Session Details
[P-EM10]Space Weather and Space Climate
Tue. May 27, 2025 5:15 PM - 7:15 PM JST
Tue. May 27, 2025 8:15 AM - 10:15 AM UTC
Tue. May 27, 2025 8:15 AM - 10:15 AM UTC
Poster Hall Exhibition Hall 7&8, Makuhari Messe
convener:Ryuho Kataoka(National Institute of Polar Research), Antti Pulkkinen(NASA Goddard Space Flight Center), Mary Aronne(NASA GSFC/CUA), Yumi Bamba(National Institute of Information and Communications Technology)
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.
[PEM10-P01]Characteristics of Magnetic Field Evolution and Onset Process of Successive X-class Flares in May 2024
*Yumi Bamba1, Kanya Kusano2, Daikou Shiota1 (1.National Institute of Information and Communications Technology, 2.Institute for Space-Eearth Environmental Research, Nagoya University)
[PEM10-P02]Statistical study of prominence eruptions observed with Nobeyama Radioheliograph
*Satoshi Masuda1, Shoya Ueda1, Seiji Yashiro2,3 (1.Institute for Space-Earth Environmental Research, Nagoya University, 2.The Catholic University of America, 3.NASA/GSFC)
[PEM10-P03]Autoencoder-Based Detection of Anomalous Stokes V Spectra in the Flare-Producing Active Region 13663 Using Hinode/SP Observations
*Jargalmaa Batmunkh1, Yusuke Iida1, Takayoshi Oba2 (1.Niigata University, 2.Max Planck Institute for Solar System Research)
[PEM10-P04]Development of a Solar Flare Prediction Model Using Feature Compression Method and Weighted Images
*Kosuke Asatsuma1, Yusuke Iida1, Tomoki Kubo1 (1.Niigata University)
[PEM10-P05]Development of Classification and Regression Models for SEP Events Forecasting with Machine/Deep Learning Methods
*Yuta Kato1,2, Kanya Kusano2, Naho Fujita1, Kentaro Doi1, Akira Tsuda1, Hiroyuki Kawasaki1, Tomoki Moriyama2, Tomoki Kubo3, Chihiro Mitsuda1,2 (1.Fujitsu Limited, 2.Institute for Space–Earth Environmental Research, Nagoya University, 3.Graduate School of Science and Technology, Electrical and Information Engineering, Niigata University)
[PEM10-P06]Development of Multi-Hierarchy Simulation Code KAMMUY and its Application to Understanding Cross-Scale Coupling in Magnetic Reconnection
*Keita Akutagawa1, Shinsuke Imada1, Munehito Shoda1 (1.The University of Tokyo)
[PEM10-P07]Development of Compact magnetogram using polarized imaging sensor for space weather monitoring
*Park Inchun1, Kenichi Otsuji1, Satoshi Morita1, Daikou Shiota1, Yumi Bamba1, Tatsuki Tahara1 (1.National Institute of Information and Communications Technology)
[PEM10-P08]Interaction among multiple CMEs to result in May 2024 Superstorm
*Daikou Shiota1, Seiji Yashiro2, Kazumasa Iwai3 (1.National Institute of Information and Communications Technology (NICT), 2.Catholic University of America, 3.Institute for Space–Earth Environmental Research, Nagoya University)
[PEM10-P09]IMAP I-ALiRT: An Expanded Dataset for Space Weather Forecasting
*Kristopher William Larsen1, Laura Sandoval1, Tori Marbois1, Greg Lucas1 (1.Laboratory for Atmospheric and Space Physics)
[PEM10-P10]Plasmaspheric Electron Content Contribution to Total Electron Content: Insights from Ground-Based and FORMOSAT-3/COSMIC Radio Occultation Data
*Chun-Yen Huang1, Jann-Yenq G Liu2, CHIYEN LIN2, Tatsuhiro Yokoyama1 (1.Research Institute for sustainable humanosphere, Kyoto University, 2.National Central University, Taiwan)
