合唱波的电子扩散:纬度波功率谱的影响

IF 2.6 3区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS
Jiang Yu, Jing Wang, Zhaoguo He, Zuzheng Chen, Liuyuan Li, Jun Cui, Jinbin Cao
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引用次数: 0

摘要

在本文中,我们研究了与纬度相关的波功率谱对合唱与电子相互作用的影响。与纬度变化模型相比,广泛采用的纬度恒定模型在评估电子扩散系数和由此产生的电子时间演化方面存在很大误差。纬度恒定模型往往会高估(低估)200 千伏以下(200 千伏以上)电子的扩散系数。高估和低估主要局限于小到中间的俯仰角,随着俯仰角的减小而增大,最高可达几个数量级。扩散系数的巨大差异极大地改变了电子相空间密度的净变化以及由此产生的电子俯仰角分布形状。我们的模拟结果表明,沿磁场线的波功率谱分布在控制辐射带电子动力学方面起着重要作用。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Electron diffusion by chorus waves: effects of latitude-dependent wave power spectrum
In the present paper, we investigate the effects of latitude-dependent wave power spectrum on the interactions of chorus with electrons. Great errors in evaluating the electron diffusion coefficients and the resultant electron temporal evolutions are introduced by the widely adopted latitudinally constant model, compared with the latitudinally varying model. The latitudinally constant model tends to overestimate (underestimate) the diffusion coefficients for electrons below (above) 200 keV. The overestimation and underestimation are mainly confined in small to intermediate pitch angles, increase with decreasing pitch angles, and can reach up to several orders of magnitude. The large differences in diffusion coefficients significantly alter the net changes of electron phase space densities and the resultant shapes of electron pitch angle distributions. Our simulations demonstrate that the wave power spectrum distribution along the magnetic field line plays an important role in controlling the dynamics of radiation belt electrons.
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来源期刊
Frontiers in Astronomy and Space Sciences
Frontiers in Astronomy and Space Sciences ASTRONOMY & ASTROPHYSICS-
CiteScore
3.40
自引率
13.30%
发文量
363
审稿时长
14 weeks
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