Polarimetry and photometry of Saturn from Pioneer 11 Observations and constraints on the distribution and properties of cloud and aerosol particles

Details Polarimetry and photometry of Saturn from Pioneer 11 Observations and constraints on the distribution and properties of cloud and aerosol particles Polarimetry and photometry of Saturn from Pioneer 11 Observations and constraints on the distribution and properties of cloud and aerosol particles

Apr 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984icar...58....1t&link_type=abstract

Icarus (ISSN 0019-1035), vol. 58, April 1984, p. 1-34. NASA-NSF-supported research.

Physics

Optics

46

Aerosols, Atmospheric Optics, Cloud Photography, Optical Polarization, Polarimetry, Saturn Atmosphere, Astronomical Photometry, Atmospheric Scattering, Cloud Height Indicators, Optical Thickness, Pioneer 11 Space Probe, Rayleigh Scattering, Saturn, Polarimetry, Photometry, Pioneer 11, Observations, Properties, Distribution, Clouds, Aerosols, Particles, Polarization, Atmosphere, Imaging Photopolarimeter Experiment, Ipp, Data, Scattering, Phases, Zones, Comparisons, Models, Optical Properties, Depth, Pressure

Scientific paper

A purpose of this paper is to present the new polarization observations of Saturn obtained during the Pioneer Saturn mission. These data have substantial coverage on the planet at reasonably high spatial resolution, and show important variations with latitude, phase angle, wavelength, and center-to-limb position. The reduced photometry and polarimetry of two latitude bands (7°S-11°S and 15°S-17°S) as well as a north-south scan are presented in detailed tables. Information regarding the single-scattering properties of the aerosols and their vertical and horizontal distributions was obtained by comparing the data with a simple multiple-scattering model. The model contained a single type of cloud particle mixed with Rayleigh scattering gas.

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