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Orszag Tang vortex - Kinetic study of a turbulent plasma

机译:orszag唐涡旋 - 动荡血浆的动力学研究

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Kinetic evolution of the Orszag-Tang vortex is studied using collisionless hybrid simulations based on particle in cell ions and fluid electrons. In magnetohydrodynamics (MHD) this configuration leads rapidly to broadband turbulence. An earlier study [1] estimated the dissipation in the system. A comparison of MHD & hybrid simulations showed similar behavior at large scales but substantial differences at small scales. The hybrid magnetic energy spectrum shows a break at the scale where Hall term in the Ohm's law becomes important. The protons heat perpendicularly and most of the energy is dissipated through magnetic interactions. Here, the space time structure of the system is studied using frequency-wavenumber (k-co) decomposition. No clear resonances appear, ruling out the cyclotron resonances as a likely candidate for the perpendicular heating. The only distinguishable wave modes present, which constitute a small percentage of total energy, are magnetosonic modes.
机译:使用基于细胞离子和流体电子的颗粒的粒子混合模拟研究了orszag-ug涡旋的动力学演变。在磁性流动动力学(MHD)中,该配置迅速地促进宽带湍流。早期的研究[1]估计系统中的耗散。 MHD&Hybrid模拟的比较显示了大尺度的类似行为,但小尺度差异很大。混合磁能谱显示在欧姆法中的霍尔术语中的规模处于突破。质子热垂直和大部分能量通过磁性相互作用散发。这里,使用频率波数(K-CO)分解来研究系统的空间时间结构。出现清晰的共振,为垂直加热的可能候选者排出回旋环谐振。存在的唯一可区分波动模式,其构成总能量的小百分比,是磁性模式。

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