软X射线掠入射望远镜的成像质量评价

刘鹏; 陈波; 张亚超; 何玲平; 王孝东

doi:10.3788/OPE.20192710.2136

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软X射线掠入射望远镜的成像质量评价

现代应用光学 | 更新时间：2020-08-13

- 软X射线掠入射望远镜的成像质量评价
- Imaging quality evaluation of soft X-ray grazing incidence telescope
- 光学精密工程 2019年27卷第10期页码：2136-2143
- 作者机构：
  
  1.中国科学院长春光学精密机械与物理研究所，吉林长春 130033
  2.中国科学院大学，北京 100049
- 作者简介：
  
  [ "刘鹏(1986-)，男，吉林舒兰人，博士，2010年于吉林大学获得学士学位，主要从事非球面表面检测等方面的研究。E-mail：liupengsbc@msn.cn" ]
  陈波(1961-)，男，吉林长春人，研究员，博士生导师，1984年于吉林大学获得学士学位，1990年、2003年于中国科学院长春光学精密机械与物理研究所分别获得硕士、博士学位，主要从事软X射线-极紫外波段光学和空间光学等方面的研究。E-mail：chenb@ciomp.ac.cn CHEN Bo, E-mail: chenb@ciomp.ac.cn
- 基金信息：
  
  国家自然科学基金资助项目(U1631117);天文联合基金资助项目(U1731114)
- DOI：10.3788/OPE.20192710.2136
  中图分类号： O434.19
- 收稿日期：2019-02-01，
  
  录用日期：2019-4-5，
  
  纸质出版日期：2019-10-15
- 稿件说明：
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刘鹏, 陈波, 张亚超, 等. 软X射线掠入射望远镜的成像质量评价[J]. 光学精密工程, 2019,27(10):2136-2143.

Peng LIU, Bo CHEN, Ya-chao ZHANG, et al. Imaging quality evaluation of soft X-ray grazing incidence telescope[J]. Optics and precision engineering, 2019, 27(10): 2136-2143.
刘鹏, 陈波, 张亚超, 等. 软X射线掠入射望远镜的成像质量评价[J]. 光学精密工程, 2019,27(10):2136-2143. DOI： 10.3788/OPE.20192710.2136.

Peng LIU, Bo CHEN, Ya-chao ZHANG, et al. Imaging quality evaluation of soft X-ray grazing incidence telescope[J]. Optics and precision engineering, 2019, 27(10): 2136-2143. DOI： 10.3788/OPE.20192710.2136.

摘要

为了评价软X射线掠入射望远镜的成像质量，提出了一种利用ZEMAX和MATLAB相结合的像质评价方法。根据这种方法编写的像质评价程序不仅考虑了孔径衍射、几何像差和装调误差等因素对成像质量的影响，而且加入了望远镜面形误差和X射线散射效应的影响。利用勒让德-傅里叶多项式和用户自定义表面，在ZEMAX中建立带有面形误差的筒状反射镜表面模型，实现对真实面形的掠入射反射镜的仿真；根据Harvey-Shack散射理论建立了ZEMAX中的BSDF散射模型，实现对X射线散射的仿真。搭建X射线有限远成像实验装置，对像质评价程序进行了验证。实验结果和仿真结果对比表明：实验光斑和仿真光斑的光强分布基本一致，以实验结果为基准，仿真光斑的半高全宽横向和纵向的相对误差分别为14.7%和11.3%。说明像质评价程序的仿真结果基本符合真实情况，对掠入射光学系统的设计和加工具有一定的指导意义。

Abstract

In order to evaluate the imaging quality of the soft X-ray grazing incidence telescope

an image quality evaluation method using ZEMAX and MATLAB is proposed. The image quality evaluation program written according to this method not only considers the aperture diffraction

the geometric aberration and the alignment errors

but also adds the telescope surface figure errors and the surface scatter effects. Using the Legendre-Fourier polynomial and User Defined Surface

a cylindrical mirror model with figure errors is created in ZEMAX

to simulate the real surface profile grazing incidence telescope. The BSDF scattering model is established according to the Harvey-Shack surface scattering theory to simulate X-ray scattering. The X-ray finite distance imaging experimental facility is built for verifying the image quality evaluation program. The comparison between the experimental results and the simulation results of the image quality evaluation program shows that the light intensity distribution of the experimental spot and simulation spot is basically the same. Using the experimental result as a standard

the relative errors of the horizontal and longitudinal directions of the simulated spot FWHM were 14.7% and 11.3%

respectively. It is proved that the simulation results of the image quality evaluation program are credible and have certain guiding significance for the design and processing of the grazing incidence optical system.

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references

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