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Occurrence conditions for two different kinds of transpolar arcs
https://doi.org/10.15094/00004070
https://doi.org/10.15094/00004070da725665-aec3-4dee-833b-74f14fe72456
名前 / ファイル | ライセンス | アクション |
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KJ00000036001 (698.9 kB)
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Item type | 紀要論文(ELS) / Departmental Bulletin Paper(1) | |||||
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公開日 | 1989-11-01 | |||||
タイトル | ||||||
タイトル | Occurrence conditions for two different kinds of transpolar arcs | |||||
言語 | ||||||
言語 | eng | |||||
資源タイプ | ||||||
資源タイプ識別子 | http://purl.org/coar/resource_type/c_6501 | |||||
資源タイプ | departmental bulletin paper | |||||
ID登録 | ||||||
ID登録 | 10.15094/00004070 | |||||
ID登録タイプ | JaLC | |||||
ページ属性 | ||||||
内容記述タイプ | Other | |||||
内容記述 | P(論文) | |||||
著者名(英) |
Makita, Kazuo
× Makita, Kazuo× Meng, Chin-I |
|||||
著者所属(英) | ||||||
en | ||||||
Faculty of Engineering, Takusyoku University | ||||||
著者所属(英) | ||||||
en | ||||||
Applied Physics Laboratory, The Johns Hopkins University | ||||||
抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | On the basis of DMSP auroral image and particle data, the occurrence conditions of sun-aligned arcs and theta auroras are examined for various solar wind conditions. Sun-aligned arcs appear during geomagnetically quiet period and also the period of northward IMF associated with high solar wind velocity. Theta auroras appear during the period of moderate geomagnetic activity and also extremely high solar wind velocity. However, IMF B_z is not always positive when theta auroras appear. These results may suggest that the source of sun-aligned arc and theta aurora are quite different. | |||||
雑誌書誌ID | ||||||
収録物識別子タイプ | NCID | |||||
収録物識別子 | AA10756224 | |||||
書誌情報 |
Proceedings of the NIPR Symposium on Upper Atmosphere Physics 巻 2, p. 123-128, 発行日 1989-11 |
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出版者 | ||||||
出版者 | National Institute of Polar Research |