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.
W., Min M., 2019, @doi [ ] 10.1051/0004-6361/201833678 , http://adsabs.harvard.edu/abs/2019A
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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.