Sulfuric acid vapor and other cloud-related gases in the Venus atmosphere: Abundances inferred from observed radio opacity

Icarus

Volumn 51, Issue 2, 1982, Pages 322-333

  Steffes, Paul G ^a   Eshleman, Von R ^a  

^a STANFORD UNIVERSITY   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 27144493454     PISSN: 00191035     EISSN: 10902643     Source Type: Journal    
DOI: 10.1016/0019-1035(82)90087-2     Document Type: Article

References (20)

1. On the vapor pressure of sulfuric acid
2. Polar cloud structure as derived from the Pioneer Venus orbiter
3. The composition and vertical structure of the lower cloud deck on Venus
4. The neutral atmosphere of Venus as studied with the Mariner V radio occultation experiments
5. Vapor-liquid equilibria for aqueous sulfuric acid
6. Aerosol component of the atmosphere of Venus according to the results of spectrophotometric measurements aboard Venera-11 and -12 descent vehicles
7. Laboratory measurements of microwave absorption in models of the atmosphere of Venus
8. Constraints on the composition of the Venus atmosphere from microwave measurements near 1.35 cm wavelength
9. 2 in the Venus atmosphere
10. The microphysics of the clouds of Venus Results of the Pioneer Venus particle size spectrometer experiment
11. The microwave spectrum, structure, and dipole moment of sulfuric acid
12. Statistical and computational uncertainties in atmospheric profiles from radio occultation: Mariner 10 at Venus
13. A model of the Venus atmosphere from radio radar and occultation observations
14. Pioneer Venus gas chromatography of the lower atmosphere of Venus
15. The structure of the clouds of Venus Results of the Pioneer Venus nephelometer experiment
16. Cloud microphysics: Analysis of the clouds of Earth, Venus, Mars, and Jupiter
17. Sulfur dioxide and other cloud-related gases as the source of the microwave opacity of the middle atmosphere of Venus
18. Laboratory measurements of the microwave opacity of sulfur dioxide and other cloud-related gases under simulated conditions for the middle atmosphere of Venus
19. 2O over sulfuric acid solutions