Abstract
In view of the possibility of employing Cassini's experiments for the diagnosis of Saturn's rings, local N-body simulations of low and moderately high optical depth regions of Saturn's rings are presented. A special emphasis is made on fine-scale spiral structures (irregular cylindric wave-type structures of the order of 100 m or so) of Saturn's main A, B, and C rings. We predict that Cassini spacecraft high-resolution images of Saturn's main rings will reveal this kind of irregular microstructure.
| Original language | English |
|---|---|
| Pages (from-to) | 770-776 |
| Number of pages | 7 |
| Journal | Advances in Space Research |
| Volume | 38 |
| Issue number | 4 |
| DOIs | |
| State | Published - 1 Jan 2006 |
Keywords
- Instabilities and waves
- N-body simulations
- Planetary rings
- Saturn's rings
ASJC Scopus subject areas
- Aerospace Engineering
- Astronomy and Astrophysics
- Geophysics
- Atmospheric Science
- Space and Planetary Science
- General Earth and Planetary Sciences