NASA NTRS · 19830041716
Cloud height differences on Saturn
Abstract
Spectrophotometry from 0.6-2.5 micron at 1.5% spectral resolution of Saturn's equator and visibly dark South Equatorial Belt near a 1980 ring-plane crossing shows substantially less absorption by methane over the equator than over the SEB. Model fits using Appleby's model atmosphere and a multiple scattering model lead to the conclusion that the pressure levels of the clouds in the two regions differ by 20%. The region of high clouds is coincident with the location of the equatorial fast jet observed by Voyager.
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Apt, J., Singer, R. B.. 1982-12-01. Cloud height differences on Saturn. https://ntrs.nasa.gov/citations/19830041716
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