日本地球惑星科学連合2025年大会

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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)


16:00 〜 16:15

[PEM12-39] Intraseasonal Variability of the Equatorial Ionosphere Responses to the Madden-Julian Oscillation

*Xu Zhou1、Guiwan Chen2、Xinan Yue1、Ruilong Zhang1Akimasa Yoshikawa3 (1.Institute of Geology and Geophysics, Chinese Academy of Sciences、2.Institute of Atmospheric Physics, Chinese Academy of Sciences、3.Department of Earth and Planetary Sciences, Kyushu University)

キーワード:Equatorial Ionosphere, Plasma Drifts, Madden-Jullian Oscillation, Whole Atmosphere Simulation, Atmospheric Tides

This study investigates the response of the equatorial ionosphere to the tropospheric Madden-Jullian Oscillation (MJO) using the Whole Atmosphere Community Climate Model-eXtended (WACCM-X). The main results indicate that the intraseasonal variability of ionospheric vertical plasma drifts (Viz) is generally strong around boreal winters and exhibits significant eastward-propagating signals. Composite analysis showed that, during the December-January-February-March (DJFM) season, Viz was generally negative when the MJO was active over the Maritime Continent (phase 5) and positive when the MJO was active over the Indian Ocean (phase 2). The magnitude of MJO impact on Viz achieves ~1.2 m/s, representing roughly 10% of the seasonal mean. The eastward-propagating wavenumber-4 is apparently strong during MJO phases 5 and 1–2, which is examined to be associated with non-migrating tides below. Term analysis revealed the importance of zonal winds in driving the Viz responses. This study emphasizes the importance of tropospheric sources that affect the geospace environment.