establish the global shape of Triton's atmosphere at about 20-km altitude by modeling the detailed shape of the central flash), (ii) obtaining one or more light curves of high signal-to-noise ratio from a large telescope (to accurately determine the thermal structure of Triton's atmosphere), and (ii
Occultations of Io in 1997–1998: Predictions for the Observations of Hot Spots
✍ Scribed by Jean-Eudes Arlot; Pascal Decamps; William Thuillot
- Publisher
- Elsevier Science
- Year
- 1997
- Tongue
- English
- Weight
- 195 KB
- Volume
- 125
- Category
- Article
- ISSN
- 0019-1035
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