Greenhouse models of Venus' High surface temperature, as constrained by Pioneer Venus measurements
- 30 December 1980
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 85 (A13) , 8223-8231
- https://doi.org/10.1029/ja085ia13p08223
Abstract
No abstract availableKeywords
This publication has 33 references indexed in Scilit:
- Composition of the Venus lower atmosphere from the Pioneer Venus Mass SpectrometerJournal of Geophysical Research, 1980
- Further Results of the Pioneer Venus Nephelometer ExperimentScience, 1979
- First Results from the Large Probe Infrared Radiometer ExperimentScience, 1979
- Further Numerical Calculations of the Circulation of the Atmosphere of VenusJournal of the Atmospheric Sciences, 1975
- Venera 8: Measurements of Solar Illumination Through the Atmosphere of Venus 1Journal of the Atmospheric Sciences, 1973
- Water vapor in the atmosphere of VenusIcarus, 1972
- Far-Infrared Collision-Induced Absorption in CO2. I. Temperature DependenceThe Journal of Chemical Physics, 1971
- Infrared transmission properties of CO, HCI, and SO2 and their significance for the greenhouse effect on VenusIcarus, 1969
- A Discussion of the Deep Circulation of the Atmosphere of VenusThe Astrophysical Journal, 1966
- A model for computing infrared transmission through atmospheric water vapor and carbon dioxideJournal of Geophysical Research, 1964