首页> 外文期刊>Journal of Geophysical Research, A. Space Physics: JGR >Hybrid simulations of plasma transport by Kelvin-Helmholtz instability at the magnetopause: Density variations and magnetic shear
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Hybrid simulations of plasma transport by Kelvin-Helmholtz instability at the magnetopause: Density variations and magnetic shear

机译:混合模拟等离子体运输在磁层Kelvin-Helmholtz不稳定:密度变化和磁剪切

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摘要

Two-dimensional hybrid (kinetic ions and massless fluid electrons) simulations of the Kelvin-Helmholtz instability (KHI) for a magnetopause configuration with a varying density jump and magnetic shear across the boundary are carried out to examine how the transport of magnetosheath plasma into the magnetosphere is affected by these conditions. Low magnetic shear conditions where the magnetosheath magnetic field is within 30° of northward is included in the simulations because KHI is thought to be important for plasma transport only for northward or near-northward interplanetary magnetic field orientations. The simulations show that coherent vortices can grow for these nearnorthward angles and that they are sometimes more coherent than for pure northward conditions because the turbulence which breaks down these vortices is reduced when there are magnetic tension forces. With increasing magnetic shear angle and increasing density jump, the growth rate is reduced, and the vortices do not grow to as large of a size, which reduces the plasma transport. By tracking the individual particle motions, diffusion coefficients can be obtained for the system, where the diffusion is not classical in nature but instead has a time dependence resulting from both the increasingly large-scale vortex motion and the small-scale turbulence generated in the breakdown of the instabilities. Results indicate that diffusion on the order of 109 m2/s could possibly be generated by KHI on the flanks of the magnetosphere.
机译:二维混合(离子动力学和质量流体模拟电子)Kelvin-Helmholtz不稳定(地块)不同密度的磁层配置跳和磁剪切边界进行检查的运输方式磁鞘等离子体在磁气圈受到这些条件的影响。磁场条件下,磁鞘是在30°向北是包含在因为川崎被认为是模拟重要的等离子体传输向北或near-northward星际磁场取向。为这些nearnorthward漩涡能长角他们有时更连贯因为纯北方条件分解这些动荡漩涡减少当有磁张力的力量。随着磁剪切角和增加密度,增长速度减少,漩涡不会长大的大小,降低了等离子体传输。跟踪单个粒子的运动,扩散系数可以获得的系统,扩散不是古典的地方自然,而是具有时间依赖性造成越来越大涡动和小规模的动荡生成的故障不稳定。结果表明,扩散的109平方米/ s可能产生在川崎重工磁气圈的侧翼。

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