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A Hybrid Solution Methodology for Efficient Solving of Radiative Heat Transfer in Non Gray Medium using WSSG Model

机译:使用WSSG模型有效解决非灰介质中辐射传热的混合求解方法

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The weighted sum of gray gases (WSGG) method has been used extensively for radiation modeling of non gray medium gases. The radiative transfer equation (RTE) for each gray gas can be solved using the Discrete Ordinate (DO) model, which is sufficiently accurate over wide range of optical thickness, but it is computationally expensive. The P1 approximation is an efficient alternative to solve the RTE, but applicable to optically thick medium only. In the present work, a hybrid solution methodology to solve RTE in a non gray medium using WSGG model is proposed. Results for the case of four gray gases are presented. The philosophy is to achieve the optimum performance using combination of the P1 and DO model with respect to the optical thickness of the gray gases being solved with minimal loss in accuracy. In this approach, the transparent and/or optically thin gases are solved using the DO model while the P1 approximation is used for the optically thick gases. This combination reduces the total number of radiation intensity equation to be solved very significantly. A study of accuracy and computational cost for the hybrid solution methodology has been done for a variety of test cases in order of increasing complexity. It has been found that the hybrid solution methodology, in which RTE for two gray gases are solved by DO model and the remaining two gray gases by P1 approximation, provided similar accuracy with significant speedup compared to the conventional approach in which RTE for all gray gases are solved with DO model. Another variant of the hybrid approach, in which DO model is used only for the transparent gas, is also considered and found to be sufficiently accurate for most of the cases.
机译:灰色气体的加权总和(WSGG)方法已广泛用于非灰色介质气体的辐射建模。可以使用离散纵坐标(DO)模型求解每种灰气体的辐射传递方程(RTE),该模型在较宽的光学厚度范围内都足够精确,但计算量大。 P1近似值是解决RTE的有效替代方法,但仅适用于光学较厚的介质。在目前的工作中,提出了一种使用WSGG模型在非灰色介质中求解RTE的混合解决方案方法。给出了四种灰色气体的结果。该理念是通过结合使用P1和DO模型来实现最佳性能,以解决灰气体的光学厚度问题,并且精度损失最小。在这种方法中,透明和/或光学上稀薄的气体使用DO模型求解,而P1近似值用于光学上较厚的气体。这种组合大大减少了要解决的辐射强度方程式的总数。为了提高复杂性,已经针对各种测试案例对混合解决方案方法的准确性和计算成本进行了研究。已经发现,与传统方法(其中所有灰分气体的RTE均采用常规方法)相比,该混合解决方案方法通过DO模型求解两种灰分气体的RTE,并通过P1近似求解剩余的两种灰分气体,可提供相似的精度和显着的加速效果。用DO模型解决。还考虑了混合方法的另一种变体,其中DO模型仅用于透明气体,并且在大多数情况下已足够精确。

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