Parametric decay of oblique Alfven waves in two-dimensional hybrid simulations

被引:22
作者
Verscharen, D. [1 ,2 ]
Marsch, E. [1 ,3 ]
Motschmann, U. [2 ,4 ]
Mueller, J. [2 ]
机构
[1] Max Planck Inst Sonnensyst Forsch, D-37191 Katlenburg Lindau, Germany
[2] Tech Univ Carolo Wilhelmina Braunschweig, Inst Theoret Phys, D-38106 Braunschweig, Germany
[3] Univ Kiel, Inst Expt & Angew Phys, D-24098 Kiel, Germany
[4] DLR, Inst Planetenforsch, D-12489 Berlin, Germany
来源
PHYSICAL REVIEW E | 2012年 / 86卷 / 02期
关键词
MODULATIONAL INSTABILITY; FINITE-AMPLITUDE; SOLAR-WIND; PLASMA; PROTON; FIELD; POWER; EXCITATION; STABILITY; DAUGHTER;
D O I
10.1103/PhysRevE.86.027401
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
Certain types of plasma waves are known to become parametrically unstable under specific plasma conditions, in which the pump wave will decay into several daughter waves with different wavenumbers and frequencies. In the past, the related plasma instabilities have been treated analytically for various parameter regimes and by use of various numerical methods, yet the oblique propagation with respect to the background magnetic field has rarely been dealt with in two dimensions, mainly because of the high computational demand. Here we present a hybrid-simulation study of the parametric decay of a moderately oblique Alfven wave having elliptical polarization. It is found that such a compressive wave can decay into waves with higher and lower wavenumbers than the pump.
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页数:5
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