A.2 Applicable Bill of Materials ........................................................................... A-1
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Introduction
General Description
1
Section 1
Introduction
1.1 General Description
The 943 series Gamma Scintillation Detectors consist of an integral gamma sensitive Nal crystal, a photo
multiplier tube, a preamplifier assembly, and various interconnecting cables for connecting the detector,
readout, and power supply. Refer to Figure 1-1 for a general view or to Appendix A for each specific
detector. All are functionally identical. The size of the crystal employed, the housing material, and whether
or not an Americium source is included in the assembly are the only differences. All photomultiplier
tube/crystal assemblies are an integral line construction.
The 943 series Gamma Scintillation Detectors are designed to be sensitive to gamma radiation. The
Gamma Scintillation material photomultiplier tube and preamplifier are contained within a cylindrical
housing. This assembly provides protection from the environment, and provides a mechanism for
installation without damaging the detector assembly.
When gamma or x-rays enter the scintillation crystal, pulses of light are emitted. The light pulses striking
the photocathode of the photomultiplier tube excites the electrons in the cathode to a high-energy state
causing them to escape from the surface of the cathode. The freed electrons are attracted by a voltage
potential to the first dynode of the photomultiplier tube. This starts a cascading effect where a charge is
passed from dynode to dynode increasing in size at each stage until a shower of electrons is passed on
to the preamplifier.
The preamplifier provides pulse conditioning and cable driving capabilities to match the input
characteristics of the Victoreen Universal Digital Ratemeter or the 960 Digital Radiation Monitoring
System (DRMS), used to monitor the detector output. The detector is supplied with an 8-foot coaxial cable
that normally terminates in a junction box supplied as a part of a complete monitoring channel.
1.2 Applications
The 943 series Gamma Scintillation Detectors may be used with Victoreen digital ratemeters or with the
960 Digital Radiation Monitoring System (DRMS). Ratemeters are used in systems where individual
control room readouts are employed, while the 960 DRMS is used when a complete digital system is
supplied.
1.3 Detector Variations
Model 943-35
The 943-35 Gamma
sodium iodine (Nal) crystal/photomultiplier tube assembly and preamplifier, enclosed in a stainless steel
housing. The stainless steel housing completely encloses the scintillator and is used where direct contact
with the process is required. The response of the detector is slightly less than the 943-36 detector, due to
the 0.045 inch thick housing.
Scintillation Detector Consists of an integral 1.5 inch diameter by 1.0 inch thick
1-1
Page 6
Victoreen 942-35,943-36,943-36H, 943-37,943-237A
Operators Manual
Model 943-36
The 943-36 Gamma Scintillation Detector consists of an integral 1.5 inch diameter by 1.0 inch thick
sodium iodine (Nal) crystal/photomultiplier tube assembly and preamplifier, enclosed in a stainless steel,
housing. The aluminum crystal housing protrudes through the process end of the detector for maximum
efficiency. The detector is normally used for monitoring of radioactive iodine, or in liquid process monitors,
where the detector is protected from the process by a stainless steel well that is part of the detector shield
assembly. The well is provided separately.
Model 943-36H
The 943-36H is similar in construction to the 943-36, and is modified to operate at process temperatures
of up to 160°F with less than a 10% decrease in output at low photon energies (below 662 keV), and less
than a 5% decrease in output at high energies (662 keV and above). This detector is recommended for
use in applications where the process temperature is above 120°F.
Model 943-37
The 943-37 Gamma Scintillation Detector consists of an integral 2.0 inch diameter by 2.0 inch thick
sodium iodine (Nal) crystal/photomultiplier tube assembly and preamplifier, enclosed in a stainless steel
housing. The stainless steel housing completely encloses the scintillator and is used where direct contact
with the process is required. The 2 inch crystal provides more sensitivity to both ambient and process
radiation than the 943-35 or 943-36 detectors, and is used in applications where low ambient background
radiation is anticipated.
Model 943-237
The 943-237A Americium Detector contains a small capsule of Americium 241, which is inserted in the
sodium iodine (Nal) crystal. The function of the Americium is to provide a high-energy pulse output for
regulation of the high voltage power supply under conditions where fluctuations in the process
temperature are expected, or where pulse height spectrometry is desired. The americium-doped
detectors are designed to be used in conjunction with the 960AM series Americium Regulator Module or
the 942-200-90 SCA/Americium Regulator board for dynamic regulation of the detector high voltage.
