Add to ORKGThe microwave absorbing properties of gaseous sulfuric acid (H2SO4) under Venus atmospheric conditions are investigated. The results are applied to measurements from Mariner 5, Mariner 10, and Pioneer/Venus Radio Occultation experiments, to determine abundancies of gaseous sulfuric acid in the Venus atmosphere. The microwave properties of the vapors accompanying liquid H2SO4 are studied to estimate the vapor pressure in an atmospheric model
Radio occultation experiments, and radio astronomical observations have suggested that significant v...
The Venus Express radio science experiment VeRa provided more than 900 neutral atmospheric profiles ...
The opportunity to determine the planetwide temperature and cloud structure of Venus using radio occ...
Radio absorptivity data for the Venus middle atmosphere (1 to 6 atm, temperatures from 500 to 575K) ...
Radio absorptivity data for planetary atmospheres obtained from spacecraft radio occultation experim...
High-accuracy laboratory measurements of the temperature dependence of the opacity from gaseous sulf...
Quite often the interpretive work on the microwave and millimeter-wave absorption profiles, which ar...
Recent observations of the millimeter-wave emission from Venus at 112 GHz (2.6 mm) have shown signif...
Accurate data on microwave and millimeter-wave properties of potential planetary atmospheric constit...
The Venus Express (VEX) Radio Science experiment VeRa utilizes radio occultation techniques to inves...
Radio absorptivity data for planetary atmospheres obtained from spacecraft radio occultation experim...
Brightness temperature spectra of Venus computed to determine amount of water vapor in lower atmosph...
As observations and models of the planets become increasingly more accurate and sophisticated, the n...
The effects of the Venus atmospheric constituents on its millimeter wavelength emission are investig...
In order to characterize possible variations in the abundance and distribution of subcloud sulfuric ...
Radio occultation experiments, and radio astronomical observations have suggested that significant v...
The Venus Express radio science experiment VeRa provided more than 900 neutral atmospheric profiles ...
The opportunity to determine the planetwide temperature and cloud structure of Venus using radio occ...
Radio absorptivity data for the Venus middle atmosphere (1 to 6 atm, temperatures from 500 to 575K) ...
Radio absorptivity data for planetary atmospheres obtained from spacecraft radio occultation experim...
High-accuracy laboratory measurements of the temperature dependence of the opacity from gaseous sulf...
Quite often the interpretive work on the microwave and millimeter-wave absorption profiles, which ar...
Recent observations of the millimeter-wave emission from Venus at 112 GHz (2.6 mm) have shown signif...
Accurate data on microwave and millimeter-wave properties of potential planetary atmospheric constit...
The Venus Express (VEX) Radio Science experiment VeRa utilizes radio occultation techniques to inves...
Radio absorptivity data for planetary atmospheres obtained from spacecraft radio occultation experim...
Brightness temperature spectra of Venus computed to determine amount of water vapor in lower atmosph...
As observations and models of the planets become increasingly more accurate and sophisticated, the n...
The effects of the Venus atmospheric constituents on its millimeter wavelength emission are investig...
In order to characterize possible variations in the abundance and distribution of subcloud sulfuric ...
Radio occultation experiments, and radio astronomical observations have suggested that significant v...
The Venus Express radio science experiment VeRa provided more than 900 neutral atmospheric profiles ...
The opportunity to determine the planetwide temperature and cloud structure of Venus using radio occ...