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  1. 020 教育 Education
  2. 01 学術雑誌掲載論文

Evaluation of the region 1 field-aligned current from the low-latitude boundary layer using the 1989 Tsyganenko model

https://iwate-u.repo.nii.ac.jp/records/12584
https://iwate-u.repo.nii.ac.jp/records/12584
66008540-9aaa-415c-9d1d-b620bfe9d9b3
名前 / ファイル ライセンス アクション
apuar-v16p13-35.pdf apuar-v16p13-35.pdf (1.6 MB)
Item type 学術雑誌論文 / Journal Article(1)
公開日 2010-01-04
タイトル
タイトル Evaluation of the region 1 field-aligned current from the low-latitude boundary layer using the 1989 Tsyganenko model
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 journal article
著者 Yamamoto, Takashi

× Yamamoto, Takashi

Yamamoto, Takashi

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Ozaki, Masao

× Ozaki, Masao

Ozaki, Masao

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Inoue, Shoshi

× Inoue, Shoshi

Inoue, Shoshi

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著者(機関)
値 Department of Earth and Planetary Science, University of Tokyo
著者(機関)
値 Institute of Industrial Science, University of Tokyo, (present address)Tokyo University of Agriculture
著者(機関)
値 Faculty of Education, Iwate University
登録日
日付 2010-01-04
書誌情報 Advances in polar upper atmosphere research

巻 16, p. 13-35, 発行日 2002-01-01
ISSN
収録物識別子タイプ ISSN
収録物識別子 1345-1065
Abstract
内容記述タイプ Other
内容記述 On the basis of the 1989 Tsyganenko magnetic field model, the field-aligned current (FAC) density distribution in the low-latitude boundary layer (LLBL) is numerically evaluated by assuming the entry of magnetosheath particles into the LLBL. The calculated FAC density/intensity profiles are consistent with observations. This FAC generation arises from the divergence of the magnetic drift current density carried by LLBL particles, and the current intensity is then increased with their kinetic energy density. The FAC generation occurs at the inner edge of the LLBL whenever sheath particles penetrate into the magnetosphere, regardless of the entry process. It is also emphasized that the LLBL FAC production is an inevitable consequence of the formation of the magnetopause, because the magnetopause currents act to shield the magnetic field originating from the currents inside the closed region of the magnetosphere, causing the LLBL inner edge to intersect the magnetic drift paths. This simple situation can be illustrated by calculating the distribution of the flux tube volume in the Tsyganenko model.
出版者
出版者 National Institute of Polar Research
権利
権利情報 (c) 2002 National Institute of Polar Research
著者版フラグ
出版タイプ VoR
出版タイプResource http://purl.org/coar/version/c_970fb48d4fbd8a85
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