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

Distortion of the nightside boundary of the "firmly-closed" region in the 1996 Tsyganenko magnetic field model

https://iwate-u.repo.nii.ac.jp/records/12583
https://iwate-u.repo.nii.ac.jp/records/12583
1c1499af-4a6b-4297-a679-345aa93cdfb0
名前 / ファイル ライセンス アクション
apuar-v15p43-60.pdf apuar-v15p43-60.pdf (663.7 kB)
アイテムタイプ 学術雑誌論文 / Journal Article(1)
公開日 2010-01-04
タイトル
タイトル Distortion of the nightside boundary of the "firmly-closed" region in the 1996 Tsyganenko magnetic field 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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Inoue, Shoshi

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Inoue, Shoshi

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Ozaki, Masao

× Ozaki, Masao

Ozaki, Masao

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

巻 15, p. 43-60, 発行日 2001-01-01
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 This paper proposes that the outer boundary of the "firmly-closed" region should be represented by field lines with the adiabaticity parameter, K, equal to unity at the equator, where K^2 is the ratio between the radius of the field-line curvature and the Larmor radius of an ion with 1 keV of energy. Just outside the boundary where K = 1, plasma particles (primarily ions) can be nonadiabatically accelerated in the presence of the dawn-to-dusk electric field. An inwardly convecting flux tube will attain the maximum content of nonadiabatically accelerated particles when it passes the K - 1 boundary. Thus, the K = 1 boundary outlines the region of the plasma population with a maximum content of nonadiabatically accelerated particles. In addition, the field lines with K = 1 are shown to have a minimum field strength of roughly 1 nT at the equator. From this fact, a field line with k < 1 may not be considered as being "firmly-closed" in the sense that such a field line may easily merge with an interplanetary field line. The outer boundary of the nightside firmly-closed region in the Tsyganenko model has an IMF Bz dependence that is consistent with observations. Moreover, this boundary is found to be "distorted", favoring the generation of region 1 field-aligned currents.
出版者
出版者 National Institute of Polar Research
権利
権利情報 (c) 2001 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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