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Modes of pulsating auroras and related geomagnetic pulsations
https://nipr.repo.nii.ac.jp/records/1261
https://nipr.repo.nii.ac.jp/records/126110171471-fb4f-4577-a4cc-198228dbdb05
名前 / ファイル | ライセンス | アクション |
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KJ00000011896 (1.6 MB)
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Item type | 紀要論文(ELS) / Departmental Bulletin Paper(1) | |||||
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公開日 | 1982-09-01 | |||||
タイトル | ||||||
言語 | en | |||||
タイトル | Modes of pulsating auroras and related geomagnetic pulsations | |||||
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 | |||||
ページ属性 | ||||||
内容記述タイプ | Other | |||||
内容記述 | P(論文) | |||||
著者名(英) |
Oguti, Takasi
× Oguti, Takasi |
|||||
著者所属(英) | ||||||
en | ||||||
Geophysical Research Laboratories, University of Tokyo | ||||||
抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | Display modes of pulsating auroras were examined in reference to classifications previously proposed. It is concluded that the pulsating auroras are reasonably classified into, 1) pure pulsations, 2) poleward propagation, 3) streaming along structures, 4) flooding beyond patch boundaries, 5) equatorward propagation, and 6) flash, all in horizontal structures or movements. Most of the modes are related to concurrent geomagnetic pulsations with a peak-to-peak correspondence, within a few seconds. The magnetic pulsations observed under the pulsating aurora are thus concluded to be consequences of the fluctuation in the ionospheric electric current caused by fluctuations in electric conductivity due to pulsating auroral precipitations. | |||||
雑誌書誌ID | ||||||
収録物識別子タイプ | NCID | |||||
収録物識別子 | AA00733561 | |||||
書誌情報 |
Memoirs of National Institute of Polar Research. Special issue 巻 22, p. 94-103, 発行日 1982-09 |