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

Matthew S. Tiscareno·Philip D. Nicholson·Joseph A. Burns·Matthew M. Hedman·Carolyn C. Porco
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Abstract

We describe a model that accounts for the complex morphology of spiral density waves raised in Saturn's rings by the co-orbital satellites, Janus and Epimetheus. Our model may be corroborated by future Cassini observations of these time-variable wave patterns.

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Matthew S. Tiscareno, Philip D. Nicholson, Joseph A. Burns, Matthew M. Hedman, Carolyn C. Porco. 2006-10-09. Unravelling Temporal Variability in Saturn's Spiral Density Waves: Results and Predictions. https://doi.org/10.1086/509120

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