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Commissioning the RMD RadCam using
coded aperture collimator
Thesis II Final Report
Faculty of Energy Systems and Nuclear Science
University of Ontario Institute of Technology
April 17, 2015
Authors:
DuHwan Kim
Supervisors:
Dr. Anthony Waker
Dr. Gloria Orchard
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Acknowledgements I would like to express our deep appreciation to our Thesis advisors Dr. Anthony Waker and Dr.
Gloria Orchard for their patience and guidance throughout the whole semesters. Their time and
dedication has motivated and enabled me to successfully complete this project.
As well, I would like to thank those professors who encouraged me during my undergraduate
career proving me with the foundations on which continues to build our academic knowledge in
Health Physics and Radiation Science.
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Table of Contents Acknowledgements ......................................................................................................................... 2
Executive Summary ........................................................................................................................ 4
1. Introduction ............................................................................................................................. 6
2. Material and Methods .............................................................................................................. 6
2.1 Calibration ........................................................................................................................ 9
2.2 Alignment ....................................................................................................................... 10
2.3 Spatial resolution ............................................................................................................ 11
3. Analysis ................................................................................................................................. 11
3.1 Calibration ...................................................................................................................... 12
3.1.1 Calibration Verification .............................................................................................. 15
3.1.2 A comparison of pinhole and coded aperture collimator ........................................... 20
3.1.3 A comparison of coded aperture collimator in narrow vs. wide view ........................ 21
3.1.4 Absolute peak efficiency and Resolution ................................................................... 23
3.2 Alignment ....................................................................................................................... 26
3.2.1 Phase I: Acquisition of a strong source ...................................................................... 27
3.2.2 Phase II: Experiment Execution ................................................................................. 28
3.3 Spatial resolution ............................................................................................................ 29
3.3.1 Phase I: Acquisition of strong two sources ................................................................ 30
3.3.2 Phase II: Experiment Execution ................................................................................. 30
4. Conclusion ............................................................................................................................. 31
5. Appendix A: Sample Calculation .......................................................................................... 34
6. Appendix B: Experimental Protocol ...................................................................................... 37
7. Appendix C: Table of Spatial resolution ULT: 100% & LLT: 60% ..................................... 41
8. Appendix D: Table of Spatial resolution ULT: 80% & LLT: 60% ....................................... 42
9. References .............................................................................................................................. 43
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Executive Summary The RMD RadCam is as spectroscopic gamma ray imaging system which provides a
qualitative image of gamma ray producing material. In order to commission the RMD RadCam
for use at the University of Ontario Institute of Technology, three major experiments including
the energy calibration, nuclear and video alignment and spatial resolution were completed. For
those experiments, the RMD RadCam was equipped with the coded aperture collimator and the
field of view was set to wide. The six point energy calibration was executed by obtaining six
separate spectra of the Cadmium-109 (Cd-109), Cobalt-57 (Co-57), Sodium-22 (Na-22),
Cesium-137 (Cs-137), Manganese-54 (Mn-54) and Unknown (Cs-137 & Zn-65). In this
experiment, chemistry standing was used to hold each point sources 2.5 cm away from the coded
aperture because source could not attached directly to the coded aperture. Using this relationship,
the calibration curve equation of y = 2.1353x + 39.708 was obtained. This equation was used to
determine the energy corresponding to channel number. The second experiment focused on the
alignment of the nuclear image with the video image. A strong source, 1 mCi (37 Bq) of Cs-137,
was used in the ERC B058 bunker. To access this source, an experimental protocol was
developed to obtain a permit from the UOIT radiation safety officer (RSO). The purpose of this
experiment was to align the nuclear image with the center of the field of view and this required
moving the source until the center of the hotpot displayed at the center of the detector field of
view, as indicated by the red cross-hairs. To align the nuclear image, the RMD Radcam was
positioned on an angle because it was determined that the Cesium Iodide (CsI) crystal was not
parallel to coded aperture. Lastly, spatial resolution experiment was performed to determine the
limitation and appropriate applications for use. Since the spatial resolution is related to the
alignment of the nuclear and video image, same experimental protocol was followed but, another
strong Cs-137 source was also used. During experiments, it was determined that the right source
seemed always brighter than left source in nuclear image. It was either RMD RadCam was in
angle to the right, focusing right source more than left source or the photomultiplier tube was
also not parallel to the CsI crystal. There were total of six experiment that executed to find the
spatial resolution in decreasing order and found that the spatial resolution was 45.7 cm.
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1. Introduction Radiation detection has played an essential role in the study and use of nuclear materials since
radiation measurements provide a sense of safety and control to Nuclear Energy Workers
(NEWs) and the public. This represents one of the characteristics of the Radiation Measurement
Device RadCam (RMD RadCam). This gamma spectroscopic imaging system provides an
intuitive picture of the intensity, distribution, location, and energy spectrum of gamma-ray
sources (User’s Manual). This device uses a Cesium Iodide detector to generate and project a
nuclear image over a video image, obtained using a video camera, of the same field of view. The
nuclear image, obtained from the detector, is superimposed over the video image, producing a
display of any present radioactive sources in a given location within the video image (User’s
Manual). In thesis I, the pinhole collimator was used to ensure the accuracy of its functionalities,
proper calibration and alignment of the nuclear and video images. In thesis II, it outlines the
similar experiments and processes performed to achieve the calibration, alignment of the gamma
camera, as well as the results obtained from such exercises using coded aperture collimator.
Thus, the new experiment called spatial resolution will be mentioned.
2. Material and Methods
The RMD RadCam is a spectroscopic gamma ray imaging system which produces a near-real
time radiation field image, or nuclear image, superimposed over a video image of the same field
of view (User’s Manual). The system consists of many components including the RMD
RadCam detector, tungsten coded aperture collimator and pinhole collimator, video camera, data
interface box and laptop computer with the IMAGE 2000 software. The following Figure 2.1
displays the main components of the system as indicated above.
Figure 2.1: RMD RadCam components(Brochure).
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The Cesium Iodide (CsI) crystal dope with sodium, used to detect the presence of gamma
radiation, is an inorganic scintillator. When incident photons interact with the scintillator
material, the electrons of the scintillator material are raised to exited states. As these electrons
de-excite, photons in the visible light range are emitted. These photons travel to the
photomultiplier tube where they pass through a photocathode and release electrons. Dynodes
within the photomultiplier tube multiply the electrons until they reach the anode. This process
allows a respectable signal to be produced (Knoll). Since the RMD RadCam is concerned with
the origin of the incident radiation, position sensitive photomultiplier tubes are used. A CsI
crystal is used over a Sodium Iodide (NaI) crystal because it is non-hygroscopic, does not attract
or absorb moisture from the air, has a high light output and is used for applications where
mechanical stability and good energy resolution are required (Custom Scintillators & Detectors).
