The effect of 3D transport-induced disequilibrium carbon chemistry on the atmospheric structure, phase curves, and emission spectra of hot Jupiter HD 189733b

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...

Detaylı Bibliyografya
Asıl Yazarlar:	Steinrueck, ME, Parmentier, V, Showman, AP, Lothringer, JD, Lupu, RE
Materyal Türü:	Journal article
Dil:	English
Baskı/Yayın Bilgisi:	IOP Publishing 2019

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