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) 09:00 〜 10:30 302 (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)、Chairperson:Hiroshi Hasegawa南條 壮汰(スウェーデン宇宙物理学研究所)


09:15 〜 09:40

[PEM15-02] The Key Role of Magnetic Curvature Scattering in Energetic Electron Precipitation During Substorms

★Invited Papers

*Ying Zou1、Xiaojia Zhang2,3、Anton V Artemyev3、Yangyang Shen3、Vassilis Angelopoulos3 (1.Johns Hopkins University Applied Physics Laboratory、2.University of Texas at Dallas、3.University of California, Los Angeles)

キーワード:Energetic electron precipitation, Whistler wave, Field line curvature scattering, Conductance

Energetic electron precipitation (EEP) significantly affects ionospheric chemistry and lower ionosphere (<100 km) conductance. Two mechanisms have been proposed to explain what causes EEP: whistler-mode wave scattering, which dominates at low latitudes (mapping to the inner magnetosphere), and magnetic field line curvature scattering, which dominates poleward. In this case study, we analyzed a substorm event demonstrating the dominance of curvature scattering. Using ELFIN, POES, and THEMIS observations, we show that 50-1,000 keV EEP was driven by curvature scattering, initiated by an intensification and subsequent earthward motion of the magnetotail current sheet. Using a combination of Swarm, total electron content, and ELFIN measurements, we directly show the location of EEP with energies up to about 1 MeV, which extended from the plasmapause to the near Earth plasma sheet. The impact of this strong substorm EEP on ionospheric ionization is also estimated.