JpGU-AGU Joint Meeting 2020

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 Magnetosphere and Ionosphere

コンビーナ:中溝 葵(情報通信研究機構 電磁波研究所)、尾崎 光紀(金沢大学理工研究域電子情報学系)、藤本 晶子(九州工業大学)、佐藤 由佳(日本工業大学)

[PEM13-P06] Plasma waves causing 20 Hz intensity modulation of pulsating aurora

*Herbert Akihito Uchida1Ryuho Kataoka2,1Kiyoka Murase1Shoya Matsuda3Yoshiya Kasahara4Masafumi Shoji5Yoshizumi Miyoshi5Iku Shinohara3Ayako Matsuoka3Satoshi Kurita5Keisuke Hosokawa6 (1.The Graduate University for Advanced Studies、2.National Institute of Polar Research、3.Institute of Space and Astronautical Science、4.Kanazawa University、5.Institute for Space–Earth Environmental Research、6.The University of Electro-Communications)

キーワード:Pulsating aurora, Chorus waves, Fast modulation

We observed ~20 Hz intensity modulation of pulsating aurora at Syowa Station by high-speed camera pointing at magnetic zenith for a few min time interval, 30 min after the aurora breakup occurred on September 22, 2018. The footprints of the Arase satellite was located within the all-sky field of view at that time, and ~20 Hz intensity modulation was observed in the intensity of the lower band chorus waves. We present the possible correlations between the plasma waves and pulsating aurora in more detail, and examine the resonant energy quantitatively.