JpGU-AGU Joint Meeting 2020

講演情報

[E] 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-EM19] Dynamics of the Inner Magnetospheric System

コンビーナ:桂華 邦裕(東京大学大学院理学系研究科地球惑星科学専攻)、Aleksandr Y Ukhorskiy(Johns Hopkins University Applied Physics Laboratory)、三好 由純(名古屋大学宇宙地球環境研究所)、Lynn M Kistler(University of New Hampshire Main Campus)

[PEM19-04] Cold ions perpendicularly heated by fast magnetosonic waves in the inner magnetosphere observed by Arase (ERG) satellite

*浅村 和史1小路 真史2三好 由純2藤井 亮佑2宮﨑 惇史2笠羽 康正3笠原 禎也4松岡 彩子1Jordanova Vania5 (1.宇宙航空研究開発機構宇宙科学研究本部、2.名古屋大学、3.東北大学、4.金沢大学、5.LANL)

キーワード:イオン加熱、磁気音波、WPIA

Fast magnetosonic (MS) waves are commonly observed in the equatorial region of the inner magnetosphere. Past numerical simulations show MS waves can accelerate cold ions through cyclotron resonance, although the observational evidence is still unclear. Arase (ERG) satellite found events of perpendicular heating of cold ions simultaneously with plasma wave activities of the MS waves. We found more than 200 events of the perpendicular heating of low-energy (10eV/q - a few keV/q) ions in a period between April 2017 to June 2018, and 70% of them coincide with the MS waves. These heated ions are distributed to all the MLT regions within magnetic latitude of +/-10deg, which is consistent with the region where the MS waves frequently observed.

We have applied the WPIA (wave-particle interaction analysis) method to the selected ion heating event with the MS waves. The results show that the MS waves accelerate the ions with pitch angles near 90 degrees. Moreover, we found these ions give their energy to EMIC waves which appears just below the local proton cyclotron frequency. Since MS waves are considered to be generated by the ring distrbution of ions, this analysis indicates energy transfer from higher-energy ions to the cold ions in the inner magnetosphere.