Results 201 to 210 of about 349,003 (221)
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Detecting the tidal dissipation in the Saturnian system
2007We examine the problem of detecting the observational signature of tides in the Saturnian system. We show that, because of energy trn,sfer encouraged by the mean-motion resonances, S-1 Mimas' secular acceleration should be detected by observing S-3 Tethys instead of Mimas itself. We have a similar conclusion for the Enceladus/Dione resonance.
Noyelles, Benoît +2 more
openaire +1 more source
A New Computation of Tidal Dissipation in Tethys
2008Orbital study of Saturn's main satellites suggests a peculiar behaviour for one of them: Tethys. Its motion is characterized by a rapid circulation of the periapsis, while the mean anomaly oscillates around this latter. Such behaviour is caused by Saturn's strong oblateness.
Lainey, Valéry +2 more
openaire +1 more source
Tidal Dissipation Within Large Icy Satellites: Applications to Europa and Titan
Icarus, 2005Gabriel Tobie, Christophe Sotin
exaly
Tidal Energy Fluxes and Dissipation in the Chesapeake Bay
Continental Shelf Research, 2006Liejun Zhong
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The Evolution of Tides and Tidal Dissipation Over the Past 21,000 Years
Journal of Geophysical Research: Oceans, 2014Sophie-Berenice Wilmes, J A M Green
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Coupling Mantle Convection and Tidal Dissipation: Applications to Enceladus and Earth-Like Planets
Journal of Geophysical Research E: Planets, 2010Marie Behounkova +2 more
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Tidal Dissipation by Solid Friction and the Resulting Orbital Evolution
Reviews of Geophysics, 1964William Mason Kaula
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