日本地球惑星科学連合2021年大会

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[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-EM12] Dynamics of the Inner Magnetospheric System

2021年6月5日(土) 13:45 〜 15:15 Ch.05 (Zoom会場05)

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)、座長:謝 怡凱(京都大学生存圏研究所)

15:00 〜 15:15

[PEM12-16] Mode-coupling Pi2 pulsations on the off-equatorial plasmapause inferred from the Arase satellite observation

*寺本 万里子1、松岡 彩子2、笠原 禎也3、笠羽 康正4、熊本 篤志4、土屋 史紀4、松田 昇也6、三好 由純5、能勢 正仁5、中川 朋子7、今城 峻5、小路 真史5、中村 紗都子5、篠原 育6 (1.九州工業大学、2.京都大学、3.金沢大学、4.東北大学、5.名古屋大学、6.宇宙航空研究開発機構 宇宙科学研究所、7.東北工業大学)

We investigated Pi2 pulsations in the electric and magnetic field and their relation to the ambient plasma density observed from the Arase satellite to explore the generation mechanism of low-latitude Pi2. At a geomagnetically quiet time, Pi2 pulsations were observed in all three components of the magnetic field and in the radial and azimuthal components of the electric field when the Arase satellite was located on the plasmapause off the equatorial plane (about 25 degrees Mlat) at midnight. The coherence and cross phase between the orthogonal electric and magnetic field components are high and approximately 90 degrees. The compressional component of the magnetic field has high coherence with the azimuthal component of the electric field. The cross phase properties indicate that the radial and field-aligned standing waves are excited on the plasmapause. These results confirm the mode coupling between the fast mode wave and Alfven waves in the plasmasphere, which was proposed by Takahashi et al. [2018].

We compared these Pi2 pulsations with those on the ground over a wide latitudinal and longitudinal range. Additionally, we discussed the generation mechanism of this event.