日本地球惑星科学連合2025年大会

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[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

2025年5月25日(日) 13:45 〜 15:15 303 (幕張メッセ国際会議場)

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)、座長:大塚 雄一(名古屋大学宇宙地球環境研究所)、Irina Zakharenkova(University Corporation for Atmospheric Research)

14:15 〜 14:30

[PEM12-09] Impact of Neutral Wind Dynamo on the Magnetospheric Configuration: MHD-GCM Coupled Simulations for May 2024 Storm

*Yue Deng1 (1.University of Texas at Arlington)

キーワード:neutral wind dynamo, ionosphere and thermosphere, magnetosphere, May 2024 storm

Through the neutral wind dynamo, thermosphere generates ionospheric currents that can affect high-latitude electrodynamics, especially during intense geomagnetic storms. However, this significant effect has not been well-studied and typically has not been included in the magnetosphere-ionosphere (MI) simulations. In this study, the influences of the ionospheric current due to neutral-wind dynamo on the electrodynamics of the ionosphere-magnetosphere system have been evaluated for the May 2024 storm, using the coupled Global Ionosphere-Thermosphere Model (GITM) and the Geospace components of Space Weather Modeling Framework (SWMF). Specifically, the neutral wind-driven field-aligned currents (FACs) are combined with the magnetospheric-origin FACs to specify the high-latitude electric potential, which is imposed back into the magnetosphere. We focus on the following three aspects: 1) to compare the distribution and magnitude of neutral wind-driven FACs from GITM and the magnetospheric-origin FACs from SWMF at high latitudes; 2) to assess how the neutral wind-driven FACs affect the magnetospheric configuration and the high-latitude potential; 3) furthermore, to evaluate the relative significance between wind-driven current and magnetospheric-origin current to the geomagnetic disturbance (GMD) at middle- and low-latitudes. Our study will help to accurately simulate the physical processes in the M-I system and provide new insights for the physical processes in the magnetosphere-ionosphere-thermosphere coupled system.