| Institution: | (1) Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, 91109, U.S.A.;(2) Goddard Institute for Space Studies, National Aeronautics and Space Administration, New York, NY, 10025, U.S.A.;(3) Alenia Aerospazio, 00131 Rome, Italy;(4) Observatoire de Paris, 92195 Meudon, France;(5) U. S. Geological Survey, Flagstaff, AZ, 86001, U.S.A.;(6) Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ, 85721, U.S.A.;(7) Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA, 91125, U.S.A.;(8) Universit’a La Sapienza, 00184 Rome, Italy;(9) Dip. Interateneo di Fisica, Politecnico di Bari, 70126 Bari, Italy;(10) British Antarctic Survey, CB3 0ET Cambridge, U.K.;(11) Facolt’a di Ingegneria, 80125 Naples, Italy;(12) University of North Dakota, Grand Forks, ND, 58202, U.S.A.;(13) Stanford University, Stanford, CA, 94305, U.S.A. |
| 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.RADAR Team LeaderThis revised version was published online in July 2005 with a corrected cover date. |
