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Azimuthal brightness variations of Saturn's rings. III - Observations at tilt angle B approximately equal to 11.5 degThe brightness variation in Saturn's ring A with orbital phase of the ring particles does not change significantly as the declination of the earth, B, decreases from about 16.5 to 11.5 deg and is noticeably more pronounced than when the rings are fully open. The present data are also not inconsistent with earlier results suggesting that the amplitude of this azimuthal effect diminishes near opposition.
Document ID
19790049172
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Lumme, K.
(Massachusetts Univ. Amherst, MA, United States)
Irvine, W. M.
(Massachusetts, University Amherst, Mass., United States)
Martin, L. J.
(Massachusetts Univ. Amherst, MA, United States)
Baum, W. A.
(Lowell Observatory Flagstaff, Ariz., United States)
Date Acquired
August 9, 2013
Publication Date
April 15, 1979
Publication Information
Publication: Astrophysical Journal
Subject Category
Lunar And Planetary Exploration
Accession Number
79A33185
Funding Number(s)
CONTRACT_GRANT: NGR-03-003-001
CONTRACT_GRANT: NGL-22-010-023
Distribution Limits
Public
Copyright
Other

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