Simulation on Emission of Whistler and Electromagnetic Waves from Kelvin-Helmholtz Instability Region in a Plasma
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概要
- 論文の詳細を見る
We present the simulation results by using a two-dimensional electromagnetic and relativistic particle-in-cell (PIC) code that both whistler and electromagnetic waves can be emitted from a region where the Kelvin-Helmholtz instability occurs in electron-ion plasmas. The emission mechanism of the whistler waves is due to the generation of electron Hall current, which is produced by the electron vortex motions associated with the Kelvin-Helmholtz instability.
- 理論物理学刊行会の論文
- 2000-04-28
著者
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Sakai J
Toyama Univ. Toyama
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SAKAI Jun-ichi
Laboratory for Plasma Astrophysics and Fusion Science, Department of Electronics and Information, Fa
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Sakai Jun-ichi
Laboratory For Plasma Astrophysics Faculty Of Engineering Toyama University
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Sakai J
Laboratory For Plasma Astrophysics Faculty Of Engineering Toyama University
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NAKAYAMA Takuya
Laboratory for Plasma Astrophysics, Faculty of Engineering, Toyama University
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NAMBU Mitsuhiro
Tokyo Metropolitan Institute of Technology
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NEUBERT Torsten
Danish Meteorological Institute
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Nakayama Takuya
Laboratory For Plasma Astrophysics Faculty Of Engineering Toyama University
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南部 充宏
東京都立科学技術大学
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Nakayama T
Laboratory For Plasma Astrophysics Faculty Of Engineering Toyama University
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Neubert T
Danish Meteorological Institute
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NAMBU Mitsuhrro
Tokyo Metropolitan Institute of Technology
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SAKAI Jun-Ichi
Faculty of Engineering, Toyama University
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