kung University, Taiwan

River sedimentation may impact hydraulic structures; in turn, threaten life and lead to loss of property. Therefore, river dredging and rectification are crucial for safety issue. However, traditional dredging methods are time-consuming and labor-intensive, as well as do not always work for all conditions. In addition, to protect the coastline from erosion, it needs to maintain sediments in estuaries. In this regard, the Sixth River Management Office has proposed a plan to disturb sediments in the floodplain; accordingly, they can be carried downstream during the event of high flow or reservoir recharge. This study thus aims to evaluate the feasibility of this proposed method by using the two-dimensional hydraulic sediment transport model, SRH-2D (Sedimentation and River Hydraulics – Two-Dimensional), developed by the Taiwan Water Resources Agency and the U.S. Bureau of Reclamation. Our numerical study reveals that Sections 78 to 88 of the Zengwen River are the suitable dredging locations to disturb the sediments. The influence of disturbance depth on dredging effectiveness to move the amount of sediments is quantified, providing a useful reference for future dredging projects. Typhoon Megi in 2016 is selected as the illustrative example for the high flow event. Our results show that the left bank of Sections 80 to 84 are acted on by greater shear stress, making them to serve as the appropriate dredging location. Additionally, we identify the optimal disturbance ranges and depths to maximize the dredging effectiveness, evidently implying that the proposed dredging method is feasible.


HS28-A012
Effective Pumping Scenario for Irrigation Reservoir : Case Study in Deasa

Jong Hyun PARK+, Hyunuk AN#
Chungnam National University, Korea, South

The water used for irrigation which comes from agricultural reservoirs should be ideally sourced from the reservoirs’ adjacent watershed areas. However, in situations that prevent regular collection methods, such as droughts or watershed areas become limited, water used for irrigation must be collected from alternative sources. In South Korea, 273 agricultural reservoirs are operated in conjunction with pump enabled facilities. Using regional characteristics, the aforementioned reservoirs perform water balance analyses which determine optimal levels of water supply. However, data collection is a challenge in Korean pump enabled facilities as storage rate data is usually only information available. Other important data, such as the amount of water supply and its effectiveness, is rarely collected or measured. To achieve efficient use and secure of water in agricultural reservoirs, it is crucial to analyze the effectiveness of pumping scenario and to prepare countermeasures for future events. In this study, meteorological data of 29 years (1991-2019) and water supply data from Daesa Reservoir which has been utilizing pumped-storage since 2016, were used to evaluate the water supply capacity. Comparing the water balance before and after utilizing water pumped storage, the water balance before pump storage was only 128 ha which is smaller than the irrigated area of 163ha. Scenario-based analysis was conducted by considering water supply amount, water supply period, year-end reservoir storage, and normal/drought year periods showed that the pumped-storage of water could increase the stored water volume by up to 10 and 62Mm3, depending on the scenarios.


HS28-A016
Assessment of the Embedded Risk Associated with the Daily Precipitation Dataset Over India

Neha GUPTA#+
Indian Institute of Technology, Ropar, India

In a country like India, changing climate has contributed to increased extreme precipitation events causing extensive damage to humans and nature. Changes in extreme precipitation have been investigated by examining the tail heaviness of daily precipitation datasets using different scalar and graphical methods. However, little is known about the actual tail risk associated with these extremes, especially among different climate types. This study shows the utility of a simple empirical risk function that provides a single concise value after analyzing the risk dispersion in tails, which host the extremes. Concentration Maps are developed to assess the risk attached to any dataset with respect to its right tail. Risk embedded into the tails is evaluated for the historical time period (1951–2019) over India, using a daily gridded precipitation dataset from IMD with a resolution of 0.250. A climate type is assigned to each grid based on a Köppen-Geiger (KG) climate classification system for which the embedded risk associated with daily precipitation datasets has been examined. Grids associated with the Tropical (BWh) followed by Polar (ET) had the most frequent and largest magnitudes of extreme precipitation as the tail risk are higher in these climate types. Proper risk estimation and assessment of extreme climatic events in a region-based framework are necessary for formulating effective response measures to cope, resist, and recover from the severe impact of extreme events in changing climate.


HS28-A017
Evaluation of Two High-resolution Soil Moisture Reanalysis Products Over Major Land Areas of China

Hongmei XU1#+, Qiuling WANG2
1China Meteorological Administration, China, 2National Climate Center, China Meteorological Administration, China

Soil moisture (SM) is one of the most important parameters of the boundary layer. In this study, the China Meteorological Administration Land data assimilation system (CLDAS) SM product, the Global Land data assimilation system (GLDAS) SM product are compared with observations from national automatic soil moisture stations. The results indicate that, (1) for 0~10cm and 10~40cm soil moisture, CLDAS outperforms GLDAS in all regions, with higher correlation coefficient and smaller root mean square error (for 0~10cm soil moisture, the COR of CLDAS in China Ⅰ to China Ⅴ is 0.94, 0.93, 0.91, 0.96 and 0.86, while the COR of GLDAS in the five regions is 0.64, 0.81, 0.75, 0.80 and 0.41; for 10~40cm soil moisture, the COR of CLDAS in China Ⅰ to China Ⅴ is 0.97, 0.88, 0.91, 0.97 and 0.82, while the COR of GLDAS in the five regions is 0.39, 0.75, 0.85, 0.35 and 0.61); (2) for 40~100cm soil moisture, CLDAS outperforms GLDAS in other regions except the southwest; (3) from the perspective of seasonal change trend, the two datasets are close to the observation of 0~10cm and 10~40cm in late summer and early autumn, but seriously overestimated in winter, meanwhile, for 40~100cm soil moisture, CLDAS can more accurately grasp the seasonal change trend, and GLDAS is seriously dry. Based on the evaluation results, it is helpful for researchers to select appropriate datasets for disaster monitoring and early warning, water and energy interaction research, and agro-meteorological modeling.


HS28-A018
Effect of Channel Adjustment on Sediment Transport

Yan-Pei HUANG#+, Weicheng LO
National Cheng Kung University, Taiwan

Sediment siltation in rivers often causes the instability of flow channels and aggravates their narrowing and deepening. Channel dredging is conventionally carried out in engineering practices to solve this problem. In Taiwan, dredging projects are often combined with soil and sand auctions, which usually fail due to the poor quality of riverbed sediments since they are customarily not useful for infrastructure construction. However, the problem of sediment siltation is urgent. Channel adjustment is another method for dredging, by altering the targeted channel section to guide the flow path to retreat back to the center of the channel. This is able to avoid the flow path towards the riverbank to damage its foot. In this study, the Sedimentation and River Hydraulics – two-dimensional model (SRH2D) is applied to conduct a moving bed analysis for the meandering river section from the downstream of the Danei Bridge to the upstream of the Zengwen Bridge, where is a S curve channel; the right bank is convex and then becomes concave. Our numerical model is established according to the digital elevation model (DEM) of the study area before and after river adjustment. Field river section-depth measurements implemented from 2011 to 2016 are applied for model calibration, while model verification is performed based on the remaining five-year measurements from 2017 to 2021. Variations in river roughness due to channel adjustment is indeed taken into account in our numerical calculation. Our results show that after channel adjustment, only a small amount of siltation occurs in the front section of the left bank because the flow path becomes stable and no longer towards the riverbank. Furthermore, erosion takes place mainly in the main channel alone. However, as simulated time increases, erosion tends to be towards the left bank and the erosion area accordingly becomes wider.


HS28-A024
Lagrangian-based Catchment-scale Rainstorm Frequency Analysis

Haochen YAN1+, Mingfu GUAN2#
1University of Hong Kong, Hong Kong SAR, 2The University of Hong Kong, Hong Kong SAR

Rainstorm frequency analysis is a fundamental procedure to learn about the characteristics of regional climate extremes for subsequent flood modeling, structure design, and risk analysis. Conventionally, rainstorm frequency analysis mainly relies on point observations of gauge stations under an Eulerian framework, i.e., the rainstorm intensities of a certain return period and a certain duration are calculated separately and statically in space. However, a significant portion of extreme rainfalls in southeast Asia is contributed by convective systems. Due to the spatial and temporal variability in each rainstorm event, a homogeneous rainfall pattern over the entire catchment can lead to spurious results of flood simulation. Besides, widely used interpolation techniques assuming the same exceeding probability among the relevant stations during an individual event also cause considerable errors, particularly for larger catchments. Despite an areal adjustment factor or the concept of regional frequency analysis can be incorporated, the spatial variability is only depicted in a statistical sense, and the temporal lagging effects induced by the storm evolution across the catchment are still omitted. Motivated by the issues mentioned above, our recent study aims to explore a new method for frequency analysis from the Lagrangian perspective, taking Hong Kong and its periphery as an example. The spatiotemporal statistics of individual rainstorms that appeared within the study domain are first extracted by a state-of-the-art tracking algorithm incorporating the Karman Filter method, based on a high spatiotemporal-resolution gridded dataset with a long time span (>20 years). The core intensities, mean transit speed and directions, dimensions, and life cycle, are considered to fit probability models under a Bayesian-copula-based framework. The disparities of spatiotemporal features obtained by the proposed Lagrangian-based approach against the Eulerian-based approach are elucidated; the associated consequences in flood modeling are discussed. Our study provides new insights and alternatives for regional rainstorm frequency characterization.


HS28-A027
Estimation of the Spatial Distribution of the Internal Density of River Embankment by Exploration Technology Using Cosmic Ray Muon

Keigo NAMIKAWA1#+, Naoki KOYAMA1, Taro KUSAGAYA2, Keiichi SUZUKI3, Tadashi YAMADA1
1Chuo University, Japan, 2NEC Corporation, Japan, 3Kawasaki Geological Engineering Co., Ltd., Japan

River embankments have been constructed and reconstructed to resist extensive damage due to failure. However, the soil materials and compaction methods used have varied over time, which can cause localized voids and land subsidence that can lead to failure. Therefore, it is very important to know the presence and location of low-density and weak areas inside embankments. There are few ways to detect them. For example, Geophysical exploration has been used to estimate inside of ground, but conventional methods do not provide information on ground based on its physical properties and require specialist skills and knowledge to estimate extent of weak points and to interpret the results. In this study, the aim is to study the effectiveness of exploration technology using cosmic ray muon for understanding the internal structure of embankments, which can directly determine the ground density and are suitable for the scale of embankment exploration (spatial resolution 0.1-1.0 m, exploration depth 1.0-10 m). To verify the validity of exploration using muon, the number of muons through the embankment is observed. To visualize the internal density distribution internal of the embankment, a tomography analysis was carried out in a way that the analytical values were independent of the initial values. The results of the analysis show that the analyzed density values internal the embankment generally agree with the actual embankment ground density data. Furthermore, the high-density areas representing the concrete are clearly visible. To improve the accuracy and resolution of the tomography analysis, a few cases of simultaneous observation by many muon detectors were executed. The results show that as the number of measurement points is increased, the analysis grid becomes smaller, and the high-density and low-density regions can be identified in more detail.


HS29-A001
A Study on the Optimal Design of Low-impact Development Technology Using K-LIDM

Joowon CHOI#+, Soonchul KWON, Youngsu JANG
Pusan National University, Korea, South

The collapse of urban water circulation systems is increasing due to the increase of impermeable layers due to urbanization. In particular, damages such as flooding in cities are occurring due to the increase in extreme rainfall and changes in rainfall patterns due to the global climate crisis. To solve these problems, the water management paradigm is changing from water supply, backwater and sewage maintenance to water circulation and water-sensitive cities for sustainable urban development and greening. In particular, the need for application to Low Impact Development (LID) for the restoration of the natural water cycle was emphasized. In this study, a study was conducted on the optimal design of low-impact development technology according to the flood management goal for the Korea GI&LID Center in Pusan ​​National University Yangsan Campus. Results were derived through runoff hydrograph analysis using the K-LIDM model using scenarios such as the area of ​​low-impact development technology for the center's disaster prevention performance.


HS29-A004
Impacts of the Environmental Changes on the Groundwater Contamination Potential

Sheng-Wei WANG#+, Yen-Yu CHEN, Chih-Yu LIN
Tamkang University, Taiwan

Groundwater is an important water resource in Taiwan. The hydrological events, industrial development, water resource depletion, and land use have caused variations in groundwater quality. The hydrological factor of rainfall and anthropogenic factor of land use are adopted in this study to evaluate the influence of environmental changes on groundwater quality characteristics. Since the unneglectable social-economic development of Taoyuan city may cause stress on groundwater quality, 20 years of monitoring data was collected, including the temperature, rainfall, land use, and groundwater quality. According to the results of the hypothesis test, a significant difference in rainfall, temperature, groundwater organic carbon, pH, and iron was found between dry and wet years. Per wet years, the positive correlations between rainfall, temperature, redox potential were determined by factor analysis. Frequently surface recharge caused oxygen infiltration and subsequence oxidative reactions in wet years. While the positive correlation among the rainfall, temperature, sulfate, and magnesium in dry years shows that mineral dissolution dominates groundwater characteristics. Moreover, the groundwater quality index (GWQI)was adopted for understanding the groundwater quality variation within 20 years. The results showed that the groundwater contamination potential in the first decade is higher than that in the last decade. Based on the distribution of GWQI by geostatistical analysis, the high potential area is different in two decades. The aggregation between contamination potential distribution and land use by applying the local indicators of spatial association (LISA). 20.7% decrease in high potential area and 4.5% increase in low potential presented the groundwater quality is gradually better. The process of urbanization limited industrial development and possible groundwater contamination. Groundwater recharge will be more significant in the future via extreme hydrological events, and the adjustment of land use of industry and agriculture in the high potential area will be an applicable adaptation to climate change.


HS29-A027
Optimal Reservoir Operations for Water Supply Under Forecast Uncertainty in Korea

Yeonju KIM#+, Young-Oh KIM, Joohyung LEE
Seoul National University, Korea, South

The Ensemble Streamflow Prediction (ESP) technique, which is the most widely employed statistical hydrological forecasting method under uncertainty, is designed for the water resource management since the 1940s, and it is actively applied to reservoir optimization around the world. Unfortunately, despite the hardship of obtaining forecast distributions, dam operation plans are being planned harnessing only single values of forecast such as the average or median, rather than the entire distribution, for operational convenience. This study aims to purpose a method of managing the water resources by utilizing the probability prediction distribution by itself, rather than the mean or median, and to show its effect on it. To this end, 21 multi-purpose dams in Korea were calculated according to the ratio of annual average inflow to total storage capacity (r). Then Dam Jangheung (JH, r = 0.8) and Dam Chuangju (CJ, r = 1.8) were selected as the subjects of the study among them. In addition, operating rules in response to the forecast distribution were derived by Stochastic Dynamic Programming (SDP), which can explicitly use the streamflow distribution. Since water supply is the most prioritized over other purposes for multi-purpose dams in Korea. The objective function was set to minimize the difference between the water supply and demand. The operating rules derived from this were simulated and the effect was evaluated through the reliability, resiliency, and vulnerability criteria. As a result, even the distribution of forecasts with the same average tended to release more conservatively as the variance increased. Through this study, it was shown that it is more reasonable to manage water resources utilizing distributions themselves rather than only the representative values. Furthermore, to obtain the distribution of this forecast, the utilization of ESP, which can perform statistical hydrological predictions, was also shown.


Fri-04 Aug | 8:15 - 10:00 | MR330
HS28 - General Topics in Hydrological Science

Session Chair(s):

HS28-A003
Verify of Groundwater Storage Changes in the Zhuoshui River Alluvial Fan in Taiwan by Complementing the GRACE and GRACE-FO Gravity Field Solutions with Singularity Spectrum Analysis

Yung-Hsun CHIEN#+, Hong Ru LIN, Jet-Chau WEN
National Yunlin University of Science and Technology

The Gravity Recovery and Climate Experiment (GRACE) approach allow for the estimation of groundwater storage in time and space, but 33 of the monthly gravity field solutions for GRACE and its follow-on mission (GRACE follow-up, GRACE-FO) have This inhibits the complete analysis and full utilization of GRACE gravity data. Moreover, since the spatial resolution of GRACE is limited to 200-500 km2 many studies have applied GRACE gravity data to explore groundwater storage at large scales (>200,000 km2), and less literature has applied the method to small-scale areas. Therefore, the purpose of this study is to use 2,561 km2 of the Turbid River alluvial fan in west-central Taiwan as the study site and to use Singular Spectrum Analysis (SSA) to compensate for missing data in GRACE and GRACE-FO gravity field solutions, and to estimate the change in groundwater storage in the Zhuoshui River Alluvial Fan in Taiwan from 2002 to 2022. In this study, we collected monthly data from 2002/04 to 2022/12 from NASA GRACE Center for Space Research at the University of Texas at Austin (CSR), and analyzed the principal component (PC) and empirical orthogonal function (EOF) of CSR data by SSA method, to create a new time series called Reconstructed Components RC for the GRACE and GRACE-FO gravity field solutions to compensate for missing data and the time series was used to verify the change of groundwater storage from 2002 to 2022 in the Zhuoshui River Alluvial Fan in Taiwan. Key words: Singularity Spectrum Analysis, GRACE, GRACE-FO, Zhuoshui River Alluvial Fan, Groundwater Storage Variability


HS28-A004
Analysis of Spatiotemporal Soil Erosion for Short-term Rainfall Events

Minho YEON+, Linh NGUYEN, May Thi Tuyet DO, Giha LEE#
Kyungpook National University

Soil erosion means soil particles detach from the soil body due to water and wind. Moreover, this environmental problem is getting worse by climate change. In South Korea, this phenomenon is mainly caused by water, especially short-term rainfall events, due to topography and climate characteristics. Therefore, it is essential to analyze soil erosion correctly to prevent and reduce it. This study analyzed spatiotemporal soil erosion using a physically based soil erosion model. First, we chose a model that reflects spatiotemporal variability because we have to explore when, where, and the amount of erosion and deposition. Secondly, we collected the study area’s climate, topography, and land use data and revised this data for this model. Thirdly, we ran this model and calibrated parameters with observed data such as discharge and sedimentation. As a result, soil erosion occurred in agricultural lands near urban areas, which is in line with the patterns of erosion and deposition found at the actual sites. The results of this study can serve as essential information for managing soil erosion control and conservation.


HS28-A008
Numerical Investigation on the Appearances of “Spatial Representativity” in Rainfall-runoff Processes

Kazuma SAITO#+, Yoshiyuki YOKOO
Fukushima University

Woods and Sivapalan (1995) demonstrated “spatial representativity” appears in rainfall-runoff processes, in which specific discharge from sub-catchment concentrates to a constant value as the area of each sub-watershed increases, based on observational data in two New Zealand catchments. Their results showed the “spatial representativity” gradually appears when sub-catchment area approaches to an area of 1 to 10 km2, indicating that spatial averaging and parameterization would be effective for rainfall-runoff modeling at the spatial resolution at 1 to 10 km2. However, their findings have not been fully verified to date. Hence we conducted numerical experiments to investigate how the "spatial representativity" appears in rainfall-runoff process using a distributed rainfall-runoff model which makes more realistic verifications than field observations. As the result, we found the sub-catchment specific normalized river discharge by the discharge at the lower end point tend to converge to a certain value with an increase in the sub-catchment area. We also found that the proportion of slower discharge components gradually increased with the increase of sub-catchment area. These results indicate that the sub-catchment specific, normalized discharge certainly converge to a constant value as sub-catchment area increases and such tendency would be caused by the increases in the proportion of the slower components.


HS28-A009
Preliminary Study on River Bedform Modeling Using Reaction-advection-diffusion Equation

Eisuke ARAKI#+, Yoshiyuki YOKOO
Fukushima University

It has been confirmed in the field of morphogenesis that stripes and mottled patterns occur under certain conditions using the reaction-diffusion equation, but there is no research in the field of river bedform research that explain their generation mechanism using reaction-diffusion equation or the reaction-advection-diffusion equation. Hence, this study attempted to clarify the possibility of modeling river bedform generation in terms of reaction-advection-diffusion equation. As the result, we could confirm that we can model river bedforms by the reaction-advection-diffusion model. However, we also confirmed that our model requires further improvements to completely represent the hydrographic experiments for riverbed morphology by Hoshino et al. (2016).


HS28-A010
Estimating Annual Transports and Mass Balance of Suspended Solids in the Japanese First-class Watersheds

Mayu TATENO#+, Yoshiyuki YOKOO
Fukushima University

We attempted to estimate suspended sediment transport rate in the downstream areas of all the 109 first-class rivers in Japan by using the relationship between suspended sediment transport rate L and river discharge Q, with the aim of understanding sediment transport across Japan and contributing to comprehensive sediment management at a watershed scale. We firstly collected the literature reporting the L-Q equations and graphs showing the relationship for clarifying the L-Q equations for all the 109 first-class rivers at their most downstream monitoring stations. Secondly, we used the L-Q equations to calculate the annual average suspended sediment transport rate, L, for all the monitoring stations. Thirdly, we calculated the annual average land uplift rates and the volumes for all the watersheds, to explore the sediment volume budget of 109 watersheds. The results showed that (1) suspended sediment transport was highest in the Shinano River basin and lowest in the Honmyou River basin, (2) the land uplift rates were higher in the areas around 40°N and the central parts of the Japanese Islands, (3) the volumetric increases were higher in the Hokkaido region, the areas around 40°N, and the central parts of the Japanese Islands, (4) the net volumetric increases were higher in the western Hokkaido, the areas around 40°N, and the Kinki region, (5) the rates of net volumetric increases were higher around 40°N. These basic data at a national scale would contribute to the comprehensive sediment and land managements in Japan.


HS28-A013
Estimation of 3D Permeability by Automatic Tracing of Observable Fractures Based on Permeability Tensor Theory

Yu TSUKURIMICHI1#+, Takato TAKEMURA1, Hinako HOSONO1,2
1Nihon University, 2National Institute of Advanced Industrial Science and Technology

For the use of underground space in the carbon capture storage (CCS) and radioactive waste disposal sites, it is important to determine the permeability. Fracture is the most important factor when considering permeability, and is the main water-pathway in the subsurface. The permeability has been measured by various methods, including laboratory experiments, field measurements, and numerical analysis. The permeability tensor theory is able to estimate the three-dimensional permeability using fracture traces in two-dimensional images based on the stereological method (Oda et al., 2002). Assuming that the fracture surfaces are parallel plates, the permeability anisotropy can be estimated as a tensor from the geometrical information of the fracture trace. It is essential to trace fractures accurately in this method, but computers have not been able to replace handpicking. Since fracture tracing by hand picking requires a large amount of work and the accuracy depends on the skill of the operator, computer-aided methods have been considered, but it is sufficiently accurate. Tsukurimichi et al. (2022) report that fractures as straight line extract from satellite images using the image analysis algorithm. They found that a single fracture was divided into several segments and that it was important to deal with noise when binarizing the image. Therefore, we investigated a fracture tracing method using machine learning. In this presentation, we compare the accuracy of fracture extraction and propose a package that performs fracture detection and permeability estimation.


Fri-04 Aug | 8:15 - 10:00 | MR336
HS28 - General Topics in Hydrological Science

Session Chair(s):

HS28-A022
Impacts of the Meteorological and Hydrological Drought on Hydroelectric Power Generation in South Korea

Jiyoung KIM+, Sung Ho BYUN, Taesik KIM, Tae-Woong KIM#
Hanyang University

Due to climate change accelerated by global warming, it is essential to expand renewable energy to reduce greenhouse gases (GHGs). Hydropower electricity generated by multipurpose dams is one of renewable energy that emits little GHGs. In recent years, due to frequent droughts, uncertainties in the hydroelectric power generation are increasing, for example, stopping hydroelectric power generation in the United States and Brazil. Therefore, this study evaluated the impact of meteorological and hydrological droughts on hydroelectric power generation using partial least squares-structural equation modeling (PLS-SEM). In this study, meteorological drought, hydrological drought, and hydroelectric power generation were used as latent variables. To represent hydroelectric power generation, the ratio of power generation performance to plan, power transaction volume, and power transaction amount were used as reflective indicators. To represent meteorological drought, SPI(Standardized Precipitation Index)3, SPI6, SPI9, SPI12 were set as reflective indicators, and hydrological drought, SSI(Standardized Streamflow Index)3, SSI6, SSI9, SSI12 were set as reflective indicators. As a result, the hypothesis that hydrological drought affects hydroelectric power generation was confirmed to be 0.381 and meteorological drought affects hydroelectric power generation was confirmed to be 0.231. This result means that the occurrence of drought affects the reduction of hydroelectric power generation, and hydrological drought has a significant impact on hydroelectric power generation more than meteorological drought. 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)(No.2022003610001).


HS28-A023
Evaluating the Impact of Adaptation Policies on Reducing Flood Damage in a Changing Climate

Seung Beom SEO1#+, Hee Won JEE1, Jaepil CHO2, Yeora CHAE3, Moon-Hwan LEE3
1University of Seoul, 2Integrated Watershed Management Institute, 3Korea Environment Institute

In this research, an evaluation framework on the reduction impact of climate change adaptation policies on flood damage was suggested. This aims for providing valuable information for governments to prioritize regional policy actions to mitigate flood damage. A non-linear regression analysis is used to develop a flood damage function that takes into account a climate variable and flood damage data. A logistic growth function is used to show that flood damage increases dramatically after a certain rainfall level and has a maximum threshold based on local conditions. Regional factors are also incorporated into the damage function to reflect the effect of adaptation strategies in the parameter of the flood damage function. By updating the parameters of the power function by reflecting two adaptation policies, it was found that flood damage decreases by 34 percent on average. Besides, future climate change scenarios are adopted for considering the agenda of limiting the increase in global average temperature announced in the Paris Agreement. In this study, +2℃ to +5℃ increase scenario was analyzed. To obtain extreme rainfall event for the future scenarios, frequency analysis was performed under the assumption of non-stationary characteristics that extreme rainfall occurrence characteristics may change over time. As a result, it was projected that the largest amount of flood damage would occur in Gangwon-do while Jeollabuk-do can take the largest reduction effect, approximately -82%, by implementing the adaptation policies. Under the +5℃ increase scenario, the amount of flood damage increased rapidly, which is align with the projection for 2060s from GCM-driven scenarios. Although there is inherent uncertainty in climate change projections, the importance of climate change adaptation policies should not be overlooked. 
Acknowledgement:
Thank study was supported by “Cooperative Research Program for Agriculture Science and Technology Development" (Project No. PJ015576)” Rural Development Administration.


HS28-A005
A Signal Processing-based Interpretation of the Nash-Sutcliffe Efficiency

Le DUC#+, Yohei SAWADA
The University of Tokyo

The Nash-Sutcliffe efficiency (NSE) is a widely used score in hydrology but is not common in the other environmental sciences. One of the reasons for its unpopularity is that its scientific meaning is somehow unclear in the literature. This study attempts to establish a solid foundation for NSE from the viewpoint of signal progressing. By assuming an additive error model between simulations and observations, it can be shown that NSE is equivalent to an important quantity in signal processing: the signal-to-noise ratio. Moreover, NSE and the Kling-Gupta efficiency (KGE) are shown to be equivalent, at least when there are no biases, in the sense that they measure the relative magnitude of the power of noise to the power of variation of observations. However, the theory reveals the failure of NSE in general cases when the additive error model is replaced by a mixed adaptive-multiplicative error model. A simple counterexample demonstrates that NSE can give misleading results in evaluating model performances. In order to secure the validity of NSE in practice, an extension of NSE is derived, which only requires to divide the traditional noise-to-signal ratio by a multiplicative factor.


HS28-A007
Correcting Systematic Bias in Dependence Representations in Climate Model Simulations – A Wavelet-based Approach

Cilcia KUSUMASTUTI1,2#+, Rajeshwar MEHROTRA1, Ashish SHARMA1
1UNSW Sydney, 2Petra Christian University

Auto- and cross-dependence structures of inter- and intra-climate variables are often required in hydrological studies. With the advancement in computing power, the latest generation of Climate Model Intercomparison Project 6 (CMIP6) provides improved performance for use in water resources planning for future. While model simulations show minimal bias in mean and standard deviation, the current climate simulations of some climate models of CMIP6 show a bias in the auto- and cross-dependence attributes in climate variables. Majority of commonly used BC approaches, such as simple linear scaling, quantile-based BC, and nested bias correction (NBC) focus on bias correcting individual climate variables and do not consider the cross-dependence structure across variables. To deal with the bias in the cross-dependence attribute, most univariate-BC approaches are extended into multivariate BC. However, complexity of these multivariate approaches increases with the number of variables or locations in space. Recently, time-frequency-based BC which employs the power of discrete and continuous wavelet transform (DWBC and CWBC) have been proposed to bias correct the mean, standard deviation, and variability, and maintain the continuity of climate change signal from current to future climate in the climate model simulations. Here, we evaluate the performance of CWBC in dealing with the auto- and cross-dependance structure of 7 (seven) climate variables. We examine the lag-1 and lag-2 auto-correlation, as well as the cross-correlation structure across the variables before and after bias correction. The results show that the univariate-CWBC can bias correct the auto- and cross-dependence attributes at multiple time scales. As the approach is applied to each variable separately at individual location, it offers no limitations in terms of number of variable and locations.


HS28-A011
Understanding Complex Forest-water Nexus in China

Mingfang ZHANG#+
University of Electronic Science and Technology of China

Forests covering an area of 220 million hectares play an important role in water cycle in China. Forest types and their corresponding ecohydrological processes are diverse resulted from a large span of climate gradients and complex topography in China. The studies of hydrological processes of natural forests and plantations at multiple spatial and temporal scales across climate gradients are crucial for water management and ecosystem protection in China. Although the history of forest hydrology dated back to 1850s, it was introduced and developed as a form discipline in China in 1960s. The development of forest hydrology in China is accompanied by its history of forest changes with dramatic forest loss due to harvesting prior to 1980s and followed by consistent forest gain especially attributed to a series of large-scale “Land Greening” programs such as Natural Forest Protection Plan and Cropland to Forest Project since the late 1990s. Accordingly, the early forest hydrology in China studies the hydrological impact of deforestation while the recent two decades has witnessed a growing studies on the effect of forestation on hydrology. This talk aims to (i) provide an overview of Chinese forest hydrology, to (ii) review prior research in forest hydrology in China, to (iii) identify knowledge gaps and provide a vision for future research on forest hydrology in China, and to (iv) provide scientific supports for water and forest management under a changing environment.


HS28-A021
Quantitative Driving Analysis of Climate on Potential Evapotranspiration in Loess Plateau Incorporating Synergistic Effects

Yao DU1+, 静 赵2#, Qiang HUANG1, Haidong GAO1
1Xi'an University of Technology, 2西安理工大学

In the context of global climate change, it is of great significance to reveal the spatiotemporal variation of potential evapotranspiration (ET0) and its response to climate change for further understanding the evolution mechanism of water cycle in changing environment. In this study, the P-M formula was utilized to calculate ET0 in 6 sub-basins of the Loess Plateau (LP) using the daily observed data from 84 meteorological stations. The Mann-Kendall trend test and Kriging interpolation were applied to analyze the temporal and spatial characteristics of ET0 on annual and seasonal scales. In addition, the multivariate adaptive regression splines model, sensitivity analysis and contribution rate were used to identify the driving factors of ET0 variations by considering the synergistic effect of multiple factors. Results showed that (1) ET0 showed an insignificant increase at a rate of 5.448mm/10a on the annual scale. At the seasonal scale, ET0 increased in spring and winter, but decreased in summer and autumn. Spatially, the annual average, spring, summer and autumn ET0 showed a trend of higher north-south and lower east-west; (2) The annual ET0 of LP is most sensitive to relative humidity (RH). At the seasonal scale, ET0 was most sensitive to sunshine hours(S) in spring and autumn, average temperature in summer and RH in winter; (3) RH is the main influencing factor of ET0 change in the LP. At the seasonal scale, wind speed (WS) and T dominated the ET0 variation in spring and winter, respectively. S dominated the ET0 variation in summer and autumn; (4) The variation trend and driving factors of ET0 in each sub-catchment were different from those in the LP, and there were significant differences among the sub-catchments. This study provides a reference for the sustainable development of vegetation restoration and the management of agricultural water resources in the LP.


Fri-04 Aug | 10:20 - 12:20 | MR330
HS22 - Big Data Analytics and Machine Learning in Hydrological and Climatological Studies

Session Chair(s): Ke-Sheng CHENG, National Taiwan University

HS22-A005
Network Flow Optimization for Agricultural Water Distribution in Frequency Domain

Chang-Ying LEE1,2+, Ming-Che HU1#
1National Taiwan University, 2National Taiwan University

The extreme hydrological events occurred in recent years seriously impact the water resource distribution in Taiwan. Under competition with civil and industrial water demand, the reduction of agricultural water supply is therefore the contingency strategy. However, the water supply transfer without considering complexity of the agricultural system could impair the system unrecoverably. This study will aim to develop a model to evaluate the optimal strategy for agricultural water distribution. The network flow programming is adopted as the backbone. The model in this study has two features: first, the flow data are presented as time-dependent function rather than constants, therefore this model could simulate dynamic water distribution over a time span. Second, the flow data are transformed from time domain into frequency domain by Fourier transformation, then using network flow model to simulate the optimal water distribution strategy in frequency domain. The proposed framework has practical significance for implement of agricultural water resources management and providing alternative view for determination of agricultural water distribution.


HS22-A008
A Physics-informed Data-driven Model Integrating Deep Learning Methods with an Optimization Algorithm for Hourly Inundation Forecasting in Urban Area

Bing-Chen JHONG#+
National Taiwan University of Science and Technology

Accurate forecast of hourly inundation depth during typhoons is critical for disaster prevention and emergency evacuation. This study aimed to improve the accuracy of inundation forecasting models and optimize the combination of input variables. To achieve this aim, a novel physics-informed data-driven model integrating deep-learning-based methods with an optimization algorithm is proposed. First, the data of inundation depths were simulated by a numerical model as the training and testing data for the proposed model. The hydrological data such as rain gauge observations were also adopted as model input. Second, an hourly inundation forecasting model based on deep learning methods is developed. Third, an optimization algorithm (e.g., genetic algorithm) is further integrated with the inundation forecasting model as the proposed model to improve model accuracy and optimize input variables. To highlight the accuracy of the proposed model, the conventional models using Back Propagation Neural Network (BPNN) and Support Vector Machine (SVM) are compared with the proposed model. An actual application to Yilan County, Taiwan is implemented to demonstrate the advantages of the proposed model. The results indicate that the proposed model outperforms the conventional models. Moreover, the input variables with suitable lag lengths can be appropriately optimized by the proposed model. The proposed physics-informed data-driven model is expected to be an useful tool for disaster prevention and mitigation.


HS22-A019
Generating an AI-based Pretraining Flood Database (AI-flood DB) Using a Transfer Learning Approach

Nobuaki KIMURA#+
National Agriculture and Food Research Organization

Deep neural networks (DNNs) have been recently applied to flood predictions in hydraulic engineering studies. One of the DNN weaknesses is that insufficient data result in the poor accuracy of flood predictions. To improve this weakness, transfer learning (TL) was coupled with a DNN-based flood prediction model in this study. In general, TL can transfer the features of source datasets into those of target datasets. For our method, the DNN model with TL is first pretrained using numerous flood datasets that were collected in source rivers, whose meteorologic characteristics are relatively similar. Secondly, the model is retrained using few flood datasets in a target river. The advantage of this method is that the pretrained DNN model can satisfactorily predict flood events using even few datasets for the flood events in the target river. Only few observed flood datasets were available in the target river, Onga River, located in a northern area in Kyushu (Japan). Our DNN model that embeds long, short-term memory architecture was pretrained using all available flood datasets (water level and rainfall) in multiple rivers in Kyushu except for the datasets of Onga River. The pretrained DNN model is referred as an AI-based pretraining flood database (hereafter, AI-flood DB). Then, the DNN with the AI-flood DB was retrained using the flood datasets except for the largest flood dataset (TOP 1) in Onga River. Finally, the model predicted TOP 1. The results demonstrate that the model with the AI-flood DB predicted more accurately than that without the AI-flood DB. The improvement rate of our method was 10–40% for 1–6 h lead times using quantitative error evaluation of the root mean square error. The flood peak was also improved. Our method may be used for large flood events in other rivers where only few datasets exist.


HS22-A009
Impact of Transbasin Diversion on Water Supply in Taipei

Han-Chi HSIAO#+, Wen-Cheng HUANG
National Taiwan Ocean University

Northern Taiwan is the political and technological center of Taiwan. The average annual rainfall is 2,934 mm. The demand for public and agricultural water is large. The use of water resources depends on the regulation and interaction of reservoirs. In order to relieve the water supply pressure of Shihmen Reservoir, Taiwan's water resources agency proposed a water diversion plan in 2021, planning to divert water from the upper reaches of Xindian River to Dahan River to reduce the risk of water shortage in Shihmen Reservoir. It is estimated that a maximum of 400,000 tons of water can be diverted per day, and 66.3 million tons of water can be diverted in a year.
Based on the daily flow of Xindian River (1988~2020), the operating rules of Taipei's Feitsui Reservoir, and the water demand of Taipei, this study conducts a simulation analysis to assess the impact of transbasin diversion on water supply in Taipei.
The results show that the current average water supply of Feitsui Reservoir is 906.80 MCM/yr, the overflow is 77.45 MCM/yr, the water shortage is 5.82 MCM/yr, and the shortage index (SI) is 0.02. On the other side, after water diversion, the water supply of Feitsui Reservoir increased slightly to 909.24 MCM/yr, the overflow slightly decreased to 75.04 MCM/yr, and the water shortage increased to 12.57 MCM/yr. The water shortage has apparently increased, and the SI has also changed to 0.09. Obviously, after water diversion, the water supply of Taipei will be affected, and the occurrence of water shortage will also increase.


HS22-A006
Risk-based Irrigation Decision-making for the Shihmen Reservoir Irrigation District of Taiwan

Ke-Sheng CHENG#+
National Taiwan University

In this study, we present an innovative risk-based irrigation decision-making approach for the Shihmen Reservoir Irrigation District in northern Taiwan. The approach derives the cumulative distribution function of the available volume for irrigation, by considering the initial reservoir storage and the cumulative reservoir inflow, and then calculates the risk of irrigation shortage, defined as the probability that the available volume for irrigation is lower than the irrigation water demand. A severe drought event that occurred in 2021 was used to demonstrate the application of the proposed approach. It was found that the drought mitigation measures taken by the Irrigation Agency for the 2021 drought event ensured a very low risk of irrigation shortage.


HS22-A017
The Localized Ghost Point Method for Two-dimensional Unsteady Burgers’ Equations

Chiung-Lin CHU+, Chia-Ming FAN#
National Taiwan Ocean University

In this study, the localized ghost point method (LGPM), a novel localized meshfree numerical method, is proposed to efficiently and accurately solve two-dimensional unsteady Burgers’ equations. The unsteady Burgers’ equations play an important role in Computational Fluid Dynamics, since it is a simple form of the Navier-Stokes equations. The LGPM, truly free from mesh generation and numerical quadrature, is formed by combining the ghost point method and the concept of localization. By distributing the ghost points within an extended domain, the LGPM outperforms the conventional localized radial basis function collocation method in terms of accuracy. Besides, by introducing the concept of localization to the ghost point method, a sparse system can be yielded and the numerical efficiency can be greatly improved. Since the numerical simulations of the LGPM can achieve high accuracy and outstanding efficiency, the LGPM is adopted for spatial discretization of the Burgers’ equations. Meanwhile, the fully implicit Euler method is responsible for temporal discretization and the Newton-Raphson method is used for solving the system of nonlinear algebraic equations at every time step. To demonstrate the merits of the proposed LGPM, several numerical examples involving two-dimensional unsteady Burgers’ equations in one and two variables are presented in this study. Furthermore, the directions of future researches, based on the provided numerical results and comparisons, will be discussed in this presentation.


HS22-A018
Numerical Solutions of Sloshing Problems by Using the Method of Fundamental Solutions and the Particle Swarm Optimization

Fu-Li CHANG+, Chia-Ming FAN#, Chiung-Lin CHU
National Taiwan Ocean University

In this study, the method of fundamental solutions (MFS) and the particle swarm optimization (PSO) are adopted to efficiently and accurately simulate two-dimensional sloshing phenomenon. In the sloshing problems, the free surface of fluid will continuously deform while the tank, partially filled with fluid, is exerted by external force. Since the computational domain will change with time, to accurately simulate the sloshing problems is very challenging from the viewpoint of computer simulation. In this study, the MFS is adopted for spatial discretization of the sloshing problems. The MFS, truly free from mesh generation and numerical quadrature, is one of the most-promising boundary-type meshless method; therefore, only boundary nodes and source are required during numerical simulation. In addition, the troublesome problems of the unknown positions of sources in the MFS is resolved by the PSO, which is one of the newly-proposed metaheuristic algorithms. In order to investigate the merits of the proposed combination of the MFS and the PSO for solving sloshing problems, numerical results and comparisons from several examples are provided. Besides, the influence of some factors on the numerical performance are systematically examined.


Fri-04 Aug | 10:20 - 12:20 | MR336
HS28 - General Topics in Hydrological Science

Session Chair(s):

HS28-A025
Hierarchical Bayesian Approach for Post Processing of Projected Streamflow Data

Jose GEORGE#+, Athira P
Indian Institute of Technology Palakkad

Climate change impact studies require a chain of models, involving multiple assumptions and simplifications. Thus, the predicted impacts include large uncertainties, often leading to inefficient adaptation policies. A probabilistic technique for correcting the biases in simulated streamflow data is developed, where the distribution of future simulations of streamflow are corrected using the historical observations. Using hindcast simulations of streamflow and historical observations, parameters for the probability distribution function P(Robserved,historical|Rsimulated,historical) are identified. This relation is then used to develop the corrected distribution for the projected streamflow, P(Rcorrected|Rsimulated,future). Parameters of the historical probability relation are identified using Bayesian updating with non-informative priors. The major assumption made in the study is that the historical observed data and the projected data follows log-normal distribution. The procedure is validated in the Bharathapuzha River Basin, India by correcting streamflow projections. Climate change information from an ensemble of climate models are used as input in the ArcSWAT hydrological model to generate streamflow projections for the region. The relationship between the observed and simulated streamflow is established through a conditional probability distribution updated using the Hierarchical Bayesian Approach for the period 1980-2000. The projected streamflow for the period 2001-2013 is then bias corrected using the established correction relationship. The performance of the approach is studied using the Kolmogorov–Smirnov test and the correlation coefficient for the period 2001-2013. The procedure is found to be able to correct the distributions of the projected streamflow and the null hypothesis of the K-S test that the corrected data and the observed data are from the same distribution is found to be satisfied at 90%confidence. The corrected data also shows correlation coefficient greater than 0.64 with the observed streamflow, while the uncorrected data show a correlation as low as -0.14.


HS28-A026
A Hydrological and Geomorphometric Approach for Integrated Assessment of Hydro-climate Extremes Using Geospatial Technology

Pawan Kumar CHAUBEY#+, Rajesh MALL, Prashant K. SRIVASTAVA
Banaras Hindu University

Globally changes in hydro-climate extremes, such as extreme precipitation influence human health, water resources, and natural environments. During the last few decades, India has observed an enormous increase in rainfall extremes during the summer monsoon (June to September) seasons of India. Flood hazard depends on factors such as Surface slope, amount of rain, drainage density, soil type, texture, etc. Also, Meteorological factors like extreme rainfall play a vital role in initiating and triggering geo-hazards such as floods (river and flash floods). Consequently, a comprehensive study is needed to evaluate the extreme rainfall events at a regional river basin level to understand the geomorphological characteristics and the pattern of rainfall events. Remote sensing (RS) and Geographic Information Systems (GIS) help in flood hazard or risk mapping for land use planning in flood-prone areas. In the above purview, the current research has focused on flood hazard or risk mapping over the Teesta River Basin (TRB). The standardized precipitation index (SPI) was used for deducing extreme rainfall incidences derived from the Tropical Rainfall Measuring Mission (TRMM) precipitation datasets. Sub-watersheds Rangeet has high peak flow, while the Ranpo, Lachung, and Lachen tributaries of TRB have the highest Drainage Density, indicating these sub-watersheds of TRB are highly vulnerable to flash floods situation. Also, the variations in heavy and intense precipitation events in a short time can be linked to extreme flood events, which lead to channel shifting and modifications over the Teesta River, which can be inferred from provided asymmetric factors and sinuosity index. The results show a significant increase in extreme events (23.37% number of events at the 90th percentile) that leads flooding in the first half of the 21st century.


HS28-A028
Surrogate Modeling-based Uncertainty Quantification of Distributed Land Surface Hydrological Models

Ruochen SUN#+, Qingyun DUAN
Hohai University

Surrogate methods are widely used for uncertainty quantification of hydrological models to improve computational efficiency. However, building a surrogate of a distributed land surface hydrological model with many output variables over large spatial and temporal domains is difficult and computationally intensive. We employ a deep autoregressive neural network to construct an accurate and reliable surrogate system of dynamic distributed model outputs. In this network, input and output fields are treated as images. The network uses a deep convolutional encoder-decoder architecture to take full advantage of the convolution in image processing. Moreover, the autoregressive strategy makes it good at handling the dynamic relationship between the time-varying model input and output. We apply this DL network to building a surrogate system of the Variable Infiltration Capacity (VIC) model simulated soil moisture over the Huaihe river basin of China. We also compare it to the long short-term memory (LSTM) model based surrogate method. The adopted deep autoregressive neural network can provide an accurate surrogate system of the high-dimensional dynamic outputs of the VIC model. In addition, it significantly outperforms the LSTM surrogate in approximating spatial patterns of VIC modelled soil moisture. This highly accurate and flexible surrogate system is promising for advancing uncertainty quantification of distributed land surface hydrological models, thus improving their predictive skills, especially in large-scale modeling.


HS28-A029
Temporal Variability of River Morphology: Intra-seasonal Insights from the Brahmaputra River

Abhishek DIXIT#, Subashisa DUTTA+, Chandan MAHANTA
Indian Institute of Technology Guwahati

We investigated the temporal variability of the Brahmaputra river's morphology on an intra-seasonal scale, which provides crucial insights into the dynamics of river channels and floodplains, especially during the monsoon season when significant changes occur due to high discharge and sediment transport. We selected a part of the river's braided floodplain reach and collected 22 Synthetic Aperture Radar (SAR) images of the Sentinel-1 satellite in Ground Range Detected (GRD) mode with a VV polarization band and a spatial resolution of 10 meters. The data were obtained from the period of April 2021 to October 2021 through Google Earth Engine, which included two major discharge peaks in July end and August end, preceded by three minor discharge peaks in mid-May, June, and July. Our observations show that the backscatter coefficient exhibited a local maximum during the periods of minor discharge peaks due to an increase in the river surface roughness caused by interaction with exposed sandbars. In contrast, during the later periods of major peaks, the backscatter coefficient remained unchanged, which suggests the presence of a stable channel with reduced morphological activity. We conclude that during the initial flooding events, sandbars contribute to energy dissipation and the formation of consistent flow paths that are not easily altered by subsequent flood events.


HS28-A030
A Spatio-temporal Urban Drainage Flood Analysis Applied to the Do Lo District in Ha Noi – Viet Nam

Ha DO MINH1,2#+, Gerald CORZO3, Wilmer BARRETO4, Chris ZEVENBERGEN3
1IHE Delft Institute for Water Education, The Netherlands, 2Delft University of Technology, 3IHE Delft Institute for Water Education, 4Catholic University of Temuco

Understanding the spatiotemporal characteristics of urban drainage floods is crucial for effective flood management and disaster risk reduction in cities. Unfortunately, current urban flood risk analysis often overlooks these characteristics due to challenges such as limited availability and integration of data, as well as the complexity of spatiotemporal analysis. To better understand and manage flood risk in cities, it is necessary to improve data collection, integration, and analysis techniques. Identifying flood-prone areas and understanding flood propagation patterns are key components of this effort, as the location and timing of rainfall can lead to different flood scenarios in different parts of the city. To address this, a study was conducted in Do Lo, Yen Nghia, Ha Dong, Ha Noi to simulate flood events in a 115-subcatchment area using SWMM5. The study included 21 rainfall scenarios extrapolated from three rainfall patterns collected from rainfall incidents in 2008, 2019, and 2020. The model was validated with flood events in 2020 and 2022. To assess rainfall movement sensitivities, two drifting rainfall scenarios were created. The study aimed to generate a spatiotemporal risk map that shows both spatial and temporal flood-prone areas and to provide a visual representation of the time priority for flood protection, evacuation, and prevention. A rate of flood change diagram was used to show the agility of the flood in time and to provide insight into the time limitations for flood preventive action. The study also assessed flood dynamics under different rainfall timelines, which can inform the development of nature-based solutions. Overall, this study provides a valuable contribution to the field of flood risk analysis by incorporating spatiotemporal analysis and highlighting the importance of considering the temporal dimension of floods in urban areas.


Fri-04 Aug | 1:10 - 3:10 | MR330
HS19 - Understanding Extreme Precipitation and Mitigation Potential Across Scales

Session Chair(s): Wenpeng ZHAO, National University of Singapore, Abhishek ABHISHEK, Indian Institute of Technology Roorkee, Li ZHOU, Sichuan University, Shuoyuan LIANG, Tokyo Institute of Technology

HS19-A001
Model-based Estimation of Long-duration Design Precipitation

Yusuke HIRAGA1#+, Yoshihiko ISERI2, Levent KAVVAS2, Michael WARNER3, Angela DUREN3, John ENGLAND3, Chris FRANS3
1Tohoku University, 2University of California, Davis, 3U.S. Army Corps of Engineers

In basins where extreme floods are driven by long-duration hydrometeorological processes, such as snow accumulation/melt or a series of storm events, design precipitation and flood need to be estimated on a basis of long-duration processes rather than only focusing on a flood peak or a single storm duration. This study proposes a new model-based methodology to estimate design precipitation for long durations during the winter and spring seasons through its application to the dam drainage areas in the Columbia River Basin. In the proposed framework, the Weather Research and Forecasting (WRF) model was used to maximize precipitation depths at the basins for the target storm events in the target water years. The precipitation maximization was performed using the Atmospheric Boundary Condition Shifting method and Relative Humidity Perturbation method with the Integrated Water Vapor Transport thresholds. Long-duration design precipitation was estimated replacing historical storm events by corresponding maximized storm events in a precipitation sequence. As a result, the greatest cumulative design precipitation depths during Oct-Mar were estimated to be 960.1 mm and 1,101.7 mm for the drainage areas of Bonneville and Libby Dams, respectively. To the author's knowledge, this is the first study to estimate design precipitation for long durations on the order of several months with accompanying atmospheric/land-surface fields. The estimated design precipitation and corresponding atmospheric/land-surface fields together will drive a snow and hydrologic model to estimate design flood at the basin in a future study.


HS19-A002
Thermodynamically Enhanced Precipitation Extremes Due to Anthropogenic Greenhouse Gases and Aerosols

Xuezhi TAN#+, Zeqin HUANG
Sun Yat-sen University

Responses of precipitation extremes to forcings by anthropogenic greenhouse gases (GHG) and aerosol (AER) emissions could significantly impact our society and ecosystems. Although human influences on changes in precipitation extremes are detectable, how precipitation extremes have responded to human-induced climate change remains unclear. Here we apply a robust physical scaling diagnostic on reanalysis-based and simulated precipitation extremes by global climate models to disentangle global and regional changes in historical precipitation extremes to thermodynamic and dynamic contributions from anthropogenic GHG and AER forcings. We show that despite large spatiotemporal uncertainties of dynamic contribution to regional changes in precipitation extremes, the increased thermodynamic effects of anthropogenic GHG on increasing precipitation extremes and the decreased thermodynamic effects of anthropogenic AER on reducing precipitation extremes have synergically resulted in the enhanced global precipitation extremes from 1960-2014. Increasing precipitation extremes are expected to exacerbate in the future, given that greenhouse gases warming will continue to increase while aerosol cooling will decrease in the coming decades.


HS19-A004
Projection of Future Precipitation and Extreme Events in the Indus River Basin

Hira SATTAR#+, Tsuyoshi KINOUCHI
Tokyo Institute of Technology

The Indus River Basin supports the lives of 180 million people. The water from the river is used for irrigation, hydropower, domestic and industrial supply. In recent years, the basin has been subjected to extreme climatic disasters, which are likely to be attributed to the global climate changes such as ENSO cycle. Therefore, it is of utmost importance to project the future precipitation in the basin considering the anthropogenic influences on future precipitation under different emission scenarios based on Shared Socio-economic Pathways (SSPs). In this study, a future with increased fossil-fuelled development (SSP5) and a future with intermediate challenges (SSP2) are considered for projection. Daily precipitation data from five GCMs, namely MIROC6, CNRM-ESM2-1, CAMS-CSM1-0, BCC-CSM2-MR and MRI-ESM2-0 were used. The raw GCM data is bias corrected by quantile delta mapping. An overall increase in precipitation was found for the period from 2015 to 2099 under SSP-5. The overall increase in precipitation is mainly explained by winter precipitation during the snowfall months, whereas the monsoon rain has been projected to decrease. The annual average precipitation in the basin increases dramatically after year 2080, with some years receiving an unprecedented precipitation amount of more than 1.4mm/day. Therefore, it can be concluded that the extreme precipitation events are likely to increase in intensity by the end of this century, although the heavy precipitation events are less frequent in the last half of the century. The trend of monthly precipitation was obtained for each GCM and was compared with the observed precipitation. It has been observed that BCC represents the monthly rainfall pattern in the basin more realistically as compared to other datasets. The projection of precipitation and selection of the most suited GCMs can be used in the estimation of impacts of climate change on extreme events in the future.


HS19-A006
Flood Risk Assessment on the Lake Kasumigaura Basin Under Changing Climate and Future Socio-economic Scenarios

Shuoyuan LIANG#+, Tsuyoshi KINOUCHI
Tokyo Institute of Technology

As global warming intensifies, issues such as sea level rise and extreme precipitation are becoming increasingly prominent. This study focuses on the Lake Kasumigaura Basin in Japan. Located next to the coast, Lake Kasumigaura is Japan’s second largest fresh water lake, with approximate 2200 square kilometre of its watershed area. This study integrates topographic data from multiple sources including satellite, aerial and radar bathymetry, and simulates flooding under compound scenarios such as sea level rise and extreme precipitation by applying HydroMT and the Super-Fast INundation of CoastS model to rapidly assess the present and future flood risk changes on the basin under different Shared Socioeconomic Pathways. The obtained flood risk maps will facilitate local decision-making of mitigation strategies and provide a useful reference for flood risk management in other areas.


HS19-A007
A New Bias Correction Approach of the Satellite Precipitation Products with Limited Gauges

Li ZHOU1#+, Yufeng REN2, Gretchen KALONJI1
1Sichuan University, 2China Yangtze Power Co., Ltd

Satellite precipitation products (SPPs) have advanced remarkably in recent decades. However, the bias correction of SPPs still performs unsatisfied in the case of a limited rain gauge network. This paper proposes a new real-time bias correction approach that includes three steps to improve the precipitation quality with limited gauges in the Min River Basin, China. We employed 66 gauges as available ground observation precipitation, APHRODITE (Asian Precipitation-Highly Resolved Observational Data Integration Towards Evaluation of Water Resources) as the historical precipitation to correct GNOW and GNRT in 2020. A total of 1020 auto-rainfall stations were used as the benchmark to evaluate the original and corrected SPPs with six criteria. The results show that the statistic and dynamic bias correction method (SDBC) improved the SPPs significantly and the cumulative distribution function matching method (CDF) could reduce the overcorrection error from SDBC. The inverse error variance weighting method (IEVW) integrations of GNOW and GNRT didn't have obvious improvement as they are using similar hardware and software processes. It is recommended to employ different SPPs for integration. In general, the proposed bias correction approach has great significance for precipitation estimation and flood prediction in data-sparse basins worldwide.


Fri-04 Aug | 1:10 - 3:10 | MR336
HS20 - Hydrology for Human-nature Coupled System

Session Chair(s): Ting Fong May CHUI, The University of Hong Kong, Jian-Ping SUEN, National Cheng Kung University

HS20-A002
The Investigation of Decreasing Subsurface Water in Wetland

Chih-Chung WU#+, Jian-Ping SUEN
National Cheng Kung University

The upwelling of hyporheic flow could improve the water quality of the surface water (due to the biogeochemical reactions in the hyporheic zone) and provide sufficient water for the aquatic ecosystem. Wu Gou Shui wetland locates at Ping-Tung County, Taiwan. The main water supply in Wu Gou Shui wetland during the dry season (November to March) are groundwater and the upwelling of hyporheic water, the subsurface water resources provide purified water to maintain the aquatic ecosystem for the local species, and make it a well-function wetland with biodiversity. In recent years, the water level in Wu Gou Shui wetland seem to decrease and the dry up of the wetland came earlier than usual. In this research, 20 years of hydraulic data, including precipitation and the water level of observation wells, were collected and analyzed. MODFLOW simulation was performed to view the change of the groundwater level in Wu Gou Shui wetland. The results showed that the decreasing of precipitation could be the reason that caused the decreasing of water level in Wu Gou Shui wetland, and the rise of temperature (more evaporation) could be another reason as well. However, there are serval reasons, such as change of landscape and land use, drawdown in the adjacent area, and evapotranspiration, for the decreasing of water level in Wu Gou Shui wetland. Further investigation should be done to have a better understanding on the decreasing of water resource in the wetland fed by the subsurface water.


HS20-A005 | Invited
Recent Intensification of Riverbed Mining in the Mekong Delta Revealed by Extensive Bathymetric Surveying

Rachel LAU1, Edward PARK1#, Duc Dung TRAN2,1+
1Nanyang Technological University, 2National Institute of Education and Earth Observatory of Singapore

Large-scale sand extraction has had significant and compounding impacts on the riverine environment of the Vietnamese Mekong Delta (VMD). Yet, effective and targeted implementation of regulations and sustainable management remains hindered by scant data availability, limiting a comprehensive understanding of the delta's sand mining scale and extent. This study assessed recent intensifying patterns of sand mining activities in the VMD mainly based on extensive bathymetric surveys carried out across 800 km2 of the VMD river channel from 2017-2022. Our results revealed severe riverbed deepening across the VMD, particularly in the upper reaches of the Hau (Bassac) and Tien (Mekong) Rivers, which recorded mean incisions of 1.7 m from 2017-2022, and 1.3 m during 2017-2020, respectively. Accordingly, sediment losses amount to approximately 208 Mm3 in the upper reach of the Hau river, and 127 Mm3 in the upper reach of the Tien river. The highly variable incisions over both spatial and temporal scales, coupled with widespread sand mining pockmarks along much of the longitudinal and cross-sectional profiles of the riverbed, affirmed the major contribution of sand mining activities to changes in riverbed morphology. Its intensification in recent years is also evident from the progressive lowering of riverbed elevation. Additionally, field surveys highlighted the proximity of perceived sites of bank collapse to pitted riverbeds, providing reliable indications of sand mining-induced erosion. Ultimately, we intend for this evidence-based assessment of sand mining activities in the VMD to contribute to informed quantitative assessments of sediment budgets and effective implementation of regulatory frameworks for sustainable sand mining in the future.


HS20-A008
Proposing a New Landscape Evolution Model Capable of Simulating Transport of Mixed-size Grains

Dongwoon KANG+, Kyungrock PAIK#
Korea University

Natural rivers are composed of particles of various sizes and the sediment transport rate of each grain size significantly differs depending on their compositions. There have been great progress in developing sediment transport formula for mixed grains. Further, 1-d morphodynamic models have been developed on the basis of such formula. Nevertheless, most whole landscape evolution models still assume uniform grain size. We, for the first time, propose to develop a new landscape evolution model that can consider the transport of mixed-size grains, on the basis of Wilcock and Crowe(2003) formula. The model takes into consideration the hiding function and applies to each particle the threshold distinct from the homogeneous sediment. The model enables the calculation and simulation of the fractional sediment transport rate for each size in the whole landscape evolution. Topography evolution can be simulated numerically by solving the equations based on a physical process, which will be presented with technical details.


HS20-A010
Stability of Slopes Implemented with Stepped Bioretention Cells

Boji CHEN, Ting Fong May CHUI#+
The University of Hong Kong

There is a growing demand of implementing Green infrastructures (GIs) in slopes given its diverse benefits. However, GIs change the surface topography and affect the subsurface hydrology, thereby reduce slope stability. This study examined the stability of slopes implemented with stepped bioretention cells which are a common form of GIs implemented in slopes. It developed a numerical model to simulate the associated hydrological and geomechanical processes. Constructing bioretention cells in slopes result in cut-and-fill slopes if there are no reinforcements. Results shows that the cut and fill significantly reduces slope stability. Formation of the groundwater mound beneath the BCs would further decrease the slope stability. It is generally safe to implement GIs in gentler slopes using the cut and fill method, but additional reinforcement measures would be required for steeper slopes to ensure stability.


HS20-A006
Flood Extent Mapping and Damage Assessment Using Optical and SAR Imagery a Case Study of the Lower Indus Basin, Pakistan

Sidrah HAFEEZ1#+, Mingfu GUAN2, Dapeng YU3,4
1The University of Hong Kong and Previsico Asia Limited, 2The University of Hong Kong, 3Loughborough University, 4Previsico Asia Limited

Floods are becoming frequent and severe due to climate change impacts. Near real-time mapping of flood extent, and damage assessment are curial for flood management, relief operations, and risk mitigation planning. This task is challenging and time-consuming with conventional land-based techniques. However, mapping floods and their impacts utilizing open-source high-resolution optical and synthetic-aperture radar (SAR) satellite data is fast and cost-effective choice. In this study, open-source optical data from Landsat and Sentinel-2 missions and SAR data from Senetinel-1 mission were considered to map flood extent in the Lower Indus basin of Pakistan. This area is affected by seasonal flooding, however, in the past decade, flood events are becoming more devastating. Floods caused huge life and economic loss in the area. Large flood events of the year 2010, 2015 and 2022 were considered for flood extent mapping and damage assessment. Multiple spectral indices and classification methods were used and compared for extracting the flooded area from optical satellite imagery. Permanent water features were masked from the water layer to find the flooded area. In SAR images, water bodies and inundated areas usually show lower backscatter than dry land. Thresholding and classification techniques were used to extract the inundated areas from SAR images. Inundated areas were mapped by comparing SAR images during and before flood events. Flooded areas extracted by optical and SAR data were compared for validating spatial agreement between both data sets. Low-lying areas were highlighted using digital elevation model (DEM) data and the time to maximum flooding for the 2010, 2015 and 2022 flood seasons was determined. For damage assessment landuse landcover data, crop classification layer and settlement layer were used in GIS overlay analysis. Our analysis highlighted that using optical and SAR data in collaboration can provide near real-time flood mapping to start early relief activities.


HS20-A007
Rescaled Width Function Considering the Spatial Distribution of Flow Velocity to Reproduce Flood Hydrographs

Jisoo LEE+, Kyungrock PAIK#
Korea University

It has been known that direct runoff hydrograph is largely explained by geomorphological setting of a given catchment. On that basis, geomorphological unit hydrograph theories have been suggested with various mathematical modeling structures. One of the promising models is to utilize the topographic width function, which represents the topological characteristics of a river network as a function of distance from the outlet. Although the width function should capture direct runoff hydrograph in theory, real width function often very differs from observations. In an earlier study, the heterogeneous flow velocity between hillslope and channel was taken into account, leading to the rescaled width function. While this is an improvement, the rescaled width function is still limited for practical applications in that no consideration is given about the velocity variation through channels. In this study, we aim to revise a rescaled width function to consider the complete spatial variability in the overland flow velocity across catchment. We anticipate the new model would shed a light in practical usage of geomorphic information in flood hydrograph simulations. Case study for a study catchment in South Korea will be presented with model details.


HS20-A011
Optimal Irrigation Water Allocation Among Different Growth Stages

Gene Jiing-Yun YOU#+, Yu-Syuan CAI
National Taiwan University

Different from other water uses which utilization any time, irrigation is not only a matter of quantity, it is more important to accurately schedule according to the water demand of crops. However, in many studies in the field of water resources or agriculture, the non-rejuvenation of crop growth is usually ignored when calculating crop yield. These studies usually simply assume that irrigation water is effective in each period, and finally add up the yield of each period as the total benefit of irrigation. To solve this problem, the study aims to explore the dynamic decision-making of irrigation schedules with the consideration of uncertainty under water scarcity. Considering the charatersitcs of crop growth, we propose an analytical model in the form of a max-inf problem to investigate a two-stage stochastic optimal allocation of water to maximize the yield expectations of the two stages. With FAO 33, an empirical production function assessing the yield response to water, we need to apply the concept of max-inf to determine the expected yield. Accordingly, we found the optimal condition which maximizing the yield, satisfying a linear relationship between the probability of the first stage dominance and the water demand and yield response factor of the two stages. With this optimal condition, we can use the known crop water demand and yield response factor to estimate the probability of the first stage dominance, and adjust the irrigation water to achieve the condition of maximum yield expectation, to achieve the goal of maximum yield. So far the decision is still discussed within two-stage framework. It is expected extending to multi-stage framework which could more reasonable presentation of crop yield decision. By this way, this study can better help us to understand irrigation decision-making among different water supply stage under uncertainty.


HS20-A003
Application of Intraspecific Competition of the Benthic Fish Species in Nanzihsian Stream for River Habitat Restoration

Lu YING-SHENG+, Jian-Ping SUEN#
National Cheng Kung University

There are many factors that affect the distribution of fish populations, which can be roughly divided into biological factors (such as competition) and abiotic factors (such as floods, temperature). The intraspecific competition of fish is mostly resource competition or interference competition, and there is a lack of research on further analysis of intraspecific resource competition at different life stages. In this study, the benthic fish species, Sinogastromyzon nantaiensis, which is highly sensitive to riffle habitat was selected. The study reaches were hit by a devastating flood in 2009, and the population of the study fish species has now roughly recovered to the level before the habitat was severely damaged. In the middle and upper reaches of Nanzihsian Stream, the research fish species, Sinogastromyzon nantaiensis, were sampled by the electric grid method, and the physical environment of each electric grid area was measured, including flow velocity, water depth, and substrate size. Through independent sample t-test statistical analysis, it is confirmed that the habitat preferences of adults and juveniles of Sinogastromyzon nantaiensis are different under the spatial scales of microhabitat, riffle system, reach and stream, which further indicates that the ecological niches between adults and juveniles of Sinogastromyzon nantaiensis are differentiated. The results also indirectly confirm the intraspecific competition between adults and juveniles of Sinogastromyzon nantaiensis, and also show that adults can inhabit faster water velocity than juveniles. Finally, we confirm that the main biotic factor structuring the population distribution of Sinogastromyzon nantaiensis along the stream is intraspecific competition, and the abiotic factor is water flow velocity, which further explains the operation mechanism of intraspecific resource competition of Sinogastromyzon nantaiensis.



Interdisciplinary Geosciences


Mon-31 Jul | 10:20 - 12:20 | MR333
IG16 - Digital Twin Paradigm for Disaster Resilience

Session Chair(s): Nobuhito MORI, Kyoto University

IG16-A004
Coastal Digital Twin – A New Attempt to Gain Collective Intelligence in Coastal Science and Engineering

Shunichi KOSHIMURA1#+, Nobuhito MORI2, Naotaka YAMAMOTO CHIKASADA3, Keiko UDO1, Junichi NINOMIYA4, Yoshihiro OKUMURA5, Erick MAS1
1Tohoku University, 2Kyoto University, 3National Research Institute for Earth Science and Disaster Prevention, 4Kanazawa University, 5Kansai University

The digital twin is now recognized as digital copies of the physical world's objects stored in digital(cyber) space and utilized to simulate the sequences and consequences of target phenomena. By incorporating the physical world’s data into the digital twin, users can fully view the target through real-time feedback. Among the research community of coastal engineering, a project has been launched to enhance coastal community's resilience by constructing "Coastal Digital Twin (CDT)". This research project aims to establish a digital twin paradigm in coastal engineering in which the study, design, and search for optimal solutions to various coastal and marine problems, which would be impossible to experiment with in the physical world due to time and cost constraints, are carried out in the cyber world. The components of CDT are the transformation from "Data" to "Information" by integrating sensing, monitoring, and simulation; "Interpretation" of data and information; "Inference" using available data and information to draw a conclusion or make a prediction from data. The fusion of these components is the key to gaining knowledge and insight for optimal solutions in the physical world. The components to be covered are the following six themes. Theme 1: Sensing and monitoring technologies for the marine and coastal environment. Theme 2: Modeling techniques provide the basis for a wide range of predictions, including real-time ocean and coastal phenomena analysis. Theme 3: Application of data-driven science to elucidate latent structures and processes behind high-dimensional sensing and monitoring data. Theme 4: Methodologies to clarify the social impact to identify better response and adaptation measures. Theme 5: Conceptual design with considerations of DT infrastructure and software requirements of CDT. Theme 6: Functional requirements for CDT archive to store the physical world's data, simulation, and inference models achieved in research activities. 


IG16-A008
High-resolution River-coastal-ocean Circulation Modelling in the Seto Inland Sea for Coastal Hazards and Resource Management

Jae-Soon JEONG1+, Han Soo LEE1#, Nobuhito MORI2, Morhaf ALJBER1, Jonathan CABRERA3,4
1Hiroshima University, 2Kyoto University, 3Hiroshima University / Davao Oriental State University, 4Davao Oriental State University

The Seto Inland Sea (SIS) is a semi-enclosed coastal sea with a length of approximately 450 km. The SIS has limited water mass exchanges with an open sea, the Pacific Ocean, via the main passages, Bungo channel and Kii channel with lengths of approximately 35 and 30 km, respectively. Tides and water mass entered from the two channels meet and interact with each other making the complex structure of circulations in the SIS. Based on a deep understanding of this environment, it is emphasized to prepare the optimal management of natural resources and coastal hazards for sustainable development in diverse fields. This study aims to build a high-resolution numerical model seamlessly to describe the SIS in detail from the open sea to the upper river scale. The Semi-implicit Cross-scale Hydroscience Integrated System Model (SCHISM) using unstructured grids was adopted as a base model due to its strengths in describing complex coastal lines and stabilizing possible numerical errors under extreme events, such as typhoons and heavy rainfall. Tides and circulation were validated for the case of Typhoon Roki in 2011. The modelling result reproduced the abnormal tides in Hiroshima Bay. When the typhoon passed off the eastern part of the SIS, the sea-level decreased by 8 cm around the northern part of the SIS due to wind set-down. Then, after eight days, the sea level rise of approximately 5 cm was simulated reproducing a similar pattern as the observed. Also, the modelling result such as tidal circulation was utilized to estimate optimal locations for tidal power generation and the potential tidal power in the SIS. The developed high-resolution SIS model is aimed to be a basis of digital twin Seto Inland Sea and will play crucial roles in coastal safety and immediate response to natural or man-made disasters in the SIS.


IG16-A003
Tsunami Flow Depth Prediction Applying Ocean-bottom Pressure Data to Machine Learning Technique

Masato KAMIYA#+, Toshitaka BABA
Tokushima University

Research involving machine learning has been active in various fields in recent years. This study investigates a method for predicting tsunami flow depths using the multilayer perceptron (MLP) in the Nankai trough, Japan. The analysis procedure is as follows. Nonlinear long-wave tsunami calculations were performed for 3,480 earthquake fault scenarios to generate teacher data. As input data to the machine learning model, we assumed to use pressure data observed by an ocean-bottom pressure gauge network in the Nankai trough. We prepared from the 3480 calculated results the maximum or average bottom pressure 3 minutes after the earthquake for 5, 10, and 15 minutes to avoid seismic noise. The prediction target was tsunami flow depth distribution in a coastal town anticipating severe tsunami damage. The MLP model consisted of three intermediate layers of 100 nodes. We constructed test data calculated using the same method above from the M9 earthquake 11 scenarios proposed by the Cabinet Office of Japan. We compared tsunami flow depths of 20 cm or greater from the test data and ones predicted by MLP with the fitting index of the geometric mean K and geometric standard deviation κ from Aida (1978). The accuracy (%) was calculated from the geometric mean K. Using average pressure as input, K-κ were estimated to be 1.57-1.78, 1.21-1.57, and 1.19-1.62 for 5, 10, and 15-minute time windows, respectively. Using the maximum pressure as input, K-κ were estimated to be 1.08-1.67, 1.01-1.65, and 0.89-1.6, respectively. The accuracy obtained from K was 64%, 83%, and 84% for the average pressure input, and 93%, 99%, and 89% for the maximum pressure input. The case of the best accuracy was the maximum pressure used as an input with 10-minute time window.


IG16-A007
Feasibility Study of Digital Twin Implementation for Coastal Management Using Satellite SAR

Lianhui WU1#+, Yoshimitsu TAJIMA2
1Tokyo University of Marine Science and Technology, 2The University of Tokyo

Sandy coasts are dynamic landscapes that evolute in response to short-term pulses, long-term pressures, and anthropogenic interventions. Since shorelines are ideal proxy for evaluating the rate and breadth of beach change, the capability of accurate and frequent monitoring of the shoreline position is significant for coastal management. Satellite Synthetic Aperture Radar (SAR) is an active sensor that emits pulses of radio waves at target scene and receives backscattered signal. SAR can therefore observe earth surface at night, through cloud-cover, or during extreme storm events, and thus is a promising tool for frequent sandy beach monitoring. Moreover, due to the rapid development in small satellite SAR, startup companies have planned to build constellations of 30 SAR satellites in near future, which enables hourly observation of the earth surface. Therefore, it is believed that satellite SAR is transforming coastal science from a “data-poor” field into a “data-rich” field. If shoreline position can be automatically identified from SAR data, a digital twin is expected to be implemented for coastal management. The digital twin is suggested to be able to visualize the historical and near-real-time shoreline position, to evaluate the evolution of the sandy beach, to predict the coastal change, and to help decision making of coastal management. In this study, we addressed our recent advances in shoreline monitoring from satellite SAR, which is fundamental to establish a digital twin for coastal management. At first, we conducted field surveys and analyzed hundreds of SAR images to investigate the suitable observation condition of SAR for shoreline extraction. Then, we developed an automatic shoreline extraction algorithm based on artificial neural network. These works have shown feasibility of digital twin implementation for coastal management using satellite SAR.


IG16-A002
Quantitative Grasping Methodology of Urban Commuting Distance, Based on Resident Location Big Data

Makoto OKUMURA#+, Yuri SAWAMURA
Tohoku University

Constraints on commuting mobility due to natural disasters bring indirect damage, such as an urban activities’ stagnation. Commuting quantity, then, may become an important index of indirect disaster damage and the resilience of cities. This study develops a methodology for quantitative grasping of urban commuting movements, based on aggregated data of residents' location big data that has become available in recent years. For that purpose, we define a zone system that can both to decrease data size enough small for handling and to appropriately evaluate the amount of commuting movement. Next, we propose a calculation method of quantitative indices such as the number of commuting people, distance, and required time. Taking the Sapporo Metropolitan area in February 2022 as an example, we show an application of the proposed method to evaluate the impact assessment of a heavy snow disaster, based on Docomo’s “Mobile Population Statistics Data.” From these results, we understand that the speed of recovery of commuting volume of each residential municipality differs depending on the difference in public transportation usage rate and distance from the city center. We also detected that there are people departing early in the morning considering the effect of the heavy snow. The contents of this study may provide suggestions for the future economic evaluation methods on disaster digital twins.


IG16-A005 | Invited
A Study on Disaster Response Using a Digital Twin of the Actual Heavy Rain Disaster

Shuji MORIGUCHI1#+, Erick MAS1, Kenjiro TERADA1, Makoto OKUMURA1, Naoko KOSAKA2, Naoko SHIGEMATSU3, Hotoshi SHIMIZU4, Akinori FUJINO4, Tsuneko KURA2, Hiroshi MATSUBARA2, Masaki HISADA2
1Tohoku University, 2NTT Space Environment and Energy Laboratories, 3NTT Human Informatics Laboratories, 4NTT Communication Science Laboratories

This study presents a digital twin which enables us to analyze effective disaster response. An actual heavy rain disaster that occurred in the past in Marumori Town, Miyagi Prefecture, Japan, is reproduced in the Geographic Information System(GIS). In the target area, Typhoon Hagibis in 2019 caused a lot of landslides and floods, resulting in extensive damage. A numerical simulation is performed to virtually reproduce the landslides and floods for the whole area of Marumori Town using the actual terrain data and rainfall data observed during the typhoon. The accuracy of the simulated results is verified by comparing them with the actual distribution maps of landslides and inundation. The simulated results are then mapped onto the GIS, and evacuation is virtually reproduced with an agent-based simulation model that considers the temporary changes in the risk due to landslides and floods. The validity of the results is confirmed by checking the consistency with the records of the heavy rain disaster. In addition, different conditions from actual disasters are given in the constructed digital twin of the heavy rainfall disaster. Specifically, several scenarios are set up under different conditions, such as the timing of issuing emergency evacuation information, and the changes seen in the digital twin are analyzed. Based on the obtained results, the differences in outcomes between different scenarios are analyzed, and the efficient disaster response for heavy rain disasters is discussed.


IG16-A001
Digital Twin and Coastal Problems

Nobuhito MORI1#+, Shunichi KOSHIMURA2, Naotaka YAMAMOTO CHIKASADA3, Keiko UDO2, Junichi NINOMIYA4, Yoshihiro OKUMURA5
1Kyoto University, 2Tohoku University, 3National Research Institute for Earth Science and Disaster Prevention, 4Kanazawa University, 5Kansai University

Although the importance of the digital twin has been put forward as a policy matter, the concept is vague, and it is unclear how it relates to the natural sciences and engineering disciplines involved in coastal areas. The general concept of a digital twin refers to a system in which virtual and real space interlink. A weather system that assimilates data from observations is an obvious example.
In this presentation, we will review the introduction and development of digital twins for various time scales and coastal issues, from real-time modeling to climate issues.


Mon-31 Jul | 1:10 - 3:10 | MR305
IG08 - Identification, Mapping, Monitoring and Forecasting of Landslide and Erosion Processes

Session Chair(s): Chih-Chung CHUNG, National Central University, Jia-Jyun DONG, National Central University

IG08-A006 | Invited
Community Based Landslide Vulnerability Assessment Towards a Risk Reduction Plan – A Study on Kurseong Subdivision, Darjeeling Himalaya, India

Kapil GHOSH#+
Diamond Harbour Women's University

Darjeeling region of the Eastern Himalaya, especially the Kurseong subdivision (study area) experiences landslides in every monsoon season. Landslide vulnerability assessment is considered an integral part of landslide hazard management strategy. The identification of risk elements provides the basic platform for assessing the landslide risk of a region. The research is focused on the application of the top-down approach to find out the most vulnerable community. Regional scale landslide hazards and vulnerability assessment has been carried out to identify the most exposed communities. The landslide hazard zonation map shows that about 8.300% and 21.68% of the study area is under very high and high hazard zone respectively. A community-level vulnerability has been assessed considering 10 socio-economic indicators. Each indicator is assigned with a score and the indicator maps are combined to get the community-level vulnerability index map. Based on the considered indicators, the vulnerability hotspots (villages) have been identified. The total vulnerability score ranges from 2.21 to 5.48. community-level vulnerability assessment shows 19 villages are characterized by relatively hard socio-economic conditions (vulnerability score is > 4.00) among 61 villages. Based on 27 indicators belonging to the three dimensions a composite vulnerability index has been formulated and vulnerability at the household level has been identified. The study reveals that about 5.77% of households belong to the low vulnerable category, 42.31% of households belong to the moderate vulnerable category, 34.61% of households belong to the high, and 17.31% to the very high vulnerable category. For better management and response, a web-based dashboard can be developed which can help to track and keep the records of the affected households and conditions at a single operating display.


IG08-A009 | Invited
Integrated Analysis of Geophysical Datasets for Slope Stability in Doi Ong Tuong Area, Hoa Binh Province, Vietnam

Duy Thong KIEU1#+, Ngoc Dat PHAM1, Van Huu TRAN2, Hop Phong LAI3, Ngoc Anh HA1, Hong Trang PHAM1
1Vietnam Academy of Science and Technology, 2Hanoi University of Mining and Geology, 3Institute of Geological Sciences - Vietnam Academy of Science and Technology

Researching on landslides in Vietnam has been conducted in many areas, but the investigation methods are often applied independently, which limits the effectiveness of earth science methods. We apply multiple geophysical methods, remote sensing and geology to investigate the slope stability in Ong Tuong hill, Hoa Binh province, Vietnam, where landslides have occurred many times. To estimate the possibility of landslides in this area, we need to know slope stability. Analysing slope stability needs information on both surface and subsurface. The remote sensing image can provide only information on the surface area. Borehole information is the most reliable for subsurface but it is local and high cost. Geophysical methods are robust tools to image the subsurface, however, the non-uniqueness of geophysical inversion significant issue. Thus, to enhance the resolution of the slope stability models, we need to exploit all available information in the research area. We use the inversion of multiple geophysical data sets to reduce the ambiguous results of the inversion and to build more reliable physical parameter models. Then geophysical models, remote sensing and geology models are the input of the integrated analysis to build a slope stability model for the research area. We applied machine learning techniques to build a pseudo-3D model from multiple 2D sections. We also applied machine learning for the integration of physical models and other data sets such as remote sensing and geological model. The final model is validated by borehole information. The results show that our approach is robust and the model is consistent with the borehole information.


IG08-A014 | Invited
Developing Landslide Scenarios Based Emergency Preparedness and Response Planning Framework for the Rural Municipalities of Mountain Nepal

Suresh CHAUDHARY#+
National Society for Earthquake Technology - Nepal

Landslides are common especially in the hilly and mountainous regions of Nepal. Each year, landslide causes significant loss of lives, and properties, posing severe threats to physical infrastructure, and economic development. This requires developing, reviewing, enhancing, or auditing an emergency response system through understanding of the hazard events that present a potential for fatalities, injuries, property damage and/or business interruption. This study aims to; assess landslide hazard scenarios; and prepare hazard-based monsoonal emergency response planning framework for. We employed multi-criteria analytic hierarchy process to assign hazard weightage to geophysical and socio-demographic factors, and performed spatial superposition analysis in the Model Builder of a Geographic Information System to produce landslide hazard scenario map, which was subjected to reliability check against existing landslide occurrence by ground truthing and using statistical models. The result shows that out of total 82.57 km2, 21.82% area of the municipality, belongs to a high level of landslide hazard. Approximately 26.53% and 6.70% belong to the very high level of hazard and extreme high level of hazard respectively which means that nearly half >55.07% of the total municipal area is highly hazardous. The low and moderate risk zones accounted for 7.53% and 37.42% respectively. High level of landslide hazard seems mostly in north and northwest, but appears in patches in the south as well, whereas the level of moderate hazard is concentrated in the southern parts of the municipality. Municipal population, rural economy, geo-environment, physical infrastructures, and intangibles properties all are currently under stress, which generally increases with elevation towards the north but is also concentrated along the road network and river buffer zones. The hazard map and the framework are expected to provide scientific evidence-base for formulating and reasonable response strategies and guidelines for consensus-based utilization and protection of human and physical resources in the municipality.


IG08-A005
Machine Learning-based Landslide Susceptibility Mapping - Inje Area, South Korea

Chanul CHOI+, Xuan-Hien LE, Giha LEE#
Kyungpook National University

Nowadays, the frequency of landslide damage in South Korea is gradually increasing due to abnormal climates such as localized heavy rains and typhoons. In the landslide, an information system provided by Korea Forest Institute, a landslide risk map is produced using LR (Logistic Regression) techniques for 9 factors, such as slope, soil depth, and forest condition, based on data from past landslide events. Landslide data due to events such as extreme rainfall have been collected since 2020, and techniques to apply machine learning to landslides are being studied domestically and internationally. Accordingly, in this study, big data created by the National Institute of Forest Science create a landslide risk map using AI techniques for Inje, Gangwondo, South Korea. As a result, it is possible to create a landslide risk map through big data, and the accuracy of RF (Random Forest) is also higher than the existing LR technique that was applied. Through this, it can be used as a tool to reduce landslide damage such as by improving the existing landslide information system and reinforcing alerting areas expected to be damaged.


IG08-A007
Assessing Landslide Hazards in a Changing Climate Considering Atmospheric Influences: A Case Study of Rokko Mountain

Ying-Hsin WU#+, Akihiko YAMAJI, Yukari NAKA
Kyoto University

We present a new hydrometeorological approach to assess the tendency of landslide hazards by considering atmospheric influences. Estimating the future risk of landslide hazards in a changing climate has been one of essential topics worldwide in recent decades. Some effects have been made to assess the future change of early-warning alert of landslide in Japan with the application of the critical line method which is the current method for real practice of landslide early warning. The critical line method uses a parametric curve of snake line, which is composed of hourly precipitation and soil-water index, to reflect the effects of short-term rainfall and long-term soil wetness. In the original method, the geometric feature of a snake line, or says conditions for early-warning alerts, is mainly determined by rainfall pattern, e.g., duration, peak intensity, and etc. Additionally, the occurrence and amount of extreme precipitation can be highly influenced by air temperature through the analysis of Clausius-Clapeyron scaling of precipitation. Therefore, in our new approach, we utilize the concept of precipitation scaling to find out the relation between ground air temperature and soil-water index. Two exponential scaling relations for precipitation and soil-water index in terms of ground air temperature are respectively proposed, and are then used to assess the maximum range of snake line for the examination of landslide hazard tendency under climate change impact. Our method was verified using 30-year historical observation in the area of Rokko Mountain with high confidence. A case study was performed to show the high potential for landslide hazard assessment.


IG08-A008
Effects of Grain Size Distribution on the High-frequency Seismic Signals Generated by Experimental Geophysical Granular Flows

Zheng CHEN#+
Chengdu University of Technology

Granular-flow hazards such as landslides, rock avalanches, and debris flows often occur in mountainous area around the Tibetan plateau, threatening human life and safety of infrastructures. These geophysical granular flows can generate high-frequency seismic signals, which can be used to extract useful information of flow characteristics (e.g. flow rate and particle size). However, quantifying such characteristics during granular flow travel downslope using the seismic technology remains a challenging issue due to the complexity of the physical mechanism of such geophysical flows in nature. Here, we focus on the generation of the high-frequency seismic signals radiated by granular flow with different grain size distributions (GSD) and initial masses in a laboratory chute setting. Four accelerometers were installed underside of a plate mounted on the chute bed to record the acceleration signals generated by particle impacts on the bed during the movement. A pressure sensor was fixed at the center of the plate to measure the basal dynamic pressures of the granular flows on the bed. The video materials were recorded using cameras, and the flow depth and velocity were analyzed. The discrete element method was utilized to construct virtual discrete particles and to simulate the dynamic process of the granular flow initiation and movement over the bed. We found that the basal pressure, the signal amplitude, the centroid frequency, and the power spectrum of the generated signals changed with changing GSD, and the differences decreased with increasing Froude number. We also found that the increasing proportion of large particles could change the granular flow regime from dense inertial to collisional. The findings of this study may contribute to a better understanding of the generation of the high-frequency seismic signals from the granular flow with variable GSDs, and they could be useful monitoring the granular-flow hazards.


IG08-A015
Mapping Priority Areas for Forest Management in a Mountainous Watershed Using Raindrop Impact Estimation and Physically-based Modeling Approaches

Charles John GUNAY1+, Tomohiro IWAMA1, Yuta KOYAMA1, Katsuhide YOKOYAMA1#, Hiroshi SAKAI1, Akira KOIZUMI1, Kenji SAKAI2, Hiroki TAKAHASHI2
1Tokyo Metropolitan University, 2Bureau of Waterworks, Tokyo Metropolitan Government

Ineffective management increases the susceptibility of forests to splash erosion driven by raindrop impacts. In a mixed forested environment like the upstream catchment of Ogouchi Dam in Japan, no two areas are truly identical in terms of canopy, understory, and forest floor properties. The differences in the management practices also influenced such variations in the forest properties, thereby altering their responses to raindrop impacts that cause soil detachment. In this study, two related techniques were used to map out and identify the areas to be subjected to intensive forest management. The first approach is the estimation of the total erodibility coefficient (TER), an index to quantify the raindrop erosion susceptibility as a function of various geophysical forest properties. The well-documented records of the relevant forest parameters from the Tokyo Metropolitan Government made it possible to compute the TER value for each forest unit. Such values were entered into a GIS platform and the low- and high-risk regions were identified. The second approach integrates the first approach with the modeling of long-term hydrological processes. The physically-based Soil and Water Assessment Tool (SWAT) was used to calculate the sediment yield per hydrological response unit (HRU). Then, the sediment yield at the HRU level was distributed based on the area and the magnitude of the TER of each forest unit. Interestingly, the maps of priority areas generated by these two techniques were not completely alike. In the absence of model inputs, the TER estimation approach can already reflect the magnitude of sediment in each forest unit. Meanwhile, the SWAT modeling approach additionally accounts for the difference in soil type and other influencing hydrological properties. Both maps are considered reliable in providing a logical reference in the decision-making of the Government regarding whether the forest unit is subject to immediate rehabilitation or not.


IG08-A016
Study on the Infiltration Characteristic of Vegetated Slope and Its Effect on Shallow Slope Stability

Jung-Tai LEE#, Chih-Hsuan LIANG+, Yun-Chen HSIEH, Ming-Jen LEE
National Chiayi University

Taiwan is a mountainous island with steep terrain and fragile geology. Typhoons and torrential rains frequently induce serious natural hazards such as landslides and mudflow. Among the landslide events, the frequency of shallow landslide is higher than that of deep landslide. Shallow landslides cause serious threat to people’s livelihood. Previous studies indicated that rainfall is the main cause of shallow landslides in Taiwan. The best slope protection method is combining civil engineering and phytoremediation techniques. However, the effects of plant root system on slope stabilization are greatly influenced by plant species, root architecture, root biomechanics and soil moisture. Plant root system can increase soil porosity and water conservation capacity, whereas it can also increase soil infiltration rate and landslide risk. Therefore, the advantages and disadvantages of phytoremediation need further study. Thus, this research project is aimed to investigate the effect of rainfall on the hydrological behavior of forestland slope in order to improve slope stabilization method. This research is exploring the effects root characteristics of commonly used grasses and trees on soil infiltration behavior. The research using nursery planting model tests, with different combinations of plant root system, rainfall condition and degree of soil compaction, will be carried out to investigate the effects of root characteristics on soil infiltration rates after rainfall, and analyze the important root trait parameters affecting soil infiltration rate for evaluating the relationships between shallow slope infiltration and root system architecture.


Mon-31 Jul | 1:10 - 3:10 | MR333
IG17 - The Role of Asia Oceania Geosciences Society in Promoting Interdisciplinary Geosciences

Session Chair(s): Punyasloke BHADURY, Indian Institute of Science Education and Research Kolkata

IG17-A002 | Invited
Some Suggestions for Regional Cooperation in Geosciences

Wing-Huen IP#+
National Central University

The long-awaited phasing out of the COVID-19 pandemic provides us an opportunity to regroup the scientific and organizational activities associated with regional cooperation. Based on inputs from a number of AOGS members, it is suggested here that, in the next step, the Regional Advisory Committee (RAC) should serve as a link between AOGS and academic societies in Southeast Asia, Indian subcontinent and the Pacific Island Countries. Cooperative interactions of these scientific entities could lead to the planning and management of local topical conferences/workshops that might eventually lead to full-scale AOGS annual meetings in future. Summer schools for young scientists, science education camps, working groups and virtual lecture/talk series by distinguished scientists should also be promoted. Some ongoing efforts will be illustrated as examples of pilot projects. To be effective, it is most desirable that these activities can be included into the master plan of AOGS.


IG17-A006
Trans-disciplinary Research: A Holistic Approach for Enhancing Regional Cooperation

U.C. KULSHRESTHA1#+, Wing-Huen IP2
1Jawaharlal Nehru University, 2National Central University

In the present era of technology and global trade, networking and communication are the key drivers for advancement of a country, which help in strengthening the bonding and club spirit of a region. Inter-governmental regional cooperation such as the Association of Southeast Asian Nations (ASEAN) and the Asia-Pacific Network for Global Change Research (APN) have played a vital role in promoting exchange of ideas, people and goods belonging to the economic, political, cultural, scientific, technical and environmental domains of the member countries. Such institutional mechanisms facilitate different states to collaborate about common interests through research, academic, trade, cultural, sports channels. There is tremendous scope in Asia for working together in a holistic manner for common interests by selecting important trans-disciplinary research topics such as green environmental management, climate change, sustainability, future design, and COVID-19 through the specific task forces consisting of physical and social science researchers from the member countries. The Regional Advisory Committee (RAC) of AOGS is also engaged in promoting regional cooperation in Asia through multilateral geoscience research. This paper provides an input to enhance the regional cooperation by developing new clusters of transdisciplinary research in Asia. The South Asian Nitrogen Hub (SANH) is a recent example of regional cooperation having all eight countries of South Asia Co-operative Environment Programme (SACEP) as part of the project. The SANH is involving a number of transdisciplinary research experts for nitrogen measurements, modelling, policy making, agricultural solutions and ecosystem impact assessment. In fact, the long-term use of nitrogenous fertilizers has raised a concern for soil health and environment. The fossil fuel emissions have affected air quality impacting human health and climate. Therefore, this is the high time when the RAC-AOGS needs to take up this issue and recommends the comprehensive nitrogen cycle research as a major activity for entire Asia.


IG17-A007
Promoting Academic Exchange Between China and Asia-Oceania Region in Cooperation of Natural Disaster Prevention and Enhancing the Role of AOGS Community

Fuqiong HUANG1,2+, Xiwei XU3, Guoguang ZHENG4#, Chong XU5, Jie LIU6, Giovanni MARTINELLI7, Haoyu SHI8, Mohammed MOKHTARI9, Jiashun HU10, Paresh Nath SINGHA ROY11, Wing-Huen IP12, Ying ZHANG13, Galina KOPYLOVA14, Nianjie MA15
1China Earthquake Networks Center, China Earthquake Administration, 2Institute of Disaster Prevention, 3China Earthquake Administration, 4National Disaster Reduction Commission, 5National Institute of Natural Hazards, 6Sun Yat-sen University, 7National Institute of Geophysics and Volcanology, 8North China Institute of Science and Technology, 9International Institute of Earthquake Engineering and Seismology, 10Southern University of Science and Technology, 11Indian School of Mines, 12National Central University, 13Ministry of Emergency Management, 14Russian Academy of Sciences, 15China University of Mining and Technology

Reviewing the Pandemic time, human being did not only meet social and economic troubles but also face severe natural hazards. In Post-Pandemic era how to improve the predictability and the capability of risk assessment on natural disasters is the current and long term scientific challenge that the Society meets. Of course, challenge means opportunity. Opportunities come from how AOGS’s being helpful to solve the challenges. The following considerations might be useful. People life-oriented & disaster reduce-oriented projects should be more considered and can be easily accepted in Asia-Oceania region. The recent two great earthquakes in Turkey awake us that the disaster does not come from earthquake itself but from the destroyed construction. Earthquake induced natural hazard chain originates from people’s awareness and end to people’s life & economic benefit. The China national project of Comprehensive Risk Survey of Natural Disasters (CRSND) that has preliminarily completed in the end of 2022 can be as a reference or a model. The project comprehensively includes all types of natural disasters of each area. The future cooperation topics involve the fields of science and technology. The titles are wide range from scientific research projects and techniques for reducing or preventing disasters for people’s daily life. “Mentor 365” platform can play significant role for this consideration in AOGS community. We can have “AOGS women Geoscientists Forum: ‘HER’ Power in Geoscience” and so on. Adhering to the humanist philosophy of ‘link-care-support’, its aims to serve Asia-Oceania region, even all the world, are passionate about the development of geosciences and related disciplines & technologies. This is worthy and effective approach to improve the Society’s scientific excellence, diversity, and outreach. To cooperate with regional journals to improve AOGS’s publishing ability can be mutual benefit our Society and the regional Journal.


IG17-A001
Disaster and Risk Management Information Systems Research Unit: Disaster Management X Information Technology

Natt LEELAWAT#+, Kumpol SAENGTABTIM, Penpitcha ARAYACHOOKIAT, Jing TANG, Supattra VISESSRI, Chatpan CHINTANAPAKDEE, Prasert AKKHARAPRATHOMPHONG
Chulalongkorn University

In 2022, some continual disasters, such as COVID-19, were mitigated due to the preparation and readiness of multiple organizations. However, during the year, many disasters still needed to be prepared. The Disaster and Risk Management Information Systems Research Unit (DRMIS) plays a part in Thailand's AOGS local advisory team to set goals for helping and collaborating with multiple stakeholders that dealt with the disasters. African and Asia regions are the main focuses for our targets. Throughout the years, we have been collaborating with Kenya on a project called Collaborative Research with External Partners under the main theme called Business Continuity Management concept towards Public Healthcare System during the disaster. In this project, the main challenge is to adopt the idea of BCM in the public healthcare system for both Thailand and Kenya, especially during the COVID-19 situation. Next, the continual joint project called SATREPS DREAM is also the main project for our research team. In this project, the main contribution and challenge are to adopt the Area-Business Continuity Management concepts, which required the partnership of multiple business stakeholders to help each other based on various perspectives, such as data and information sharing during the disaster period. Lastly, our research team organized the 17th APRU MULTI-HAZARDS SYMPOSIUM 2022 by encouraging international and national researchers to present their works under Innovation Towards Sustainable Growth And Disaster Risk Reduction theme. All these international collaborations and co-events are examples of what can help promote awareness about the risk of disaster and let them be ready for future disasters in Thailand and other countries.


IG17-A003
ISTPNext and the ITM Great Observatory

Larry KEPKO1#+, Douglas ROWLAND2
1National Aeronautics and Space Administration, 2NASA Goddard Space Flight Center

Heliophysics is the study of the Sun and its effects throughout the solar system. It covers an incredible range of scales, from plasma physics at the electron scale to the boundary that separates our solar system from interstellar space. It also includes a diverse array of sub disciplines and expertise, with measurements spanning in situ particles and fields from the ionosphere out to the Sun’s corona, to remote sensing of the Sun, heliosphere, and near-Earth environment at multiple wavelengths and in energetic neutral atom observations. Many of the biggest unanswered science questions that remain across Heliophysics center around the interconnectivity of the different physical systems that comprise the Heliosphere, and the role of mesoscale dynamics in modulating, regulating, and controlling that interconnected behavior. These are complex, yet ultimately fundamental questions of how the Sun-Heliosphere and Geospace interact, and answers are needed to more accurately predict and model space weather impacts on and around Earth, the moon, and Mars. To answer these long-standing questions on the Sun-Heliosphere and Geospace as system-of-systems, we believe that Heliophysics requires a coordinated, deliberate, worldwide scientific effort. We suggest that the worldwide Heliophysics discipline should embark on a grand program to study these system-of-systems holistically, with coordinated, multipoint measurements, with particular emphasis on resolving mesoscale dynamics, and a whole-of-science approach that includes ground-based measurements and advanced numerical modeling. Without such a unified, next generation ISTP-type program, these questions will remain largely unanswered. In this paper we lay out the case for such an approach, and discuss how the ITM community is using the upcoming NASA GDC mission as a cornerstone to develop the ITM Great Observatory, a grass-roots, holistic approach to studying the ITM system. 


IG17-A004
Promoting Academic Exchange Between China and ASEAN in Aerospace Intelligence: The Initiative and Recent Progress for Regional Cooperation and SDGs

Haixia LYU1,2#+, Hongping ZHANG1, Weiping JIANG1, Jingnan LIU1
1Wuhan University, 2Universitat Politècnica de Catalunya

To foster the innovation, entrepreneurship, and understanding of Aerospace Intelligence, the People’s Government of Xiamen, the United Nations Global Geospatial Knowledge and Innovation Centre (UNGGKIC), and Wuhan University work together to build the new Aerospace Intelligence Research Institute. It aims for becoming a base for international cooperation with BRICS countries and the countries along the “Maritime Silk Road” in the field of GNSS/Beidou spatiotemporal information, and plans to be more engaged in the Sustainable Development Goals (SDGs) implementation. Drawing on over 60 years of top-notch education work in Geomatics of Wuhan University, this institute will attract graduate students in Geoscience both in China and around the world and equip them, not only with the technical knowledge to serve the society, but also with the sustainability insights to transform the society in a responsible manner. The training activities will boost regional skills capacity and support the society to deliver the SDGs. Transformation of scientific knowledge into tools, products, and services will be encouraged to promote economic and social development and support decision-making for the shared future, making the society more resilient. It is hoped to bridge the cultural and language difference, create a conducive environment by jointly undertaking research and exchanging knowledge, and build new partnerships for the development in Asia and beyond. Our philosophy, vision, and recent progress of the new institute will be presented.


Tue-01 Aug | 8:15 - 10:00 | MR335
IG06 - Space Science and Education Using Nano/microsatellite(s)

Session Chair(s): Kwangsun RYU, Korea Advanced Institute of Science and Technology, Minakshi DEVI, Gauhati University

IG06-A004 | Invited
Developing Hands on Space Education and Small Satellite Capacity Building at National Central University: Lessons Learned and Future Plans

Loren CHANG#+
National Central University

Building on a long history of space science and space environment research, National Central University (NCU) established Taiwan’s first Department of Space Science and Engineering in 2020. Since then, three classes of undergraduates, as well as a growing graduate student group of diverse backgrounds have been working with the faculty of the department to further develop and enhance capacity in small spacecraft development and utilization both for scientific research and hands on education. In addition to hands on cross-disciplinary emphasizing the integrative nature of space science and engineering, we have also sought to drive and participate in new and ongoing research and development projects targeting science and technology development through small satellite and payload missions in collaboration with international partners, government, and private industry. In this presentation, I will provide a brief overview of lessons learned in past and ongoing projects, including self-developed and international small satellite science missions as part of the International Satellite Program in Research and Education (INSPIRE) consortium, as well as development of Taiwan’s first lunar science payload. This allows students to understand the real-world implications of their science and engineering coursework, allowing for a better appreciation of the value of mathematical and scientific theory as tools for analysis, prediction, and design, while also producing a new generation workforce for the space sector with relevant hands-on experience and know how. As spaceflight capacity is an iterative process highly dependent upon heuristic findings, we hope the lessons learned here will be useful for other institutions also engaged in such capacity building.


IG06-A005 | Invited
Development of Plasma Probe for In-situ Measurement in the Mesosphere Layer

Siti Harwani MD YUSOFF#+
Universiti Sains Malaysia

The study of the mesosphere region has a lot of constraints due to the layer's altitude. Environmental conditions related to gravitational forces cause the measurement of data in this layer to be complicated for satellites, and no aircraft can reach more than 30 km yet. The study of mesosphere particles in this region plays a crucial role in anticipating seismic activity, which can be forecasted several days to several hours ahead. The early detection of earthquakes can provide early warning and thus may reduce life losses. This study aims to develop a plasma probe instrument for in-situ measurement in the mesosphere layer, equipped with a telemetry system that can receive telemetry, log, and process the information from the instrument in real time. Due to its robust design, the probe can be mounted on the satellite, sounding rockets and High Altitude balloons. This probe measures the floating potential shift (𝛥𝑉𝑓) characteristics of an electrode immersed in plasma. The 𝛥𝑉𝑓 characteristic of the plasma will then be retrieved from the device where the plasma's electron temperature (𝑇𝑒) together with the density (𝑁𝑒), can be acquired. The telemetry system is tested on the ground for real-time data transmission. To conclude, the probe is capable of measuring in-situ measurement of electron density and temperature in the mesosphere layer and transmitting the data in real time.


IG06-A006 | Invited
Nano/microsatellite Activities in S. Korea

Hae-Dong KIM#+
Gyeongsang National University

This paper introduces the current status of nanosat/microsat developed in Korea. Nanosat, also called Cubesat, began developing earnestly in Korea in 2012. Since 2015, eight nanosatellites have been developed, starting with the development of 6U Cubesat by KARI. In this paper, I will introduce essential nanosatellites developed in Korea and discuss each mission and lesson from development and launch.


IG06-A007 | Invited
A CubeSat for the Ionospheric Observation Under the Inter-university Collaborative Human Resource Development Program

Kentaro KITAMURA1#+, Hirokazu MASUI1, Shuji ABE2, Teiji UOZUMI2, Mariko TERAMOTO1, Akiko FUJIMOTO1, Kei SANO1, Akimasa YOSHIKAWA2, Meng CHO1
1Kyushu Institute of Technology, 2Kyushu University

Approximately 8,000 satellites have been launched between 2013 to 2023, about 25 % of those were categorized in CubeSat with the weight of less than 10 kg. As the number of CubeSats has increased, their missions have also shifted from educational and/or technology demonstrations to more practical and advanced missions including the many scientific observations. Kyushu Institute of Technology (Kyutech) has developed and launched 26 nano-satellites from 2012 to 2022. Some of these satellites had several science missions related to the magnetospheric and ionospheric observations. In order to conduct the magnetospheric or ionospheric observation by nano-satellites, the miniaturization of the instrument for plasma and electromagnetic fields measurements is often the most difficult challenge in their development. On the other hand, COTS (Commercial Off-The-Shelf) components for space science observation applications come to be available. This enabled younger students, such as undergraduates, to participate in more practical scientific observation missions. In Yotsuba-KUlover project is now undergoing to develop the 2U size CubeSat for geomagnetic observation by using such a COTS Fluxgate magnetometer. The satellites is developed by mainly undergraduate student as a hand-on training of the systems engineering in the framework of the inter-university cooperative program between the faculty of engineering in Kyutech and the faculty of science in Kyushu university. The science target of the mission is to observe the perturbation field of the geomagnetic field due to the Sq (Solar quiet) ionospheric current system, the IHFAC (Inter Hemispheric Field Aligned Current) and night side magnetic variations associated with the substorm activities. In this paper we report the recent achievement of the nano-satellite programs in Kyutech and ongoing Yotsuba-KUlover project in more details.


IG06-A011 | Invited
Small Satellites “Equatorial Sentinels” for Environmental Monitoring

Erick LANSARD#+
Nanyang Technological University (NTU)

There is an urgent need to better understand the environmental phenomena that are threatening the populations that live in equatorial regions: Typhoons, floods, earthquakes, tsunamis, volcanoes, wildfires, pollutions etc. due to climate change and geo-hazards are causing huge damages to the societies and huge financial losses to the economies. Forecast models are existing but with limited accuracy and available data have a poor sampling above equatorial regions, especially for fast-varying phenomena. To improve this situation, new data are mandatory. Missing data could be provided by a constellation of environmental satellites in near-equatorial orbit – so called ”Equatorial Sentinels” – that would fully exploit the exceptional revisit time offered by this orbit (10 times better than polar orbit!). This would help to better understand extreme events and to mitigate their impact. On-board these "Equatorial Sentinels", all kind of space sensors and technologies have to be considered, with emphasis on innovative small satellites and nanosatellite pathfinders: cheaper and faster to develop, they disruptive potential must be assessed and optimized in terms of cost/benefit/risk. “Equatorial Sentinels” should not replace but complement the fleet of global environmental satellites owned by big space countries (e.g.: NASA, ESA, JAXA etc), with focus on filling the data gap above equatorial regions. “Equatorial Sentinels” would not only benefit the equatorial regions but also benefit the rest of the planet, by feeding global and regional models with unique high revisit time measurements. “Equatorial Sentinels” will also bring many business opportunities for the public and private stakeholders that will have invested in this concept. These new and quite unique equatorial data, with unprecedented revisit time, will trigger the sustainable development of new services and new applications for the benefit of governments and citizens.


IG06-A015 | Invited
Improving Geometric Accuracy of Small Satellite SAR Images Using AIS and Deep Learning for Ship Detection

Duk-jin KIM#+, Juyoung SONG
Seoul National University

Small satellites have gained popularity in the new space era due to their affordability, but the use of relatively inexpensive components like GNSS and IMU can result in lower quality satellite images. To improve image quality, there is a need for software techniques. The geometric accuracy of satellite images is influenced by the sensor's acquisition geometry, and precise measurement of the sensor's position, velocity, and motion is important. GCPs are often used to achieve this, but accurate calibration and correction are limited in ocean SAR images. To address this, positional information of marine targets like ships is necessary, and the AIS can provide real-time monitoring information. However, interpolation of AIS data is required to determine the exact location of the ship since AIS acquisition time does not coincide with the SAR acquisition time. Deep learning technology is widely used for ship detection in ocean SAR images, but the relatively inaccurate geometry of the SAR sensor can cause significant errors in the position of detected ships. To improve geometric accuracy, a software technique was developed in this study involving matching the spatial arrangement of ships acquired by AIS with the spatial arrangement of detected ships in SAR images using deep learning technology. The technique's effectiveness was evaluated using HiSEA-1 small SAR satellite images with 1 m resolution, and the results showed significant geometric enhancement as the number of ships in the SAR image increased, particularly when additional static information such as the location of the AIS equipment within the ship was used to determine the ship's location.


Tue-01 Aug | 8:15 - 10:00 | MR336
IG04 - Advanced Tools for Water Quality Monitoring: Remote Sensing and Machine Learning

Session Chair(s): Jeanne Jinhui HUANG, Nankai University

IG04-A007
Measuring Sand Mining Budget in the Mekong Delta Through Deep Learning

Sonu KUMAR1+, Edward PARK1#, Duc Dung TRAN2,1, Adam SWITZER1, Jingyu WANG1
1Nanyang Technological University, 2National Institute of Education and Earth Observatory of Singapore

Riverbed sand is widely used in concrete production, land reclamation, and high-tech industries due to its angular shape and mineral richness. This has resulted in an unstainable rate of river sand mining leading to adverse environmental consequence such as salinity intrusion and bank collapse. However, information on the sand mining budget, crucial for quantifying and reducing the environmental impact of sand mining, is scant due to a lack of monitoring systems and costly bathymetry surveys. Here, we develop a novel framework to estimate the sand mining budget in the Mekong Delta (MD), a regional hotspot of sand mining, without the need for expensive field surveys. Our proposed framework uses deep learning algorithms that can detect sand-mining barges in satellite images automatically. For our method, we first generate a boat density map showing the spatial distribution of sand-mining activity. Next, we developed a regression model that integrates field survey-based river bathymetry difference maps and boat density maps to estimate the riverbed incision rate and sand mining budget. We have trained our model with manually labeled boat datasets consisting of 1,300 Barge with Cranes (BCs), 1,800 Sand Transport Boats (STBs), and 10,000 Other boats obtained from Sentinel 1 imagery using a batch size of 16 and for 1000 epochs. Our model achieved precision and recall of 89.5% and 88.4%, respectively, indicating an accurate and suitable model for our purpose. Our estimated boat density ranged from 0 to 10 barges per km2-day and has been validated with on-site field surveys. We expect our novel framework for the sand mining budget would fill current knowledge gaps in Fluvial Science by providing an actual amount of sand extracted for urbanization. Our framework, fully validated across the MD, has a strong potential to be scaled globally thanks to its cost-effectiveness and higher accuracy over manual methods.


IG04-A004
Evaluation and Mapping of River Water Quality Under Pollution and Hydroclimate Scenarios by Integrating QUAL2K and GIS

Mummidivarapu SATISH KUMAR+, Rehana SHAIK#, Avantika LATWAL
International Institute of Information Technology, Hyderabad

The Bhadravathi segment of the Bhadra river is one of the most polluted river stretches in India due to excessive pollutant discharge from the industries, and climate change has exacerbated pollution risks under hydroclimatic variability. Thus, the current study aimed to evaluate and map the river water quality under different climatic and pollution scenarios by integrating the river water quality simulation tool QUAL2K, Water Quality Index (WQI), and Geographical Information System (GIS). This research was applied on the Bhadra river stretch, which is approximately 27 km long and is separated into three reaches, each containing elements of 1 km as 3, 4, and 20 for each reach. The water quality model QUAL2K was calibrated (for 91 months) and validated (for 41 months) for simulation of water temperature, pH, Dissolved Oxygen (DO), Biological Oxygen Demand (BOD), nitrates, ammonia, and alkalinity. The impact of climate and pollution change on DO and water temperature are simulated using hypothetical scenarios. The WQI was estimated with the weighted arithmetic-WQI method by using the QUAL2K simulated river water quality indicators. The water quality maps are developed using equal interval mode with a graduated visualization technique in Quantum-GIS software. The WQI values range from 106 to 146 for observed conditions and the results revealed that the study stretch falls in class E/ unsuitable for drinking water quality. The WQI grade changed from class E to class C and class B for the 40% and 50% pollution reduction scenarios. The developed water quality map will help to identify the pollution hotspots to control pollution and the water quality charts under climatic and pollution scenarios are helpful to the policymakers and pollution control agencies.


IG04-A001
An Ensemble Machine Learning Model for Water Quality Estimation in Coastal Area Based on Remote Sensing Imagery

Xiaotong ZHU+, Jeanne Jinhui HUANG#, Hongwei GUO
Nankai University

The accurate estimation of coastal water quality parameters (WQPs) is crucial for decision-makers to manage water resources. Although various machine learning (ML) models have been developed for coastal water quality estimation using remote sensing data, the performance of these models has significant uncertainties when applied to regional scales. To address this issue, an ensemble ML-based model was developed in this study. The ensemble ML model was applied to estimate chlorophyll-a (Chla), turbidity, and dissolved oxygen (DO) based on Sentinel-2 satellite images in Shenzhen Bay, China. The optimal input features for each WQP were selected from eight spectral bands and seven spectral indices. A local explanation method termed Shapley Additive Explanations (SHAP) was employed to quantify contributions of each feature to model outputs. In addition, the impacts of three climate factors on the variation of each WQP were analyzed. The results suggested that the ensemble ML models have satisfied performance for Chla (errors = 1.7%), turbidity (errors = 1.5%) and DO estimation (errors = 0.02%). Band3 (B3) has the highest positive contribution to Chla estimation, while Band Ration Index2 (BR2) has the highest negative contribution to turbidity estimation, and Band7 (B7) has the highest positive contribution to DO estimation. The spatial patterns of the three WQPs revealed that the water quality deterioration in Shenzhen Bay was mainly influenced by input of terrestrial pollutants from the estuary. Correlation analysis demonstrated that air temperature (Temp) and average air pressure (AAP) exhibited the closest relationship with Chla. DO showed the strongest negative correlation with Temp, while turbidity was not sensitive to Temp, average wind speed (AWS), and AAP. Overall, the ensemble ML model proposed in this study provides an accurate and practical method for long-term Chla, turbidity, and DO estimation in coastal waters.


IG04-A005
Integration Approach of Remote Sensing Techniques with Hydrological Model and Field-based Observations for Water Quality Monitoring

Avantika LATWAL+, Mummidivarapu SATISH KUMAR, Rehana SHAIK#, K.S. RAJAN
International Institute of Information Technology, Hyderabad

Inland waterbodies are under tremendous stress due to increasing nutrient contamination under pronounced land use changes in the contributing watersheds globally. Contaminants quantification of inland waterbodies is limited due to the expensive field-based studies and computationally and data-intensive modelling frameworks. Satellite-based data facilitates studying the spatial spread of contaminants globally, providing integration and validation with field and modelled estimates. However, Remote sensing data have some limitations, including that it can be used only in the absence of clouds, atmospheric and processing errors, and mismatch of spatio-temporal with observed data. Thus, Remote Sensing Data, coupled with modelled and field-based observations, provides a more comprehensive ability to assess and monitor the quality and quantity of water resources. The present study goal is to develop a holistic approach to detect and quantify the contamination of inland waterbodies by integrating satellite-based remote sensing data and validating with field observations and water quantity-quality models. Therefore, the present study aims to detect contamination using remote sensing techniques and relate to the hydrological modelled observation between the period 2016-2018 in the Bhadra Reservoir. This study selected chlorophyll-a (Chl-a) content which was used as a proxy of nutrient contamination derived from Sentinel 2 satellite data. The nutrient load was simulated using a process-based hydrological model, SWAT (Soil and Water Assessment Tool), correlated with field-based nitrates and satellite-based Chl-a content. The research findings of the present study showed that Chl-a content spread was moderate during the post-monsoon month, and the spread was very low during the winter and monsoon months. The statistical analysis reveals a good correlation (R = 0.84) with a significance level of p < 0.05 between Chl-a and nitrate. The current study demonstrates the significance of using a hydrological model in conjunction with satellite-based data to monitor and evaluate inland water bodies in a qualitative manner.


IG04-A003
Comprehensive Comparison of Landsat-8 Oli Atmospheric Correction Techniques for Inland and Coastal Waters

Jeanne Jinhui HUANG#, Shang TIAN+, Xiaotong ZHU
Nankai University

Atmospheric correction (AC) is a crucial step in the quantitative analysis of inland and coastal waters. In this study, the performances of six water-based AC methods (SeaDAS, ACOLITE-DSF/EXP, C2RCC, iCOR) were evaluated by using multiple global datasets (N = 139). Four evaluation strategies were applied including spectral similarity and Chlorophyll-a retrieval. The results showed that SeaDAS and ACOLITE-DSF performed the best in terms of analytical match, band ratios, Chlorophyll-a retrieval, and spectral similarity. SeaDAS had the lowest RMSE in the blue-green bands and showed good consistency across the spectral with the lowest median spectral angle of 7°. It should be noted that ACOLITE-DSF outperforms SeaDAS in high turbidity waters. SeaDAS coupled with Chlorophyll-a retrieval algorithms of OC3 and Clark had the lowest RMSE, which showed the advantage of SeaDAS in Chlorophyll-a retrieval. This study provides scientific basis for choosing AC methods of Landsat-8 data for aquatic environment monitoring.


Tue-01 Aug | 10:20 - 12:20 | MR306
IG01 - Near Surface Investigation and Modeling for Groundwater Resources Assessment

Session Chair(s): Ping-Yu CHANG, National Central University, Jui-Pin TSAI, National Taiwan University, Chun-Wei HUANG, Ming Chi University of Technology

IG01-A018 | Invited
Advective Pollutant Plumes in Groundwater Regimes Resulting from Deep Injection Boreholes

A.P.S. SELVADURAI#+
McGill University

The migration of contaminants in porous geological media is a topic of fundamental importance to environmental geosciences and of particular interest to water resources management. The transport mechanisms in general can involve both advective and diffusive processes that are governed by flow velocities and concentration gradients, respectively. Although the fundamental processes governing the modes of transport can be highly non-linear and dependent on the morphology and geochemistry of the porous medium, the linear theories associated with these basic transport processes provide useful first approximations for the study of both advective and diffusive processes. In the linear theories, the advective transport is related to the flow velocity, which is usually governed by Darcy’s law and the diffusive transport process is governed by Fick’s law. The extent to which one or the other process dominates depends primarily on the flow characteristics as opposed to the diffusive transport characteristics of the system. There are, however, situations characterized by a Peclet Number greater than unity, where the flow velocities are sufficiently large to transport the chemical species solely by advective means. This paper presents approximate analytical solutions to the problems dealing with the advective transport of a chemical species from cavity in the shape of an elongated needle-shaped cavity, emanating from a deep borehole located in a porous medium of infinite extent. The solutions are developed by considering the advective transport from prolate spheroidal cavities situated in a porous medium of infinite extent. The flow velocities are determined by considering an appropriate solution of the Darcy flow in the porous medium, where the boundaries of the spheroidal cavity with a prolate shape is maintained at a constant potential. Analytical solutions provide valuable tools for examining the potential for groundwater contamination where the input parameters can exhibit variability.


IG01-A016
Study of Multispecies Chlorinated Solvents in Groundwater Using Numerical Modeling

Kumar RISHABH GUPTA#+, Pramod KUMAR SHARMA
Indian Institute of Technology Roorkee

There has been a long concern related to groundwater quality in the past, but it has become a severe interest to alter the conditions of subsurface water judicially. This study deals with the migration of chlorinated solvents and their decaying products in the subsurface media, as these pose a threat to the drinking water and pollute the surface water and groundwater. The accurate prediction of their fate and the extent to which it leads needs explicit modeling. A two-dimensional model is developed for multispecies chlorinated byproducts taking into consideration of transverse and longitudinal dispersion along with advection. A finite difference scheme is used to solve the two-dimensional advection-dispersion equation numerically. Five species of chlorinated solvents are considered, and the analysis is carried out using different types of dispersivities in order to account for the heterogeneity involved in the porous media. Constant, linear, and exponential distance-dependent dispersivities are applied to carry out the analysis, and the plume concentration level provides a broad spectrum of variations. The mobility of plume behavior depicts the physical and chemical processes involved in the decay chain reaction. Also, spatial moment analysis encapsulates the extent to which these daughter products can migrate into the groundwater and the area it hindrances in water management. This study offers a valuable method for assessing the effectiveness of monitoring plume attenuation caused by natural processes at a site using chlorinated solvents. These findings are of utmost importance to the policymakers and technical experts for planning, designing, and foreseeing the remediation techniques that would provide safety for human health and make sustainable groundwater management.


IG01-A004
Applying Deep Learning on Borehore Drill-core Image Classification -An Exploratory Study

Chun-Wei HUANG1#+, Si Ying YAU2, Liang Cheng CHANG3, Huan Huang CHEN3, Chuen-Fa NI2
1Ming Chi University of Technology, 2National Central University, 3National Yang Ming Chiao Tung University

Hydrogeological exploration is the foundation of not only groundwater management but also the prevention of land subsidence, seawater intrusion, and groundwater contamination. However, the classification of hydrogeological conditions is mainly based on the subjective judgement of applied geological engineers. This study explored the potential of deep learning technologies for identifying categories of unconsolidated sediment types, using drill core images. We tested a semantic segmentation-based model, termed U-Net. The results of this exploratory study showed that the U-Net can identify gravels with over 90% accuracy. Deep learning technology reveals the potential to be a useful tool to automatically classify geological types. In doing so, we can compile big data for future hydrogeological research.


IG01-A005
Spatial Estimated Groundwater Storage Maps Derived from GRACE and GLDAS

Tatas TATAS1,2#+, Hone-Jay CHU1
1National Cheng Kung University, 2Institut Teknologi Sepuluh Nopember

The Gravimetry Recovery and Climate Experiment (GRACE) satellites are identical satellites in low near-polar orbit. The satellites use space-based gravimetry, which can be used to quantify changes in groundwater storage directly. GRACE has also helped to estimate regional groundwater storage changes. Otherwise, data from the Global Land Data Assimilation System (GLDAS) show terrestrial variations that combine satellite data products and ground-based observations. With the help of advanced land surface models, the data can be used to estimate fluctuations and land surface conditions (LSMs). In detail, NOAH LSM presents canopy water storage, soil moisture, snow water equivalent, and surface water data. This study aims to create a global map illustrating areas where groundwater storage has increased or decreased and to calculate the statistical impact of these changes. The study will encompass all continents except the South Pole, as the GLDAS only covers that specific region. The GRACE data will be adjusted to align with the GLDAS coordinate system. The resulting global groundwater storage change map will highlight locations with declining or increasing trends. Specific regions, such as Greenland, Northern Canada, Southern Alaska, Southern Chile, and Northern India, exhibit consistent and significant decreases in groundwater storage. The statistical analysis reveals that the average groundwater storage change decreased more in the first ten years compared to the subsequent ten years. Additionally, 95% of the regions analyzed show a normal distribution of groundwater storage change over the 20 years, ranging from -130 cm to 111 cm. However, it is worth noting that the minimum and maximum groundwater storage values recorded were -1064 cm and 856 cm, respectively.


IG01-A008
Shallow Groundwater Exploration for Paleochannels in Prolonged Drought Area, A Case Study at Dan Chang District, Suphan Buri Province, Central Thailand

Passakorn PANANONT1#+, Songsak MUANGNOI1, Kasian PRASERTWONGPHILAI1, Niran CHAIMANEE2, Koichi HAYASHI3, Kevin P. FURLONG4, Oranuj LORPHENSRI5, Banjong PROMCHAN6
1Kasetsart University, 2Department of Marine and Coastal Resources, 3Geometrics Inc., 4Penn State University, 5Department of Mineral Resources, 6Department of Groundwater Resources

In recent years, various parts of Thailand have suffered from drought which has created difficult times for people living in rural areas where water resources are limited, and agriculture is an important part of the local economy. We have used a range of geophysical techniques to explore shallow groundwater resources, less than 15 m deep, to define paleochannels in Dan Chang district, Suphan Buri province in central Thailand; a region where severe drought has continuously occurred over the past several years. We use a suite of integrated techniques, including remote sensing, geology, and combined geophysical surveys (2D resistivity imaging, Ground Penetrating Radar, 2D Multichannel Analysis of Surface Wave, and multi-frequency electromagnetic surveys). Through this study, we have been able to define a shallow groundwater resource within paleochannels. At a target depth of less than 15 m, the resources have flow rates of 3.2-8.2 m3/hr. Most typical groundwater wells in the study area have depths between 30-50 m deep and are therefore very expensive to drill. Shallow groundwater resources from paleochannels allow the local community in this rural area to develop critical water resources with minimum expense. The use of integrated geophysical tools to define potential shallow groundwater resources in paleochannels provides locals, especially those who live in severe drought areas, with the opportunity to grow alternative plants for additional income and leads to a better quality of life. This economically feasible pilot project demonstrates the potential for developing shallow groundwater resources in paleochannels for rural communities that are suffering from drought.


IG01-A012
Investigating Near-surface Infiltration Measurements from Mini Disc Infiltrometer to Estimate Saturated Hydraulic Conductivity

Aparimita Priyadarshini NAIK#+, Sreeja PEKKAT
Indian Institute of Technology Guwahati

The near-surface saturated hydraulic conductivity (Ks) is one of the significant properties considered to govern the flow through porous media. Its accurate characterization is essential for determining the rate of water entry at the soil-atmosphere interface, quantifying soil water redistribution, reliable modeling of flow processes to prevent ground water contamination, and effective flood/drought modeling. A general practice to characterize Ks of a soil is by employing infiltration measurements. The objective of this study is to critically appraise any variability in the Ks of a given soil, determined from laboratory and in-situ infiltration tests of a compact, portable disc infiltrometer, called mini disc infiltrometer (MDI). Two different locally available soil types; one coarse-textured sand and one fine-textured loam, were used to conduct the in-situ and laboratory infiltration tests with MDI with adequate repetitions. Numerical modelling with the help of software HYDRUS 3D was conducted to inversely estimate the Ks from the cumulative infiltration (CI) measurements of MDI for both field and laboratory tests. The accuracy of the optimized Ks from field (MDI-F) and laboratory (MDI-L) infiltration measurements were evaluated by comparing with the reference Ks obtained from falling head permeameter tests for the two soil textures. The results showed that the mean Ks for both the soil textures were highly comparable with the reference Ks with a maximum difference of only a single order. The statistical analysis of the Ks results confirmed that both MDI-F and MDI-L were comparable with the reference Ks with relative error (for the log-transformed values) < 20% in all the cases. The investigations from this study demonstrate the utility of using numerical inversion technique to accurately quantify Ks from MDI infiltration measurements and shows that both field and laboratory MDI tests are capable of producing accurate and identical Ks estimates.


Tue-01 Aug | 10:20 - 12:20 | MR335
IG06 - Space Science and Education Using Nano/microsatellite(s)

Session Chair(s): Koichiro OYAMA, International Center for Space and Planetary Science

IG06-A002
Propagation Experiment Using Kurz-above-band Radio in Low Earth Orbit CubeSats

Chi-Kuang CHAO#+, Wei-Rong HUANG
National Central University

PEARL (Propagation Experiment using kurz-Above-band radio in Low earth orbit) mission currently consists of two 6U XL CubeSats, named as PEARL-1C and PEARL-1H, integrated by National Central University (NCU) and Hon Hai Precision Industry Co., Ltd. (Foxconn) for educational training/scientific research on earth-space radio propagation channel experiments over Taiwan. Two payloads, a Ka-band communication payload (KCP) for broadband communication experiment and a Compact Ionospheric Probe (CIP) for ionospheric plasma measurement, will be installed on PEARL-1C. KCP is developed by Rapidtek Technologies and NCU to perform like a transponder, a transmitter, a transceiver, and a channel study with ground stations over Taiwan. CIP is an all-in-one in-situ ion sensor developed by NCU to measure global ionospheric ion concentration, velocity, and temperature. A Communication PayLoad (CPL) developed by Tron Future will be installed on PEARL-1H for broadband communication experiment with beam-steering phase array antenna. These two CubeSats are scheduled to launch in SpaceX Transporter-9 rideshare mission in 2023.


IG06-A003
Development of Self-calibratable Plasma Probe for CAS500-3 and Its Implication to the Future Cubesat Missions

Kwangsun RYU1#+, Seunguk LEE2, Chang-Ho WOO1, Jinkyu KIM1, Wonho CHA1, Dongkook KIM1, Bon-ju KOO1, Seong-og PARK1, Dooyoung 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-III(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. The trade-off studies on probe antenna types and on circuit configurations are introduced including theoretical backgrounds. The qualification model of IAMMAP was developed and the scheme of self-calibration is demonstrated based on the ground test using a plasma chamber which can generate the plasma condition of the ionosphere. Finally, the implications of IAMMAP instrument for the future cubesat missions are introduced.


IG06-A010
Magnetospheric –ionispheric-tropospheric –lithospheric (MITL) Coupling Dynamics and Role of Nanosatellite Toward the Realization

Minakshi DEVI1#+, Subrat DAS1, Samiran PATGIRI1, Alaka MEDHI1, Arup J.D. SARMA2, Ananda BARBARA1
1Gauhati University, 2Assam Down Town University

The MITL coupling dynamics is based on complex systems involving the entire space from the magnetosphere to the lithosphere thus both Geomagnetic Storms (GMS) and Earthquakes (EQ) come as sources of disturbances. The devastating effect of an EQ while primarily confined to the earth's surface, a strong GMS event could affect the entire space-bound systems. The paper has thus the basic aim to define preludes under this combined background and to identify the effective role of the two events in modifying system dynamics by analyzing low to mid-latitude TEC (GPS/global). scintillation (GHz), ionization density, troposphere temperature, Cn2 & wind flow features, along with DST (>90 nT) and Global EQ of M>5.5.The EQ-GMS combined role is seen as changing the positive ionospheric effect to a negative one at low latitudes resulting in inhibition of the EQ-induced strong scintillation and similarly at high latitudes the negative ionospheric effect of GMS and absence of scintillation, helping the satellite communication to be more reliable in this environment. This situation is discussed in light of the negative ionospheric effect that inhibits RT instability which is associated with the growth of small-scale irregularities leading to scintillation. The TEC-modulated wave structures received from low-azimuthal satellites in EQ-GMS platform are observed to be of tropospheric origin. The strong GMS while lowering the tropopause temperature at low latitudes partly contributed by the Forbush effect, the strong EQ events induce tropospheric wind as the prelude, by modifying the horizontal temperature gradient developed from vertical shear, which changes over the thermally localized horizontal distance between the epicenter and the source, resulting in the growth of wind. The paper finally stresses that with a large number of parameters involved in the coupling dynamics, the simultaneous monitoring of the variabilities will be necessary and is possible only through Nanosatellite with multiple sensors.


IG06-A008
Future Opportunities on Mars and Venus Exploration Using Cubesats

Wing-Huen IP#+
National Central University

Because of their small sizes, simple designs and low cost, much attention has been given to the development of cubesats for Earth observations. Famous examples are the very successful PlanetScope program of Planet Lab and the SeaHawk cubesat for ocean color imaging (OCI) observations. Serious plans are being pushed forward to establish cubesat networks for quantum communications. Concerning planetary exploration, ESA, NASA, JAXA and other space agencies are in the process of building up their lunar cubesat programs actively. It is therefore expected that the time will come soon for extension of the cubesat technology to other planets. In this presentation, we will describe two possible types of cubesat missions. The first type is suitable for a single cubesat paired with a mothership for in-situ measurements of the atmospheric and ionospheric environments of Mars and Venus, respectively. The second type is designed for multi-point meteorological measurements as now being done by the Formosa 7/COSMIC 2 microsat mission on Earth. To overcome the difficulties of long-distance data transmission from the cubesats to the Earth, optical inter-satellite communication will be necessary. It is foreseeable that such mission concepts might be applied to the explorations of other planetary objects like Europa, Ganymede, Titan, Enceladus and the Saturnian rings in not too distant future. 


IG06-A019
A Modular and Scalable Satellite Platform for Advanced Distributed Space Mission

Mihindukulasooriya Sheral Crescent TISSERA#+, Shu Ting GOH , Kai Jie Ethan FOO, Kay Soon LOW
National University of Singapore

Lumelite is a modular and scalable satellite platform designed by the Satellite Technology And Research Centre (STAR) of National University of Singapore (NUS). The research focus of STAR is on the study and development of distributed space system whereby a number of small satellites will be flying together in formation or constellation to perform collaborative sensing. To date, the satellite design has been successfully implemented by two satellite missions for a formation flying program with 3 satellites and an advanced VHF data exchange system (VDES) with 1 satellite. In this paper, the Lumelite-4 satellite which is carrying an advanced VDES payload will be presented as an example to illustrate the Lumelite’s potential as a satellite platform for distributed space mission. The 16-kilogram Lumelite-4 was built by researchers and students in STAR. It is among the first four microsatellites build by STAR. Its communication payload was developed by Institute of Infocom Research (I2R) of A*STAR. This collaboration signifies the pioneering effort to develop a satellite based high performance VDES that will significantly improve the maritime communication and traffic management. The development of Lumelite-4 followed a rapid proto-flight model development approach and the flight model has been completed in February 2023. The satellite is expected to be launched into a near-equatorial low earth orbit. This paper will present the development of Lumelite-4 and also introduce its attitude determination and control system (ADCS) together with the in-house developed ADCS hardware-in-the-loop setup which is used as an educational module for teaching and research. Experimental results of the satellite’s performance will be presented.


IG06-A017
Plan of Space Experiment on Effects of High-power Microwave Radiation on Ionospheric Plasma for Solar Power Satellite

Koji TANAKA1#+, Takumi ABE1, Atsushi KUMAMOTO2, Hirotsugu KOJIMA3, Satoshi KURITA3, Tomohiko MITANI3, Yoshiyuki FUJINO4, Yasuyuki MIYAZAKI1, Koichi IJICHI5
1Japan Aerospace Exploration Agency, 2Tohoku University, 3Kyoto University, 4Toyo University, 5Japan Space Systems

We are planning space experiments on the effects of high-power microwave radiation on ionospheric plasma for a Solar Power Satellite (SPS) using a 100kg-class small satellite and a separate observation probe. A tethered SPS concept designed in Japan radiates C-band microwaves with a power density of around 1kW/m2. Such high-power microwaves possibly interact with ionospheric plasmas. The disturbed ionospheric conditions associated with these interactions may adversely affect the pointing accuracy of microwave beams for space-to-ground wireless power transmission by causing scintillation. Also, several potential non-linear interactions between ionosphere and microwave have been identified. These include parametric instability excitation, electron thermal runaway in the lower ionosphere, and thermal self-focusing of the microwave beam in the ionospheric F-region. These effects need to be confirmed by the space experiments before the development of the practical SPS. A rectenna and the plasma/excited wave observation instruments will be installed on the probe that have the size of almost 6U cube satellite. We will conduct wireless power transmission experiments between the satellite and the probe, measure the plasma parameters and exited waves at that time, and evaluate the interactions. This paper describes the design of the mission.


IG06-A016
Constellation of Small Satellites to Study Earthquake Precursor of Ionosphere

Koichiro OYAMA1,2#+
1International Center for Space and Planetary Science, 2Asia Space Environment Research Consortium

We are studying abnormal behavior of ionosphere which appears before large earthquake (M>7, Depth<30 km) Our past data analysis shows the followings; DE -2 data shows that O + density at the height of 300 km shows the minimum over the epicenter, as well as at geomagnetic equator. Two minima which is away from each other about 6-10 days before other merges on 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. In this case we cannot identify the epicenter in Japan. It is noted also that the plasma density shows 2 day’s oscillation for about a week before earthquake. 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.


IG06-A014
Science Experiment on NTU's Nano and Micro Satellites - Solar Spectral to Ionosphere Measurement

Wee Seng LIM1#+, Amal CHANDRAN2, Kashyapa BRAMHA NAREN ATHREYAS 1, Joji JOHN VARGHESE 1, Sir Yang LIM1, Edwin TEO1, Tony TSANG1, Erry GUNAWAN 1
1Nanyang Technological University, 2University of Colorado Boulder

The Satellite Research Centre (SaRC) at NTU School of Electrical and Electronic Engineering has developed and operated 10 nano and microsatellites since 2011. The center has trained many students and engineers on the technological aspect of satellite building. The recent satellites development have worked on various space science studies. In early 2015, work on GPS radio occultation have been implemented using COT GPS receivers on VELOX-CI microsatellite. In 2022, a student based SCOOB-I 3U nano has been launched to observe the Sun in 18 channels from Ultra-Violet to Infra-Red. This is for calculating the Sun energy output which helps in Earth’s radiation budget calculation. The energy from the Sun is absorbed in different parts of the Earth’s atmosphere. By understanding the energy output of the Sun in different parts of the electromagnetic spectrum, the energy input to the different layers of the atmosphere can be estimated. Further scientific experiment are also been implemented on the ARCADE satellite platform. This is targeting an equatorial orbit launch in mid 2023. The science motivation is to study the variability in the equatorial ionosphere and characterize the lower and upper atmosphere coupling. SaRC shall takes the opportunity to share the various satellite development works and seek collaboration with international partners. A new on-going development is the Very Low Earth Orbit (VLEO) Satellite, which will also study on the protection against Atomic Oxygen Effect. https://www.ntu.edu.sg/sarc.


Tue-01 Aug | 1:10 - 3:10 | MR306
IG02 - Natural Hazards and Disaster Risk

Session Chair(s): Magfira SYARIFUDDIN, State Agriculture Polytechnic of Kupang, Vena Pearl BONGOLAN, University of the Philippines Diliman

IG02-A002
Emerging Disease Outbreak During Cascading Natural Hazards

Gabriel Lorenzo SANTOS1,2#+, Vena Pearl BONGOLAN1, Jesus Emmaneul SEVILLEJA3
1University of the Philippines Diliman, 2Ateneo de Manila University, 3National Center for Mental Health

Disease outbreaks emerge from cascading natural hazards, regardless of the initial triggering hazard. Being exposed to natural hazards changes the behavioral dynamics of a vulnerable population which may possibly expose them to a higher risk of infection. An example is when a population is forced to evacuate to a location where social distancing is limited in the midst of a respiratory infection outbreak. Similar to other types of hazards, disease outbreaks also increase the risk of other hazards occurring. It is essential to understand the contribution of disease outbreaks to the overall impact of cascading hazards. 
This research aims to show the dynamic nature of cascading risks and how to minimize them by assessing their impact using three risk metrics: income lost, persons requiring assistance, and damage to infrastructure. The first part is to generate potential hazard cascade scenarios from known interactions of hazards occurring within a given region, assess the overall impact of these scenarios in terms of the chosen risk metrics, and rank each hazard based on its contribution to the overall impact. The second part is to assess the effectiveness of current and prospective mitigation options in controlling the impact of the cascades and generate optimal mitigation options based on set risk targets. This research aims to develop a multi-hazard risk assessment tool that disaster risk planners can use in developing optimal mitigation options or assessing their current mitigation projects. 


IG02-A004
Changes in Online Public Sentiment in Relation to Rainfall Related Disasters Amid COVID-19

Magfira SYARIFUDDIN1#+, Ratih Indri HAPSARI2, Mariko OGAWA3, Satoru OISHI4,5
1State Agriculture Polytechnic of Kupang, 2State Polytechnic of Malang, 3Kyoto University, 4Kobe University, 5RIKEN

The COVID-19 pandemic has been the attention of the global public opinion and press. The prolonged crisis of COVID-19 could intersect with disasters caused by natural hazards (e.g., earthquakes, floods, and typhoons). During the pandemic, Japan experienced the 2020 Kyushu floods in July and the 2021 Southwestern floods in August. The widespread use of social media provides a new way to obtain disaster information, and comments released by affected people become first-hand information about the disaster. Amongst all social media platforms, Twitter has been used to study online public sentiment during disasters. Additionally, Japan is the second-largest share of Twitter users in the world. This research aims to identify the change in online public sentiments on rainfall-related hazards amidst the COVID-19 by leveraging Twitter data. Japan-geolocated tweets posted during two major flood events in Southwestern Japan on June 28-July 8, 2018, and July 3-14, 2020 was retrieved. We sampled about 700-1000 tweets for each flooding event and classified them as positive, neutral, and negative tweets by a supervised method. Using the natural language program, the feature word vectors were extracted. Finally, data features were trained to predict the sentiment using Naïve Bayesian Classifier. Public sentiments related to flood events in 2020 was compared to those captured in the 2018 flooding event. Based on the polarity of the emotion revealed by the sentiment analysis, the study outcome is expected to contribute to the decision-making during the concurrent crisis.


IG02-A011
Reviewing COVID Modeling Assumptions

Vena Pearl BONGOLAN#+
University of the Philippines Diliman

As vaccines rolled out, and we all began to breath a little easier, we took time to reflect on the work we have done in the past, and sought to test our models, starting with our most basic assumptions. Our theory of age-stratification was easily proven, by looking at world-wide data. We also looked back to look at local histories and data for the pandemic, and compared with the earliest data set from Hubei, from February 2020. We saw an expected difference in the scatter of the two data sets, reinforcing age stratification. We also reviewed the robustness of our models, which we have used for vaccine allocation scenarios (in a country like the Philippines, prioritizing low-income people might be more efficient) and school reopening scenarios (not surprisingly, areas with a history of vaccine hesitancy were the last to be given the go-signal), and now includes frequently over-looked parameters like a population's vital statistics. Our work continues, as we join the chorus trying to answer "What Did We Learn From Covid". One important thing that we were warned about, early on, was this: the next epidemic will concern mental health. We are only beginning to study this phenomenon, with tools currently being developed for a cascade of disasters. Preliminary results will be discussed.


IG02-A012
A Study on the Analysis of the Causes of Road Tunnel Accidents by Heavy Snow and the Derivation of Improvement Measures

Eun-Byul KIM1#+, Bu-Saeng KIM2, Yeonju KIM1
1National Disaster Management Research Institute, 2Ministry of the Interior and Safety

Due to extreme weather caused by climate change, weather disasters are also occurring in Korea, and damage caused by heavy snow and cold waves is also increasing in addition to summer storm and flood damage. Among them, the occurrence of casualties due to highway accidents due to heavy snow or freezing on road surfaces has become a social issue. According to an analysis of weather conditions in the past 10 years when traffic occurs, 24 deaths per 1,000 accidents occur in snowy days, 27% higher than the overall average of traffic accidents. Therefore, this study attempted to come up with improvement measures through field surveys and cause analysis for cases with high social ripple effects due to large casualties among traffic accidents caused by snowfall. When analyzing the cause, it was intended to analyze not only the effect of snowfall on the occurrence of an accident, but also the cause of the expansion of damage caused by large-scale casualties. To this end, an on-site survey was conducted on the accident environment such as weather phenomena, structural characteristics of road tunnels, and installation status of traffic safety facilities for a total of 48 people, including 5 deaths from heavy snow. As a result, the cause of the increase in accidents and casualties was suggested due to the weather phenomenon of heavy snow, the structural characteristics of road tunnels, personal carelessness such as traffic violations, and inappropriate initial responses. In addition, nine improvement tasks were presented to prevent accidents from occurring under the same weather conditions in the future.


IG02-A026
The Trans-disciplinary Construction of a Comprehensive Seismic Scenario for Weinan City: A Pilot Action Research to Address Major Gaps in Earthquake Disaster Risk Reduction in China

Guiwu SU1#+, Janise RODGERS2, Wenhua QI3, Philip ENGLAND4, Timothy SIM5, John YOUNG6, Dongming WANG7, Zhiqiang LI8, Emily SO9, Xijie FENG10, Kun CHEN3, Yue CAO11, Jinli ZHAO10, Xiaoli LI8, Chunlan GUO 12, Jie GAO7, Junlei YU13, Yaohui LIU14, Benyong WEI1, Lei SUN15, Barry PARSONS4, David MILLEDGE16, Alexander DENSMORE17, Craig DAVIS2, Arrietta CHAKOS18, Zhixiang YUAN10, Qi ZHOU19
1Institute of Geology, China Earthquake Administration, 2GeoHazards International, 3China Earthquake Administration, 4University of Oxford, 5Singapore University of Social Sciences, 6International Network for Advancing Science and Policy, 7China Earthquake Disaster Prevention Center, 8China Earthquake Networks Center, 9University of Cambridge, 10Shaanxi Earthquake Agency, 11Overseas Development Institute, 12The Chinese University of Hong Kong, 13Jinan University, 14Shandong Jianzhu University, 15Fudan University, 16Newcastle University, 17Durham University, 18Urban Resilience Strategies, Berkeley, 19Baoji University of Arts and Sciences

Earthquake disaster reduction approach in China is essentially top-down, which is highly effective in mobilizing large-scale activities. However, a society’s total resilience to earthquake also depends on actions from various bottom-up actors (e.g., family, community), pointing to the need for a governance model that integrates government-led top-down approaches with broad bottom-up engagement of grass-roots and the public. To accumulate research evidences for developing that governance, the overall objective of constructing a seismic scenario for Weinan city, Shaanxi province, China, was thus planned to address in particular the following two major gaps in China’s earthquake disaster risk reduction (DRR): (i) between top-down and bottom-up approaches, and (ii) between science and DRR policies. Using trans-disciplinary participatory action research, the Weinan scenario work delivered this objective through direct interactions and close collaborations between two different groups of people: multi-disciplinary China-UK-USA collaboration research team and various local DRR practitioners. The overall progresses include, (1)using action research as a process tool, the two groups worked closely together to co-identify earthquake risk, co-explore pathways to risk reduction, which ensured the reliability of the scenario results, the local context-appropriateness of the DRR recommendations, and the direct & immediate in-situ/on-site “science into policies”. (2)By serving both governments and bottom-up actors and by examining issues from multi-scale viewpoint, improvement of top-down, bottom-up, and key linkages of the two of earthquake DRR policies were all co-addressed by the two groups. (3)Focusing on bettering disaster education and inspiring long-lasting action improvement, two versions of storytelling-led and latest science-grounded scenario narratives were co-created: one for government officials, the other for the general public. The trans-disciplinary participatory action research-guided Weinan scenario work has utility of “throwing out a brick to attract a jade” for China’s earthquake DRR field, it also provides international similar studies with valuable experience from China context.


IG02-A017
Benefit Evaluation Research in Disaster Prevention and Reduction of Tropical Cyclone Based on Social Investigation

Minghui LYU#+
China Meteorological Administration

There are many types of meteorological disasters in China. Among them, tropical cyclones have a greater impact on the central and eastern regions. Usually there are 6-7 typhoons landing on mainland China each year, which bring winds and heavy rains as well as secondary disasters, and causing certain damages and losses. Based on review of literature and examples in relevant fields, taking into account the disaster prevention system of "Government-led, Sectoral linkage and Public participation" in China, the evaluation of the benefits of typhoon disaster prevention and mitigation focuses on the evaluation of typhoon meteorological services, and the comprehensive assessment of the effectiveness of typhoon defense. Combing the whole process of typhoon disaster prevention and mitigation meteorological services, select the relevant indicators and parameters to establish the evaluation index system and calculation formula. This paper provides a preliminary evaluation of the services assessment and the benefits of disaster prevention and reduction about 27 tropical cyclones which are landed on mainland from 2017 to 2021. Combined with the current general evaluation technology and sociological research methods, this study proposes a social-economic benefit assessment method based on the disaster prevention and reduction system in China and the evaluation index system can also be used in assessing other process of severe weather disasters prevention and reduction. Based on survey data and the results calculated with the integrated method, this study can also provide the evaluation to the government and stakeholder to improve the comprehensive service ability and improve the efficiency of disaster prevention and disaster reduction.


IG02-A009
A Study on the Cause of High-rise Building Wind Accidents and Improvement Measures

Yeonju KIM1+, Eunbyul KIM1#, Bu-Saeng KIM2
1National Disaster Management Research Institute, 2Ministry of the Interior and Safety

The average number of typhoons that affect the Republic of Korea is about 3.4 per year, but in the case of 2019, 7 typhoons directly or indirectly affected it. Particularly, due to the influence of climate change, typhoons and local gusts with maximum wind speeds exceeding 40 m/s are increasing. As urban concentration accelerates, the construction of high-rise buildings is increasing, and high-rise buildings are being concentrated in cities such as Seoul and Busan, which are close to typhoon entry locations. High-rise buildings cause building wind phenomena increasing wind speed and wind pressure in locations around high-rise buildings, such as vortex phenomena and venturi effects when typhoons and strong winds occur. If the window is damaged and scattered by the strong wind speed itself caused by the building wind, it can be classified as a dangerous disaster factor causing large-scale loss of lives. The building wind-related laws in Korea vary by relevant institutions, so it is impossible to effectively reduce damage caused by building wind. Therefore, in this study, the cause of high-rise building wind accidents and improvement measures were prepared through the identification of the current status of the legal system by each relevant institution, and the current status of high-rise buildings, the analysis of accident cases, and network analysis.


IG02-A021
Quantifying Uncertainties in Tropical Cyclone Wind Risk Due to Synthetic Track Stochastic Variability

Wei JIAN1#+, Pane STOJANOVSKI2, Edmond LO2
1Institute of Catastrophe Risk Management, Nanyang Technological University, 2Nanyang Technological University

Extreme tropical cyclones (TCs) present serious threat to Southeast Asian (SEA) communities, causing widespread loss of lives and property damages. Probabilistic TC risk assessment has been widely used in catastrophe risk analysis, using catalogues of TC tracks with storm-defining parameters as the necessary input. Reliable historical TC records in the SEA region are limited in length, with the best track datasets for the region covering at most about 70 years. A widely explored approach to overcome this deficiency of limited historical records is the generation of synthetic TC tracks, based on resampling and modelling from historical records and meteorological datasets from climate models. Given that extreme TC events are sensitive to the statistical variations in the underlying event catalogue, proper quantification of their influence on model uncertainties is crucial for understanding and communicating disaster risk.
In this study, we investigate the uncertainties in TC wind risk metrics arising from stochastic variability in the synthetic track ensembles. We focus on landfall TCs in the National Capital Region (NCR) of the Philippines, using ten realisations from a single synthetic TC generation model. Each synthetic event set is statistically equivalent in capturing the storm severity and frequency affecting the NCR. The risk assessment shows that the ensemble spread in the mean gust wind speed, measured by the coefficient of variation, is 0.09. When applying the same exposure and vulnerability models to these ensemble sets, the dispersion around the ensemble mean Average Annual Loss is 0.88. Our study can complement the conventional risk assessment using synthetic TC tracks by explicitly assessing the modelling uncertainty in the TC risk metrics for more rigorous loss estimation, insurance/reinsurance applications, and risk management planning.


Tue-01 Aug | 3:30 - 5:15 | MR306
IG02 - Natural Hazards and Disaster Risk

Session Chair(s): James TERRY, Zayed University, Chung-Pai CHANG, National Central University

IG02-A003 | Invited
Applicability of CHIRPS-based Satellite Precipitation Products to Model Extreme Rainfall-induced Landslide Event

Thapthai CHAITHONG1#+, Kulapramote PRATHUMCHAI1, Monapat SASINGHA1, Suttisak SORALUMP1, Daisuke KOMORI2
1Kasetsart University, 2Tohoku University

Rainfall data are critical for generating landslide susceptibility and hazard maps. Based on historical landslide events, landslide prone areas are typically mountainous, where it is difficult to install rain gauges. Landslide events can be analysed with rainfall data from nearby weather stations, which may be far away from the site of a landslide occurrence. Satellite technology and remote sensing techniques can estimate rainwater amounts, which enhances the usefulness of rainfall data in landslide analyses. This study aims to develop a technique for modelling rainfall-induced landslides using CHIRPS-based satellite precipitation data from a landslide case study from Nakhon Si Thammarat Province (1988). The three major processes in developing a rainfall-induced shallow landslide model are: (1) bias correction and spatial downscaling of satellite precipitation; (2) groundwater table calculation; and (3) calculation of safety factors based on the infinite slope stability model. The receiver operating characteristic curve was used to validate the performance of the proposed technique. According to our calculations, this proposed technique using CHIRPS-based satellite precipitation data can identify landslide areas in the Nakhon Si Thammarat Province.


IG02-A010
An Integration of Data Across Space and Time to Assess Potential Slope Disaster Over Indigenous Communities

Shih-Yuan LIN1#+, Yu-Ching LIN2, Chen-Wei LAN3, Ching-Fang LEE3, Wen-Ray SU4, Tzu-Yin CHANG4
1National Chengchi University, 2National Defense University, 3Sinotech Engineering Consultants Inc., 4National Science and Technology Center for Disaster Reduction

Potential large-scale landslides and debris flow torrent are located in mountainous areas. In Taiwan, these areas mostly overlap with indigenous communities. Since the Morakot typhoon in 2009, in order to reduce the impact of disasters caused by heavy rainfall, the government has been investing resources to monitor slope instability over disaster-prone areas. Together with implementation of disaster management measures, it is expected to reduce the possible severe loss of life and economy occurred in indigenous communities. However, the observations of disaster signs and the monitoring results of terrain changes are not effectively shared with the communities. In addition, as the indigenous people themselves also have traditional local knowledge about disasters, the practice of disaster avoidance is questioned and challenged by the residents. The main goal of this study is to establish a disaster information integration and communication system to bridge local disaster knowledge and monitoring information derived from geomatics techniques. To achieve this, the system mainly takes the remote sensing and volunteered geographic information system as the core. We implemented time series differential interferometric SAR (D-InSAR), set Internet of Things (IoT) sensors, developed application (app.) on mobile phone for reporting disaster signs. By doing so, we collected disaster-related-data including wide extent and also local specific location, long time sequence and also short-term period, static and also dynamic response, historical and also contemporary knowledge. After integrating and filtering the aforementioned multiple data, the potential disaster areas were identified and provided to the residents in both dynamic and static manners through the mobile app. for broadcasting disaster potential area and the publication of community safety map. This study took Wulai District in New Taipei City in northern Taiwan as the research area. We will report the production, integration and communication of disaster knowledge and present the results of cooperation with community residents.


IG02-A008
Effective Factors Analysis for Optimal Check Dam Location to Prevent Debris Flow Damage Based on Numerical Analysis

Seungjun LEE1+, Hyunuk AN2#, Minseok KIM1
1Korea Institute of Geoscience and Mineral Resources, 2Chungnam National University

The check dam is one of the most effective countermeasures to reduce the damage caused by debris flows. While several previous studies have tried to find the priority factor of check dam construction, there are still limitations in terms of quantitive analysis for figuring out the factor of check dam influencing debris flow damages. This study analyzed the most influential factor to assess the best location for the mitigation effect through numerical simulations, which are on the Raemian apartment at Mt. Umyeon in Seoul and Gallam-ri in Gangwon-do, the Republic of Korea, in 2011 and 2019, respectively. The simulation results were quantitatively analyzed by Spearman's rank correlation method. As a result, it was found that the topographical components are more reasonable than flow characteristics in the construction of the check dam. In particular, the check dam constructed at the point which could store more debris revealed the best performance in mitigation effect. This work was supported by the National Research Foundation of Korea (NRF) grant funded by the Korea government (MSIT) (No. 2021R1A2C200553012)


IG02-A001
Flash Floods of July 2022 in the United Arab Emirates: Event Analysis, Disaster Mitigation and Some Perspectives on Risk Reduction

James TERRY1#+, Amna ALRUHEILI2, Maitha ALMARZOOQI1, Amani ALSHEHHI1, Reem ALMHEIRI 1
1Zayed University, 2Sultan Qaboos University

The hyper-arid Arabian Peninsula is one of the harshest climatic regions on Earth. During the scorching hot summer months in the UAE, precipitation is normally absent. Rare rainstorm events, when they do occur however, are capable of producing rapid runoff in dry watercourses known as wadis. The intense nature of unpredictable large rainstorms across the arid landscape therefore makes it imperative to examine their characteristics, causes and historical context. Major cities also have an increasing flash flood risk, owing to expanding urbanisation following economic development and population growth over recent decades. In late July 2022, unexpectedly heavy rainstorms occurred across the north-eastern UAE. The extreme event broke 30-year records. Some climate stations received over 200 mm of rain, exceeding the average annual total in just two days. Widespread flash floods were generated in Fujairah City on the Gulf of Oman (Arabian Sea) coast and in neighbouring areas. However, owing to effective and coordinated responses by the national disaster agency, emergency services and the military, almost nine hundred people were safely rescued and a major disaster was averted. This presentation investigates the summer 2022 storm event and the resulting flash floods. Rainfall characteristics are analysed and compared with long-term records. Important factors influencing the severity of the floods are examined. This is followed by some perspectives on reducing flood risks in the UAE, against the background of projected climate change scenarios for the Arabian Peninsula.


IG02-A013
A Decadal Review (2010-2021) of IRDR ICoE-Taipei

Ying LIAO1#+, Chung-Pai CHANG2, Jian-Cheng LEE1, Yue-Gau CHEN1
1Academia Sinica, 2National Central University

Integrated Research on Disaster Risk (IRDR) is a decade-long, international interdisciplinary research program initiated and sponsored by the International Science Council (ISC) in partnership with the United Nations office for Disaster Risk Reduction (UNDRR). The first IRDR International Centre of Excellence (IRDR ICoE) was established in Taipei in 2010 at Academia Sinica, and incorporated into the Center for Sustainability Science in 2012. The goal of ICoE-Taipei is to serve as an international platform for 1) promoting integrated research on disaster risk from both the natural and social science perspectives, 2) building a research network of Disaster Risk Reduction (DRR), and 3) sharing practical experiences of disaster early warning and preparation in Taiwan via international training courses, workshops and Advanced Institutes. During the first decade (2010-2021), the center has become an international hub in Southeast Asia for DRR research and developed a mature operation model on interdisciplinary collaborations such as hosting schools and funding regional cross-country research teams. By the end of 2021, the center has organized 15 AIs, provided training workshops to over 300 early-career scientists from over 20 countries, and supported trainees’ further development with competitive seed grants. ICoE-Taipei is expected to be an active player in the DRR prevention, preparedness, and resilience on the world map in the next decade and beyond.


IG02-A030
Evaluating West Halmahera Exposure to the Potential Gamalama’s Landslide-induced Tsunamis

Saaduddin SAADUDDIN1#+, Jurgen NEUBERG2, Mark THOMAS2
1Laboratory of Ocean and Coastal Dynamics, Department of Geophysics, Hasanuddin University, 2University of Leeds

Mount Gamalama is an active steep-flank volcanic island located in the west of Halmahera Island. This volcano has a history of tsunami generation in 1608, 1840, and 1871. Additionally, the existence of Tolire Kecil, Tolire Besar, and Laguna maars shows the potential instability on the flank. Based on numerical modelling, Mt Gamalama poses 5.56 km3 of potential volcanic landslide material which could generate tsunamis reaching West Halmahera. The calculated run-up reaches 20 m height in Sidangoli which is the closest borough to Mt. Gamalama. This is a centre of economic activities and has a ferry port, settlements, farms, and several public buildings (schools, market, mosques, and church). Furthermore, there are 4197 inhabitants threatened by the tsunamis in Sidangoli, and 24,954 inhabitants in West Halmahera. Therefore, this potential hazard must be considered and analyzed to minimize the potential exposure, vulnerability, and risk.


IG02-A016 | Invited
Geovisualization of Tsunami-related Studies Around the World

Bruce Enki Oscar THOMAS1#+, Jean ROGER2, Yanni GUNNELL3, Irem PALA4
1Institute of Geodesy, University of Stuttgart, 2GNS Science, 3Université Lumière Lyon 2, 4University Grenoble Alpes

The number of peer-reviewed publications dealing with tsunami research has increased substantially since the Indian ocean disaster of December 2004. The reporting of tsunami events has become more systematic but has tended to focus on classic tsunami areas such as South-East Asia, Japan and the US Pacific coast. Meanwhile, tsunami research interest for areas lying off the beaten track has been lagging. For example, despite being located in a well-known hazard area, the 2022 Tonga volcanic eruption caused an unexpected tsunami, highlighting the scarcity of observations, of simulation models and of impact studies for these islands. By applying simple computational search methods in bibliometric analysis, we present a comprehensive, geography-focused overview of tsunami-related research in the existing literature. Results identify clear gaps in the geographic coverage of tsunami catalogues – even along the Pacific Ring of Fire, where most devastating natural hazards occur. Whereas Japan, for example, has benefited from ~5500 tsunami-related publications since 2005 (Scopus search), Tonga totals only 105, i.e. almost two orders of magnitude less – and more than half of them published in the last year. Tsunami studies along the US west coast tend to magnify the specificities of each state, whereas tsunami hazards in Central America are usually addressed for the whole region rather than by country. Tsunami-prone areas like the SW coast of Africa are covered by fewer than 10 publications. These examples of uneven coverage highlight the absence of resources allocated to tsunami research in poorly documented but nonetheless vulnerable tsunami hazard regions. A comprehensive geovisualization tool for mapping tsunami-related publications is proposed as a basis for identifying information gaps, promoting new research areas, and correcting existing imbalances.


Wed-02 Aug | 10:20 - 12:20 | MR305
IG13 - The Effect of Extreme Weather, Heat Waves, and Urban Heat Islands on Public Health and Agriculture: Vulnerability, Impacts, Adaption, and Mitigation

Session Chair(s): Paolo TAROLLI, University of Padova, Yuei-An LIOU, National Central University

IG13-A002
Changes of Extreme Climate Events in Rice-growing Regions Under Different Warming Scenarios

Weixing ZHAO#+, Jieming CHOU
Beijing Normal University

Scientific prediction of critical time points of the global temperature rise and assessment of the associated changes in extreme climate events can provide essential guidance for agricultural production, regional governance and disaster mitigation. Using daily temperature and precipitation model outputs from the Coupled Model Intercomparison Project (CMIP6), the time points of the temperature rise by 1.5°C and 2.0°C have been assessed under three different greenhouse discharge scenarios (SSP126, SSP245, SSP585). To characterize the change of extreme climate events in rice growing regions in China, six indices have been designed, and a time slice method is used. An analysis from an ensemble of CMIP6 models shows that under SSP245, the global mean temperature rises by 1.5°C/2.0°C around 2030/2049. A global warming of 2.0°C does not occur under SSP126. The time for a 1.5°C/2.0°C warming all becomes earlier under SSP585. Under a 1.5°C warming, the number of warm days (TX90p), rice heat damage index (Ha), consecutive dry days (CDD), five-day maximum precipitation (Rx5day) and the number of annual total extreme precipitation events (R99pTOT) clearly increase, while the number of cold damage (Cd) events decreases. All the indices show a strong variability regionally. For example, the consecutive dry days (CDD) increases significantly in the Central China and South China rice growing region. The monthly maximum consecutive 5-day precipitation increases by as much as 6.8mm in the Southwest China rice growing region.


IG13-A004
Ecosystem Service Underpins Sustainable Development Goals in the Changing World

Wenwu ZHAO#+, Caichun YIN
Beijing Normal University

The Sustainable Development Goals (SDGs), adopted by the United Nations in 2015, act as the heart of the 2030 Agenda for Sustainable Development and provide a shared blueprint that incorporates social, economic and environmental dimensions of sustainability. They express the urgent need to end hunger and poverty, improve health and education, promote development and reduce inequality while addressing climate change and land degradation in the changing world. Embedded in the SDGs agenda, there is a crucial aim to value ecosystem services (ESs) and restore and enhance their integrity and functions. Due to the multifaceted development vision covered by the 17 Goals, achieving the SDGs is an ambitious task that requires multidisciplinary efforts. The ESs that soil provide for agriculture, water conservation, and biodiversity are vital to achieving the SDGs. ESs are the benefits that humans obtain from ecosystems. ESs support human well-being from basic livelihood (e.g., water and food) to higher-level needs (e.g., garden cities and ecotourism), contributing directly or indirectly to SDGs’ achievement. ESs are the benefits that humans obtain from ecosystems. ESs support human well-being from basic livelihood (e.g., water and food) to higher-level needs (e.g., garden cities and ecotourism), contributing directly or indirectly to SDGs’ achievement. For the future research on ecosystem services and sustainable development, we not only need to protect ecosystem for better ecosystem services, but also integrate ecosystem services into the achievement of sustainable development goals, and make the best use of ecosystem services for a better future.


IG13-A009
Climate Change-induced Drought: Agriculture in Northeastern Italy During the Extremes of 2022

Paolo TAROLLI+, Eugenio STRAFFELINI#
University of Padova

Agriculture is widespread in Italy, especially in the lowland area of the northeast crossed by the Po River. It is one of the most important rural landscapes in Europe and is crucial for food production. However, human-induced climate change is affecting the entire sector, with potentially devastating impacts in the future. One of the most worrying trends is the increasing frequency of long and intense droughts, making the climate progressively more arid. Due to heatwaves and severe water shortages, the summer of 2022 was one of the most difficult seasons in decades. Crop losses, irrigation problems, and saltwater intrusion in the Po River delta have severely affected agriculture. Quantifying agricultural drought is not easy, and several methods exist. Among the most widely used procedures are specific indices based on satellite observations that can map drought-affected spots for vast rural regions. In this research, we applied the Vegetation Health Index (VHI) in northeastern Italy in the summer of 2022. The calculation was done through the Google Earth Engine platform, which combines a vast catalog of spatial data with powerful computational capabilities, using MODIS products and following guidelines offered by the UN-SPIDER Portal (United Nations Platform for Space-based Information for Disaster Management and Emergency Response). Specifically, we mapped which areas were most affected by drought, and identified the agricultural systems that experienced the greatest stress. In a climate change perspective where similar extreme weather conditions could happen again in the near future, knowing which areas are at risk is a first step toward more resilient management of agriculture and water resource. *Acknowledgments - This study was carried out within the Agritech National Research Center and received funding from the European Union Next-GenerationEU (PIANO NAZIONALE DI RIPRESA E RESILIENZA (PNRR) – MISSIONE 4 COMPONENTE 2, INVESTIMENTO 1.4 – D.D. 1032 17/06/2022, CN00000022).


IG13-A010
Saltwater Intrusion in the Po River Delta (Italy) During Drought Conditions: Analyzing its Spatio-temporal Evolution and Potential Impact on Agriculture

Jian LUO1+, Eugenio STRAFFELINI2#, Paolo TAROLLI2
1Inner Mongolia University, 2University of Padova

Saltwater intrusion is a complex process controlled by multiple factors and thus fluctuates with a highly nonlinear nature and time-varying characteristics. It is challenging to monitor saltwater intrusion. The objective of this study was to clarify the spatial-temporal variation of saltwater intrusion and its potential impact on agriculture in the Po River Delta (Italy). 2006 was the most severe year of saltwater intrusion in the period we considered (we did not consider the critical year of 2022 since data are still under analysis). In this study, the Hilbert-Huang transform (HHT) and rescaled range (R/S) were used to identify the multi-time scales and change trends of the salinity and discharge in 2006. After that, the time-dependent intrinsic correlation (TDIC) was used to depict intrinsic relationships between salinity and discharge at different time scales. The results showed that discharge and salinity exhibited behaviours of positive long-range correlation during different periods. The temporal series of salinity and discharge was decomposed into six intrinsic mode functions (IMF) and residuals based on the EEMD method. The sum of variance contribution rates of IMF1 (4 days), IMF2 (10 days), and IMF3 (12.1 days) of salinity was more than 75%. All measured TDICs have highlighted strong correlations between salinity and discharge. Furthermore, we interpolated the salinity data along the rivers using a GIS approach to clarify the dynamic changes of saltwater intrusion under extreme drought conditions. Outcomes show a significant negative correlation between salinity and NDVI, indicating that the study area's agricultural greening was affected by saltwater intrusion. *Acknowledgments - This study was carried out within the Agritech National Research Center and received funding from the European Union Next-GenerationEU (PIANO NAZIONALE DI RIPRESA E RESILIENZA (PNRR) – MISSIONE 4 COMPONENTE 2, INVESTIMENTO 1.4 – D.D. 1032 17/06/2022, CN00000022). The authors also thank Start-up funding from Inner Mongolia University (21800-5223728).


IG13-A012
Remote Sensing Assessment of the Weeds Adaptability to Soil Salinization Induced by Extreme Droughts on Coastal Agriculture

Nebojša NIKOLIĆ#+, Eugenio STRAFFELINI, Roberta MASIN
University of Padova

Soil salinization is a critical factor contributing to the loss of crop production. Worldwide, the area of salinized soils is increasing. This phenomenon seriously affects the arid and semi-arid regions but is expanding towards temperate regions. More attention should be given to the role of weeds in this scenario. Weed adaptability to adverse environmental conditions might promote their diffusion and competition capability under increasing salinity. Remote sensing techniques may be used to obtain useful information at different spatial scales. The Structure from motion (SfM) technique paired with Unmanned Aerial Vehicles (UAV) was used to map the distribution changes of Abutilon theophrasti and Echinochloa crus-galli in July and August 2022 in different crop fields in the Po river delta, North-Eastern Italy. Orthomosaics obtained had an image resolution of 2 cm, allowing an accurate photo interpretation and precise distribution maps creation. Salinity maps of these fields were created by spatializing the salinity values in the study area using spatial interpolation tools of the Geographic information system (GIS) software, based on the electrical conductivity values of soil samples collected. The salinity maps overlapped the maps of single plants of the studied species. Both multi-temporal surveys show that weed species studied can be found in areas with soil salinity higher than 8 dS/m, where most crop plants have perished. The presence of studied weed species in these areas indicates that weeds can tolerate soil salinity better than the crops and can therefore outcompete them. These results suggest that soil salinization can negatively affect crop production and food security, causing abiotic stress and increasing competition. Acknowledgments: This study was carried out within the Agritech National Research Center and received funding from the European Union Next-GenerationEU (PIANO NAZIONALE DI RIPRESA E RESILIENZA (PNRR) – MISSIONE 4 COMPONENTE 2, INVESTIMENTO 1.4 – D.D. 1032 17/06/2022, CN00000022).


IG13-A001
Dynamics of Golf Course Land in the Hanoi City Metropolitan by Remote Sensing and GIS

Kim Anh NGUYEN#+, Yuei-An LIOU
National Central University

Urbanization has been taking place with continuous population growth over the major cities all over the world for decades. With the rapid development of society, people's entertainment needs are increasing day by day in order to keep good health. To fulfill the needs, some types of sports thus become popular, such as volleyball, football, swimming, and golf. Among them, golf that typically requires a huge area for one standard course especially built over the natural area may likely affect the environment and hence deserve much attention in a fast-developing country such as Vietnam. In this study, remote sensing has been applied to monitor the spatiotemporal distribution of golf courses in the Hanoi City Metropolitan, North Vietnam where has 24 golf courses out of a total of 58 golf courses across the country and occupies 9.27 thousand hectares of land. We use the multi-satellite data to examine the spatial dynamics of the golf courses and investigate the evolution of features of the golf courses in the Hanoi City Metropolitan and their surrounding areas. GIS is adopted to assist the analysis of the information acquired from satellite images and consensus data. The main results of this work include (1) the database of golf courses in the Hanoi City Metropolitan determined by remote sensing, (2) the analysis of the dynamics change of the golf course lands in the past decades; and (3) the analysis of conversion from the other lands types to golf courses and its impacts. The proposed golf course mapping scheme can be applied for extracting different elements in the golf course such as trees, water, bunkers, fairway, and green surface, or even tree types for the region of interest. The results of the study may be potentially useful in assisting the management of golf course for the environmental sustainability.


IG13-A016
Equalizing the Spatial Accessibility of Emergency Medical Services in Shanghai-A Trade-off Perspective

Mengya LI#+
East China Normal University

Planning public services needs to promote equal access across geographic areas and between demographic groups. However, most location-allocation models emphasize efficiency such as minimal travel burden or maximal demand coverage while omitting the equality issue. This case study optimizes the emergency medical service (EMS) in Shanghai from a trade-off perspective by comparing two models. One is the 2-step optimization (2SO) model that uses the maximum covering location problem (MCLP) to site new facilities and then a quadratic programming (QP) method to optimize capacities, the other performs location selection and capacity optimization simultaneously through greedy optimization (GO). There are several findings from various simulation scenarios. First, the GO model is more effective in optimizing equality, but the 2SO model offers a more balanced approach by covering more people within the mandatory response time while improving access equality. Secondly, solutions of both models change as demands and travel costs vary over time and call for dynamic adjustment of resource allocation. Thirdly, it is important to coordinate EMS with other agencies to ensure reasonable road connectivity and make contingency plans in events such as floods, earthquakes and other natural disasters.


Wed-02 Aug | 10:20 - 12:20 | MR323
IG18 - Geoscience Education

Session Chair(s):

IG18-A001
Public Awareness as a Key Success Factor of Environmental Policy: a Case of Environmental Education for Sustainable Groundwater Use

Minha LEE+, Heejung KIM#
Kangwon National University

The exacerbating global environmental issues are pressurizing the world to become smarter, bolder, and more diligent at local, regional, national, and international levels to achieve sustainable development. On the contrary, forcing an individual, an industry, or a nation into a particular action through policy effectuation is becoming increasingly difficult in today’s competitive and globalized world. In combination, environmental education has become one of the key factors to establish sustainable lifestyle at individual, industrial and national levels. Ultimately, the effectiveness of every environmental policy implemented boils down to smarter choices, more diligent and proactive decisions made by an individual person. For a correlation test between public awareness and policy acceptance, the paper compared tax/fee resistance level of “reusable cup deposit” to “groundwater charge.” The national environmental education contents have been studied to compare public educational exposure on “plastic pollution” and “groundwater depletion.” The data was further examined against policy implementation rate across major cities of South Korea on two environmental policies. Finally, a survey was conducted to 300 individuals residing in South Korea to double check education effects and policy acceptance level against collected data. The three-step analysis revealed positive contribution of public promotion and education towards public awareness enhancement on the subjected topic and improved policy compliance on related environmental policies. These results suggest that the addition of groundwater in the environmental education curriculum may contribute towards sustainable groundwater use.


IG18-A002
A Case of Literary and Historical Interdisciplinary Earth Science Education: Kangxi Taipei Lake

Yi-Chen HSU#+
Foothill Story Cafe of Gomach

In 1694, there was a significant mystery disaster occurred in northern Taiwan. It started from earthquakes in Taipei basin, and end as a huge lake recorded from ancient books. This lake named as Kangxi Taipei Lake. General consideration is a large earthquake induce Shanchiao fault subsidence then make seawater intrusion into Taipei basin. However, recent years researches reveal doubts about the scenario of the large earthquake and the authenticity of Kangxi Taipei Lake. Through the analysis of the clues and the investigation of climate change evidences of northern Taiwan, this study suggests that the precipitation anomaly should be the main driver and reconstructs a more reliable scenario of the 1694 Taipei earthquakes and the existence of Kangxi Taipei Lake. Moreover, a novel based on the new scenario integrates Taiwan’s aboriginal tribes and international exchanges of northern Taiwan in 17th century has published to propagate the historical story combines the earth science background. In addition, a solid model of Kangxi Taipei Lake also established to demo different possibilities of lakes upon the Taipei basin across all the geological ages. The combination of literary novel and solid model to promote the interdisciplinary story has successfully displayed in the stall of Taiwan Science Festival and the story coffee shop with earth science and historical theme for wider expansion of interdisciplinary earth science education.


IG18-A003
Development of a Space Science Curriculum for Students

Hoe Teck TAN#+
School of Science and Technology

The Discover Space Camp is conceived as part of the Discover Camp that the School of Science and Technology Singapore (SST) organises for its graduating students. The aims of the Discover Camp are to expose the students to career and academic possibilities that they will be making decisions in the near future. The Discover Camp is designed to incorporate Applied Learning approaches in its delivery. Applied Learning includes activities that are learner centred, active, relevant, process focused, integrated, authentic, or community focused. Space Science encompasses all of the scientific disciplines that involve space exploration and the study of natural phenomena and physical bodies occurring in outer space, such as space medicine and astrobiology. The Discover Space Camp was conceived because of its growing presence in the educational and career landscape that the students in the near future will be exposed to. The programmes consisted mostly of theory lessons, talks by scientists, and hands-on applications in the field of Space Science. The AOGS community plays an important part in helping to shape the development of this programme. They provided insights to the field of Space Science through their direct research and applications of the Space Science and Technologies. The response from the students were favourable as the information and learning provided were directly from the people in the industry. Through this sharing, I hope to motivate the audience to develop programmes to further the outreach of Space Science and Geo-Science alike. This is also an invitation to gather other interested geoscientists or space scientists to contribute to such programmes in the future.


IG18-A004
An AR-integrated Board-game for Promoting the Education of Net-zero Emissions Issue: The Design and Effectiveness

Ping-Han CHENG#+
National Taipei University of Education

This research presents the development and effectiveness of a Net-Zero Emissions AR (Augmented Reality)-integrated board game, which improve the learning of climate-change issues. The education of climate-change and Net-Zero Emissions will profoundly impact the future development of human societies. However, there are vital educational issues to address, including low learning motivation, abstract and complex systemic concepts, and the gap between learning outcome and learning transfer. In this study, we developed a board game to assist learners in constructing systemic concepts as well as cultivate their attitudes and behaviors, and integrated AR technology to strengthen learners' scientific and social inquiry ability. Based on situated learning, the participants of the game played the role of citizens. They need to consider transportation, housing, food, and other behaviors in daily life, so that they can live comfortably while taking into account a friendly environment. After playing the game, we used the Likert-scale questionnaire to evaluate participants’ attitude and the concept-map test to exam their systemic concept of Net-Zero Emissions. Moreover, we also used the situated assessment to inspect learners' scientific and social inquiry ability. Based on the result, this study will show how AR-integrated materials can help solve the key difficulties faced during learning climate-change issues by improving motivation, systemic conception, fostering learners' high-level cross-domain competencies, and finally bridge the gap between outcome and transfer of learning.


IG18-A005
Space Weather Outreach Education of Central Weather Bureau in Taiwan

I-Te LEE1,2#+, Jyun-Ying HUANG3, Chao-Yen CHEN2
1Central Weather Adminstration, 2National Central University, 3Central Weather Bureau

Recently, changes in the space environment have aroused people's interest with the rise of the global space industry and the gradual increase of solar activity. Although the term of “space weather” refers to all variable physical parameters and conditions on the Sun and in the space environment, such as solar wind and radiation, plasma density, high-energy particles, and magnetic fields. But the solar surface and formation of auroras are the two topics that remain of greatest interest to the general public. Therefore, the Central Weather Bureau has developed materials and outreach activities based on these two themes in the past two years. To observe sunspots and prominences by solar telescopes, to demonstrate the formation of the aurora by a plasma globe, as well as to explain the color of aurora by a set of spectrum tubes. Moreover, images composed from satellite observations to be use for spherical projection systems, such as the Science on a Sphere and the Dagik Earth. In order to promote preventive notions of disasters and provide information about space weather, the Central Weather Bureau in Taiwan not only monitors and forecasts space weather conditions as well as conducts education outreach activities. This presentation will demonstrate achievements of outreach education and introduce and discuss for more details about these experiments and activities.


IG18-A007
Advancing Geoscience Literacy in the Philippines Amidst Covid-19 Pandemic Using the Central Visayan Institute Foundation (CVIF)-dynamic Learning Program (DLP)

Janneli Lea SORIA1#+, Ruby Anna RAÑOA2, Jodivine NAVAROSA2, Benia Nika LAO-TABIGUE2
1Institute of Environmental Science and Meteorology, University of the Philippines-Diliman, Quezon City, 2Central Visayan Institute Foundation

The CVIF-DLP is a learning framework developed by 2010 Ramon Magsaysay Awardees and acclaimed Filipino theoretical physicists, Dr. Ma. Victoria Carpio-Bernido and Dr. Christopher Bernido, which, in partnership with the PLDT-Smart Foundation, Inc., has spread to more than 200 institutions at the elementary, secondary, and tertiary levels in the Philippines. This learning program which was implemented at the Central Visayan Institute Foundation since 2002 aims to develop independent learners and improve their academic performance despite the manifold socioeconomic constraints that typically plague the Philippine educational system such as lack of qualified teachers and limited learning infrastructures. These learning obstacles were even further amplified when Covid-19 pandemic caused global disruptions in the delivery of goods and services including education. In this case study, we present learning activities in geosciences that were developed and distributed to K11 and K12 students at the height of the Covid-19 pandemic in 2020 until the present. We highlight the value of local contextualization of geological concepts in stimulating the curiosity of the learners and developing their interest in geosciences. In using local examples, learners are exposed to concepts that are accessible and relevant to their daily lives rather than hard isolated facts that are only grasped through textbooks. Our formative assessment tools including written learning activities, quizzes, and performance tasks indicate that despite minimal teacher intervention and limited access to fast internet needed for synchronous online classes, learning can be nurtured. This study provides insight on the elements for designing locally contextualized learning activities which may be used even during disruptive events such as pandemic or disasters.


IG18-A009
Comprehensive Learning of Geology Through Peer-evaluated Group Projects in a General Education Course

Xuran ZUO#+
The Chinese University of Hong Kong (Shenzhen)

General Education is an essential part of the university curriculum that exposes students to multiple disciplines. A geology-themed course in General Education always attracts students who are interested in but have no systematic knowledge about Geosciences. However, comprehensive teaching and learning activities for all the topics of geology are limited by the class hours scheduled for one single course and students’ personal interests. To ensure the comprehensiveness of the course and also to encourage students’ active learning, peer-evaluated group projects are designed as a major assessment component of our course. Students can choose from various topics in the field of Earth Sciences, e.g. geoparks, mass extinctions, lunar explorations, climate-related issues, etc., and then work in groups for a thorough and comprehensive presentation of their own topics. Groups with similar topics are required to carefully examine and evaluate the project outcomes mutually, based on their own research in the same area. Meanwhile, they are invited to participate in the presentations of all the other groups. By evaluating their classmates’ projects, students can better understand their target topics and reflect on the pros/cons of their projects. They can also broaden their views through the presentations of other groups. After doing so, the course instructors become guides and facilitators instead of formal authorities dispensing knowledge. Unlike passive learning in a traditional classroom, students become more responsible for their learning. Meanwhile, knowledge becomes something to be constructed, developed, and evaluated rather than content to be received as usual. This pedagogical paradigm has been used twice in our geology course of General Education. It is believed to have enhanced the comprehensive and active learning about various topics of geology, evidenced by students’ overall better academic performance and positive responses throughout the course.


Wed-02 Aug | 1:00 - 5:15 | Summit
IG - Interdisciplinary Geosciences Poster Session

IG01-A001
Development of a Hydrogeological Apparent Model for Choushuichi Alluvial Fan by Integrating Geophysical Exploration Measurements and Machine Learning Analysis

Ping-Yu CHANG#+, Jordi Mahardika PUNTU
National Central University, Taiwan

This study aims to develop a hydrogeological apparent model for Choushuichi alluvial fan by integrating geophysical exploration measurements and analyzing them with machine learning methods. The apparent model is an advanced technology that can substitute traditional conceptual models and provide a more accurate representation of subsurface hydrogeological conditions in the area. The study involves collecting geophysical exploration measurements, including borehole resistivity logs, electrical resistivity, and transient electromagnetic survey data, from the target area. These measurements will be analyzed using machine learning algorithms and borehole core records to extract relevant information about subsurface hydrogeological conditions. The information will be integrated to create an apparent model that can be used to predict subsurface sediment distributions. The results of this study will demonstrate the potential of the hydrogeological apparent model as a powerful tool for understanding subsurface hydrogeological conditions. By using machine learning methods, the apparent model can provide a more accurate and detailed representation of subsurface conditions than traditional conceptual models.


IG01-A002
Hydraulic Properties Evolution Caused by Pore Clogging from ISCO Injection

Bing-Shiun KE#+, Jui-Pin TSAI
National Taiwan University, Taiwan

ISCO (in situ chemical oxidation) is one of the most frequently used soil and groundwater remediation approaches. However, three popular ISCO amendments, Potassium permanganate, Fenton’s reagent, and Sodium persulfate, usually cause pore-clogging due to the formation of precipitation, leading to a decrease in hydraulic conductivity (K). In other words, pore-clogging due to ISCO amendment injection changes the spatial distribution of K, causing a change in the flow paths of amendment and plume. To quantify the spatial change in K, an advanced hydraulic test, hydraulic tomography (HT), can be a useful tool to delineate the spatiotemporal evolution of the K field. In this study, we conduct a sandbox experiment with Fenton’s reagent injection. HT is employed to quantify the spatial change in K, and the soil cores were sampled at the place where K was significantly reduced. Inductively coupled plasma-optical emission spectrometry is also used to measure the increase in Fe(III) in the soil samples. The results show that the concertation of Fe(III) was raised in the areas with decreased K values after injection. The results reveal that HT is the appropriate method for delineating spatiotemporal K fields during the ISCO remediation. This study can benefit the study related to hydraulic – geochemical studies, especially valuable for those related to groundwater remediation.


IG01-A003
Using Signal Analysis and Light Gradient Boosting Machine to Analyze Groundwater Levels of Choushui River Alluvial Fan in Taiwan

Tzung-Hsin TSAI+, Shien-Tsung CHEN#
National Cheng Kung University, Taiwan

This study applied signal analysis on the groundwater level in Choushui River Alluvial Fan in Taiwan. The wavelet analysis and independent component analysis were used to extract principle component information of groundwater level. Moreover, the correlation between the groundwater level and other hydrological variables (rainfall, pumping data, and river flow) were also analyzed by using the signal analysis. Analysis results exhibit that these signal analysis techniques can reveal the interaction of groundwater level with other variables, and can contribute to the understanding of groundwater level variation in the study area. In addition, this study applied the light gradient boosting machine (LGBM) to develop a prediction model for short-term prediction and long-term projection of groundwater level. The LGBM is capable of processing large data sets and category characteristics to build a groundwater level prediction model for the study area. The signal analysis results were used to improve the input selection of the groundwater level prediction model. The prediction performance for one-month lead time is satisfactory in terms of correlation coefficient and efficiency coefficient. Climate change scenarios of SSP2-4.5 and SSP5-8.5 were used to perform long-term projections for the future short-term (2021 to 2040) and mid-term (2041 to 2060) groundwater levels.


IG01-A006
Hydrogeological Investigation using the Transient Electromagnetic Method

Lingerew Nebere KASSIE1+, Ping-Yu CHANG1#, Jun-Ru ZENG1, Hsin-Hua HUANG2, Chowson CHEN1, Yonatan Garkebo DOYORO1, Ding-Jiun LIN 1, Jordi Mahardika PUNTU 1, Haiyina Hasbia AMANIA 1
1National Central University, Taiwan, 2Academia Sinica, Taiwan

We used Transient Electromagnetic (TEM) to map the hydrogeological structures in the Choushui River Alluvial Fan in Yunlin county of central Taiwan. 63 TEM measurements were collected using the FASTSNAP system with 50x50m in-loop configurations in the middle and distal fan. The 1D model, based on prior information, was constructed from the inverted soundings. Results showed a thin, resistive shallow layer and a 40m low-resistive (6-42 ohm-m) zone beneath it. High-resistive zones (50-170 ohm-m) were found from 50-120m depth, and low-resistive zones were revealed below 120m in some areas. Results were consistent with resistivity and lithology logs from nearby wells. We interpolated resistivity at 10m, 50m, 100m, and 160m depth from the 1D model results to produce a slice map of the area, which indicated variations, trends, and depths of the sediment deposits. The TEM method successfully identified the hydrogeological structures, showing that the upper 40m of sediment acts as a confining layer for the aquifer structure from 50m to 120m depth.


IG01-A007
Characterizing the Hydraulic Heterogeneity of a Contaminated Site in Taiwan Using Hydraulic Tomography and Fiber Bragger Grating Multilevel Monitoring System

Jui-Pin TSAI1#+, Tian-Chyi YEH2, Yen-Te HO3
1National Taiwan University, Taiwan, 2The University of Arizona, United States, 3CITPO Technology, Taiwan

Hydraulic tomography (HT) is a new hydraulic test method for characterizing heterogeneous aquifer properties. We need to perform sequential pumping/injection tests for the HT test, and a group of wells is employed to measure the groundwater pressure variations for every test. The pressure variations are then transformed into aquifer properties using the geostatistics approach. In the traditional HT test, the conventional wells for collecting pressure data often open screens at a single target depth. In other words, a single well can only measure the pressure in one depth range. In contrast, a multilevel well has several open-screen at the target depths. Thus, the number of pressure observations from the multilevel well can be several times more than that of a traditional well. Accordingly, this study employed a new multilevel well system, developed by fiber Bragg grating technology, to conduct HT at a contaminated site in Taiwan. We then compare the estimate with those from depth-average pressure data, which represents the traditional well. The results show that the parameter estimate from FBG multilevel well is better than that of a conventional well. Results also reveal that HT with a multilevel well system benefits HT and has the potential to be the next-generation hydraulic test.


IG01-A009
Evaluation of Hydraulic Control on the Remediation of Groundwater Chlorinated Contamination

Chih-Yu LIN#+, Sheng-Wei WANG
Tamkang University, Taiwan

Groundwater chlorinated organic contamination is a global concerning issue. Biostimulation by injecting organic carbon substrate is an environmental-friendly in-situ remedy. Due to the slow transport of groundwater flow, the concept of groundwater circulation well has been widely applied for increasing the effectiveness of bioremediation. In this study, a groundwater vinyl chloride (VC) contaminated site is collected to simulate the transport and chemical reactions by MODFLOW program with RT3D package. The average hydraulic conductivity and hydraulic gradian are 4.93 m/day and 0.0003, respectively. Three pumping wells with a flow rate of 60 m3/day were set up in the downstream area of this model. Monitoring groundwater levels were used for model calibration. The difference between simulated and observed heads was reduced to 0.45m by Parameter Estimation (PEST). According to the results of model verification, the simulated drawdown and flow velocity coincide with the field measurement. The groundwater velocity increases from 6.11×10-5 m/day to 1.45×10-2 m/day by continuous pumping. Moreover, a significant difference in VC decreased by injecting persulfate between the natural groundwater flow and the hydraulic control scenarios. Advanced persulfate injection with hydraulic control effectively accelerates the degradation of VC plume. The established model can be used as a convenient and fast assessment tool for the design of pumping wells network in the future.


IG01-A011
Making the Invisible Visible: Evaluation of Inter-catchment Groundwater Flow Using Deterministic and Stochastic Method

Hsin-Yu CHEN#+, Hsin-Fu YEH
National Cheng Kung University, Taiwan

The hydrological model, often known as the closed model, typically assumes that there is no groundwater exchange at the boundaries between catchments. Yet, this assumption is rarely satisfied. To assess inter-catchment groundwater flow (IGF), five adjacent catchments in Taiwan's Choshui River Basin were chosen as the study area. The Generalized Likelihood Uncertainty Estimation (GLUE) method and the Shuffled Complex Evolution - University of Arizona (SCE-UA) optimization algorithm were combined in the open lumped rainfall-runoff abcd model to assess groundwater exchange from the stochastic and deterministic perspectives, respectively. To understand whether each catchment was in a gaining, leaking, or isolating state, the open rainfall-runoff model's groundwater exchange parameter (xg) and the effective catchment index (ECI) were utilized simultaneously. For instance, groundwater was received by the Nei-Mao-Pu catchment. The deterministic method estimated the change of IGF over time, and the results showed that the performance of open rainfall-runoff model was superior to the closed model. The stochastic method estimated the possible intervals of IGF at each time step. However, since IGF cannot be measure directly, this study collected additional water balance fluxes and compared the consistency between simulated evapotranspiration and observed evapotranspiration to indirectly verify the justifiability of estimated IGF. In addition, the proportion of IGF to the rainfall was larger in the dry season than in the wet season. This study suggested that groundwater exchange plays a significant role in the hydrological cycle. This study is expected to advance our scientific knowledge of groundwater and contribute to the sustainable groundwater development.


IG01-A013
Hydraulic Heterogeneity Estimation Using Convolutional Neural Network and Hydraulic Tomography

Yukai CHEN#+, Jui-Pin TSAI
National Taiwan University, Taiwan

Hydraulic tomography (HT) is a well-developed approach for estimating three-dimensional hydrogeological parameter fields. The widely used inverse method for HT is the successive linear estimator (SLE). SLE is a well-proved geostatistical method employed in various scale problems. However, SLE’s computational efficiency decreases as the number of parameters and observations increases. To overcome this issue, we propose an HT-based convolutional neural network (HT-NN) to replace SLE for converting head/drawdown data to hydraulic heterogeneity. We developed a two-dimensional groundwater flow model via VSAFT2 to generate large data pairs (head data and K/Ss). These data pairs are then used to train the HT-NN. The results reveal that HT-NN successfully converts the head dataset to K and Ss fields. The values of MAE, RMSE, and R2 of the predicted K field in the validation process are 2.502, 3.269, and 0.623, respectively. Besides, the values of MAE, RMSE, and R2 of the predicted Ss field in the validation process are 0.001, 0.002, and 0.795, respectively. These results reveal that the developed HT-NN can be an efficient tool to accurately delineate the hydraulic heterogeneity and benefit groundwater-related studies.


IG01-A014
Analysis of the Impact Extents of Salinity by Seawater Intrusion in the Geumgang Estuary Using Opengeosys

Hyun Jung LEE1+, Hyung-Ju YOO1, Seung-Jin MAENG2, Seungoh LEE1#
1Hongik University, Korea, South, 2Chungbuk National University, Korea, South

Discharge and water surface elevation in Geumgang estuary are controlled by roller gates to secure living, industrial, and agricultural water in the basin. However, because of mostly operated as the closed estuaries, requests are conflicting in the view of the demand for opening to form a brackish water area and concerns about crop damage due to saltwater intrusion when opened. Currently, 5.0 x 10^6 m^3, which takes 62.2% of the annual groundwater use upstream of the estuary is used for agricultural purposes, mainly for paddy rice. Thus, it is crucial to consider the spatial and temporal extent of seawater intrusion impact. To consider the optimal seawater distribution between making brackish water zone and the minimum seawater intrusion distance upstream, three scenarios were set according to the period and the water level difference with three different numerical models: MODFLOW, FEFLOW and OpenGeoSys. Boundaries of this study area were constructed with a digital elevation model (DEM) with a spatial resolution of 90 m, and water level and salinity data from four groundwater observed stations. Model was verified by obtaining Root Mean Squared Errors of 0.1~ 0.16 m and 0.89 ~ 0.92 of coefficient of determination (R2) between observed groundwater level and predicted values acquired from 2018 to 2022. Then, the model was applied to the Geumgang area to identify the extents of seawater wedge. If meteorological data like temperature, rainfall and tidal level from the Representative Concentration Pathways (RCP) are added to further study, it could be used to predict and prevent the impact of the seawater intrusion from climate change.


IG01-A017
Experimental Study on Non-Darcian Flow and Hydraulic Conductivity Variation Through a Single Fracture

Snigdha PANDEY#+, Pramod KUMAR SHARMA
Indian Institute of Technology Roorkee, India

The groundwater flow rate, in general, varies spatially through the volume of fractured rocks. This is attributed to their fundamental characteristic of spatial variation in hydraulic conductivity. Therefore, the standard methods used for the characterization of porous media hold limited significance in the case of fractured rock aquifer (FRA) systems. The proposed study is aimed to study the influence of geometric and hydraulic parameters on the flow and hydraulic conductivity of a single artificial fracture. A series of laboratory experiments were conducted to simulate groundwater flow through a single rough-walled fracture with 3 mm and 12 mm fracture apertures under unconfined flow conditions. Flow characteristics through fracture were found to be essentially non- Darcian for different flow velocities. Evaluation of Local cubic law further suggested the dominance of inertial terms for the flow. With the increase in aperture size, the gradient of Reynold’s number with average flow velocity was found to increase. The flow-characterizing parameters of the Darcy, Izbash, and Forchheimer models were calculated using nonlinear regression, and their suitability was tested for the prevailing flow conditions. Hydraulic conductivity was found to vary with space for different apertures and hydraulic gradients, mainly due to the surface roughness and induced 2-D torturous flow in the fracture.


IG01-A020
An Integrated Platform for Real-time Groundwater Modeling and Data Visualization

Chuen-Fa NI#+, I-Hsien LEE, Gumilar Utamas NUGRAHA, Thai Vinh Truong NGUYEN, Ping-Yu CHANG
National Central University, Taiwan

The integrated technologies and multidisciplinary knowledge of groundwater have enhanced the understanding of dynamics in groundwater systems. Taking advantage of wide developments in computer sciences and web services, the web platform provides an excellent open environment for groundwater investigations. The study aims to develop an online web-based platform for groundwater data visualization, temporal and spatial data analysis, mesh generation, and flow modeling. The study integrates multiple program languages to bridge the data flow and online visualization. The interactive real-time web environment enables users to screen temporal and spatial measurements on the web map, conduct online data analyses, and develop numerical groundwater models. With a well-designed database and numerous modules for data analyses and modeling, the platform allows users to share data and develop collaborative activities. The built-in analysis tools can also improve the efficiency of groundwater management and decision-making processes.


IG02-A005
What Did We Learn from COVID?

John Barnett GAANO#+, Camille RULE, Jimuel Jr CELESTE, Vena Pearl BONGOLAN
University of the Philippines Diliman, Philippines

We revisit the previous modelling we did, which revealed: a) prioritizing the low-income group in a low-income country might be the better strategy and b) the high cost of vaccine hesitancy. Various improvements were done to the previous model, all calibrated by Philippine data. As Covid nears its fourth year, it now makes sense to add a population’s vital statistics to the model, to make it more responsive to changes in demographics, following through on our previous theory of age-stratification. Hypothetical scenarios such as reinfections and waning immunity were likewise factored in, although these are far from certain due to succeeding outbreaks being caused by different variants. More difficult to catch would be a population’s underlying “genetic vulnerabilities”, i.e., if they are prone to one or more of the known Covid co-morbidities. There is little local data on this, and we might have to rely on international data if they can be reasonably be used as a similar datapoint.


IG02-A006
Vulnerable Communities: Examining the Cost of Forgoing Vaccination in the BARMM Region

Jose Marie Antonio MIÑOZA1#+, Vena Pearl BONGOLAN1, Roselle Leah RIVERA1, Romulo DE CASTRO2
1University of the Philippines Diliman, Philippines, 2University of San Agustin, Philippines

This study examines past research on the BARMM region in the Philippines, an area that was expected to have high vaccine hesitancy. Previous studies found that factors such as low income, low pre-Covid vaccination rates, and poor delivery of services did not greatly affect vaccine allocation methods. The current study examines the impact of school reopening scenarios and finds that regions with low or slow vaccination rates, such as BARMM, were among the last to reduce risks from the ongoing pandemic. This suggests that there may be a cost associated with vaccine hesitancy. The study then utilizes a cost utility function, based on Bayesian Regret, to evaluate the expected reduction in infection and death rates under a scenario of no vaccine hesitancy (optimal strategy).


IG02-A007
Detection of Thermokarst and Vegetation Succession from Multitemporal Satellite Images

Hitoshi SAITO1,2#+, Yoshihiro IIJIMA3, Takashi KIRIMURA4
1Nagoya University, Japan, 2The University of Tokyo, Japan, 3Mie University, Japan, 4Kogakkan University, Japan

Eastern Siberia is characterized by widespread permafrost thawing and subsequent thermokarst development in open natural and anthropogenic landscapes. The thermokarst development affects the hydrological processes, ecosystems, and human society accompanied by vegetation succession and degradation. In the last few years, a satellite constellation system attracted a tremendous amount of interest in acquiring frequent cloud-free images. This study detected the early-stage thermokarst and vegetation succession using multitemporal satellite images of PlanetScope. We focus on the changes in the normalized difference vegetation index (NDVI) of grasslands around the Churapcha area in eastern Siberia. The results showed that the NDVI of grasslands with early-stage thermokarst landforms was higher than that of grasslands without thermokarst development. The differences in NDVI were large during the summer growing season from June to August. Analysis of the time series NDVI over the past 20 years showed an increasing tendency in NDVI in early-stage thermokarst grasslands with a history of anthropogenic land use. These results indicate that increases in soil moisture and soil temperature may affect rapid vegetation growth and succession at the early-stage thermokarst landforms. Further study is necessary to verify the results using field observation over a wide area of eastern Siberia.


IG02-A014
Performance of the Drought Indices in the Different Agricultural Systems

Seonyoung PARK#+
Seoul National University of Science and Technology, Korea, South

Drought has a significant impact on a region's economy, and its severity is determined by the level of infrastructure in the affected region. For adequate assessment and mitigation, it is important to consider not only the conventional environmental properties of drought, but also the infrastructure of the target region. Drought indicators are provided to interpret the various meteorological, agricultural, and hydrological characteristics of droughts. However, because each of these drought indices has its own characteristics, it is difficult to contemplate an adequate assessment of drought impact. In this study, we investigated the applicability of satellite-based drought indices over South and North Koreas, which have different agricultural infrastructure systems. Over the Korean Peninsula, we compared satellite-based drought indices to in-situ drought indices, the standardized precipitation index (SPI), and rice yield. Drought indices were derived for the period from 2001 to 2018 using data from the Moderate Resolution Imaging Spectroradiometer (MODIS), Tropical Rainfall Measuring Mission (TRMM), and the Global Land Data Assimilation System (GLDAS). The performance of the indices in monitoring meteorological and agricultural droughts revealed opposed correlation patterns between the two countries. It is considered that drought impacts differed due to differences in agricultural systems, especially irrigation. The vegetation condition index (VCI) and the evaporative stress index (ESI) are ideally suited to assessing agricultural drought in well-irrigated regions such as South Korea. In contrast, most of the drought indices—with the exception of the temperature condition index (TCI)—are appropriate for regions with poor agricultural infrastructure, such as North Korea.


IG02-A015
Landslide Risk Analysis in Ciletuh Geopark Area, Ciemas Subdistrict, West Java, Indonesia

Qonita Nur SHOFIYAH#, Kemala WIJAYANTI+
Universitas Padjadjaran, Indonesia

Landslide is one of the disasters that often occur in the Ciletuh Geopark area, Sukabumi Regency, West Java Province, because of the rock conditions and topography. This study aims to determine the magnitude of the potential for landslides in Ciemas District, which often occur, to determine the impact of landslides on the environment and people's lives, and to determine ways to reduce the effects of landslides. The methods used in this research are secondary research methods, literature studies, and scoring methods. The data analysis used is in the form of quantitative data analysis with a descriptive approach. Landslide-prone areas in Ciemas District are divided into four categories based on slope parameters, rainfall, bedrock type, soil type, geological structure, and land cover. The four categories are low vulnerability covering 24% of the study area; moderate vulnerability covering 33% of the study area; high vulnerability surrounding 33% of the study area; and very high exposure covering 10% of the study area. Districts with a high level of vulnerability to landslides are Cibenda, Ciemas, Girimukti, Mekarjaya, Mekarsakti, and Tamanjaya Districts. The impact of landslides on the environment and people's lives in Ciemas District is damage to people's houses with severe to light levels of damage, disruption of toll road access, and temporary closure of tourist areas. In addition, mitigation efforts can be carried out in structural and non-structural mitigation. Disaster mitigation that can be done is planting taproot vegetation in areas with grassland land cover and the built-up regions, building gabions in areas with steep slopes, making landslide zoning maps, conducting counselling, and outreach about landslides and their mitigation.


IG02-A019
Stochastic Simulation of Tropical Cyclones for Risk Assessment at One Go: A Multivariate Functional PCA Approach

Chi YANG1#+, Jing XU2
1Beijing Normal University, China, 2Chinese Academy of Meteorological Sciences, China

Tropical cyclones (TCs) are one of the biggest threats to life and property around the world. However, the infrequent nature of catastrophic TCs invalidates the standard actuarial loss estimation approaches. TC risk assessment requires estimation of catastrophic TCs having a very low occurrence probability, or equivalently a very long return period spanning up to thousands of years. Since reliable TC data are available only for recently decades, stochastic modeling and simulation turned out to be an effective approach to achieve more stable TC risk estimates for regions where little or no historical TC records exist. Here we present a novel model for the full-track simulation of TCs for risk assessment, via multivariate functional principal component analysis approach. Elemental variables of TC along the track necessary for risk assessment, such as center coordinates, maximum wind speed, minimum central pressure and ordinal dates, can be simulated simultaneously at one go, using solely the best-track data with no data supplemented from any other sources. The simulation model is optimally determined by means of the ladle estimator. A TC occurrence model using the Conway–Maxwell–Poisson distribution is proposed as well, by which different dispersion features of annual occurrence can be represented in a unified manner. With the occurrence model, TCs can be simulated on an annual basis. The modeling and simulation process are programmed and fully automated such that little manual intervention is required, which greatly improves the modeling efficiency and reduces the turnaround time, especially when newly available TC data are incorporated periodically into the model. Comprehensive evaluation shows that this approach is capable of generating high-performance synthetic TCs in terms of distributional and extreme value features, which can be used in conjunction with wind field and engineering vulnerability models to estimate economic and insurance losses for governments and insurance/reinsurance industry.


IG02-A020
Landslide Preparedness and Response of Selected Communities in the Philippines

Maria Regina REGALADO#+, Decibel FAUSTINO-ESLAVA, Beth Zaida UGAT, Jenielyn PADRONES, Loucel CUI, Juan Miguel GUOTANA, Rosemarie Laila AREGLADO, Bianca Maria Laureanna PEDREZUELA1,1, Jefferson RAPISURA, Gabriel Angelo MAMARIL
University of the Philippines Los Baños, Philippines

Aside from studying the geophysical characteristics of landslides, understanding the perception of the local communities residing in landslide prone areas is a great help in planning for disaster risk management. While planning for engineering-based solutions, risk reduction can also be effective by mainstreaming risk information in communities. However, it is important to determine first the perception of the local communities. To determine risk perception, landslide preparedness and response towards landslide occurrences, household surveys were conducted in the provinces of Benguet, Albay, Sorsogon, and Northern Samar, Philippines. This study also looked into the available sources of landslide information of respondents from the study areas. Results of the survey showed that respondents who think they are prone to landslides are willing to relocate. However, the results also showed that several respondents, despite residing near landslide areas, believed that they are not at risk to landslides. Results also indicated that the top trusted source of information of the respondents are TV, radio, community leaders, and local government officials. While choosing information campaign materials, respondents from Benguet, Northern Samar, and Sorsogon preferred radio and posters, while respondents from Albay preferred radio and videos made available over the internet. The results of the survey have shown varying responses from each of the provinces. Thus, this should be accounted for in determining adequate landslides information and efficient pathways of information dissemination to the different communities.


IG02-A022
Cost-effectiveness of Wind Mitigation Strategies

Ayat AL ASSI#+, Rubayet Bin MOSTAFIZ, Carol J. FRIEDLAND
Louisiana State University, United States

Severe winds cause billions of dollars in annual losses and significant damage to buildings, resulting in economic losses for homeowners. Mitigation strategies beyond minimum building code requirements are essential to improve home quality and resilience. The FORTIFIED home program has effectively minimized wind risk. This study evaluates the cost effectiveness of FORTIFIED's Roof, Silver, and Gold designation levels for new single-family homes using life-cycle benefit-cost analysis (LCBCA) over 30- and 70-year periods. The study includes wind hazard insurance and flood risk reduction. The LCBCA is conducted with and without including the wind hazard insurance considering the flood risk reduction (i.e., average annual loss) as the absolute benefits. Results provide actionable information to stakeholders and simplify the mitigation decision-making process to reduce wind risk.


IG02-A023
Application of FLOW-3D to Simulate Slump-flow Behavior in the Slump Test of Sediment Slurries

Ming-Wei LIAO#+, Chyan-Deng JAN, Tung-Yang LAI, Yu-Chao HSU
National Cheng Kung University, Taiwan

The slump test is used to measure the slump behavior of the test body, and the result is used to evaluate the test-body flow behaviors. In the slump test, the slump and slump-flow speeds are very fast and difficult to record, resulting in only the final slump and spread being recorded. In addition, it is not easy to maintain the same slump-cone lifting speed in the test. In order to improve the problems, this study uses FLOW-3D to simulate the slump test. It is assumed that the test body is a sediment slurry, being a kind of Bingham fluid, of two rheological parameters, such as yield stress and viscosity in this study. Five different test slurries were used in the slump-test simulation, and the results were compared with those by manual slump tests. The measured parameters of the simulation include slump velocity, slump-flow velocity, final slump, final spread, and final time of slump-flow. The simulated results are close to the manual slump-test measurements, with errors of less than 10%. It shows the FLOW-3D software has good applicability in slump tests. These simulations and manual measurements indicated that the slump parameters of the tested slurries are closely related to their rheological parameters. In addition, simulations show that the slump-cone uplift velocity affects the slump behavior, but the impact has an upper limit. After the uplift velocity exceeds a certain value, the slump behavior does not change significantly. It is concluded that the FLOW-3D can be used to simulate the slump test, and the slump parameters so obtained can be used to estimate the rheological parameters of the test slurries. As the slump-cone lifting speed is set to be higher than a certain threshold value in the simulation, the lifting-speed effect on simulation results can be ignored.


IG02-A024
Interpretation of Riverbed Sediment Grain Size Distribution Using UAV Aerial Images Combined With Basegrain Software

Hsiang-Wei CHEN#+, Tung-Yang LAI, Chyan-Deng JAN
National Cheng Kung University, Taiwan

Knowing sediment grain size distribution in the riverbed helps to estimate the sediment transport and morphology of the river. The traditional grain size investigation method is limited by manpower, and cannot carry out large-scale investigation. This study uses the BASEGRAIN software to interpret the riverbed surface grain size from aerial images, and explores accuracy of the interpretations. Indoor experiment was carried out by laying sediment of known particle size distribution on a platform, taking a vertical-view photo, and then using BASEGRAIN software to interpret the particle size distribution. Field photo taking were conducted in Heshe River and its upper reaches in Nantou County, Taiwan. Ten riverbed photos were taken by unmanned aerial vehicles, and high-resolution orthophotos were constructed, and then the BASEGRAIN software was used to interpret the particle size distribution, and the effects of the selected software parameters on interpretations were also discussed. Comparing the interpretation results by BASEGRAIN with those by the traditional line pebble sampling method, the indoor experiment results show that the differences in the index particle sizes D16, D30, D50, D60 and D84 by the two methods are about 29%, 17%, 3%, 5% and 17%, the closer to the median particle size, the smaller the relative error obtained by the two methods. Interpretation results of the field aerial photos show that the difference in D30, D50 and D84 by the above two methods are about 25%, 21% and 30%, respectively. The results of field-photo interpretation may vary greatly due to factors such as terrain undulations, and material stacking and burial. Application of BASEGRAIN can quickly and massively interpret the particle size of the riverbed surface, but there are still some problems in the accuracy of the interpretations, and how to improve the accuracy needs further research.


IG02-A025
Assessment of Rheological Parameters of Debris Flow Sediment Slurry by Using the Slump Test

Fang-Yu CHANG#+, Chyan-Deng JAN, Tung-Yang LAI, Yu-Chao HSU
National Cheng Kung University, Taiwan

The movement behavior of debris flow is related to its rheological properties, and the rheological properties of debris flow are related to its sediment concentration and particle size composition. To master the rheological characteristics of debris flow, it is necessary to obtain sediment materials from the channel bed debris flow to measure its rheological characteristics and related parameters. In this study, debris-flow sediment samples were taken from the riverbed of Jiaopu Creek that is a debris-flow river in Tainan, and brought them back to the laboratory to analyze the particle size distributions of these samples. The samples so obtained were mixed with clean water to form sediment slurries with different volume concentrations for rheological measurements and slump test to obtain rheological parameters and slump parameters, respectively. We analyze the relationship between the obtained rheological parameters and slump parameters so as to understand their relations, and the relations can be used to estimate debris-flow rheological parameters from its slump parameters. The slump test was carried out with debris-flow sediment slurries of different concentrations, and the slump parameters were measured to estimate its rheological properties, so as to evaluate the feasibility of indirectly estimating the rheological parameters from the on-site debris-flow slump test.


IG02-A032 | Invited
The Potential Landslide-induced Tsunamis of Iya Volcano in Sawu Sea

Sakka SAKKA1#, Muh. Alimuddin HAMZAH1, Amiruddin AMIRUDDIN1, Saaduddin SAADUDDIN2+, Darmawan HERLAN3, Devy Kamil SYAHBANA4, Ainun Mawaddah ABDAL1, Miswar TUMPU1, Yatimantoro TATOK5, Norman Patrick Lucky Bire Riwu KAHO6
1Hasanuddin University, Indonesia, 2Laboratory of Ocean and Coastal Dynamics, Department of Geophysics, Hasanuddin University, Indonesia, 3Gadjah Mada University, Indonesia, 4Center for Volcanology and Geological Hazard Mitigation, Indonesia, 5Indonesian Agency for Meteorology Climatology and Geophysics, Indonesia, 6Nusa Cendana University, Indonesia

A comprehensive study should be conducted to evaluate the exposure and risk related to the potential landslide-induced tsunamis in Sawu Sea which could be triggered by the activities of Iya volcano. This is an active volcano located in the coastal area in the southernmost of Ende, East Nusa Tenggara Province in Indonesia. The current Iya’s edifice shows a potential sector collapse as a consequence of the flank instability. Furthermore, this condition could trigger landslide-induced tsunamis in Sawu Sea. This study will reanalyse the existing rupture surface which is considered as the source of the potential landslide-induced tsunamis for the input parameter of tsunami modelling. A finite element method will be applied to model the tsunami generation to numerically solve Navier-Stokes equation for the approach of incompressible flows in a multi-material simulation. The expected outputs are the physical parameters of tsunami such as: run-out distance, run-up, and arrival time to neighbouring islands, Kupang dan Sumba. Further, this study will be equipped with risk vulnerability analysis as the part of risk mitigation for the authorised institutions and the local government.


IG03-A002
Bayesian Seismic Tomography Based on Particle-based Variational Inference in Velocity-space for Physics-informed Neural Network

Ryoichiro AGATA#+, Kazuya SHIRAISHI, Gou FUJIE
Japan Agency for Marine-Earth Science and Technology, Japan

In this study, we consider Bayesian seismic tomography using physics-informed neural networks (PINN). PINN is a recently proposed framework in deep learning that offers enhanced capabilities of physics-based simulations and inverse analyses. PINN-based deterministic seismic tomography incorporates two moderate-sized neural networks (NNs): one to predict seismic velocity and the other to predict travel time. Widely adopted naive approaches of Bayesian neural network fail to handle the high-dimensional space spanned by the weight parameters of these NNs. To address this problem, we propose a novel approach called velocity-space Stein variational gradient descent for PINN-based seismic tomography (vSVGD-PINN-ST). This approach targets only the network predicting seismic velocity in the Bayesian estimation, while the network predicting travel time is used only for deterministic travel time calculations, with the help of the adjoint method. Furthermore, it performs Bayesian estimation for the velocity network by introducing a function-space Stein variational gradient descent (SVGD), which conducts a type of particle-based variational inference in the space of function predicted by the NN (i.e., seismic velocity), but not in the weight space of the NN. These improvements drastically decrease the complexity of the problem and allows for more accurate and physically consistent Bayesian estimation for PINN-based seismic tomography, confirmed by synthetic tests of one- and two-dimensional tomographic problems. Our new approach allows PINN to be applied to Bayesian seismic tomography practically for the first time. In addition, it can be a powerful tool for general PINN-based Bayesian estimation problems associated with similar sizes and formulations of NNs.


IG03-A003
Shrinkage-induced Crack Pattern Formation Based on Variational Energy Physics-informed Neural Network

Shin-ichi ITO#+
The University of Tokyo, Japan

Cracks on the surface of thinly spread dense colloidal suspensions (desiccation cracks) show complicated patterns, and such patterns are observed in various scientific and industrial scenes. Although the numerical simulations of the crack pattern formation are necessary to understand the underlying physics, obtaining accurate crack formations has still been a computationally challenging task due to the scale gap between the crack width and the whole domain of the pattern. In order to tackle this problem, this study proposes a phase-field modeling of the time evolution of the desiccation cracks based on a variational energy physics-informed neural network (VE-PINN) approach. The proposed VE-PINN model enables the computation of crack dynamics in high resolution since it learns and outputs the crack pattern as a spatiotemporally continuous function. The numerical experiments reveal the proposed model shows the rich pattern formations corresponding to the patterns observed in the real experiments.


IG03-A007
U-Net: A Deep-learning Method for Improving Summer Precipitation Forecasts in China

Qimin DENG#+, Peirong LU
China University of Geosciences, China

A deep-learning method named U-Net was applied to improve the skill in forecasting summer (June–August) precipitation for at a one-month lead during the period 1981–2020 in China. The variables of geopotential height, soil moisture, sea level pressure, sea surface temperature, ocean salinity, and snow were considered as the model input to revise the seasonal prediction of the Climate Forecast System, version 2 (CFSv2). Results showed that on average U-Net reduced the root-mean-square error of the original CFSv2 prediction by 49.7% and 42.7% for the validation and testing set, respectively. The most improved areas were Northwest, Southwest, and Southeast China. The anomaly same sign percentages and temporal and spatial correlation coefficients did not present significant improvement but maintained the comparable performances of CFSv2. Sensitivity experiments showed that soil moisture is the most crucial factor in predicting summer rainfall in China, followed by geopotential height. Due to its advantages in handling small training dataset sizes, U-Net is a promising deep-learning method for seasonal rainfall prediction.


IG03-A008
Assessment of the Effectiveness of a Convolutional Autoencoder for Digital Image-based Automated Core Logging

Jaesung PARK+, Suwan SO, Jina JEONG#
Kyungpook National University, Korea, South

Widely applicable convolutional neural network (CNN)-based lithology classification models are limited to interpret soundness of a trained model and require high computational cost. This study proposes a convolutional autoencoder (CAE)-based classification model to improve the efficiency of rock-core-logging analysis based on digital rock-core images (CAE model I) and suggest a more understandable classification model by extracting the lithological feature information from the network structure of the model. Moreover, input digital-image data transformation using the Canny edge-detection algorithm was implemented (CAE model II). The applicability of the developed models is validated by comparing them with a CNN model and the model proposed by the previous study (RGBE model). While implementing the proposed model, digital images of 85-m-long cores were used, which were acquired from the Satyr 5 well in the Northern Carnarvon Basin, Western Australia. It was found that CAE models I and II showed classification accuracy comparable to the CNN model (CAE model I: 96.4%, CAE model II: 94.9%, CNN model: 97.5%, and RGBE model: 94.4%). The extracted features of the trained CAE models are effective in interpreting the trained network structure. In addition, in terms of computational efficiency and training time, the CAE-based models are significantly better than the CNN model (CAE model I: 7 min 21 s, CAE model II: 7 min 34 s, CNN model: 12 min 6 s, and RGBE model: 24 min 35 s). Overall, the results demonstrate the feasibility of the proposed CAE-based models for automated rock-core logging.


IG03-A016
Method of Assessing the Origin of South Korea Using Deep Learning-based Feature Extraction Technology

Subi LEE+, Jina JEONG#
Kyungpook National University, Korea, South

Isotope data of environmental samples, such as soil, groundwater, or rock, contain information about specific regional environmental characteristics, making it possible to guess the samples' origin. For this reason, isotopic data is widely applied to various research areas, including origin tracking, source tracing of environmental pollution or climate change research, etc. In particular, the ratio of 87Sr, which is naturally abundant in strontium isotope data, varies depending on the type of rocks and geological eras. Therefore, the geographical and geological origin can be inferred by comparing the strontium isotope ratio in the samples with baseline databases of strontium isotope ratios of each region. As a preliminary study to develop a model that can infer the origin of the environmental samples from the isotope data, this study quantitatively characterized geological properties of each geographical and geological origin, including information on rock type, tectonic provinces, major geochemical elements of rocks, and strontium isotopes. Autoencoder (AE), a deep learning technique, was applied to identify the complexity of the relationship between the origin and the various geological information. Before applying the AE, principal component analysis (PCA) was applied to discriminate the primary input data of the AE, influencing the characterization of the geochemical properties of origin. The actual database (soil samples) acquired from South Korea nationwide was applied to validate the proposed method in this study. Based on the low-dimensional features extracted from the AE, a total of eight origins were clustered, which was utilized to produce a map of the isotope content and estimate the origin of unknown environmental samples.


IG03-A017
Reconstruction of Electron Radiation Belts Using Machine Learning and Data Assimilation

Dmitri KONDRASHOV1#+, Alexander DROZDOV1, Yuri SHPRITS2
1University of California, Los Angeles, United States, 2GFZ German Research Centre for Geosciences, Germany

The radiation belts consist of electrons and protons trapped by the Earth’s magnetic and are a major source of damaging space weather effects on near-Earth spacecraft. The inner electron belt is located typically between 1.2 and 2.0 Earth radii, while the outer belt extends from about 3 to ∼8 Earth radii. Relativistic electron fluxes in the outer belt are highly variable; this variability is due to the competing effects of source and loss processes, both of which are forced by solar-wind-driven magnetospheric dynamics and by resonant interactions of plasma waves and particles. Understanding the mechanisms of build-up and decay of radiation belt electron fluxes is one of the fundamental problems of modern space physics. While significant progress has been achieved in understanding the electron radiation belt dynamics using physics-based models, it is still incomplete, due to the very limited number of satellites operating at different orbits in space and providing measurements of radiation belt electron fluxes. Presented approach for a global reconstruction of radiation belt electron fluxes represents the gray box combination (via data assimilation) of physics-based and machine learning (ML) models and considers errors (uncertainties) in both. First, low-Earth-orbiting (LEO) Polar Orbiting Environmental Satellites (POES) measurements are mapped by machine learning (ML) to medium-Earth-orbiting (MEO) Van Allen Probes dataset. The ML-based LEO-to-MEO mapping can be interpreted as creating high-quality Van Allen Probes-like (“virtual”) satellite measurements. To map POES measurements, two ML methods are considered: multivariate linear regression (MLR) and neural network (NN). The ML-mapped flux is then included by data assimilation with the Versatile Electron Radiation Belts (VERB) physics-based model and compared with Van Allen Probes observations as “ground truth”.


IG03-A019
Simple Physically-Based Emulator of the MATSIRO Land Surface Model

Roman OLSON#+, Kei YOSHIMURA, Tomoko NITTA
The University of Tokyo, Japan

Land surface and hydrological models are key tools to analyze and predict hydrological variables such as runoff. However, their major shortcoming is their relatively slow speed. This often precludes these models from being used for a host of tasks such as uncertainty quantification, sensitivity analysis, and so on. For these purposes, one requires a simple model approximating the original model’s behavior – a so-called “emulator”. Emulators of hydrologic models are a topic of active research. However, so far, to our best knowledge realistic global model emulators have only been constructed on a monthly scale, which considerably reduces their usefulness for many applications. Here we develop a simple and fast emulator of MATSIRO land surface model on a daily scale. The emulator takes as input five atmospheric variables (surface air temperature, precipitation, surface atmospheric pressure, snowfall, and surface specific humidity). The output of the emulator includes snow water equivalent, upper layer soil moisture, wetland water storage and runoff. Notably, in contrast to deep learning methods, emulator parameters and state are physically interpretable, which offers insights into soil moisture and runoff dynamics. We achieve improvements in speed via code written in modern Fortran with parallel programming using coarrays. The emulator operates at spatial scales ranging from a single grid point to regional to global. Emulator parameters are month and location-dependent. We optimize the parameters by minimizing simulation error at each grid point. We benchmark emulator performance and compare it with the original MATSIRO model, evaluate the emulator using a range of metrics, perform cross-validation, and discuss the emulator’s applicability under conditions of global climate change. We discuss data structures that help to speed up the emulator. Finally, we outline plans for coupling the emulator with other climate and social system component models (e.g., CaMa-Flood river hydrodynamics model), and enumerate future application areas.


IG03-A025
Quantitative Petrographical Criteria for the Exploration of Chromitites as Methanation Catalysts. A Data Analysis Example from Greek Peridotites

Haezan JANGARUN1, Elena IFANDI1#+, Stavros KALAITZIDIS2, Basilios TSIKOURAS1
1Universiti Brunei Darussalam, Brunei Darussalam, 2University of Patras, Greece

Carbon capture and catalytic conversion to methane have been proposed as a carbon-neutral energy production method. Recent studies show that platinum group minerals within chromitites catalyse Sabatier reactions and produce abiotic methane. Hence chromitites could be used as natural methanation catalysts for the production of syngas. In this respect, it is important to characterise the mineralogical aspects of rocks with different levels of methane to identify the optimum exploration targets for catalyst-bearing chromitites. Spinel is the host and/or the support of the natural catalyst(s) in chromitites. Statistical analyses of point counting data show that higher abundances of methane are found in chromitites with moderate (250-500 um) to large (500-1500 um) spinel crystal sizes whereas the methane-poor rocks include spinel with small crystal sizes (<250 um). Veining is important for the circulation of hydrothermal fluids. The rich-in-methane chromitites have the highest abundance of veins (approximately 10% higher than the rocks with moderate methane levels). In the rich-in- methane rocks, about 20% of the veins are classified as small (<100 um) and about 15% as moderate size (100-500 um). The methane-poor chromitites have limited veins (less than 10%). Overall, massive chromitites with adequate veining and moderate to large spinel size seem to host the highest abundance of methane. These petrographical characteristics probably enhance the effectiveness of the fluid-rock interaction in catalysis. Petrographical analyses are quick, low-cost and have low environmental impact for the characterisation of chromitites with catalytic potential for industrial scale.


IG03-A028
Spatiotemporal Dynamics and Forecasting of Ecological Security Pattern under the Consideration of Species Habitat: A Case Study of the Poyang Lake Ecoregion

Daohong GONG1#+, Min HUANG2, Hui LIN3, Changjiang XIAO4
1jiangxi normal university, China, 2Jiangxi Normal University, China, 3Jiangxi Normal University, China, China, 4Tongji University, China, China

With human activities' continuous expansion and development, many species' habitats face serious destruction and threats, and ecological security issues are becoming increasingly prominent. Therefore, constructing an ecological security pattern considering species' habitats is crucial for protecting biodiversity and maintaining ecological balance. As a paradise for wildlife, Poyang Lake is the habitat and breeding ground for many birds, fish, and other aquatic organisms. In this study, we selected the ecological circle around the Poyang Lake Ecoregion (PYLE) as an example. We produced Land Use and Land Cover (LULC) maps of the PYLE in 2000 and 2020 using the random forest classification method. Additionally, the Cellular Automata (CA)-Markov model was used to forecast the LULC in 2040. By combining morphological spatial pattern analysis (MSPA) analysis, landscape pattern index, landscape connectivity index, and Linkage Mapper with long-term LULC data, we constructed a long-term ecological security pattern in the PYLE. The dynamics of ecological security patterns over long-time series were compared and analyzed. Based on PYLE's predicted ecological security pattern in 2040, we propose an optimized ecological security pattern scheme of "one area, two zones, and multiple points". This study provides valuable insights for the sustainable development of the PYLE and the protection of species' habitats.


IG06-A001
Problems to Get Reliable Ionosphere Parameters Te and Ne with Small Satellite

Koichiro OYAMA1,2#+
1International Center for Space and Planetary Science, Japan, 2Asia Space Environment Research Consortium, Japan

Contamination of the electrode in Langmuir probe to measure electron temperature, Te and electron density, Ne, produces inaccurate data. This problem has not been paid attention to large satellite mission so far. At the stage when we are entering small/cube satellite mission, this problem is further worse, because the contamination of the satellite frame which act as the reference electrode also exists. We repeat here the serious problem of Langmuir probe measurement, in order to get reliable and accurate data. We need to make the maximum effort to save money, time and energy.


IG06-A009
Application Potentialities of Nanosatellite in Earthquake-prediction in Complex Solar Geomagnetic Environments by Adopting Ionospheric Equatorial Anomaly as the Precursive Feature

Minakshi DEVI#+
Gauhati University, India

Earthquakes are serious hazards in global scenarios, thus a need arises for a reliable prediction of such events, even though there are largescale efforts in this direction. The paper deals here with this aim by taking two basic issues (i) What are the Earthquakes (EQ) sources? and (ii) How effective is the role of Equatorial Ionospheric Anomaly (EIA) in identifying EQ precursors at wide and complex solar-geomagnetic ambiances? The data for the study consists of global EQ events with magnitude M>4.5 and TEC data from Global profiles covering high and low solar years of cycles 23/24 over the west Pacific and South Asia zones. An extensive analysis of the growth of the EQ and TEC with solar geomagnetic activity shows that EIA strength calculated from global TEC profiles reflects complex modulation before an impending EQ dictated by the solar geomagnetic environment., when its strength reaches a high, not at its maximum but 70 % to 60% below the RZ peak, and the same is true for geomagnetic status. Thus, intense solar background inhibits the growth of EIA, an important feature for EQ prediction and modeling. Further, the paper focuses on the adaptation of the growth of anomalous EIA at the night sector of the epicenter longitude as the precursors of an impending EQ by analyzing a few massive EQ events of M>7.0. Explanations for such growth of anomaly and its inhibition are provided through the EQ-induced E field and the Forbush effect. However, for reliable prediction and modeling, the simultaneous monitoring of magnitude. & direction of the E field, upper ionosphere density, and temperature at different heights under a qualified solar geomagnetic background are essential. Here nanosatellites with multisensor probes are the most effective solution, especially over the longitude zone covering the ring of fire location where our interest lies.


IG06-A012
Orbit Analysis of Very Low Earth Orbit (VLEO) Satellites

Sui CHEN1#+, Erick LANSARD2
1Politecnico di Milano, Italy, 2Nanyang Technological University (NTU), Singapore

The Very Low Earth Orbit (VLEO) (at altitudes below 450 km) offers an alternative solution to ease the congestion in LEO. Being closer to the Earth, satellites operating in VLEO also benefit from higher image resolution and lower communication link-budgets. However, they also experience a significantly larger atmospheric drag that will quickly lead to orbital decay, due to much denser atmosphere present in VLEO. Another challenge associated with operating in VLEO is the large modelling error of atmospheric density. This project focuses on predicting the orbit of a future VLEO satellite and subsequently proposing thrusting strategies for orbit maintenance. It is hoped that the results will provide insightful guidance for mission designers with an enhanced understanding of VLEO as an operational region for satellites. A 100kg satellite operating in VLEO with a dual-thruster electric propulsion system is considered. The impact of solar activity on atmospheric drag is investigated by modelling the F10.7 solar index based on observation data of the past 4 solar cycles. The upcoming solar activity cycle, depending on the sources, is expected to be similar or much stronger than the previous one, with a peak of 220 sfu occurring in December 2024. Using MATLAB, the satellite’s orbit subject to atmospheric drag is propagated. Without any orbit-raising manoeuvre, the satellite is predicted to re-enter the atmosphere after 1190 days. After predicting the satellite’s orbit under passive fall, a trade-off study is conducted to analyse different thrusting strategies by varying altitude, thrusting frequency, thrusting duration, delta-V and thrust magnitude. Finally, comparison between electric propulsion and the traditional chemical propulsion is drawn by computing their delta-V ratio. This project demonstrates the potential and feasibility of operating satellites in VLEO using electric propulsion. The results serve as a steppingstone towards enabling more VLEO satellite missions to be advanced in the future.


IG06-A013
Gemini Mission: An Education and Industry-academy Cooperation CubeSat Mission

Alfred CHEN#+, Jia-Ting LIN, Chia wen CHUANG
National Cheng Kung University, Taiwan

The Gemini mission led by the National Cheng Kung University was kicked off in 2022 to fabricate two 3U CubeSats for scientific experiments of GNSS receiver and UHV/VHF transponder, technology verification, and the proof of the space system engineering of a Taiwan space startup company. These two CubeSats are scheduled to place into a sun-synchronized orbit by an innovative hybrid rocket in 2024 Q2 or Q3. In this mission, two postdoctoral researchers, more than twenty undergraduate students, and an engineering team from the Taiwan space industry work together to build these CubeSats step by step. In addition to space system engineering, several Taiwan domestic industries also joined the development of the CubeSats and contributed their products for validation. This presentation introduces the development and strategy of this industry-academy cooperation mission, and its impact and outcome will also be discussed.


IG06-A018
Development of the Magnetometer EQM Model for the CAS-500

Seunguk LEE1#+, Kwangsun RYU2, Dooyoung CHOI1, Chang-Ho WOO2, Jinkyu KIM2, Wonho CHA2, Dongkook KIM2, Bon-ju KOO2, Seong-og PARK2, Cheongrim CHOI1, Dae-Young LEE1
1Chungbuk National University, Korea, South, 2Korea Advanced Institute of Science and Technology, Korea, South

The Ionospheric Anomaly Monitoring by Magnetometer And Plasma-probe (IAMMAP) is a space science payload package on the Compact Advanced Satellite 500-3 (CAS-500) planned for launch by the Korean Space Launch Vehicle (KSLV-III) in 2025. IAMMAP aims to understand the correlation between equatorial electro-jet (EEJ) and equatorial ionization anomaly (EIA), which plays a very important role in the plasma dynamics of the equatorial ionosphere. To measure the EIA, the instrument is equipped with a plasma probe, Impedance probe (IP) and Langmuir probe (LP), and to measure the magnetic field perturbation caused by the EEJ current, a fluxgate-type magnetometer, Adaptive In-phase MAGnetometer (AIMAG). The main feature of AIMAG is an in-phase circuit that keeps the phase of the output signal constant even when the temperature changes to solve the temperature dependence problem of fluxgate-type magnetometers. The EEJ is a variable flow of strong currents about 100 kilometers above the equator. Since the CAS-500 target orbit is a solar synchronous orbit of about 500 kilometers, the magnetic field perturbations generated at 100 kilometers above the Earth's surface are measured at 500 kilometers above the equator. The perturbed magnetic field of the measured EEJ is expected to be about tens of nT. AIMAG is operated with a sensitivity of several hundred pT to measure the EEJ. To exclude magnetic field contamination from the satellite, three AIMAGs will be installed on CAS-500: two on each end of the solar panels and one on the main body.


IG08-A001
The Approach of the Kinematics Modeling for Slip Surface Estimation, Characteristics, and Types of Landslide Using the Geodetic Method

Vera SADARVIANA#+, Hasanuddin Z. ABIDIN, Djoko SANTOSO, Joenil KAHAR
Bandung Institute of Technology, Indonesia

On the landslide anatomy, the slip surface separates the stable and unstable material on the slope. In the limit equilibrium method, the slip surface is used as a reference for calculating the safety factor. Landslide observation using GPS satellite technology is useful for monitoring the material slope displacement and eventually, disaster mitigation. This study's results are expected to contribute to the characteristics, types, and slip surface estimation in the Ciloto landslide zone using the kinematic model approach. Estimation of the slip surface is carried out in the first, dividing the slope into several parts based on the similarity of the horizontal displacement directions of the monitoring points. The similarity of the horizontal displacement directions indicates that the monitoring points are on the same slip surface. Second, the function of the maximum-minimum geodetic method for the velocity trend lines and polynomial approximation for the vertical profile. The intersection of the velocity trend lines shows the position of the slip surface when the material slides. The ideal planar slip surface is determined by infinite slope analysis and the circular slip surface is determined by circular arc analysis. The intersection of the two observed point velocity trend lines provides an estimate of the location of the slip surface. A geodetic approach can provide an estimate of the scarp's position as well. It was on a vertical profile to ensure conformity with the results of geological studies at the same study site. The Ciloto landslide zone has a very slow speed (5 x 10-5 - 5 x 10-7 mm/sec). The nature of horizontal displacement has a variety of directions. This characteristic indicates that the landslide zone has many slip planes. From this study. The landslide type is multiple compounds (rotational and translational) debris avalanches.


IG08-A002
Development and Testing of Small Array Corner Reflectors and Synthetic Aperture Radar for Slope Monitoring

Chih-Chung CHUNG#+, Chun-Cheng LIN
National Central University, Taiwan

This study aims to enhance the protection of lives and properties in hillside areas by proposing the implementation of a more advanced monitoring system using Synthetic Aperture Radar (SAR) and a small corner reflector (CR). The CR design is focused on being compact, lightweight, portable, and effortless to install, to provide more dependable SAR reflection points for landslide detection. Theoretically, altering the length of the sides of the CR can modify the maximum radar cross-section scattering (RCS) and reflection angle. To further simplify installation and reduce weight, a smaller and more manageable installation is proposed. Despite the smaller size of the reflector, the RCS may not be sufficient, hence the CR array setup is expected to enhance the reflection strength. The feasibility of this concept was verified through simulations using a multiphysics finite element modeling software and field testing with ground-based SAR, which showed that adding a small CR array increases the signal strength for a specific angle. Further field tests will be conducted to advance the practical implementation of this research.


IG08-A003
Landslide Mapping Using Google Earth Engine: A Case Study in Taiwan

Tee-Ann TEO#+, Tsung-Han WEN
National Yang Ming Chiao Tung University, Taiwan

Google Earth Engine (GEE) platform offers an easy-to-use interface for accessing open data, as well as the ability to develop custom applications using online cloud computing resources. Earth observation satellite images can be utilized for landslide mapping by comparing their spectral features between two different time periods. The stacking of multi-temporal satellite image creates a time-series satellite image which contain valuable information about the ground surface conditions. Due to the availability of time-series satellite images processing capabilities in GEE, this study aims to perform landslide mapping using deep learning techniques and time-series satellite images from GEE. In this study, we employ a Long Short-Term Memory (LSTM) neural network to classify regions as either landslide or non-landslide, using 30m time-series Landsat-8 images. The focus of this landslide detection is on regions, rather than individual pixels. A multiscale image segmentation approach is applied to identify regions with similar spectral characteristics. Each region is then analyzed for its time-series spectral information, which is used for landslide detection. The LSTM model is trained by manually digitized landslide labels and segmented regions. The accuracy of the model is evaluated by precision and recall, using an individual check area. The training area is located in the mountainous central region of Taiwan and covers an area of 2600km2. The individual check area is located in the southern part of Taiwan and approximately 1800km2. The time-series image was created using Landsat-8 images from the years 2015 to 2018. The proposed LSTM model uses time-series spectral information to identify landslide regions. The preliminary experimental results show that, the precision and recall for landslide areas were 51% and 72%, respectively. In conclusion, GEE provides a convenient platform for constructing time-series satellite images, and the proposed landslide detection achieved a 70% accuracy using 30m satellite images.


IG08-A010
In Situ Monitoring and Analysis of Slope Stability in the Baoshan Village of Kaohsiung

Huai-Houh HSU#+, Yen-Chi HUANG, Chen-Hsun HSIEH
National Kaohsiung University of Science and Technology, Taiwan

Baoshan village is located in Taoyuan District, Kaohsiung City. The geology here is mainly the Lushan formation, composed of weathering and broken slate. According to the geological survey data, it has been observed that there are many disaster potentials in this area. This paper analyzes the possibility of sliding here using in situ surveys and monitoring. In terms of field investigation, it was observed that there were noticeable cracks in many structures and retaining walls in Baoshan Elementary School. In the Baoshan village, multiple floor bulges, broken walls, and floors were found. According to the in situ survey results, this study set up three inclinometer casings with depths of 22m, 40m, and 50m, respectively, and seven tiltmeters at this campus. The monitoring frequency is about once a month, and the monitoring data, groundwater table, and rainfall are collected and analyzed. The long-term monitoring was carried out from 2018 to 2022, and it was observed that the slope mainly slowly moved toward the northwest direction. The relative movement of layers deformed the inclinometer casing on the north side of the campus. This displacement was observed at a depth of 46m below the ground surface. While Comparing the data of rainfall and groundwater table, it is speculated that the typhoon brought concentrated heavy rainfall to cause the groundwater table to rise and trigger the slope of a slide.


IG08-A011
Deriving Rainfall-landslide Thresholds for Tectonically and Geomorphologically Heterogeneous Regions: The Philippine Example

Beth Zaida UGAT1#+, Decibel FAUSTINO-ESLAVA1, Jefferson RAPISURA1, Bianca Maria Laureanna PEDREZUELA1,1, Maria Regina REGALADO1, Gabriel Angelo MAMARIL1, Jenielyn PADRONES1, Rosemarie Laila AREGLADO1, Loucel CUI1, Juan Miguel GUOTANA1, Cristino Jr. TIBURAN2, Jayson ARIZAPA1
1University of the Philippines Los Baños, Philippines, 2University of the Philippines, Philippines

Landslide disasters in the Philippines are often caused by the geographical location of the country exposing the land to extreme weather events frequently damaging properties and causing losses of lives. In an area vulnerable to such, intensive research and study that requires extensive data are beneficial. The national government has identified the need to mitigate landslide disasters through initiatives such as Project LIGTAS or “Landslide Investigations on Geohazards for Timely Advisories in the Philippines”. Project LIGTAS focuses on the generation of a non-structural preventive approach to mitigate landslides using rainfall-landslide thresholds. Furthermore, landslide events and rainfall data mining and population are being done by Project LIGTAS. This study aims to present the generated thresholds for the provinces of Benguet and those in the Southern Tagalog region. This paper discusses the encountered challenges in data acquisition and the solutions employed by the team. Lastly, potentials to operationalize a localized landslide early warning system within the study areas are also presented. Various methods and platforms were utilized for data acquisition such as from partner national government agencies. With the current data, huge differences have been derived for different geological areas. Approximately 27 mm of rainfall already triggers slope failures in the CALABARZON region, while selected areas in the Bicol region trigger landslides at around 90 mm of rainfall. Lower thresholds were generated for the Benguet province where slope failures start at lows of 12mm of rainfall. Continuous data collection and correlation can further improve threshold values and be used in the formulation of localized early warning systems protocol for the study areas. The results of this work are used in the landslide warning system posted on the LIGTAS website (www.ligtas.uplb.edu.ph). Additionally, the simplicity of the method provides a higher chance of adaptation by other regions in the country.


IG08-A012
Rainfall-Pore Pressure Response of a Dip Slope: Insights from a Tank Model Based on 3-D Geological Model

Alvian R. YANUARDIAN#+, Jia-Jyun DONG
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 condition of a 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. In order to identify the orientation and distribution of the lithology in the research area, we used the average of 3 types of orientations; 1) a planar-like feature on the east slope of the research area, 2) the orientation of key-bed from 3 boreholes that show distinct sedimentary structure called wavy laminations, 3) orientation of shale layers from 2 boreholes and an outcrop. Afterward, 14 boreholes were adjusted based on the average bedding plane orientation in order to identify the rock units and boundaries. Subsequently, applying linear regression to construct a 3-D geological model and also clarifying it using a cross-section. The result shows that the 3 types of orientation show similarities in orientation indicating the lithologies are spatially distributed well in the research area. We also defined 6 rock units and colluvium-infilling material, with 6 boundaries. On the other hand, calibrating the tank model's parameters based on a hydraulic test is used to get the best fit simulated groundwater level’s result. Therefore, re-calibrating is proposed to make sure the tank model’s parameters based on the hydraulic test fit well for the rainfall cases. The slow responses of pore pressure induced by rainfall which is represented by the good fitness of the tank model’s simulation, indicate that geological conditions, including joint sets, are responsible for it. Moreover, the parameters of the tank model’s simulation can be used to predict future pore pressure responses induced by rainfall which can trigger landslides.


IG09-A002
Cascading Impacts of Tsunamis and Coastal Vulnerability in the Indian Ocean

Anawat SUPPASRI1#+, Ryuto MIZUSHIMA1, Constance Ting CHUA1, Elisa LAHCENE1, Miwako KITAMURA1, Pescaroli GIANLUCA2, David ALEXANDER2, Fumihiko IMAMURA1
1Tohoku University, Japan, 2University College London, United Kingdom

The 2004 Indian Ocean tsunami left its fingerprints on coastal communities across the Indian Ocean basin, demonstrating the far-reaching potential of a single tsunami event. A tsunami does not only impact the population but can also have cascading impacts on the critical infrastructure which the population depends upon. For instance, tsunami damage to port facilities as well as power generation plants does not only affect the local population, but it can also impact on regional and global supply chain. The objective of this study is to provide a preliminary vulnerability assessment of coastal communities against tsunami hazards and their cascading impacts in the Indian Ocean. Vulnerability of coastal communities will be considered from the perspectives of population size, age and gender. For this purpose, we collect some data that can be used to identify tsunami vulnerability such as high-resolution world population data (including age, gender and migration status) and locations of ports and power generation plants. Though tsunami hazard assessments have been performed at macro scales for the region, there has been limited focus on tsunami hazards under the influence of a changing climate. Therefore, we also consider the effects of rising sea levels in the event of tsunamis.


IG09-A006
Extreme Nearshore Surface Currents in Singapore

Jun Yu PUAH1#+, David LALLEMANT1, Ivan HAIGH2, Dongju PENG1, Kyle MORGAN1, Adam SWITZER1
1Nanyang Technological University, Singapore, 2University of Southampton, United Kingdom

Despite the importance of extreme currents in key applications such as ship navigation, sediment transport and coral growth, research remains scarce due to the lack of long-term observational records. In this study, we model the profile of extreme shallow-water currents off Pulau Hantu and Kusu Island, both located along the Singapore Strait, and investigate their potential drivers. We decomposed about 12 months of observed currents into their tidal and residual components by applying harmonic analysis. The tail distribution of the residual component was estimated using extreme value analysis by fitting a non-homogeneous Poisson process to the data, accounting for temporal and directional dependences. Random simulations of tidal currents were then combined with residual currents via the Joint Probability Method to generate new observed current realizations. Finally, we extracted wind speeds from ERA5 Reanalysis to investigate how well monsoonal winds correlate with residual currents across monsoon periods. Tidal variance ranges from 29-69% across all sites, which is lower than expected given the dominance of tidal currents in the Singapore Strait. Extreme currents orient primarily along the coastline contours. Mean speed in Pulau Hantu is greater than Kusu Island and may be attributed to the hydrodynamic pressure gradient set up by the monsoons. Lastly, the stronger correlation observed in some sites during the inter-monsoon periods suggests that localized wind systems such as the Sumatra squalls are critical in driving extreme currents. The variability of the study results highlights the challenges in modelling currents in the Singapore Strait given its complex bathymetry, equatorial weather patterns and complex tidal regime. Future work could include the integration of shipborne Automated Information Systems to derive extreme surface currents in Singapore and the Sunda Shelf region.


IG09-A009
A Stochastic Model of Potential Tsunami Impacts Originating from the Southern Part of the Manila Trench

Elaine HZ TAN1#+, Linlin LI2, Qiang QIU3, Constance Ting CHUA4, Masashi WATANABE1, Adam SWITZER1
1Nanyang Technological University, Singapore, 2Sun Yat-sen University, China, 3South China Sea Institute of Oceanology, Chinese Academy of Sciences, China, 4Tohoku University, Japan

Tsunami can impact both near and far field locations, as illustrated by the 2004 Indian Ocean, 2018 Palu and the 2011 Tohoku-Oki events. In Southeast Asia, the tsunami hazard is often tied to the subduction zone systems in Indonesia. The Manila Trench in the South China Sea is also likely able to generate damaging tsunamis however available studies have predominantly concentrated on the northern sectors of the fault and examined the potential tsunami impact on Luzon, Philippines, Vietnam, Hong Kong, Macau and China. Little is known about the tsunami risk posed by the southern segments of the fault. Our study seeks to fill this gap by conducting tsunami hazard assessment for this region. We model heterogeneous slip distributions from the southern segment of Manila Trench (13-16°N) for earthquake events, with magnitudes ranging from Mw 7.4 to 8.4, and their wave propagations. Using the obtained peak nearshore tsunami amplitude, we developed hazard curves for fifty-two (52) study sites. The study sites were selected based on population density and economic importance. Our preliminary analysis indicates that areas in close proximity like the Philippines are at most at risk with localised tsunami heights of up to 5.4m followed by areas in southern Vietnam where localise tsunami height can be up to 4.3m. In contrast, Singapore, Malaysia, Indonesia, Thailand and Cambodia are likely to be less affected and modelled tsunami heights do not exceed 1 m. As our preliminary study does not consider wave run-up or tsunami currents, this hazard is likely to be an underestimate at this current point.


IG09-A011
Numerical Simulation of Storm Wave Propagation Over Structural Complexity of Coral Reefs at Komaka Island, Japan

Masashi WATANABE1#+, Hironobu KAN2, Ken TOGUCHI3, Yosuke NAKASHIMA4, Volker ROEBER5, Taro ARIKAWA6
1Nanyang Technological University, Singapore, 2Kyushu University, Japan, 3University of the Ryukyus, Japan, 4Ariake College, Japan, 5University of Pau and Pays de l'Adour , France, 6Chuo University, Japan

Propagation of storm waves across coral reef is affected by geomorphology over reef slope. Complex structures of several meters over reef slopes, such as spur and groove formations, are also believed to affect current or wave propagation. A spur is topography whose elevation is partially high over the reef slope to the reef edge and a groove is a depression between the spurs. In particular, the direction and energy of wave are controlled by the structural complexity. However, measurements of water depth data in shallow water regions, such as reef slopes over coral reefs, have recently become possible using multibeam echosounders installed in small vessels. Therefore, to date, measured water depth data, including several-meter-sized complex structures, have not been used for numerical simulations. The objective of our research is to investigate the effect of several-meter-sized complex structures on coastal wave run-up and propagation based on numerical simulation using real topographic data. To reveal the role of the structural complexity of coral reefs, we conducted numerical simulation of storm wave at coral reefs of Komaka Island. We first conducted a multibeam survey to reveal the topography of the reef on Komaka Island. The high-resolution bathymetry of 1 m grid size was observed by multibeam echo sounding (MBES) survey was used for the simulation. We then conducted a three-dimensional simulation using the measured topography with a supercomputer, and this simulation results can explain observed significant wave height during strong waves from typhoons at Komaka Island. After that, we conducted two-dimensional simulation of storm waves and estimated wave friction factor which can explain simulation result of the three-dimensional simulation. After the setting of wave friction factor, we investigated effect of the structural complexity against storm wave propagation from our simulation results.


IG09-A015
The Development of Deep Learning-based Tsunami Forecasting for Early Warning System in Java Island, Indonesia

Muhammad Rizki PURNAMA#+, Anawat SUPPASRI, Kwanchai PAKOKSUNG, 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 notable area span from Java to Nusa Tenggara, such as Pelabuhan Ratu, Pangandaran, Yogyakarta, Bali Island, Mandalika, and Nusa Tenggara. Therefore, Indonesia needs a decent Tsunami Early Warning System. There are only six existing cable-based tsunameters (CBT), which use bottom pressure gauges to inspect tsunami wave propagation in Indonesia's deep-sea area to issue an early warning. In this paper, we assessed the optimal deployment of tsunami buoys along The Southern part of Java Island to Nusa Tenggara and make an optimization scheme using a Deep Learning-based model. First, we create a set of synthetic tsunami scenarios using a stochastic-slip earthquake model with Mw 8.0-9.2 for the Java Megathrust fault to generate multiple tsunami-earthquake scenarios. Next, we apply the empirical orthogonal functions (EOF) based on the tsunami scenarios to determine the initial location for the deployment of each tsunameter. Finally, we apply an optimization scheme to forecast maximum tsunami height and arrival time in the coastal area using Convolutional Neural Network (CNN). Tsunami wave height at each initialized tsunameters are defined as an input in our model. Then, we do the sensitivity analysis to find the optimal placement by reducing the number of the tsunameters while evaluating its MSE. Thus, this scheme will lead to the improvement of the tsunami early warning system in Indonesia.


IG09-A021
Engineering Properties Measurement from Free-fall Penetrometer in Sandy Soils: A Preliminary Study in Theoretical Approach

Chun-Hung LIN#+, Wei-Jong TIEN, Po-Yin LIN
National Sun Yat-sen University, Taiwan

Free-fall penetrometer is an efficient tool to investigate the offshore shallow sub-seabed, especially in the transition zone and shallow water. It can provide the engineering properties of the sub-seabed. However, currently, most of the applications are based on empirical formulas. The aim of the study is to establish a theoretical-based algorithm to measure the engineering properties of the free-fall penetrometer. A 1-D theoretical-based algorithm for homogeneous and isotropic soils was established to study the behavior of change of velocity of free-fall penetrometer after penetrating into sandy sub-seabed. A linear inversion skill was applied to invert the engineering properties of the sandy soils. The results show that the algorithm can better describe the penetrating behavior with reasonable engineering properties. A further experimental study should be conducted to verify the measured engineering properties.


IG10-A001
Technique Development for Intersection Between Fracture System and Objects by Means of Hybrid Domain Model

Chuen-Fa NI1, Yun-Chen YU2,1, I-Hsien LEE1#+
1National Central University, Taiwan, 2Atomic Energy Council, Taiwan

Detecting precise start location of containment is crucial for numerical modeling of groundwater flow and transport, especially for some of the containments are stored inside the containers. Due to the low water-conducted feature of rock matrix, the fractured rocks are one of the potential host rocks for containment disposal. However, the fracture system of fractured rocks plays an important role on groundwater flow and transport, and the hydraulic characteristic of rock matrix is critical as well. In this study, we present a hybrid domain (HD) model, which can consider fracture system and rock matrix simultaneously, to simulate groundwater flow and transport in fractured rock. A series of objects are also embedded in a complex conceptual fractured rock for developing the technique of intersection between fracture system and objects. The interactions between fracture system and objects is detected, and the additional nodes are generated on the intersections for the following flow and transport purpose. The system of equation for flow field of the complex conceptual fractured domain is solved by means of the mesh generation algorithm, which employs two-dimensional (2D) triangle for fracture system and surfaces of objects and three-dimensional (3D) tetrahedron for rock matrix and interior of objects. Results show that the detection technique is successfully developed, so does the mesh generation algorithm for the complex conceptual fractured domain. Results also show the detail flow field and the accurate flow velocity on the intersection between fracture system and objects are simulated. These results are critical information for containment transport modeling in the fractured rocks.


IG11-A001
A Data Management Plan Starting with Climate Change Data Services

Tzu-Ming LIU#, Shih-Yao LIN+, You-Syuan CHEN, Yung-Ming CHEN
National Science and Technology Center for Disaster Reduction, Taiwan

Taiwan Climate Change Projection Information and Adaptation Knowledge Platform (TCCIP), with the support of the National Council of Science and Technology, has been providing climate change-related scientific data, information, knowledge and tools that Taiwan needs to promote climate change research and adaptation programs since 2012. In order to ensure the data quality of climate change big data and expand the scientific application services of research data, we have tried to draw up the TCCIP Data Management Plan (DMP) with reference to international experience and with the FAIR principle as the vision since 2019. The original intention of DMP is to effectively plan and implement data management, which includes the life cycle of data, from "planning", "production", "checking", "storage", to "publishing", respectively. Behind the climate change data services provided by TCCIP, the DMP is the core of climate change integration services, which includes external data service policies and internal data management regulations. This study will use the experience of TCCIP to illustrate the content of the DMP behind the climate change integration service platform, how to implement it into external data services, and provide reference for climate services.


IG11-A002
Open Data Produced by “Minna De Honkoku”

Yasuyuki KANO1,2#+, Yuta HASHIMOTO3
1The University of Tokyo, Japan, 2The University of Tokyo, Japan, 3National Museum of Japanese History, Japan

“Minna de Honkoku” (https://honkoku.org/) is crowdsourced and online collaborative project to transcribe historical materials written in old Japanese. "Minna de Honkoku" was launched as an online citizen science project to transcribe earthquake-related historical materials from Earthquake Research Institute Library, the University of Tokyo. On July 2019, the system of Minna de Honkoku was upgraded to support IIIF, International Image Interoperability Framework. Broader range of manuscripts on digital archives adopting IIIF can be registered for transcription. The subjects of the project was extended to cover wide variety of historical materials as well as earthquake-related materials. AI-assisted transcription was also implemented. More than 3,500 documents are registered on the system. Total number of characters transcribed is about 28 million. The transcribed text data is shared using Creative Commons licenses (CC BY-SA). The data is used for, for example, editing bibliographic information at libraries, museums and so on. The text is also used for publishing e-books that translates classical literature. An experiment of OCR text conversion of digitized materials of the National Diet Library, Japan (NDL) Lab utilized the transcribed text of Minna de Honkoku. The OCR Training dataset is also published by NDL Lab.


IG11-A003
NASA’s Science Discovery Engine: Enabling Interdisciplinary Open Science

Kaylin BUGBEE1#+, Ashish ACHARYA 2, Emily FOSHEE2, Kumar RAMASUBRAMANIAN2, Carson DAVIS2, Xiang LI2, Rahul RAMACHANDRAN1, Shawn FOLEY3
1NASA Marshall Space Flight Center, United States, 2University of Alabama in Huntsville, United States, 3All Points, United States

NASA is committed to fostering an inclusive open science community, defining open science as collaborative, technology-enabled sharing of data, information, and knowledge to accelerate scientific research and understanding. NASA champions the Open-Source Science Initiative (OSSI) to support this. OSSI's cyberinfrastructure includes the Science Discovery Engine (SDE), which enables the discovery of data, software, and documentation across NASA’s five science disciplines. The SDE increases potential data reuse and fosters interdisciplinary science by making data and information more discoverable to a larger audience. The beta SDE version was released in December 2022 and includes over 84,000 datasets, 700,000 documents, and 9,000 science terms. The SDE development was collaborative and guided by subject matter experts. In this presentation, NASA shares lessons learned while developing the SDE and seeks community feedback on the SDE's information and features.


IG12-A002
Attempt to Estimate Long-term Vertical Land Surface Movement Using Archaeological Information in Actively Subsiding Sedimentary Basin, Niigata, Japan

Yuka ITO1#+, Seiichi SHIMADA2, Tomochika TOKUNAGA1
1The University of Tokyo, Japan, 2Nippo Co., Ltd., Japan

The Niigata Plain, central Japan, is an actively subsiding sedimentary basin with its tectonic subsidence rate to be ca. 3-4mm/yr at its coastal area. In addition, anthropogenic activities such as groundwater abstraction may accelerate compaction, which results in the formation of accommodation space for sedimentation.
Archaeological surveys have been investigated in this plain, and the elevation of paleo-ground surfaces have been determined from buried sediments and in the paleo lake bottom sediments. Depths of archaeological sites excavated in the Niigata Plain are much deeper than those in other plains in Japan. Therefore, previous studies have indicated the possibility that local ground deformation (e.g., earthquakes) may have caused the burial of archaeological sites or the expansion of lagoons.
In this study, we attempt to understand the long-term land surface movement of this plain by extracting buried heights from many archaeological survey reports and by mapping the extracted data spatially. Paleo-surface during ca. 1000 years ago to the present tends to be deeper towards the western side of the plain while shallower towards the eastern side. This characteristic spatial pattern indicates that the western part of the plain may have subsided faster relative to the eastern part. Because the stratigraphic analysis suggested that the sites were not affected by flood events that dramatically buried the remains nor by sea-level changes of recent 1000 years period, the spatial pattern of land surface movement extracted from the archeological reports is likely reflecting the long-term subsidence of the plain.


IG12-A003
On the Observation of Signal Behavior from Magnetotelluric Survey in the Urban Area of Taiwan

Haiyina Hasbia AMANIA1+, Ping-Yu CHANG1#, Ding-Jiun LIN1, Jordi Mahardika PUNTU1, Yin-Long CHEN1, Lingerew Nebere KASSIE1, Jun-Ru ZENG1, Yonatan Garkebo DOYORO2,1
1National Central University, Taiwan, 2Academia Sinica, Taiwan

Geophysical survey has made understanding of the Earth’s subsurface possible and thus aids the planning and the execution of natural hazard mitigation as well as energy resource exploration. Many geophysical methods are developed to suit various exploration targets. Magnetotelluric (MT) is one of the common methods that can be used to retrieve subsurface information both from shallow and deep target. It is a passive geophysical method that measure the naturally occurring electromagnetic (EM) field at the earth surface. The MT survey can record EM waves in the frequency range between 10-4-104 Hz. Such a wide band frequency makes it possible for MT to yield tens to a few hundreds of kilometers subsurface information. Yet, it is due to this reason that the MT method suffers from electromagnetic noise contamination that lies between its broadband frequency range. While the noise source can come from natural phenomenon such as a complex geological condition, artificial sources are also significantly affecting the recorded signal. A few examples are power transmission lines, urban constructions, communication devices and electric railway. The contamination often results in distorted MT data and the decrease in reliability of the subsurface information. Thus, obtaining a good quality MT data has been a challenge for many years. In this study, we begin by observing the MT timeseries recorded in urban area where noise source is abundant. We analyze the timeseries and attempts to work out how signal from difference sources are affecting the data and what are their approximate frequency range. This can be helpful to identify the character of each signal and better help preserve the target signal to avoid underestimation or overestimation. This work serves as a groundwork for our future studies in attempt to obtain an improved result from MT survey, especially in the urban area of Taiwan.


IG12-A008
Changing Patterns and Determinants of Green Buildings in Guangzhou, China

Lijie LIN#+
Guangdong University of Technology, China

With the development of the economy and society, energy crises and environmental problems have been a worldwide concerned issue. Considering that energy consumption in construction and related sectors is much higher than that in others, the concept of green building is accordingly processed. In accordance with China’s carbon goals of energy saving and emission reduction, it is necessary to study the spatiotemporal patterns of green buildings in China and to reveal the driving forces of such patterns. The previous study of spatial and temporal variations of green buildings in China mainly focused on a national or regional scale, while the disparity of green buildings within a particular city has not received much scholarly attention. Based on the data of green buildings label projects from 2008 to 2021, by taking Guangzhou as a study case, this study aims to explore the spatiotemporal patterns and the major driving forces of uneven green buildings development in Guangzhou. It is found that: (1) Green buildings developed a lot in Guangzhou from 2008 to 2021. The growth rate of the number of projects and construction areas reached a peak in 2013 and then moderated to a stable lower trend. (2) Most of the green building projects gathered in the central west and south of the city, while small parts of them gathered in the northeast. Additionally, there is a significant disparity in ratings of green buildings in the spatial dimension. (3) Economic factors and resource factors are the main factors affecting the development of green buildings.


IG12-A010
Changes in Productivity and Deep Water Oxygenation at Central South Pacific Across the Mid-Pleistocene Transition - A Benthic Foraminiferal Proxy

Nirakara MAHANTA#+, Raj Kumar SINGH, Sunil Kumar DAS
Indian Institute of Technology Bhubaneswar, India

The emergence of 100 kyr glacial cycles after the mid-Pleistocene transition (MPT) has always been linked with a long-term decrease in atmospheric pCO2 levels. The Southern Ocean plays a major role in decreasing glacial pCO2 through enhanced productivity and stratification of the water masses. To assess these variabilities, we analysed the benthic foraminifera of the sediment cores recovered from IODP Site U1540 (55o08.5’S, 114o50.5’W, 3580 m depth) for the period up to 1.5 Ma. The distribution pattern of benthic foraminifera are ideal proxy to assess the variations in productivity, organic carbon flux, and changes in the dissolved oxygen contents of the bottom water. The site is located in the Central South Pacific (CSP) and responds to global atmospheric fluctuation. The high productivity group, which includes Melonis pompilliodes, Melonis barleeanum and Uvigerina peregrina showed an increasing trend from pre-MPT to post-MPT period, but the amplitude of fluctuations increased during the post-MPT. This suggests a switch to 100 kyr, high amplitude change in productivity at CSP during various glacial-interglacial period. This is also evident from the increase in infaunal vs epifaunal ratio and increase in benthic foraminiferal species diversity. The bottom water corrosiveness was nearly absent during the pre-MPT and early transition period, which increased towards last phase of MPT marked by the abundance of Nuttallides umbonifera. This study observed high-amplitude fluctuation in all the proxies after the MPT in response to long-term glacial-interglacial changes at CSP.


IG12-A011
Participatory Resource and Landscape Services Mapping of an Upland Mining Community: Case Study of Ampucao Village in Itogon, Benguet, Philippines

Rico Neil QUIERREZ1,2#+, Ma. Catriona DEVANADERA3, Edgar Jr REYES3, Casper Boongaling AGATON3, Leonida BUGAYONG2, Jessie SAMANIEGO4, Cris Reven GIBAGA4, Alexandria TANCIONGCO5,6, Carlo ARCILLA5
1University of the Philippines, Philippines, 2University of the Philippines Open University, Philippines, 3University of the Philippines Los Baños, Philippines, 4Philippine Nuclear Research Institute, Philippines, 5University of the Philippines Diliman, Philippines, 6University of the Philippines Diliman, Philippines

Long-term sustainable management of mining areas entails better understanding of human-environment interaction including environmental impacts, land use and landscape services among local communities. The study area, Ampucao Village in Itogon, Benguet, has long been a mining community hosting a sixty-year-old large-scale mining company and numerous artisanal small scale gold mining. In this research, participatory mapping and focus group discussion were conducted to characterize the human-environment interactions of an upland mining community in Philippine context through a community drawn resource map outlining their natural, economic and social resources. Sketch maps were then digitized using QGIS 3.22.8 for spatial occurrences and analyses. Results show that landscape services enjoyed by Ampucao community from their environment mainly include food, geological resources, ornamental resources, fuel, raw materials, spiritual values, aesthetics and social relations. Generated maps show geographic patterns of each landscape service. Identification and mapping of community’s local spatial knowledge are critical inputs to sustainable management of mineral rich areas and could serve as essential guide for policy makers regarding mixed-used natural resources management.


IG12-A012
Urban Change Detection in Metro Manila, Philippines Using Sentinel-1 SAR Coherence

Ma. Criselda BALDAGO#+, James Cesar REFRAN, Paul Daniel ANG, Gay Jane PEREZ
Philippine Space Agency, Philippines

Monitoring urban change is of significance to policy makers, city planners, and social and environmental scientists in addressing problems that may arise from the growth or decline of an urban settlement. Metro Manila, Philippines is one of the most rapidly growing urban regions in East Asia and the Pacific with a current population of 18,649,422 increasing at a rate of 2.05 percent annually. Among the challenges in studying the urbanization of Metro Manila, is identifying centers of rapid population increase. This rapid and dispersed growth in urban areas is difficult to monitor on the ground. Consequently, problems such as pollution, transportation, lack of resources and inequality would result from failure to monitor these growth centers. Satellite remote sensing is an advantageous tool for urban change detection, having global coverage and consistent revisits of the same area which is ideal for monitoring. Particularly, the Synthetic Aperture Radar (SAR) instrument offers reliable, wide-scale data regardless of the time of day and weather condition. Buildings and other man-made structures have a high radar reflectance when observed in multi-temporal SAR images. Coherence is the similarity of radar reflectance between two SAR images of the same area taken at different times. In this study, Sentinel-1 SAR images of Metro Manila, Philippines were processed to obtain the difference in coherence between consecutive monthly images dated 2018 to 2022. Geospatial Information System (GIS) operations were performed to determine how urban areas evolved in the last four years. Validation of generated coherence maps through optical imagery confirmed detectable changes in industrial and commercial districts as well as large residential areas in Metro Manila. Effectively monitoring the centers of population growth in urban areas would aid in building more sustainable and livable cities.


IG12-A015
Integrated Geophysical Studies to Decipher Subsurface Configuration and Evolution of a Non-volcanic Geothermal System Along Mahanadi Rift Basin, India

Aurobindo Kumar BASANTARAY1+, Animesh MANDAL2#
1Earth Sciences, Indian Institute of Technology Kanpur, India, 2Indian Institute of Technology Kanpur, India

Non-volcanic hot springs within intracontinental rifted but relatively stable continental part are often less studied owing to its inherent low-enthalpy nature and sedimentary provenance. Present integrated geophysical study using gravity and magnetic methods, combined with the results of previous near-surface investigations, aims to map sub-surface structure, and to understand the evolution of hot springs in the Atri and Tarabalo region of the Mahanadi rift basin, Odisha, India. Gravity-magnetic study reveals deeper structure and its effect on geothermal activity. The 3D gravity model deciphers the presence of high density (>2750 kg/m3) igneous formations beneath the metamorphic and sediment formations as well as the depth extent of Mahanadi fault. Deeper Moho (depth ~34 km) than the estimated average curie depth (as 29 km) for the area supports the presence of felsic intrusion as observed in 3D model. Based on geophysical inferences and previous geological findings the study hypothesises that Mahanadi rift basin may have originated from a pull-apart basin formation during the Permian period, leading to multiphase tectonic and sedimentation processes until the separation of Australia, Antarctica, and India during early Cretaceous. The Mahanadi graben has undergone transformation due to breakup after ignition of plume activity, resulting in the Khondalite group of rocks and igneous rock formations around the edges of the graben. Both rock formations act as heat sources in the hot spring region. Faulted metamorphosed formation overlain by sedimentary formations is identified as the strata for heat transfer to meteoric water via convection processes, and the strata may be considered as the hot water reservoir. Smaller faults and fissures that link Mahanadi fault act as conduits for hot fluid outside of the geothermal system's heat source and reservoir, and may have evolved during the basin's rifting phase.


IG12-A016
The Origin of Pyrite in the Soils of Brunei Darussalam

Pavlos TSIKOURAS1, Stavros KALAITZIDIS1, Elena IFANDI2, Azrina BOEY2, Basilios TSIKOURAS2#+
1University of Patras, Greece, 2Universiti Brunei Darussalam, Brunei Darussalam

Pyrite deposition in sedimentary basins is an intriguing topic due to the great variety of the forming processes, often overlapping. Additionally, its formation plays an important role in the global Fe and S cycles, largely affecting the redox chemistry of the atmosphere. Pyrite is abundant in all the detrital Miocene sedimentary formations of Brunei Darussalam. X-ray diffraction data and microscopic studies show the abundance of octahedral and/or cubic pyrite, frequently associated with clay and/or coal layers, suggesting an authigenic, rather than detrital, origin and slow rates of crystallisation. Infrequently pyrite is associated with gypsum and native sulphur. It is likely that the pyrite formation in Brunei is triggered by sulphate-reducing bacteria (SRB), which mediate in the formation of pyrite from the transformation of mackinawite and/or greigite, formed in euxinic environments. Microbial H2S is capable to convert FeS to FeS2 (pyrite). The occurrence of sulphur S0 promotes the conversion of mackinawite into pyrite and may derive either from the oxidation of bisulphide (HS-), a common metabolic product of SRB, or from the organic matter in the sediments, which consumes oxygen and releases sulphur. It has been suggested that pyrite-forming reactions are coupled with methane formation with the synergistic aid of methanogen microorganisms. In outcropping formations and/or nearby surfaces of recent sediments, the pyrite is extensively oxidized to Fe-oxides forming red ferricrust. The occurrence of gypsum may be explained by the oxidation of pyrite and the production of H2SO­4, which reacts with Ca2+ of the abundant micro- and nannofossils hosted in the Miocene formations. This natural acid drainage process is thought to be responsible for the highly acidic soils in Brunei Darussalam and requires close monitoring for potential adverse effects on agricultural activities and groundwater contamination.


IG12-A018
Assessment of the Geochemical Contamination Levels in the Agricultural Soils of Brunei - Muara District, Brunei Darussalam

Khairunnisa Nazirah KARIM, Elena IFANDI#+, Azrina BOEY, Adlina MISLI, Haezan JANGARUN, Syahrul Nizam ADENAN, Basilios TSIKOURAS
Universiti Brunei Darussalam, Brunei Darussalam

Recently, the Government of Brunei Darussalam has recognised the need to increase agricultural productivity in line with the country's Wawasan 2035. To this end, soil conditioners and fertilisers have been used to improve the properties of naturally acidic soils. However, these practices may have unintended effects on the soil quality and public health. Geochemical analyses were conducted on 370 topsoil and 370 subsoil samples collected from a grid with a density of one sample per km2 in Brunei-Muara District to assess potential contamination. Results showed enrichments of potassium, manganese, sodium, nickel, zinc and phosphorus in agricultural topsoil, with lesser intensity in the subsoil. In order to ascertain whether the enrichment of these elements had reached concerning levels, statistics and heatmaps were used to identify threshold values and evaluate the degree of contamination. The heatmaps highlighted geochemical anomalies in the southwestern region of the District, where mostly paddy plots are found. We suggest that the geological setting has a significant role in this, as the Jerudong anticline acts as a natural barrier, trapping the aforementioned elements in the soil of its west limb. Additionally, organic matter and clay minerals contribute to the retention of these elements in the agricultural soils. Copper contents show a positive correlation with zinc, which is typically found in soils where poultry manure is applied, a practice that has been actively implemented in the country until recently. Although there were intense geochemical anomalies of these elements, the enrichment factor and geoaccumulation index suggest that the contamination is currently at a manageable level. However, if proper agricultural practices are not adopted and implemented, contamination may reach concerning levels in the near future. Therefore, it is essential that the relevant stakeholders take proactive steps to ensure that the agricultural soils remain uncontaminated and of high quality.


IG13-A003
Decomposition of Carbon Emission Driving Factors and Judgment of Peak Status in Countries Along the Belt and Road

Yuanmeng LI#+
Beijing Normal University, China

Most of the countries along the “Belt and Road” are still developing countries, and most of their carbon emissions have not yet reached their peak. However, there is currently a lack of comprehensive analysis and research to judge the current carbon peak state of the countries along the “Belt and Road” and quantify the contribution of key driving factors to the carbon emissions of the countries along the “Belt and Road”. This study fills this gap by developing a new method for judging the peak carbon status of a country based on the time series of carbon emissions. We divide the status of all countries along the Belt and Road into four categories: Has reached the peak, Peak plateau period1 (the downward trend is not significant), Peak plateau period2 (obvious recession), Not reached the peak. The results show that the main positive driving factor of the three countries that have reached the peak is GDP PPP per population, while other driving factors make negative contributions to carbon emissions. However, in some years, these countries briefly experienced a negative contribution of GDP PPP per population to carbon emissions. The driving factors of the country's carbon emissions in the Peak plateau period play a role and are not stable. The contributions of GDP PPP per population, energy intensity and carbon intensity fluctuate periodically, sometimes positive and sometimes negative. In countries that have not reached the peak of carbon emissions, population growth and economic growth are very significant positive contributors to carbon emissions, and the effect of driving factors that negatively contribute to carbon emissions is not so obvious.


