  We have analyzed 5.5 years of timing observations of 7 ``slowly'' rotating
radio pulsars, made with the Westerbork Synthesis Radio Telescope. We present
improved timing solutions and 30, mostly small new glitches. The most
interesting results are: 1) The detection of glitches one to two orders of
magnitude smaller than ever seen before in slow radio pulsars. 2) Resolving
timing-noise looking structures in the residuals of PSR B1951+32 by using a set
of small glitches. 3) The detections of three new glitches in PSR J1814-1744, a
high-magnetic field pulsar. In these proceedings we present the most
interesting results of our study. For a full coverage, we refer the reader to
Janssen & Stappers (2006).