Americium 241 is selected as the source of calibrating energy for the regulated detector, because the
equivalent energy level of the pulse (approximately 5.4 MeV) is relatively distant from that of the isotopes
normally being monitored.
1.4 Specifications
The 943 series Gamma Scintillation Detectors have been assembled with parts selected for the high
reliability required in nuclear applications. Unauthorized repairs made to the detector will void the
warranty and may affect the nuclear qualification. The detectors should be returned to Fluke Biomedical
for authorized, qualified (ANSI 45.2.6, Skill Level II) service or repair.
The following detector models are no longer
manufactured, and may be replaced as shown
below.
Obsolete Model Description Replacement
943-38 2 x 2 in crystal, carbon steel housing 943-37
943-238A 2 x 2 in crystal, carbon steel housing, with Americium 943-237A
NOTE
1-2
Page 7
Detector
Dimensions943-35: 9.5 x 2.5 in (24.1 x 6.4 cm) 943-36, 943-36H: 9.5 x 2.5 in (24.1 x 6.4 cm)
943-37, 943-237A: 10.5 x 2.5 in (26.7 x 6.4 cm)
Weight Approximately 3 lbs (1.4 kg)
Housing Material Stainless Steel
End Window Material 943-36, 943-36H: Aluminum
943-35,943-37, 943-237A: Stainless Steel
Photomultiplier Tube 2 inch photocathode, 10-stage, integral crystal
Crystal Size 943-35, 36, 36H: 1.5 in diameter x 1 in thick
Operating Temperature 32° to 122°F (0° to 50°C), (160°F for 943-36H)
Storage Temperature 32° to 122°F (0° to 50°C), (160°F for 943-36H)
Relative Humidity 0 to 95% non-condensing
1.5 Functional Description
Refer to Figure 1-1 for aid in understanding the functional description.
Figure 1-1. Typical Model 943-36 Series Gamma Scintillation Detector (Not Drawn To Scale)
Gamma or x-rays that have enough energy to penetrate the crystal or outer housing and interact with the
Nal crystal scintillator, will produce light pulses proportional to the energy deposited in the scintillator. A
photomultiplier tube, optically coupled to the scintillator detects visible light emitted and converts this light
into pulses of electrical energy, whose voltage is proportional to the energy deposited. The electrical
pulses are sent to the preamplifier in the detector housing.
Outer Housing
The preamplifier circuit amplifies the pulses received from the photomultiplier tube/scintillator assembly
with a fixed gain of six (6). The current drive output of the preamplifier circuit will drive a 50 ohm
transmission line up to 1500 feet without degradation of the signal.
Should a very high intensity radiation source be detected, the photomultiplier tube may become saturated.
That is, visible light from successive photon collisions within the scintillator may occur so often that they
are essentially continuous. This would have the effect of holding the output voltage of the preamplifier at a
relative constant output voltage. Since the readout is designed to count pulses that represent individual
particle collisions, a high intensity signal could be interpreted as a low or no radiation condition. The
readout device should include an overrange setpoint of 2E7 CPM that will result in the display of an
overrange error message instead of a radiation value. Although the actual radiation value will not be
displayed under this extreme condition, it will prevent misrepresentation of the radiation value during
overrange conditions.
Integral Sodium Iodine (Nal) Crystal/Photomultiplier Tube
The Nal crystal and photomultiplier tube are supplied as an integral assembly within the detector housing.
The Nal crystals used in the detector are single crystal elements. They are hermetically sealed into a
metal can with an optical window on one end of the can to permit the light pulses to escape the crystal.
The interior of the can is lined with a highly reflective media to enhance the collection of light.
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Introduction
Functional Description
The Nal crystal is optically coupled to the photomultiplier tube so that light pulses occurring in the crystal
are visible to the photocathode of the photomultiplier tube. The electrons in the photocathode become
excited by the light, resulting in emission of electrons from the surface of the photocathode. The voltage
potential differences in the dynode network start a cascade of electrons, which, upon reaching the anode,
become a pulse of current. The anode collects this pulse and makes it available to the preamplifier.
1
Preamplifier
The preamplifier provides amplification of the output from the photomultiplier tube and cable driving
capabilities. Operational amplifier Z1 is configured to provide a voltage gain of 6 for the output of the
photomultiplier tube. Transistors Q1 and Q2 provide cable-driving capability for up to 1500 feet of cable.
