Impact of uncertainties in CO2, HCl, and H2O cross sections on simulations of Venus mesospheric chemistry

EGU General Assembly Conference Abstracts 2026 Open access

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Authors: Franklin P. Mills
DOI: 10.5194/egusphere-egu26-4927
Cited by: 0

Abstract

The atmospheres of Venus and Mars are primarily CO2 which photolyses at wavelengths ∼

Fields of Study & Subjects

Planetary Science and Exploration Astro and Planetary Science Atmospheric Ozone and Climate

Publication details

Journal / source
EGU General Assembly Conference Abstracts
Publication date
13 March 2026
Language
EN