A single image from the Huygens Descent Imager/ Spectral Radiometer
(DISR) instrument of a dark plain area on Titan, seen during descent to
the landing site, that indicates flow around bright 'islands'. The areas
below and above the bright islands may be at different elevations.
The Descent Imager/Spectral Radiometer is one of two NASA instruments on
the probe.
The Cassini-Huygens mission is a cooperative project of NASA, the
European Space Agency and the Italian Space Agency. The Jet Propulsion
Laboratory, a division of the California Institute of Technology in
Pasadena, manages the Cassini-Huygens mission for NASA's Science Mission
Directorate, Washington, D.C. The Cassini orbiter and its two onboard
cameras were designed, developed and assembled at JPL. The Descent
Imager/Spectral team is based at the University of Arizona, Tucson, Ariz.
For more information about the Cassini-Huygens mission visit,
http://saturn.jpl.nasa.gov. For more information about the Descent
Imager/Spectral Radiometer visit http://www.lpl.arizona.edu/~kholso/.