Using the detector as typically set up by the Fluke Biomedical calibration process, the output of the
photomultiplier tube produces a negative pulse from approximately 200 millivolts to 6 Volts, corresponding
to an 80 keV to 2 MeV photon energy range. This signal is amplified to a 12 Volt negative pulse at the
emitter of Q2, which is coupled to the cable by capacitor C6.
The combination of impedance matching resistor R11 and the termination resistor in the readout (ideally
50 ohms) results in a received pulse with a pulse height proportional to incident energy.
1.6 Receiving Inspection
Upon receipt of the package:
1. Inspect the cartons (s) and contents for damage. If damage is evident, file a claim with the carrier
and notify Fluke Biomedical, Radiation Management Services at 440.248.9300.
2. Carefully remove the contents from the packing material. The crystal end is fragile.
3. Verify that all items listed on the packing list have been received and are in good order.
NOTE
If any of the listed items are missing or damaged,
notify Fluke Biomedical.
1.7 Storage
Instruments storage must comply with Level B storage requirements as outlined in ANSI N45.2.2 (1972)
Section 6.1.2(.2). The storage area shall comply with ANSI N45.2.2 (1972) Section 6.2 Storage Area,
Paragraphs 6.2.1 through 6.2.5. Housekeeping shall conform to ANSI N45.2.3 (1972).
Level B components shall be stored within a fire resistant, tear resistant, weather tight enclosure, in a
well-ventilated building or equivalent.
Instrument storage must comply with the following:
1. Inspection and examination of items in storage must be in accordance with ANSI N45.2.2 (1972)
Section 6.4.1.
2. Requirements for proper storage must be documented and written procedures or instructions must
be established.
3. In the event of fire, post-fire evaluation must be in accordance with ANSI N45.2.2 (1972), Section
6.4.3.
4. Removal of items from storage must be in accordance with ANSI N45.2.2 (1972), Sections 6.5 and
The equipment described in this manual is intended to be used for the detection and measurement of
ionizing radiation. It should be used only by persons who have been trained in the proper interpretation of
its readings and the appropriate safety procedures to be followed in the presence of radiation.
Although the equipment described in this manual is designed and manufactured in compliance with all
applicable safety standards, certain hazards are inherent in the use of electronic and radiometric
equipment.
WARNINGS and CAUTIONS are presented throughout this document to alert the user to potentially
hazardous situations. A WARNING is a precautionary message preceding an operation that has the
potential to cause personal injury or death. A CAUTION is a precautionary message preceding an
operation that has the potential to cause permanent damage to the equipment and/or loss of data.
Failure to comply with WARNINGS and CAUTIONS is at the user’s own risk and is sufficient cause to
terminate the warranty agreement between Fluke Biomedical and the customer.
Adequate warnings are included in this manual and on the product itself to cover hazards that may be
encountered in normal use and servicing of this equipment. No other procedures are warranted by Fluke
Biomedical. It shall be the owner’s or user’s responsibility to see to it that the procedures described here
are meticulously followed, and especially that WARNINGS and CAUTIONS are heeded. Failure on the
part of the owner or user in any way to follow the prescribed procedures shall absolve Fluke Biomedical
and its agents from any resulting liability.
Indicated battery and other operational tests must be performed prior to each use to assure that the
instrument is functioning properly. If applicable, failure to conduct periodic performance tests in
accordance with ANSI N323-1978 (R1983) Radiation Protection Instrumentation Test and Calibration,
paragraphs 4.6 and 5.4, and to keep records thereof in accordance with paragraph 4.5 of the same
standard, could result in erroneous readings or potential danger. ANSI N323-1978 becomes, by this
reference, a part of this operating procedure.
1-6
Page 11
2.1 Installation
Operation
Installation
2
Section 2
Operation
Ensure all power is removed prior to installing the
943 Series Detector.
If the detector is used in a process monitoring
system, refer to the applicable system manual for
all applicable system drawings and special
mounting instructions. Electrical and mechanical
drawings for the detector are provided in Appendix
A.
The detector is designed for use in a number of process monitoring configurations in a number of
Victoreen sampler assemblies. Installation is system dependent. Installation will generally consist of
mounting the detector in the desired configuration, performing electrical interconnections, and performing
any system testing which may be required. Refer to the applicable system manual for installation
instructions for the sampler assembly supplied.
