宇宙惑星科学(P)
セッション小記号太陽地球系科学・宇宙電磁気学・宇宙環境(EM)
セッションIDP-EM19
タイトル和文Dynamics of the Inner Magnetospheric System
英文Dynamics of the Inner Magnetospheric System
タイトル短縮名和文Inner Magnetospheric System
英文Inner Magnetospheric System
代表コンビーナ氏名和文桂華 邦裕
英文Kunihiro Keika
所属和文東京大学大学院理学系研究科地球惑星科学専攻
英文Department of Earth and Planetary Science, Graduate School of Science, The University of Tokyo
共同コンビーナ 1氏名和文Aleksandr Y Ukhorskiy
英文Aleksandr Y Ukhorskiy
所属和文Johns Hopkins University Applied Physics Laboratory
英文Johns Hopkins University Applied Physics Laboratory
共同コンビーナ 2氏名和文三好 由純
英文Yoshizumi Miyoshi
所属和文名古屋大学宇宙地球環境研究所
英文Institute for Space-Earth Environmental Research, Nagoya University
共同コンビーナ 3氏名和文Lynn M Kistler
英文Lynn M Kistler
所属和文University of New Hampshire Main Campus
英文University of New Hampshire Main Campus
発表言語E
スコープ和文The inner magnetosphere is highly variable because dynamical
variations of incoming energy from the solar wind, magnetospheric tail,
and the ionosphere. Cross-regional/cross-scale/cross-energy couplings
are key processes to understand this dynamical system, and coordinated
observations by multi-satellites and ground-based observations are
very essential to reveal these processes. In the 24th solar cycle,
a number of satellites such as Van Allen Probes, MMS, THEMIS, DSX and
Arase, coordinated ground-based observations (THEMIS-GBO, SuperDARN,
EISCAT, magnetometers, riometer, etc), and numerical simulations
(global kinetic model, MHD model, micro PIC, hybrid simulations) have
successfully investigated the inner magnetosphere system. Papers on recent results
on the inner magnetosphere and/or its coupling with the other regions,
including the ionosphere and the outer magnetosphere are invited. And
presentations on new projects for the inner magnetosphere are also
welcome.
英文The inner magnetosphere is highly variable because dynamical
variations of incoming energy from the solar wind, magnetospheric tail,
and the ionosphere. Cross-regional/cross-scale/cross-energy couplings
are key processes to understand this dynamical system, and coordinated
observations by multi-satellites and ground-based observations are
very essential to reveal these processes. In the 24th solar cycle,
a number of satellites such as Van Allen Probes, MMS, THEMIS, DSX and
Arase, coordinated ground-based observations (THEMIS-GBO, SuperDARN,
EISCAT, magnetometers, riometer, etc), and numerical simulations
(global kinetic model, MHD model, micro PIC, hybrid simulations) have
successfully investigated the inner magnetosphere system. Papers on recent results
on the inner magnetosphere and/or its coupling with the other regions,
including the ionosphere and the outer magnetosphere are invited. And
presentations on new projects for the inner magnetosphere are also
welcome.
発表方法口頭および（または）ポスターセッション