The effect of 3D transport-induced disequilibrium carbon chemistry on the atmospheric structure, phase curves, and emission spectra of hot Jupiter HD 189733b
On hot Jupiter exoplanets, strong horizontal and vertical winds should homogenize the abundances of the important absorbers CH4 and CO much faster than chemical reactions restore chemical equilibrium. This effect, typically neglected in general circulation models (GCMs), has been suggested to explai...
| Κύριοι συγγραφείς: | , , , , |
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| Μορφή: | Journal article |
| Γλώσσα: | English |
| Έκδοση: |
IOP Publishing
2019
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