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首页> 外文期刊>Applied optics >USE OF ARTIFICIAL NEURAL NETWORKS FOR HARTMANN-SENSOR LENSLET CENTROID ESTIMATION
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USE OF ARTIFICIAL NEURAL NETWORKS FOR HARTMANN-SENSOR LENSLET CENTROID ESTIMATION

机译:人工神经网络在哈特曼传感器小透镜质心估计中的应用

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摘要

For adaptive optical systems to compensate for atmospheric-turbulence effects, the wave-front perturbation must be measured with a wave-front sensor (WFS). A Hartmann WFS typically divides the optical aperture into subapertures and then measures the slope of the wave front within each subaperture. Hartmann WFS slope measurements are based on estimating the location of the centroid of the image that is formed from a guide star within each subaperture. Conventional techniques for centroid estimation involve the use of a Linear estimator and conversion tables. Neural networks provide nonlinear solutions to this problem. We address the use of neural networks for estimating the location of the centroid fi om the subaperture image. We find that neural networks provide more accurate estimates over a larger dynamic range and with less variance than do the conventional linear centroid estimator. [References: 18]
机译:对于补偿大气湍流效应的自适应光学系统,必须使用波前传感器(WFS)测量波前摄动。 Hartmann WFS通常将光学孔径分为多个子孔径,然后测量每个子孔径内的波前斜率。 Hartmann WFS斜率测量基于估计由每个子孔径内的引导星形成的图像质心的位置。用于质心估计的常规技术涉及使用线性估计器和转换表。神经网络为该问题提供了非线性解决方案。我们解决了使用神经网络估计子孔径图像质心的位置的问题。我们发现,与传统的线性质心估计器相比,神经网络在较大的动态范围内提供更准确的估计,并且方差较小。 [参考:18]

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