Abstract

Recently, the cumulative wavenumber method was formulated and its viability demonstrated for the prediction of radiative heat transfer in high temperature CO 2 and H 2O. This paper presents enhancements to the cumulative wavenumber method, formalizing a mathematical definition for the cumulative wavenumber distribution function, introducing the joint cumulative wavenumber for gas mixtures, extending the method to non-homogenous, non-isothermal media, and demonstrating its application to gas mixtures with non-gray particles. The methodology for applying the cumulative wavenumber method to mixtures is explored using several different theoretical approaches. Model predictions are compared with line-by-line benchmark integration of the RTE. Finally, the relationship between the cumulative wavenumber and previously proposed spectral distribution functions is summarized.

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