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Voyager image processing at the Image Processing LaboratoryThis paper discusses new digital processing techniques as applied to the Voyager Imaging Subsystem and devised to explore atmospheric dynamics, spectral variations, and the morphology of Jupiter, Saturn and their satellites. Radiometric and geometric decalibration processes, the modulation transfer function, and processes to determine and remove photometric properties of the atmosphere and surface of Jupiter and its satellites are examined. It is exhibited that selected images can be processed into 'approach at constant longitude' time lapse movies which are useful in observing atmospheric changes of Jupiter. Photographs are included to illustrate various image processing techniques.
Document ID
19800066835
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Jepsen, P. L.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Mosher, J. A.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Yagi, G. M.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Avis, C. C.
(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)
Garneau, G. W.
(California Institute of Technology, Jet Propulsion Laboratory, Pasadena Calif., United States)
Date Acquired
August 10, 2013
Publication Date
September 1, 1980
Publication Information
Publication: vol. 33
Subject Category
Lunar And Planetary Exploration
Accession Number
80A51005
Funding Number(s)
CONTRACT_GRANT: NAS7-100
Distribution Limits
Public
Copyright
Other

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