大相对孔径宽波段Dyson光谱成像系统

薛庆生; 王淑荣; 于向阳

doi:10.3788/OPE.20132110.2535

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大相对孔径宽波段Dyson光谱成像系统

现代应用光学 | 更新时间：2020-08-12

- 大相对孔径宽波段Dyson光谱成像系统
- Dyson spectral imaging system with large relative aperture and wide spectral region
- 光学精密工程 2013年21卷第10期页码：2535-2542
- 作者机构：
  
  中国科学院长春光学精密机械与物理研究所,吉林长春,130033
- 作者简介：
- 基金信息：
  
  波长轮换与相移扫描相结合的表面形貌干涉测量方法()
- DOI：10.3788/OPE.20132110.2535
  中图分类号： O433.1;TH744.1
- 收稿日期：2013-04-08，
  
  修回日期：2013-05-15，
  
  网络出版日期：2012-10-19，
  
  纸质出版日期：2013-10-15
- 稿件说明：
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薛庆生王淑荣于向阳. 大相对孔径宽波段Dyson光谱成像系统[J]. 光学精密工程, 2013,21(10): 2535-2542

XUE Qing-sheng WANG Shu-rong YU Xiang-yang. Dyson spectral imaging system with large relative aperture and wide spectral region[J]. Editorial Office of Optics and Precision Engineering, 2013,21(10): 2535-2542
薛庆生王淑荣于向阳. 大相对孔径宽波段Dyson光谱成像系统[J]. 光学精密工程, 2013,21(10): 2535-2542 DOI： 10.3788/OPE.20132110.2535.

XUE Qing-sheng WANG Shu-rong YU Xiang-yang. Dyson spectral imaging system with large relative aperture and wide spectral region[J]. Editorial Office of Optics and Precision Engineering, 2013,21(10): 2535-2542 DOI： 10.3788/OPE.20132110.2535.

摘要

提出了一种改进型Dyson光谱成像系统，以克服传统Dyson光谱成像系统焦平面探测器安置困难的缺点。首先，基于折射球面罗兰圆理论，提出了这种改进型Dyson光谱成像系统的光学设计方法。然后，利用MATLAB软件编制了初始结构参数快速计算程序。作为实例，设计了一个相对孔径为1/2，波段为200～1 000 nm的Dyson光谱成像系统。利用自己编制的MATLAB程序计算了初始结构参数，利用光学设计软件ZEMAX-EE对该光谱成像系统进行了光线追迹和优化设计，并对设计结果进行分析。分析结果表明，在整个工作波段（200～1 000 nm）内，点列图半径均方根值小于4.2 m，实现了大相对孔径宽波段像散同时校正，在宽波段内同时获得了良好的成像质量，满足设计指标要求。得到的结果验证了所提出的光学设计方法是可行的。

Abstract

A modified Dyson spectral imaging system was proposed to overcome the problems that the focal plane detector is hard to be arranged in a classical Dyson spectral imaging system. Firstly

the optical design method of the modified Dyson spectral imaging system was developed based on the Rowland circle theory of refractive spherical surface. Then

the initial parameter computing program was programmed using MATLAB software. As an example

a Dyson spectral imaging system operating in 200-1 000 nm with a relative aperture 1/2 was designed. The initial parameters were computed using proposed MATLAB program

and the ray tracing and optimization for the spectral imaging system were performed with ZEMAX-EE sofware. The analyzed results demonstrate that the Root Mean square(RMS) of a spot radius is less than 4.2 m in the whole working waveband (from 200 nm to 1 000 nm)

which implements astigmatism correction and obtains a good imaging quality in a wide spectral region and a large relative aperture. These results prove the feasibility of the optical design method proposed.

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references

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