Item type |
紀要論文(ELS) / Departmental Bulletin Paper(1) |
公開日 |
1998-01-01 |
タイトル |
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タイトル |
Postnoon aurora observed at Zhongshan Station, Antarctica - A case study - |
言語 |
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言語 |
eng |
資源タイプ |
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資源タイプ識別子 |
http://purl.org/coar/resource_type/c_6501 |
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資源タイプ |
departmental bulletin paper |
ID登録 |
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ID登録 |
10.15094/00004234 |
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ID登録タイプ |
JaLC |
ページ属性 |
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内容記述タイプ |
Other |
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内容記述 |
P(論文) |
著者名(英) |
Makita, Kazuo
Kikuchi, Masayuki
Sato, Natsuo
Ayukawa, Masaru
Wang, Xing
Yang, Huigen
Liu, Ruiyuan
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著者所属(英) |
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en |
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Takushoku University/National Institute of Polar Research/National Institute of Polar Research/National Institute of Polar Research/Polar Research Institute of China/Polar Research Institute of China/Polar Research Institute of China |
抄録(英) |
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内容記述タイプ |
Other |
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内容記述 |
The characteristics of postnoon auroras are examined with all-sky TV data at Zhongshan (invariant latitude 74.49°in Antarctica). From a comparison between ground aurora and DMSP particle data, energetic electrons higher than 1 keV are responsible for the postnoon band aurora. It is remarkable that the postnoon band aurora shows a periodic latitudinal movement with its period about 125s to 160s. It is also noted that a bright region moves from the west to the east along the longitudinal direction within the band aurora. These charactreristics are partly similar to auroral behavior obtained in our previous observations at Ny-Alesund in Spitzbergen. |
雑誌書誌ID |
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収録物識別子タイプ |
NCID |
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収録物識別子 |
AA10756224 |
書誌情報 |
Proceedings of the NIPR Symposium on Upper Atmosphere Physics
巻 11,
p. 19-27,
発行日 1998-01
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出版者 |
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出版者 |
National Institute of Polar Research |