日本地球惑星科学連合2024年大会

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[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-EM10] Dynamics of Magnetosphere and Ionosphere

2024年5月27日(月) 13:45 〜 15:00 展示場特設会場 (2) (幕張メッセ国際展示場 6ホール)

コンビーナ:今城 峻(京都大学大学院理学研究科附属地磁気世界資料解析センター)、家田 章正(名古屋大学 宇宙地球環境研究所)、佐藤 由佳(日本工業大学)、藤本 晶子(九州工業大学)、座長:渡辺 正和(九州大学大学院理学研究院)、門倉 昭(国立極地研究所)

14:15 〜 14:30

[PEM10-13] Characteristics of eastward expansion of substorm auroral bulge

*門倉 昭1 (1.国立極地研究所)

キーワード:サブストーム、オーロラ

After the expansion phase onset of a substorm, auroral bulge expands poleward, westward, and eastward. Its westward expansion is characterized by the rapid westward motion of the Westward Traveling Surge (WTS) on the expanding front. On the other hand, diffuse and pulsating aurora, auroral torch, and Omega-band usually appear and embedded in the eastern part of the bulge, and a discrete aurora is expanding eastward around the poleward edge of the bulge. Such features are well-known and a large amount of studies on the evolution of the substorm bulge have been done so far. But number of studies on the mechanism of the eastward expansion of the bulge seems not so large, comparing with that of the WTS, although number of studies on the evolution of the torch, Omega-band, and pulsating aurora is relatively large. In this study, we will examine details of the evolution of the eastward expansion of bulge at the eastward expanding front by using ground-based observations at Syowa Station, Antarctica.