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Momentum transfer of solar wind plasma in a kinetic scale magnetosphere

http://hdl.handle.net/10655/00013572
http://hdl.handle.net/10655/00013572
379d0887-c627-4062-b8f9-d81ce1896138
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13770_Phys.Plasmas.pdf 13770_Phys.Plasmas (4.2 MB)
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Item type 学術雑誌論文 / Journal Article(1)
公開日 2023-03-14
タイトル
タイトル Momentum transfer of solar wind plasma in a kinetic scale magnetosphere
言語
言語 eng
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 MORITAKA, Toseo

× MORITAKA, Toseo

MORITAKA, Toseo

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KAJIMURA, Yoshihiro

× KAJIMURA, Yoshihiro

KAJIMURA, Yoshihiro

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USUI, Hideyuki

× USUI, Hideyuki

USUI, Hideyuki

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MATSUMOTO, Masaharu

× MATSUMOTO, Masaharu

MATSUMOTO, Masaharu

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MATSUI, Tatsuki

× MATSUI, Tatsuki

MATSUI, Tatsuki

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SHINOHARA, Iku

× SHINOHARA, Iku

SHINOHARA, Iku

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著者ID
内容記述タイプ Other
内容記述 0000-0003-2513-0453
抄録
内容記述タイプ Abstract
内容記述 Solar wind interaction with a kinetic scale magnetosphere and the resulting momentum transfer process are investigated by 2.5-dimensional full kinetic particle-in-cell simulations. The spatial scale of the considered magnetosphere is less than or comparable to the ion inertial length and is relevant for magnetized asteroids or spacecraft with mini-magnetosphere plasma propulsion. Momentum transfer is evaluated by studying the Lorentz force between solar wind plasma and a hypothetical coil current density that creates the magnetosphere. In the zero interplanetary magnetic field (IMF) limit, solar wind interaction goes into a steady state with constant Lorentz force. The dominant Lorentz force acting on the coil current density is applied by the thin electron current layer at the wind-filled front of the magnetosphere. Dynamic pressure of the solar wind balances the magnetic pressure in this region via electrostatic deceleration of ions. The resulting Lorentz force is characterized as a function of the scale of magnetosphere normalized by the electron gyration radius, which determines the local structure of the current layer. For the finite northward IMF case, solar wind electrons flow into the magnetosphere through the reconnecting region. The inner electrons enhance the ion deceleration, and this results in temporal increment of the Lorentz force. It is concluded that the momentum transfer of solar wind plasma could take place actively with variety of kinetic plasma phenomena, even in a magnetosphere with a small scale of less than the ion inertial length.
書誌情報 Physics of Plasmas

巻 19, 号 3, p. 032111, 発行日 2012-03-23
出版者
出版者 American Institute of Physics
ISSN
収録物識別子タイプ ISSN
収録物識別子 1070-664X
書誌レコードID
収録物識別子タイプ NCID
収録物識別子 AA10987555
DOI
関連タイプ isIdenticalTo
識別子タイプ DOI
関連識別子 10.1063/1.3683560
権利
権利情報 This content may be downloaded for personal use only.
権利
権利情報 Any other use requires prior permission of the author and the publisher.
権利
権利情報 This material originally appeared in Physics of Plasmas 19, 032111 (2012) and may be found at https://doi.org/10.1063/1.3683560.
権利
権利情報 Copyright 2012 Author(s).
権利
権利情報 This article is distributed under a Creative Commons Attribution (CC BY) License.
情報源
関連名称 Physics of Plasmas 19, 032111 (2012); https://doi.org/10.1063/1.3683560
関連サイト
識別子タイプ DOI
関連識別子 https://doi.org/10.1063/1.3683560
関連名称 Publisher version
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
NAIS
13770
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MORITAKA, Toseo, KAJIMURA, Yoshihiro, USUI, Hideyuki, MATSUMOTO, Masaharu, MATSUI, Tatsuki, SHINOHARA, Iku, 2012, Momentum transfer of solar wind plasma in a kinetic scale magnetosphere: American Institute of Physics , 032111– p.

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