Local simulations with up to 60,000 self-gravitating dissipatively colliding particles indicate that dense unperturbed ring systems with optical depth Ο > 1 can exhibit spontaneous viscous oscillatory instability (overstability), with parameter values appropriate for Saturn's B ring. These axisymmet
β¦ LIBER β¦
Optical reflectance polarimetry of Saturn globe and rings I. Measurements on B ring
β Scribed by Audouin Dollfus
- Publisher
- Elsevier Science
- Year
- 1979
- Tongue
- English
- Weight
- 783 KB
- Volume
- 37
- Category
- Article
- ISSN
- 0019-1035
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