Computer Science – Numerical Analysis
Scientific paper
Jun 1975
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975jats...32.1025p&link_type=abstract
(NASA, State University of New York, AAS, and AGU, Conference on the Atmosphere of Venus, NASA Goddard Institute for Space Studi
Computer Science
Numerical Analysis
12
Astronomical Models, Atmospheric Circulation, Radiative Heat Transfer, Solar Heating, Venus Atmosphere, Cloud Cover, Greenhouse Effect, Infrared Radiation, Numerical Analysis, Thermal Absorption, Venus Clouds
Scientific paper
Results are reported for accurate multiple-scattering calculations to determine the solar-energy deposition profile in the atmosphere of Venus. It is found that most of the absorbed energy is deposited in the main cloud-layer region, located at altitudes above 35 km, and that the ground receives approximately 3% of the energy absorbed in toto by Venus. Using these results, vertical temperature profiles are computed under conditions of pure radiative equilibrium and radiative-convective equilibrium. Since the latter results satisfactorily match the temperature structure determined from various spacecraft observations, it is inferred that the greenhouse effect can account for the high surface temperature. Aerosols make an important contribution to the infrared opacity in these calculations. Preliminary three-dimensional calculations of the general circulation of the atmosphere are discussed which incorporate the results of the radiative calculations.
Pollack James B.
Young Robert
No associations
LandOfFree
Calculations of the radiative and dynamical state of the Venus atmosphere does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Calculations of the radiative and dynamical state of the Venus atmosphere, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Calculations of the radiative and dynamical state of the Venus atmosphere will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-750352