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Particle-in-cell simulations of the relaxation of electron beams in inhomogeneous solar wind plasmas

机译:非均匀太阳风等离子体中电子束弛豫的粒子模拟

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摘要

Previous theoretical considerations of electron beam relaxation in inhomogeneous plasmas have indicated that the effects of the irregular solar wind may account for the poor agreement of homogeneous modelling with the observations. Quasi-linear theory and Hamiltonian models based on Zakharov’s equations have indicated that when the level of density fluctuations is above a given threshold, density irregularities act to de-resonate the beam–plasma interaction, restricting Langmuir wave growth on the expense of beam energy. This work presents the first fully kinetic particle-in-cell (PIC) simulations of beam relaxation under the influence of density irregularities. We aim to independently determine the influence of background inhomogeneity on the beam–plasma system, and to test theoretical predictions and alternative models using a fully kinetic treatment. We carry out one-dimensional (1-D) PIC simulations of a bump-on-tail unstable electron beam in the presence of increasing levels of background inhomogeneity using the fully electromagnetic, relativistic EPOCH PIC code. We find that in the case of homogeneous background plasma density, Langmuir wave packets are generated at the resonant condition and then quasi-linear relaxation leads to a dynamic increase of wavenumbers generated. No electron acceleration is seen – unlike in the inhomogeneous experiments, all of which produce high-energy electrons. For the inhomogeneous experiments we also observe the generation of backwards-propagating Langmuir waves, which is shown directly to be due to the refraction of the packets off the density gradients. In the case of higher-amplitude density fluctuations, similar features to the weaker cases are found, but also packets can also deviate from the expected dispersion curve in $(k,unicode[STIX]{x1D714})$-space due to nonlinearity. Our fully kinetic PIC simulations broadly confirm the findings of quasi-linear theory and the Hamiltonian model based on Zakharov’s equations. Strong density fluctuations modify properties of excited Langmuir waves altering their dispersion properties.
机译:先前在不均匀等离子体中电子束弛豫的理论考虑表明,不规则太阳风的影响可能解释了均质模型与观测结果的较差一致性。准线性理论和基于Zakharov方程的汉密尔顿模型表明,当密度波动的水平超过给定阈值时,密度不规则现象会引起束流与等离子体相互作用的失谐,从而限制了Langmuir波的增长,从而浪费了束流能量。这项工作提出了在密度不规则的影响下束弛豫的第一个全动力学单元内粒子(PIC)模拟。我们旨在独立确定背景不均匀性对束流-等离子体系统的影响,并使用完全动力学处理来测试理论预测和替代模型。我们使用完全电磁的,相对论的EPOCH PIC代码,在背景不均匀性不断提高的情况下,对尾部凸块不稳定电子束进行一维(1-D)PIC模拟。我们发现,在均匀背景等离子体密度的情况下,在共振条件下会产生Langmuir波包,然后准线性松弛会导致所产生波数的动态增加。没有看到电子加速-与不均匀实验不同,所有实验均产生高能电子。对于非均匀实验,我们还观察到向后传播的朗缪尔波的产生,这直接表明是由于数据包从密度梯度折射而来。在高振幅密度波动的情况下,发现了与较弱情况相似的特征,但是由于非线性,数据包也可能偏离$(k, unicode [STIX] {x1D714})$-空间中的预期色散曲线。我们的全动力学PIC仿真广泛地证实了准线性理论和基于Zakharov方程的汉密尔顿模型的发现。强烈的密度波动会改变激发的朗缪尔波的特性,从而改变其色散特性。

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