1. Install the detector into the desired mounting location (refer to the Appendix A, the readout manual,
or the system manual for specific mounting details).
2. Set the high voltage potentiometer to its lowest setting (not required if the detector and readout
were factory calibrated prior to shipment).
3. Connect the appropriate cables between the detector and the readout.
Do not exceed 1200 VDC @ 500 μA to the detector
under any circumstances. Failure to comply will
result in damage to the detector.
4. If the detector is part of a radiation monitoring system, turn on channel power and verify the high
voltage is set to the value indicated on the factory calibration sheet. If the detector is a replacement
part, turn on channel power and slowly increase the high voltage until a count rate of approximately
3000 CPM is achieve (this count rate assumes that the detector is in open air and that the
discriminator threshold is set at 0.2 VDC in the readout). If the detector is placed within a lead
shield, the high voltage should be increased until a count rate of approximately 100 CPM is
achieved.
5. Allow a one-hour warm-up before proceeding to calibration.
A brief review of gamma radiation is necessary to understand the absorption processes that are inherent
to the operation in the spectrometer mode. This consideration is necessary because in practical
applications, not all of the energy of the incident photon is given up in every case. There are three
absorption processes: Compton scatter, pair production, and photoelectric process.
Compton scatter is a process where penetrating photons are scattered by the electrons that are in the
crystal. In this process, part of the energy is given up to the electron and part is retained by the photon.
The ratio of retained energy to that given off is dependent on the angle of collision. The electron will give
rise to secondary ionization of somewhat less total energy than the energy of the incident photon. The
lower energy output is generally referred to as Compton smear or scatter, most common at intermediate
photon energies.
Pair production is a process where the photon gives up energy to create an electron-positron pair. This
requires minimum energy of 1.02 MeV since it is a transformation of kinetic energy into mass. Photo
energy in excess of 1.02 MeV appears as kinetic energy of the electron and positron. The energy is
absorbed by the Nal crystal through ionization. The positron, being unstable in the presence of electrons,
will annihilate, causing two photons with 0.51 MeV each. Either of these photons may be absorbed
through the photoelectric process, through Compton scatter, or escape the crystal. In practice, pair
production becomes evident with incident photons above 2 MeV.
In the photoelectric process, all of the photon's energy is given up to one electron within the Nal crystal.
The charged electron will have a short ionization path within the crystal resulting in a light output that is
directly proportional to the incident radiation energy. This process permits using the detector to identify
the energy level of the incident gamma ray. With many isotopes, isotopic identification can be performed
using information derived from the gamma ray.
Photons derived from various sources, whether radioactive or visible light, impinge on the metal shield at
the front of the detector. Any photons containing energy less than a specific value (approximately 20 keV)
are highly attenuated by the shield. The remaining high-energy photons penetrate the shield and interact
with the Nal crystal, causing a pulse of light to be produced. The amount of light emitted is proportional to
the energy of the absorbed photon. The crystal is optically coupled to a 10-stage photomultiplier tube
(PMT). The light produced from the crystal is seen by the photocathode in the PMT. The cathode is
excited by the light and emits electrons from its surface. A string of 10 Dynodes in the PMT, at
sequentially increasing potentials, causes a cascade effect that delivers a shower of electrons at the
anode of the PMT. This appears as a negative pulse, proportional to the energy of the original photon. By
varying the PMT high voltage, the gain of the detector and output pulse height may be set to achieve a
specific output, based upon the isotope and activity of the incident radiation.
The 943 series Gamma Scintillation Detector requires no routine maintenance. Periodic verification of the
high voltage and discriminator setting supplied by the readout device, however, is recommended. If the
detector requires repair, the following assembly/disassembly procedure is to be used.
Ensure all power is removed prior to disassembly of
the 943 Series Detector.
Detector Disassembly
If additional information is required, refer to the
assembly drawing in Appendix A.
1. Disconnect the cable from the readout device.
2. Remove the four flat head hex screws from the detector sleeve (connector end).
3. For the 943-35, 943-37, and 943-237A detectors, using the detector cable, gently pull the detector
end plate, preamp, and photomultiplier/crystal assembly out from the detector sleeve. The
photomultiplier/crystal assembly may then be removed from its socket for replacement and/or the
preamplifier circuit board may be repaired.
