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) 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:細川 敬祐(電気通信大学大学院情報理工学研究科)、傅 維正(名古屋大学 宇宙地球環境研究所)


16:30 〜 16:45

[PEM12-17] Ionospheric Lamb Waves with Conical Phase Fronts Following the 2022 Tonga Eruption Unveiled by Beidou GEO Observations

*Ruoxi Li1、Jiuhou Lei1、Shun-Rong Zhang2Huixin Liu3 (1.University of Science and Technology of China、2.Massachusetts Institute of Technology、3.Kyushu University)

Prior observational uncertainties have hindered the precise understanding of the link between tropospheric Lamb waves and ionospheric disturbances. In this study, we precisely extracted ionospheric Lamb waves originating from the epicenter of the January 15, 2022 Tonga eruption, propagating upward in a conical structure. This was achieved by using line-of-sight observations from the Beidou geostationary satellites, which eliminated the spatiotemporal ambiguity introduced by the relative motion of GPS satellites, enabling the clear extraction of the Lamb signal in the ionosphere. The observed L1 mode speed (~323 m/s) and period (~30 min) were consistent with those of the tropospheric Lamb wave, suggesting that the ionospheric Lamb wave is likely driven by the surface Lamb wave, leading to a conical wave-front that expands with altitude. This study highlights the significant role of Lamb waves in transmitting energy from epicenters through Earth’s atmosphere and plasma systems.