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Effect of perpendicular a.c. electric field on the oblique whistler mode instability in the earth's magnetosphere

机译:垂直交流的影响磁层倾斜惠斯勒模式电场的不稳定性

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The elements of dielectric tensor and dispersion relation for obliquely propagating whistler waves with finite k(perpendicular to) in an infinite magnetoplasma are obtained for a kappa distribution in the presence of perpendicular a.c. electric field. Integrals and modified plasma dispersion functions are reduced in power series form. Numerical calculations have been performed to obtain temporal growth rate and real frequencies of the plasma waves for magnetospheric plasma, using linear theory of dispersion relation. The effect and modification introduced by the perpendicular a.c. electric field on the temporal growth rates, real frequencies and resonance condition are discussed for kappa and Maxwellian distributions. Our results and their interpretation are compared with known whistler observations obtained by ground-based techniques and satellite observations.
机译:对于存在垂直交流电时的κ分布,获得了在无限的磁等离子体中倾斜传播具有有限k(垂直于)的惠斯勒波的介电张量和色散关系的元素。电场。幂级数形式减少了积分和改进的等离子体弥散函数。利用色散关系的线性理论,已经进行了数值计算以获得磁层等离子体的等离子体波的时间增长率和实际频率。垂直交流电引入的效果和修改讨论了关于Kappa和Maxwellian分布的时间增长率,真实频率和共振条件的电场。我们的结果及其解释与通过地面技术和卫星观测获得的已知哨声观测结果进行了比较。

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