Imaging and image restoration of an on-axis three-mirror Cassegrain system with wavefront coding technology

被引:8
作者
Guo, Xiaohu [1 ]
Dong, Liquan [1 ]
Zhao, Yuejin [1 ]
Jia, Wei [2 ]
Kong, Lingqin [1 ]
Wu, Yijian [1 ]
Li, Bing [3 ]
机构
[1] Beijing Inst Technol, Sch Optoelect, Beijing Key Lab Precis Optoelect Measurement Inst, Beijing 100081, Peoples R China
[2] Typonteq Co Ltd, Beijing 100081, Peoples R China
[3] Hebei Normal Univ, Coll Informat Technol, Shijiazhuang 050024, Hebei, Peoples R China
基金
中国国家自然科学基金;
关键词
EXTENDED DEPTH; ABERRATION; FIELD;
D O I
10.1364/AO.54.002798
中图分类号
O43 [光学];
学科分类号
070207 ; 0803 ;
摘要
Wavefront coding (WFC) technology is adopted in the space optical system to resolve the problem of defocus caused by temperature difference or vibration of satellite motion. According to the theory of WFC, we calculate and optimize the phase mask parameter of the cubic phase mask plate, which is used in an on-axis three-mirror Cassegrain (TMC) telescope system. The simulation analysis and the experimental results indicate that the defocused modulation transfer function curves and the corresponding blurred images have a perfect consistency in the range of 10 times the depth of focus (DOF) of the original TMC system. After digital image processing by a Wiener filter, the spatial resolution of the restored images is up to 57.14 line pairs/mm. The results demonstrate that the WFC technology in the TMC system has superior performance in extending the DOF and less sensitivity to defocus, which has great value in resolving the problem of defocus in the space optical system. (C) 2015 Optical Society of America
引用
收藏
页码:2798 / 2805
页数:8
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