Add to ORKGThe profiles of upward, downward and net solar flux on Venus were measured at altitudes from about 62 km to the surface in three spectral bands at a vertical resolution of a few hundred meters. These data measured the penetration and absorption of solar energy in Venus' lower atmosphere quantities that are essential in evaluating the role of the greenhouse mechanism in supporting Venus' remarkably high surface temperature. In addition, the data constrained the vertical structure and optical properties of the Venus clouds
Our knowledge of the upper atmosphere and ionosphere of Venus and its interaction with the solar win...
The two defining characteristics of the planet Venus are its atmospheric super-rotation and the plan...
peer reviewedWe present aeronomical observations collected using remote sensing instruments on boar...
Instruments flown on the Pioneer Venus orbiter and probes measured many of the properties of the atm...
Spatially-resolved near-infrared spectra from the Visible and Infrared Thermal Imaging Spectrometer ...
The thermal emission of Venus was recorded during the winter of 1970-1971, and in 1973 using the 2.7...
The spectra of the daytime sky of Venus were recorded on the Venera-11 and Venera-12 descent vehicle...
The characteristics of the field of radiation in the near surface layer of the atmosphere and on the...
A sophisticated radiative transfer model that considers absorption, emission, and multiple scatterin...
A 1 metre increment modelled pressure profile is used to study the troposphere of Venus from the sur...
From the discovery that Venus has an atmosphere during the 1761 transit by M. Lomonosov to the curre...
Mariner II radar and radiometric observations of Venus during 1962 conjunction - physical dat
Pioneer Venus observations of temperatures and radiative fluxes are examined in an attempt to unders...
We calculated the net thermal flux in the atmosphere of Venus from the surface to 100 km altitude. O...
Experimental measurements by ultraviolet photometers aboard Venera-9 and -10 are presented, discusse...
Our knowledge of the upper atmosphere and ionosphere of Venus and its interaction with the solar win...
The two defining characteristics of the planet Venus are its atmospheric super-rotation and the plan...
peer reviewedWe present aeronomical observations collected using remote sensing instruments on boar...
Instruments flown on the Pioneer Venus orbiter and probes measured many of the properties of the atm...
Spatially-resolved near-infrared spectra from the Visible and Infrared Thermal Imaging Spectrometer ...
The thermal emission of Venus was recorded during the winter of 1970-1971, and in 1973 using the 2.7...
The spectra of the daytime sky of Venus were recorded on the Venera-11 and Venera-12 descent vehicle...
The characteristics of the field of radiation in the near surface layer of the atmosphere and on the...
A sophisticated radiative transfer model that considers absorption, emission, and multiple scatterin...
A 1 metre increment modelled pressure profile is used to study the troposphere of Venus from the sur...
From the discovery that Venus has an atmosphere during the 1761 transit by M. Lomonosov to the curre...
Mariner II radar and radiometric observations of Venus during 1962 conjunction - physical dat
Pioneer Venus observations of temperatures and radiative fluxes are examined in an attempt to unders...
We calculated the net thermal flux in the atmosphere of Venus from the surface to 100 km altitude. O...
Experimental measurements by ultraviolet photometers aboard Venera-9 and -10 are presented, discusse...
Our knowledge of the upper atmosphere and ionosphere of Venus and its interaction with the solar win...
The two defining characteristics of the planet Venus are its atmospheric super-rotation and the plan...
peer reviewedWe present aeronomical observations collected using remote sensing instruments on boar...