IG13-A013
The Effects of Human-made and Natural Disturbances on the Eco-environment from a Global View

Yuei-An LIOU#+, Kim Anh NGUYEN
National Central University, Taiwan

It has been well recognized that human activities have negative impacts on the nature. Here, we introduce a framework to assess the eco-environmental vulnerability due to human-made and nature disturbances on a global scale with emphasis on the former factor. Since COVID-19 pandemic has caused a significant impact to the whole world in the past few years, it has been chosen to be a key influential factor in the current study. To prevent the spread of COVID-19 virus, it has been a typical measure to impact lockdown over a region, city, or even a whole country during the first couple years after pandemic outbreak except China where zero COVID-19 policy was implemented till January 2023. Under lockdown circumstance, the human activities are either significantly reduced, or even essentially ceased. In this study, global eco-environmental vulnerability maps with quantified levels before COVID-19 and during pandemic will be presented. Their comparison reveals the improved environmental conditions over the whole world as expected. The improvement, due to lockdown policy, can be considered as the benefit brought to the environment with the sacrifice of human beings’ welfare or even life. It becomes an interesting question should the human activities be ceased to protect the natural environment for the sustainable development of the world?


IG13-A015
Resilience in Response to Climate Change and Social Sustainability Assessment: Case Study of Aquaculture Industry in Pingtung, Taiwan

Li-Sheng WANG, Ching-Hsien HO#, CHIH-HENG CAI+
National Kaohsiung University of Science and Technology, Taiwan

In the event of future climate change and extreme climate hazards, the global fishery industry will have to face the compound impact caused by long- and shortterm climate hazards. With the intensification of climate change and extreme weather, however, forecasting changes in the natural environment is laden with high uncertainty and variations. Taiwan’s geographic location is favourable for aquaculture, which has evolved into an important primary industry and source of animal protein for the residents of Taiwan. Aquaculture plays a critical role in Taiwan’s aquatic product supply chain. Since 2011, the annual output of aquaculture has been maintained at approximately 310,000 tons, with a monetary value of approximately 40 billion NTD. In recent years, both long-term climate change and extreme climate hazards (for example, extremely high or low temperatures) have led to shocks to the aquaculture industry, such as environmental degradation and sudden deaths or losses of certain species, causing operational losses for fishers. The instability of and fluctuations in aquaculture, in turn, directly affect supply of and demand for aquatic products in the market. As such, this study attempts to perform a case study of aquaculture in Pingtung, Taiwan that incorporates social concern assessments of risk perception and the judgement of risk acceptance through risk management processes. Furthermore, the study incorporates stakeholder participatory processes to reduce the gap in awareness of adaptation and increase the opportunity of reaching a consensus and to develop an integrated risk management model that makes decision making better meet the actual needs of society. It is expected that these measures will enhance all parties’ willingness to adapt and help achieve the goal of public-private collaboration in facing the challenge of climate change.


IG15-A002
MIOS Radar Interferometry

Haiyong XIE1#+, Guozhu LI2, Yi LI2, Lianhuan HU2
1Institute of Geology and Geophysics, Chinese Academy of Sciences, China, 2Chinese Academy of Sciences, China

The Meteor and ionospheric Irregularity Observation System (MIOS), which consists of radar subsystem at Ledong (18.4°N, 109°E), and multi-station optical subsystem at Ledong and Sanya (18.3°N, 109.6°E), has been fully operated since December 2021. The radar subsystem includes a coherent radar with an operational frequency of 47.5 MHz and a peak power of 72 kW. It employs an active phased array consisting of 135 three-element Yagi antennas. The phased array is divided into 15 identical subarrays arranged in an area shaped like a sword. One capability of this radar is to unambiguously locate backscatter echoes using the multi-base-line spatial-domain interferometry. In order to calculate ambiguities and avoid the effects of mutual impedance, crossed subarrays 2, 4, 10, 11, and 15 with spacings of 4λ, 4.5λ and 8.5λ are used. Radar system phase offset calibration is critical to the interferometry analysis. Considering that the multi-station optical subsystem of MIOS can obtain the accurate spatial location of an ablating meteoroid. We used a common meteor and calibrated the radar system phase offsets. A good agreement between the positions of non-specular echoes derived from the radar interferometer and those of optical meteors was found, validating that the radar system phase offsets have been properly calibrated. And then, the backscatter echoes could be located accurately after the calculations of phase differences and ambiguities. Based on this work, the development of coherent radar imaging technique will be carried out in the future.


IG15-A008
Multireceiver and Multifrequency Techniques Used with VHF Atmospheric Radar for Volume Imaging

Zhen-Xiong YOU1#+, Yen-Hsyang CHU2, Ching-Lun SU2, Chien-Ya WANG3, Hiroyuki HASHIGUCHI4
1China Medical University, Taiwan, 2National Central University, Taiwan, 3Chinese Culture University, Taiwan, 4Kyoto University, Japan

Very-high-frequency (VHF) atmospheric radar is a pulsed, phase-arrayed, and powerful instrument for remote sensing of the atmosphere. In addition to clear-air turbulence and plasma echoes, precipitations and meteors are also observed frequently by such kind of radar. To improving the spatial resolution of echoes for obtaining additional information of the targets in the radar volume, observational techniques with multiple receivers and multiple frequencies are one of the approaches. Adaptive retrieval algorithms are commonly applied to these multi-channel received radar echoes, and as a result, multiple layers, multiple echo centers, and so on, in the radar volume could be resolved to some degree. In this report, high-resolution observations of the atmosphere using multireceiver and multifrequency techniques are present, including clear-air turbulence, precipitations, small-scale and wavy layer structures, field-aligned plasma irregularities, meteors, aspect sensitivity in neutral and ionospheric irregularities, and so on.


IG16-A006
Real-time Anomaly Detection in Population Data from Mobile Spatial Statistics for Disaster Mitigation

Erick MAS#+, Shunichi KOSHIMURA
Tohoku University, Japan

Observation of population dynamics is possible due to GPS technology and localization of users connected to telecommunication towers. Many studies have used GPS mobile data for various applications in multiple fields. However, those studies use samples from a particular cellphone provider or small sets of a larger population. Limited data may incorporate biases or incorrect recommendations that may be critical, at least for disaster mitigation. Another approach is Mobile Spatial Statistics (MSS) which estimates the number of people in rectangular cells (mesh) at regular intervals. MSS uses GPS-enabled devices, adoption rates, and spatial statistics to correct for biases. Thus, population counts in MSS data correspond not only to mobile phone users but also those from different providers or even with off-portable terminals. Here, we used MSS data to develop a real-time system for anomaly detection to grasp the effects of disasters on population dynamics. We discuss the challenges in this kind of application, focusing on the methodologies, event duration, the spatiality of the problem, and online implementation requirements. Finally, this study provides a step toward a Coastal Digital Twin for Disaster Mitigation. Population dynamics are followed in real-time and analyzed to flag anomalies due to possible disasters or emergencies.


IG16-A009
Investigating the Link Between the River Profile and Streambed Texture of Mixed-grain Size

Dongwoon KANG+, Kyungrock PAIK#
Korea University, Korea, South

There has been a long debate on the relationship between the concavity of river profile and the streambed texture. A school of thought claimed that the concavity increases as bed sediment size grows. Another argued exactly the opposite: the concavity diminishes as particle size increases. We aim to test which of these hypotheses is appropriate, using a whole landscape evolution model with selective transport of mixed-size sediments. We aim to run the model over geologic time scale to reproduce whole landscape evolution, under ideal tectonic and climate scenarios. The selective transport of particles causes downstream fining to emerge, and as the distribution of grain sizes changes, so does the local slope. Simulation results and in-depth scientific discussions will be presented.


IG17-A005
GEWEX and International Research Collaboration in Asia

Petrus (Peter) VAN OEVELEN#+
George Mason University, United States

The Global Energy and Water EXchanges (GEWEX) project of the World Climate Research Programme (WCRP) has for more than 30 years supported and promoted successfully international research collaboration on climate, energy and water. During these more than 3 decades a clear change in how research has evolved from more disciplinary to inter- and transdisciplinary has manifested itself. With that change the challenges regarding collaboration have grown but likewise the opportunities. In this presentation a short overview is given on past, present and future developments within GEWEX on promotion of international research collaboration and how that is relevant and applicable to the Asia and Oceania region and what are the main take away messages that can also be of use and relevance to other actors.


IG17-A009
Earth Sciences for a Sustainable Future: The AOGS Initiative in Advancing SDGs

Ping-Yu CHANG#+
National Central University, Taiwan

The Asian Oceania Geosciences Society is one of the organizations in Asia that recognizes and works towards reaching the Sustainable Development Goals (SDGs) through science cooperation. AOGS founded the Interdisciplinary Geoscience Section, which aims to collaborate with scientists studying geoscience in different disciplines, especially in sustainable approaches and studies. We are concerned with issues that can help the regional society achieve more sustainable, safe, and resilient infrastructure through the application of earth science technology and observations. One of our recent missions is to promote SDGs through geoscience research efforts. Since 2020, SDGs video contests have been held every year for students and members to promote awareness of the SDGs to the geoscience society and the general public. Participants can upload their videos to YouTube and have them evaluated by invited judges. Through new media broadcasting abilities, we hope not only to promote SDGs awareness to the public but also to recognize and promote research groups in geosciences over the Asian-Oceania region for their contribution to the SDGs.


IG17-A010
Project PIPE DREAM for Regional and International Cooperation

Yi-Shiang TZENG1#+, Wing-Huen IP1, Gilbert PI2
1National Central University, Taiwan, 2Charles University, Czech Republic

As the pace for manned missions to the Moon and Mars has been picked up, the study of space weather effects has also gained more and more attention in the context of interplanetary travels and lunar and Martian settlements. These considerations lead to the discussion of necessary deployments of small spacecraft and/or CubeSats at the Sun-Earth L4 and/or L5 Lagrangian points for solar and heliospheric observations. The basic idea is that the L5 point provides the best vantage point for viewing the eastern limb of the sun, thus allowing a high-precision forecast of space weather effects due to the impact of geoeffective CME impacting the Earth's magnetosphere. On the other hand, the L4 point is the best place to monitor extreme SEP events occurring on the west limb at ~ W60, with GeV ions capable of causing ground-level events (GLEs) on Earth, which are also dangerous to the Moon and Mars explorers. It is therefore clear that in the coming decades, we will see spacecraft stationing at different strategic positions around the Earth's orbit (or beyond) to provide inputs to space weather forecasts on an interplanetary scale. This is also the meaning of PIPE DREAM for "Patrolling Interplanetary Explorers and Deep-space Research Mission." In this presentation, we will discuss how Project PIPE DREAM representing a large-scale international cooperation might be realized by combining the solar space observatory missions to be launched and under planning by different space organizations.


Thu-03 Aug | 10:20 - 12:20 | MR307
IG12 - General Session

Session Chair(s): Ping-Yu CHANG, National Central University, Vena Pearl BONGOLAN, University of the Philippines Diliman

IG12-A004
What Are We to Do with the SDGs?

Vena Pearl BONGOLAN#+, John Rowan DE GUZMAN, Brandon Kahel MARTIN
University of the Philippines Diliman

In 2015, the United Nations adopted 17 Sustainable Development Goals (SDGs) with 169 targets for transformation toward a more sustainable future by 2030. This study aims to analyze 14196 unique target interactions, to determine resolutions for problematic interactions, and to find synergistic interactions that will improve the efficiency in achieving the set goals. Two methods are employed in the analysis. First, experts with over five years of SDG-related experience evaluated interactions using a 7-point scale proposed by the International Science Council. Second, a non-parametric Spearman rank correlation is used on official indicator data from the UN with resulting coefficients serving as interaction scores. Interaction scores are then interpreted to mean that target pairs interact positively (synergies), negatively (trade-offs), or neutrally (nonclassified). Targets are also modeled as nodes and interactions as edges in graphs presented in sdg-interactions.herokuapp.com. Currently, there are 1322 target interactions evaluated by experts, 76.24% are synergies, and 3.86% are trade-offs. The official indicator data, with all 14196 interactions evaluated, 2.06% are synergies, and 1.66% are trade-offs, the rest are unclassified. As this study continues, more experts will be able to evaluate target interactions and attempt to resolve conflicts, to make for a more efficient implementation of the SDG targets and goals.


IG12-A001
Study on Nowcasting Lightning Based on Deep Learning Method Using Multi-source Data

Wenjie YIN1+, Xu YANG2, Ting HUANG3, Chen ZHOU1#
1Wuhan University, 2Nanjing University of Information Science & Technology, 3Hefei University of Technology

Lightning discharge, as a natural phenomenon occurring in the atmosphere, has posed great threat to the civilian life and assets, thus arousing numerous attentions in the lightning forecast. Since lightning is associated with intricate dynamic and microphysical processes, improving the accuracy of the lightning prediction system requires the full utilization of various meteorological parameters. Owing to the rapid progress in machine learning(ML) techniques and the burst of the meteorological data, it has motivated many researchers to utilize data-driven models for lightning forecasting. This study analyzes different prediction methods, including numerical parameterization method and ML method. The pros and cons of classical parameterization methods are studied in detail for the purpose of making use of the domain knowledge inside those methods. Multi-source data include radar reflectivity provided by Doppler weather radar, the past total lightning location data by VLF lightning locating system and simulation data by the Weather Research and Forecasting (WRF) model. Different data types possess different characteristics, which makes it difficult for data fusion. However, it is feasible for machine learning method to exploit complementary information and teleconnection distributed across various data sources. We propose a framework based on machine learning method which can effectively combine multi-source data to nowcast lightning incidence. The preliminary result shows the great potential of the application of machine learning method to lightning prediction.


IG12-A005
The Weakened Jet Stream and Its Influence on Flight Time During Solar Proton Events

Yi WANG1#+, Fengsi WEI1, Xueshang FENG2
1Harbin Institute of Technology, 2Chinese Academy of Sciences

Analyzing the effects of climate variability and space weather on aviation is a new and developing topic. It has been commonly accepted that the flight time of the polar flights may increase during solar proton events, because the flights have to change their route to avoid the high-energy particles. Recent analysis has also indicated that the flight durations will be influenced by climate. However, solar proton events resulted changes in atmospheric circulation and its influence on flight time have never been reported. Based on the analyses of 39 representative international air routes around westerlies, it is found that 89.74% (84.62%) of the commercial airplanes on the westbound (eastbound) air routes reveal shorter (longer) flight time during solar proton events compared to those during quiet periods, and the averaged magnitude of change in flight time is ~5-6 min. Further investigation on the vertical profiles of trends in south-north temperature difference and zonal wind characteristics implies that the solar proton events associated atmospheric heating will change the flight durations by weakening the polar jet stream. This is the first report to detail the impact of solar proton events on atmospheric circulation and flight time. These findings are important for aviation, as they may help airlines optimize routes, reduce fuel costs, and even contribute to climate change mitigation efforts.


IG12-A009
Impact of Still-in-use Greenhouses on the Prevalence and Distribution of Soil Microplastics

Wainkwa Chia ROGERS#+, Jin-Yong LEE, Minwook LEE
Kangwon National University

The use of greenhouses to enhance crop cultivation has been in use for a very long time. Today, many studies are focusing on the growing prevalence of microplastics (MP) in soil because of their rapidly increasing environmental risks. Among these studies, soil MP contamination is often only recorded in abandoned greenhouses. However, there is still a knowledge gap on the occurrence and distribution of MP in greenhouse soils still in use. In this study, topsoil samples were collected from a three-year-old greenhouse for growing tomatoes and a Fourier transform infrared microscopy was used to identify MP size, shape, and intensity. In just three years, the greenhouse contaminated soils with a total of 1107 items kg−1 and the average abundance of 221.4 items kg−1. Most MPs were either transparent or white, and the dominant MP shape was fragmented (32.79%). MPs identified were classified into 4 sizes such as 20–49, 50–99, 100–299, and 300 μm and above but the size 20-299 μm was dominant (99.7%). Six MP types namely, polypropylene, polyethylene, polyethylene terephthalate, polyvinyl chloride, polyethylene amide, and polymethyl methacrylate. were detected. Soil MP contamination in the greenhouse may have originated from external contamination by farmers during crop planting and groundwater used for irrigation during growth in the greenhouse. This study provides first-hand data on the contribution of the utilization of greenhouses for tomato growth in a short period of time before being abandoned or recycled on MP in Korea. This information is useful as background information to understand MP contamination of top and its possible influence on environmental geology. This work was supported by the Research Institute for Earth Resources through the Basic Science Research Program of the National Research Foundation of Korea (NRF) funded by the Ministry of Education (No.2019R1A6A1A03033167).


IG12-A014
Direct Confirmation of Widespread Illegal Sand Mining in the Mekong Delta Through Government Statistics

Kai Wan YUEN1#+, Edward PARK1, Duc Dung TRAN2,1, Ho Huu LOC3, Lian FENG4, Jingyu WANG1, Charles-Robin GRUEL5, Adam SWITZER1
1Nanyang Technological University, 2National Institute of Education and Earth Observatory of Singapore, 3Asian Institute of Technology, 4Southern University of Science and Technology, 5Centre National de la Recherche Scientifique

Sand is being extracted illegally from many Southeast Asian rivers for economic and urban development. As a global mining hotspot, we used the Vietnamese Mekong Delta (VMD) as a representative case study for illegal mining and we quantified the extent of illegal sand mining in the VMD for the first time by verifying provincial-level sand budget data from the local government with field-based measurements. The amount of illegally mined sand decreased from 16.7 Mm3/yr in 2013 to 15.5 Mm3/yr in 2018-2020. An increase in the allowable rate of sand extraction from 11.5 to 17.7 Mm3/yr in three provinces contributed to this decrease as the illegal mining rate was the difference between the allowable rate of sand extraction set by the government and the actual volume of sand mined. To ensure the sustainability of sand resources, we recommend that local rates of sand extraction should not exceed the sediment replenishment rate.


IG12-A017
The Evolution of Tropical Peatlands in Brunei Darussalam: Palaeoenvironmental and Palaeoclimatic Archives

Adlina MISLI1, Basilios TSIKOURAS1#+, Muhammad Syazwan OMAR1, Syahrul Nizam ADENAN1, Stavros KALAITZIDIS2, Kimon CHRISTANIS2, Elena IFANDI1
1Universiti Brunei Darussalam, 2University of Patras

Tropical peatlands are important ecosystems, which have the capability to store high amounts of carbon and comprise significant archives for understanding environmental conditions of the past. Tasek Merimbun is a modern lake system surrounded by mires, whereas Temburong mire is associated with a system of meandering rivers and their tributaries close to the coastline, in Brunei Darussalam. Field work included mapping and coring, whereas laboratory work comprised proximate and ultimate analyses, along with grain size analysis in samples from both systems. The maximum cored peat thickness is ca. 10 and 1.50 m for Tasek Merimbun and Temburong, respectively. Peat formation started around 6,500 years BP (during the Fast Fluctuation period) at the SE part of the Tasek Merimbun and 2,500 years BP (during the Mild Cooling period) at Temburong, both likely as paralic mires in estuarine environments. The accumulation of organic matter in both areas initiated in topogenous mires (fen), which later transitioned into ombrogenous ones. The accumulation rates were generally low in both domains, similar to other Southeast Asian peatlands; the Tasek Merimbun peatland shows an expected accelerated rate during the Warming Period of mid-Holocene. It is suggested that the coastline of Brunei Darussalam after the Last Glacial Period and sea-level rise, was a few kilometres south of the present one. The subsequent combined effect of eustatic sea-level changes with the deposition of large amounts of river sediments eventually shifted the modern coastline northwards.


IG12-A021
A Soil Moisture Decohesion Model for Predicting Railway Slope Failure Under Heavy Rainfall

Sudath LOKU-PATHIRAGE1, Jiye CHEN2#+
1University of Moratuwa, 2University of Portsmouth

Global climate change brings extremely heavy rainfalls every year, which causes natural and engineering slope failures in many countries across the world. The slope failure as natural disaster can cause extensive human suffering and financial losses worldwide. This paper develops a novel soil moisture decohesion model (SMDM) for predicting railway slope failure under heavy rainfall. In this paper, a correlation between rainfall intensity and soil moisture content is established first thus investigation of rainfall intensity effect is identical to that from soil moisture content. Considering slope failure mechanisms dominated by soil or slope material cohesion lost due to heavy rainfall, the SMDM is developed to express that soil cohesion varies with different soil moisture contents, and to reflect soil cohesion reduction when increasing soil moisture content or rainfall intensity. The SMDM is incorporated into the extended cohesive damage element (ECDE) method to fundamentally study slope failure mechanisms under different soil moister contents. As an example, the proposed SMDM-ECDE approach is applied in prediction of damage scale of a selected railway embankment slope under varied soil moisture contents or rainfall intensities, and a prediction of failure initiation at the selected railway embankment site under a critical soil moisture content or rainfall intensity is successfully completed. The proposed SMDM-ECDE approach provides a new tool to fundamentally study slope failure mechanisms and forecast slope failure under heavy rainfall.


Thu-03 Aug | 1:10 - 3:10 | MR307
IG03 - Data-driven Modeling in Geoscience

Session Chair(s): Shin-ichi ITO, The University of Tokyo, Ryoichiro AGATA, Japan Agency for Marine-Earth Science and Technology

IG03-A011 | Invited
Bayesian Variational Geophysical Inversion

Xin ZHANG#+
China University of Geosciences

In Earth sciences scientists often need to characterise subsurface properties using data recorded at the surface, which is usually achieved by solving an inverse or inference problem. Due to nonlinearity of the problem, insufficient data coverage and noise in the data, the inverse problem almost always has nonunique solutions and therefore the uncertainty must be estimated. Monte Carlo sampling methods are often used for this purpose, but they are generally computationally intractable for large data sets and high-dimensional parameter space. To extend uncertainty analysis to larger systems, we apply variational inference to solve the inverse problem. Variational methods solve the Bayesian inference problem as an optimization problem, yet still provide fully nonlinear, probabilistic results. We first apply variational inference to two types of 2D seismic inverse problems using synthetic and real data: travel time tomography and full waveform inversion (FWI). In each case we compare the results to solutions given by a variety of Monte Carlo methods. The results demonstrate that variational inference can produce accurate approximations to the results of Monte Carlo sampling methods at significantly reduced computational cost. To further extend the method, we apply variational inference to 3D and time-lapse FWI problems. The results demonstrate that variational inference can be practically applicable in solving 3D FWI problems and monitoring changes in the subsurface. We therefore conclude that variational inference provides a valuable tool to image the subsurface and quantify uncertainties.


IG03-A015
Detection of Deep Low-frequency Tremors from Continuous Paper Records at a Station in Southwest Japan About 50 Years Ago Based on Convolutional Neural Network

Ryosuke KANEKO, Hiromichi NAGAO#+, Shin-ichi ITO, Hiroshi TSURUOKA, Kazushige OBARA
The University of Tokyo

Since deep low-frequency tremors are considered to be associated with large earthquakes that occur adjacently on the same subducting plate interface, it is important to investigate tremors that occurred before the establishment of modern seismograph networks such as the High Sensitivity Seismograph Network (Hi-net). We propose a deep-learning solution to detect evidence of tremors in the scanned images of paper seismogram records from over 50 years ago. In this study, we fine-tuned a convolutional neural network (CNN) based on the Residual Network (ResNet), pre-trained based on images of synthetic waveforms in our previous study, using a dataset comprised of images generated from real seismic data recorded digitally by Hi-net to facilitate a supervised analysis. The fine-tuned CNN was able to predict the presence or absence of tremors in the Hi-net images with an accuracy of 98.64%. Gradient-weighted Class Activation Mapping (Grad-CAM) heatmaps created to visualize model predictions indicated that the CNN’s ability to detect tremors is not degraded by the presence of teleseisms. Once validated using the training images, the CNN was applied to paper seismograms recorded from 1966 to 1977 at the Kumano observatory in southwest Japan, operated by Earthquake Research Institute, The University of Tokyo. The CNN showed potential for detecting tremors in scanned images of paper seismogram records from the past, facilitating downstream tasks such as the creation of new tremor catalogs. However, further training using an augmented dataset to control for variables such as inconsistent plotting pen thickness is required to develop a universally applicable model.


IG03-A014
Rapid Large Continental Earthquake Characterization Using High-rate GNSS by Deep Learning

Wenfeng CUI+, Kejie CHEN#, Mingzhe LYU, Feng ZHU, Guoguang WEI
Southern University of Science and Technology

The 6 February 2023 earthquake doublet in Turkey has again reminded us of the vast destructions caused by large continental ruptures. To this regard, Earthquake Early Warning (EEW) systems, which determine the earthquake magnitude, location in real time , have been operated in many places around the world for fast and efficient post-seismic response. Existing EEW mainly rely on seismic waveforms and treat the earthquake as a point source for simplification. However, the seismographs will clip and strong motion sensors may drift during large earthquakes. Furthermore, large continental earthquakes can cause hundreds of kilometers ruptures involving several asperities that accounts for localized strong shakings. In this study, based on High Rate Global Navigation Satellite System (HR-GNSS), which measures co-seismic displacement waveforms directly without saturation, we develop a multi-branch neural network framework aiming to characterize large continental earthquakes rapidly. A full range of over fifty thousand scenario earthquakes together with HR-GNSS observations are first generated following related scaling laws and physics. In addition to the already mapped fault traces, we also take account of the fault complexity. Feasibility of the framework has been demonstrated through the case study of the 2021 Mw 7.4 earthquake with a time cost of less than 110 milliseconds on a single CPU. 


IG03-A013
Seismic-Phase Detection Using Multiple Deep Learning Models for Global and Local Representations of Waveforms

Tomoki TOKUDA+, Hiromichi NAGAO#
The University of Tokyo

The detection of earthquakes is a fundamental prerequisite for seismology and contributes to various research areas, such as forecasting earthquakes and understanding the crust/mantle structure. Recent advances in machine learning technologies have enabled the automatic detection of earthquakes from waveform data. In particular, various state-of-the-art deep-learning methods have been applied to this endeavor. In this study, we proposed and tested a novel phase detection method employing deep learning, which is based on a standard convolutional neural network in a new framework. The novelty of the proposed method is its separate explicit learning strategy for global and local representations of waveforms, which enhances its robustness and flexibility. Prior to modelling the proposed method, we identified local representations of the waveform by the multiple clustering of waveforms, in which the data points were optimally partitioned. Based on this result, we considered a global representation and two local representations of the waveform. Subsequently, different phase detection models were trained for each global and local representation. For a new waveform, the overall phase probability was evaluated as a product of the phase probabilities of each model. This additional information on local representations makes the proposed method robust to noise, which is demonstrated by its application to the test data. Furthermore, an application to seismic swarm data demonstrated the robust performance of the proposed method compared with those of other deep learning methods. Finally, in an application to low-frequency earthquakes, we demonstrated the flexibility of the proposed method, which is readily adaptable for the detection of low-frequency earthquakes by retraining only a local model.


IG03-A005
NASSA: An Automated Earthquake Detection and Location Method Based on the Neighborhood Algorithm and the Source Scanning Algorithm

Jian WEN1#+, Sheng DONG1, Xiaofei CHEN2
1University of Science and Technology of China, 2Southern University of Science and Technology

We propose a new high efficiency automatic earthquake detection and location method from continuous data, based on the neighborhood algorithm (NA) and the source scanning algorithm (SSA). First, a new brightness function is introduced to shrink the model space from 4D to 3D. Second, before location, the time window that includes the candidate events is elected by the Density-Based Spatial Clustering of Applications with Noise (DBSACN). The seismogram without candidate events are abandoned. Third, to reduce the forward computation costs of the brightness, the NA is applied to substitute the time-consuming grid search method. Moreover, the traditional SSA always uses seismograms or characteristic functions (CFs) based on the statistical characteristics of seismograms to compute the brightness. However, the CFs’ peaks are only close to but not strictly equal to the true phase arrival time. Such differences will become the source of location errors. The phase picking by Machine Learning (ML) is high efficient, with the similar precision as manual picks by human analysts. Therefore, we choose the phase probability curve as a new CF. Finally, we define a confidence parameter that can quantitatively evaluate the inversion and help to select the true event from candidate events. We applied our new method (NASSA) to 20 days of continuous waveform data (2019.03.02~2019.03.21) at Changning−Zhaotong Shale Gas Field.


IG03-A020
Forecasting Aftershocks Immediately After the Large Main Shock with Epidemic-type Aftershock Detection Function

Kosuke MORIKAWA1#+, Hiromichi NAGAO2, Naoshi HIRATA2
1Graduate School of Engineering Science, Osaka University, 2The University of Tokyo

Immediate forecasting of the temporal and spatial distribution of aftershock sequences is vital for disaster prevention. However, identifying the number of aftershocks immediately after the main shock is challenging due to the contaminations of arriving seismic waves. To overcome this difficulty, some researchers introduced detection functions of the aftershocks to correct the bias. However, existing models of the detection probability for an aftershock do not utilize the information on aftershock sequences that occurred before the aftershock, which vitiates model flexibility. Our goal is to propose a model that can fully employ the local information of the aftershock sequences. The Omori-Utsu law is well-known for the law of the aftershock frequency, and the ETAS (epidemic-type aftershock sequences) model is its extension to making past information available. We propose a simple detection function that can use the past information of the aftershocks like ETAS. An effective estimation method for the model is also proposed.


IG03-A010
Fast Advanced Prediction of Water-filled Structure Using Transient Electromagnetic Method Based on Deep Learning

Rongjiang TANG1#+, Fengli SHEN2, Lu GAN2, Fusheng LI2
1Yangtze River Delta Institute (Huzhou),University of Electronic Science and Technology of China, 2University of Electronic Science and Technology of China

The transient electromagnetic method (TEM) is widely used for low-resistivity structure detection ahead of tunnel. However, it is not feasible to implement the 2D or 3D inversion of whole-space geo-electric models, due to the narrow space within the underground tunnel and non-uniqueness of TEM inversion. To solve this problem, we develop a fast inversion operator guided by deep learning to translate time-domain TEM measurements directly into the spatial probability of water-filled anomalies position. Trained by synthetic data, our system shows impressive adaptability to predict 3D position of water-filled anomalies, with different transmit current, source waveforms, number of coil turns, abnormal body size being implemented. The effectiveness of this method has been further confirmed by physical model experiments. This inversion operator can support instantaneous TEM low-resistivity detection in the tunnel activities.


Thu-03 Aug | 3:30 - 5:15 | MR307
IG03 - Data-driven Modeling in Geoscience

Session Chair(s): Dmitri KONDRASHOV, University of California, Los Angeles, Shin-ichi ITO, The University of Tokyo

IG03-A001
Opportunities for Sustainability with Minerals Value Chain Integration

Mark LINDSAY#+, Yufu NIU, Richard SCALZO, Sandra VILLACORTA, Lequn ZHANG, Peter COGHILL, Sandra OCCHIPINTI
Commonwealth Scientific and Industrial Research Organisation

Recent advances in sensing have augmented ore discovery, mining and sorting procedures that promise to improve the effectiveness and sustainability of mining operations. While these activities operate at different spatial and temporal scales, combining posterior models can further benefit the sustainability of exploration and mining operations. Discovering the combination of data and modelling techniques that operate across scales to achieve reliable predictions takes time and effort. Traditionally, we use geophysics at the regional to camp scales. Interpreted datasets such as gravity and magnetics successfully identify trans-crustal shear and fault networks that transport hydrothermal fluids and magmas to deposition sites and help to reduce the exploration search space. The utility of geophysics at these scales means they are almost ubiquitous features for machine learning prospectivity models predicting locations of mineralisation for both green- and brownfields exploration. The critical link between geophysics and geology is petrophysical data. For example, density data helps with gravity geophysics and is a critical rock property at all scales, from exploration to mining. The distribution of pay metals in mined rock detected by sorting methods and association with essential rock types, mineralogy or structures helps refine our conceptual, regional, and mining models. It is because models at different scales convey different predictions. A map with a large scale can only show general information with minimal detail, while higher resolution and diverse data are only available at smaller scales. Despite the potential benefits, integrating posterior models from different mining value chain activities is uncommon. This presentation presents the challenges, benefits, and potential solutions for multi-physics and –scale data integration in the minerals value chain.


IG03-A027
Bayesian Model Estimates on the Possible Geographical Origins for Isotopic Data

Jiao LI#+
Northwest University

The official handicraft industry was an important economic section during the Qin Dynasty (221-206 BCE). The records about employees, production management, and product circulation were well documented, while the source of raw materials was relatively obscure. We here conducted isotopic analysis on cattle bones excavated from a Qin Dynasty bone workshop Niejiagou at Xianyang, together with cluster analysis and Bayesian statistical model (LocateR) to permit tentative estimation of the regions of source from craft bones for the first time. Our data showed that cattle (n=57) in the Niejiagou bone workshop had isotopic composition with limited variations, indicating that most animals likely shared similar origins. Specifically, the δ13C (-3.5±0.8‰) of bone showed that C4 crops contributed significantly to the cattle diet, and the δ18O of atmospheric precipitation estimated from the δ18O of bone (-7.7±0.6‰) was slightly lower than that of the present. At the same time, the 87Sr/86Sr values (0.71156±0.00019) of Niejiagou cattle bone are similar to the strontium isotope baseline of river water in the Guanzhong area. Cluster analysis suggested that most animals (n=52) might come from the nearby Guanzhong area, whilst only a few individuals (n=5) were from the north of the Chinese Loess Plateau or the east of the Qinling Mountains. It is worth noting that the strontium isotope in the contemporary Xuechi sacrificial site showed that the cattle and horses were imported afar. The significant differences between the two sites were possibly rooted in the differences in their functions and properties: the sacrificial site was designed to proclaim the territories, while the handicraft sites preferred the uniform quality of products.


IG03-A006
Machine Learning-based Reconstruction of All-sky 1 Km MODIS Land Surface Temperature Considering Cloud Effects

Dongjin CHO1#+, Dukwon BAE1, Cheolhee YOO2, Jungho IM1, Yeonsu LEE3, Siwoo LEE1
1Ulsan National Institute of Science and Technology, 2The Hong Kong Polytechnic University, 3UNIST

A high spatio-temporal resolution land surface temperature (LST) is important for various research fields because it plays a crucial role in the energy exchange between the atmosphere and the ground. The moderate-resolution imaging spectroradiometer (MODIS) LST has been widely used, but it is contaminated by clouds. This study proposed a machine learning-based reconstruction of all-sky MODIS LST in South Korea during the summer seasons, considering the cloud effects on LST. In South Korea, a Local Data Assimilation and Prediction System (LDAPS) with a relatively high spatial resolution of 1.5 km has been operated since 2013. The LDAPS model’s analysis, binary MODIS cloud cover, and auxiliary data were used as input variables, while MODIS LST and cloudy-sky in-situ LST were used as target variables for training light gradient boosting machine (LightGBM) model. When performing spatial five-fold cross-validation using MODIS LST, the proposed model had a coefficient of determination (R2) of 0.89–0.91 with a root mean square error (RMSE) of 1.11–1.39 °C during the daytime, and an R2 of 0.96–0.97 with an RMSE of 0.59–0.60 °C at nighttime. In addition, the reconstructed LST under the cloud was evaluated using leave-one-station-out cross-validation (LOSOCV) using 22 weather stations. From the LOSOCV results under cloudy conditions, the LightGBM model had an R2 of 0.55–0.63 with an RMSE of 2.41–3.00 °C during the daytime, and an R2 of 0.70–0.74 with an RMSE of 1.31–1.36 °C at nighttime. These results indicated that the reconstructed LST had higher accuracy than the LDAPS model. This study also demonstrated that cloud cover information improved the cloudy-sky LST estimation accuracy by adequately reflecting the heterogeneity of the relationship between LST and input variables under clear and cloudy skies. The reconstructed all-sky LST can be used in various research applications.


IG03-A022
The Challenge of Striking a Balance Between Data-intensive and Other Foundational Climate Research Activities - An Early Career Researcher Perspective

Shipra JAIN1#+, Julia MINDLIN2, Gerbrand KOREN3, Carla GULIZIA2, Claudia STEADMAN4, Gaby LANGENDIJK5, Marisol OSMAN6, M. Adnan ABID7, Yuhan RAO8, Valentina RABANAL9
1Centre for Climate Research Singapore, 2Universidad de Buenos Aires, 3Utrecht University, 4The University of Edinburgh, 5Climate Service Center Germany, 6Centro de Investigaciones del Mar y la Atmósfera, 7The Abdus Salam International Centre for Theoretical Physics, 8North Carolina Institute for Climate Studies, 9Servicio Meteorológico Nacional

During the past decades, climate model data has progressively increased in size and is expected to continue to grow in the future. This is leading to a shift towards data-intensive research activities in climate sciences at the expense of other research activities. It is especially affecting the scientific and professional development of Early Career Researchers (ECRs), for which spending time challenging the current understanding of science and critical thinking and analysis is crucial. In this presentation, we will highlight some of the structural challenges currently faced by the ECRs. We highlight an urgent need for a better balance between data-intensive and other foundational climate science activities, more open-ended research opportunities that reinforce the scientific freedom of the ECRs, and strong coordinated action to provide infrastructure and resources to the ECRs working in under-resourced environments. Possible ways to address these challenges are also discussed, such as stronger motivation and arguments to produce more data, increasing support towards ECR-led projects and positions, longer and more stable research opportunities for the ECRs, or having dedicated software engineers and data managers. Through this presentation, we aim to raise awareness and start a community discussion around this topic. This presentation and discussion will also inform our follow-up perspective paper which will include insights and experiences from the wider climate community.


IG03-A024
Estimating Deterministic Causality of Climate System Using Normalized Information Flow as a Measure of Probabilistic Causality

Chin-Hsien CHENG#+, Simon REDFERN
Nanyang Technological University

To understand the interactions among processes of a complex system, such as how climate change influences the biogeochemical sphere through coupled feedbacks, it is important to quantify causal contributions between time series variables. Ideally, we would like to estimate causal contributions deterministically and build a mathematical causal model to describe the processes. We define the causal sensitivity (CS) of such deterministic causality by the ratio of causal contributions to an effect-variable to the change in cause-variable via the deterministic causal model, and define the normalized causal sensitivity |nCS| by normalizing |CS| over the maximal |CS| of the causal model. With a series of empirical verification, we found that deterministic |nCS| can be estimated by probabilistic causality, the normalized information flow, |nIF|, which appears to probabilistically normalize the same causal model through the overall information flow (IF) received by the effect-variable in relation to that from the cause-variable. Thus, for a common causal model with changing coefficients, both |nCS| and |nIF| are comparable among i) causes, ii) at different times and iii) from various locations. We will present the concept behind the proposed |nCS| ~ |nIF| and illustrate its applications via empirical data and actual climate-data.


Fri-04 Aug | 8:15 - 10:00 | MR305
IG09 - Interdisciplinary Research on Coastal Extremes: Advancement in Perspectives, Techniques and Applications

Session Chair(s): Jedrzej MAJEWSKI, Nanyang Technological University, Masashi WATANABE, Nanyang Technological University

IG09-A018
Discrete-continuous Model for the Simulation of Submarine Landslide-induced Tsunamigenesis

Jose Marie Antonio MIÑOZA1#+, Vena Pearl BONGOLAN1, Nigel WINSPEAR2
1University of the Philippines Diliman, 2CATRISX Services Ltd

Submarine landslides, also known as submarine mass failures (SMFs), can be a significant source of hazardous tsunamis. To better understand and model the displacement of these landslides, we propose a coupled discrete-continuous model that combines a diffusion model with a cellular automata model derived from the ultradiscretization of the diffusion equation. The diffusion model, based on fluid flow equations, captures the continuous behavior of the landslide, while the cellular automata model captures the discrete elements of the failure, such as rock fall. By using this model, we can track the change in height of the mass and translate it into force vectors used to solve the shallow water equation for generating tsunami waves. We demonstrate the effectiveness of our model through simulations of the Anak Krakatau tsunami in Indonesia and the potential for landslides in the Northwest Borneo region. Our model provides a valuable tool for understanding and predicting the impacts of submarine landslides on tsunamis, which can be used to identify areas at risk and develop strategies for mitigating potential impacts.


IG09-A008
Application of transfer learning techniques to heterogenous data sets for effectively performing tsunami scenario detection

Reika NOMURA1#+, Yu OTAKE1, Shuji MORIGUCHI1, Shunichi KOSHIMURA1, Randall LEVEQUE2, Kenjiro TERADA1
1Tohoku University, 2University of Washington

Some recent studies suggest that machine learning techniques are promising tools for early prediction of tsunami risks. Since their performances are governed by not only the learning techniques but also by the quality of database, the number of scenarios considered must be sufficiently large. However, the quality of synthetic database is potentially inherent to the used modeling (e.g., numerical simulation scheme, approximation in the discretization, or fault rupture modeling), and thus produces uncertainty in the resultant prediction. Therefore, there must be great demands on effectively accommodating such heterogeneity in the scenario databases consisting of different numerical schemes or modeling techniques in the context of machine learning-based tsunami forecasts. From such a perspective, a class of transfer learning techniques is expected to be effective since it has been established for improving learning process of a targeted database by transferring the important information of another database, which is called the "source domain". Against this background, in this study, we apply the transfer learning methods to the heterogeneous data sets to realize the previous tsunami risk evaluation method, in which the most probable scenario is detected from the database using the Bayesian update and unsupervised learning. To this end, we first set up two different databases, which are created by two different tsunami propagation/inundation simulation tools with the corresponding techniques for generating fault rupture. With these two databases both consisting of over 2000 tsunami scenarios triggered by Nankai Trough, we proceed to the unsupervised learning by proper orthogonal decomposition (POD) where the so-called “frustratingly easy domain adaption” is implemented. Comparing the prediction results based on the learning with (1) simple database summation and with (2) a single database, we then argue the applicability and the possibility of the transfer-learning for the early tsunami forecast.


IG09-A007
Optimization of Offshore Tsunami Gauge Configuration with Robust Principal Component Analysis

Saneiki FUJITA#+, Reika NOMURA, Yu OTAKE, Shunichi KOSHIMURA, Shuji MORIGUCHI, Kenjiro TERADA
Tohoku University

It has been a serious concern in Shikoku area (Japan), which is close to the plate boundary, the tsunami is estimated to attack immediately after the earthquake. Therefore, real-time observation networks play an important role in forecasts and mitigation for coastal communities. Considering the installation/management cost, such systems must be spatially sparse enough to be set up on a nationwide scale. In this study, we present an optimization scheme for the configuration of offshore wave gauges using machine learning and sparse sensing techniques. The present approach uses spatial modes extracted from datasets of pre-computed tsunami wave heights to identify a sparse observation network. Such a limited number of gauges are configured so as to possess super-resolution ability to reconstruct the entire wave field. For that purpose, we employ the robust principal component (RPCA) analysis to extract low-dimensional spatial modes while eliminating high-dimensional components in nearshore areas. In other words, the gauges’ configuration is optimized according to the impact of observation effects only by the low-rank spatial modes that are supposed to dominate the gauges far from the coast. To validate the proposed method, the database of tsunami wave histories is synthetically generated by TUNAMI-N2 simulations for 1564 possible Nankai Trough earthquakes. Then, the optimal observation network off the coast of Shikoku is designed by RPCA techniques. The detected gauges’ configuration is scrutinized by its forecast capability in the previous tsunami scenario detection framework. As a result, a detected sparse optimal configuration, which covers coastal to offshore areas, satisfies the accuracy and speed of tsunami prediction. Although the tsunami forecast demonstration focuses on the Nankai megaquake and the Shikoku coastal area, our framework is applicable to other earthquake scenarios and regions.


IG09-A014
Quantifying the Impact of Shallow Bathymetry Resolution on Coastal Tsunami Modelling

Raquel FELIX1#+, Kaya WILSON2, Adam SWITZER3, Judith HUBBARD3
1NTU, 2AECOM, 3Nanyang Technological University

Using high-resolution bathymetry is preferred at shallow coastal region to havea more accurate model of tsunamis, however, they are often inaccessible. Hence, a globally available dataset with coarser resolution is instead commonly used. We examine how variations in bathymetric resolution, from 5 m to ∼455 m (GEBCO), affect simulated coastal tsunamis. Our case study includes four sites with available 1 m resolution-LiDAR bathymetry. At each site 30 sets of points were randomly extracted from the LiDAR bathymetry and used to generate bathymetric grids with resolutions of 5, 10, 20, 30, 40, 50, 100, 200, and 300 m. These were also compared to bathymetry based purely on the GEBCO dataset for that region (∼455 m resolution). In COMCOT software, we set up a hypothetical fault model and initiated an instantaneous rupture to generate and propagate the tsunami towards the coast. Using the simulation with 5 m resolution bathymetry as the reference model, we observed that 10 – 50 m resolution bathymetries can reproduce wave heights reasonably well, with the maximum wave height overestimated by ≤5% or underestimated by ≤10%. For coarser bathymetric grids, there is an increasing trend of underestimation. Wave heights are underestimated by at least 10% and with up to 30%, 40% and 60% underestimation for bathymetric resolutions of 100, 200, and 300 m, respectively. GEBCO model underestimated coastal tsunami heights by as much as 70%. The tsunami arrival time for 10 – 50 m bathymetry models show that the first wave arrives 10% earlier than expected, while coarser resolutions showed more variability, with the first wave arriving either ≤20% later or ≤10% earlier. Overall, a reasonably accurate result can be achieved using a bathymetric grids with a resolution in the 10 m – 50 m range, and is achievable with reasonable computational efficiency.


IG09-A003
Tsunami Impacts on the Global Port Network: A Case-study on the Manila Trench in Light of Rising Sea Levels

Constance Ting CHUA1#+, Takuro OTAKE1, Masashi WATANABE2, Anawat SUPPASRI1, Fumihiko IMAMURA1, Adam SWITZER2
1Tohoku University, 2Nanyang Technological University

Extreme sea level (ESL) events such as the 2011 Tohoku tsunami and 2021 Typhoon Rai have demonstrated the vulnerabilities of seaports to coastal hazards. The impact of an ESL event on ports can result in considerable economic losses beyond just physical damage. The 2011 Tohoku tsunami resulted in an estimated loss of US$ 3.4 billion in seaborne trade a day in the months following the tsunami. Any port inoperability affects trade flows in and out of the affected port and disrupts shipping routes to it, which then propagates throughout the rest of the maritime network.
The South China Sea (SCS) basin is home to some to some of the world’s busiest ports. Previous studies have shown that the Manila megathrust, which lines the eastern boundaries of the SCS basin, is capable of generating basin-wide tsunami waves. Furthermore, in light of a warming climate, a tsunami compounded with rising sea levels could have greater impacts on coastal infrastructure within the SCS basin. With many major ports concentrated in the region and most of them located in low-lying coastal areas, a tsunami event from the Manila trench could result in detrimental economic consequences beyond the affected port. The objective of this study is to develop an approach to quantify the impacts of tsunami on the global port network through network analyses, using a potential Manila-trench tsunami as a case scenario. This study will also consider the impacts of tsunami on ports under the influence of rising sea levels, based on the scenarios stipulated in the Intergovernmental Panel on Climate Change (IPCC, 2022) AR6 report. The methods applied in this study could potentially be used to quantify the impacts of other coastal hazards such as storm waves and storm surges on the global port network.


IG09-A017
Assessment of the Impact of Human Activities on the Tsunami Risk in a Coastal Lagoon Area in South China

Yilin ZHANG+, Linlin LI#
Sun Yat-sen University

Tsunamis can cause high numbers of casualties, as well as direct and indirect economic losses to coastal regions. While human activities are widely acknowledged to be the primary determinants of coastal disasters such as tsunamis and storm surges, quantitative assessment studies are rare. In this study, we choose a typical coastal county in south China to quantitative evaluate the evolution of its potential tsunami hazard with the influence of human activities since 1950. The study area is located in the east of Wanning City and connected to the northern South China Sea(18°47′~53′N,110°26′~34′E) through the biggest lagoon (Xiaohai) in Hainan Island. Because of the existence of a typical barrier-lagoon-tidal inlet system, this region is potential exposed to more severe tsunami hazard. Moreover, with the rapid economic development and booming population in coastal region, intense human activities put more infrastructures and people under threat. We examine the influence of human activities e.g. land reclamation, population migration on tsunami risk and its temporal changes through numerical modeling approach. The results of the tsunami risk change analysis will help us understand the current tsunami risk and predict the potential risk changes in the future. In addition, it is necessary to prepare tsunami prevention measures in advance and formulate tsunami emergency plans for Xiaohai lagoon and other areas facing potential tsunami threats.


IG09-A004
Recent Decadal Perspective on Sea Level Fluctuations in the Five Ocean Basins

Jonathan CABRERA1,2#+, Han Soo LEE3
1Hiroshima University / Davao Oriental State University, 2Davao Oriental State University, 3Hiroshima University

According to the recent IPCC report, the global sea level is rising at a rate of 3.3 mm/yr in the 21st century due to global warming. However, sea level fluctuations vary significantly across different regions of the globe. In this study, the sea level fluctuation in the five major ocean basins was analyzed using time series observations from 2001 to 2020. Data were obtained from the Permanent Service for Mean Sea Level and analyzed using 1,477 tide gauge stations. The results indicate that the global mean sea level rise (SLR) is 3.70 ± 0.04 mm/yr, slightly higher than the value of the IPCC report. Furthermore, the analysis of ocean basins revealed that SLR (mm/yr) was 3.93 ± 0.02, 3.74 ± 0.01, 0.85 ± 0.02, 2.74 ± 0.01, and 3.30 ± 0.01 in the Arctic, Atlantic, Indian, Pacific, and Southern Ocean, respectively. The Pacific Ocean was further subdivided into three cases: Pacific-Asia, Pacific-America, and Pacific Islands. Results indicated that Pacific Island countries are more susceptible to SLR, with a rate of 3.45 ± 0.01 mm/yr, compared to the other two sub-basins. Additionally, stations from the Mediterranean and the Black Sea were analyzed, with a rate of 2.2 ± 0.01 mm/yr, which is lower than the global mean sea level. The study also focused on the Indian Ocean, finding a rate of 0.3 ± 0.02 (West Australia), 3.4 ± 0.02 (Asian continent), and 4.9 ± 0.01 in the African area. Overall, the results demonstrate that SLR varies based on the ocean basin, highlighting the need for localized studies of sea level variability to identify and implement region-specific countermeasures to prepare, mitigate, and adapt to SLR. To further investigate, understanding the relationship between SLR and meteorological phenomena is highly recommended for successful regional mitigation and adaptation against SLR.


IG09-A024
Area-business Continuity Management User Interface Design for Flood Disasters

Jing TANG1#+, Natt LEELAWAT1, Bhunaron SORNKLIN1, Methasit CHAWEEWONGPAISAL1, Yada VIKRAIPAISARN1, Yanisa BHISITCHAROENTAT1, Penpitcha ARAYACHOOKIAT1, Kunruthai MEECHANG2, Akira KODAKA3, Yuko IWASAKI2, Masahiro INOUE3, Kenji WATANABE2
1Chulalongkorn University, 2Nagoya Institute of Technology, 3Keio University

Flooding is a common natural disaster in many parts of the world, causing damage to human life and property. Many businesses may have to stop operations due to the impact of flooding, such as power outages or damage to machinery. In response, JICA and AHA Center initiated a concept called Area Business Continuity Management (Area-BCM) to enable businesses to continue operating amidst and reduce the impact of a disaster. Recognizing its importance and benefits, Area-BCM website application has been developed to support various stakeholders in the face of disasters. We have conducted surveys to understand the stakeholders and the needs of users. With the interview results, we designed functional requirements and the system’s Unified Modeling Language (UML) functional diagrams. Subsequently, user-centric design concepts were used to implement the high-fidelity prototype to be user-friendly. We also developed the full-stack web application with visualizations of various flood indicators, flood simulations, and business impact analysis.


Fri-04 Aug | 8:15 - 10:00 | MR321
IG05 - Research and Applications from Operational Geostationary Satellites

Session Chair(s):

IG05-A004
GEO-LEO Aerosol Data Fusion Open-source Package

Jennifer WEI1#+, Sally ZHAO2,3, Neil GUTKIN2,4, Xiaohua PAN1, Pawan GUPTA1, Robert LEVY1
1NASA Goddard Space Flight Center, 2NASA Intern, 3University of Maryland, College Park, 4Virgina Tech

The retrieval of aerosol optical depths (AODs) from sun-synchronous polar orbiting satellites, such as MODISs, VIIRSs, OMI, TROPOMI, etc., has been widely adopted as a method for obtaining information regarding particulate matter (PM) and related atmospheric processes. However, the advent of recently launched geostationary satellites, such as GOES-16/17/18, Himawari-8/9, and Meteosat Third Generation (MTG), has led to an increased temporal resolution of AOD observations (order of 10 minutes), resulting in typically one or more images per hour during daylight hours, compared to the once-per-day observations obtained from LEO satellites. By integrating these observations, the diurnal cycle of global AOD can be characterized at local, regional, and global scales. The scientific community is still examining the novel data from geostationary satellite observations and evaluating methods for effectively merging these observations with differing spatial and temporal resolutions. This presents a significant "Big Data" challenge, encompassing not only data storage, but also data discoverability, accessibility, and migration within cloud computing environments. This study presents our attempts at fusing Level 2 aerosol data from six satellites, three of which are geostationary (GOES-16/17 and Himawari-8) and three of which are polar orbiting (TERRA/MODIS, AQUA/MODIS, and SNPP-VIIRS), using the Dark Target aerosol retrieval algorithm. The ability to fuse remote sensing products on demand into desired temporal and spatial domains empowers researchers and practitioners to more efficiently work with satellite and sensor data. It is our hope that through making our open-source package and accompanying functionality available, the scientific community will have improved access to aerosol data processing resources.


IG05-A002
Joint Retrieval of Surface BRDF from Geostationary and Polar-orbiting Satellite Sensors

Weile WANG1#+, Hirofumi HASHIMOTO2, Taejin PARK1, Yujie WANG3, Alexei LYAPUSTIN3, Ian BROSNAN1
1NASA Ames Research Center, 2California State University Monterey Bay, 3NASA Goddard Space Flight Center

The latest geostationary sensors like GOES 16/17 ABI and Himawari 8/9 AHI provide high frequent observations of the Earth surface with continuously changing solar illumination geometries, which allow us to retrieve the surface Bidirectional Reflectance Distribution Function (BRDF) with dedicated atmospheric correction algorithms like MAIAC (Multi-Angle Implementation of Atmospheric Correction). However, because the viewing geometry of a specific location from the geostationary satellites are fixed, the angular sampling of surface BRDF by GEO (Geostationary Earth Orbit) sensors is far from comprehensive. This study tries to address this issue by exploring a GEO-LEO (Low-Earth-Orbit) synergy, in particular, jointly retrieving surface BRDF parameters with concurrent ABI/AHI and VIIRS top-of-atmosphere (TOA) reflectance for the near-infrared (NIR) band. The NIR band is chosen because the ABI, AHI, and VIIRS instruments have very similar spectral response functions in this band and therefore simplifies the requirements for cross-sensor radiometric calibration. We compile ABI/AHI and VIIRS TOA data with the best quality (cloud-free and low aerosol loading) at chosen AERONET sites. We then run the GeoNEX MAIAC algorithm to retrieve the Ross-Thick-Li-Sparse (RTLS) surface BRDF parameters with or without the AEORNET measured atmospheric aerosol optical depth (AOD) as inputs. The joint retrieval results are considered the best estimate of surface BRDF. We compare the joint BRDF retrievals with the corresponding MAIAC BRDF products, retrieved with ABI/AHI or VIIRS separately, to evaluate their differences. We expect that the jointly retrieved BRDF data are more robust than the standard products and may help us reduce uncertainties in higher-level earth observation satellite products.


IG05-A007
Development of Carbon Flux Model Using ABI Data Over the Conterminous US

Hirofumi HASHIMOTO1#+, Weile WANG2, Taejin PARK2, Andrew MICHAELIS2, Ian BROSNAN2
1California State University Monterey Bay, 2NASA Ames Research Center

The satellite-driven carbon flux estimation has been playing important role to estimate continental-scale carbon budget. One of the biggest recent advances in the satellite-driven carbon flux modeling is utilization of high-frequent geostationary satellites to estimate diurnal cycle in carbon fluxes. The satellite based carbon flux estimation used the polar orbiting satellite sensors (e.g., Moderate Resolution Imaging Spectroradiometer (MODIS)), which allow us to observe target regions only once during the day. The new generation of geostationary satellite sensors provide frequent observations, often less than every 10 minutes. Here, we use GOES Advanced Baseline Imager (ABI) data to estimate hourly NEE over the conterminous US. We used the Terrestrial Observation Prediction System (TOPS) model for estimating hourly NEE. TOPS is a diagnostic ecosystem process model that simulates the fluxes of carbon and water through vegetation in response to climate variability. For the climate input, we developed hourly climate data using the same algorithm with NASA Earth Exchange Gridded Daily Meteorology (NEX-GDM) datasets based on machine learning techniques. The hourly climate data includes precipitation, maximum temperature, minimum temperature, dew point temperature, and solar radiation were derived from the Geostationary observations. The spatial patterns of ecosystem parameters used in TOPS are optimized using satellite Solar Induced Fluorescence (SIF) data. The high frequency GPP estimations from geostationary satellite sensors make it comparable to the instantaneous SIF data than daily GPP. We also used Ameriflux data for optimization of model parameters and the validation of the output. The derived data addresses the diurnal dynamics of carbon cycling at large scales and should help in reducing the uncertainties in carbon budget studies.


Fri-04 Aug | 10:20 - 12:20 | MR305
IG09 - Interdisciplinary Research on Coastal Extremes: Advancement in Perspectives, Techniques and Applications

Session Chair(s): Constance Ting CHUA, Tohoku University, Masashi WATANABE, Nanyang Technological University, Jedrzej MAJEWSKI, Nanyang Technological University

IG09-A005 | Invited
Comparing Modern and Historical Records of Cyclone Induced Coastal Flooding Using Lessons from Northwest Australia and the Central Philippines

Adam SWITZER1#+, Joseph CHRISTENSEN2, Janneli Lea SORIA3
1Nanyang Technological University, 2University of Western Australia, 3Institute of Environmental Science and Meteorology, University of the Philippines-Diliman, Quezon City

To date most natural hazard risk assessments in Australasia do not incorporate long-term and/or prehistoric records of extreme events and coastal development continues to rely on short historical records as a reflection of the long-term behaviour of a hazard. In some locations historical records may be appropriate as consistent records have been kept that span several centuries or more. However, for much of the Asia-Pacific this is rare as the historical archives rarely stretch beyond World War II. Clearly such short records are inadequate for determining the natural variability of a hazard at multi-decadal timescales and for the extrapolation of extreme events. While it is well known that the historical record is fragmentary, incomplete and limited in spatial balance, the historical record does provide a key link between instrumental datasets and the prehistoric record that allows for the detailed reconstruction of past events. Here, we compare known historical tropical cyclone events to recent ones in Western Australia (UC1921 and cyclone Herbie) and the central Philippines (Typhoon Haiyan and Ty1897) as examples of integrated studies. These two examples demonstrate the utility of the integrated approach and allow an examination of the similarities and differences between the events.


IG09-A001
Novel Sampling of Karst Pockets for Tsunami Sediments on Limestone Coasts of Malta, Central Mediterranean

James TERRY1#+, Derek MOTTERSHEAD 2, Piero BELLANOVA3, Margret MATHES-SCHMIDT3, Lisa FEIST3, Aaron MICALLEF 4
1Zayed University, 2University of Portsmouth, 3RWTH Aachen University, 4University of Malta

The Mediterranean Sea is known to have experienced large tsunamis in the past. However, the pattern of timing, frequency and magnitudes of these events, and the relative importance of possible tsunamigenic mechanisms (undersea earthquakes, volcanic eruptions, major landslides) are not well understood. In this respect, the Maltese archipelago is uniquely situated for tsunami research in the Mediterranean domain, since the small islands are exposed to waves approaching from any direction. Previous studies on Malta seeking sedimentary evidence of Holocene palaeotsunamis have tended to focus on the hydrodynamic characteristics of large coastal boulders. This study takes an innovative approach. In the Aħrax area on the northernmost peninsula of island Malta, we examined solution hollows (‘karst pockets’) that pockmark exposed limestone terrain at elevations of 10-12 m asl. Within the pockets are deposited shelly marine sands. Lined by insoluble terra rossa soils, the pockets act as excellent repositories from which accumulated sands are not easily removed by subsequent aeolian action or overland flow. This presentation describes the sampling methods, some challenges, and early results of laboratory analysis. Preliminary findings show the moderately-sorted sands contain a rich microfossil assemblage of mostly benthic species, comprising foraminifera, gastropods, echinoidea, serpulidae and bryozoa. Strongly altered forms occur alongside well-preserved forms. Altered forms are both reworked bioliths from the Miocene bedrocks and Holocene specimens that were broken by wave action or aeolian transport near the coast. Sediment stratigraphy within the karst pockets suggests a single depositional episode, while the site elevations of 10-12 m are beyond the reach of storm waves and thereby indicate the minimum inundation run-up of the tsunami event responsible.


IG09-A019
Sediment Analysis of the 2018 Palu-Donggala Tsunami Deposit, Indonesia

Jedrzej MAJEWSKI1#+, Adam SWITZER1, Rachel GUAN1, Benazir BENAZIR2, Ella MEILIANDA3, Peter PARHAM1,4, Robert WEISS5, Stacey MARTIN6, Lillian PEARSON7, Jessica PILARCZYK8, Benjamin HORTON1,9
1Nanyang Technological University, 2Universitas Syiah Kuala, 3Tsunami and Disaster Mitigation Research Center, 4Universiti Kebangsaan Malaysia, 5Virginia Tech, 6Australian National University (ANU), 7The University of Southern Mississippi, 8Simon Fraser University, 9Rutgers University

Preparing for tsunami impacts on coastlines requires a comprehensive understanding of their sedimentary characteristics. However, the sedimentary characteristics of tsunamis generated by landslides are poorly understood. In 2018 the Mw 7.5 Palu- Donggala earthquake occurred on the Palu-Koro fault in Indonesia. The shaking generated multiple landslides which in turn generated a tsunami that impacted the coastlines surrounding Palu Bay, Indonesia.
Following the Palu-Donggala tsunami, we conducted a post-event field survey and analysed the sedimentary characteristics of the tsunami deposit along three transects in Palu Bay, two in Palu City and one 20 km north in Pantoloan. The transects spanned the entire extent of the sediment deposited by the tsunami inundation. We analysed the tsunami deposit at 1 cm intervals to compare sediment thickness, grainsize, skewness, and sorting. We also surveyed boulders carried by the tsunami up to 125 m inland at Pantoloan. Collectively, the sediment and boulder data were used in the TSUFLIND and the boulder transport models, respectively, to model the flow velocity and depth of the tsunami wave that created the deposits. The tsunami deposit was massive with weak fining upwards sequence. The deposit was thickest near the coast at 8 cm, and thins landwards. The sediments also fine landwards from course sands close to the sea to medium and fine sands further inland. The deposit tends to be poorly sorted and coarse skewed. The modelled flow depths range between 1 to 8 m, flow velocities range between 1.5 and nearly 6 m/s. The highest flow depths and velocities were modelled for the Pantoloan transect, which also had the most complete sediment coverage. These results will inform future efforts to prepare development on coastlines prone to landslide tsunamis.


IG09-A022
The April 2022 Cascading Tropical Cyclone-landslide-tsunami Disaster in Pilar, Abuyog, Leyte Island, Central Philippines

Likha MINIMO1#+, Janneli Lea SORIA2, Alfredo Mahar LAGMAY1,3, Angelu BERMAS4, Kayla Milcah MARASIGAN4, Jannine VASQUEZ4, Adrian Gelo TIANCHON4, Richard YBANEZ4, Audrei Anne YBAÑEZ4, Victor ROMERO II5, Allan Fritzgerald AMISTOSO5, Genaro CUARESMA4, Christer Kim GERONA5
1University of the Philippines Diliman, 2Institute of Environmental Science and Meteorology, University of the Philippines-Diliman, Quezon City, 3University of the Philippines, 4University of the Philippines Resilience Institute, 5University of the Philippines Visayas Tacloban College

On April 12, 2022, videos of the first recorded landslide-induced tsunami in the Philippines spread on social media. These showed debris flowing over what was Barangay Pilar in Leyte Island, central Philippines where intense rainfall was sustained due to Tropical Storm Megi (Agaton). This event left 54 people dead, 49 injured and 33 missing in Pilar. We reconstructed the timeline and described the mechanism of this cascading disaster from multiple datasets: social media, news, incident reports, accounts of survivors and rescuers, satellite images, drone survey, field mapping, and 3D modelling. Results show that the residents pre-emptively evacuated days prior, but many returned to the village to replenish supplies hours before then Tropical Depression Megi weakened into a Low-Pressure Area. Approximately 5.2 x 10⁵ m³ of volcaniclastic deposits slumped from the fault-cut ridge south of the village and was transported downstream by at least two distinct debris flow events. Not recorded on the videos was the first debris flow that buried half the area of the village. Its impact into the sea generated a tsunami that smashed through the rest of Pilar and reached neighbouring villages. Interviews and field investigation consistently indicate that the first and apparently larger tsunami obliterated structures along the coast of Pilar and drowned people trying to escape the landslide. Search and rescue teams arrived but had to narrowly escape the succeeding debris-flow and tsunami. The debris field and wrack lines indicate tsunami runup heights from 5 m to as high as ~12 m above mean sea level. This disaster convinced the government officials and residents to finally relocate the village. Equally important is to adjust disaster risk reduction plans to consider cascading hazards like landslide-tsunami scenarios.


IG09-A010
Investigating the Risk of Tropical Cyclone Induced Storm Surges Around the Coast in Singapore Using a Step-wise Scenario Based Approach

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. It was generally believed that tropical cyclones are unlikely to form near the equator because the Coriolis effect is minimal. However, on 27 December 2001, a tropical cyclone - Typhoon Vamei formed to the southeast of Singapore, which demonstrates that there is a potential localised risk of cyclone induced storm surges in Singapore. This risk could be potentially amplified in a warming climate, where typhoon intensity is likely to increase and sea levels are expected to rise. In this study, we investigated the risk of the storm surge around Singapore based on numerical simulations at highest astronomical tide. We used Delft-3D/SWAN to calculate both the potential storm surge and waves induced by typhoons. Typhoon Vamei has been classified as a Category 1 tropical cyclone. Its maximum central pressure and maximum 10-minute sustained wind velocity were 1006 hPa and 85 km/h, respectively. Using a parametric hurricane model, we created air pressure and wind fields of the typhoon Vamei as an input condition of our simulation. We then investigate the risk of storm surge around Singapore coasts by varying intensities, typhoon paths and initial water levels. Our results show that a direct strike from a Category 2 cyclone at highest astronomical tide would result in a maximum storm surge of 0.68 m with the highest values occurring on south east coast.


IG09-A012
A Novel Way of Assessing Storm Surge Multi-scenarios Based on Ensemble Tropical Cyclone Forecast

Md Rezuanul ISLAM#+, Le DUC, Yohei SAWADA
The University of Tokyo

Ensemble forecast is a promising tool to help robust decision-making against the risk of coastal storm surges. Although many operational weather prediction systems adopt tropical cyclone (TC) ensemble forecasts, the potential of ensemble disaster prediction has yet to be fully investigated. Here, we present a novel and efficient way to maximize the potential of an extremely large ensemble (=1000 members), performing scenario-based storm surge analysis and discuss its’ implication for robust decision-making. This research involved simulating the TC Hagibis (2019) using the Japan Meteorological Agency's (JMA) non-hydrostatic model. Later, we utilized ensemble atmospheric prediction as inputs to a statistical surge model, which is recently developed under a framework of the Storm Surge Hazard Potential Index (SSHPI) and estimated the peak surge height along the central coast of Japan where Hagibis made landfall. The SSHPI fairly reproduced peak surge heights that were observed both in the inner bay locations and open coasts. We show that identifying Pareto-optimized solutions from ensemble storm surge forecasts can reasonably describe potential worst (maximum) and optimum (minimum) storm surge scenarios while exemplifying a diversity of trade-off surge outcomes among coastal places. For example, some of the Pareto-optimized solutions that illustrate worst surge scenarios for inner bay locations are not necessarily accountable for bringing severe surge cases along open coasts. We further emphasize that a comprehensive analysis of Pareto members’ meteorological variables including track, wind intensity, and size of TC can provide useful insights to the forecasters and decision makers on effective decision-making (e.g., evacuation planning, issuing surge warning).


Fri-04 Aug | 10:20 - 12:20 | MR321
IG15 - Radar Techniques and Applications to Atmosphere and Ocean

Session Chair(s): Guozhu LI, Chinese Academy of Sciences, Zhen-Xiong YOU, China Medical University

IG15-A003 | Invited
The Spatial Features of E Region Irregularities Revealed by All-sky Radar

Wenjie SUN#+
Chinese Academy of Sciences

All-sky radar measurements provide a unique capability to resolve the spatial structure of E region irregularities over a large zonal region. With the all-sky radar interferometry observations at Ledong (18.4°N, 109.0°E) in Hainan, China, the spatial structure and zonal drift of low latitude E region irregularities over a large region are investigated. It is revealed that the E region irregularities, including both the continuous and quasi-periodic (QP) types shown in radar range-time-intensity maps, occurred most frequently in summer. The continuous type was observed being generated locally without obvious zonal drift. The QP type generally covered ~40-500 km zonally, and consisted of up to 9 (peaking at 3-4) irregularity patches separated by ~20-130 km (peaking at ~60 km). The spatially separated irregularity patches predominantly drifted westward at the speed ~50-200 m/s. Gravity waves were surmised to be a major source for causing the spatially separated structures of low latitude QP type E region irregularities. Further, a unique case of wavelike structure of E region irregularities elongating more than 200 km zonally were observed, providing concrete evidence for the gravity wave modulating mechanism for their generation.


IG15-A001
Radar Observations of Daytime F Region Irregularity

Haiyong XIE1#+, Guozhu LI2, Xiukuan ZHAO2, Lianhuan HU2, Wenjie SUN2, Yi LI2, Baiqi NING2
1Institute of Geology and Geophysics, Chinese Academy of Sciences, 2Chinese Academy of Sciences

Ionospheric F-region irregularity backscatter plumes are commonly regarded as a nighttime phenomenon at equatorial and low latitudes. At daytime, there are very few reported cases of F-region backscatter echoes. It is still not clear what caused the daytime echoes. Using the low latitude Sanya VHF radar (18.4°N, 109.6°E, dip lat. 12.8°N) with a peak power of 24 kW and an operational frequency of 47.5 MHz, special experiment designed for daytime F-region echoes was conducted. The statistical results show that the daytime F-region echoing structures had an unexpected high occurrence ~13% in June solstice of solar minimum. They could appear at any time during 0700 – 1800 LT, with a maximum occurrence around 0900 LT. Radar interferometry revealed that these daytime echoes were from plume structures consisting of field-aligned irregularities. The radar multi-beam range-time-intensity maps show that the irregularities appeared mostly above 350 km altitude, extending up to 650 km or more with apparent westward drifts at times. For the origin of daytime F region irregularities, there could be several possibilities. One is that the plume structures could be remnants of equatorial plasma bubble (EPB) irregularities generated on the previous night which could survive unexpectedly long time and drift together with background plasma. On the other hand, radar observations released that they also could be newly generated near dawn during a geomagnetic storm. Another possibility is that they could be generated artificially, such as triggered by rocket-induced ionospheric hole.


IG15-A005 | Invited
A Comparative Study of the Es Layers Observed by FMICW HF Surface Wave Radar and Ionosonde

Yen-Hsyang CHU#+
National Central University

It has long been aware that the sea echoes of HF Surface Wave Radar (HFSWR) employed for the ocean wave monitoring are prone to be contaminated with the clutters reflected by ionospheric layers or scattered by electron density irregularities, which would degrade quality of the sea echoes and pose a difficulty in processing radar return for ocean wave and current observations. Nevertheless, the ionospheric clutters observed by HFSWR have potential to provide useful information for ionospheric monitoring. In this paper, on the basis of the radar returns of the HFSWR located at Pengjiayu (25°37’46”N, 122°04’17”E), which is a frequency modulation interrupted continuous wave (FMICW) radar, we develop a method to identify and extract ionospheric clutters from the radar returns. After correcting the range aliasing effect on the ionospheric clutters, we find that the Es layers observed by Pengjiayu FMICW radar are very consistent with those observed by Chung-Li ionosonde (24.97°N, 121.19°E). In addition, ionospheric plasma irregularities detected by the former are also compared with those by the latter. The differences in the two are presented and discussed as well.


IG15-A004
Identification and Tracking of Vessels Based on Range-azimuth Radar Imaging of Linear-arrayed Coastal Radar

Zhen-Xiong YOU1#+, Duy-Toan DAO2, Hwa CHIEN3
1China Medical University, 2Hanoi University of Civil Engineering, 3National Central University

Linear-arrayed coastal radars have been used for decades in measurement of oceanic surface parameters such as sea current, wave height, surface wind field, and so on. Such kind of coastal radar is also capable of detecting the vessels on the sea surface, giving the positions, tracks, and moving velocities of vessels. The latter is the topic of this study. Different from the treatment of vessel echoes on range-Doppler map that is commonly used in vessel detection, however, identification and tracking of vessels in this study are based on the range-azimuth map of echo intensity that are retrieved from an adaptive beamforming algorithm, i.e., norm constrained-directionally constrained minimization of power (NC-DCMP) method. To suppress the sea echoes and retain the vessel echoes for beamforming process, a selected bandstop filter is employed to filter out most of sea echoes around the first-order Doppler spectral line, and the filtering is carried out in time domain. As a result of beamforming at various azimuth directions, the vessel echoes can emerge on the 2D range-azimuth map when the vessel echoes are stronger than those around. After that, a location process based on the contours of the retrieved range-azimuth echo intensity is developed to locate the echo centers, which are possibly the vessel locations. Finally, a tracking process is applied to the echo centers determined from the successive range-azimuth maps to track the vessels as far as possible. The vessel tracks are verified with the Automatic Identification System (AIS) tracks to demonstrate the usability of the methods and processes employed in the study.


IG15-A007
Application of Coastal-based X-band Marine Radar to Nearshore Eddies

Mingyi CHEN#+, Hwa CHIEN, Haoyuan ZHENG
National Central University

This study sets out to develop hardware and software improvements for coastal X-band marine radar. In terms of hardware, we have modified the overall hardware structure, using USRP (Universal Software Radio Peripheral) structure and FPGA (Field Programmable Gate Array) firmware to realize the ability to simultaneously complete radar signal A/D and PPI image disassembly. For the software part, we developed an algorithm to retrieve wave, current and bathymetric information from the PPI images. By observing and analyzing the speed and direction of waves propagating in shallow water, and then applying the wave dispersion theory to invert the ocean currents and topographic features in the near-shore area. Eddy currents play an important role in the nearshore mixing of salinity, sediment and pollutants, and have an impact on fishery resources, pollution diffusion speed, etc. Rapid changes in topographic water depth are one of the factors that cause dangerous phenomena such as rip currents, which pose a threat to people's safety when conducting marine industries and recreational activities. Coastal X-band radar has the advantages of near real-time and large-scale continuous observation of nearshore sea states. It enables continuous monitoring and research of those phenomena. This study focuses on the dynamic mechanism of the generation and dissipation of nearshore eddies, discusses them using the X-band radar retrieval results of nearshore currents, and compares them with wave buoy observation data and model fields.


Fri-04 Aug | 1:10 - 3:10 | MR321
IG14 - Land Subsidence: Measurement, Mitigation and Adaptation

Session Chair(s):

IG14-A001
Geometrical and Physical Measurements for Detecting and Mitigating Land Subsidence in Taiwan

Cheinway HWANG#+
National Yang Ming Chiao Tung University

Land subsidence can be measured using sensors installed in space, on the ground surface, and sub-surface. Typical space-borne sensors are interferometric synthetic aperture radar (InSAR) and Global Navigation Satellite System (GNSS). Mature ground-based subsidence-detecting devices are precision levels and magnetic-based sensors deployed at multiple depths in a borehole. These measurements are geometrical and solely for detecting the magnitudes of land subsidence. Such measurements may be fed to hydrogeological models for predicting land subsidence and for guiding groundwater-use policies. As groundwater over-pumping is the leading cause of land subsidence, there is a need to quantify the change in groundwater mass associated with groundwater use. Unlike groundwater wells, space-based and ground-based gravimetry can provide physical measurements for quantifying regional groundwater mass changes at ~300 km and ~1 km scales, respectively. This presentation will use the geometrical measurements in Yunlin and Pingtung County, Taiwan, to show how land subsidence is detected, and use the physical (gravity) measurements to show how such measurements can be used for aiding the mitigation of land subsidence.


IG14-A006
Assessment of the Schemes to Mitigate Land Subsidence in South Beijing Plain, China

Shujun YE1#+, Binhao YOU1, Fang TIAN2, Yong LUO2
1Nanjing University, 2Beijing Institute of Hydrogeology and Engineering Geology

Land subsidence (LS) has become a worldwide geological disaster, which affects social security, regional economy, environmental and ecological coordination and sustainable development. China is one of the most serious countries suffering LS disaster. North China Plain (NCP) is one of the most serious LS areas, and LS in the Beijing-Tianjin-Hebei region is most serious in NCP. At present, the area with moderate to strong developed LS in Beijing has reached 55% of the Beijing plain area, which makes the mitigation of LS in Beijing, as the capital, urgent. The study area includes Daxing District of Beijing City and parts of Langfang and Gu 'an cities of Hebei Province, total of 1392km2, which is the south LS area of Beijing Plain. The land subsidence model including three-dimensional groundwater flow model and one-dimensional subsidence model is developed, which is calibrated and verified with the observation data of water levels and displacements of the aquifer system from 2008 to 2018. Four mitigation schemes, corresponding to four different ground water resources management schemes, are assessed by using the LS model to predict the LS development in the next 12 years (2019-2030). The results show that without any groundwater control (Scheme 1), the LS will continue to develop and the average LS rate will be 24 mm/a in 2030. Under different groundwater control conditions (Schemes 2, 3 and 4), such as groundwater reduction and ecological water replenishment, LS can be controlled to different extents. Scheme 4, using south water to replace the groundwater for living and industrial usage, implementing water saving agriculture, reducing 37% groundwater exploitation, and naturally recharging 0.77 million m3/a water by the Yongding River, could effectively decrease average LS rate to 8 mm/a.


IG14-A003
The Sudden Occurrence of a Sinkhole in Puebla Mexico and the Methods of Study

José Jorge CARACHEO GONZÁLEZ1#+, Pedro Francicsco RODRIGUEZ ESPINOSA1, Estefanía MARTÍNEZ TAVERA2, Karen Mineli OCHOA GUERRERO1
1Instituto Politécnico Nacional, 2Universidad Popular Autónoma del Estado de Puebla

In this study, the physical parameters of the soil, the grain size, and the plastic and liquid limits are obtained. From a geotechnical and civil engineering standpoint, soils are a three-phased compound, made of water, solids, and air (voids). The voids calculation helps to sustain the theory of collapse due to the loose conditions of the soil getting these calculations helps to support the theory of the occurrence of the sinkhole in an anomalous environment. The sudden occurrence of a sinkhole in a non-karstic environment in Puebla, Mexico, ended up swallowing an entire house and affecting the economical agriculture-related activities performed in the zone by the inhabitants due to the loss of arable land. Studying these events may give us the opportunity of understanding why and how they occur and how can they be prevented. Sinkholes are geomorphological structures that involve the interaction between water and the strata of a determined region, by definition, sinkholes are a depression or a hole that appears on the ground due to the collapse of the surface layers, usually, sinkholes tend to occur on karstic terrains (CaCO3) or on evaporites (Na, CaSO4), nevertheless, these events can occur suddenly swallowing anything located over them. For this reason, sinkholes represent a threat to the population located on karstic terrains and in fine-grained soils where underground water is strongly used for agricultural purposes.


IG14-A004
Time to Think More Effectively About Monitoring Land Subsidence

Wei-Chia HUNG1#+, Cheinway HWANG2, Yi-An CHEN3, Shao-Hung LIN1, Pei-Ching TSAI4
1Green Environment Engineering Consultant Co. Ltd, 2National Yang Ming Chiao Tung University, 3National Central University, 4National Cheng Kung University

Nineteen percent of the global population may face a high probability of land subsidence. Evidence mounts that climate change is rapidly affecting subsidence. How to effectively monitor land subsidence has become a major issue in the world. In this paper, we introduce a multiple-sensor monitoring system for land subsidence in central Taiwan, including 50 continuous operation reference stations (CORS), multi-temporal InSAR (MT-InSAR), a 1000-km leveling network, 34 multi-layer compaction monitoring wells, 2 automatic record extensometers, and 116 groundwater monitoring wells. This system can monitor the areal extent of land subsidence and provide data for studying the mechanism of land subsidence. We develop new low-cost high-performance GNSS equipment and automatic multi-layer compaction monitoring equipment to monitor land subsidence. We also use the Internet of Things (IoT) technology to control and manage the sensors and develop a big data processing procedure to analyze the data from the system of sensors. The procedure makes land subsidence monitoring more efficient and intelligent.


IG14-A005
Displacement Mapping of Joshimath, India Using Conventional DInSAR and LiCSBAS Techniques

Yalamanchili SUBRAHMANYESWARA RAO#+, Shubhayan ROY CHOWDHURY
Indian Institute of Technology Bombay

The Joshimath town of Northern India is situated on the Himalayan terrain with slopes exceeding 60 to 70 degrees. Due to the sliding of Joshimath over the time and significant movement in January 2023, several buildings and roads have developed cracks, and about 120 families are relocated. ISRO, NRSC is the first to report the results using Sentinel-1 SAR data publicly. Later, the researchers from Greece and Strasbourg Universities processed Sentinel-1 data through ESA Network of Resources and reported their preliminary findings through a blog. We also processed Sentinel-1 SAR data of ascending and descending passed for time series displacement analysis with conventional Differential SAR Interferometry (DInSAR) using free software such as ESA-SNAP. Also used the Persistent Scatterer InSAR technique (LiCSBAS) for time series displacement mapping. We first used yearly data (2018-19, 2019-20, 2020-21, 2021-22 and 2022-23) of the same season with two data sets using conventional DInSAR so that maximum coherence between the two dates can be observed. The average displacement map observed over the Joshmath is -40 cm/y, -5 cm/y, -12 cm/y, -14 cm/y and -1.2 cm/y, respectively. Due to a one-year gap between the two acquisitions, phase unwrapping problems and atmospheric changes are seen clearly. That is why, a significant displacement is observed wrongly in 2018-19. Using GACOS tropospheric correction method, we observed atmospheric phase delay. The maximum coherence was observed when we took 12-day interval data (Dec. 27, 2022 and Jan. 8, 2023). The displacement for 12-day period is demarcated, with varying from -4 to -7 cm. LiCSBAS time series displacement is also observed with and without atmospheric correction using GACOS data. When we take a shorter duration (i.e. 2020 to 2022), we get better results than with a more extended period, i.e., 2018-2022.


IG14-A007
Space Geodesy in Coastal Resilience

Xie HU#+, Xiao YU
Peking University

Coastal land is the most vulnerable continental regions amid climate change and sea-level rise (SLR), which may lead to hazardous consequences such as floods/inundation, saltwater intrusion, and ecological disturbance. Coastal areas at an altitude less than two meters above the mean sea level are the most vulnerable terrain to SLR. About 267 million population were in high risk (situation in 2020). Coastal areas were usually built on reclaimed land surface subject to land subsidence, which may amplify the relative vertical land motion to the sea level. When the rates of land subsidence and sea-level rise are comparable, land subsidence can hasten coastal inundation by about half of the time span on the scale of hundreds of years given the present-day rates of sea-level rise. Synthetic Aperture Radar (SAR) imagery has been widely used to map the land deformation and surface changes associated with natural hazards and land alterations. Here we present two case studies about land subsidence in coastal environment. A condominium in Surfside, Florida collapsed catastrophically and claimed 98 lives on 24 June 2021. We use time-series Interferometric SAR (InSAR) analysis to detect any precursors of land motion prior the building collapse. We further investigate the relative vertical land motion and predict when the Miami beach will be engulfed by the seawater. The critical port city Tianjin in China has been in trouble with groundwater extraction and the consequent land subsidence since the early 1900s. The government launched the South-to-North Water Diversion project in 2003 to alleviate water shortage in Northern China including Tianjin. We retrieve the ground deformation history using time-series InSAR analysis to assess the effectiveness of multi-decadal, mega-engineering project in groundwater recovery. Our study demonstrates the importance of space geodesy in coastal resilience.



Ocean Sciences


Mon-31 Jul | 8:15 - 10:00 | MR306
OS11 - Influence of Natural and Human Activities on Coastal Environment Risk

Session Chair(s):

OS11-A008
Estuary Hypoxia Expansion Caused by Human Activities: Case Study of the Pearl River Estuary

Yue NAN#+, Jia-Tang HU
Sun Yat-sen University

The Pearl River Estuary (PRE) has undergone rapid urbanization in recent decades and has become an estuary strongly influenced by human activities, resulting in the deterioration of the estuary DO levels and expansion of low-oxygen area. To explore the inner causes of low-oxygen and hypoxia expansion, the research used observed data to analyze the changes of nutrient (DIN and DIP) levels, suspended sediment concentration (SSC) and dissolved oxygen (DO) levels in the PRE from 1990 to 2017, and simulated the distribution of hypoxia in two typical stages (low-nutrient high-suspended-sediment stage (1991-1996) and high-nutrient low-suspended-sediment stage (2013-2017)) using a three-dimensional water quality model. The results showed that there was an obvious expansion of low-oxygen and hypoxia area in the PRE. Compared with nutrient increase, declining (SSC) brought more hypoxic expansion by increasing light in the water column. DO concentration in the upper reach was mainly affected by the input of low-oxygen freshwater and terrestrial POC. In the lower reach of the PRE, the expansion of hypoxia was dominated by the growth of marine-sourced matters brought by the changes of nutrient and SSC, accounted for more than 50%. The study projected the development of hypoxia in the PRE over the next decade based on recent measures, and the results showed that hypoxic condition would improve but still occur. Considering the numerous changes that exist in the future, hypoxia mitigation in the PRE will be more difficult.


OS11-A003
Landsat Satellite Observations of the Impacts of Hong Kong International Airport on Water Quality from 1986 to 2022

Zhengyi WANG1+, Zhihua MAO2#, Longwei ZHANG3, Xianliang ZHANG2, Dapeng YUAN4, Youzhi LI5, Zhongqiang WU6
1Shanghai JiaoTong University, 2Second Institute of Oceanography, 3Zhejiang University, 4Southern Marine Science and Engineering Guangdong Laboratory (Guangzhou), 5Nanjing University, 6Hainan Normal University

Hong Kong international Airport (HKIA) is an important sea airdrome in China. We evaluated the impacts of this reclamation to the Northwestern Bay of Hong Kong (NWBHK). The constructions of HKIA are divided into three stages: stage 1: construction of HKIA's first and second runways from 1992 to 1995; stage 2: the construction of the Hong Kong Port from 2013 to 2016; stage 3: construction of the HKIA's third runway from 2017 to 2020. 117 landsat-5 TM and 45 landsat-8 OLI images were used to match the marine water data of 18 in-situ monitoring points, acquiring 458 and 119 sets of data. The suspended particulate matter, orthophosphate-phosphorus and dissolved inorganic nitrogen have been retrieved based on the BPNN algorithms. By analyzing the temporal variations and spatial distributions, we found that: (1) During the construction period of HKIA, the construction activities would cause the rise of SPM, PO4P and DIN concentrations of water; (2) The injection of Tung Chung River was intercepted by HKIA and the impact of Tung Chung River on NWBHK decreased, while the impact of Tuen Mun River on NWBHK increased; (3) The interception impact of HKIA to the transportation of pearl river became stronger.


OS11-A005
Bait Input Altered Microbial Community Structure and Increased Greenhouse Gases Production in Coastal Wetland Sediment

Genmei LIN1#+, Xianbiao LIN2
1Sun Yat-sen University, 2Ocean University of China

Coastal wetland reclamation contributed to development of aquaculture industry, and the residual bait accumulation in aquaculture processes could threaten ecological functions and services in aquaculture and adjacent ecosystems. In this study, A 90-day incubation experiment was conducted using sediment collected from coastal wetland in Qi'ao Island in southern China, followed by the observations of temporal variations of physicochemical properties, sediment microbial community, and greenhouse gasses (GHGs) production in response to different amounts of bait input (0, 20, and 40 mg bait g−1 wet sediment). The results showed that dissolved oxygen of overlying water was profoundly decreased owing to bait input, while dissolved organic carbon of overlying water and several sediment properties (e.g., organic matter, sulfide, and ammonium) varied in reverse patterns. Meanwhile, bait input led to significant loss of microbial community richness and diversity, and strongly altered microbial compositions from aerobic, slow-growing, and oligotrophic to anaerobic, fast-growing, and copiotrophic. Moreover, both GHGs production and global warming potential were significantly enhanced by bait input. The increment cumulative CO2e production from the increased aquaculture area (4.25×103 km2) with medially and heavily bait input accounted for approximately 0.01% and 0.02%, respectively, of the global GHGs fluxes (4.94×1010 t CO2e in 2016), despite only covering approximately 0.0008% of the earth's surface area (5.1 × 108 km2). These results indicated that the aquaculture ecosystem is an important hotspot for global GHGs emission. Overall, bait input triggered quick responses of physicochemical properties, sediment microbial community, and GHGs production, followed by long-term resilience of the ecosystem. This study could provide new insight into temporal interactive effects of bait input in coastal zones, which can enhance the understanding of the temporal dynamics and ecological impacts of coastal aquaculture activities and emphasize the necessity of sustainable assessment and management in aquaculture ecosystems.


OS11-A006
InSAR-derived Surface Deformation of Chaoshan Plain, China: Exploring the Role of Human Activities in the Evolution of Coastal Landscapes

Zhaoquan HUANG1+, Fengling YU2#
1Xiamen University, 2Xiamen University, China

Understanding the characteristics of different human-induced coastal surface deformation will improve our understanding of recent temporal-spatial evolution trends of the coastal terrain, and help better predict the risks of coastal disasters. However, few surface deformation studies have focused on the distinction between different types of anthropogenic ground deformation. Based on Sentinel-1 SAR data, this study employs the multi-temporal InSAR method to extract the surface deformation of Chaoshan Plain from 2015 to 2020, with a spatial resolution of 30 m × 30 m. A series of historical optical satellite images and groundwater extraction data are used to help distinguish different types of human activities that have induced surface deformation. Results show that InSAR ground deformation in the study area is mainly caused by three types of human activities: groundwater extraction, land reclamation, and construction. Groundwater extraction has impacted >50% of the regional surface deformation by area. The interannual variability of the surface deformation rate corresponds well to that of groundwater extraction, and the subsidence effect can last for more than five years with seasonal variability. The maximum surface subsidence rate in land reclamation areas reaches ~100 mm/year, with a linear decreasing trend against time. Without extra compaction, the reclamation area can continue to deform almost at the same rate for several years. The rapid increase of overlying loads caused by construction in the reclamation area has led to a sharp decrease in the deformation rate within 2–3 years after the completion of the construction. In areas absent of other human-induced deformation, construction activities are shown to cause surface subsidence of 10–20 mm/year in a relatively short period. In areas experiencing a combination of construction and groundwater extraction, land subsidence rates of >50 mm/year are observed. 


OS11-A009
Sediment Dynamics and Transport Under the Effect of Moderate Gale on the Intertidal Beach, Hangzhou Bay

Lingpeng MENG+, Daidu FAN#, Junbiao TU
Tongji University

Tidal beaches represent a series of coastal types in transition from wave-dominated beaches to tide-dominated tidal flats, and both tides and waves control their sediment dynamics by modulating each other. This paper analyzes the intertidal beach sediment dynamic and transport characteristics under the influence of moderate gale, based on continuous observations obtained in Lingang Beach, Hangzhou Bay. The results show that the short-term strong wind events obviously enhance the currents and waves, producing apparent tidal velocity asymmetry. The strong current and wave exert more significant bed shear stress on the bed, reducing the time when the total bed shear stress is less than the critical shear stress, then the high concentration of suspended sediment mainly come from the sediment resuspension. In addition, the directions and durations of strong wind are equally crucial for net sediment transport. The alongshore sediment transport flux under strong wind conditions is enhanced significantly, and the current asymmetry generating net flooding-direction sediment transport. Besides, it is significantly correlate with the relative wave height, but the cross-shore sediment transport does not correlate. Under weak wind conditions, the bed shear stress is low, and the high suspended sediment concentration mainly from the sediment settling. The settling-lag leads to the onshore sediment transport, which makes the intertidal zone suffering from strong wave-current erosion recover rapidly. This paper highlights the importance of the modulation of tides and waves for tidal beaches, the wave-current interaction under variable wind conditions makes the sediment dynamical processes of tidal beaches show distinctive characteristics.


OS11-A002
A General Unit Hydrograph Theory for Tidal Wave Propagation and Residual Water Level Distribution in Estuaries

Huayang CAI#+
Sun Yat-sen University

Understanding the tidal river dynamics in terms of longitudinal tidal range and residual water level in river deltas or estuaries is essential for water resources management since it directly influences the flood control, salt intrusion, delta evolution, wetland conservation etc. Numerous approaches (including harmonic tidal analysis, nonparametric regression techniques, analytical solutions and numerical models) have been adopted to quantify the nonlinear interactions between river discharge and tidal waves (including storm surges); however, the general dynamics of tidal range and residual water level on the tidally-averaged scale are still insufficiently understood owing to the highly nonstationary river discharge influence. In this study, we propose a simple, general, and analytical model on the basis of Guo’s general unit hydrograph (GUH) theory to describe the tidal wave propagation and residual water level distribution along the estuary axis. The flexibility of the proposed GUH model was assessed by applying it to the Yangtze River estuary with substantial river discharge impacts on tidal hydrodynamics, where we observe a surprisingly good agreement with measured tidal ranges and residual water levels. The model can be used to analytically identify the critical position corresponding to the maximum tidal damping upstream of which tidal damping is reduced landward, and the critical river discharge beyond which the tidal damping is reduced with increasing river discharge. Finally, the potential impacts of human interventions on tidal river dynamics were quantified making use of calibrated parameters of the GUH model before and after the Three Gorges Dam’s operation, which demonstrates that the proposed model can be a useful tool for assessing human-induced and natural changes.


Mon-31 Jul | 8:15 - 10:00 | MR309
OS01 - Tropical Cyclone-ocean Interactions: from Weather to Climate

Session Chair(s): Il-Ju MOON, Jeju National University, Lei ZHOU, Shanghai Jiao Tong University

OS01-A024
Air-sea Interaction Observed by Uncrewed Surface Vehicle Saildrones in Hurricanes

Dongxiao ZHANG1,2#+
1University of Washington, 2NOAA Pacific Marine Environmental Laboratory

Surface air-sea fluxes play an important role in the development and maintenance of tropical cyclones (TCs). However, even outside of the TC environment, air-sea flux observations are challenging, requiring a suite of atmospheric and oceanic variables to be measured concurrently in the air-sea interaction zone. The lack of continuous high-quality surface measurements in TCs has limited our understanding and the prediction skill of TC intensification. Uncrewed Surface Vehicle (USV) saildrones have demonstrated their ability to observe multiscale and multi-process air-sea interactions in the tropical Pacific and Atlantic since 2017, providing concurrent measurements of surface fluxes and near-surface atmospheric and oceanic properties, including currents and waves (significant wave height and dominant period). During the 2021 Hurricane season, 5 USV saildrones intercepted 5 TCs (4 tropical storms and Category 4 Hurricane Sam). The data were sent in real time to GTS. Saildrones coordinated with other subsurface and airborne observations in the area. One saildrone measured ocean surface heat release of up to 1200 W/m2 and 14 m wave height near the eyewall of Hurricane Sam. Seven saildrones were deployed for the 2022 Hurricane Mission in the Gulf of Mexico, Caribbean Sea, the western tropical and subtropical North Atlantic, which began on August 1. We will present results from these 2021-2022 deployments, including a newly added capability to determine the 2-D directional wave spectrum using the high frequency measurements by the Inertial Measurement Unit (IMU) in the saildrone hull. The bulk and direct covariance air-sea fluxes will be compared in different conditions of surface currents, wind waves and swells. This analysis demonstrates the importance of collecting concurrent measurements of surface fluxes, currents, and waves to better understand and monitor TC air-sea interaction.


OS01-A013
A Novel Mechanism for Extreme El Niño Events: Interactions Between Tropical Cyclones in the Western North Pacific and Sea Surface Warming in the Eastern Tropical Pacific

Xin WANG1#+, Bo TONG2, Dongxiao WANG3, Wen ZHOU2
1Chinese Academy of Sciences, 2Fudan University, 3Sun Yat-sen University

This study presents a novel mechanism for the generation of extreme El Niño events by analyzing interactions between tropical cyclones (TCs) in the western North Pacific (WNP) in spring (March–April–May, MAM) and summer (June–July–August, JJA) and sea surface warming in the eastern tropical Pacific. It is suggested that anomalously strong TCs in the WNP in MAM and JJA are essential for the formation of extreme El Niño events. MAM TCs excite considerable westerly wind bursts (WWBs) and facilitate the generation of El Niño events in late spring. The sea surface temperature (SST) in the central-eastern tropical Pacific increases prominently during the following summer, which is due to the warm water carried by downwelling Kelvin waves induced by the anomalous westerlies in the western tropical Pacific associated with the WNP TCs, as well as the lessening cold water upwelling resulting from the deepening thermocline in the eastern tropical Pacific. The developing El Niño in turn contributes to the TC activities over the southeastern quadrant of the WNP in summer, characterized by a stronger intensity, higher frequency, and longer duration. The resulting JJA TC-induced westerlies could further enhance the eastern tropical Pacific warm SST anomalies, and thus an extreme El Niño event tends to appear in the following autumn and winter. These physical processes are verified by several sets of atmosphere–ocean coupled model experiments.


OS01-A008
Unexpected Limitation of Tropical Cyclone Genesis by Subsurface Tropical Central-north Pacific During El Niño

Cong GAO1+, Lei ZHOU1#, Chunzai WANG2, I-I LIN3, Raghu MURTUGUDDE4
1Shanghai Jiao Tong University, 2Chinese Academy of Sciences, 3National Taiwan University, 4University of Maryland

The genesis of tropical cyclones (TCs) requires energy from the warm ocean as one of the necessary conditions, although the full dynamics controlling the TC frequency remain a persistent mystery. It has been proposed that the easterly trade winds tend to weaken due to the reduction of the zonal sea surface temperature (SST) gradient, favoring an El Niño-like pattern in the tropical Pacific. Therefore, an examination on the contrasts in TC genesis between El Niño and La Niña, the two phases of El Niño-Southern Oscillation, is an analog to advance our understandings of TC genesis under global warming. During El Niño, the western Pacific warm pool extends eastward. However, the number of TCs does not increase significantly with the expanding warm pool and it remains comparable between El Niño and La Niña. Here, we show that the subsurface heat content change counteracts the favorable SSTs in the tropical central-north Pacific. Due to the anomalous positive wind stress curl, the 26 °C isotherm shoals during El Niño over this region and the heat content diminishes in the tropical central-north Pacific, even though warm SST anomalies prevail. This negative correlation between SST and 26 °C isotherm depth anomalies is opposite to the positive correlation in the tropical eastern and western Pacific. This is critical because quantifying the dynamics of the subsurface ocean provides insight into TC genesis. The trend in TC genesis continues to be debated. Future projections must account for the net effect of the surface-subsurface dynamics on TCs, especially given the expected El Niño-like pattern over the tropical Pacific under global warming.


OS01-A016
Multiphase Physics of the Air-sea Interface in Rapid Intensification and Decay of Tropical Cyclones

Alexander SOLOVIEV1#+, Breanna VANDERPLOW1, Roger LUKAS2, Brian HAUS3, Isaac GINIS4
1Nova Southeastern University, 2University of Hawaii, 3University of Miami, 4University of Rhode Island

Under tropical cyclones, microphysics of the air-sea interface is an essential factor in mass, momentum, and enthalpy exchange (Sroka and Emanuel 2022). The sea surface is covered with a two-phase environment (whitecaps, whiteout, etc.). Whitecaps including a mixture of bubbles and spray cover ~4% of the sea surface; and the whiteout occupies the rest of the surface (Holthuijsen et al. 2012). Soloviev et al. (2017) hypothesized that whiteout is a product of the Kelvin-Helmholtz type instability (KH) at the air-sea interface above 33-35 m/s wind. KH at the air-sea interface is stable on average (Miles 1959) but unstable to wind fluctuations (Farrell and Ioannou 2008). KH develops within tens of milliseconds - it is an effective mechanism for the disruption of the air-sea interface between whitecaps. The suppression of short surface waves by KH reduces the sea surface roughness, making it “slippery”, forming an aerodynamic drag well (ADW) that may explain the RI and rapid decay (RD) of tropical cyclones. Using the multiphase model VOF-to-DPM (Vanderplow et al. 2020) verified at UM SUSTAN, Kyoto facility, and field gas exchange data (Krall et al. 2019, McNeil and D’Asaro 2007), we have estimated the contribution of sea spray in the ADW. The sea spray generation function obtained with the VOF-to-DPM (Soloviev et al. 2023) indicated that in major tropical cyclones, spume can increase the drag coefficient Cd thus controlling the ADW on the high wind-speed side. Remarkably, the multiyear dataset of dropsonde measurements in tropical cyclones reanalyzed by Richter et al. (2021) reveals the ADW within the 35-65 m/s wind speed range. The perceived importance of Ck/Cd (Emanuel 1995, Lee et al. 2022) for the tropical cyclone intensity, RI, and RD calls for investigating the potential effect of microphysics on the enthalpy coefficient Ck.


OS01-A001
Modulation of Upper Ocean Vertical Temperature Structure and Heat Content by a Fast-moving Tropical Cyclone

Han ZHANG#+
Second Institute of Oceanography, Ministry of Natural Resources

The ocean temperature response to tropical cyclones (TCs) is important for TC development, local air-sea interactions and the global air-sea heat budget and transport. The modulation of the upper ocean vertical temperature structure after a fast-moving TC was studied at the observation stations in the northern South China Sea, including TC Kalmaegi (2014), Rammasun (2014), Sarika (2016) and Haima (2016). The upper ocean temperature and heat response to the TCs mainly depended on the combined effect of mixing and vertical advection. Mixing cooled the sea surface and warmed the subsurface, while upwelling (downwelling) reduced (increased) the subsurface warm anomaly and cooled (warmed) the deeper ocean. An ideal parameterization that depends on only the nondimensional mixing depth (HE), nondimensional transition layer thickness (HT) and upwelling depth (HU) were able to roughly reproduce sea surface temperature (SST) and upper ocean heat change. After TCs, the subsurface heat anomalies moved into the deeper ocean. The air-sea surface heat flux contributed little to the upper ocean temperature anomaly during the TC forcing stage and did not recover the surface ocean back to pre-TC conditions more than one and a half months after the TC. This work shows how upper ocean temperature and heat content varies by a TC, indicating that TC-induced mixing modulates the warm surface water into the subsurface, and TC-induced advection further modulates the warm water into the deeper ocean and influences the ocean heat budget. This work has been accepted by Journal of Physical Oceanography, doi: https://doi.org/10.1175/JPO-D-22-0132.1.


OS01-A011
Off-equatorial Wave Energy Source for the Atlantic Niño Events Identified by Wave Energy Flux

Qingyang SONG1#+, Youmin TANG2
1Hohai University, 2University of Northern British Columbia

In the tropical Atlantic Ocean, extreme climate events with anomalous sea surface temperature, current, and precipitations are often referred to as the Atlantic Niño. It has many similarities with the EI Niño including the analogous mechanism that winds above the western equatorial ocean will excite oceanic waves to amply the temperature anomaly in the east. However, the Atlantic Niño presents more diversity in its intensity and occurrence time, especially in recent years, eg. 2019 and 2021, in which the classic theory becomes insufficient to explain. This study focuses on ocean responses to atmospheric forcing, manipulating the wind forcing in both equatorial and off-equatorial regions to excite linear ocean models for three types of events that occurred in 1999, 2019, and 2021 respectively. This study has found those extraordinary Atlantic Niños may owe to the wind in the off-equatorial region, where the winds can also excite oceanic waves that transfer energy to the western boundary and reflect back to the equatorial Atlantic. The interaction between the energy from the equatorial and the off-equatorial region makes the event less predictable. The participation of off-equatorial wave energy leads to the diversity of the Atlantic Niños. Hence, for the Atlantic Niño forecast, more concerns about ocean dynamics to cover a wider latitude range should be required.


Mon-31 Jul | 8:15 - 10:00 | MR310
OS06 - Coastal Hazards: Impacts of Tropical Storms and Tsunamis

Session Chair(s): Nobuhito MORI, Kyoto University

OS06-A067
Study on Prediction Method of Storm Surge Using Long Short-term Memory Neural Networks

Tomohiro YASUDA1#+, Hayato NAKATANI1, Yuji ARAKI2, Ryoya TOMODA1
1Kansai University, 2Pacific Consultants Co., Ltd.

Since using numerical simulation models for real-time storm surge forecasting is computationally expensive, machine learning can be a solution for the cost reduction. This study uses a Long Short-Term Memory Neural Network (LSTM), which is suitable for time series forecasting in machine learning methods, to perform storm surge prediction. However, the actual number of storm surge observations is limited, and it is difficult to construct an LSTM based on observation data only. Thus, this study uses stochastic typhoon datasets for 25000 years by Nakajo et al., 2014. The storm surge simulation using a nonlinear shallow water model SuWAT (Kim et al., 2007) is conducted for top 300 intense typhoons which passed Ise Bay, Japan. This allows us to generate a sufficient amount of data for LSTM construction. The accuracy of the LSTMs is compared by test dataset, and the usefulness of the LSTMs is examined by predicting the storm surge anomaly of Typhoon Vera, which caused severe inundation damage in 1959.The training data are pressure (P), east-west wind speed (U), north-south wind speed (V) at 14 weather stations around Ise Bay, and time series of calculated storm surge at the Port of Nagoya. Test data which is 30% of dataset was used for validation and selection of the number of hidden layers (NHL). The 600 of NHL showed best performance with correlation coefficient of 0.81 and RMSE 0.19 m. LSTM was applied for the Typhoon Vera, and LSTM could predict the timing and trend of rising tide but underestimate the peak water level. Another LSTM was constructed with selected training data around peak time and applied for Vera, it was able to fairly predict peak storm surge level but overestimate timing of rising tide.


OS06-A003
Modeling the Storm Surge of the Northern East China Sea to Different Types of Extratropical Cyclones

Dongxue MO1#+, Po HU2
1Institute of Oceanology, Chinese Academy of Sciences, 2Chinese Academy of Sciences

Sea level response to extratropical cyclones, one of the most disastrous weather systems, varies depending on cyclone types and tracks. This study presents a systematic modeling assessment of storm surge induced by extratropical cyclones in the northern East China Sea using an ocean-wave coupled model, based on the Coupled Ocean-Atmosphere-Wave-Sediment Transport (COAWST) model system. We identified the type of extratropical cyclone most likely to cause disasters and the areas likely to suffer the worst effects. We conducted sensitivity experiments to analyze the driving mechanisms (such as wind, air pressure, tide, and wave) and influencing mechanisms (such as local and remote meteorological effect and Ekman effect) of storm surge. During strong winds, positive and negative storm surges were consistent with the wind direction, and formed source of coastal trapped waves. When an abnormally high water level occurred in a semi-enclosed sea area, it propagated mainly along the cyclone direction. The energy of coastal trapped waves was easy to dissipate in case of caps and other locations with large topographic changes. Tide-surge-wave interaction and propagation were also greatly affected by coastal trapped waves.


OS06-A043
Validation of Long-term Historical Sea Levels Using Reanalysis and Best Track TC Data

Shohei OHATA1#+, Tomoya SHIMURA1, William PRINGLE2, Takuya MIYASHITA1, Andrew KENNEDY3, Joannes WESTERINK3, Nobuhito MORI1
1Kyoto University, 2Argonne National Laboratory, 3University of Notre Dame

It is essential to estimate extreme sea levels for planning coastal protection. Reanalysis is often used for simulating long-term sea levels. However, resolutions of the reanalysis are generally not enough to capture tropical cyclones' actual wind and pressure. In this study, we simulated storm surges in the northwestern pacific using wind and pressure from best tracks as input and compared sea levels with reanalysis-driven storm surges. We also validated the effect of using fine meshes in particular areas of interest. The result is helpful for better long-term estimation of extreme sea levels.


OS06-A017
Flood Simulation Under Compound Flooding Condition in the Yagyu River, Japan

Kazuki HARUYAMA1#+, Masaya TOYODA1, Shigeru KATO1, Nobuki FUKUI2
1Toyohashi University of Technology, 2Tottori University

There is a growing risk of compound disasters occurring with recent climate change. In Japan, the risk of combined flooding is particularly high when typhoons strike. Thus, coastal regions should be considered the impact both storm surges and river discharge on river water level. Especially in small and medium-sized rivers, the time between starting rainfall and the rising river water levels is short. Therefore, it tends to superimpose the storm surge and high river discharge at the estuary. In this study, the assessments of compound flooding was conducted for the estuary of the Yagyu River that is a small and medium-sized river flowing into Mikawa Bay in Japan. There is the urban area in downstream sector of the Yagyu River, damaged by historical typhoon event (e.g. Typhoon Vera, Typhoon Melor). The analysis was performed based on observation of storm surge caused by Melor (3.64 m at the Yagyu River estuary) and planned high-water discharge (350 m3/s). The inundation area was analyzed using the iRIC, a two-dimensional flood flow analysis software. As a result, the water level rosed at the point where the river channel shape was narrow pass and overtopping occurred. Inundation occurred from both banks of the river, with a maximum inundation area of approximately 191 ha. The results also showed that the river water level at the estuary reached the embankment height (4.5 m) before the respective peaks under the simultaneous occurrence of storm surges and river discharge. It is suggested that even if the magnitude of storm surge and river discharge are within the planning scale, compound flooding may occur in the case of their superimposition.


OS06-A036 | Invited
Applicability of the Maximum Storm Surge Prediction Model for Extreme Typhoon Event

Junbeom JO1, Sooyoul KIM2#+, Jung Soo KIM3, Nobuhito MORI1
1Kyoto University, 2Kumamoto University, 3University of Bucheon

Typhoon-caused storm surges are a significant factor that aggravates flood damage in coastal cities, where river flow is increased due to torrential rain and the drainage capacity of sewer systems is reduced. Therefore, it is essential to estimate the maximum storm surge height with accuracy in order to predict urban flooding in coastal areas. Storm surge height can be predicted using a method simulated by a numerical model and an empirical formula derived from various data. However, appropriate typhoons, topographical data, and long-term calculation time are required in the case of numerical simulation experiments, whereas the empirical formula has the advantage of being able to calculate in a short period of time with a small number of data. Empirical formulas have been developed based on past typhoon events. Therefore, it is not suitable for predicting the maximum storm surge height of the future, considering the impact of climate change. To overcome these limitations, a series of numerical simulation experiments in shallow simplified bathymetry were conducted in this study. The bathymetry consisted of a coastline of 200 km and a uniform bottom slope of 1/30, and a typhoon scenario passing through the center of the coastline was selected. As parameters of a typhoon, central pressure (950~1000 hPa), maximum wind speed radius (40~80 km), typhoon incident angle (±70°), and typhoon moving speed (20~80 km/h) were selected. The simulated results were used in a multiple regression analysis to develop a prediction model for the maximum storm surge height. The model was validated by comparing the results of typhoon reproduction simulations with the observed storm surge height generated by TC202211 at the southern coastline of Jeju Island, Korea. As a result, it is demonstrated that the model can predict the storm surge height more accurately.


OS06-A072
Long-term Assessment of Relative Sea Level Variability Considering Tectonic Deformations, Sea-level Rise, Storm Surge and Ocean Waves: The Case Study of Chilean Coast

Francisco MOLTENI-PEREZ#+, Nobuhito MORI, Tomoya SHIMURA, Takuya MIYASHITA
Kyoto University

Chile is one of the most seismic countries worldwide, with approximately 86.000 km of coastline and a permanent need for development and management. Because of the Nazca plate subducting the South American plate, coastal evolution is modeled by oceanographic variables and plate tectonics. Coastal towns are under permanent tsunami and storm risks, unregulated real estate development, and climate-driven sea-level rise (SLR). IPCC AR6 SSP5-8.5 scenario summarized future trends in Global Mean Sea-Level Rise (GMSL) of ~0.1 m in the near term (2021-2040), ~0.2 m in the medium term (2041-2060), and ~0.6 m in the long term (2081-2100) along the coast. However, relative sea level is affected by large coseismic uplift and/or subsidence which may be comparable to or larger than SLR (Montecino et al., 2017). Using satellite and tidal gauge data, a comparison between the GMSL and relative mean sea level (RMSL) was conducted along the Chilean coast between 1993 and 2020 (Figure 1). By Merging satellite altimetry and tide gauge measurements (Cazenave et al.,1999) vertical land motions (VLM) rates at the tide gauge positions were obtained. Earthquake displacements were obtained from measurements along the coast and InSAR works. A combination of RMSL, coseismic displacements, and GMSL projections under the SSP5-8.5 scenario was conducted to estimate possible changes in the RMSL. Oceanographic agents interacting with VLM were analyzed. Storm Surge, Waves, and Wave Run up were calculated from JR-55 Reanalysis data. Impacts, trends, and their variability were analyzed to understand the vertical changes affection. As conclusion, RMSL strongly varies while the GMSL maintains similar values along the Chilean coast. VLMs were obtained to compare crustal surface motion rates with those projected by SLR. Earthquakes coseismics displacements can affect various locations with different orders of magnitude and directions (uplift/Subsidence).


OS06-A039
A Comparative Study and Coastal Engineering Application of SCHISM and Delft3D: South-east Asia Regional Model

Chun Hin Adrian LAI#+, Jie HU, Kuifeng ZHAO, Yaodong ZHANG
Surbana Jurong Private Limited

The projected sea level rise and increase in extreme events resulting from climate change have led to more focused studies of coastal adaptation measures recently. For coastal engineering designs, it is important to have accurate and efficient hydrodynamics circulation and waves models to derive the necessary design parameters, of which the effects of tide, storm surge, and waves must be accounted for. In this study, we compared two well established hydrodynamics circulation models SCHISM and Deltares’ Delft3D with a focus in tide and surge heights using a South-East Asia Regional model. The predictions of both models are generally in good agreement with the observations of tidal gauges in the region. The modelled typhoon storm surge and submarine earthquake tsunamic are also compared. While both models can be used in a regional model setup, a unique feature and advantage of the SCHISM model is that its formulation is designed for seamless simulation across the coastal-estuary-shelf-ocean scales. We found that the computation time required of SCHISM is not much sacrificed when the mesh size is further refined towards the coastline of the site of interest, whereas in other models the computation time can be significantly increased. This circumvented the need to setup a local model with boundary conditions extracted from the regional model as is typically done in coastal engineering consultancy. However, Deflt3D is also well established as a general and validated modelling suite which can simulate other important aspects such as morphology and water quality, and will continue to stand as one of key tools in coastal engineering consultancy.


Mon-31 Jul | 8:15 - 10:00 | MR327
OS02 - Mixing Matters

Session Chair(s): Zhenhua XU, IOCAS

OS02-A001 | Invited
A Simple Approach for Disentangling Vortical and Wavy Motions of Oceanic Flows

Zhiyu LIU1#+, Chuanyin WANG2, Hongyang LIN1
1Xiamen University, 2Southern Marine Science and Engineering Guangdong Laboratory (Zhuhai)

A long-standing challenge in dynamical oceanography is to distinguish nonlinearly intermingled dynamical regimes of oceanic flows. Conventional approaches focus on time-scale or space-scale decomposition. Here, we pursue a dynamics-based decomposition, where a mean flow is introduced to extend the classic theory of wavy and vortical modes. Mainly based on relative magnitudes of the relative vorticity and the modified horizontal divergence in spectral space, the full flow is decomposed into wavy and vortical motions. The proposed approach proves simple and efficient, and can be used particularly for online disentangling vortical and wavy motions of the simulated flows by ever-popular tide-resolving high-resolution numerical models. This dynamical approach, combined with conventional time-scale- or space-scale-based approaches, paves the way for online mixing parameterizations using model simulated vortical (for isopycnal mixing) and wavy (for diapycnal mixing) motions, and for understanding of multi-regime and multi-scale interactions of oceanic flows.


OS02-A002
Energy Conversion Rate from Subinertial Surface Tides to Internal Tides

Yuki TANAKA#+
Fukui Prefectural University

Subinertial, topographically trapped diurnal internal tides are an important energy source for turbulent mixing in the subarctic oceans. However, their generation may not be estimated by the conventional barotropic-to-baroclinic conversion because their vertical structure is sometimes barotropic unlike superinertial internal tides that are always baroclinic. Here, a new energy diagram is presented, in which the barotropic mode is decomposed into the surface and topographic modes, with the latter being classified as part of the internal modes together with the baroclinic mode. The energy equation for the newly defined topographic mode is then derived, providing an appropriate formulation of the energy conversion rate from the subinertial surface tides to the topographically trapped internal tides. A series of numerical experiments confirm that the formulation successfully predicts the energy conversion rate for various cases, with the relative contribution of the baroclinic and topographic modes varying significantly depending on the bottom topography and stratification. Furthermore, this surface-to-internal conversion is demonstrated to give a significantly larger estimate than the barotropic-to-baroclinic conversion for subinertial tides. Applying the formulation to the results of a realistic numerical simulation in the Kuril Straits, an area with the strongest mixing due to subinertial diurnal tides, shows that the surface mode is converted into the baroclinic and topographic modes with comparable magnitudes, responsible for most of the energy dissipation in this area. These results indicate the need to re-estimate the global distribution of the generation rate of the subinertial internal tides using our new formulation and to clarify their dissipation mechanisms.


OS02-A008
Energy Transfer from Near-inertial to High-frequency Internal Waves

Wei YANG1#+, Hao WEI1, Liang ZHAO2
1Tianjin University, 2Tianjin University of Science and Technology

The near-inertial and near-buoyancy motions, which are the low and high ends of internal waves, both represent important modes of ocean variability. The near-inertial inertial waves (NIWs) and high-frequency internal waves (HFIWs) have many different properties. For example, the low-vertical-mode HFIWs can travel in all directions and long distances in the ocean with their dispersive effects balanced by nonlinear effects, while the NIWs are more likely to dissipate locally. The investigation of energy transfer between NIWs and HFIWs can, therefore, facilitate the understanding of wave energy redistribution and spatial distribution of diapycnal mixing in the ocean. Here, the energy pathway from NIWs to HFIWs is examined based on measurements obtained at the East China Sea shelf slope. We reveal that after the occurrence of parametric subharmonic instability (PSI) which is able to cascade energy from large-scale internal tides to smaller-scale subharmonic waves (which is near-inertial), energy can be further transferred from the PSI-generated subharmonic waves to HFIWs through nonlinear interactions between them. This interprets the observed similar varying trends of magnitude between internal waves at near-inertial and high-frequency bands. Bispectrum and bicoherence estimates confirm that the M1 subharmonic wave interacts with a pair of HFIW which have larger vertical scales and a broad range of frequencies. The averaged net value of the energy transfer rate reaches 2 10-7 W kg−1, which has implications for a further significant role of this energy pathway on the spatial distribution of ocean mixing.


OS02-A016
A Clustering Approach to Investigate Non Homogeneous Ocean Mixing

Alessandro STOCCHINO1#+, Daniele LAGOMARSINO2, Annalisa DE LEO2, Andrea CUCCO 3
1The Hong Kong Polytechnic University, 2University of Genova, 3National Research Council

Mixing and stirring water masses is a complex phenomenon strongly influenced by the local character of the circulations. The ability of a flow to mix and transport mass is linked to specific flow features such as large or meso-scale vortices, tidal currents that generate complex periodic currents in coastal areas. Recent contributions focus the attention on the role of long living macro-vortices on the dispersion analyzing the process in terms of dispersion tensor, see Ryzhov, E. A., & Berloff, P. (2022). Journal of Fluid Mechanics, 939, among many others. At the same time, there is a high interest in describing the typical time scales in terms of Lagrangian integral time and spinning time (Lumpkin, R. (2016) Jgr, 121(2)). In the present study, using the results of one year numerical simulation in a coastal area, we propose a new methodology to analyze the non-homogeneous character of the dispersion processes. Starting from tow dimensional depth-averaged Eulerian flow fields, we compute Lagrangian numerical particles and the corresponding auto-correlation functions. In order to distinguish areas with differential mixing properties, in terms of absolute dispersion, we employ a clustering techniques based on K-means algorithm. The target functions used for the clustering were the auto-correlation functions. After a training of the algorithms and a sensitivity analysis varying several parameters, we have conducted the analysis choosing an optimal number of clusters. The results suggest that coupling a clustering method to Lagrangian functions strictly linked to the dispersion processes is an efficient methodology to describe the non-homogeneous character of the absolute dispersion. Moreover, we suggest a modified model to describe in the same framework auto-correlation functions linked to looping and non-looping trajectories, extending the well-known model of Veneziani et al (2004) Journal of physical oceanography, 34(8).


OS02-A004
Enhanced Mixing in the Eddy Core Explains the Inverse SST Signature of Mesoscale Anticyclones

Alexandre STEGNER1,2#+, Alexandre BARBONI3,1, Evangelos MOSCHOS2, Solange COADOU3,1
1Ecole Polytechnique, 2AMPHITRITE, 3Institut Pierre-Simon Laplace

Mesoscale eddies are tracked through satellite altimetry but they are known to have a marked surface temperature signature, usually warm for anticyclone and cold for cyclones. Recent regional studies challenged this view and showed the importance of warm-core cyclones and cold-core anticyclones, called 'inverse' surface temperature. This study shows, in the Mediterranean Sea, that the emergence of cold-core anticyclones is a seasonal phenomenon. We use remote sensing observations and in situ data to analyse the eddy-induced SST anomaly over a 3-year period (2016–2018). We find that 70% of eddy anomalies are inverse in May and June both for cyclones and anticyclones. In order to understand the underlying dynamical processes, we performed idealized numerical simulations, using the high-resolution model CROCO. We investigate the dynamical response of a mesoscale anticyclone to realistic 1h-frequency atmospheric forcing. We found that the transition from a warm core anticyclone to inverse (cold core) surface signature is triggered by an enhanced vertical mixing in the upper layers inside the eddy core. This differential mixing is induced by the high frequency atmopsheric forcing. Ocean-atmosphere fluxes retroaction to SST are also explored and allow to better retrieve eddy-induced mixed layer depth anomalies.


OS02-A014
The Role of Diurnal Forcings on the Merging of Surface and Bottom Boundary Layers in the Coastal Ocean and Implications for Vertical Mixing

Bicheng CHEN1#+, Jiahao HUANG1, Qing LI2
1Xiamen University, 2The Hong Kong University of Science and Technology (Guangzhou)

The turbulent flow in shallow-water coastal regions controls substance mixing and exchanges within these regions. These mixing mechanisms get highly involved in processes such as air-sea exchanges, diapycnal transport, and sediment resuspension in the coastal ocean, which are key focuses of the marine environment and climate change. Oceanic boundary layers in coastal regions are driven by diurnal external forces such as wind, waves, tides, and currents, resulting in a highly complex dynamical system. Previous studies have mainly focused on either wind-wave-driven surface boundary layer (SBL) or tide-current-driven bottom boundary layer (BBL) in the ocean. Recent studies have shown that the SBL and BBL in shallow water can have strong interactions and merge into one layer. However, the physical mechanisms of such a process have not been revealed. In this study, we use the large eddy simulation (LES) to investigate the evolution of SBL and BBL in the coastal area and the merging processes. The results show LES reproduces high-fidelity turbulent flow within the coastal ocean, directly resolving interactions between SBL-BBL as well as the vertical mixing processes. The relation between the merging and the diurnal external forcings is characterized, and three regimes of SBL-BBL mixing are identified.


OS02-A003
Critical Latitude and Mixing Dependencies on Relative Vorticity

Robin ROBERTSON1#+, Tianyu ZHOU2
1Xiamen University Malaysia, 2University of Delaware

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 the impacts on the mixing and internal waves 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. A relation was developed to translate the critical latitude shift with the amount of additional relative vorticity.


Mon-31 Jul | 10:20 - 12:20 | MR306
OS07 - Ocean Salinity Variability and Its Impact on Weather, Climate and Biogeochemistry

Session Chair(s): Hailong LIU, Shanghai Jiao Tong University, SungHyun NAM, Seoul National University

OS07-A014 | Invited
Global Ocean Salinity Products Have Some Serious Issues After 2015

Chao LIU1, Xinfeng LIANG1#+, Rui M. PONTE2, Don CHAMBERS3
1University of Delaware, 2Atmospheric and Environmental Research, Inc., 3University of South Florida

Salinity is a fundamental ocean variable and essential for understanding changes in the ocean and climate systems. Various gridded ocean salinity products, which since the 2000s are largely based on Argo measurements, have been created and widely used for ocean and climate-related studies. However, after 2015 there has been a significant discrepancy between satellite-based and Argo-based salinity estimates. Here, we examine the salinity variability over 2005-2019 and provide a thorough assessment of abnormality and consistency in the gridded salinity products. We found that most Argo-based data products show an unprecedented and unrealistic increase after 2015, and disagreements between those products have also greatly increased. Over 2015-2019, the average rate of salinity increase in the upper 2000 m global ocean ranges from 4.0±0.9×10-4 g/kg/yr to 13.7±1.8×10-4 g/kg/yr for most data products, which is more than an order larger than satellite-based observations on sea level and mass changes. The temporal and spatial structure of the disagreements are also obtained, and the inconsistency is particularly apparent in the southern hemisphere between 700-2000 m. The significant discrepancies could be attributed to instrumental problems and different quality control processes between research groups. These issues should be an urging concern for the ocean and climate community.


OS07-A002
Ocean Salinity Indices of Interannual Modes in the Tropical Pacific

Jianwei CHI1#+, Tangdong QU2, Yan DU1, Jifeng QI1, Ping SHI1
1Chinese Academy of Sciences, 2University of California, Los Angeles

This study investigates the interannual modes of the tropical Pacific using salinity from observations, ocean reanalysis output and CMIP6 products. Here we propose two indices of sea surface salinity (SSS), a monopole mode and a dipole mode, to identify the El Niño—South Oscillation (ENSO) and its diversity, respectively. The monopole mode is primarily controlled by atmospheric forcing, namely, the enhanced precipitation that induces negative SSS anomalies across nearly the entire tropical Pacific. The dipole mode is mainly forced by oceanic dynamics, with zonal current transporting fresh water from the western fresh pool into the western-central and salty water from the subtropics into the eastern tropical Pacific. Under a global warming condition, an increase in the monopole and dipole mode variance indicates an increase in both the central and eastern Pacific El Niño variability. The increase in central Pacific El Niño variability is largely due to enhanced vertical stratification during global warming in the upper layer, with intensified zonal advection. An eastern Pacific El Niño-like warming pattern contributes to the increase in eastern Pacific El Niño, with enhanced precipitation over the central-eastern tropical Pacific.


OS07-A005
Minimum Warming in the South Indian Ocean Thermocline in a Warming Climate Linked to Freshening Processes

Yu HONG#+
Chinese Academy of Sciences

The Southern Ocean (SO) is one of the key regions in absorbing and storing anthropogenic heat. An analysis of the CMIP6 models finds a distinct warming minimum/cooling and freshening in the subtropical ocean thermocline of the South Indian Ocean (SIO) under a medium-emission scenario (SSP245). The warming minimum/cooling has also been found in other warming scenarios in previous studies. However, the freshening here has received less attention. On account of increased precipitation in the models, the SO high latitudes get fresher in a warmer world. We show that this freshening anomaly is advected to the north of the deep mixed layer by the horizontal current and then subducts into the ocean interior in the SIO. As a result, the isopycnal surfaces become fresher, deeper, and cooler. This freshening and cooling signal then propagates to the north along isopycnals through the subtropical gyre and leads to freshening and cooling on the depth coordinates where the vertical movement of isopycnals (heaving) is insignificant. Lacking deep enough mixed layers, the other two basins show smaller freshening and cooling signs in the models. Here the importance of freshening in temperature redistribution in the ocean interior in the SIO under extensive global warming is emphasized. The result helps interpret the future heat storage in the SO in a warmer world.


OS07-A010
Decadal Variability of the Barrier Layer in the Tropical Atlantic Ocean

Xiao MA+, Hailong LIU#
Shanghai Jiao Tong University

Using Simple Ocean Data Assimilation 2.2.4 dataset for 1948–2008, we analyze the decadal variability of barrier layer thickness (BLT) in the Tropical Atlantic Ocean and its role in the phase transition process of the Atlantic Multidecadal Oscillation (AMO). The decadal variability of BLT shows a close relation with AMO. The AMO‐induced spatial distribution of BLT is similar to its first Empirical Orthogonal Function mode, showing a meridional tripolar pattern. AMO can exert an influence on the decadal variations of pressure and wind field in the tropical North Atlantic to indirectly modulate decadal variations in BLT. Weakened pressure over the tropical North Atlantic associated with a positive AMO phase strengthens the precipitation and therefore deepen mixed layer depth, which further decrease BLT. Meanwhile, the negative wind stress curl anomaly inhibits the upwelling in the West Bank of Africa, further deepening the isothermal layer, and increases BLT. At the same time, the weakened wind reduces the ocean heat loss, and deepens the mixed layer dominated by temperature in the east coast of Brazil, and thus decreases the BLT. The opposite is true for the negative AMO phase.


OS07-A011
Intraseasonal Variability and Mechanism of Sea Surface Salinity in the Northern Bay of Bengal

Rong CUI+, Xuhua CHENG#
Hohai University

In response to abundant freshwater from rainfall and river discharge, the northern Bay of Bengal (nBoB) features with low sea surface salinity (SSS) and strong intraseasonal variability (ISV). In order to explore the characteristic of SSS ISV in the nBoB and underlying dynamic mechanisms, satellite and reanalysis salinity data are deployed in this study. The salinity budget analysis indicates that the horizontal advection plays a dominant role, while the effect of freshwater flux is modest. Further analysis highlights the non-negligible significance of riverine freshwater, both geographically and temporally. The ISV of SSS is mainly concentrated near the mouth of the Ganges-Brahmaputra River and along the east coast of India, where the horizontal salinity gradient varies greatly. Once currents cross the salinity field, large horizontal advection anomalies come into existence and favor SSS ISV. Besides, SSS ISV in the nBoB is notably in phase with freshwater transport, which pinks from July to November.


OS07-A012
Relation Between Sea Surface Salinity, Ocean Circulation and Air-sea Interaction Around the Maritime Continent

Byoung Woong AN1#+, Hugh ZHANG2
1Centre for Climate Research Singapore, 2CCRS

The Maritime Continent (MC) sits in the middle of the warmest body of water known as the Indian and western Pacific warm pool, and has complex land-sea distribution and bathymetry. Therefore, it is challenging to make prediction of high-impact events in this region associated with multi-scale variabilities and interactions. In this study, the multi-scale spatio-temporal variability in sea surface salinity (SSS) around the Maritime Continent from 2014 to 2020 and their relation with ocean circulation and air-sea interaction are analyzed. Numerical experiments are conducted to quantify the contribution from the effects of freshwater flux and the dynamics of ocean circulation within this region. To understand the role of barrier layer thickness (BLT) in air-sea dynamics, we have calculated the BLT from numerical experiments and evaluated its effect on the upper ocean responding to Madden-Julian Oscillation (MJO). Results show that the thickness of model mixed layer and the isothermal layer are sensitive to wind and precipitation forcing and the sensitivity of the model performance to its vertical layer structure will also be discussed.


Mon-31 Jul | 10:20 - 12:20 | MR310
OS06 - Coastal Hazards: Impacts of Tropical Storms and Tsunamis

Session Chair(s): Tomohiro YASUDA, Kansai University, Huabin SHI, University of Macau

OS06-A009 | Invited
Coastal Flood Risk with Rising Sea Level in Macau

Jie YANG#+
Hohai University

Hato (2017) and Mangkhut (2018) are the latest and also strongest typhoons that flooded the Pearl River Estuary, but with different hazard mechanisms. Due to the vulnerability of coastal community exacerbated by future climate change and sea level rise (SLR), adaptation measures are urgently needed to defend storm surges and flooding induced by Mangkhut-like typhoons or even worse events. This study quantitatively compared the flooding dynamics by these two typhoons, estimated relative SLR under the RCP8.5 scenario in the South China Sea and investigated the potential upper and lower bounds of the maximum flooding depths in Macau City induced by Typhoon Mangkhut. Extreme tidal levels are assumed to be coincident with the pre-landfall hour of Mangkhut during its movement towards the coast. Under SLR scenarios by 2050 and 2100, flooding caused by astronomical tides indicate a significantly shortened return period of flood events with a rising sea level. The tidal barrier with a crest elevation designed according to Typhoon Hato can effectively protect the Inner Harbor region from flooding by astronomical tides or Mangkhut-like typhoons occurring at low tides; however this effectiveness is lost under high tides. The results indicate the dominant role of tidal timing at flooding depths, which is also influenced by modulated surge heights owing to nonlinear tide–wave–surge and SLR–surge interactions. Despite of decreased surges affected by SLR around Macau, Defence engineering infrastructure of tidal barrier cannot fully protect Macau, more comprehensive engineering countermeasures should be planned to cope with severe floods by compound unfavorable factors.


OS06-A004
Numerical Simulation of Coastal Flooding of Zhuhai Under Combined Influence of Storm Surge and Heavy Rainfall During Typhoon “Hato”

Yusi WU1#+, Pengzhi LIN1, Yi WEN1,2
1Sichuan University, 2The University of Tokyo

The super typhoon “Hato” was quickly strengthened before landing in Zhuhai and resulted in 24 deaths and $6.82 billion economic losses. In this study, the precipitation and wind of typhoon “Hato” are simulated by the mesoscale meteorological model WRF, and the induced storm surge and storm waves are simulated by the two-way coupled wave-ocean model FVCOM-SWAVE. The simulated storm surge is used as the initial and boundary conditions for the shallow water model for simulation of the flooding process along the eastern coast of Zhuhai. The numerical results are compared against the observed data of wind speed, precipitation and water level. The characteristics of coastal flooding process considering both storm surge and extreme rainfall are discusses and the impact of storm surge and local rainfall on coastal flooding is quantitatively analyzed. Besides, the dynamic risk analysis is presented to provide basis of proper disaster mitigation measures.


OS06-A034
Numerical Projection of the Sea Level Rise and Coastal Inundation Around Guangdong-Hongkong-Macao Greater Bay Area Over the Next Century

Danya XU1#+, Fu Hai DAO2, Kangyou ZHONG2
1Southern Marine Science and Engineering Guangdong Laboratory (Zhuhai), 2Sun Yat-sen University

The increasing sea level will have a great impact on coastal areas due to global warming. According to IPCC projections, the sea level of the major megacity groups near the coast could rise by up to 1 meter by the end of the 21st century. However, the resolution of the most numerical models utilized in IPCC projections are very course rath suitable for coastal inundation evaluation. Using the Sun Yat-sen university Community Integrated Model (SYSU) with a resolution about meters unstructured grids, evaluated the impact of climate change-induced sea-level rise (SLR) on the future coastal inundation over the Guangdong-Hong Kong-Macao Greater Bay Area (GHMGBA). The three time sections of 2020, 2050 and 2100 are simulated and the under the background of global warming and sea level rise, we simulated the inundation area of the Great Bay Area in 2020, 2050 and 2100. The simulated results show that under the condition of unchanged terrain, from 2020, the inundated area of the Great Bay Area will be increased by 25% by 2050 and 39% by 2100 compared with 2020 respectively. This implies that with sustained Sea Level Rise, especially for those low-lying regions around the Guangdong-Hong Kong-Macao Greater Bay Area will be vulnerable more severely to the warming climate.


OS06-A071
Hazard Assessment of Storm Surge Flooding in Small Coastal Cities – Taking Macao as an Example

Huabin SHI#, Huimin ZHENG, Kailun HU+, Guoyou LI
University of Macau

Coastal cities are facing an increasing risk of storm surge flooding due to the sea level rise. Macao is a small-scale lowing lying city, densely populated and highly urbanized. It is extremely vulnerable to tropical cyclones and the induced storm surge. In 2017 and 2018, the Super Typhoon Hato and Mangkhut both caused catastrophic damage in Macao, more than 150 injuries/deaths and billion dollars economic losses. For disaster prevention and mitigation in Macao, it is critical to assess the vulnerability to storm surge in the future. However, the assessment of storm surge hazard in such a small-scale low-lying, densely populated, and highly urbanized city has never been reported. In our study, an assessment framework of the storm surge hazard in Macao is developed, in which an index system of hazard is suggested. The index system includes hazard, social vulnerability, and disaster-bearing capability indexes with both subjective and objective methods adopted to determine their weights. The hazard risk levels of different districts of Macao in specific typhoon cases are determined. The study aims to help improve the disaster prevention and mitigation as well as city plan and emergency management in small-scale coastal cities.


OS06-A023
Effect of Wave Drag and Wave Setup on Storm Surge in the Northern East China Sea: A Semi-enclosed Basin

Shuiqing LI#+
Chinese Academy of Sciences

The northern East China Sea (NECS) is a semi-enclosed basin that is frequently attacked by the tropical cyclones (TCs), and the storm surge acts to be a huge threat to the coastal regions. In this study, a numerical study on the wave contribution to the storm surge in the NECS is performed, with emphasizing on the two dominant wave effects, wave-induced surface stress (wave drag) and wave radiation stress (wave setup). Two TC cases (TCs Lekima and Muifa) translating into the study region in quite different paths are considered. Comparisons with the gauge tide observation reveal that the numerical simulations can be significantly improved by considering the wave drag by using a wave-steepness-dependent roughness parameterization, in particular in the coastal regions of Bohai Sea. Sensitivity tests indicate that wave drag plays a primary role as it can be up to about 22% increment of the peak storm surge in the inner bay, and wave setup accounts by up to about 10% increase in peak storm surge in the outer regions. The impact of wave drag is accumulative along the long cross shoreline direction while that of wave setup is largely nearshore locally-induced. The significant impact of wave drag in the inner bay is attributed to the the young fetch-limited wind waves suffering shoaling effect. The results highlight the necessity of considering the influence of topography-wave-drag interaction on surge level in a semi-enclosed basin.


OS06-A008
Feedback of Building Structure on Mass Conservation in Subgrid-scale Modeling of Storm Surge Inundation in a Coastal Urban Area

Nobuki FUKUI1#+, Nobuhito MORI2, Sooyoul KIM3, Tomoya SHIMURA2, Takuya MIYASHITA2
1Tottori Univerfsity, 2Kyoto University, 3Kumamoto University

Storm surge-induced inundation simulations using an ultra-high-resolution topography considering artificial structures such as buildings have been done; however, they are challenging because of the high computational cost. This work improves a subgrid-scale model, called the individual drag force model (iDFM), to efficiently simulate floods over coastal urban areas using coarser grids than building widths based on the storm surge model using 2D shallow water equations. The original iDFM implements the effect of building on inundation flow by the total sum of the drag forces on a group of buildings in a grid cell in the momentum conservation. The improved iDFM newly considers the feedback of buildings on mass conservation using the ratio of wet area to area of grid cell, which is calculated using subgrid topography in high resolution (finer than 5 m). The authors performed a series of numerical simulations focusing on the coastal urban area (30 m grid size) in Sumida-ward and Koto-ward next to Tokyo Bay using the meteorological field by the pseudo global warming experiment of Typhoon Hagibis (2019). The validation employs the structure resolving model using 5 m grid cell size as a reference value. The improved iDFM models about 45.4% larger inundation depths than the original iDFM and succeeded in improving accuracy. If the ground elevation does not include the building height as the still water depth in the computational grid cell, the effect of the building such as the water level rise by blocking is not considered in the calculation of the water level in the mass conservation. However, the improved iDFM addresses the issue since the feedback of buildings on mass conservation is considered. The results of further analysis focusing macroscopic view such as the time series of inundated areas, and the relationship between building and water volumes will be presented.


OS06-A037
Typhoon-generated Extreme Wave Reanalysis with Data Assimilation of Drifting Buoy Observations

Gota YAMASAKI#+, Nobuhito MORI, Tomoya SHIMURA, Takuya MIYASHITA
Kyoto University

Typhoon-generated extreme waves have caused coastal disasters historically, and typhoon intensity is anticipated to be intensified by global warming. Therefore, accurate typhoon wave simulation is important for disaster risk reduction. Data assimilation is a promising tool for the improvement of wave simulation. However, the amount of typhoon wave observation in the open ocean has been small for data assimilation. On the other hand, small and low-cost wave buoys are available recently thanks to technological innovation. Our research group has deployed an open ocean drifting buoy network in the Western North Pacific. In this study, we developed a system to assimilate the drifting buoy observations into the spectral wave model, WAVEWATCH III, to improve its accuracy. We implemented Optimal Interpolation as data assimilation method. We conducted typhoon wave simulations in the Western North Pacific, targeting the summer of 2022. The strongest typhoon in 2022 had 910 hPa minimum central pressure. The accuracy of wave simulations was estimated using the Japanese coastal wave observation network. At first, we conducted the initialized experiment in which the initial condition is assimilated with drifting buoy observations, and the model runs for three days without assimilation. As a result, the model improves immediately after data assimilation (initial condition), and the improvement continues for 71 hours. Next, we conducted a sequential data assimilation experiment in which the assimilation process was operated every 1 hour. The sequential data assimilation reduced the wave model error by up to 2.72 m when drifting buoys observed extreme typhoon waves near the center. Even when the assimilation process is operated every 3 hours, the wave model error was reduced by up to 2.36 m. Our results show that drifting buoys observation data assimilation can meaningfully improve the wave model for extreme typhoons waves.


OS06-A027
Characterizing Extreme Wave Heights in the East Asian Marginal Seas

Ahmad BAYHAQI1+, Jeseon YOO2#
1University of Science and Technology, 2Korea Institute of Ocean Science and Technology

Historical extreme wave events have occurred in the East Asian Marginal Seas (EAMS), causing devastating damage to the coastal environment. Since extreme wave events are influenced by global climate change, an understanding of extreme wave events needs to be deepened for coastal adaptation to their impact of it. Herein, the hourly significant wave height (Hs) from the ERA5 reanalysis data is mainly considered to characterize Hs extremes (HsE) in the EAMS. The occurrence of HsE is statistically analyzed to compute its metrics such as intensity, duration, and frequency over the period of 1980-2021. In addition, the HsE seasonality is characterized using the Generalized Extreme Value (GEV) distribution method. The findings reveal that HsE in the study area has occurred 2-8 events per year, having an intensity of up to 1.5 m and lasting from 8 to 35 hours on average. Among the EAMS (i.e., the East China Sea (ECS), the Yellow Sea (YS), and the East Sea (ES)), the longest and largest intensity are found in the ECS, while the most frequent is observed in the YS and ES. The HsE with the return periods of 20, 50 and 100 years in the ES (YS) tend to be higher in the winter (fall) season. Meanwhile, the highest return values among EAMS which reaches 7-8 meter on average are found in ECS during summer. The HsEs in ES and YS are associated with the intensified local wind, owing to the enhanced pressure gradient. On the other hand, those in ECS are mainly induced by typhoon activities.


Mon-31 Jul | 10:20 - 12:20 | MR327
OS02 - Mixing Matters

Session Chair(s): Robin ROBERTSON, Xiamen University Malaysia

OS02-A022 | Invited
Observed Internal Tides in the Deep Northwestern Pacific by Argo Floats

Zhenhua XU#+
IOCAS

This study aims to extract the observed internal wave signals in the northwestern Pacific from Argo floats with Iridium-telecommunication that can directly measure the hourly temperature, salinity and pressure near 1000 dbar. Vertical displacements and spectral features of internal tides can be interpreted from Argo float data. More than 10,000 parking-phase observations of 252 Argo floats were used to estimate their spatial-temporal characteristics. Vertical displacements attributed to internal tides exceeded 30 dbar near energetic sources, such as the Luzon Strait, Izu ridge, Mariana Arc and Palau. The observed internal tides feature both seasonal and spring-neap cycles corresponding to barotropic tidal variations. The diurnal and semidiurnal peaks in the energy spectra differed with latitude in related to different internal wave properties. Particularly, energetic local-trapped diurnal internal tides or topographic waves occurred at 33°N near Izu Ridge, which is poleward of diurnal critical latitude. The internal tidal energy was calculated by theoretical fitting the vertical displacements from one layer to the full-depth water. The observed e-folding decay scales of the semidiurnal internal tidal energy were estimated as ~550-950 km in the deep basin. The Argo parking data provide a unique view for observing the basin-scale pattern and energy sink of deep-ocean internal tides, which could supplement the widely-used surface altimetry observations and contribute to a more accurate parameterization of tidal mixing.


OS02-A018
M2 Internal Tide Energetics and Behaviors in the Subpolar North Pacific

Jia YOU1#+, Zhenhua XU2, Qun LI3, Peiwen ZHANG1, Baoshu YIN1, Yijun HOU1
1Chinese Academy of Sciences, 2IOCAS, 3Polar Reasearch Institute of China

Energetic internal tides in the Pacific Ocean are generated from multiple sources and generally characterized, although the subpolar North Pacific (SNP) is known as a high-latitude hotspot that remains less explored. The present study is the first detailed investigation on M2 internal tide energetics and dynamics in the SNP by high-resolution numerical simulations. M2 internal tides in the SNP mainly originate from the Aleutian Ridge (~5.51 GW of barotropic-to-baroclinic conversion rate), wherein the Amukta Pass is the most significant source. The Amukta Pass radiates northward ~0.55 GW to the Bering Sea and southward ~1.40 GW to the North Pacific. The subsequent south-north asymmetric radiation pattern is consistent with satellite altimeter detection. In the Bering basin, multiwave superposition in the near field between the Amukta Pass and the adjacent sources generates two vortex flux patterns. After approaching the Bering Sea slope, remote internal tides from Aleutian Ridge enhance local generation and dissipation. The dissipation field is relatively similar to the generation map, which is explained by the higher local dissipation efficiency (>1/2) in these generation sites and the faster energy attenuation than in the mid-latitudes. The simulated dissipation rates compare favorably with the estimate from fine-scale parameterization, indicating the dominance of internal tidal mixing. The averaged dissipation rate in SNP is O (10-10) W/kg, and the depth-integrated dissipation rates can reach O (10-1) W/m2 near the Amukta Pass. The unique internal tidal physical process and dissipation behaviors at high latitudes are indispensable for understanding the redistribution of global baroclinic tidal energy and global ocean mixing.


OS02-A012
Ocean Trench Circulation Driven by Tidal Mixing

Hongzhou XU1#+, Huichang JIANG2
1Institute of Deep-sea Science and Engineering, Chinese Academy of Sciences, 2Chinese Academy of Sciences

Hadal trenches are the deepest regions of the ocean. The Challenger Deep in the Mariana Trench is the deepest of all. Due to the challenge of sampling in the extreme environment, the deep circulation of the Challenger Deep is still poorly understood. An observational array comprised of four subsurface moorings was deployed to investigate the circulation structure, volume transport and temporal variation in this trench. Results showed a three-layer circulation below 3,600 m, varying from westward circulation to cyclonic circulation then to anticyclonic circulation as depth increases. The annual mean LCDW (Lower Circumpolar Deep Water) transport through the Challenger Deep is estimated to be -1.86 Sv. The LCDW intrusion with significant seasonal variations controls the temporal variation of westward circulation above 6,000 m. The cyclonic-anticyclonic circulation was relatively steady during the observed period. Numerical experiments suggest that the three-layer circulation is modulated by the LCDW intrusion, unique topography and turbulent mixing. The turbulent mixing is decisive for driving the cyclonic-anticyclonic circulation below 6,000 m. This study provides a dynamic basis for the material transport, sedimentation process and species migration in the trench, and shows an example for using ocean models to study hadal trenches.


OS02-A005
Diapycnal Mixing and Turbulent Heat Salt and Dissolved Oxygen Fluxes in the Northwestern Sea of Japan

Dmitry STEPANOV1#+, Alexander OSTROVSKII2
1V.I. Il`ichev Pacific Oceanological Institute, 2Shirshov Institute of Oceanology

The Sea of Japan is a well-ventilated and oxygen-rich basin in the northwestern Pacific Ocean. However, quantitative estimates of the intensity diapycnal mixing based on observations are still catastrophically small. For the first time, the “Aqualog” profiler (as a Wirewalker) carried out continuous collocated measurements of temperature, electrical conductivity, dissolved oxygen and current velocities on the continental slope in the northwestern Sea of Japan. The resulting vertical profiles with high vertical resolution served as the basis for estimating the intensity of dissipation of the kinetic turbulence energy and coefficient of turbulent mixing. To estimate these quantities, we are applying fine-scale parameterization (Gregg-Henyey-Polzin parameterization), based on the assumption of the leading role of the weakly nonlinear interaction internal waves. Variations of turbulent mixing from season to season and an increase in mixing intensity with depth are discovered. We register the elevating intensity of turbulent mixing when passing through the station mesoscale eddies. The influence of double diffusion processes on the diapycnal mixing is discussed. This study was supported by the Russian Science Foundation N 23-27-00333 (https://rscf.ru/en/project/23-27-00333/).


OS02-A019
Mixing in the Philippine Sea: Geography Variability and Parameterization

Peiwen ZHANG1#+, Zhenhua XU2, Jia YOU1, GuangHong LIAO3, Baoshu YIN1, Robin ROBERTSON4
1Chinese Academy of Sciences, 2IOCAS, 3Hohai University, 4Xiamen University Malaysia

The Philippine Sea Mixing Experiment (PhiMix) was carried out in 2021 concurrently from two research vessels, obtaining microstructure measurements and fine structure-based estimates of turbulence and diffusivity covering nearly the whole Philippine basin for the first time. The inhomogeneous spatial distribution and weak magnitudes of turbulent mixing in the Philippine Sea basin were revealed, according to the upper-ocean turbulence measurements and full-depth CTD datasets. The averaged diffusivities in the Philippine Basin were ~10-2 m2s-1 in the surface mixed layer and ~10-5.5 m2s-1 in the ocean interior. Below the thermocline, the diffusivities generally increased and reached 10-4 m2s-1 above rough topography. Centered on the Palau Ridge, a significant east-west asymmetry was noted, with stronger mixing on the east side of the ridge. Additionally, the diapycnal diffusivity’s spatial variability coincided with that inferred from tidal mixing between 500-3000 m. Typical dissipation rate and diapycnal diffusivity profiles in the Philippine Sea differed from the global averaged profiles, which form the basis of most existing mixing parameterizations. Here we proposed an improved parameterization scheme based on these new direct microstructure observations in the Philippine Sea. The new mixing parameterization scheme (PhiMixPar-PMP) performed well for the Northwest Pacific Ocean in ocean simulations. This regional study on mixing properties in the Philippine Sea can fill a knowledge gap in the big picture of global mixing geography and improve turbulence parameterizations in the ocean models.


OS02-A026
On Shoaling Internal Solitary Waves with Enhanced Mixing in the Dongsha Region, South China Sea by Seismic Reflection Data

Haibin SONG#+, Yunyan KUANG, Kun ZHANG
Tongji University

Shoaling internal solitary waves in the Dongsha region in the South China Sea dissipate their energy and enhance diapycnal mixing, which have an important impact on the oceanic environment and primary productivity. The enhanced diapycnal mixing is patchy and instantaneous. Evaluating its spatiotemporal distribution requires comprehensive observation data. Fortunately, seismic oceanography meets the requirements, thanks to its high spatial resolution and large spatial coverage. In this paper, we studied several internal solitary wave packets in the region and calculated their spatial distribution of diapycnal diffusivity. Our results show that the average diffusivity in internal solitary waves with reversing polarity is 3 times that of the nonpolarity reversal region. On a seismic section, we observed two internal solitary wave packets in the deep water area (500-1000m) and shallow water area (300-400m) of the upper slope respectively, which have obviously different waveform characteristics. Three internal solitary waves of the internal solitary wave packet in shallow water region are complex, showing chaotic reflection characteristics in the wave core, which may be the internal solitary waves with trapped vortex core. The estimated diffusivity rate is O (10-2.5) m2 s-1. There is a mode-2 internal solitary wave ahead of the internal solitary wave packet. Although the waveform of internal solitary waves in the packet in deep water is relatively simple, the induced turbulent mixing intensity is also strong, forming zones of high dissipation rate and diffusion rate within internal solitary waves development and a region with a thickness of 200m above the continental slope. In the deep and shallow water areas of the upper slope of the Dongsha region, the internal solitary waves continuously dissipate energy and enhance the turbulent mixing.


OS02-A015
Towards a Better Parameterization of Ocean Turbulent Mixing in the Estuarine-shelf Environment

Qing LI1#+, Bicheng CHEN2
1The Hong Kong University of Science and Technology (Guangzhou), 2Xiamen University

Ocean turbulent mixing is important small scale physical processes in the ocean that requires parameterization in ocean circulation models. Existing parameterizations fail to agree with each other under many forcing conditions. In the estuarine-shelf environment such as the Pearl River Estuary, a combination of multiple factors including the presence of ocean surface waves, strong stratification and fronts due to river runoff, tidal currents, and relatively shallow water depth makes an accurate representation of ocean turbulent mixing even more challenging. Here we present preliminary results of a modeling effort towards a better parameterization of ocean turbulent mixing in such estuarine-shelf environment. In this work, we use a combination of large eddy simulations, which directly resolve the energy containing turbulence, and idealized ocean circulation simulations, which provide the large scale forcing and background conditions representing an idealized estuary. The focus is on the response of ocean boundary layer turbulence to the changing forcing and background conditions in typical estuarine-shelf environment.


OS02-A021
Water Quality and Estuary Characteristics of the Chao Phraya River During the Dry Season

Kachapond CHETTANAWANIT1#+, Watin THANATHANPHON2, Narongrit LUANGDILOK2, Sathit CHANTHIP2, Piyamarn SISOMPHON2
1Hydro – Informatics Institute, Ministry of Higher Education, Science, Research and Innovation, 2Ministry of Higher Education, Science, Research and Innovation

The Chao Phraya River is a major river in Thailand's central region, which provides water for agriculture, hydrant water, and a variety of other activities that contribute significantly to the country's economy. However, the river suffers from low water quality, saline intrusion, and environmental issues in the estuary zone during the dry season, which affects the people living along the river. This study aimed to investigate water quality and estuary characteristics along 100 kilometers of the Chao Phraya River during the dry season (November to March) in 2021 and 2022. The field survey was divided into 29 observation points for measuring salinity, water quality, and vertical current profiles. As the results indicated, the vertical current profile and salinity profile indicated that the estuary was well-mixed in the dry season. The eutrophication zone was observed approximately 20–50 kilometers from the river mouth, where saltwater and freshwater meet. Because of the well-mixed condition, zero dissolving oxygen and high levels of chlorophyll-a (Chl-a) were found in the whole water column in that area. On the other hand, a large flood event in late 2021 will bring high discharge from upstream to the Chao Phrya River. During that time, salinity can intrude only 10–20 kilometers from the river mouth, and the vertical profile was identified as a partially mixed estuary. The eutrophication zone was not clearly observed. In conclusion, the estuary characteristics and water quality were affected by the physical condition of the ocean and discharge volume. To reduce the low water quality, the adjustment of discharge from the upstream influence greatly changes the quality of the water in the river.


Mon-31 Jul | 1:10 - 3:10 | MR306
OS08 - Oceanic Big Data and Artificial Intelligence Oceanography

Session Chair(s): Guangjun XU, Guangdong Ocean University, Alexandre STEGNER, Laboratoire de Météorologie Dynamique/ National Centre for Scientific Research

OS08-A003 | Invited
How AI Computer Vision on SST Imagery Combined to Satellite Altimetry Can Improve the Accuracy of Oceanic Eddy Detection and Provide a New Tool for Model Validation?

Alexandre STEGNER1,2#+, Evangelos MOSCHOS2, Alisa KUGUSHEVA2, Briac LE VU2
1Ecole Polytechnique, 2AMPHITRITE

Today, most of the eddy detection algorithms operate on satellite altimetry gridded observations, which provide daily maps of sea surface height and surface geostrophic velocity. However, the reliability and the spatial resolution of altimetry products (AVISO/DUACS) is limited by the strong spatio-temporal averaging of the mapping procedure. Yet, the availability of high-resolution satellite imagery makes eddy detection possible at a much finer scale, via advanced computer vision methods. We propose a novel eddy detection method via a transfer learning schema, using the ground truth of high-resolution ocean numerical models to link the characteristic streamlines of eddies with their SST signature. Combining the independent eddy signatures both on AVISO/DUACS products and high-resolution SST allows for a highly reliable detection of reference eddies. When these two independent eddy detections are coherent in space and time, we obtain a very high reliability and accuracy that cannot be achieved with standards methods. We are then able to build, from satellite observations, a reliable data base of oceanic eddies that can be used as a reference data-set for real time validation of numerical models.


OS08-A004 | Invited
Short-term Forecasting of Coastal Surface Currents Based on High Frequency Radar Observations and Machine Learning

Lei REN1,2#+, Yaqi WANG1,2, Lingna YANG1, Jun WEI1, Michael HARTNETT3
1Sun Yat-sen University, 2Southern Marine Science and Engineering Guangdong Laboratory (Zhuhai), 3University of Ireland

Surface currents primarily driven by winds can flow for thousands of kilometers and can reach depths of hundreds of meters. Its movement carries heat and mass from place to place in the Earth system. Timely and accurate forecasting of surface currents in coastal regions is of great importance for a variety of aspects such as development of marine economics and environmental protection. In this research, firstly, temporal and spatial characteristics of sea surface currents were analyzed, and then short-term surface current forecasting models based on integrated ensemble learning algorithms and the shore-based High Frequency radar observations were established. In order to improve the model's forecasting ability and accuracy, the model structure was examined in details. Error variation of the reconstructed model for short-term forecasting of surface currents is outperform that of traditional ANN models. Meanwhile, the number of forecasting factors needed for the optimal model increases with the number of forecasting steps. When forecasting time increases, the effect of tidal influence increases. When the number of forecasting time is greater than a critical value, the effect of wind speeds is dominant. Forecasted short-term surface current information will provide scientific basis and important reference for marine engineering construction, disaster prevention and reduction and coastal rescue for coastal areas.


OS08-A010 | Invited
Developing a Deep Learning-based Storm Surge Forecasting Model

Hongchun ZHANG1#+, Wenhong XIE1, Guangjun XU2,3, Changming DONG1,3
1Nanjing University of Information Science & Technology, 2Guangdong Ocean University, 3Southern Marine Science and Engineering Guangdong Laboratory

Storm surge is the anomalous rising of the sea surface induced by intense atmospheric disturbances. The storm surge caused by tropical cyclones often causes great socio-economic, human activity, and life and property hazards to coastal areas. In terms of research resource consumption and computational time, machine learning algorithms that depend on data-driven strong nonlinear mapping skills outperform standard numerical model forecasting. To obtain a lighter and faster storm surge shortcoming forecast, we use a deep learning-based single-station water level prediction model for a storm surge at several locations in this work. In contrast to earlier research, this study employs convolutional neural networks to extract two-dimensional wind field information and merge them with local water level features to produce a more time-efficient intelligent forecast.


OS08-A011 | Invited
Deep Learning Approach for Forecasting Sea Surface Temperature Response to Tropical Cyclones in the Western North Pacific

Han ZHANG#+
Second Institute of Oceanography, Ministry of Natural Resources

Tropical cyclones (TCs) induce sea surface temperature cooling (SSTC), which is important for TC development itself as well as for variations of regional air-sea environment. TC-induced SSTC patterns and its prediction is still a challenge. In this study, a long short-term memory neural network deep learning model is developed to forecast TC-induced SSTC in the western North Pacific (WNP) using TCs during 2002-2016 as training cases and TCs during 2017-2018 as prediction and test cases. The 6-hour TC-induced SSTC biases to the right-rear area of TC center, with a maximum of ~0.6 °C on average, while SSTC is greater in higher latitudes than lower latitudes. The input variables for the deep learning model are surface wind at 10 m (U10 and V10), sea surface height (SSH), sea surface temperature (SST), and temperature at 100 m depth (T100), the output variable is SST 6 hours after TC. The model can predict TC-induced SSTC patterns, with an average mean absolute error of ~0.081 °C, a root mean square error of ~0.126 °C and a spatial anomaly correlation coefficient of ~0.948. This work indicates that post-TC SSTC follows similar physical processes and nonlinear relationships with TC wind, initial SSH and ocean temperature, especially in deep-water regions. Although with some limitations, the deep learning model has the potential to be applied to operational forecasts.


OS08-A012 | Invited
Global Ocean Heat Content Reconstruction from Remote Sensing and Climate Models Based on Artificial Intelligence Methods

Wenfang LU1#+, Hua SU2, Lijing CHENG3
1Sun Yat-sen University, 2Fuzhou University, 3Institute of Atmospheric Physics, Chinese Academy of Sciences

Retrieving information concerning the ocean's interior using satellite remote sensing data has significant benefits for studies of ocean dynamics and climate changes; however, the lack of information within the ocean limits such studies about the global ocean. In this study, we use AI approaches to connect the surface remote sensing observation and the global ocean heat content (OHC) estimates from the gridded Argo product, over four different depths down to 2000 m. The method allows for the reconstruction of the OHC to other periods beyond the Argo-era training period. By applying an ensemble technique, the hindcasting uncertainty could also be estimated by using different time periods for training and then calculating the standard deviation across ensemble members. This new OHC product is called the Ocean Projection and Extension neural Network (OPEN) product. Using this approach, we further use climate models to reconstruct historical OHC changes with considerable accuracy, with good variability and trend estimates. The OPEN product can therefore provide a valuable complement for studies of global climate changes.


OS08-A001
A Deep Learning-based Approach for Empirical Modelling of Local Wave Spectra in Oceans

Haoyu JIANG#+, Yuhao SONG
China University of Geosciences

Directional wave spectra are of importance for numerous practical applications such as the design of coastal structures and hazard assessment. Previous studies have demonstrated a correlation between the wave spectral densities at a certain point in the ocean and the local or remote wind field. This feature can be used to predict the wave spectrum at that point using the wind field. In this study, a deep neural network (DNN) model was established to estimate wave spectra at a target point using the wind field from the ERA5 dataset. A geospatial range where the wind could impact the target point was selected and then the historical wind field data within the range was analyzed to extract meaningful features. For the spectral densities at a given direction, the wind data along the opposite direction of wave propagation were used as the input of the DNN. The model was trained to minimize the error between the DNN-predicted and ERA5 re-analysis spectral density. The data structure of the wind input is reorganized using a spherical multiple-cell grid to make the model applicable to different locations worldwide. The model allows for the prediction of local wave spectra with low computational cost and can be helpful for the study of local spectral wave climate.


OS08-A002
Estimation and Prediction of Sea Surface Current Around the Korean Peninsula Using Artificial Neural Network

Jeong-Yeob CHAE, Jae-Hun PARK#+
Inha University

Recent advancement of numerical ocean modelling makes it possible to predict a realistic ocean with the help of data-assimilation and fine spatial resolution. Nevertheless, the well-developed model requires high computational power and time, making it hard to be utilized for practical purposes sometimes. To compensate the high computational costs, there is a need to develop novel approaches with efficient computational costs, combined with the numerical model outputs. In that way, artificial neural networks could be one of the solutions because they need low computational power since it utilizes pre-trained networks. Here, we present a current prediction framework applicable to the seas around the Korean peninsula using three-dimensional convolutional neural networks (3D-CNN). The network is based on the 3D-Unet structure and modified to predict ocean currents using oceanic and atmospheric variables. It is optimized to minimize the error of the next day’s ocean current field, and its recursively predicting structure allows more days to be predicted. The network's performance is evaluated by changing input days and variables to find the optimal surface-current-prediction artificial neural network model, which demonstrates its strong potential for practical uses near future.


OS08-A014
AI-enabled Method for Predicting Sea Ice Accurately Based on Complex Environmental Change Mechanism

Guangcun SHAN1,2#+, Zejian DING3
1Beihang University & City University of Hong Kong, 2City University of Hong Kong, 3Beihang University

Arctic sea ice is showing an annual melting trend in the context of global warming. The traditional study paradigm for Arctic sea ice prediction is a prediction system based on physical equations, which requires the physical mechanisms to be resolved first, which has high average absolute errors and makes it difficult to meet practical application needs. In recent years, artificial intelligence (AI)-based models have been playing a more and more important role in the studies of predicting Arctic sea ice. The new AI paradigm for predicting Arctic sea ice based on AI models can first develop accurate predicting models, and then invert the physical mechanisms to achieve high spatial and temporal resolution. In response to the problems of unreliable sea ice prediction results and unclear complex environmental mechanisms, the high-resolution AI-enable prediction model for predicting Arctic sea ice is proposed to unravel the complex mechanisms of spatial and temporal regions, environmental elements and physical processes affecting sea ice changes implied by the model. Based on an online incremental learning training system and integrating domain knowledge-based and jointly data-driven method, our work presented here has carried out a high-resolution Arctic sea ice predicting model. A new paradigm of AI for sea ice predicting research is constructed through high-precision forecast model and meanwhile in-situ observation of Arctic sea ice change mechanisms, ultimately enabling the sub-kilometer level predicting model for Arctic sea ice.


Tue-01 Aug | 10:20 - 12:20 | MR308
OS06 - Coastal Hazards: Impacts of Tropical Storms and Tsunamis

Session Chair(s): Iyan MULIA, RIKEN Cluster for Pioneering Research, Yong WEI, University of Washington

OS06-A001 | Invited
History and Improvements of the Japanese Tsunami Warning System

Kenji SATAKE#+
The University of Tokyo

Following the 1896 and 1933 Sanriku tsunamis, each caused thousands of casualties, Japan Meteorological Agency (JMA) started a tsunami warning system in 1941 for the Sanriku coast, and the near-field tsunami warning system covered the entire Japanese coast in 1950. The tsunami warning system for far-field tsunamis was established in 1962, following the 1960 Chilean tsunami. For the 1983 and 1993 earthquakes in Japan Sea, the tsunami warning was issued 14 and 5 minutes after the earthquake, respectively, but the tsunami arrived on the nearest coast earlier. Since 1999, JMA has adopted numerical simulation and its database to improve accuracy. Once the location and magnitude are determined in 3 to 5 minutes after an earthquake, the database is searched to predict arrival times and heights on the coasts. For the 2011 Tohoku earthquake (M 9.0), the tsunami warning was issued in 3 minutes, but the forecast tsunami heights were much lower than the actual ones because the magnitude was underestimated as 7.9. Following the 2022 tsunami from Tonga eruption, which started several hours earlier than the expected tsunami arrival time, JMA now announces arrival times of atmospheric pressure waves for large-scale volcanic eruptions in the world. For timely and accurate issuance of a tsunami warning, seismic and/or geodetic observations are essential. A reliable warning should be based on observations of tsunamis, i.e., sea level. Recent deployments of offshore bottom pressure gauges such as S-net or DONET help to confirm tsunami generation and propagation and improve the reliability of the warning. JMA adopts the tFISH system, which inverts offshore tsunami waveforms to estimate the tsunami source then coastal heights. It is also possible to issue a warning based on tsunami data assimilation, without estimating the tsunami source.


OS06-A013
Long-lasting Tsunami Simulations for Appropriate Withdrawal of Tsunami Warning

Naoko SHINMOTO#+, Toshitaka BABA
Tokushima University

In order to cancel tsunami warnings and advisories with clear numerical evidence, improving prediction techniques for tsunami attenuation is necessary. This study investigated the attenuation process of the tsunami of the 2011 Pacific coast of Tohoku earthquake using numerical simulations. We used the moving root mean square (MRMS) amplitude defined by Hayashi (2010) for comparisons between observation and calculation results. Our numerical simulation solved the long-wave equations on the nesting grids from the tsunami source of Satake et al. (2013). The analysis points were six tide gauges at Hanasaki, Mera, Okada, Chichijima, Awayuki, and Amami, one wave gauge at Kushiro Port (NOWPHAS), and three offshore GPS wave gauges off North Miyagi, Central Miyagi, and Kaiyo-Tokushima.We repeated 48-hour tsunami simulations by changing the calculation area and resolutions. The high-resolution topographic grids around the observation point improved the reproducibility of the MRMS amplitude waveforms in the calculation using the northern Pacific Ocean. However, for the calculation with the limited calculation area to the emperor seamount chain, high-resolution topographic grids around the observation point did not improve the reproducibility of MRMS amplitude. The topographic resolution required to reproduce MRMS amplitude waveforms differed by the analysis point. While a minimum grid interval of 20 arc-sec was sufficient for Hanasaki, 20/3 arc-sec was required for Mera, 20/9 arc-sec for Okada, and 20/27 arc-sec for Chichijima, Awayuki, and Amami. The minimum grid interval of 20 arc-sec was sufficient for Kushiro Port, North Miyagi, Central Miyagi, and Kaiyo-Tokushima because of offshore gauges. The required resolution for accurate prediction depends on the surrounding topography.


OS06-A038
Morphological Structure Variation Controls Fault Slip Behaviors in the Aleutian-Alaska Subduction Zone

Qiang QIU1#+, Linlin LI2, Xiaodong YANG1, Jian LIN3
1South China Sea Institute of Oceanology, Chinese Academy of Sciences, 2Sun Yat-sen University, 3Woods Hole Oceanographic Institution

Understanding how morphological structure of a fault affects slip behaviors and extent of a subduction earthquake is crucial for seismic and tsunami hazards assessment. However, such behaviors are poorly known at many subduction zones due to the lack of near fault-zone measurements. Here, we integrate GNSS, tsunami waveforms, seismic-profile determined structural data sets, and dynamic earthquake-cycle modelling to examine the slip characteristics of the 2020 Mw 7.8 Simeonof (Shumagin segment) and the 2021 Mw 8.2 Chignik (Semidi segment) earthquakes and to gain a comprehensive understanding of the rupture behaviors of the neighboring segments along the Aleutian-Alaska subduction zone, respectively. We uncover why these neighboring segments behave contradictorily over seismic cycles by illuminating the strong variations in morphology, steepness, and serpentinization level of the megathrust zone on the plate interface. We identify a structural and mechanical boundary that seats under the Shumagin Island, which separates the megathrust into west and east portions. The west portion (from eastern Unimak to western Shumagin) is a steep-planar megathrust and is characterized by several large-isolated-steep patches, which coincides the oceanic to continental transition boundary – Beringian margin where it exists gravity and serpentinization anomaly. A rough and fluid-saturated megathrust may explain the weak coupling to rupturing as small to moderate earthquakes, but rarely to nucleating as large earthquake in seismic cycles. While the east portion (from eastern Shumagin to western Semidi Island), develops a smooth-curved and low serpentinization plate interface, failing as many partial or full ruptures like the moderate to large earthquakes observed in rupture history. We highlight that such structural variation and changes in fluid concentration controls rupture behaviors and shapes the slip extent in the 2020-2021 earthquakes as did previously, resulting in a low tsunami risk in the west portion but a moderate to high tsunami potential for the east portion.


OS06-A059
Consideration of Evacuation Routes Based on Tsunami-inundated Probability

Fukuto YOSHIDA+, Masaki ISHIYAMA, Taro ARIKAWA#
Chuo University

The expected height of the largest class of tsunamis has increased since the Great East Japan Earthquake on March 11, 2011. Given this, conventional hardware measures and software measures have become more important. Furthermore, the effectiveness of evacuation support using tsunami information in advance has been demonstrated to improve the success rate of evacuation. However, Ishiyama et al. (2022) showed that the mortality rate increases when the prediction is erroneous compared to the actual arrival time of the tsunami. Therefore, it is considered necessary to provide evacuation assistance according to probabilistic risk. This study aims to construct and assess a model that can calculate the probability of tsunami arrival time after the earthquake using multiple tsunami inundation scenarios and calculate a route with a low tsunami encounter probability based on the shortest route to the evacuation shelter in some target areas. The results show that the mortality rate decreased for evacuation immediately before flooding compared to Sakata et al. (2020), who used the predicted tsunami arrival time, and the case using the expected erroneous tsunami arrival time. However, the time required to reach the evacuation shelter may increase due to the choice of low-risk routes depending on the start time of evacuation. Furthermore, in some cases, evacuees may sometimes encounter a tsunami during the evacuation process due to the increased evacuation time. Therefore, in the future, incorporating the route selection method that considers the evacuation time is necessary.


OS06-A025
Sensitivity Analysis of Fault Parameters to Tsunami Height Along the West Coast of Japan with Stochastic Source Models

Kenta FUJIMOTO#+
Kyoto University

Future tsunami events include a variety of uncertainties. Especially on megathrust earthquake tsunamis, the tsunami hazard intensity at coastal cities highly depends on the source characteristics such as fault width, length, slip distribution, and location of the large slip area. To facilitate these uncertainties, many studies on probabilistic tsunami hazard assessment (PTHA) have been conducted with consideration of numerous source scenarios. However, these PTHA studies typically consider fixed subfault geometry. In addition, subfault depths are mostly based on geological surveys or analysis on historical earthquake events but the results may have some uncertainty. It is important to quantitatively estimate the effect of the uncertainty on tsunami height in coastal areas. This study aims to quantify the sensitivity of fault depth and rake to the coastal tsunami height. The target earthquake source is the subduction zone along the Nankai Trough, conditioned on the southwest of Japan. First, possible ranges of the fault parameters are investigated. The spatial distribution of fault depth is compared using existing two major fault models, Slab2 and the Cabinet Office of Japan. Regarding the rake angle, a statistical analysis is conducted using historical earthquake catalogs. Second, the numerical tsunami simulation for many hypothetical source models is conducted. The numerical model is based on the nonlinear shallow water equations. Different eight patterns of fault depth and rake angle with the same slip distributions are considered. Each pattern contains 100 source models with a moment magnitude of 9.1, thus, 800 tsunami simulations in total are performed. Numerical results showed the significant effect of fault depth and rake to coastal tsunami heights along coastal zones of West Japan. At several coasts, the median tsunami heights between 100 scenarios with 5 km deeper faults were more than 1 m larger than those with the original depth of the existing model.


OS06-A014
Tsunamis in Lingding Bay, China, Caused by the 2022 Tonga Volcanic Eruption

Yuchen WANG1#+, Peitao WANG2, Hoiio KONG3, Chan-Seng WONG4
1Japan Agency for Marine-Earth Science and Technology, 2Ministry of Natural Resources, 3City University of Macau, 4Macao Meteorological Society

Tsunamis in Lingding Bay, China, Caused by the 2022 Tonga Volcanic Eruption The Hunga Tonga-Hunga Ha’apai volcano eruption resulted in propagation of tsunamis globally. Atmospheric pressure disturbances and tsunamis were recorded in Lingding Bay, China, situated more than 9000 km from the volcano. We studied the features of tsunamis in Lingding Bay and its surrounding areas by using records from tide gauges and meteorological stations. Lamb waves were observed in the bay approximately 8, 44, and 80 h after the volcanic eruption. The first and second tsunami waves arrived approximately 11 and 45–47 h following the eruption, respectively, indicating consistency with the arrival time of Lamb waves. In addition, wavelet and Fourier analyses were applied to the sea level records to investigate the frequency characteristics. The ratio of the tsunami spectra to the background spectra for two tsunami waves was calculated as the source spectra. The source spectra of two tsunami waves were mostly of the same shape, with dominant periods of ~17 and ~46 min. This is the first study that investigates the features of a real tsunami event in the Lingding Bay region. It also provides information for the theoretical investigation of tsunamis caused by the Tonga volcanic eruption. This study was published by Geophysical Journal International (doi:10.1093/gji/ggac291). It was highlighted by the Royal Astronomical Society on September 20, 2022: https://ras.ac.uk/news-and-press/research-highlights/hunga-volcano-special-issue-gji-analysis-tsunamis-lingding-bay.


OS06-A046
The Characteristics of Tsunami Waves Generated by Submarine Landslides: Case Studies in the South China Sea

Xiaoyi PAN1+, Linlin LI2#, Huabin SHI1, Zhiyuan REN3
1University of Macau, 2Sun Yat-sen University, 3Northwestern Polytechnical University

The common detection and analysis of tsunami signals generally rely on tide gauges in the nearshore and DARTs in the deep sea. Compared to the earthquake-generated tsunami, the characteristics of landslide-generated tsunamis is difficult to be distinguished due to the complexity of the landslide motion and local bathymetric effect. Previous studies usually justify the landslide-generated wave signals by their short periods (2-15 min) and the time of occurrence. However, the periods of landslide-generated tsunami waves are greatly affected by multi factors of the source landslides (e.g. lengths, widths, slide materials) as well as local bathymetries. In this study, we investigate the characteristics of tsunami waves generated by submarine landslides through waveform analysis. We first collect and examine historical waveform records of tsunami events with presumable landslide tsunami signals (e. g. the 1998 Papua New Guinea tsunami and the 2011 Tohoku tsunami event). We then use a combined modeling approach: NHWAVE and FUNWAVE to numerically simulate 3 representative submarine landslides in the South China Sea (SCS): the Baiyun slide, the Zengmuansha (Brunei) slide and the 109 meridian slide and investigate wave characteristics at different water depths. Virtual gauges are specified at 20 m, 200 m and 1000 m contours. We conduct spectra analysis of waveforms recorded by these synthetic gauges to obtain the wave periods generated by different scenarios. It is shown that the tsunami wave periods in deep water interrelate closely with the dynamic sliding process, which offer references for identifying possible landslide tsunami signals.


OS06-A015 | Invited
Finite Fault Model of the 2009 Samoa Earthquake Estimated from Simultaneous Inversion of Ocean-bottom Pressure and Electromagnetic Tsunami Records

Toshitaka BABA1#+, Hiiro YOKOI1, Zhiheng LIN2, Takuto MINAMI3, Hiroaki TOH4
1Tokushima University, 2The Institute of Statistical Mathematics, 3Kobe University, 4Kyoto University

On 29 September 2009, a magnitude 8.0 earthquake, the 2009 Samoa earthquake, occurred in the southern Pacific Ocean adjacent to the Tonga Trench subduction zone. This was a doublet earthquake initiated as a normal-faulting event seaward of the trench axis followed by a thrust-faulting event on the subduction zone interface close to the trench axis. Ocean-bottom pressure and electromagnetic meters deployed in the Pacific Ocean recorded the tsunami caused by this earthquake. Although tsunami inversion analysis generally uses only ocean-bottom pressure data, we also used ocean-bottom electromagnetic data to estimate the slip distribution of the 2009 Samoa earthquake. Our joint inversion of pressure and electromagnetic data was the first time to our knowledge. The electromagnetic fluctuation was converted to sea level fluctuation using an analytical solution. The background noise level of the converted sea level (5.2 mm in RMS) was larger than that of ocean-bottom pressure observations (0.5 mm). Based on the noise level, we determined the weight between these datasets in the joint inversion. We also included frequency dispersion and self-attraction and loading effects in the tsunami propagation calculations, allowing the use of tsunami waveforms recorded at distant locations. In the obtained finite fault model, the significant slip on the normal fault appeared near the epicenter. The slip zone on the thrust fault extended north–south direction on the shallower part of the fault plane. The large slip area on the thrust fault was narrower in the east–west direction than that estimated from pressure and tide gauge data in a previous study. Our slip model well explained both electromagnetic and pressure data from the 2009 Samoa tsunami.


Tue-01 Aug | 10:20 - 12:20 | MR328
OS03 - Seasonal-to-interannual Climate Variability and Predictability

Session Chair(s): Takeshi DOI, Japan Agency for Marine-Earth Science and Technology, Chaoxia YUAN, Nanjing University of Information Science & Technology

OS03-A019 | Invited
Impacts of Oceanic Mesoscale Structures on Simulating Sea Surface Temperature in the Arabian Sea and Indian Summer Monsoon

Yoko YAMAGAMI1#+, Hiroaki TATEBE1, Takahito KATAOKA1, Tatsuo SUZUKI1, Masahiro WATANABE2
1Japan Agency for Marine-Earth Science and Technology, 2The University of Tokyo

A cold bias in the sea surface temperature (SST) of the Arabian Sea remains in recent climate models. Since the SST in the Arabian Sea plays a critical role in simulating the Indian monsoonal rainfall, it is required to deepen the understanding of the processes that impact the Arabian Sea SST. This study investigates the effects of mesoscale oceanic variability on both the Arabian Sea SST and the Indian summer monsoon precipitation through coupled climate model experiments, including non-eddying and eddy-permitting ocean components.
In the eddy-permitting configuration, mesoscale variability transports warm water to the Arabian Sea, leading to an increase in the western Arabian Sea SST of up to 1.6°C. The lateral eddy heat advection enhances the warm water outflows from the Red Sea and Persian Gulf and suppresses the surface temperature cooling due to the coastal upwelling during the summer monsoon season.
The eddy-permitting configuration demonstrates a decrease (increase) of summer precipitation over the southeastern Arabian Sea (western and northern India). The increased SST in the western Arabian Sea may contribute to the precipitation difference and the formation of cyclonic wind anomaly over the northern Arabian Sea, which further amplifies wind convergence and precipitation in northwestern India. The AGCM sensitivity experiments suggest that the change in the precipitation pattern is partially attributed to changes in the Arabian Sea SST.
To examine the role of topography on the Arabian Sea SST and the Indian summer monsoon, we also performed two simulations using the non-eddying configuration, one including and one excluding the Persian Gulf and Red Sea. The results show that the presence of the Persian Gulf and Red Sea accounts for less than 50% of the SST increase in the western Arabian Sea seen in the eddy-permitting configuration and less increase in precipitation is observed in western India.


OS03-A006
On the Predictability of the Extreme Drought in East Africa During the Short Rains Season

Takeshi DOI#+, Swadhin BEHERA, Toshio YAMAGATA
Japan Agency for Marine-Earth Science and Technology

We have been developing a dynamical seasonal prediction system based on a climate model called the Scale Interaction Experiment-Frontier ver. 2 (SINTEX-F2) under the EU–Japan collaborative framework. It has demonstrated high skills in the prediction of climate phenomena in the tropical Pacific and Indian Oceans (e.g., El Niño/Southern Oscillation (ENSO), ENSO-Modoki, and Indian Ocean Dipole events) and their teleconnections. Encouraged by the performance, we further explored the predictability of drought in East Africa during the short rains season of 2021. Many parts of East Africa experienced extremely dry conditions during the short rains season of October–December of this year. Interestingly, this was predicted a few months earlier by the 108-member ensemble seasonal prediction system based on the SINTEX-F climate model. Based on the co-variability of inter-member anomalies, we found that the 108-member ensemble prediction system has an advantage in finding possible co-variability patterns influencing predictions of precipitation, in which the signal-to-noise ratio is low relative to predictions of temperature. This analysis demonstrates that the 2021 negative Indian Ocean Dipole was responsible for the unusually dry conditions over East Africa. We also developed a hybrid statistical-dynamical framework that was found to be more skillful than the original SINTEX-F model at predicting drought in East Africa for a longer lead time. We hope this added predictability will help people take the necessary mitigation measures to reduce the devastating impact of the drought.


OS03-A015
Characteristics of the Interannual Variability of the Significant Wave Height in Bay of Bengal

Shaotian LI#+, Yineng LI, Shiqiu PENG
Chinese Academy of Sciences

The ocean surface waves play an important role in the oceanic variability, which help to control the energy flux between atmosphere and ocean and the upper ocean mixing, and further influence the climate change. The spatio-temporal variations of the significant wave height (SWH) in the Bay of Bengal (BOB) region, as well as their driving mechanisms, are investigated based on the long-term (1981-2019) simulation by a WAVEWATCH III model. We apply the EOF and EEMD methods to the boral summer (June to August) and winter (December to January in the next year). In winter, the SWH of notable variability occurs in the west BOB, accounting for 43.98% of the variability. It is associated with El Nino-Southern Oscillation (ENSO) event at an interannual scale and has a significant increasing trend. The 2nd mode of the EOF (21.77%) shows a dipole pattern and is regulated by the sea surface temperature of the east region of Indian Ocean Dipole (IOD). In summer, the 1st Principal component (PC1) of the SWH variability, accounting for 56.38%, significantly correlates with the Southeast Asian Summer Monsoon (SEASM) over the Southeast Asia. The SEASM dominates the variability of the SWH in summer.


OS03-A004
Understanding Extremely Pluvial Winters Over Yangtze–Huai River Basin in China: Their Complexity and Tropical Oceans Influences

Jiaying HE1#+, Jing-jia LUO1, Takeshi DOI2
1Nanjing University of Information Science & Technology, 2Japan Agency for Marine-Earth Science and Technology

In 2018/19 winter, the Yangtze–Huai River Basin (YHRB, one of the most developed areas in China) experienced an extremely pluvial condition with excessive and long-duration precipitation. Other three extremely pluvial winters during 1979/80–2018/19: 1997/98, 2002/03 and 1989/90 winters were also found. In 2018/19, 2002/03 and 1997/98 winters, similar low-level circulation pattern of anomalous southwesterlies (southeasterlies) over the southern (northern) YHRB was found. However, we found different tropical ocean states for the events. In 2018/19 winter, a combination of a moderate El Niño in the tropical Pacific and warm sea surface temperature (SST) anomalies in the tropical western Indian Ocean (IO) and Atlantic was seen. In 1997/98 winter, we found an extreme eastern Pacific El Niño with warm SST anomalies in the western tropical IO. In 2002/03 winter, a central Pacific El Niño occurred. In contrast, no significant warm SST anomalies were seen in 1989/90 winter. Based on coupled model numerical experiments, the tropical SST anomalies contributed almost half of the YHRB precipitation anomalies in 2018/19 and 1997/98 winters. In particular, the tropical IO warm SST anomalies induced anomalous anticyclones over the South China Sea and northeastern China, with moisture convergence over the YHRB. In 2002/03, the tropical Pacific SST anomalies contributed almost half of the YHRB precipitation anomalies, although its contribution could be reduced due to the inter-basin interactions. For 1989/90 winter, we discussed possible impacts of mid-high latitude wave trains. The results indicate the complexity and diverse potential predictability among the four extreme pluvial winters.


OS03-A005
Delayed Impacts of ENSO on the Frequency of Summer Extreme Hot Day in the Asian Monsoon Region and Its Implication for Seasonal Prediction

Xinyu LU#+, Chaoxia YUAN
Nanjing University of Information Science & Technology

Understanding and predicting extreme weather and climate are ultimately important for adaptation and resilience. Here, we assess the prediction skills of frequency of summer extreme hot day (SEHD) in the Asian monsoon region (AMR) by using the 1981-2014 hindcasts of POAMA-2 subseasonal-to-seasonal prediction system. Generally, the good prediction skills of SEHD frequency appear in the southern AMR south of 30˚N including the Indian subcontinent, Indo-China peninsula and the Philippines; the anomaly correlation coefficients between the observed and predicted region-mean SEHD anomalies are 0.72, 0.72, 0.70, 0.60, 0.61 and 0.61 at 6-1 month lead, respectively, all statistically significant at the 99.9% confidence levels. The high prediction skills in the POAMA-2 are due to its capacity on reproducing the observed delayed ENSO impacts on the large-scale atmospheric circulation, the seasonal surface air temperature and thus the SEHD frequency in the southern AMR via provoking the Indo-western Pacific ocean capacitor effect. Since the POAMA-2 only provides the prediction at most half a year in advance, we also conduct the hindcasts in the SINTEX-F that can reproduce well the robust ENSO-SEHD relationship and has high prediction skill of ENSO itself. Results show that skillful prediction of the region-mean SEHD frequency can be up to 14 months in advance.


OS03-A021 | Invited
Eastward Shift of Interannual Climate Variability in the South Indian Ocean Since 1950

Lei ZHANG1#+, Weiqing HAN2, Kristopher KARNAUSKAS2, Yuanlong LI3, Tomoki TOZUKA4
1South China Sea Institute of Oceanology, 2University of Colorado Boulder, 3Chinese Academy of Sciences, 4The University of Tokyo

The subtropical Indian Ocean dipole (SIOD) and Ningaloo Niño are the two dominant modes of interannual climate variability in the subtropical south Indian Ocean. Observations show that the SIOD has been weakening in the recent decades, while Ningaloo Niño has been strengthening. In this study, we investigate the causes for such changes by analyzing climate model experiments using the NCAR Community Earth System Model, version 1 (CESM1). Ensemble-mean results from CESM1 large-ensemble (CESM1-LE) show that the external forcing causes negligible changes in the amplitudes of the SIOD and Ningaloo Niño, suggesting a dominant role of internal climate variability. Meanwhile, results from CESM1 pacemaker experiments reveal that the observed changes in the two climate modes cannot be attributed to the effect of sea surface temperature anomalies (SSTA) in either the eastern tropical Pacific Ocean or tropical Indian Ocean. By further comparing different ensemble members from the CESM1-LE, we find that a warm pool dipole mode of decadal variability, with opposite SSTA in the southeast Indian Ocean and the western-central tropical Pacific Ocean plays an important role in driving the observed changes in the SIOD and Ningaloo Niño. These changes in the two climate modes have considerable impacts on precipitation and sea level variabilities in the south Indian Ocean region.


OS03-A009
ENSO–IOD Inter-basin Connection Is Controlled by the Atlantic Multidecadal Oscillation

Jiaqing XUE1#+, Jing-jia LUO1, Wenjun ZHANG1, Toshio YAMAGATA2
1Nanjing University of Information Science & Technology, 2Japan Agency for Marine-Earth Science and Technology

The interactions between El Niño-Southern Oscillation (ENSO) and Indian Ocean Dipole (IOD) are known to have great implications for global climate variability and seasonal climate predictions. Observational analysis suggests that the ENSO–IOD inter-basin connection is time-varying and related to the Atlantic Multidecadal Oscillation (AMO) with weakened ENSO–IOD relationship corresponding to AMO warm phases. A suite of Atlantic pacemaker simulations successfully reproduces the decadal fluctuations in ENSO–IOD relationship and its link to the AMO. The warm sea surface temperature (SST) anomalies associated with the AMO drive a series of Indo-Pacific mean climate changes through tropical-wide teleconnections, including the La Niña-like mean SST cooling over the central Pacific and the deepening of mean thermocline depth in the eastern Indian Ocean. By modulating ocean–atmosphere feedback strength, those mean state changes decrease both ENSO amplitude and the Indian Ocean sensitivity to ENSO forcing, therefore decoupling the IOD from ENSO.


OS03-A007
Weakening of the Indian Ocean Dipole in the Mid-Holocene Due to the Mean Oceanic Climatology Change

Shanshan LIU1#+, Chaoxia YUAN1, Jing-Jia LUO1, Xiaofan MA1, Xuecheng ZHOU2, Toshio YAMAGATA3
1Nanjing University of Information Science & Technology, 2Meteorological Service Center of Jiangsu Province, 3Japan Agency for Marine-Earth Science and Technology

The Indian Ocean Dipole (IOD) is one of the leading modes of interannual climate variability in the tropical Indian Ocean (IO). Understanding variations in the IOD and its relationship to the altered background mean state can advance our knowledge of tropical climate dynamics. Paleoclimate provides the opportunity to address this issue under real climate scenarios in the past. Based on 18 models from the Paleoclimate Modelling Intercomparison Project phase 3 and 4 (PMIP 3/4), we investigate IOD changes during the mid-Holocene compared to the preindustrial period. The multimodel mean reveals that the IOD variability weakens by 14% as measured by the standard deviation of the Dipole Mode Index, which is defined using the zonal sea surface temperature (SST) difference. Such attenuation is dominated by the spatially consistent suppression in the western-pole SST variability, while the eastern pole contributes little due to the opposite-signed changes in its northwestern and southeastern portions. The primary reason for the aforementioned changes comes from the altered climatic background, which displays a positive IOD-like pattern during IOD growing seasons, with intensified westward currents along the equator and northwestward currents in the southeastern equatorial IO. Such changes in the mean-state currents modulate the strength of the IOD-related anomalous advection and subsequently cause alterations in the IOD variability. Further analyses show that the IOD attenuation in the mid-Holocene is likely irrelevant to the concurrently subdued El Niño–Southern Oscillation in the tropical Pacific because of the diminished connections between the two oscillations themselves. The above simulated changes in both the IO mean climatology and IOD variability agree well with the available paleo-records in literature.


Tue-01 Aug | 10:20 - 12:20 | MR332
OS01 - Tropical Cyclone-ocean Interactions: from Weather to Climate

Session Chair(s): Chunzai WANG, Chinese Academy of Sciences, Lei ZHOU, Shanghai Jiao Tong University

OS01-A004
Recent Increases in Tropical Cyclone Rapid Intensification Events in Global Offshore Regions

Youmin TANG1#+, Yi LI1, Shuai WANG2, Ralf TOUMI3, Xiangzhou SONG1, Qiang WANG1
1Hohai University, 2Princeton University, 3Imperial College London

Rapid intensification (RI) is an essential process in the development of strong tropical cyclones and a major challenge in prediction. RI in offshore regions is more threatening to coastal populations and economies. Although much effort has been devoted to studying basin-wide temporal-spatial fluctuations, variations of global RI events in offshore regions remain uncertain. Here, we show that compared with open oceans, where the annual RI counts do not show significant changes, offshore areas within 400 km of the coastline have experienced a significant increase in RI events, with the count tripling from 1980 to 2020. Furthermore, this consequential landward variation was found to stem from changes in global ocean warming, tropical cyclone potential intensity, and large-scale climate variability. This work yields an important new finding that an increasing threat of RI in coastal regions has occurred in the preceding decades, which may continue in a future warming climate.


OS01-A007
Seasonal Variation of Tropical Cyclone-induced Sea Surface Cooling in the Western North Pacific

Vineet Kumar SINGH+, Il-Ju MOON#
Jeju National University

The impact of tropical cyclones (TCs) on sea surface temperature (SST) cooling is a crucial factor in determining the intensity of TCs in the western North Pacific. This study aims to investigate the seasonal variation of TC-induced SST cooling, specifically comparing summer (June–August) and autumn (September–November) for the period 1982–2021. The findings show that, despite a higher mean TC intensity in autumn (89.9 knots) compared to summer, the average maximum TC-induced SST cooling in autumn is only -0.47°C, which is 30% lower than the cooling observed in summer. This is due to a deeper mixed layer depth, weaker thermal gradient in the ocean sub-surface and a shift of TC tracks towards the equator in autumn, which prevent the entrainment of cooler subsurface water and result in lower SST cooling. Since, TC-induced SST cooling has negative feedback on TC intensity, these results can partly explain the seasonal differences in the TC intensity in this basin. This is a novel contribution to the understanding of the underlying mechanisms behind the seasonal variability of TC-induced SST cooling in the basin. Funding Information: This research was supported by “Development of technology to support and utilize numerical forecasting” funded by the Korea Meteorological Administration and “Study on Northwestern Pacific Warming and Genesis and Rapid Intensification of Typhoon” funded by the Korean Ministry of Oceans and Fisheries (20220566)”.


OS01-A009
Stage-dependence of Tropical Cyclone Seeds and Their Future Change

Jung-Eun CHU1#+, Timmermann AXEL2, Pavan Harika RAAVI2, Sun-Seon LEE3, Johnny CHAN4,1, Hung Ming CHEUNG1, Minhee CHANG5
1City University of Hong Kong, 2Center for Climate Physics, Institute for Basic Science, 3IBS Center for Climate Physics, 4Asia-Pacific Typhoon Collaborative Research Center, 5Korea Institute of Science and Technology

Tropical cyclones (TCs), the generic name for typhoons, are among the most destructive natural hazards. It is important to understand how climate change affects TC frequency, to minimize human and economic losses. However, the origin of the TCs from the initial precursory vortex called a TC seed, and their survival rate (i.e., the proportion that successfully develops into TCs) are not well understood. Key challenges are mainly due to a lack of consensus in TC seed definition and a lack of computing resources for TC modeling. This study aims to meet the above challenges, through the following tasks: (1) to identify the representation of TC seeds and survival rate based on three different stages: early-, intermediate- and mature-stage definitions; (2) to investigate the contribution of TC seeds and survival rate to future changes in TC genesis using a high-resolution fully-coupled Community Earth System Model (CESM) simulations. Experiments with fixed CO2 concentrations under present-day, doubling, and quadrupling conditions with an atmospheric resolution of 0.25° and an ocean resolution of 0.1° were used. Our results show that the spatial distributions of the TC seeds and survival rate largely depend on the different stages of the seed definition. TC seeds defined by early-stage definition show more equatorward distribution with a strong connection to vertical velocity, while those defined by intermediate- and mature-stage are located 2-5° poleward. In response to greenhouse gas warming, TC seeds obtained by all three definitions exhibit a statistically significant reduction in the frequency of TC seeds while the survival rate remains unchanged. This study is the first to examine the sensitivity of TC seeds and survival rate to various stages of the definition and their future change using the highest resolution fully coupled model global warming simulations.


OS01-A006
Tropical Cyclone-induced Inertial and Sub-inertial Motions Observed by High-frequency Radar

Jun WEI1#+, Tianyi LU1, Langfeng ZHU1, Dong-Ping WANG2
1Sun Yat-sen University, 2Stony Brook 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.


OS01-A022
What Caused the Increase of Tropical Cyclones in the Western North Pacific During the Period of 2011-2020?

Haili WANG1+, Chunzai WANG2#
1SCSIO, 2Chinese Academy of Sciences

Based on satellite data after 1979, we find that the tropical cyclone (TC) variations in the Western North Pacific (WNP) can be divided into three-periods: a high-frequency period from 1979 to 1997 (P1), a low-frequency period from 1998 to 2010 (P2), and a high-frequency period from 2011 to 2020 (P3). Previous studies have focused on WNP TC activity during P1 and P2. Here we use observational data to study the WNP TC variation and its possible mechanisms during P3. Compared with P2, more TCs during P3 are due to the large-scale atmospheric favorable conditions of vertical velocity, relative vorticity and relative humidity. Warm sea surface temperature (SST) anomalies are found during P3 and migrate from east to west, which is also favorable for TC genesis. The correlation between the WNP TC frequency and SST shows a significant positive correlation around the equator and a significant negative correlation around 36°N, which is similar to the warm phase of the Pacific Decadal Oscillation (PDO). The correlation coefficient between the PDO and TC frequency is 0.71, above the 95% confidence level. The results indicate that the increase of the WNP TC frequency during 2011–2020 is associated with the PDO and warm SST anomalies.


OS01-A021
A Transfer-learning-based Deep Learning Model to Locate Tropical Cyclone Centers from Satellite Infrared Imagery

Chong WANG1#+, Xiaofeng LI2
1Institute of Oceanology, 2Chinese Academy of Sciences

This paper developed a deep learning (DL) model based on transfer learning (TL) for locating tropical cyclone (TC) centers from satellite infrared images observed by the Himawari-8 geostationary satellite. We collected 97 TC cases from 2015 to 2018 over the Northwest Pacific to train, validate and test the TC center location model. The Best Track dataset for TCs provided by the China Meteorological Administration (CMA) was used to label TC images. First, the ResNet model was trained to locate the TC center, and the mean location error (MLE) of the ResNet model is 34.5 km. Second, the attention mechanism and residual fully-connected modules were added to the ResNet model, and the MLE of the improved ResNet model is 34.1 km. Third, the TL is used to improve the TC center location accuracy. The TL method consists of two steps: first, obtain a pre-trained model with the Imagenet data and then fine-train the pre-trained model with TC data. Compared to the ResNet model without TL, the ResNet model with TL has a 14.1% performance improvement. In addition, the ResNet model with TL has less MLE than the ResNet model without TL in TS (17.1 m/s - 32.4 m/s), H1 (32.5 m/s - 42.2 m/s), H2 (42.3 m/s - 48.9 m/s), H3 (49.0 m/s - 57.6 m/s), H4 (57.7 m/s - 70.0 m/s), and H5 (> 70.0 m/s) intensity categories. For example, the MLE of the ResNet model with TL is 29.3 km, less than 20 km for H2-H5 intensity categories. In addition, the model visualization results show that the ResNet model with TL can better capture TC center-related features, such as TC eye, TC profile, etc.


OS01-A017
Tropical Cyclogenesis Bias Over the Central North Pacific in CMIP6 Simulations

Yi-Peng GUO#+
Nanjing University

Current coupled climate models contain large biases in simulating tropical cyclogenesis, reducing the confidence in tropical cyclone (TC) simulations and projections. 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. Positive TC genesis biases were found over the tropical Central North Pacific (CNP) in most of climate models, including the high-resolution models. A warm SST bias over the tropical CNP in the coupled models is the main cause of TC genesis biases. We showed that 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 generation over the CNP. The current results highlight the importance of understanding the SST-related TC simulation biases in state-of-the-art climate models, which sheds light on reducing model biases and improving confidence in future projections.


Tue-01 Aug | 1:10 - 3:10 | MR308
OS06 - Coastal Hazards: Impacts of Tropical Storms and Tsunamis

Session Chair(s): Linlin LI, Sun Yat-sen University, Yuzhu Pearl LI, National University of Singapore

OS06-A050 | Invited
Short- and Long-term Tsunami Hazard Assessment Based on Deterministic and Probabilistic Methods

Yong WEI1,2#+, Vasily TITOV3,4, Christopher MOORE2, Eddie BERNARD2
1University of Washington, 2NOAA Pacific Marine Environmental Laboratory, 3National Oceanic and Atmospheric Administration, 4University of Colorado

At the NOAA Center for Tsunami Research (NCTR), we usually consider two types, short-term and long-term, tsunami hazard assessments. The goal of a short-term hazard assessment is to address real- or near-real-time forecasting of tsunami inundation caused by a specific event in progress. Examples of the short-term hazard assessment include the flooding forecast capability based on the DART data assimilation, and the quick flooding model forecast in the near field assembled during a progressive tsunami. A long-term tsunami hazard assessment, however, is the use of the best-available high-resolution model to identify the long-term, potential impact of tsunami hazards for a coastal community at risk. It is usually based on well-established knowledge of history of the tsunami impact at an interested site. NCTR’s tsunami modeling capability is well recognized in many tsunami hazard assessment projects (Figure 1) that are supported domestically by state and federal stakeholders in the United States, as well as internationally through the United Nations’ Intergovernmental Oceanographic Commission (IOC). In this study, we highlight NCTR’s research in short- and long-term tsunami hazard assessments using both the deterministic and the probabilistic methods, along with a path of two-decade development of deep-ocean observational and modeling technologies within and outside NOAA. These efforts have largely contributed to tsunami inundation forecasting at the NOAA’s Tsunami Warning Centers (TWCs), the National Tsunami Hazard Mitigation Program (NTHMP)’s goal of Tsunami-Ready societies, and as well to the establishment of first national and international provision on tsunami load and effect.


OS06-A019
Tsunami Simulation of River-run-up Using High-resolution Topographic Data

Yuta NIIMI#+, Toshitaka BABA
Tokushima University

Numerical tsunami calculations require digital topographic data. We generally survey land and sea topography separately and making continuous topographic data at the land-sea boundary is demanding. In recent years, advances in surveys using green lasers have enabled it to obtain continuous, high-resolution topographic data at the boundaries between land and sea. In this study, we conducted a tsunami simulation of river run-up using high-resolution topographic data measured by green laser to determine how much detailed resolution is needed to predict river run-up tsunamis accurately. This study used the open-source tsunami simulation code (JAGURS, Baba et al., 2015). To verify the accuracy of the JAGURS model, we compared the JAGURS simulation with the analytical solution of Carrier (1991). We computed the tsunami waveforms on a two-dimensional horizontal floor in two cases, Case01 L=85.8 km and Case02 L=343 km, where L is the initial wavelength. The waveforms calculated by linear dispersive wave equations of JAGURS matched the theoretical waveforms. The spatial resolution of the green laser data we used was 50 cm, which is more than ten times higher than the spatial resolution used in tsunami hazard maps. We created five topographic datasets with grid spacing of 0.5 m, 5.0 m, 7.5 m, 10 m, and 15 m to clarify the difference in the calculated tsunami waveforms in a river. We calculated a tsunami running up a river using nonlinear long-wave equations. The tsunami source came from the anticipated source model for the great Nankai earthquake proposed by the Cabinet Office, Japan. The results showed that the grid with the coarser spacing underestimated the tsunami amplitude. However, the computed waveforms using the 5 m and 0.5 m topographic grids were almost identical. Accordingly, the grid spacing of 5m is sufficient for accurately predicting tsunami propagation on the river.


OS06-A044
On the Tsunami Resonance in the South China Sea

Zhiyuan REN1#+, Yuchen WANG2, Xi ZHAO3, Hua LIU3
1Northwestern Polytechnical University, 2Japan Agency for Marine-Earth Science and Technology, 3Shanghai Jiao Tong University

In this study, we investigated tsunami resonance and multiscale standing waves generated by a potential extreme tsunami in the South China Sea (SCS). The nonlinear shallow water equation model was adopted to model tsunami propagation. Then, the sea surface elevation during 24 h following the earthquake was used for spectral analysis. The edge waves and standing waves could be identified due to tsunami oscillations. The numerical results indicated that standing waves between 29 and 256 min were the dominant wave modes in the SCS. Spectral analysis at different spatial scales indicated wave trapping and tsunami resonance over the continental shelf and along the coast. The tsunami resonance modes induced by the potential extreme tsunami reveal information regarding energy concentrations and long-lasting tsunamis in the coast. This study provides a novel perspective for identifying at-risk regions in tsunami hazard assessment.


OS06-A045
Nearshore Tsunami Height Probability Around the Pearl River Estuary

Xiaojing NIU#+, Xingyu GAO, Guangsheng ZHAO, Feng MA
Tsinghua University

This study aims to quantify the probability of the peak nearshore tsunami elevation (PNTE) around the Pearl River Estuary posed by the earthquakes along the Manila Trench. An approach for probabilistic tsunami hazard assessment has been introduced. The procedure to obtain the probability of PNTE is divided into three steps: 1) To compute the joint probability density of tsunami period and height at offshore sites, based on the numerical simulation of millions of potential earthquake scenarios; 2) To calculate the coastal amplification factor at each nearshore point, considering the effect of wave period, height and tidal level. 3) To estimate the exceedance probability of PNTE at each nearshore point based on the offshore boundary condition and the amplification factor. Tsunami waves caused by 1,380,000 potential earthquake scenarios along the Manila Trench have been effectively simulated using the previously proposed superposition method. The assessment considers the randomness of event occurrence time and the variation of tidal level. Two approaches are proposed to calculate the PNTE considering the effect of tide. One approach is a linear superposition of tsunami wave upon the tidal level, and the other considering the influence of tidal level on tsunami nearshore amplification. The results considering the effect of tide show that the PNTE corresponding to short return period is obviously larger than that based on the mean sea level, but no obvious difference in the case of long return period. Moreover, in the study area, the two approaches considering the effect of tide show only slight difference in estimating the probability of PNTE, which suggests the applicability of the linear superposition method in nearshore tsunami hazard assessments.


OS06-A063
Turbulence-resolving Simulations of Bottom Boundary Layers Under Tsunamis

Asim ONDER1#+, Philip Li-Fan LIU2
1National Sun Yat-sen University, 2National University of Singapore

Tsunamis are long shallow water waves that are subject to bottom friction across the ocean basin. Realistic parameterization of these frictional effects is central to operational tsunami forecasting, mitigation efforts and morphological modelling. The bottom drag under a tsunami depends on the characteristics of wave-induced boundary-layer flow and hydrodynamic roughness. Due to the enormous scale and rarity of the tsunami events, very little is known about these fundamental properties. Reynolds-averaged models where turbulence is completely modelled were recently employed to study tsunami boundary layers. However, such turbulence models suffer significant uncertainties due to lack of benchmark data. This study aims to address this limitation using turbulence-resolving simulations. First, billion-points scale direct numerical simulations (DNS) are conducted. Bottom shear stress, roughness functions and turbulent profiles are analysed in detail using DNS data. These datasets are then utilized to develop large-eddy simulation (LES) models which allow the study of tsunami boundary layers in shallower nearshore regions. Using LES, the boundary-layer thickness and bottom shear stress variations are obtained in a wide range of roughness and Reynolds-number regimes. In the final part, the drag results are interpreted in terms of Manning’s roughness coefficient.


OS06-A016
A Coupled Numerical Model of Tsunami-induced Scouring and Seepage Around a Submarine Pipeline

Yuzhu Pearl LI1#, Wen-Gang QI2, Zhengyu HU1+
1National University of Singapore, 2Chinese Academy of Sciences

Tsunami can induce massive sediment motion in the form of bed load and suspended load. It also induces strong pore pressure gradients (or seepage force) in the porous sandy seabed, creating soil instability during the drawdown phase and increasing momentary liquefaction risks in some locations. Experimental studies have been conducted to understand the tsunami induced scour around marine structures e.g. a vertical cylinder (Tonkin et al. 2003) and soil responses (e.g. Yeh and Mason, 2014). At the same time, numerical modelling works have also been performed to simulate tsunami scour (Larsen et al. 2017) around a marine structure. However, none of the modelling works so far have investigated the effect of tsunami-induced seepage in the porous seabed on the scouring process around a marine structure. Li et al. (2020) took the first step to consider the effect of constant upward seepage on scour around a submarine pipeline. However, with tsunami waves, the seepage in the seabed is time-varying. In this study, we will couple the seepage effect induced by the tsunami waves with the sediment transport process. The seepage velocity inside the porous seabed will alter the boundary layer velocity profile and the bed friction velocity at the seabed surface. Meanwhile, with seepage the angle of repose and the threshold of incipient sediment motion for the bed particles are also modified. This will further affect the sediment transport process and the scour patterns around the submarine pipeline. The present model is based on a fully-coupled hydrodynamic and morphologic model (Jacobsen, 2011) and the modified scour-seepage model by Li et al. (2020). Experiments on long waves induced scour around a pipeline will be conducted as a validation of the numerical model. A comparison study on tsunami scour with and without considering the coupled seepage effect will be performed.


OS06-A068
Numerical Simulation of Tsunami-driven Debris Motion Using a 3D Immersed Boundary-Cumulant Lattice Boltzmann Model

Guangwei LIU+, Qinghe ZHANG#, Jinfeng 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.


Tue-01 Aug | 1:10 - 3:10 | MR310
OS03 - Seasonal-to-interannual Climate Variability and Predictability

Session Chair(s): Takeshi DOI, Japan Agency for Marine-Earth Science and Technology

OS03-A024 | Invited
Predicting Multiyear El Niño and La Niña Events in 2-year Long ECMWF Reforecasts

S SHARMILA1#+, Harry HENDON1, Oscar ALVES1, Antje WEISHEIMER2, Magdalena BALMASEDA2
1Bureau of Meteorology, 2European Centre for Medium-Range Weather Forecasts

El Niño-Southern Oscillation (ENSO) is one of largest sources of climate variability, which typically spans over 9-12 months and tends to recur every 2-7 years. However, on occasions, the warm (El Niño) and cold phases (La Niña) of ENSO can last for 2-3 years, exacerbating their length of impacts on regional climate. The most recent example is the ongoing triple-dip La Niña event which has induced persistent rain and widespread flooding in eastern Australia since 2020-21. Given their potential link to prolonged droughts/flooding followed by extensive socioeconomic impacts, understanding and skilful prediction of multiyear ENSO events at sufficient lead time is thus crucial. Our recent study shows that ENSO can be skilfully predicted up to 18 lead-months but the skill beyond the first year is conditioned to the ENSO phase (Sharmila et al. 2023). Here, we further assess the capability of ECMWF SEAS5-20C coupled model in predicting the 1-yr and 2-yr or multiyear ENSO events using the same 110 years of 24-month-long 10-member ensemble reforecasts for the period 1901-2010. We show that the model can predict the duration of back-to-back El Niño events and the first 18-months of multiyear La Niña from onset to persistence from strong El Niña initialised state. However, prediction of multiyear La Niña events are limited from La Niña initialised state. The model also well predicts the differences between 1-yr and 2-yr ENSO event, which appear to be rooted in the initial conditions, particularly in the western Pacific. The role of subsurface processes and subseasonal atmospheric variability in predicting 1-yr and 2-yr ENSO events will be discussed. The emerging results will be valuable for developing operational multiyear ENSO forecasts and to achieve greater confidence in future real-time prediction. [Sharmila et al.(2023) JClim, 36(5):1269-1285].


OS03-A026
The Off-equatorial Southeasterly Winds Create Tropical Inconsistent Air-sea Coupled States During the Development of Second-year La Niña Event

Tingwei CAO#+
Chinese Academy of Sciences

Corresponding to the first-year La Niña event, the anomalous sea surface temperature (SST) is generally weaker while the easterly wind anomalies are evidently stronger, conflicting with the traditional ENSO theory through displaying a stronger Bjerknes feedback process during the second-year La Niña event. It mainly comes from a stronger sensitivity of the zonal wind anomaly to the zonal gradient of sea level pressure (SLP) anomaly, which is caused by the fact that the observed zonal easterly wind anomalies are partly explained by the zonal pressure gradient anomaly in the second-year event. It is the main factor to the development of the SST anomalies during the developing phase. The other part easterly wind anomalies origin from the off-equatorial southeasterly winds over the southeast Pacific which act as the trigger role of the event. Based on the lead regression, the off-equatorial signal emerges two-month lead before the onset of the second-year event, and it is more pronounced in the off-equatorial subsurface layer occupied cold-water, which may serve as an indicator to predict the second-year event.


OS03-A020
Optimal Precursors for Central Pacific El Niño Events in GFDL CM2p1

Zeyun YANG#+
National Marine Data and Information Service

Compared to the canonical eastern Pacific El Niño, the understanding and ability to predict the central Pacific (CP) type event still need further improvement. In this study, the principal component analysis based particle swarm optimization algorithm (PPSO) is applied in Geophysical Fluid Dynamics Laboratory Climate Model version 2p1 (GFDL CM2p1) to obtain the optimal precursors (OPRs) for CP El Niño events, based on the conditional nonlinear optimal perturbation (CNOP) method. For this, three normal years with neither El Niño nor La Niña events, i.e., three cases, are chosen as the reference states. The obtained OPRs for these cases exhibit a consistent positive sea surface temperature (SST) perturbation distribution in the subtropical Northern Pacific (20°–40°N, 175°E–140°W), which is further proven to be crucial for the evolution of CP El Niño based on the northern and southern hemisphere significance test results. Mechanically, these positive SST perturbations are enhanced and reach the equatorial Pacific via wind-evaporation-SST (WES) feedback to evolve into a CP El Niño at the end of the year. The nonlinear approach is adopted to investigate the predictability of CP El Niño events and can shed some lights on future studies.


OS03-A016
Effects of Seasonal Atmospheric Heating on the ENSO Spring Predictability Barrier

Dakuan YU+, Meng ZHOU#
Shanghai Jiao Tong University

The Spring Predictability Barrier (SPB) of the El Niño‐Southern Oscillation (ENSO) phenomenon describes the rapid decrease in the predictability of sea surface temperature anomaly (SSTA) in the eastern tropical Pacific during the spring. Employing statistical methods, previous studies have revealed that the increase in chaotic degrees of the ENSO system in spring is responsible for the SPB phenomenon. However, the underlying inherent physical mechanisms for this SPB are not fully understood. Utilizing the reanalysis data and a Box model for the ENSO dynamics, the strong atmospheric heating process in spring is found to be responsible for causing an increase in chaotic degrees of the ENSO system. The strong atmospheric heating in the eastern tropical Pacific will slow the southerly cross-equatorial winds which cause the strong atmospheric deep convection and weak ocean upwelling in spring. The strong deep convection will enhance the thermodynamic feedback between SSTA and atmospheric heating. The weak upwelling will decrease the thermocline feedback between the zonal SST gradient and upwelling velocity. Results from the ENSO dynamics prescribed by the Box model will reveal a turbulence-like chaotic regime transition that causes the SPB phenomenon in spring.


OS03-A029
Role of Pacific Preconditioning in Modulating the Relationship Between the Spring North Tropical Atlantic SST and the Ensuing El Niño

Sheng CHEN#+, Jiepeng CHEN, Zhuoqi HE, Xin WANG, Ziniu XIAO
Chinese Academy of Sciences

Previous literature has indicated that a spring cold sea surface temperature (SST) anomaly in the North Tropical Atlantic (NTA) could induce an ensuing El Niño event. However, observations show that this relationship is not always robust. For example, the spring cold NTA SST anomalies are not necessarily accompanied by El Niño events in the ensuing winter. Two types of cases are further classified for comparison: a spring cold NTA SST anomaly accompanied by an El Niño (tagged as NTA-El Niño) and a spring cold NTA SST anomaly accompanied by no El Niño (tagged as NTA-Normal). Statistical analysis indicates that Pacific preconditioning acts an important role in modulating the NTA SST and El Niño relationship. The zonal wind anomaly over the eastern subtropical Pacific serves as an important medium linking the spring NTA SST anomaly to the subsequent development of El Niño, and this part of the zonal wind anomaly in spring and summer is largely associated with the preceding winter tropical Pacific SST anomaly. The proposed mechanism is verified by two groups of Coupled General Circulation Models (CGCMs) runs with a weak and strong La Niña condition. Compared with the strong La Niña case, under a weak La Niña case in the previous winter, the spring cold NTA SST anomaly is more capable of modulating the development of the ensuing El Niño event. The present study suggests the importance of Pacific preconditioning while forecasting ENSO with the precursor of the spring NTA SST anomaly.


OS03-A014
Spatiotemporal Features of Tropical Pacific SST: A Comparison of Two Rotated EOF Methods

Juying XU1#+, Chundi HU2, Lifei LIN1, Song YANG1
1Sun Yat-sen University, 2Zhejiang University

Empirical orthogonal function (EOF) analysis results in various modes of the interannual variability of tropical Pacific sea surface temperature (SST), but it can hardly explain the features revealed physically due to the orthogonality constraints. Rotating EOF analysis, on the other hand, is a widely accepted approach to overcome this issue and make the modes easier to interpret. This study compares statistically rotated EOF (REOF) and pairwise rotated EOF (PREOF) analysis to examine the leading two modes and the principle components of interannual variability of tropical Pacific SST. The results show that PREOFs have the advantage of describing the nonlinear evolution of El Niño/Southern Oscillation (ENSO) but underestimate the amplitude of SST anomalies in the eastern Pacific. On the other hand, REOFs capture both the structure and evolution of different flavors of ENSO. Based on the characteristics identified by REOFs, we develop a new pair of ENSO indices (named REPI and RCPI) using a multiple linear regression method. The spatiotemporal features of this pair of indices are highly consistent with those of REOF.


OS03-A013
Joint Effect of the North Pacific Victoria Mode and the Tropical Pacific on El Niño Diversity

Liang SHI1+, Ruiqiang DING2#, Shujuan HU1
1Lanzhou University, 2Beijing Normal University

This study investigates possible mechanisms under what circumstances the North Pacific Victoria mode (VM) is more likely to trigger the eastern Pacific (EP) or central Pacific (CP) El Niño event. Results indicate that while positive VM events can provide the initiates to the onset of El Niño events via forcing initial warming of sea surface temperature (SST) anomalies to occur in the central equatorial Pacific from springtime to summer, the changes in background conditions of the equatorial Pacific at the same period also are crucial contributors to the development of VM-EP or VM-CP El Niño events. That is when we predict the spatial patterns of El Niño events in advance, the extratropical variabilities and changes in the background conditions of the tropical Pacific should be both taken into consideration, rather than considered individually. For VM-EP El Niño cases, the significantly negative SST anomalies from the eastern tropical Pacific experience a fast transition into positive. These SST anomalies are usually accompanied by sign reversal of zonal wind anomalies near the dateline, finally together supplying favorable conditions for the eastward propagation of the initial warming anomalous SST generated by VM event. For VM-CP El Niño cases, there are also negative SST anomalies in the eastern equatorial Pacific, however, they can linger much longer than the former case and transit relatively slow to positive SST anomalies, which together along with the muted anomalous westerlies around the dateline suppress the eastward propagation of the warm SST anomalies generated by VM events. The changes in subsurface water are further in accord with the results in the sea surface. Two simple statistical models for EP and CP El Niño prediction are derived depending on evolutionary features in both the North and tropical Pacific, showing high prediction skills by 2 seasons in advance. 


Tue-01 Aug | 3:30 - 5:15 | MR308
OS06 - Coastal Hazards: Impacts of Tropical Storms and Tsunamis

Session Chair(s): Yu-Lin TSAI, Kyoto University, Masaya TOYODA, Toyohashi University of Technology

OS06-A060 | Invited
Numerical Investigation of Submerged Flexible Vegetation Dynamics and Wave Attenuation Under Combined Waves and Following Currents

Sudong XU#+, Kai YIN, Mengqi LI
Southeast University

Wave attenuation by flexible vegetation is an increasingly significant research area in coastal and ocean engineering. Given the numerical research on flexible vegetation along with the combined waves and currents conditions have received insufficient emphasis, this study seeks to extend the application range of established numerical models to conditions with combined waves and currents, and further quantitatively reveal the effects of colinear following currents on submerged flexible vegetation dynamics and wave attenuation. By comparing with measurement data obtained from previous experimental studies, the reliability of the applied numerical methods in simulating flexible vegetation motions and wave attenuation under combined waves and following currents is confirmed. Scenario simulations illustrate that the Keulegan–Carpenter number and velocity ratio exert substantial nonmonotonic effects on the maximum horizontal force, stem tip excursion, and maximum horizontal stem tip displacement of flexible vegetation. And the presence of following currents can both enhance and suppress the wave attenuation by flexible vegetation. This investigation can broaden the application of the flexible vegetation model and further advance the understanding of wave attenuation by flexible vegetation.


OS06-A006
Parameterization of the Mangrove Shape (Rhizophora Stylosa) for Coastal Disaster Risk Reduction

Nobuhito MORI#+, Che-Wei CHANG
Kyoto 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 data, significant correlations for hydrodynamic modeling were found among the key parameters, such as the trunk diameter at breast height, tree height, prop roots height, and the root system's projected areas. We also discussed the correlation of these representative factors with the tree age. These empirical relationships are summarized for numerical modeling at the end. The limit load of wave conditions for the mangrove is also discussed.


OS06-A056
Experimental and Numerical Investigation of Wave-induced Dynamics of Emergent Flexible Vegetation

Kai YIN#+, Sudong XU, Jianxin HAO, Liuyan MAO
Southeast University

Understanding and modeling the dynamics of flexible vegetation is fundamental to investigating wave attenuation by flexible vegetation, which is fast becoming an essential issue in nature-based coastal defense. Currently, satisfactory development has been achieved in the areas of flexible vegetation dynamics and resulting wave attenuation. However, existing studies are mainly restricted to submerged vegetation and linear wave assumptions. This study aims to propose a new mathematic model to describe the dynamics of emergent flexible vegetation, and investigate the dynamic characteristics of emergent flexible vegetation together with a flume experiment. Hence, a new mechanical model for simulating wave-induced emergent flexible vegetation dynamics is developed by considering the dynamic variation of submergence ratio. Meanwhile, a set of wave flume experiments on emergent flexible vegetation dynamics driven by waves are conducted. Based on experimental measurements, the reliability of the developed model in simulating emergent flexible vegetation dynamics is revealed. Experimental data indicates that emergent flexible vegetation dynamics are influenced by Ursell number, Cauchy number, Excursion ratio, Keulegan–Carpenter number, and Reynolds number. And the correlations between maximum horizontal force and the Keulegan–Carpenter number as well as Reynolds number can be further increased by considering the relative water depth. Simulation results also demonstrate that dynamic variation of submergence ratio has a substantial influence on emergent flexible vegetation dynamics. There is a considerable difference of simulated horizontal force and stem postures in terms of emergent flexible vegetation between the previous submerged flexible vegetation dynamic model and the developed new emergent flexible vegetation dynamic model. The results from this study optimize the simulation theory and method of wave-induced flexible vegetation dynamics, and generate new insights into the dynamic characteristics of emergent flexible vegetation.


OS06-A024
Numerical Investigation of Regular Wave Attenuation and Mangrove Resistance Using Fully-nonlinear Weakly-dispersive Boussinesq-type Model

Yu-Lin TSAI#+, Che-Wei CHANG, Nobuhito MORI
Kyoto University

Mangroves, serving as an eco-friendly solution due to their efficiency in damping wave energy, are getting more attention in protecting coastlines from tsunamis, storm surges, and waves. However, the mechanism behind is relatively less explored, especially the mangrove-induced inertia forces. Thus, to fill this gap, a fully-nonlinear weakly-dispersive Boussinesq-type equation model is used, and both mangrove-induced drag and inertia forces formulated by the Morison-type equation (Morison et al., 1950; https://doi.org/10.2118/950149-g) are considered in the depth-dependent momentum equations. The experiments conducted in the wave flume of PARI (Port and Airport Research Institute), Japan were used to calibrate our model. The 3D-printed Rhizophora mangrove model with props roots was adopted in the experiments, presenting a more factual vegetation model in the laboratory. More experimental details can be found in Chang et al. (https://doi.org/10.1029/2022jc018653). Non-breaking regular waves with a wave-height-to-depth ratio from 0.1 to 0.3 are focused. Wave attenuation within mangroves was first examined between numerical results and experiments. The coefficients of mangrove-induced drag and inertia forces evaluated by the model were later compared with laboratory-measured ones. The spatial distributions of drag and inertia coefficients were also discussed. Moreover, the relationship of Reynolds and Keulegan-Carpenter numbers with mangrove-induced resistance was tested. More details of this study will be presented at the 2023 AOGS conference.


OS06-A030
Effect of Submerged Leafy Vegetation on Regular Wave Attenuation and Cross-shore Profiles Evolution

Shangpeng GONG1,2#+, Jiarui LEI2, Sudong XU1
1Southeast University, 2National University of Singapore

Aquatic vegetation provides a variety of ecosystem services. Our study provides fundamental advances in modelling a key process in water environments, namely the role of aquatic vegetation in protecting shorelines from wave energy and sediment erosion. This study included the creation of the leafy vegetation model and a generalized well-sorted sand beach to evaluate the effect of submerged flexible vegetation on wave attenuation and beach profile morphology response behind it. A set of laboratory flume experiments was conducted, in which instantaneous water depths, flow velocities, and vegetation force were measured in various hydrodynamic conditions. It was found that the measured wave heights experienced a reduction, ranging from 60 % to 78 %, due to the presence of vegetation. Beach profile measurements, with and without artificial vegetation, are taken along the surf zone allowing the analysis of sediment transport under different monochromatic wave conditions. The wave height reduction and characteristics of the erosion profile were used to evaluate the coastal protection efficiency of the vegetation. The earlier wave breaking and more turbulence will happen within the vegetation zone, where distorted waveforms and the higher-order Stokes wave were observed when waves travel to the coast. Besides, the existence of flexible vegetation does not significantly change the type of beach profile after wave action, and the overall shape of the profile after the same wave condition is similar. Compared with the bare beach, when flexible vegetation exists, the scour and silting position of the beach moves towards the shore as a whole.


OS06-A007
Detection of Coasts That Vulnerable to Typhoons Using Long-term Cross-sectional Survey Data: A Case Study of Omotehama Coast, Japan

Masaya TOYODA1#+, Shigeru KATO1, Mieko KATAOKA1, Tomoya SHIMURA2
1Toyohashi University of Technology, 2Kyoto University

The sandy coasts is not only significant as natural embankment, but also plays an important role in comfortable coastal use, and sustainable coastal development is required. However, there are only a few sites that have been observed over a long period of several decades in Japan. In addition, there have not been enough attempts to detect sensitive points to typhoons and to understand the characteristics of typhoons that have a large impact on sandy coasts. This study aims to detect the characteristics of typhoons that lead to erosion of coasts, and sensitive coasts to typhoon by using long-term cross-sectional survey data from 1999 at Omotehama coast in Japan (Takatsuka, Terasawa, Kojima, and Hosoya) and long-term wave simulation results. As a result of analysis, it was found that erosion occurs during typhoons that cause significant wave heights exceeding 4 m on the Omotehama coast. On the other hand, erosion does not occur during relatively small wave heights of about 2.5 m, and that some typhoons have a tendency to sediment. In addition, Hosoya is the most sensitive to typhoon (erosion and sedimentation) in four survey points. Furthermore, Kojima shows a different change trend from the other three points. The Kojima coast is eroded regardless of the characteristics of the typhoon. Therefore, it can be said that the Kojima coast is vulnerable to typhoons. On the other hand, the survey for Kojima started in 2006, and the number of data is less than the other three points. Accumulation of data by continuous surveying is required to understand more robust trends.


OS06-A054
Effect of Density on Wave Forces Under Sediment Laden Tsunamis Based on Three-dimensional Numerical Simulation

Riku TAKAKURA+, Naoki TANIGUCHI, Yota ENOMOTO, Taro ARIKAWA#
Chuo University

The tsunami caused by the 2011 Great East Japan Earthquake contained sediment, and the density of the liquid collected was 1.1g/cm3. According to the FEMA (Federal Emergency Management Agency) guidelines for evacuation of buildings during tsunami, the fluid density of tsunami flow is taken as 1.1 times the density of seawater (ρs=1128 kg/m3). However, the exact mechanism of the wave force of sediment-laden tsunami is still unknown. The current design standard are based on pure water studies for wave forces, so it is necessary to investigate how the inclusion of sediment in a tsunami affects the wave force. In this study, the wave force of sediment-laden tsunami inundation flows was investigated through hydraulic model experiments and numerical simulations. Two types of sediment, silt and sand, were considered in the experiment. In a control experiment, wave forces were measured without any sediment. Numerical simulations were performed using CADMAS-surf3D/2f. It was previously shown that flows containing bentonite and silica sand may exhibit the characteristics of a Bingham fluid. Therefore, a non-Newtonian fluid model with spatially and temporally varying viscosity was used to simulate a sediment-laden tsunami. A comparison of the numerical results with the experimental results confirmed that wave forces were reproduced in the numerical simulation. Furthermore, the sustained wave pressure was larger than that of pure water, which is likely due to the effect of density. Moreover, the impact wave pressure may increase because of viscosity; thus, the maximum- impact wave pressure is greater than the rate of increase in density. The results indicate that it is important to account for the effects of density increase and viscosity when investigating the wave force of sediment-laden tsunamis.


Tue-01 Aug | 3:30 - 5:15 | MR310
OS03 - Seasonal-to-interannual Climate Variability and Predictability

Session Chair(s): Takeshi DOI, Japan Agency for Marine-Earth Science and Technology

OS03-A012
Coherent Interannual-decadal Variability of Potential Temperature in the Tropical-north Pacific Ocean and Deep South China Sea

Yuxin LIN1+, Zhiqiang LIU1#, Zhongya CAI2
1Southern University of Science and Technology, 2University of Macau

This study conducts multivariate empirical orthogonal function analysis on long-term hydrographic observations to attain coherent surface temperature variations in the Tropical (TPO) and Northern Pacific Ocean (NPO) and rationalize the functioning mechanism of the predominant climatic variabilities therein in regulating the undocumented potential temperature variabilities in the deep South China Sea. The extrinsic forcings in the TPO and NPO regulate the interannual-decadal variabilities of potential temperature, through modulating the volume transport in the Luzon Strait, but having no robust relationship with the well-known El Niño-Southern Oscillation (ENSO) and the Pacific Decadal Oscillation (PDO) indexes. On the atmospheric bridge, these extrinsic forcings alter the upper-layered LST through tunning the bifurcation of the North Equatorial Current and the intensity of the western boundary current (Kuroshio) in the NPO. On the oceanic pathway, climatic variabilities overriding the arriving NPO waters disturb potential temperature through altering the deep-layered LST and the vertical motion inside the basin.


OS03-A033
Interannual Changes of the Summer Circulation and Hydrology in the East China Sea: A Modeling Study from 1981 to 2015

Yu-Heng TSENG1#+, Yi-Chun KUO1, Yang YU2
1National Taiwan University, 2Chinese Academy of Sciences

This study investigated long-term interannual changes in summer circulation and hydrology in East China Sea (ECS) by performing 35-year high-resolution ocean model simulation from 1981 to 2015. The sea surface temperature (SST) warming trend was considerably weaker in summer than in winter. To the east of the Yangtze Estuary, the interannual variation of SST in summer was mainly dominated by horizontal advection associated with variations in the Taiwan warm current and heat flux in the offshore region north of the Yangtze Estuary. Baroclinic circulation during summer played a crucial role in subsurface mixing. Near the surface, the significant atmospheric wind mode (EOF1) and Kuroshio mode (EOF2) dominate interannual variations in ocean circulation. In the subsurface, local wind around the Tsushima Strait dominated the interannual ocean variation. Anomalous northeasterly winds induced a southwestward pressure gradient due to topographical confinement. These anomalies propagated to the south along the continental shelf through topographic Rossby waves. This study identified two types of anomalous features based on combinations of surface and subsurface EOFs. The combination represents an in-phase contribution between wind and Kuroshio forcings and between the surface and subsurface circulation that enhances the hydrological variability in the ECS. The implication of the relevant biogeochemical and ecological studies in the East China Sea is also very crucial at the interannual time scale.


OS03-A031
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

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.


OS03-A018
The Subsurface Process to Cause the Seasonal Cycle of the Sea Surface Temperature in the Equatorial Atlantic

Ling QIN#+, Masanori KONDA
Kyoto University

Atlantic Nino (AN) has a significant seasonal phase lock, which coincides with the seasonal cooling of sea surface temperature (SST) from April to August. This coincidence can be an important key to understanding the onset mechanism of AN. We focused on the mechanism to cause the mean annual cycle of temperature in the equatorial Atlantic region. Most previous studies were done based on the one-dimensional mixed layer heat budget, which may ignore the subsurface processes and the spatial connection. In this research, we adopted the heat budget analysis of the whole equatorial Atlantic region, which expanded zonally and included both the mixed layer and the subsurface layer. Results show that the rapid decrease of SST is mostly attributed to the subsurface cooling through the vertical diffusion at the bottom of the mixed layer in the eastern portion. The source of the cold water was found in the South American coastal region, where both the equatorward coastal currents and the effect of the barrier layer due to the freshwater from the Amazon River contributed to subsurface cooling. This subsurface cooling in the western portion transported eastward by the equatorial undercurrent. Eventually, the seasonal cycle of SST in the equatorial Atlantic cannot be explained simply by local processes. A seed of the seasonal decrease of SST from April could be found in the meridional transportation in the western portion, which through an enlarged vertical diffusion in the eastern portion due to the subsurface cooling by the eastward temperature advection. These processes indicate the importance of off-equatorial regions in the seasonal cycle. To clarify the physical processes of AN, it is necessary to investigate the interannual variation of both the local and remote processes which contribute to the seasonal cycle of SST. 


OS03-A022
Understanding the Intermittence of the Boundary Current Synchronization

Rui TANAKA1#+, Tsubasa KOHYAMA1, Shoichiro KIDO2
1Ochanomizu University, 2Japan Agency for Marine-Earth Science and Technology

Recently, the sea surface temperatures of the Kuroshio and the Gulf Stream regions were reported to be synchronized, and named as the Boundary Current Synchronization (BCS). The BCS is believed to exert a widespread impact on midlatitude weather and coastal fisheries, but the synchronization is intermittent with both periods of large and small correlations that exist in observational records and outputs from high-resolution atmosphere-ocean coupled models. In this study, we perform a simple model simulation and data analysis to investigate why there exist periods of strong and weak synchronization. As an idealized model of the BCS, we use a conceptual model of the mid-latitude atmosphere coupled to two oceans with western boundary currents. A series of simulations show that both variations in internal parameters, such as the deformation radius, and external stochastic noise can reproduce the non-stationary nature of the strength of synchronization. This suggests that both changes in background conditions and random forcing can modulate the strength of the BCS. Based on the above-mentioned results, we define the Boundary Current Asynchronization (BCA) index as a measure of asynchronization. The regression map of sea surface temperature on the BCA index exhibits a strong signal in the eastern equatorial Pacific; indeed, the Niño.3 index and BCA index peaked together in 2015/2016 boreal winter, suggesting that the El Niño Southern Oscillation interfered with the synchronization of the two currents. Furthermore, the regression map of sea level pressure on the BCA index exhibits opposite anomalies between the Aleutian Islands and around Iceland, suggesting that the so-called “Aleutian Low-Islandic Low Seesaw” variability may also contribute to the asynchronization in the two basins.


OS03-A030
Changes in the Factors Controlling Northeast Asian Spring Surface Air Temperature in the Past 60 Years

Shanshan FU+, Zhiwei ZHU#, Rui LU
Nanjing University of Information Science & Technology

Exploring the predictability sources of Northeast Asian spring surface air temperature (NEAST) is of great socioeconomic importance. In the present study, three factors that alternately take control of NEAST during different epochs in the past 60 years are identified. Specifically, NEAST was found to be closely associated with the Arctic Oscillation (AO) in 1961–1994 (E1), the rainfall over the tropical Indian Ocean (RIO) in 1995–2004 (E2), and the tripole pattern of North Atlantic sea surface temperature (NAT) in 2005–2020 (E3). During E1, zonally elongated barotropic cyclonic anomalies associated with the negative phase of the AO led to negative NEAST. During E2, negative diabatic heating related to suppressed RIO stimulated a Rossby wave train propagating from the Arabian Sea to Northeast Asia, resulting in barotropic cyclonic anomalies in the region and negative NEAST. During E3, positive diabatic heating anomalies in the extratropical North Atlantic induced by NAT caused two quasi-barotropic Rossby wave trains over the mid-to-high latitudes of continental Eurasia. The Rossby wave trains both ended with a barotropic cyclonic anomaly over Northeast Asia, leading to negative NEAST. Further analyses show that the rapid decline in Arctic sea-ice cover in the Sea of Okhotsk and Bering Sea in the mid-1990s, weakening of the central Asian westerly jet, and enhancement of NAT-related rainfall anomalies around the mid-2000s, were responsible for the changes in the factors controlling NEAST. A physical-based empirical model constructed using the three identified factors and their precursors nicely reproduced and reforecasted the variation in NEAST, outperforming the five dynamical coupled models of ENSEMBLES project.


Wed-02 Aug | 10:20 - 12:20 | MR309
OS10 - General and Multidisciplinary Oceanography

Session Chair(s): Yusuke UCHIYAMA, Kobe University

OS10-A005 | Invited
Relationship Between Global Ocean Mixing and Mesoscale Eddies

GuangHong LIAO#+
Hohai University

Numerous studies have indicated that mesoscale eddies play an important role in diapycnal mixing and drive global water circulation. Although the relationships between eddy surface features and turbulent mixing have been discussed for individual cases of typical eddies, global studies cannot rely on ship-based microstructural measurements. Fine-scale methods have been developed, wherein either the vertical shear of velocity or density strain is used to estimate turbulent mixing. In this study, the turbulent dissipation rate was estimated using strain information from Argo floats trapped in eddies. Spatially averaged estimates revealed the global distribution patterns of the dissipation rates inside the eddies. In addition, the relationships between eddy features (polarity, radius, vertical extent, and aspect ratio) and turbulent dissipation rates were analyzed. Three main conclusions were made from this study. First, turbulent dissipation rates inside anticyclones were generally larger than those inside cyclones. Second, turbulent dissipation rates inside eddies are related to their vertical extent but not to their horizontal scale. For shallow eddies (with a vertical extent less than 250 m for cyclones and 300 m for anticyclones), the deeper the vertical extent, the larger the turbulent dissipation rate. Finally, the relationship between the eddy aspect ratio and turbulent dissipation rate was characterized by skewness. The average turbulent dissipation rate reached a maximum value when the cyclone aspect ratio was approximately 0.007; conversely, no maximum value was reached for anticyclones. This work establishes a correlation between eddy features and turbulent dissipation rates, which will help guide numerical simulations of mesoscale eddies.


OS10-A018
Global Ocean Mesoscale Eddy Atmospheric-oceanic- Biological Interaction Observational Dataset

Changming DONG1,2#+, Lingxiao LIU1
1Nanjing University of Information Science & Technology, 2Southern Marine Science and Engineering Guangdong Laboratory

Amongst the variety of oceanic processes running the gamut of spatiotemporal scales, mesoscale eddies are the most common and often have region-specific characteristics. The large kinetic energy inherent to eddies themselves is a strong modulator of the global climate, ocean circulation, productivity, and freshwater transport. This study uses multi-source satellite remote sensing observation data to construct a multi-parameter eddy dataset for the 1993–2019 period, which differs significantly from a few of previous published eddy datasets that include only basic sea surface eddy physical features. Eddies within the dataset have life cycles of greater than four weeks, and their corresponding sea surface chlorophyll, sea surface temperature, and wind fields are provided. Atmospheric and oceanic variables are used to present a comprehensive picture of a given mesoscale eddy’s impact on the local physical, but also biological environment. The dataset would find immense value in research on mesoscale eddies, their impact on the atmosphere, and related biological processes.


OS10-A025
Chlorophyll Distribution in Global Ocean and Its Influence Mechanism Affected by Mesoscale Eddies

Zhiwei YOU1+, Lingxiao LIU1, Changming DONG1,2#
1Nanjing University of Information Science & Technology, 2Southern Marine Science and Engineering Guangdong Laboratory

Oceanic mesoscale eddies have significant effects on the chlorophyll distribution. Based on the dataset of mesoscale eddies and their matching chlorophyll concentration from satellite remote sensing data, the chlorophyll distribution in the global ocean affected by mesoscale eddies is analyzed using a polar coordinate composition method. The results show that the composite chlorophyll concentration induced by eddies is consistent with the global background concentration, and it is higher in the northern hemisphere than that in the southern hemisphere. Within 1.5 times the eddy radius, the chlorophyll concentration is significantly affected by the eddy, and its difference between the center and the boundary of the cyclone (anticyclone) is about 0.01 (-0.011) mg/m3, but outside of this area, the chlorophyll concentration basically not affected by the eddy polarity, high values occur in the north (east) in the northern (southern) hemisphere. The absolute difference in chlorophyll concentrations inside and outside the eddies is stronger in the Northern Hemisphere, about twice as strong as in the Southern Hemisphere. The mechanisms for generating such features by eddies are discussed.


OS10-A010
Influence of Oceanic Mesoscale Eddy on the Atmospheric Boundary Layer Based on an Idealized Model

Jin-Lin JI1#+, Changming DONG1,2
1Nanjing University of Information Science & Technology, 2Southern Marine Science and Engineering Guangdong Laboratory

Often, numerical models rely on parameterization schemes to represent currently unresolved or insufficiently understood phenomena. The influence of ocean mesoscale eddies on the overlying atmosphere is such a phenomenon. Using the Weather Research and Forecasting (WRF) model, the Regional Ocean Modeling System (ROMS) and the Coupled Ocean-Atmosphere-Wave-Sediment Transport (COAWST) modelling system, this study investigates the influence of idealized oceanic mesoscale eddies on the atmospheric boundary layer (ABL). The idealized model is horizontally homogeneous and set on an f-plane at 35°N. The cyclonic (anticyclonic) eddy causes sea level pressure (SLP) to increase (decrease) and reduces (increases) latent and sensible heat fluxes, surface winds, marine ABL, and atmospheric precipitable water in the coupled and uncoupled cases. Moreover, a momentum budget analysis of the model output shows that the pressure gradient term is the primary contributor to atmospheric momentum balance. Additionally, it should be noted that the SLP adjustment mechanism is important when advection is weak. Comparing the uncoupled and coupled WRF cases, the eddy's effect on atmospheric parameters is more intense in the uncoupled than in the coupled case, which can increase precipitation by 50% and wind speed and heat flux by 20–30%. These results may be potentially important for future parameterizations of mesoscale air-sea interaction processes in numerical model development.


OS10-A016
Wind Stress Work on Eddies in the Northeast Tropical Pacific

Fangyuan TENG1,2+, Changming DONG1,2#
1Nanjing University of Information Science & Technology, 2Southern Marine Science and Engineering Guangdong Laboratory

How atmospheric kinetic energy enters the ocean is one of the most important issues in climate study, which strongly depends on the kinetic condition at the sea surface. Most of previous studies showed that wind stress did negative work on mesoscale eddies, that is so-called ‘eddy killer’. Our recent theortical study shows that the positive wind work on an eddy can be found after the eddy adapts to the wind field. The present talk uses satellite remote sensing wind stress data and vortex data to demonstrate that the wind work on eddies could be positive in the Northeast Tropical Pacific, where the eddies are generated by the wind curl. It is found that the wind work on eddies in this area has seasonal variation characteristics and is related to wind stress curl and eddy polarity, and the wind stress does not always kill eddies. This work will further enhance our understanding of mesoscale air sea interaction processes.


OS10-A007
Growth of Ocean Thermal Energy Conversion Resources Under Greenhouse Warming Regulated by Oceanic Eddies

Tianshi DU1+, Zhao JING1#, Lixin WU1, Hong WANG1, Zhaohui CHEN1,2, Xiaohui MA1, Bolan GAN1, Haiyuan YANG1
1Ocean University of China, 2Qingdao National Laboratory for Marine Science and Technology

The concept of utilizing a large temperature difference (>20°C) between the surface and deep seawater to generate electricity, known as the ocean thermal energy conversion (OTEC), provides a renewable solution to fueling our future. However, it remains poorly assessed how the OTEC resources will respond to future climate change. Here, we find that the global OTEC power potential is projected to increase by 46% around the end of this century under a high carbon emission scenario, compared to its present-day level. The augmented OTEC power potential due to the rising sea surface temperature is partially offset by the deep ocean warming. The offsetting effect is more evident in the Atlantic Ocean than Pacific and Indian Oceans. This is mainly attributed to the weakening of mesoscale eddy-induced upward heat transport, suggesting an important role of mesoscale eddies in regulating the response of thermal stratification and OTEC power potential to greenhouse warming.


OS10-A006
Mesoscale Dynamics and Meridional Eddy Heat Transport in the Sea of Japan

Dmitry STEPANOV#+, Nata KUZNETSOVA
V.I. Il`ichev Pacific Oceanological Institute

This study investigates generation mechanisms of mesoscale dynamics and the role of mesoscale eddies in the meridional heat transport in the Sea of Japan (SJ) from 1990 to 2010, based on retrospective eddy-resolving numerical simulations. The simulated circulation properly reproduced both the SJ major basin-scale currents and mesoscale dynamics features. We confirm mesoscale eddies can significantly deepen isotherms/isohalines up to a hundred meters and transport heat from southern to northern SJ. From winter to spring, the baroclinic instability of the basin-scale currents is a leading generation mechanism of the SJ mesoscale dynamics. In summer, the barotropic instability of the SJ currents dominates in the mesoscale dynamics generation. We found that the meridional heat transport is mainly polewards. As well, we point out different paths of eddy heat transport across the Subpolar Front: along the western and eastern SJ boundaries. Near the Tsugaru Strait, we found an intensive westward eddy heat transport reaching its maximum in the first half of the year and decreasing to the minimum by summer. This study was supported by the Russian Science Foundation N 22-17-00267.


OS10-A021
Evaluating Conventional and New Methods of Estimating Eddy Kinetic Energy

Guidi ZHOU#+, Xuhua CHENG
Hohai University

Eddy kinetic energy (EKE) is a very important quantity of oceanic motions representing the dynamical state of mesoscale eddies and smaller scale processes. Studies on multi-scale interactions between e.g., currents and mesoscale eddies rely on precise estimation of the EKE as part of the energy cycle. However, conventional methods either do not ensure orthogonal scale decomposition and therefore result in an additional energy reservoir besides the EKE and the mean-flow kinetic energy, or mathematically too complex. Here we introduce two new methods to decompose the scales and calculate the EKE: the piecewise Reynolds mean (PREM) and the eddy detection and extraction (EDEX), both time-variant and exact. Being a direct extension of the canonical Reynolds mean method, the PREM evaluates the EKE of a predefined length scale, compromising orthogonality and instantaneity. It does not distinguish mesoscale eddies and other forms of mesoscale energy. The EDEX is based on objective mesoscale eddy detection from satellite altimeter maps, and is adaptive to eddies of different size and shape, without the need of subjectively-chosen partition scale. It includes pure mesoscale eddies. Evaluation based on 27-years of satellite-derived velocity and sea level data showed that the new methods agree well in terms of EKE pattern and correlation, and exhibit some difference to the often-used running mean method (RUM). RMS difference between EKEs of PREM and RUM reaches 50 J/m3 in tropical and midlatitude strong current regions, and the relative difference can be up to over 200% in the tropics and subpolar north Pacific.


Wed-02 Aug | 10:20 - 12:20 | MR310
OS06 - Coastal Hazards: Impacts of Tropical Storms and Tsunamis

Session Chair(s): Kaiyue SHAN, Tsinghua University, Tso-Ren WU, National Central University

OS06-A040 | Invited
A New Realistic Model of Generating Pressure and Wind Fields of Typhoon for Storm Surge Forecasting

Tso-Ren WU#+, Satriana ROGUNA, Jun-Wei LIN
National Central University

In conventional Holland-type models, a typhoon or hurricane is modeled as a symmetric or quasi-symmetric vortex. These symmetric assumptions fit the observation well in deep-ocean areas or areas with flat topography. A tall mountain, however, will cause these models to produce significant errors. In this paper, we aim to create a new weather model for storm surge calculation while only the track and intensity are known for a tropical cyclone, and this model shall be able to present the terrain blockage effect. Because the wind velocity is much faster than the moving speed of the typhoon, the flow field soon transfers from a transition stage into a quasi-steady state. As a result, the weather field is primarily controlled by storm intensity and topography and has less effect from the storm trajectory. This paper presents a new statistical method for generating a realistic weather field based on the location and intensity of the typhoon. We adopted the ERA-5 reanalysis data from the European Centre for Medium-Range Weather Forecasts (ECMWF) with total of 3200 data from 1981 to 2021. ERA-5 reanalysis data were validated against ground observation from Central Weather Bureau (CWB) in Taiwan, including pressure and wind speed gauge data. The storm surge was simulated using the COMCOT-SS model. The results were compared with the tidal gauge data from CWB as well. Excellent comparison results can be seen. After the validation, the ERA-5 data were used as the database to generate the weather field by providing the location and intensity of the typhoon.


OS06-A022
Global Tropical Cyclone Prediction Using Non-hydrostatic AGCM at Various Spatiotemporal Scales and Applicability to Storm Surge Simulation

Tomoki SHIRAI#+, Taro ARIKAWA
Chuo University

Storm surges are driven by tropical cyclones (TCs) and occur in coastal areas around the world. There is a growing interest in storm surge forecasting at various spatio-temporal scales, from days to months ahead, or even decades into the warming future. Global storm surge simulations are generally expensive, but improvements in computer performance are making them feasible (e.g., Shimura et al.,2022). Meanwhile, storm surges are sensitive on the results of TCs in atmospheric global circulation models (AGCM). That means, if TCs in AGCM have large errors, storm surge predictions may not make sense. One of the most important keys is a resolution of AGCM. Although 10 km resolution AGCM would be used in the next few years for global surge prediction, the necessity of downscaling of 10 km AGCM have not been well studied yet. In this study, a 10 km AGCM performance for TC prediction and its applicability to surge simulations were verified. For AGCM, the WRF (Weather Research and Forecasting) model was selected. The advantages of using WRF are that much knowledge has been accumulated on high-resolution TC simulations and that the non-hydrostatic basic equations essential for high-resolution AGCM are employed. In the 10 km AGCM, we confirmed that TC structure was resolved well, compared with the 5km-resolution downscaled run while TC intensity was predicted weaker than that of downscaled run. Using the outputs of AGCM, storm surges were simulated with a model based on the nonlinear shallow water theory. The 10 km AGCM results were then compared with results from other resolution AGCMs (20 km-100 km). We expect that our results will help future global storm surge risk assessments in discussing the best AGCM configuration in terms of both reliability (or accuracy) and computational cost.


OS06-A035
Enhanced Understanding of Tropical Cyclone Intensification Based on a Theoretical Model

Shen ZHONGHUI1+, Xiping YU2#, Kaiyue SHAN1
1Tsinghua University, 2Southern University of Science and Technology

Tropical cyclones (TCs) are one of the most devastating natural disasters. It is still an open question how to improve the prediction of TC intensity and structure due to the complex characteristics of TC dynamics and thermodynamics. The heat and momentum flux changes of the air-sea interface are the key processes to strengthen TCs. However, there remain significant uncertainties about the role of surface heat and momentum flux coefficients (Ck and Cd) on TC intensification. Based on the theoretical concept model of a dissipative engine, this study emphasizes that TC intensification is largely affected by two additional heating processes of viscous dissipation of kinetic energy due to surface friction and the small-scale turbulence at the outflow layer. The calculation of the theoretical upper bound of TC intensity by Emanuel (1986), i.e., the maximum potential intensity (MPI) is modified. With the two additional heating processes, TC MPI can increase by 27% from the result of Bister and Emanuel (1998) and 55% from the result of Emanuel (1986) when Ck/Cd=0.5. In addition, an improved time-dependent model of TC intensification is developed including two key variables, the relative efficiency factor and the percentage of the viscous frictional dissipation heating the surface layer. The relationship between the TC intensification and surface fluxes could be well explained by them jointly. Furthermore, the relative efficiency factor and the percentage of the viscous frictional dissipation heating the surface layer under the different Cd and Ck also are investigated. It is found that the more significant Ck/Cd corresponds to the small relative efficiency and the small percentage of the viscous frictional dissipation heating the surface layer during the middle intensification stage. The potential destructive power of TC-induced coastal hazards, including storm surge, coastal flooding, and extreme rainfall, may also exceed our understanding.


OS06-A033
Initial Condition Plays an Important Role in the Evolution Process of Tropical Cyclone Kinetic Energy

Cong WANG1+, Kaiyue SHAN1, Xiping YU2#, Peida HAN1
1Tsinghua University, 2Southern University of Science and Technology

Tropical cyclones (TCs) are one of the most destructive natural disasters around the world. The destructive power of TCs is generally measured by kinetic energy. How the initial conditions affect TC kinetic energy is not well understood. In this study, the effects of initial conditions, including the initial large-scale environment and initial vortex structure, on the kinetic energy of TCs over the western North Pacific (WNP) ocean basin over 2007-2020 are investigated. It is found that the lifetime maximum kinetic energy of TCs is closely related to their evolution type. TCs are classified into two types according to their evolution processes, i.e., the difference between the times when the TC first reaches its peak maximum sustained wind speed (Vmax) and size (R0). Type A TCs have a peak R0 later than the Vmax, while Type B TCs show the opposite pattern. Based on statistical tests and composite analyses, it is indicated that the lifetime maximum kinetic energy of Type B TCs is approximately 2.7 times that of Type A TCs, largely due to the differences in the initial conditions. Compared with Type A TCs, the initial atmospheric environment of Type B TCs is more unstable, leading to deeper vortexes and smaller latent heat energy distribution in the lower troposphere. The environmental instability dominates the initial distribution of latent heat energy and the intensity of secondary circulation through facilitating the development of outer rainbands, leading to the enhanced activity of TC convection.


OS06-A066
Numerical Simulation of Extreme Sea Levels Along Lianyungang Coast Combining Monte Carlo Model

BaiWen LIU#+
Southeast University

The prediction of extreme sea levels in maritime space has been a prominent requirement of coastal engineering designing and planning. The research was based on the background of frequent disasters caused by typhoon storm surges in China and the demand for reasonably improving building protection engineering standards in coastal zones. In this research, a hydrodynamic model and a Monte Carlo model were integrated to predict extreme sea levels in Lianyungang sea area of Jiangsu province in China. To produce the meteorological driving forces of typhoons, the Monte Carlo method was used to randomly generate typhoon characteristic sequences for typhoon parameter data with different return periods. In Delft3D-FLOW hydrodynamic model, meteorological factors of storm surge were generated by the Monte Carlo model and coupled with the astronomical tide to simulate extreme sea level scenarios in the research sea area. Extreme sea level was estimated by ranking maximum levels in each simulated storm surge event. Compared with the prediction results of the existing frequency analysis methods, this programming was feasible. The Research result predicted extreme sea levels of Lianyungang sea area for 100 and 200 years. Meanwhile, the programming could be adopted to predict extreme sea levels of other research stations in this region and analyze the spatial characteristics of extreme sea level distribution. The results of this research revealed that the extreme sea level had significant spatial variations, which might be related to the concavity of coastline, islands, and terrain. Estimating spatial extreme sea levels could better cognize the influence of flood disasters in coastal areas, which was conducive to the design of coastal disaster prevention projects.


OS06-A042
Bayesian Network-based Disaster Risk Assessment of Tropical Cyclone and Its Application to the Southeast Coast of China

Li XIN#+, Tian CHENG, Li MING, Tian JUNWEI, Du YANG
National University of Defense Technology

At present, the indicator system approach is commonly adopted for tropical cyclone disaster risk assessment, but it inherently fails to describe and portray the complexity and uncertainty of tropical cyclone disasters. To address this problem, this paper adopt Bayesian network (BN), which has the excellent capability of expressing and processing for complex uncertain problems, to construct a new tropical cyclone disaster risk assessment model combined with geographic information system (GIS). Based on the natural disaster risk theory, a total of 15 assessment indexes in four aspects, namely, hazard of disaster-causing factor, sensitivity of disaster-inducing environment, vulnerability of disaster-bearing body, and disaster prevention and mitigation capacity, are selected as model inputs, and direct economic losses are quantified as disaster risk levels as model outputs. Then, the model was applied to the southeast coast of mainland China, and was trained by tropical cyclone disaster data from 1980 to 2016. It was found that the evaluation accuracy of the model is high up to 87.55%, which indicates the model is capable of assessing and predicting uncertain disaster risks by automatically mining the causal relationships among disaster factors from historical data, and expressing them quantitatively in the form of probabilities. To test the generalization ability of the trained model, the data from 2017 to 2020 were used as test samples. The results show that the accuracy of the model is decreased, but it is still as high as 80.79%, and the risk level value it predicted are highly consistent with the actual disaster loss distribution in spatial pattern. Compared with other mainstream machine learning algorithms, the model has higher prediction accuracy and richer disaster risk assessment results, which provides new ideas and new methods for tropical cyclone disaster risk assessment and helps to plan and formulate disaster prevention and mitigation measures.


OS06-A012
An Approach to Predict Shoreline Change at a Long Scale with Wave Climate Calibrated Model

Xinyu CHEN#+, Nobuhito MORI, Tomoya SHIMURA, Takuya MIYASHITA
Kyoto University

Climate change has already posed a significant threat to our surrounding environment. The increasing greenhouse gas emissions induce global warming, leading to sea-level rise (SLR) and consequently causing significant economic loss and threatening human lives, which is unacceptable for everyone. A reduced complexity model is proposed based on the ShoreFor model (Splinter et al., 2014) which takes wave climate and SLR into account. The Hasaki beach is selected as the research area because of its high-resolution data on shoreline change and wave observation. The model's performance in capturing shoreline change at different scales (from hour to year) is assessed. Besides that, two dominant parameters (Φ, c) in the model are studied by interpreting their physical meaning behind them. Φ is proven to be related to the wave's seasonal variance at beaches and the time scale of waves. c, the calibration parameter for shoreline change speed, is no longer set as a time-independent parameter but a time-variant parameter. And the calibration of c more relies on the wave records instead of the past shoreline records, which gives more confidence in predicting the shoreline change at the beach without adequate data combined with downscaled wave models.


OS06-A073
Numerical Simulation and Factor Analysis for Rip Current

Shu-Min WANG1#+, Dong-Jiing DOONG1, Cheng-Han TSAI2
1National Cheng Kung University, 2National Taiwan Ocean University

Coastal areas, especially beaches, are vulnerable to the potentially deadly effects of rip currents. To safeguard public safety, an understanding of the mechanisms underlying rip current formation is critical. The SCHISM&WWM wave-current coupling model was used to simulate the flow field under varying meteorological and wave conditions in this research, in order to elucidate the dynamics of rip current formation. The model was rigorously verified by comparing simulated data to actual measurements, with excellent agreement observed for water level, wave, and period. In addition, The Image analysis process was established to collect rip current cases from optical image by wavelet transform technology, resulting in the development of an image automatic detection technology capable of identifying existing cases with an accuracy rate of approximately 80%. In summary, a parameter sensitivity analysis indicated that significant wave height, average period, wave direction, and beach type exerted substantial influences on occurrence of rip current . These findings offer valuable insights into the complex dynamics of rip currents, and can be utilized to develop more effective monitoring and forecasting systems for offshore currents in Taiwan.


Wed-02 Aug | 1:10 - 3:10 | MR309
OS10 - General and Multidisciplinary Oceanography

Session Chair(s): Yusuke UCHIYAMA, Kobe University

OS10-A017 | Invited
Cross-slope Heat and Salt Transport Induced by Slope Intrusion Eddy's Horizontal Asymmetry in the Northern South China Sea

Chunhua QIU1#+, Zhenhui YI1, Danyi SU1, Hailong LIU2, Pengfei LIN2, Dongxiao WANG1
1Sun Yat-sen University, 2Chinese Academy of Sciences

Material transport caused by mesoscale eddies has been revealed much in the open ocean; however, it is still unclear how much eddy-induced mass transport in the slope region of the northern South China Sea (SCS). Using the LASG/IAP Climate System Ocean Model (LICOM) from 2007 to 2017, we identified 47 anticyclonic eddies and 97 cyclonic eddies that intruded onto the continental slope, termed slope intrusion eddies. The slope intrusion eddies are more horizontally asymmetric and energetic than those without entering the slope. These eddies induced cross-slope heat and salt transport of O(1012) W and O(104) kg s−1 owing to their horizontal asymmetry in both Xisha Islands and Dongsha Islands, where are the intrusion zones of mesoscale eddies. Based on the potential vorticity budget, we found that the horizontal asymmetry of velocity was caused by the asymmetry of potential vorticity, which was mainly generated by eddy-current nonlinear effect in the Dongsha Islands and topographic beta effect in the Xisha Islands, respectively. This study may promote our understanding on the mesoscale dynamics and oceanic energy redistribution in the continental shelf zone of marginal sea.


OS10-A034
Influence of Slope Topography and Upper Lateral Exchanging Flow on Layered Circulation in the South China Sea

Qibang TANG#+, Zhongya CAI
University of Macau

A process-oriented modeling approach was used to how the vertical structure and intensity of the layered circulation respond to the changes in bottom slope and upper intrusion from the open ocean. By setting the mixing intensity of the basin and the open ocean to be different, a three-layer circulation structure is triggered, in which the upper cyclonic(<500m) - middle anticyclonic(500-2300m) - deep cyclonic(>2300m). Differs between the vertical structure of the integrated continental slope current in the ocean basin and the three-layer water exchange at the Luzon Strait. The changes in the bottom slope modulate the layered circulation, particularly the deep and middle layers that directly interact with it, by influencing the lateral exchanging current. With the steeper slope, the deep layer cyclonic circulation will be intensified with large thickness, which in turn squeezes and also strengthens the middle layer anticyclonic circulation. Therefore, according to the theoretical analysis of potential vorticity conservation, the average water depth of the deep layer will be greater at steeper slopes, and the deep cyclonic circulation will be greater than that on the gentler slopes. On the other hand, the strong upper layer intrusion (5 Sv) from the open ocean directly strengthens and widens the upper layer cyclonic circulation by providing more positive planetary vorticity, and it is also noted that it largely intensifies the deep cyclonic circulation by 45.8% indirectly. Although it intensifies deep intrusion through the LS, the increases in the deep intrusion are much smaller than the vertical interplay, the intrinsic coupling over the meandering slope plays the larger role. The vorticity dynamics illustrate that the stretching of the deep layer is intensified by the intrusion of the western boundary current from the open ocean, which leads to enhanced deep cyclonic circulation.


OS10-A036
Summer Surface Warming Driven by the Strong El Niño in the South China Sea

Qin-Yan LIU#+
Chinese Academy of Sciences

The interannual variability of sea surface temperature (SST) in the South China Sea (SCS) exhibits two peaks around January and August in the subsequent year of the El Niño. We show that the second basin-scale summer SST warming feature peaked in August [+1] is only distinct after strong El Niño events, not regular El Niño events. The upper ocean heat budget analysis demonstrates that the abnormal Ekman advection (Eka) dominants the second warming features during the whole developing stages from June [+1] to August [+1], while the abnormal geostrophic advection (Goa) leads to the warm tendency in June [+1], by reducing the Vietnam coastal upwelling. The local dynamical effects of abnormal Eka and Goa in the SCS are attributed to the advanced abnormal easterly wind breakout in the western Pacific, coincided with the development of West North Pacific anomalous anticyclone (WNPAC) in response to strong El Niño. Our results suggest that the second warming features of SCS SST during the next summer are the footprints of strong El Niño events via the establishment of the WNPAC, which is tightly related to Indo-Pacific remote processes.


OS10-A033
Hydrodynamic Modeling for forecasting Circulation and Object Tracking in the Gulf of Thailand

Kachapond CHETTANAWANIT1#+, Watin THANATHANPHON2, Narongrit LUANGDILOK2, Sathit CHANTHIP2, Piyamarn SISOMPHON2
1Hydro – Informatics Institute, Ministry of Higher Education, Science, Research and Innovation, 2Ministry of Higher Education, Science, Research and Innovation

Accurately predicting water level and circulation in the Gulf of Thailand is crucial for maintaining the marine ecosystem, fishery productivity, and supporting coastal activities in Thailand. The Gulf of Thailand covers a vast area, spanning over three thousand kilometers across 22 provinces. To tackle this issue, a hydrodynamic model using the Delft3D model was developed to simulate the water level and circulation in the Gulf of Thailand. The model domain covered the whole of the Gulf of Thailand. The open boundary of the model was forced by 14 tidal constituent components from TPXO 9.0, and wind forcing was provided by the GFS 0.25 model. Seasonal circulation pattern was validated with surface current tracking buoys, and the model was found to be consistent with the path of the current tracking buoy. This validation process gave confidence in the accuracy of the model in predicting circulation. The model was used to estimate the location of the bodies and objects of the shipwreck where 31 people were lost at sea. To do this, the model was set up into three cases: tide-wind, tide-wave-wind, and wind only. Twenty drogues were used for drogue tracking in the model. The results showed that drogues in cases 1 and 2 floated in the same direction, which was consistent with the location where the lost people were found. However, the wind-only forcing case showed the drogues' positions relative to the life jacket and lifeboat, which are lightweight and float on the surface with the wind current. In conclusion, the model performed well in predicting circulation and object tracking in the Gulf of Thailand. The accuracy of the model can help in making informed decisions and can be used as a valuable tool for the management of natural resources in the Gulf of Thailand.


OS10-A029
Emergence of Climate Change in the Tropical Pacific and Its Sources of Uncertainty

Jun YING1#+, Matthew COLLINS2, Wenju CAI3,4
1Ministry of Natural Resources, 2University of Exeter, 3Ocean University of China and Qingdao National Laboratory for Marine Science and Technology, 4Commonwealth Scientific and Industrial Research Organisation

Future changes in the mean climate of the tropical Pacific and characteristics of the El Niño–Southern Oscillation (ENSO) are established as likely. Determining the time of emergence (ToE) of climate change signals from the natural variability is critical for mitigation strategies and adaptation planning. Here, by using multi-model ensemble simulations as well as three large ensembles of model simulations, we explore both the ToEs of climate change signals in the tropical Pacific as well as their sources of uncertainty. The results show that for the multi-model mean result the annual-mean sea surface temperature (SST) signal has already emerged across much of the tropical Pacific, appearing last in the east. The signal of a wetter annual-mean rainfall in the east is expected to emerge by mid-century, with some sensitivity to emission scenario. However, the ENSO-related rainfall variability signal is projected to emerge earlier than ENSO-related SST variability signal. As for the sources of uncertainty, we find that internal variability contributes to less than half of the total uncertainty in both the ToEs of annual-mean SST and rainfall, while internal variability contributes to a major part of the total uncertainty in the ToEs of ENSO-related SST and rainfall.


OS10-A023
Tracking the Pumice Rafts from the Recent Eruption of the Submarine Volcano Fukutoku-Okanoba, Japan Using Satellites and Lagrangian Particles Tracking

Mochamad Riza ISKANDAR1,2+, Young Gyu PARK1#
1Korea Institute of Ocean Science and Technology, 2National Research and Innovation Agency of Indonesia (BRIN)

On 13 August 2021, the Fukutoku-Okanoba submarine volcano in the North Pacific Ocean was erupted. Satellites detected many pumice rafts that drifted westward to reach southern Japan in about two months. To cope with potential danger due to the pumice rafts, it is crucial to predict their trajectories. Using a Lagrangian particle tracking model, the trajectories of the rafts were investigated. The model results showed strong sensitivity to the windage coefficient of pumice rafts, which is uncertain and could cause large errors. By comparing the model results with satellite images using a skill score, the distance between a simulated particle and the nearest observed raft divided by the travel distance of the particle, an optimal windage coefficient was estimated. The optimal windage coefficients ranging between 2 to 3% produced pathways comparable to the observations from satellites. The pumice rafts moved from Fukutoku-Okanoba, toward the Ryukyu Islands for approximately two months before being pushed toward Taiwan by the intensified wind. The techniques presented here may become helpful in managing coastal hazards due to diverse marine debris.


OS10-A013
Long-lasting Marine Heatwaves Instigated by Ocean Planetary Waves in the Tropical Indian Ocean During 2015/16 and 2019/20

Ying ZHANG1+, Yan DU2#, Ming FENG3, Shijian HU2
1South China Sea Institute of Oceanology, Chinese Academy of Sciences, 2Chinese Academy of Sciences, 3Commonwealth Scientific and Industrial Research Organisation

Marine heatwaves (MHWs) in the tropical Indian Ocean (TIO) showed remarkable increases in duration and frequency during the satellite observing era, responding to rising sea surface temperature. Long-lasting MHWs were found in three upwelling regions of the TIO in 2015-2016 and 2019-2020, closely related to persistent downwelling oceanic planetary waves. In 2015, a prolonged MHW (149 days) in the western TIO was initiated by the downwelling Rossby waves associated with the co-occurring super El Niño and positive Indian Ocean dipole (IOD) events. In the following year, the negative IOD sustained the longest MHW (372 days) in the southeastern TIO, prompted by the eastward-propagating equatorial Kelvin waves. In 2019-2020, the two longest MHWs recorded in the southwestern TIO (275 days in 2019 and 149 days in 2020) were maintained by the downwelling Rossby waves associated with the 2019 extreme IOD. This study revealed the importance of ocean dynamics in long-lasting MHWs in the TIO.


Wed-02 Aug | 1:10 - 3:10 | MR310
OS09 - Global Western Boundary Currents: Their Physical, Chemical, and Biological Impacts on Climate and Ecosystems (ii)

Session Chair(s): Xiaopei LIN, Ocean University of China, Akira NAGANO, Japan Agency for Marine-Earth Science and Technology

OS09-A002
Biogeochemical Aspects of the Kuroshio Large Meander

Hakase HAYASHIDA1#+, Andrew KISS2, Toru MIYAMA1, Yasumasa MIYAZAWA1, Sayaka YASUNAKA3
1Japan Agency for Marine-Earth Science and Technology, 2Australian National University, 3Tohoku University

The large meander of the Kuroshio western boundary current is well known to influence the local climate, fisheries, and aquaculture by greatly modulating regional heat transport, but its impacts on biogeochemical processes remain unclear. Using high-resolution numerical ocean modelling and long-term observational datasets, we show that the path of the Kuroshio determines the extent of the shallow nutricline region, where winter convective mixing replenishes nutrient availability for subsequent blooms of phytoplankton during spring. During the large meander phase, this mechanism triggers offshore phytoplankton blooms that are otherwise absent during the non-large meander phase. The large meander also modulates the spatial distributions of primary production, air-sea carbon flux, and export production. These biogeochemical impacts of the Kuroshio large meander exert bottom-up control on regional marine ecosystems that is disproportionate to the thermal effect, and therefore need to be assessed to understand the large meander’s overall impacts on fisheries and aquaculture.


OS09-A013
On the Contributions of Nitrogen from Different Sources to Exported Organic Nitrogen from the East China Sea

Jing ZHANG1#+, Xinyu GUO2, Liang ZHAO1
1Tianjin University of Science and Technology, 2Ehime University

The export of organic matter fixed by photosynthetic activities, which is defined as export production, is crucial for sustaining oceanic carbon uptake. To quantify it in shelf seas is still challenging due to vigorous cross-shelf and water-sediment hydrodynamics. Here, a unique 3D physical-biological coupled model with tracking approach is applied to evaluate the export production supported by multi-source DIN over the East China Sea. The total export production is 6.83 kmol N s-1 (=17.16 Tg C yr-1) which is a little smaller than reported atmospheric CO2 absorption. About 80% of PON are exported via off-shelf transport and the remaining 20% are buried in sediments. The PON supported by DIN from rivers accounts for 8% of the export production with a e-ratio of 0.09, while that from the Kuroshio contributes 64% with a e-ratio of 0.22. We suggest that off-shelf outflow and offshore areas play an important role in carbon sequestration over continental shelves.


