日本地球惑星科学連合2018年大会

講演情報

[EE] 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-EM15] Dynamics in magnetosphere and ionosphere

2018年5月20日(日) 15:30 〜 17:00 303 (幕張メッセ国際会議場 3F)

コンビーナ:田中 良昌(国立極地研究所)、堀 智昭(名古屋大学宇宙地球環境研究所)、中溝 葵(情報通信研究機構 電磁波研究所、共同)、尾崎 光紀(金沢大学理工研究域電子情報学系)、座長:海老原 祐輔(京都大学生存圏研究所)、長谷川 洋(JAXA宇宙科学研究所)

16:15 〜 16:30

[PEM15-22] Spectral characteristics of EMIC waves observed at THEMIS probes in the outer magnetosphere

*Gi-Jeong Kim1Khan-Hyuk Kim1 (1.Kyung Hee University)

We have statistically examined the properties of EMIC waves observed by THEMIS probes in the outer magnetosphere (L = 6~12) for 2008-2011. The wave events were identified in 3-min intervals through a semiautomated wave selection procedure. Using Fourier spectral analysis for each 3-min segments, we determine the ellipticity, the azimuth orientation angle of the polarization ellipse, and wave normal angle between the wave propagation vector orientation and background field direction. Unlike previous studies, spectral properties are examined for wave events showing high coherence (> 0.7) between two transverse (δBx: radial and δBy: eastward) components (i.e., phase-coherent sinusoidal wave events) because wave polarization characteristics obtained from the spectral analysis are meaningful only in the case of a plane wave. We found that only ~10% of EMIC waves show high coherence. This indicates that most of EMIC waves in the outer magnetosphere are phase-incoherent waves. In this study we compare previous observations and our statistical results. In addition, we also compare the wave normal angles obtained from Fourier analysis and the minimum variance analysis.