核态势监测系统中CdTe探测器球形吸收器确定脉冲伽玛辐射源方向精度的实验评价

I. Cherniavskiy, M. Chomik, V. Tiutiunyk, Ihor Rolin, V. Starenkiy, M. Tverezovskyi, Oleksandr Sheptur, T. Kurtseitov, Oleksandr Salii, Mykola Pidhorodetskyi
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引用次数: 0

摘要

在核情况监测系统中建立一个剂量测量通道以确定穿透性伽玛辐射源方向的必要性和可能性已经得到证实。利用球形吸收器和碲化镉探测器对脉冲辐射源方向的测定进行了实验评估。只有有适当的电子设备,根据它们的特性和高强度脉冲辐射的光谱-时间特性来构造,才能有效地使用这些探测器。在脉冲模式下确定了美国瓦里安Clinac 600C直线加速器用碲镉探测器的高强度脉冲辐射方向。这允许进行一项实验,以确定从每个探测器记录脉冲的比例系数与直线加速器脉冲辐射源的方向角的依赖关系。通过比较接收到的实验数据与基于物理和数学模型的理论依赖来评估减小的误差。建议将从0°到360°的整个角度范围划分为五个子范围,其中三个或两个比例系数负责确定伽玛源的空间角度。最大减小误差不超过10%,最大角度误差不大于8.4°。在辐射源的空间和能量的所有角度的比例系数的理论计算和实验数据库存在的情况下,可以进行对辐射源角度的最精确的确定
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Experimental Evaluation of Accuracy in Determining the Direction to a Pulsed Source of Gamma-Radiation by a Spherical Absorber With CdTe Detectors in a System of Nuclear Situation Monitoring
The necessity and possibility of creating a dosimetric channel for determining the direction to the source of penetrating gamma-radiation in the nuclear situation monitoring system have been substantiated. The experimental assessment of a reduced error of the device for determining the direction to pulsed sources of radiation using a spherical absorber and CdTe detectors was carried out. These detectors can be used effectively only if there is appropriate electronic equipment, constructed in accordance with their characteristics and spectral-temporal characteristics of highly intense pulsed radiation. The direction to high-intensity pulsed radiation of linear accelerator Varian Clinac 600C (USA) by telluride-cadmium detectors was determined in the pulsed mode. This allowed conducting an experiment to determine the dependence of the coefficient of proportionality of recording pulses from each detector on the angle of direction to the source of pulsed radiation of the linear accelerator. A reduced error was assessed by comparing the received experimental data with a theoretical dependence based on a physical and mathematical model. It was recommended to divide the entire range of angles from 0° to 360° into five sub-ranges, in which three or two proportionality coefficients are responsible for determining the angle in space on gamma sources. The maximum reduced error does not exceed 10 % and the maximum angle error is not more than 8.4°. The most accurate determining of the angle to a radiation source can be carried out in the presence of a theoretically calculated and experimental database of proportionality coefficients for all angles in space and energy of radiation sources
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