The physical and chemical properties of the clouds of Venus are reviewed, with special emphasis on data that are related to cloud dynamics. None of the currently-popular interpretations of cloud phenomena on Venus is consistent with all the data. Either a considerable fraction of the observational evidence is faulty or has been misinterpreted, or the clouds of Venus are much more complex than the current simplistic models. Several lines of attack are suggested to resolve some of the contradictions. A sound understanding of the clouds appears to be several years in the future
The instrumentation is analyzed for determining the composition of the clouds on Venus. Direct analy...
Clouds on Venus are formed of sulfuric acid aerosols. The clouds are optically very thick in the vis...
International audienceWe present here three-dimensional simulations of the Venus photochemistry and ...
The spectral and polarization data for Venus are consistent with micron-sized, aerosol cloud particl...
The planet Venus is the closest to the planet Earth both geographically and geometrically, with an a...
The two defining characteristics of the planet Venus are its atmospheric super-rotation and the plan...
International audienceVenus is completely enveloped by clouds. The main cloud layers stretch from al...
A condensing cloud parameterization is included in a super-rotating Venus General Circulation Model....
We report on the implications of the observations of the glory phenomenon made recently by Venus Exp...
Determination of ice clouds and water vapor in Venus atmosphere from balloon observation
Spatially-resolved near-infrared spectra from the Visible and Infrared Thermal Imaging Spectrometer ...
Venus’ atmosphere has a rich chemistry involving interactions among sulfur, chlorine, nitrogen, hyd...
Venus’ appearance is deceptive. The history of scientific research about Venus is full of mistaken a...
More than three decades have passed since the publication of the last review of the Venus clouds and...
The instrumentation is analyzed for determining the composition of the clouds on Venus. Direct analy...
Clouds on Venus are formed of sulfuric acid aerosols. The clouds are optically very thick in the vis...
International audienceWe present here three-dimensional simulations of the Venus photochemistry and ...
The spectral and polarization data for Venus are consistent with micron-sized, aerosol cloud particl...
The planet Venus is the closest to the planet Earth both geographically and geometrically, with an a...
The two defining characteristics of the planet Venus are its atmospheric super-rotation and the plan...
International audienceVenus is completely enveloped by clouds. The main cloud layers stretch from al...
A condensing cloud parameterization is included in a super-rotating Venus General Circulation Model....
We report on the implications of the observations of the glory phenomenon made recently by Venus Exp...
Determination of ice clouds and water vapor in Venus atmosphere from balloon observation
Spatially-resolved near-infrared spectra from the Visible and Infrared Thermal Imaging Spectrometer ...
Venus’ atmosphere has a rich chemistry involving interactions among sulfur, chlorine, nitrogen, hyd...
Venus’ appearance is deceptive. The history of scientific research about Venus is full of mistaken a...
More than three decades have passed since the publication of the last review of the Venus clouds and...
The instrumentation is analyzed for determining the composition of the clouds on Venus. Direct analy...
Clouds on Venus are formed of sulfuric acid aerosols. The clouds are optically very thick in the vis...
International audienceWe present here three-dimensional simulations of the Venus photochemistry and ...