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Auroral zone X-ray pulsations associated with VLF pulsations: B15-3N balloon experiment
https://nipr.repo.nii.ac.jp/records/1597
https://nipr.repo.nii.ac.jp/records/159741d06592-8ced-460a-8401-8bb190470b55
名前 / ファイル | ライセンス | アクション |
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KJ00000012230 (1.8 MB)
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Item type | 紀要論文(ELS) / Departmental Bulletin Paper(1) | |||||
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公開日 | 1984-07-01 | |||||
タイトル | ||||||
言語 | en | |||||
タイトル | Auroral zone X-ray pulsations associated with VLF pulsations: B15-3N balloon experiment | |||||
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) |
Yamagishi, Hisao
× Yamagishi, Hisao× Ono, Takayuki× Fukunishi, Hiroshi× Yamagami, Takamasa× Nishimura, Jun× Kodama, Masahiro× Hirasima, Yo× Murakami, Hiroyuki× Holtet, Jan A.× Ullaland, Stein× Pellinen, Risto J. |
|||||
著者所属(英) | ||||||
en | ||||||
National Institute of Polar Research/National Institute of Polar Research/National Institute of Polar Research/The Institute of Space and Astronautical Science/The Institute of Space and Astronautical Science/Department of Physics, Yamanashi Medical College/Department of Physics, Rikkyo University/Department of Physics, Rikkyo University/Institute of Physics, University of Oslo/Department of Physics, University of Bergen/Finnish Meteorological Institute | ||||||
抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | A stratospheric balloon, carrying a Nal (T1) scintillation counter for measuring 20-100keV bremsstrahlung X-rays was launched from Stamsund (L=5.6) in Norway during the recovery phase of a magnetic substorm. The scintillation counter recorded many examples of X-ray microbursts and pulsations at a ceiling altitude of 7mb (33km). The ground-based VLF receiver at Andφya (L=6.1), located at 160km northeast of Stamsund, and at Syowa Station, Antarctica (L=6.1) observed polar chorus emissions and quasi-periodic (QP) emissions during the balloon flight. In the study of cross correlations between the X-ray and the VLF emissions, it has been found that the X-ray microbursts precede VLF chorus at Andφya by about 1.7s, while the VLF chorus at Syowa occurred almost simultaneously with the X-ray microbursts. This is qualitatively explained by the nature of counterstreaming type wave-particle interaction and the echoing of whistler mode wave packets in the magnetosphere. X-ray pulsations and rising-tone type QP emissions with periods of 20-30s showed a good coherency. This similarity suggests that both phenomena are closely related to each other through the cyclotron wave-particle interaction in the magnetosphere. | |||||
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 31, p. 124-136, 発行日 1984-07 |