The IR absorption of the pure CO2 gas in the region of 15 mum was examined.
A special attention was given to the line mixing effect that influences th
e spectral shape of the vibration-rotation absorption bands in the Q-branch
regions. Two methods in shape description were analyzed. The first method
uses the Rosenkranz line shapes with the line mixing parameters, which are
found from an empirical rotational relaxation matrix. The second method is
based on the strong collision model with adjusted branch coupling (ABC-mode
l). The merits and the demerits of these two methods are discussed, and the
results of the corresponding calculations are compared to the measured sha
pes. It is inferred that the ABC-model for the absorption coefficient calcu
lations can be successfully applied for solving the non-LTE radiative trans
fer problem in CO2 bands in the atmospheres of Earth-like planets. (C) 2001
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