Experimental Studies of ZnS Alpha Particle Counters and Methods for Minimizing Detector Background

B. Masters
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引用次数: 1

Abstract

The zinc sulfide scintillation counter employed at IBM for low-level alpha flux monitoring of device and packaging materials is described. This counter provides almost 100% counting efficiency for alpha particles of 1.5MeV or greater energy emitted from the surface of planar samples up to 130 cm2 in area, and exhibits a sea level background count rate on the order of 0.005 counts/cm2-hr. The contributions of electrical noise, cosmic radiation, and radioactive contamination to this background count rate have been studied experimentally. For near sea level operation, only the cosmic ray and radioactivity contributions are found to be significant. At 50°N geomagnetic latitude, the sea level contribution from cosmic ray interactions appears to be about 0.003 counts/cm2-hr. This component is strongly dependent upon altitude, increasing to about 0.1 counts/cm2-hr. at an altitude of 4.36 km. In the presence of very heavy external shielding, total backgrounds on the order of 0.002 counts/cm2-hr. may be realized, and this residual is attributed primarily to naturally-occurring radioactive contaminants which are present in the construction materials of the detector.
ZnS α粒子计数器的实验研究及最小化探测器背景的方法
描述了IBM用于器件和包装材料低水平α通量监测的硫化锌闪烁计数器。该计数器对面积达130 cm2的平面样品表面发射的1.5MeV或更高能量的α粒子提供几乎100%的计数效率,并显示出海平面背景计数率为0.005计数/cm2-hr。实验研究了电噪声、宇宙辐射和放射性污染对本底计数率的贡献。对于近海平面作业,只有宇宙射线和放射性的贡献是显著的。在地磁纬度50°N处,宇宙射线相互作用对海平面的贡献约为0.003计数/cm2-hr。该成分与海拔高度密切相关,增加到约0.1个计数/cm2-hr。海拔4.36千米。在存在非常重的外部屏蔽时,总背景约为0.002计数/cm2-hr。这种残余主要归因于存在于探测器结构材料中的自然发生的放射性污染物。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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