Hydrodynamical Simulations of Narrow Planetary Rings. I. Scaling
β Scribed by Ignacio Mosqueira; Paul R. Estrada; Leigh Brookshaw
- Publisher
- Elsevier Science
- Year
- 1999
- Tongue
- English
- Weight
- 997 KB
- Volume
- 139
- Category
- Article
- ISSN
- 0019-1035
No coin nor oath required. For personal study only.
π SIMILAR VOLUMES
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
A molecular dynamics (MD) simulation of 35,000 picoseconds (ps) has been carried out to study the conformational interconversions of 1,l-difluoro-4,4dimethylcycloheptane at room temperature using the MM3 force field. The exchange between axial and equatorial fluorine atoms was the only conformationa