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为了实现强噪声干扰下的远场光斑质心高精度计算, 研究了一种基于物理信息神经网络的质心定位方法—质心物理信息神经网络(centroid-PINN), 该方法利用U-Net神经网络优化质心计算误差损失. 为了验证该方法, 利用模拟产生不同强度的两种类型噪声(斜坡噪声和白噪声)干扰下的高斯光斑训练网络. 通过两种类型的光斑(高斯光斑和类Sinc函数光斑)测试神经网络, 均得到了较高的质心定位精度. 相比传统质心定位计算方法, centroid-PINN无需根据噪声水平设置参数, 特别是能够处理斜坡噪声的干扰, 获得高精度定位结果. 成果可用于高性能激光光斑质心参数测量设备的研制, 对于夏克-哈特曼波前测量装置的研制也有一定的借鉴意义.To determine the centroid of far-field laser beam spot with high precision and accuracy under intense noise contamination, a positioning algorithm named centroid-PINN is proposed, which is based on physical information neural network. A U-Net neural network is utilized to optimize the centroid estimation error. In order to demonstrate this new method, Gaussian spots polluted by two kinds of noises, i.e. ramp noise and white noise, are generated by simulation to train the neural network. The neural network is tested by two kinds of spots, i.e. Gaussian spot and Sinc-like spot. Both are predicted with high accuracy. Compared with traditional centroid method, the centroid-PINN needs no parameter tuning, especially can cope with ramp noise interference with high accuracy. This work will be conducive to developing the far-field laser beam spot measurement device, and can also serve as a reference for developing the Shack-Hartmann wavefront sensor.
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Keywords:
- measurement /
- centroid computation /
- neural network /
- adaptive optics
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[1] Booth M J 2014 Light Sci. Appl. 3 165Google Scholar
[2] Ji N 2017 Nat. Methods 14 374Google Scholar
[3] 冯国斌 2014 博士学位论文 (西安: 西安电子科技大学)
Feng G B 2014 Ph. D. Dissertation (Xi’an: Xidian University) (in Chinese)
[4] Andrews L C, Phillips R L 2005 Laser Beam Propagation Through Random Media (Bellingham, Wash: SPIE Press) p4
[5] Ma X, Rao C, Zheng H 2009 Opt. Express 17 8525Google Scholar
[6] 李自强, 李新阳, 高泽宇, 贾启旺 2021 强激光与粒子束 33 081001Google Scholar
Li Z Q, Li X Y, Gao Z Y, Jia Q W 2021 High Power Laser Particle Beams 33 081001Google Scholar
[7] Guo Y, Zhong L, Min L, Wang J, Wu Y, Chen K, Wei K, Rao C 2020 OEA 5 200082
[8] Thomas S, Fusco T, Tokovinin A, Nicolle M, Michau V, Rousset G 2006 Mon. Not. R. Astron. Soc. 371 323Google Scholar
[9] Lardière O, Conan R, Clare R, Bradley C, Hubin N 2010 Proc. SPIE 7736 773627Google Scholar
[10] Akondi V, Steven S, Dubra A 2019 Opt. Lett. 44 4167Google Scholar
[11] Xu L, Wang J, Yao K, Yang L 2021 Opt. Lett. 46 4196Google Scholar
[12] Gilles L, Ellerbroek B L 2008 Opt. Lett. 33 1159Google Scholar
[13] Leroux C, Dainty C 2010 Opt. Express 18 1197Google Scholar
[14] Vyas A, Roopashree M B, Prasad B R 2010 IJCA 1 32
[15] Vargas J, Restrepo R, Estrada J C, Sorzano C O S, Du Y Z, Carazo J M 2012 Appl. Opt. 51 7362Google Scholar
[16] Ding W, Gong D, Zhang Y, He Y 2014 International Conference on Intelligent Computing and Signal Processing Hangzhou, China, Oct. 19–23, 2014 p774
[17] 李晶, 巩岩, 呼新荣, 李春才 2014 中国激光 41 0316002Google Scholar
Li J, Gong Y, Hu X R, Li C C 2014 Chin. J. Laser 41 0316002Google Scholar
[18] 张艳艳, 郝晓龙, 陈洁伟 2015 光学技术 41 59Google Scholar
Zhang Y Y, Hao X L, Chen J W 2015 Opt. Techn. 41 59Google Scholar
[19] Kong F, Polo M C, Lambert A 2017 Appl. Opt. 56 6466Google Scholar
[20] LeCun Y, Bengio Y, Hinton G 2015 Nature 521 436Google Scholar
[21] Montera D A, Welsh B M, Roggemann M C, Ruck D W 1996 Appl. Opt. 35 5747Google Scholar
[22] Mello A T, Kanaan A, Guzman D, Guesalaga A 2014 MNRAS 440 2781Google Scholar
[23] Li Z, Li X 2018 Opt. Express 26 31675Google Scholar
[24] Raissi M, Perdikaris P, Karniadakis G E 2019 J. Comput. Phys. 378 686Google Scholar
[25] Ronneberger O, Fischer P, Brox T 2015 arXiv: 1505.04597
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