OS09-A005 | Invited
Dynamical and Ecological Interaction Between the Kuroshio and Coastal Circulation: Collaborative Study with Stakeholders Around Suruga Bay, Japan

Kiyoshi TANAKA1#+, Toru MIYAMA2, Takahiro TOYODA3, Kunio KUTSUWADA4, Masato NIKI4, Daisuke TAKAHASHI4, Kazuyuki UEHARA4, Yukio UNNO5, Kenichi KOBAYASHI5
1The University of Tokyo, 2Japan Agency for Marine-Earth Science and Technology, 3Japan Meteorological Agency, 4Tokai University, 5Shizuoka Prefectural Research Institute of Fishery and Ocean

Coastal circulation off the south coast of Japan interacts strongly with the Kuroshio current. The interaction process plays an important role in ecosystems along the Kuroshio Current and adjacent coastal seas, because large amounts of water including heat and nutrients are exchanged between them through the interaction. Moreover, the interaction also plays an important role in Kuroshio Current dynamics, because the path of the Kuroshio Current (the straight or large meander paths) depends strongly on nonlinearity of the flow due to the interaction (mesoscale and sub-mesoscale processes). Therefore, we are currently conducting a research project designed to investigate the interaction between the coastal circulation and the Kuroshio current. In particular, an area around Suruga Bay is selected as a pilot study area, where strong dynamical and ecological interaction between inside and outside the bay occurs due to variation of the Kuroshio Current, and where coastal fisheries are well developed. The goal of our project is to present a clear vision for future ocean science in the coastal regions and along the Kuroshio, meeting the expected outcome of the UN Decade of Ocean Science. To achieve this goal, we have three objectives: development of numerical simulation, establishment of sustainable in situ observation, and collaboration with stakeholders. With regard to the numerical simulation, high-resolution ocean circulation models (JCOPE and MRI.COM models) have started simulating the processes directly. Moreover, recent downsized instruments enable the observation to be conducted easily utilizing ordinary fishing boats, aquaculture facilities, and commercial ships. A key point is that the numerical simulation is validated by the in situ observations. Moreover, establishment of synergistic collaboration with stakeholders, such as local fishers and a shipping agency, is essential to the project.


OS09-A014
Injection of High Chlorophyll-a Waters by a Branch of Kuroshio Current Into the Nutrient-poor North Pacific Subtropical Gyre

Chun Hoe CHOW1#+, Yi-Chen LIN1, Wee CHEAH2, Jen-Hua TAI3, Yu-Chun SU1
1National Taiwan Ocean University, 2University of Malaya, 3Academia Sinica

We observed an unusual eastward current branching out from the northward-flowing Kuroshio Current east of Taiwan in summer 2010. The eastward current flowed roughly along 21°N for a few months and then reached 137°E. It transported warmer, fresher, and higher-chlorophyll-a waters far to the east into the poor-nutrient and high-saline North Pacific subtropical gyre. Along the eastward current, the transported waters had similar temperature-salinity properties as those from the Kuroshio Current, and thus we called it the eastward cross-shore Kuroshio Branch (ECKB). Its geostrophic-flow speed was about 0.5 meters per second on average, based on observations from satellite altimeters, a surface Lagrangian drifter, and a CTD-casting transect. Its depth could reach 100 meters, measured by the CTD-casting transect roughly along the 137°E, by assuming no motion at 1000 meters. The ECKB mechanism was linked to a surface cyclonic wind anomaly, which cooled the ocean surface via Ekman suction. Then, the subtropical ocean front was enhanced and subsequently induced the ECKB that bifurcated from the Kuroshio main stream. The ECKB could also be observed in summer 2013.


OS09-A022
Is the Subsurface Kuroshio Just a Nutrient Conduit or a Spreader?

Takeyoshi NAGAI1#+, Gloria Silvana DURAN GOMEZ1, Hiroaki SAITO2, Hiroshi OGAWA2, Toru KOBARI3, Naoki YOSHIE4, Nakamura HIROHIKO3, Iára Andressa TORRES CABRERA1
1Tokyo University of Marine Science and Technology, 2The University of Tokyo, 3Kagoshima University, 4Ehime University

While the Kuroshio transports a large amount of nutrients in their dark subsurface layers, it has been unclear whether these nutrients are supplied to the sunlit surface layers before it reaches the Kuroshio Extension regions. The nutrient concentrations on the density surface along the Kuroshio and the Gulf Stream show elevated values suggesting diapycnal nutrient flux. This is particularly important as these positive nutrient anomalies on the relatively less dense water are more susceptive to surface mixing processes and injected easily to the euphotic zone, playing a role in maintaining the major net CO2 sinks along the Kuroshio Extension. However, recent studies concluded that the horizontal advection of the Gulf Stream carries this anomaly from the upstream tropical regions with negligible diapycnal mixing. In contrast, the Kuroshio flows over rough topography more frequently. In this study, using a numerical model of the Kuroshio nutrient stream, and direct microscale turbulence measurements, the importance of the diapycnal mixing in the Kuroshio is reexamined. A series of the tow-yo microstructure observations in the Kuroshio flowing over the rough topography shows that the large nitrate diffusive diapycnal flux of 1-10 mmol m-2day-1 are frequently observed. The time scale required for the diapycnal nitrate flux at 1 mmol m-2day-1 to generate the observed positive anomaly of nitrate concentrations is found to be as short as 50 days, assuming the area of nitrate injection of 1000 km2. The observations suggest that the nitrate injection at 1 mmol m day over the area of 1000 km2 is plausible. Therefore, unlike the Gulf Stream, the diapycnal turbulent diffusive flux is unlikely negligible in the Kuroshio nutrient stream.


OS09-A023
Turbulent Mixing, Submesoscale Upwelling of Nutrients and Their Influences on Productivity in the South of Japan Along the Kuroshio

Gloria Silvana DURAN GOMEZ1#+, Takeyoshi NAGAI1, Toru KOBARI2, Nakamura HIROHIKO2, Kristinn ÞRÖSTUR SIGURDARSON1, Ingibjorg BJORGVINSDOTTIR1
1Tokyo University of Marine Science and Technology, 2Kagoshima University

The Kuroshio Current carries a large amount of nutrients in dark subsurface layers, as a nutrient stream. However, questions remain as to whether and how these subsurface nutrients can be supplied to sunlit layers along the coast of Japan. Since the Kuroshio frequently flows over rough topography, strong turbulence and eddy induced upwelling generated over topographic features could be the key processes to support the high productivity. Yet, detailed mechanisms are not fully clear. The objective of this research is to elucidate the effects of turbulent diffusive nutrient supplies on lower trophic level of the ecosystem, and to quantify the submesoscale nutrient upwelling and its influences on the producers. For this purpose, surveys were conducted in the Tokara Strait at different times of the year in June and November 2021, and November 2022. The latter direct observations are focused on determining the effect of submesoscale cyclonic eddy at the southwest of Yakushima, where the Kuroshio flows close proximity. For this case, we also attempt to reproduce the observed features in time by using a high-resolution model coupled with a N2P2Z2D2 ecosystem model. In the upstream Kuroshio, observations show that nitrate diffusive flux occurs in the subsurface layers during the stratified season, affecting the subsurface chlorophyll-a. Also, camera images imply that chlorophyll-a distributions could be affected by zooplankton grazing. Meanwhile, during the fall-winter season, subsurface mixing above the seamounts can bring nitrate upward into a deeper surface mixed layer (~100 m). More importantly, during this season, submesoscale nitrate upwelling structures appear and seem to be associated with submesoscale mixed layer cyclonic eddies. These results shed a light on the role of the Kuroshio in supplying nutrients to the upper layers that may influence on where and how phytoplankton, zooplankton and marine snow increase along the Kuroshio flowing over the topographic features.


Wed-02 Aug | 3:30 - 5:15 | MR309
OS10 - General and Multidisciplinary Oceanography

Session Chair(s): Yusuke UCHIYAMA, Kobe University, Sung Yong KIM, Korea Advanced Institute of Science and Technology

OS10-A002 | Invited
Dynamics of Internal Tides Generated by a Flow-tide Interaction Along the Kuroshio

Eiji MASUNAGA1#+, Hitoshi TAMURA2, Yusuke UCHIYAMA3
1Ibaraki University, 2Port and Airport Research Institute, 3Kobe University

This study presents internal tide dynamics generated by an interaction of background shear flows (the Kuroshio) and tides over a shallow ridge, Izu-Ogasawarea Ridge off the mainland Japan, using numerical simulations and field observations. Strong generation of internal tides occur over the ridge and gen eared internal tides propagate several hundreds of toward the upstream of the Kuroshio. Internal tides finally shoal to the coast, at Cape Shino-Misaki, and dissipate. A long-term monitoring data at the Cape shows variations of the internal tide kinetic energy influenced by the Kuroshio path. Internal tides shoal into the head of the cape from the generation site when the Kuroshio approaches to the coast. On the other hand, the magnitude of internal tides is much lower when the Kuroshio meander occurs than that when the Kuroshio approaches to the coast. These results imply that the path of the Kuroshio modulates propagations/generations of internal tides along the Kuroshio path. In addition, the recent long-term Kuroshio meander (2017–present) may largely influence coastal physical processes through internal tides.


OS10-A022
Interpreting Observed 152°W Radionuclide Tracers Using Surface Drifters

Sachiko YOSHIDA#+, Alison MACDONALD, Irina RYPINA
Woods Hole Oceanographic Institution

To improve the understanding of fate and the origin of the observed radiocesium signal at 152°W on timescale of 1-5 years, a muti-iteration approach was applied to Global Drifter Program trajectory data in the North Pacific. Following the North Pacific Drift, the eastward surface current splits northward into the Alaskan gyre and southward following into the California Current. The estimated probability and time travel maps were constructed using the drifter trajectories coming into and leaving from the source boxes which corresponded to the elevated radiocesium near-surface sampling location between 30°N and 50°N. As predicted, the majority of trajectories moved eastward through the source box at 35°-45°N, turned southward following the California Current (~1 year), and entering the Subtropical Gyre after ~2 years. The northern pathway was only seen from the trajectories departing at and north of 45°N. These trajectories entered and followed the Alaskan Coastal Current along the coasts of Canada and Alaska to turn westward within ~1 year. Toward the southern end of source box closer to 30°N where the surface flow slows down and reverses direction, the North Equatorial Current captures drifters sending them westward and there is no pathway northward. Backward time simulations demonstrate that the most, but not all, pathway leading into the source box at 35-45°N could be continuously traced back to Kuroshio and its extension on timescales of about 2 years.


OS10-A003
Transport Processes in the Japan Sea Investigated with Particle Tracking Simulations and Surface Drifter Data

Kazuhiro HARADA1#+, Eiji MASUNAGA1, Yusuke UCHIYAMA2
1Ibaraki University, 2Kobe University

In order to understand the transport processes of materials in the ocean, we conducted particle tracking simulations in the Japan Sea. Particle tracking simulations were conducted using the Regional Oceanic Modeling System with a Lagrangian particle tracking model. Particles were released from the Tsushima Strait in four seasons (winter, spring, summer and fall). Two particle types were simulated: (1) surface drifter particles moving only the surface layer and (2) 3-D particles moving with 3-D velocities (u, v, w). Particles are mainly transported toward the east side of the sea and some fraction of particle are transported to the Pacific Ocean through the Tsugaru Strait. Dispersion of 3-D particles are higher than surface drifters and 3-D drifters distribute the whole area of the Japan Sea. The higher dispersion of 3-D particle is is caused by submesoscale eddies accompanied by intensified vertical motions. Surface drifters tend to beaching by comparing 3D particles. Particles released in winter and fall tend to distribute over a wide area, while those released in spring and summer are distributed along the coast. Vertical advection and eddies contribute to the diffusion and transport of particles in the winter season. In addition, we investigate surface drifter data provided by the Global Drifter Program (GDP). The observed and simulated trajectories were compared in terms of spatial distributions, velocity distributions and spectrum. The GDP data are consistent with our numerical simulations, which implies that our regional numerical model well reproduce transport processes in Japan Sea.


OS10-A038
Differences Between Mixed Layer Depth and Turbulent Process in Humboldt and California Current Systems and Its Consequences on Chlorophyll Abundance

Diego OTERO#+, Takeyoshi NAGAI
Tokyo University of Marine Science and Technology

The Humboldt and California Current System in the eastern Pacific Ocean, are important for oceanic ecosystems due to their intense upwelling that allows the blooming of phytoplankton and, therefore, an abundant fishing resources biomass. It is known that the time of greatest upwelling intensity in the Northern and Southern Hemispheres is during the months of July, August and September, being summer and winter respectively. However, as for chlorophyll, it is higher during their respective summers regardless of the upwelling intensity, suggesting that restratification is the key to induce phytoplankton bloom. Recent studies have suggested that the mixed layer depth (MLD), being deeper during winter and shallower during summer, can affect the seasonality of the mixed layer eddy activity, having highest activity during winter. Further, several studies showed that these eddies play a role in subducting these upwelled nutrients before they are used by phytoplankton, reducing the biological production. From this point of view, it can be hypothesized that the more active eddies during winter in Humboldt upwelling regions can subduct more nutrients than that of California. In this study, using temperature, salinity, and water velocity data obtained from the GLORYS12V1 reanalysis product for global ocean eddy-resolving (1/12° horizontal resolution, 50 vertical levels and 1993 onwards) and chlorophyll provided by Global Ocean Satellite Observations, we attempt to elucidate what is the consequence of the opposite timing of deepest MLD with respect to the strongest upwelling season in both the eastern boundary currents.


OS10-A008
Oceanic Thermal and Dynamical Responses to Typhoon Kalmaegi (2014)

Xiaojie LU1#+, Changming DONG1,2, Han ZHANG3
1Nanjing University of Information Science & Technology, 2Southern Marine Science and Engineering Guangdong Laboratory, 3Second Institute of Oceanography, Ministry of Natural Resources

Tropic storms could cause the strong oceanic responses in the ocean, however such responses are not well observed in most storms. Typhoon Kalmaegi (2014) in the northern South China Sea (SCS) are well recorded by a cross-structure well-designed cross-structure in-situ oceanic observation system. Oceanic thermal and dynamic responses to the typhoon are analyzed using the in-situ observational data together with satellite remote sensing data. The sea surface temperature (SST) shows that the maximum cooling of 3.77 ℃ occurs on the right side of the typhoon track, corresponding to the well-known “rightward bias”. The effects of “heat pump” and “cold suction” well captured by the in-situ observations at the stations of two sides of the typhoon track: warmer (colder) on the right (left) side. The spectral analysis of in-situ oceanic currents demonstrates that the near-inertial kinetic energy (NIKE) is the strongest immediately after the typhoon passes and propagates downward. The maximum depth the NIKE can reach is affected by the wind stress curl, oceanic current vorticity polarity: strong curl and negative vorticity can push the NIKE go deeper. The possible connection between the near-inertial waves and vertical heat transport is discussed.


OS10-A039
Coastal Climatology from a Large Coastal Embayment Using a Hydrodynamic Model: The Case of Bay of Plenty, Aotearoa New Zealand

Mireya MONTANO1,2#+, Ata SUANDA3, Joao SOUZA2
1University of Otago, 2MetOcean Solutions, 3University of North Carolina Wilmington

Understanding coastal water dynamics and their variability is critical for human activity and for improving management practices and emergency response situations. Therefore, baseline knowledge of the ocean’s state is crucial to assess current and future scenarios better. This study developed an Eulerian and Lagrangian climatology for the Bay of Plenty (BoP), a shallow, ≈190 km wide embayment on the northeast continental shelf of Aotearoa, New Zealand. We used a downscaled 25+ years (1994-2020) high-resolution hindcast ROMS model (BoPM hereinafter, ≈1 km horizontal resolution). The BoPM resolves the mesoscale features of the oceanic circulation, has realistic tide and atmospheric forcing, high-resolution bathymetry, and includes four islands near the coast. The Eulerian climatology was first evaluated against a high-resolution remote sensing product, showing that the BoPM is capable of reproducing the climatological aspects of the region. Afterwards, further analyses showed a typical sea surface temperature (SST) seasonal cycle, with stronger interannual variability in the nearshore region during austral summer. A portion of the nearshore SST interannual variability in the BoP is explained by the local winds and El Niño Southern Oscillation. However, the BoP showed no seasonal cycle for the flow transport. The lack of a seasonal cycle could be associated with the high eddy variability in the region due to the presence of a western boundary current. Therefore, we used climatological Lagrangian Coherent Structures (cLCS) to obtain a Lagrangian climatology and complement the description of the Eulerian climatology. The cLCS provided insight into coastal persistent transport patterns not visible in the climatological Eulerian flow. Additionally, they highlighted the importance of resolving coastal processes and including coastal features (i.e., islands) to understand the coastal dynamics of a region such as the BoP.


Wed-02 Aug | 3:30 - 5:15 | MR310
OS09 - Global Western Boundary Currents: Their Physical, Chemical, and Biological Impacts on Climate and Ecosystems (ii)

Session Chair(s): Yasumasa MIYAZAWA, Japan Agency for Marine-Earth Science and Technology, Akira NAGANO, Japan Agency for Marine-Earth Science and Technology

OS09-A003
Cold‑ Versus Warm‑season‑forced Variability of Net Kuroshio Transport South of Japan

Yuma KAWAKAMI1#+, Hideyuki NAKANO1, Shogo URAKAWA1, Takahiro TOYODA2, Kei SAKAMOTO2, Goro YAMANAKA2, Shusaku SUGIMOTO3
1Meteorological Research Institute, 2Japan Meteorological Agency, 3Tohoku University

The ocean responds to atmospheric variations. Changes in sea surface winds, surface air temperature, and surface air humidity cause upper ocean variability by modulating air-sea momentum and heat exchanges. Upper ocean variability in the mid-latitudes on inter-annual and longer timescales has previously been considered to be attributable to atmospheric variations in the cold season, because atmospheric forcing is stronger in the cold season than in the warm season. However, this idea has not been sufficiently confirmed yet. The ocean model is a useful tool to evaluate the impact of the atmospheric forcing in each season, although there are no past studies having examined ocean model responses respectively to the cold- and warm-season atmospheric forcing. In this study, we performed numerical experiments with an eddy-resolving ocean general circulation model and investigated oceanic responses to cold- and warm-season atmospheric forcing, focusing on the Kuroshio in the North Pacific. We found that net Kuroshio transport south of Japan is dominantly controlled by wind stress curl (WSC) in the central North Pacific in the cold season: through westward propagation of oceanic Rossby waves, net Kuroshio transport responds to WSC variations in the central North Pacific, which strongly reflect atmospheric fields in the cold season. Warm-season WSC variations in the central North Pacific are too small to generate oceanic Rossby waves, resulting in little influence on the net Kuroshio transport. This result suggests that cold-season atmospheric variations are key to obtaining insights into variability of the Kuroshio and the western North Pacific subtropical gyre.


OS09-A008
Increasing Deep-water Overflow from the Pacific Into the South China Sea Revealed by Decade-long Mooring Observation

Xin XIAO#+, Chun ZHOU, Wei ZHAO, Jiwei TIAN
Ocean University of China

Cold and dense water from the deep western boundary current in the North Pacific Ocean that spills through the Luzon Strait, the only deep conduit between the South China Sea (SCS) and the Pacific Ocean, renews deep water-mass, modulates hydrographic and biogeochemical cycles, and drives abyssal and overturning circulations in the SCS. Variability of this key oceanic process, however, has been poorly studied mainly due to a lack of sustained observations. A comprehensive observational program that started in 2009 has provided 12 years of continuous time series of velocity and volume transport within the Luzon Strait. This study presents the first observation-based assessment of decadal trends of deep-water transport through this vital passage. It shows that the 12-year mean volume transport of the deep-water overflow into the SCS is 0.84 ± 0.39 Sv (1 Sv = 106 m3 s-1). A linear upward trend with an increase of 0.074 ± 0.045 Sv, or about 9 ± 5%, of volume transport accompanied by a cooling of -0.010 ± 0.008 ℃ per decade is revealed. This is consistent with long-term changes in satellite-observed ocean bottom pressure (OBP) and sea level height. Results of this study may have broad implications for the deep western boundary current systems, overturning circulations and biogeochemical processes including carbon cycles in this region.


OS09-A017 | Invited
Spatio-temporal Scale Dependency of Air-sea Coupling via the Vertical Mixing Mechanism Over WBCs

Dian PUTRASAHAN#+, Jin-Song VON STORCH
Max Planck Institute for Meteorology

Global coupled climate models such as CMIP-type models show a dominance of atmospheric forcing onto the ocean, e.g. strong winds blowing over ocean surface that lead to enhanced turbulent heat flux and thus cooler sea surface temperatures (SSTs). On the other hand, satellite observations and eddy-resolving coupled models show a dominance of mesoscale ocean forcing on the atmosphere over mesoscale eddy-rich regions like western boundary current (WBC) areas. For instance, a destabilisation of the atmosphere overlying warm mesoscale anomalies would enhance downward transfer of momentum from winds aloft to the surface (vertical mixing mechanism; VMM), thereby increasing surface winds and turbulent heat flux over warm SST anomalies. If winds are blowing along downwind to SST gradients, this can induce wind stress divergence. The differing dominance in forcing, be it from ocean or atmosphere, indicates a spatial scale dependence of oceanic vs atmospheric variability in driving the coupled variability of air-sea interactions. Aside from the spatial scales of air-sea coupling, temporal scales of these interactions are also unclear. At what range of timescales would air-sea coupling continue, deteriorate or cease to occur? We therefore employ the global coupled 5-km ICON simulation, whereby the atmosphere is able to feel the full mesoscale ocean features, and investigate the spatial and temporal scale dependency of air-sea coupling associated with the VMM. For various WBC regions, we evaluate the frequency-wavenumber cross-spectra between downwind SST gradients and windstress divergence to identify the dominant temporal and spatial scales for air-sea coupling via the VMM. For example, over the Gulf Stream region, we find that such interactions are prevalent on spatial scales of roughly 100-1000km and longer than 5-days timescale. For the first time, the dominant spatial and temporal scales of air-sea coupling via the VMM in various regions of the world's ocean is quantified.


OS09-A010
Enhanced Atmospheric Response Shaped by Submesoscale Oceanic Front-induced Mixing

Haiyuan YANG1+, Zhaohui CHEN1,2#, Mingkui LI1, Lixin WU1
1Ocean University of China, 2Qingdao National Laboratory for Marine Science and Technology

Oceanic submesoscale fronts, characterized by a spatial scale of 1–10km, are critical to oceanic vertical tracer transport and air-sea heat exchanges. However, our understanding of its role in regulating the overlying atmosphere is still limited due to lack of comprehensive field observations. Here, for the first time based on shipboard observations, we describe the structure of a strong oceanic submesoscale front and examine its impact on the overlying atmosphere in the mid-latitude Kuroshio Extension (KE) region, a key area for atmosphere-ocean interactions. The submesoscale front is associated with a cross-front change in the sea surface temperature (SST) by 12℃ within 10km, which is much sharper than that obtained from current satellite observations, reanalysis data and eddy-resolving models. Fueled by this strong SST gradient, the marine atmospheric boundary layer (MABL) height depicts a 700m difference across the front, which is accompanied by a downdraft of order 0.1m/s. The observed responses of MABL processes and surface wind associated with vertical mixing mechanism, not represented by current state-of-the-art climate models, are much stronger than those induced by mesoscale fronts and can regulate local atmosphere movement and cloud formation, highlighting the importance of submesoscale air-sea interactions. Thus, our results call for a proper representation of submesoscale air-sea exchanges in the next generation of weather and climate models.


OS09-A016
Hidden Upwelling Systems Associated with Major Western Boundary Currents

Fanglou LIAO1, Xinfeng LIANG2#+, Yun LI2, Michael SPALL3
1Northwestern Polytechnical University, 2University of Delaware, 3Woods Hole Oceanographic Institution

Western boundary currents (WBCs) play an essential role in regulating global climate. In contrast to their widely examined horizontal motions, less attention has been paid to vertical motions associated with WBCs. Here, we examine vertical motions associated with the major WBCs by analyzing vertical velocity estimates from five ocean synthesis products and one eddy-resolving ocean simulation. These data reveal robust and intense subsurface upwelling in five major subtropical WBC systems. These upwelling systems are parts of basin-scale zonal overturning circulations and are likely driven by the meridional pressure gradients along the western boundary. Globally, the WBC upwelling contributes significantly to the vertical transport of water mass and ocean properties. The WBC upwelling and the basin-wide zonal overturning circulations are therefore essential yet overlooked branches of the global ocean circulation. In addition, the WBC upwelling intersects the oceanic eutrophic and mixed layers, and thus plays important roles in ocean biological and chemical processes by transporting nutrients, carbon, and other tracers vertically inside the ocean. This study calls for more research into the dynamics of the WBC upwelling and their roles in the ocean and climate systems.


OS09-A019
Predictions of the Kuroshio and Gulf Stream with an Initialized Eddy-resolving Ocean General Circulation Model

Shoichiro KIDO#+, Masami NONAKA, Yasumasa MIYAZAWA
Japan Agency for Marine-Earth Science and Technology

The Kuroshio and Gulf Stream, which are the western boundary currents (WBCs) flowing in the North Pacific and the North Atlantic respectively, serve as key components of the wind-driven circulation. Since both currents play a key role in regulating extratropical climate variability and marine ecosystems, an accurate understanding and prediction are of paramount importance for various fields, such as weather prediction and fishery management. Although our knowledge on the physical mechanisms responsible for spatiotemporal variations in the WBC systems have been significantly advanced by recent modelling and observational studies, predictability of frontal-scale variations in the WBCs have not been fully quantified yet. To address this issue, we have conducted a series of forecasting experiments using an initialized eddy-resolving ocean general circulation model. It is found that observed year-to-year variations in the intensities of the jets and eddies in the Kuroshio Extension and Gulf Stream regions can be skillfully predicted with a lead time of about 2 years. A detailed analysis of the predicted fields demonstrated that sources of predictability mostly come from initial ocean memories and their slow propagation in the form of oceanic waves, and that changes in local atmospheric conditions play a secondary role.


OS09-A020
Interannual Eddy Kinetic Energy Variability in the Sulawesi Sea Modulated by Pacific Western Boundary Currents

Zhanjiu HAO1#+, Zhenhua XU2, Ming FENG3, Peiwen ZHANG4, Baoshu YIN4
1Institute of Oceanology, Chinese Academy of Sciences, 2IOCAS, 3Commonwealth Scientific and Industrial Research Organisation, 4Chinese Academy of Sciences

Interannual variations in eddy kinetic energy (EKE) in the Sulawesi Sea and their driving mechanisms are investigated based on the outputs of Ocean Forecasting Australia Model version 3 (OFAM3) from 1979 to 2014. The interannual EKE variability is found to be primarily modulated by the Mindanao Current intrusion transport (MCIT). By regulating the intensity of barotropic instability of the cyclonic loop current in the Sulawesi Sea, the MCIT fluctuation leads to the downstream interannual EKE variations. Further analysis suggests that the paths of Mindanao Current (MC) and New Guinea Coastal Current and Undercurrent (NGCC/NGCUC) influence the interannual MCIT variability. During high-EKE periods, the NGCC/NGCUC is weakened, and the MC retroflection extends to south of 5N, which causes MCIT to increase by 0.60 Sv and strengthens the barotropic energy conversion from mean kinetic energy to EKE in the Sulawesi Sea. During low-EKE periods, the NGCC/NGCUC is intensified whereas the MC retroflection retreats to a northernmost path, resulting in a decrease of 0.58 Sv in MCIT and thus a low EKE level. In addition, mesoscale eddies to the east of the Sulawesi Sea in the western Pacific also have an impact on the MC intrusion. This study highlights the significance of the nonlinear dynamics of western boundary currents in modulating eddy activities in the formation region of the Indonesian Throughflow.


Thu-03 Aug | 8:15 - 10:00 | MR309
OS10 - General and Multidisciplinary Oceanography

Session Chair(s): Yusuke UCHIYAMA, Kobe University

OS10-A011 | Invited
Numerical Study on the Possible Occurrence of Rip Currents After a Fasting-moving Storm

Yuli LIU1#+, Changming DONG1,2
1Nanjing University of Information Science & Technology, 2Southern Marine Science and Engineering Guangdong Laboratory

Rip currents are strong, narrow seaward water jets that can sweep unexpected swimmers into deep water, where exhaustion and panic often result in drownings. Waves and topography features are widely perceived as the main control of rip currents in sandy beaches, while meteorology conditions are relatively less connected to their occurrences. Fast-moving storms and the storm-induced meteotsunamis were recently found to be a possible cause of rip currents, even under moderate waves. Nevertheless, the associated generation processes have not been systematically examined and the characteristics of rip currents after a fast-moving storm remain unclear. In this talk, we aim to reveal the detailed hydrodynamic processes that lead to rip current occurrences using the coupled wave-current model SCHISM-WWM III. A set of numerical experiments is conducted to simulate rip currents along China’s southeastern coastline under a set of idealized storms with different propagation speeds, directions, and atmospheric pressure/wind disturbances. Results show that the passage of a fast-moving storm can induce free progressive or standing edge waves along the coastline. The induced high-frequency water level fluctuations of meteotsunamis can module wave-breaking induced vortices and shear instability of longshore currents to generate rip currents. The storm propagation speeds and directions are critical to the occurrence and timing of rip formation at coastal beaches. A heuristic approach is also explored to estimate rip current speeds from atmospheric disturbance and storm velocity. Overall, the study helps to elucidate the connection between rip current occurrence and fasting-moving storms at typical sandy beaches along China’s southeastern coasts. The findings help provide crucial beach safety messages to our coastal communities.


OS10-A009
Wave Effects on Lagrangian Transport and Dispersal in the Nearshore Zone

Yusuke UCHIYAMA1#+, Koki KATAOKA1, Kimika TAKEYASU1, Satoshi MITARAI2
1Kobe University, 2Okinawa Institute of Science and Technology Graduate University

In numerical Lagrange particle tracking modeling widely used for marine environmental problems, wave effects have been implemented crudely, i.e., simply as a linear sum of Stokes drift and background Eulerian velocity. In this study, the Lagrange equation of motion is theoretically revisited to show how it should be under wave action, and a wave-averaged 3D Eulerian circulation model with a vortex force formalism known as ROMS-WEC is exploited to examine wave effects on transport and dispersal of virtual reef coral larvae. We found that wave-driven currents strongly influence the initial dispersion and subsequent processes. The conventional ad hoc addition of Stokes drift to the Eulerian currents estimated without wave effects is likely to greatly underestimate the wave effects. This work suggests the proper direction in which the model-based oceanic material dispersion analysis should be taken under wave effects with a state-of-the-art 3D ocean modeling technique.


OS10-A001
Elliptical Near-inertial Surface Currents in a Coastal Region and Modification of Their Temporal Decays

Sung Yong KIM#+
Korea Advanced Institute of Science and Technology

We interpret seasonal and cross-shore variability of near-inertial variances in the coastal radar-derived surface currents off Oregon with a fully extended slab layer model, allowing all non-linear terms of horizontal shear and strain components and anisotropic frictional terms, by investigating the roles of vorticity and divergence on the coastal near-inertial currents. Dominant clockwise variance and non-negligible counter-clockwise variance in the near-inertial frequency band appear as elliptical near-inertial motions. The ellipticity of the near-inertial currents, which appears as a regionally dominant clockwise polarization up to −0.5 offshore and −0.2 near the coast, is associated with vorticity modifying the effective Coriolis frequency by up to half of the local Coriolis frequency. The temporal decay scales of near-inertial currents are enhanced in fall and winter and weakened in spring and summer, which are influenced by non-isotropic frictional coefficients and seasonal divergence and convergence related to ageostrophic currents. The proposed slab layer model shows that (1) the effective Coriolis frequency is modulated by background vorticity and difference of anisotropic frictional coefficients; (2) the effective frictional coefficient, including horizontal divergence terms, plays a role in accelerating and decelerating the temporal decay of near-inertial motions; and (3) The feasibility of the model in interpreting the near-inertial motions in the coastal regions where horizontal shear and strain flows and anisotropic bottom frictions become significant. 


OS10-A032
Spatial-temporal Characteristics of Submesoscale Fronts in Bay of Bengal and Their Impact to Vertical Thermohaline Structure

Wei DUAN+, Xuhua CHENG#
Hohai University

Based on a high resolution model output (MITgcm LLC4320), characteristics of different types of fronts in Bay of Bengal (BoB) and their effect to the vertical thermohaline structure are investigated. Geographic maps of temperature, salinity and density horizontal gradients reveal vigorous submesoscale frontal structures in the northern BoB with horizontal scale of ~ O (1) km. In the surface, salinity instead of temperature controls the density fronts. In winter, the intensity of fronts are more pronounced ascribe to the deeper mixed layer and more storage of available potential energy (APE). Turner angle in northern BoB reveal the coexistence of compensation and synergy effects with remarkable seasonal feature. At surface frontal region, synergy effect acts in summer and fall while compensation effect dominate over the rest period. At subsurface where salinity lose its control on density, there are more synergy signals around density fronts and more compensation signals around salinity/temperature fronts. During the generation periods of fronts, restratified effect of frontogenesis induced secondary circulation counteracts with surface convergent flow, preventing further development of surface fronts. When fronts get arrest, the isopycnals collapse within a short time due to gravitational adjustment.


OS10-A015
Numerical Study of Three-dimensional Flow Field with Convectively Unstable Processes in a Rotating Frame

Qian CAO1+, Changming DONG1,2#
1Nanjing University of Information Science & Technology, 2Southern Marine Science and Engineering Guangdong Laboratory

Convectively unstable processes caused by heavy water subsidence are frequently occuring phenomena in high-latitude oceanic regions, which have significant impacts on mass and heat transports as well as mixing processes in the ocean. In the present study, the large eddy simulation (LES) method is used to analyze the three-dimensional flow field structure of heavy water subsidence through an ideal numerical experiment with forced salt fluxes at the sea surface to simulate the phenomenon of icing and salting out at high latitudes. The results show that the average three-dimensional flow field of heavy water subsidence is in a hollow cone-shaped distribution, and there is a rising compensation of seawater inside the cone surrounding by sinking water. The horizontal flow field is a horizontal annular vortex rotating in the counterclockwise direction under the balance between the pressure gradient and Coriolis force. The vertical velocity oscillates in a frequency of internal wave. In addition, the heavy water subsidence processes also induce a vertical secondary circulation on both sides of the main sinking flow. The sinking plume of the high-salinity water mass rotates clockwise with a period of 8 h. Moreover, the effect of different rotational conditions on the structure of the three-dimensional flow field of heavy water subsidence is analyzed by sensitivity tests in this study.


OS10-A012
Modelling Study on the Sediment Dynamics and the Formation of the Flood-tide Delta Near Cullendulla Beach in the Batemans Bay, Australia

Gang YANG#+
Nanjing University of Information Science & Technology

The first 3-D current-wave-sediment coupled model of the semi-exposed estuary Batemans Bay, New South Wales, Australia, was developed in our study based on the Finite Volume Coastal Ocean Model (FVCOM). Our study explored the hydrodynamics, sediment dynamics and morphology change inside the Batemans Bay under large wave events. The modelled monthly-averaged residual flow, sediment flux and suspended sediment concentration with a combined tidal and wave forcing in the inner bay were significantly different to those only with tidal forcing, this is because the storm wave events can generate wave-induced currents and large bottom stresses, influencing the sediment transport. In addition, the morphology change of the flood-tide delta (FTD) inside the Batemans Bay under wave effects was also investigated in this study. According to previous studies, the FTD is a sediment deposit located on the landward side of tidal inlets, formed by the incoming tidal currents and ocean waves, which is an important morphology coastal feature influencing the sediment exchange with adjacent beach systems. Yet, the dynamic processes of FTDs have not been fully understood and explored quantitatively in sheltered estuaries. Based on our model results, the FTD near Cullendulla Beach is controlled by wave effects and was in an equilibrium status. The rocky headland adjacent to the FTD contributed to the formation of the FTD due to sheltering effects, and the FTD actually developed at the ‘wave shadow areas’ behind the headland in Batemans Bay, which were dominantly controlled by sheltering effects. Despite being termed a ‘Flood-Tide Delta’, ‘Tide’ here is misleading, and a new name of ‘Wave Shadow Shoal’ should be given to describe such wave-dominated coastal features. In conclusion, this study demonstrated that waves played the dominant role in the hydrodynamic processes, sediment transport and morphology change in Batemans Bay.


OS10-A004
Dynamic Changes of Huizhou Coastline in Nearly 50 Years Based on Landsat Images and DSAS

Guifang ZHANG#+
Sun Yat-sen University

On the foundation of 6 periods of Landsat satellite images from 1973 to 2019, this paper obtained coastline data of each period and calculated the changes both in its length and type by means of human-machine interactive interpretation. Detailed analysis in terms of Net Shoreline Movement (NSM), the End Point Rate (EPR) and the Linear Regression Rate (LRR) in the Digital Shoreline Analysis System (DSAS) were conducted to explore the potential driving factors regarding the dynamic changes of the coastline. The results show that from 1973 to 2019, the total length of coastline of Huizhou increased from 224,565m to 249,656m, with an average NSM of 185.46m and an average EPR of 4.04m/a. The coastline was mainly characterized by erosion from 1973 to 1984 and showed an overall expansion trend afterwards. The expansion amplitude of coastline exceeded the highest during 1984-1993, with NSM reaching 100.2m. In addition, the artificial coastline shown the most remarkable change (8.27%~57.45%) among the different coastline types, which is mainly distributed in Daya Bay Petrochemical Zone, northern Fanhe Bay reclamation and aquaculture Section, Huizhou Port, western Kaozhou Bay reclamation and aquaculture Section, and vicinity of Huangbu Town section. The main reasons of coastline change include development of coastal aquaculture, construction of ports, industrial areas and coastal tourist areas, and the expansion of construction land due to population growth and economic development. Some segments of coastline, such as the core area of Xunliao Bay, as well as the east and the west flank of Shuangyue Bay, remained stable during the whole time period. We conclude that human impact was the mainly driving factor and natural factors have little influence in charge of the coastline change during past nearly 50 years. 


Thu-03 Aug | 8:15 - 10:00 | MR310
OS04 - Understanding Multiscale Sea-level Change Using Observations and Models: Global to Local

Session Chair(s): Dhrubajyoti SAMANTA, Nanyang Technological University, Trina NG, Centre for Climate Research Singapore/NTU, Xuebin ZHANG, Commonwealth Scientific and Industrial Research Organisation, Oceans and Atmosphere

OS04-A018 | Invited
What Do We Really Know About Historical Sea-level Change?

John CHURCH1#+, Jinping WANG2
1University of New South Wales, 2Ocean University of China

Accelerating sea-level rise in much of the world will result in impacts through the 21st century and beyond. Despite the clear identification of an accelerating rise, many uncertainties remain. Understanding historical sea-level change is a prerequisite for building confidence in useful and accurate predictions of future changes. For many decades, our limited knowledge of the contributions to sea-level change could not explain the rise measured by coastal tide gauges – the sea level enigma. New and improved in situ and satellite observations of the ocean, improved understanding of the “solid Earth”, and better understanding and improved modelling of the climate system have helped resolve this enigma. A number of recent studies have argued that the sum of contributions from both observations and model estimates to sea-level change over the satellite era, the last half century and since 1900 adequately explains the observed sea-level rise, which means the sea-level budget is closed. The major contributions are from ocean thermal expansion and contributions from glaciers, with an accelerating ice sheet contributions over the recent decades. Our recent work has explored the sensitivity of global and regional sea-level reconstructions to poorly known land motions and the factors causing temporal and regional variations in the rate of rise. With this knowledge, existing reconstructions of global mean sea level are mostly not significantly different to each other from 1900 to the present, both in the time-averaged rate and the temporal variability. However, while the averaged rate over 1900 to present is similar to that from the sum of contributions, the rate of reconstructed GMSL rise is significantly smaller/larger than the sum of contributions prior to 1940/after 1970. Why is this? What do we really know? What are potential explanations for this continuing enigma? And can we constrain projections for the 21st century and beyond?


OS04-A010 | Invited
Sea-level Science: Above the Water

Benjamin HORTON1,2#+
1Nanyang Technological University, 2Rutgers University

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 3–4°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, we illustrate the ways in which current methodologies and historical data sources can constrain future projections, and how accurate projections can motivate the development of new sea-level research questions to adapt and mitigate to climate change.


OS04-A011
Observed Sea-level Rise in the Southeast Asian Seas: Causes and Implications

Nidheesh GANGADHARAN1#+, Trina NG2, Aurel MOISE1
1Centre for Climate Research Singapore, 2Centre for Climate Research Singapore/NTU

Satellite observations since 1993 of sea surface height variations show that the mean sea level is rising in the southeast Asian Seas (SEAS) with a regional mean rate of 4.3 mm/yr, which is slightly higher than the global-mean sea-level rise (~ 3.4 mm/yr) for the same period. The rates of relative and geocentric sea-level rise deviates significantly from each other at many selected tide-gauge stations in the SEAS, suggesting the significance of vertical land movements driving the relative sea-level rise in the region. Further analyses in conjunction with ocean reanalysis data showed the respective contributions of sterodynamic sea-level (SDSL) changes and the sea-level change from contemporary mass redistribution (CMR) to the observed sea-level rise with distinct spatial signatures in the SEAS. Thermosteric sea-level rise controls the SDSL rise in the deep basins while the SDSL rise in the shallow shelf seas is mostly driven by mass loading associated with steric sea-level gradients. The spatial distribution of sea-level-rise trends from CMR is nearly uniform in the SEAS, with a few regions showing notable deviations.


OS04-A014
Influence of ENSO, PDO and IOD on the Sea Level Variability Over South East Asia

Johnson ZACHARIAH1, Daiane FALLER1, Nidheesh GANGADHARAN2, Bijoy THOMPSON1,3#, Pavel TKALICH1+
1National University of Singapore, 2Centre for Climate Research Singapore, 3TCOMS

Sea-level rise and variability are important indicators for climate change, with direct impacts on coastal society, island countries and far-reaching effects on global population and economy. The present study investigates the influence of air-sea coupled phenomena such as, El Nino Southern Oscillation (ENSO), Pacific Decadal Oscillation (PDO) and Indian Ocean Dipole (IOD) on the regional sea level variability over the South East Asian region. To determine the impact of the phenomena over different regions of the domain, available tide gauge stations are decisively selected which holds a continuity over the time period 1961-2022. Initially the estimated monthly sea surface height and anomalies from the tide gauges measurements were compared with the monthly Sea level anomalies (SLA) from the satellite altimetry (TOPEX/Poseidon, 1993-2020) employing the statistical techniques. Both the data sets shows good agreement with their temporal variability. The data sets were de-trended and low-pass filtered to eliminate the seasonal and intra-seasonal signals. To determine the embedded sea level signals due to the PDO, ENSO and IOD phenomena, the monthly sea level anomalies were low pass filtered for respective frequencies. The sea level signals are well correlated with the multivariate ENSO, PDO and IOD indices. The results reveals that the low frequency sea level variability over the entire region is mainly determined by the ENSO and PDO forcings; however, the IOD induced sea level variability is prominent only over the eastern regions of domain. The spatial variability and the magnitude of sea level deflection due to the PDO, ENSO and IOD phenomena are analysed and discussed.


OS04-A004
Role of Mass Redistribution in South China Sea Regional Sea Level Variability and Trends

Bijoy THOMPSON1,2#, Svetlana JEVREJEVA3, Johnson ZACHARIAH1, Daiane FALLER4, Pavel TKALICH1+
1National University of Singapore, 2TCOMS, 3Centre for Climate Research Singapore, 4Federal University of Rio de Janeiro

Along with the glacial isostatic adjustment (GIA) and barystatic-gravitational, rotational and deformational (GRD) fingerprints, the sterodynamic processes is an important contributor to the regional sea level changes. The study investigates the role of steric and ocean mass redistribution (OMR) on the regional sea level seasonal variability and long-term trends over the South China Sea (SCS) using a high-resolution regional ocean model simulation, and tide-gauge as well as satellite observations. Ocean hindcast simulations, carried out for 1958-2022 period, using the Nucleus for European Modelling of the Ocean (NEMO) ocean circulation model configured for the Maritime Continent (MC) region is employed in the study. Analysis of model sea surface height (SSH) linear trend together with available tide gauge and satellite SSH observations is presented. In general, reasonable agreement is found between the sea level linear trends estimated from the model simulations and tide-gauge/satellite observations. In the annual cycle, the sea level over the shallow shelf regions in the SCS is dominantly determined by the OMR. In the long-term trends, the OMR acts as a mechanism to balance the contrasting steric induced sea level changes over the open SCS and sallow continental shelf region in the south and northwestern regions.


OS04-A016
Understanding Historical Australian Sea Level Trends and Variability

Xuebin ZHANG1#, Kathy MCINNES2, John CHURCH3+, Julian OGRADY2, Matt KING4, Benoit LEGRESY2, Claire TRENHAM2
1Commonwealth Scientific and Industrial Research Organisation, Oceans and Atmosphere, 2Commonwealth Scientific and Industrial Research Organisation, 3University of New South Wales, 4University of Tasmania

Global mean sea level has been rising and is attributed to anthropogenic climate change forcing. The causes are mainly thermal expansion due to ocean warming and addition of water mass into the ocean from melting of land ice. Regional sea levels can deviate significantly from global mean sea level due to different processes at various spatiotemporal scales. In this study, we examine Australian sea levels and underlying mechanisms based on observations from 1880s to current, including direct sea level measurements by in-situ tide gauges and satellite altimetry, as well as other relevant oceanic and atmospheric observations. We focus on three aspects to explain the regional distribution of Australian sea levels. Firstly, we examine the connection of sea levels with modes of climate variability (e.g., ENSO) and driving physical processes (e.g., wave propagation). Secondly, the regional sea level budget from 1966 to present from selected tide gauges are analysed to identify the dominant factors for sea level trends, including ocean dynamics, sea level fingerprints, vertical land movement and inverse barometer effect. Thirdly, the connection between Australian sea levels and ocean gyre circulation and boundary currents (such as the South Pacific subtropical ocean gyre and East Australian Current) are identified, focusing on coastal sea levels in response to strength and position of ocean gyres and boundary currents. Findings from this historical study improve our understanding of sea level changes and variability around Australia, which will help us to project future sea level changes in coming decades with more confidence and reliability.


Thu-03 Aug | 10:20 - 12:20 | MR309
OS13 - Ocean Observations: Data Processing, Assimilation, Reconstruction and Application

Session Chair(s): Lijing CHENG, Institute of Atmospheric Physics, Chinese Academy of Sciences, Shiqiu PENG, Chinese Academy of Sciences

OS13-A041 | Invited
Evaluation of GNSS Interferometric Reflectometry Method for Sea Level Estimation in Indonesia

Lisa A. CAHYANINGTYAS1#+, Dudy Darmawan WIJAYA1, Aditya K. UTAMA1, Rega HIMAWAN2
1Bandung Institute of Technology, 2PT Wisesa Berkah Bumi

Over the last decade, GNSS interferometric reflectometry (GNSSIR) has been developed as a technique for observing sea level height using data from GNSS satellite observations. GNSSIR estimates sea level height from the phase center antenna using the reflection of the extracted GNSS signal on the sea surface. With a large number of tidal stations equipped with GNSS antennas, GNSSIR has the potential to be implemented in Indonesia. GNSSIR observations can also cover sea surface areas tens to hundreds of kilometers away from where the antenna is located in coastal areas. Furthermore, the installation of a GNSS antenna at a safe height on land allows for the observation of sea levels during extreme conditions such as storms and cyclones. To employ GNSSIR effectively, several factors must be considered, including signal-to-noise ratio (SNR) data analysis, data processing, filtering control variables, and increased frequency extraction. However, the value of the parameters will be affected by the coastal characteristics. This study will focus on increasing temporal resolution by identifying the best control variables for each study area with different coastal characteristics in Indonesia. The results will be validated by comparing the sea level from GNSSIR and tide gauges. Furthermore, the tidal constituents from both sea levels will be compared by calculating the error absolutes of the amplitude and phase tidal constituents.


OS13-A007
Error Propagation Characteristics of Ocean Models and Assimilating Experiment in the South China Sea

Zhongjie HE#+, Yueqi ZHAO
Harbin Engineering University

Improper parameter setting is one of the sources of model error, which can be reflected in the propagation characteristics of mode error. However, this information is usually ignored in current assimilation Algorithm. In this study, a new assimilation algorithm called ensemble optimal smoothing (EnOS) was proposed, which utilizes the error propagation information to improve assimilating effect. This scheme was a straightforward extension of the ensemble optimal interpolation (EnOI) by involving time correlation information in the Kalman gain. The main advantage of this scheme was the ability to estimate the present state from the time history of observation. We applied the assimilation scheme to the South China Sea SST, and the results showed that the EnOS was more effective in eliminating model errors when compared to the EnOI scheme.


OS13-A015
Background Error Analysis and Data Assimilation of Ocean Waves Using EnOI and Satellite Altimeter

Peng QI#+, Lei CAO
Chinese Academy of Sciences

Evaluation of assimilation of satellite altimeter significant wave height (SWH) data into the third-generation wave model WaveWatch III using the ensemble optimal interpolation (EnOI) method is presented. Sampling strategy is discussed first. Differences of SWH in 24-hour interval are sampled as an estimate of background errors for members of the stationary ensemble used in the EnOI. Anisotropic distributions of the background error variance (BEC) are achieved. Hindcast/forecast experiments including assimilation run and control run are done in two monsoon areas: the South China Sea and the north Indian Ocean. It is shown that the BEC structures are of significant flow-dependency. Effects of the EnOI assimilation on analysis and forecast are evaluated with observations from several buoys. It is suggested that the altimeter SWH data assimilation using the present EnOI scheme works well. The improvement in model skill can be retained throughout the short-range forecast period. And the EnOI-based assimilations are found to have the greatest impact in areas and seasons where and when the sea-state is dominated by swells. A parallel module of the EnOI assimilation has currently been developed and embedded into the ocean wave model, which can be a new choice for operational applications due to its low computational cost.


OS13-A024
Preliminary Results of Multi-incremental Four-dimensional Variational Data Assimilation in a High-resolution Regional Ocean Model

Pinqiang WANG#+, Huizan WANG, Senliang BAO, Zhenli GAO, Yan CHEN, Weimin ZHANG
National University of Defense Technology

Four-dimensional variational data assimilation (4DVar) is one of the most widely used and sophisticated methods in the numerical weather prediction (NWP). However, there are still many limitations in the application of 4DVar in the ocean data assimilation, one major obstacle is the huge computation cost. An important feature of 4DVar in the NWP is that a multi-incremental form is adopted, that is, the tangent linear model and adjoint model are running at lower resolution than the nonlinear model. We applied the multi-incremental 4DVar to a South China Sea regional ocean modeling system. The horizontal resolution of fine/coarse grid is 1/40° and 1/8°, respectively. The results of experiments indicated that multi-incremental 4DVar has the potential to be applied to ocean modeling system, the small-scale processes were well observed in the high-resolution system and the computation cost is affordable. However, the divergences of sea surface heights (SSHs) and sea surface temperatures (SSTs) occurred after several cycles, especially for the SSH, as a result, the assimilation system collapsed. One reason may be the emergence of fast oscillations, the digital filter or incremental analysis update (IAU) is needed to handle this problem.


OS13-A035
Adjoint-based Arctic Ocean-sea Ice Reanalysis: Description, Assessment, and Future Development

Guokun LYU1#+, Meng ZHOU1, Armin KOEHL2, Detlef STAMMER2
1Shanghai Jiao Tong University, 2University of Hamburg

Arctic ocean and sea ice reanalyses are increasingly used in understanding Arctic changes. In this study, we introduce the INTRAROS-SJTU reanalysis, a dynamically consistent Arctic ocean and sea ice reanalysis product covering the period of 2007-2021. The spatiotemporal variation of Arctic sea surface temperature, sea ice concentration, and sea ice thickness is substantially improved after the assimilation of ocean and sea ice observations. In addition, INTAROS-SJTU reproduces the spatiotemporal variability sea ice state better than the newly-developed RARE, ASTE_R1, and TOPAZ4b datasets, but its ocean temperature needs to be further improved in the future release. A distinguished feature of the adjoint method is that the reanalysis strictly follows the model dynamics, permitting meaningful analysis of closed budgets at grid scales. The data provides valuable sources for understanding the causes and consequences of the Arctic sea ice changes.


OS13-A038
A Fusion Method to Improve the Value of Long-term Wave Height Reanalysis Data Based on DIVA

Tian JUNWEI#+, Li XIN, Du YANG, Tian CHENG
National University of Defense Technology

Analyzing the characteristics of long-term changes of ocean waves is very important for ocean engineering, such as offshore oil development, cross-sea bridge design and breakwater design, etc. However, the wave height of reanalysis data are usually lower than that of observation, which may lead to greater risks in practical application. In response to this problem, this paper first selected the wind wave and swell height data from ICOADS in recent decades years, which observed by ships, buoys, and other platform types, and then fused it with the wave height data from the ERA5 reanalysis through the DIVA interpolation algorithm. The parameters of interpolation algorithm were determined by calculating the monthly sum of RMSE between fusion date and reanalysis that both were max-min normalized, based on the similarity of their spatial distribution trends. The results show that monthly and annual averaged wave height of the new data are significantly increased and more close to the observations, in the case of retaining original distribution characteristics of ERA5. Based on the new fusion data, the temporal and spatial distribution characteristics of swell in the North Pacific during recent decades years were analyzed by EOF method. It shows that the spatial distribution of the 1st mode likes as a belt gradually decreasing from north to south with the same phase symbol in the whole basin, which is similar to the results of ERA5. However, the spatial distribution of the 2nd mode is generally positive in the north and near sea of the basin, while it is negative in the south and distant ocean. This distribution is different from that of ERA5 results, which shows negative in east and positive in west.


OS13-A017
An Observation Thinning Method for Unstructured Grid Based on the K-dimension Tree

Yan CHEN#+, Huizan WANG, Pinqiang WANG, Senliang BAO, Xiaohui WANG, Weimin ZHANG
National University of Defense Technology

Observation data need to be preprocessed before data assimilation. The observation thinning method is one step of the preprocessing which thining spatially dense observations relative to model grid, so as to remove the redundant observation information and/or the spatial correlation of observations. In general, regular structure grids are stored in the form of two-dimensional array, and equally spaced in the east-west direction and the north-south direction, which can effectively search which grid the observation is in. However, unstructured grids are stored in one-dimensional array, and arranged disorderly, and most observation thinning methods for unstructured grid use the violent search algorithm for present. The violent search algorithm computes very slow without parallel, and it can not meet the time requirements for the operational data assimilation with 106-108 model grids and 106-107 observations. We established an observation thinning method for unstructured grid based on the K-Dimension (KD) tree which has high computational efficiency for disordered data. Using the global Finite-Volume Community Ocean Model (FVCOM) with about 105 unstructured triangular grids, an experiment for 1/20° OSTIA SST observation thinning is conducted in Tianhe-1. Without parallel, the KD tree thinning method only takes about 15s to process about 107 observations, but the violent search algorithm needs over 200s to process only 1 observation. The acceleration of the KD tree thinning method is significant and has large implications for researchers applying the method for operational applications, such as data assimilation in high-resolution ocean models or numerical weather prediction models.


Thu-03 Aug | 10:20 - 12:20 | MR310
OS05 - On “timescale” of Ocean Motions

Session Chair(s): Zhiqiang LIU, Southern University of Science and Technology

OS05-A016 | Invited
Space and Time Dependent Global Ocean Energy Transfers in the Frequency Domain Inferred from Satellite Observations

Yang YANG1#+, X. San LIANG2
1Xiamen University, 2Fudan University

Using a new analysis tool, namely, multiscale window transform (MWT), and the MWT-based theory of canonical transfer, this study investigates the spatio-temporal variations of the nonlinear interactions among the mean flows, interannual variabilities, quasi-annual fluctuations and eddies in the global ocean. It is found that the canonical kinetic energy (KE) transfers are highly inhomogeneous in space, maximized in the western boundary current (WBC), Southern Ocean and equatorial regions. In contrast to the equatorial and WBC regions where the temporal KE cascades are mainly forward, the Southern Ocean is the very place where coherent large-scale patterns of inverse KE cascade take place. The canonical transfers are also found highly variable in time. Specifically, in the Kuroshio Extension, the transfer from the mean flow to the interannual variability is in pace with the external winds from the eastern North Pacific; in the subtropical gyre, the mean flow-to-eddy transfer is responsible for the variability of the eddy kinetic energies (EKE) at both interannual and seasonal scales; in the tropics, the downscale transfers to the eddies from the other three scales all contribute to the interannual modulation of the EKE, and these transfers tend to decrease (increase) during El Niño (La Niña) events. In the Southern Ocean, the high-frequency eddies are found to feed KE to the low-frequency variability through temporal inverse cascade processes, which have been strengthened due to the enhanced eddy activities in the recent decade. Also discussed here is the relation between the seasonal EKE variability and the eddy-quasi-annual fluctuation interaction.


OS05-A012 | Invited
Rapid Vertical Exchange at Fronts in the Northern Gulf of Mexico

Lixin QU1#+, Leif THOMAS2, Aaron WIENKERS3, Robert HETLAND4, Daijiro KOBASHI5, John TAYLOR3, Fucent HSU6, Jennifer MACKINNON7, Kipp SHEARMAN6, Jonathan NASH6
1Shanghai Jiao Tong University, 2Stanford University, 3University of Cambridge, 4Pacific Northwest National Laboratory, 5Texas A&M University, 6Oregon State University, 7Scripps Institution of Oceanography

Over the Texas-Louisiana Shelf in the Northern Gulf of Mexico, the eutrophic, fresh Mississippi/Atchafalaya river plume isolates saltier waters below, supporting the formation of bottom hypoxia in summer. The plume also generates strong density fronts, features of the circulation that are known pathways for the exchange of water between the ocean surface and the deep. Using high-resolution ocean observations and numerical simulations, we demonstrate how the summer land-sea breeze generates rapid vertical exchange at the plume fronts. We show that the interaction between the land-sea breeze and the fronts leads to convergence/divergence in the surface mixed layer, which further facilitates a slantwise circulation that subducts surface water along isopycnals into the interior and upwells bottom waters to the surface. This process causes significant vertical displacements of water parcels and creates a ventilation pathway for the bottom water in the northern Gulf. The ventilation of bottom water can bypass the stratification barrier associated with the Mississippi/Atchafalaya river plume and might impact the dynamics of the region's dead zone.


OS05-A015
Spatiotemporal Characteristics and Dynamics of Submesoscale Processes in the Northern Bay of Bengal

Yifei ZHOU+, Xuhua CHENG#
Hohai University

The spatiotemporal characteristics and dynamics of submesoscale processes (SMPs) in the north BoB (nBoB) are investigated by the output of a high-resolution model simulation. The results show that the nBoB have abundant energetic submesoscale processes, with significant seasonality and geographic variability. The head basin (region A) and central basin (region B) of the nBoB are identified as two typical spots of submesoscale motions. Seasonally, SMPs in region A are strongest in spring and are highly correlated with mesoscale strain rate (MSR). By contrast, SMPs in region B are more active in winter and late summer due to the combined effects of deep mixed layer depth and strong MSR. Energy analysis suggests that baroclinic instability is a dominant generation mechanism for energetic SMPs in region B during winter and summer. During spring, the prevalent submesoscale kinetic energy (KE) reservoir in region A is fueled by wind forcing, buoyancy conversion, and the forward KE cascades from mesoscale processes, and mainly balanced by the inverse KE cascades from submesoscale to large-scale processes.


OS05-A017
The Response of Water Exchange to Climate Control and Cumulative Local Intrusion/offshore Force in Northern South China Sea

Lingbo CUI1#+, Zhongya CAI1, Zhiqiang LIU2
1University of Macau, 2Southern University of Science and Technology

The exposure time(θ) was used as a tool to explore the response of the water exchange in marginal sea to the climate control and compare discrepancies of the cumulative effect between the long-term water transport and local hydrodynamic force. The water exchange has the annual averaged mean θ of ~ 75days in Northern South China Sea and the timescale of it shows clear spatial and seasonal variation. Spatially, the nearshore region occupied the high θ (~150-300 days )and the largest θ occurred in Beibu Gulf, further more, the costal region(<50m) and middle Beibu Gulf shows the opposite changes with southeastern shelf varies seasons. In water column, local intrusion/offshore force established the vertically uneven distribution of θ, but the average cumulative effect of the long-term water transport is only significant in specific places, such as the northeast side of Hainan Island, outside of the Pearl River Estuary, and the west side of Taiwan Island, which has the discrepancies with the long-term cumulative local hydrodynamic force. Temporally, θ was the shortest in the winter(~60days) and longest in spring(~80days). In the interannual timescale, the exchanges time scale is strongly modulated by the ENSO, particularly over the Beibu Gulf. During the El Nino year with the northeastward flow anomaly, a relatively strong eastward transport occurred with the weak water exchange, therefore, cause the θ increased, while in the La Nina year, because of the southwestward flow anomaly, the θ decreased with the strengthen westward water transport.


OS05-A006
Material Transport by Oceanic Coherent Eddies

Tongya LIU#+
Second Institute of Oceanography, Ministry of Natural Resources

In this study, millions of Lagrangian particles are advected by satellite-derived surface geostrophic velocities over a period of 1993-2019. Using the method of Lagrangian-averaged vorticity deviation, we present a global Lagrangian eddies dataset. This open-source dataset contains not only general features (eddy center position, equivalent radius, rotation property, etc.) of eddies with lifespans of 30, 90, and 180 days, but also the trajectory of particles trapped by coherent eddy boundaries over the lifetime. We present the statistical features of Lagrangian eddies and compare them with those of the most widely used sea surface height (SSH) eddies, focusing on generation sites, size, and propagation speed. Our eddy dataset provides an additional option for oceanographers in studying the interaction between coherent eddies and other physical or biochemical processes in the Earth system.


OS05-A011
Enhanced Cross-shore Exchange by the Front Associated Eddies

Tingting ZU1#+, Lixin QU2, Zhiqiang LIU3, Zhongya CAI4
1Chinese Academy of Sciences, 2Shanghai Jiao Tong University, 3Southern University of Science and Technology, 4University of Macau

Cross-shore flows could be driven by a variety of physical processes on different time scale. In this study, simulated circulations show synoptically enhanced cross-shore flow over the western shelf of the northern South China Sea during pre-summer monsoon period. The enhanced cross-shore exchange flows are caused by eddies generated through the baroclinic instability of shelf fronts during monsoon transition periods. A buoyant plume dominated salinity front and a temperature dominated thermal front co-exist over the western shelf during this period, and the alternating of the along-shore wind over the shelf triggers two trains of eddies along the fronts. These eddies interact with each other and lead to the enhanced exchange flow and material transport.


OS05-A003
Hypoxia Formation Off the Pearl River Estuary: Sediment-water Fluxes and Time Scale of Hypoxia Occurrence

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 exchange processes are crucial for the water column oxygen dynamics and hypoxia formation. Utilizing a three-dimension physical-biogeochemical model of the Pearl River Estuary (PRE) coupling to different sediment parameterizations, we investigate the impacts of sediment-water fluxes of oxygen and nutrients on the water column biogeochemistry and hypoxia generation in the typical eutrophic coastal environment. Model results show that the simulated oxygen content and the hypoxic extent are markedly sensitive to the parameterization of sediment-water fluxes, highlighting the critical role of sediment processes in regulating oxygen dynamics off the PRE. We find that coupling the physical model with a sediment oxygen consumption (SOC) rate as a function of the bottom water oxygen level, bottom temperature, and the summer climatology of surface chlorophyll concentration alone (i.e., without water column oxygen consumption) can reasonably reproduce the observed hypoxia spatial distribution, further revealing the importance of SOC to hypoxia formation off the PRE. In addition to directly contributing to hypoxia through SOC, our experiments show that sediment-released nutrients significantly promote hypoxia development by fueling water column organic matter production. Finally, we estimate the timescale of hypoxia occurrence, defined as the ratio of initial oxygen level above hypoxia to net oxygen consumption rate in the water column and sediment. The timescale of hypoxia occurrence is compared with water residence time to identify the hotspots and the underlying physical and biogeochemical drivers for hypoxia formation off the PRE.


Thu-03 Aug | 1:00 - 5:15 | Summit
OS - Ocean Sciences Poster Session

OS01-A002
Interactions Between Ocean and Successive Typhoons in the Kuroshio Region in 2018 in Atmosphere–ocean Coupled Model Simulations

Yuma KAWAKAMI1#+, Hideyuki NAKANO1, Shogo URAKAWA1, Takahiro TOYODA2, Kei SAKAMOTO2, Hiromasa YOSHIMURA1, Eiki SHINDO1, Goro YAMANAKA2
1Meteorological Research Institute, Japan, 2Japan Meteorological Agency, Japan

Typhoons decrease sea surface temperature (SST) along their wakes through upwelling of subsurface water, vertical mixing in the upper ocean, and heat release from the sea surface, and these cold wakes can influence subsequent typhoons. In this study, we investigated interactions between the upper ocean and typhoons in the North Pacific subtropical gyre with focuses on Kuroshio's response and feedback using atmosphere–ocean coupled model simulations. In late August and early September 2018, typhoons SOULIK, CIMARON, and JEBI passed through the northwestern subtropical gyre. During the passages of SOULIK and CIMARON, SST decreased along their paths due to vertical mixing except in the Kuroshio region. We quantitatively revealed that the Kuroshio stayed warm because the deep mixed layer along its path and small vertical temperature gradient around the mixed layer base, which are unfavorable conditions for cooling by vertical mixing, limited the cooling effects. After SOULIK and CIMARON had passed, SST recovered through horizontal Kuroshio heat transport and radiative heating. The possibility that the SST field after SOULIK and CIMARON passages influences JEBI was also discussed. Although impacts on JEBI intensity were not identified, it is implied that the turbulent heat flux (THF; sum of the sensible and latent heat fluxes) around JEBI was modulated by the SST field: heat release from the ocean was reduced in the region with decreased SST and enhanced over the sustained high SST of the Kuroshio. Furthermore, the large THF over the Kuroshio may have caused an increase of JEBI-associated precipitation around Japan.


OS01-A012
Typhoon Hinnamnor Interacting with Underlying Marine Heatwaves

Saranya J.S., SungHyun NAM#+
Seoul National University, Korea, South

Typhoons draw their energy from underlying warm oceans. In a warming climate, oceans are often experiencing extreme sea surface temperature conditions known as marine heatwaves. The interactions between typhoons and marine heatwaves constitute a significant concern in a changing climate and require immediate attention. Typhoon Hinnamnor was a severe typhoon that interacted with underlying marine heatwave conditions near the Korean strait before hitting the southern part of the Korean Peninsula on September 6, 2022; it is an excellent case to study the interaction between typhoons and marine heat waves. After reaching maximum intensity in the open ocean, typhoon Hinnamnor started moving northward from September 2 towards the Korean strait and initially declined its strength. However, the typhoon reintensified from September 3 to September 5, increasing the maximum wind speed from 75 kt to 90 kt in the presence of underlying marine heatwave (MHW) conditions. This study resolves the crucial ocean-atmosphere interactions during the typhoon's intensification and decay in the presence of marine heat waves. We analyzed in-situ time-series observational data observed at multiple locations in the seas around the Korean Peninsula along with the ECMWF Reanalysis v5 (ERA5) reanalysis data before, during, and after the typhoon passage. Results show that increased latent heat flux from the ocean to the atmosphere associated with the MHWs in the Korea Strait sustained the typhoon's high intensity. In contrast, the MHWs decayed abruptly due to strong typhoon wind-induced vertical mixing (mixed layer thickened from 10 m to 30 m) and sea surface cooling up to 2.72 °C. Our results provide a case study on the interactions between two major extreme events in the climate system, providing crucial insights into the interplay between MHWs and typhoons and their combined impacts on the coastal environments and marine ecosystems.


OS01-A014
The Upper Ocean Response Due to Three Sequential Tropical Cyclones in the Bay of Bengal

Abhishek KUMAR#+, Arun CHAKRABORTY, Biplab SADHUKHAN
Indian Institute of Technology Kharagpur, India

The physical and biological response of the three sequential tropical cyclones(TCs) was investigated in the Bay of Bengal region using in-situ observations, multi-satellite data, and biogeochemistry model outputs from November-December 2013. We looked at the responses of TC Helen, Lehar, and Madi. The Lehar cyclone formed in the Andaman Islands soon after storm Helen made landfall, whereas the Madi cyclone formed eight days after the Lehar cyclone dissipated. Helen and Lehar's journey lowered the sea surface temperature (SST) by 1°C. Despite this, the SST in the region stayed over 26.5°C, allowing cyclone Madi to develop. The initial chlorophyll-a (CHL-a) boost was linked to CHL-a redistribution associated with TC-induced vertical mixing and Ekman pumping at the base of the mixed layer post-TC Helen and Lehar. Following TC Madi, Ekman pumping, entrainment, and eddy pumping pushed nutrient-rich cold waters into the euphotic layer, resulting in a more spectacular CHL-a bloom and net primary production. Upwelling was the principal strategy for replenishing nutrients towards the right side of the cyclone track channel. The near-surface dissolved oxygen content has increased significantly as a result of TC-induced vertical mixing and enhanced CHL-a photosynthesis. The consecutive cyclones' turbulence mixing and upwelling were principally responsible for preserving the lower temperature region and phytoplankton blooms. The study's goal is to deduce the reactions to these three consecutive TCs and their related physical works for phytoplankton growth and sea surface cooling.


OS01-A018
Downcoast Redistribution of Changjiang Diluted Water Due to Typhoon Chan-Hom (2015)

Yunpeng LIN1+, Yunhai LI2, Shuai CONG3, Meng LIU1, Liang WANG4, Binxin ZHENG4, Jingping XU1#
1Southern University of Science and Technology, China, 2Ministry of Natural Resources, China, 3Ocean University of China, China, 4State Oceanic Administration, China

Typhoons are known to substantially influence the coastal circulation and the associated biogeochemical processes. The transport of Changjiang Diluted Water (CDW), an important source to the coastal current in the East China Sea (ECS), varies markedly under the influence of typhoons. This study quantitively details the downcoast transport of CDW driven by Typhoon Chan-Hom in the summer of 2015. Salinity measurements 3 days after the typhoon’s passage showed the presence of a large volume of low salinity water, up to 70 km wide and 20 m thick along the Zhejiang-Fujian coastal area with an estimated freshwater volume of 3.7×1010 m3. A three-endmember mixing model shows that the CDW’s contribution to the study area’s surface waters (<10 m) immediately after the typhoon was as high as 40% (average 32%), much greater than the contribution under normal summer conditions of 8% (average 3%). The vast spreading of CDW along the Zhejiang-Fujian coast created a strong stratification in the upper water column that limited the diffusion of CDW in the study area. The calculated and observed results suggest that these abnormal low salinity water could stay in the study area for 13-21 days. Additional nutrients in the CDW elevated the Chlorophyll-a concentration in the upper water column (mean 3.74 mg m-3) and produced large amount of particulate organic carbon (POC).


OS01-A020
Decrease of Annually Accumulated Tropical Cyclone-induced Sea Surface Cooling and Diapycnal Mixing in Recent Decades

Xueyang ZHANG+, Fanghua XU#, Yanluan LIN, Jishi ZHANG
Tsinghua University, China

Tropical cyclones (TCs) are an important source of turbulent mixing for the upper ocean at low latitudes, causing sea surface cooling and subsurface warming. A new estimate of annually accumulated sea surface cooling and upper ocean diapycnal diffusivity induced by TCs is obtained by using quantified cold wake sizes, which were largely ignored by previous studies. Both the annually accumulated tropical cyclone-induced sea surface cooling and upper ocean diffusivity on a global scale show a significant decreasing trend over the period of 1982–2016, at a rate of −0.09 ± 0.03 °C/decade and −0.03 ± 0.01 cm2/s/decade respectively. The strengthening of ocean stratification with global warming contributes to the decrease of sea surface cooling and mixing, while the changes of tropical cyclone characteristics (such as translation speed, intensity, number, lifetime and size) contribute differently in various ocean basins.


OS01-A025
Sea Surface Salinity Response to Typhoons in the Northwest Pacific Using Satellite Salinity Data Over the Past Decade

Kyung-Ae PARK1#+, Jae-Jin PARK1, Wenqing TANG2
1Seoul National University, Korea, South, 2Jet Propulsion Laboratory/California Institute of Technology, United States

To investigate the potential use of satellite salinity data in studying the oceanic response to typhoons in the Northwest Pacific, the accuracy of such data was assessed by comparing it with Argo float and buoy observations over the past decade (2011-2020). The findings revealed that satellite salinity data from SMAP (Soil Moisture Active Passive) and Aquarius exhibited relatively high accuracy, particularly during the summer season and in low-latitude subtropical seas. However, despite these encouraging results, the usefulness of satellite salinity data during the typhoon season is constrained by certain limitations. To delve deeper into the topic, a comprehensive analysis was conducted on a selection of typical typhoons over the past decade, employing objective classification based on parabolic trajectories. The oceanic response to these typhoons was examined. Both Aquarius and SMAP satellites demonstrated a salinization pattern on the right side of the typhoon path, while desalination occurred on the left side. Notably, areas of reduced salinization corresponded to regions experiencing intense precipitation to the left of the typhoon's center. Additionally, there was an inverse relationship between precipitation and satellite salinity, with a salinity desalination-to-precipitation rate ratio estimated at approximately -0.0401 psu mm-1 h-1. Analyzing the vertical distribution of Argo data before and after typhoon events revealed distinctive cooling in the surface layer of seawater following a typhoon's passage. The depth of the mixed layer increased, and freshening phenomena were observed on the left side. Furthermore, transforming the coordinate system along the typhoon's path and examining the atmospheric environment exposed a localized freshening phenomenon appearing slightly ahead and to the left of the typhoon's center.


OS01-A026
Satellite Significant Wave Height Variations during Typhoon Period in the Northwest Pacific

Hye-Jin WOO, Kyung-Ae PARK#, Hee-Young KIM+, Ji-Hyun LEE, Sunwoo KIM, Park HYEWON
Seoul National University, Korea, South

The Northwest Pacific has a variety of ocean and atmospheric phenomena which show obvious spatial and temporal variability of significant wave height (SWH). In addition, the Northwest Pacific is one of the oceans with the most frequent high-intensity tropic cyclones. The typhoons are accompanied by heavy rains and huge waves as well as strong winds, which have a great impact on the coastal environment. As the intensity of typhoons is becoming stronger due to climate change, extreme wave height induced by typhoons and hazardous events can also increase in the Northwest Pacific. However, in spite of the urgent need to understand the characteristics of the extreme height in the region where typhoons occur frequently, studies on the estimation of extreme SWH in the Northwest Pacific are insufficient. In this study, the 100-year return period of SWHs was estimated by applying the Peak over Threshold method (PoT) as one of representative extreme value analysis to satellite altimeter data from 1992 to 2016. To analyze the suitability of the PoT method in the Northwest Pacific, where typhoons frequently occur, the estimated PoT-derived SWHs were compared with the maximum SWHs within the upper 0.1% of satellite observations. It was suggested that PoT method could be applied to reliably estimate the extreme SWH using the accumulated satellite observation SWH data in the Northwest Pacific.


OS02-A006
An Improved Parameterization of Wind-driven Turbulent Vertical Mixing Based on an Eddy-resolving Climate Model

Man YUAN1+, Zhuo SONG1#, Zhao JING1, Zhuoran LI1, Ping CHANG2, Bingrong SUN1, Hong WANG1, Xin LIU3, Shenghui ZHOU4, Lixin WU1
1Ocean University of China, China, 2Texas A&M University, United States, 3Qilu University of Technology (Shandong Academy of Sciences), China, 4Pilot National Laboratory for Marine Science and Technology (Qingdao), China

Turbulent vertical mixing in the stratified ocean interior has a huge impact on global ocean circulations and the climate system. Although parameterizations of vertical mixing furnished by internal tides have been built into state-of-the-art coupled global climate models (CGCMs), efforts in parameterizing wind-driven vertical mixing in CGCMs are still limited. In this study, we apply a modified finescale parameterization (MFP) to an eddy-resolving Community Earth System Model (CESM) to represent the wind's contribution to vertical mixing in the stratified ocean interior. The spatial pattern of the MFP-parameterized wind-driven vertical mixing in the thermocline agrees with the observation derived from the finestructure measurements of Argo floats, reproducing the enhanced values in the Kuroshio, Gulf Stream extensions, and the Southern Ocean where the winds inject great amount of energy into the internal wave field. The MFP also captures the observed seasonal variation of wind-driven vertical mixing in the thermocline of these regions that exhibits enhancement and weakening in winter and summer, respectively. Application of the MFP to a non-eddy-resolving CESM fails to reproduce the observed wind-driven vertical mixing. Specifically, the magnitude of parameterized wind-driven vertical mixing in the thermocline of Kuroshio, Gulf Stream extensions, and the Southern Ocean is systemically smaller than those in the observation and eddy-resolving CESM; so is the case for the amplitude of seasonal cycle. The results highlight the benefit of eddy-resolving CESM compared to its standard-resolution counterpart in parameterizing the wind-driven vertical mixing and provide insight into developing parameterizations for wind-driven vertical mixing in eddy-resolving CGCMs.


OS02-A010
Extreme Ocean Mixing in Coastal Seas

Arnaud VALCARCEL1+, Joanne O'CALLAGHAN2, Ata SUANDA3, Glenn CARTER4, Cynthia BLUTEAU5,6, Fiona ELLIOTT7, Craig STEVENS8,9#
1Oceanly, New Zealand, 2OceanlyScience, New Zealand, 3University of North Carolina Wilmington, United States, 4University of Hawaii, United States, 5Innovation Maritime, Canada, 6University of Quebec, Canada, 7University of Bergen, Norway, 8National Institute of Water and Atmospheric Research, New Zealand, 9University of Auckland, New Zealand

Turbulence-driven mixing is an essential mechanism that regulates energy transformations in the ocean and its role in the global climate. Mixing matters crucially in coastal seas, key regions of the Earth system for biological productivity and atmospheric carbon uptake. There, winds and tides can stimulate energetic turbulence in boundary layers that can interact in the interior, regulating stratification, air-sea exchanges and nutrient fluxes. The magnitude of diapycnal diffusivity, the central quantity to estimate vertical fluxes of heat and mass in the ocean, is scaled by a mixing efficiency factor often assumed to be constant. The efficiency of extreme turbulent mixing driven by high winds and fast tidal flows were investigated in an energetic ocean passage, Te Moana o Raukawa (Cook Strait, Aotearoa - New Zealand), using an extended glider dataset of in situ turbulent rates and background flow conditions, and atmospheric wind records. > 15 m/s winds and > 1.5 m/s depth-integrated tides intensified turbulence (buoyancy Reynolds numbers, Reb, up to 10^8) and extended boundary influence (a function of the Ozmidov scale, of isotropic turbulent motions) to the full water depth. For most samples, mixing efficiency coefficient (Γ) values were reduced by up to 3 orders of magnitude from the widely-used canonical Γ = 0.2 (Rf = 0.16) value. Lower energy turbulent patches free from boundary influence (i.e. Ozmidov-limited) operated with significant scatter within a standard deviation of Γ = 0.2. Moderately energetic surface or bottom boundary-influenced samples affirmed the Γ ∝ Reb^(−1/2) relationship of shear-driven turbulence. Extremely energetic turbulence influenced by both boundaries revealed a new regime for mixing efficiency variability, decreasing drastically along Γ ∝ Reb^(−9/10). The results presented here have the potential to inform how mixing efficiency parameterizations should be treated in global ocean models.


OS02-A013
Large Eddy Simulations of Ocean Vertical Mixing in the Transition Region Between Coastal and Open Oceans

Zheng WEI1+, Qing LI1#, Bicheng CHEN2
1The Hong Kong University of Science and Technology (Guangzhou), China, 2Xiamen University, China

Ocean vertical mixing is driven by complex forcings such as winds, buoyancy, and tides, and modulates the vertical exchange of energy and substance in the ocean. Physical processes that drive ocean vertical mixing are too small to be resolved in ocean general circulation models and are often parameterized. Such parameterization can be divided into two categories: bulk models and differential models. However, both categories have limitations in representing the vertical mixing in the transition region between the coastal ocean, where mixing extends throughout the whole water column, and the open ocean, where the surface and bottom boundary layers are well separated. In the transition region, the surface and bottom boundary layers can develop, interact with each other, and even merge into one layer. Nevertheless, the physical mechanisms behind this process have not been clarified. We have been using large eddy simulations to investigate the evolution of boundary layer turbulence in such transition region. Preliminary results of the turbulent kinetic energy budget analysis indicate that internal waves are generated in the stratification layer between the surface and bottom boundary layer and may play a role in the energy transfer process between the two layers. Results of large eddy simulations of boundary layer turbulence in such transition region under more complex conditions, such as changing wind forcing, surface buoyancy flux, and tides, and including the effect of topography, will be discussed. The goal is to explore the parameter space to provide basic knowledge for further improvement of ocean vertical mixing parameterizations in such transition region.


OS02-A023
The Internal Surfzone in Regional Ocean Models

Ata SUANDA#+
University of North Carolina Wilmington, United States

Realistic regional-scale ocean modeling uses the hydrostatic approximation and turbulence closure such that it does not resolve all scales of turbulence nor the dispersive aspects of coastal internal waves. Despite these limitations, output from these numerical models are what is available through regional ocean observing networks, used to forecast water properties and provide stakeholders with valuable predictions of oceanic conditions. Particularly in regions with strong internal waves, we must better understand both resolved and unresolved mixing in coastal models and improve representations of internal wave driven mixing. A recent observation-based parameterization suggests that wave-averaged, depth-integrated coastal internal wave dissipation is equivalent to internal wave energy flux divergence (Becherer et al., 2022). In this framework, a self-similar “internal surf zone” develops shoreward of an internal wave energy-saturated water depth that is a function of mean stratification and internal tide energy flux, both properties available from tidal-resolving numerical models. In this presentation, a series of shelf-focused numerical simulations of shoreward-propagating internal tides will be conducted and analyzed to quantify the kinematic similarity between the observational parameterization the internal surfzone and what is produced by the hydrostatic, RANS-type of regional models. Where available, observations of internal wave dissipation will also be discussed.


OS02-A025
Tides and Tidal Mixing at the Shelf Break in the Timor Sea North of Australia

Robin ROBERTSON#+
Xiamen University Malaysia, Malaysia

In order to characterize the tidal fields and mixing over the shelf and at the shelf break in the Timor Sea, three 51 hour time series of CTD/LADCP/VMP profiles were conducted. The shelf break and one of the shelf time series occurred during spring tide and the other shelf break time series occurred during neap tide. The time series alternated using the CTD/LADCP or VMP at two hour intervals, so a profile was collected at hourly intervals. Semidiurnal tides dominated all three time series with the hydrography changing with the tides due to tidal advection. There was also energy at 4 cpd. Intrusions of different water types occurred at various depths, indicating the generation of different water types nearby. Anomalies in temperature and salinity propagated deeper in the water column with time, indicating upward propagation of energy. Both tidal advection, intrusions, and the anomalies were stronger during spring tide. Surprisingly, mixing was just as strong during neap tides as spring tide.


OS02-A028
Estimating Diapycnal Mixing Parameters of the Eddy Regions in the Western Arctic Ocean by Using Multi-channel Seismic Reflection Method

Shun YANG1#+, Haibin SONG1, Bernard COAKLEY2, Kun ZHANG1
1Tongji University, China, 2University of Alaska, Fairbanks, United States

Turbulence mixing is considered to be an important process for maintaining oceanic overturning circulation. In recent years, the sea ice cover in the Arctic Ocean has decreased sharply, resulting in the enhancements of turbulent mixing and eddy activities. However, due to the scarcity of observations, our understanding of turbulent mixing in the ocean is still insufficient. In this work, 11 eddies are identified in the ice-free Chukchi borderland of the western Arctic Ocean using concurrent multi-channel seismic reflection data and the current velocity derived from an ADCP (Acoustic Doppler current profiler). These eddies have a horizontal scale of ~10 km, which is consistent with the local Rossby radius, so they are all mesoscale eddies. Most of these eddies are anticyclonic eddies in the halocline, consistent with existing studies. Turbulent dissipation rate can be estimated by tracing seismic events and fitting the slope spectrum of seismic events and Bachelor spectrum. Then, according to the Osborn’s method, the diapycnal diffusivity Kρ is obtained. The results show that the turbulent mixing around eddies is generally strong. Kρ at the upper boundary of eddies is high, and can reach 1×10-4 m2s-1, which may be caused by strong vertical shear. However, there is no obvious mixing enhancement at the lower boundary of eddies with strong shear, which may be caused by the underestimating buoyancy frequency at the lower boundary. Kρ at the edge of eddies is strong, which may be the result of the thermohaline intrusion or eddy stirring. Uncertainty calculations indicate that estimating turbulent mixing using seismic events is a reliable method. Given the scarcity of turbulence observation in the ocean at present, there is great potential for the application of a large number of historical seismic data in the global oceans.


OS02-A029
The Characteristics and Enhanced Diapycnal Mixing of a Cyclonic Eddy Offshore Southeast North Island, New Zealand from Multichannel Seismic Data

Kun ZHANG1#+, Haibin SONG1, Linghan MENG2, Shun YANG1
1Tongji University, China, 2School of Ocean and Earth Science, China

Mixing induced by mesoscale eddies impacts the climate and ecosystems profoundly. Multichannel seismic (MCS) data can provide high-resolution acoustic images of thermohaline fine structures in the water column, known as seismic oceanography. In this study, we analyzed a cyclonic eddy captured by the MCS data acquired on November 8th and 9th, 2017, offshore southeast of North Island, New Zealand. A concave-down structure with strong dipping and weak reflections on seismic section is identified as a typical eddy structure in the study region. The eddy has a width of over 120 km and a thickness of about 1500 m. The strong dipping reflections representing submesoscale features (e.g. fronts and filaments) at the periphery of the eddy. We used sea surface height and geostrophic current velocity derived from satellites to detect eddies in the study region. The location of the concave-down structure matched the cyclonic eddy, with a lifetime of over 30 days. To diagnose eddy activities in the region, we used physics reanalysis data from Copernicus Marine Service and Hybrid Coordinate Ocean Model. Both showed a negative Okubo-Weiss parameter at the location of the cyclonic eddy. The sea surface chlorophyll concentration derived from Aqua-MODIS satellite showed high-value spiral bands at the location of the eddy, indicating enhanced primary production in the eddy region. We computed horizontal wavenumber spectra from vertical displacements of tracked seismic reflections to estimate the diapycnal mixing rate. The mean diapycnal diffusivity in the eddy region had an average level of O (10-3.9) m2s-1, much higher than that of the open ocean. The mean diapycnal diffusivity showed a patchy distribution in the front and filament region. These findings may contribute to a better understanding of the process of energy cascade and eddy pumping in enhancing primary production in the ocean.


OS02-A030
Calculation and Analysis of the Horizontal Dispersion Coefficient in Yueqing Bay

Jia LI1#+, Yanming YAO2, Tao ZHANG1
1Ministry of Natural Resources, China, 2Zhejiang University, China

In coastal waters, the dispersion process was not longitudinal one-dimensional like in rivers, but expended horizontal two-dimensional. Based on the research result of the longitudinal dispersion process in rivers, a method to calculate the horizontal dispersion coefficient was inferred theoretically. Then a three dimensional model is used to simulate the tidal circulation in Yueqing Bay, combined with the output of which, the temporal and spatial distribution of horizontal dispersion coefficient in the bay was obtained. The analysis result indicated that the topographic influence to the horizontal dispersion appeared the character of duality: one is the positive correlation, the other is that there is some relationship between the marked changed in topography and the horizontal dispersion. At the same time, the velocity is an important factor for the horizontal dispersion, too. There is also the positive correlation between them and the tidal range and vertical distribution of the tidal current are important factors simultaneously. Furthermore, it is found that the horizontal dispersion coefficient can be estimated using an expression constructed by vertical mean velocity, tidal range and water depth.


OS03-A001
Effects of Climate Variability in Marine Ecosystems as a Bottom-up Control Regulator in the Pacific Ocean

Kuo-Wei LAN1#+, Yan-Lun WU1, Ting-Yu LIANG1, Lu-Chi CHEN2
1National Taiwan Ocean University, Taiwan, 2Fisheries Research Institute, Taiwan

How top predators behave and are distributed depend on the conditions in their marine ecosystem through bottom‐up forcing; this is because where and when these predators can feed and spawn are limited and change often. This study investigated how the catch rates of immature and mature cohorts of bigeye tuna (BET) varied across space and time; this was achieved by analyzing data on the Taiwanese longline fishery in the western and central Pacific Ocean. We also conducted a case study on the time series patterns of BET cohorts to explore the processes that underlie the bottom-up control of the pelagic ecosystem that are influenced by decadal climate events. Wavelet analysis results revealed crucial synchronous shifts in the connection between the pelagic ecosystem at low trophic levels in relation to the immature BET cohort. Many variables exhibited decreasing trends after 2004–2005, and we followed the Pacific Decadal Oscillation as a bottom-up control regulator. The results indicated that low recruitment into the mature cohort occurs 3 years after a decrease in the immature cohort’s food stocks, as indicated by a 3-year lag in our results. This finding demonstrated that, by exploring the connection between low-trophic-level species and top predators at various life stages, we can better understand how climate change affects the distribution and abundance of predator fish.


OS03-A010
Ningaloo Niño/Niña in CMIP6 Models: Characteristics, Mechanisms, and Climate Impacts

Jiaqing XUE1#+, Hongpei YANG2, Jing-jia LUO1, Chaoxia YUAN1, Boni WANG3, Toshio YAMAGATA4
1Nanjing University of Information Science & Technology, China, 2Sun Yat-sen University, China, 3Jiangsu Meteorological Service Center, China, 4Japan Agency for Marine-Earth Science and Technology, Japan

As a dominant climate mode of the southeast Indian Ocean, Ningaloo Niño/Niña has paramount impacts on regional climate and marine ecosystems. Using outputs from the latest phase of Coupled Model Intercomparison Project (CMIP6), we have systematically evaluated the simulation of Ningaloo Niño/Niña in the state-of-the-art coupled models. Eighteen out of 28 CMIP6 models well reproduce the spatial pattern and seasonality of Ningaloo Niño/Niña, whereas the simulated amplitudes show large spread across the models. Main processes of the oceanic and atmospheric El Niño-Southern Oscillation teleconnections and the coastal Bjerknes feedback are successfully captured by most of the CMIP6 models, but their uncertainties in the simulation are responsible for the inter-model difference in amplitude. The CMIP6 models are also skillful in reproducing the regional climate impacts of Ningaloo Niño/Niña. Compared to Coupled Model Intercomparison Project Phase 5, a larger fraction of models in CMIP6 well reproduce the Ningaloo Niño/Niña, which provides a good hope for projecting its future changes.


OS03-A027
The Modulations of the Pacific North Equatorial Current Bifurcation by Interannual-to-decadal Climate Variability

Li-Chiao WANG#+
National Central University, Taiwan

Long-term reanalysis data were used to assess interannual-to-decadal modulations of the North Equatorial Current (NEC) bifurcation in the Pacific. Wind stress curl anomaly (WSCA) in the region of 10N–15N and 160E–170E (C-BOX) generates oceanic Rossby waves and affects the NEC bifurcation along the Philippine coast. Our analysis results show that oceanic Rossby waves are preferentially generated in either the negative Pacific Decadal Oscillation (PDO) phase when the El Niño–Southern Oscillation (ENSO) signal dominates, or in the positive PDO phase when the ENSO signal is overshadowed. In the phase when the positive PDO counteracts with the ENSO signal, neither ENSO nor PDO has a significant influence on oceanic Rossby wave generations through the WSCA. Moreover, our further analysis revealed that the WSCA has also been remotely modulated by the Southern Annular Mode (SAM). It is demonstrated that the SAM shifted to its positive phase at this transition and began strongly impacting the WSCA in the C-BOX and the NEC bifurcation. During the positive SAM phase after the early 1990s, strong climate variability occurred in the tropical to the subtropical area of the North Pacific, with a clear footprint connected to the Antarctic region. During the positive SAM phase, a dipole sea surface temperature pattern was generated in the South Pacific; this induced an atmospheric Rossby wave train in upper-level wind shear that propagated northward to the North Pacific. Such effects further enhanced downward motion and divergence at the surface, intensifying the easterlies in the equatorial area and the anticyclonic WSCA in the C-BOX. The anticyclonic WSCA in the C-BOX substantially excited downwelling oceanic Rossby waves at the surface, inducing an equatorward trend of NEC bifurcation after the early 1990s.


OS03-A028
Early Warning of the Indian Ocean Dipole Using Climate Network Analysis

Zhenghui LU#+
National Institute of Natural Hazards, Ministry of Emergency Management, China

The Indian Ocean Dipole (IOD), an air-sea coupled phenomenon over the tropical Indian Ocean, has substantial impacts on climate, ecosystem and human society. Due to the winter predictability barrier, however, a reliable prediction of the IOD has been only limited with three or four months in advance. Our work approaches this problem from a new data driven perspective, the climate network analysis. Using this network-based method, an efficient early warning signal for the IOD event was revealed in boreal winter. As a result, our finding can correctly forewarn the IOD events from December of the previous year with one calendar year in advance with a hit rate of higher than 70%, which strongly outperforms that of the current dynamical models.


OS03-A032
Impacts of Diverse El Niño Events on North Tropical Atlantic Warming in Their Decaying Springs

Weihao GUO#+
South China Sea Institute of Oceanology, China

Previous studies have demonstrated that North Tropical Atlantic (NTA) warming can be modulated by El Niño events through atmospheric teleconnections. Considering the diversity of El Niño events, this study focuses on different responses of the NTA sea surface temperature (SST) to eastern Pacific (EP), central Pacific type I and type II (CP‐I and CP‐II) El Niño events in their decaying springs. In EP and CP‐II El Niño events, the pattern of NTA warming is well established, while the NTA SST fails to warm in CP‐I El Niño events. In EP and CP‐II El Niño events, anomalous cyclones can be excited in the subtropical Atlantic. Consequently, anomalous southwesterly winds in the NTA weaken the background northeasterly winds and suppress oceanic latent heat loss, leading to NTA warming. However, in CP‐I El Niño events, anomalous anticyclones are excited in the subtropical Atlantic and anomalous northeasterly winds in the NTA strengthen the background northeasterly winds, which facilitate oceanic latent heat loss and lead to NTA cooling. The inconsistent remote atmospheric responses of the NTA are attributed to the different patterns of warm and/or cold SST anomalies in the tropical Pacific in the decaying springs of different types of El Niño events. The physical mechanism linking the SSTs in the tropical Pacific and the NTA has been verified in a slab ocean model.


OS03-A034
Upper Arctic Ocean Properties and Relationships with Sea Ice in CMIP6 Historical Simulations

Wei CHENG#+
University of Washington, United States

While current-generation CMIP and OMIP models have biases in their upper Arctic Ocean hydrography, it is less clear how these biases impact the models' ability to simulate the observed Arctic sea ice. In this study we seek to quantify relationships between sea ice and ocean states in CMIP6 historical simulations and identify common model behaviors. Multi-model mean (MMM) simulations exhibit accelerated changes in the ice and ocean system since the late 20th century. Underlying the MMM is strong inter-model variation in the simulated ice and ocean mean states, trends, and variability. However, despite the inter-model differences, simulations show consistent relationships between upper ocean property and sea ice changes, in particular, there is a common ratio between sea ice reduction and upper ocean warming or stratification increase across the models. Our results highlight the urgent needs for reliable Arctic Ocean observations or data products in order to better contextualize modeling results.


OS04-A003
Surge Residuals at the Singapore Coast

Zhi Yang KOH#+, Benjamin GRANDEY, Lock Yue CHEW
Nanyang Technological University, Singapore

We analyse the non-tidal residual at Singapore’s coast using tide gauge records at Tanjong Pagar from 1999 to 2018 and at Johor Bahru from 1993 to 2013. Using harmonic analysis software UTide to estimate the tidal time series, we find that coastal water level has deviated from tidal predictions by more than ±600 mm in the past. The greatest deviations are caused by phase differences between the tidal time series and the tide gauge time series. Extreme exceedances are found to occur more frequently 4 to 6 hours before high tide at Tanjong Pagar and 4 to 7 hours before high tide at Johor Bahru, with frequency peaking at 5 hours before high tide at both locations. This shows that tides are arriving earlier than the predictions from harmonic analysis, but whether this is caused by tide-surge interactions warrants further study.


OS04-A006
Estimation of Tidal Energy Flux Change Related to the Tidal Flat Reclamation in the East China Seas

Byoung Jun LIM#+, You-Soon CHANG
Kongju National University, Korea, South

This study simulated tidal energy flux change in response to tidal flat reclamation of Jiangsu Shoalwater coast and Gyeonggi Bay in the East China Seas using MOHID (MOdelo HIDrodinâmico) ocean circulation model. Based on previous studies and historical coastal information maps, we carried out several numerical experiments with reliable coastal topography change around these two areas.
Results show the different tidal energy redistribution processes. The energy flux from Gyeonggi Bay disperses in the open sea, but most of it remains inside the Yellow Sea. This residual energy steadily increases the tidal amplitude in the Yellow Sea with the tidal flat disappearance. Most of the tidal energy flux from the Jiangsu Shoalwater coast was found to pass out of the East China Sea through the South Sea of Korea, which caused a sea level decrease in the East China Sea. This result indicates that coastal topography change in a specific area can cause sea level change in the surrounding area as a far-field effect through the tidal energy redistribution process and its modification.


OS04-A007
Sea Level Variability Along the Western Coast of India Simulated in a High-resolution Ocean General Circulation Model

Yoko YAMAGAMI#+, Tatsuo SUZUKI, Hiroaki TATEBE
Japan Agency for Marine-Earth Science and Technology, Japan

­Sea level variability along the coast of India is influenced by the coastal Kelvin wave. Wind forcing around the southern tip of India and east of Sri Lanka dominates seasonal variability (Suresh et al., 2016), while intraseasonal variability is mainly driven by equatorial forcing (Suresh et al., 2013). As sea level rise in the northern Indian Ocean is projected to be faster than the global average (IPCC AR6), the densely populated coastal areas will face serious risks from coastal storm surges and extreme tidal events in the future. However, most climate projections are based on climate models with a horizontal resolution in the ocean of about 1°. Therefore, it should be closely examined whether standard climate models can adequately represent coastal sea level variability due to coastal Kelvin waves. In this study, we examine the sea level variations in the northern Indian Ocean based on a comparison of non-eddying and eddy-resolving Ocean General Circulation Model (OGCM) experiments. We find that the eddy-resolving OGCM can better simulate the intraseasonal and seasonal sea level variability in the Indian Ocean. In particular, the eddy-resolving OGCM can reproduce intraseasonal extreme sea level events along the western coast of India that are underestimated by the non-eddying OGCM. The intraseasonal sea level variation is explained by a coastal Kelvin wave from the equatorial ocean in the eddy-resolving OGCM, which is consistent with previous studies based on a linear stratified model. However, the non-eddying OGCM does not simulate the propagation of coastal Kelvin waves in the Bay of Bengal due to its coarse resolution. This study implies that current climate models tend to underestimate the extreme sea level events and thus the future risks of sea level rise in the coastal region of India.


OS04-A008
The Evaluation of Sea Level Budget in the Northwestern Pacific Marginal Seas

Hyeonsoo CHA1#+, Jae-Hong MOON1, Taekyun KIM1, Yuhe Tony SONG2
1Jeju National University, Korea, South, 2Jet Propulsion Laboratory, California Institute of Technology, United States

Despite of recent advances in observation for underlying processes in the global mean sea-level rise (SLR), the process-based assessment on regional scales is challenging due to the physical processes having spatial and temporal variability. Understanding and quantifying these processes are important to projecting sea-level change and improving the basis for future vulnerability. In this study, we estimate the underlying process of the regional sea level rise on the northwestern Pacific marginal seas and assess whether the regional SLR budget can be closed with a combination of observation and ocean reanalysis datasets. The process-based budget assessment shows that the ocean mass change between deep ocean and shallow marginal seas, which are playing a role in driving regional SLR trend and its variability along the continental shelves. In this presentation, we will further discuss the sterodynamic estimation can be decomposed into two major processes (local steric sea level change and ocean mass redistribution) based on an observational approach.


OS04-A009
Sea-level Trends at Nine Southeast Asian Coastal Cities from 1993 to 2018

Trina NG1#+, Dhrubajyoti SAMANTA2, Julius OELSMANN3, Nidheesh GANGADHARAN4, Tanghua LI2, Aurel MOISE4, Benjamin HORTON2,5
1Centre for Climate Research Singapore/NTU, Singapore, 2Nanyang Technological University, Singapore, 3The Technical University of Munich, Germany, 4Centre for Climate Research Singapore, Singapore, 5Rutgers University, United States

Global mean sea level has been rising since the 19th century, but this rate of change is not uniform across the globe. Ocean dynamics, Gravity, Rotation and Deformation (GRD) effects of land ice and water mass distribution on the Earth’s surface, and vertical land motion are processes that influence relative sea-level rise on a local scale over varied temporal periods. For this reason, many low-lying Southeast Asian coastal cities are susceptible to relative sea-level rise. Here, we compiled all available tide gauge data within a 10km-radius of the coastal cities in Southeast Asia. The average number of years these tide gauges possess is 34 years, and majority (80%) have less than 50 years of data. Linear sea level trends from tide gauge and satellite data from 1993 to 2018 were shown and discussed for nine selected cities: Malacca, Penang, Singapore, Bangkok, Phuket, Prachuap Khiri Khan, Chumphon, Manila and Cebu City. The mean relative sea-level rise from tide gauge data across these cities was 4.16 ± 2.37 mm/yr (1993 – 2018). The contribution of GRD effects and ocean dynamics from internal variability to the sea level trends had an influence on regional sea level trends and spatial patterns over the last two decades. Vertical land motion due to anthropogenic activity and tectonics was conjectured to be the main driving process in cities such as Phuket and Manila. This study highlighted the non-uniformity of relative sea-level rise on a local scale and the importance of continuous long-term monitoring of sea level and vertical land motion in this region for more robust sea level projections.


OS04-A015
Spatiotemporal Analysis of Extreme Sea Levels Along the Korean Peninsula

Jung-A YANG#+
Korea University, Korea, South

Various countries around the world have been experiencing coastal disasters caused by coastal flooding, and Korean Peninsula is no exception. Most coastal flooding occurs during extreme sea level conditions which is comprised astronomical tides, nontidal residuals, wind wave, and mean sea level. To respond to coastal flooding disasters, it is important to understand the characteristics of extreme sea levels. Therefore, this study analyzed the spatiotemporal patterns of extreme sea levels along the Korean Peninsula and evaluated the effects of the astronomical tides and nontidal residuals represented by storm surges on extreme sea levels among the components constituting extreme sea levels. At this time, when analyzing the impact of the storm surge, it was evaluated whether the storm surge was caused by tropical cyclones or extra-tropical cyclones, and what storm condition were more dangerous in the Korean Peninsula. This study collected observed tidal data from 1979 to 2021 at 48 tide stations which are installed along the coast of the KP and performed a hormonic analysis to distinguish them into astronomical and storm surge components. In this case, storm surges occurring in summer and winter were considered to be caused by tropical cyclones and continental cyclones, respectively. In addition, to more accurately analyze the regional characteristics, the Korea’s coast was divided in the three zones: the East Sea, the West Sea, and the South Sea. As a result of the study, it was found that the extreme sea levels along the Korean Peninsula showed regional differences, and in the case of the south coast, storm surges generated by tropical cyclones were the main drive of extreme sea levels.


OS05-A002
Numerical Sensitivity Experiment on Seasonal Variation of Circulation in Jinhae and Masan Bays

Jiha KIM1#+, Byoung-Ju CHOI2, Ho Kyung HA3
1National Institute of Meteorological Sciences, Korea, South, 2Chonnam National University, Korea, South, 3Inha University, Korea, South

Jinhae and Masan Bays in Korea are semi-closed embayments that are affected by freshwater discharge from the Nakdong River. Although many oceanographic studies have been carried out in bays, research on seasonal and interannual variations of circulation is scarce. In this study, seasonal variation of hydrography and currents are examined using a three-dimensional ocean circulation model. Sensitivity experiments were conducted to investigate the effect of tides, winds and river discharges on regional ocean circulation.
The ocean circulation in Jinhae and Masan Bays was found to be characterized by two distinct patterns. In the western Jinhae Bay, the effects of tides and winds were dominant. Surface and bottom currents flowed toward the south and north, respectively, during the winter months. The tide mixing in winter lowered the density difference between the western Jinhae Bay and Gadeok channel in the southeast. The density difference between the surface and bottom layers was reduced due to wind mixing. The strong wind forcing in the surface layer caused the slope of the sea surface. During the summer, the density difference between the north and south increased, leading to the surface and bottom currents flowing toward the east and west, respectively, by geostrophic balance. Tidal mixing in summer lowered the density difference between the surface and bottom layers while, wind mixing, increased the thickness of the surface mixed layer.
The currents in the central Jinhae Bay and Masan Bay were significantly influenced by the wind in winter, and tides in summer. The river discharge was found to have a relatively large effect on ocean circulation in Masan Bay throughout the year. The currents in the surface and bottom layers of Masan Bay flowed to the open sea and the head of the estuary, respectively.


OS05-A005
Transient Response of Langmuir Turbulence to the Changing Forcings in a Diurnal Cycle

Wentao PAN#+, Qing LI
The Hong Kong University of Science and Technology (Guangzhou), China

Langmuir turbulence results from the interaction between ocean surface waves and background turbulence. It is an important physical process in the ocean surface boundary layer that affects the air-sea exchange of heat, momentum and gases. However, its evolution under transient forcing and interaction with changing stratification in a diurnal cycle are not well understood yet. This largely contributes to the existing biases when parameterizing its effects on turbulent mixing in ocean general circulation models and climate models. In this study, Langmuir turbulence with various diurnally varying wind, wave, and surface buoyancy fluxes is investigated using Large Eddy Simulation (LES). By directly resolving the turbulent structures of Langmuir turbulence with high spatial and temporal resolutions, we focus on the transient response of Langmuir turbulence to the changing ocean surface forcing and background conditions during a diurnal cycle. Here we present preliminary results of such LES experiments and discuss the implications for improving existing parameterizations of Langmuir turbulence.


OS05-A007
Latitudinal Shifts of the Intertropical Convergence Zone in the Eastern Equatorial Atlantic During the Last 513 Kyr

Leyla BASHIROVA1,2#+, Liubov KULESHOVA1
1Shirshov Institute of Oceanology of Russian Academy of Sciences, Russian Federation, 2Immanuel Kant Baltic Federal University, Russian Federation

Equatorial Atlantic is characterized by a complex of surface and subsurface currents – some of them flow westward, while others (countercurrents) direct eastward. Most of the year this region is influenced by the Intertropical Convergence Zone (ITCZ), a narrow belt of converging trade winds and strengthening of ascending air fluxes, resulting in an abundant precipitation. The latter leads to a decrease in surface water salinity and increased vertical stratification. Modern seasonal ITCZ migration is well known: over the central Atlantic ITCZ shifts between 6°N in boreal winter and 15°N in boreal summer (relative to the African coast), associated with regional rearrangements of atmospheric and surface ocean circulations due to changes in the meridional gradient of surface temperatures. Here, we present evidence of pronounced glacial-interglacial and millennial-scale variations in ITCZ position and related deep-water upwelling and surface biological productivity. We analyzed stable isotope, geochemical, and micropaleontological records from core ANS-33047 (08°16.38'N, 31°42.87'W, 4027 mbsl, 5.16 mbsf) retrieved from the southern part of the Cape Verde Basin east of the Mid-Atlantic Ridge. The modern annual ITCZ position over the core site allowed estimating the latitudinal displacements of the paleo-ITCZ during the last 513 kyr, based on RN/Gg proxy for mixed layer depth (Portilho-Ramos et al., 2017). This proxy was calculated using the ratio of three key species of planktic foraminifera. A southward displacement of the ITCZ has been suggested during mid-MIS 9, at the beginning of MIS 7, late MIS 5, and within MIS 3–2. Enhanced bioproductivity associated with northward ITCZ migration has been determined during MIS 13/12, early MIS 11,9,7, and MIS 1. Stronger deep-water upwelling and shoaling of the mixed layer over the study site preceded these intervals. The research was funded by the RSF (grant No.22-17-00170).


OS05-A008
High-resolution Sedimentary Record from the Gardar Drift: Surface and Deep-water Variability in the Subpolar North Atlantic During the Last 340 Yr

Liubov KULESHOVA1#+, Leyla BASHIROVA1,2, Evgenia DOROKHOVA3,2, Ekaterina NOVICHKOVA3
1Shirshov Institute of Oceanology of Russian Academy of Sciences, Russian Federation, 2Immanuel Kant Baltic Federal University, Russian Federation, 3Russian Academy of Sciences, Russian Federation

Changes in paleoceanographic conditions on the Gardar Drift are inferred over the last 340 yr from the high-resolution study of planktic (PF) and benthic foraminiferal (BF) assemblages, AMS14C dates, variations in stable isotopes (δ18O, δ13C), sortable silt mean grain size (SS), ice-rafted debris, and total organic carbon (TOC) content in multicore AMK-5687 (59°29.916'N, 24°40.001'W, 2530 mbsl). This time interval corresponds to the latter half of the Little Ice Age (LIA) and the Modern Period (MP). A mean sedimentation rate is ∼0.1 cm/yr. Average sea-surface temperatures (0-50 m) ranging from 8-9.2 °C (winter) to 10-11.5 °C (summer), with minima at ∼1725 AD followed the Maunder solar minimum. The subsequent warming apparently caused the melting of the sea ice in the northern latitudes and, as a consequence, the appearance of a cold freshwater "cap" in the upper ocean layer south of Iceland. A sharp increase in the abundance of the planktic subpolar species Turborotalita quinqueloba and a simultaneous decrease in the subsurface species Globorotalia inflata collectively indicate the Sub-Arctic Front (SAF) position east of the Reykjanes Ridge and the thermocline shoaling at the end of the LIA. North- and westward shift of the SAF as well as warm and salty surface water conditions were proposed for LIA–MP transition by reduced δ18O, an increase in G. inflata, and low abundance of T. quinqueloba. Simultaneously, an enhanced bottom-current intensity occurred according to high values of SS, and an increased carbonate corrosiveness existed leading the PF fragmentation and a significant decrease in δ13C values. A combination of BF diversity indices and TOC content allowed to reconstruct a relatively high surface bioproductivity and an organic carbon flux to the sediments during 1750-1790 and 1940-2010 AD. The study was supported by the RSF (grant No.22-17-00170).


OS05-A009
Estimating the Transport Timescale of Terrestrial Dissolved Substances in the Pearl River Estuary by Using Passive Tracers

Bo HONG#+
South China University of Technology, China

The Pearl River Delta is experiencing environment degradation resulting from the tremendous input of terrestrial dissolved substances (TeDS). The fate and transport timescales of TeDS in the Pearl River Estuary (PRE) was investigated to predict the pollutant transport coming from upstream. By using passive tracers in a calibrated 3D numerical model, the TeDS transport time was computed by using the concept of water age, which is a measure of the time that has elapsed since the tracer was transported from the upstream boundary to the downstream concerned area. The tracer impacted area was defined by the area with tracer concentrations > 0.2 (arbitrary unit). The domains that were impacted by the tracer coming from each outlet group were identified separately. In the wet season, the impacted area was larger than in other seasons. The most prominent variations appeared in the Jiaomen-Hengmen-Hongqili (JHH) and Modaomen (MD) outlets. The hydrodynamic conditions controlled the offshore spreading of the TeDS. Assuming the TeDS were conservative, it took approximately 10-20 days for the TeDS to be transported from the head water to the entrance of the outlet. For the TeDS coming from the head water of the Humen outlet, it took approximately 40 (80) days for the TeDS to be transported out of the mouth of the Lingding Bay during the wet (dry) season. For the MD, Jiti and Yamen–Hutiao outlets, it usually took approximately 10 days for the TeDS to be transported from the head water to the inner shelf. The correlation coefficient between the river flow and tracer concentrations was 0.78, and between the river flow and transport timescale it was −0.70 at a station in the lower Lingding Bay. Other forcing fields (i.e., wind and tide) have stronger impacts at the estuary mouth.


OS05-A013
Inversely Inferring the Diapycnal Diffusivity and Overturning Circulation with Ideal Ventilation Age

Boer ZHANG1#+, Marianna LINZ1, Andrew F. THOMPSON2
1Harvard University, United States, 2California Institute of Technology, United States

The ideal age (or ventilation age) is a commonly used bulk metric of the ocean circulation timescale, and is equivalent to a tracer that is transported by both advective and diffusive ocean motions. In this work, we propose a integrated version of the Munk balance for the ideal age tracer, or a water mass transformation analysis on it, where the sum of the advective and diffusive fluxes across an isopycnal surface equals the volume below it, corrected by an extra air-sea exchange flux if the surface outcrops. The theory is tested in a set of idealized single-basin simulations which mimic the Atlantic basin. With this integrated constraint on total diapycnal age flux, the effective diapycnal diffusivity at an isopycnal level can be inferred from the spatial distribution of the ventilation age near that level and prior knowledge of velocity field. Furthermore, a ratio between the effective diffusivity and the total diapycnal overturning circulation can be inferred by the age distribution, with proper separation of the upwelling and the downwelling region. Our theory provides conceptual clarification on the interpretation of the ideal age distribution, and we find that overturning strength is reflected by the difference of mean age between the upweling and downwelling zones, with the confounding effects of diapycnal diffusion and spatial correlation between age and diapycnal velocity, instead of the absolute value of ideal age itself. Our framework can be applied to realistic clock-like tracers (e.g. radiocarbon, Aragon, oxygen) to constrain the diapycnal diffusivity and overturning strength, which could be a particularly meaningful tool for paleoceanography.


OS05-A014
Multiscale Analysis of Typhoon-induced Oceanic Responses

Gang LI1#+, Yijun HE1, Yang YANG1, Guoqiang LIU2, Xiaojie LU1, William PERRIE2,3
1Nanjing University of Information Science & Technology, China, 2Bedford Institute of Oceanography, Canada, 3Fisheries and Oceans Canada, Canada

A localized multiscale energetics framework is used to study the multiscale interactions between near-inertial and mesoscale processes during the passage of Typhoon Kalmaegi in the South China Sea. The original HYCOM variable fields are decomposed into a low-frequency background flow window, a mid-frequency flow window and a high-frequency process window. Our results show that the background window represents mesoscale processes and Kuroshio currents well and the mid-frequency window captures near-inertial processes influenced by typhoon-induced wind stresses. The kinetic energy transfers from the near-inertial window to the background window, mainly on the right-hand side of the typhoon track. Advection redistributes energy, transporting kinetic energy downward from the ocean surface. Pressure work, which is stronger than advection processes, contributes to the accumulation of kinetic energy in the mid-frequency flow window and enhances ocean mixing. Negative vorticity has a significant impact on the distribution and downward propagation of the near-inertial energy, leading to heterogeneity in the mixing of the upper ocean. Negative vorticity and pressure work partially result in “leftward abnormal enhancement”, the magnitude of which is smaller than the increase in the near-inertial energy. We offer new insights into understanding the multiscale interactions between typhoons and the upper ocean.


OS06-A002
Deep Learning Application for Emulating Atmospheric Forcings in Storm Surge Modeling

Iyan MULIA1#+, Naonori UEDA2, Takemasa MIYOSHI3,4, Takumu IWAMOTO5, Mohammad HEIDARZADEH6
1RIKEN Cluster for Pioneering Research, Japan, 2RIKEN Center for Advanced Intelligence Project, Japan, 3RIKEN Center for Computational Science, Japan, 4University of Maryland, United States, 5Port and Airport Research Institute, Japan, 6University of Bath, United Kingdom

Due to their computational efficiency, parametric models are often used to simulate atmospheric forcings in typhoon-induced storm surge modeling. However, such models need better predictive skills in areas far from the typhoon center, during the extratropical transition, and landfall due to topographic effects. Numerical Weather Prediction (NWP) models are generally more accurate than parametric models, especially when incorporating a proper data assimilation scheme. Nonetheless, their accuracy should be compensated by the high computational cost. In this study, we aim to develop a method that can produce comparable accuracy to the NWP models yet with a minimum computational resource similar to that required for the parametric models. To that end, we propose using deep learning to emulate the atmospheric forcings for our storm surge model efficiently. In this study, a deep learning approach is implemented based on generative adversarial networks (GAN). The input is constructed from the widely adopted parametric model (Holland, 1980) using typhoon best track dataset, and the ground truth or target is based on the DSJRA-55 dataset having a spatial resolution of 5 km at a one-hour time interval. We utilize typhoon data passing through our study area around Japan from 1981-2012, considering 34 events for a training set and four for a test set. Furthermore, we design our GAN model to predict the wind and pressure fields of up to a 12-hour lead time using the current and previous four-hour states. The resulting forcing fields by GAN are then used for the storm surge model using a regional ocean model known as ROMS. The proposed method can achieve comparable storm surge model accuracy to the NWP-based forcings. Moreover, the transformation of parametric model outputs by GAN takes only approximately one second for a typhoon event using a standard computer.


OS06-A011
Analysis of Compound Floods from Storm Surge and Extreme Precipitation in China

Jianlong FENG#+
Tianjin University of Science and Technology, China

The variations and underlying drivers of the compound floods caused by storm surges and heavy precipitation are critical for flooding mitigation and risk reduction in China’s coastal cities. The variability of compound floods from storm surge and extreme precipitation from 1958 to 2014 was analyzed using daily maximum sea level data and daily cumulative precipitation at 16 tide gauges along the coast of China. More than 70% of the storm surges that caused damage from 1989 to 2014 at 14 out of 16 tide gauges were compound floods. We found a strong and seasonally varying dependence between the storm surges and extreme precipitation along the Chinese coast. These were generally positive trends in the annual number of compound events at tide gauges south of 35°N. Compound floods variability was related to large-scale climate modes. The Arctic Oscillation in March was significantly negatively correlated with the compound events at tide gauges north of 35°N, while the opposite was true at tide gauges south of 35°N. The compound events were significantly correlated with the Pacific Decadal Oscillation (PDO) in June at 10 out of 16 tide gauges, and negatively correlated with the Niño1+2 index in February at 7 out of 16 tide gauges. By modifying the East Asian summer monsoon and typhoons, the large climate modes are supposed to impact the occurrence of compound floods. Owing to the large population and low capacity of drainage systems in many cities along the coast of China, our study on the variations and underlying drivers of the compound floods serves as an important reference for flood risk management.


OS06-A020
Effects of Grain Size on the Movement of Submarine Landslides and the Generated Tsunamis

Xiafei GUAN1+, Huabin SHI2#
1University of Macau, China, 2University of Macau, Macau

Submarine landslide is one of the common marine geological hazards with massive sediment transport, large velocity and huge kinetic energy, which threatens seabed pipelines, cables and infrastructure along the propagation path. In addition, generated tsunamis may crush coastal cities with casualties and property losses. The movement of submarine landslides is affected by many physical properties, such as the composition and initial compaction of the slide and the topography. It is reported that the grain size of solid particles has a significant effect through the drag between the solid and the fluid phases. Besides, submerged slides composed of coarse and fine sediment behave differently in the shear dilation/contraction process. Accordingly, the deformation and movement of submarine landslides as well as the tsunami generation are notably affected by the grain size, especially in the initial stage. In this paper, a two-phase SPH model is utilized to study the effects of grain size on the initial acceleration of submarine landslides, a key factor of landslide-induced tsunami generation. The collapsing process of submerged granular landslides on a slope, the generated tsunami, the inter-phase drag force in the slide, and the inter-grain pressure in the cases of different grain sizes are compared. It is shown that the initial acceleration of submarine landslides with fine grains is smaller than that of the coarse-grain ones and consequently leads to a lower tsunami wave. The smaller grain size induces a larger inter-phase drag which hinders the initial movement of granular slides. However, the accelerating duration of submarine landslides with fine sediment is longer, which causes a greater translational velocity and momentum in the balance and deceleration stages.


OS06-A026
A Review of Historical and Paleo-tsunamigenic Earthquakes Along the Littoral Fault Zone in the Northern South China Sea

Linlin LI1#+, Qiang QIU2, Zhigang LI1
1Sun Yat-sen University, China, 2South China Sea Institute of Oceanology, Chinese Academy of Sciences, China

The Littoral Fault Zone (LFZ) was developed along the southeast coast of China in the northern continental shelf in the South China Sea. The 1000 km-long LFZ has high seismic activity, posing a great threat of seismic and tsunami hazard to the southern coast of China. Historically, the fault had generated many moderate to large earthquakes including 18 events with Mw >6 and 4 events with Mw >7 since 1600. Newly obtained geological records indicate strong earthquakes may have occurred in the segment previously assumed less seismogenic. However, little is known about the tsunami hazards associated with earthquakes from the LFZ. Here, we review the historical and paleo-earthquakes which either have documented tsunami phenomenon or have tsunamigenic potential. Based on the available geophysical data and historical documents, we briefly explain the seismogenic behaviors of the LFZ. And taking one of devastating earthquakes: the 1918 Nanao earthquake as an example, we demonstrate the key features of tsunami hydrodynamics and discuss how the earthquake focal mechanisms affect their tsunamigenic capacity. Our results suggest that the tsunami generated by earthquakes along the littoral fault possesses two unique features which may cause substantial damage in future: 1) the long tsunami duration (longer than 48 hours) due to shelf resonance and edge wave trapped in the very broad continental shelf of northern South China Sea; 2) strong tsunami currents induced by rapid change of sea level will pose significant threat to coastal infrastructures, e.g. ports, wharfs and aquaculture farms in southern China. Our sensitivity tests on earthquake parameters suggest that the tsunamigenic capacity is strongly affected by the source mechanism and fault geometries. Detailed marine geophysical surveys are required to better understand the geometrical characteristics and seismogenic behavior of the littoral fault.


OS06-A029
Marine Inundation History During the Last 3000 Years at a Coastal Lake on the Pacific Coast of Central Japan

Yumi SHIMADA1#+, Yuki SAWAI1, Dan MATSUMOTO1, Koichiro TANIGAWA1, Kazumi ITO1, Toru TAMURA1, Yuichi NAMEGAYA1, Masanobu SHISHIKURA1, Shigehiro FUJINO2
1National Institute of Advanced Industrial Science and Technology, Japan, 2University of Tsukuba, Japan

We found geological evidence of marine inundations during the last 3000 years at a coastal lake on the Pacific coast of central Japan. The lacustrine sediments consisted mainly of organic silt, and inundation events were identified from eighteen event deposits (E1–E18, from top to bottom) interbedded with the organic silt. Visual observation by the naked eye identified thirteen sand layers (E1–E3, E5, E8, and E11–E18), one gravel layer (E6), and one volcanic ash layer (E10) as event deposits. The other three event deposits (E4, E7, and E9) were detected only on computed tomography images as layers with higher density than the underlying and overlying organic silt layers. The spatial distribution of the event deposits in seaward areas, diatom assemblages, and frequency of inundation events suggested that thirteen (E1–E8, E11–E15) of the eighteen event deposits were formed by tsunamis or extraordinary storms. To constrain the depositional ages of the event deposits, a Bayesian age-depth model was constructed based on the radiocarbon ages of macrofossils and concentrated pollen grains and the cesium-137 profile. The age model allowed us to correlate five or possibly six event deposits with historical tsunamis along the Nankai Trough: E2, either of E3 or E4, E5, E7, and E8 corresponded to the 1707 CE Hoei, the 1605 CE Keicho, the 1498 CE Meio, the 1096 CE Eicho, and the 684 CE Hakuho tsunamis, respectively. E1 perhaps corresponded to the 1944 CE Showa-Tonankai tsunami.


OS06-A041
Detection and Warning of Sudden High Swells on the East Coast of the Korean Peninsula

Youjung OH1+, Il-Ju MOON1#, Sang Myeong OH2, Pilhun CHANG2
1Jeju National University, Korea, South, 2Korea Meteorological Administration, Korea, South

In recent several years, sudden high swell waves have often occurred on the east coast of the Korean Peninsula, especially in the winter season, which caused many casualties and property damage. These sudden swells have the characteristics of suddenly generating high waves even though the wind does not blow strongly, sweeping away unwary people on breakwaters or causing property damage such as ports and fish farms located on the coast. This study develops a detection and warning system for sudden high swells that frequently occur on the Korean Peninsula's east coast in winter. First, we developed a method to separate the wind and swell components based on the one-dimensional wave spectrum, wind speed, wind direction, and wave direction observed from coastal buoys. Using the calculated swell-wind wave height difference, significant wave height, and wind speed, we developed a sudden swell warning system in three stages (Warning, Watch, and Attention). Analysis reveals that this system successfully detected three recent swell-related accidents on the east coast. Further experiments by applying the system to the prediction results of the wave model showed that the method successfully issued a warning 24 hours before a sudden swell reached the east coast of the Korean peninsula. The developed system can provide quantitative and consistent forecast information, which will significantly contribute to preventing accidents caused by sudden high swells along the east coast of the Korean Peninsula. Acknowledgment: This research was supported by the Korea Meteorological Administration, National Institute of Meteorological Sciences, titled “Development of marine meteorology monitoring and next-generation ocean forecasting system (KMA2018-00420)”, and the National Research Foundation of Korea (NRF) grant funded by the Korea government (Ministry of Science and ICT) (No. RS-2022-00144325)


OS06-A047
Comparison of Coastal Inundation and Deposition Characteristics Accompanied with Tsunamis and Storm Waves Based on Numerical Simulations

Fating LI1+, Linlin LI1#, Kangyou HUANG1, Adam SWITZER2
1Sun Yat-sen University, China, 2Nanyang Technological University, Singapore

The South China Sea (SCS) region, frequently hit by typhoons and tropical cyclones from the northwest Pacific Ocean, is also at risk from multiple tsunami sources, including the Manila subduction zone (MSZ). Reconstructing the frequency and magnitude of past catastrophic wave events in the SCS is still a great challenge due to the difficulties of distinguishing tsunami deposits from storm deposits. Hainan Island in the northern part of SCS features numerous high sand barrier lagoons along the shoreline, which provide suitable environments to preserve overwash deposits, offering the potential for a better interpretation of long-term coastal hazard records. The Xincun Lagoon and Li’an Lagoon in the southeast of Hainan Island, both connected to the open sea through narrow inlets, contain reported sandy deposits. Here, we use numerical simulations to contrast the physical processes of inundation and sediment transportation in the lagoons produced by representative tsunami scenarios and extreme historical storm events at Hainan Island, China. Our preliminary results show that great earthquakes (~Mw9.0) from MSZ could produce large tsunami waves (~7 m) capable of inundating the lagoons and carrying plenty of sediment deposits. This study aims to identify the key source factors affecting the characteristics of tsunami deposits and storm deposits in this specific site. Such site-specific studies are essential for a deeper understanding of the overwash deposition process in the barrier-lagoon system, thus benefiting the subsequent tsunami and storm surge hazards preparation and mitigation in the SCS and worldwide.


OS06-A051
Coastal Tsunami Prediction in Tohoku Region, Japan, Using S-net Observations Based on Artificial Neural Network

Yuchen WANG1#+, Kentaro IMAI1, Keisuke ARIYOSHI1, Takuya MIYASHITA2, Narumi TAKAHASHI1
1Japan Agency for Marine-Earth Science and Technology, Japan, 2Kyoto University, Japan

After the 2011 Tohoku earthquake, Seafloor observation network for earthquakes and tsunamis along the Japan Trench (S-net) was installed offshore Japan. It provides observations for tsunami early warning. Coastal tsunami prediction using offshore tsunami observations contains two main types: tsunami inversion (e.g., tsunami Forecasting based on Inversion for initial sea-Surface Height; Tsushima et al., 2009) and tsunami data assimilation (Maeda et al., 2015). The first type must consider the initial source information, whereas the second type is affected by coseismic deformation. Recently, artificial neural network was introduced to real-time tsunami prediction (Mulia et al., 2020; 2022). We adopted a denoising autoencoder (DAE) model for coastal tsunami prediction. It is a neural network with the encoder-decoder structure trained to denoise or correct corrupted data (Goodfellow et al., 2016). We used 1,000 stochastic earthquake models (M7.0–8.8) in Tohoku region, Japan, and calculated synthetic tsunami waveforms at 50 S-net stations and two coastal stations. The DAE model was trained using 800 synthetic scenarios. Then, we tested the model against 200 unseen synthetic scenarios and two real tsunami events: the 2016 Fukushima earthquake and the 2022 Tonga volcanic eruption. S-net stations had real tsunami records of these two events. DAE model makes accurate prediction of coastal tsunami waveforms for synthetic events. The maximum amplitude was accurately predicted for the 2016 Fukushima tsunami with a forecast accuracy of over 90%. The entire waveforms were also fairly predicted. However, coastal waveforms were not satisfactorily predicted for the 2022 Tonga volcanic tsunami, likely due to its different generating mechanism (i.e., meteorological tsunami). Our research is the first study to apply artificial neutral network to coastal tsunami prediction using real offshore observations. In the future, we will use more tsunami scenarios for model training to make it robust for different types of tsunamis.


OS06-A052
Experiments on the Characteristics of Impact Forces of Bore Waves with Rectangular Drifting Objects

Kensei KUDO#+, Toshinori OGASAWARA
Iwate University, Japan

Tsunamis cause damage directly from wave force and secondary injury from drifting debris. Impact forces exerted by the floating objects on structures are necessary to be correctly evaluated. In this study, we conduct an experiment using a rectangular model to investigate the impact force exerted by drifting objects on a structure and clarify the effect of the impact angle on the impact force. Experimental conditions were set up by satisfying Froude's similarity rule, load cells were placed on the model structure, and impact forces were measured. The experimentally measured impact forces were compared with those obtained by the FEMA equation to verify the validity of the FEMA equation.
The results show that the FEMA equation for impact force is more excessive than the experimental values. As a factor in the overestimation, we focused on the impact angle when drifting objects collide with structures. The collision angles were calculated from the impacting images of drifting objects, and the cases were classified into plane and point impacts. The impact forces for the point are more significant than those for the plane, even when the generated bore waves are under the same conditions. Although the maximum velocities are similar in the drifting process, there is a difference in the decrease in velocities just before the impact. The forces were determined based on the accelerations obtained from the velocity slopes. The force was defined as the damping force. The impact force plus the damping force was considered the total force exerted by the bore wave on the drifting object. The damping force of the plane impact was greater than that of the point impact, indicating that the damping force may strongly influence the difference in impact force.


OS06-A053
Causes of Pressure Instability Problem in Explicit-MPS and Its Improvement Method

Yo OTOBE#+, Toshinori OGASAWARA
Iwate University, Japan

MPS (Moving Particles Simulation) is a typical particle method used for fluid and structural analysis. MPS methods include the semi-implicit algorithm, which solves for pressure implicitly, and the explicit algorithm, which solves for pressure explicitly. Previous studies have proposed methods to suppress pressure oscillations, mainly semi-implicit algorithms. A method to suppress pressure oscillations must also be developed for the explicit algorithm. This paper aims to investigate hydrostatic pressure as an important study for suppressing pressure oscillations and propose a method for suppressing them. One cause of pressure oscillations is that particles inside the fluid are misjudged as free surface particles, causing the pressure value to be calculated as zero even though it exists. Therefore, we examined the distribution characteristics of other particles within the radius of influence on the central particles. The results show that the center of gravity of other particles within the radius of influence of the fluid particle misjudged as a free surface particle is concentrated within 0.005 m of the central particle. Fluid particles were determined conditionally on the distance, and the pressure of misjudged fluid particles was corrected. Furthermore, it was found that there were many particles, even those determined to be fluid particles, that the pressure was more significant than the hydrostatic pressure. The pressure values for these fluid particles were taken as the average of the pressure values for the other particles within the radius of influence as the alternate values. The proposed method significantly reduced the number of misjudged particles and fluid particles with anomalous pressure values. It was possible to obtain pressure distributions that follow the hydrostatic pressure distribution.


OS06-A061
Influence of Urban Buildings on Tsunami Inundation Behavior Using Numerical Simulation

Keisuke HAGA+, Taro ARIKAWA#
Chuo University, Japan

The probability of a Mw.8-9 class Nankai Trough earthquake occurring in Japan within the next few decades is said to be over 80%, and the damage is expected to be enormous. Especially in urban areas, where people and buildings are more concentrated than in plain areas, the tsunami flow and its reach will differ significantly depending on buildings and houses, and the damage is likely to be extensive. Therefore, it is crucial to reproduce the topography of urban areas using numerical simulations to understand the hazards. Although there have been studies on inundation area and depth considering buildings, most of them have focused mainly on inundation depth and arrival time, and there have been few studies on detailed flow velocity and inundation area. In recent years, the improved performance of computers has made it possible to calculate tsunami inundation using high-resolution topography at 10 m or less. Therefore, in this study, numerical tsunami simulations for a Nankai Trough earthquake in an urban area were performed on a 2-meter high-resolution topography, taking buildings into account, and the changes in water level, flow velocity, inundation area, etc., were examined in detail. In addition, the random-phase tsunami model developed by Goda et al. was used to study many tsunami scenarios to cover the uncertainty of the earthquake magnitude. These results will suggest optimal evacuation routes and disaster prevention education for possible future tsunamis in the target area.


OS06-A062
A New O/U-tube to Generate Oscillatory Flows

Cheng-Hsien LEE#+, Jia-You CHEN
National Sun Yat-sen University, Taiwan

This study introduces a new coastal research facility, referred to as an O/U-tube due to its combinations of an O-tube and a U-tube. This new facility has a circulating, enclosed water tunnel and two vertical columns with open tops. The two vertical columns can avoid pressure surges. A valve is installed in the O/U-tube. The O/U-tube becomes a U-tube when the valve closed. Two impeller pumps are used to drive fluid. For steady flows, the force applied by the impellers on fluid is countered by the resistance force. Therefore, there exists a relationship between the rotation speed and flow velocity, which can be used to generate steady flows. For oscillatory flows, the gravity force and the inertia force also have effect on flows. Such relationship cannot be used to generate oscillatory flows. To generate target oscillatory flows, an open-loop control scheme is developed based on a numerical hydrodynamic model and a genetic algorithm. The scheme allows the O/U-tube to generate target oscillatory flows with given velocity skewness and asymmetry.


OS06-A064
A Numerical Simulation Study on the Influence of Flexible Vegetation on Coastal Profile Evolution Under Regular Waves

Yiran WANG#+, Sudong XU
Southeast University, China

Wetland vegetation can effectively resist waves and storm surge disasters, and has the characteristics of lower cost and sustainability, which leads to significant advantages compared with traditional coastal structures. Therefore, flexible vegetation is of important research value on coastal profile evolution. At present, most of the research on the influence mechanism of coastal vegetation has generalized the aquatic vegetation into a rigid cylinder, and little research has directly simulated the erosion and sedimentation effects of flexible vegetation on beach. This paper uses physical model experiments to explore the difference of erosion and sedimentation characteristics between the flexible vegetation beach(FVB) and non-vegetated beach. Then the numerical simulation model: XBeach was well verified by physical model data to simulate and study the erosion and sedimentation characteristics and differences between FVB and rigid vegetation beach(RVB). Physical model tests obtain profiles of non-vegetated beach and FVB under different water depths, wave heights, and periods. Results show that the erosion and sedimentation of FVB are generally smaller than that of non-vegetated beach and present a more near-shore distribution. Numerical simulation results show that the erosion and sedimentation extent of FVB is generally 3% to 14% greater than those of RVB, while the corresponding erosion and sedimentation sites of FVB are generally more offshore than those of RVB. With the increase of wave height, the positions of the first erosion/sedimentation points continue to move offshore. Meanwhile, the range and extent of significant coastal morphological deformation have increased respectively. Periodic tests follow the same results.


OS06-A065
The Research on the Interaction of Coastal Multi-branched Flexible Vegetation with Random Waves in Submerged Environment

Hui XU+, Sudong XU#
Southeast University, China

Storm surges and extreme wave disasters caused by tropical cyclones have caused great economic damage in coastal areas. Therefore, it is of great significance to find reasonable and feasible measures for shore protection to improve the capacity of marine disaster prevention and mitigation and increase the level of coastal ecological environment restoration and management. Compared to traditional coastal protection, nature-based coastal ecological protection has become a hot topic for research on viable solutions to marine hazards due to its ecologically sustainable nature. Coastal wetland flexible vegetation, as a new type of coastal disaster prevention and reduction method, is an significant section in coastal ecological restoration. Flexible vegetation such as reeds and mangroves grow in most of our coastal cities, all of which have a distinctive branching structure. The bending and oscillation of the branches interact with the random waves can reduce the wave energy and thus protect the embankment. However, due to the shading effect of the branching structure and complex dynamic characteristics, a simplified study is carried out here in order to quantify the movement of the flexible vegetation. Most previous work has simplified flexible vegetation to a uniaxial column, ignoring the shading effect of the branching structure of flexible vegetation on the main stem, thereby it is generalised to a uniaxial, multi-branched flexible vegetation model. Based on theoretical analysis and the selection of existing vegetation models, the research intends to carry out physical model experiments to analyze the action mechanism of flexible vegetation on random wave attenuation, and reveal the interaction between the flexible vegetation and random waves under submerged circumstance in a laboratory wave flume. The successful conduct of this experiment can reduce losses and promote the study of coastal ecological revetment for the sake of resisting marine hazards caused by tropical cyclones.


OS07-A001
Existence Periods of Salinity Front as a Feature of Fresh Water Plug During Northwest Monsoon in the Main Pathway of Indonesian Through Flow

Amirotul BAHIYAH1+, Iskhaq ISKANDAR1#, Muhammad Rizki NANDIKA2, Anindya WIRASATRIYA3, Wijaya MARDIANSYAH1
1Sriwijaya University, Indonesia, 2National Research and Innovation Agency, Indonesia, 3Faculty of Fisheries and Marine Science, Indonesia

Freshwater plug is a vigorous phenomenon that widely altered water mass characteristics of Indonesian throughflow (ITF), from Java Sea to Banda Sea. This phenomenon coupled with atmospheric circulation triggered Indo-Pacific climate change. This study investigates salinity front as a feature of freshwater plugs in the main pathway of ITF. However, rainfall on Borneo Island has a significant impact on anomalies’ energetics. Research analyses utilized the remote sensing approach, including atmosphere, ocean, and land analyses. This study's findings are the existence of salinity front and its energetics-long periods that are influenced by ENSO and IOD events. Moreover, a similar study has never been presented previously in Indonesian waters. The study area showed massive salinity front anomalies with the value reaching more than 1 PSU. Its elongated shape closes the main line of ITF and Java Sea pathway. Shorter existence periods (January to May) were discovered in 2015 and 2016 as the result of extreme El Niño 2015-2016 and low positive IOD 2015 events, whereas the anomalies along Jan-May 2019 and 2020 were influenced by moderate El Niño 2018-2019 and extreme positive IOD 2019 events. This condition was followed by a lower total of front less than 1 PSU/100. Longer periods occurred from January to June 2017 and 2018 attributed to moderate negative IOD 2016 and low La Niña 2018. However, more energetic anomalies were illustrated in 2017 than in 2018 due to heavier rainfall anomalies on Borneo Island with a difference of total front value around 0.6 PSU/100. Input sources of river discharge that are revealed from Borneo Island, are eastern (southern) of Borneo. Its drainage actively supplied river runoff during Jan-Jun (Apr-May). It can be concluded that salinity front anomalies are significantly influenced by river discharge from Borneo Island with its energetics determined by Indo-Pacific climate anomalies.


OS07-A003
How Well Do CMIP6 Models Simulate Salinity Barrier Layers in the North Indian Ocean?

Shanshan PANG1,2+, Xidong WANG3#, Jérôme VIALARD1
1Sorbonne University, France, 2Sorbonne University, France, 3Hohai University, China

Previous studies have hypothesized that climatologically thick salinity-stratified Barrier Layers (BL) in the North Indian Ocean (NIO) could influence upper ocean heat budget, sea surface temperature (SST) and monsoon. Here, we investigate the performance of state-of-the-art climate models from the Coupled Model Intercomparison Project phase 6 (CMIP6) in simulating the barrier layer thickness (BLT) in the NIO. CMIP6 models generally reproduce the main features of BLT seasonal cycle and spatial distribution, but with shallow November-February (NDJF) BLT biases in regions with thick observed BLT (eastern equatorial Indian Ocean [EEIO], Bay of Bengal [BoB] and southeastern Arabian Sea [SEAS]). CMIP6 models display an easterly equatorial zonal surface wind bias linked to dry rainfall and cold SST biases in the southern BoB, through the Bjerknes feedback. The easterly equatorial bias is also responsible for shallow isothermal layer depth (ILD) and BLT bias in the EEIO. The underestimated rainfall over the BoB leads to higher sea surface salinity (SSS) and too deep mixed layer depth (MLD), resulting in the BoB BLT bias. The intensity of the easterly equatorial bias also contributes to the inter-model spread in BoB BLT bias, through the propagation of EEIO ILD signals into the coastal waveguide. Finally, the SEAS BLT bias is due to a too-deep MLD, which is predominantly controlled by the high SSS related to attenuated monsoonal currents around India and a reduced inflow of BoB low-salinity water. BLs effect on the mixed layer entrainment cooling does not seem to operate in CMIP6 simulations. Rather, deep salinity-related MLD biases in the BoB result in a diminished cooling rate in response to winter negative surface heat fluxes, and hence alleviate cold BoB SST biases. This suggests that salinity effects alleviate the biases that develop through positive Bjerknes feedback between BoB SST, rainfall, and equatorial wind stresses in CMIP6.


OS07-A007
The Spatial Heterogeneity of Paleoenvironmental Conditions in Baltic Sea During the Late Holocene

Tatiana PUGACHEVA1,2#+, Ekaterina PONOMARENKO2
1Immanuel Kant Baltic Federal University, Russian Federation, 2Russian Academy of Sciences, Russian Federation

The Baltic Sea ecosystem is highly influenced by sporadic salt inflows from the North Sea, which are the main mechanism for water ventilation below the permanent halocline, especially in the central Baltic. Furthermore, the high anthropogenic load and climate variability strongly affect the Baltic Sea environment. The work presents the reconstruction of the paleoenvironmental conditions based on the complex analysis (micropaleontological, grain-size, XRF, and loss-on-ignition) of five short sediment cores retrieved from the Arcona, Bornholm, and Gdansk Basins. The reconstruction of past conditions is crucial for understanding the ecosystem’s natural variability and separating the latter from the reaction to ongoing climatic changes. The results reveal the difference in paleoenvironmental conditions of the studied basins as the response to the heterogeneous impact of the North Sea inflows and climatic fluctuations during the Late Holocene. According to the foraminiferal data, during the whole sediment accumulation period, the salinity of the bottom layer was higher in the Arcona and Bornholm Basins due to the vicinity of the inflow source (Danish Straits).The grain size composition of the cores indicates that the Arcona Basin and the Gdansk-Gotland Sill (Gdansk Basin) were characterized by the most hydrodynamic conditions in the near-bottom layer, which could be partly connected to the shallowness of these areas. Moreover, the Arcona Basin is the most proximal to the inflow source. Among the three basins, the Gdansk Basin was characterized by a higher content of organic matter in the sediments, which could be explained by the river runoff impact due to the proximity to the land, as well as by the repeating hypoxic conditions favoring the organic matter preservation in the sediments. The study was founded by Russian Science Foundation (grant №22-17-00170)


OS07-A009
The Presence of Barrier Layer in the Arctic

Hailong LIU1#+, Hualing WANG2
1Yunnan University, China, 2Shanghai Jiao Tong University, China

Barrier layer (BL) is an important representative variable reflecting salinity stratification. It is defined as the difference between mixed layer depth and isothermal layer depth (Lukas and Lindstrom 1991). Its existence not only weakens the warming effect of entrainment on the upper layer due to a roughly consistent lower temperature within BL than subsurface temperature above warm Atlantic water layer, but also limits the kinetic energy in the upper layer by salinity-induced stratification. Much attention has been paid to the role of halocline in the Arctic in the previous research. By using MOSAiC hydrographic observations and introducing multiple metrics, we focus on the evolution of barrier layer and associated mechanism in this present study. Our results show that BL demonstrates strong seasonal variation and potential role in modulating the interface interaction.


OS08-A005
Three-dimensional Oceanic Eddy Identification in the South China Sea Based on Machine Learning

Guangjun XU1,2#+, Wenhong XIE3, Xiayan LIN4, Yu LIU4, Changming DONG3,2
1Guangdong Ocean University, China, 2Southern Marine Science and Engineering Guangdong Laboratory, China, 3Nanjing University of Information Science & Technology, China, 4Zhejiang Ocean University, China

Oceanic mesoscale eddies play an important role in transports of heat, freshwater, mass in the ocean, therefore understanding three-dimensional structure of oceanic eddies is of significance to climate study and oceanic applications. However, detection of three-dimensional (3D) structures is a big challenge though many algorithms of sea surface 2D eddy detection are developed. In this study, a novel approach by using 3D U-Net residual architecture (3D-U-Res-Net) is proposed to identify 3D structure of oceanic eddies in the South China Sea. The sensitivity tests to input variables are conducted to optimalize the input setting. Trained by 3D eddy data provided by a kinetic eddy detection method, the AI-based method can identify different kinds of eddy vertical structures and moreover can dig out more eddy information in deeper layers. This study has significant implications for the further application of the AI-based algorithm in oceanic study.


OS08-A006
Wave Prediction Based on Improved Empirical Wavelet Transform Decomposition and Long Short-term Memory Network

Jin WANG1,2#+
1Southern Ocean Science and Engineering Guangdong Laboratory (Zhuhai), China, 2Nanjing University of Information Science & Technology, China

Ocean wave is one of the common ocean phenomena. Its formation and propagation are affected by many factors. Ocean waves are nonlinear and non-stationary. In order to improve the accuracy of wave forecast, we propose a wave prediction method base on improved empirical wavelet transform (EWT) decomposition and long short-term memory (LSTM) network. Firstly, as a time series, the significant wave height is used for Fourier transform to obtain the frequency spectrum. Then, according to the wave variation characteristics (yearly, monthly and daily), the segmentation interval of the wave spectrum is determined and divided. According to the divided spectrum, the wavelet filter is used to decompose the signal, so as to obtain the waves of different frequency bands. And then, LSTM method is used to predict the waves of different frequency bands obtained above. Finally, the prediction results of different frequency bands are superimposed to obtain the predicted significant wave height. In this paper, buoy in the North Pacific from National Data Buoy Center(https://www.ndbc.noaa.gov/) is taken as an example for modeling and prediction analysis. The results show that the method has high prediction accuracy. With the increase of forecast windows, the advantage of prediction accuracy is more obvious, which shows the important application values.


OS08-A007
Ocean Data Fusion for High Resolution Surface Current Maps

Evangelos MOSCHOS1,2#+, Hannah BULL2, Alisa KUGUSHEVA3,2, Alexandre STEGNER4
1École Polytechnique, Amphitrite, France, 2AMPHITRITE, France, 3ENS Paris-Saclay, France, 4Laboratoire de Météorologie Dynamique/ National Centre for Scientific Research, France

Ocean circulation is a complex process, making real-time reconstruction of surface currents a particularly challenging inverse problem. Currently, real-time maps of surface currents are produced using inhomogeneous measurements of Sea Surface Height (SSH) and strong spatiotemporal interpolation. However, these maps suffer from significant uncertainties, particularly in regions that are not sampled by altimetric satellites, and local current intensities tend to be underestimated as altimeter observations sample only the geostrophic component of the total velocity. To address these limitations, we propose a novel method that fuses SSH with Sea Surface Temperature (SST) observations to improve the accuracy of ocean circulation maps. In this study, we develop an end-to-end pipeline employing multi-modal input and an encoder-decoder neural network. An Observing System Simulation Experiment generates synthetic SSH and SST data by simulating altimetric along-track measurements as well as infrared sensor cloud coverage. Our data-generating process allows efficient sampling of the learning domain, while a simple data augmentation method is adopted to simulate cloud coverage. The model is thus robust to noisy and missing data due to clouds. Our results on synthetic satellite data demonstrate that this approach leads to improved reconstruction accuracy for both current intensity and direction, compared to the standard reconstruction methods. To validate our results on real data, we use in-situ measurements obtained from drifters. This allows us to compare the real-time nowcast of operational numerical models and our real-time reconstruction method, with improved characterization of ocean circulation at the mesoscale. The results of our experiments demonstrate the effectiveness of a data-driven approach for a real-time reconstruction of high-resolution ocean current maps.


OS08-A013
A Multi-mode Neural Network for the Long-term Ocean Wave Reanalysis

Jiawen LIAO1+, Yineng LI2#, Shiqiu PENG2, Shaotian LI2, Junmin LI2
1学生, China, 2Chinese Academy of Sciences, China

Long-term significant wave height reanalysis is crucial in the application of coastal engineering. The lack of observations and large biases of wind in the coastal region results in significant biases in the numerical model of ocean wave. In this work, we established single-mode and multi-mode correction models based on the Long-short term memory neural network (SCM_LSTM and MCM_LSTM) to revise the results of the numerical model using the in situ observations in 2020. Although the traditional single-mode correction model can efficiently revise low sea state characteristics, it is unsatisfactory in high sea state due to the imbalance of low sea state data and high sea state data. To solve this problem, the MCM_LSTM was built and separately studied the low and high sea state conditions. The correction results for 2021 show that the SCM_LSTM can significantly improve the RMSE and MAE of modeled results with a reduction of 50% and 62.1%, respectively. Compared to the SCM_LSTM, the MCM_LSTM’s RMSE decreases by 5.9%, and its correlation increases by 2.5%. The multi-mode correction model shows great superiority, especially in the case of the high sea state.


OS09-A001
North Pacific Gyre Oscillation and Reorganization During the Holocene with Deglaciation

Xufeng ZHENG1#+, Lixin WU2, Victoria PECK3, Xun GONG4, Hong YAN5, Xu ZHANG6, Martin FRANK7, Frank LAMY8, Li-Wei ZHENG1, Anchun LI5, Zhong CHEN5, Shiming WAN5, Wen YAN5, Yan DU5, Xiao MA9, Lisa BRETSCHNEIDER7, Xiaodong DING10, Lijuan LU5, Shuzhuang WU11, Shuh Ji KAO12
1Hainan University, China, 2Ocean University of China, China, 3British Antarctic Survey, United Kingdom, 4China University of Geosciences, China, 5Chinese Academy of Sciences, China, 6Helmholtz Centre for Polar and Marine Research, Germany, 7GEOMAR Helmholtz Centre for Ocean Research Kiel, Germany, 8Alfred-Wegener-Institut Helmholtz-Zentrum für Polar- und Meeresforschung, Germany, 9State Oceanic Administration, China, 10North Minzu University, China, 11University of Lausanne, China, 12Xiamen University, China

The North Pacific Subtropical Gyre (NPSG) vents enormous amounts of heat poleward, modulating the circum-Pacific and global climate1,2. However, orbital and millennial scales oscillations of the NPSG and its interactions with climate systems during current and past warming periods remain undetermined1,3-5, complicating accurate predictions of future ocean circulation and climatic changes. Here, using proxies of current strength and past sea surface temperature gradients, we find that the NPSG was markedly enhanced between 8 and 4 ka. Meanwhile, warming in the northwest and cooling in the northeast is manifested by intensified east-west mid-latitude North Pacific SST gradient, which is in phase with elevated temperature of > 2°C in intermediate waters. The intensified NPSG, potentially caused by strengthened Pacific trade winds, is associated with a climatology sea surface temperature pattern resembling the negative phase of Pacific decadal oscillation, which promotes basin-wide heat uptake in the North Pacific. In addition, the periodicity of NPSG variability shifted remarkably from ~1500 years to ~870 years at ~ 6 ka when the Laurentide ice sheet (LIS) melted away, implying that the presence of the LIS might have suppressed tropical forcing, and thus constitutes a critical tipping point of reorganization of the gyre dynamic over the North Pacific.


OS09-A004
Multi-platform Observation of the Atmosphere and Ocean in the Origin Region of the Kuroshio, East of the Philippines

Akira NAGANO#+, Iwao UEKI, Masaki KATSUMATA, Masahide WAKITA
Japan Agency for Marine-Earth Science and Technology, Japan

Sea surface temperature (SST) variation in the western tropical and subtropical North Pacific is related to atmosphere and ocean variations on various timescales from days to decades such as typhoons, El Niño-Southern Oscillation, and Pacific decadal oscillation. In addition to variations of sea surface forcing, the entrainment of deep water from the subsurface layers is responsible for the SST variation and also the sea surface salinity. Deploying a mooring buoy at 13˚N, 137˚E, named the Philippine Sea mooring observation (PHSMO) site, we initiated the observation in December 2016. As of now, we obtained temperature, salinity, dissolved oxygen concentration, and current velocity data down to a depth of 300 m for longer than 5 years at PHSMO site, and observed their interannual variations at the site. Further, we have conducted field campaigns around the site by the JAMSTEC R/V Mirai. Sea surface and near-surface water became cold and saline just before the occurrent of the 2018/2019 El Niño. Associated with this, the apparent oxygen utilization increased, so that deep old water might be upwelled in the east due to the precedent La Niña and advected to the site. Our observation contributes to monitor the upper-ocean conditions in the western North Pacific tropical and subtropical region and leads to the improvements of predictions of the regional and global climate changes and marine ecosystems, the main goals of the 2nd Cooperative Study of the Kuroshio and the Adjacent Regions (CSK-2) programme registered to the UN Decade of Ocean Science for Sustainable Development.


OS09-A006
A Stability Condition of a Topographically Constrained Geostrophic Current and Its Application to the Large Meander Path of the Kuroshio

Yuki TANAKA#+
Fukui Prefectural University, Japan

A general condition for the stability of a two-layer quasi-geostrophic flow constrained by bottom and coastal topography is derived and applied to the Kuroshio paths south of Japan. First, using a conserved quantity called pseudoenergy that is proportional to the square of the disturbance amplitude, we theoretically derive a sufficient condition for stability for the simplest steady background field in which the potential vorticity and the stream function are proportional to each other. The condition enables us to judge the stability of various background fields by explicitly taking into account the limitation imposed on the scale of the disturbance by the domain size. We then perform an idealized numerical simulation with a realistic situation in mind where the Kuroshio flows over Koshu Seamount and is confined within the Shikoku Basin (a basin bounded by Kyushu Island to the west and the Izu-Ogasawara Ridge to the east). It is shown that a flow similar to the straight path of the Kuroshio becomes unstable while passing over the seamount, developing into a flow similar to the large meander path of the Kuroshio. The application of the above-obtained stability condition shows that the stability of the two flow states can be successfully distinguished, suggesting that the Shikoku Basin stabilizes the large meander path of the Kuroshio while Koshu Seamount fixes the position of the crest and trough of the meander. This result may provide a reasonable explanation for the recently revealed path variability of the Kuroshio south of Japan.


OS09-A007
Change and Variability of Kuroshio Under Global Warming

Jo-Hsu HUANG+, Yu-Heng TSENG#, Yi-Chun KUO
National Taiwan University, Taiwan

Kuroshio plays a critical role on the ocean ecosystem, weather, and even climate in the Western North Pacific through its significant heat transport and air-sea interaction. The future change and dominant mechanism behind it under global warming remain unclear. Some previous studies suggested a negative midlatitude wind stress curl (WSC) tendency, potentially driven by El Niño or Arctic Oscillation, may accelerate the Kuroshio recirculation. The other studies found that the warmer subtropical mode water (STMW) might transport to the east of the Kuroshio along the isopycnals and enhance the upper-layer velocity around Ryukyu island under a warmer climate. Our analysis of the ensemble of 28 CMIP6 low-resolution models in the SSP5-8.5 future scenario shows that the kinetic energy (KE) tendency is positive to the north of 30N and negative to the south. To the south of 30N, the KE of Kuroshio increases in the upper 300m and decreases below 300m (i.e., baroclinic change). Compared with the result above, the ensemble of 5 eddy-permitting models shows that the Kuroshio recirculation north of 30N enhances more dramatically and the Kuroshio extension moves poleward, while the KE in the upper layer decreases in the south of 30N. This suggests the consistent baroclinic increase south of 30N is not evident in the eddy-permitting models. We also find that the meridional transport change negatively correlates well with the WSC change overall. Particularly, the meridional transport change north of 30N is more sensitive to the WSC in eddy-permitting models. Further future scenario ocean model sensitivity experiments suggest that the warmer SST dominates the upper 300m Kuroshio change to the south of 35N, but the WSC affects at depth (below 300m). The warmer isopycnal temperature transport clarifies the STMW pathway, increasing the Kuroshio’s baroclinicity.


OS09-A012
Impact of Kuroshio Meander on Pressure Changes in 2012 to 2013 Along Nankai Trough

Keisuke ARIYOSHI1#+, Akira NAGANO1, Takuya HASEGAWA1, Takeshi IINUMA1, Masaru NAKANO1, Demian SAFFER2, Hiroyuki MATSUMOTO1, Shuichiro YADA1, Eiichiro ARAKI1, Narumi TAKAHASHI1, Takane HORI1, Shuichi KODAIRA1
1Japan Agency for Marine-Earth Science and Technology, Japan, 2University of Texas, Austin, United States

Since DONET station covers above the source region of the 1944 Tonankai earthquake and its shallower extension, it has been also expected to monitor stress accumulation/release process around there from pressure gauges. Recently, it has been well known that slow slip event (SSE), which is one of slow earthquake family (Ide et al., 2007), repeatedly occurs in major subduction zones in shallower extension of the source regions of megathrust earthquakes as well as deeper one (Obara and Kato, 2019). For the shallower extension, SSE has been detected repeatedly from pore pressure extracted from the combination of pressure sensors in a borehole and on the seafloor close to DONET (Araki et al., 2017). For smaller magnitude of SSE about Mw5, its crustal deformation could not be detected from inland observation networks because of amount of displacement for long distance (Ariyoshi et al., 2021). On the other hand, seafloor pressure gauge contains atmospheric and oceanic fluctuations in addition to leveling change due to crustal deformation (e.g., Araki et al., 2017; Ariyoshi et al., 2021). In recent studies, there are several ways to extract the crustal deformation component from pressure gauges on the seafloor and in the boreholes. In this presentation, we reinvestigate the possible SSEs in 2012 and seafloor pressure change in 2013 from the view of crustal deformation on the basis of pore pressure in the borehole and oceanic fluctuation expected from an ocean modeling, JCOPE (Japan Coastal Ocean Predictability Experiment) (Miyazawa et al., 2004).


OS09-A015
Effects of Interannual Variations in the Kuroshio and Oyashio Fronts on Atmospheric Circulation and Storm Track

Xiang LI+, Guidi ZHOU#, Xuhua CHENG
Hohai University, China

Recent findings showed that midlatitude oceanic fronts in the Kuroshio-Oyashio Extension (KOE) region may significantly influence the overlying atmosphere on the interannual timescale. However, the exact mechanism and the combined effects of both the Kuroshio Extension Front (KEF) and the Oyashio Extension Front (OEF) are still largely unknown. Here we use front-resolving ERA5 reanalysis data to investigate the characteristics and mechanisms of the atmospheric response to interannual fluctuations of the KEF and OEF latitudinal position in a consistent way. It is found that the when the fronts meridionally migrate, response of the marine atmospheric boundary layer is remarkable. The response is mostly equivalent barotropic, with upper atmosphere intensification and sign reversal of temperature anomalies. Significant response of the storm track is also found. Diagnosis showed that eddy-mean flow feedback mediated by the storm track is responsible for the large-scale circulation changes, by means of both eddy heat flux and eddy vorticity flux. The spatial pattern of the KEF influence is a zonal dipole and the OEF is a monopole. The northward excursion of the KEF and OEF generally forces atmospheric responses with reverse sign. However, as the KEF and OEF moves in opposite directions with a lag time of 2.5 years, their atmospheric impacts sustains each other.


OS09-A018
Global Warming Effect on Oceanic Mesoscale Eddy Energetics

Junghee YUN1+, Kyung-Ja HA2#, Sun-Seon LEE3
1Yonsei University, Korea, South, 2Pusan National University, Korea, South, 3IBS Center for Climate Physics, Korea, South

Mesoscale eddies are of ubiquity in the ocean and play an essential role in transporting heat, salt, volume, and bio-geochemical properties on a global scale, which could modulate the interplay between the ocean and atmosphere and potentially affect the regional and global climate. However, it remains unclear how climate change will affect ocean eddies due to the lack of observational long-term records and model simulations with high spatiotemporal resolution. Here, we examine changes in ocean eddy activity due to global warming by employing an ultra-high-resolution climate simulation project, fully coupled global climate simulations using Community Earth System Model version 1.2.2 (CESM1.2.2) with different levels of greenhouse gas condition: Present-day run (PD, fixed CO2 concentration of 367 ppm), Doubling CO2 run (2xCO2, 734 ppm), Quadrupling CO2 run (4xCO2, 1468 ppm). We use the eddy kinetic energy (EKE), defined as the time-varying component of ocean kinetic energy, to measure the variability of mesoscale eddies. Model simulations show the inhomogeneous changes of the EKE under global warming conditions. To find the underlying processes, we focus on identifying changes in ocean circulation and stratification and their impacts on eddy energetics.


OS09-A021
Observed Subsurface Lens-like Features East of the Mindanao Island

Linlin ZHANG#+, Weiqi SONG, Dunxin HU
Chinese Academy of Sciences, China

Two subsurface anticyclonic lenses (Lens12 and Lens17) were observed with in-situ measurements along the 8 N transect east of the Philippines during the December 2012 and December 2017 cruises. The isopycnals above the lens center dome upward and those below depress downward. The horizontal scales of Lens12 and Lens17 are approximately 176 km and 210 km, centered at approximately 800 m and 1000 m, respectively, and their vertical extents exceed 1500 m. Mean swirl velocity of Lens17 measured by Lowered Acoustic Doppler Current Profilers is approximately 15 cm/s below 400 m and generally exhibits vertically coherent characteristics. The isopycnal undulations induced by lenses result in substantial temperature anomalies in depth. Temperature anomalies associated with Lens12 reach −3 °C and 1 °C at the depth range of 200–400 and 800–1500 m, respectively. On isopycnals, prominent positive temperature and salinity anomalies associated with Lens12 reach 0.5 °C and 0.1 psu near 26.82, implying that Lens12 carries alien warm and saline water. Combining the water mass properties of Lens12 and the mooring measurements, it is suggested that Lens12 originates from the east and travels westward with a phase speed of approximately 5.2 cm/s. Differing from Lens12, Lens17 shows no evident anomalous water mass properties on isopycnals. Mooring measurements imply that Lens17 probably originates from the south or southeast along the western boundary. By analyzing the outputs from an eddy-resolving ocean general circulation model (OGCM), this study further investigated the statistics of subsurface eddies east of the Philippines, including their geographic characteristics, and eddy-induced transport.


OS10-A014
A Persistent Marine Heatwave in the Northeast Pacific During 2021 Spring and Summer

Haocheng YANG#+
Ocean University of China, China

Marine heatwaves (MHWs)——extreme, prolonged, and dispersed weather events manifested by anomalous warming of seawater, have been found in the near two decades. A persistent marine heatwave has been found in the northeast pacific (NEP) region during the 2021 spring and summer. We used the heat budget to quantitatively analyze the oceanic and atmospheric processes inducing this NEP MHW. During May 2021, a decreasing latent heat loss, which was induced by decreased background westerlies, was the main reason for the onset of this NEP MHW. We can see that the atmospheric process played a crucial role during the occurrence of this MHW. In June, though the temperature tendency was negative, enhancing vertical mixing and entrainment maintained this MHW, while the net surface heat flux gave a negative contribution to the development. This situation was kept until August when the oceanic and atmospheric processes offset each other, causing the slight decay of the NEP MHW event. The atmospheric processes in erecting MHW and oceanic processes in maintaining the developing MHW are significant in spring and summer, which gives us the insight to predict MHW events in the NEP region.


OS10-A019
Role of Local and External Forcing on the Variability of Mixed Layer Depth Over the Bay of Bengal

Biplab SADHUKHAN#+, Arun CHAKRABORTY, Abhishek KUMAR
Indian Institute of Technology Kharagpur, India

To evaluate the climatic scenario of the Indian subcontinent, the study of Mixed Layer Depth (MLD) variability over the Bay of Bengal (BoB) is imperative, as it governs the climatic variability over this region. The BoB is a distinct region, with a large freshwater influx from numerous rivers and monsoon reversal winds in various seasons. The present study examines the role of local and external forcing on the seasonal, interannual, and decadal variability of MLD over the BoB. The analysis spans 36 years between 1980 and 2015 using reanalysis products. The wavelet analysis confirms that the MLD includes prominent interannual and decadal signals throughout the period. The seasonal variation demonstrates that the MLD over the BoB deepens during the summer and winter monsoons and shallows during the pre- and post-monsoons. The interannual variability of MLD is related to the different phases of the Indian Ocean Dipole (IOD), which shows that the positive (negative) phase of IOD is related to the shallower (deeper) MLD over the BoB. The variations in the second downwelling Kelvin and associated Rossby waves over BoB for the opposing phases of the IOD years substantially contribute to this. For a decadal timescale, the MLD over BoB is found to have more significant variance in the western bay and be comparably deep for regime-1 (1980–1998) and shallow for regime-2 (1999–2014). It is found that the decadal variability of BoB MLD is significantly modulated by local forcing like wind, wind-related processes, and Evaporation minus Precipitation (E-P). Moreover, there is a strong correlation between the Interdecadal Pacific Oscillation (IPO), which modulates the MLD of the coastal region of the BoB via propagating coastal Kelvin waves on a decadal timescale.


OS10-A026
Coupling of Alkenones SST and N-alkanes Records in Sediment from the North Atlantic ODP Site 980 During the Past 500 Kyr

Sangmin HYUN1#+, Yeonjee SUH2, Jeongwon KHANG1
1Korea Institute of Ocean Science and Technology, Korea, South, 2Global Oceon Research Center, Korea, South

Two typical biomarkers, alkenones and n-alkanes, from the drilling sediment of the ODP Site 980, North Atlantic sector were analyzed to reconstruct linkage and variabilities between SST and paleoclimate variation since the last 500 kyr. The variations of SSTs by alkenones ranged from 7.59 to 22.63oC with distinctive 100ka orbital cycle. Both the warmest and the coldest SSTs were observed during MIS 7, and MIS 8, and corresponding well to the SSTs from the result of previously measured benthic foraminiferal oxygen isotope. This implies that the alkenone SST and their fluctuation well reflected paleoceanographic and paleoclimate variations. The distribution patterns of n-alkanes were characterized by high odd number predominance, particularly nC27, nC29 and nC31, and by the variation of even number n-alkanes distribution. The drastic fluctuations in the abundance of total n-alkane abundance show 100ka cycle and their individual n-alkanes occurred in specific time can be explained by changes in plants habitat of source areas. Therefore, n-alkanes distribution suggests vegetation community changes, and thus paleoclimate changes of source areas. The variations of Average Chain Length (ACL) and Carbon Preferences Index (CPI) were coincident with n-alkanes distribution, reflecting that the vegetation community has been changed in response to global paleoclimate variations with glacial-interglacial time-scale. Strong coincident between alkenones based SST (cycle) and terrestrial total n-alkanes abundance (cycle) imply that the influx of terrestrial organic compound may be associated with paleoclimatology and local paleoceanography in North Atlantic area for the last 500 ka.


OS10-A027
Simulation of Drifting Trajectory of Garbage Discharged Into the Ocean from Rivers in Taiwan

Chung-Ru HO#+, Guan-Yu LIN, Wei-Chih LIN, Yu-Hao TSENG
National Taiwan Ocean University, Taiwan

Marine garbage has become one of the main sources of harm to the ocean. It is well known that a portion of marine garbage is discharged from rivers. In order to understand the drift of Taiwan's garbage after it flows into the ocean from rivers, this study uses the flow field and wind field data from satellite remotely-sensed data, and applies the Oceandrift model in the open source software OpenDrift to simulate the trajectories of garbage discharged from Taiwan's three major rivers on the ocean. These rivers are the Danshui River, the Gaoping River, and the Lanyang River. They are located in northwest, southwest, and northeast Taiwan, respectively. The simulation results show that if the influence of wind drag is not considered, the discharged garbage is mainly affected by ocean currents, especially the Kuroshio flowing through east of Taiwan. If the wind drag effect is considered at the same time, the direction of the Kuroshio and the northeast monsoon is opposite in winter, most of the garbage stays in the waters near Taiwan or even goes down to the Luzon Strait. Garbage with a high wind drag coefficient, it can even be flown to the South China Sea. When the southwest monsoon prevails in summer, under the action of wind drag and the Kuroshio, marine garbage is brought to the ocean around Japan. As for spring and autumn when the monsoon is relatively insignificant, the wind has less impact on marine garbage than ocean currents, so most marine garbage moves mainly with ocean currents, but at a relatively slow speed.


OS10-A030
A CFD Study on Suspended Sediment Transport Analysis at Connection Pier-bridge Between Busan New-Port and Nakdong River Estuary

Sung-Chul JANG#+, Han-sam YOON, Lee SANGHYUB
Pukyong National University, Korea, South

Busan New-Port has undergone large-scale port development, and many projects are currently being implemented or planned, and changes in the marine environment are continuously occurring. In particular, the deposition of suspended sediment causes burial in the harbor, continuously creating an area where the planned water depth is not secured on the front of the quay. These problems hinder the efficiency of port operation by causing unsecured navigation safety of using vessels. In this study, a numerical model simulation is performed to identify the sedimentation characteristics of suspended sediment generated inside the Busan New-Port. For the numerical analysis model, a discrete particle model was applied to the reproduction of suspended sediments, and various simulation cases were set and performed focusing on diffusion according to topographical characteristics.


OS10-A035
Using Shipboard Sonar Data to Identify Subseafloor Intrusive Rock

Pengcheng CHEN+, Shaoping LU#, Chen CAI
Sun Yat-sen University, China

Shipboard sonar is a marine acoustic device that uses a known and repeatable source signature to observe seafloor topography and bathymetry. The advantage of the technology is that it possesses the ability to offer a vertical shallow subseafloor resolution on a decimeter scale. Nowadays, the technology presents potential in exploration to provide direct evidence for identifying subseafloor events relating to sedimentary events, seafloor spreading, mass-transport deposits, and submarine landslides. It is usually used to interpret sedimentary stratigraphy information, but we found that intrusive rock signals could be captured in the sonar data. However, the signals are weak and blurry in comparison with horizons, by which it makes manual picking very difficult. In this research, we propose a novel workflow to identify the intrusive rock signals from the sonar data automatically. This workflow can be divided into three steps. In the first stage, we detect vibration events from the data. After that, the events are clustered based on density-based spatial clustering of applications with noise (DBSCAN) to find areas of increased energy concentration. Finally, the clustered results are combined with the data, the point cloud in the identified area is recovered into one or more lines, and the ones belonging to intrusive signals are determined. The effectiveness of the proposed approach on identifying intrusive signals is verified using survey data from the National Oceanic and Atmospheric Administration (NOAA).


OS10-A037
The South-north Equatorial Asymmetrical Distribution of Chlorophyll in El Niño Events in the Observations and CMIP6 Models

Lixia PAN+, Haigang ZHAN, Xin WANG#
Chinese Academy of Sciences, China

The interannual variability of chlorophyll (Chl) in the tropical Pacific Ocean is influenced by El Niño. When El Niño occurs, insufficient nutrients (suppressed upwelling), reduced shortwave radiation reaching the surface (increased precipitation), and eastward zonal current (U) anomalies, which transport low Chl from western Pacific warm pool water to the east, can cause a reduction in tropical Pacific Chl. The El Niño-induced Chl anomaly is asymmetrically distributed across the equator between 10°S and 10°N, and is particularly significant in extreme El Niño events. This asymmetric phenomenon is mainly caused by asymmetrical anomalies of the eastward U and precipitation. During El Niño events, U and precipitation anomalies are much stronger north of the equator, which can cause a greater reduction in Chl, which is asymmetrical. Models from the Coupled Model Intercomparison Project Phase 6 (CMIP6) are used to evaluate the simulation of the north-south asymmetry of Chl under extreme El Niño events. It finds that the simulation of U and precipitation anomalies is the key parameter to the simulation of this asymmetry. Among 15 CMIP6 models that provided Chl data, only 5 of them (MIROC-ES2 L, MPI-ESM1-2-HR, MPI-ESM1-2-LR, NorESM2-LM, and NorESM2-MM) can be used to investigate the asymmetrical distribution of Chl during extreme El Niño after comparison with observational Chl. Among the 5 selected models, only 2 (NorESM2-LM, NorESM2-MM) can show asymmetry during extreme El Niño events, and the other three models (MIROC-ES2 L, MPI-ESM1- (MIROC-ES2 L, MPI-ESM1-2-HR, MPI-ESM1-2-LR, NorESM2-LM, and NorESM2-MM) 2-HR, MPI-ESM1-2-LR) show symmetrical distributions. From the composite distribution of U and precipitation for these five models, it can be seen that the key reasons for whether a model can simulate the asymmetry lies in the simulation of U and precipitation.


OS10-A040
Geophysical Study on the Relationship Between Offshore and Onshore Faults in the South China Sea

Jun CHEN#+
Tongji University, China

The study on the fractures distribution of offshore and onshore faults and their relationship will help to reveal the history of the continental margin of the South China Sea, the Cenozoic geodynamic process of the western Pacific active continental margin. Through potential field separation and various derivative calculations of gravity and magnetic anomalies, combined with geological and geophysical data, the spatial distribution characteristics of faults in the South China Sea and its surrounding areas were obtained. Our results show that the northwest-trending fault extends from the South China continent to the northern slope of the South China Sea. And some of them even cross the South China Sea and enter Luzon Island. Most of the northeast-trending faults were cut and staggered by northwest-trending faults. The northwest-trending faults in Luzon Island extend into the South China Sea, but most of them become north—north—east or near east—west direction. The northwest-trending fault of the Indo-China block gradually deviates to the south in the process of extending to the southeast. The northeast-trending fault cuts the Yuedong fault and the Wanandong fault individually, but not much extension to the sea area. It shows that the Honghe fault, Yuedong fault and Wanandong fault formed the boundary between the Indo-Chinese block and the South China Sea. The fault systems on both sides are quite different. Most of the northwest-trending faults in Kalimantan region extended into the sea area and cut most of the northeast-trending faults in Nansha.


OS11-A001
Establishing a Risk Assessment Framework for Marine Assets and Assessing Typhoon Lekima Storm Surge for the Laizhou Bay Coastal Area of the Bohai Sea, China

Dongxue MO1#+, Jian LI2
1Institute of Oceanology, Chinese Academy of Sciences, China, 2State Oceanic Administration, China

Effective risk assessment can reduce the economic losses and physical damage caused by marine dynamic processes, such as storm surges. Most risk assessments of marine disasters are based on regional parameters and discrete hazard grades. Targeted, multi-level, and multi-angle risk assessments are urgently needed. This study focuses on specific types of affected infrastructure. We established a sensitivity matrix by considering the effects of different disaster causal factors on different types of affected infrastructure. Through this matrix, hazards, vulnerability, and emergency response and recovery capability were effectively combined in a risk assessment framework. We completed the risk calculation for multiple concurrent effects of disasters in areas with superimposed key infrastructure using complementary risk superposition. The hazard grade, vulnerability grade, and coefficient of emergency response and recovery capability were established based on the means of return period, characteristics of disaster distribution, types of affected infrastructure and disaster relief distance, and were continuous by solving functions, normal cumulative distributions, and analytic functions. On the basis of reasonable MIKE21 numerical simulation and abstract spatial distribution of vulnerable assets, we tested the rationality of the assessment system in the Lekima typhoon storm surge process. The results showed that the assessment system accurately reflected the risk of damage to the important infrastructure in terms of spatial distribution. Therefore, this risk assessment framework was suitable for the assessment of a marine dynamic disaster process in the lower Laizhou Bay coastal area of the Bohai Sea, China. Moreover, it provided a reference for disaster prevention and reduction, guided the way for decision making, and effectively reduced disaster losses.


OS11-A004
Spatiotemporal Variations and Controlling Mechanism of Low Oxygen in a Highly Urbanized Complex River System

Rui-Chen MA+, Jia-Tang HU#
Sun Yat-sen University, China

Numerous aquatic systems are prone to low-oxygen issues due to the anthropogenic impacts. Located in the Pearl River Basin and the upper reaches of the Pearl River Estuary, DongJiang River Network suffered from multiple pollution stressors and experienced prominent low-oxygen events despite effective control on local anthropogenic pollutant loads. A well-validated model was used to reconstruct its spatiotemporal distribution and dynamics processes of DO and to further explore the controlling factors and mechanism of low oxygen. As shown in simulations, DO exhibited significant spatial discrepancies and seasonal variations. The low oxygen was primarily happened in summer and early autumn, and a large-extent low oxygen frequently occurred in the lower region. As the DO budget revealed, photosynthetic production and the microbial oxidation of organic matter were the dominant factors controlling the source and sink terms of DO, respectively. Further scenario experiments indicated that oxygen depletion was dominated by the oxidation of organic carbon from external inputs and in-situ primary production, which contributed 67% and 36% on the low-oxygen volume, respectively. Moreover, phytoplankton played a significant role in DO source-sink processes (e.g., photosynthetic production, autotrophic respiration and heterogeneous respiration), serving as an oxygen source in the upper and middle regions, and as an oxygen sink in the lower region. Collectively, this study revealed the underlying causes of low-oxygen conditions under multi-stressors in a highly urbanized river system and provided a scientific basis for low-oxygen mitigation and management for similar areas.


OS11-A007
Construction of Tsunami Experience System to Improve Evacuation Awareness Using Photogrammetry with VR

Rena NAITO+, Taro ARIKAWA#
Chuo University, Japan

 On March 11, 2011, the tsunami following the Tohoku earthquake caused substantial damage. The people who did not evacuate despite the earthquake suffered from normalcy bias. Thus, it is necessary to educate the public to avoid normalcy bias by conducting evacuation drills on a regular basis and other means to prepare for disasters. In recent years, virtual reality (VR) technology has been used to educate the public on how to behave optimally in specific disaster situations, focusing on evacuation and disaster preparedness.
 Moreover, to experience a tsunami using VR, information on buildings and roads in the target city is necessary. In Japan, building and topographic data for 3D urban models have been established for urban areas––referred to as Project PLATEAU, which is led by the Ministry of Land, Infrastructure, Transport and Tourism––but not thus far for non-urban areas where tsunami damage is a concern. Therefore, in this paper, we propose creating a VR space that represents a cityscape by using photogrammetry, which creates a 3D model by photographing a subject from various angles. A 3D model was created for town A in Mie Prefecture, and the results and improvements are shown. Further, we propose guidelines regarding the photogrammetry method and how to create 3D models; it is expected that VR spaces can be easily created in any location in the future.
 By combining the results of inundation calculations with 3D models, the construction of a VR tsunami experience system will potentially improve evacuation awareness in a more realistic space. This would let the public experience a simulated tsunami experience, leading to early evacuation in the event of a disaster.


OS11-A011
Sedimentary Response to Human Activities in Daya Bay, China

Shuwei ZHANG+, Yunpeng LIN, Jingping XU#
Southern University of Science and Technology, China

Daya Bay, a small embayment in Guangdong province, China, is better known for a nuclear power plant nearby. Sediment from ten surface and five core samples collected in Daya Bay in the summer of 2022 were analyzed for grain-size, loss-on-ignition (LOI), and 210Pb dating, parameters that help investigating the environmental changes due to human activities or otherwise. Surface sediments from stations near the outlet of the power plant cooling water discharge are the largest in mean size and poorest in sorting. Three (D2, D13 and D16) of the five sediment cores can be divided into upper (0-23 cmbsf), middle (23-42 cmbsf) and lower (42-100 cmbsf) sections based on grain-size. The lower section displays a gentle upward fining trend, suggesting a stable sedimentary environment. Sediments in the middle section become much finer, indicating a significant change of sedimentary environment. The upper section has the smallest Mz and much weaker variation, implying a stable environment with weak hydrodynamic force. For D16, the core located in the center of the study area, the Mz clearly decrease upward, from 25.8 μm in the middle and lower to 12.4 μm in the upper section. Meanwhile, the LOI increase from 4.55% to 7.78%, indicating a significant increase of organic matter in the upper part of the core. 210Pb dating of D6 core results in a deposition rate of 0.5 cm·yr-1 in the study area. Thus the one-meter core contains sediment deposit of roughly 200 years assuming constant deposition rate. Applying this time frame to the five sediment cores shows that the 23 cmbsf and 42 cmbsf (two boundaries separating the three sections) correspond to 1980s and 1940s respectively. These to timelines happen to coincide with the intensification of human activities spurred by China’s Reform and Opening Up policy and the construction of the Daya Bay Waterway.


OS13-A003
Applications of Ensemble Coupled Data Assimilation in El Niño–southern Oscillation Prediction

Yanqiu GAO1#+, Youmin TANG2
1Second Institute of Oceanography, Ministry of Natural Resources, China, 2Hohai University, China

El Niño-Southern Oscillation (ENSO) is the most prominent short-term climate oscillation on Earth, which significantly influences the climate and weather anomalies in most regions globally. However, its practical forecast is still highly uncertain. In recent years, much research effort in climate prediction has been devoted to reduce initial and model error issues. In this work, ensemble based data assimilation approaches was employed to the Zebiak-Cane model to form an ensemble coupled assimilation–prediction system. Based on the ensemble system, by assimilating sea surface temperature (SST) and wind stress anomalies, we investigated the impacts of initial condition estimation, parameter estimation, and model tendency error (the comprehensive effect of different sources of errors) estimation on ENSO prediction in sequence. Results showed that, with the initial conditions estimation (i.e. state estimation only), the correlations of predicted Niño3.4 SST anomalies were improved remarkably and the root mean square errors were reduced compared with the values based on the original model. Further results indicated that model parameter estimation achieved better ENSO prediction skills than state estimation only. Model tendency error estimation effectively reduced model error effects in ENSO prediction. Aiming at the filter divergence problem raised by limited ensemble size, we proposed a new covariance inflation scheme to prevent the collapse of ensemble spread. The proposed scheme obtained the best parameter estimation and thereby ENSO prediction skill among the current inflation schemes. Overall, this work provides a promising approach to further improve prediction skill and a useful platform for real-time prediction.


OS13-A005
Research Progress of Ocean Temperature Data Quality Control System

Bin ZHANG#+, Huanping REN
Institute of Oceanology Chinese Academy of Sciences, China

Data quality is the prerequisite condition determining the correctness of the research. However, there’re still a lot of data quality problems existing in the international sharing marine data nowadays. Especially, it is hard to identify the non-conventional “artificial” data error by the traditional methods of quality control. Based on the previous quality controlling about the WOD09 data which is widely used in the world, it is found that among the data of 301740 stations randomly sampled from different geographical areas, data of 4351 stations is failed in error identification in total, accounting for 1.44% error information. The existence of such error information will great possibility affect the research findings. Targeting for such quality problems of international sharing data, we develop the global temperature and salinity data management system to collect and standardize data from diverse sources according to the independently designed ODSF1 data format, which helps optimize the traditional methods for data quality control and repeated data removal. Besides, for the data processed by artificial means (falsification data) and the “simulation” data of the quasi-repeated measurement station, we develop a whole set of “error information identify, analyze, and diagnose technologies”, thereby providing multiple types of data quality control analysis through the way of “expert-machine” combination. The construction of this system has effectively diagnosed and marked a great of data quality problems existing in the international marine data that is now under circulating, and has formed a data set which is more competitive in quality compared with the WOD data; established a set of quality control system for different sea areas, different months, different levels, different temperature and salinity observation parameters within the region from China offshore to Western Pacific, thereby consolidating a sound foundation for scientific researchers using the international sharing data.


OS13-A006
A New Quality Control Scheme for Marine Buoy Temperature and Salinity Data

Huanping REN#+
Institute of Oceanology Chinese Academy of Sciences, China

Based on the errors diversity of marine buoy observational data, this study presents a new quality control (QC) system for marine buoy temperature and salinity data. This QC scheme includes 6 checks with PauTa criterion as its core. The innovation of this scheme is that we present a new quality control algorithm that combines the traditional Spike check and PauTa criterion check. Its robustness has been verified by the seawater temperature and salinity data of buoy in the Yellow Sea and East China Sea. Many spurious measurements or outliers in long time series can be effectively identified. We further suggest this new scheme can be used in the quality control of buoy observation data in the future. Furthermore, we stress that the quality-controlled data could be used for marine scientific research, marine meteorological prediction, marine disaster forecast and fishery development.


OS13-A018
Estimation of Ocean Subsurface Thermal Structure in the South China Sea: An Ensemble-based Machine Learning Approach

Jifeng QI#+, Chuanyu LIU, Bowen XIE, Jianwei CHI
Chinese Academy of Sciences, China

Ocean interior information is vital for a better understanding of Earth's climate and oceans. This study presents a novel ensemble machine learning (Ens-ML) model for reconstructing the ocean subsurface thermal structure (OSTS) in the South China Sea (SCS) utilizing a combination of satellite-derived sea surface data and Argo data. The inputs to the model include sea surface height (SSH), sea surface temperature (SST), sea surface salinity (SSS), sea surface wind (SSW), and geographical information (including longitude and latitude). The performance of three machine learning algorithms (extreme gradient boosting, RandomForest, and light gradient boosting machine) is compared, and the advantages of combining their outputs via an artificial neural network technique are demonstrated. The results suggest that incorporating geographical information into the model significantly improves the accuracy of the OSTS estimate. The Ens-ML model was found to outperform individual models in terms of accuracy and precision. The model's performance varies seasonally, with the best results achieved in winter, likely due to weaker stratification. This study highlights the potential of multi-model ensemble machine learning algorithms for retrieving ocean interior information and provides evidence of their ability to produce more accurate results than individual models. The results of this research contribute to the advancement of oceanography and have implications for future studies on ocean and climate.


OS13-A028
The Mesoscale Eddy Hindcast Experiment for the South China Sea Based on 4DVar Method

Jun ZHAO+, Shan GAO#, Fan WANG
Chinese Academy of Sciences, China

Ocean mesoscale eddy is essentially a large scale motion satisfying quasi geostrophic equilibrium. Theoretically, its motion will be mainly constrained by the quasi geostrophic equilibrium relationship in a short time, while the influence of external forcing field will not change its motion characteristics significantly. Therefore, a prediction scheme of mesoscale eddy was proposed based on the initial field of four-dimensional variational assimilation. To test the feasibility of the scheme, a regional ocean model system (ROMS) and its built-in the primal formulation of incremental strong constraint 4-dimensional variational (I4D-Var) module were used to establish a marine assimilation simulation system for the South China Sea (SCS). First, AVISO altimeter data were assimilated into the ocean numerical simulation by the I4D-Var method, and the ideal mesoscale eddy assimilation simulation results were obtained. The statistical results of assimilation, model simulation, and observation show that the path, radius, sea surface height anomaly and amplitude of the mesoscale eddies simulated by the assimilation system are in good agreement with those observed by AVISO. Meanwhile, the depth analysis shows that the temperature, salinity, and density of eddies could be effectively adjusted. Secondly, the simulation results of the assimilation system were used as the initial field to simulate and quantitatively analyze the mesoscale eddies in the SCS in a certain period. By comparing the SSHA (sea surface height anomaly) correlation coefficient, eddy center distance, and radius absolute error of the corresponding eddies in the post prediction simulation and observation data, the post prediction time of mesoscale eddies in this scheme reached at least 10 days. The results of the post prediction experiments verified the feasibility of the proposed scheme, which provides a theoretical basis and a feasible scheme for the prediction of mesoscale eddies.


OS13-A042
Products of HY-1C/D Ocean Color Satellites

Jianqiang LIU, Xiaomin YE#+, Qingjun SONG, Bin ZOU
National Satellite Ocean Application Service, China

The HY-1C and HY-1D satellites are the first operational ocean color constellation in China. HY-1C and HY-1D was launched in September 7, 2018 and Jun 11, 2020, respectively. Chinese Ocean Color and Temperature Scanner (COCTS), Coastal Zone Imager (CZI), Ultra-Violet Imager(UVI), Satellite-based Calibration Spectrometer (SCS) and Automatic Identification System (AIS) are the key payloads onboard HY-1C and HY-1D. The HY-1C/D constellation has been detecting the global ocean color twice and sea surface temperature (SST) four times every day, and high- resolution (50m) China’s coastal zone and offshore environments twice every three days.In this study, the HY-1C/D satellites and the specifications of the payloads, flow-process, product levels and distribution of data products are introduced. The HY-1C/D satellites complete processing chains for generating raw data, radiances, ocean color and sea surface temperature (SST) from the payloads by Geo-location, radiometric and atmospheric correction, geophysical parameters retrieval, data gridding and merging. There are different data products associated with the five levels of processing (Level 0 to Level 4). Data products of Level-1 (radiances), 2 (ocean color parameters and SST), 3 (gridded products) and 4 (merged gridded products) are available from the China Ocean Satellite Data Service Center to the general public for free. The HY-1C/D satellites product structure system is complete and data product processing and distribution are efficient. The typical products of Chlorophyll-a concentration and SST, the applications on floating green tides algae Ulva prolifera, sea ice and polar ice, offshore aquaculture, inland water and tropical cyclones are also presented in this study. The typical products and application shown in this study indicates that the sensors and the data products of HY-1C/D have high quality and great application potential in marine and coastal environmental monitoring.


OS13-A043
A Sea Surface Temperature Retrieval Method of China Ocean Color and Temperature Scanner (COCTS)

Bin ZOU, Xiaomin YE#+, Qimao WANG, Qingjun SONG
National Satellite Ocean Application Service, China

The Chinese Haiyang-1C (HY-1C) and Haiyang-1D (HY-1D) satellites were launched in September 2018 and June 2020, respectively. These satellites are both equipped with the COCTS, a moderate-resolution imaging scanner with a nadir spatial resolution of 1.1 km and a viewing swath width of more than 2900 km. The satellite measures signals in 8 visible and near-infrared (VNIR) bands and 2 thermal infrared (TIR) bands (10.3~11.3μm,11.5~12.5μm). By using the non-linear algorithm for SST (NLSST) of split window, we retrieve SST from the two thermal infrared spectrum channels of 11 and 12 µm of COCTS. The Multiple Channel Sea Surface Temperature (MCSST) is used to be as the first guess of NLSST equation. The coefficients of both NLSST and MCSST are regression to ocean buoys and ship measurements. The retrieval SSTs from Jan. 1, 2019 to Mar. 31, 2020 were evaluated by the in situ measurements from iQuam with root mean square errors (RMSEs) of 0.84 °C for daytime and 0.97 °C for nighttime and robust standard deviations (RSDs) of 0.73 °C for daytime and 0.72 °C for nighttime, respectively. RMSEs of 0.65 °C and 0.71 °C and RSDs of 0.51 °C and 0.47 °C were obtained for the daytime and nighttime SSTs of the COCTS/HY-1D recorded from April 26 to August 31, 2021, using a spatiotemporal matching window of 4 hours and 2.5 km. Daily gridded retrieval SSTs from COCTS on both HY-1C and HY-1D were compared with SSTs from the moderate-resolution imaging spectroradiometer (MODIS) on Terra satellite and the visible infrared imaging radiometer (VIIRS) on the Suomi National Polar-orbiting Partnership (S-NPP) satellite. Both daytime and nighttime SSTs from COCTS are consistent with those from MODIS and VIIRS.


OS13-A045
Exploring Deep Ocean Bottom Using OBS and Impacts of Mass Blocks

Tianzhu LUO1+, Qingyu YOU1#, Lei ZHANG1, Jinhai ZHANG2
1Chinese Academy of Sciences, China, 2Institute of Geology and Geophysics, Chinese Academy of Sciences, China

Hadal trench—the deepest region of ocean, lying within oceanic trenches, is a promising place to uncover geological and geophysical mysteries of the deep ocean. China’s deep-sea submersible mother ship, Tansuo-1, deployed an ocean bottom seismometer (OBS) at the Hadal trench. This OBS recorded three events triggered by mass blocks (~400 kg for each), which can be regarded as vertical force sources. Here, we first utilized the grid search method to find the best-matching azimuth angle corresponding to the minimum energy ratio between the tangential and radial components. Then, we performed time-frequency analysis to present the time-frequency response of porous ocean bottom. Finally, we obtained the seismic wave velocities derived from body waves and surface waves. This research provides the first active detection using OBS and impacts from mass blocks with horizontal distance of <300 meters at the deep ocean bottom, which is helpful for future works on the investigation of seabed structure in hadal trench zones.


OS13-A047
Parameter Optimization and Observing System Evaluation Based on Data Assimilation to Improve Water Quality Monitoring and Prediction

Zhouxiao LIU+, Liuqian YU#
The Hong Kong University of Science and Technology (Guangzhou), China

Coastal waters have been increasingly degraded worldwide due to human disturbance and climate change. Quantitative knowledge of the status, underlying drivers, and future trend of coastal degradation is of paramount importance to designing scientifically-sound management strategies. Ocean biogeochemical models are a vital tool to serve the purpose, but their performance and predictive capability are often limited by the inaccurate description of ecosystem processes, uncertain parameters, and inadequate observations for validation and calibration, among others. This work aims to conduct parameter optimization to improve an ocean biogeochemical model and evaluate the observing system design through data assimilation, with the goal of informing water quality management. We will take Deep Bay, a shallow eutrophic system under intensified human perturbation in southern China, as a case study. The Bay has five long-time series stations monitoring water quality monthly since the 1990s. It also exists a 3D coupled physical-biogeochemical model that has been developed for a larger spatial scale beyond the Bay and thus has not been vigorously calibrated for the Bay area. Considering the computation costs for directly optimizing parameters and performing a large number of sensitivity tests in the 3D model, we alternatively build a 1D surrogate model that consists of multiple horizontal well-mixed boxes and is tuned to represent major biophysical features of Deep Bay. In the twin experiment framework, we evaluate the performance of parameter optimization by assimilating data from the existed monitoring system versus alternative observational sampling schemes. Through these analyses, we gain insight into where, how frequently, and what variables we should observe to maximize the benefit of data assimilation to improve model prediction and inform water quality management. We also explore to what extent the optimized parameter set from the 1D model can improve the 3D counterpart for providing spatially-explicit estimation and prediction.


OS13-A048
Observed Taylor Cap Around a Seamount Intensified by a Surface Mesoscale Eddy in the Northwest Pacific

Yansong LIU#+
Chinese Academy of Sciences, China

Observations from 4 current and pressure-recording inverted echo sounders (CPIESs) deployed in the northwest Pacific from 2018 to 2019 reveal an anticyclonic cap around a seamount. Significant increases in velocity can be found from mid-November 2018 to January 2019 and verified the coexistence with the “cold dome” combined with numerical model data. The Taylor cap induced by the impinging flow toward the seamount plays a primary role in the anticyclonic current structure
compared with tide rectification. The relationship between the impinging flow and surface mesoscale eddy in the northwest Pacific was further analyzed by combining the satellite altimeter data. When the surface cyclonic eddy moved to the center of the seamount in November 2018, the absolute sea level anomaly (SLA) increased, the temperature at the summit decreased, and the deep velocity impinging toward the seamount decreased and then intensified the Taylor cap around the seamount.


OS13-A052
Deviations of Satellite-measured Sea Surface Salinity Caused by Environmental Factors and Their Regional Dependence

Yating OUYANG1+, Yuhong ZHANG1#, Jianwei CHI1, Qiwei SUN2, Yan DU1
1Chinese Academy of Sciences, China, 2Southern Marine Science and Engineering Guangdong Laboratory (Guangzhou), China

Satellite measurements have largely improved sea surface salinity (SSS) observations in the recent decade, including Soil Moisture Ocean Salinity (SMOS), Aquarius/Satélite de Aplicaciones Científicas (SAC) –D, and Soil Moisture Active-Passive (SMAP). This study evaluates the deviations between the satellite SSS products and the in-situ observations (ΔS) and analyses their relationships with the environmental factors, including sea surface temperature (SST), precipitation, and wind speed. The level 3 satellite SSS generally correlates well with Argoobserved SSS but differs in the middle and high latitudes and the tropical convergence zones. The smallest ΔS appears in the subtropical open oceans, where the sea surface features warm SST, rare precipitation, and low wind speed. The variations in mean |ΔS| for the three satellites show a robust dependence on SST, precipitation, and wind, with large ΔS (outside 5%–95% interval) in particular tending to occur in areas of cold SST, heavy rainfall, and high wind speeds. The most pronounced SSS deviations occur in the middle and high latitudes (beyond 40°) due to cold SST. In particular, heavy rainfall in the subpolar regions and strong westerly winds in the mid-latitudes also make the satellite SSS measurements less accurate. In the tropical convergence zones, large SSS deviations are mainly related to heavy rainfall, showing significant surface freshening. The fresh biases related to rainfall are more significant in Level 2 SSS than in Level 3, due to the short period of the convective rainfall. In addition, surface freshening is more obvious in low wind speed scenarios, showing that the fresh skin layer induced by rain is more common on the calm ocean surface.


OS13-A053
Ocean Surface Wind Speed Inversion from the First Order Echo of HF Surface Wave Radar

Xiaoyan LI+, Xiongbin WU#, Liang YU, Fuqi MO
Wuhan University, China

The traditional methods of retrieving sea surface wind speed by high frequency(HF) surface wave radar are mainly based on the second order echo. However, due to the low signal-to-noise ratio and complex nonlinear effect of the second order echo, the detection range and accuracy of wind speed retrieved from radar are limited. Recently, some wind speed inversion approaches have been proposed based on the first order echo. But most of them utilize only a single operating frequency or a single radar station, thus the range of wind speed estimation from radar is usually limited for using restricted information of frequency and viewing angle. To address this issue, a wind speed inversion method based on the first order echo for a dual-frequency dual-station HF surface wave radar system is proposed. For each radar frequency, the spreading factor parameter which represents the growth state of wind waves, can be extracted from the ratios of positive and negative Bragg peaks of the two radar stations by using a cosine model as the angular distribution function. It has been inferred from in suit data that there is an ambiguity between the spreading factor of a fixed frequency and the wind speed. The problem is solved by using spreading factors of two frequencies retrieved from radar. The proposed wind speed inversion method is applied to an HF surface wave radar system operating at 7.94MHz and 12.365MHz and installed along the coast of the Taiwan Strait. In addition, a comparison between radar-derived, buoy-measured and ERA5 wind speed at the location 100km away from both radar stations is given to validate the proposed method.


OS13-A054
Spatiotemporal Variation of the Departure in Simulation from HF Radar Doppler Spectra Measurements

Fuqi MO+, Xiongbin WU#, Liang YU, Xiaoyan LI
Wuhan University, China

Directional ocean wave spectrum extraction from HF radar Doppler spectra has been a challenge with the limitations of second-order theories in high sea states. Whereas, the inversion of wind speed and direction for HF radar has been widely used to get relatively accurate results. These wind field information could be utilized to simulate corresponding radar backscatter spectrum with empirical ocean wave spectrum model by the first and second order theory. But, the departure of these simulated spectrum from radar Doppler spectra measurements is universal phenomenon during our field experiment in the Taiwan Strait with a complex topography. Due to the influence of wind field and geomorphic factors, the practical ocean wave spectrum is unable to described by existing empirical model. Although, the analysis of spatiotemporal variations in those departure could provide more details about the features of practical ocean wave spectra and then the interconnection between them. The field experiment carried out in Fujian Province collected a few months of data with dual radar system. Also, buoy and ERA5 data is prepared for verification. The comparison shows this analysis of the departure contributes to measure ocean dynamic parameters.


OS14-A006
Holocene Sea-level Evolution in Western Australia

Nicole KHAN1#+, Kayla MURAI1, Michael O'LEARY2, Erica ASHE3, Tanghua LI4, Abang NUGRAHA5, Rahul KUMAR4, Adam SWITZER4
1The University of Hong Kong, Hong Kong SAR, 2The University of Western Australia, Australia, 3Rutgers University, United States, 4Nanyang Technological University, Singapore, 5Earth Observatory of SIngapore, Nanyang Technological University, Singapore

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, 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 1) review, re-evaluate, and aggregate RSL data from Western Australia following international standard protocol and 2) explore the potential of sedimentary archives from beach ridge systems from southwest Western Australia to produce accurate, high-resolution records of Holocene 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 RSL during the Holocene will also provide new data for enhancing our understanding of earth rheology, ice sheet dynamics, and natural variability of sea-level changes under warm, interglacial climate states.


OS14-A009
The Utility of Vertical Zonation of Intertidal Microfossils and Stable Carbon Isotope and C/N Geochemistry for Sea-level Reconstruction in the Pearl River Delta

Howard Kwok Yin YU#+, Nicole KHAN
The University of Hong Kong, Hong Kong SAR

Determining the rates and mechanisms of relative sea level (RSL) change in the past can help enhance local projections of future RSL change, which is especially important in populated regions such as the Pearl River Delta (PRD), China. However, the late Holocene RSL history in this region is incomplete, and most of the data from existing reconstructions consist of limiting points that lack detailed bio- and chemo-stratigraphic analysis, which introduces uncertainty into the RSL record. Microfossils (foraminifera and diatoms) are used as RSL indicators because their community assemblages change across the elevation and environmental gradient in the intertidal zone. Moreover, stable carbon isotopes (δ13C) and the ratio of total organic carbon to total nitrogen (C/N) are able to identify the sources of organic matter that deposit in coastal sediments. To reduce potential bias in RSL reconstructions, a full understanding on the factors that control local modern microfossils distribution and δ13C and C/N geochemistry are required. Here, we investigate the utility of microfossils to generate a high-resolution (decadal to centennial age and ± 0.1 m vertical) late Holocene RSL reconstruction from sediments in Deep Bay, PRD. We describe the contemporary distribution of foraminifera, diatoms, and δ13C and C/N geochemistry from three transects that cover subtidal, intertidal (mudflat and mangrove) to upland environments. We examine the effect of elevation, total organic carbon content, and porewater salinity on the vertical distribution of microfossil groups using principal component analysis (PCA) and partitioning around medoids analysis (PAM). We develop a weighted averaging partial least squares regression (WA-PLS) transfer function from foraminifera and diatom assemblages and apply it to a core collected from mangrove in Mai Po, Deep Bay. Our approach could generate new late Holocene RSL records and improve our understanding of the rates and mechanisms of RSL change in the region.


OS14-A012
Foundations for Analysis and Machine Learning of Coral Microatoll Surface Features

Rohan GAUTAM1#+, Aron MELTZNER1, Khai Ken LEOH1, Nurul Syafiqah TAN2
1Nanyang Technological University, Singapore, 2Earth Observatory of Singapore, Singapore

Coral microatolls are coral colonies found in shallow reef environments. Their unique surface morphology of concentric rings is a result of relative sea-level (RSL) change and other environmental conditions that can affect the coral's growth over time. Invasive techniques involve physically extracting a slab of the coral microatoll to study the coral's annual growth bands to precisely determine RSL as the coral grew. However, such invasive techniques may not be viable at every site. Non-invasive techniques and methods of analysis are essential for large scale, cost-effective, and sustainable studies of coral microatolls. Examples of this technique include digital reconstructions of coral microatolls obtained via photogrammetry and LiDAR techniques. These digital models are further analyzed for tasks such as estimating growth variability across corals, detecting overgrowth and ring structures on the coral surface, and direct comparison of two coral surfaces. Conventional techniques for carrying out such analyses involve human intuition in key steps and are subject to significant human errors and biases. In our study, we work with digital reconstructions of corals to develop key foundations for analyzing and comparing different regions of the coral surface. We define a mathematical and computational notion of similarity between surface patches of varied sizes. We then develop the necessary data preprocessing pipelines and machine learning algorithms that use the initial formulation of the notion of similarity and apply it to analysis tasks. In doing so, we aim to support and formalize human intuition traditionally used for these tasks and significantly reduce human-induced errors, along with enabling more rigorous and larger-scale analysis of coral microatoll surfaces. 


OS14-A013
Using Non-invasive Techniques to Estimate Growth Variabilities of Living Coral Microatolls on St. John’s Island, Singapore

Khai Ken LEOH1#, Nurul Syafiqah TAN2, Lucas KOH1, Junki KOMORI1, Rohan GAUTAM1, Aron MELTZNER1+
1Nanyang Technological University, Singapore, 2Earth Observatory of Singapore, Singapore

Multi-decadal sea-level histories are crucial for quantifying processes that drive relative sea-level (RSL) change and for forecasting future RSL rise. However, tide gauge records maybe short, discontinuous or have poor spatial coverage. To overcome this, coral microatolls can be used to reconstruct RSL over decadal to centennial scales. Microatolls are coral colonies that grow in the intertidal zone, whose upward growth is limited by low-water levels. The exposed portions die, forming characteristic concentric rings that track RSL over the coral’s lifetime. The established method for reconstructing RSL from a microatoll involves extracting a radial slab, a cross section revealing the coral’s growth history. This may not always be viable, therefore inferences of the coral’s growth history are determined from its surface morphology. This is complicated by variable coral growth rates that form different surface morphologies on coeval microatolls. Overgrowth, out-of-sequence growth on the inner rings of a microatoll, is highly sensitive to growth rates. Both the growth rate and overgrowth must be considered for RSL reconstructions. In this study, we explore three-dimensional (3D) photogrammetry as a non-invasive technique to study the surface morphology of coral microatolls. Focusing on five living coral microatolls on St John’s Island, Singapore, we created digital elevation models (DEMs) using structure-from-motion (SfM) photogrammetry. We differentiated overgrowth regions and quantified the relative intra- and inter-coral growth variabilities based on distinctive features from multiple radial surface profiles. Next, we combined these results with literature values to estimate the true growth rates of each coral. In this session, we present two complementary techniques for RSL and coral microatoll research. Komori et al. introduces a simulator to model coral growth in response to RSL change. Gautam et al. uses an algorithm to quantify similarities in gradient changes across fixed coral transect lengths.


OS16-A008
Global Oceanic Diazotroph Database Version 2 and Elevated Estimate of Global Oceanic N2 Fixation

Yangchun XU+, Ya-Wei LUO#
Xiamen University, China

N2 fixation by marine diazotrophs is an important bioavailable N source to the global ocean. In 2012, the first version of the global oceanic diazotroph database (version 1) was published. Here, we present an updated version of the database (version 2), significantly increasing the number of in situ diazotrophic measurements from 13,565 to 55, 286. Data points for N2 fixation rates, diazotrophic cell abundance, and nifH gene copy abundance have increased by 184%, 86%, and 809%, respectively. Version 2 includes two new datasheets for the nifH gene copy abundance of non-cyanobacterial diazotrophs and cell-specific N2 fixation rates. Consequently, when estimating global oceanic N2 fixation rates using the geometric means of different ocean basins, version 1 and version 2 yield similar rates (43–57 versus 45–63 Tg N yr-1). In contrast, when using arithmetic means, version 2 suggests a significantly higher rate of 223±30 Tg N yr-1compared to version 1 (74±7 Tg N yr-1). Specifically, substantial rate increases are estimated for the South Pacific Ocean (88±23 versus 20±2 Tg N yr-1), and the North Atlantic Ocean (40±9 versus 10±2 Tg N yr-1). Moreover, version 2 estimates the N2 fixation rate in the Indian Ocean to be 35±14 Tg N yr-1, which could not be estimated using version 1 due to limited data availability. Furthermore, a comparison of N2 fixation rates obtained through different measurement methods at the same months, locations, and depths reveals that the conventional 15N2 bubble method yields lower rates in 69% cases compared to the new 15N2 dissolution method. This updated version of the database can facilitate future studies in marine ecology and biogeochemistry.


OS16-A009
N2 Fixation in Trichodesmium Does Not Require Spatial Segregation from Photosynthesis

Weicheng LUO1+, Keisuke INOMURA2, Han ZHANG3, Ya-Wei LUO1#
1Xiamen University, China, 2University of Rhode Island, United States, 3Shandong University, China

The dominant marine filamentous N2 fixer, Trichodesmium, conducts photosynthesis and N2 fixation during the daytime. Because N2 fixation is sensitive to O2, some previous studies suggested that spatial segregation of N2 fixation and photosynthesis is essential in Trichodesmium. However, this hypothesis conflicts with some observations where all the cells contain both photosystems and the N2-fixing enzyme nitrogenase. Here, we construct a systematic model simulating Trichodesmium metabolism, showing that the hypothetical spatial segregation is probably useless in increasing the Trichodesmium growth and N2 fixation, unless substances can efficiently transfer among cells with low loss to the environment. The model suggests that Trichodesmium accumulates fixed carbon in the morning and uses that in respiratory protection to reduce intracellular O2 during the mid-daytime, when photosynthesis is downregulated, allowing the occurrence of N2 fixation. Cell membrane barrier against O2 and alternative non-O2 evolving electron transfer also contribute to maintaining low intracellular O2. Our study provides a mechanism enabling N2 fixation despite the presence of photosynthesis across Trichodesmium.


OS16-A013
Impacts of River-discharged Freshwater on Surface Ocean Environments Revealed by Satellite Measurements

SoYoung KANG1+, Jae-Hong MOON1#, Taekyun KIM1, Chanhyung JEON2
1Jeju National University, Korea, South, 2Pusan National University, Korea, South

A Large amount of freshwater discharged from the Changjiang River supplies high concentrations of nutrient and organic matter into the East China Sea (ECS). The river-discharged freshwater plays an important role in physical and biochemical responses of ocean environment, which are also closely related to regional carbon cycle. In this study, we used satellite-derived datasets for sea surface temperature (SST), chlorophyll a(Chl-a), and sea surface salinity (SSS) to investigate the impacts of freshwater on surface ocean environments in the northern ECS over 2015–2022. The corrected SSS shows a distinct interannual variation, with a strong seasonal cycle in winter maximum and in summer minimum. By comparing with SST and chl-a anomalies, we found that the river-induced low-salinity water is closely linked to SST warming and high levels of chl-a concentration relative to their long-term means. In addition, relatively low partial pressure of carbon dioxide (pCO2) estimated appears in the northern ECS in 2016, which corresponds to the regions where in the SST warming and high levels of chl-a concentration are significant. These results suggest that warm and nutrient-rich freshwater at the surface may contribute to a reduction of surface pCO2 by prompting biological uptake of CO2.


OS16-A014
The Role of Mixotrophs in Lower Trophic Levels of Marine Food Webs

Mengting QIAN+, Ya-Wei LUO#
Xiamen University, China

Mixotrophy, the combination of autotrophy and heterotrophy in the same organism, is widespread among protist plankton. Mixotrophs range in size from pico- to megaplankton and vary in type. For a long time, most aquatic scientists thought that mixotrophs were not universal or of little significance, but as more mixotrophs were discovered, realizing their importance for energy budgets and elemental cycling in planktonic ecosystems was largely ignored. Mixotrophy alters the basic trophic structure of marine planktonic ecosystems, and most unicellular organisms in lower trophic level of plankton food web can no longer be considered strictly producers or consumers. Mixotrophy has a profound impact on marine planktonic ecosystems and may enhance primary production, biomass transfer to higher trophic levels, and the functioning of the biological carbon pump. But now the representation of mixotroph community is highly simplified, and further explicit inclusion of mixotrophs into biogeochemical models is necessary to improve our understanding of marine food webs and the global carbon cycle. So we built a plankton food web model incorporating mixotrophic functional diversity. We distinguish the size and type of mixotrophs, simulating how mixotrophs regulate plankton dynamics, primary production and carbon biomass transfer under different marine environmental conditions. Our study suggests that mixotrophic functional diversity can significantly alter our understanding of ecosystem dynamics within the lower trophic levels of marine food webs.


OS16-A016
Negative Surface Chlorophyll Concentration Anomalies in the Southeastern Arabian Sea During 2015 and 2019 Summers

Huaming HUANG#+
Sun Yat-sen University, China

Two extremely low surface chlorophyll concentration events in the southeast Arabian Sea (SEAS, 6oN-15oN, 72oE-77oE) during summers of 2015 and 2019 have been found since 1998. Although warm sea surface temperature (SST) and low nutrients are the direct cause for the anomalously low surface chlorophyll concentration, the physical processes leading to the warm SST anomalies during 2015 and 2019 summer are different. Satellite observations, model outputs and reanalysis data are used to explore the related mechanisms. In 2019, the combined effects of northward local wind anomaly due to extreme positive IOD and westward-propagating downwelling Kelvin wave driven by the easterly anomaly in eastern Sri Lanka weaken the upwelling in the SEAS, leading to warm SST anomaly and suppressing the upward transport of the subsurface nutrients to the surface. A weaker positive IOD occurred in 2015, leading to stronger upwelling in the SEAS than during 2019. Yet, seawater in the SEAS experienced extreme warming (lowest SST exceeded 28.5oC) due to the development of super El Niño in 2015. The significant seawater warming can shoal mixed layer and prevent the nutrients in the subsurface from reaching surface, which is unfavorable for the chlorophyll growth. The thermal balance analysis suggests that the extreme warming in the SEAS was mainly related to more downward shortwave radiation.


OS16-A021
Residual Overturning Circulation in the East/Japan Sea

Yujin KIM+, Hajoon SONG#
Yonsei University, Korea, South

An overturning circulation connects the surface ocean to the interior and is a critical component of the global climate system. The overturning circulation also exists in the East/Japan Sea (EJS), a marginal sea surrounded by Korea, Japan, and Russia, evidenced by a relatively high concentration of dissolved oxygen in the deep sea. However, there are not enough studies on overturning circulation. In particular, the residual circulation, which includes the role of eddies in addition to the wind-driven Eulerian circulation, has not yet been calculated in the EJS, even with its significant role in distributing heat, salt, freshwater, and other tracers. As a result, the contribution of eddies to the overturning circulation has not been discussed in the EJS yet. Here, we use a regional ocean model configured in the Northwest Pacific to compute the residual circulation in the EJS. In the annual average circulation, the clockwise circulation at 36-41°N appeared both in the Eulerian and residual circulation. The latitudes at which subsidence occurs during summer and winter were different. Eddy-driven circulation, the difference between residual and Eulerian circulation, intensified or weakened the circulation at 700m depth.


OS16-A022
Impact of Phytoplankton-induced Change in Mixed Layer Depth on Carbon Export Production in the Subpolar North Atlantic: A Modeling Assessment

Zhuowei XU+, Liuqian YU#, Qing LI
The Hong Kong University of Science and Technology (Guangzhou), China

Phytoplankton light absorption changes ocean optical properties, causing a vertical redistribution of heat that warms the ocean surface and cools the subsurface. The altered temperature distribution can modulate the mixed layer depth (MLD). Changes in MLD have long been recognized as a critical factor in governing the onset, duration, magnitude and variability of phytoplankton blooms, thus affecting carbon export production. However, the impact of phytoplankton-induced change in MLD on carbon export has been overlooked in most ocean biogeochemical models that do not account for the biological feedback to physics (e.g., phytoplankton light absorption). This work aims to assess how much phytoplankton light absorption modulates the seasonal cycle of MLD and to what extent these changes escalate to affect the timing, evolution, and magnitude of phytoplankton bloom and consequently the carbon export production. To achieve the goal, we set up a one-dimensional physical-biogeochemical model that explicitly resolves the bio-optical attenuation and its feedback on heat flux and ocean physics. The model is optimized to best reproduce the climatological annual cycles of phytoplankton biomass in the Subpolar North Atlantic, a region characterized by massive spring blooms. By conducting a series of model experiments with and without activating the feedback from biology to physics, we assess the impact of phytoplankton light absorption on upper ocean dynamics and carbon export production. Implications of this assessment for including such biological-physical feedback mechanisms in climate models will also be discussed.


OS16-A026
Assessment of the Impact of Ultraviolet Radiation on Global Marine Primary Productivity Observations

Weili CHEN#+, Ya-Wei LUO
Xiamen University, China

Oceans contribute nearly half of the global net primary productivity (NPP). Therefore, accurate assessment of its level plays a key role in understanding the global carbon cycle, climate change and ecosystem functions. It is found that ultraviolet radiation (UVR) has negative and positive effects on marine NPP. Nevertheless, the majority of culture flasks currently used have low transmittance to UVR, thus shielding the UVR effects on marine NPP. In our study, based on existing research, we use a multivariate generalized additive model (GAM) to analyze the UVR effects on marine NPP. The predictors are UVA (320-400 nm) and UVB (280-320 nm) irradiance, cell size obtained by mesh filtration, and primary productivity with UV shielding, and the response factors are the effects of UVR in UVA and UVB bands on NPP. The models are further applied to obtain corrected values. The results show that there is little difference between the global marine NPP estimations from satellite remote sensing and NPP values after UVR correction. Spatially, there are significant differences in the UVR effects: (1) in the vertical distribution, UVR significantly inhibits surface NPP, but at deeper depths, UVR (mainly UVA) promotes it; (2) in the horizontal distribution, mainly affected by cell size, UVR inhibits nearshore NPP but promotes it in the open ocean at low latitudes and mid-latitudes; and (3) in the latitudinal distribution, also mainly controlled by cell size, UVR inhibits NPP in the Northern Hemisphere but promotes it in the Southern Hemisphere. Overall, UVR may not significantly change the estimation of the global marine primary productivity total level, but its impact on NPP in different sea areas and water depths is quite different. This provides a certain reference value for further research.


OS16-A028
Influence of Power Plant Cooling Water Discharge on the Biogeochemical Processes in Daya Bay, China

Hanying CAO+, Yunpeng LIN, Fukang QI, Jingping XU#
Southern University of Science and Technology, China

Water samples collected at 25 stations in the summer of 2022 were analyzed for the lateral and vertical distribution of temperature, salinity, Chlorophyll-a, nutrients (including nitrates, ammonium, nitrites, and phosphates), particulate organic carbon and nitrogen (POC and PN), and carbon isotopic composition (δ13CPOC) within the water column of Daya Bay, a coastal embayment in Guangdong province, China. The mean nutrient concentrations are 4.6 μmol L-1 for dissolved inorganic nitrogen (DIN, include NH4+, NO2, and NO3) and 0.2 μmol L-1 for reactive phosphate (DIP, mainly H2PO4) respectively, and all increase toward the bottom. The nutrient ratio (DIN/DIP=23) was greater than the Redfield value (16:1), suggesting phosphorus limited in Daya Bay. The δ13CPOC and C/N ratio ranged from -23.84‰ to -18.95‰ and 3.95 to 6.91 respectively, suggesting a dominated marine source of POC. The cooling water discharge from the power plant increased the water temperature by 2-4°C and decreased the salinity by 2-4 PSU, compared to the surrounding water. Concentration of Chlorophyll-a, nitrate, and ammonium were found lower in the vicinity of the outlet of the cooling water discharge, probably resulting from degradation due to the high temperature inside the power plant. In contrast, the POC and PN concentrations at the outlet (0.9 and 0.17 mg L-1) were higher than those of the surrounding water (0.7 and 0.14 mg L-1). This is because (1) POC and PN concentrations are normally high near the surface (where the intake of cooling water is located), and (2) POC and PN are not as easily degradable as Chlorophyll-a or nutrients. Thus, even though the power plant’s cooling water discharge may have reduced the primary productivity, it may not have significantly changed the deposition and burial of organic matter in the area.


OS16-A029
Study of Cohesive and Non-cohesive Sediment on the Northern Bay of Bengal Shelf Using ROMS-CSTMS Climatological Simulation

Mohd IMARAN+, Arun CHAKRABORTY#, Subhasish TRIPATHY
Indian Institute of Technology Kharagpur, India

The Northern Bay of Bengal is one of the world's largest bays, receiving vast influxes of fresh water and sediment from India's monsoonal rivers at its head. We set up the integrated community sediment transport modelling system (CSTMS) within Regional Ocean Modelling System (ROMS) for our study domain in order to analyze the cohesive (silt) and Non cohesive (sand) sediments. The model was stabilized after one year of simulation, and as it nears the end of its full run, it gets even more stable. We have tested the model under two alternative scenarios: (1) with river and (2) without river simulation, to understand the sediment dynamics close to the coast. The Ganges-Brahmaputra, Mahanadi, and Irrawaddy Rivers revealed a very high vertically averaged silt and very low sand at their mouths while presence of river in simulation. Additionally, where the averaged silt concentration is very high, the bottom stress brought on by wave-current interaction is also strong. Furthermore, bottom stress is the primary cause of sediment migration near the coastal zone. Due to sand's faster settling velocity than silt, it has a larger bed fraction than the silt. Moreover, the averaged silt and sand are also noticeably less at the mouths of the Ganges-Brahmaputra, Mahanadi, and Irrawaddy rivers when the rivers are not included in the simulation. The primary factors in the coastal water of the Bay of Bengal sediment transport modelling are water quality and flow calculations on time scales of days to seasons. Finally, the model output is compared to the satellite that was observed, and the findings show a good agreement.


Fri-04 Aug | 8:15 - 10:00 | MR309
OS13 - Ocean Observations: Data Processing, Assimilation, Reconstruction and Application

Session Chair(s): Yuanlong LI, Chinese Academy of Sciences, Huizan WANG, National University of Defense Technology

OS13-A055 | Invited
International Framework for Quality Control and Management of Oceanographic Data and Information

Toru SUZUKI#+
Marine Information Research Center

The IODE of UNESCO/IOC is a programme to facilitate an international exchange and sharing of oceanographic data and information among IOC member states and has established since 1961. The IODE consists of the National Oceanographic Data Centers and Associate Data/Information Units which is established to promote to collect and discover the oceanographic data and information, and to encourage the long-time archive and provide them to scientists and experts. The World Ocean Database (WOD) is one of the IODE project initiated by NCEI/NOAA and is the most popular oceanographic database which is unified format and quality control is performed. The achievement of Global Oceanographic Data Archeology and Rescue which was also one of IODE projects to discover and increase the volume of historical oceanographic data are merged to WOD. The international projects such as WOCE and JGOFS also established data management group, and the data derived by those projects also merged to WOD and takes over to CLIVAR/CCHDO, CDIAC and so on. In addition, IQuOD, International Quality-controlled Ocean Database, is initiated to construct a climate-quality ocean temperature database using a consists and unified quality control standard. For ocean carbon parameters there are two global databases are updated: one is GLODAPv2 which is performed by secondary quality control procedures to WOCE/CLIVAR/GO-SHIP repeat hydrographic data, and the other is SOCAT, global sea surface mapping of ocean CO2 performed by expert quality control. The activities for developing oceanographic data and information under higher quality control would be support and useful for data analysis, assimilation and training of machine learning methods in order to progress of oceanography and multidisciplinary sciences.


OS13-A049 | Invited
The Reliable Sampling Interval for Monitoring Interannual Variability of the Kuroshio Transport at 18°N

Linlin ZHANG#+, Jing HUANG
Chinese Academy of Sciences

The sampling interval for reliably monitoring interannual variability of the Kuroshio transport was studied using satellite altimeter data and outputs from HYbrid Coordinate Ocean Model (HYCOM). Interannual variations of the Kuroshio velocity and transport crossing 18°N were derived with different sampling interval, and their deviations from the ‘true’ interannual signals derived from original time series were estimated. The results indicate that sampling with an interval shorter than 20 days is required to obtain the reliable interannual signals, i.e., the Root Mean Square of the deviation is <50% of the interannual signal. However, the longer sampling intervals will lead to serious aliasing and degradation of the true interannual signals, which is mainly attributed to the energetic intraseasonal oscillations in this region. Power spectrum analysis reveal that there are significant 80-day intraseasonal variations as well as semiannual fluctuations in the Kuroshio transport at 18°N, which brings substantial sampling deviations relative to the true interannual variation. An ideal experiment is constructed to confirm the reliable sampling interval around 20 days, which can resolve the intraseasonal oscillation and capture interannual variations of the Kuroshio at 18°N reliably. This study provides an important reference for the future monitoring of the interannual variation of the Kuroshio.


OS13-A019
Spatial Reconstruction of Long-term (2003-2020) Sea Surface pCO2 in the South China Sea Using a Machine Learning Based Regression Method Aided by Empirical Orthogonal Function Analysis

Zhixuan WANG1, Guizhi WANG1, Xianghui GUO1, Yan BAI2, Yi XU1, Minhan DAI1#+
1Xiamen University, 2State Oceanic Administration

The South China Sea (SCS) is the largest marginal sea of the North Pacific Ocean, where intensive field observations including mappings of sea-surface partial pressure of CO2 (pCO2) have been conducted over the last two decades. However, cruise-based sea surface pCO2 datasets are still temporally and spatially sparse. Using a machine learning-based method facilitated by empirical orthogonal function (EOF) analysis capable of constraining the spatiality, this study provides a reconstructed dataset of the monthly sea surface pCO2 in the SCS with a reasonably high spatial resolution (0.05º×0.05º) and temporal coverage between 2003 and 2020. The input data in our reconstructed model include remote sensing-derived sea surface salinity, sea surface temperature, and chlorophyll, the spatial pattern of pCO2 constrained by EOF, atmospheric pCO2, and time labels (month). We validated our reconstruction with three independent testing datasets that are not involved in the model training. Among them, Test 1 includes 10% of our in situ data, Test 2 contains four independent underway datasets corresponding to four seasons, and Test 3 is an in situ monthly dataset available from 2003–2019 at the South East Asia Time-Series (SEATs) station located in the SCS basin. These test runs validated our reconstructed pCO2 data are well in order with overall root-mean-square errors (RMSE) smaller than <10 µatm as compared to the in situ observations. Using the reconstructed dataset, we show the long-term trends of sea surface pCO2 in 5 sub-regions of the SCS with differing physico-biogeochemical characteristics. We show that mesoscale processes such as the Pearl River plume and China Coastal Currents significantly impact sea surface pCO2 in the SCS during different seasons. While the SCS is overall a weak source of atmospheric CO2, the northern SCS shelf acts as a sink with an increasing strength over the past two decades.


OS13-A011
An Update for IAP Ocean Heat Content Data and Implications for Earth's Energy Imbalance

Lijing CHENG#+
Institute of Atmospheric Physics, Chinese Academy of Sciences

Ocean observational gridded product is vital for monitoring ocean heat content (OHC) change and Earth’s energy imbalance (EEI). This presentation describes the new 4th version of the Institute of Atmospheric Physics (IAPv4) ocean objective analysis product accounting for recent advanced developments of quality-control (QC) procedure, climatology, bias correction (bottle, XBT, MBT, APB), vertical interpolation, mapping and uncertainty quantification methods. The new product is available for the upper 2000m since 1955 for monthly and 1°×1° resolution. The IAPv4 is compared with the previous generation of IAPv3 as well as to the other independent data including independent in situ data, sea surface temperature records and satellite observations. With improved techniques, the IAPv4 shows some new features of OHC changes, many of them are superior than the past IAPv3 data. The newly developed bias correction schemes for XBT, MBT and bottle data are mainly responsible for the difference of the 1955-2005 OHC trend in IAPv4 compared with IAPv3. QC plays a critical role for the 2005-2021 OHC trend. The month-to-month variability of OHC0-2000m for IAPv4 has been reduced than IAPv3 and smaller than other investigated data products, indicating more successful suppression of monthly noises. The annual variation of OHC0-2000m is compared with EEI observed by satellite at the top of atmosphere. With IAPv4, an updated sea level and earth’s energy budget are derived and discussed in this presentation.


OS13-A012
Estimating Subsurface Thermohaline Structure Rapidly from Satellite Data: A Deep Network with Embedded Empirical Orthogonal Functions

Hengqian YAN#+, Ren ZHANG, Huizan WANG, Senliang BAO
National University of Defense Technology

Estimating subsurface thermohaline structure from concurrent satellite data is a meaningful way to enrich internal oceanic observations. As a powerful tool for data mining, many studies have used machine learning in subsurface reconstruction, but most conventional applications have been purely black-box in nature without further consideration of oceanic characteristics. Instead, proposed here for the first time is a semi-explicit deep network for reconstructing the oceanic interior from surface data. Named EEFFNN, the method embeds empirical orthogonal functions extracted from reanalysis data (the EE part of the name) into the inner framework of a feed-forward neural network (the FFNN part of the name). Comparison with Argo profiles and reanalysis data shows that EEFFNN can significantly outperform conventional machine-learning algorithms in estimating subsurface thermohaline structures and especially subsurface-intensified eddies. Also, EEFFNN can perform thermohaline reconstruction in one pass, making it more lightweight than "shallow" machine-learning algorithms such as random forest. Overall, EEFFNN shows promise for being applied to operational thermohaline reconstruction in the near future.


OS13-A027
Global Ocean Reanalysis CORA2 and Its Inter-comparison with a Set of Other Reanalysis Products

Hongli FU#+
National Marine Data and Information Service

We present version 2 of the China Ocean ReAnalysis (CORA2) in this paper. We compare CORA2 with its predecessor CORA1, and with other ocean reanalysis products (GLORYS12v1, HYCOM, GREP, SODA3, and ECCO4) during 2004-2019, to show its improvement and reliability. In addition to providing tide and sea ice signals, the accuracy and eddy kinetic energy of CORA2 are also improved due to enhanced resolution to 9 km and updated data assimilation scheme, when compared with CORA1. Error analysis shows that the root-mean-square error (RMSE) of CORA2 sea-surface temperature remains around 0.3°C, which is comparable to that of GREP and smaller than those of the other products. The subsurface temperature (salinity) RMSE of CORA2 at 0.87°C (0.15 psu) is comparable to that of SODA3, smaller than that of ECCO4 and larger than those of GLORYS12, HYCOM and GREP. CORA2 and GLORYS12v1 can better represent sub-monthly-scale variabilities of subsurface temperature and salinity compared with the other products. Although the correlation coefficient of sea-level anomaly (SLA) in CORA2 does not exceed 0.8 in the whole region as GREP and GLORYS12v1 do, it is better than ECCO4 and SODA3 in the Indian Ocean and Pacific Ocean. CORA2 can reproduce the variations of steric sea level and ocean heat content on the multiple timescales as the other products. The linear tread of steric sea level of CORA2 is closer to that of GREP compared with the other products; and the long-time warming trends of global OHC in the high-resolution CORA2 and GLORYS12 are larger than those in the low-resolution EN4 and GREP. Although CORA2 shows slightly poor performance in the Atlantic Ocean, it becomes good from 2009 onward. We plan to further improve CORA2 by assimilating available best observation data, using the incremental analysis update procedure and improving SLA assimilation method.


Fri-04 Aug | 8:15 - 10:00 | MR310
OS04 - Understanding Multiscale Sea-level Change Using Observations and Models: Global to Local

Session Chair(s): Xuebin ZHANG, Commonwealth Scientific and Industrial Research Organisation, Oceans and Atmosphere, Dhrubajyoti SAMANTA, Nanyang Technological University, Trina NG, Centre for Climate Research Singapore/NTU

OS04-A005
What Forcing Mechanisms Affect the Co-variability of Interannual Sea Level Variations Between the Northeast and Southeast Coasts of the United States?

Ou WANG1, Tong LEE1#+, Thomas FREDERIKSE2, Rui M. PONTE3
1Jet Propulsion Laboratory, California Institute of Technology, 2University of California Los Angeles, 3Atmospheric and Environmental Research, Inc.

Interannual sea level variations between the Northeast and Southeast Coasts of the United States (U.S.) separated by Cape Hatteras are significantly less correlated than those within the respective sectors. We investigate forcing mechanisms affecting the co-variability of interannual sea-level variations at Nantucket and Charleston, as two representative locations for the U.S. Northeast and Southeast Coasts, by using an adjoint sensitivity analysis of sea-level reconstruction and decomposition in the framework of Estimating the Circulation and Climate of the Ocean (ECCO) ocean state estimate. This method is more rigorous than correlation-based methods to determine causal mechanisms for a quantity of interest (interannual sea-level variations here) by wind stress and buoyancy forcing from different regions. Onshore wind stress north of Cape Hatteras and buoyancy forcing, especially that from the subpolar North Atlantic, both cause interannual sea-level variations to co-vary between Nantucket and Charleston. Offshore wind stress contributes much more to interannual sea-level variation at Charleston than to that at Nantucket and has larger contribution than onshore wind stress for Charleston. Offshore wind stress is the major factor causing incoherent interannual sea-level variations between Nantucket and Charleston. Buoyancy forcing south of Charleston, including the Florida shelf, the Gulf of Mexico, and the Caribbean Sea, can have noticeable contribution to Charleston sea-level variations, but not to Nantucket. But such buoyancy forcing contribution is much smaller than that of offshore wind stress in causing the incoherence of interannual sea-level variations between the Northeast and Southeast Coasts of the United States.


OS04-A017
Local Sea-level Projections for Coastal Adaptation and Decision-making in Southeast Asia

Jennifer WEEKS1#+, Benjamin HORTON2,3, Benjamin HARRISON1, Matthew PALMER1, Trina NG4
1Met Office, 2Nanyang Technological University, 3Rutgers University, 4Centre for Climate Research Singapore/NTU

Understanding decadal-to-centennial future sea levels across Southeast Asia is important due to the region’s densely populated and low-lying coastlines. Relative sea level change in Southeast Asia is complicated by tectonic activity and/or intensive groundwater extraction leading to Vertical Land Movement (VLM). National assessments of sea-level change in Southeast Asia have typically provided regional-to-local likely range (i.e. characterising the central two-thirds of the distribution) sea-level projections for the 21st century. Here, we present continuous sea-level projections for locations across Southeast Asia generated using two approaches: (1) Palmer et al., (Earth’s Future, 2020), where projections are rooted in Coupled Model Intercomparison Project Phase 5 (CMIP5) models and in methods used in the Intergovernmental Panel on Climate Change (IPCC) Fifth Assessment Report (AR5), with an emulator-based methodology to provide extended projections to 2300; and (2) IPCC Sixth Assessment Report (AR6) (available to 2150), where projections are rooted in CMIP6 models and constrained to an assessed climate sensitivity. Comparisons between the two approaches reveal the projections are broadly consistent, but the representation of the sterodynamic and VLM components in studies can lead to significant differences at a given location (e.g. ~30cm at Sembawang, Singapore). Alongside scientific advancements in generating process-based sea-level projections, there has been an increasing need to improve the utility of projections in coastal adaptation planning and decision-making. We apply a framework developed by Palmer et al., (in prep) to generate physically consistent high-end storylines for locations in Southeast Asia. These storylines use recently published projections of Antarctic ice sheet mass loss and span the full uncertainty space of AR6 GMSL rise. This allows for a pragmatic approach to high-end sea-level rise where risk tolerances and decisions made in Southeast Asia may vary considerably over the coming centuries.


OS04-A001
Fusion of Model-based and Expert-based Projections of Sea Level

Benjamin GRANDEY#+, Lock Yue CHEW
Nanyang Technological University

Model-based and expert-based projections of mass loss from ice sheets differ substantially. This drives ambiguity in probabilistic projections of sea-level change. To combine the complementary strengths of the model-based and expert-based projections, we propose a fusion. Our fusion of different projections caters to diverse stakeholders by providing a single probability distribution that provides useful information in both the centre and the tails of the distribution.


OS04-A013
Does Mean Sea Level Trend Mask Historical Storm Surge Trend: Evidence from Tropical Cyclones Affecting Japan Since 1980

Md Rezuanul ISLAM#+, Le DUC, Yohei SAWADA, Masaki SATOH
The University of Tokyo

Variability in storminess, storm surge, and mean sea level (MSL) can substantially alter coastal hazards associated with extreme sea levels (ESL). However, the detection and attribution of past changes in tropical cyclone (TC) and associated storm surges are hampered by inhomogeneous TC records. Here we investigate spatiotemporal changes in storm surge levels in Japan from 1980–2019, a period when observational platforms including tide gauges and storm records are highly consistent. We find statistical evidence of the increase of surge annual maxima in several places including the bay area of Tokyo since 1980. This rate of change is comparable to that observed for MSL rise over the same period. These findings doubt the current hypothesis on the flood adaptation plan in which future surge extremes will remain the same and MSL changes are only considered. We demonstrate that the changes in ESL in the last 40 years cannot be explained by the rise of MSL alone, rather, the northeastward shifting of TC landfall location as well as intensifying and widening of TC might have altered the likelihood of ESL including surge extremes. The substantial influence of these TC meteorological variables on surge levels coupled with the rise of MSL suggests that current coastal planning practices including critical heights for flood defenses might be inadequate in the future.


OS04-A002
Changing Tides Alleviating Nuisance Flood Around Lingding Bay, China

Xiaoya LUO#+
CCCC-FHDI Engineering Co., Ltd.

Nuisance flooding, also known as minor flooding, is a low-level flooding event that is non-destructive but has a chronic and significant impact on coastal cities. Over time, the socio-economic losses caused by frequent nuisance floods have been found to be greater than those caused by rare extreme floods in some areas. As such, based on observed tidal levels from 1960s to 2010s, we analyze the trends of nuisance flood duration and frequency at seven stations around Lingding Bay, China. Our results show that both the flood duration and frequency have increased at all stations, with a highly correlative relationship between flooding acceleration and sea level acceleration. This indicates that sea level rise could be accelerating nuisance flooding. However, changing tides may play a counteracting role in Lingding Bay. Through the use of the UTide harmonic analysis package, we have reconstructed historic tidal levels in Hong Kong based on the first 18-years' data. The result reveals that compared to modern nuisance floods, the reconstructed flood duration is longer and grows faster, due to a decrease in tidal range in Hong Kong in recent decades, which offsets the influence of sea level rise to some degree.


Fri-04 Aug | 10:20 - 12:20 | MR309
OS13 - Ocean Observations: Data Processing, Assimilation, Reconstruction and Application

Session Chair(s): Yuanlong LI, Chinese Academy of Sciences

OS13-A046
A Smart Unmanned System for Ocean Environment Monitoring

Guangcun SHAN1,2#+, Zejian DING3, Xin LI3, Shunping ZHAO4
1Beihang University & City University of Hong Kong, 2City University of Hong Kong, 3Beihang University, 4Radiation Environmental Monitoring Technology Center of the Ministry of Environmental Protection

Based on ResNet50 Deep Network Model and the radionuclide enrichment and detection device, a new smart unmanned system is studied and designed for the marine environment monitoring. The unmanned system is equipped with an embedded neural network computing unit for attitude estimation, a motion control unit and a nuclide enrichment detection device. The nuclide enrichment detection device implements rapid enrichment and in-situ detection of radionuclides by adsorption nanoporous composite materials and γ-ray detector. Taking a camera-captured picture directly as input, the modified ResNet50 Network Model implements a six-degree-of-freedom pose estimation of the current position via using two sub-networks with shared partial parameters, which archives position and angle estimation errors of 1.23m and 5.07°, and 1.68m and 4.25° on DeepLoc dataset and King's College dataset, respectively. Our results demonstrate that the developed unmanned system in this work can achieve a very high precision navigation, which is vital for versatile ocean observations as a smart unmanned ocean environment monitoring tool.


OS13-A010
Coupled Parameter Estimation for Oceanic Vertical Mixing in the Community Earth System Model and Its Impact on the Initialization of ENSO Prediction

Zheqi SHEN#+, Youmin TANG, Yihao CHEN
Hohai University

Parameter estimation (PE) is the process that adjusts or optimizes the model parameters using observations. It can constrain the uncertainty of parameterization schemes that induce model errors. Coupled parameter estimation has shown the potential to improve coupled model reanalysis and prediction. However, performing PE in coupled general circulation models (CGCMs) with real observations is still a challenge. In this study, a data assimilation system using the fully coupled Community Earth System Model (CESM) is used to assimilate multiple ocean observations to initialize the prediction of ENSO. It assimilates gridded satellite SST data and the subsurface temperature and salinity (T/S) profiles not only to provide the initial states of the coupled model but also to estimate some critical parameters in oceanic vertical mixing parameterization. Furthermore, the analysis fields and parameters are used as initial conditions to perform ensemble predictions of ENSO. The comparison between PE experiment results and those from a state estimation experiment which uses the default parameters, reveals that PE can improve the analysis quality and increase the ENSO prediction skills of the CESM.


OS13-A025
A Vortex-implanted Initialization Scheme for the Mesoscale Eddy Prediction: Idealized Experiments

Yuhang ZHU+, Yineng LI, Shiqiu PENG#
Chinese Academy of Sciences

Mesoscale eddy prediction has been a big challenge to oceanographers and marine environment forecasters. Although the traditional initialization for the prediction, i.e., through assimilating the satellite-derived sea level anomalies (SLA) into a model, has some improvement, it is yet unable to predict well the main characteristics of a mesoscale eddy, including its three-dimensional (3D) structure, moving track, size, and intensity. In this study, a vortex-implanted initialization scheme for the mesoscale eddy prediction (VISTMEP) is developed. With the VISTMEP, a bogus vortex is first constructed in terms of 3D SLA-derived currents, and then it is implanted into the model initial field to obtain a more accurate 3D current field of a mesoscale eddy for prediction. The results from idealized experiments show that the VISTMEP can significantly improve prediction of the mesoscale eddy with a longer valid prediction length up to 30 days compared to the experiment with the traditional initialization. Detailed analysis indicates that, as the model is integrated forward, a more “realistic” 3D structure of the eddy in terms of both current and temperature fields is formed when the VISTMEP is employed, leading to the improvement of the eddy prediction regarding to the moving track, size, and intensity of the eddy, which is largely influenced by the accuracy of the initial current field of the eddy obtained by the VISTMEP. This study provides an innovative method for the mesoscale eddy prediction, which could have great potential application in operational services of the marine environments.


OS13-A050
Development of Marine Electronic Sensor Tags for Animal and Environmental Monitoring

Yang YANG1#+, Zihong WEI1, Hai ZHANG1, Tohru SUGAHARA2, Chenjing SHANG3
1Chinese Academy of Sciences, 2Kyoto Institute of Technology, 3Shenzhen University

The marine observatory network is an integral part of the marine monitoring and detection system, and is critical for safeguarding marine interests, developing marine resources, early warning of disasters, and protecting the marine environment. Especially, underwater mobile platforms have broadened the scope of application of the ocean observation network, allowing it to complete complex and intelligent tasks with extended duration and larger coverage. Marine electronic tags are sensors attached to marine animals. They are an effective tool for monitoring marine animals and their surrounding environment. These tags integrate various sensing elements, such as position, temperature, pressure, and salinity, for tracking the physiological state, behavior, and environment of marine life (Hussey et al. 2015, Yang et al. 2021). As these animals are often on the move, migrating between areas with changing seasons and oceanic environments, their activities span much further than traditional submarine observation networks and mobile platforms. As such, tags can be used to collect data on the oceanic environment, such as density and sound velocity profiles, in different regions and depths. This data can be transmitted to coastal stations for further analysis, helping to create a dynamic database of the marine environment. In this contribution, we will report our recent progress in the development of marine electronic sensor tags. Specifically, we will focus on three main points: (1) Achieving a higher integration and miniaturization of the tags, allowing them to be used for a wider range of marine species and expand the coverage of observation platforms. (2) Non-invasive and harmless deployment of tags, reducing the impact on the activities of marine animals. (3) Low power consumption and the collection of high-frequency and high-precision environmental elements in order to complete long-term and stable monitoring. This work was financially supported by the National Natural Science Foundation of China (42222606, 62103400, 42211540003).


OS13-A032
Application of Phenomena-resolving Assessment Methods to Satellite Sea Surface Salinity Products

Senliang BAO1+, Huizan WANG1#, Hengqian YAN1, Ren ZHANG1, Jian CHEN2
1National University of Defense Technology, 2Beijing Institute of Applied Meteorology

It is necessary to evaluate satellite sea surface salinity (SSS) L3 products prior to using them to analyze SSS variability. Instead of performing comparison analysis on the accuracy of products (e.g., Root Mean Square Deviation (RMSD)), two new evaluation methods, information entropy and local variance, are introduced to assess the performance of satellite SSS products in resolving SSS fronts in the tropical Pacific from a new perspective. The satellite SSS except for SMOS BEC have captured the zonal displacement of SSS fronts under the strong El Niño in 2015. It is effective to use entropy and local variance for the assessment of the capability of satellite SSS products, which can provide new sights for analyzing the variability and distributions of SSS. The spatial distribution of local variance identified the abnormal SSS of the satellite products on or near the islands and the result of SSS entropy is beneficial to the analysis of the mechanisms of the SSS variability. In general, the SMOS CATDS and SMAP_70km product are recommended for scientific applications in the tropical Pacific.


OS13-A022
Study on Spatial Varying Bottom Friction Coefficient Estimation to Improve Tide and Surge Simulation

Xiaohui WANG#+, Huizan WANG, Weimin ZHANG
National University of Defense Technology

Tide and surge models play a major role in forecasting coastal flooding due to extreme events or climate change. The model performance is strongly affected by parameters with large uncertainties such as bottom friction. Bottom friction is the term that cannot be directed measured but strongly affects the tide energy dissipation and the vertical transport of momentum and materials. Bottom friction is often described as a function of bottom friction coefficient and the quadratic velocity. We investigated the parameter uncertainties by analyzing the tide energy distribution globally. And sensitivity tests are performed by perturbating spatial varying bottom friction coefficient to compare the model performance with observations. Moreover, parameter estimation is an art-of-state to provide more accurate forecast by reducing the uncertainties of those parameters. The bathymetry and spatial bottom friction coefficient are estimated with a computation- and memory-efficient iterative parameter estimation scheme (time–POD-based coarse incremental parameter estimation; POD: proper orthogonal decomposition). Estimation results show that model performance is significantly improved both for the deep ocean and shallow waters. The spatial vary bottom friction coefficient is an important factor that influences the tide simulation in the shallow waters. Further study would focus on the detailed spatial distribution of bottom friction coefficient in the shallow water with large tide energy dissipation and its relationship with the bathymetry, sediment topography and the tidal current.


Fri-04 Aug | 10:20 - 12:20 | MR310
OS16 - Physical and Biogeochemical Processes: Observational and Modeling Studies

Session Chair(s): Shinichiro KIDA, Kyushu University, Hajoon SONG, Yonsei University

OS16-A010 | Invited
Ocean Mesoscale Air-sea Interactions: Physics, Impacts, and Role of Surface Waves

Hyodae SEO#+
Woods Hole Oceanographic Institution

Recent observations and coupled modeling studies have identified a widespread regime of ocean-atmosphere coupling mediated by mesoscale variability of sea surface temperature and ocean surface currents and their interaction with surface waves in the western boundary current regions. This presentation will provide a broad overview of the current scientific understanding of the physics and the impacts of ocean mesoscale air-sea interaction, as documented in a recent comprehensive review paper by the US CLIVAR Working Group (Seo et al. 2023, JCLI). I will then discuss the impacts of wave-wind and wave-current interactions on air-sea momentum fluxes. Analyses of the parameterized wind stress from high-resolution coupled model simulations against the direct covariance flux measurements in the Atlantic Oceans indicate that the advanced wave-based bulk flux algorithms, such as the COARE v3.5, misrepresent the surface wave impact on the surface drag, especially in mixed sea conditions. Various approaches will be discussed to mitigate such deficiencies in COARE, which offer a path forward to the improved regime-based understanding and representation of the air-sea-wave interaction physics in high-resolution Earth System models.


OS16-A024
Changes in the Upwelling of the South China Sea Under the Global Climate Change

Yineng LI+, Shiqiu PENG#
Chinese Academy of Sciences

Long-term variations in the upwellings in the South China Sea (SCS) are connected with the global climate change. In this study, the ERA5 reanalysis winds and the simulation from the Princeton Ocean Model (POM) are used to investigate the inter-annual to decadal variations of upwelling in the SCS for the time period from 1958 up to 2015. The variations of four main upwellling regions, the eastern coast of Vietnam (VE), the western region of Hainan Island (HNW), the eastern coast of Hainan Island (HNE) and the southern coast of Shantou City (ST) in the SCS, are affected by the PDO, ENSO and IOD. Specifically, the intensity of IOD significantly enhances after the 1990s, and thus the upwelling intensities in the four regions vary significantly. Since the weakening effect of ENSO on the southwest monsoon is significantly strengthened after the 1990s, the negative effect of ENSO on the upwelling intensity in VE is significantly enhanced. However, the effects are weaken in the other three regions. The southwest monsoon in the SCS is enhanced in the central and northern SCS due to the significantly intensification of IOD after the 1990s. As a result, significant intensification of upwelling in VE, HNW and ST occurs after the 1990s. The positive effect of IOD on the upwelling in HNE before the 1990s is changed into the negative feedback after the 1990s due to the change of wind stress curl.


OS16-A019
Sensitivity Analysis of Tsunami Generation by Eruption Around Hunga Tonga-Hunga Ha’api.

Tatsuhiko TOKUTA+, Taro ARIKAWA#
Chuo University

The eruption of Hunga Tonga Ha'apai on January 15, 2022 caused extensive damage to the surrounding islands. Sudden atmospheric pressure changes accompanied by the eruption caused no small sea-level fluctuations around the world. On the other hand, the tsunami that hit the islands around the submarine volcanoes is considered to be mostly caused by the sea-level change due to the eruption. It is important to understand the mechanism of tsunami generation by eruptions in order to quickly determine the arrival time and height of waves in the event of similar phenomena in the future. In this study, sensitivity analysis using numerical simulation was conducted to examine how much the sea-level rise due to eruption affects the sea-level oscillations. In calculation condition, we assume that sea-level rise due to eruptions is caused by seawater upwelling from the crater of a submarine volcano. We also examine how much sea-level rise should be given to be consistent with the observed data and inundation conditions of the islands around the submarine volcanoes. In addition, sensitivity analysis of pressure fluctuations was also conducted to take into account the effect of changes in atmospheric pressure associated with the eruption on the sea-level change.


OS16-A027
Oceanic and Ecological Response to Native Typhoons Cempaka and Lupit (2021) Along the Northern South China Sea Continental Shelf: Comparison and Evaluation of Regional and Global Operational Oceanography Forecasting Systems

Xueming ZHU1#+, Shaojing GUO2, Hui WANG3
1Southern Marine Science and Engineering Guangdong Laboratory (Zhuhai), 2Sun Yat-sen University, 3National Marine Environmental Forecasting Center

The in-situ and satellite observations were employed to compare and evaluate the Global Operational Oceanography Forecasting System from Mercator Océan (MO) and the regional South China Sea Operational Oceanography Forecasting System (SCSOFSv2), with focuses on oceanic and ecological responses to two consecutive native typhoons Cempaka and Lupit in July-August 2021. Results show that SCSOFSv2 performs better in simulating structure of Chla, while MO exhibits a well simulation of the temperature profile in the Pearl River Estuary. On the contrary, variations of SCSOFSv2 SST (MO Chla) are in good correspondence with observations along the northern SCS shelf. Simulated maximum SST cooling is larger and 2~3 days earlier than observations. SCSOFSv2 (MO) maximum Chla is stronger than that of climatological average and the timing of Chla bloom occurs leading to 3 (2) days after passage of typhoon. Typhoon-induced vertical variations of Chla and NO3 reflect different processes of Chla bloom from the coastal waters to continental shelf. Discharge brings extra nutrients to stimulate Chla bloom in the coastal waters, and model results manifest that discharge’s impact extends to the continental shelf 50-150 km away from the coastline. However, bottom nutrients are uplifted to contribute Chla enhancement in the upper and middle layer in the shelf. It is possible that nutrient transported from the open sea along continental slope with the bottom cold water to trigger Chla enhancement in the Taiwan Bank.


OS16-A005
Impact of a Semi-enclosed Estuary on Freshwater Outflow and Biogeochemical Response for a Small-scale River

Shinichiro KIDA1#+, Kiyoshi TANAKA2, Tomonori ISADA3, Tomohiro NAKAMURA3
1Kyushu University, 2The University of Tokyo, 3Hokkaido University

Shallow and large estuaries are often found at river mouths, limiting the direct input of freshwater from the river to the ocean. An idealized numerical model was used to understand how such a lagoon-type estuary may change the dynamics of freshwater outflows from rivers compared to a classical river plume established by large-scale rivers. Model experiment shows that the water mass exchange flow between the estuary and the ocean occurs with considerable time variability across the narrow inlet channel by forming freshwater and oceanic water plumes. A freshwater plume forms in the ocean from the late-ebb to early-flood period while an oceanic plume forms in the estuary from the late-flood to early-ebb period. The area size of the estuary determines the strength of the oceanic plume that intrudes into the estuary and the shallow depth makes this plume barotropic and well-mixed in the vertical. The tidally forced plumes are found to play a significant role by exporting freshwater from the estuary to the ocean through eddy freshwater flux as the strength of the tidal exchange flow overwhelms that expected for the estuary circulation. Model results also show nutrients discharged through freshwater outflow mixing with oceanic water below and inducing phytoplankton blooms along the interface of the freshwater and oceanic water.


Fri-04 Aug | 1:10 - 3:10 | MR309
OS13 - Ocean Observations: Data Processing, Assimilation, Reconstruction and Application

Session Chair(s): Huizan WANG, National University of Defense Technology

OS13-A021 | Invited
Progress, Challenges and Future Applications of Interferometric Remote Sensing in the Observation of Sub-mesoscale Ocean

Yongsheng XU#+
Chinese Academy of Sciences

Submesoscale processes in the ocean control the energy exchange of sea-air materials and the vertical transport of nutrients and heat in the ocean, which is an important aspect of the study of ocean energy budget balance and energy cascade. However, the conventional radar altimeter satellites cannot resolve the ocean submesoscale processes. Future improvements in the resolution of ocean satellites will concentrate mostly on interferometric remote sensing technologies, such as interferometric altimetry and interferometric current measurements. The new generation of interferometric remote sensing technology for sub-mesoscale ocean processes has been selected as one of the top ten marine science frontier issues and engineering technical issues in the 2020 World Marine Science and Technology Forum. At present, SWOT, a wide-swath interferometric remote sensing satellite designed to detect submesoscale sea surface high changes, has been launched for two months, and its ability to resolve submesoscale ocean processes is being tested. Preliminary research projects on submesoscale current observations using interferometric techniques have been initiated in Europe, the United States, and China. We anticipate that these new generation of interferometric remote sensing observations will soon become available and play an important role in ocean research science. This presentation will introduce the development of Marineinterferometric remote sensing technologies in China, including related projects, sea experiments, error correction and the development of data processing methods. The challenges, recent developments, and future applications of interferometric remote sensing in the study of submesoscale ocean processes will be presented using a combination of theoretical explanations and concrete examples.


OS13-A008
Updated Estimate of the Indonesian Throughflow Transports

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 observation-based quantification of its volume transport and variability 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 schemes and newly available salinity reconstruction products. The mean ITFG of 1993-2018 is 8.6±0.2 Sv (error representing data uncertainty), in which contributions of the temperature and salinity components (ITFT and ITFS) are 6.0±0.2 and 2.8±0.1 Sv, respectively. While the interannual variability of ITFG (~2.7 Sv in standard deviation) is dominated by ITFand slightly attenuated in amplitude by ITFS, the strengthening trend of 0.80 Sv decade-1 during 1983-2018 arises primarily from ITFS.


OS13-A004
Dynamics of the Meridional Overturning Circulation in the Indian Ocean

Lei HAN#+
Xiamen University Malaysia

The Indian Ocean Meridional Overturning Circulation (IMOC) was well known for its remarkable seasonal variation, which was attributed to Ekman flow plus its barotropic compensation (Lee and Marotzke, 1998). However, by tracking the isopycnal displacement of the Indian Ocean, I defined a sloshing MOC streamfunction, which was found highly resembling the traditional Eulerian MOC streamfunction (see the attached figure). It was thus concluded that the IMOC is predominantly a sloshing mode, associated with the isopycnal displacement. By recognizing these isopycnal signals as the first-baroclinic long Rossby wave, I found the IMOC strength was determined by the zonally-integrated Ekman pumping anomaly. As a result, the deep inflow into the Indian Ocean also had seasonal variation that could be attributed to this sloshing mode of overturning circulation, which could be partly verified by the cross-basin transect survey across 32oS that were fully occupied three times in history. The diffusivity dichotomy problem can be also explained by this new perspective. The importance of the Indian Ocean overturning in the global conveyor-belt was therefore challenged. This study was done with the assimilated product, ECCO v4r3. It has been published as Han (2021, JPO).


OS13-A057
Multi-source Estimations on Warming of the Seas Around China

Xiaohui TANG#+, Fan WANG, Yuanlong LI
Chinese Academy of Sciences

This study broadly reviews and evaluates the seawater warming trends in the seas around China (SAC), which includes the Bohai, Yellow Sea, East China Sea, and South China Sea. The average SST trend of the entire SAC was 0.10-0.14 °C per decade during 1950-2021, based on various datasets, stronger than the global average trend. While the overall warming is unequivocal, the specific rate is sensitive to the differences in time span, region, and data source. Interdecadal variabilities are prominent in the SAC, with a rapid warming after the 1980s, a cooling during the global surface warming slowdown period from 1998 to the early-2010s, and then an accelerated warming after 2011. The East China Sea exhibits the fastest warming rates in the SAC, especially in boreal winter, attributable to the weakening of the winter monsoon and strengthening of warm-water intrusion from the Kuroshio. Estimations of subsurface warming have more uncertainties, hindered by the shortage of observations. Subsurface data from various analysis products are preliminarily evaluated and cross-validated with in-situ observations. Stratification changes in the SAC is roughly discussed.


OS13-A001
Changes in Temperature, Pressure, and Flow Velocity of Seawater Near Seabed Caused by Typhoon

Ching-Ren LIN#+, Feng-Sheng LIN, Kun-Hui CHANG, Ban-Yuan KUO
Academia Sinica

In the northwestern Pacific Ocean, if a typhoon forms, it usually goes northwest. Taiwan region is located at the center of the typhoon's path. On average, three to four typhoons hit areas near Taiwan every year. On 2020/8/17, a tropical disturbance was generated in the eastern waters of Luzon Island, Philippines. By 2 pm on 8/21, Taiwan’s Central Weather Bureau (CWB) upgraded it to a tropical depression and gave it the number TD10. The path moved all the way north and A Tropical Depression Advisory was issued at 4:10 p.m. At 9 a.m. on 8/22, the Japan Meteorological Agency upgraded it to a tropical storm, gave it the international number 2008, and named it "BAVI". On the afternoon of 8/24, it was upgraded to a moderate typhoon. At 11 am on 8/25, the China Meteorological Administration upgraded BAVI to a severe typhoon. At about 8:30 on 8/27, BAVI made landfall on the coast of North Pyongan Province near the border between China and North Korea. It turned into an extratropical cyclone in the afternoon and disappeared. During typhoon BAVI, the Institute of earth science, Academia Sinica just deployed two broadband ocean bottom seismometers with Seafloor Current Meter (SCM) attached to the west end of the Okinawa Trough offshore northeast Taiwan. The storm range of BAVI covers the area where the SCM is deployed. According to the data analysis, before the formation of a typhoon thousands of kilometers away, the change of atmospheric pressure will change the pressure, velocity of seabed flow and the slight change of seabed temperature, which in turn will affect the change of water sound velocity. This article will take Typhoon BAVI as an example to discuss the changes in seawater temperature, pressure, and flow velocity near the seabed caused by typhoons.


OS13-A002
Retrievals of Wind Vectors from Buoy-measured Directional Wave Spectra Using Deep Learning

Haoyu JIANG#+
China University of Geosciences

High-frequency parts of ocean wave spectra are strongly coupled to the local wind. Measurements of ocean wave spectra can be used to estimate sea surface winds. In this study, two deep neural networks (DNNs) were used to estimate the wind speed and direction from the first five Fourier coefficients from buoys. The DNNs were trained by wind and wave measurements from more than 100 meteorological buoys during 2014-2018. An independent validation shows that the overall root-mean-square error (RMSE) of the estimated wind speed is 1.3 m/s and that of wind direction is 17°when wind speed > 7 m/s. It is also found that the wave measurements can best represent the wind information about 30 minutes ago because the high-frequency portion of the wave spectrum integrates preceding wind conditions. When using the wave spectra from buoys to retrieve the wind speed and direction 30 minutes ago, the overall RMSEs become 1.1 m/s for wind speed and 14°for wind direction (wind speed > 7 m/s). This model can not only be used for the wind estimation for compact wave buoys but also for the quality control of wind and wave measurements from meteorological buoys.


OS13-A009
Destinations and Pathways of the Indonesian Throughflow Water in the Indian Ocean

Yaru GUO#+
Chinese Academy of Sciences

Passage of the Indonesian Throughflow (ITF) water through the Indian Ocean constitutes an essential section of the upper limb of the Global Ocean Conveyor Belt. Although existing studies have identified a major exit of the ITF water to the Atlantic Ocean through the Agulhas Current system, our knowledge regarding other possible destinations and primary pathways remains limited. This study applies the Connectivity Modelling System (CMS) particle tracking algorithm to seven model-based ocean current datasets. The results reveal a robust return path of the ITF water to the Pacific Ocean. The partition ratio between the Atlantic and Pacific routes is 1.60±0.54 to 1, with the uncertainty representing inter-dataset spread. The average transit time across the Indian Ocean is 10-20 years to the Atlantic and 15-30 years to the Pacific. The “transit velocity” is devised to describe the three-dimensional pathways in a quantitative sense. Its distribution demonstrates that the recirculation structures in the southwestern subtropical Indian Ocean favor the exit to the Atlantic, while the Antarctic Circumpolar Current in the Southern Ocean serves as the primary corridor to the Pacific. Our analysis also suggests the vital impact of vertical motions. In idealized tracing experiments inhibiting vertical currents and turbulent mixing, more water tends to linger over the Indian Ocean or return to the Pacific. Turbulence mixing also contributes to vertical motions but only slightly affects the destinations and pathways of ITF water.


OS13-A037
An Energy Conservative Estimate of Ocean Meridional Heat Transport

Yuying PAN1+, Lijing CHENG2#
1Chinese Academy of Sciences, 2Institute of Atmospheric Physics, Chinese Academy of Sciences

Because of its large specific heat, ocean has an enormous impact on the global energy budget, which can vary significantly on annual and longer time scales. The poleward heat transported by the oceans accounts for one third of the total meridional heat transport. The observed oceanic meridional heat transport (OMHT) can be estimated as a residual of the net sea surface heat flux (FS) and the ocean heat content tendency (OHCT). Here we used four sets of ocean heat content products and two sets of FS products to produce estimates of OMHT. For the global ocean, an immediate check and constraint on the results of OMHT is that they must go to zero at the boundaries. However, due to the mismatch between FS and the OHCT globally, it occurs the accumulated inferred value at Antarctica when we integrate OMHT southward from the North Pole. Trenberth et al (2019) proposed to distribute the error at the Antarctic coast to the global oceans by latitude weighting. In this study, we take the uncertainties between different data into account, and convert the error at 78.5°S to the adjustment of the whole ocean by taking the value of uncertainty as the weight. The mean state, annual cycle and interannual variability of OMHT are computed and presented. We find that the major uncertainties of climatological mean OMHT come from the choice of FS products (DEEP-C Version 5.0 provided by Liu and Allan, TF2018 provided by Trenberth and Fasullo), between which difference arises from lack of land surface heat flux adjustment in TF2018. On the interannual or decadal scale, the result shows there is a global-scale slowdown of the OMHT.


Fri-04 Aug | 1:10 - 3:10 | MR310
OS16 - Physical and Biogeochemical Processes: Observational and Modeling Studies

Session Chair(s): Hajoon SONG, Yonsei University, Yong-Jin TAK, Gangneung-Wonju National Unversity

OS16-A002
Studies of Marine Nitrogen Fixation from Physiology to Ecosystems: Data Synthesis and Models

Ya-Wei LUO#+, Weicheng LUO, Zhibo SHAO, Hua WANG
Xiamen University

Marine N2 fixation, mainly conducted by cyanobacterial diazotrophs, is comparable to other external source of the biologically available nitrogen into the global ocean, supporting primary production and regulating carbon export in a large part of ocean that is N-limiting. We established several eco-physiological models to study the dominant marine nitrogen-fixer, Trichodesmium. One model quantitatively supported that ocean acidification (OA) reduced Trichodesmium N2 fixation and suggested that the reduction was mainly caused by decrease in nitrogenase efficiency under OA. We further predicted that under the RCP 8.5 scenario, OA would reduce N2 fixation potential of Trichodesmium by 27% within this century. Another model solves the conflict between the O2-evolving photosynthesis and O2-inhibiting Nfixation in Trichodesmium, finding that the two processes could coexist in a single cell during daytime just by temporally segregating their peaks. We suggest that the long-believing view of the spatial segregation between photosynthesis and Nfixation does not benefit Trichodesmium. At the ecosystem level, we examined both the top-down and bottom-up controls on marine Nfixation by synthesizing historical data. We found that non-cyanobacterial diazotrophs (NCDs), which are presumably heterotrophs, are more abundant in the environment of high productivity, high nutrient, low iron and mesoscale cyclonic eddies, suggesting a niche separation from autotrophic cyanobacterial diazotrophs. We also analyzed the logarithmic regression relationship between N2 fixation rates and diazotrophic biomass using historical dataset, and found that Trichodesmium was subject to a stable top-down control, which however is weaker than its bottom-up control; the top-down pressure on unicellular diazotrophs has large spatiotemporal variations. These analyses can help us to further understand the spatiotemporal distribution of Nfixation in the ocean and predict its future changes.


OS16-A003
Comparison of Ocean Deoxygenation in the Last Half Century Between CMIP Models and an Observational Dataset in the North Pacific

Yumi ABE#+, Shoshiro MINOBE
Hokkaido University

We investigated the relationship between the observed and simulated dissolved oxygen (O2) inventory changes in the North Pacific by analyzing an observational dataset and the Coupled Model Intercomparison Project Phase 5 and 6 (CMIP5/6) model ensembles between 1958 and 2005. A total of 20 models were analyzed for CMIP5/6, with one to three ensemble members for each model. While the multi-model ensemble mean is lower than the observed O2 inventory decreasing trend, several model ensembles showed a decreasing trend higher than the observed value. This result suggests that instead of the forced response, internal variability and model dependency are more important for reproducing the observed trend. An inter-ensemble empirical orthogonal function (EOF) analysis revealed that the different simulated magnitudes of the decreasing O2 trend is closely associated with the first EOF mode, and ensembles with strong decreasing trends are characterized by large oxygen reduction in the subarctic, especially around the boundaries between the North Pacific Ocean and the Okhotsk as well as the Bering Seas. The high O2 decrease in the subarctic is consistent with the spatial pattern of the observed O2 trend. Therefore, the internal climate variability plays a vital role in the observed strong ocean deoxygenation in the North Pacific. Further analysis of climate models indicated that the O2 decrease in the subarctic was primarily caused by physical factors because a significantly high correlation is present between the potential temperature and O2 inventory trend in the subarctic, followed by sea ice volume, whereas a minimal correlation coefficient is present between dissolved organic carbon and the O2 inventory trend. However, the observations have a larger ratio of O2 inventory trend to temperature trend than any of the ensembles, and thus the relationship between O2 and temperature change in the subarctic seen in the CMIP5/6 simulations is inaccurate.


OS16-A006
Effect of Sea Surface Warming on Primary Production and Phytoplankton Size Classes (PSCs) in the Coastal Oyashio and Oyashio Regions, Northwest Pacific

Willy ANGRAINI1#+, Koji SUZUKI1, Hiromi KASAI2, Tomonori ISADA1
1Hokkaido University, 2Japan Fisheries Research and Education Agency

Oceanic primary production by phytoplankton photosynthesis has a fundamental role as essential support on marine food webs and biogeochemical processes. Ocean color satellite remote sensing has recently estimated the global net primary production decline of approximately 0.8 Pg C y-1 between 1998 to 2015, probably associated with increasing thermal water column stratification and decreasing nutrient supply to the surface mixed layer. A recent study reported the Oyashio Regions, northwest Pacific, which is well known as low temperature and rich in macronutrients, have shown the abruptly increasing temperature from 2010-2016 likely promoted the altered species abundance and distribution (e.g. phytoplankton, mesozooplankton, subtropical and tropical fish migrants). The environmental forces may change the biomass and community structure of marine phytoplankton as the basis of marine ecosystem in the northwest Pacific, which has the highest fishery production among the world’s oceans. Nonetheless, little is known about the impact of rising sea surface temperature (SST) on primary productivity (PP) associated with the phytoplankton size classes (PSC) and chlorophyll-a concentration. In this study, we conducted monthly field campaigns in the Coastal Oyashio water of Akkeshi Bay in 2022 to investigate the relationship between PP and PSC or the absorption coefficient of phytoplankton (aph(lambda)). Micro-sized phytoplankton with high chlorophyll-a concentration was predominant during spring (March-April), gradually declined with time and rapidly increased in summer (August). We also found a strong positive correlation between aph(443) and PP in surface waters. Therefore, aph(443) could be a promising parameter for estimating surface PP using satellite ocean color data such as from MODIS-Aqua. We will demonstrate the effect of enhanced SST on the spatiotemporal variation of surface PP and PSC in the Coastal Oyashio and oceanic Oyashio regions through the 20-year time series data of MODIS-Aqua.


OS16-A015
Equatorial Western Pacific Phytoplankton Blooms During “double-dip” La Niña Events

Ruyan CHEN#+
South China Sea Institute of Oceanology, Chinese Academy of Sciences

Phytoplankton in the equatorial western Pacific tends to bloom during consecutive (“double-dip”) La Niña events with nonlinear characteristics: extremely high chlorophyll-a (Chl-a) concentrations typically occur during the second-year La Niña events even when the associated SST anomalies are significantly weakened. Photosynthetically available radiation is found to have the strongest correlation with the equatorial western Pacific Chl-a fluctuations. However, barrier layer variation is critical in driving the strong bloom events seen in the second-year La Niña, which can be further explained by the nonlinear thermal advection within the isothermal layer. To improve the current climate models’ performance in simulating the western Pacific phytoplankton bloom events, it is recommended that the influence of barrier layer should be better considered.


OS16-A018
Quantifying Aquaculture Bivalve-environmental Interactions with a Hybrid Eulerian/Individual-based Model

Liuqian YU1#+, Ye LIU2
1The Hong Kong University of Science and Technology (Guangzhou), 2The Hong Kong University of Science and Technology

Bivalve aquaculture plays a significant and growing role in providing food, nutrition, and employment for human society. Ensuring sustainable development of bivalve aquaculture requires a quantitative understating of the dynamic bivalve aquaculture-environment interactions. Yet such quantification has often been limited by the computational constraints on modelling a large number of bivalve ecophysiology and physical-planktonic variables in 3D spatially explicit domains. To alleviate the computational constraints and accurately represent the bivalve-environment interactions, we are developing a hybrid Eulerian/Individual-based modelling framework. The hybrid model can combine the benefit of the grid-based Eulerian model in efficiently tracking the physical-planktonic dynamics and the advantage of the individual-based model to simulate higher trophic level predator groups (e.g., bivalves) that have complex life-history and physiological processes. Here we present a hybrid model coupling an ocean physical-biogeochemical model, which simulates the hydrodynamics and lower-tropic-level food web dynamics, and a Dynamic Energy Budget (DEB) model, which simulates the growth and reproduction of bivalves. We will show simulation results from the hybrid model implemented in the 1D framework for different time-series stations in Pearl River Estuary. Despite the model being one-dimensional, insights on bivalve aquaculture-environment interactions and feedback in a typical growing season of the farmed oysters in the estuary are gained. Lastly, critical steps toward implementing the hybrid model in the 3D framework for the entire estuary are discussed.


OS16-A020
Global Warming-driven Changes in the Carbon to Phosphorous Ratio of Marine Dissolved Organic Matter

Sreeush M G1#+, Eun Young KWON2, Sun-Seon LEE3
1Pusan National University, 2IBS Centre for Climate Physics, 3IBS Center for Climate Physics

Stoichiometric ratios of carbon (C) to phosphorus (P) in marine organic matter play an important role in sustaining marine ecosystems and regulating the ocean’s carbon sequestration from the atmosphere. The C:P ratios of dissolved organic matter (DOM) are particularly important for long-term carbon sequestration through a process called the microbial carbon pump. However direct observations of the stoichiometric ratios of DOM are sparse and highly noisy. Using the large ensemble simulations based on an Earth system model, we suggest that the C:P ratios in DOM are highly sensitive to nutrient stresses for phytoplankton in the global ocean and that anthropogenically forced increases in the C:P ratios might have already emerged in majority of the global ocean. The C:P ratios in DOM are projected to increase by up to two fold in low-latitude as of 2100, due to increasing phytoplankton C:P ratios and increasing uptake rates of dissolved organic phosphorus by phytoplankton. The associated increases in refractory dissolved organic carbon are only 1% globally and confined to the surface as of 2100. Yet, combined with the effects of slower ocean overturning rates and phytoplankton C:P plasticity, the enhanced microbial carbon pump may enable the deep ocean to store additional carbon in a warmer climate, which has previously been overlooked. 


OS16-A030
Hydrodynamic and Ecological Effects of Large-scale Suspended Mussel Farms: Field Observations and Numerical Simulations

Wei ZHONG1+, Jun LIN1#, Hidekatsu YAMAZAKI2,3
1Shanghai Ocean University, 2Sun Yat-Sen University, 3Okinawa Institute of Science and Technology

The hydrodynamic and ecological effects of the largest suspended mussel farms in the East China Sea near Gouqi Island, was investigated using a high-resolution 3D ocean model and field observations. To capture the farm effects, an additional momentum sink term and trace decay term were introduced in the model. The model results compared well with the observations. The present model and observational results indicate that the presence of farms reduces the flow by more than 79%, 55%, and 34% in the upper, middle, and bottom layers at the farm center, respectively. The field observations of vertical profiles of current suggest that the thickness of surface canopy boundary layer can reach 5m upstream the farm during flood tide, increases gradually downstream, and up to 10m under the cumulative influences of the farm. And a wake zone was observed downstream of the farm during flood tide. The results of sampled phytoplankton abundance show that aquaculture water layer (5 m beneath sea surface) is much lower than that of outside the farm during summer, while there are no significant differences between inside and outside the farm by winter. The simulations of spatiotemporal pattern of mussel food depletion show that spring tide is much lower than neap tide. The high degree of food depletion within the farming area is in a northeast-southwest direction due to the tidal motion and shelter effect of the islands. The channel plays an important role for water exchange between the inside and outside of the farming area, in addition to facilitating passage, and that food depletion in the farming area can be well improved by optimizing the channel layout. Understanding farm-induced hydrodynamic and ecological effects provides insight into how to optimize farm layouts based on local hydrodynamics, to maximize farm productivity and minimize the environmental impacts.


