The
seismic refraction technique involves inducing a seismic impulse ('shot)
in the ground, and recording the arrival times of the seismic energy
which travels through ground, at a series of geophones (a 'spread')
laid at the surface. By firing shots at both ends of each spread it
is possible to calculate depths to rockhead, typically to an accuracy
of between +/-10 and 20%.
The
best type of seismic impulse is produce by very small explosive charges,
typically of the order of 100 or 200 gms. These shots are fired in holes
dug to around 1 - 1.5 metres depth; the shots generally produce very
little or no appreciable noise. Hammers and other similar methods of
producing a seismic impulse are not suitable except where the rockhead
is close to the surface, typically within 5 metres, due to energy dissipation
within the overburden.
Further
small charges are fired at locations along each spread, to determine
shallow seismic velocities.
A
typical spread designed to locate rock at depths up to 50 metres would
consist of 48 geophones at 5 metre intervals, resulting in a spread
length of 235 metres.