瑞利-泰勒不稳定增长之谜:飞马座的线性研究

M. Sheppard, W. Atchison, R. Keinigs, J. Stokes
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引用次数: 4

摘要

Pegasus上的RTMIX系列的目标是研究金属-泡沫界面上收敛几何形状的瑞利-泰勒不稳定增长和混合,作为材料强度和初始扰动幅度的函数。给出了三个实验的结果。在之前的脉冲功率会议上报道的第一个实验涉及到一个固体z -夹紧衬垫,由/spl sim/5.5 MA的Pegasus电流驱动到高密度泡沫靶上。在第一次实验中,衬垫的内径是光滑的。正如预期的那样,在诊断的分辨率极限下没有观察到不稳定生长或混合。在第二个实验中,在内径上加工了波长为1.0 mm、振幅为12.5 /spl mu/m和50 /spl mu/m的方位对称正弦波扰动。预测了大振幅扰动的增长,但预计小振幅扰动的增长将被Cu的材料强度所抑制。振幅扰动都没有增加。第三个实验是第二个实验的重复,用低强度的Sn/In合金(代替Cu),应该在内爆早期熔化。Sn/In层与其取代的Cu层质量匹配。由于Sn/In层在不稳定减速阶段应该是液态的,所以材料强度不应该稳定,而且两个振幅扰动都应该显示出显著的增长。该实验的x光片初步检查表明没有瑞利-泰勒不稳定增长。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Rayleigh-Taylor instability growth enigma: liner studies on Pegasus
The goal of the RTMIX series on Pegasus is to study Rayleigh-Taylor instability growth and mixing in a convergent geometry, at a metal-foam interface, as a function of material strength and initial perturbation amplitude. Results of three experiments are presented. The first experiment, reported in the previous Pulsed Power Conference, involved a solid Z-pinch liner driven by a Pegasus current of /spl sim/5.5 MA onto a high-density foam target. The inside diameter of the liner was smooth for the first experiment. No instability growth or mixing was observed at the resolution limit of the diagnostics, as expected. In the second experiment, azimuthally symmetric sine-wave perturbations were machined onto the inner diameter with a wavelength of 1.0 mm and amplitudes of 12.5 /spl mu/m and 50 /spl mu/m. Growth of the large amplitude perturbations was predicted, but growth of the small amplitude perturbations was expected to be inhibited by the material strength of the Cu. Neither amplitude perturbation grew. The third experiment was a repeat of the second with a low-strength Sn/In alloy (in place of the Cu) that should have melted early in the implosion. The Sn/In layer was mass-matched to the Cu layer that it replaced. Since the Sn/In layer was expected to be liquid during the unstable deceleration phase, no material strength stabilization should have occurred, and both amplitude perturbations should have shown dramatic growth. Preliminary inspection of radiographs from this experiment indicates no Rayleigh-Taylor instability growth.
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