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Study of stability in a liner-on-target gas puff Z-pinch as a function of pre-embedded axial magnetic field

机译:作为预嵌入式轴向磁场的函数的衬里靶气体滤波中的稳定性研究

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Gas puff Z-pinches are intense sources of X-rays and neutrons but are highly susceptible to the magneto-Rayleigh-Taylor instability (MRTI). MRTI mitigation is critical for optimal and reproducible yields, motivating significant attention toward various potential mitigation mechanisms. One such approach is the external application of an axial magnetic field, which will be discussed here in the context of recent experiments on the Zebra generator (1 MA, 100ns) at the University of Nevada, Reno. In these experiments, an annular Kr gas liner is imploded onto an on-axis deuterium target with a pre-embedded axial magnetic field Bz 0 ranging from 0 to 0.3T. The effect of Bz0 on the stability of the Kr liner is evaluated with measurements of plasma radius, overall instability amplitude, and dominant instability wavelength at different times obtained from time-gated extreme ultraviolet pinhole images. It was observed that the external axial magnetic field does not affect the implosion velocity significantly and that it reduces the overall instability amplitude and the presence of short-wavelength modes, indicating improved pinch stability and reproducibility. For the highest applied Bz0=0.3 T, the stagnation radius measured via visible streak images was found to increase. These findings are consistent with experiments reported in the literature, but here, the Bz0 required for stability, Bz0=0.13Ipk/R0 (where I-pk is the driver peak current and R-0 is the initial radius), is lower. This could be attributed to the smaller load geometry, both radially and axially. Consistent with other experiments, the cause of decreased convergence cannot be explained by the additional axial magnetic pressure and remains an open question. (C) 2020 Author(s). All article content, except where otherwise noted, is licensed under a Creative Commons Attribution (CC BY) license (http://creativecommons.org/licenses/by/4.0/).
机译:气体粉扑Z-Cipches是X射线和中子的强源,但高易受磁瑞利 - 泰勒不稳定性(MRTI)的影响。 MRTI缓解对于最佳和可重复的产量至关重要,激励对各种潜在缓解机制的重大关注。一种这样的方法是轴向磁场的外部施加,这将在这里将在Nevada大学Zebra发生器(1 MA,100ns)上的最新实验中讨论。在这些实验中,将环形KR气体衬垫用预嵌入的轴向磁场BZ 0从0到0.3T的预嵌入的轴向磁场BZ 0喷射到轴上的氘靶上。 BZ0对KR衬里的稳定性的影响,评估了从时间门控极紫外针孔图像获得的不同时间的等离子体半径,整体不稳积幅度和主要不稳定性波长的测量。观察到,外部轴向磁场不会显着影响内部速度,并且它降低了整体不稳定性幅度和短波长度模式的存在,表明改善的夹紧稳定性和再现性。对于最高施加的BZ0 = 0.3T,发现通过可见条纹图像测量的停滞半径增加。这些发现与文献中报道的实验一致,但这里,稳定性所需的BZ0,BZ0 = 0.13iPK / R0(其中I-PK是驱动器峰值电流,R-0是初始半径)。这可能归因于径向和轴向较小的负载几何形状。与其他实验一致,收敛性降低的原因不能通过额外的轴向磁力来解释,仍然是开放的问题。 (c)2020作者。除其他否则指出的情况外,所有文章内容都是根据Creative Commons atjection(CC)许可证的许可(http://creativecommons.org/licenses/by/4.0/)。

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