Depending on the application of the RMD RadCam, the position of the crystal within the
detector is adjustable. Using the adjuster knob on the back of the RMD RadCam, as noted in
Figure 2.2, the position of the crystal can be changed to a wide field of view, or narrow field of
view. The wide field of view is set when the adjuster knob is fully clockwise with the arrow
pointing towards the two dots. At this position, the crystal is at the face of the pinhole or coded
aperture collimator. The narrow field of view is set when the adjuster knob is fully counter
clockwise. At this position, the crystal is set further back from the pinhole or coded aperture
(User’s Manual). For the purpose of the experiments completed this term, the wide field of view
was primarily used.
Figure 2.12: RMD RadCam wide versus narrow view(User’s manual).
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Two types of collimators can be interchanged on the face of the RMD RadCam. These
tungsten collimators include the pinhole collimator and coded aperture collimator. The pinhole
collimator determines the location of high intensity gamma fields in a quick manner. The coded
aperture collimator is a collection many pinholes of various shapes in a specific pattern which
provide great number of events in spectrum (Brochure). In other words, coded apertures utilize
an alternate geometric method to recreate the object space. For example, when photon pass
through a pattern of open and closed apertures, this system can be thought of as an array of
pinhole imaging devices, with overlapping images (Farber).
Figure 2.3: Schematic view of RMD RadCam, using coded aperture collimator (Farber).
In addition to the coded aperture collimator, the unique holes pattern are uniquely designed
for accurate reconstruction of the nuclear and can reverse itself upon a 90° rotation (anti-mask
position) of the coded aperture. Each hole in the pattern becomes solid in the rotated anti-mask
position and each location in the 0° (mask position) that was a solid becomes a hole. Combining
the mask and anti-mask position of the coded aperture collimator enhances nuclear image quality
by reducing in the image gamma events that do not correlate with the mask/anti-mask positons of
the coded aperture (Rennie).
The video camera, mounted on the top of the RMD RadCam as seen in Figure 2.1 captures
video image of the same field view of the nuclear image generated by the detector. The images
captured by the detector and video camera are processed using the data interface box in unison
with the laptop computer. The nuclear image captured using the detector, and video image
CsI Crystal
Photomultiplier
tube
Coded aperture
Detector
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captured using the video camera are sent to the laptop where the IMAGE 2000 software
superimposes the nuclear images over a black white video image of the field of view. The
IMAGE 2000 software allows the detection period to be set using different stop conditions,
displays a color scheme for nuclear image as well as an energy spectrum of the radiation
detected. The image interval can be determined by the selection of four different stop
conditions. The conditions include max time (stops when input time is reached), max counts
(stops when input counts is reached), max time or max counts (stops when input time or counts is
reached) and max time and max counts (requires manual stop). For the experiments completed
this term, the most appropriate stop condition was determined to be max time. When a nuclear
image is generated, a color scheme is displayed to indicate the strength of the hotspot. The
intensity of the gamma radiation is presented in colour, red corresponding to higher gamma
activity. The brighter red color represents the hotspot of the gamma activity. These colours may
be adjusted based on user preference. The energy spectrum is generated based on the source(s)
being detected. The spectrum can be uncalibrated (counts as a function of channel) or calibrated
using the software (counts as a function of energy). Area of interest can be selected to show the
number counts or energy for each channel.
2.1 Calibration
To compare the previous year of calibration experiment using pinhole collimator, this
experiment was conducted using coded aperture collimator in different procedure. The energy
calibration of the spectrum generated using the RMD RadCam was completed using six point
sources: Cadmium-109 (Cd-109), Cobalt-57 (Co-57), Sodium-22 (Na-22), Cesium-137 (Cs-137),
Manganese-54 (Mn-54) and Unknown (Cs-137 & Zn-65) each with an activity of 1 µCi. In
previous year of the experiment procedure, each point sources were attached directly to the
pinhole of the camera with masking tape. For this experiment, chemistry standing was used to
hold each point sources 2.5 cm away from the coded aperture as seen in Figure 2.1.1. The
pinhole collimator area was very small that each point sources were able to attach directly to it
instead, the coded aperture collimator was too large. The calibration was obtained by running
six separate measurements of gamma emitters Cd-109, Co-57, Na-22, Cs-137, Mn-54 and
Unknown for a live time of 600 seconds, using the stop condition of max time. Upon the
completion of the outlined detection periods, the center of each peak was selected and the
channel number was recorded. Following the experiment, the spectral data was saved in tabular
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form. Using this data, the energy calibration was achieved by generating the calibration curve as
discussed in subsequent section 3.1.
Figure 2.1.1: Calibration
2.2 Alignment
To perform the alignment of the nuclear and video image using coded aperture collimator, a
strong source of 1 mCi (37 Bq) Cesium-137 (Cs-137) source was used again. For the purpose of
completing the alignment, an experimental protocol was developed to obtain a permit from the
UOIT radiation safety officer (RSO). Please refer Appendix B for more detail. This protocol was
developed by providing an overview of the need for a high activity source, outlining the method
of transporting and manipulating the source and the steps to complete the alignment during the
experiment. This exercise was conducted in the bunker, ERC B058, because of the strength
source. At the start of the experiment, an exclusion zone, as described in the protocol, was setup
using masking tape. Following the exclusion zone set-up, the RMD RadCam, data interface box,
and laptop was transported to the bunker and the video nuclear alignment was initiated using the
IMAGE 2000 software. Then, the designated nuclear energy workers (NEWs), Dr. Gloria
Orchard, used two meter tongs to maneuver the source to the first location, approximately 5
meters directly in front of the RMD RadCam. The source was moved by the NEW and various
images were taken until the nuclear image was aligned with the center of the field of view of the
detector, as indicated by the red cross-hairs. Following the nuclear alignment, the video image
was manually adjusted so the hot spot was placed directly over the location of the source. Using
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this image, the source was zoomed in on, and the alignment was “set”. This process and results
will be further discussed in section 3.2 of the report.
