Add to ORKGMass spectrometer experiments installed on the descent vehicles of the Venera-11 and the Venera-12 are described. Data on the chemical composition of the lower atmosphere of Venus is discussed with emphasis on the isotope state of the basic components (carbon, oxygen, nitrogen) and of the inert gases
An X-ray radiometeric experiment is described along with the results of measurements of the elementa...
Preliminary investigation of mass spectra of gaseous products of pyrolyzed Venusian cloud particles ...
We present a re-examination of mass spectral data obtained from the Pioneer Venus Large Probe Neutra...
The instrumentation is analyzed for determining the composition of the clouds on Venus. Direct analy...
International audienceThe composition of Venus' lower atmosphere, beneath the clouds, has been inves...
The design and use of mass spectrometers to measure and identify atmospheric gas compositions of pla...
Measurement of noble gas abundances on Venus remain a high priority for planetary science. These stu...
The composition the atmosphere of Venus results from the integration of many processes entering into...
International audienceWe review the progress in our understanding of the composition of the Venus at...
The spectra of the daytime sky of Venus were recorded on the Venera-11 and Venera-12 descent vehicle...
Venus is the closest and most similar planet to Earth in the whole solar system, yet, basic measurem...
International audienceThe composition the atmosphere of Venus results from the integration of many p...
The deuterium hydrogen abundance ratio in the Venus atmosphere was measured while the inlets to the ...
The exploration of Venus continues to be a top priority of planetary science. The Planetary Decadal ...
Venus’ atmosphere has a rich chemistry involving interactions among sulfur, chlorine, nitrogen, hyd...
An X-ray radiometeric experiment is described along with the results of measurements of the elementa...
Preliminary investigation of mass spectra of gaseous products of pyrolyzed Venusian cloud particles ...
We present a re-examination of mass spectral data obtained from the Pioneer Venus Large Probe Neutra...
The instrumentation is analyzed for determining the composition of the clouds on Venus. Direct analy...
International audienceThe composition of Venus' lower atmosphere, beneath the clouds, has been inves...
The design and use of mass spectrometers to measure and identify atmospheric gas compositions of pla...
Measurement of noble gas abundances on Venus remain a high priority for planetary science. These stu...
The composition the atmosphere of Venus results from the integration of many processes entering into...
International audienceWe review the progress in our understanding of the composition of the Venus at...
The spectra of the daytime sky of Venus were recorded on the Venera-11 and Venera-12 descent vehicle...
Venus is the closest and most similar planet to Earth in the whole solar system, yet, basic measurem...
International audienceThe composition the atmosphere of Venus results from the integration of many p...
The deuterium hydrogen abundance ratio in the Venus atmosphere was measured while the inlets to the ...
The exploration of Venus continues to be a top priority of planetary science. The Planetary Decadal ...
Venus’ atmosphere has a rich chemistry involving interactions among sulfur, chlorine, nitrogen, hyd...
An X-ray radiometeric experiment is described along with the results of measurements of the elementa...
Preliminary investigation of mass spectra of gaseous products of pyrolyzed Venusian cloud particles ...
We present a re-examination of mass spectral data obtained from the Pioneer Venus Large Probe Neutra...