Measurements and semi-empirical calculations of CO2 + CH4 and CO2 + H2 collision-induced absorption across a wide range of wavelengths and temperatures. Application for the prediction of early Mars surface temperature
Author:
Funder
Horizon 2020
Swiss National Science Foundation
Publisher
Elsevier BV
Subject
Space and Planetary Science,Astronomy and Astrophysics
Reference32 articles.
1. Testing the early Mars H2-CO2 greenhouse hypothesis with a 1-D photochemical model;Batalha;Icarus,2015
2. Early Mars serpentinization-derived CH4 reservoirs, H2-induced warming and paleopressure evolution;Chassefière;Meteorit. Planet. Sci.,2016
3. 3D modelling of the early martian climate under a denser CO2 atmosphere: temperatures and CO2 ice clouds;Forget;Icarus,2013
4. Collision-induced absorption of CH4-CO2 and H2-CO2 complexes and their effect on the ancient Martian atmosphere;Godin;ESSOAr,2019
5. The early Mars climate system;Haberle,2017
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