The Lower Atmosphere of Venus After Vega 1 and 2 Missions
Abstract
We have computed the physical parameters for the Venus atmosphere between 0 64 km altitude by using Vega measurements. The proposed model can be used in order to study the structure of Venus atmosphere and its chemical comoposition between 60 64 km, where an inversion in temperature profiles has been measured by Vega.
- Publication:
-
Earth Moon and Planets
- Pub Date:
- October 1988
- DOI:
- 10.1007/BF00056477
- Bibcode:
- 1988EM&P...43...45P
- Keywords:
-
- Atmospheric Composition;
- Atmospheric Density;
- Atmospheric Pressure;
- Lower Atmosphere;
- Venus Atmosphere;
- Atmospheric Physics;
- Atmospheric Temperature;
- Temperature Distribution;
- Temperature Inversions;
- Vega Project;
- Lunar and Planetary Exploration