  We revisit the evidence for a "dust cloud" observed by the Cassini spacecraft
at Saturn in 2006. The simultaneous data of 3 instruments are compared to
interpret the signatures of a coherent swarm of dust that could have remained
floating near the equatorial plane. The conspicuous pattern, as seen in the
dust counters of the Cosmic Dust Analyser (CDA) and in the magnetic field
(MAG), clearly repeats on three consecutive revolutions of the spacecraft. The
data of the Radio Plasma and Wave Science (RPWS) appear less decisive but do
back our conclusions. The results support the idea of a "magnetic bubble" as
reported from both Voyager flybys in the early 1980ies. That particular cloud,
which we firstly discovered in the CDA data, is estimated to about 1.36
Saturnian radii in size, and probably broadening. Both the bulk of dust
particles and the peak of the magnetic depression seem to drift apart, but this
can also be an effect of hitting the cloud at different parts during the
traverse.
