Martin K. Denison
Brent W. Webb
ABSTRACT The previously published mathematical correlations of the absorption-line blackbody distribution function, central to the spectral-line based weighted-sum-of-gray-gases model (SLW), have been extended to elevated pressures by introducing a dependence on an effective broadening pressure. Comparisons between experimentally determined total emissivities and those calculated with the model show good agreement. Good agreement at elevated pressure between line-by-line benchmarks, and model predictions is also demonstrated.
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