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The decoding principle of a tetra wedge anode, which is a development of the wedge and strip anode, is described. The influence of charge cloud size on decoding accuracy is studied using the Monte Carlo method. Simulation results show that the decoding error is large when the size of charge clouds collected by the anode is small. Thus, the charge clouds collected by the tetra wedge anode should reach a necessary size to ensure accurate decoding. Finally, using the ultraviolet photon counting imaging system, the linearity and the spatial resolution of the system are tested. Experimental results show that the system has a good linearity and the spatial resolution is better than 100 μm. 相似文献
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影响X射线像增强器分辨率的因素分析 总被引:3,自引:0,他引:3
对采用双近贴聚焦成像结构的MCP(Micro Channel Plate)-X射线像增强器的工作原理与结构进行了分析,对影响其空间分辨率的主要因素进行了研究.影响X射线成像系统分辨率的因素主要有X射线源焦斑的大小和X射线像增强器自身的分辨率,而影响X射线像增强器分辨率的因素主要有MCP输出面到荧光屏之间的距离、MCP输出面与荧光屏之间的电压差以及MCP自身的分辨率.通过对两种具有不同参量的X射线像增强器分辨率的理论计算及分辨率测试实验,将理论计算结果与测试实验结果对比,验证了分辨率计算公式及影响分辨率因素分析的正确性. 相似文献
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<正>Compared with the traditional image intensifier with phosphor screen readout,the photon-counting imaging detector with charge induction readout is more beneficial in several aspects(e.g.,good imaging properties and time resolution) to astronomy,reconnaissance,bioluminescence,and materials research.However, the annealing temperature during the tube-making process can affect the properties of the Ge film,and consequently impair the performance of the detector.Therefore,the influence of annealing temperature on Ge film and on the detector is studied in order to determine the crucial parameters.The Ge films are prepared on ceramic and quartz glass by the use of an electron gun.They are analyzed by scanning electron microscope(SEM),high-resistance meter,and X-ray diffraction(XRD).The results show that the optimum substrate and annealing temperature are ceramic plate and 250℃,respectively. 相似文献
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研制了用于脉冲星导航的X射线光子计数探测器原理样机, 该探测器主要由对X射线灵敏度较高的CsI光电阴极、微通道板电子倍增器和收集阳极组成. 对X射线光子计数探测器灵敏度、时间分辨率和整个系统的死时间进行了测试, 实验结果表明该探测器的灵敏度在5 keV时可达5.2× 103 A/W, 时间分辨率可达到1.1 ns, 系统整体的死时间为100 ns.
关键词:
脉冲星导航
光子计数探测器
灵敏度
时间分辨率 相似文献
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