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Cloud height differences on SaturnSpectrophotometry 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.
Document ID
19830041716
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Apt, J.
(California Institute of Technology, Jet Propulsion Laboratory, Earth and Space Sciences Div., Pasadena, CA; NASA, Johnson Space Center Houston, TX, United States)
Singer, R. B.
(Hawaii, University Honolulu, HI, United States)
Date Acquired
August 11, 2013
Publication Date
December 1, 1982
Publication Information
Publication: Icarus
Volume: 52
Subject Category
Lunar And Planetary Exploration
Accession Number
83A22934
Funding Number(s)
CONTRACT_GRANT: NSG-7323
CONTRACT_GRANT: NAS7-100
Distribution Limits
Public
Copyright
Other

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