2.3 Spatial resolution
Since the spatial resolution is related to the alignment of the nuclear and video image, same
experimental protocol was followed. After aligning the nuclear image to center of the red cross-
hair, the designated nuclear energy workers (NEWs), Dr. Gloria Orchard, used two meter tongs
again to remove another Cesium-137 (Cs-137) source from pit #2. Using 2 m tongs, the position
of the previous Cs-137 source was adjusted on the tripod near the center of the field of view,
7.50 m away from the RMD RadCam. Then, another source was moved ~75% toward to the
right edge of the field of view of the nuclear image. The Cs-137 source that right in the center of
the field of view stayed as same instead, the Cs-137 source ~75% toward to the right edge of the
field of view of the nuclear image was moved to the left by ~25% until two sources are close
each other. This process and results will be further discussed in section 3.3 of the report.
3. Analysis
In previous year, the main purpose of thesis I was to commission RMD RadCam using
pinhole collimator by conducting two experiments: calibration and alignment. In result, there
were several problems that found during experiments: Firstly, there was problem crashing
IMAGE 2000 software during calibration experiment. Secondly, the nuclear image was unable to
be right in the center of the red cross-hair during alignment experiment. The IMAGE 2000
software crashes because of the old patched version but, as long as the software reinstall, it does
not crashes anymore. The nuclear image was unable to be right in the center of the red cross-hair
because the inside of the Cesium Iodide (CsI) crystal was not parallel to pinhole collimator.
However, as long as the RMD RamCam is in certain angle, the nuclear image was able to get
close to the center of the red cross-hair. In thesis II, the similar experiments and processes were
performed to achieve the calibration, alignment of the gamma camera using coded aperture
collimator to see if they also causes same problems. In addition to the thesis II experiment,
spatial resolution was performed to determine the limitation and appropriate applications for use.
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3.1 Calibration
The peak visible at chancel number 43 is an energy peak for the Cadmium-109 (Cd-109)
decay energies of 88 keV with 3.61 percent yield per decay. Displayed in Figure 3.1.1 is the
uncalibrated Cd-109 spectrum, counts as a function of channel, collected for a live time of 600
seconds.
Figure 3.1.1: Uncalibrated Cadmium-109 spectrum, counts as a function of channel number.
The peak visible at channel number 52 is a combined energy peak for the Cobalt-57 (Co-57)
decay energies of 122 keV and 136 keV. The energy of the peak was determined to be 124 keV
by calculating a weighted average of the two decay energies, weighting heavier towards the 122
keV energy since it decays 96.3 percent of times with this energy (Wagenaar). Displayed in
Figure 3.1.2 is the uncalibrated Co-57 spectrum, counts as a function of channel, collected for a
live time of 600 seconds.
0
2000
4000
6000
8000
10000
12000
0 100 200 300 400 500 600 700
Co
un
ts
Channel Number
Cadmium-109: Counts as a Function of Channel
Number
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Figure 3.1.2: Uncalibrated Cobalt-57 spectrum, counts as a function of channel number.
Two peaks visible at chancel number 187 and 568 are energy peaks for the Sodium-22 (Na-
22) decay energies of 511 keV and 1275 keV with 180 percent yield per decay. Please note that
energy peak of 511 keV was used during calibration verification. Displayed in Figure 3.1.3 is
the uncalibrated Na-22 spectrum, counts as a function of channel, collected for a live time of 600
seconds.
Figure 3.1.3: Uncalibrated Sodium-22 spectrum, counts as a function of channel number.
The peak visible at chancel number 260 is an energy peak for the Cesium-137 (Cs-137) decay
energies of 662 keV with 85.1 percent yield per decay. Displayed in Figure 3.1.4 is the
0
5000
10000
15000
20000
25000
30000
0 100 200 300 400 500 600 700
Co
un
ts
Channel Number
Cobalt-57: Counts as a Function of Channel
Number
0
500
1000
1500
2000
2500
3000
0 100 200 300 400 500 600 700
Co
un
ts
Channel Number
Sodium-22: Counts as a Function of Channel
Number
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uncalibrated Cs-137 spectrum, counts as a function of channel, collected for a live time of 600
seconds.
Figure 3.1.4: Uncalibrated Cesium-137 spectrum, counts as a function of channel number.
The peak visible at chancel number 404 is an energy peak for the Manganese-54 (Mn-54)
decay energies of 835 keV with 100 percent yield per decay. Displayed in Figure 3.1.5 is the
uncalibrated Mn-54 spectrum, counts as a function of channel, collected for a live time of 600
seconds.
Figure 3.1.5: Uncalibrated Manganese-54 spectrum, counts as a function of channel number.
0
1000
2000
3000
4000
5000
6000
7000
0 100 200 300 400 500 600 700
Co
un
ts
Channel Number
Cesium-137: Counts as a Function of Channel
Number
0
1000
2000
3000
4000
5000
6000
0 100 200 300 400 500 600 700
Co
un
ts
Channel Number
Manganese-54: Counts as a Function of
Channel Number
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Three peaks visible at chancel number 245, 383 and 494 are energy peaks for the Unknown
(Cs-137 & Zn-65) decay energies of 511 keV, 662 keV and 1115 keV with 50.6 percent yield per
decay. Please note that energy peak of 1115 keV was used during calibration verification.
Displayed in Figure 3.1.6 is the uncalibrated Unknown spectrum, counts as a function of
channel, collected for a live time of 600 seconds
Figure 3.1.6: Uncalibrated Unknown spectrum, counts as a function of channel number.
3.1.1 Calibration Verification
From the plot, it was illustrated that the relationship between channel number and energy is a
positive linear function with an equation of best fit of y = 2.1353x + 39.708, where y was the
energy and x is the channel number. The R2 value measures how closely the data conforms to
the linear relationship. This value ranges from 0 to 1, 1 representing an exact fit. The value for
the data collected, R2 = 0.9794, which confirmed that the measurements almost resemble a linear
fit. Cadmium-109 (Cd-109), Cobalt-57 (Co-57), Sodium-22 (Na-22), Cesium-137 (Cs-137),
Manganese-54 (Mn-54) and Unknown (Cs-137 & Zn-65) were used to explore their respective
calibrated energy curves. Please refer Table 3.1.1.1 to see each sources’ center channel number
of the peak. Using equation (b), the calibration line equation, the energy of each channel number
was calculated.
