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Dynamic feature analysis for Voyager at the Image Processing LaboratoryVoyager 1 and 2 were launched from Cape Kennedy to Jupiter, Saturn, and beyond on September 5, 1977 and August 20, 1977. The role of the Image Processing Laboratory is to provide the Voyager Imaging Team with the necessary support to identify atmospheric features (tiepoints) for Jupiter and Saturn data, and to analyze and display them in a suitable form. This support includes the software needed to acquire and store tiepoints, the hardware needed to interactively display images and tiepoints, and the general image processing environment necessary for decalibration and enhancement of the input images. The objective is an understanding of global circulation in the atmospheres of Jupiter and Saturn. Attention is given to the Voyager imaging subsystem, the Voyager imaging science objectives, hardware, software, display monitors, a dynamic feature study, decalibration, navigation, and data base.
Document ID
19790043569
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Yagi, G. M.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Lorre, J. J.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Jepsen, P. L.
(California Institute of Technology, Jet Propulsion Laboratory, Pasadena Calif., United States)
Date Acquired
August 9, 2013
Publication Date
January 1, 1978
Subject Category
Ground Support Systems And Facilities (Space)
Meeting Information
Meeting: Conference on Atmospheric Environment of Aerospace Systems and Applied Meteorology
Location: New York, NY
Start Date: November 14, 1978
End Date: November 16, 1978
Accession Number
79A27582
Funding Number(s)
CONTRACT_GRANT: NAS7-100
Distribution Limits
Public
Copyright
Other

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