[PEM10-P11]Ionospheric scintillation and geomagnetic disturbance caused by space hurricanes
*Sheng Lu1, Zan-Yang Xing1, Qing-He Zhang2,1, Yong-Liang Zhang3, Hui-Gen Yang1,4, Kjellmar Oksavik5,6, L. R. Lyons7, Kazuo Shiokawa8, Yong Wang1, Yu-Zhang Ma1, Xiang-Yu Wang1, Zhong-Xin Deng9, Tong Xu9, Duan Zhang2, Guo-Jun Li10 (1.Shandong Provincial Key Laboratory of Optical Astronomy and Solar-Terrestrial Environment, Institute of Space Sciences, Shandong University, Weihai, China. , 2.State Key Laboratory of Space Weather, Center for Space Science and Applied Research, Chinese Academy of Sciences, Beijing, China., 3.Applied Physics Laboratory, The Johns Hopkins University, Laurel, Maryland, USA, 4.Polar Research Institute of China, Shanghai, China., 5.Department of Physics and Technology, University of Bergen, Bergen, Norway. , 6.Arctic Geophysics, University Centre in Svalbard, Longyearbyen, Norway., 7.Department of Atmospheric and Oceanic Sciences, University of California, CA, Los Angeles, United States, 8.Institute for Space Earth Environmental Research, Nagoya University, Nagoya, Japan., 9.China Research Institute of Radiowave Propagation, Qingdao, China., 10.Lab of BLOS Reliable Information transmission, Chongqing University of Posts and Telecommunications, Chongqing, China.)
[PEM10-P12]Development of an Automated Detection System for Satellite Surface Charging of Satellites Using DMSP Satellite ObservationData
*Masuno Hayato1, Mariko Teramoto1, Daichi Araki1, Yusuke Iida2, Akitoshi Hanazawa1, Tomoya Iwase1, Kentarou Kitamura1, Teppei Okumura3, Kiyokazu Koga3, Hiroyuki Okamoto3 (1.Kyushu Institute of Technology, 2.Niigata University, 3.JAXA)
[PEM10-P13]High energy particle environment at geosynchronous orbit during May 2024 severe storm event
*Tsutomu Nagatsuma1, Kaori Sakaguchi1, Yuki Kubo1 (1.National Institute of Information and Communications Technology)
[PEM10-P14]Development status of the geostationary orbit high energy proton flux measurement instrument (RMS-p) IV
*Kenichi Otsuji1, Kaori Sakaguchi1,2, Shinji Saito1, Taku Namekawa1, Park Inchun1, Takefumi Mitani3, Shin-ichiro Meigo4, Yuji Yamaguchi4 (1.National Institute of Information and Communications Technology, 2.Ministry of Internal Affairs and Communications, 3.Japan Aerospace Exploration Agency, Institute of Space and Astronautical Science, 4.Japan Atomic Energy Agency, J-PARC)
[PEM10-P15]Comparison of two methods of auroral altitude estimation based on two-point observations
*Kyutaro Yanagisawa1, Daniel Whiter2, Ryuho Kataoka3, Kanako Seki1, Yoshizumi Miyoshi4, Kazuo Shiokawa4, Martin G Connors5, Satoshi Nakahira6, Shoji Torii7 (1.Graduate School of Science, University of Tokyo, 2.School of Physics & Astronomy, University of Southampton, 3.National Institue of Polar Research, 4.Institue for Space-Earth Environmental Research, Nagoya university, 5.Athabasca university, 6.Japan Aerospace eXploration Agency, 7.Waseda Research Institute for Science and Engineering)
[PEM10-P16]UT dependence of severe space weather event defined by geomagnetic indices: another unusual aspect of the May 2024 event
Masatoshi Yamauchi2, *Tsubasa Kotani1, Sota Nanjo2, Jürgen Matzka3 (1.Data Analysis Center for Geomagnetism and Space Magnetism, Graduate Schoold of Science, Kyoto University, Kyoto, Japan, 2.Swedish Institute of Space Physics, Kiruna, Sweden, 3.GFZ Helmholtz Centre for Geosciences, Potsdam, Germany )
