Pressure-induced absorption coefficients for radiative transfer calculations in Titan's atmosphere
作者： Régis Courtin
DOI: 10.1016/0019-1035(88)90004-8
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摘要: The semiempirical theory of Birnbaum and Cohen (1976) is used to calculate the FIR pressure-induced absorption (PIA) spectra N2, CH4, N2 + Ar, H2 under conditions like those in Titan troposphere. results are presented graphically compared with published data from laboratory measurements PIA same gases mixtures (Dagg et al., 1986; Dore 1986). Good agreement obtained, only a slight underestimation at 300-400/cm case CH4. coefficients tables, it suggested that present findings value for evaluating effects tropospheric clouds on spectrum studying greenhouse effect near surface. 24 references.
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