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中国物理学会期刊

激光驱动平面含混合层Richtmyer-Meshkov不稳定性增长实验研究

CSTR:32037.14.aps.75.20251432

Experimental study of laser-driven planar Richtmyer-Meshkov instability with a mixed layer

CSTR:32037.14.aps.75.20251432
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  • 金属材料内爆压缩过程中, 材料动态破坏形成的喷射物质会在材料界面之间形成具有密度分布的混合层, 该混合层会对后期的流体力学不稳定性发展及混合产生重要影响, 因此, 准确预测高能量密度条件下具有混合层的Richtmyer-Meshkov不稳定性增长及其引起的湍流混合, 对于理解天体物理中的多种现象和惯性约束聚变中的工程设计有着重要作用. 与激光装置上流体力学不稳定性实验研究常用的X射线背光成像方式相比, 本工作利用超环面弯晶测量泡沫材料中钛原子K壳层荧光信号, 实现了流体力学不稳定性增长过程中低密度混合层界面混合增长的测量. 基于神光Ⅲ原型激光装置, 开展了预热实验研究, 证实通过降低入射激光功率和掺杂的方式, 基本消除了预热对铝材料界面初始状态的影响. 在此基础上开展了不同密度混合层条件下的Richtmyer-Meshkov不稳定性实验研究, 实验结果显示, 在界面粗糙度相同的条件下, 阿特伍德数越大, 混合层与铝层界面非线性增长阶段的θ值越大, 低密度的混合层材料更有利于压缩, 扰动界面处存在更高的密度梯度和压力梯度, 从而在扰动界面处生成更多的涡量, 因此较低混合层密度条件下的Richtmyer-Meshkov不稳定性增长速度更快.

    During the implosion of metallic materials, the ejecta formed where the fragments were ejected from the shocked metal surface, and a mixed layer with finite width appears between two fluids, the mixed layer significantly influences the subsequent development of hydrodynamic instabilities and mixing. In inertial confinement fusion (ICF), the shock that passes through the roughened metal interface also causes the formation of ejecta. Therefore, accurate prediction of the growth of Richtmyer-Meshkov (RM) instability involving the mixed layer is crucial for understanding various phenomena in astrophysics and optimizing ICF engineering designs. However, in the experimental studies of RM instability on metal interfaces RM instability with a mixed layer, the opacity difference between the mixed layer and the metal sample is relatively small, this makes it difficult to accurately measure the RM instability growth using traditional X-ray backlighting imaging techniques.
    To address this issue, this study applies X-ray fluorescence imaging technology to the measurement of RM instability growth. This technique possesses fluid tracing characteristics and localized diagnostic capabilities. The K-shell fluorescence signals of titanium atoms in foam material are obtained by the curved bent crystal imaging system, it enables the measurement of the mixing evolution in low-density regions. More importantly, the signal intensity is approximately proportional to the density of the fluorescing material in X-ray fluorescence imaging, whereas the signal in traditional X-ray backlighting decays exponentially with material density. This allows fluorescence imaging to capture the perturbation structures of the mixing layer under much lower density conditions, obtain higher confidence data on the mixing growth at the interfaces between the mixing layer and the adjacent materials.
    In laser direct-drive experiments, the hard X-rays and superhot electrons generated by the direct laser loading of CH samples can heat the metal perturbation sample ahead of the shock. Preheating modifies the initial state of the perturbed interface before the shock arrives, thereby complicating the analysis of hydrodynamic instability evolution that depends on these original conditions. A preheat calibration experiment is conducted at the Shenguang-III prototype laser facility, the experimental results show that a 50 μm thick CH (3% bromine doping) layer and reducing the laser power can block the preheat, the increase in temperature before the arrival time of the shock wave is less than 200 K, which has little influence on the initial state of rear interface of the aluminum layer.
    In an effort to better understand the RM instability with a mixed layer, a laser-driven RM instability experiment under two mixed layer density conditions (0.2 and 0.5 g/cm3) has been performed at the Shenguang-III prototype laser facility. The experimental results show that under the condition of the same interface roughness, a larger Atwood number leads to a larger θ value during the nonlinear growth stage. The total amount of vorticity deposited by the shock wave determines the growth rate of the instability, the mixed layer with lower density exhibits better compressibility, and there are steeper density and pressure gradients. Therefore, the low-density mixed layer tends to deposit more vorticity at the interface, which in turn leads to a faster growth of RM instability.

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