日本地球惑星科学連合2015年大会

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インターナショナルセッション(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 in magnetosphere and ionosphere

2015年5月28日(木) 11:00 〜 11:45 302 (3F)

コンビーナ:*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)、田中 良昌(国立極地研究所)、堀 智昭(名古屋大学太陽地球環境研究所 ジオスペース研究センター)、座長:三好 由純(名古屋大学太陽地球環境研究所)

11:30 〜 11:45

[PEM09-24] 持続する磁気リコネクションジェットを伴う磁気圏尾部電流層の振動:ジオテイル衛星観測

*長谷川 洋1篠原 育1長井 嗣信2斎藤 義文1 (1.JAXA宇宙科学研究所、2.東京工業大学)

キーワード:磁気リコネクション, 磁気圏尾部, 電流層, キンクモード, グラッド・シャフラノフ方程式, 定常磁気圏対流

We present and analyze quasi-periodic crossings of the magnetotail current sheet observed by the Geotail spacecraft at (-26, 9, 0) Re in GSM on 11 October 2014. The event occurred when the magnetosphere was moderately driven by the solar wind and southward interplanetary magnetic field, i.e., during a period of so-called steady magnetospheric convection. Reconnection jets with an earthward velocity 〜700 km/s, comparable to the lobe Alfven speed, were observed almost continuously in the plasma sheet for an interval 0900-1100 UT. In order to reveal the orientation and structure of the observed current sheet, whose crossings occurred with a period of 2-3 minutes, we applied the Grad-Shafranov reconstruction technique [Hau and Sonnerup, 1999; Hu and Sonnerup, 2002] assuming 2-D structures. The results indicate that kink-type waves were propagating approximately earthward in the plasma sheet, with a wavelength of 〜15 Re and amplitude of order 1 Re. To the best of our knowledge, this is the first identification of sunward-propagating MHD-scale kink-mode waves in the magnetotail. The generation mechanism of the observed oscillations is discussed based on the nature of the reconstructed current sheet structures, ion velocity distributions observed in the current sheet, and results from other single-spacecraft methods such as minimum variance analysis and minimum Faraday residue method [Terasawa et al., 1996; Khrabrov and Sonnerup, 1998].

References:
Hau, L.-N., and B. U. O. Sonnerup (1999), Two-dimensional coherent structures in the magnetopause: Recovery of static equilibria from single-spacecraft data, J. Geophys. Res., 104, 6899-6917.
Hu, Q., and B. U. O. Sonnerup (2002), Reconstruction of magnetic clouds in the solar wind: Orientation and configuration, J. Geophys. Res., 107(A7), 1142, doi:10.1029/2001JA000293.
Khrabrov, A. V., and B. U. O. Sonnerup (1998), Orientation and motion of current layers: Minimization of the Faraday residue, Geophys. Res. Lett., 25, 2372-2376.
Terasawa, T., H. Kawano, I. Shinohara, et al. (1996), On the determination of a moving MHD structure: Minimization of the residue of integrated Faraday's equation, J. Geomagn. Geoelectr., 48, 603-614.