GSMP-30A Potassium "SuperSenser" Magnetometer /
Gradiometer Airborne System

Potassium
"SuperSenser" is the most advanced airborne sensor on the market today.
To address industry requirements, Terraplus introduced "SuperSenser" -
the highest resolution magnetometer / gradiometer airborne system
available. The SuperSenser (GSMP-30A) is based on a unique optically
pumped Potassium sensor - a technology that offers an order-of magnitude
increase in resolution over other systems. It also provides:
- Reduced "heading" errors
- Highest absolute accuracy
- Decreased maintenance costs
It offers a number of benefits for fixed wing and towed survey
configurations, including:
- Highest sensitivity (i.e. highest signal-to-noise) for enhanced
resolution of geological and cultural features in a variety of
applications.
- Highest absolute accuracy (varying by no more than +/- 0.1 nT
between sensors)
- Negligible orientation (heading) errors
- Faster sampling
- Insensitivity to microphonics
- Lowest maintenance (no re-alignments)
As well, Terraplus offers advanced base station capabilities, such as:
- Potassium & Overhauser
- 3 modes for flexible base station scheduling
- GPS option for precise time synchronization with onboard GPS
The worldwide application of airborne magnetic and gradiometric data is
growing -- driven by the increasing demand for high-resolution, low cost
data to:
- Map targets, geology and geological structures in mineral
exploration
- Perform frontier evaluation and augment seismic data in hydrocarbon
exploration
- Detect Unexploded Ordnance (UXO)
- Map pipelines and other cultural objects in environmental and
engineering investigations
Key Components
The SuperSenser technology comprises:
- Sensor head
- Radio Frequency (RF) pre-amplifier and drive electronics module
- Cable (1 to 10m - standard 4m) to separate sensor and electronics
for noise elimination
- Optional signal processor / console and cable
Optically
pumped Potassium SuperSenser (GSMP-30A) sensor and cable. Can also be
configured with additional sensors for Gradiometer readings
The sensor deploys as a single unit, or in combination with other sensors
for magnetic gradient measurements. The GSMP-30 can also be deployed in
a multi-sensor configuration for gradient and total field magnetic
measurements. As shown above, four Potassium units can be installed in a
special “bird†with two fins at the tips of an imaginary tetrahedron to
allow for measurement of Total Magnetic Field and the gradients in three
directions:
- Vertical gradient
- Horizontal gradient (along-the-track)]
- Horizontal gradient (across-the-track)
Horizontal gradient measurements are increasingly popular for providing
details about the lateral extent of subsurface anomalies located between
survey lines. Vertical gradients can assist significantly in identifying
geologic / structural contacts and near-surface targets (such as UXO).
In the example above (main pictures above), we show the system deployed
in a fixed wing “stinger†implementation for acquisition of high
resolution Total Magnetic Field data.
Implementing your solutions

The
GSMP-30A system can be interfaced either to the signal processing
console which provides 32 MBytes of memory for data acquisition, or to
other recorders and data acquisition systems. We can provide technicians
to facilitate set up for:
- Installation assistance for "fixed-wing" or "stinger" configurations
- Custom "bird" design and development for "towed" configurations
- Conversion of output voltages into corresponding frequency and
magnetic field values
- Electronics interfacing to on-board recording and navigation systems
Airborne Base Station Configurations
Another area of application for advanced magnetometers is in airborne base
station monitoring. Our customers have the choice of working with
GSMP-30A or
Overhauser (GSM-19) units. The
GSMP-30A implementation offers advantages for surveys where very high
resolution diurnal corrections are needed.
GSM-19 also delivers good resolution and economical pricing. Both
implementations share a number of advanced features (introduced in
version 6.0 firmware release), including:
- Precise time synchronization of field and base station units using a
built-in GPS option. This capability is particularly important for
working in noisy magnetic conditions and provides the highest accuracy
possible.
- Flexible scheduling (up to 30 on / off periods). Simply define a
series of intervals and the base station will turn itself on as you
need. This mode provides the greatest flexibility for longer surveys
where leaving your base station on increases efficiency. Immediate start
and daily modes are also provided.
Benefiting from the Natural Properties of Potassium Optical Pumping
With more than a decade of experience with Potassium technologies, we feel
confident that your next survey will benefit in many ways, including
acquisition of:
- Highest sensitivity data (reflecting Potassium spectrum
characteristics and high natural frequency of 7 Hz/nT)
- Highest absolute accuracy (a variation of only +/- 0.1 nT between
sensors makes the GSMP-30A an ideal choice for gradiometer
installations)
- Data with minimal heading errors (reflecting the insensitivity of
Potassium to aircraft / bird orientation)]
- Data that is not affected by phonics (low frequency vibration in the
audio range)
Maintenance costs are minimal in comparison with other systems as key
components can be replaced in the field.
SuperSenser Specifications
Performance
| Sensitivity: |
|
0.001 nT @ 20 readings / sec |
|
Resolution: |
|
0.0001 nT |
| Absolute Accuracy: |
|
+/- 0.1 nT |
| Dynamic Range: |
|
10,000 to 120,000 nT |
| Gradient Tolerance: |
|
Over 2000 nT/m |
| Sampling Rate: |
|
up to 20 readings / sec |
Orientation
| Sensor Angle: |
|
Optimum angle 30° between sensor head axis & field vector. |
| Orientation: |
|
10° to 80° & 100° to 170° |
| Heading Error: |
|
< 0.1 nT between 10° to 80° and 360° full rotation about axis. |
Dimensions & Weights
| Sensor: |
|
89mm diameter. x 152mm length, and < 1.3 kg |
| Pre-amplifier: |
|
30.6cm x 8.5cm x 7.5cm, and 1.6 kg |
Power
| Power Supply: |
|
18 to 35 V DC |
| Power Requirements: |
|
Approx. 25 W at start up, dropping to 8 W after warm-up |
|
Power Consumption: |
|
8 W typical at 20°C |
|
Warm-up Time: |
|
<15 minutes @ -40°C |
Environmental
| Operating Temperature: |
|
-40°C to +55°C |
| Storage Temperature: |
|
-70°C to +55°C |
| Humidity: |
|
0 to 100%, splashproof |
Outputs
Cycled measurements of the Total Magnetic Field with position & time as
digital readout or graph form on the console or as ASCII format through
an RS-232 COM port. Pre-amplifier outputs are continuous signals at the
Potassium Larmor frequency which is proportional to the magnetic field
(7 Hz/nT).
Components
Sensor, pre-amplifier box, 4m sensor / pre-amplifier cable, manual & ship
case.
Optional pre-amplifier to signal processor cable (1.0 to 100.0m)
Ordering Information
| Description |
|
Order Number |
| GSMP-30A |
|
28MAR02-CDN-MS |