Fri-04 Aug | 1:10 - 3:10 | MR322
OS14 - Quantifying Relative Sea-level Changes from Geological Archives and Geophysical Modelling: Using the Past to Constrain the Future

Session Chair(s): Tanghua LI, Nanyang Technological University, Timothy SHAW, Nanyang Technological University

OS14-A004
Detecting 21st-century Antarctic Ice-sheet Meltwater with Oxygen Isotope

Hyuna KIM1#+, Axel TIMMERMANN2
1IBS Center for Climate Physics, 2Pusan National University

The Antarctic ice-sheets contain oxygen isotopes with depleted δ18O values, ranging from -20 to -60 ‰. This substantial difference between the δ18O values in ice and the surrounding seawater (around -1 ‰) makes seawater δ18O (δ18Osw) a promising tool for measuring 21st-century Antarctic ice-sheet meltwater discharge. Here, we determine the timing and location of the emergence of the meltwater signal by conducting a series of hosing experiments on an isotope-enabled Community Earth System Model (iCESM). The artificial meltwater discharge into the model was based on results from the other fully-coupled ice-sheet model in Shared Socioeconomic Pathways (SSP) scenarios, taking into account the amplitude and spatial distribution. The additional freshwater with negative δ18Osw anomalies freshens the ocean, hinders deep water formation, intensifies upper ocean stratification, and leads to surface cooling and an increase in sea-ice growth. Our results show that δ18Osw offers better detectability compared to salinity in the presence of inter-annual variability of sea-ice and forced increases in sea-ice growth, which can obscure the meltwater signal in salinity. It further demonstrates that the emergence of Antarctic ice-sheet melt in the surface ocean provides the best site for quickly and accurately detecting the meltwater signal.


OS14-A011
Modeling Approach for Reconstructing Past Sea-level Curve from Surface Geometries of Coral Microatolls

Junki KOMORI#+, Khai Ken LEOH, Aron MELTZNER
Nanyang Technological University

Coral microatolls are colonies of coral that inhabit the shallow tropical seafloor, and their vertical growth is precisely limited by the sea surface. Therefore, fossil coral microatolls can be used as proxies to reconstruct past relative sea-level (RSL) curves by retrieving their growth history. The internal growth structure of coral microatolls retains precise details of the coral’s growth history and hence the changes the coral experienced in relative sea level (RSL) as it grew. Past studies involved the physical extraction of a vertical radial slab through a microatoll to examine this growth structure and reconstruct RSL, but increasingly efforts are being made to quantify RSL changes using ‘remote sensing’ of the coral’s surface morphology, avoiding destruction of the coral specimen. To enable a more rigorous reconstruction of past sea-level curves based on a digital elevation model (DEM) of a coral's outer surface, we developed a numerical simulator for modeling the growth of coral microatolls using Blender, an open-source 3D graphics software package. Our simulator allows for geometrical calculations through a graphical user interface and can interactively display microatoll geometries, including the outer surface and annual bands, by changing model parameters such as sea-level curve and growth speed. In this presentation, we will demonstrate the simulator's capabilities with synthetic coral models generated from RSL data, as well as examples of inversely reproduced RSL from observed coral morphologies. Our simulator is a powerful tool for research and can greatly aid in reconstructing past sea-level curves with greater accuracy and efficiency.


OS14-A008
Reconstructing Sea-level Using Coral Microatolls from Indonesia

Jedrzej MAJEWSKI1#+, Aron MELTZNER1, Adam SWITZER1, Fangyi TAN1, Jennifer WALKER2, Danny NATAWIDJAJA3, Bambang SUWARGADI3, Benjamin HORTON1,2
1Nanyang Technological University, 2Rutgers University, 3Indonesian Institute of Sciences

Instrumental records from tide gauges have been the primary source for understanding relative sea-level (RSL) changes through the 20th and 21st century. However, the scarcity of reliable, long-term tide-gauge records in tropical regions creates significant uncertainty in the understanding RSL change. Coral microatolls, which are coral colonies vertically constrained by sea level, can be used as a proxy for RSL. Therefore, coral microatolls can fill in a gap in understanding of RSL change in areas with scarce or non-existent instrumental. Here we reconstruct RSL for Belitung Island, Indonesia, an area without tide gauge records. The reconstruction is based on two Porites sp microatolls from Tanjung Kubu and Tanjung Pandan, on the Northwestern coast of Belitung. Microatolls were chosen for their size (length of record) and only from freely draining locations to avoid ponding which can disrupt the RSL record. We cut radial slices from each microatoll, x-rayed them to reveal internal structure and reconstructed their RSL records. The record spans from 1967 to 2006 and comprises 8 sea level index points. We used an Errors-In-Variables Integrated Gaussian Process model to calculate total RSL change and rate. RSL rose by 9.6 cm from 1967 to 2006 at a rate of 2.2 ±3.5 mm/yr. (2𝜎), within uncertainty of the global rates for the late 20th century. Our reconstruction is based on only two individual microatolls and additional corals could reduce the uncertainty and extend the length of the record. The use of coral microatolls to reconstruct RSL has potential for wider application in other tropical areas without access to tide-gauge data.


OS14-A014
Mid Holocene Relative Sea-level Changes from Coral Microatolls of Pulau Biola, Singapore

Jennifer QUYE-SAWYER1#+, Lin Thu AUNG1, Nurul Syafiqah TAN2, Jing Ying YEO1, Zihan AW1, Aron MELTZNER1
1Nanyang Technological University, 2Earth Observatory of Singapore

Coral microatolls are precise proxies for rates and magnitudes of relative sea-level (RSL) change in low-latitude coastal regions. These coral colonies live in the intertidal zone, where occasional partial aerial exposure and mortality produce a three-dimensional concentric ring structure reflecting local sea-level changes during the coral’s lifetime. Therefore, the surface morphologies of well-preserved fossil microatolls may be used to determine rates of past RSL change and augment the local Holocene sea-level curve if fossil ages, and elevations compared to living counterparts, can be reliably constrained. In this study, we present preliminary sea-level reconstructions from Pulau Biola (Violin Island), Singapore. We have combined radiometric ages, structure-from-motion photogrammetry and LiDAR models, and levelling surveys of several Porites sp. and Diploastrea heliopora fossil microatolls to generate a RSL history spanning more than two centuries in the mid Holocene. We have also compared the elevations of these fossils to local living corals of the same genus to estimate absolute magnitudes of past water level and produce sea-level index points. For Pulau Biola, preliminary calibrated radiocarbon ages and fossil elevations are consistent with an overall rise in sea level between 7.7 and 7.4 kyr BP, with initial analysis suggesting RSL approximately 0.2 to 0.7 m higher than present. In addition, decimetre-scale sea-level fluctuations during this period are inferred from decreasing and increasing ring elevations within corals. These fluctuations indicate a more complex sea-level history than has been resolved by other proxies in this region.  Ongoing work aims to refine absolute coral chronology using additional dating techniques and compare corals across local field sites, from which we hope to generate a more complete understanding of Holocene sea level in Singapore. 


OS14-A010
Sea-level Markers Preserved in a Late Holocene Beach Ridge System on Phra Thong Island, Thailand

Rahul KUMAR1#+, Adam SWITZER1, Chris GOURAMANIS2, Charles BRISTOW3, Dominik BRILL4
1Nanyang Technological University, 2Australian National University, 3Birkbeck, University of London, 4University of Cologne

The existing instrumental sea-level record is insufficient to understand the relation of sea-level with global temperature on centennial timescales. Regional coastal development strategies for major infrastructure need planning that is informed by sea-level histories spanning at least the Common Era and these have not been widely studied in Southeast Asia. This period is crucial to provide a pre-industrial context to understand changes in sea-level with climate. This study examines the efficiency of beach ridge system’s stratigraphy as a proxy for the regional sea-level record. Beach ridge systems are coastal landforms that exist globally and here we present Ground Penetrating Radar (GPR) profiles on a prograded coast in Thailand. In the shore-normal GPR profile, we identify the downlap point marking the boundary between beachface and shoreface facies and use this as an index point of past sea-level. GPR reflection profiles were collected from the northern segment of Phra Thong Island (Thailand) beach ridge system in 2014 using a 100 MHz antenna. The processed 800 m long shore-normal GPR profile was topographically corrected, and a series of index points interpreted across the profile were connected to approximate past sea-level. Optically Stimulated Luminescence (OSL) dates collected at locations slightly offset from the same profile line were incorporated to create the temporal sea-level record. The record shows an overall falling trend of sea-level in the region from ~2700 years BP to ~400 years BP. We account for errors induced in elevation and OSL dates data and present a sea level curve that is consistent with other proxy based sea-level curves obtained in the region. The outcome of this study confirms that the study of tropical beach ridge systems armed with GPR and OSL techniques can be highly effective for reconstructing regional sea-level trends.


OS14-A007
Constraining Late Holocene Sea Level Using Mangroves – A Case Study from Singapore

Christabel TAN1#+, Timothy SHAW1, Stephen CHUA1, Yudhishthra NATHAN1, Niamh CAHILL2, René DOMMAIN1, Jedrzej MAJEWSKI1, Fangyi TAN1, Yun Fann TOH 1, Tanghua LI1, Margaret CHRISTIE3, Benjamin HORTON1,4
1Nanyang Technological University, 2Maynooth University, 3McDaniel College, 4Rutgers University

The reconstruction of late Holocene relative sea level (RSL) is important to understand the drivers of sea level and prepare for future sea-level rise. Here, we investigated mangrove environments in Pulau Ubin, Singapore to develop sea-level index points (SLIPs) and reconstruct late Holocene RSL changes. We established transects across terrestrial, mangrove and tidal flat environments and sampled surface sediments for grain size, total organic carbon content and pollen composition. We also surveyed vegetation zones to estimate the indicative meaning of mangroves relative to the mean tide level (MTL) and applied the indicative meaning to basal mangrove sediments collected from sediment cores in an upland-mangrove transition area. From these cores, we extracted plant macrofossils and fine fraction (<63 μm) sediments from basal sediments for radiocarbon dating and applied an Errors-In-Variables Integrated Gaussian Process (EIV-IGP) model that considers the vertical and temporal uncertainty of SLIPs to reconstruct the magnitude and rate of RSL changes. The indicative range of mangroves in Pulau Ubin is between 1.16 ± 0.01 m MTL and 0.08 ± 0.01 m MTL, which is a 33 % reduction than the approach used in previous mangrove-based studies in Singapore. We developed eight new SLIPs with elevations from -0.17 ± 0.56 m MTL to -0.70 ± 0.56 m MTL and radiocarbon ages between 2305 ± 123 and 526 ± 25 cal. yrs. BP. Application of the EIV-IGP model shows RSL was stable between ~2300 and 520 cal. yrs. BP varying from -0.67 ± 1.08 m MTL to -0.45 ± 1.28 m MTL. There is a mismatch between the reconstruction and GIA model predictions that shows RSL above present throughout the late Holocene. Possible driving processes for the mismatch include shelf subsidence, global cooling during pre-industrial Common Era and/or atmosphere ocean interactions.


OS14-A005
A Re-evaluation of Holocene Relative Sea-level Change Along the Fujian Coast, Southeastern China

Fengling YU1#+, Nannan LI2, Zhaoquan HUANG2, Haixian XIONG3,4, Tanghua LI5
1Xiamen University, China, 2Xiamen University, 3Southern Marine Science and Engineering Guangdong Laboratory, 4Sun Yat-sen University, 5Nanyang Technological University

The southeastern China coast is of special interests in the study of past and present relative sea-level (RSL) change, given its distal location from giant ice sheets. During the past decades, a large number of sea-level indicators have been retrieved from the Fujian coastal region which allows for recalibration and recalculation of sea-level index points (SLIPs). This study constructs a database of Holocene RSL observations for the Fujian coast, southeastern China. The database contains 59 quality-controlled SLIPs which show that Holocene RSL for the Fujian coast did not exceed present, except potentially during 7.5 – 5.5 cal. kyr BP and 1.8 – 0.7 cal. kyr BP. Rates of RSL change were highest during the early Holocene and have decreased over time, due to the diminishing response of the Earth’s mantle to GIA and reduction of meltwater input. A series of sea-level oscillations were recorded in our SLIPs-based reconstructions which might correspond to global climate warming or cooling events. We compared the spatial variability of RSL histories with the ICE-6G_C (VM5a) GIA model and ANC-ICE models, and substantial misfits were recognized: (1) the deceleration of the early-Holocene sea-level rise ended about one millennia earlier in the ICE-6G_C VM5a model than in the SLIPs-based reconstructions; (2) GIA model predictions show a mid-Holocene sea-level highstand of 1 – 3 m which is absent from our SLIPs-based reconstructions; and (3) all GIA model predicted a gradual RSL fall to 0 m since the middle Holocene, while our reconstruction displays significant RSL oscillations. It is presently unknown whether these misfits are caused by regional tectonic movement or parameters used in the GIA models. Future applications of spatiotemporal statistical techniques are required to better quantify the gradient of the isostatic contribution and to provide improved context for the assessment of the ongoing acceleration of sea-level rise.


OS14-A002
“Treasure Map” of the Mid-Holocene Sea-level Highstand in Southeast Asia

Tanghua LI1#+, Stephen CHUA1, Nicole KHAN2, Patrick WU3, Benjamin HORTON1,4
1Nanyang Technological University, 2The University of Hong Kong, 3University of Calgary, 4Rutgers University

The mid-Holocene highstand is a common characteristic of Holocene relative sea level (RSL) reconstructions from regions distal from ice sheets when sea level reached higher than present-day levels. The mid-Holocene highstand’s timing and magnitude vary spatially due to hydro-isostatic processes including ocean syphoning and continental levering. However, the highstand properties (e.g., timing, magnitude, spatial pattern) are poorly constrained in Southeast Asia with a paucity of highstand RSL data due mainly to poor preservation of highstand records. 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 in Southeast Asia. We produced the “treasure map” by considering the residual between present-day topography (GEBCO_2022 Grid) and accommodation space produced by predicted highstand elevations across Southeast Asia 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 northern east coast and central west coast of Malay-Thai Peninsula, east coast of Sumatra, north coast of Java, and southwest coast of Borneo. The “treasure map” can guide future RSL data collection efforts.



Planetary Sciences


Mon-31 Jul | 10:20 - 12:20 | MR334
PS01 - Planetary Space Weathers: Fundamental Plasma Interactions in Space Environments

Session Chair(s): Zhonghua YAO, The University of Hong Kong

PS01-A010 | Invited
Energetic Electron Precipitation from Plasma Sheet Injections: The Role of Whistler-mode Waves

Anton ARTEMYEV1#+, Xiao-Jia ZHANG2, Vassilis ANGELOPOULOS1
1University of California, Los Angeles, 2The University of Texas at Dallas

Plasma sheet injections is the main source of energetic (~100keV) electron population in the inner magnetosphere. These injections are associated with electron adiabatic heating, formation of anisotropic electron populations, and generation of various electromagnetic waves. Whistler-mode waves are one such wave mode that is often observed around plasma sheet injections. These waves are very effective in isotropizing energetic electrons and scattering them into loss-cone. In this presentation, we combine numerical simulations, near-equatorial THEMIS observations, and low-altitude ELFIN CubeSat observations to investigate the effect of whistler-mode waves on energetic electrons in the plasma injection region. We will demonstrate that electron resonant interactions with whistler-mode waves can significantly change the pitch-angle distribution of energetic electrons and thus warrant to be incorporated in existing injection models. In addition, we will discuss the importance of such resonant interactions for injection physics in the context of magnetosphere-ionosphere coupling.


PS01-A009
Observations of a Planetary-scale 'Heat Wave' Emanating from Jupiter's Aurora Following a Solar Wind Compression

James O'DONOGHUE1,2#+, Luke MOORE3, Henrik MELIN4, Tom STALLARD5, Tanapat BHAKYAPAIBUL6, Chihiro TAO7, William KURTH8, J. E. P. CONNERNEY9,2, Go MURAKAMI1, Hajime KITA10
1Japan Aerospace Exploration Agency, 2NASA Goddard Space Flight Center, 3Boston University, 4University of Leicester, 5Northumbria University, 6University of Illinois Urbana-Champaign, 7National Institute of Information and Communications Technology, 8The University of Iowa, 9Space Research Corporation, 10Tohoku University

At Jupiter, magnetosphere-ionosphere coupling gives rise to intense auroral emissions and enormous energy deposition in the magnetic polar regions. Here we show ground-based maps of Jupiter's upper atmosphere temperatures obtained via the emissions of the major upper-atmospheric ion, H3+. The maps have a spatial resolution of 2 degrees longitude and latitude from pole to equator and trace the global temperature gradient. We found that temperatures decrease steadily from the auroral polar regions to the equator, indicating that the aurora act as a planet-wide heating source. However, during a period of enhanced activity in the auroral region which a solar wind model and Juno WAVES data imply was due to a solar wind compression, a high-temperature planetary-scale-sized structure was also observed on top of this gradient. This presentation reports on the particulars of this feature, including how it appears to be propagating away from the main auroral oval (as determined by estimates of the features' velocity at several longitudes) and its implications for global energy circulation at Jupiter and other planets.


PS01-A017
Statistical Study of the Jovian Decametric Radio Emissions Based on Multiple-view Observations

Ruobing ZHENG1+, Yuming WANG1#, Xiaolei LI1, Chuan Bing WANG1, Xianzhe JIA2
1University of Science and Technology of China, 2University of Michigan

To better understand the physical processes associated with Jovian decametric (DAM) radio emissions, we present a statistical study of DAM emissions and inferred characteristics of DAM sources based on multi-view observations from the Wind and STEREO spacecraft. Altogether 81 isolated strong events in radio dynamic spectra were analyzed from 2008 to 2014. The apparent rotation speed of DAM events derived from multiple spacecraft observations can be used to distinguish Io-related and non-Io-related DAM. We find that the rotation speed of Io-DAM events is in the range of 0.15–0.6 ΩJ and that of non-Io-DAM events is between 0.7–1.2 ΩJ. And the occurrence probability of isolated strong Io-DAM events is found to be about 7 times that of isolated strong non-Io-DAM events. We locate the sources of 79 DAM events and infer their emission angles and associated electron energies. The statistical results show that the DAM source locations (both Io- and non-Io-) are distributed in three preferred high-latitude regions, two in the southern hemisphere (around 30° to 150° and 270° to 330° in System III longitudes) and one in the northern hemisphere (150° to 210°), which is probably caused by the non-symmetrical topology of Jupiter's magnetic field. The difference between Io-DAM source footprints and Io auroral UV spots changes with Io's position in System III longitude, consistent with the previous results from Bonfond et al. (2017) and Hinton et al. (2019). In addition, for the same type of DAM events, the emission angles of non-Io-DAM are smaller than those of Io-DAM, and all the emission angles range from 60° to 85°. Correspondingly, the energies associated with the electrons responsible for exciting the radio emissions are estimated to range between 2 and 22 keV.


PS01-A015 | Invited
A Global Perspective on the Interaction Between Solar Wind and Planets

Yong WEI#+
Institute of Geology and Geophysics, Chinese Academy of Sciences

The solar wind is a continuous stream of charged particles that flows from the Sun and interacts with the planets in our solar system. The nature of this interaction is determined by various factors, including the strength and direction of the solar wind, the magnetic field of the planet, and the composition of its atmosphere. Through decades of space exploration, we have learned that the exchange of energy and matter between the solar wind and the planets can be seen as a dynamic exchange between the Sun and the planets. This exchange of matter and energy also occurs between the Sun and satellites, as well as between planets and their satellites, all driven by the solar wind. Over billions of years, the forms of these interactions have continuously changed, and their effects have accumulated. These interactions play a crucial role in the evolution of planetary atmospheres and magnetic fields, and also impact physical and chemical processes on planetary surfaces and interiors.


PS01-A018
Extreme Space Weather on Jupiter: Auroral-driven Stratospheric Heating, Chemistry and Dynamics

James SINCLAIR1#, Thomas GREATHOUSE2, Rohini GILES2, John LACY3, Julianne MOSES4, Vincent HUE5, Thibault CAVALIE6, Robert WEST1, John BARBARA7, Denis GRODENT8, Bertrand BONFOND8, Chihiro TAO9, Emma DAHL1, Glenn ORTON1+, Leigh FLETCHER10, Patrick IRWIN11
1Jet Propulsion Laboratory, California Institute of Technology, 2Southwest Research Institute, 3University of Texas at Austin, 4Space Science Institute, 5Aix-Marseille Université, 6University of Bordeaux, 7NASA Goddard Institute for Space Studies, 8University of Liege, 9National Institute of Information and Communications Technology, 10University of Leicester, 11Oxford University

Jupiter has the largest and strongest planetary magnetic field and the most volcanically-active moon (Io) in the Solar System. This drives extreme space weather phenomena and makes Jupiter a unique target for studying the coupling between the atmosphere and external space environment. In this work, we present analyses of multiple datasets that capture the modulation of Jupiter’s middle atmosphere, or stratosphere, by the magnetosphere and solar wind. Using a time series of mid-infrared images recorded by NASA’s Infrared Telescope Facility (IRTF), Subaru, and Gemini observatories from 1994 to present, we demonstrate that the magnitude and morphology of stratospheric CH 4 emissions of Jupiter’s auroral regions vary on timescales as short as several days. We interpret this as resulting from variable auroral-related heating of Jupiter’s upper stratosphere in response to magnetosphere and solar wind events. We captured one such event using high-resolution spectra recorded by TEXES (Texas Echelon Cross Echelle Spectrograph) on Gemini on March 17-19th, 2017. We inverted these observations using radiative transfer software and demonstrated that there was a 9 K warming of the upper stratosphere in response to the arrival of a solar-wind compression on March 18th. By performing a retrieval analysis on IRTF spectra similar to those recorded by TEXES, we also determined that the CH4 homopause altitude is higher inside Jupiter’s main auroral regions compared to elsewhere on the planet. This suggests that the energy deposited by the aurora drives turbulence and vertical winds that ultimately transports CH4 and its photochemical by-products to higher altitudes. In general, we find evidence that auroral processes modulate the thermal structure, chemistry and dynamics of Jupiter’s stratosphere at a larger magnitude and on shorter timescales than analogous processes on other planets.


PS01-A003
Trapped and Leaking Energetic Particles in Injection Flux Tubes of Saturn’s Magnetosphere

Xuzhi ZHOU1#+, Ze-Fan YIN1, Yixin SUN2, Dongxiao PAN1, Zhonghua YAO3, Chao YUE1, Qiugang ZONG1
1Peking University, 2Institute of Space Physics and Applied Technology, 3The University of Hong Kong

In Saturn’s magnetosphere, the circulation of magnetic fluxes requires the inward motion of localized flux tubes, in which the equatorial magnetic field is sharply enhanced, and the plasma density is much lower than that in the ambient environment. These flux tubes also carry energetic particles towards the inner magnetosphere. The azimuthal drift motion of the injected energetic particles can produce energy-dispersive signatures, which have been utilized to estimate the age and starting position of the returning flux tubes. In this paper, we demonstrate that the drift motion can be significantly modified by the sharp magnetic gradient at the edges of the flux tubes, which enables the trapping motion of the particles with 90-degree pitch angles. The bouncing particles, on the other hand, are hardly affected by the gradient and therefore can leave the flux tubes to continue their drift around the planet. The coexistence of the trapped and leaking particles, together with the evolution of the trapping region during the inward motion of the returning flux tubes, indicate the diversity of dispersive and/or dispersionless signatures depending on particle pitch angle and spacecraft traversal path across the returning flux tubes. These results improve our understanding of the particle dynamics in Saturn’s magnetosphere, and also indicate that caution should be applied in the interpretation of the observational data for flux tube properties.


PS01-A022
Successive Dipolarization Fronts with a Stepwise Electron Acceleration During a Substorm in Saturn's Magnetotail

Sibo XU+, Shiyong HUANG#
Wuhan University

Substorms are a fundamental phenomenon in planetary magnetospheric systems. Using Cassini measurements, we report a typical event in which four successive dipolarization fronts (DFs) were observed within 1 hour during the substorm in Saturn's magnetotail. The last three DFs caused a type of stepwise electron acceleration and generated energetic electrons. The pitch angle distributions of the electrons show evidence of the Fermi acceleration mechanism behind these DFs. Therefore, we infer the magnetotail dynamics process during Saturn's substorm: The stepwise acceleration by successive DFs powerfully accelerates the field-aligned electrons and generates field-aligned energetic electrons. These high energy electrons are injected into the inner magnetosphere and become an important trigger of Saturn's aurora. Our results show an efficient acceleration mechanism for the electrons caused by successive DFs and confirm an important source of energetic particles during the substorm in Saturn, and these findings improve our understanding of Saturn's substorm and magnetotail dynamics.


Mon-31 Jul | 10:20 - 12:20 | MR335
PS24 - Mercury Science and Exploration

Session Chair(s): Go MURAKAMI, Japan Aerospace Exploration Agency, Joe ZENDER, European Space Agency, Johannes BENKHOFF, European Space Agency

PS24-A007
Updated Status of BepiColombo and Initial Reports on Mercury Flybys

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. The first and second Mercury flybys were completed on 1 October 2021 and 23 June 2022, respectively. In both flybys the closest approach altitudes were ~200km at the southern hemisphere. We performed science observations with almost all the instruments onboard Mio for about +-24 h from the closest approach. In addition, the third Mercury flyby will be completed on 20 June 2023. Here we present the updated status of BepiColombo mission, initial results of the Mercury flybys, and the upcoming observation plans.


PS24-A004 | Invited
Late Accretion Onto Mercury

Ryuki HYODO#+
Japan Aerospace Exploration Agency

Impacts are a fundamental process by which planets grow and are modified. Small impacts, namely crater impacts, affect only a small area of the planet's surface and are much more frequent than stochastic giant impact (Melosh 2011). Here, using analytical and Monte Carlo approaches combined with the updated scaling laws (Hyodo and Genda, 2020, 2021) for the escape mass of the target material and the accretion mass of the impactor material during cratering impacts, we investigated (1) whether late accretion significantly erodes Mercury, and (2) the fate of impactors on Mercury during late accretion. Existing dynamical models of late accretion suggest that Mercury experienced an intense impact bombardment after 4.5 Ga (a total mass of $\sim 8 \times 10^{18} - 8 \times 10^{20}$ kg with a typical impact velocity of $30 - 40$ km s$^{-1}$, depending on the dynamical model). For this parameter range, we found that late accretion could remove 50 m to 10 km of Mercury's early (post-formation) crust, but the change in the core-to-mantle ratio is negligible. Although cratering is notable for erasing Mercury's older geological surface record, we have shown that $\sim 40 - 50$wt% of the impactor's exogenic materials, including volatile-bearing materials, can be heterogeneously implanted on Mercury's surface as a late veneer (at least $\sim 3 \times 10^{18} - 1.6 \times 10^{19}$ kg in total). About half of the accreted impactor's material is vaporised, and the rest is completely melted on impact. In conclusion, late accretion seems to be an inevitable dynamical process at the very last stage of planet formation, and it affects Mercury's surface in both mechanical, chemical and thermal aspects (Hyodo et al. 2021; see also Mojzsis et al. 2018).


PS24-A003
Forming Mercury by Striping Its Primordial Mantle in Tidal Encounters

Hongping DENG1#+, Tong FANG2
1Shanghai Astronomical Observatory, 2Shanghai Astronomical Observatory, Chinese Academy of Sciences

Compared to all other terrestrial planets in the solar system, Mercury has an unusually large metal core, comprising ∼70% of its mass. Giant impacts could have removed a significant fraction of the silicate mantle of a chondritic proto-Mercury, forming the iron-rich present-day Mercury. However, such high-temperature giant impacts seem at odds with the retention of moderately volatile elements on present-day Mercury. We identify a series of extreme close encounters, with the closest approach as small as 3 Venus radii, between proto-Mercury and proto-Venus in N-body simulations of terrestrial planet formation. Further hydrodynamic simulations show that proto-Mercury is partially deprived of its silicate mantle, while its iron core remains intact in such encounters. We find, in favorable cases, four close encounters with fast-spinning projectiles (resulting from previous encounters) can explain Mercury’s present-day iron fraction. These hyperbolic encounters have various outcomes, such as orbital decay, binary planets, and spin rate changes. Hybrid N-body and hydrodynamic simulation are warranted to couple the orbital and encounter dynamics self-consistently and solve the puzzle in Mercury's Origin.


PS24-A005 | Invited
Geochemical Unit Classification on Mercury Using Multivariate Analysis of MESSENGER/XRS Data

Kaori HIRATA1#+, Tomohiro USUI2
1The University of Tokyo / ISAS, JAXA, 2Japan Aerospace Exploration Agency

On the surface of Mercury, volatile elements are more abundant than on other terrestrial planets [Peplowski+ 2012], suggesting that numerous impact events after its formation caused the surface modification and volatiles sensitively reflect them [Hyodo+ 2017]. Two types of different materials are distributed on the surface of Mercury: endogenous and exogenous materials. Endogenous materials constituted the planet soon after its formation and were exposed to the surface by subsequent volcanic eruptions [e.g., Denevi+ 2013]; Exogenous materials are those originally constituted the impactors and were brought to Mercury by late accretion. Thus, understanding chemical compositions requires a comparison with geological backgrounds that reflects the volcanic and impact history. However, a huge gap in spatial resolutions between chemical and geological data makes a detailed comparison difficult [Peplowski+ 2012; Nittler+ 2020]. This study aims to determine the chemical unit classification in the spatial resolution comparable to the geological data using multivariate analyses. We analyzed major element ratios (Mg, Al, S, Ca, and Fe abundances normalized by Si abundance) acquired by MESSENGER/XRS using the k-means clustering method and principal component analysis. The yielded cluster boundaries and PC1 are dominated by Mg/Si ratio, indicating that the chemical heterogeneity on the surface of Mercury is almost described by the variation of the Mg/Si ratio.The chemical compositions of >3 compositional clusters cannot be reproduced by a linear mixture only of 2 end-member components, which suggests that chemical composition mainly characterized by Mg/Si has the potential to discriminate >3 different lithologies. Additionally, the relationship between Mg/Si ratio and the crater number densities on the surface, which reflect the resurfacing age, implies the link between the chemical variation of surface material and the temporal variation of the degree of partial melting in the mantle.


PS24-A011
Reestimate Mercury's Dipole Moment by Employing a New Technique

Zhaojin RONG1#+, Zhen SHI2
1Institute of Geology and Geophysics, Chinese Academy of Sciences, 2Chinese Academy of Sciences

The early surveys of Mercury 10 showed that Mercury should have a global dipole magnetic field. The global dipole field is not confirmed until the arrival of MESSENGER spacecraft. MESSENGER into orbit around Mercury in 2011, and operate successively for four years. Using the magnetometer data of Mercury 10 and MESSENGER, many researchers estimate the dipole moment with different methods, and the yielded moments are volatile. Based on some assumptions and complicated data processes, such as analyzing the deviation position of the magnetic tail current plate near Mercury and deducting the magnetic field outside the magnetosphere model, the current acceptable knowledge demonstrates that the global magnetic dipole moment of Mercury is 195 nT*RM^-3, the dipole Angle is less than 3°, and the dipole center is shifted 480km to the north. Here, being different from previous studies, we use a state-of-art method to diagnose the Mercury’s dipolar field which is assumed to originate from a magnetic dipole. This method can effectively separate and solve the dipole parameters (six parameters with three dipole center, two dipole axis, and one dipole moment), and gives the error of how much the dataset of sampled magnetic field deviated from the dipole field. By employing this method and the MESSENGER field data, the dipole parameters are derived and compared at different altitudes, latitudes and local times. The derived results are compared and discussed with previous results.


PS24-A008
The Relation Between the Surface Composition Anomaly and Distribution of the Exosphere of Mercury

Yudai SUZUKI1#+, Kazuo YOSHIOKA2, Go MURAKAMI1, Ichiro YOSHIKAWA2
1Japan Aerospace Exploration Agency, 2The University of Tokyo

In celestial bodies with tenuous collisionless atmospheres, such as Mercury, the spatial distributions of exospheteres are expected to reflect surface compositions. In this study, we discuss whether the distributions of Mg, Ca, and Na, the primary exospheric components of Mercury, exhibit exosphere-surface correlations by analyzing observational data of the Mercury Atmospheric and Surface Composition Spectrometer (MASCS) and X-Ray Spectrometer (XRS) onboard the MErcury Surface, Space ENvironment, GEochemistry, and Ranging (MESSENGER) spacecraft. It was found that Mg has a strong exosphere-surface correlation and Ca has a weak one. The Monte Carlo simulations of their trajectories in the exosphere show that the weak correlation of Ca is due to the relatively large solar radiation acceleration. In addition, Na production rate in the high-temperature regions is longitudinally dependent. This can be explained by considering that the weakly physisorbed Na layer on the surface is depleted under high temperature and that the distribution of strongly chemisorbed Na atoms is reflected in the exosphere. Based on these results, the conditions for components with a correlation in celestial bodies with thin atmospheres may include low volatility and low solar radiation acceleration. 


PS24-A010 | Invited
The UV Reflectance of Mercury Measured by BepiColombo/PHEBUS

Jean-Yves CHAUFRAY1#+, Eric QUEMERAIS1, Dimitra KOUTROUMPA1, Rozenn ROBIDEL1, Francois LEBLANC2, Aurélie REBERAC1
1Laboratoire Atmosphères, Milieux, Observations Spatiales, 2National Centre for Scientific Research

Probing the Hermean Exosphere By Ultraviolet Spectroscopy (PHEBUS) is an ultraviolet spectrograph on board the Mercury Planetary Orbiter (MPO) of the BepiColombo mission. The main goal of the instrument is to measure the exosphere of Mercury and the albedo of the surface of the permanently shaded regions near the poles. BepiColombo will be inserted around Mercury in December 2025, but during the cruise phase, several opportunities to observe the illuminated surface of Mercury are possible. Such opportunities are important since these observations will not be possible during the nominal science phase when the spacecraft is close to Mercury. The first observation of the illuminated surface of Mercury by PHEBUS with the EUV detector (55 – 155 nm) was done on 10 Oct 2021 few days after the first flyby from a distance of 0.03 AU at a phase angle of 72°. The solar reflected spectrum is detected from ~80 nm to 160 nm and the geometric albedo is lower than the lunar’s albedo by a factor of 0.5- 0.6 in agreement with the observations done by Mariner 10. This difference will be interpreted in light of the more recent findings from MESSENGER.


PS24-A006
UCSD Analysis of the Large-scale BepiColombo Plasma Environment Throughout the Spacecraft Cruise Phase Using ISEE IPS Data

Matthew BRACAMONTES1#, Bernard JACKSON1+, Andrew BUFFINGTON1, Munetoshi TOKUMARU2, Kazumasa IWAI2, Ken'ichi FUJIKI2, Go MURAKAMI3, Daniel HEYNER4, Beatriz SANCHEZ-CANO5, Mathias ROJO6, Sae AIZAWA7, Nicolas ANDRE8, Alain BARTHE6, Emmanuel PENOU9, Andrey FEDOROV8, Jean-Andre SAUVAUD6, Shoichiro YOKOTA10, Yoshifumi SAITO11
1University of California San Diego, 2Nagoya University, 3Japan Aerospace Exploration Agency, 4Institute of Geophysics and Extraterrestrial Physics, 5University of Leicester, 6Institute for Research in Astrophysics and Planetology, 7Laboratoire de Physique des Plasmas, 8University of Toulouse, 9Institute for Research in Astrophysics and Planetology (IRAP), National Center for Scientific Research (CNRS) - University of Toulouse (UPS) - National Center for Space Studies (CNES), 10Osaka University, 11Institute of Space and Astronautical Science / Japan Aerospace Exploration Agency

Remotely-sensed interplanetary scintillation (IPS) from the Institute for Space-Earth Environmental Research (ISEE), Japan, allows a determination of solar wind parameters at BepiColombo as it moves on its orbit in the inner heliosphere. We show several examples of these analyses that certify the validity of the 3-D analysis technique developed from the ISEE data sets. The analyses are used not only to forecast plasma velocity, density, and component magnetic fields at BepiColombo, but can even more effectively return these large scale solar wind parameters from archived data. We show several time period examples of corotating structure and CME analyses. During March, 2022, BepiColombo at half the distance of Earth, was aligned with the STEREO A spacecraft, and later with Earth, and mapped both corotating structure and CMEs during a period of high solar activity. Several CMEs were measured in the ESA MPO/MAG instrument, and also by the JAXA Mio MEA instrument that was situated beneath the spacecraft protective Sun-shroud covering. Two of these CMEs were seen as depressions of high energy particles in the JAXA Mio MPE/SPM instrument that were viewed shortly later as Forbush decreases in neutron monitors at Earth. These observations map well with STEREO A, near-Earth spacecraft, and Solar Orbiter measurements. Our analyses also show the location of nearby heliospheric propagation paths associated with Solar Energetic Particle propagation and the CME structure that provides high-energy particle mitigation for the BepiColombo-observed Forbush decreases that occur during this interval.


Mon-31 Jul | 1:10 - 3:10 | MR334
PS01 - Planetary Space Weathers: Fundamental Plasma Interactions in Space Environments

Session Chair(s): William DUNN, University College London

PS01-A023 | Invited
Contribution of Bepicolombo to Planetary Space Weather: Overview of Interplanetary Cruise and Planetary 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 during the interplanetary cruise phase, the BepiColombo mission can contribute to the heliospheric physics and planetary space weather in the inner solar system. We have performed several science observation campaigns with other missions and successfully obtained science data during cruise. These multi spacecraft observations provide us great opportunities to investigate the inner heliosphere. In addition we have performed science observations during two Venus flybys (in October 2020 and August 2021) and two Mercury flybys (in October 2021 and June 2022). The third Mercury flyby is planned on 20 June 2023. Here we present the updated status of BepiColombo mission, initial results of the science observations during the interplanetary cruise and planetary flybys, and the upcoming observation plans.


PS01-A012
A New Tool for Understanding Solar Wind-Venus Interaction: 3D Multi-fluid MHD Model

Tong DANG1#+, Binzheng ZHANG2, Maodong YAN1, John LYON3, Zhonghua YAO2, Sudong XIAO4, Tielong ZHANG5,1, Jiuhou LEI1
1University of Science and Technology of China, 2The University of Hong Kong, 3Dartmouth College, 4Harbin Institute of Technology, Shenzhen, 5Austrian Academy of Sciences

As the sister planet of the Earth, Venus is a hot and dry planet and lacks an intrinsic magnetic field. Here we present a new global multifluid MHD model for the interaction of the solar wind with Venus. The continuity, momentum, energy equation for H+, O+, O2+, and CO2+ are solved self-consistently together with the Faraday's law. The photochemistry of ionospheric ions are considered as the source term in the density, momentum, and energy equations for each ion. We found that the simulated ionospheric density and temperature and the bow shock location are consistent with previous observations and simulations, for both solar maximum and minimum. The simulated magnetic fields are also consistent with the Venus Express observations. Meanwhile, the high resolving power and low numerical diffusion makes model have the capability of capturing the fine structures of the Venusian induced magnetosphere, such as the Kelvin-Helmholtz instability and the nightside wake. The escape rate has also been estimated and the results are similar to previously estimations. The high-resolution model could be an efficient tool for the exploration of the fine structures of the Venusian space environment system, and also for the application to other unmagnetized planets.


PS01-A032
Gamma-ray Burst, GRB221009A, Detected by the Danuri Gamma-ray Spectrometer in Deep Space

Kyeong Ja KIM1#+, Suyeon KIM1, Yire CHOI1, Junghun PARK1, Yong-Kwon KIM2, Kilsoon PARK2, K.B. LEE3
1Korea Institute of Geoscience and Mineral Resources, 2NuCare, 3Korea Research Institute of Standards and Science

The KPLO orbiter (Danuri) was launched by a SpaceX Falcon 9 rocket from Cape Canaveral Space Force Station on August 5, 2022(KST). The Danuri orbiter includes a gamma-ray spectrometer (KPLO Gamma-Ray Spectrometer, KGRS) as one of six scientific instruments. The KPLO’s lunar trajectory is a low-energy, fuel-efficient ballistic lunar transfer (BLT) trajectory. The KPLO has arrived to lunar orbit of an altitude of 100 km on December 27, 2022. During the cruise period of 4 months and 3 weeks, The KGRS was monitoring both gamma-ray burst and background as scientific objectives in deep space. The KGRS detected a strongest gamma-ray burst on October 9, 2022 called as GRB221009A at a distance of 1,510,000 km from the Earth. The gamma-ray intensity of GRB221009A was as high as 98 time from the background level although it is different in energy interval settings. The KGRS’s GRB221009A signal is well compared with other publicly reported gamma-ray monitoring data. There were a number of gamma-ray burst during the cruise period detected by KGRS. Also, two long-lasting gamma-ray increasing events, which lasted for few days, monitored by the KGRS in both September and October, 2022. This type event is interesting to compare with solar activities that emit radiations of both X-ray and gamma-rays. However, the latter case should be considered with respect to unwanted data in collection of gamma-rays on the Moon. KGRS is the first gamma-ray spectrometer which is used in deep space. It is important to consider this type of scientific objectives of radiation monitoring during for future planetary missions, especially for a long journey in the solar system. This presentation demonstrates all gamma-ray bursts measured by KGRS during the cruise mission for 4 months and 3 weeks.


PS01-A014
On the Seasonal Variations of the Ion Precipitating Into the Upper Atmosphere of Mars

Xinzhi QIU#+, Yiqun YU
Beihang University

Without a global intrinsic magnetic field, Mars’ planetary ions can be picked up by the solar wind directly. The majority of the pickup ions escape, while some can precipitate into the atmosphere. Using the data obtained by the SWIA instrument onboard MAVEN spacecraft from 2018 to 2021, we calculated precipitating ion fluxes through integration over any ions detected in the SWIA angular bins whose FOVs are within a cone angle of 75∘ along the positive radial direction relative to the center of Mars in order to analyze the seasonal behaviors of the Martian ion precipitation. It is found that from Mars season Ls 0 –180◦ to Mas season Ls 180 –360◦, the response of ion precipitation flux varies with energy. It is also found that the seasonal behaviors of the Martian ion precipitating are related to Solar Zenith Angle (SZA). Additional, crustal magnetic field topology also has its influence.


PS01-A030 | Invited
Recent Advances by Numerical Simulation for Understanding Jovian Aurorae

Binzheng ZHANG1#+, Peter DELAMERE2
1The University of Hong Kong, 2University of Alaska Fairbanks

Both space telescope and in-situ observations have shown that the Jovian aurora exhibits dynamic variations and is largely different from the terrestrial aurora. The understanding of physical processes driving the Jovian aurora has been significantly advanced since Juno arrived at Jupiter, combined with HST. Due to the lack of global observation coverage, numerical simulations based on global magnetohydrodynamics play an important role in facilitating the understanding of the dynamic evolution of the Jovian aurora. In this presentation, we show recent advances on the understanding of physical processes driving various Jovian aurora using global-scale, high-resolution simulations of the interaction between the solar wind and Jovian magnetosphere, including the main emission, auroral injection, dawnstorms and polar emission. These physical understandings may also be applicable to other rotation-dominated systems with complicated magnetospheric topology.


PS01-A019
Hydroxylation of Lunar Soil with Solar Wind

Li Hsia YEO#+
NASA Goddard Space Flight Center

Solar wind, which comprises high energy hydrogen ions, continuously strikes the lunar surface, which is rich in oxygen. This presents an opportunity for hydroxylation - the creation of OH on lunar soil. Both OH and H2O have been detected on the lunar surface, with some variability in abundance throughout the lunar day. It is important to understand how space weathering contributes to the production and proliferation of hydrogen-bearing resources such as water within the lunar environment. O-H bonds show a distinct absorption feature in the infrared (IR) at ~3 µm-1 that can be readily studied. Fourier Transform Infrared (FTIR) Spectroscopy is a fast and accurate way to detect changes in the infrared spectra of lunar soil. Previous studies have examined the changes in IR spectra of amorphous silica and olivine, as well as lunar soil before and after hydrogen irradiation. However, the evolution of the OH band and other IR features has not been studied during hydrogen radiation itself. It is especially important to not expose the samples to terrestrial air, which will contaminate the samples with water. We present FTIR spectra on Apollo-era soil samples obtained simultaneously with high energy hydrogen plasma irradiation, similar to the solar wind. Samples are first prepared by baking under vacuum to drive off any surface water. Samples are also brought through thermal cycling and heated to 400K (lunar dayside maximum temperature) in-situ, and changes in their IR spectra are reported. Comparisons between Apollo samples with different minerology and with a control of crushed SiO2 are also provided. Results show broad but distinct growths in the 3 µm-1 absorption band for lunar samples compared to a sharper peak for SiO2. Since the samples are not exposed to terrestrial water during measurements, the evidence of hydroxylation presented is likely due to hydrogen irradiation.


PS01-A027
Electron Cyclotron Maser Emission with Two Components of Electrons and Saturnian Kilometric Radiation

Hao NING+, Yao CHEN#, Chuanyang LI
Shandong University

Planetary radio emissions, such as Saturnian kilometric radiations (SKRs), are widely attributed to electron cyclotron maser emission (ECME) mechanism. Earlier studies on ECME mainly considered simplified dispersion relations of the extraordinary mode assuming that only one component of electrons (either cold or hot electrons) exist in the plasma. Although the assumption is valid for Auroral Kilometric Radiations (AKRs), both cold and hot electron components have been measured simultaneously in SKR sources by Cassini spacecraft. Combining analysis of plasma kinetic linear theory and particle-in-cell (PIC) simulations, we investigated the dispersion relation and ECME mechanism in plasmas consisting of energetic electrons and a cold component. In such condition the dispersion relation of X mode could be modified, resulting in different results of wave amplification. A new branch of wave mode called “trapped” mode is present around gyrofrequency, which is most unstable, and the fundamental X mode (X1) could not be amplified with the cutoff frequency higher than gyrofrequency. We also performed parametric studies of the density ratio of energetic electrons to total electrons. We found that the X1 emissions could be amplified only if the density ratio is higher than 90%.


Mon-31 Jul | 1:10 - 3:10 | MR335
PS05 - Solar Wind Interaction with Intrinsic Magnetospheres: Simulation and Observations

Session Chair(s): Weijie SUN, University of California, Berkeley, Gangkai POH, NASA Goddard Space Flight Center

PS05-A012 | Invited
Low-energy Plasma Observed by Mercury Plasma Particle Experiment Onboard Mio/BepiColombo During Its Mercury Flybys

Sae AIZAWA1#+, Nicolas ANDRE2, Yoshifumi SAITO3, Jean-Andre SAUVAUD4, Andrey FEDOROV2, Shoichiro YOKOTA5, Alain BARTHE6, Emmanuel PENOU6, Mathias ROJO4, Moa PERSSON7, Wataru MIYAKE8, Go MURAKAMI9
1Laboratoire de Physique des Plasmas, 2University of Toulouse, 3Institute of Space and Astronautical Science / Japan Aerospace Exploration Agency, 4Institute for Research in Astrophysics and Planetology, 5Osaka University, 6Institute for Research in Astrophysics and Planetology (IRAP), National Center for Scientific Research (CNRS) - University of Toulouse (UPS) - National Center for Space Studies (CNES), 7The University of Tokyo, 8Tokai University, 9Japan Aerospace Exploration Agency

BepiColombo was launched in October 2018 and is currently en route to Mercury. Although its orbit insertion is planned for December 2025, BepiColombo will acquire new measurements during planetary flybys. During the cruise phase, the two spacecraft are docked together with Mio being protected behind the MOSIF sun shield. Thus, only partial observations of plasma distribution functions can be obtained by the Mercury Plasma Particle Experiment (MPPE) onboard Mio. Up until now, BepiColombo conducted two Mercury flybys (Oct 2021 and Jun 2022) and simultaneous low-energy plasma observations have been made. These observations provide us a wealth of information that we were not able to obtain in past. In particular, the two Mercury Electron Analyzer (MEA) of MPPE will provide us with new and unique measurements in the range of 5 eV to 3 keV when in solar wind mode and 3 eV to ~ 26 keV when in magnetospheric mode. Mercury Ion Analyzer (MIA) of MPPE will provide us ion measurements in the range of a few tens of eV to 25 keV. We will present the interesting observations obtained by MEA and MIA onboard Mio/BepiColombo during its Mercury flybys, and we will focus on the properties of the low-energy ion populations and high-energy electron populations observed during its crossing of Mercury’s magnetosphere.


PS05-A002
Natural Orthogonal Component Analysis of Daily Magnetic Variations at the Martian Surface: Insight Observations

Hao LUO#+
Institute of Geology and Geophysics, Chinese Academy of Sciences

Distinguishing different sources of magnetic field variations at InSight is important to understand dynamic processes in the Martian ionosphere as well as the coupling between the solar wind and the Martian induced magnetosphere. Recent studies based on magnetic field measurements from InSight have suggested that the daily and seasonal variations in the magnetic field at the Martian surface are at least partially the result of neutral wind-driven ionospheric dynamo currents and their seasonal variations. However, the sources of the daily variations with different time scales need be further investigated. In this paper, magnetic field variations in a sol as well as during nearly a whole Martian year from InSight observations were decomposed into their natural orthogonal components (NOC). We found that the first eigenmode shows the previously-identified early- to mid- morning peak, and varies with season. This corresponds to the solar quiet variations. The second and higher eigenmodes manifest the quasi-Carrington and sub-Carrington rotation periodicity represent disturbed components that may be stimulated by variations in the draped interplanetary magnetic field (IMF) and/or the Martian ionospheric electron density. Different from their counterparts at the Earth, the amplitude of the first eigenmode is comparable with the sum of second to fifth ones, showing that the quiet and disturbed diurnal variations contribute similarly to the total diurnal variation. Decomposition of Martian surface magnetic field variations could provide monitoring of the Martian ionospheric current system as well as the solar wind conditions in the near-Mars space, which will be greatly enhanced when combined with Zhurong Martian surface field measurements in the future.


PS05-A004
Enhanced Ion Escape Rate During IMF Rotation Under Weak Intrinsic Magnetic Field Conditions on a Mars-like Planet

Shotaro SAKAI1#+, Kanako SEKI2, Naoki TERADA1, Hiroyuki SHINAGAWA3, Ryoya SAKATA2, Takashi TANAKA4, Yusuke EBIHARA5
1Tohoku University, 2The University of Tokyo, 3National Institute of Information and Communications Technology, 4Kyushu University, 5Kyoto University

Magnetized planets are affected by the orientation of the interplanetary magnetic field (IMF) in terms of its interaction with the solar wind. The IMF rotation particularly provides details of the escape mechanism that varies with the interaction between the intrinsic magnetic field and the IMF. A multispecies magnetohydrodynamic simulation is conducted on a Mars-like planet under the conditions of a weak intrinsic magnetic field and the IMF rotating by 180˚ over twelve hours, which is comparable to the CME time scale. The total ion escape rate increases from ~5 × 1023 s-1 to ~3 × 1025 s-1 during the IMF rotation from due north (parallel to the assumed intrinsic magnetic field) to due south (antiparallel to the assumed intrinsic magnetic field). The escape rate increases significantly with the IMF rotating from due north to clock angles of 45˚ – 75˚, followed by a gentle increase until the IMF rotates to due south. The trigger for the large increase is multiple reconnections in the magnetospheric flank region, and the subsequent increase is due to the expansion of the reconnection area into the equatorial region. The IMF mass loading in the ionosphere is also responsible for the gentle increase with IMF clock angles above 90˚ in addition to the flank reconnection. The IMF rotation is a general feature for a coronal mass ejection (CME). Exoplanets orbiting in the vicinity of M-dwarfs might be frequently affected by IMF rotation, as they could be exposed to severe stellar winds such as in CME environments, and the current study could be helpful for future planned observations of the exoplanetary environment.


PS05-A009 | Invited
Magnetic Reconnection at Planetary Magnetopauses: Observations at Earth and at Saturn

Stephen FUSELIER1#+, Steven PETRINEC2, Karlheinz TRATTNER3
1Southwest Research Institute, 2Lockheed Martin Advanced Technology Center, 3University of Colorado Boulder

When the Interplanetary Magnetic Field (IMF) is southward, magnetic reconnection produces long X-lines at the Earth’s magnetopause. These primary X-lines are quasi-steady in space and time for quasi-steady upstream solar wind conditions. The location, length, and orientation of these X-lines is well-described by an empirical model called the maximum magnetic shear model. There is strong evidence that a similar model is applicable at Saturn’s magnetopause despite the differences in the solar wind in the outer and inner heliosphere and despite the differences in the sizes of the two magnetospheres. In addition to the primary X-line at the Earth’s magnetopause, magnetic reconnection produces secondary X-lines that are not quasi-steady in space or time. This talk reviews the model-observation comparison at Earth and Saturn and discusses the evidence for secondary X-lines at the two planets.


PS05-A001 | Invited
Jupiter’s Low-altitude Auroral Zones: Fields, Particles, Plasma Waves, and Density Depletions

Ali SULAIMAN1#+, Barry MAUK2, Jamey SZALAY3, Frederic ALLEGRINI4,5, George CLARK2, Randy GLADSTONE4, Stavros KOTSIAROS6, William KURTH7, Fran BAGENAL8, Bertrand BONFOND9, J. E. P. CONNERNEY10,11, Robert EBERT4, George HOSPODARSKY7, Vincent HUE4, Daniel GERSHMAN11, Robert LYSAK1, Sadie ELLIOTT1, Ondrej SANTOLIK12,13, Joachim SAUR14, Scott BOLTON4
1University of Minnesota, 2Johns Hopkins University Applied Physics Laboratory, 3Princeton University, 4Southwest Research Institute, 5University of Texas at San Antonio, 6Technical University of Denmark, 7The University of Iowa, 8University of Colorado, Boulder, 9University of Liege, 10Space Research Corporation, 11NASA Goddard Space Flight Center, 12Czech Academy of Sciences, 13Charles University, 14University of Cologne

The Juno spacecraft's polar orbits have enabled direct sampling of Jupiter's low-altitude auroral field lines. Jupiter's main aurora has been classified into distinct “zones”, based on repeatable signatures found in energetic electron and proton spectra. We combine fields, particles, and plasma wave data sets to analyze Zone-I and Zone-II, which are suggested to carry upward and downward field-aligned currents, respectively. We find Zone-I to have well-defined boundaries across all data sets. H+ and/or H3+ cyclotron waves are commonly observed in Zone-I in the presence of energetic upward H+ beams and downward energetic electron beams. Zone-II, on the other hand, does not have a clear poleward boundary with the polar cap, and its signatures are more sporadic. Large-amplitude solitary waves, which are reminiscent of those ubiquitous in Earth's downward current region, are a key feature of Zone-II. Alfvénic fluctuations are most prominent in the diffuse aurora and are repeatedly found to diminish in Zone-I and Zone-II, likely due to dissipation, at higher altitudes, to energize auroral electrons. Finally, we identify significant electron density depletions, by up to two orders of magnitude, in Zone-I, and discuss their important implications for the development of parallel potentials, Alfvénic dissipation, and radio wave generation.


PS05-A017
Solar Wind Driving of the Uranian Magnetosphere: Predictions for Global Magnetospheric Convection, Magnetosphere-ionosphere Coupling, and Auroral Activity at Uranus

Drew TURNER#+, Ian COHEN, George CLARK, Peter KOLLMANN, Leonardo REGOLI
Johns Hopkins University Applied Physics Laboratory

We present new results from an investigation of the unique magnetosphere of Uranus and its interaction with the solar wind. We developed and validated a simple yet valuable and illustrative, 3D model of Uranus’ offset, tilted, and rapidly-spinning magnetic field and magnetopause. With this model, we investigated details of the seasonal and interplanetary magnetic field (IMF) orientation dependencies of dayside and flank reconnection along the Uranian magnetopause. We found that anti-parallel (magnetic field shear angle greater than 170-degrees [i.e., Masters, 2014]) reconnection occurs nearly continuously along the Uranian dayside and/or flank magnetopause under all seasons of the 84 (Earth) year Uranian orbit and all of the most likely IMF orientations. We present hypotheses that such active and continuous driving of the Uranian magnetosphere should result in constant loading and unloading of the Uranian magnetotail. We demonstrate that unlike the other magnetospheric systems that are Dungey-cycle driven (i.e., Mercury and Earth) or rotationally driven (Jupiter and Saturn), global magnetospheric convection of plasma, magnetic flux, and energy flow may occur via three distinct cycles, two of which are unique to the Ice Giants: Uranus and Neptune (as we also demonstrate briefly here). Our simple model is also used to map signatures of dayside and flank reconnection down to the Uranian ionosphere, explaining how “spot”-like auroral features should be very common on the Uranian dayside, consistent with observations from Hubble Space Telescope. We have much to learn about Uranus’ unique and intriguing magnetosphere, which might have important analogs to exoplanetary magnetospheric systems. Our hypotheses can be tested with further work involving more advanced models, new auroral observations, and unprecedented missions to explore the in situ environment from orbit around Uranus. Our results highlight why any future mission to orbit Uranus should include a complement of magnetospheric instruments in the payload.


PS05-A003 | Invited
Wave Phenomena Revealing Interaction of Planetary Magnetosphere with Solar Wind

Shengyi YE1#+, Siyuan WU1, Georg FISCHER2, Zhonghua YAO3, William KURTH4, Yuening CHEN1, Binzheng ZHANG5
1Southern University of Science and Technology, 2Austrian Academy of Sciences, 3Chinese Academy of Sciences, 4The University of Iowa, 5The University of Hong Kong

Rapid changes in solar wind conditions perturb the planetary magnetospheres, changing their sizes and properties of the plasma within, providing energy for the generation of radio emissions and plasma waves, revealing the dynamic processes in and around the planetary magnetospheres, e.g. magnetic reconnections and hot plasma injections. The emissions often display periodicities caused by fast planetary rotation and magnetic compression waves induced by solar wind impact, providing valuable information about the coupling process between magnetosphere and ionosphere. 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.


Tue-01 Aug | 8:15 - 10:00 | MR307
PS20 - Surface Science and Exploration of the Moon and Airless Planetary Bodies

Session Chair(s): Tirtha Pratim DAS, Indian Space Research Organisation Headquarters, Benjamin GREENHAGEN, Johns Hopkins University Applied Physics Laboratory

PS20-A003 | Invited
Indian Lunar Exploration Program

Anil BHARDWAJ#+
Physical Research Laboratory

The space program of India started in November 1963 with launch of a rocket from Thumba. More than 4 decades later, the planetary exploration program began in 2008 with the launch of Chandrayaan-1 orbiter mission to the Moon. The Chandrayaan-1 mission made a huge impact in the advancement of lunar science, with many new findings, including discovery of OH/H2O molecules on Moon and presence of lunar Mini-Magnetospheres, and that the Moon is geologically and tectonically an active body. The next Indian lunar mission to Moon is the ongoing Chandrayaan-2 mission; the orbiter is working very well and providing high-quality science data. India will be launching this year the third mission to Moon – the Chandrayaan-3 Lander-Rover mission to study the Moon in-situ. Other missions are being planned for future. This talk will discuss the Indian lunar exploration program, challenges for missions, and briefly highlight the science derived from them.


PS20-A036 | Invited
Lunar Trailblazer: A Pioneering Smallsat for Lunar Water and Lunar Geology

Rachel KLIMA1#+, Bethany EHLMANN2
1Johns Hopkins University Applied Physics Laboratory, 2California Institute of Technology

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 fall 2023. 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).


PS20-A025
Lunar Polar Exploration (LUPEX) Project: Joint Mission by JAXA-ISRO for Searching the Lunar Polar Water

Makiko OHTAKE#+
The University of Aizu

Japan Aerospace Exploration Agency (JAXA) and Indian Space Research Organisation (ISRO) are jointly planning a lunar polar exploration mission, which is named as "Lunar Polar Exploration (LUPEX) ". The spacecraft will be launched by JAXA’s H-3 rocket and JAXA is mainly responsible for developing and operating the rover, and ISRO for developing and operating the lander. We are finalizing the mission instruments selection. Expected instruments are, Resource investigation water analyzer (REIWA), Advanced Lunar Imaging Spectrometer (ALIS), Ground Penetrating Radar (GPR), Mid-infrared Imaging Spectrometer (MIR), Neutron Spectrometer (NS), and Exospheric Mass Spectrometer for LUPEX (EMS-L). REIWA consists of four sub-systems; Lunar Thermogravimetric Analyzer (LTGA), Triple-Reflectance Reflectron (TRITON), Aquatic Detector using Optical Resonance (ADORE), and ISRO’s Sample Analysis Package (ISAP). The rover will conduct direct measurements of the underground water by drilling and picking up regolith samples from different depths up to ~1.5 m. We are in a process for selecting exploration site for the mission. This process consists of selection of sites in three lateral scales; selecting i) landing site within the polar region, ii) way points (detailed exploration area for the rover; one way point roughly correspond to a size of 30 x 30 m), and iii) drilling site within the way points. For discussion of i), we selected ~10 candidates from a perspective of finding a safe, feasible and suitable site for the lander and the rover. For the ii) and iii) selection, we are trying to determine how to evaluate each landing site candidate. And for the evaluation, we are going to use data obtained by previous lunar exploration missions and an ongoing mission (Chyandrayaan-2 orbiter) and derived by estimation of the underground temperature at the exploration sites. Status of the mission planning, designing, discussion of output will be discussed at the meeting.


PS20-A027
Identification of Potential Candidate Landing Areas for ESA’s Prospect Instrument

Sarah BOAZMAN1#+, David HEATHER1, Matt HUTTON1, Marius SCHWINNING1, Nicole SCHMITZ2, Alessandro FRIGERI3, Michelangelo FORMISANO3, Elliot SEFTON-NASH1, Csilla ORGEL1, Christian GSCHEIDLE4, Cristina DESANCTIS3, Tristram WARREN5, Philipp REISS4, Neil BOWLES5, Berengere HOUDOU1
1European Space Agency, 2German Aerospace Centre, 3Institute of Astrophysics and Planetary Science, 4Technical University of Munich, 5University of Oxford

Many upcoming missions including ESA’s PROSPECT instrument are targeting the south polar region of the Moon due to it’s high illumination conditions, important for solar power, and the potential abundance of volatiles beneath the surface. PROSPECT (Package for Resource Observation and inSitu Prospecting for Exploration Commercial exploitation and Transportation) has been selected for flight on the 10th NASA Commercial Lunar Payload services (CLPS) mission. NASA CLPS-10 will be a static lander and contain a range of instruments including PROSPECT which, using the Drill, will sample the lunar surface up to 1 m depth with the aim to detect volatiles including water ice if present. Potential candidate landing sites within the region 84 -90° S have been identified using a range of datasets with GIS software and remote sensing methods. Sites were identified which met the following criteria; slopes of less than 10 °, Earth visibility of > 50%, Illumination of > 30% and had thermal conditions for ice stability between 0-10 cm depth beneath the surface. Where there were 4 pixels or more that met these criteria, a point of interest was placed. Down selection of these points of interest was done using a science matrix, which analyzed whether the science requirements for PROSPECT were met. Four candidate areas were identified which best fulfil the science requirements of PROSPECT; Amundsen crater rim, Cabeus crater rim, north of de Gerlache crater and between Shackleton and Shoemaker crater. These four candidate areas are located near sites of interest within the literature and therefore landing in any of these locations would improve the geological knowledge of the south polar region and test the volatile abundance within these areas, which is of interest for future missions. At AOGS the four candidate sites, including the reasons for the preferred site will be presented. 


PS20-A033
Farside Seismic Suite (FSS): Environmental Testing to Prepare for the Farside of the Moon

Bea CHIKANI1#+, Simon CALCUTT1, Neil BOWLES1, Ian STANDLEY2, William Thomas PIKE3, Mark PANNING4
1University of Oxford, 2Kinemetrics, 3Imperial College London, 4Jet Propulsion Laboratory, California Institute of Technology

The Farside Seismic Suite (FSS), will collect seismic data, the first since the Apollo missions and a first for the farside of the Moon. FSS is a NASA funded project under the Payloads and Research Investigation on the Surface of the Moon (PRISM) and with its planned launch in 2025, it will return data with unprecedented sensitivity over multiple lunar diurnal cycles after outliving the delivery lander. FSS will carry two seismometers to the Schrödinger basin, an impact crater on the farside of the Moon. The seismic data collected will help with understanding the internal structure of the Moon and the differences in the nearside and farside seismic activity. One seismometer is the three component Short Period (SP) seismometer which is based on the MEMS seismometer successfully deployed by the Insight mission to Mars. Our goal is to adapt the Martian design to operate on the Moon, an airless body, and to support the integration, test and calibration of the FSS flight instrument. In particular the SP sensor is investigated and a number of tests are carried out including shock testing, push testing, vibration testing, and thermal vacuum atmosphere chamber (TVAC) testing. These tests are essential in order to understand the harsh environments the instrument can experience as spacecraft are subjected to high frequency shocks and intense vibrations during launch. TVAC testing ensures the instrument can withstand the extreme temperatures and conditions of space. Other testing relating to the FSS project specifically includes noise testing and cross calibration. These environmental tests ensure the physics and dynamics of outer space and the Moon are understood beforehand and therefore allowing a successful mission. We will present our experiments, data and discuss new insights into FSS and lunar seismology.


PS20-A002
Model Derived Lateral Heat Transport for Prospective Sites on the Moon - Implications for the Future Lunar Exploration

G. AMBILY#+, Durga Prasad KARANAM
Physical Research Laboratory

Understanding the thermophysical behaviour of the lunar surface is essential for the prospecting and future exploration on the Moon. Present studies have comprehended this complex behaviour at a global scale. But the role of local relief, such as rocks, hillocks on the surface and sub-surface temperatures, has yet not been addressed completely. If the local relief is large, it could significantly affect the sub-surface temperature and could not be ignored. Along with the topography, the thermophysical behaviour also varies according to the relative position of the Moon with respect to Sun and Earth. Efforts taken so far to understand the surface and sub-surface temperatures are mainly based on low-resolution datasets and one-dimensional models respectively. The variation in lateral heat transport and its implications are often not considered. Comprehending this lateral heat and its variation is necessary for future exploration since it is focused on long-term sustenance on Moon.
How the local relief is affecting the surface and sub-surface temperatures and does it have a significant impact are the two major scientific problems to be addressed. In order to understand these aspects, a comprehensive three-dimensional finite element thermal model of the Moon has been developed and validated. Making some improvements in the present model supported by remote sensing datasets, lateral heat transport of certain potential latitudinally distinct sites on the Moon has been analysed. Results showed a significant variation in lateral heat transport due to local relief and other parameters. Comparative analyses and assessments of these sites for future lunar exploration will be presented and discussed.


Tue-01 Aug | 8:15 - 10:00 | MR334
PS23 - Observational and Theoretical Aspects of Exoplanets

Session Chair(s): Ing-Guey JIANG, National Tsing Hua University

PS23-A029 | Invited
The Never-ending Story of Giant Planets

Sharon Xuesong WANG#+
Tsinghua University

Giant planets like hot Jupiters are the easiest planets to find, which is why they are the first population of exoplanets ever discovered. Three decades later, we now know over a thousand giant planets. However, there are still numerous mysteries around their formation, evolution, and their impact on their natal planetary systems. In this talk, I will introduce our recent research on how special samples of giants would shed light on some of the clues in their formation and evolutionary processes.


PS23-A003
From Pebbles to Exoplanets

Beibei LIU#+
Zhejiang University

Our understanding of the planet formation has been rapidly evolving in recent years. The classical planet formation theory, developed based on our own Solar System, has been revised to account for the observed diversity of the exoplanetary systems. We present the new developments in planet formation theory. A significant fraction of solids is not growing past the pebble-sizes in young protoplanetary disks. The reservoir of pebbles plays an important role in the growth of planetary cores from pebble accretion. The characteristic mass of super-Earth is set by the pebble isolation process. Super-Earth masses increase linearly with the mass of its stellar host, which corresponds to one Earth mass around late M-dwarf stars and 20 Earth masses around solar-mass stars. Pebble-driven planet formation models succeeds in quantitatively reproducing several important observed properties of exoplanets and correlations with their stellar hosts.


PS23-A001
The Formation of Misaligned Planets in and Around Binary Star Systems

Jeremy SMALLWOOD#+
Academia Sinica

The majority of stars born in dense stellar clusters are part of binary star systems. Circumbinary discs of gas and dust commonly surround binary star systems and are responsible for accreting material onto the binary. The gas flow dynamics from the circumbinary disc onto the binary components have significant implications for planet formation scenarios in binary systems. Misalignments between the circumbinary disc and the binary orbital plane are commonly observed. A misaligned circumbinary disc undergoes nodal precession. For a low initial inclination, the precession is around the binary angular momentum vector, while for a sufficiently high initial inclination, the precession is around the eccentricity vector. Dissipation causes the disc to evolve to align coplanar to the binary orbital plane or perpendicular (i.e., polar) to the binary orbital plane. I present 3-dimensional hydrodynamical simulations and linear theory on the evolution of highly misaligned circumbinary discs. I show that polar-aligned circumbinary discs are favorable environments for forming polar circumbinary (P-type) planets. Moreover, misaligned and polar circumbinary material flows around each binary component, forming misaligned and polar circumstellar discs. These circumstellar discs undergo long-lived Kozai-Lidov oscillations that may prompt the formation of giant circumstellar (S-type) planets in binary star systems. The evolution of protoplanetary discs in and around binary star systems bears important implications for planet formation.


PS23-A028
Formation of Inner Planets in the Presence of an Early-formed Cold Jupiter

Kangrou GUO1#+, Eiichiro KOKUBO2
1Shanghai Jiao Tong University, 2National Astronomical Observatory of Japan

We investigate the scenario where a population of planetesimals in the inner disk region evolves under the coupled effect of perturbations by an external giant planet and gas drag. In particular, we focus on the alignment of orbits and the relative velocities of planetesimals to examine the likelihood of the formation of planetary embryos in the inner disk. The mass and eccentricity of the perturbing planet (embryo) is varied in order to explore the dependence of the planetesimal relative velocities on these two parameters. While the gas drag introduces a size-dependent phasing (alignment) of orbits and keeps the relative velocity low for similar-size bodies, it prevents orbital alignment for different-size planetesimals. For the fiducial model in which the planet resembles Jupiter, the relative velocities of identical-size planetesimals are on the order of 1 m/s near 1 au and 10 m/s near 2.6 au, which are consistent with the results in previous studies. Regardless of the semi-major axis and the planetesimal mass ratio, the increase in the mass and the eccentricity of the existing planet always lead to higher relative velocities of planetesimals, which makes the inner disk more hostile for planet formation. We are currently working on the latest updates where we consider planetesimals of sizes on the order of 100 km (as predicted by the streaming instability model) and implement the inter-particle gravitational interaction, which was usually neglected in previous studies due to high computational cost. We also consider the preferred location for planetesimal formation by initially distributing the planetesimals in a ring where a pressure bump might act as a trap for dust. 


PS23-A030
Early Planet Formation via Fragmentation of Magnetised Protoplanetary Disks

Hongping DENG#+
Shanghai Astronomical Observatory

Protoplanetary discs as young as 0.5 Myr bear gaps and rings, arguable signposts of protoplanets. The evolution of young discs is crucial to our understanding of planet formation, and here we report on some unprecedented high-resolution simulations (up to 70M particles) of young discs. In the early stages, the disc is unstable due to gas self-gravity and spiral density waves feature. Spirals can drive large-scale vertical circulations and amplify any seed magnetic fields to nearly thermal amplitudes. This dynamo is vigorous even in poorly ionized regions of the protoplanetary disc. If the spiral collapses due to efficient cooling, the magnetic fields will wrap up the fragment and effectively isolate the fragment from the turbulent disc. We found fragments as light as Neptune survive in discs thanks to the protection of magnetic fields. They may later capture solids in their cores, and thus a rapid top-down formation is possible for major types of planets.


PS23-A027
Formation of Exoplanetary Systems in an Evolving Disk with Disk Winds and Photoevaporation

Masahiro OGIHARA1#+, Yasunori HORI2, Masanobu KUNITOMO3, Kenji KUROSAKI4, Eiichiro KOKUBO5, Takeru SUZUKI6, Alessandro MORBIDELLI7
1Shanghai Jiao Tong University, 2Astrobiology Center, 3Kurume University, 4Kobe University, 5National Astronomical Observatory of Japan, 6The University of Tokyo, 7Observatoire de la Cote d'Azur

Models of protoplanetary disk evolution have been proposed that take into account the effects of magnetically driven disk winds and photoevaporation. We investigate the formation of exoplanetary systems in such a protoplanetary disk model using N-body simulations. The direction and speed of type I migration change when the distribution of the disk gas surface density changes due to disk winds. When the type I migration is suppressed, many super-Earth cores form outside the inner disk edge of the protoplanetary disk and are captured in mean-motion resonances. The system then undergoes orbital instability as the disk dissipates, and the resulting super-Earths are found to deviate from the mean-motion resonance. We also find that the super-Earth core can avoid accreting a large amount of atmosphere from the disk, which rapidly dissipates due to photoevaporation. The super-Earth system formed in our simulation is consistent with some features of observed super-Earth systems. In addition, disks that dissipate rapidly due to photoevaporation also prevent hot and warm Jupiters from accreting a large envelope, leading to the reproduction of features of observed hot and warm Jupiters with large metal mass fractions.


Tue-01 Aug | 10:20 - 12:20 | MR305
PS04 - Aeronomy and Plasma Physics of Planetary Environments

Session Chair(s): Yuki HARADA, Kyoto University, Shaosui XU, University of California, Berkeley

PS04-A010 | Invited
Stellar Winds and Atmospheric Escape: Lessons from a Half-century of Ion Measurements at Venus, Earth, and Mars

Robin RAMSTAD#+
University of Colorado Boulder

The number of discovered exoplanets increases steadily, along with the emerging ability to characterize exoplanetary atmospheres. Before long, we will face the challenge of explaining the diversity of atmospheres on these otherwise inaccessible worlds. The task is daunting, considering that the atmospheric evolution of planets in our own solar system is not well-determined; in particular what is the cause for the widely divergent atmospheric evolution of Venus, Earth, and Mars? Atmospheric loss driven by solar activity is one of the least understood processes affecting atmospheric evolution, as well as the roles of gravity and intrinsic magnetic fields. In this talk, we will provide a nuanced understanding of atmospheric escape from an overview spanning 50 years of studies of the solar system terrestrial planets, focusing on atmospheric ion escape. We will examine how atmospheric escape rates are affected by solar conditions and planetary properties, with implications not only for the evolution of planets in the solar system, but also for what we may expect to find beyond.


PS04-A014
Solar Wind Interaction with Venus: From the Planetary Interior to Interplanetary Space

Chuanfei DONG1#+, Yuxi CHEN2, Janet LUHMANN3
1Boston University, 2Princeton University, 3University of California, Berkeley

Unlike Earth, Venus has no intrinsic dipole magnetic field and thus serves as the prototype of the solar wind interaction with unmagnetized planets. Venus Express (VEX) observations confirmed the complexity of the induced Venusian magnetosphere, especially given the observed magnetic reconnection in the near Venusian magnetotail. On the other hand, penetration of the interplanetary magnetic field (IMF) into an insulating crust is routinely seen at the Moon but the ionosphere of Venus presents an induced field barrier whose ability to shield the body varies with external plasma and field conditions. We expect Venus to be influenced by penetrating IMF in certain circumstances, and explore the observational and physical consequences. We study the solar wind interaction with Venus, for the first time, by incorporating the planetary interior, i.e., an electrically conductive core and a resistive mantle, in a fully self-consistent manner. We mainly focus on the influence of the coupled planetary interior on the Venusian magnetic topologies under varying solar wind conditions. This new model is capable of revealing how external IMF propagates from interplanetary space to satellite altitudes and all the way down to the surface and planetary interior in a self-consistent way, and thus allows us to investigate the transition to more moon-like plasma interactions.


PS04-A008
A New Magnetosphere-ionosphere Current System Observed on Mars

Jiawei GAO1#+, Zhaojin RONG2, Yong WEI2, Haoyu LYU3
1Chinese Academy of Sciences, 2Institute of Geology and Geophysics, Chinese Academy of Sciences, 3Beihang University

Magnetic field and currents in the Martian space environment controls the movement of the planetary particles, and thus play an essential role for understanding Martian atmospheric escape processes and climate history. It’s well known that an induced magnetosphere is formed as a result of the interaction between solar wind and non-magnetized planet. Previous works identified two current systems in the induced magnetosphere, that is, the ionospheric current system and the magnetotail current system. However, these two current systems cannot explain the hemisphere asymmetry of magnetic field as well as the sunward and tailward currents observed in the magnetosphere. Here, we investigated the magnetic field and currents distribution in the Martian ionosphere using Mars Atmosphere and Volatile EvolutioN (MAVEN) data. We found another current system, coupling both magnetosphere and ionosphere, which have tailward component in the low altitude of ionosphere and sunward component in the high altitude of ionosphere. We proposed that the physical mechanism of the new current system is the collision between solar wind and planetary plasma, and then validated by a global multi-fluid magnetohydrodynamic (MHD) simulation. Our results suggested that this current system is most likely a universal phenomenon for a non-magnetized planetary with ionospheres interacted with high-speed plasma.


PS04-A003
Global MAVEN Distribution of Kelvin-Helmholtz Vortices from a Machine Learning and Statistical Approach

Ze-Wen KOH1,2#+, Gangkai POH3,2, Christopher FOWLER4, Jacob GRUESBECK3, Dona KURUPPUARATCHI3, Gina DI BRACCIO3, Jared ESPLEY3
1Cornell University, 2Catholic University of America, 3NASA Goddard Space Flight Center, 4West Virginia University

The Kelvin-Helmholtz (K-H) instability is driven at velocity shear boundaries, and can occur at the interaction between solar wind and non-magnetized planets. While K-H vortices have previously been observed in Mars Atmosphere and Volatile EvolutioN (MAVEN) measurements along Mars' induced magnetospheric boundary (IMB), their properties and distribution remain unknown, and their role in Mars’ atmospheric loss poorly constrained. To this end, we surveyed MAVEN magnetic field (MAG) and plasma measurements (SWEA, SWIA, STATIC) for K-H vortices based on key characteristics including quasi-periodic sawtooth magnetic field perturbations and the co-existence of magnetosheath protons with planetary ions. Using minimum variance analysis on the sawtooth signature, we confirmed that the hodograms were indicative of boundary crossings and not flux ropes. Additionally, we trained a recurrent neural network to identify instances of the IMB for a candidate-flagging pipeline. From our survey of ~1 year of MAVEN data, we found six intervals of K-H vortices observed at solar zenith angles between 70° to 135°. The K-H vortices have peak-to-peak amplitude and periods ranging from 5 to 25 nT and 0.5 to 3.5 minutes, respectively. Using previous estimates that K-H vortices travel at a mean deHoffmann–Teller velocity of 175 km, the characteristic K-H wavelengths varied between 7,000 to 35,000 km. We further correlated the events with solar wind conditions to determine the K-H instability onset conditions and vortex growth. Overall, we concluded that the K-H vortices comprised a global distribution in both hemispheres and at varying longitudes. By estimating the linear growth rate and mass flux of ionospheric ions within each vortex, we were able to improve constraints on Mars’ atmospheric loss from detached plasma clouds caused by K-H instability. These findings can be used for the future synthesis of modelling parameters to better understand the formation and evolution of K-H vortices.


PS04-A013
Species-dependent Response of the Martian Ionosphere to the 2018 Global Dust Event

Dandan NIU1+, Jun CUI2,3#, Shiqi WU2, Hao GU2, Yutian CAO2, Zhaopeng WU2, Xiaoshu WU2, Jiahao ZHONG2, Ming-Yu WU4, Yong WEI5, Tielong ZHANG6,7
1NANJING UNIVERSITY, 2Sun Yat-sen University, 3Chinese Academy of Sciences, 4Harbin Institute of Technology, 5Institute of Geology and Geophysics, Chinese Academy of Sciences, 6Austrian Academy of Sciences, 7University of Science and Technology of China

Global dust storms (GDS) are an important dynamical phenomenon of the Martian lower atmosphere but are known to have important impacts on the Martian middle/upper atmosphere and ionosphere. Despite extensive studies over the past several decades, how the composition of the Martian ionosphere is modified during the GDS has only been studied from a theoretical point of view. Here we present for the first time the observations of the compositional variation of the Martian ionosphere during the GDS in 2018, using the ion density measurements made by the Neutral Gas and Ion Mass Spectrometer onboard the Mars Atmosphere and Volatile Evolution. At a representative altitude of 170 km, the variations of ionospheric species during the GDS show either enhancement (CO2+, Ar+, HO2+, H2O+, H2+, ArH+) or depletion (O2+, O+, N2+/CO+, OH+). Despite the apparent diversity, the observations are mostly understandable within the established framework of ionospheric chemistry on Mars, which further demonstrates that the variation of ion species during the GDS is a good diagnostic of the variation of relevant neutral species in the thermosphere. In particular, the observed ionospheric variation strongly supports a scenario that H2O is substantially enhanced in the Martian thermosphere during the GDS. However, the variations of O2+ and H2+ are inconsistent with predictions from ionospheric chemistry and require further investigation.


PS04-A005
Solar Wind Energetic Neutral Atom Observation at Mars by MINPA Onboard the Tianwen-1 Orbiter

Wenya LI#+, Linggao KONG, Jijie MA
Chinese Academy of Sciences

The Mars Ion and Neutral Particle Analyzer (MINPA), one of the seven scientific payloads onboard the Tianwen-1 orbiter, was designed to measure ions and energetic neutral atoms (ENAs) at Mars. From November 2021, MINPA started to collect scientific data around Mars. Here, we present MINPA's first results of the solar-wind ENAs, which are produced through the charge exchange process between the solar-wind hydrogen ions and the Martian neutral exosphere. We perform a comprehensive comparison between the inflight ENA data and ground calibration results to understand the energy and angular distributions of the solar-wind ENA signals. The possible contamination of these observations by ions and solar extreme ultraviolet (EUV) is evaluated by comparing the ENA measurements with the ion data. We will present several cases of solar wind ENA observations. Their intensities are estimated to be 105~106 cm-2 sr-1 s-1, which agrees with previous in situ measurements and predictions using models.


PS04-A001 | Invited
Multipoint Observation of the Solar Wind Interaction with Strong Lunar Magnetic Anomalies by Artemis Spacecraft and Chang’E-4 Rover

Lianghai XIE1#+, Lei LI2
1National Space Science Center, Chinese Academy of Sciences, 2Chinese Academy of Sciences

A shock or a mini-magnetosphere was once thought to be formed by the solar wind interaction with strong lunar magnetic anomalies. However, the full structure of a mini-magnetosphere has never been verified and whether a mini-magnetosphere can be completely formed remains a controversy. In this work, we present a unique multipoint observation of such an interaction by the ARTEMIS spacecraft and the Chang’E-4 rover. Both solar wind deceleration and penetration are observed by the Chang’E-4 rover on the lunar surface near the magnetic anomaly. Meanwhile, a shock is observed by the ARTEMIS spacecraft downstream from the magnetic anomaly. It is suggested that the magnetic anomaly cannot stand off the solar wind, and there is no bow shock but just a boundary layer near the magnetic anomaly. Accordingly, a mini-magnetosphere is not completely formed and the downstream shock observed the ARTEMIS spacecraft just corresponds to a trailing shock.


Tue-01 Aug | 10:20 - 12:20 | MR307
PS20 - Surface Science and Exploration of the Moon and Airless Planetary Bodies

Session Chair(s): Anil BHARDWAJ, Physical Research Laboratory, Kyeong Ja KIM, Korea Institute of Geoscience and Mineral Resources

PS20-A013 | Invited
Chandrayaan-2: Science Outcome and Accomplishments

Megala S#, Tirtha Pratim DAS+
Indian Space Research Organisation Headquarters

Chandrayaan-2, the second Indian mission to the Moon was launched on 22nd July 2019. Though the soft-landing attempt could not be accomplished as planned, the mission life of Orbiter is extended to 7 years. The Orbiter completed three and half years around the Moon at 100km and all the payloads are operational. The suite of instruments on Chandrayaan-2 are providing a wealth of data to address several important questions in lunar science. The Imaging IR spectrometer on Chandrayaan-2 was specifically designed to resolve the ambiguity in the signature of the 3-micron hydration feature used to detect wide spread presence of water-ice, first reported by our Chandrayaan-1 mission. Using the extended detection wavelength of upto 5 microns, IIRS observations showed the unambiguous detection of Lunar hydration absorption feature around 3 μm at all latitudes and surface types. Characterisation of noble gas dynamics in the sunlit lunar exosphere is done by the mass spectrometer by global mapping of Argon-40 that originate from radioactive Potassium-40 from lunar interior. Dual frequency SAR is providing full polarimetric measurements to image permanently shadowed regions and to identify water-ice deposits in the polar regions. The X-ray spectrometer on the Orbiter has mapped the abundance of sodium on the Moon for the very first time. In addition, minor elements such as Chromium and Manganese were detected due to high sensitivity of the instrument. When the Moon enters the geotail once a month, enhancement in particle environment is observed. The solar X-ray monitor has detected large number of microflares occurring outside the Sun’s active region which may provide clues to the coronal heating problem. The scientific data are made available to public. Significant results from Chandrayaan-2 payloads and their value addition to lunar scientific knowledge will be discussed in this paper.


PS20-A028 | Invited
Introduction to the First Results of KPLO Gamma-ray Spectrometer on the Moon

Kyeong Ja KIM1#+, Suyeon KIM1, Yire CHOI1, Junghun PARK1, Yong-Kwon KIM2, Kilsoon PARK2, K.B. LEE3
1Korea Institute of Geoscience and Mineral Resources, 2NuCare, 3Korea Research Institute of Standards and Science

The gamma-ray spectrometer onboard the Korean Pathfinder Lunar Orbiter (KPLO), also named as Danuri, has been successfully measuring lunar gamma-rays since the arrival date to the Moon, December 17, 2022. The Danuri was launched by a SpaceX Falcon 9 rocket from Cape Canaveral Space Force Station on August 5, 2022(KST). The KPLO’s lunar trajectory is a low-energy, fuel-efficient ballistic lunar transfer (BLT) trajectory. The Danuri orbiter includes a gamma-ray spectrometer (KPLO Gamma-Ray Spectrometer, KGRS) as one of six scientific instruments. The KPLO has arrived to the lunar orbit of an altitude of 100 km on December 27, 2022. The KPLO Gamma-Ray Spectrometer (KGRS) is a compact low-weight instrument for the elemental analysis of lunar surface materials within a gamma-ray energy range from ~30 keV to 12 MeV. The major components of KGRS consist of a primary LaBr3 gamma-ray detector with an anti-coincidence counting module of 5% boron-loaded plastic scintillator to reduce both gamma-ray background from the spacecraft and housing materials, and cosmic ray background. The science goals of KGRS are associated with investigations of both lunar geology and lunar resources down to a half-meter depth of the lunar surface. Every 10 seconds, KGRS is able to collect three set of gamma ray data : two gamma-ray data of both high-gain and low-gain signals from the main sensor, LaBr3 and data from the shielding detector. KGRS has collected lunar GRS data for one and half months. This allows to present the performance of KGRS on the Moon. This presentation demonstrates both the performance of KGRS instrument and the first results of gamma-ray data from the KGRS onboard Danuri.


PS20-A024
Alpha Particle X-ray Spectrometer on Board Chandrayaan-3 Rover

Arpit PATEL#, M. SHANMUGAM, Santosh VADAWALE, Mithun N.P.S., Tinkal LADIYA, Nishant SINGH, Sushil KUMAR, Shiv Kumar GOYAL, Hitesh ADALJA, Deepak PAINKRA, Anil BHARDWAJ+
Physical Research Laboratory

Alpha Particle X-ray Spectrometer (APXS) is one of the scientific instruments on board the rover of the upcoming Indian lunar mission Chandrayaan-3. APXS employs the techniques of Particle Induced X-ray Emission (PIXE) and X-ray Fluorescence (XRF) to measure the abundance of various elements in the lunar soil and boulders near the landing site. Alpha particles and X-rays from the Cm-244 source assembly of the instrument cause emission of characteristic X-rays from the constituents of lunar soil, which is recorded by the Silicon Drift Detector (SDD) based spectrometer. APXS spectral measurements in the 0.8-25 keV energy range with a resolution of ~135 eV at 5.9 keV allow the identification of major and minor elements having atomic number higher than ten. From the line intensities, quantitative estimates of abundances can be obtained. APXS is mounted on a motor-based mechanism underneath the rover chassis. During rover movements, the instrument will be in stowed condition, and it will be deployed at each rover stop to carry out measurements of the lunar surface. APXS for the Chandrayaan-3 rover has undergone space qualification tests and has been successfully integrated with the rover. In order to obtain measurements of abundances from the observed X-ray spectra, we have followed a semi-empirical approach. X-ray spectra of a suite of geo-chemical reference materials were obtained using the APXS flight model. From these spectra, correlations of line intensities with the standard abundance values taking into account the matrix effects. Using these correlations, one can follow an iterative procedure to obtain abundances from APXS spectra of an unknown sample, such as lunar samples. Here we present an overview of the APXS instrument, its ground performance, and calibration efforts to obtain abundance measurements from the observed spectra of the lunar surface sample.


PS20-A035
Geological Characterization of New Mg-spinel Exposures on the Moon: Seeking Insights Into the Formation Mechanisms

Sachana SATHYAN1#+, Dibyendu MISRA1, Megha BHATT1, Deepak DHINGRA2, Suchit PUROHIT3
1Physical Research Laboratory, 2Indian Institute of Technology Kanpur, 3Gujarat University

Pink Spinel Anorthosite (PSA), a rare lunar rock type, rich in Mg-Al spinel and plagioclase with limited olivine and pyroxene, was identified with near-infrared reflectance spectroscopy by the Moon Mineralogy Mapper instrument (M³) onboard Chandrayaan-1 mission [1, 2, 3]. Most of the reported Mg-spinel detections are concentrated in the mid-latitudes along the basin rings and complex craters (wall and central peaks) with limited studies at high latitudes [4]. The Mg-Spinel bearing rocks on the Moon with small exposures need to be studied globally for understanding their origin mechanisms. Some of the key formation mechanisms proposed for Mg-Spinel lithology include magmatic assimilation of anorthositic highland crust and high Mg# magmas [3] and/or rapid crystallization of impact melts at shallow depths [5]. The distribution of this lithology has also been found to be commonly associated with areas of thin crust. Making use of spinel’s strong near-infrared spectral properties, global M3 data has been searched for new spinel detections using machine learning approach [6]. The present study is aimed at understanding the association of various lithologies and their geological setting in and around the newly detected spinel exposures at high latitudes (beyond ±60o) by preparing IBD and band ratio images using M³ reflectance data. Quantification of these spinel exposures will be done by studying 2 µm absorption band depth. The work will focus on new Mg-Spinel detections at Clavius, Rutherfurd, Bailly, Petzval, Doerfel, Anaximenes and Philolaus craters. References: [1] Pieters, C. et al (2011) JGR 116(4), 1-14. [2] Dhingra, D. et al (2011) GRL 38, L11201. [3] Pieters, C. et al (2014) American Mineralogist, 99(10), 1893–1910. [4] Sodha G et al (2022), LPI Contributions 2894. [5] Treiman A. H. et al (2019) American Mineralogist (104), 370–384. [6] Bhatt. et al. (2022), LPI Contributions 2678.


PS20-A012
Development and Characterization of a Multi-detector Large Area X-ray Spectrometer Using Silicon Drift Detectors with ASIC Based Readout

Nishant SINGH#, M. SHANMUGAM, Arpit PATEL, Sushil KUMAR, Deepak PAINKRA, Tinkal LADIYA, Santosh VADAWALE, Shreeya NATRAJAN+
Physical Research Laboratory

The use of silicon-based X-ray spectroscopy has been increasingly widespread in various fields, such as planetary elemental studies, solar studies, X-ray imaging, and astronomical observations. We have already developed a single-channel X-ray spectrometer with discrete components- Solar X-ray Monitor, flown on the Chandrayaan-2 orbiter. In this work, we have developed a large-area Silicon Drift Detector (SDD) based X-ray spectrometer using multiple SDDs that are readout by a multi-channel Application Specific Integrated Circuit (ASIC). This will be a compact instrument with very low power consumption. The developed system employs the VERDI ASIC, capable of readout from eight detectors simultaneously. The ASIC comprises of a preamplifier, a shaper with adjustable shaping times, and a peak stretcher with a baseline holder in each channel. The system enables to stack multiple SDD modules in a compact assembly with excellent energy resolution in the range of 0.5 keV to 15 keV with fast readout. The performance of the large-area X-ray spectrometer has been characterized for various electrical parameters such as shaping time, channel gain, detector temperature and dynamic range of the ASIC. The spectrometer provides an energy resolution of ~145 eV at 5.9 keV with 5 detector channels for the optimum shaping time of ~2 µs, at a detector temperature of approximately -30°C. The instrument is an excellent candidate for future planetary exploration missions and X-ray astronomy missions. The performance and results from the instrument will be presented at the conference.


Tue-01 Aug | 10:20 - 12:20 | MR334
PS23 - Observational and Theoretical Aspects of Exoplanets

Session Chair(s): Nader HAGHIGHIPOUR, University of Hawaii

PS23-A006
Planetary Census Through Time and Space Aided by LAMOST-Gaia-Kepler

Ji-Wei XIE#+
Nanjing University

Since the discovery of the first exoplanet (51 Peg b) orbiting a solar star in 1995, the study of exoplanets has been one of the most active frontiers. To date, over 5000 exoplanets have been discovered and thousands of candidates are yet to be confirmed. 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. In this talk, I will introduce our recent work aiming to address this question, which has been aided by the LAMOST, Gaia and Kepler surveys.


PS23-A002
Observational Effects of Multiple Exomoon Systems

Alex TEACHEY#+
Academia Sinica

If the Solar System is any guide, we can reasonably expect exoplanets may often be accompanied by not just one, but several, exomoons. Until now, however, the search for and characterization of exoplanets potentially hosting exomoons has utilized a single-exomoon model almost exclusively. Here we present new work that investigates and quantifies the degree to which the single-exomoon model is an appropriate choice, and where such a choice may be obscuring or even eliminating evidence for the presence of exomoons in the system. In particular, we explore the observational signatures of multi-moon systems in the context of the so-called “exomoon corridor”, identify a mass-stability relationship of these systems with implications for an observational bias towards single moon systems, and examine the impacts of single-moon model fitting for light curves containing multiple moons. These model choices have the potential to impact both the success of future searches, and our understanding of the dearth of exomoon discoveries to date.


PS23-A019
Observational Evidence of Planetary Evolutions in Clusters

Huigen LIU#+
Nanjing University

Stars usually formed in cluster environments. The dynamics and radiation of star clusters reshape the planetary disk, and influence the formation and evolution of planetary systems, as well as the occurrence rate of exoplanets. In this talk, I will demonstrate the observational evidence of correlation between the occurrence rate of exoplanets and the relative stellar velocity, based on Gaia and Kepler. We also choose a sample of planets in star clusters with different ages. A "gap" of Neptune-sized exoplanet between 20-100 Myr exists, but may be probably interpreted by sample limits. Then we statistics the fraction of planets with different radius, and find that the fraction of terrestrial and sub-Neptune planets increases with time, while that of the giant planet decreases in the first ~100 Myr, as predicted by photoevaporation model. Our results provide observational evidences on planet formation and evolution timescales in clusters.


PS23-A031
Planetary Orbit Eccentricity Trends (POET). I. The Eccentricity-metallicity Trend for Small Planets Revealed by the LAMOST-Gaia-Kepler Sample

Dong-Sheng AN+, Ji-Wei XIE#, Yuanzhe DAI, Ji-Lin ZHOU
Nanjing University

Orbital eccentricity is one of the basic planetary properties, whose distribution may shed light on the history of planet formation and evolution. Here, in a series of works on Planetary Orbit Eccentricity Trends (dubbed POET), we study the distribution of planetary eccentricities and their dependence on stellar/planetary properties. In this paper, the first work of the POET series, we investigate whether and how the eccentricities of small planets depend on stellar metallicities (e.g., [Fe/H]). Previous studies on giant planets have found a significant correlation between planetary eccentricities and their host metallicities. Nevertheless, whether such a correlation exists for small planets (e.g., super-Earths and sub-Neptunes) remains unclear. Here, benefiting from the large and homogeneous LAMOST–Gaia–Kepler sample, we characterize the eccentricity distributions of 244 (286) small planets in single (multiple) transiting systems with the TDR method. We confirm the eccentricity–metallicity trend whereby the eccentricities of single small planets increase with stellar metallicities. Interestingly, a similar trend between eccentricity and metallicity is also found in the radial velocity sample. We also found that the mutual inclination of multiple transiting systems increases with metallicity, which predicts a moderate eccentricity–metallicity rising trend. Our results of the correlation between eccentricity (inclination) and metallicity for small planets support the core accretion model for planet formation, and they could be footprints of self (and/or external) excitation processes during the history of planet formation and evolution.


PS23-A023
3D Configuration of a Compact Multi-giant System Lying at the Stability Boundary

Xianyu WANG#+, Songhu WANG
Indiana University

The WASP-148 system, composed of a transiting hot Jupiter and a non-transiting warm Jupiter, provides a singular opportunity to study the genesis and evolution of gas giants in close proximity. In this presentation, the three-dimensional configuration of the system will be discussed, incorporating the following key findings: (1) Rossiter-McLaughlin effect measurements of WASP-148 b, obtained through the use of WIYN/NEID and Keck/HIRES, indicate an orbit that is aligned, marking one of the few instances of this measurement in a compact multi-planet system and one of the inaugural scientific outcomes of the NEID instrument. (2) The mutual inclination between the two planets was calculated by combining archived and newly-collected transit, radial velocity, and transit timing variation data resulting in a mutual inclination of $26.5^{+5.3}{-6.6}$ degrees and a stable configuration. This stands in contrast to the previous study, which yielded a mutual inclination of $41.0^{+6.2}{-7.6}$ degrees with a stability probability of only $2.5%$. Our stability analysis further suggests that the WASP-148 system is located at the brink of its stability boundary, implying that it may be in a transitional phase between compact multi-planet systems and isolated-planet systems with more pronounced dynamical activity. The three-dimensional configuration of WASP-148 derived from our study provides observational support for a unified theory of exoplanetary formation, connecting the configurations found in compact multi-planet and isolated-Jupiter systems.


PS23-A026
Dynamical Evolution of Multiple Planetary Systems Subject to Atmospheric Mass-loss

Su WANG1#+, D.N.C. LIN2
1Purple Mountain Observatory, Chinese Academy of Sciences, 2University of California, Santa Cruz

A gap in exoplanets' radius distribution has been widely attributed to the photo-evaporation threshold of their progenitors' gaseous envelope. The outflowing gas endures tidal torque from the planets and their host stars. Alongside the planet-star tidal and magnetic interaction, this effect leads to planets' orbital evolution. In multiple super-Earth systems, especially in those which are closely spaced and/or contain planets locked in mean motion resonances, modest mass-loss can lead to dynamical instabilities. Through our work, we find that, the innermost planet may not lose too much atmosphere, less than 10% of its total planetary mass, to keep the system stable. Long-time stable multiple planetary systems which formed through orbital migration from the outer disk favor a slower mass-loss process. Planets in multiple planetary systems with rapid photoevaporation process especially with high fraction of mass-loss are prone to orbital crossing to destroy the system or leave fewer planets in widely separated configurations after fierce collide and merge process. Based on our work, the destiny of the closely packed multiple planetary systems can be classified into three possible types. (I) The system is far away from the central star with mean motion resonances configuration. Multiple planets in such systems undergo orbital migration which make them in or near MMRs and find their stable configuration finally. (II)The innermost planet is close to the central star and formed with little atmosphere. The system can keep in stable and chain resonances configuration after little mass-loss. (III) The innermost planet is close to the central star and formed with a certain atmosphere. The stable configuration they have formed can be destroyed leaving a single planet system or system with wide separated planets after the mass-loss process.


PS23-A033
Investigate the Formation of Giant Planets Around M Dwarfs

Tianjun GAN#+, Shude MAO, Sharon WANG
Tsinghua University

Over the last two decades, hundreds of transiting giant planets are detected but only few of them are orbiting M dwarfs even if M dwarfs are the most abundant stars in our Milky Way. With the highest planet-to-star mass ratio among planetary systems, giant planets around M dwarfs are the extreme cases to test planet formation theories. In this talk, I will present our statistical studies on the mass ratio and stellar metallicity distribution as well as occurrence rate of such systems. I will compare the observational results with predictions from theoretical works and investigate the formation channel. I will also present our preliminary result on the systematical search for transiting giant planets around late-type M dwarfs with TESS. Finally, I will discuss the origins of hot Jupiters around M dwarfs and the prospects with JWST.


PS23-A037
Evolution of the Planetary Obliquity Under the Competition of Eccentric Kozai-Lidov Resonance and the Equilibrium Tide

Xiumin HUANG1#+, Jianghui JI2, Shangfei LIU3, Ruobing DONG4, Su WANG2
1Chinese Academy of Sciences, 2Purple Mountain Observatory, Chinese Academy of Sciences, 3Sun Yat-sen University, 4University of Victoria

The planetary obliquity is a significant factor in determining the physical properties of planetary surfaces and the climate. Since direct detection is limited by the observation accuracy, dynamical theories are helpful to predict the evolution of the planetary obliquity. Based on the conservation of angular momentum, the competition between the Eccentric Kozai-Lidov (EKL) resonance and the equilibrium tide is utilized in this work to investigate the diverse secular evolution paths of planetary obliquity. For close-in S-type terrestrial planets in binary star systems, when the initial timescale ratio of the secular resonance and the tidal dissipation ttide/tkl > 1, the planetary obliquity will first undergo the excitation and the planetary rotation axis will be triggered to flip, then the obliquity enters the quasi-equilibrium state between 40° and 60°. The maximum obliquity can reach 130° when ttide/tkl > 104. The qualitative simulation results indicate the maximum obliquity increases with the semi-major axis ratio a1/a2 and the perturbing body's eccentricity e2. The equilibrium timescale teq and the timescale in relation to the obliquity going down to zero, are both positively correlated with a1. When ttide is comparable to tkl, an abrupt rise of teq will occur at a1~0.5 au and a2=20 au. For several observed hot-Jupiters in binary star systems, we present the equilibrium obliquity map to predict their possible obliquity. For terrestrial planets around M-dwarfs, we further estimate the initial orbital conditions to maintain the stable obliquity in the habitable zone.


Tue-01 Aug | 1:10 - 3:10 | MR307
PS20 - Surface Science and Exploration of the Moon and Airless Planetary Bodies

Session Chair(s): Durga Prasad KARANAM, Physical Research Laboratory, Ottaviano RÜSCH, Westfälische Wilhelms-Universität Münster

PS20-A038 | Invited
Possibility of Charged Dust in Lunar Exosphere

Varun SHEEL#+, Jayesh PABARI
Physical Research Laboratory

The Moon as a non-magnetized, airless body is exposed to UV radiation and solar wind from the Sun. This leads to lunar surface charging and formation of plasma sheath near the surface. Typically, the surface potential can be ~20 V and -4000 V on the day and night side, respectively. Due to surface charging, finer (micron and sub-micron) dust particles are charged and levitated in the environment. We explore possibility of charged dust levitation on Moon and its transportation in the lunar exosphere.


PS20-A017 | Invited
Young Volcanism in the Procellarum KREEP Terrane on the Moon

Yuqi QIAN1#+, Long XIAO2, Zaicong WANG2, James HEAD3, Joseph MICHALSKI1
1The University of Hong Kong, 2China University of Geosciences, 3Brown University

The young mare basalts are the products of recent lunar volcanism, mainly distributed in the center of the Procellarum KREEP Terrane (PKT) with elevated heat-producing elements. The young basalts were proposed to be rich in olivine based on their spectral features and younger flows tend to have higher abundances. These young basalts had not been sampled by previous missions. Recently, they were first investigated in-situ by Chang’e-3, and then sampled by Chang’e-5, which provides significant ground truth to constrain the mineralogy, chronology, and evolution of the young basalts. We found that the Chang’e-3/Chang’e-5 basalts have a broad 1 μm spectral absorption from the in-situ data as the same as the remote sensing observations. However, Chang’e-3 APXS data and laboratorial investigation of Chang’e-5 samples indicate that olivine is not abundant (<10%). The misinterpretation of high olivine abundance in previous studies may be due to the special composition of pyroxene. In addition, the mineralogy of young basalts is not homogeneous in the PKT. Based on the newly obtained model ages of young basalts calibrated by the Chang’e-5 basalts, we found the youngest unit is located to the northeast of Kepler crater, with an age of ~1.19 Ga (U17). Mare basalts with ages of ~2.0 Ga are widespread in the center of the PKT, indicating an additional heat source or mechanism may be needed. When considering the composition and ages together, the younger basalts tend to have higher abundance of TiO2 and no clear trend of olivine. Two distinct young mare regions were identified within the PKT, i.e., U3 and U17, with highest olivine abundance and youngest age. We propose that they should be listed as high priority sample-return targets for future missions to understand late lunar thermal history.


PS20-A023
Lunar Dust: Recent Observation and Experimental Studies

Xiao-Ping ZHANG1#+, Hong GAN1, 良海 谢2
1Macau University of Science and Technology, 2National Space Science Center, Chinese Academy of Sciences

Lunar dust has been regarded as a major problem for lunar surface explorations since the Apollo era, as these very abrasive and fine dust grains are harmful for both the instruments and human beings. Lunar horizon glows (LHGs) observed in the Surveyor and the Apollo missions provided direct evidence for lunar dust levitation and transport near the terminator. LHG was interpreted as forward scattered sunlight from a cloud of lofted dust grains, with an altitude depending on the radii of the dust grains (rd) that is less than 1 m for the Surveyor observations (rd ≈ 5 μm) and tens of kilometers for the Apollo observations (rd ≈ 0.1 μm). Recent remote sensing measurements by Clementine and Lunar Reconnaissance Orbiter showed a very tenuous lunar dust exosphere with a dust density of less than 1 m−3. A high-density dust cloud was also absent in the in-situ measurements by the Lunar Atmosphere and Dust Environment Explorer (LADEE), where the tenuous asymmetric dust cloud was interpreted as the impact ejecta of cometary grains. However, the micrometeoroid impact mechanism could not explain the duration and the dust abundance (about 104 m−3) of the observed LHGs in Apollo era. Why the later observations show distinct different results compared with Apollo missions? What is the mechanism responsible for the transportation of large amount of lunar dust into an altitude of tens of kilometers? These open questions need to be addressed. Here, we provide new evidence of long-term dust deposition according to Chang’E-3 observation. We also show five dust enhancements events observed by LADEE mission near twilight craters. These new observations support the mechanism of electrostatic dust transportation. Corresponding experimental results of dust transportation under an electron beam radiation will also be presented. (Funded by the Science and Technology Development Fund of Macau (0014/2022/A1).


PS20-A008
Kinematic Consideration on the Top-shaped Figure of Asteroid Ryugu

Noriyuki NAMIKI1#+, Koji MATSUMOTO1, Naru HIRATA2, Ryuhei YAMADA2, Yoshiaki ISHIHARA3, Hitoshi IKEDA3, Hiroshi ARAKI1, Keiko YAMAMOTO1, Shinsuke ABE4, Fumi YOSHIDA5, Arika HIGUCHI6, Sho SASAKI7, Shoko OSHIGAMI3, Seiitsu TSURUTA1, Kazuyoshi ASARI1, Seiichi TAZAWA1, Makoto SHIZUGAMI1, Hideaki MIYAMOTO8, Hirohide DEMURA2, Toshimichi OTSUBO9, Naoyuki HIRATA10, Gaku NISHIYAMA8, Fuyuto TERUI3, Sei-Ichiro WATANABE11, Takanao SAIKI3, Satoru NAKAZAWA3, Makoto YOSHIKAWA3, Yuichi TSUDA3, Alexandre DE LARMINAT12
1National Astronomical Observatory of Japan, 2The University of Aizu, 3Japan Aerospace Exploration Agency, 4Nihon University, 5University of Occupational and Environmental Health Japan, 6Kyoto Sangyo University, 7Osaka University, 8The University of Tokyo, 9Hitotsubashi University, 10Kobe University, 11Nagoya University, 12Université de Paris

The shape of rubble pile asteroids can provide a clue to the transportation mechanism of volatiles inside the snow line. Previously the ellipsoids were regarded as the likely equilibrium figure of rotating self-gravitating aggregates while in situ observation of Hayabusa2 and OSIRIS-REx have disclosed top-shaped figures. However, the formation process of the top-shaped figure is still under debate, and it is important to clarify whether the mass transfer is constrained in the surficial layer or is involved in internal deformation. We consider in this study a simple kinematic balance of self-gravity and centrifugal force near the surface of asteroid Ryugu. The stability of the slope is evaluated simply by a ratio of traction along the slope and resistance caused by friction and cohesion, that is, a factor of safety, FoS. The local gravity is calculated assuming the current figure of Ryugu and constant density inside. Also, we take into account cohesion stress among regolith and boulders. We assume that the current shape of Ryugu was critical in the past fastest rotation. Thus we set FoS-1 = 1 and calculate cohesion stress per unit length as a function of latitude for given P and angle of repose. We have thoroughly examined ranges of P and the angle of repose. A condition for plausible P and the angle of repose is arbitrary set such that the standard deviation of cohesion per unit length is less than 5x10-6 m/s2. Consequently, P, the angle of repose, and cohesion per unit length that match the present top-shaped figure are constrained to be between 3.8 and 4 hr, 20° and 25°, and less than 2.5x10-6 m/s2, respectively. This kinematic model is further tested using slopes of large craters. P at the crater formation is constrained between 4.1 and 7.6 hr.


PS20-A020
Hydrothermal Evolution on CM Chondrite Parent Bodies

Shreeya NATRAJAN#+, Kuljeet Kaur MARHAS
Physical Research Laboratory

The CM type chondritic meteorites are said to have water rich parent bodies that formed in the early stages of the solar system. These primitive samples show evidences for prograde alteration with an early period at lower temperatures (<150℃) and later affected by short lived thermal metamorphism at~200℃ to >750 ℃. They record significant interaction between liquid water, silicate rocks and organic content. The exact conditions of these hydrothermal alterations are very crucial in understanding the formation and evolution of hydrous asteroids. The extent of aqueous alteration has been quantified through various techniques some of which indicates that it may have been driven primarily by impact rather than by radiogenic heating. Moreover, the wide range of hydrothermal conditions affect the formation, destruction and transformation of the organic content within. The influence of water and related activity on the organics encased in meteorites makes their origin inextricably linked. Furthermore, the recent study of C-type near-Earth asteroids (e.g. Bennu and Ryugu) and the presence of CM chondrite material embedded in other meteorites implies that the CM parent body was disrupted and could have supplied material to Earth. Their similarity makes the analysis of CM chondrites essential to the interpretation of these enigmatic bodies. In this study we have performed a multi-technique study of IOM extracted from 18 carbonaceous (CI, CM,CR) meteorite samples with an aim to understand the aqueous alteration processes using FTIR, Raman and XANES analyses. We propose a state of chemical equilibrium that is reached between IOM and SOM during hydrothermal alteration where IOM could have evolved from SOM modification and organo-mineral interactions.


Tue-01 Aug | 1:10 - 3:10 | MR334
PS23 - Observational and Theoretical Aspects of Exoplanets

Session Chair(s): Su WANG, Purple Mountain Observatory, Chinese Academy of Sciences

PS23-A049
Resonance Diversity and Resonance Offsets in Multi-planet Resonant Chains are Natural Outcomes of Their Formation

Nader HAGHIGHIPOUR#+
University of Hawaii

The discovery of multi-planet resonant chains such as those in TRAPPIST-1 and Kepler-90, where adjacent planets are in different resonances, has raised questions on the formation of these systems. It is widely accepted that these systems formed through the combination of migration and resonance-capture where migrating planets capture each other in resonances. There is, however, an issue with this scenario as migrating planets tend to capture each other in the same resonance. It has been suggested that tidal forces are the reason that resonant-chain planets are in different commensurabilities. The latter motivated us to examine the validity of this statement. We have carried out extensive simulations of planet formation and migration, and determined the probability of capture for different resonances. Results demonstrate that migrating planets can in fact be captured in different resonances confirming that the diversity of resonances observed in resonant chains is a natural consequence of the formation and resonance capture mechanism, and does not require a secondary, post-formation process. Results also show that the probability of capture (and, therefore, the final commensurabilities) is highly depended on the characteristics of the systems, especially the planets’ mass-ratio and migration speed. Finally, our simulations indicate that capture in a resonance never occurs at the resonance’s exact commensurability and there is always some deviation. The extent of this deviation also depends on the mass-ratio and orbital characteristics of the planets and the mechanism through which migrating planets lose energy. This also confirms that unlike previous studies, no post-capture mechanism is needed to explain the deviation from exact resonances observed in Kepler (and RV) planet pairs. We present the details of our study and discuss their implications for the formation and orbital architecture of resonant, multi-planet systems.


PS23-A038
Effects of Planetesimal Scattering: Explaining the Observed Period Ratio Offsets from 3:2 and 2:1

Sourav CHATTERJEE#+, Tuhin GHOSH
Tata Institute of Fundamental Research

The deficit and excess of adjacent planet pairs narrow and wide of 3:2 and 2:1 have intrigued many since first observed. Our most recent simulations suggest that without any fine tuning, dynamical interactions between a mixture of resonant and near-resonant planet pairs, and nearby planetesimals, presumably left-over from the planet-formation process, can naturally explain the observed distribution of period ratios near 3:2 and 2:1. While the deficits narrow of the mean motion resonances (MMR) are caused primarily by initially non-resonant planet pairs jumping across the MMRs due to interactions with the planetesimals, the excesses wide of the MMRs are caused by a combination of initially resonant and non-resonant planet pairs creating a pile up. We further find that the observations can be best explained if ~25% (<1%) of all systems were trapped into the 3:2 (2:1) MMR at the onset of this process. The difference in the importance of initially trapped MMRs is consistent with MMR trapping efficiency for planets in this mass range. Not more than a few percent of systems are expected to be in these MMRs at present.


PS23-A004
Probing Hot Jupiters Through Transit Timing and Transmission Spectrum

Ing-Guey JIANG#+
National Tsing Hua University

As one of major exoplanet populations, the existence, formation, evolution, and properties of hot Jupiters have been investigated extensively. In order to address these topics, we perform transit observations with a network of telescopes and obtain transit light curves, transit timing, and broad-band transmission spectrum. We present a review of our main scientific results and also discuss our future development.


PS23-A013
Vetting Kepler Planet Candidates with Long Orbital Periods and Small Transit Depths Using the Similarity Method

Xinyu YAO1#+, Jian GE1, Hui ZHANG2
1Chinese Academy of Sciences, 2Shanghai Astronomical Observatory

Detecting planets with long orbital periods and small size is significant in studying planet occurrence rates, especially for those terrestrial-like planets orbiting FGK main sequence stars in the habitable zone. However, there is an obvious problem in the search for such planetary systems to distinguish transit signals with low signal-to-noise ratios from instrument noises and stellar variability. Because of this, the Kepler mission has only a small number of confirmed planets of this type. In this presentation, we will introduce a new method to examine ∼190 Kepler DR25 planet candidates, which have long orbital periods (>300 days), long transit durations (>4 hours), and small transit depths (<2500 ppm). This method is based on the use of the RMS, curve-length, and area of two or more different transit-like signals to measure the similarity between transit signals of KOI candidates and then apply to the simulated and real transit planets and false alarms with the same parameter distribution as these KOI candidates for the statistical analysis, and then determine whether each KOI candidate has high confidence to be a false alarm or a planet candidate. Using this method, we were able to select ~20% KOIs as false alarms with high confidence. In addition, we were also able to confirm several KOI candidates as planets with high confidence. This work will help save follow-up time in the future using HST or JWST and improve the efficiency of planet validation.


PS23-A051
Explaining the Formation of Giant Planet Orbiting M Dwarfs

Mengrui PAN#+, Beibei LIU
Zhejiang University

As the smallest and most common stars in the Galaxy, M dwarfs are theoretically hard to form giant planets around them, only if the disk is extraordinary massive and the rapid inward migration of planets is significantly suppressed. While approximately 20 percent of observed planets orbiting M dwarfs were gas giants, which highlights the crucial need to understand the formation of massive planets around low-mass stars. Here we propose a more efficient mass growth mechanism by combining both pebble and planetesimal accretion. Two-component disk model is used to explore the dynamic evolution of planets. We identify the planet-forming regions of disks with different local turbulent viscosity throughout single embryo tests. Results shows that the planet-forming region expands with the decrease of the local viscosity. Yet the collision of planets around transition radius in local high-viscosity disk implies a greater possibility of giant planet formation. The architectures of synthetic planetary systems are quite different, and some of them harvest habitable planets. Our research provide a plausible way for the formation of giant planets and the structure of planetary systems around M dwarfs. We also predict the occurrence of terrestrial planets in the vicinity of gas giant to be confirmed by future observations.


PS23-A020
YunMa: A Cloud and Radiative Transfer Model Optimised for Retrieval Study of Exoplanets

Sushuang MA1#+, Yuichi ITO2, Ahmed AL-REFAIE1, Quentin CHANGEAT3, Billy EDWARDS4, Giovanna TINETTI1
1University College London, 2National Astronomical Observatory of Japan, 3Space Telescope Science Institute, 4Netherlands Institute for Space Research

The fast development of exoplanetary observation and transit spectroscopy enables the effective study of exoplanetary atmospheres. The atmospheric features can be obscured in spectra with the formation of clouds and hazes. It adds difficulty to observing the atmospheric chemistry and imposes uncertainties in constraining the atmospheric parameters using transit spectroscopy. The high-quality transit spectra offered by the next generation of facilities, such as JWST and Ariel, allow observing the signatures of clouds and hazes via transit spectroscopy, thus allowing the detailed study of their size distribution. In this work, we built YunMa, an exoplanetary cloud retrieval model, to deepen the understanding of cloud formation from transit spectra and cloud microphysics, an essential mechanism of cloud formation. In YunMa, we simulated the vertical cloud particle size distribution and the corresponding transit spectra of the cloudy atmosphere. We took advantage of the TauREx 3 platform, an open Bayesian framework for spectral retrieval, to enable the retrieval function of YunMa. We validated our model by comparing our simulation with previous literature results. We set the sedimentation efficiency (fsed), which controls the cloud microphysics, as a free parameter in retrieval. We evaluate the retrieval performances on a synthetic temperate super-Earth. We aim to present YunMa to demonstrate retrievals with cloud microphysics considered.


PS23-A048
A Newly Developed Adaptive Magnification Map Grid Search Algorithm Used for the Analysis of Planetary Microlensing Events

Jiyuan ZHANG#+
Tsinghua University

Microlensing light curve is a time series with ever-changing magnifications. It is easy to calculate the light curve of a planetary microlensing event given a set of parameters, but relatively difficult to extrapolate these parameters from the light curve. A global search method with fixed parameters named as grid search algorithm is thus used to determine the parameters of planetary microlensing events. However, calculating magnification is the most time-consuming part of this algorithm, thus the magnification map method which calculating and storing magnification in advance and utilizing the magnification maps through the interpolation method is developed. The speed of grid search algorithm is thus greatly improved. Still, the magnification map method of uniform mesh has a trade-off between accuracy and speed. In fact, in the vicinity of caustics, the magnification changes dramatically, while in other areas, the magnification changes relatively gently. To solve this problem, we propose an adaptive magnification map grid search algorithm used for the analysis of planetary microlensing events and thus achieve high accuracy without losing too much speed.


PS23-A034
RVxTESS: Mitigating RV Signal Induced by Stellar Jitter

Jiaxin TANG#+, Sharon WANG
Tsinghua University

The Radial Velocity (RV) method, measuring the Doppler Shifts from stellar spectra, is widely used for the detection and characterization of exoplanets. For low-mass planets, RV detection typically requires cm/s precision, whereas the stellar jitter becomes an issue at the m/s level. Thus, it is essential to mitigate such stellar jitter in order to detect Earth-like planets using RVs. Our project focuses on the asteroseismic signals of stellar jitter, including stellar oscillation and granulation. We study HD 5562 with fitting the model of stellar jitter to the observational data from the Transiting Exoplanet Survey Satellite (TESS) and RVs from the Carnegie Planet Finder Spectrograph on the Magellan II Telescope (Magellan/PFS). We perform a Gaussian Process (GP) regression on the star's photometric and RV data to describe its asteroseismic signals. The simultaneous fit model suggests that the primary mode of its oscillation is around 15 minutes or around 1000 muHz. We have reduced the RV scatter from 2.01 m/s to 0.72 m/s by fitting a GP model, which was trained on the TESS light curves, to the RV time series. We also explore multiple ways to model the oscillation in the photometry and how it could be transferred effectively to the RV domain. Our project is part of the RVxTESS program (RVxTESS.com), which combines simultaneous TESS photometry with ground-based RV observations to study stellar jitter.


Tue-01 Aug | 3:30 - 5:15 | MR307
PS20 - Surface Science and Exploration of the Moon and Airless Planetary Bodies

Session Chair(s): Varun SHEEL, Physical Research Laboratory

PS20-A031 | Invited
Understanding Thermal Emission from the Lunar Epiregolith

Benjamin GREENHAGEN1#+, Carlie WAGONER1, Parvathy PREM1, Neil BOWLES2, Kerri DONALDSON HANNA3, Nandita KUMARI4, Paul LUCEY5, Tyler POWELL6
1Johns Hopkins University Applied Physics Laboratory, 2University of Oxford, 3University of Central Florida, 4Stony Brook University, 5University of Hawaii at Manoa, 6University of California, Los Angeles

On the Moon and other airless bodies the uppermost portion of regolith, the “epiregolith”, represents the boundary layer between the surface and space that dominates remote sensing observations from far-ultraviolet reflectance to far-infrared emission. The epiregolith is typically a few cm in thickness with the layer most critical to thermal emission spectroscopy ~2 mm in thickness. Thermally, the epiregolith is characterized by significant temperature gradients (~60K / 100 μm). These conditions make spectral emission from airless bodies wholly different from Earth and Mars (where the epiregolith is essentially isothermal) and complicate the interpretation of remote sensing data, especially thermal infrared (TIR) emission spectroscopy. In this presentation, we review the past and ongoing efforts to understand epiregolith effects on thermal emission and look toward additional information that future datasets and models may provide. Our ongoing research uses orbital data from NASA’s Lunar Reconnaissance Orbiter (LRO) Diviner Lunar Radiometer (Diviner), laboratory experiments in simulated lunar environment, and radiative transfer models. Diviner is a multispectral radiometer that has observed solar reflectance and TIR emission from the Moon at a wide range of illumination and viewing geometries to constrain radiative balance and spectral emission. We also use the environment chambers such as the Simulated Airless Body Emission Laboratory (SABEL) at the Applied Physics Laboratory to reproduce a relevant thermal environment. SABEL and similar chambers can create thermal gradients of variable magnitude and simulate the wide range of temperatures relevant to a wide range of studies. Thermal models also help predict the behavior observed by Diviner and laboratory experiments. Insights gained from these studies are used to investigate the thermal structure of and spectral emission from the epiregolith and to improve interpretations of TIR datasets of the Moon and airless bodies for Diviner and upcoming missions such as Lunar Trailblazer and BepiColombo.


PS20-A041 | Invited
The Search for Liquid Water Beneath the Martian South Polar Layered Deposits

Roberto OROSEI1#+, Graziella CAPRARELLI2, Barbara COSCIOTTI3, Jamaledin BANIAMERIAN3, Sebastian E. LAURO3, Elisabetta MATTEI3, Elena PETTINELLI3, Katie PRIMM4, Francesco SOLDOVIERI5, David STILLMAN6
1Istituto Nazionale di Astrofisica, 2University of Southern Queensland, 3Università degli Studi Roma Tre, 4Planetary Science Institute, 5Consiglio Nazionale delle Ricerche, 6Southwest Research Institute

The Mars Advanced Radar for Subsurface and Ionosphere Sounding (MARSIS) was built to probe the Martian subsurface down to depths of kilometers by transmitting electromagnetic pulses in the MHz frequency range. Echoes coming from a depth of about 1.5 km, stronger than surface reflections, were repeatedly detected in a 20 km wide area centered at 193°E, 81°S. Quantitative analysis of such echoes yielded values of the relative dielectric permittivity at the base of the South Polar Layered Deposits (SPLD) greater than 15, matching that of water-bearing materials.
Reanalysis of observations, using signal processing procedures previously applied to terrestrial polar ice sheets, confirmed that the properties of MARSIS echoes match those of reflections from subglacial lakes, while the analysis of subsequent observations revealed the presence of other wet areas nearby. Because of the very low temperatures expected beneath the SPLD, it was proposed that the waters are hypersaline perchlorate brines, known to form at Martian polar regions and thought to survive for an extended period of time on a geological scale at below-eutectic temperatures.
Because of its significance in the study of the biologic potential of Mars, the identification of liquid water has been closely scrutinized by the scientific community at large, and several counter-arguments and alternative interpretations of MARSIS measurements have been proposed over last four years. Here we aim at providing a summary of the existing literature on the topic, and at assessing the current status of the debate.


PS20-A004
Surface Science of the Moon from Laboratory Studies on Analogues Under Simulated Lunar Environment

Durga Prasad KARANAM#+, G. AMBILY, P. KALYAN REDDY
Physical Research Laboratory

Measurements of certain key properties of lunar analogous materials and their variability under simulated environment provide key support to the definition of science objectives of any mission; instrument design and calibration; mission planning; analysis and interpretation of retrieved data. They also support modelling studies which is often used to derive global perspectives. Due to the exotic nature of lunar environment, these investigations are unique, challenging, but at the same time are of great significance which are often ignored and given least priority. Some of the niche areas that require support of such experimental studies are lunar surface composition and chemistry, geophysical studies for understanding formation and evolution of the Moon, thermophysical studies for prospecting water-ice and future in situ exploration, Solar wind/Particle interaction and dust studies. For example, electrical properties measurements in the ac/dc frequency regime provide support for compositional and structural studies, physical and mechanical properties help modeling rheology and thermodynamics, thermophysical and electrical properties for geological evolution and polar water-ice prospecting and so on. An experimental facility for mimicking the lunar surface environment - temperatures, pressures and surface strata, has been indigenously designed and developed. This facility has unique capabilities for making systematic measurements for different geo-physical settings of the Moon which are otherwise not possible. No such attempt is currently being made elsewhere globally. On the other hand, large-scale exploration including future sample return and ISRU activities will also be greatly benefitted. Several experiments were carried out to demonstrate the capability of the facility. Such a facility can bring paradigm shift in carrying out future in situ exploration of the Moon. Details of the facility and results from recent experiments will be presented. Details on possible experiments using the facility to address various lunar science problems will also be discussed.


PS20-A011
Decoding Magmatism on the Eastern Limb of the Moon: Tell-tale Signs from Mare Marginis and Mare Smythii

Neha PANWAR1,2#+, Neeraj SRIVASTAVA1, Megha BHATT1, Anil BHARDWAJ1
1Physical Research Laboratory, 2Indian Institute of Technology Gandhinagar

The lunar eastern nearside-farside boundary is an excellent region to understand the lunar magmatic processes in detail. Several uniquely emplaced basalts on the Moon, such as the Mare Australe and Mare Marginis, are present at this boundary. Mare Marginis (13.3°N, 86.1°E) is a large mare deposit lying north of the pre-Nectarian Smythii Basin (13.3°N, 86.1°E). The Smythii Basin is an ~880km multiring basin with three rings identified using GRAIL and is partially flooded with mare basalts. The GRAIL data suggested the absence of any impact basin where the Mare Marginis is emplaced. Thus, the Mare Marginis basalts, unlike most widespread lunar basalts confined inside an impact structure, are emplaced within a topographic low that is not associated with any impact basin. The presence of equally widespread volcanism inside and outside an impact basin, viz. Smythii, in this case, is perplexing. Thus, it is paramount to understand the geological factors responsible for such unique volcanism on the Moon. Results from Clementine Mission suggested a common source for the Mare Marginis and Mare Smythii basalts based on their similar FeO wt% and TiO2 wt %. In this study, we carried out a detailed investigation of the mineralogy of the basalts belonging to Mare Marginis and Mare Smythii using high-resolution spectral data from M3 onboard Chandrayaan-1 and derived data from Kaguya’s Multiband Imager (MI) (FeO wt%) and LRO's WAC (TiO2 wt%) to delineate their compositional diversity. Preliminary investigation revealed that the basalts of Mare Marginis are compositionally diverse. The basalts in the western Marginis region show a relatively higher Ca2+ than the rest of Mare Marginis and Mare Smythii basalts. Further, structural features such as the Linear Gravity Anomaly, Crisium Basin rings etc., have been observed that exert controls on the region's geology.


PS20-A030
Recent Advances in the Understanding of the Evolution of Lunar Surface Rocks

Ottaviano RÜSCH1#+, Rachael M. MARSHAL1, Markus PATZEK1, Valentin T. BICKEL2, Christian WOEHLER3, Marcel HESS3, Ben AUSSEL1
1Westfälische Wilhelms-Universität Münster, 2University of Bern, 3Technical University of Dortmund

Orbital and in situ high-spatial resolution observations of the Moon reveal rocks (boulders) scattered across the surface. These rocks preserve the chemistry, mineralogy and petrology of the lunar crust and its evolution. Rocks are affected by surface processes and thus inform on regolith formation and evolution. Furthermore, boulders influence processes such as dust lofting and migration, and surface thermal emission. Here we review our recent advances in the understanding of the evolution of rocks upon exposure to the lunar surface environment. We assessed pristine rock topography at the m and sub-mm scale and estimated its effects on photometry in orbital optical images. We developed a new technique to determine the age of rock populations based on size frequency distributions, the measured size frequency distribution of meteoroids and rock shattering functions. We determined that while primary impactors control the shattering of >m sized rocks, the survival time of cm-sized rocks is strongly influenced by low-velocity secondary impactors. We modeled the topography of debris aprons around mature rocks as a function of surface exposure age and rock diffusivity (material strength). The model enables to relatively estimate rock strength as well as exposure age of single rocks, using orbital and/or in situ optical images. To determine the effects of diurnal temperature variations on lunar rocks, we experimentally simulated temperature excursions in high vacuum and induced (thermal fatigue) stresses on cm-sized lunar samples. In addition to the formation of new cracks within the samples, we observed formation and removal of micrometer-sized flakes. This phenomenon is likely related to rocks of glass and plagioclase-rich petrologies, such as lunar and impact (melt) breccias. Applications based on this new set of understanding will be shown. For example, to assess the evolution of regolith and the history of specific regions on the Moon.


PS20-A001
Water-ice in Lunar PSRs: Experiments and Modelling for Its In-situ Detection and Quantification

Sanjeev MISHRA#, Janmejay KUMAR, G. AMBILY+, Chandan KUMAR, P. KALYAN REDDY, Durga Prasad KARANAM
Physical Research Laboratory

While Moon was considered bone-dry a few decades back, recent studies have concluded presence of water on the Moon, especially in the Lunar Permanently Shadowed Regions (PSRs). This regolith bound water-ice is believed to be present in the sub-surface of the Moon. The presence of water-ice has led to many proposed and scheduled missions to the Moon in near future. Water is also a critical component of the In-Situ Resource Utilization (ISRU) missions of the future and therefore makes the understanding of the source, transport and storage of water and water-ice very important. While radars and other remote sensing techniques can be used for sub-surface water-ice detection, it is only through direct in-situ observations can one detect and quantify the water-ice and throw light on the stratigraphic variations of its presence in the sub-surface. An impedance probe based on Wenner electrode array technique working at very low frequencies, typically in mHz to kHz range, is very well suited for such measurements. By looking for the unique signature of the water-ice in the mHz-kHz range owing to the phenomenon of dielectric relaxation unique to water-ice in this range, one can detect the presence of traces of water-ice. By employing the multi-phase mixing models, the water-ice can be quantified and its bulk spatial distribution be predicted. We have carried out a number of experiments in controlled environments with lunar analogue samples and have compared the results with the model predictions and similar results available in the literature. Also, we have been developing an FEM model for simulating the Impedance probe and solving the non-inductive Maxwell’s Equations in its vicinity (Lunar PSRs) incorporating various elements of the lunar regolith. The paper will detail the experiments, methodology, results from the experiments and also, some of the initial modelling results.


Tue-01 Aug | 3:30 - 5:15 | MR334
PS23 - Observational and Theoretical Aspects of Exoplanets

Session Chair(s): Ji-Wei XIE, Nanjing University

PS23-A017 | Invited
The Earth 2.0 Space Mission

Jian GE1#+, Hui ZHANG2
1Chinese Academy of Sciences, 2Shanghai Astronomical Observatory

The “Earth 2.0 (ET)” mission in China is to address a few of fundamental questions in the exoplanet field: How frequently habitable Earth-like planets orbit solar type stars (Earth 2.0s)? How do terrestrial planets form and evolve? Where did floating planets come from? ET consists of six 30 cm diameter transit telescope systems with each field of view of 500 square degrees and one 35 cm diameter microlensing telescope with a field of view of 4 square degrees. The ET transit mode will monitor ~1.2M FGKM dwarfs in the original Kepler field and its neighboring fields continuously for four years while the microlensing mode monitors over 30M I< 20.5 stars in the Galactic bulge direction. ET will merge its photometry data with that from Kepler to increase the time baseline to 8 years. This enhances the transit signal-to-noise ratio, reduce false positives, and greatly increases the chance to discover Earth 2.0s. Simulations show that ET transit telescopes will be able to identify ~17 Earth 2.0s, about 5000 Earth-sized terrestrial planets and over 30,000 new planets. The ET microlensing telescope will be able to identify over 1000 microlensing planets. With simultaneous observations with the ground-based KMTNet telescopes, ET will be able to measure masses of over 300 microlensing planets and determine the mass distribution functions of free-floating planets and cold planets. ET will be operated at the Earth-Sun L2 orbit with a designed lifetime longer than 4 years. The mission status will be reported.


PS23-A021
Characterising Exoplanets with Machine Learning: Lesson Learnt from the Ariel Data Challenge

Kai Hou YIP1#+, Ingo WALDMANN1, Giovanna TINETTI1, Quentin CHANGEAT2
1University College London, 2Space Telescope Science Institute

Current endeavours in exoplanet characterisation rely on atmospheric retrieval to quantify crucial physical properties of remote exoplanets from observations. However, the scalability and efficiency of the technique are under strain with increasing spectroscopic resolution and forward model complexity. The situation becomes more acute with the recent launch of the James Webb Space Telescope and the Ariel Space Mission. Machine learning (ML) techniques lands itself as a promising alternative. Developing techniques of this kind is an inter-disciplinary task, one that requires domain knowledge of the field, access to relevant tools and expert insights on the capability and limitations of current ML models. These stringent requirements have so far limited the developments of ML in the field to a few isolated initiatives. Accepted as part of the competition track in NeurIPS 2022, the goal of the Ariel Data Challenge is to open up the problem to the global community and identify reliable and scalable method(s) to perform planetary characterisation. Participants were given 4 months to train a model that can provide the approximate conditional distribution of key planetary properties. The data challenge is positively received by the community and has attracted 200+ participants from 39 countries around the globe to participate. In this talk I will focus on the outcomes of the data challenges. In particular, I will talk about 1.) the winning solutions 2.) the publicly available ABC database and 3.) the impact of distribution shift on model performance


PS23-A009
Modeling Statistical Properties of Close-in Super-earths with Giant Impacts

Pin-Gao GU1#+, Yuji MATSUMOTO2, Eiichiro KOKUBO2, Shoichi OSHINO3, Masashi OMIYA4, Kenji KUROSAKI5
1Academia Sinica, 2National Astronomical Observatory of Japan, 3The University of Tokyo, 4National Institutes of Natural Sciences, 5Kobe University

Both the radial-velocity methods and transit-timing variations suggested that most late-type M dwarfs do not harbor super-earths, while the KEPLER transit survey discovered numerous close-in super-earths around solar-type stars. We show that this difference can be modeled by planet formation through giant impacts. Furthermore, with photoevaporation, our giant impact model makes an attempt to simultaneously model two key KEPLER results for the first time — the bimodal size distribution and peas-in-a-pod (similar in size and regularly spaced in multiple-planet systems) of close-in super-earths around solar-type stars. We shall show that our model is generally consistent with the KEPLER results.


PS23-A015
Transiting Exoplanet Yield Predictions of the ET Mission

Hui ZHANG1#+, Jian GE2, Xu HUANG3, Kevin WILLIS4
1Shanghai Astronomical Observatory, 2Chinese Academy of Sciences, 3University of Southern Queensland, 4Science Talent Training Center

The Earth 2.0 (ET) mission is a space telescope being developed to detect thousands of terrestrial exoplanets over a wide range of orbital periods including the not-yet-discovered Earth 2.0s------habitable Earth-like planets (0.8-1.25 Earth radius) orbiting solar-type stars. A series of precise predictions on the planet yield are essential to optimize the payload design, target selection and observation strategy. For each different design (with different optics design, detector noise level, number of downloadable targets, observation time baseline and etc.), we generate a population of FGKM dwarfs (up to 1.2M stars) and their planetary systems according to the stellar properties from the TESS Input Catalog (TIC) v8.2 and the up-to-date planet occurrence rates from the latest Kepler and TESS results. Then we derive the detectability of each transiting planet with its Noise-to-Signal Ratio (NSR) which is mainly determined by its relative size and the combined noise (photon noise, stellar activity and instrument noises), observation duty-cycle and pipeline efficiency. For the optimized design, our simulation predicts that the ET mission would find over 30K different kinds of transiting planets of which about 5K are terrestrial planets. And the most important, ET would find 10-20 Earth 2.0s within the 4-year mission time.


PS23-A024
A Revisit of Mass-metallicity Trends in Transiting Exoplanets

Qinghui SUN1#+, Sharon WANG1, Johanna TESKE2, Luis WELBANKS3
1Tsinghua University, 2Carnegie Institution for Science, 3Arizona State University

The atmospheric chemical abundances of exoplanets reveal important information regarding planetary formation and evolution. The metallicities of gas giants could be very different under the two prevailing formation scenarios: 1) outer disk formation followed by migration, and 2) in situ formation. The gas giants are predicted to have decreasing metallicity with increasing planet mass under the migration scenario, while no such trend under the in situ formation scenario. By using the transmission spectra from the Hubble Space Telescope, Welbanks et al. (2019, W19) derived Na, K, and H2O abundances for a sample of 19 exoplanets that span from cool mini-Neptunes to hot Jupiters (Teq ∼ 300 - 2700 K). They found a weak trend that the H2O abundance increases with the decreasing planetary mass, and in general, the gas giants have substellar H2O while the Neptunes/mini-Neptunes have stellar/super stellar H2O. However, they lack Na, K, O abundances of the host stars, and the stellar abundances used to normalize the planet atmospheric abundances in W19 are usually [Fe/H] (or [M/H]) from the literature. In this talk, we show our thorough spectroscopic analysis used to derive the host stars' C, O, Na, S, K abundances, and present the rederived mass-metallicity trend using the re-normalized planet atmospheric abundances. We compute the Bayesian factors for both the linear regression model (in log scale, in fact a power law model) and the independent distribution model to test the validity of the trend. Our result suggests that the linear model is not obviously better than the independent distribution model for H2O, Na, and K. The additional Monte Carlo Simulations suggest that more high quality data will be needed to confirm (or reject) the mass-metallicity trend, which is promising in the era of JWST.


PS23-A014
Investigating Stellar Magnetic Fields from Kepler Light Curves: Difference Between Main-sequence Stars and Giant Stars

Jiapeng ZHU1#+, Jian GE2, Hui ZHANG3, Xinyu YAO2
1Shanghai Astronomical Observatory, Chinese Academy of Sciences, 2Chinese Academy of Sciences, 3Shanghai Astronomical Observatory

Stellar magnetic activities are the key to understand stellar formation and evolution and produce significant noises when detecting planet signals in stellar light curves and spectra. Among them, the flare activity is triggered by the interaction between the magnetic field, produced by the stellar dynamo, and the convection. Stellar flares can strongly influence planetary evolution via interaction with planetary atmosphere. To date, there are many statistical studies on stellar flares of main-sequence stars (MS) and giant stars independently, but few on their comparison following the stellar evolutional stage. The difference between their activities would provide insights into stellar dynamo evolution as the stellar structure (e.g., the convection size) varies from MS to giant stars. We analyzed Kepler light curves with flares and measured stellar flare magnetic fields and spot magnetic fields, and found that these two types of magnetic fields are correlated but located at two different branches in the flare and spot magnetic field diagram. It appears that the surface gravity (log g) dominates these two branches and giant stars have stronger magnetic fields than MS stars. Our new results will be reported.


PS23-A035
The Updated KMTNet Photometry Pipeline Powers Systematic Reanalysis of Achieved Microlensing Events

Hongjing YANG#+
Tsinghua University

Microlensing is a unique method that can find exoplanets in a wide mass range. We updated the photometry algorithms of the microlensing survey, the Korean Microlensing Telescope Network (KMTNet). The outcome noise is close to the photon Poisson noise. With this more stable and more accurate photometry data, we start a project to systematically reanalyze achieved microlensing events in the KMTNet database. The new data enable the discovery of previously missed anomalies in the light curves with low false positive rates. A statistical sample can be defined with the new data as well. I will present the updates of the photometry pipeline and the discoveries made by the new data.


Wed-02 Aug | 10:20 - 12:20 | MR307
PS11 - Microwave and Infrared Remote Sensing of Solar System Objects

Session Chair(s): Paul HARTOGH, Max Planck Institute for Solar System Research, Yi-Jehng KUAN, National Taiwan Normal University

PS11-A005 | Invited
Juno MWR and the Next Generation MWR for Ice Giants

Steven LEVIN1#+, Alexander AKINS1, Scott BOLTON2, Shannon BROWN1, Sidharth MISRA1
1Jet Propulsion Laboratory, California Institute of Technology, 2Southwest Research Institute

The Juno Microwave Radiometer (MWR) has measured radio emission from Jupiter’s atmosphere in 6 channels, at wavelengths ranging from 1.4 to 50 cm, over a wide range of latitudes, longitudes and emission angles. MWR has yielded a number of significant results, as well as prompting new questions, related to Jupiter’s atmospheric composition and dynamics at depths from 0.5 bar to 500 bar, distribution of lightning, and microwave reflection over the auroral region. MWR observations have also shed new light on Jovian synchrotron emission and on the ice shells of Ganymede and Europa. This experience has demonstrated the value of microwave radiometry for giant planets and their moons, and has also led to an improved design concept. We will describe the next-generation MWR, and how it could be used at Uranus and Neptune.


PS11-A002
Exploring Ice Worlds with Low-frequency Passive Microwave Radiometers: Insights from Juno MWR at Ganymede and Europa

Shannon BROWN1#+, Scott BOLTON2, Zhimeng ZHANG1, Matthew SIEGLER3, Jianqing FENG3, Steven LEVIN1, Sidharth MISRA1, David STEVENSON4, Lea BONNEFOY5
1Jet Propulsion Laboratory, California Institute of Technology, 2Southwest Research Institute, 3Planetary Science Institute, 4California Institute of Technology, 5Observatoire de Paris

On 7 June 2021, Juno had a close flyby of Jupiter’s moon Ganymede, flying within 1000 km of the surface and on 29 Sep 2022, Juno flew within 350 km of Europa. During each flyby, Juno’s Microwave Radiometer (MWR) observed the ice shell of each moon, partially mapping the microwave brightness temperature at six frequencies ranging from 600 MHz to 22 GHz. The radiance at these frequencies originates from successively deeper layers of the sub-surface and may reach to depths of 20km at 0.6 GHz. Pure water ice, particularly at the cold temperatures of Ganymede’s and Europa’s surface (~100K), is extremely transparent at low microwave frequencies (<10GHz). Microwave radiometers have been used to remotely probe temperature and physical properties of Earth’s ice sheets, but this is the first time they have been used to observe an icy moon. At cm-wavelengths, the signal originates from the subsurface at a depth dependent on the frequency, ice temperature, density, purity and liquid water content, allowing one to infer properties of the ice, such as temperature, composition and potentially depth. Multi-frequency microwave radiometers offer a unique way to “sound” the upper layers of the ice sheet. Here we report on the interpretation of the MWR observations and discuss what new constraints the data offer on the ice shell properties, including purity, sub-surface structure and conducting layer thickness. We will describe how future radar sounding measurements of the moons later in the decade, when combined with the passive observations, will help to further constrain the properties and reduce ambiguities in the interpretation of the passive microwave observations. Finally, Juno MWR was not designed to specifically to observe an ice shell. We will discuss basic design considerations for future radiometer instruments on deep space missions that will improve the information content returned.


PS11-A015 | Invited
Next Generation of Compact Wide-band Submm Instruments for Planetary Investigations

Imran MEHDI#+, Jose SILES, Goutam CHATTOPADHYAY, Alain MAESTRINI
NASA Jet Propulsion Laboratory

The successful mission of the Microwave Instrument on Rosetta (MIRO) and the upcoming launch of Submillimeter-Wave Instrument (SWI) on JUICE point to the unique capabilities of submm-wave instruments for planetary investigation. Recent technological advances have now made it possible to implement a new generation of submm-wave instruments that are compact but with tremendously enhanced capabilities in terms of sensitivity, bandwidth, and imaging capability. It is now possible to envision instruments weighing less then 10 kg with almost full coverage of the 500-600 GHz range with an array architecture. The receiver compactness is achieved by infusing advanced technologies such as CMOS based System-on-a-Chip that allow for enhanced capability with lower resources. An example of such a technology is the ASIC based digital backends that can provide required spectral resolution for planetary missions. The bandwidth of the instrument has been enhanced by successful demonstrating of on-chip power combining/dividing techniques that have now enabled sources that can provide over 20 mW of output power consistently over the 500- 600 GHz range, a critical piece of the spectrum for water and other critical molecules. Finally, larger LO power has made it possible to now entertain multi-pixel room-temperature based receiver systems that can provide imaging capability. Such instruments can provide tremendous increase in science throughput and could provide plume sensing, spectroscopy, and isotopic measurements for planetary body investigations.


PS11-A014 | Invited
Heterodyne Instrument Far-infrared Spectroscopy Space Telescope

Andrey BARYSHEV1#+, Martina WIEDNER2, Raymond BLUNDELL3, Paul GRIMES3, Asantha COORAY4
1University of Groningen, 2Paris Observatory, 3Center for Astrophysics | Harvard & Smithsonian, 4University of California, Irvine

The proposed NASA probe series FIRSST (Far-Infrared Spectroscopy Space Telescope) mission aims to study the formation and evolution of galaxies as well as comets in our solar system, with a key objective of determining H to D ratios to understand the origin of water on Earth.
The H to D ratio is critical in understanding the mechanisms that led to the formation of water in our solar system, including on Earth. By studying the ratio of hydrogen to deuterium in water vapor, researchers can gain insights into the origins of water on our planet.
The FIRSST mission will deploy a dual-band heterodyne instrument designed to study the H to D ratio with high sensitivity and spatial resolution. The instrument will operate simultaneously in two frequency bands around 570 GHz and 1.1 THz. The instrument will have dual polarization 5 pixel focal plane arrays that will allow for more efficient mapping of the sky and improved calibration in comparison to Herschel's HIFI instrument. The instrument's ability to make simultaneous dual frequency observations allows for more accurate determination of H to D ratios, particularly in time varying sources such as comets.
The Superconductor Insulator Superconductor (SIS) and Hot Electron Bolometer (HEB) mixer technologies of the instrument enables high spectral resolution and accurate measurement of molecular line profiles, which is essential for the precise determination of the H to D ratio, and for using line tomography to study the distribution of water and its isotope ratios in unresolved sources. This technology will pave the way for more detailed and accurate measurements of the H to D ratio in space, and in particular in comets.
We will discuss the instrument system and optical design, instrument predicted sensitivity and observing modes, that are particularly useful for observing comet bodies in the Solar system.


PS11-A010
Experimental Analysis of Terahertz Scattering from the Lunar Surface

Kazuma HIRAMATSU1#+, Yukio NAKANO2, SUYUN WANG1, Takayoshi YAMADA1, Yasuko KASAI3
1National Institute of Information and Communications Technology, 2Tokyo Gakugei University, 3Tokyo Instutute of Technology

The Lunar Terahertz Surveyor for Kilometer-scale Mapping (TSUKIMI) mission aims to obtain global-scale observations of the brightness temperature and physical parameters on the lunar surface and subsurface such as dielectric constant, water distribution map, and topographic roughness others. In satellite observations, topographic roughness is one of the predominant variables that determine radar scattering, thermal emission, optical reflectivity, and spectral radiance. Therefore, the verification of rough surface scattering in the terahertz band will support the future design of terahertz sensors with application to lunar exploration and promising to other planets. In this study, using a sample that simulates the lunar surface, we are exploring Brewster phenomena, monostatic and bistatic scattering at the terahertz band from the aspects of simulations and measurements. To comprehensively understand the physical mechanisms, we investigate the effects of rough surface properties in terms of root-mean-square (RMS) height, correlation length, rough spectrum, and dielectric constant, as well as the probing specifications concerning frequency, polarization, and observation angle on terahertz scattering. We further examine the roughness effect on the Brewster shift by the reflectivity model, which simultaneously accounts for the geometric and dielectric properties. The rough surfaces used for the measurements were made from Durable Resin V2 by 3D printing technology with statistically defined power spectral density, height probability density function, and variation of RMS height and correlation length, and the dielectric constant was measured by THz-TDS. The scattering measurement was conducted using transceiver module, two-stage polarizing component, and scattering chamber ranging from 330 to 500 GHz and we compared with the model. In this presentation, I will show the characteristics of Brewster's phenomenon and monostatic and bistatic scattering in the terahertz band with different rough surface conditions.


PS11-A001
Optimizing Deep Space Exploration: A Study on Efficient Data Processing for Lunar Resource Exploration Project TSUKIMI

Ryodo HEMMI1#+, Yasuko KASAI2, Takayoshi YAMADA1, SUYUN WANG1, Shigeru SATO1, Hideaki MIYAMOTO3, Takashi EISHIMA4, Narihiro OKUMA4, Hayato WATANABE5, Akihiro SHIBUYA5
1National Institute of Information and Communications Technology, 2Tokyo Instutute of Technology, 3The University of Tokyo, 4Axelspace Corporation, 5Space BD Inc.

The increasing size, complexity, and cost of deep space exploration missions pose challenges, and efficient exploration is necessary to revitalize the private space development and space industry. This study proposes an interface that combines existing software and exploration data to effectively derive continuous observation footprints and their data from satellite orbit and attitude information and observation equipment information. The research used spacecraft and planetary ephemerides data for the Moon resource exploration project "TSUKIMI" and simulated footprints on the Moon's surface. The study found that using a polar orbit with a periapsis close to the South Pole yielded footprints with high spatial density, and surface roughness, mineral ratios, surface temperature distribution, etc. can be obtained on a per-observation footprint basis from existing remote sensing databases. The research shows that more realistic exploration and observation information can be efficiently acquired beforehand by utilizing existing software and datasets and expanding their functions. In the future, the study aims to expand the functionality by using more detailed observation modes and schedules as inputs, expanding the Moon surface database, and constructing a user-friendly interface/platform with a business orientation.
Acknowledgments: This study is supported by the Ministry of Internal Affairs and Communications, Japan. (JPJ010777/JPMI00316).


Wed-02 Aug | 10:20 - 12:20 | MR334
PS18 - Planetary Atmospheres and Climates in and Beyond the Solar System

Session Chair(s): Feng DING, Peking University

PS18-A001 | Invited
Characterizing the Atmospheres of Temperate Rocky Planets in the Era of JWST

Thaddeus KOMACEK1#+, Yoav ROTMAN2, Erin MAY3, Thomas FAUCHEZ4, Geronimo VILLANUEVA4
1University of Maryland, 2Arizona State University, 3Johns Hopkins University Applied Physics Laboratory, 4NASA Goddard Space Flight Center

The advent of JWST has enabled the first broadband spectroscopic studies of rocky exoplanets in the infrared. Importantly, JWST will provide an opportunity to constrain the atmospheric composition of rocky exoplanets that lie within the habitable zones of late-type M dwarf stars. However, such observational characterization via transmission spectroscopy may be formidable due to challenges associated with stellar activity, atmospheric loss, and high-altitude aerosols. In this talk, I will discuss recent efforts to determine the extent that clouds impact the transmission spectra of temperate rocky exoplanets orbiting M dwarf stars. To simulate the impact of clouds on the climate state and observable properties of rocky exoplanets, we use the ExoCAM GCM post-processed with the Planetary Spectrum Generator (PSG) Global Emission Spectra (GlobES) radiative transfer code. I will present simulated transmission spectra both for idealized systems of rocky exoplanets orbiting M dwarf stars, as well as the best habitable zone candidate for characterization with JWST NIRSpec/PRISM, TRAPPIST-1e. We find that cloud coverage does not prevent detection of both the key habitability indicator water vapor as well as the potential carbon dioxide-methane biosignature pair in the atmosphere of TRAPPIST-1e over the nominal lifetime of JWST. Additionally, we find that the impact of climate variability on transmission spectra does not affect the detectability of spectral features in TRAPPIST-1e with JWST NIRSpec/PRISM. 


PS18-A003 | Invited
Combining 3D N-Body Simulations and Climate Modeling to Decipher the Climates of Exoplanets in Compact Multi-planet Systems

Howard CHEN1#+, Ravi KOPPARAPU2, Gongjie LI3, Adiv PARADISE4
1Florida Institute of Technology, 2NASA Goddard Space Flight Center, 3Georgia Institute of Technology, 4University of Toronto

Climate modeling has shown that tidal locking, particularly of terrestrial exoplanets orbiting M-dwarfs, can lead unique atmospheric dynamics and surface conditions. However, chaotic libration and rotation induced by planetary interactions in compact planetary systems may destabilize attendant exoplanets away from synchronized states. Here, we use a three-dimensional N-body integrator and an intermediately-complex general circulation model to simulate the evolving climates of TRAPPIST-1 e and f under the influence of different orbital and spin evolution pathways. Planet f perturbed by mean motion resonance effects are colder and dryer compared to their synchronized counterparts due to the zonal drift of the substellar point away from the eyeball open water belt. The differences between perturbed and synchronized planet e are minor due to higher instellation and warmer climates. This is the first study to incorporate the outcomes of direct gravitational N-body simulations into 3D climate modeling and our results show that planets at the outer edge of the habitable zones (OHZ) of multiplanet systems are vulnerable to rapid global glaciation. In the absence of external mechanisms such as orbital forcing or tidal heating, these planets could be trapped in permanent snowball states.


PS18-A007
Interaction of Planetary Atmospheres with Stellar Winds and Its Observational Manifestations

Ildar SHAIKHISLAMOV1#+, Maxim KHODACHENKO2, Marina RUMENSKIKH1,3, Artem BERESUTSKII1, Ilya MIROSHNICHENKO1
1Siberian Branch of the Russian Academy of Sciences, 2Austrian Academy of Sciences, 3INASAN

Among very diverse planetary populations, close orbiting hot exoplanets possess a unique feature of hydrodynamic outflow of upper atmospheres. This phenomenon was revealed for a number of hot Jupiters and warm Neptunes via observations of transit absorption in VUV lines of such elements as H, He, C, O, Mg, Si. The multicomponent and partially ionized atmospheric material overflowing with a supersonic velocity the Roche lobe collides with the stellar wind plasma. This interaction principally differs from the processes in tenuous planetary exospheres in the Solar system. The escape of upper atmospheres of hot exoplanets is a complex phenomenon, and quantitative interpretation of observational data requires numerical simulations. The comparison of spectrally resolved transit measurements of particular exoplanets and 3D simulations of their dynamical environments gives a tantalizing evidence of planetary and stellar winds interaction, enabling to draw important conclusions about both the atmosphere of an exoplanet and the parameters of the stellar wind plasma. In this talk, we summarize about two decades of a rapid development of the modelling approaches from relatively simple semi-empirical formulas to the large-scale 3D multi-fluid aeronomic models and global Monte-Carlo and MHD codes. Fast increase of quality and amount of observations, new instruments, new approaches to the probing of planetary winds, including the new spectral windows, multi-spectral and multi-instrumental observations of targets require further development of the modeling tools capable of complex simulation and interpretation of all available observations. // The recearch is carried out under RSF project 23-12-00134. MK acknowledges the support of FWF project I2939-N27, S11606.


PS18-A009
Interpretation of Transit Absorptions in the Atmosphere of HD-189733b

Marina RUMENSKIKH1,2#+, Ildar SHAIKHISLAMOV1, Maxim KHODACHENKO3, Artem BERESUTSKII1, Ilya MIROSHNICHENKO1
1Siberian Branch of the Russian Academy of Sciences, 2INASAN, 3Austrian Academy of Sciences

The atmosphere of hot Jupiters is heated by intense radiation of the host star and undergoes an outflow outside the Roche lobe. The transit spectroscopy of hot exoplanets is used to obtain the main characteristics of exoplanetary atmospheres and plasmaspheres, such as composition, temperature, density, as well as to study the effects that occur at interaction of planetary streams with the stellar wind. Many hot exoplanets consist mostly of hydrogen, and the Ly-a spectral line is valuable for providing evidence of atmospheric escape. However, it is strongly absorbed in interstellar medium and contaminated by geocoronal emission. As it was suggested in [1], the absorption by a metastable helium in the 23S state at 10830 Å offers an alternative way to probe the evaporating exoplanetary atmospheres. It is not affected by the interstellar medium and can be observed by ground telescopes with high resolution. A 3D gas-dynamic model which takes into account the processes of recombination and plasma-photochemistry of plasma components [2, 3] was used in this work to reproduce the transit absorptions in metastable helium 10830 A line of the planet HD-189733b to obtain the best fit to the observational data. As a result, the most probable atmospheric parameters for the case of HD-189733b planets have been determined. // The recearch is carried out under RSF project 23-12-00134. MK acknowledges the support of  FWF project I2939-N27, S11606 // References: [1] Oklopčić A., Hirata C. M., ApJ Lett., 2018. V. 855. No. 1. P. L11 [2] Shaikhislamov I. F. et al. MNRAS, 2018. V. 481. №. 4. P. 5315. [3] Shaikhislamov I. F. et al. MNRAS, 2021. V. 500. №. 1. P. 1404.


PS18-A010
Blowing in the Wind: Temporal Variability of Titan's High-altitude Circulation System

Martin CORDINER1#+, Theresa MARLIN2, Conor NIXON1, Richard COSENTINO3, Nicolas TEANBY4, Claire NEWMAN5, Ingo MUELLER-WODARG6, Eliot YOUNG7, Katherine DE KLEER2, Imke DE PATER8, Steven CHARNLEY1
1NASA Goddard Space Flight Center, 2California Institute of Technology, 3Space Telescope Science institute, 4Bristol University, 5Aeolis Research, 6Imperial College London, 7Southwest Research Institute, 8University of California, Berkeley

Recent observations of Titan using the Atacama Large Millimeter/submillimeter Array (ALMA) have revealed the presence of a surprisingly fast, time-variable zonal wind (jet) encircling the equator at high altitudes. This unexpected discovery presents a major challenge for our understanding of how momentum is transported throughout the atmospheres of terrestrial-like planets. Moreover, it reveals that Titan's wind field can vary on timescales as short as a few Earth months, yet the true magnitude and cadence of this variability remains poorly characterized. Further studies are also warranted because previous measurements of Titan's wind speeds (as a function of latitude), using optical refraction measurements are at odds with the recent ALMA data. Here we present results from a new, multi-epoch campaign to obtain Doppler (radio) and occultation (optical) observations of Titan's winds using state-of-the-art instruments. High resolution Doppler measurements of HNC, HC3N, CH3CN and C2H5CN in Titan's mid-to-upper atmosphere using ALMA reveal the wind velocities as a function of latitude, longitude, altitude and time. We also obtained near-simultaneous, high-cadence near-IR photometry of a stellar occultation by Titan on 2022-09-05, observed using the Keck, Gemini-N and IRTF telescopes, which provide an independent probe of the zonal wind field. This unique, multi-wavelength dataset allows us to investigate the origin, evolution, and stability of Titan's high-altitude jets, and for the first time, attempt to reconcile the discrepancy between prior optical and radio observations of the zonal wind velocities.


PS18-A011
Observed Dawn and Twilight Pressure Sudden Peaks in the Global Martian Surface and Possible Relationships with Atmospheric Tides

Chengyun YANG#+
University of Science and Technology of China

Multi landers and rovers on Mars have recorded the diurnal variation in surface pressure (ps) with two significant peaks that occur at dawn and dusk (around LT0800 and LT2000) at different locations. Previous studies suggest similar pressure variation was related to buoyancy waves driven by nearby topographic effects. These short-period surface pressure perturbations at specific local times are typically observed near the Martian equinox. Similar phase-locked surface pressure fluctuations are simulated by the Martian General Circulation Model at the Dynamic Meteorology Laboratory (LMD). The ps perturbation at a certain local time not only occurs at several different locations observed by multiple Mars landers and rovers, but also occurs over most areas of the middle and low latitudes, as suggested by GCM simulations. This phenomenon is thus likely to be global rather than local. By reconstructing the surface pressure variation from the horizontal mass flux, the pressure fluctuations in a sol can be attributed to the diurnal variation in the horizontal wind divergence and convergence in the Martain tropical troposphere in the GCM simulations. The background diurnal variation in ps is related to the diurnal migrating tidal wind, while the enhanced convergence due to the overlap of the 4-hour and 6-hour tides before LT0800 and LT2000 is responsible for the ps peaks occurring at dawn and twilight. Although the amplitudes of the 4-hour and 6-hour tides are smaller than those of diurnal tides, the phases of these tides remain similar in the Martain troposphere, which suggests that the convergences and divergences due to 4 h/6 h tidal winds at different altitudes are in phase and together create a mass flux comparable to that induced by diurnal/semidiurnal components and lead to rapid pressure fluctuations.


Wed-02 Aug | 1:10 - 3:10 | MR305
PS17 - Small Bodies: From Telescopic Observations To In-situ Explorations

Session Chair(s): Xian SHI, Shanghai Astronomical Observatory, Zhong Yi LIN, Institute of Astronomy

PS17-A015 | Invited
The Evolution of Dimorphos’s Ejecta from the DART Impact Revealed by the Hubble Space Telescope

Jian-Yang LI1#+, Toshi HIRABAYASHI2, Tony FARNHAM3, Jessica M. SUNSHINE3, Matthew M. KNIGHT4, Gonzalo TANCREDI5, Fernando MORENO6, Brian MURPHY7, Cyrielle OPITOM7, Steven CHESLEY8, Daniel SCHEERES9, Harold WEAVER10, Cristina A. THOMAS11, Eugene G. FAHNESTOCK8, Andrew F. CHENG12, Andy RIVKIN12
1Sun Yat-sen University, 2Auburn University, 3University of Maryland, 4United States Naval Academy, 5Departamento de Astronomía, Facultad de Ciencias, 6Instituto de Astrofísica de Andalucía, 7University of Edinburgh, Royal Observatory, 8Jet Propulsion Laboratory, California Institute of Technology, 9University of Colorado Boulder, 10Johns Hopkins University, 11Northern Arizona University, 12Johns Hopkins University Applied Physics Laboratory

NASA’s Double Asteroid Redirection Test (DART) spacecraft successfully impacted asteroid Dimorphos on September 26, 2022. The DART experiment provided a unique opportunity for understanding the ejecta evolution from asteroidal impact. We observed the evolution of the DART-driven ejecta with the Hubble Space Telescope from impact time T+15 min. The images revealed distinct features and complex patterns in the ejecta formed by the gravity of Didymos and solar radiation pressure (SRP). The particle size, ejection speed, and direction dominated the evolution of the ejecta. Ejecta with speeds >~2 m/s escaped the binary system directly, forming a cone-shaped morphology viewed from the side within T+8 hours. Slower ejecta with speeds a few times the escape speed was appreciably influenced by the gravity of Didymos, which slowly distorted the base of the ejecta cone to form curved and rotating features one day after the impact. This phenomenon is unique for the ejecta in a binary system. In the meantime, SRP pushed the ejecta toward the antisolar direction, continuously modifying the cone morphology and leading to the overlapping streaks pattern. The slowest dust formed a long, narrow tail starting from T+3 hours and lasting for months after the impact. Modeling suggested µm- to cm-sized particles in the tail with broken power law slopes of -2.6 and -3.7 for dust <~3 mm and larger, respectively. The distinct ejecta morphologies of Dimorphos’s ejecta and that of Comet 9P/Tempel 1 from Deep Impact are presumably related to their different volatile compositions and surface and subsurface conditions. The similar morphology of Dimorphos’s tail to those of some active asteroids thought to be due to impulsive dust emission caused by impact or rotational instability unambiguously demonstrates that impact is one key driver to generating active asteroids.


PS17-A013 | Invited
The ESA Hera Mission: Detailed Investigation of the NASA DART Impact Outcome and Characterization of the Binary Asteroid Didymos

Michael KUEPPERS1, Patrick MICHEL2#+, Paul A. ABELL3, Alan FITZSIMMONS4, Simon F. GREEN5, Monica LAZZARIN6, Seiji SUGITA7, Stephan ULAMEC8, Ian CARNELLI1, Paolo MARTINO1
1European Space Agency, 2Observatoire de la Côte d'Azur, 3NASA Johnson Space Center, 4Queen's University Belfast, 5Open University, 6University of Padova, 7The University of Tokyo, 8German Aerospace Center

The Hera mission is in development at the European Space Agency (ESA) in collaboration with JAXA for launch in October 2024. Consisting of a mother spacecraft and two cubesats, it will rendezvous with the binary asteroid (65803) Didymos in early 2027 and over the following 6 months will investigate the effects of the successful impact of the NASA DART probe and precisely measure the properties of Didymos and its small moon Dimorphos. DART successfully impacted on the 160 meter-size Dimorphos on 26 September 2022. Two weeks before impact, it deployed the Light Italian Cubesat for Imaging of Asteroids (LICIACube) that provided images during the few minutes following the impact. Observations from Earth and space provided distant images of the event, which were used to determine a reduction of 33 min in the orbital period of Dimorphos around Didymos. The Hera mission will investigate the outcome of the DART impact in detail. In particular, it will determine the effects of the impact on Dimorphos’ surface, e.g., whether it produced a crater, and if so its properties, and/or whether it led to global reshaping of Dimorphos. It will accurately measure the mass of Dimorphos, which will allow quantification of the momentum enhancement factor, which is a crucial parameter to evaluate the efficiency of the kinetic impactor technique. Hera will also determine in detail the physical, thermal and compositional properties of the asteroid, including the internal properties, which have a critical influence on the impact outcome. With Hera and DART together, we will have a fully documented deflection test and impact experiment that will allow us to verify our numerical impact models, to be able to extrapolate this deflection test to other asteroids and to improve our understanding of the complex geological properties and response of small asteroids.


PS17-A016
Revealing the Rings of the Centaur (10199) Chariklo from JWST Through a Stellar Occultation

Zhong Yi LIN1#+, Pablo SANTOS-SANZ2, Bryan HOLLER3, Altair R. GOMES JÚNIOR4, Bruno E. MORGADO5,6, John STANSBERRY3, Heidi B. HAMMEL7, Jose L. ORTIZ2, Bruno SICARDY8, Nicolás MORALES2, Josselin DESMARS8, Noemi PINILLA-ALONSO9, Richard FRENCH10, Estela FERNANDEZ-VALENZUELA9, Mónica VARA-LUBIANO2, Mike KRETLOW2, Damya SOUAMI11, Felipe BRAGA-RIBAS 12, Julio CAMARGO13,14, Gustavo BENEDETTI-ROSSI 15,14, Flavia L. ROMMEL13,14, Rene DUFFARD2, Marcelo ASSAFIN6,14, Rodrigo LEIVA2
1Institute of Astronomy, 2Instituto de Astrofísica de Andalucía (IAA-CSIC), 3Space Telescope Science Institute, 4Federal University of Uberlândia, 5Valongo Observatory, 6Universidade Federal do Rio de Janeiro, 7AURA Astronomy, 8Paris Observatory, 9University of Central Florida, 10Wellesley College, 11Observatoire de la Côte d'Azur, 12Universidade Tecnológica Federal do Paraná, 13Observatório Nacional, 14LineA, 15São Paulo State University

Rings around minor bodies have recently been discovered around the centaurs Chariklo (Braga-Ribas + 2014) and Chiron (Ortiz + 2015; Sickafoose + 2019), the dwarf planet Haumea (Ortiz + 2017), and the trans-Neptunian object Quaoar (Morgado + 2023). Such rings provide important clues to the dynamical and collisional history of the outer Solar System (Araujo + 2018; Wood + 2018), as well as to the formation mechanism of satellites, which is under debate after the discovery of the ring of Quaoar outside its Roche limit (Morgado + 2023). Another important open question is to unravel how these dense rings are confined and why they appear to be closer to the 3:1 spin-orbit resonance (Sicardy + 2019, 2020). With all this in mind, we predict and observe a stellar occultation by the ringed centaur Chariklo from JWST on October 18, 2022. We will present the results of this occultation detected by NIRCam as part of Heidi Hammel's GTO program ID 1271: ToO TNOs: 'Unveiling the Kuiper belt by stellar occultations' (PI: P. Santos-Sanz). This is the first stellar occultation observed from JWST and is a successful proof of concept of the feasibility of JWST to characterize solar system objects using this powerful technique. The challenging tasks performed to predict the stellar occultation visible from JWST and the instrumental setup used to observe this occultation will also be discussed. Finally, we will present preliminary results from this successful stellar occultation, showing us in-depth details of Chariklo's rings and possibly other structures.


PS17-A019 | Invited
Measuring Orbit Drift of Mars-crossing Asteroids by Yarkovsky Effect

Xin LIU1#+, Xiyun HOU1, Roberto ARMELLIN2
1Nanjing University, 2The University of Auckland

Mars-crossing asteroids (MCAs), also known as Mars crossers (MCs), are asteroids that can intersect the orbit of Mars. According to the Minor Planet Center, there are currently 20,501 known MCAs as of February 2023. The immigration rate of MCAs is high. The Yarkovsky effect now can be safely detected for some Near-Earth Objects (NEOs). However, it may not be easy to detect this effect for MCs because the observed Mcs are typically have diameters in the kilometer range and the Yarkovsky effect is weaker when compared with the NEOs due to their further distances from the Sun. Moreover, compared with the NEOs, the Mcs are more perturbed by the main-belt asteroids whose model still have large uncertainties nowadays. The goal of this study is to try to accurately measure the Yarkovsky effect of the MCAs. To this end, we plan to create a highly precise dynamical model by including ephemerides of large main belt asteroids and a ring structure for the remaining mass of the main belt main belt asteroids. We will then apply an initial candidate selection to all MCAs and use a standard orbit determination process to measure the Yarkovsky effect for the selected candidates. After the orbit determination, we will calculate the ratio between retrograde and prograde rotators and compare it with that of the NEO.


PS17-A002
A Photometric Study of Members of the Neos Atiras Population

Eduardo RONDON#+, Daniela LAZZARO
Observatorio Nacional

The observation of objects of the Atiras population is a challenge due to the narrow time-window in which observations are possible and, even so, at very low altitudes. This is due to the orbit of these objects, internal to that of the Earth. In this work we present the results of a photometric observational campaign of Atiras aiming to determine their physical parameters using the rotational light curve, the solar phase curve and the photometric spectrum. The period and amplitude have been determined for the asteroids (163693) Atira, (413563) 2005 TG45 and 2017 YH. In the case of (163693) Atira, we have determined a plausible rotational period P = 3 . 1532 ± 0 . 0001 , where the composite light curve presents structure usually related to the presence of a companion, as it has been suggested by radar observations of this asteroid. For asteroids (163693) Atira, (413563) 2005 TG45, (481817) 2008 UL90 and 2018 JB3 it was possible to derive the absolute magnitude and the phase coefficient. The obtained values are similar to those observed for asteroids with intermediate to low albedo. Finally, for asteroid (163693) Atira we have obtained a featureless photometric spectrum which is compatible in the Carvano taxonomic scheme with the Xp, Dp or Cp classes. No appreciable surface variations were observed for this object.


PS17-A034
Perihelion Activity of (3200) Phaethon is Not Dusty: Evidence from STEREO/COR2 Observations

Man-To HUI#+
Macau University of Science and Technology

We present an analysis of asteroid (3200) Phaethon using coronagraphic observations from 2008 to 2022 by the COR2 cameras onboard the twin Solar TErrestrial RElations Observatory spacecraft. Although undetected in individual images, Phaethon was visible in stacks combined from the same perihelion observations, yet only at small (≲30°) but not large (≳150°) phase angles. The observations are in line with the contribution from a bare nucleus, thereby seriously contradicting the interpretation based on HI-1 observations that attributes the perihelion activity to the ejection of μm-sized dust. We obtained an upper limit to the effective cross section of μm-sized dust to be ≲105 m2, at least three orders of magnitude smaller than earlier estimates based on HI-1 data. On the contrary, the COR2 observations cannot rule out the existence of mm-sized or larger debris around Phaethon. However, the fact that no postperihelion debris tail has ever been detected for Phaethon suggests the unimportance of such dust in the perihelion activity. We thus conclude that the perihelion activity of Phaethon is highly unlikely relevant to the ejection of dust. Rather, we deduce that the activity is associated with gas emissions, possibly Fe I and/or Na D lines. To verify our conjecture and to fully understand the perihelion activity of Phaethon, more observations at small heliocentric distances are desired. We compile a list of observing windows ideal for the search of gas emissions of the asteroid from ground telescopes. The best opportunities will be during total solar eclipses. The detailed description of the analysis was published as Hui (2022, AJ, 165, 94).


PS17-A004
The Common Trend of Saltation Particle on the Surface of Fast Rotating Asteroids

Song ZHIJUN1+, Yu YANG1#, Cheng BIN2, Wenyue DAI2, Jing LV1, Baoyin HEXI2
1Beihang University, 2Tsinghua University

The asteroid spun up to its critical limit has unique surface mechanical properties, that the gravity and the centrifugal force largely balance, creating a relaxation environment where low-energy events like mass shedding may trigger the long complex subsequent motion of the regolith grains. Exploring such an evolution process may provide key clues for understanding the early formation of multi-asteroid systems. This paper investigates the complex evolution process of loose particles triggered by shedding events and the dependency of their dynamical propagation on the contact mechanical properties of the asteroid surface. We present a numerical model for tracking the trajectory of the shed particle that considers the collision between the particle and the asteroid’s surface. Monte Carlo simulations are performed to reflect the statistical behavior of shed particles. Zero-velocity surfaces are introduced to our data-based analysis in order to reveal the intrinsic invariance of the evolutionary processes. The average mechanical energy of the particle cloud is employed to check the connection between their contact property and the temporal-spatial distribution of the shed particles. We sketched a common evolutionary path of the particle in the vicinity of a fast-rotating asteroid, i.e., particles dislodged from the unstable region will eventually enter, through several collisions with the surface, non-return orbits which are launching from the minimum geopotential area of the unstable region. We take this trend as an invariant property for asteroids near their critical spin limits, independent of particular asteroid morphology, and all shed particles (no matter where they originate from) will enter the same evolutionary path. We also find orbital energy of the particle cloud is statistically independent of the surface contact property, meaning that the collision coefficient of restitution is a non-sensitive parameter in the outward spreading process of the shed particles.


PS17-A017
Shape, Morphology and Spin-axis Evolution of Kuiper Belt Objects Due to Nucleus Activities

Yuhui ZHAO1#+, Ladislav REZAC2, Yuri SKOROV2
1Chinese Academy of Sciences, 2Max Planck Institute for Solar System Research

One of the key findings of the Rosetta mission to the Jupiter family comet 67P/CG was its peculiar bi-lobed shape along with the apparent north/south dichotomy in large scale morphology. This has reignited scientific discussion on the topic of origin, evolution and age of the nucleus. In this work we aim to investigate the role of activity on the overall shape, spin axis, and orbit evolution for comet candidate objects during their ‘storage’ phase in the Kuiper belt. We consider four classes of three-dimensional (3D) shapes for various initial condition of spin-axis and orbital parameters, propagating them for ~109 years. Accounting for solar driven CO ice sublimation (and Knudsen diffusion), we estimate the spin states change and derive upper limits on mass loss distribution on the surface. The results provide argument for activity driven origin of large scale morphology structures, as well as significant alteration of pre-existing landforms due to sublimation. Furthermore, we suggest that the peculiar oblate shape of Arrokoth, which is visited by New Horizons mission, could be of evolutionary origin due to volatile outgassing in a timescale of about 1–100 Myr, while its spin state would not be dramatically affected. We further argue that such a process may be ubiquitous in the evolution of the shape of Kuiper belt objects shortly after their formation. This shape-changing process could also be reactivated when Kuiper belt objects dynamically evolve to become Centaurs and then Jupiter-family comets and receive markedly increased solar heating.


PS17-A018
Progress in Mission Design of Crown: A Constellation of Heterogenous Wide-field Neo Surveyors

Xiaojing ZHANG#+
China Academy of Aerospace Science and Innovation

Only approximately one third of the total estimated population of NEOs ≥ 140 m in diameter (Potentially Hazardous Objects, PHOs), which are capable of causing extensive damage on regional or global scales resulting in extreme loss of life and property, have been found to date. Thus discovering the remaining NEOs within this size range has been recognized as a high priority (Stokes et al., 2003; 2017). Once a PHO is identified, subsequent characterization of the object is required to assess the threat in order to perform the right mitigation efforts. Here we present the progress of the mission concept study for an distributed NEO surveillance system also referred to as CROWN – the Constellation of heteRogeneOus Wide-field Near-earth objects surveyors (Huo et al., 2019). A-sub 2500 kg spacecraft system (one mothership plus six daughter microsat) will be deployed on the Venus-like orbits to search and spectrally inspect PHOs. The transfer and deployment trajectories of the proposed constellation are investigated based on the three-body problem model. The deployment can be completed within five years using values of less than 300 m/s velocity increment. The surveillance constellation can be applied for asteroid orbit determination (OD) and the OD accuracy is approximately 5 km after 40 days of measurement using one surveyor or 10 days of measurement using two different surveyors. Furthermore, we investigated a concept of carrying a nano-size lander housing a set of scientific instruments to perform opportunistic in-situ characterization of a PHO or an asteroid with potential value. Detailed estimates of all critical subsystem parameters were derived to demonstrate the feasibility of this concept.


Wed-02 Aug | 1:10 - 3:10 | MR307
PS08 - Science and Exploration of Mars and Venus

Session Chair(s): Yeon Joo LEE, Institute for Basic Science, Varun SHEEL, Physical Research Laboratory

PS08-A013 | Invited
Methane on Mars: A Survey of Detection Attempts and Mechanisms to Explain Its Presence

Franck MONTMESSIN1#+, Kevin OLSEN2, Franck LEFÈVRE1, Jean-Loup BERTAUX3, Lucio BAGGIO1, Anna FEDOROVA4, Elise W. KNUTSEN1, Abdenour IRBAH1, Gaétan LACOMBE5, Andrey PATRAKEEV4
1National Center for Scientific Research (CNRS) / Laboratoire Atmosphères, Observations Spatiales (LATMOS), 2Oxford University, 3University of Versailles Saint-Quentin-en-Yvelines, 4Space Research Institute of Russian Academy of Sciences, 5Laboratoire "Atmosphères, Milieux, Observations Spatiales" (LATMOS)

Since the 2004 report of multiple detections of methane on Mars by several teams, its presence has laid the ground for a framework to explain its presence or to confirm it by superior detection means. Since the lifetime of methane should prevent it from appearing and disappearing on short time scales, several scenarios have been proposed to explain how a local and intermittent release could mimic the behavior of methane as reported when associated with specific chemical pathways or mechanisms not yet accounted for. In parallel, attempts to detect methane have been made from the surface of Mars with Curiosity and from the orbit by the Mars Express and Trace Gas Orbiter missions, leading to conflicting measurements and interpretations. In this work, we will present a comprehensive overview of all studies conducted so far to elucidate its presence and potential causes.


PS08-A017
Mars Methane: Can Both MSL and TGO Be Correct?

Scot RAFKIN1#+, Jorge PLA-GARCIA2, Alison BRIDGER3
1Southwest Research Institute, 2Centro de Astrobiología (CSIC-INTA), 3San Jose State University

The Mars methane mystery has not yet been resolved. In situ detections by the Mars Science Laboratory (MSL) indicate methane background concentrations of ~0.5 ppbv with occasional spikes an order of magnitude larger. In contrast, the Trace Gas Orbiter (TGO) has found no evidence of methane down to threshold detection levels. We utilize high resolution (~3 km grid spacing) mesoscale model simulations with Eularian tracers and Lagrangian trajectory modeling driven by the model winds to evaluate the possibility that methane released at the surface could be detected by MSL and not detected by TGO. The complex, 3-D nature of methane transport and diffusion in the atmosphere is revealed, and considering the possibility of rapid near-surface methane destruction, we identify specific cases where both MSL and TGO could be valid and discuss the likelihood of such events.


PS08-A014 | Invited
Sounds from Mars : Results of the Microphones on Perseverance

Ralph LORENZ#+
Johns Hopkins University Applied Physics Laboratory

Mars 2020/Perseverance is the first planetary mission to return significant amounts of human-audible acoustic data. In addition to their public appeal, these data reveal important aspects of the Martian environment. Positioned on the rover’s mast, the SuperCam microphone records sounds from 20 Hz to 10 kHz. A separate body-fixed microphone is associated with the EDL cameras. Detected sounds originate from three main sources: the atmosphere (turbulence, wind), the crack of the SuperCam laser blasts on rocks, and other artificial sounds, such as the compressor pump on MOXIE, or the aeroacoustic signal generated by the high-speed rotating blades of the Ingenuity helicopter. (i) the turbulence/wind-induced acoustic signal starts from the lowest frequency, continuously up to few hundred Hz depending on the wind activity, with a spectral slope consistent with the dissipative regime. (ii) The laser-induced spark lies at higher frequencies (2 - 10 kHz) where it shows destructive interference gaps due to echoes on the mast structure. (iii) Three of the Ingenuity helicopter flights are heard, at the blade’s passing frequency of ~84Hz (with a small Doppler shift due to flight speed) and its first harmonic at 168 Hz. Passive microphone observations are now made routinely to characterize turbulence, where the observations can access timescales shorter than conventional wind sensors. Similarly, the propagation times of the crack sounds from rapid series of laser shots can interrogate temperature fluctuations on length scales smaller than is possible with conventional temperature sensing. The observations also constrain the acoustic propagation in the Martian atmosphere, where the abundant CO2 causes appreciable attenuation, especially at high frequencies. This presentation will review results to date. By Ralph Lorenz, Baptiste Chide, Sylvestre Maurice, Naomi Murdoch, Alexander Stott, David Mimoun and the Mars 2020 Acoustic Working Group and Atmospheres Working Group.


PS08-A021
The Influence of Dust on the Atmosphere of Mars as Seen by the Radio Science Experiments on Mars Express and Mars Global Surveyor

Silvia TELLMANN1#+, Martin PATZOLD2, Kerstin PETER1, Bernd HÄUSLER3, David P. HINSON4
1Rhenish Institute for Environmental Research, 2RIU-Planetary Research at University of Cologne, 3Universität der Bundeswehr München, 4Stanford University

The low atmospheric pressure as well as its pronounced topographical diversity lead to a highly dynamical atmosphere on Mars. Atmospheric dust, lifted from the surface, transported to other regions where sedimentation occurs has a strong influence on the dynamical processes on Mars. Atmospheric dust absorbs solar radiation and emits in the infrared, influencing the local weather as well as the global climate via diabatic heating and cooling. Dust is therefore strongly correlated with atmospheric waves, clouds, and the transport of aerosols and atmospheric species. Its importance is comparable to the water cycle on Earth. The atmospheric heating can have strong effects even far away from the surface in the thermosphere.
The Mars Express Radio Science Experiment MaRS retrieves vertical profiles of the refractive index from the lower atmosphere to the topside of the ionosphere. These measurements are used to derive temperature, pressure, and neutral number density profiles in the lower atmosphere (from a few hundred metres above the surface up to ~ 40-50 km) and electron density profiles in the ionosphere of Mars. The atmospheric profiles have a high vertical resolution of only a few hundred metres. They contain valuable information about small scale vertical structures as the planetary boundary layer, or small-scale gravity waves. Radio waves are not sensitive to dust. They can propagate through dust loaded atmosphere which is inaccessible for other instruments. Additionaly, radio occultation data from Mars Global Surveyor (MGS) will be used to study the influence of dust over an extended time range. The atmospheric measurements can be used in combination with the information about atmospheric dust determined independently by other instruments, to study the influence of atmospheric dust in the lower atmosphere. Possible correlations between atmospheric heating, enhanced wave activity, and the atmospheric dust content can therefore by revealed.


PS08-A011
Recent Improvements of the Mars PCM to Better Model the Martian Dust Cycle

Ehouarn MILLOUR1,2#+, Francois FORGET3, Aymeric SPIGA1, Antoine BIERJON1
1Sorbonne Université, 2National Centre for Scientific Research, 3University Pierre et Marie Curie

Our Mars Planetary Climate Model (Mars PCM, formerly known as the LMD Global Climate Model) simulates all the details of the atmospheric environment of Mars. It is developed at LMD (Laboratoire de Meteorologie Dynamique, Paris, France) in close collaboration with several teams in Europe (LATMOS, France, University of Oxford, The Open University, the Instituto de Astrofisica de Andalucia), and with the support of ESA (European Space Agency) and CNES (French Space Agency). It is used to generate the Mars Climate Database (MCD), the latest version (version 6.1) of which was released in 2022. At AOGS we will report on specific work in the implementation of parametrizations related to improving the Mars PCM modeled dust cycle concerning:
- The implementation of a dust injection scheme interactively driven by target atmospheric dust scenarios (based on observations).
- The implementation of a parametrization of "rocket dust storms" which now allows to generate the enigmatic detached dust layers observed between 20 and 30 km altitude, but only during the dust storm season.
- The implementation of a dust injection recycling due to winds along the flancs of salient topographical obstacles (such as volcanoes), which help generate dust detached layers during the clear season.


PS08-A022
Characterization of Boundary Layer Turbulence at Different Locations on Mars

Varun SHEEL#+, Shefali UTTAM
Physical Research Laboratory

The Martian boundary layer is the lowest part of the atmosphere that is directly influenced by the surface. It responds to the surface forcing in a timescale of an hour or less, therefore the vertical mixing is strong. It is important in the Martian atmosphere, as it is the source of dust injection that leads to dust loading, dust devils and local and regional dust storms. The local topography, solar radiation, and dust content in the atmosphere play a key role in guiding the local and regional scale meteorology and local turbulence of the atmosphere, which cannot be computed by a global scale model. The dust present in the atmosphere also affects the spatial and temporal variability of the turbulence within the boundary layer. We use a mesoscale model (LMD-Mars Mesoscale Model) to study about the local and regional scale meteorology and turbulence on different locations of Mars. The locations chosen in this work are: (1) Arsia Mons (~8°S, ~120°W); (2) Gale Crater (~5°S, ~137°E); (3) Jezero Crater (~18°N, ~77°E); (4) Pathfinder landing site (~19 °N, ~33 °W); and (5) Insight landing site (~4 °N, ~136 °E). The computations are carried out for ~10 days during the southern summer season (Ls = ~297º). The effect of dust on the local meteorology, and difference in the turbulence at these locations, during varying atmospheric dust loading, will be discussed in this presentation.


Wed-02 Aug | 3:30 - 5:15 | MR305
PS17 - Small Bodies: From Telescopic Observations To In-situ Explorations

Session Chair(s): Man-To HUI, Macau University of Science and Technology, Jian-Yang LI, Sun Yat-sen University

PS17-A021 | Invited
Temporally Distributed Parent Body Accretion in the C Reservoir of the Early Solar System

Wladimir NEUMANN1,2#+, Audrey BOUVIER3, Mario TRIELOFF4
1Technical University Berlin, 2German Aerospace Center, 3Bayreuth University, 4University of Heidelberg

Planetesimal melting and differentiation require heating that can be provided by 26Al, but only early after the formation of Ca-Al-rich inclusions (CAI). Thus, achondrite parent bodies (PB) are considered to have formed early (and mostly in the NC region). Late accretion in the C region is believed to have produced chondritic objects, e.g., the CR PB that formed close to 4 Ma after CAIs. Aqueous alteration of Ryugu, CI, and CM samples suggests similar accretion times. However, presence of evolved CR-like achondrites suggests earlier accretion also in the C reservoir. The meteorite record provides only weak accretion time estimates from chondrule or mineral phases´ formation ages, and no information about the PB size. However, thermal evolution and differentiation modeling provides a valuable tool for constraining the PB accretion time (and size, internal structure, and meteorite layering depths). Temperature and porosity evolution models showed that Ryugu´s PB was <10 km and formed at ≈1-3 Ma, while CI and CM carbonate formation ages are reproduced in PBs of 20-25 km that accreted at ≈3.75 Ma after CAIs. More precisely, models can be fitted to the thermo-chronological data. Fits for Flensburg, CR, NWA 011, and NWA 6704 (altered chondrites, equilibrated chondrites, and achondrites) suggest a temporally distributed accretion ranging from 0 Ma to ≈4 Ma, with ≈3.7 Ma, ≈1.5-2.75 Ma, ≲0.6 Ma, and ≲0.7 Ma for CR, Flensburg, NWA6704, and NWA011 PB, resp. These results imply that accretion processes in the C reservoir started as early as in the NC reservoir and produced differentiated PBs with carbonaceous compositions in addition to undifferentiated CC PBs. Accretion times correlate inversely with the meteorite alteration, metamorphism, or differentiation degree, and those for CI, CM, Ryugu, and Tafassites of ≈3.75 Ma, ≈3.75 Ma, ≈1-3 Ma, and ≈1.1 Ma, resp., fit well into this picture.


PS17-A009 | Invited
The Next-generation Ground-based Planetary Radar: Distributed Aperture Deep-space Radar

Zehua DONG#+, Tao ZENG, Zegang DING, Tianyi ZHANG, Yangka WEI, Teng LONG
Beijing Institute of Technology

Planetary radar is the most powerful method for post-discovery, remote physical and dynamical characterization of near-Earth objects (NEOs). Radar observations of NEOs can constrain their sizes and shapes, prevent newly discovered objects from being lost, reduce uncertainties on orbital elements by orders of magnitude, and greatly improving impact probability estimates compared to optical-only datasets. The key facilities for planetary radar are the 305-meter Arecibo Observatory (decommissioned in 2020 after two cable failures) in Puerto Rico and 70-meter Goldstone Solar System Radar (GSSR) in California, which play a critical and unique role in the tracking and characterization of near-Earth objects in past decades. However, the Arecibo and GSSR are Centralized system which uses a single-dish antenna and high-power transmitter, so the observation range is limited by physical constraints of antenna size and transmitter power. Here, we report innovative concept and latest research progress of the distributed aperture deep-space radar system, which consists of dozens of 30-meter radars and can be equivalent to a large-scale radar via coherent signal processing technology that aligning the phases of electromagnetic waves transmitted by each radar. The system would become the most powerful planetary radar in the world when it is completed in 2027 and its observation range can be constantly extended by increasing the quantity of radars. We believe that the distributed aperture deep-space radar system will play a critical role in planetary science and planetary defense in future.


PS17-A014
ALMA Mapping of Volatiles Produced from the Nucleus and Coma of Comet 46P/Wirtanen

Martin CORDINER#+, Stefanie MILAM, Nathan ROTH, Steven CHARNLEY
NASA Goddard Space Flight Center

The molecules observed in cometary atmospheres (comae) originate primarily from outgassing due to the sublimation of nucleus ices, whereas some molecules are produced by secondary chemical processes in the coma. The majority of cometary gases observed at radio wavelengths have yet to be mapped, so their production mechanisms, and therefore their abundances inside the nucleus, remain uncertain. Here we present observations of six molecular species in the coma of comet 46P/Wirtanen, obtained using the Atacama Large Millimeter/submillimeter Array (ALMA) during the comet's extremely close (~0.1 au) approach to Earth in December 2018. Interferometric maps of HCN, HNC, CH3OH, CH3CN, H2CO and CS were obtained at an unprecedented sky-projected spatial resolution of up to 25 km, enabling the nucleus and coma sources of these molecules to be quantified. These unique observations reveal HCN, CH3OH and CH3CN spatial distributions that are consistent with primary production from direct outgassing by the nucleus, whereas CS, HNC and H2CO are found to originate predominantly from distributed sources in the coma.


PS17-A020
Ceres Endogenous Activities and Implications for Its Origin, Evolution and Habitability

Ottaviano RÜSCH1#+, Antonio GENOVA2, Lynnae C. QUICK3, Wladimir NEUMANN4
1Westfälische Wilhelms-Universität Münster, 2Sapienza University of Rome, 3NASA Goddard Space Flight Center, 4Technische Universität Berlin

The NASA Dawn mission and its international instrument payload performed orbital measurements of dwarf planet Ceres from 2015 to 2018. Observations revealed the dwarf planet as a partially differentiated, volatile-rich world, capable of endogenous and geologically-recent activity. Here the evidence and implications for this activity is reviewed based on three kinds of data. First, optical images and derived topography revealed the presence of relatively bright 1-10 km large topographic reliefs, which three-dimensional shapes indicating material extrusion onto a preexisting surface (e.g., Ahuna Mons, Cerealia Tholus). Second, near-infrared observations indicated the extruded material is rich in carbonates, ammoniated- and Mg-phyllosilicates, as well as hydrated sodium chlorides. The presence of aliphatic organic compounds has been additionally suggested, although it is unambiguously detected only elsewhere on Ceres, away from sites of endogenous activity. Water ice is probably present as well, although its surface sublimation constrains its detectability to spatially limited (<km) spots. Third, a gravity anomaly is present beneath one of the most recent domes, suggesting a deep-seated mantle source of the cryovolcanic extrusive material. Furthermore, an interplay between endogenous and exogenous-driven activity is suggested for domes within impact craters. Evidence from these three kinds of orbital data strongly suggest the presence of brines in Ceres mantle and in the near-subsurface (~m), potentially still liquid today or in the recent (few Myr) past. Among several key questions relating to the origin, evolution and habitability of protoplanets, future spacecraft missions could determine the chemical evolution of the brines and of the organic compounds. Surface in situ measurements would be highly valuable to accomplish this task and would require a good understanding of the local scale and near surface properties of Ceres.


PS17-A022
Mengxi - Ceres Exploration Program

Robert WANG1#+, Jiaqi CHEN2, Pingping LU1, Yanan DANG1
1Chinese Academy of Sciences, 2Hohai University

Ceres, located between Mars and Jupiter, is the largest object in the asteroid belt and the only dwarf planet in this region. The Dawn mission discovered organic material on the surface of Ceres and found liquid ocean in its interior. The Mengxi mission plans to explore Ceres through an orbital exploration, utilizing a suite of instruments including a surface penetrating radar, terahertz radiometer, and integrated image and spectral detector. The mission aims to achieve the following scientific objectives: 1) Quantitatively measure the fugitive gas content in Ceres' exosphere and analyze its variation over space and time. Explore the origins of water on Earth and Ceres by analyzing the homology of water on them and comparing the hydrogen-oxygen isotopic characteristics and water chemistry. 2) Explore the subsurface structure and composition of Ceres, observe water-conducting channels between the subsurface ocean and the surface, and study the distribution, depth, form, and activity of the subsurface ocean. 3) Identify cryovolcanic eruptions around cryovolcanoes and their surroundings, analyze the material and geological composition and activity of these regions. 4) Determine the distribution and isotopic characteristics of ammonia gas to unravel the mysteries of Ceres' origin through observing Ceres' molecular lines of rarefied atmosphere. The Mengxi mission has designed a three-in-one payload design scheme to address these scientific objectives, defining core technical indicators, and identifying corresponding key technologies, expected results, and existing risks. This promotion and implementation of this mission will be of great significance in revealing the early history and evolution of the Ceres, Earth, and solar system.


PS17-A006
Hopping Dynamics of the Internal-torque-actuated Small Body Surface Rover

Yonglong ZHANG1,2#+, Xiangyuan ZENG3
1Taiyuan University of Technology, 2Tsinghua University, 3Beijing Institute of Technology

Small body exploration is a popular topic in deep space exploration. Roving on the surface of small bodies can achieve particular and abundant scientific data. The hopping rover, especially the internal-torque-actuated hopping rover, is currently recognized as one of the most suitable type for small body surface exploration. Although such rovers have been successfully demonstrated in the Hayabusa 2 mission, their dynamical problem of its hopping motion has not been studied enough. Consequently, this paper first builds the rover’s hopping dynamical model based on the Polygonal Contact Model in considering the flywheel braking process. The hopping motion is then numerically simulated on two kinds of planes, including an ideally flat plane and a complex rocky terrain. Furthermore, numerical studies of the rover’s hopping process are implemented by considering the flywheel’s non-constant reaction torque during braking, the multi-contact, the surface deformation, and the slip cases. Particularly, the multiple times of micro-contact phenomenon between the rover and the small body surface before the departure is discovered. The effect of the flywheel’s braking process, contact stiffness, and friction coefficient on the hopping characteristics of the rover are investigated. Moreover, their intrinsic dynamical mechanisms are also illustrated. This study could provide a reference for future missions that require roving on the surface of a small celestial body.


PS17-A011
Accelerating Discrete Polyhedral-element Method with CUDA

Tongge WEN#+, Xiangyuan ZENG
Beijing Institute of Technology

Recent space missions reveal that most small bodies have rubble-pile structures and they are gravitational aggregates of loosely consolidated materials. Discrete Element Method is one of favorable numerical tools in studying those bodies. Classical spherical representation of granular particles loses the shape feature of angular particles, which may be inappropriate for problems where particle shape plays a significant role. This paper presents a numerical implementation of the discrete polyhedral-element method (DPEM) in using non-spherical particles. The work builds up on a previous code implementation and extends its capabilities. A parallel algorithm is proposed to accelerate the DPEM code with CUDA (Compute Unified Device Architecture). The linear bounding volume hierarchy technique is introduced to handle contact detection between non-spherical particles. Morton Code is adopted to transform the construction of the Bounding Volume tree into a sorting problem; therefore, the tree can be traversed into a top-down manner. Such an implementation is more suitable for GPU architecture, and it can minimize the divergence in GPU. Benchmarking test of elastic collision between spheres is performed to monitor the accuracy and convergence of the code as a validation. Low-velocity impact of a lander on the regolith surface of a small body is investigated by using the above method. Dynamical responses of the lander and the particle bed by varying the physical properties of the regolith are systematically explored, which could provide reference for lander deployment on gravel terrains.


PS17-A003
Virtual Asteroid Generation and Application

Xizhi LI#+
Shanghai Astronomical Observatory

The complex shape of asteroids and comets is the joint outcome of various geological processes that define their present physical state, provide insight into their past, and serve as a geological basis for their subsequent evolution. Current remote or in-suit observations of the small bodies reveal only a tiny fraction of their total shape but form the basis of our knowledge. Therefore, numerical simulation is employed as another powerful tool to provide clues and constraints on the formation and evolutionary history of small bodies, e.g., by simulating impact cratering, and various interior mass distributions.
In this paper, we propose a numerical approach to constructing virtual asteroids at any spatial resolution. The aim is to test the influence of asteroid shapes with various internal differentiations and surface morphologies for any scientific or operational investigations. More precisely, we modeled virtual asteroid shapes with different mass distributions using a non-uniform sphere packing algorithm, and synthesized high-resolution topography with user-defined, locally controlled spot noise models. Having a realistic virtual asteroid or comet allows for testing mission scenarios using an object that looks real and whose internal differentiation, and surface material properties match the type of object we plan the mission for (at least to the best of the current state of knowledge about that object). This is fundamental to many applications such as navigations, classifications, shape reconstructions, and dynamical evolution simulations. We demonstrate how this technique can be used to generate a variety of asteroid shapes that combine stochastic internal differentiations and topographies.


Wed-02 Aug | 3:30 - 5:15 | MR307
PS08 - Science and Exploration of Mars and Venus

Session Chair(s): Shuanggen JIN, Henan Polytechnic University, Durga Prasad KARANAM, Physical Research Laboratory

PS08-A003
Atmospheric Evolution of Mars Indicated by C, N, Ar, and H Isotopes

Renyu HU#+
Jet Propulsion Laboratory, California Institute of Technology

The isotopic composition of carbon, nitrogen, argon, and hydrogen in Mars's atmosphere, together with the extent of carbonates, nitrates, and hydrated minerals found on the planet, provides information about its atmospheric evolution. We have developed a novel model to trace the evolution of the Martian atmosphere, including the impacts of outgassing, escape to space, and sequestration into the crust. Recognizing that the evolution involves a trajectory in a multi-dimensional phase space of many variables, we have used a million-model approach to rigorously perform quantitative tests against the isotopic composition of the atmosphere and the size of crustal volatile reservoirs. I will show that the current atmospheric 13C/12C ratio points to an evolutionary history of CO2 that started from a moderately dense atmosphere (i.e., <~1 bar) after the Late Heavy Bombardment. Only scenarios with large amounts of carbonate formation in open lakes permit higher pressures up to 1.8 bar. I will also show that a previously unknown family of evolutionary solutions can explain the isotopic composition of nitrogen, without invoking a multi-bar early CO2 atmosphere or excessive outgassing in the Amazonian. This new family of solutions implies that Mars had an N2-rich early atmosphere, with a partial pressure of ~0.3 bar. The outgassing models are consistent with the constraints from Ar’s isotopic composition and suggest mantle sources with the oxygen fugacity more reduced than IW. Lastly, I will discuss how ocean-scale volumes of water on ancient Mars are simultaneously compatible with the evidence of widespread hydrated minerals, H escape rate estimates, and D/H measurements. Collectively, these empirical constraints indicate a multi-component atmosphere in the late Noachian and provide a new path forward to explain the geologic records that suggest intermittent conditions for liquid water on ancient Mars’s surface.


PS08-A002
Martian Proton Aurora Brightening Controlled By Solar Wind Dynamic Pressure

Fei HE1#+, Kai FAN1, Andrea HUGHES2, Yong WEI1, Jun CUI3,4, Markus FRAENZ5, Zhaojin RONG1, Xiao-Xin ZHANG6
1Institute of Geology and Geophysics, Chinese Academy of Sciences, 2Embry-Riddle Aeronautical University, 3Sun Yat-sen University, 4Chinese Academy of Sciences, 5Max Planck Institute for Solar System Research, 6National Center for Space Weather, China Meteorological Administration

Ion loss during solar events early in Mars history may have been the major cause to the long-term evolution of the Mars atmosphere. Restricted by observation data, the relationship between ion loss and solar wind is still in debate. The Martian proton aurora is a distinct aurora phenomenon resulting from the direct deposition of solar wind energy into Mars’ dayside atmosphere. What solar wind parameters influence the aurora activity in the short term is yet unknown, as are the associated repercussions in the Martian atmospheric ion loss. Using MAVEN observations, we have found observational evidence of synchronized proton aurora brightening and atmospheric ion loss intensifying on Mars, controlled by solar wind dynamic pressure. The solar wind dynamic pressure possibly has a saturation effect on brightening proton aurora. Significant erosion of the Martian ionosphere during periods of high dynamic pressure indicates at least five-to-tenfold increase in atmospheric ion loss. An empirical relationship between ion escape rate and auroral emission enhancement is established, providing a new proxy of Mars’ atmospheric ion loss with optical imaging that may be used remotely and with greater flexibility. The results presented in this study shed light on the direct control of dynamic pressure on interactions of the solar wind with Mars and other objects in solar system (e.g., Venus and Titan), and presumably stellar wind with exoplanets.


PS08-A005
Evaluating Atmospheric and Surface Drivers for the O2 Variations Observed by MSL SAM at Gale Crater

Daniel LO1#+, Sushil ATREYA1, Michael WONG1, Melissa TRAINER2, Heather FRANZ2, Timothy MCCONNOCHIE3, Daniel VIÚDEZ-MOREIRAS4, Paul MAHAFFY2, Charles MALESPIN2
1University of Michigan, 2NASA Goddard Space Flight Center, 3Space Science Institute, 4National Institute for Aerospace Technology

The Sample Analysis at Mars (SAM) instrument suite on the Mars Science Laboratory (MSL) Curiosity rover conducts periodic measurements of the volume mixing ratios (VMRs) of CO2, N2, Ar, O2, CO, and CH4 in the ambient atmosphere around the rover. Over the observation period spanning Mars Years 31–34, the O2 VMR showed significant variations of ~20% in excess of the transport effects driven by seasonal condensation and sublimation of CO2 at the poles that also affect the N2 and Ar VMRs. With the photochemical lifetime of O2 being >10 years, variations of such magnitude on a seasonal and interannual timescale are unexpected. Variations of similar relative magnitudes have also been observed in column-averaged O2 VMR from MSL ChemCam. We explore and evaluate potential reservoirs and processes that could drive the observed O2 VMR variations. Through photochemical modeling, we found that the atmospheric O2 has to be released as O2 from surface/subsurface reservoirs, rather than converted by photochemistry from another gaseous species released from those reservoirs. We also found atmospheric photochemistry, decomposition of (sub)surface H2O2, dissolution from brines, and plasma chemistry from dust activity to be insufficient from reservoir size and/or rate. Currently, the most plausible driver lies with surface oxychlorines, sustaining an equilibrium atmospheric O2 through oxychlorine decomposition by solar ultraviolet radiation and regeneration via O3. Seasonal H2O variations can drive O3 variations, which in turn controls the drawing out of O2 to form oxychlorines at the surface. This is consistent with the tentative observation that increases in water vapor are associated with increases in O2. The prevalence of oxychlorines at the surface would make this is a global phenomenon. Nonetheless, further laboratory experiments and modeling are required to accurately scale the measured rates to Martian conditions and fully elucidate the driving mechanisms.


PS08-A025
Three-dimensional Numerical Simulation of the Thermal Evolution of Planetary Mantle: Discussion on the Causes of Different Convective Modes

Song XIANG1, Bingcheng WU2, Jinshui HUANG2#+
1Chinese Academy of Sciences, 2University of Science and Technology of China

Convection is an important process in the planet's mantle and an important mechanism for the outward transfer of heat from the planet's interior. Today, the earth's mantle is characterized by plate tectonics, but Venus’s mantle convection is in stagnant mode. A common assumption is that the Venusian mantle convection in the early stages is the same as that in the nowadays earth; therefore, there will be a transition from plate tectonics to stagnant mode. Some studies on the earlier Earth showed that the Earth's plate tectonics may have only been operated in the past two billion years, or even in the late Proterozoic. Therefore, understanding the controls on the mantle convection mode is significant for understanding the thermal evolution history of planets. In this study, we use a three-dimensional finite element numerical model to study the thermal evolution process of planets and explore the control factors of mantle convection in different modes. Here we focus on the influence of viscous structure, yield stress, and internal heat on the convection mode of the mantle which has been studied in detail. The calculation results show that different reference viscosity, internal heat, and yield stress can lead to different mantle convection modes. For small reference viscosity, small yield stress, and small endogenous heat, the model is favorable for mantle convection in plate mode. For larger reference viscosity, large yield stress, and larger internal heat, the model prefers to generate mantle convection in stagnant mode. Within a certain range of parameters, the model can generate mantle convective patterns that periodically transition between different modes.


PS08-A027
Martian Polygon Terrains and the Implication for Ancient Climate on Mars

Lei ZHANG1#+, Chao LI2, Jinhai ZHANG2
1Chinese Academy of Sciences, 2Institute of Geology and Geophysics, Chinese Academy of Sciences

Polygonal terrain has been reported mainly in mid-to-high-latitude regions of Mars. Both surface and underground Martian polygonal terrains can provide important information from their formative period on thermal conditions and/or aqueous activity. However, the geometric features of polygonal terrain and their relationship with the ancient climate on Mars have not been fully investigated. Here, we processed images from the High-Resolution Imaging Science Experiment (HiRISE) and detected the boundaries of polygonal terrains on Mars. Then, the statistical information of the area, orientation, and polygon edge density were quantitatively analyzed. Finally, we built up some constraints on the formation mechanism of the polygonal terrains. In addition, we report special frequency-variation patterns of Zhurong radar reflections and interpret them as a buried polygonal terrain below the surface, suggesting a wide distribution of such terrain under Utopia Planitia. Occurring at low midlatitudes (~25˚N), the polygonal terrain interpreted as having formed by freeze-thaw cycles makes a compelling case for high obliquity on early Mars. The contrast of the subsurface structures with the covering materials overlying the buried palaeo-polygonal terrain suggests a significant palaeoclimatic transformation some time thereafter. This study proposes a series of quantitative methods for recognizing the features of polygonal terrain and provides a new perspective for the investigation of climatic condition of ancient Mars.


PS08-A029
A Miniature Meteorology Sensor Network for Future Mars and Venus Missions

Durga Prasad KARANAM#+, Chandan KUMAR
Physical Research Laboratory

Exploration efforts of our two neighboring planets, Mars and Venus, have been gaining momentum in the recent times as evident by series of missions planned in coming decades. One of the important aspects to be addressed is the meteorology and climate studies. Understanding the climate of Mars at various strategic locations is not only important to improve climate models/database but also essential to aid in situ robotic/human exploration in future and to determine if Mars could have the conditions to support life. One of the regions is the Planetary Boundary Layer (PBL) which is extremely important, both scientifically and operationally, because it is the region within which lander/spacecraft must operate. Till date, this region of the atmosphere has been studied directly, by landers, and from orbital remote sensing, though not to the extent that is necessary to fully constrain its character and behaviour. On the other hand at Venus, balloons provide a unique platform to carry-out in-situ investigations in its middle atmosphere cloud regime. One of the important aspects that can be addressed only by experiments using Balloons is the understanding of cloud dynamics, regional scale turbulence, local meteorology which are the driving factors for the ongoing large scale phenomenon such as super-rotation, atmospheric dynamics, transport and coupling etc. To address these, we have proposed and developing a Miniature Meteorology Sensor Network (MMSNET). Each device of MMSNET weighs ~100 grams. The target parameters of measurement from MMSNET are Atmospheric Pressure, Temperature, Humidity, Winds, Solar Insolation/Radiation (UV-VIS-NIR) and Imaging. MMSNET is planned to be deployed using a CubeSat and expected to provide long-term in situ measurements in geographically distinct locations. A laboratory prototype of the instrument has been developed and evaluated. Engineering model design is underway. Details on the instrument development and evaluation results will be presented.


Thu-03 Aug | 8:15 - 10:00 | MR305
PS02 - Comparing Giant Planets and Their Moons

Session Chair(s): Michel BLANC, Institute for Research in Astrophysics and Planetology

PS02-A006
Atmospheric Flows Imprint the High-degree Gravity Field of Jupiter

Yohai KASPI1#+, Eli GALANTI1, Ryan PARK2, Keren DUER1, Nimrod GAVRIEL1, Daniele DURANTE3, Luciano IESS3, Marzia PARISI4, Dustin BUCCINO4, Tristan GUILLOT5, David STEVENSON6, Scott BOLTON7
1Weizmann Institute of Science, 2Jet Propulsion Laboratory, California Institute of Technology, 3Sapienza University of Rome, 4NASA Jet Propulsion Laboratory, 5Observatoire De La Cote D'Azur, 6California Institute of Technology, 7Southwest Research Institute

Since the first gravity measurements of Juno at Jupiter, the odd gravity harmonics J3 to J9 have been used to determine the depth of the zonal wind observed at the cloud level. Later on, combining solutions from internal models, the gravity harmonics J6, J8 and J10 were added to the analysis, which reinforced the conclusion that the observed zonal flows extend to a depth of around 3,000 km and imprint the gravity signal. The harmonics higher than J10 were not used in the analysis since their individual uncertainty was too large. In this study, we revisit the wind-gravity analysis, when the gravity retrieval is constrained at the high latitudes, and show results for higher gravity harmonics. This gives more detail about the structure of the deep zonal flows and allows better explaining the structure of the measured gravity spectrum. This confirms that indeed the observed flows are the ones which imprint the gravity spectrum. Moreover, this analysis allows to better determine which part of the wind field most contributes to the gravity signal, implying on the depth of individual jet streams. We also show how this analysis allows to refine the surface gravity field, particularly in the latitudinal range of the closest approach of the spacecraft.


PS02-A011 | Invited
Jupiter's Temperature and Composition Revealed from Juno Microwave Observations

Cheng LI1#+, Michale ALLISON2, Sushil ATREYA1, Leigh FLETCHER3, Andrew INGERSOLL4, Liming LI5, Glenn ORTON6, Fabiano OYAFUSO6, Paul STEFFES7, Michael H. WONG8, Zhimeng ZHANG9, Steven LEVIN6, Scott BOLTON10
1University of Michigan, 2Goddard Institute for Space Studies, 3University of Leicester, 4Geological and Planetary Sciences, California Institute of Technology, 5University of Houston, 6Jet Propulsion Laboratory, California Institute of Technology, 7Georgia Institute of Technology, 8SETI Institute, 9California Institute of Technology, 10Southwest Research Institute

We analyze the Juno microwave observations of Jupiter’s atmosphere and find a warmer interior temperature than previously assumed based on the Voyager’s radio occultation measurement (Lindal et al., 1981, JGR-Space Physics, 86.A10, 8721-8727) and the Galileo Probe (Seiff et al., 1998, JGR-Planets, 103.E10, 22857-22889). By analyzing globally averaged observations from 1.4 – 50 cm wavelength, we find that the deep isentrope of Jupiter is at 169 K referenced at 1 bar pressure level. The globally averaged kinetic temperature at 1-bar is closer to 175 K and Jupiter’s weather layer is stably stratified. On the other hand, the 1-bar temperature inverted from Juno microwave observations at the Equatorial Zone between 0 and 5 oN remains low at 166 K, consistent with the previous remote sensing measurements made at the equator from the infrared (Fletcher et al., 2016, Icarus 278, 128-161). This also implies a vertical temperature gradient at the equator which is super-adiabatic. Our results suggest that the potential temperature difference between 1-bar and the deep isentrope is approximately 2.8 K. To avoid dynamic instability, the super-adiabatic temperature gradient must be stabilized by a change of mean molecular weight within the 5 – 10 bars pressure levels which only water can provide. The result implies that an abundance of water at the equator is constrained to a value between 2.2 and 6.2 times solar.


PS02-A005
The Shape of Jupiter and Saturn Based on Atmospheric Dynamics, Radio Occultations and Gravity Measurements

Eli GALANTI1#+, Yohai KASPI1, Tristan GUILLOT2
1Weizmann Institute of Science, 2Observatoire de la Côte d’Azur / National Centre for Scientific Research

The shape of two gas giants, Jupiter and Saturn, is determined primarily by their rotation rate, and interior density distribution. It is also affected by their zonal winds, causing a perturbation of O(10 km) at low latitudes. However, uncertainties in the observed cloud-level wind and the polar radius, translate to uncertainty in the shape with the same order of magnitude. This prevents an exact comparison against the shape based on radio-occultation measurements, the only other available data. The Juno (Jupiter) and Cassini (Saturn) missions gave unprecedentedly accurate gravity measurements, constraining better the uncertainty in the wind structure. Using an accurate shape calculation, and a joint optimization, given both gravity and radio-occultation measurements, we calculate the possible range of dynamical height for both planets. We find that for Saturn there is an excellent match to the radio-occultation measurements, while at Jupiter the shape does not reflect the radio-occultations measurements on that scale.


PS02-A007 | Invited
Magnetic Fields of the Outer Planets: Gas and Ice Giants, No Two Alike?

J. E. P. CONNERNEY1,2#+
1Space Research Corporation, 2NASA Goddard Space Flight Center

The systematic mapping of Jupiter’s magnetic field by the Juno spacecraft, in polar orbit since July 2016, has demonstrated its worth as a probe of the interior and reminds us of the limited knowledge afforded by flyby trajectories. Juno’s Prime Mission revealed a surprisingly intense and non-dipolar magnetic field undergoing secular variation. The Lowes’ radius fit to model spherical harmonics (JRM33, to degree 18) identifies a putative dynamo radius of 0.807 +/- 0.006 Rj, which we interpret as the depth to which Helium rain stabilizes the metallic Hydrogen-Helium mixture against convection. In contrast, Jupiter’s twin, Saturn, could not be more different: possessing an axisymmetric and nearly dipolar magnetic field suggestive of a dynamo at depth (~0.5 Rs) beneath a conductive shell (Helium rain, again) in differential rotation above. The Juno experience suggests we know but little of the magnetic fields of Uranus and Nepune, beyond the first two or three degrees in a spherical harmonic expansion, but even that is sufficient to whet one’s appetite: extraordinary dipole tilts (60 and 47 degrees, respectively) combined with extraordinary non-dipolarity. The ice giant dynamos are unlike those of the gas giants, a challenge for dynamo theory. Charged particle motion in those magnetospheres is likely to be rather complicated; even Jupiter’s field, near the surface, offers some unanticipated surprises: field lines without a magnetic equator external to the 1-bar surface as well as field lines with more than one magnetic equator above the 1-bar surface. With a mission to Uranus under consideration, the Juno experience argues for a polar mapping orbit to achieve the resolution needed to probe the dynamo region. Juno’s extended mission offers a view of what that might look like, as the spacecraft periapsis latitude marches northward towards the dipole axis at about 1 degree each orbit.


PS02-A017 | Invited
Jupiter Below the Clouds: Active, Stable & Still Mysterious

Tristan GUILLOT1#, Scott BOLTON2+
1Observatoire De La Cote D'Azur, 2Southwest Research Institute

The largest planet of our solar system is known for its active, turbulent atmosphere, governed by strong zonal winds, evolving vortices and powerful storms. Numerous signs of convective activity, added to the large intrinsic luminosity (more than 10,000 times larger than the Earth's), led to the paradigm of a mostly convective and largely well-mixed planet. While this picture remains in part true, new observations, in particular from the Juno spacecraft in orbit around the planet since 2016, have led to considerable changes in our vision of Jupiter: Evidence of imperfect mixing and non-zero static stability have arisen both in the deep atmosphere and interior. We know that Jupiter's zonal winds extend deep, to about 3000 km, but we cannot yet fully account for their braking by the interior magnetic field. The interior temperature profile deep temperature gradient is not well understood. I will review these changes and how they affect our understanding of the evolution and structure of giant planets in general.


PS02-A012 | Invited
5 Years of Galilean Moons Observations by JIRAM on Juno

Alessandro MURA1#, Rosaly LOPES2+
1National Institute for Astrophysics, 2Jet Propulsion Laboratory, California Institute of Technology

The Juno mission to Jupiter has been observing the gas giant since 2016 from a polar, highly elliptical orbit. Although not in the main scientific objectives, Juno also investigated the Galilean moons from a very favorable position, using some of the cameras on board: JIRAM, JunoCam and SRU. In particular, The Jovian Infrared Auroral Mapper (JIRAM) is a dual-band imager and spectrometer in the infrared (2 to 5 microns). The pixel angular resolution (0.01°) is small enough for imaging the moons during the several Juno close passages (and, in some cases, flybys). The spatial resolution at the surface of the moons varies along the s/c distance and is of the order of 100 km/pixel or even smaller. Here we present JIRAM’s images and spectra of Europa, Ganymede, Callisto and Io after six years of Juno mission, with a particular emphasis on Io. On Io, in fact, these observations characterize the location and possible morphology, and some temperatures, of the volcanic thermal sources; the identification and distribution of SO2, the possible identification of CO2 and other materials.
Recent Juno flybys, at distance down to 50'000 km, allows unprecedented imaging of the moon with resolution of about 10 km. This allows reconstructing the morphology of hot spots, and a better mapping of their distribution, in location and emitted power.


Thu-03 Aug | 8:15 - 10:00 | MR307
PS16 - Planetary Seismology: Moon, Mars and Beyond

Session Chair(s): Taichi KAWAMURA, Université Paris Cité, Institut de physique du globe de Paris, CNRS, Daoyuan SUN, University of Science and Technology of China

PS16-A002
Coherence Analysis of Apollo Short-period Seismometer Data for the Detection of New Moonquakes

Keisuke ONODERA1,2#+
1The University of Tokyo, 2Institut de Physique du Globe de Paris

The deployment of seismometers on the Moon during Apollo missions (12, 14, 15, and 16) brought us new insights into the seismic activity and internal structure of our neighbor. Until today, more than 13,000 seismic events (e.g., deep moonquakes, shallow moonquakes, and meteoroid impacts) have been identified and used for analyses over 50 years. It has been believed that all seismic events have been discovered and cataloged. However, it is expected that there are potential moonquakes not detected yet because the current event catalog builds on the events mostly discovered from the long-period seismometer data. In fact, the majority of short-period (SP) seismometer data has not been analyzed because of many artifacts and/or glitches. In this study, I denoised the SP data so that I can use them to find new moonquakes, especially shallow moonquakes that excite high-frequency energy more sensible by the SP sensor. In the analysis, I searched for new events by taking coherence between reference moonquakes (which have already been cataloged) and the continuous SP data. As a result, I successfully detected lots of candidates for new moonquakes. In the presentation, I will report newly detected lunar seismic events and describe in which type of moonquake they can be classified. Furthermore, I am willing to discuss how this discovery makes an impact on the evaluation of lunar seismicity.


PS16-A013
Instrumental Challenge for Joint Detection of Lunar Normal Modes and Gravitational Waves from the Moon

Philippe LOGNONNÉ1#+, Sébastien DE RAUCOURT1, Taichi KAWAMURA2, Raphael GARCIA3, Jani KARAN4, Simone DELL'AGNELLO5, Josipa MAJSTOROVIC1
1Université Paris Cité, 2Université Paris Cité, Institut de physique du globe de Paris, CNRS, 3Institut Supérieur de l'Aéronautique et de l'Espace, 4Vanderbilt University, 5Laboratori Nazionali di Frascati

The main goal of the Apollo 17 gravimeter was to detect oscillations of the moon excited by either lunar normal modes or gravitational waves. This instrument unfortunately failed to operate in nominal mode and was likely not sensitive enough. We start by presenting the amplitude of the expected signals of normal modes excited by moonquakes or by gravitational waves on seismic monitoring systems, either with inertial systems or strainmeters. This is done for the typical Moonquakes occuring at weekly rate on the Moon, and for typical gravitational events, such as intermediate-mass black hole mergers, occuring at monthly rate. We then focus on new estimations of the micro-seismic noise of the noise including space and time noise coherency losses due to scattering. This noise is not only related to the hum of natural impacts, but also to the deep moonquake (DMQ) activity, down to the bottom part of seismic bandwidth, e.g. ~0.5 mHz. This is first done by estimating the amplitude of normal modes of the Moon for the various DMQ and then by using Apollo lunar seismicity catalog for summing up contributions of the continuous activity of DMQs. This first allow us to estimate the amplitude of the Moon Normal modes for DMQs and includes the Slichter mode associated to a possible Moon inner core, which is a key geophysical target for estimating the amount of light elements in the outer core. But this gives also an estimation of the micro-seismic noise, including for the low order angular modes, which are the critical seismic source of noise for long period gravitational wave signals. We finaly describe how strainmeters coupled with very high sensitivities lunar optical very broad band seismometers can perform these joint goals and conclude on the challenge for developing them for flight opportunities earlier than 2035.


PS16-A012
Investigation on Seismic Exploration of Small Bodies: Implication to the Japanese Next Generation Small Body Sample Return Project

Gaku NISHIYAMA1#+, Taichi KAWAMURA2, Keisuke ONODERA1, Takeshi TSUJI1, Satoshi TANAKA3, Hiroyuki KUROKAWA4, Naoya SAKATANI3, Yuri SHIMAKI3
1The University of Tokyo, 2Université Paris Cité, Institut de physique du globe de Paris, CNRS, 3Japan Aerospace Exploration Agency, 4Tokyo Institute of Technology

Seismic exploration of planets and satellites has been one of the most successful approaches to uncovering the internal structure of these bodies. Following the success of previous missions such as Apollo, InSight, and Philae, we are now considering seismic exploration of small bodies to understand their inner structures and, consequently, their formation and evolution histories. Particularly, we propose possible seismic exploration of a small body with active seismic experiments. These experiments are under consideration as a part of the Japanese Next Generation Small Body Sample Return Project, a proposed mission to bring back samples from a comet. Since active seismicity is not expected on comets, we will achieve our science goal through active experiments. We consider two types of seismic sources: a motor-type portable active seismic source (PASS) and an artificial impact like the Hayabusa-2 Small Carry-on Impactor (SCI). We conducted numerical simulations with some possible comet structures to evaluate the expected seismic signals. One key challenge we identified was that the low/zero gravity condition of the comet can decouple seismometers from the ground even with small ground acceleration generated by a seismic source. To overcome this challenge, we propose a penetrator system that is currently under development for planetary and terrestrial use. With a penetrator, we can embed our seismometers as well as the active seismic source into the comet to ensure the coupling. We will present our current configuration for future seismic exploration on a comet.


PS16-A011
Summary of Elastic Properties of Asteroid Ryugu Samples

Keisuke ONODERA1,2#+, Yuta INO3, Satoshi TANAKA4, Taichi KAWAMURA5, Rei KANEMARU4, Takuya ISHIZAKI4, Ryota FUKAI4, Takeshi TSUJI1, Tomoki NAKAMURA6, Masayuki UESUGI7, Hisayoshi YURIMOTO8, Takaaki NOGUCHI9, Ryuji OKAZAKI10, Hikaru YABUTA11, Hiroshi NARAOKA10, Kanako SAKAMOTO4, Shogo TACHIBANA12, Sei-Ichiro WATANABE13, Yuichi TSUDA4
1The University of Tokyo, 2Institut de Physique du Globe de Paris, 3Kwansei Gakuin University, 4Japan Aerospace Exploration Agency, 5Université Paris Cité, Institut de physique du globe de Paris, CNRS, 6Tohoku University, 7Japan Synchrotron Radiation Research Institute, 8Hokkaido University, 9Kyoto University, 10Kyushu University, 11Hiroshima University, 12University of Tokyo, 13Nagoya University

Until today, seismology has been applied to extraterrestrial bodies such as the Moon (Apollo), Mars (Viking, InSight), and comet 67P/Churyumov-Gerasimenko (Philae), contributing to a better understanding of their internal structures as well as elastic properties. As a new application case, here we report the first seismic measurement of an asteroid performed in the framework of the Japanese Hayabusa 2 mission. Hayabusa 2 was launched in Dec 2014 and explored asteroid Ryugu from June 2018 to Nov 2019. Although in-situ seismic observations were not realized, the returned rock samples opened the way to “asteroid seismology”. Our team was allocated two mm-sized samples (C0002-No3 and C0002-No4) and measured seismic wave velocities using the pulse transmission method. Additionally, combined with the density value, elastic parameters (e.g., Young’s modulus) were also estimated. As a result, we obtained 2.1 km/s, 1.2 km/s, and 7.0 GPa for P-wave velocity, S-wave velocity, and Young’s modulus, respectively. Comparing our results with those of the known carbonaceous chondrites, we found that Ryugu samples showed similar elastic properties to those aqueously altered chondrites such as Tagish Lake and Tarda. In the presentation, we will summarize the obtained elastic properties of Ryugu samples and discuss how our results can contribute to improving our knowledge of asteroid science. 


PS16-A008
Martian Crustal Model from a Joint Inversion of Receiver Functions and Apparent Shear Wave Velocity

Mingwei DAI+, Daoyuan SUN#
University of Science and Technology of China

Receiver function (RF) based studies have revealed the layered Martian crustal structure beneath the InSight, which provides key information about the composition, rock alteration, deep magma process, and thermal history of Mars. However, limited by the used frequency and trade-offs between the thickness and velocity, by inverting RFs alone, it is difficult to provide an accurate image of the upper crust. Here, by achieving stable measurements of the apparent shear wave velocities (Vs,app) at different frequencies for high quality marsquakes, we perform a joint inversion with the RFs. Our crustal models differ from previous models by having an extra shallow structure in the upper crust, either a layer with a sharp velocity jump interface at 5.0 ± 1.8 km depth or a gradient structure with shear wave velocity increasing gradually from 1.2 ± 0.2 km/s near the surface to 2.3 ± 0.3 km/s at a depth of 8.0 ± 2.6 km, which well fits both RFs and Vs,app’s. Such a crustal model is consistent with the depth-decaying of porosity due to self-compaction and indicates a highly porous upper crust with a surface porosity larger than 30%. However, if we assume the whole crust is basaltic, a much higher porosity decay constant than that scaled from the Moon is needed, suggesting possible different mechanical properties of the lunar and Martian crust.


PS16-A010
Machine Learning-based Classification of the Martian Dust Devils Observed by InSight: Implication for Better Estimation of the Martian Subsurface Structure

Ryoji OTSUKA1#+, Satoshi TANAKA2, Keisuke ONODERA1, Taichi KAWAMURA3
1The University of Tokyo, 2Japan Aerospace Exploration Agency, 3Université Paris Cité, Institut de physique du globe de Paris, CNRS

NASA’s InSight (Interior Exploration using Seismic Investigations, Geodesy and Heat Transport) quasi-continuously conducted seismic and meteorological observations (e.g., pressure, temperature, wind speed) from February 2019 to December 2022. Dust devil or convective vortex is one of the most common meteorological phenomena observable on Mars. While dust devils reflect local atmospheric activity on Mars, they also cause ground deformation associated with temporal pressure drops. In the InSight pressure and seismic data, we can observe various characteristics of pressure drop events and ground motions associated with those events. In previous studies, shallow subsurface structures have been estimated by using seismic and pressure signals related to dust devils and/or convective vortices. While those studies used any events as long as high correlation between pressure and seismic signal is achieved (i.e., a good air-solid coupling is realized), this study pays more attention to the differences in air-solid interaction depending on the type of dust devils. The objective of this study is (i) to clarify how dust devil-related signals can be classified based on their features and (ii) to extract the high-quality events for compliance analysis to better estimate the subsurface structure. Extracting the pressure drop events (~13,000) listed in the existing catalog (Spiga et al., 2021), we classified their pressure profiles using machine learning. As a result, we found that there were two types of events; one type showed sharp pressure drop (type-I) and the other did gradual fluctuations (type-II). In the presentation, we report the detailed characteristics of each dust devil type and discuss the difference in air-solid coupling made by the respective types of events. Furthermore, we will give a constructive implication for better evaluating the subsurface structure through compliance analysis.


Thu-03 Aug | 10:20 - 12:20 | MR305
PS02 - Comparing Giant Planets and Their Moons

Session Chair(s): Paul HARTOGH, Max Planck Institute for Solar System Research

PS02-A001
An Early Dynamical Instability Among Solar System Giant Planets

Beibei LIU#+
Zhejiang University

The Solar System's orbital structure is thought to have been sculpted by an episode of dynamical instability among the giant planets. However, the instability trigger and timing have not been clearly established. Here we use dynamical simulations to show that the giant planets' instability was probably triggered by the dispersal of the gaseous disk. As the disk evaporated from the inside out, its inner edge swept successively across and dynamically perturbed each planet's orbit in turn. The associated orbital shift caused a dynamical compression of the exterior part of the system, ultimately triggering instability. The final orbits of our simulated systems match those of the Solar System for a viable range of astrophysical parameters. The giant planet's instability therefore took place as the gaseous disk dissipated, constrained by astronomical observations to be a few to ten million years after the birth of the Solar System. Terrestrial planet formation would not complete until after such an early giant planet instability; the growing terrestrial planets may even have been sculpted by its perturbations, explaining the small mass of Mars relative to Earth.


PS02-A019 | Invited
A Juno View of Planet-moons-magnetosphere Interactions at Jupiter

Michel BLANC#+
Institute for Research in Astrophysics and Planetology

The electrodynamics of the Jupiter system is controlled by complex coupling processes between the planet’s interior, its conducting upper atmosphere, moons and the solar wind, on which the Juno mission has shed unique new light. Generation of the planetary magnetic field, including its surface anomalies and their variations at the decadal scale, has been characterized. Juno has also been able to observe in detail the different components of the giant electric current loop that connects the Jovian upper atmosphere to the magnetodisk, transferring angular momentum and partly driving the main auroral emission. Juno also revealed the complexity of auroral acceleration processes, particularly the relative importance of Alfvenic and electrostatic acceleration. Juno has also shed light on the sources and mechanisms controlling the other types of auroral features: polar cap auroral emission features seem sometimes related to bi-directional particle acceleration, including upward acceleration of electrons, and to Mega-volt electrostatic potential drops; finally, auroral spots and tails generated by Galilean moons have been studied in great detail, opening a first window on the specific particle acceleration processes generated by moon-magnetosphere interactions. Finally, Juno studies have been been able to show the importance of momentum deposition into the thermosphere produced by high-latitude ionospheric currents, which combines with Joule heating and particle precipitation to drive large-scale meridional and zonal wind systems in the auroral and polar thermosphere, thus redistributing high-latitude energy deposition to other latitudes. Overall, Juno has been working as a unique laboratory to study the diversity of Planet-Moons-Magnetosphere electrodynamic interactions. Its studies open the way to a deeper understanding of “universal” processes driving planetary aurorae and of their connection to the dynamics of the system as a whole. Our talk will summarize these achievements and identify some of the many new unresolved questions left for investigation by future missions.


PS02-A008 | Invited
Results from the Juno Microwave Radiometer at Jupiter

Steven LEVIN1#+, Virgil ADUMITROAIE1, Sushil ATREYA2, Scott BOLTON3, Shannon BROWN1, Leigh FLETCHER4, Andrew INGERSOLL5, Yohai KASPI6, Cheng LI2, Jonathan LUNINE7, Sidharth MISRA1, Glenn ORTON1, Fabiano OYAFUSO1, Daniel SANTOS-COSTA3, Paul STEFFES8, Zhimeng ZHANG1
1Jet Propulsion Laboratory, California Institute of Technology, 2University of Michigan, 3Southwest Research Institute, 4University of Leicester, 5Geological and Planetary Sciences, California Institute of Technology, 6Weizmann Institute of Science, 7Cornell University, 8Georgia Institute of Technology

Juno is a spinning spacecraft in a highly eccentric polar orbit about Jupiter, with perijoves at about 5000 km above the cloud tops, and has completed 52 orbits as of July 2023. From Juno’s unique vantage point, the Juno Microwave Radiometer (MWR) has measured the radio emission in 6 channels, at wavelengths ranging from 1.4 to 50 cm, with 100 mS sampling throughout each spin of the spacecraft, since the first science pass in August of 2016. This data set covers the Jovian atmosphere over a wide range of latitudes, longitudes and emission angles, as well as observations of the inner radiation belts and of Ganymede and Europa. MWR has yielded a number of results, as well as prompting new questions, related to Jupiter’s atmospheric composition and dynamics at depths as deep as 300 km, distribution of lightning, microwave reflection over the auroral region, Jovian synchrotron emission, and the ice shells of Ganymede and Europa. We will present an overview of MWR results to date.


PS02-A018
Ganymede and Europa in the 21st Century as Observed by JunoCam

Michael RAVINE1#+, Candice HANSEN2, Geoffrey COLLINS3, Paul SCHENK4, Erin LEONARD5, Michael CAPLINGER1
1Malin Space Science Systems, 2Planetary Science Institute, 3Wheaton College, 4Universities Space Research Association, 5Jet Propulsion Laboratory, California Institute of Technology

The Juno extended mission includes encounters with the inner three Galilean Satellites, enabling JunoCam to provide the first broad-spatial-coverage, km-scale images of those bodies in four decades. The Ganymede encounter occurred on Juno’s 34th perijove (7 June 2021); the Europa encounter on PJ45 (29 September 2022) and the upcoming Io encounters on PJ57 and PJ58 (30 December 2023 and 3 February 2024). We present results from the Ganymede and Europa encounters. Images obtained from each encounter was similar: four broadband color images, from the terminator to the limb, covering an area several thousand km square at scale of 1-4 km per pixel. Overlapping coverage enabled derivation of surface relief over much of the area. Ganymede: JunoCam coverage of Ganymede spanned from western Perrine Regio eastward past the eastern margin of Barnard Regio, and provides good resolution of craters Sati, Neith and Tros as well as Phrygia and Sicyon Sulci. No changes were observed from the 1979 Voyager 1 coverage. Ten possible cryovolcanoes were observed. A 3 km topographic dome at the subjovian point was confirmed and its shape determined. Significant refinements were made in the geologic map over the center section of the coverage area. Europa: JunoCam coverage represents significant improvements for geologic interpretation of the center of the coverage area. Many more lineaments are resolved, and they are now traceable across areas of previous poorer resolution. Low sun in the area near the terminator allows chaos and regional plains units to be more accurately distinguished. With higher image quality, Crater Gwern does not appear to be a crater at all, reducing the number of craters on Europa larger than 1 km to 40. Troughs and pits that conform to the global-scale pattern possibly associated with true polar wander were resolved by JunoCam. No evidence of plumes were observed.


PS02-A003
A Complex Region of Europa’s Surface Revealed in High-resolution by Juno’s Stellar Reference Unit

Heidi BECKER1#+, Meghan FLORENCE1, Jonathan LUNINE2, Paul SCHENK3, Candice HANSEN4, Martin BRENNAN1, Yasmina M. MARTOS5, Scott BOLTON6, James ALEXANDER1
1Jet Propulsion Laboratory, California Institute of Technology, 2Cornell University, 3Universities Space Research Association, 4Planetary Science Institute, 5NASA Goddard Space Flight Center, 6Southwest Research Institute

On 29 September 2022 Juno’s low-light sensitive Stellar Reference Unit (SRU) captured a high-resolution (256-340 m/pixel) broadband visible (450-1100 nm) image of Europa’s surface during the first close encounter with the icy Jovian moon since Galileo’s final flyby in 2000. Collected at a sub-spacecraft altitude of 412 km while the surface was illuminated only by Jupiter-shine (incidence angle: 48-51 degrees), the SRU image reveals a 3x104 km2 region of Europa’s surface between ~0-6°N and 43.5-51°W in remarkable detail; the highest resolution image ever for that region. Prior coverage of the area by Galileo was under high-sun conditions at 1 km resolution, leading to characterization of the terrain as ridged plains with undifferentiated linea. The SRU image reveals a much richer and complex picture. Intricate networks of cross-cutting ridges and lineated bands surround an intriguing 37 km (east-west) by 67 km (north-south) chaos feature that appears to have undergone a unique, local geologic process. Low-albedo deposits, similar to features previously associated with hypothesized subsurface activity [Quick & Hedman, Icarus, 2020], flank nearby ridges. The SRU image enables updated geologic mapping of this fascinating region of Europa’s surface, provides new data to hold up against the various theories of the chaos formation process, and presents new puzzles that await future high-resolution imagery.


PS02-A009
Juno Microwave Radiometer Observations of Europa’s Subsurface Ice Shell

Scott BOLTON1#+, Zhimeng ZHANG2, Shannon BROWN2, Lea BONNEFOY3, Jianqing FENG4, Matthew SIEGLER4, Steven LEVIN2, Jonathan LUNINE5, Sidharth MISRA2, Paul HARTOGH6, Anton ERMAKOV7, David STEVENSON8
1Southwest Research Institute, 2Jet Propulsion Laboratory, California Institute of Technology, 3Observatoire de Paris, 4Planetary Science Institute, 5Cornell University, 6Max Planck Institute for Solar System Research, 7University of California, Berkeley, 8California Institute of Technology

On 29 Sep 2022, Juno has a close flyby of Jupiter’s moon Europa, flying within 350 km of the surface. During the flyby, Juno’s Microwave Radiometer (MWR) observed Europa, obtaining several swaths across Europa using Juno’s spin to map Europa’s subsurface ice shell at six frequencies ranging from 600 MHz to 22 GHz. The ice transparency at microwave frequencies is dependent on purity; assuming pure ice, the observations probe depths ranging from meter to kilometers. The MWR observations represent the first resolved interrogation of Europa’s subsurface ice shell revealing new constraints on porosity, fracturing, differences in terrain type and possibly the thickness of the conductive ice shell. These unprecedented measurements on Europa and Ganymede will provide new insights into the comparative nature of the surfaces and interiors of the Jovian satellites.


Thu-03 Aug | 10:20 - 12:20 | MR323
PS16 - Planetary Seismology: Moon, Mars and Beyond

Session Chair(s): Ceri NUNN, Jet Propulsion Laboratory, California Institute of Technology

PS16-A003 | Invited
Seismology on Mars After 2 Martian Years of SEIS/InSight Monitoring

Philippe LOGNONNÉ1#+, William Bruce BANERDT2, John CLINTON3, Raphael GARCIA4, Domenico GIARDINI3, Brigitte KNAPMEYER-ENDRUN5, Mark PANNING2, William Thomas PIKE6, InSight SCIENCE TEAM2
1Université Paris Cité, 2Jet Propulsion Laboratory, California Institute of Technology, 3ETH Zürich, 4Institut Supérieur de l'Aéronautique et de l'Espace, 5University of Cologne, 6Imperial College London

SEIS, the international seismometer of NASA’s InSight mission performed 2 Martian years of seismic monitoring, with data rates up to 100sps until end of December 2022. For the first time, a robotic seismometer installation was made on the ground followed by wind shield deployment. This allowed the Very-Broad-Band sensors of SEIS to reach ultra-low noise (down to 2x10 m/s/Hz between 0.1-1Hz) during the much of the night. This lowered the detection threshold to M<3 in the InSight hemisphere and to M~4 in the antipodal one. Noise was much larger during the rest of each day, exceeding the noise recorded on the Moon but still 10 times less than the quietest sites on Earth in the 0.1-1H bandwidth. More than 1300 events were detected during two Martian years, including a Mw=4.7 marsquake, 34 teleseismic events with determined distances (and azimuths, giving locations, for half of them), 8 impacts confirmed by orbital crater imaging, two with very large craters and a thousand regional crustal high frequency quakes. During the windy period, SEIS also detected several thousand pressure drops associated with atmospheric vortices, and during sunset thousands of very shallow local thermal cracks. We present some of the achievements and successes of the SEIS/InSight science team and services. These include the first models for the subsurface, for the crust below InSight and between InSight and several epicenters, and for the mantle as well as the determination of the core radius. We present also results in term of anisotropy, attenuation and scattering. Seismic source analyses have determined magnitude, depth and centroid moment tensors for the largest marsquakes and provided better understanding of impact processes, including partitioning of blast energy in the subsurface and atmosphere. We conclude with perspectives for the future of Mars and planetary seismology.


PS16-A007 | Invited
Chang’E-7 Lunar Seismograph

Jinhai ZHANG#+
Institute of Geology and Geophysics, Chinese Academy of Sciences

The lunar internal structure is important for understanding the origin and evolution of the Moon. However, the detection of the internal structure of the Moon is challenging on both designing and deploying the lunar seismograph, considering the limited power supply and critical thermal control against the dramatic near-surface temperature over 300 K and long period of polar days/nights at the south pole. The lunar seismographs in the Apollo Era have made prominent contributions to revealing the mysteries of the interior of the Moon. However, the exploration results of the lunar interior structure are still controversial. Chang'E-7 mission plans to land around the south pole of the Moon and deploy China's first lunar seismograph to detect the interior structure of the Moon. Here we analyze some possible challenges in the development and deployment of the Chang’E-7 lunar seismograph; then, we present some ideas on how to overcome or avoid potential difficulties, including issues about thermal control, automatic deploying and automatic leveling, to guarantee a long-term high-precision observation; next, we propose some suggestions on developing new methods for the subsequent scientific research; finally, we show some progresses of developing the Chang'E-7 lunar seismograph.


PS16-A014
Farside Seismic Suite (FSS): The First Challenge to Lunar Farside Seismicity

Taichi KAWAMURA1#+, Mark PANNING2, Sharon KEDAR2, Renee WEBER 3, Neil BOWLES4, Simon CALCUTT4, Melanie DRILLEAU5, Raphael GARCIA5, Sreejaya KIZHAEKKE PAKKATHILLAM6, Philippe LOGNONNÉ7, Josipa MAJSTOROVIC7, David MIMOUN8,9, Ceri NUNN2, William Thomas PIKE10, Dilan PORTELA-MOREIRA5, Sébastien DE RAUCOURT7, Arnaud WILHELM5
1Université Paris Cité, Institut de physique du globe de Paris, CNRS, 2Jet Propulsion Laboratory, California Institute of Technology, 3NASA Marshall Space Flight Center, 4University of Oxford, 5Institut Supérieur de l'Aéronautique et de l'Espace, 6Institut de Physique du Globe de Paris, Université Paris Cité, 7Université Paris Cité, 8Institut Supérieur de l'Aéronautique et de l'Espace , 9University of Toulouse, 10Imperial College London

For the first time since the termination of Apollo Passive Seismic Experiment in 1977, we are now ready to start again seismic observations of the Moon. Farside Seismic Suite(FSS) was funded under the Payloads and Research Investigation on the Surface of the Moon (PRISM) program and will be delivered to the lunar surface as a part of NASA’s Commercial Lunar Payload Servise(CLPS). The launch is planned in 2025 and the seismic package will be deployed in Schrödinger Basin, one of the youngest impact basins on the Moon. FSS is not only the first seismic observation that will be performed on the moon after half a century but it will also be the first seismic station to be monitoring the seismicity of the lunar farside. Since all the Apollo stations were on the lunar nearside, seismicity of the farside is still yet to be uncovered. The aim of the experiment will be to: 1. Investigating deep lunar structure and the difference between near and farside 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 (with important implications for the Artemis human exploration program). To achieve these goals, FSS consists of two flight proven seismometers, a vertical Very BroadBand (VBB) seismometer and 3 axis Short Period (SP) sensor. Both instruments are heritage of Mars InSight mission and their high performances are well known. They will be packaged into a stand-alone module which enables us to perform long term observations. We will present our experiment and discuss how FSS can open a new window to lunar seismology. 


Thu-03 Aug | 1:00 - 5:15 | Summit
PS - Planetary Sciences Poster Session

PS01-A001
A Comparison of the Ionospheric Dynamo Current of Mars Above the Landing Sites of Insight and Zhurong: Modeling and Observations

Lin TIAN+, Hao LUO#
Institute of Geology and Geophysics, Chinese Academy of Sciences, China

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 [Johnson et al., 2020; Lillis et al., 2019; Mittelholz et al., 2020a; Mittelholz et al., 2020b]. However, it needs further study whether there are significant differences in the strength, the configuration, and the diurnal and seasonal variation of the dynamo current in different regions of the Martian upper atmosphere. This study compares the similarities and differences between the wind driven dynamo current over the InSight landing site (4.50° N, 135.62° E) and the Zhurong rover (25.07° N, 109.90° E). The results show that the dynamo current as well as its magnetic signal at around perihelion on surface at Zhurong is smaller than that at InSight due to weaker magnetic field in the ionosphere. This study also indicates that the seasonal effect, or the solar zenith angle (SZA), would affect the plasma density which should be included when dealing with off-equatorial locations. The direction and strength of the magnetic field and neutral wind, along with SZA, impact the intensity of the dynamo currents at Zhurong. The study provides a reference in an attempt to promote the understanding of the solar wind – Mars induced magnetosphere – ionosphere – Mars surface coupling process.


PS01-A002
The Injections of Plasma and Aurorae at Jupiter

Zhonghua YAO#+
The University of Hong Kong, Hong Kong SAR

Jupiter’s powerful auroral emissions include a substantial component from the region at lower latitudes than the main auroral oval, named outer auroral emission. Besides the persistent auroral footprint of Jupiter’s natural moon Io, auroral injections are often observed in the outer auroral region, manifesting the magnetospheric plasma injection from the middle/outer magnetosphere to the inner magnetosphere. Magnetospheric plasma injections sometimes have auroral counterparts, while sometimes have not. It is yet to be understood what controls the auroral counterparts of magnetospheric plasma injections. In this presentation, we show a long-lasting auroral injection events captured by the Hubble Space Telescope, together with simultaneous particle measurements from the Juno spacecraft. Multiple auroral substructures were identified in the injection region, which is likely associated with the observed filament plasma injections. A comparison between terrestrial and jovian processes could greatly help the understanding of auroral injection from a universe perspective.


PS01-A004
Study on Magnetic Field Signature of Intermediated-sized Impact Craters: Modeling and Observations

Kuixiang ZHANG#+
Chinese Academy of Sciences, China

Impact cratering is a dominant geologic process on Mars, with the crust demagnetized or remagnetized in the presence of a dynamo field. Thus the large impact craters are used to constrain the history of the Martian dynamo, however, the absence of crustal magnetic fields above the large basins suggesting the core dynamo cessation during their formation is controversial. Because impacts could excavate large portions of the strongly magnetic crust, making craters demagnetization completely even when the dynamo is alive. We select the intermediated-sized craters (150 km ~ 500 km in diameter) on Mars whose magnetic anomalies are associated with the topography. we find that the magnetic field magnitude of craters in the South Province is weak and has no magnetic edge effect, in other words, the crust is formed without an active Martian dynamo. We compare the observed magnetic field signature to the random magnetization model, the results show that the magnetic field variation (Bin/out) caused by impact and crater diameters are anti-correlation. Combining with the absolute model age of craters, we conclude that the Martian dynamo may start after the primordial crust formed, become weak or even cease at about 4.0 Ga, and likely become stronger or restart at about 3.7 Ga. High-resolution magnetic field characteristics analysis of more young and small impact craters will be required to constrain the evolution of the martian dynamo accurately.


PS01-A005
Long-term Monitor of Cometary Materials and the Potential Influences on the Earth During the Close Visit

Yong ZHAO1#+, Zhonghua YAO2
1INSTITUTE OF GEOLOGY AND GEOPHYSICS, CHINESE ACADEMY OF SCIENCES (IGGCAS), 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 on the Earth during close visit.


PS01-A006
Hourly Periodic Variations of Ultralow-frequency (ULF) Waves in Jupiter’s Magnetosheath

Weidong GU1#+, Zhonghua YAO2, Dongxiao PAN3, Yan XU2, Binzheng ZHANG4, Peter DELAMERE5, Suiyan FU6, Lun XIE6, Shengyi YE7, Yuening CHEN7, William DUNN8, Yong WEI1
1Institute of Geology and Geophysics, Chinese Academy of Sciences, China, 2Chinese Academy of Sciences, China, 3China University of Geosciences, China, 4The University of Hong Kong, Hong Kong SAR, 5University of Alaska Fairbanks, United States, 6Peking University, China, 7Southern University of Science and Technology, China, 8University College London, United Kingdom

Periodic variations are widely identified in Jovian system, varying from 10s of seconds to several days or even longer. These processes are strongly influenced by solar wind conditions, planetary rotation and Io’s volcanic activity. The ultralow-frequency (ULF) waves at 10s of minutes, which are the typical time scale of field-line resonance, are considered as a crucial process in driving Jovian energy circulation. The longer time-scale periodicities are likely associated with global mass circulation. While in this study, we focus on multi-hour variations of the ULF wave energy, which are difficult to identify within the magnetosphere due to the rapid planetary rotation modulation. Using the magnetic field observations from Juno and Galileo in Jupiter’s magnetosheath, we found multiple significant multi-hour periodicities, widely distributed from 2 to 10 hours, peaked at different values from case to case. The most common periodicities were between 3h and 5h, existing in both the dawn and dusk sides. These common periodicities are likely associated with the energy transport from inside to the magnetosheath.


PS01-A007
Excitation of Saturnian ECH Waves Within Remote Plasma Injections: Cassini Observations

Minyi LONG+, Xing CAO#, Xudong GU, Binbin NI
Wuhan University, China

Based on Cassini observations, we report representative electrostatic electron cyclotron harmonic (ECH) wave events observed in Saturn’s magnetosphere within remote plasma injections. Unlike local injections, remote injections are ‘older’ injection events that have evolved to form a dispersed signature in particle energy spectrum. We show that Saturnian ECH waves within remote injections present a strong fundamental band and much weaker high harmonic bands. By calculating the linear wave growth rates based on the measured electron distributions, we indicate that Saturnian ECH waves can be excited by the loss cone distribution of remotely injected, hot electrons of ~100 eV to several keV. We find that ECH waves tend to intensify with increased fluxes of injected hot electrons but weaken with increased evolution time of the flux tubes, which is consistent with the results of wave growth rates and improves the current understanding of the generation of ECH waves at Saturn.


PS01-A011
Automated Classification of Auroral Images with Deep Neural Networks

Zhiyuan SHANG#+
Chinese Academy of Sciences, China

Terrestrial auroras are highly structured that visualize the perturbations of energetic particles and electromagnetic fields in Earth’s space environments. However, the identification of auroral morphologies is often subjective, which results in confusion in the community. Automated tools are highly valuable in the classification of auroral structures. Both CNNs (convolutional neural networks) and transformer models based on the self-attention mechanism in deep learning are capable of extracting features from images. In this study, we applied multiple algorithms in the classification of auroral structures and performed a comparison on their performances. Trans-former and ConvNeXt models were firstly used in the analysis of auroras in this study. The results show that the ConvNeXt model can have the highest accuracy of 98.5% among all of the applied algorithms. This study provides a direct comparison of deep learning tools on the application of classifying auroral structures and shows promising capability, clearly demonstrating that auto-mated tools can help to minimize the bias in future auroral studies.


PS01-A016
Magnetic Field Structures in the Near-terminator Induced Magnetospheres of Venus and Mars

Sudong XIAO1#+, Tielong ZHANG2,3, Guoqiang WANG4, Ming-Yu WU4, Tong DANG3, Yuequn LOU4, Yuanqiang CHEN4
1Harbin Institute of Technology, Shenzhen, China, 2Austrian Academy of Sciences, Austria, 3University of Science and Technology of China, China, 4Harbin Institute of Technology, China

Venus and Mars, our two neighboring planets, have no global intrinsic magnetic fields, and the induced magnetospheres are formed in their solar wind interactions through mass loading of magnetic flux tubes carried by the solar wind and draping around the highly conducting ionosphere. Although they have similar global magnetic environments in their induced magnetosphere controlled by the interplanetary magnetic field and the solar wind motional electric field, their differences in planetary size, solar wind conditions, crustal magnetic fields, etc. also have measurable impacts. We comparatively study the magnetic field structures in the Venusian and Martian induced magnetospheres near the terminator via observations. The nature of their current systems and the features of magnetic structures such as flux ropes are examined in the near-terminator space and the effects of solar activity, interplanetary magnetic field, and crustal fields are explored. The results reveal the solar wind interaction with unmagnetized planets near the terminator, and a simulation provides a three‐dimensional view.


PS01-A020
Magnetic Reconnection in Jupiter's Undulating Magentodisk Current

Ruilong GUO1#+, Z. H. YAO2
1Shandong University, China, 2Chinese Academy of Sciences, China

Magnetic reconnection is crucial in magnetospheric dynamics and aurora borealis processes on planets. Magnetic reconnection is often identified in the diurnal magnetopause and the magnetotail. At Jupiter, rapid rotation and internal mass sources lead to an additional magnetodisk current sheet that encircles the planet. It is generally accepted that the magnetodisk reconnection site begins in the pre-evening sector and ends in the dawn sector before encountering the magnetopause. Here we demonstrate that the magnetodisk reconnection is not restricted to the night side but discretely distributed at all local times inside the magnetosphere. The reconnection sites also rotate with the magnetosphere, and the corresponding disturbed current exhibits undulating features.


PS01-A021
Global Spatial Distribution of Dipolarization Fronts in the Saturn's Magnetosphere: Cassini Observations

Sibo XU+, Shiyong HUANG#
Wuhan University, China

Dipolarization front (DF), characterized by a sharp increase of the south-north component of the magnetic field, is suggested to play an important role in transferring plasmas, magnetic fluxes, and energy in the planetary magnetosphere. Using the measurements from the Cassini spacecraft between January 1, 2005 and June 15, 2011, we successfully selected 96 DF events, and obtained the global spatial distribution of DFs in the Saturn's magnetosphere. For the first time, we found that DFs are distributed not only in the nightside magnetotail but also in the dayside magnetosphere. The dayside DF events are mainly located from X = 10 RS to X = 30 RS (RS is the Saturn's radius) while the nightside events have a wide range, up to X∼−50 RS. Moreover, the DFs are observed to be asymmetric in the south-northern hemisphere: ∼70% of events in the northern hemisphere and ∼30% of events in the southern hemisphere, which is likely to be due to the asymmetric orbit coverage of the Cassini in south-northern hemisphere. The occurrence of dayside DFs provides a strong evidence that the magnetic reconnection could also occur in the dayside of Saturn's magnetosphere. Thus, our results concerning the location and distribution of DFs are helpful for the study of the site of magnetic reconnection and energy transport/dissipation in Saturn's magnetosphere.


PS01-A024
Prediction of Axial Asymmetry in Jovian Magnetopause Reconnection

Junjie CHEN1#+, Binzheng ZHANG1, Dong LIN2, Peter DELAMERE3, Zhonghua YAO4, Oliver BRAMBLES5, Kareem SORATHIA6, Viacheslav MERKIN6, John LYON7
1The University of Hong Kong, Hong Kong SAR, 2National Center for Atmospheric Research, United States, 3University of Alaska Fairbanks, United States, 4Chinese Academy of Sciences, China, 5O.J. Brambles Consulting, United Kingdom, 6Johns Hopkins University Applied Physics Laboratory, United States, 7Dartmouth College, United States

We show the possible existence of a significant axial asymmetry in the reconnection separator at the Jovian magnetopause using first-principle, physics-based global simulations. Under eastward interplanetary magnetic field (IMF) conditions near Jupiter’s orbit, reconnection occurs at the southern-dusk and northern magnetopause with large shear angles between the magnetospheric and magnetosheath magnetic fields. When driven by the westward IMF, the reconnection position switches to the northern-dusk and southern magnetopause. Component reconnection at the southern-dusk/northern-dusk magnetopause is associated with the interaction of the IMF with the nearly-dipolar background fields. Nearly-antiparallel reconnection near the noon-midnight plane at the northern/southern magnetopause is related to the dawn-dusk asymmetric, helical, closed lobe magnetic fields, which is a consequence of significant planetary corotation effects and not expected at Earth. Such configuration is testable as Juno has proceeded its orbit to the high-altitude cusps and provides new insight into the interpretation of measurements from other rotationally-driven systems.


PS01-A028
The Responses of Jovian Broadband Kilometric Radio Emissions to Different Compressional Conditions

Yuening CHEN1#+, Shengyi YE1, Zhonghua YAO2
1Southern University of Science and Technology, China, 2Chinese Academy of Sciences, China

In planetary magnetosphere, plasma waves act as the medium for particles to transfer energy. Jupiter is the largest planet in our solar system, and the giant magnetosphere is full of energetic particles, producing intense radio emissions. When shock waves in the solar wind interact with the Jovian magnetosphere, the characteristics of Jovian radio emissions show distinct variations accordingly. This study focuses on the morphological characteristics of Jovian broadband kilometric radio emissions under different solar wind compressional conditions, i.e., quiet and compressed. Using observations from Juno and the Hubble Space Telescope, both the frequency range and duration of Jovian broadband kilometric radio emissions are studied, and we compared their variations during compressed and quiet solar wind conditions. Our results show that the frequency range of Jovian broadband kilometric radio emissions was greater under solar wind compression conditions, together with significantly longer duration. The distinct features of radio emissions under different solar wind conditions imply that solar wind conditions have important influences on Jovian auroral processes, and thus the radio emissions can be used as a diagnostic tool of solar wind interaction with Jovian magnetosphere.


PS01-A029
A Rapid Localized Deceleration of Earth's Radiation Belt Relativistic Electrons Driven by Storm Proton Injection

Zhaoguo HE1#+, Zhenpeng SU2
1Sun Yat-sen University, China, 2University of Science and Technology of China, China

Earth's radiation belt relativistic electron dropouts frequently occur during the main phase of geomagnetic storms, which have been partially attributed to the ring current ion enhancements causing geomagnetic field reconfigurations. In contrast to early studies on the global radiation belt response to the ring current buildup on a timescale of several hours, we here describe a rapid, localized, significant decay of relativistic electrons driven by freshly injected energetic protons during the 27 May 2017 geomagnetic storm. Near the proton injection front, the magnetic field lines were stretched outward, with an inferred migration of their equatorial crossings by ∼0.5 RE during several minutes. Because of the betatron and Fermi decelerations, the relativistic electron fluxes decreased by 2–3 orders of magnitude with pitch-angle distributions evolving from pancake/flat-top type to cigar type. This rapid localized response pattern of relativistic electrons could be general over strong particle injections during both geomagnetic storms and substorms.


PS02-A002
Measuring the Depth of Planetary-scale Changes in Jupiter from Juno Microwave Radiometer Observations

Glenn ORTON1#+, Shawn BRUESHABER2, Michael H. WONG3, Thomas MOMARY1, Steven LEVIN1, Scott BOLTON4, Kevin BAINES5, Emma DAHL1, James SINCLAIR1
1Jet Propulsion Laboratory, California Institute of Technology, United States, 2Western Michigan University, United States, 3SETI Institute, United States, 4Southwest Research Institute, United States, 5University of Wisconsin-Madison, United States

We report on variability of the microwave brightness of Jupiter’s axisymmetric bands over 2016-2022 using Juno Microwave Radiometer (MWR) observations. We first examined the depth of changes in regions where visible changes have taken place. The variability in channels sensitive to depths of 9-50 bars of pressure are generally much smaller than those at pressures of 0.7-3 bars. An exception to this is in the northern component of Jupiter’s Equatorial Zone (2°N-6°N), whose variability at depth does not correspond to any visible feature in the upper atmosphere, although it might be a precursor to the short-lived 2018-2019 Equatorial Zone disturbance. At 0.7-3 bars, a decrease in the antenna temperature in the northern component of the North Equatorial Belt (12°N-15°N) is coincident with its visible brightening and drop of 5.1-µm radiance, both implying increased cloud and NH3 opacity in 2021. Even though the visibly dark North Equatorial Belt expanded northward into latitudes more typically associated with visibly bright regions that are cold at 5.1 µm (16°N-19°N), known as the North Tropical Zone (Fletcher, et al. 2017. Geophys. Res. Lett. 44, 7140), we do not detect any corresponding change of the MWR antenna temperature. Although there are substantial changes in the visible and 5.1-µm appearance of the northern component of the North Temperate Belt (24°N-26°N) as well as in the MWR antenna temperatures, the two do not appear to be correlated with one another. An important part of our next steps in this research will be to examine which of the MWR variabilities in the zonal-mean microwave brightness are the result of zonally discrete features in the atmosphere, particularly the North Equatorial Belt (6°N-15°N).


PS02-A014
A Juno-era View of Electric Currents in Jupiter's Magnetodisk

Zhiyang LIU1#+, Qiugang ZONG1, Michel BLANC2
1Peking University, China, 2Institute for Research in Astrophysics and Planetology, France

Recent observations from Juno provided a detailed view of Jupiter's magnetodisk, including its magnetic fields, waves, plasmas and energetic particles. Here, we contribute to Juno results by determining the electric currents threading the magnetodisk and their coupling to field-aligned currents (FAC) in the midnight-to-dawn local time sector. We first derive from Juno magnetic field data the spatial distributions of the height-integrated radial (Ir) and azimuthal (Ia) currents in the magnetodisk, and then calculate the FACs from the divergence of the two current components. The Ir-associated FAC, Jr, flows into and out of the magnetodisk at small and large radial distances, respectively, approximately consistent with the axisymmetric corotation enforcement model. On the other hand, Ia decreases with increasing local time everywhere in the local time sector covered, indicating an additional FAC (Ja) flowing out of the magnetodisk. From Ia and Ja, we conclude that the influence of the solar wind, which compresses the dayside magnetosphere and thus breaks the axisymmetry of currents and fields, reaches deep to a radial distance of at least 20 Jupiter radii. Our results provide observational constraints on Jupiter's magnetosphere-ionosphere-thermosphere coupling current systems, on their relation to the main auroral emission and on the radial mass transport rate in the magnetodisk, which we estimate to be close to ~1500 kg/s.


PS04-A002
Photoelectron Boundary: The Top of the Dayside Ionosphere at Mars

Shaosui XU1#+, David MITCHELL1, James MCFADDEN1, Christopher FOWLER2, Gwen HANLEY1, Tristan WEBER3, David A. BRAIN3, Yingjuan MA4, Gina DI BRACCIO5, Christian MAZELLE6, Shannon CURRY1
1University of California, Berkeley, United States, 2West Virginia University, United States, 3University of Colorado Boulder, United States, 4University of California, Los Angeles, United States, 5NASA Goddard Space Flight Center, United States, 6Institute for Research in Astrophysics and Planetology (IRAP), National Center for Scientific Research (CNRS) - University of Toulouse (UPS) - National Center for Space Studies (CNES), France

The interaction between Mars and the solar wind results in different plasma regimes separated by several boundaries, among which the separation between the sheath flow and the ionosphere is complicated. Previous studies have provided different and sometimes opposite findings regarding this region. In this study, we utilize observations from the Mars Atmospheric and Volatile EvolutioN (MAVEN) mission to revisit boundaries within this region and perhaps reconcile some differences. More specifically, we start with the photoelectron boundary (PEB), a topological boundary that separates magnetic field lines having access to the dayside ionosphere (open or closed) from those connected to the solar wind on both ends (draped). We find that large gradients in the planetary ion density occur across the PEB and that the dominant ion switches from heavy planetary ions to protons near the PEB, indicating the PEB falls within the ion composition boundary (ICB). Furthermore, our results show that the PEB is not a pressure balance boundary; rather the magnetic pressure dominates both sides of the PEB. Meanwhile, we find that the PEB is located where the shocked solar wind flow stops penetrating deeper into the ionosphere. These findings suggest the PEB marks the top of the Mars dayside ionosphere and also the interface that the sheath plasma flow deflects around the obstacle going downstream.


PS04-A004
Sporadic E-like Event Driven by Wind Shear in the Martian Ionosphere

Rong TIAN#+, Chunhua JIANG
Wuhan University, China

Sporadic E is the oldest known ionospheric disturbance on Earth, which can affect the propagation of radio signals. According to recent studies, Es-like events on Mars are driven by magnetic shear. The rift, which was not observed on Earth, was also observed on Mars. While both magnetic and wind shear can theoretically drive the formation of Es-like events, no observational evidence shows that wind shear can also drive the formation of Es-like events on Mars. In this study, we report a new observation of a sporadic E-like (Es-like) event with both layer and rift in the ionosphere of Mars by NASA's Mars Atmosphere and Volatile EvolutioN (MAVEN) spacecraft. Wind shear was observed during the event, and our preliminary statistics suggest that wind shear may be a common phenomenon on Mars. This study provides new observations of Es-like events on Mars and constructs a picture of Es-like events through observations of neutral wind fields from NGIMS. The observational result supports the theory that wind shear could drive Es-like events on Mars.


PS04-A006
Partial Absorption of Surface Echoes Observed by MARSIS During the December 2014 Solar Event at Mars: Initial Results from a Data-model Comparison

Yuki HARADA1#+, Yuki NAKAMURA2, Beatriz SANCHEZ-CANO3, Mark LESTER3, Naoki TERADA2, Francois LEBLANC4
1Kyoto University, Japan, 2Tohoku University, Japan, 3University of Leicester, United Kingdom, 4National Centre for Scientific Research, France

Solar energetic particles (SEPs) drive a variety of phenomena in planetary atmospheres. At Mars, the SEP precipitation leads to the global emission of "diffuse aurora" from the nightside atmosphere. Since the recent discovery of the Martian diffuse aurora, their properties have been investigated from both observation and modeling perspectives. A Monte Carlo model developed by Nakamura et al. is one of the numerical models solving the interaction between SEPs and the Martian atmosphere. Based on the measured SEP energy spectra, this model is capable of reproducing the peak altitude and relative altitude profile of the observed auroral emission. The new model by Nakamura et al. also provides the altitude profile of electron density in the nightside ionosphere of Mars during SEP events, thereby suggesting another use case of data-model comparison focusing on "radar blackouts" at Mars. Radar blackouts refer to a significant attenuation of trans-ionospheric radar signals from Martian orbiters caused by enhanced ionization and electron-neutral collisions below ~100 km altitudes as often observed during SEP events. The degree of signal attenuation provides a proxy for the low-altitude electron densities that are otherwise difficult to measure. We investigate the evolution of the low-altitude electron densities during SEP events and discuss the relative roles of different ionizing agents by comparing Nakamura et al.'s model against the radar signal attenuation recorded in the MARSIS Active Ionospheric Mode data during the December 2014 SEP event. We report the initial results from the data-model comparison.


PS04-A007
Escape of Martian Ionospheric Proton Due to the Resonant and Non-resonant Interactions with Large-amplitude Magnetosonic Waves

Xiaotong YUN1+, Fu SONG1#, Binbin NI1, Jun CUI2,3
1Wuhan University, China, 2Sun Yat-sen University, China, 3Chinese Academy of Sciences, China

Ion escaping frequently occurring in the Martian space leads to a significant influence on Martian plasma and atmospheric environment. However, the dominative mechanism of ion escaping remains unclear. In this study, we quantitatively investigate the wave-induced proton escaping driven by large amplitude magnetosonic (MS) waves in the Martian ionosphere. The resonant condition analysis shows that via Landau resonance the protons with Ek0 = ~10–104 eV can interact with MS waves. By using our developed test particle code, we simulate the proton dynamics and find that on the time scale of ~6 s, the MS waves combined with the crustal magnetic fields scatter the protons’ pitch-angle as <(Δα)2> = 10-2–10-1 rad2 and diffuse the protons’ energy as <(ΔEk/Ek0)2> = ~ 10-2. The calculations also suggest that beyond the Landau resonance, the non-resonant effect can effectively scatter the protons with lower energy ~1–10 eV. Furthermore, to represent the proton escaping at the topside of the crustal magnetic field, we construct a global test particle simulation code involving the wave scattering effect. The results suggest that the net proton escaping probability caused by the MS wave-driven resonant and non-resonant process is 0.6269%, which is ~2 times higher than that without MS waves. Our results indicate that the large-amplitude MS waves are very important on Martian ionospheric proton escaping by wave-particle interactions, which is helpful for better understanding the evolution of the Martian plasma and atmospheric environment.


PS04-A011
A Study of the Energy Spectrum of Photoelectrons and Auger Electrons Emitted from the Sunlit Lunar Surface

Masahisa KATO1#+, Yuki HARADA1, Shaosui XU2, Andrew POPPE2, Jasper HALEKAS3, Yohei MIYAKE4, Hideyuki USUI4, Masaki NISHINO5, Toru MATSUMOTO1
1Kyoto University, Japan, 2University of California, Berkeley, United States, 3The University of Iowa, United States, 4Kobe University, Japan, 5Japan Aerospace Exploration Agency, Japan

Since the moon does not have a dense atmosphere and its global intrinsic magnetic field, the lunar surface directly interacts with its ambient plasma. The lunar surface potential changes as a result of the interaction. Auger electron emission is one of the interactions between photons and solid surfaces. Auger electrons are emitted from the surfaces with characteristic energy depending on the chemical composition and the process. In this study, we developed a numerical model which explains an energy spectrum of photoelectrons and Auger electrons emitted from the lunar surface. Through this model, we discuss the electrostatic potential distribution with a height from the lunar surface.


PS04-A012
An Unexpected Double-peak Structure in Diurnal Variation of Martian Upper Atmosphere

Huijun LE1#+, Libo LIU1, Yiding CHEN2, Ruilong ZHANG1, Hui ZHANG2
1Institute of Geology and Geophysics, Chinese Academy of Sciences, China, 2Chinese Academy of Sciences, China

Previous studies have shown that the Martian ionosphere and thermospheric atmosphere are mainly controlled by photochemical processes, especially near the peak electron density height of the ionosphere. Therefore, it can be considered that the diurnal variation of ionospheric electron density and thermospheric neutral density on Mars is mainly controlled by solar irradiation flux, which increases rapidly after sunrise, peaks around noon, and drops sharply after sunset. Maven has accumulated more than eight years of data since October 2014, covering different Martian seasons, local times, solar activity and altitudes. Through statistical analysis, we found for the first time that the diurnal variation of the ionospheric electron and ion density and thermospheric gas density of Mars has a significant double-peak structure, with the first peak appearing around LT 08-09, the second peak appearing around LT15-17, and an low value at ~LT12. To further confirm the accuracy of the results, we conducted empirical modeling of electron density, ion density and neutral gas density based on the LWP and NGISM observation data, and the model results reproduced the double-peak structure found statistically. This further confirms the double-peak structure of the ionosphere. These studies show that the changes in Mars' upper atmosphere are far more complex than we had expected, with direct effects from the solar wind above, effects from the lower atmosphere below, and strong dust storms that can propagate up to the upper atmosphere.


PS05-A007
Statistical Properties of Plateau-like Turbulence Spectra in the Martian Magnetosheath: Maven Observations

Hui LI1#+, Wence JIANG2, Xiaodong LIU2, Daniel VERSCHAREN3, Chi WANG2
1National Space Science Center, Chinese Academy of Sciences, China, 2Chinese Academy of Sciences, China, 3University College London, United Kingdom

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.


