The phase function of Venus cloud particles from Mariner 10 data

Details The phase function of Venus cloud particles from Mariner 10 data The phase function of Venus cloud particles from Mariner 10 data

Dec 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978georl...5.1067h&link_type=abstract

Geophysical Research Letters, vol. 5, Dec. 1978, p. 1067-1070. NASA-supported research.

Physics

Cloud Photographs, Light Scattering, Mariner 10 Space Probe, Phase Shift, Venus Clouds, Brightness, Forward Scattering, Polarization (Waves), Visual Photometry, Imagery, Polarization, Observations, Particles, Photometry, Venus, Mariner 10, Clouds, Brightness, Scattering, Phase Angles, Data

Scientific paper

Mariner 10 images of Venus taken at several phase angles were photometrically reduced. The analysis shows that the phase function of the cloud particles is not isotropic, as had been deduced earlier from the brightness distribution on spacecraft images taken at a single phase angle, but has a broad minimum near 60 deg and is forward-scattering. The scattering properties are in quantitative agreement with previous deductions from earth-based polarization measurements by Hansen and his associates.

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