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Spectral Characteristics of Separation Shock Unsteadiness

机译:分离冲击不稳定的光谱特征

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Spectra of wall pressure fluctuations caused by separation shock unsteadiness were compared for data obtained from wind tunnel experiments, the HIFiRE-1 flight test, and large-eddy simulations. The results were found to be in generally good agreement, despite varying Mach number and two orders of magnitude difference in Reynolds number. Relatively good agreement was also obtained between these spectra and the predictions of a theory developed by Plotkin, which depicts the separation shock unsteadiness as linearly damped Brownian motion. Further, the predictions of this theory are qualitatively consistent with the results of experiments in which the shock motion was synchronized to controlled perturbations. The results presented here support the idea that separation unsteadiness has common features across a broad range of compressible flows.
机译:比较了由分离冲击不稳定引起的壁面压力波动的频谱,这些数据是从风洞实验,HIFiRE-1飞行试验和大涡模拟中获得的数据进行了比较。尽管变化的马赫数和雷诺数有两个数量级的差异,但结果基本一致。这些光谱与Plotkin提出的理论的预测之间也获得了相对较好的一致性,该理论将分离冲击的不稳定描述为线性阻尼布朗运动。此外,该理论的预测在质量上与冲击运动与受控扰动同步的实验结果一致。此处提出的结果支持这样的想法,即分离不稳定在广泛的可压缩流中具有共同的特征。

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