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We describe a model that accounts for the complex morphology of spiraldensity waves raised in Saturn's rings by the co-orbital satellites, Janus andEpimetheus. Our model may be corroborated by future Cassini observations ofthese time-variable wave patterns.Comment: 9 pages, 5 figures; In press at Astrophysical Journal Letter

Unravelling Temporal Variability in Saturn's Spiral Density Waves: Results and Predictions