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首页> 外文期刊>Physics of plasmas >Interactions between H+ band EMIC waves and radiation belt relativistic electrons: Comparisons of test particle simulations with quasi-linear calculations
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Interactions between H+ band EMIC waves and radiation belt relativistic electrons: Comparisons of test particle simulations with quasi-linear calculations

机译:H +带EMIC波与辐射带相对主义电子之间的相互作用:用准线性计算比较测试粒子仿真

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摘要

We develop a general 3-D relativistic test particle (TP) simulation code to examine the trajectories and pitch angle variations of test electrons. We investigate the conditions when the electrons transit broadband, parallel propagating H+ band electromagnetic ion cyclotron (EMIC) waves to find whether the classical quasilinear theory (QLT) can be applied to interactions between H+ band EMIC waves and radiation belt relativistic (and ultra-relativistic) electrons. We find that to reach good consistency between TP scattering coefficients and QLT calculations, the wave-particle resonant interaction time (which indicates the time of particles traveling in the wave fields and being resonant with the wave fields) must be carefully calculated to ensure the validity of the linear diffusion process. This wave-particle resonant interaction time depends largely on the wave amplitude, the bandwidth, and the initial parameters of electrons for TP simulations; once the time of electrons traveling in the wave fields becomes large enough when the pitch angles of electrons scattered by wave fields reach the maximal value limited by the resonance condition and cannot be diffused any longer, the linear diffusion process of particles defined by QLT will not be valid any longer. When the resonant electrons start to travel through the wave field, they undergo the linear diffusion process resulting from the pitch angle scattering by the H+ band EMIC wave field. As the time of traveling in the wave fields increases, the test electrons will suffer effective pitch angle scattering and the pitch angles of these electrons will reach the maximum value limited by the resonance condition, which is determined by the wave and electron parameters. These electrons are then reflected by the wave fields and the linear wave-particle interactions defined by QLT will not be valid anymore. This kind of wave-particle interaction subsequently introduces considerable deviation of TP diffusion coefficients fro
机译:我们开发了一个一般的3-d相对论测试颗粒(TP)仿真代码检查轨迹和测试电子的桨距角的变化。我们研究的条件,当电子运输宽带,平行传播的H +频带电磁离子回旋(EMIC)波找到经典拟线性理论(QLT)是否可以应用到H +频带EMIC波和辐射带相对论(和超相对论之间的相互作用)电子。我们发现,要达到TP散射系数和QLT计算之间的一致性好,波粒共振作用时间(这表明在波场旅行,是与波场共振粒子的时间)必须精心计算,以确保有效性的线性扩散过程。此波粒共振相互作用时间在很大程度上取决于波振幅,带宽,和电子供TP模拟的初始参数;一旦电子在波场行驶时变得足够大时,由波场散射电子的桨距角到达由共振条件的限制的最大值,并且不能在任何较长的扩散,通过QLT定义颗粒的线性扩散过程中不会有效不再。当共振电子开始通过波场行进,它们经历从由H +频带EMIC波场俯仰角散射得到的线性扩散过程。如该波场增加行驶时,测试电子将受到有效节距角散射和这些电子的桨距角会到达由谐振条件,这是由波和电子参数来确定限制的最大值。这些电子然后通过QLT定义将不再有效的波场和线性波 - 粒子相互作用反射。这种波粒相互作用的随后介绍TP扩散系数的相当大的偏差来回

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  • 来源
    《Physics of plasmas》 |2019年第3期|共8页
  • 作者单位

    Wuhan Univ Sch Elect Informat Dept Space Phys Wuhan 430072 Hubei Peoples R China;

    Wuhan Univ Sch Elect Informat Dept Space Phys Wuhan 430072 Hubei Peoples R China;

    Univ Sci Technol China Dept Geophys &

    Planetary Sci CAS Key Lab Geospace Environm Hefei 230026 Anhui Peoples R China;

    Chinese Acad Sci Inst Geol &

    Geophys Key Lab Earth &

    Planetary Phys Beijing 100029 Peoples R China;

    Univ Calif Los Angeles Dept Earth Planetary &

    Space Sci Los Angeles CA 90095 USA;

    Wuhan Univ Sch Elect Informat Dept Space Phys Wuhan 430072 Hubei Peoples R China;

    Wuhan Univ Sch Elect Informat Dept Space Phys Wuhan 430072 Hubei Peoples R China;

    Wuhan Univ Sch Elect Informat Dept Space Phys Wuhan 430072 Hubei Peoples R China;

    Wuhan Univ Sch Elect Informat Dept Space Phys Wuhan 430072 Hubei Peoples R China;

    Wuhan Univ Sch Elect Informat Dept Space Phys Wuhan 430072 Hubei Peoples R China;

    Wuhan Univ Sch Elect Informat Dept Space Phys Wuhan 430072 Hubei Peoples R China;

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  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类 等离子体物理学;
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