PS05-A008
ULF Modulations on Plasma Environment and Coherent Waves of Mercury's Magnetosphere: Messenger's Observation

Jiutong ZHAO#+, Qiugang ZONG
Peking University, China

Ultra low frequency (ULF) waves are fundamental waves that can energize, transport, and scatter charged particles in planetary magnetospheres. With the measurements from MErcury Surface, Space ENvironment, GEochemistry, and Ranging (MESSENGER), we investigate the proton flux fluctuations and coherent waves associated with a series of ULF waves on the flanks of Mercury's magnetosphere. The ULF waves are mainly compressional with a frequency of ∼15 mHz and significantly modulate the intensity of proton flux. The coherent waves accompanied by the ULF waves correspond to a higher frequency (∼1 Hz). The wave power and compressibility of the coherent waves vary quasi-periodically with the ∼15 mHz ULF waves. We conclude that the compressional ULF waves modulate the coherent waves with higher frequency. This modulation might result from the associated periodic proton flux changes and helps us understand the nature of the ∼1 Hz waves better.


PS05-A010
MMS Observations of Upstream 3-seconds Waves in Earth’s Foreshock Region

Gangkai POH1,2#+, Guan LE1, Scott BOARDSEN3, Norberto ROMANELLI1, Daniel GERSHMAN1, Weijie SUN4, Li-Jen CHEN1
1NASA Goddard Space Flight Center, United States, 2Catholic University of America, United States, 3University of Maryland, Baltimore, United States, 4University of California, Berkeley, United States

Ultra-low frequency (ULF) waves have been observed and studied extensively in the Earth’s ion foreshock region, with their basic wave properties determined. ULF waves can be formed from the backstreaming ions in the ion foreshock region upstream of the bow shock when the solar wind interacts with the terrestrial bow shock. 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 [Le et al., 1992; Blanco-Cano et al., 1999] and more recently by MMS [e.g. Wang et al., 2021]. 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 ~25 potential 3-seconds wave intervals as observed by MMS. 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 also analyzed the MMS FPI Burst mode data 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.


PS05-A011
MESSENGER Observations of Distribution of Planetary Ions Near Mercury’s Space: Their Escape Rates and Dependence on True Anomaly Angle

Weijie SUN1#+, Ryan DEWEY2, James SLAVIN2, Jim RAINES2, Gangkai POH3,4
1University of California, Berkeley, United States, 2University of Michigan, United States, 3NASA Goddard Space Flight Center, United States, 4Catholic University of America, United States

This study presents MESSENGER observations of the distribution of O+-group ions and Na+-group ions in the regions near Mercury’s space. The regions include the solar wind, magnetosheath, and magnetosphere. We have investigated the distributions of O+-group ions and Na+-group ions in these regions separately and divided them into four true anomaly angles (TAAs) groups. We have shown their distributions under convection electric field coordinates. The densities of O+-group ions and Na+-group ions are the highest in the magnetosphere and the lowest in the solar wind, and their densities show clear dependencies on the TAAs. The escape rates of the O+-group ions and Na+-group ions are estimated in different regions and different TAA intervals.


PS05-A013
Validation of the AWSoM Solar Wind Magnetic Field Model with Upstream Mercury Solar Wind Conditions from MESSENGER Observations

Rayta PRADATA1,2#+, Gangkai POH2,3, Ana PERUZA4, Zhenguang HUANG5, Nishtha SACHDEVA5, Evangelia SAMARA6
1University of Delaware / Catholic University of America, United States, 2NASA Goddard Space Flight Center, United States, 3Catholic University of America, United States, 4George Mason University, United States, 5University of Michigan, United States, 6Royal Observatory of Belgium, Belgium

Previous studies from MESSENGER have shown that plasma dynamical processes within Mercury’s magnetosphere are strongly driven by its solar wind conditions. However, the upstream region of Mercury’s magnetosphere has no constant solar wind monitor to provide information about them when the spacecraft is inside the planet’s plasma environment, which emphasizes the importance of a solar wind model to accurately predict their conditions. This project aims to validate and assess the capability of the Alfvén Wave Solar Atmosphere Model (AWSoM) developed at the University of Michigan in predicting solar wind Interplanetary Magnetic Field (IMF) condition (polarity and magnitude) by comparing its simulated outputs with solar wind data from MESSENGER. We have identified solar wind intervals in the MESSENGER’s magnetic field measurements from three Carrington Rotations (i.e. CR 2132, 2138, and 2139) to be compared with AWSoM’s simulation results using ADAPT-GONG magnetograms as the input. Each of the 12 ADAPT realizations for each Carrington rotation period was compared with the solar wind data IMF measurements, and assessed on how well they agree with MESSENGER’s observations. The comparative analysis technique Dynamic Time Warping (DTW) is used to make this assessment in this study, due to the time-shifted alignment typically observed between the observed and simulated solar wind data. The technique is implemented on all 12 realizations of each simulation run to determine the “best-fit” comparison, accounting for the time shift, using the DTW “cost” or “score” parameter. The data-model comparison methods and results presented in this study will contribute to future studies related to solar activity and solar wind IMF, and applied towards other planetary environments (e.g. MAVEN for Mars) and future spacecraft missions to Mercury (e.g. Bepi-Colombo).


PS05-A016
Magnetic Shielding of Earth’s Atmosphere from the Solar Wind

Parker HINTON1#+, David A. BRAIN1, Neesha SCHNEPF1, Yingjuan MA2, Fran BAGENAL3
1University of Colorado Boulder, United States, 2University of California, Los Angeles, United States, 3University of Colorado, Boulder, United States

For decades it has been accepted canon by many that Earth’s intrinsic magnetic field works to shield its atmosphere from escape caused by the solar wind (Watson and Junge 1962, Hutchins and Jakosky 1997, Lundin et al. 2007). This hypothesis has recently fallen under the criticism that even without an intrinsic magnetic field a magnetosphere will still be induced, which can protect the unmagnetized planet from solar wind ablation (Gunell et al. 2018, Ramstad et al. 2021). We use BATSRUS, a compressible multi-species magnetohydrodynamic code, to globally simulate the plasma interaction between the solar wind and Earth’s magnetosphere under two different scenarios i) the present-day dipole magnetic field and ii) demagnetized Earth (no intrinsic field). We present first results quantifying and comparing atmospheric escape between the two scenarios, helping answer the question as to whether or not Earth’s intrinsic magnetic field shields its atmosphere. We also explore what atmospheric escape from Earth may be like during geomagnetic reversal, which is when the Earth's magnetic field reverses polarity. Reversals occur in Earth's history on average every 450 ky. The last major event in the geologic record is the Brunhes–Matuyama reversal, which occurred 780 ky ago and lasted for 22 ky. Such an event can leave the Earth relatively unprotected by its generally strong intrinsic dipole magnetic field for an extended period of time.


PS05-A018
Global MHD Simulation of the Planetary Magnetosphere: Uranus and Neptune

Kyung Sun PARK#+
Chungbuk National University, Korea, South

Global magnetohydrodynamic (MHD) has successfully reproduced overall magnetospheric dynamics and ionospheric phenomena for the Earth. However, understanding how the energy and momentum transfer from the Sun to Uranus and Neptune is a complex problem with many different aspects. The surface magnetic field at the dipole equator of Uranus and Neptune have smaller than Earth. Also, one of the significant characteristics of Uranus and Neptune is that the rotation axis and the magnetic dipole axis are separated by a large angle. To understand where the magnetic reconnection occurs, how the reconnected field lines move to the tail, and how much energy is transported from the solar wind, I have performed a three-dimensional global MHD simulation to examine the effect of the tilt with a weak solar wind condition. The input parameter of the simulation used the average value of solar wind observed from Voyager 2 and NEW HORIZONS. The simulation box is (nx, ny, nz) = (600, 400, 400) with a uniform grid spacing of 0.5 Rp. The simulation results show the large-scale 3D magnetic field configuration and plasma flow in outer planetary magnetospheres and the main differences between the two planetary configurations will be discussed in this study.


PS06-A002
Desorption of Hydrogen Sulfide Induced by VUV Irradiation

Yen-Yu HSU1#+, Chun-Chi HUANG1, Yu-Jung CHEN1, Guillermo Manuel MUÑOZ CARO2
1National Central University, Taiwan, 2Centro de Astrobiología (INTA-CSIC), Spain

In cold dense clouds, most of the molecules should exist in the solid phase because of the low temperature near 10 K. However, astrophysicists can still observe a large number of gas phase molecules. Since thermal desorption is absent in this region, therefore photon-induced desorption or photodesorption is expected to contribute to the ejection of molecules from ice in cold regions of space. The secondary vacuum ultraviolet (VUV) field caused by the cosmic rays reacting with molecular hydrogen is a significant photon source in dark cloud interiors and radiation-protected circumstellar regions.
Hydrogen sulfide (H2S), one of the most abundant sulfide-bearing species in the interstellar medium (ISM), can be seen as a precursor of biochemical molecules. Oba et al. (2018) proposed the chemical desorption caused by hydrogen atoms should be more effective than the photodesorption in cold dense clouds. However, they estimated the value by the absorption cross-section of H2S instead of measuring its photodesorption directly. Under the VUV irradiation, Cazaux et al. (2021) showed H2Sx (x>1) and S-chain (Sx) molecules are the main photoproducts, but there is no photodesorption information in detail.
In this study, the effect of structure effect on VUV photondesorption of H2S ice was measured by depositing H2S ice at 13 K and 70 K, respectively. The results show that the photodesorption yield of H2S ice deposited at 13 K is higher than that deposited at 70 K, and this might be related to the binding energy and the effective surface area of ice. Furthermore, the H2S ices with different initial thicknesses were examined, and the energy transfer length for photodesorption is around 5−10 ML.
References:
1. Cazaux, S., et al. arXiv preprint arXiv:2110.04230 (2021).
2. Oba, Y., et al. Nature Astronomy 2.3 (2018): 228-232.


PS06-A007
VUV Photoinduced Energy Transfer in 13CO Ice Deposited on CO/CO2 Ice

Chun-Chi HUANG1#+, Yen-Yu HSU1, Guillermo Manuel MUÑOZ CARO2, Yu-Jung CHEN1
1National Central University, Taiwan, 2Centro de Astrobiología (INTA-CSIC), Spain

The VUV-induced photodesorption of CO ice has been studied in the last few decades. Chen et al. (2014) show that the process of CO photodesorption induced by VUV photons with broadband energy is more complex than the sum of individual processes induced by the monochromatic light source at the same energy range. It results from the difference in absorption cross-section between the parent molecules (CO) and photoproduct (CO2) in the Ly-α and molecular H2 emission ranges. In this study, 13CO ice (7 ML) is deposited on the top of CO or CO2 ice (18 ML) and irradiated by VUV photons with a high proportion of Ly-α emission (76.4%) produced by a microwave-discharged hydrogen flow lamp (MDHL). We find that for the 13CO ice deposited on the CO2 ice, the photodesorption yield of 13CO is higher than that deposited on CO ice. The result supports that more energy can transfer from products (CO2) to parent molecules (CO). Furthermore, the energy transfers from CO2 to CO decreases because CO­2 dissociates into CO during the VUV irradiation.


PS06-A009
Formation of Insoluble Organic Material from the Ultraviolet Irradiation of Laboratory Ice Photolysis Residues

Michel NUEVO1#+, Brian FERRARI2,3, 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 preliminary results from the study of ice photolysis residues which were exposed to ultraviolet (UV)/extreme UV (EUV) photon radiation. The residues were produced from the simultaneous deposition and UV irradiation of ice mixtures of astrophysical interest (H2O, CH3OH, CO, NH3, without/with N2 and/or O2, and without/with small quantities of aromatic compounds) at 15–20 K using an H2 lamp, which emits 10.2-eV (121.6 nm) Lyman-α photons and a continuum at 7.5–8 eV (155–165 nm). After warm-up to room temperature and subsequent sublimation of volatile compounds, the refractory materials (residues) recovered at room temperature were analyzed with infrared (IR) microscopy and then further irradiated with UV/EUV photons at a synchrotron facility, on a beamline providing a broad-band photon beam in the 4–45-eV range with a ~1016 photons s-1 flux.2 The residues were UV/EUV irradiated with increasing photon doses ranging from ~1018 to ~1021 photons, i.e., covering 4 orders of magnitude and relevant to those experienced by ice-coated grains in the protosolar nebula.1. After UV/EUV irradiation, residues were analyzed with IR microscopy and the data compared to those before irradiation to identify changes in chemical composition as a function of the photon dose. UV/EUV-irradiated residues were also analyzed with other techniques such as nanoscale secondary-ion mass spectrometry (nanoSIMS) to the study the changes in isotopic composition, and scanning transmission electron microscopy to look at variations in structure and C bonding distribution. Results will be compared with data from extraterrestrial materials, in particular, meteoritic insoluble organic material (IOM) and interplanetary dust particles (IDPs). References: [1] Ciesla, F.J., Sandford, S.A., Science, 336, 452 (2012). [2] Nuevo, M., Chen, Y.-J., Hu, W.-J., et al., Astrobiology, 14, 119 (2014).


PS06-A012
Observations of Various Meteor Optical and Plasma Trails with MIOS and the Properties of Their Parent Meteoroids

Guozhu LI1#+, Yi LI1, Lianhuan HU1, Haiyong XIE2, Wenjie SUN1, Xiukuan ZHAO1, Baiqi NING1
1Chinese Academy of Sciences, China, 2Institute of Geology and Geophysics, Chinese Academy of Sciences, China

Meteoroids entering the Earth’s atmosphere significantly disturb the background ionosphere, producing ionized columns and plasma density irregularities, change the ionospheric composition, and even seed large-scale ionospheric irregularity structures. Under the support of the National Natural Science Foundation of China, the Meteor and ionospheric Irregularity Observation System (MIOS) facility, which consists of multi-station optical subsystem at Ledong (18.4°N, 109°E) and Sanya (18.3°N, 109.6°E), and radar subsystem including a 38.9 MHz all-sky interferometric radar and a 47.5 MHz coherent phased array radar at Ledong, was recently completed. The MIOS was specifically designed to have the following capabilities: (a) To simultaneously obtain radar and optical features of meteors within a large field of view; (b) To observe meteor echoes in specific directions with high sensitivity by steering a narrow radar beam; (c) To unambiguously locate meteor echoes using multi-baseline spatial-domain interferometry in order to identify field-aligned and non-field-aligned irregularities; (d) To observe the structural evolution of plasma density irregularities by steering a narrow radar beam on a pulse-to-pulse basis or by using fixed wide radar beam multi-baseline imaging techniques; (e) To obtain the physical and chemical properties of meteoroids producing/not producing meteor echoes. In this talk we will present some preliminary observations of various meteor optical and plasma trail phenomena and the properties of their parent meteoroids.


PS06-A013
Some Characteristics of the Geminids Meteor Shower Through TMDS Observations Between 2018 and 2022

Zhong Yi LIN1#+, Po-Chih CHUNG2, Jim LEE3, Hsin-Chang CHI4
1Institute of Astronomy, Taiwan, 2National Central University, Taiwan, 3Taipei Astronomical Museum, Taiwan, 4National Dong Hwa University, Taiwan

We have obtained the characteristics of the Geminid meteoroid stream by TMDS (Taiwan Meteor Detector System) through observations from 2018 to 2022. Meteors with radiant from Geminids are summarized as observed over an eligible period between early December and mid-to-late December amid the peak shower activity was found on Dec. 13. The associated solar longitude during this period is from 237° to 289° and the peak period is between 261° and 262°. In total, more than six thousand meteors have been identified as Geminids. The absolute magnitudes, the geocentric velocity, the radiant of the shower, and population index distributions are therefore statistically analyzed for comparisons with available investigations. No obviously outburst of the Geminids meteor shower has been detected. In addition, meteors with components from simultaneous multi-station detections in the TMDS are sorted out to determine associated orbits (~ 400 orbits), of which the similarities with their parent body, (3200) Phaethon, are attained successively by invoking the DSH criterion.


PS06-A015
Study of Meteor Spectra Recorded by the MIOS

Yi LI#+, Guozhu LI, Zhi WU
Chinese Academy of Sciences, China

Understanding the physical and chemical properties of meteoroids is helpful to reveal how the Solar System formed. A double-station optical video subsystem located in Ledong (18.4°N, 109°E) and Sanya (18.3N,109.6°E), China, which is a part of the Meteor and ionospheric Irregularity Observation System (MIOS), was developed recently. The MIOS is designed for investigating the properties of meteoroids entering the Earth’s atmosphere and how they affect the Earth’s space environment, for example the ionosphere. The observations of meteor spectra and common volume optical trails from the MIOS optical subsystem allow us to determine the emission from meteoroids and atmospheric species, and calculate the meteor velocity, trajectory and orbital parameters, and then we can distinguish the characteristics of populations of differently sized meteoroids and infer the relationship between meteoroids and their parent bodies. Numerous meteor spectra and their related trails were observed by the MIOS optical subsystem. Here we report preliminary results of the meteoroids observed in 2019 and 2020.


PS06-A018
Reflectance Spectral Variation of Hydrated and Dehydrated Carbonaceous Chondrites

Jinfei YU1,2+, Haibin ZHAO1#, Yunzhao WU3
1Chinese Academy of Sciences, China, 2University of Science and Technology of China, China, 3Purple Mountain Observatory, Chinese Academy of Sciences, China

Carbonaceous chondrites provide vital information on the early Solar System and their parent bodies’ history. We Investigated the 1-25 μm infrared spectral features of 17 carbonaceous chondrites with different petrologic properties and alteration degrees, and the spectral variation laws of the alteration and metamorphism were developed. With the increasing of aqueous alteration, the 3 μm band, diagnostic of OH-bearing minerals and water, and the 6 μm band, diagnostic of water molecules, both features increase in strength and band centers shift to the short-wavelength. With more alteration, a sharp absorption feature at 2.72μm shows in 3 μm band, which is similar to serpentine’s 3 μm absorption feature. Vibrational features of silicate minerals control the 10μm and 20μm regions. The 12.4 μm /11.4 μm reflectance ratio reduces and the reflectance peak in 9-14 μm region shifts to short-wavelength because of the conversion of anhydrous silicates to phyllosilicates. In the 15-25 μm region, with the thermal metamorphism processes, the single reflectance peak at 22.1 μm changes to two peaks at 19 μm and 25 μm, spectral curve becomes rough, which is likewise explained by the increase of anhydrous silicate with the increase of recrystallized olivine. These results can provide new constraints on C-complex asteroids’ volatile-rich compositions and their parent bodies’ thermal evolutionary history.


PS08-A006
Observing the Martian Atmosphere in the Ultraviolet: Science Updates from MAVEN IUVS

Daniel LO1#+, Sumedha GUPTA2, Roger YELLE3, Joseph EVANS4, Emmaris SOTO4, Matteo CRISMANI5, Sonal JAIN2, Justin DEIGHAN2, Nick SCHNEIDER2
1University of Michigan, United States, 2University of Colorado Boulder, United States, 3The University of Arizona, United States, 4Computational Physics, Inc., United States, 5California State University, United States

Since entering Martian orbit more than eight years ago (four Mars years), MAVEN’s Imaging Ultraviolet Spectrograph (IUVS) has been making observations of the Martian atmosphere in the far and mid ultraviolet (110--340 nm). Regular dayglow and occasional occultation observations have allowed us to map the composition and structure of the atmosphere, as well as to monitor how these vary diurnally, seasonally, interannually, and in response to solar events. The recent improvement in our characterization of the O I dayglow emission at 297 nm has extended our high-frequency monitoring of temperatures and wave activity from the original 130--170 km altitude down to 80 km. IUVS has also made the first direct detection and measurement of atomic carbon in the Martian atmosphere, and these measurements point to higher carbon abundances and escape rates than modeled. Since its discovery of a Mg+ layer in the atmosphere in 2015, IUVS has continued to map this meteoric ion layer in unprecedented detail. We found this layer to be persistent, but with significant variation with latitude, longitude, season and local time. We will be providing more details on these observations and recent scientific results.


PS08-A008
In-flight Calibration of the Magnetometer on the Mars Orbiter of Tianwen-1

Zhuxuan ZOU1+, Yuming WANG1#, Tielong ZHANG2,1, Guoqiang WANG3, Sudong XIAO4, Zonghao PAN1
1University of Science and Technology of China, China, 2Austrian Academy of Sciences, Austria, 3Harbin Institute of Technology, China, 4Harbin Institute of Technology, Shenzhen, China

Mars Orbiter Magnetometer (MOMAG) is one of seven science payloads onboard Tianwen-1’s orbiter. Unlike most of the satellites, Tianwen-1’s orbiter is not magnetically cleaned, and the boom where placed the magnetometer’s sensors is not long enough. These pose many challenges to the magnetic field data processing. In this paper, we introduce the in-flight calibration process of the Tianwen-1/MOMAG. The magnetic interference from the spacecraft, including spacecraft generated dynamic field and slowly-changing offsets are cleaned in sequence. Then the calibrated magnetic field data are compared with the data from the Mars Atmosphere and Volatile EvolutioN (MAVEN). We find that some physical structures in the solar wind are consistent between the two data sets, and the distributions of the magnetic field strength in the solar wind are very similar. These results suggest that the in-flight calibration of the MOMAG is successful and the MOMAG provides reliable data for scientific research.


PS08-A012
Observation Plans for Mars and Its Moons by Using the MMX Infrared Spectrometer (MIRS)

Takahiro IWATA1#+, Hiromu NAKAGAWA2, Fuminori TSUCHIYA2, Shohei AOKI3, Moe MATSUOKA4, Hiroyuki KUROKAWA5, Tomoki NAKAMURA2, Maria Antonietta BARUCCI6, Jean-Michel REESS6, Pernelle BERNARDI6, Alain DORESSOUNDIRAM6, Sonia FORNASIER7, Michel LE DU8, Veronique PIOU8, Eric SAWYER8, Nathalie PONS8
1Japan Aerospace Exploration Agency, Japan, 2Tohoku University, Japan, 3The University of Tokyo, Japan, 4National Institute of Advanced Industrial Science and Technology, Japan, 5Tokyo Institute of Technology, Japan, 6Paris Observatory, France, 7Paris Diderot University, France, 8National Centre for Space Studies, France

MIRS (MMX InfraRed Spectrometer) is a push-broom imaging spectrometer in the wavelength range of 0.9 to 3.6 micrometers which is one of the instruments to be installed on the Martian Moons Exploration (MMX) spacecraft. It has a field-of-view (FOV) of 3.3 deg width with instantaneous-FOV (IFOV) of 0.35 mrad, which can be scanned by the inner along-track scan mirror in the range of ±20 deg. MIRS will observe absorptions of hydroxide or hydrated minerals on Phobos and Deimos. It will also monitor the Martian atmosphere with particular attention to spatial and temporal changes as clouds, dust and water vapor. We will report and discuss on the science targets, the observation plans, and the design results of instruments. 


PS08-A023
Noachian Volcanism: Implication for Thermo-chemical Evolution of Early Mars

ALKA RANI1#, Yash SRIVASTAVA2+, Amit Basu SARBADHIKARI2
1NASA Marshall Space Flight Center, United States, 2Physical Research Laboratory, India

Geochemical information derived from the Martian orbiter missions provides insight into the various geologic processes. An earlier study based on orbiter geochemical data on Hesperian and Amazonian surfaces depicts that magmatism has chemically evolved. However, persistent weathering and resurfacing could have caused substantial geological changes that make a thorough examination of Noachian volcanism difficult. Therefore, understanding the thermo-chemical processes and evolution at the early stage of Mars is limited by the less constrained composition of the Noachian period. To understand the thermo-chemical evolution of the Martian interior at its early stage we investigate the Noachian-aged volcanic regions Arabia Terra, Solis (N1), and Argyre (N2). For the bulk chemical composition of the study areas, we use the latest geochemical provinces dataset of Mars, which is based on the latest elemental mass fraction maps of five-degree resolution by Nuclear Gamma-Ray Spectroscopy (GRS) data onboard Mars Odyssey 2001. Using pMELTS we derive formation pressure (P) and temperature (T) conditions and estimate the depth and mantle potential temperature. The average formation pressure of Arabia Terra shows a range from 1.3 to 1.7 GPa, whereas the average formation pressure of N1 and N2 ranges from 1.4 to 1.7 GPa with and without normalization of volatiles, overlapping with Arabia Terra. The calculated mantle potential temperature varies from 1310-1400 ᵒC for the studied Noachian regions. The degree of partial melt is ~8 % in Arabia Terra, ~12 % in N1, and ~11 % in N2. The melting depth is consistent in all three Noachian provinces, which is 130-150 km. Compared to the Hesperian and Amazonian magma formation conditions, the Noachian volcanic regions have relatively lower pressure and higher temperature of formation. This pioneering work of Noachian volcanics using an orbiter geochemical dataset suggests a cooling trend of the Martian mantle over time.


PS09-A007
Titan’s Surface Chemical Composition: What We Learned After 13 Years of Cassini Exploration

Anezina SOLOMONIDOU1#+, Alice LE GALL2, Athena COUSTENIS3,4, Paul HAYNE5
1Hellenic Space Center, Greece, 2Laboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS-UVSQ), France, 3Paris Observatory/ National Centre for Scientific Research, France, 4PSL Research University, France, 5University of Colorado Boulder, United States

The Cassini spacecraft spent 13 years in the Saturnian system and performed observations of Titan through 127 flybys, along with the in situ observations of the surface by Huygens. This led to the detailed investigation of Titan’s surface composition at both local and global scales. However, due to the complexity of Titan’s atmosphere and surface, the surface composition is only partially unveiled and is still considered to be one of Titan’s largest mysteries. Titan resembles Earth more than almost any other planetary body in the solar system, despite its frigid surface temperatures of -180 C (~93 K). Instead of silicate rocks, the crust is dominated by water ice. Sedimentary deposits in the form of hydrocarbon grains cover the top layer of the surface, while liquid hydrocarbons are found in the polar lakes. Titan’s active geology with its resurfacing processes creates topography where exposed materials from the underlying old crust along with new atmospheric sediments are present. After Cassini and Huygens with their several instruments investigated Titan for more than a decade one of the prevailing questions that still remains unanswered is whether and where water ice is exposed on the surface. Additionally, advanced knowledge with regards to the mixtures and the materials that create and cover the surface is yet to be gained from future missions and ground/space telescopes that would carry advanced technology. Here, we present an overview of what we have learned so far about the composition as well as its correlation and constraints with regards to Titan’s astrobiology.


PS11-A004
The Chirp Transform Spectrometer Flight Model on JUICE-SWI After NECP

Paul HARTOGH#+
Max Planck Institute for Solar System Research, Germany

The Chirp Transform Spectrometer (CTS) is the only heterodyne real-time spectrometer backend that was successfully flown on a deep space mission. A version with 180 MHz bandwidth and 4096 channels was operated in space without any problems between the Rosetta launch in 2004 and the end of the mission in 2016 as part of the MIRO (Microwave Instrument of the Rosetta Orbiter) instrument. A new version with 1 GHz bandwidth and 10000 spectral channels was developed for the JUICE-SWI instrument. It is based on the same basic principles, however is using a higher degree of digital technologies which results in higher flexibility (e.g. programmable input bandwidth, centre frequency, spectral resolution etc.), more than 6 times lower mass and about 4 times lower power consumption than the MIRO version. The FM and FS CTSs were completed mid 2020 and mid of 2022 respectively. This presentation focuses on the determined functional performance during the AIVT and NECP phases.


PS11-A007
Radiative Transfer (RT) and Inversion Codes for Characterizing Planetary Atmospheres: An Overview

Miriam RENGEL1#+, Jakob ADAMCZEWSKI1,2
1Max Planck Institute for Solar System Research, Germany, 2Georg-August-Universität Göttingen, Germany

The study of planetary atmospheres is crucial for understanding the origin, evolution, and processes that shape these celestial bodies. To interpret planetary spectra, it is necessary to have a detailed understanding of radiative transfer (RT) and its application through computational codes. With the advancements in observations, atmospheric modeling, and inference techniques, there has been a proliferation of RT and retrieval codes in planetary science. However, selecting the most suitable code for a given problem can be challenging. To address this, we provide a comprehensive mini-overview of the different RT and retrieval codes currently developed or available in the field of planetary atmospheres. This study serves as a valuable resource for the planetary science community by providing a clear and accessible list of codes, and it offers a useful reference for researchers and practitioners in selecting and applying RT and retrieval codes for planetary atmospheric studies.


PS11-A016
Microwave Spectrometry as a Tool to Target Io's Volcanic Plumes for Sample Collection

Neal TURNER1#+, William SMYTHE1, John PEARSON1, Paul HARTOGH2, Ryan OGLIORE3
1Jet Propulsion Laboratory, California Institute of Technology, United States, 2Max Planck Institute for Solar System Research, Germany, 3Washington University in St. Louis, United States

We model the microwave spectrum emitted from the plume of a major volcano on Jupiter's innermost Galilean moon, Io. The model covers hundreds of emission lines of the main gas component SO2, as well as lines of the lesser species SO, S, O, and NaCl. The thermal continuum emission from the pyroclastic silicate particles ejected with the gas is also included. We synthetically observe the resulting spectra using the parameters of the Submillimeter-Wave Instrument developed for the JUICE mission, and show that this instrument has sufficient sensitivity, speed, and angular and spectral resolution to map the plume's particle-rich central core during approach on a Jupiter-centered orbit suitable for collecting a sample from the plume.


PS13-A005
Numerical Simulation on the Evolution Process of Lunar Craters and Its Implication to the Dating of Lunar Craters

Junce ZHANG+, Caibo HU1,1#
University of Chinese Academy of Sciences, China

The dating of lunar craters is an important scientific issue for exploring the evolution process of the moon. Dating work in the Earth sciences often relies on Isotopic dating of rock samples, but it is relatively difficult to obtain moon rock samples. Therefore, the current mainstream method of dating lunar craters mainly relies on the analysis of statistics of crater or boulder. For lunar craters, predecessors gave a classification basis based on the geometric characteristics of craters. In other words, there are some key geometric parameters corresponding to the type of craters on the lunar surface. Since there is no wind and water erosion on the lunar surface and the tectonic activity is weak, the landform evolution process of the craters on the lunar surface can be simulated by the linear diffusion equation. Taking simple craters on the lunar surface as an example, if we can find key geometric markers that are easy to measure directly and discover their quantitative relationship with time, we can find a new method for crater dating based on physical processes. In this study, the lunar surface diffusion equation is used to simulate the evolution of the lunar craters, and two dimensionless key geometric indicators of craters are selected for analysis. The quantitative relationship between the key geometric indicators and the age of craters is given. Finally, we propose a new method for preliminary quantitative dating of simple lunar craters based on physical processes and dimensionless parameters of lunar surface geometry.


PS13-A006
New Insights Into Subsurface Composition Variations of Mars South Polar Caps from Weak-reflection Zones in SHARAD Data

Peng FANG1+, Jinhai ZHANG2#
1Chinese Academy of Sciences, China, 2Institute of Geology and Geophysics, Chinese Academy of Sciences, China

The polar layered deposits (PLDs) of Mars preserve its Amazonian climate history which correlates to the orbital forcing. Characterization of stratigraphy and composition of the PLDs is critical for understanding the evolution of martian geology and climate. Radar sounding is a powerful tool for studying stratigraphy and composition the PLDs. Bright reflections represent the variations in the dielectric properties of subsurface materials, and these signals are widely used to inverse the structure and compositions of PLDs. However, geologic units or structures can also hide in weak reflection areas. Some of them have been proven to be CO2 ice, which is critical for understanding the paleoclimate of Mars. Some weak-reflection areas could also be artifacts caused by inferred interference or large topography variations. Few studies have focused on the differentiation of the artifacts and geological meaning signals. Here, using data from shallow Radar (SHARAD) onboard Mars Reconnaissance Orbiter, we propose a new method for distinguishing the weak-reflection signals in SHARAD radargram from data-processing artifacts. SHARAD original data processing consists of range compression and azimuth processing (i.e., synthetic aperture processing). The range compression produces the unfocused radargram that have enhanced resolution in the range direction and the azimuth processing generates focused radargram that has enhanced resolution both in along-track directions. Our method investigates the difference in waveform characteristics between unfocused and focused radargrams and then automatically detects the location of artifacts. We applied the method to SHARAD data across the south PLD and detected a series of shadow zones from abundant adjacent radargrams clustered in a small region near the south pole (86°~87°S). This quasi-linear array of connected shadow zones along a 50-kilometer-long meandering path is unique, and it may help to inform a paleogeology setting different from that of current Mars.


PS13-A014
Effect of Ice Depth and Abundance on the Evolution of Water Production Rate: Case Study of 67P/Churyumov-Gerasimenko

Xian SHI1#+, Xuanyu HU2, Yuri SKOROV3
1Shanghai Astronomical Observatory, China, 2Technische Universität Berlin, Germany, 3Max Planck Institute for Solar System Research, Germany

Water production rate is an important indicator of a comet’s physical nature. It sheds light on the composition and structure of the cometary nucleus, as well as the mechanism of its activity. As a comet approaches the Sun, its water production rate generally increases due to the intensification of insolation. However, the actual trend could vary between individual comets and between different orbits of the same comet. It is not entirely clear how this relation is dependent on various properties of the cometary nucleus. Measurements by ESA’s Rosetta spacecraft have provided a unique dataset for probing this problem. During its over two years’ rendezvous with the Jupiter Family Comet 67P/Churyumov-Gerasimenko, the water production was retrieved with high temporal resolution by multiple payloads on board. The resulting curve deviates from the commonly intuited inverse square law dependence on the heliocentric distance. In this study, we implement different thermo-physical models to simulate the evolution of water production rate of 67P. We demonstrate that the slope of the water production can be significantly influenced by the abundance and depth of the ice in the subsurface of the nucleus. Because both parameters can vary over time and across the nucleus, the global production of water vapour is unlikely a useful indicator for inferring the ice distribution of the comet. Moreover, the incorporation of diurnal water ice cycle in the model could notably alter the steepness of the water production curve, hence further complicates the scenario.


PS13-A015
A Complex Paleo-surface Revealed by the Yutu-2 Rover at the Lunar Farside

Jialong LAI1+, Yi XU2#, Ling ZHANG3
1Jiangxi University of Science and Technology, China, 2Macau University of Science and Technology, Macau, 3Sun Yat-sen University, China

The observable lunar surface is represented by a ubiquitous layer of fine-grained materials produced by billions of years of hypervelocity pounding of its crustal layer. These events are randomly distributed both in size and frequency, but the rate is thought to have declined significantly since the early formation stages of the Solar System. The data from the Radar (LPR) onboard Chang’e-4 (CE-4) rover (Yutu-2), which is exploring the Von Kármán Crater on the lunar farside, are helping to peel back the upper layer of finely comminuted materials, interpreted as a thick layer of ejecta from the neighboring Finsen crater, to reveal a complex paleo-surface morphology.
The LPR on the Yutu-2 rover of CE-4 mission has been surveying the lunar farside since the beginning of 2019. In this paper, we report the first 25 days of LPR data revealing a complex ancient lunar surface (paleo-surface), the elevation profile of which has been substantially modified after about 3.1 billion years of formation. During its 560 m journey, at a depth varying between 7 and 20 m, distinct variations in the returned signal characteristics reveal a possible 270 m ± 10 m buried crater with an estimated age of less than 100 m.y. A smooth surface depression might not be the remnant of a degraded crater but a related surface expression of the hidden structure. The geomorphology, the subsurface structure affected by the shock wave, the impact melt deposits, and the derived exposed time of the crater, are analyzed in the paper.


PS14-A008
Thermal Structure of the Upper Atmosphere in the Venusian Polar Region Simulated by a GCM with the Akatsuki Horizontal Wind Assimilation

Hiroki ANDO1#+, Yukiko FUJISAWA2, Norihiko SUGIMOTO2, Masahiro TAKAGI1, Yoshihisa MATSUDA3
1Kyoto Sangyo University, Japan, 2Keio University, Japan, 3Tokyo Gakugei University, Japan

The thermal structure of the upper atmosphere in the Venusian polar region is reproduced by the assimilation of horizontal winds in low- and mid-latitudes derived from the Akatsuki ultra-violet images. The obtained structure is well consistent with infrared and radio occultation measurements. In particular, the unique thermal structure in the Venusian polar vortex such as cold collar and warm polar region in our model is realistic: the level where the cold collar is located and the temperature difference between cold collar and warm polar region are consistent with the measurements. The reasons why the thermal structure of the upper atmosphere in the polar region is realistic are that the zonal wind distribution around the cloud top level and the structure of the residual mean meridional circulation induced by the thermal tides are improved. Our results also suggest that the thermal structure in the Venusian upper polar region is closely related to the atmospheric dynamics.


PS14-A012
Aerosol Properties in the Enormous Cloud Cover of Venus as Inferred from Improved IR2 Night-side Data

Takehiko SATOH1#+, Takao SATO2, Takeshi HORINOUCHI3, Takeshi IMAMURA4, George HASHIMOTO5
1Japan Aerospace Exploration Agency, Japan, 2Hokkaido Information University, Japan, 3Hokkaido University, Japan, 4The University of Tokyo, Japan, 5Okayama University, Japan

A very abrupt change of cloud opacity seen in the night-side disk of Venus, which we call Enormous Cloud Cover (ECC), was imaged by Akatsuki/IR2 and Venus Express/VIRTIS-M (Peralta et al., 2020). Similar phenomena were repeatedly recorded by the ground-based instruments since the beginning of the night-side observations (Allen and Crawford, 1984), suggesting this phenomenon is common in the Venus atmosphere and may include essential dynamical implication. We reported last year the analysis of six sets of Akatsuki/IR2 observations (cleaned with the RSS method of Satoh et al., 2021) as well as seven of VEx/VIRTIS observations (tabulated in Peralta et al., 2020). Darkening of normal region (just west of ECC, named Background Cloud or BC) to ECC in the two passbands (1.735 um and 2.26 um) was measured to characterize how aerosol size and number density changes from BC to ECC. To improve the photometric accuracy, needed especially for the extremely-low radiance region (ECC in 2.26-um), an alternative method to clean the IR2 1.735- and 2.26-um data has been developed. The new method uses an over-exposed (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, therefore one of six IR2 data, 27 March 2016, is excluded from this new analysis. Once the IR2 images are cleaned, the radiance measurements in BC and ECC regions and characterization in the M3L coordinates (Satoh et al., 2021) are done just the same as before. We will discuss the improvement of the photometric accuracy, compare the obtained characteristics of the ECC for different observing times. Implication to the possible mechanism of this large-scale phenomenon will also be discussed.


PS16-A004
Tracing Seismic Phases Across the Moon

Ceri NUNN1#+, Benjamin FERNANDO2, Sharon KEDAR1, Mark PANNING1
1Jet Propulsion Laboratory, California Institute of Technology, United States, 2University of Oxford, United Kingdom

The Farside Seismic Suite is a planned seismic mission, which will land in Schrödinger Basin on the farside of the Moon. The mission, due to launch in 2025, is part of NASA’s Commercial Lunar Payload Services (CLPS) and will be the first seismic mission to the farside. From seismic experiments carried out during the Apollo missions, we know that the Moon is generates moonquakes and is frequently hit by meteoroids. In preparation for the FSS, we use AxiSEM3D, a full-waveform seismic propagation tool, to further explore how seismic waves propagate on the Moon. We compare our simulations to the impacts of the Apollo Saturn IV boosters and used Lunar Ascent Modules, which were deliberately crashed into the Moon. We simulate the artificial impacts because the locations, velocities, mass and trajectories of the impactors are known. Our analysis of the artificial impacts shows that seismic phases which have previously been labeled as shear arrivals are mislabeled (since there is no change to the polarization of the wave or the frequency of the arrivals). Instead, the observed increase in amplitude is likely to be somewhat random and may indicate energy arriving from an internal boundary. This absence of distinct shear arrivals is consistent with our simulations. In our simulations, which are modeled as pure explosions, no shear wave travels from the source. Secondly, our simulations show that direct arrivals are often too small to be observed, but later arrivals may be observed. This makes it difficult to label seismic phases observed in moonquakes, since later phases can be mislabeled as direct arrivals. By better understanding the propagation of seismic phases across the whole Moon, we will be in a better position to understand seismic data from future seismic missions, and explore the interior structure of the farside of the Moon.


PS16-A006
Dichotomy in Crustal Melting on Early Mars Inferred from Antipodal Effect

Lei ZHANG1#+, Jinhai ZHANG2, Ross MITCHELL1
1Chinese Academy of Sciences, China, 2Institute of Geology and Geophysics, Chinese Academy of Sciences, China

The Martian crustal dichotomy (MCD) between the southern highlands and the northern lowlands is the planet’s most ancient crustal structure, but its origins and evolution remain enigmatic. Understanding of the MCD comes largely from present-day and shallow crustal constraints. Lacking ancient and deeper constraints, hypotheses for the origin of the MCD range from an early giant impact, partial melting from sustained mantle convection, or some combination. The antipodal effect is when a large impact has body and surface seismic waves that travel through and around the globe to meet at the planet’s antipode where the focused seismic energy induces crustal uplift and fracturing and subsequent volcanism. The antipodal effect has been investigated on the Moon, Mercury, and even Earth, but the antipodal pair of the Hellas Basin and the Alba Patera volcano of Mars has always been regarded as the exemplar among the terrestrial planets and moons. Here we investigate with seismological modeling the antipodal effect of Hellas-Alba. The volcano is latitudinally offset ~2°(~119 km) from the expected antipode, and we explore whether the MCD can explain this deflection. Variations across the MCD in topography, thickness, and composition have only minor effects. Simulations capable of sufficiently decelerating southern surface waves require the presence of 2%–5% more partial melt in the southern highlands. As the age of impact ca. 4 billion years ago post-dates the formation of the MCD, our partial melting results thus imply that, with or without an early giant impact, the MCD was modified by mantle convection to supply enough heat for crustal melts for several hundreds of millions of years after Mars formation.


PS16-A009
Focal Mechanism Inversion of the Largest Marsquake, S1222a

Huixing BI+, Daoyuan SUN, Mingwei DAI#
University of Science and Technology of China, China

S1222a, with a magnitude of Mw 4.7, is the largest marsquake detected by the InSight seismometer on Mars. Different from the previously recorded marsquakes and the meteorite impacts, this event is the first observed tectonic marsquake that has both clear body and surface waves. Furthermore, it originates away from the seismic active region, Cerberus Fossae graben. Thus, its seismogenic mechanism remains vague. Here, we use the Cut-And-Paste (CAP) method to invert the focal mechanism by fitting the direct P, S, and subsequent body waveforms filtered between 0.08 and 0.32 Hz. In the CAP method, different phases can be shifted separately to minimize the effects of the uncertainties of the velocity models. By including the later arrivals, such as depth phases and surface-reflected waves of PP, better constraints on the fault mechanism and the focal depth are achieved. Although S1222a has the waveform features of both high-frequency (HF) and low-frequency (LF) family events, our inversion prefers a deeper source depth, as suggested in the previous LF marsquake studies. Our inversion result shows that S1222a is a normal faulting event with a slight strike-slip component, suggesting an extensive seismotectonic regime around Apollinaris Mons or the dichotomy southeast to Elysium Planitia. We also apply this method to other LF events originated at Cerberus Fossae and obtain similar normal fault results as Brinkman et al. (2021). The extensional tectonic setting of S1222a, along with the normal faults at Cerberus Fossae may be indicative of possible volcanic activities within the deep crust or mantle of Mars.


PS17-A001
Research on the Activity of Comets 60P/Tsuchinshan 2 and 62P/Tsuchinshan 1

Jianchun SHI1#+, Yuehua MA2
1Shanghai Astronomical Observatory, Chinese Academy of Sciences, China, 2Chinese Academy of Sciences, China

Comets 60P/Tsuchinshan 2 and 62P/Tsuchinshan 1 belong to JFCs. The activity of comets 60P/Tsuchinshan 2 and 62P/Tsuchinshan 1 is analysed by creating their Secular light curves (SLCs). We obtained the main activity parameters, the results show that both comets could be classified as middle-age comets in early apparitions, and their activity lasting for more than 300 d. The orbital changes (decrease of perihelion distance) of comets 60P/Tsuchinshan 2 and 62P/Tsuchinshan 1 in recent apparitions enhanced their activity. To study the physical properties and activity characteristic of 60P/Tsuchinshan during its 2018-2019 apparition, we observed 60P/Tsuchinshan with broadband B, V and R filters from November 2018 to March 2019 by using the 80 cm Yaoan High Precision Telescope at Yaoan Station of Purple Mountain Observatory, Chinese Academy of Sciences. Morphological analysis and photometric studies of 60P/Tsuchinshan were performed. The color indices, Af ρ values and dust production rates of 60P/Tsuchinshan were obtained. Compared to other Jupiter-family comets at similar heliocentric distances, we found that 60P/Tsuchinshan was a very active comet.


PS17-A005
A Note on the Yarkovsky Effect Detection with Ground-based Observations for Earth Quasi-satellites

Shoucun HU#+
Purple Mountain Observatory, Chinese Academy of Sciences, China

Earth quasi-satellites are objects in a specific type of co-orbital configuration (1:1 orbital resonance) with the Earth where the objects stay near the planet over many years. Due to the multiple-oppositions, they may be observed by ground-based facilities every year, making their observations more abundant then other general asteroids. We numerically find that their orbital drift under the influence of the Yarkovsky effect can be constrained due to the Earth quasi-satellite resonance, which may hinder the detection of the Yarkovsky effect from orbital fit using ground-based observations. We will quantitatively demonstrate this feature by performing a batch of orbit determination for several quasi-satellites and the corresponding detection SNRs are compared to those non-quasi-satellites that in the 1:1 orbital resonance with Earth.


PS17-A007
Regolith Properties of Large Main Belt Asteroid (704) Interamnia

Jiang HAOXUAN1#+, Jianghui JI2, Liang Liang YU3, Bin YANG4, Shoucun HU2, Yuhui ZHAO1
1Chinese Academy of Sciences, China, 2Purple Mountain Observatory, Chinese Academy of Sciences, China, 3Macau University of Science and Technology, China, 4European Southern Observatory, Chile

(704) Interamnia is one of the largest asteroids that locates in the outer main-belt region, which may contain a large amount of water ice underneath its surface. We observe this asteroid using 8.2 m Subaru telescope at mid-infrared wavebands, and utilize thermophysical model for realistic surface layers (RSTPM) to analyze mid-infrared data from Subaru along with those of IRAS, AKARI and WISE/NEOWISE. We optimize the method to convert the WISE magnitude to thermal infrared flux with temperature dependent color corrections, which can provide significant references for main-belt asteroids at a large heliocentric distance with low surface temperature. We derive best-fitting thermal parameters of Interamnia - a mean regolith grain size of 190-180+460 μm, with a roughness of 0.30-0.17+0.35 and RMS slope of 27−9+13 degrees, thereby producing thermal inertia ranging from 9 to 92 Jm−2s−1/2K−1 due to seasonal temperature variation. The geometric albedo and effective diameter are evaluated to be 0.0472 −0.0031+0.0033 and 339−11+12 km, respectively, being indicative of a bulk density of 1.86 ± 0.63 g/cm3. The low thermal inertia is consistent with typical B/C-type asteroids with D ≥ 100 km. The tiny regolith grain size suggests the presence of a fine regolith on the surface of Interamnia. Moreover, the seasonal and diurnal temperature distribution indicates that thermal features between southern and northern hemisphere appear to be very different. Finally, we present an estimation of volume fraction of water ice of 9% ∼ 66% from the published grain density and porosity of carbonaceous chondrites.


PS17-A010
Scenario-based Platform for Simulation and Inversion of Asteroid Light-curves

Kaiyu LEI1+, Xian SHI2, Fenzhi WU1, Xiao LIANG1, Yuehan AN1, Yanpeng WU1#, Wei ZHAO3, Peng LIU3, Yong YU2
1Beijing Institute of Spacecraft System Engineering, China, 2Shanghai Astronomical Observatory, China, 3Harbin Institute of Technology, China

An asteroid’s light-curve is the sequence of its apparent brightness over time. So far, most light-curve data is acquired with telescopic observations, while there is an increasing amount of data from spacecraft missions to asteroids. To fulfill the needs for the investigation of various types of light-curve data, we constructed a light-curve simulation and inversion platform based on realistic observing scenarios. By using modules and standard interfaces between them, the system covers the simulation, data reduction, and inversion of asteroid light-curves. We show with test cases, that this platform can be readily applied to further research on the asteroid light-curve inversion algorithm as well as the planning and operation of asteroid exploration missions. The platform is mainly composed of input data standardization, simulation, and inversion modules. Formatted files are used as interfaces between modules, making the system applicable to any target object and observation mode. The input data standardization module converts the shape and physical parameters of the target object, observation epochs, and observational geometries into standardized inputs for the other modules. In the simulation module, the standardized input data is rendered to obtain synthetic observations, which could be used for calculating the target’s apparent brightness and simulated light curves. The inversion module can use either the simulated light curves or observed light curve data for the inversion of physical parameters of the target, including its rotational properties and shape. To verify the feasibility and efficiency of the platform, we conducted a series of experiments with both ground-based and in-orbit asteroid light-curve observations. Results show that the simulated light-curves agree with observations. The inversion results obtained by using simulated light-curves are consistent with those obtained using actual observations. We expect to use this system for further studies of the light-curve inversion algorithm, and the planning and operation of future asteroid missions.


PS17-A030
Optical Landmark Searching and False-matches Elimination for Asteroid Pinpoint Landing

Yaqiong WANG#+, Huan XIE
Tongji University, China

Pinpoint landing on asteroids presents fundamental challenges for mission design and execution. Terrain relative navigation (TRN) is an efficient technology for precise landing for planetary exploration missions. Natural Feature Tracking (NFT) is a mapped landmarks-based optimal navigation method, which offer benefits in adaptive to feature appearance changes and present advantages when the spacecraft state is correctly estimate. As the spacecraft location and illumination conditions are not always precisely available to produce an optimally accurate map for feature matching and pose estimation, a robust landmark searching and false-matches elimination method is necessary. The proposed method is also based on the feature correlation between the 3D photometric data- based mapped landmark feature and the navigation image. Specially, we proposed a discriminative correlation filter (DCF) based landmark detection and matching method and a novel affine covariant feature false-matches elimination formulation. Firstly, based on specific image texture feature representations and circular matrix strategy, multi-channel DCF was employed to rapidly detect and match the landmarks features within current navigation camera image. Secondly, geometric topological relationships between the detected features were exploited to eliminate false matches. The false-matching features elimination was conducted by matching two sets of triplets under a global transformation model. A novel triples’ correspondence was proposed to describe the feature location correspondence, which improves the performance by exploiting local geometric structure of the feature. Furthermore, a novel latent variable model combining the feature frame and descriptor distinctness was employed, which significantly improves the convergence speed and matching performance in high-outlier-ratio cases. Images captured by the Touch and Go Camera System (TAGCAMS) of the Bennu asteroid were used to evaluate the performance of the proposed method. Qualitative and quantitative results illustrate the advancement of the proposed method in adapting to feature distortion and robustness to outliers.


PS17-A033
Thermal Properties of Small-sized Near-earth Asteroids from WISE/NEOWISE Observations

He HAOQING1, Jianghui JI2, Jiang HAOXUAN1#+
1Chinese Academy of Sciences, China, 2Purple Mountain Observatory, Chinese Academy of Sciences, China

The number of near-Earth asteroids that have been discovered exceeds 31000 to date, among which the number of small-sized near-Earth objects with a diameter of less than 100 meters exceeds 18000. Besides, due to observational selection effects, the actual number of small-sized asteroids is higher than observed. These asteroids will pose a serious threat to the security of the Earth. However, because the lack of observational data, only a few asteroids' physical properties have been obtained. This work will improve the NEATM model by considering the influence of reflected light from the sun, and combine the observation data of WISE/NEOWISE to obtain the albedo, diameter and other thermophysical parameters of small-sized near-Earth asteroids around the earth, which can provide useful information to the near-Earth object defense missions.


PS17-A035
Orbit Determination and Gravity Field Recovery Around Asteroids Using Inter-satellite Range Data

Haohan LI1#+, Xiyun HOU1, Haowen CHENG2
1Nanjing University, China, 2National Astronomical Observatories, China

High precision orbit determination and gravity recovery have been an important part of asteroid exploration. High quality measurement data can improve the accuracy. Inter-satellite range link is a type of high quality relative measurement and has been widely used in orbit determination of Earth satellites, but not so widely used in missions around small bodies. In our study, we assume that high accuracy inter-satellite range data can be obtained around small bodies, between the chief spacecraft and some low-cost deputies, and study the orbit determination along with the recovery of important parameters such as the gravity coefficients of the asteroid and the coefficient of solar radiation pressure. By comparing the results of with or without the inter-satellite range data, we show that the accuracy can be improved.


PS17-A036
Stability of Asteroidal Ring Systems Under Close Encounters with Small Objects

Ren IKEYA#+, Naoyuki HIRATA, Keiji OHTSUKI
Kobe University, Japan

Recent stellar occultations revealed that not only giant planets but small objects can also possess ring systems. To date, rings are found around Centaurs (10199) Chariklo, a dwarf planet (136108) Haumea, and (50000) Quaoar. These discoveries imply that asteroidal ring systems may be common, particularly in the outer solar system. Ring systems are susceptible to various dynamical mechanisms that disrupt ring systems in a relatively short timescale. One of those disrupting mechanisms is close encounters with a perturbing object (perturber), since close encounters are a ubiquitous and fundamental evolutionary process in the solar system. We carried out a series of numerical calculations to investigate the stability of ring systems during close encounters with small objects. We found that even if the encounter takes place at the immediate vicinity of the ring, a perturber with mass ratio of ≥ 10-3 is required to cause a noticeable damage (the maximum change in eccentricity ~ 0.01). Unless the perturber is similar or greater in size than the ringed objects, a substantial disruption (the maximum change in eccentricity ≫ 0.01) would not occur. The change in eccentricity shows a good match with the analytical expression called “Exponential regime” given by Heggie & Rasio (1996) because the secular effect is not at work for encounters that bring devastating consequences on the ring system. The change in eccentricity is also in good accordance with the analytical expression derived from the impulse approximation (ZT04Imp) given by Zakamska & Tremaine (2004) although the conditions of the impulse approximation are not fully satisfied. We investigated the probability for severe close encounters by making use of the collision probability, and conclude that for both of Haumea and Chariklo such encounters are highly unlikely to take place even over the age of the solar system.


PS18-A002
Constraining the Warming Effect of High-altitude Water Ice Clouds on Early Mars in a 3D Moist General Circulation Model with a Simplified Cloud Microphysical Scheme

Feng DING1#+, Kaitlyn LOFTUS2, Robin WORDSWORTH2
1Peking University, China, 2Harvard University, United States

Geologic evidence suggests >102-yr-long lake-forming climates persisted on Mars 3-4 Ga. These early warm climates cannot be explained by the greenhouse effect of CO2 and water vapor alone. Recently, a warming mechanism for early Mars based on high-altitude water ice clouds was proposed, for situations where the surface water inventory is limited and far away from tropical regions. However, microphysical representations of clouds and precipitation remain one of the main uncertain factors for climate modeling of terrestrial planets, including present-day Earth. Here we use a three-dimensional moist general circulation model (3D moist GCM) with a simplified cloud microphysical scheme to constrain the potential warming effect of high-altitude water ice clouds in a physical parameter space. In our GCM, the cloud sink term is characterized by a constant timescale that can be interpreted as the conversion timescale from clouds to precipitation. Two distinct climate regimes emerge as the conversion timescale of cloud particles is varied in the GCM simulations, separated by the time scale of ~10 days when the global climate dramatically jumps from a cold state to a warm state. We show that this dramatic climate transition results from a strong positive feedback loop among surface evaporation, cloud mass, and the atmospheric greenhouse effect, and develop a toy model with such positive feedback to reproduce the GCM simulations. The behavior of dramatic climate transition is robust as we vary the surface ice distribution, surface CO2 pressure, and the obliquity of the planet in the GCM simulations. Our findings suggest that theoretical or experimental studies on cloud microphysics (e.g., cloud radii, conversion timescales) in ancient Mars' atmospheric conditions are crucial for quantifying the warming effect of high-level water ice clouds.


PS20-A007
NASA Moon Trek's Lunar Mission Planning Tools

Emily LAW1#+, Brian DAY2
1NASA Jet Propulsion Laboratory, United States, 2National Aeronautics and Space Administration, United States

NASA’s Moon Trek (https://trek.nasa.gov/moon/) is one of a growing number of interactive, browser-based, online portals for planetary data visualization and analysis produced by NASA’s Solar System Treks Project (SSTP). Moon Trek continues to be enhanced with new data and new capabilities enabling it to facilitate the planning and conducting of upcoming lunar missions by NASA, its commercial partners, and its international partners, as well as scientific research. Moon Trek’s innovation visualization and analysis tools are already being used by a growing number of missions and scientists around the world. The tools deployed including interactive 2D and 3D visualization, a DEM and Ortho Mosaic Image production pipeline as well as tools for distance measurement, elevation profile generation, solar altitude and azimuth calculation, 3D print file generation, virtual reality visualization generation, annotation, lighting analysis, electrostatic surface potential analysis, slope analysis, rock detection, crater detection, rockfall detection, profiling of raster data, line of sight calculation. This presentation will highlight Moon Trek’s tools for Lunar mission planning and demonstrate their use cases.


PS20-A015
A Low-cost Lander and Rover Investigation of the Reiner Gamma Lunar Magnetic Anomaly and Swirl: Lunar Vertex

David BLEWETT1#+, Jasper HALEKAS2, George HO3, Benjamin GREENHAGEN1, Brian ANDERSON1, Joshua CAHILL1, Edward CLOUTIS4, Brett DENEVI1, Shahab FATEMI5, Lon HOOD6, Jorg-Micha JAHN3, Rachel KLIMA1, Peter KOLLMANN1, Myriam LEMELIN7, Heather MEYER1, Leonardo REGOLI1, Sonia TIKOO8, Sarah VINES1, Dany WALLER1, Mark WIECZOREK9, Xiao-Duan ZOU10
1Johns Hopkins University Applied Physics Laboratory, United States, 2The University of Iowa, United States, 3Southwest Research Institute, United States, 4The University of Winnipeg, Canada, 5Umeå University, Sweden, 6The University of Arizona, United States, 7Université de Sherbrooke, Canada, 8Stanford University, United States, 9Institut de Physique du Globe de Paris, France, 10Planetary Science Institute, United States

Lunar Vertex is a mission at the intersection of planetary geoscience and space plasma physics. The first of NASA's Payloads and Research Investigations on the Surface of the Moon (PRISM) investigations, scheduled for delivery to the Reiner Gamma (RG) magnetic anomaly in 2024 aboard a commercial lunar lander, Lunar Vertex will unravel the nature of the RG anomaly, examine the enigmatic high-reflectance RG lunar swirl surface feature, and probe plasma interactions and the RG "mini-magnetosphere". Lunar Vertex includes three instruments on the lander: a suite of magnetometers (Vector Magnetometer – Lander, VML), a fixed-mounted set of cameras (Vertex Camera Array, VCA), and a low-energy ion and electron plasma analyzer (Magnetic Anomaly Plasma Spectrometer, MAPS). In addition, another suite of commercial fluxgate magnetometers (Vector Magnetometer – Rover, VMR) and a multispectral imager (Rover Multispectral Microscope; RMM) are carried on a small rover that will travel a distance of at least 500 m from the lander, providing additional multi-point measurements. The combination of magnetic field measurements taken during cruise and descent by VML and during surface operations by both VML and VMR will characterize the magnetic source and thus lend clues to its origin. The combined magnetic field and plasma measurements from VML and MAPS will provide direct observations of plasma populations reaching the lunar surface and the associated local magnetic field configuration. In addition, the regolith at locations along the rover's traverse within the RG swirl will be studied by RMM to reveal the surface texture, composition, and particle-size distribution, allowing hypotheses for swirl formation to be tested. VCA images will provide geologic context and yield data on the light-scattering properties of the surface. Correlations between magnetic-field data and soil properties determined by RMM and VCA will elucidate the role of solar-wind ion bombardment in the weathering of the surface.


PS20-A016
Lunar Mineralogical Prospecting Through Integrated Spectral Analysis

Rachel KLIMA#+, Angela DAPREMONT, Ellen LEASK
Johns Hopkins University Applied Physics Laboratory, United States

Danuri, Korea’s first mission to the Moon will provide valuable data for future lunar landed exploration. In support of that mission, we are working with existing data from Chandrayaan-1’s Moon Mineralogy Mapper (M3) and the Lunar Reconnaissance Orbiter Diviner Lunar Radiometer to provide mineral analyses to supplement Danuri’s measurements of elemental data through the Gamma Ray Spectrometer (KGRS) and imaging data collected by Lunar Terrain Imager. Our analysis focuses on characterizing the composition of minerals and potential resources at the sites targeted by Danuri. In advance of the return of science data from the mission, we have been working with existing Lunar Prospector Gamma Ray Spectrometer, M3, and Diviner data to develop our data processing pipeline, with the goal of being ready to combine derived mineralogical variability with the KGRS elemental data to create global low (1.5 km/pixel) and regional higher (250 m/pixel) resolution mineralogical, hydroxyl, and elemental maps. The data will be used for basic scientific analysis and to help assess the mineralogical composition and resource potential of candidate landing sites from orbit. Our specific scientific project is geared towards using these joint products to focus on investigation of orthopyroxene-dominated regions, exploring two specific questions: (1) What are the compositions of orthopyroxene-rich deposits exposed on the lunar surface and what is the range in their cooling rates? and (2) Is there a relationship between orthopyroxene modal abundance, composition, cooling rate, associated hydroxyl and specific types of terrain? Orthopyroxenes on the lunar surface could originate as cumulate layers of orthopyroxenite or norite in igneous intrusions, as crystallization of trapped melt entrained in the anorthosite floatation crust of the moon, or as orthopyroxenite in the lunar mantle.


PS20-A018
Advanced Lunar Imaging Spectrometer (ALIS) for Lunar Polar Exploration (LUPEX) Project

Kazuto SAIKI1#+, Yuusuke NAKAUCHI2, Noboru EBIZUKA3, Takayuki OKAMOTO3, Yoshiko OGAWA4, Masahiro KAYAMA5, Kohei KITAZATO4, Minoru SASAKI6, Hirohide DEMURA4, Hiroshi NAGAOKA3, Teruyuki HIRANO7, Takashi MIKOUCHI5, Yutaka YAMAGATA3, Yoshiaki ISHIHARA8, Ryusuke NISHITANI8, Hiroyasu MIZUNO8, Dai ASOH8
1Ritsumekan University, Japan, 2Ritsumeikan University, Japan, 3RIKEN, Japan, 4The University of Aizu, Japan, 5The University of Tokyo, Japan, 6Toyota Technological Institute, Japan, 7Astrobiology Center, Japan, 8Japan Aerospace Exploration Agency, Japan

Several studies that focus on searching for water ice resources in the lunar permanently shadowed regions (PSRs) reported positive results. However, the abundance, condensation mechanism, and lateral and vertical distribution of water at the PSRs remain unclear. To solve these problems, the Lunar Polar Exploration (LUPEX) project started by Indian Space Research Organization (ISRO) and Japan Aerospace Exploration Agency (JAXA) (Ohtake et al.,2021).We proposed a hyperspectral near-infrared camera named Advanced Lunar Imaging Spectrometer (ALIS) for LUPEX and it was selected as a candidate instrument for the rover in April 2020. ALIS can identify rock-forming minerals in the target area and confirm and quantify the existence of water ice. ALIS is composed of the following four blocks; ALIS-C (Camera): the main block, which contains the image sensor, spectroscopic optics, and electrical circuits, ALIS-M (Mirror): a movable mirror for shifting the field of view in elevation and azimuth directions, ALIS-L (Light): a light source that enables observation in PSRs, and ALIS-D (Diffuse reflector): a standard diffuse reflector to calibrate the spectral data of ALIS. There is an absorption band of water ice near 1500 nm, and we aim to use this absorption band to quantitatively detect trace ice with lower detection limit 0.5 wt% or better. We will also detect OH groups phases using the absorption band around 1400-1500nm and identify major rock-forming minerals using the absorption band around 1000nm. To improve the ice quantification accuracy of ALIS, we have developed a micro-ice production apparatus and are continuing the observation verification test by a BBM of ALIS. We estimate SNR value of the detector required to detect 0.5 wt% ice as to be ~220 for olivine and ~120 for plagioclase, respectively (Ogishima and Saiki, 2021). We have also started quantitative experiments using frosted highland regolith simulants.


PS20-A019
Testing and Characterisation of Front-end Electronics of Chaste Payload for Chandrayaan -3 Lander

Chandan KUMAR#+, Durga Prasad KARANAM, Sanjeev MISHRA, P. KALYAN REDDY, Janmejay KUMAR
Physical Research Laboratory, India

Chandra’s Surface Thermophysical Experiment (ChaSTE) aims to understand the thermophysical properties of the top 10 cm of the Lunar surface. The experiment has an electronics package, and a low thermal conductivity probe with Platinum RTD sensors mounted on it with a separation of 1cm. The Front-End electronics for the experiment has a constant low current excitation scheme with a low offset gain stage with a rail-to-rail amplifier. Each temperature sensor has an independent signal conditioning multiplexed onto a serial ADC for data handling and storage. The calibration and characterisation of the system (Sensor + Front End Electronics) were carried out using a custom-developed dry block calibration facility with an accuracy of better than 0.1K for the sensor and the integrated system. A Liquid Nitrogen bath was used to achieve an extremely lower temperature point. The calibration was done at three levels: sensor, probe and system. The electronics offset is first corrected at the sensor level by cross-referencing the sensor readings with a standard RTD Calibrator. After this, each RTD Sensor is calibrated over the entire range of temperatures. Since the sensors are mounted in the probe in this case, the effect of probe material, design and dimensions will also be accounted for. The same procedure is followed for instrument-level characterisation as well. We have also completed all the qualification tests per the project specification, and the package was cleared for flight. In addition, detail calibration and characterisation studies are also being carried out in an in-house developed Lunar simulation chamber. Using this setup, temperatures and thermophysical properties have been estimated for samples of various lunar analogous materials and compared with their known values for reference. Performance results, calibration and characterisation results will be discussed.


PS20-A021
Mineralogical and Morphological Investigation in and Around the Bowditch Crater of Lunar Farside: Insight to the Complex Volcanic Processes

Nabamita CHAUDHURI#+, Kusuma K.N., Aravind BHARATHVAJ
Pondicherry University, India

The mare units within the Bowditch crater (25.0° S, 103.1° E) and Lacus Solitudinis (27.8° S, 104.3° E) show an anomalous presence of basalts within the anorthosite-rich highlands of farside. We have analysed Moon Mineralogy Mapper (M3) to understand the nature of basalts available in this region. We have applied Integrated Band Depth (IBD) which targets the absorptions in visible near-infrared (VNIR) spectra diagnostic of lunar minerals. IBD colour composite was generated by assigning IBD1000, IBD2000 and IBD1250 to red, green and blue channels, respectively. The colour composite displays Bowditch and Lacus Solitudinis to be distinctly basaltic amidst the feldspathic highlands but in different hues and intensities, implying lithological variations. The Bowditch crater exhibits yellow colour, indicating the presence of pyroxene having absorptions at 1000 nm and 2000 nm. Comparatively, Lacus Solitudinis has a predominant presence of purple in the colour composite, generated due to the addition of red and blue, representing IBD1000 and IBD1250, indicating the presence of olivine along with pyroxene. The presence of various rilles and channels between the two units suggests that Lacus Solitudinis could be the source of basalts in Bowditch. A geomorphological study of the area using LROC-NAC data revealed the presence of many dark mantling deposits and fresh boulder patches along the rille shoulders, especially in the region near Bowditch. This indicates a relatively younger age of the region with a complex evolutionary history.


PS20-A029
Composition of Magma Composing Lunar Linear Gravity Anomalies: Implication to Magmatism During Ancient Lunar Expansion

Gaku NISHIYAMA1#+, Tomokatsu MOROTA1, Noriyuki NAMIKI2, Kazuki INOUE1, Seiji SUGITA1
1The University of Tokyo, Japan, 2National Astronomical Observatory of Japan, Japan

Several numerical simulations on the lunar interior evolution have proposed that the Moon has experienced an expansion stage in its history. After the lunar mantle overturn transported heat-producing elements, the radioactive heat warmed the lunar interior, causing a volumetric expansion. This phenomenon has been evidenced by linear gravity anomalies (LGAs) identified in high-resolution lunar gravity data acquired by NASA’s GRAIL mission. These long, narrow, and positive LGAs have been interpreted as ancient magmatic intrusions formed under extensional stress. Because the composition of magma reflects its origin and related processes, compositional analysis on LGAs may offer a new hint to decipher the ancient lunar thermomechanical state. In this study, we surveyed spectral and gravity datasets around 160-km-sized Rowland and Roche craters located on LGAs. Although LGAs have no prominent spectral feature right above them, LGAs weakened inside these craters suggest that ancient magma could have been excavated and distributed around them. Analyzing spectral absorptions with the Kaguya Multiband Imager (MI) and Chandrayaan-1Moon Mineralogy Mapper (M3) data, we first identified non-mare spots holding high-calcium pyroxene (HCP). Whether the discovered exposures originate from the LGA intrusion is next discussed in a comparison between data and impact simulation with iSALE hydrocode. Our spectral and gravity analysis indicates that Rowland crater did not excavate LGA material. No clear HCP exposures were found in its periphery, and the gravity drop inside Rowland did not lie within the range of our simulation. On the other hand, more than 30 HCP exposures were discovered around Roche. Together with gravity consistency between data and simulation, these exposures are likely to originate from the subsurface intrusion. Their low-Ti composition suggests that a mantle plume from overturned Ti-rich materials did not compositionally contribute to ancient LGAmagma but rather provided only heat to the LGA volcanism.


PS23-A005
Searching for Orbital Decay Candidates from Exoplanet Transit Databases

Li-Chin YEH#+, Ing-Guey JIANG
National Tsing Hua University, Taiwan

A huge number of mid-transit times from ExoClock and TESS projects are employed to investigate the possible non-linear transit timing variations of exoplanets by performing data-model fitting with both the fixed orbit and the orbital variation models. Several exoplanets in favor of orbital decay are found. Their tidally evolutionary orbits are also studied and presented.


PS23-A012
GTLS: A GPU Algorithm for Speeding up Periodic Transit Detection

Quanquan HU#+, Jian GE
Chinese Academy of Sciences, China

The Transit Least Squares (TLS) algorithm is a powerful tool for exoplanet transit searches in large datasets of photometric light curves. With its higher sensitivity and faster search speed than the traditional Box Least Squares (BLS) algorithm, TLS has become increasingly popular. However, it still takes a long time to run the TLS algorithm on the CPU to search for transit signals, which largely affects the search efficiency. An innovative GPU algorithm has been developed by us to speed up the TLS processing speed, allowing us to search more data for transit planet signals and improve search cadences for detecting weak transit signals or transit signals with shorter durations than those detected before. This GPU-based TLS algorithm is called GTLS, which has been tested and significantly improved the search speed using the TLS algorithm while still producing reliable results. This presentation reports this GTLS, its testing and early searching results from the TESS data.


PS23-A016
Forecasting Consecutive Transits of Circumbinary Planets in One Conjunction. Application to TOI-1338 b

Mutian WANG#+, Huigen LIU
Nanjing University, China

Current transiting circumbinary planets (CBPs) found by Kepler and TESS display significant transit time variations (TTVs) up to a few days. The dominant source of TTVs comes from the relative motion between the binary star and planet. In special cases, there will be multiple closely-spaced CBP transits over the same star present in one binary period, which we dub as ‘tight transits’. The frequency of tight transits significantly depends on the planet-to-stellar velocity ratio and the degree of co-planarity of the system. We derive analytical constraints to characterize the system architectures and binary and planetary phases when tight transits can occur. After refining the system parameters of TOI-1338 b using the newly-observed CBP transits during TESS Extended Mission, we found that the most recent tight transit of TOI-1338 b over the secondary star would be around February 23rd, and 27th 2024. Due to the large luminosity contrast between the primary and secondary star in the system, the apparent depth of the predicted tight transits will be around 200 ppm in the TESS band, but the visibility will be improved if redder photometry is employed. Finally, we develop an analytical approximation to explain the predicted timing and detectability’s dependence on the uncertainties of orbital parameters, which informs us how the detection of tight transits can yield a more precise three-dimensional architecture of TOI-1338 b system.


PS23-A025
Simultaneously Orbital Evolution and Gas Accretion of Giant Planets Embedded in the Protoplanetary Disk

Hui ZHANG1#+, David C. C. YEN2
1Shanghai Astronomical Observatory, China, 2Fu Jen Catholic University, China

Recent Transit and RV surveys have revealed that multiple-planet systems with more than one giant planet are common. And some giant planet pairs even show an orbit period ratio close to MMRs, which is an evidence of convergent orbital migration. How does the gas accretion process affect with the dynamical interaction between two gas-accreting planets? Will the convergent migration lead to a competition of gas? In this paper, we perform a series of hydrodynamic simulations that simultaneously model the orbital evolution and gas accretion of two giant planets embedded in the protoplanetary disk. Our results show that the convergent migration of two giant planets usually leads to a mass ratio (Mp_outer to Mp_inner) close to 1, which explains the similarity in mass of neighboring giant planets. And the final mass ratio significantly depends on the disk properties, e.g. density profile, viscosity, etc., and the orbital evolutions of the two interacting giants. This is also consistent to the large spread in the distribution (which is centered at 1) of the mass ratio of two adjacent giant planets.


PS23-A050
Prediction of the Free-floating Planet Event Rate for Microlensing Surveys

Qiyue QIAN1#+, Weicheng ZANG2, Hongjing YANG1, Shude MAO1
1Tsinghua University, China, 2Center for Astrophysics | Harvard & Smithsonian, United States

Free-floating planets (FFPs) are expected to be common in our Galaxy. The mass function and number density of the FFP population can provide constraints on planet formation theories. However, FFPs are difficult to detect because they are faint and unbound. Microlensing is currently the only method of detecting FFPs with wide mass and distance ranges. In this work, we will use simulations to predict the FFP event rate for future space microlensing surveys (e.g., ET, Roman). We will compare the expected detections and current observational results, discuss the potential reason for any gap between observations and our simulations, and outline optimizing strategies for future searches.


PS24-A001
North–south Plasma Asymmetry Across Mercury’s Near-tail Current Sheet

Jun ZHONG1#+, 良海 谢2, L. C. LEE3, James SLAVIN4, Jim RAINES4, Wing-Huen IP5, Yoshifumi SAITO6, Yong WEI1
1Institute of Geology and Geophysics, Chinese Academy of Sciences, China, 2National Space Science Center, Chinese Academy of Sciences, China, 3Academia Sinica, Taiwan, 4University of Michigan, United States, 5National Central University, Taiwan, 6Institute of Space and Astronautical Science / Japan Aerospace Exploration Agency, Japan

Among the nearly 300 near-Mercury tail current sheet crossings performed by the MESSENGER spacecraft, we identified 34 traversals of an asymmetric current sheet, wherein the lobe densities on opposite sides differed by a factor of three or more. These asymmetric current sheet crossings primarily occur on the dawnside. Additionally, a global magnetohydrodynamic (MHD) simulation was found to be in excellent agreement with the observations. The results suggest that the north–south density asymmetry is caused by the solar wind entering via an upstream-connected window in one hemisphere. Moreover, the Parker spiral interplanetary magnetic field (IMF) controls the near-tail density asymmetries, whereas Mercury’s offset dipole magnetic field controls those in the mid- or distant-tail regions. We propose that hemispheric asymmetries in Mercury’s magnetospheric convection occur under strong IMF conditions.


PS24-A002
MESSENGER Observations of Standing Whistler Waves Upstream of Bow Shock of Mercury

Yang WANG1#+, Jun ZHONG2
1INSTITUTE OF GEOLOGY AND GEOPHYSICS, CHINESE ACADEMY OF SCIENCES (IGGCAS), China, 2Institute of Geology and Geophysics, Chinese Academy of Sciences, China

This paper reports on the standing whistler waves upstream of Mercury’s quasi-perpendicular bow shock. Using MESSENGER's magnetometer data, 36 wave events were identified during interplanetary coronal mass ejections (ICMEs). These elliptic or circular polarized waves were characterized by: (1) a constant phase with respect to the shock, (2) propagation along the normal direction to the shock surface, and (3) rapid damping over a few wave periods. We inferred the speed of Mercury’s bow shock as ~31 km/s and a shock width of 1.76 ion inertial length. These events were observed in 20% of the MESSENGER orbits during ICMEs. We conclude that standing whistler wave generations at Mercury are generic to ICME impacts and the low Alfvén Mach number (MA) collisionless shock, and are not affected by the absolute dimensions of its bow shock. Our results further support the theory that these waves are generated by the current in the shock.


PS24-A009
Learning from MESSENGER – Lessons for Tides Derivation with BepiColombo’s Laser Altimeter

Oliver STENZEL#+, Martin HILCHENBACH, Lukas MAES
Max Planck Institute for Solar System Research, Germany

The joint ESA-JAXA mission BepiColombo to Mercury [1] is set to arrive in orbit in late 2025. After commissioning the actual measurement campaigns of the BepiColombo Laser Altimeter BELA [2] will start during spring 2026. BELA will map the planet in high detail over the whole mission and will create a dataset the will allow us to estimate the Love number h2 from the cyclic deformation of the surface [3]. Measuring the Hermian surface between 2011 and 2015, NASA MESSENGER’s Laser Altimeter (MLA) [4] provides a multi year dataset from northern hemisphere, mostly that can be used to test data processing and tides derivation models. We will present our ongoing efforts to filter and select laser altimeter data with classical robust filtering and machine learning approaches [5], [6].

[1] J. Benkhoff et al., ‘BepiColombo—Comprehensive exploration of Mercury: Mission overview and science goals’, Planet. Space Sci., vol. 58, no. 1, pp. 2–20, Jan. 2010, doi: 10.1016/j.pss.2009.09.020.
[2] N. Thomas et al., ‘The BepiColombo Laser Altimeter’, Space Sci. Rev., vol. 217, no. 1, p. 25, Feb. 2021, doi: 10.1007/s11214-021-00794-y.
[3] R. N. Thor et al., ‘Prospects for measuring Mercury’s tidal Love number h2 with the BepiColombo Laser Altimeter’, Astron. Astrophys., vol. 633, p. A85, Jan. 2020, doi: 10.1051/0004-6361/201936517.
[4] J. F. Cavanaugh et al., ‘The Mercury Laser Altimeter Instrument for the MESSENGER Mission’, Space Sci. Rev., vol. 131, no. 1, pp. 451–479, Aug. 2007, doi: 10.1007/s11214-007-9273-4.
[5] O. J. Stenzel, I. Hall, and M. Hilchenbach, ‘Mercury Tide Parameter Estimation from Laser Altimeter Records’, presented at the 53rd LPSC, Mar. 2022. [6] O. J. Stenzel, M. Hilchenbach, and I. Hall, ‘Influence of Surface Properties from Laser Altimeter Data on Mercury Tide calculations’, 44th COSPAR Scientific Assembly, Athens, Jul. 2022, vol. 44, p. 470. https://ui.adsabs.harvard.edu/abs/2022cosp...44..470S.


PS24-A012
BepiColombo - Images from 3 Mercury Flybys

Johannes BENKHOFF1#, Joe ZENDER1, Go MURAKAMI2+
1European Space Agency, Netherlands, 2Japan Aerospace Exploration Agency, Japan

BepiColombo is a joint project between the European Space Agency (ESA) and the Japanese Aerospace Exploration Agency (JAXA). The mission consists of two orbiters, the Mercury Planetary Orbiter (MPO) and the MercuryMagnetospheric Orbiter (MIO). Both spacecraft has been launched with an ARIANE V in October 2018 for an arrival at Mercury in late 2025. From dedicated orbits the two spacecraft will be studying the planet and its environment. On its route BepiColombo will perform flybys at Earth, Venus, and Mercury. Especially during these flybys but also during its cruise into the inner solar system some scientific and engineering operations have been scheduled. A short overview status of the mission and measurements taken by the three monitoring cameras during the first three Mercury flybys en route to Mercury will be given. 


PS24-A013
Detection of Species in Mercury's Exosphere with the Visible Channels of PHEBUS During BepiColombo Flybys

Rozenn ROBIDEL1#+, Eric QUEMERAIS1, Jean-Yves CHAUFRAY2, Dimitra KOUTROUMPA1, Francois LEBLANC3, Aurélie REBERAC1
1Laboratoire Atmosphères, Milieux, Observations Spatiales, France, 2University Pierre et Marie Curie, France, 3National Centre for Scientific Research, France

BepiColombo, the ESA/JAXA joint mission has performed its first flyby of Mercury on October 1, 2021 and its second on June 23, 2022. PHEBUS (Probing of Hermean Exosphere By UltraViolet Spectroscopy) was able to observe during these flybys notably with its visible channels. The channel c404 is centered on 404 nm (K emission line), and the other one, c422, is centered on 422 nm (Ca emission line). During both flybys, the slit was removed and the acquisitions were made every 10s with an exposure time of 8s. The count rate as a function of time of both channels clearly indicates the observation geometry of the flybys, the transit in the shadow of Mercury in particular, and the maximum of the emission on the dawn side, after the closest approach. We present for the first time Mercury’s extended exosphere of Ca beyond ~12,000 km. We report a nightside/dayside asymmetry and show evidence for two different energetic populations of Ca. The distribution could be consistent with a two-step process: the first one ejects Ca-bearing molecules and the second one produces highly energetic Ca atoms. It is more difficult to state which species were detected by the other channel, c404. Its bandwidth is large enough to detect the emission lines of K, Mn, Al and even Ca+. However, K has not been observed by MESSENGER at this wavelength [1] while Mn has been observed only at the end of the MESSENGER mission, in the pre-dawn nightside region and between TAA of 0° and 70° [1], which does not correspond to the TAA of BepiColombo flybys. Finally, we make preliminary comparisons with the third Mercury’s Swing-By (June 2023). Reference: [1] Vervack et al., 2016


PS24-A014
3D Hall-MHD and MHD-EPIC Simulations of Mercury’s Dayside Reconnection-driven Dynamics

Changkun LI, Xianzhe JIA#+
University of Michigan, United States

Mercury possesses a miniature but dynamic magnetosphere driven primarily by the solar wind through magnetic reconnection. A prominent feature of the dayside magnetopause reconnection that has been frequently observed is flux transfer events (FTEs), which are thought to be an important player in driving the global dynamics at Mercury. In our initial work, we have used the BATSRUS Hall MHD model to conduct a series of global simulations to investigate the generation and characteristics of FTEs under different solar wind Alfvénic Mach numbers (MA) and IMF orientations. An automated algorithm was developed to consistently identify FTEs and extract their key properties from the simulations. In all simulations driven by steady upstream conditions, FTEs are formed quasi-periodically with recurrence time ranging from 2 to 9 seconds and the FTEs characteristics evolve in time as they interact with the surrounding plasma and magnetic field. The key properties of the simulated FTEs, including spatial size, traveling speed and core field strength, all exhibit notable dependence on the solar wind MA and IMF orientation, and the trends identified from the simulations are consistent with previous MESSENGER observations. Following the Hall-MHD simulations, we have employed the MHD with Embedded PIC (MHD-EPIC) model to perform the same sets of simulations to investigate the importance of kinetic effects in driving Mercury’s magnetopause reconnection. Our initial results suggest that the general properties of FTEs formed in MHD-EPIC follow very similar trends as in Hall-MHD simulations. In the MHD-EPIC runs, features like particle precipitation and localized diamagnetic depression are commonly found in the cusps as a result of dayside reconnection, which resemble the cusp filaments that have been observed by MESSENGER. We will present comparisons between the Hall-MHD and MHD-EPIC simulations and discuss the impact of kinetic physics on the formation and characteristics of FTEs.


Fri-04 Aug | 8:15 - 10:00 | MR307
PS09 - Geology, Geophysics, and Habitability in Our Solar System

Session Chair(s): Rosaly LOPES-GAUTIER, Jet Propulsion Laboratory, California Institute of Technology, Anezina SOLOMONIDOU, Hellenic Space Center

PS09-A003 | Invited
Giant Planets Systems: Habitable Environments and Their Future Exploration

Athena COUSTENIS1,2#+
1Paris Observatory/ National Centre for Scientific Research, 2PSL Research University

Measurements by the space missions Voyager, Galileo and Cassini-Huygens, as well as observations from the ground, revealed habitable conditions in the solar system beyond the snow line focusing on the natural satellites of gas giants. Several of these show evidence of harboring organic chemistry in their atmospheres or exospheres, undersurface liquid water oceans, as well as energy sources. Europa, Callisto and Ganymede are hiding, under their icy crust, undersurface liquid water oceans which, in the case of Europa, may be in direct contact with a silicate mantle floor and kept warm by tidally generated heat [1,2]. These aspects will be investigated in the future by ESA’s JUICE (launch in April 2023-arrival in 2031 [3]) and NASA’s Europa Clipper mission with similar arrival times allowing for some synergistic investigations. Titan and Enceladus, were found by the Cassini-Huygens mission to possess active organic chemistry [4], unique geological features and internal liquid water oceans [2,5,6]. Titan will be further explored by NASA's Dragonfly mission [7]. If the silicate mantles of Europa and Ganymede and the liquid sources of Titan and Enceladus are geologically active as on Earth, giving rise to the equivalent of hydrothermal systems, the simultaneous presence of water, geodynamic interactions, chemical energy sources and a diversity of chemical elements may fulfill the conditions for habitability. References: [1] Coustenis, A., Encrenaz, Th., 2013. CUP. ISBN:9781107026179. [2] Hand, K.P., etal., 2020. Space Sci. Rev. 216, id.95. [3] Coustenis, A., etal., 2021. The Bridge on space exploration, 51, pp. 41-50. [4] Coustenis, A., 2021. In Read, Oxford Research Encyclopedia of Planetary Science. [5] Lunine, J., etal., 2018. In “Enceladus and the Icy Moons of Saturn”. LPI/UA/Space Science Series. [6] Nixon, C. A., et al., 2018. PSS, 155, 50-72. [7] Barnes, J. et al., The Plan. Sci. J., 4, 18.


PS09-A001
Europa Clipper Mission Update

Haje KORTH1#+, Robert PAPPALARDO2, Bonnie BURATTI2, Kate CRAFT1, Samuel HOWELL2, Rachel KLIMA1, Erin LEONARD2, Alexandra MATIELLA NOVAK1, Cynthia PHILLIPS2
1Johns Hopkins University Applied Physics Laboratory, 2Jet Propulsion Laboratory, California Institute of Technology

With a launch readiness date of late 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 more than 40 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 comprise 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 project, flight system, and payload have completed their Critical Design Reviews, and the project has completed its System Integration Review, so that Europa Clipper is now formally in mission Phase D. The spacecraft and payload are currently under construction, as assembly, testing, and launch operations (ATLO) are well underway. Recent major milestones include the delivery to ATLO of the Propulsion Module and six instruments and the assembly of the solar array wings. The remaining instruments are in mature stages of assembly and will be delivered in the next months. The science team is in the process of evaluating minor changes to the candidate tour, and is preparing a set of manuscripts describing the mission’s science and instruments.


PS09-A018
A Horizon 2061 Perspective on Future Missions and Key Technologies for Planetary Exploration

Jeremie LASUE1#, Bernard FOING2+, Michel BLANC3, Pierre BIOUSQUET4, Veronique DEHANT5, Manuel GRANDE6, guo LINLI7, Aurore HUTZLER8, Ralph MCNUTT9, Maria-Antonietta PERINO10, Heike RAUER11
1Institute for Research in Astrophysics and Planetology (CNRS-University of Toulouse-CNES), 2Leiden University, 3Institute for Research in Astrophysics and Planetology, 4National Centre for Space Studies, 5Royal Observatory of Belgium, 6University of Aberystwyth, 7China Academy of Space Technology/DFH Satellite Co., Ltd., 8European Space Agency, 9Johns Hopkins University Applied Physics Laboratory, 10Thales Alenia Space, 11German Aerospace Center

"Planetary Exploration, Horizon 2061" is a long-term foresight exercise initially proposed by the Air and Space Academy and led by scientists, engineers and technology experts heavily involved in planetary sciences and in the space exploration of the Solar System. This exercise involved three successive steps designed to build progressively what have been called the four "pillars" of Planetary Exploration: 1. Major scientific questions on planetary systems; 2. Different types of space missions to fly to address these questions; 3. Key technologies required to master to make these missions flyable; 4. Ground-based and space-based infrastructures needed in support to these missions. This talk will focus on the set of representative space missions recommended to be flown by 2061 to address the six key scientific questions identified in our community foresight exercise. These missions can be classified in terms of six "provinces" of destinations (the Earth and near-by orbits; the Earth-Moon system; Terrestrial planets; Giant planets; Small bodies; The Heliopause boundary and beyond) and of their degree of complexity (from Earth-based observations through fly-bys and ultimately to sample return). The exercise also identified the key requirements for the technologies that will be needed to fly these missions within the Horizon 2061 time frame. The authors of this abstract would like to express their sincere thanks to the over 200 participants in the different Horizon 2061 meetings, whose inputs and ideas are the basis for this report. The full report of the exercise can be found at http://horizon2061.cnrs.fr/


PS09-A017
The New Jupiter: Results from Juno and Lessons for Future Missions

Scott BOLTON#+
Southwest Research Institute

Juno has transformed our view of Jupiter through major discoveries about its interior structure, origin, and evolution; atmospheric dynamics and composition; magnetic field and magnetosphere. Juno’s extended mission began in August 2021 and includes new objectives that reach beyond the planet itself to the Galilean satellites and Jupiter’s enigmatic ring system. Close flybys of Ganymede in the summer of 2021 and of Europa in September of 2022 provided new and unique views of the satellites. Two close flybys of Io in December, 2023 and February, 2024, are complemented by Juno’s multi-orbit campaign to monitor Io’s volcanic activity and explore variability in the Io torus and Jovian aurora. Results from Juno’s primary and extended missions as well as the satellites and ring system will be presented. Lessons learned from Juno relevant to the planning and implementation of future solar system exploration will also be presented.


PS09-A009
Phase Behavior of Clathrate Hydrates in Presence of Ammonia - Implications for Titan

Mathieu CHOUKROUN1#+, Elodie GLOESENER1, Tuan VU1, Helen MAYNARD-CASELY2, Ashley DAVIES1, Arnaud DESMEDT3, Christophe SOTIN4
1Jet Propulsion Laboratory, California Institute of Technology, 2Australian Nuclear Science and Technology Organisation, 3Institut des Sciences Moleculaires, Bordeaux, 4Nantes Universite

We report new results from recent work performed to better understand the phase behavior of Methane clathrate hydrates (MCH) and their implications for methane outgassing on Titan. Titan’s present-day atmospheric CH4 would only last a few tens to 100 My because of active photochemistry that dissociates CH4 and N2 and recombines them into heavier hydrocarbons and nitrogen-rich organic molecules. Methane clathrate hydrates (MCH) have long been proposed as a potential internal reservoir of CH4. Persistent MCH dissociation would release CH4 into the atmosphere and sustain its presence in Titan’s atmosphere over geological timescales. However, the past 20 years of exploration, recent laboratory experiments, and numerical simulations require revisiting some aspects of this scenario. Indeed, the Cassini-Huygens mission has shown a paucity of unambiguous cryovolcanic features on Titan, although its surface is relatively young (between 500 and 1,000 My). Also, laboratory experiments and thermal models have shown that pure MCH are so stable on Titan that inhibitors such as ammonia are needed to dissociate them under present day conditions. Furthermore, there is growing evidence that comets are the building blocks of outer Solar System objects, which implies that the abundance of MCH inhibitors like NH3 would be on the order of ~ 1-2% relative to H2O, instead of the ~ 5-15% that were foreseen in early models. Lastly, MCH may incorporate small amounts of NH3 inside their crystalline structure, instead of forcing it to remain in a liquid or hydrate phase, however this is an area of active research.


PS09-A016
Solar Ring Mission: Building a Panorama of the Sun and Inner-heliosphere

Chenglong SHEN#+, Yuming WANG, Jingnan GUO
University of Science and Technology of China

Solar Ring (SOR) is a proposed space science mission to monitor and study the Sun and inner heliosphere from a full 360 perspective in the ecliptic plane. It will deploy-three 120°-separated spacecraft on the 1-AU orbit. The first spacecraft, S1, locates 30° upstream of the Earth, the second, S2, 90° downstream, and the third, S3, completes the configuration. This design with necessary science instruments, e.g., the Doppler-velocity and vector magnetic field imager, wide-angle coronagraph, and in-situ instruments, will allow us to establish many unprecedented capabilities: (1) provide simultaneous Doppler-velocity observations of the whole solar surface to understand the deep interior, (2) provide vector magnetograms of the whole photosphere — the inner boundary of the solar atmosphere and heliosphere, (3) provide the information of the whole lifetime evolution of solar featured structures, and (4) provide the whole view of solar transients and space weather in the inner heliosphere. With these capabilities, Solar Ring mission aims to address outstanding questions about the origin of solar cycle, the origin of solar eruptions and the origin of extreme space weather events. The successful accomplishment of the mission will construct a panorama of the Sun and inner-heliosphere, and therefore advance our understanding of the star and the space environment that holds our life.


Fri-04 Aug | 8:15 - 10:00 | MR308
PS06 - Astrochemical Processes Leading to the Formation of Planetary Bodies in the Solar System

Session Chair(s): David DUBOIS, NASA Ames Research Center

PS06-A006
Electron-stimulated Desorption and Molecules Diffusion in the Astrophysical Ice Mixture

Chun-Yi LEE1#+, Antonio JIMENEZ-ESCOBAR2, Angela CIARAVELLA2, Cesarean CECCHI-PESTELLINI2, Yu-Jung CHEN1
1National Central University, 2INAF—Osservation Astronomico di Palermo

In the evolution of interstellar clouds, the icy mantle is expected as a bilayer structure composed of a water-rich ice mixture layer including methane and ammonia covered by carbon monoxide and its hydrogenation production layer during the CO freeze-out stage. Several kinds of energy sources in space such as secondary UV field, cosmic rays, and electrons may induce the complex reaction in the ice and also stimulate the desorption. Ciaravella et al. (2022) reported that the molecules from the deep layer can travel through several hundred monolayers and enhances the desorption during the X-ray irradiation of the layered ice. The molecular mixing enhances chemical reactions from which complex organic species, including many of prebiotic interest, are formed. Furthermore, diffusion drives the desorption of species that would otherwise remain buried near the surface of dust, thus enhancing their abundance in the gas, where they can be detected in the radio-wave domain. In this work, the layered ice is composed of H2O:13CH4:NH3 (2:1:1) covered by the ice mixture CO:CH3OH (3:1). The low-energy electron is chosen as the energy source to induce the product 13CO diffusion from the bottom layer ice and to investigate the diffusion coefficient and also the mechanism for the long-distance diffusion.


PS06-A008 | Invited
From Interstellar Ice Grains to Evolved Solar System Icy Bodies – Tracing the Ice and Organics

Murthy GUDIPATI#+
Jet Propulsion Laboratory, California Institute of Technology

In the JWST era, it is more timely than ever before to understand “whether, how, and to what extent” organic molecules and ice structures are preserved as our solar system went through its formation steps over 4.6+ billion years through various stages. Synthesis or a wide range of organic molecules and preserving them in primordial amorphous ice grains is one of a few working postulates on the Origin of Life on Earth. While in the interstellar phase ice grains containing organics are understood to exist under very cold conditions with little or no thermal processing but irradiation through cosmic rays and local stellar ultraviolet photons, how these ice grains evolved as they accreted onto a protostar and protoplanetary stage is still an open question. Further, we need to understand local thermal and radiation environments that contribute to material changes in the past 4.6 billion years as reflected in the composition of present-day comets. At the “Ice Spectroscopy Laboratory (ISL)” of Jet Propulsion Laboratory, we have been engaged in simulating these ices, synthesis of organics, and thermal and radiation environments they would potentially undergo. Our goal is to determine water-ice phases and molecular species that are tracers of “primordial” grains starting their journey in the interstellar medium and becoming a part of cometary precursors. This presentation discusses an overview of the research we conducted at the ISL on ice physics and chemistry and summarizes outstanding questions. Acknowledgments: The research presented here was funded by NASA Research and Analysis Programs such as Solar System Workings (SSW), Discovery Data Analysis Program (DDAP), and was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration (NASA).


PS06-A014
A New Breakup Mechanism for the Heterogeneous Meteoroid in an Improved Granular Method

Ziwen LI1#+, Qingbo GAN2, Yao ZHANG2, Jing LIU2, Xiangyuan ZENG1
1Beijing Institute of Technology, 2National Astronomical Observatories of China

Most meteoroids originating from small celestial bodies have heterogeneous structures and various mass distributions. The dynamical evolution of meteoroids is the comprehensive result of gravity, aerodynamic forces, ablation, and breakup behaviors. Prior studies focused on the influence of the initial mass distributions on the breakup results, while the spatial positions of the inner groups have not been concretized. This paper proposes a non-spherical N-body method to investigate the meteoroid entry problem. Numerous granules with designated positions construct the meteoroids with different shapes and porosities. For simulating the coarse surfaces and the volume change under ablation, the vertices of the polyhedral granules are manipulated according to the impact angle of the freestream. A new dynamical mechanism for meteoroid breakup is presented to explain the peculiar phenomenon where the subsequent breakup happens under smaller stagnation pressure than the initial breakup. This phenomenon contradicts the Weibull strength scaling law (fragment strengths increase with decreased size), and its mechanism is unclear. According to the heterogeneous ablation of meteoroids, the concentrated detonation products with significant repulsive influence on the surrounding objects are investigated. If the pressure of the concentrated detonation products exceeds the strength, meteoroid fragmentation is also considered to be triggered. The feasibility of this newly-presented method is verified in demonstrating the separation of the Morávka meteoroid. The meteoroids constituted with blocks in different properties or layered granules are proposed to discuss the influence of the structure.


PS06-A011
A Quantum Chemical Perspective on Biomolecular Synthesis in Astrophysical Ices

Partha BERA1,2#+
1NASA Ames Research Center, 2The Bay Area Environmental Research Institute

Identification of nucleobases in extraterrestrial carbonaceous chondrites implies their formation in an abiotic condition, and supports their prebiotic role in early Earth. Physicochemical processes by which these complex molecules are synthesized in icy grains are not well understood. The products (amino acids, nucleic acids, sugars) of UV photo-irradiation of mixed molecular ices containing H2O, NH3 and CH4 have been explored using robust new density functional theory (DFT) methods (wB97M–V) along with large correlation consistent basis sets and explicit solvent calculations using a polarized continuum model (PCM), and compared against laboratory experimental results. Mechanisms studied include those starting with neutral and cationic counterparts, and then reacting with neutrals and radicals generated by radiation. The calculations reveal that the formation of nucleobases is energetically and kinetically favorable. The gas phase mechanism of their formation proved ineffective, and the presence of one or several water molecules is necessary in order for the final products to form. These computational results support the scenario in which prebiotic molecules, such as the nucleobase uracil, and complex organic molecules such as sugars, and nucleobases can be formed under abiotic processes in astrophysically relevant interstellar environments, and on surfaces of icy grains before being delivered to telluric planets such as Earth. [1] Bera, P.P. et al. (2019) Astrophys. J. 884, 64 [2] Materese, C.M. et al. (2020), Astrobiology. 20, 601. [3] Sandford, S.A. et al. (2020) Chem. Rev. 120, 4616, [4] Bera P. P. et al. (2017) Astrobiology, 17, 771-785, (2017). [5] Bera, P. P. et al. (2016) J. Chem. Phys, 144, 144308. [6] Sandford, S. A. et al. (2014) Topics in Curr. Chem., Vol-2. [7] Materese, C. K. (2013) Astrobiology, 13, 948. [8] Bera P. P. et al. (2010) J. Chem.Phys., 133, 104303. [8] Sandford et al. (2020) Chem. Rev. 120, 4616.


PS06-A016
Observations of Meteor Specular and Non-specular Echoes Using All-sky Meteor Radar

Yi LI1#+, Guozhu LI1, Haiyong XIE2, Lianhuan HU1, Wenjie SUN1, Xiukuan ZHAO1
1Chinese Academy of Sciences, 2Institute of Geology and Geophysics, Chinese Academy of Sciences

In this study, we employ the specular and non-specular echo observations by all-sky meteor radars to investigate the meteor properties and orbital parameters of meteor shower, such as the October Draconid meteor shower. Four outbursts (2011, 2012, 2018 and 2019) of the October Draconids were observed between 2009 and 2021. The observations confirmed the predictions of the outburst of the Draconids in 2019, which is important for the improvement of the prediction model and exploring the orbit of the parent comet as it changes throughout time. On the other hand, we study the occurrences of meteor trail non-field-aligned irregularities (NFAIs) at low latitudes. The non-specular meteor echoes backscattered from NFAIs have weak magnetic sensitivity, in contrast to the high magnetic aspect sensitivity of background ionospheric irregularities (i.e. field-aligned irregularities, FAIs). These NFAI events peak around the morning hours, with the beginning (end) altitudes up to (down to ) 120 km (~80 km). Their mean heights are about 2-6 km higher than specular meteor echoes. The occurrence of the NFAIs echoes peaks on certain days that is probably related to meteor showers. On average, the ratio of the detected NFAIs echoes to specular echoes is less than 1‰. Possible factors responsible for the NFAIs at low latitudes are discussed based on the current understanding of the meteor dust trail.


Fri-04 Aug | 10:20 - 12:20 | MR307
PS09 - Geology, Geophysics, and Habitability in Our Solar System

Session Chair(s): Anezina SOLOMONIDOU, Hellenic Space Center

PS09-A002
Habitability of Hydrocarbon Worlds: Titan and Beyond

Rosaly LOPES1#+, Michael MALASKA1, Steven VANCE1, Robert HODYSS1, D'Arcy MEYER-DOMBARD2, Sarah FAGENTS3
1Jet Propulsion Laboratory, California Institute of Technology, 2University of Illinois at Chicago, 3University of Hawaii at Manoa

Titan is an ocean world, an icy world, and an organic world. Titan’s subsurface ocean and ductile ice are the most likely habitable environments on the moon. The ocean may be in contact with an organic-rich ice-rock core, potentially providing redox gradients, heavier elements, and organic building blocks critical for a habitable environment. Titan’s abundant surface organics could be delivered to the aqueous environment through processes such as impact cratering and potential convective cycles in the ice shell. Our work investigates the pathways for atmospheric organic products to be transported from the surface to the ocean/core and the potential for ocean/deep ice biosignatures and organisms to be transported to the shallow crust or surface for interrogation and discovery. Our overarching goal is to characterize the habitable environments on Titan and identify their potential biosignatures. We will present a summary of the work conducted by the team to date, which focuses on the following objectives: (i) Determine the pathways for organic materials to be transported (and modified) from the atmosphere to surface and eventually to the subsurface ocean (the most likely habitable environment). (ii) Determine whether the physical and chemical processes in the ocean create stable, habitable environments. (iii) Determine what biosignatures would be produced if the ocean is inhabited. (iv) Determine how biosignatures can be transported from the ocean to the surface and atmosphere and be recognizable at the surface and in the atmosphere. This work is funded by NASA’s Astrobiology Institute grant NNN13D485T. Part of this work was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under contract with NASA.


PS09-A005
The Global Interplay of Mountains, Dunes and Cryovolcanic Landscapes of Titan – Connecting Organics with Water Ice for Habitability

Jani RADEBAUGH1#+, Ben LAKE1, Jason BARNES2, Elizabeth TURTLE3, Madeleine WRIGHT1, Delaney ROSE1, Eric CHRISTIANSEN1, Anezina SOLOMONIDOU4, Rosaly LOPES-GAUTIER5, Michael MALASKA5
1Brigham Young University, 2University of Idaho, 3Johns Hopkins University Applied Physics Laboratory, 4Hellenic Space Center, 5Jet Propulsion Laboratory, California Institute of Technology

The surface of Saturn’s moon Titan exhibits many Earth-like landscapes, including rivers and lakes, mountain belts, volcanoes and vast sand seas. These features formed through atmospheric and surface processes of wind and methane-based liquids doing work on landforms, and through contractional and extensional tectonism and extrusion of liquid water during cryovolcanism. Many of these processes are actively shaping the landscape today. The distribution of mountains across Titan, measured from a global database, reveals extension may be dominant near Xanadu while contraction has formed E-W equatorial ridges. Dunes are broadly distributed across equatorial regions. Dune orientations reveal W-E sand transport, interrupted by elevated regions and topographically low Xanadu. Sand in Titan’s dunes could be from evaporites, sintering of fallout or erosion of bedrock. The spectral and material properties of the VIMS blue materials compared to the VIMS bright, and the proximity of these materials to the upwind sand sea margins, make these a candidate for sand sources. Perhaps uplift along a fissure west of Xanadu has exposed VIMS blue material to erosion to source sands for sand seas. Doom Mons, with the associated flow feature Mohini Fluctus, is currently the best candidate cryovolcano, but other features have been proposed as resulting from maar-like processes or lava flows. If these landscapes are all cryovolcanic in origin, it would suggest that heat flow is widely dispersed. Erosion and transport, impacts and cryovolcanic eruptions could cause interactions between water ice-rich materials and organics, perhaps creating a transient environment for prebiotic processes or even life. The Dragonfly rotorcraft lander will land among dunes, near the Selk impact crater and rugged terrain. Closeup views will augment current global views, revealing more about the materials and interplay of geologic processes at work on Titan’s surface, and the potential for prebiotic chemistry and life on this unique body. 


PS09-A010
Size and Geometry Influences the Atmospheric Circulation and Surface Fluxes Over Titan’s Lakes

Scot RAFKIN1#+, Audrey CHATAIN2, Alejandro SOTO1, Enora MOISAN3
1Southwest Research Institute, 2University of the Basque Country, 3École Normale Supérieure de Lyon

Saturn’s moon Titan is unique among the solar system. It has a thick nitrogen atmosphere with lesser abundances of volatiles. Methane is the most abundant of these volatiles, and the evaporation, condensation, and precipitation of methane results in a cycle analogous to Earth’s hydrologic cycle. The sensible and latent heat exchange between the atmosphere and Titan’s lakes and seas is quantified in this study using the mesoscale Titan WRF (mtWRF) model, and the impact of air-sea exchange to Titan’s global methane and energy cycle based on these model-resolved exchange studies is discussed. 
mtWRF has recently been extended to three dimensions and a radiative transfer scheme has been implemented. These new physics enable the important effects of lake geometry on air-sea exchange, the atmospheric circulation forced by these exchanges, and the thermal impact on the lake to be investigated. Idealized lake shapes demonstrate how lake size and lake shore concavity influence surface fluxes and atmospheric circulation. The shape of the lake shore drives regions of near-surface convergence and divergence, depending on the concavity. The overall size of the lake has an influence on the strength and scale of the resulting sea and land breezes, which are driven by diurnal radiative forcing and methane evaporation. Within these near-surface circulations, the wind speed is accelerated or decelerated, which exerts a strong control on the sensible and latent heat fluxes. Consequently, the mixed layer lake temperature is influenced by the lake geometry.
More realistic lake shapes based on Cassini radar are simulated to quantify how air-sea exchange and the resulting atmospheric circulations might operate on Titan. Because most of Titan’s lakes are in the high northern latitudes, the strong seasonal variation of insolation is further explored and is shown to exhibit a strong influence on the results.


PS09-A011
The Effect of Surface Temperature on Moon Convection

Yuxiao ZHI#+, Yaolin SHI
University of Chinese Academy of Sciences

The surface temperature is an important thermophysical parameter in planetary studies and a fundamental boundary condition in thermal evolution simulations, affecting the thermal state and evolution of the interior. The surface temperature of planets has usually been set to a constant value in previous studies. However, on the surface of non-atmospheric bodies such as the Moon and Mercury, the temperature is significantly correlated with latitude. The difference between the average temperature at the lunar poles and the equator can be more than 100K. To investigate the effect of surface temperature on lunar convection, we intercepted lunar temperature data from 2009 to 2017 based on Diviner measurements, calculated the average temperature per 0.5 latitudes, and used it as an external boundary condition to complete the thermal evolution simulation of the two-dimensional spherical crustal convection model. The results of the simulations show that the surface temperature strongly influences the lunar convection pattern. The poles tend to form downwelling plumes due to lower temperatures, and upwelling plumes prefer to start from the equatorial position, which is particularly evident in early evolution. The difference in lithospheric thickness between the lunar poles and the equator can reach more than 400 km after 4.5 billion years of evolution due to the surface temperature. The simulation results also show that the latitudinal distribution of surface temperature influences the tectonic distribution of the lunar surface to some extent. In future studies of planetary thermal evolution, especially early evolution, the influence of the latitudinal distribution of surface temperature should be considered.


PS09-A006
Alteration of Subaqueous Volcaniclastic Deposits in the Ancestral Cascades Arc in Southern Washington State

Rui-Lin CHENG#+, Joseph MICHALSKI
The University of Hong Kong

The Wildcat Creek beds (WCB) in Southern Washington State exclusively consist of a succession of different volcaniclastic facies, which record explosive Ancestral Cascades volcanism in the Oligocene. These beds are dominated by pumice breccia. Most of them contain angular volcanic clasts, and some beds also preserve accretionary lapilli and fiamme. Facies analysis interpreted these beds are fed by subaerial eruptions and sedimented in a subaqueous environment by either tephra fallout over water or pyroclastic flows crossing the shoreline into water. In this study, we conducted a detailed mineralogical study of pumice breccia from a well-exposed, continuous stratigraphy at Wildcat Creek, which included unaltered, partly devitrified and altered, and entirely devitrified and altered samples. The unaltered (compared to others) sample still preserves the vesicular texture featured by many cavities and contains montmorillonite, illite, and mordenite. In other altered samples, vesicles are filled with secondary minerals. The clay fractions of altered breccia are dominated by Fe-rich chlorites, and contain illite ranging from almost none to moderate, and to a great deal, together with different types of zeolites. The assemblages of chlorites with illite of varied content in the WCB pumice breccia reflect different alteration processes after tephra or pyroclastic flows emplaced into subaqueous environments, which may also provide implications to chlorite-illite deposits on Mars.


PS09-A012
Multipole Expansion: Unifying Formalism for Earth and Planetary Gravitational Dynamics

Benjamin F. CHAO#+, Sheng-An SHIH
Academia Sinica

The powerful method of multipole expansion has found wide utility in classical electromagnetics and quantum-mechanics. In contrast, the gravitational mechanics traditionally have only seen peripheral mentions of the corresponding (mass-density) multipoles in specific applications. Here we develop the general theory of the multipole formalism for the classical two-body gravitational dynamics, a most prevalent subject in planetary (and global Earth) dynamics. We treat two general, well-encountered configurations: (i) The interior “mantle-inner core gravitational (MICG)” type of configuration consisting of concentric bodies; and (ii) the exterior type of configuration of “planet + satellite” separate bodies in the general form of tidal interactions. We derive concise and exact formulas in terms of multipole expansions; by retaining the leading term(s) of relevance, typically up to the quadrupolar terms that include the planetary triaxiality, one can evaluate to the precision desired while bearing in mind that higher subtleties are readily available in the higher multipole terms. The two-body problems that are so formulated range from potential energy, satellite orbit, to tides, librations of sorts and precession/nutation, to planetary rotational normal modes and wobbles. We demonstrate that, via its various symmetry properties, the multipole formalism provides a theoretical unification framework for these gravitational phenomena that are conventionally treated topic-by-topic in textbook literature.


PS09-A008
Joint Forward Modeling with the Open Source Framework PlanetProfile

Steven VANCE#+, Marshall STYCZINSKI
Jet Propulsion Laboratory, California Institute of Technology

Constraining the interior properties and processes in planetary bodies relies heavily on the inversion of geophysical data, resulting in non-unique solutions. This is a problem especially for efforts to understand the habitability of ocean worlds. Joint inversion of multiple data streams can reduce non-uniqueness. Large probabilistic forward models using precise and self-consistent laboratory data will make it possible to infer interior water content and heat sources, and ultimately to locate drivers of chemical energy that might support life. To provide the needed forward models, we continue to develop the PlanetProfile open-source framework for understanding planetary interiors. This software has been a key component to studies of the ocean worlds in terms of: seismicity (Panning et al. 2018, Stähler et al. 2018, Vance et al. 2018, Marusiak et al. 2023), magnetic properties (Vance et al. 2021), and geodynamic and impact processes (Marusiak et al. 2022, Carnahan et al. 2022, Crósta et al. 2022).In recent months, we have converted PlanetProfile from Matlab into a Python version that improves access to the software and streamlines its operation. The source code is available on GitHub at https://github.com/NASA-Planetary-Science/PlanetProfile with instructions for its use. We encourage user contributions. The new version links to other scientific software packages, including for evaluating equation-of-state data, magnetic induction calculations, and seismic calculations (Vance et al. 2021). Calculations of internal Love numbers via ALMA3 is being implemented (Melini et al. 2022). We are actively involved in developing fundamental data for these packages, which will enable the fidelity of forward modeling needed to infer the salinity, heat flow, and other clues to the habitability of internal oceans in icy worlds. Here, we describe recently obtained electrical conductivity data, summarize models for major moons across the outer solar system, and discuss new inferences about the interior structures of several bodies.


PS09-A013
What Kind of Thing is a Planet?

Rohan BYRNE#+
University of Melbourne

How does a bundle of methods targeting a common subject coalesce into a true first-order science? As planetary scientists, we await an ontology that inaugurates us as custodians of a unique way of thinking: the 'logos' that would make us 'planetologists'. Drawing on insights from complexity and dynamical systems theory, we use our database of millions of computational numerical planetary evolution simulations to argue for the uniqueness and independence of planets in the taxonomy of material structures, analogous to fields in physics, atoms in chemistry, and species in biology. By testing the sensitivity of even very simple planet-like systems to minor perturbations, and observing their ultimate convergence upon certain canonical pathways, we give a sense of what a self-possessed science of planets could look like, what its principal objects of discourse would be, and what it might offer to our own field and to the wider scientific endeavour.


Fri-04 Aug | 10:20 - 12:20 | MR308
PS06 - Astrochemical Processes Leading to the Formation of Planetary Bodies in the Solar System

Session Chair(s): David DUBOIS, NASA Ames Research Center

PS06-A005
Petrogenesis of the Andesitic Achondrite EC 002

Ziliang JIN#+
Macau University of Science and Technology

In the collection of our meteorites, andesitic achondrites are rare but important. Currently, the parent body of the early andesitic rocks in our solar system and their evolutional history are still unclear. To better understand the genesis of early andesitic rocks, we conducted detailed chemical and isotopic analysis on the minerals in the andesitic achondrite Erg Chech 002 (EC 002), the oldest fragment of an igneous crust. EC002 is composed of andesitic groundmass and disequilibrium orthopyroxene xenocrysts. Our analytical results show that the δ18O values of the xenocrysts are >0.5‰ larger than those of the pyroxene minerals from the andesitic groundmass. The 18O depleted signature of the minerals from the andesitic groundmass indicates that the parent body of EC002 that formed in the inner solar system could have accreted outer solar system materials resembling CR chondrites. The addition of these materials could also have (1) modified the redox of the parent body and (2) brought “wet” components that drove the generation of the andesitic magma.


PS06-A001
Low-temperature Nitrogen Ion Chemistry Modeling of the Atmosphere of Saturn's Moon Titan

David DUBOIS1#+, Alexander RAYMOND2, Ella SCIAMMA-O'BRIEN1, Farid SALAMA1
1NASA Ames Research Center, 2Jet Propulsion Laboratory

In Titan’s atmosphere, complex chemistry induced by photolysis and radiolysis of its main constituents, N2 and CH4, results in the formation of gaseous species (radicals, hydrocarbons, nitriles) and solid particles that form Titan’s haze. The Cassini mission unveiled the presence of large charged species in Titan’s ionosphere, highlighting the important role ions play in the atmospheric reactivity. Furthermore, the nitrogen-rich compounds are expected to play a key role in the chain of reactions occurring in Titan’s atmosphere. Many laboratory experiments have been developed to investigate the chemical pathways involved in Titan’s atmospheric organic growth. In parallel, photochemical models have substantially advanced our understanding of Titan’s ionospheric chemistry. However, these models have faced obstacles due to the limited availability of reaction rates. Here, we investigated Titan's low-temperature (150 K) gas phase N2-CH4-based chemistry using both numerical and experimental work: (1) the Titan Haze Simulation (THS) experiment developed on the COsmic Simulation Chamber (COSmIC) at NASA Ames Research Center allows simulating Titan’s atmospheric chemistry at low temperature using a plasma discharge in the stream of a jet-cooled gas expansion; and (2) a 1D chemical network model using a fluid mechanical framework is employed to simulate the ion-neutral chemical reactivity occurring at low temperature in the COSmIC/THS. We have updated the reaction rates in our numerical model and studied the sensitivity of changing plasma conditions on the resulting ion chemistry. We also investigated specific nitrogen-rich pathways to determine their influence as gas phase precursors. Elemental composition of the gas-phase products and comparisons with recently published compositions of the Titan aerosol analogs produced in COSmIC/THS will be presented. Finally, the implications of these results will be compared to other laboratory and numerical simulations demonstrating the importance of plasma chemistry experiments and modelling to improve our understanding of cold planetary environments.


Fri-04 Aug | 1:10 - 3:10 | MR305
PS11 - Microwave and Infrared Remote Sensing of Solar System Objects

Session Chair(s): Scott BOLTON, Southwest Research Institute

PS11-A012
Chlorides in Ceres’ Molecular Exosphere

Yo-Ling CHUANG#+, Hsien-Ju TSAI, Yi-Jehng KUAN, Chia-Cheng CHIANG
National Taiwan Normal University

Ceres, one of the targets of the Dawn mission, is known to have a warm, liquid-bearing interior rich in volatiles. The detection of aliphatic organic matter on an aqueously-altered body admits the possibility that extensive prebiotic synthesis could have occurred on Ceres. Ceres hence becomes an object of intense interest for the study of primitive solar-system bodies and astrobiology. Observations of water ice, hazes and organic compounds on the surface of Ceres by Dawn mission point to the likely existence of an exosphere via mechanisms such as sputtering by solar wind particles, cryovolcanism and thermal sublimation that allow their removal into space. As a result, molecular species identified in the exosphere may reflect the surface chemical composition of Ceres. We therefore observed the dwarf planet Ceres using the Atacama Compact Array to look for spectral emission in Ceres’ molecular exosphere. The preliminary results indicate that we have detected molecular emission of NaCl and KCl toward Ceres tentatively. Detections of exospheric chlorine-containing species implies the existence of salt-containing water ice on Ceres’ surface which results from volumes of subsurface salty liquid water most likely. The discovery of NaCl and KCl if confirmed would provide circumstantial evidence for the existence of sizable subsurface salty water reservoirs on Ceres. Detections of chlorides allow for measurements of chlorinity in the reservoirs which is also essential to our understanding of Ceres’ origin.


PS11-A006
An HCN Vertical Distribution Reference for Titan and Hot Super-Earths

Miriam RENGEL1#+, Denis SHULYAK2,1, Paul HARTOGH1, Raphael MORENO3, Christopher JARCHOW1, Dieter BREITSCHWERDT4
1Max Planck Institute for Solar System Research, 2Instituto de Astrofísica de Andalucía, 3Paris Observatory, 4Technische Universität Berlin

Hydrogen cyanide (HCN) is an important component of nitrogen-dominated atmospheres in hot super-Earths and exoplanets with Titan-like characteristics. To enhance our understanding and observation of such atmospheres, we present a comprehensive reference HCN vertical distribution based on quasi-simultaneous ground-based submillimeter and Herschel observations in Titan's stratosphere. By utilizing a line-by-line radiative transfer code and retrieval algorithm, we calculated synthetic spectra and derived vertical profiles. Through inter-comparing space and ground-based observations, we ensured consistency and developed a robust reference profile for use in climate models and chemistry calculations. Our reference profile will aid in future observations of Titan and Titan-like exoplanets, and serve as a valuable resource for characterizing these atmospheres


PS11-A009
Origin of Neutral Gas with Peculiar Velocity in the Saturn E-ring

Yueh-Ning LEE1,2#+, Yi-Jehng KUAN1, Yo-Ling CHUANG1
1National Taiwan Normal University, 2National Center for Theoretical Sciences

The materials of Saturn E-ring are known to have originated from the satellite Enceladus. Once leaving the satellite, either by surface sputtering, outgassing plumes, or other mechanisms, the ejected material is subject to several forces in synergy, among which gravity, electromagnetic forces, and radiation forces. In consequence, unlike Enceladus, which is massive enough to follow a Keplerian orbit, all kinds of trajectories are manifested by small particles. Particles with large mass-to-charge ratio barely feel the sweeping magnetic field that is co-rotating with Saturn. On the other hand, particles with small mass-to-charge ratio have small gyro-radius, and thus are bound to the magnetic field lines. Through Hamiltonian analysis, we discovered that particles with intermediate mass-to-charge ratio may form a distinct population of ring particles. This population can exhibit velocity signatures that are verifiable through observations. Given that neutral molecular gas can only follow Keplerian orbits before they suffer from further collision or ionization, they could reflect the velocity of their parent body, if the latter is charged, for a relatively short time span before their trajectories diverge. Therefore, if some neutral molecular gas with peculiar velocity is found through observation, this must suggest there are some sources constantly replenishing them.


PS11-A008
Neutral Gas Molecules in the Vicinity of Enceladus: Plume vs. Torus

Yi-Jehng KUAN1#+, Chia-Cheng CHIANG1, Hsien-Ju TSAI1, Yo-Ling CHUANG1, Yueh-Ning LEE1,2
1National Taiwan Normal University, 2National Center for Theoretical Sciences

The Cassini mission discovered an active plume composed of water vapor and ice grains emanating from Saturn’s icy moon Enceladus. The composition of salt‐rich ice grains, gravitational measurements and the libration of Enceladus are clear evidences for the argument for a warm and salty subsurface ocean. Cassini’s Ion and Neutral Mass Spectrometer data indicate Enceladus’ plume neutral gas consists of mostly H2O, and minor ingredients H2, CO and/or N2, CO2, NH3, HCN, CH4, H2CO, H2S plus some organic molecules such as CH3OH and C2H5OH, and possibly ketene and glycine (Waite+ 2009, 2017; Magee & Waite, 2017). Identification of key species and trace compounds in the plume is thus critical to constrain theories for the internal constitution and composition of the subsurface ocean, and also, in the form of various simple organic molecules, provide biomarkers for the persistence of any subsurface life. On the other hand, most of the ejected neutrals, including water vapor, in the plume escaped from Enceladus feed the magnetospheric plasma and form a donut‐shaped neutral torus around Saturn. Through charge‐exchange scatterings and neutral‐neutral collisions, H2O and dissociated products spread around Saturnian system. The OH and H2O tori were detected (Shemansky+ 1993; Hartogh+ 2011). Enceladus gas torus contains molecules and atoms created by photolysis processes and chemical reactions on chemical compounds delivered via the plume, whereas the plume would contain the most original composition of the subsurface ocean. To investigate whether Enceladus is life sustainable, it is crucial to study the molecular ingredients of Enceladus’ subsurface ocean, namely, chemical compositions of the plume and gas torus. Therefore, we observed Enceladus using the Atacama Large Millimeter/submillimeter Array. In this report, we will present our latest findings of the gas molecules detected in the vicinity of Enceladus and discuss their possible origins.


PS11-A003
The Submillimetre Wave Instrument (SWI) on JUICE: Launch Phase and NECP Results

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 satellites 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. The JUICE launch is scheduled for mid April 2023. It follows the Near-Earth Commissioning (NECP) of the spacecraft and the instruments. According to current plans the NECP will be completed on 18 July 2023. In this presentation the instrument specifications as determined during the AIVT phase and the first results from the SWI NECP will be reported.


Fri-04 Aug | 1:10 - 3:10 | MR307
PS14 - Venus:  Evolution of the Interior, Surface, and Atmosphere

Session Chair(s): Yang LIU, National Space Science Center, Chinese Academy of Sciences, James HEAD, Brown University

PS14-A004
Venus Volcano Imaging and Climate Explorer Mission

Yang LIU1#+, Xiaolong DONG2, Jieying HE2, Feng ZHANG2, Jian XU2, Yuyan ZHAO3, Yu WANG2, Haotian ZHU2, Yongmei WANG4, Wenyu WANG1, Zhiming CAI5
1National Space Science Center, Chinese Academy of Sciences, 2Chinese Academy of Sciences, 3Chengdu University of Technology, 4National Space Science Center, CAS, 5Innovation Academy for Microsatellites

Venus Volcano Imaging and Climate Explorer (VOICE) is an orbiting mission to investigate the Venusian volcanic and thermal evolution history, water and plate tectonics, internal structure and dynamics, climate evolution, possible habitable environment and life information in the clouds. Three state-of-the-art scientific payloads, the Polarimetric Synthetic Aperture Radar (PolSAR), the Microwave Radiometric Sounder (MWRS) and the Ultraviolet-Visible-Near Infrared Multi-Spectral Imager (UVN-MSI), will be flown on a polar-circular orbit of about 350 km. The PolSAR with meter resolution surface imaging capability enables refined exploration of Venusian tectonic and volcanic activity and evolution history. The MWRS, with a combination of a nadir-looking module and a limb-looking module, has the capability to refine the thermal structure and composition of the Venusian atmosphere, including near surface, below-inside and above the clouds, and will reveal the exchange and interaction between the surface and lower atmosphere. The MWRS will also investigate biosignatures, such as PH3 and NH3, in the cloud to further the fundamental scientific questions on the habitable environment and life information in Venus' atmosphere. The UVN-MSI can map the global atmosphere and look through the atmosphere with NIR windows. The scientific objective of the VOICE mission is to advance the understanding of the geological and thermal history and evolution of Venus, the mechanisms of the global circulation of Venusian atmosphere, past and current habitable environments, and the possible existence of life in the clouds of Venus. The mission goals are to search for evidence of water and plate tectonic activities, reveal the type of volcanic activity and thermal evolution history of Venus; establish the composition and thermal structure of middle and lower atmosphere of Venus; reveal the mechanism of runaway greenhouse effect, and explore whether Venus has a habitable environment and whether life (once) existed.


PS14-A002
From Berlin to Venus – Laboratory Spectroscopy and the Venus Emissivity Mapper

Jorn HELBERT1#+, Giulia ALEMANNO1, Alessandro MATURILLI1, Darby DYAR2, Aurelie VAN DEN NEUCKER1, Solmaz ADELI1, Suzanne SMREKAR3
1German Aerospace Center, 2Planetary Science Institute, 3Jet Propulsion Laboratory

The Planetary Spectroscopy Laboratory (PSL) at DLR has supported planetary missions for 20 years. With its state-of-the-art tools and equipment, the laboratory can measure emissivity spectra of planetary analogs at temperatures up to 1000K in a vacuum environment. This capability includes acquisition of VNIR emissivity spectra ca. 750K, which is crucial in supporting the VERITAS and EnVision missions. PSL has measured emissivity of >100 rock and mineral samples at 750K with hundreds more expected before Venus data are acquired. Two hemispherical reflectance units modified to acquire both visible and infrared measurements under vacuum are also available. Cross-calibration is essential for effectively interpreting spectroscopic data from upcoming Venus missions that will observe the surface. Leading the way is the Venus Emissivity Mapper (VEM) on the NASA VERITAS and ESA EnVision missions. VEM uses a 14-band filter array to discriminate among global rock types and detect active volcanic activity by mapping thermal emission and near-surface water vapor abundance. VEM is a pushbroom multispectral imaging system with three lens elements and a single-element objective. The filter array is imaged by a two-element relay optic onto the FPA using an uncooled InGaAs detector. In addition to six surface channels, eight bands are dedicated to cloud structure, water vapor and background removal. DLR's experience with VIRTIS on Venus Express and its dedicated Venus surface emissivity measurements laboratory make it a leader in the investigation of emission spectroscopy of Venus. When combined with machine learning classification and regression techniques, these spectra will inform surface geology on Venus in new and pioneering ways.PSL at DLR plays a critical role in advancing our understanding of planetary science and is an essential resource for the international community. Its advanced tools, equipment, and spectral libraries position it as a leader in the field of planetary research.


PS14-A003
The Venus Climate Database, VCD Version 2.2

Ehouarn MILLOUR1,2#+, Sebastien LEBONNOIS1, Antoine MARTINEZ1, Thomas PIERRON1,2, Alexandre BOISSINOT3, Francois FORGET4, Aymeric SPIGA1, Jean-Yves CHAUFRAY4, Franck LEFÈVRE5, Franck MONTMESSIN5, Fabrice CIPRIANI6
1Sorbonne Université, 2National Centre for Scientific Research, 3Laboratoire de Météorologie Dynamique, 4University Pierre et Marie Curie, 5National Center for Scientific Research (CNRS) / Laboratoire Atmosphères, Observations Spatiales (LATMOS), 6European Space Agency

Based on the state-of-the-art Venus Planetary Climate Model (PCM, formerly known as the Venus IPSL GCM) developed by our team, we have generated a Venus Climate Database (VCD) (http://www-venus.lmd.jussieu.fr/). This tool was developed with funding from ESA in the context of the preparation of the EnVision mission. VCD v2.2 was released in February 2023. The VCD provides mean values and statistics of the main meteorological variables (atmospheric temperature, density, pressure and winds) as well as atmospheric composition and related physical fields. It extends from the surface up to and including the thermosphere (~250km). The database contains high resolution temporal outputs (using 24 hourly bins) enabling the representation of the diurnal evolution of quantities over a climatological Venusian day.
As the goal of the VCD is to provide information about the state of the Venusian atmosphere, various realistic settings have been used to run a series of baseline GCM simulations, namely:
- Simulations using various Extreme UltraViolet (EUV) input from the Sun, as this forcing influences significantly the thermosphere (~120km and above).
- Some supplementary simulations with extreme values of UV cloud albedo, to bracket the state of the atmosphere below the thermosphere. In addition to the aforementioned VCD scenarios, the following features are available:
- A "high resolution" mode based on a high resolution topography map (at 23 pixels/degree).
- Access to the Venusian intra-hour variability (RMS) of main meteorological variables, as well as the Venusian day-to-day variability thereof.
- The possibility to add perturbations to the climatological fields in order to generate realistic weather conditions. The VCD is distributed as (i) a main Fortran subroutine that users can interface and directly call from their own programs, interfaces to call this gateway routine using other programming languages (e.g. C, Python, IDL, Matlab, ...) are also provided; (ii) a web interface, for quick looks (http://www-venus.lmd.jussieu.fr).


PS14-A009
Observing Waves on Venus Dayside Upper Cloud with VIRTIS

Jose SILVA1#+, Yeon Joo LEE1, Javier PERALTA2, Daniela ESPADINHA3
1Institute for Basic Science, 2Universidad de Sevilla, 3Universidade de Lisboa

An atmospheric internal gravity wave is an oscillatory perturbation on an atmospheric layer in which buoyancy acts as the restoring force. As such, they can only exist in a continuously stably stratified atmosphere, that is, a fluid in which the static stability is positive and horizontal variations in pressure are negligible when compared to the vertical variations (in altitude) [Gilli et al. 2020; Peralta et al. 2008]. These waves are of particular interest because they represent an effective means of energy and momentum transport across various atmospheric layers, as these waves can form on one atmospheric region and travel through the atmosphere, sometimes over great distances, and dump their contained energy upon wave dissipation or breaking [Alexander et al. 2010]. Given these properties, study of atmospheric waves on Venus becomes important as another tool to answer some of the fundamental questions surrounding its atmosphere dynamics, mainly the origin and support mechanism of the remarkable superrotation of the atmosphere. We present here observations of wave-like structures on the dayside of Venus’s atmosphere using three different wavelength regions (280-320 / 365 / 600 nm) from VIRTIS-M images, as each seems to target slightly different altitudes in the cloud deck [Sanchez-Lavega et al. (2008); Horinouchi et al. (2018); Hueso et al. (2015); Jessup et al. (2015)]. Our goal is to evaluate the population of atmospheric waves in this region using previously unexplored data from VIRTIS, measure their properties and distribution and establish possible links with previous studies of waves. This work follows a previous study performed by Peralta et al. (2008) and by Silva et al. (2021), in an attempt to establish links between theses structures across several atmospheric layers of Venus.


PS14-A013
Reprocessing Pioneer Venus Orbiter Radio Occultation Data

Martin PATZOLD1#+, Silvia TELLMANN2, Kerstin PETER2, Janusz OSCHLISNIOK2, Matthias HAHN3
1RIU-Planetary Research at University of Cologne, 2Rhenish Institute for Environmental Research, 3University of Cologne

RIU-Planetary Research has won funding support for the reprocessing and the interpretation of the original raw open-loop occultation data taken by the Pioneer Venus Orbiter radio science experiment ORO from 1979 to 1988. These original raw open-loop data are available from the PDS while original processed atmospheric and ionospheric (temperature and electron density, respectively) profiles from the Venus atmosphere are not. We shall apply modern software code together with a new version of the Venus gravity field and newly processed orbit data available as SPICE kernels. A review of the original data sets showed a variety of observation lengths ranging from a few minutes to about 20 minutes duration. The longer observation sets contain presumably ingress and egress data. We shall present atmospheric and ionospheric profiles processed from exemplary original Pioneer Venus Orbiter raw open-loop data sets and compare them with VEX VeRa radio occultation profiles for comparable observation conditions.


PS14-A014
Long-term Studies of the Venusian Atmosphere by the Radio Occultation Experiments on Venus Express and PVO

Silvia TELLMANN1#+, Martin PATZOLD2, Bernd HÄUSLER3, Hiroki ANDO4, Takeshi IMAMURA5, Katsuyuki NOGUCHI6, Janusz OSCHLISNIOK1, Kerstin PETER1
1Rhenish Institute for Environmental Research, 2RIU-Planetary Research at University of Cologne, 3Universität der Bundeswehr München, 4Kyoto Sangyo University, 5The University of Tokyo, 6Nara Women's University

The exploration of Venus by spacecraft began in the early 1960s and since these early days, radio science experiments became an integral part of almost all planetary missions. The first Radio Occultation experiment at Venus was conducted during the flyby of Mariner 5 in 1967, followed by Mariner 10 and several Soviet Venera missions. The Pioneer Venus Orbiter spacecraft (PVO) orbited Venus between 1978 and 1992. After this very active aera of Venus exploration only Magellan could retrieve a small number of radio occultation profiles until Venus Express reached Venus in 2006 and orbited it until 2014. So far, Venus Express (VEX) provided by far the most extensive data set of radio occultation profiles at Venus. VEX was followed by the Japanese spacecraft Akatsuki which is still in orbit around Venus. This extensive data set covers already several decades which provides the opportunity to study not only the short-term variability in the Venus atmosphere but also long-term changes. Especially the data sets from PVO and Venus Express in combination with results from Akatsuki can be used to investigate changes in the thermal structure of Venus on different time scales. The dense cloud layer on Venus is a region of particular interest. Atmospheric waves, generated here are assumed to play a significant role for the maintenance of the atmospheric superrotation. The decipherment of the atmospheric fine structures seen in this altitude region is therefore of significance. Long-term changes in the zonal wind structure as well as changes in the SO2 content in the atmosphere have been observed in this region. The radio occultation measurements on Venus cover the upper troposphere (above ~ 35 km) and mesosphere (~ 100 km). They provide an excellent basis for the study of short-term as well as long-term changes on Venus.


Fri-04 Aug | 1:10 - 3:10 | MR308
PS13 - Surface Processes on Rocky Bodies in the Solar System

Session Chair(s): Man-To HUI, Macau University of Science and Technology

PS13-A002
A New Look at the Procellarum and Imbrium Maria Through Microwave Data

Roberto BUGIOLACCHI1,2#+
1Macau University of Science and Technology, 2Honorary Research Associate

This study focuses on the largest mare expanse on the Moon, which is dominated by Oceanus Procellarum and Mare Imbrium, and it is contained mainly within the Procellarum-KREEP-Terrane. A new analytical approach to microwave data acquired by the CELMS (CE-2 Lunar Microwave Sounder) radiometer onboard the Chang’e-2 mission reveals previously unseen variation patterns within the lunar surface geology. The derived differences in Temperature Brightness (TB) between day and night were compared, and large temperature anomalies were highlighted and studied in detail. We employed the data from the 3 GHz frequency channel (C1) which carry a potential maximum representation of several meters below the surface. Strong correlations with compositional maps, in particular, variations of pyroxenes species (derived from multispectral data), rock abundance (derived from infrared data) and topography were noted, and numerical relationships were calculated. Differences from the results of other investigative methodologies, which are mostly based in the UV-IR range, derive from the potential of microwave data to represent much of the regolith layer below the outermost micron-thick skin. A region-wide analysis of 16 regions of interest also reveals commonalities and differences between this vast lunar region and hints at a possible contribution from a linear cluster of relatively recent impact events. This region is still at the centre of much research on the thermal history of the Moon and has been the host of two recent lunar missions from China; further, it will be the target soon by several international enterprises. This work aims at helping in selecting eventual exploration targets and regions of interest. Finally, the results attest to the geological interpretative potential of microwave data and its complementary potential with established datasets.


PS13-A001 | Invited
Untrackable Distal Ejecta on the Moon and Terrestrial Planets

Zhiyong XIAO#+
Sun Yat-sen University

It is a conventional knowledge that impact ejecta on the Moon and terrestrial bodies follow radial distributions, and this knowledge is a basic assumption used to constructing strategraphic systems of exteresstrial bodies. Meanwhile, planetary rotations, especially on fast rotating bodies, posses significant diversions on trajectories of impact ejecta, especially those with relative high ejection speeds. Inelastic collisions of impact fragments in ejecta curtains could also cause nonradial distributions of impact ejecta. This abstract reports abrupt changes of ejection angles during impact spallation, which are caused by heterogeneous shock impedances of impactor and/or target materials. Non-radial distributions of impact ejecta are ubiquitous on the Moon and terrestrial bodies. Their products (e.g., background secondaries, non-radial rays, homeless fluidized ejecta) have significants implications on interpretations of planetary geology and age determination based on crater statistics.


PS13-A012
Omni-directional Geological Structure Revealed by the Chang'e-4 Lunar Penetrating Radar

Ling ZHANG1#+, Yi XU2, Huaqing CAO2, Jialong LAI3
1Sun Yat-sen University, 2Macau University of Science and Technology, 3Jiangxi University of Science and Technology

Since early 2019, the Lunar Penetrating Radar (LPR) onboard Chang'e-4 (CE-4)’s Yutu-2 rover has been gathering data relating to the subsurface structure of the Von Kármán crater within the South Pole-Aitken Basin (SPA) on the lunar farside. Low-frequency radar data have the potential of carrying geological information of about 300 m worth of strata below the traversed path. With the continuous progress of Yutu-2 rover, stratigraphy and more new underground structures continue to be discovered. From top to bottom,buried ejecta is overlaid by at least four layers of distinct lava flows that probably occurred during the Imbrium Epoch, with thicknesses ranging from 12m up to about 100 m, providing direct evidence of multiple lava-infilling events that occurred within the VK crater. From front to back, forty-two days’ data have revealed a bifurcated structure within the layered structure, whose origin might be linked to the deposition of ejecta from the Schrödinger impact, affecting the overlying reflectors between 90 and 310 m. The LPR results provide an important scientific basis for understanding the geological history of the far side of the Moon.


PS13-A013
Probing Surface Deposits in Balmer-Kapteyn Cryptomare Using CE-2 MRM Data

Zhiguo MENG#+, Tianqi TANG, Yongzhi WANG
Jilin University

Cyptomare records the early-stage mare volcanisms and large-scale impact cratering, which can provide important information about the thermal evolution of the Moon. In this study, we built a mixing dielectric constant model to represent the cryptomare deposits mixed by highland debris and mare deposits, and the proper radiative transfer simulation was constructed to simulate the thermal emission features of surface deposits in the cryptomare. The microwave radiometer data in the Balmer-Kapteyn region were extracted, and the linear interpolation method was used to generate brightness temperature (TB) maps at noon and at night. To enhance the correlation between cryptomare deposits and TB performances, normalized TB (nTB) and TB difference (dTB) maps were also generated. Combined with the Lunar Reconnaissance Orbiter Wide Angle Camera, Lunar Orbiter Laser Altimeter, and Diviner and Clementine UV–VIS, the main findings are as follows: (1) The mare-like cryptomare deposits were discovered and identified according to the nTB and dTB performances. Combined with the surface compositions, at least two kinds of buried mare deposits were identified in the B-K region, which erupted during different episodes. (2) A construct-like volcanic feature was suggested by the nTB and dTB performances. (3) The results of our analysis indicated the presence of materials with low dTB anomalies in the northern and southwestern parts of the cryptomare region and in the mare unit within the Vendelinus crater, which illustrates the heterogeneity of the lunar crust in the vertical direction.


PS13-A010
High-precision Subsurface Structure of China’s Tianwen-1 Landing Site at Utopia Basin, Mars

Chao LI1+, Lei ZHANG2, Jinhai ZHANG1#
1Institute of Geology and Geophysics, Chinese Academy of Sciences, 2Chinese Academy of Sciences

The Martian subsurface structure records the magmatic activity, sedimentary process, and meteorite impact history of Mars, and is a promising region to explore the geological evolution and ancient water activities of Mars. On 15 May 2021, China’s first Mars mission, Tianwen-1, successfully landed on the south of Utopia Planitia and released the Zhurong rover to in-situ detect the subsurface structure with the equipped ground penetrating radar (Rover Penetrating Radar, RoPeR). Using the low-frequency channel radar data recorded in the first 113 Sols, the high-precision radar imaging result of more than 80 m below the surface is obtained, after effective random noise attenuation and velocity inversion. According to features of the radar reflection, there shows an obvious vertical stratification structure and relatively weak lateral variation. Previous studies have mainly focused on the vertical stratification structure of the radar profile, but the weaker lateral variations have not been intensively studied. In this paper, we effectively extracted the lateral variation features of the radar profile by the time-frequency analysis method. The vertical stratification structure of the radar profile represents large-scale multi-period resurfacing events, while the lateral variation of the radar profile may represent the local dynamics process during the extensive resurfacing background, such as lateral structural differences due to meteorite impacts and mud volcanic material upwellings, which closely related to the complex dynamical evolutionary processes and water activity on Mars. According to the extracted the lateral variation, we reconstructed subsurface complex geological evolution processes in the Tianwen-1 landing site, providing an important constraint on the geological evolution and paleo-environmental changes of Mars.


PS13-A009
Heterogeneous Distribution of Martian Soil Unveiled by Ground-penetrating Radar of Zhurong Rover

Ruonan CHEN+, Yi XU#, Ling ZHANG, Renrui LIU
Macau University of Science and Technology

Much of the Martian surface is covered by a soil layer formed by various geological processes, such as impact gardening and eolian erosion, which is essential for resolving some key geological questions, including the potentiality of liquid water on the surface or near-surface. On May 15, 2021, the Zhurong Mars rover carried by China's first Tianwen-1 Mars mission successfully landed in the southern part of the Utopia Plain and began its exploration journey. Using CH2 HH (horizontal transmit and horizontal receive) polarization mode data provided by Mars Rover Penetrating Radar (RoPeR) on board the Zhurong rover, a fine radargram of subsurface soil was obtained within the depth of ~4.5 m, which does not feature noticeable continuous reflections or distinctive layered stratification. However, the distribution of local regolith is characterized by structures resembling partial or complete crater walls and near-surface impact lenses at very shallow depths, heterogeneous and geologically complex. In contrast, no well-structured craters or strongly reflective buried structures have been found in the lunar regolith in the Von Kármán crater measured by the ground-penetrating radar of the Yutu-2 rover of Chang’e-4 mission except for a couple of continuous thin ejecta layers caused by local small impact events. The close-to-surface subsurface Martian crater suggests an accelerated occultation rate for small craters on the surface of Mars as compared to the rate on the Moon, which is probably due to the eolian process burring the craters on the Martian surface and then shielded them from further erosion. The high loss tangent indicates that the regolith at the Tianwen-1 landing site is not dominated by water ice.


PS13-A007
Analyses of Water/ice-related Landforms in the Zhurong Landing Region: Implications for the Aqueous History of Southern Utopia Planitia, Mars

Jiannan ZHAO1#+, Jun HUANG2, Jiang WANG2, Long XIAO2
1China University of Geosciences, Wuhan, 2China University of Geosciences

Aqueous activities on Mars gradually declined after the Noachian period (>3.7 Ga). Nevertheless, analyzing the records of water/ice-related processes in the Hesperian and Amazonian Mars is of great significance as it is closely related to the searching of traces of martian life and the evaluation of martian habitability. In 2021, China’s Zhurong rover successfully landed on the southern Utopia Planitia to conduct in-situ investigation, and the Tianwen-1 orbiter also performed targeted observations of the landing region, which obtained high-resolution orbital and in-situ data, providing unprecedent chances for detailed study of the geomorphological features in the landing region. In this paper, we mapped a series of possible post-Noachian water/ice-related landforms in the landing region such as polygonal troughs, pitted cones, layered ejecta craters, pitted-wall craters, etc. We analyzed their morphological characteristics, stratigraphic relationships, and possible origins. On this basis, we discussed the aqueous history of the southern Utopia Planitia, and proposed that aqueous activity in the landing region may have persisted until the recent periods.


PS13-A011
First Measurements of Low-energy Cosmic Rays on the Surface of the Lunar Farside from Chang’e-4 Mission

Peng-Wei LUO1+, Xiao-Ping ZHANG1#, Shuai FU1, Yong LI1, Cun-Hui LI2, Jinbin CAO3
1Macau University of Science and Technology, 2Lanzhou Institute of Physics, 3Beihang University

Space radiation, dominated by cosmic rays (CRs), severely restricts human activities on the lunar surface. Our study presents the first measurements of low-energy CR spectra (about 10 to 100 MeV/nuc) obtained from China's Chang'E-4 (CE-4) mission around solar minimum 24/25. We find that for the proton, helium, CNO, and heavy-ion groups, the ratios of the CE-4 fluxes to those from the near-earth spacecraft are 1.05 ± 0.15, 1.30 ± 0.18, 1.08 ± 0.16, and 1.24 ± 0.21, respectively, and to those predicted by the models [CRÈME96 and CRÈME2009] are instead [1.69 ± 0.17), 2.25 ± 0.23], [1.66 ± 0.17, 1.76 ± 0.18], [1.08 ± 0.11, 1.07 ± 0.11], and [1.33 ± 0.18, 1.17 ± 0.15]. Furthermore, it is observed that the 3He/4He ratio is enhanced at ~12 MeV/nuc, and the Dawn-Dusk symmetry of CRs is confirmed. These findings provide valuable insights into the CRs on the surface of the lunar farside and will benefit future lunar exploration. (Footnote: Funded by the project "Technical support for dust characteristic analysis of Main-belt comet and load development".)



Solar and Terrestrial Sciences


Mon-31 Jul | 8:15 - 10:00 | MR308
ST02 - Upper Atmosphere and Whole Atmosphere Models for Satellite Drag and Space Weather Applications

Session Chair(s): Jiuhou LEI, University of Science and Technology of China

ST02-A023
Thermosphere Density Data, Modeling and Model Assessment

Sean BRUINSMA#+
Centre National D'Etudes Spatiales

Forecasting and modeling atmospheric drag is the main challenge when predicting current and future locations of objects in Low Earth Orbit (LEO). Atmospheric drag is proportional to the mass density and composition of the neutrals in Earth’s thermosphere, which is highly variable, both spatially and temporally, due to varying solar EUV emissions and geomagnetic activity. To improve and assess the quality of thermosphere or whole atmosphere models we need high-quality (total and partial) neutral density data that is well-distributed in space and time. The most precise observations are inferred from accelerometers on the missions CHAMP, GRACE, GOCE and GRACE-FO, but they also are affected by (systematic) errors. Other errors that contribute to the total modeling error in atmospheric drag is due to the use of solar and geomagnetic proxies, the simple and coarse modeling algorithm of semi-empirical models, errors in the satellite model, and the sparseness/errors/inconsistencies of the density data used in the model fit. This presentation will show the relation between density data, empirical thermosphere models, and model assessment.


ST02-A025
Assessment of Thermospheric Models During the Geomagnetic Storm Times in NASA/CCMC CAMEL Framework

Jack WANG1#+, Richard MULLINIX1, Jia YUE1, Sean BRUINSMA2, Chiu WIEGAND1, Tzu-Wei FANG3, Mariangel FEDRIZZI3, Eric SUTTON3, M. Leila MAYS4, Masha M. KUZNETSOVA1
1NASA Goddard Space Flight Center, 2Centre National D'Etudes Spatiales, 3University of Colorado Boulder, 4The Catholic University of America

This paper is a follow-up study after Bruinsma et al. (2021, doi: 10.1051/swsc/2021002), which assesses the performance of empirical and physics-based thermosphere models during geomagnetically storm times. Thermospheric models available at the NASA Community Coordinated Modeling Center (CCMC) are unbiasedly evaluated in this study, which include the CTIPe, DTM2013 and DTM2020, GITM, JB2008, NRLMSIS 2.0, TIE-GCM, and WACCM-X. Neutral density from model simulations during given storm event is first divided into four phases (pre-storm, main, recovery, and post-storm) with respect to the time of minimum Dst. This is followed by evaluating the model performance by comparing the model datasets to the drag-derived neutral density, including CHAMP, GOCE, and GRACE within each phase. The performance of space weather modeling during storm main and recovery phases for several selected geomagnetically storm events is presented in this talk. Metrics of the neutral density, such as mean density ratios and standard deviation, are also utilized in the Comprehensive Assessment of Models and Events using Library Tools (CAMEL) framework developed by the CCMC. Utilizing the model validation in CAMEL can facilitate the model-data comparison to users and establish access to scorecards with consistent and identical metrics, which can help users select the best models for their objective. All data stored in CAMEL are publicly accessible via APIs/webservice calls. Original data files submitted for the validation campaign are also stored in a public repository. This demonstration can pave the way for comprehensive model validation in the future that also support the open science initiative.


ST02-A024
Advancing Satellite Drag and Space Weather Capabilities with the Geospace Dynamics Constellation

Katherine GARCIA-SAGE1#, Douglas ROWLAND1+, Eric SUTTON2, Marcin PILINSKI2, Larry KEPKO3
1NASA Goddard Space Flight Center, 2University of Colorado Boulder, 3National Aeronautics and Space Administration

Set to launch around the end of the decade, the Geospace Dynamics Constellation (GDC) is a six-satellite mission to characterize the ionosphere-thermosphere system and its geomagnetic drivers from an altitude of 400 km. This mission will make unprecedented measurements of the thermospheric density, composition, and temperature at a range of temporal and spatial scales, improving our understanding of the satellite drag environment. Its measurements of ionospheric variability will greatly advance our knowledge of irregularities affecting navigation and communications systems. As a NASA Living With a Star (LWS) mission, the goal of GDC is to pursue basic research enhancing our understanding of the space weather environment. However, GDC is also well-positioned to be a pathfinder for future operational missions, with certain space weather-relevant measurements available to our operational partners in near-real-time via a low-latency space weather data stream. In this talk, we will outline the pathway to space weather applications of GDC data, as well as discuss plans for advancing satellite drag studies with a combination of in-situ thermospheric measurements and GNSS accelerometry.


ST02-A034
Heating and Cooling of the Thermosphere During Magnetic Storms: Impact on Satellite Orbital Drag and the New Geospace Dynamics Constellation Mission

Denny OLIVEIRA1,2#+, Eftyhia ZESTA1, Kevin DELANO1, Marcin PILINSKI3, Shaylah MUTSCHLER4, W. Kent TOBISKA4, Daniel GERSHMAN1, Mark MOLDWIN5
1NASA Goddard Space Flight Center, 2University of Maryland, Baltimore County, 3University of Colorado Boulder, 4Space Environment Technologies, 5University of Michigan

Magnetic storms enhance thermospheric density levels leading to increased air drag forces on low-Earth orbit (LEO) satellites, which in turn affect their acceleration resulting in altitude losses, lifetime reduction, and orbital tracking uncertainties. Many recent studies have shown that, along with thermosphere heating and its subsequent upwelling, large amounts of Nitric Oxide (NO) molecules are produced particularly during severe and extreme events. NO plays a major role in the thermosphere dynamics because it acts as a cooling agent in the thermosphere by irradiating heat back into space. We study the global thermosphere response to storms by means of superposed epoch analysis of the thermosphere mass density response based on near two decades of data from the CHAMP, and GRACE LEO satellites for the period of September 2001 to 2020. We use NO observations by the SABER instrument onboard NASA’s TIMED satellite to uncover the role NO plays in the faster cooling of more intense storms. We find that storms with the most extreme heating are the fastest to cool off during the storm recovery phase. These responses are not predicted by our current models, leading to large errors in in-track predictions of low-Earth orbit (LEO) satellites. The new Geospace Dynamics Constellation (GDC) mission, currently in Phase A, will be a constellation of 6 satellites that in different configurations during its lifetime will study the responses of the upper atmosphere to energy input from the magnetosphere as well as its subsequent internal reconfiguration processes. GDC follows and greatly enhances the CHAMP, GRACE and SWARM missions. We will briefly introduce the two selected instruments that will be providing the magnetospheric energy inputs for the GDC mission: the Comprehensive Auroral Precipitation Experiment (CAPE) and the Near Earth Magnetometer Instrument in a Small Integrated System (NEMISIS) investigations.


ST02-A028
A Data Quality Control Method for Data Assimilation of Near Space Weather

Cunying XIAO1#+, Xiaoqi WU1, Xiong HU2, Wenbin CHEN3
1Beijing Normal University, 2Chinese Academy of Sciences, 3Fudan University

Data assimilation plays an important role in the refined description and accurate forecast of near space weather. Data is introduced and used by data assimilation in a manner of "observational increment". Due to the limitation of detection principle, observation conditions, inversion algorithm and other conditions, the observations inevitably have outliers, so the quality control of the observation data must be carried out before assimilation. The double weight method is used to identify outlier data of TIMED/SABER in this study. In this method, threshold criteria are used to determine the abnormal data quantity, that is, the amount of data to be eliminated in the quality control part of the assimilation process. In order to make the remaining data used in the assimilation process closer to the normal distribution in frequency distribution, have a small vertical correlation of errors, and the covariance matrix of which is close to the diagonal matrix, the selection of threshold is very important. The method of step-by-step iteration is adopted to determine the threshold. These processes can provide high quality observation data for the subsequent assimilations.


ST02-A001
Prediction of the Ionospheric Sporadic E Layer Based on GNSS Radio Occultation Data

Bingkun YU1#+, Xianghui XUE2, Xinan YUE3, Xiankang DOU4
1Deep Space Exploration Laboratory, 2University of Science and Technology of China, 3Chinese Academy of Sciences, 4Wuhan University

The intense plasma irregularities within the ionospheric sporadic E (Es) layers at 90–130 km height have a great impact on radio communications and navigation systems. Prediction of the Es layer is very important for the accuracy and reliability of global navigation satellite system. We have constructed an empirical model of the Es layer based on COSMIC radio occultation measurements in the period 2006-2014. The model can provide the climatology of the intensity of Es layers as a function of altitude, latitude, longitude, universal time, and day of year. The correlation coefficients of the hourly foEs and the daily maximum foEs between the ground-based ionosonde observations and model outputs at Beijing are 0.52 and 0.68, respectively. The model prediction of the Es layer can be implemented in comprehensive models for a description of the Es layer and provide morphology of the global Es layer.


Mon-31 Jul | 8:15 - 10:00 | MR311
ST07 - Coupling Between Inner-magnetospheric, Ionospheric and Thermospheric Particle Populations

Session Chair(s): Chao YUE, Peking University, Dedong WANG, GFZ German Research Centre for Geosciences

ST07-A006 | Invited
Ionospheric Oxygen Outflows Directly Injected Into the Inner Magnetosphere

Qiugang ZONG#+
Peking University

Ionospheric oxygen outflows (IOOs) are frequently observed in Earth's inner magnetosphere. As a potential fast mass source of the inner magnetosphere, they have been extensively studied for decades. In this study, we identified 271 IOO events from 6-year Van Allen Probes (VAPs) data and conducted a statistical study to reveal when, where, and how they occur. All the events are observed in the nightside magnetosphere, with the occurrence rate peaking at the L-shells corresponding to the auroral oval. The spatial scale of IOOs in the equatorial plane is estimated from the two-spacecraft configuration of the VAP mission. The results show that, in statistics, IOOs are 3.9-hr wide in magnetic local time and 1.0-Earth radius wide in L-shell. Further investigation shows that IOOs would shift to lower L-shells and occupy a larger L-shell extent as the AE index increases. Analysis of the environment conditions reveals that IOOs are statistically associated with AE-index enhancements, ultra-low-frequency (ULF) waves, and magnetic field dipolarization, but not with any systematic variations in the SYM-H index and the solar wind parameters. From this observation, we suggest that geomagnetic substorms and substorm-associated processes (e.g., ULF waves) are potential triggers of inner-magnetosphere IOOs.


ST07-A005 | Invited
The Controversial Role of Ionospheric Ions in the Dynamics of the Inner Magnetosphere

Elena KRONBERG#+
University of Munich

During geomagnetic storms, ionospheric ions can dominate the plasma pressure in the ring current. The increased plasma pressure may alter the strength of geomagnetic storms, leading to stronger disturbances. Strong pressure gradients enhance field-aligned currents, which in turn trigger even more ionospheric outflow via changing conductance in the ionosphere. Therefore, the coupling between ionosphere, magnetosphere and ring current creates a self-amplifying process which further increases the ring current. On the other hand, the increased plasma pressure may stretch the geomagnetic field. This reduces access of the warm plasma population to the ring current and as a consequence make it weaker. Additionally, ionospheric ions affect the properties of waves, the charge exchange rate and Coulomb interactions with the thermal plasmasphere, non-linearly changing the properties of the ring current. The complexity of the role of ionospheric ions will be reviewed.


ST07-A002
Ionospheric Electron Density Modulation Caused by EMIC Wave-driven Proton Precipitation

Yiqun YU#+
Beihang University

Energetic protons of tens of keV can be pitch angle scattered by electromagnetic ion cyclotron (EMIC) waves excited in the magnetosphere, resulting in loss cone proton precipitation down to the upper atmosphere and proton aurora. The ionosphere could therefore experience disturbances following the deposited energy from the space. Previous studies have reported field-of-view integrated disturbances in the ionosphere, but no direct evidence on height-dependent response has been shown. Using simultaneous space-borne and ground-based measurements, we report for the first time height-dependent disturbances in the ionosphere in response to isolated proton aurora (IPA), driven by EMIC wave-associated proton precipitation. On March 06, 2019, the Polar Orbiting Environmental Satellites (POES) observed significant proton precipitation in the dusk sector (MLT~19), while ground-based magnetometers detected a clear signature of EMIC waves. Meanwhile, an IPA was detected by the all sky imager at the conjugated location, and the nearby Poker Flat incoherent scatter radar (PFISR) showed enhanced electron density in the E region. These observations suggested a potential consequence of the EMIC wave-driven proton precipitation in the magnetosphere-ionosphere system. We further verified the ionospheric responses with the Global Airglow (GLOW) model. By fitting the observed precipitating fluxes of both electrons and protons assuming Maxwellican distribution shapes, we obtained the precipitating flux spectra as the model inputs. Simulation results showed a good agreement with PFISR observations on the electron density profiles when the proton precipitation is taken into account, suggesting that the proton precipitation is the major cause to the E region disturbances. This study confirmed physical links from the magnetosphere to the ionosphere through EMIC-driven proton precipitation.


ST07-A008 | Invited
Patterns of Energetic Electron Precipitation in Earth’s Radiation Belts: Overview of ELFIN Observations

Xiao-Jia ZHANG1#+, Anton ARTEMYEV2, Vassilis ANGELOPOULOS2
1The University of Texas at Dallas, 2University of California, Los Angeles

Energetic electron precipitation due to wave-particle resonant interactions is their main loss mechanism from the Earth's outer radiation belt. In this presentation, we will review various patterns of such precipitation events as revealed by recent observations of ELFIN CubeSats, including: sub-relativistic electron precipitation due to nonlinear Landau resonance with very oblique whistler-mode waves, relativistic microburst precipitation due to cyclotron resonance with field-aligned ducted whistler-mode waves, relativistic and ultra-relativistic electron precipitation due to resonant scattering by electromagnetic ion cyclotron waves, and quasi-periodic electron precipitation driven by whistler-mode waves that are modulated by compressional ultra-low-frequency waves. We will also briefly discuss other precipitation patterns and open questions in modeling wave-particle resonant interactions.


ST07-A003 | Invited
Unique Banded Structures of Plasmaspheric Hiss Waves in the Earth’s Magnetosphere

Binbin NI1#+, Danny SUMMERS2, Zheng XIANG1, Xiankang DOU1, Bruce TSURUTANI3, Nigel MEREDITH4, Junhu DONG1, Lunjin CHEN5, Geoff REEVES6, Xu LIU5, Xin TAO7, Xudong GU1, Xin MA1, Juan YI1, Fu SONG1, Wei XU1
1Wuhan University, 2Memorial University of Newfoundland, 3Jet Propulsion Laboratory, California Institute of Technology, 4British Antarctic Survey, 5The University of Texas at Dallas, 6Los Alamos National Laboratory, 7University of Science and Technology of China

Plasmaspheric hiss is an electromagnetic wave mode that occurs ubiquitously in the high-density plasmasphere and contributes crucially to the dynamic behavior of the Earth’s Van Allen radiation belts. While plasmaspheric hiss is commonly considered to be a broadband emission with frequencies from ∼100 Hz to several kHz, here we report Van Allen Probes measurements of unambiguous banded signatures of plasmaspheric hiss, uniquely characterized by an upper band above ∼200 Hz, a lower band below ∼100 Hz and a power gap in between. In statistics, banded plasmaspheric hiss occurs with the probability ~8% in the postnoon sector within 2.5-5.0 Earth radii, showing strong dependence on geomagnetic and solar wind conditions. Based upon observations, this talk will also discuss the possible mechanism(s) that may account for the formation of banded hiss waves.


ST07-A007
Dependence of ECH Wave-induced Electron Scattering Rates on the Hot Plasma Temperature

Katja STOLL1,2#+, Leonie PICK1, Dedong WANG3, Yuri SHPRITS3, Xing CAO4, Binbin NI4
1DLR Institute for Solar-Terrestrial Physics, 2University of Potsdam, 3GFZ German Research Centre for Geosciences, 4Wuhan University

Resonant wave-particle interactions in the Earth’s magnetosphere can lead to the scattering of plasma sheet electrons into the atmospheric loss cone, which can consequently cause the optical phenomenon of diffuse aurora. The Earth’s diffuse auroral precipitation poses the main source of energy input into the high-latitude nightside upper atmosphere and therefore provides a strong coupling mechanism between the magnetosphere and the ionosphere. Specifically, electrostatic electron cyclotron harmonic (ECH) waves can effectively precipitate low-energy (100s of eV to 10s of keV) electrons into the upper atmosphere and contribute to the formation of diffuse aurora. In order to describe the ECH wave-induced electron scattering process, bounce-averaged quasi-linear diffusion coefficients need to be calculated. As ECH waves are thought to be generated by the loss cone instability of the ambient hot electron distribution, the numerical calculation of ECH wave-induced scattering rates requires the specification of the wave propagation characteristics, the background magnetic field and plasma density as well as properties of the hot plasma sheet electrons responsible for the wave excitation. In this study, we analyze the dependence of the bounce-averaged quasi-linear scattering rates by ECH waves on the temperature of the hot electron components in the electron distribution. By assuming the background plasma parameters based on previous observations, scattering rates are computed for hot electron temperatures varying from hundreds of eV to several keV, which is consistent with observations as well. A wave power spectral profile based on statistical wave properties is assumed and used to calculate weighted diffusion coefficients. We find that the hot electron temperature influences the growth rate and wave normal angle of the waves, changing the magnitude of the diffusion coefficients over a large range of pitch angles and energies. This also changes the lifetimes of the electrons near the loss cone.


Mon-31 Jul | 8:15 - 10:00 | MR328
ST18 - Prediction of Space Weather Events Using Both Physics-based Methods and Machine Learning Techniques

Session Chair(s): Fang SHEN, Chinese Academy of Sciences

ST18-A001 | Invited
Next Generation Space Weather Modeling Framework with Uncertainty Quantification and Data Assimilation

Gabor TOTH#+
University of Michigan

Supported by the Space Weather with Quantified Uncertainty (SWQU) NSF program, we are developing the Next Generation Space Weather Modeling Framework at the University of Michigan to provide useful probabilistic forecast of major space weather events about 24 hours before the geospace impact occurs. We are using the Space Weather Modeling Framework in combination with uncertainty quantification and data assimilation. Using the advanced MaxPro experimental design, we have performed about a thousand simulations with our solar corona and heliosphere model generating steady state solar wind solutions and coronal mass ejections. The uncertainty quantification analysis shows that the physically meaningful ranges of the background solar wind model parameters depend on the solar cycle. We have identified the four most important parameters that impact the background solar wind and the CME eruption model. The reduced dimensionality of the parameter space enables reducing the size of the ensemble. Data assimilation provides further opportunity to improve the predictions. We are using in-situ observations at L1 prior to the CME and coronal while-light image observations right after the eruption to find the optimal parameters for the ensemble simulations. The CME arrival time error is very well correlated to the white light image comparisons providing a path to improved CME arrival time forecast. To make the ensemble simulations feasible, the model should take advantage of GPUs. We have already ported the Geospace model to run efficiently on a GPU. The operational Geospace model can run on a single GPU significantly faster than real time at the same speed as using about 100 CPU cores. We are currently porting the solar corona and heliosphere model to multiple GPUs. The main product of the project, the Michigan Sun-to-Earth Model with Quantified Uncertainty and Data Assimilation (MSTEM-QUDA) is available as an open-source distribution at https://github.com/MSTEM-QUDA to the entire community.


ST18-A018
Geospace System Response to an Extreme Solar Flare

Jing LIU#+
Shandong University

The Earth’s magnetosphere is the outermost layer of the geospace system deflecting energetic charged particles from the Sun and solar wind. The solar wind has major impacts on the Earth’s magnetosphere, but it is unclear whether the same holds for solar flares—a sudden eruption of electromagnetic radiation on the Sun. Here we use a recently developed whole geospace model combined with observational data from the 6 September 2017 X9.3 solar flare event to reveal solar flare effects on magnetospheric dynamics and on the electrodynamic coupling between the magnetosphere and its adjacent ionosphere, the ionized part of Earth’s upper atmosphere. We observe a rapid and large increase in flare-induced photoionization of the polar ionospheric E-region at altitudes between 90 km and 150 km. This reduces the efficiency of mechanical energy conversion in the dayside solar wind–magnetosphere interaction, resulting in less Joule heating of the Earth’s upper atmosphere, a reconfiguration of magnetosphere convection, as well as changes in dayside and nightside auroral precipitation. This work thus demonstrates that solar flare effects extend throughout the geospace via electrodynamic coupling, and are not limited—as previously believed—to the atmospheric region where radiation energy is absorbed .


ST18-A008
A Method of Qualitative Post-diction and Prediction of Grand Solar Minimum in the History and the Future

Limei YAN1+, Jiansen HE2, Yong WEI1#, Fei HE1, Xinan YUE3, Hui TIAN2, Kai FAN1, Yuqi WANG3
1Institute of Geology and Geophysics, Chinese Academy of Sciences, 2Peking University, 3Chinese Academy of Sciences

The grand solar minimum is a particular state of the Sun when solar activity is highly depressed and potentially affects the Earth’s climate. The continuous weakening of solar activity since solar cycle 22 raises considerable concern about whether the Sun is entering a new grand solar minimum. Here, based on the group sunspot number since 1700, a relatively regular varying component of solar activity is extracted to conduct “post-diction” and prediction. The “post-diction” through backward extrapolation from 1000 BCE to 1700 CE is successful. The prediction suggests that solar activity will probably enter a new grand minimum centered around 2053 CE.


ST18-A003
Warning and Tracking of CMEs Based on Machine Learning Techniques

Yi YANG1#+, Fang SHEN2
1National Space Science Center, Chinese Academy of Sciences, 2Chinese Academy of Sciences

Coronal mass ejections (CMEs) are one of the most violent explosive events from the Sun. When reaching the Earth, CMEs can cause large geomagnetic storms, bring disastrous effects on human society and cause huge economic losses. Therefore, it is of great significance to give early warning of CME and to track its propagation. We use an advanced machine learning method based on convolutional neural network (CNN) to automatically detect whether there is a CME in the coronagraph image, and realize the accurate warning of CME. By identifying and tracking a CME from a time series of coronagraph images, physical parameters such as velocity and angular width of the CME can be obtained. In the future, the propagation process of CME events can be simulated and predicted by combining the automatic detection method with a CME propagation model.


ST18-A013
Statistical Models for Solar Flare Predictions

Yang CHEN#+
University of Michigan

We present novel statistical methods towards early forecasting of solar flare events, and compare them with machine learning approaches that we have adopted in our previous work. The data sources that we use include: Geostationary Operational Environmental Satellites (GOES), Solar Dynamics Observatory (SDO)/Helioseismic and Magnetic Imager (HMI) and SDO/Atmospheric Imaging Assembly (AIA). The results that I will show in the talk include: (1) strong and weak flare classification with spatial statistics features, together with SHARP and topological parameters; (2) active region based solar flare intensity prediction with mixed LSTM regression; and (3) tensor Gaussian process contraction model for solar flare forecasting combining data of various types and sources (SHARP parameters, HMI and AIA images).


Mon-31 Jul | 8:15 - 10:00 | MR329
ST11 - The Formation, Evolution, Geoeffectiveness, and Prediction of Southward Magnetic Fields.

Session Chair(s): Chenglong SHEN, University of Science and Technology of China, Jiajia LIU, University of Science and Technology of China

ST11-A001
Multipoint Interplanetary Coronal Mass Ejections Observed with BepiColombo, Tianwen-1 and MAVEN

Yutian CHI1#+, Chenglong SHEN2, Junyan LIU2, Yuming WANG2, Mengjiao XU2, Bingkun YU1, Dongwei MAO2, Zhihui ZHONG2, Zhiyong ZHANG2
1Deep Space Exploration Laboratory, 2University of Science and Technology of China

We present the first two multi-points interplanetary coronal mass ejections (ICMEs) detected by Tianwen-1 and MAVEN spacecraft near the Mars and Bepicolombo spacecraft in December 5 to 31, 2021. Due to the lack of the heliospheric observations, we use the Heliospheric Upwind eXtrapolation time model to connect the multiple in-situ observations and the coronagraphs observations from STEREO/SECCHI and SOHO/LASCO. The first fast CME event (∼761.2 kms−1), which erupted on December 4, collided with the Mars centrally and grazed the Bepicolombo by its western flank. The west flank of the CME was decelerated by the ambient slow solar wind, and it confirmed that the CME event can be strongly distorted by the ambient structured solar wind. The second slow CME event (∼390.7 km/s) undergo an acceleration from its eruption to somewhere within the 0.69 AU and then travels with constant velocity in the ambient solar wind level. These findings indicate the importance of background solar wind in determining the interplanetary evolution and global morphology of CMEs. The observations from multiple locations are a treasure trove for space-weather studies and merit more exploration in the future.


ST11-A007
Multipoint Interplanetary Shocks Observed at Venus and Earth

Can WANG#+, Chenglong SHEN, Mengjiao XU, Zhihui ZHONG, Dongwei MAO
University of Science and Technology of China

Interplanetary (IP) shock is a disturbance that propagates into the interplanetary medium as a consequence of the speed difference between the medium and the structure, they are often associated with space weather phenomena such as Interplanetary Coronal Mass Ejections (ICMEs) and Co-rotating Interaction Regions (CIRs). We present comprehensive surveys of 143 IP shocks during 2006-2014 using Venus Express high-resolution magnetic field data at 0.72 AU, and examine shock occurrence and their parameter characteristics as they evolve through the heliosphere. We propose a statistical analysis to investigate the shock and driver properties near Venusian orbit. The shock occurrence near Venus shows a correlated variation with solar activities as measured by the sunspot number, while shock angle θBn and magnetic compression ratio do not show such correspondence. The average shock angle at 0.72 AU is about 46º, the magnetic compression ratio is peaked in the range from 2.0 to 2.25, with a mean value of 2.1. Comparison with previous observational results at 1 AU, it is noted that shock strength seems to decrease from 0.72 AU to 1 AU, and shock angle θBn become more perpendicular as they move outward in the heliosphere. As IP shocks propagate radially from the Sun, shock properties may evolve significantly. We further consider multispacecraft observation of IP shocks at Venus and Earth while radially aligned. Using STEREO/SECCHI COR, heliospheric imager (HI) data and in situ observations from multiple vantage points, an IP shock on 18 March 2011 was detailed analyzed to study shock strength increase from 0.72 AU to 1 AU, the speed profile shows that the shock accelerates during its propagation, which may relate to the shock strength enhancement.


ST11-A008 | Invited
Conditions That Determine the Initial Turnings of Interplanetary Magnetic Field Behind the Interplanetary Shock

Chin-Chun WU1#+, Kan LIOU2
1Naval research laboratory, 2Johns Hopkins University Applied Physics Laboratory

Geomagnetic storms are one of the most important space weather events. A severe storm can damage costly space vehicles, interrupt telecommunication causing air traffic jam, and harm the health of astronauts working in space. Previous studies have suggested that most severe storms are usually associated with an interplanetary (IP) shock driven by coronal mass ejections. In addition, a large southward field immediately downstream of the shock can lead to a two step storm when the shock driven cloud also contains a large southward field. Therefore, predicting the sign of IMF in the leading part of the sheath (e.g., IMF initial turnings) plays a key role in space weather forecasting. In this study we analyze CME events that occurred from 1994 to 2014 to seek conditions that control IMF initial turnings (either southward or northward). It is found that IMF initial turning direction can be organized by the source location of CMEs and the orientation of IMF upstream of the shock. We will present our statistical result and provide an explanation for this finding.


ST11-A004 | Invited
How Solar Wind Controls the Recovery Phase Morphology of Intense Magnetic Storms

Hui LI1#+, Xiaodong LIU2, Chi WANG2
1National Space Science Center, Chinese Academy of Sciences, 2Chinese Academy of Sciences

Geomagnetic storms are critical phenomena due to the solar wind and magnetosphere interaction. Most studies focus on the main phase of magnetic storms, leaving the morphology of the recovery phase still an open question. In this study, we conducted a statistical survey of 85 isolated intense magnetic storms from 1995-2018 and obtained the characteristics of recovery phase morphology. All magnetic storms can be classified into two categories, i.e., one-stage recovery with a single fast exponential recovery, two-stage recovery with a rapid exponential recovery in the first stage, and a slow linear recovery in the second stage. The two-stage recovery storms are dominant, with a proportion of ~ 60%. Meanwhile, the two-stage recovery storms tend to be accompanied by Alfven fluctuations with long-duration and intense southward interplanetary magnetic fields. Furthermore, for the second stage of recovery, the decay rate of the Dst index correlates with the amplitude of the south magnetic field when the solar wind has a high degree of Alfvenicity.


Mon-31 Jul | 10:20 - 12:20 | MR308
ST02 - Upper Atmosphere and Whole Atmosphere Models for Satellite Drag and Space Weather Applications

Session Chair(s): Jiuhou LEI, University of Science and Technology of China, Sean BRUINSMA, Centre National D'Etudes Spatiales

ST02-A013 | Invited
Impacts of Thermospheric Variations on Low Earth Orbit Satellites

Hitoshi FUJIWARA1#+, Yasunobu MIYOSHI2, Ryuho KATAOKA3, Daikou SHIOTA4, Hidekatsu JIN4, Chihiro TAO4, Hiroyuki SHINAGAWA4
1Seikei University, 2Kyushu University, 3National Institute of Polar Research, 4National Institute of Information and Communications Technology

Since the launch of the Sputnik satellite in 1957, 14,816 space objects have been registered in the Outer Space Object Index (https://www.unoosa.org/oosa/osoindex/ search-ng.jspx) of the United Nations Office for Outer Space Affairs (as of January 2023). In recent years, the number of satellite launches has increased rapidly. In particular, the number of Low Earth Orbit (LEO) and small satellites is increasing. Demand for the LEO satellites is expected to grow significantly in the future (e.g., satellite communication business) due to the significant reduction in satellite costs and the global coverage by satellite constellation. Problems have also been found in the operation of these satellites. For example, the Starlink satellite accident in February 2022 was an important lesson for future satellite operations. Dang et al. (2022) and Kataoka et al. (2022) reported the space weather effects on the Starlink satellites during 3-4 February 2022 geomagnetic disturbances caused by the solar CME arrival at the Earth. They suggested that the thermospheric mass density enhancements (> 50 %) affected the satellites at 210 km altitude through the large atmospheric drag. In this presentation, we will discuss contributions of space weather modeling studies on civil life and industry. In particular, we have developed the whole atmosphere-ionosphere model, GAIA. In addition to ionospheric variation prediction by using GAIA (Tao et al., 2020), we will discuss the usefulness of GAIA in satellite operations.


ST02-A027 | Invited
Scientific and Operational Advances in the Space Weather Prediction Center's Whole Atmosphere Model

Adam KUBARYK1,2#+, Tzu-Wei FANG1, Tim FULLER-ROWELL1, Zhuxiao LI1, George MILLWARD1
1University of Colorado Boulder, 2NOAA Space Weather Prediction Center

The Whole Atmosphere Model-Ionosphere Plasmasphere Electrodynamics (WAM-IPE) Forecast System (WFS) is an operational model at the National Centers for Environmental Prediction (NCEP), developed at the NOAA/NWS Space Weather Prediction Center (SWPC). The neutral atmosphere component, WAM, provides both a realtime nowcast and up to two-days-in-advance forecast specification of neutral density up to 400-600km. Recent increases of solar activity through solar cycle 25 have highlighted the significant impacts space weather can have on satellites operating in Low-Earth Orbit (LEO). A recent operational upgrade to WFS demonstrates advances in seasonal bias correction as well as significant improvements to the timeliness of data availability, both of which aim to enhance SWPC's ability to provide satellite operators at LEO with actionable information. Additionally, planned future advances in operational capabilities will be highlighted, including recent work toward a Unified Forecast System (UFS)-based nonhydrostatic Finite Volume Cubed Sphere (FV3)WAM.


ST02-A026
Thermospheric Neutral Density Variation During the SpaceX Storm: Implications from Physics-based Whole Geospace Modeling

Dong LIN1#+, Wenbin WANG1, Katherine GARCIA-SAGE2, Jia YUE2, Viacheslav MERKIN3, Joseph MCINERNEY4, Kevin PHAM1, Kareem SORATHIA3, Michael WILTBERGER1
1National Center for Atmospheric Research, 2NASA Goddard Space Flight Center, 3Johns Hopkins University Applied Physics Laboratory, 4University Corporation for Atmospheric Research

On 3 February 2022, following a launch of 49 satellites, 38 of the satellites were lost before they fully arrived in their designated orbits. The loss was attributed to two moderate geomagnetic storms that occurred consecutively on February 3-4. We investigate the thermospheric neutral mass density variation during these storms with the Multiscale Atmosphere-Geospace Environment (MAGE) model, a first-principles, fully coupled geospace model. Simulated neutral density enhancements are validated by Swarm satellite measurements at the altitude of 400-500 km. Comparison with standalone TIEGCM and empirical NRLMSIS 2.0 and DTM-2012 models suggests better performance by MAGE in predicting the maximum density enhancement and resolving the gradual recovery process. Along the Starlink satellite orbit in the middle thermosphere (~200 km altitude), MAGE predicts up to 150% density enhancement near the second storm peak while standalone TIEGCM, NRLMSIS 2.0 and DTM-2012 suggest only ~50% increase. MAGE also suggests altitudinal, longitudinal, and latitudinal variability of storm-time percentage density enhancement due to height dependent Joule heating deposition per unit mass, thermospheric circulation changes, and travelling atmospheric disturbances. This study demonstrates that a moderate storm can cause substantial density enhancement in the middle thermosphere. Thermospheric mass density strongly depends on the strength, timing, and location of high-latitude energy input, which cannot be fully reproduced with empirical models. A physics-based, fully coupled geospace model that can accurately resolve the high-latitude energy input and its variability is critical to modeling the dynamic response of thermospheric neutral density during storm time.


ST02-A002
Contribution of the Lower Atmosphere to the Day-to-day Variation of Thermospheric Density

Jia YUE1#+, Wandi YU2, Nicholas PEDATELLA3, Sean BRUINSMA4, Ningchao WANG5, Huixin LIU6
1NASA Goddard Space Flight Center, 2Hampton University, 3National Center for Atmospheric Research, 4Centre National D'Etudes Spatiales, 5NASA Langley Science Center, 6Kyushu University

In this paper we carried out a numerical experiment using the Specified Dynamics mode of the Whole Atmosphere Community Climate Model with thermosphere and ionosphere eXtension (SD-WACCM-X). One SD-WACCM-X run was with realistic Kp and F10.7 and the other with constant Kp and F10.7. By comparing the day-to-day variability of thermosphere mass density at 300 km (low earth orbit, LEO) and 120 km (reentry level) in these two runs, we find that the density variation at 300 km is mainly driven by geomagnetic and solar forcing while at 120 km it is exclusively controlled by the lower atmosphere. At LEO altitudes, during solar minimum and geomagnetic quiet days, the impact from the lower atmosphere is much smaller than the effect of solar and geomagnetic variations but is not negligible (5–10% vs 20%).


ST02-A016 | Invited
The Impacts of the Solar Eclipse and Volcanic Eruption on the Thermosphere

Ruoxi LI1#+, Juergen KUSCHE2, Shunrong ZHANG3
1University of Science and Technology of China, 2University of Bonn, 3Massachusetts Institute of Technology

In this presentation, the solar eclipse and Tonga volcanic eruption effects on the thermosphere are reported on the basis of the retrieved neutral densities from satellite Precise Orbit Determination (POD) data and accelerometer data. The eclipse could not only induce significant density depletion in the moon-shadow region but also generate large-scale TADs propagating globally. Meanwhile, the Tonga eruption on 15 Jan. 2022 caused dramatic thermospheric disturbances and the associated thermospheric density waves at ~500 km altitudes, which propagate concentrically and globally.


ST02-A017
Observation and Simulation of Neutral Air Density in Middle Atmosphere During the SSWs

Junfeng YANG#+
Chinese Academy of Sciences

The sudden stratospheric warming (SSW) is a dramatic event in the winter stratosphere, during which the stratospheric temperature rapidly increases and the zonal winds reverse over the Poles. The variation of the neutral air density in the middle atmosphere during the major sudden stratospheric warmings is investigated, using the observations from Microwave Limb Sounder (MLS), the Global Navigation Satellite System (GNSS) Occultation Sounder (GNOS) on board the Chinese FengYun 3 (FY-3) and the Solar Occultation for Ice Experiment (SOFIE). A rapid increase of neutral air density over high latitudes around the SSW onset date is observed. The positive anomaly of density covered the latitudes from ~60°N to the North Pole and got bigger as latitude increasing. The temporal evolutions and horizontal distributions of density were generally consistent with pressure in temporal-spatial structure. The simulation by the Whole Atmosphere Community Climate Model (WACCM) agrees well with the observation. The simulation shows that the evolution of density is attributed to the air mass transport, which is dominated by the residual meridional circulation. In addition, according to the geostrophic wind principle, the wind is controlled by the polar vortex. It is demonstrated distinctly that there is a negative correlation between the zonal mean zonal wind and the pressure anomaly in the simulation.


ST02-A031
Self-consistent Global Transport of Metallic Ions with WACCM-X

Jianfei WU#+
University of Science and Technology of China

The NCAR Whole Atmosphere Community Climate Model with thermosphere and ionosphere eXtension (WACCM-X) v2.1 has been extended to include the neutral and ion–molecule chemistry and dynamics of three metals (Mg, Na, and Fe), which are injected into the upper mesosphere–lower thermosphere by meteoric ablation. Here we focus on the self-consistent electrodynamical transport of metallic ions in both the E and F regions. The model with full ion transport significantly improves the simulation of global distribution and seasonal variations of Mg+, although the peak density is slightly lower (about 35 % lower in peak density) compared with the SCIAMACHY measurements. Near the magnetic equator, the diurnal variation in upward and downward transport of Mg+ is generally consistent with the “ionosphere fountain effect”. The thermospheric distribution of Fe is shown to be closely coupled to the transport of Fe+. The effect of ion mass on ion transport is also examined: the lighter ions (Mg+ and Na+) are transported above 150 km more easily than the heavy Fe+. We also examine the impact of the transport of major molecular ions, NO+ and O+2, on the distribution of metallic ions.


Mon-31 Jul | 10:20 - 12:20 | MR311
ST07 - Coupling Between Inner-magnetospheric, Ionospheric and Thermospheric Particle Populations

Session Chair(s): Dedong WANG, GFZ German Research Centre for Geosciences, Chao YUE, Peking University

ST07-A004
A Statistical Model of Plasmaspheric Electron Density Based on the Van Allen Probes Observations

Xiao-Xin ZHANG1#+, Jingtian LV2, Fei HE3, Ruilin LIN4
1National Center for Space Weather, China Meteorological Administration, 2China Meteorological Administration, 3Institute of Geology and Geophysics, Chinese Academy of Sciences, 4Chinese Academy of Sciences

As an important part of the inner magnetosphere, the Earth's plasmasphere plays a very important role in the link of the occurrence and development of each space weather process. The spatial distribution temporal evolution of the electron density in the plasmasphere is key to understand other physical processes in the inner magnetosphere. Based on electron density observations from September 2012 to July 2019 by the Van Allen Probes (VAP) spacecraft, we compiled a new empirical model of plasmaspheric electron density in the MEP associated with geomagnetic conditions. The statistical results show that the plasmaspheric electron density in the MEP has an obvious Magnetic Local Time (MLT) dependence. With the increase of Kp index, the asymmetrical distribution of plasmaspheric electron density in the MEP increases. The distribution of plasmaspheric electron density in the low L-value (L is shell parameter) region (L = 1.6 - 2.0) is less affected by the geomagnetic activity than that in the high L-value region (L ≥ 3.6). Comparison between the model output and the VAP’s observations indicates that this model could accurately describe the dynamic distribution characteristics of plasmaspheric electron density in the MEP during magnetic storms, such as erosion and refilling. This statistical model is convenient for operational space weather forecast and can potentially be embedded into global space weather forecast models. Combined with field-aligned model, the total electron content in the ionosphere-plasmasphere system can be obtained to characterize the radio wave propagation environment more accurately.


ST07-A018
Second‐harmonic Generation of EMIC Waves in the Inner Magnetosphere

Zuxiang XUE+, Zhigang YUAN#, Xiongdong YU
Wuhan University

Observations of non-linear second harmonic (SH) in various waves have recently been reported by several studies. However, the quantitative relation of the amplitudes between the fundamental wave (FW) and the SH has not been derived and verified yet. In this study, the quantitative relation of the amplitudes between FW and SH of the electromagnetic ion cyclotron (EMIC) wave is theoretically derived and verified through 1-D hybrid simulations. The quantitative influences of the fundamental wave frequency and wave normal angle on the SH excitation mechanism in an electron-H+ plasma are obtained. We further provide detailed analyses of EMIC wave cross-band SH generation in a multi-ion plasma. The SH can be generated around or even exactly on the normal modes of the plasma system, leading to a more efficient energy transfer than that in H+-only plasmas. The detailed parametric analysis manifests the vital role of heavy ions in promoting SH’s amplitude.


ST07-A015
Magnetospheric Multiscale Satellite Observations of Ions Jetting by Accelerating Slow Electron Holes

Yue DONG+, Zhigang YUAN#
Wuhan University

Electrostatic solitary waves (ESWs) are ubiquitous in collisionless space plasmas and are manifestations of strongly nonlinear processes. Some of these are interpreted as electron holes (EHs). In the recent study of plasma electron hole kinematics, hole acceleration or growth can cause momentum changes of an ion stream of specified velocity. Furthermore, the local ion velocity distribution affects hole velocity and stability. However, there have been few satellite observations of EH self-acceleration or EH-ion interactions. In this report, four slow electron holes (EHs) are observed by the Magnetospheric Multiscale (MMS) spacecraft in the Earth’s magnetotail. We have obtained for the first time the acceleration of structures (slow EHs) using MMS multi-satellite observations. In combination with the recent theory of plasma electron hole kinematics, the velocity distribution changes of ions before and after passing through the electron hole are close to the theoretical calculation results, which indicates that the electron holes in the accelerated state have a certain acceleration effect on the passed ions. On the other hand, ion accumulation is observed between the two separated slow EHs, and these ions are trapped by constant reflection between positive potentials. The trapped ions have parallel drift velocities comparable to that of the slow EHs. The advantages of MMS satellite's high resolution and short separation distance are fully utilized when studying small-scale structures in the space plasmas, such as EHs. We propose a method to obtain structures acceleration using multi-satellite observations and provide the direct observations of ions trapped by separated electron holes and ions jetting by holes acceleration, respectively.


ST07-A022 | Invited
Electron-only Reconnection as a Transition from Quiet Current Sheet to Standard Reconnection in the Magnetotail

San LU#+, Quanming LU, Rongsheng WANG
University of Science and Technology of China

Standard magnetic reconnection couples with both electron- and ion dynamics. Recently, a new type of magnetic reconnection, electron-only reconnection without the coupling of ion dynamics, has been observed in space. Using a two-dimensional particle-in-cell simulation, we show that in the externally-driven magnetotail, electron-only reconnection is a transition from quiet current sheet to standard reconnection. We find that (1) energy conversion j*E' is around zero in quiet current sheet but nonzero in electron-only reconnection, and (2) ion temperature does not change across electron-only reconnection but peaks at the center of standard reconnection. These two differences can be used as criteria to distinguish magnetotail electron-only reconnection from quiet current sheet and standard reconnection, respectively. Based on the two criteria, we justify that the MMS 17 June 2017 event is a magnetotail electron-only reconnection event.


ST07-A021
Electron Heating In Magnetosheath Turbulence: Dominant Role of the Parallel Electric Field Within Coherent Structures

Qianyun XU1+, Meng ZHOU1,2#, Wenqing MA1, Jiansen HE3, Shiyong HUANG4, Zhihong ZHONG1, Ye PANG1, Xiaohua DENG4
1Nanchang University, 2University of California, Los Angeles, 3Peking University, 4Wuhan University

How particles are being energized by turbulent electromagnetic fields is an outstanding question in plasma physics and astrophysics. This paper investigates the electron acceleration mechanism in strong turbulence (δB/B0 ~ 1) in the Earth’s magnetosheath based on the novel observations of the Magnetospheric Multiscale (MMS) mission. We find that electrons are magnetized in turbulent fields for the majority of the time. By directly calculating the electron acceleration rate from Fermi, betatron mechanism, and parallel electric field, it is found that electrons are primarily accelerated by the parallel electric field within coherent structures. Moreover, the acceleration rate by parallel electric fields increases as the spatial scale reduces, with the most intense acceleration occurring over about one ion inertial length. This study is an important step towards fully understanding the turbulent energy dissipation in weakly collisional plasmas.


ST07-A023 | Invited
Stepwise Development of the Auroral Onset Arc and the Near-earth Magnetotail Associated with Substorm Onsets

Yukinaga MIYASHITA1,2#+, Shinobu MACHIDA3
1Korea Astronomy and Space Science Institute, 2Korea National University of Science and Technology, 3Nagoya University

Our previous studies showed that an auroral arc develops stepwise at the beginning of a substorm. After initial auroral brightening, the auroral onset arc extends azimuthally while its wave-like structure gradually grows. The wave-like structure then enhances further and grows more rapidly, and finally poleward expansion begins. Here, using data from the Time History of Events and Macroscale Interactions during Substorms (THEMIS) spacecraft and ground-based all-sky imagers, we attempted to link stepwise auroral onset arc development to near-Earth magnetotail changes associated with substorms. Case studies show that low-frequency waves are amplified in the plasma sheet, accompanying a pressure increase likely due to the arrival of an earthward flow from a tailward region, a few minutes after initial auroral brightening and nearly simultaneously with enhancement of the wave-like auroral structure. Another few minutes later dipolarization began nearly simultaneously with auroral poleward expansion. Furthermore, we estimated the growth rate of ballooning instability in the near-Earth magnetotail from a magnetohydrodynamic (MHD) theory. We find that the growth rate of ballooning instability develops in three steps in conjunction with auroral three-step development. Based on these observations, we discuss a possible scenario of near-Earth magnetotail development in the substorm initial phase.


ST07-A025
The Transient Bifurcation Topology on the Verge of Substorm Onset in a 3D Global MHD Simulation

Peikun XIONG#+, Dongsheng CAI
University of Tsukuba

In our study, we observe a transient bifurcation in the 3D topology of the terrestrial magnetosphere that takes place right before the onset of substorm in a global MHD simulation. We use the geodesic level set method to determine the 2D manifolds of the separatrices. These separatrices are constructed from the magnetic nulls or critical points near Earth north and south poles and magnetotail. Our study visualizes the magnetospheric topologies at various times before and after the substorm onset and identifies a particular pair of saddle-connected CPs. This saddle-connection includes two separator lines that bifurcate respectively towards the north and south, allowing the outside southward IMF to connect to the Earth magnetic field. This special topology appears on the verge of the substorm onset.


Mon-31 Jul | 1:10 - 3:10 | MR308
ST02 - Upper Atmosphere and Whole Atmosphere Models for Satellite Drag and Space Weather Applications

Session Chair(s): Sean BRUINSMA, Centre National D'Etudes Spatiales

ST02-A014 | Invited
Probabilistic Thermospheric Density Modeling for Satellite Drag Forecasting

Piyush MEHTA#+, Smriti PAUL, Richard LICATA
West Virginia University

For objects in the low Earth orbit (LEO), uncertainty in atmospheric density is an important source of orbit prediction error with impacts on satellite conjunction analysis towards space traffic management and space sustainability. Most existing models can be classified as empirical or physics-based with their primary limitations being low-fidelity and computationally expensive, respectively. Additionally, all existing models are deterministic. We leverage machine learning to develop state-of-the-art probabilistic density models that lie between empirical and physics-based models on the fidelity/complexity spectrum. “HASDM-ML” uses the 20-year SET HASDM database to provide a global data-driven model. “CHAMP-ML” uses in-situ estimates of density derived from CHAMP accelerometer to develop a high-fidelity but limited data-driven model. “MSIS-UQ” uses the in-situ density estimates to enhance the existing MSIS model. Lastly, TIE-GCM ROPE develops a surrogate for the TIE-GCM model with probabilistic capabilities. In this talk, we will discuss the model development process and finally characterize its impact on orbit state and covariance prediction for operations.


ST02-A008
An Overview of the Recent Progress of the Upper Atmospheric Modeling in USTC

Jiuhou LEI1#+, Ruoxi LI1, Dexin REN1, Haibing RUAN2
1University of Science and Technology of China, 2Nanjing University of Information Science & Technology

In this presentation, we report the recent progress of the upper atmospheric modeling in the University of Science and Technology of China (USTC). Both satellite Precise Orbit Determination and accelerometers data were used to derive thermospheric density with higher accuracy and time resolution. Subsequently, based on the derived neutral densities and thermospheric models, several approaches are applied to improve the upper atmospheric density specification. The polynomial fitting, the Principal Component Analysis, assimilation and particle filter techniques were utilized to reconstruct the global temperature and density. These thermospheric models from different methods are compared and discussed.


ST02-A003
A Dynamic Calibration Model for the Upper Thermospheric Temperature and Density

Haibing RUAN1#+, Jiuhou LEI2
1Nanjing University of Information Science & Technology, 2University of Science and Technology of China

Thermospheric density plays a critical role in the spacecraft operation, while it is still a challenging issue of the thermospheric determination due to the complex driven sources. The empirical models can usually capture the long-term trends of the upper thermosphere rather than the small-scale and short-term variations. In this study, we aim to develop an optimal method to dynamically calibrate the empirical models. Based on the CHAMP and GRACE observations, the exospheric temperatures are firstly derived with the aid of the empirical models, and then the dynamic calibration could be conducted by quantifying the variation of the model residuals day-by-day after removing the local time and seasonal dependence. The result indicates a good improvement of thermospheric temperature and density specification.


ST02-A015
TLE-based Thermospheric Mass Density Specification from Intelligent Optimized Particle Filtering

Dexin REN+, Jiuhou LEI#
University of Science and Technology of China

Accurate estimation of the thermospheric density is essential for orbit prediction of low Earth orbit satellites. Recently, we conducted an intelligent optimized particle filtering algorithm to quantify the uncertain parameters in a physics-based model by comparing the simulations and observations. Here we report characteristics and variations of the upper thermosphere by assimilating two-line element (TLE) data into the model. Our results suggest that this particle filtering model can greatly improve the accuracy of thermospheric mass density specification globally.


ST02-A005
Improving the Extraction Ability of Thermospheric Mass Density Variations from Observational Data by Deep Learning

Wenbo LI1+, Libo LIU1#, Yiding CHEN2, Zhuowei XIAO1, Huijun LE1, Ruilong ZHANG1
1Institute of Geology and Geophysics, Chinese Academy of Sciences, 2Chinese Academy of Sciences

Understanding the variation of Thermospheric Mass Density (TMD) is important for solar-terrestrial physics and spacecraft safety. The thermosphere, being an open system, is impacted by a variety of space environment conditions and has complicated temporal and spatial features. Consequently, TMD observations contain a wealth of multi-scale feature information. How to extract and process from such observations is a challenge that requires ongoing research. It is vital to improving our understanding of the TMD features. Deep learning (DL) can learn complex representations directly from raw data, which makes it a compelling feature extraction and modeling tool for providing a novel perspective for TMD modeling. For the DL models, the number of stacked layers (depth) of the model is usually correlated with the model’s performance. The Residual Network (ResNet) is used in our study to build a DL model with deep network architecture. The observations of CHAllenging Minisatellite Payload (CHAMP) are utilized in the training phase, while the Gravity Recovery and Climate Experiment (GRACE-A), High Accuracy Satellite Drag Model (HASDM) and Naval Research Laboratory Mass Spectrometer and Incoherent Scatter radar Extended model (NRLMSISE-00) are used to evaluate the performance of the DL model. The results reveal that, compared with the shallow model of the typical Multi-Layer Perceptron (MLP), the DL model can better extract multi-scale features in the observation while retaining generalization capabilities. Controlled simulation experiments allow us to extract the effects of different physical processes on TMD, which improves the interpretability of the DL model. It is demonstrated that the DL model can discriminate the physical processes corresponding to the different space environment indices by simulating Equatorial Mass density Anomaly and geomagnetic storms.


Mon-31 Jul | 1:10 - 3:10 | MR311
ST08 - Remaining Challenges and Future Directions of Magnetospheric Dynamics

Session Chair(s): Kyungguk MIN, Chungnam National University, Yukinaga MIYASHITA, Korea Astronomy and Space Science Institute

ST08-A007 | Invited
Imaging the Solar Wind-magnetosphere-ionosphere Interaction by the SMILE Mission

Tianran SUN1#+, Chi WANG1, Graziella BRANDUARDI-RAYMONT2, Hyunju CONNOR3, Andrey SAMSONOV2, Yingjie ZHANG1, Xue WANG1, Fei WEI1, C. Philippe ESCOUBET4, Steve SEMBAY5, Jenny CARTER5, Andy READ5, Kip KUNTZ6, Syau-Yun HSIEH6, David SIBECK3
1Chinese Academy of Sciences, 2University College London, 3NASA Goddard Space Flight Center, 4European Space Agency, 5University of Leicester, 6Johns Hopkins University Applied Physics Laboratory

The solar wind – magnetosphere – ionosphere is a system that constitutes the near-Earth space environment, and the interaction in this system is an essential topic for the study of space weather. In situ satellites provide detailed observations of the system in localized regions, nevertheless, there are still key problems that prevent us from a complete understanding of the overall interactions on system level. In this context, Solar wind Magnetosphere Ionosphere Link Explorer (SMILE) is jointly proposed and supported by the European Space Agency (ESA) and Chinese Academy of Sciences (CAS), which is due for launch around 2024-2025. SMILE will observe the solar wind – magnetosphere – ionosphere system via simultaneous in situ solar wind detections, soft X-ray imaging of the magnetosphere, and UV imaging of the aurora. This talk will briefly review the recent progress of SMILE, including (1) a novel detection technique inspired by SWCX X-ray observations from astronomical satellites, (2) the mission profile and current status, (3) science objectives, and (4) preparations from the Modelling Working Group (MWG).


ST08-A006 | Invited
Solar Energetic Particles from the Sun to the Interplanetary Space

Jinhye PARK#+
Kyung Hee 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 in the heliosphere. Large-scale SEP events are one of the most critical phenomena in terms of space weather. They pose a risk of radiation exposure to humans and equipment in space. SEPs are accelerated in magnetic reconnection regions and by coronal mass ejection (CME)-driven shocks in the solar corona. After the acceleration process of the SEPs in the corona region, they propagate along solar magnetic fields into the interplanetary space. During the propagation, they are affected by solar wind and heliospheric magnetic fields as well as they can interact with other activities in the heliosphere. The temporal and spatial variations of SEPs strongly depend on physical quantities of source activities, magnetic connectivities between the sources and the photospheric magnetic footpoints of spacecraft, and the conditions in the interplanetary space. Recently, remote sensing observations and in-situ measurements from a fleet of spacecraft have been able to give a better understanding of the features of SEPs. In this talk, I will present the characteristics of SEPs observed by multiple spacecraft and their associated solar activities. Also, the interactions with other systems from the Sun to the interplanetary space will be discussed.


ST08-A004 | Invited
Soft X-ray Imaging of the Magnetopause Reconnection Under Low-temperature Solar Wind Conditions

Yosuke MATSUMOTO1#+, Yoshizumi MIYOSHI2
1Chiba University, 2Nagoya University

Since the first discovery of X-ray emissions from the comet Hyakutake, the charge exchange between heavy ions in the solar wind and neutral atoms (SWCX) has been understood as a bright source of the soft X-ray. GEO-X (Geospace X-ray imager, Ezoe et al., 2020) mission was proposed to visualize global structures of the magnetosphere by measuring the soft X-ray emission through the SWCX with the hydrogen atoms from the Earth's atmosphere (geocorona). The proposal has been approved as a very-small satellite mission by ISAS. By observing the emission at the low-latitude orbit 60 Re from the Earth, a global map of the dayside magnetosphere and its response to the solar wind variations can be obtained with a spatial resolution of 0.2 Re within 1-hour time resolution. For this purpose, we have developed a global MHD simulation model of the magnetosphere by using the public MHD code CANS+ (Matsumoto et al., 2019). The model can provide spatial distributions of the plasma mass density, pressure, and velocity necessary to calculate the X-ray intensity. Thus we can understand how the global intensity map reflects the magnetospheric dynamics. We examined soft X‐ray emission around the Earth's magnetosphere using the global MHD model under different solar wind conditions. The dayside magnetopause reconnection heats and accelerates the plasma whereby the X‐ray emission becomes as bright as ∼6 × 10−6 eV cm−3 s−1 under the southward interplanetary magnetic field conditions. In particular, under low plasma‐beta solar wind conditions, we found that the X‐ray intensity reflects the bulk motion of outflows from the reconnection region. We propose that this particular solar wind condition would allow visualization of the mesoscale magnetopause reconnection site, as observed in the solar corona.


ST08-A008 | Invited
What is the Role of Soft Precipitation in the Cusp?

Magnus IVARSEN1#+, Yaqi JIN1, Jaeheung PARK2, Andres SPICHER3, Jean-Pierre ST-MAURICE4
1University of Oslo, 2Korea Astronomy and Space Science Institute, 3University of Tromsø, 4University of Saskatchewan

The cusp serves as a vital point of connection in the interaction between the ionosphere and the solar wind and magnetosphere. There, constant ionization is provided by soft precipitation, outflow, and Joule heating. The F-region ionosphere is particularly turbulent in the cusp-region, producing what is arguably the most prominent plasma irregularity hotspot at high-latitudes. Soft precipitation has been thought of as vital to the production of irregularities in the cusp, in a scenario involving instabilities driven by density gradients that originate with impacting soft precipitation. However, seasonal trends in irregularity occurrence are opposite that of dayside soft precipitation. The former maximizes during winter and during geomagnetically active times, while the latter maximizes during summer and during quiet times. We present a statistical investigation into the role of soft precipitation in producing density irregularities in the cusp. Perhaps surprisingly, we show that, on average, there is no real increase in the soft electron energy flux during storm-time. Instead, other factors drive irregularities, such as the convection of dense plasma from the dayside into the cusp. That stated, soft precipitation still plays a vital role in the occurrence of irregularities. We find that whole spectrum of precipitation is effectively regulating irregularity dissipation rates in the cusp by controlling the ratio of E- to F-region Pedersen conductance, a role commonly ascribed to solar EUV photoionization. This novel finding is made possible by translating precipitating energy flux from particle detectors into altitude profiles of ionization rate. We find a near-perfect correlation between the ratio of E- to F-region precipitation-induced ionization and the occurrence of GNSS scintillations in the cusp. These results have implications for the greater high-latitude ionosphere, and indicate a much larger role for conductivity dynamics in the irregularity landscape than has thitherto been thought.


ST08-A010
Large-scale Energy Conversion in Magnetotail Reconnection

Keizo FUJIMOTO#+
Beihang University

Magnetic reconnection is a key process in the magnetospheric dynamics, yielding a fast energy conversion from the magnetic field energy into plasma kinetic energy. The magnetic dissipation to drive reconnection takes place in a localized region formed around the x-line, while the process can extend to a large distance beyond the kinetic scales. However, the large-scale process of energy conversion has been poorly understood yet for collisionless reconnection. The current study has performed large-scale PIC simulations with the adaptive mesh refinement (AMR), where the reconnection exhaust extends downstream in an MHD scale. The simulations show that the ion energy gain significantly dominates the electron energy gain and is carried out mainly in the exhaust center rather than the exhaust boundaries. The simulation results demonstrate that the energy conversion mechanism in collisionless reconnection essentially differs from that in the Petschek-type MHD reconnection where most energy conversion occurs at slow mode shocks formed at the exhaust boundaries. The current study suggests that the MHD approximation may not be appropriate in collisionless plasma even for the processes much larger than the kinetic scales.


ST08-A001
A Formation Process of Auroral Spiral During the Late Substorm Recovery Phase Observed with Successive Space- and Ground-based Auroral Images

Motoharu NOWADA1#+, Yukinaga MIYASHITA2,3, Noora PARTAMIES4, Alex DEGELING1, Quanqi SHI1
1Shandong University, 2Korea Astronomy and Space Science Institute, 3Korea National University of Science and Technology, 4The University Centre in Svalbard

The ultraviolet imager (UVI) of the Polar spacecraft and an all-sky camera at Longyearbyen contemporaneously detected an auroral vortex structure (so-called “auroral spiral”) on 10th January 1997. From space, the auroral spiral was observed as a “small spot” (one of an azimuthally-aligned chain of similar spots) in the poleward region of the main auroral oval from 18 h to 24 h magnetic local time. These auroral spots were formed while the substorm-associated auroral bulge was subsiding and several poleward-elongated auroral streak-like structures appeared during the late substorm recovery phase. Corresponding Bz (north-south) component of Interplanetary Magnetic Field (IMF) abruptly turned from long-lived (at least 4 h) weak southward (negative) to northward (positive) directions, while IMF-By (dawn-dusk) had a dominantly dawnward (negative) component. We could see significant variations in neither the associated solar wind plasma conditions nor spiral profiles. During the spiral interval, the geomagnetically north-south and east-west components of the geomagnetic field, which were observed at several ground magnetic stations around Svalbard island, showed significant negative and positive bays caused by the field-aligned currents related with the aurora spiral appearance. The negative bays were reflected in the variations of local geomagnetic activity index (SML) which was provided from the SuperMAG magnetometer network at high latitude. To pursue the spiral source region in the magnetotail, we trace each UVI image along field lines to the magnetic equatorial plane of the nightside magnetosphere using an empirical magnetic field model. Interestingly, the magnetotail region corresponding to the auroral spiral covered a broad region from Xgsm ~ -40 to -70 RE at Ygsm ~ 8 to 12 RE. The appearance of this auroral spiral suggests that extensive areas of the magnetotail (but local regions in the ionosphere) remain active even when the substorm almost ceases, and geomagnetic conditions are almost stable.


ST08-A014
Two Types of Electron Density Depletion Observed in the Polar Cap Ionosphere

Hyuck-Jin KWON1#+, Khan-Hyuk KIM2, Changsup LEE1, Young-bae HAM1, Terence BULLETT3, Nikolay ZABOTIN3
1Korea Polar Research Institute, 2Kyung Hee University, 3University of Colorado Boulder

Korea Polar Research Institute (KOPRI) has been operated multi-instruments at Jang Bogo Station (JBS, 74.6°S, 164.2°E) to monitor upper atmosphere and magnetic field. In this study, we examined the F-region electron density depletions observed by VIPIR/Dynasonde (JVD). The JVD observed long-lasting (> 11 hr) severe depletion during moderate geomagnetic storm on 11 May 2019. Other instruments installed at JBS also observed phenomena associated with electron density depletion and the geosynchronous orbit, located ~2.5 hr west of JBS, also observed negative magnetic field perturbations in the azimuthal component, which is related to the field-aligned currents. We confirmed that the reduction of O/N2 ratio as a result of TIEGCM model. From these observations and modelling, we concluded that transpolar ionospheric currents connected to the field-aligned current corresponding to substorm contributed to the ionospheric density depletion. Under quiet geomagnetic conditions, JVD observed the electron density depletion, especially during winter/nighttime. We investigated 45 depletion (known as polar hole) events in 2019 when Kp ≤ 1+ for 6 hr. All of events started over a wide range of nighttime and JVD measured exponential density decrease with e-fold decay times distributed in the range of 0.5 to 4 hr. The horizontal drift velocity (Vhor) estimated from JVD monotonically goes down from ~190 m/s at dusk to ~100 m/s at post-midnight. Such relation between density depletion and Vhor implies that the ionospheric density depletion is due to the enhancement of plasma residence time without the source of ionization under quiet conditions.


ST08-A005 | Invited
Japanese Current and Future Heliospheric System Science Exploration

Yoshifumi SAITO1#+, Yoshizumi MIYOSHI2, Kanako SEKI3, Shinsuke IMADA3
1Institute of Space and Astronautical Science / Japan Aerospace Exploration Agency, 2Nagoya University, 3The University of Tokyo

The inner heliosphere system consists of several sub-systems, Geospace, planetary system, interplanetary space, and the Sun. ISAS/JAXA is currently operating the Arase, BepiColombo/Mio, Hinode, and Akatsuki satellites. Solar-C EUVST is scheduled for launch in the near future. These missions will be linked together with other satellite missions such as Solar-Orbiter, Solar Parker Probe, Cluster, THEMIS, MMS etc. to realize exploration of the inner Heliosphere with unprecedented scale in the late 2020s. The Heliospheric system science exploration will further expand its area to the whole heliosphere beyond that time frame. The future exploration will also contribute to the space weather research/forecast that supports human activities in Geospace, Moon and other planets. Concerning the exploration of the planetary environment, Japanese Solar Terrestrial Physics group will conduct in-situ observation of space plasmas with MMX (Martian Moons Exploration) in the Martian system and with JUICE (Jupiter Icy Moons Explorer) in the Jovian system. Japanese Solar Terrestrial Physics group is currently considering a future formation-flight satellite mission FACTORS in order to reveal the energy coupling mechanisms and mass transport between the space and Earth’s atmosphere. In the late 2030s, another formation-flight magnetospheric satellite mission the science target of which includes understanding the cross-scale / cross-region coupling is also under consideration hopefully on orbit at the same time with European future mission Plasma Observatory. These future missions will closely collaborate with NASA’s future GDC and Magnetospheric Constellation missions. Collaboration between Japanese Solar Physics and Solar Terrestrial Physics groups for considering the future out-of-ecliptic-plane mission is also about to start. In order to realize the future Heliospheric system science exploration, significant technological development is mandatory. Current status of the technological development in Japan for enabling the future Heliospheric system science exploration will also be presented.


Tue-01 Aug | 10:20 - 12:20 | MR309
ST04 - Modelling Magnetohydrodynamic Processes in the Solar Atmosphere

Session Chair(s): Viktor FEDUN, The University of Sheffield

ST04-A002
Excitation of Multi-periodic Kink Motions in Solar Flare Loops: Possible Application to Quasi-periodic Pulsations

Mijie SHI1#+, Bo LI1, Shao-Xia CHEN1, Mingzhe GUO2
1Shandong University, 2KU Leuven

Magnetohydrodynamic (MHD) waves are often invoked to interpret quasi-periodic 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 = 57s) being attributed to the radial fundamental kink mode and the short-period component (PS = 5.8s) 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.


ST04-A006
The Recurring Coronal Rains Driven by Self-consistent Heating Process in a Radiative Magnetohydrodynamic Simulation

Zekun LU#+, Jinhan GUO, Feng CHEN, Mingde DING, Can WANG
Nanjing University

Solar coronal loops are dense structures mainly seen in extreme ultraviolet (EUV) images throughout atmosphere of the Sun. For the lack of three-dimensional coronal magnetic field and thermodynamic data in observations, what heats the plasma to millions of degrees and drives the mass cycles is a fundamental but still challenging question. In this work, resorting to state-of-the-art radiative magnetohydrodynamic (RMHD) code MURaM, we reproduce a three-dimensional evolution of an active region resembling realistic observations, which successfully links the coronal heating with the large-scale characteristics of the coronal loops. Driven by convective motions, the coronal loops are heated self-consistently by a series of intermittent magnetic reconnections, namely magnetic braiding. We find that such heating rate is quasi-steady, stratified and strong enough to induce sufficient chromospheric evaporation, making the loops in a state of thermal non-equilibrium (TNE) and then triggering catastrophic cooling through thermal instability. Moreover, the simulation covers more than one TNE cycle that manifests as variations of EUV intensities and the co-temporal recurring coronal rains, where the motion of rain plumes clearly reflects the multi-strands fine structures of the coronal loops. These results provide a new perspective for inferring properties of coronal magnetic field and heating mechanisms from global behaviors of the coronal loops.


ST04-A007
Transverse Waves in Strongly Magnetized Sunspot and Its Heating Effect

Ding YUAN#+
Harbin Institute of Technology, Shenzhen

The solar corona is 2 to 3 orders of magnitude hotter than the underlying photosphere, and the energy loss of coronal plasma is extremely strong at this temperature, with a heating flux over 1,000Wm−2 required to maintain its high temperature. Using the 1.6-meter Goode Solar Telescope, we report the detection of ubiquitous and persistent transverse waves in umbral fibrils in the chromosphere of a strongly magnetized sunspot. The energy flux carried by these waves was estimated to be 7.52 × 106Wm−2, 3 to 4 orders of magnitude stronger than the energy loss rate of active region plasma. Two-fluid magnetohydrodynamic (MHD) simulations reproduced state-of-the-art observations and showed that these waves dissipate significant energy, indispensable for coronal heating. Such transverse oscillations and associated strong energy flux may exist in a variety of magnetized regions on the Sun and could be the observational target of next-generation solar telescopes.


Tue-01 Aug | 10:20 - 12:20 | MR330
ST12 - Applications of Remote Sensing in Monitoring Ionospheric Physics and Ionospheric Weather Forecasting

Session Chair(s): Chunhua JIANG, Wuhan University, Tatsuhiro YOKOYAMA, Kyoto University

ST12-A007 | Invited
Automatic Scaling of foF2 and foEs from Ionograms Obtained at Shigaraki MU Observatory

Tatsuhiro YOKOYAMA#+, Yuki UNEYAMA, Peng LIU, Mamoru YAMAMOTO
Kyoto University

In Shigaraki MU Observatory, where the MU radar is a main facility, an ionosonde has been operated since the beginning of the MU radar operation. Digital images after 2001 are available in the database of Research Institute for Sustainable Humanosphere (RISH), Kyoto University ( http://database.rish.kyoto-u.ac.jp/arch/mudb/ionosonde/). However, the scaled parameters of the Shigaraki ionograms have not been available in the database, so that users have to scale the ionograms by their own. In order to utilize the Shigaraki ionosonde easily, we have been developing an auto-scaling system of ionograms. A representative model of instance segmentation, which is called Mask Region-Convolutional Neural Network (R-CNN), is used as a background model. By using the machine learning model, foF2 and foEs can be successfully scaled automatically. The system was trained separately for scaling foF2 and foEs. Approximately 500 ionogram images in which ionospheric traces of F and Es layers are labeled manually. The obtained foF2 values are generally consistent with those from Kokubunji ionosonde operated by National Institute of Information and Communications Technology (NICT), whose distance from Shigaraki ionosonde is about 350 km. The scaled foF2 can be used to determine absolute electron density of incoherent scatter observation by the MU radar. Auto-scaling of foEs also shows high accuracy with an averaged error of as low as 0.24MHz. A distribution of foEs values are similar with that from Kokubunji ionosonde, which implies the auto-scaling works correctly. However, one-to-one comparison of foEs obtained in the two stations at the same time show a relatively low correlation coefficient (0.51). It suggests that a large-scale formation of Es layer is common over Shigaraki and Kokubunji, while the distribution of a neutral wind and metallic ions have a different pattern over the two stations. From a long-term analysis, we did not find a dependence on solar activity.


ST12-A002 | Invited
The Temporal Evolution of F-region Equatorial Ionization Anomaly Owing to the 2022 Tonga Volcanic Eruption

Kedeng ZHANG#+, Hui WANG
Wuhan University

The dynamic evolutions of the noon ionospheric Equatorial Ionization Anomaly (EIA) owing to the 2022 Tonga volcanic eruption were investigated using the ionospheric plasma measurements from the Swarm satellite and the science experiment of the Constellation Observing Systems for Meteorology, Ionosphere, and Climate (COSMIC) mission, thermospheric wind observations from the Ionospheric Connection Explorer (ICON). At 14.1 universal time (UT), the noon EIA was enhanced for the upward plasma drifts, when the F2 layer was significantly uplifted from 360 km to 410 km. At 15.6 UT, because of the downward drifts, the intensity of EIA reduced, and hmF2 decreased to 270 km. At 17-18 UT, EIA recovered and reformed, and hmF2 increased to 350 km. A two-peak structure in the plasma was observed at Swarm altitudes. The temporal evolution might be related to the vertical plasma drifts (both downward and upward) from the E-region electric field.


ST12-A001
Study of the Ionospheric Scintillation Radio Propagation Characteristics with COSMIC Observations

Yang LIU#+, Zhuo CHEN
Beihang University

The ionosphere has important influences on trans-ionosphere radio propagation. When signals pass through ionospheric irregularities, their amplitude and phase are often attenuated and distorted. In this work, the statistical features of scintillation observed by the Global Navigation Satellite System (GNSS) and low earth orbit (LEO) satellites are investigated with Constellation Observing System for Meteorology, Ionosphere, and Climate (COSMIC) data in solar cycle 24. The amplitude scintillation propagation channel is fitted by the Nakagami-m, a-μ and κ-μ models. The performance is evaluated in terms of root mean square error (RMSE), kurtosis and information entropy. The results reveal that the a-μ model achieves the best performance in all considered scintillation intensities, while the Nakagami-m model achieves better performance under severe scintillation in the GNSS-LEO propagation channels. The global ionospheric scintillation feature for radio propagation is investigated with the COSMIC occultation data from 2010 to 2019. The statistical characteristics of the amplitude scintillation index and SNR are analyzed, and the radio propagation channel feature is extracted. It was found that the probability for weak scintillation accounts for the largest proportion, with approximately 69%, while the moderate and strong scintillation accounts for approximately 20%, and 11% respectively. The fitting performance is analyzed in different solar activity years. The fitting interval analysis was discussed to evaluate the fitting performance. The fitting interval length of the Nakagami-m distribution increases with increasing normalized S4; a-m distribution meets the 100% confidence level in the whole range; κ-m distribution has a similar trend as that of the Nakagami-m distribution, while it does not reach 100% in the whole range. The skewness–kurtosis profile extracted in this work shows similar features as revealed by a previous study, indicating that the amplitude scintillation propagation channel is probably related to the nonlinearity of ionospheric irregularity and potential influential factors of the ionosphere.


ST12-A003 | Invited
Oscillations of the Ionosphere Caused by the 2022 Tonga Volcanic Eruption Observed with Superdarn Radars

Jiaojiao ZHANG1#+, Jiyao XU2, Wei WANG2, Guojun WANG2, J. RUOHONIEMI3, Atsuki SHINBORI4, Nozomu NISHITANI4, Chi WANG2, Xiang DENG2, Ailan LAN2, Jingye YAN2
1National Space Science Center, Chinese Academy of Sciences, 2Chinese Academy of Sciences, 3Virginia Tech, 4Nagoya University

On 15 January 2022, the submarine volcano on the southwest Pacific island of Tonga violently erupted. Thus far, the ionospheric oscillation features caused by the volcanic eruption have not been identified. Here, observations from the Super Dual Auroral Radar Network radars and digisondes were employed to analyze ionospheric oscillations in the Northern Hemisphere caused by the volcanic eruption in Tonga. Due to the magnetic field conjugate effect, the ionospheric oscillations were observed much earlier than the arrival of surface air pressure waves, and the maximum negative line-of-sight (LOS) velocity of the ionospheric oscillations exceeded 100 m/s in the F layer. After the surface air pressure waves arrived, the maximum LOS velocity in the E layer approached 150 m/s. A maximum upward displacement of 100 km was observed in the ionosphere. This work provides a new perspective for understanding the strong ionospheric oscillation caused by geological hazards observed on Earth.


ST12-A005
Verification of the Response of the Earth’s Ionosphere by Solar Flare Spectra Using GAIA

Shinnosuke KITAJIMA1#+, Kyoko WATANABE1, Hidekatsu JIN2, Chihiro TAO2, Michi NISHIOKA2
1National Defense Academy of Japan, 2National Institute of Information and Communications Technology

The sudden increase in X-ray to extreme ultraviolet (EUV) emissions from solar flares promote ionization in the ionosphere. The communication failure caused by the absorption of the radio waves, due to fluctuations in electron density in the ionospheric D region is called the Dellinger phenomenon. The occurrence of the Dellinger phenomenon can be known from the value of the minimum reflection frequency (fmin) observed by the ionosonde. However, there are many cases in which the fmin value is not proportional to the X-rays. Thus, it is necessary to consider flare emission wavelengths other than X-rays, which affect the electron density of the ionospheric D region. We investigated the relationship between X-ray and EUV emissions and the fmin values obtained from the ionosondes which are provided by NICT in Wakkanai, Kokubunji, Yamagawa and Okinawa. We analyzed 38 solar flare events of >M3 class observed during daytime in Japan between May 2010 and May 2014.Next, using the Ground-to-Topside Model of Atmosphere and Ionosphere for Aeronomy (GAIA), a physical model of the Earth's atmosphere, and the Appleton-Hartree equation to calculate the fluctuations of ionosphere and the absorption of short-wave radio due to solar flare spectra. Detailed event analysis on May 13, 2013 shows that the main source of ion density fluctuations is X-ray in the D region and EUV emission in the E and F regions. The absorption of the short-wave was found to be ~90-100 % in the D region and ~10 % in the E region. Finally, we tried to estimate the magnitude of the Dellinger phenomenon. We improved the accuracy of the black-out capture rate from 31 % to 62 % using not only the GAIA calculation but also the solar zenith angle-corrected X-ray flux Fχ, were used as the variable for ion density in the D region.


ST12-A006
Climatology Study of Ionospheric Electron Content Features in the Polar Regions Shown in GIMs and a Sample Dataset for TOI

Haixia LYU1,2#+, Manuel HERNÁNDEZ-PAJARES2, Enric MONTE-MORENO2, Hongping ZHANG1, Min LI1
1Wuhan University, 2Universitat Politècnica de Catalunya

The ionosphere at high latitudes is considerably complex due to the fact that nearly vertical magnetic field-lines connect the high latitudes to the outer part of the magnetosphere which is driven by the solar wind. Plasma density irregularity at high latitudes, associated with intense levels of scintillation, can severely disrupt High Frequency radio communication, surveillance and satellite navigation systems. With the increase of human activities relying on such systems, the ionospheric features in the polar regions are of increasing interest. Thus, it is essential to understand the morphology and climatology of different features, such as Tongue of Ionization (TOI), polar cap patches, troughs etc. The Global Ionosphere Maps (GIMs) derived from International GNSS Service (IGS) GNSS data have been successfully used to detect important polar ionospheric features, including TOI, depletion, flux transfer event, theta-aurora, ionospheric convection patterns and storm enhanced density (Hernández‐Pajares et al., 2020; Monte-Moreno, et al., 2021). Taking advantage of the continuous, global coverage and low-cost characteristics of IGS GNSS data, the GIMs covering 25 years provide an unprecedently valuable dataset regarding the spatial and temporal coverage for the climatology study of interesting ionospheric features in the polar regions, opening a new opportunity for detection and thus probably provide new evidence and arouse new insights for plausible theoretical assumptions. In this work, the climatology analysis of ionospheric features in the polar regions by an unsupervised clustering - learning vector quantization will be presented. Besides, a sample data set of TOI and segmented polar cap patches through manual interpretation will be built to support future work on climatology study.


ST12-A010
An Improved Method for Automatic Scaling of Oblique Ionograms

Chunhua JIANG#+, Tongxin LIU, Guobin YANG
Wuhan University

In this study, an improved method was developed to carry out automatic scaling of oblique ionograms. The proposed method adopts the Quasi-Parabolic Segments (QPS) model to represent the ionosphere. Firstly, numerous candidate electron density profiles and corresponding vertical traces were, respectively, calculated and synthesized by adjusting the parameters of the QPS model. Then, the candidate vertical traces were transformed to oblique traces by the secant theorem and Martynˈs equivalent path theorem. On the other hand, image processing technology and characteristics of oblique echoes were adopted to automatically scale the key parameters (the maximum usable frequency and minimum group path, etc..) from oblique ionograms. The synthesized oblique traces, whose parameters are close to autoscaled parameters, were selected as the candidate traces to make correlation with measured oblique ionograms. Lastly, the proposed algorithm searches the best-fit synthesized oblique trace by comparing the synthesized traces with oblique ionograms. To test its feasibility, oblique ionograms are automatically scaled by the proposed method and these autoscaled parameters are compared with manual scaling results. The preliminary results show that the scaling results of the F2 layer are accurate enough for space weather. It inspires us to improve the proposed method in the future studies.


Tue-01 Aug | 1:10 - 3:10 | MR309
ST04 - Modelling Magnetohydrodynamic Processes in the Solar Atmosphere

Session Chair(s):

ST04-A009 | Invited
Improved Thermal Conduction Models for the Solar Corona

Tony ARBEER#+, Tom GOFFREY
University of Warwick

Thermal transport in the solar corona is often modelled using the Braginskii (Spitzer-Harm) local conduction model. This model fails when the thermal mean-free-path exceeds about 1% of the temperature scale-length. When this happens there are two non-local effects which must be accounted for - flux limiting and pre-heat. The simplest approach is to use a thermal flux-limiter but this does not include pre-heat modelling and requires a free parameter to be set against observations. It is also known to be inaccurate from studies of laser-plasmas. Instead more advanced non-local models can be used and the most promising for thermal transport is the SNB model. This has no free parameters and includes both flux-limiting and pre-heat. This model will be assessed for typical coronal values.


ST04-A013
Phase Mixing In Partially Ionised Plasmas

Max MCMURDO#+, Viktor FEDUN, Gary VERTH, Istvan BALLAI
The University of Sheffield

The coronal heating problem is described as the rapid increase in temperature of the solar atmosphere from approximately 6000 Kelvin (K) in the photosphere to a few million K in the corona occurring over a few thousand kilometers. Effective plasma heating requires large gradients over short spatial scales in the magnetic and velocity fields respectively. Phase mixing is one of the most promising wave mechanisms for explaining the heating of the solar atmosphere by producing small transversal scales to the magnetic field but requires large transversal gradients in the equilibrium Alfvén speed. Fortunately, large transversal gradients due to the equilibrium magnetic field are abundant in the solar atmosphere and these will greatly increase phase mixing. Using a single fluid approximation of a partially ionised chromospheric plasma we study the effectiveness of the damping of phase mixed shear Alfvén waves and investigate the effect of varying the ionisation degree on the dissipation of waves. Our results show that the dissipation length of shear Alfvén waves strongly depends on the ionisation degree of the plasma, but more importantly, in a partially ionised plasma the damping length of shear Alfvén waves is several orders of magnitude shorter than in the case a fully ionised plasma, providing further evidence that phase mixing is a large contributor to heating the solar plasma in the chromosphere.


Tue-01 Aug | 1:10 - 3:10 | MR309
ST16 - Solar Magnetic Fields: Measurements, Extrapolations And (R)MHD Simulations

Session Chair(s): Xiaoshuai ZHU, National Space Science Center, Chinese Academy of Sciences

ST16-A006 | Invited
Solar Coronal Magnetic Field Measurements Using Spectral Lines Available in Hinode/EIS Observations

Yajie CHEN1#+, Xianyong BAI2, Hui TIAN3, Wenxian LI2, Feng CHEN4, Zihao YANG3
1Max Planck Institute for Solar System Research, 2Chinese Academy of Sciences, 3Peking University, 4Nanjing University

Recently, it has been proposed that the magnetic-field-induced transition (MIT) in Fe X can be used to measure coronal magnetic field strengths. Several techniques, the direct line ratio technique and the weak and strong magnetic field techniques, are developed to apply the MIT theory to spectroscopic observations taken by EUV Imaging Spectrometer (EIS) onboard Hinode. However, the suitability of coronal magnetic field measurements based on the weak and strong magnetic field techniques has not been evaluated. Besides, temperature diagnostics is also important for measuring coronal magnetic field based on the MIT theory, but how to determine the accurate formation temperature of the Fe x lines from EIS observations still needs investigation. We synthesized emissions of several spectral lines from a 3D radiation magnetohydrodynamic model of a solar active region, and then derived magnetic field strengths using different methods. We first compared the magnetic field strengths derived from the weak and strong magnetic field techniques to the values in the model. Our study suggests that both weak and strong magnetic field techniques underestimate the coronal magnetic field strength. Then we developed two methods to calculate the formation temperature of the Fe x lines. One is based on differential emission measure analyses, and the other is deriving temperature from the Fe ix and Fe xi line pairs. However, neither of the two methods can provide temperature determination for accurate coronal magnetic field measurements as those derived from the Fe x 174/175 and 184/345 Å line ratios. More efforts are still needed for accurate coronal magnetic field measurements using EIS observation.


ST16-A002
Diagnosing the Magnetic and Plasma Properties of Coronal Mass Ejections with the Coronal Solar Magnetism Observatory Large Coronagraph

Xianyu LIU1#+, Hui TIAN1, Tibor TOROK2, Sarah GIBSON3, Zihao YANG1, Wenxian LI4, Tanmoy SAMANTA5, Steven TOMCZYK3
1Peking University, 2Predictive Science Inc., 3National Center for Atmospheric Research, 4Chinese Academy of Sciences, 5Indian Institute of Astrophysics

The proposed COronal Solar Magnetism Observatory (COSMO) Large Coronagraph (LC) will pro- vide unique observations to study the coronal mass ejections (CMEs) with its ability to diagnose the magnetic and plasma properties in the solar coronal material. Here we take a realistic magnetohydrodynamic CME model, and then synthesize the signals of several coronal emission lines (CELs) to perform the forward modeling of COSMO LC observation of a CME. We use the Stokes parameters of the Fe xiii 10747 ̊A line to diagnose the magnetic and plasma properties of the flux rope. The results show that COSMO LC can provide magnetic field measurements of CME progenitors with a high spatial resolution (2''). By using a worse resolution (6''), the COSMO LC can also be used to qualitatively study the evolution of the magnetic field during the CME eruption. We then use the synthetic signals of several other CELs to diagnose the physical conditions in the CME leading front, including the shock. The COSMO LC observations of Fe xiii 10798/10747 ̊A and Ar xiii 8300/10143 ̊A line pair can provide density diagnostics of the front. By observing several CELs with different formation temperatures, the COSMO LC can be used to diagnose the temperature and ionization states in the front. We suggest that Fe xiii 10747 ̊A line should be given the highest priority in observing the CMEs, while the observations Fe xiii 10798 ̊A, Fe xiv 5303 ̊A, Fe xv 7062 ̊A, and Ar xiii 10143 ̊A lines can also give valuable information on the CMEs.


ST16-A005
Measuring Local Physical Parameters in Coronal Loops by Spatial Seismology

Guoyin CHEN1#+, Yang GUO1, Mingde DING1, Robertus ERDELYI2
1Nanjing University, 2The University of Sheffield

Spatial seismology can invert the physical parameters, such as the density and the magnetic field, by numerically optimizing the parametric model to best fit the oscillation amplitude profile along the loop. Compared with the seismology in time domain, it relies only on the detection of fundamental mode rather than higher order overtone, thus it can use on a wider range. Besides, because of the increased constraints in spatial domain, is can limit a certain magnetic field or density distribution instead of a pure averaging density or magnetic field strength. Furthermore, the inverted magnetic field and density by spatial seismology coincides well with the magnetic field extrapolated by potential model and the density derived from differential emission measuring (DEM) analysis, which supports the feasibility and validity of the spatial seismology.


Tue-01 Aug | 1:10 - 3:10 | MR330
ST10 - Kinetic Physics And Multi-scale Dynamics Associated With Magnetic Reconnection

Session Chair(s): Wenya LI, Chinese Academy of Sciences, Zhihong ZHONG, Nanchang University, Hiroshi HASEGAWA, Institute of Space and Astronautical Science, JAXA

ST10-A001 | Invited
Kinetic Simulations of Magnetic Reconnection in the Downstream of the Earth's Bow Shock

Quanming LU1#+, Jin GUO1, Xueyi WANG2
1University of Science and Technology of China, 2Auburn University

Magnetic reconnection is usually observed in the downstream of the Earth’s bow shock. Using two-dimensional hybrid simulations, we investigated the characteristics of the quasi‐parallel magnetosheath of the bow shock. Current sheets with widths of several ion inertial lengths are found to be produced in the magnetosheath after the upstream large‐amplitude electromagnetic waves penetrate through the shock and are then compressed in the downstream. Magnetic reconnection consequently occurs in these current sheets.


ST10-A007
Electron Dynamics in Guide-field Magnetic Reconnection

Binbin TANG1#+, Hanwen WANG2, Yongcun ZHANG2
1National Space Science Center, Chinese Academy of Sciences, 2Chinese Academy of Sciences

Magnetic reconnection is a fundamental process that rapidly converts energy from the magnetic field to plasma. Recent studies have shown that a large E|| can appear in guide-field reconnection, and its magnitude can be several times larger than the reconnection electric field. However, the generation of this large E|| is still not fully understood, and the reaction of electrons to this E|| has not been fully investigated. In this study, we focus on these issues in a strong guide-field reconnection event (the normalized guide field is ~ 1.5) from Magnetospheric Multiscale (MMS) observations. With the presence of a large E|| in the electron current sheet, electrons are accelerated when streaming into this E|| region from one direction, and decelerated from the other direction. Some decelerated electrons can reduce the parallel speed to ~ 0 to form relatively isotropic electron distributions at one side of the electron current sheet, as the estimated acceleration potential (Φ|| ~ 2 kV) satisfies the relation eΦ|| ≥ kT||, where T|| is the electron temperature parallel to the magnetic field. Therefore, a large E|| is generated to balance the parallel electron pressure gradient across the electron current sheet, since electrons at the other side of the current sheet are still anisotropic. Based on these observations, we further show that the electron beta is an important parameter in guide-field reconnection, providing a new perspective to solve the large parallel electric field puzzle in guide-field reconnection.


ST10-A025 | Invited
Whistler Waves Associated with Electron Beams in Magnetopause Reconnection Diffusion Regions

Shan WANG1#+, Daniel GRAHAM2, Olivier LE CONTEL3,4, Yuri KHOTYAINTSEV2, Benoit LAVRAUD3
1Peking University, 2Swedish Institute of Space Physics, 3National Centre for Scientific Research, 4Ecole Polytechnique

In magnetopause reconnection, whistler waves are commonly observed and are often associated with electron beams. We analyze seven MMS crossings surrounding the electron diffusion region (EDR) to study the role of electron beams in whistler excitation. Waves have two major types: (a) Narrow-band waves with high ellipticities and (b) broad-band waves that are more electrostatic with significant variations in ellipticities and wave normal angles. While both types of waves are associated with electron beams, the key difference is the anisotropy of the background population, with perpendicular and parallel anisotropies, respectively. The linear instability analysis suggests that the first type of wave is mainly due to the background anisotropy, with the beam contributing additional cyclotron resonance to enhance the wave growth. The second type of broadband waves are excited via Landau resonance, and as seen in one event, the beam anisotropy induces an additional cyclotron mode. The results are supported by particle-in-cell simulations. We infer that the first type occurs downstream of the central EDR, where background electrons experience Betatron acceleration to form the perpendicular anisotropy; the second type occurs in the central EDR of guide field reconnection. A parametric study is conducted with linear instability analysis. A beam anisotropy alone of above ∼3 likely excites the cyclotron mode waves. Large beam drifts cause Doppler shifts and may lead to left-hand polarizations in the ion frame. Future studies are needed to determine whether the observation covers a broader parameter regime and to understand the competition between whistler and other instabilities.


ST10-A002
Enhanced Energy Conversion by Turbulence in Collisionless Magnetic Reconnection

Runqing JIN1#+, Meng ZHOU1,2, Yongyuan YI1
1Nanchang University, 2University of California, Los Angeles

Magnetic reconnection and turbulence are two of the most important energy dissipation mechanisms in collisionless plasma. The role of turbulence in magnetic reconnection is one outstanding problem in astrophysics and plasma physics. Whether the turbulence could modify the reconnection process, such as enhance the reconnection rate and energy conversion rate, is largely unknown. Using the unprecedented high-resolution data from the magnetospheric multiscale spacecraft, we provide direct evidence that turbulence promotes the energy conversion and production of energetic particles in reconnection. The conclusion is achieved after comparing magnetotail reconnection events, which have similar inflow Alfven speed and plasma β but different amplitudes of turbulence. The difference in the energy conversion and energetic particles is thus due to the strength of turbulence. Stronger turbulence induces more coherent structures with smaller spatial scale, which are important in contributing to energy conversion in reconnection. These results significantly advance our understanding of the relationship between turbulence and reconnection in space plasma.


ST10-A013
Hall Effect Providing the Core Field Inside a Magnetic Flux Rope in an Antiparallel Magnetic Reconnection

Yong Cun ZHANG#+, Lei DAI, Chi WANG
Chinese Academy of Sciences

The observations from the Magnetospheric Multiscale mission on 2015 November 12 showed the existence of tripolar Hall magnetic fields north of the X line in a quasi-antiparallel reconnection at the dayside of the magnetopause. The bipolar variation in the normal component of the magnetic field inside the middle polar region of the tripolar Hall fields indicated the presence of an ion-scale magnetic flux rope. The coexistence of Hall fields and a magnetic flux rope provides the first evidence that the Hall effect in quasi-antiparallel magnetic reconnection can generate the core field inside a magnetic flux rope. There is one dip in the core field of the observed magnetic flux rope. We interpret the core field and the dip with the Hall effect associated with sequential multiple-X-line reconnection. The results of this study shed light on the mechanism of the generation of the core field inside the magnetic flux rope.


ST10-A012
Magnetospheric Multiscale Observations of Ion-scale Magnetic Flux Rope Generated from Electron-scale Magnetopause Current Sheet

Hiroshi HASEGAWA1#+, Richard DENTON2, Kyunghwan DOKGO3, Kyoung-Joo HWANG3, Takuma NAKAMURA4, James BURCH3
1Institute of Space and Astronautical Science, JAXA, 2Dartmouth College, 3Southwest Research Institute, 4Austrian Academy of Sciences

We present in-depth analysis of three southward-moving meso-scale (ion- to magnetohydrodynamic-scale) flux transfer events (FTEs) and subsequent crossing of a reconnecting magnetopause current sheet (MPCS), which were observed on 8 December 2015 by the Magnetospheric Multiscale spacecraft in the subsolar region under southward and duskward magnetosheath magnetic field conditions. Our aims are to understand the generation mechanism of ion-scale magnetic flux ropes (ISFRs) and to reveal causal relationship among magnetic field structures, electromagnetic energy conversion, and kinetic processes in magnetic reconnection layers. Magnetic field reconstruction methods suggest that a flux rope with a length of about one ion inertial length existed in the MPCS and grew from an electron-scale current sheet (ECS), supporting the idea that ISFRs can be generated through secondary magnetic reconnection in ECS. Grad-Shafranov reconstruction applied to the three FTEs shows that the FTE flux ropes had axial orientations similar to that of the ISFR. This suggests that these FTEs also formed through the same secondary reconnection process, rather than multiple X-line reconnection at spatially separated locations. Four-spacecraft observations of electron pitch-angle distributions and energy conversion rate J*E' suggest that the ISFR had three-dimensional magnetic topology and secondary reconnection was patchy or bursty. Previously reported positive and negative values of J*E', with magnitudes much larger than expected for typical magnetopause reconnection, were seen in both magnetosheath and magnetospheric separatrix regions of the ISFR. Many of them coexisted with bi-directional electron beams and intense electric field fluctuations around the electron gyrofrequency, consistent with their origin in separatrix activities.


ST10-A005
Kinetic Scale Magnetic Reconnection with a Turbulent Forcing: Particle-in-cell Simulations

San LU#+, Quanming LU, Rongsheng WANG, Xinmin LI
University of Science and Technology of China

Turbulent magnetic reconnection has been observed by spacecraft to occur commonly in terrestrial magnetosphere and the solar wind, providing a new scenario of kinetic scale magnetic reconnection. Here by imposing a turbulent forcing on ions in particle-in-cell simulations, we simulate kinetic scale turbulent magnetic reconnection. We find formation of fluctuated electric and magnetic fields and filamentary currents in the diffusion region. Reconnection rate does not change much compared to that in laminar Hall reconnection. At the X-line, the electric and magnetic fields both exhibit a double power law spectrum with a spectral break near local lower-hybrid frequency. The energy conversion rate is high in turbulent reconnection, leading to significant electron acceleration at the X-line through stochastic acceleration. The accelerated electrons form a power law spectrum in the high energy range, with a power law index of about 3.7, much harder than one can obtain in laminar reconnection.


ST10-A004
R-T Instability Observed at the Dayside Magnetopause Under Northward IMF

Guangqing YAN#+
Geovis Environment Technology Co., Ltd.

Under northward interplanetary magnetic field (IMF), periodical fluctuations with the period of 85 seconds have been observed by one of the Time History of Events and Macroscale Interactions during Substorms (THEMIS) spacecraft at the dayside magnetopause when the solar wind dynamic pressure suddenly dropped. The observed magnetic field distortions, characterized by the compression of the main component as well as the flapping of the perpendicular components, are in line with the theoretical predictions of the Rayleigh-Taylor (R-T) instability excited at the magnetopause. With the convective electric field and the mean electric field removed, the perturbations in the electric field are identified as typical 2 sinusoidal signals with a 90° phase difference, consistent with previous prediction of the attendant electrostatic field arising from the R-T instability. The transverse motions of the plasmas resulting from the electric drifting driven by the electrostatic field are observed both in pitch-angle distributions and in distribution functions. The growth rate of the R-T instability is about 43 seconds, implying that the instability has time to grow during the disturbances. Using the Gauss theorem, the calculated net charge density based on the electric field observation is one part of 27 compared to the totally observed plasma density, indicating that only a tiny fraction of the charge separates to set up the electrostatic field, which is due to a collective effect in the plasma.


Tue-01 Aug | 1:10 - 3:10 | MR333
ST13 - ULF Waves in Geospace: Investigating Wave Generation, Propagation and Wave-particle Interaction Through Observations, Simulation and Theory

Session Chair(s): Xueling SHI, Virginia Tech

ST13-A003 | Invited
Foreshock Transient-triggered ULF Waves and the Related Periodic Discrete Aurora

Boyi WANG1#+, Jiaqi LIU1, Xinyu XU1, Yukitoshi NISHIMURA2, Vassilis ANGELOPOULOS3, Yen-Jung WU4, Harald FREY4
1Harbin Institute of Technology, Shenzhen, 2Boston University, 3University of California, Los Angeles, 4University of California, Berkeley

The typical foreshock transients are known as Hot Flow Anomalies (HFAs), foreshock cavities, and foreshock bubbles. They are frequently observed upstream from the bow shock and many of them can compress or inflate the magnetosphere and transfer energies from the solar wind into the magnetosphere through compressional ultra-low frequency (ULF) waves. These ULF waves can further transfer energies and precipitate electrons into the ionosphere and trigger discrete and diffuse auroral brightenings. The auroral images can in turn provide the two-dimensional information of the magnetospheric ULF waves that are triggered by foreshock transients. However, the relationship between foreshock transient-induced ULF waves and discrete aurora has not been thoroughly studied yet. In this presentation, the conjunction between the THEMIS probes and the all-sky imager at the AGO south-pole station is utilized to examine the periodic discrete auroral patterns during foreshock transient events. Two categories of the periodic discrete aurora are identified: 1) the periodic discrete aurora embedded in or across the discrete auroral oval, which is possibly related to traveling convection vortices (TCVs); 2) the field-line resonance (FLR)-related discrete aurora (poleward-moving east-west arc at lower latitudes than the discrete auroral oval), which has been reported by Wang et al. (2019). We further investigate the different characteristics of these two types of discrete aurora and compare the magnetospheric and ground magnetic fields between these events. In addition, with auroral images with different emission lines, the energy and energy fluxes of the precipitating electrons are possible to be estimated.


ST13-A010
A Conjunction of Pc5 ULF Waves from Spaceborne and Ground-based Observations

Xingxin ZHAO1#+, Jianjun LIU1, Qiugang ZONG2, Chao YUE2, Xuzhi ZHOU2, Zhiyang LIU2
1Polar Research Institute of China, 2Peking University

The ultra-low frequency (ULF) waves play a significant role in the inner magnetosphere dynamics. Large scale (low wavenumber m) ULF waves observed in the inner magnetosphere can propagate into the ionosphere and to the ground, which is recognized as magnetic pulsations by ground-based magnetometers. We present the conjunctive observation of Pc5 ULF waves from Van Allen Probes (at ~6MLT, earlier), GOES13 (at ~1MLT, later), SuperDARN radar (at ~6MLT), and ground magnetometers. The phase shifts of the waves observed by satellites at different MLTs indicate westward propagation from the noon sector. The traveling Alfven waves propagate along the field line and reflect mostly at the ionosphere, while a few waves propagate to the ground. Thus, we conclude that standing waves are observed by the spacecraft while traveling signals are observed by ground-based magnetometers in the form of electromagnetic waves. By mapping the ground magnetic pulsations to the magnetic equatorial plane, the expected ULF waves match well with the satellite observations, suggesting that the ULF waves are physically congenetic and propagate in the magnetosphere-ionosphere-atmosphere system.


ST13-A015
Intense Geoelectric Field Perturbations Driven by Ultra-low Frequency Waves

Xueling SHI1,2#+, Michael HARTINGER3, Joseph BAKER1
1Virginia Tech, 2National Center for Atmospheric Research, 3Space Science Institute

Geomagnetic perturbations related to various phenomena in the near-Earth space environment can induce geoelectric fields within the electrically conducting Earth. In turn these geoelectric fields drive geomagnetically induced currents (GIC) that can cause potential damage to technological infrastructure. Ultra-low frequency (ULF: 1 mHz - several Hz) waves have recently been reported to be a common driver of intense geoelectric fields during geomagnetic storms. Though numerous past studies have examined ULF wave related geomagnetic fields from a space weather perspective, few studies have linked ULF waves with geoelectric fields due to limited direct measurements of these fields. Using 1-second cadence geoelectric field measurements made at recently available magnetotelluric survey sites distributed widely across the United States, we explore the relationship between ULF waves and intense geoelectric field perturbations. Detailed case studies demonstrate that the ULF wave driven geoelectric fields have significant spatial variation in contrast to relatively uniform geomagnetic field perturbations, consistent with spatially varying Earth conductivity. We further show that geoelectric fields driven by ULF waves during geomagnetic storms have comparable amplitudes to once-per-century geoelectric hazard maps. Our results highlight the need for more research characterizing geoelectric fields driven by ULF waves.


ST13-A020
Energetic Electron Microinjections Observed by MMS in the Dusk Plasma Sheet and Drift Resonance Interpretation

Zhekai LUO+, Lun XIE#, Suiyan FU, Zuyin PU, Ying XIONG, Xuzhi ZHOU, Qiugang ZONG, Li LI
Peking University

Microinjection phenomena, characterized by dispersive oscillations of electron fluxes at the Pc5 period and bi-directional pitch angle anisotropy, are frequently observed by MMS in the dusk to midnight plasma sheet. In our work, two such events are analyzed and the features of toroidal mode drift resonance measured meanwhile are shown in detail. The prominent observation is that the fluctuations of the electron flux and the electric field have either -90˚ or +90˚ phase difference at the resonant energy, and the phase difference rises as the energy increases. We extend the theory for drift resonance of toroidal mode wave with only the equatorial moving electrons in a dipole field to include bouncing electrons. The predicted phase differences based on the new theory are consistent well with the observations in the microinjection events. It is thus suggested that drift resonance may act as the forming mechanism for the observed microinjections.


ST13-A008
Off-equatorial Minima Effects on ULF Wave-ion Interaction in the Dayside Outer Magnetosphere

Xingyu LI1+, Zhiyang LIU1, Qiugang ZONG1#, Jianjun LIU2, Suiyan FU1, Xuzhi ZHOU1, Yixin HAO1
1Peking University, 2Polar Research Institute of China

The ultra-low frequency wave-particle drift-bounce resonance in the inner magnetosphere has been studied in detail, due to its important role in particle energization. However, it remains an open question how drift-bounce resonance manifests in the dayside outer magnetosphere, where particles' orbits show bifurcations because of off-equatorial magnetic field minima. Here, we investigate this question, by analyzing 5 years of Magnetospheric Multiscale observations and conducting numerical simulations. A generalized theory is proposed, in which the effects of off-equatorial minima, time-evolving fields and particle bounce motion are taken into account. In the presence of off-equatorial minima, the observed pitch angle-time spectrograms show "paw-track shaped" structures. The time-of-flight effect of particle bounce motion forms latitude-dependent dispersions besides "paw-tracks", while evolving wave fields cause additional time-dependent phase shifts. We find there are more than two resonant pitch angles at fixed energy, since off-equatorial minima change the relationship between the bounce (drift) frequency and pitch angle. These results reveal a new drift-bounce acceleration mechanism in the dayside outer magnetosphere, which potentially affects the efficiency of particle energization during geomagnetic activities like geomagnetic storms.


ST13-A018
Pc4 Cavity Mode Wave Frequency Variation Associated with Inward Motion of the Magnetopause During Interplanetary Shock Compression

Dianjun ZHANG1+, Wenlong LIU1#, Zhao ZHANG1, Xinlin LI2, Theodore SARRIS3, Jerry GOLDSTEIN4, Dmitry SORMAKOV5
1Beihang University, 2University of Colorado Boulder, 3Democritus University of Thrace, 4Southwest Research Institute, 5Arctic and Antarctic Research Institute

A cavity mode wave, referring to a trapped or radially standing fast mode wave between different magnetospheric boundaries, has been developed in theory and reported in observation studies. In this study, we present an interplanetary shock (IPS)-induced cavity mode wave event observed outside the plasmasphere on 31 August 2017 with multispacecraft measurements. The phase delay of 90 degrees between the azimuthal electric field and compressional magnetic field indicates that the fast-mode wave triggered by the IPS is a standing wave, presumably radially trapped in the cavity between the magnetopause and plasmapause. Taking advantage of the location of VAP-B spacecraft right outside the plasmapause and the AARI ground-based high-latitude array mapped in the noon sector, it is suggested that the observed compressional wave associates to cavity mode with its inner boundary at the plasmapause and its outer boundary at the magnetopause. The peak frequency of the wavelet spectrum of the compressional magnetic field increases from 10.5 to 12.5 mHz, which is consistent with the theoretically calculated cavity eigenfrequencies before and after the IPS. We also provide the first evidence that the peak frequency of the cavity mode increases due to the inward motion of the magnetopause during IPS compression.


Tue-01 Aug | 3:30 - 5:15 | MR309
ST16 - Solar Magnetic Fields: Measurements, Extrapolations And (R)MHD Simulations

Session Chair(s): Yingna SU, Purple Mountain Observatory, Chinese Academy of Sciences

ST16-A007 | Invited
Dynamic of Emerging Flux in a Developing Penumbra Observed by GST

Jie ZHAO1#+, Jiangtao SU1, Brigitte SCHMIEDER2, Xu YANG3, Hui LI1, Wenda CAO4
1Chinese Academy of Sciences, 2Observatoire de Paris/ Université PSL/ National Centre for Scientific Research/ Sorbonne Université/ Université de Paris, 3Big Bear Solar Observatory, New Jersey Institute of Technology, 4New Jersey Institute of Technology

With the aid of high-resolution observations from GST, we present an investigation of emergence, coalescence and submergence of magnetic features in the region of a developing penumbra. The results show the emerging flux has magnetic field greater than 500G and is dominated by horizontal component. The kinetic feature shows upflow at the inner part and downflow at the outer part, indicating a pattern of Evershed flow. The magnetic flux emerges accompanying with the expansion of granule, which has several striations inside just like the twisted features found in the penumbra filament (Scharmer et al. 2002). Our analysis shows that although these striations have different properties of magnetic field and kinetics, the one intimately related with the kernel part of the emerging flux show high local twist and vertical current density. By investigating the evolution, it shows the region where the emerging flux emerges and submerges becomes more penumbra-like at the end, i.e., adjacent positive and negative values of elongated magnetic features which parallel with each other, indicating that the dynamic of emerging magnetic flux is important for the development of a mature penumbra. The 3D magnetic field is also investigated in this case.


ST16-A013
Recent Progress on Developing the Magneto-hydro-static Extrapolation

Xiaoshuai ZHU1#+, Thomas WIEGELMANN2
1National Space Science Center, Chinese Academy of Sciences, 2Max Planck Institute for Solar System Research

The magnetohydrostatic (MHS) extrapolation is developed to model the three-dimensional solar magnetic fields as well as plasma with measured vector magnetogram used as boundary condition. It differs from the nonlinear force-free field (NLFFF) extrapolation in that it takes into account plasma forces include pressure gradient and gravity. In this presentation, I will report the recent progress in two aspects on developing the MHS extrapolation. The first one is the development of a preprocessing method to deal with the non-MHS vector magetograms. The reason of doing this is that there are a small number of the vector magnetograms which are not consistent with the MHS equilibria. The second one is the combination of the MHS extrapolation and the NLFFF extrapolation to improve the efficiency of the computation.


ST16-A008
Building a Large-scale Dataset of Three-dimensional Solar Magnetic Fields Extrapolated by Nonlinear Force-free Method

Zhongrui ZHAO+, Long XU, Xin HUANG#
Chinese Academy of Sciences

Limited by the development of computing power, the previously published data sets about the three-dimensional magnetic field of the Solar, especially the magnetic field of the active region, are mainly small number of typical samples. It is difficult to conduct studies of a large number of samples, for example, the comparative study of the three-dimensional evolution of multi-active regions, and the modeling of artificial intelligence-based techniques in the field of computing. So we build a large-scale three-dimensional Solar active regions database based on nonlinear force-free fields (NLFFF) algorithms. This work includes three parts: magnetic field extrapolation, flare labeling, and data and toolkit distribution. Magnetic field extrapolation We used the Wiegelmann's NLFFF extrapolation triple grid algorithm based on Spaceweather HMI Active Region Patch (SHARP) data. We selected 73,000 magnetic field samples at a temporal resolution of 96 minutes between 2010 and 2019. For the batch extrapolation, we designed an efficient task allocation and scheduling algorithm to improve the computational resource utilization. The final product occupies 200 TB which contains most of the typical flares and their samples at multiple time points, offering the possibility of multi-active region comparison and single-active region evolution. In addition, in order to make this database fully accessible to other engineering fields, we have also used GEOS x-rays data to label all samples with multiple forecast modes of flares. We have also developed a platform to publish the dataset, which is available for online viewing and download. To make the work scalable, we open source the code. Through this work, we hope to provide solar physics researchers with a large sample of Solar active regions based on NLFFF algorithms.


ST16-A012
Local Enhancement of a Moreton Wave in the Quiet Sun

Yiwei NI#+, Jinhan GUO, Peng-Fei CHEN, Chuan LI
Nanjing University

Moreton Waves are a large-scale global wave phenomenon generated by solar eruptions, manifested as bright fronts in the Hα line center and blue wing (or dark fronts in the Hα red wing). Generally, Moreton waves are considered as the footprint on the chromosphere of coronal fast-mode shock waves. As the fast-mode shock propagates further away from the eruption source region, the corresponding Moreton wave generally becomes weaker and weaker until it disappears. However, when analyzing an X-class solar flare with the data obtained by the Chinese Hα Solar Explorer (CHASE), we recent found that as the Moreton wave propagates out, the strength of wave front has an abnormal enhancement at a special location. We analyzed the multi-wavelength difference images and perform the global nonlinear force-free field extrapolation, and it is revealed that the special location corresponds to the root of a quasi-separatrix layer (QSL). We propose that the coronal fast-mode shock wave experiences a mode conversion around the QSL, and much of its energy is transferred to a slow-mode wave, which is trapped inside the magnetic field line, leading to the abnormal enhancement of Moreton wave at the footpoint of the QSL


ST16-A015
Closed Magnetic Field Lines Crossing the Coronal Hole Boundaries

Chia-Hsien LIN#+, Guan-Han HUANG
National Central University

Coronal holes (CHs) are regions with unbalanced magnetic flux. The objective of this study is to investigate the characteristics of their magnetic structures. We apply a potential-field (PF) model to construct the magnetic fields of the coronal holes, and, as a comparison, also use a thermodynamic magnetohydrodynamic (MHD) model to synthesize coronal images, and identify CHs from the synthetic images. The results from both models reveal that there is a significant percentage of closed field lines extending beyond the CH boundaries and more than 50% (17%) of PF (MHD) CHs do not contain OMF lines. The boundary-crossing field lines tend to be located slightly closer to the CH boundaries, and are more likely to be found in the lower latitudes during active times. The CHs without open field lines are often smaller and less unipolar than those with open field lines. The main difference between the results of the two models is that the dominant field lines in the PF and MHD CHs are closed and open field lines, respectively.


ST16-A017
Coronal Magnetic Field Measurements Through 2D Coronal Seismology

Zihao YANG1#+, Hui TIAN1, Xianyu LIU1, Steven TOMCZYK2, Richard MORTON3, Sarah GIBSON2
1Peking University, 2National Center for Atmospheric Research, 3Northumbria University

Coronal seismology, a technique of magnetic field diagnostics based on observations of magnetohydrodynamic (MHD) waves, has been widely used to estimate the field strengths of oscillating structures in the solar corona. However, previously coronal seismology was mostly applied to occasionally occurring oscillation events, providing an estimate of only the average field strength or one-dimensional distribution of field strength along an oscillating structure. This restriction could be eliminated if we apply coronal seismology to the pervasive propagating transverse MHD waves discovered with the Upgraded Coronal Multi-channel Polarimeter (UCoMP). Using several UCoMP observations of the Fe XIII 1074.7 nm and 1079.8 nm spectral lines, we obtained maps of the plasma density and wave phase speed in the corona, which allow us to map both the strength and direction of the coronal magnetic field in the plane of sky routinely. We also compared the results with emissivity-weighted magnetic field from PSIMAS models, and confirmed the measured results are emissivity-weighted magnetic field along the line-of-sight. Such measurements could provide critical information to advance our understanding of the Sun’s magnetism and the magnetic coupling of the whole solar atmosphere.


Tue-01 Aug | 3:30 - 5:15 | MR330
ST10 - Kinetic Physics And Multi-scale Dynamics Associated With Magnetic Reconnection

Session Chair(s): Hiroshi HASEGAWA, Institute of Space and Astronautical Science, JAXA

ST10-A014 | Invited
Intense Energy Conversion Events at the Magnetopause Boundary Layer

Meng ZHOU1,2#+, Hengyan MAN1, Xiaohua DENG3
1Nanchang University, 2University of California, Los Angeles, 3Wuhan University

This presentation shows recent results on intense energy conversion events (IECEs) at the dayside magnetopause boundary layer (MBL) using high-resolution data from the Magnetospheric Multiscale (MMS) spacecraft. Most events were detected by MMS in a duration less than 0.5 s, corresponding to a thickness below one ion inertia length. About three-quarters of the events occurred in local reconnecting current sheets. Interestingly, there are more electron-only reconnections than standard reconnections. Most of the reconnection IECEs are within the exhaust of the primary reconnection and the Kelvin-Helmholtz vortices, suggesting that secondary reconnections are important building blocks for the overall energy conversion at the magnetopause. The non-reconnection events are also primarily within the reconnection exhaust and the Kelvin-Helmholtz vortices, highlighting the importance of reconnection and Kelvin-Helmholtz instability in regulating the energy conversion at the MBL.


ST10-A006
Particle Acceleration and Plasma Turbulence in a 3D Current Sheet with Magnetic Islands in PIC Approach

Valentina ZHARKOVA1#+, Qian XIA2
1Northumbria University, 2Culham Centre for Fusion Energy

We investigate using particle-in-cell (PIC) approach particle acceleration and generated kinetic turbulence in a reconnecting current sheet (RCS) with X- and O-nullpoints. We carry out simulations of magnetic reconnection in a thin current sheet with 3D magnetic field topology affected by tearing instability until the formation of two large magnetic islands. The model utilises a strong guiding field that leads to separation of the 8 particles of opposite charges, generation of a strong polarisation electric field across the RCS and suppression of kink instability in the ’out-of-plane’ direction. The accelerated particles of the same charge entering an RCS from the opposite edges are shown accelerated to different energies forming the ‘bump-in-tail’ velocity distributions that generates plasma turbulence in different locations. The turbulence-generated waves produced by either electron or proton beams can be identified from the energy spectra of electromagnetic field fluctuations in the phase and frequency domains. From the phase space analysis we gather that the kinetic turbulence may be generated by accelerated particle beams, which are later found to evolve into a phase-space hole indicating the beam breakage.The collective turbulence power spectra are consistent with the high-frequency fluctuations of perpendicular electric field, or upper hybrid waves, to occur in a vicinity of X-nullpoints, where Langmuir (LW) waves are generated by accelerated electrons wile further from X-nullponts and on the edges of magnetic islands Bernstein waves are formed. Fluctuations of the perpendicular electric field component of turbulence are consistent with oblique whistler waves generated by intense electron beams on the ambient density fluctuations.


ST10-A008
Scalable Simulations of 3D Turbulence Fine Structure in Nanoflare Using a Novel Plasma Statistical Algorithm

Bojing ZHU#+
Chinese Academy of Sciences

Based on algorithms of solving directly MHD partial differential equation algorithm, conventional simulation methods cannot attain the extreme range of scale for 3D turbulence fine-structure in flare-CME phenomena, especially for nanoflare heating problems. Here we present a parallel lattice Boltzmann algorithm based on plasma statistical physics, which allows us to reach even the relativistic regime necessary for modeling 3D turbulence fine-structure evolution. This innovative approach can simultaneously describe the continuous features of plasma at the macro-spatio-temporal scale, particle features of plasma at the micro-spatio-temporal scale, and particle features enforced by magnetic fields. However, the novel algorithm brings several challenges for fine-structure large-scale simulation, such as the gargantuan memory and storage requirements due to high dimensions and output data, and long simulation time, because each run takes a week. We propose optimization technologies for data access, communication, I/O, etc. These optimizations make it possible to achieve scalable and robust simulation (using up to 100,000 cores on the Tianhe-2 supercomputer) and the most extensive system ever run. For the first time, we can analyze the 3D turbulence fine structure by interacting with plasmas and magnetic fields in nanoflare.


ST10-A009 | Invited
MESSENGER Observations of Reconnection in Mercury's Magnetotail Under Strong IMF Forcing

Jun ZHONG1#+, L. C. LEE2, James SLAVIN3, Hui ZHANG4, Yong WEI1
1Institute of Geology and Geophysics, Chinese Academy of Sciences, 2Academia Sinica, 3University of Michigan, 4Chinese Academy of Sciences

The MESSENGER spacecraft typically crossed Mercury's magnetotail current sheet relatively close to the planet, that is, less than 2.5 RM (planet radius; 2,440 km). Magnetometer measurements are used to detect active reconnection events by identifying the quadrupole Hall magnetic field signatures that form about X-lines. Statistical analyses of the 51 active reconnection events detected in this manner indicate that they occur most frequently on the duskside and typically at a mean altitude greater than 1.5 RM. In contrast, the dawnside events occur at altitudes of ~1 RM. In addition, a higher recurrence rate of flux ropes formed in the Hall region was observed on the dawnside. Applying the Kan-Lee solar wind-magnetosphere coupling function confirmed that these near-tail reconnection events at Mercury are observed under strong forcing by the interplanetary magnetic field. We further propose that the reconnection-driven nightside magnetosphere-planet interaction is characterized by a pronounced dawn-dusk asymmetry and may significantly influence the near-Mercury space environment.


ST10-A026
Auroral Spiral Structure Formation Through Magnetic Reconnection in the Auroral Acceleration Region

Kai HUANG1#+, Yi-Hsin LIU2, Quanming LU1, Zejun HU3, Kristina LYNCH2, Michael HESSE4, Andris VAIVADS5, Huigen YANG3
1University of Science and Technology of China, 2Dartmouth College, 3Polar Research Institute of China, 4NASA Ames Research Center, 5KTH Royal Institute of Technology

Discrete aurorae, usually displayed as auroral arcs, are universal phenomena in the ionosphere of the Earth and other planets, and are generated by precipitations of electrons from the magnetosphere, ionosphere, and solar wind. Spirals, as frequently observed vortex structures in arcs, have drawn great attention. The formation of auroral spirals is considered to be related to the magnetosphere-ionosphere coupling process during both magnetically active and quiet times. However, how the auroral spirals develop is still an open question. It is suggested that magnetic reconnection occurs in the auroral acceleration region, typically above ∼4,000 km altitude in the field-aligned current sheet. Using particle-in-cell simulations, we study the role of magnetic reconnection in the formation of auroral spirals. We propose a model to explain the formation of auroral spiral structure. In our model, an auroral arc develops through precipitations of electrons accelerated during magnetic reconnection in the auroral acceleration region. The arc morphology at low altitudes can be modified by electron-scale magnetic flux ropes, which are generated through secondary oblique tearing modes in the intensified current sheet along one particular branch of the primary reconnection separatrices. The resulting vortex structures agree well with high-resolution observations of auroral spirals. We find that the rotational sense of these spirals is determined by electron kinetic processes and controlled by the guide field direction. Our study further suggests that when the field-aligned length of the auroral acceleration region is shorter than a critical length, these auroral spiral structures will not form.


ST10-A016
Sub-structures of the Separatrix Region During Magnetic Reconnection

Kui JIANG+, Shiyong HUANG#, ZhiGang YUAN, Xiaohua DENG, Yunyun WEI, Qiyang XIONG, Sibo XU, Jian ZHANG, Zehao ZHANG, Rentong LIN, Lin YU
Wuhan University

Utilizing data from the Magnetospheric Multiscale mission, the sub-structures of the separatrix region during reconnection are investigated. A small current system in the separatrix region is embedded in the large Hall current system, which appears as a quadrupole current. This small current system has an opposite direction to the Hall current and cancels part of the Hall magnetic field. The formation of the quadrupole current is possibly related to the patchy parallel electric field. The electric field in the separatrix region can be divided into three sub-layers according to the electron frozen-in condition. En enhances in two outside sub-layers, where the strong En is supported by the Hall term and electron pressure gradient term, and the nearly zero En, separating the enhanced electric fields, is caused by a small flow and electron density gradient. Our observations imply complex dynamics in the separatrix region during magnetic reconnection.


Tue-01 Aug | 3:30 - 5:15 | MR333
ST13 - ULF Waves in Geospace: Investigating Wave Generation, Propagation and Wave-particle Interaction Through Observations, Simulation and Theory

Session Chair(s): Xueling SHI, Virginia Tech

ST13-A006 | Invited
Excitation of Drift-compressional Mode Waves by Drift Resonance with Ring Current Ions: Arase Observation

Kazuhiro YAMAMOTO1#+, Aleksandr RUBTSOV2, Danila KOSTAREV2, Pavel MAGER2, Dmitri KLIMUSHKIN2, Masahito NOSÉ3, Ayako MATSUOKA4, Kazushi ASAMURA5, Yoshizumi MIYOSHI3, Shoichiro YOKOTA6, Satoshi KASAHARA1, Yoshiya KASAHARA7, Atsushi KUMAMOTO8, Fuminori TSUCHIYA8, Masafumi SHOJI3, Satoko NAKAMURA3, Iku SHINOHARA5
1The University of Tokyo, 2Institute of Solar-Terrestrial Physics of the Siberian Branch of the Russian Academy of Sciences, 3Nagoya University, 4Kyoto University, 5Japan Aerospace Exploration Agency, 6Osaka University, 7Kanazawa University, 8Tohoku University

Compressional Pc 5 waves are important for the energy dynamics in the terrestrial inner magnetosphere because they can accelerate the relativistic electrons (Ukhorskiy et al., 2009). One of the origins of compressional Pc 5 waves is local plasma instability, but the generation mechanism of the compressional Pc 5 waves is still controversial. Recently, drift compressional instability has been focused on because it can generate compressional waves even if plasma beta is less than unity (Rubtsov et al., 2018; Mager et al., 2019; Takahashi et al., 2022). However, its wave property and excitation mechanism are not fully understood due to the lack of observation. This study first reports the role of drift resonance in the excitation of drift compressional waves by analyzing the compressional Pc 4-5 waves observed by the Arase satellite at L ~6 and ~21 MLT around the magnetic equator on 19th November 2018. Plasma beta reached ~1 but the instability threshold of the drift mirror instability was not satisfied. From the theoretical calculations of the wave frequency (Mager et al., 2013) and pressure perturbation (Takahashi et al., 2022), we concluded that the observed wave is the drift compressional mode. We estimated the azimuthal wave number (m number) from the finite Larmor radius effect and obtained m ~ -140. This is consistent with the drift resonance with protons at 20-30 keV, whose fluxes showed the most coherent oscillations. We examined whether the drift resonance also contributes to wave excitation or not, while there was a positive ion temperature gradient that can excite drift compressional waves. We found that an inward phase space density gradient and positive df/dW sometimes appeared, which indicates that the drift resonance gives free energy to the wave, where f and W are phase space density and energy, respectively.


ST13-A013 | Invited
The Correlation Study of Pc5 ULF Waves in High-latitudes Between East Antarctic and West Greenland Magnetometer Chains

Zhonghua XU1#+, Michael HARTINGER2, Hyomin KIM3, Shane COYLE4, Sungjun NOH3, Daniel WEIMER4, Doğacan S. ÖZTÜRK5, Ilya KUZICHEVE3, James WEYGAND6, Robert CLAUER4
1Virginia Tech, 2Space Science Institute, 3New Jersey Institute of Technology, 4Virginia Polytechnic Institute and State University, 5University of Alaska, Fairbanks, 6University of California, Los Angeles

In the Earth’s Magnetosphere-Ionosphere (MI) system, ULF waves are known to affect magnetospheric dynamics immediately during magnetic storms in high latitude regions. The interhemispheric asymmetries in these regions are shown by the observations from East Antarctica and West Greenland magnetometer arrays at such high-latitudes. There are a variety of dynamics related to the observed interhemispheric asymmetric signatures, such as solar wind conditions, boundary between open and closed magnetic field lines, auroral patterns and electrojets, ionospheric conductivity and others. It is crucial to understand how each source of asymmetry interacts with each other and how asymmetric structures incorporate this information in a global picture. In this study, the magnetic field variations observed at East Antarctica and West Greenland are analyzed to identify the spatiotemporal characteristics and magnitudes of interhemispheric asymmetries in high-latitudes. The correlations surveys at the similar magnetic coordinate locations are compared under different Solar Wind-Magnetospheric-Ionospheric (SWMI) and seasonal changes of conductivity to investigate the causes of asymmetric processes. These results would be helpful to understand the space weather predictions in global view.


ST13-A001
The Role of Wave Cross-scale Coupling in Particle Dynamics in the Earth’s Magnetosphere and the Solar Wind

Chris COLPITTS1#+, Sadie ELLIOTT1, Cynthia CATTELL1, Theo MAHAFFEY1, Corie GUGGEMOS1, Mike JOHNSON1, Bale STUART2, David MALASPINA3
1University of Minnesota, 2University of California, Berkeley, 3University of Colorado Boulder

We present observations of modulation of higher frequency waves (lower hybrid, whistler mode, magnetosonic, ion acoustic) by lower frequency waves (electromagnetic ion cyclotron, ultra-low frequency) in the Earth’s magnetosphere including the radiation belts, plasma sheet boundary layer, and magnetotail, as well as in the solar wind. This cross-scale coupling links the vastly different ion and electron temporal and spatial scales, and can have dramatic effects on wave-particle interactions. Such modulations can have a significant impact on the formation and depletion of Earth’s radiation belts, and the mechanisms that control the heat flux in the solar wind. We have recently developed a new automated technique to identify modulations in the RBSP data using the filterbank data products, and found that such modulation is considerably more common than previously understood. Similar modulations were observed in MMS measurements taken in the radiation belts and elsewhere in the magnetosphere, as well as PSP measurements in the solar wind. We will run the algorithm for the entire RBSP dataset, as well as PSP, which also includes a filterbank data product, to catalog all of the modulated events. We are developing an MMS analog to the RBSP filterbank data which will be then used to automatically detect modulated wave events. This will produce a database of all modulated events and characteristics of the waves and plasma environment including geomagnetic conditions, which will allow us to determine the prevalence of this process and under which conditions it can occur. We will also perform event studies investigating the details of the distribution functions, composition, and wave properties, as well as ray tracing studies, to quantify the effects of the modulation on particle dynamics. Lastly, we will conduct comparative studies between events at Earth and those observed in the solar wind by PSP.


