'Compton imaging' diaporamas de présentation

Zachariadou Katerina et al

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Imaging devices for medicine and security

Imaging devices for medicine and security. Andy Boston ajboston@liv.ac.uk. Outline of presentation. Focus on ionising radiation and gamma-rays What are the challenges? What detector technology can we consider? Select example projects & links to fundamental research The future prospects.

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A dvanced GA mma T racking A rray

A dvanced GA mma T racking A rray. Performance of an AGATA prototype detector estimated by Compton-imaging techniques. Francesco Recchia INFN - Legnaro on behalf of the AGATA collaboration. The g -ray spectrometer AGATA. R int = 23 cm. Efficiency: 43% (M g =1) 28% (M g =30)

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Planar semiconductor Compton imaging using pulse shape analysis

Planar semiconductor Compton imaging using pulse shape analysis. Anthony Sweeney Position Sensitive Detectors 9 Aberystwyth 2011. Outline. Motivation Compton camera principles Pulse shape analysis Initial result Silicon Detector Future work. Motivation. Homeland security

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Compton imaging with the PORGAMRAYS detector

Compton imaging with the PORGAMRAYS detector. D S Judson. UNTF Forum 2010 - Salford. Outline. The Compton imaging process The PORGAMRAYS project What is it? How does it work? Detector description Spectroscopic performance GEANT simulations Experimental Compton imaging performance

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Preliminary Compton Imaging results of the AGATA A006 detector

Preliminary Compton Imaging results of the AGATA A006 detector. Mike Slee IOP Conference - Glasgow 06/04/2011. Motivation. Data has been taken with the AGATA A006 detector to develop Compton imaging capabilities. Overview. Introduction to AGATA

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Development of a Segmented Planar Germanium Imaging Detector

Development of a Segmented Planar Germanium Imaging Detector. University of Liverpool, STFC Daresbury Laboratory, e2v, Ortec. The Objective of the Project.

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Preliminary Compton Imaging results of the AGATA C001 detector

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Towards a Compton Telescope for Gamma-Ray Astronomy in the MeV range

Towards a Compton Telescope for Gamma-Ray Astronomy in the MeV range. CSNSM-Orsay, AIM/CEA-Saclay, APC-Paris, MPE-Garching, NSI-Copenhagen. The 0.1 ? 10 MeV photon energy range is the domain of nuclear line spectroscopy. Interaction of low-energy CRs with the ISM

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Current Compton Imaging Effort for Homeland Security at LLNL

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