Characterization of the Imploding Plasma Sheath in Triple Nozzle Gas-Puff Z-Pinches at 1 MA

E. Lavine, S. Rocco, J. Angel, E. Freeman, W. Potter, J. Greenly, D. Hammer, B. Kusse
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Abstract

Triple nozzle gas-puff implosions on the 1 MA, 220 ns COBRA generator at Cornell University provide an efficient source of intense x-ray radiation and are of interest for magneto-inertial fusion studies with an applied magnetic field. These implosions are susceptible to the magneto-Rayleigh-Taylor instability (MRTI); however, observations indicate that they are more stable than predicted by simple MRTI theory. Furthermore, the instability growth rate, characterized by an effective Atwood number, is observed to depend on gas species and initial fill density. Detailed measurements of the plasma parameters in the imploding plasma sheath can help to provide an explanation for these observations and can be used to validate simulation codes. To this end, we have used collective Thompson scattering, Zeeman polarization spectroscopy, and laser shearing interferometry to characterize the imploding plasma sheath at a radius of 1-1.5 cm for neon, argon, and krypton implosions with comparable linear mass densities. The preliminary results of this study are presented here.
1毫安时三喷嘴吹气z -夹紧中内爆等离子体护套的特性
康奈尔大学的1毫安、220毫安COBRA发生器上的三喷嘴气泡内爆提供了一种高效的强x射线辐射源,对应用磁场的磁惯性聚变研究很有意义。这些内爆易受磁-瑞利-泰勒不稳定性(MRTI)的影响;然而,观察表明,它们比简单的MRTI理论预测的更稳定。此外,观察到以有效阿特伍德数为特征的不稳定增长率取决于气体种类和初始填充密度。内爆等离子体鞘层中等离子体参数的详细测量有助于为这些观测提供解释,并可用于验证模拟代码。为此,我们使用了集体汤普森散射、塞曼偏振光谱和激光剪切干涉术来表征具有相似线性质量密度的氖、氩和氪内爆半径为1-1.5 cm的等离子体鞘层。本文给出了本研究的初步结果。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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