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.
An inherently mass-conserving semi-implicit semi-lagrangian discretiza- tion of the deep-atmosphere global non-hydrostatic equa- tions,
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WASP-96b shows super-solar metallicity of 2-6x stellar, roughly stellar C/O, tentative SO2 consistent with photochemistry, and an optical slope from scattering aerosols, supporting core-accretion formation beyond the water snowline.
3D radiative-hydrodynamical simulations of HD 209458b with parameterized phase-equilibrium clouds and radiative feedback show altered thermal structure, sensitivity to f_sed and deep T-P profile, and improved matches to observations.
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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.
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Super-Solar Metallicity and Tentative Evidence for Photochemistry on WASP-96b from JWST and Ground-Based VLT Transmission Spectroscopy
WASP-96b shows super-solar metallicity of 2-6x stellar, roughly stellar C/O, tentative SO2 consistent with photochemistry, and an optical slope from scattering aerosols, supporting core-accretion formation beyond the water snowline.
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Overcast on Osiris: 3D radiative-hydrodynamical simulations of a cloudy hot Jupiter using the parameterised, phase-equilibrium cloud formation code EddySed
3D radiative-hydrodynamical simulations of HD 209458b with parameterized phase-equilibrium clouds and radiative feedback show altered thermal structure, sensitivity to f_sed and deep T-P profile, and improved matches to observations.