  We present the impact rates of dust particles recorded by the Cosmic Dust
Analyzer (CDA) aboard the Cassini spacecraft. The "dust counters" evaluate the
quality of an impact and give rise to the apparent density of dust particles in
space.
  The raw data is pre-selected and refined to a new structure that serves to a
better investigation of densities, flows, and properties of interplanetary dust
grains. Our data is corrected for the dead time of the instrument and
corresponds to an assumed Kepler orbit (pointing of the sensitive area). The
processed data are published on the website for the Magnetosphere and Plasma
Science (MAPSview), where it can be correlated with other Cassini instruments.
  A sample is presented for the Titan flyby on DOY 250/2006. We find that the
dust density peaks at two times, at least, in a void region between Titan and
Rhea. Such features may point to extended clouds of small particles drifting
slowly in space. These density clouds seem to be stable for as long as several
months or few years before dispersing.
