日本地球惑星科学連合2019年大会

講演情報

[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-EM13] 内部磁気圏

2019年5月28日(火) 15:30 〜 17:00 A04 (東京ベイ幕張ホール)

コンビーナ:海老原 祐輔(京都大学生存圏研究所)、Danny Summers(Memorial University of Newfoundland)、三好 由純(名古屋大学宇宙地球環境研究所)、齊藤 慎司(名古屋大学 大学院理学研究科)、座長:三好 由純(名古屋大学宇宙地球環境研究所)、Danny Summers

16:40 〜 16:55

[PEM13-10] Conjugated quasi-periodic ELF/VLF emissions between the Arase satellite and both Van Allen Probes

*Claudia Martinez Calderon1,2Frantisek Nemec3Kazuo Shiokawa2Yuto Katoh1Yoshiya Kasahara4Shoya Matsuda2Fuminori Tsuchiya1Atsushi Kumamoto1Mariko Teramoto2Ayako Matsuoka5Yoshizumi Miyoshi2Ondrej Santolik6,3George Hospodarksy7 (1.Dept. Geophys., Grad. Sch. Sci., Tohoku University、2.Instute for Space-Earth Environmental Research, Nagoya University、3.Faculty of Mathematics and Physics, Charles University, Prague, Czech Republic、4.Kanazawa University、5.Japan Aerospace Exploration Agency、6.Institute of Atmospheric Physics, Prague, Czech Republic、7.Department of Physics and Astronomy, University of Iowa, USA)

キーワード:conjugated event, VLF, QP, Arase, RBSP, plasma waves

Extremely Low (ELF) and Very Low Frequency (VLF) emissions are naturally occurring magnetospheric plasma waves in the frequencies of 3 Hz to 30 kHz. They play a fundamental role in radiation belt dynamics, accelerating or scattering electrons through wave-particle interactions. We report the first quasi-periodic (QP) emission simultaneously observed by the Arase (ERG) satellite and both Van Allen Probes (RBSP). This is one of few known conjugated satellite events where the waves show very similar spectral and temporal features. The event was observed on November 29, 2018 from approximately 11 to 13:30 UT by both RBSP, while ERG observed it from 12 to 14 UT. Using wave analysis, propagation parameters, and intensities simultaneously measured at several locations we will discuss the approximate location of the source region. We will also discuss the eventual timing differences between QP periodicity at different locations. Some slight variation in the spectral shapes is observed. We will discuss possible relationships with the variations of plasma number density, magnetic field, and energetic electron distribution.