[E] Oral
P (Space and Planetary Sciences ) » P-EM Solar-Terrestrial Sciences, Space Electromagnetism & Space Environment
convener:Kunihiro Keika(Department of Earth and Planetary Science, Graduate School of Science, The University of Tokyo ), Aleksandr Y Ukhorskiy(Johns Hopkins University Applied Physics Laboratory), Yoshizumi Miyoshi(Institute for Space-Earth Environmental Research, Nagoya University), Lynn M Kistler(University of New Hampshire Main Campus)
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.
*Milla Kalliokoski1, Emilia Kilpua1, Drew Turner2, Allison Jaynes3, Adnane Osmane1, Lucile Turc1, Harriet George1, Minna Palmroth1,4 (1.University of Helsinki, 2.Johns Hopkins University Applied Physics Laboratory, 3.University of Iowa, 4.Finnish Meteorological Institute)
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*Yikai Hsieh1, Yuko Kubota1, Yoshiharu Omura1 (1.Reserach Institute for Sustainable Humanosphere, Kyoto University)
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*Shinji Saito1, Satoshi Kurita2, Yoshizumi Miyoshi2 (1.National Institute of Information and Communications Technology, 2.ISEE, Nagoya Univ.)
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*Naoko Takahashi1, Kanako Seki1, Mei-Ching Fok2, Yihua Zheng2, Yoshizumi Miyoshi3, Satoshi Kasahara1, Kunihiro Keika1, David Hartley4, Yoshiya Kasahara5, Yasumasa Kasaba6, Nana Higashio1, Ayako Matsuoka7, Shoichiro Yokota8, Tomoaki Hori3, Iku Shinohara7 (1.Graduate School of Science, The University of Tokyo, 2.NASA Goddard Space Flight Center, 3.Institute for Space-Earth Environmental Research, Nagoya University, 4.The University of Iowa, 5.Information Media Center, Kanazawa University, 6.Planetary Plasma and Atmospheric Research Center, Tohoku University, 7.Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, 8.Graduate School of Science, Osaka University)
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*Yoshizumi Miyoshi1, Vania Jordanova2, Yuto Katoh3, Shinji Saito4, Satoshi Kurita5, Sandeep Kumar1, Yoshiya Kasahara6, Shoya Matsuda7, Masafumi Shoji1, Fuminori Tsuchiya3, Atsushi Kumamoto3, Ayako Matsuoka5, Satoshi Kasahara8, Shoichiro Yokota9, Tomoaki Hori1, Kunihiro Keika8, Yoichi Kazama10, Shiang-Yu Wang10, Chae-Woo Jun1, Takefumi Mitani7, Takeshi Takashima7, Nana Higashio7, Iku Shinohara7 (1.Institute for Space-Earth Environmental Research, Nagoya University, 2.Los Alamos National Laboratory, 3.Tohoku University, 4.NICT, 5.Kyoto University, 6.Kanazawa University, 7.JAXA, 8.The University of Tokyo, 9.Osaka University, 10.ASIAA)
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*Kirolosse Mina GIRGIS1,2, Tohru Hada3,4, Shuichi Matsukiyo3,4 (1.Department of Earth System Science and Technology (ESST), Interdisciplinary Graduate School of Engineering Sciences (IGSES), Kyushu University, Japan , 2.Aerospace Engineering Department, Faculty of Engineering, Cairo University, Egypt, 3.Department of Advanced Environmental Science and Engineering, Faculty of Engineering Sciences, Kyushu University, Japan, 4.International Center for Space Weather Science and Education (ICSWSE), Kyushu University, Japan)
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