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Lucy-Richardson迭代解谱在X射线荧光分析的应用
引用本文:祝宇轩,陆景彬,赵晓帆,刘晓艳,崔苇苇,李炜,王于仨,吕中华,陈勇. Lucy-Richardson迭代解谱在X射线荧光分析的应用[J]. 光谱学与光谱分析, 2021, 41(9): 2823-2828. DOI: 10.3964/j.issn.1000-0593(2021)09-2823-06
作者姓名:祝宇轩  陆景彬  赵晓帆  刘晓艳  崔苇苇  李炜  王于仨  吕中华  陈勇
作者单位:吉林大学物理学院,吉林 长春 130012;中国科学院高能物理研究所,北京 100049;吉林大学物理学院,吉林 长春 130012;中国科学院高能物理研究所,北京 100049;黑龙江大学核科学与技术学院,黑龙江 哈尔滨 150080;中国科学院高能物理研究所,北京 100049;中国科学院大学,北京 100049
基金项目:国家自然科学基金项目(U1838201, U1838202, U1838105)资助
摘    要:硬X射线调制望远镜是我国第一颗X射线天文卫星,其载荷低能X射线望远镜采用了SCD型探测器CCD236,主要对能量在0.7~13.0 keV的软X射线光子进行观测.卫星发射前,需要对探测器进行详细的性能标定,其中包括能量响应矩阵的标定.能量响应矩阵是能谱分析的关键.CCD236探测器输出能谱并不是观测光源的真实发射谱,而...

关 键 词:X射线探测器CCD236  Lucy-Richardson迭代  X射线荧光分析
收稿时间:2021-04-28

An Application of Lucy Richardson Iterative in X-Ray Fluorescence Analysis
ZHU Yu-xuan,LU Jing-bin,ZHAO Xiao-fan,LIU Xiao-yan,CUI Wei-wei,LI Wei,WANG Yu-sa,LÜ,Zhong-hua,CHEN Yong. An Application of Lucy Richardson Iterative in X-Ray Fluorescence Analysis[J]. Spectroscopy and Spectral Analysis, 2021, 41(9): 2823-2828. DOI: 10.3964/j.issn.1000-0593(2021)09-2823-06
Authors:ZHU Yu-xuan  LU Jing-bin  ZHAO Xiao-fan  LIU Xiao-yan  CUI Wei-wei  LI Wei  WANG Yu-sa    Zhong-hua  CHEN Yong
Affiliation:1. College of Physics, Jilin University, Changchun 130012, China2. Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China3. University of Chinese Academy of Sciences, Beijing 100049, China4. College of Physical Science and Technology, Heilongjiang University, Harbin 150080, China
Abstract:Hard X-ray Modulation Telescope (HXMT) is China’s first X-ray astronomical satellite. Low Energy X-ray Telescope (LE) is one of the HXMT’s payloads, which used a special swept charge device (SCD) CCD236 detector to observed photons in an energy band of 0.7~13.0 keV. The CCD236 detectors need to be calibrated well before the launch of HXMT, including the calibration of the energy response matrix, which is the key to energy spectrum analysis. The output spectrum of CDD236 is not the actual emission spectrum of the observation source but the convolution result of the emission spectrum and the energy response matrix (RSP). Generally, we can apply a direct deconvolution method to restore the spectrum of the source. A general deconvolution algorithm is the Lucy-Richardson iterative method which uses the Bayes theorem of conditional probability to carry out repeated operations. Using this method, one can use the RSP to deconvolute with the output spectrum, and restoration of the actual spectrum can be obtained by this method. The spectrum of 55Fe radioactive source can be restored using LR iterative algorithm for verifying the robustness of this method. After the iteration, the energy resolution is optimized from 144.3 to 65.6 eV @ 5.9 keV, and the continuous plateau is obviously suppressed. The restoration spectrum, which is composed of two Gaussian peaks with very narrow FWHM, can well characterize the structure of the real emission X-ray of 55Fe. At the same time, the X-ray fluorescence spectrum of a composite was inversely solved by this method, and the X-ray fluorescence spectrum of the material was reproduced by iteration. The FWHM of each spectrum line was very small, and the main spectrum line of Ag element in the material was changed into an independent line spectrum by iteration. This kind of inverse energy spectrum can be well used for the analysis of element composition.
Keywords:X-ray detector CCD236  Lucy-Richardson iterative method  X-ray fluorescence analysis  
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