urn:nasa:pds:cassini-coradar:coradr_0065.ancillary:titan_flyby_id_table.txt
1.0
Cassini Titan flyby table
1.9.0.0
Product_File_Text
Elachi, C.; Allison, M. D.; Borgarelli, L.; Encrenaz, P.; Im, E.; Janssen, M. A.; Johnson, W. T. K.; Kirk, R. L.; Lorenz, R. D.; Lunine, J. I.; Muhleman, D. O.; Ostro, S. J.; Picardi, G.; Posa, F.; Rapley, C. G.; Roth, L. E.; Seu, R.; Soderblom, L. A.; Vetrella, S.; Wall, S. D. Wood, C. A.; Zebker, H. A.
2004
Title: "Radar: The Cassini Titan Radar Mapper"
Publication: The Cassini-Huygens Mission, by Russell, Christopher T., ISBN 978-1-4020-3147-2. Kluwer Academic Publishers, 2004, p. 71
DOI: 10.1007/1-4020-3874-7_2
Abstract: The Cassini RADAR instrument is a multimode 13.8 GHz multiple-beam sensor that can operate as a synthetic-aperture radar (SAR) imager, altimeter, scatterometer, and radiometer. The principal objective of the RADAR is to map the surface of Titan. This will be done in the imaging, scatterometer, and radiometer modes. The RADAR altimeter data will provide information on relative elevations in selected areas. Surfaces of the Saturn's icy satellites will be explored utilizing the RADAR radiometer and scatterometer modes. Saturn's atmosphere and rings will be probed in the radiometer mode only. The instrument is a joint development by JPL/NASA and ASI. The RADAR design features significant autonomy and data compression capabilities. It is expected that the instrument will detect surfaces with backscatter coefficient as low as -40 dB.
2021-03-18
1.0
conversion of PDS3 CO RADAR archive to comply with PDS4 Information Model
urn:nasa:pds:context:node:node.imaging
has_association
urn:nasa:pds:context:investigation:mission.cassini-huygens
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TITAN_FLYBY_ID_TABLE.TXT
extras.TITAN_FLYBY_ID_TABLE.TXT
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TITAN_FLYBY_ID_TABLE.TXT
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This file contains a cross reference table of the four different
identifying numbers for each Titan flyby in the Prime Mission.
The four columns from left to right are: Titan flyby number,
data take number, sequence number, and rev number.
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