Planetary isophotes as a clue to aerosol characteristics. II - Observations of Venus from spacecraft

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Aerosols, Isophotes, Limb Darkening, Optical Polarization, Venus Clouds, Albedo, Atmospheric Scattering, Isotropism, Mariner 10 Space Probe, Mie Scattering, Sulfuric Acid, Venera Satellites, Wavelengths, Mariner 10, Sulfuric Acid, Aerosols, Venera 9, Atmosphere, Clouds, Planets, Venus

Scientific paper

Contrary to published reports, the limb-darkening observed by Mariner 10 is consistent with the sulfuric-acid aerosol scattering that explains the polarization and spectroscopic features of Venus. A combination of both geometric and photometric systematic errors explains the previously reported discrepancy. Although the aerosol model cannot be distinguished from isotropic scattering at the Mariner 10 phase angle, Venera 9 data at larger phases clearly favor the aerosol model. There is no evidence for isotropic scattering in the clouds of Venus.

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