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-EM15] Dynamics of Magnetosphere and Ionosphere

2025年5月29日(木) 15:30 〜 17:00 302 (幕張メッセ国際会議場)

コンビーナ:今城 峻(京都大学大学院理学研究科附属地磁気世界資料解析センター)、佐藤 由佳(日本工業大学)、藤本 晶子(九州工業大学)、山本 和弘(名古屋大学宇宙地球環境研究所)、座長:堀 智昭(名古屋大学宇宙地球環境研究所)、吹澤 瑞貴(国立極地研究所)


16:30 〜 16:45

[PEM15-21] Diurnal periodicity in Earth’s radio emissions

*Alexandra Ruth Fogg1、Caitríona M. Jackman1、Simon J. Walker1、Matthew J. Rutala1 (1.School of Cosmic Physics, Dublin Institute for Advanced Studies, DIAS Dunsink Observatory, Dublin D15 XR2R, Ireland)

キーワード:Earth, Space Weather, Radio Emissions, Auroral Kilometric Radiation, Diurnal periodicity, Substorm

Planetary radio emissions have potential as a very valuable remote diagnostic of planetary rotation rates as well as magnetospheric dynamics. Auroral Kilometric Radiation (AKR) is Earth’s strongest natural radio emission, and is anisotropically beamed from a source locked to auroral latitude magnetic field lines. These field lines are tied to the deep interior of the rotating planet, and hence it is theorised that an observer at a fixed local time will observe a diurnal variation in AKR power, as if the Earth and its emission were a lighthouse. In this study we explore this proposed 24 hour periodicity in AKR power using a decade of observations from Wind/WAVES.