Kristina Shizuka Yamase Skarvang2、*Patrick J Espy1、Robert E. Hibbins1、Willem E. van Caspel1 (1.Norwegian Univ. of Science and Technology, Birkeland Centre for Space Science、2.Norwegian Univ. of Science and Technology)
セッション情報
[E] 口頭発表
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.
[PEM12-02] Dynamical characteristics of the middle atmosphere associated with the Antarctic sudden stratospheric warming in 2019.
★Invited Papers
[PEM12-03] WACCMX Simulations of the 2002 and 2019 Southern Hemisphere Sudden Stratospheric Warmings
★Invited Papers
*Nicholas M Pedatella1 (1.National Center for Atmospheric Research)
*JING LI1、TAO LI2,3、QIAN WU4、YIHUAN TANG2、ZHAOPENG WU1,3、JUN CUI1 (1.Planetary Environmental and Astrobiological Research Laboratory (PEARL), School of Atmospheric Sciences, Sun Yat-sen University, Zhuhai, Guangdong, China、2.CAS Key Laboratory of Geospace Environment, School of Earth and Space Sciences, University of Science and Technology of China, Hefei, Anhui, China、3.CAS Center for Excellence in Comparative Planetology, Hefei, Anhui, China、4.High Altitude Observatory, National Center for Atmospheric Research, Boulder, CO, USA)
*Irina Medvedeva1,2、Konstantin Ratovsky1、Alla Suvorova3 (1.Institute of Solar-Terrestrial Physics SB RAS, Irkutsk, Russia 、2.Obukhov Institute of Atmospheric Physics RAS, Moscow, Russia 、3.GPSARC National Central University, Taoyuan, Taiwan)
*Jia-Ting Lin1、Charles Lin1、Loren Chang2,3、Hanli Liu4、Nicholas M Pedatella4,5 (1.Department of Earth Sciences, National Cheng Kung University, Taiwan、2.Center for Astronautical Physics and Engineering, National Central University, Taoyuan, Taiwan、3.Graduate Institute of Space Science, National Central University, Taoyuan, Taiwan、4.High Altitude Observatory, National Center for Atmospheric Research, Boulder, CO, USA、5.COSMIC Program Office, University Corporation for Atmospheric Research, Boulder, CO, USA)