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GSMP-30 Ground Potassium Magnetometer /
Gradiometer System

Introduction
GSMP-30 is a high sensitivity
potassium magnetometer and gradiometer system, providing
unmatched sensitivity and absolute accuracy, in addition
to near zero orientation or heading error effect.
The GSMP-30 operates on principles
similar to other alkali vapour magnetometers such as the
Cesium magnetometer, but benefits from the unique
nuclear properties of Potassium.
The unmatched sensitivity of
GSMP-30 systems, allow the magnetometers and
gradiometers to be used for applications that demand
more sensitivity than other alkali vapour systems can
deliver.
Features
Some of the important benefits of
the GSMP-30 optically pumped magnetometer and
gradiometer systems include:
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almost no orientation errors
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highest sensitivity available
in a portable magnetometer
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best absolute accuracy
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fast start-up and recovery -
only seconds for the GSMP-30 to re-establish
oscillator lock after an orientation change from a
dead zone into the active zone
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fast tracking - the GSMP-30
measures precise Larmor frequency changes in
response to field changes of several thousand nT
within a sample period
GSMP-30 Advantages
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insensitivity to orientation -
virtually zero heading error result from the nuclear
properties of potassium
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sensitivity - inherent
potential sensitivity results from the nuclear
properties of potassium. The very narrow spectral
lines of potassium provide sensitivities that are
the highest among all optically pumped magnetometers
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absolute accuracy - the
GSMP-30’s unmatched absolute accuracy (a variance of
only ± 0.1 nT between any GSMP-30 sensors) makes
this sensor the best choice for all gradiometer
installations. Cesium's broad spectral lines
severely limit the determination of the absolute
accuracy of these systems
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no regular calibrations,
GSMP-30 sensors do not require periodic calibration
as the relative position of the RF exciting coil and
the optical axis, does not impact performance
Because of Cesium’s spectral line
configuration, the relative position of the RF coil and
optical axis is critical, impacting performance.
Mechanical vibrations alter the relative positions,
resulting in the need for regular calibrations or
balancing of the sensor.
GSMP-30 console
GSMP-30 Orientation Indifference
Advantage
Variations in heading or spin
error1 responses between individual sensors, lead to
errors in magnetic gradient measurements of the same
order of magnitude as gradients of interest. This fault
is manifested in magnetometer systems that feature
Cesium magnetometer sensor technology.
The GSMP-30 sensor, with virtually
no orientation or heading error, does not introduce
orientation "noise" into the magnetic or magnetic
gradient measurement and as a result, high system
sensitivity can be realized in both dynamic and static
environments.
Applications
The long term stability, high
sensitivity and fast response to the changing magnetic
field make the GSMP-30 ideal for a wide variety of
applications, such as:
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Ferrous ordnance location - for
the detection of ordnance and mines by portable
methods
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Ground portable magnetic and
magnetic gradient surveying - for archaeological
searches, engineering applications for detection of
buried drums containing hazardous wastes and mineral
and oil exploration
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Base station magnetic
monitoring for observing diurnal magnetic activity
and disturbances
GSMP-30 System Setup
A GSMP-30 magnetometer system is
comprised of:
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staff mounted sensor and RF
drive electronics / pre amplifier assembly
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data acquisition / display
console
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24 VDC battery belt and harness
GSMP-30 Sensor Head
The lightweight (less than 2.9 lbs)
GSMP-30 sensor head houses the electro-optical detection
system. All components of the sensor head, including the
outside plastic housing, are made of carefully screened,
nonmagnetic materials. The compact plastic housing has a
diameter of 3.5" and a length of 6.0", allowing the
GSMP-30 sensor to adapt seamlessly into existing
airborne, marine, portable and base station
installations. The electro-optical detection assembly
includes a potassium lamp and absorption cell and
photodetector, all housed in an insulated plastic
housing to reduce warm-up time and power consumption,
during survey operations.

