A simple algorithm for estimation of source-to-detector distance in Compton imaging.
Compton imaging is used to predict the location of gamma-emitting radiation sources. The X and Y coordinates of the source can be obtained using a back-projected image and a two-dimensional peak-finding algorithm. The emphasis of this work is to estimate the source-to-detector distance (Z). The algorithm presented uses the solid angle subtended by the reconstructed image at various source-to-detector distances. This algorithm was validated using both measured data from the prototype Compton imager (PCI) constructed at the Los Alamos National Laboratory and simulated data of the same imager. Results show this method can be applied successfully to estimate Z, and it provides a way of determining Z without prior knowledge of the source location. This method is faster than the methods that employ maximum likelihood method because it is based on simple back projections of Compton scatter data.
Rawool-Sullivan
Mohini W
MW
MS B230, IAT-1, Los Alamos National Laboratory, Los Alamos, NM 87545, USA. Mohini@lanl.gov
Sullivan
John P
JP
Tornga
Shawn R
SR
Brumby
Steven P
SP
D000465:Algorithms; D003198:Computer Simulation; D005720:Gamma Rays; D008962:Models, Theoretical; D011829:Radiation Dosage; D011874:Radiometry / Q000379:methods*; D015203:Reproducibility of Results; D012680:Sensitivity and Specificity