JpGU Meeting 2020
Session outline| Space and Planetary Sciences(P) | ||
|---|---|---|
| Session Sub-category | Solar-Terrestrial Sciences, Space Electromagnetism & Space Environment(EM) | |
| Session ID | P-EM19 | |
| Title | Dynamics of the Inner Magnetospheric System | |
| Short Title | Inner Magnetospheric System | |
| Main Convener | Name | Kunihiro Keika |
| Affiliation | Department of Earth and Planetary Science, Graduate School of Science, The University of Tokyo | |
| Co-Convener 1 | Name | Aleksandr Y Ukhorskiy |
| Affiliation | Johns Hopkins University Applied Physics Laboratory | |
| Co-Convener 2 | Name | Yoshizumi Miyoshi |
| Affiliation | Institute for Space-Earth Environmental Research, Nagoya University | |
| Co-Convener 3 | Name | Lynn M Kistler |
| Affiliation | University of New Hampshire Main Campus | |
| Session Language | E | |
| Scope | 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. | |
| Presentation Format | Oral and Poster presentation | |