Japan Geoscience Union Meeting 2024

Presentation information

[E] Oral

P (Space and Planetary Sciences ) » P-EM Solar-Terrestrial Sciences, Space Electromagnetism & Space Environment

[P-EM12] Coupling Processes in the Atmosphere-Ionosphere System

Thu. May 30, 2024 10:45 AM - 12:00 PM Exhibition Hall Special Setting (2) (Exhibition Hall 6, Makuhari Messe)

convener:Keisuke Hosokawa(Department of Communication Engineering and Informatics, University of Electro-Communications), Huixin Liu(Earth and Planetary Science Division, Kyushu University SERC, Kyushu University), Yuichi Otsuka(Institute for Space-Earth Environmental Research, Nagoya University), Loren Chang(Department of Space Science and Engineering, National Central University), Chairperson:Jeff Klenzing(NASA Goddard Space Flight Center), Huixin Liu(Earth and Planetary Science Division, Kyushu University SERC, Kyushu University)

10:45 AM - 11:00 AM

[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)

Keywords: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.