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The Cassini Radar InvestigationThe Cassini/Huygens Mission is a nineteen-year multinational project to design, construct and execute an investigation of the Saturn system, with emphasis on its largest moon, Titan. Titan's atmosphere is nearly opaque at optical wavelengths, so a Ku-band radar imaging system was required to map its surface. In this paper we describe the radar instrument, discuss some of the challenges to its design, and review its operating modes. We briefly summarize the surprises that the radar instrument has revealed while investigating Titan.
Document ID
20090039491
Acquisition Source
Jet Propulsion Laboratory
Document Type
Other
External Source(s)
Authors
Wall, Stephen D.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Date Acquired
August 24, 2013
Publication Date
June 2, 2008
Subject Category
Communications And Radar
Distribution Limits
Public
Copyright
Other
Keywords
Cassini
radar instrumentation

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