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26日(月) 15:30 〜 17:00 303 (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:西山 尚典(国立極地研究所)、Yang-Yi Sun(China University of Geosciences)


15:45 〜 16:00

[PEM12-38] The Variability of the Equatorial Ionospheric Vertical and Field-aligned Plasma Drifts During the SSW

*Ruilong Zhang1 (1.Institute of Geology and Geophysics, Chinese Academy of Sciences)

キーワード:vertical plasma drift, field-align plasma drift, neutral wind, SSW

We use the measurements of the Ionospheric Connections Explorer (ICON) and Communication/Navigation Outage Forecasting System (C/NOFS) satellites to present the responses of the equatorial ionospheric vertical and field-aligned plasma drift during the 2009 and 2021 sudden stratosphere warmings (SSW). The observations show that both the vertical and field-aligned drifts present the semidiurnal disturbances during the SSW. The ICON records the afternoon northward disturbance in field-aligned plasma drift mainly due to the disturbance meridional wind. Based on the whole atmosphere model Ground-to-topside model of Atmosphere and Ionosphere for Aeronomy, the meridional wind can contribute to the disturbance field-aligned drift. Further, the semidiurnal disturbances in vertical and field-aligned drift can well explain the responses of the total electron content to the SSW and their hemispheric differences. Further, the disturbances in vertical and field-aligned plasma drifts can cause the ionosphere-plasmasphere coupling in equatorial and low latitudes. Our results give a new perspective for understanding the ionospheric perturbations during SSW.