Multicolor CCD images at selected wavelengths from 370 to \(900 \mathrm{~nm}\) obtained at Pic-du-Midi Observatory during four different phases of the development of Saturn's equatorial disturbance are used to analyze its photometric properties. Three epochs and four morphologically different region
Saturn's equatorial haze
β Scribed by L. Trafton
- Publisher
- Elsevier Science
- Year
- 1983
- Tongue
- English
- Weight
- 365 KB
- Volume
- 3
- Category
- Article
- ISSN
- 0273-1177
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