Compton Camera development for the imaging of high energy gamma rays 1 Martin Jones UNTF 2010...
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Compton Camera development for the imaging of high energy gamma rays
1
Martin Jones
UNTF 2010 Salford – April 14th 2010
Email: [email protected]
Martin Jones – UNTF April 2010
Overview
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•Introduction to the Distinguish Project
•Compton Imaging
• Detectors
•Current work
•Summary
Martin Jones – UNTF April 2010
The Distinguish project
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• Developing a highly specific detection and imaging system for the detection and quantification of narcotics and more notably, explosives.
• Current imaging systems are based on methods such as conventional X-ray imaging through to CT scanners which provide the user with a high level of shape and density information of objects contained within luggage/cargo.
• This method does not provide any nuclide identification .• Industry has indicated a desire to deduce the composition of suspect objects using current novel imaging techniques.
Martin Jones – UNTF April 2010
The Distinguish project
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• Explosives/narcotics contain combinations of the lighter elements
•Elements such as Oxygen, Carbon and Nitrogen which have characteristic gamma rays
• After neutron interrogation these characteristic gamma rays will be emitted
An illustration of the chemical difference between Dynamite (a) and TNT (b)
(a) (b)
Martin Jones – UNTF April 2010
•Oxygen - 6.13MeV, Nitrogen - 5.11MeV, 2.31MeV, 1.64MeV, Carbon – 4.43MeV
Compton Imaging
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E1
E2
E1
E2
Projected Cones
Location of point source
01
2 111
EEcmCos o
0E
•The Compton imaging technique is to be
used to localise the source of gamma
rays
•Cone reconstruction method defines that the
area of maximum overlap is attributed to
source location
• Scatter detector – good energy resolution,
position dependence
•Absorber detector - high stopping power and
position dependence
• Looking at energies in the range of 0.5-
5.0MeV
210 EEE
Martin Jones – UNTF April 2010
Gamma-ray detection and imaging
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The scatter detector • Planar HPGe detector
• 60 x 60 x 20mm active volume
•12 x 12, 5mm wide orthogonal strips
• position resolution – in order of a cubic mm
• Energy resolution (1.53keV @ 122keV)
Martin Jones – UNTF April 2010
Gamma-ray detection and imaging
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The absorber detector • 64 pixel CsI detector (8 x 8)
•Photomultiplier – 64 pixels (8 x 8)
• 64 individual preamps
• High stopping power
• 51.6 x 51.6 x 50mm active volume with 4.48 x 4.48 x 50mm pixels
Martin Jones – UNTF April 2010
Geant4 validation
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L.J. Harkness, et al., Nucl. Instr. and Meth. A (2009)
Current progress – Simulations
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• Germanium - Germanium configuration
• 5cm source – detector and detector – detector separation
• Germanium - Caesium Iodide configuration (5cm, 2cm and 10cm CsI simulations)
• 5cm source – detector and detector – detector separation
Martin Jones – UNTF April 2010
Simulations
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Simulations
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Simulations
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Simulations
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Klein-Nishina
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Klein-Nishina
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Simulated detector ‘maps’
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The next step
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1. Generate images using current Compton reconstruction code that has been developed in Liverpool.
2. Assess image quality. (Efficiency and image resolution).
3. Add in other factors to the simulations such as energy resolution and position resolution.
4. Implement all of the above experimentally.
Martin Jones – UNTF April 2010
The next step.
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• Full detector characterisation to be complete. Detector is on scanning table
• Will be performed using X-Y scanning table.
• Move in increments of 1mm.
• Collimated beam of 122keV gamma-rays. (Co-57).
• Quantify the uniformity of each pixel.
Martin Jones – UNTF April 2010
The next step.
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Summary.
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•Energies of interest 0.5-5.0MeV.
• Geometry decided based on simulated efficiency.
• Initial simulated images. - Image quality/position resolution.
• Raster scan of CsI detector using Co57
• Aim to complete imaging with Ge/Ge and Ge/CsI in Compton camera mode.
Martin Jones – UNTF April 2010
M.P.Jones1 , A.J. Boston1, H.C Boston1, R.J. Cooper 1 M.R. Dimmock1,
L.P. Gaffney1, A.N. Grint1, L.J. Harkness1, D. Judson1, P.J. Nolan1, D.C. Oxley1,
B. Pietras1, A. Sweeney1, M.J. Joyce2, R.O. Mackin2, M.D. Aspinall2, A.J. Peyton3,
R.G. Silfhout3
1 Department of Physics, University of Liverpool, UK
2 Department of Engineering, Lancaster University, UK
3 School of Electronic and Electrical Engineering, The University of Manchester,
UK
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