日本地球惑星科学連合2021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-EM11] Coupling Processes in the Atmosphere-Ionosphere System

2021年6月3日(木) 09:00 〜 10:30 Ch.05 (Zoom会場05)

コンビーナ: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)、Chang Loren(Institute of Space Science, National Central University)、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)、座長: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)、木暮 優(国立極地研究所)

09:30 〜 09:45

[PEM11-03] High Resolution Ionosphere/Thermosphere Modeling Studies of Equatorial Plasma Bubbles

★Invited Papers

*Joseph Huba1、Hanli Liu、Erich Becker (1.Syntek Technologies, Inc)

キーワード:equatorial bubbles, ionosphere/thermosphere modeling

We report results from a high resolution global simulation study of the ionosphere/thermosphere system that self-consistently generates large-scale equatorial spread F (ESF) plasma bubbles. The coupled model comprises the ionospheric code SAMI3 and the atmosphere/thermosphere codes WACCM-X and HIAMCM. An important feature of the study is that a high resolution grid is used globally with scale sizes 50 km. Several cases are studied for different seasons and solar activity. We show one case that is consistent with recent GOLD observations [Huba and Liu, 2020]. In addition to seasonal and solar activity variations in the onset of ESF, we also find a strong longitudinal and day-to-day variation. Importantly, the bubbles are initiated self-consistently by atmospheric gravity waves in the WACCM-X and HIAMCM models as opposed to artificial, numerical ionosphere perturbations.

Huba, J.D. and H.-L. Liu, Global modeling of equatorial spread F with SAMI3/WACCM-X, Geophys. Res. Lett., 47, e2020GL088258. https://doi.org/10.1029/2020GL088258 2020.