*ALEXEI DMITRIEV1,2、S.O. Adamson3、A.A. Berlin4、Y.A. Dyakov5、L.V. Eppelbaum6、G.V. Golubkov3,5、A.A. Lushnikov6、M.I. Manzhelii7、M.G. Golubkov3 (1.Institute of Space Science and Engineering, National Central University, Jungli City, Taiwan、2.Skobeltsyn Institute of Nuclear Physics, Lomonosov Moscow State University, Moscow, Russia、3.Semenov Federal Research Center for Chemical Physics, Russian Academy of Sciences, Moscow 119991, Russian Federation 、4.Department of Earth Sciences, Tel Aviv University, Tel Aviv 69978, Israel、5.National Research Center “Kurchatov Institute”, Moscow 123182, Russian Federation、6.Geophysical Center, Russian Academy of Sciences, Moscow 119296, Russian Federation、7.Center for Chemical Physics of Atmosphere, Moscow 119991, Russian Federation)
セッション情報
[E] ポスター発表
セッション記号 P (宇宙惑星科学) » P-EM 太陽地球系科学・宇宙電磁気学・宇宙環境
[P-EM12] 大気圏ー電離圏結合
コンビーナ:Huixin Liu(九州大学理学研究院地球惑星科学専攻 九州大学宙空環境研究センター)、大塚 雄一(名古屋大学宇宙地球環境研究所)、Yue Deng(University of Texas at Arlington)、Loren Chang(Institute of Space Science, National Central University)
The Atmosphere-Ionosphere (A-I) system forms the so-called near-Earth space. Recent rapidly expanding use of satellite constellations in Low-Earth Orbit (LEO) drives a high demand for better understanding and accurate forecast of the global A-I system for scientific and operational purposes. This session aims to provide a forum for research advances and frontiers related to these aspects, and we invite presentations on global A-I coupling at all temporal and spatial scales. This includes but is not limited to: A-I coupling via atmospheric waves (tides, gravity waves, planetary waves) and trace gases (CO2, O3, H2O), A-I response to Space Weather events (solar flares, CMEs, CIRs), polar-equatorial or inter-hemispheric coupling via TADs/TIDs/disturbance dynamo/penetration electric field, ionospheric plasma irregularities, ionospheric currents, etc. Observations, theoretical studies, model simulations, data assimilation, instruments development are all highly welcome.
*楊 時賢1、Pan Chen-Jeih1、Das Uma2、林 千喬3 (1.國立中央大學、2.Department of Physics, Indian Institute of Information Technology, India、3.長榮大學)
*Chen-Jeih Pan1、Shih-Sian Yang1、Uma Das2、Wei-Sheng Chen1 (1.Institute of Space Science, National Central University, Taiwan、2.Department of Physics, Indian Institute of Information Technology, India)
*Chaosong Huang1 (1.Air Force Research Laboratory Albuquerque)
*Ravil Rakhmatulin1 (1.Institute of Solar-Terrestrial Physics, SB RAS)
*渡邊 太郎1、柿並 義宏2、山本 真行1、Miguel Larsen3、Mark Conde4、佐藤 隆雄2、嘉賀 雄一2、嘉賀 多賀子2 (1.高知工科大学、2.北海道情報大学、3.クレムソン大学、4.アラスカ大学)
*Nur Izzati Mohd Rosli1、Nurul Shazana Abdul Hamid1、Mardina Abdullah1、Akimasa Yoshikawa2、Teiji Uozumi2 (1.Universiti Kebangsaan Malaysia、2.Kyushu University)
*馬 冠一1、Li Qi1、丸山 隆2,1、Li Jinghua1、Wan Qingtao1、Wang Xiaolan1、Fan Jiangtao1、Zhang Jie1 (1.中国科学院国家天文台、2.情報通信研究機構)
*Philippe Baron1、Satoshi Ochiai1、Hideo Sagawa2、Akinori Saito3、Takatoshi Sakazaki3、Masato Shiotani3、Makoto Suzuki4 (1.National Institute of Information and Communications Technology、2.Kyoto Sangyo University、3.Kyoto University、4.Japan Aerospace Exploration Agency)
Innokentiy Alexeevich Golikov1、Artem Yurevich Gololobov2、*Ilia Ilyich Varlamov1,2 (1.Yu.G.Shafer Institute of Cosmophysical Research and Aeronomy (IKFIA), Siberian Branch of the Russian Academy of Sciences、2.M. K. Ammosov Northeastern Federal University (NEFU),)
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*Tsai-Ju Yu1、Loren C. Chang1、Jann-Yenq Liu1、Tung-Yuan Hsiao2 (1.Graduate Institute of Space Science and Engineering, National Central University, Taoyuan City, Taiwan、2.Accelerator Laboratory, Nuclear Science and Technology Development Center, National Tsing Hua University, Hsinchu, Taiwan)
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*Nakayama Sayuka 1、Liu Huixin1 (1.Earth and planetary science division,Kyushu university,Japan)
*Michi Nishioka1、Hideo MAENO1、Hiroyuki YAMAKAWA1、Takumi Kondo1、Takuya Tsugawa1、Mamoru Ishii1 (1.National Institute of Information and Communications Technology)