Results for 13-cm absorptivity and H2SO4 abundance profiles from the season 10 (1986) Pioneer Venus Orbiter radio occultation experiment

Icarus

Volumn 90, Issue 1, 1991, Pages 129-138

  Jenkins, Jon M ^a   Steffes, Paul G ^a  

^a GEORGIA INSTITUTE OF TECHNOLOGY   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0010964439     PISSN: 00191035     EISSN: 10902643     Source Type: Journal    
DOI: 10.1016/0019-1035(91)90075-5     Document Type: Article

References (14)

1. The Composition, Vertical Structure, and Global Variability of the Lower Cloud Deck on Venus as Determined by Radio Occultation Techniques
2. The radio occultation method for the study of planetary atmospheres
3. Comment on absorbing regions in the atmosphere of Venus as measured by radio occultations
4. [Pleuropericarditis and Pyoderma gangrenosum during remission of a hemorrhagic rectocolitis].
5. The neutral atmosphere of Venus as studied with the Mariner V radio occultation experiments
6. Composition and structure of the Venus atmosphere: Results from Pioneer Venus
7. Statistical and computational uncertainties in atmospheric profiles from radio occultation: Mariner 10 at Venus
8. Measurements of thermal structure and thermal contrasts in the atmosphere of Venus and related dynamical observations Results from the four Pioneer Venus probes
9. Laboratory measurements of the microwave opacity and vapor pressure of sulfuric acid under simulated conditions for the middle atmosphere of Venus
10. Evaluation of the microwave spectrum of Venus in the 12 to 22 centimeter wavelength range based on laboratory measurements of constituent gas opacities
11. Observations of the microwave emission of Venus from 1.3 to 3.6 cm.