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Titel Spatially resolved self-gravity wakes in Saturn's A and B rings from Cassini UVIS occultations
VerfasserIn Miodrag Sremcevic, Larry Esposito, Joshua Colwell
Konferenz EGU General Assembly 2011
Medientyp Artikel
Sprache Englisch
Digitales Dokument PDF
Erschienen In: GRA - Volume 13 (2011)
Datensatznummer 250057379
 
Zusammenfassung
After 6 years of Cassini mission the UVIS instrument recorded more than hundred stellar occultations by Saturn's rings. Most of the observed occultations have excellent spatial resolution on the order of ten meters or even better. In a recent, specially crafted high-resolution occultation of the mid A ring we for the first time directly resolved individual self-gravity wakes. The occultation was designed to track the orbital motion of ring particles, achieving the true resolution in the co-rotating ring plane of less than a meter. In this unique occultation the self-gravity wakes manifest themselves as opaque or nearly opaque regions (tau>1.5) and constitute about 30% of the total occultation signal. The observed wake lengths can be as large as 200m. Another 30% of the ring is practically transparent (tau<0.05), and somewhat shorter (L<100m). The opaque and transparent regions are interspersed with material in an intermittent state (0.05