Air mixture radiative property modelling in the temperature range 10,000-40,000 K.

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Radiative Transfer: Plasma

Scientific paper

A model based on the distribution functions of the absorption coefficients is used to describe the radiative properties of an air plasma at atmospheric pressure between 10,000 and 40,000 K. In order to account for spectral fine structure effects on radiative transfer in nonuniform media, fictitious species whose spectra reasonably satisfy the scaling approximation are introduced. The absorption spectra of these fictitious species are assumed to be spectrally uncorrelated. Radiative properties are described in terms of absorption coefficients and the model can be used with arbitrary radiative transfer equation solvers. Model parameters are generated from spectral high resolution calculations. The different approximations required to implement the model are discussed and their validity is checked by comparisons with line-by-line benchmarks. It is shown that the model can predict radiative transfer along strongly nonisothermal columns within a few percent.

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