ST13-A004
Characteristics of Electron Precipitation Directly Driven by Poloidal ULF Waves

Ze-Fan YIN1+, Xuzhi ZHOU1#, Wen LI2, Xiaochen SHEN3, Robert RANKIN4, Ji LIU4, Zejun HU5, Jianjun LIU5, Qiugang ZONG1, Li LI1, Yongfu WANG1
1Peking University, 2Boston University, 3Shandong University, 4University of Alberta, 5Polar Research Institute of China

A mechanism recently proposed for magnetospheric electron loss into the atmosphere is the precipitation directly driven by ultralow-frequency (ULF) waves. In this study, we quantitatively analyze the properties of ULF wave-induced precipitation by simulating the electron bounce and drift motion in poloidal-mode waves excited in a dipole magnetic field. Our results reveal that precipitation occurs only when electrons encounter a westward-directed wave electric field in the magnetosphere, which leads to cross-field energy enhancements and reduces their mirror heights. The simulations also demonstrate longer duration electron precipitation at the drift-resonance energy. We calculate the temporal variations of the energy spectrum for precipitating electrons and the total precipitating energy fluxes. These results improve our understanding of ULF wave-induced electron precipitation as well as provide a point of comparison for observations from balloons or ground-based instruments.


ST13-A005
Simulating the Global Distribution of Particle Precipitation in Response to ULF Waves

Long Xing MA#+, Yiqun YU, Wenlong LIU, Jinbin CAO
Beihang University

The global distribution of particle precipitation is closely related to the formation and evolution of aurora. ULF waves in the magnetosphere are believed to contribute to the particle scattering and subsequent precipitation down to the upper atmosphere, resulting in the auroral arcs, and the fluctuations of auroral intensity. In this study, we investigate the global distribution of both ion and electron precipitations using our ring current model considering the role of ULF waves during the September 2017 geomagnetic storm. We compare the different responses of trapped and precipitating particles to ULF waves in the main phase and recovery phase of the storm and find that the significant effects of ULF waves on precipitating particles occur on the dawn-dusk side during the main phase while on the dayside during the recovery phase. The precipitating fluxes of low-energy and high-energy electrons and low-energy protons are significantly modulated by ULF waves.


ST13-A014
Solar Wind Dynamic Pressure Fluctuation Driven Electromagnetic Energy Input to the Ionosphere-thermosphere Under Northward Interplanetary Magnetic Field

Dong LIN1#+, Wenbin WANG1, Xueling SHI2,1, Michael HARTINGER3, William LOTKO1, Roger VARNEY4, Michael WILTBERGER1, Joseph BAKER2, Kevin PHAM1, Viacheslav MERKIN5, Kareem SORATHIA5, Shibaji CHAKRABORTY2
1National Center for Atmospheric Research, 2Virginia Tech, 3Space Science Institute, 4University of California, Los Angeles, 5Johns Hopkins University Applied Physics Laboratory

Alfvenic Poynting flux is an important pathway to transmit electromagnetic energy from the magnetosphere to the ionosphere-thermosphere. Previous studies have shown that Alfvenic Poynting flux is preferential on the nightside under southward interplanetary magnetic field (IMF) when earthward bursty bulk flows break and convert kinetic energy into electromagnetic energy. Under northward IMF when the tail activity is relatively quiet, solar wind energy can be still transferred into geospace. Solar wind dynamic pressure (Pd) fluctuations are known to drive dayside magnetospheric ultra-low frequency (ULF) waves. Magnetopause oscillations due to Pd fluctuation launch compressional magnetohydrodynamic (MHD) waves in the dayside magnetosphere which propagate isotropically. Compressional waves couple with field line resonance (FLR) mode where the eigen frequency matches the source frequency. Field-aligned Alfvenic Poynting flux associated with FLR becomes an important mechanism of transmitting solar wind energy to the ionosphere under northward IMF. In this study, we use the Multiscale Atmosphere-Geospace Environment (MAGE) model to carry out idealized numerical simulations of Alfvenic Poynting flux driven by oscillating solar wind dynamic pressure under northward IMF. We will investigate the energy transfer efficiency due to solar wind fluctuations and its dependence on spatial location, the source frequency, and ionospheric conductance. This study aims to quantify the importance of a special energy transfer pathway under northward IMF.


Wed-02 Aug | 10:20 - 12:20 | MR332
ST16 - Solar Magnetic Fields: Measurements, Extrapolations And (R)MHD Simulations

Session Chair(s): Xiaoshuai ZHU, National Space Science Center, Chinese Academy of Sciences

ST16-A020 | Invited
MHD Simulation of Solar Eruption Initiation in Multipolar Magnetic Field

Chaowei JIANG1#+, Xinkai BIAN1, Xueshang FENG2
1Harbin Institute of Technology, Shenzhen, 2Chinese Academy of Sciences

Recently we established a fundamental mechanism of solar eruption initiation, in which an eruption can be initiated from a bipolar field through magnetic reconnection in the current sheet (CS) that is formed slowly in the core field as driven by photospheric shearing motion. Here using a series of fully 3D MHD simulations with a range of different photospheric magnetic flux distributions, we extended this fundamental mechanism to the quadrupolar magnetic field containing a null point above the core field, which is the basic configuration of the classical breakout model. As is commonly believed, in such multipolar configuration, the reconnection triggered in the CS originated at the null point (namely, the breakout reconnection) plays the key role in eruption initiation by establishing a positive feedback-loop between the breakout reconnection and the expansion of the core field. However, our simulation showed that the key of eruption initiation in such multipolar configuration remains to be the slow formation of the CS in the sheared core rather than the onset of fast breakout reconnection. The breakout reconnection only helps the formation of the core CS by letting the core field expand faster, but the eruption cannot occur when the bottom surface driving is stopped well before the core CS is formed, even though the fast reconnection has already been triggered in the breakout CS. This study clarified the role of breakout reconnection and confirmed formation of the core CS as the key to the eruption initiation in a multipolar magnetic field.


ST16-A001 | Invited
Three-dimensional Turbulent Reconnection Within Solar Flaring Current Sheet

Yulei WANG#+
Nanjing University

Solar flares can release coronal magnetic energy explosively and may impact the safety of near-earth space environments. The popular standard flare model, based on magnetic reconnection theory, has interpreted many macro-scale observational features successfully but failed to explain fine dynamical structures in recent high-resolution observations. Here, we achieve a self-consistent high-resolution three-dimensional magnetohydrodynamical simulation of turbulent magnetic reconnection within a flare current sheet. It is found that fragmented current patches of different scales are spontaneously generated with a well-developed turbulence spectrum at the current sheet, as well as at flare loop-top region. The close coupling of tearing mode and Kelvin-Helmholtz instabilities plays a critical role in developing turbulent reconnection and in forming dynamical structures above the flare loop top as often observed but still unsolved. This sophisticated modeling provides a direct physical link from small-scale turbulent reconnection to large-scale flare phenomena, revolutionizing the well-established standard flare model.


ST16-A010
Field-aligned and Magnetic Reconnection Flows in a Magnetohydrodynamic Simulation of Prominence-cavity System

Tie LIU1#+, Yingna SU2, Yang GUO1, Jie ZHAO3, Haisheng JI3
1Nanjing University, 2Purple Mountain Observatory, Chinese Academy of Sciences, 3Chinese Academy of Sciences

Nested ring-shape line-of-sight (LOS) oriented flows in coronal cavities are observed in recent years but rarely explained. Using a magnetohydrodynamic simulation of a prominence-cavity system, we investigate the relationship between the simulated field-aligned flows, magnetic reconnection flows and the LOS-oriented flows observed by the Coronal Multi-Channel Polarimeter. The field-aligned flows are along magnetic field lines towards the dips and driven by the hydrodynamic forces exerted by the prominence condensation. The reconnection flows are driven by the overlying reconnection and tether-cutting reconnection. The velocity of the reconnection flows increases from the quasi-static phase to fast rise phase, reaching several km s −1, which is similar to the speed of the field-aligned flows. We calculate the synthetic Doppler images by forward modeling and compare them with the observed LOS-oriented flows. The LOS-oriented flows of one ring with opposite internal flow driven by the field-aligned flows are found in this simulation, and the synthetic Doppler images of different LOS with the included angle of about 10◦ can resemble the observed direction reversal of the LOS-oriented flows in about 20 hours. These findings suggests that the observed LOS-oriented flows of one ring with opposite internal flow may be due to the LOS integration effect of field-aligned flows along different loops.


ST16-A018
On the Dynamics of a Confined Eruption of a Magnetic Flux Rope Based on Radiative Magnetohydrodynamic Simulation

Can WANG#+, Feng CHEN, Mingde DING, Zekun LU
Nanjing University

It is known that magnetic flux rope acts as the key to driving solar eruptions, which include solar flares and coronal mass ejections. However, some flares are not associated with CMEs, which are usually called confined eruptions. Here, we analyse a confined eruption of a flux rope in a three-dimensional radiative magnetohydrodynamic simulation conducted with the MURaM code, focusing on the forces controlling its dynamic evolution. Before the flare onset, the flux rope undergoes a slow-rise phase with a velocity of a few km/s, during which the counterbalance between gravity and Lorentz force sustains its quasi-static evolution. Once the flux rope reaches a height where the condition of torus instability is satisfied, the Lorentz force begins to dominate its dynamics, resulting in a transition from the slow-rise phase to the main-acceleration phase. Fast magnetic reconnection is then induced within the current sheet under the flux rope, further enhancing the Lorentz force and providing a positive feedback to the eruption. The main-acceleration phase of flux rope is almost simultaneous with the impulsive flare phase, during which the flux rope accelerates to more than 400 km/s. Although the external toroidal field above is still in a torus-unstable regime, the flux rope is eventually prevented from a successful eruption by Lorentz force components other than the strapping force, which may include the constraining force from its nonaxisymmetry and the tension force from the external guide field. Magnetic reconnection between the flux rope and external field may also contribute to the confinement of eruption. Our results suggest that the gravity of flux rope plays an important role during the slow-rise phase, while the onset and confinement of the eruption are dominated by the Lorentz force from both ideal magnetohydrodynamic instability and magnetic reconnection.


ST16-A023
Unveiling the Mechanism for the Rapid Acceleration Phase in a Solar Eruption

Ze ZHONG1#+, Yang GUO2, Thomas WIEGELMANN3, Mingde DING2, Yao CHEN1
1Shandong University, 2Nanjing University, 3Max Planck Institute for Solar System Research

Early kinematics of solar eruptions are usually characterized by a rapid acceleration phase. Two proposed mechanisms may drive the solar eruptions: the ideal magnetohydrodynamic (MHD) instability and the resistive magnetic reconnection. Due to coupling of the two mechanisms, their respective contribution remains elusive in a real situation. Here, we report a data driven MHD modeling for the flux rope eruption on 2011 August 4, by inputting a time series of photospheric magnetograms. Major observations of the eruption, such as the macroscopic morphology, early kinematics of the flux rope and flare ribbons, match well with the simulation. We estimate the energy converted from the large-scale Lorentz force acting on the flux rope and the effect of magnetic slingshot above the current sheet during the rapid acceleration phase, and find that (1) the work done by the large-scale Lorentz force is about four times higher than the latter to drive the eruption, (2) decreased strapping force generated by the overlying field facilitates the eruption. We suggest that the loss of equilibrium associated with the large-scale Lorentz force is the key player in the rapid acceleration for solar eruptions.


ST16-A014
Formation Mechanism of the Filament as Observed

Haitang LI1#+, Xin CHENG1, Jinhan GUO1, Xiaoli YAN2
1Nanjing University, 2Yunnan Observatories, Chinese Academy of Sciences

Solar filament, as an important manifestation of solar activities, is believed to be the pre-eruptive configuration of coronal mass ejections. It can be divided into two components, the cool filament materials and filament channel, a plasma volume where the magnetic field is primarily aligned with the polarity inversion line. There have been many numerical simulations focus on the formation and eruption of the magnetic flux rope, which generally deemed to be filament channel. Nevertheless, observational evidence of the filament formation mechanism is still elusive. In this talk, I will present a detailed study on the formation of the filament to understand its formation mechanism, including the build-up of filament channel and the supplement of filament materials. It shows the filament channel, likely a hybrid state with sheared arcades and twisted fluxes coexisting, is gradually built up via a series of small-scale reconnection events as intermittently appeared Ha/EUV bursts and is closely associated with the rapid flux cancellation. In addition, the chromospheric plasm is continuously evaporated into the corona and condensed along the filament channel to supplement the filament materials, of which the drainages expectedly produce red doppler shift at the filament footpoints as observed in Ha spectrogram.


ST16-A016
Association Between Magnetic Pressure Difference and Movement of Solar Pores

Merlin MENDOZA#+, Chia-Hsien LIN
National Central University

Solar pores are associated with the concentration, dissipation, and transportation of solar magnetic fluxes. Their observable characteristics can provide important constraints to improve models and simulations of magnetic flux emergence and formation. In this work, we have investigated the horizontal movements of solar pores. The goal is to probe possible correlations of observable quantities with the movement of the pore. Our statistical analysis on 61 compact pores identified from the Spaceweather HMI Active Region Patches from 2011 to 2018 shows that the direction of movement is either parallel or anti-parallel to the direction of maximum magnetic pressure difference at the opposite sides of the edges of the pores. The correlation coefficients for both parallel and anti-parallel cases are both higher than 0.74. Despite having a high correlation, our information theoretic analysis using transfer entropy indicates no significant causal relationship between the direction of motion and the direction of maximum magnetic pressure difference.


Wed-02 Aug | 10:20 - 12:20 | MR333
ST17 - Emic Waves and Their Effect on Particle Dynamics

Session Chair(s): Dedong WANG, GFZ German Research Centre for Geosciences

ST17-A010 | Invited
Role of Source Regions Conditions on Occurrence Characteristics and Modulations in Electromagnetic Ion Cyclotron (EMIC) Waves Observed from Ground

Aditi UPADHYAY#+, Bharati KAKAD, Amar KAKAD
Indian Institute of Geomagnetism

The EMIC waves are the traverse plasma waves observed in the Earth’s magnetosphere. They can resonate with electrons with a wide energy range, from 500 keV to hundreds of MeV, and are also known to cause isolated proton auroras which is a result of their interaction with the ring current ions. The EMIC waves are typically generated by the temperature anisotropy (T > T||) of medium energy (1 - 100 keV) ring current protons. There can be multiple reasons for the enhancement in the anisotropy of the ions, one of the recognized sources being the energetic particle injections into the inner magnetosphere during storms and substorms. Another possible source is solar wind pressure. We are presenting the effect of the solar wind pressure and auroral electrojet indices on the local time distribution of EMIC waves in different frequency ranges using long-term ground observations (2011-2017) from the Indian Antarctic station, Maitri (L~ 5). Moreover, the presence of special features like modulations in EMIC wave has also been reported by various satellite missions and ground magnetometers. We have also examined this aspect using from the same dataset and report a statistical analysis of the modulation of EMIC waves by short and long periodicities. We have identified 6845 EMIC wave events and of them, 80% showed the presence of short periodicities and 35% showed the presence of long periodicities. The duration of the short period decreases with an increase in the peak frequency of the EMIC wave, whereas the variation in long periods is attributed to the decrease in the magnetic field line oscillation period at lower L-shells. We have validated the observed trends using nonlinear theory. Such a study is important to improve our overall understanding of EMIC wave generation and modulation.


ST17-A009
Simulating Simultaneous Satellite and Ground Observations of EMIC Waves

Robert RANKIN#+
University of Alberta

Electromagnetic ion cyclotron (EMIC) waves are important because of their essential role in reducing the amount of radiation in the Earth's radiation belts under geomagnetic storm conditions. In this presentation, we show results from a new simulation model of EMIC waves and compare them with SWARM satellite data and ground-based observations [I. P. Pakhotin et al., Geophys. Res. Lett., 2022, doi:10.1029/2022GL098249]. The EMIC wave model is a first-of-a-kind in accounting for wave propagation in the magnetosphere and a realistic ionosphere specified using the IRI and MSIS empirical models. Including a realistic ionosphere in the model enables new pathways to the upper atmosphere to be identified, which is crucial for understanding the waves detected on the ground. We show using a model-data comparison that EMIC wave energy is reflected at different locations in the ionosphere toward the equator to form standing waves. This is a new resonance phenomenon created by interference of waves that produces an amplitude peak in the upper atmosphere at lower latitudes, far from the location of the initial source. Understanding such pathways is crucial for correctly diagnosing the location of EMIC wave populations in space and assessing their role in radiation belt loss.


ST17-A001 | Invited
Modeling the Simultaneous Dropout of Energetic Electrons and Protons by EMIC Wave Scattering

Weichao TU1#+, Xingzhi LYU1, Qianli MA2, Wen LI2, Luisa CAPANNOLO2
1West Virginia University, 2Boston University

Recent observations by NASA Van Allen Probes have revealed concurrent and fast dropout of both radiation belt (RB) electrons and ring current (RC) protons. Theoretically, electromagnetic ion cyclotron (EMIC) waves could cause a simultaneous dropout of radiation belt electrons and ring current protons. However, their effects on the dropout of both plasma populations have not been quantified in previous studies. In this work, we model the simultaneous dropout of MeV electrons and 100s keV protons observed by Van Allen Probes within ~40 min on 27 February 2014. The wave and particle measurements during the period of most intense EMIC waves at L ~ 5.2 are used to calculate the quasilinear diffusion coefficients and simulate the evolution of both energetic electrons and protons. Our model well captures the dropout of electrons with energies > 1 MeV and pitch angles < 75°, and the concurrent dropout of protons with energies > 200 keV and pitch angles > 40°. This is the first modeling work quantitatively reproducing the simultaneous dropout of both populations due to EMIC wave scattering.


ST17-A007
Simultaneous Macroscale and Microscale Wave–ion Interaction in Near-earth Space Plasmas

Zhiyang LIU1#+, Qiugang ZONG1, Robert RANKIN2, Hui ZHANG3, Yongfu WANG1, Xuzhi ZHOU1, Suiyan FU1, Chao YUE1
1Peking University, 2University of Alberta, 3SHANDONG UNIVERSITY (Weihai)

Identifying how energy transfer proceeds from macroscales down to microscales in collisionless plasmas is at the forefront of astrophysics and space physics. It provides information on the evolution of involved plasma systems and the generation of high-energy particles in the universe. Here we report two cross-scale energy-transfer events observed by NASA’s Magnetospheric Multiscale spacecraft in Earth’s magnetosphere. In these events, hot ions simultaneously undergo interactions with macroscale ultra-low-frequency waves and microscale electromagnetic-ion-cyclotron (EMIC) waves. The cross-scale interactions cause energy to directly transfer from macroscales to microscales, and finally dissipate at microscales via EMIC-wave induced ion energization. The direct measurements of the energy transfer rate in the second event confirm the efficiency of this cross-scale transfer process, whose timescale is estimated to be roughly ten EMIC-wave periods about (1 min). Therefore, these observations experimentally demonstrate that simultaneous macroscale and microscale wave-ion interactions provide an efficient mechanism for cross-scale energy transfer and plasma energization in astrophysical and space plasmas.


ST17-A004 | Invited
Modeling Electron Variability Induced by EMIC Waves

Lunjin CHEN#+
The University of Texas at Dallas

Electromagnetic ion cyclotron waves have been known as one of major loss mechanisms in the radiation belts during storm times. In addition to slower quasi-linear scattering, nonlinear wave-particle interaction due to the large amplitude of EMIC waves has attracted attention. Several nonlinear mechanisms—phase trapping, phase bunching, and boundary reflection effects—have been suggested to affect relativistic electrons in terms of advection and diffusion processes rather than the diffusion process alone in the quasi-linear theory. Observationally, such type of pitch angle distribution has been identified in the presence of strong EMIC wave amplitude. Here the interaction of EMIC waves with energetic electrons is investigated using test particle simulation to examine signatures in electron flux variations due to EMIC wave scattering. The simulated pitch angle distribution near the equator due to EMIC wave scattering exhibits a secondary peak just above the loss cone, which is consistent with the observation. In addition, we examine electron precipitation patterns due to EMIC waves, by placing two virtual particle detectors at north and south ionospheric footpoints, respectively. Two different precipitation patterns induced by EMIC waves are found, one with significant energy dispersion in the precipitation flux and the other one with no energy dispersion at lower energy. The two precipitation patterns are attributed to resonant and non-resonant scattering processes, respectively. The results will be valuable for understanding the variability of electron precipitation fluxes observed by low-earth-orbit satellites.


ST17-A002 | Invited
Quasilinear and Nonlinear Interactions Between Intense Electromagnetic Ion Cyclotron Waves and Radiation Belt Electrons and Ring Current Protons

Qianli MA1,2#+, Miroslav HANZELKA3, Wen LI2, Jacob BORTNIK1, Longzhi GAN2
1University of California, Los Angeles, 2Boston University, 3GFZ German Research Centre for Geosciences

Intense electromagnetic ion cyclotron (EMIC) waves with magnetic amplitudes higher than 1 nT frequently occur in the Earth's magnetosphere. Satellite observations and radiation belt modeling have demonstrated the key role of EMIC waves in dropout and long-term decay of relativistic electron and ring current proton fluxes and in the heating of cold electrons and thermal protons when the waves are oblique. Quasilinear theory predicts well the loss rate of relativistic electrons and ring current protons due to the pitch angle scattering induced by EMIC waves, including the resultant particle pitch angle distribution, supported by satellite observations. However, the large amplitude of EMIC waves raises the question of whether the quasilinear assumption applies to the entire pitch angle and energy space. Many previous models focused on the EMIC wave effects due to the first-order cyclotron resonance because the resonance energy matches the energies of relativistic electrons or ring current protons. The satellite observations show that the EMIC waves could have large wave normal angles, which may induce higher-order harmonic resonances and Landau resonance. We present the recent modeling of the interaction between EMIC waves and energetic particles in the Earth's outer radiation belts. A series of test particle simulations are performed to resolve the variations of particle pitch angle and energy along the bouncing trajectory. The scattering rates and advection rates are obtained from the simulations and compared with quasilinear modeling results. We also perform test particle simulations with large wave normal angles to examine the potential effects of higher-order resonances and Landau resonance. A monochromatic wave is adopted in our simulations, which differs from the observed wave spectra; nevertheless, our simulations demonstrate the potential nonlinear resonant effects due to intense EMIC waves.


ST17-A003
Anomalous Resonance Between Low-energy Particles and Electromagnetic Plasma Waves

Jinghuan LI#+, Xuzhi ZHOU, Zhiyang LIU, Li LI
Peking University

Cyclotron resonance between plasma waves and charged particles is a fundamental and ubiquitous process in the plasma universe, during which the particle’s gyromotion has a constant phase in the wave field to enable a sustained energy exchange. In this classical picture, however, the particle’s angular velocity is determined only by the background magnetic field. Here, we show that the classical condition of cyclotron resonance fails to describe the observations of low-energy particles in resonance with large-amplitude waves, which highlights the roles of the wave field in nonlinearly modifying the resonant picture. The revised scenario of anomalous resonance is then validated by the agreement between test-particle simulations and ultrafast spacecraft measurements, which present in-phase and/or antiphase relationships between the wave magnetic field and ion flux oscillations at energy and pitch-angle ranges incompatible with the classical resonance condition. This revision could significantly affect the wave-particle energy exchange and wave evolution processes.


ST17-A006
Amplitude-dependent Properties and Excitation Mechanisms of EMIC Waves in the Earth’s Inner Magnetosphere

Yun YAN+, Chao YUE#, Ze-Fan YIN, Xuzhi ZHOU, Qiugang ZONG, Jinghuan LI
Peking University

Large-amplitude (Bw > 1 nT) electromagnetic ion cyclotron (EMIC) waves can cause the rapid loss of > 1MeV electrons, greatly impacting radiation belt dynamics. With long-term Van Allen Probe B observations from 2013 to 2018, we conducted a statistical survey to reveal the amplitude-dependent wave properties and excitation mechanisms of EMIC waves in the Earth’s inner magnetosphere. Statistical results show that large-amplitude EMIC waves prefer to occur in the afternoon-dusk sector and tend to be more left-hand polarized with smaller wave normal angles. In addition, the high proton parallel beta conditions also favor the generation of EMIC waves with larger amplitude. With the variation of EMIC wave occurrence rate as a function of SME index and solar wind dynamic pressure, we find that small-amplitude EMIC waves prefer high solar wind dynamic pressure conditions, while large-amplitude EMIC wave generation is more influenced by strong substorm activity, and these two conditions have almost the same effects on medium-amplitude EMIC wave excitation. The normalized magnetic field perturbations during EMIC wave appearance, which enable us to distinguish the relative roles of magnetospheric compression and substorm injection in the excitation of different-amplitude EMIC waves, further provide direct evidence that as wave amplitude increases, substorm injection plays a more important role in EMIC wave excitation, and magnetospheric compression is also an indispensable trigger.


Wed-02 Aug | 1:00 - 5:15 | Summit
ST - Solar and Terrestrial Sciences Poster Session

ST01-A005
Suprathermal Electron Spectra at the Earth's Bow Shock

Xinnian GUO#+, Linghua WANG, Zixuan LIU, Liu YANG
Peking University, China

We present a comprehensive study of the in situ electron acceleration during 138 terrestrial bow shock crossings with good suprathermal electron observations by the Wind/3DP instrument from 1994 to 2004. For all 138 cases, we obtain the shock parameters from the nonlinear least-square shock fitting techniques and fit the observed omnidirectional electron flux JA (JD) at suprathermal energies at ~0.1-200 keV in the ambient solar wind (downstream) to a generalized triple-power-law energy function. According to the electron spectrum fitting results, we find that the downstream suprathermal electrons generally have three types of spectra: single-power-law spectrum, double-power-law spectrum, and triple-power-law spectrum. Furthermore, for significant shock electron acceleration (JD/JA > 1.5), JD/JA at ~0.4-10 keV tends to be correlated with the magnetic compression ratio rB.


ST01-A007
Research on Connection Arrangement Between Space Particle Radiation Detector and Its Front-end Readout Circuit

Xiangqian YU#+, Xin YANG, Linghua WANG, Weihong SHI, Yongfu WANG, Ao CHEN, Youlong WANG, Hongfei CHEN, Qiugang ZONG
Peking University, China

There are AC-coupled and DC-coupled configurations between the space particle radiation detector and its front-end readout circuit. This paper studies how these two configurations behave on the output amplitude, noise and signal-to-noise ratio. A theoretical model is derived to fully describe the transfer function from the input charge to the output voltage. The parameters of two typical Si detectors were took into the analysis. One is thick and small area while the other is thin and large area. The readout circuit consists of discrete components for convenience. Experiments were also done to verify the theoretical results. Generally, the gain of the preamplifier is larger for DC-coupled than AC -coupled. DC-coupled is suitable for the detector of smaller capacitance that is thick and small area. Furthermore, DC -coupled reduces the complexity of the circuit by fewer devices, so it benefits to multi-pixel detectors. While AC-coupled can reduce the input current of the readout circuit, thus reduces the pressure at the input. It is suitable to the detector of larger capacitance that is thin and large area. Furthermore, for PKU interplanetary ultralow-noise three-dimensional energetic particle instrument, we selected an appropriate coupled configurations to achieve the best performance. What’s more, the method proposed can also be applied to other space particle radiation detector system to select the appropriate coupled configurations to achieve their best performance.


ST01-A009
Range Expansion Technology for Space Particle Radiation Detector Readout Application Specific Integrated Circuits

Xiangqian YU#+, Youlong WANG, Linghua WANG, Weihong SHI, Yongfu WANG, Xin YANG, Ao CHEN, Qiugang ZONG
Peking University, China

Despite the widespread use of application specific integrated circuits (ASICs), their fixed measurable ranges are major limitations for some application. There are three method to solve this problem: paralleling the capacitor at the input of ASIC, decreasing the value of coupling capacitance between the detector and ASIC, employing a junction field-effect transistor source follower (JFET SF) as the first input stage of the ASIC. In this study, theoretical analysis, PSpice simulation analysis and experimental verification were carried out for the three method to find their best application situation. Furthermore, for ASIC (RENA-3) used in PKU interplanetary ultralow-noise three-dimensional energetic particle instrument, we selected an appropriate method to expand its energy detection range of proton channel. What’s more, the method proposed can also be applied to other space particle radiation detector system to expand its energy detection range for some situation.


ST01-A011
Multi-spacecraft Study of Solar Energetic Particles in Late October and Early November 2021

Ya-Hui YANG1#+, Shao-Chun LU2, Mao-Xiang WU2, You-Min CHEN1
1Department of Space Science and Engineering, National Central University, Taiwan, 2National Central University, Taiwan

Two active regions (ARs) NOAA 12887 and 12891 are responsible for lots of solar flares in late October and early November 2021. In particular, the X1.0 flare erupted from AR 12887 on 2021 October 28 is relevant to the first ground-level enhancement (GLE) in solar cycle 25, and the M1.7 flare occurred at AR 12891 on 2021 November 2 is associated with the intense geomagnetic disturbances about two days later. Moreover, both flares are accompanied by EUV waves, CMEs, and solar radio bursts, indicating the possible role of CME-driven shocks or ICMEs on particle acceleration except flares. In this study, we attempt to characterize the solar energetic particles and their potential accelerators based on multi-spacecraft measurements in the interplanetary space (e.g., STEREO-A, WIND, PSP, or SolO) during October 28 - November 5, 2021. The shock analysis, including the estimations of shock parameters and propagation time, combined with the lightcurves and spectral evolutions of energetic particles are implemented to quantify the acceleration efficiency. The causes of flux enhancement in energetic particles other than shocks will be discussed as well.


ST01-A012
Solar Energetic Particles Produced During Two Fast Coronal Mass Ejections

Xiaolei LI#+, Jingnan GUO, Yuming WANG
University of Science and Technology of China, China

Two recent extremely fast coronal mass ejections (CMEs) are of particular interest. The first one originated from the southern hemisphere on 2021 October 28 and caused strong solar energetic particle (SEP) events over a wide longitude range from Earth, STEREO-A, to Mars. However, the other one, originating from the center of the Earthviewed solar disk 5 days later, left weak SEP signatures in the heliosphere. Based on the white-light images of the CMEs from the Solar and Heliospheric Observatory (SOHO) and the Ahead Solar Terrestrial Relations Observatory (STEREO-A), in combination with the observations of the corresponding solar flares, radio bursts, and in situ magnetic fields and particles, we try to analyze the series of solar eruptions during October 28–November 2 as well as their correspondences with the in situ features. It is found that the difference in SEP features between the two CMEs is mainly due to (1) the seed particles probably supplied by associated flares and (2) the magnetic connection influenced by the preceding solar wind speed.


ST01-A014
Solar Energetic Electron Events Observed by Solar Orbiter and Wind

Wenyan LI#+, Linghua WANG
Peking University, China

Solar energetic electron (SEE) events are the observed most common solar particle acceleration phenomenon in the interplanetary space. In order to improve the understanding of solar acceleration and interplanetary transport of solar energetic electrons, we will present a comprehensive study of SEE events observed both by SolO/EPD and Wind/3DP at different distances and longitudes. First, we will investigate the evolution of SEE events (e.g., the electron temporal profile, energy spectrum, pitch angle distributions, etc.) from SolO to Wind, to separate the solar acceleration information from the interplanetary transport effects. Secondly, we will locate the solar source of SEE events (e.g., flares, coronal jets, coronal mass ejections, etc.), using the remote-sensing measurements from SolO, SDO, and SOHO.


ST01-A016
Energetic Particle Instrument Developed by Peking University

Linghua WANG#+, Xiangqian YU, Weihong SHI, Yongfu WANG, Qiugang ZONG
Peking University, China

The PKU energetic particle instrument (EPI) is designed to make measurements of the three-dimensional distribution of suprathermal electrons and ions with good time, energy and angular resolutions in the interplanetary space, respectively, at energies from 20 keV to 1 MeV and from 20 keV to 11 MeV. The EPI consists of three sets of dual-double-ended foil/magnet semi-conductor telescopes, which cleanly separate electrons in the energy range of 20–400 keV and ions from 20 keV–6 MeV. The output of front detectors is taken in anti-coincidence with center detectors, to achieve the low background. The magnet telescopes also employ the well-established dE/dx vs. total energy approach to determine some ion species including 4He and 3He. The development of this instrument is funded by the national major scientific instrument development project from the National Natural Science Foundation of China (NSFC).


ST01-A017
The 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

Double-power-law energy spectra have been observed in many large solar energetic particle (SEP) events. Itis an important feature for understanding the acceleration and propagation of high-energy particles, but its formation mechanism remains unclear. We first perform numerical modeling of particle acceleration near the Sun at a CME-driven shock propagating through a streamer magnetic field by solving the Parker transport equation. We find that the energy spectra 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 different source regions where the acceleration rates differ significantly. We also examine the double-power-law formation mechanism by analyzing the variation of particle energy spectra during propagation in the interplanetary space. Assuming that the SEP energy spectrum in the source region is a power-law with exponential rollover, we find that the superposition of energetic particles from different regions can produce a double power-law distribution during the interplanetary propagation. 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.


ST01-A019
Evolution of the Electron Acceleration Site in Solar Flares by Using Time-of-flight Analysis with Multiple Time-windows

Masaya YAKURA#+, Satoshi MASUDA
Nagoya University, Japan

It is well known that a large number of particles are accelerated during a solar flare. However, the particle acceleration process and where it happens has not been clearly revealed yet. The most outstanding study was done by Aschwanden et al. (1996) using the so-called Time-of-Flight (ToF) analysis technique. They concluded that the electron acceleration site is located slightly above the flare loop. Although the time evolution of the acceleration site during a flare is important for understanding the acceleration process, there are no studies on this topic. In this situation, we try to obtain new information on the evolution of the acceleration site using high-time resolution X-ray data derived from the Gamma-ray Burst Monitor (GBM) on board the Fermi Gamma-ray Space Telescope. To investigate the time evolution of the acceleration site, ToF analysis was applied for each time-window including an outstanding spike that appeared in the hard X-ray light curve for flares occurring near the limb. We expect a time series of time-lags between different energy ranges can be derived. To confirm that this new analysis method effectively works for our purpose, we applied it to an M-class flare occurring on 25 June 2015. Then, we actually got a result suggesting that the ToF distance changed during the flare. This means that the acceleration site moved during the flare. Then, we extended this analysis method to several flares and derived some initial results. In this paper, we focus on the motion of the acceleration site during a flare and discuss about the physical interpretation of the results.


ST01-A024
Investigation of the Pitch Angle Distribution of the Accelerated Electrons Generating a Fast Propagation of a Microwave Source During a Solar Flare Observed with Nobeyama Radioheliograph

Keitaro MATSUMOTO1#+, Satoshi MASUDA1, Kazumasa IWAI1, Takafumi KANEKO2,3, Takashi MINOSHIMA4
1Nagoya University, Japan, 2Lockheed Martin Solar and Astrophysics Laboratory, United States, 3National Center for Atmospheric Research, United States, 4Japan Agency for Marine-Earth Science and Technology, Japan

The mechanism of particle acceleration during solar flares still remains controversial in solar physics. The pitch angle distribution of the accelerated electrons represents an important element in understanding this mechanism. Electrons that are accelerated to nearly relativistic speeds emit non-thermal microwaves. By using the Nobeyama Radioheliograph (NoRH), [Yokoyama+2002] estimated the pitch angle of accelerated electrons by analyzing the propagation velocity of non-thermal microwave sources. We found another flare event (an M-class flare on October 22, 2014) that showed similar observational features and evaluated the pitch angle of the accelerated electrons through multi-wavelength observations with NoRH, SDO, and Fermi, and computer simulations with the coronal magnetic field obtained from the NLFFF model. Finally, we concluded that electron injection took place toward one footpoint of the loop and also obtained results indicating a bouncing motion of the injected electrons along the magnetic loop (submitted to ApJL). This presentation will undertake a theoretical examination of the position and pitch angle distribution of injected electrons within the loop. By solving the Fokker-Plank equation, we will determine the phase space density with pitch angle and energy as independent variables in an 1D coordinate system along the magnetic loop, as determined by the NLFFF model. This will allow us to investigate the bouncing motion of electrons along the loop. The time-varying 17 GHz microwave emission along the loop will be determined through the solution of the Fokker-Plank equation. Our results indicate that electron injection occurred in the direction of the footpoint on one side. Our aim is to carry out an examination of the factors that influence the injection location and pitch angle distribution of accelerated electrons, using the simulations. We will then compare our results with available observations and discuss, in particular, the injection of accelerated electrons in this event.


ST01-A030
The Nonthermal Property of a Microflare

Zhentong LI1#+, Yang SU2
1Chinese Academy of Sciences, China, 2Purple Mountain Observatory, CAS, China

In this poster, I will firstly show the energy release and plasma heating processes in the microflare first reported by Glesener et al. 2020, which shows the existence of a nonthermal component down to 6.5 keV in the X-ray spectrum. Using careful differential emission measure (DEM) analysis and the calculated multithermal X-ray component, we confirm the existence of the nonthermal component in the observed X-ray spectrum. Most importantly, we report the first imaging evidence for low-energy cutoff of energetic electrons in EM maps of >10 MK plasma, which first appeared as two coronal sources significantly above the chromospheric footpoints. This study reveals the important role of electron thermalization and low-energy cutoffs in the physical processes of microflares.


ST02-A006
Modeling of Thermospheric Atmospheric Density Based on MBiLE Model

Qian PAN1+, Chao XIONG1#, Zhou CHEN2, Peian WANG2, Chunyu XU1, Xu YANG3
1Wuhan University, China, 2Nanchang University, China, 3National University of Defense Technology, China

In this study, an ensemble learning algorithm based on a bidirectional long and short-term memory neural network (BiLSTM) and a multilayer perceptron (MLP) is used to build a model for prediction of the thermospheric mass density, MBiLE. We use the thermospheric density derived from the onboard accelerometer of Swarm C, which flies at about 450 km, for training and constructing the model. As expected, the MBiLE model predictions agree well with the Swarm C observations. We further checked the MBiLE model predictions at a wider altitude range, and compared the predictions with observations from the Swarm B (flying at about 500 km), CHAMP (flying at about 350 km), and GOCE satellite (flying at about 250 km). For example, for comparison with observations from GOCE, the prediction coefficient of determination of the model proved to be 0.96 with a root mean square error of 2.537×e-12. The comparison show that our MBiLE model has good robustness and generalization, and can achieve the prediction of thermospheric density covering a wide altitude range.


ST02-A021
Short-period Variation of Atmospheric Turbulence Activity in the MLT Region Over Langfang

Zewei WANG1+, Cunying XIAO1#, Xiong HU2, Junfeng YANG2, Xuan CHENG2, Qingchen XU2
1Beijing Normal University, China, 2Chinese Academy of Sciences, China

In this paper, we investigate the atmospheric turbulence activity in the MLT region and the relationship between atmospheric turbulence activity and atmospheric fluctuation activity. We use data from the Langfang MF radar (39.4◦N,116.7◦ E) from July 2019 to June 2020 and NRLMSIS 2.0 to calculate the parameters of atmospheric fluctuation activity and atmospheric turbulence energy dissipation rate. The atmospheric turbulent energy dissipation rate is modulated by different periods at different altitudes, with 12h and 24h period variations at all altitudes. At lower altitudes, there are more periodic variations; at higher altitudes, the 12h period is more pronounced than the 24h period, and the 8h period is more pronounced. A comparison of the atmospheric turbulent energy dissipation rate with atmospheric tidal wave activity shows that tidal waves have an effect on the atmospheric turbulent energy dissipation rate, and at higher altitudes, the effect of tidal waves on the turbulent energy dissipation rate is more evident. The pattern of variation in the atmospheric turbulent energy dissipation rate is similar to that of atmospheric gravity wave activity, with both turbulent energy dissipation rate and atmospheric gravity wave activity showing significant semi-annual variation.


ST02-A022
Ionospheric Disturbance Over Thailand and Nearby Regions in Southeast Asia During St. Patrick’s Day Geomagnetic Storm

Paparin JAMLONGKUL1#+, Suwicha WANNAWICHIAN1, Larry PAXTON2, Clayton CANTRALL2, Pornchai SUPNITHI3
1Chiang Mai University, Thailand, 2Johns Hopkins University Applied Physics Laboratory, United States, 3King Mongkut's Institute of Technology Ladkrabang, Thailand

This work focuses on the ionospheric disturbance in the Southeast Asia regions including Thailand, based on the thermospheric-ionospheric model and observations during the 17-18 March 2015 St. Patrick’s Day geomagnetic storm event. For thermospheric neutrals, the observational O/N2 column density ratio was measured by GUVI instrument on board TIMED spacecraft. The observed O/N2 compared to O/N2 computing from the WACCM-X SD model, based on high-latitude inputs including magnetospheric and geomagnetic states from two models, Heelis and Weimer. Global TEC (total electron content) data were obtained by the Madrigal GNSS database. Regional ionospheric data (TEC) were observed by several GNSS stations in the Asian sector including the KMIT Thailand station. The observed GNSS TEC is further compared to simulated TEC by the WACCM-X SD model. The preliminary comparisons show that the WACCM-X SD O/N2 from both Heelis and Weimer high-latitude drivers is consistently greater than GUVI O/N2 on global scales. Ionospheric results from TEC model-observation comparison show a slower response of the WACCM-X SD data. For regional ionospheric comparisons, WACCM-X SD TEC during the event has a significant variation in small response with KMIT TEC. The ionospheric response in low-latitude regions on localized scales is discussed. Moreover, the significant ionospheric response over Thailand could be interpreted in form of continuing irregularities among regions in Southeast Asia during the event in detail further.


ST02-A029
Midlatitude Ca+ Layers in the Mesosphere: Observations and Modeling

Jing JIAO#+
Chinese Academy of Sciences, China

Long-lived meteoric metal ions (1 day above 100 km altitude) converge to form dense ion layers, causing plasma irregularities in the ionosphere. Therefore, it is imperative to observe and understand the transport and formation of metallic ion layers. However, it is technically challenging to detect specific ion species, especially tracing ion transport over large vertical ranges and time durations. Numerous instruments detect electron density but cannot distinguish ion species. Rocket-borne mass spectrometers can distinguish ion species but provide only snapshots. Lidars provide a powerful tool to profile and trace metallic species over extended periods by exciting specific resonance fluorescence. The only metal ions detectable by ground-based lidars are Ca+, and previous lidar measurements reached ∼180 km. Our Ca+ lidar upgraded with narrowband lasers has achieved high detection sensitivity, enabling the Ca+ profiling up to 300 km. Such lidar measurements of dynamical Ca+ layers open a new window to study plasma irregularities.


ST02-A030
The COSPAR International Space Weather Action Teams (ISWAT) Initiative: Updates and Roadmap Progress

Mario BISI1#+, Masha M. KUZNETSOVA2, Anna BELEHAKI3, Sean BRUINSMA4, Shing FUNG2, Jingnan GUO5, Alexi GLOVER6, Manolis GEORGOULIS7, Insoo JUN8, Larisza KRISTA9, Ian MANN10, Arnaud MASSON11, Dibyendu NANDI12, Hermann OPGENOORTH13,14, Alexei PEVTSOV15, Christina PLAINAKI16, Martin REISS17, Camilla SCOLINI18, Manuela TEMMER19, Barbara THOMPSON2, Ilya USOSKIN20, Zhonghua YAO21, Yihua ZHENG2
1United Kingdom Research and Innovation - Science & Technology Facilities Council - RAL Space, United Kingdom, 2NASA Goddard Space Flight Center, United States, 3National Observatory of Athens, Greece, 4Centre National D'Etudes Spatiales, France, 5University of Science and Technology of China, China, 6European Space Agency, Germany, 7Academy of Athens, Greece, 8NASA Jet Propulsion Laboratory, United States, 9University of Colorado, Boulder, United States, 10University of Alberta, Canada, 11European Space Agency, Spain, 12Indian Institute of Science Education and Research-Kolkata, India, 13University of Umea, Sweden, 14University of Leicester, United Kingdom, 15National Solar Observatory, United States, 16Italian Space Agency, Italy, 17National Aeronautics and Space Administration, United States, 18University of New Hampshire, United States, 19University of Graz, Austria, 20University of Oulu, Finland, 21Chinese Academy of Sciences, China

Modern society is becoming ever-more reliant on complex technologies and infrastructures that are highly susceptible to deleterious space-weather effects due to the temperamental nature of our dynamic Sun. Understanding and predicting space weather and its impact on society is acknowledged as a global challenge and was addressed by the initial COSPAR/ILWS Roadmap in 2015 (Schrijver et al., ASR, doi:10.1016/j.asr.2015.03.023, 2015). To better address many of the challenges identified in this initial roadmap, the COSPAR Panel on Space Weather (PSW) established the International Space Weather Action Teams (ISWAT) initiative. The ISWAT initiative is a bottom-up community-driven active network of teams, clustered by heliophysics domain, overarching activities, and key space-weather impact areas (see: https://iswat-cospar.org/ for further details). After several years of good progress across all areas of space-weather science and pathways to impacts (as well as with overarching activities in data utilisations, assessment, education and outreach, etc…), under the COSPAR PSW terms of reference to update the space-weather roadmap every ~five years, an updated roadmap was embarked upon led by both the ISWAT initiative and the PSW – but this time with a multi-paper approach across two Topical Issues in the COSPAR Advances in Space Research (ASR) journal. Here, we will provide an update on the COSPAR ISWAT initiative, how we work and how anyone in the wider community is welcome and can get involved, as well as an update on the updated roadmap progress to date.


ST02-A032
A Simulation Study on the Variation of Thermospheric O/N2 Ratio with Solar Activity

Xiaoli LUAN#+, Zhongli LI, Jiuhou LEI
University of Science and Technology of China, China

The ratio of number density of atomic oxygen (O) to that of molecular nitrogen (N2) in the thermosphere (O/N2) is an important parameter connecting the terrestrial thermosphere and daytime ionosphere. Previous studies demonstrated that the thermospheric O/N2 increases with increasing solar activity, and the changes in O/N2 with solar activity show a significant difference between winter and summer hemispheres. However, the root causes, which are responsible for the solar activity variation of O/N2, are not fully understood. In this study, we use the Thermosphere Ionosphere Electrodynamics General Circulation Model to investigate the contributions of various physical and chemical processes on the response of O/N2 to the solar radiation change. The controlled simulation results suggested that the chemical processes lead to the increase of thermospheric O/N2 over the globe with increasing solar activity. The increase of O/N2 with solar activity is dominated by the enrichment of O abundance and the loss of N2 abundance in the lower and upper thermosphere, respectively. Moreover, the simulation results suggested that a stronger hemispheric asymmetry in solstices is attributed to the stronger thermospheric circulation.


ST03-A003
Daytime Ionospheric Large-scale Plasma Density Depletion Structures Detected at Low Latitudes Under Relatively Quiet Geomagnetic Conditions

Wenjie SUN1#+, Guozhu LI1, Lianhuan HU1, Xiukuan ZHAO1, Haiyong XIE2, Yi LI1, Baiqi NING1
1Chinese Academy of Sciences, China, 2Institute of Geology and Geophysics, Chinese Academy of Sciences, China

The ionospheric electron density is expected to enhance after sunrise during geomagnetic quiet days. We present a case of anomalous large-scale ionospheric TEC depletion structure occurring in morning hours over low latitudes in China under relatively quiet geomagnetic conditions. The depletion structure, which occurred over a wide longitude range of more than 35°, developed toward higher latitudes at the speed of ~250 m/s. A statistical analysis using the data in 2018-2020 showed that such large-scale daytime TEC depletion mainly occurred in summer (mostly with Kp<3), with large intensity at ~16-30°N. The geomagnetic ΔH measurements at the stations near and away from the magnetic dip equator showed positive values, which rules out the possible contribution from a westward electric field. Observations from multiple ionosondes revealed a net downward plasma transport during the TEC depletion. An enhanced poleward neutral wind during the early morning hours, which may induce downward plasma transport, was surmised to play a leading role in driving the large-scale morning TEC depletion.


ST03-A007
Limb Sounders Tracking Perturbations from the Stratosphere to the Ionosphere Associated with Near-surface Sources

Xiangxiang YAN#+, Tao YU, Chunliang XIA
China University of Geosciences, China

Near-surface sources (earthquake/tsunami/volcano/typhoon) are known to induce atmospheric acoustic gravity waves (AGWs), which could propagate upwards through the lower atmosphere into the ionosphere. In this study, we employ three types of satellite data from two different limb sounders: the COSMIC radio occultation (RO) technique and the Sounding of the Atmosphere using Broadband Emission Radiometry (SABER) instrument to study the vertical coupling of near-surface sources-induced perturbations from the stratosphere to the ionosphere. For the 2011 Tohoku tsunami and 2015 Chile tsunami cases, all three types of datasets, including temperature profiles from 10 to 55 km and 16 to 107 km, and electron density profiles from 120 to 550 km, recognized perturbations of different scales at different heights after the tsunamis. The vertical scales identified by the wavelet analysis are from 1–2 km, 5–9 km, and 25–50 km in the stratosphere, mesosphere, and ionosphere, respectively. Another interesting point is that the temperature perturbations recorded by the SABER from 70–100 km altitude are found to arrive earlier than the tsunami wavefront. For the 2022 Tonga volcano case, the eruption induced strong GWs in the mesosphere are recorded by the SABER, these GWs have dominant vertical wavelengths of ~10-20 km. Not surprisingly, these disturbances also have profound effects on the ionosphere, one of which is the significant depletion of the ionosphere recorded by the RO data. This destructive depletion of the ionosphere had a marked effect on local short-wave communications. It is believed that these large near-surface sources disturbed the whole atmosphere space, and the scale of these signals gradually increases with the increase in altitude but decreases with time. The findings in this study suggest that the limb-sounding technique is a useful instrument in studying the vertical coupling of disturbances associated with near surface sources.


ST03-A014
Variation Trend of Shortwave Absorption in the Low-latitude Ionosphere

Xiaoli JIANG#+, Huimin LI, Lixin GUO
Xidian University, China

In this study, we propose a more comprehensive and valid ionospheric absorption model by incorporating an electron-collision model and the latest version of the geomagnetic model, based on the atmospheric model and the ionospheric model with reference to the Appleton-Hartree formulation. The absorption model is used to study the variation trend of the total absorption with frequency and elevation angle during two different times (day and night) in a low latitude ionosphere based on the ionospheric stratification theory, and some interesting phenomena are observed. Traveling ionospheric disturbances (TIDs) are commonly observed ionospheric disturbances, which influence the propagation process of radio waves. So based on the previous ionospheric model, the traveling ionospheric disturbances induced by the atmospheric gravity waves are modeled. Simultaneously, the variation trend of the absorption attenuation is analyzed under the existence of TID. Finally, in order to draw further conclusions, take the absorption with or without considering TID into comparison.


ST04-A008
Resonant Damping of Kink Modes in Solar Coronal Slabs

Hui YU1#+, Bo LI1, Shao-Xia CHEN1, Mingzhe GUO2
1Shandong University, China, 2KU Leuven, Belgium

We examine resonantly damped kink modes in straight coronal slabs, paying special attention to the effects of the formulation for the transverse density distribution (“profile”). We work in the framework of pressure-less, gravity-free, resistive magnetohydrodynamics, and we adopt the dissipative-eigenmode perspective. The density profile is restricted to be one dimensional, but nonetheless allowed to take a generic form characterized by a continuous transition layer connecting a uniform interior to a uniform exterior. A dispersion relation (DR) is derived in the thin-boundary limit, yielding analytical expressions for the eigenfrequencies that generalize known results in various aspects. We find that the analytical rather than the numerical solutions to the thin-boundary DR serve better the purpose for validating our self-consistent resistive solutions. More importantly, the eigenfrequencies are found to be sensitive to profile specifications, the ratio of the imaginary to the real part readily varying by a factor of two when one profile is used in place of another. Our eigenmode computations are also examined in the context of impulsively excited kink waves, suggesting the importance of resonant absorption for sufficiently oblique components when the spatial scale of the exciter is comparable to the slab half-width.


ST04-A010
A Neural Network Approach to Understanding the Flow Dynamics Photospheric Flux Emergence

Matthew LENNARD1#, Benoit TREMBLAY2, Andrés ASENSIO RAMOS3, Hideyuki HOTTA4, Haruhia IIJIMA4, Sung-Hong PARK4, Viktor FEDUN5+, Gary VERTH5, Suzana DE SOUZA E ALMEIDA SILVA5
1University of Sheffield, United Kingdom, 2National Solar Observatory, United States, 3Instituto de Astrofisica de Canarias, Spain, 4Nagoya University, Japan, 5The University of Sheffield, United Kingdom

Advances in modelling magnetic flux inside the Sun’s convective region (see e.g. Hotta & Iijima, 2020; Chen et al, 2021) have provided high resolution data, which allow the study of photospheric flows and their relationship with intense emerging magnetic flux. In the literature, photospheric velocity fields have been mostly inferred by employing optical feature tracking with e.g., local correlation tracking (LCT). This is useful for understanding flows mainly on supergranular scales, however results are influenced easily by noise, creating holes and large errors when performing tracking at smaller scales. Neural networks (NNs) such as DeepVel (DV) (see Asensio Ramos et al., 2017) have been developed for deriving transverse flows from time-consecutive images of the photosphere by learning from numerical simulations. DV works for photospheric observations at a wide range of spatial resolutions and cadences, only limited by the training data. The combination of speed and accuracy of recovering these data from a trained version of DV are an improvement on the often-used Fourier LCT (FLCT) algorithm. These highly detailed velocity fields can be used to analyse plasma flow organisation and subsurface flows using methodologies such as the Finite-Time Lyapunov Exponent (FTLE). In this work, we have tested and compared the ability of both FLCT and DV to recover velocities from the R2D2 simulation. We have found notable features within the FTLE field, which may be used to forecast flux emergence hours before there are any visible indicators, such as the appearance of pores or sunspots.


ST04-A011
Mode Conversion Near the Magnetic Null Point: Current Sheet Formation

Zhang CHAO#+, Mingzhe GUO, Zhenghua HUANG, Bo LI, Lidong XIA, Hui FU, Hengyuan WEI, Deng KAIWEN, Li HAIYI
Shandong University, China

Magnetoacoustic waves are thought to be ubiquitous in the solar atmosphere, in which fast waves are physically trapped by the null point, causing the collapse of the null points. Therefore, fast waves could be responsible to the sympathetic explosion that is energy release triggered by a remote activity. In this study, based on an initial state of the potential field with magnetic null point and Athena++ code, we perform a two-dimensional numerical experiment to study the dynamics when the slow wave propagating through the magnetic null point. We found that mode conversion occurs in the vicinity of the sound speed equal to the Alfvén speed and fast waves are generated and propagate towards magnetic nulls. Consequently, part of the energy of the fast waves is trapped by the magnetic null point, causing the collapse of the magnetic null point and formation of current sheet. As the current sheet becomes thinner, the plasmoid instability is triggered and the reconnection rate increases. The simulations help us better understand the relationship between MHD waves and magnetic spots, also provide an scenario sympathetic eruption.


ST04-A014
Vorticity and Energy Transport in Photospheric Vortex Tubes

Suzana DE SOUZA E ALMEIDA SILVA1#+, Istvan BALLAI1, Erico L. REMPEL2, Sergiy SHELYAG3, Luiz Augusto CAMARGO ARANHA SCHIAVO4, Viktor FEDUN1
1The University of Sheffield, United Kingdom, 2Instituto Tecnológico de Aeronáutica, Brazil, 3Deakin University, Australia, 4University of Manchester, United Kingdom

In this study, we use the instantaneous vorticity deviation method to detect three-dimensional vortex tubes in a solar plage simulation. Our analysis suggests that the vorticity in the vortex tubes is mainly created by the misalignment of magnetic pressure and density gradients, indicating the importance of the magnetic field for the vortex evolution. The vortices also present prevailing magnetic energy, transported up and downwards within each tube, creating a circulation of electromagnetic energy across the lower solar atmosphere. The vertical component of Poynting flux is mainly generated by horizontal motions leading to a nonuniform and time-dependent distribution of energy flux. Thereby, collectively, the vortices create a net upward propagating energy flux of 1.38x108 ergs/(s cm 2), enough to explain chromospheric temperatures. Moreover, our findings indicate that the dynamics imposed by vortex motion can help enhance energy transport and heating mechanisms such as viscosity and current dissipation.


ST05-A002
Identification and Velocity Characterisation of a Heliospheric Transient Using Interplanetary Scintillation with the Murchison Widefield Array

Angelica WASZEWSKI1#+, John MORGAN2, Rajan CHHETRI3, Mark CHEUNG3, Ramesh BHAT1, Melanie JOHNSTON-HOLLITT1
1Curtin University, Australia, 2CSIRO Space and Astronomy, Australia, 3CSIRO - Space and Astronomy, Australia

Interplanetary scintillation (IPS) is a phenomenon which causes sufficiently small radio sources to “twinkle” in the solar wind. IPS is a fantastic space weather tool as it is able to measure the solar wind density along any lines of sight an arbitrary distance from the Sun, giving it unlimited reign to probe the entire heliosphere. In the last few years, we have breathed new life into this old technique, adapting it for modern low-frequency instruments such as the Murchison Widefield Array (MWA). The key advance we have made is to exploit the enormous field of view of the MWA. This allows us to monitor all IPS sources across a field of view 30 degrees across, leading to an unprecedented density of measurements of around 250 sources per 900 sq deg. These capabilities have already been exploited to launch the IPS space weather era of the MWA, with the first detection and characterisation of a coronal mass ejection. Alongside this initial space weather work, a recently completed survey of IPS sources in the sky above the MWA has become the basis of this work. We have conducted a blind search of 49 days of MWA IPS observations from mid-2019, with overlapping daily observations approximately East and South-East of the Sun at an elongation of 30 degrees. This search has revealed several interesting transient features characterised by higher than usual scintillation levels (in spite of the observations being taken at solar minimum). One solar wind enhancement is captured in two observations several hours apart, allowing the plane-of-sky velocity to be inferred. After close inspection of solar event catalogues and white-light coronagraph images, it was determined that this heliospheric transient is not an effect caused by a coronal mass ejection, but has a most likely source of a co-rotating interaction region.


ST05-A003
UCSD Iterative 3-D Analyses: Forecast of the March 10, 2022, CME Using ISEE IPS Data

Bernard JACKSON1#+, Munetoshi TOKUMARU2, Kazumasa IWAI2, Ken'ichi FUJIKI2, Matthew BRACAMONTES1, Andrew BUFFINGTON1, Mario BISI3, Go MURAKAMI4, Daniel HEYNER5, Beatriz SANCHEZ-CANO6, Mathias ROJO7, Sae AIZAWA8, Nicolas ANDRE9, Alain BARTHE7, Emmanuel PENOU10, Andrey FEDOROV9, Jean-André SAUVAUD10, Shoichiro YOKOTA11, Yoshifumi SAITO12
1University of California San Diego, United States, 2Nagoya University, Japan, 3United Kingdom Research and Innovation - Science & Technology Facilities Council - RAL Space, United Kingdom, 4Japan Aerospace Exploration Agency, Japan, 5Institute for Geophysics and Extraterrestrial Physics, Germany, 6University of Leicester, United Kingdom, 7Institute for Research in Astrophysics and Planetology, France, 8Laboratoire de Physique des Plasmas, France, Metropolitan, 9University of Toulouse, France, 10Institute for Research in Astrophysics and Planetology (IRAP), National Center for Scientific Research (CNRS) - University of Toulouse (UPS) - National Center for Space Studies (CNES), France, 11Osaka University, Japan, 12Institute of Space and Astronautical Science / Japan Aerospace Exploration Agency, Japan

Remotely-sensed interplanetary scintillation (IPS) from the Institute for Space-Earth Environmental Research (ISEE), Japan, allows a determination of solar wind parameters throughout the inner heliosphere. We show the 3-D time-dependent analysis technique developed for these data sets that is used to forecast plasma velocity, density, and component magnetic fields at Earth, as well at the other inner heliospheric planets and spacecraft. One excellent March 10, 2022, Coronal Mass Ejection (CME) example is shown here that was viewed not only in the ISEE IPS analyses, but also by the spacecraft near Earth that could measure the CME 1 AU arrival. Solar Orbiter that was nearly aligned along the Earth radial at 0.45 AU also measured the CME in plasma density, velocity, and magnetic field. BepiColombo at 0.44 AU, aligned with the STEREO A spacecraft, also measured this CME passage in the European Space Agency Mercury Planetary Orbiter MAG instrument. In addition, the Japan Aerospace Exploration Agency BepiColombo Mio Mercury Plasma Particle Experiment/Mercury Electron Analyzer recorded an enhancement of electrons and the Solar Particle Monitor on Mio measured a Forbush decrease from below the protective Sun-shroud covering that timed the passage of this event. This presentation summarizes the analysis from the ISEE, Japan real-time data for the CME forecast, and provides a synopsis of the results, and confirmation of the CME morphology, from the different data sets available after the CME arrival.


ST05-A004
Solar Wind 3-D Reconstructions Using STEREO and SMEI Thomson Scattering Data: Attempts to Define Mesoscale Structures Near Earth

Bernard JACKSON1#+, Matthew BRACAMONTES1, Andrew BUFFINGTON1, Jackie DAVIES2, David BARNES2, Munetoshi TOKUMARU3
1University of California San Diego, United States, 2United Kingdom Research and Innovation, United Kingdom, 3Nagoya University, Japan

We now use the University of California, San Diego (UCSD) iterative tomography analyses to provide high resolution Solar Mass Ejection Imager (SMEI) and STEREO Heliospheric Imager (HI) 3-D reconstructed plasma density volumes of the inner heliosphere. These analyses also include Earth-based interplanetary scintillation (IPS) instrumentation data from the Institute for Space-Earth Environmental Research (ISEE), Japan, to help provide more refined high-resolution plasma densities and velocities. Because we use both SMEI and STEREO HI data with a long temporal base removed, we can study the morphology of Stream Interaction Regions (SIRs) as well as that of Interplanetary Coronal Mass Ejections (ICMEs). Here we present the densities at one-hour cadences, and with comparable few-degree, latitude, longitude, and solar distance resolutions that are well within mesoscale sizes that take less than a half a day to pass over an observer. The analyses show that the structures that propagate past the spacecraft and near Earth are often very “corrugated” and “patchy” at these high resolutions. These 3-D reconstructions have the ability to explain some of the differences in multipoint in-situ observations from spacecraft near Earth and further afield (e.g., STEREO-A). Here we address the amount to which these structures continue to evolve as they move outward and interact with each other. Patchy structures present difficulties for most forecasting techniques, which assume smooth structures that propagate outward from the solar surface, unlike those revealed by the tomography. Our analyses prototype the forecasting capability needed for future similar spaceborne heliospheric imager instruments such as the NASA Small Explorer PUNCH, UCSD’s All Sky Heliospheric Imager (ASHI), or the Vigil heliospheric imager.


ST05-A006
ASHI: An All Sky Heliospheric Imager Designed to Maximize the Scientific Return from Solar Wind Structures Passing Earth

Matthew BRACAMONTES1#+, Bernard JACKSON1, Stephen KAHLER2, Mario BISI3, Andrew BUFFINGTON1, Stuart VOLKOW1, Ed STEPHAN4, Philippe LEBLANC4, Ron QUILLIN4
1University of California San Diego, United States, 2Air Force Research Laboratory, United States, 3United Kingdom Research and Innovation - Science & Technology Facilities Council - RAL Space, United Kingdom, 4Stephan Design-Build, United States

We have conceived, designed, and have evaluated components for an All-Sky Heliospheric Imager (ASHI), suitable for flight on future space missions. ASHI was tested last summer on a NASA-sponsored topside balloon flight; this presentation highlights the images taken by this instrument on its successful overnight flight. A successful space-borne flight will have an order of magnitude more throughput than SMEI or the STEREO HI instrumentation, and thus provide a far better science and forecast capability than possible before. ASHI is currently manifested on a DoD Space Test Program satellite. As a simple, light weight (~6kg), and relatively inexpensive instrument, the ASHI system has the principal objective of providing a minute-by-minute and day-by-day near real time acquisition of precision Thomson-scattering photometric maps of the inner heliosphere. The instrument's unique optical system is designed to view a hemisphere of sky starting a few degrees from the Sun. A key photometric specification for ASHI is 0.1% differential photometry in one-degree sky bins at 90 degrees elongation that enables the three dimensional (3-D) reconstruction of heliospheric density extending outward from near the Sun. The ASHI system, unlike coronagraphs or planned heliospheric imagers, is intended to maximize the scientific return of heliospheric structures that pass the spacecraft. This will allow density structure measured in-situ to be extended outward into the surrounding plasma close to Earth. This is especially important where recent high-resolution Solar Mass Ejection Imager (SMEI) and STEREO Heliospheric Imager (HI) analyses have shown CMEs have an evolving and “corrugated” structure when they pass nearby.


ST05-A010
Next Generation Interplanetary Scintillation Observation for Better Three-dimensional Reconstruction of the Heliosphere

Kazumasa IWAI#+, Munetoshi TOKUMARU, Ken'ichi FUJIKI
Nagoya University, Japan

Interplanetary scintillation (IPS) is a radio scattering phenomenon caused by the turbulences in the solar wind. The IPS observation using ground-based radio telescopes has been an important technique to investigate the three-dimensional (3D) structure of the solar wind in the heliosphere. The IPS observation has also been used for space weather research and operations. Institute for Space–Earth Environmental Research (ISEE), Nagoya University have observed IPS to derive the solar wind velocity and density irregularities for several decades using large radio telescopes at 327 MHz. The 3D structure of the heliosphere has been reconstructed by the tomography technique. The derived solar wind characteristics are also included in the three-dimensional (3D) global magnetohydrodynamic (MHD) simulation of the heliosphere to forecast the arrival of the solar wind and coronal mass ejections (CMEs). The recent space weather requires more accurate prediction of the solar wind that requires more IPS observations. Now, a new project to develop the next generation IPS observation system is in progress. We consider a new ground-based radio observation system at 327 MHz by constructing a 2D flat phased-array antenna system consisting of multiple dipole antennas, and installing digital beam forming devices. The multidirectional simultaneous IPS observation using this system enables the solar wind observation 10 times as much as the conventional radio instruments have been done. This project will greatly contribute to understanding the solar wind and improving the accuracy of space weather forecasts. We have developed a prototype of the digital phased array instrument. This instrument has 8 analog-digital converters (ADCs), field-programmable gate array (FPGA), and 10-Gbit Ethernet output. This system enables us to measure 8 beams simultaneously by processing 8 types of different beamforming in parallel. A small scall array system is under construction as a phase-I project.


ST05-A011
Three-dimensional Structure of the Ionospheric Disturbances Over Japan Following the Eruption of Hunga Tonga-Hunga Ha'apai on 15 January 2022

Susumu SAITO1#+, Taisei NOZAKI2, Mamoru YAMAMOTO2, Nicholas SSESSANGA3
1National Institute of Maritime, Port and Aviation Technology, Japan, 2Kyoto University, Japan, 34D-Space, Norway

After the intense eruption of the submarine volcano Hunga Tonga-Hunga Ha'apai on 15 January 2022, strong ionospheric disturbances were observed over the world. The ionospheric disturbances which attracted attention were the traveling ionospheric disturbances (TIDs) propagating radially from the volcano together with the atmospheric waves and its projection to the opposite hemisphere [1].
After the passage of TIDs and after the local sunset, there were many reports of irregularities with sharp depletion of the ionospheric density. However, it appears that there was no appropriate interpretation of such disturbances. We tried to understand the phenomena by using observations by a dense GNSS network over Japan which is the GNSS Earth Observation NETwork (GEONET) operated by the Geospatial Information Authority Japan.
The depletions of the ionospheric density accompanied small-scale irregularities and embedded in the region of enhanced total electron content (TEC). It was similar to the storm-induced plasma stream (SIPS) observed during a strong magnetic storm [2]. We investigated three-dimensional ionospheric density structures by using a GNSS tomography technique [3], and found that the structure was consistent with the theory of SIPS. The results indicated that the thermospheric neutral wind may have modified after the eruption.[1] Saito, Ionospheric disturbances observed over Japan following the eruption of Hunga Tonga-Hunga Ha’apai on 15 January 2022, Earth Planets and Space, 2022.
[2] Maruyama et al., Storm-induced plasma stream in the low-latitude to midlatitude ionosphere, J. Geophys. Res.: Space Physics, 2013.
[3] Ssessanga et al., Complementing regional ground GNSS-STEC computerized ionospheric tomography (CIT) with ionosonde data assimilation, GPS Solutions, 2021.


ST05-A012
LOFAR4SpaceWeather (LOFAR4SW) – Increasing European Space-weather Capability with Europe’s Largest Radio Telescope: Updates and Potential Future Prospects

Mario BISI1#+, Richard FALLOWS2, Rene VERMEULEN2, Stuart ROBERTSON3, Mark RUITER2, Nicole VILMER4, Hanna ROTHKAEHL5, Barbara MATYJASIAK5, Joris VERBIEST6, Peter GALLAGHER7, Tobia CAROZZI8, Michael OLBERG8, Michael LINDQVIST8, Eoin CARLEY9, Carla BALDOVIN2, Paulus KRUGER2, Maaijke MEVIUS2, Biagio FORTE10, Steve MILAN11, David JACKSON12, Bernard JACKSON13, Dusan ODSTRCIL14,15, Oyuki CHANG3, David BARNES3
1United Kingdom Research and Innovation - Science & Technology Facilities Council - RAL Space, United Kingdom, 2ASTRON - The Netherlands Institute for Radio Astronomy, Netherlands, 3United Kingdom Research and Innovation, United Kingdom, 4Observatoire de Paris, France, 5Space Research Centre of Polish Academy of Sciences, Poland, 6Bielefeld University, Germany, 7Dublin Institute for Advanced Studies, Ireland, 8Onsala Space Observatory, Sweden, 9N/A, Ireland, 10University of Bath, United Kingdom, 11University of Leicester, United Kingdom, 12Met Office, United Kingdom, 13University of California San Diego, United States, 14George Mason University, United States, 15NASA Goddard Space Flight Center, United States

Space-weather (SW) monitoring/forecasting/operations, and its unpinning research, are all important topics of the global effort to better understand and mitigate-against SW impacts. Knowledge/understanding of interactions in the Sun-Earth system, the physics behind observed SW phenomena, and the direct impact on modern technologies are all crucial areas of technological and scientific interest. A better understanding of the Heliosphere-Earth system is crucial, and this can be achieved by exploiting novel ground-based radio observations of such. The tracking of plasma structures across the inner-heliosphere is possible using instruments such as the LOw Frequency ARray (LOFAR) via observations of radio-wave scintillation – in the heliosphere, this is known as interplanetary scintillation (IPS). LOFAR is also capable of detecting ionospheric scintillation as well as undertaking other scientific investigations of the ionosphere and heliosphere. LOFAR observes over a wide radio bandwidth (~10-250 MHz) at high spatial/temporal resolutions and has capabilities that enable studies of several aspects of SW to be progressed beyond today’s state-of-the-art. However, in its present setup, it can only be used for SW campaigns. This severely limits its ability to contribute to SW monitoring/forecasting beyond its core strength of enabling world-leading scientific research. The LOFAR For Space Weather (LOFAR4SW) project (see: http://lofar4sw.eu/) was a Horizon 2020 (H2020) INFRADEV design study to undertake investigations into upgrading LOFAR for regular SW science/monitoring observations in parallel with normal radio-astronomy/scientific operations. It involved all aspects of political/scientific engagement with various stakeholders under the full recognition that SW is a worldwide threat with varied local/regional/global impacts. Here, we summarise key LOFAR observing capabilities in the context of LOFAR4SW, and, where possible, explore project ideas aiming to investigate how LOFAR can be utilised for advanced forecasts of SW conditions/impacts, via a new understanding of the Earth’s magnetosphere-ionosphere space-environment.


ST05-A015
Observations of Radio Wave Scintillation in the Auroral Ionosphere from Various Instruments

Biagio FORTE1#+, Richard FALLOWS2, Mario BISI3, Pawel FLISEK4, Kacper KOTULAK4, Andrzej KRANKOWSKI4, Maaijke MEVIUS2, Kasia BESER2, Antti KERO5, Ingemar HÄGGSTRÖM6
1University of Bath, United Kingdom, 2ASTRON - The Netherlands Institute for Radio Astronomy, Netherlands, 3United Kingdom Research and Innovation - Science & Technology Facilities Council - RAL Space, United Kingdom, 4University of Warmia and Mazury in Olsztyn, Poland, 5University of Oulu, Finland, 6EISCAT Scientific Association, Sweden

Inhomogeneities in the spatial distribution of electron density in the ionosphere can form as a consequence of plasma instability mechanisms. These inhomogeneities (or irregularities) are characterised by a gradient in the electron density that takes place over various spatial scales. In the presence of turbulent processes, larger scale irregularities cascade to smaller scale irregularities. On the basis of observations from artificial satellites, irregularities in the equatorial and high latitudes ionosphere can originate radio wave scintillation at frequencies between the VHF and C band, whereas irregularities forming in the middle latitude ionosphere can originate scintillation mainly at VHF (occasionally, L-band scintillation has been observed as a consequence of plasma structures expanding equatorward from high latitudes during disturbed magnetic conditions). Radio wave scintillation arising from irregularities in the ionosphere has been somehow regularly observed by means of the Low Frequency Array (LOFAR) radio telescope. These observations mainly relate to plasma structures forming in the middle latitude ionosphere. This contribution discusses measurements of radio wave scintillation carried out by using the KAIRA station (which is based on technology similar to standard LOFAR stations) whilst observing the Cassiopeia A object. These observations were carried out in a typical auroral ionosphere under varying magnetic conditions. The comparison between observations from KAIRA and from Global Navigation Satellite Systems (GNSS) enables to identify and characterise ionospheric irregularities forming in the auroral ionosphere. This comparison also allows to discuss any contribution originating outside of the Earth’s ionosphere (e.g., in the inner heliosphere).


ST07-A001
Investigation of Outflow O+ Dynamics in the Earth’s Magnetosphere by 3-D Global Hybrid Simulation

Xueyi WANG1#+, Chih-Ping WANG2, Yu LIN1
1Auburn University, United States, 2University of California, Los Angeles, United States

Outflow oxygen (O+) ions from the ionosphere are one of main particle source for the magnetosphere contributing to mass, momentum, and energy coupling between the ionosphere and magnetosphere. The O+ kinetic dynamics is thus crucial to understanding magnetosphere-ionosphere coupling physics. This presentation is to investigate the global properties of O+ ions and their dynamics both inside and outside the magnetosphere by using a self-consistent 3D global hybrid simulation model, ANGIE3D, developed at Auburn. Specifically, we will present a unique scenario that O+ ions could leak from dayside magnetosphere to the magnetosheath and get access into the upstream solar wind in the presence of a particular type of the IMF directional tangential discontinuity (TD). Some of the leaked O+ ions of ~10’s keV, when encounter the TD in the magnetosheath, can gyrate sunward into the solar wind. These O+ ions get continuously accelerated in the solar wind by convection electric field to > 100 keV without conserving the first adiabatic invariant, and some of them eventually move back to the inner magnetosphere and become part of the ring current. This scenario for generating ring current O+ ions is different from another more typical scenario that ions convect inward from the plasma sheet to the inner magnetosphere and get adiabatically energized.


ST07-A009
Correlations Between Giant Undulations and Plasmapause Configurations

Yijia ZHOU+, Fei HE#
Institute of Geology and Geophysics, Chinese Academy of Sciences, China

In this letter, we report the correlations between giant undulations (GUs) and plasmapause (PP) configurations based on GUs' images and corresponding PP crossings of satellites between 2005 and Typically, GUs occur when the plasmasphere is eroded to form a thin and sharp PP during the storm main phase and early recovery phase. The thicknesses of the PP are usually comparable with the azimuthal wavelengths of the GUs and are smaller than the radial amplitudes of the GUs. The amplitudes and wavelengths are quasi-proportional to the thicknesses of the PP and are inversely quasi-proportional to the ion density gradients around the PP. The radial centers of GUs are typically aligned with the PP surfaces and their radial geocentric locations show positive correlations for different geomagnetic storms. These results would provide both physical insights and model constrains on the magnetosphere-plasmasphere-ionosphere energy coupling and the generation mechanisms of the GUs and plasmapause surface waves.


ST07-A010
Observation of Lunar Tide Effects in Earth’s Magnetosphere

Quanqi SHI#+, Chao XIAO, et AL.
Shandong University, China

Tides are universal and affect spatially distributed systems, ranging from planetary to galactic scales. In the Earth–Moon system, effects caused by lunar tides were reported in the Earth’s crust, oceans, neutral gas-dominated atmosphere (including the ionosphere) and near-ground geomagnetic field. However, whether a lunar tide effect exists in the plasma-dominated regions such as the magnetosphere has not been explored yet. Here we show observational evidence of a lunar tide-induced signal in the plasmasphere (see DOI: 10.1038/s41567-022-01882-8, and other regions in the magnetosphere). We obtain these results by analyzing variations in the plasmasphere’s boundary location over the past four decades from multi-satellite observations. The signal possesses distinct diurnal (and monthly) periodicities, which are different from the semidiurnal (and semimonthly) variations dominant in the previously observed lunar tide effects in other regions. We identified a magnetospheric electric field variation of the same lunar period that can account for the observed plasmapause modulation. Where and how this electric field is generated also has been discussed.


ST07-A011
Downgoing, Upgoing, and Mirroring Expected Electron Spectra and Electron Precipitation Mechanisms by Geomagnetic and Ionospheric Conditions

John DOMBECK1#+, Frdrick ALONZI1, Maria BALVANERA MONTANO1, Clayton JOHNSON1, Joshua MAGNUS2
1University of Minnesota, United States, 2The University of Arizona, United States

Auroral electrons are one of the primary components of magnetosphere-ionosphere-thermosphere (MIT) coupling. Their precipitation, mirroring, interaction in the ionosphere and backscatter account for and affect many of the MIT coupling processes as well as ionospheric conditions. Understanding their composition, characteristics, and dependence on geomagnetic conditions is critical for understanding MIT coupling and ionospheric dynamics. We present the results of a new study which provides the statistically expected effective spectra and variance of downgoing, upgoing, and mirroring electron populations by geomagnetic and ionospheric conditions and location utilizing data from the entire FAST mission. Since the electron populations can be anisotropic and this is not accounted for in most ionospheric models, the effective spectra are calculated. That is the equivalent isotropic spectra over the entire loss cone that would result in the same downgoing or upgoing electron energy flux by energy as the actual distribution. We also present the results, again by geomagnetic and ionospheric conditions and location, of electron precipitation mechanism identification, e.g. wave scattered (or directly precipitating) isotropic precipitation, quasistatic potential structure (QSPS) and Alfvénic acceleration, even when multiple precipitation mechanisms are occurring simultaneously and the QSPS potentials are low compared to the isotropic precipitation temperature.


ST07-A013
The Effects of the Polar Rain on the Polar Wind Ion Outflow from the Nightside Ionosphere

Kun LI#+
Sun Yat-sen University, China

The polar wind, consisting of low-energy ions and electrons, is an outflow along the open magnetic field lines from the polar cap ionosphere to the magnetosphere. Previous studies found that both solar radiation and solar wind electromagnetic energy are the two main energy sources for the polar wind. The polar rain, being field-aligned precipitating electrons from the solar wind to the polar cap, may provide additional energies for the polar wind. This scenario is complicated as simulation studies show that polar rain changes the electric potential structures over the polar cap ionosphere. It is unclear how the polar rain affects the polar wind ion outflow. In this study, we show a positive correlation between the polar wind and the polar rain. Meanwhile, the polar wind is generally diminished in regions with strong Earth’s magnetic field, suggesting the B modulates the penetration depth of the polar rain through the magnetic mirror force and thus the energy dissipation of the polar rain. Therefore, the polar rain can be an additional energy source for the polar wind although the polar rain has generally smaller energies and intensities than the particle precipitations in the auroral regions.


ST07-A014
Lifetime of Energetic Electrons Due to Their Interactions with Chorus Waves

Dedong WANG#+, Yuri SHPRITS, Bernhard HAAS
GFZ German Research Centre for Geosciences, Germany

Energetic electrons in the Earth's magnetosphere can be dangerous to satellites. Chorus waves can cause the loss of energetic electrons in this area via pitch-angle scattering. To quantify the effect of chorus waves on energetic electrons, we calculate the bounce-averaged quasi-linear diffusion coefficients. In this study, using these diffusion coefficients, we calculated the lifetime of the electrons with an energy range from 1 keV to 2 MeV using two different methods. We parameterize the electron lifetime as a function of $L$-shell and electron kinetic energy in each MLT and geomagnetic activity (Kp). The parameterized electron lifetimes show a strong functional dependence on $L$-shell and electron energy. This new model of electron lifetime is more advanced than previous models. In particular, the current model fills the gap that previous models have on the dusk side of the Earth's magnetosphere. This improvement is critical for radiation belt and ring current modelling studies.


ST07-A016
Arase and Van Allen Probes Observations of Variations of Energetic Ion Pitch Angle Distribution and Rapid Flux Variation During Substorm Time Scales

Trunali SHAH1#+, Veenadhari BHASKARA1, Masahito NOSÉ2
1Indian Institute of Geomagnetism, India, 2Nagoya University, Japan

The study investigates variations in the ion flux and pitch angle distribution for the substorms in the inner magnetosphere for the years 2017-2019. The temporal evolution of O+, H+, and He+ ion flux distribution is studied using Arase and Van Allen Probes (VAP/RBSP) spacecraft. RBSP and Arase satellites have different inclinations which give us an opportunity to study the spatiotemporal effect of the substorm time flux variation. The flux variations are also accompanied by magnetic field dipolarization. Previous studies of magnetic field dipolarization in the outer magnetosphere revealed that it is capable of accelerating ions to a few hundred keV. This study focuses on substorm-associated magnetic field dipolarization in the inner magnetosphere as it would play an important role in developing the ring current through in situ acceleration of ions. The Helium Oxygen Proton Electron (HOPE) spectrometer, the Electric Magnetic Field Instrumentation Suit, and Integrated Science (EMFISIS) data on board the RBSP satellite are used. The Low-energy particle experiments (LEPi) and Medium-energy particle experiments (MEPi) data cover the energy range 0.01 keV/q to 180 keV/q which is significant for the substorm time particle dynamics is also used. The purpose of this study is to investigate the possible relationship between ion flux variation and corresponding particle dynamics. The detailed results with analysis of a significant number of events and related mechanisms will be discussed in the meeting.


ST07-A024
Dynamics of Turbulence Behind the Bow Shock and Its Dependence on the Solar Wind Conditions

Liudmila RAKHMANOVA1#+, Maria RIAZANTSEVA1, Alexander KHOKHLACHEV 1, Georgy ZASTENKER2, Yuri YERMOLAEV1
1Space Research Institute of the Russian Academy of Sciences, Russian Federation, 2Russian Academy of Sciences, Russian Federation

Magnetosheath serves as a link between the solar wind and the Earth’s magnetosphere. Experimental studies of last decades demonstrated significant role of the magnetosheath processes and turbulent variations in the global magnetosphere dynamics. Though properties of the magnetosheath turbulence are generally known, the global picture of its development behind the bow shock is still unclear. Present study considers evolution of the turbulence properties while solar wind plasma crosses the bow shock and propagate from the subsolar magnetosheath toward the flanks. Simultaneous observations in three points of the near-Earth’s space are considered – in the solar wind, in the dayside magnetosheath and at the flanks – for various solar wind conditions. The study uses Fourier analysis of fast measurements (with 4/s cadence or better) from a chain of spacecraft such as Wind, Cluster, Themis, Spektr-R and MMS. The work is focused on features of the turbulent cascade around ion scales, where MHD description of plasma flow may not provide satisfactory results and kinetic processes become important. The results show that for undisturbed slow solar wind the fluctuation spectra deviate from typical scaling just in the magnetosheath region close to the bow shock. On the other hand, during the disturbed solar wind (like ICMEs) such deviation occurs in the whole dayside magnetosheath. Spectra tend to restore their initial shape when plasma moves toward the flanks. However, interaction of the compressed solar wind (such as CIRs) with the magnetosheath results in arising of additional compressive fluctuations accompanied with flattening of the fluctuation spectra at the kinetic scales at the magnetosheath flanks. Thus, the conditions in the solar wind play crucial role in dynamics of the magnetosheath turbulence both at MHD and kinetic scales, that can be important for global magnetosphere dynamics. The work is supported by Russian Science Foundation grant № 22-12-00227.


ST07-A026
Complex Magnetospheric Dynamics Based on Forward and Inverse Karman Vortex Coupling

Dongsheng CAI#+
University of Tsukuba, Japan

Complex Magnetospheric Dynamics based on Forward and Inverse Karman Vortex Coupling Kelvin-Helmholtz (K-H) vortexes have been intensively studied using 3D global MHD simulations in the northward IMF. However, they discuss K-H instability theory based on the linear theory and none of them discuss about their nonlinear evolutions and their non-linear behaviors like Karman vortex street, vortex coherency or coherent turbulent structure etc. Those linear vortices evolve to be the so-called the Karman vortex pairs or vortex street between the inner and outer side of the magnetopauses in both dawn and dusk side of the magnetosphere, where the inner vortices are induced by some mechanism under investigation. These vortices are the so-called longitudinal vortices and generated along the earth magnetic field toward both north and south pole. When these vortices extend toward the north and south pole, both vortices from the dawn and dusk sides face each other near the north and south ionosphere and form the so-called inverse Karman vortexes. This is because when they face each other near the ionosphere the rotational direction is inverse to the ordinary Karman vortexes. Thus, the coupling mechanism through the vortex induction between two vortex systems at dawn and dusk side of the magnetosphere are generated. In addition, these inverse Karman vortex coupling are also related to the lobe reconnections.


ST08-A002
Latitudinal Differences of Substorm Expansion Auroras Between Polar VIS and UVI Observations

Suwicha WANNAWICHIAN1#+, Yukinaga MIYASHITA2,3
1Chiang Mai University, Thailand, 2Korea Astronomy and Space Science Institute, Korea, South, 3Korea National University of Science and Technology, Korea, South

Auroral images taken by the Visible Imaging System (VIS) and the Ultraviolet Imager (UVI) instruments onboard the Polar spacecraft were studied in this work to reveal the locations of initial brightening and maximum poleward expansion during 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). The poleward expansions of visible auroral emissions reach higher latitudes than the expansions of far ultraviolet auroral emissions. The latitude of initial brightening was also higher for the visible emissions than for the far ultraviolet emissions. These results suggest that high-energy precipitating electrons producing far ultraviolet aurora tend to be distributed or generated more in the near-Earth magnetotail, while low-energy particles (mostly soft electrons) producing visible aurora are distributed to the more tailward region.


ST08-A003
Unusual Shrinkage and Reshaping of Earth's Magnetosphere Under a Strong Northward Interplanetary Magnetic Field

Xiang-Yu WANG1+, Qing-He ZHANG1#, Chi WANG2, Yongliang ZHANG3, Binbin TANG4, Zanyang XING1, Kjellmar OKSAVIK5, Larry LYONS6, Michael LOCKWOOD7, Qiugang ZONG8, Guo-Jun LI9, Jing LIU1, Yu-Zhang MA10, Yong WANG1
1Shandong University, China, 2Chinese Academy of Sciences, China, 3Johns Hopkins University Applied Physics Laboratory, United States, 4National Space Science Center, Chinese Academy of Sciences, China, 5University of Bergen, Norway, 6University of California, Los Angeles, United States, 7University of Reading, United Kingdom, 8Peking University, China, 9Chongqing University of Posts and Telecommunications, China, 10Shandong University, Weihai, China

The Earth’s magnetosphere is the region of space where plasma behavior is dominated by the geomagnetic field. It has a long tail typically extending hundreds of Earth radii (RE) with plentiful open magnetic fluxes threading the magnetopause associated with magnetic reconnection and momentum transfer from the solar wind. The open-flux is greatly reduced when the interplanetary magnetic field points northward, but the extent of the magnetotail remains unknown. Here we report direct observations of an almost complete disappearance of the open-flux polar cap characterized by merging poleward edges of a conjugate horse-collar aurora (HCA) in both hemispheres’ polar ionosphere. The conjugate HCA is generated by particle precipitation due to Kelvin-Helmholtz instability in the dawn and dusk cold dense plasma sheets (CDPS). These CDPS are consist of solar wind plasma captured by a continuous dual-lobe magnetic reconnections, which is further squeezed into the central magnetotail, resulting in a short “calabash-shaped” magnetotail.


ST08-A009
Investigating Proton Temperature Anisotropy of the Slow Solar Wind with Alfven-wave Turbulence and Micro-instabilities

Hwanhee LEE1#+, Jungjoon SEOUGH1, Bo LI2, Yeon-Han KIM1, Kyungsuk CHO1
1Korea Astronomy and Space Science Institute, Korea, South, 2Shandong University, China

We investigate a one-dimensional solar-wind model that incorporates a curved magnetic field and low-frequency Alfven-wave turbulence. The mechanism for plasma heating and acceleration in this model is represented by the wave dissipation of anisotropic turbulent cascade used in the fast solar wind near a polar coronal hole (Chandran et al. 2011). We extend this mechanism to apply to the slow solar wind by considering a curved magnetic field and also consider the effect of the micro-instabilities on proton temperature anisotropy. The characteristics of the steady-state solution described in this model appears to be associated with those of the Alfvenic slow solar wind stream that are recently reported in the inner heliospheric missions. It is suggested that the dissipation mechanism can be applied in common to both slow and fast solar winds and that the proton cyclotron instability may work effectively near 10-30 solar radii and Earth.


ST08-A012
Soft X-ray Imaging of the Earth's High-latitude Reconnection Region Under Northward Interplanetary Magnetic Fields

Ryota MOMOSE1#+, Yosuke MATSUMOTO1, Yoshizumi MIYOSHI2
1Chiba University, Japan, 2Nagoya University, Japan

The charge exchange between high charge-state ions in the solar wind and the Earth's exosphere (geocorona) emits soft X-rays. This emission process, termed SWCX (Solar Wind Charge eXchange), is useful for visualizing the dayside magnetosphere and its response to solar wind variations. The SMILE and GEO-X missions have been proposed to provide soft X-ray images of the magnetosheath and cusps and will contribute to a better understanding of the dynamic response of the Earth's magnetosphere. For this purpose, we have developed a global magnetohydrodynamic simulation model of the magnetosphere (Matsumoto and Miyoshi, 2022). The model can provide three-dimensional distributions of the soft X-ray intensity from the plasma parameters. Then line-of-sight integrations of the intensity distribution give a two-dimensional X-ray map as a virtual observation in the simulation domain. Therefore, simulation runs under different solar wind conditions allow us to understand how the global intensity map reflects the magnetospheric dynamics. We studied 2D X-ray maps under northward interplanetary magnetic field conditions seen from a high-latitude spacecraft orbit. We found that virtual observations successfully identified the shape of the high-latitude magnetopause. Furthermore, we found that under low plasma-β solar wind conditions, the X-ray intensity can reflect the bulk motion of outflows from the high-latitude reconnection region. This particular observation will give great opportunities to visually understand the spatial extent of the high-latitude magnetic reconnection.


ST08-A013
Why Should We Pay Attention to the Space Environment During Solar Minimum?

Kyung Sun PARK1#+, Jinhye PARK2, Young-Sil KWAK3
1Chungbuk National University, Korea, South, 2Kyung Hee University, Korea, South, 3Korea Astronomy and Space Science Institute, Korea, South

We carried out a high-resolution 3D MHD simulation of the interaction between the solar wind and the magnetosphere during a strong magnetic substorm on June 8, 2019, during the solar minimum. The input parameter to the simulation was from the OMNI solar wind and IMF data for 8 hour period on June 8. The solar wind density is over 20 cm-3 and it increases up to 49 cm-3 with a slow velocity. The dynamic pressure of the solar wind is in the range of 2-12 nPa. The IMF Bz has decreased to -18.5 nT at 1655 UT. In this period, there was no solar flare and CME, and zero sunspot number. However, the AL index reached the minimum value of -1500 nT when the Dst index was not changed significantly. The cross-polar cap potential value from SuperDARN had up to 83 kV while it maintained above 60 kV. Similar disturbances phenomena were frequently observed in 2019 even though the solar minimum. We selected several similar events to identify the causes and differences. From the simulation results, we show that the configuration of the magnetic field lines is dramatically changed by the IMF angle. The stretched closed field lines appear at dawn and dusk flank region. The strong tail reconnection occurs during the strong southward IMF at 1655 UT but the plasma sheet become thin after the tail reconnection and the strong tailward flow in there. The flow in the throat region (near noon) is poleward on the dayside and enhanced energy flux on the dayside is confined in the cusp region. The open-closed boundary extends at 66° on the night side. The cross-polar cap potential is governed by IMF Bz in this event. The simulated cross-polar cap potential is consistent with the inferred from the SuperDARN observation.


ST10-A003
Quantitative Analysis of Electron Acceleration in Coalescing Magnetic Flux Ropes at Earth’s Magnetopause

Wenqing MA1+, Meng ZHOU1,2#, Zhihong ZHONG1
1Nanchang University, China, 2University of California, Los Angeles, United States

The coalescence of magnetic flux ropes (MFRs) is widely acknowledged as a crucial mechanism for electron acceleration in astrophysics. However, in-situ observations of electron acceleration resulting from flux rope coalescence are limited due to the vast spatial scale in astrophysical environments. Our study, using magnetospheric multiscale (MMS) observations, reveals the presence of three coalescing MFRs in pairs at Earth’s magnetopause, which resulted in the generation of superthermal electrons. We find that the superthermal electron flux in the coalescing MFRs was several times higher compared to that in the magnetosheath. Two primary mechanisms, Fermi acceleration and parallel electric fields (E||), were responsible for the electron acceleration, with betatron acceleration being negligible. The majority of Fermi acceleration was observed in the squeezed magnetic flux rope at the center of the three MFRs, while E||-driven acceleration occurred primarily at the reconnection site between the coalescing MFRs. Our results indicate that coalescence enhances Fermi acceleration more than non-coalescing MFRs.


ST10-A010
Magnetospheric Multiscale Observations of Kelvin-Helmholtz Waves and Magnetic Reconnection Under Southward Interplanetary Magnetic Field

Tongkuai LI1#+, Wenya LI1, Binbin TANG2, Chi WANG1
1Chinese Academy of Sciences, China, 2National Space Science Center, Chinese Academy of Sciences, China

Kelvin-Helmholtz (K-H) waves and magnetic reconnection are two important physical phenomena frequently occurring at the Earth's magnetopause, which play a crucial role in transporting mass, momentum, and energy from the solar wind into the magnetosphere. Whether the K-H waves and magnetic reconnection can occur simultaneously under southward interplanetary magnetic field (IMF) is still unclear. Here, based on in-situ observations from the Magnetospheric Multiscale (MMS) mission, we analyzed one K-H wave event under southward IMF accompanied by on-going magnetic reconnection. The K-H waves are identified by the quasi-periodic fluctuations, the plasma with low density and high speed, and the variation of the boundary normal vectors on the leading and trailing edges. The on-going magnetic reconnection is identified by the Alfvenic ion jets and escaping of the magnetospheric electrons. The signals of on-going reconnection are found in most current sheet crossings on both the trailing and leading edges. These results indicate that the co-occurring process of the K-H waves and magnetic reconnection under southward IMF is different from that under northward IMF. The K-H waves can promote the excitation of magnetic reconnection by the current-sheet thinning along the magnetopause. On the other way, magnetic reconnection may likely suppress the evolution of the K-H waves.


ST10-A011
Energization of Cold Ions in Asymmetric Reconnection: Particle-in-cell Simulation

Liangjin SONG1+, Meng ZHOU1,2#, Yongyuan YI1, Xiaohua DENG3
1Nanchang University, China, 2University of California, Los Angeles, United States, 3Wuhan University, China

Cold ions from Earth's ionosphere and plasmasphere are frequently observed at the Earth's magnetopause, impacting reconnection in ways such as altering the reconnection rate and energy budget. Despite extensive research on reconnection, the fluid properties and kinetics of cold ions in magnetopause reconnection remain unclear. Our recent 2-D particle-in-cell simulation provides new insight into cold ion dynamics in asymmetric reconnection. Our simulation shows that cold ions, initially located only in the magnetosphere, absorb 10% to 25% of the total released magnetic energy, primarily converting it into thermal energy through stochastic heating, that is, the viscous heating associated with the non-gyrotropic pressure tensor. Cold ions are step-by-step accelerated by the Hall electric field during meandering motion across the magnetopause current sheet. The velocity distribution functions of cold ions in different regions are made up of two types of particles, differentiated by their ability to penetrate into the magnetosheath. The reconnection electric field has different effects on these two types of cold ions. As reconnection continues, the velocity distribution functions of the cold ions diffuse, leading to bulking heating. These findings significantly enhance our understanding of cold ion dynamics at the Earth's magnetopause.


ST10-A022
Formation of Negative J*E' in the Electron Diffusion Region During Magnetic Reconnection: PIC Simulations and MMS Observations

Qiyang XIONG1+, Shiyong HUANG1#, Meng ZHOU2,3, Zhigang YUAN1, Xiaohua DENG1, Kui JIANG1, Yunyun WEI1, Sibo XU1, Jian ZHANG1, Rentong LIN1, Lin YU1
1Wuhan University, China, 2Nanchang University, China, 3University of California, Los Angeles, United States

It is widely acknowledged that high positive energy conversion J*E’ from the fields to the plasma occurs in the electron diffusion region (EDR) during magnetic reconnection. There also exists negative J*E’ which means the particles return the energy to the field. How this kind of negative energy conversion appears in the reconnection is still lack of comprehensive explanation. In this study, we applied 2.5-D full kinetic particle-in-cell (PIC) simulations and high-resolution data from Magnetospheric Multiscale mission (MMS) to reveal the formation of the negative J*E’ near the EDR. Two main regions are found to have the negative energy conversion gathering: one is the outer EDR, and the other one is the inflow edge of the inner EDR. The PIC simulations suggest that in the outer EDR the negative J*E’ is contributed by the electron inertial term of the generalized Ohm’s law due to the deceleration of the electrons. This deceleration is caused by the opposite electric field which is induced by the magnetic field accumulation in the outer EDR. On the other hand, both PIC simulations and MMS observations verify that the negative J*E’ in the inflow edge is balanced by the electron pressure tensor term. The energy loss of the electrons plays the dominant effect in this term and the energy decline is caused by the electric field which induced by the decreasing magnetic field in the inflow region. These results provide significant insights to expand the understanding of the reconnection regimes.


ST10-A023
Simultaneous Observations of Dayside Magnetopause Crossings from MMS and THEMIS

Chongle ZHANG1#+, Wenya LI1, Binbin TANG2
1Chinese Academy of Sciences, China, 2National Space Science Center, Chinese Academy of Sciences, China

Response of the magnetopause to the upstream solar wind is an important issue to understand the mass and energy transfer across this boundary, but the spatial-temporal effect is usually hard to distinguish. In this study, we have performed simultaneous observations of dayside magnetopause crossings from MMS and THEMIS to investigate the magnetopause activities spatially. We search for such magnetopause crossing events under the constraints that the time difference of the magnetopause crossing between MMS and THEMIS is less than 5 minutes. The results show that the MMS and THEMIS can observe either similar or dissimilar magnetopause activities (i.e. The reconnection jet) at different events at a separation of several Earth radii. These observations can be attributed to the limited spatial extent of magnetopause activities and/or different responses to the upstream solar wind.


ST10-A024
Observations of Dynamical Flux Ropes and Active Multiple X-line Reconnection at Earth’s Magnetopause

Zhihong ZHONG1#+, Guangya LEI1, Meng ZHOU1,2, Meng ZHANG1, Rongxin TANG1,3, Daniel GRAHAM4, Ye PANG1, Xiaohua DENG5, Yuri KHOTYAINTSEV4
1Nanchang University, China, 2University of California, Los Angeles, United States, 3Memorial University of Newfoundland, Canada, 4Swedish Institute of Space Physics, Sweden, 5Wuhan University, China

We present the Magnetospheric Multiscale (MMS) observations of three flux ropes (FRs) sequentially in a reconnection exhaust at Earth’s magnetopause. Three active X-lines, which are responsible for the formation of these FRs, were also detected by MMS, providing strong evidence that the FRs were generated by multiple X-line reconnection. We find that the core field inside the FRs considerably affects the Hall current in the adjacent X-lines. The intense core field of the FRs deflected the electron outflow jet, forming the electron-scale Hall magnetic field on the magnetosheath side. Additionally, an active secondary reconnection was observed at the center of one FR. This secondary reconnection split the FR into two smaller FRs and produced sharp density gradients and intense fluctuations of electric field and current within the FR. Our observations advance the understanding of the formation and evolution of FRs during multiple X-line reconnection at magnetopause.


ST11-A002
Forecasting the Final Dst Index with Temporal Convolutional Network

Junyan LIU1#+, Chenglong SHEN1, Mengjiao XU1, Yutian CHI2, Zhihui ZHONG1, Dongwei MAO1, Zhiyong ZHANG1, Can WANG3
1University of Science and Technology of China, China, 2Deep Space Exploration Laboratory, China, 3China Earthquake Administration, China

The Dst Index(disturbance storm time index) is one of the most important geomagnetic indices to describe the strength of geomagnetic activity. The accurate prediction of the Dst index helps avoid the hazards of severe space weather events. Therefore, Dst prediction has been a hot topic in space physics and space weather forecasting for a long time. Using observational data such as three components of the magnetic field, solar wind speed, proton density, etc., this paper incorporates the temporal Convolutional Network (TCN) to predict the Dst indices. Compared to the previous machine learning model, our model has very high forecast accuracy. The specific results are: the mean square root error (RMSE) between the prediction value and the real value is 2.876, the average absolute error (MAE) is 2.003 and the correlation coefficient r is 0.9846. Our single model can reach equivalent accuracy predicted by several machine learning models together. Besides, we also try to explain our model with the integrated gradient(IG) algorithm. The past Dst index, the z component of magnetic field $B_z$, and the plasma flow speed during the past two hours are the main control parameters for the Dst index prediction. These results confirm that the TCN algorithm can help us to improve the space weather forecast accuracy and understand the physical processes in space weather at the same time.


ST11-A003
Interplanetary Coronal Mass Ejection Southward Magnetic Field Estimation at Venus Based on In-situ Observations at 1AU

Dongwei MAO1+, Chenglong SHEN1#, Yutian CHI2, Mengjiao XU1, Zhihui ZHONG1, Junyan LIU1, Zhiyong ZHANG1, Can WANG3
1University of Science and Technology of China, China, 2Deep Space Exploration Laboratory, China, 3China Earthquake Administration, China

Development of human activities at other planets calls for space weather forecasting, especially southward magnetic field of Interplanetary Coronal Mass Ejections(ICMEs) which are related to intense magnetic storms. We select several ICMEs that can be detected by both Venus Express and WIND and estimate their magnetic fields at Venus based on in-situ observations at Earth. The magnetic structure of ICMEs is described with Lunquist model, and parameters of the model are gained from a least square fitting method. The propagation of ICMEs is assumed to be self-similar, so the ICME magnetic structure at Venus can be calculated from which at Earth. A drag-based model is used to estimate the arrival time of ICMEs at Venus based on the speed profile and time of arrival at Earth. 


ST11-A005
Variations in Regional Precipitation Under Extreme Solar Activity

Yuqi WANG1+, Yong WEI2#
1Chinese Academy of Sciences, China, 2Institute of Geology and Geophysics, Chinese Academy of Sciences, China

Extreme solar activity can cause space weather hazards and have a significant impact on the Earth's weather and climate. Direct observations of sunspots date back about 400 years, when Maunder Minimum (1645-1715) was discovered and accompanied by prolonged periods of severe cold in the Earth's climate. This research contributes to analyse the regional precipitation variations under extreme solar activity. A unique approach was taken to reconstruct the continuous annual precipitation in Seoul from 1625 to the present based on the ancient book, including the world's earliest continuous instrumental rainfall records. Based the independent precipitation database, we found a significant correlation between solar activity and regional precipitation on multiple time scales. (i) An 11-year sunspot cycle exists in regional precipitation variation. (ii) During periods of the great Solar Minimum, summer rainfall and winter snowfall are significantly reduced on an interdecadal scale. (iii) Extreme precipitation is more likely to occur during sunspot maximum or minimum. The mechanisms by which solar activity affects sea-air coupling and hence precipitation in the Pacific region are complex. Investigating precipitation changes under extreme solar activity is of great significance to human production and to help deal with drought and flood disasters. 


ST11-A006
The Interplanetary Origins of Geomagnetic Storm with Dst < -50 nT During Solar Cycle 24 (2009–2019)

Zhiyong ZHANG#+, Shican QIU
University of Science and Technology of China, China

In this study, we analyzed 149 geomagnetic storms of moderate and intensity (i.e., Dstmin < -50 nT) occurred during the solar cycle 24 from 2009 to 2019, and identified their interplanetary sources. Among them, there are 20 strong storms with -200 nT < Dstmin < -100 nT, and 2 super–strong storms with Dstmin < -200 nT. We have found that corotating interaction regions (CIRs) account for 37% (55/149) of geomagnetic storms, interplanetary coronal mass ejections (ICMEs) result in 30% (45/149) of geomagnetic storms and sheath regions (SH) are responsible for 15% (23/149) of geomagnetic storms. Meanwhile, 18/20 of the strong storms are caused by the structures associated with interplanetary coronal mass ejections (ICME, SH, and SH + ICME), while the CIR constitutes only to 2/20 of the strong storms. It is found that the two super–strong geomagnetic storms are caused by the SH + ICME. Our findings also suggest that geomagnetic storms in different periods of solar activity are caused by different interplanetary structures, which is consistent with previous research. In comparison to solar cycle 23, there is no substantial geomagnetic storm induced by CIR during the dwindling and subsiding phases of solar cycle 24. In the descending stage, the proportion of moderate events caused by ICME decreases, and ICMEs cause no super–strong event. In ascending stage, neither strong nor super strong events occur.


ST11-A009
Analysis of the Interaction Between Coronal Mass Ejections Based on a Simplified Collision Model

Zhihui ZHONG1+, Chenglong SHEN1#, Yutian CHI2, Can WANG1, Mengjiao XU1, Dongwei MAO1
1University of Science and Technology of China, China, 2Deep Space Exploration Laboratory, China

Coronal mass ejection (CME) is a large-scale solar explosion, which carries a large amount of plasma into interplanetary space and affects the interplanetary environment. The continuous bursts of multiple CMEs, specially the interaction between CMEs, will make the magnetic field and plasma environment in solar-terrestrial space more complex. According to previous studies, the interaction between CMEs will change the propagation direction and velocity of CMEs, and even super-elastic collision occurs. However, due to the complex structure of CMEs and the lack of observation equipment, the interaction process between CMEs cannot be well explained. In this work, a simplified collision model is proposed to analyze the interaction between CMEs. In order to verify the effectiveness of this model, we analyzed two events. The results show that our simplified collision model can effectively describe the interaction process of the two CMEs and predict the velocity and direction of post-interaction CMEs.


ST12-A009
Interference Suppression Method of Oblique Backscatter Ionogram Based on Adaptive Partitioning of Eigen-subspaces Filtering

Chongzhe LAO#+, Guobin YANG, Tongxin LIU, Chunhua JIANG
Wuhan University, China

The oblique backscatter sounding method can provide ionospheric state information with a radius of several thousand kilometers in all directions, which is a promising ground-based detection technology. However, some celestial interference and industrial interference will greatly reduce the signal-to-interference-noise ratio of the ionospheric oblique backscatter detection signal, making it difficult to extract ionospheric information from the ionogram. In this study, an interference suppression algorithm based on adaptive partitioning of eigen-subspaces for low power oblique backscatter detectors is proposed. The interference data of WIOBSS is decomposed and subjected to an adaptive subspace division based on the plural criterion, the echoes are projected into the signal subspace to filter out the interference, and the background noise is homogenized by a constant false alarm, with an energy contrast stretching algorithm to enhance the signal in the HF band to obtain a high contrast oblique back scatter ionogram with a uniform background, which greatly improves the information extraction capability of the oblique backscatter ionogram. Both simulation and experimental results are provided to illustrate the performance of the proposed method. This algorithm is more reliable than the image domain algorithm, has lower hardware requirements and is easier to implement than the air domain algorithm, which has good engineering application value.


ST13-A007
Features of Low-frequency Waves in the Plasma Sheet Associated with Dipolarization for Substorms and Pseudosubstorms

Kanpatom KASONSUWAN1#+, Yukinaga MIYASHITA2,3, Suwicha WANNAWICHIAN1
1Chiang Mai University, Thailand, 2Korea Astronomy and Space Science Institute, Korea, South, 3Korea National University of Science and Technology, Korea, South

Substorms and pseudosubstorms (pseudobreakups) involve explosive auroral activities which are caused by the magnetotail dynamics. Previous studies showed that substorms and pseudosubstorms have some different characteristics in both spatial and temporal development. This study mainly focuses on the features of low-frequency (0.002 - 0.006 Hz), Pi2, and Pi1 waves in the plasma sheet, such as wave power and Poynting flux, based on superposed epoch analysis of data from the Time History of Events and Macroscale Interactions during Substorms (THEMIS) spacecraft. We find that low-frequency and Pi2 waves are amplified before dipolarization onset, followed by Pi1 waves at the onset. This result suggests that an instability related to low-frequency waves, such as ballooning instability, is excited before dipolarization onset, and then other instabilities related to higher-frequency waves are excited at dipolarization onset. The power and parallel Poynting flux toward the ionosphere of low-frequency, Pi2, and Pi1 waves for substorms are more intense than those for pseudosubstorms. Moreover, the wave powers of the magnetic field during pseudosubstorms decrease earlier than those during substorms. These results suggest that both an instability related to low-frequency waves and instabilities related to higher-frequency waves grow sufficiently for full-fledged substorms or auroral poleward expansion. The wave power of the parallel component related to magnetosonic waves is more intense than those of the perpendicular components related to Alfven waves for both substorms and pseudosubstorms. The wave parallel Poynting flux toward the earth ionosphere after dipolarization onset during substorms is larger and lasts longer than that during pseudosubstorms.


ST13-A009
Global ULF Waves Excited by Positive Solar Wind Dynamic Pressure Impulses: Ground-based Statistical Study

Zikang XIE1+, Qiugang ZONG1#, Jie REN2, Chao YUE1, Zhiyang LIU1, Li LI1, Ze-Fan YIN1, Xingyu LI1
1Peking University, China, 2China University of Geosciences (Beijing), China

The positive solar wind dynamic pressure pulse is one of the sources of ULF waves. Based on 1s-resolution magnetic field observations from global geomagnetic stations between the beginning 2012 and the end of 2019, we conducted statistics on temporal and spatial variations of gloal ULF power after the positive dynamic pressure pulse arrival. The magnetosphere responds quickly to the dynamic pressure pulse within 1 minute, and at low L values, it takes 4 to 6 minutes for the ULF waves to reach a power maximum, with a local decay time scale of about 10 minutes in magnitude. A dawn-dusk Pc3 power asymmetry is independent of solar wind conditions. indicating that Pc3 fluctuations may be excited by multiple sources and influenced by the effects of propagation. There is a north-south asymmetry in ULF fluctuations, and higher latitudes in the northern hemisphere tend to have stronger fluctuations. The magnetic field power in different bands exhibits seasonal effects, which can be further explained by the R-M effect. Based on the integrated power intensity of different bands of the global geomagnetic stations, and it would be helpful to compare the results with observations of satellites in GEO orbit such as the SWARM and Champ. Widespread asymmetries in different IMF conditions need to be further studied.


ST13-A011
The Structure Particle Distribution and Aurora Associated with Magnetospheric Compressional Pc5 Waves

Anmin TIAN#+
Shandong University, China

Pc5 compressional wave observed in the Earth magnetosphere is attracting extensive attention due to its high occurrence, rich wave-particle interaction processes and possible ionospheric effects. The complete geometric picture and particle pitch angle distributions (PADs) are keys to understand the generation and spatial effects of this kind of wave. However, there has been a lack of sufficient observation support. In our recent works, we built the three dimensional geometric structure of the wave and obtained the statistical characteristics of electron PADs and aurora phenomena related to the wave using data from MMS and THEMIS mission. It is found that the equatorial cross-section of the magnetic decreases (troughs) of compressional Pc5 waves has an 'eccentric wedge-like' shape with a radial scale larger than 4Re. The electron PADs in the magnetic troughs are classified into three types: cigar, butterfly, and pancake. The dependence of electron PAD types on electron energy depends on whether whistler waves are observed in the magnetic troughs or not. We further systematically expounded the modulation effect of Pc5 compressional wave on aurora based on THEMIS spacecraft and ground all sky imager observations.


ST13-A012
Spatial Propagation of Ground ULF Magnetic Field Oscillations Excited by Different Types of Foreshock Bubbles

Jiaqi LIU1+, Boyi WANG1#, Terry LIU2, Desheng HAN3, Yi WANG1, Vassilis ANGELOPOULOS2
1Harbin Institute of Technology, Shenzhen, China, 2University of California, Los Angeles, United States, 3Tongji University, China

Foreshock bubbles are transient structures caused by the interaction of suprathermal backstreaming ions upstream of the bow shock with rotational discontinuities (RDs) or tangential discontinuities (TDs). Due to their hot tenuous cores, foreshock bubbles can inflate the magnetopause and excite magnetospheric Pc5 (1.66~6.66 mHZ) ultra-low frequency (ULF) waves, which are proposed to be global by hybrid simulations. These waves are possibly transported to the ground through the coupled magnetospheric and ionospheric system. However, how do foreshock bubbles contribute to ground magnetic field disturbances and does this contribution depends on the characteristics of foreshock bubbles are still poorly understood. In this study, we investigate the differences between RD-driven and TD-driven foreshock bubbles in generating ground magnetic field oscillations (primarily in Pc5 band), based on the conjugated observations by the THEMIS satellites and high-latitudinal (60-75 MLAT) ground-based magnetometers in 2008, 2009 and in 2019. Multiple foreshock bubble events show that foreshock bubbles can indeed generate significant ground magnetic field Pc5 ULF oscillations. But we further found that whether these induced oscillations can propagate globally or propagate through only one side of the magnetosphere (duskward or dawnward) probably depend on the types of the associated interplanetary magnetic field (IMF) discontinuities (TD or RD), their normals and the relative position between the core of a foreshock bubble and its associated IMF discontinuity. More relationships between the characteristics of foreshock bubbles with the associated ground magnetic field oscillations will also be discussed.


ST13-A016
Statistical Characterization of Joule Heating Related to Ionospheric ULF Perturbations Using SuperDARN Data

Xueling SHI1,2#+, Shibaji CHAKRABORTY1, Joseph BAKER1, Michael HARTINGER3, Dong LIN2, Wenbin WANG2, J. RUOHONIEMI1, Kevin STERNE1
1Virginia Tech, United States, 2National Center for Atmospheric Research, United States, 3Space Science Institute, United States

Ultra-low frequency (ULF; 1 mHz - several Hz) waves are ubiquitous in the solar-terrestrial environment. They play important roles in transporting and coupling energy throughout the geospace system. Despite the fact that ULF pulsations have been studied for over a century, major questions remain regarding their significance for energy deposition through Joule heating in the ionosphere-thermosphere (I-T) system. The objective of this study is to quantify the energy deposition in the I-T system related to ionospheric ULF perturbations. We use measurements from SuperDARN HF coherent scatter radars operating in a special mode, in which three camping beams are sampled at ~ 18 s by interleaving soundings on the camping beams with successive beams of the normal azimuth scan. The Joule heating rate associated with ULF perturbations is estimated by using ionospheric electric fields from SuperDARN measurements and height-integrated Pedersen conductance from empirical models. We report statistical results on the ionospheric ULF wave occurrence and related electric field distributions. The dependencies of the ULF wave-related Joule heating rate on wave properties, solar wind conditions, and geomagnetic activity level are investigated. The results provide new insights into the role of ULF waves in energy transfer and dissipation in the geospace system.


ST13-A023
Statistical Study on the Azimuthal Mode Number of Pc5 ULF Wave in the Inner Magnetosphere

Wenlong LIU#+
Beihang University, China

The azimuthal mode number, m, of the ULF wave is important in the wave-particle interaction with radiation belt electrons because it determines the resonating energy of the particles. Based on multi-point magnetic field measurements of GOES satellites from January to September 2011, we statistically analyze the characteristics of the m value of Pc5 ULF waves. The wave propagation directions are classified into eastward or westward directions according to the sign of m. We find that in the dayside, the waves propagate predominantly westward (eastward) in the post-non (pre-noon), i.e., propagating anti-sunward. We also find that during quiet periods, the waves of |m|≤3 dominate in the inner magnetosphere. With increasing solar wind and geomagnetic activity, the intensity of ULF waves in the magnetosphere is also enhanced and the waves of |m|>3 have a stronger response to substorm activity at nightside.


ST14-A003
The Dynamics of Near-solar Charged Nanodust During the Rising Phase of the Solar Cycle 24

Yi-Shiang TZENG1#+, Li-Ping YANG2, Wing-Huen IP1
1National Central University, Taiwan, 2National Space Science Center, China

For decades, the information on the near-solar dust cloud has been acquired through not only remote-sensing observations but the detections of high-speed nanodust impacts by spacecraft, such as Ulysses and Parker Solar Probe (PSP). These nanodust impact measurements are generally believed to result from the so-called hyperbolic beta-meteoroids, which break apart from larger bodies through collision or sublimation in the near-sun region. These tiny particles can be propelled radially forward by solar radiation. Moreover, when fragmented small enough, they can also be deflected by electromagnetic forces. As previous research pictures a scenario of understanding the near-solar dust environment by multi-point measurements by PSP and future Solar Orbiter (SolO), we believe that it is crucial and worthwhile to conduct more in-depth studies of the nanodust dynamics in the near-sun region. Therefore, in order to explore the charged nanodust sources, distributions, and their potential impacts on objects within the inner solar system, such as spacecraft and planets, here we conduct a comprehensive survey of the charged nanodust behavior during the rising phase of the Solar Cycle 24, based on a 3D SIP-AMR-CESE MHD solar-wind model. This work could also be beneficial in preparing for future, more detailed analyses of PSP and SolO observations.


ST14-A006 | Invited
Modeling CME-driven Shocks Through an Inhomogeneous Solar Wind: Challenges and Future Improvements

Meng JIN1#+, Nariaki NITTA2, Christina COHEN3
1Lockheed Martin Advanced Technology Laboratories, United States, 2Lockheed Martin Solar and Astrophysics Laboratory, United States, 3California Institute of Technology, United States

In the past decade, significant efforts have been made in developing physics-based solar wind and coronal mass ejection (CME) models, which have been or are being transferred to national centers (e.g., SWPC, CCMC) to enable space weather predictive capability. However, the input data coverage for space weather forecasting is extremely limited. One major limitation is the solar magnetic field measurements, which are used to specify the inner boundary conditions of the global magnetohydrodynamic (MHD) models. In this study, by using the Alfven wave solar model (AWSoM) to simulate a realistic solar eruptive event on 2013 April 11, we demonstrate that due to the inhomogeneous background solar wind and dynamical evolution of the CME, the CME-driven shock parameters change significantly both spatially and temporally as the CME propagates through the heliosphere. The input magnetic map has a great impact on the shock connectivity and shock properties in the global MHD simulation. Therefore this study illustrates the importance of taking into account the model uncertainty due to the imperfect magnetic field measurements when using the model to provide space weather predictions. In addition, we discuss strategies to improve model performance, especially by incorporating newly available state-of-the-art in-situ and remote-sensing observations.


ST14-A007
On the Activities in the Lower Corona Associated with the Formation of a Streamer Blob

Li HAIYI#+, Zhenghua HUANG, Lidong XIA, Hui FU, Deng KAIWEN, Hengyuan WEI, Zhang CHAO
Shandong University, China

Small-scale propagating blobs in helmet coronal streamers could be an important source of the slow solar wind. They are widely believed to be results of magnetic reconnection between open and close magnetic field. However no direct observations has been reported to either support or deny such mechanism. Using observations from SUVI/GOES and AIA/SDO, here we study precusors of a streamer blob as seen in the corona below 2.0 solar radii. We found that at altitudes below 2.0R the streamer blob was formed due to the gradual merging of three clumps of materials initiated from the lower corona. One of the clumps of materials may have been formed by the expansion and stretching of the loop structure at the base of the helmet coronal streamer. The other two clumps of materials may have been formed by the swing of the loop structure in the north-south direction in the base of the helmet streamer. In these observations, we do not observe reconnection between loops and open field lines. We raise a question whether magnetic reconnection actually occurred to drive the observed streamer blob. We also propose a possible mechanism to interpret the formation of this event. These observations might help us understand small-scale transients that frequently found in the solar wind near the sun.


ST14-A013 | Invited
Three-dimensional Anisotropy and Scaling Properties of Solar Wind Turbulence at Kinetic Scales in Inner Heliosphere: Parker Solar Probe Observations

Jian ZHANG1+, Shiyong HUANG1#, Jiansen HE2, Tieyan WANG3, Zhigang YUAN1, Xiaohua DENG1, Kui JIANG1, Yunyun WEI1, Sibo XU1, Qiyang XIONG1, Rentong LIN1, Lin YU1
1Wuhan University, China, 2Peking University, China, 3Yunnan University, China

We utilize the data from Parker Solar Probe (PSP) mission at its first perihelion to investigate the three-dimensional (3D) anisotropies and scalings of solar wind turbulence for the total, the perpendicular and the parallel magnetic-field fluctuations at kinetic scales in the inner heliosphere. By calculating the five-point second-order structure functions (SFs), we find that the three characteristic lengths of turbulence eddies for the total and the perpendicular magnetic-field fluctuations in the local reference frame (LPerp, lPerp, l||) defined with respect to local mean magnetic field Blocal feature as l||>LPerp>lPerp in both the transition range and the ion-to-electron scales, but l||>LPerp~lPerp for the parallel magnetic-field fluctuations. For the total magnetic-field fluctuations, the wavevector-anisotropy scalings are characterized by l||~lPerp0.78 and LPerp~lPerp1.02 in the transition range, and they feature as l||~lPerp0.44 and LPerp~lPerp0.73 in the ion-to-electron scales. These observational results need more complete kinetic-scale turbulence model to account for.


ST14-A017
Radial Evolution of the Wavelike Compressional Turbulence in the Inner Heliosphere

Jiansen HE1#+, Die DUAN1, Xingyu ZHU2, Daniel VERSCHAREN3, Trevor BOWEN4, Bale STUART4
1Peking University, China, 2University of Alabama in Huntsville, United States, 3University College London, United Kingdom, 4University of California, Berkeley, United States

The quasi-radial alignment between Parker Solar Probe (PSP) and other spacecraft further away from the sun provides a great opportunity to observe the radial evolution of the wavelike compressional turbulence from the inner heliosphere near the solar corona to the near-earth environment. We choose the 4th and 11th encounters of PSP with their respective perihelion distances of ~30 Rs and 13 Rs away from the sun to address this issue. Similar time profiles of solar wind variables' changes are observed from both PSP and Wind (at 1 au) measurements. The accelerating-solar-wind model could be more suitable than the constant speed model for the observation, which means the solar wind is still accelerating from the perihelion distance (e.g., 30 Rs) to 1 au. Both PSP and Wind measure the co-existence of the Alfvenic and compressive fluctuations in the solar wind. It is interesting to note that the good correlation between radial velocity component (dVR), proton density (dn) and temperature (dT) fluctuations indicate the nature of the compressive fluctuations are outward-propagating slow-mode waves. However, dn and d|B| is well not correlated for PSP measurements, but in good correlation for Wind measurements, which indicates the propagating direction of the slow-mode waves is evolving along the distance from the quasi-parallel direction to the quasi-perpendicular direction. Comparing the radial evolution of the energies of both Alfvenic and compressive fluctuations with the WKB model, we find the observed energy decays slower than the theoretical prediction, which indicates the existence of extra energy injection and energy cascade during the solar wind expansion.


ST14-A018
Scaling Anisotropy with Stationary Background Field in the Near-sun Solar Wind Turbulence

Honghong WU1#+, Jiansen HE2, Shiyong HUANG1, Li-Ping YANG3, Xin WANG2, ZhiGang YUAN1
1Wuhan University, China, 2Peking University, China, 3National Space Science Center, China

The scaling of magnetic fluctuations provides crucial information for the understanding of solar wind turbulence. However, the observed magnetic fluctuations contain not only turbulence but also magnetic structures, leading to the violation of the time stationarity. This violation would conceal the true scaling and influence the determination of the sampling angle with respect to the local background magnetic field. Here, to investigate the scaling anisotropy, we utilize an easy but effective criterion $\phi<10^\circ$ to ensure the time stationarity of the magnetic field, where $\phi$ is the angle between the two averaged magnetic fields after cutting the interval into two halves. We study the scaling anisotropy using higher-order statistics of structure functions \textbf{under the condition of stationarity} for the near-Sun solar wind turbulence for the first time based on measurements obtained from Parker Solar Probe (PSP) at 0.17 au. We find that the scaling indices $\xi$ of magnetic field show a linear dependence on the order $p$ close to $\xi(p)=p/4$. The multifractal scaling of magnetic-trace structure functions becomes monoscaling close to $\xi(p)=p/3$ with the local magnetic field perpendicular to the sampling direction and close to $\xi(p)=p/4$ with the local magnetic field parallel to the sampling direction when measured with the stationary background magnetic field. The scaling of velocity-trace structure functions has similar but less significant changes. The near-Sun solar wind turbulence displays different scaling anisotropies with the near-Earth solar wind turbulence, suggesting the evolution of the nonlinear interaction process during the solar wind expansion.


ST14-A019
Observations of Preferential Heating and Acceleration of Solar Wind Alpha Particles in the Inner Heliosphere

Jingyu PENG1#+, Jiansen HE1, Xingyu ZHU2, Ziqi WU1, Die DUAN1
1Peking University, China, 2University of Alabama in Huntsville, United States

Remote sensing of the nascent solar wind in the solar corona shows that heavy ions can be faster and hotter simultaneously than protons. While in situ detection of the near-Earth solar wind illustrates that hotter and faster states of heavy ions than protons do not happen simultaneously. So it is curious what happens to the heating and acceleration of heavy ions in the inner heliosphere. The answer would also be helpful for understanding the mechanisms for the preferential heating and acceleration of heavy ions and its competition with another important physical process, Coulomb collisions. Specifically, what is the spatial extent of the zone of preferential heating and acceleration for heavy ions? Although it is speculated to start from less than one solar radiu above the solar surface and continue to tens of solar radii, the hypothesis is not yet observationally examed. Parker Solar Probe is currently the closest spacecraft to the Sun and is highly anticipated to cross the outer boundary of the preferential heating and acceleration zone and provide additional clues to the related mechanisms. Using observations from Parker Solar Probe, we find that larger α-proton drift speeds in the solar wind correspond to larger α-proton temperature ratios close to the corona. This feature differs from in situ detections farther from the Sun (e.g., Helios, Wind at 0.3~1AU). Collisions and instabilities may be responsible for this radial evolution of the α-particle properties in the solar wind. In addition, we try to identify the outer boundary of the preferential heating and acceleration zone. We find that preferential heating is weaker than the effect of cooling due to collisions, with no significant preferential heating zone observed. We also find that the preferential acceleration is obvious within 0.16 au, which may correspond to the preferential acceleration zone.


ST14-A020
Kinetic Effects of Alpha Proton Participation on the Turbulence Decaying

Qiyang XIONG+, Shiyong HUANG#
Wuhan University, China

Turbulence is acknowledged to exist extensively in the space plasma environments, functioning on the mass transferring, particles heating, and energy dissipation. The alpha particles can have an extensive detection in the turbulent solar wind and planetary space with various accumulated density. Whether the alpha species have the same kinetic impact on the turbulence with different participation ratios has not been fully addressed. In the present study, we investigate the kinetic effects of the alpha protons on the turbulence evolution by full kinetic particle-in-cell (PIC) simulations. Six run cases in total are performed with different proton-to-alpha density ratio. It is revealed that the anisotropy and the heating efficiency of both the protons and alpha particles are changed as the proportion of the alpha particle increases. The ion-alpha differential flow plays the essential part in the anisotropic heating, and its effect varies as the alpha particle density changes. These features are also distinguishable between the time of peak magnetic field energy and the time of later decaying. Our results are significant in building the fundamental of studying the astrophysical turbulence with complicate plasma composition.


ST14-A022
The Three-dimensional Reconstruction of Transients in the Outer Corona by the CORAR Technique Based on Multi-view Observations from STEREO

Shaoyu LYU+, Yuming WANG#, Xiaolei LI, Quanhao ZHANG
University of Science and Technology of China, China

Based on the simultaneous white-light observations of STEREO twin spacecraft, we proposed the CORrelation-Aided Reconstruction (CORAR) technique to locate and reconstruct the three-dimensional (3D) structures of solar wind transients in the interplanetary space. For the study of transients in the outer corona, we apply the CORAR method on synthetic and real images of COR-2 onboard STEREO. By comparing the reconstruction quality and precision of synthetic transient blobs under various conditions, we find that transients are generally reconstructed well when the separation angle between two spacecraft (θSun) is between 120 and 150, and the optimal θSun for reconstruction is close to 135. Based on the conclusion, we study the 3D reconstruction and evolution of real small-scale transients observed by COR-2 during Jan 2010 - May 2010. The valid transients are automatically detected according to the velocity uncertainty and image comparison. We confirm that the transients can be located and reconstructed well by comparing reconstructed structures with the corresponding transients fitted by the self-similar expanding model. The reconstructed transients generally have the typical acceleration characteristic of slow solar wind, which fits the trans-coronal radio observation and the previous researches of blobs. Most transients are located near the top of streamer belts, and can be traced into the boundaries of coronal holes or open-field regions on the photosphere. It supports the opinion that the slow solar wind originates from the interchange magnetic reconnection between open and closed field.


ST14-A031
Jet-flow Fluctuations and Plasma Blobs as a Mediator Between Interchange Mangetic Reconnection in Solar Corona and Alfvénic Velocity Spikes in Interplanetary Space

Chuanpeng HOU1+, Alexis ROUILLARD2#, Jiansen HE1, Bahaeddine GANNOUNI2, Victor REVILLE2
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

Solar Orbiter (SolO) detects many Alfvénic velocity spikes in the solar wind at solar distances of nearly 0.38 au. It remains inconclusive about these spikes' origin, properties, and impact on the background solar wind. Some of these Alfvénic spikes show decreasing radial magnetic field (Br) and nearly constant magnetic field strength (|B|), similar to the kink/switchbacks observed by Parker Solar Probe in the near-sun solar wind (<0.3au). Other spikes show reducing radial magnetic fields, decreasing magnetic field magnitude, and increasing density and temperature, presenting the characteristics of pressure-balanced structures. Using a two-step ballistic backmapping method, we trace the Alfvén velocity spikes observed by SolO back to the boundary of a coronal hole at low latitudes. We find that the number of bright points near the coronal hole boundary shows a periodic fluctuation, which period is comparable to the waiting time of velocity spike clusters. Among these coronal bright points, there occurs one typical interchange magnetic reconnection event, which is recorded by EUI aboard SolO and AIA aboard Solar Dynamics Observatory. With the imaging with high temporal and spatial resolution from multiple perspectives, we directly analyze the dynamic properties of plasma blobs and the fluctuating motion of jet flow materials. We compare these observational analysis results with a 2.5D MHD simulation of interchange magnetic reconnection. We speculate that plasma blobs and outward fluctuations may act as a kind of mediator between interchange magnetic reconnection and the formation process of velocity spikes/magnetic switchbacks.


ST14-A032
Generation of Flux Ropes in the Small-scale Interchange Magnetic Reconnection Process Observed by Solar Orbiter

Chuanpeng HOU1+, Alexis ROUILLARD2#, Jiansen HE1
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

Parker Solar Probe has detected abundant magnetic inversions and velocity spikes in the young solar wind, the origins of which are still highly debated. Numerous studies based on observational data and numerical simulations favor the causal correlation between the interchange magnetic reconnection process and these velocity spikes. However, the specific process by which interchange magnetic reconnection leads to these structures is still inconclusive. Some simulation works consider flux ropes, which they think may propagate into interplanetary space after generating from reconnecting current sheet, to be responsible directly for the observed magnetic inversions and velocity spikes. However, some other simulation works of interchange reconnection show that the flux ropes will reconnect with the post-reconnected open field lines and excite multi-wave modes. In this work, we show imagery observations of an interchange magnetic reconnection event and the motion of relevant flux ropes. Based on the high-resolution images (HRI) of Solar Orbiter/EUI, we analyze the dynamic process of flux ropes, the interaction between flux ropes and surrounding field lines, and the amplitude of wave modes near the cusp region of the interchange magnetic reconnection. Our analysis will provide an observational constraint on the numerical simulation of interchange magnetic reconnection and the interpretation of corresponding simulational results.


ST15-A005
A Comparative Study on the Polar Cap Hot Patch and Cold Patch by Using Multi-instrument Observations

Yu-Zhang MA1+, Qing-He ZHANG2#, Larry LYONS3, Kjellmar OKSAVIK4, Zanyang XING2, Marc HAIRSTON5, Balan NANAN2, Yong WANG2
1Shandong University, Weihai, China, 2Shandong University, China, 3University of California, Los Angeles, United States, 4University of Bergen, Norway, 5The University of Texas at Dallas, United States

Polar cap hot patch is a newly identified enhanced density structure which is associated with particle precipitation, ion upflow and flow shears. Based on combined observations from DMSP satellites, EISCAT radar, and all-sky imagers at the Chinese Yellow River Station, the different characteristics between hot patch and classical polar cap patch (cold patch) are investigated. Poleward moving auroral forms (PMAFs) and throat aurora are observed equatorward of both types of patches, which are located in narrow anti-sunward flow regions that are surrounded by sunward flow. Compare to the cold patch, the hot patch is closer to the cusp region and is associated with strong auroral emissions. Both hot and cold patches show enhanced F region density, but the hot patch is associated with higher electron temperature and enhanced E region electron density, which may due to the particle precipitation. We suggest that the hot patch and cold patch may represent different states of the same density structure, and the difference between them may be due to the decay of particle precipitation when patches move from cusp region to polar cap.


ST15-A012
A Statistical Study of Space Hurricanes in the Northern Hemisphere

Sheng LU1+, Zanyang XING1#, Qing-He ZHANG1, Yongliang ZHANG2, Yu-Zhang MA3, Xiang-Yu WANG1, Kjellmar OKSAVIK4, Larry LYONS5, Balan NANAN1, Jing LIU1, Yong WANG1, Zhong-Xin DENG6, Kai XIA1, Di SONG1
1Shandong University, China, 2Johns Hopkins University Applied Physics Laboratory, United States, 3Shandong University, Weihai, China, 4University of Bergen, Norway, 5University of California, Los Angeles, United States, 6China Research Institute of Radiowave Propagation, China

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 satellite from 2005 to 2016, we found that the space hurricane in the Northern Hemisphere occurs in summer and has a maximum occurrence rate in the afternoon sector around solar maximum. In particular, the space hurricanes are more likely to occur in the dayside polar cap at magnetic latitude greater than 80°, and their MLT (magnetic local time) dependence shows a positive relationship with the IMF (interplanetary magnetic field) clock angle. We also found the space hurricane occurs mainly under dominant positive IMF By and Bz and negative Bx conditions. It is suggested that the stable high-latitude lobe reconnection, which occurs under the conditions of large Earth’s dipole tilt angle and high ionosphere conductivity in summer, should be the formation mechanism of space hurricanes. The result will give a better understanding of the solar wind-magnetosphere-ionosphere coupling process under northward IMF conditions.


ST16-A003
Forward Modeling of Magnetic Field Measurements at the Bases of Stellar Coronae Through Extreme-ultraviolet Spectroscopy

Xianyu LIU1#+, Hui TIAN1, Yajie CHEN2, Wenxian LI3, Meng JIN4, Xianyong BAI3, Zihao YANG1
1Peking University, China, 2Max Planck Institute for Solar System Research, Germany, 3Chinese Academy of Sciences, China, 4Lockheed Martin Advanced Technology Laboratories, United States

Measurements of the stellar coronal magnetic field are of great importance in understanding the stellar magnetic activity, yet the measurements have been extremely difficult. Recent studies proposed a new method of magnetic field measurements based on the magnetic-field-induced-transition (MIT) of the Fe x ion. Here we construct a series of stellar coronal magnetohydrodynamics (MHD) models and synthesize several Fe x emission lines at extreme-ultraviolet wavelengths, and then diagnose the magnetic field strength at the bases of the coronae using the MIT technique. Our results show that the technique can be applied to some stars with magnetic fields more than three times higher than that of the Sun at solar maximum. Furthermore, we investigate the uncertainty of the derived magnetic field strength caused by photon counting error and find that a signal-noise ratio of ∼50 for the Fe x 175 ̊A line is required to achieve effective measurements of the stellar coronal magnetic field.


ST16-A004
Where and How Does a Decay-index Profile Become Saddle-like?

Runbin LUO+, Rui LIU#
University of Science and Technology of China, China

The decay index of solar magnetic fields is known as an important parameter in regulating solar eruptions from the standpoint of the torus instability. In particular, a saddle-like profile of decay index, which hosts a local torus-stable regime at higher altitudes than where the decay index first exceeds the instability threshold, is found to be associated with some confined or two-step eruptions. To understand the occurrence of such a profile, we employed dipoles to emulate different kinds of photospheric flux distributions. Corroborated by observations of representative active regions, our major results are as follows: (1) in bipolar configurations the critical height increases away from the AR center along the polarity inversion line (PIL) and its average is roughly half of the centroid distance between opposite polarities; (2) in quadrupolar configurations saddle-like profiles appear above the PIL when the two dipoles oriented in the same direction are significantly more separated in this direction than in the perpendicular direction, and when the two dipoles are oriented differently or have unequal fluxes; and (3) saddle-like profiles in quadrupolar configurations are associated with magnetic skeletons such as a null point or a hyperbolic flux tube, and the role of such profiles in eruptions is anticipated to be double-edged if magnetic reconnection is involved.


ST16-A009
Magnetic Field Extrapolation in Active Region Well Constrained by Observations in Multiple Layers

Fu YU1,2+, Jie ZHAO1#, Xiaoshuai ZHU1, Yang GUO3, Yang SU4, Jinhua SHEN5, Hui LI1
1Chinese Academy of Sciences, China, 2University of Science and Technology of China, China, 3Nanjing University, China, 4Purple Mountain Observatory, CAS, China, 5Xinjiang Astronomical Observatory, China

Magnetic field extrapolation is an important tool to reconstruct the 3D magnetic field above the solar photosphere. However, the prevalently used force-free field model might not be applicable in the lower atmosphere with non-negligible plasma beta, where the crucial process of flux rope formation and evolution could happen. In this work, we perform extrapolation in an active region, based on an recently developed magnetohydrostatic (MHS) method which takes plasma forces into account.
By comparing the results with those from the force-free field extrapolation methods, we find that the overall properties, which are characterized by the magnetic free energy and helicity, are roughly the same. The major differences lie in the magnetic configuration and the twist number of magnetic flux rope (MFR). Unlike previous works either obtained sheared arcades or one coherent flux rope, the MHS method derives two sets of MFR, which are highly twisted and slightly coupled. Specifically, the result in the present work is consecutively constrained by the high-resolution observations from the chromosphere, through the transition region to the corona, such as the filament fibrils, pre-eruptive braiding characteristics and the eruptive hot channel.
Overall, our work shows that the newly developed MHS method is more promising to reproduce the magnetic fine structures that can well match the observations at multiple layers, and future data-driven simulation based on such extrapolation will benefit in understanding the critical and precise dynamics of flux rope before eruption.


ST16-A011
The Causes of Homologous Eruptions from NOAA AR 11302 Through the Data-constrained MHD Simulation

Wentai FU#+, Yang GUO, Mingde DING, Ye QIU, Ze ZHONG
Nanjing University, China

In this work, we obtain the coronal magnetic configuration for this region using a NLFFF extrapolation based on the photospheric magnetogram at 12:00 UT. Taking it as the initial condition, we perform a data-constrained MHD simulation to study the evolution of the magnetic topology for this region. We reproduce two homologous eruptions through MHD simulation, including a successful eruption and a confined eruption. By analyzing the magnetic null point and three-dimensional quasi-separatrix layers, we divide the magnetic structures into three magnetic ropes and two spine-fan structures. The observed flare ribbons and flare loops correspond to these magnetic structures, which further explains the reliability of our simulation. We also analyze the Lorentz force and decay index of the two eruptions. We find that torus instability plays a role in driving the successful eruption. After the successful eruption, due to the occurrence of magnetic reconnection, the direction of medium magnetic flux rope overlying magnetic field configuration has changed. Therefore, the direction of Lorentz force change to be downward, which makes the second eruption be confined.


ST16-A022
Solar Cycle Variation in the Properties of Photospheric Magnetic Elements

Song ANCHUAN1#+, Yuming WANG1, Quanhao ZHANG1, Rui LIU1, Jie JIANG2, Xiaolei LI1
1University of Science and Technology of China, China, 2Beihang University, China

Photosheric convective motions, energy transports, and eruption phenomena on the Sun, are inextricably related to solar magnetic field. The solar surface is widely covered with Magnetic Elements (MEs). We investigate physical properties of these MEs by analyzing magnetograms from 2010 to 2021 observed by Helioseismic and Magnetic Imager (HMI) on board Solar Dynamics Observatory (SDO). Utilizing “clumping” algorithm to identify MEs, we show that the distribution of MEs parameters follow the two segments power-law separated as small-scale and large-scale MEs. MEs with small-scale parameters (magnetic flux less than 5.5∗10^18 Mx or area less than 5.5 ppm or magnetic energy per unit depth less than 5.5*10^14 J/m) have almost no correlation with solar cycle but MEs with large-scale parameters have strong correlation with solar cycle. Meanwhile, the magnetic field strength (maximal value of MEs) versus area of MEs fit well with radical function. The fitting slope has strong correlation with solar cycle on all flux-scale MEs and almost no correlation with solar cycle on small flux-scale MEs. These implies large-scale and small-scale MEs are generated by different physical mechanisms.


ST16-A025
A Study of Pre-flare Solar Coronal Magnetic Fields: Magnetic Energy and Helicity

Aiying DUAN1#+, Chaowei JIANG2, Xueshang FENG3
1Sun Yat-sen University, China, 2Harbin Institute of Technology, Shenzhen, China, 3Chinese Academy of Sciences, China

Solar flares fall into two types with eruptive ones associated with coronal mass ejection (CME) and confined ones without CME. To explore whether there are pre-flare conditions in terms of magnetic energy and helicity that can effectively determine the types of flares, here we analyzed a suite of related parameters of the reconstructed pre-flare coronal magnetic field of major solar flares, either eruptive or confined, from 2011 to 2017 near the solar disk center. The investigated parameters include the extensive-type quantities such as the total magnetic energy ET, the potential energy EP, the free energy EF, the relative helicity HR, and the non-potential helicity HJ, as well as the intensive-type indices EF/EP, |HJ/HR, |HR/phi'2| and |HJ/phi'2|, where phi' is half of the total unsigned magnetic flux. We have the following key findings: (1) None of the extensive parameters can effectively distinguish the eruptive and confined potential of the pre-flare coronal fields, though the confined events have averagely larger values; (2) All the intensive parameters have significantly larger average and median values for eruptive flares than the confined events, which indicates that the field for eruptive flares have overall higher degree of non-potentiality and complexity than that of the confined flares; (3) The energy ratio EF/EP and the normalized non-potential helicity |HJ/phi2|, which are strongly correlated with each other, have among the highest capability of distinguishing the fields that possibly produce a major eruptive or confined flare, as over 75\% of all the events are successfully discriminated between eruptive and confined flares by using critical values of EF/EP>=0.27 and |HJ/phi'2|>=0.009.


ST16-A026
Investigation Into the Stability of Magnetic Structure Producing Eruptive Flares in Solar Active Regions

Jihye KANG1#+, Satoshi INOUE2, Yong-Jae MOON3
1Kyung Hee University, Korea, South, 2New Jersey Institute of Technology, United States, 3School of Space Research, Kyung Hee University, Korea, South

We study a flare onset process in terms of stability of a three-dimensional (3D) magnetic field in several active regions, such as 12371, 11890, 12673, producing eruptive flares. In order to reveal the 3D magnetic structure, we first extrapolate the 3D coronal magnetic fields based on the photospheric vector magnetic fields under a nonlinear force-free field (NLFFF) approximation. The NLFFFs nicely reproduce the observed pre-eruptive magnetic configuration. Using the NLFFFs, we investigate the sheared arcade loops to explore the onset process of the eruptive flare using three representative magnetohydrodynamic(MHD) instabilities: the kink, torus, and double arc instabilities. Consequently, the NLFFFs are found to be quite stable against the kink and torus instabilities. We expect that the double arc instability is a key for understanding the onset process of the sheared arcade loops producing the eruptive flares. We also try to apply NLFFFs as the initial conditions to observation-based MHD models to reconstruct its process of the eruptive events.


ST16-A028
Twist and Writhe of the Eruptive Quiescent Filament on 2013 August 2

Yudi OU1#+, Yingna SU2
1Chinese Academy of Sciences, China, 2Purple Mountain Observatory, Chinese Academy of Sciences, China

Multi-wavelength observations of a filament eruption provide an opportunity to uncover the physical mechanism of the triggering and evolution process of the eruption. In this work, we investigate a quiescent filament that erupted on 2013 August 02, observed in H-alpha and EUV by SDO and GONG. At first, the eastern part of the filament starts to rotate in counterclockwise direction, then the western part of the filament shows clockwise rotation, finally the entire filament rises up and erupts. More interestingly, the filament shows two helical structures near its right footpoint during the eruption. We construct magnetic field models of this source region using the flux rope insertion method. The estimated twist number of the erupting flux rope based on the magnetic field model exceed the threshold value of kink instability, which suggests that kink instability might play a major role in the onset of the eruption. The critical height of torus instability increases from the eastern footpoint to the western footpoint of the filament, which may explain why the eruption begins at the eastern footpoint.


ST17-A008
Simultaneous Evolutions of Inner Magnetospheric Plasmaspheric Hiss and EMIC Waves Under the Influence of a Heliospheric Plasma Sheet

Nigang LIU#+
Sun Yat-sen University, China

Plasmaspheric hiss and electromagnetic ion cyclotron (EMIC) waves are two of the most important magnetospheric plasma waves inside the Earth's high-density plasmasphere. In this work, utilizing observations from the WIND and Van Allen Probes missions, we investigate the simultaneous evolutions of inner magnetospheric plasmaspheric hiss and EMIC waves under the influence of a heliospheric plasma sheet (HPS). The long duration impingement of high-density solar wind HPS onto the magnetosphere produced hot anisotropy electrons and protons, and then caused excitations of plasmaspheric hiss and EMIC waves in the duskside plasmasphere (L ∼ 6.75, MLT ∼ 16.85). In contrast, the solar wind decompression associated with the subsequent cessation of the HPS led to decreases in hot electron and proton fluxes, triggering prompt disappearances of the compression-related plasmaspheric hiss and EMIC waves. The presented results highlight the importance of solar wind conditions for the Earth's space weather and provide new insights into the solar wind-magnetosphere coupling.


ST17-A011
A Statistical Study of Superfast Precipitation of Energetic Electrons Observed by POES Satellites

Zheng XIANG#+, Deyu GUO, Binbin NI, Yangxizi LIU, Junhu DONG
Wuhan University, China

Energetic electron precipitation plays an important role in the magnetosphere-ionosphere-atmosphere coupling system, leading to chemical and electric effects in the upper atmosphere. Based on the quasi-linear theory, the population of trapped electrons is always larger than the precipitated ones. However, recent observations from ELFIN-A satellite found that precipitation electron fluxes can often exceed the trapped electron fluxes. This phenomenon is called superfast precipitation and is likely caused by nonlinear electron interactions with intense plasma waves. To comprehensively investigate the spatiotemporal features of the superfast precipitation phenomenon under different magnetic storm levels, we conduct a statistical study of superfast precipitation using long-term observations from POES satellites. The results show that superfast precipitation mostly occurs in the region L>7 with the largest occurrence rate of ~15% at nightside. These results can help to identify the wave mode driving the superfast precipitation.


ST18-A002
New Empirical Model of Radiation Belt Energetic Electrons

Qianyi MA#+, Linghua WANG, Qiugang ZONG, Zhiyang LIU, Yongfu WANG
Peking University, China

The energetic electrons magnetically trapped in the Earth’s radiation belt can pose severe hazards to spacecraft and astronauts. In order to improve the forecast of spatial and temporal distributions of energetic electrons in terrestrial radiation belt, we develop a new empirical model with seven parameters: the electron energy, magnetic local time (MLT), magnetic latitude, L-shell, time, solar wind velocity and AE index, using the 50-600 keV energetic electron measurements by the Image Electron Spectrometer (IES) on board a Chinese Navigation Beidou satellite in an inclined (55°) geosynchronous orbit from 2015 to 2020. First, we build up a quiet-time radiation belt model of energetic electrons, based on a statistical study of energetic electron spectra observed by BD/IES during geomagnetic quiet times (Ma et al., in preparation). Secondly, we extend this quiet-time model to an all-time model by introducing a magnification factor Q as a function of the electron energy, the AE index, and MLT, based on a statistical study of energetic electron spectra observed by BD/IES during geomagnetic active times. Compared with the popular NASA’s AE-8 model, the adjusted coefficient (that quantifies the model prediction accuracy) of our model is improved from 0.35 to 0.88. We will also compare the prediction accuracy of our model with some popular physics-based radiation belt environment models (e.g., RBE in the SWMF).


ST18-A004
Solar Wind with Magnetic Fields and Energetic Particles (SOFIE): A Physics-based Model to Predict the Solar Energetic Particles

Lulu ZHAO#+, Igor SOKOLOV
University of Michigan, United States

Radiation hazards caused by solar energetic particle (SEP) events are of great concern for space exploration. SEPs are suggested to be accelerated to high-energy either by magnetic reconnection-driven processes in solar flares or by shocks driven by coronal mass ejections. SEPs can be accelerated up to tens of GeV, and the flux of >10 MeV protons could exceed their background level by several orders of magnitude. Protons of >150 MeV are very difficult to shield, and the sparsity and large variation of the SEP events make them difficult to predict. We present a data-driven and self-consistent SEP forecast model, SOFIE, to simulate the acceleration and transport processes of energetic particles using the Space Weather Modeling Framework (SWMF). In this model, the background solar wind plasma in the solar corona and interplanetary space is modeled by the Alfven Wave Solar-atmosphere Model-Realtime driven by the near-real-time hourly updated GONG magnetogram. In the background solar wind, the coronal mass ejections are launched employing the Eruptive Event Generator using Gibson-Low configuration by inserting a flux rope estimated from the free magnetic energy in the active region. The acceleration and transport processes are then modeled self-consistently by the multiple magnetic field line tracker. We will demonstrate the capability of SOFIE to make now-cast and forecast of solar energetic particles.


ST18-A005
Research on the Effect of Data Assimilation for Three-dimensional MHD Simulation of Solar Wind

Fang SHEN1#+, Hanke ZHANG1, Yi YANG2
1Chinese Academy of Sciences, China, 2National Space Science Center, Chinese Academy of Sciences, China

As an important part of space weather forecasting, the prediction of solar wind parameters in the near-Earth space is particularly significant. The introduction of data assimilation (DA) method can improve the reliability of numerical prediction. In this study, we use a three-dimensional (3D) magnetohydrodynamics (MHD) numerical model with Kalman filter to infer the impact of the DA on solar wind modeling. We use the 3D MHD numerical model with near-Earth in situ observations from the OMNI database to reconstruct solar wind parameters between 21.5 solar radii and 1 AU. The period from 2018 to 2021 is simulated, when the solar activity in the decay of the 24th solar cycle to the rising of 25th solar cycle. The numerical model generates two separate results, one without DA and one with DA directly performed on the model-only results. Statistical analysis of observed, modeled and assimilated solar wind parameters at 1 AU reveals that assimilating simulations provide a more accurate forecast than the model-only results with a sharp reduction in the root mean square error and an increase of correlation coefficient.


ST18-A007
Automatic Recognition of Sunspot Based on Chinese Hα Solar Explorer

Huimin LI#+, Dalin YE, Lixin GUO
Xidian University, China

Sunspots are solar phenomena that occur in the solar sphere, and the overall situation of sunspots on the solar disk can reflect the level of solar activity. With the development and advancement of solar physics and observation technology, the automatic identification and feature extraction of sunspots has become a realistic requirement for studying solar activity. In this paper, the polynomial fitting method is used to remove the limb darkening effect from the CHASE images, and then threshold segmentation and mathematical morphology are combined for automatic identification of sunspots, and calculate the number and area of sunspots. In order to verify the accuracy of the method in this paper, the number and area of sunspots calculated from the CHASE were compared with the relevant parameters published by NOAA/SWPC. It was found that the calculation results had a good correlation with the SRS release. The results showed that for CHASE images, the method proposed in this paper could realize the automatic recognition of sunspots and obtain more accurate sunspot features, which is of great significance for the study of solar activity.


ST18-A009
Deep Learning Based Eruptive Flare Forecasting

Hemapriya RAJU#+, Saurabh DAS
Indian Institute of Technology Indore, India

Solar eruptions such as CMEs, flares disrupt geomagnetic and communication systems on Earth. While flares are abrupt, bright events that occur in the solar atmosphere and emit massive amounts of energy in the 10^28 to 10^32 erg range, CMEs are intense eruptions that hurl plasma into interplanetary space. CMEs can be found in conjunction with flares, filaments, or independent. Although both flares and CMEs are understood as triggered by a common physical process magnetic reconnection, yet, the degree of association is unknown. In this work, we study the time series of magnetogram data derived from SHARP (Space weather HMI Active Region Patches) to understand eruptive flare mechanism using Machine Learning models SVM,LDA and Deep learning model LSTM. Here, we use 18 SHARP parameters as input to our Machine Learning model from the year 2011-2021. The task here is to perform binary classification, hence two classes, predicting whether a flare will be accompanied by CMEs or not. We initially attempt to study the features at different time lags that will be more responsible for eruptive flare. For example, MEANSHR shows deviated mean between two classes at 48h time lag, while MEANGBZ shows it at 8-24h time lag before the event occurence. Therefore, we determine the appropriate time lag for each feature using our Deep Learning model LSTM, coupled with ML models SVM and LDA, to perform binary classification. We further attempt to study the model’s predictions and behaviour using Explainable ML methods such as variable-importance measure and shapley.


ST18-A014
The Equivalent Indices of Geomagnetically Induce Currents in Local Power Grid

Jin LIU#+
Yunnan University, China

The geomagnetic induced currents (GICs) generated in power grid by large-scale solar events may lead to electrical equipment damage and widespread power outages. So it is important to achieve effective GIC prediction and risk assessment for local grid. The Hilbert-Huang Transform (HHT) method is used to analyze the geomagnetic component and the GIC monitoring data. By extracting the GIC responses to storms, the equivalent disturbance indices is synthesized by instantaneous amplitude. In addition, the GIC potential risk of local power grid is evaluated comprehensively by considering the solar wind energy injection, dual-band geomagnetic disturbance and the GIC surge.


ST18-A015
Relationship of the Largest GIC During Geomagnetic Storms with Solar Wind-IMF Parameters

Balan NANAN1#+, Wen-Bin LI1, Ruth SKOUG2, Zanyang XING1, Manu VARGHESE1, Li-Kai LIANG1, Qing-He ZHANG1
1Shandong University, China, 2Los Alamos National Laboratory, United States

The association of GIC (geomagnetically induced current) with various solar and geophysical conditions has been known. However, what determines the time of occurrence and amplitude of the largest GIC during geomagnetic storms, which during extreme storms can cause sudden damage of vulnerable utility systems, is not yet known. We address this important question by analyzing the GIC data measured in Finland for 21 years (1999-2019) during 106 geomagnetic activities (DstMin ≤-50 nT) at low, mid and high latitudes and the corresponding solar wind velocity V, dynamic pressure P and north-south component of interplanetary magnetic field (IMF Bz) measured using the ACE satellite, and the products VBz and PBz. The results show for the first time that the largest GIC (≥10 A) occurs at the time of the largest -(VBz) in all seasons and solar activity levels with its time determined by the time of the largest -Bz and magnitude determined by both V and -Bz, except in one case. The two power outages happened in the 21-year period (06 November 2001 and 30 October 2003) also occurred at the UT time of the largest GICmax. The correlation of largest GICmax is highest (0.92) with the largest -(VBz) at September equinox. The results highlight the importance of (1) measuring the solar wind velocity at the L1 point at high time resolution even under extreme space weather conditions, which with the existing instrument in the ACE satellite is not possible, (2) single station GIC measurements, and (3) the possibility of improving the forecasting of the rate of change of the local horizontal geomagnetic field (dH/dt) directly related to GIC.


ST18-A016
Double Superposed Epoch Analysis of Geomagnetic Storms and Corresponding Solar Wind and IMF in Solar Cycles 23 and 24

Manu VARGHESE#+, Balan NANAN, Qing-He ZHANG, Zanyang XING
Shandong University, China

The weakest solar cycle 24 (SC24, 2010-2019) in 100 years was 1/3rd less active compared to the previous solar cycle 23 (SC23, 1996-2009). We identify 135 and 61 ICME (interplanetary coronal mass ejection) driven clear geomagnetic storms (DstMin ≤-50 nT) in SC23 and SC24, respectively, giving a reduction of 55% storms in SC24, and present the double superposed epoch analysis (DSEA) of the storms/activities in SC23 and SC24 using the Dst, SymH, Kp and AE indices. The DSEA method for the corresponding solar wind velocity V, north-south component of the interplanetary magnetic field (IMF Bz) and the product VBz are also presented. Compared to SC23, the maximum storm/activity intensity in SC24 reduces by 52%, 12% and 45% at low, mid and high latitudes and the corresponding maxima in -VBz, V and -Bz reduce by 39%, 17% and 38%, respectively. The epoch average storm/activity intensity reduces by 27%, 11% and 4% at low, mid and high latitudes and average maxima in -VBz, V and -Bz reduce by 24%, 14% and 13%, respectively. The results seem to reveal that the average reduction in the main driver -VBz (~24%) might have caused nearly the same and equal average storm/activity intensity reductions in all latitudes (~25%), though the irregular nature of the AE index makes the reduction very small (4%) at high latitudes, and small (~11%) at mid latitudes mainly due to the small (0-9) quasi logarithmic scale of the Kp index.


ST18-A017
Spectral Analysis of Geomagnetically Induced Current and Local Magnetic Field During the 17 March 2013 Geomagnetic Storm

Zanyang XING#+, Wen-Hao XU, Balan NANAN, Li-Kai LIANG, Yan-Ling WANG, Qing-He ZHANG, Zi-Dan SUN, Wen-Bin LI
Shandong University, China

Geomagnetically induced current (GIC) is known to be closely related to the rate of change of local horizontal magnetic field (dBx/dt); and their spectra can give better insight into the relationship. We study the spectral characteristics of GIC measured in Finland and dBx/dt measured 30 km away during the 17 March 2013 intense geomagnetic storm (SymHMin = 132 nT). Two bursts of large GIC (up to 32A) and dBx/dt occurred at 16 UT and 18 UT during the storm main phase. For the first time, the cross wavelet transform (XWT) and wavelet coherence (WTC) techniques are used to investigate the correlation and phase relationship of GIC and dBx/dt in time-frequency domain. Their WTC correlation is strong (over 0.9) over the entire storm period, indicating dBx/dt is the main factor causing GIC. Their XWT spectra show two enclosed periods (8–42 min and 2–42 min) in the high energy region corresponding to the two bursts of activity in GIC and dBx/dt. Morever, we use continuous wavelet transform (CWT) and discrete wavelet transform (DWT) to analyze the spectral characteristics of GIC and dBx/dt. It is found that the CWT and DWT spectra of the two are very similar, especially in the low frequency characteristics, without continuous periodicity. Wavelet coefficients become large when GIC and dBx/dT are large; and the third-order coefficient, which corresponds to low-frequency part, best reflects the disturbance of GIC and dBx/dt.


ST18-A020
Global Model Output and Variable Reliability in Solar Wind Input

Ramon LOPEZ#+, Espen FREDRICK
The University of Texas at Arlington, United States

Global models of the geospace system use solar wind data as the outer boundary conditions of the simulations. The data are generally provided by the OMNI dataset, which takes observations in the solar wind (typically collected at the L1 Lagrange point), and ballistically propagates them to the bow shock. However, the actual solar wind conditions at Earth may at times be poorly correlated with the OMNI data. In this study we take two periods of OMNI data, one where the correlation between the OMNI data and data taken just outside the bow shock is good, and a period where the correlation is bad. The two time series for each period (the OMNI data and the near Earth solar wind data) are used to drive a global model and we compare the results to both observations to and to each other. This comparison will allow us to begin to quantify the range of potential error in the global model output as a function of solar wind input reliability, which is an important consideration for space weather prediction.


ST19-A003
Developing a New Technique to Identify Foreshocks

Yu HUAIZHONG#+, Zeping LI
China Earthquake Networks Center, China

On average, more than 100 earthquakes of magnitude 6.0 and above occur in the world annually, of which about 15% have foreshocks. The existence of foreshocks may provide an opportunity for the prediction of the upcoming larger mainshocks. Unfortunately, the method to identify foreshocks has not been found yet. The detection of the potential of a larger event immediately after a moderate earthquake is still unresolved. In this work, we devised an approach to determine whether an earthquake is a foreshock to a larger mainshock by evaluating loading/unloading states. This is done by calculating the Coulomb fracture stress (CFS) change induced by earth tides along the tectonically preferred slip direction on the seismogenic fault surface of each of the candidates. The technique is based on the load/unload response ratio (LURR) method, but it can decide, not assume, the slip direction of CFS. Using the approach, we tested the Ms > 4.0 foreshocks of the Ms > 6.0 earthquakes on the Chinese mainland since 2000 and the earthquake swarms, where no subsequent larger mainshocks were expected, in the past 10 years. The former mostly occurred in the loading process, while the latter arose more frequently in a random process. The statistical results indicate that the occurrence of earthquakes during loading may imply the critical state of the seismogenic faults, and the derived stress is more likely to trigger a larger event than that of the earthquakes that occurred during unloading. This work has been supported by the Earthquake Joint Funds of NSFC (Grant No. U2039205) and the National Key Research and Development Project (Grant No. 2018YFE0109700).


ST19-A007
Estimations of the Number of Chinese Annual Seismic Hazard Region Based on R-score and Statistical Models

Zhengyi YUAN#+, Yu HUAIZHONG
China Earthquake Networks Center, China

Some tentative studies are carried out on the number of Chinese annual seismic hazard region, aiming at giving the best estimation of which from the statistical point of view, and giving some reference to the practice of Chinese annual earthquake prediction. Firstly, formula for estimating the above number is derived by using R-score. Meanwhile, the traditional clustering algorithm is improved to identify the earthquake cluster areas that meet certain distance requirements. On this basis, the numbers of annual earthquakes above target magnitudes, earthquake cluster areas and isolated earthquakes in Mainland China during 1950 to 2019 are counted respectively. Finally, a variety of statistical models are fitted to determine the reasonable upper limit of the seismic hazard region number. Then results show that the estimation values obtained from the two statistical results are slightly different. The first value based on the annual incidence of earthquakes above MS5.5 in western (west of 108°E) and MS6.0 in eastern (east of 108°E) of Mainland China is 9, which is suitable for the prediction of earthquakes with slightly higher magnitudes, while the second one based on the cluster areas identification results of annual earthquakes above MS5.0 in Mainland China is 13, which is consistent with the number used by the China earthquake networks center at present, and has good application effect for determining annual earthquakes above MS5.0.This work has been supported by the National Key Research and Development Project of China (Grant No. 2018YFE0109700) and the Earthquake Joint Funds of NSFC (Grant No. U2039205).


ST19-A011
Spatiotemporal Evolutions of Large Earthquake Sequences in Tianshan Mountain Fault

Cheng CHANG#+, Chi-Chia TANG
China University of Geosciences, China

The foreshocks and aftershocks of large earthquakes provide valuable information for studying earthquake nucleation, fault rupture processes, and postseismic deformation. The Tianshan Mountain fault is a typical ongoing lithospheric deformation in an intracontinental setting. It formed during the accretion of the Altaids in the Paleozoic and was rejuvenated in the Cenozoic, and this might be a far-field response to the India-Asia collision. Tianshan Mountain fault is one of the most intense seismic areas in mainland China. In the past 20 years, there have been 13 earthquakes of Mw>5. To clarify evolutions of large earthquake sequences, we focused on the four large earthquakes with Mw>5.5 in the Tianshan region and used the matched filter technique to detect missing microearthquakes one month before and after the mainshocks. The newly detected events are at least three times more than that listed in the China Earthquake Networks Center catalog. The four large earthquakes have no foreshock sequence but have an Omori’s type decay with a logarithmic slope p~1. We found that aftershocks following Jinghe Mw6.3 earthquake migrated toward the west side while other aftershock sequences showed no evident migration. Geological structures around the mainshock hypocenters may affect the migration patterns of the aftershocks. Based on these phenomena, we attempt to describe the spatiotemporal evolution process and seismic properties of the mainshocks.


ST19-A013
Seasonal Variations of Parkinson Vectors

Zhiqiang MAO1+, Chieh-Hung CHEN1#, Aisa YISIMAYILI2
1China University of Geosciences, China, 2Earthquake Agency of Xinjiang Uygur Autonomous Region, China

Parkinson vector (or induction vector) is an effective indicator to investigate the underlying conductivity structures and pre-earthquake conductivity anomalies. Typically, the factors influencing Parkinson vectors (PVs) come from underground. Recently, the seasonal effects have been observed in the PVs. However, causal mechanisms of the seasonal effects on the PVs are not fully understood. In this study, we utilize ten years three-component geomagnetic data from 24 stations operated by the Geomagnetic Network of China to study the spatiotemporal characteristics of the PVs through vertical transfer function (VTFs). The analytical results show that the PVs exhibit seasonal variations that the magnitude of PVs reach maximum in summer and winter, which are pronounced in lower frequency bands. In addition, the PVs at all stations consistently exhibit a counterclockwise rotation in June (summer), and a clockwise rotation in December (winter). The Inter-hemispheric field-aligned current in the ionosphere is one of the potential reasons to explain the seasonal variations. This study finds that the PVs are also affected by ionospheric current systems. As a result, the seasonal effect on PVs should be examined when we study the pre-earthquake conductivity anomalies.


ST19-A014
Promising Anomalous Phenomena of Residing Waves Before Earthquakes

Chieh-Hung CHEN1#+, Yang-Yi SUN1, Xuemin ZHANG2, Kai LIN1
1China University of Geosciences, China, 2China Earthquake Administration, China

The instrumental array was established in Leshan, Sichuan, China for monitoring vibrations and perturbations in the lithosphere, atmosphere and ionosphere (MVP-LAI). Ground vibrations from the broadband seismometers, air pressure from the barometers, the magnetic field from the magnetometer, and total electron content from the ground-based Global Navigation Satellite System receivers retrieved from the MVP-LAI system share frequencies exceeding ~1 month before major earthquakes. Those geophysical parameters distributed from the Earth’s surface to the altitude of ~350 km suggest the existence of the LAI coupling before earthquakes. Meanwhile, the frequencies varies from low (~10-4 Hz) to high (~10-2 Hz or higher) with the approaching of the forthcoming earthquakes. The variable frequencies further suggest that seismo-waves reside in wide areas well covering the epicenters. The residing waves would be a promising candidate for predicting earthquakes.


ST20-A004
Results of the Wave Measurements by the WHU VLF Wave Detection System at the Chinese Great Wall Station in Antarctica

Xudong GU1#+, Binbin NI1, Wei XU1, Shiwei WANG1, Zejun HU2
1Wuhan University, China, 2Polar Research Institute of China, China

A Very Low Frequency (VLF) wave detection system has been designed at Wuhan University (WHU) and recently deployed by the Polar Research Institute of China at the Chinese Great Wall station (GWS, 62.22°S, 58.96°W) in Antarctica. With a dynamic range of ~110 dB and timing accuracy of ~100 ns, this detection system can provide observational data with a resolution to facilitate space physics and space weather studies. Located southwest and ~370 km from the Palmer station, the GWS site complements and provides new data for VLF wave studies using the Palmer station data. This paper presents the first results of the wave measurements by the WHU VLF wave detection system at GWS to verify the system's performance. With a three-month routine operation, the system can acquire the dynamic changes of the wave amplitudes and phases of various ground-based VLF transmitter signals emitted in North America and Europe. A preliminary analysis indicates that the properties of the VLF transmitter signals observed by the GWS wave detection system during the X-class solar flare events are consistent with previous studies. As the HWU-GWS path crosses the South Atlantic Anomaly (SAA) region, the observations also imply a good connection in space and time between the VLF wave disturbances and the lower ionosphere variation potentially caused by magnetospheric electron precipitation during the geomagnetic storm period. It is therefore well expected that the acquisition of VLF wave data at GWS, in combination with datasets from other instruments, can be beneficial for space weather studies related to the radiation belt dynamics, terrestrial lightning discharge, whistler wave propagation, and the lower ionosphere disturbance, etc., in the polar region.


ST20-A007
Statistical Analysis of Magnetosonic Waves in Plasmaspheric Plumes

Yun-Gi HAN+, Kyungchan KIM#
Chungbuk National University, Korea, South

Magnetosonic waves, also known as equatorial noise, are whistler-mode emissions distributed near the Earth’s magnetic equator between the proton cyclotron frequency and the lower hybrid resonance frequency. So far, much effort has been devoted to improving our understanding of their origin and characteristics inside and outside the plasmasphere, owing to their potential role in scattering energetic electrons and protons. In contrast, their characteristics in plasmaspheric plumes have not been reported yet. In this study, we, for the first time, statistically investigate magnetosonic waves in the plasmaspheric plumes based on the entire mission period (the year 2012-2019) of Van Allen Probes A and B. Statistical results show that magnetosonic waves are observed in plumes with an occurrence rate of ~10-20% depending on geomagnetic activity. Their amplitude and wave normal angle are distributed with an average of ~40 pT and 84o-88o, respectively. Increased geomagnetic activity enhances the amplitude and the ratio of plasma frequency to electron cyclotron frequency. In addition, approximately 80% of all selected magnetosonic wave events are observed simultaneously with the plasmaspheric hiss, which is known to be most effective in scattering electrons in the plume.


ST20-A010
Frequency Chirping of Chorus Subpackets in the Upstream and Downstream Regions

Huayue CHEN1#+, Xueyi WANG1, Lunjin CHEN2, Yoshiharu OMURA3
1Auburn University, United States, 2The University of Texas at Dallas, United States, 3Kyoto University, Japan

Chorus waves are electromagnetic emissions that are commonly detected in the Earth’s inner magnetosphere, which play a significant role in regulating electron dynamics, including the acceleration of electrons to ~MeV energies, and the precipitation of ~10 keV electrons into the ionosphere. These waves are believed to be excited in the upstream of the equator, with an amplitude enhancement in the downstream. The spectrum of chorus waves typically contains a series of discrete elements with an upward frequency chirping, known as rising-tone elements. In general, a chorus element is composed of several “subpackets” (or “subelements”), with a duration of about 5-10 ms. However, how the frequency chirps in the subpackets is still an open question. With a one-dimensional (1D) general curvilinear particle-in-cell (gcPIC) simulation in the dipole field at L=4, we investigate the frequency chirping of chorus subpackets. We find that the frequencies of subpackets have a comparable chirping rate with that of the entire chorus element in the upstream, but keep almost constant in the downstream. The mechanism of this kind of chirping has been further studied. Our study provides a fresh perspective on the theory of frequency chirping in chorus waves.


ST20-A017
Statistics of the Wave Normal Angle Distribution of Two-band Plasmaspheric Hiss

Junhu DONG+, Zheng XIANG#, Binbin NI
Wuhan University, China

The unique banded structure of plasmaspheric hiss has been recently reported by Ni et al (2023). Such banded hiss waves exhibit characteristically both an upper band above ~ 200 Hz and a lower band below ~150 Hz, with a gap in power in between. Using ~7-year datasets from Van Allen Probes, we establish a robust database of banded hiss events and investigate statistically the global wave normal angle (WNA) distribution for each band, along with which the statistical features of the wave amplitude for each band are also considered. Our results show that WNA of lower band hiss is smaller than that of upper band hiss, which suggests distinct generation mechanisms of two bands. Based on parameterization as functions L-shell, magnetic local time (MLT), magnetic latitude (MLAT) and geomagnetic (AE*) index, we also construct the empirical models of the wave amplitude and power-weighted wave normal angle of two-band plasmaspheric hiss, the results of which are further verified via data-model comparisons to show good performance.


ST20-A021
A Forecast Model of the Dst and AE Indices from Solar Wind Parameters Observed at the L-1 Point Based on Machine Learning Method

Hanyu HUANG1+, Zhengyang ZOU1#, Wentao ZHOU2
1Zhuhai MUST Science and Technology Research Institute, China, 2Macau University of Science and Technology, Macau

The Earth's magnetosphere is highly sensitive to the geomagnetic storms and substorms induced by kinds of interplanetary disturbances, such as CME and CIR events. Knowing the variations of the geomagnetic indices driven by solar winds could be an easy access to investigate magnetospheric physics. We present a machine learning approach to forecast Dst and AE indices based on the time series of more than 10 solar wind parameters observed on the L-1 point. The forecast result can well rebuild DST and AE evolutions during both geomagnetic and quiet times.


ST21-A001
Phase Space Density Hole/hill Formation by Whistler-mode Chorus in a Multi-component Plasma

Kyungguk MIN#+
Chungnam National University, Korea, South

Whistler-mode chorus waves in the inner magnetosphere are excited by a process involving phase trapping of energetic electrons in a dipole magnetic field. The critical element that gives rise to strong nonlinear wave growth is the formation of phase space density (PSD) hole which is asymmetric in gyro-phase space as a result of positive frequency chirping of chorus elements and the spatial gradient of the Earth’s magnetic field. Previous studies mainly assumed a two-component electron plasma where a cold dominant population provides a medium for wave propagation and a tenuous, anisotropic bi-Maxwellian or loss-cone distribution provides a necessary condition to form a PSD hole. On the other hand, earlier studies hinted that depending on the initial temperature anisotropy, either a PSD hole or hill can be formed. Then, a situation can arise where the presence of a relatively isotropic distribution can produce a PSD hill that counteracts the PSD hole produced by the anisotropic energetic bi-Maxwellian population, thereby reducing the nonlinear growth rate. In this paper, we expand the idea of the earlier studies and quantitatively show that phase-trapped particles by a rising tone element closely follow single wave characteristics. This indicates that the formation of PSD hole or hill is strongly related to the anisotropy of an initial distribution function. We suggest that the detailed structure in a realistic electron distribution far from an ideal single bi-Maxwellian can be important for chorus wave evolution.


ST21-A003
Revealing the Relationship Between Transpolar Arc Occurrence and Solar Wind Conditions Using the Novel Neural Network (Potential Learning): Initial Results

Motoharu NOWADA1#+, Ryozo KITAJIMA2, Ryotaro KAMIMURA3, Quanqi SHI1
1Shandong University, China, 2Tokyo Polytechnic University, Japan, 3Tokai University, Japan

Transpolar arcs (TPAs) are one of the interesting auroral phenomena that the bar-shaped emissions are growing from the poleward edge of the nightside main auroral oval to the dayside, occurred under northward and non-zero interplanetary magnetic field (IMF) conditions. Based on a novel machine learning algorithm: Potential Learning (PL), we reveal the relationship between high TPA occurrence rate and solar wind conditions, extracting the most significant solar wind parameter(s), closely related with the TPA appearance, from large databases of the OMNI solar wind and auroral image data from 1996 to 2005. PL is a neural network technique that can extract the most relevant parameter(s) to the output parameter among the input parameters. In this study, we set up the six solar wind parameters, such as the IMF-By and northward Bz components, solar wind velocity, number density, dynamic pressure, and solar wind energy coupling function, which is described with a formula proposed by Newell et al. (2007), as the PL input parameters. The output parameter of PL is the TPA presence/absence, represented with 1 or 0. Under these setup conditions, we examine the most significant solar wind parameter(s) when the output shows “1”. In this stage, we test the algorithm to evaluate the PL performance and confirm that the TPA appearance can be predicted with ~ 69.5% accuracy from input solar wind parameters. We will present the initial results on more detailed relationship between TPA occurrence and solar wind parameters, based on PL.

Reference:
Newell, P. T., Sotirelis, T., Liou, K., Meng, C.-I., and Rich, F. J. (2007), A nearly universal solar wind-magnetosphere coupling function inferred from 10 magnetospheric state variables, J. Geophys. Res., 112, A01206, doi:10.1029/2006JA012015.


ST21-A007
Layered Structure of Current Density Near Magnetic Equatorial Plane in the Inner Magnetosphere: Multi-spacecraft Observation

Xin TAN1, Malcolm DUNLOP1,2#+, Junying YANG1, Yanyan YANG3, Xiangcheng DONG4, Yingshuai DU1, Chris RUSSELL5
1Beihang University, China, 2Rutherford Appleton Laboratory, United Kingdom, 3China Earthquake Administration, China, 4Yunnan University, China, 5University of California, Los Angeles, United States

The Earth’s ring current forms a complex current system at the boundary of the inner magnetosphere. It is highly dynamic because of the interaction between the solar wind with the Earth's magnetosphere (the influence of space weather), while its morphology depends on the nature of the magnetospheric-ionospheric (M-I) coupling, generating field-aligned currents (FACs). Its behaviour can therefore have a huge impact on the terrestrial environment. According to Ampere's law, these currents can be directly measured by perturbations in the magnetic field using multi-spacecraft observation techniques. We have analyzed the magnetic field data from the four MMS spacecraft in their small-sale configuration to obtain the in-situ current density and have carried out statistical analysis from several years of data. The form of the current density distribution and its changing nature has been investigated. Our results show that the current density exhibits a three-dimensional layered structure in the ring current region. The significant westward current on the day side flows to higher magnetic latitudes and complete closure there rather than to the magnetic equator. There are some differences between geomagnetic quiet period and storm period on current density, but the basic spatial structure remains similar and compares well with previous space mission data. Comparison with Swarm data at low Earth altitudes, we found that the stratification is consistent with the distribution of the R2 field-aligned currents seen both adjacent to the ring current and at ionospheric altitudes (at Swarm). In addition, significant continuous eastward currents exist in some latitudes and some regions, indicating the complexity of the ring current. Some of them can be explained by the formation of banana currents.


ST21-A008
Solar Abundance Fractionation in an Active Region Related to the Existence of the Alfvén Wave in the Chromosphere

Kyoung-Sun LEE#+, Jongchul CHAE
Seoul National University, Korea, South

The elemental abundance in the solar corona is different from the photosphere. The fractionation between photospheric and coronal abundances is related to the “First Ionization Potential (FIP) effect.” In the corona, the low FIP (FIP < 10 eV) elements are enhanced by factors of 3–4 relative to the photospheric abundances. In contrast, the high FIP elemental abundance ratio to photospheric is approximately equal. Still, it is not revealed how the solar abundance is fractionated. Recently, the most probable model is “Abundance fractionation by the Pondermotive force”. The pondermotive force induced by the Alfvén wave preferentially affects the ionized elements (low FIP element), not the neutral in the chromospheric plasma, which is partially ionized. Then, the force drags up (or down) the low FIP elements depending on the Alfvén wave existence and their energy density in the chromosphere. For investigating the relations between the abundance fractionation and wave energy density in the chromosphere, we analyze the H alpha and Ca II data from GST/FISS for the Alfvén wave detection and Si X (low FIP element) and S X (high FIP element) spectra from Hinode/EIS for determining the relative abundance in an active region. We present the preliminary result of detecting Alfvén waves in the chromosphere compared to the spatial distribution of the abundance fractionation.


ST21-A017
Statistical Study of Mid- and Low-latitude Electric Field Response Corresponding to the CW Structure That Develops During Substorms

Moe HAYASHI1#+, Akimasa YOSHIKAWA1, Akiko FUJIMOTO2, Shin OHTANI3
1Kyushu University, Japan, 2Kyushu Institute of Technology, Japan, 3Johns Hopkins University Applied Physics Laboratory, United States

The purpose of this study is to comprehensively understand the evolution of global 3D current system from polar to equatorial ionosphere during substorms. There are two types of current systems in the polar ionosphere: the R1-current linked to the magnetospheric convection system, and the R2-current linked to the pressure gradient in the inner magnetosphere [Iijima and Potemra, 1976, 1978]. In addition to these currents, when substorms are occurred by strong plasma injections, current wedge (CW) is generated by the plasma vorticities at the edge of the plasma flow. They have the same current polarities as the R1-current system. Magnetic field generated by CW development are significant in the nightside mid- and low-latitude, and these variations was modeled by McPherron et al. [1973]. We capture the spatio-temporal development of CW during substorm by using MAGDAS and SuperMag magnetic field data. By comparing them with the electric field (E-field) from the FM-CW radar in Paratunka, Russia, we are analyzing the electromagnetic dynamic responses in the mid- and low-latitude. We performed a comparative analysis of ionospheric electric and geomagnetic fields for 50 of the 1790 isolated substorms from 09/21/2006 to 12/31/2010, in which the E-field changed significantly with onset. The results show that the amplitude of E-field is correlated with auroral electrojets (AEJ). Furthermore, the direction of E-field reflects E-field caused by the Hall polarization effect due to the ionospheric current induced by CW (simulated by Yoshikawa et al. [2013]), based on classification of the relative positions of the CW and observation points from mid-latitude geomagnetic data. However, similar analyses of the other 1,740 cases showed that these models alone could not explain the results. In this presentation, we report the results of our interpretation of E-field variations by comparing Kp and solar wind conditions in addition to substorm indices.


ST21-A019
SSUSI Aurora Forecast Model

Syau-Yun HSIEH#+, Yongliang ZHANG, Robert SCHAEFER, Larry PAXTON
Johns Hopkins University Applied Physics Laboratory, United States

The SSUSI Aurora Forecast Model has been developed and used to predict the global auroral quantities using the remote-sensing ultraviolet measurements from DMSP/SSUSI instruments. This model predicts the equatorward boundary of auroral oval and precipitating the electron energy flux and mean energy estimated based on the empirical GUVI global model for up to 1 day or 15 DMSP orbits in advance. We will present the current implementation, capability, validation and forecast results of this model and discuss the current/future development. Particle precipitation in the auroral oval serves as an important connection between the magnetosphere and ionosphere/atmosphere. Particle precipitation, an important source of energy for the high-latitude upper atmosphere, not only creates extra ionization in the high-latitude ionosphere which leads to absorption and disturbances in radio communication but also enhances the Joule heating by creating the Hall and Pedersen conductivity which alters the thermospheric convection and composition and further causes the global ionospheric disturbances. If we can accurately characterize the auroral region energy inputs and conductivity, we will have a better capability for nowcasting and forecasting the ionospheric conditions in the high latitude region for space weather.


ST21-A022
Radial Variations of the Heliospheric Current Sheet Tilt Angle During Solar Minimum Years: Magnetohydrodynamic Simulations

Chin-Chun WU1#+, Kan LIOU2
1Naval research laboratory, United States, 2Johns Hopkins University Applied Physics Laboratory, United States

Here we present results from a study of dynamic effects on the tilt angle (peak latitude) of the heliospheric current sheet (HCS) as a function of the heliospheric radial distance from ~0.08 to 15 AU using our time-dependent, three-dimensional, global magnetohydrodynamic (MHD) simulation model, G3DMHD. Specifically, we simulate solar wind during solar quiet years (1994-1995) to minimize effects from coronal mass ejections. We use the two years worth of photospheric magnetic field measurements from Mountain Wilson Observatory to drive the MHD model continuously and uninterruptedly. The locations of the HCS at different radial distances are derived from our simulation results and are compared with the tilt angle of the neutral line inferred from the potential field model at 2.5 Rs. Our results reveal a large peak in tilt angles in the northern hemisphere within 2 AU, suggesting steepening of the HCS. After 2 AU, the tilt angle reduces (e.g., flattening of the HCS) with the radial distance. In the southern hemisphere the trend mirrors those found in the northern hemisphere, forming near symmetric (about the equator) variations. We will present the results in detail and discuss possible causes of the HCS steepening and flattening.


ST21-A024
Extension of the Electron Density Enhancement from Middle to High Latitudes Observed by Swarm-A in Summer of the Southern Hemisphere

Jin WANG1#+, Yang-Yi SUN2, Tao YU2
1China University of Geosciences (Wuhan), China, 2China University of Geosciences, China

The major causal mechanism for the eastward movement of the electron density (Ne) enhancement associated with the southern Midlatitude Summer Nighttime Anomaly (MSNA) was attributed to the field-aligned thermospheric neutral wind at the middle geomagnetic latitude in the fixed local time coordinate. In the study, the Ne and horizontal cross-track ion drifts observed by the Swarm-A satellite at 462 km altitude show that the horizontal drifts can drive the Ne enhancement of the southern MSNA in the local summer of the Southern Hemisphere. Both the eastward and westward ion drifts transport the enhancement from the middle to the high geomagnetic latitudes, which results in the enhancement evolving at all the longitudes in the whole day.


ST21-A026
Two Distinct Brightness Distributions of Microwave Loop During an M-class Flare

Sujin KIM1#+, Jeongwoo LEE2, Satoshi MASUDA3
1Korea Astronomy and Space Science Institute, Korea, South, 2New Jersey Institute of Technology, United States, 3Nagoya University, Japan

We have studied the solar flare, SOL2013-10-28T02:01 (GOES class M9.1), with a sequence of microwave brightness maps obtained with the Nobeyama Radioheliograph (NoRH) at 17 GHz and 34 GHz. Hard X-ray maps from the Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI) and the extreme ultraviolet (EUV) images from the Atmospheric Imaging Assembly (AIA) onboard the Solar Dynamics Observatory (SDO) were also studied for the context. For the total six peaks of the bursts are counted in the microwave fluxes, the dominant microwave source appears to be dynamically changing its position within a simple loop oriented north-south near the limb. During the first three microwave flux peaks, the microwave source appears in the south while the X-ray source lies in the northern end of the loop. During the other three peaks, the opposite trend appears that the microwave source at the time of the peaks appears in the northern end while the X-ray source lies in the southern end of the loop. At the times between the peaks, the microwave intensity in the north substantially decreases while in the south, it changes little. Based on the results, we discuss the physical difference and the cause of two distinct brightness distribution of the microwave flare loop.


ST21-A030
An EUV Jet Driven by a Series of Transition Region Micro-jets

Hengyuan WEI1#+, Zhenghua HUANG1, Hui FU1, Ming XIONG2, Lidong XIA1, Zhang CHAO1, Deng KAIWEN1, Li HAIYI1
1Shandong University, China, 2National Space Science Center, China

Jets are one of the most common eruptive events in the solar atmosphere, and are believed to be important in the context of coronal heating and solar wind acceleration. We present an observational study on a sequence of jets with the data obtained from SDO and IRIS. This event includes an EUV jet, about 29 arcsec long with a dome-like base, a bundle of transition region (TR) flux ropes, and a series of transition region microjets. The bundle of flux ropes rises as a response to the TR microjets, with the rising motion eventually triggering the EUV jet. We propose a scenario involving a set of magnetic reconnections, in which the series of TR microjets are associated with the processes to remove the constraints to the TR flux ropes and thus allow them to rise and trigger the EUV jet. Our study demonstrates that small-scale dynamics in the lower solar atmosphere could be complex and are crucial in understanding the energy and mass connection between the corona and the lower solar atmosphere, even though many of them might not pump mass and energy to the corona directly.


ST21-A032
Automatic Recognition of Coronal Mass Ejection

Dalin YE#+, Huimin LI, Lixin GUO
Xidian University, China

Coronal Mass Ejection (CME) is a large-scale and the intense eruptive phenomenon, and also the main driving source of disastrous space weather, which is related to many phenomena such as flares, solar energetic particles, and geomagnetic storms. With the development and advancement of solar physics and observation technology, manual identification of CME can no longer efficiently process the rapidly increasing solar observation data, and automatic identification and feature extraction of CME has become a realistic requirement for studying solar activity. In this paper, the SOHO/LASCO C2 white-light images are preprocessed by running difference, threshold segmentation, and polar coordinate transformation, and then projected to obtain the intensity profile of the 1D projection along the angular and radial direction. Finally, the parameters of the central position angle, angular width, and speed of the CME are obtained by threshold segmentation and linear fitting. In order to verify the accuracy of the method in this paper, the central position angle, angular width, and speed calculated from 50 CME events in 2003 are compared with the corresponding parameters in the CDAW catalog, and it is found that the accuracy of CME feature extraction is 0.79. The results show that for SOHO/LASCO images, the method in this paper can realize the automatic identification of CMEs and obtain a more accurate description of the features, which is of great significance for the study of solar activity.


ST21-A033
Self-organized Criticality Characteristics and Statistical Studies of Flare Ribbons

Yue ZHANG+, Rui LIU#
University of Science and Technology of China, China

Each brightening distributed on the solar flare ribbons may be a small explosive reconnection event, and the single complex dynamic process can be regarded as a single avalanche. The UV (1600 and 1700) filter channel data of the Atmospheric Imaging Assembly (AIA) carried on the Solar Dynamics Observatory (SDO) are used to observe flare ribbons. We use morphological methods to deal with image data, thus flare ribbons can be extracted by setting a reasonable threshold and made as binary graphs convenient for the further statistical processing. It is expected that the duration, peak intensity, magnetic field, and dimming of the flare ribbon can be well described by power-law distribution functions. We explore the frequency distribution of each brightening’s physical parameters, and the distribution can be approximated with a power-law function. We find that the power-law index (i.e., the slope of the linear fitting part in the log-log graph, marked as index=average ± standard deviation) is insensitive to the threshold of flare ribbons identification (for Duration: αT=-1.5426±0.0050, for Peak intensity: αP=-1.4736±0.0561, for Line-of-sight magnetic field: αBz )=-1.4212±0.0132), which means these indices change little when the threshold changes. Since the idea of self-organized criticality (SOC) has been embodied in many natural phenomena, we attempt to explore the SOC characteristics within solar flare ribbons. And these results obtained can be explained as evidence of the existence of SOC in flare ribbons. In the future, we expect that there are also corresponding power-law relationships between different parameters, and deal with flares with other shapes or magnitudes to compare the characteristics of power-law presented by different flare ribbons.


ST22-A006
Correlation Study of the Variation in the Topside Ionosphere and F-region Along the Magnetic Field Line

Yen-Jung WU#+, Thomas IMMEL, Brian HARDING, Colin TRIPLETT, L. Claire GASQUE
University of California, Berkeley, United States

NASA's Ionospheric Connection Explorer (ICON) was launched in 2019 to investigate the interaction between the neutral atmosphere and the ionosphere. At altitudes in the F-region and below, ICON reports on various ionospheric quantities such as O+ profile, NmF2, and HmF2, as well as neutral wind, temperature, and disk O/N2. The Ion Drift Meter (IVM) on ICON, at an altitude of approximately 600 km, provides in-situ plasma measurements of the topside ionosphere. This study examines the relationship between daytime topside ion density and other ICON measurements on different time scales. The results show that disk O/N2 has the highest correlation with a value of 0.46 in the annual time scale. When the data is grouped by noontime equatorial crossings with a 14-day window size, the topside ion density has strong correlations with HmF2 and IVM's meridional drift, with mean correlations of 0.60 and 0.51, respectively. Furthermore, in the equatorial crossing groups, HmF2 has a significant positive correlation with NmF2 and field-aligned drift, while significant negative correlations are found with ion density and meridional drift. This exercise provides valuable information for developing a machine learning model that can estimate topside ion density and ion drift using measurements from lower altitudes.


ST22-A008
New Findings of Earth Ionosphere from Three Year Observations of FORMOSAT7-COSMIC2

Charles LIN1#+, P. K. RAJESH1, Jia-Ting LIN1, Chi-Yen LIN2, Shih-Ping CHEN1, Cheng -Yung HUANG3
1National Cheng Kung University, Taiwan, 2National Central University, Taiwan, 3National Space Organization, Taiwan

FORMOSAT7-COSMIC2 Mission consists 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 very important to understand the ionosphere further.


ST23-A005
MHD Modeling of CMEs - Recconstructing Remote and In-situ Observations

Nishtha SACHDEVA#, Zhenguang HUANG+, Gabor TOTH, Ward MANCHESTER, Bart VAN DER HOLST, Aniket JIVANI, Hongfan CHEN
University of Michigan, United States

Successful modeling of solar transients like Coronal Mass Ejections (CMEs) is an important step towards accurately forecasting their space weather impact. It is therefore crucial to improve the models and tools to reconstruct CMEs by validating simulations with observations of the solar corona and the inner heliosphere at various heliospheric distances with multi-viewpoint observations. The Space Weather Modeling Framework (SWMF) includes MHD modeling of the solar wind and CMEs from the Sun to the Earth and beyond. The Alfven Wave Solar atmosphere Model (AWSoM) is a 3D extended-MHD solar corona model within SWMF that reproduces the solar wind background into which CMEs can propagate. The Eruptive Event Generator (EEG) module within SWMF is used to obtain flux-rope parameters to model realistic CMEs within AWSoM using different flux-rope configurations. In this work supported by the NSF SWQU and LRAC programs, we use an ensemble of solar wind backgrounds to obtain the best solar wind plasma environments into which CMEs can be launched. We vary the flux-rope parameters within a fixed range to do an ensemble of CME simulations to match the model reconstructed results with remote coronagraph observations near the Sun (LASCO C2/C3 and STEREO COR1/COR2) as well as with in-situ observations of solar wind plasma at 1 au. The ensemble modeling is a step forward towards improving the accuracy of the tools that provide flux-rope parameter estimates as well as the uncertainty quantification of CME modeling.


ST23-A007
The Dynamics of Turbulent Cascade Inside and Around ICME Propagating from the Sun

Maria RIAZANTSEVA1#+, Liudmila RAKHMANOVA1, Igor VOLODIN 2, Timofey TREVES 1, Alexander KHOKHLACHEV 1, Yuri YERMOLAEV1, Georgy ZASTENKER3
1Space Research Institute of the Russian Academy of Sciences, Russian Federation, 2HSE University, Russian Federation, 3Russian Academy of Sciences, Russian Federation

The study is devoted to the dynamics of the turbulent cascade inside and around ICMEs based on multipoint measurements of Wind, Spektr-R, Themis at the Earth orbit and Parker Solar Probe or Solar Orbiter closer to the Sun. Both case study and statistical analysis of turbulent properties in different positions in the heliosphere are performed. The ICMEs are selected with the help of the catalog of large-scale structures http://iki.rssi.ru/pub/omni/catalog/. Only data intervals with the best temporal resolution are used, which makes it possible to estimate the dynamics of the turbulent cascade on the ion-kinetic scales. As a rule, fast measurements are available only for interplanetary magnetic field. However, high-resolution plasma measurements on Spektr-R are also used for comparison with other spacecraft and for the statistical analysis. Comparison of magnetic field magnitude and ion flux fluctuations is possible as fluctuations of both quantities represent compressive fluctuations. Results reveal that typically fluctuation spectra have shape similar to the predictions of turbulence models in the undisturbed solar wind before ICME, become steeper at the kinetic scales in the Sheath region before of the ICME and tend to restore to the initial shape inside the ICME. It was shown also that the shape of the turbulent cascade can conserved both at the MHD and at the kinetic scales from the Sun to the Earth, while the fluctuation power decreases when moving away from the Sun. Plasma structures responsible for the steepening of the spectra at the kinetic scales and the enhancement of dissipation in the Sheath region are discussed. The work is supported by Russian Science Foundation grant № 22-12-00227.


ST23-A009
Helium Abundance Behavior in the ICMEs During Solar Activity Decrease in 23-24 Solar Cycles

Alexander KHOKHLACHEV 1#+, Yuri YERMOLAEV1, Irina LODKINA2, Maria RIAZANTSEVA1, Liudmila RAKHMANOVA1
1Space Research Institute of the Russian Academy of Sciences, Russian Federation, 2Russian Academy of Sciences, Russian Federation

The ICMEs are statistically characterized by the increase of average values of the relative abundance of doubly ionized helium ions. In this study we investigate the changing of the behavior of the helium abundance inside the ICMEs during the significant decrease in solar activity in 23-24 solar cycles. The change in solar activity observed in 23-24 solar cycles is widely discussed in recent years. One of the effects of activity decline is a decrease in the average values of the plasma and interplanetary magnetic field parameters, including the helium abundance (Yermolaev et al., JGR, 2021). Based on the hourly average data from the OMNI database, we consider changes in the helium abundance vs other solar wind parameters in two epoch of different solar activity. These epochs cover two periods - 21 and 22 solar cycles, when solar activity was high, and 23-24 cycles, when solar activity decreased significantly. In addition to the interplanetary magnetic field and solar wind plasma parameters, we analyzed the distance between the observation point and the ICME axis. The results of the statistical analysis show that the relative helium abundance increases in the ICME central region in comparison to the peripheral. This dependence is observed in both epochs of solar activities. An increase in the helium abundance near the center of the ICME confirms the hypothesis about the existence of a helium-enriched electric current near the ICME axis, suggested in the paper (Yermolaev et al., JGR, 2020). The dependences of the helium abundance on the magnetic field magnitude and the plasma beta parameter, which was shown at previous stage (Khokhlachev et al., Cosmic Research, 2022) and also confirm the above hypothesis, tend to conserve during the change of epochs. The work is supported by Russian Science Foundation grant № 22-12-00227.


ST24-A003
Clarification of Atmospheric Tidal Modes Appearing in Ionospheric Currents by Independent Component Analysis

Kumi TAKAYAMA#+, Akimasa YOSHIKAWA, Yasunobu MIYOSHI
Kyushu University, Japan

Daytime ionospheric currents are complexly superimposed the Sq-EEJ current system induced by solar radiation and currents excited by various modes of atmospheric waves. Therefore, no method has yet been established to separate each phenomenon from the observed data. In this study, we used Independent Component Analysis (ICA), which separates and extracts independent components from multivariate signals, to extract variations due to atmospheric waves from ground magnetic field data of the MAGnetic Data Acquisition System/Circum-pan Pacific Magnetometer Network (MAGDAS/CPMN) on magnetically quiet days for 1992-2004. As a first step, we reduce the dimension of the data with Principal Component Analysis (PCA) to remove noise. Since [Gurubaran, 2002] suggests that the first principal component is the Sq-EEJ current system and atmospheric tidal variations appear in the addition of the 2nd through 5th principal components. Therefore, we applied ICA to the 2nd through 5th principal components as four variables. Also, we visualize the horizontal current structure from each independent component as equivalent current. In addition, we reproduce each atmospheric tidal mode influenced on the ionospheric currents with an atmosphere-ionosphere coupled model (GAIA) and compare with the current structure of each independent component to discuss which mode has a strong influence on the ionospheric current.


ST24-A007
Ionospheric Disturbances During and After the Annular Solar Eclipse on 21 June 2020 Due to the Convergence Effects

Xiaoyin LI1+, Jin WANG2, Tao YU1#
1China University of Geosciences, China, 2China University of Geosciences (Wuhan), China

An annular solar eclipse passed through the East Asia at low latitudes on 21 June 2020, which provides us an opportunity to study the eclipse-induced ionospheric disturbances at low latitudes. In this study, we analyze the observations of the ionosondes at Wuhan (30.4°N, 114.4°E, 82.4% obscuration), Xiamen (24.2°N, 118.07°E, 97.8% obscuration), and Nanning (22.7°N, 109.25°E, 81.1% obscuration), as well as the total electron content (TEC) data from the Global Navigation Satellite System (GNSS) of the Global Ionosphere Maps (GIMs) to examine the ionospheric behaviors in the F-region on 21 June 2020 solar eclipse day. The observations show that a TEC enhancement occurred after the major depression near the center path of obscuration, along with the occurrence of the TEC depletions both in the northern and southern sides. The TEC enhancement lasts to midnight on the solar eclipse day. The independent in-situ electron density (Ne) observation from the Swarm-B satellite and the slant TEC profile from the radio occultation technique of COSMIC-2 also observed the long-lasting enhancement in the F2 region near midnight. The solar eclipse-induced convergence effects can result in the long-lasting ionospheric perturbations, which may further cause the spread-F in the nighttime.


ST24-A008
Assimilated Ionosphere - Thermosphere Coupled Model for Lower and Equatorial Latitudes

I-Te LEE1,2#+, Jyun-Ying HUANG3, Mark CHENG3
1Central Weather Adminstration, Taiwan, 2National Central University, Taiwan, 3Central Weather Bureau, Taiwan

The Space Weather Operational Office (SWOO) of the Central Weather Bureau (CWB) in Taiwan response for providing space weather information and forecasts daily and locally. Due to the geolocation of Taiwan, higher plasma density during the day time period overhead are recorded associated with the equatorial ionization anomaly, and to observe plasma bubbles/irregularities in the evening to midnight period. Those phenomena significantly influence high-frequency and satellite communication as well as navigation and positioning services. Thus, in order to provide a useful and reliable forecast of ionosphere locally, a data assimilated ionosphere and thermosphere coupled model is operated by SWOO since 2018. The coupled model is the NCAR TIE-GCM, and the assimilated data includes total electron content derived by global ground-based GNSS receivers and electron density profiles measured by the FORMOSAT-7/COSMIC-2 radio occultation (RO). The assimilation system is routinely updated hourly, and then forecasts the condition of the ionosphere and thermosphere for the next six hours. The evaluation of assimilated results with ionosonde observations shows the correlation coefficient of foF2 is about 0.85, particularly yielding a better performance at the latitudinal region between 40° and -40°. On the other hand, the results further show an additional improvement of peak density by assimilated F7/C2 RO electron density profiles. Furthermore, the assimilated results also indicate the daily density maximum occurred earlier than control run at lower latitudes and thus lead to more studies. These assimilated dataset are archived by SWOO from 2019 till now, it could be used to conduct more study for lower and equatorial ionosphere and thermosphere.


ST24-A009
Variability of Equatorial Plasma Bubble Occurrence Rate from OI 135.6nm GOLD Observations

Deepak KARAN1#+, Richard EASTES1, Carlos MARTINIS2, Robert DANIELL3, Quan GAN1, Wenbin WANG4, William MCCLINTOCK1
1University of Colorado Boulder, United States, 2Boston University, United States, 3Ionospheric Physics, United States, 4National Center for Atmospheric Research, United States

Equatorial Plasma Bubbles (EPBs) are the manifestations of post sunset plasma irregularities that are associated with the depleted plasma densities that occur over the equatorial- and low latitudes. The seeding, development, and persistence of the plasma irregularities depend on many factors, including the alignment of the dusk terminator with the magnetic field lines, thermospheric winds, waves, electric fields, etc. These factors change with day-to-day, seasons and solar flux conditions, producing variabilities in the EPB occurrence rate. Further, the varying nature of these factors at different longitude sectors creates longitudinal variability in the EPB occurrence rate. OI 135.6 nm emission images from the NASA GOLD (Global‐scale Observations of the Limb and Disk) imager detect EPBs ~1-1.5hrs after sunset over the South America, Atlantic, and West African longitude sectors. In this work, we use the GOLD data to investigate the day-to-day, seasonal and longitudinal variations of EPBs occurrence rates and their solar activity dependence over these three longitude sectors from 2019 to 2021 during the equinoxes and solstices. Over the South American and Atlantic longitude sectors, the EPB occurrence rate was around ~95% in December solstices. The occurrence rate over the West African longitude sector in the same month was ~10%. Results suggest that (i) the March equinox is more favorable than the September equinox for EPBs occurrence during low solar activity period, (ii) EPBs occurrence increases from September to December in all three years, (iii) EPB occurrence increases with increasing solar activity from 2019 to 2021 at all the longitude sectors, and (iv) a prominent quasi 6-day periodicity is observed in the EPBs daily occurrence rate over the South America longitude sector. The day-to-day, seasonal, and longitudinal variations of EPBs occurrence rates and their solar activity dependence will be discussed in this work.


ST25-A002
Role of Q2DW-Tide-GW Interactions at SH Mid-latitudes in Interhemispheric Coupling

Zishun QIAO1#+, Alan LIU1, Nicholas PEDATELLA2, Gunter STOBER3, Iain REID4,5
1Embry-Riddle Aeronautical University, United States, 2National Center for Atmospheric Research, United States, 3University of Bern, Switzerland, 4ATRAD Pty. Ltd., Australia, 5University of Adelaide, Australia

Most theoretical investigations into the mechanism of interhemispheric coupling (IHC) have previously focused on the modulation of mesospheric meridional circulation driven by forcing of GWs originating in the troposphere and recently on the role of quasi-two-day waves (Q2DW) and GWs in-situ generated in the middle atmosphere. This study utilizes paired meteor radar observations (CONDOR, 31.2ºS,70.0ºW and Buckland Park Meteor Radar, 34.6ºS,138.4ºW) and SD-WACCM-X simulations to provide observational confirmation on the role of Q2DW and GWs at summer hemisphere mid-latitudes to IHC mechanisms. Specifically, Q2DW-tide interactions as well as their child waves are investigated during the 2021 NH SSW. The connection between Q2DW-tide-GW interactions and IHC mechanism during the 2021 NH SSW will be presented.


ST25-A003
Latitude Dependence of Ionospheric F2 Layer Plasma Drift Characteristics

Blessy VARGHESE1#+, Tiju JOSEPH MATHEW2
1Christian College Chengannur, University of Kerala, India, 2Christian College, India

The comparison of Ionospheric F2 layer plasma drift characteristics at different latitudes is presented in this work. The zonal and vertical plasma drift velocities were obtained over an equatorial station, Boa Vista (2.8° N; 60.7° W) and a mid-latitude station, Eglin (30.5° N; 86.5° W) using a Digital Ionosonde. Quiet days (Kp < 5) during one year from November 2013 to October 2014 are selected for analysis of seasonal behaviour. Some interesting systematic and regular features with strong seasonal dependence are observed during sunrise and sunset. The latitude dependence of these features is analyzed. Resultant plasma drift vectors in the zonal-vertical plane for these stations are obtained, perhaps for the first time using simultaneous observations of the zonal and vertical plasma drift components.


ST25-A006
Simultaneous Observations of Thermospheric Na Layers at Two Nearby Midlatitude Lidar Stations

Fang WU+, GuoTao YANG#, Jing JIAO
Chinese Academy of Sciences, China

The metal layers in the Earth’s upper atmosphere have received growing attention in recent years because of the discovery of the Thermosphere-Ionosphere metal (TIMt) Layers by lidar. In the reports of lidar detection TIMt Layers, the highest metal atom layer is Thermosphere-Ionosphere Na (TINa) Layers observed at Yanqing station (40.42°N, 116.02°E), while the Ca+ Ions Transport From ∼80 to 300 km. In 2014, another Na lidar was developed at Pingquan station(41.0°N, 118.7°E), which is about 250 km away from Yanqing station. Simultaneous detection of metal atoms and metal ions by resonance fluorescence lidars and an all-solid-state lidar at that two nearby midlatitude stations. We divide thermospheric Na layers (defined here as 110-200km) observed in two stations into four types, including lower thermosphere sporadic Na layers, dawn thermosphere-ionosphere Na layers, midnight thermosphere-ionosphere Na layers and mid-latitude thermosphere-ionosphere Na layers (Mid-TINa), depending on their occurrence, temporal evolution, other characteristics, and referring to the previous reports. Moreover, there are rare reports of the small-scale horizontal distributions of TINa layers. According to the observation results of Na, Ni, Ca and Ca+ inos, it suggested that Mid-TINa is not neutralized from the Es layer, which may be triggered by other possible formation mechanisms.


ST25-A009
Three-dimensional Ionospheric Plasma Properties of Space Hurricane

Sheng LU1+, Zanyang XING1#, Qing-He ZHANG1, Yongliang ZHANG2, Kjellmar OKSAVIK3, Larry LYONS4, Yu-Zhang MA5, Xiang-Yu WANG1, Balan NANAN1, Yong WANG1, Zhong-Xin DENG6
1Shandong University, China, 2Johns Hopkins University Applied Physics Laboratory, United States, 3University of Bergen, Norway, 4University of California, Los Angeles, United States, 5Shandong University, Weihai, China, 6China Research Institute of Radiowave Propagation, China

We report a space hurricane event in the Northern Hemisphere observed by multiple instruments. Based on the convective velocity observations from ground-based radars and ionospheric satellites, we confirm that space hurricane rotates clockwise at the altitude of the ionosphere and can modulate the ionospheric convection pattern in polar cap. From plasma in-situ measurement of incoherent scattering radar, we firstly obtain the 3D plasma properties of space hurricane including: (1) strong flow shears, (2) ion temperature enhancements caused by Joule heating, (3) electron density precipitation, (4) multiple ion temperature enhancements corresponding to sunward velocity one by one, which is considered to be caused by spiral arms. These results complete the picture of space hurricane at the altitude of ionosphere and give a better understanding of the magnetosphere-ionosphere coupling process in polar cap.


ST25-A011
Chinese and Russian Atmospheric Electric Field Joint Observation Along a Meridian Chain

Lei LI#+
National Space Science Center, China

There are three main sources which influence the atmospheric ionization: solar activities, meteorological activities (vapor, wind, ice, precipitation, cloud and lightning) and geological activities. Since the variation of atmospheric electric field is characterized by local and global effects, atmospheric electric field observations at different latitudes are more comprehensive and meaningful. China and Russia have 42 observation stations at different latitudes (20°N~70°N). Based on the different latitudinal observed data from a same meridian chain stations in both Russia and China, the researchers can compare and study: (1) The processes that solar activities such as solar flare, SEP (solar energetic particle), CME (corona mass eject), CME with -magnetic cloud influence the atmospheric electric field. (2) Meteorological activities that influence the atmospheric electric field. (3) The physical processes how geological activities influence local atmospheric electric field.


Thu-03 Aug | 8:15 - 10:00 | MR333
ST16 - Solar Magnetic Fields: Measurements, Extrapolations And (R)MHD Simulations

Session Chair(s): Xiaoshuai ZHU, National Space Science Center, Chinese Academy of Sciences

ST16-A027 | Invited
Magnetic Structure and Eruption of Complex Magnetic System

Yingna SU#+
Purple Mountain Observatory, Chinese Academy of Sciences

The latest high-resolution observations show that more and more solar eruptions occur in complex magnetic systems, such as double and multiple filament systems, double hot channel systems, as well as filament and hot channel systems. In this talk, I will present our recent progress in multi-wavelength observations and magnetic field modeling, as well as data-constrained MHD simulation of these complex magnetic systems. We focus on the magnetic configuration of these systems, the evolution of observed brightenings and photospheric magnetic fields, twist and writhe of observed filament and hot channels during the eruption, and so on. Such questions as how the eruptions are initiated, why two filament eruptions in similar photospheric magnetic configurations lead to opposite results, and how are the erupting structures formed have been addressed.


ST16-A021 | Invited
A Magnetic Reconnection Model for the Hot Explosion with Both Ultraviolet and Halpha Wing Emissions

Lei NI#+, Cheng GUANCHONG
Chinese Academy of Sciences

Ultraviolet (UV) bursts and Ellerman bombs (EBs) are two kinds of small transient brightening events that occur in the low solar atmosphere. Observations show that about 20% of the hot UV bursts connect with the much colder EBs, and their formation mechanisms are still not clear, challenging our understanding of magnetic reconnection and heating mechanisms in the partially ionized lower solar atmosphere. In this talk, we will present our high resolution RMHD simulations about magnetic reconnection in the partially ionized and highly stratificated low solar atmosphere. The more realistic radiative cooling model for the photosphere and chromosphere, and the time dependent ionization degrees were included in the MHD simulations. We also used the radiative transfer code RH1.5 D to synthesize the Si IV and Hα spectral line profiles based on the MHD simulation results. Magnetic reconnection between the emerged and the background magnetic fields leads to the formation of a thin curved current sheet at beginning, then the plasmoid instability starts to occur. The temperature in the current sheet is always below 8,000 K before t=269s. Later, the current sheet becomes more vertical and the dense plasmas are drained by gravity, the plasmoid instability results in the nonuniform distributions of plasma density in the reconnection region at the same time. The hot plasmas above 20,000 K start to appear in the regions with a relatively lower plasma density. When the line of sight passes through the turbulent reconnection region, the synthesized Si IV emission intensity can reach above 10erg s−1 sr-1 cm−2 A−1 and the width of the Si IV spectral line profile can be wider than 100 km s−1, which are consistent with observations of the UV burst. The synthesized Hα spectral line profile through this region also show the similar characteristics for a typical EB.


ST16-A024
In Detail About the Regression of Sunspot Groups

Judit MURAKOZY#+
Institute of Earth Physics and Space Science

The emergence and decay of the sunspot groups are driven by different mechanisms. In this presentation, only the decay phase will be studied on a large sample, based on the SOHO/MDI-Debrecen Sunspot Database (SDD). The SDD allows us to distinguish the sunspots with different magnetic polarities, thus the leading and following parts of the groups can be investigated separately. Altogether more than 140 sunspot groups were selected and checked as real decaying groups, which have clear maxima on the solar disk, and their umbral area decay is observable for at least four days. Results for the decay properties of sunspot groups will be presented, such as their rates depending on the maximum area, and these are in descending order: following penumbrae, following umbrae, leading penumbrae, leading umbrae. Their long-term cyclical and hemispherical variations will also be investigated on more than 750 sunspot groups by using the Debrecen Photoheliographic Data (DPD) and the revised version of the Greenwich Photoheliographic Results (GPR).
The research leading to these results has received funding from National Research, Development and Innovation Office -- NKFIH, 141895.


Thu-03 Aug | 8:15 - 10:00 | MR334
ST20 - Advances in Understanding Radiation Belt Dynamics: Theory, Observation and Simulation

Session Chair(s): Qianli MA, University of California, Los Angeles

ST20-A009 | Invited
Long-term Variations of Relativistic Electrons of the Outer Belt, Plasma Sheet Electrons and Plasmasphere

Yoshizumi MIYOSHI1#+, Satoshi KURITA2, Ryuho KATAOKA3, Shinji SAITO4, Shun IMAJO2, Tomoaki HORI1, Chae-Woo JUN1, Inchun PARK1, Mariko TERAMOTO5, Takefumi MITANI6, Iku SHINOHARA6, Takeshi TAKASHIMA6, Nana HIGASHIO6, Satoshi KASAHARA7, Shoichiro YOKOTA8, Kunihiro KEIKA7, Kazushi ASAMURA6, Ayako MATSUOKA2, Fuminori TSUCHIYA9, Atsushi KUMAMOTO9, Shoya MATSUDA10, Yoshiya KASAHARA10, Yoichi KAZAMA11, Shiang-Yu WANG11, Sunny W. Y. TAM12
1Nagoya University, 2Kyoto University, 3National Institute of Polar Research, 4National Institute of Information and Communications, 5Kyushu Institute of Technology, 6Japan Aerospace Exploration Agency, 7The University of Tokyo, 8Osaka University, 9Tohoku University, 10Kanazawa University, 11Academia Sinica, 12National Cheng Kung University

The Arase satellite has observed the inner magnetosphere since 2017 and has provided continuous data on plasma/particles, as well as fields/waves, covering the declining phase of cycle 24 and the early rising phase of cycle 25. During several magnetic storms, glowing peaks in the phase space density were observed during the recovery phase, suggesting a local acceleration process contributing to the significant flux enhancement of outer belt electrons. The location of the glowing peaks in the phase space density was found to be dependent on both the plasmapause and the inner edge of the plasma sheet electrons. We also observed temporal variations in the electron energy spectrum outside the plasmapause. During the main phase of the storm, the energy spectrum became softer, with an increase in tens of keV to multi-hundred keV electron flux and a decrease in MeV electron flux at L=4-6. Tens of keV electrons are believed to contribute to the source populations of whistler mode chorus waves, while multi-hundred keV electrons contribute to the seed populations of outer belt electrons. During the late main phase to the early recovery phase of the storm, the energy spectrum became harder, with a gradual increase in MeV electrons and a decrease in multi-hundred keV electron flux, suggesting the presence of a local acceleration process inside the outer belt. To understand the electron acceleration process, we conducted a computer simulation focused on the impact of ambient plasma density on electron acceleration. The simulation results indicated that significant electron acceleration occurred outside the plasmapause. Results of this study is consistent with cross-energy coupling driven by wave-particle interactions, in which acceleration by whistler mode waves is dependent on the ratio of plasma frequency to cyclotron frequency and the populations of source electrons for wave generation.


ST20-A003
Competition Between Source and Loss Processes of Radiation Belt Source, Seed, and Relativistic Electrons Induced by A Magnetic Cloud Event

Zhengyang ZOU1#+, Pingbing ZUO2, Binbin NI3, Jiayun WEI2, Wentao ZHOU4, Hanyu HUANG1
1Zhuhai MUST Science and Technology Research Institute, 2Harbin Institute of Technology, Shenzhen, 3Wuhan University, 4Macau University of Science and Technology

We study the competition between source and loss processes of radiation belt source (~10 keV), seed (~100 keV), and relativistic (> 1 MeV) electrons during a typical magnetic cloud event on 19-20 July 2016 that triggered a moderate geomagnetic storm. Across the interplanetary (IP) shock, the relativistic electrons experienced a “one-kick” energization at lower L-shells while having a moderate dropout at higher L-shells. The dropout continued enhancing during the storm main phase. However, the seed electrons had a light decrease after the shock and recovered to the pre-event level in the main phase, while source electrons continued increasing during the whole event time. Further analysis demonstrates that the loss processes (e.g., magnetopause shadowing connected with ULF-induce outward transport) were competing with the source processes (e.g., shock-induced energization for relativistic electron, substorm ejections as well as accelerations via wave-particle interactions), which are strongly sensitive to electron energy and L-shells. By quantitatively comparing the PSD change in (Energy vs. L*) space during different stages of the storm, we find that L*= ~ 4 and Ek = 102 – 102.5 keV could be typical values that the source and the loss processes arrived in the dynamic equilibrium. By tracing the temporal evolutions of source, seed, and relativistic electrons in response to a magnetic cloud event, the present study gives quantitative and comprehensive insight into the competition between source and loss mechanisms for radiation belt electrons, which would be valuable to further investigations in magnetic cloud-radiation belt coupling.


ST20-A012
Prompt Enhancements of Radiation Belt Electrons Over a Wide Energy Range Based on Phase Space Density Variations: A Detailed Case Study

Xiaoyu WANG+, Xing CAO#, Xudong GU, Binbin NI
Wuhan University

Based on Van Allen Probes observations, we report a prompt enhancement event of radiation belt electrons over a wide energy range from tens of keV to multiple MeV spanning January 13 - 15, 2013. During this period, we also observe prolonged moderate substorm activities and intense whistler-mode chorus emissions. To differentiate the underlying mechanisms responsible for this prompt electron enhancement process, we investigate in details the evolution of electron phase space densities (PSDs) for various values of the first and second adiabatic invariants (μ and K). The results show that tens to hundreds of keV electrons rapidly penetrated to L* < 4 during the substrom period, with the corresponding PSDs increasing by more than three orders of magnitude within about one day. Comparatively, the PSD enhancements of higher energy electrons are less significant and shift to higher L*. We find that the fast acceleration of hundreds of keV seed electrons to multi-MeV electrons may be reasonably attributed to interactions with the concurrent chorus waves. Specifically, the electron PSD increases for μ ≥ 300 MeV/G become less pronounced as K increases, consistent with the pitch angle dependence of chorus-induced electron energy diffusion at high energies. Our results therefore provide a clear observational evidence for the combined effect of substorm-induced injection and chorus wave scattering on the prompt enhancements of radiation belt electrons over a wide energy range within a couple of days.


ST20-A002
Response of Electric Field in Radiation Belt to Interplanetary Shock

Dianjun ZHANG1+, Wenlong LIU1#, Yiqun YU1, Xinlin LI2, Theodore SARRIS3
1Beihang University, 2University of Colorado Boulder, 3Democritus University of Thrace

Electric field impulses generated by interplanetary shocks can cause a series of dynamic processes in the Earth’s magnetosphere and were previously explained by either fast-mode wave propagation or flow related to compression of the magnetopause. Based on a Space Weather Modeling Framework simulation, we suggest a new scenario in which the evolution of the impulse is due to both the propagation of the fast-mode wave and the compression of the magnetopause, which can explain the simulation and observations in previous related studies. The onset of the electric field impulse is determined by the propagation of the fast-mode wave in the magnetosphere while the peak of the impulse is determined by the propagation of the compression of the magnetopause. The new understanding of the impulse is important for the generation of subsequent ultralow frequency waves through the coupling of the fast-mode to Alfvén waves and field line resonances and related radiation-belt electron acceleration.


ST20-A015
Analyzing the Effect of the Convection Electric Field on the Energy Spectrum of Energetic Electrons Scattered by the NWC Transmitter Signals

Yangxizi LIU+, Zheng XIANG#, Binbin NI, Deyu GUO, Junhu DONG, Jingle HU
Wuhan University

The very-low-frequency signals emitted from the NWC transmitter using for submarine communication can leak into the magnetosphere and resonant with hundreds of keV electrons in the inner radiation belt. The energy of electrons scattered by the NWC transmitter signals decreased with increasing L values, which is termed by ‘wisp’. Based on the energy spectrum of 100 – 400 keV electrons within L = 1.6 – 1.95 measured by the DEMETER satellite, we find that the position of ‘wisp’ structure in the spectrum changes with longitudes, indicating that the drift shell of electrons scattered by the NWC transmitter signals varies during the eastward drifting. The ‘wisp’ structure agrees well with the resonant energy calculated from first-order resonance between the electrons and the transmitter signals close to the NWC transmitter position. The ‘wisp’ shift to below the resonance curve when the longitude difference between the transmitter and the satellite is about 50º, and move to above the resonance curve when the longitude difference is around 150º. We introduce a dawn-to-dusk convection electric field to explain these phenomena. Assuming the conservation of the first and the second adiabatic invariants, we calculate the changes in L values and energies of electrons during the drift. Our results indicate that the electric field with the amplitude of 1~2 mV/m can well explain the longitudinal dependence variation of the ‘wisp’ in the spectrum.


ST20-A019
Parametric Sensitivity of Electron Scattering Effects by Electrostatic Electron Cyclotron Harmonic Waves

Yuequn LOU1#+, Xudong GU2, Xing CAO2, Ming-Yu WU1, Sudong XIAO3, Guoqiang WANG1, Binbin NI2, Tielong ZHANG4,5
1Harbin Institute of Technology, 2Wuhan University, 3Harbin Institute of Technology, Shenzhen, 4Austrian Academy of Sciences, 5University of Science and Technology of China

It is well known that electron cyclotron harmonic (ECH) waves can effectively precipitate hundreds of eV to tens of keV electrons into the upper atmosphere, resulting in the production of diffuse aurora. To deepen our outstanding of the contributions of ECH waves to diffuse aurora, in this study we perform a detailed analysis of the sensitivity of ECH wave-induced electron scattering to ambient magnetic field intensity, total electron density and density ratio between hot and cold electrons. Our results show that for various parameter sets, ECH waves can cause the precipitation loss of diffuse auroral electrons at energies of 100 eV to several keV and are capable of accelerating 100 eV to keV electrons at intermediate pitch angle, therefore contributing to the formation of butterfly pitch angle distribution. We also find that the variations of background parameters significantly change the magnitude of diffusion coefficients and resonant pitch angle range of < ∼1 keV electrons, while the scattering efficiency of >∼1 keV electrons is almost unaffected. For <∼1 keV electrons, an increase of magnetic field intensity or density ratio between hot and cold electrons weakens the electron scattering efficiency and narrows the resonant region to lower pitch angles, while an increase of total electron density generally plays an opposite role. In addition, the momentum diffusion can be stronger than pitch angle diffusion at large pitch angles for <∼1 keV electrons, while it can be negligible at higher energies.


ST20-A022
Modulation of Chorus by Field Line Resonance and Mirror-mode ULF Waves

Li LI1+, Yoshiharu OMURA2, Xuzhi ZHOU1#, Qiugang ZONG1, Robert RANKIN3, Chao YUE1, Suiyan FU1, Jie REN4
1Peking University, 2Kyoto University, 3University of Alberta, 4China University of Geosciences (Beijing)

Previous observations of wave modulation showed that chorus waves are often excited preferentially near the magnetic field troughs of ULF waves. In this study, we report for the first time the periodic occurrence of lower-band chorus waves near the crests of ULF wave field, although upper-band chorus waves are still excited near ULF wave troughs. This feature differs dramatically from previous observations, which is attributed to different modes of the observed ULF waves. In this event, ULF waves are identified to be drift-mirror mode rather than field-line resonances, which are characterized by the antisymmetric profile of wave magnetic field with respect to the equator. It is the antisymmetric profile that periodically adjusts the second-order derivative of the background magnetic field, which in turn modifies the threshold amplitude for nonlinear growth of chorus waves and consequently fosters chorus wave excitation near ULF wave crests. We demonstrate that the electron distributions modulated by ULF waves also play a role in modifying the threshold amplitude, which contributes to the excitation of upper-band chorus waves near ULF wave troughs. The good agreement between the theory and the observations highlights the combined effects of ULF wave field configuration and electron distributions in modulating chorus waves.


Thu-03 Aug | 10:20 - 12:20 | MR333
ST14 - The Near-Solar Environment: Advances, Challenges, and Prospects

Session Chair(s): Nour E. RAOUAFI, Johns Hopkins Applied Physics Laboratory

ST14-A004 | Invited
Statistical Properties of Solar Wind Velocity Within 20-60 Rs During the Minimum to Ascending Phase of Solar Cycle 24

Yuming WANG#+, Xiaolei LI
University of Science and Technology of China

Solar wind is the main way through which the mass, momentum and energy continuously transit from the Sun to heliosphere and therefore influence planets. So far, the full-sky solar wind is not well learnt and understood as it is hard to be detected remotely. Recently, we developed a correlation-aided reconstruction method to recognize and locate remote solar wind transients from the dual-view imaging data of the Heliospheric Imager-1 (HI1) onboard Solar Terrestrial Relations Observatory (STEREO), and then developed a technique to generate synoptic maps of solar wind radial velocity between 20 and 60 solar radii (Rs). By applying the technique to the HI1 data during Carrington Rotations 2081 - 2104, when solar activity went through minimum to ascending phase, we obtain the statistical properties of the background solar wind radial velocity within 20-60 Rs. This region is in the Mercury's orbit and is merely explored by human probes. More details will given in the talk.


ST14-A026 | Invited
Parker Solar Probe Observations of Turbulence in the Near-sun Solar Wind and Solar Corona

Christopher CHEN#+
Queen Mary University of London

Since its launch, Parker Solar Probe has allowed us an unprecedented opportunity to understand how solar wind turbulence works up close to the Sun, and the role that it plays in shaping the solar wind that we see. In this presentation, I will discuss what we have learnt from the most recent orbits where PSP crossed several times into sub-Alfvenic wind and saw clear changes in the turbulence properties. In particular, we see a change in the evolution of turbulence amplitudes that allow testing of the WKB vs non-WKB evolution of the fluctuations. We see a clear decrease of amplitudes in the sub-Alfvenic wind, as expected, that shows up prominently in the normalised amplitude dB/B - this is compared to theoretical predictions, allowing us to study the processes responsible for the fluctuations growing to the large amplitudes seen in the super-Alfvenic wind (dB/B~1, also known as "switchbacks"). We also discuss how other turbulence properties change in the sub-Alfvenic wind, including the magnetic compressibility, cross-helicity, and Elsasser spectra. These results will be discussed in the context of understanding the mechanisms for both the acceleration of the solar wind and the generation of the magnetic switchbacks.


ST14-A014 | Invited
Anisotropy of Magnetic Field Spectra at Kinetic Scales of Solar Wind Turbulence in the Inner Heliosphere

Shiyong HUANG#+
Wuhan University

Using the Parker Solar Probe data taken in the inner heliosphere, we investigate the power and spatial anisotropy of magnetic field spectra at kinetic scales (i.e., around sub-ion scales) in solar wind turbulence in the inner heliosphere. We find that strong anisotropy of the magnetic spectra occurs at kinetic scales with the strongest power in the perpendicular direction with respect to the local magnetic field (forming an angle θB with the mean flow velocity). The spectral index of the magnetic spectra varies from −3.2 to −5.8 when the angle θB changes from 90° to 180° (or 0°), indicating that strong anisotropy of the spectral indices occurs at kinetic scales in the solar wind turbulence. Using a diagnosis based on the magnetic helicity, we show that the anisotropy of the spectral indices can be explained by the nature of the plasma modes that carry the cascade at kinetic scales. We discuss our findings in light of existing theories and current development in the field.


ST14-A001
Joint Effects of Solar Activity and Solar Inertial Motion on Terrestrial Atmosphere

Valentina ZHARKOVA1#+, Irina VASILIEVA2, Simon SHEPHERD3, Elena POPOVA4
1Northumbria University, 2The Main Astronomical Observatory, 3Sorbonne Universite, 4Universidad Bernardo O’Higgins

By applying spectral analysis to the averaged sunspot numbers and to the summary curve of eigen vectors derived with Principal Component Analysis from full disk synoptic magnetic maps, we demonstrate that the main period of solar activity is mainly associated with 11-year cycles and a secondary period of about 330-380 years, grand solar cycles. These two periods are interpreted by two magnetic waves generated by the solar dynamo from dipole magnetic sources in two layers of the solar interior with periods close to 11 years and these wave interference leading to grand solar cycles separated by grand solar minima (GSMs). A further long-term two-millennial (2100-2300 years) period (Hallstatt’s cycle) was derived from the abundances of carbon and beryllium isotopes caused by solar irradiance variations. This two-millennial period is also detected in the oscillations of the baseline solar background magnetic field (SBMF) derived with PCA for 120 thousand years. We demonstrate that the S-E distance is reduced by 0.005 au in the millennium M1 600-1600 and by 0.011 au in millennium M2 1600-2600 that in the current phase of Hallstatt’s cycle caused by solar inertial motion leads to an increase of solar radiation deposited to Earth until 2600. The combined effects of solar activity and SIM on the terrestrial temperatures in the current millennium are also discussed.


ST14-A002
Magnetic Field Structure, Doppler Shift, and Intensity of Active Regions and Their Connections with the Solar Wind

Hui FU#+, Chi MA, Zhenghua HUANG, Lidong XIA, Jinmei ZHENG, Xinzheng SHI, Bo LI
Shandong University

The properties of active regions and their connections with the solar wind are important issues. In this study, nine isolated active regions near the solar disk center were chosen. The relationships between blueshift, intensity, magnetic concentrated areas (MCAs), and the potential-field source-surface (PFSS) open magnetic field of active regions were analyzed. Whether an active region contributes to the solar wind was identified only based on the relationship between the properties of in situ solar wind and the large structure of the corona. Then the two phenomena (blueshift and PFSS open magnetic field) for inferring whether an active region contributes to the solar wind were tested. We found that the blueshift areas appear in all cases and the average Doppler speed ranges from −6 to −23 km s−1. The blueshift areas generally root inside MCAs and are far from the neutral lines. The intensity of blueshift areas negatively correlates with the blueshift speed. Statistically, 10 of 16 blueshift areas are associated with the PFSS open magnetic field lines, and all 10 PFSS open magnetic field areas are accompanied by blueshift. We demonstrate that a polarity of an active region generally contributes to the solar wind if it is associated with a PFSS open magnetic field. There are 9 of 10 (13 of 16) PFSS open magnetic field areas (blueshift regions) associated with the solar wind. The results of this study should help determine the observation target of SPICE on board the Solar Orbiter whose scientific goal is connecting the Sun and the heliosphere.


ST14-A030
Energy Conversion and Partition Across Interplanetary Shocks in the Solar Wind

Die DUAN#+, Jiansen HE, Weining WANG
Peking University

Solar wind experiences significant heating during its transportation in the heliosphere. How the solar wind is heated is one of the cutting-edge issue in space physics. Interplanetary shocks are considered as one of the mechanism for the heating. When the shocks propagate through the solar wind plasma, the solar wind is compressed and heated. Dissipation of the solar wind turbulence is another mechanism for the heating. It is found that shocks also can amplify the turbulence in the downstream flows. The energy contribution to solar wind heating from the interplanetary shocks needs quantitive clarification. In this work, we estimate the amount of the energy conversion of the shocks in the solar wind, and investigate how the energy is partitioned between different types of bulk averaged energy (including thermal energy, bulk kinetic energy of different plasma species, and magnetic field energy) and turbulent fluctuating energy. Using the measurements from Wind at 1 au and PSP in the inner heliosphere, we statistically study the energy conversion and partition at different heliocentric distances, from the inner heliosphere to the outer heliosphere. We estimate the heating rate from the shocks, and compare it with the turbulent heating rate. We find the shock heating is much stronger than the turbulent heating for one shock, but have similar order of magnitude considering the occurrence frequency of the shocks.


Thu-03 Aug | 10:20 - 12:20 | MR334
ST20 - Advances in Understanding Radiation Belt Dynamics: Theory, Observation and Simulation

Session Chair(s): Zheng XIANG, Wuhan University

ST20-A001 | Invited
Internal Source of Plasmaspheric Hiss

Zhenpeng SU#+
University of Science and Technology of China

Plasmasphere is an upward extension of the ionosphere at low and middle latitudes along the closed magnetic field lines rooted in the Earth, where the trapped whistler-mode waves in the frequency range from tens to thousands of Hertz are named as plasmaspheric hiss. Since its discovery, plasmaspheric hiss has been considered an important plasma wave to drive the precipitation loss of the Van Allen radiation belt electrons. However, the origin of plasmaspheric hiss has long been under debate. There have been two classes of sources proposed for the plasmaspheric hiss: (1) background plasma noises inside the plasmasphere and (2) other plasma waves outside the plasmasphere. Here, on the basis of Van Allen Probes observations and numerical modeling, we show that a combination of linear and nonlinear instabilities of energetic electrons can effectively produce the hiss waves in both the plasmaspheric main body and plume over a broad range of magnetic local times.


ST20-A018
Realistic Dispersion of Plasmaspheric Hiss in the Inner Magnetosphere and Its Effect on Wave-induced Electron Scattering Rates

Xin MA+, Xing CAO#, Binbin NI, Qi ZHU, Zheng XIANG
Wuhan University

The cold plasma approximation is a common treatment to study wave–particle interactions between plasmaspheric hiss and magnetospheric electrons, which, however, can become a challenge during periods of disturbed geomagnetic activity. To assess the validity of the cold plasma dispersion relation of plasmaspheric hiss, we adopt the cold plasma theory to calculate the wave magnetic field intensities from the electric field intensities observed by Van Allen Probe A from 2012 October 1 to 2018 February 28. Comparisons between the observed and converted hiss magnetic field intensities capture pronounced differences with the enhancement of substorm activity, and exhibit the largest discrepancies on the nightside MLT sector for low-frequency hiss waves. We also use both the hiss dispersion curves derived from the observations and the cold plasma dispersion relation to evaluate hiss induced electron diffusion coefficients under different substorm activity conditions. The results indicate that the profiles of electron diffusion rates vary considerably for the two hiss dispersion relations and that the differences between them become increasingly distinct with substorm activity intensification. Our study therefore demonstrates that the cold plasma theory can become less reliable for plasmaspheric hiss waves under disturbed geomagnetic circumstances and that the realistic wave dispersion is essential to better quantify the electron scattering effect of hiss waves, which needs to be carefully incorporated into future global simulations of the generation and propagation of plasmaspheric hiss and associated dynamic variability of radiation belt electrons.


ST20-A023
Generation Processes of Whistler-mode Rising-tone Emissions in the Inner Magnetosphere

Yoshiharu OMURA#+, Takeshi NOGI
Kyoto University

We have performed a series of particle simulations for whistler-mode wave-particle interaction in a parabolic magnetic field with 12 different frequencies of triggering waves and three different plasma frequencies specifying cold plasma densities. Under a given plasma condition, a specific frequency range of the triggering wave exists that can generate rising-tone emissions. The generation region of rising-tone emission shifts upstream. The velocity of the wave generation region is dependent on duration of the subpacket, which is controlled by formation of the resonant current in the generation region. When the source velocity [1], which is a sum of the resonance and group velocities, is approximately the same as the velocity of the wave generation region, a long-sustaining rising-tone emission is generated. When the spatial and temporal gap between subpackets exists due to damping phase of short subpacket generation, resonant electrons in the gap of the subpackets are carried at the resonance velocity to the upstream region, and the velocity of the wave generation region becomes large in magnitude. When formation of resonant currents is delayed, the velocity of the generation region becomes smaller than the source velocity in magnitude. Below one quarter of the cyclotron frequency, coalescence of subpackets takes place, suppressing formation of the resonant current in the generation region [2]. Since gradual upstream shift of the generation region is necessary for the wave to grow locally, the source velocity should be a small negative value. References:
[1] Nogi, T., & Omura, Y., Upstream shift of generation region of whistler-mode rising-tone emissions in the magnetosphere, submitted to J. Geophys. Res. Space Physics.
[2] Nogi, T., & Omura, Y. (2022). Nonlinear signatures of VLF-triggered emissions: A simulation study. Journal of Geophysical Research: Space Physics, 127 (1), e2021JA029826.


ST20-A024
Developing Chorus Wave Model Using Van Allen Probe and Arase Data

Dedong WANG1#+, Yuri SHPRITS1, Ting FENG2, Thea LEPAGE3, Ingo MICHAELIS1, Geoff REEVES4, Ondrej SANTOLIK5,6, Yoshizumi MIYOSHI7, Yoshiya KASAHARA8, Satoko NAKAMURA7, Atsushi KUMAMOTO9, Shoya MATSUDA8, Ayako MATSUOKA10, Iku SHINOHARA11, Fuminori TSUCHIYA9
1GFZ German Research Centre for Geosciences, 2Wuhan University, 3Luleå University of Technology, Sweden, 4Los Alamos National Laboratory, 5Czech Academy of Sciences, 6Charles University, 7Nagoya University, 8Kanazawa University, 9Tohoku University, 10Kyoto University, 11Japan Aerospace Exploration Agency

Chorus waves play an important role in the dynamic evolution of energetic electrons in the Earth’s radiation belts and ring current. Due to the orbit limitation of Van Allen Probes, our previous chorus wave model developed using Van Allen Probe data is limited to low latitude. In this study, we extend the chorus wave model to higher latitudes by combining measurements from the Van Allen Probes and Arase satellite. As a first step, we intercalibrate chorus wave measurements by comparing statistical features of chorus wave observations from Van Allen Probes and Arase missions. We first investigate the measurements in the same latitude range during the two years of overlap between the Van Allen Probe data and the Arase data. After the intercalibration, we combine the chorus wave measurements from the two satellite missions and develop an analytical chorus wave model which covers all magnetic local time and extends to higher latitudes. This chorus wave model will be further used in radiation belt and ring current simulations.


ST20-A006
A Parametric Study About the Dependence of Chorus Wave Properties on Magnetic Field Inhomogeneity

Zeyin WU#+, Xin TAO, Yifan WU
University of Science and Technology of China

Chorus waves, one of the electromagnetic whistler mode waves, frequently manifest as discrete, repetitive, and quasi-monochromatic emissions with frequency chirping. With different wave amplitude and frequency chirping rates, chorus waves have been observed in the past few decades not only in the magnetosphere of Earth but also in the magnetospheres of other planets, such as Saturn and Jupiter. Motivated by understanding different properties of chorus waves in these magnetospheres using the recently proposed ''Trap-Release-Amplify'' 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 critical role of background magnetic field inhomogeneity in affecting chorus wave properties at different planets.


ST20-A005
Frequency Chirping of Electromagnetic Ion Cyclotron Waves in Earth's Magnetosphere

Zeyu AN1+, 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

Electromagnetic ion cyclotron waves are observed to exhibit frequency chirping, contributing to rapid scattering and acceleration of energetic particles. However, the physical mechanism of chirping remains elusive. Here, we propose a new model to explain the chirping and provide direct observational evidence from satellites for validation. Our results relate the frequency chirping of the wave to both wave amplitude and magnetic field inhomogeneity for the first time. The general applicability of the model's underlying principle opens a new path to understanding the frequency chirping of other waves.


ST20-A011
Non-resonant Scattering Effect on Radiation Belt Electrons by H+ Band EMIC Waves

Ruoxian ZHOU1+, Fu SONG1#, Binbin NI1, Xin TAO2
1Wuhan University, 2University of Science and Technology of China

In this study, we have estimated the scattering effect on radiation belt electrons induced by electromagnetic ion cyclotron (EMIC) waves and investigated the potential non-resonant scattering mechanism. By using the test particle simulations, we have calculated the wave-induced diffusion coefficients. The results show that the scattering rates in (Ek, αeq) space are significantly different in three Regimes: Regime I: Ek > 1 MeV and αeq < ~80°, with maximum pitch angle diffusion rates of ~10-2 s-1 and energy diffusion rates of < 10-8 s-1; Regime II at all energies and αeq > ~85°, with maximum pitch angle diffusion rates of ~10-3 s-1 and energy diffusion rates of ~10-5 s-1; and Regime III at the other energies and pitch angles where the pitch angle diffusion rates can reach ~ 10-5 s-1 and the energy diffusion rates <10-8 s-1. By analysis of the resonant conditions, the cyclotron resonance is thought to be responsible for the electron scattering effect within Regime I, while the dominative mechanism in Regimes II and III remains unclear. The subsequent single particle tracing suggests that the scattering effect for electrons at Regimes II and III is mainly due to the variation of the electrons’ parallel velocity, which is modulated by the parallel electric field of the EMIC waves. We further validate that the modulations are caused by the non-resonant process and exclude the potential Landau and bounce resonant mechanisms. Briefly, beyond the resonant scattering process, the reported non-resonant scattering effect can produce strong diffusion and advection effect on relativistic electrons, which is important for better understanding the dynamics of the radiation belt electrons.


Thu-03 Aug | 1:10 - 3:10 | MR309
ST19 - Lithosphere-Atmosphere-Space Coupling

Session Chair(s): Chieh-Hung CHEN, China University of Geosciences, Tao CHEN, Chinese Academy of Sciences

ST19-A008 | Invited
Predicting Epicenter by West Zone Characteristics

Tao CHEN#+
Chinese Academy of Sciences

In northern hemisphere, continent is manly at middle latitude. The characteristics of middle latitude atmospheric wind is oriented east, namely west wind. So, in northern hemisphere middle latitude region, most countries in northern hemisphere in middle latitude west zone, such as China, Turkey and American. Once any TEC (Total Electronic Content ) abnormality in the ionosphere that is related an imminent earthquake appears, the epicenter region must be located northwest off the TEC abnormality region due to the west wind zone and acoustic gravity wave from the crust sudden thermal emission.


ST19-A002
The Role of Great Deep-focus Undersea Earthquakes in the Lithosphere–Atmosphere–Ionosphere (LAI) Coupling Process

Dan TAO1#+, Guangxue WANG1, Jiayi ZONG1, Yuanzheng WEN1, Jinbin CAO2, Roberto BATTISTON3, Zhima ZEREN4
1Chengdu University of Technology, 2Beihang University, 3University of Trento, 4China Earthquake Administration

Even though many seismic anomalies have been found in the ionosphere, this physical process of LAI coupling is still unclear and even controversial, and there are still plenty of issues or details that need to be carefully worked through. On the one hand, such studies rarely distinguish between inland and submarine seismic events and mainly focus on the strong cases with a shallow focus (generally less than 100 km or less). On the other hand, it is difficult to identify the earthquake associated effects due to the fuzzy background noises resulting from natural and artificial non-seismic sources, in addition to solar and global geomagnetic perturbations. This work is an attempt to critically analyze the correlation between great deep-focus undersea earthquake and possible ionospheric anomalies. The significant TEC (total electron content) temporal and spatial anomalies were detected over the epicenter of 2007 Mw 7.5 Jakarta–Java earthquake, and they coincide well with the striking plasma anomalies in the ionosphere in situ observed by the LEO (low Earth orbit) satellite. The localization and synchronization of the disturbances during the earthquake suggest that these ionospheric anomalies are highly related to this large undersea earthquake. In order to identify this correlation, we made efforts to distinguish seismo-associated signals from large electromagnetic noise due to solar and geomagnetic activities, natural non-seismic sources and known artificial signals. Nevertheless, the difficulties of this work should be recognized and approached with caution. This special (deep-focus and undersea) case study here provides us with valuable information on the study of lithosphere–atmosphere–ionosphere (LAI) coupling process and reminds us that deep-focus undersea seismic events need to be treated more carefully and discreetly in the future.


ST19-A012 | Invited
Pre-earthquake Transients Features. Case Study for the M8.2 July 28th, 2021, Chignik, Alaska Earthquake

Dimitar OUZOUNOV1#+, Xuhui SHEN2, Sergey PULINETS3, Jann-Yenq (Tiger) LIU4, Katsumi HATTORI5, Rui YAN6, Menas KAFATOS1, Patrick TAYLOR7
1Chapman University, 2Chinese Academy of Sciences, 3Space Research Institute (IKI) Russian Academy of Sciences, 4National Central University, 5Chiba University, 6Institute of Natural Hazards, 7NASA Goddard Space Flight Center

We present a study of multi-parameter analysts of transient phenomena observed in the lithosphere/atmosphere /ionosphere associated with the M8.2 earthquake of July 28th in Chignik, Alaska, the largest U.S. earthquake in 50 years. We used multi-platform satellite sensor data to study critical processes in the atmosphere that modify the Earth's plasma environment and are associated with earthquakes. We are collecting data from multiple-satellite observations: 1/ Electric, magnetic field, and plasma observations from the China/Italy Seismo-Electromagnetic Satellite (CSES1), 2/. Outgoing long-wavelength radiation (OLR obtained from NPOESS) and 3/. Atmospheric Data -Temperature, Pressure, and Relative humidity obtained from NASA GEOS assimilation system; and 4/. Electron density variations in the ionosphere via GPS Total Electron Content (GPS/TEC).NOAA satellite thermal observations show an increase in infrared radiation associated with the acceleration of OLR from NOAA15/18 polar-orbiting satellites. Increases in OLR data from the satellite were preceded by five days with an intensification in the atmospheric chemical potential (on July 16th ), measured near the epicentral area. The Electric and magnetic field observations from the CSES1 satellite indicated a distinct disturbance from orbits on 19 and 27 July over the July 29 quake. The GPS/Total Electron Content data suggests an increase of electron concentration in the ionosphere on July 26, 1 to 2 days before the M8.2 earthquake, by integrating satellite data and assimilation models; we recorded data patterns inside the Dobrovolsky-Bowman estimated area of earthquake preparation. We will show that by combining the near-space and assimilation data accordingly to the physical concept of the LAIC model, we were able to identify, on a regional basis, anomalous patterns of pre-earthquake related features in the atmosphere-ionosphere environment associated with M8.2, July 28th Chignik, Alaska earthquake.


ST19-A016 | Invited
Seismo-ionospheric Precursors of the Total Electron Content in Global Ionosphere Maps Before the 6 February 2023 M7.8 and M7.5 Turkey Earthquakes

Jann-Yenq (Tiger) LIU#+, Yun-Sheng WEN, F.Y. CHANG, Chi-Yen LIN, Yuh-Ing CHEN
National Central University

On 6 February 2023 at 01:17 UTC, an M7.8 earthquake occurred in South-Eastern Turkey (37.2°N 37.0°E, 10.0 km depth), and several strong aftershocks have also been observed in the region, notably a magnitude M7.5 (38.0°N 37.2°E, 10 km depth) at 10:24 UTC the same day. Spatial analyses of the total electron content (TEC) of the global ionosphere map (GIM) are employed to observe the latitude-longitude distributions of seismo-ionospheric anomalies (SIAs) during January-February 2023. A global search of 5183 (=73x71) lattices shows that SIAs of significant TEC increases specifically appear near the epicenter on day 24-22 (12-16 January) and 2-0 (4-6 February) before the two earthquakes. The ion density and ion velocity measured by the science payload of Advanced ionospheric Probe (AIP) onboard the FORMOSAT-5 (F5) satellite and those by ion velocity meter (IVM) onboard FORMOSAT-7 are used to find the ionospheric electric fields over the epicenter area during the two periods of 12-16 January and 4-6 February 2023.


ST19-A010 | Invited
Development of LF Broadband Interferometer for Identification of Earthquake Precursor LF Band Electromagnetic Radiation: Preliminary Report

Yuichiro OHTA1, Katsumi HATTORI1#+, Kenshin MIURA1, Chie YOSHINO1, Noriyuki IMAZUMI2,3
1Chiba University, 2The Institution of Professional Engineers, 3Idemitsu Kosan

Precursors of earthquakes associated with the LF band have been reported for many years. As an example, Oike & Yamada reported an increase in the number of LF-band pulses at the Uji station before the Hyogo-ken Nanbu earthquake. However, Izutsu later reported that some of the pulse increases were due to lightning activity. In the observation of LF band electromagnetic radiation associated with earthquakes, it is a challenge to distinguish it from lightning activity. On the other hand, ICT technology and GPS technology are now more advanced than those days, making it possible to develop an interferometer. An interferometer is a system that observes electric field changes at multiple locations about 20 km apart and estimates the spatio-temporal electromagnetic wave source from the phase difference of waveforms obtained at each location. In this research, as part of the development of the "LF band broadband interferometer", detection of LF band noise related to earthquakes and pulse number investigation by waveform survey using one interferometer element, and three interferometer elements performance evaluation as an interferometer system. As a result, the waveform data observed by the interferometer element was analyzed, and it was found that the LF/VLF waveform signal due to the anti-mine was successfully recorded. We also detected an LF band signal different from the above anti-mine waveform. Although it is possible that it is the effect of intra-cloud discharge, it was found that the possibility that it is a signal related to an earthquake cannot be ruled out. In addition, when we evaluated the operation of the interferometer system, we found that although there were no problems with the recording waveform characteristics between the elements, there was a discrepancy in the trigger timing (synchronization) between the elements. The details will be shown in the presentation.


ST19-A006 | Invited
Ionospheric Disturbances Observed Over China After 2022 Jan 15 Tonga Volcano Eruption

Yongxin GAO1#+, Ting LI1, Xuemin ZHANG2, Y. SUN3
1Hefei University of Technology, 2China Earthquake Administration, 3Kyushu University

On 15 January 2022, a powerful eruption of the submarine Hunga Tonga-Hunga Ha’apai volcano occurred at about 30 kilometers south of the Ha'apai Islands in the Kingdom of Tonga (at -20.55N, -175.39E), which causes atmospheric waves spreading world widely. In this study we investigate the TEC variation over China using the BeiDou Navigation Satellite System (BDS). For comparison, the atmospheric pressure records were examined, which show that the Lamb wave passed by the same stations four times with a constant speed of 310 m/s. However, the TEC results show that the ionospheric disturbances passing over China four times with different speeds within four days after the eruption, two traveling along the short-path direction (S1 and S2) and two along the long-path direction (L1 and L2). The primary front of the first short-path S1 event travels with a speed of 340 m/s that is higher than the Lamb wave (310 m/s). The faster speed suggests that the primary front cannot be fully attribute to the Lamb wave and further studies need to explore its mechanism. The second short-path (S2) and first long-path (L1) events travel with speeds of 301 m/s and 310 m/s, respectively, close to the speed of the Lamb wave, and may be caused by upward energy leakage during the propagation of the Lamb wave. The second long-path (L2) event travels with a speed of 264 m/s, possibly induced by the gravity waves.


ST19-A015 | Invited
Disturbances in Lithosphere, Atmosphere, and Ionosphere and Their Interaction Due to the Tonga Eruption

Yang-Yi SUN1#+, Chieh-Hung CHEN1, Xuemin ZHANG2, Yongxin GAO3, Kai LIN1, Jann-Yenq (Tiger) LIU4
1China University of Geosciences, 2China Earthquake Administration, 3Hefei University of Technology, 4National Central University

The explosive eruption of the Tonga underwater volcano (20.53°S, 175.38°W) occurred at ~4:15 UT on 15 January 2022 and caused disturbances with periods ranging from minutes to hours that propagate and interact in geospheres. In this study, the networks of ground-based barometers, magnetometers, and global navigation satellite system receivers recorded disturbances that traveled away from the eruption with acoustic speeds in the atmosphere and ionosphere. The primary disturbances with periods of several hours in the magnetic fields and total electron content (TEC) observations reveal the electrodynamics changes in the upper atmosphere and the coupling of E- and F-region dynamo. The atmospheric Lamb wave propagating upward caused the secondary waves in the ionosphere and seeds irregularities following the leading front of the primary disturbances. The radio occultation technique onboard the FORMOSAT‐7/COSMIC2 (F7/C2) mission sounds the ionosphere in the vertical direction, which shows the large-scale disturbances and irregularities. On the other hand, the co-located instruments monitored perturbations in the lithosphere, atmosphere, and ionosphere simultaneously at 29°N, 103°E that is ~ten thousands of kilometers northwest away from the eruption. The primary phenomena of the eruption-associated disturbances are the long-period changes (period of ~ 2 hr) in the ionospheric TEC and the magnetic field in the upper atmosphere, indicating the interactions of the ionospheric electrodynamics. The secondary phenomena included wind disturbances in the troposphere, which contribute to short-period changes (up to ten minutes) in air pressure, ground vibrations, and atmospheric electric field. The disturbances propagating upward further triggered short-period variations in the geomagnetic field and TEC. The primary changes in ionospheric electrodynamics, wind disturbance in the lower atmosphere, its upward propagation, and the resonance reveal the complex coupling phenomena due to the eruption and enrich our understanding of the geosphere coupling.


ST19-A009
Recent Advances and Challenges in the Seismo-electromagnetic Study: A Brief Review

Hongyan CHEN1#+, Peng HAN1, Katsumi HATTORI2
1Southern University of Science and Technology, 2Chiba University

Due to their potential application in earthquake forecasting, seismo-electromagnetic phenomena were intensively studied for several decades all over the world. At present, measurements from ground to space have accumulated a large amount of observation data, proving an excellent opportunity for seismo-electromagnetic study. Using a variety of analytical methods to examine past earthquake events, many electromagnetic changes associated with earthquakes have been independently reported, supporting the existence of pre-earthquake anomalies. This study aimed to give a brief review of the seismo-electromagnetic studies preceding earthquakes and to discuss possible ways for the application of seismo-electromagnetic signals at the current stage. In general, seismo-electromagnetic signals can be classified into electric and magnetic changes in the lithosphere and perturbations in the atmosphere. We start with seismo-electromagnetic research in the lithosphere, and then we review the studies in the lower atmosphere and upper atmosphere, including some latest topics that aroused intense scholarly interest. The potential mechanisms of seismo-electromagnetic phenomena are also discussed. It was found that although a number of statistical tests show that electromagnetic anomalies may contain predictive information for major earthquakes, with probability gains of approximately 2–6, it is still difficult to make use of seismo-electromagnetic signals efficiently in practice. To address this, finally, we put forward some preliminary ideas about how to apply the seismo-electromagnetic information in earthquake forecasting.


Thu-03 Aug | 1:10 - 3:10 | MR310
ST25 - Vertical and Latitudinal Coupling Processes in the Lower Thermosphere and Ionosphere, and the International Meridian Circle Project

Session Chair(s): Shunrong ZHANG, Massachusetts Institute of Technology

ST25-A008 | Invited
Scientific Objectives and Observational Priorities of the International Meridian Circle Programs

Weining William LIU1#+, Liwen REN2
1National Space Science Center, Chinese Academy of Sciences, 2Chinese Academy of Sciences

Through a global networking of a variety of ground-based instruments, the International Meridian Circle Program (IMCP) is poised to study the coupled Sun-Earth system with unprecedented coverage and coordination. It, for the first time, offers the realistic opportunity to track mass and energy flow from the sun to earth’s surface, as well as how changes in the earth interior (e.g., secular variation of geomagnetic field) might impact processes in geospace and the atmosphere. The assemblage of a coherent research programs calls for a multidisciplinary approach and an awareness of whole-system flows of energy and electricity. In this talk the whole-system architecture of the IMCP science is outlined, and some key research objectives discussed.


ST25-A007 | Invited
Coupling Processes in the Lower Thermosphere and Ionosphere: Vision and Contributions of the CEDAR Community

Larisa GONCHARENKO#+
Massachusetts Institute of Technology

The Coupling, Energetics, and Dynamics of Atmospheric Regions (CEDAR) is a program funded by the United States National Science Foundation’s Atmospheric and Geospace Sciences Division with a mission to understand the fundamental properties of the space-atmosphere interaction region. Understanding coupling processes in the lower thermosphere and influence of these processes on the upper thermosphere and ionosphere is one of the important CEDAR topics that gained a lot of attention within the last decade. CEDAR community is probably the largest national research community that includes several hundreds of scientists and engineers, although it has a significant international component. CEDAR is a truly diverse community that includes instrument developers (both ground-based and space-based), model developers, and scientists using various datasets and models to advance CEDAR topics. Annual CEDAR workshop (held on June 25-30, 2023) is attended by ~350 participants and is a primary opportunity to self-organize and exchange ideas and recent progress. This talk will highlight most recent accomplishments and plans of the CEDAR community that are relevant to the coupling processes in the mesosphere and lower thermosphere. Development of ground-based assets is a fundamental component of the needed solution. The talk will describe current status and future plans for variety of ground-based techniques, including meteor radars, airglow imagers, Fabry-Perot interferometers, HF radars, ionosondes, and incoherent scatter radars. As community realizes importance and critical need for new global observations of MLT winds, composition and temperature, I will describe current effort and status of several planned NASA missions, including AWE, DYNAMIC, and a joint ESA-NASA Lower Thermosphere-Ionosphere (ENLoTIS) effort. The talk will include several highlights of recent results from different observational platforms and theoretical models.


ST25-A005 | Invited
Prospects for a Vivid Collaborative Science Between the GDC Mission and the Ground-based Community

Bea GALLARDO-LACOURT1,2#, Larry KEPKO3, Douglas ROWLAND1, Katherine GARCIA-SAGE1, Guiping LIU1+
1NASA Goddard Space Flight Center, 2The Catholic University of America, 3National Aeronautics and Space Administration

With a launch NET 2029, NASA’s Geospace Dynamics Constellation (GDC) would serve as a strategic focus for worldwide, coordinated ITM science. This coordination will involve space-based and ground-based assets, as well as simulations and theory, under the umbrella of the “ITM Great Observatory.” GDC’s science team has formed a community group to plan coordinated science between GDC and the worldwide community’s ground-based assets. This GDC ground-based community group serves as an entry point for ground-based observers to learn more about the GDC mission and its science, as well as facilitate coordination of ground-based efforts to leverage GDC measurements to extend and enhance both GDC and broader ITM science objectives.


ST25-A004 | Invited
Climate Changes in the Upper Atmosphere Driven by the Changing Greenhouse Gas Concentrations and the Earth's Magnetic Field

Liying QIAN1#+, Joseph MCINERNEY2, Wenbin WANG1, Stanley SOLOMON1, Hanli LIU1
1National Center for Atmospheric Research, 2University Corporation for Atmospheric Research

We simulate climate changes (trends) in the upper atmosphere for the 20th century driven by the changing greenhouse gas (GHG) concentrations and the earth's magnetic field (MF), and examine the relative importance of these two drivers, using the Whole Atmosphere Community Climate Model - eXtended (WACCM-X). Model simulations show that the upper atmosphere cool and contract in the 20th century, with the largest mean global average rate in the upper thermosphere, at ~ -1.8 K/decade for neutral temperature and ~ -2.8%/decade for neutral mass density. In the thermosphere, trends are predominantly driven by the GHG driver. However, the MF driver plays an important role in the ionosphere trends in the longitude sector ∼120oW–20oE. Near the mesopause, temperature trends are small compared to interannual variations, so trends in this region are uncertain. In the mesosphere, dynamics significantly impact temperature trends, so in the summer upper mesosphere, temperature trends can become near zero or positive; solar irradiance effects on the global-average temperature are positive and decrease monotonically with decreasing altitude; the global average temperature trends are negative, with the maximum at ~ -1 K/decade in the middle to lower mesosphere.


ST25-A010
Ionospheric Dynamical Responses to the 2003-11-20 Superstorm Observed by Millstone Hill Incoherent Scatter Radar

Shunrong ZHANG#+, Philip ERICKSON, Ercha AA, Anthea COSTER
Massachusetts Institute of Technology

The super geospace storm of 20 November 2003 is notable for its -422 nT minimum Dst index at 18:15 UT, resulting from a long-lasting and strongly negative IMF Bz, which reached a minimum of -52 nT at 15:50 UT. This event is the second-largest Dst drop since 1960, behind only the superstorm of 14 March 1989. Previous studies have primarily focused on strong plasma density enhancements at low latitudes in the American sector, with longitudinal variations suggesting effects associated with prompt penetration electric fields and potentially disturbance dynamo electric fields. Limited studies have reported Storm Enhanced Density (SED) at subauroral latitudes and the Tongue of Ionization (TOI) at the polar cap during this event, and the more general super-storm characteristic ionospheric variations at subauroral latitudes remain unclear. In this presentation, we report on Millstone Hill incoherent scatter radar observations that demonstrate the electron density profile evolution, with a dramatic elevation of hmF2 (reaching up to ~600-700 km altitude), substantial ion up-flow, and associated extremely large ion flux, as well as prominent heating to the ionosphere. We also compare the ionospheric responses of this superstorm with those of a regular geospace storm (the 2015 St. Patrick's Day storm). We will also provide important context regarding the local ionospheric observation in relation to super-storm regional and global ionospheric changes, specifically those related to the occurrence of SED plumes and Large Scale Traveling Ionospheric Disturbances (LSTIDs).


ST25-A012
Response of Equatorial Ionization Anomaly to Magnetic Declination Observed by Radio Occultation of FORMOSAT-7/COSMIC-2 in 2020-2021

Jann-Yenq (Tiger) LIU#+, Mei-Yu CHEN, Po-Han LEE
National Central University

Radio occultation (RO) ionospheric electron density profiles of FORMOSAT-7/COSMIC-2 (F7/C2) are used to study structures and dynamics of the equatorial ionization anomaly (EIA) during 2020-2021. Occurrence times, altitudes, and strengths of EIA crests in the northern and southern hemisphere as well as their differences along three longitudes with the maximum, zero, and minimum magnetic declinations (hereafter, the most positive-declination, DP, -165°E to -105°E geographic; the most the most negative-declination, DN, -60°E to 0°E; and around zero-declination, DZ, 90°E to 150°E, respectively are isolated and examined. The EIA crest appears earlier in the winter hemisphere than in the summer hemisphere. The altitude of EIA crests mainly appears at about 250-350 km; the one in the summer hemisphere is higher than that in the winter hemisphere; and however, the two altitudes are at similar during equiaxial months. The EIA appearance time is related to plasma flows dragged by trans-equatorial neutral winds; the EIA altitude is a function of eastward electric fields associated with the magnetic declination; and the EIA electron density can be affected by the trans-equatorial neutral wind, seasons, and magnetic declination.


Thu-03 Aug | 1:10 - 3:10 | MR333
ST14 - The Near-Solar Environment: Advances, Challenges, and Prospects

Session Chair(s): Nour E. RAOUAFI, Johns Hopkins Applied Physics Laboratory

ST14-A029 | Invited
Solar Coronal Jets, the Magnetic Flux Changes Leading to Jets, and Implications for Eruptions on Larger and Smaller Size Scales

Alphonse STERLING1#+, Navdeep PANESAR2, Ronald MOORE1
1NASA Marshall Space Flight Center, 2Bay Area Environmental Research Institute

Large-scale solar eruptions often include ejection of a filament, a solar flare, and expulsion of a coronal mass ejection (CME). Unravelling the magnetic processes that build up the free energy for these eruptions and trigger that energy's release in the eruption is a continuing challenge in solar physics. Such large-scale eruptions are comparatively infrequent, with the moderate level ones (say, GOES M-class events) occurring perhaps once every few days on average during active-activity times, and much less frequently during quieter times. In contrast, solar coronal jets, which are long (~50,000 km), narrow (<~10,000 km), transient (~10---20 min) plasma spires with bright bases and that are seen in soft X-rays and EUV, occur much more frequently, likely several hundred times per day independent of large-scale solar activity level. Recent studies indicate that coronal jets are small-scale versions of large-scale eruptions, often produced by eruption of a small-scale "miniflament," that results in a "miniflare" analogous to a larger typical solar flare, and that sometimes produces a CME analogue (a "narrow CME" or "white-light jet"). Under the assumption that jets are small-scale eruptions, their higher occurrence frequency and faster build-up evolution reveals perhaps fundamental aspects of all eruptions that are not as easy to discern in the more-complex magnetic environment and the slower build up to the larger eruptions. For example, several studies show that jets occur at locations where magnetic flux cancelation in occurring, suggesting that this is a key energy build-up and release process for eruptions of all sizes. This work was supported by NASA's Heliophysics Guest Investigator (HGI), Heliophysics Supporting Research (HSR), and Heliophysics System Observatory Connect (HSOC) Programs, and by the NASA/MSFC Hinode Project.


ST14-A011 | Invited
Mission: A Close Encounter with the Sun

Jun LIN#+
Yunnan Observatories, Chinese Academy of Sciences

This work is to introduce a proposed deep space mission, which aims to perform in situ detection of the central structure, namely the magnetic reconnection current sheet, which drives the large scale eruption on a star. The main focus of this mission is on the fine physical characteristics of the large scale magnetic reconnection taking place on the Sun, our nearest star, revealing the secret of the most violent energy release process, also known as the solar storm, in the solar system. The scientific goal of this mission, magnetic reconnection, is a kernel process of energy conversion occurring in the magnetized plasma in the universe, and has long been a fairly important research topic or even research area in solar physics, space science, plasma physics, and the related fields. In situ detection enhances the spatial resolution of the instruments used on the Earth 5∼20 times, will provide us extra-clear images of the Sun and the related information. We are thus able to study, to learn, and to understand the Sun on an unprecedented platform, and further resolve the long-standing puzzle in the solar community regarding the fine physical property of the kernel process driving the solar eruption, as well as that of the corona heating.


ST14-A021 | Invited
Early Results and In-flight Calibrations of the ASO-S Mission

Weiqun GAN, Li FENG#+
Chinese Academy of Sciences

The ASO-S mission was launched in October 2022. It 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. Both flares and CMEs originate from the evolution of solar magnetic fields. The mission aims to simultaneously observe the magnetic fields, solar flares, and CMEs on a single platform, which constitute the main characteristics of ASO-S. For simplicity, we use “1M2B” to outline the scientific goals of ASO-S in which “1M” means magnetic field, “2B” means two bursts, i.e. flares and CMEs. In this talk, the in-flight calibrations of the three payloads will be introduced. We will also show some early scientific results of the mission.


ST14-A027
Numerous Correlations and Their Implications in Solar Wind Turbulence: Parker Solar Probe Observations

Guo-Qing ZHAO1#+, Romain MEYRAND2, Heng Qiang FENG1, De-Jin WU3
1Luoyang Normal University, 2University of Otago, 3Chinese Academy of Sciences

Numerous correlations exist between plasma and magnetic parameters in solar wind turbulence, which can provide important indications and constraints on the physics of turbulence evolution and heating processes. Based on Parker Solar Probe observations, this talk will present the correlations of six parameters (the proton temperature, bulk speed, magnetic power spectral density (PSD), cross helicity, magnetic helicity, and spectral index at proton inertial/kinetic scales), and explore the relations between these correlations. These correlations indicate the following: (1) the turbulence with a larger PSD is characterized by a higher cross helicity; (2) a larger PSD corresponds to a higher proton temperature, faster bulk speed, and steeper proton-scale magnetic spectrum; (3) a higher cross helicity accounts for higher proton-scale magnetic helicity. To be precise, the PSD has the largest correlation coefficient (CC) of 0.85 with proton temperature and has a considerably large CC of 0.70 with a proton-scale spectral index. The cross helicity has a moderate CC of 0.52 with magnetic helicity in the low beta case (beta < 0.6), where beta is the ratio of plasma to magnetic pressure. The correlation between cross helicity and PSD is also considerable with a CC exceeding 0.6 in the low beta case but tends to be negligible when beta approaches 1.5. These findings are understood by the “helicity barrier” mechanism. We propose, to the best of our knowledge for the first time, the observational correlation between the magnetic helicity and cross helicity as evidence of the invariant of generalized helicity in turbulence, which is relevant to the helicity barrier. The correlation between the cross helicity and PSD in the low beta case is proposed to be a signature of the helicity barrier.


ST14-A009
Observing the Near-solar Environment by Solar Conjunction of Spacecraft with Very Long Baseline Interferometry Telescopes

Maoli MA1#+, Guifré MOLERA CALVÉS2, Giuseppe CIMO3, Ming XIONG4, Jiansen HE5, Yidan HUANG1
1Shanghai Astronomical Observatory, 2University of Tasmania, 3Joint Institute for VLBI ERIC, 4National Space Science Center, 5Peking University

Probing the solar corona is crucial to study the coronal heating and solar wind acceleration. However, the transient and inhomogeneous solar wind flows carry large-amplitude inherent Alfvén waves and turbulence, which make detection more difficult. We report the solar conjunction observation of China's Tianwen and ESA's Mars Express with radio telescopes within 30 Rs. The observations were carried out in 2021. Several coronal mass ejection (CME) passed across the ray paths of the telescope beams. We obtain the frequency fluctuations (FFs) of the spacecraft signals from each individual telescope. First, we visually identify the drift of the frequency spikes near the solar environment especially when the transient solar wind flows happened. They are used as traces to estimate the solar wind velocity. Then, we perform the cross-correlation analysis on the time series of FF from different telescopes to study the solar wind velocity and the inhomogeneity of solar wind. At last, we make a statistical analysis of the FFs during different heliocentric distance. Our analysis shows the ground-station pairs are able to form particular spatial projection baselines with high resolution and sensitivity to study the propagation of the nascent dynamic solar wind structure.


ST14-A012
Parker Solar Probe: Discoveries and Outlook

Nour E. RAOUAFI1+, Robert DECKER2#
1Johns Hopkins Applied Physics Laboratory, 2Johns Hopkins University Applied Physics Laboratory

On January 2023, NASA's Parker Solar Probe (PSP) mission had completed 14 of its scheduled 24 orbits around the Sun, with the closest approach (i.e., perihelion) of 13.28 solar radii from the Sun's center. PSP's primary science goal is to determine the structure and dynamics of the Sun's coronal magnetic field, understand how the solar corona and wind are heated and accelerated, and determine what processes accelerate energetic particles. The science data returned by PSP led to significant discoveries and potential breakthroughs, yielding more than 700 peer-reviewed publications. The first four years of the prime mission were mainly during the solar cycle minimum. With the rise of solar activity, PSP will explore solar wind variability as the cycle progress to its maximum. I will present an overview of the major scientific discoveries by PSP and the mission's outlook.


ST14-A015
Modelling the Socio-economical Impact of Extreme Solat Storms - With Application to the Great Britain

Ding YUAN#+
Harbin Institute of Technology, Shenzhen

An extreme solar storm is a hazardous space weather event in the solar system and will threaten the modern infrastructures in the near solar environment. Although a number of advances were made in both instrumentation and physics-based modeling, there is still a lack of quantitative estimates of the socioeconomic impact of solar storms. In this study, we developed an integrated model for assessing the risk and dynamical economical loss at the national scale. This model includes the estimate of the occurring rate of extreme solar storms, the couple of geomagnetic disturbances to the power grid, the probability of failure for transformers, and the dynamical inoperability of the sectorial economy. The modeling shows that in a solar storm of 1-in-1,000,000 years, Great Britain could lose 80-90% of its power supply. Our model could provide a quantitative assessment of the socioeconomic impact of solar storms, and could be applied to hazard mitigation and policy-making for a government.


