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90. With the completion of the second Voyager Saturn encounter, the Voyager spacecraft have now returned more than 62,000 images of Jupiter, Saturn, and their entourages. More than a random accumulation of photographs, these images constitute carefully planned and executed time-lapse sequences of atmospheric volcanic or ring activity, multispectral mosaics of geologic surfaces, or extensive scans of small-scale ring structure. This treasure of stunning and informative pictures greatly exceeds the original imaging plans for Voyager and represents the successful efforts of several thousand talented individuals who have devoted their skills to this mission. A few of these people, those who are directly associated with this report, are listed below. J. B. Plescia (crater counts), L. A. Sromovsky (Saturn and Titan measurements); P. Thomas (satellite radiometry), T. C. Duxbury (Hyperion); P. Goldreich, J. J. Lissauer E. Grun, G. Morfill (ring structure and formation); S. W. Squyres (geology), J. L. Anderson, P. L. Jepsen, and G. M. Yagi (image processing); G. W. Garneau (atmospheric feature tracking for sequence predictions); G. P. Dimit, L. Garcia, D. Godfrey, A. Piumpunyalerd, E. T. Simien and E. S. Thompson (data handling and manuscript preparation); JPL's photolab and graphics departments, Image Processing Laboratory, and Mission and Test Imaging System, and two reviewers, including M. J. S. Belton. G.E.H. is supported by the Science and Engineering Research Council, Great Britain. This report presents the results of one phase of research carried out at the Jet Propulsion Laboratory under NASA contract 7-100.
Last updated Feb-27-1997