日本地球惑星科学連合2021年大会

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[E] 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-EM12] Dynamics of the Inner Magnetospheric System

2021年6月5日(土) 17:15 〜 18:30 Ch.04

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)、三好 由純(名古屋大学宇宙地球環境研究所)、W Lauren Blum(University of Colorado Boulder)、Yuri Shprits(Helmholtz Centre Potsdam GFZ German Research Centre for Geosciences)

17:15 〜 18:30

[PEM12-P05] Global characteristics of cold protons in the near-Earth magnetotail: MMS/HPCA observations

*桂華 邦裕1、星野 真弘1、浅見 隆太1 (1.東京大学大学院理学系研究科)

キーワード:磁気圏プラズマ輸送、磁気圏尾部プラズマの起源、2成分プラズマ

We conduct a statistical study of cold protons in the near-Earth magnetotail under quiet magnetotail conditions. Performing two-component Maxwellian fits to velocity distributions, we extract densities and temperatures of cold protons. Cold protons are separated into three distinct populations in the density-plasma b space. We interpret that Population I, characterized by a positive correlation of density to b, is solar-wind origin plasma transported over the polar regions. Population II, seen only in the high-b (>0.1) and tailward region (r > 20 Re) particularly on the dusk side, is solar-wind origin plasma entering through the flank magnetopauses and remains cold. Population III, clearly identified in the near-Earth region (r < 10 Re), is of ionospheric origin. The results also suggest that plasma supply to the plasma sheet is dominated by Population I and that cold plasma in the near-Earth magnetotail is mostly of ionospheric origin.