Saturn's Upper Atmospheric Hazes Observe
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Erich Karkoschka; Martin G. Tomasko
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Article
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1993
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Elsevier Science
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English
β 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