Item type |
紀要論文(ELS) / Departmental Bulletin Paper(1) |
公開日 |
1988-02-01 |
タイトル |
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タイトル |
Auroral X-ray images observed by B15-3 balloon over Syowa Station, Antarctica |
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 |
10.15094/00004033 |
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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) |
Suzuki, Hiromu
Yamagishi, Hisao
Kojima, Toshiharu
Hirasima, Yo
Murakami, Hiroyuki
Sato, Natsuo
Yamagami, Takamasa
Kodama, Masahiro
Fukunishi, Hiroshi
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著者所属(英) |
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en |
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Department of Physics, Rikkyo University/National Institute of Polar Research/University of Electro-Communications/Department of Physics, Rikkyo University/Department of Physics, Rikkyo University/National Institute of Polar Research/The Institute of Space and Astronautical Science/Department of Physics, Yamanashi Medical College/Faculty of Science, Tohoku University |
抄録(英) |
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内容記述タイプ |
Other |
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内容記述 |
A balloon observation of auroral X-rays was carried out over Syowa Station in Antarctica on December, 1985 by using a set of three inclined NaI (T1) scintillation counters. The energy-dependent structures of X-rays with energies greater than 22keV were measured. In a case study of the X-ray event occurred at 0145 UT on December 14,an X-ray source region moved toward lower latitudes with a velocity of about 1km/s. This experimental result was confirmed by a simulation calculation for auroral X-ray sources. The spatial distributions of auroral X-rays were found to be consistent with the north-south dependence of 30MHz cosmic noise absorption observed by a scanning-beam riometer at Syowa Station. |
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 1,
p. 46-55,
発行日 1988-02
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出版者 |
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出版者 |
National Institute of Polar Research |