Computer Science
Scientific paper
Sep 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991icar...93....3r&link_type=abstract
Icarus (ISSN 0019-1035), vol. 93, Sept. 1991, p. 3-24.
Computer Science
22
Optical Thickness, Orbital Resonances (Celestial Mechanics), Radio Occultation, Saturn Rings, Density Wave Model, Satellite Orbits, Voyager 1 Spacecraft, Wave Propagation
Scientific paper
Individual and comparative analyses are conducted for 29 of the wavelike features revealed by optical depth profiles of Saturn's rings; of these, 18 are in Ring A, one is in Ring B, and 10 are in Ring C. Only 20 of these were identifiable with known resonances, and all eight of the unexplained wave features are in Ring C. For 14 weak density waves in Ring A, a linear density wave theory modeling of the waveform near resonance yields independent estimates of the surface mass density together with reliable estimates of resonance location.
Marouf Essam A.
Rosen Paul A.
Tyler Leonard G.
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