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RADAR Reveals Titan TopographyThe Cassini Titan RADAR Mapper is a K(sub u)-band (13.78 GHz, lambda = 2.17 cm) linear polarized RADAR instrument capable of operating in synthetic aperture (SAR), scatterometer, altimeter and radiometer modes. During the first targeted flyby of Titan on 26 October, 2004 (referred to as Ta) observations were made in all modes. Evidence for topographic relief based on the Ta altimetry and SAR data are presented here. Additional SAR and altimetry observations are planned for the T3 encounter on 15 February, 2005, but have not been carried out at this writing. Results from the T3 encounter relevant to topography will be included in our presentation. Data obtained in the Ta encounter include a SAR image swath
Document ID
20050170605
Acquisition Source
Headquarters
Document Type
Conference Paper
Authors
Kirk, R. L.
(Geological Survey Flagstaff, AZ, United States)
Callahan, P.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Seu, R.
(La Sapienza Univ. Rome, Italy)
Lorenz, R. D.
(Arizona Univ. Tucson, AZ, United States)
Paganelli, F.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Lopes, R.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Elachi, C.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Date Acquired
September 7, 2013
Publication Date
January 1, 2005
Publication Information
Publication: Lunar and Planetary Science XXXVI, Part 11
Subject Category
Lunar And Planetary Science And Exploration
Distribution Limits
Public
Copyright
Public Use Permitted.
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