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VLA observations of Saturn at 1.3, 2, and 6 cmRadio maps with a resolution of 1.5 arcsec were made of Saturn at 1.3, 2, and 6 cm. The inclination of the ring plane was -5.4 deg. A fraction of 0.49 + or - 0.08 of Saturn's emitted light is transmitted through the rings at 2 and 6 cm. This value converts to an effective head-on or normal optical depth of 0.07 + or - 0.02. The transparency at this small inclination angle must be provided entirely by the regions of very low optical depth, e.g., the Cassini and Encke's Divisions, and to achieve the desired number this requires either a relatively large fraction of gaps or a strong forward scattering by the ring particles. The planetary disk appears to be much less limb darkened in the N-S than the E-W direction, while cuts across the planet, averaged over all directions, agree with the theoretical limb-darkening curves for a planet with a uniform atmosphere and solar abundances for all chemical elements.
Document ID
19820056832
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
De Pater, I.
(Arizona, University Tucson, AZ, United States)
Dickel, J. R.
(Illinois, University Urbana, IL, United States)
Date Acquired
August 10, 2013
Publication Date
April 1, 1982
Publication Information
Publication: Icarus
Volume: 50
Subject Category
Lunar And Planetary Exploration
Accession Number
82A40367
Funding Number(s)
CONTRACT_GRANT: NGR-14-005-176
CONTRACT_GRANT: NSG-7558
Distribution Limits
Public
Copyright
Other

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