The brightening of Saturn's F ring

@article{French2009TheBO,
  title={The brightening of Saturn's F ring},
  author={Robert S. French and Mark R. Showalter and Rafael Sfair and Carlos A. Arguelles and Myriam Pajuelo and Patricio Becerra and Matthew M. Hedman and Philip D. Nicholson},
  journal={Icarus},
  year={2009},
  volume={219},
  pages={181-193}
}
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RWG Executive Summary : Cassini has
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Figure 1: Main rings of Saturn; the image is registered along its top edge with a radial profile of the ring optical depth from a Cassini UVIS stellar occultation. The optical depth (usually denoted
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Saturn's F Ring As Seen By Cassini UVIS
Saturn's F Ring: Kinematics and Particle Sizes from Stellar Occultation Studies
Abstract The occultation of GSC5249-01240 by Saturn's rings was observed in a spectrally resolved mode using the Faint Object Spectrograph on the Hubble Space Telescope. By combining these data with
Voyager Photometry of Saturn's A Ring
Abstract Saturn's A Ring samples a wide range of dynamical environments, from the relatively unperturbed, optically thick inner region to the outer part of the ring, which contains numerous density
CASSINI UVIS STELLAR OCCULTATION OBSERVATIONS OF SATURN's RINGS
The Cassini spacecraft's Ultraviolet Imaging Spectrograph (UVIS) includes a high-speed photometer (HSP) that has observed more than 100 stellar occultations by Saturn's rings. Here, we document a
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Moonlets wandering on a leash-ring
Since the Voyager flybys, embedded moonlets have been proposed to explain some of the surprising structures observed in Saturn's narrow F ring. Experiments conducted with the Cassini spacecraft
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