The profile of Saturn's ring a as derived from stellar occultations
โ Scribed by J. O. Piironen
- Publisher
- Springer Netherlands
- Year
- 1978
- Tongue
- English
- Weight
- 230 KB
- Volume
- 19
- Category
- Article
- ISSN
- 1573-0794
No coin nor oath required. For personal study only.
๐ SIMILAR VOLUMES
We present optical depth profiles for Saturn's rings at wavelengths of 0.9, 2.1, 3.3, and 3.9 ยตm, obtained from the occultation of the star 28 Sgr on 3 July 1989 when the rings were near their maximum opening angle. The radial resolution of the data is โผ18 km, as set by the angular diameter of the s
## We analyze an extensive data set of immersion and emersion 2 Visiting Astronomer, Cerro Tololo Inter-American Observatory, lightcurves of the occultation of 28 Sgr by Saturn's atmosphere National Optical Astronomy Observatories, operated by the Association on 3 July 1989. The data give profiles