4. For the 943-36 and 943-36H detectors, the crystal assembly must be separated from its socket
while removing the detector end plate. This may be accomplished by applying a slight rocking
motion while gently pulling on the detector cable.
To remove the photomultiplier/crystal assembly, the RTV used to seal the front end of the detector
must be removed to expose and remove the 38-34 outer retaining ring. Next, the 38-35 crystal
retaining ring and 843-36-51 crystal mounting with o-ring may be removed, followed by the 38-34
inner retaining ring. The photomultiplier/crystal assembly may then be removed for replacement.
CAUTION
NOTE
Use extreme care when removing the detector
preamplifier and photomultiplier assembly to
prevent damage to these delicate components.
5. The o-rings in the assembly may be remove with a small screwdriver, using care not to damage the
If additional information is required, refer to the
assembly drawing in Appendix A.
1. Prior to assembly, inspect the following parts for damage:
All
P/N 46-35 Detector end plate o-ring
P/N 843-133-4 Detector crystal cushion
943-35
P/N 843-35-6 PMT alignment spacer
P/N 46-20 o-ring
943-36 & 943-36H
P/N 38-34 Inner/outer mounting rings
P/N 38-35 Crystal retaining ring
P/N 843-36-51 Crystal alignment mounting ring
P/N 46-73 o-ring
2. Lightly lubricate the 46-35 rear end plate o-ring with o-ring grease (MST-3306 or equivalent) and
install on end plate.
3. For the 943-36, 943-36H, 943-37, and 943-237A detectors install the PMT/crystal assembly into the
socket and insert the PMT/crystal and preamplifier assembly into the sleeve, ensuring the four
screw holes on the sleeve are aligned with the end plate holes.
4. For the 943-35 detector, install the PMT/crystal assembly into the socket assembly. Re-install the
P/N 843-35-6 PMT alignment spacer over the crystal, sliding it up to the PMT housing. Lightly
grease the P/N 46-20 o-ring and install in the groove provided on the crystal housing. This will
ensure proper alignment of the PMT/crystal assembly in the sleeve. Insert the PMT/crystal and
preamplifier assembly into the sleeve, ensuring the four screw holes on the sleeve are aligned with
the end plate holes. Press fit the unit together with moderate hand pressure.
5. Re-install the four screws on the base of the detector.
6. For the 943-36 and 943-36H detectors only the crystal retainers at the front of the detector must be
re-installed. First, re-install the P/N 38-34 inner retaining ring in the groove provided on the detector
sleeve to retain the PMT. Next, lightly grease P/N 46-73 o-ring and install in the groove provided on
the P/N 843-36-51 crystal alignment mounting ring. The P/N 38-35 retaining ring is then installed in
the groove provided on the crystal housing to properly position the crystal in the mounting ring. The
P/N 38-34 outer retaining ring is then installed in the outer sleeve groove to properly position the
complete assembly. The assembly is completed by filling in the entire area between the crystal and
the sleeve with RTV (MST-4341, GE #167, or equivalent) to prevent ambient air leakage path
through the detector.
7. Reconnect the detector cable to the readout device.
8. Detector is now ready for calibration.
4-2
Page 17
Maintenance, Calibration, and Troubleshooting
Calibration
4
4.2 Calibration
The 943 series Gamma Scintillation Detector is factory calibrated and is shipped with a calibration data
sheet. It is usually shipped as part of a monitoring system and the ratemeter or scaler (960 DRMS)
module high voltage supply, upper and low discriminator are adjusted for a specific response over the
entire operating range. With the factory calibration, a dead time correction factor (Tau) is also provided.
At regular intervals after initial installation of the detector, if the detector is replaced, if a dramatic change
in detector output is noticed, or if the power supply output voltage changes, calibration should be
repeated.
NOTE
The count rate will increase and decrease in
conjunction with detector and pulse height voltage.
If the high voltage reaches 1000 VDC without
137
achieving the necessary
Cs pulse height, suspect
a defect in the detector, wiring, or readout device.
The 943-series Gamma Scintillation Detectors are calibrated by adjusting the high voltage supply to the
photomultiplier tube (adjusting photomultiplier tube gain based on the photons that impinge on the Nal
scintillator).
