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TURBULENCE-RADIATION INTERACTIONS IN FLAMES: A CHAOTIC-MAP BASED FORMULATION

机译:火焰中的湍流-辐射相互作用:基于混沌映射的公式

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In this paper we report initial efforts in developing large-eddy simulation (LES) subgrid-scale (SGS) models capable of treating turbulence-radiation interactions in sufficient detail to permit calculation of radiation intensity fluctuations on small scales. These models are constructed with a fluctuating component consisting of a discrete dynamical system (chaotic map) and are thus completely deterministic. We present an outline of the development of this formulation and then employ experimental data to generate large-scale behavior permitting what might be viewed as part of an a priori test of the SGS model. We display spatially extensive instantaneous fluctuating temperatures produced by the model as well as time series of fluctuating intensity calculated from the radiative transfer equation at several heights in a pool fire. We conclude that such results are physically realistic (and very efficiently computed) and warrant continued investigations, but we have at this time not yet completely validated the approach due to lack of detailed laboratory data.
机译:在本文中,我们报告了开发大型涡流模拟(LES)子网格规模(SGS)模型的初步努力,该模型能够足够详细地处理湍流-辐射相互作用,以允许在小尺度上计算辐射强度波动。这些模型由包含离散动态系统(混沌图)的波动分量构成,因此具有完全确定性。我们提出了该配方的发展概况,然后利用实验数据来生成大规模行为,从而允许将其视为SGS模型的先验测试的一部分。我们显示了由模型产生的空间广泛的瞬时波动温度,以及根据池火中几个高度处的辐射传递方程计算的波动强度的时间序列。我们得出的结论是,这样的结果在物理上是现实的(并且可以非常有效地计算出)并且需要继续进行研究,但是由于缺乏详细的实验室数据,我们目前尚未完全验证该方法。

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