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Figure 4. Comparison of the theoretical estimations based on the current (solid line) and the previous (Courtin 1988) (dashed line) models. The absorption spectra are shown at temperatures of 70°, 120°, and 170°K and frequencies up to 600 cm-1.
Régis Courtin, Pressure-induced absorption coefficients for radiative transfer calculations in Titan's atmosphere, Icarus, Volume 75, Issue 2, August 1988, Pages 245-254, https://doi.org/10.1016/0019-1035(88)90004-8



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