日本地球惑星科学連合2014年大会

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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-EM37_30PM1] 磁気圏構造とダイナミクス

2014年4月30日(水) 14:15 〜 16:00 414 (4F)

コンビーナ:*三好 由純(名古屋大学太陽地球環境研究所)、長谷川 洋(宇宙航空研究開発機構宇宙科学研究所)、座長:栗田 怜(東北大学大学院理学研究科惑星プラズマ・大気研究センター)、渡部 重十(北海道大学大学院理学院宇宙理学専攻)

14:30 〜 14:45

[PEM37-09] サブストーム発生時における磁気圏近尾部Pi型磁気波動

*櫻井 亨1門倉 昭2田中 良昌2佐藤 夏雄2 (1.東海大学、2.国立極地研究所)

キーワード:磁気圏物理, サブストーム, Pi型波動

The THEMIS satellite observations showed that Pi 1 and Pi 2 period range oscillations of the magnetic and electric fields play an important role at a substorm onset in the near-Earth magnetotail. They associated energetic particle accelerations toward the inner magnetosphere. The energetic particle accelerations were observed with very similar oscillation signatures to the Pi 1 and Pi 2 period range oscillations observed in the magnetic and electric fields.. This observation suggests that the Pi 1 and Pi 2 period range oscillations might play an important role for contribution to the auroral particle accelerations at substorm onset in the near-Earth magnetotail . The examination has been done on a substorm event observed on 28 February, 2009 at a THEMIS GBO station, Kuujjuaq (KUUJ) (Mag. Lat.=66.89 N, Mag. Lon.=13.23 E, Mag. Midnight =4.15 UT, L-value = 6.4 ) in the west coast at the high latitude of the North America Continent. This substorm event was simultaneously observed in the near-Earth magnetotail by the three THEMIS satellites, THEMIS-A, -E, and ?D located in the midnight region at ~8 Re, ~8 Re and ~11 Re, respectively. The data examined in this study are the magnetic field, all-sky images (ASI) and keograms (ASK) obtained at KUUJ and the satellite observations of the magnetic field, electric field, and the electron and ion energy spectra in the ESA peir, and peer data. The results show very interesting facts of the Pi 1 and Pi 2 period range oscillations in the magnetic field and auroral activities observed on the ground and their conjunctions of the magnetic, electric fields, and the associated accelerated particles in the near-Earth magnetotail. The implication of this work provides the importance of the Pi 1 and Pi 2 period range oscillations for controlling the substorm onset plasma processes in the near-Earth magnetotail.