Pioneer Venus observations of temperatures and radiative fluxes are examined in an attempt to understand the thermal balance of the lower atmosphere. If all observations are correct and the probe sites are typical of the planet, the second law of thermodynamics requires that the bulk of the lower atmosphere heating must come from a source other than direct sunlight or a thermally driven atmospheric circulation. Neither the so-called greenhouse models nor the mechanical heating models are consistent with this interpretation of the observations. One possible interpretation is that two out of the three probe sites are atypical of the planet. Additional lower atmosphere heat sources provide another possible interpretation. These include a plane...
This study investigates the global characteristics of the Venus lower atmosphere below the cloud lay...
The evolution of our solar system remains one of the most fascinating questions since ancient astron...
Current knowledge of the temperature structure of the atmosphere of Venus is briefly summarized. The...
Pioneer Venus observations of temperatures and radiative fluxes are examined in an attempt to unders...
Instruments flown on the Pioneer Venus orbiter and probes measured many of the properties of the atm...
A 1 metre increment modelled pressure profile is used to study the troposphere of Venus from the sur...
We calculated the net thermal flux in the atmosphere of Venus from the surface to 100 km altitude. O...
The profiles of upward, downward and net solar flux on Venus were measured at altitudes from about 6...
From the discovery that Venus has an atmosphere during the 1761 transit by M. Lomonosov to the curre...
A sophisticated radiative transfer model that considers absorption, emission, and multiple scatterin...
Venus has a complex and dynamic upper atmosphere. This has been observed many times by ground-based,...
This article investigates the greenhouse effect on Venus and ascertains whether it is wholly respons...
International audienceWe present here the thermal structure of the upper atmosphere of Venus predict...
The paper explains why the physics involved in atmospheric and sub-surface heat transfer appears to ...
ESA’s Venus Express Mission has monitored Venus since April 2006, and scientists worldwide have used...
This study investigates the global characteristics of the Venus lower atmosphere below the cloud lay...
The evolution of our solar system remains one of the most fascinating questions since ancient astron...
Current knowledge of the temperature structure of the atmosphere of Venus is briefly summarized. The...
Pioneer Venus observations of temperatures and radiative fluxes are examined in an attempt to unders...
Instruments flown on the Pioneer Venus orbiter and probes measured many of the properties of the atm...
A 1 metre increment modelled pressure profile is used to study the troposphere of Venus from the sur...
We calculated the net thermal flux in the atmosphere of Venus from the surface to 100 km altitude. O...
The profiles of upward, downward and net solar flux on Venus were measured at altitudes from about 6...
From the discovery that Venus has an atmosphere during the 1761 transit by M. Lomonosov to the curre...
A sophisticated radiative transfer model that considers absorption, emission, and multiple scatterin...
Venus has a complex and dynamic upper atmosphere. This has been observed many times by ground-based,...
This article investigates the greenhouse effect on Venus and ascertains whether it is wholly respons...
International audienceWe present here the thermal structure of the upper atmosphere of Venus predict...
The paper explains why the physics involved in atmospheric and sub-surface heat transfer appears to ...
ESA’s Venus Express Mission has monitored Venus since April 2006, and scientists worldwide have used...
This study investigates the global characteristics of the Venus lower atmosphere below the cloud lay...
The evolution of our solar system remains one of the most fascinating questions since ancient astron...
Current knowledge of the temperature structure of the atmosphere of Venus is briefly summarized. The...