0
1000
2000
3000
4000
5000
6000
0 100 200 300 400 500 600 700
Co
un
ts
Channel Number
Unknown (Cesium-137 & Zinc-65): Counts as a
Function of Channel Number
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Table 3.1.1.1: Six point sources that used for calibrated energy curve
Nuclide Center
channel
number
Energy
(keV)
FWHM Error
(FWHM/2)
Cd-109 42.84818 88 9.11289 ±4.556445
Co-57 51.75553 124 10.65918 ±5.32959
Na-22 187.47661 511 29.29028 ±14.64514
Cs-137 260.1716 662 55.18208 ±27.59104
Mn-54 404.17681 835 39.74358 ±19.87179
Unknown
(Cs-137 &
Zn-65)
503.61347
1115
49.70898 ±24.85449
y�EnergykeV� = 2.1353xchannelnumber� + 39.708
3.1.1(b)
Figure 3.1.1.1: Calibration curve, energy as a function of channel number
Using equations (c) and (d), the count rate and its associated error at each energy was
calculated.
CountRate = CountsLiveTime 3.1.1(c)
CountRateError = √CountsLiveTime 3.1.1(d)
y = 2.1353x + 39.708
R² = 0.9794
0
200
400
600
800
1000
1200
0 100 200 300 400 500 600
En
erg
y (
Ke
V)
Channel Number
RMD Calibration Curve: Energy as a Fucntion
of Channel Number
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Completing the above, the calibrated energy spectra of Cd-109, Co-57, Na-22, Cs-137, Mn-54
and Unknown were generated as shown from Figure 3.1.1.2 to Figure 3.1.1.7 below. Refer to
Appendix A for a sample calculation of the energy, count rate, and count rate error.
Figure 3.1.1.1.2: Calibrated Cadmium-109 Count Rate as a function of energy. The
energy of each channel was calculated using equation (b). Assume no error is associated
with the energy. The count rate at each energy was calculated using equation (c). The
error associated with the count rate was calculated using equation (d). Note: the error
in the count rate is smaller than the data point.
Figure 3.1.1.3: Calibrated Cobalt-57 Count Rate as a function of energy. The energy of
each channel was calculated using equation (b). Assume no error is associated with the
energy. The count rate at each energy was calculated using equation (c). The error
associated with the count rate was calculated using equation (d). Note: the error in the
count rate is smaller than the data point.
0
2000
4000
6000
8000
10000
12000
0 200 400 600 800 1000 1200 1400
Co
un
t R
ate
(cp
s)
Energy (keV)
Cadmium-109 Count Rate as a Fucntion of
Energy
0
5000
10000
15000
20000
25000
30000
0 200 400 600 800 1000 1200 1400
Co
un
t R
ate
(cp
s)
Energy (keV)
Cobalt-57 Count Rate as a Fucntion of Energy
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Figure 3.1.1.4: Calibrated Sodium-22 Count Rate as a function of energy. The energy of
each channel was calculated using equation (b). Assume no error is associated with the
energy. The count rate at each energy was calculated using equation (c). The error
associated with the count rate was calculated using equation (d). Note: the error in the
count rate is smaller than the data point.
Figure 3.1.1.1.5: Calibrated Cesium-137 Count Rate as a function of energy. The
energy of each channel was calculated using equation (b). Assume no error is associated
with the energy. The count rate at each energy was calculated using equation (c). The
error associated with the count rate was calculated using equation (d). Note: the error
in the count rate is smaller than the data point.
0
500
1000
1500
2000
2500
3000
0 200 400 600 800 1000 1200 1400
Co
un
t R
ate
(cp
s)
Energy (keV)
Sodium-22 Count Rate as a Fucntion of Energy
0
1000
2000
3000
4000
5000
6000
7000
0 200 400 600 800 1000 1200 1400
Co
un
t R
ate
(cp
s)
Energy (keV)
Cesium-137 Count Rate as a Fucntion of
Energy
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Figure 3.1.1.6: Calibrated Manganese-54 Count Rate as a function of energy. The
energy of each channel was calculated using equation (b). Assume no error is associated
with the energy. The count rate at each energy was calculated using equation (c). The
error associated with the count rate was calculated using equation (d). Note: the error
in the count rate is smaller than the data point.
Figure 3.1.1.1: Calibrated Unknown Count Rate as a function of energy. The energy of
each channel was calculated using equation (b). Assume no error is associated with the
energy. The count rate at each energy was calculated using equation (c). The error
associated with the count rate was calculated using equation (d). Note: the error in the
count rate is smaller than the data point.
The dead time of the RMD RadCam was investigated after completing the separate
measurements using Cd-109, Co-57, Na-22, Cs-137, Mn-54 and Unknown sources. The
calculated dead time were the following: Cd-109 was 3.29%, Co-57 was 1.19%, Na-22 was
0
1000
2000
3000
4000
5000
6000
0 200 400 600 800 1000 1200 1400
Co
un
t R
ate
(cp
s)
Energy (keV)
Manganese-54 Count Rate as a Fucntion of
Energy
0
1000
2000
3000
4000
5000
6000
0 200 400 600 800 1000 1200 1400
Co
un
t R
ate
(cp
s)
Energy (keV)
Unknown (Cescium-137&Zinc-65) Count Rate as a
Fucntion of Energy
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3.94%, Cs-137 was 2.00%, Mn-54 was 2.82% and Unknown was 1.57%. Refer to Appendix A
for a sample calculation of the dead time. Assume no error exists in the time measurements.
The dead time percentage was calculated using this following equation (Orchard):
DeadTime%� = .RealTimes� − LiveTimes�RealTimes� 0 × 100% 3.1.1(e)
3.1.2 A comparison of pinhole and coded aperture collimator
For Figure 3.1.2.1 and Figure 3.1.2.2, there are two graphs of Cesium-137 (Cs-137) and
Cobalt-57 (Co-57) using pinhole and coded aperture collimator. The two graphs which shows the
major differences between pinhole and coded aperture collimator concluded that the resolution of
the peaks were much better and clear to see if coded aperture collimator was used.
Figure 3.1.2.1: Uncalibrated Cesium-137 spectrum, counts rate as a function of channel
number pinhole vs. coded aperture collimator
0
2
4
6
8
10
12
0 100 200 300 400 500 600 700
Co
un
t R
ate
(c
ps)
Channel Number
Cs-137: Count Rate as a Function of Channel
Number
pinhole coded aperture
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Figure 3.1.2.2: Uncalibrated Cobalt-57 spectrum, counts rate as a function of channel
number pinhole vs. coded aperture collimator
3.1.3 A comparison of coded aperture collimator in narrow vs. wide view
From Figure 3.1.3.1 to Figure 3.1.3.4 there are four graphs of Cadmium-109 (Cd-109),
Cobalt-57 (Co-57), Manganese-54 (Mn-54) and Unknown (Cs-137 & Zn-65) using coded
aperture collimator in narrow and wide view. The four graphs which shows the major differences
between narrow and wide view, concluded that the resolution of the peaks are much better and
clear to see if coded aperture collimator in wide view was used.