The detector provides a linear output for all levels of gamma radiation. Although the output is essentially
linear, at high counting rates the dead time of the crystal and preamplifier combination causes pulses that
are produced at the same time or very nearly the same time to appear as one pulse, reducing the actual
pulse output of the detector. Linearity can be improved by using a dead time correction. In digital systems,
an algorithm automatically compensates for dead time based on an operator-entered constant. Setting
the detector for the proper output count rate at any point in its operating range assures an accurate
measurement at any other point.
Victoreen detectors are factory calibrated to provide a fixed output count rate and pulse height over an
energy range of 60 keV to over 2 MeV. All Victoreen Primary calibrations are based on detectors that are
set-up to provide the same gain, using a master set of button sources and a standard geometry fixture
retained permanently at Fluke Biomedical. This permits the use of secondary, or transfer button sources,
to reset the high voltage (i.e. re-calibrate) in the field to obtain the same detector efficiency used in the
original detector/sampling geometry primary isotopic calibrations. Transfer button sources and standard
geometry fixtures are normally provided with Victoreen radiation monitoring systems. The factory
calibration procedure is contained in the each applicable system manual.
Calibration Where Calibration Data and Button Sources are Available
Calibration of the gamma scintillation detector requires a standard button source (s) of known gamma
activity and P/N 844-36 standard geometry. The button source is used to reproduce a known count rate
using the standard geometry.
The standard geometry is used to consistently position the detector and button source with respect to
each other. The detector should be connected to the readout device with the cable that will be in place
during normal operation (high voltage setting is slightly cable dependent). At the readout device set the
discriminator level to the level indicated on the calibration data sheet (normally 0.2 VDC).
1. Insert the detector into the cavity provided in the standard geometry. Allow detector to warm up for
approximately 1 hour.
2. Determine the background count rate by allowing the detector readout device to run for ten
minutes. Record this rate on the calibration data sheet. The following Max count rates should be
displayed on the readout device (detector dependent):
Ba button source (P/N 844-36-15), blank side up in the slide drawer of the standard
geometry, and insert drawer into geometry.
4. The expected count rate for the button source should be determined. It is recorded on the factory
calibration data sheet. Correction must be made for decay. (The half-life of the source is 10.74
years).
133
5. Run a 2-minute count (10,000 CPM minimum), using the
Ba source.
6. Adjust the high voltage power supply to the detector so that the net count rate corresponds to the
expected count rate calculated in step 4. (Net count rate is indicated count rate minus background
count rate). A ± 2% tolerance is acceptable.
7. The count rate will increase and decrease in conjunction with the high voltage setting. If the high
voltage reaches the maximum allowable setting without achieving the necessary count rate,
suspect a defect in the detector, wiring or readout device.
8. If additional button sources were provided, repeat step 5 for each source. A 6% tolerance is
acceptable.
133
9. If the above sources are not within ± 6%, the gain may be incorrectly set on the 356 keV
133
photopeak and not on the 80 keV
Ba photopeak. Using a
and adjust the high voltage so that the
137
Cs photopeak is at approximately 2.3 Volt average (1.65
137
Cs source and an oscilloscope, verify
Ba
Volts for Americium regulated detectors). Step 6 should then be repeated being sure to adjust the
high voltage in the negative direction only.
Calibration Without Transfer Button Sources
In the event secondary transfer sources are not available, the detector high voltage may be set to the
value stated on the calibration data sheet by using a
137
height of the
Cs photopeak is approximately 2.3 Volts, at the high voltage stated on the calibration data
sheet, and may be checked to determine proper detector alignment. Without a set of secondary sources,
however, the overall detector response in terms of counts per minute, μCi per cm
the user's primary calibration.
137
Cs source and an oscilloscope. The average
3
must be determined by
4.3 Troubleshooting
Extreme care must be used when troubleshooting a
system that has power applied. All standard
troubleshooting precautions apply.
Extreme care must be used when troubleshooting
in close proximity to the high voltage output.
Once a problem has been located, remove all
power before continuing with the repair.
4-4
WARNING
WARNING
WARNING
Page 19
Maintenance, Calibration, and Troubleshooting
Troubleshooting
4
CAUTION
Personnel performing the following procedure must
be familiar with the operation of the monitoring
system and the location of each piece of equipment
used in the system.
Troubleshooting is indicated for the detector when the measured output of the check source or other
gamma source shows a marked increase or decrease in the number of counts observed at the readout
while high voltage has remained constant. Check for any visible signs of malfunction. To troubleshoot the
system, refer to the applicable drawings located in Appendix A. Insure that all electrical connections are
correct. If necessary, refer to the wiring diagrams for electrical connections.
