日本地球惑星科学連合2016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-EM18] 磁気圏-電離圏ダイナミクス

2016年5月25日(水) 15:30 〜 17:00 103 (1F)

コンビーナ:*堀 智昭(名古屋大学宇宙地球環境研究所)、田中 良昌(国立極地研究所)、中溝 葵(情報通信研究機構 電磁波計測研究所)、尾崎 光紀(金沢大学理工研究域電子情報学系)、中野 慎也(情報・システム研究機構 統計数理研究所)、三好 由純(名古屋大学宇宙地球環境研究所)、座長:元場 哲郎(名古屋大学)、尾花 由紀(大阪電気通信大学工学部基礎理工学科)

16:15 〜 16:30

[PEM18-16] Plasma density enhancements in the period of Pc 2 observed near the plasmapause in association with Pi 2 and auroral breakup

*櫻井 亨1 (1.東海大学)

キーワード:substorm, aurora, Pc2 oscillations, Pi2 oscillations, Plasmapause

Plasma density enhancements in the period range of Pc 2 (T = ~ 10 sec) were observed near the plasmapause around midnight in association with Pi 2 oscillations and the initial auroral brightening at 0826 UT on 04 April 2009. During this substorm the THEMIS B satellite took an inbound-pass and crossed the plasmapause, observed extraordinary large plasma density oscillations with the period of Pc 2, which enhanced in close association with Pi 2 oscillations. Enhancements of the Pc 2 oscillations were observed with the magnetic, electric field and plasma instruments on board the satellite. Large amplitude plasma density oscillations well correlated with the electric field oscillations and the polarization of the magnetic field Pc2 oscillations showed a left-hand polarization through the event. Therefore the oscillations seem to be the ion-cyclotron oscillations. Auroral breakup and associated Pi 2 oscillations were observed at the THEMIS GBO stations covering over the wide range longitudes from east to west of the Canada. The dominant period of Pi 2 oscillations was almost similar at both these THEMIS GBO stations and the satellite location. The relationships between the Pc2 enhancements and Pi 2 oscillations will be discussed in the presentation in more detail.