Figure 3.1.3.1: Uncalibrated Cadmium-137 spectrum, counts rate as a function of channel
0
10
20
30
40
50
0 100 200 300 400 500 600 700
Co
un
t R
ate
(c
ps)
Channel Number
Co-57: Count Rate as a Function of Channel
Number
pinhole coded aperture
0
2
4
6
8
10
12
14
16
18
20
0 25 50 75 100 125 150 175 200
Co
un
t R
ate
(cp
s
Channel Number
Cadmium-109: Count Rate as a Function of Channel
Number
narrow wide
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number narrow vs. wide view
Figure 3.1.3.2: Uncalibrated Cadmium-137 spectrum, counts rate as a function of channel
number narrow vs. wide view
Figure 3.1.3.3: Uncalibrated Cadmium-137 spectrum, counts rate as a function of channel
number narrow vs. wide view
0
5
10
15
20
25
30
35
40
45
50
0 50 100 150 200 250 300 350 400 450 500 550 600
Co
un
t R
ate
(cp
s)
Channel Number
Cobalt-57: Count Rate as a Function of Channel
Number
narrow wide
0
1
2
3
4
5
6
7
8
9
10
-50 50 150 250 350 450 550
Co
un
t R
ate
(cp
s)
Channel Number
Manganese-54: Count Rate as a Function of Channel
Number
narrow wide
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Figure 3.1.3.4: Uncalibrated Cadmium-137 spectrum, counts rate as a function of channel
number narrow vs. wide view
3.1.4 Absolute peak efficiency and Resolution
For Figure 3.1.4.1 to Figure 3.1.4.2 there are two graphs of Absolute Peak Efficiency and
Resolution graph. Thus, both of the graphs were computed by using each peak of six point
sources: Cadmium-109 (Cd-109), Cobalt-57 (Co-57), Sodium (Na-22), Cesium-137 (Cs-137),
Manganese-54 (Mn-54) and Unknown (Cs-137 & Zn-65). In Table 3.1.4.1 below shows all the
variables that needed to calculate absolute efficiency and resolution. To find absolute efficiency,
first thing was to find the current activity of each sources. Then, it needed to find the counter
under peak. Using equation (f,g), the current activity and peak area of each source were
calculated. To see the full calculations, please refer Appendix I for more detail.
A = 3°e5λt 3.1.4(f)
Peakarea =89: − ; − 3�9< + 9=2=
:>< 3.1.4(g)
Table 3.1.4.1: Variables that used for finding absolute efficiency and resolution (Firestone)
0
1
2
3
4
5
6
7
8
9
10
-50 50 150 250 350 450 550 650
Co
un
t R
ate
(cp
s)
Channel Number
Cescium-137&Zinc-65: Count Rate as a Function
of Channel Number
narrow wide
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Nuclide Counter under
peak (counts)
Activity (Bq) Branching ratio
(%)
FWHM Real time
(s)
Cd-109 12520.7 28342 3.61 9.11289 620.4
Co-57 300788.3 24198 96.3 10.65918 607.2
Na-22 26363.2 2438.3 180 29.29028 624.6
Cs-137 80852.5 29267 85.1 55.18208 612
Mn-54 64135.5 24716 100 39.74358 617.4
Unknown (Cs-
137 & Zn-65)
21614.7 22977 50.6 49.70898 609.6
Finally using equation (h,i), the current absolute efficiency and resolution of each source were
calculated. In this report, absolute peak efficiency was computed because it depends on the
detector of counting geometry and intrinsic efficiency depends on the detector material radiation
energy and physical thickness of the detector in direction of incident radiation (Gloria). In other
words, it need to factor out the solid angle while calculating intrinsic efficiency. Thus, absolute
peak efficiency and resolution were decreasing because they depends on probability of
increasing energy peak. In other words, there will be more Compton scattering as the energy
peak increases. No additional error was being created from the absolute efficiency and resolution
in this cause since they assumed to have no error associated with it. This means that the only
error present is from the measured counts error, so this error needs to be divided by either
absolute efficiency or resolution to obtain the error impacting decays per second.
Absoluteefficiency = Counterunderpeakgammaemittedbysource 3.1.4(h)
Resolution = FWHMCenterchannelnumber 3.1.4(i)
Absoluteefficencyerror = ErrorEFGAbsoluteefficency 3.1.4(j)
Resolutionefficencyerror = ErrorEFGResolution 3.1.4(k)
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Table 3.1.4.2: Data for absolute efficiency and resolution
Nuclide Center
channel
number
Energy
(keV)
Absolute
Efficiency
Resolution
Cd-109 42.84818 88 0.0197 0.213
Co-57 51.75553 124 0.0213 0.206
Na-22 187.47661 511 0.00962 0.156
Cs-137 260.1716 662 0.00530 0.212
Mn-54 404.17681 835 0.00420 0.0983
Unknown
(Cs-137 &
Zn-65)
503.61347
1115
0.00305 0.0987
Figure 3.1.4.1: Absolute Peak Efficiency
-5.00E-03
0.00E+00
5.00E-03
1.00E-02
1.50E-02
2.00E-02
2.50E-02
0 200 400 600 800 1000 1200
Ab
osl
ute
Pe
ak
Eff
icie
ncy
Energy (KeV)
Aboslute Peak Efficiency Graph
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Figure 3.1.4.2: Resolution
3.2 Alignment
This experiment was executed to acquire the maximum accuracy when using the RMD
RadCam. The proper alignment of the nuclear and video image provides an output with
information of the location and energy of each gamma emitter. The video camera produces a
black and white video snapshot as seen in Figure 3.2.1. The nuclear image, displayed in Figure
3.2.2, is generated from the detection of the gamma rays by a sensor head composed of, a
pinhole, a scintillator with a inorganic solid material (Cesium Iodide crystal), and a position-
sensitive photomultiplier tube. The nuclear image provides a color scale application which
reveals the intensity of radiation from each point in the camera’s field of view.
0
0.05
0.1
0.15
0.2
0.25
0 200 400 600 800 1000 1200
Re
solu
tio
n
Energy (KeV)
Resolution Graph
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Figure3.2.1: Video Image (Black and White) taken in
the Bunker during alignment experiment.
Figure 3.22.2: Nuclear Image taken in the bunker
during alignment experiment. It shows hotspots
caused by the 137Cs source of 37 MBq.