[PEM10-P17]Statistical analysis of geomagnetically induced current data measured around Tokyo
*Shinichi Watari, Yusuke Ebihara1, Aoi Nakamizo2 (1.Research Institute for Sustainable Humanosphere, Kyoto University, 2.National Institute of Information and Communications Technology)
[PEM10-P18]Forecast of CIR-driven geomagnetic storms using the deep neural networks
*Naoko Takahashi1, Naoto Nishizuka1 (1.National Institute of Information and Communications Technology)
[PEM10-P19]Ionospheric space weather forecast by the data assimilation of SuperDARN data with AI emulator
*Ryuho Kataoka1, Shin ya Nakano2, Shigeru Fujita2, Aoi Nakamizo3 (1.National Institute of Polar Research, 2.The Institute of Statistical Mathematics, 3.National Institute of Information and Communications Techonology)
[PEM10-P20]Education of Observation and Data Processing with a Digital Image-Recording Soda Bottle Magnetometer
*Shun Imajo1 (1.Data Analysis Center for Geomagnetism and Space Magnetism, Graduate School of Science, Kyoto University)
[PEM10-P21]Variations in the ozone concentration in the mesosphere observed at Syowa Station associated with energetic particle precipitation
Hikaru Suzuki1, *Fuminori Tsuchiya1, Akira Mizuno2, Isao Murata1, Yasumasa Kasaba1, Tomoo Nagahama2, Hirofumi Goto2, Masaki Tsutsumi3, Yoshihiro Tomikawa3, Kaoru Sato4, Atsuki Shinbori2 (1.Tohoku University, 2.Nagoya University, 3.NIPR, 4.The University of Tokyo)
[PEM10-P22]Statistical study of the relationship between NO variability and magnetospheric activities/energetic particles based on mm-wave observations at Syowa Station
*Akira Mizuno1, Hirofumi Goto1, Tomoo Nagahama1, Tac Nakajima1, Ryuho Kataoka2, Yoshimasa Tanaka2, Mitsumu K. Ejiri2, Yoshihiro Tomikawa2, Fuminori Tsuchiya3 (1.Institute for Space-Earth Environmental Research, Nagoya University, 2.National Institute of Polar Research, 3.Tohoku University)
[PEM10-P23]New observation with a full-scale muon detector at Syowa Station, Antarctic
*Yuki Hayashi1,2, Chihiro Kato1, Ryuho Kataoka2,3, Shoko Miyake4, Masayoshi Kozai5, Akira Kadokura5,2, Kazuoki Munakata1 (1.Shinshu University, 2.National Institute of Polar Research, 3.Polar Science Program, Graduate Institute for Advanced Students, SOKENDAI, 4.Department of Electrical and Computer Engineering, National Institution of Technology (KOSEN), Gifu, 5.Polar Environment Data Science Center, Joint Support-Center for Data Science Research, Research Organization of Information and Systems)
[PEM10-P24]Development and Evaluation of Ionospheric Data Assimilation Model Using GAIA
*Hidekatsu Jin1, Satoshi Andoh1, Chihiro Tao1, Yasunobu Miyoshi2, Hiroyuki Shinagawa1, Hitoshi Fujiwara3 (1.National Institude of Information and Communications Technology, 2.Kyushu University, 3.Seikei University)
[PEM10-P25]Ionospheric Changes over the Western Pacific Ocean near and after the End of Annular Solar Eclipse on 21 June 2020
*Jin Wang1, Yang-Yi Sun1 (1.China University of Geosciences (Wuhan))
[PEM10-P26]Simultaneous observation of the time of flight and the Doppler frequency shift of each HF wave refracted in the ionosphere
*Takashi Iwamoto1, Mao Konishi1 (1.Advanced Technology R and D Center, Mitsubishi Electric Corporation)