日本地球惑星科学連合2021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] Dynamics of the Inner Magnetospheric System

2021年6月5日(土) 10:45 〜 12:10 Ch.05 (Zoom会場05)

コンビーナ:桂華 邦裕(東京大学大学院理学系研究科地球惑星科学専攻)、三好 由純(名古屋大学宇宙地球環境研究所)、W Lauren Blum(University of Colorado Boulder)、Yuri Shprits(Helmholtz Centre Potsdam GFZ German Research Centre for Geosciences)、座長:山本 和弘(東京大学理学研究科)

11:05 〜 11:20

[PEM12-07] Multipoint measurements to understand the drivers and structure of EMIC waves in the inner magnetosphere

*Lauren W Blum1 (1.University of Colorado Boulder)

キーワード:EMIC waves, inner magnetosphere, radiation belt

Wave-particle interactions provide a primary source of scattering and energization of energetic electrons in the Earth’s radiation belts. Electromagnetic ion cyclotron (EMIC) waves are one intense wave mode observed in the inner magnetosphere that have been shown to contribute to scattering and loss of both energetic electrons and ions. Using multi-point measurements from the Heliospheric Systems Observatory, including NASA’s Van Allen Probes, we examine the properties and source regions of EMIC waves in the inner magnetosphere, exploring the formation and evolution of plasma structures as they relate to observed wave growth. We also investigate the effects of this wave structure on energetic electrons in the outer radiation belt. These studies aid in the understanding of outer radiation belt dynamics and the relationship between electromagnetic waves, global magnetospheric conditions, and solar wind drivers.