Verify ± 15 VDC and detector high voltage are present at the detector cable termination point. If the
above voltages are present, and no output pulse exists, a failure in the detector preamplifier or
photomultiplier tube is suspected. Any fault that cannot be isolated to the detector must be in the wiring to
the readout or the readout itself. Consult the readout manual for troubleshooting procedures pertaining to
the readout.
Refer to cable connector pin outputs below for pin and function:
Pin Function
A High Voltage
B High Voltage Shield
C Signal (negative pulses)
D Signal Shield
E +15 VDC Supply
F -15 VDC Supply
G Power ± 15 VDC Ground
If the detector is determined to be at fault, it must be sent back to Fluke Biomedical for repair or repaired
by a technician qualified to ANSI 45.2.6, 1978, Skill Level 2.
NOTE
If a problem cannot be resolved by applying the
calibration or troubleshooting procedures described
above, contact Fluke Biomedical at 440.248.9300
for assistance.
Dynode Test Measurement
NOTE
The photomultiplier tube must be removed from the
detector tube socket during this test.
1. Turn off channel power at the readout device.
2. Disassemble the detector according to the instructions provided in "Detector Disassembly".
4-5
Page 20
Maintenance, Calibration, and Troubleshooting
Troubleshooting
CAUTION
Preamplifier input is easily damaged. Ground pin 3
of Z1 before applying power and measuring
photomultiplier tube anode or dynode voltage.
3. Using a DVM, measure the total DC resistance of the dynode string. The value should be 9.67
megohms ± 15%. If no reading is obtained, check dynode resistor interstage connections.
4. Connect the cable to the readout device.
5. Turn on channel power and apply 900 Volts to the detector. Measure the anode resistor voltage
(R13) using an electrostatic voltmeter. The value should be 900 Volts.
6. Remove channel power.
NOTE
If the "Preamplifier Check-out" is to be performed,
omit step 7.
7. Reassemble the detector according to the instructions provided in "Detector Assembly".
Preamplifier Checkout
CAUTION
The high voltage must be removed for this test.
NOTE
If the "Dynode Test Measurement" was performed,
omit steps 1 and 2.
1. Turn off channel power at the readout device.
2. Disassemble the detector according to the instructions provided in "Detector Disassembly".
3. Remove the grounding jumper from pin 3 of Z1.
4. Connect an oscilloscope to the input circuitry of the readout (50 ohms terminated).
5. Turn on channel power.
6. Using a pulse generator, inject negative pulses of 0.50 Volts amplitude, 1 μs pulse duration, at a
frequency of 1 kHz, to the node of R13 and C6 (+) and ground (-).
7. Output pulses should be -1.6 VDC ± 20% amplitude. If pulses are not present, check Z1 and
associated circuitry.
If the preamplifier and dynode tests are positive, the detector malfunction is probably in the
photomultiplier tube. Remove all power, replace the photomultiplier tube and reassemble the detector
according to the instructions provided in "Detector Assembly".
4
4-5
Page 21
Appendix
Applicable Drawings and Bill of Materials
Appendix A
Applicable Drawings and Bill of Materials
A.1 Applicable Drawings
Drawing Number Description
943-35-5 Gamma Scintillation Detector Assembly
943-36-5 Gamma Scintillation Detector Assembly
943-36H-5 Gamma Scintillation Detector Assembly
943-37-5 Gamma Scintillation Detector Assembly
943-237A-5 Gamma Scintillation Detector Assembly
943-25-25 Preamplifier Assembly
A
843-25-10 Preamplifier Assembly, PC Board
843-25-3 Schematic Diagram
50-100 Cable
50-111 Cable
A.2 Applicable Bill of Materials
Document Number Description
943-35-5 Gamma Scintillation Detector Assembly
943-36-5 Gamma Scintillation Detector Assembly
943-36H-5 Gamma Scintillation Detector Assembly
943-37-5 Gamma Scintillation Detector Assembly
943-237A-5 Gamma Scintillation Detector Assembly
943-25-25 Preamplifier Assembly
843-25-10 Preamplifier Assembly PC Board
A-1
Page 22
Fluke Biomedical
Radiation Management Services
6045 Cochran Road
Cleveland, Ohio 44139
440.498.2564
www.flukebiomedical.com/rms
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