Item type |
紀要論文(ELS) / Departmental Bulletin Paper(1) |
公開日 |
1974-03-01 |
タイトル |
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言語 |
en |
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タイトル |
Hβ Emission during Auroral Breakup |
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 |
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) |
Oguti, T.
Fukunishi, H.
Tohmatsu, T.
Nagata, T.
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著者所属(英) |
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en |
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Geophysics Research Laboratory, University of Tokyo/Geophysics Research Laboratory, University of Tokyo/Geophysics Research Laboratory, University of Tokyo/Geophysics Research Laboratory, University of Tokyo |
抄録(英) |
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内容記述タイプ |
Other |
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内容記述 |
The behaviour of H_β emission is examined at the onset and in the course of auroral breakup, on the basis of meridian scanning data of photometers for H_β and green line along with all-sky photographs obtained at Syowa Station, Antarctica in 1971. The result shows that an auroral breakup starts at the poleward boundary of the pre-existing hydrogen arc, that a global breakup frequently starts when an electron auroral arc comes into contact with the pre-existing hydrogen arc, that the enhancement of H_β takes place in the region bounded by the westward travelling surge, the poleward shifting arc and the pre-existing hydrogen arc with a spatial negative correlation between electron aurora and hydrogen emission, and that the behaviour of a local breakup is substantially similar to that of a global breakup though it has no "contact" of electron aurora. |
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 |
AA00733561 |
書誌情報 |
Memoirs of National Institute of Polar Research. Special issue
巻 3,
p. 10-20,
発行日 1974-03
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