urn:nasa:pds:cassini-coradar:coradr_0195.data:bibqf36s166_d195_t056s01_v03
3.0
co-ssa-radar-5-bidr-v1.0 bibqf36s166_d195_t056s01_v03
1.13.0.0
Product_Observational
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
3.0
Apache Velocity Template for CORADR BIBQ images
2009-06-06T19:41:44.522Z 2009-06-06T20:18:16.986Z
Science
Derived
"The data values in this file are Synthetic
Aperture Radar (SAR) normalized backscatter cross-section values in
logarithmic form. The observed values have been corrected for
incidence-angle effects and converted to decibels (db). The raw
backscatter values have been multiplied by the function f(I), where I is
the incidence angle and f(I) = 0.2907/(f1(I)+f2(I)+f3(I)), for
f1(I)=2.8126*(cos(I)^4+893.9677*sin(I)^2)^(-1.5),
f2(I)=0.5824*(cos(I)^4+34.1366*sin(I)^2)^(-1.5), and
f3(I)=0.3767*cos(I)^1.9782. The corresponding decibel value is db = 10
log10 (cross-section * f(I)). The scaling between raw data number and db
is specified by the SCALING_FACTOR and OFFSET."
cassini-huygens
Mission
urn:nasa:pds:context:investigation:mission.cassini-huygens
data_to_investigation
cassini orbiter
Spacecraft
cassini radar
Instrument
TITAN
Satellite
TOUR
1623010993
1623013185
BIBQF36S166_D195_T056S01_V03.IMG
display_settings_to_array
Sample
Left to Right
Line
Top to Bottom
BIBQF36S166_D195_T056S01_V03.IMG
cartography_parameters_to_image_object
360.0000000
0.0000000
34.0533051
-81.4612348
Oblique Cylindrical
0.000000
0.000000
-31.9247290
178.1236370
90.0000000
-26.536812
69.995792
306.233405
(-0.84828844,-0.02779029,-0.52880470)
(0.43213493,0.54083238,-0.72163685)
(0.30604920,-0.84067118,-0.44677270)
LEFT
Coordinate Pair
1404.4446
1404.4446
32.0000000
32.0000000
134826.6816
3460551.4944
Planetographic
TITAN
2575000
2575000
2575000
Positive West
BIBQF36S166_D195_T056S01_V03.IMG
processing_information_to_data_object
LBDR_14_D195_V03
RANDOLPH L. KIRK
U.S.G.S. FLAGSTAFF
BIBQF36S166_D195_T056S01_V03.IMG
2018-01-30T17:13:13.000Z
BIBQF36S166_D195_T056S01_V03.IMG
4800
2
Last Index Fastest
UnsignedByte
1.0000012E-01
-2.0100010E+01
Line
4864
1
Sample
480
2
0