The structure of Saturn's rings: Implications from the Voyager stellar occultation
โ Scribed by L.W. Esposito; M. O'Callaghan; R.A. West
- Publisher
- Elsevier Science
- Year
- 1983
- Tongue
- English
- Weight
- 922 KB
- Volume
- 56
- Category
- Article
- ISSN
- 0019-1035
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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
dense main rings where collisions and collective processes play an important role, the particle concentration is so We have reanalyzed the data acquired by the planetary radioastronomy (PRA) experiment during the passage of Voyager small in these faint rings that the grains behave indepen-1 through