Abstract
In view of the possibility of employing Cassini’s experiments
for the diagnosis of Saturn’s rings, a semi-review is given of recent studies of
morphology and dynamics of low and moderately high optical depth regions of
Saturn’s rings with special emphasis on its fine-scale radial structure (irregular
cylindric structures of the order of 100 m or so). We predict that forthcoming
(2004) Cassini spacecraft high-resolution images of Saturn’s rings may reveal
this kind of radial structure.
for the diagnosis of Saturn’s rings, a semi-review is given of recent studies of
morphology and dynamics of low and moderately high optical depth regions of
Saturn’s rings with special emphasis on its fine-scale radial structure (irregular
cylindric structures of the order of 100 m or so). We predict that forthcoming
(2004) Cassini spacecraft high-resolution images of Saturn’s rings may reveal
this kind of radial structure.
| Original language | English |
|---|---|
| Title of host publication | Order and Chaos in Stellar and Planetary Systems |
| Pages | 129 |
| Number of pages | 1 |
| Volume | 316 |
| ISBN (Electronic) | 9781583812518 |
| State | Published - 2004 |
Publication series
| Name | ASP Conference Series, |
|---|