间歇性是大涡度模拟更快收敛的必然特征

Marcel Bock, Khaled Yassin, H. Kassem, Johannes Theron, L. J. Lukassen, Joachim Peinke
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引用次数: 0

摘要

研究了作为高分辨率数值模拟初始条件的高斯和间歇合成湍流。湍流场,即曼恩模型和间歇时间映射曼恩模型,被注入到大涡模拟中,随后研究了它们的收敛性。除了通常的一点和两点特征外,我们还研究了速度增量的高阶矩,以把握间歇性。在这里,我们表明,与初始条件无关,不断演化的湍流会收敛到一个共同的状态,这在科尔莫格罗夫的经典间歇湍流中得到了很好的体现。研究结果表明,如果将流入场的间歇参数调整为共同状态的参数,收敛行为会更快。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Intermittency, an inevitable feature for faster convergence of large eddy simulations
Gaussian and intermittent synthetically generated turbulences are investigated as initial conditions for high-resolution numerical simulations. Turbulent fields, namely the Mann and the intermittent Time-mapped Mann model, are injected into large eddy simulations, and subsequently their convergences are investigated. In addition to the usual one-point and two-point characterizations, the higher moments of the velocity increments are addressed to grasp the intermittency. Here, we show that independent of the initial conditions, the evolving turbulence converges to a common state, which is well represented by the classical intermittent turbulence of Kolmogorov. The findings reveal that if the intermittency parameters of the inflow field are adjusted to those of the common state, the convergence behavior is much faster.
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