Abstract
Transport coefficients of equilibrium Martian atmosphere have been calculated in the second non-vanishing Chapman-Enskog approximation and compared with existing literature results. The present work improves previous calculations by considering a very detailed chemistry model of Martian atmosphere that includes 53 species and by extending the temperature range up to 50 000 K.
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Catalfamo, C., Bruno, D., Colonna, G. et al. High temperature Mars atmosphere. Part II: transport properties. Eur. Phys. J. D 54, 613–621 (2009). https://doi.org/10.1140/epjd/e2009-00193-6
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DOI: https://doi.org/10.1140/epjd/e2009-00193-6