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Blast-wave driven Kelvin-Helmholtz shear layers in a laser driven high-energy-density plasma

机译:激光驱动的高能量密度等离子体中的爆炸波驱动的Kelvin-Helmholtz剪切层

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摘要

The first successful high energy density Kelvin-Helmholtz (KH) shear layer experiments (O. A. Hurricane et al. in Phys. Plasmas, 16:056305, 2009; E. C. Harding et al. in Phys. Rev. Lett., 103:045005, 2009) demonstrated the ability to design and field a target that produces, in a controlled fashion, an array of large diagnosable KH vortices. Data from these experiments vividly showed the complete evolution of large (~400 μm) distinct eddies, from formation to apparent turbulent break-up in the span of about 75 ns. A second set of experiments, in which the density of a key carbon-foam material was varied, was recently performed. The new series showed a great deal of fine-structure that was not as apparent as in the original experiments. In this paper, the results of both experiments will be discussed along with supporting theory and simulation. An attempt is made to connect these observations with some turbulent scale-lengths. Finally, we speculate about the possible connection of these experiments to astrophysical contexts.
机译:第一个成功的高能密度开尔文-亥姆霍兹(KH)剪切层实验(OA Hurricane等人在Phys。Plasmas,16:056305,2009; EC Harding等人在Phys。Rev. Lett。,103:045005,2009 )展示了设计和部署目标的能力,该目标以受控方式产生大量可诊断的KH涡流。这些实验的数据生动地表明,在约75 ns的跨度内,大的(〜400μm)独特涡旋已完全演化,从形成到明显的湍流破裂。最近进行了第二组实验,其中改变了关键碳泡沫材料的密度。新系列显示出大量的精细结构,不像原始实验中那样明显。本文将对这两个实验的结果以及支持理论和仿真进行讨论。试图将这些观测值与一些湍流尺度长度联系起来。最后,我们推测了这些实验与天体物理环境的可能联系。

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