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)

[PEM19-10] Recent Progress in ULF Wave’s Interaction with Cold Electrons and Ions in the Earth’s Inner Magnetosphere

★Invited Papers

*Jie Ren1Qiugang Zong1Xuzhi Zhou1Chao Yue1Robert Rankin2 (1.Peking University、2.University of Alaska)

キーワード:ULF Waves, Cold Plasma, Acceleration and Tansport

In terms of particle energy and species, the inner magnetosphere can be divided into three regions, including the inner and outer radiation belts, ring current and plasmasphere. It is widely accepted that ULF waves can cause the acceleration and transport of outer radiation belt electrons and ring current ions through drift/drift-bounce resonance. Recent studies in the last two or three years presented the observational evidence of cold particle acceleration/energization by ULF waves. Cold plasmaspheric electrons can be rapidly accelerated by the poloidal-mode ULF wave electric fields via drift-bounce resonance, which show bi-directional pitch angle distributions, phase space density enhancement and density enhancement. The spatial distributions in the equatorial plane, occurrence conditions as well as resonant energy range of the cold plasmaspheric electrons also have been investigated using six years Van Allen Probes data. Different species of cold plasmaspheric ions can be energized to different energies due to the mass dependence of ExB effect by ULF waves. Besides, observations suggest that the polarization drift can lead to the real acceleration of cold O+ ions. The recent progress can promote our understanding of ULF waves’ impact on the cold particles, and let the science community realize the potential research value of ULF waves in the dynamics of cold plasma environment.