Fig. 2

a) Incident radiative spectrum of M-dwarf Gliese 581 at the top of the atmosphere (black line) and on the surface of Gl 581d for the dry condition with Ps = 5 bar (CO2 condensation is not taken into account). The red and blue lines indicate surface incident radiative spectra with and without Rayleigh scattering, respectively. b) Red line: percentage of incident radiation absorbed by CO2 as a function of Ps, and blue line: percentage of incident radiation absorbed and scattered by CO2.
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