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Seismic
Sensors
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The Integrated Seismic System (ISS) can be based on any
combination of geophone, accelerometer and force balance accelerometers,
in uni-, bi- and tri-axial combinations. Each sensor type has different
advantages in terms of amplitude range, frequency range, reliability
and cost. The tri-axial configuration affords the most accurate
estimates of source parameters. An ISS International systems engineer
would be happy to discuss the sensors and configurations best suited
to your application - so please contact us at your convenience.

Tri-axial geophone
click to view enlargement

Tri-axial geophone
with integrated
waterblock cable
click to view enlargement
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Geophones are usually the sensor of choice
in most mining applications, because of the low cost, large bandwidth
and excellent reliability. ISSI routinely manufactures two kinds
of geophones, with natural frequencies of 4.5Hz and 14Hz. The 4.5Hz
geophone has a usable frequency bandwidth of between 3Hz and 2000Hz
but must be installed to within 2 degrees of it's pre-set orientation
with respect to the vertical. The 14Hz geophone is omni-directional
and can be installed at any angle, with a usable frequency bandwidth
of between 10Hz and 2000Hz.
Accelerometers are usually used where high-precision
records of high-frequency events are demanded. The accelerometer
that ISSI manufactures has a bandwidth of between about 0.2Hz and
2300Hz, with an extremely low intrinsic noise level.
Please download the PDF
for more information.
Non-seismic Sensors
Any sensor with a slowly varying output which
may be conditioned between -5V and +5V or 4mA and 20mA may be monitored
as part of the ISS. Strain meters, creep meters, tilt meters, CSIRO
cells and thermometers have all been successfully employed.
This page last updated: January
2007
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