日本地球惑星科学連合2018年大会

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[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-EM16] Dynamics of Earth's Inner Magnetosphere and Initial Results from Arase

2018年5月21日(月) 13:45 〜 15:15 303 (幕張メッセ国際会議場 3F)

コンビーナ:Danny Summers(Memorial University of Newfoundland)、三好 由純(名古屋大学宇宙地球環境研究所)、細川 敬祐(電気通信大学大学院情報理工学研究科、共同)、海老原 祐輔(京都大学生存圏研究所)、座長:三好 由純(名古屋大学宇宙地球環境研究所)

14:45 〜 15:00

[PEM16-11] VLF Conjugate events between Arase (ERG) and Kannuslehto: differences between cases on the noon and midnight sides.

*Claudia Martinez Calderon1Yuto Katoh1Kazuo Shiokawa2Mitsunori Ozaki3Satoshi Kurita2Jyrki Manninen4Yoshiya Kasahara3Shoya Matsuda2Atsushi Kumamoto1Fuminori Tsuchiya1Ayako Matsuoka5Yoshizumi Miyoshi2 (1.Dept. Geophys., Grad. Sch. Sci., Tohoku University、2.Institute for Space-Earth Environmental Research, Nagoya, Japan、3.Kanazawa, University, Kanazawa, Japan、4.Sodankyl Geophysical Observatory, University of Oulu, Sodankyla, Finland、5.Institute of Space and Astronautical Science, JAXA, Japan)

キーワード:VLF, Arase , Conjugate event, ERG, QP, whistler-mode

Quasi-periodic (QP) emissions, are naturally occurring magnetospheric plasma waves (3 Hz < f < 30 kHz) propagating in the whistler-mode with a fairly regular periodic modulation of their wave intensity. Through wave-particle interactions, whistler-mode waves play an important role in the regulation of radiation belt dynamics. Understanding the processes behind their generation and propagation, including their spatial extent, can help us quantify their part in the acceleration and scattering of electrons in the radiation belts. This study presents two rare QP conjugate events between the ground station of Kannuslehto [MLAT=64.4N, L=5.3], Finland, and the Arase (ERG) satellite. Case 1 on March 28, 2017 from ~22:30 to 23:00 UT, happened on the post-midnight side and during the recovery phase of a storm with a period of sustained high solar-wind speed and high AE (400 < AE < 800 nT). Case 2 on November 30, 2017 from ~09:30 to 10:20 UT was observed on the noon side, during a geomagnetic quiet time with a Dst > 10 nT and AE < 100 nT. Using these events, we estimated the size and characteristics of the active wave source for each event, the region where the waves are generated with the same frequency and spectral features. We discuss the coherence and spatial extent of the waves, and their local source size. We also investigate the role that density plays in the variations in the spectral features of the observed waves. We use correlation and wave analysis to compare wave propagation between the two cases. Finally, we discuss electron pitch angle distributions. This study presents the first opportunity to compare two conjugate events between the same ground-station and satellite, at different geomagnetic conditions and on almost opposite sides of the magnetosphere.