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首页> 外文期刊>Nuclear technology & radiation protection >Radiation portal monitors response to gamma radiation and to the detection capability of Orphan radioactive sources: Contribution of the Strass project
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Radiation portal monitors response to gamma radiation and to the detection capability of Orphan radioactive sources: Contribution of the Strass project

机译:辐射门户监测对伽马辐射的反应以及孤儿放射源的检测能力:串行项目的贡献

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Radiation portal monitors are commonly used to detect and intercept unauthorized movement of nuclear and other radioactive materials at country borders. A total of twelve double-pillar portal monitors are present at the Greek-North Macedonian border, each containing two polystyrene scintillating detectors per pillar. Spatial and spectral response testing of the scintillating detectors to gamma radiation was performed by using different radioactive sources and comparing the measurement results with Monte Carlo simulations. A good agreement of the experimentally deduced activities of different point sources, needed for alarm triggering of the radiation portal monitors with Monte Carlo calculated values, was observed. Spectral results show no photopeaks in the spectra due to low resolution of these detectors. The broad peaks observed in the spectra correspond to the Compton edge. Measured spectra with a 137Cs source placed directly on the scintillating detector, at several positions away from the photo multiplier tube, show an energy shift of the Compton edge towards lower energies, as the source is moving away from the photo multiplier tube. The energy shift is due to light transfer mechanisms within the scintillator volume and therefore, it is only observed in optical simulations and not in gamma-ray particle simulations.
机译:辐射门户监测器通常用于在国家边界检测和拦截未经授权的核和其他放射性物质的运动。希腊 - 北马其顿边境中共有十二个双支柱门户门户显示器,每个都是每个柱子的两个聚苯乙烯闪烁探测器。通过使用不同的放射源进行闪烁探测器对伽马辐射的空间和光谱响应测试,并将测量结果与Monte Carlo模拟进行比较。观察到对不同点源的不同点源的活动的良好一致性,需要对蒙特卡罗计算值进行辐射门户监测器的报警触发。光谱结果显示由于这些检测器的低分辨率,光谱中的Photopaks在光谱中。在光谱中观察到的宽峰对应于康普顿边缘。用直接放置在闪烁检测器上的137℃源的测量光谱,在远离照片乘法管的几个位置,显示康柏边缘朝向更低的能量的能量偏移,因为源极远离照片乘法器管。能量偏移是由于闪烁体体积内的光传递机制,因此,仅在光学模拟中观察并且不在伽马射线粒子模拟中观察。

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