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-EM09] Dynamics of Magnetosphere and Ionosphere

2021年6月6日(日) 10:45 〜 12:15 Ch.05 (Zoom会場05)

コンビーナ:藤本 晶子(九州工業大学)、尾崎 光紀(金沢大学理工研究域電子情報学系)、佐藤 由佳(日本工業大学)、中溝 葵(情報通信研究機構 電磁波研究所)、座長:長谷川 洋(宇宙航空研究開発機構宇宙科学研究所)、西野 真木(宇宙航空研究開発機構宇宙科学研究所)

10:45 〜 11:10

[PEM09-08] A Case Study of Transversely Heated Low-Energy Helium Ions by EMIC Waves in the Plasmasphere

★Invited Papers

*Khan-Hyuk Kim1 (1.School of Space Research, Kyung Hee University)

キーワード:EMIC waves, Low-energy ion heating, Plasmasphere

The Van Allen Probe A spacecraft observed strong ~0.5-Hz helium (He+) band and weak ~0.8-Hz hydrogen (H+) band EMIC waves on 17 April 2018, at L = ~4.5-5.2, in the dawn sector, near the magnetic equator, and close to the plasmapause. We examined low-energy ion fluxes observed by the Helium Oxygen Proton and Electron (HOPE) instrument onboard Van Allen Probe A during the wave interval and found that low-energy He+ flux (< 10 eV) enhancements occur nearly simultaneously with He-band and H-band EMIC wave power enhancements in a direction mostly perpendicular to the background magnetic field without significant low-energy H+ and O+ flux variations. We suggest that cold He+ ions (<1 eV) are preferentially and transversely heated up 10 eV through the interaction with EMIC waves inside the plasmasphere. The low-Earth orbit spacecraft observed localized precipitations of energetic protons in the upper ionosphere at subauroral latitudes near the magnetic field footprint of Van Allen Probe A. Our observations provide a clear evidence that EMIC waves play an important role in the overall dynamics in the inner magnetosphere, contributing to the high-energy particle loss and low-energy particle energization.