Modulational instability of the interacting electron whistlers and magnetosonic perturbations

IF 2.1 3区 物理与天体物理 Q2 PHYSICS, FLUIDS & PLASMAS Journal of Plasma Physics Pub Date : 2024-02-28 DOI:10.1017/s002237782400014x
Jiao-Jiao Cheng, Fang-Ping Wang, Zhong-Zheng Li, Wen-Shan Duan
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Abstract

A modulational instability of nonlinearly interacting electron whistlers and magnetosonic perturbations is studied in the present paper. For typical parameters, there is no modulational instability. However, modulational instability appears in special cases. For example, when the whistler wavenumber is small enough, there is modulational instability. Its growth rate decreases as the angle between the external magnetic field and the perturbed wave's direction increases, while it increases as the whistler wavenumber increases. It is also found that there is no modulational instability when the whistler wavenumber is larger than a critical value ( $k_0 > 0.05$ ), in which the perturbed wave frequency increases as the angle between the external magnetic field and the perturbed wave's direction increases when the angle between the external magnetic field and the perturbed wave's direction is large enough. Whereas, the perturbed wave frequency first increases as the whistler wavenumber increases, reaches a peak value and then decreases as whistler wavenumber increases.
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相互作用的电子啸风的调制不稳定性和磁声扰动
本文研究了非线性相互作用的电子哨兵和磁声扰动的调制不稳定性。对于典型参数,不存在调制不稳定性。然而,在特殊情况下会出现调制不稳定性。例如,当啸子的波数足够小时,就会出现调制不稳定性。其增长率随着外磁场与扰动波方向夹角的增大而减小,而随着惠斯勒文波数的增大而增大。研究还发现,当惠斯勒波文数大于临界值($k_0 >0.05$)时,扰动波频率不会随着外磁场与扰动波方向夹角的增大而增大,当外磁场与扰动波方向夹角足够大时,扰动波频率不会随着外磁场与扰动波方向夹角的增大而增大。而扰动波频率则是先随着惠斯勒波文数的增加而增加,达到峰值后再随着惠斯勒波文数的增加而降低。
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来源期刊
Journal of Plasma Physics
Journal of Plasma Physics 物理-物理:流体与等离子体
CiteScore
3.50
自引率
16.00%
发文量
106
审稿时长
6-12 weeks
期刊介绍: JPP aspires to be the intellectual home of those who think of plasma physics as a fundamental discipline. The journal focuses on publishing research on laboratory plasmas (including magnetically confined and inertial fusion plasmas), space physics and plasma astrophysics that takes advantage of the rapid ongoing progress in instrumentation and computing to advance fundamental understanding of multiscale plasma physics. The Journal welcomes submissions of analytical, numerical, observational and experimental work: both original research and tutorial- or review-style papers, as well as proposals for its Lecture Notes series.
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