日本地球惑星科学連合2024年大会

講演情報

[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] Coupling Processes in the Atmosphere-Ionosphere System

2024年5月30日(木) 10:45 〜 12:00 展示場特設会場 (2) (幕張メッセ国際展示場 6ホール)

コンビーナ:細川 敬祐(電気通信大学大学院情報理工学研究科)、Liu Huixin(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)、Chang Loren(Institute of Space Science, National Central University)、Chairperson:Jeff Klenzing(NASA Goddard Space Flight Center)、Liu Huixin(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)

10:45 〜 11:00

[PEM12-06] Scientific advances from the Center for Geospace Storms

★Invited Papers

*Viacheslav G Merkin1、Dong Lin2、Kevin Pham2、Kareem Sorathia1、Shanshan Bao3、Anthony Sciola1、Roger Varney4、Joe Huba5、Wenbin Wang2、Michael Wiltberger2 (1.Johns Hopkins University Applied Physics Laboratory、2.National Center for Atmospheric Research、3.Rice University、4.University of California, Los Angeles、5.Syntek Technologies)

キーワード:geomagnetic storms, center for geospace storms, stormtime geospace, NASA DRIVE

The Center for Geospace Storms (CGS) is one of the three NASA DRIVE Science Centers currently in Phase II, and it is the only one focusing on the physics of geospace. CGS science is rooted in the understanding of stormtime geospace as a system that is highly coupled across a wide range of spatiotemporal scales. This necessitates the need for physical models that are both holistic, i.e., treat all the relevant processes and domains, and possess sufficiently high resolution to capture all the relevant scales, within the limitations of the existing computer power. To this end, CGS is developing a Multiscale Atmosphere-Geospace Environment (MAGE) model that satisfies the above requirements. In this presentation, we review the recent work by the CGS team, using both the MAGE model and accompanying observations, concentrating on the multiscale nature of stormtime interactions in the geospace system. The highlights include the recent work by the CGS team highlighting the importance of realistic physics-based high- and mid-latitude driving of the ionosphere-atmosphere system, including: energetic particle precipitation into the ionosphere; thermosphere density enhancements and travelling ionospheric and atmospheric disturbances; mesoscale polar ionosphere density structure and its implications for the global magnetosphere among others. We conclude by placing these representative cross-scale coupling processes in the context of the global mass and energy redistribution characteristic of stormtime geospace dynamics.