  We present the discovery of 24 pulsars in 15 Globular Clusters (GCs) using
the Five-hundred-meter Aperture Spherical radio Telescope (FAST). These include
the first pulsar discoveries in M2, M10, and M14. Most of the new systems are
either confirmed or likely members of binary systems. M53C, NGC6517H and I are
the only three pulsars confirmed to be isolated. M14A is a black widow pulsar
with an orbital period of 5.5 hours and a minimum companion mass of 0.016 \Ms.
M14E is an eclipsing binary pulsar with an orbital period of 20.3 hours. With
the other 8 discoveries that have been reported elsewhere, in total 32 GC
pulsars have been discovered by FAST so far. In addition, We detected M3A
twice. This was enough to determine that it is a black widow pulsar with an
orbital period of 3.3 hours and a minimum companion mass of 0.0125 \Ms.
