Gravity wave momentum fluxes of 10-30 m² s⁻² and drag of 0.003-0.03 m s⁻² were estimated from Akatsuki radio occultation temperature data across 40-95 km altitudes on Venus.
Journal of Atmospheric Sciences , year = 1996, month = jul, volume =
3 Pith papers cite this work. Polarity classification is still indexing.
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MELTYQ couples magma-atmosphere equilibrium models with spectral retrievals to constrain sub-Neptune magma oxidation states and volatile inventories from transmission spectra.
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.
citing papers explorer
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Variation of Venusian Gravity Wave Absolute Momentum Fluxes and Drag as Retrieved from the Akatsuki Mission
Gravity wave momentum fluxes of 10-30 m² s⁻² and drag of 0.003-0.03 m s⁻² were estimated from Akatsuki radio occultation temperature data across 40-95 km altitudes on Venus.
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Coupling magma-ocean and atmospheres in spectral retrievals of sub-Neptunes
MELTYQ couples magma-atmosphere equilibrium models with spectral retrievals to constrain sub-Neptune magma oxidation states and volatile inventories from transmission spectra.
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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.