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  1. F300 宇宙地球環境研究所
  2. F300a 雑誌掲載論文
  3. 学術雑誌

Decay of nonlinear whistler mode waves : 1D versus 2D

http://hdl.handle.net/2237/00029071
http://hdl.handle.net/2237/00029071
ade5f9bb-20f8-4160-9b0e-a83a204abcfc
名前 / ファイル ライセンス アクション
1_5031483.pdf 1_5031483 (3.6 MB)
Item type 学術雑誌論文 / Journal Article(1)
公開日 2018-11-14
タイトル
タイトル Decay of nonlinear whistler mode waves : 1D versus 2D
言語 en
著者 Umeda, Takayuki

× Umeda, Takayuki

WEKO 87987

en Umeda, Takayuki

Search repository
Saito, Shinji

× Saito, Shinji

WEKO 87988

en Saito, Shinji

Search repository
Nariyuki, Yasuhiro

× Nariyuki, Yasuhiro

WEKO 87989

en Nariyuki, Yasuhiro

Search repository
アクセス権
アクセス権 open access
アクセス権URI http://purl.org/coar/access_right/c_abf2
権利
言語 en
権利情報 Copyright 2018 American Institute of Physics. This article may be downloaded for personal use only. Any other use requires prior permission of the author and AIP Publishing.The following article appeared in (Physics of Plasmas. v.25, n.7, 2018, p.072118) and may be found at (http://dx.doi.org/10.1063/1.5031483).
抄録
内容記述 Direct comparison between one-dimensional (1D) and two-dimensional (2D) models for the development of a nonlinear, short-wavelength, and monochromatic electromagnetic whistler mode wave is made by means of fully electromagnetic particle-in-cell simulations. The 1D and 2D simulations are performed for low beta conditions in which the plasma pressure is much lower than the magnetic pressure, although the plasma kinetic energy in the direction perpendicular to the ambient magnetic field is highly dominant due to the velocity field of the imposed parent whistler mode wave. A three-wave parametric decay of the parent whistler mode wave was reconfirmed in the 1D simulation. On the other hand, a rapid decay of the parent whistler mode wave thorough a five-wave interaction or double three-wave interactions was seen in the 2D simulation. Electron heating processes in the 2D simulation are also different from those in the 1D simulation. It is suggested that the present 2D decay process is a new instability which is quite different from velocity space instabilities driven by temperature/energy anisotropy.
言語 en
内容記述タイプ Abstract
内容記述
内容記述 ファイル公開:2019/07/01
言語 ja
内容記述タイプ Other
出版者
言語 en
出版者 AIP Publishing
言語
言語 eng
資源タイプ
資源タイプresource http://purl.org/coar/resource_type/c_6501
タイプ journal article
出版タイプ
出版タイプ AM
出版タイプResource http://purl.org/coar/version/c_ab4af688f83e57aa
DOI
関連タイプ isVersionOf
識別子タイプ DOI
関連識別子 https://doi.org/10.1063/1.5031483
ISSN(print)
収録物識別子タイプ PISSN
収録物識別子 1070-664X
ISSN(Online)
収録物識別子タイプ EISSN
収録物識別子 1089-7674
書誌情報 en : Physics of Plasmas

巻 25, 号 7, p. 072118, 発行日 2018-07
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