Article ID Journal Published Year Pages File Type
8143568 Planetary and Space Science 2014 8 Pages PDF
Abstract
Venus׳ atmosphere consists of about 95% of carbon dioxide, which accounts for most of the absorption of the radiation emitted by its hot surface. The large densities and high temperatures of Venus׳ atmosphere make the absorption much more complex than for low density atmospheres such as Earth or Mars. Available experimental data are at present insufficient and theoretical models inadequate to describe complex absorption line shapes and collision-induced phenomena. Here we present a survey of all absorption and scattering processes which influence the transparency of Venus׳ atmosphere for what concerns carbon dioxide.
Related Topics
Physical Sciences and Engineering Earth and Planetary Sciences Geophysics
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