Dynamics, winds, circulation and turbulence in the atmosphere of Venus

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Atmospheric Circulation, Atmospheric Turbulence, Dynamic Models, Venus Atmosphere, Wind (Meteorology), Albedo, Convection Currents, Infrared Radiometers, Lower Atmosphere, Meridional Flow, Rossby Regimes, Turbulent Diffusion, Upper Atmosphere, Wind Velocity, Zonal Flow (Meteorology)

Scientific paper

With the possible exception of the lowest one or two scale heights, the dominant mode of circulation of Venus' atmosphere is a rapid, zonal, retrograde motion. Global albedo variations in the ultraviolet may reflect planetary scale waves propagating relative to the zonal winds. Other special phenomena such as cellular convection in the subsolar region and internal gravity waves generated in the interaction of the zonal circulation with the subsolar disturbance may also be revealed in ultraviolet imagery of the atmosphere. We discuss the contributions of experiments on the Orbiter and Entry Probes of Pioneer Venus toward unravelling the mystery of the planet's global circulation and the role played by waves, instabilities and convection therein

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