日本地球惑星科学連合2023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

2023年5月22日(月) 13:45 〜 15:00 106 (幕張メッセ国際会議場)

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)、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)、Yue Deng(University of Texas at Arlington)、Chairperson:Christina Arras(TU Berlin, Germany)、新堀 淳樹(名古屋大学宇宙地球環境研究所)


14:30 〜 14:45

[PEM12-29] Horizontal wind effects on the thermospheric composition during the geomagnetic storm

*Tingting Yu1、Zhipeng Ren、Xuguang Cai (1.INSTITUTE OF GEOLOGY AND GEOPHYSICS, CHINESE ACADEMY OF SCIENCES)

キーワード:O/N2, geomagnetic storm, horizontal wind

During the 20 April 2020 geomagnetic storm, a long-lived O/N2 depletion at middle latitudes was observed by GOLD. The observed O/N2 depletion tilts latitudinally with the lowest latitude of ~20° N at ~75° W, and changes orientation near 75° W, with a north-westward tilt to the west of ~75° W and a north-eastward tilt to the east of ~75°W. The TIEGCM shows the similar O/N2 depletion patterns and magnitudes. Furthermore, the global simulation shows a neutral ‘tongue’ structure, which is an area of positive O/N2 variations sandwiched by two regions of negative O/N2 variations. The neutral 'tongue' was gradually transported to dayside accompanied by dissipation, and was also observed by GOLD during the storm recovery phase. Horizontal wind plays a major role in forming the O/N2 depletion and neutral ‘tongue’ structure. For the O/N2 depletion, the high-latitude westward zonal wind and the middle-latitude eastward zonal wind maintained its long existence. While the neutral ‘tongue’ was mainly driven by the poleward wind.