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Voyager imaging experimentThe Voyager imaging experiment, which involves two independently operated television systems (a narrow- and a wide-angle camera), is designed to conduct investigations of the atmospheres and surface properties of Jupiter, Saturn, their satellites and Saturn's rings. Objects of the investigations include the horizontal and vertical structure of visible clouds, the vertical structure of high, optically thin scattering layers on Jupiter and Saturn, the Great Red Spot, the South Equatorial Belt, chromophores on Io and Titan, the geology of several satellites, the masses, spin axes and periods of rotation of several satellites, the radial distribution of material in Saturn's rings, and the optical scattering properties of the primaries, rings, and satellites at a variety of wavelengths and phase angles.
Document ID
19780037729
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Smith, B. A.
(Arizona, University Tucson, Ariz., United States)
Briggs, G. A.
(Arizona Univ. Tucson, AZ, United States)
Danielson, G. E.
(California Institute of Technology, Jet Propulsion Laboratory, Pasadena Calif., United States)
Cook, A. F., II
(Harvard College Observatory and Smithsonian Astrophysical Observatory, Center for Astrophysics, Cambridge Mass., United States)
Davies, M. E.
(Rand Corp. Santa Monica, Calif., United States)
Hunt, G. E.
(Meteorological Office Bracknell, Berks., United Kingdom)
Masursky, H.
(Arizona Univ. Tucson, AZ, United States)
Soderblom, L. A.
(U.S. Geological Survey Washington, D.C., United States)
Owen, T. C.
(New York, State University Stony Brook, N.Y., United States)
Sagan, C.
(Cornell University Ithaca, N.Y., United States)
Date Acquired
August 9, 2013
Publication Date
November 1, 1977
Publication Information
Publication: Space Science Reviews
Volume: 21
Subject Category
Lunar And Planetary Exploration
Accession Number
78A21638
Distribution Limits
Public
Copyright
Other

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