Velocity moment-based quasilinear theory and particle-in-cell simulation of parallel electron firehose instability

被引:22
|
作者
Yoon, P. H. [1 ,2 ,3 ]
Lopez, R. A. [1 ]
Seough, J. [3 ]
Sarfraz, M. [4 ]
机构
[1] Univ Maryland, Inst Phys Sci & Technol, College Pk, MD 20742 USA
[2] Kyung Hee Univ, Sch Space Res, Yongin, South Korea
[3] Korea Astron & Space Sci Inst, Daejeon 305348, South Korea
[4] GC Univ Lahore, Dept Phys, Katchery Rd, Lahore 54000, Pakistan
基金
新加坡国家研究基金会;
关键词
PROTON TEMPERATURE ANISOTROPY; SOLAR-WIND; MAGNETOSHEATH; SIGNATURES; CONSTRAINT; PLASMAS;
D O I
10.1063/1.4997666
中图分类号
O35 [流体力学]; O53 [等离子体物理学];
学科分类号
070204 ; 080103 ; 080704 ;
摘要
The present paper investigates the physics of electron firehose instability propagating parallel to the direction of ambient magnetic field vector, by means of particle-in-cell simulation and macroscopic quasilinear kinetic theory. The electron firehose instability is excited when parallel electron temperature exceeds perpendicular temperature, T-parallel to e > T-perpendicular to e, under high beta conditions. A recent paper [Sarfraz et al., Phys. Plasmas 24, 012907 (2017)] formulated the quasilinear theory of parallel electron firehose instability by assuming that the electron and proton velocity distribution functions can be approximately described by bi-Maxwellian forms for all times but allowing for dynamical changes in perpendicular and parallel temperatures as well as the wave intensity. The present paper examines the validity of such an approach by making direct comparison against particle- in-cell simulation. It is shown that the macroscopic quasilinear approach provides a qualitative description of the nonlinear phase of the instability, but some quantitative discrepancies are also found. Possible causes for the discrepancies are discussed. Published by AIP Publishing.
引用
收藏
页数:14
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