Three‐Dimensional Turbulence‐Resolving Modeling of the Venusian Cloud Layer and Induced Gravity Waves: Inclusion of Complete Radiative Transfer and Wind Shear

Venus' convective cloud layers and associated gravity waves strongly impact the local and global budget of heat, momentum, and chemical species. Here we use for the first time three‐dimensional turbulence‐resolving dynamical integrations of Venus' atmosphere from the surface to 100‐km alti...

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Veröffentlicht in:	Journal of geophysical research. Planets 2018-10, Vol.123 (10), p.2773-2789
Hauptverfasser:	Lefèvre, M., Lebonnois, S., Spiga, A.
Format:	Artikel
Sprache:	eng
Schlagworte:	Altitude Astrophysics Atmosphere Atmospheric models Balloons Chemical speciation Clouds Computer simulation Convection Convective activity Diurnal cycle Diurnal variations Equator Geophysics Gravitational waves Gravity waves Latitude modeling Momentum Organic chemistry Physics Radiative forcing Radiative transfer Turbulence Venus Venus atmosphere Venus clouds Venus Express (ESA) Venus surface Vertical orientation Vertical wind shear Wind Wind shear
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