A dozen lightcurves obtained during the ground-based observations of the occultation of 28 Sgr by Titan (3 July 1989) are reanalyzed. Profiles of density and temperature between altitude levels z 1 Partly supported by a grant from the Institut Universitaire de France. of 290 and 500 km (pressures p
Occultation of Sgr A
โ Scribed by KRISHNA, GOPAL; SWARUP, G.; SARMA, N. V. G.; JOSHI, M. N.
- Book ID
- 109683357
- Publisher
- Nature Publishing Group
- Year
- 1972
- Tongue
- English
- Weight
- 329 KB
- Volume
- 239
- Category
- Article
- ISSN
- 0028-0836
- DOI
- 10.1038/239091a0
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