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Infrared scans of SaturnScans are presented at five wavelengths between 7.8 and 25 microns north-south along Saturn's central meridian and east-west parallel to the equator through the subearth point. The brightening of Saturn's South Pole at 12.7 microns was more enhanced in 1977 than in 1978 due to the 5 deg greater declination of the polar axis in 1977. There is a plateau in the Southern Hemisphere between -30 and -60 deg latitude in the 7.8 and 12.7 micron scans. The apparent temperature of the rings decreased as Saturn approached the equinox. It is found generally that the strongest ring emission arises from the C ring.
Document ID
19800058155
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Sinton, W. M.
(Hawaii Univ. Honolulu, HI, United States)
Macy, W. W.
(Hawaii Univ. Honolulu, HI, United States)
Good, J.
(Hawaii, University Honolulu, Hawaii, United States)
Orton, G. S.
(California Institute of Technology, Jet Propulsion Laboratory, Earth and Space Sciences Div., Pasadena Calif., United States)
Date Acquired
August 10, 2013
Publication Date
May 1, 1980
Publication Information
Publication: Icarus
Volume: 42
Subject Category
Lunar And Planetary Exploration
Accession Number
80A42325
Funding Number(s)
CONTRACT_GRANT: NGL-12-001-057
Distribution Limits
Public
Copyright
Other

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