日本地球惑星科学連合2023年大会

講演情報

[E] オンラインポスター発表

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

2023年5月23日(火) 09:00 〜 10:30 オンラインポスターZoom会場 (1) (オンラインポスター)

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)、Theodore E Sarris(Democritus University of Thrace)、Evan G Thomas(Dartmouth College)

現地ポスター発表開催日時 (2023/5/23 17:15-18:45)

09:00 〜 10:30

[PEM13-P15] Phase difference of ECH waves observed by using the interferometry observation mode of the Arase satellite

*滝 朋恵1栗田 怜2、新城 藍里1中村 紗都子3小嶋 浩嗣2笠原 禎也4松田 昇也4松岡 彩子5三好 由純6篠原 育7 (1.京都大学大学院工学研究科、2.京都大学生存圏研究所、3.名古屋大学高等研究院、4.金沢大学大学院自然科学研究科、5.京都大学理学研究科地磁気世界資料解析センター、6.名古屋大学宇宙地球環境研究所、7.宇宙航空研究開発機構/宇宙科学研究所)

キーワード:電子サイクロトロン高調波、インターフェロメトリ観測

Electron Cyclotron Harmonic (ECH) waves are a type of plasma wave observed in the magnetosphere that with a harmonic structure of intensity peaks between integer multiples of the electron cyclotron frequency. ECH waves were first observed by the OGO-5 satellite and have been observed in the magnetospheres of Earth, other planets and satellites. ECH waves have been reported to have large amplitudes, suggesting that they can affect the surrounding plasma environment. For example, ECH waves can cause pitch angle scattering of electrons, and observations have suggested that ECH waves are associated with the excitation of diffuse auroras. ECH waves have also been used to estimate the cold electron temperature because their dispersion relation depends on the cold electron parameters.
We report that interferometric observations by the Arase satellite provide phase differences in ECH waves. The Arase satellite has four wire probe antennas in the spinning plane, which are typically used as two sets of dipole antennas. In interferometric mode, on the other hand, two of these antennas, V1 and V2, are used as monopole antennas, and the potential difference between each antenna and the satellite ground is observed. The phase difference between the two waveforms Ev1 and Ev2 is calculated from the observed ECH waves. The phase difference was calculated for each frequency using a complex Fourier spectrum.
The results show that the phase differences of the observed ECH waves are significantly different between the phase difference of one harmonic band and the phase difference of the other harmonic band. This suggests that the wave vector of ECH waves in one harmonic band may be different from the ECH wave vector in the other harmonic band.