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(ポスター発表)

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) 17:15 〜 18:30 ポスター会場 (国際展示場 6ホール)

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)

17:15 〜 18:30

[PEM08-P12] Periodic Ion Flux Modulation observed by Van Allen Probes in Ring Current Region

*山本 和弘1能勢 正仁2Kletzing Craig3Smith Charles4MacDowall Robert5Spence Harlan4Reeves Geoff6,7Larsen Brian6,7 (1.京都大学大学院理学研究科、2.京都大学大学院理学研究科附属地磁気世界資料解析センター、3.アイオワ大学、4.ニューハンプシャー大学、5.ゴダード宇宙飛行センター、6.ロスアラモス国立研究所、7.ニューメキシココンソーシアム)

キーワード:wave-particle interaction, drift-bounce resonance, geomagnetic pulsations, oxygen ions, ring current, Van Allen Probes

In the drift-bounce resonance that was theoretically introduced by Southwood et al. [1969], the interaction is expected between ULF waves and electrons or ions. Through the interaction, charged particles in the ring current can be accelerated or deaccelerated and the population of ring current particles can be changed. There are many observations of drift-bounce resonance for protons [e.g., Kokubun et al., 1977; Takahashi et al., 1990; Dai et al., 2013], whereas only a few observations of drift-bounce resonance are reported for O+ ions [Yang et al., 2010, 2011].
In this study, we report several events of periodic flux modulation of protons and O+ ions observed by Van Allen Probes in 2012-2016. We find periodic flux modulation of O+ ions and Pc5 waves on November 4, 2015 (event A) and November 30, 2015 (event B). In event A, the flux modulation is recognized at 1-50 keV and dispersed in energy. In event B, however, the flux modulation is limited at ~10 keV. We will examine dependence of the flux variations on pitch angles and energies, and discuss if the variations are due to drift-bounce resonance.