Auroral UV and X-Ray Emission in Antarctica
スポンサーリンク
概要
- 論文の詳細を見る
The ultraviolet and X-ray features of the polar aurora were studied by means of the sounding rockets which were launched from Syowa Station, Antarctica in 1971. The distribution of energetic electrons was obtained from the data of the X-ray counters. The photometric data of the ultraviolet ionization chambers revealed a dual structure of the optical excitation in the active aurora.
- 国立極地研究所の論文
著者
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Oguti T.
Geophysics Research Laboratory University Of Tokyo
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Nagata T.
Geophysics Research Laboratory, University of Tokyo
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Tohmatsu T.
Geophysics Research Laboratory, University of Tokyo
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Kaneda E.
Geophysics Research Laboratory, University of Tokyo
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Kodama M.
Research Institute of Physics and Chemistry
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Tohmatsu T.
Geophysics Research Laboratory University Of Tokyo
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Nagata T.
Geophysics Research Laboratory University Of Tokyo
関連論文
- Interrelations of Upper Atmosphere Disturbance Phenomena in theAuroral Zone
- Auroral VLF Emissions in Antarctica
- Auroral UV and X-Ray Emission in Antarctica
- Hβ Emission during Auroral Breakup