The alignment is a delicate process that requires the precision of placing the source hot spot
(the nuclear image) obtained from the detector as near as possible over the center of field of
view, or the center of the red cross-hairs, of the RMD RadCam detector. Then, by manually
adjusting the video image to align the real life source location with the hot spot, alignment is
achieved.
To proceed with the alignment of the video and nuclear image there were some phases that
needed to be overcome as outlined below.
3.2.1 Phase I: Acquisition of a strong source
For the purpose of doing this experiment a strong source was required in order to locate the
source at a far distance (User’s Manual). Therefore, access to one of the strong sources located
in the pits, room B058 at UOIT was needed. Cesium-137 (Cs-137) was the chosen source due to
the fact that it was the strongest available source with an activity of 37 MBq (1 mCi). In order to
acquire a permit necessary to handle the sources, a research test plan or protocol was generated
and addressed to the UOIT Radiation Safety Officer (RSO). Refer to Appendix B for the
approved experimental protocol. A detailed description of the research test plan was outlined to
assure safety was maintained during the use of the source in ERC B058.
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3.2.2 Phase II: Experiment Execution
Following the preparation of the experimental protocol, the alignment experiment in the ERC
room B058 (bunker) was executed. The purpose of this experiment was to align the nuclear
image of the source with video image of the same field of view. Before starting the experiment,
an exclusions zone was set-up, as stated in the protocol. Refer to Figure 3.2.2.1 below for an
outline of the experimental set-up in the bunker.
Figure 3.2.22.2.1: Map of room ERCB058, location of alignment experiment.
This exclusion zone was decided to ensure both NEWs and non-NEWs were not
unnecessarily exposed. Following the source manipulation steps outlined in the experimental
protocol, the source was placed in the desired location. Using the IMAGE 2000 software,
data was collected until a noticeable hotspot was generated. Using the software alignment
function, the center of field of view, determined by the red cross-hairs, was made visible over
the generated image. Several nuclear images were acquired while moving the source, in
order to determine the center of the nuclear image (User’s Manual). This required counting
with the detector for a live time of 5 minutes and collecting the data obtained from the
source. Figure 3.2.2.2 below, a sample nuclear image, is an example of the imaged
generated during the alignment.
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Figure 3.2.2.2: First nuclear image obtained with
the RMD RadCam.
As shown in Figure 3.3.2.3, the source needed to be moved to the left in order to get the
center hotpot to the red cross-hairs. After several attempts to manipulate the source so the
hotspot appeared over the red cross-hairs with no success, it was determined that the CsI crystal
was not positioned perfectly parallel with the coded aperture as well. In order to achieve nuclear
alignment with the center of field of view of, the angle of the RMD RadCam was adjusted.
3.3 Spatial resolution
The main purpose of the spatial resolution is to measure of how closely lines between two
sources can be resolved in an image using RMD RadCam. In other words, it was to explore the
spatial resolution of the RMD Radcam to determine the limitation and appropriate applications
for use.
Figure 3.2.22.2.3: Second nuclear image obtained
using the RMD RadCam shows center spot farther
from the point.
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To proceed with the alignment of the video and nuclear image there were some phases that
needed to be overcome as outlined below.
3.3.1 Phase I: Acquisition of strong two sources
Since the spatial resolution is related to the alignment of the nuclear and video image, same
experimental protocol was followed but, another strong Cesium-137 (Cs-137) source was also
used. Please refer section 3.2.1 for more detail.
3.3.2 Phase II: Experiment Execution
After aligning the nuclear image to center of the red cross-hair, the designated nuclear energy
workers (NEWs), Dr. Gloria Orchard, used two meter tongs again to remove another Cesium-
137 source from pit #2. Using 2 m tongs, the position of the previous Cesium (Cs-137) source
was adjusted on the tripod near the center of the field of view, 7.50 m away from the RMD
RadCam. Then, another source was moved ~75% toward to the right edge of the field of view of
the nuclear image as seen in Figure 3.3.2.1. The Cs-137 source that right in the center of the
field of view stayed as same instead, the Cs-137 source ~75% toward to the right edge of the
field of view of the nuclear image was moved to the left by ~25% until two sources are close
each other.
During experiments, right source seemed always brighter than left source in nuclear image as
seen in Figure 3.3.2.2. These problems could occurred either RMD RadCam was in angle to the
right, focusing right source more than left source or the photomultiplier tube was also not parallel
to the Cesium Iodide (CsI) crystal.
There were total of six experiment that executed to find the spatial resolution: For first four
experiment in distance of 77.5 cm, 54.6 cm. 49.5 cm and 47.0cm in decreasing order, there were
clearly two sources’ hot spots that visible in nuclear image. However, for last two experiment in
distance of 44.5 cm and 39.37 cm, only one source hot spot that visible in nuclear image. In
conclusion, the spatial resolution was 45.7 cm. Please refer Appendix C and Appendix D to see
the six figures of spatial resolution in each distances.
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4. Conclusion
The RMD RadCam is a spectroscopic gamma ray imaging system which produces a near-real
time radiation field image, or nuclear image, superimposed over a video image of the same field
of view (User’s Manual). Using a Cesium Iodide crystal, tungsten coded aperture collimator or
pinhole collimator, video camera, data interface box and laptop computer with the IMAGE 2000
software, a colour coded nuclear image is superimposed over a video image, indicating the
presence and location of any radiation in the field of view of the RMD RadCam.
In thesis I RMD RadCam was commissioned using pinhole collimator. In this term, it was
commissioned using coded aperture and three major experiments including the energy
Figure 3.3.23.2.1: Experiment setup of spatial
resolution
Figure 3.3.23.2.2: Experiment 1 of spatial
resolution: 77.5 cm away from each other
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calibration, nuclear and video alignment and spatial resolution were completed. The completion
of the energy calibration involved collecting six separate spectra of a 1 μCi Cadmium-109 (Cd-
109), Cobalt-57 (Co-57), Sodium-22 (Na-22), Cesium-137 (Cs-137), Manganese-54 (Mn-54)
and Unknown (Cs-137 & Zn-65) for a live time of 600 seconds. Using the channel of the peaks
and the known energy of each source, a calibration curve with the linear equation y = 2.1353x +
39.708 was obtained. Using this equation, the energy of each channel was calculated and used to
plot a calibrated spectrum of the six source measurement. The two graphs which shows the major
differences between pinhole and coded aperture collimator concluded that the resolution of the
peaks are much better and clear to see if coded aperture collimator was used.
