首页|深度神经网络在TIE波前探测中的应用

深度神经网络在TIE波前探测中的应用

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提出了一种用于光强传输方程(TIE)波前探测的深度神经网络(DNN)训练模型。该模型的输入为两个不同传输距离的光强分布之差,输出为引起该光强变化的相位畸变对应的4~79阶Zernike系数。对比不同DNN模型下的波前重构精度,最终采用ResNet34骨干网络,提出用于颈网络的线性权重池化方法,并根据任务的物理背景设计了加权平均绝对误差损失函数。仿真结果表明,相较于传统的线性重构方法,DNN可以显著降低TIE波前探测对激光功率的要求,同时有效提升波前探测的精度。当激光功率为 5 W时,DNN的探测精度相当于线性重构方法在激光功率为 200 W时的水平,大大降低了对激光功率的要求(~40倍)。当激光功率超过20 W时,DNN的探测误差约为200 nm RMS,达到79阶Zernike多项式的探测精度上限。
Application of Deep Neural Network in Wavefront Sensing Based on Transport of Intensity Equation
The Transport of Intensity Equation(TIE)offers an effective method for wavefront sensing,utilizing the variations in near-field defocused intensity distribution patterns across multiple propagation distances to reconstruct the phase aberrations introduced by turbulent media,such as the atmosphere.YANG Huizhe et al have explored TIE-based wavefront sensing for satellite-ground laser communication systems,addressing challenges related to the Point-Ahead Angle(PAA).Their simulations and bench experiments,using a Zernike-based linear reconstruction method,demonstrated effectiveness under high Signal-to-Noise Ratio(SNR)conditions.However,linear wavefront reconstruction faces significant nonlinear errors,rendering it ineffective in low SNR environments,which are common in low laser power scenarios typical of laser communication systems.To address these challenges,this paper proposes a Deep Neural Network(DNN)training model.The model utilizes the differences in intensity distributions observed at two distinct propagation distances as the input data.The outputs of the model are the first 4 to 79 orders of the Zernike coefficients corresponding to the phase aberrations.The input and output data used for DNN training are simulated through two processes based on the actual satellite-ground laser communication systems.The first process is the uplink propagation of a collimated laser beam through the atmospheric turbulence,while the second process is the reimaging of the backscattered patterns from these different altitudes.To generate a diverse set of datasets,three variable parameter sets are employed:the atmospheric coherence lengths of 0.05,0.10,and 0.15 meters;the turbulence layer heights of 0,5,and 10 kilometers;and the laser powers of 5,10,20,50,100,200,and 300 watts.This results in 63 unique combinations.Each combination contains 10,000 random phase screens,yielding a total of 630,000 training data.By comparing the Wavefront Errors(WFE)between the original and reconstructed phases,different model architectures,loss functions,and optimizers are evaluated.Ultimately,ResNet34 is chosen as the backbone network.A linear weight pooling method is proposed for the neck network,along with the Weighted Mean Absolute Error(WMAE)function and the SophiaG optimizer.Simulation results provide compelling evidence that the DNN approach significantly outperforms the traditional linear reconstruction methods.Notably,it substantially reduces the laser power requirements essential for effective wavefront sensing.For instance,at a laser power level of 5 W,the reconstruction accuracy achieved by the DNN model matches that of linear methods operating at a substantially higher power of 200 W.Furthermore,as the laser power exceeds 20 W,the detection error for the DNN approach stabilizes at approximately 200 nm RMS,reaching the accuracy limits of the 79th order Zernike polynomial.Moreover,the execution time is also a crucial indicator of its practicality,especially in real-time adaptive optics systems.Testing one thousand datasets on a single PC with an NVIDIA A 5 000 GPU yielded a total processing time of 0.52 seconds for the DNN,resulting in an average processing time of approximately 0.52 milliseconds per dataset,thereby meeting the real-time requirements of adaptive optics systems with a KHz sampling frequency.In contrast,under the same hardware conditions the linear reconstruction method needs approximately 27.31 milliseconds per dataset.The DNN method is about 52 times faster than the linear reconstruction method,highlighting the significant advantages of DNNs in practical applications.Although the DNN method demonstrates excellent performance in wavefront sensing accuracy and execution efficiency,it still has some shortcomings.First,the reliance on training data is a common issue for DNNs.The performance of DNNs is highly dependent on the quality and diversity of the training data.If the actual turbulent conditions differ significantly from the training data,the model's performance can decline sharply.Therefore,it is necessary to further enhance the diversity of the training data to cover a broader range of turbulent conditions and noise levels.Second,the model's interpretability is limited.DNNs are often regarded as black boxes,making their internal decision-making processes difficult to explain using physical laws.In this paper,we designed the linear weight pooling and a weighted mean absolute error loss function based on the physical context of the task.However,further efforts are required to integrate DNNs with the physical models to improve the model's interpretability and robustness.

Wavefront sensingDeep neural networkTransport of intensity equation

杨慧哲、张昊然、刘进、万晶、赵路明、梁永辉

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国防科技大学 前沿交叉学科学院,长沙 410073

国防科技大学 南湖之光实验室,长沙 410073

波前探测 深度神经网络 光强传输

2024

光子学报
中国光学学会 中国科学院西安光学精密机械研究所

光子学报

CSTPCD北大核心
影响因子:0.948
ISSN:1004-4213
年,卷(期):2024.53(12)