Particle Size Variations in Saturn's Rings from Occultation Statistics

Details Particle Size Variations in Saturn's Rings from Occultation Statistics Particle Size Variations in Saturn's Rings from Occultation Statistics

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf.1282c&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.1282

Computer Science

Scientific paper

The size of particles in Saturn's rings can introduce an excess variance in stellar occultation data if the particles (or clumps of particles) are not small compared to the size of the field of view [1, 2]. We present an analysis of Cassini UVIS stellar occultation data of Saturn's rings showing distinct particle populations between different regions and ringlets in the ring system.

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