Saturn's Upper Atmospheric Hazes Observe
โ
Erich Karkoschka; Martin G. Tomasko
๐
Article
๐
1993
๐
Elsevier Science
๐
English
โ 967 KB
We observed Saturn with the Hubble Space Telescope at wavelengths \(0.30-0.89 \mu \mathrm{m}\) for the purpose of determining the distribution of hazes. In the stratosphere, haze optical depths in the ultraviolet are essentially zero for midnorthern latitudes, are small ( \(\sim 0.2\) ) at low latit