Thu-03 Aug | 1:10 - 3:10 | MR334
ST21 - General Session in Solar and Terrestrial Sciences Including Space Weather

Session Chair(s): Dedong WANG, GFZ German Research Centre for Geosciences, Balan NANAN, Shandong University

ST21-A018
The Solar Wind Variations in the Last Solar Cycle from MHD Simulations

Zhenguang HUANG#+, Gabor TOTH, Nishtha SACHDEVA, Bart VAN DER HOLST, Igor SOKOLOV, Ward MANCHESTER, Tamas GOMBOSI, Lulu ZHAO
University of Michigan

We describe our first attempt to systematically simulate the solar wind during different phases of the last solar cycle with the Alfven Wave Solar atmosphere Model (AWSoM) developed at the University of Michigan. Key to this study is the determination of the optimal values of one of the most important input parameters of the model, the Poynting flux, which prescribes the energy flux passing through the chromospheric boundary of the model in the form of Alfven wave turbulence. It is found that the optimal value of the Poynting flux parameter is correlated with the open magnetic flux and the area of the open magnetic field regions. These highly linear correlations could shed light on understanding how Alfven wave turbulence accelerates the solar wind during different phases of the solar cycle and estimating the Poynting flux parameter for real-time solar wind predictions with AWSoM. Supported by the NSF SWQU and LRAC programs


ST21-A002
The Butterfly Diagram and Power-law Distribution of Coronal Jets

Jiajia LIU1#+, Song ANCHUAN1, David JESS2, Jie ZHANG3, Mihalis MATHIOUDAKIS2, Szabolcs SOÓS4,5, Francis KEENAN2, Yuming WANG1, Robertus ERDELYI6
1University of Science and Technology of China, 2Queen's University Belfast, 3George Mason University, 4Eötvös Loránd University, 5Hungarian Solar Physics Foundation, 6The University of Sheffield

Power-law distributions have been studied as a significant characteristic of non-linear dissipative systems. Since discovering the power-law distribution of solar flares that was later extended to nano-flares and stellar flares, it has been widely accepted that different scales of flares share the same physical process. Here, we present the newly developed Semi-Automated Jet Identification Algorithm (SAJIA) and its application for detecting more than 1200 off-limb solar jets during the Solar Cycle 24. Power-law distributions have been revealed between the intensity/energy and frequency of these events, with indices found to be analogous to those for flares and coronal mass ejections (CMEs). These jets are also found to be spatially and temporally modulated by the solar cycle forming a butterfly diagram in their latitudinal-temporal evolution, experiencing quasi-annual oscillations in their analysed properties, and very likely gathering in certain active longitudinal belts. Our results strongly suggest that the same nonlinear statistics of scale-free processes is behind these different scales of eruptive events, including flares, jets, and CMEs, in solar and stellar atmospheres. Although these jets, like flares and other large-scale dynamic phenomena, are found to be significantly modulated by the solar cycle, their corresponding power-law indices still remain similar.


ST21-A020
The Firefly Constellation: Enabling a Holistic View of the Sun and Its Environment

Nour E. RAOUAFI1#+, J. Todd HOEKSMA2, Sarah GIBSON3, Lisa A. UPTON4, Jeffrey NEWMARK5, Thomas E. BERGER6,7, Angelos VOURLIDAS8, Anthony CASE9, Susan T. LEPRI10, Donald M. HASSLER4, James KINNISON8, Manolis GEORGOULIS11, George HO4, Nicholeen M. VIALL5, Louise HARRA12,13, Marco VELLI14, Adam SZABO15, Marta CASTI16, Sofiane BOUROUAINE17, Vamsee K. JAGARLAMUDI8, Juliana T. VIEVERING8, James P. MASON8
1Johns Hopkins Applied Physics Laboratory, 2Stanford University, 3National Center for Atmospheric Research, 4Southwest Research Institute, 5NASA Goddard Space Flight Center, 6National Oceanic and Atmospheric Administration, 7National Weather Service, 8Johns Hopkins University Applied Physics Laboratory, 9Harvard-Smithsonian Center for Astrophysics, 10University of Michigan, 11Academy of Athens, 12World Radiation Center, 13ETH-Zurich, 14University of California, Los Angeles, 15National Aeronautics and Space Administration, 16The Catholic University of America, 17Florida Institute of Technology

Firefly is an innovative mission concept study for the Decadal Survey for Solar and Space Physics (Heliophysics) 2024-2033 to fill long-standing knowledge gaps in Heliophysics. A constellation of spacecraft will provide both remote sensing and in situ observations of the Sun and heliosphere from a whole 4π-steradian field of view. The concept implements a holistic observational philosophy that extends from the Sun’s interior, to the photosphere, through the corona, and into the solar wind simultaneously with multiple spacecraft at multiple vantage points optimized for continual global coverage over much of a solar cycle. The mission constellation includes two spacecraft in the ecliptic and two flying as high as ~70º solar latitude. The ecliptic spacecraft will orbit the Sun at fixed angular distances of ±120º from the Earth. Firefly will provide new insights into the fundamental processes that shape the whole heliosphere. The overarching goals of the Firefly concept are to understand the global structure and dynamics of the Sun’s interior, the generation of solar magnetic fields, the origin of the solar cycle, the causes of solar activity, and the structure and dynamics of the corona as it creates the heliosphere. We will provide an overview of the Firefly mission science and architecture and how it will revolutionize our understanding of long-standing heliospheric phenomena such as the solar dynamo, solar cycle, magnetic fields, solar activity, space weather, the solar wind, and energetic particles.


ST21-A023
Statistical Investigation of Langmuir Waves in Type III Solar Radio Burst Sources

Will TREVETT1, Iver CAIRNS2#+, Daniel GRAHAM3
1The University of Sydney, 2University of Sydney and CUAVA, 3Swedish Institute of Space Physics

Type III solar radio bursts involve streaming electrons that produce Langmuir waves that then couple wave energy into radio emission. These Langmuir waves can be driven to large enough amplitudes that they undergo electrostatic (ES) decay into a backward propagating Langmuir wave and forward propagating ion acoustic wave. The forward and backwards propagating Langmuir waves can then ''beat'' together to produce characteristic Langmuir waveforms and spectra, plus radio emission. Stochastic growth theory (SGT) predicts that the probability distribution of the Langmuir wave electric field strength should be lognormal, with known modifications if nonlinear processes like ES decay are occurring. Other analyses suggest Pearson distributions may be relevant. Here, previous work on Langmuir waves in type III source regions is generalized and tested by analysing the probability distributions of the waveforms of Langmuir waves observed by the STEREO spacecraft. The focus is on a set of published events identified using spectral analyses to have or not have spectral evidence for ES decay. For events for which spectral analyses provide evidence of ES decay, 86\% of the probability distributions are consistent with the combination of SGT and a nonlinear process like ES decay, while of those without spectral evidence for ES decay 78% of the probability distributions are well fitted by pure SGT. Moreover, better fits with stronger statistical significance are obtained for pure and nonlinear SGT than for Pearson distributions in the majority of events (~90%). These results provide strong evidence for SGT and ES decay proceeding in type III burst source regions.


ST21-A025
Space Weather Effects on the CUAVA-1 and INSPIRE-2 CubeSat Orbits

Vanathy ARUDSELVAN1, James LEE1, Tony MONGER1, Iver CAIRNS2#+
1The University of Sydney, 2University of Sydney and CUAVA

We investigate the effects of space weather on the time-varying orbits of the Australian CubeSats CUAVA-1 and INSPIRE-2. Time series for two orbital parameters were used in this comparison, both sourced from NORAD’s Keplerian Two-Line Element Sets (TLEs): the temporal rate of change of the apogee altitude and the B* (BSTAR) drag term. These were compared with NASA time series for the F10.7cm solar radio flux, Dst, and Kp indices and GOES X-ray and EUV data. The time series of the CUAVA-1 and INSPIRE-2 orbital parameters show events superposed on slowly varying secular changes with relatively small amounts of noise, with the events correlated by eye with changes in the space weather indices. Lomb-Scargle analyses reveal very similar, quasi-periodic, variations in the orbital parameters and space weather indices at approximately 25-day intervals. The 25±1 day periods found are close to the synodic rotational period of the solar equator. Cross-correlation analyses show strong peaks, and so significant correlations, at time lags near 0 ± 5 days, some consistent with causality. The observed periods and cross-correlations provide strong evidence that the orbital changes are driven by space weather. Qualitatively, this may be due to enhanced ionisation and heating of the atmosphere, causing it to expand and increase satellite drag. More detailed interpretative work is ongoing, as are analyses of other satellites, to establish how specific space weather phenomena caused the clear effects observed on the orbits of CUAVA-1 and INSPIRE-2.


ST21-A004
Relationships Between Microwave and EUV Spectra in Solar Flare and Their Estimation by Machine Learning

Kyoko WATANABE1#+, Mamoru MAEDA1, Masumi SHIMOJO2, Kosuke NAMEKATA2, Satoshi MASUDA3
1National Defense Academy of Japan, 2National Astronomical Observatory of Japan, 3Nagoya University

It is known that there is a good correlation between the radio emission from the Sun and the EUV emission spectrum in the solar cycle variation. We have investigated this relationship using daily data from the Nobeyama Radio Polarimeters (NoRP; 1, 2, 3.75, 9.4 GHz) and TIMED/SEE (0.5-190 nm) for the period 2002-2016 and found that radio emissions at all frequencies correlated well with EUV emission spectra. However, it is difficult to accurately derive the relationship between radio and EUV emission spectra only by comparing the observed data, because the emission mechanisms are different between them. Therefore, we reproduced EUV emission spectra from multiple frequencies of radio data using machine learning with reference to Zhang & Paxton (2018). As a result, we were able to reproduce most of the EUV wavelengths with correlation coefficients above 0.90. The frequencies contributing to the reproduction of EUV spectra were also checked, and it was found that the contribution of 2 GHz was high in the short wavelength (10-50 nm), and that of 1 GHz and 2 GHz was high in the longer wavelength (50-124 nm). It was also found that the frequencies contributed for EUV emission varied depending on the solar activity level. On the other hand, in solar flares, the relationship between radio and EUV emission has not been mentioned. However, it is the solar flare emissions that causes large fluctuations in the Earth's ionosphere, and if its effects can be estimated from the radio data, it will be important information for space weather forecasting. Then in this study, we show the results of our investigation of the relationship between radio and EUV emission in solar flares. We also report the results of our attempt to reproduce the solar EUV emission spectrum from multiple frequencies of radio data using machine learning.


ST21-A029
Statistical Studies of Geomagnetic Storms and Their Effect on Earth Atmosphere Currents During Solar Cycle-24

Raja Adibah RAJA HALIM SHAH1#+, Nurul Shazana ABDUL HAMID1, Mardina ABDULLAH1, Adlyka ANNUAR1, Idahwati SARUDIN2
1Universiti Kebangsaan Malaysia, 2Universiti Sains Malysia

This study presents geomagnetic storm statistics for 24 solar cycles from 2009 to 2019 while looking at the storm effects on Earth's atmosphere currents using selected events. Our analysis characterized the geomagnetic storm using the Dst index for the entire year of the solar cycle 24. This work observes the (GIC) and (EEJ) current changes based on observational data at different latitudes. The geomagnetic stations detect GIC existence at high and medium latitudes. At the same time, variation in EEJ current is observed using data collected from stations located in the geomagnetic equatorial region. This study identified several variations in the geomagnetic phases, even in the same geomagnetic storm type, such as long, rapid, and complex recovery during moderate storms. In addition, our analysis observed that the value of GIC was higher in high-latitude geomagnetic areas. Furthermore, the EEJ current is disturbed during geomagnetic storms in equatorial areas. This EEJ current also seems related to the AE index and GIC, indicating the current chain from high latitude to the equator region.


Thu-03 Aug | 3:30 - 5:15 | MR309
ST19 - Lithosphere-Atmosphere-Space Coupling

Session Chair(s):

ST19-A004
Deep Postseismic Creep Following Large Earthquakes Revealed by Repeating Aftershocks in the Southeastern Tibetan Plateau

Shujun LIU#+, Chi-Chia TANG
China University of Geosciences

Large earthquakes and the subsequent postseismic period are the most dramatic part of the seismic cycle that usually lasts hundreds to thousands of years. However, the fault dynamics which account for the postseismic events are yet to be fully understood. It is well known that aftershock evolutions can reveal the geometry and rupture process of the seismogenic fault. Repeating aftershock, a type of repeating earthquake, is an effective tool for studying the deep fault behavior after strong earthquakes. Here we selected templates from the National Earthquake Data Center catalog between three years before and one year after the mainshock origin time and then used the fast matched filter to detect missing earthquakes. Next we use the seismicity of repeating aftershock sequences (RASs) as a proxy to reveal postseismic slips following the four large earthquakes in the southeastern Tibetan Plateau. We find 136 RASs after the Lushan, Jiuzhaigou, and Jinggu mainshocks, whereas only one RAS was detected after the Ludian mainshock that occurred on a conjugate fault. The seismicity shows the aftershock migrated couples of minutes after the mainshocks while the RAS occurred a few hours later. This observation suggests the brittle faulting preceeded to the deep creeps. The deep creeps mainly follow a velocity-strengthening friction mode and decay with an Omori-law p-value of ~1. The results may indicate that the combination of fault healing and geometry together controls the deep fault behaviors. We develop two models to explain the evolution of fault dynamics after large earthquakes. Our results provide new insights into spatiotemporal fault evolutions after large earthquakes.


ST19-A017
Analysis of Geomagnetic and Ionospheric Total Electron Content Disturbances for Earthquake Precursor Detection

Nur Fatin Irdina ZULHAMIDI1#+, Mardina ABDULLAH1, Nurul Shazana ABDUL HAMID1, Khairul Adib YUSOF2
1Universiti Kebangsaan Malaysia, 2Universiti Putra Malaysia

The effectiveness and accuracy of earthquake precursors are measured by the ability of the precursors to determine the time, epicentral distance, and magnitude of the earthquake for short-term earthquake prediction. This study sought to enhance the reliability of earthquake forecasting by monitoring two different parameters of geomagnetic and ionospheric total electron content in investigating both parameters’ responses prior to earthquakes (EQ). Through the SuperMAG database, a 1-min sampling (low-fidelity) period of global geomagnetic daily variations data recorded by global magnetometer stations between the years 2000 - 2020 with a magnitude above 5.0 were downloaded and analyzed. The diurnal variation ratio (DVR) method using threshold value has been employed in finding the earthquake precursor. Meanwhile, the TEC data from the GPS station near the earthquake epicenter were acquired by The National Institute of Information and Communications Technology (NICT). Based on selected earthquake events, data from GPS stations were downloaded and analyzed. The TEC variations before the earthquake were analyzed by utilizing the upper and lower bound method (by using the median and interquartile range in the upper and lower bound calculation) to detect the TEC anomalies prior to the earthquake. The anomalous behaviors exhibited by each earthquake event in geomagnetic diurnal ratio variations were concluded to be detected in all components prior to the earthquakes. All geomagnetic N, E, and Z components showed anomalous behavior during the quiet days but with temporal lags between the components. Anomalous observations on TEC parameter were also found to be related to geomagnetic anomalies before the earthquake.


Thu-03 Aug | 3:30 - 5:15 | MR309
ST22 - New Results from Cosmic-2, Gold, and Icon Missions

Session Chair(s): Yen-Jung WU, University of California, Berkeley

ST22-A005
Ultraviolet Remote Sensing of the Thermosphere-ionosphere System from GEO – Beyond Solar Minimum

Richard EASTES1#+, Deepak KARAN1, Quan GAN1, Fazlul LASKAR1, Xuguang CAI1, William MCCLINTOCK1, Wenbin WANG2
1University of Colorado Boulder, 2National Center for Atmospheric Research

Recent increases in solar activity have significantly increased forcing the thermosphere-ionosphere (T-I) system from above. Consequently, forcing from above has increased relative to forcing from below. This change in above versus below contributions to the total forcing, is expected to produce changes in the observable characteristics of the T-I system, changes that the GOLD mission is uniquely positioned to observe and help us understand. Some preliminary comparisons of recent and solar minimum observations will be discussed. This talk will also discuss some new data that can be obtained from limb observations. These provide additional information about the temperature, composition and density profiles in the T-I system. They can provide a fuller picture of the T-I system’s structure and weather. By expanding and extending GOLD’s observations, continued advances in understanding and modeling the weather of the T-I system, as well as it’s interaction with other regions of the geospace system in different phases of a solar cycle, can be expected.


ST22-A002
Hunga Tonga Volcanic Eruption’s Thermospheric Temperature Perturbation: Gold Observation and Modelling

Saurav ARYAL1#+, Sharon VADAS2, Erich BECKER2, Hanli LIU3, Quan GAN1, Joseph EVANS4, Wenbin WANG3, Richard EASTES1
1University of Colorado Boulder, 2NorthWest Research Associates, 3National Center for Atmospheric Research, 4Computational Physics, Inc.

The powerful Hunga Tonga-Hunga Ha'apai volcanic eruption on January 15, 2022, released a significant amount of energy into the whole atmosphere. Observations show that the eruption generated a spectrum of waves some of which propagated globally. The NASA Global Observation of the Limb and Disk (GOLD) mission detected the eruption's global-scale thermospheric signatures from 12-16 UT. Wave-like features observed in GOLD disk temperatures during this period had peak deviations of greater than 100 K. These observations allow us to quantify the difference in wave characteristics of the primary waves in the lower altitudes and the subsequent thermospheric waves. Comparison with models provides insight into how wave preturbations are transferred between different atmospheric layers during such events. We will present comparison of GOLD observations with the MESORAC/HIAMCM and the WACCM-X model studies. Preliminary comparison of GOLD (~ 150-160 km) and MESORAC/HIAMCM (near 155 km) temperatures show good first order agreement, but there are differences that will be analyzed further.


ST22-A003
Gold and Icon Observations of Thermospheric Responses to the Nov 3rd 2021 Geomagnetic Storm

Quan GAN1#+, Yen-Jung WU2, Xuguang CAI1, Scott ENGLAND3, Wenbin WANG4, Liying QIAN4, William MCCLINTOCK1, Richard EASTES1
1University of Colorado Boulder, 2University of California, Berkeley, 3Virginia Tech, 4National Center for Atmospheric Research

Leveraging observations made by two NASA missions – GOLD (Global-scale Observations of the Limb and Disk) and ICON (Ionospheric Connection Explorer), we investigate the responses of thermospheric composition, temperature, and neutral winds in the middle thermosphere to a geomagnetic storm on Nov 3rd, 2021, as well as the interplay amongst them for the first time. These synergetic observations reveal the depletion of up to 60% in O/N2 and the enhancement of ~ 100 K in temperature poleward of 30-deg in the middle thermosphere. Meridional winds at ~ 250 km are altered by ~ 25 m/s, characterized by a reversal of seasonal, prevailing northward winds to the geomagnetic storm driven southward winds in the NH low latitudes. This study fills a long-lasting gap of observing concurrent and collocated responses of composition, temperature, and neutral winds in the thermosphere following a geomagnetic storm.


ST22-A004
Short-term Variability of DE3 and Its Impacts on the Ionosphere

Manbharat DHADLY#+, McArthur JONES, Douglas DROB, Scott BUDZIEN
Naval Research Laboratory

This study is focused on resolving daily diurnal eastward propagating tide with zonal number 3 (DE3) (3,3) Hough mode variations and their potential impact on the ionosphere. We utilized TIMED/TIDI, TIMED/SABER, and ICON/MIGHTI for DE3 tidal estimation and COSMIC-2 Global Ionospheric Specification (GIS) and TIME-GCM/NAVGEM-HA to study its impact on the ionosphere. A Hough mode fitting approach was used to estimate (3,3) amplitudes and phases from observations, while Fourier decomposition was utilized for TIME-GCM/ NAVGEM-HA and COSMIC-2/GIS to validate and probe potential ionospheric impacts. In 2020-2021, TIDI, SABER, and MIGHTI (3,3) daily tidal estimates were in good agreement, with correlation coefficients ranging from 0.73-0.83. In 2010, mean daily (3,3) amplitude variability in TIDI and SABER reached ~5 m/s and ~2 K, respectively, but could increase by a factor of 2 or more over a week. Furthermore, strong increases in DE3 from days-to-weeks correspond with similar increases in F-region ionospheric wave-4 amplitudes from both models and observations. This combined data and modeling approach signifies the impacts of lower atmospheric meteorology on the ionosphere.


ST22-A001
Altered Mesosphere Lower Thermosphere Mean Circulation from a Major Sudden Stratospheric Warming: Icon Perspectives

Federico GASPERINI#+
Orion Space Solutions

Sudden stratospheric warmings (SSWs) are large-scale phenomena characterized by dramatic dynamic disruptions in the stratospheric winter polar regions. Previous studies, especially those employing whole atmosphere models, indicate that SSWs have strong impacts on the circulation of the mesosphere lower thermosphere (MLT) and drive a reversal in the mean meridional circulation (MMC) near 90-125 km altitude. However, the robustness of these effects and the roles of SSW-induced changes in global-scale wave activity to drive the reversal have been difficult to observe simultaneously. This work employs horizontal lower thermospheric (~93-106 km altitude) winds near 10S-40N latitude from the Michelson Interferometer for Global High-resolution Thermospheric Imaging (MIGHTI) instrument onboard the Ionospheric Connection Explorer (ICON) to present observational evidence of a prominent MLT MMC reversal associated with the January 2021 major SSW event and to demonstrate connections to semidiurnal tidal activity and possible associations with a ~3-day ultra-fast Kevin wave (UFKW). Concurrent observational impacts on the topside ionosphere are also investigated.


Thu-03 Aug | 3:30 - 5:15 | MR310
ST24 - Advances in the Understanding of Equatorial and Low Latitude Ionosphere-thermosphere System Processes Through Observations and Modellings

Session Chair(s): Yuichi OTSUKA, Nagoya University, Deepak KARAN, University of Colorado Boulder

ST24-A010 | Invited
Solar and Geomagnetic Activity Dependence of 150-km Echoes Observed by the Equatorial Atmosphere Radar in Indonesia

Tatsuhiro YOKOYAMA#+, Rieko TAKAGI, Mamoru YAMAMOTO
Kyoto University

150-km echoes frequently observed by VHF radars in equatorial and low-latitude regions have been a puzzling phenomenon for more than a half century. They are observed from the direction perpendicular to the geomagnetic field and generally show a necklace-like pattern in range-time-intensity plots and a narrow spectral width. The occurrence characteristics of 150-km echoes in low-latitude regions are studied using the Equatorial Atmosphere Radar (EAR) in Indonesia. The long-term observation of the 150-km echoes by the EAR enables us to study the occurrence characteristics of 150-km echoes statistically. It is shown that the occurrence rate of the 150-km echoes observed by the EAR shows a semiannual variation with two peaks in solstices and a negative correlation with both the EUV flux and Sigma Kp index, that is, the solar and the geomagnetic activity. Geomagnetic activity correlates with the occurrence rate of 150-km echoes observed one day after when the Sigma Kp was measured. However, the occurrence rate is always low during the high solar activity period regardless of the geomagnetic activity. While the seasonal variation and the solar activity dependence of the occurrence of 150-km echoes are consistent with previous studies, this is the first time a negative correlation with geomagnetic activity is reported. Further studies are required to discover unknown factors that control the occurrence of 150-km echoes.


ST24-A012
Equatorial Plasma Bubbles Growth Rate Modulation During Geomagnetic Storms Revealed by Numerical Simulations

Shasha ZOU1#+, Zihan WANG2, Joseph HUBA3, Aaron RIDLEY1
1University of Michigan, 2University of Texas at Arlington, 3Synteck Technologies

The Equatorial Plasma Bubbles (EPBs) are low-density plasma structures embedded in the large-scale Equatorial Ionization Anomaly (EIA). They are known to host ionospheric irregularities that can cause severe satellite signal scintillations and even signal loss lock, thereby affecting communication and navigation. However, our understanding of the variability of EIA and EPBs during space weather events, particularly geomagnetic storms, is still illusive and thus prohibits forecasting capabilities. In recent years, the rapidly developing ground-based GNSS receiver network has enabled regional to continental scale measurements of the ionosphere and has revealed rich dynamic structures in those regions during storm time, such as much widened or asymmetric EIA crest and super EPBs reaching mid-latitudes, e.g., equatorward boundary of the main trough. Using comprehensive observational tools and the coupled GITM and SAMI3 models, we focus on the EIA and EPB dynamics during geomagnetic storms, calculate the relative contributions of the plasma drift, thermospheric wind, and gravitational term to the EPB growth rate, compare with and without E region drivers, and evaluate the dependence of the growth rate on local times and the phase of geomagnetic storms.


ST24-A004
A Statistical Analysis of Conjugate Equatorial Plasma Bubbles Based on 630 Nm Airglow Observations

Tao YU1#+, Zu-Kang DAI1, Na YANG1, Jin WANG2, Di FU3, Xiang-peng FENG3, Yu-Tao FENG3
1China University of Geosciences, 2China University of Geosciences (Wuhan), 3Chinese Academy of Sciences

Using the observations of the 630-nm all-sky imagers (ASIs) located in the geomagnetic conjugate points in the American sector from 2014 to 2017, this study statistically analyzed the features of conjugate equatorial plasma bubbles (EPBs), including their occurrence rate, zonal width, location and zonal drift velocity. The results show that the occurrence rate of the EPBs that occur simultaneously at geomagnetic conjugate points is ∼84%. The zonal widths of the EPBs are mainly ∼100 km, and the width differences of EPBs between the northern and southern hemispheres are mainly within ±30 km. The zonal displacements of the center locations of the northern and southern EPBs are within ±50 km. The zonal drift velocities of the northern and southern EPBs are nearly equal. However, it should be noted that the velocity of the EPBs in the northern hemisphere is 10% faster than that in the southern hemisphere. The results suggest that conjugate EPBs are common. Moreover, the non-conjugate EPBs in the northern and southern hemisphere can occur occasionally, which is probably associated with the different ionospheric backgrounds between the two hemispheres. The features of the conjugate EPBs as shown in this study provides support for the nowcasting of EPBs in the conjugate hemispheres.


ST24-A002 | Invited
Equinox Transition of the Nighttime Ionospheric F-region Densities Observed by Gold

Wenbin WANG1#+, Xuguang CAI2, Liying QIAN1, Quan GAN2, Fazlul LASKAR2, Richard EASTES2
1National Center for Atmospheric Research, 2University of Colorado Boulder

Ionospheric F-region densities are influenced by multiple processes, including ion production and loss due to chemical reaction, and transport by electric fields and neutral winds. All these processes vary with solar EUV radiation, solar zenith angle (season and local time) and geomagnetic activity, and are regulated by the Earth’s magnetic field that changes with longitude and is hemispherically asymmetric. This produces complicated seasonal variations and hemispheric asymmetry in the ionosphere and thermosphere. Recent studies using the NASA GOLD (Global-scale Observations of the Limb and Disk) data have shown that the durations of the December and June solstice seasons in thermospheric composition are not the same and different between the two hemispheres. The equinox transition of composition is short and highly variable with longitude. In this work, we employ the nighttime GOLD disk observations of 135.6 nm airglow radiance, a proxy for ionospheric F2 peak density, to investigate the nighttime ionospheric equinox transition. We focus on the duration and timing of this transition for the hemispherically asymmetric electron density with respect to the geomagnetic equator. Preliminary results indicate that at 0° longitude, the equinox transition occurs at the March equinox and lasts for about 7-10 days, but at 45°W, the transition occurs before the March equinox by 5-7 days and persists for about 2 weeks, suggesting a longitudinal dependence. On the other hand, due to the relatively low F2-peak density during the June solstice, the hemispheric asymmetry in electron density is not clearly defined in the GOLD data, making it difficult to determine the September transition. Nevertheless, the September transition occurs much later in the late October with a short duration and longitude dependence. In this presentation, we will also examine the dependence of the equinox transition on solar activity and discuss the relevant physical processes.


ST24-A001
Investigation of Merged Nighttime EIA Structure Based on GOLD Observations and WACCM-X Simulations

Liying QIAN1#+, Kun WU1, Wenbin WANG1, Xuguang CAI2, Joseph MCINERNEY3
1National Center for Atmospheric Research, 2University of Colorado Boulder, 3University Corporation for Atmospheric Research

Unique contrasting Equatorial Ionization Anomaly (EIA) structures were observed by the Global-scale Observation of the Limb and Disk (GOLD) mission during the storm of November 03 - 04, 2021: during the pre-reversal enhancement (PRE) period of the two nights, the two EIA crests were well separated on November 03 (the initial phase of the storm) but they were merged at some longitudes (the recovery phase of the storm). We use the Whole Atmosphere Community Climate Model (WACCM-X) model to simulate the EIA structures during these two nights. The simulations show two separated EIA crests on November 03 but merged EIA crests on November 04, which are qualitatively consistent with the observations from GOLD. Based on the simulations from the WACCM-X model, we found that the formation of merged EIA crests was due to weakened E x B drifts during PRE. Further diagnostic analysis revealed that this was driven by disturbance dynamo electric field (DDEF) during the storm recovery phase, which weakened the PRE eastward electric field.


ST24-A006
Seasonal and Solar Cycle Dependences of the Nighttime Equatorial Ionization Anomaly Crests as Observed by the GOLD Mission

Richard EASTES1#+, Deepak KARAN1, Carlos MARTINIS2, Robert DANIELL3, Quan GAN1, Wenbin WANG4, William MCCLINTOCK1
1University of Colorado Boulder, 2Boston University, 3Ionospheric Physics, 4National Center for Atmospheric Research

Each day the GOLD (Global-scale Observations of the Limb and Disk) imager observes the Equatorial Ionization Anomaly (EIA) from ~8° E to ~80° W geographic longitude, beginning just after sunset and continuing into the night. GOLD’s observations have been used to quantify the EIA crests' latitudes and densities. Daily measurements of these characteristics provide tests of our understanding of how winds and tides, solar radiation, chemistry, and electric and magnetic fields influence the thermosphere-ionosphere system. Previously, monthly averages of the crests’ latitude versus longitude during March, September and December 2020 were analyzed. These solar minimum measurements exhibited seasonal differences that had previously been omitted when analyzing the EIA‘s nighttime latitudes. While December solstice differed significantly from the equinoxes, a dependence on the subsolar point was evident for all three seasons. The data indicated that the magnetic equator to subsolar point separation has a significant influence on the nighttime crests’ average latitudes, possibly more significant than winds or magnetic declination, during solar minimum. This presentation will describe an extension of that analysis to observations in the ascending phase of the current solar cycle and will compare the results with previous, solar minimum results.


ST24-A005
Gold Observation of Thermospheric Temperature Changes During the July 2nd, 2019 Solar Eclipse

Saurav ARYAL1#+, Joseph EVANS2, Fazlul LASKAR1, Wenbin WANG3, Richard EASTES1, Deepak KARAN1
1University of Colorado Boulder, 2Computational Physics, Inc., 3National Center for Atmospheric Research

Rapid reduction in incident high energy Solar radiation by eclipses’ is expected to induce cooling in the Earth’s Thermosphere-Ionosphere (TI) system. However, the scale of the cooling has not been quantified due to difficulty in making in-situ measurements and available co-incidences with LEO satellite in this region of the atmosphere during transient solar events. The Global Observation of Limb and Disk (GOLD) mission synoptically observed the temperature changes associated with the July 2nd, 2019 total solar eclipse over South America, first such measurements made in the middle thermosphere near 160 km. Preliminary analysis shows that the observed temperature reduction near the totality is significant (>50K). Initial comparison with T-I modeling for the eclipse show that model underestimate the GOLD observed, eclipsed-induced temperature and composition change. At the moment, the reason for the data-model discrepancy is not known. Recent GOLD observations of other eclipses have also been made and further observations are planned for the 2024 eclipse over the continental North America, in conjunction with other ground-based measurements. Further multi-instrumental comparison with T-I modeling could help the T-I community rectify the shortcoming in predicting T-I response to transient events like solar eclipses. GOLD’s observational result of the temperature and composition change (published recently) for the 2019 total solar eclipse will act as a template to plan for the April 8, 2024 eclipse.


Thu-03 Aug | 3:30 - 5:15 | MR333
ST14 - The Near-Solar Environment: Advances, Challenges, and Prospects

Session Chair(s): Die DUAN, Peking University, Nour E. RAOUAFI, Johns Hopkins Applied Physics Laboratory

ST14-A016
Observation and Simulation of Solar Wind Proton Energization Associated with Alfvenic Pulses

Jiansen HE1#+, Qiaowen LUO2, Xingyu ZHU3, Die DUAN1, Daniel VERSCHAREN4, Jun CUI2,5, Hairong LAI2
1Peking University, 2Sun Yat-sen University, 3University of Alabama in Huntsville, 4University College London, 5Chinese Academy of Sciences

How Alfvenic pulses (also called magnetic switchbacks in case of large amplitude) contribute to the heating and acceleration of the solar wind in the inner heliosphere is a critical issue in the heliophysics. To address this issue, we conduct a comprehensive study involving the observational analysis and numerical simulation. In the first part, we analyze magnetic field data and plasma data of the selected Alfvenic pulse events measured by PSP during its encounters. We investigate the anisotropic thermalization of Alfvenic pulses by studying the measured proton temperatures in parallel and perpendicular directions as well as proton density and specific proton fluid entropy. We find that the protons in most Alfvenic pulse events are hotter than outside the Alfvenic pulses, showing characteristics of parallel and perpendicular heating. We find that the density of most Alfvenic pulse events decreases rather than increases, which indicates that proton heating inside the Alfvenic pulses is not caused by adiabatic compression, but is probably generated by non-adiabatic heating caused by field-particle interaction. Accordingly, the proton fluid entropy inside the Alfvenic pulses is higher than that in the ambient solar wind. In the second part, we perform a test-particle simulation to explore how magnetic Alfvenic pulses affect their energization. We introduce square waves to imitate recurrent Alfvenic pulse intervals and their ambient quiet intervals between which fluctuating magnetic field have different angles. Besides, the Boris algorithm is employed to advance the movement of test-particles in the time-varying electromagentic fields. We report the following three findings after analyzing the simulation results. (1) When the amplitude of simulated Alfvenic pulse increases, the heating effect of test-particles is more prominent. (2) The velocity distribution of test-particles is temporarily modulated by the encouter of Alfvenic pulse interval. (3) Preferential perpendicular heating of test-particles can be observed.


ST14-A023
The First Flare Observation with a New Solar Microwave Spectrometer Working in 35–40 GHz

Zhao WU+, Fabao YAN, Yao CHEN#, Ziqian SHANG, Bing WANG, Lei ZHANG
Shandong University

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 cross-calibrate. 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 NoRP-CBS 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 (Itt4.8) 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-A024 | Invited
Nature of Intermittent Structures and Their Effect on Power Spectra of Solar Wind Fluctuations

Xin WANG#+
Beihang University

Intermittent structures are ubiquitous in the solar wind turbulence, and they can significantly affect the power spectral index of magnetic field fluctuations which reflects the cascading process of the turbulence. However, the nature of them and an analytical relationship between intermittency level and the magnetic spectral index have not been shown yet. Here we classify the magnetic intermittent structures mainly into three types depending on the profiles of time series of partial variance increments of magnetic vectors, and present the continuous variation of the magnetic spectral index in the inertial range as a function of the intermittency level. The measurements from the Parker Solar Probe during its first two orbits are used in this study. We calculate partial variance increments (PVI) of magnetic fluctuations, and consider the intervals that satisfy the condition |PVI(t)| > 3 as intermittent structures. Then the intermittent structures are classified into discontinuities, magnetic solitons, and magnetic vortex / wave packages according to the profiles of the time series of PVI. We find that at 0.17 AU, the three types of intermittency account for 43%, 32%, and 25%, respectively. We also establish an empirical relation between intermittent level and magnetic spectral index in the inertial range. The result will help us to know more details about the nature of intermittency in the near-Sun region, and the contributions of the intermittent structures on the magnetic power spectra.


ST14-A028 | Invited
Investigation of the Source Region of the Solar Wind Based on the CHASE Observations

Jie ZHAO1#+, Fu YU1,2, Shihao RAO3, Chuan LI3, Yang SU4, Hui LI1
1Chinese Academy of Sciences, 2University of Science and Technology of China, 3Nanjing University, 4Purple Mountain Observatory, CAS

The solar wind has been extensively studied recently with the in-situ observations from Parker Solar Probe (PSP), while its counterpart near the solar surface is rarely investigated and its initiation is still elusive. With the spectral observation from Chinese Hα Solar Explorer (CHASE) which is launched in 2021, the full-disk Doppler velocity is firstly obtained simultaneously. By investigating the statistics of the Doppler velocity at the chromosphere, we show the distributions in the coronal holes, which are easily determined from the dimming regions in AIA/193, and in the open regions, which are derived from PFSS extrapolation. We also investigated the footprints of the open field lines in the ecliptic plane. Our results indicate that the solar wind initiation may be highly associated with the layer of chromosphere and the different pattern of solar wind may already influenced by the solar atmosphere at the chromospheric layer in a complicated way.


ST14-A010
Higher-order Turbulence Statistics in the Sub-Alfvénic Solar Wind Observed by Parker Solar Probe

Jian ZHANG+, Shiyong HUANG#, Zhigang YUAN, Kui JIANG, Sibo XU, Yunyun WEI, Qiyang XIONG, Zhao WANG, Lin YU, Rentong LIN
Wuhan University

Parker Solar Probe has been the first spacecraft to enter the deep corona below the Alfvén critical point. Here we examine the higher-order statistical properties of magnetic-field fluctuations in the sub-Alfvénic solar wind and compare the results with the neighboring super-Alfvénic region. The intermittency and multifractal properties are analyzed by inspecting the probability density functions, the scale-dependent kurtosis and fractal spectrum of magnetic-field fluctuations. It is found that the magnetic-field fluctuations present distinct intermittency and multifractal properties in the inertial range and the BR component reveals much higher intermittency and more asymmetrical multifractal spectrum than the other components. The non-Gaussian self-similarity of fluctuations of BR at larger scales has also been observed. Further comparative analysis shows that all the solar wind periods share nearly the same intermittency and multifractal features, and the only difference lies on that the fluctuations of the BT and BN components exist slight variations.


Thu-03 Aug | 3:30 - 5:15 | MR333
ST23 - Cme Initiation and Propagation Through the Heliosphere

Session Chair(s): Yuming WANG, University of Science and Technology of China

ST23-A001
Investigating Pre-eruptive Magnetic Properties at the Footprints of Erupting Magnetic Flux Ropes

Wensi WANG1#+, Jiong QIU2, Rui LIU1, Qiang HU3, Yuming WANG1
1University of Science and Technology of China, 2Montana State University, 3The University of Alabama in Huntsville

It is well established that solar eruptions are powered by free magnetic energy stored in the current-carrying magnetic field in the corona. It has also been generally accepted that magnetic flux ropes (MFRs) are a critical component of many coronal mass ejections. What remains controversial is whether MFRs are present well before the eruption. Our aim is to identify progenitors of MFRs, and investigate pre-eruptive magnetic properties associated with these progenitors. Here we analyze 28 MFRs erupting within 45 deg from the disk center from 2010 to 2015. All MFRs' feet are well identified by conjugate coronal dimmings. We then calculate the magnetic properties at the feet of the MFRs, prior to their eruptions, using Helioseismic and Magnetic Imager vector magnetograms. Our results show that only 8 erupting MFRs are associated with significant nonneutralized electric currents, 4 of which also exhibit pre-eruptive dimmings at the footprints. Twist and current distributions are asymmetric at the two feet of these MFRs. The presence of pre-eruption dimmings associated with nonneutralized currents suggests the pre-existing MFRs. Furthermore, the evolution of conjugate dimmings and electric currents within the footprints can provide clues about the internal structure of MFRs and their formation mechanism.


Thu-03 Aug | 3:30 - 5:15 | MR334
ST21 - General Session in Solar and Terrestrial Sciences Including Space Weather

Session Chair(s): Kyoko WATANABE, National Defense Academy of Japan

ST21-A005
A Fresh Look at the Intensity and Impulsive Strength of Geomagnetic Storms Having Positive MPO

Balan NANAN#+, Manu VARGHESE, Qing-He ZHANG, Zanyang XING
Shandong University

We notice that the values of the SymH and Dst indices during the main phase (MP) and recovery phase (RP) of the geomagnetic storms having positive main phase onset (MPO) are significantly less than their actual values. We correct the inconsistency in 391 such storms (out of 596 storms) in the 1-minute resolution SymH index available since 1981 by raising the 0-level of SymH to the MPO-level. The corrected/revised storm intensity (SymHMin) and impulsive strength (IpsSymH) increase by up to -149 and -136 nT, respectively. The correction seems important for studying all aspects of global space weather. For example, the revised IpsSymH clearly identifies all three severe space weather (SvSW) events that caused power outage and six extreme space weather (ESW) events that caused minor system damages since 1981 from 577 normal space weather (NSW) events not causing such severe effects with a large separation of 31 nT. The correction also helps understand the high geo-effectiveness of the second of the super double storms.


ST21-A031
Extreme Value Analysis for Hazardous Extreme Geomagnetic Storms Based on the Mean Value of Dst Index During the Main Phase

Lihui CHAI#+
Institute of Geology and Geophysics, Chinese Academy of Sciences

Estimating the probability of the hazardous geomagnetic storms is important to modern human society, since the geomagnetic storms have potential to disrupt or damage the navigation and communication systems that the modern human society relies on. A new index IpsDst, defined as the mean value of the index Dst during the main phase of geomagnetic storms, is found to be more indicative of the hazard of the geomagnetic storms than the commonly-used index Dst. Thus, we use the new index IpsDst from 1957 to 2016, instead of the commonly-used Dst minimum, to estimate the probability of the hazardous geomagnetic storms by employing the extreme value theory. Our results show the shape parameter is negative, which indicates that the IpsDst has an upper bound, and then the occurrence possibility and the return level of the hazardous geomagnetic storms are calculated. The return level of the Quebec event is about 312 years, which indicates that the Quebec-like event is very rare. The return level of the events on Nov 06, 2001 and Oct 30, 2003 (Halloween event) is about 1 to 2 decades, which indicates that we should take precautions for these kind of events. The difference between our results and previous results based on Dst minimum are also discussed.


ST21-A016
NASA’s Geospace Dynamics Constellation (GDC) Mission: A Multi-spacecraft Mission to Explore the Ionosphere-thermosphere

Douglas ROWLAND1#+, Larry KEPKO2, Jared BELL1, Laila ANDERSSON3, Daniel GERSHMAN1, Mehdi BENNA1, Mark MOLDWIN4, Phillip ANDERSON5
1NASA Goddard Space Flight Center, 2National Aeronautics and Space Administration, 3University of Colorado Boulder, 4University of Michigan, 5The University of Texas at Dallas

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 by the end of the decade, 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.


ST21-A015
Dynamics of Low Frequency Oscillations of the Magnetic Field and Ion Flux Upstream of the Interplanetary Shock

Natalia BORODKOVA1#+, Olga SAPUNOVA2, Yuri YERMOLAEV1, Georgy ZASTENKER2
1Space Research Institute of the Russian Academy of Sciences, 2Russian Academy of Sciences

The structure of several fronts of quasi-perpendicular interplanetary collisionless shocks with low Mach number and low beta was studied using the data of the BMSW plasma spectrometer onboard the Spektr-R supplemented by magnetic field measurements. The main attention was paid to the trains of coherent oscillations of both the ion flux and the magnetic field, extending upstream from the shock ramp and are low-frequency (<10 Hz) magnetosonic whistler waves. It was shown that trains of magnetic field oscillations propagate at angles from 20 to 40 degrees with respect to the upstream average magnetic field and at angles of 40-50 degrees from the shock normal vector. They are right-hand polarized with respect to the magnetic field in the spacecraft reference frame. An analysis of the oscillations of the ion flux upstream of the ramp showed that they were elliptically polarized, have both left and right polarizations, and propagated at small angles with respect to the shock normal direction. With approaching the ramp, the frequency of oscillations in the trains of both the magnetic field and the ion flux increases, and the angle between the direction of train propagation and the magnetic field vector also increases A comparison of the trains of oscillations in the magnetic field generated by different parts of the ramp of the same shock was made. Based on the analysis of three cases, it was shown that trains of magnetic field oscillations propagating from different parts of the ramp have different angles with respect to the upstream magnetic field, which is connected with the nonstationarity and reformation of the shock front. This work was partially supported by the Russian Science Foundation, grant N. 22-12-00227.


ST21-A006
Magnetic Perturbations in Electron Phase-space Holes: Contribution of Electron Polarization Drift

Fan YANG1+, Xuzhi ZHOU1#, Yan ZHUANG1, Chao YUE1, Qiugang ZONG1, Zhiyang LIU1, Anton ARTEMYEV2
1Peking University, 2University of California, Los Angeles

Electron phase-space holes are a type of Debye-scale structures commonly observed in space plasmas, characterized by localized electrostatic potentials. Recent observations show that these structures are often accompanied by localized magnetic field perturbations. Sources of these magnetic perturbations have been considered to contain Lorentz transformation of electric field under high propagation velocity, as well as localized currents such as electron ExB currents. Here we consider the contribution of electron polarization drift to the current and then the magnetic field perturbations, validated by a comparison to MMS observations of 69 electron holes based on a superposed epoch technique. Our results show that polarization drift induced magnetic perturbations can be significant compared to the Lorentz transformation effect, especially in regions with low magnetic strength and large electron density.


ST21-A009
In Situ Observation of a Magnetopause Indentation That is Correspondent to Throat Aurora and is Caused by Magnetopause Reconnection

Huixuan QIU+, Desheng HAN#
Tongji University

Throat auroras have been suggested to correspond to magnetopause indentations, but how such indentations can be generated is an open question. Using coordinated magnetopause in situ and two-dimensional auroral imaging observations, we showed that a transient magnetopause crossing observed by THEMIS near the dayside magnetopause corresponds to a throat aurora observed by DMSP/SSUSI. The magnetopause crossing was confirmed to present a localized magnetopause indentation rather than arise from motion of the whole magnetopause. Using the minimum variance analysis and Walén test methods, we captured clear reconnection signatures at either boundary of the indentation. Also, an upstream solar wind discontinuity and a magnetosheath variation were identified to correlate well with the magnetopause indentation occurrence. These observations suggest that the magnetopause indentation was generated by reconnection and lend solid support to an assumption that throat aurora is produced by a particular reconnection that can develop inward the magnetosphere at a much-localized region.


ST21-A036
Inter-hemispheric Asymmetries of Energy Input Into the Magnetosphere-ionosphere System During Magnetic Storms: Poynting Flux and Particle Precipitation

Denny OLIVEIRA1,2#+, Eftyhia ZESTA1, Kevin DELANO1, John DORELLI1, Daniel GERSHMAN1, Mark MOLDWIN3
1NASA Goddard Space Flight Center, 2University of Maryland, Baltimore County, 3University of Michigan

We present a two-decade study with DMSP observations of magnetospheric energy input into the magnetosphere-ionosphere (MI) system during magnetic storms with different intensities for interhemispheric comparisons. DMSP observations are for Poynting flux, electron precipitation, and proton precipitation, all with resolution of 1 second. A smoothing Savitzky-Golay filter is applied to all the data to eliminate possible biases caused by data spikes. More than 300 magnetic storms are grouped with respect to storm intensity (weak to extreme), seasons, and local time. Our data only comprise simultaneous observations in both hemispheres for all events to allow for a more concise inter-hemispherical comparison of the results (“bow-tie” diagrams). We report that climatological studies, i.e., long-term observations, show that the northern hemisphere has a slight preference to receive magnetospheric energy during storms in comparison to the southern hemisphere. This result is consistent with previous observations, but the level of preference here is lower than what has been reported before. We also show that such slight symmetry is broken when short term drivers (IMF By and local time variations), and mid-term variations (seasons and solar cycle), act upon the magnetosphere-ionosphere system. Some implications for the future NASA’s GDC (Geospace Dynamics Constellation) mission will be presented as well.


Fri-04 Aug | 8:15 - 10:00 | MR333
ST23 - Cme Initiation and Propagation Through the Heliosphere

Session Chair(s): Prasad SUBRAMANIAN, Indian Institute of Science Education and Research, Pune

ST23-A008 | Invited
New Insights Into the Initiation and Propagation of Coronal Mass Ejections

Nat GOPALSWAMY#+
NASA Goddard Space Flight Center

Coronal mass ejections (CMEs) are the most energetic phenomena in the heliosphere and are of interest from the science and application points of view. Although we know CMEs originate from closed magnetic regions on the Sun (active regions, quiescent filament regions), we do not fully understand how they are initiated. The current paradigm is that in the source region, a seed flux rope is in equilibrium located above the polarity inversion line. The seed flux rope can be cold as in the case of filament regions or hot flux ropes often observed in EUV. Due a trigger such as an emerging flux, the flux rope loses equilibrium and rises due to an instability such as the torus instability. The rise results in the so-called flare reconnection that fattens the seed flux rope by adding poloidal flux to it. Simultaneously formed in the source active region is the post eruption arcade. When the reconnection ends, the flux rope becomes mature and cruises into the interplanetary medium. The propagation effects include one or more of drag, deflection, rotation, flux erosion, expansion, and interaction with other large-scale structures. This talk illustrates these processes using specific examples.


ST23-A010 | Invited
Predicting CMEs' Arrival at Earth with Machine Learning Methods

Jiajia LIU1#+, Yimin WANG2, Simone CHIERICHINI3, Yudong YE4, Robertus ERDELYI3, Yuming WANG1, Marianna KORSOS5, Chenglong SHEN1
1University of Science and Technology of China, 2Qingdao University of Science and Technology, 3The University of Sheffield, 4Sun Yat-sen University, 5University of Catania

Coronal Mass Ejections (CMEs) are one of the most violent eruptions in the Solar System. CMEs can cause severe disturbances in interplanetary space and even affect human activities in many respects, causing damage to infrastructure and losses of revenue. Fast and accurate prediction of CMEs' arrival at Earth, as well as their arrival time, is then vital to minimize the disruption CMEs may cause when interacting with geospace. In this talk, I will summarize the series of work we have done in the past few years in predicting CMEs' arrival at Earth with Machine Learning methods, including SVM, Random Forest, XGBoost and Convolutional Neural Networks. Our results indicate that Machine learning methods are promising in realizing fast and accurate space weather forecasts.


ST23-A006
Study of CME and SIR Interaction Using SWASTi Framework

Prateek MAYANK1#+, Bhargav VAIDYA1, Wageesh MISHRA2, Dibyendu CHAKRABARTY3
1Indian Institute of Technology Indore, 2Indian Institute of Astrophysics, 3Physical Research Laboratory

Coronal Mass Ejections (CMEs) are the central component of solar eruptions. And solar wind streams, acting as a background, govern their propagation in the heliosphere and drive geomagnetic storm activities. Understanding the effect of ambient solar wind on CME evolution is therefore essential to accurately compute its arrival time and thus mitigate its impact. To comprehend the evolution of CME structure in the inner heliosphere, several qualitative studies have been done. However, the quantitative understanding of these interactions and their effect on the evolution of CMEs is still lacking. The quantitative study of CME evolution requires the absolute isolation of CME structure from ambient solar wind. And with the current observational and simulation techniques, it is very challenging to accomplish this. Here, we propose a unique method for isolating the CME structure in the heliosphere and analyzing its interaction with stream/corotating interaction regions (SIR/CIR). We will demonstrate a newly developed MHD CME model, SWASTi-CME, which is based on the PLUTO code. To rightfully study the interaction of CME with SIR and analyze its effect on CME evolution, we established two setups. The first setup (real case) is the default setup of the SWASTi-CME flux rope model, whereas the second setup (ideal case) is a hypothetical case where solar wind is constant everywhere initially; as a result, there’s no SIR formation in the ideal case. And to quantify the deviation in CME properties due to SIR/CIR, the ideal case is treated as a reference, and the real case results are compared with them. We will present the results of our study and discuss the qualitative and quantitative analysis of i) deformation of the CME front, ii) volumetric evolution, iii) thermal, kinetic, and magnetic pressure evolution, and iv) drag force on the CME.


Fri-04 Aug | 8:15 - 10:00 | MR334
ST03 - Recent Advance in Understanding Ionospheric Disturbances and Irregularities Link to Waves from Below

Session Chair(s): Charles LIN, National Cheng Kung University

ST03-A005 | Invited
Upward Propagation of Gravity Waves and Ionospheric Perturbations Triggered by the 2022 Hunga-Tonga Volcanic Eruption

Yasunobu MIYOSHI1#+, Hiroyuki SHINAGAWA2
1Kyushu University, 2National Institute of Information and Communications Technology

On 15th January 2022, the Hunga Tonga-Hunga Ha'apai volcano erupted at about 04:15 UT. After the eruption, Large-amplitude Lamb waves and traveling ionospheric disturbances (TIDs) are observed. In this study, using an atmosphere-ionosphere coupled model (GAIA), atmospheric and ionospheric perturbations triggered by the 2022 Hunga-Tonga volcanic eruption are investigated. In order to examine Lamb and gravity waves associated with the Hunga-Tonga eruption, GAIA with a higher horizontal resolution (about 1degree longitude by 1degree latitude) is used. Our result shows that ionospheric perturbations are caused by neutral wind perturbations associated with gravity waves. Gravity waves with fast horizontal phase speeds of 200-310 m/s are excited in the troposphere near the Hunga-Tonga volcano, and propagate upward into the thermosphere. The amplitude of the eruption-generated gravity waves is small in the troposphere (~1 m/s), and grows exponentially with height because of the exponential decrease of the density, reaching 60‒80 m/s at 300 km height. TIDs are excited by the eruption-generated gravity waves propagating from the troposphere into the thermosphere. We can conclude that the eruption-generated gravity waves whose horizontal phase velocity is close to the sound speed play an important role in thermospheric and ionospheric perturbations after the Hunga-Tonga volcano eruption. Furthermore, the geomagnetic variation triggered by the Hunga-Tonga eruption is discussed.


ST03-A011
Observations of Super Plasma Bubbles Over Asia-pacific Region Triggered by Tonga Volcano Eruption

P. K. RAJESH1#+, Charles LIN1, Jia-Ting LIN1, Shih-Ping CHEN1, Chi-Yen LIN2, Jann-Yenq (Tiger) LIU2, Min-Yang CHOU3, Jia YUE3
1National Cheng Kung University, 2National Central University, 3NASA Goddard Space Flight Center

This study examines the extreme plasma bubble activity over Asia-Pacific region (100-150°E) triggered by the Tonga volcano eruption on 15 January 2022 during the recovery phase of a moderate geomagnetic storm by using ground-based Global Navigation Satellite System (GNSS) total electron content (TEC) measurements, in situ ion density observations by ion velocity meter (IVM) onboard the FORMOSAT-7/COSMIC-2 (F7/C2), and global ionosphere specification (GIS) three-dimensional (3D) electron density profiles constructed by using by using the F7/C2 Tri-GNSS radio occultation system (TGRS) as well as ground-based GNSS slant TECs. The IVM and rate of TEC index (ROTI) observations over the Asia-Pacific region revealed super plasma bubbles, expanding to geomagnetic latitudes beyond 30° in the conjugate hemispheres, attaining apex altitudes over 3000 km. This was preceded by a sharp decrease of equatorial ionization anomaly (EIA) crest density and an unusually strong pre-reversal enhancement (PRE) of low latitude ionosphere as seen from the GIS electron density maps. The enhanced F-region wind over EIA by the negative storm, when combined with volcano induced perturbations, apparently intensified the PRE and generated suitable conditions for super plasma bubbles. In presence of the strong PRE, seed perturbations from volcano induced variations triggered the super plasma bubble activity.


ST03-A002 | Invited
Recent Advances in the Study of EPBs in East and Southeast Asia Based on the IONISE and LARID Observations

Guozhu LI1#+, Lianhuan HU1, Wenjie SUN1, Xiukuan ZHAO1, Haiyong XIE2, Baiqi NING1
1Chinese Academy of Sciences, 2Institute of Geology and Geophysics, Chinese Academy of Sciences

Equatorial plasma bubbles (EPBs) are known to be initiated at ionospheric F region bottomside around magnetic equator. EPBs can drift zonally more than 2000 km and extend along magnetic field lines to low- even middle-latitudes of 40° or higher under some conditions. In the east and southeast Asia, there exist significant differences in the generation rates of EPBs at closely located stations, indicating that the decorrelation distance of EPB generation is small in longitude. Identifying the possible seeding sources for EPBs and accurately predicting their occurrence, especially when the onset locations of EPBs are far outside the observation sector, is still a difficult task. To capture ionospheric disturbances of various scales by natural sources and reveal their possible seeding in the generation of EPBs, an Ionospheric Observation Network for Irregularity and Scintillation in the East and southeast Asia (IONISE), together with a Low lAtitude long Range Ionospheric raDar (LARID) supported by the Chinese meridian project phase II are being developed. In this talk we will briefly review the current knowledge of EPBs in the east and southeast Asia. Some recent results on the initial generation and evolution of EPBs from IONISE and LARID will be presented. Some unresolved issues related to the day-to-day variability of EPBs will be discussed.


ST03-A015
When Traveling Ionospheric Disturbances Meet with Equatorial Plasma Bubbles

Charles LIN1#+, Min-Yang CHOU2, Shih-Ping CHEN1, Joseph HUBA3, P. K. RAJESH1, Jong-Min CHOI1
1National Cheng Kung University, 2NASA Goddard Space Flight Center, 3Synteck Technologies

There are observations of suppresion of the equatorial plasma bubbles (EPBs) due to the nighttime medium-scale traveling ionospheric disturbances (MSTIDs), and the extreme poleward extension of EPBs after arrival of the TIDs driven by the 2022 Tonga volcano eruption. To understand their underlying interactions theorectically, the Naval Research Laboratory first-principles ionosphere model SAMI3/ESF is performed to study the two coupling effects. For the interactions between MSTIDs and EPBs, the synthetic dynamo currents are imposed into the potential equation to induce polarization electric fields for generating the MSTIDs. Simulations demonstrate that the MSTIDs can inhibit the upward growth of EPBs; however, MSTIDs alone are insufficient to explain the disappearance of EPBs. We found that the meridional winds likely contribute to the disappearance of MSTIDs by reducing the background electron density and polarization electric fields within the EPBs. Then, the MSTIDs transport plasma to fill the EPB depletions up via E × B drifts. Both MSTIDs and meridional winds are necessary to comprehend the underlying mechanism of EPB disappearance. Additionally, we also found that the zonal and vertical E × B drifts within the MSTIDs affect the morphology of EPBs, leading to a reverse-C shape structure. For the extreme EPBs during volcano eruption, the TIDs play the role of accelerating growth of EPBs at the seeding phase. It also requires strong uplift of the ionospheric layer in order to accelerate upward/poleward extension of EPBs over 2500 km or to mid-latitude. This theoretical study help understand the role of TIDs in generation of EPBs.


ST03-A004
Modeling the Day-to-day Variability of Midnight Equatorial Plasma Bubbles with SAMI3/WACCM-X

Min-Yang CHOU1#+, Jia YUE1, Fabrizio SASSI1, Joseph HUBA2, Sarah MCDONALD3, Jennifer TATE4, Nicholas PEDATELLA5, Cora RANDALL6, V. Lynn HARVEY6
1NASA Goddard Space Flight Center, 2Synteck Technologies, 3Naval Research Laboratory, 4Computational Physics, Inc., 5National Center for Atmospheric Research, 6University of Colorado Boulder

It is well-known that equatorial plasma bubbles (EPBs) are highly correlated to the post-sunset rise of the ionosphere on a climatological basis. However, when proceeding to the daily EPB development, what controls the day-to-day/longitudinal variability of EPBs remains a puzzle. In this study, we investigate the underlying physics responsible for the day-to-day/longitudinal variability of EPBs using the Sami3 is A Model of the Ionosphere (SAMI3) and the Whole Atmosphere Community Climate Model with thermosphere-ionosphere eXtension (WACCM-X). Simulation results on October 20, 22, and 24, 2020 were presented. SAMI3/WACCM-X self-consistently generated midnight EPBs on October 20 and 24, displaying irregular and regular spatial distributions, respectively. However, EPBs are absent on October 22. We investigate the role of gravity waves on upwelling growth and EPB development and discuss how gravity waves contribute to the distributions of EPBs. Of particular significance is that we found the westward wind associated with solar terminator waves and gravity waves causes midnight vertical drift enhancement and collisional shear instability, which provides conditions favorable for the upwelling growth and EPB development. The converging and diverging winds associated with solar terminator waves and midnight temperature maximum also affect the longitudinal distribution of EPBs. The absence of EPBs on October 22 is related to the weak upward drift due to weak westward wind associated with solar terminator waves.


ST03-A006 | Invited
Post-sunrise Traveling Ionospheric Disturbance Observations Using the Millstone Hill Incoherent Scatter Radar and GNSS Receiver Networks

Shunrong ZHANG#+, Philip ERICKSON, Anthea COSTER, Ercha AA
Massachusetts Institute of Technology

Traveling ionospheric disturbances result from forcing both "above" and "below." The "above" forces are linked to solar and interplanetary disturbances, while the "below" forces are related to lower atmospheric and lithospheric processes. The solar terminator offers a potential source of predictable and recurring gravity waves and TIDs. Previous studies have confirmed the existence of these neutral and ionospheric perturbations that are associated with the terminator. However, it is noteworthy that these atmospheric waves tend to propagate primarily in a zonal direction, perpendicular to the terminator. This means that the UxB force is expected to generate electric fields that are embedded within those TIDs/GWs. To study the vertical propagation of TIDs/GWs and the polarization electric fields associated with them, we conducted experiments using the Millstone ISR. Our results revealed that oscillating zonal ion drifts in the F region, which are equivalent to meridional electric fields, were present during morning hours when TIDs in electron density showed a downward progression in the vertical direction. Furthermore, we performed a long-term analysis of TIDs using GNSS receiver networks over the continental US, with a particular focus on sunrise TIDs. Our statistical outcomes indicate that these sunrise TIDs play a significant role in daytime ionospheric variability.


ST03-A013
Nighttime Ionospheric Disturbances and Irregularities Induced by Solar Eclipse

Yang-Yi SUN1#+, Jin WANG2, Chieh-Hung CHEN1, Tianya LUO3
1China University of Geosciences, 2China University of Geosciences (Wuhan), 3Guangxi Transportation Science and Technology Group CO., LTD.

A solar eclipse is a daytime phenomenon that significantly disturbs the atmosphere and ionosphere and induces irregularities during the moon obscuration. Significant atmospheric changes can trigger gravity waves that propagate upward and cause disturbances and irregularities during the obscuration. However, the nighttime disturbances and irregularities that occur after a solar eclipse are unclear. In this study, we examined the occurrence and development of disturbances and irregularities in the nighttime due to the solar eclipse on 21 June 2020. We analyzed the dense ground‐based Global Navigation Satellite System (GNSS) total electron content (TEC) data, the critical frequency of the ionospheric F2 layer (foF2) and its height (hmF2) recorded by the ionosondes data in East Asia during and after the solar eclipse occurred at June solstice. In the results, the eclipse induced not only a major daytime depression but also nighttime perturbations in the ionosphere. The TEC perturbed intermittently from noon to midnight between 80° and 150°E on the eclipse day. The perturbations behave as terminator wave that propagates in a northwestward direction after sunset. The ionosonde observations observed the pre-reversal enhancement that surprisingly occurred in its unfavorable growing season at the June solstice during solar minimum. On the other hand, the rate of TEC index (period < 5 min) indicates the occurrence of irregularities that evolve from the large or coarse structures with a period ranging from hours to dozens of minutes in the nighttime due to the eclipse. The adaptive analysis exposes the temporal and spatial evolutions of the irregularities from larger structures continuously. The ionosondes observations show the spread F that correspondents to the irregularities. The effects of thermal convergence on the ionosphere can be attributed to the development of nighttime disturbances and irregularities.


Fri-04 Aug | 10:20 - 12:20 | MR333
ST01 - Particle Acceleration and Transport at the Sun and in the Heliosphere

Session Chair(s): Linghua WANG, Peking University

ST01-A021 | Invited
Status and Early Results of ASO-S/HXI

Yang SU1#+, Wei CHEN2, Zhe ZHANG2, Fanxiaoyu XIA2, Yiming HU2, Dengyi CHEN2, Yan ZHANG2, Fu YU2,3, Wei LIU2, Jian WU2, Yu HUANG2, Yongqiang ZHANG2, Mingsheng CAI2, Zhentong LI2, Youping LI2, Weiqun GAN2
1Purple Mountain Observatory, CAS, 2Chinese Academy of Sciences, 3University of Science and Technology of China

The Hard X-ray Imager (HXI) on board the Advanced Space-based Solar Observatory (ASO-S) is an instrument designed to observe spectra and images of X-ray bursts in solar flares. HXI has 91 sub-collimators to modulate X-rays and obtains 45 visibilities. The energy range for imaging is ~15 keV- 300 keV. The highest spatial resolution is ~3.1 arcsec and the highest time resolution is 0.125 s during burst mode. HXI was launched on 9 Oct. 2022 and powered up on 17 Oct. 2022. After the in-orbit testing phase lasting for about four months, HXI is now in regular observation mode. More than 100 flares have been observed. The reconstructed images reveal interesting and fine structures of solar hard X-ray sources. More importantly, HXI and Solar Orbiter/STIX provide us, for the first time, HXR images of solar flares from two different viewing angles, which is particularly important for understanding HXR directivity and flare-accelerated electrons. A brief introduction of HXI payload, the status of the instrument, the cross-calibrations between HXI and STIX, and early results will be presented in this talk.


ST01-A022
Numerical Modeling of Energetic Electron Acceleration, Transport, and Emission in Solar Flares: Connecting Looptop and Footpoint Hard X-ray Sources

Xiangliang KONG1#+, Bin CHEN2, Fan GUO3, Chengcai SHEN4, Xiaocan LI5, Jing YE6, Lulu ZHAO7, Zelong JIANG1, Sijie YU2, Yao CHEN1, Joseph GIACALONE8
1Shandong University, 2New Jersey Institute of Technology, 3Los Alamos National Laboratory, 4Harvard-Smithsonian Center for Astrophysics, 5Dartmouth College, 6Yunnan Observatories, 7University of Michigan, 8The University of Arizona

The acceleration and transport of energetic electrons during solar flares is one of the outstanding topics in solar physics. Recent X-ray and radio imaging and spectroscopy observations have provided diagnostics of the distribution of nonthermal electrons and suggested that, in certain flare events, electrons are primarily accelerated in the loop top and likely experience trapping and/or scattering effects. By combining the focused particle transport equation with MHD simulations of solar flares, we present a macroscopic particle model that naturally incorporates electron acceleration and transport. Our simulation results indicate that physical processes such as turbulent pitch-angle scattering can have important impacts on both electron acceleration in the loop top and transport in the flare loop, and their influences are highly energy-dependent. A spatial-dependent turbulent scattering with enhancement in the loop top can enable both efficient electron acceleration to high energies and transport of abundant electrons to the footpoints. We further generate spatially resolved synthetic HXR emission images and spectra, revealing both the loop-top and footpoint HXR sources. Similar to the observations, we show that the footpoint HXR sources are brighter and harder than the looptop HXR source. We suggest that the macroscopic particle model provides new insights into understanding the connection between the observed loop-top and footpoint nonthermal emission sources by combining the particle model with dynamically evolving MHD simulations of solar flares.


ST01-A023
Numerical Modeling of the Transport of Energetic Protons in the Sustained Gamma-ray Flare on 2014 September 1

Zelong JIANG1#+, Xiangliang KONG1, Fan GUO2, Meng JIN3, Yao CHEN1
1Shandong University, 2Los Alamos National Laboratory, 3Lockheed Martin Advanced Technology Laboratories

Fermi/LAT has detected more than 30 solar flare events with delayed >100 MeV gamma-ray emission beyond the impulsive phase, known as long-duration gamma-ray flares or sustained gamma-ray flares. The gamma-ray emission is believed to be produced by the nuclear reaction between high-energy protons with energies >300 MeV and the solar atmosphere, but the origin of these high-energy protons remains elusive, either from direct flare acceleration or accelerated by the CME-driven shock. The gamma-ray flare event on 2014 September 1 lasted about 2 hours, far exceeding the flare impulsive phase, and the gamma-ray emission region is located away from behind-the-limb flare site. Therefore, a possible explanation is energetic protons are accelerated at the CME-driven shock and then they propagate from the shock back to the solar surface to produce the gamma-ray emission. In this work, we numerically model the transport of energetic protons by combining the particle transport model with data-driven MHD simulation of the solar eruption for the 2014 September 1 event. We find that the position of precipitated protons on the solar surface is close to that of the gamma-ray emission region, and the energy spectrum and fraction of precipitated protons are consistent with the observations. Our simulation results indicate that >300 MeV protons accelerated at the CME-shock may explain the gamma-ray emission in this event.


ST01-A025 | Invited
Multi-spacecraft Observations of Energetic Particle Events from 0.3 to 1.0 Au

George HO1#+, Glenn MASON2, Robert ALLEN2, Robert WIMMER-SCHWEINGRUBER3, Javier RODRIGUEZ-PACHECO4, Raul GOMEZ-HERRERO4
1Southwest Research Institute, 2Johns Hopkins University Applied Physics Laboratory, 3University of Kiel, 4University of Alcalá

The propagation and radial evolution of solar energetic particle (SEP) events can only be studied by multiple-point simultaneous in-situ measurement within the heliosphere. The joint ESA/NASA Solar Orbiter mission that was launched in February 2020, is designed to study the Sun and inner heliosphere in greater detail than ever before. The Energetic Particle Detector (EPD) investigation on Solar Orbiter is a suite of four different sensors that measure the energetic particles from slightly above solar wind energies to hundreds of MeV/nucleon. Since launched, EPD already observed numerous large SEP events inside of 1 au in greater temporal and spectral resolutions than ever before. Many of these events were also measured by spacecraft at 1 au such as ACE and/or STEREO. On April 2, 2022, an active region (AR 12975) on the western limb (W54) of the Sun produced a large SEP event and associated fast moving (>1300 km/s) coronal mass ejection (CME). During that time, the Solar Orbiter spacecraft was cruising near its perihelion distance (~0.35 au) at W109 relative to the Earth-Sun line, and the STEREO Ahead spacecraft was at E35. Together, the particle instruments on these probes measured the SEP and the plasma and field instruments detected the associated interplanetary shock/CMEs. In this paper, we report the multi-spacecraft observations of this and other events that were measured by Solar Orbiter, and we discuss the propagation and transport of SEPs from 0.3 to 1 au.


ST01-A013
Solar Energetic Electron Events with a Spectral Bump

Wenyan LI1#+, Linghua WANG1, Wen WANG2, Zixuan LIU1
1Peking University, 2National University of Defense Technology

The energy spectrum of solar energetic electron (SEE) events carries crucial information on the origin/acceleration of energetic electrons at the Sun. Using the Wind 3DP electron measurements at ~1 to 200 keV during 1995-2019, we select 11 good SEE events with a bump-like break in the peak flux vs. energy spectrum, different from the typical SEE events with a double-power-law spectrum. For the selected 11 events, the background-subtracted electron peak flux versus energy spectrum fits well to two functions: the sum of a single-power-law and a Gaussian function (spectral function #1) and the product of a single-power-law and the natural exponential form of a Gaussian function (spectral function #2). For the spectral function #1 (#2), on average, the fitted spectral index is 2.6±0.4 (2.7±0.6), significantly larger than the low-energy power-law index of typical SEE events, while the fitted center energy of spectral bump is 24±7 keV (75±38 keV) and the ratio of bump width and center is 2.0±0.7 (3.4±2.8). Among these 11 events, respectively, ~78%, ~89%, ~90%, 100% and ~55% are associated with GOES SXR flares, RHESSI HXR flares, west-limb CMEs, type III radio bursts and type II radio bursts. Thus, these bump events have a stronger association with flares, coronal mass ejections (CMEs) and type II radio bursts, compared to the typical SEE events. In addition, we find a positive correlation between the center energy of bump and the CME speed. Therefore, we come up with an acceleration picture of these bump SEE events: the power-law portion is probably accelerated by flares with the acceleration efficiency larger at lower energies, while the bump portion is likely accelerated in CME-related processes with the acceleration efficiency increasing with the CME speed.


ST01-A018 | Invited
Variability of Ionic Composition in Gradual Solar Energetic Particle Events and Shock Geometry

Nariaki NITTA1#+, Meng JIN2, Christina COHEN3
1Lockheed Martin Solar and Astrophysics Laboratory, 2Lockheed Martin Advanced Technology Laboratories, 3California Institute of Technology

It is generally thought that particles in the so-called gradual solar energetic particle (SEP) events are accelerated at shock waves driven by coronal mass ejections (CMEs) and that their ionic composition resembles that of the solar wind. However, some of gradual SEP events show enhancement of heavy ions such as iron. One theory links iron-rich gradual SEP events to quasi-perpendicular shocks, which may preferentially accelerate suprathermal particles from earlier or concomitant flares that already have flare-like abundance. It is difficult to test this hypothesis since the magnetic field of the corona is not directly observed on a routine basis, and CMEs and related structures are observed only in projection to the plane of the sky. Using a data-driven global MHD model AWSoM (Alfven-Wave Solar Model), we have simulated eight major eruptions that produced SEPs, and compared the shock angle with the Fe/O ratio in the 10-25 MeV/n range as observed at 20 locations that consist of L1 and STEREO-A/B. We do not find a strong correlation between iron-rich SEP events and quasi-perpendicular shocks beyond a marginal trend. We discuss the results including alternative possibilities for the variability of the ionic composition in gradual SEP events, and also give a warning as to how to interpret the simulation results that depend on the input magnetic maps.


ST01-A020
Investigation of the Alfven Wave Turbulence Effect on the Dynamics of a SEP Event Decay Phase

Valeriy TENISHEV#+, Igor SOKOLOV
University of Michigan

Understanding the radiation environment due to solar energetic particles in the heliosphere and the Earth’s magnetosphere is a challenging and practically important task. The most vulnerable are exploratory missions when outside of the Earth’s magnetosphere. In this work, we investigate the effect of pitch angle scattering on the decay phase of SEP events. We model the transport of solar energetic particles moving along magnetic field lines by solving the focused transport equation. These magnetic field lines extend to 5 AU to capture the effect of possible pitch angle scattering when energetic particles are beyond 1 AU. The latter could have a significant impact on the decay of a SEP event. Modeling the transport of SEPs is coupled with simulating the solar wind dynamics, interplanetary magnetic field, and parameters of the Alfven wave turbulence. This presentation discusses the integrated modeling approach employed in this study and the effect of pitch angle scattering at large heliocentric distances on the dynamics of the decay phase of SEP events.


Fri-04 Aug | 10:20 - 12:20 | MR334
ST03 - Recent Advance in Understanding Ionospheric Disturbances and Irregularities Link to Waves from Below

Session Chair(s):

ST03-A001
Contemporaneous Observations of Coupling from the Lower and Middle Thermosphere to the Topside Ionosphere via Ultra-fast Tropical Waves as Revealed by in Situ and Remotely-sensed Satellite Observations

Federico GASPERINI#+
Orion Space Solutions

Global-scale waves from the lower and middle atmospheric wave spectrum with periods between about 0.5 days to 10 days constitute a significant source of ionosphere-thermosphere (IT, 100-600 km) variability. Due to the geometry of magnetic field lines near the equator, much of this IT coupling occurs at low latitudes (<30°) and is driven by ultra-fast tropical waves (UFTW) excited by deep convective processes in the tropical troposphere. UFTW propagate upwards into the IT system generating electron density variability that translates to uncertainties in navigation and communications systems, and neutral density variability that translates to uncertainties in orbital and reentry predictions. Despite recent progress, many unresolved questions regarding the impacts from these waves on the low-latitude IT system exists. In this work, in-situ total ion densities from Ion Velocity Meter (IVM) instruments onboard the Ionospheric Connection Explorer (ICON), the Scintillation Observations and Response of the Ionosphere to Electrodynamics (SORTIE), the Constellation Observing System for Meteorology, Ionosphere, and Climate-2 (COSMIC-2), and the Defense Meteorological Satellite Program along with with remotely-sensed lower (ca. 105 km) and middle (ca. 200 km) horizontal neutral winds from ICON’s Michelson Interferometer for Global High-resolution Thermospheric Imaging (MIGHTI) instrument are used to study the role that UFTW play in dynamically coupling lower atmospheric variability with IT variability at low and middle latitudes during 2020-2022.


ST03-A010
Evidence for 2019 Southern Hemispheric SSW Triggered Q6DW-tide-GW Interactions Observed at 30ºS

Zishun QIAO1#+, Nicholas PEDATELLA2, Alan LIU1, Gunter STOBER3, Iain REID4,5, Javier FUENTES6, Chris ADAMI4
1Embry-Riddle Aeronautical University, 2National Center for Atmospheric Research, 3University of Bern, 4ATRAD Pty. Ltd., 5University of Adelaide, 6Gemini Observatory Southern Operations Center

Observations from CONDOR and Buckland Park meteor radar at 30ºS reveal that a strong westward propagating quasi-6-day wave with zonal wavenumber 1 is associated with the rare 2019 Southern Hemispheric Sudden Stratospheric Warming (SSW) and interacts with the diurnal tide and gravity waves. The diurnal tide is amplified every 6 days, and a 21h child wave occurs which could be attributed to the Q6DW-diurnal tide nonlinear interaction. Gravity wave (GW) variances computed by a recently developed 3DVAR algorithm appear to oscillate with a 4-6 days periodicity and might be responsible for the period and phase shift of Q6DW. Both of the 21h child wave and Q6DW-modulated GW could propagate vertically to the ionosphere and be responsible for producing the ionospheric 6-day periodicity. Enhancement observed in the first results of meteor radar observed Q6DW Eliassen-Palm flux agrees with SD-WACCM-X simulation, and may facilitate the global perturbation and persistence of the Q6DW. We conclude that observational confirmations of SSW triggered Q6DW-tide and Q6DW-GW interactions play an important role in the coupling between the ionospheric 6-day variability and the lower atmospheric forcing.


ST03-A017
Non-migrating Atmospheric Tides Shift and Deform the Ionospheric Current Over Asia

Pengyu ZHANG1+, Yang-Yi SUN2#
1China University of Geosciences,Wuhan, 2China University of Geosciences

It was known that the atmospheric tide is the main driver for the ionospheric current system. Changes in the thermospheric wind and ionospheric conductivity contribute to the variability of the current system. This study shows the analysis of observations of the geomagnetic field from ground-based magnetic observatories and the thermospheric horizontal wind from TIMED/TIDI over Asia and the investigation of the ionospheric dynamo process. We reconstructed the polarized current based on the estimated non-migrating tidal components. The superimposition of the polarized current and the basic vortex current is consistent with the equivalent current derived from ground-based geomagnetic field observation. The polarized current can shift and deform the Sq current vortex. The results also suggest that the variations in the magnetic field can be a way to reflect the tidal weather in the lower thermosphere.


Fri-04 Aug | 10:20 - 12:20 | MR334
ST15 - The New Frontier: Coordinated Multi-point Ground- and Space-based Observations of the Ionosphere and Thermosphere

Session Chair(s): Shasha ZOU, University of Michigan

ST15-A008 | Invited
Coordinated Investigations of the Global Ionosphere-Thermosphere System Through Data Assimilation and Numerical Modeling

Gang LU#+
National Center for Atmospheric Research

The ionosphere and thermosphere are closely connected with the magnetosphere above and the lower atmosphere below. Energy input from the magnetosphere via the high-latitude ionosphere plays a major role in regulating thermospheric dynamics and chemistry, especially during geomagnetic storms. Upward propagating atmospheric waves are another source of thermospheric/ionospheric variability, and their effects are more pronounced under quiet conditions but are overwhelmed by magnetospheric forcing under disturbed conditions. Joule heating and auroral precipitation are the two main forms of magnetospheric energy input. An accurate specification of high-latitude energy input is critically important to understanding how magnetospheric forcing affects the thermosphere. The specification of Joule heating and auroral precipitation requires global patterns of electric field or plasma convection and precipitating energy particles from the magnetosphere, which are traditionally obtained from statistical analysis of observations taken over a long period of time under similar geophysical conditions. Although statistical patterns describe the average behavior of ionospheric electrodynamics, they are often inadequate in representing real storm events. For that reason, advanced data assimilation techniques have been developed to synthesizing various ground and satellite observations during a real event. The Assimilative Mapping of Ionospheric Electrodynamics (AMIE) procedure is one of such tools. In this presentation, I will discuss the main features of AMIE as well as its potential utility for the upcoming GDC mission. I will also highlight how the more realistic AMIE patterns help improve the thermospheric response to storms in the Thermosphere-Ionosphere Electrodynamics General Circulation Model (TIEGCM) simulations.


ST15-A013 | Invited
ROKITS: Space-borne Wide-field Auroral/Airglow Imager

Woo Kyoung LEE1#+, Young-Sil KWAK1, Hyosub KIL2, Larry PAXTON2, Geonhwa JEE3, Sunghwan CHOI1, Kyoung-Min ROH1, Gwanghui JEONG4, J.-Y. PARK1, Dukhang LEE1, Jihun KIM1, Tae-Yong YANG1, Yunjong KIM1, Ji-Hye BAEK1, Jaeheung PARK1, Jong-Kyun CHUNG1
1Korea Astronomy and Space Science Institute, 2Johns Hopkins University Applied Physics Laboratory, 3Korea Polar Research Institute, 4AntBridge

The Republic Of Korea Imaging Test System (ROKITS) is a wide-filed auroral/airglow imager being developed by the Korea Astronomy and Space Science Institute. ROKITS will be on board in Compact Advance Satellite 500– 3, launched in 2025. The orbit altitude is 600 km with an inclination of 98° (LTAN: 12:30 PM). ROKITS has three cameras; two main cameras with a narrow bandpass filter (3nm, FWHM), and one auxiliary camera without a filter. Main cameras observe aurora and airglow emissions at two spectral bands (OI 557.7 nm and OI 630.0 nm), respectively. The field of view of each camera is 90°, so the imaging swath is over 700 km. The main scientific objective of ROKITS is to identify the boundary of the auroral oval and auroral shapes. Comparing the ROKITS observations with the FUV airglow observations by DMSP/SSUSI will allow us to investigate the similarity/difference of the auroral boundary and fine auroral structures between visible and FUV wavelengths. We will also assess ROKITS observations by coordinating coincident ground-based observations of aurora using all-sky imagers in collaboration with the Korea Polar Research Institute. We also expect that the measurement of OI 557.7 nm emission provides information on atmospheric gravity waves, which is meaningful as detecting atmospheric gravity waves from space.


ST15-A004 | Invited
Interaction Between Nighttime MSTID and Mid-latitude Field-aligned Plasma Depletion Structure: First Results from Hanle, India

Sumanta SARKHEL1#+, Virendra YADAV2, Rahul RATHI1, Dibyendu CHAKRABARTY3, M. V. SUNIL KRISHNA1
1Indian Institute of Technology Roorkee, 2Aryabhatta Research Institute of Observational Sciences, 3Physical Research Laboratory

In this study, we report an interaction between a nighttime Medium Scale Traveling Ionospheric Disturbance (MSTID) and geomagnetic north-south oriented field-aligned plasma depletion structure over Hanle, Ladakh (32.7°N, 78.9°E; Mlat. ~24.1°N), India on a geomagnetically quiet night (06 May 2019, Ap = 4). The results are based on the observations carried out using a newly established airglow imager operating at 630.0 nm at Hanle which is a transition region of geomagnetically low-mid latitude. A sequence of processes constituted this unique interaction that includes developing phase of a MSTID within the imager’s field of view, gradual bending of the field-aligned plasma depletion structure and eventual merging with the MSTID, and propagation of the merged structure in the form of a single MSTID structure post-interaction. The mechanism appears to be controlled by unequal but oppositely directed polarization electric fields within the dark and bright bands of the developing MSTID, whose projection on the horizontal plane is observable in the airglow images. The present work is the first observation illustrating the interaction between a developing phase of MSTID and plasma depletion structure over a geomagnetic low-mid latitude transition region, which assumes importance for understanding the underlying plasma irregularity processes. The details of the results from this study will be discussed in the conference.


Fri-04 Aug | 1:10 - 3:10 | MR333
ST01 - Particle Acceleration and Transport at the Sun and in the Heliosphere

Session Chair(s): Kyoko WATANABE, National Defense Academy of Japan

ST01-A001 | Invited
Suprathermal Ion Observations Associated with the Heliospheric Current Sheet Crossings by Parker Solar Probe During Encounters 7-11

Mihir DESAI#+
Southwest Research Institute

We report observations of <100 keV/nucleon suprathermal (ST) H, He, O, and Fe ions in association with three separate crossings of the heliospheric current sheet that occurred near perhelia during PSP encounters 7-11. In particular, we compare and contrast the ST ion time-intensity profiles, velocity dispersion, pitch-angle distributions, spectral forms, and maximum energies during the three HCS crossings. We find that these unique ST observations are remarkably different in each case, with those during E07 posing the most serious challenges for existing models of ST ion production in the inner heliosphere. In contrast, the ISOIS observations during 4 separate HCS crossings during E08-11 appear to be consistent with a scenario in which ST ions escape out of the reconnection exhausts into the separatrix layers after getting accelerated up to ~50-100 keV/nucleon by HCS-associated magnetic reconnection-driven processes. We discuss these new observations in terms of local versus remote acceleration sources as well as in terms of expectations of existing ST ion production and propagation, including reconnection-driven and diffusive acceleration in the inner heliosphere.


ST01-A027
Observations of Suprathermal Particles (5-70 Kev) in Association with Shocks

Stefano LIVI1#+, Philippe LOUARN2, Christopher OWEN3, Raffaella D'AMICIS4, Andrey FEDOROV5, Benjamin ALTERMAN1, Susan T. LEPRI6, Jim RAINES6, Antoinette GALVIN7, Lynn KISTLER7, Frederic ALLEGRINI1, Keiichi OGASAWARA1, Peter WURZ8, Ryan DEWEY6, Roberto BRUNO4
1Southwest Research Institute, 2Institute for Research in Astrophysics and Planetology, 3University College London, 4Institute for Space Astrophysics and Planetology, 5University of Toulouse, 6University of Michigan, 7University of New Hampshire, 8University of Bern

The Heavy Ion Instrument (HIS) onboard Solar Orbiter measures mass, charge, and full 3-D velocities of ions in the energy/charge range 0.5-75keV/charge. Using the data from HIS we study how interplanetary events like shocks or CME fronts create suprathermal tails in the velocity distribution and how those tails change with time. HIS observed the passage of three interplanetary shocks during the period October 2021 - May 2022. The three events were characterized by the acceleration of plasma from the solar wind energy regime (~1keV per amu/charge) to higher energies (5-70 keV), commonly referred to as suprathermal ions; later during the events, energetic particles (100keV and above) were measured by the EPD instrument. This energization process was characterized by a clear dependence upon mass/charge, and found consistent with preferential acceleration of ions present in the high energy tails of solar wind distributions, the seed population. Details of the distribution functions during the three events are presented and contrasted to each other.


ST01-A015
The In Situ Shock Acceleration of Suprathermal Electrons at 1 AU

Linghua WANG#+, Zixuan LIU, Liu YANG, Xinnian GUO
Peking University

The shock acceleration is an important particle acceleration mechanism in the interplanetary space, but the electron shock acceleration process is not fully understood yet. Here we summarize the observational properties of in situ shock acceleration of solar wind suprathermal electrons at 1 AU, using the Wind measurements and MMS measurements. For both the Earth’ s bow shock and shocks driven by interplanetary coronal mass ejections (ICMEs), the observed power-law spectral index of shocked suprathermal electrons is significantly larger than the theoretical prediction of first-order Fermi acceleration, while the flux enhancement ratio between the downstream shocked and upstream unshocked suprathermal electrons peaks near 90° pitch angle. These observations favor the shock drift acceleration process. However, the shocked electron spectra appear to exhibit different behaviors for ICME-driven shocks and terrestrial bow shock. At ICME-driven shocks, the significantly shocked suprathermal electrons generally have a double-power-law spectrum bending upwards at a break near 2 keV with a low-energy spectral index of ∼3.7 and high-energy spectral index of ∼2.5, similar to the upstream unshocked suprathermal electrons. At the terrestrial bow shock, the strongly shocked suprathermal electrons show a double-power-law spectrum bending downwards at a break near 65 keV with a low-energy spectral index of ∼3.1 and high-energy index of ∼7.6, different from the upstream unshocked suprathermal electrons. Furthermore, the observed break energy is comparable to a critical electron energy with its cross-shock gyrodiameter equal to the bow shock’s ramp thickness. These results suggest that the shock drift acceleration process of suprathermal electrons could strongly depend on the electron trapping efficiency at the shock.


ST01-A004
Electron Acceleration at the CIR Shocks Observed by Wind and MMS

Xinnian GUO#+, Linghua WANG, Zixuan LIU
Peking University

The corotating interaction region (CIR) shocks are an important particle acceleration source in the interplanetary medium. Here we investigate the local electron acceleration at a CIR forward shock on 8 January 2018 (Case 1) and a CIR reverse shock on 7 February 2020 (Case 2), combining the electron measurements from the Wind and Magnetospheric Multiscale 1 (MMS1) spacecraft near 1 AU. For both cases with a shock arriving first at Wind and then at MMS1, we obtain the shock parameters from the nonlinear least-square shock fitting techniques and analyze the suprathermal electron measurements after the removal of instrumental effects. Across both CIR shocks, the observed electron enhancements peak near 90 pitch angle, indicating that shock drift acceleration plays a major role. In Case 1, the observed electron flux ratio between the shock’s downstream and upstream, JD/JU, measured by Wind is greater (less) than 1.5 at 0.16-8.9 keV (40-66 keV), for the estimated drift electric field Edrift of ~3.9 mV/m at the shock surface. The JD/JU observed by MMS1 is less than 1.5 at 0.16 -0.32 keV, for the estimated Edrift of ~2.4 mV/m. In Case 2, the JD/JU measured by Wind is less than 1.5 at 0.14-66 keV, for the estimated Edrift of ~1 mV/m; the JD/JU observed by MMS1 is near 1.5 at 0.13 -0.44 keV, for the estimated Edrift of ~0.8 mV/m. We find that as the CIR forward shock in Case 1 (reverse shock in Case 2) evolves from Wind to MMS1, the Edrift gets weaker (similar) and the electron drift length becomes similar (longer), leading to a weaker (stronger) shock drift acceleration.


ST01-A028
Iron Heating at a Shock Observed by Solar Orbiter's Heavy Ion Sensor

Benjamin ALTERMAN1#+, Christopher OWEN2, Philippe LOUARN3, Roberto BRUNO4, Andrey FEDOROV5, Susan T. LEPRI6, Antoinette GALVIN7, Lynn KISTLER7, Frederic ALLEGRINI1,8, Keiichi OGASAWARA1, Peter WURZ9, Ryan DEWEY6, Yeimy RIVERA10, Sarah SPITZER6, Christopher BERT6, Tim HORBURY11, Domenico TROTTA11, Heli HIETALA11, Virginia ANGELINI11, Ed FAUCHON-JONES11, Helen O'BRIEN11, Janelle HOLMES6, Irena GERSHKOVICH6, Colby HAGGERTY12, Georgios NICOLAOU2, Daniel VERSCHAREN2, Timothy STUBBS13, David BURGESS14, Raffaella D'AMICIS4
1Southwest Research Institute, 2University College London, 3Institute for Research in Astrophysics and Planetology, 4Institute for Space Astrophysics and Planetology, 5University of Toulouse, 6University of Michigan, 7University of New Hampshire, 8University of Texas at San Antonio, 9University of Bern, 10Center for Astrophysics | Harvard and Smithsonian, 11Imperial College London, 12University of Hawaii, 13NASA Goddard Space Flight Center, 14Queen Mary University

Solar Obiter’s Heavy Ion Sensor (HIS) observed a quasi-parallel CME-driven shock on March 11, 2022. HIS’ time, mass, and charge resolution enable it to resolve individual velocity distribution functions (VDFs) of iron 8+ through 12+ on the timescale of minutes. Using these 1D VDFs, we report that the thermal portion of the Fe distribution heats across the shock in a Q/M-dependent way.


ST01-A031
Nature of Ion-to-electron Scale Field Fluctuations in the Solar Wind: Insight from Artemis Observations, Simulations and Linear Theory

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 at 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.


ST01-A029 | Invited
Electron Heating Associated with Magnetic Reconnection in the Earth’s Foreshock Turbulence

Shan WANG1#+, Yan YANG2, Yi QI3
1Peking University, 2University of Delaware, 3University of Colorado Boulder

The shock transition region is rich of waves and instabilities, forming a turbulent environment where kinetic structures like magnetic reconnection develop. Reconnection is potentially important for contributing energy dissipation at the shock, but its exact role on this aspect is not yet clear. We perform a 2D particle-in-cell simulation starting from the ion-ion instability to simulate the foreshock region, which excites the ULF wave, develops current sheets and eventually leads to reconnection. The probability distribution of Te exhibits a shift to higher values near reconnection X-lines compared to elsewhere. By examining Te evolution using the superposed epoch analysis, we find that Te is higher in reconnection than in non-reconnecting current sheets, and Te increases over the ion cyclotron time scale. The heating rate of Te is 10%-40% miVA2, where VA is the average ion Alfvén speed in reconnection regions. These results demonstrate the importance of reconnection in heating electrons. We further investigate the bulk electron energization mechanisms by decomposing under guiding center approximations. Parallel electric field, Fermi and magnetization terms contribute to electron heating and their importance at different reconnection stages are evaluated. The reconnection structures can be complicated due to flows originated from the ion-scale waves, and interactions between multiple reconnection sites, etc. Our simulation results may assist future analysis of observation data.


ST01-A010
Quiet-time Energy Spectra of 50-600keV Electrons in the Terrestrial Radiation Belt

Qianyi MA#+, Linghua WANG, Qiugang ZONG, Yongfu WANG
Peking University

Quiet-time energetic electrons in the terrestrial radiation belt could provide seed populations for electron acceleration during storm times. We statistically survey the 50-600 keV electron energy spectra in the L-shell > 6.5 terrestrial radiation belt measured by the Image Electron Spectrometer (IES) on board a Chinese Navigation BeiDou satellite in an inclined (55°) geosynchronous orbit during quiet times from 2015 October to 2020 February, in order to investigate their origin and/or acceleration. We identify 6704 quiet-time 30-minute intervals and select a 5-min sample for each interval. For each sample, we utilize the pan-spectrum function [Liu et al., 2020] to self-consistently determine the energy spectral type of average omnidirectional electron fluxes, after considering the uncertainties both in electron flux J and energy E. The selected 6704 samples can be divided into three spectral types: 4371 show a generalized power-law (PL) spectrum, 1243 have a logarithmic parabola (LP) spectrum, and 1100 exhibit a generalized Ellison-Ramaty (ER) spectrum. We find that the double-power-law spectrum bending downwards at a break energy Eb of 202±61 keV with a low-energy spectral index β1 of 1.6±0.5 and a high-energy spectral index β2 of 2.9±0.8 is the most common spectral type for the quiet-time terrestrial radiation belt energetic electrons. According to the spectral shape, electron spectra are categorized into a downward-bending group that usually shows higher flux and a non-downward-bending group that usually shows lower flux. By analyzing the different temporal profiles of solar wind velocity and geomagnetic indices (AE, SYM-H) corresponding to the 2 different spectral groups, we conclude that the variation of energetic electrons' spectral shapes is mainly due to the different solar wind velocity conditions before the electron flux observation.


Fri-04 Aug | 1:10 - 3:10 | MR334
ST15 - The New Frontier: Coordinated Multi-point Ground- and Space-based Observations of the Ionosphere and Thermosphere

Session Chair(s): Shasha ZOU, University of Michigan, Douglas ROWLAND, NASA Goddard Space Flight Center

ST15-A011 | Invited
Measuring Small-scale Turbulence in the High-latitude E- and F-regions Simultaneously

Magnus IVARSEN1#+, Jean-Pierre ST-MAURICE2, Glenn HUSSEY2, Andres SPICHER3, Adam LOZINSKY2
1University of Oslo, 2University of Saskatchewan, 3University of Tromsø

The high-latitude ionosphere exhibits widespread turbulent structuring visualized by the auroral displays seen in Earth’s polar regions. Such plasma irregularities have been studied for decades, but plasma turbulence remains an elusive phenomenon. We examine scale-dependent measurements of irregularities simultaneously from the ground-based ICEBEAR 3D radar in Canada and from ESA’s Swarm satellites to characterize small-scale irregularities that exist concurrently in the E- and F-regions. For the first time, we demonstrate the clear mapping of turbulent information vertically along the Earth’s magnetic field lines, for irregularities with field-perpendicular wavelengths down to 1.5 km. Using several new techniques, we show that this statement is true for small-scale structuring in plasma density, field-aligned currents, and tentatively also electric fields. In addition to case studies, we perform a statistical analysis on an aggregate from both the E-region and the F-region. We connect density spectral shapes to Pedersen conductance in the E-region and discuss what we deem a fundamental similarity between turbulence in the polar cap and in the nightside aurora. Our results create a picture of the northern hemisphere polar cap and auroral region as a turbulent system that is in a constant state of growth and decay during storm-time. Moreover, our results show irregularities that seem intrinsically associated with E-region ionization, and we suggest that the electrodynamics of a conducting E-region should be explicitly considered when discussing plasma turbulence at high latitudes.


ST15-A001
Thermospheric Temperature and Density Variations from Gold, MSIS and WACCM-X

Guiping LIU1#+, Douglas ROWLAND1, Quan GAN2, Hanli LIU3, Jeffrey KLENZING1, Scott ENGLAND4, Richard EASTES2
1NASA Goddard Space Flight Center, 2University of Colorado Boulder, 3National Center for Atmospheric Research, 4Virginia Tech

The Global-scale Observations of the Limb and Disk (GOLD) mission in geostationary orbit at 47.5oW longitude has made near-synoptic observations of the temperature, composition, and densities in the thermosphere and ionosphere. The disk observations made within GOLD’s filed-of-view are concurrent, globally unified, and spatially resolved, allowing for separation between spatial and temporal variations. Here we analyze the daytime thermospheric temperature and column integrated O/N2 ratio observations by GOLD over 120oW-20oE longitude and 60oS – 60oN latitude throughout 2019-2020 and compare these with the results from NRLMSIS and NCAR’s Whole Atmosphere Community Climate Model with thermosphere/ionosphere extension (WACCM-X). Both observations and simulations reveal similar annual and semiannual changes and latitudinal variations, but significant differences are also noted.


ST15-A014
On the Sunrise Phase Perturbation Observed in the 22.1 kHz VLF Signal Recorded in the North of Finland

Liliana MACOTELA1#+, Mark CLILVERD2, Neil THOMSON3, David NEWNHAM2, Thomas ULICH4
1University of Bath, 2British Antarctic Survey, 3University of Otago, 4Sodankylä Geophysical Observatory

The night-to-day variability from very low frequency (VLF) sub-ionospheric radio wave phase measurements shows a phase perturbation followed by a phase recovery to normal daytime values. We monitor the variability of the size of the phase perturbation, including the time of its maximum perturbation with the aim of identifying its associated physical cause. In this study, we used the VLF signal from the 22.1 kHz UK transmitter (call sign GVT) recorded in the north of Finland, from 2010 to 2017. The timing of the maximum phase perturbation has an annual pattern that is well described by the seasonal variation of the sunrise time 28 km above the transmitter. Variations in ozone number density at stratospheric altitudes are better correlated with the size of the phase perturbation than at any other altitudes below ~80 km. Our results show that the main characteristics of the observed sunrise VLF phase recovery arise from shadowing of short wavelength solar UV flux in the D-region ionosphere due to stratospheric ozone absorption.


Fri-04 Aug | 1:10 - 3:10 | MR335
ST05 - Three-dimensional Analyses of the Solar, Heliospheric, and Planetary Plasmas

Session Chair(s): Bernard JACKSON, University of California San Diego

ST05-A013 | Invited
An Empirical Relationship Between Tomographic Density and Solar Wind Velocity in the Middle Corona

Kaine BUNTING#+, Huw MORGAN
Aberystwyth University

Accurate forecasting of space weather conditions at Earth requires an understanding of the physical state of the solar wind's origin, the solar corona. This work outlines recent developments in Coronal Rotational Tomography (CRT) which forms the basis of novel inner boundary conditions for heliospheric solar wind models. CRT is applied to white light coronagraph observations to generate maps of the coronal electron density at heliocentric heights where both the solar wind flow and coronal magnetic field are predominantly radial (4-8 solar radii), thus avoiding the complex inner corona which is most difficult to model. An empirical inverse model is derived allowing a conversion of tomographic densities into solar wind velocities, forming inner boundary conditions for the highly efficient HUXt solar wind model. Model predictions of the solar wind conditions at 1 AU are compared to predictions based on commonly used magnetic field extrapolation inner boundary conditions and in-situ observations. Results show the use of tomographic density maps provide a valid alternative to coronal magnetic models and offer a significant advancement of the field given the routine availability of spaced-based coronagraph observations. The tomography derived inner boundary condition will be implemented for operational use for the UK Met Office in the coming months.


ST05-A009
Forecasting Deep Space Weather Using Spacecraft Radio Signals and VLBI Radio Telescopes

Guifré MOLERA CALVÉS1#+, Jasper EDWARDS1, Pradyumna KUMMAMURU1, Giuseppe CIMO2, Masdiana NOOR SAID1
1University of Tasmania, 2Joint Institute for VLBI ERIC

University of Tasmania (UTAS) and the Joint Institute for VLBI-ERIC conduct regular observations of deep space missions to study the solar wind and forecast space weather. Tracking the radio signal transmitted by a spacecraft with VLBI ground-based antennas enhances the scientific outcome of the missions by providing interplanetary medium diagnosis. We use multi-frequency observations (in S, X and Ka-band), in-beam multi-spacecraft, and simultaneous VLBI radio telescopes at various locations on the ground [1]. Current tracking capabilities includes support to the European Space Agency missions of Bepi Colombo, Mars Express, Trace Gas Orbiter, Solar Orbiter, the Chinese National Space Agency Tianwen-1, and NASA’s Mars Insight and Juno. The analysis of the fluctuations in amplitude, frequency, and phase of the signal transmitted by each spacecraft provides characteristics of the propagation media such as electron density profiles for the line-of-sight, interplanetary scintillation of solar wind, magnetic field, and propagation orientation and speed of Coronal Mass Ejections [2]. The ESA Jupiter Icy Moons Explorer (JUICE) space mission will be launched in April this year. Planetary Radio Interferometry and Doppler Experiment is a scientific instrument on board of the mission and lead by JIVE and this team. JUICE will provide a new insight of solar wind and space weather enabling observations at X and Ka-band during its phase cruise in the inner Solar System. Here we present data from the last Martian solar conjunction in October 2021. We conducted an extensive campaign to cover the ingress and egress of the solar conjunction of Mars to study the coronal structure heating and solar wind acceleration. During this campaign, we detected CME and density enhancements that crossed along the ray paths of the telescope’s sightlines. We will link the outcome of this campaign to the initial results obtained from JUICE spacecraft after its launch.


ST05-A005 | Invited
Three-dimensional Reconstruction of CMEs Using MHD Simulation with Interplanetary Scintillation Data Observed from Radio Sites ISEE and LOFAR

Kazumasa IWAI1#+, Richard FALLOWS2, Mario BISI3, Daikou SHIOTA4, Bernard JACKSON5, Munetoshi TOKUMARU1, Ken'ichi FUJIKI1
1Nagoya University, 2ASTRON - The Netherlands Institute for Radio Astronomy, 3United Kingdom Research and Innovation - Science & Technology Facilities Council - RAL Space, 4National Institute of Information and Communications Technology, 5University of California San Diego

Interplanetary scintillation (IPS) is a useful tool for detecting coronal mass ejections (CMEs) throughout interplanetary space. Global magnetohydrodynamic (MHD) simulations of the heliosphere, which are usually used to predict the arrival and geo-effectiveness of CMEs, can be improved using IPS data. In this study, we demonstrate an MHD simulation that includes IPS data from multiple ground-based stations to improve the 3D reconstruction of CME modelling. The CMEs, which occurred on 09-10 September 2017, were observed over the period 10-12 September 2017 using the Low-Frequency Array (LOFAR) and IPS array of the Institute for Space-Earth Environmental Research (ISEE), Nagoya University, as they tracked through the inner heliosphere. We simulated CME propagation using a global MHD simulation, SUSANOO-CME, in which CMEs were modeled as spheromaks, and the IPS data were synthesised from the simulation results. The MHD simulation suggests that the CMEs merged in interplanetary space, forming complicated IPS g-level distributions in the sky map. We found that the MHD simulation that best fits both LOFAR and ISEE data provided a better 3D reconstruction of the CMEs and a better forecast of their arrival at Earth than from measurements when these simulations were fit from the ISEE site alone. More IPS data observed from multiple stations at different local times in this study can help reconstruct the global structure of the CME, thus improving and evaluating the CME modelling.


ST05-A007 | Invited
Heliospheric 3-D MHD ENLIL Modeling

Dusan ODSTRCIL1,2#+, Bernard JACKSON3, Mario BISI4, Munetoshi TOKUMARU5
1George Mason University, 2NASA Goddard Space Flight Center, 3University of California San Diego, 4United Kingdom Research and Innovation - Science & Technology Facilities Council - RAL Space, 5Nagoya University

We present the results of global heliospheric simulations in March 2022 computed by the 3-D magnetohydrodynamic (MHD) heliospheric code ENLIL. This code can use outputs from: (1) the coronal WSA model utilizing the GONG photospheric observations and (2) UCSD tomographic data using the ISEE interplanetary Scintillation (IPS) observations. The geometric and kinematic parameters of coronal mass ejections (CMEs) are calculated from the coronagraph observations. This modeling system can provide a near-real-time prediction of heliospheric space weather. In this presentation, we simulated the global structure of solar wind in March 2022. We will provide a global context for interpreting multi-spacecraft observations and compare results with in-situ measurements by ACE, STEREO-A, Parker Solar Probe, BepiColombo, and Solar Orbiter spacecraft.


ST05-A008
Widefield Interplanetary Scintillation Measurements: Tracking Disturbances Through the Heliosphere from 10-100 Solar Radii

John MORGAN1#+, Rajan CHHETRI2, Angelica WASZEWSKI3, Mark CHEUNG2
1CSIRO Space and Astronomy, 2CSIRO - Space and Astronomy, 3Curtin University

Over the last few years we have developed the IPS technique, exploiting modern, large-N interferometers such as the Murchison Widefield Array (MWA) and the Australian Square Kilometre Array Pathfinder (ASKAP) to make simultaneous measurements of hundreds of line of sight, with a density of measurements approaching 1 per square degree. In the last year there has been very rapid progress on applying this new technique for Space Weather measurements.
First, in a submitted paper, we have demonstrated that we have sufficient density of IPS measurements to image the location of a CME front. Secondly, we are rapidly developing the capability to do similar widefield IPS observations with ASKAP, measuring IPS from all sources in an annulus around the Sun covering elongations of 5-15 degrees. 
In this talk, I will summarise these advances, as well as discussing novel new techniques for reconstructing the Heliosphere in 3D using these new observables. Finally, I will suggest possible future efforts to incorporate these data into heliospheric modelling and prediction.


ST05-A014 | Invited
Use of Scintillation Observations from Radio Telescopes for the Modelling of Plasma Irregularities

Biagio FORTE1#+, Richard FALLOWS2, Mario BISI3, Pawel FLISEK4, Kacper KOTULAK4, Andrzej KRANKOWSKI4, Maaijke MEVIUS2, Kasia BESER2
1University of Bath, 2ASTRON - The Netherlands Institute for Radio Astronomy, 3United Kingdom Research and Innovation - Science & Technology Facilities Council - RAL Space, 4University of Warmia and Mazury in Olsztyn

Radio wave scintillation arises from the propagation of radio waves through spatial inhomogeneities (or irregularities) in the plasma density distribution, which drift across the ray path. Scintillation manifests as temporal fluctuations of the intensity and phase of radio waves that traversed plasma irregularities. These temporal fluctuations are the result of a diffraction pattern that is associated with a particular distribution of irregularities. In the case of plasma density irregularities in the Earth’s ionosphere, radio wave scintillation can be observed on radio signals transmitted from artificial satellites as well as on radio signals emitted from radio objects and received on Earth. The amount of scintillation varies according to the distribution of the plasma density fluctuations, and it typically is subdivided in two intervals: low scintillation and high scintillation. In the presence of low scintillation, a weak scattering approximation can be utilised to retrieve some information about irregularities (e.g., the drift velocity); on the other hand, in the presence of strong scintillation multiple scattering becomes necessary to describe the problem. In the weak scattering approximation, it is assumed that irregularities are confined to a phase-changing screen; in the presence of multiple scattering, irregularities can be modelled by means of subsequent phase screens. Multiple scattering can originate strong and saturating scintillation. This contribution will discuss examples of scintillation recorded by means of radio telescopes as well as satellite receivers in the presence of ionospheric irregularities. The problem of retrieving information about irregularities and their distribution is analysed and characterised. The merit of weak scattering approximation and of multiple scattering is considered: the impact of different scattering approximations in the retrieval of information about irregularities is analysed. This analysis enables a discussion on scintillation originating beyond the Earths’ ionosphere, for example, in the interplanetary medium.


ST05-A001 | Invited
Real-time Ionosphere Observations with a Dense GNSS Network by a Three-dimensional Tomography Technique

Susumu SAITO1#+, Taisei NOZAKI2, Mamoru YAMAMOTO2, Nicholas SSESSANGA3
1National Institute of Maritime, Port and Aviation Technology, 2Kyoto University, 34D-Space

Information on the three-dimensional (3-D) ionospheric density profiles are very important to understand the behavior and physics of the ionosphere. However, techniques to observe the 3-D ionospheric density profiles are quite limited. It is especially difficult to obtain them in continuous basis. Tomographic reconstruction with total electron content (TEC) measurements by a network of Global Navigation Satellite System (GNSS) receivers is one of the techniques which enable us to access such information.
We have developed a system to reconstruct 3-D ionospheric density profiles over Japan [1]. Real-time GNSS data obtained by 200 selected receivers of the GNSS Earth Observation NETwork (GEONET) operated by the Geospatial Information Authority Japan is used to compute many TEC data which are converted to 3-D ionospheric density profiles over Japan with 15 minutes cadence with about 6 minutes latency.
The results were shown to be in good agreement with ionosonde, radio occultation, and incoherent scatter radar measurements. However, it was also found that the accuracy of reconstruction were degraded when the ionospheric peak height was extraordinary low [2]. We have assimilated the ionospheric peak density and height information obtained by ionosonde stations into the GNSS tomography [3], which improved the accuracy of the tomographic reconstruction of the ionosphere. The technique has been further improved for better and efficient processing.
In this paper, the technique and some results in the ionospheric disturbances will be presented. Results of real-time ionospheric density reconstruction will also be presented.[1] Saito et al., Real-time ionosphere monitoring by three dimensional tomography over Japan, NAVIGATION, 2017.
[2] Saito et al., Real-time 3-D ionospheric tomography and its validation by the MU radar, AP-RASC 2019, 2019.
[3] Ssessanga et al., Complementing regional ground GNSS-STEC computerized ionospheric tomography (CIT) with ionosonde data assimilation, GPS Solutions, 2021.



Solid Earth Sciences


Mon-31 Jul | 10:20 - 12:20 | MR332
SE02 - Cross-Scale Observation and Modeling of Surface Processes and Tectonic Evolution

Session Chair(s): Haibin YANG, Zhejiang University, J. Bruce H. SHYU, National Taiwan University

SE02-A009 | Invited
Coseismic Surface Rupture and Structural Change of the Superficial Seismogenic Fault of the 2022 Ms6.9 Menyuan Earthquake, Western Haiyuan Fault, China

Haibing LI1#+, Jiawei PAN2, Marie-Luce CHEVALIER3, Dongliang LIU3, Liqing JIAO2, Chao LI2, Fucai LIU2, Qiong WU2, Haijian LU2
1Chinese Academy of Geological Sciences, Institute of Geology, 2Chinese Academy of Geological Sciences, 3Institute of Geology, Chinese Academy of Geological Sciences

The 2022 Ms6.9 Menyuan earthquake ruptured the central and western segments of the Haiyuan fault in NE Tibet. Coseismic surface ruptures with tension cracks, tensional-shear cracks, shear cracks, mole tracks, and sags are seen over ~27 km. That such rather small magnitude earthquake produced such long surface rupture with impressive surface deformation suggests that the focal depth may be shallower than the 10 km indicated. The ~5 km-long western segment of the rupture displays a maximum horizontal offset of ~85±10 cm, the 8 km-long central segment a maximum of ~3.7 m, and the 14 km-long eastern segment a maximum of ~3.8 m. This earthquake has left-laterally offset the tunnel of the Lanzhou-Xinjiang railway, which we studied using long-distance LiDAR scanning inside the tunnel. We strike difference between the tunnel and the surface rupture is ~41°, the maximum rupture dip angle is ~40°, the left-lateral offsets of the eastern and western tunnel walls are ~4 and ~3.8 m, respectively, with ~0.5 m vertical offset. The dip between the rupture in the tunnel and that at the surface is ~40° near the surface, inconsistent with the nearly-vertical dip rupture shown by focal mechanisms. Here, we found that the local stress field changed due to the decrease of gravity load during the formation of the strike-slip fault from deep to shallow depths, yielding the surface rupture to become low angle, is in agreement with numerical simulation using the discrete element method. That the fault dip can easily vary at the surface of a high mountain has great implication for the construction of other railroads, such as that of Sichuan-Tibet, which will cross a series of very active strike-slip faults at the eastern margin of the Tibetan plateau.


SE02-A019
Numerical Modelling of Earthquake Cycles Based on Navier-stokes Equations with Viscoelastic-plasticity Rheology

Haibin YANG1#+, Louis MORESI2, Huihui WENG3, Julian GIORDANI4
1Zhejiang University, 2Australian National University, 3Nanjing University, 4Sydney University

Visco-elastic-plastic modelling approaches for long-term tectonic deformation assume that co-seismic fault displacement can be integrated over 1,000s-10,000s years (tens of earthquake cycles) with the appropriate failure law, and that short-timescale fluctuations in the stress field due to individual earthquakes have no effect on long-term behavior. Models of the earthquake rupture process generally assume that the tectonic (long-range) stress field or kinematic boundary conditions are steady over the course of multiple earthquake cycles. In this study, we develop a numerical framework that embeds earthquake rupture dynamics into a long-term tectonic deformation model by adding inertial terms and using highly adaptive time-stepping that can capture deformation at plate-motion rates as well as individual earthquakes. We reproduce benchmarks at the earthquake timescale to demonstrate the effectiveness of our approach. We then discuss how these high-resolution models degrade if the time-step cannot capture the rupture process accurately and, from this, infer when it is important to consider coupling of the two timescales and the level of accuracy required. To build upon these benchmarks, we undertake a generic study of a thrust fault in the crust with a prescribed geometry. We find that lower crustal rheology affects the periodic time of characteristic earthquake cycles and the inter-seismic, free-surface deformation rate. In particular, the relaxation of the surface of a cratonic region (with a relatively strong lower crust) has a characteristic double-peaked uplift profile that persists for thousands of years after a major slip event. This pattern might be diagnostic of active faults in cratonic regions.


SE02-A025 | Invited
Rheological Heterogeneities in the Lower Crust in Eastern Tibet

Yan HU1#+, Yunguo CHEN2, Bin ZHAO3, Qi WANG4, Guojie MENG3
1Deep Space Exploration Laboratory/University of Science and Technology of China, 2University of Science and Technology of China, 3China Earthquake Administration, 4China University of Geosciences

Postseismic deformation of large earthquakes help gain insights into the rheological structure and property of the lithosphere and upper mantle. We have developed three dimensional viscoelastic finite element models to study deformation processes of the 2008 Mw7.9 Wenchuan and 2010 Mw6.9 Yushu earthquakes. The model includes an elastic upper crust, viscoelastic lower crust and upper mantle. Viscoelastic relaxation of earthquake-induced stresses in the lower crust and upper mantle is simulated by the biviscous Burgers rheology. The time-dependent, stress-driven afterslip is simulated through thin weak shear zone attached to the fault. The model successfully reproduces the overall pattern of GPS observations. Model results indicate that the viscosity in the lower crust increases from about 5 x 1018 Pa s at the Yushu fault to about 2 x 1019 Pa s at the Longmenshan fault in the East. The other feature is that the viscosity of the lower crust in eastern Tibet increases by one order of magnitude from the southern edge of the Longmenshan fault to its northern edge. The viscosity of the upper mantle is determined to be no less than ~1020 Pa s. The afterslip of the fault takes place mostly within the first year after the earthquake and decays rapidly with time.


SE02-A021 | Invited
Accelerating Boundary Element Method for fully- and Quasi-dynamic Earthquake Simulations

Ryosuke ANDO1#+, So OZAWA2
1The University of Tokyo, 2Stanford University

Earthquake simulations require the interaction between the elastic response of the medium and the temporally evolving boundary condition due to fracture and friction. The system is highly nonlinear and requires the accurate evaluation of stress singularity on the boundary surfaces, which are characterized by geometrical complexity. We develop efficient numerical algorithms capable of fully utilizing high-performance computers to simulate the earthquake rupture/cycle processes of arbitrarily shaped faults. We use the dynamic and static boundary element method (BEM), given the advantages of fracture mechanical analyses and modeling non-planar fracture surfaces. For the dynamic-BEM, we introduce an efficient method called the Fast Domain Partitioning Method (FDPM), which considers each phase of seismic waves separately and reduced the memory requirement from O(N^2 M) to O(N^2) for each time step. We also adopt the Hierarchical matrices for the matrix vector product and acceleration of the MPI communication by assigning the blocks of MPI to the lattice structure. H-matrices reduce the numerical complexity of the matrix vector product to O(N LogN) from the original dense matrices of O(N^2). The Latice H-matrices reduces the MPI communication costs to O(N) from the original H-matrices of O(N Np) with the number of MPI Np, which was associated with the compressibility. Several examples of using these methods will be discussed.


SE02-A027
Response of River Profiles to Active Faulting Around the Diancang Shan, SE Tibetan Plateau

Yangfan HUANG+, Xuhua SHI#, Rong YANG, Jinhan WANG, Hanlin CHEN
Zhejiang University

The Diancang Shan (DCS) Fault zone, located at the northwestern end of the dextral-slip Red River Fault (RRF) zone, is characterized by normal slip with a minor component of dextral-slip, in the southeastern Tibetan Plateau. Its complex geometry and kinematics are crucial for understanding the timing and nature of the northward propagation of the RRF and regional kinematics of the southeastern Tibetan Plateau. While previous studies have provided extensive insights into the regional metamorphic belt, lower crust deformation, and active periods since the Cenozoic era, some questions remain regarding the temporal and spatial evolution of the faults and geomorphology during the Quaternary. Here we focus on how river profiles of the Diancang Shan respond to the spatiotemporal faulting around the DCS, based on analyses of channel steepness (Ksn) values, the spatial distribution of knickpoints along the river profiles, together with the seismicity data of the 2021 Mw 6.4 Yangbi earthquake that relates to blind faulting in the region. Our Ksn values and knickpoint distribution suggest that there exist several phases of the accelerating normal faulting around the DCS, with differential vertical motion among different segments of the DCS normal fault. The spatial pattern of these parameters is consistent with the northward propagation of the RRF during the Quaternary. The integrated analysis of Ksn values, the spatial distribution of knickpoints and the high-precision relocated aftershock sequence, suggest that fluvial geomorphic indices may delineate the blind fault that is discernable on the surface, thus facilitating the regional seismic hazard assessment. Such an analysis can be applied to other tectonically active regions without obvious geomorphic expressions of faulting.


SE02-A008
Geometry, Kinematics, and Late Pleistocene-Holocene Slip Rates of the South Riyueshan Fault in the NE Margin of the Tibetan Plateau, China

Jinrui LIU1#+, Zhikun REN2, Edwin NISSEN3, Chi ZHANG1
1China Earthquake Administration, 2Institute of Geology, China Earthquake Administration, 3University of Victoria

Due to the distal effects of the India-Eurasia convergence, the northeast margin of the Tibetan Plateau is an outstanding natural laboratory to elucidate the growth of topography in continental collision zones. The dominant structures in the area are the nearly E-W trending Haiyuan and Kunlun sinistral strike-slip faults, both well-studied due to their fast slip-rates (~5 and ~10-12 mm/yr, respectively) and recent large earthquakes. However, distributed deformation in between the major faults — evident in distinct NNW-trending dextral strike-slip faults and E-W trending reverse faults — is currently poorly understood. The focus of this study is to quantify the late Quaternary activity of one of the most prominent of these faults, the NNW-trending South Riyueshan fault (SRYSF), which has not previously been reported. We interpret the detailed geometry of the SRYSF using topography data at a range of spatial scales and resolutions, including DEMs generated from GF-7 satellite stereo pairs and drone photogrammetric surveys. North of 35oN, the southern, Duohemao segment of the SRYSF splits into two branches, the Waligong segment in the west and the Guide segment in the east. A pair of published magnetotelluric profiles hint that the Waligong segment terminates northwards into the Qinghai Nanshan thrust and that the Guide segment terminates near the West Qinling fault. Distributions of pre-Quaternary strata and granite plutons are consistent with this interpretation. Furthermore, by dating offset landforms with Optically Stimulated Luminescence and Radiocarbon, we constrained the late Holocene slip rates of the Guide and Duohemao segments to be 3.6±0.2 mm/yr and 1.7±0.3 mm/yr, respectively. These multi mm/yr slip rates highlight the importance of these NNW-trending strike-slip faults, despite their shorter lengths relative to the Kunlun and Haiyuan faults.


SE02-A004
Construction of a Multi-lake Palaeosismometer for the Xianshuihe Fault System (SE Tibet)

Marie-Luce CHEVALIER1#+, François LEMOT2, Pierre SABATIER3, Anne REPLUMAZ2, Christian CROUZET2, Patrick RIOUAL4, Mingkun BAI5, Ziqi FANG6, Ciqi ZHANG6, Chenglong GE6, Nathaniel FINDLING2, Haibing LI7
1Institute of Geology, Chinese Academy of Geological Sciences, 2Institut des Sciences de la Terre/ Université Grenoble Alpes/ Université Savoie Mont Blanc/ National Centre for Scientific Research, 3cEDYTEM/ National Centre for Scientific Research/ Université Savoie Mont Blanc, 4Chinese Academy of Sciences, 5China Earthquake Administration, 6Chinese Academy of Geological Sciences, 7Chinese Academy of Geological Sciences, Institute of Geology

Although mountain lakes are remarkable archives of seismic events globally, precise quantitative estimates of both palaeointensities and locations are challenging to obtain, as earthquake records in lake sediment depend on numerous external (i.e., earthquake characteristics) and internal (e.g., sedimentation rate, basin geometry) factors. However, palaeo-earthquake characteristics are missing, preventing precise calibration of lake sensitivity with documented earthquakes, necessary to reconstruct long-term earthquake return periods and thus hazard assessment in this area. We sampled nine mountain lakes (37 cores up to 137 cm long using a gravity corer) located along the very active Xianshuihe fault system in SE Tibet. We conducted preliminary analyses on sediment cores using short-lived radionuclides and radiocarbon ages, as well as a multiproxy approach that includes granulometry, loss-on-ignition, continuous XRF core scanning and discrete quantitative measurements, XRD, and SEM for microfacies analyses. These observations allowed us to identify event deposits related to historical earthquakes, including that of the 1955 Mw7.5 Kangding earthquake, and validate their coseismic origin, thanks to the Chinese seismic catalogs covering the last three centuries for the eastern plateau region. We discuss how magnitude, rupture extent, and epicenter-lake distance control the triggering of event deposits at each site. Considering the calibrated site sensitivity, triangulating between several lakes where events are recorded provides a regional palaeosismometer yielding events intensity and location.


SE02-A022
Viscoelastic Relaxation of the Upper Mantle and Stress-driven Afterslip Following the 2016 Mw7.8 Kaikōura Earthquake

Kai WANG1#+, Yan HU2
1University of Science and Technology of China, 2Deep Space Exploration Laboratory/University of Science and Technology of China

Understanding postseismic processes following the 2016 Kaikōura earthquake remains challenging due to the time-dependent afterslip over the complex forearc system including crustal faults and megathrust, and the viscoelastic relaxation of the upper mantle. We have derived the 5-year postseismic displacements from Global Positioning System time series of 75 stations to study postseismic processes through a three-dimensional viscoelastic finite element model. In this work, we assume that viscoelastic relaxation of the upper mantle is represented by the biviscous Burgers rheology. Afterslip of the fault is simulated through a 2-km thick weak shear zone attached to the fault. Test models have determined the optimal steady-state viscosities of the crustal shear zone, megathrust shear zone, Australian upper mantle and Pacific upper mantle to be 1018 Pa s, 4×1017 Pa s, 2×1019 Pa s and 1020 Pa s, respectively. Afterslip over crustal faults and the megathrust are both required to reproduce the first-order pattern of horizontal GPS observations. In the model, stress interaction from the ruptured crustal faults to the subduction systems promotes aseismic afterslip over the megathrust. Coseismic rupture and afterslip over the megathrust are required to better fit eastward motions of coast stations. The stress-driven afterslip over crustal faults within the first 5 years after the earthquake is up to 80 cm, and the afterslip over the megathrust is up to 60 cm. Additional Kapiti slow slip is inverted from the residual between observations and model predictions near the Kapiti coast, and is up to ~11 cm within the first year after the earthquake.


Mon-31 Jul | 1:10 - 3:10 | MR307
SE17 - General Session

Session Chair(s): Florian M. SCHWANDNER, NASA Ames Research Center, J. Bruce H. SHYU, National Taiwan University

SE17-A013
WDMAM v. 2.1: Improved World Digital Magnetic Anomaly Map Released

Jerome DYMENT1#+, Yujin CHOI2, Vincent LESUR2, Andreina GARCIA REYES2, Manuel CATALAN3, Takemi ISHIHARA4, Tamara LITVINOVA5, Mohamed HAMOUDI6
1Université Paris Cité / Institut de Physique du Globe de Paris and National Centre for Scientific Research, 2Institut de Physique du Globe de Paris/ University of Paris/ National Centre for Scientific Research, 3Real Observatorio del Armada, 4Geological Survey of Japan, 5Russian Geological Research Institute, 6Universiy of Sciences and Technologies Houari Boumediene

The World Digital Magnetic Anomaly Map is prepared under the auspices of IAGA and the CGMW (Commission for the Geological Map of the World) of UNESCO. The first version was released in 2007 (Korhonen et al., CGMW map, 2007), and the second one in 2015 (Dyment et al., EPSL, 2015; Lesur et al., EPS, 2016) with the mandate to update the version 2.0 using the same methodology when the availability of new data would make it necessary. The present version 2.1, compiled at 5 km interval, at 5 km altitude above the continents and at sea-level over the oceans, includes new datasets: (1) the complete digital aeromagnetic map of Brasil made available by ANP; (2) an improved version of the aeromagnetic map of Russia prepared by V-SEGEI; (3) the second version of the Antarctic Digital Magnetic Anomaly maP (ADMAP; Golynsky et al., GRL, 2018) which results from a remarkable international effort during and after the Second International Polar Year; (4) a new map of the Caribbean plate and Gulf of Mexico resulting from the compilation and re-processing of existing marine data in the area (Garcia and Dyment, EPSL, 2021, 2022); (5) the updated Magnetic Anomaly Map of Eastern Asia prepared by the CCOP (MAMEA; Ishihara and Uchida, 2021); and (6) a new marine magnetic anomaly data compilation prepared by T. Ishihara and coworkers. The remaining data gaps are filled with the satellite anomaly model of Thebault et al. (GRL, 2021). Long wavelengths of degree and order lower than 120 are filtered and replaced by those computed between order and degree 16 and 120 using the magnetic anomaly model of Thebault et al. (GRL, 2021) derived from CHAMP and Swarm satellite data. The new map will be presented and its significant improvements over the previous version discussed.


SE17-A027
Crystal-melt Interfaces in Mg2SiO4 Forsterite at High Pressure: Structural and Energetics Insights from First-principles Simulations

Bijaya KARKI1#+, Dipta GHOSH1, Jianwei WANG1, Shun-Ichiro KARATO2
1Louisiana State University, 2Yale University

The interplay between crystal-melt (solid-liquid) and grain boundary interfaces in partially melted polycrystalline aggregates controls many physical properties of mantle rocks. To understand this process at the fundamental level requires improved knowledge about the interfacial structures and energetics. Here we report the results of first-principles molecular dynamics simulations of two grain boundaries of (0l1)/[100] type for tilt angles of 30.4 and 49.6o and the corresponding solid-liquid interfaces in Mg2SiO4 forsterite at the conditions of the upper mantle-transition zone. Our analysis of the simulated position-time series shows that structural distortions of the solid-liquid interfacial region are stronger than intergranular interfacial distortions. The calculated formation enthalpy of these solid-solid interfaces increases nearly linearly from 1.0 to 1.6 J/m2 for the 30.4o tilt and from 0.7 to 1.0 J/m2 for the 49.6o tilt with pressure from 0 to ~25 GPa at 1500 K, being consistent with the experimental data. The solid-liquid interfacial enthalpy takes comparable values in the range 0.9 to 1.6 J/m2 over similar pressure interval. The dihedral angle of the forsterite-melt system estimated using these interfacial enthalpies takes values in the range of 70o to 150o and shows a decreasing trend with pressure. We also present the implication of our predicted relatively large dihedral angles for partial melts in deep mantle.


SE17-A026
Fluorine in the Solid Earth: Unearthing Where Fluorine is Incorporated in Forsterite, Mg2SiO4

Jun Hao Brendan TEO#+, Simon REDFERN
Nanyang Technological University

Fluorine is known to be highly reactive due to its high electronegativity. This makes fluorine’s reactions with various chemicals and minerals an important topic of study. Much of the fluorine in the Earth is currently believed to be concentrated in Earth’s interior, including the mantle. With the relatively low quantities present at the surface, fluorine is typically benign to human health. However, when the mantle-locked fluorine does manage to infiltrate the surface, it can prove hazardous. One such effect is fluorosis, whereby excess fluorine intake into the body leads to bone embrittlement and tendency to fracturing. Yet, despite this potential danger, our understanding of fluorine abundance and how it is stored in the solid Earth, in particular in the mantle, is woefully insufficient. Our study uses computational structure simulations to determine where fluorine can be stored within forsterite, the most abundant mineral found in Earth’s upper mantle. Previous studies have elucidated forsterite’s capacity to hold significant amounts of fluorine but were unable to determine where fluorine is stored within the crystalline lattice. Our calculations show that fluorine is readily stored within nominally anhydrous forsterite in conjunction with hydroxyl ions (OH-) in the ratio 1:3 within a hydrogarnet-like defect. We further show that any additional replacements of hydroxyl ions with fluorine are not favoured. In summary, our results suggest that the relationship between fluorine and hydroxyl ions helps to control where and how much fluorine can be stored in forsterite. These observations enable us to further our understanding of fluorine in the mantle and estimate how much may be released to the surface from magmatic processes.


SE17-A008
Factors Controlling the Mud Crack Patterns: Insights from Analogue Experiments

Uddalak BISWAS1#+, Atin Kumar MITRA1, Nibir MANDAL2
1Indian Institute of Engineering Science and Technology, 2Jadavpur University

Mud cracks are a common signature of desiccation in muddy layers under atmospheric conditions. Geologists often use them to reconstruct paleoenvironments from rock records, considering that the crack pattern is a reliable indicator of specific environmental conditions. Despite significant progress in the study of external factors, such as ambient temperature, humidity, sun exposure time, and new fluid incorporation guiding the desiccation process, the conditions required for their specific pattern formation are not comprehensively understood. This article accounts for a set of physical factors: mud layer thickness, compositional variations, and drastic thermal change to demonstrate their effects on the mud crack patterns from controlled laboratory experiments. The experiments were conducted with varying mud layer thicknesses (Tm) in the range 0.5 cm to 2.0 cm and mud slurry compositions with talc, and cocopeat mixtures at 1:1, 1:2 and 1:3 ratios. We also ran a set of experiments in the hot air oven for 6 to 7 hours at 50° C to investigate temperature effects on the mud crack patterns. The laboratory experiments produced desiccation cracks with three characteristic geometrical patterns: isolated linear cracks (IL), inter-connected straight cracks (ICS), and inter-connected dendritic patterns (ICD). An increase in Tm resulted in a gradual transition of the crack pattern from ICS to IL, following a remarkable enhancement of the crack initiation time (ti), which again widens with increasing ambient temperature. On the other hand, increasing mud to talc and cocopeat ratios transformed the pattern from ICS to IL and ICD to IL and finally to highly dense ICD, respectively. The crack frequency and the inter-crack angle in the crack network are found to be sensitive to mud layer thickness as well as the composition and thermal condition. We finally propose a mechanical model to explain the mud crack patterns.


SE17-A019
Failure Criteria of Rocks in Tensile Tests Under Confining Pressure to Consider the Mechanism of Fault Movement with Hydraulic Fracturing

Yu AOJI1#+, Takato TAKEMURA1, Daisuke ASAHINA2
1Nihon University, 2Geological Survey of Japan

On June 29, 2012, an earthquake of M4.5 with a depth of 0 km occurred on Chiba Prefecture in Japan. The 0km-depth earthquake affects the safety of underground geoengineering activities such as geological disposal and carbon capture sequestration. Therefore, it is important to understand the mechanism such 0km-depth earthquake. We have conducted the direct shear tests on the sedimentary rock distributed at the area where the 0km-depth earthquake occurred, and drew the Coulomb failure criteria. Based on the results, the stress polygon was used to estimate the stress field, and it was inferred that this earthquake occurred in the tensile stress condition. This could be due to the effect of excess pore pressure in the crust, which also generate the tensile stress condition. The purpose of this research is to study the failure criteria of rocks through tensile tests under confining pressure for elucidating the fracture mechanism of the 0km-depth earthquake. Also, a comparison is made between the failure criteria obtained in this study and the Griffith criteria obtained from the uniaxial tensile strength. The failure criteria, which covered the tensile stress condition, is applicable in the presence of excess pore pressure, for example, the mechanism of fault movement with hydraulic fracturing.


Mon-31 Jul | 1:10 - 3:10 | MR332
SE02 - Cross-Scale Observation and Modeling of Surface Processes and Tectonic Evolution

Session Chair(s): Zhikun REN, Institute of Geology, China Earthquake Administration, Marie-Luce CHEVALIER, Institute of Geology, Chinese Academy of Geological Sciences

SE02-A003 | Invited
Combining Multi-component Thermochronology and Tectono-thermal Modeling to Constrain Tectonics and Exhumation Along the Margins of the Tibetan Plateau

Kevin P. FURLONG1#+, Eric KIRBY2
1Penn State University, 2University of North Carolina

The utilization of thermal-chronological data to explore the interplay between tectonics and erosion during mountain building relies on associations among rock uplift, exhumation, and cooling during orogenesis. Because neither uplift or exhumation is readily observed, the reconstruction of temperature-time histories via thermochronologic systems provides a proxy method to relate the cooling history of the rock to the evolution of the orogen. Although the cooling experienced by a rock sample and the exhumation history are often assumed to be directly linked, for the rapid exhumation rates that characterize most active orogenic systems, the thermal history will differ from simple linear cooling with exhumation because of the effects of heat advection, propagation of thermal perturbations, and other processes that affect the cooling behavior. Simple assumptions of a constant temperature gradient may be adequate to describe slowly eroding regions, but the advection of heat at exhumation rates greater than ~0.2-0.3 mm/yr make these simple assumptions untenable. Moreover, an increasing suite of thermochronologic data, spanning a range of closure temperatures, suggest that many (most?) orogenic systems are characterized by non-steady exhumation over timescales of a few Ma. Time-varying uplift and exhumation generates transient crustal thermal regimes that place important constraints on the orogenic evolution. We apply these lessons to several extensive multi-component data sets from the high-relief ranges that demarcate the eastern margin of the Tibetan Plateau in order to determine their exhumation histories. Our results provide constraints on the onset of Cenozoic exhumation, the subsequent pace of exhumation, and on the tectonic history of one of the major fault systems in the central Longmen Shan.


SE02-A005
Timing and Exhumation History of the Gaoligong and Chongshan Shear Zones, Se Tibetan Plateau, and Geodynamic Implications

Mingkun BAI1+, Anne REPLUMAZ2, Marie-Luce CHEVALIER3#, Philippe LELOUP4, Xiong OU5, Haibing LI6, Zhikun REN7
1Institue of Geology, China Earthquake Administration, 2Institut des Sciences de la Terre/ Université Grenoble Alpes/ Université Savoie Mont Blanc/ National Centre for Scientific Research, 3Institute of Geology, Chinese Academy of Geological Sciences, 4Université de Lyon/ École Normale Supérieure de Lyon/ National Centre for Scientific Research, 5Université Grenoble Alpes, 6Chinese Academy of Geological Sciences, Institute of Geology, 7Institute of Geology, China Earthquake Administration

The Three Rivers region in the southeastern Tibetan Plateau, where the Salween, Mekong, and Yangtze Rivers flow parallel to each other, accommodates one of the strongest deformation around the Eastern Himalayan Syntaxis following the India-Asia convergence, with geologic landforms compressed together, in sharp contrast to what occurs farther north and south. The region’s tectonic and landscape evolution history have significant implications for further understanding the mechanisms of intracontinental deformation and plateau growth. In this study, we present K-Ar dating results of fault gouges from the Chongshan shear zone, as well as fission-track thermochronology data from the Gaoligong and Chongshan shear zones. We then compile thermochronologic ages from published studies and model them using the thermo-kinematic code Pecube to constrain their exhumation and deformation history. The compilation indicates that the onset timing of the Gaoligong shear zone is consistent with the southeastward extrusion of Indochina. Modeling results along the Gaoligong and Chongshan shear zones also suggest that rapid rock uplift along the shear zones gradually became younger northwards, which indicates a coeval exhumation history of these two shear zones after the mid-Miocene. In addition, K-Ar dating of the fault gouge suggests a brittle deformation event at ~7 Ma near the bend in the Chongshan shear zone, but without rapid cooling recorded. This may indicate that tectonics may not have been the main reason for exhumation, but that incision of the large rivers is also responsible for rapid exhumation.


SE02-A023 | Invited
Lithospheric Flexural Response to Water Loads and Triggered Seismicity Around a Large Reservoir

Xuhua SHI1+, Yuanhai SHU1, Roland BÜRGMANN2, Lei XIE3, Libo HAN4, Zhongcheng CAO5, Wenbin XU3, Teng WANG5, Guojie MENG6, Austin MADSON7, Eric KIRBY8, Hanlin CHEN1#, Ren-Qi LU4, Qi YAO4, Xiaogan CHENG1, Shufeng YANG1
1Zhejiang University, 2University of California, Berkeley, 3Central South University, 4China Earthquake Administration, 5Peking University, 6Institute of Earthquake Forecasting, China Earthquake Administration, 7University of Wyoming, 8University of North Carolina

The transition to low-carbon energy generation requires a diverse portfolio of energy sources. However, large hydropower stations may pose significant seismic hazard as impoundment of water exerts stresses in the Earth’s crust. The distribution of such earthquakes and causal mechanisms remain largely uncertain. Here, we addressed this question around the world’s 4th largest hydropower station in Xiluodu, China, using interdisciplinary analyses of relocated earthquakes, geodetic data and numerical simulation. The modeled ground deformation pattern due to hydrologic loading at the Xiluodu and Xiangjiaba Reservoirs is consistent with geodetic observations. Approximately 79% of the earthquakes are located within ~15 km of the subsidence center. The events temporally relate to rapid hydrologic loading/unloading periods and their spatiotemporal outward migration may be caused by the viscoelastic relaxation. This work reveals that reservoir-induced flexural deformation may control the distribution of triggered seismicity, highlighting an urgent need to strengthen geohazard monitoring efforts around such structures.


SE02-A011
Imaging Fold Growth from Transverse Drainages: Implications from the Tugerming Anticline in the Southern Tianshan Foreland

Feng LI1+, Xuhua SHI1#, Julien CHARREAU2, Rong YANG1, Xiaogan CHENG1, Jin GE1, Hanlin CHEN1, Jinhan WANG1
1Zhejiang University, 2Université de Lorraine

Folding topography is typical in the foreland landscape. How surface processes interact with growth and lateral linkage of folds remains a leading-edge problem. Here we analyze geomorphic expressions of transverse drainages, a unique feature in particular fold area, together with landscape numerical modeling, to explore how such features respond to the actively growing Tugerming anticline, southern Tian Shan foreland. Based on detailed geomorphic analysis of the Tugerming fold and 14 transverse bedrock rivers along the fold axis, we found that the Tugerming fold grows laterally toward both ends, exhibiting significant along-strike variations in fluvial and geomorphic features among different fold segments. Moreover, both ephemeral and perennial transverse rivers show similar channel morphology in response to changes in local uplift and subsidence when flowing across the growing fold. We find that river-fold interactions are dominated by (1) aggradation processes in upstream and downstream of the fold. Reaches increase their channel sinuosity to decrease the channel slope, and the enhanced aggradation is also marked by high values of valley floor width-to-height ratio (Vfw:Vh); (2) erosion processes flowing across the fold axis, where bedrock channels with high uplift rates and quick variations in bedrock strength. In this case, reaches decrease their channel sinuosity to increase the channel slope, and the enhanced vertical incision capacity is marked by low values of valley floor width-to-height ratio (Vfw:Vh). Our results also suggest that hinterland catchments and possible river network reorganizations should be explicitly considered, which could significantly change the ratio of sediment supply to transport capacity before river flows across the anticlines within foreland. These results illustrate how fluvial geomorphology can be successfully used to understand folding processes along tectonically active mountain fronts.


SE02-A024
Integrated Rupture Mechanics for Slow Slip Events and Earthquakes

Huihui WENG1#+, Jean-Paul AMPUERO2
1Nanjing University, 2Université Côte d’Azur/ National Centre for Scientific Research/ Observatoire de La Cote d’Azur

Slow slip events occur worldwide and could trigger devastating earthquakes, yet it is still debated whether their moment-duration scaling is linear or cubic and a fundamental model unifying slow and fast earthquakes is still lacking. Here, we show that both slow and fast earthquakes can be understood by a new theory of dynamic fracture mechanics. This new theory accounts for an essential ingredient that was missing in previous models and experiments, the “finite seismogenic depth”: the portion of the fault that slides during a large event has a limited depth extent, shorter than its horizontal length. A continuum of rupture speeds, from arbitrarily-slow speeds up to the S-wave speed, is primarily controlled by a non-dimensional energy ratio: the ratio between the available elastic energy and the energy dissipated by fault slip, as predicted by the new theory. We find that shear stress heterogeneity can produce a cubic scaling on a single fault while effective normal stress variability produces a linear scaling on a population of faults, which reconciles the debated scaling relations. This model provides a new framework to explain how slow slip might lead to earthquakes and opens new avenues for seismic hazard assessment integrating seismological, laboratory and theoretical developments.


SE02-A017
Early Quaternary Tectonic Transformation of the Helan Shan: Constraints Due to Quantitative Geomorphology

Yige LI1+, Wenjun ZHENG1#, Yang JINGJUN1, Dongli ZHANG2, Haoyu ZHOU1, Ting LIU1
1Sun Yat-sen University, 2中山大学

The Helan Shan is located on the front edge of the expanding Tibetan Plateau. However, how the topography here responds to this propagation and its precise time constraints remain unknown. Based on the response process of fluvial landforms and tectonic evolution, we conducted a quantitative landform analysis of the Helan Shan region. Here, the spatial distribution features of various geomorphic indices were coupled, demonstrating that the mountain is tilting toward the west and north. The steeper downstream and gentle upper reaches indicate that the fluvial landforms have experienced an accelerated incision event, which can be attributed to the tectonic activity along the East Helan Shan Fault. Furthermore, the response time of the tectonic knickpoints ranges from 0.1 to 1.4 Ma based on the paleochannel reconstruction method. Combined with previous studies on low temperature thermochronology and active tectonics, we proposed a tectonic transformation model where the Helan Shan shifted its tilting from the southwest to the northwest, as induced by the northeast expansion of the Tibetan Plateau from 0.1 to 1.4 Ma.


SE02-A026
Fluvial Response to Differential Activity of the Litang Fault System in Southeast Tibet: Implications for Fault Immaturity and Kinematics Around the Eastern Himalayan Syntaxis

Jinhan WANG+, Xuhua SHI#, Rong YANG, Hanlin CHEN
Zhejiang University

Large and secondary active faults bounding or within the Chuan-Dian block, a major block surrounding the eastern Himalayan syntaxis (EHS) in the southeastern Tibetan Plateau, play important roles in the kinematic and geodynamic evolution of the southeastern Tibetan Plateau. Previous studies mainly focused on large-scale faults (e.g., the arcuate Ganzi and Xianshuihe faults) bounding the Chuan-Dian block, how secondary faults within the block evolve in time and space and affect the landscape evolution, remains largely unknown. Here, we target the Litang fault, slipping left-laterally with a normal component, in the central Chuan-Dian block, to evaluate the fault’s spatial variations in tectonic activity and kinematics, from fluvial geomorphic analyses. Our results of hypsometrical integral, channel steepness, and knickpoint distribution, suggest that the Maoya segment of the Litang fault is most active among its all four (Cuopu, Maoya, Litang and Jiawa from northwest to southeast) segments. The knickpoint migration modeling suggests that knickpoints of the Cuopu and Maoya segments in the northwest formed around 0.37 and 0.58 Ma, respectively, and those of the Litang segment in the southeast around 3.2-1.5 Ma, much earlier than those in the northwest. These observations suggest the northwest younging or propagation of normal-slip faulting. These results together with the geometry and segmentation of the Litang fault, implying that this fault remains immature and its kinematics pattern is likely associated with clockwise crustal rotation around the EHS. We demonstrate that geomorphic evidence, tectonic knickpoint and stream profiles are useful tools to evaluate the activity and spatial-temporal evolution for strike-slip faults with vertical slip component.


SE02-A001
Late-stage Structural Evolution from Near-bottom Topographic and Magnetic Surveys of the Suda Seamount (West Pacific)

Tao WU1#+, Bin SUI2, Chunhui TAO2, Jianping ZHOU2
1Second Institute of Oceanography, Ministry of Natural Resources, 2Ministry of Natural Resources

The late-stage evolution of seamounts is widespread in the West Pacific and may control the distribution of manganese nodules on the lower seamount flanks and adjacent debris aprons. However, due to the paucity of near-bottom observational data, little research exists specifically focused on the late-stage evolution of seamount structures. To fill this knowledge gap, we systematically investigated the tectonic features and evolution of Suda Seamount based on rock samples, magnetic surveys, and high-resolution topographic data. We discovered that the central area of the seamount summit exhibits a negative magnetic anomaly related to a group of minor volcanic structures, while the collapse of volcanic structures on the northeast seamount flank is associated with an extensive positive magnetic anomaly. Surprisingly, we found that a late-stage intrusive dyke with significantly high magnetic susceptibility originates from the lower part of a minor group of volcanic structures but cannot be clearly distinguished below the main summit volcanic structure (hereinafter referred to as the main mound complex). These results demonstrate that at least two late-stage periods of intense magmatic activity occurred during the evolution of the seamount, one centered on the main mound complex and one on the edge of the summit platform. By combining fine-scale topographic and satellite gravity data, we deduce that gravitational slip caused by magma intrusion along a fracture was the main cause of the original seamount flank collapse. The late-stage processes resulted in a change in the seamount morphology and distributed widely clastic rock debris along the flanks, which might contribute to the uneven distribution of manganese nodules along the lower seamount flanks and determine the distribution of subsequently formed nodules.


Tue-01 Aug | 8:15 - 10:00 | MR305
SE17 - General Session

Session Chair(s): J. Bruce H. SHYU, National Taiwan University, Florian M. SCHWANDNER, NASA Ames Research Center

SE17-A022
Seismic Observation of Lithospheric Structure of the Socotra Island Through Interferometry of Teleseismic P Waves

Shenbo YANG1+, Wei WANG1, Jinhai ZHANG2#
1Chinese Academy of Sciences, 2Institute of Geology and Geophysics, Chinese Academy of Sciences

Socotra is the name of an island in the Indian Ocean which is located around 400 kilometer south of the Arabian Peninsula. As suggested by previous results, Socotra Island is part of south margin of the Gulf of Aden, which is considered as the result of the separation of the Arabian Plate and the Somalian Plate at 20-18Ma. Previous receiver function analysis shows that the crustal structure differs from east to west part of the Socotra Island that the crustal thickness decreases from westward. An interpretation that east and west part of the island belong to different divisions of passive rifted margin region respectively was proposed though the results of previous seismic observations are displayed up to 40 kilometers depth and the deeper structure characteristics remain less discussed. The correlation method revealing receiver side structure from teleseismic P waves is considered as the general form of receiver functions and a special case of seismic interferometry and enables us to retrieve P reflections from only vertical component of the records. We conducted seismic interferometry with spectral whitening correlation method by first estimating the incident wavefield from the array stacking then cross correlate the incident wavefield the residual of vertical component subtracted by the incident wavefield and finally obtain the common reflection point(CRP) stacking image with reflecting points calculated with IASP91 model. Our CRP image shows obvious eastward dipping features in consistence with the previous results that shows the crustal thickness decrease westward but up to 80 kilometers depth. Consequently, the deeper structure should also be taken into consideration while discussing the allocation of different parts of the island to different divisions of rifted region.


SE17-A018
Effects of Water on Shear Plane Displacement of Rocks by Means of Visual Measurement System

Takahisa ENDO1#+, Daisuke ASAHINA2, Takato TAKEMURA1
1Nihon University, 2Geological Survey of Japan

On shear planes with large displacements, such as seismogenic faults, asperity rupture is known to trigger fault slip. The fault slip is related to the structural characteristics of the fault (e.g., damage zone) as well as the mechanical conditions (e.g., excess pore pressure) around the shear plane. In order to understand the mechanism of fault slip, it is important to observe and measure the slip processes on the shear plane. In the laboratory, triaxial compression tests and direct shear tests are conducted to reproduce the fault slip. However, the specimen is generally placed in the shear box or into the triaxial chamber in the conventional testing equipment, and visual information about the specimens cannot be obtained. We have recently developed the visual measurement system using a camera to observe the mechanical behavior of the specimen. The system visually captured the shear behavior of the specimens which have shear plane, and it can observe the changing of the shear behavior with the water. In addition, using digital image correlation (DIC), we have succeeded in visualizing the details of the mechanical behavior of the specimen. The DIC results show more local displacements or strain distributions of the specimens’ surface than the measurements from various sensors.


SE17-A012
Quantitative Evaluation of Overpressure Increased by Tectonic Compression Stress and Its Significance -A Case Study from Dabei Field in Kuqa Depression

Gang WANG#+
Northwest University

The overpressure increased by tectonic compression stress (OITCS) plays important roles in influencing deformation of rocks, triggering seismic events, and controlling migration and accumulation of hydrocarbon in sedimentary basin. Generally, the process of tectonic compression can be divided into three stages including initial layer-parallel shortening strain, folding and faulting. The OITCS mainly occurs at the first two stages. While rocks rupture, the tectonic stress and fluid pressure would decouple due to overpressure transfer and stress release. On the basis of geomechanical model construction, we developed a new method for quantitative estimating the OITCS. The new method considers the process of volumetric strain and distortion of rock in maximum, minimum horizontal and vertical stress regime and has strong feasibility and practical applicability. The application of the new method in the thrust belt of Dabei Gas Field suggests that (1) the OITCS can significantly increase the fluid pressure and reduce the friction coefficient of tectonic activity, (2) the intense OITCS made the strata deformed and formed a series of anticlines which offered the traps for hydrocarbon accumulation, (3) the OITCS enhanced the driving power for hydrocarbon migrating into tight reservoir and leaded to the forming of enriched Dabei Gas Field.


SE17-A023
Three-dimensional Body Wave Attenuation Structure of the Gofar Transform Fault, East Pacific Rise

Jing HU#+
Chang‘an University

The westernmost Gofar transform fault (GTF) can generate large earthquakes (Mw ~6.0) quasi-periodically every 5~6 years, which are not able to rupture the whole fault. Previous studies of the local seismicity and seismic P- and S-wave velocity tomography have shown that the fault structure plays an important role to control the rupture process of large earthquakes and the distribution of local micro-seismicity, which shows that there would be variations of material properties along GTF. However, seismic behavior mechanism is still unclear. To better understand the relationship between seismic behavior mechanism and GTF zone seismic attenuation structure which is greatly sensitive to the underground fluid, crack and temperature. In this study, we have collected high resolution relocated catalog and corresponding seismic waveforms and three-dimensional (3-D) P- and S-wave velocity obtained from (Guo et al., 2018) to invert 3-D P- and S-wave attenuation structure around the GTF area. We will explore the possible seismic behavior mechanism by through combining obtained attenuation model with seismic velocity model and local seismicity.


SE17-A016
Characteristics of the First Higher-mode Ambient Noise Rayleigh Waves Observed in Taiwan Island

Chun-Fu LIAO1,2+, Ying-Nien CHEN1#, Yuancheng GUNG2
1National Chung Cheng University, 2National Taiwan University

Resulting from the energy exchange between ocean waves and solid earth, microseisms, namely, ambient noise, are the dominant signals in seismic records. Various studies pointed out that the fundamental mode surface waves are the most predominant oscillations in microseisms, while under some particular weather conditions or geological structures, body waves and higher-mode surface waves could be triggered efficiently. Previous noise studies in Taiwan reported that in the frequency band 0.03~0.5 Hz, noise interferograms of the vertical component only reveal the empirical Green’s functions of the fundamental mode surface waves. Utilizing multicomponent interferometry, we show that the 1st higher-mode and fundamental mode Rayleigh waves could coexist in the frequency band of the short period secondary microseisms (SPSM, 0.2-0.5 Hz). The combination of a dense seismic array and the diversity in geology and bathymetry of Taiwan Island provides a unique opportunity to investigate the excitation mechanisms of the 1st higher-mode ambient noise surface waves. Based on the spatial-temporal analysis of interferograms, the amplitudes of the 1st higher-mode and fundamental mode ambient noise Rayleigh waves are influenced by surrounding ocean settings and the monsoon system. Moreover, the spatial distribution of the amplitude ratio between the 1st higher-mode and fundamental mode Rayleigh waves is correlated to the shallow structures of Taiwan Island. With dispersion measurements, we show that the published velocity models tend to overestimate velocities of the shallow crust in the western plains of Taiwan. Based on the new dataset proposed in this study, we could probe shallow structures in detail in a near future.


SE17-A028
Novel Autonomous and Cabled Ocean Bottom Seismometer Solutions for Offshore Seismic Research

Ella PRICE#, James LINDSEY, Neil WATKISS+, Phil HILL
Guralp Systems Ltd

Seismologists have historically focused on land-based seismic research, due to the logistical and financial challenges presented by offshore installations. Guralp 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 allow users flexibility in deployment and ability to redeploy in different locations. The Guralp 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. These features allow researchers to monitor and transmit data without offshore cabling, reducing logistical challenges whilst maintaining some degree of real-time data transmission. Alternatively, cabled solutions give users access to high-resolution data in real-time via a physical link to an onshore data centre. As an example, the Guralp 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. Guralp is deploying a demonstration SMART Cable system to monitor volcanic and seismic activity offshore 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.


SE17-A006
A New Broad-band Seismometer for Seismicity Monitoring and Passive Seismic Acquisition: Design, Modeling and Evaluation

Nikos GERMENIS#+
GEObit-Instruments

A new, improved approach in the design of a compact digital broadband seismometer is presented. Each sensing element (seismic sensor) of the proposed seismometer is based on a modified seismic accelerometer followed by a continuous time integrator for providing velocity voltage output. It has a broadband response, flat in velocity from 120s to 75Hz, high sensitivity 1500V/(m/s) and 40Vpp differential output range. Other configurations like 60s to 100Hz and 30s to 120Hz are also available. The acceleration integration method provides high performance at low frequencies, with self-noise well below the New Low Noise Model at the range 80s ‒ 16Hz. The mechanical system provides a perfectly linear response of its displacement sensing system. Evaluation, classification, and noise determination of the presented instrument are performed in terms of direct experimental measurements, simulations and calculations based on raw data from the proposed sensor and from a commercial product with approximately equivalent performance. Additionally, the performance in earth ambient noise recording of these broad-band sensors is demonstrated followed by a comparison with the performance of two electrodynamic sensors, one with bandwidth of 20sec to 50Hz and a single geophone with corner frequency  4.5Hz.


Tue-01 Aug | 8:15 - 10:00 | MR306
SE10 - Advances in Satellite-based Techniques for Earth and Environmental Hazards Monitoring

Session Chair(s): Jeffrey T. FREYMUELLER, Michigan State University, Antonio PEPE, Italian National Research Council, Aron MELTZNER, Nanyang Technological University

SE10-A001
Machine Learning Classification of Crop Types Using AVIRIS-NG Hyperspectral Remote Sensing Data

Prachi SINGH1+, Prashant K. SRIVASTAVA1#, Rajesh MALL1, Jochem VERRELST2, George P. PETROPOULOS3
1Banaras Hindu University, 2Universitat de València, 3Harokopio University of Athens

Hyperspectral remote sensing technology with narrow contiguous spectral bands can prove useful in a significant spectral measurement capability over the conventional remote sensor systems and hence holds great capability in discriminating different crop types. The main objective of the present study is to assess and compare the potential use of Airborne Visible /Infrared Imaging Spectrometer-New Generation (AVIRIS-NG) data for discriminating different crop types growing in Anand district, Gujarat. Various types of supervised machine learning classification algorithms namely Discriminant Analysis, Ensemble Learning, and Random Forest (RF) i.e. were applied to AVIRIS-NG data. Thirteen crop type classes namely Bajra, Banana, Brinjal, Cabbage, Chickpea, Chicory, Chilli, Cowpea, Fennel, wheat, Maize, Tobacco, Sorghum, Linseed, Castor, Pigeon pea, Fennel and Chickpea were identified. The performance of selected supervised classifiers was assessed using overall accuracy and kappa coefficient. SVM (Support Vector Machine) technique yielded better overall accuracies and kappa coefficients compared to other machine learning classifiers. Overall accuracy and Kappa coefficient for SVM it is 94.42% and 0.94 respectively. The results of the present study highlight the significance of hyperspectral data in discriminating crop types of an area.


SE10-A003
Assessment of Coastal Subsidence and Inundation Risk Due to Sea Level Rise in Kerala, India, Using MT-InSAR Technique

Aparna R#+, Chandrakanta OJHA
Indian Institute of Science Education and Research Mohali

The coastal state of Kerala, due to its varied geographical features, has been experiencing several natural hazards in the past few decades. However, the coastal subsidence by natural and anthropogenic processes, whose compounding effect with sea level rises (SLR), contributes to the relative sea level (RSL) change and exacerbates future coastal hazards. This study aims to analyze the vertical land motion (VLM) over the Kerala coast, which is spread across 589.5 kilometers from Kasargod to Thiruvananthapuram, using Multi-temporal Interferometric Synthetic Aperture Radar (MT-InSAR) technique and combining the results with the tide gauge data to study the relative sea level rise and mapping the flood inundation regions. For VLM, descending (DSC) pass data from the Sentinel-1 satellite of the European Space Agency (ESA) has been used in the study. 840 scenes of 17 different frames from two different paths; 63 and 165, are used in the continuous and accurate monitoring of land subsidence over the region from 2017 to 2022. The VLM result obtained from path 165 depicts the wetlands of the Kuttanad region, known as the ‘rice bowl of Kerala', experiencing a maximum subsidence rate of 40 mm/year, which is vulnerable to future flood inundation due to the SLR. Similarly, from NASA’s Intergovernmental Panel on Climate Change (IPCC) AR6 report, the SLR along the Cochin region of Kerala projected 0.71 meter till 2100 using the socioeconomic scenario SSP3-7.0, and the local RSL trend of 1.54 ± 0.27 mm/year from 1939 to 2013 using the tide gauge station. However, we are further investigating the VLM map along the entire coastline of Kerala and analyzing the SLR data to map vulnerable flood inundation regions. This will help policymakers to take precautionary measures to avoid coastal disasters and minimize potential future socio-economic losses.


SE10-A004
Comparison of GNSS and InSAR Measurements for Crustal Deformation Caused by the 2021 Alaska Earthquake

Akino NAITOH#+, Toshitaka BABA
Tokushima University

The Alaska-Aleutian subduction zone is one of the most seismically active regions, where the Pacific plate subducts beneath the North American plate. An Mw 8.2 earthquake occurred on the plate interface at a depth of 35 km in 2021 (hereafter, the 2021 Alaska earthquake). The crustal deformation caused by this earthquake was estimated by land-based GNSS observation networks but not yet by InSAR. InSAR analysis may enable us to detect small-scale deformations caused by secondary fault movement, landslides, etc. This study, therefore, applied InSAR analysis to the 2021 Alaska earthquake to obtain spatial continuous crustal deformation. We used PALSAR-2 data on ALOS-2 satellite. InSAR image showed that the crustal displacement near the epicenter was about 30 cm away in the satellite line-of-sight direction. We compared these displacements estimated from InSAR with those from the GNSS observation networks. However, there was a non-negligible difference of about 7 cm to 16 cm between InSAR and GNSS estimations. This difference may be because the InSAR analysis included long-wavelength errors for various reasons, such as disturbances in the ionosphere. Therefore, we successfully obtained the spatially continuous crustal deformation of the 2021 Alaska earthquake from the InSAR analysis. The result indicated that the land near the epicenter moved away from the satellite by about 20 cm in the satellite's line-of-sight direction. There still was no small-scale deformation such as secondary fault movement, landslide, etc. Even with the GNSS-corrected InSAR estimates, there was a difference (about 9 cm~27 cm) from the GNSS observations at Sand Point, Nagai Island, and Charnabula Island. This difference is due to the proximity of the ocean, which is a non-interference area.


SE10-A005
Assessment of Land Subsidence and Groundwater Depletion Using InSAR Technique Over Jodhpur City, Rajasthan, India

Pooja DHAYAL#, Chandrakanta OJHA+
Indian Institute of Science Education and Research Mohali

Groundwater (GW) depletion is becoming a significant concern across the world. In India, GW is used for more than 60% of irrigation and 85% of drinking water purposes. In a state like Rajasthan, due to extreme climate change, over-extraction of underground resources for agriculture and industrial purpose leads to a significant decline in groundwater levels. Eastern and western Rajasthan are the most susceptible to drought. However, over-exploitation of GW may cause land subsidence and leads to infrastructure damage, hence requiring a frequent monitoring system. In that context, this study focuses on Jodhpur, a metropolitan and iconic historical city of Rajasthan. We used a multi-temporal interferometry technique (MT-InSAR) for measuring land subsidence and correlating GW data for groundwater dynamics. The city experienced average rainfall of about 337 mm from 2000 to 2021, much less than the national average, with the lowest one observed, 87.58 mm in 2002 and a maximum of 461.87 mm in 2010. Analyzing 21 years of GW data, we observed a five mbgl decline in groundwater level. In particular, well stations Kairu and Narwa, located in the western part of Jodhpur city, show negative decline rates of -0.16 mbgl/yr and -0.14 mbgl/yr, respectively. Similarly, the Gangani and Kuri regions in the northeast part of the city show a GW rate of about 0.023 mbgl/yr. For InSAR deformation analysis, we select 144 SAR imageries from the P107 descending orbital track of Sentinel-1A from Mar 2017 to Dec 2021. The data were processed using the Small BAseline Subset (SBAS) technique using the GMTSAR tool by Sandell et al., 2011. We noticed 90 to 100 mm of land subsidence in the western and central parts of Jodhpur city, which shows a good correlation with the head-level decline in the region.


SE10-A011
Subsidence of Islands Across the Pacific Due to Global Loading Deformation from Present-day Mass Redistribution and Glacial Isostatic Adjustment

Jeffrey T. FREYMUELLER#+, Katarina VANCE
Michigan State University

GPS sites on islands across the Pacific are observed to subside systematically, although at low subsidence rates, based on the analysis of continuous GPS data. Some of this subsidence can be explained as being due to very long-wavelength (global) signals such as Glacial Isostatic Adjustment (GIA) and the effects of present-day mass redistribution produce global deformation patterns. Although small signals, they are not insignificant compared to the precision and accuracy of modern GNSS data. For example, across most of the Pacific, both GIA and present-day mass redistribution predict subsidence rates of a few to several tenths of a mm/yr; the combined signal approaches 1 mm/yr. Accurately accounting for small long-wavelength signals can be important in discriminating between alternate models of local signals such as deep volcanic processes or ongoing flexural loading. For example, in Hawaii, all GPS sites far from the currently active volcanoes show an additional subsidence signal likely caused either by ongoing flexural loading under the growing volcanic load, or dynamics of the deep magma system. We use a variety of GIA models for which the predicted 3D velocities are available, and also recent present-day mass loading models. For the Pacific, the subsidence predicted by the sum of present-day mass loading and GIA predicts a regional subsidence signal similar to that we observe. The displacements due to present-day mass loading are time-dependent and have an overall trend. At present, the year to year variations appear to be lower than the noise level for Pacific island sites, but not for locations closer to the changing glacial loads such as the North Atlantic. We are continuing to investigate whether existing models are accurate enough to use them for calibration to remove long-wavelength effects.


SE10-A009 | Invited
A Daily Grace Solution After Removing Residual Aliasing via Combined Gravity Field Modeling

Yunzhong SHEN#+, Qiujie CHEN, Yufeng NIE
Tongji University

To reduce the residual aliasing leakage after the non-tidal atmosphere and ocean mass variability is corrected with the AOD1B RL06 model from Dobslaw et al. (2017), the Earth’s gravity field model is combinedly modeled, where the spherical harmonic (SH) coefficients up to degree and order (d/o) 6 are expressed with a daily periodical function and the rest parts are denoted with monthly mean SH coefficients. Then the combined gravity field model is solved with the observations of the satellite mission of gravity recovery and climate exploration (GRACE). The results show that the SH coefficients are significantly improved in the combined GRACE solution, especially in the higher d/o coefficients. Furthermore, after the daily variation signals are removed from the observations, a daily GRACE gravity field model is computed with the daily GRACE observations via the adaptive regularization approach, in which the covariance matrix of the monthly solution is taken as the regularization matrix and the multiple regularization parameters are adaptively determined. Due to removing the residual aliasing effects, the quality of the daily GRACE solution will be improved as expected.


SE10-A007
Investigating Land Subsidence Exploring Sentinel-1 Data Using MT-InSAR Technique Over Mumbai City, India

Chandrakanta OJHA1#+, Divya Sekhar VAKA2, Antonio PEPE3, Yalamanchili SUBRAHMANYESWARA RAO2
1Indian Institute of Science Education and Research Mohali, 2Indian Institute of Technology Bombay, 3Italian National Research Council

In the era of climate change and rapid urbanization, increasing anthropogenic activities lead to geo-hazard phenomena across various coastal cities worldwide. Last few decades, Mumbai city, one of the most populous metropolitan cities in India, has been rapidly developing its infrastructure and exploiting groundwater resources for industrialization and daily purpose, which led to local-scale subsidence and may cause future infrastructure damage. However, a frequent monitoring mechanism has yet to be established to observe the city's local to regional subsidence. In this context, the research focuses on exploring Sentinel-1 (S1) data of the Europeans Space Agency using an advanced multi-temporal interferometric synthetic aperture radar (MT-InSAR) methodology (Berardino et al., 2002) for deformation monitoring over the Mumbai. Here, we considered 136 imageries of the S1-A descending pass collected from September 2016 to October 2021. The applied methodology follows through several systematic steps, including SAR image co-registration through a reference image (9 June 2018), followed by a multi-looking factor (8x2 along azimuth x range), interferogram generation (using spatial and temporal baselines thresholds of 100 m and 48 days), topographic correction (using 30 m SRTM-DEM), multi-temporal EMCF-based phase unwrapping (Pepe and Lanari, 2006), and atmospheric phase screening (Lundgren et al., 2001). The unwrapped interferograms undergo least-square inversion (using SVD) to generate a deformation velocity map and displacement time series along the line-of-sight direction. The result shows greater subsidence in four distinct areas in the metro city, which include Wadala East (~20 mm/yr), Shivaji Nagar (~15 mm/yr), Navi Mumbai international airport (~15 mm/yr), and Jawaharlal Nehru Port Trust (JNPT) Navi Mumbai (~15 mm/yr). We further noticed about 4 mm/yr of coastal subsidence in various places along the city coast, which is vulnerable to future coastal inundation with the impact of relative sea level rise.


Tue-01 Aug | 1:00 - 5:15 | Summit
SE - Solid Earth Sciences Poster Session

SE01-A006
Mineralogical and Geochemical Occurrence of Mercury in Mine Tailings from Abandoned Mercury Mine in Palawan: Implications in Environmental Impact

Alexandria TANCIONGCO1,2#+, Jessie SAMANIEGO3, Gawen JENKIN4, Carlo ARCILLA1, Leon HICKS4, Vimalnath SELVARAJ4, Cris Reven GIBAGA3, Rico Neil QUIERREZ3
1University of the Philippines Diliman, Philippines, 2University of the Philippines Diliman, Philippines, 3Philippine Nuclear Research Institute, Philippines, 4University of Leicester, United Kingdom

One of the legacy mines in the Philippines, a mercury mine in Puerto Princesa City in Palawan Island, was operated by the Palawan Quicksilver Mines Inc. (PQMI) from 1953 to 1976. The tailings left behind was processed through calcination and was allegedly dumped in the jetty port in Honda Bay and surrounding villages. In this paper, the mineralogy and geochemistry of Hg is analyzed from sediments of three alleged mine waste dumping areas surrounding PQMI, namely, from the Honda Bay Wharf (HBW), from Sitio Matahimik (SMK; the village 300 meters away from former open pit site) and from the Puerto Princesa City Landfill (PPCL). Based on grain size analysis, the sediments with size less than 63µm show the highest mercury concentration reaching up to 885 ppm in SMK. Through automated scanning electron microscopy energy-dispersive X-ray spectroscopy (SEM-EDS) analysis of composition, Hg is found to occur in mercury sulfides (HgS, cinnabar) surrounded by ferric oxide minerals and silica for all sampling sites. The cinnabar grains from both SMK and PPCL are relatively large (10µm size) and do not contain visible zoning, indicating that no processing had occurred while grains from HBW are smaller (<2µm) and broken in textural form. It is inferred that the “mine wastes” dumped in SMK and PPCL are the low-grade ore materials that did not pass the cut-off grade while those in HBW are the calcined ores. From these findings, it was confirmed that the finer grain size fractions that are more prone to inhalation through dust are concentrated with cinnabar minerals. Meanwhile, lower HgS amount in HBW occurring within goethite phases assures low biotoxicity of the metal provided it is not reacted with acidic water. This study contributes to the current knowledge in abandoned mine tailings in the Philippines and its implications in mine environmental safety.


SE02-A006
Late Quaternary Tectonic Activity of NW-trending Elashan Fault in the Ne Margin of the Tibetan Plateau and Implications for Plateau Deformation Mechanism

Zhikun REN1#+, Jinrui LIU2, Wei MIN2, Zhimin LI3, Dengyun WU2
1Institute of Geology, China Earthquake Administration, China, 2China Earthquake Administration, China, 3Earthquake Administration of Qinghai Province, China

Due to the effects of India-Eurasia convergence, the northeast margin of the Tibetan Plateau still has complex and intense deformation, which can be the best natural laboratory to study the expansion and growth process of the Tibetan Plateau. The main fault system around Qinghai Lake block are EW-trending Haiyuan and Kunlun faults, and NNW-trending Elashan and Riyueshan faults. The strain partitioning and seismic hazard in this faults system are pivotal to understanding the fault interaction, and also the key to deciphering the kinematic mechanism of the northeastern margin of the Tibetan Plateau. However, the slip rates of the Elashan and Riyueshan faults are still controversial, and their role in the growth and expansion of the plateau is still unclear. Therefore, we target the NNW-trending Elashan fault and use multiple levels of high-resolution topography data, including DEMs generated from WorldView and GF-7 stereo pairs of satellite images, unmanned aerial vehicle (UAV)-derived DEMs, to interpret its detailed and fine geometry. Furthermore, combining optically stimulated luminescence (OSL), radiocarbon, and cosmogenic isotope dating methods, we constrained the late Quaternary slip rates of the north and south segments of the Elashan fault to be ~1.5-2.5 mm/yr and ~3-4 mm/yr, separately. We suggest that the Elashan and the Riyueshan faults are the result of adjusting the difference between the high shear rate of the Kunlun fault and the low shear rate of the Haiyuan fault, and are a way of accommodating continuum deformation between the major EW-trending fault systems.


SE02-A010
Quantitative Landscape Analysis of Eastern Cape York Peninsula, Australia

Kangqiao CHEN1#+, Renjie ZHOU1, Tara JONELL2
1The University of Queensland, Australia, 2The University of Glasgow, United Kingdom

Cape York Peninsula (CYP) in tropical far north Queensland in Australia is the northernmost extension of the Great Dividing Range, a section of the East Australian passive margin created during opening of the Tasman Sea. This section of the Great Dividing Range is tectonically unique because of the ongoing collision to the north in Papua New Guinea. Influenced by a combination of tectonic and climatic processes, landscape dynamics in CYP are complex yet offer a natural laboratory in which to study their interaction. To explore landscape controls in CYP, it is essential to first fundamentally characterise the landscape. We derive a range of maps including the slope map, relief map, basin distribution and network maps from the SRTM 90-m DEMs. We also use SRTM 90-m DEMs with TopoToolbox 2.0 and RStudio to generate swath profiles, longitudinal profiles, hypsometric curves, slope-elevation plots, normalized steepness-lithology plots, elevation-lithology plots and slope-lithology plots. Our preliminary data suggests that igneous and high-grade metamorphic rock units, ranging from Proterozoic to Cretaceous in age, are correlated with steep and rough landscape. Results also show that lithology dictates highland and escarpment locations, along with catchment-wide geometric features. This study highlights how catchments are characterised under the tropical climate and northeastern Australian passive margin tectonism.


SE02-A020
The Impact of the 2018 Lombok Earthquake Sequence, Indonesia on the Unrest Rinjani-Samalas Volcanic Complex Inferred from the Time-dependent Seismic and Volcanic Source Models

Siyuan ZHAO#+, Simon MCCLUSKY, Meghan MILLER, Phil CUMMINS
Australian National University, Australia

In 2018, four deadly (Mw 6.2 to 6.9) earthquakes struck the north coast of Lombok Island, on 28 July, 5 August, and 19 August, distributed between the Flores back-arc thrust and the Rinjani-Samalas volcanic complex. We performed a comprehensive analysis of relocated aftershocks, static coulomb stress changes, and co-seismic and post-seismic deformation, to improve our understanding of this earthquake sequence. The fault geometries and slip distributions of the three mainshocks are modelled by inverting the co-seismic deformation imaged using an interferometric analysis of Sentinel-1 InSAR measurements, based on a multi-layered elastic half-space. The earthquake sequence aftershocks were analysed using an unsupervised learning method (ST-DBSCAN) to cluster these relocated aftershocks so that we can identify the source of each aftershock. We perform an InSAR time-serie analysis to investigate the time-dependent post-seismic deformation in the two years following the Lombok 2018 earthquake sequence, deriving a combined model that simulates the viscoelastic relaxation and afterslip simultaneously. The Coulomb stress change modelling based on the co-seismic and post-seismic rupture models indicates the stress change around the Barujari Crater region, which affects the open of the magma conduct, reflected as edifice-scale deflation and inflation. To quantify the influence of the earthquake sequence on the spatiotemporal deformation pattern of the volcano edifice, we extended our InSAR time-series range forward to the year 2014, just prior to the two eruptions that occurred on 25th October 2015 and 1st August 2016, and perform Principal Component Analysis to investigate the time-dependent inflation and deflation signals. We modelled the volume change and the location of the volcano pressure source for a better understanding of how changes in the magma body and magma movement may have been influenced by the 2018 Lombok earthquake sequence. A double-source compound model is used to invert the parameters of the magma chamber.


SE03-A013
Discovery of Volcaniclastic Deposits on the Eastern Wall of Aso Caldera (SW Japan): Implications for Characteristics and Frequency of Holocene Mass Movement in the Central Kyushu Region

Yasuo MIYABUCHI1#+, Hideo HOSHIZUMI2
1Kumamoto University, Japan, 2Geological Survey of Japan, Japan

Several volcaniclastic deposits discovered at the foot of the eastern wall of Aso caldera, central Kyushu, southwestern Japan, are divided into two types: lahar deposits (Lh1–Lh5 in descending order), which contain abundant subangular to subrounded lithic clasts (<3.5 m in diameter) set in a sandy to silty matrix, and debris avalanche deposits (DA1 and DA2), which include numerous plastically deformed fragments of tephra (ash and scoria) and soil layers in a homogenous silty to clay matrix. DA2, which underlies a paleosol dated at 5.4 cal ka BP (calibrated 14C age), is the largest volcaniclastic deposit observed in the section (more than 2.5 m thick and about 70 m wide). Because the debris avalanche deposits display no evidence that they were transported by water, they are likely to have originated from landslides triggered by intense earthquakes. Tephra chronology and 14C-dating on paleosols along the succession suggest that lahars occurred once over 900 years (6.3–5.4 cal ka BP), three times over 1400 years (5.4–4 cal ka BP), once over 400 years (4–3.6 cal ka BP) and twice (including the 2012 lahar) in the last 3600 years. This evidence indicates that the lahars occurred at an interval of 400–1800 years. In contrast, two debris avalanche deposits exist in the same succession spanning the last 6300 years. Including landslides and associated debris avalanches triggered by the 2016 Kumamoto earthquake (Mj 7.3), landslides generating debris avalanches in the Aso caldera occurred at least three times in the last 6300 years. This may suggest the frequency of large earthquakes triggering debris avalanches in the central Kyushu region, which has many active faults.


SE05-A004
Numerical Modeling on the Growth Dynamics of Fold-and-thrust Belts in the NE Margin of the Tibetan Plateau

Qizhi CHEN1,2+, Caibo HU1,1#, Felipe ORELLANA-ROVIROSA3, Yaolin SHI1
1University of Chinese Academy of Sciences, China, 2University of Chinese Academy of Sciences, China, 3Southern China University of Science and Technology, China

The NE margin of the Tibetan Plateau, as the leading edge of the northeastward growth and expansion of the Tibetan Plateau, formed a series of horizontally-arcuate structural belts since the late Cenozoic, and additionally, several historical, strong earthquakes have occurred here. We present a series of 3D-time-dependent finite-element models with elasto-plastic and frictional nonlinearities to understand the formation-evolution of arcuate folds here comprising real regional fault-zones including the Haiyuan, Xiang Shan–Tianjing Shan, Yantong Shan, and Niushou Shan faults since about ~10 Ma. Our reference simulation, having adequate parameter values from the available literature plus suitable boundary conditions for the region, produces four distinct major EPS concentration zones that are horizontally arcuate and developed outwardly-NE in spatio-temporal sequence, and symmetrically-perpendicular to the contraction direction. These major plasticity bands are spatially highly-correlated with the main regional geologic faults: Haiyuan fault, Xiang Shan–Tianjing Shan fault, Yantong Shan fault, and Niushou Shan fault on the NE margin of the Qinghai–Tibetan Plateau. Our reference-model-based sensitivity analysis suggest that the horizontal northeastward pushing-advancement-contraction of the region being bounded by a frictional vicinity (rigid Alxa and Ordos blocks hindering the advancement) have the dominant control on the formation and evolution of these arcuate fold-and-thrust belts perpendicular to the contraction axis, while the rotations imprinted by the Ordos and Alxa blocks and the shearing of the Qinghai–Tibetan Plateau, have only secondary effects. An additional, generic sensitivity analysis reveals that the folds’ horizontal curvature per unit horizontal shortening-displacement increases with the friction on the bounding vicinity, and this result could be considered for other Earth scenarios and planets.


SE05-A008
Intracontinental Multi-stage Deformation of the Langshan Tectonic Belt on the Western Margin of the North China Craton

Liyun ZHOU1#+, Yu WANG2
1China University of Geosciences (Beijing), China, 2China University of Geosciences, China

Precise dating of multiple-stage deformation in intracontinental settings and during cratonic destruction is difficult to achieve, and understanding the mechanisms involved is challenging. After various assemblies of microcontinents in the late Paleozoic, west and east China underwent different intracontinental tectonic evolutions with various tectonic frameworks on either side of the N–S-trending Helanshan–Liupan–Xueshan tectonic belt. The Langshan area in the northern part of this tectonic belt records a variety of tectonic mechanisms and evolutionary processes. During the Mesozoic–Cenozoic, at least four stages of deformation occurred along the belt, including (1) thrusting towards the south, which involved the crystalline basement and accompanied followed the emplacement of voluminous granitic rocks; (2) transpression, which produced NE–SW strike-slip faults and ductile shear zones as a result of NW-verging ductile compression; (3) NW-to-SE thrust faulting, which thrust the crystalline basement over Cretaceous strata; and (4) Cenozoic E–W extension, high-angle normal faulting, and rift basin formation. Zircon U–Pb LA–ICP–MS dating, as well as 40Ar/39Ar dating of synkinematic muscovite, sericite, and deformed biotite, yielded Mesozoic time constraints so that (1) N–S contraction occurred at 242–206 Ma, slightly later than the intrusion of granites at 242–234 Ma; (2) NE–SW-sinistral strike-slip motions and NW-verging compression took place at 183–160 Ma; (3) NW–SE contraction took place at 126–117 Ma; and (4) high-angle normal faulting occurred at 15–13 Ma (apatite fission track dating). The tectonic stresses involved were all far-field effects transmitted from continental margins. The N–S-trending tectonic belt marks the geographic boundary between west and east China, and it played the role of a weak zone in the crust that was reactivated repeatedly in response to a variety of distant tectonic events, and it therefore records a complex history of tectonic activity.


SE05-A009
Sedimentology and Provenance of Late Cretaceous Basins in the Sichuan-Hubei-Hunan Fold-thrust Belt, South China: A Record of Intracontinental Deformation

Qihui ZHANG1+, Liang QIU2#, Dan-Ping YAN 1, Minglong LI 3, Tao YANG 1, Shahnawaz ARISER4, Boyong YANG3, Xuesong ZHAO 3
1China University of Geosciences, China, 2China University of Geosciences (Beijing), China, 3Hubei Geological Bureau, China, 4Geological Survey of Pakistan, Pakistan

Plate tectonics theory assumes that the interior of the continent is rigid and difficult to deform. However, previous studies on the early Mesozoic strata in South China Block have verified the process of intracontinental deformation by using paleomagnetism, geochronology, and structural analysis. Sedimentology and provenance of basins also well record the intracontinental deformation. This paper presents detailed sedimentology, paleocurrent direction, sandstone component, and heavy minerals of the Jianshi, Enshi, Qianjiang, and Laifeng basins in the South China Block. Late Cretaceous red sandstone strata are principal across the study area and unconformably overlie the underlying strata. The sandstones contain abundant quartz with minor amounts of feldspar and lithic fragments. The spatial variation of the zircon-tourmaline-rutile (ZTR) index suggests that the Jianshi basin is nearer to the main source area than the Laifeng basin. The sediments of these basins show a high proportion of hematite, magnetite, ilmenite, pyrite, leucoxene, zircon (round), rutile, garnet, and epidote. The NW-trending paleocurrent and the parent rock type of mainly intermediate-basic magmatic rocks reflect that the Dabashan fold-thrust belt becomes the main source area. The increase of apatite content in Qianjiang basin and the SE-trending paleocurrent indicate that Xuefeng orogenic belt also provides potential sources. Provenance analysis results combined with previous geochronological data prove the uplift and denudation of Dabashan fold-thrust belt and Xuefeng orogenic belt in the Late Cretaceous. In addition, the normal faults control the deposition of the Jianshi, Enshi, and Laifeng basins, indicating that the Sichuan-Hubei-Hunan fold-thrust belt experienced extension in the Late Cretaceous.


SE05-A010
Molybdenum and Boron Isotopic Evidence for Carbon-recycling via Carbonate Dissolution in Subduction Zones

Yunying ZHANG1#+, Min SUN2, Chao YUAN3, Zhen SUN3, Qian LIU4
1South China Sea Institute of Oceanology, Chinese Academy of Sciences, China, 2The University of Hong Kong, Hong Kong SAR, 3Chinese Academy of Sciences, China, 4Northwest University, China

Subduction zones are critical sites for carbon recycling between the earth surface and interior, which modulate the global carbon budget and influence Earth’s climate. To balance the carbon flux in subduction zones, carbon release through dissolution of carbonate minerals has been highlighted based on recent studies of fluid inclusions in high-pressure metamorphic rocks. However, the lack of direct evidence from arc lavas hampers our understanding of carbonate dissolution. Besides, it remains unclear to what extent the subducted carbonates can be recycled back to the overriding plate. To explore the role of slab-derived fluids in the deep carbon cycle, herein we report Mo and B isotopic data for Silurian arc andesites (426 Ma) and adakitic andesites (422 Ma) from the Chinese Tianshan, which represent partial melts of fluid-modified mantle wedge and dehydrated oceanic crust, respectively. The arc andesites yielded δ98Mo values (0.33–1.08‰) significantly higher than that (about –0.20‰) of the depleted mantle, which could be ascribed to the incorporation of crustal material with heavy Mo isotopes in the mantle source. Since marine carbonate is featured by both heavy Mo and B isotopes and our arc andesites also give heavy δ11B (–1.63 to +4.00‰) values, we consider that marine carbonate was possibly involved as a component of the subducted slab. In contrast, the younger adakitic andesites have light δ98Mo (–0.48 to –0.27‰) and δ11B (–9.43 to –2.05‰) values, implying an isotopically Mo- and B-light source without carbonate signature. Given the preferential transport of heavy 98Mo and 11B to the fluid phase during slab dehydration, their remarkably light δ98Mo and δ11B values support a dehydrated oceanic crust as their magma source. The contrasting Mo–B isotopes for such two kinds of andesites highlight that most carbonates can be removed from the subducted slab to the overriding plate during oceanic subduction.


SE05-A011
Formation of Shear Bands in Foliated Granitic Rocks: A Field-based Analysis

Nandini CHOUDHURY1#+, Atin Kumar MITRA1, Nibir MANDAL2
1Indian Institute of Engineering Science and Technology, India, 2Jadavpur University, India

Micro- to macro-scale shear bands are quite common signatures of tectonic deformations in most of the granitic gneissic terrains, and they play a crucial role in syn-kinematic material transport processes during high-temperature metamorphic segregations. Understanding the mechanisms of their formation is thus important to theorize a range of petrological as well as structural phenomena. This study reports shear bands from strongly anisotropic foliated rocks in granite gneisses of the Chotonagpur Granite Gneissic Complex (CGGC), with an aim to show the mechanisms of their formation in association with fold structures produced by buckling instability. Realignment of mineral grains during the buckle-induced microfolds has resulted in the localization of discrete weak planes, which ultimately define a new set of mineral fabrics that completely obliterated the earlier fabrics. Using field correlations we recognize the initiation of shear bands during this structural transformation and their growth with progressive deformations. In CGGC the gneissic foliations are often asymmetrically buckled, where the short limbs of the consecutive folded layers show intense shear localization, forming a shear band structure. Moreover, some shear bands have been observed to be associated with kink band geometry. This article presents the characteristic features of these types of bands.


SE05-A012
Differential Uplift of Granite Mass in the Basu Region of the Eastern Bangong-Nujiang Suture Zone: Evidences from Zircon and Apatite Fission Track

Xunzhang ZHU1, Dongliang LIU2#+, Haibing LI3, Jiawei PAN1, Zhongbao ZHAO1, Yong ZHENG1, Chao LI1
1Chinese Academy of Geological Sciences, China, 2Institute of Geology, Chinese Academy of Geological Sciences, China, 3Chinese Academy of Geological Sciences, Institute of Geology, China

The Bangong-Nujiang New Tethys Ocean suture zone is an important tectonic boundary, separating the Qiangtang block and the Lhasa block in the Qinghai-Tibet Plateau. This suture zone is one of the important windows to deciphering the growth history of the Qinghai-Tibet Plateau. This suture zone can be divided into three parts: the western, middle and eastern sections. Few studies were involved in the eastern section, which contains abundant structural evolution information. In this study, a vertical profile of granite near Guoqing village of Basu County is taken to study the tectonic uplift process by the fission track dating, including zircon fission track (ZFT) and apatite fission track (AFT) with laser ablation inductively coupled plasma mass spectrometry (LA-ICPMS). The zircon U-Pb ages center at ~180 Ma, indicating that its crystallization age is the Early Jurassic. The ages of ZFT and AFT are ~180-130 Ma and AFT are ~86-61Ma, respectively. The QTQt simulation showed that the upper NJ-01 sample of the profile had a fast erosion rate during ~130-60 Ma, the middle NJ-03 sample and NJ-04 sample had a slower erosion rate during ~130-40 Ma, and the lower NJ-06 sample maintained the slowest during rate since ~130 Ma. This differential uplift is caused by the earlier slab break-off in southward subduction than in the northward subduction, which induced the negative slope of the Age-Elevation Relation of ZFT and positive slope of the Age-Elevation Relation of AFT. Based on this and previous research results, the granites with age of 180 Ma in the Basu area are resulted by the northward subduction of the Bangong-Nujiang suture zone, the erosion uplift induced zircon fission track cooling age since ~180 Ma, and the erosion uplift generated apatite fission track cooling age during ~86-61 Ma.


SE05-A013
Late Mesozoic Tectonic Transformation on the Eastern Margin of the Yangtze Block

Xin CHEN#+, Songnan LIU, Liyun ZHOU
China University of Geosciences, China

Yangtze platform formed in the Neoproterozoic, as the second platform of China has an important status. It is adjacent to the Mid-Korean quasi-platform in the north west, and adjacent to the South China fold system in the south east. The Ningzhen Mountains are located on the northern edge of the Lower Yangtze platform, spread from southwest-northeast to east-west, about 100 kilometers long. Complex folds and thrust faults are widely developed in this area, the field survey and data analysis show that there are mainly two sets of structural systems: one is east-west and the other is northeast. EW trending folds such as Longtan-Cangtou folds have an inverse ”S” shape axis, which means that on its sides the axis is twisted to the northeast. Low angle EW trending overthrust faults develop on Triassic limestone and Jurassic sandstone along the edges of folds. The NNE trending strike-faults (Liuhe-Jiangpu, Guabu-Tiexinqiao, Fangshan-Danyang, Maoshan fauls) cut through the existing EW trending structures forming a unique vertical tectonic pattern. There are also NW trending strike-faults cutting Ningzhen Mountains into some transvers block in some areas. Volcanic rocks are mainly in Yanshanian period and there is a set of conglomerate developed in the area. The U-Pb Age analysis shows that the granitic dikes cutting across the strike-fault are 104.2±1.3 Ma and 102.6 ±1.1 Ma. How do these structures relate to each other? What is the specific age of those deformations? Whether and how the subduction of the paleo-Pacific plate influenced the transformations of the structure orientations? Those questions remain to be clarified.


SE05-A015
Velocity Structure of the Sulu Orogenic Belt in the Yellow Sea, East China: Evidence from Wide-angle Ocean Bottom Seismograph Data

Weina ZHAO1#+, Chenguang LIU2, Zhiqiang WU3
1Northwestern Polytechnical University, China, 2Ministry of Natural Resources, China, 3Qingdao Institute of Marine Geology, China

The Sulu orogenic belt, formed by the collision between Sino-Korean and South China blocks, has important tectonic implications due to its unique tectonic setting. To understand the deep crustal structure of the extension of the Sulu orogenic belt in the Yellow Sea, we presented a active-source ocean bottom seismometer wide-angle reflection/refraction profile across the Yellow Sea. The obtained P-wave velocity structure exhibits significant horizontal and vertical variations. The middle and upper crustal regions of the north beneath the survey line exhibit a higher velocity and larger thickness than those of the south, whereas the opposite is the case with the lower crust. Due to undulating Moho interface and varying crustal velocities the Qingdao–Rongcheng fault is suggested as a fault in the Sulu orogenic belt without the significance of tectonic zoning. This study shows that the Sino-Korean Block, Sulu orogenic belt, and South China Block are bounded by the Jimo–Muping faults (an extension to the sea), Qianliyan fault, and deep fault of the South Yellow Sea. Furthermore, the Sulu orogenic belt may have been formed by the northward subduction of the South China Block beneath the Sino-Korean Block during the Indo-Sinian orogeny to the east of the Shandong peninsula.


SE05-A021
An Optimal Spatial-filtering Method Derived from Eigenvalue Perturbation for Extending the Courant-Friedrichs-Lewy Stability Limit

Zhongzheng MIAO1+, Jinhai ZHANG2#
1INSTITUTE OF GEOLOGY AND GEOPHYSICS, CHINESE ACADEMY OF SCIENCES (IGGCAS), China, 2Institute of Geology and Geophysics, Chinese Academy of Sciences, China

The numerical simulation of wave propagation is a vital importance tool for imaging the interior structure of the Earth and simulating long-term geodynamic evolutions. The explicit time-marching scheme is widely used in numerical simulation owing to its low memory demand and simplicity of numerical implementation. However, its maximum time step is constrained by the Courant-Friedrichs-Lewy stability limit. To overcome this limitation and improve the computational efficiency of the explicit time-marching scheme, the eigenvalue perturbation and spatial-filtering methods have been developed. The eigenvalue perturbation method has high numerical accuracy but requires unaffordable memory demand and computational cost even for middle-scale models. In contrast, the spatial filtering method can be naturally integrated into the pseudo-spectral method but has high large numerical errors under large time steps. However, the intrinsic connection between these two methods is still unclear. By considering the eigenvalue perturbation method for the homogeneous model, we reveal the intrinsic relation between these two methods. Based on this relation, we obtain the analytical spatial filter for the homogeneous model and the optimal spatial filter for the heterogeneous model. Compared with the traditional spatial filtering method, which directly removes all high wavenumber components, the proposed method eliminates those wavenumber components that lead to instability and retains those wavenumber components that help maintain numerical accuracy. With the same numerical accuracy, the maximum time step allowed by the proposed method is about twice that of the traditional spatial filtering method. Compared with the eigenvalue perturbation method, this method can be directly applied to large-scale models without extra memory consumption and computation cost. The proposed method can significantly accelerate the speed of numerical simulation of seismic waves and long-term geodynamic evolutions.


SE05-A025
Dynamics of Oceanic Slab Tearing During Transform-fault Oblique Subduction: Insights from 3D Numerical Modeling

Jie XIN1#+, Huai ZHANG1, Zhong-Hai LI1, Felipe ORELLANA-ROVIROSA2, Liang LIU3, Yigang XU3, Zhen ZHANG1, Yaolin SHI1
1University of Chinese Academy of Sciences, China, 2Southern China University of Science and Technology, China, 3Guangzhou Institute of Geochemistry, China

Oceanic slab tearing is identified during plate subduction, and the resulting slab window allows hot mantle materials to pass through, resulting in anomalous thermal and chemical conditions in convergent-margin environments. To understand the mechanism of vertical slab tearing, we introduce a 3D numerical model to investigate the characteristics of transform-faulted oceanic slab during oblique subduction, and we compare model results with natural observations from seismic imaging. We find that (i) transform-fault ages-offset and (ii) subduction horizontal obliqueness have the first-order control on the generation of vertical tearing, even without the lateral physical property (density and viscosity) differences. Regarding the two patterns of vertical tearing, we find that young overall lithosphere (average <30 Myr) at medium-low subduction obliqueness angles (<40°) tends to produce fault-perpendicular slab tearing. In contrast, combinations of high-medium obliqueness angles (>10°) and large age ratios of the older slabs (average >30 Myr) tend to produce fault-parallel tearing. Our modeling results also suggest that the continual along-trench variation in subduction dip angle may be related to oblique subduction's early stages of evolution. Observing the age contrast across faults and the horizontal obliqueness of plates' motion may allow predictions of the tearing pattern, evolution, and local mantle flow.


SE05-A026
Introducing Underworld3 - A High Performance Geodynamic Modelling Code Focused on Usability

Louis MORESI1#+, Julian GIORDANI2, Haibin YANG3, Andres RODRIGUEZ4
1Australian National University, Australia, 2The University of Sydney, Australia, 3Zhejiang University, China, 4The University of Melbourne, Australia

We introduce underworld3, a finite element, solid-Earth modelling code designed to be both straightforward to use and highly scalable to peak high-performance computing environments. underworld3 inherits the design patterns of earlier versions of underworld such as 1) A python user interface that is inherently safe for parallel computation. 2) A symbolic interface that allows users to construct and simplify combinations of functions, unknowns and gradients-of-unknowns on the fly that are then used to construct the finite element representation of the problem. 3) Fast, robust, parallel numerical solvers, 4) Flexible, Lagrangian "particle" swarms for modeling transport-dominated quantities that are fully interchangeable with other data-types and can be treated as symbolic quantities. 5) Mesh adaptivity that falls fully within the symbolic framework. The design philosophy of Underworld is to provide readable python code that stays close to the mathematics of the problem definition and is scalable (unedited) from Jupyter notebooks all the way to tens of thousands of cores. Typical problems of interest are subduction zone models coupled to over-riding plate deformation, groundwater flow studies on a whole-of-basin scale, and earthquake rupture models coupled with tectonics. 


SE05-A028
Source Characterization of the November 2022 Mw 5.6 Cianjur Earthquake in West Java, Indonesia

Yukuan CHEN#+, Karen LYTHGOE, Rino SALMAN, Christina WIDIWIJAYANTI, Lujia FENG, Dannie HIDAYAT, Eleanor AINSCOE, Shi Tong CHIN, Benoit TAISNE, Sang-Ho YUN, Shengji WEI
Nanyang Technological University, Singapore

A damaging Mw 5.6 earthquake struck West Java, Indonesia, on 21 November 2022 and killed more than 300 people. Here, we characterize the source parameters of the mainshock and aftershocks to better understand the damage and the hosted fault of the earthquake. We conducted a finite fault inversion for the mainshock using static and high-rate GNSS data. To detect and locate the mainshock and aftershocks, we collected continuous waveform data from nearby seismic stations around the Gede volcano, mostly running by the lab volcano at Earth Observatory of Singapore. We applied a deep-learning neural network named Earthquake Transformer (Mousavi et al., 2020), to automatically detect and pick P and S-wave arrivals from the continuous waveform data. Then all the seismic phase arrival times were fed into the REAL (Zhang et al., 2019) program to associate them with earthquakes. After association, the NonLinLoc method (Lomax et al., 2000, 2014) was applied to locate the detected earthquakes. Finally, we further refined the relative location of these events using the double-difference relocation (hypoDD) method (Waldhauser & Ellsworth, 2000). The relocated high-resolution aftershock seismicity distributes in the depth range of 2-8 km, delineating a SE-NW oriented fault, which matches well with geodetic observations, yet surface rupture was not detected. Combined with the focal mechanism of the mainshock and the finite fault models on two conjugate fault planes, we concluded that the mainshock ruptured a shallow portion of a strike-slip fault with a strike ~345o, with rupture directivity towards the northwest, which agrees with observed ground damages.


SE05-A029
Blind Fault Branching Beneath Central Myanmar Basin Revealed by High-resolution Aftershock Location and Focal Mechanism of the 2019 Mw 5.5 Ye-u Earthquake Sequence

Win Shwe Sin OO1#+, Wardah FADIL1, Karen LYTHGOE1, Yukuan CHEN1, Dannie HIDAYAT1, Lin Thu AUNG1, Phyo Maung MAUNG1, Hongyu ZENG1, Ei Mhone Nathar MYO2, Shengji WEI1
1Nanyang Technological University, Singapore, 2National Taiwan University, Taiwan

Near-field seismic observations are usually not available for high-resolution source studies, and even when they are, high-frequency analysis are rarely conducted to extract more information. Here I study a unique dense nodal array data acquired by the development of the 2019 Mw 5.5 strike-slip earthquake in Central Myanmar Basin. The network, composed of 20 nodal stations with station spacing of approximately 5 km, was deployed 2 weeks after the mainshock for 40 days. A machine-learning based algorithm (Earthquake Transformer) was applied to detect 677 aftershocks from the dataset. Double difference relocation reveals that these events are distributed between 9 to 16 km in depth with a nearly northwest-southeast trending horizontal distribution, which is consistent with left-lateral fault plane solution of the mainshock. On the vertical component of most stations, a strong phase between the P and S-wave arrivals is present. This is an S-to-P converted phase produced by a sharp velocity boundary between the basin and the bedrock. The optimal 1D velocity model, constrained by 3-component waveform modelling, suggests a sedimentary layer thickness of approximately 3.5 km beneath the stations. To determine the focal mechanism of aftershocks, I conducted waveform inversion at 0.5-2Hz that results in high-quality waveform fits. For very small aftershocks (~Mw 1), the focal mechanism inversion is done at higher frequency 2-8 Hz and the unmodeled structural effect is corrected by applying Amplitude Amplification Factor (AAF). The focal mechanisms include strike-slip, reverse thrust, oblique thrust with strike-slip components and a few normal events. Highly diverse aftershock focal mechanisms suggest the fault system is likely immature. The thrust and normal events indicate that the mainshock rupture had branched into or activated nearby secondary faults, which allow the strike-slip fault to propagate and develop a more complex fault system.


SE05-A030
Earthquakes and Faulting at the Southernmost Mariana Subduction Zone

Han CHEN1,2+, Han CHEN3, Hongfeng YANG3#, Gaohua ZHU3, Min XU4, Jian LIN5,4, Qingyu YOU4
1Sun Yat-sen University, China, 2Southern Marine Science and Engineering Guangdong Laboratory, China, 3The Chinese University of Hong Kong, Hong Kong SAR, 4Chinese Academy of Sciences, China, 5Woods Hole Oceanographic Institution, United States

Near-field observational data are collected in the Southern Mariana subduction zone by three newly deployed ocean-bottom seismographs (OBS) networks. We process data by using both conventional seismic data processing techniques and recently developed Machine Learning (ML) earthquake detection techniques. This is the first time that the ML earthquake detection methods are applied to OBS observation data at the southern Mariana trench. Our result gives new insight into the fault and seismicity in the Southern Mariana subduction zone. We utilize machine learning-based earthquake detection methods (PhaseNet and EQTransformer) in the first two near-field data and locate the detected earthquakes by using both absolute and relative earthquake location methods. More than 1975 earthquakes are detected, of which 1972 earthquakes are relocated. The location result reveals a heterogeneous distribution of seismicity with a cluster of outer-rise events. The precise location of the cluster events reveals an outer-rise fault that reaches a depth of 50 km and strikes in the same direction as the inherited seafloor fabrics, indicating that there might be larger water input in the southern Mariana Trench than in the previous estimation. The location result of all three data sets also reveals significant along-strike variations in seismicity density and depth distribution pattern, based on which we inferred double seismogenic zones (DSZs) in the eastern region of the slab but a lack of such feature in the western region. We suggest that the dehydration embrittlement of the subducted plate controls the generation of IDEs in the study area. Keywords: Outer-rise fault, Mariana subduction zone, EQTransformer, Ocean Bottom Seismometer, Intermediate-depth earthquake.


SE05-A033
Late Paleozoic to Cenozoic Deformation of the Qilian Shan, NE Tibetan Plateau: Insights from the Huangcheng Basin

Jiabao JIA1,2+, Wenjun ZHENG1#, Renjie ZHOU2
1Sun Yat-sen University, China, 2The University of Queensland, Australia

The Qilian Shan in NE Tibetan Plateau has recorded the deformation history during the closure of the Paleo-Tethys Ocean and northeastern growth of Tibetan Plateau. We focus on the Huangcheng Basin where origins of Late Mesozoic sediments and styles of deformation of faults-folds systems remain controversial. Based on field mapping, fault locations and their correlations fault-folds systems are identified. We also documented two sets of slickensides on fault planes and typical sections of basin stratigraphy. Eleven detrital zircon samples from the Cretaceous to Neogene were collected for detrital zircon U-Pb dating and trace element analysis. Among the two sets of slickensides, one shows NE-SW movement while the other implies E-W compression. Zircon U-Pb ages show major peaks around 265 Ma and 455 Ma. There is also an age-dependent trend of zircon Eu/Eu* values. Our preliminary results suggest that the study region might have experienced three episodes of compression from the 400 Ma to the Neogene. The first episode may represent crustal thickening at ~350 Ma. The second episode is characterized by NNE-SSW trending compression, which could reflect the convergence between the Alashan block and Qilian Shan-Nan Shan block. The third episode reflect tectonic activities related to the regional strike-slip motion. We also infer that Neogene sediments were sourced from the Qilian Shan while Cretaceous sediments were sourced from the North China Craton and Alashan Block.


SE05-A036
Magnetostratigraphy of the Laolongwan Basin in the Northeastern Margin of the Tibetan Plateau and Its Tectonic Significance

Kang LIU1#+, Weitao WANG1, Renjie ZHOU2
1Sun Yat-sen University, China, 2The University of Queensland, Australia

Understanding the activity periods of the Haiyuan Fault, a major boundary fault on the northeastern margin of the Tibetan Plateau, is of great significance for understanding the expansion of the Tibetan Plateau. The Laolongwan Basin is a Cenozoic sedimentary basin developed within the Haiyuan Fault zone on the northeastern margin of the Tibetan Plateau. Its sedimentary evolution provides a detailed record of the tectonic deformation process along the Haiyuan Fault since the Cenozoic. Here we present evidence for inception and evolution of the Laolongwan basin, based on magnetostratigraphy combined with cosmogenic nuclide burial ages that date the basin fills to be from ca.14 to 0.8 Ma. Angular unconformity and growth strata indicate that the Haiyuan Fault underwent two tectonic activities ca.14 and 3.4 Ma. Evidence for 10 to 15 Ma widespread synchronous deformation throughout the Tibetan Plateau and its margins suggests that during this period, the Cenozoic deformation along the northeastern Tibetan Plateau reached their modern extent.


SE05-A038
Multi-stage Growth Process Since the Cenozoic in the Northern Margin of the Tibetan Plateau

Hulu JING#+, Weitao WANG
Sun Yat-sen University, China

The Cenozoic deformation of the surrounding area of the Tibetan Plateau is an important window to understand the pattern of plateau expansion. Tianshan is a typical Cenozoic resurgent orogenic belt affected by the remote effect of the India-Eurasian plate collision. The Cenozoic foreland deposits in the northern piedmont have recorded the evolution process of Tianshan in the Cenozoic. Constrained by the chronological framework of North Tianshan magnetostratigraphy, sedimentation rate changes and terrain simulations based on the foreland basin morphology revealed by seismic reflection profiles indicate that the North Tianshan piedmont has experienced three periods of growth since ~ 26 Ma, ~ 15 Ma and ~ 6 Ma. The deformation since about 30 Ma and 15 Ma widely existed in the northern and northeastern margins of the Tibetan Plateau, which indicates that the growth of the surrounding areas of the Tibetan Plateau is a quasi-synchronous process.


SE05-A039
Plio-Pleistocene Depositional and Tectonic History of Sulawesi Based on U-Pb Zircon Geochronology and Heavy Minerals of the Sedimentary Rocks in Palu, Indonesia

Abang NUGRAHA1#+, Juliane HENNIG-BREITFELD2, Robert HALL2
1Earth Observatory of SIngapore, Nanyang Technological University, Singapore, 2Royal Holloway University of London, United Kingdom

The Celebes Molasse in Palu has generally been considered to be associated with the Pliocene collision. However, sedimentological, provenance, and zircon geochronological analyses suggest that the sedimentary unit was deposited in an alluvial fan to braided river setting as the syn-orogenic deposit that records gradual uplift rocks related to Neogene extension. The youngest zircon age from this study gives the maximum depositional age of c. 2.5 Ma. Heavy minerals indicate a mixed source from acid to basic igneous and metamorphic rocks, which are now widely exposed in the Neck and west Central Sulawesi. Detrital zircons show a single Proterozoic zircon, a prominent Mesozoic age population with a Triassic peak, and a significant Late Cenozoic peak similar to zircon populations analysed from metamorphic and granitoid rocks in the Neck and west Central Sulawesi. These characteristics differ from the so-called Celebes Molasse formations related to the Sula-Spur collision in eastern Sulawesi. Variations in depositional time, sediment composition and sedimentation history suggest that the ‘Celebes Molasse’ term causes confusion and is too general to provide detailed depositional history for the sedimentary basins across Sulawesi.


SE05-A041
Time Constraint on Danangou Mammalian Fauna in the Nihewan Basin, 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, located in Hebei Province, North China. It has abundant gullies developed along both banks of the Sanggan River and Huliu River during and after the demise of Nihewan paleo-lake, creating a number of outcrops of the Nihewan Beds of fluvio-lacustrine origin, which are underlain by the Pliocene eolian Red Clay and overlain by the late Pleistocene loess. The fluvio-lacustrine sequence is rich sources of mammalian faunas and Paleolithic sites, thus providing unique insights into our understanding of land mammal biochronology and early human settlements in East Asia. Among the Nihewan Fauna (sensu lato), the Danangou (DNG) fauna is one of the important Pleistocene and Pliocene mammalian faunas in the Nihewan Basin. Except for a biostratigraphy, precise age control on the DNG fauna remains unavailable. Here we report a high-resolution magnetostratigraphic results that stringently constrain their ages. Rock magnetism and thermal demagnetization results show that magnetite and hematite dominate the remanence carriers in the DNG fluvio-lacustrine sequences. High-resolution magnetic polarity stratigraphy indicates that the DNG sequence recorded the Brunhes normal chron, the Matuyama reverse chron and the late Gauss normal chron, yielding the fossil-rich layers of DNG fauna with an age of ca. 1.95 Ma to 1.78 Ma during the Olduvai normal subchron. This result, together with previously published magnetochronology data obtained in the eastern basin, constructs a precise age constraints on the chronological framework of the Nihewan faunas and Paleolithic sites, especially during the Plio-Pleistocene transition.


SE05-A042
Field Observations and Zircon U-Pb Analyses of the Paleoproterozoic Rocks in the Gogeumdo Area, Sw Korean Peninsula

Kyoungtae KO#+
Korea Institute of Geoscience and Mineral Resources, Korea, South

The Yeongnam Massif is one of the Paleoproterozoic tectonic units, which is located in the southeastern part of the Korean Peninsula. The Gogeumdo area, which is the focus of this study, is located on the southwestern margin of the Yeongnam Massif. The study area mainly consists of the Paleoproterozoic rocks, which are covered by the Cretaceous volcanic rocks. Based on field observations, the Paleoproterozoic rocks are divided into metasedimentary rocks and metagranitoids. In addition, the Paleoproterozoic metagranitoids are subdivided into foliated granite, porphyritic granite, and biotite granite. LA-MC-ICP-MS zircon dating shows that the minimum depositional age of the Paleoproterozoic metasedimentary rocks is constrained to be at ca. 1870 Ma based on the metamorphic age of overgrown zircon rims. However, the Paleoproterozoic metagranitoids are emplaced during ca. 1875~1857 Ma. Our results of detailed field observations and geochronological data suggest the presence of Paleoproterozoic strata in the southwestern margin of Yeongnam Massif which is yet to be discussed.


SE06-A003
Petrogenesis and Implications of the Basalts in the Yap Trench, Western Pacific: Constraints from Geochemistry and Sr-Nd-Pb Isotopes

Limei TANG#+
Second Institute of Oceanography, Ministry of Natural Resources, China

The nascent arc magmatism is significant to elucidate the subduction mechanism and early evolution of the subduction zone. For a better understanding evolution process of the island arc, the basalt lavas collected from the north and south of the Yap trench were analyzed for their major, trace and Sr-Nd-Pb isotopes. The results reveal the difference of petrogenesis and implications between the north and south of the Yap Trench. The content of Nb and Ta suggests its mantle source is similar to Mariana Trough which consist of depleted mantle and Sr isotope is higher (0.704 646~0.704 794), indicating it was subjected to alteration of seawater. Combined with the other geochemical characteristics, we considered that the northern lava of the Yap Trench represents the crust of the Parece Vela Basin which was thrusting above the initial Yap Arc during the geological process of the collision between the Caroline Ridge and the Yap Trench. Compared with northern samples from the Yap Trench, the southern samples had lower content of MgO (4.18%~5.14%), TiO2(0.69%~0.80%) and CaO(8.64%~10.25%) and lower ratio of Ti/V(11.56~14.07). The REE pattern is relatively flat which is the typical trace element characteristics of subduction-related igneous rocks. The geochemical characteristics of the lava in the south of the Yap Trench indicate that it is the result of collision between the Caroline Ridge and the Yap Trench, which leads new nascent arc magmatism and increasement of the temperature of Yap Forearc. And the dehydration of the subducted plate in the shallow part of the arc, which induces a new island arc magmatism. Finally, the Yap Trench lava are exposed to the bottom of the trench due to subduction erosion.


SE06-A007
Molybdenum Isotopic Constraints on the Origin of EM1-type Basalts

Liang MA#+
Chinese Academy of Sciences, China

The origin of enriched mantle 1 (EM1) component in the mantle has long been debated. EM1 source of basalts has been variously attributed to recycled sub-continental lithosphere, recycled lower continental crust, or recycled oceanic crust plus pelagic sediments. Molybdenum stable isotope systematics has the potential to resolve this debate, because of the significant isotopic differences between mantle and crustal reservoirs. Here we present molybdenum isotope data for EM1-type continental intraplate basalts from Nuominhe (NMH), Northeast China. The NMH basalts display significant variations in both d98/95Mo and Mo/Ce, and strong correlations between d98/95Mo, Mo/Ce and Hf isotope and trace elements. EM1 end-member of the NMH basalts shows the lightest d98/95Mo and lowest Mo/Ce values. The involvement of continental crust and sub-continental lithospheric mantle cannot account for the light Mo isotopic compositions of the basalts. By contrast, the recycled oceanic crust with pelagic sediments, characterized by low d98/95Mo and Mo/Ce values, is the satisfactory candidate for the EM1 component in the NMH basalts. Our results also suggest a residual slab reservoir with light d98/95Mo values (<0.5‰) in the mantle beneath Northeast China, representing the complementary reservoir to heavy Mo isotope continental crust. Identification of this reservoir makes the Mo isotope system a powerful tracer of crust-mantle interactions.


SE06-A009
Osmium Isotope and Highly Siderophile Element of the Subduction Zone Mantle: Constraints from Data on the Yap Trench Peridotites

Ling CHEN#+, Limei TANG
Second Institute of Oceanography, Ministry of Natural Resources, China

Highly depleted peridotites from the Yap Trench in the western Pacific Ocean have been studied for highly siderophile elements (HSEs) and osmium isotope. The abundance of HSEs in Yap Trench peridotites is extremely low compared with that in oceanic peridotites from the mid-ocean ridge and other subduction-zone environments, indicating the extensive extraction of the sulfde melt. The peridotites have variable 187Os/188Os ratios (0.12043–0.14867), with the suprachondritic 187Os/188Os ratios indicating modification of the mantle wedge by slab-derived fluid and melt and the sub-chondritic 187Os/188Os ratios corresponding to a Re depletion age of 0.24–1.16 billion years. The osmium isotope results suggest that some of the Yap Trench peridotites represent old mantle residue of ancient melting events and old depleted mantle fragments may contribute substantially to the chemical heterogeneity of the oceanic mantle. Chondrite-normalized HSE patterns of the Yap Trench peridortites are heterogeneous and exhibit strong fractionation of platinum-group elements (PGEs) and slight enrichment of Re and Au. The Ru/Ir (1.64–16.12), Os/Ir (0.15–7.19), and Pt/Pd (0.53–13.17) ratios in most of the studied samples are higher than those in CI chondrite (Ru/Ir: 1.49; Os/Ir: 1.06; and Pt/Pd: 1.67). These suprachondritic PGE ratios result from the exhaustion of the base metal sulfde (BMS) and the formation of platinum-group minerals and alloys, such as Os–Ru-rich sulfdes and Pt–Fe alloys, that are selectively enriched with certain HSEs. We recommend that the high oxygen fugacity, hydrous melting, and high degree melting of the subduction-zone mantle may result in the exhaustion of the BMS in highly depleted peridotites, promoting the formation of platinum-group minerals and HSE-rich alloys, in which the HSEs are significantly fractionated.


SE06-A011
Magmatism and Crustal Structure of the Southern Kyushu-Palau Ridge from Seismic Refraction Profiles

Jie ZHANG1#+, Jiabiao LI2, Weiwei DING3, Aiguo RUAN1, Xiaodong WEI3, Pingchuan TAN4
1Second Institute of Oceanography, Ministry of Natural Resources, China, 2State Oceanic Administration, China, 3Ministry of Natural Resources, China, 4Second Institute of Oceanography,Ministry of Natural Resources, China

The Kyushu–Palau Ridge (KPR) is the result of the subduction of the Pacific Plate, separated from the proto-Izu–Bonin–Mariana arc by the back-arc spreading, showing variations in arc structures. The internal structure not only reveals the arc characteristics but also contains crisis information about how the arc formed from initial subduction to initial back-arc spreading. However, the less revealed velocity structure in the southern KPR might hinder an understanding of the mechanism of crustal variations. In this work, we model the crustal structure across the southern KPR, using data from two 2D wide-angle seismic profiles. The southern KPR crust is 6.0-11.0 km (Vp=1.9-7.0 km/s) without developing a distinct middle crust. The across-ridge diversities in arc structures suggest that the KPR is not a uniform magma body but comprises several independent seamounts with different periods of magmatism. By analyzing the evolution of the KPR, we conclude that multiple volcanic sources and episodic magmatism caused the diversities in arc structures. This research was granted by the Scientific Research Fund of the National Natural Science Foundation of China (91858214, 42025601, 42276075).


SE06-A016
Experimental Constraints on the Potential Significance of Rodingite in the Mantle

Yu WANG1#+, Yi-Xiang CHEN2
1Guangzhou Institute of Geochemistry, Chinese Academy of Sciences, China, 2University of Science and Technology of China, China

Rodingites are calcium-rich silica-undersaturated rocks formed by metasomatic alteration (rodingitization) of mainly gabbros and basalts, and are often found associated with serpentinite. They are commonly composed of Ca-minerals including grossular, vesuvianite, epidote, prehnite and diopside, and have been documented in various tectonic settings, such as active seafloor spreading centers, rifted continental margins, greenstone belts, and orogenic belts. However, as an important component in both oceanic lithosphere and in ophiolites, the significance of rodingite in affecting mantle heterogeneity through subduction has been long overlooked, and the melting process of rodingite in the mantle remains poorly constrained. Here we report the first HTHP experimental results on partial melting of rodingite in the mantle to investigate the PT stability of both regular and dehydrated rodingite, compositions of the melts and residual facies, elemental behaviors, and the potential significance of rodingite in altering the oxidation state and compositional heterogeneity in the mantle.


SE06-A020
Seismic Evidence for Mantle Heterogeneity Caused by Trapped Water in the Southwestern South China Sea

Jinyu TIAN1+, Zhitu MA2, Jian LIN3#, Min XU4, Xun YU2, Ba Manh LE3, Xubo ZHANG4, Fan ZHANG5
1Shanghai Jiao Tong University, China, 2Tongji University, China, 3Southern University of Science and Technology, China, 4Chinese Academy of Sciences, China, 5South China Sea Institute of Oceanology, Chinese Academy of Sciences, China

Water is the most common volatile component inside the Earth. A substantial amount of water can be carried down to the interior of the Earth by subducting plates. However, how the subducted water evolves after the subducting slab breaks off remains poorly understood. Here we used the data from a passive seismic experiment using ocean bottom seismometers (OBSs) together with the land stations to determine the high-resolution, three-dimensional seismic structure of the Southwest Sub-basin (SWSB). At depths below 40 km, the mantle shear-velocity beneath the northern side of the SWSB is similar to that of the conventional oceanic pyrolite mantle, but roughly 3% shear-velocity reduction was found beneath the southern side of the SWSB. Results of thermal dynamic modeling reveal that the observed significant shear-velocity reduction could be explained by the presence of 150–300 ppm of water and 5–10% of lower continental crust. The inferred high-water content at the southern side of the SWSB is consistent with a model in which the Proto-SCS plate subducted southward prior to and during the formation of the SCS basin, releasing water into the upper mantle of the SWSB.


SE06-A023
Sedimentary Budget of the Okinawa Trough Since the Middle Miocene

Haiqin WANG1#+, Weiwei DING2
1Second Institute of Oceanography, Ministry of Natural Resources, China, 2Ministry of Natural Resources, China

The Okinawa Trough (OT), a back-arc basin formed by the subduction of the Philippine Sea Plate into the Eurasian Plate, is the receiving end of the sediment transport from the Asian continental margin to the sea. So it is the key place to study the source-sink process in the continental margin of East Asia. As the average water depth in this area exceeds 1000 m, it is difficult to carry out extensive drilling exploration in this area, so it greatly limits the systematic and long-term sedimentary process research. Based on 45 multi-channel seismic lines covering the OT, the sedimentary budget and spatial distribution characteristics of thicknesses in different geological periods are obtained, and the controlling factors and possible sources are discussed. The results show that the sedimentary budget of the OT have been increasing since the Middle Miocene. On the one hand, the sedimentary budget of the middle segment (MOT) and the northern segment (NOT) increased similar before the Middle Pleistocene, but NOT decreased after the middle Pleistocene. On the other hand, before the early Pleistocene, the total sediment budget in the southern segment (SOT) was low and increased rapidly since the early Pleistocene. Changes in sediment budget are mainly controlled by the the multi-stage expansion of the OT, and are also strongly related to river development in East Asia and global sea level changes. in addition, global climate change can accelerate or slow down the continental erosion. Temporal and spatial distribution of sediments in the OT indicates that the contribution of sediment sources to basin filling is different in different geological periods. In this study, the semi-quantitative constraints on the sedimentary processes of the OT have improved the understanding of the source-sink processes of the East Asian continental margin. Keywords: Okinawa trough; sediment budget; controlling factors; sediment provenance.


SE06-A024
Zircon U-Pb and Hf Isotopic Constraints on the Tectonic Event in West Java

Yu-Ming LAI1#+, Wai-Ki LEUNG2, Sun-Lin CHUNG3, Iwan SETIAWAN4, Hao-Yang LEE2, Lediyantje LINTJEWAS5, Yoshiyuki IIZUKA2
1National Taiwan Normal University, Taiwan, 2Academia Sinica, Taiwan, 3National Taiwan University, Taiwan, 4Indonesian Institute of Sciences, Indonesia, 5National Research and Innovation Agency, Indonesia

The western Sunda Arc is located in the southern margin of the Sundaland in Southeast Asia. The subduction system can be separated into two parts: the Sumatra arc is oblique subduction, whereas Java Arc is a normal one. Sunda Strait is the transition zone between these two arc systems, the different stress directions of tectonic setting eventually lead to the opening of Sunda Strait. However, when did the Sunda Strait open is still debated. Here we present zircon Hf isotopic data with known U-Pb ages in the western part of the West Java. According to these data, we deduce the time of slab tearing beneath the western West Java-Sunda Strait area and the Sunda Strait opening. A total 102 zircon Hf isotopic data from 14 andesites in Danau Volcanic Complex, Ciemas area, North and South Bayah Dome were analyzed. Miocene to Pliocene zircons (17.0 to 5.0 Ma, n = 76) with higher εHf values from +15.3 to +9.6 while Quaternary zircons (1.0 to 0.4 Ma, n = 26) with lower εHf values from +7.5 to +1.2. Zircons with higher εHf values are similar to the eastern Sumatra (15 to 13 Ma and 4 to 0 Ma, εHf values = +18 to +7) which can be referred to the ‘normal Sunda Arc magmatism’ signal. However, the lower εHf values from Quaternary zircons needs another enriched component to contribute. We refer to several previous tectonic modals beneath the western West Java-Sunda Strait area, and we suggest a slab tearing caused asthenospheric extra heat to melt the subducted sediments during 5.0 to 0.7 Ma according to our data. We further argue that the slab tearing was as a result of the opening of Sunda Strait. Therefore, the time of Sunda Strait opening might not younger than 1 Ma.


SE06-A026
Slab Breakoff Induced by Seamount Subduction at the Java Trench

Dan LIANG1#+, Weiwei DING2
1Shanghai Jiao Tong University, China, 2Ministry of Natural Resources, China

Slab windows or holes have been observed along circum-Pacific zone. Slab break-off mechanism is gradually to be a debated topic. According to the studies of several regions, high bathymetric collide with trench which may be the main factor in slab break-off information, such as Nazca plateaus subducted beneath North America continent, Zhenbei-Huangyan Seamount Chain subducted in the southern part of the Mariana Arc. Java subduction zone is located at the southernmost part of the southeast Asian subduction zone. Since the middle Eocene (about 45 Ma), the Indo-Australian plate has subducted northward to the southern Java Trench. The recent geophysics research suggested the existence of the slab tears between 250-450 km, including P-wave tomography, S-wave splitting results. Meanwhile, the intraplate volcanoes in Central Java are potassic (K)-rich and have been hypothesized to be caused by a supply of volcanic material in the deeper asthenosphere. We suggest that seamounts play a significant role in the subduction process of the Australian plate and the possible formation of the slab break-off in the Java. We designed a serials of numerical modeling experiments with variable parameters to discuss the slab break-off mechanism, which including plate convergence velocity, the age of slab, subduction angle, seamount size and lithospheric rheology. Generally, seamount with weak lithospheric rheology or fault-weakening lead the slab to breakoff more easily. The convergence rate is a key parameter affecting the break-off timing and depth. It’s difficult for seamount subduction to breakoff under fast velocity. Slab age shows complex rheological behavior in the process of plate subduction and detachment. The result of model is consistence with tomography of Java.


SE06-A027
The Oceanic Crustal Structure and the Magmatic Accretion History of the South China Sea

Chenghui ZENG1#+, Zhen SUN1, Yongjian YAO2
1Chinese Academy of Sciences, China, 2Guangzhou Marine Geological Survey, China

Plate separation is accommodated by magmatic accretion and tectonic extension, it is important to study the plate dynamics based on the ratio between them. The South China Sea (SCS) is symbolic of the slow-intermediate spreading marginal sea. However, there is lack of holistic quantitative calculation of the magmatic accretion from the perspective of spatio-temporal distribution, which limits the cognition of the seafloor spreading process of the SCS. We calculate the spatial distribution characteristics of M number, which marks the ratio of separation accommodated by magmatic accretion, in the SCS through seismic profiles. The main conclusions are:(1) The M number of the SCS fluctuates in the range of 0.5~0.95. For each sub-basin, the M of the main spreading area of the northwest sub-basin (NWSB) of the SCS can reach above 0.9. In the east sub-basin (ESB), the M can be above 0.9 and a few areas can be as low as 0.7~0.8 in the early spreading stage (> 23.6 Ma). In the late spreading period (< 23.6 Ma), the values of M number vary alternately between 0.5~0.8 and 0.8~0.95 along the single seismic profile or along the single magnetic anomaly lineation in the ESB and the southwest sub-basin (SWSB).(2) When the M number attain 0.93, planar faults are developed in the oceanic crust, the horizontal displacement is less than ~0.5 km. When the M value decrease to 0.66, low-angle detachment faults are developed, the horizontal displacement can reach ~3 km. The dip angle of fault plane is less than ~30°.(3) We speculated that the mantle serpentinization began to occur when the M number decrease between 0.7~0.8. Because the M number of SCS is generally greater than 0.5, serpentinized mantle exhumation is difficult to occur.


SE06-A028
Bifurcation of Mantle Plumes by Interaction with Stagnant Slabs in the Mantle Transition Zone: Evidence from Late Cenozoic Basalts Within Southeast Asia

Fan YANG1#+, Xiao-Long HUANG2, Yigang XU3
1Southern Marine Science and Engineering Guangdong Laboratory (Guangzhou), China, 2Guangzhou Institute of Geochemistry, Chinese Academy of Sciences, China, 3Guangzhou Institute of Geochemistry, China

Mantle plumes and plate tectonics, the two basic geodynamic systems operating on Earth, frequently interact. One of the interaction scenarios is that mantle plumes encounter stagnant slabs in the mantle transition zone (MTZ) during their ascent from the lower mantle to Earth’s surface, which remains poorly understood. Here we present new data on a spatial thermal–lithological–chemical heterogeneity in the mantle over a vast area of southeast Asia that reflects variable influence of a late Cenozoic mantle plume. Mid-ocean ridge basalts (MORBs) in the southwest sub-basin of the South China Sea (SCS; IODP Site U1433) locate near the center of the seismically imaged mantle upwelling. They are derived from a peridotite-dominated and normal temperature mantle source with a depleted Nd–Hf and enriched 207Pb/206Pb isotopic composition. In contrast, MORBs from IODP Site U1431 within the eastern sub-basin of the SCS and other intraplate basalts from the Hainan–Leizhou area, the eastern Indochina block, and elsewhere in the SCS are dominantly sourced from higher temperature pyroxenite-enriched mantle material that records mantle plume activity. These observations are contrast with previous models involving a s ingle plume rising from the lower mantle beneath the SCS that then tilted toward Hainan Island. Instead, the observations from this region maybe indicative of plume–stagnant slab interaction. The shallow upper mantle beneath Site U1433 has not been influenced by a mantle plume as the presence of stagnant slabs within the MTZ prevented further upwelling of the plume. In contrast, a mantle plume passed through the weaker MTZ within the eastern sub-basin and circum-SCS areas, allowing plume-related magmatism to occur. The bifurcation of a deep-rooted mantle plume by stagnant slabs in the MTZ produced a cluster of small mantle upwellings that ascended to shallow depths, consistent with new multiscale global tomographic data for southeast Asia.


SE06-A030
Hydrous Mantle Induces Rapid Continental-oceanic Transition of the South China Sea Rifted Margin

Zhiyuan ZHOU1#+, Jian LIN2
1Southern University of Science and Technology, China, 2Woods Hole Oceanographic Institution, United States

Recent investigations of IODP Expeditions 367/368 have revealed that the transition from continental to oceanic lithosphere is surprisingly fast and mantle exhumation and serpentinization is not observed at the South China Sea (SCS) continental margin. It makes SCS margin significantly different with typical magma-poor margin such as the Atlantic Iberia–Newfoundland margin. Recent studies imply that SCS margin might be a magma-moderate margin with a hot mantle. However, the mechanism for rapid continental-oceanic transition of the SCS margin is still enigmatic though it is hypothesized to be related to subduction. Here we establish a model of continental rifting and breakup due to extension and mantle upwelling, in which we innovatively incorporate the water content in the asthenosphere mantle to quantitatively evaluate the effect of hydrous mantle on the rifting and breakup processes of the SCS margin. Modeling results reveal that a low-moderate mantle temperature (1,300 – 1,350 °C) is required to form both a failed rift center and a successful breakup point. Moreover, significant water (100-300 ppm) in the asthenosphere beneath the SCS margin is required to cause both rapid continental-oceanic transition and enough magma for observed large crust accretion at initial spreading center. It is further hypothesized that the preceding subduction before continental rifting might bring substantial water into the mantle beneath the SCS margin and accelerate mantle upwelling and continental breakup. Furthermore, our models reveal that melt migration could induce significant asymmetry in crustal underplating on the two conjugated margins, explaining the observed asymmetric high-velocity layer at SCS margin. Our models provide new insights to the origin and evolution of most of the marginal seas at the western Pacific Ocean, which are highly influenced by subduction processes.


SE06-A033
Suture Zone of Paleo-Pacific Ocean and Tectonic Inheritance in Rifting of the South China Sea Continental Margin: Revealed by Deep Seismic Profile

Zongdong PAN1+, Shaoping LU1#, Han CHEN1,2
1Sun Yat-sen University, China, 2Southern Marine Science and Engineering Guangdong Laboratory, China

The Northern South China Sea (SCS) margin, roughly includes the continent-ocean boundary (COB) and the South China Block margin, which has transformed from a Mesozoic active continental margin to a Cenozoic passive continental margin. The evolution of the South China block is considered to have been influenced significantly by the subduction of the paleo-Pacific plate since the Mesozoic as evidenced by widespread igneous rocks. However, the mechanism of the transition from active continental margin to passive continental margin and the opening of the SCS is inconclusive. the location of the ancient Pacific suture zone is also controversial. Paleo-suture zone corresponds to “weak” structures and is a key factor influencing the evolution of rifting and seafloor opening. According to tectonic inheritance, the closed remnants of the destroyed paleo-Pacific in the SCS region represent the suture zone. The precise location of the suture zone is crucial in understanding the rifting history of the SCS region. The deep seismic reflection profile can provide information on crust-mantle structure, which can be correlated to surface geological information and provide key evidence to reveal the evolutionary history of the tectonic assembly. We interpret the deep seismic reflection profile on the northeastern SCS and locate the suture zone of the paleo-Pacific Ocean by combining gravity, magnetic anomalies, and geochemical data. We propose that the SCS opening is initiated at the suture zone of the paleo-Pacific Ocean and tectonic inheritance plays a key role in rifting of the SCS continental margin.


SE06-A036
Crustal Structure and Its Tectonic Significance of the East Subbasin, South China Sea: Seismic Evidence from OBS Refraction/reflection Survey

Lu ZHANG#+, Chen CAI
Sun Yat-sen University, China

The South China Sea (SCS) is one of the largest marginal seas of the Pacific, which is located at the junction of the Eurasian plate, Philippine plate, and Indo-Australian plate. The spreading history and mechanism of the SCS have long been studied and debated. A recent 750-km long north-south trending OBS refraction/reflection seismic profile led by Sun Yat-sen University was carried out across the East Sub-basin, SCS, covering the entire oceanic basin and part of the continental crust to the south. The P-wave velocity model along the line was obtained by forward/inversion of the travel-time picks with Rayinvr program. Taking the fossil spreading ridge (i.e., the Huangyan-Zhenbei seamount chain) as the boundary, the velocity model reveals a thicker northern sub-basin with a mean thickness of ~7.7 km compared to the southern one with a mean thickness of ~5.9 km. The asymmetry feature of crustal thickness of the oceanic basin may be a joint result of the ridge jump event and the melt flow addition caused by the Hainan plume to the northern flank at zero-age crustal accretion. Our result also presents a low-velocity body within the upper crust slightly south of the fossil spreading ridge, suggesting asymmetric serpentinization to the southern flank along detachment faults formed during the last stage slow-spreading episode. We, therefore, recommend that the Hainan plume played an important role in the seafloor spreading process and in shaping the oceanic crustal thickness asymmetry.


SE08-A001
Mantle Source Characteristics of Cenozoic Volcanoes in Central Asia: Constraints from Olivine Compositions and Whole-rock B-Mo Isotopes

Yunying ZHANG1#+, Min SUN2, Chao YUAN3, Zhen SUN3, Qian LIU4
1South China Sea Institute of Oceanology, Chinese Academy of Sciences, China, 2The University of Hong Kong, Hong Kong SAR, 3Chinese Academy of Sciences, China, 4Northwest University, China

Cenozoic continental basalts are diffusely distributed in central Asia, and are dominated by alkaline basalts with subordinate tholeiites and show oceanic island basalt-like trace element features. The geodynamic settings and ultimate magma origin of these basalts remain mysterious, which are largely due to the short of knowledge on their source lithology. Phenocrystic olivine is always the first silicate phase to crystallize from primary basaltic melts and thus could faithfully record information about the magma source. Besides, boron and molybdenum isotope systematics, in the past two decades, have proven to be of great value in tracking recycled oceanic crust in the mantle source of within-plate basalts. Voluminous basalts with ages from 30 Ma to 5 ka and volume up to 2900 km3 erupted in the Hangai dome and Mongol–Chinese Altai region. Representative basalts from the Central Hangai and Chinese Altai were collected for geochemical investigation to constrain their mantle lithology and geodynamic mechanism responsible for the widespread intraplate basalts. The phenocrystic olivines are featured by lower Ca, Mn, Mn/Zn and Mn/Fe but higher Ni than their counterparts in the peridotitic melts, indicating a pyroxenite-rich mantle source. Besides, the light B and variable Mo isotopic compositions of the Chinese Altai basalts indicate that recycled, dehydrated oceanic crust was likely involved in the mantle source, since subduction dehydration preferentially transports heavy 11B and 98Mo to the fluid phase. It is proposed that the pyroxenite was formed by reaction of recycled oceanic crust with its ambient peridotite, based on their light B and Mo isotopic compositions, and negative correlations between B isotopes and B contents, and between oxygen fugacity and olivine Mn/Zn. The far-field effect of India–Eurasia convergence possibly tapped the upper asthenospheric mantle, subsequent melting of which gave rise to the dispersive Cenozoic volcanoes.


SE08-A010
Interaction of the Kerguelen and Amsterdam-St. Paul Dual Hotspots with the Eastern Indian Ocean

Yiming LUO#+, Jian LIN, Zhiyuan ZHOU
Southern University of Science and Technology, China

We investigated the influences of the Kerguelen and Amsterdam-St. Paul (ASP) hotspots on the crustal accretion of nearby spreading ridges in the Eastern Indian Ocean. Gravity analysis and 3-D geodynamic modeling revealed enhanced ridge magmatism caused by Kerguelen and ASP hotspots, resulting in anomalously thick crust. Ridge-hotspot distance and plume flux are key factors controlling the strength of interaction. Our results reveal that in the top 200 km lid, the plate-driven shear flow controls the distribution of plume anomalies, and the plumes links to the nearby ridge due to ridge capture. By comparing the dual hotspots and single hotspot models, we found that the existence of Kerguelen hotspot leads to a ~200 km offset of the temperature and crustal anomalies of ASP, implying potential hotspot-hotspot interaction, which may also apply to other dual/multiple hotspots-ridge systems around the world.


SE08-A014
Unusual Activities Revealed by the Recent Fluid Geochemical Results in the Tatun Volcanic Group, Northern Taiwan

Hsiao-Fen LEE1,2#+, Ai-Ti CHEN3, Yuji SANO4, Ya-Chuan LAI5,6, Min-Hung SHIH7, Cheng-Horng LIN8, Ching-Hua LO3, Guo-Teng HONG9
1National Center for Research on Earthquake Engineering, National Applied Research Laboratories, Taiwan, 2Taiwan Volcano Observatory at Tatun, Taiwan, 3National Taiwan University, Taiwan, 4Kochi University, Japan, 5Taiwan Volcano Observatory - Tatun, Taiwan, 6National Center for Research on Earthquake Engineering, Taiwan, 7National Applied Research Laboratories, Taiwan, 8Academia Sinica, Taiwan, 9Central Geological Survey, Taiwan

The Tatun Volcanic Group (TVG) is an active volcano located in northern Taiwan. Volcanic activity could have significant impacts due to proximity to metropolitan areas. The Tatun Volcanic Observatory has been established since 2011. Its main task is to monitor the seismic activities, patterns of volcanic fluid flows and surface deformations of the TVG. Combined with recent changes in geochemical indicators and seismic event monitoring results, volcanic activities were relatively quiet during 2017-2018. At the end of 2018, there was a deep hydrothermal upwelling, and the exhalation gases of hydrogen chloride in the whole region began to increase. At the same time in 2019, the number of seismic activities increased, and several large-scale and deep-focus seismic events occurred in the TVG area. Helium concentrations of the venting gases increased, while the concentration of hydrogen chloride continued to increase. Numbers of seismic activities peaked in 2020, and then it was observed that the cation concentrations of hot spring of Dayoukeng (DYK) area, the most active area in the TVG, increased sharply in the late 2020. It was possibly due to the upwelling of a large number of deep hydrothermal fluids. Gas and water anomalies continue to occur in 2021, but seismic activities have slowed down as the pressure has been released. According to the surveillance video, in December 2021, a new fumarole appeared above the main fumarole in the DYK area. Surface environmental features also suggest mud splashes from this period. At the same time, several important parameters of fumarolic gas, such as SO2/H2S, HCl/CO2, He/Ar ratios, also changed significantly. The concentration of cations also reached the highest peak. Based on these changes, it is speculated that a small hydrothermal eruption might have occurred in the end of 2021.


SE08-A015
Simulating the Effect of Sea Level Change on Internal Stresses in the Tectonic Plates Along Subduction Zones to Study Its Impact on the Likelihood of Volcanism

Nathan TEO#+, Benoit TAISNE
Nanyang Technological University, Singapore

Prior research suggests sea level rise has an impact on volcanic activity, where, in coastal volcanoes, empirical data suggest volcanism increases with sea level rise. This project aims to explore the effect of sea-level change on various components of the internal stresses within the tectonic plates through finite-element physics simulations in COMSOL. The study is centred around profiles of Sumatra and Java, Indonesia, and Honshu, Japan, which are one of the most active regions in the world. Those two locations are also displaying differences in bathymetry leading to asymmetrical stress changes within the crust. A parametric study of the bathymetric profiles from the two regions is performed, applying the change in pressure attributed to sea level rise or drawdown on the top surface. The change in horizontal stress and gradient of the change in pressure with depth is analysed to infer the impact of sea level change on magmatic rise and consequently volcanic activity. The results of the simulation agree with the empirical data, with sea level drawdown discouraging magmatic rise and sea level rise favouring magmatic rise. Furthermore, a comparison of the asymmetry in the bathymetry between Indonesia and Japan is used to demonstrate significant differences in the stress response to sea level change and implications in volcanism and its location.


SE09-A005
Crustal Attenuation of Lg Wave in Eastern Tibet Plateau

Jing HE1#+, Qingju WU2, Eric SANDVOL3
1National Institute of Natural Hazards, Ministry of Emergency Management of China, China, 2China Earthquake Administration, China, 3University of Missouri, United States

Crust rheology is vital for understanding whether there is a large-scale crustal flow and its role in the lateral expansion of the Tibetan plateau. Here we apply the Reversed Two-Station Method using the waveforms recorded by the dense seismic networks to obtain the crustal Lg attenuation model in eastern Tibet, which is sensitive to crustal rheology, especially the partial melting, temperature, and fracture. Prominent low Q values, i.e., high crustal attenuation, are found beneath the Songpan-Ganzi block, the northwestern Sichuan sub-block, the Xiaojiang fault zone, and the Tengchong volcano. The low Q value in the Songpan-Ganzi block is strictly blocked by large faults, indicating the presence of partially molten crust related to the crustal composition and tectonic deformation. We interpret the geometry of low Q in the Songpan-Ganzi block as the signature of the localized crustal flow controlled by major faults. Low Q anomalies beneath the Xiaojiang fault and its adjacent region indicate a melt-weakened crust, which may be caused by a combination of fractured upper crust formed by the strike-slip faults, heating due to the thickening of the felsic mid-lower crust, and the possible thermal upwelling from the upper mantle.


SE09-A007
Groundroll Suppression in Qiangtang Basin Based on Local Orthogonalization

Xiao PAN#+, Xiaotao WEN
Chengdu University of Technology, China

As one of the large basins in Qinghai-Xizang Plateau, Qiangtang Basin attracts increasing attention. It owns good gas and oil accumulation condition and becomes the best potential reservoir. Seismic survey helps quantitively evaluate the reservoir with high resolution. Due to complex geological condition and unstable acquisition condition, groundroll exists and it masks reflections. In order to get accurate interpretation result, groundroll suppression is necessary to improve seismic data quality. In this paper, we apply local bandlimited orthogonalization method to iteratively separate reflections and groundroll. Compared with conventional FK filter, local orthogonalization has better ability to identify reflections and noise in detail. With the help of bandpass filtering, groundroll can be removed with much less reflection missing. Field data application proves that local bandlimited orthogonalization method works well in Qiangtang Basin and it improves the quality of seismic profile a lot. Good seismic profile helps to get an accurate interpretation result, which improves the understanding of the underground resources.


SE09-A011
The Spatial Distribution and Dynamic Mechanism of Low Viscosity Channels in the Middle and Lower Crust of the Sichuan-Yunnan Region

Bin SHAN#+
China University of Geosciences, China

The Sichuan-Yunnan region is located in the southeastern margin of the Qinghai-Tibet Plateau, plays an important role in explaining the dynamic processes of the uplift of the Qinghai-Tibet Plateau, the deformation of lithosphere and the eastward flow of materials from the Qinghai-Tibet Plateau. Therefore, the deep understanding of the lithospheric structure of the Sichuan-Yunnan region is the key to the recognition of the lithospheric deformation mechanism of the Qinghai-Tibet Plateau. Due to the respective limitations of different research methods, the lithospheric structure obtained for the Sichuan-Yunnan region and the modelling of possible tectonic evolution are still controversial, the lithospheric rheological structure is the basis for the understanding of these controversial issues. This paper constructs the lithospheric temperature structure in the Sichuan-Yunnan region with multiple geophysical observations, then the lithospheric lithological structure is constructed combining the petrology, geochemistry and seismic sounding data, finally this paper constructs the lithospheric rheological structure for the Sichuan-Yunnan region. This paper proposes that the impact of collision and compression between the Indian plate and the Eurasian plate since the Cenozoic era, on the one hand, led to the thickening and partial melting of the crust in the Qinghai Tibet Plateau, and on the other hand, led to the upwelling of deep mantle thermal materials in the southern Sichuan-Yunnan region, and weakened the lithosphere of the IndoChina block and the Sichuan Yunnan Diamond block. The weak material heading eastward from the middle and lower crust of the Qinghai Tibet Plateau can only flow to the Sichuan Yunnan Diamond block with relatively low strength and enter the IndoChina block across the Red-River fault zone, because it is blocked by hard formations such as the Sichuan Basin and Emeishan Large Igneous Province. Therefore, the Sichuan Yunnan region has become an important channel for the outflow of material from Tibet.


SE09-A017
Study on the Coseismic Surface Deformation and Seismic Risk Change Caused by the 2008 Wenchuan Earthquake

Mingqian SHI+, Caibo HU1,1#
University of Chinese Academy of Sciences, China

Coseismic deformation of large earthquakes is an important factor in causing significant property and personnel losses, which requires quantitative research of multiple disciplines such as joint geodesy, geological investigation, seismic tomography, and seismic dislocation theory. The 2008 Ms 8.0 Wenchuan earthquake is one of the most complex and strongest intraplate earthquakes. The Longmenshan fault zone, where the Wenchuan earthquake occurred, has an elevation difference of 4 km. The crustal thickness of the Qinghai-Tibet Plateau and Sichuan Basin beside the fault zone differ by tens of kilometers, and there is an obvious difference in composition. We have carried out a series of parallel finite element models to calculate the coseismic surface deformation of the 2008 Wenchuan earthquake. The parallel finite element models introducing split nodes and high-performance parallel computing technology can consider the effects of the regional material heterogeneity and geometric complexity of the earthquake. The correctness of the parallel elastic finite element program is verified by comparing the results of four ideal earthquake cases with the analytical solutions of seismic dislocation theory. The simulation results of the coseismic deformation of the Wenchuan earthquake are consistent with the geodetic GPS and InSAR data. Based on the coseismic stress field obtained by the finite element models, we calculated the Coulomb stress change on the main faults around the earthquake to evaluate the seismic risk change. The parallel finite element models lay an important foundation for the inversion of the coseismic fracture process based on the inhomogeneous model in the future. This research was financially supported by the National Science Foundation of China (42074117) and supported by the Fundamental Research Funds for the Central Universities. 


SE09-A019
Seismological Results Reveal That the Upwelling of Magma Led to the Uplift and Surficial Processes of the Namche Barwa Massif as One of the Most Active Areas

Siyuan CHENG+, Xuzhang SHEN#
Sun Yat-sen University, China

High-resolution imaging of the deep structure in the crust may be an important breakthrough to solve the problem of whether the rapid uplift of the Namche Barwa massif (NBM) is led by extremely high erosional exhumation or controlled by deep tectonics. Based on the seismic data recorded by 400 short-period dense seismic array located in the NBM, 4785 P-wave receiver functions (PRFs) are calculated and selected to obtain the migration image. The results show that there is a large range of weak (or missing) Moho under the Yarlung-Zangbo river in the northern margin of the NBM, and the upper crust is pushed upward in an inverted "V" shape. They are simulated and verified with spectral-element method (SEM). The results reveal that the ultrafast uplift and surface exhumation in the NBM may be caused by the upwelling of magma in the upper mantle, with its channel under the Yarlung-Zangbo river.


SE09-A028
The 2021 Luxian Ms 6.0 Earthquake: A Complete Release of the Localized Compressive Stress on a Limited-size Fault

Chaoliang WANG1#+, Liang CHUNTAO1, Jiangtao LIAO1, Zhenxing YAO2, Rui XU1, Yihai YANG3
1Chengdu University of Technology, China, 2Chinese Academy of Sciences, China, 3Shaanxi Earthquake Agency, China

On 16 September 2021, a destructive earthquake with surface-wave magnitude (Ms) of 6.0 broke the seismic quiescence of the Luxian county in the inner Sichuan Basin, China. Here, we explore the seismogenic structure of the Luxian earthquake by characterizing sedimentary faults in the spatiotemporal distribution of aftershocks, via the focal mechanism solutions and via the coseismic rupture model based on synthetic aperture radar interferometry (InSAR) data. Our results show that aftershocks concentrated at two clusters in the broad syncline. Seismicity of the northern cluster reveals that the main shock ruptured an east-southeast striking fault with a dip angle of ~ 45° to the southwest (F0), and activated a gently dipping (~ 18°) fault (F1) below F0 and a nearly vertical shallow fault (F2) on the northern side of F0. These three faults outline the edges of a thrust wedge in the sedimentary cover. The northern cluster occurred on two conjugate fault systems within which steep faults with different dipping direction interlaced downward forming ‘V’ shapes. Evidences from the aftershock focal mechanisms, Coulomb stress change and the post seismic stress field coherently indicate a reversal of the stress regime from the near north-south subhorizontal compressive stress regime before the main shock to the normal slip favored stress regime with the subvertical maximum principal stress. Further, the apparent deficit of seismicity at the periphery of the coseismic slip area on the fault plane indicates a limited size of the seismogenic fault. All these results indicate that complex fault system developed within the thick sedimentary cover, and inhomogeneous deformation of the sedimentary cover might cause localized stress concentration in the Sichuan Basin during multiple phases of tectonic deformation. We suggest that the Luxian Ms 6.0 earthquake as a typical event completely released the localized compressive stress.


SE09-A031
Magnetic Anomaly Characteristics and Magnetic Basement Structure in Earthquake-affected Changning Area of Southern Sichuan Basin, China: A New Perspective from Land-based Stations

Chao DONG#+
Institute of Geophysics, China Earthquake Administration, China

The Changning area is located in the southern Sichuan basin and the western Yangtze Plate and is the most abundant shale gas exploration area in China. In recent years, Changning has experienced frequent earthquakes with moderate magnitudes, attracting extensive interest. To investigate the magnetic characteristics in Changning, 952 land-based stations were employed to establish a magnetic anomaly model with a resolution of 2 km, and the subsurface magnetic basement structure was obtained by an iterative algorithm in the Fourier domain. The magnetic anomaly model shows significant distinctions between the northern salt mine area and the southern shale gas area. The magnetic basement includes the crystalline basement and the Sinian sedimentary rock metamorphic basement, which has strong magnetism. The large intracratonic rift that developed in the Sinian–Early Cambrian plays an important role in the evolution of Changning, which also impacts magnetic anomalies and the magnetic basement structure. Finally, by comparing the seismic wave velocity ratio structure, the deeper magnetic basement that corresponds to the higher seismic wave velocity ratio can be explained. This article implies that magnetic anomalies and magnetic basement depth have a certain correlation with earthquakes in Changning, and it provides a geodynamic reference for Changning and the southern Sichuan basin.


SE09-A038
Seismic Imaging of Crustal Structure Underneath the Foreland Basin and Siwalik in Nepal Himalaya Using Receiver Function Modeling

Sushrat MISHRA1#+, Kajaljyoti BORAH2, Aakash ANAND2, Pousali MUKHERJEE3, Dipok BORA4
1Indian Institute of Science Education and Research, Kolkata, India, 2Indian Institute of Science Education and Research Kolkata, India, 3Kyoto University, Japan, 4Diphu Government College, India

Flexure of the down-going Indian plate beneath the overriding Himalayas resulted in the formation of the Himalayan foreland basin. The thick sediments in the basin can cause local site amplification of seismic waves generated even from small-magnitude earthquakes. Also, due to these thick sedimentary layers, the underlying structure beneath the foreland basin and adjoining Siwalik becomes highly unreachable, and the dominance of multiples in the receiver function due to the sedimentary phase makes crustal imaging highly challenging. Hence the proper seismic image of the crustal structure is extremely important not only to assess seismic hazard in the region but also to get a handle on the mountain-building activity. We investigated the thickness and composition of the sedimentary layer and crust using H-κ stacking and NA (Neighbourhood Algorithm) modelling of receiver functions at 26 seismographs operated in the Siwaliks and Indo-Gangetic Plain in the Eastern Nepal Himalaya. Our study shows that in the foreland basin, sediment thickness varies from ~4.1-5 km, with Vp/Vs varying between ~2.31-2.78. In the Siwalik, the sediment thickness and Vp/Vs ratio are ~2.5-3.5 km and ~2.14-2.78, respectively. Similarly, the thickness and average Vp/Vs ratio of the crust in Indo-Gangetic Plain (IGP) and Siwaliks vary between ~40-44 km, 1.8-1.86 and 42.5-46 km, 1.77-1.87, respectively. In the­ first ~1-1.5 km of the sediment layer, we have observed very low Vs (<1.5 km/s) due to the very loose sediments having high seismic hazard potential. The average values of Vp and Vs suggest that in the sedimentary layer, the most probable rocks are sandstone and mudstone. Similarly, the possible lower crustal rocks underneath the IGP and Siwalik vary between Mafic garnet granulite and Mafic granulite. Our result has implications for modelling of mountain building activity and seismic hazard assessment in the region.


SE09-A041
Performance of LD-Array During the 2022 Mw 6.6 Luding Earthquake, Sichuan, China

Xinzhong YIN1#+, Qibin SHI2, Wenze DENG3, Jiuhui CHEN1, Shengji WEI4
1China Earthquake Administration, China, 2University of Washington, United States, 3China Earthquake Networks Center, China, 4Nanyang Technological University, Singapore

The 5 September 2022 Mw6.6 Luding earthquake (LDEQ) occurred on the Moxi segment of the highly active Xianshuihe fault (XSHF) zone in eastern Tibetan Plateau, in Sichuan Province, China, causing 93 casualties and 24 people missing, and substantial damages in the epicentral regions. The Luding Array (LD-Array) is covered the mainshock area. The LD-Array is consists of three types of seismographs, including low-cost acceleration intensity sensors (758), strong motion meters (323) and broadband seismographs (106). Using a path-calibration method, we select the highest quality strong motion and broadband stations mostly on the bedrock sites to derive a Multiple-Point-Source (MPS) model for the mainshock. We then perform joint inversion on the static GPS, strong motion and teleseismic body waves to obtain a finite fault model of the mainshock. This is followed by forward modeling of all the LD-Array stations to verify the array performance. The array observations are also used to test the recent ground-motion prediction equations (GMPE) for the Southwestern parts of China. We find: 1) The MPS model composes of three major subevents that are distributed in a compact area where the aftershock seismicity shows a clear gap. 2) Finite fault model shows a compact slip distribution with along strike dimension of ~14 km. 3) LD-Array clearly captured the rupture directivity of the mainshock. Most of the amplitude of the low-cost acceleration intensity sensor waveforms are reliable and part of waveforms could be modeled. The GMPE from Zhao et al. (2017) generally fits well the PGA from observations, but there is still room for improvement, such as considering azimuthal variation (i.e. focal mechanism); 4) The LD-Array can be applied to other areas to enable seismological research such as seismic event detection and location, deep structure imaging, earthquake source physics, as well as earthquake early warning.


SE09-A042
Study on Present Gravity Change and Deep Crust Deformation of the Red River Fault Zone

Jian WANG#+
China Earthquake Administration, China

In order to detect the current material migration and deformation characteristics in the crust along the Red River fault zone (RRFZ), we analyzed and removed the gravity changes caused by vertical surface movement, surface water circulation, denudation, and glacial isostatic adjustment effects based on mobile gravity observation data of 3 profiles in the northern and middle section of the RRFZ from 2013 to 2019, and obtained the trend of gravity change caused by the migration of materials in the deep crust. Based on recent gravity changes and crustal structure models, the deformation characteristics of Moho surface along the northern, middle, and middle- southern sections of the RRFZ are inverted. The results shows gravity change of the RRFZ has segmental characteristics, gravity change rate of the northern /middle/ middle-southern section of the RRFZ are -0.39±1.30, 0.16± 1.57, 0.29±1.25μGal/a. Moho beneath the RRFZ uplifts continuously with an average rate of 0.54 cm/a in recent period. Average deformation rate of the northern, middle, and middle-southern section of the Red River fault zone is -0.06 cm/a, 1.36 cm/a and 0.32 cm/a, reflecting the effect of regional unbalanced tectonic movement to a certain extent.


SE09-A047
Implications of Various Magnitude Scales in Western China

Zujun XIE#+
China University of Geosciences, China

Magnitude is a parameter measuring the size of an earthquake, yielding units of order 1 which are intuitively attractive, and is indispensable in seismic scientific research and seismic hazard assessment. The definition of magnitude has various scales, like ML, mb, MS (MS_BB), mB (mB_BB) and MW, based on different calibration. The discrepancy of the definitions results in the commonly different values, mainly because of diverse seismic phases and frequent bands adopted. Although magnitude conversions are often proposed for scientific research purpose, such as seismicity analysis, their differences revealing the different characteristics of seismic sources should be deserved more of a concern. In this study, the waveform of earthquakes of M > 4.5 in western China since 2009 have been collected and three magnitude scales, MS(BB), mB(BB), re-estimated according to the New National Standard of Magnitude issued in 2017 in China and MW, assessed by waveform inversion, are compared and analyzed statistically. The results show, (1) differences between magnitude scales depend on the research region, implying the differences between tectonic environments. Earthquakes with large MS and mB relative to MW correspond to regions with stronger crustal lithosphere strength, suggesting the accumulated stress on the faults are probably more higher. Contrarily, earthquakes with large MW relative to MS and mB are prone to rupture on the mature seismic faults, implying that the heterogeneities of fault zones maybe not relatively distinct. (2) differences between various magnitudes also rely on the source type of focal mechanism, which may reflect the different frictional strength. (3) those events occurred in the neighboring region, with similar MS (mB) but significant discrepancy of Mw indicate the different rigidity of the medium structure in the local area near the fault zones, which has relatively significant influence on the magnitude of MW.


SE10-A002
Pumice Erupted by Fukutoku-Oka-no-Ba Observed in and Around Taiwan from Satellite Imagery

Sin-Mei NG#+, Hong-Xuan CHEN
Chinese Culture University, Taiwan

Fukutoku-Oka-no-Ba (FOB), a submarine volcano, is situated at approximately 60 km south of Loto Island in the Ogasawara Islands (also known as the Bonin Islands) which are, in turn, a part of the Izu–Bonin – Mariana (IBM) arc system in the eastern Philippine Sea. On 13th August, 2021, a large eruption occurred; and it ended two days later. An approximately 1 km, horseshoe-shaped, new island was formed and reported by the Japan Coast Guard on 15th August, 2021. Besides the formation of the new volcanic island, the large submarine eruption also produced a large quantity amount of pumice. A week after the eruption, pumice with gray, vesicular, and having a groundmass that contains black enclaves were collected in the ocean near FOB. Clinopyroxene, plagioclase and rare olivine phenocrysts were found in the pumice clasts. By the end of November, the drifting pumice had already reached the Green Island in the southeast; and, by the early to mid-December, it appeared in the northern coast of Taiwan. The sudden surge of large amount of pumice from the FOB eruption in the coast may cause marine hazard. Previous studies integrated multiple optical and SAR data to investigate similar pumice raft events and tracked the sequential motions. Pumice is rhyolite glass in which expanding gas bubbles have distended the magma to form a highly vesicular material. In this poster, we are going to show the trace of pumice in and around Taiwan region seen by satellite imagery.


SE10-A010
Tectonic Vertical Land Motions in Southeast Asia Through the Lens of Geodetic Observations and Earthquake Deformation Models

Grace NG1#+, Dongju PENG1, Lujia FENG1, Xin ZHOU2, Haipeng LUO3, Kelin WANG4, Chien Zheng YONG5, Susilo SUSILO6, Irwan MEILANO7, Emma HILL1
1Nanyang Technological University, Singapore, 2Ministry of Emergency Management of China, China, 3University of Victoria, Canada, 4Geological Survey of Canada, Canada, 5School of Surveying, University of Otago, New Zealand, 6National Agency for Research and Innovation, Indonesia, 7Bandung Institute of Technology, Indonesia

Regional sea-level changes in Southeast Asia are highly variable due to the influence of both climate and solid Earth processes. In particular, vertical land motions (VLM) due to tectonics are a major source of local spatial variability and uncertainty owing to recent earthquake history and mantle dynamics at regional subduction zones. Over the last two decades, the Sumatran subduction zone hosted a series of large earthquakes starting with the 2004 Mw 9.2 Sumatra-Andaman earthquake. These large earthquakes not only rapidly changed land heights by several meters near the earthquake locations, but also induced longer-term changes in the distant back-arc regions through broadscale mantle processes. At some locations, the tectonic VLM changes can be comparable to or greater than climate-induced sea-level changes. Thus, to generate accurate and robust regional sea-level projection models for coastal risk assessment and adaptation planning, it is imperative to quantify the contribution of tectonic VLM. To quantify the tectonic VLM, we use a variety of modelling techniques to estimate the surface deformation caused by the recent earthquakes, focusing on the postseismic viscoelastic relaxation process controlled by the mantle rheological structure. To constrain our models, we employ new techniques to derive VLM from satellite altimetry and tide gauge data to supplement GNSS observations that are often limited by spatial and temporal availability in our region. From our results, many Southeast Asian countries – including Thailand, Peninsula Malaysia, and Singapore – are vulnerable to postseismic subsidence following the Sumatran earthquakes. The broad subsidence can last for years or even decades. Though some of these countries are far from the trench and the rate of subsidence is small, the total cumulative subsidence over many years is non-negligible and adds to the climate-induced relative sea-level rise.


SE13-A003
Empirical and Physical-based Waveform Simulations for Moderate-large (M6+) Earthquake Scenarios in Taiwan

Min-Hsuan CHANG#+, Yen-Yu LIN, Ming-Che HSIEH
National Central University, Taiwan

Earthquake early warning systems have been used to mitigate injuries and damage worldwide for many years. To improve the efficiency of the systems, more studies account for machine learning approaches to predict the intensity distribution without calculating magnitude and location of the event. However, lack of seismic records for moderate-large (M6+) earthquakes may give unstable extrapolations while predicting intensities. To fill the lack, we demonstrate two approaches, the empirical Green's function (EGF) and the strain Green's tensor (SGT), in simulating seismic waveforms for moderate-large earthquake scenarios in Taiwan. In the EGF approach, we first compute the relative source-time function (RSTF) between the small event with the observed waveforms and the scenario event. We then convolve the RSTF and the observed waveforms to simulate the waveforms of the scenario event. On the other hand, the SGT approach allows us to perform synthetics of the scenarios physically, considering possible rupture dimension, speed, asperity, as well as 3D velocity structure and site effect. Here, three M6+ events in Taiwan, the 2013 Nantou, the 2016 Meinong, and the 2019 Hualien earthquakes, are selected to validate the two approaches. In the EGF approach, the intensities from the synthetic waveforms are similar to those from the observations in the frequency range of 0.2~1 Hz for all events. However, the synthetics of the SGT approach show good intensity predictions for the Hualien event but underestimated intensities for the Nantou and the Meinong events in the same frequency range. It may be due to the underestimates of site effect, which needs further investigation. Our results suggest that both approaches may fill the lack of seismic records for moderate-large earthquakes and have the potential to provide synthetic data as inputs for adjusting the available ground motion models and even machine learning for early warning.


SE13-A004
Relationship Between Inland Seismicity and Crustal Deformation After the 2011 Tohoku Earthquake Derived from the Refined Earthquake Catalog

Koji TAMARIBUCHI#+, Hisao KIMURA
Meteorological Research Institute, Japan

After the 2011 Mw 9.0 Tohoku earthquake, seismic activity increased throughout Japan. Due to the large number of earthquakes, microearthquakes (M<2 inland, M<3 offshore) were not always catalogued, making it difficult to comprehensively quantify the changes in seismic activity after the 2011 Tohoku earthquake. We developed an automatic hypocenter determination method using machine learning and detected earthquakes that were three times larger than those in the conventional earthquake catalog from March 2011 to February 2012. We then merged the automatically determined catalog and the JMA unified catalog and extracted the inland seismic activity throughout Japan from the obtained merged catalog. In this study, we quantified the seismic activity after the 2011 Tohoku earthquake based on the ETAS model. The obtained relative changes in seismic activity show that, on average, the background seismicity rate in April 2011 is 2-3 times higher than that before the Tohoku earthquake. The background seismicity rate gradually returned to its original level over time. We compared the background seismicity rate with the maximum shear strain rate in the surrounding area based on the one-month difference in GNSS data. We found that a positive correlation. These results should help quantify the impact of large earthquakes on inland seismic activity and lead to future risk assessments. Acknowledgements: We used the waveforms from JMA, NIED, universities, and institutions, and the JMA unified earthquake catalog. We used GEONET (F5) coordinate data from GSI. We used etas_solve from Kasahara et al. (2016) to estimate ETAS parameters, and Shen et al. (1996, 2015) to calculate strain rates.


SE13-A007
An Earthquakes Rate Model of the Sumatran Fault Considering Rupture Complexity and Its Application to Seismic Hazard Assessment

Rizki WULANDARI1#+, Chung-Han CHAN2
1Sumatera Institute of Technology (ITERA), Indonesia, 2National Central University, Taiwan

The Sumatran fault zone (SFZ) is 1900 km in length in the Sumatran fore-arc. According to geological and geomorphological evidence and ruptures of historical earthquakes, SFZ consists of 40 strike-slip fault segments, however, its potential rupture behaviour and the possibility of multiple-fault ruptures remain controversial. In this study, we aim to develop a more realistic rupture model for seismic hazard assessment of the SFZ. We apply an approach, namely ‘Seismic hazard and earthquake rate in fault systems’ (also known as ‘SHERIFS’), that models fault activities in the form of complex multiple-segment rupture by considering slip rate of the segments, instrumental catalogue data and paleoseismic record. The instrumental catalogue is implemented to defined background seismicity through magnitude frequency distribution. We analyse several fault rupture hypotheses, defined as criteria based on fault geometry, distance, and location of the segments. By comparing seismic rate obtained by paleoseismic data and the partitioning rate of single-rupture and multiple-fault ruptures, we identified the better fit probability of each hypotheses. The earthquake probability for a larger magnitude in the SFZ could be higher due to elevated characteristic magnitude of the rupture in a multiple-segments scenario. The procedure of this study could be applied to other fault system with complex rupture behaviours and our outcomes in the form of magnitude-frequency distribution for seismic activity in the SFZ provide crucial parameters for subsequent probabilistic seismic hazard assessment in Sumatra.


SE13-A008
Time-dependent Seismic Hazard Analysis in Chinese Mainland Based on BPT Model

Weijin XU1#+, Jian WU2, Mengtan GAO3
1Institute of Geophysics, China Earthquake Administration, China, 2China Earthquake Disaster Prevention Center, China, 3China Earthquake Administration, China

The results of probabilistic seismic hazard analysis are important basis for seismic hazard mapping, seismic safety assessment of major engineering sites and seismic risk management, etc. Seismic temporal activity model is the main theoretical basis for probabilistic seismic hazard analysis. In this study, we calculate the time-dependent seismic rate of the seismic sources of characteristic earthquakes in mainland China based on the Brownian Passage Time (BPT) model. By using the probabilistic earthquake hazard calculation method, we select an appropriate ground motion model to evaluate the time-dependent seismic hazard in mainland China. The results are compared with those based on Poisson model. Results show that the time dependent characteristic of earthquake has a significant impact on the result of the probability seismic hazard. Compared with the Poisson model-based seismic hazard results, the time-dependent seismic hazard results are significantly higher than those based on Poisson model in seismic source regions with relatively long elapsed time and large elapsed rate (greater than 1), with the maximum increase of more than 50%. On the contrary, the time-dependent seismic hazard results in the seismic source regions with short elapsed time are significantly reduced compared with Poisson's model, with a maximum reduction of about 50%. The coefficient of variation of earthquake recurrence interval also has significant influence on the seismic risk results, so the study on the uncertainty of earthquake recurrence interval should be strengthened. The results also show that the time-dependent seismic activity characteristics have a consistent effect on the seismic hazard results under different exceedance probabilities. The results of this study are an important supplement to the traditional time-independent (Poisson model) seismic hazard results, and have important significance for earthquake risk management, earthquake insurance and the formulation of earthquake protection and disaster reduction policies.


SE13-A019
Microtremor Analysis Using Horizontal to Vertical Spectral Ratio Method in Central Java, Indonesia

Nur RAHMI#+, Shindy ROSALIA, Zulfakriza
Bandung Institute of Technology, Indonesia

Central Java is known for its complex and active geological conditions, with a variety of geological features such as active volcanoes, tectonic plates, and fault lines. The region is located on two major tectonic plates, the Indo-Australian Plate and the Sunda Plate, which creates a high level of seismic activity and is prone to earthquakes. The existence of active volcanoes including Mount Merapi, Mount Merbabu, Mount Ungaran, Mount Slamet, and the Dieng Plateau is also evidence of the dynamic geological condition in Central Java. In addition, the Kendeng Basin, which is a continuation of the North Serayu Mountains that continues to the eastern part of Java makes the study of the geological conditions in Central Java challenging, especially for seismic hazard analysis. A microtremor analysis study is needed to complete the understanding of the subsurface structures in Central Java. In this study, the HVSR method is used to identify the dominant frequency of the site, the site-specific amplification, and Vs30 which is a key factor in determining the seismic hazard and risk. The data used in this study was data from 120 seismometers of MERAMEX network (July 2004). Our result shows that the dominant frequency values for the Central Java region range from 0.5 to 10.5 Hz with low frequency shown in the west of Jogjakarta to the north. The amplification values of this region are in the range of 0.7-13.6 with high amplification shown in the western part of Central Java, and the shear wave velocity values of 30 meters depth are found between 150-685 m/s.


SE13-A021
Probabilistic Seismic Hazard Analysis Based on Arias Intensity in Chinese Mainland

Xuejing LI1#+, Mengtan GAO2, Weijin XU3
1Institute of Geophysics, China Earthquake Administration, China, 2China Earthquake Administration, China, 3Institute of Geophysics, China Earthquake Administration, China

Arias Intensity is a parameter of ground motion obtained by integrating the square of ground motion acceleration through the whole duration of a seismic record. It is an important index to describe the intensity of ground motion and plays an important role in characterizing earthquake disasters such as earthquake-induced landslides and liquefaction. We carry out probabilistic seismic hazard analysis based on Arias intensity in Chinese Mainland. In this paper, we adopt the Fifth Generation Seismic Source Model of China (FGSSMC), and two sets of Arias intensity prediction equations (Travasarou and Bray(2003), Foulser-Piggott and Stafford (2012)) to calculate the values of Arias intensity at 10% exceedance probability in 50 years in Chinese Mainland. The results show that in Chinese Mainland, the Arias intensity is greater than 0.11m/s in 60% of the area, which has a risk of earthquake-induced landslides, the Arias intensity is greater than 0.32m/s in 30% of the area, which has a high risk of earthquake-induced landslides, and the Arias intensity is greater than 0.54m/s over 15% of the area which has a very high risk of earthquake - induced landslides. The provincial capitals and most prefecture-level cities in western China are located in the regions with Arias intensity values greater than 0.32m/s. The Arias intensity around the main fault zone is above 0.54m/s. It means that western China has a high risk of earthquake-induced landslides and liquefaction. In addition, the probabilistic seismic hazard analysis based on Arias intensity takes into account the impact of large earthquakes more than the probabilistic seismic hazard analysis based on peak ground acceleration, which has important reference value for the seismic safety assessment of major construction projects. The research results of this paper are of great significance to the prediction and prevention of earthquake disasters in mainland China.


SE13-A023
Risk Assessment of People Trapped in Earthquake Disasters Based on Single Buildings: A Case Study in Xichang City, Sichuan Province, China

Benyong WEI#+, Guiwu SU, Wenhua QI
Institute of Geology, China Earthquake Administration, China

Earthquakes are the most unpredictable natural hazards. A quake occurs almost instantaneously, but the impact lasts for a long time and causes great human losses. Strengthening the study of trapped personnel distribution in an earthquake not only ensures the efficiency and orderliness of earthquake rescue but also maximizes the survival probability of trapped people and reduces casualties. Through distinguishing the use functions of buildings, this study constructed an assessment model of people trapped in a collapsed single building due to an earthquake and evaluated the risk of individuals trapped in Xichang area, China. The results showed that the risk level of people trapped in collapsed buildings in Xichang area is high. Under the influence of seismic intensity Ⅸ, the proportion of people trapped in collapsed buildings has reached approximately 1-2% of the total regional population. The risk level of trapped people in the daytime and at nighttime caused by the same earthquake scenario is significantly different. The number of potentially trapped people at night is nearly two times greater than that during the day. The low seismic performance of buildings is the most important factor causing the high risk of people trapped. The use function of buildings also has an important effect on the risk assessment of the trapped population distribution. Improving the seismic performance of buildings is the basic way to reduce the risk of regional people trapped. It is also necessary to increase the investigations and studies of the law of regional population flow, by introducing mobile big data and high-precision household census data. Building-level data could provide more practical disaster information for ESAR and decision-making, due to it can significantly distinguish the use functions of single buildings and population distribution during the daytime and nighttime.


SE13-A025
Multi-sensing Based Approach to Mapping Exposure and Seismic Vulnerability of Buildings in a Context of Rapid Socioeconomic Growth: A Case Study in Tangshan, China

Wenhua QI#+, Guiwu SU, Benyong WEI
Institute of Geology, China Earthquake Administration, China

Due to dynamic urban growth, exposure and seismic vulnerability of buildings is highly variable over short time scales, especially in areas with rapid socioeconomic development. In this regard the continuous monitoring of building-related conditions is a challenging task, particularly in large-area. Fortunately, Earth Observation (EO) and Information and Communication Technology (ICT) has provided unprecedented hope for addressing the challenging task. Synthetically using EO and ICT, we develop a remote- and social-sensing based approach to mapping exposure and seismic vulnerability of buildings in a context of rapid socioeconomic growth. This approach employs different strategies to extract vulnerability-related parameters of buildings in urban and rural part, respectively. For buildings in urban area, data of VHR imageries and passive social sensing (e.g., internet-resources/mobile signaling), and techniques of deep learning (ARC-Net) and machine learning (Random Forest) were used to derive vulnerability-related parameters at building level. These parameters include footprint/shape, number of stories, structure-type, age, and usage. For buildings in rural area, vulnerability-related parameters were extracted at village level through active social sensing (crowdsourcing). Using Geographical Citizen Science framework, citizens from pilot villages and project members co-determined the collection form to and co-designed the mobile APP to gather building-related data. The structure-type ratio, age ratio, and function ratio of buildings in whole village was obtained. Besides, this co-designed APP can be used to gather more detailed parameters of single typical building, such as construction-material, structural column setting, and soil condition. This approach is demonstrated in Tangshan, China, which was hit severely by the 1976 earthquake with Ms 7.8. The exposure and vulnerability-related parameters of buildings in 2020 were obtained. The verification showed that this approach has good accuracy and substantial labor-/time-/money-saving in covering large areas. Therefore, this multi-sensing based approach might have promising prospects in actual seismic loss risk reduction challenges.


