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29日(水) 13:45 〜 15:15 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)、海老原 祐輔(京都大学生存圏研究所)

14:40 〜 14:55

[PEM13-25] Multiple Satellite Observations of Oxygen Torus in the Inner Magnetosphere

*能勢 正仁1松岡 彩子2熊本 篤志3笠原 禎也4Goldstein J5,6寺本 万里子1土屋 史紀3松田 昇也2小路 真史1今城 峻1生松 聡7山本 和弘7尾花 由紀8野村 麗子9藤本 晶子10篠原 育2三好 由純1Kurth S11Kletzing C11Smith C12MacDowall R13 (1.名古屋大学宇宙地球環境研究所、2.宇宙航空研究開発機構宇宙科学研究所、3.東北大学大学院理学研究科、4.金沢大学総合メディア基盤センター、5.Space Science and Engineering Division, Southwest Research Institute、6.University of Texas at San Antonio、7.京都大学大学院理学研究科、8.大阪電気通信大学工学部、9.国立天文台、10.九州工業大学、11.Department of Physics and Astronomy, University of Iowa、12.Institute for the Study of Earth, Oceans, and Space, University of New Hampshire、13.Solar System Exploration Division, Goddard Space Flight Center)

A recent study employing the Arase and Van Allen Probes A satellites at different MLT revealed an event in which the inner magnetospheric O+ density enhancement (know as the dense oxygen torus) does not extend over all MLT. Rather, the torus is skewed toward the dawn sector, being described more precisely as a crescent-shaped torus or a pinched torus [Nosé et al., 2018]. In the reported event of 24 April 2017, Arase flying in the morning sector detected an enhancement of the average plasma mass up to ~3.5 amu around L=4.9–5.2, while Van Allen Probe A flying in the afternoon sector observed no clear enhancements in the average plasma mass. In the present study, we focus on simultaneous observations of the magnetic field and plasma waves made by the Arase and Van Allen Probes A and B satellites on 12 September 2017. For this event the orbital configuration of the satellites is opposite to that in the study by Nosé et al. [2018]; that is, Arase is in the afternoon and the Van Allen Probes are in the morning. It is found that only Probe B observed a clear enhancement in the average plasma mass up to ~4 amu around L=3.5 and MLT=9.0 hr. This result demonstrates that the crescent-shaped O+ torus is not a unique (single-event) occurrence, and thus may be a general feature of the density enhancement in the inner magnetosphere.