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  1. 115 理学系研究科・理学部
  2. 06 地球惑星科学専攻
  3. 1150610 学術雑誌論文
  1. 0 資料タイプ別
  2. 10 学術雑誌論文
  3. 014 自然科学

Pressure-driven and ionosphere-driven modes of magnetospheric interchange instability

http://hdl.handle.net/2261/38138
http://hdl.handle.net/2261/38138
a27c1a9a-944a-41d5-921e-b4a358371cea
名前 / ファイル ライセンス アクション
JGR_A114_a02224.pdf JGR_A114_a02224.pdf (299.0 kB)
Item type 学術雑誌論文 / Journal Article(1)
公開日 2016-12-28
タイトル
タイトル Pressure-driven and ionosphere-driven modes of magnetospheric interchange instability
言語
言語 eng
キーワード
主題Scheme Other
主題 interchange instability
キーワード
主題Scheme Other
主題 MHD instability
キーワード
主題Scheme Other
主題 inner magnetosphere
資源タイプ
資源 http://purl.org/coar/resource_type/c_6501
タイプ journal article
著者 Miura, Akira

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Miura, Akira

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著者所属
著者所属 Department of Earth and Planetary Physics, University of Tokyo
抄録
内容記述タイプ Abstract
内容記述 A general stability criterion for magnetospheric interchange instability, which includes an ionospheric destabilizing contribution, is derived for an arbitrary finite-β magnetospheric model satisfying the magnetohydrostatic force balance. The derivation is based on the magnetospheric energy principle. Unperturbed field-aligned currents in finite-β nonaxisymmetric magnetospheric models are assumed to close via diamagnetic currents in the magnetosphere or in the ionosphere. By exploiting the limit of a very large perpendicular wave number and the eikonal representation for the perpendicular plasma displacement, the magnetospheric interchange mode is shown to be compressible. In this limit the kink mode makes no contribution to the change in the magnetospheric potential energy. By using magnetospheric flux coordinates, the explicit form of the magnetospheric potential energy change is calculated for interchange perturbations, which do not bend magnetospheric magnetic fields. For a nonaxisymmetric finite-β magnetospheric model, a combined effect of the pressure gradient and field line curvature, not only in the meridional plane but also in the plane parallel to the longitudinal direction, is responsible for pressure-driven interchange instability. For an axisymmetric, north-south symmetric and low-β magnetospheric model, in which the magnetic field is approximated by a dipole field, the m = 1 or m = 2 ionosphere-driven mode, where m is the azimuthal mode number, has an upper critical equatorial β value for instability in the order of 1. Thus a substantial region of the inner magnetosphere or the near-Earth magnetosphere may be unstable against ionosphere-driven interchange instability caused by a horizontal plasma displacement on the spherical ionospheric surface
書誌情報 Journal of geophysical research. A

巻 114, p. A02224, 発行日 2009-02
ISSN
収録物識別子タイプ ISSN
収録物識別子 01480227
書誌レコードID
収録物識別子タイプ NCID
収録物識別子 AA10819721
DOI
識別子タイプ DOI
関連識別子 info:doi/10.1029/2008JA013663
権利
権利情報 copyright 2009 by the American Geophysical Union
日本十進分類法
主題Scheme NDC
主題 450
出版者
出版者 American Geophysical Union
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