compton imaging with the porgamrays detector
DESCRIPTION
Compton imaging with the PorGamRays Detector. D S Judson. Imaging 2010, Stockholm, 8 th -11 th June 2010. Outline. PorGamRays project outline Detector description Spectroscopic performance GEANT simulations Experimental Compton imaging performance Summary. PorGamRays: Aims. - PowerPoint PPT PresentationTRANSCRIPT
Compton imaging with thePorGamRays Detector
D S Judson
Imaging 2010, Stockholm, 8th-11th June 2010
Outline
PorGamRays project outline
Detector description
Spectroscopic performance
GEANT simulations
Experimental Compton imaging performance
Summary
PorGamRays: AimsPortable Gamma-Ray Spectrometer
The project aims to develop a gamma-ray spectrometer that is
Handheld and battery operated
Able to work at room temperature
Capable of providingIsotope identificationImaging
Potential applications for this sensor include:
decommissioning, security and
safety monitoring
6 CZT detectors
Modular design
Energy range:
60 – 2000 keV
PorGamRays: Schematic
gamma
Pixelated CZT
ASICDaughter board
MotherboardLaptop
PorGamRays: CZT detectors
Dimensions of 20 x 20 x 2 mm
Pixelated (10 x 10)
2 x 2 x 2 mm voxels
PorGamRays: CZT detectors
Dimensions of 20 x 20 x 2 mm
Pixelated (10 x 10)
2 x 2 x 2 mm voxels
Detector wire bonded
to daughter board
Data read out through
custom built ASICs
The PorGamRays demonstrator
Two CZT detectors
5 mm separation
Running from external
power supplies
NUCAM II ASICS [1]
Energy range of up to 350 keV
[1] P Seller et. al., IEEE Nuclear Symposium Conf. Rec., V6, 3786, ‘06
Spectroscopic performance of CZT
At 60 keV (241Am), FWHM ~ 6 keV, noise ~ 20 keV
Geant4 simulations
Simulated data used to evaluated the effects of the 20 keV noise level and 350 keV energy limit
Simulated two CZT detectors in PorGamRays configuration
Two different gamma-ray energies were used: 121 and 356 keV
Geant4 simulations
121 keV γ-rays deposit little energy in the scatter detector
Scatterer
Absorber
Eγ (keV)0 20 40 60 80 100 120 140 160 180 200
Eγ (keV)
Geant4 simulations
356 keV γ-rays deposit 140-220 keV in each detector
Scatterer
Absorber
0 50 100 150 200 250 300 350 400
Eγ (keV)
Source located at
x = y = 100 mm
z = 40 mm
x (mm)
y (m
m)
FWHM ~ 20 mm
120
120
100
100
y (mm)
x (mm)
Compton images – 133Ba – 356 keV
Compton images – 133Ba – 356 keV
x (mm)
y (m
m)
FWHM ~ 20 mm
Source located at
x = 105mm y = 115 mm
z = 40 mm
120
120
100
100
y (mm)
x (mm)
Possible to resolve changes in source position of only a few mms
x position (mm)
x = 95 mm
x = 115 mm
Compton images – 133Ba – 356 keV
Multi-spectral imaging
133Ba (356 keV) 57Co (121 keV)
x = 110, y = 120 mm x = 130 mm, y =85 mm
Conclusions
A CZT based Compton camera has been developed
Energy resolution of ~ 10 % at 60 keV
Position resolution of ~ 20 mm FWHM has been demonstrated
Changes in position of ~ 10 mm can easily be resolved
Simultaneous measurement of 2 different source demonstrated
CollaboratorsA J Boston1, P J Coleman-Smith2, D M Cullen3,
A Hardie4, L J Harkness1, L L Jones4, M Jones1,
I Lazarus2, P J Nolan1, V Pucknell2, S V Rigby1, D P Scraggs1,
P Seller4, J Simpson2, M Slee1, A Sweeney1
and the PorGamRays collaboration.
1 The University of Liverpool
2 STFC Daresbury Laboratory
3 The University of Manchester
4 STFC Rutherford Appleton Laboratory
Funded jointly by the EPSRC and TSB