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NASA JPL Mission To Jupiter Galileo NIMS Europa 15 & 16 Encounters CD GO_1116 V1 -- Spectral Image Cubes and Browse Products Volume 16 S/C Clock 4498598 to 4646936 --
In good condition. New and still sealed. Please see detailed photos.
GO_1116 is the sixteenth CD-ROM volume to contain Galileo Near InfraredMapping Spectrometer (NIMS) Spectral Image Cubes and associated browseproducts. It was generated by the NIMS team in collaboration with thePlanetary Data System (PDS) and the Multimission Image ProcessingSubsystem (MIPS) for distribution to the various Galileo projectinvestigators, and to the community of planetary scientists.
This volume is the result of systematic processing of Experiment DataRecords (EDRs) derived from NIMS instrument data taken during Galileo'sfifteenth and sixteenth encounters with Jupiter and its satellites: theEuropa 15 (E15) and Europa 16 (E16) encounters, which continue Galileo'sEuropa Mission (GEM), an extension of the Primary Mission. Earlier volumesin this series covered the Venus encounter, the two Earth/Moon encountersand the Jupiter Primary Mission; later volumes will contain cubes fromsubsequent GEM encounters of Jupiter and its satellites. (NIMS EDRsare archived in a separate CD-ROM series: GO_10xx.)
The Galileo NIMS instrument is an imaging spectrometer which covers thespectral range 0.7 to 5.2 micrometers, measuring both reflected sunlightand emitted thermal radiation in a region incompletely studied by thePioneer and Voyager spacecraft. Seventeen detectors and a diffractiongrating operate to produce spectra over as many as 408 wavelengths. Asecondary mirror scans through 20 positions in the cross-track directionat each grating step to produce a swath of data. The scan platform onwhich the instrument is mounted is commanded in two dimensions to conductextensive mapping observations over the target. A complete description ofthe NIMS instrument and scientific objectives is provided in the article"NEAR-INFRARED MAPPING SPECTROMETER EXPERIMENT ON GALILEO", R. W. Carlsonet al., Space Science Reviews v. 60 p. 457-502, 1992. A digital preprintof this article is included on this CD-ROM in the DOCUMENT.NIMSINSTdirectory. Additional information about NIMS may be found on the NIMSweb site (http://jumpy.igpp.ucla.edu/~nims) which is also linked fromthe Galileo web site (http://www.jpl.nasa.gov/galileo/). WARNING: Thelong-term existence and location of the Galileo and NIMS web sitesis uncertain.
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