Photonic integrated interference imaging system based on front-end S-shaped microlens array and Con-DDPM

被引:1
|
作者
Pan, Xiaoyan [1 ,2 ,3 ,4 ]
Yang, Zhikun [1 ,2 ,3 ,4 ]
Jia, Rui [1 ,2 ,3 ,4 ]
Ren, Ge [1 ,2 ,3 ,4 ]
Peng, Qi [1 ,2 ,3 ,4 ]
机构
[1] Chinese Acad Sci, Natl Key Lab Opt Field Manipulat Sci & Technol, Chengdu 610209, Peoples R China
[2] Chinese Acad Sci, Key Lab Opt Engn, Chengdu 610209, Peoples R China
[3] Chinese Acad Sci, Inst Opt & Elect, Chengdu 610209, Peoples R China
[4] Univ Chinese Acad Sci, Beijing 100049, Peoples R China
来源
OPTICS EXPRESS | 2024年 / 32卷 / 17期
关键词
21;
D O I
10.1364/OE.530187
中图分类号
O43 [光学];
学科分类号
070207 ; 0803 ;
摘要
Aiming at the problems of uneven UV spatial frequency sampling and inverse Fourier transform (IFT) artifacts of the photonic integrated interference imaging system, this study proposes a new imaging system based on a front-end S-shaped microlens array, combined with a conditional denoising diffusion probabilistic model (Con-DDPM). The front-end S-shaped microlens array improves the uniformity of UV spatial frequency sampling, increasing the average peak signal-to-noise ratio (PSNR) and structure similarity index measure (SSIM) by approximately 5 dB and 0.16, respectively. In addition, the deep learning reconstruction algorithm based on Con-DDPM is employed to process the IFT images. This algorithm effectively removes artifacts and restores the detailed information of the images. As a result, the average PSNR and SSIM are improved by approximately 9 dB and 0.38, respectively. These enhancements have significantly improved the imaging quality, laying a solid foundation for the future development of space-based telescopes. (c) 2024 Optica Publishing Group under the terms of the Optica Open Access Publishing Agreement
引用
收藏
页码:29112 / 29124
页数:13
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