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Inhomogeneous models of the Venus clouds containing sulfur

Authors :
Smith, S. M
Pollack, J. B
Giver, L. P
Cuzzi, J. N
Podolak, M
Publication Year :
1979
Publisher :
United States: NASA Center for Aerospace Information (CASI), 1979.

Abstract

Based on the suggestion that elemental sulfur is responsible for the yellow color of Venus, calculations are compared at 3.4 microns of the reflectivity phase function of two sulfur containing inhomogeneous cloud models with that of a homogeneous model. Assuming reflectivity observations with 25% or less total error, comparison of the model calculations leads to a minimum detectable mass of sulfur equal to 7% of the mass of sulfuric acid for the inhomogeneous drop model. For the inhomogeneous cloud model the comparison leads to a minimum detectable mass of sulfur between 17% and 38% of the mass of the acid drops, depending upon the actual size of the large particles. It is concluded that moderately accurate 3.4 microns reflectivity observations are capable of detecting quite small amounts of elemental sulfur at the top of the Venus clouds.

Subjects

Subjects :
Lunar And Planetary Exploration

Details

Language :
English
Database :
NASA Technical Reports
Notes :
RTOP 195-21-01-01
Publication Type :
Report
Accession number :
edsnas.19790014817
Document Type :
Report