Detection and location of gamma-ray sources with a modulating coded mask

被引:15
作者
Anderson, DN [1 ]
Stromswold, DC [1 ]
Wunschel, SC [1 ]
Peurrung, AJ [1 ]
Hansen, RR [1 ]
机构
[1] Pacific NW Natl Lab, Richland, WA 99352 USA
关键词
gamma-ray detection; homeland security; poisson;
D O I
10.1198/004017005000000463
中图分类号
O21 [概率论与数理统计]; C8 [统计学];
学科分类号
020208 ; 070103 ; 0714 ;
摘要
The detection of high-energy gamma-ray sources is vitally importanito national security for numerous reasons, particularly nuclear materials smuggling interdiction and threat detection. This article presents two methods of detecting and locating a concealed nuclear gamma-ray source by analyzing detector data of emissions that have been modulated with a coded mask. The advantages of each method, derived from a simulation study and experimental data, are discussed. Energetic gamma-rays readily penetrate moderate amounts of shielding material and can be detected at distances of many meters. Coded masks are spatial configurations of shielding material (e.g., small squares formed from plates of lead or tungsten) placed in front of a detector array to modulate the radiation distribution. A coded mask system provides improved detection through an increased signal-to-noise ratio. In a search scenario it is impossible to obtain a comparison background run without the presence of a potential concealed source. The developed analysis methods simultaneously estimate background and source emissions and thus provide the capability to detect and locate a concealed high-energy radiological source in near real time. An accurate source location estimate is critically important to expedite the investigation of a high-probability gamma-ray source. The experimental examples presented use a proof-of-concept coded mask system of a 4 x 4 array of NaI detectors directed at a gamma-ray source in a field-of-view roughly 4 m wide x 3 m high (approximately the size of the side panel of a small freight truck). Test results demonstrate that the correct location of a radiologic source could be determined in as little as 100 seconds when the source was 6 m from the detector.
引用
收藏
页码:252 / 261
页数:10
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