Transmission spectrum of WASP-94A b reveals morning limb cooler and cloudy versus evening limb hotter with H2O features, interpreted as cloud droplets forming on morning side and evaporating on evening side.
Photochemical Hazes Dramatically Alter Temperature Structure and Atmospheric Circulation in 3D Simulations of Hot Jupiters,
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Cloudy mornings and clear evenings on a gas giant exoplanet
Transmission spectrum of WASP-94A b reveals morning limb cooler and cloudy versus evening limb hotter with H2O features, interpreted as cloud droplets forming on morning side and evaporating on evening side.