Resonant Absorption and Fluctuations via Hybrid Simulations on Coronal Loops. I. Plasma Multifluid Description

Hugo A. Carril, Jaume Terradas, Roberto E. Navarro, Adolfo F. Viñas and Marcel Goossens
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Abstract

We investigate the resonant absorption process of a combination of left- and right-hand polarized waves (with a fixed perturbation amplitude) in a plasma slab with linearly inhomogeneous particle densities. Different thicknesses of the layers and angles of the background magnetic field to the plane of the slab, representing the degree of magnetization of the slab, are studied via 2D−3V PIC-hybrid simulations with a fixed perturbation amplitude. We identify the process of resonant absorption of the large-scale mode in the inhomogeneous layers and compare the damping rate of the transverse oscillations with single-fluid, linear MHD estimations. By following the spectral densities of the magnetic field fluctuations, it is found that kinetic scales are achieved in most of the simulated cases, particularly in the case of thinner inhomogeneous layers and in cases where the plasma slab is not weakly magnetized. In particular, the scales of the fluctuations can reach the proton inertial length. The small-scale fluctuations are identified as quasi-perpendicular oscillations localized within the inhomogeneous layers, and their properties in the spectral representation agree with theoretical properties of kinetic Alfvén waves predicted by kinetic and Hall-MHD theories.
基于日冕环混合模拟的共振吸收和波动。1 .等离子体多流体描述
我们研究了在线性非均匀粒子密度的等离子体板中左右极化波(具有固定扰动振幅)的共振吸收过程。通过固定扰动幅值的二维−3V pic混合模拟,研究了不同层厚度和背景磁场与板料平面的夹角(代表板料的磁化程度)。我们确定了非均匀层中大尺度模式的共振吸收过程,并将横向振荡的阻尼率与单流体线性MHD估计进行了比较。通过跟踪磁场波动的谱密度,发现在大多数模拟情况下,特别是在较薄的非均匀层和等离子体板不是弱磁化的情况下,都实现了动力学尺度。特别是,波动的尺度可以达到质子惯性长度。小尺度波动被确定为局部定域于非均匀层内的准垂直振荡,其谱表示性质与动力学理论和Hall-MHD理论预测的动力学alfv波浪的理论性质一致。
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