Abstract
For the purpose of calculating the far-infrared thermal radiation from Titan's atmosphere, the pressure-induced absorption in pure N2, CH4 and in N2Ar, N2CH4, and N2H2 mixtures has been modeled using recent laboratory measurements. The results are tabulated as a function of wavenumber and temperature, and gaseous absorption spectra are calculated for the composition and temperatures known to be typical of the troposphere of Titan.
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