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-EM07] Dynamics in magnetosphere and ionosphere

2016年5月24日(火) 15:30 〜 17:00 103 (1F)

コンビーナ:*三好 由純(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)、堀 智昭(名古屋大学宇宙地球環境研究所)、座長:宮下 幸長(名古屋大学宇宙地球環境研究所)

15:30 〜 15:45

[PEM07-07] Magnetosphere-Ionosphere Coupling by Alfvén waves during Geomagnetic Storms

*Christopher Carew Chaston1,2Van Allen Probes Team (1.University of California Berkeley、2.University of Sydney)

キーワード:Alfven waves, ionosphere, ring current

We present observations from the Van Allen probes which show the coincident occurrence of Alfvénic fluctuations in the equatorial plane, field-aligned electrons and outflowing energized ionospheric ions during geomagnetic storms. Based on these observations we build a model for the observed wave-fields and the particle acceleration that occurs within them. It is shown how Alfvén waves extract ions from the topside ionosphere and through the action of trapping and stochastic acceleration drive the acceleration of these ions to energies which may exceed 100 keV in the equatorial plane. The agreement in the form and evolution of the observed and simulated ion distributions provides confidence in the veracity of the modelling and simulation results. It is estimated for observed wave amplitudes and ion densities that this process may make a significant contribution to magnetospheric ion energy density. This is supported by statistical results which reveal an inverse correlation between the time rate of change of Dst and Alfvén wave spectral energy density.