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Laboratory observation of secondary shock formation ahead of a strongly radiative blast wave

机译:强烈辐射爆炸波之前二次冲击形成的实验室观察

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摘要

We have previously reported the experimental discovery of a second shock forming ahead of a radiative shock propagating in Xe. The initial shock is spherical, radiative, with a high Mach number, and it sends a supersonic radiative heat wave far ahead of itself. The heat wave rapidly slows to a transonic regime and when its Mach number drops to two with respect to the downstream plasma, the heat wave drives a second shock ahead of itself to satisfy mass and momentum conservation in the heat wave reference frame. We now show experimental data from a range of mixtures of Xe and N-2, gradually changing the properties of the initial shock and the environment into which the shock moves and radiates (the radiative conductivity and the heat capacity). We have successfully observed second shock formation over the entire range from 100% Xe mass fraction to 100% N-2. The formation radius of the second shock as a function of Xe mass fraction is consistent with an analytical estimate.
机译:我们先前已经报道了在Xe中传播的辐射冲击之前形成第二个冲击的实验发现。初始冲击是球形的,辐射性的,马赫数高,并且会发出超音速的辐射热波。热波迅速减慢到跨音速状态,并且当其马赫数相对于下游等离子体降到2时,热波会在自身之前驱动第二次冲击,从而满足热波参考系中的质量和动量守恒。现在,我们显示了一系列Xe和N-2混合物的实验数据,这些数据逐渐改变了初始激波的性质以及激波在其中移动和辐射的环境(辐射传导率和热容)。我们已经成功地观察到从100%Xe质量分数到100%N-2整个范围内的第二次冲击形成。作为Xe质量分数的函数的第二次冲击的形成半径与分析估计一致。

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