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长春理工大学 光电工程学院,吉林 长春 130022
[ "张艺蓝(1992-),女,吉林长春人,博士研究生,2018年于长春理工大学获得硕士学位,主要从事偏振像差及光学设计方面的研究。E-mail: 673258464@qq.com" ]
[ "史浩东(1989-),男,吉林长春人,讲师,硕士生导师,2017年于长春理工大学获得博士学位,主要研究方向为光学系统设计、自由曲面光学系统像差理论、偏振探测与定标技术等。E-mail:shihaoodong08@163.com" ]
[ "姜会林(1945-),男,辽宁辽中人,1969年本科毕业于长春光机学院,1987年博士毕业于中科院长春光机所,2015年当选为中国工程院院士,曾任长春理工大学校长,现任校学术委员会主任,兼任中国兵工学会副理事长、中国光学学会和中国光学工程学会常务理事、中央军委科学技术委员会航天领域专家委员会成员、长春光机所应用光学国家重点实验室学术委员会副主任等职务,长期从事应用光学技术研究。E-mail:cclgdxkjs@163.com" ]
收稿日期:2021-05-10,
修回日期:2021-06-04,
纸质出版日期:2021-12-15
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张艺蓝,史浩东,王超等.基于自由曲面的空间光学系统偏振像差分析[J].光学精密工程,2021,29(12):2783-2796.
ZHANG Yi-Lan,SHI Hao-dong,WANG Chao,et al.Analysis of polarization aberration of space optical system based on freeform surface[J].Optics and Precision Engineering,2021,29(12):2783-2796.
张艺蓝,史浩东,王超等.基于自由曲面的空间光学系统偏振像差分析[J].光学精密工程,2021,29(12):2783-2796. DOI: 10.37188/OPE.20212912.2783.
ZHANG Yi-Lan,SHI Hao-dong,WANG Chao,et al.Analysis of polarization aberration of space optical system based on freeform surface[J].Optics and Precision Engineering,2021,29(12):2783-2796. DOI: 10.37188/OPE.20212912.2783.
针对含有自由曲面的空间光学系统中偏振像差对探测精度和成像质量的影响,基于琼斯表示法,提出以条纹泽尼克多项式为表征函数的自由曲面离轴光学系统偏振像差分析方法,构建了自由曲面反射光学系统偏振像差解析模型,分析了条纹泽尼克多项式低阶系数对视场离轴光学系统偏振像差分布的影响;通过全视场偏振光线追迹仿真及系统引入自由曲面前后的对比,揭示了自由曲面对离轴光学系统相位像差、相位延迟和二向衰减3种偏振像差的作用规律;最后,设计了含有自由曲面的大视场离轴三反偏振成像光学系统,并分析了系统全视场的偏振像差。分析结果表明:相位像差分布与自由曲面面形矢高分布一致,自由曲面引起的二向衰减和相位延迟占系统总体二向衰减和相位延迟的52.5%。掌握这种偏振特性变化对于设计深空天文望远镜等甚高精度的光学系统具有重要意义。
The influence of polarization aberration on detection accuracy and imaging quality in a spatial optical system containing freeform surfaces was analyzed. First, based on the Jones notation, a freeform surface off-axis optical system with fringe Zernike polynomials as the characterizing function was proposed. Second, the polarization aberration analysis model of reflective optical system with freeform surface was developed. The influence of fringe Zernike polynomial low-order coefficients on the polarization aberration distribution of the field of view off-axis optical system was analyzed. Then, by tracing the polarized light through full field of view and by comparing before and after the freeform surface was introduced, the freeform surface effected on three types of polarization aberrations, that is, phase aberration, retardance, and diattenuation, of the field-bias optical system were verified. Finally, a wide-field off-axis three-mirror optical system with freeform surface and the polarization aberration of the full field of view were analyzed. The analysis results show that the phase aberration distribution is consistent with the freeform surface sagittal height distribution, and the retardance and diattenuation caused by the freeform surface account for 52.5% of the retardance and diattenuation of the total system, respectively. Improving this polarization characteristic change is important for the design of very high-precision optical systems such as deep-space astronomical telescopes.
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