Morphology and movements of polarization features on Venus as seen in the Pioneer Orbiter Cloud Photopolarimeter data

Computer Science – Sound

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Pioneer Venus Spacecraft, Polarimetry, Satellite Sounding, Venus Clouds, Haze, Intensity, Morphology, Phase Shift, Venus, Morphology, Polarization, Features, Pioneer Missions, Orbiters, Clouds, Photopolarimeter, Motion, Orbiter Cloud Photopolarimeter, Ocpp, Observtions, Comparisons, Brightness, Intensity, Wavelengths, Particles, Size, Haze, Mixing, Ultraviolet, Layers, Pressure, Optical Properties, Depth, Circulation, Atmosphere, Calculations, Data, Formation, Spectra, Photographs, Latitude

Scientific paper

Polarization observations obtained from the Orbiter Cloud Photopolarimeter (OCPP) show local, organized features whose morphology is similar to that of the ultraviolet clouds. No obvious correlation between the observed amount of polarization and relative brightness was found. Many of the features that can be seen even at 935 nm wavelength are believed to be signatures of local variations in the haze of submicron-size particles that have been detected from the OCPP data (K. Kawabata et al., 1980). Substantial variations in the structure and visibility of the polarization features that are observed suggest that the haze amount mixed with and above the main cloud layer may not be constant. The rapid retrograde circulation suggested by the movements of haze features in the polarimetry data would indicate that the layer in which such rapid circulation exists is fairly deep.

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