  About 76 glitches in 25 pulsars have been reported to date. Most glitches are
`giant', with fractional increases of frequency dnu_0/nu_0 ~ 10^{-6}. 25
glitches were analysed and presented by Shemar & Lyne (1996) who detected them
mainly at Jodrell Bank during the monitoring of a sample of 279 pulsars in a
regular timing programme up to MJD 49500. This paper is a continuation of their
work up to MJD 50500. We present the detection and analysis of a further 14
glitches in 9 pulsars, 6 of which have glitched for the first time since
monitoring had started. Eleven of these glitches are small (dnu_0/nu_0 ~
10^{-9}) and below the completeness threshold of Shemar and Lyne(1996). We
report a giant glitch in PSR B1930+22, the second largest reported hitherto,
with a dnu_0/nu_0 = 4.5 x 10^{-6}. We also report four recent glitches in PSR
B1737$-$30 which continues to exhibit frequent glitches. Few of these pulsars
show any recovery after the glitch.