To align the nuclear image with the video image, the use of a high activity source was
required. The source desired was the 1 mCi Cesium-137 (Cs-137) source located in the pit of the
ERC B058 bunker. In order to use the source, an experimental protocol was developed outlining
the method of source manipulation and transportation, and the steps required to complete the
alignment. This protocol was approved by the UOIT RSO granting a permit to use the high
activity source to perform the alignment. During the alignment experiment, an exclusion zone
was first established to reduce the exposure to both NEWs and non-NEWs. Then the alignment
option in IMAGE 2000 was initiated to align the nuclear image with the center of the field of
view of the detector. The Cs-137 source was placed in line with the RMD RadCam
approximately 5 meters away and an image was collected. The source was continually moved
horizontally until the source hotspot (nuclear image) was displayed at the center of the red cross-
hairs. It was determined that the crystal was not exactly parallel with the pinhole, therefore the
detector had to be angled in order to achieve perfect alignment.
After aligning the nuclear image to center of the red cross-hair, spatial resolution was
performed. Since the spatial resolution is related to the alignment of the nuclear and video image,
same experimental protocol was followed but, another strong Cesium-137 (Cs-137) source was
also used. During experiments, it was determined that right source seemed always brighter than
left source in nuclear image. It was either RMD RadCam was in angle to the right, focusing right
source more than left source or the photomultiplier tube was also not parallel to the Cesium
Iodide (CsI) crystal. There were total of six experiment that executed to find the spatial
resolution in decreasing order and found that the spatial resolution was 45.7 cm.
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In conclusion, the familiarization, calibration, alignment and spatial resolution of the RMD
RadCam using coded aperture collimator presented to be successful. It is true that coded aperture
was also had same problem as pinhole but clearly, coded aperture is much more useful and
convenient tool than pinhole when it comes to collect great number of spectrum in small amount
of time.
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5. Appendix A: Sample Calculation
SamplecalculationfortheenergyofthecombinedCobalt-57peak.ForCobalt-57,energies122keV86%�and136keV11%�.EnergyofcombinedpeakkeV� = 122keV × L0.860.97M + 136keV × L0.110.97M = 124keVSamplecalculationofthepeakenergycorrespondingtothechannelnumber3.1.1a�.ForCobalt-57,i.echannelnumber10.y�EnergykeV� = 2.1353xchannelnumber� + 39.708 = 2.1353 × 10 + 39.708
= 61.1keVSamplecalculationofthecountrateataspecificenergy3.1.1b�.ForCobalt-57,energy61.061keV,counts4048.394,livetime553.2seconds.CountRate = CountsLiveTime = 4048.394counts553.2s = 7.32cpsSamplecalculationoftheerrorassociatedwiththecountrate3.1.1c�.ForCobalt-57,counts4048.394,livetime553.2seconds.CountRateError = √CountsLiveTime = √4048.394counts553.2s = 0.115cpsSamplecalculationofthesystemdeadtime3.1.1d�.ForCobalt-57,livetime600seconds,realtime611seconds.DeadTime%� = .RealTimes� − LiveTimes�RealTimes� 0 × 100% = L607.2s − 553.2s607.2s M × 100%
= 8.89%Samplecalculationoftheerrorassociatedwiththecalibrationcurve3.1.1e�.ForCobalt-57.CalibrationError = FWHM2 = 10.659182 = ±5.33Samplecalculationofactivityandpeakareaneededtocalculateabsoluteefficiency3.1.4f,g�.i� ActivityforCobalt-57.GivensCurrentActivityJan162015�ManufactureddateAug012014�t = Jan162015 − Aug012014 = 0.46yearsAo=1µciTT UV = 0.75years
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SolutionsA = AWe5XYA = 1μci�e5L [\U�].^_`abcdM].ef`abcd� = 0.654μciii� PeakareaforCobalt-57.GivensCi=336136.3878countsA=Channelnumber25B=Channelnumber66CA=1180.83countsCB=543.4696countsSolutionsPeakarea = 8Ch − B − A� Ci + Cj2
j
h>i
Peakarea = 8336136.3878counts − 66 − 25� 1180.83counts + 543.4696counts2j
h>i= 300788countsSamplecalculationoftheabsoluteefficiencyandresolution3.1.4h,i�.i� AbsoluteefficiencyforCobalt-57.GivensCounterunderpeak=300788.3countsActivityforCobalt-57=0.654µciReal-time=607.2secondsBranchingratio=96.3%SolutionsAbsoluteefficiency = Counterunderpeakgammaemiitedbysource
= 300788counts0.654μci × 3.7 × 10T]BqCi × Ci10f × 607.2seconds × 0.0963 = 0.0213
ii� ResolutionforCobalt-57.
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Resolution = FWHMCenterchannelnumber = 10.6591851.75553 = 0.206Samplecalculationoftheerrorabsoluteefficiencyandresolution3.1.4j,k�i� AbsoluteefficiencyerrorforCobalt-57.AbsoluteEfficiencyError = ErrormndAbsoluteEfficiency = 0.115cps0.0213 = ±5.40ii) Resolution error for Cobalt-57
ResolutionError = ErrormndResolution = 0.115cps0.206 = ±0.558
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6. Appendix B: Experimental Protocol
RMD RadCam
Research Test Plan
Revision 1
Proposed Dates of Experiment:
Friday March 06, 2015
Location:
ERC B056 and B058, UOIT, Oshawa, ON
Sources: 2 x 37 MBq 137Cs
Personnel Involved:
Dr. Anthony Waker
Dr. Gloria Orchard
DuHwan Kim
Work Plan Authorization:
Name Title Signature Date
Tanya Neretljak UOIT RSO
Anthony Waker Supervisor
Gloria Orchard Co-Supervisor
Overview:
The RMD RadCam is a spectroscopic gamma-ray imaging system designed for superimposing a
nuclear image of gamma radiation over a black and white video image for the same field of view.
In thesis I, preliminary tests were performed in September of 2014 using a small button source (1
µCi 137Cs). The source strength was determined to be too low for detection at moderate
distances and alignment of the nuclear and video images. Therefore, one larger sources of
cesium-137 (37 MBq) is required. In thesis II, there are two parts of the experiments that will be
performed using the RMD RadCam to align the nuclear image with the video image and spatial
resolution with using coded aperture.
Anticipated Doses:
The calculations of the expected dose are included in Appendix A.
General Comments:
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1. The source will be handled at all times in accordance with the as low as reasonably
achievable (ALARA) principle.
