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Whistler turbulence at the magnetopause: A nonlinear generation mechanism
Cai CL(蔡春林); Cao JB(曹晋宾); Zhou GC(周国成); Wang GJ(王国军); 北京8701信箱
Source PublicationPhysics of Plasmas
KeywordCollisionless Magnetic Reconnection Plasma-maser Waves Fluctuations Layer
AbstractThe plasma maser effect in the existence of enhanced kinetic Alfven wave turbulence is investigated as the generation mechanism of the whistler turbulence at the magnetopause. The numerical results of the growth rate show that on the scale of neither the ion inertial length nor the electron inertial length, the whistler waves can be excited, and the peak of the maximum growth rate occurs on the scale of the effective ion Larmor radius. The kinetic Alfven wave dynamics associated with the scale length of the effective ion Larmor radius is intrinsically important in the magnetic reconnection and leads to the generation of whistler turbulence. The theoretical model of the generation of whistler turbulence is useful for explaining the observations of intense electromagnetic fluctuations at the magnetopause.
Indexed BySCI
Funding Project中国科学院空间科学与应用研究中心
Document Type期刊论文
Corresponding Author北京8701信箱
Recommended Citation
GB/T 7714
Cai CL,Cao JB,Zhou GC,et al. Whistler turbulence at the magnetopause: A nonlinear generation mechanism[J]. Physics of Plasmas,2001,8(1):272-276.
APA 蔡春林,曹晋宾,周国成,王国军,&北京8701信箱.(2001).Whistler turbulence at the magnetopause: A nonlinear generation mechanism.Physics of Plasmas,8(1),272-276.
MLA 蔡春林,et al."Whistler turbulence at the magnetopause: A nonlinear generation mechanism".Physics of Plasmas 8.1(2001):272-276.
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