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

Author:

Ozak N.12ORCID,Aharonson O.1ORCID,Halevy I.1ORCID

Affiliation:

1. Department of Earth and Planetary Sciences; Weizmann Institute of Science; Rehovot Israel

2. Now at Centre for Mathematical Plasma-Astrophysics; KU Leuven; Leuven Belgium

Publisher

American Geophysical Union (AGU)

Subject

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

Reference7 articles.

1. High pressure Cavity Ring Down spectroscopy: Application to the absorption continuum of CO2 near 1.7 μm;Kassi;Journal of Quantitative Spectroscopy and Radiative Transfer,2015

2. Updated database plus software for line-mixing in CO2 infrared spectra and their test using laboratory spectra in the 1.5-2.3 μm region;Lamouroux;Journal of Quantitative Spectroscopy and Radiative Transfer,2010

3. Spectra calculations in central and wing regions of CO2 IR bands. IV: Software and database for the computation of atmospheric spectra;Niro;Journal of Quantitative Spectroscopy and Radiative Transfer,2005

4. Radiative transfer in CO2-rich atmospheres: 1. Collisional line mixing implies a colder early Mars;Ozak;Journal of Geophysical Research: Planets,2016

5. Temperature-dependent measurements and modeling of absorption by CO2-N2 mixtures in the far line-wings of the 4.3 μm CO2 band;Perrin;Journal of Quantitative Spectroscopy and Radiative Transfer,1989

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