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Three-wave coupling and parametric decay of kinetic Alfven waves

机译:动态Alfven波的三波耦合和参数衰减

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The dynamic equation and coupling coefficient of the three-wave interaction among kinetic Alfven waves (KAWs) are derived by use of plasma kinetic theory. Linear and nonlinear effects of finite ion Larmor radius are kept for arbitrary value of the 'kinetic variable' k = k_⊥ρi. The parametric decay KAW → KAW + KAW is investigated and the threshold amplitude for decay instability in a Maxwellian plasma is calculated. The growth rate of decay instability varies as k_⊥~2 in both limits k~2 1 and k~2 1. The main tendency of KAWs is towards nonlinear destabilization at very low wave amplitudes B_k/B_0 approx.< 10~(-3). Two applications concerning KAW dynamics in the magnetosphere and in the solar corona show that three-wave resonant interaction among KAWs may be responsible for the turbulent character of their behaviour, often observed in space plasmas.
机译:利用等离子动力学理论推导了动力学阿尔夫文波之间的三波相互作用的动力学方程和耦合系数。对于“运动变量” k =k_⊥ρi的任意值,保持有限离子拉莫尔半径的线性和非线性影响。研究了参数衰减KAW→KAW + KAW,并计算了麦克斯韦等离子体中衰减不稳定性的阈值幅度。在两个极限k〜2 1和k〜2 1中,衰减不稳定性的增长率都随k_⊥〜2的变化而变化。KAW的主要趋势是在非常低的波幅B_k / B_0约<10时趋向于非线性失稳。 〜(-3)。关于磁层和太阳日冕中KAW动力学的两个应用表明,KAW之间的三波共振相互作用可能是其行为的湍流特征的原因,通常在空间等离子体中观察到这种行为。

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