GSMP-30 High Sensitivity Potassium Magnetometer Sensor
Assembly
GSMP-30 Data Acquisition Console
The GSMP-30 console is equipped
with a graphic display and a 16 key alphanumeric
keyboard. The graphic display is an 8 line (30
characters/line) reflective monochrome LCD that can also
display 30 x 8 characters. The console contains the
magnetometer's Larmor signal processing electronics, in
addition to providing data storage and retrieval
facilities and functionality to graphically review data
in real time and from system memory. All of the GSMP-30
system features, including optional, advanced navigation
features, are accessible through an easy to use,
interactive menu system.
Universal Gradiometer Staff
The GSMP-30G is supplied with a
universal staff (patent pending) that is uniquely
constructed, permitting the measurement of both vertical
and horizontal magnetic gradients, through the use of
the same apparatus. The staff's unique construction
assures that the angle between the magnetic field vector
and the sensor(s)'s optical axis is constant, regardless
of the sensor's elevations above the ground. This
important feature, reduces the problems of "drop outs"
that plague other alkali vapour magnetometer systems.
Optional GPS Navigation
Subsystem
In addition to providing support
for a variety of OEM GPS receivers integrated into the
GSMP-30 console, a GSMP-30 can accept data from other
GPS receivers in NMEA format, a standard which virtually
all receivers support.
All of the survey navigation
features provided with the integrated OEM GPS receiver
option are supported with external GSP receivers as
well.
An important benefit of the OEM GPS
receiver is that the magnetic interference generated by
the GPS subsystems is shielded from the sensitive
magnetometer sensors, by the GSMP-30 chassis.
Some of the GSMP-30 navigation
features include:
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real-time coordinate
transformation to UTM and local X-Y coordinate
rotations
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survey "lane" guidance , with
cross-track display and audio indicator
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user selectable (and user
defined) datums, such as the commonly utilized
WGS-84
Advanced GPS Integration
Features
The GSMP-30 data acquisition
console offers an unprecedented level of GPS
integration, if the console is fitted with an optional
32.0 Mb of FLASH memory for logging GPS raw ranges, and
supplied with optional firmware.
Similar to standard GSMP-30
firmware, GPS X-Y positions are captured and written
along with each magnetometer or gradiometer record.
However, the advanced GSMP-30 GPS
integration option provides the ability to write raw
ranges to a separate file in GSMP-30 memory, for DGPS
post processing.
GSMP-30 Sensor Specifications
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Sensitivity: 0.001 nT/ÖHz
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Absolute accuracy: ± 0.1 nT
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Dynamic Range: 10,000 to
100,000 nT
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Sample Rate: up to 20 readings
per second, programmable
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Heading Error: less than 0.1 nT
combined for sensor
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spins on all orientations from
10° to 80°
Environmental
Power Requirements
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Approx. 25 W at start up
dropping to approx. 8 W after warm up
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Power Consumption: 8 Watts
typical at 20°C
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Outputs: Continuous signals at
the Larmor frequency which is proportional to the
magnetic field
"Walking" Magnetometer /
Gradiometer
Aegis Instruments pioneered the
innovative "Walking" option that enables acquisition of
nearly continuous data on survey lines. The "Walking"
option is a standard feature of every GSMP-30. Similar
to an airborne survey in principle, data is recorded at
discrete time intervals (up to 20 readings per second)
as the instrument travels along the line. At each major
survey picket (fiducial), the operator touches a
designated key. The Walking Magnetometer automatically
assigns a linearly interpolated coordinate to all
intervening readings. A main benefit of the Walking
option is that the high sample density improves
definition of geologic structures. And because the
operator can record data on a near-continuous basis, the
Walking Magnetometer increases survey efficiency and
minimizes field expenditures -- especially for highly
detailed ground-based surveys.
Optional Omnidirectional VLF
With omnidirectional VLF option, up
to three stations of VLF data can be acquired without
orienting. Moreover, the operator is able to record both
magnetic and VLF data with a single stroke on the
keypad.
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Frequency Range: 15 - 30.0 kHz
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Parameters Measured: Vertical
in-phase & out-of-phase components as % of total
field. 2 relative components of horizontal field.
Absolute amplitude of total field
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Resolution: 0.1%
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Number of Stations: Up to 3 at
a time
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Sensor Dimensions: 140 x 150 x
90 mm(5.5 x 6 x 3")
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Sensor Weight: 1.0 kg (2.2 lb)
Theory of Operation
A typical alkali vapour
magnetometer consists of a glass cell containing the
evaporated alkali metal, which is exposed to light of a
specific wavelength.
According to quantum theory, in
every population of alkali atoms, there is a set
distribution of valence electrons between two energy
levels, represented by 1 and 2 in the figure below.
A wavelength of light is applied to
the cell to excite electrons only from level 2 to level
3. This is called polarization. As the number of atoms
with electrons at level 2 decreases, the cell will stop
absorbing light, and will turn from opaque to
transparent.
Electrons at energy level 3 are not
stable, and will spontaneously decay back to levels 1
and 2. Eventually, level 1 will become fully populated,
and level 2 will become depopulated, and the cell will
be completely transparent. That’s where RF
depolarization comes into play. RF power of a wavelength
that corresponds to the energy difference between levels
1 and 2 is applied to the cell to move electrons from
level 1 back to level 2.
The significance of this act is
that the energy difference between levels 1 and 2 (the
frequency of the RF depolarizing field) is proportional
to the magnetic field.

The entire weight of the GSMP-30G
staff & sensor assembly
is suspended by 2 attachments to
the backpack
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