The spectra of the daytime sky of Venus were recorded on the Venera-11 and Venera-12 descent vehicles at various altitudes above the planet's surface, within the interval of 4500 to 12,000 Angstroms. The angular distribution of the brightness of the scattered radiation was recorded and the ratio of water and carbon dioxide were studied, with respect to the cloud cover boundaries
International audienceIn 1985 the VEGA 1 and VEGA 2 spacecraft dropped two descent probes into the n...
The spectrum of the dayglow of Venus between 1250 and 1430 A was measured in high resolution with th...
Ground-based near-infrared observations of the Venus night side reveal anomalous bright features at ...
The infrared spectrum of Venus in the spectral range 1.6 to 2.8 was measured by means of the spectro...
The thermal emission of Venus was recorded during the winter of 1970-1971, and in 1973 using the 2.7...
The profiles of upward, downward and net solar flux on Venus were measured at altitudes from about 6...
Experimental measurements by ultraviolet photometers aboard Venera-9 and -10 are presented, discusse...
The characteristics of the field of radiation in the near surface layer of the atmosphere and on the...
Aerosol concentration profiles were measured by an aerosol spectrometer above the landing sites of t...
Theoretical and investigation calculations of Venus brightness temperature, and radio emission pecul...
The Pioneer Venus Orbiter Infrared Radiometer and Venera 15 Fourier Transform Spectrometer observati...
Spatially-resolved near-infrared spectra from the Visible and Infrared Thermal Imaging Spectrometer ...
The instrumentation is analyzed for determining the composition of the clouds on Venus. Direct analy...
Mass spectrometer experiments installed on the descent vehicles of the Venera-11 and the Venera-12 a...
Results of the preliminary processing of the Vega 1 and 2 descender data on the cloud layer structur...
International audienceIn 1985 the VEGA 1 and VEGA 2 spacecraft dropped two descent probes into the n...
The spectrum of the dayglow of Venus between 1250 and 1430 A was measured in high resolution with th...
Ground-based near-infrared observations of the Venus night side reveal anomalous bright features at ...
The infrared spectrum of Venus in the spectral range 1.6 to 2.8 was measured by means of the spectro...
The thermal emission of Venus was recorded during the winter of 1970-1971, and in 1973 using the 2.7...
The profiles of upward, downward and net solar flux on Venus were measured at altitudes from about 6...
Experimental measurements by ultraviolet photometers aboard Venera-9 and -10 are presented, discusse...
The characteristics of the field of radiation in the near surface layer of the atmosphere and on the...
Aerosol concentration profiles were measured by an aerosol spectrometer above the landing sites of t...
Theoretical and investigation calculations of Venus brightness temperature, and radio emission pecul...
The Pioneer Venus Orbiter Infrared Radiometer and Venera 15 Fourier Transform Spectrometer observati...
Spatially-resolved near-infrared spectra from the Visible and Infrared Thermal Imaging Spectrometer ...
The instrumentation is analyzed for determining the composition of the clouds on Venus. Direct analy...
Mass spectrometer experiments installed on the descent vehicles of the Venera-11 and the Venera-12 a...
Results of the preliminary processing of the Vega 1 and 2 descender data on the cloud layer structur...
International audienceIn 1985 the VEGA 1 and VEGA 2 spacecraft dropped two descent probes into the n...
The spectrum of the dayglow of Venus between 1250 and 1430 A was measured in high resolution with th...
Ground-based near-infrared observations of the Venus night side reveal anomalous bright features at ...