磁声波场中电子随机运动的研究:测试粒子模拟

IF 2.9 3区 地球科学 Earth and Planetary Physics Pub Date : 2021-12-21 DOI:10.26464/epp2021052
Kai Fan, XinLiang Gao, QuanMing Lu, Shui Wang
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引用次数: 1

摘要

利用测试粒子模拟方法,研究了能量为300 keV的电子在单色磁子波场中的随机运动。本研究的动机是违反准线性理论假设,当强MS波(振幅高达~ 1nt)存在于地球磁层中时。首先,当波幅超过一定阈值时,电子运动可以变得随机。如果一个电子最初通过弹跳共振与MS波发生共振,随着弹跳共振阶数的增加,电子随机运动的振幅阈值增加,直到在我们研究的第11阶左右达到峰值,然后振幅阈值缓慢下降。此外,我们发现电子和MS波之间的反弹和朗道共振的共存将显著降低振幅阈值。在某些情况下,在振幅低于1nt的MS波场中,电子运动可能会变得随机。无论如何,如果最初既不满足弹跳条件,也不满足朗道共振条件,那么随机运动的幅度阈值在低频时呈上升趋势,在高频时呈下降趋势,尽管幅度阈值总是很大(>5 nT)。我们的研究表明,在模拟地球磁层中强MS波调节的电子动力学时,也应考虑电子随机运动。
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Study on electron stochastic motions in the magnetosonic wave field: Test particle simulations

Using the test particle simulation method, we investigate the stochastic motion of electrons with energy of 300 keV in a monochromatic magnetosonic (MS) wave field. This study is motivated by the violation of the quasi-linear theory assumption, when strong MS waves (amplitude up to ~1 nT) are present in the Earth’s magnetosphere. First, electron motion can become stochastic when the wave amplitude exceeds a certain threshold. If an electron initially resonates with the MS wave via bounce resonance, as the bounce resonance order increases, the amplitude threshold of electron stochastic motion increases until it reaches the peak at about the 11th order in our study, then the amplitude threshold slowly declines. Further, we find that the coexistence of bounce and Landau resonances between electrons and MS waves will significantly reduce the amplitude threshold. In some cases, the electron motion can become stochastic in the field of an MS wave with amplitudes below 1 nT. Regardless, if neither the bounce nor Landau resonance condition is satisfied initially, then the amplitude threshold of stochastic motion shows an increasing trend for lower frequencies and a decreasing trend for higher frequencies, even though the amplitude threshold is always very large (> 5 nT). Our study suggests that electron stochastic motion should also be considered when modeling electron dynamics regulated by intense MS waves in the Earth’s magnetosphere.

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来源期刊
Earth and Planetary Physics
Earth and Planetary Physics GEOSCIENCES, MULTIDISCIPLINARY-
自引率
17.20%
发文量
174
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