基于CCD和CsI闪烁体的硬X射线成像

陆波; 王于仨; 杨彦佶; 崔苇苇; 陈勇

doi:10.3788/OPE.20172511.2865

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基于CCD和CsI闪烁体的硬X射线成像

X射线光学 | 更新时间：2020-07-07

- 基于CCD和CsI闪烁体的硬X射线成像
- Hard X-ray imaging based on CCD and CsI scintillator
- 光学精密工程 2017年25卷第11期页码：2865-2871
- 作者机构：
  
  中国科学院高能物理研究所粒子天体重点实验室, 北京 100049
- 作者简介：
  
  [ "陆波(1984-), 男, 浙江舟山人, 助理研究员, 2010年于复旦大学获得硕士学位, 主要从事高能粒子探测器读出ASIC设计。E-mail:luboihep@outlook.com" ]
  陈勇(1970-), 男, 江苏海门人, 研究员, 1992年于复旦大学获得学士学位, 1998年于中国科学院高能物理研究所获得博士学位, 主要从事高能天文实验与数据分析。E-mail:ychen@ihep.ac.cn CHEN Yong, E-mail:ychen@ihep.ac.cn
- 基金信息：
  
  国家自然科学基金资助项目(11603027);国家自然科学基金资助项目(11403024);中国科学院重点部署项目大科学前沿与交叉课题
- DOI：10.3788/OPE.20172511.2865
  中图分类号： TN386.5;O434.19
- 收稿日期：2016-12-09，
  
  录用日期：2017-1-5，
  
  纸质出版日期：2017-11-25
- 稿件说明：
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陆波, 王于仨, 杨彦佶, 等. 基于CCD和CsI闪烁体的硬X射线成像[J]. 光学精密工程, 2017,25(11):2865-2871.

Bo LU, Yu-sa WANG, Yan-ji YANG, et al. Hard X-ray imaging based on CCD and CsI scintillator[J]. Optics and precision engineering, 2017, 25(11): 2865-2871.
陆波, 王于仨, 杨彦佶, 等. 基于CCD和CsI闪烁体的硬X射线成像[J]. 光学精密工程, 2017,25(11):2865-2871. DOI： 10.3788/OPE.20172511.2865.

Bo LU, Yu-sa WANG, Yan-ji YANG, et al. Hard X-ray imaging based on CCD and CsI scintillator[J]. Optics and precision engineering, 2017, 25(11): 2865-2871. DOI： 10.3788/OPE.20172511.2865.

摘要

根据CCD的工作特点，采用曝光控制和多帧图像叠合技术，研制了基于CCD和CsI闪烁体的硬X射线成像探测器，以提高对硬X射线的探测效率。搭建了实验平台，以微加工技术制作的镍准直器为成像目标进行了实验验证。实验中，利用

Fe放射源对CCD进行直接成像；然后利用

241

Am放射源同时对CCD和硬X射线成像探测器分别进行直接成像和间接成像。最后，对图像中出现的拖影、清晰度渐变和区域亮度不同等现象进行分析。分析结果表明：相比CCD本身，这种技术不仅拓展了探测器的可响应能区，而且提高了的量子效率，并且在

241

Am放射源照射下，实现了对硬X射线的高分辨成像，其空间分辨优于50 μm。该器件可作为位置灵敏探测器应用于未来空间天文观测。

Abstract

In consideration of the working characteristics of a Charge Coupled Devices(CCD)

an imaging detector based on CCD and CsI scintillator was presented by using flexible exposure control and multi-frame superpositioning techniques to improve the detection efficiency of hard X-ray. An experimental platform was built

in which a nickel collimator based on a micromachining techniques was adopted as the imaging spatial target. In the experiment

the

Fe X-ray source was adopted for direct imaging of CCD itself. Then

the

241

Am X-ray source was used for both direct imaging by CCD itself and indirect imaging by the hard X-ray imaging detector. Finally

some phenomenon exhibited in the images such as drag shadows

clarity gradients

and different area brightness were analyzed. The results indicate that the techniques presented not only expands the responsive energy range

but also improves the quantum efficiency significantly as comparing with CCD itself. In addition

under exposure with

241

Am X-ray sources

hard X-ray imaging with a spatial resolution better than 50 μm was achieved. The imaging detector is promising to be a position sensitive detector for future space astronomical observations.

关键词

Keywords

references

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