Space and Planetary Sciences (P) | ||
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Session Sub-category | Solar-Terrestrial Sciences, Space Electromagnetism & Space Environment(EM) | |
Session ID | P-EM10 | |
Title | Space Weather and Space Climate | |
Short Title | Space Weather and Space Climate | |
Main Convener | Name | Ryuho Kataoka |
Affiliation | National Institute of Polar Research | |
Co-Convener 1 | Name | Antti Pulkkinen |
Affiliation | NASA Goddard Space Flight Center | |
Co-Convener 2 | Name | Mary Aronne |
Affiliation | NASA GSFC/CUA | |
Co-Convener 3 | Name | Yumi Bamba |
Affiliation | National Institute of Information and Communications Technology | |
Session Language |
E |
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Scope |
We share the latest scientific papers to understand how the space environment changes in various time scales and to discuss how we will react via international and interdisciplinary collaborations. More specifically, welcomed papers include space climate studies to reconstruct the long-term variations; cutting-edge observational and modeling studies of space weather from the Sun to surface of the Earth; applied science such as operational space weather forecast using machine-learning techniques and hazard assessments for deep space human spaceflight activities at Moon and at Mars. |
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Presentation Format | Oral and Poster presentation | |
Joint Session with | AGU | |
Invited Authors |
James F Spann (NOAA NESDIS Office of Space Weather Observation) Maria M Kuznetsova (NASA Goddard Space Flight Center) Larisza D Krista (University of Colorado Boulder) Haruhisa Iijima (Institute for Space-Earth Environmental Research, Nagoya University) Yoshizumi Miyoshi (Institute for Space-Earth Environmental Research, Nagoya University) Naoyuki Takeuchi (Kyoto Univesity) |
Time | Presentation No | Title | Presenter |
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Oral Presentation May 27 AM1 | |||
9:00 - 9:15 | PEM10-01 | Space Weather at NOAA | James F Spann |
9:15 - 9:30 | PEM10-02 | Status of ICAO space weather information services | Mamoru Ishii |
9:30 - 9:45 | PEM10-03 | NASA GSFC Space Weather Priorities and Activities | Antti Pulkkinen |
9:45 - 10:00 | PEM10-04 | Community Coordinated Modeling Center Efforts to Advance Space Weather Predictive Capabilities and to Improve Research-to-Operations Pipeline. | Maria M Kuznetsova |
10:00 - 10:15 | PEM10-05 | Moon to Mars Space Weather Analysis Office: Activities Supporting Exploration Throughout the Solar System | Mary Aronne |
10:15 - 10:30 | PEM10-06 | New space weather alert considering social impact and space weather information usage guideline | Takuya Tsugawa |
Oral Presentation May 27 AM2 | |||
10:45 - 11:00 | PEM10-07 | Investigating Coronal Dimmings and EUV Flare Precursors for Improved Space Weather Forecasting | Larisza D Krista |
11:00 - 11:15 | PEM10-08 | Implementation of a physics-based flare prediction model κ-scheme to operational space weather forecasting in NICT | Yumi Bamba |
11:15 - 11:30 | PEM10-09 | CME Velocity Estimations from Solar Radio Bursts Observed in 2024-2025 | Naoto Nishizuka |
11:30 - 11:45 | PEM10-10 | Predicting Extreme Solar Energetic Particle Events with a Transformer Network | Si Chen |
11:45 - 12:00 | PEM10-11 | Top 57 Major Forbush Decrease Events Observed by the Nagoya Muon Detector (1976–2024) | Chihiro Kato |
12:00 - 12:15 | PEM10-12 | Tracing Evidence of the Young Sun's Magnetic Activity from the Lunar South Pole Regolith | Emika Fujii |
Oral Presentation May 27 PM1 | |||
13:45 - 14:00 | PEM10-13 | The effect of expansion factor in intermediate region on solar wind speed | Tokoro Kyogo |
14:00 - 14:15 | PEM10-14 | Radiative Magnetohydrodynamic Modeling of the Solar Wind and Interplanetary Magnetic Field Incorporating Small-Scale Interchange Reconnection | Haruhisa Iijima |
14:15 - 14:30 | PEM10-15 | Relationship between Evolution of IMF and Solar Magnetic Field in Solar Cycles 21-25 | Minami Yoshida |
14:30 - 14:45 | PEM10-16 | Spatio-Temporal Evolution of Solar Plasma Ejecta Approaching from a Multi-Point Comparison of Galactic Cosmic Ray Variations | Gaku Kinoshita |
14:45 - 15:00 | PEM10-17 | Radiation Monitors for Space weather (RMS): Introduction and development status | Shinji Saito |
15:00 - 15:15 | PEM10-18 | The Deep Space Radiation Probe: Development and First Results from a First Lunar Science Payload for Space Environment Studies and Capacity Building | Loren Chang |
Oral Presentation May 27 PM2 | |||
15:30 - 15:45 | PEM10-19 | Observational Results of Space Energetic Particles from the Fengyun-3E Polar Orbit Satellite | chunqin wang |
15:45 - 16:00 | PEM10-20 | Statistical Insights into Surface Charging Events and Plasma Environment in the Inner Magnetosphere | Masao Nakamura |
16:00 - 16:15 | PEM10-21 | Low-latitude auroral appearance associated with compressed magnetosphere as revealed by citizen science | Tomohiro M. Nakayama |
