A total of 9242 seismic events, recorded since the start of the erupti
on on Montserrat in July 1995, have been uniformly relocated with stat
ion travel-time corrections. Early seismicity was generally diffuse un
der southern Montserrat, and mostly restricted to depths less than 7 l
an. However, a NE-SW alignment of epicentres beneath the NE flank of t
he volcano emerged in one swarm of volcano-tectonic earthquakes (VTs),
and later nests of VT hypocentres developed beneath the volcano and a
t a separated location, under St. George's Hill. The overall spatial d
istribution of hypocentres suggests a minimum depth of about 5 km for
any substantial magma body. Activity associated with the opening of a
conduit to the surface became increasingly shallow, with foci concentr
ated below the crater and, after dome building started in Fall 1995, V
Ts diminished and repetitive swarms of 'hybrid' seismic events became
predominant. By late-1996, as magma effusion rates escalated, most sei
smic events were originating within a volume about 2 km diameter which
extended up to the surface from only about 3 km depth - the diminutio
n of shear failure earthquakes suggests the pathway for magma discharg
e had become effectively unconstricted. Individual and composite fault
plane solutions have been determined for a few larger earthquakes. We
postulate that localised extensional stress conditions near the linea
r VT activity, due to interaction with stresses in the overriding lith
ospheric plate, may encourage normal fault growth and promote sector w
eaknesses in the volcano.