From a critical comparison and synthesis of data from the four Pioneer Venus Probes, the Pioneer Venus Orbiter, and the Venera 10, 12, and 13 landers, models of the lower and middle atmosphere of Venus are derived. The models are consistent with the data sets within the measurement uncertainties and established variability of the atmosphere. The models represent the observed variations of state properties with latitude, and preserve the observed static stability. The rationale and the approach used to derive the models are discussed, and the remaining uncertainties are estimated.
Models of the structure of the atmosphere of Venus from the surface to 100 kilometers altitude
Advances in Space Research ; 5 , 11, 1
1985-01-01
Miscellaneous
No indication
English
Skane from an Altitude of 900 Kilometers
NTIS | 1973
|LOW-ALTITUDE EXPLORATION OF THE VENUS ATMOSPHERE BY BALLOON
British Library Conference Proceedings | 2010
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