JpGU-AGU Joint Meeting 2020

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] 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)

[PEM13-24] Short review for recent studies of pulsating aurora in Japan during Arase era

★Invited Papers

*細川 敬祐1三好 由純2尾崎 光紀3大山 伸一郎2小川 泰信4栗田 怜2笠原 禎也3笠羽 康正5八木谷 聡3松田 昇也7土屋 史紀5熊本 篤志5片岡 龍峰4塩川 和夫2宮岡 宏4田中 良昌4野澤 悟徳2寺本 万里子6高島 健7篠原 育7藤井 良一8 (1.電気通信大学、2.名古屋大学宇宙地球環境研究所、3.金沢大学、4.国立極地研究所、5.東北大学、6.九州工業大学、7.宇宙航空研究開発機構宇宙科学研究所、8.情報システム研究機構)

キーワード:オーロラ、磁気圏、コーラス波動

Pulsating aurora (PsA) is one of the major types of aurora often seen in the lower latitude part of the auroral region in the morning side. PsA is known to have two distinct periodicities. One is the main pulsation whose period ranges from a few to a few tens of seconds. The other is so-called internal modulation which is ~3 Hz luminosity modulation during the ON phase of main pulsation. Previous studies indicated that ~50% of PsA are accompanied by the internal modulation (i.e., internal modulation is often seen, but not always observed during PsA). Recent coordinated ground/satellite observations of PsA suggested that these two periodicities are closely associated with the intensity modulation of whistler mode chorus waves in the morning side magnetosphere. In particular, the association between the main pulsation and bursts of chorus was confirmed for example by Nishimura et al. (2010) and more recently by Kasahara et al. (2018). However, it has still been under debate which characteristics of chorus waves control the existence/absence of internal modulation. This review talk will be focused on several results from recent coordinated ground/satellite observations of PsA (e.g., Ozaki et al., 2019; Hosokawa et al., 2020) since the launch of the Arase satellite. Especially, we will introduce conjugate high-time resolution measurements of fine-scale temporal variations of chorus waves in space and PsA seen from the ground.In addition, we will talk about recent ground-based radar observations of PsA showing the simultaneous precipitation of sub-relativistic electrons during PsA, which will be one of the primary scientific objectives of EISCAT_3D currently being prepared in Scandinavia.