2022年5月25日(水) 10:45 〜 12:15
303 (幕張メッセ国際会議場)
コンビーナ:桂華 邦裕(東京大学大学院理学系研究科地球惑星科学専攻)、コンビーナ:三好 由純(名古屋大学宇宙地球環境研究所)、Blum Lauren W(University of Colorado Boulder)、コンビーナ:Shprits Yuri(Helmholtz Centre Potsdam GFZ German Research Centre for Geosciences)、座長:謝 怡凱(京都大学生存圏研究所)、桂華 邦裕(東京大学大学院理学系研究科地球惑星科学専攻)
The inner magnetosphere is highly variable due to dynamic variations of energy input from the solar wind through the magnetotail and plasma supply from the ionosphere. Cross-regional, cross-scale, and cross-energy couplings are the key processes for understanding this dynamic system. Coordinated observations by multi-satellites and ground-based observations are very essential to revealing these processes. In the 24th and 25th solar cycles, a number of satellites (Van Allen Probes, MMS, THEMIS, DSX, Arase, etc.), coordinated ground-based observations (THEMIS-GBO, SuperDARN, EISCAT, magnetometers, riometer, etc), and numerical simulations (global kinetic model, MHD model, micro PIC, hybrid simulations, etc.) have successfully investigated the inner magnetosphere system. We invite papers on recent results of the inner magnetosphere and its couplings/connections with the other regions including the ionosphere and the outer magnetosphere. Papers on new projects (sounding rocket experiments, data assimilation/machine learning, etc.) and future spacecraft missions are also welcome.