Carbon dioxide opacity of the Venus׳ atmosphere

Author:

Snels Marcel,Stefani Stefania,Grassi Davide,Piccioni Giuseppe,Adriani AlbertoORCID

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference107 articles.

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2. A comparison of water vapor line parameters for modeling the Venus deep atmosphere;Bailey;Icarus,2009

3. Collision-induced absorption by CO2 in the region of ν1, 2ν2;Baranov;J. Mol. Spectrosc.,1999

4. Collision-induced absorption in the CO2 Fermi Triad for temperatures from 211 to 296K;Baranov,2002

5. On the origin of the band structure observed in the collision-induced absorption bands of CO2;Baranov;J. Mol. Spectrosc.,2003

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1. Ames-2021 CO2 Dipole Moment Surface and IR Line Lists: Toward 0.1% Uncertainty for CO2 IR Intensities;The Journal of Physical Chemistry A;2022-08-25

2. References;Collisional Effects on Molecular Spectra;2021

3. Line mixing and broadening of carbon dioxide by argon in the v3 bandhead near 4.2 µm at high temperatures and high pressures;Journal of Quantitative Spectroscopy and Radiative Transfer;2020-09

4. ExoMol line lists – XXXIX. Ro-vibrational molecular line list for CO2;Monthly Notices of the Royal Astronomical Society;2020-06-30

5. Multispectral surface emissivity from VIRTIS on Venus Express;Icarus;2020-01

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