SE13-A028
Macroseismic Map of the 21 July 2022 Keng Tung Earthquake in Eastern Myanmar and the Relationship Between the Felt Intensity and Ground Motion Data

Ei Mhone Nathar MYO1#+, Yu WANG1, Yih-Min WU1, Hsin-Hua HUANG2, Chung-Han CHAN3, Myo THANT4,5, Lin Thu AUNG6
1National Taiwan University, Taiwan, 2Academia Sinica, Taiwan, 3National Central University, Taiwan, 4University of Yangon, Myanmar, 5Myanmar Earthquake Committee, Myanmar, 6Nanyang Technological University, Singapore

In 21 July 2022, a moderate Mw 5.9 earthquake occurred ~ 30 km south east part of the Keng Tung (Kyaing Tone) Township in eastern Myanmar, close to the western end of the Wan Ha fault within the Shan Fault system. Reports from social media and local news suggests the earthquake caused building damages and landslides near the mainshock epicenter, and was felt from the southernmost Yunnan to the central Thailand area. In order to understand the mechanism of this earthquake event, and to built the regional relationship between the felt intensity and the instrumental peak ground motions, we collect felt reports and damaging photos from the social media and digital news to conduct the macroseismic investigation of this earthquake events. Meanwhile, we also use data from the regional seismic network to relocate Keng Tung earthquake sequence to determine the source of this earthquake sequence. After the Double Difference Relocation analysis, we found the relocated Keng Tung earthquake sequence delineate the NE-SW trending Wan Ha Fault trace, with focal depth between 20 to 35 km. This suggests the main trace of the Wan Ha fault is indeed the source of the Keng Tung earthquake. As for the macroseismic investigation, we interpret more than 75 felt reports from the mainshock and compare these felt accounts to the instrumental data. Our analysis suggests the felt intensity fits the PGV data better than the PGA in the region of Myanmar and Thailand, and the building damages near epicenter is likely caused by the combination of poor construction quality and site conditions. We hope these results will help us to establish a better model to describe the earthquake damage and ground motion in the central part of mainland SE Asia in the future.


SE13-A029
Accelerograph Records of Ground Motion in Metro Manila During Two Earthquake Events

Hannah PEÑA1#+, Alfredo Mahar LAGMAY2,3
1University of the Philippines Resilience Institute, Philippines, 2University of the Philippines Diliman, Philippines, 3University of the Philippines, Philippines

A number of studies explored and quantified the effect of factors that either attenuate or amplify ground motion during an earthquake. Among the earliest predictors of site response include earthquake magnitude and proximity of a site from the earthquake source. In this study, we look at two earthquake events wherein ground shaking was instrumentally recorded in Metro Manila – the 2019 Mwp6.1 Central Luzon earthquake and the 2022 Mw7.0 Northwest Luzon earthquake which ruptured approximately 85 km and 340 km away from Metro Manila, respectively. Values of ground motion are derived from accelerograph data recorded in various measurement sites in the study area. Furthermore, this study explores the relationship of ground motion and subsurface characteristics by using borehole data taken from different locations within the region. In preparation for the next rupture event along the ~100km-long West Valley Fault which runs through Metro Manila, this study aims to contribute new insights to the study of seismic hazards which can help mitigate the effects of the next big earthquake, possibly a >M7 event, in this area which is among the most densely-populated regions in the world.


SE14-A004
Upper Mantle Anisotropy in North China Craton from SKS Splitting

Zhengyang QIANG1#+, Qingju WU2, Yonghua LI2
1Institute of Geophysics , China Earthquake Administration, China, 2China Earthquake Administration, China

The North China Craton (NCC) is one of the oldest continental nuclei in the world. Formed by the amalgamation of the eastern NCC (ENCC) and western NCC (WNCC) along the Trans-North China Orogen (TNCO) at ∼1.9 Ga, the NCC was essentially stable until the Mesozoic when the ENCC experienced significant tectonic reactivation and destruction, despite the apparent lack of internal deformation in WNCC. Being the major part of the WNCC, the Ordos Block is surrounded by Circum-Ordos Rifts. Since the Cenozoic, the Rifts were relatively active and developed strong destructive earthquakes. The Ordos block has a thick crust (40 ∼ 48 km) and lithosphere (160 ∼ 200 km), in contrast to the relatively thin crust (30 ∼ 36 km) and lithosphere (80 ∼ 140 km) beneath the TNCO, indicating lithospheric remobilization and thinning. In order to understand the lithospheric deformation and the possible mantle flow thereby, we estimate over 2,000 shear wave splitting parameters from 84 teleseismic earthquakes recorded at 465 temporary broadband stations dispersed over the western and central North China Craton. A thick Archean cratonic keel has been mapped in the interior of the Ordos Block, where W-E trending fast polarization directions with small delay times are indicative of stable terrane. While a combined effect of the APM-induced mantle fabric and a mantle flow around the southeast edges of the Ordos Block explains the dominant W-E fast orientations with relatively large delay times. The prominent rift-orthogonal fast orientations beneath rifts to the northern Ordos Block imply the existence of active mantle flow. Also, it is inferred that a mantle plume is responsible for generating the parabolic fast direction pattern beneath the Datong Volcano. This work was supported by the National Natural Science Foundation of China (Grants U1839210, 41804084)


SE14-A010
Delineation of Crustal Configuration of the Eastern Ghats Mobile Belt, Odisha, India Using Global Gravity Data and Its Relation with the Non-volcanic Geothermal Systems

Ananya P. MUKHERJEE1, Aurobindo Kumar BASANTARAY2, Animesh MANDAL1#+
1Indian Institute of Technology Kanpur, India, 2Earth Sciences, Indian Institute of Technology Kanpur, India

The Eastern Ghats Mobile belt (EGMB) has a complex tectonic evolution history but is generally considered as a stable continental region. The presence of geothermal systems scattered within the belt are in contradiction to the stable region, whose thermal sources are said to be non-volcanic in nature. Satellite derived globally gridded topography and free-air gravity data are used in this study to investigate the subsurface structures below the region covering three such non-volcanic geothermal systems, namely, Tarabalo, Atri and Taptapani hot-springs, located near the east Indian coastal region in Odisha, India. The calculated Bouguer gravity anomaly shows that the hot-springs are situated in regions showing moderate to high gravity anomalies which lie at proximity to major shear zones making up the EGMB region. The radially averaged power spectrum analysis reveals the deepest interface to be at ~20.7km. The residual Bouguer gravity anomaly obtained by removing the 20 km upward continued regional anomaly from the complete Bouguer anomaly shows the presence of some lineaments lying close to the hot-springs. Applying edge enhancement techniques delineated these lineaments and are correlated with the existing structural information available for the study region. Parker-Oldenburg iterative inversion algorithm is utilized to obtain the Moho structure prevalent below the study area, with depths to the Moho surface ranging from 28 to 38 km. The shallowest Moho is observed around the Mahanadi rift basin region, where the Tarabalo and Atri hot-springs are located and the Taptapani hot-spring region shows a Moho depth of ~34 km. The obtained results from the global gravity data indicates that the moderately shallow Moho structure owing to the crustal reworking and the major lineaments resulting due to past supercontinent reconstructions involving the EGMB, play a significant role in aiding the formation of the heat source and evolution of these non-volcanic hot-springs.


SE15-A008
A Method for Predicting Shallow Landslide Induced by Climate Change in Permafrost Areas

Yu LUO#+
Institute of Mountain Hazards and Environment, Chines Academy of Sciences, China

Landslide is one of the most serious geological hazard in mountainous regions around the world. It is well known that landslide is associated with many environment factors, such as rainfall, earthquake, human activities, and so on. In recent years, with the globe temperature growing, there are more and more landslides occur in permafrost areas. Researchers found that climate change is the main environment factor lead to landslide in permafrost areas. Therefore, this study considers the effect of temperature change on active layer in permafrost areas, combined with the infinite slope theory, propose a new physical-based model to predicting the landslide induced by temperature change in frigid zone. That is a new method proposed here, in order to help researches to producing temperature-change-induced landslide hazards maps in permafrost areas, under the condition that the globe climate change result in the globe temperature growing.


SE15-A009
The Volcanic Ash Dispersion System in Meteorological Service Singapore

Zhong-Yi CHIA1#+, Chee-Kiat TEO2, Efthymia PAVLIDOU1, Boon Ning CHEW2
1Meteorological Service Singapore, Singapore, 2Centre for Climate Research Singapore, Singapore

Singapore is located near the Pacific Ring of Fire. The country’s aviation industry and air quality could be impacted by the volcanic ash, should a volcano eruption happen within the region. Therefore, Meteorological Service Singapore (MSS) monitors the regional volcano eruptions and provides volcanic ash alert to local stakeholders when there is a significant eruption. As part of the effort in volcanic ash monitoring, MSS maintains a volcanic ash dispersion modelling system that forecasts the atmospheric dispersion of the volcanic ash. The system is broadly based on a similar system operated by the UK Met Office (UKMO) for the London Volcanic Ash Advisory Centre (VAAC). It is built on the Numerical Atmospheric-dispersion Modelling Environment (NAME), an atmospheric dispersion model developed by the UKMO. This system estimates the ash plume from a set of prescribed eruption parameters – namely the location and height of the volcano, the eruption plume height, the eruption starting time and duration. The turbulent transport of the volcanic ash within the atmosphere is simulated using the meteorological data from the numerical weather forecast from the Integrated Forecasting System (IFS) maintained by European Centre for Medium-Range Weather Forecasts (ECMWF). Here, we discuss the modelling results of some eruption cases in Southeast Asia. The model uncertainties and potential areas for improvement will also be discussed.


SE15-A015
Long Term Deformation Analysis Inferred from Space Borne Geodetic Observation in NW Himalaya

Somalin NATH1#+, Rajat Subhra CHATTERJEE2, Onkar DIKSHIT1, B. NAGARAJAN1
1Indian Institute of Technology Kanpur, India, 2Indian Institute of Remote Sensing, India

The complex tectonic settings of NW Himalaya have drawn considerable attention from various researchers because of the vulnerability of seismic hazards at different scales. DInSAR offers the typical advantages of the remote sensing techniques. However, it is important to underline that high quality results can only be achieved by employing an adequate InSAR processing (image registration, filtering, phase unwrapping, etc.), coupled with an appropriate statistical treatment of the DInSAR observations. For strain accumulation analysis, we used L band ALOS PALSAR 1 & 2 image pairs with long temporal baselines and large areas of coverage for investigating deformation over NW Himalaya. The data sets were further spatial-temporally analyzed with phase and atmospheric correction. The corrected phase profile with major tectonic structures show the possible areas of strain accumulation with comparatively consistent high phase value over the years. The DInSAR phase profiles using ALOS 1 and 2 data show a maximum value show a maximum phase over the area in and around MCT depicts a major strain accumulation zone around MCT with a LOS displacement of ~2 cm per year. High phase value around MCT suggests the possible area of strain accumulation with considerable number of seismic events with a deformation up to ~100 kms up to HFT. This high phase value near MCT shows no correlation with surface elevation, indicating that the effect of tropospheric delay has been correctly compensated.


SE15-A019
Hazard Assessment of Volcanic Debris Avalanches at the Northwest Flank of Merapi Volcano

Sulistiyani SULISTIYANI1#+, Dary Putra Utama ASMARAKUSUMA1, Raditya PUTRA1, Dwi JAYANTO1, Yulianto YULIANTO1, Agus Budi SANTOSO1, Christina WIDIWIJAYANTI2
1Geological Agency, Indonesia, 2Nanyang Technological University, Singapore

Merapi Volcano entered a new effusive eruption episode on January 4, 2021, manifested by lava dome growth-producing rock falls, pyroclastic density currents (PDC), and lahars. For the first time in history, Merapi has two lava domes in one eruption period that grew simultaneously at the southwest side of the outer crater wall and in the (center) crater. The precursory signs are indicated by the gradual increase in seismicity and deformation (slope-distance of the summit Electronic Distance Measurements (EDM) reflector (RB1) measured from the Babadan Observatory) observed from June to September 2020. Towards the eruption onset, a sectorized shortening that was only observed at this West-Northwest flank’ EDM was accelerated concurrently with the heightened seismicity, which revealed a non-concentric deformation field over the Merapi edifice. The total slope distance shortening until February 13, 2023, was 15.5m, confirmed by measurement at the second reflector (RB2) located 150m below RB1 (2,645m elevation). This posed a new concern on possible flank instability that could initiate sector collapse of the northwest sector of Merapi, which was represented by the 1888 lava block. As part of the hazard mitigation effort, we performed the assessment of different scenarios, e.g., debris avalanche, PDC, and rockfall, with the granular flow simulation model using Titan2D software. Our objective is to delineate areas potentially impacted by such hazards, with a possible range of scenarios reflecting different initial source conditions, source volume, and flow mobility. In addition to the existing volcano hazard map created post-2010 eruption, it is essential to perform short-term hazard evaluation to anticipate the evolving hazards during the ongoing eruption of Merapi, which is useful for contingency planning.


SE15-A021
A Rugged, Portable and Intelligent Analogue Seismometer for Future and Pre-existing Arrays – Güralp Certis

Ella PRICE#, Neil WATKISS+, James LINDSEY, Phil HILL
Guralp Systems Ltd, United Kingdom

Seismic networks often face logistical and financial challenges that require portability, longevity and interoperability with existing equipment.
Güralp have combined proven ocean bottom, borehole and digitiser technology to produce an analogue seismometer with intelligence that benefits networks of all sizes. The Güralp Certis is a broadband analogue instrument that incorporates specific aspects of its sister digital instrument (Certimus) while still remaining compatible with third-party digitisers.
Each Certis stores its own serial number, calibration and response parameters internally and will automatically communicate these to a connected Minimus digitiser. This allows seismometer-digitiser pairings to be changed without manual entry of new parameters. If using GDI-link streaming protocol with the Minimus, these metadata parameters are transmitted within (and therefore inseparable from) the datastream itself. Therefore, this small piece of intelligence in the analogue sensor removes the need for any manual re-entry of response parameters anywhere along the sensor-digitiser-client chain.
Certis enables users to install in locations with poor horizontal stability (e.g., glaciers, dynamic landslide scarps, water-saturated soils), without the need for cement bases or precise levelling, as the sensor can be deployed at any angle regardless of which model digitiser is connected. Due to its small size, low weight and ultra-low power consumption, Certis significantly reduces logistical efforts and makes short term temporary deployments far easier.
Certis addresses many challenges of traditional seismometer deployments, including cost, but provides a flexible and simple solution for seismic monitoring applications across all disciplines.


SE15-A027
Seismic Velocity Changes Associated with the 2020-2022 Activity of Semeru Volcano as Inferred from Auto-correlations of Ambient Seismic Noise

Yasa SUPARMAN1#+, Ahmad BASUKI1, Heruningtyas Desi PURNAMASARI1, Oktory PRAMBADA1, Devy Kamil SYAHBANA1, Hendra GUNAWAN1, Francois BEAUDUCEL2
1Center for Volcanology and Geological Hazard Mitigation, Indonesia, 2Institut de Physique du Globe de Paris, France

Semeru has been the most active volcano in Java manifested by periods of intermittent explosion and lava effusion occurred at the summit crater. The ongoing eruption that started since April 2014 producing various phenomena e.g. explosions, ash plumes, lava flows, pyroclastic flows, lahars, and dome collapse. The 4 December 2021 eruption was the first monitored explosive eruption of Semeru that produced partial column collapse PDC, which characterised by a more energetic PDC compared to the usual gravitational pyroclastic cone collapse event. This explosive eruption produced 16 km PDC runout and syn-eruptive lahars that destroyed settlements area and public infrastructures along the Besuk Kobokan river channel at the southeastern flank. Here we analyze the autocorrelation of seismic ambient noise at Semeru volcano, observed between September 2020 to December 2022 using the vertical component data of short period seismometer located at the flanks of Semeru Volcano. The Moving-Window Cross-Spectral (MWCS) method was employed to measure seismic velocity variation in the 0.5 – 1 Hz frequency band. This study indicated changes in seismic velocity preceded 2 large PDC events of Semeru, observed concurrently with baseline changes between GPS stations: 1) Decreased in seismic velocity observed from early October to mid November 2020, which proceeded the 1st December 2020 PDC event. 2) continuous decreased in relative velocity variation since June until December 2021, proceeded the 4th December 2021 event. We suggest that seismic velocity changes might reflect the stress changes induced by over pressurization of the magma reservoir due to new magma recharge. 


SE16-A003
Summary of Oct. 8, 2022 Earthquake Swarm in the Tatun Volcano Group, Northern Taiwan

Ya-Chuan LAI1,2#+, Min-Hung SHIH3, Cheng-Horng LIN4, Hsiao-Fen LEE5,6
1Taiwan Volcano Observatory - Tatun, Taiwan, 2National Center for Research on Earthquake Engineering, Taiwan, 3National Applied Research Laboratories, Taiwan, 4Academia Sinica, Taiwan, 5National Center for Research on Earthquake Engineering, National Applied Research Laboratories, Taiwan, 6Taiwan Volcano Observatory at Tatun, Taiwan

The Tatun Volcano Group (TVG) locates in the north part of Taiwan, only 15 km away from the Taipei metropolitan area, may induce strong impact if it active again in the future. The seismicity is one of most important indices of volcano activity, hence a broadband seismic network was installed in the TVG. A series of earthquake swarm with largest magnitude 3.1 occurred in the TVG during Oct. 7 to 9, 2022. An unexpected number of micro-events were detected by the dense seismic array in the Tatun volcanic area. More than a thousand of events occurred, almost equal to the half of the annual average of the background seismicity of the TVG. Such sequences with a lot amount micro-earthquakes only happened twice before in the past decade. One is the 2014 ML 4.2 Shilin earthquake, the biggest one occurred in the TVG recently. The sequence of earthquakes was majorly located in the northern of Mt. Dajianhou, where is the area with obvious variation of seismicity. Most of the earthquakes were clustered in the Mt. Dajianhou and its northern flank with their focal depths less than 5 km. The major felt earthquakes were located at depths around 3-4 km within a significant dip plane composed of the accompanied micro-earthquakes. Such pattern of hypocenter distribution may be related to the local hydrothermal activity process. The importance of hydrothermal system was also demonstrated by the focal mechanisms of major felt earthquakes. The determination of first P-wave motion was predominantly non-double-couple. It’s notable that the geochemical anomalies may be linked to this sequence of swarm.


SE16-A004
Lidar Observations of Eruptive Products of Sakurajima Volcano, Japan

Haruhisa NAKAMICHI#+
Kyoto University, Japan

Two lidar instruments were installed at Sakurajima volcano, Japan at the end of November 2014. These Sakurajima lidar instruments were the first to specifically observe the eruptive products of this volcano in Japan. Sakurajima volcano is one of the most active volcanoes in the world and is in the best location for observing eruptive products. Volcanic ash is the most fine-grain of eruptive products with the particles size of atmospheric aerosols. The lidar instruments can observe such fine volcanic ash. Small eruptions, unreported by the Japan Meteorological Agency, can be detected by the lidar instruments set up at Sakurajima volcano. The small eruptions detected by the lidar instrument were also confirmed by extension meters and seismometers at an underground tunnel in Sakurajima. Large volcanic eruptions are a concern in Sakurajima Island, during which prevailing westerly winds could disperse volcanic ash to the Japanese Islands. Therefore, this ash is expected to be observed using lidar instruments in the Japanese Islands.


SE16-A005
Hazard Assessment and Modeling of Lava Flow Hazard on Tatun Volcano Group, Northern Taiwan

Huai-Yu TANG1+, Sheng-Rong SONG1, Yu-Ming LAI2#
1National Taiwan University, Taiwan, 2National Taiwan Normal University, Taiwan

Lava flows, one of the hazards of volcanoes, can extend tens of kilometers from an erupting vent, destroying everything in their path. To better understand volcanic hazard of lava flow and prepare for emergencies at active volcanoes, lava flow simulations can be useful. The Tatun Volcano Group (TVG) is a Quaternary dominantly andesitic active volcano located near the capital of Taiwan, Taipei City. Two nuclear power plants and a city with a large population (about seven million people live in the vicinity) are located only a few kilometers away from the TVG, any volcanic hazards would be catastrophic for life and cause huge economic losses. In this study, we focus on the lava flows of the TVG and provide two main highlights of our work: (1) Measurements of the length and volume of past lava flow eruptive events as a reference for assessing the eruptive characteristics and physical properties of lava flows in the TVG. (2) To predict the likely extent of future lava flow eruptions by simulating several potential eruptive craters or sites(ex: Mt. Qixing, Mt. Huangzui, Mt. Shamao…etc) within the TVG using the Q-lavHA simulation software. Provide quantitative scientific data for volcanic hazards assessment and emergency preparedness planning.


SE16-A007
Dive Into Volcano Earthquake Swarm Beneath Active Fumarole Area in the Tatun Volcano Group, Northern Taiwan

Min-Hung SHIH1#+, Ya-Chuan LAI2,3, Cheng-Horng LIN4, Hsiao-Fen LEE5,6, Hsin-Chieh PU7
1National Applied Research Laboratories, Taiwan, 2Taiwan Volcano Observatory - Tatun, Taiwan, 3National Center for Research on Earthquake Engineering, Taiwan, 4Academia Sinica, Taiwan, 5National Center for Research on Earthquake Engineering, National Applied Research Laboratories, Taiwan, 6Taiwan Volcano Observatory at Tatun, Taiwan, 7Central Weather Bureau, Taiwan

Qixingshan (aka Qixing Mountain) is the highest volcanic peak in the Tatun Volcano Group in northern Taiwan. In this mountain area, a series of active fumaroles, hot springs, and ancient phreatic eruptions can be found on the surface. Meanwhile, a lot of microseismic events were detected underground. Due to the Qixingshan neighboring the Taipei Metropolitan Area, the monitoring of volcanic activity is an essential topic for local governments and research institutes. To looking more details of the velocity structure in Qixingshan area, we had been deployed a dense seismic array around the mountain, which consists of 60 FairfieldNodal ZLand 3C nodes with a station spacing of 100-200 meters. On April 25, 2022, there was an earthquake swarm occurred in this area, which followed by ~60 smaller earthquakes determined by the real-time broadband seismic network. This sequence is also well recorded by this highly dense array. In this study, we will process the Zland data for the period of this earthquake sequence to detect more micro signals. More details will be discussed in the future.


SE16-A008
A Preliminary Rock Magnetic Results of the Kusatsu-Shirane Volcano, Japan

Nagisa SAWADA1#+, Nobuko KAMETANI2, Kazuo KAWASAKI1, Yasuo ISHIZAKI1, Akihiko TERADA3
1University of Toyama, Japan, 2Yamanashi Prefectural Government, Japan, 3Tokyo Institute of Technology, Japan

The active Kusatsu-Shirane volcano in Gunma, Japan is composed of three pyroclastic cones and has repeatedly produced small phreatic eruptions (JMA, 2013). This study was a test to see if magnetic analyses could estimate the eruption styles and contrast unit boundaries between two outcrops, and thereby, to show that detailed magnetic characterization are useful for active volcanoes that repeatedly erupt on a small scale. The samples used for analyses were 54 and 35 levels of Holocene sediments collected from two natural outcrops, a "hairpin" turn along Route 292 and Sessyogawara geothermal area, respectively. Samples were dried at room temperature for at least 72 hours after collection. Based on the results of room temperature, high and low temperature magnetic analyses, the main magnetic mineral of the sediments is pseudo-single domain titanomagnetite. Further, the high-temperature magnetic analyses showed one or two Curie temperature, suggesting two different Ti content in the titanomagnetites. The results of low-temperature magnetic analyses showed that the magnetite and maghemite are almost negligible. Thus, the observed different magnetic characteristics of the samples are found to be largely effects of their Ti content. The heating curves of temperature dependence of magnetic susceptibility (k-T) is different the ones of strong-direct field thermomagnetic curves and the k-T heating behavior are divided into two obvious trends. These trends could be caused by the different mineralogy such as sulfides and/or iron-oxides and may help to characterize the eruption styles. In addition, the observed different trends of k-T curves appear alternately and repeatedly at both outcrops, suggesting the possibility of contrasting unit boundaries. Therefore, magnetic characterization of sediments by detailed rock magnetism can be an effective method to contrast the outcrops surrounding an active volcano.


SE16-A015
Direct Observation of Dynamic Stress Waves from Turkey Earthquakes of Feb. 2023, Which May Trigger the Japanese Volcanoes Eruption

Yongqian CHEN1,2+, Fuzhen LI1, Tianxiang REN3, Huai ZHANG1, Yaolin SHI1#
1University of Chinese Academy of Sciences, China, 2Shanxi Earthquake Agency, China, 3Chinese Academy of Geological Sciences, China

Two days after the two Ms7.8 earthquakes occurred on February 6, 2023, at 9:17:37 AM and 18:24:50 PM (UTC+8) in Turkey, At around 10:00 AM (UTC+8) on February 8, two successive eruptions occurred at Sakurajima Showa caldera in Japan, which was the first eruption after nearly five years since 2018. Dynamic triggering of volcanic eruptions by great earthquakes has been suggested. However, the lack of direct observations of the dynamic stress waves makes the research on triggering full of uncertainty. For the Turkey earthquakes, we have two(Yingxian and Yuyu) four-component borehole strainmeters right located on the great arc between the Turkish earthquake epicenter and the Sakurajima volcano. The distance of the Japanese volcano from the epicenter in Turkey is 73.84°. Although we have no direct stress record at the volcano, there is a directly observed stress record at the epicenter distance of 56.88° on the great circle, which is only 16.96° away from the volcano, it is helpful to interpret the stress record of the station to understand the dynamic stress condition at the volcano. In this work, different seismic phases such as P-wave, S-wave, and surface waves are identified, their characteristics are analyzed by the stress petal method, the dynamic stress changes caused by each of them are calculated, the largest stress fluctuation occurred when the surface wave arrived, with oscillation period of about the 20s, an amplitude of up to 14kPa. The triggering mechanisms of remote earthquakes on volcanic eruptions are discussed based on the results. The ideas and methods of this work provide useful insight into research on the possible triggering effects of remote earthquakes on volcanoes. 


SE17-A003
Subsurface Imaging of Short-offset Field Seismic Data Using Time- and Depth-processing

Woohyun SON#+, Byoung-Yeop KIM, Dong-Geun YOO, Gwangsoo LEE
Korea Institute of Geoscience and Mineral Resources, Korea, South

In general, seismic processing results depend on the velocity structure. So, a reasonable initial velocity should be used as input data to image accurate subsurface structures in the depth domain. To generate a reasonable initial velocity, various processing techniques were applied in the time domain. For example, to remove noise, data processing techniques such as frequency filter, trace editing, and swell noise attenuation were applied. In addition, various demultiple techniques such as deconvolution, surface-related multiple elimination, and Radon filter were applied to attenuate water-bottom (WB) multiples. By applying these processing techniques, the first and second WB multiples with strong amplitudes were greatly attenuated. A reasonable velocity in the time domain was derived by performing velocity analysis on the data after signal processing with noise and WB multiples attenuated. Then, the tomography-based MVA (migration velocity analysis) method was applied to accurately image the subsurface structures in the depth domain. Depth-processing using MVA is performed as follows. First, the initial velocity for depth processing is derived by converting the velocity generated by time processing into the depth domain. Then, the data after time-processing are sorted into common offset data. We perform Kirchhoff pre-stack depth migration using common offset data. We sort the migrated data into CRP (common reflection point) gather and perform RMO correction. Finally, we update the depth-domain velocity. After the application of MVA, the reflection events are aligned flatter. Through this result, we could confirm that the updated depth-domain velocity is reasonable. Therefore, by applying various time- and depth-processing methods to short-offset (250 m) field data, we could generate reasonable velocity structures. From the final migrated section in the depth domain, we could also confirm that the processing techniques proposed in this study improve the connectivity of the strata.


SE17-A007
Depth Dependency in High-frequency Source Radiation Energy of Small Earthquakes in Japan Estimated from Full Seismogram Envelopes

Masashi OGISO#+
Japan Meteorological Agency, Japan

Structural heterogeneities have been believed to affect little the amplitude of seismic coda waves, especially late coda waves. The Coda normalization method is based on such an assumption and is widely used to estimate site amplification factors and/or source spectra. On the other hand, recent progress in the theory of seismic wave scattering has shown that the excitation of coda waves depends on hypocentral depth, and analyses of coda waves recorded by dense seismic networks have revealed heterogeneous excitation of coda waves, which leads to the violation of the assumption of coda normalization method. Hence, we propose a method to estimate source radiation energy from seismogram envelopes considering heterogeneous seismic structures. In the proposed method, we calculate synthetic envelopes using the Monte Carlo simulation based on the radiative transfer theory and the Born scattering coefficients with a 3-D velocity structure. We conduct a grid search to find appropriate parameters of intrinsic and scattering attenuation that reproduce the shape of each observed envelope, then we calculate source and site amplification terms by an envelope fitting method. We applied the proposed method to small to moderate earthquakes that occurred around central Japan. The range of magnitude was 3.0 to 4.5, and the depth was down to 100 km. Because of the limitation of the Born approximation, we calculated source radiation energy at the frequency ranges of 1-2 and 2-4 Hz. The estimated source radiation energy correlated with magnitude in both frequency ranges. In addition, we found that deeper earthquakes tended to have larger energy than shallower earthquakes. This result may reflect the depth dependency of the physical properties of the earth. Acknowledgments: We used the seismic records of the Hi-net (doi: 10.17598/NIED.0003). This work was partly supported by the JSPS KAKENHI Grant Nos. JP18K13622 and JP21K14002.


SE17-A009
Understanding the Infantile-to-mature Subduction in Southwest Japan Via Self-consistent Formation of a Weak Slab Interface

Changyeol LEE1#+, YoungHee KIM2
1Yonsei University, Korea, South, 2Seoul National University, Korea, South

The weak slab interface controls the long-term subduction dynamics. In particular, a weak hydrous layer at the slab interface promotes slab-mantle decoupling and converts a hot forearc mantle to a cold mantle, often referred to as a cold nose, which plays a key role in the transition from infantile to mature subduction. This study was first to numerically demonstrate the self-consistent formation of a weak hydrous layer with permeability anisotropy, based on the case of the Southwest Japan subduction zone, where the transition-related geological features were present. Our models showed that mechanical decoupling by spontaneous downdip growth of the weak hydrous layer created a cold nose by converting a hot forearc mantle to a cold mantle. This result explained (1) the migration of the forearc-to-arc volcanic front, expressed as the formation of mid-Miocene forearc high-magnesium andesite and Quaternary arc adakite, and (2) present-day geophysical and geochemical observations in the forearc. 


SE17-A011
Discrimination of Explosions and Earthquakes Using Amplitude Ratio of Body-wave

Mikyung CHOI#+, Jayoung YANG, Kyungmin MIN, Jimin LEE, Sun-Cheon PARK
Korea Meteorological Administration, Korea, South

The Korean Meteorological Administration uses various methods to distinguish between earthquakes and explosions. The methods of discriminating explosions from earthquakes are ratio of regional P/S amplitudes and infrasound analysis. We are also trying to develop a method to separate seismic events associated with the collapse of underground cavities from explosions and earthquakes. Recent analysis such as amplitude ratios of body-waves shows separation between three different types of events (Walter et al., 2018).
In this study, we review the method for distinguishing between explosions, collapses and earthquakes using the amplitude ratio of body-wave suggested by Walter et al. (2018). The amplitude ratios of body-waves (Pn, Lg) according to frequency bands are analyzed and compared using the data from regional seismic station on regional earthquakes, the 1st to 6th explosions by the Democratic People’s Republic of Korea (DPRK) and collapse that occurred after the 6th explosion. In addition, the same method is applied to mining collapse in South Korea to distinguish between collapses and earthquakes.


SE17-A014
The Relationship Between Seismic Swarm and Fluid Migration Beneath the Western Foothills of Taiwan

Chia-Nan LAI+, Strong WEN#
National Chung Cheng University, Taiwan

Taiwan is located at the junction of the collision of the Eurasian plate and the Philippine Sea plate, and in the western foothills at the front of the orogenic belt, this provides a good environment for the occurrence of seismic swarms. Swarms tend to occur in areas with high subsurface heterogeneity and fractured structures, and these will triggered by stress variation, high fluid pressure, or aseismic slip. For example, two seismic swarms occurred in Zhushan area in Nov. 2017, which is in the deformation front of orogenic belt. From the analysis, we observed that the velocity structure in this area exhibited significant variation before and after the seismic swarms, and we found that the stress field rotated horizontally at different time period as well. The results we obtained in temporal and spatial distribution are highly consistent with the “seismic clouds” caused by hydraulic fracturing. Hydraulic fracturing is the technique of injecting high-pressure fluids into subsurface rock formations, which can propagate along existing fractures or create new cracks, and these processes can generate many small earthquakes. Since there was no stress disturbance provided by moderate earthquakes during the time period when the seismic swarms occurred, and there was no known aseismic slip zone in this area, through the analysis of this study, it is believed that the seismic swarm that occurred in the western foothills is associated with the fracture zone and related to fluid migration. Since the western coastal plain and the western foothill belt in Taiwan were passive continental rift margins before orogeny, and developed a series of normal faults, most of these fault systems have re-active at the deformation front due to orogeny process. Therefore, using the results obtained in this study, the mechanism of the seismogenic activity in the western foothills of Taiwan can be clarified.


SE17-A020
Tortoises or Hares – Characterizing the Turbidity Currents Observed in the Manila Trench, South China Sea

Meng LIU1+, Zhiwen WANG2, Kaiqi YU1, Jingping XU1#
1Southern University of Science and Technology, China, 2National Marine Environmental Monitoring Center, China

Sediment gravity flows are the most direct and efficient transport mechanisms for moving terrestrial sediments into deep oceans. Scarcity of firsthand measurements, however, has hindered the quantitative, even qualitative characterization of such flows. Here we present a unique year-long data record from ~4000 m depth in the Manila Trench that captured two very different gravity flows in terms of their hydraulic and sedimentary properties. The first flow was of slow speed (~40 cm s-1) and long duration (~150 hours), thus nicknamed ‘Tortoises’, and carried very fine sediment with low concentration (~0.01%). The fast (~150 cm s-1) but short-lived (~40 hours) flow, nicknamed ‘Hares’, carried much coarser sediment with higher concentration (~1.2%). Notably, tidal current in the deep trench modulated the ‘Tortoises’ flow and had likely prolonged its lifespan. Clay mineral compositions suggested that the ‘Tortoises’ originated from upstream canyon wall slumping, whereas the ‘Hares’ was likely submarine canyons Southwest of Taiwan Island due to typhoon. Grain size is a key factor in determining whether a turbidity current evolves into ‘Tortoises’ or ‘Hares’. Finally, the sediment load by turbidity currents accounts for about 17.8% of the yearly average sediment flux of the Gaoping River.


SE17-A029
Forearc Structures in the Manila Subduction Zone and Its Effects on Gas Hydrate BSR Distribution

Elisha Jane MAGLALANG#+, Karla May SAYEN, Leo ARMADA, Carla DIMALANTA
University of the Philippines Diliman, Philippines

Along-strike variations in the forearc character of the Manila Trench control the distribution of gas hydrate BSRs in the area. To the north, BSRs are concentrated in two regions – within the accretionary prism with depths ranging from 285 m to 526 m below the seafloor, and in the western portions of the North Luzon Trough, at depths of 714 m to 812 m. To the south, the BSRs occur within the basin fill of the West Luzon Trough, with an average depth of ~720 m. In the northern segment of the forearc, the accretion of the continent derived sedimentary cover of the subducting crust provides hydrocarbon sources and promotes the formation of thrust faults and gas chimneys, resulting to pervasive fluid migration and forming widespread BSRs within the accretionary prism. In the North Luzon Trough, the sedimentary fill is mostly composed of arc derived turbiditic sequences and mass transport deposits (MTDs) sourced from the collapse of the frontal wedge, possibly due to the oversteepening of slopes or gas hydrate dissociation. Fluid migration along the landward tilted sedimentary sequences of the North Luzon Trough further contributes hydrocarbon-rich fluids needed for gas hydrate formation in the accretionary prism and western parts of the basin. Along the southern segment of the forearc, the incoming South China Sea crust is characterized by a thinner sedimentary cover and bathymetric highs, forming an erosive margin that prevents the accumulation of gas hydrates within the accretionary prism. The BSRs are mainly found within the West Luzon Trough. Fluid migration is facilitated by the normal faults cutting through the basin sediments. Disequilibrium conditions caused by the uplift of the Stewart Bank and by seamount subduction led to the formation of double BSRs in the northern parts of the West Luzon Trough, which reflect changes in gas hydrate stability.


SE17-A030
Forearc Heterogeneity Along Manila Trench Forearc Region: Seamount Subduction or Differential Erosion?

Karla May SAYEN#+, Elisha Jane MAGLALANG, Leo ARMADA, Carla DIMALANTA
University of the Philippines Diliman, Philippines

The complex forearc morphology in offshore western Luzon is attributed to the subduction of the heterogeneous South China Sea basin along the Manila Trench. The Vigan High is one of several bathymetric features in the Manila Trench region. This bathymetric high is a flat-topped feature bounded by submarine canyons. Previous models proposed that it was associated with the forearc uplift due to accreted fragments of the Scarborough Seamount Chain (SSC) (South China Sea extinct spreading ridge) subducted at 16ºN latitude. This preliminary study attempted to map the bathymetric high using new seismic reflection data to understand its geologic characteristics. The seismic reflection data were gathered from the recently concluded LGD-2201 marine scientific cruise and the ORV-041 cruise. Analysis of the seismic reflection profiles indicates faults and fractures bounding the Vigan High. NW-SE trending major faults were identified in the seismic profiles, bounding the Vigan High to the north and south, corresponding to the submarine canyons. The delineated major faults are interpreted as offshore strands of the Philippine Fault Zone (PFZ). Available gravity and magnetic data were also used in this study to complement the seismic reflection data. A combination of the first and second-order horizontal and vertical derivatives indicate NW-SE trending major faults bounding the bathymetric high. The derivative maps support the idea that these faults may correspond to the offshore extension of the PFZ. The gravity and magnetic data show that high gravity and magnetic signature patches characterize the Vigan, and this might suggest that the Vigan High is unrelated to a subducted seamount. Instead, we propose that the present configuration of this bathymetric high is affected by differential erosion across the offshore faults, resulting in the submarine canyons bounding the Vigan High.


SE19-A010
Rupture Model of the 2017 Mw 5.5 Pohang Earthquake, South Korea

Eunbyeol CHO1+, Jeong-Ung WOO2, Junkee RHIE1#, Tae-Seob KANG3, So-Young BAAG1
1Seoul National University, Korea, South, 2Stanford University, United States, 3Pukyong National University, Korea, South

On November 15, 2017, about two months after the last fluid injection was conducted at the enhanced geothermal system development site in Pohang, South Korea, a MW 5.5 earthquake occurred at a distance of about 600 m from the site. It was concluded that the Pohang earthquake was a “runaway earthquake” triggered by the hydraulic stimulation on the critical-state fault. To estimate the spatiotemporal slip history and analyze the characteristics of the rupture process of the Pohang earthquake, which is an uncommon type of earthquake, the finite fault inversion was performed using an empirical Green’s function method. The rupture process can be identified as three phases: first, slip initiated and propagated only to the southwest from the hypocenter during the initial 0.6 s; after then, in the second phase until 2.4 s, the slip propagated to the both southwest and northeast; at last, in the third phase until 6.0 s, slip is diffused around the edge of the fault plane, especially in the deep northeast. The seismic moment was released in each phase as approximately 6%, 59%, and 35%, respectively. The first phase can be interpreted as a separate foreshock, but it is difficult to determine quantitatively whether it is a foreshock. Overall, most of the slip distributed to the southwest well agrees with the rupture directivity result of the apparent source time function analysis. Despite the average stress drop (~1 MPa) of the Pohang earthquake rather lower than that (~20 MPa) of the MW 5.5 Gyeongju earthquake which naturally occurred in a nearby area, it is difficult to conclude that the cause is only the fluid injection. These results improve our comprehension of the source process of the Pohang earthquake and the rupture model can be helpful to understand the complex source process of the triggered earthquake.


SE19-A014
A Preliminary Attempt to Study the Assimilation Analysis of Earthquake Precursor Data Using EMD-LSTM Method

Yibo TIAN1+, Fuqiong HUANG2,1#, Baiyang CHEN1
1Institute of Disaster Prevention, China, 2China Earthquake Networks Center, China Earthquake Administration, China

Assimilation analysis of various observation data is the first step for the development of numerical seismic prediction. EMD-LSTM neural network is an effective method for predicting time series data developed in recent years. The empirical modal decomposition method is used to decompose the original time series data to obtain the IMFs(Intrinsic Mode Functions) signals, and the EMD-LSTM neural network is used to predict the decomposed individual IMF signals, and the final results can be obtained by superimposing the prediction results of each component. EMD-LSTM as a precursor data processing method, a section of actual monitored gravity data is selected for decomposition and prediction, and the relative error between its prediction results and the actual measurement results is The relative error is 0.091%, and in the inverse normalized data, the mean square error is 17976.796, the root mean square error is 134.077, the mean absolute error is 90.871, and the relative error level is 0.091%. EMD-LSTM method provides a new method for predicting time series data, and solves the non-smooth and non-linear prediction problems. The next step is to analyze different types of precursor data in combination with the dilation diffusion model with physical constraints proposed by Scholz, and observe whether the variation of the data in the frequency domain matches the development of the model.


SE19-A015
Preliminary Results of Investigation North-south Trending Blind Fault Associated with November 21, 2022 Cianjur Earthquake from Relocated Mainshock-aftershock Analysis

Aditya RAHMAN1#, Aprilia Nur VITA1+, Retno Agung PRASETYO KAMBALI1, Asep NURACHMAN1, Rahmat Setyo YULIATMOKO1, Abraham ARIMUKO1, Ade Andika SAPUTRA1, Nova HERYANDOKO2, Supriyanto ROHADI1, Suko Prayitno ADI1, Dwikorita KARNAWATI1
1Indonesian Agency for Meteorology, Climatology and Geophysics, Indonesia, 2Institute of Technology Bandung, Indonesia

At 13:21 local time on November 21, 2022, a magnitude-5.6 inland earthquake occurred in Cianjur-West Java Indonesia region, resulting at least 602 deaths and damage to 58 thousands houses. We deployed 6 temporary seismic stations soon after the mainshock around aftershocks region. We carried out preliminary auto-detection of seismic events using Lassie and detected 770 aftershocks events in the two-weeks dataset. The preliminary detection result then located using SeiscomP and we relocated the hypocenter of the mainshock and aftershock from temporary station using Hypo-DD. Our relocated mainshock-aftershock show that the earthquake sequence ruptured on hidden and unmapped fault within Cianjur Area. The distribution of seismicity reveals a previously unknown North-South trending fault (N350E) which in this study we proposed as Cugenang Fault in the northern of known Cimandiri fault. The newly identified fault calls for further investigation for future seismic hazard assessments in the region.


SE19-A016
The Application of Optical Fiber Clinometer to Solid Tide Measure

Wentao ZHANG#+, Wenzhu HUANG, Minggan LOU
Chinese Academy of Sciences, China

Solid tide is the only geophysical phenomenon that can be calculated theoretically. Therefore, solid tides measurement would have significant application prospects in geodynamics, earthquake prediction, etc. However, the solid tide phenomenon is very weak, and high performance of the instrument is required. Previously, we had observed earthquakes and solid tides using optical fiber sensors. In this paper, an optical fiber clinometer based on fiber optic Michelson interferometer was proposed and crustal deformation was measured and analyzed. The optical fiber clinometer was a Michelson fiber interferometer with an arm length difference of 0.4 m. The clinometer received signals based on the pendulum's vertical principle. The Michelson interferometer adopted Faraday rotator mirrors was able to eliminate polarization fading. A high-precision fiber-optic general signal demodulation device with resolution better than 0.0001 rad/√Hz from 0.01 Hz to 50 Hz was used. The optical fiber clinometer was installed in the borehole. The sampling rate of the system was set to 10 Hz. After the clinometer was stabilized, the phase change has good consistency with temperature change measured by a platinum resistance temperature sensor on a long-time scale, and the correlation coefficient was 0.964. Solid tide signal was covered by temperature. But solid tide waveform was recorded when the temperature change was gentle. The recorded phase waveform was basically consistent with the theoretical solid tide. Additionally, the power spectral density (PSD) showed a peak at 0.000023 Hz, which corresponded to a main period of solid tide. Therefore, although the fiber optic clinometer was affected by temperature, it had the potential to record solid tide. We believe that if several methods such as reference temperature compensation are used, better results of solid tide can be obtained.


SE19-A017
Analysis and Statistical Validation of Global Ionospheric Perturbation Using Arima as Seismogenic Precursory Signature for Western Nepal Earthquake on 8th Nov 2022

Bijoy DUTTA#+, Javed MALIK
Indian Institute of Technology Kanpur, India

Global navigation satellite systems (GNSS) derived Total Electron Content (TEC) data are being used extensively for analyzing ionospheric perturbations to detect earthquake precursory signals. In this paper we have reported prominent evidences for pre-seismic ionospheric anomalies along with its statistical validation using ARIMA over the epicentral region for a devastating earthquake in western Nepal on 8th November 2022 (Mw 5.7) and its several aftershocks (Mw 5.4, 4.2) in and around Uttarakhand. Temporal variation of TEC of the nearest grid point to the epicentre was analyzed based on median, upper and lower bounds (defined by standard deviation) for a time span of a month prior to the quake. After ruling out all possible contributions from solar terrestrial environment, anomalous (-ve) behaviour of TEC (~12 units) is observed 3-22 days prior to the earthquake. In order to visualize the TEC anomaly in spatio-temporal domain, we have plotted 2D latitude-longitude time (LLT) maps considering the nearest plate boundary and Global Ionospheric Map (GIM). Using these we have determined the probable epicenter which showed very promising correlation in comparison to actual epicenter; the offset is found to be ~85 km and 125 km respectively. In order to validate this anomaly as seismogenic origin we have also used a statistical model ARIMA. After choosing proper ARIMA model from ACF and PACF we have forecasted the data for those anomalous days. After optimizing hyper parameters and training the model, a significant number of –ve anomalies have been observed on those anomalous days. The forecasted data gives a promising accuracy in trend with the GNSS derived data. This model has an adequate potential to forecast ionospheric TEC and to detect anomalous behaviour with considerable accuracy prior to any disastrous quake. This will provide some new beneficial insight to study seismo ionospheric coupling from new aspect.


SE19-A020
Slip Rate and Locking Status of the Xianshuihe Fault Inferred from Dense Geodetic Observations

Faqi DIAO#+, Yage ZHU, Xiong XIONG
China University of Geosciences, China

The Xianshuihe-Xiaojiang fault (XXF) that lies in the southwest of China, is one of the largest left-lateral faults surrounding the Tibetan Plateau. The northern segment of the XXF is called Xianshuihe fault, which is a well-known seismogenic fault due to the high frequency of strong earthquakes. Therefore, the present seismic risk of this fault has aroused wide concern. The slip rate and locking status of seismogenic faults are crucial for seismogenic mechanisms and regional seismic hazard assessments. Presently, elastic models have been routinely used in probing the fault slip rate and locking status with geodetic observations. However, recent studies revealed that elastic models could highly affect the fault parameter estimate, while models incorporating viscoelastic effect of substrate ductile layers can yield reliable results. Here we construct viscoelastic deformation models based on dense GPS velocities near the Xianshuihe fault to invert for the slip rate and locking status of the fault. Our results suggest that elastic models will highly overestimate the fault locking depth, and thus seismic moment accumulation rate. Besides, the block division strategy also plays an important role on resulted fault slip rate and locking distribution. Based on the inverted fault locking distribution, we identify four potential asperities along the Xianshuihe fault, which show clear spatial correlation with the historical ruptures. This result suggests that the fault locking status may control the rupture extent of strong earthquakes on this fault, which has important implications on future seismic hazard assessment. Moreover, the 2022 M 6.8 Luding earthquake was found only ruptured a part of an identified asperity, while the seismic moment accumulated on the unruptured segment is corresponding to an Mw 6.8 earthquake, highlighting that the potential seismic risk there should be carefully monitored.


SE19-A029
Rupture Press of Large Earthquake Based on Seismic Signals Recorded by Gravimeter

Hongbo TAN#+
Institute of Seismology,China Earthquake Administration, China

Gravimeters can provide 1Hz sampling data, including a large number of complete seismic wave records. Frequency spectrum analysis have been done after analyzing the data of Lushan Ms7.0 earthquake in 2013 recorded by gravimeters and seismometers in the same stations. The rupture process of Luding Ms6.8 earthquake in 2022 have been inversed and the following preliminary understanding can be obtained. 1) The relationship between P-wave travel time and epicentral distance recorded by gPhone and STS-1 are consistent well. 2) The dominant frequency spectrum of the P wave is quite similar, mainly concentrated in the range of 0.05 to 0.3 Hz. With the increase in the epicenter distance, the consistency between the two is better. The power spectrum image shows that the main energy of the seismic wave is concentrated between 0-0.5 Hz. 3) Based on the 1Hz gravity data, the rupture model of the Luding Ms6.8 earthquake in 2022 is inversed. The results show that the fault strike direction is 163° and the dip Angle is 77°. The rupture area is about 42 km along the strike direction and 6-27km in the dip. The main rupture zone is near the epicenter, with a maximum slip of 1.05m. The average slip angle of the fault is 9.8°. The seismic moment of the earthquake is 1.33×1019 N∙m, corresponding to a magnitude of Mw6.7. The picture of the source time function shows that the earthquake has two major sub-events: the first peak of moment release rate reach to 1.50×1018 N∙m/s at 5s; the second peak reach to 6.74×1017 N∙m/s. at 14s. The whole rupture time is about 22s. These results are basically consistent with the results of other seismograph inversion and can have reflected the main process of this earthquake rupture.


SE19-A031
The Significance of Seismic Signal Recorded by Gravimeter

Hongbo TAN#+
Institute of Seismology,China Earthquake Administration, China

The records of continuous gravimeters contain seismic wave signals that were conventionally removed as noise in the past for tidal processing analysis. However, with the Crustal Movement Observation Network of China, 80 digital stations have been formed, in which more than 60 sets of gPhone and GWR gravimeters can provide 1Hz sampling data, including a large number of complete seismic wave records. Whether these seismic data can become a new source for the study of the focal mechanism has been plaguing earthquake scientists. Whether it can be effectively unified is a good topic worthy to be analyzed. In this study, the frequency spectrum analysis and the rupture process inversion have been done after analyzing the data of Lushan Ms7.0 earthquake recorded by gravimeters and seismometers in the same stations, and the following preliminary understanding can be obtained. 1) The relationship between P-wave travel time and epicentral distance recorded by gPhone and STS-1 are consistent well. But the differences in amplitude are larger while the epicentral distance become smaller. 2) The waveforms of the seismic waves recorded by the two instruments are basically the same. The dominant frequency spectrum of the P wave is quite similar, mainly concentrated in the range of 0.05 to 0.3 Hz. With the increase in the epicenter distance, the consistency between the two is better. The power spectrum image shows that the main energy of the seismic wave is concentrated between 0-0.5 Hz. The gPhone gravimeter can record the main signal energy. The seismic waves recorded by the gravimeter can be used in the study of the earthquake rupture mechanism and it is an important supplement to the seismograph records.


Wed-02 Aug | 10:20 - 12:20 | MR306
SE19 - Faults and Earthquakes: Networks, Precursors and Monitoring Systems

Session Chair(s): Tao CHEN, Chinese Academy of Sciences

SE19-A019 | Invited
Distributed Fiber-optic Monitoring of the Frequently-slip Milun Fault Zone in Eastern Taiwan: The MiDAS Project

Hsin-Hua HUANG1#+, Kuo-Fong MA1,2, En-Shih WU3, Yun-Ze CHENG1, Chin-Jen LIN1, Chin-Shang KU1
1Academia Sinica, 2National Central University, 3National Taiwan University

Seismic or aseismic slips on a fault are highly controlled by fault zone structures and properties in space and time. However, the buried subsurface locations or strongly weathered outcrops of active faults often hinder high-resolution in-situ observations to study. The frequently-slip Milun fault that ruptured during the 1951 and 2018 Hualien earthquakes in eastern Taiwan, with a relatively well-known geometry, offers a rare venue to probe the active fault zone with an emerging technique of distributed acoustic sensing (DAS). The DAS exploits the interaction of photons with intrinsic defects of fiber to translate the phase shift of scattering echos into longitudinal dynamic strain every few meters along the fiber, rendering continuous and high-resolution monitoring across the fault zone. Launched in late 2021, the Milun Fault Drilling and All-inclusive Sensing project (MiDAS) drilled two holes in the hanging wall (Hole A) and footwall (Hole B) of the Milun fault and met the fault zone at ~500 meters of Hole A. Deployment of a 3-D fiber array including two downhole fiber segments and surface segments that connect the two was sequentially completed in late 2022. With this valuable DAS dataset, we clearly identify a 20-meter-thick major fault zone, which coincide with the retrieved cores, and several hidden faults along the depth thanks to special properties of the strain data in contrast to typical velocity/acceleration data of seismometers. The unique 3-D geometry of the MiDAS fiber array also permits us to investigate and visualize the spatiotemporal variations of ground (strain) motions in response to anthropogenic and environmental sources of the region in great detail.


SE19-A021 | Invited
Predicting the Seismicity Monitoring Capability of the Planned Seismic Network in Chinese Mainland

Jiawei LI#+
Southern University of Science and Technology

The China Earthquake Administration (CEA) has currently launched an ambitious nationwide seismic network project, which will increase the number of stations from approximately 2,000 to 15,000 in total, from 950 to 2000 for the broadband seismic stations used to compile earthquake catalog. The new network is planned to go online by the end of 2023. More than half of Chinese mainland, the inter-station distance of the planned broadband seismic network will soon be smaller than 100 km, 27% be 50 km, and 6% be 25 km. Of all possible ways to characterize the higher-resolution monitoring of the frequent smaller earthquakes expected inside Chinese mainland, the completeness magnitude (Mc) remains one of the most commonly used. Using the prior model of the Bayesian Magnitude of Completeness (BMC) method calibrated on the Chinese earthquake catalog from January 1, 2009 to June 26, 2022, we predict the spatial distribution of Mc for the new network based on the planned network configuration. If almost the entire Chinese mainland is at present covered down to Mc = 3.3, this threshold will fall to Mc = 2.9 in the near future. This means approximately 2 times more earthquakes will be recorded in the complete catalog available for statistical analysis per year (for a = 6.82 and b = 0.80 in the Gutenberg-Richter law log10N = a - b·Mc). Based on the observation that abnormal seismicity as precursors are most likely to be observed at least at 3 units below the mainshock magnitude, and assuming earthquakes to be potentially damaging at M ≥ 5, the new seismic network shall achieve the goal of 76% coverage for optimal seismic-based earthquake prediction research.


SE19-A002 | Invited
SWRI : Sustainable Water Resources Infrastructure: Concept & Application : A Research Study

Mukesh VERMA1,2+, Narayan Prasad DEWANGAN3,1#
1Chhattisgarh Swami Vivekanand Technical University, 2National Institute of Technology, 3Chhattisgarh Government

The demand for water has enormously increased with the rapid growth of modern civilization. Mankind is witnessing a crisis of water and its requirement is constantly increasing with the development of civilization. These crises can be effectively mitigated by the integrated development and utilization of available water resources. Conceptual, visionary and technological viable planning for attaining Sustaining Water Resources Infrastructure (SWRI) is the focal point of this research. The Components of the system are reservoirs, canal networks and, recharging zones. Surface water can be stored in the reservoirs and, identifying recharging zones augmented through the system of recharging canal networks thereby developing a system that constantly augmenting the groundwater and creating a ground water sustainability condition which can be termed as SWRI. The planning approach for the SWRI consists of the development of a network of storage reservoirs involving the preparation of water potential map and identification of the surface storage works in a systematic manner. The possibility of inter-basin water transfer should also be explored and incorporated which will help in efficient diversion of the surface surplus water to the drought prone areas. The development of ground water zones can be ascertained which involves the preparation of the drainage map of a river basin for a complete and commendable analysis of drainage and serves as a basis for the design of the networks of efficient ground recharging zones. The adaptation and implementation of this holistic approach will definitely prove to be very powerful tool for the developing a sustainable infrastructure of the available water resources.


SE19-A006
Unconventional Seismic Hazard Assessment by Geochemical Methods

Giovanni MARTINELLI1#+, Gianluca FACCA2, Fabrizio GHERARDI2, Lisa PIEROTTI2
1National Institute of Geophysics and Volcanology, 2National Research Council of Italy

Studies on the occurrence of geofluids in faulted areas may provide useful information about the local stress-strain fields and their evolution over time. The occurrence of warm spring waters, the degassing of CO2, CH4, noble gases, and, among them, Helium originated in the crust under various conditions results in the release of volatiles from rocks and their transfer to the surface. The permeability of the host geological formations is sensitive to changes in geophysical parameters, and geofluids may help to define a more effective description of areas previously considered by Probabilistic Seismic Hazard Assessment and by Neo-Deterministic Seismic Hazard Assessment approaches (Zhang et al., 2021). Due to the occurrence of geothermal resources being present in highly deformable crustal segments, geochemical and isotopic characteristics were examined in local geofluids, allowing comprehensive geochemical characterization of detected locations. Several authors discovered relationships between 3 He/ 4 He levels and stain rates. Crustal permeability anisotropies caused by tectonic activity can have an impact on geochemical parameters. Crustal permeability anisotropies exhibited by the presence of geofluids such as thermal springs and, finally, anomalous Helium isotopic characteristics may be used as a signal of large forecasted seismic occurrences in Seismic Hazard Assessment operations. Thermal springs mapping has evidenced areas affected by strong tectonic activity.  In general, all places where considerable tectonic activity is overlaid on thermal spring areas should continue to host seismic events that mirror the Gutenberg-Richter features of a considered earthquake catalogue (e.g. Storchak et al. 2013). Outside of recognised seismically active places, anomalous geofluid sites releasing large mantle-derived components have been also found. Thus, mantle-derived geofluids could be emitted in concomitance with strong seismic events (M>6) that maintained relatively high crustal permeability values over geological time, despite the lack of significant earthquakes in catalogues, volcanic vents and heat flux anomalous values.


SE19-A009
The Hour Scale Precursor Characteristics of the Atmospheric Electric Field Negative Abnormality

Tao CHEN#+
Chinese Academy of Sciences

By global inner continent earthquake case study, the hour-scale precursor characteristics of inland earthquakes (EQs) are revealed. Several Chinese EQ cases have been mainly reported. As indicated by a table listing 23 inland EQs with their shock time, epicentral location, magnitude, near-epicenter weather conditions, precursor beginning time, and precursor duration, the weather conditions are fair near the epicenter, and an anomalously negative atmospheric electrostatic signal is readily observed approximately 2-48 hours before an inland EQ occurs. Moreover, a successful single station alarm for the nearby middle class and the possible mechanism is stated. The EQ process changes the electrostatic field is explained as the release of radioactive gases from the subsurface into the atmosphere via large (regional)-scale pre-existing microfractures in the rock at the source depth. These gases considerably ionize the atmosphere, and the separated positive and negative ions establish a special macroscopic electric field. Finally, a critical stage of 2-48 hours may be regard as a stable tectonic process before EQs.


SE19-A012
Physical Process of Anomalously Negative Atmospheric Electric Field

Lei LI#+
National Space Science Center

Long-term observational studies of atmospheric electric fields have been executed since the 1980s by different research teams using atmospheric electric field meter in Sichuan, Yunnan, Beijing, Hebei, etc. Recent research show an anomalously negative atmospheric electrostatic signal is readily observed approximately several hours to one day before an inland earthquake occurs. In this abstract, hourly scale physical mechanism about anomalously atmospheric electric field will be briefly described. Before an earthquake, underground radioactive gases (such as CO2, helium, radon, and water vapor) from the hypocentral depth are released into the atmosphere, which enhances the output of thermal radiation and undergo decay and emit α particles, which may further ionize the local atmosphere within minutes. Then many positively and negatively charged particles are injected close to the surface near the epicenter, and they in turn changes the normal atmospheric electric field.


SE19-A013
The Progress of Short-term Predictability of Strong Earthquakes in China Mainland Within Recent 10 Years: A Review

Fuqiong HUANG1,2#+, Jie LIU3, Jian XUE4, Haoyu SHI5, Nianjie MA6, Tao CHEN4, Yibo TIAN2, Baiyang CHEN2
1China Earthquake Networks Center, China Earthquake Administration, 2Institute of Disaster Prevention, 3Sun Yat-sen University, 4Chinese Academy of Sciences, 5North China Institute of Science and Technology, 6China University of Mining and Technology

Short-term predictability has been hot topic again after recent double strong earthquakes occurred on Feb 6, 2023, in Turkey. This topic has long been discussed after 2008 Wenchuan great earthquake in Sichuan China Mainland. Many scientists contributed efforts to retrospectively confirm the precursors and the predictability of strong earthquakes in short-term before events from multidisciplinary approaches. This article tries to review the progress within recent 10 years which have made in China Mainland. Through improving the sampling techniques of experiment in laboratory, scientists of tectonophysics successfully captured the process of meta-instability stage before failure occurrence and give the time division related to the whole process. Theoretically, using the time division in laboratory to reality, considering the interval between two events as 300 years, the meta-instable stage I should occupy one year to half one year and the meta-instable stage II should occupy 3 months to days. The characteristics of strain and temperature which are measured in laboratory accelerate in above periods. This time division result fit for the routine operation of short-term earthquake prediction practice in China Mainland. To extract the accelerating process from observation data is the main task to search the precursor aiming at short-term prediction. At the same time, scientists of rock mechanics also find the acceleration precursor of catastrophic in rock-like materials which can be well described by power law relationship. The variation of reduced exponent can be used to predict the catastrophic rupture. Through CT techniques, rock physicist playback the deformation process of rock under 3-axial pressurized condition and statistically analyze the parameters changing with time. The results show that all the parameters accelerate near failure occurrence. While with satellite observation techniques, scientists find hourly scale precursors of inland earthquakes and tested global cases. At this stage triggering plays key role of earthquake occurrence.


Wed-02 Aug | 10:20 - 12:20 | MR308
SE09 - In and Around the Tibetan Plateau: the Deep Structure, Geodynamics, Geohazards and Georesources

Session Chair(s): Yangfan DENG, Guangzhou Institute of Geochemistry, Chinese Academy of Sciences, Liang CHUNTAO, Chengdu University of Technology

SE09-A002
Northward Growth of the West Kunlun Mountains

Dongliang LIU1#+, Haibing LI2, Yadong WANG3, Jiawei PAN4, Yong ZHENG4, Marie-Luce CHEVALIER1
1Institute of Geology, Chinese Academy of Geological Sciences, 2Chinese Academy of Geological Sciences, Institute of Geology, 3China Academy of Sciences, 4Chinese Academy of Geological Sciences

The Cenozoic collision between India and Asia promoted the widespread uplift of the Tibetan Plateau, with significant deformation documented in the Pamir Plateau and West Kunlun Mountains. Low-temperature thermochronology and basin provenance analysis have revealed three episodes of rapid deformation and uplift in the Pamir–West Kunlun Mountains during the Cenozoic. However, there is very little low-temperature thermochronology age–elevation relationship (AER) data on fast exhumation events in this area – especially in the West Kunlun Mountains – leading to uncertainty surrounding how these events propagated within and around the mountain range. In this study, we produced an elevation profile across granite located south of Kudi, Xijiang Province, China, to reveal its exhumation history. Apatite fission track AER data show that a rapid exhumation event occurred at ~26 Ma in the southern West Kunlun Mountains. When combined with published data, we interpret that the initial uplift events related to the India–Asia collision began in the central Pamir, southern West Kunlun, and northern West Kunlun regions during the Late Eocene, Oligocene, and Middle Miocene periods, respectively. Therefore, the Cenozoic northward growth process occurred from south to north around West Kunlun.


SE09-A009
A Comparative Study of Seismic Tomography Models of Southwest China

Xuezhen ZHANG+, Xiaodong SONG#, Feiyi WANG
Peking University

The margin of the Tibetan Plateau of southwest China is one of the most seismically active regions of China and is the location of the China Seismic Experimental Site (CSES). Many studies have developed seismic velocity models of southwest China, but few have compared and evaluated these models which is important for further model improvement. Thus, we compared six published seismic shear-wave velocity models of southwest China on absolute velocity and velocity perturbation patterns. The models are derived from different types of data (e.g., surface waves from ambient noise and earthquakes, body-wave travel times, receiver functions) and inversion methods. We interpolated the models into a uniform horizontal grid (0.5° × 0.5°) and vertically sampled them at 5, 10, 20, 30, 40, and 60 km depths. We found significant differences between the six models. Then, we selected three of them that showed greater consistency for further comparison. Our further comparisons revealed systematic biases between models in absolute velocity that may be related to different data types. The perturbation pattern of the model is especially divergent in the shallow part, but more consistent in the deep part. We conducted synthetic and inversion tests to explore possible causes and our results imply that systematic differences between the data, differences in methods, and other factors may directly affect the model. Therefore, the Southwest China velocity model still has considerable room for improvement, and the impact of inconsistency between different data types on the model needs further research. Finally, we proposed a new reference shear-wave velocity model of southwest China (SwCM-S1.0) based on the three selected models with high consistency. We believe that this model is a better representation of more robust features of the models that are based on different data sets.


SE09-A016
Crustal Structure and Deformation of East Haiyuan Arcuate Tectonic Region in the Northeastern Tibetan Plateau

Yanqi LIN#+
Sun Yat-sen University

The Haiyuan arcuate tectonic region is located in the northeastern margin of the Tibetan Plateau, it is the transition zone between Tibetan Plateau, Alxa block and Ordos block. The Cenozoic tectonic deformation in the study area is a response to the collision between the Indian plate and the Eurasian plate. The tectonic zone consists of a series of oblique left-lateral thrust faults, which are Haiyuan-Liupanshan fault zone, Xiangshan-Tianjingshan fault zone, Yantongshan fault zone and Niushoushan- Luoshan fault zone from south to north. The Haiyuan arcuate tectonic region is the edge of the outward expansion of the Tibetan Plateau, which is a desired place to study the frontier scientific issues such as the crustal material escape and the interaction between blocks. A lot of researches have been carried out in this area, but the deep structure of each tectonic unit is still not well understood. In order to image the fine crustal structure, a short-period dense nodal array was run off roughly in the northeast-southwest direction, crossing the Haiyuan arcuate tectonic region. The teleseismic waveforms used in this study were recorded by 299 nodal geophones with a spacing of 1 km. P-wave receiver function was used to capture the fine structure of deep crust in the studied area. The CCP stacking and forward modeling was used to analyze and interpret the receiver functions. The results show that the Niushoushan-Luoshan fault zone is the latest boundary of the northeastern Tibetan Plateau. The crust was thickened significantly, especially the lower crust. The thickening mode was pure shear caused by the crustal shortening, and there is no partial melting in the crust.


SE09-A018
A Generalized Strategy from S-wave Receiver Functions Reveals Distinct Lateral Variations of Lithospheric Thickness in Southeastern Tibet

Zhou ZHANG1+, Yangfan DENG2#
1Chinese Academy of Sciences, 2Guangzhou Institute of Geochemistry, Chinese Academy of Sciences

The selected rotation angle and deconvolution time window during S-wave receiver function (SRF) calculations, and the final SRF quality control may introduce artificial interference. Here we overcome these problems by proposing a new strategy named GC_SRF for obtaining the lithospheric thickness from S-wave receiver functions, which employs grid search and correlation analysis to obtain reliable SRFs. Extensive tests using synthetic and real data suggest that the GC_SRF strategy is a robust and reproducible approach for estimating lithospheric thickness. Specifically, this GC_SRF strategy can restore the weak Sp phases from full wavefield synthetic seismograms. Clear and distinct discontinuity patterns that do not involve artificial interference compared with those obtained in previous studies of southeastern Tibet are produced here. The post-stack migrated SRFs reveal distinct lateral variations of lithospheric thickness in southeastern Tibet: (a) Tengchong volcano has a thin crust and thin lithosphere–asthenosphere boundary (LAB) (∼90 km); (b) the Chuandian region has a thicker crust and either a poorly defined or unclear LAB. The absence of a continuous LAB in the Chuandian region may suggest lithospheric regrowth due to the recovery processes of the mantle plume; (c) a thinner crust and clear LAB of ∼160 km depth are presented beneath the Sichuan Basin.


SE09-A022
Crustal Structure of the Western Haiyuan Arcuate Tectonic Belt and Implications for Outward Growth of the NE Tibetan Plateau

Zizhao YUAN#+
Sun Yat-sen University

The northeastern Tibetan Plateau marks the northeastern margin of the Tibetan plateau. With the onset of the Neotectonics during Cenozoic, the Tibetan Plateau is undergoing plateau-wide extrusion toward the northeast and resulted in the generation of the Haiyuan Arcuate tectonic belt that protrudes to the NE. Therefore, it has been an ideal place to study the tectonic expansion of the Tibetan Plateau owing to its typical tectonic location. In this paper, we deployed a 200km-long short-period seismic array across the Longzhong Basin, Haiyuan Arcuate Tectonic Belt and the Hexi corridor transition zone. To ensure the basal composition, we used the common conversion point stacking method (CCP) and calculated the wave velocity ratio. Combined previous studies in petrology and geophysics in the study area, the results show that the Haiyuan Arcuate Tectonic Belt is weak in mechanical strength and prone to deformation. It is attributed to a tectonic accretionary wedge that might have been produced during amalgamation between the Alax and the Qilian orogen during Early Paleozoic. The tectonic features determine the Haiyuan Arcuate belt is sensitive to the compression from the NE escape of the Tibetan Plateau, which resulted in the arcuate shape of the belt that protrudes to the northeast. Moreover, the obtained crustal-scale architecture outlines a lower-crustal shortening and upper crustal-expansion in a way of stepwise thrusting toward the northeast. This scenario is similar to the deformation across the Liupanshan fold-thrust belt and both show that the Tibetan Plateau is undergoing northeastward expansion in a pattern of lower-crustal shortening but upper crustal thrusting above a detachment shear zone to a shallower depth. The whole process has involved adjacent tectonic units into growth of the Tibetan Plateau.


SE09-A024
Geodynamics of the Southeastern Tibetan Plateau from 3D Anisotropy Structure and Velocity Model

Feihuang CAO+, Liang CHUNTAO#
Chengdu University of Technology

With the deformation pattern of the southeastern Tibetan Plateau remaining controversial, its anisotropic structure and the three-dimensional (3D) velocity model are powerful parameters for understanding this issue. In this work, we applied an azimuth dependent joint inversion method (Cao et al., 2022) to the ChinArray (ChinArray, 2006) for the high-resolution 3D anisotropy structure and velocity model on the eastern Tibetan Plateau. In our model, the vertically consistent fast propagation direction in the Songpan-Ganzi block (SGB) and the north Chuandian block (NCDB) suggested that the deformation in this region is largely coupled vertically. Our model provides anisotropic evidence of the Yangtze crystalline basement extending to the SGB. The low-velocity zone (LVZ) was much thicker and more prominent in the NCDB than in the SGD. Anisotropy in the middle lower crust of the NCDB does not show any sign of an LVZ flowing from the SGB or the Qiangtang block to the NCDB. These observations are contrary to those of the crust flow model, suggesting that the LVZ was generated locally. The mushroom-shaped high-velocity structure beneath the southern Chuandian block and boundary fault zone may be a relic of the Emeishan paleo-mantle plume. Reference Cao, F. et al. (2022) ‘3D velocity and anisotropy of the southeastern Tibetan plateau extracted by joint inversion of wave gradiometry, ambient noise, and receiver function’, Tectonophysics, 848, p. 229690. doi: https://doi.org/10.1016/j.tecto.2022.229690. ChinArray, 2006. China Seismic Array waveform data. China Earthquake Administration. https://doi.org/10.12001/ChinArray.Data.


SE09-A035
The Crustal Structures of the East Kunlun Fault and Its Adjoining Faults Revealed by Receiver Functions

Xiaofei TONG#+, Xiao XU
Sun Yat-sen University

Previous studies have suggested that the Tibetan Plateau has undergone eastward-extrusion since the Miocene, and the sinistral strike-slip of the eastern Kunlun fault zone is strong evidence for this. To gain a better understanding of the deformation, transfer, and transport of material in the Plateau, it is crucial to correctly identify the structure and location of faults. Geodetic and geomorphic research have pointed to a diminishing slip rate of the fault eastward, particularly in the Roergai basin, which is covered by a variety of Quaternary sediments. However, due to the basin's alpine herbaceous swamp nature, it is difficult to trace faults on the surface. To overcome this, a dense array of 110 seismic stations with an interval of around 1 km, as well as 6 broadband stations, were used to investigate the crustal scale identification of the East Kunlun fault in the Ruoergai Basin in this study. By comparing the discontinuities of the strata in the crust and the depth variation of the Moho, it was determined that the East Kunlun fault continues to extend eastwards through the Ruoergai Basin. Additionally, the similarities in crustal structure between the Tazang fault and East Kunlun fault were used to judge their inheritance relationship. The results of this study provide high-resolution evidence for the outward growth of the Plateau.


SE09-A021 | Invited
The Wave Gradiometry Method and Its Applications to Obtain 3D Velocity, Anisotropy, Attenuation of the Crust and Uppermost Mantle

Liang CHUNTAO#+, Feihuang CAO
Chengdu University of Technology

The Wave Gradiometry Method(WGM) has emerged as a powerful multipurpose tool to extract strain and rotation tensor, identify phases, and most importantly to image the near surface or deep structure. The WGM measures the spatial gradients of the wavefield within a subarray to extract 4 major attributes: phase velocity, wave directionality, geometrical spreading and radiation pattern. These attributes can be further used to extract strain and rotation tensor and structural information. An azimuth-dependent dispersion curve inversion (ADDCI, https://doi.org/10.1029/2019TC005747) is applied together with the WGM method to extract both 3D shear wave velocity and 3D azimuthal anisotropy. Additionally, the geometrical spreading extracted by the WGM is used to find the attenuation of the materials. In this study, we review the theoretical foundation, technical development, major applications of the WGM and compare the WGM with other major array-based imaging method. Similar with the Ambient Noise tomography, the WGM is also boiled down to dispersion curve inversion. Even though it can be applied to arrays with a wide range of scales, here we concentrate on the applications to large scale arrays such as the USARRAY (average spacing of 70km), CHINARRAY (average spacing of 40km). It may also be applied to any other dense regional array, such as the ALPARRAY and others. The imaging depth is only limited by the corner frequency of the seismometer. We will compare our results with that from other techniques to highlight its advantage and disadvantages (Cao et al. 2022). References: Cao F H, Liang C T. 2022, 3D velocity and anisotropy of the southeastern Tibetan plateau extracted by joint inversion of wave gradiometry, ambient noise, and receiver function, Tectonophysics, https://doi.org/10.1016/j.tecto.2022.229690.


Wed-02 Aug | 1:10 - 3:10 | MR306
SE19 - Faults and Earthquakes: Networks, Precursors and Monitoring Systems

Session Chair(s): Gang LUO, Wuhan University, Dimas SIANIPAR, State College of Meteorology, Climatology, and Geophysics, Giovanni MARTINELLI, National Institute of Geophysics and Volcanology

SE19-A003
Psycho-social Framework for Post- Disaster Management -Indian Perspective on Global Scenario

Pratibha DEWANGAN1+, Pranay DEWANGAN2#
1Government College of Teachers Education, 2GAIL India Limited

The visible and measurable part of every disaster are deaths, injuries and destruction but the invisible and immeasurable part remains the mental health, agony and trauma of the survivors suffering from losses of persons, properties and livelihood, which often escapes notice of the decision makers. Such invisible effects and rehabilitation are of utmost importance otherwise causing prolonged agonies. This recognition and importance of psychosocial counselling immediately after the disaster has encouraged innovative research and practices on community-based approaches which can be imparted in a scientific and systematic manner with concept, methods and techniques of the training. The National Institute of Disaster Management, an apex body in India, has created an Act of Parliament for training, capacity building, research and documentation on disaster management and introduces a ToT module which provide general and specific guidelines as well to carry out the training programme without much external assistance. The valuable feedbacks from the participants, community workers and the affected communities itself have provided relevance and this ToT module and can be applied as a model for other developing and under-developed nations with their psychosocial and natural conditions.


SE19-A001
TSK Fuzzy Model for Generating PGA for Distant Earthquakes

Narayan Prasad DEWANGAN1,2#+
1Chhattisgarh Government, 2Chhattisgarh Swami Vivekanand Technical University

This paper presents the identification of a Takagi-Sugeno-Kang fuzzy logic system based on Type-2 fuzzy logic modelling with formation of clusters in the data space and translation of these clusters into the TSK rules such that the model obtained is closer to the real system. The presented system is a seismic observation site whose peak ground acceleration is to be modelled based on the parameters like the earthquake magnitude, epicentral distance, standard penetration result, soil density, primary and the shear wave velocities. These data have been compiled from the Kyoshin Net, Japan. The model is trained and tested with these input parameters. It has been shown that the Type-2 TSKFLS is a suitable tool for estimating the PGA of various sites with different seismic criteria and also when the system has a noise. The model result can be used for estimating the potential loss and making mitigation and the other preparatory measures.


SE19-A005
The Different Patterns of Temporal Occurrence Between Big Interplate and Intraplate Earthquakes

Xibo JIN1#+, Gang LUO1, Mian LIU2
1Wuhan University, 2University of Missouri

Many studies have reported different temporal patterns of earthquakes, but the cause of these variations remain poorly understood. In this study, we analyzed twenty-two earthquake catalogs from twenty interplate and intraplate seismic zones in the world, with time scales ranging from several hundred years to more than one thousand years. We found that temporal patterns of big interplate and intraplate earthquakes are significantly different: most (> 91%) big interplate earthquake sequences tend to be quasiperiodic (COV<1), but 82% big intraplate earthquake sequences tend to clustered (COV>1). Analysis of these earthquake catalogs shows a clear correlation of the temporal patterns of big earthquakes with fault slip rate. When the fault slip rate is fast (> 5 mm/yr), the big earthquakes tend to be quasiperiodic; conversely, slow fault slip rates are correlated with clustered earthquakes. We suggest that viscoelastic stress relaxation is a major factor contributing to such correlations. Using a three-dimensional viscoelastoplastic finite-element model, we investigated the competing stressing from tectonic loading and viscoelastic relaxation; we were able to reproduce the observed correlation between fault slip rates and the major features of the temporal patterns of big earthquakes.


SE19-A007
What Can Cause Seismicity Acceleration and Deceleration Patterns During an Earthquake Cycle?

Gang LUO#+, Xibo JIN
Wuhan University

The acceleration and deceleration patterns of seismic moment release and Benioff strain release over time before a big earthquake or between two big earthquakes, have been observed in various regions of the world. However, the physical mechanisms or factors to control them have not been fully clarified. In this study, we analyzed temporal patterns of regional seismicity including acceleration and deceleration patterns from seismic catalog data of different seismic zones or regions in the world, and developed and used a three-dimensional viscoelastoplastic finite-element model and an analytical model to explain their controlling factors. We found that viscosity in lower crust and upper mantle can control seismicity acceleration and deceleration patterns during an earthquake cycle: the low viscosity tends to cause seismicity deceleration pattern but the high viscosity prefers to produce seismicity acceleration pattern. Fast stress relaxation in viscoelastic layers due to their low viscosity following an earthquake can cause fast postseismic stress accumulation within upper crust and lead to frequent occurrence of regional earthquakes at early stage of an earthquake cycle, generating deceleration pattern. On the contrary, high viscosity can encourage acceleration pattern with frequent occurrence of regional earthquakes at late stage of an earthquake cycle. Between the low and high viscosity, a transitional viscosity zone roughly from ~1×1019 to ~1×1020 Pa s exists. When regional average viscosity in lower crust and upper mantle stays within this range, seismicity acceleration and deceleration patterns can coexist at similar percentages and it is statistically hard to distinguish which pattern dominates in the region. Furthermore, we also found that regional tectonic loading velocity can impact seismicity acceleration and deceleration patterns during an earthquake cycle: slow tectonic loading velocity tends to cause seismicity deceleration pattern, but fast tectonic loading velocity favors to induce seismicity acceleration pattern.


SE19-A032
Localized Tsunami Source and Rupture Feature Revealed by High-resolution Moderate-size Aftershocks of the 2010 Mw 7.8 Mentawai Earthquake

Gatut DANIARSYAD1#+, Afnimar PAGACANCANG2, Shengji WEI3, Dimas SIANIPAR4, Daryono DARYONO1, Suko Prayitno ADI1, Dwikorita KARNAWATI1
1Indonesian Agency for Meteorology, Climatology and Geophysics, 2Bandung Institute of Technology, 3Nanyang Technological University, 4State College of Meteorology, Climatology, and Geophysics

Source parameters of offshore earthquakes in the subduction zones are critical to understand earthquake physics, plate tectonics as well as the seismic and tsunami hazards in the region. Here we demonstrate that, by using regional and global waveform observations, a high-resolution focal mechanism catalog is derived for the aftershocks of the 2010 Mw7.8 Mentawai tsunami earthquake. We invert focal mechanisms of the moderate-size aftershocks by applying the Cut-and-Paste (CAP) method to the regional waveforms. Their centroid depths are then verified using high-frequency teleseismic depth phases modelling. The surface wave cross-correlation relative relocation method is also applied to further refine their horizontal locations. Compared with all other global catalogs, our results show much more compact location distribution, where the lineation of the thrust events matches slab2.0 much better. Most of the shallow dip angle thrust events are located further down-dip on the plate interface, and largely overlapping with the postseismic slip of the mainshock as well as the background seismicity belt. Therefore, we consider these aftershocks were driven by the afterslip and background stress heterogeneity. There are five thrust events located at the edge of Mw7.8 coseismic rupture, likely due to incomplete mainshock rupture. Two of these five events are located very close to the trench at the depth of ~10km below the sea level. They are also very close to the normal faulting aftershock cluster that surrounds a subducting seamount, implying that the stress distribution within the oceanic plate may be affected by bathymetric anomalies along the trench. This location is highly consistent with high slip concentration near the trench as shown in the models derived from tsunami and/or geodetic data. We therefore suggest both the shallowest thrust and normal faulting events were triggered by the coseismic stress perturbation.


SE19-A026
Characteristics of Apparent Stress Before Moderate Earthquakes in Western Guangxi, China

Sha LI#+
Earthquake Agency of Guangxi Zhuang Autonomous Region

Apparent stress of seismic is the product of seismic efficiency and average stress and can be used as a lower limit estimate of absolute stress level in the source area. We calculated apparent stresses for 232 earthquakes(2.5≤ML≤4.3) occurring in western Guangxi of China since 2008. There were 6 times of stress rise in western Guangxi. Except that there were no earthquakes of M≥4 corresponding to the rise from March to August 2009, earthquakes of M≥4 occurred during or after the rise of the other 5 times of apparent stress. For example, since July 2019, the apparent stress suddenly increased with a large abnormal amplitude, and the high value lasted for 4 months. During the high value period, the Jingxi M5.2 earthquake occurred on November 25, 2019, and the apparent stress recovered to the normal level after the earthquake. Five months before the Debao M4.8 on August 4, 2021, the apparent stress gradually increased again. During the rising process, the Debao earthquake occurred. So, the apparent stress of moderate-small earthquakes in western Guangxi has the characteristic of “Rising-seismicity” with time, and the risk of moderate earthquakes occurring in 3-6 months after the apparent stress increase should be paid attention to, the index can be used as an effective criterion for tracking the pre-earthquake conditions of moderate earthquakes in western Guangxi. It is worth noting that after the 2021 Debao M4.8 earthquake, the apparent stress still rises and continues to the bottom of the 2021, which, combined with the active small earthquakes in western Guangxi, indicates that the regional stress is still at a relatively high level, we should track and analyze other precursory anomaly indexes and pay close attention to the risk of moderate earthquake in this area.


Wed-02 Aug | 1:10 - 3:10 | MR308
SE09 - In and Around the Tibetan Plateau: the Deep Structure, Geodynamics, Geohazards and Georesources

Session Chair(s): Xiaofeng LIANG, Chinese Academy of Sciences

SE09-A004
Moho Geometry Beneath the Eastern Himalayan Orogenic Belt Imaged by Receiver Function 3DCCP Method

Chunsen LI#+, Xiaoyu GUO, Xiao XU, Bo XIANG, You WU, Jiajie WU, Xucong LUO, Jiahao YU, Xiaofei TONG
Sun Yat-sen University

The ongoing India-Eurasia collision along the Yarlung-Zangbo suture zone since 55 Ma constructed the Himalayan orogenic belt. The question regarding their tectonic interactions at depths remains open. Identification of the Moho geometry will be the key responsible for understanding of the deep contact relationship between the Indian and Eurasian plates. In this study, based on the short-period dense array and previous studies on broadband stations, with employment of the teleseismic P-wave 3DCCP stack method after the improved Moho pickup algorithm, we obtained the high-resolution 3D Moho geometry in the region beneath the east-northern Himalayan tectonic belt. Together with previous studies on the 2DCCP profiles, tomography, and magnetotelluric profiles, the results show: (1) an increasing Moho depth from ~60 km beneath the Great Himalayans to ~70 -75 km beneath the dominant collision zone; (2) an offset Moho geometry within a 120 km-long east-west oriented depth gradient at about 28.9° N; (3) the northward-dipping Moho interface of the subducting Indian crust and no further extent beyond the YZSZ to the north. In a broader context, an integrated analysis drives us to propose that this Moho depth gradient to the south of the YZSZ in the east-northern Himalayans resulted from the subduction resistance and the contemporaneous clockwise rotation of the Indian continent that is pulled by the ongoing subduction of the Indian oceanic crust to the east of the Eastern Himalayan Syntax.


SE09-A006
A Semi-analytic Method for Solving the Acoustic Wave Equation in D'alembert Media

Zhiliang WANG#, Guojie SONG, Rong HUANG+
Southwest Petroleum University

Whether the simulation results can accurately portray the propagation process of seismic waves in the actual stratigraphic medium is not only related to the numerical method but also influenced by the mathematical-physical model. Both free oscillations of the Earth and the Experimental study of ultrasonic in rocks have shown that seismic waves exhibit energy attenuation over a wide range of frequencies and spaces. The inherent attenuation due to fluid flow in the medium and friction between rock particles are usually characterized by the quality factor Q based on viscoelasticity theory. Considering the rationality and simplicity of the D'Alembert medium model, the D'Alembert viscous acoustic wave equation is used in this paper to characterize the propagation process of viscous acoustic waves. This paper provides a framework to construct numerical methods for solving the D'Alembert viscous acoustic wave equation rather than a particular method. So, it is still possible to construct discrete formats of varying accuracy within the framework. Specifically, the semi-analytic formulation of the time domain of the D'Alembert viscous acoustic wave equation is first obtained based on the theory of differential equations. Then, the semi-analytic formulation is discretized according to the fixed solution conditions, and finally, different numerical methods are obtained by matching different spatial discretization formats. This paper not only gives the construction method of the discrete frame but also gives the general empirical formula to satisfy the stability condition based on the theory of partial differential equations, analyzes the numerical dispersion and viscosity characteristics of different methods, and studies the influence of the viscosity coefficient on the results. The results of numerical examples show that the proposed algorithm can effectively simulate the viscous acoustic wave field in complex media.


SE09-A012
Joint Inversion of Surface-wave Dispersions and Receiver Functions Based on Deep Learning

Feiyi WANG1+, Xiaodong SONG1#, Jiangtao LI2
1Peking University, 2Wuhan University

Joint inversion of surface-waves and receiver functions has been widely used to image Earth structures to reduce the ambiguity of inversion results. We propose a deep learning method (DL) based on multi-label Convolutional Neural Network (CNN) and Recurrent Neural Network (RNN) with a spatial attention module, named SrfNet, for deriving the Vs models from Rayleigh-wave phase and group velocity dispersions and receiver functions (RFs). We use a spline-based parameterization to generate velocity models instead of directly using the existing models from real data to build the training dataset, which improves the generalization of the method. Unlike the traditional methods, which usually set a fixed Vp/Vs ratio, our new method takes advantage of the powerful data mining ability of CNN to simultaneously constrain the Vp model. A loss function is specially designed that focuses on key features of the model space (such as the Moho and the surface sedimentary layer). Tests using synthetic data demonstrate that our proposed method is accurate and fast. Application to southeast of Tibet shows a consistent result and comparable misfits to observation data with the previous study, indicating the proposed method is reliable and robust.


SE09-A014 | Invited
The Thickness of Mantle Transition Zone Beneath Tarim Basin and Adjacent Region

Yangfan DENG1#+, Zhongfa HU2, Xiaofeng LIANG2
1Guangzhou Institute of Geochemistry, Chinese Academy of Sciences, 2Chinese Academy of Sciences

Tarim basin is a strong block that locates to the south of Tienshan Orogen, north of Tibetan Plateau. Previous tomography studies demonstrated the lithospheric subduction around the boundary between Tibet and Tarim, Tarim and Tienshan. However, it is still unclear whether these slabs suducted to the mantle transition zone (MTZ) or not. In addition, there are numerous studies showing a possible Permian mantle plume beneath Tarim, does this plume feature still reflect on the MTZ thickness? In order to target these questions, we take the advantage of the recent permeant stations (TA) inside Tarim basin, and stations from IRIS and Chinese Earthquake Administration to do the receiver function to estimate the feature of MTZ. 1-D and 3-D velocity model are used to do the migration. We find a similar MTZ thickness in Tienshan orogen compared with previous studies, which shows there is a thin MTZ beneath western Tienshan and a thick MTZ in central Tienshan. In addition, we find a thicker MTZ than normal beneath eastern Tarim and this feature is not caused by the sediment, but by the detached slab. The central and western parts of Tarim have a thinner MTZ, which indicates a hot upwelling that may drive by the subducted slab. The results provide useful knowledge on the deep process between Tibet and Tarim, Tarim and Tienshan.


SE09-A034
Restoration Method of Disequilibrium Compaction Overpressure in Tectonically Uplifted Area

Xiaojie HAN#+
Northwest University

Tectonic uplift not only reduces formation pressure but also causes pore rebound to change formation physical properties, which leads to errors in disequilibrium compaction identification and disequilibrium compaction overpressure calculation. To identify the accurate disequilibrium compaction formation and calculate the disequilibrium compaction overpressure in tectonic uplift areas, this paper first analyzes the mudstone log changes caused by tectonic uplift, and removes this part of the changes from the present mudstone compaction curves, then obtains the mudstone compaction law in the ancient burial depth period, which can be used to identify the disequilibrium compaction condition. Through the porosity measurement experiment, the pore rebound coefficient is calculated, then the change of loading curve caused by the rebound is obtained, and next the loading curve before the rebound is recovered, and finally, the disequilibrium compaction overpressure is calculated based on it. The results show that pore rebound leads to the decrease of the acoustic time difference and density, and the increase of resistivity and neutron porosity at the beginning of the disequilibrium compaction section, which is different from that in the unuplifted area. Furthermore, by comparing the calculation results of the loading-unloading curve method, formation pressure simulation, and equivalent depth method, it is found that the calculation overpressure of the conventional disequilibrium compaction method without considering pore rebound is larger. This study shows that both the identification of disequilibrium compaction and the calculation of overpressure in the tectonic uplifting area need to consider the influence of pore rebound, so as to provide a more effective research basis for pressure evolution, hydrocarbon accumulation and prediction in the tectonic uplifting area.


SE09-A044 | Invited
Shallow Crustal Structure of Tarim Basin: A Study Based on Multi-frequency P-wave Receiver Functions

Xiaofeng LIANG1#+, Wentao LI1, Xu WANG1, Sicheng ZUO1, Shilin LI2, Chen QU3
1Chinese Academy of Sciences, 2Southern University of Science and Technology, 3Chinese Academy of Geological Sciences

Tarim basin is characterized by its thick sediment over ancient crystalline basement. There are also widespread igneous rocks, such as basalt and rhyolites, discovered in the thick sedimentary strata as product of Permian mantle plume activity. The thick sedimentary basin records the tectonic deformation since Paleozoic with a Protozoic basement. The structure of the sediments and the topography of the crystalline basement is a useful proxy to understand the evolution of Tarim craton. Since the Permian large igneous province emplaced in the sediment strata, the sediment structure is important to understand the interaction between the mantle plume and the shallow crust. Here we utilized a joint inversion of multi-frequency receiver functions and horizontal-to-vertical ratios of seismic waveforms from two temporary broadband seismic arrays in the Tarim basin. We constructed the S-wave velocity (Vs) structure above 15 km depth. Various tests including changing smooth factors and initial velocity models demonstrated the stability of our inversion results. There were several high-velocity uplift regions and low-velocity depression areas in our velocity model, consistent with existing geological and seismic reflection data. High Vs anomalies of 3.3-4.2 km/s identified at Bachu Uplift and Tanan Uplift were interpretated as plutonic intrusions of Permian igneous activities, while those identified at Tazhong Uplift are suggested as older magmatic activities related with amalgamation of South and North Tarim.


SE09-A046
The Community Velocity Model V2.0 of Southwest China, Constructed from Dense Array Body and Surface Wave Data

Ying LIU1#+, Ziye YU2, Zhiqi ZHANG1, Huajian YAO1, Weitao WANG2, Haijiang ZHANG1, Hongjian FANG3, Lihua FANG2
1University of Science and Technology of China, 2China Earthquake Administration, 3Sun Yat-sen University

Located at the southeastern margin of Tibetan Plateau, southwest (SW) China has undergone extensive tectonic deformation due to the ongoing collision between Indian and Eurasian plate. It is playing a role in transition channel of material extrusion from the active Tibetan Plateau. Strong seismic activities associated with several active faults in SW China caused significant casualties and economic loss, including the devastating 2008 M8.0 Wenchuan earthquake. Currently, seismic monitoring, strong ground motion prediction and probabilistic seismic hazard analysis are essential in SW China. A community velocity model is crucial for these studies. The first version of community velocity model proposed by Liu et al. (2021) was constructed from joint inversion of body and surface wave data recorded at permanent seismic stations. In this study, we assembled seismic data of dense arrays in SW China to improve model resolutions. In total, more than 7 million body wave data and 100 thousand surface wave dispersion curves (5-50 s) are used. By applying joint body and surface wave travel time tomography, we obtained 3D Vp and Vs models with horizontal resolution up to 20-30 km as well as high precision relocations of seismic events. We observed high heterogeneities in the upper crust, two unconnected low velocity zones in the middle-lower crust and high velocity anomalies in the inner zone of Emershan large igneous province. High velocity anomalies are observed in the source region of the 2008 Mw7.9 Wechuan earthquake, the 2013 M7.0 Lushan earthquake and the 2017 M7.0 Jiuzhaigou earthquake.


Wed-02 Aug | 1:10 - 3:10 | MR334
SE07 - Large Igneous Province Record and Their Likely Connection with Supercontinents: with Special Emphasis to the Indian Shield

Session Chair(s): Greg SHELLNUTT, National Taiwan Normal University, Hafida El BILALI, Carleton University

SE07-A006
Distinct Mafic Dyke Swarms from the Bhanupratappur, Central Bastar Craton, India: Constraints from Geochemical Studies

Ankur ASHUTOSH#+, Gulab Chand GAUTAM, Rajesh Kumar SRIVASTAVA, Amiya Kumar SAMAL
Banaras Hindu University

Nine distinct Precambrian mafic dyke swarms are reported from the Bastar craton. The central region, particularly around the Bhanupratappur, comprises three prominent dyke swarms trending in NW, NNW and ENE. The NW-trending dykes are undoubtedly dated ca. 2.36 Ga. Field evidences suggest that NNW- and ENE-trending dykes cut the ca. 2.36 Ga NW-trending dykes, suggesting younger ages. Shellnutt et al. (2018) dated a NW-trending dyke that yields ca. 1.88 Ga age, however, later it is confirmed that this dyke is trending NNW and not NW. The third dyke swarm is trending in ENE and supposed to be part of the ca. 2.25 Ga Chhura swarm. The present work is aimed to study mafic dykes of these three swarms for their geochemical characteristics to verify whether these three swarms show different geochemistry or not. Broadly, samples of all the three swarms show basaltic to basaltic-andesite composition and exhibit fractionation of olivine, clinopyroxene, plagioclase and Cr-spinel. However, geochemically, they show slightly different nature. The ca. 2.36 Ga and ca. 2.25 Ga dykes show enriched LREE and flat HREE patterns, however, samples of ca. 2.25 Ga exhibit more enrichment in LREE than the ca. 2.36 Ga samples; probably due to difference in variable crustal component mixing. REEs of the ca. 1.88 Ga dykes are exclusively different as they show almost flat pattern suggesting high percentage of melting of the mantle source without any crustal contamination. These geochemical differences support their derivation from different mantle melts, however, melts of two older swarms, i.e., ca. 2.36 Ga and ca. 2.25 Ga, are derived from similar mantle sources but variable crustal contamination. Furthermore, these three distinct swarms can be linked with the ca. 2.37-2.36 Ga Bangalore, the ca. 2.26-2.25 Ga Ippaguda, and the ca. 1.89-1.88 Ga Bastanar large igneous provinces of the Indian Shield.


SE07-A005
Spatial Variations in Geochemistry and Emplacement Systematics of the Ca. 2.08 Ga Devarabanda Radiating Dyke Swarm of the Eastern Dharwar Craton: Implications for Multiple Magma Pulses from a Concentric Magma Chamber

Srinjoy DATTA#+, Amiya Kumar SAMAL, Sayandeep BANERJEE, Rajesh Kumar SRIVASTAVA, Aishwarya MOHAN
Banaras Hindu University

Despite thorough study, regional variations in geochemistry and magma flow dynamics in radiating dyke swarms remains poorly understood. The studied ca. 2.08 Ga Devarabanda dyke swarm of the eastern Dharwar Craton displays a classical radiating geometry that consists of three distinct sub-swarms trending in ~N, ~NW and ~NE. In earlier studies, the intra-swarm variability of geochemistry and emplacement systematics was either not tracked or there were insufficient representative samples from all the three sub-swarms. Herein, we undertake a comparative study between the three sub-swarms to understand their spatial variations in geochemistry together with magnetic fabrics and constrain their emplacement mechanisms. The ~NE-trending sub-swarm displays a relatively primitive signature, i.e., depleted REE-trace element values, higher Mg#, Ni and Cr, and lower Zr and TiO2, as compared to its counterparts, i.e., N-trending sub-swarm, and NW-trending sub-swarm. However, all three the sub-swarms follow common differentiation trends attributing to their common genetic linkage. Our geochemical data further advocate a crustal influence at source for all the three sub-swarms suggesting melting of a common sub-continental lithospheric mantle source. Available radiometric ages also corroborate this inference, therefore, we suggest involvement of multiple magma pulses from a magma chamber, for emplacement of ca. 2.08 Ga swarm, with the ~NE-trending dykes derived from an earlier primitive pulse, whereas the other two sub-swarms representing later differentiated pulses. Furthermore, Anisotropy of Magnetic Susceptibility (AMS) analyses indicate lateral magma flow for the ~NE-trending dykes, whereas other two were fed through vertical magma injection, which further strengthen the involvement of independent magma pulses in the emplacement of the three sub-swarms. AMS data of country rock and regional fracture analyses suggest a combined control of the regional and local stress fields in emplacement of ca. 2.08 Ga dyke swarm. An emplacement model is also presented.


SE07-A001 | Invited
The Panjal Traps: New Data, New Insights

Greg SHELLNUTT#+
National Taiwan Normal University

The Panjal Traps of the western Himalaya are composed of basalt with subordinate silicic volcanic rocks. Radioisotopic dating of the silicic (288.1 ± 3.7 Ma; 289.0 ± 2.5 Ma; 289.3 ± 1.4 Ma) and mafic (288.2 ± 0.3 Ma) rocks confirm their Early Permian eruption age. The dacitic volcanic rocks have Neoarchean (2.6-2.5 Ga), Paleoproterozoic (2.4-1.8 Ga), Mesoproterozoic (1.4-1.0 Ga), Neoproterozoic (0.9-0.6 Ga), and Early Paleozoic (0.58-0.42 Ga) inherited zircons. The mafic rocks have compositions that range from continental tholeiite to ocean-floor basalt. The initial basalt eruptions have chondritic Sr-Nd isotopes (87Sr/86Sri = 0.7043 to 0.7073; eNd(t) = -1.4 to +1.3) whereas the later flows have a wide range of Sr-Nd (87Sr/86Sri ³ 0.7083; eNd(t) = -6.8 to -1.5) isotopic values. The basalt from the northern Pir Panjal Range are compositionally distinct (87Sr/86Sri = 0.7081 to 0.7172; eNd(t) = +2.4 to +4.3) from other regions of the Panjal Traps including those from the southern Pir Panjal Range (87Sr/86Sri = 0.7086 to 0.7110; eNd(t) = -6.1 to -4.4). New Os- and O-isotopic data confirm that the northern Pir Panjal Range rocks are distinct (d18OVSMOW = 6.8-7.9‰; 187Os/188Osi = 0.1230-0.1256) from others regions of the Panjal Traps (d18OVSMOW = 9.0-12.9‰; 187Os/188Osi = 0.1343-0.2832). The silicic volcanic rocks were derived by partial melting of the Himalayan crust (87Sr/86Sri = 0.7073 to 0.7119; eNd(t) = -7.2 to -8.9). The primary melt composition of the basalt is picritic with mantle potential temperatures (TP) of 1400-1450oC. It is likely that the early lavas erupted within a continental rift setting that eventually transitioned into a nascent ocean basin and formation of Neotethys Ocean.


Wed-02 Aug | 3:30 - 5:15 | MR306
SE19 - Faults and Earthquakes: Networks, Precursors and Monitoring Systems

Session Chair(s): Fuqiong HUANG, China Earthquake Networks Center, China Earthquake Administration

SE19-A025 | Invited
Elastic Wave Reverse Time Imaging for Earthquake and Microseismic Sources

Wei ZHANG#+, Nan HU
Southern University of Science and Technology

Source Reverse Time Imaging (RTI) utilizes the wave-equation to back-propagate the recorded waveforms to detect and locate the event locations. It can detect and locate weaker events because RTI uses wave-equation to enhance the coherent signals from the source and suppress noise. But the slip mechanism of earthquake and microseismic sources causes the recovered wavefield by time-reversal calculation does not focus at the true location but exhibits a spatial distribution due to the slip source radiation pattern. In this talk, we will introduce an imaging condition with less image artefacts for elastic wave source location by utilizing the directional coherency of the P and S wave propagations, and a model-based interferometric approach and a deep-learning network approach to correct the effect the radiation pattern on the detection and location of the earthquake and microseismic events. The proposed method can detect and locate weaker events with strong noise in complex velocity structures, which can produce more small event locations to better derive the 3D fault geometry and to help to analysis the earthquake risk.


SE19-A035 | Invited
Three-dimensional Numerical Simulation of the Influence of Transverse Heterogeneous Viscosity on Seismic Cycles in a Strike-slip Fault Model

Jinshui HUANG#+, Peng ZHAI, Haigang ZHENG
University of Science and Technology of China

Numerical modeling of earthquake cycles provides a physics-based framework to study fault slip, stress drop, earthquake recurrence, and postseismic deformation, thus helping to understand long-term earthquake source processes and even contributing to earthquake prediction. Evidence from postseismic deformation of large earthquakes strongly supports the existence of lateral viscosity contrast across many strike-slip faults. Heterogeneity in lithospheric viscosity structure can influence the efficiency of stress transfer and thus may have a great effect on the seismic cycle. In this study, we formulated a 3D quasi-static finite element viscoelastic model and the advantage of this model is that it can simulate interseismic creep and coseismic slip above the brittle-ductile transition zone and viscoelastic relaxation of the deeper portion of the model simultaneously. The main focus of this study is to explore the effect of the across-strike viscosity variation on the earthquake recurrence interval and interseismic ground surface deformation. The numerical results show that: 1) the basic seismic cyclic characteristics, such as the accumulation and release of stress-strain, are consistent with the results of earlier 2D models; 2) with the decrease of the effective viscosity, the coulomb stress value required to produce coseismic rupture is greater, and it takes longer time to accumulate shear stress, thus increasing the seismic interval; 3) for the model with viscosity difference across the fault, the seismic process is mainly controlled by the side with low viscosity; and 4) the viscosity difference across the fault will cause the asymmetric distribution of the surface deformation.


SE19-A034
Reservoir as Precursors and Controllers of Seismic Activity

Bhaskar CHANDRAKAR1#, Mohan GUPTA2, Shashikant JAISWAL2, Narayan Prasad DEWANGAN3,1+
1Chhattisgarh Swami Vivekanand Technical University, 2Bhilai Institute of Technology Durg, 3Chhattisgarh Government

Earthquakes occurring due to the obstruction of naturally flowing stream and concentrating the huge dynamicity of flowing water into enormous potential energy stored in the upstream of the dam, has caused the faults present in the underground lineament of Earth to slip and shake the ground level as well, resulting in an earthquake. Several cases in history were suspected to have occurred due to the construction of large dams and reservoirs. This phenomenon could be executed for inducing controlled small scale fault movements underground through fluid injection which would result in reducing the magnitude of natural earthquake whenever the same occurs. David Evans experiment in oilfields of Rangeley, Colorado demonstrated the feasibility of inducing controlled seismic activity. This paper highlights the case studies of Reservoir induced seismicity and application of this phenomenon, if replicated for artificial response generation to release the high pore pressure inside the rocks deep beneath the crust.


SE19-A008
Fault Movements in Natural Gas Exploration and Environmental Sustainability Practices for the Corporate Sectors--GAIL India Perspective for Global Scenario

Pranay DEWANGAN#+
GAIL India Limited

We are witnessing the climate change and, is evident even than before as also the strengths of the voices raised in so many world summits attended by the world powers and the environmental activists. It has therefore become imperative now to reduce our carbon emissions for a clearer environment. As we energizing growth, coherent efforts are essential towards improving environmental, social and corporate governance for better performance. In this sector, the GAIL India is committed to reduce carbon footprints by scientific methods and adopting a business model having direct positive impact on environmental and social parameters. While exploring natural gas entrapped in the extremely impleadable hard rock foundations wherein the fluid injection and evacuation of the gas produces variable pressure differences into the different ground level and subsequently leading to differential fault settlements and the quakes. GAIL promotes R & D in this front to enhance its environmental performance.


Wed-02 Aug | 3:30 - 5:15 | MR308
SE09 - In and Around the Tibetan Plateau: the Deep Structure, Geodynamics, Geohazards and Georesources

Session Chair(s): Hongfeng YANG, The Chinese University of Hong Kong, Xiaoyu GUO, Sun Yat-sen University

SE09-A048 | Invited
Do Only Large Earthquakes Rupture the Surface?

Hongfeng YANG#+, Suli YAO
The Chinese University of Hong Kong

Surface rupture produced by earthquakes can pose great threat on near-surface infrastructures and elevate damages. Accessing the surface-breaching potential of earthquakes is critical to mitigating such hazards. To understand the controlling mechanisms, we first collect source parameters for earthquakes with Mw>6.5 and M<6 surface-breaching events globally. For strike-slip and normal events, almost all earthquakes with magnitudes over 6.7 broke the surface. In contrast, buried and surface-breaching events co-exist with moderate magnitude (6.0-6.7). For reverse events, there is no clear magnitude boundary, as thrust buried ruptures can be quite large due to the downdip size of the seismogenic zone. The relocated hypocenter depths for moderate-to-large events are concentrated at depth of 5-20 km. Differently, all M<6 surface-breaching events occurred at very shallow depths (<5 km). We then conduct dynamic rupture simulations and propose two conceptual models of whether ruptures may break the surface. The first model represents a fault with a continuous but heterogeneous seismogenic zone (velocity-weakening). In this case, ruptures need to overcome the shallow velocity-strengthening zone (VS) with certain energy sink to reach the surface. Therefore, a thinner shallow VS zone and a higher stress drop of the earthquake can promote surface rupture, consistent with our observations. However, ruptures nucleating from different locations on heterogeneous faults may lead to different surface rupture patterns and final magnitudes, shedding lights on the diverse behaviors among moderate earthquakes. The second model is for small surface-breaching earthquakes. Those events are supposed to occur on shallow isolated velocity-weakening patches, consistent with the fact that usually no large earthquakes have been reported on the same fault zones. Such asperities may be formed on bodies with high-strength materials, leading to energetic ruptures with intense stress release. Our study contributes to the understanding of the surface rupture behaviors references for assessing near-surface damage in future earthquakes.


SE09-A008
Stress Transfer Along the Western Boundary of the Bayan Har Block on the Tibet Plateau from the 2008 to 2020 Yutian Earthquake Sequence in China

Ke JIA1#+, Shiyong ZHOU2, Jiancang ZHUANG3, Changsheng JIANG4
1Northwestern Polytechnical University, 2Peking University, 3Institute of Statistical Mathematics, 4China Earthquake Administration

Eight Ml≥7.0 earthquakes have occurred around the Bayan Har block, NW Tibet, China, since 2000, resulting in a large number of casualties. Near the western boundary of the Bayan Har block, four Ml≥6.0 Yutian earthquakes have occurred from 2008 to 2020. Stress interactions among them are comprehensively investigated by applying the ETAS (Epidemic-Type Aftershock Sequence) model and calculating (Coulomb failure stress change) from a 3D linear viscoelastic mode. The combined (coseismic plus postseismic) induced by proceeding Yutian earthquakes on hypocenters of the 2012, 2014 and 2020 Yutian earthquakes are -1.5×10-4 , 3.6×10-3 and 1.5×10-1 MPa, respectively. The background probabilities of the 2008, 2012, 2014 and 2020 Yutian earthquakes are 0.87, 0.97, 1.5×10-3 and 8.7×10-5, respectively. Combining those two independent approaches, we conclude that the 2008 and 2012 Yutian earthquakes are more like background earthquakes and that the 2014 and 2020 Yutian earthquakes were triggered by the proceeding Yutian earthquakes.


SE09-A020 | Invited
New Insights Into the Active Seismicity and Tectonics of Myanmar and Surrounding Regions from a Unified Earthquake Focal Mechanism Catalog (1963-2021)

Shengji WEI#+, Wardah FADIL, Kyle BRADLEY
Nanyang Technological University

We integrate a refined earthquake focal mechanism catalog with available catalogs in the Myanmar region to provide new insights into the active seismicity and tectonics and their seismic hazard implications. We divide the earthquakes into several tectonic sub-regions and conduct a stress analysis using the principal stress orientations derived from the focal mechanisms. We find that: 1) Active crustal seismicity beneath the Central Myanmar Basin (CMB) reveals a diffuse deformation zone between the subduction front and the Sagaing Fault, 2) A ~220-km long seismic gap on the central Sagaing Fault is adjacent to a seismic gap beneath the CMB, suggesting a potential triggering relation between the Sagaing Fault and faults within the adjacent crust, 3) A backstop-fault system accommodates ~E-W compression between the accretionary wedge at the eastern Indo-Myanmar Range and the forearc crust, 4) Intraslab mechanisms reveal stress in the slab is mostly induced by the subslab trench-parallel mantle flow, 5) Nodal plane orientations in a locally unfolded Indian slab reference frame suggest potential re-activation of subducted lithospheric fabrics related to the NW-SE oriented spreading beneath the Bay of Bengal and N-S oriented spreading beneath the Wharton Basin, 6) The lack of plate interface earthquakes along the Rakhine-Bangladesh Megathrust in the past six decades, despite active convergence suggested by geodetic and paleo-seismological studies, indicates potential strain accumulation. These new findings necessitate a re-assessment of the seismic hazard within the region, given the identified seismic gaps and active structures accommodating deformation on and away from the plate boundaries.


SE09-A025 | Invited
Fault Zone Geometry of the 2021 Ms 6.4 Yangbi Earthquake Sequence Revealed by a Dense Seismic Array

Chunquan YU#+, Xianwei ZENG
Southern University of Science and Technology

The 2021 MS 6.4 Yangbi earthquake occurred near the southwestern boundary of the Chuandian block in the SE Tibetan Plateau, with a right-lateral strike-slip focal mechanism. It is widely believed that its occurrence is related to the SE extrusion of the Chuandian block. However, previous studies found that the mainshock occurs off the main boundary fault – the Weixi-Qiaohou-Weishan fault. The mechanism of the 2021 Yangbi earthquake is still debated. Soon after the mainshock, we deployed a dense array of 200 nodal seismometers in the vicinity of the 2021 Yangbi earthquake source region. Station spacing is about 2~3 km. In this study, we use the three-month-long continuous recordings of the dense array to precisely locate the aftershocks of the 2021 Yangbi earthquake sequence and to determine the focal mechanisms of relatively large aftershocks. We obtained 88934 high-resolution event locations and 625 reliable focal mechanisms. Based on aftershock locations and focal mechanisms, we constructed a detailed 3D fault zone geometry model of the 2021 Yangbi earthquake sequence. The main fault generally dips to the southwest in a shovel shape with a clear bend in the middle. We also detected several conjugate faults. One of them dips to the northeast and intersects with the main fault at a depth of about 6 km, which might be the seismogenic fault of the largest foreshock. It appears that there is another listric fault below the main fault, which might connect to the mapped Weixi-Qiaohou-Weishan fault at the surface. Our study provides new insights into the mechanism of the 2021 Yangbi earthquake sequence. The 3D fault-zone geometry can potentially be used for dynamic source modeling to better understand the initiation and rupture process of the main shock.


SE09-A029
Lithospheric Rheological Properties Beneath Himalayas Inferred from Postseismic Deformation of the 2015 Mw7.8 Gorkha Earthquake

Jian ZHANG1+, Yan HU2#, Bin ZHAO3
1University of Science and Technology of China, 2Deep Space Exploration Laboratory/University of Science and Technology of China, 3China Earthquake Administration

The 2015 Mw7.8 Gorkha (Nepal) earthquake was the largest event along the Himalayan arc in the past 80 years. Two weeks later, the largest aftershock of magnitude Mw 7.3 occurred about 150 km east of the mainshock. These two earthquakes induced prolonged postseismic deformation that may be controlled by afterslip over the fault and viscoelastic relaxation in lower crust and upper mantle according to previous studies. We constructed a three-dimensional viscoelastic finite element model to study the two deformation processes through first 5-year postseismic GPS observations. We considered a reliable geometry of the underthrusting Indian lower crust and upper mantle based on various geophysical images. Model results show that the models with a wholescale elastic Indian lower crust fail to fit the vertical observations. A heterogeneous Indian lower crust with the transition from elastic (high-viscosity) to low-viscosity approximately under the Main Central Thrust is required to reproduce the postseismic uplift between China-Nepal border and Peiku Lake, indicating the weakness of the Indian lower crust from the Lesser to High Himalaya. The afterslip simulated using a weak shear zone is distributed downdip of the rupture area and may be the primary process controlling deformation in the near field. Test models have determined viscosity of the Tibetan lower crust, weakened Indian lower crust and shear zone to be 3 × 1018, 1019 and 4 × 1018 Pa s, respectively. The viscosity of the underthrusting Indian upper mantle was roughly estimated to be greater than 1021 Pa s. The inferred rheological properties of the lithosphere may help better understand the formation and evolution of the Himalayas.


SE09-A003
Constraints on the Geometry and Frictional Properties of the Lenglongling Fault Using Earthquake Cycle Deformation in the Northeast Tibetan Plateau

Guangyu XU1#+, Xiwei XU2, Yaning YI3, Yangmao WEN4
1East China University of Technology, 2China University of Geosciences, 3Ministry of Emergency Management of China, 4Wuhan University

The Lenglongling fault located in the northeast margin of the Tibetan Plateau plays an important role in accommodating the eastward component of the movement of Tibet relative to the Gobi-Ala Shan platform to the north. The 8 January 2022 Mw6.6 Menyuan earthquake occurred on the western segment of the Lenglongling fault, which provides an opportunity to investigate the detailed geometry of this fault. Here, we use interseismic, coseismic, and postseismic geodetic data to investigate the coseismic slip distribution, postseismic deformation following the Menyuan earthquake, and the interseismic strain accumulation. We devised a strike-variable fault geometry constrained by the SAR offset tracking results and Gaofen-7 optical images and used a Bayesian method incorporating epistemic uncertainties to solve for the fault geometry and coseismic slip. The inversion results suggest that at least two faults were involved in Menyuan earthquake. The main fault corresponds to the western segment of the Lenglongling fault; the secondary fault corresponds to eastern end of Tuolaishan fault, and two faults form a lying Y-shaped layout. The majority of slip occurred between 0~9 km depth on the main fault, and 0~4 km depth on the secondary fault. We further investigate the major controlling mechanism for the postseismic period and frictional properties along the fault. We find that the earthquake cycle geodetic observations can play a complementary role in constraining fault geometry. Finally, we discuss the interaction of active faults in Qilian-Haiyuan fault zone and evaluate the future seismic hazard in this area.


SE09-A045
Provenances of the Lower—middle Permian in Beishan Region, Central Asian Orogenic Belt and Its Paleogeographic Implication

Dongdong ZHANG#+, Yazhuo NIU, Jianqiang WANG
Northwest University

The marine Permian strata from Beishan Region play an important role in the paleogeographic reconstruction of the late stage of the Paleo-Asian Ocean (PAO) as one of the youngest marine deposits in the Central Asian Orogenic Belt (CAOB). However, the paleogeographic discussion of the PAO is hindered by the unbalanced distribution of the provenance data and the lack of statistical analysis. This study reports 681 U-Pb ages and 192 Hf isotopic data from eight sections from the central and southern Beishan regions. The paleogeographic pattern is reconstructed based on isochronous stratigraphic correlation and statistical analysis of published samples of detrital zircons from the Lower –Middle Permian strata. During the Early–Middle Permian, the southward subduction of the Hongshishan ocean resulted in the Heiyingshan arc and a back-arc rifting basin. The deposits on the northern margin of this rifting basin were fed from the Precambrian basement (926 ~ 775Ma) and Ordovician –Silurian plutons (485 ~ 421 Ma) in the Hanshan Block. The sediments on the southern margin were sourced from the Mazongshan Uplift. This uplift composed of the Ordovician–Devonian plutons (470 ~ 367Ma) was caused by the closure of the Hongliuhe–Xichangjing ocean in the early Paleozoic. The realm of this uplift covers the main areas of the Maozongshan arc and northern Shuangyingshan block. Detritus of the southern and northern margins of the Liuyuan rifting basin were respectively sourced from Carboniferous–Permian volcanic rocks (322~ 270 Ma) and early Paleozoic plutons of the Mazongshan Uplift. The detrital exchange occurred in the depocenter of the Liuyuan basin. The paleogeographic reconstruction indicates that the Hongshishan ocean as the main branch of the PAO lasted in the Early–Middle Permian and several rifting basins developed in the back arc regions.


Wed-02 Aug | 3:30 - 5:15 | MR334
SE14 - Cratons: Structure and Evolution

Session Chair(s): XIA BING, CUG, Hans THYBO, SinoProbe Laboratory

SE14-A009
Formation and Evolution of the Ordos Block Basement, North China Craton: Constraint from the U-Pb Dating and Lu-Hf Isotopes of Zircons from the Mesoproterozoic Sandstones

Yang HU#+, Chengli ZHANG, Jinglan LUO
Northwest University

The Ordos block (OB) is an important part of the North China Craton and plays a crucial role to understand the early crust evolution. However, little is known about its basement due to overlying sedimentary covers. The U-Pb dating and Lu-Hf isotope analyses were performed on the detrital zircons from the Mesoproterozoic sandstones in the OB to disclose the basement evolution. The zircon U-Pb data exhibit three age clusters of the 2.55-2.4 Ga, 2.2-2.0 Ga, and 1.95-1.8 Ga as well as minor Paleo- to Neoarchean ages. Of which, Paleo- to Mesoarchean zircons have εHf(t) of -7.1 to -5.1 and TDMC of 4.3-3.9 Ga. While 2.8-2.6 Ga zircons show εHf(t) of +0.6 to +6.4 and TDMC of 3.3-2.8 Ga. These suggest that the initial crust was formed in the Paleoarchean and then subjected to crustal reworking. Thereafter, massive juvenile crust growth occurred ca. 2.7 Ga, marking that the dominant crust had been formed in the OB around 2.7 Ga. While, the tectonothermal events of the 2.55-2.4 Ga, 2.2-2.0 Ga, and 1.95-1.8 Ga proposed the OB subjected three important tectonothermal events after 2.7 Ga. In which, the 2.55-2.4 Ga zircons yield εHf(t) of -6.9 to +7.7 and TDMC of 3.39-2.47 Ga, being a result of the crust reworking and juvenile crust additions. The 2.2-2.0 Ga and 1.95-1.8 Ga zircons also have wide εHf(t) (-13.4 to +7.5 for the former, -14 to +4.13 for the latter) and TDMC (3.5-2.2 Ga, 3.4-2.3 Ga), indicative of the mixture of the Meso- to Neoarchean and juvenile crustal materials. Consequently, the dominant crust materials of the OB were formed ca. 2.7 Ga after the primary crust had been formed and reworked in the Paleoarchean, and then subjected to three tectonothermal event modifications.


SE14-A003
Water and Oxygen Isotope Insights Into Genesis of TTGs in the Eastern Block, North China Craton

Dingyi ZHAO#+, Guochun ZHAO, Min SUN
The University of Hong Kong

Continental crust on Earth were voluminously formed during Archean time. Controversy has long surrounded the issue of whether the partial melting of mafic crust to form Archean TTG rocks occurred under plate tectonic settings (e.g. island arc) or under some pre-plate tectonics (e.g. mantle plume, sagduction, etc.). In this case, water contents, oxygen isotopes and some other trace elements of the source rocks are regarded as important insights as they should be different between plate tectonic settings and other pre-plate tectonic settings. Therefore, we report variations in water contents, oxygen isotopes, hafnium isotopes and trace elements of zircons, associated with whole-rock major and trace elements of the ~2.5 Ga Taipingzhai TTG gneisses in the Eastern Block of the North China Craton. Based on these data, we prove that oxygen and water in zircons can be used as a good proxy for primordial oxygen and water in TTG magmas. In this study, zircons from the Taipingzhai TTG gneisses have high oxygen isotopes but relatively low water component, with no or weakly negative correlation between water and oxygen isotopes, indicating that the source rocks of TTG were hybridized hydrated mafic rocks with majority of slightly hydrous oceanic plateau and minority of high-δ18O supracrustal materials. Such results indicate a combined two-stage mantle plume-sagduction model, in which minor TTG (mantle-like δ18O, low H2O) and voluminous TTG (high δ18O, low H2O) were formed at ~2.7 Ga and ~2.5 Ga from the Eastern Block of North China Craton, respectively. Acknowledgement: This work was financially supported by NSFC Major Project (41890831) and Hong Kong RGC grants (17307918), and HKU Internal Grants for Member of Chinese Academy of Sciences (102009906) and for Distinguished Research Achievement Award (102010100). This work is a contribution of the Joint Laboratory of Chemical Geodynamics between HKU and GIGCAS.


SE14-A002
How Cratonic Roots Survive with Weak Mid-lithosphere Discontinuities?

Qionghua GUO#+, Huilin WANG
Huazhong University of Science and Technology

Cratons are the ancient cores of continental plates and have remained stable for billions of years. High strength of the cratonic root is considered to be the key factor for the survival of thick craton root in the vigorously convicting mantle. However, since the last 20 years, increasing seismic studies have observed the presence of the mid-lithospheric discontinuities (MLDs) layer in the cratonic roots, where the seismic velocity is reduced by 2-6%. MLDs were initially used to interpret the negative Sp phase detected at mid-lithospheric depth in the North American craton. This feature has been successively observed in global cratons such as South African, Scandinavian and Indian cratons, at a depth of ~100 km. Xenoliths and seismic studies suggest MLDs may be formed through metasomatism and are weaker than the surrounding cratonic mantle. This raised the question of how the thick cratonic roots are preserved with the widely distributed weak MLDs? Using two-dimensional finite element numerical models, we systematically test the MLDs’ geometry and distribution role in the craton stability during the long-term plate motion. Our models show that the mantle flow can shear the deep craton roots off along the weak MLDs by several hundreds of kilometers, as long as the distribution of MLDs is laterally continues. However, when the MLDs is laterally discontinues and the intermission is >40 km, the craton root can remain stable. Our results indicated that MLDs may be originated from non-homogeneous reactions at different periods and/or locations to make them laterally disconnected, and these small “gaps” make the craton survive.


SE14-A006 | Invited
The Causality Between Subduction of Paleo-Pacific Plate and Destruction of North China Craton: A Magmatic Perspective

Qiang MA1#+, Jian-Fang GUO1, Yigang XU2, Jian-Ping ZHENG1
1China University of Geosciences, 2Guangzhou Institute of Geochemistry

Eastern China provides a precious opportunity to explore how subduction drives destruction of the overlying continental lithosphere. This issue is addressed here by examining examine temporal and spatial variations in distribution, composition and generation of Mesozoic magmas in the North China Craton and adjacent NE China. Our study highlights a trend of magma migration that swept inland in the Jurassic and then swept back to the trench in the Cretaceous. This behavior, together with the spatiotemporal variations in petrology, chemistry and isotopes of the igneous rocks, the crustal-deformation patterns and the migration of basins, collectively suggests a geodynamic transition at ca 145–140 Ma from forward-flat-subduction to rollback of the Paleo-Pacific slab. We also observed a temporal variation in chemical and isotopic compositions of the Mesozoic volcanic rocks from individual basins, suggesting a transition of magmatic source varying from lithospheric mantle to lithospheric mantle plus lower crust, and then to the lower-middle crust. This shift is interpreted to changes in lithospheric thickness caused by interaction between subducted plate/asthenosphere and the overlying continental lithosphere. The Mesozoic magmatism, as well as the lithospheric destruction, across the North China Craton is therefore proposed as the consequence of a change in subduction geodynamic regime of the Paleo-Pacific slab and its interaction with overlying continental lithosphere, which involves an active continental arc in the early-middle Jurassic, progressive shallowing of the subducting Paleo-Pacific plate in the middle-late Jurassic, and subsequent slab rollback in the early Cretaceous.


SE14-A012 | Invited
Heterogeneous Cratonic Mantle and Kimberlite Magmatism

Irina ARTEMIEVA#+
GEOMAR Helmholtz Centre for Ocean Research Kiel

Compositional heterogeneity of lithospheric mantle is known from kimberlite-type magmatism in Precambrian cratons (Artemieva, 2011). This magmatism should lead to a significant thermo-chemical modification of the cratonic lithosphere (Artemieva, 2009), while geochemical studies of mantle xenoliths provide the basis for many geophysical interpretations. Magmatism-related thermo-chemical processes are reflected in the thermal, density, and seismic velocity structure of the cratonic lithosphere (Artemieva, 2007, 2009, 2011; Artemieva & Vinnik, 2016ab; Cherepanova & Artemieva, 2015). Based on joint interpretation of geophysical data, I demonstrate the presence of significant lateral and vertical heterogeneity in the cratonic lithospheric mantle worldwide. This heterogeneity reflects the extent of lithosphere reworking by kimberlite-type magmatism (e.g. Kaapvaal, Siberia, Baltic and Canadian Shields) and tectono-magmatic processes, e.g. associated with LIPs and subduction systems such as in the Siberian (Cherepanova & Artemieva, 2015; Artemieva et al., 2019) and North China cratons (Xia et al., 2020). The results show a strong correlation between the calculated density of the lithospheric mantle, the crustal structure, the spatial pattern of kimberlites, and their emplacement ages. In all studied cratons, blocks with the lowest values of mantle density are not sampled by kimberlites and may represent the “pristine” Archean mantle (Artemieva, 2007; Artemieva & Vinnik, 2016ab; Cherepanova & Artemieva, 2015; Shulgin & Artemieva, 2019; Artemieva et al., 2019). The results show that cratonic lithospheric mantle is highly heterogeneous both laterally and vertically, with kimberlite magmatism restricted to anomalous lithosphere (Artemieva et al., 2019). An important conclusion is that the Nature’s sampling by kimberlite-hosted xenoliths is biased and therefore is non-representative of pristine cratonic mantle.


SE14-A001
Effective Elastic Thickness of Earth’s Continental Lithosphere: Evidence for Time-dependent Control

Zhezhe LU1#+, Pascal AUDET2, Jiabiao LI3, Tao ZHANG4, Chun-Feng LI5
1Second Institute of Oceanography, Ministry of Natural Resources, 2University of Ottawa, 3State Oceanic Administration, 4Ministry of Natural Resources, 5Zhejiang University

Earth’s tectonic history has been punctuated by several cycles of supercontinent assembly and breakup. Continents are the last puzzles preserving the history and records of global tectonic evolution, with the oldest continental rocks being up to ~4.0 Ga. The formation, growth, and reworking of continental lithospheres affect their thermal structure and deformation. The effective elastic thickness of the lithosphere (Te) corresponds to the thickness of an idealized, equivalent elastic plate bending under transverse (i.e., vertical) long-term (>105 yr) applied loading, which reflects the lithosphere’s depth-integrated strength and is useful for deciphering the complex evolution of continents. In this study, we present a high-resolution (15’ x 15’) Te map of Earth’s major continents based on a spectral analysis of topography and gravity anomalies. The continents have a Te range from <5 km to 140 km, with a mean and standard deviation of 50 and 33 km, respectively. Based on a cluster analysis of the Te distribution, we delineate the old cores, cratons, weak provinces, and intermediately transitional lithosphere. The distribution of various clusters coincides well with geological settings. Cratonic lithosphere of Asia and Africa are respectively weaker and more fragmented than previously inferred. Moreover, we find global Te is logarithmically correlated with the age of the last orogenic event, indicating that the long-term strength of the continental lithosphere is time-dependent and it can be reset during regional thermotectonic (orogenic) events.


SE14-A011 | Invited
Craton Modification: Recent Geophysical Evidence

Hans THYBO1#+, Irina ARTEMIEVA2
1SinoProbe Laboratory, 2GEOMAR Helmholtz Centre for Ocean Research Kiel

Abundant evidence show that “stable” cratons are modified during their existence, as illustrated in the following examples: The Baltic Shield formed during the Svecofennian Orogeny around 1.7 Ga and its western parts were reworked by the Sveconorwegian/Grenvillian orogeny. Recent geophysical interpretations image a large body of crustal material in eclogite facies beneath the present Moho in the central shield. This body probably formed after the initial cratonisation (Buntin et al., Nature Comm. 2021). The isopycnicity hypothesis proposes that a trade-off between composition and temperature of the lithospheric mantle maintains constant topography in cratons (Jordan, Nature 1978) based on kimberlite data from South Africa. However, gravity data from Siberia shows that kimberlite pipes solely modify cratons in isostatic equilibrium (Artemieva et al., EPSL 2019). Therefore, kimberlite sampling is non-representative, and the real composition of most cratonic mantle lithosphere is unknown. Strong seismic anisotropy is observed in many cratons and is commonly attributed to the mantle due to frozen-in lithospheric features or asthenospheric flow. Recently it was demonstrated that a major part of the anisotropy resides in the crust of the Kalahara craton and that the fast axes are parallel to the strike of major dyke swarms and orogenic fabric (Thybo et al., Nature Comm. 2019). This finding indicates significant craton modification by magmatic intrusion. Modification by external stresses and induced magmatism even may split existing cratons. Integrated interpretation of existing data and geodynamic modelling show that a linear sequence of volcanic harrats in the Arabian craton potentially represents the formation of a new plate boundary (Artemieva et al., Earth Science Review 2022). It is probable that the extension in the northern Red Sea rift will jump to the volcanic lineament, which eventually will develop into new ocean spreading and effectively split the existing craton.


Thu-03 Aug | 8:15 - 10:00 | MR306
SE05 - From Plate Subduction to Intracontinental Tectonics: Natural Observation, Analytical Data, and Numerical Modeling

Session Chair(s): Yu WANG, China University of Geosciences

SE05-A001
Triassic Time-transgressive Sedimentology and Detrital Zircon Record Along the Southwestern North China Block: Insights Into the Tectonic Evolution of Eastern Paleo-Tethys Ocean

Yanhua XU1#+, Dengfa HE2
1China University of Geosciences Beijing, 2China University of Geosciences

Syntectonic sediments directly records the tectonic processes of adjacent orogenic belts. The closing process of the eastern Paleo-Tethys Ocean (EPTO) from east to west remains controversial which sedimentology and provenance -associated clues are powerful approaches for settling. Located in the southwestern North China Block (NCB), the South Ordos Basin (SOB) which preserves the most complete Triassic stratigraphic record on the north of the Qinling Orogenic Belt (QB) is crucial for understanding the coupling between the QB and SOB. In this study, geochronological methods of sedimentology, petrological, and detrital zircon U-Pb were used to study the three parts (eastern, central, and western) of the SOB Triassic sedimentary filling and provenance. Sedimentological analysis identified two periods of fluvial progradation which occurred in the Early Triassic eastern SOB, and the Middle Triassic central and western SOBs (the upper Zhifang Formation to lower Tongchuan Formation). The provenance of the central and western SOB mainly comprised pre-Triassic sedimentary cover in the south NCB and North Qilian during the Middle Triassic, respectively. Since the Late Triassic, provenances from the QB which has a distinct zircon age peak at 1000–900 Ma were mixed. Provenance differences from east to west are also confirmed by the thin section survey and heavy mineral analyses. Regional detailed comparison of these detrital zircon results with published data from Triassic strata in the eastern SOB indicates that the sediments of the SOB deposited influenced by the QB and detritus from the QB appeared from east to west during the Early Triassic to Late Triassic. Time-transgressive provenance shifts and sedimentary filling transition of the three parts of the SOB suggest that the surface of QB underwent an asynchronous onset of uplift beginning from the Early Triassic in the east, propagating westward and reaching its maximum extent in the early Late Triassic.


SE05-A002
Meso-Cenozoic Tectonic Evolution in Eastern China Response to the West Pacific Plate Subduction Processes

Yu WANG#+, Liyun ZHOU, Songnan LIU, Xin CHEN
China University of Geosciences

The timing of events during the Meso-Cenozoic tectonic evolution of the east China region, as well their tectonic settings are still in debated. Extension, compression, transpression, and shearing occurred throughout the eastern China since ~270 Ma. These main structural stages and the temporal evolution of the structural framework and kinematics have been studied, but they are intracontinental tectonics. We present here data from multiple structural and magmatic stages related to temporally varying kinematics and deformation mechanisms during the evolution of the post-convergence of the Yangtze-North China collision and Siberia-North China convergence. The timing of each stage is constrained using isotopic dating, along with the timing of magmatic intrusion, dyke intrusion, and basin formation associated with tectonic transformation of the NE China, North China and South China. Age data indicate distinct structural and magmatic stages at 270–200, 170–155, 130-–110, 75–65, and 25–20 Ma, relating to basin formation and continental uplift or collapse. The tectonic setting and movement direction of adjacent plates changed multiple times during the various stages. The stages are as follows: formation of the Central Asian orogenic belt (CAOB) and northwards subduction of the Yangtze plate, resulting in closure of the Qinling Ocean; the rapid initial formation of the western Pacific plate and subsequent subduction; and final closure of the Mongol–Okhotsk Ocean, combined with closure of the Bangong–Nujiang Suture Zone and southwards movement of the Siberian continent. Moreover, temporal and spatial changes in middle-late Mesozoic-Cenozoic deformation, magmatism, and basin formation, as well as kinematic and mechanical transformations, occurred in response to the changing tectonic setting and movement direction of the west Pacific plate.


SE05-A003
Were Tectonic Evolution and Frameworks on the Northwest Margin of the Sichuan Basin Response to the Paleo-Pacific Plate Subduction?

Songnan LIU#+, Xin CHEN, Yu WANG
China University of Geosciences

Mesozoic is a key period of geographical environmental changes for Chinese continents, as disappearance of oceanic basin and predominant continental sediments. Intracontinental deformation along Longmenshan–Micangshan–Dabashan and conglomerate accumulation in northwestern Sichuan basin recorded two-stage Early Jurassic to Early Cretaceous tectonic events. Structural orientation and sedimentary distribution indicate that the compressive stress is WNW in Longmenshan front belt, and N in Micangshan–Dabashan front belt. These events were considered as the consequences of intracontinental orogeny of Qinling. While Middle–Late Jurassic subduction of the paleo-Pacific Plate played an important role in building the orogens and basins in North China and South China. As mentioned in many publications, the paleo-Pacific plate subducted beneath the Eurasia plate at a very low angle during 180~160 Ma, which could not only act on plate boundary but also create 1300 km wide intracontinental orogen characterized by NNE-trending folds and thrusts. In recent years, it has been proved the force created by the paleo-Pacific Plate subduction can be transferred to the western Ordos Basin and eastern Sichuan Basin. The Longmenshan thrust belt, a NNE-trending transpressional belt formed since Triassic, experienced multi-stage deformation during Mesozoic-Cenozoic. It constitutes the west boundary of Sichuan basin and extend northward to the west boundary of the Ordos Basin. It is close to the area that affected by the paleo-Pacific Plate subduction. Whether it was ever controlled by the paleo-Pacific Plate tectonic domain during 180~160Ma is worth thinking. If so, when did the Longmenshan thrust belt change from Tethys tectonic domain to paleo-Pacific tectonic domain? how was the stress been transferred? In addition, when the change of subduction direction of the paleo-Pacific plate happened and how it affected the framework of Chinese plates? Here, some geological and chronological evidence have been referred to answer these questions.


SE05-A020
Kinematics of Foreland-vergent Crustal Accretion: Inferences from Evolution of Chuanexiang Fold-thrust Belt (South China)

Liang QIU1+, Dan-Ping YAN 2#, Tao YANG 2, Qihui ZHANG2, Wei GAN2, Zhicheng ZHOU2, Bingyan HAN2, Shouheng SUN2, Chang YANG2, Yangfan YUE2
1China University of Geosciences (Beijing), 2China University of Geosciences

Structural and sedimentary records of orogeny in continental lithosphere are essential for deciphering episodic plate subduction. The fold-thrust belt and related sedimentary basins on the overriding plate record the subduction history and continental deformation, providing key clues to reconstruct the geodynamics. The thin-skinned Huayingshan belt and thick-skinned Xuefengshan belt of the Yangtze fold-thrust system in South China block is an excellent natural laboratory. Here, we present fault slip vectors, conjugated joints, and anisotropy of magnetic susceptibility (AMS), and filed geological mapping for the Huayingshan thrust belt and four related Late Cretaceous basins in the northwestern Yangtze fold-thrust system. On the one hand, for the Huayingshan thrust belt, the conjugated joints and fault slip vectors show four stages of paleostress, including D1 N-S shortening, D2 NW-SE extension, D3 NW-SE shortening, and D4 NE-SW shortening. The AMS results exhibit NW-SE shortening, NE-SW shortening, and NW-SE compression during the deposition of the Lower Triassic, the Middle-Upper Triassic, and the Jurassic, respectively. On the other hand, the Jianshi and Enshi half-graben basins are controlled by a boundary normal fault, and the Laifeng and Qianjiang piggy basins developed on the limbs of fault-propagation folds. The tensors of slickensides and joints within the Upper Cretaceous indicate the NW-SE extension and NE-SW extension. The AMS data of the Upper Cretaceous suggest a dominated NW-SE extension and NE-SW extension. Combining these structural data on map view and mesoscopic scale, we propose that the Laifeng and Qianjiang basins formed during the shortening and propagation of Yangtze fold-thrust system and the Jianshi and Enshi basins developed subsequently during extension in the retroarc foreland thrust belt. Thus, we propose that the NW-ward shortening and subsequent NE-SW shortening created the curved Huayingshan thrust belt during the intracontinental orogeny and the tectonic switch potentially records the rollback and delamination of Paleo-Pacific plate.


Thu-03 Aug | 8:15 - 10:00 | MR308
SE06 - Geodynamics of Plate Convergence in Southeast Asia and Coupled Marginal Sea Evolution

Session Chair(s): Jie ZHANG, Second Institute of Oceanography, Ministry of Natural Resources, Zhiyuan ZHOU, Southern University of Science and Technology

SE06-A006
Geodynamic Processes of the Southeastern Neo-Tethys Ocean and the Formation of the Curved Subduction System in Southeast Asia

Weiwei DING1#+, Rixiang ZHU2, Bo WAN2, Xiongwei NIU1, Liang ZHAO2, Pan ZHAO2
1Ministry of Natural Resources, 2Chinese Academy of Sciences

Southeast Asia is located at the intersection of the Tethys and Pacific domains. The superimposed effects of the two tectonic domains have resulted in complicated deep structure, surface magma responses, and dynamic processes of Southeast Asia. Based on the latest long-term passive seismic experiment and numerical modeling, this study reconstructs the dynamic processes of the closure of the Neo-Tethys Ocean and the formation of the Curved Subduction System in Southeast Asia since the Late Mesozoic. P-wave velocity structure shows a remnant of the Neo-Tethys subducted slab in the lower mantle beneath Southeast Asia at a depth of approximately 1500 km. On the Java–East Timor subduction zone, the remnant slab is coupled with the Indo-Australian subducting slab in the upper mantle with the same direction, while on the Sumatra subduction zone, the remnant slab is decoupled from the Indo-Australian subducting slab in different directions. The formation of the Curved Subduction System in Southeast Asia is resulted from the northward subdcutions of previous Neo-Tethys and current Indo-Australian Plate, and the westward subduction of the Pacific Plate since Mesozoic. The former is characterized by continuous subduction and subsequent continental block collision, forming the current continental lithosphere in Southeast Asia and the curve-shaped Sumatra–Java subduction zone; the latter is characterized by subduction retreat and back-arc spreading, forming the eastern Philippine subduction zone and a series of marginal sea basins. Since the Early Cretaceous, the opening of the North Australian Sea resulted in stagnation of the Australian Block in the high latitude area of the southern hemisphere for a long time. The North Australian Sea was dominated by out-dipping double subduction from 45 Ma, which resulted in rapid northward drifting of the Australian Block and final collision with the Sundaland.


SE06-A008 | Invited
Role of Recycled Oceanic Crust in the Mantle of the South China Sea

Xiao-Long HUANG1#+, Yu-Xin CAI2, Yang YU2, Fan YANG3, Yigang XU4
1Guangzhou Institute of Geochemistry, Chinese Academy of Sciences, 2Chinese Academy of Sciences, 3Southern Marine Science and Engineering Guangdong Laboratory (Guangzhou), 4Guangzhou Institute of Geochemistry

Recycling of crustal materials has been considered as the major mechanism for the compositional heterogeneity of the mantle. However, the participation of recycled oceanic crustal components in mantle source of mid-ocean ridge basalt (MORB) may be rather limited. The evaluation of the role of recycled oceanic crust (ROC) in the MORB genesis is crucial for understanding the geochemical recycling process between mantle and crust. Here we present geochemical and petrological evidence for the contribution of ROC to the mantle source of MORBs in the South China Sea (SCS). The SCS MORBs exhibit a large variation in δ98/95Mo values, in contrast to the restricted composition of global MORB. The δ98/95Mo values of SCS MORBs are mostly lower than those of depleted mantle, attributed to the involvement of ROC in their mantle source. The interaction of a mantle plume with stagnant slabs in the mantle transition zone (MTZ) beneath the SCS caused subbasin-scale heterogeneity in the mantle. The ESB MORBs show lower δ98/95Mo values than the SWB MORBs owing to higher proportion of material from the stagnant slabs in the MTZ carried by the mantle plume. In addition, the ESB MORBs show similar decoupled Nd–Hf isotopes to the Pacific MORBs, indicating that the stagnant slabs in the MTZ beneath the SCS are similar to those beneath the NCC. Thus, the overlying upper-mantle region in the SCS might be regarded as the southern part of the big mantle wedge in East Asia. The SCS experienced a rapid transition from continental rifting to seafloor spreading. Thus, continuous subduction occurred prior to and during seafloor spreading allowed significant amounts of subducted crust to be preserved in the upper mantle or as stagnant slabs in the MTZ. Therefore, mantle recycling in marginal sea basins distinctly differs from that occuring in open oceans.


SE06-A022
New Constraints on Cenozoic Subduction Between India and Tibet

Liang LIU1#+, Lijun LIU2, Jason MORGAN3, Yigang XU1, Ling CHEN4
1Guangzhou Institute of Geochemistry, 2University of Illinois at Urbana-Champaign, 3Southern University of Science and Technology, 4Chinese Academy of Sciences

The type of lithosphere subducted between India and Tibet since the Paleocene remains controversial; it has been suggested to be either entirely continental, oceanic, or a mixture of the two. As the subduction history of this lost lithosphere strongly shaped Tibetan intraplate tectonism, we attempt to further constrain its nature and density structure with numerical models that reproduce the observed history of magmatism and crustal thickening in addition to present-day plateau properties between 83˚E and 88˚E. By matching time-evolving geological patterns, we find that Tibetan tectonism away from the Himalayan syntaxis is consistent with the initial indentation of a craton-like terrane at 55±5 Ma, followed by a buoyant tectonic plate with a thin crust, e.g., a broad continental margin (Himalandia). This new geodynamic scenario can explain the seemingly contradictory observations that had led to competing hypotheses like the subduction of Greater India versus largely oceanic subduction prior to Indian indentation.


SE06-A005
Azimuthal Anisotropy Tomography of the Southeast Asia Subduction System

Yuanyuan HUA1#+, Dapeng ZHAO2, Yigang XU1
1Guangzhou Institute of Geochemistry, 2Tohoku University

A detailed 3-D model of P wave isotropic velocity and azimuthal anisotropy beneath SE Asia is obtained by jointly inverting local earthquake arrival times and teleseismic relative travel-time residuals. Our results show that the high-velocity (high-V) subducting Australian slab has penetrated through the mantle transition zone (MTZ) and reached a depth of ∼1,200 km beneath Sumatra, whereas the high-V slab has subducted toward the north and trapped within the MTZ beneath Java. The Hainan mantle plume is revealed clearly as a significant low-velocity anomaly beneath the MTZ, which extends down to the bottom of our model (∼1,600-km depth). The upwelling of the Hainan plume is resisted by the stagnant slab in the MTZ, resulting in divergent fast-velocity directions of azimuthal anisotropy beneath the stagnant slab. The detailed results of seismic tomography and azimuthal anisotropy provide important new information on the complex mantle structure and dynamics of the SE Asian region, in particular, the subducting slabs and the Hainan plume, as well as their interactions.


SE06-A013
Molybdenum Isotopic Constraint from Java on Slab Inputs to Subduction Zone Magmatism

Yang YU1#+, Xiao-Long HUANG2, Sun-Lin CHUNG3, Jie LI1, Yu-Ming LAI4, Iwan SETIAWAN5, Min SUN6
1Chinese Academy of Sciences, 2Guangzhou Institute of Geochemistry, Chinese Academy of Sciences, 3National Taiwan University, 4National Taiwan Normal University, 5Indonesian Institute of Sciences, 6The University of Hong Kong

Mechanism of Mo isotopic variation in arc magmas is still debated. Here we present whole-rock Mo-Sr-Nd-Hf-Pb isotopic data for the Continental Arc Basalt (CAB) and Back Arc Basalt (BAB) from Java, Indonesia, to investigate the role of slab inputs in Mo isotopic variation of the Sunda arc magmatism. The CAB samples have variable K2O contents (0.44–2.49 wt%) and are mainly classified as calc-alkaline series, while the BAB samples are shoshonitic with markedly high K2O contents (2.12–6.90 wt%) relative to the CABs. The Java CABs and BABs have similar Mo isotopic compositions (δ98/95Mo = -0.65 to -0.07‰ and -0.66 to -0.07‰, respectively, relative to NIST SRM3134), suggesting that such a significant Mo isotopic variation should not be caused solely by the isotopic fractionation during the subduction. Instead, δ98/95Mo values of the Java basalts positively correlate with Pb isotopic ratios. This implies that the Mo isotopic variations in the Java arc rocks should result from the metasomatism in the mantle wedge by hybrid agents, including varying proportions of melts from subducted sediments (with heavy Mo isotope) and melts from the subducted altered upper oceanic crust (SAOC) (with light Mo isotope). The light Mo isotope of the Java arc rocks, compared with the Mariana arc basalts, suggests that melts from the SAOC have much lighter Mo isotopic compositions than the components from the lower oceanic crust. The Java CABs show along-arc variations in Mo-Sr-Nd-Hf-Pb isotopes, which is related closely with the thermal status of the subducted slab. Upwelling of the asthenosphere due to the slab tearing beneath the Java arc might have enhanced partial melting of subducted sediments nearby the slab window. The complicated subduction system in the Sunda arc has strongly controlled composition of arc magmas, which changes with input of different subduction components into the mantle wedge along arc.


SE06-A014
The Tearing of the Java Subducting Plate Comes from the Constraints by Earthquake Depth and Surface Bathymetry Data

Pingchuan TAN1#+, Fansheng KONG2
1Second Institute of Oceanography,Ministry of Natural Resources, 2Ministry of Natural Resources

The kinematics and dynamics of a subducting plate change with the increase of the subduction depth, and accordingly this change will cause a deformation of the plate. The tearing of the subducting plate belongs to such deformation, but has been few studied. The Sumatra subduction zone is considered to be an ideal place to study the tearing of the subducting plate, as mantle tomography data have roughly revealed the tearing of the subducting plate, and geochemical data show that the Quaternary largest land crater Toba over the Sumatra subduction zone may also be related to the tearing of the subducting plate. However, the mantle tomography has relative low-resolution and non-uniqueness, whether the tearing of the subducting plate existed has been a subject of debate. In this study, we use more than 40000 earthquake depth to image the configuration of the subduction plate along the Southeast Asian subduction zone from 95°E to 120°E. Along the trench by very 10 km, we make 1707 different profiles perpendicular to the subduction zone. For each profile, the configuration of the subducted plate is indicated by the distribution of the earthquake depth. Our result shows that from northwest to southeast, the maximum depth of the subducted plate gradually increases from 250km to 650km with growing subduction angle from 11° to 50°. However, along the subduction zone at 110°E-115°E, the plate subduction angle is anomalous small with significant uplift of the trenches and shallowing accretionary wedges. This combined with the configuration of the subducted plate suggest that there may be a tearing of the subduction plate at depths of 300-500 km.


Thu-03 Aug | 10:20 - 12:20 | MR306
SE05 - From Plate Subduction to Intracontinental Tectonics: Natural Observation, Analytical Data, and Numerical Modeling

Session Chair(s): Yu WANG, China University of Geosciences, Liang QIU, China University of Geosciences (Beijing)

SE05-A027 | Invited
Partial Melting of Eclogite by Omphacite-breakdown Hinders the Preservation of High Pressure Metamorphic Records on Early Earth

Guibin ZHANG#+
Peking University

Eclogite melting is an efficient mechanism for continental differentiation and growth, but pertinent melt compositions, anatectic reactions, and thermal regimes for this melting are not well documented via natural samples. Here we report the results of detailed petrological, geochronological and geochemical analyses on eclogites and separated leucosomes from the central Himalaya, on which basis we characterize the eclogite melting process. Thermodynamic modeling and zircon geochemistry and Hf isotopes reveal that eclogitization occurred at >2.3 GPa and 770–830 ℃ during 22–18 Ma, and subsequent high-pressure granulite metamorphism took place at 0.9–1.0 GPa and 840–890 ℃ during 17–15 Ma. Two types of eclogite melting reactions are inferred: early muscovite dehydration melting occurred dominantly in the high-pressure domain, and later omphacite broke down during exhumation. The separated leucosomes are characterized by high SiO2, Na2O/K2O, Sr/Y, and low (La/Yb)N and display similar trace elemental patterns with omphacite and decoupled canonical ratios (Nb/Ta, Zr/Sm, etc.) with the eclogite. Integration of the above results, we propose that the subducting Indian crust was eclogitized during the early Miocene and then heated by upwelling asthenospheric mantle through a rupture in the lithospheric mantle, triggering long-lived partial melting (ca. 22−12 Ma). The granulitized eclogites were subsequently accreted to the upper plate and exhumed into the shallow crust, likely via extrusion between deeply rooted out-of-sequence faults (+/− channelized flow). Besides, these findings suggest that partial melting of omphacite hinders the preservation of high-pressure records and can explain the absence of eclogite in Archean metamorphic terranes.


SE05-A044
Prediction of Potassium Host Minerals in Earth's Deep Mantle

Shidong YU#+, Simon REDFERN
Nanyang Technological University

40K is considered one of the major sources of radiogenic heat in Earth’s interior, but is also considered depleted in the mantle. Recently, K is detected in high concentration in a sample from the lower mantle, which indicates K-rich regions might exist as hidden reservoirs in deep Earth. However, it is unclear how K can be hosted in minerals at high pressure, and how they are transported to the deep mantle. In this work, via first-principles calculations and structure predictions, stable K-silicate structures in the K2O-SiO2 binary system are thoroughly investigated up to 130 GPa. Results show that six K-silicate compounds have their stable pressure ranges in the lower mantle, which can act K host minerals in deep Earth. Especially, four compositions are stable in the D'' region, so they could participate in the chemical exchange at the CMB. Density profiles indicate that K could be concentrated in these silicates during subduction and be easily incorporated into upwelling mantle plumes due to high buoyancy. Our results suggest large reservoirs of K in deep Earth and provide insights to the cycling process of K in the mantle.


SE05-A037
Oligocene-miocene Northward Growth of the Tibetan Plateau: Insights from Intermontane Basins in the West Qinling Belt, Nw China

Yipeng ZHANG1#+, Peizhen ZHANG1, Renjie ZHOU2, Weitao WANG1
1Sun Yat-sen University, 2The University of Queensland

Studies of interior basins within the northern Tibetan Plateau provide new sediment accumulation, provenance, paleodrainage, and deformation timing data that enable a reconstruction of the far-field tectono-geomorphic evolution of the rising Tibetan Plateau. Along the northern plateau margin, topographic growth in the West Qinling Belt is inferred to have initiated in the Eocene, coeval with the India-Asia collision, and in the late Miocene. However, geological knowledge about the intervening period remains at present enigmatic, and the kinematics and dynamics are uncertain. To fill this gap, this study presents a multidisciplinary dataset from the intermontane Anhua–Huicheng Basin. Magnetostratigraphic dating, regional mapping, and sedimentological analysis imply that contractional deformation and thrust-top basin systems formed within the West Qinling Belt in the Oligocene (not later than ~24 Ma). A combination of observations including paleocurrent changes, detrital zircon U-Pb age variations, and appearance of growth strata along the Anhua–Huicheng Basin reveal the rapid uplift of the West Qinling Belt at ~15 Ma. Sedimentation in the intermontane basins ended after the late Miocene (~8.0 Ma), when the region experienced intrabasinal deformation, uplift and erosion with the establishment of an external drainage system. Since the late Miocene, the growth of the West Qinling Belt reached a climax with the lack of substantial contractional deformation in Cenozoic sequences heralding the onset of the modern kinematic regime and attainment of high elevation. Observed transitions in the tectonostratigraphy and paleodrainage define different phases of deformation and plateau-wide shifts in stress reorganization, which led to the northward growth and later lateral expansion of the Tibetan Plateau.


SE05-A014
Crustal Eclogitization and Lithosphere Delamination Can Account for the Crustal Extension in Mountain Belts

Jiakuan WAN#+, Huilin WANG
Huazhong University of Science and Technology

Mountain belts are a consequence of crust shortening. It’s accompanied by crust thickening and surface uplift since the rocks undergo negligible or no change in volume. Negative dilatation strain rate and thrust faults are expected to appear in the crust that is shortening, and that is the case in most mountain belts. But crustal extension and normal faults have been revealed by geodetic observations and focal mechanism solutions in some potions of mountain belts, for instance the high Andes, the northern Tibet Plateau and the Honduras depression. Based on the 2-D thermal-mechanical numerical experiments, we have confirmed that crustal eclogitizarion and lithosphere delamination can account for the crust extension in mountain belts. These two process both change the local lithospheric density structure to make influences on crust deformation but in a different way. During lithosphere delamination, dense lithosphere mantle is replaced by light asthenosphere materials to produce positive buoyance that leads to surface uplift and lateral crustal spreading. The max horizontal extension rate appears in the crust blow which the lithosphere mantle just broke away. Eclogitization takes place in the thicken crust root and makes the rocks denser than lithosphere mantle. So, eclogitozed crust root produces negative buoyance that causes local convergence and gathers neighboring crustal materials. In this case, crustal extension does not appear above the crust root but in its vicinity.


SE05-A019
Rheological Properties of Sumatra Subduction Zone Constrained from Postseismic Deformation of the 2004 Mw 9.2 Sumatra and 2005 Mw 8.6 Nias Earthquakes

Siyuan YANG1#+, Yan HU2
1University of Science and Technology of China, 2Deep Space Exploration Laboratory/University of Science and Technology of China

Study on the postseismic deformation following the 2004 Mw 9.2 Sumatra and the 2005 Mw 8.6 Nias earthquakes gains insights to better understand the rheological heterogeneity of the northern Sumatra subduction zone. We have constructed a three dimensional viscoelastic finite element model to model the postseismic deformation following the 2004 and 2005 earthquakes. The model consists of an elastic continental crust and oceanic subducting slab, a viscoelastic mantle wedge, oceanic asthenosphere, and oceanic upper mantle. We also study effects of weakened regions of the spreading center in the Andaman sea and Toba volcano. Stress-driven and time-dependent afterslip is simulated by a 2-km-thick shear zone. We use the biviscous Burgers rheology to describe the viscoelastic relaxation of earthquake-induced stresses in the upper mantle. Test models have determined the mantle wedge viscosity to be 1019 Pa s. A test model with weakened areas in the Andaman spreading center and Toba volcano provides better fit to GPS observations. The viscosity in the shear zone is determined to be 2 х 1017 Pa s. However, the viscosity of the shear zone at the southern edge of the 2005 rupture area has to be as low as 1016 Pa s to better fit the GPS observations in this region. Afterslip of the fault is up to 200 cm within the first year after the earthquake and decays rapidly with time. Afterslip at the 10th year after the earthquake is no more than 10 cm.


Thu-03 Aug | 10:20 - 12:20 | MR308
SE06 - Geodynamics of Plate Convergence in Southeast Asia and Coupled Marginal Sea Evolution

Session Chair(s): Weiwei DING, Ministry of Natural Resources

SE06-A019 | Invited
Electrical Structure Across the Fossil Ridge at the Southwest Sub-basin of the South China Sea

Fan ZHANG1#+, Bo YANG2, Jian LIN3, Tao ZHANG4, Xubo ZHANG2
1South China Sea Institute of Oceanology, Chinese Academy of Sciences, 2Chinese Academy of Sciences, 3Southern University of Science and Technology, 4Ministry of Natural Resources

The southwest sub-basin (SWSB) of the South China Sea (SCS) has a propagative spreading history during ~23 to 16 Ma. Recent studies indicated complex mantle source compositions beneath the SWSB. To better understand the upper mantle structure of the fossil ridge of the SWSB and to test the hypothesis that the evolution of the SCS had been affected by subduction of PCSC, a 120 km long marine magnetotelluric (MT) transect perpendicular to the extinct mid-ocean ridge in the southwest sub-basin of SCS was carried out at September 2021. The recorded time series were processed using a standard robust approach to estimate the MT impedance. By correcting the recorded azimuths, all data are oriented to geographic coordinates. Phase tensor analysis of the MT data shows that the subsurface electrical structure at great depth tend to be three-dimensional (3D). The 3D inversion was thus carried out using ModEM to fit the four complex impedance tensor components. The initial electrical resistivity model shows an obvious high conductive anomaly at a depth of 20-60 km. This anomaly is asymmetrical on the northern and southern of the fossil spreading ridge and mainly located on the southern region, which may represent the asymmetrical spreading signature or relate to the post-spreading volcanism.


SE06-A002
Aftershocks Monitoring of the 2019 Mw5.4 Earthquake Occurred in the Central Basin of the South China Sea

Aiguo RUAN1#+, Xiongwei NIU2,3, WenFei GONG3
1Second Institute of Oceanography, Ministry of Natural Resources, 2Tohoku University, 3Ministry of Natural Resources

On September 5, 2019, a moderate Mw5.4 earthquake unexpectedly occurred in the quiescent central basin of the South China Sea. We immediately carried out a continuously three terms monitoring of aftershocks around the epicenter from October 2019 to October 2010 using five, three and two sets of broadband OBS respectively. Because the main shock epicenter is located at the cross point of “Zhongnan Fault” with the direction turning place of the residual seafloor spreading ridge, and also coincident with the fracture boundary determined by our previous OBS active seismic model. This paper presents the preliminary observation and study results from the three OBS stations (two lost) during the first monitoring term. A total of 21, 68, and 89 micro-earthquakes were picked out from the three OBSs within distance of 30km, respectively. The dominant frequency of micro-earthquakes is 12-15Hz, indicating tectonic fracturing. During the first two months after the main-shock the seismicity is relatively stronger, and micro-earthquakes are still occurring occasionally till the end of observation, indicating the epicenter area is active. The distribution of micro-events has nothing to do with the “Zhongnan Fault”, but is related to the fossil ridge. These micro-events are concentrated in the south of the main-shock epicenter. The depth range of the focal area is relatively large, and it is not clear whether the main-shock in the mantle.(3) Based on teleseismic records and using the method of receiver function and H-κ stacking, we obtained the focal area lithospheric S-wave velocity structure and Poisson’s ratio. The velocity of the deep crust or mantle is relatively large indicates a relatively hard medium, but there is also a low-velocity layer which benefits for earthquake generation. There are differences in lithospheric properties between the north and south sides of the main-shock, which may be the reason why the fossil ridge turns.


SE06-A029 | Invited
Subduction Initiation Along the Flores-Wetar Backthrust in the Sunda-Banda Arc: New Insights from Combined Geodetic and Geophysical Observations

Xiwu LUAN1#, Xiaodong YANG2+, Jian LIN3, Zhiyuan ZHOU4, Liangyu ZHU5, Zhiwen ZHANG6, Xinyuan WEI1
1Shandong University of Science and Technology, 2South China Sea Institute of Oceanology, Chinese Academy of Sciences, 3Woods Hole Oceanographic Institution, 4Southern University of Science and Technology, 5China Earthquake Administration, 6Chinese Academy of Sciences

Initiation of a new subduction zone is a fundamental geodynamic process for Earth’s plate motions. Despite significant advances on the mechanism of subduction initiation (SI) made through natural observations, numerical and physical modelling, the tectonic process, structural deformation of SI and their significance for great natural hazards remain ambiguous. In the east Sunda-Banda arc, the Flores-Wetar backarc thrust, marking the induced subduction initiation by polarity reversal, has hosted several devastating earthquakes and tsunamis, thus affording a great opportunity to address these outstanding SI issues. Here, we combined the seismicity, focal mechanism, GPS velocities, seismic velocity models to investigate the active tectonics and geohazard implications in the Sunda-Banda Arc in light of backarc subduction initiation. Our new results suggest that: (1) the subduction inception began at ~5 Ma along the Flores-Wetar backarc thrust, with a 0.3-4.5 Ma delay from arc-continent collision at ~5.3-9.5 Ma; (2) this new subduction plate has attained >150-km-long and >50-km-deep beneath the Banda arc and just above the early subducted Australian oceanic lithosphere, i.e. no slab breaking off; (3) along strike it propagates westward from north of the Wetar island to the Bali basin with reducing convergence rate from 30 mm/yr to 5 mm/yr at present day, and given such rate, the ~600-km-wide (in N-S direction) Banda Sea will be consumed by subduction in ~20 Ma; (4) the good correlation of high compressional rates and recorded large thrusting events > MW 6.6 reveals considerable earthquake and tsunami threats posed by the new subduction zone to east Indonesia. Future research efforts should be dedicated to study the fault segmentation, seismogenic area, earthquake potential, and tsunami characteristics along the Flores-Wetar thrust so as to provide scientific basis to authorities for mitigating potential large geohazards.


SE06-A001
Heavy Mo Isotope Composition of Northern Bataan Adakites, Philippines: Evidence for Fore-arc Subduction Erosion?

Hai-Quan LIU#+
Guangzhou Institute of Geochemistry, Chinese Academy of Sciences

The identification of eroded fore-arc crust component in arc magmas is challenging due to the combined effects of source contamination in the mantle wedge and crustal contamination in the upper-plate crust. Here we present Molybdenum (Mo) isotope composition in conjunction with Sr-Nd-Hf isotopic and elemental data to identify eroded fore-arc crust components in adakitic lavas from the Cuyapo and Balungao volcanoes of the northern Bataan Segment of the Luzon Arc, Philippines. The δ98/95MoNIST3134 (relative to NIST3134) of these adakites exhibit increase with increasing εNd values and Ba/Nb ratios. The low δ98/95Mo (-0.36 – -0.26‰) of the Cuyapo adakites are associated with unradiogenic Sr-Nd-Hf isotopic ratios, consistent with contributions of remnant slab that had lost isotopically heavy Mo during dehydration at shallow depth. The high δ98/95Mo (-0.18 – 0.00‰) Balungao adakites have Mo isotope composition and radiogenic Sr-Nd-Hf isotopic ratios resembling the Luzon basement. Elevated Nb/Ta and high Sr/Y ratios indicate their parental magmas are in equilibrium with residual rutile and garnet±amphibole assemblages, suggesting a source region (>~45 km) deeper than the present Luzon crust (~33 km). These chemical features thus suggest the heavy Mo of the Balungao adakites are derived from partial melting of eroded crust in the mantle wedge. This study not only demonstrates that Mo isotopes can be a potential tracer of eroded crust, but also highlights the possibility that the combined high δ98/95Mo, εNd and Ba/Nb for arc lavas emplaced at subduction zones with juvenile arc crust can be a result of subduction erosion.


Thu-03 Aug | 1:10 - 3:10 | MR306
SE03 - Earthquakes, Tsunamis and Volcanic Eruptions in History

Session Chair(s): Yasuyuki KANO, The University of Tokyo

SE03-A012
Seismic Activity in Southern Miyagi Prefecture in the 18th Century Revealed from "Takano Family Record”

Sunao URUSHIBARA, Yasuyuki KANO1,1#+, Junzo OHMURA
The University of Tokyo

"Takano Family Record” is investigated to reveal seismic activity in southern Miyagi Prefecture in the 18th century. "Takano Family Record" is a diary recorded by the successive heads of the Takano family between 1696 and 1782 and is included in a published collection of historical documents on earthquakes in Japan. About 150 days of felt records are newly found from our investigation of microfilmed original records kept in the library of the Graduate School of Arts and Letters, Tohoku University. Comparison between the number of felt earthquakes recorded in the "Takano Family Records" that observed by modern observations shows that the author of the "Takano Family Records" recorded earthquakes of JMA seismic intensity 2 or higher, as well as some earthquakes of intensity 1. "Takano Family Records" also contains descriptions of earthquake damage. Location and magnitude of the May 4, 1767, and October 22, 1767 earthquakes are reexamined from distribution of damage and felt records as well as the number of aftershocks.


SE03-A003
Fire Spread Areas and Fire-stopping Points During the 1854 Ansei Nankai Earthquake, Japan

Rena MINAMI#+, Toshitaka BABA
Tokushima University

Earthquake-induced fires are not negligible because they can spread to expansive areas resulting in severe damage. Although many records of fires exist in historical documents, they need to be investigated more. Based on historical documents and drawings, this study attempts to clarify the fires in Tokushima, Wakayama, and Kochi prefectures during the 1854 Ansei Nankai earthquakes. Detailed records of the fires exist in Uchimachi, Komatsushima, Tanabe, Kochi, and Sukumo. The fire in Uchimachi broke out in three places and spread. We identified the two fired houses from the historical drawings. The residences' fences, roads, and rivers prevented the spread of fire. In Komatsushima, a fire broke out in a restaurant. The temple's walls, the river, and the paddy fields prevented the spread of fire. The fire in Tanabe broke out in a collapsed house and spread to a town of lower-class Samurai soldier residences due to the changing wind direction. The drawings show the existence of Tanabe Castle surrounded by moats at that time. The fire stopped at watersides, houses, and roads. In Kochi, a big city consisting of Samurai soldier residences, townspeople, and farmland, a fire broke out in sixteen places. The fire spread and stopped at riversides, houses, and farmlands. The fire in Sukumo broke out in three collapsed houses. We confirmed from the drawings that the city included Sukumo Castle, towns for Samurai soldier residences, townspeople, and farmland. The fire stopped at large houses, farmlands, and loads. We conclude that the houses, loads, farmlands, and watersides worked as fire-stopping points for the fires caused by the 1854 Ansei Nankai earthquake. Kochi had the most severe damage among the investigated cities because of multiple fire outbreaks in a big city.


SE03-A001
The 1923 and Previous Kanto Earthquakes and Future Probability of Occurrence

Kenji SATAKE#+
The University of Tokyo

The great Kanto earthquake (M 7.9) occurred on September 1, 1923, and caused the worst earthquake disaster in Japan with ~105,000 casualties, among which the majority (~ 90 %) were due to fire. The Kanto earthquakes (M~8) occur along the Sagami trough, where the Philippine Sea plate subducts beneath the Kanto region. The penultimate Kanto earthquake, the 1703 Genroku earthquake, caused larger crustal deformation and worse tsunami disasters in the southern Boso peninsula. Historical documents and tsunami deposits indicate that the 1293 Showo earthquake was also a Kanto earthquake (Shimazaki et al., 2011, JGR). The 1495 Meio earthquake, considered to be confused with the 1498 earthquake along Nankai trough, may be another Kanto earthquake. Possibilities of the 878 and 1433 Kanto earthquakes have been also pointed out (Ishibashi, 2020, SRL). Marine terraces on the southern Boso peninsula indicate that the 1703 (Genroku) type earthquake recurred approximately 2,300 year interval. The Japanese government’s Earthquake Research Committee (ERC) annually estimates and announces long-term forecasts, in terms of occurrence probability in the next 30 years. For the M~8 Kanto earthquakes, the probability was estimated as 0 – 5 %, based on historical and geological data, while the Genroku type event was estimated as 0 %. The recurrence interval becomes 209 years for the above six historical events, 261 years for the five (excluding 1433) events, 210 years for the four (excl. 878 and 1433 or 1495) events, and 315 years for three (1923, 1703 and 1293) events. The occurrence probabilities in the next 30 years vary from 0 to 12 % for the Brownian Passage Time model, and 9 to 13 % for the Poisson model.


SE03-A004
Tsunami Source of the 1946 Showa Nankai Earthquake Estimated by Nonlinear Tsunami Inversion Algorithm

Masato KAMIYA#+, Toshitaka BABA
Tokushima University

This study proposes a complete nonlinear inversion method for tsunami trace heights by repeatedly solving nonlinear long-wave equations using a high-performance computer and the Levenberg-Marquardt method. We applied the new nonlinear tsunami inversion to estimate the fault slip during the 1946 Nankai earthquake. We created eight subfaults referring to the N3 and N4 seismic segments in Annaka et al. (2003). The tsunami calculation used the nonlinear long-wave equations on three topographic nesting layers gridded by 18, 6, and 2 arc-sec intervals. The integral time was 3 hours with a time width of 0.1 s. Observed tsunami height stemmed from a database of Tohoku University. In the iterative inversion, we used highly reliable data (rank A) higher than 50 cm above the sea level and less than 100 m run-up distance. The total number of tsunami trace heights was 122. The geometric mean K and the geometric standard deviation κ from Aida (1978) indicated a degree of fitting. We also calculated the residual sum of squares between observation and calculation in the tsunami heights. Our obtained fault model showed a larger slip than the models previously proposed in the region off Shikoku and Kii Channel, with a maximum slip of 7.2 meters. The seismic moment was calculated to be 6×10^21 (N-m), which is higher than the 3.5×10^21 (Nm) in Baba et al. (2005) and comparable to the 7×10^21 (Nm) in Annaka et al. (2003). Our new slip model of the 1946 Nankai earthquake explained the observed tsunami heights well. The K-κ and the residual sum of squares for the calculated values and trace heights were 0.99-1.26 and 43.8 m^2, while Annaka et al. (2003) model, these were 1.08-1.37 and 82.6 m^2.


SE03-A006
Seismic Risk Assessment of Selected Ancient Monuments in Bagan / Nyaung U Area, Myanmar

Aung Kyaw MYAT#+
Myanmar Engineering Council

When the remarkable damage on monuments in Bagan City after 2016 Chauk Earthquake has been occurred, the research project on the seismic hazard and vulnerability assessment for Bagan/ Nyaung U area of Myanmar was conducted as Phase I work and a report was issued by Technical Expert Team (TET) in 2019 September. As a continuation of that research project, the seismic risk assessment of some selected ancient monuments in Bagan City, is being conducted as the phase II of the project by a team led by Myanmar Engineering Council with the collaboration of Department of Archaeology and National Museum (DOANM) Myanmar. The selection of monuments depends upon typology, configuration, seismicity and soil condition. The nine selected monuments are proposed and computations are carried out with the following methodology. Step (1) Rapid Visual Screening Step (2) Investigation of Material Properties Step (3) Structural Assessment Step (4) Modelling and Analysis Step (5) Safety Assessment Three types of structural analysis were performed on the selected temple in order to explore the structural behavior. They are (1) Gravity load analysis (2) Modal analysis to identify the dynamic parameters and (3) Transient analysis to characterize the earthquake behavior. In the above analysis, the Ansys Software (Version 18.2) has been used and the input data for the said software were produced by means of Revit Software (Version 2023) in order to have 3D drawings. By reviewing the analysis results, the vulnerable portion of the monuments can readily be defined and the strengthening work can be considered for different hazard levels. The behavior of the different monuments with different hazard levels can be determined and the various strengthening methods can be considered for critical parts of the monuments. [1] Prof Aung Kyaw Myat, Ph.D, President of MEngC [2] Thet Mon San, Ph.D, Senior Technical Engineer, HPBC, Myanmar.


SE03-A018
New Evidence of Earthquake Induced Liquefaction Features in the Meizoseismal Area of 1897 Shillong Earthquake, India

Md.Mujahed BABA1,2#+, Laksmi BV1, Deenadayalan K1, Rokade V.M.2, Patil S.N.2
1Indian Institute of Geomagnetism, 2Kavayitri Bahinabai Chaudhari North Maharashtra University

In an alluvium covered seismically active region, constraining the paleoseismic events using liquefaction features in the suitable landform is challenging. The suitable landforms, known history and chance discovery of liquefaction features in young stratigraphic horizons are crucial. The article presents the new evidence of the presence of liquefaction features and their utility in assessing the paleoseismicity of the region around Krishnai and Dudhnai rivers, lying to the north of SP, India. The study aims to locate, characterize and assess their significance as indicators of palaeoseismicity. Paleoseimological field investigations were carried out in the meizoseismal areas of great 1897 Shillong earthquake (M 8.3) in order to understand seismic hazard and past seismic history through documentation of liquefaction features. The trenches excavated at eight locations revealed extensive liquefaction features with multiple sand dykes. The studied sections show evidences of extensive liquefaction at ~2-3 m depth from the ground surface in highly saturated sand-silt column in the point bar deposits of Krishnai and Dudhnai rivers. The sections show multiple tabular sand dykes along with interconnected patches of coarse brown sand. These deformation features are potential evidences of past seismicity and point to the occurrence of seismic events of magnitude ≥5.


Thu-03 Aug | 1:10 - 3:10 | MR308
SE01 - Geodynamic and Metallogeny of Asia Oceania Region: Critical Metals and Precious and Base Metals Resources

Session Chair(s): Khin ZAW, University of Tasmania, Jillian Aira GABO-RATIO, University of the Philippines Diliman

SE01-A009 | Invited
Preliminarly Study on Mineralogical Characteristics of the Heavy Sulfide Zone at the Grasberg Porphyry Cu-Au Deposit, Papua, Indonesia

Kotaro YONEZU1#+, Shunnosuke OMACHI1, Thomas TINDELL1, Adrian BOYCE2, Euis Tintin YUNINGSIH3, Mega Fatimah ROSANA3
1Kyushu University, 2Scottish Universities Environmental Research Centre, 3Padjadjaran University

The Grasberg deposit, one of the largest porphyry Cu-Au deposits in the world is located at Papua Indonesia. Porphyry mineralization is closely associated with Pliocene intrusive rocks, Grasberg Igneous Complex (GIC). GIC mainly consists of Dalam Intrusion (DI), Main Grasberg Intrusion (MGI) and Kali Intrusion (KI). In addition, another mineralized zone, Heavy Sulfide Zone (HSZ) is developed at peripheral zone of porphyry Cu-Au mineralization. The mineralization characteristic and formation timing has not yet well studied, therefore, we focus on the mineralization at HSZ in this study. To achieve the objectives, petrography and trace elements in sulfide and sulfur isotope study were conducted. Copper mineralization styles included in HSZ are dissemination and vein. The dominant ore minerals in both types are chalcopyrite and bornite. Chalcopyrite coexists with bornite as a result of exsolution from bornite solid solution. Pyrrhotite typically formed under low sulfidation state was observed with pyrite and chalcopyrite. Covellite, chalcocite and digenite were precipitated along the fracture of pyrite vein. In addition, native gold is present with covellite, suggesting that it was remobilized and precipitated by retrograde cooking during mineralization. Ore mineral assemblage observed in HSZ was three stages. First one is porphyry copper type mineralization formed at higher temperature and sulfur fugacity characterized by chalcopyrite and bornite. Second one is characterized by pyrrhotite and minor native gold under relatively low temperature and sulfur fugacity conditions. Third one is retrograde cooling stage of the mineralization by Cu-Fe sulfide and native gold (the highest gold grade among 3 stages by remobilization). Those 3 stages observed at HSZ may be linked with main Cu-Au mineralization at around GIC.


SE01-A010 | Invited
Geology and Genesis of the Bonanza-Sandy Epithermal Vein System, Masara Gold District, Mindanao, Philippines

Jillian Aira GABO-RATIO1#+, Alfred Elmer BUENA1, Barbie Ross VILLAPLAZA1, Betchaida PAYOT1, Carla DIMALANTA1, Karlo QUEANO2, Eric ANDAL3, Graciano Jr. YUMUL4
1University of the Philippines Diliman, 2Mines and Geosciences Bureau, 3Itogon-Suyoc Resources Inc., 4Cordillera Exploration Company, Inc.

The Masara Gold District in southern Philippines has a long history of gold production since its discovery in 1937. It is located in caldera structures within the dilational jog of the Philippine Fault Zone in southeastern Mindanao island. This study documents the geologic characteristics of the NW-trending Bonanza-Sandy epithermal veins from underground exposures to constrain the metallogeny of the gold mineralization.
The epithermal veins are largely confined along the NW-trending Masara Fault Zone. They are hosted by Eocene clastics, Early Miocene quartz diorite, and several Late Miocene diorite phases. Wall rocks adjacent to the veins are altered to muscovite, illite and chlorite. Epithermal mineralization in the NW veins is divided into three main stages: Stage 1 characterized by massive quartz-sulfide veins with chalcopyrite, pyrite, sphalerite and galena; Stage 2 consisting of massive to open-space fill quartz-carbonate veins; and Stage 3 distinguished by colloform-crustiform to cockade-brecciated quartz-rhodochrosite veins with sphalerite, galena, pyrite and chalcopyrite. Stage 1 is the main gold mineralization phase, with gold and tellurides associated with the sulfides while Stage 3 contains invisible gold in the sulfides. The minimum mineralization age is Early Pliocene (5.12±0.16 Ma) determined from K-Ar dating of illite separates from the diorite porphyry host rock.
The magmatic arc setting, dominant chalcopyrite-pyrite mineralogy, muscovite-illite-chlorite alteration, and sphalerite compositions of 2.26-8.72 mol% FeS in Stage 1 and 0.55-1.13 mol% FeS in Stage 2 point to intermediate sulfidation mineralization characteristics. The Bonanza-Sandy veins were formed from hydrothermal fluid that was probably exsolved from the Late Miocene intrusive rocks and precipitated in the NW-trending, NE-dipping Masara Fault Zone. The influence of magmatic-hydrothermal fluid and its further cooling and mixing with meteoric waters, along with fluid boiling, are inferred to be the primary ore-forming mechanisms responsible for the formation of the epithermal veins in the Masara Gold District.


SE01-A004
Fluid Inclusion and Ore Mineralogy Study of the Phayaung Taung Deposit, Mandalay Myanmar

Naing Aung KHANT1+, Heejung KIM1#, Chungwan LIM2
1Kangwon National University, 2Kongju National University

Myanmar is gifted with a wide variety of metallic and nonmetallic mineral reserves, some of which have lately been developed as world-class mines. Phayaung Taung Gold deposit is located within the Slate Belt and Chaung Magyi Group. The Phayaung Taung gold deposit from the Slate Belt is hosted in phyllite, schist, and quartzite. Phyllite and Quartzite are the most important stratigraphic units in the Phayaung Taung gold mine area. Phyllite and Quartzite are the most important stratigraphic units in the Phayaung Taung gold mine area. Gold is not related with silver minerals and mostly occurs with Chalcocite and covellite. Gold in the Phayaung Taung is from the secondary origin and is formed mostly in the sulfide ore stage. Gold occurs in tourmaline-quartz and sulfide-bearing quartz veins. There is also an additional paragenetic oxide ore stages of Iron Oxide and Titanium Oxide which is not connected to gold formation. The Phayaung Taung fluid inclusion system contains a lot of bi-phase liquid rich inclusions. The melting temperature of the Phayaung Taung is -2.26 to -9 °C, while the homogenization temperature is 225-450 °C. And the salinity level ranges from 3.39 to 12.85 wt.% NaCl equivalent. The TmCO2 of these inclusions are fixed at -49°C and ThCO2 is 28 to 29°C even though the standard TmCO2 should be at -57°C. The Raman analysis of the CO2 inclusion show that there is no water content inside the bubble and the density of the CO2 inclusion are ranging from 312.1881 kg/m³ to 302.8516 kg/m³. Field nature and the characteristics of fluid inclusions are showing that Phayaung Taung deposit is the mesothermal (orogenic-gold deposit) type.


SE01-A002 | Invited
Two-stage Metallogenic Model of Sediment-hosted/orogenic Gold Deposits in Sibumasu Terrane

Khin ZAW#+, Charles MAKOUNDI
University of Tasmania

The Sibumasu Terrane in mainland SE Asia encompasses western Thailand, western Peninsular Malaysia, and eastern Myanmar and is bordered by the Sagaing Fault in the west in Myanmar and the Inthanon Terrane to the east in Thailand. The sediment-hosted/orogenic gold deposits are widely distributed in the Sibumasu Terrane (Khin Zaw et al., 2014; Makoundi et al., 2023). These gold deposits are hosted in relatively undeformed and unmetamorphosed carbonaceous and calcareous sedimentary rocks to highly deformed metamorphic rocks of the mostly Phanerozoic. They are largely confined to fold belts (e.g., Huai Kham On, Langu in Sukhothai fold belt, Thailand) and in/near suture zones (e.g., the Selinsing, Tersang, and Penjom in Bentong-Raub Suture, Malaysia). Major orogenic gold deposits also occur along crustal-scale faults/sutures in Myanmar (e.g., Kyaukpahto, Phayaung Taung, Modi Taung, Shwegyin, and Meyon deposits) (Khin Zaw et al., 2017). Geochemical, mineralogical, and pyrite trace element studies of the Sediment-hosted/orogenic gold deposits in SE Asia show that the ore formation process can be explained by a two-stage model which is very similar to many well-known sediment-hosted gold deposits around the world (Large et al., 2011). Due to the rapid and massive uplift and erosion in the India–Himalaya–Asia region, facilitated by pulses or cycles of oxygenation of the earth's atmosphere, accumulation of gold in diagenetic pyrites occurred together with other redox-sensitive trace elements such as Mo, Ni, As, and V trapped in organic muds in continental-derived sediments such as black shales or carbonaceous shales at the margin of Sibumasu terrane. The second stage involves subsequent subduction of the terranes associated with repeated and widespread metamorphic–magmatic processes associated with collision–accretion and structural deformation that released gold–arsenic-rich metamorphic fluids in favorable structural sites. We suggest that this two-stage model may have important implications for mineral exploration.


Thu-03 Aug | 1:10 - 3:10 | MR336
SE13 - Seismic Hazard and Risk Assessments: Observations, Models, and Applications

Session Chair(s): Kazuyoshi NANJO, University of Shizuoka

SE13-A015
Parameter Selection for Extracting Statistical Periodicity from Origin Time of Earthquakes

Jinbo ZHENG1+, Jinhai ZHANG2#
1Chinese Academy of Sciences, 2Institute of Geology and Geophysics, Chinese Academy of Sciences

The catalog of earthquake is important for analyzing the potential seismic periodicity. Natural earthquakes are randomly recorded; thus their origin time of occurrence needs to be regularized to generate evenly sampled data sets for extracting statistical periodicity. A small sampling interval would bring many samples, which is helpful on improving the resolution of statistical analyses. However, a too-small sampling interval would result in many null values, which might introduce numerical artifacts. Thus, an appropriate selection of time interval is critical for statistical analyses on the catalog of earthquakes. However, such topic has not been fully discussed, limiting the resolution of the statistical analyses. Here, we propose a method on time interval selection based on time-frequency analysis and spectral superposition. First, we validated the proposed method with synthetic data containing periodic signals and strong random noise with extra added zero values. Then, we illustrate the reliability of the proposed method in extracting weak periodicity from a strong noise. Using this method, we analyzed the catalog of M1.0+ earthquakes in Japan observed since 2002 by the Japan high sensitivity seismograph network (Hi-net). We found that the minimum time interval for the presence of daily period for M1.0+ and M2.0+ events was ~10 minutes, and that there is no noticeable periodicity in the M3.0+ an M4.0+ events due to the small number of earthquakes. This work provides a reference for the selection of optional parameters in statistical seismology studies. The observed higher-resolution diurnal periodicity of earthquakes at smaller time intervals verified the existence of the diurnal earthquake periodicity in Japan.


SE13-A011
A Preliminary Report on Evaluating Online Seismicity: A Demonstration Experiment Using the Space-time ETAS Model

Kazuyoshi NANJO#+
University of Shizuoka

Among candidate space-time ETAS (Epidemic Type Aftershock Sequence) models, the hierarchical version of the model (HIST-ETAS model, or the Hierarchical Space-Time ETAS model) has been intensively studied (Ogata, 2011, 2022). One of the features of this model is its ability to implement space-time forecasting of history-dependent seismicity rate based on a previously defined time frame. This computer-program package is publicly available and open source (Ogata et al., 2021, https://www.ism.ac.jp/editsec/csm/index.html). Using this package, a demonstration experiment to evaluate online seismic activity is currently underway. Two experiment regions were employed: the first included all of Japan while the other only included the Nankai trough. The following three steps are being performed daily by automatic processing. (1) The creation of a catalog that consists of earthquakes that occurred until the day prior to the iteration, by extracting necessary information from the webpage of the Preliminary Catalog using the Hi-net (High Sensitivity Seismograph Network) Automatic System of the NIED (National Research Institute for Earth Science and Disaster Resilience, https://www.hinet.bosai.go.jp/?LANG=en). (2) Processing the output of various calculation results based on the input of earthquake information in the catalog created in (1) by the software package programs. (3) Automatically posting, on Twitter, figures that show the resulting output from the process in (2). Given that the experiment in ongoing, the Twitter account has been set to private mode and followers, including the author, follow this Twitter account. In this preliminary report, an overview of the ongoing demonstration experiment will be provided. Acknowledgments: The author thanks Y. Ogata and J. Zhuang for discussion, and Y. Noda for help with the experiment's automatic processing. This study was partially supported by the MEXT of Japan, under the STAR-E (Seismology TowArd Research innovation with data of Earthquake) Program (Grant Number JPJ010217), and Chubu Electric Power's research based on selected proposals.


SE13-A020
Seismic Hazard Potential in New Zealand: New Insight from Geodetic and Seismic Moment Rates

Neha CHOUDHARY1#+, Sumanta PASARI1, Yogendra SHARMA2, Kuo-En CHING2
1Birla Institute of Technology and Science, Pilani, 2National Cheng Kung University

For seismic hazard analysis, the comparison between geodetic moment accumulation and seismic moment release is one of the key parameters for quantifying the high seismic potential areas in a tectonically active region. The present study aims to evaluate the crustal deformation caused by the contemporary earthquake cycle and consequent seismic hazard potential in New Zealand. For this, we applied the state-of-the-art seismic-moment-budget-estimation technique to quantify the earthquake potential along 14 different segments in New Zealand. In this regard, the geodetic and seismic moment rates for each segment are calculated and compared. The geodetic moment rates are calculated from the geodetic strain field estimated through the updated velocity field of about 180 continuous GPS stations, whereas the seismic moment rates are computed from the earthquake data of ~180 years. A comparison of these two rates reveals segment-wise total energy budget that could possibly release in future devastating earthquakes. The emanated results show that (i) the geodetic strain field has a dominant compressional rate (0–75nstrain/yr) rather than extensional rate (0–30nstrain/yr) along the Alpine fault; (ii) the higher value of the maximum shear strain rates (~225nstrain/yr) is aligned to the northeastern boundary of the South Island; (iii) the estimated geodetic moment rate ranges between 3.15*1017–9.00*1017Nm/yr, whereas the seismic moment rate lies in the range between 0.10*1017–83.92*1017Nm/yr and (iv) finally, based on the comparison between the segment-wise moment accumulation and the moment release rates, the possible maximum earthquake potential of 14 segments in New Zealand varies between Mw6.7–8.0. In essence, the spatial distribution of seismic moment budget in New Zealand suggests that segments with high seismic potential indicate the areas of interseismic strain accumulation, whereas segments with lower earthquake potential correspond to the areas encompassing the rupture areas of recent large events.


SE13-A010
Seismic Hazard Function (SHF) Study Prior to Large Earthquake Event Along Off Coast of the Sumatra Island: The SHF Analysis Based on the Change of the B-value

Wahyu TRIYOSO#+, Joshua B. KURNIAWAN
Bandung Institute of Technology

The seismic hazard function analysis around the off coast of Sumatra Island is investigated based on the changes of the b-value using the shallow crustal earthquake catalog data. The study areas are analyzed around the large earthquake events that took place from 2000 to 2010. The change of the b-value is estimated using the maximum likelihood method with a constant number. First, the b-value surrounding the center area of interest with a radius of about 150 km is calculated based on the earthquake catalog data from 1963 to 2016 (b50). Second, the b-value based on five years with a one-year moving window (b5) is estimated before the large earthquake event from 2000 to 2010. The b5 is calculated based on the constant number of events of 25, 50, 75, and 100, and we evaluate the mean b-value. Furthermore, the SHF of b50 and b5 are calculated, and then they are compared. The results showed that the Probability of Exceedance (PE) of SHF b5 increased by at least about five years before the large earthquake events. Therefore, the results obtained in this study might be very beneficial for earthquake mitigation and modeling efforts for the possible potential of the earthquake hazard study and future analysis.


SE13-A016
Analysis of Multichannel Analysis of Surface Wave Measurement in Samosir Island

Pupung SUSILANTO#+, Supriyanto ROHADI, Thomas HARDY, Retno Agung PRASETYO KAMBALI, Arif Rachman HAKIM, Asep NURACHMAN, Angga Setiyo PRAYOGO, Rahmat Setyo YULIATMOKO, Suko Prayitno ADI, Dwikorita KARNAWATI
Indonesian Agency for Meteorology, Climatology and Geophysics

Samosir is an island in Lake Toba that has high tourism development. Its position on the island of Sumatra makes Samosir Island potentially dangerous from seismicity. Therefore, mitigation efforts are the main thing to reduce the impact of an earthquake. One of the mitigation efforts is to determine the shallow subsurface conditions using the shear wave velocity analysis approach of 0-30 m or Vs30. The Vs30 parameter was obtained from 31 data point measurements using the multichannel analysis of surface wave (MASW) method on Samosir Island. MASW Measurements using the Doremi Seismograph with 24 geophones with a geometry measurement of 5 m offset distance and 2 m spacing between geophones to reach an estimated depth of 30 m. The results of MASW processing obtained Vs30 values ​​between 125–774 m/s, with the dominance of the measurement area being soft soil types and medium soil types. The distribution of soft soil and stiff soil is in the coastal district. Pangururan, Palipi, Onan Runggu, and Nainggolan. This area is thought to have relatively thicker sediments and is an area that has the potential to experience stronger shocks when an earthquake occurs.


SE13-A014
Site Characterization of the Chiang Rai Basin, Northern Thailand

Passakorn PANANONT1#+, Kasian PRASERTWONGPHILAI1, Koichi HAYASHI2, Kevin P. FURLONG3, Patinya PORNSOPIN4
1Kasetsart University, 2Geometrics Inc., 3Penn State University, 4Thai Meteorological Department

Chiang Rai province in northern Thailand has high seismic hazard compared to other parts of Thailand with regions devastated by the M6.2 Mae Lao earthquake in 2014. This work studies the site characteristics of the Chiang Rai basin by measuring the ground response using seismic microtremor measurement and shear wave velocities using the spatial autocorrelation (SPAC) method from seismic ambient noise. The ground response measurements provide the short and long-period ground response of 0.07-1.00s and 1.00-3.98s respectively. Except in the Mae Sai basin, the ground responses of most areas in Chiang Rai province have elevated short period response which will affect the shaking of the short structures such as residential houses in the event of an earthquake. Shear wave measurements at 120 sites in Chiang Rai province indicate that the Vs30 varies from 193-700 m/s which can be classified as soil type classes D (stiff soil) and C (very dense soil and soft rock) based on the National Earthquake Hazards Reduction Program’s soil type classification. Combining the Probabilistic seismic hazard analysis return periods of 475, 950, and 2475 years for the Chiang Rai province with the new Vs30 from this work suggests that the expected PGA is between 0.369g-0.797g which is 20-45% higher than those of the previous studies that assumed the rock ground characteristics; the Spectral Accelerations (SA) calculated with the new Vs30 increase by 20-300%. The result will be integrated into the production of the national seismic hazard map of Thailand in the future.


Thu-03 Aug | 3:30 - 5:15 | MR306
SE03 - Earthquakes, Tsunamis and Volcanic Eruptions in History

Session Chair(s): Kenji SATAKE, The University of Tokyo, Javed MALIK, Indian Institute of Technology Kanpur

SE03-A007
Decamillennial Timescale of Quaternary Large Earthquakes Cycles Along the Yuguang Graben Fault of Northern Shanxi Grabens

Peng HUI1+, Wenjun ZHENG1#, Shaopeng DONG2, Qiyun LEI2, Haiyun BI3, Xulong WANG4, Dongli ZHANG5, Xinnan LI2, Zhikang GONG1
1Sun Yat-sen University, 2China Earthquake Administration, 3Institute of Geology, China Earthquake Administration, 4Chinese Academy of Sciences, 5中山大学

Excavations of deposits related to paleoseismic events in the boundary zones of active tectonic blocks are crucial for the forecast and hazard assessment of strong earthquakes. The Yuguang Graben, situated in the northern Shanxi Grabens (the eastern boundary of the Ordos Block), has formed a significant quantity of fine Quaternary fine sediments, which are beneficial to paleoearthquake research. However, investigation of paleoearthquakes on the Yuguang Graben Fault (YGF) is limited. In this study, we excavated a trench on terrace T2 of the YGF and obtained fine-structure photographs of the profile by LiDAR. Based on optically stimulated luminescence dating of colluvial wedges, we identified at least four strong paleoearthquakes on the YGF (> 77.6 ± 5.1, 63.9 ± 5.1, 51.0 ± 4.3, and 37.3 ± 0.3 ka). Combining our results with previous studies, we interpreted seven paleoseismic events corresponding to the characteristic earthquake model with an average recurrence interval of 11.5 ± 2.8 ka and a coefficient of variation of 0.25 since the late Pleistocene. Furthermore, we obtained the quantified slip rate at the Maizituan site based on field investigation, topographic surveying, and optically stimulated luminescence dating, and reconstructed the slip rates along the fault since the late Pleistocene based on previous studies. The results show an increasing fault slip rate that corresponds to a decrease in the earthquake recurrence interval from the late Pleistocene to the Holocene. The elapsed time since the most recent large earthquake is close to that of a recurrence cycle. Moreover, existing paleoearthquake studies in the northern Shanxi Grabens show that seismic behavior along the block boundary tends to be clustered, and seismic activity along the YGF may be influenced by neighboring faults. Our findings suggest a high risk of an imminent large earthquake along the YGF.


SE03-A009
Building the Paleo-seismic History of the Allah-bund Fault, Great Rann of Kachchh, Western India

Nayan Kirpashankar SHARMA1#+, Mahendrasinh GADHAVI2, Rabiul BISWAS1, Kenji SATAKE3, Eshaan SRIVASTAVA1, Mitthu DHALI1, Javed MALIK1
1Indian Institute of Technology Kanpur, 2L. D. College of Engineering, 3The University of Tokyo

The Kachchh rift basin, located in the western part of India, was formed during the early Jurassic and is now passing through the rift reversal phase from extension to compression regime in response to the compressive stresses active on the Indian plate after the Himalayan collision. Although being part of the Stable Continental region (SCR), the Kachchh basin has hosted several moderate to large magnitude earthquakes, including 1668 CE (Mw 7.0), 1819 CE (Mw 7.8), 1845 CE (Mw 6.3), 1956 CE (Mw 6.0), and 2001 CE (MW 7.7). Out of these, the Great Rann of Kachchh Allah-Bund earthquake in 1819 CE is the second-largest earthquake in the SCR. The 1819 earthquake not only created a 90-km long scarp but also disrupted the flow of rivers that previously used to flow through the Great Rann of Kachchh (GRK) and changed the overall landscape of the region. However, Great Rann's seismic history and the earthquake-related primary deformation have not yet been precisely documented. This study aims to investigate the paleo-seismic signatures and the tectonic forcings prevailing in the GRK region. A detailed tectono-geomorphic map was prepared using the remote sensing dataset, and the geomorphic markers were identified. A river section on the Allah-Bund scarp was excavated and analyzed thoroughly, and three events were identified. Out of these three events, two events are interpreted as secondary deformation caused due to the earthquake from a nearby source, and one is identified as primary deformation due to the earthquake triggered on the Allah-Bund Fault. Total 8 sediment samples were collected from the section for Optically Stimulated Luminescence (OSL) dating. Sample ages will suggest whether the Allah-Bund scarp has resulted from a single 1819 event or multiple past seismic events. Thus, this study answers the question regarding the region's seismic history and earthquake-related primary deformation.


SE03-A010
Surface Rupture Evidence of the Great Medieval Earthquake Along the Himalayan Frontal Thrust: Inferences from Paleoseismic Studies, Kumaun, Central Himalaya

Mitthu DHALI1#+, Javed MALIK1, Eshaan SRIVASTAVA1, Nayan Kirpashankar SHARMA1, Mahendrasinh GADHAVI2, Gurvinder SINGH3
1Indian Institute of Technology Kanpur, 2L. D. College of Engineering, 3Panjab University Chandigarh

One of the seismically active mountain belts in the globe, the Himalayan orogenic belt, accumulates strain during the interseismic period and releases it during an earthquake. Some of the largest continental earthquakes in the world have occurred there just in the past century. The recent earthquake in Gorkha in 2015 casts doubt on our knowledge of Himalayan earthquakes. Greater Himalayan earthquakes may have ruptured the frontal part in recent and medieval periods. The Central Himalaya has undergone several significant earthquakes throughout recorded history, several of which occurred in the medieval era. There exist large uncertainties in determining the most recent surface rupturing event in the Central Himalaya. The great earthquake of CE 1505 and the most recent one, which occurred in CE 1803, significantly impacted the region. However, there is a debate among the scientific community over the surface rupture of the CE 1803 earthquake and the spatial extent of the great CE 1505 earthquake in the kumaun region. This study mainly focuses on understanding past earthquake activity and the uncertainty associated with them in the Kumaun region of Central Himalaya. We have mapped river terraces, fan surfaces, and fault scarps exposed in the region using CARTOSAT-1 and UAV to generate a high-resolution DEM to get a 3D view of the terrain. We excavated a trench on a 15-20 m uplifted alluvial fan surface along the Himalayan Frontal Thrust (HFT) in Haldwani, Kumaun (Central) Himalaya and collected 27 samples from different lithounits for Optically Stimulated Luminescence (OSL) dating and 15 Charcoal samples for Radiocarbon dating. Furthermore, we have collected samples for OSL dating from the region's older alluvial fan surfaces, river terraces, and fault scarps. The sample from the trench and the terraces suggest evidence of the surface rupture of the great 1505 AD earthquake from this region.


SE03-A008
The Temporal-spatial Distribution of Global Tsunamigenic Volcanoes

Kan ZHANG+, Linlin LI#, Gui HU, Xiaoyi PAN
Sun Yat-sen University

Volcanoes, as an atypical source of tsunamis, have received little attention, yet the tsunamis they trigger can cause tremendous losses locally and even affect global seas. Due to the complexity of the tsunami-triggering mechanism of volcanoes and the wide range of disciplines involved, further research is still needed on the characteristics, theoretical research and disaster assessment of volcanic tsunamis. Here, we review multiple disaster databases, including NOAA tsunamis and volcanoes, as well as information of the Global Volcanism Program, and sort out the global historical volcanic tsunami events. According to the geographical overview, geological structure and historical records of volcanic tsunamis, we divide the potential tsunamigenic volcanoes into eight regions globally. We summarize the generation mechanisms of past volcanic tsunami events into five categories: volcanic earthquake, volcanic structure instability, underwater explosion, pyroclastic flow and atmospheric pressure wave. Through a careful analysis of the eruption level, triggering mechanism, and geographical locations of past volcanic tsunami events, we propose several criteria which could be used to classify the tsunamigenic potential of volcanoes. Based on the criterion, we point out a list of volcanoes, such as lle des Cendres islands, Ly Son volcano islands and volcanoes with large-scale eruption potential on the Philippine Island arc and Indonesian Sunda arc could be potentially tsunamigenic and pose great threat to the South China Sea and its surrounding regions. Finally, we assess the potential tsunami hazard triggered by lle des Cendres volcano island on the nearby coast using a numerical approach.


Thu-03 Aug | 3:30 - 5:15 | MR308
SE01 - Geodynamic and Metallogeny of Asia Oceania Region: Critical Metals and Precious and Base Metals Resources

Session Chair(s): Naing Aung KHANT, Kangwon National University, Khin ZAW, University of Tasmania, Jillian Aira GABO-RATIO, University of the Philippines Diliman

SE01-A003
Ore-forming Conditions of the Kematu Epithermal Deposit, T’boli, Philippines: Insights from Ore, Alteration, and Sulfur Isotope Compositions

Alan Royce TIZON1#+, Jillian Aira GABO-RATIO1, Ma. Yna Rose GARCIA2, Juan Alex Vianne AMOROSO3, Pearlyn MANALO4, Ryohei TAKAHASHI 4
1University of the Philippines Diliman, 2University of the Philippines, 3Apex Mining Corporation, 4Akita University

Several epithermal gold-silver deposits and prospects are found in T’boli, South Cotabato, Mindanao island, Philippines. The area is characterized by a Late Cretaceous metamorphic basement overlain by Cenozoic clastic and carbonate sequences. These formations were dissected by normal faults, that resulted from either the reactivation of the northwest-trending Sindangan-Daguma-Cotabato fault or as a back-arc extension of the Cotabato trench. The most prominent deposit is in Kematu, characterized by high-grade stockwork veins hosted in dacite porphyry and volcaniclastic rocks belonging to the Parker Volcanic Complex. Major veins are oriented east-west, namely, North-, South-, and the Maria veins. Mineralization also occurs as either disseminations in fault gouge or filling in the vugs of dacitic breccia. The sulfide minerals identified are galena, pyrite, sphalerite, and chalcopyrite. Electrum occurs as inclusions or along the fractures of anhedral to subhedral pyrite. Textures observed are pseudo-bladed quartz and rhombohedral adularia indicative of boiling leading to ore precipitation. Drusy quartz veins on the dacite porphyry may have formed from the slowly cooling hydrothermal fluids. The XRD analysis and petrography revealed the presence of chlorite, albite, and muscovite in the veins and the altered wall rocks, which are indicative of near-neutral pH and reduced conditions of the mineralizing fluids. δ34SCDT values range from 0.1 to 1.6 ‰ for pyrite, and -5.3 to 0.5 ‰ for galena, sphalerite, and chalcopyrite. The δ34SCDT values with a narrow range and close to zero indicate that the sulfur was derived from magma. The tectonic setting, ore-, and alteration mineralogy indicate that the deposit is a low-sulfidation epithermal type.


SE01-A005
Ore-forming Processes of the Skarn Fe-Cu Deposit in the Masara Gold District, Eastern Mindanao, Philippines

Ma. Yna Rose GARCIA1#+, Jillian Aira GABO-RATIO2, Juan Alex Vianne AMOROSO3, Pearlyn MANALO4, Ryohei TAKAHASHI 4
1University of the Philippines, 2University of the Philippines Diliman, 3Apex Mining Corporation, 4Akita University

One of the major mineral districts in the Philippines is the Masara Gold District, which hosts epithermal gold deposits and porphyry copper prospects. It also has reported skarn mineralization, albeit with limited information. Thus, this study aims to characterize the mineralogy, identify the type of skarn and reveal the sulfide mineralogy and ore-forming processes of the skarn mineralization in Masara. The identified skarn zones include garnet skarn, magnetite skarn, epidote-chlorite skarn and hematite skarn zones. The garnet skarn zone is mainly characterized by yellowish garnet. This zone is cut by the magnetite skarn zone dominated by magnetite disseminations and veins. Sulfides such as pyrite, chalcopyrite with minor sphalerite, galena, ilmenite and hematite are observed. The epidote-chlorite skarn zone occurred at the same stage with the magnetite zone, both of which are part of the retrograde skarn stage. Hematite skarn zone overprinted all other skarn zones. Fluid inclusions trapped within the retrograde skarn alteration minerals are all liquid-rich vapor and liquid inclusions. Homogenization temperatures and salinities of fluid inclusions from calcite, epidote and chlorite are 280-300 °C and 3-17 wt% NaCl equiv., 312-342 °C and 18-20 wt% NaCl equiv., and 406 °C and 13 wt% NaCl equiv., respectively. The data plotted in a salinity vs homogenization temperature diagram show a horizontal slope trend. This suggests mixing of the hydrothermal fluids as the system cooled during the retrograde stage, which are typical in most skarn systems. The δ34SCDT from pyrite and chalcopyrite from magnetite skarn zones range from -0.3 to 4.0 ‰. Mineral chemistry analysis of the garnets revealed Al-rich compositions. Majority of the garnet contain Fe-rich core and Al-rich rim, indicating a shift from oxidized to reduced environment of formation. In summary, the retrograde stage alteration is dominantly observed in the calcic skarn Fe-Cu mineralization in the Masara Gold District.


SE01-A008
Geochemistry and Geochronology of Intrusive Rocks Southwestern and Northeastern, Cambodia: Implications for the Tectonic Evolution of the Loei Fold Belt

Sirisokha SEANG1#, Khin ZAW2+, Kret KAKDA1, Kotaro YONEZU3, Koichiro WATANABE3, Hoeun SEANGLENG 4
1Institute of Technology of Cambodia, 2University of Tasmania, 3Kyushu University, 4Industrial Mining & Environment Consulting Services

The Phnom Sro Ngam and Halo Prospects are potential targets for exploring porphyry, epithermal skarn-related gold deposits, and porphyry copper-molybdenum in Cambodia. The areas are located in the southwestern and northeastern parts of Cambodia extending from the highly mineralized Loei fold belt in Thailand and Laos [1]. However, the characteristics and tectonic significance of intrusive rocks of this fold belt remain ambiguous. In this paper, we present new geochemical data, zircon U-Pb ages for intrusive rocks from southwestern and northern Cambodia. Geochemically, the intrusive rocks from both areas were formed in a subduction-related tectonic setting under a volcanic arc setting. In addition, all intrusive rock plots into I-type granite in the SiO2 vs. Zr diagram. Trace elements spider diagrams being normalized to primitive mantle display strong enrichment in large ion lithophile elements such as Rb, Ba, and K and depletion in some high-field strength elements such as Nb and Ti, suggesting that the magma was generated in a subduction-related tectonic setting. REE patterns show slight enrichments in light REE relative to heavy REE and weak negative Eu anomalies. Distinct negative Eu anomaly indicates possible fractionation of Eu to plagioclase. Considering La/Yb as a crustal thickness proxy in intermediate to felsic calc-alkaline rocks, the arc crustal thickness in Phnom Sro Ngam was probably <40 km at the time of emplacement of normal calc-alkaline granitoid. Zircon U-Pb dating results showed Triassic to late Permian which ranges from 229 to 282 Ma, and they correspond to magmatic activity in the Loei Fold Belt, which was a back-arc basin formed during the eastward subduction of the Plaleo-Tethys Ocean beneath the Indochina terrane. Keywords: zircon U-Pb geochronology, REE, Plaleo-Tethys Ocean


Thu-03 Aug | 3:30 - 5:15 | MR336
SE13 - Seismic Hazard and Risk Assessments: Observations, Models, and Applications

Session Chair(s): Teraphan ORNTHAMMARATH, Mahidol University

SE13-A017
Shear Wave Velocity Model of Surface Using Passive and Active Seismic Methods in Cianjur Regency West Java Indonesia

Jimmi NUGRAHA#+, Rahmat SETYOYULIATMOKO, Thomas HARDY, Retno Agung PRASETYO KAMBALI, Supriyanto ROHADI, Dwikorita KARNAWATI
Indonesian Agency for Meteorology, Climatology and Geophysics

The condition of the Cianjur Regency is close to subduction zones and local faults, and it has a high level of earthquake hazards. Research on the level of vulnerability to earthquakes in the Cianjur West Java using passive seismic methods in HVSR and active seismic with MASW has been implemented. The total data collection consists of 175 HVSR points and 27 MASW points covering Cianjur and Karang Tengah. The shear wave velocity (Vs) value is obtained by combining the HVSR and MASW inversion methods, where both methods can complement each other's weaknesses. The distribution of shear wave velocity values describes the subsurface conditions related to the earthquake hazard vulnerability of the study area.
The 1D profile (Vs) of each point from the HVSR measurement and MASW inversion is interpolated to obtain a 3D Vs30 model. The results showed that the value of Vs30 in Cianjur Regency varied around 193–577 m/s. Layers with a relatively low (Vs) value have thick dominant sediment deposits in the eastern (MC 16) Hegarmanah Village, District of Karang Tengah. Layers with a relatively high (Vs) value have thin dominant sediment deposits in the northern (MC 22) Sukajadi Village, District of Karang Tengah. The soil type in this area is mainly composed of site class SC is hard soil, very dense and soft rock, and SD is medium soil. The subsurface structure layer model of measurement result by the Vs30 value is dominant in the form of two layers. The Vs30 contour pattern of the measurement results compared to the Vs30 USGS model has differences in the northeast and middle regions of the study area. Therefore, theoretically, the Hegarmanah Village District of Karang Tengah area has a relatively higher vulnerability to earthquake hazards than other areas in Karang Tengah and Cianjur District of Cianjur Regency.


SE13-A001
Development of Ground Motion Models for South Korea

Seonjeong PARK#+
Korea Institute of Nuclear Safety

Ground Motion Prediction Equations (GMPEs) is one of the most important factors for the Probabilistic Seismic Hazard Analysis (PSHA) which is crucial in terms of seismic safety of nuclear facilities. However, it is difficult to derive GMPEs empirically based on the observed ground motion data in South Korea due to its low seismicity and lack of the data. There has been a few GMPEs developed in South Korea. All of them used the stochastically simulated motions. In this study, GMPEs are developed for South Korea using the hybrid empirical method (HEM) suggested by Campbell (2003). Western United States (WUS) is selected as a host region and five NGA-West2 GMPEs are used as empirical GMPEs of the host region. Derived GMPEs are for magnitudes from 5.0 to 7.5 and rupture distances from 10 to 500 km. Median GMPEs are provided with aleatory standard deviations. Predictive values by the derived GMPEs were compared with ground motions from the available earthquake records for moment magnitudes 5.0 and 5.5. The notable advantages of the GMPEs developed in this study are as follows: All previous studies for GMPEs in South Korea used the same stochastic method. Because this study uses HEM, it supplements the limitations of the stochastic method, such as lack of near-source ground motion characteristics. Site-specific input parameters for the South Korea are used in the simulations of ground motions. The ground motions predicted by the developed GMPEs are compared with those from available observed data including earthquakes with moderate magnitude to check their applicability. Unlike previous GMPEs, the aleatory standard deviations are provided with GMPEs in this study so that they can be directly used in PSHA.


SE13-A006
A Progressive Model for a Probabilistic Seismic Hazard Assessment of Sumatra, Indonesia

Rizki WULANDARI1#+, Chung-Han CHAN2
1Sumatera Institute of Technology (ITERA), 2National Central University

The Sumatra region is known for its history of devastating earthquakes, with the most significant being the 2006 Mw9.2 Aceh earthquake that occurred at subduction interface. In fact, not only the great potential from the Sunda megathrust but also the threat due to the activities of the Sumatran fault system. In this study, we conduct a probabilistic seismic hazard assessment. In order to better illustrate possible seismic activity of each seismogenic source, our analysis incorporates the time-dependent Brownian Passage Time (BPT) model and the modelling earthquake rates considering complex multiple-segment ruptures along the Sunda Trench and the Sumatran fault. To overcome the lack of ground-motion models, we employed earthquake scenarios to select appropriate ground motion prediction equations for shallow active, subduction interface, and subduction intraslab regions, respectively. To understand the impact of seismic sources to some target sites, we demonstrate the hazard contributions of magnitude-distance distribution sets through disaggregation. Our results indicate that the Sumatran fault system is the primary contribution to the overall seismic hazard in the region, with peak ground acceleration (PGA) at bedrock sites of Sumatra in both short and long return periods, i.e., 10% and 2% probability of exceedance in 50 years, respectively. The outcomes of this study can provide valuable information for emergency response planning, urban development, and preparedness of governmental agencies before a disastrous earthquake in the Sumatra region.


SE13-A002
Seismic Hazard Assessment for Ryukyu and Taiwan

Chung-Han CHAN1#+, Asako IWAKI2
1National Central University, 2National Research Institute for Earth Science and Disaster Resilience

In this study, we promote research regarding integrated seismic hazard analysis along the Ryukyu Trench by sharing data and models to benefit next-generation national seismic hazard research for both Japan and Taiwan. Both Japan and Taiwan are located adjacent to the subduction zone and have high levels of seismic activities and frequent occurrences of devasting earthquakes. Facing the potential earthquake threats, it is urgent to propose a comprehensive plan for seismic hazard mitigation based on state-of-the-art geoscience research. Thus, many types of research in the two countries focus on hazard mitigation. Among them, seismic hazard assessment is a practical approach. This study promotes research toward assessing seismic hazards along Ryukyu Islands and Taiwan by sharing data and models. We aim to (i) integrate the earthquake catalogs, geodetic observations, and active fault database to propose a new model to illustrate seismicity behavior in the Ruykyu subduction system; (ii) harmonize strong ground motion observations for the earthquakes taking place in the study area to validate some existing ground motion prediction equations. The outcome could contribute to drill preparation for rapid response after a disastrous event. Tsunami scenarios that incorporate potential earthquakes present plausible inundated regions for different earthquake cases. Such outcomes could contribute to (i) a probabilistic seismic hazard map assessed by considering various seismogenic sources with their earthquake probability and possible ground shaking; (ii) minimized response times when real earthquake cases occur in the future; (iii) drill preparations for the public; and (iv) urban planning for local governments and building code legislation for central governments; and (v) raising the public’s awareness of damage from earthquakes. Our study could be beneficial to hazard mitigation for government agencies and raise the public’s awareness of damage from earthquakes and tsunamis.


SE13-A018
Peak Ground Displacement and Magnitude Estimation of Mw5.6 November 21st, 2022 Cianjur Earthquake Using High Rate GNSS Data

Thomas HARDY1#+, Supriyanto ROHADI1, Susilo SUSILO2, Irwan MEILANO3, Hasanuddin Z. ABIDIN3, Aditya RAHMAN1, Ajat SUDRAJAT1, Retno AGUNG PRASETYO1, Alpon SEPRIANDO1, Dwikorita KARNAWATI1
1Indonesian Agency for Meteorology, Climatology and Geophysics, 2National Agency for Research and Innovation, 3Bandung Institute of Technology

A catastrophic earthquake struck Cianjur Regency on 21st November 2022, with the magnitude Mw5.6, at a depth of 11 km. The quake caused more than 330 deaths and more than 10.000 houses damaged. There are 2 GNSS Stations near the epicenter from InaCORS networks could record surface displacement due to the earthquake, CJUR and CLDO. The PPP AR (Precise Point Positioning Ambiguity Resolution) approach utilizes to analyze High Rate (HR) 1 Hz GNSS data to determine surface displacement resulting from earthquakes. We can estimate Peak Ground Displacement (PGD) in CJUR, and CLDO as 12.81 cm and 3.71, respectively. We use PGD Scaling Law to calculate the earthquake magnitude using GNSS data that can reach 5.8.


SE13-A005
Strong Ground Motion Simulation and Fragility Function for Local and Public Buildings Damages from Mw 6.1, 2014 Northern Thailand Earthquake

Teraphan ORNTHAMMARATH1#+, Constance Ting CHUA2, Anawat SUPPASRI2, Piyawat FOYTONG3
1Mahidol University, 2Tohoku University, 3Khon Kaen University

Simulated ground shaking has been adopted in this study with available seismological information, recorded ground motion, and observed damage to investigate its impact on local and public building damages within the epicentral region. Moreover, empirical seismic fragility models have been proposed for different building types. This information could be useful for developing appropriate strategies to ensure safety of local communities for moderate earthquakes for similar structures within the Indochina region in the future.


Fri-04 Aug | 8:15 - 10:00 | MR306
SE08 - Understanding Magma Storage, Migration, and Eruption Through Geochemical Analyses, Numerical and Analogue Modelling, and Monitoring Data

Session Chair(s): Weiran LI, The University of Hong Kong

SE08-A020
Volcanic Geology, Petrology and Geochemistry of Primitive Basalts in Macolod Corridor, Southwestern Luzon Arc, Philippines

John Michael AUSEJO1#+, Americus PEREZ2, Julius PASCO1, Betchaida PAYOT1
1University of the Philippines Diliman, 2Kanazawa University

Textures and mineral chemistry of primitive arc lavas can be utilized to decipher petrogenetic processes within inaccessible magmatic systems. Primitive arc lavas have been recognized in the Macolod Corridor, a NE-SW extensive region of Quaternary volcanism located in southwestern Luzon arc, Philippines. Here we carried out textural, whole-rock and mineral chemistry analyses of primitive basalts obtained from scoria cones, tuff cones and polygenetic volcanoes to shed light on the pre-eruptive storage conditions and processes beneath the Macolod Corridor. Most basaltic samples are primary juvenile clasts obtained from monogenetic centers while basaltic lava flows represent polygenetic volcanoes. Four distinct magma compositions are identified based on their modal mineralogy such as (1) olivine basalt (OB); (2) olivine-clinopyroxene basalt (OCB); (3) olivine-bearing basalt (OBB); and (4) olivine-plagioclase basalt (OPB). Crystal types, modal abundances, and textures significantly differ from all primitive lavas examined. Phenocryst, microphenocryst and glomerocryst assemblages include clinopyroxene, olivine and plagioclase with trace amounts of fine-grained spinel embedded in a glassy matrix. Bulk-rock geochemistry of these primitive basalts (Mg#~69) indicates sub-alkaline, medium-K and medium-Fe tholeiite affinities. They display a wide range of MgO (6.3-11.8 wt.%) while OBs are the most magnesian (9.6 wt.% MgO) among all samples. Olivines in the most primitive samples (OCB: Fo77-88 and OB: Fo82-89) have an average value of ~0.26 wt.% NiO and 0.19 wt.% MnO contents. Whole-rock compositions from OCB and OB are in equilibrium with olivine phenocrysts while non-equilibrium with the clinopyroxene phenocryst. Clinopyroxene phenocrysts and glomerocrysts from OB and OCB have a wider range of Mg#71-87 compared with their olivine constituents. Plagioclase anorthite (An) has the widest range of compositions among all the assemblages of primitive lavas which is An40-97. Further geochemical studies of these primary phases will be performed to understand the evolution of their magma plumbing systems.


SE08-A016
Petrography and Geochemistry of Volcanic Rocks from Dinem Island, Batanes, Philippines

Noel Patrick SOBERANO#+, Betchaida PAYOT, Gabriel Theophilus VALERA
University of the Philippines Diliman

The Babuyan segment of Luzon arc in the Philippines is divided into an older west volcanic chain (WVC) and a younger east volcanic chain (EVC) based on geochemical and geochronological characteristics of their volcanic rocks. The Batanes Group of Islands form part of the northern portion of the Babuyan segment. Extinct Miocene volcanoes and Quaternary volcanoes in these islands belong to WVC and EVC, respectively. Mantle and crustal xenoliths have been previously recognized in the volcanic rocks of Batan and Sabtang islands. In this work, we present new petrographic and geochemical data on volcanic rocks from Dinem Island of EVC, which also host mantle and crustal xenoliths. The Dinem volcanic rocks are generally porphyritic andesites, with dominant plagioclase and amphibole grains as phenocrysts and minor clinopyroxene and Fe-Ti oxides. A positive correlation of major oxides and trace elements with SiO2 is observed in K2O, Na2O, Rb, Ba, Th and Zr while plots of MgO, FeOt, TiO2, CaO, Ni and Cr show negative correlation. (La/Sm)N and Th/Yb show high values while Ba/Th are low relative to Sabtang and older Batan of the WVC. The Dinem volcanic rocks show enrichment in large ion lithophile elements (LILEs) and light rare earth elements (LREEs) and depletion in middle to heavy rare earth elements (MREEs to HREEs) and HFSEs, which are typical of arc volcanic rocks. High (La/Sm)N, Th/Yb and low Ba/Th ratios are good indicators of sediment input and slab-derived fluids in the source of magma. From these trace element ratios and enriched LREE signature, Dinem and younger Batan volcanics of EVC record significant influence of sediment input compared to older Batan and Sabtang of WVC. This study contributes to the existing body of knowledge on the petrogenesis of rocks in Babuyan segment of Luzon arc.


SE08-A004
Volcanism-induced Generation of High-silica Granite: A Snapshot from Yandangshan Caldera, Southeastern China

Jing-Yuan CHEN#+
Chang'an University

Silicic magmatism was ubiquitous in the coastal areas of southeastern China. Today, the numerous volcanic fields and granitic plutons provide excellent locations to advance our understanding of upper crustal magmatic processes. We examine the petrogenetic links between alkali feldspar granites, porphyritic monzonites and syenites and coeval silicic volcanic rocks from the Yandangshan caldera and surrounding area using zircon U-Pb ages, trace elements, and Hf isotopic ratios, and bulk-rock geochemistry. Our results strongly suggest that lithological differences within the Yandangshan caldera are the result of silicic melt segregation. The porphyritic monzonites and syenites are enriched in Sr and Ba with high Zr/Hf and positive to weak negative Eu anomaly and interpreted to represent cumulate residues of crystal-melt segregation. The alkali feldspar granites and rhyolites are enriched in Rb and depleted in Sr, Ba, and Eu and display low Zr/Hf and Eu/Eu* and high Rb/Sr ratios. Both units are interpreted to represent the evolved silicic melts that were extracted from a crystal-rich mush. Compared with the erupted rhyolites, the alkali feldspar granites have a higher silica content and Rb/Sr ratio and lower Sr and Ba contents and Eu/Eu* ratios. Furthermore, zircons of the alkali feldspar granites have the most evolved trace element signatures (high Hf, Nb, Y, U; low Zr/Hf and Eu/Eu*) of the entire suite. These features together with zircon U-Pb age indicate that the granites formed after the eruption of the rhyolitic melts. We propose that, following the eruption of the rhyolitic melts, more-evolved granitic melts were generated and successively extracted from the underlying, complementary feldspar-rich mush. By comparing the geochemical characteristics of simultaneous silicic plutonic and volcanic rocks in the coastal area of southeastern China, we demonstrate that large volumes of high-silica granitic magma were accumulated in succession to silicic eruptions.


SE08-A002
Reconstruction of Magmatic Plumbing System for the Lamprophyre Dykes from the Tuoyun Basin of the Western Tianshan

Xiangsong WANG#+, Min SUN, Guochun ZHAO
The University of Hong Kong

The geochemistry of mineral assemblages combined with textural features can provide crucial information on magmatic processes in magmatic plumbing system. Here we present systematic petrological, mineralogical, and geochronological data for the newly identified lamprophyre dykes in the Tuoyun basin of the Western Tianshan. The apatite U-Pb dating reveals that the lamprophyre dykes were emplaced at 66 Ma. These lamprophyre dykes consist of three mineral assemblages: (I) Type-Ⅰ Cpx; (II) Amp core and Ap; and (III) Amp rim, Type-II Cpx, Kfs and Pl. These mineral assemblages are in chemical disequilibrium, thus corresponding to three magma reservoirs within the transcrustal magmatic system. Textural and geochemical features demonstrate that Type-I Cpx represents antecrysts captured from lower crustal crystal mushes. The Amp cores have the same rare earth element patterns as their enclosing Type-I Cpx inclusions, demonstrating the Amp cores were produced through peritectic reactions consuming Cpx. The third assemblages occur as microlites that were formed by the shallow crystallization of evolved melts. Thermobarometric calculations suggest a lower crust magma reservoir at 30–40 km depth, a middle crust magma reservoir at ~15 km depth, and a shallow upper crust magma reservoir at <10 km depth, making up a transcrustal magmatic system of the lamprophyre dykes. The magmatic plumbing system contains multi-stage open-system processes of early-formed crystals recycling, multiple magma replenishment, peritectic reactions, and crystal fractionation, resulting in the formation of lamprophyre dykes. Acknowledgements: The present study was financially supported by Hong Kong RGC Joint Laboratory Funding Scheme (JLFS/P-701/18), NSFC Major Project (41890831) and Hong Kong RGC grants (17307918), and HKU Internal Grants for Member of CAS (102009906) and for Distinguished Research Achievement Award (102010100). This work is a contribution of the Joint Laboratory of Chemical Geodynamics between the University of Hong Kong and Guangzhou Institute of Geochemistry, CAS.


SE08-A018 | Invited
Pre-eruptive Magma Conditions at Toba Caldera, Sumatra: Constraints from Melt Inclusion and Amphibole Geobarometry

Wei Jie Daniel LEE1, Ying-Jui HSU1#+, Francesca FORNI1,2, Caroline BOUVET DE MAISONNEUVE1, Marcus PHUA1, Hamdi RIFAI3, Simon REDFERN1
1Nanyang Technological University, 2University of Milan, 3Universitas Negeri Padang

The Toba Caldera Complex represents the largest volcanic (super-)eruption in the Quaternary. The late-stage evolution of large silicic reservoirs in the shallow upper crust as well as reservoir’s growth, longevity and eruption styles are largely controlled by volatile contents in magma in pre- and syn-eruptive conditions at depth. We focus on three major caldera-forming eruptions: The Youngest Toba Tuff (YTT; ~74 ka), the Middle Toba Tuff (MTT, ~501 ka) and the Oldest Toba Tuff (OTT, ~840 ka) to better constrain the pre-eruptive magma storage conditions. We combine melt inclusion data and amphibole geobarometry. We determined volatile contents (H2O and CO2) in quartz-hosted melt inclusions using micro-Fourier Transform Infrared Spectroscopy (µ-FTIR). The measurements were done in unexposed, single-polished quartz chips, adopting method [1]. We successfully extended the applicability of this method to melt inclusions embedded in thicker host quartz with a precision similar to that obtained in transmission mode for melt inclusions exposed on both sides. The estimated volatile contents range between 5.0–6.2 wt% H2O and 0–300 ppm CO2 for YTT, 4.8–6.3 wt% H2O and <100 ppm CO2 for MTT, and 4.6–5.5% wt% H2O and <100 ppm CO2 for OTT, giving that our data are about 0.5-1.0 wt% H2O higher than previously estimates [2]. The amphibole mineral chemistry was determined by electron microprobe to calculate the equilibrium pressure of magma storage. Our results suggest that YTT magma could have resided at a deeper depth than MTT and OTT magmas before eruption, and demonstrate the value of this method for probing magma storage conditions in ancient eruptions. 
[1] Peter Tollan, Ben Ellis, Juliana Troch & Julia Neukampf. Contributions to Mineralogy and Petrology (2019), 174, 24.
[2] Craig A. Chesner and James F. Luhr. Journal of Volcanology and Geothermal Research (2010), 197, 1–4.


SE08-A021
On Creating a Global Volcanic Rock Classification of Holocene Volcanoes by Linking the Geochemistry of Rocks of the Ocean and Continents and the Global Volcanism Program Databases

Frederique OGGIER#+, Christina WIDIWIJAYANTI, Fidel COSTA
Nanyang Technological University

We have developed an algorithm (deployed in DashVolcano, https://github.com/feog/DashVolcano) to associate volcanic rock names to Holocene volcanoes using more than 138,000 rock sample geochemical compositions available in the Geochemistry of Rocks of the Ocean and Continents (GEOROC) database. It relies on identifying different samples as belonging to the same volcano, through both a geographical and name matching procedure, and on mapping chemical composition to rock names via the Total Alakali-Silica diagram (TAS). We consider a list of Holocene volcanoes provided by the Volcanoes of the World (VOTW) of the Smithsonian’s Global Volcanism Program (GVP), whose database provides together with each Holocene volcano, a list of so-called major rocks (they consist of more than 10% of the total population) and minor rocks (they consist of less than 10%). The results we obtained are overall consistent with those listed by GVP. Our method is transparent and reproducible, and since GEOROC provides different types of materials, we are able to obtain the classification for whole rock, volcanic glass, inclusion and minerals. We provide several visualization tool and case examples to illustrate and validate the data. The geochemical composition of rocks of a volcanic system is an important factor for understanding its eruption processes and styles. The GEOROC database contains a wealth of information that this work uses to make the volcanic rock classification available at once for more than 1000 Holocene volcanoes (https://doi.org/10.21979/N9/BDRRSI).


Fri-04 Aug | 8:15 - 10:00 | MR322
SE15 - Techniques and Methods for Geological Hazard Monitoring and Mitigation

Session Chair(s): Mirzam ABDURRACHMAN, Bandung Institute of Technology, Benoit TAISNE, Nanyang Technological University

SE15-A004
Building a Future Scenario Earthquake for Seismic Hazard Analysis in Kathmandu, Nepal

Kazuki KOKETSU1,2#+, Hiroe MIYAKE2, Koji OKUMURA3
1Keio University, 2The University of Tokyo, 3Hiroshima University

We first proposed a distribution of the source regions of great historical earthquakes in the Main Himalayan Thrust (MHT) using Bilham (2019) and results of trench surveys (Okumura et al., 2023). In this distribution, a certain rectangle can be the source region of a future scenario earthquake for seismic hazard analysis in Kathmandu, Nepal. The rectangle is neighboring Kathmandu, and the previous events in the rectangle occurred in 1255 and 1344. They are the oldest among the great historical earthquakes in MHT. The displacement rates observed by GNSS are similar along the southern boundary of MHT (Tabei et al., 2023), and it can be assumed that the great historical earthquakes mostly released accumulated strain. Therefore, it is the most probable for the rectangle, where the previous events are the oldest, to generate a great future earthquake the soonest. The area of the rectangle is measured to be 17,600km2 with a length of 220km and width of 80km. The 2015 Gorkha earthquake recently occurred in the MHT. Kobayashi et al. (2016) performed a source inversion for this earthquake, obtaining seismic moment M0=7.4x1020Nm (Mw7.8) and the slip distribution. We trim insignificant slips off the slip distribution following the scheme of Somerville et al. (1999). This trimming results in a rupture area of 9,600km2. This area corresponds to M0=8.9x1020Nm (Mw7.9) using the formula of Somerville et al. (1999), while it corresponds to M0=5.2x1020Nm (Mw7.7) using the formula of Murotani et al. (2008). The actual M0 falls between these, so that we use the both formulas to determine two characterized source models for the future scenario earthquake with the rupture area of 17,600km2. The formula of Somerville et al. (1999) gives M0=2.2x1021Nm (Mw 8.2), average stress drop Δσc=2.3MPa, asperity area Sa=4,000km2. Meanwhile, the formula of Murotani et al. (2008) gives M0=1.3x1021Nm (Mw8.0), Δσc=1.4MPa, Sa=4,400km2.


SE15-A010
Spatial Distribution of Landslide Along the Near Active Fault Zones: A Case of the Litang Fault Zone in the Eastern Tibetan Plateau

Yigen QIN1+, Dongli ZHANG2#, Wenjun ZHENG1, Bingxu LIU1, Zhikang GONG1
1Sun Yat-sen University, 2中山大学

The active fault zone is where geohazards such as landslides occur, especially near-fault zones. Using the Litang fault zone in the eastern Tibetan Plateau as an example, this study cataloged landslides within a certain range on both sides of the fault zone. The study area was divided into four sections based on the landform characteristics and spatial distribution of the active faults. The landslide probability density (LPD) distribution and landslide area percentage (LAP) were used to analyze the spatial distribution of landslides of the Litang fault zone and to explore the control effect of active faults on near-fault landslides under different geomorphological conditions. The random forest (RF) model was used to evaluate landslide susceptibility. The results show that the landslide area percentage was positively correlated with slope and local relief. The control effect of active faults on landslides mainly includes (1) the distance effect, (2) the hanging wall effect, (3) the locked segment effect, and (4) the direction effect. The active faults had different control effects on near-fault landslides under different geomorphological conditions. When the landforms near faults are dominated by unilateral mountains, the distribution of landslides has obvious hanging wall effect. When the fault passes through the middle of the canyon, both sides of the fault show symmetric distribution characteristics. When the fault passes through the middle of the basin, the landslide is mainly distributed in the basin margin. The results of landslide susceptibility zoning showed that the area under the receiver operator characteristic curve of the RF model was 0.8983, indicating high prediction accuracy. The results can provide a scientific reference for exploring the spatial distribution of landslides in near-fault zones.


SE15-A006
Ascending Volcanic Fluids Revealed by Spatiotemporal Variations of the Earthquake Mechanisms in the Tatun Volcano Group in Northern Taiwan

Hsin-Chieh PU1#+, Cheng-Horng LIN2, Hsiao-Fen LEE3,4, Ya-Chuan LAI5,6, Min-Hung SHIH7
1Central Weather Bureau, 2Academia Sinica, 3National Center for Research on Earthquake Engineering, National Applied Research Laboratories, 4Taiwan Volcano Observatory at Tatun, 5Taiwan Volcano Observatory - Tatun, 6National Center for Research on Earthquake Engineering, 7National Applied Research Laboratories

We examined the spatiotemporal variations in the focal mechanisms of micro-earthquakes at the Tatun Volcano Group (TVG) in northern Taiwan, where the local residents reach a number of approximately 7.5 million and a variety of phenomena associated with volcanic activities were observed. We found a series of similar variations appeared in two time-dependent observations: the occurrence rate of shallower (0–2 km) reverse-type earthquakes and deeper (2–4 km) normal-type earthquakes. The similar variations progressed in a stepwise manner as the depth range of the observation decreased. Such variations also appeared in the temporal variation of gas compositions sampled at the fumarole. To interpret the spatiotemporal variations of such observations, we construct a model involving the ascending volcanic fluids in the conduit and hydrothermal layer. On the basis of this model, the ascending volcanic fluids seems to be monitored at the TVG.


SE15-A029
Global Volcano Monitoring Data Governance in WOVOdat & GVMID Databases

Christina WIDIWIJAYANTI1#+, Benoit TAISNE1, Fidel COSTA1, Nang THIN ZAR WIN1, Tania ESPINOSA-ORTEGA1, Chris NEWHALL2, Antonius RATDOMOPURBO3
1Nanyang Technological University, 2Mirisbiris Garden and Nature Center, 3Geological Agency

Global volcano monitoring data plays a central role in our ability to understand volcanic processes, improve eruption forecast and hazard mitigation, which aimed at saving lives and achieve economic sustainability. The ever-increasing amount of global volcano monitoring data in this digital-era, which becoming more diverse and of higher resolution, poses significant challenge in data management. Aimed to address these, we created WOVOdat (volcano unrest) and GVMID (volcano monitoring infrastructure) global databases to integrate worldwide’ volcano monitoring data in a standardized and centralized open access repository. The wealth of accessible data, allow to answer questions of generality in volcanology that only can be addressed by integration of global data and by comparing various cases studies using a coherent data management framework in a global scale databases. Good data governance is crucial to preserve the important scientific value of these datasets and to address FAIR (Findability, Accessibility, Interoperability, and Reusability) scientific data lifecycle. To achieve this objective, the data should be: 1) curated with their metadata, common identifier, and annotations; 3) processed, to obtain a more meaningful variable that can be quantifiable with quality assessment; 4) integrated and archived in centralised server; 5) managed in database management system, using common identifier, archive in a standardized format and structure, using unified classification and term, enable storing multi-variable data and can be contextualized with its metadata; 6) findable via data query tools, so that the integrated datasets can be mined and analysed together in a global scale, and link with other databases resources; 7) open access, with data policy; 8) reusable, can be analysed together with other data types, integrated for multi-variable analysis, allowing spatio-temporal analysis, compared across different unrest/eruptions/volcanoes. Volcano community could potentially also use the dataset to perform basic research on eruption processes, teaching and outreach.


SE15-A016
The 2018-2022 Merapi Eruption, Hazard Mitigation and Crisis Response

Hanik HUMAIDA1#+, Agus Budi SANTOSO1, Naning AISYAH2, Sulistiyani SULISTIYANI1, Christina WIDIWIJAYANTI3, Andika Bayu AJI3,1, Raditya PUTRA1, Lestari AGUSTININGTYAS1
1Geological Agency, 2Center for Research and Technological Development Kegunungapian, 3Nanyang Technological University

Following the 2010 VEI 4 eruption, Merapi volcano experienced series of phreatic eruptions in between July 2012 - April 2014. On 21 May 2018, the volcano alert level increased to level-2 (out of 4) due to series of phreatic eruptions and increased in seismicity, followed by lava dome extrusion in August, which was then destroyed by series of explosion in 2019 until 21 June 2020. Afterwards, the unrest signs (seismic, deformation and gas) progressively intensified, which resulted in increased of the volcano alert level to level-3. The heightening of unrest signs continued and culminated at the end of December 2020. Early January 2021 marked the beginning of effusive eruption phase that manifested by incandescent rockfalls from outer crater wall at the Southwest side. Two lava dome extrusion observed at the southwest side and in the middle of Merapi crater, which still continue growing until present day. Despite significant loses of monitoring infrastructure due to the explosive 2010 and the following eruptions, we continuously improving volcano monitoring capabilities e.g. spatial coverage, complimentary techniques (DSLR, drone survey), continuity and stability of the data transmission, automatic data processing and analysis, database management and visualization interface. Potential volcanic hazards were assessed based on range of hazard scenarios with its respective phenomena (e.g. PDC, lahar, debris avalanche), updated through time following the evolving activities, which is then being used as contingency plan by the local authorities. Hazard evaluations also performed under advisory of national and international volcano experts. To improve disaster preparedness we actively engage with community around Merapi through intensive coordination with the local government e.g. socialisation, Compulsory Disaster Management Training for those living within the main hazard zone areas (KRB III). Dissemination information about update in Merapi activities was carried out through social media platforms by creation of Information and Communication Team.


SE15-A031
Activity of Anak Krakatau for the January – February 2023 Period

Heruningtyas Desi PURNAMASARI1#+, Ahmad BASUKI1, Hendra GUNAWAN1, Iyan MULYANA1, Francois BEAUDUCEL2, Mirzam ABDURRACHMAN3,4
1Center for Volcanology and Geological Hazard Mitigation, 2Institut de Physique du Globe de Paris, 3Bandung Institute of Technology, 4Indonesia Association of Geologists

Anak Krakatau volcano is still continuously growing since the last edifice collapse on December 22, 2018. Its morphology continuously evolving, started with Surtseyan eruptions from the submarine vent, then formed a crater lake in 2019. Intermittent explosive and effusive eruptions built up the volcano edifice, both vertically and laterally. Between 2019 and 2021, a volcanic cone formed at the active vent of 50 m height, and lava flow with runout reached ~750 m towards southwest. Since February 2022, the eruption continues almost every month. The SiO2 content of the 2018’ volcanic ash ranged from 53-55 wt%, which indicates a condition similar to magma after the 1883 eruption. A more comprehensive monitoring infrastructure was established, aimed to better understand Anak Krakatau’ plumbing system and to detect the magmatic processes. We deployed 4 seismic broadband, 1 tiltmeter, and 4 GNSS stations located at Anak Krakatau, Sertung, and Panjang islands, in addition one seismic station located in Banten (northwest Java). Here, we present results of our investigation focusing on understanding the activities within the period of January to February 2023. We observed an increase of VT earthquakes and tremors preceding the January 2023 eruption. The seismic ambient noise autocorrelation shows that the relative velocity variation (dv/v) highly fluctuated, which indicated high stress level within the plumbing system. The deformation data from tiltmeter and GNSS also indicate inflation of the pressure source located ~6.2 km beneath the surface, which we interpret as magma recharge at the lower part of the magma chamber. In February 2023 the magma then migrated to the surface, revealed by the depth of pressure source obtained from GNSS data moved to ~1 km depth, while tiltmeter data showed no significant changes. In comparison, InSAR data indicate deflation between early to mid-February. 


SE15-A030
The January 2023 Eruption of Marapi Volcano as Observed from the Multiparameter Stations

Dannie HIDAYAT1#+, Hetty TRIASTUTY2, Dini NURFIANI3, Yizhou LUO1, Christina WIDIWIJAYANTI1, Ahmad BASUKI2, Benoit TAISNE1, Hendra GUNAWAN2
1Nanyang Technological University, 2Center for Volcanology and Geological Hazard Mitigation, 3National Research and Innovation Agency

After a long paused of eruption, Marapi Volcano in West Sumatra, Indonesia, started to erupt on 7 January 2023. Compared to last recent episodes of eruptions, they consist of many explosions and degassing events. We analyse the time interval between explosions of Marapi from the beginning of the eruptions to a month after. We observed in the beginning of eruptions, almost every hour there was an explosion, after a week time, the time interval became longer until no explosion occurred a month the first explosion. We will also explore the mechanism of explosions from the infrasound data because the infrasound waveforms are simpler than those of the seismic waveforms. We observed the waveforms and the amplitude of infrasound in the beginning of eruption was simpler and very large at the station 300m from the active vent (> 20 Pa peak-to-peak) then the later explosions the amplitudes became smaller, and the waveforms became more oscillating coda. This suggest the source, in the beginning it is filled with gas and fragmented magma and later the source is partially filled. The explosions were also recorded by 4 other infrasound stations installed around the volcano up to the distance of 10 km from the vent. The infrasound is one component of parametric stations jointly installed by Earth Observatory of Singapore and Centre for Volcanology and Geological Hazard Mitigation to monitor Marapi Volcano. The other aspect would be to explore tilt data from 2 stations: PCAK, located near the vent, while the other, BTPL, located at distance about 5 km from the vent. Several months before the eruptions the tilt showed interesting signals. Based on what we observed in the tilt data the source of the eruption started from shallow to deeper depth which suggest the eruption was driven by convecting magma.


Fri-04 Aug | 10:20 - 12:20 | MR306
SE08 - Understanding Magma Storage, Migration, and Eruption Through Geochemical Analyses, Numerical and Analogue Modelling, and Monitoring Data

Session Chair(s): Benoit TAISNE, Nanyang Technological University

SE08-A011 | Invited
The Emergence of Fumaroles at Kelud Volcano in 2020-2022: An Indication of a New Magma Supply

Hanik HUMAIDA1#+, Harry CAHYONO1, Lestari AGUSTININGTYAS1, Andika Bayu AJI2,1, Nurudin NURUDIN1, Sri SUMARTI3, Tannisa APRIANTI1, Arif HIDAYAT1
1Geological Agency, 2Nanyang Technological University, 3National Research and Innovation Agency

After the last VEI 4 eruption in February 2014, Kelud Volcano (East Java, Indonesia) started showing signs of unrest in September 2020. In response to this, we conducted a geochemical investigation and visual observation around Kelud crater lake area. New observable phenomena were observed, e.g. increased fumarolic activities, changes in the crater lake water colour, subaqueous bubbling and gas bubbles in the crater lake, and red deposits found on the rim of the crater lake. These phenomena started appearing in September 2020 and were correlated with the emergence of deep volcanic earthquakes recorded by Kelud seismic network. The temperature of the crater lake water also increased and became more acidic. Stable isotope data of Oxygen-18 (18O) and Deuterium (2H) fumarole condensate indicate the type of meteoric water, while isotope values of crater lake water indicate a mixture of volcanic and meteoric water. We suggest that the ascent of magmatic gases from a new magma supply at depth emitted through the lake water caused these changes. The period of unrest at Kelud volcano between September 2020 and March 2022 is attributed to the deep magma recharge.


SE08-A005 | Invited
Monitoring of Sulfur Dioxide Flux from Fukutoku-Oka-No-Ba and Nishinoshima Volcanoes, Japan

Masaaki MORITA#+
The University of Tokyo

Even though there has been much progress in monitoring equipment in recent years, monitoring volcanic activities at a remote underwater volcano or a subaerial volcanic island is still a significant challenge. Satellite observations using a geostationary sensor with a high temporal resolution and a sensor in a polar orbit with a high spatial resolution can significantly contribute to solving this problem. In this study, we have applied an analysis of sulfur dioxide (SO2) flux using a satellite sensor to monitor recent eruptions at Fukutoku-Oka-no-Ba (FOB) and Nishinoshima volcanoes, Izu–Bonin arc. We used data from an ultraviolet sensor Tropospheric Monitoring Instrument (TROPOMI) onboard Sentinel-5 Precursor and a visible/infrared sensor Advanced Himawari Imager onboard Himawari-8/9. Based on a daily snapshot of SO2 spatial distribution taken by TROPOMI and wind field data from a weather model, we estimated an hourly SO2 flux for these volcanoes. For the August 2021 eruption of FOB volcano, SO2 flux during the first sustained plume phase was more than 10,000 t d–1 and up to 75,000 t d–1. In the later Surtseyan explosion phase, SO2 flux decreased to less than 1,000 t d–1 and was sometimes below the detection limit (100 t d–1). For Nishinoshima volcano from August 2021 to December 2022, the daily SO2 flux during the non-eruptive period was 100–1,000 t d–1 and often below the detection limit. The daily SO2 flux during the eruptions in August 2021 and September–October 2022 was more than 3,000 t d–1 and reached more than 10,000 t d–1 in October 2022. These results indicate that the satellite monitoring of SO2 flux using TROPOMI is an effective tool for eruptive activities at a remote underwater volcano and a subaerial volcanic island.


SE08-A009
Constraints on Magma Storage Conditions Based on Geodetic Volume Change and Erupted Magma Volume and Application to the 2011 and 2018 Eruptions at Kirishima Shinmoe-dake Volcano, Japan

Tomofumi KOZONO1#+, Takehiro KOYAGUCHI2, Hideki UEDA1, Taku OZAWA1, Tadashi YAMASAKI3
1National Research Institute for Earth Science and Disaster Resilience, 2The University of Tokyo, 3Geological Survey of Japan

We investigated magma storage conditions prior to the 2011 and 2018 eruptions at Kirishima Shinmoe-dake volcano in Japan based on the relationship between geodetic volume change of magma chamber and erupted magma volume. We derived an analytical expression for the ratio of the erupted magma volume to the geodetic volume change ("volume ratio''), which was formulated as a function of parameters related to the magma storage conditions. This expression shows that the volume ratio is strongly dependent on the effective compressibility of the magma chamber, which in turn depends on the rigidity of surrounding host rocks and shape of the chamber. For the Shinmoe-dake eruptions, the magnitude of the volume change (i.e., deflation) of a spherical magma chamber associated with lava effusion was estimated based on geodetic observations. The erupted magma volume was estimated from a SAR image analysis of the lava accumulation inside the summit crater. Based on these observations, we estimated that the volume ratio in 2011 and 2018 was 2.69 and 2.33, respectively. Substituting the estimated volume ratio into the analytical expression revealed that the observed geodetic data and volume ratio can be explained only when the magma chamber, which was assumed to be spherical, is filled with bubble-free magma. This result suggests that efficient gas segregation from the chamber occurred prior to the eruptions. Our results indicate that combining multi-observation data based on the volume ratio provides valuable information about the magma storage process, such as the behavior of the gas phase in the magma chamber.


SE08-A013
Revisiting Volcanic Earthquake Classification for Merapi Volcano

Andika Bayu AJI1,2#+, Benoit TAISNE1, Agus Budi SANTOSO2
1Nanyang Technological University, 2Geological Agency

Merapi Volcano, located in Java (Indonesia), is arguably one of the most active volcanoes in the world. Its activity is being monitored by an observatory named Balai Penyelidikan dan Pengembangan Teknologi Kebencanaan Geologi (BPPTKG), a division under the Centre for Volcanology and Geological Hazard Mitigation (CVGHM) – Geological Agency. The observatory carries a multiparameter monitoring system, one of which is seismic monitoring. An automatic detection of volcanic earthquakes based on the STA/LTA technique is employed, whereas the earthquake classification is done manually by the volcano observers. Earthquake classification is critical for understanding magmatic processes that are underway beneath a volcano edifice. However, because of this manual classification, there might be inconsistencies in the classification due to human error. To address the issue, we conducted a preliminary study in which we used classified/master events comprising: shallow volcano-tectonic (VTB), Hybrid/Multi-Phase (MP), Degassing (DG), and Rock Fall (RF) types. We used similarity in the frequency domain to cluster these master events. The clustering result reveals that about half of the total VTBs and MPs belong to one cluster, one-third of the total DGs form a separate cluster, while the RFs do not form a specific cluster. The result suggests that at Merapi Volcano, the VTBs and MPs have similar frequency contents, implying that those two types of earthquakes have a similar source mechanism. However, the result can also confirm that there is an inconsistency in the manual earthquake classification used by the observatory.


SE08-A007
2011 Tengchong Earthquake Swarm: Fluid Migration, Earthquake Faulting and Possible Magma Chamber

Min LIU1#+, Yen Joe TAN1, Yunpeng ZHANG2, Hongyi LI3
1The Chinese University of Hong Kong, 2China Earthquake Administration, 3China University of Geosciences

Earthquake swarms are frequently observed in volcanic regions, with the underlying driving mechanism often inferred to be some aseismic processes such as magma intrusions or hydrothermal fluid diffusion. In this study, we investigate an earthquake swarm in the Tengchong volcanic field which includes two M 5.2 earthquakes (2011-06-20 and 2011-08-09). We apply a series of state-of-the-art methods, including machine-learning-based phase picker and associator, as well as a series of location algorithms, to build a high-resolution earthquake catalog of the swarm. The newly-developed catalog contains ~3,000 well-located earthquakes with depths ranging from 10 km to 13 km. These earthquakes reveal a spiral structure surrounding a low-seismicity zone which coincides with a previously-inferred magma chamber from magnetotelluric imaging. The swarm started with some small earthquakes in November 2010 and then underwent a complex evolution until December 2011, which can be divided into multiple sub-swarms based on their magnitudes and spatiotemporal distribution. Part of the migration fronts can be well-modelled by fluid diffusion with a relatively slow diffusion rate (0.003~0.1 m/s2), implying that fluids may play an important role in controlling the swarm evolution. We also find that the seismicity further migrated away immediately after the relatively large events, indicating that these large earthquakes may serve as valves, which facilitated fluid diffusion further.


SE08-A003
Observations of Long-period Earthquakes at Alaskan Volcanoes and Their Relation to Magma Transport and Storage

Zilin SONG1#+, Yen Joe TAN1, Diana C. ROMAN2
1The Chinese University of Hong Kong, 2Carnegie Institution for Science

Seismic signals are commonly observed in volcanic regions, manifesting stress disruption in the crusts, hydrothermal, and magmatic systems. Long-period earthquakes (LPs) are seismic signals radiating low-frequency energy predominantly and are sometimes recorded preceding eruptions, such as the 1991 Pinatubo eruption. As a potential precursor, it provides a window into magma transport and storage under volcanoes. However, due to the emergent arrivals and rich low-frequency contents, LPs are difficult to be detected by traditional earthquake detection methods. In this study, we select 9 volcanoes at the Aleutian volcano arc where there are a sufficient number of manual-labeled LPs and seismometers. We then reclassify all the seismicity and identify LPs systematically by spectra analysis. These LPs are used as templates to cross-correlate with years of continuous data to detect more LPs automatically. So far, we obtain at least two times more LP detections than LP templates at 7 volcano candidates, including Akutan, Aniakchak, Makushin, Okmok, Pavlof, Veniaminof volcano, and Katmai volcano group. By earthquake relocation and clustering, at Akutan Volcano, we find that deep LPs occur preferentially when the inferred magma reservoir inflates. The relatively uniform frequency contents of deep LPs across the seismic network suggest that deep LPs are likely due to source effects like unsteady magma transport, instead of just path or station site effects. We are currently analyzing LPs at other volcanoes to investigate how they relate to magma transport and storage at Alaska.


SE08-A012
Global Assessment of the Impact That Seismic Network Locations Have in the Detection of Magma Migration Using SARA

Tania ESPINOSA-ORTEGA1#+, Katie JAMES2, Chiou Ting TAN3, Benoit TAISNE1
1Nanyang Technological University, 2Earth Observatory of Singapore, 3Science Centre Board

Volcanic eruptions are frequently preceded by magma migration towards the surface that trigger seismic swarms, these seismic events often overlap and saturate the seismic signal, limiting the analysis techniques that can be effectively applied in real time crises. The Seismic Amplitude Ratio Analysis (SARA) provides a simple method to image the dynamics of seismic magma migration as it happens using the continuous seismic wave form. In this project, we analyse how the location of the seismic networks can impose spatial contraints that limit the effectiveness of SARA. We introduce a method to quantify the detection capability of the seismic network for different magma migrations and analyse how the detection capability could be improved by changing the seismic stations locations. We use the Global volcano monitoring infrastructure database (GVMID) and IRIS to study different seismic networks and the land elevation data from NASA’s Shuttle Radar Topography Mission (SRTM) to consider the volcano’s topography. For each seismic network we analyse their potential to detect vertical magma migration and side vent formations. Moreover, we estimate the magma migration coverage volume and the impact of adding or removing a seismic station in the detection capability of the network, we also inspect what makes some seismic networks more efficient than others. This method provides a quick and straightforward way for volcano observatories to identify any detection gaps in a network when the SARA is applied, as well as a guide on how the seismic network design could improve their ability to detect magma migration in real time using this method. Thus, we expect our work to help observatories by enhancing their monitoring and hazard prevention capabilities.


Fri-04 Aug | 10:20 - 12:20 | MR322
SE15 - Techniques and Methods for Geological Hazard Monitoring and Mitigation

Session Chair(s): Benoit TAISNE, Nanyang Technological University, Mirzam ABDURRACHMAN, Bandung Institute of Technology, Christina WIDIWIJAYANTI, Nanyang Technological University

SE15-A020
Recover the Hidden Traces of Spectral Change in Continuous Monitoring Waveform

Yizhou LUO1#+, Benoit TAISNE1, Ahmad BASUKI2, Hetty TRIASTUTY2, Hendra GUNAWAN2
1Nanyang Technological University, 2Center for Volcanology and Geological Hazard Mitigation

Volcanoes are dynamic systems that can demonstrate various activities before the onset of an eruption. Some of the activities are evident and considered as precursors for eruptions; while some can be subtle which may be missed during real-time analysis. We have introduced a new technique that looks for subtle changes in continuous monitoring data. It compares the distribution difference in waveform spectra between reference and sample timeframe, and a large difference signifies some sort of disturbance in the system. Here we apply the technique on several case studies that represent different volcanic activities, including the Marapi (Indonesia) Jan 2023 explosion and Apr 2018 phreatic eruption. The results present the detection signature of different activities using this technique. It also reveals detailed spectral change that can be related to physical processes in the volcanic system.


SE15-A018
Petrographic and Geochemical Characteristics of Lokon Volcanic Complex to Determine the Tectonic Setting and Magma Signature of That Area

Kevin SENDUK#+, Mirzam ABDURRACHMAN
Bandung Institute of Technology

The Lokon Volcano Complex (LVC) is located on the northern arm of Sulawesi Island which was formed due to the activities of the Maluku Sea collision. The research method is the identification of mineral composition characteristics and special textures of magma kinematic indicators using Petrography analysis. There are 13 lava samples representing each Crown from the Lokon Mountain complex. In this research, mineral texture can indicate the mineral formation environment as well as the magmatic textural stratigraphy. The petrography analysis, three groups of structures based on the mineral formation environment: the deeper magma chamber, shallow magma chamber (convection flow-related texture), and eruption-related texture. Geochemical analysis shows that the TiO2 value is below 1,4 wt% which is characteristic of subduction-related magmatism. The TiO2-MnO-P2Oanalysis on the basalt sample concludes that this is an oceanic island arc. Alternatively, andesite in the study area concludes that this arc is undergoing a transition from island arc to mature andesite arc. Higher enrichment of Rb and Zr compared to a selected volcano in Java with a similar tectonic setting shows that the high value of Rb is estimated due to the presence of continental element contamination and the presence of fractionation of potassic minerals. While Zr is estimated to be sediment contamination in the magma chamber.


SE15-A002
Tephra Analysis of 2010 Bromo Eruption and Application for Volcanic Ash Hazard Assessment

Aisyah QURRATA AINI1#+, Idham ANDRI KURNIAWA1, Mirzam ABDURRACHMAN1,2
1Bandung Institute of Technology, 2Indonesia Association of Geologists

As one of the tourist attractions and farming centers, Tengger Complex encountered danger from Bromo’s eruption. To learn more about the eruption, we decided to do research that aims to know the mechanism of the eruption along with deterministic and probabilistic modeling of ash fall using TephraProb. This research focused on the 2010 eruption. This study used event tree analysis, tephrastratigraphy, physical analysis of tephra such as material properties analysis, ash composition, petrography, and textural analysis, along with deterministic and probabilistic modeling of eruption. Event tree analysis shows that ash fall is the hazard with the highest probability. From tephrastratigraphy and physical examination, it is known that there are four phases of the eruption. The first phase is the vent opening phase which consists of phreatomagmatic eruption; the second phase consists of strombolian eruption; the third phase consists of ash eruption; and the final phase consists of ash and phreatomagmatic eruption. Based on deterministic modeling, in phase 1, the ash fall is spread as far as ~30 km to the east, ~ 70 km to the southeast in phase 2, ~30 km to the east in phase 3, and ~25 km to the east in phase 4. A probabilistic analysis was conducted using wind data from 2010-2022 to determine the probability of ash fall danger. From probabilistic modeling, we know the all-year and April-August scenarios show the ash fall incline to the west. Meanwhile, in September-March, ash falls lean towards the east. The probabilistic modeling indicates that the Putus and Wonokitri areas have a hazard risk due to ash fall with an accumulation of up to 300 kg/m2. The existing KRB Map does not yet convey the collection of ash fall, so other media are needed to inform about the risk of the ash fall.


SE15-A023
Analysis of Eruption Mechanism and Modeling of Tephra Fall from Phase 2B-3 of Galunggung Mountain in 1982-1983 West Java Province

Salma SAKINAH1#+, Idham ANDRI KURNIAWA1, Mirzam ABDURRACHMAN1,2
1Bandung Institute of Technology, 2Indonesia Association of Geologists

The eruption of Galunggung Volcano in 1982-1983, which had a duration of nine months, caused morphological changes up to a radius of 20 km from the center of the eruption. To learn more about the potential dangers of an eruption, the authors conducted a study that aimed to determine the eruption mechanism and deterministic modeling of the 1982-1983 eruption. The study used tephra grain analysis, including grain component, grain morphology, Bubble Number density (BND), Microlite Number Density (MND), decompression rate, and magma ascent rate, as well as tephra fall modeling using the TephraProb. The results of component analysis and grain morphology show that the product of the 2B-3 phase eruption is dominated by vesicular juvenile material. In phase 2B, BND has a value of 6,2x1011-3,9x1012 m-3, and MND has a value of 2,9x1012-1,1x1013 m-3. In phase 3, BND has a 1x1012-3,1x1012 m-3, and MND has a value of 5,8x1012-1,1x1013 m-3. The analysis of decompression rate and magma ascent rate results show that the range of values ​​for phase 2B is 1,5x103-1,8x104 Pa/s and 0,06-0,7 m/s, and for phase 3 is 1,1x104-1,8x104 Pa/s and 0,5-0,7m/s. The results of grain analysis using various methods showed the mechanism of the eruption that occurred at the beginning of the phase 2B phreatic eruption decreased, then increased to phase 3 (strombolian). The high value of decompression rate and magma ascent rate found a correlation with BND and MND. Based on the eruption modeling with parameters that have the most significant level of danger, namely on October 14, 1982, volcanic ash was found scattered over a 25 km radius leaning towards the west with a volume of 106 m3, ash column height of 9 km, and with a product mass that produced about 38,75x108 kg.


Fri-04 Aug | 1:10 - 3:10 | MR306
SE16 - Advancement in Volcanology and Strengthening Collaboration in Volcanic Disaster Prevention

Session Chair(s): Benoit TAISNE, Nanyang Technological University, Masato IGUCHI, Kyoto University

SE16-A009
Activity of Asian Consortium of Volcanology (ACV)

Eisuke FUJITA1#+, Benoit TAISNE2, Susanna JENKINS2, Christina WIDIWIJAYANTI2, Ma. Antonia BORNAS3, Hendra GUNAWAN4, Oktory PRAMBADA4, Jiandong XU5, Cheng-Horng LIN6, Ya-Chuan LAI7,8, Weiran LI9, Sung-Hyo YUN10,11, Cheolwoo CHANG12, Tomofumi KOZONO1, Takahiro MIWA1, Masato IGUCHI13
1National Research Institute for Earth Science and Disaster Resilience, 2Nanyang Technological University, 3Department of Science and Technology - Philippine Institute of Volcanology and Seismology, 4Center for Volcanology and Geological Hazard Mitigation, 5China Earthquake Administration, 6Academia Sinica, 7Taiwan Volcano Observatory - Tatun, 8National Center for Research on Earthquake Engineering, 9The University of Hong Kong, 10Pusan National University, 11Volcano Specialized Research Center / The Jeju Volcanological Institute, 12Volcano Specialized Research Center, 13Kyoto University

Asia is one of the most populated areas both in terms of human beings and volcanoes. We are always faced with violent volcanic disasters and it is necessary to coexist with volcanoes for our sustainable developments in Asian region. Therefore, we established "Asian Consortium of Volcanology" for the promotion in volcanology as well as the development of strategies for volcanic disaster prevention, through collaboration between volcanologists and authorities. ACV mainly focuses on the development and sharing the knowledge between young volcanologists. This provides a space for early career researchers to build collaborations and network with other early career, and more experienced, volcanologists across the region. ACV Field Camps have been held as: the 1st camp: Oct. 28 – Nov. 05, 2015 @Fuji, Japan, the 2nd camp: Apr. 17 – 21, 2017 @Sakurajima, Japan, the 3rd camp: Nov. 19 – 22, 2018 @Merapi, Indonesia, the 4th camp: Oct. 28 – Nov. 02, 2019 @Tatun, Taiwan, the 5th camp: Mar. 13 – 17, 2023, Izu-Oshima, Japan. The lectures, trainings and group discussions for the topics on both volcanology and countermeasure techniques are provided, as well as we experienced the field excursions at these volcanoes. Each participants make a poster presentation about his/her research at each volcano, and WOVOdat is utilized as a platform of our discussion. We welcome the Asian-Pacific colleagues to participate in this consortium and would like to promote collaborative projects in near future.


SE16-A006
Dynamics of 2010-2018 Sinabung Eruption in Indonesia: Insight from Evolution of Seismic Multi-parameters

Vico Luthfi IPMAWAN1,2#+, Masato IGUCHI1, Takahiro OHKURA1, Takeshi TAMEGURI1
1Kyoto University, 2Institut Teknologi Sumatera

Eruptive activity of Sinabung volcano is divided into 7 phases 1) phreatic (August-September 2010 and September 2013); 2) the first dome growth and collapse with PDC (18 December 2013–10 January 2014); 3) lava-flow and collapse (10 January 2014–mid-September 2014); 4) second dome growth and collapse with PDC (mid-September 2014–July 2015); 5) dominancy of Vulcanian phase with PDC (August 2015–December 2017); 6) paroxysmal event (February 19, 2018); 7) recurrence of eruption with PDC (August 2020). We analyzed seismic data from August 2010 to February 2018. The waveforms are classified into types: LF, Hybrid, VT, Rockfall, Gas Emissions, and PDC. In the quiescence period within phreatic phase, VT epicenters show a linear distribution that may be generated by fault activity triggered by stress from the minor magma intrusion. In June 2013, VT seismicity increased at shallow area indicating magma intrusion below the summit, followed by appearance of LF earthquake in November 2013. Magma approaching the surface causes the release of gas. This leakage of gas may make increasing in magma viscosity resulting in lava dome growth associated with an increase in Hybrid earthquakes. Hybrid seismicity became dominant. A decrease in stress drop of Hybrid occurs and we interpreted it as a result of pressure release due to lava dome extrusion. In January and February 2014, magmatic activity was highest, characterized by high rockfall and PDC events activity. The following month until September 2014, the process of magma transport and lava extrusion occurred indicated by an increase in RSAM of <5 Hz. The formation of plugs with lower density in the second of dome growth may be difficult to allow higher pressures to accumulate and may cause a decrease in Hybrid's seismic moment and stress drop compared to the first one.


SE16-A002
Development and Implementation of a Multi-channeled Seismometer System with Phase-shifted Optical Interferometry for Volcanological Observations

Haruhisa NAKAMICHI1#+, Yoshiharu HIRAYAMA2
1Kyoto University, 2Hakusan Corporation

It is necessary to monitor volcanoes for stable operation of seismic observation equipment over time as the equipment may fail because of lightning or high temperatures. In addition, when an electric wire from the ground sensor is connected to the recording equipment, the effect of the lightning surge is obvious in the seismic records. Lightning device failures and lightning-surge noise contamination are unavoidable as long as electric wires are used. Optical fibers have recently been used for seismic observations without these wires. One of the methods is distributed acoustic sensing (DAS), which observes ground motion using optical fibers. In contrast, an optical sensor system using phase-shift optical interferometry was developed as a method to observe ground motion using a sensor connected to an optical fiber as a signal communication route. The DAS method measures the strain vibration in the optical cable direction, whereas the optical sensor system measures the three-component vibration of translational acceleration. We have developed an optical sensor as a seismic observation system suitable for a volcanic environment. A three-component sensor was developed that is smaller, lighter, and has a lower natural frequency than the previous one. The sensors were installed at three locations for array observation, and seismic observations at Sakurajima volcano were conducted for six months from June 2019. Earthquakes associated with 267 eruptions were recorded by the optical sensor system during the observation period, and the array analysis results showed that the seismic waves traveled from 1.6 km below sea level, just below the active crater (Nakamichi et al., 2022). A comparative observation was also conducted with a micrometer, wherein noise from lightning surges was detected but there was none in the optical sensor system (Nakamichi et al., 2022). Thus, this system was shown to be suitable for seismic observations in volcanic environments.


SE16-A001
Statistical Features of the Ground Deformation Database for Vulcanian Explosions at Sakurajima Volcano

Kyoka ISHII#+, Masato IGUCHI
Kyoto University

In order to assess ash fall hazards, it is needed to forecast the size and timing of eruptions. The probability distribution of the size and timing of eruptions would be helpful to quantify possibility of ash fall including uncertainty. Sakurajima volcano, Japan is characterized by frequent Vulcanian explosions, which can provide a huge database of eruptions. Before and after the eruption, ground deformation is typically observed, which suggests inflation and deflation of magma chamber. Therefore, this study aims to investigate the statistical feature of the ground deformation related to Vulcanian explosion that occurred at Showa and Minami-dake craters in 2009–2020, and to quantify the probability of the size and timing of the eruption. We focused on four indicators in strain records obtained at underground tunnel: duration of inflation, inflation volume, deflation volume, and deflation rate (= deflation volume/inflation volume). We made databases of these four indicators and determined the model distribution which can represent the distributions of these indicators. Candidate models are Log-logistic distribution, Weibull distribution, and Exponential distribution. The model parameters for each distribution were constrained by maximum likelihood estimation. As a result, we found that the best model for the four indicators is Log-logistic distribution regardless of crater. Log-logistic distribution is one of the common models for the repose interval of Vulcanian explosions, which suggests the existence of competing processes such as increase and decrease in pressure. Therefore, the inflation and deflation process accompanied by Vulcanian explosions at Sakurajima volcano could be controlled by a balance between pressurization and depressurization in the conduit. Moreover, model parameter k of Log-logistic distribution, which represents the regularity of deformation, temporally changed. The periods when k is high correspond to the magma intrusion period implied by long-term deformation. It suggests that a large magma supply would realize the recurrent explosions.


SE16-A011
Ashfall Hazard Curves in Areas Surrounding Izu-Oshima and Aso Volcanoes, Japan

Setsuya NAKADA1,2#+, Naomi NAGATA3, Shimpei UESAWA4, Yasuo MIYABUCHI5
1National Research Institute for Earth Scinence and Disaster Resilience, 2The University of Tokyo, 3Kokusai Kogyo Co., Ltd., 4Central Research Institute of Electric Power Industry, 5Kumamoto University

When there are sufficient data on ash distribution for historical eruptions, such as those at Izu-Oshima and Aso volcanoes in Japan, it would be possible to assess ashfall hazard quantitatively at various locations at each volcano. Here, we adapt Yang and Bursik’s (2016) method for volcanic ash thickness data from abundant discrete stations to automatically create ash fall contour maps for each eruption event and to determine the ash thickness at any given point and the eruption volume of each event. From real-time data on ashfall during and soon after the eruption, automatic thickness contours and total eruption volumes can be computed independent on the personal skill of the geologist. By overlaying recent ashfall data, ashfall hazard curves (annual exceedance frequency vs. ash thickness) at arbitrary points can be obtained. This makes it possible for decision makers to plan evacuation measures and installation of infrastructure facilities to minimize ashfall damage for future volcanic eruption. For Izu-Oshima volcano, we used ashfall data for about 25 eruptions for the last 1500 years by Koyama and Hayakawa (1996), and for Aso volcano, we used ashfall values of more than 50 eruptions up to the last few tens of thousands of years ago from the original data of publications by Miyabuchi and others. For Izu-Oshima, the data covers almost all eruptions, so that hazard curves can be properly drawn and useful information on evacuation routes and locations of infrastructure facilities can be obtained. In the case of Aso, however, the probability assessment cannot be done simply because it goes back to old times and lacks data on smaller eruptions in those times. There, it is necessary to create the hazard curves by taking into account time and eruption scales.


SE16-A010
Synergistic Approach to Robustly Reconstruct Eruption Plume Dynamics: Application to Campi Flegrei

Beatriz MARTINEZ MONTESINOS1#+, Yujiro SUZUKI1, Antonio COSTA2, Leonardo MINGARI3
1The University of Tokyo, 2Istituto Nazionale di Geofisica e Vulcanologia, 3Consejo Superior de Investigaciones Científicas

Explosive volcanic eruptions can inject high quantities of magmatic materials into the atmosphere representing a risk for life and society. Atmospheric dispersal models are commonly used to forecast the impact on an eruption providing important information for civil protection, government agencies and other interested stakeholders. As input for the computation of numerical simulations these models need eruption source parameters (ESPs) and empirical constants whose goodness increases with the knowledge of the dynamics of eruption columns. For old eruptions, for which there are no monitoring observations, ESPs can be estimated by applying inversion methods to the tephra deposits volume obtained from field work. Campi Flegrei (CF) caldera, in Italy, has generated several explosive eruptions in the recent geological times, including the ~39 ka Campanian Ignimbrite (CI) super-eruption that is the largest explosive eruption in Europe in the last 200 ka, for which several outcrops are available in the region. CF is currently a densely populated area under busy air traffic routes where the monitoring system of the Vesuvius Observatory highlights some variations in the state of the volcanic activity. An eruption there would have a major impact on human life and health, air traffic, and infrastructure. Enhanced ESPs enable better assessment of volcanic hazard, which is crucial for forecasting what will happen in the next few hours when a volcano is erupting or quantifying the potential impacts of a future eruption. In this work, we use the FALL3D ash dispersal model to determine source conditions by inverting field data within an ensemble-based method, and the SK3D three-dimensional model of pseudo-gas and marker particles to resolve the volcanic plume. The estimation of the ESPs obtained from one approach is used in the other to better reconstruct the eruption plume dynamics of the Plinian and co-ignimbrite phases of the CI super-eruption.