16:15 - 16:30 | PEM10-22 | Improving Predictions of Geomagnetic Storms | Nariaki Nitta |
16:30 - 16:45 | PEM10-23 | Citizen science and Bayes inference of auroral oval evolution during super storms | Ryuho Kataoka |
16:45 - 17:00 | PEM10-24 | Geospace response to the May 2024 geomagnetic storm: Insights from Arase observations | Yoshizumi Miyoshi |
Oral Presentation May 28 PM1 | |||
13:45 - 14:00 | PEM10-25 | Global Distribution of the Martian Nightside Ionosphere and Its Response to Space Weather and Crustal Magnetic Fields Based on MEX and MAVEN Observations | Naoyuki Takeuchi |
14:00 - 14:15 | PEM10-26 | Ionospheric convection associated with low-latitude auroras | Nozomu Nishitani |
14:15 - 14:30 | PEM10-27 | Electron Density Variations and the Short-wave Fadeout During X-Class Solar Flares in May 2024 Using PHITS | Shinnosuke Kitajima |
14:30 - 14:45 | PEM10-28 | Features of ionospheric irregularities during geomagnetic storms in 25th solar maximum revealed by GNSS ROTI maps | Iurii Cherniak |
14:45 - 15:00 | PEM10-29 | Prosecces of Earth's Atmospheric Expansion Caused by Solar Activity and Its effect on Orbits of CubeSats | Hayato Tanaka |
15:00 - 15:15 | PEM10-30 | Triple Ionosophere PhotoMeter onboard Fengyun-3E satellite: Data validation and ionosphere information extraction | fang jiang |
Presentation No | Title | Presenter |
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Poster Presentation May 27 PM3 | ||
PEM10-P01 | Characteristics of Magnetic Field Evolution and Onset Process of Successive X-class Flares in May 2024 | Yumi Bamba |
PEM10-P02 | Statistical study of prominence eruptions observed with Nobeyama Radioheliograph | Satoshi Masuda |
PEM10-P03 | Autoencoder-Based Detection of Anomalous Stokes V Spectra in the Flare-Producing Active Region 13663 Using Hinode/SP Observations | Jargalmaa Batmunkh |
PEM10-P04 | Development of a Solar Flare Prediction Model Using Feature Compression Method and Weighted Images | Kosuke Asatsuma |
PEM10-P05 | Development of Classification and Regression Models for SEP Events Forecasting with Machine/Deep Learning Methods | Yuta Kato |
PEM10-P06 | Development of Multi-Hierarchy Simulation Code KAMMUY and its Application to Understanding Cross-Scale Coupling in Magnetic Reconnection | Keita Akutagawa |
PEM10-P07 | Development of Compact magnetogram using polarized imaging sensor for space weather monitoring | Park Inchun |
PEM10-P08 | Interaction among multiple CMEs to result in May 2024 Superstorm | Daikou Shiota |
PEM10-P09 | IMAP I-ALiRT: An Expanded Dataset for Space Weather Forecasting | Kristopher William Larsen |
PEM10-P10 | Plasmaspheric Electron Content Contribution to Total Electron Content: Insights from Ground-Based and FORMOSAT-3/COSMIC Radio Occultation Data | Chun-Yen Huang |
PEM10-P11 | Ionospheric scintillation and geomagnetic disturbance caused by space hurricanes | Sheng Lu |
PEM10-P12 | Development of an Automated Detection System for Satellite Surface Charging of Satellites Using DMSP Satellite ObservationData | Masuno Hayato |
PEM10-P13 | High energy particle environment at geosynchronous orbit during May 2024 severe storm event | Tsutomu Nagatsuma |
PEM10-P14 | Development status of the geostationary orbit high energy proton flux measurement instrument (RMS-p) IV | Kenichi Otsuji |
PEM10-P15 | Comparison of two methods of auroral altitude estimation based on two-point observations | Kyutaro Yanagisawa |
PEM10-P16 | UT dependence of severe space weather event defined by geomagnetic indices: another unusual aspect of the May 2024 event | Tsubasa Kotani |
PEM10-P17 | Statistical analysis of geomagnetically induced current data measured around Tokyo | Shinichi Watari |
PEM10-P18 | Forecast of CIR-driven geomagnetic storms using the deep neural networks | Naoko Takahashi |
PEM10-P19 | Ionospheric space weather forecast by the data assimilation of SuperDARN data with AI emulator | Ryuho Kataoka |
PEM10-P20 | Education of Observation and Data Processing with a Digital Image-Recording Soda Bottle Magnetometer | Shun Imajo |
PEM10-P21 | Variations in the ozone concentration in the mesosphere observed at Syowa Station associated with energetic particle precipitation | Fuminori Tsuchiya |
PEM10-P22 | Statistical study of the relationship between NO variability and magnetospheric activities/energetic particles based on mm-wave observations at Syowa Station | Akira Mizuno |
PEM10-P23 | New observation with a full-scale muon detector at Syowa Station, Antarctic | Yuki Hayashi |
PEM10-P24 | Development and Evaluation of Ionospheric Data Assimilation Model Using GAIA | Hidekatsu Jin |
PEM10-P25 | Ionospheric Changes over the Western Pacific Ocean near and after the End of Annular Solar Eclipse on 21 June 2020 | Jin Wang |
PEM10-P26 | Simultaneous observation of the time of flight and the Doppler frequency shift of each HF wave refracted in the ionosphere | Takashi Iwamoto |