2. The source will only be handled by designated Nuclear Energy Workers (NEW) at UOIT.
3. Any NEWs handling the sources will be equipped with an electronic personal dosimeter
(EPD) during unpacking, transport, use and packing. The EPD will be set to alarm at a
level of 0.2 mSv.
4. A calibrated radiation survey meter will be used to monitor radiation fields during
unpacking, transport, use and packing.
5. Minimum safe distance will be maintained between any persons and the source at all
times as outlined in Figure 1 by the indicated exclusion zone.
6. The source will only be handled using 2 m tongs.
7. The source will never be left unattended.
8. The source will be returned to pit #1 in ERC B058 at the end of experiment period.
Transportation of Sources from/to Storage:
1. The source will be moved from the pit in ERC B058 and placed onto the tripod using 2 m
tongs by Anthony Waker and/or Gloria Orchard. It will be monitored by a calibrated
radiation survey meter.
2. Experiments will be conducted as per the tests outlined below.
3. At the end of the experiments for each day, the source will be returned to the pit in ERC
B058 reversing the steps above.
Manipulating Sources in Room:
1. The source will remain in the pit until all other experimental material and hardware are
setup.
2. A platform to hold the source will be placed in the room at required location(s). Refer to
Figure 1 for the map of the experimental setup.
3. When the experiment is ready to begin, the source will be removed from the pit, using the
2 m tongs, and placed on the platform. This procedure will take no more than 30
seconds.
4. The radiation fields at points of entry to the room will be monitored and recorded.
5. Non-NEWs will remain outside of the exclusion zone at all times. Once the source is in
place, those manipulating the source will retreat to outside the exclusion zone and the
dose rate will be monitored.
6. When the source requires repositioning in the room, 2 m tongs will be used to move the
source.
7. At the end of the experiment, the source will be returned to the pit in ERC B058.
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Figure 1: Map of experimental setup in ERC room B058. Note that non-NEWs will remain
outside of the exclusion zone at all times.
Experiment #1: Image Alignment using one Cesium-137
Objective:
To align the nuclear image of the RMD RadCam with the video image.
Procedure:
1. Setup RMD RadCam and software at the east side of ERC B058. This will be the
location of all personnel, the RMD RadCam and the computer when not in operation
mode.
2. Initiate the “Video Nuclear Alignment” of the RMD RadCam using software. Remove
the Cesium-137 source from pit #2 (see Figure 1) using 2 m tongs and place it on the
tripod near the center of the field of view, 7.50 m away from the RMD RadCam and take
an image of the source.
3. Using 2 m tongs, adjust the position of the source on the platform and take an additional
image of the source. Repeat this step until the nuclear image is superimposed on the
center of the red cross-hair displayed on the software of the computer screen.
4. Manually adjust the video camera while images are being taken until the video image of
the source is superimposed on the nuclear image of the source.
5. Using the 2 m tongs, move the previous source ~75% toward the edge of the field of view
of the nuclear image. Acquire the nuclear image and magnify the video image using the
computer software to achieve the alignment of nuclear and video image.
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Experiment #2: Spatial resolution using two Cesium-137
Objective:
To explore the spatial resolution of the RMD RadCam to determine the limitation and
appropriate applications with using coded aperture.
Procedure:
1. Remove another Cesium-137 source from pit #2 (see Figure 1) using 2 m tongs.
2. Using 2 m tongs, again adjust the position of the previous Cesciusm-137 on the tripod
near the center of the field of view, 7.50 m away from the RMD RadCam and take an image of
the source.
3. Using the 2 m tongs, move another Cesium-137 the source ~75% toward the edge of the
field of view of the nuclear image.
4. The Cesium-137 source that right in the center of the field of view will not be moved but,
only the Cesium-137 source ~75% toward the edge of the field of view of the nuclear image will
be moved to the left by ~25% until two sources are close each other.
5. Return the two sources to the bunker using the 2 m tongs after finishing all the
experiments.
Appendix A – Dose Calculations
Cs-137 gamma constant = 1.02 × 105e opq×orsc×tju
Cs-137 contact dose rate = 12.5 opqsc×tjufor encapsulated sources
UOIT Action level = 0.3 mSv (1/3 CNSC public whole body dose limit)
Benchmark: 1 meter dose (two sources):
At 1 meter, the dose rate is 7.55 µSv/hr
The time to get to action level at 1 meter is 39.8 hours
Removal of source from pig using tongs: 2 m dose (two sources):
This conservatively assumes that the dose at 2 m (tong length) is the same as the whole body dose.
At 2 meter, the dose rate is 1.887 µSv/hr
The time to get to action level at 2 meter is 159 hours
Average distance of personnel from sources during experiment: 5.15 meter (two sources):
At 5.15 meter, the dose rate is 0.292 µSv/hr
The time to get to action level at 5.15 m is 1054 hours
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7. Appendix C: Table of Spatial resolution ULT: 100% & LLT:
60%
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8. Appendix D: Table of Spatial resolution ULT: 80% & LLT: 60%
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9. References
i) Farber, M. A. (2013). Coded-Aperture Compton Camera for Gamma-Ray Imaging. The
University of Arizona Retrieved from:
http://arizona.openrepository.com/arizona/bitstream/10150/311555/1/azu_etd_13097_sip
1_m.pdf
ii) Firestone, R. B. (2000). Exploring the Table of Isotopes. Ernest O. Lawrence Berkeley
National Laboratory Retrieved from: http://ie.lbl.gov/education/isotopes.htm
iii) Knoll, G. F. (2010). Radiation Detection and Measurement. Danvers, MA: John Wiley &
Sons, Inc.
iv) Orchard, G. (2012). Lecture 2B, 3A - General Properties of Radiation Detectors
Continued. RADI 4550 Lecture Notes. University of Ontario Institute of Technology.
v) Rennie, G (2006). Imagers Provide Eyes to See Gamma Rays. Lawrence Livermore
national laboratory Retrieved from: https://str.llnl.gov/str/May06/Fabris.html
vi) Unknown. Custom Scintillators & Detectors. CA: San Rafael: Berkley Nucleonics
Corporation. Retrieved from:
http://www.berkeleynucleonics.com/products/Custom_Scintillators_Probes.html
vii) Unknown. RMD RadCamTM Spectroscopic Gamma-Ray Imaging System Brochure.
Watertown, MA: RMD Inc.
viii) Unknown. RadCamTM User’s Manual. Watertown, MA: RMD Inc.
ix) Wagenaar, D. J. Cobalt-57 Decay. JPNM Physics Isotopes. Retrieved from:
http://www.med.harvard.edu/jpnm/physics/isotopes/Co/Co57/dec.html