亚阿尔芬等离子体膨胀

B. Ripin, J. Huba, E. Mclean, C. Manka, T. Peyser, H. Burris, J. Grun
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引用次数: 86

摘要

当亚阿尔菲尼膨胀到磁场中时,大离子拉莫尔半径等离子体经历了一种特别强大的瑞利-泰勒不稳定性。报告了这种不稳定性的实验研究结果,并与理论进行了比较,特别是磁流体动力学(MHD)处理,包括霍尔项,广义动力学低混合漂移理论,以及计算机模拟。许多理论预测得到了证实,但仍有一些特征无法解释。在这种不稳定性的发展过程中出现了新的和不寻常的特征。在线性阶段,存在一个对磁场不敏感的起始判据,初始密度团块(相对于交换),线性增长率远高于“经典”MHD体制,以及与等离子体密度尺度长度数量级的主要不稳定波长。在非线性极限自由流的凹槽中,凹槽的明显分裂(分岔),电子回旋意义上的凹槽卷曲,以及高度不对称的膨胀。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Sub-Alfvenic plasma expansion
A large ion Larmor radius plasma undergoes a particularly robust form of Rayleigh–Taylor instability when sub‐Alfvenically expanding into a magnetic field. Results from an experimental study of this instability are reported and compared with theory, notably a magnetohydrodynamic (MHD) treatment that includes the Hall term, a generalized kinetic lower‐hybrid drift theory, and with computer simulations. Many theoretical predictions are confirmed while several features remain unexplained. New and unusual features appear in the development of this instability. In the linear stage there is an onset criterion insensitive to the magnetic field, initial density clumping (versus interchange), linear growth rate much higher than in the ‘‘classic’’ MHD regime, and dominant instability wavelength of order of the plasma density scale length. In the nonlinear limit free‐streaming flutes, apparent splitting (bifurcation) of flutes, curling of flutes in the electron cyclotron sense, and a highly asymmetric expansion are ...
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