  We revisit the evidence for a "dust cloud" observed by the Cassini spacecraft
at Saturn in 2006. The data of four instruments are simultaneously compared to
interpret the signatures of a coherent swarm of dust that would have remained
near the equatorial plane for as long as six weeks. The conspicuous pattern, as
seen in the dust counters of the Cosmic Dust Analyser (CDA), clearly repeats on
three consecutive revolutions of the spacecraft. That particular cloud is
estimated to about 1.36 Saturnian radii in size, and probably broadening. We
also present a reconnection event from the magnetic field data (MAG) that leave
behind several plasmoids like those reported from the Voyager flybys in the
early 1980s. That magnetic bubbles happened at the dawn side of Saturn's
magnetosphere. At their nascency, the magnetic field showed a switchover of its
alignment, disruption of flux tubes and a recovery on a time scale of about 30
days. However, we cannot rule out that different events might have taken place.
Empirical evidence is shown at another occasion when a plasmoid was carrying a
cloud of tiny dust particles such that a connection between plasmoids and
coherent dust clouds is probable.
