Infrared polarization of Venus

Computer Science

Scientific paper

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Atmospheric Composition, Cloud Cover, Infrared Instruments, Polarization Characteristics, Venus Atmosphere, Atmospheric Models, Instrument Errors, Sulfuric Acid, Venus, Polarization, Infrared, Wavelengths, Earth-Based Observations, Models, Comparisons, Sulfuric Acid, Clouds

Scientific paper

Infrared polarization of Venus was measured as several phase angles during 1977, 1978, and 1979. Observations revealed a significant degree of polarization at wavelengths of both 3.6 and 4.8 microns in contrast with little or no polarization in wavelengths shorter than 3 microns. Although the sulfuric acid cloud model seems a likely explanation of these measurements, a small discrepancy was found between these results and the calculations by Mukai and Mukai (1979).

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