Comment on “Radiative Transfer in CO2 -Rich Atmospheres: 1. Collisional Line Mixing Implies a Colder Early Mars”-Reference-Cited by-同舟云学术

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

Published:2017-11 Issue:11 Volume:122 Page:2362-2365
ISSN:2169-9097
Container-title:Journal of Geophysical Research: Planets
language:en
Short-container-title:J. Geophys. Res. Planets

Author:

Turbet M.¹,Tran H.¹

Affiliation:

1. Laboratoire de Météorologie Dynamique, IPSL, UPMC Université Paris 06, Ecole Polytechnique, Ecole Normale Supérieure, Sorbonne Universités, Université Paris-Saclay, PSL Research University, CNRS; Paris France

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Geochemistry and Petrology,Geophysics

Link

http://onlinelibrary.wiley.com/wol1/doi/10.1002/2017JE005373/fullpdf

Reference17 articles.

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2. 3D modelling of the early Martian climate under a denser CO2 atmosphere: Temperatures and CO2 ice clouds;Forget;Icarus,2013

3. Roto-translational collision-induced absorption of CO2 for the atmosphere of Venus at frequencies from 0 to 250 cm−1, at temperatures from 200 to 800 K;Gruszka;Icarus,1997

4. Haberle R. Clancy , R. Forget , F. Smith , M. Zurek , R. 2017 The Atmosphere and Climate of Mars https://www.cambridge.org/core/books/atmosphere-and-climate-of-mars/cambridge-planetary-science/3949809C23D0F91CF91C3D1B95E39374

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