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Simulation of high energy tail of electron distribution function
https://doi.org/10.15094/00006376
https://doi.org/10.15094/0000637667a61f0b-378e-4196-93ad-9a0e2b3eb4b7
名前 / ファイル | ライセンス | アクション |
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KJ00000729571 (265.8 kB)
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Item type | 紀要論文(ELS) / Departmental Bulletin Paper(1) | |||||
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公開日 | 2004-08-01 | |||||
タイトル | ||||||
タイトル | Simulation of high energy tail of electron distribution function | |||||
言語 | ||||||
言語 | eng | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | Incoherent scatter spectra | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | active experiments | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | artificial airglow | |||||
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 | |||||
ID登録 | ||||||
ID登録 | 10.15094/00006376 | |||||
ID登録タイプ | JaLC | |||||
ページ属性 | ||||||
内容記述タイプ | Other | |||||
内容記述 | P(論文) | |||||
著者名(英) |
Gustavsson, Björn
× Gustavsson, Björn× Sergienko, Timothy× Haggstrom, Ingemar× Honary, Farideh× Aso, Takehiko |
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著者所属(英) | ||||||
en | ||||||
National Institute of Polar Research | ||||||
著者所属(英) | ||||||
en | ||||||
Swedish Institute of Space Physics | ||||||
著者所属(英) | ||||||
en | ||||||
EISCAT Scientific Association | ||||||
著者所属(英) | ||||||
en | ||||||
Department of Communication systems, Lancaster University | ||||||
著者所属(英) | ||||||
en | ||||||
National Institute of Polar Research | ||||||
抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | This report presents Monte Carlo simulations of the electron energy distribution for alow ionized plasma interacting with the F-region neutral gas. The results show a depletion in theelectron distribution above 2 eV between 10 and 80 %, decreasing with altitude. The depletion ismainly due to electron energy loss to . This micro-physical energy transfer model gives goodagreement with optical observations of enhanced emissions from at 6300Å and EISCATUHF measurements of electron cooling during HF radio wave heating experiments. Someimplications for incoherent scatter spectra are derived. The results suggest that a weak(approximately 1000 times weaker than the ion-line) and wide (2 MHz) peak around +-1 MHz fromthe ion-line in the EISCAT VHF incoherent scatter spectrum should be a consequence of theelectron-neutral interaction. | |||||
雑誌書誌ID | ||||||
収録物識別子タイプ | NCID | |||||
収録物識別子 | AA11397422 | |||||
書誌情報 |
Advances in polar upper atmosphere research 巻 18, p. 1-9, 発行日 2004-08 |
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出版者 | ||||||
出版者 | National Institute of Polar Research |