Rotating Alfvén waves in rotating plasmas

被引:2
|
作者
Rax, J. -m. [1 ,2 ]
Gueroult, R. [3 ]
Fisch, N. J. [4 ]
机构
[1] Princeton Univ, Andlinger Ctr Energy Environm, Princeton, NJ 08540 USA
[2] Univ Paris Saclay, IJCLab, F-91405 Orsay, France
[3] Univ Toulouse, CNRS, UPS, INPT,LAPLACE, F-31062 Toulouse, France
[4] Princeton Univ, Dept Astrophys Sci, Princeton, NJ USA
关键词
plasma waves; plasma dynamics; MAGNETIC ANTENNA EXCITATION; ORBITAL ANGULAR-MOMENTUM; LIGHT; POLARIZATION; EQUILIBRIUM; STABILITY;
D O I
10.1017/S0022377823001368
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
Angular momentum coupling between a rotating magnetized plasma and torsional Alfven waves carrying orbital angular momentum (OAM) is examined. It is demonstrated not only that rotation is the source of Fresnel-Faraday rotation - or orbital Faraday rotation effects - for OAM-carrying Alfven waves, but also that angular momentum from an OAM-carrying Alfven wave can be transferred to a rotating plasma through the inverse process. For the direct process, the transverse structure angular rotation frequency is derived by considering the dispersion relation for modes with opposite OAM content. For the inverse process, the torque exerted on the plasma is derived as a function of wave and plasma parameters.
引用
收藏
页数:15
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