Physics – Optics
Scientific paper
Jan 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982apopt..21..214b&link_type=abstract
Applied Optics, vol. 21, Jan. 15, 1982, p. 214-227. NASA-supported research.
Physics
Optics
1
Astronomical Photography, Jupiter (Planet), Saturn (Planet), Spaceborne Photography, Voyager Project, Atmospheric Composition, Natural Satellites, Satellite Atmospheres, Satellite Television, Satellite-Borne Instruments, Saturn Rings, Star Trackers, Voyager 2 Spacecraft, Atmosphere, Circulation, Features, Plumes, Composition, F Ring, Europa, Braided Rings, Temperatures, Emissions, Plasmas, Weather, Discovery, Io, Comparisons, Observations, Planets, Jupiter, Saturn, Voyager 1, Imagery, Voyager 2, Satellites,
Scientific paper
The Voyager imaging system is described, noting that it is made up of a narrow-angle and a wide-angle TV camera, each in turn consisting of optics, a filter wheel and shutter assembly, a vidicon tube, and an electronics subsystem. The narrow-angle camera has a focal length of 1500 mm; its field of view is 0.42 deg and its focal ratio is f/8.5. For the wide-angle camera, the focal length is 200 mm, the field of view 3.2 deg, and the focal ratio of f/3.5. Images are exposed by each camera through one of eight filters in the filter wheel on the photoconductive surface of a magnetically focused and deflected vidicon having a diameter of 25 mm. The vidicon storage surface (target) is a selenium-sulfur film having an active area of 11.14 x 11.14 mm; it holds a frame consisting of 800 lines with 800 picture elements per line. Pictures of Jupiter, Saturn, and their moons are presented, with short descriptions given of the area being viewed.
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