Method of inverting wavefront phase from far-field spot based on deep learning

被引:0
|
作者
Zhang Y. [1 ]
He Y. [1 ]
Ning Y. [1 ]
Sun Q. [1 ]
Li J. [1 ]
Xu X. [1 ]
机构
[1] College of Advanced Interdisciplinary Studies, National University of Defense Technology, Changsha
关键词
Adaptive optics; Adaptive wavefront sensing-less correction; Deep residual network; Wavefront phase inversion;
D O I
10.3788/IRLA20200363
中图分类号
学科分类号
摘要
In the adaptive optics system, the accuracy and robustness of wavefront sensor greatly affect the ability of aberration detection and closed-loop correction. In the condition of the nonuniformity of amplitude distributions or insufficient of beacon light energy, it will cause accuracy decrease of Hartmann wavefront sensing due to the lack of sub-aperture light. Meanwhile, the real-time performance of the wavefront sensing-free adaptive system based on far-field spot inversion cannot meet the practical requirements. The method of the wavefront inversion based on deep learning is to directly obtain aberrations by inputting the far-field light intensity image, which can be used as an effective supplement to the adaptive optical system. Through numerical simulation, this paper proved that the deep residual neural network could directly predict the Zernike coefficient of the wavefront phase through the far-field spot. And experimental demonstrated the corrected residual RMS between input and reconstructed wavefront phase was 0.08 waves, the average computation time was less than 2 ms by GPU acceleration. This method can predict the Zernike coefficient of incident wavefront distortion more accurately, and has a good aberration correction capability, suitable for measuring and correcting the main components of wavefront distortion in traditional adaptive optics method, or providing a good initial wavefront estimation for optimized adaptive optics. © 2021, Editorial Board of Journal of Infrared and Laser Engineering. All right reserved.
引用
收藏
相关论文
共 22 条
  • [1] Jiang Wenhan, Progresses on adaptive optics techniques--a review of SPIE's 1991 international symposium on optical applied science and engineering, Opto-Electronic Engineering, 19, 4, pp. 50-60, (1992)
  • [2] Zhao Feifei, Huang Wei, Xu Weicai, Et al., Optimization method for the centroid sensing of Shack-Hartmann wavefront sensor, Infrared and Laser Engineering, 43, 9, pp. 3005-3009, (2014)
  • [3] Barchers J D, Fried D L, Link D J., Evaluation of the performance of Hartmann sensors in strong scintillation, Appl Opt, 41, 6, pp. 1012-1021, (2002)
  • [4] Wei Ping, Li Xinyang, Luo Xi, Et al., Influence of lack of light in partial subapertures on wavefront reconstruction for Shack-Hartmann wavefront sensor, Chinese Journal of Lasers, 47, 4, (2020)
  • [5] Gonsalves R A., Phase retrieval and diversity in adaptive optics, Opt Eng, 21, 5, pp. 829-832, (1982)
  • [6] Gonsalves R A, Chidlaw R., Wavefront sensing by phase retrieval, Proc SPIE, Applications of Digital Image Processing III, 207, pp. 32-39, (1979)
  • [7] Paxman R G, Schulz T J, Fienup J R., Joint estimation of object and aberrations by using phase diversity, Journal of the Optical Society of America A, 9, 7, pp. 1072-1085, (1992)
  • [8] Yang Huizhen, Liu Rong, Liu Qiang, Model wavefront-sensorless adaptive optics system based on eigenmodes of deformable mirror, Infrared and Laser Engineering, 44, 12, pp. 3639-3644, (2015)
  • [9] Sandler D G, Barrett T K, Palmer D A, Et al., Use of a neural network to control an adaptive optics system for an astronomical telescope, Nature, 351, pp. 300-302, (1991)
  • [10] Barrett T K, Sandler D G., Artificial neural network for the determination of Hubble Space Telescope aberration from stellar images, Appl Opt, 32, 10, pp. 1720-1727, (1993)