An analysis of the Mariner 2 microwave observations of Venus.
Mariner 2 limb darkening measurements of Venus at microwave range, discussing peak brightness temperature and opacity models
Engineering topics
Publications and source records attributed to Sagan, C..
Mariner 2 limb darkening measurements of Venus at microwave range, discussing peak brightness temperature and opacity models
Indigenous biology in Venus clouds, proposing isopycnic float bladder macroorganism ingesting water and minerals blown up from surface by pinocytosis
Spacecraft sterilization standards and microbial contamination of Mars
Theoretical, observational, and laboratory work on planetary environments
Martian secular changes and dark area regeneration attributed to movement of sand, dust and wind caused by elevation and slope differences
Statistical correlation of latitude with time of maximum darkening of Mars dark areas, noting consistency of 2 models
Component of Mars ionosphere due to solar protons
Thermodynamic equilibrium composition of Venus atmosphere computed from atomic composition deduced spectroscopically
Thermodynamic equilibrium composition of all combinations of C, H, O and N at average pressure and temperature calculated for atmospheres of earth, Venus, Mars and Jupiter
Radar measurements of Doppler spectra and power reflectivity of Mars interpreted as surface elevation differences between dark and bright areas
Anisotropic nonconservative scattering in modified Schuster-Schwarzschild approximation and Venus cloud layer
Critical test of electric discharge model for Venus microwave emission
Decision theory biological search strategies and planetary quarantine aspects of Mars exploratory missions
Canals on bright areas of Mars surface, from comparisons of observer sketches and Mariner IV PHOTOGRAPHS and Doppler spectroscopic results for dark areas
Doppler radar spectroscopy of Mars surface - elevation differences between bright and dark areas
Method for calculating properties of monochromatic radiation through layer of dispersed particles and its application to Venus clouds