日本地球惑星科学連合2016年大会

講演情報

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-EM08] Inner magnetosphere: Latest results and new perspectives

2016年5月23日(月) 15:30 〜 17:00 103 (1F)

コンビーナ:*Summers Danny(Dept of Math and Stats,Memorial University of Newfoundland)、海老原 祐輔(京都大学生存圏研究所)、三好 由純(名古屋大学宇宙地球環境研究所)、座長:三好 由純(名古屋大学宇宙地球環境研究所)

16:30 〜 16:45

[PEM08-15] 相対論的電子マイクロバーストと放射線帯電子加速:SAMPEX・Van Allen Probes衛星による観測

*栗田 怜1三好 由純1 (1.名古屋大学宇宙地球環境研究所)

キーワード:放射線帯、chorus waves

It has been suggested that whistler mode chorus is responsible for both acceleration of MeV electrons and relativistic electron microbursts through resonant wave-particle interactions. Relativistic electron microbursts have been considered as an important loss mechanism of radiation belt electrons. Here we report on the observations of relativistic electron microbursts and flux variations of trapped MeV electrons during the 8-9 October 2012 storm, using the SAMPEX and Van Allen Probes satellites. Observations by the satellites show that relativistic electron microbursts correlate well with the rapid enhancement of trapped MeV electron fluxes by chorus wave-particle interactions, indicating that acceleration by chorus is much more efficient than losses by microbursts during the storm. It is also revealed that the strong chorus wave activity without relativistic electron microbursts does not lead to significant flux variations of relativistic electrons. We also find that the microburst occurrence rate during the acceleration event has a peak around which the phase space density peak is identified by the Van Allen Probes satellites. We conclude that effective acceleration of relativistic electrons is caused by chorus that can cause relativistic electron microbursts, and that microbursts can be a proxy of internal acceleration of MeV electrons by whistler-mode chorus.