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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

Validity of the fluid description of critical β and Alfvén time scale of ballooning instability onset in the near-Earth collisionless high-β plasma

http://hdl.handle.net/2261/38136
http://hdl.handle.net/2261/38136
256dc354-607f-4b0c-bd89-074109dd5eb9
名前 / ファイル ライセンス アクション
JGR_A109_NA02_02211.pdf JGR_A109_NA02_02211.pdf (724.9 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 Validity of the fluid description of critical β and Alfvén time scale of ballooning instability onset in the near-Earth collisionless high-β plasma
言語
言語 eng
キーワード
主題Scheme Other
主題 ballooning instability
キーワード
主題Scheme Other
主題 MHD description
キーワード
主題Scheme Other
主題 collisionless high-beta plasma
キーワード
主題Scheme Other
主題 Alfvén time scale
キーワード
主題Scheme Other
主題 near-Earth tail
キーワード
主題Scheme Other
主題 substorm onset
資源タイプ
資源 http://purl.org/coar/resource_type/c_6501
タイプ journal article
著者 Miura, Akira

× 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 For a realistic, highly stretched, two-dimensional tail configuration, in which the pressure gradient force is balanced with the curved field line tension force at the equator, the growth rates and the real frequencies of the ideal magnetohydrodynamic (MHD) and two component fluid (nonideal MHD) ballooning modes, in which the phrase “two component fluid” means that the Hall and the electron pressure gradient terms are included in the generalized Ohm's law, the ion bounce frequency ω bi , the ion magnetic drift frequency ω di , the ion diamagnetic drift frequency ω*i , and the ion cyclotron frequency ω ci are calculated numerically at the equator as a function of X from the near-Earth tail (X = −15 R E ) to the midtail (X = −30 R E ). Contrary to the well-known dipole field case, in which the bounce frequency decreases with increasing ∣X∣, the ion bounce frequency increases with ∣X∣ for the tail configuration. The ion magnetic drift frequency dominated by the curvature drift frequency also increases with increasing ∣X∣. The exact growth rates of the ideal and nonideal ballooning modes, γ e and γ ne , which are nearly equal, are given by 1.22V A /R c , where V A is the Alfvén velocity and R c is the field line curvature radius at the equator, and satisfy ω bi , ω di , ω*i < γ e < ω ci on average in the near-Earth tail at X ∼ −15 R E . Also, the ion motion remains adiabatic in the near-Earth tail at X ∼ −15 R E . Therefore it is a posteriori verified that the fluid or MHD description of the linear stability of the ballooning instability is valid, and the critical β and the Alfvén time scale τ A ∼ R c /V A of the ballooning instability onset obtained by the fluid theory are validated in the near-Earth tail as close as 15 R E from the Earth. Despite the plasma being collisionless and high-β in the near-Earth tail, the subtle collisionless kinetic effects due to the field line curvature in high-β collisionless plasma are not significant enough to invalidate the fluid description in the near-Earth tail. The Alfvén time scale of an e-folding growth of the Alfvén wave trapped within R c in the equatorial region is of the order of a few tens of seconds or less in the near-Earth tail. It is faster than the bounce time of the bulk of ions and can explain the observed rapid time scale of a substorm onset. There is excellent agreement between the critical β and the Alfvén time scale obtained analytically for the two component fluid plasma and those obtained by a three-dimensional particle simulation.
書誌情報 Journal of geophysical research. A

巻 109, 号 2, p. A02211, 発行日 2004-02
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/10.1029/2003JA009924
権利
権利情報 copyright 2004 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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