日本地球惑星科学連合2023年大会

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[E] オンラインポスター発表

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 the Inner Magnetospheric System

2023年5月23日(火) 09:00 〜 10:30 オンラインポスターZoom会場 (1) (オンラインポスター)

コンビーナ:桂華 邦裕(東京大学大学院理学系研究科地球惑星科学専攻)、三好 由純(名古屋大学宇宙地球環境研究所)、Theodore E Sarris(Democritus University of Thrace)、Evan G Thomas(Dartmouth College)

現地ポスター発表開催日時 (2023/5/23 17:15-18:45)

09:00 〜 10:30

[PEM13-P14] The inner edge location of SAPS electric field and the ring current in the equatorial magnetosphere as observed by Arase and SuperDARN

*堀 智昭1三好 由純1中村 紗都子1笠羽 康正2中川 朋子3北原 理弘2松田 昇也4西谷 望1、Shepherd S. G.5、Ruohoniemi J. M.6熊本 篤志2土屋 史紀2笠原 禎也4浅村 和史7Jun Chae-Woo1、風間 洋一8、Wang S.-Y.8、Tam Sunny, W. Y.9桂華 邦裕10笠原 慧10横田 勝一郎11松岡 彩子12篠原 育7 (1.名古屋大学宇宙地球環境研究所、2.惑星プラズマ・大気研究センター、3.東北工業大学、4.金沢大学、5.ダートマス大学、6.バージニア工科大学、7.宇宙航空研究開発機構、8.台湾中央研究院、9.台湾成功大学、10.東京大学、11.大阪大学、12.京都大学地磁気世界資料センター)

Electric field (E-field) enhancement of subauroral polarization streams (SAPS) and associated particle boundaries in the inner magnetosphere is extensively investigated by analyzing particle and field data obtained by the Arase satellite and ionospheric convection data obtained by Super Dual Auroral Radar Network (SuperDARN). A previous study using Arase and SuperDARN revealed that there are two types of the SAPS events in terms of the spatial correspondence with the ring current: (type A) the inner edge location of SAPS matches with that of the ring current in some cases, while, (type B) in some other cases, their inner edge locations do not match well, and the ring current appears to extend further inward from SAPS. To address why these two types of spatial relationship occurs and what condition controls them, we statistically examined their correlation with substorm activity. Our statistical study indicates that almost all the type-B SAPS events are accompanied by some preceding substorm activity including intermittent occurrence of multiple substorms. This result suggests that a ring current portion located inward of SAPS has been injected by preceding substorms. Such a fossil population drifts around the Earth for some time and its azimuthal pressure gradient would be smeared out, unable to drive downward field-aligned current and thus SAPS. In contrast to type-B, we do not find a clear-cut tendency about the type-A events: they occur either during isolated substorms after prolonged (~several hours) quiet periods, or during a substorm preceded by separate ones. We speculate that these conditions somehow create a relatively simple structure of injected ions at its inner edge, leading to a smaller separation of SAPS inner edge.