日本地球惑星科学連合2025年大会

講演情報

[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-EM13] Dynamics of the Inner Magnetospheric System

2025年5月28日(水) 17:15 〜 19:15 ポスター会場 (幕張メッセ国際展示場 7・8ホール)

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)、Goldstein Jerry(Southwest Research Institute)、Sun YIXIN(Peking University)


17:15 〜 19:15

[PEM13-P16] Direct Measurement of Pitch Angle Scattering in EMIC-Proton Interactions by the WPIA method

*竹内 亘平1三好 由純1浅村 和史2寺澤 賢哉1Jun Chae-Woo1笠原 禎也3笠羽 康正4松田 昇也3土屋 史紀4熊本 篤志4堀 智昭1新堀 淳樹1松岡 彩子5寺本 万里子6山本 和弘1篠原 育2北村 成寿1 (1.名古屋大学宇宙地球環境研究所、2.宇宙航空研究開発機構 宇宙科学研究所、3.金沢大学、4.東北大学、5.京都大学、6.九州工業大学)


Electromagnetic ion cyclotron waves (EMIC), a type of plasma waves, are known to exchange energy with ions through a process called wave-particle interaction. This interaction is supposed to contribute to the acceleration and scattering of ions in the magnetosphere. The Wave-Particle Interaction Analysis (WPIA) is a method that enables direct and quantitative measurement of such interactions. By applying WPIA to observational data from the Arase satellite, Shoji et al. (2017, 2021) successfully demonstrated the direct detection of energy transfer between EMIC waves and ions, as well as frequency variations in EMIC waves. However, direct observations of the Lorentz force, which is responsible for pitch-angle scattering, remains. In this study, we applied the WPIA method to the Arase satellite observations to directly detect the pitch angle changes caused by the Lorentz force. We analyzed an event on October 27, 2022, when the Arase satellite observed intense proton-band EMIC waves associated with pitch angle scattering.
By calculating V×B, which represents change of pitch angle, and V・E, which represents energy exchange between protons and EMIC waves, we successfully detected proton energy loss. Simultaneously, we found that the Lorentz force induced by the plasma waves caused pitch angle changes toward the loss cone.