Comment on "Radiative Transfer in CO₂-Rich Atmospheres: 1. Collisional Line Mixing Implies a Colder Early Mars"

M. Turbet (1) , H. Tran (1)

1 LMD - Laboratoire de Météorologie Dynamique (UMR 8539)

Ozak et al. (2016) claimed that explicitly including the effect of CO₂ collisional line mixing in their radiative transfer calculations yield CO₂ atmospheres that are more transparent to infrared radiation than when spectra calculations are made using sub-Lorentzian line shapes. This would in particular imply significantly colder surface temperatures (up to 15 K) for early Mars than estimated in previous studies. Here we show that the relative cooling that Ozak et al. (2016) associated to the effect of collisional line mixing is in fact due to a wrong choice of broadening species (air instead of CO₂). We then calculated line-by-line spectra of pure CO₂ atmospheres using a line-mixing model developed for self-broadened CO₂. Using the LMD Generic model (in 1-D radiative-convective mode), we find that calculations made with the proper collisional line mixing model and with sub-Lorentzian line shapes lead to differences between early Mars surface temperatures smaller than 2 K only.

Mots clés: planetary atmospheres; Mars; line mixing; CO<SUB>2</SUB>; radiative transfer; spectroscopy; Astrophysics - Earth and Planetary Astrophysics

Domaines: Planète et Univers [physics]

M. Turbet, H. Tran. Comment on "Radiative Transfer in CO₂-Rich Atmospheres: 1. Collisional Line Mixing Implies a Colder Early Mars". Journal of Geophysical Research. Planets, 2017, 122, pp.2362-2365. ⟨10.1002/2017JE005373⟩. ⟨insu-03727045⟩