We previously reported [1] the first
steps in the development of the SPanish Meteor Network
(SPMN) by using innovative low-scan all-sky
CCD cameras that are reaching +2/+3 meteor limiting
magnitude [1]. During 2006 new progress has been
made by setting up two additional all-sky CCD stations
and three video stations in order to increase our
atmospheric coverage of meteor and fireball activity
[2]. During 2006, we have built the first cameras with
(inner) rotating shutter in order to get measurements of
meteor velocities. Additionally, for those all-sky CCD
cameras still working without rotating shutter we have
used video cameras for obtaining meteor velocities in
the monitorized common fields. As a consequence of
all this effort, valuable trajectory and orbital data of
meteors and fireballs is being obtained. We focus here
in a description of recorded activity of cometary meteor
showers also including orbital information of one
of the brightest fireballs observed last year. Particularly,
we describe some Earth encounters with dense
cometary meteoroid streams that can be useful for
identifying a likely origin of recovered Interplanetary
Dust Particles (IDPs)
