共查询到17条相似文献,搜索用时 359 毫秒
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由于Zernike环多项式各项在环域上正交,以此为基准可以得到Zernike圆多项式拟合环孔径波面求解Seidel像差系数的误差。为了对Zernike圆多项式与环多项式求解的Seidel系数进行准确的比较,根据波像差理论推导并建立对比实验模型,进行量化比较。比较对于具有较大遮拦比的环孔径波面采用Zernike环多项式拟合与采用Zernike圆多项式拟合求取Seidel系数的差别。实验结果表明,采用Zernike圆多项式进行拟合求取Seidel系数时,主要的相对误差存在于离焦、球差和慧差。9项Zernike圆多项式拟合求取的Seidel系数比36项Zernike圆多项式更接近Zernike环多项式求取的系数。同时,如果参与拟合的项数继续减少,求取的Seidel误差反而增大。 相似文献
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针对非圆域波面拟合中Zernike多项式失去正交特性、拟合系数交叉耦合的问题,提出非圆域Zernike正交基底函数构造方法。以圆Zernike为基底,采用Gram-Schimdt正交组构造方法,线性表出单位正交基底。通过构造不同遮光比环形光阑下的正交基底与环Zernike多项式进行比较,验证了此方法的正确性。然后采用圆Zernike多项式和构造的新基底对矩形光阑下的波面进行了拟合,从拟合残余误差、各项基底系数的稳定性、传递矩阵的条件数等分析,结果表明针对特定的非圆域构造的新基底可靠性和抗扰动能力优于圆Zernike多项式。此方法不需要具体求出基底的解析表达式,不同非圆域仅是正交化系数矩阵发生改变,为非圆域正交基底构造提供了一种新途径。 相似文献
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于晓光 《中国光学与应用光学文摘》2006,(1)
TB922006010672基于Zernike多项式进行波面拟合研究=Study on wave-front fitting using Zernike polynomials[刊,中]/张伟(哈尔滨工业大学空间光学工程研究中心.黑龙江,哈尔滨(150001)),刘剑峰…∥光学技术.—2005,31(5).—675-678基于Zernike多项式利用Householder变换法对不同空间频率径向误差和不同口径局部误差进行了拟合,得到了拟合误差的均方根(RMS)值,分析了Zernike多项式的局限性。结果表明,Zernike在拟合径向误差时,受到最大空间频率的限制;在拟合局部误差时要受到局部误差口径大小的限制,并且会引起额外的波动。图7参8(于晓… 相似文献
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《光学学报》2016,(3)
以随机相位屏构造光束波前畸变模型,运用不同阶数的Zernike多项式对其进行拟合。通过对比分析原始波前及拟合波前的功率谱密度,明确了波面拟合过程中Zernike多项式对波前中高频成分拟合存在的不足,进而提出了基于Zernike多项式的分块拟合方式加以改进。研究结果表明:在常规的拟合方式下,随着拟合阶数的增加,能准确反映的波前相位空间频率逐渐向高频范围扩展,但其扩展幅度并不大;此外,即使采用较高的拟合阶数,Zernike多项式也难以准确反映波前空间频率中的高频成分;而采用分块拟合方式后,Zernike多项式的拟合效果明显提升,并能有效反映畸变波前空间频率中的高频成分;在提高波面拟合精度上,增加分块数的效果明显优于增加Zernike多项式拟合阶数;对于分块拟合方式,当分块数一定时,增大子区域拟合所使用的Zernike阶数的拟合效果明显优于增大整体拟合所使用的Zernike阶数。 相似文献
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基于泽尼克多项式进行面形误差拟合的频域分析 总被引:3,自引:3,他引:0
获得泽尼克多项式的频谱信息是正确利用该多项式进行误差拟合的关键。推导出了泽尼克多项式的傅里叶变换公式,在频域中分析了不同阶数该多项式的径向频谱信息和幅角频谱信息,得到了有限项泽尼克多项式能够有效表达面形误差的最大径向空间频率和角频率。基于频域分析理论,利用泽尼克多项式对不同口径局部误差进行了拟合,并利用齐戈(Zygo)干涉仪对带有不同面形误差的光学元件进行了试验分析。结果表明,当误差的径向空间频率或角频率超出泽尼克多项式所能表达的频谱范围时,拟合误差迅速变大。 相似文献
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本文就专著和文献中关于Zernike多项式拟合干涉波面几乎都建设采用Gram-Schimdt正交化方法,而不采用比较简单的传统经典的最小二乘法问题进行了深入研究,从理论和实践上严格地证明了两种方法的等价性。实践中发现,用最小二乘法求解Zernike多项式拟合系数的速度比用Gram-Schimdt正交化方法提高了三倍之多。由于在精密光测技术中,Zernike多项式已被广泛采用,因此,“等价性”的证明具有重要意义,并对于其它类似问题也有着普遍的参考价值。 相似文献
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A new method is proposed to simulate the Kolmogorov phase screen. A hybrid phase screen is achieved by linearly combining two phase screens simulated by both spectral and Zernike polynomials methods. Unlike the imperfection of phase structure function existing at some spatial frequencies in each of the two methods, the mean structure function of the hybrid phase screens coincides remarkably well with theory in the whole spatial frequency domain. Apart from advantage on accuracy, the proposed method also saves considerable computational time. For a phase screen with certain accuracy, the new method is ten times and seven times faster compared with the spectral method and Zernike polynomials method, respectively. 相似文献
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1 Introduction Weoftendescribethestaticordynamicwavefrontaberrationsascombinationofdifferentmodes,suchaspiston ,tilt,defocus,coma,spheralandsoon .ThesemodesaresimilarassomelowerordersofZernikepolynomials.TheZernike polynomialsarenormalizedorthogonalincir… 相似文献
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The theory of orthogonal polynomial (Zernike) expansions of functions on a disk, as used in the diffraction theory of optical aberrations, is applied to obtain (semi-) analytical expressions for the spatial impulse responses arising from a non-uniformly moving, baffled, circular piston. These expressions are in terms of the expansion coefficients of the non-uniformity and the responses of the orthogonal expansion functions. The latter impulse responses have a closed form as finite series involving the Legendre functions and the sinc function. The method is compared with a similar method, proposed by P. R. Stepanishen [J. Acoust. Soc. Am. 70, 1176-1181 (1981)] where zeroth order orthogonal Bessel functions, rather than Zernike polynomials, are used as expansion functions. 相似文献
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A “practically applicable” spot images based aberration retrieval method was developed. The method was systemized with the
following techniques. 1) The real part and imaginary part of the spatial spectrum of the focal plane were expanded with the
finite lower Zernike polynomials, respectively, and the method was reduced to the nonlinear least squares problem which calculates
these coefficients. This technique will identify both the aberration and the intensity distribution of the spatial spectrum.
2) The intensity distributions of spot images were calculated using the Nijboer-Zernike polynomials in order to avoid a long
calculation time and the numerical errors caused by Fourier transform or convolution. 3) Two noise reduction methods were
applied to the present method, and some numerical and practical experiments were performed to demonstrate the technique’s
effectiveness. Four kinds of practical experiment based on theories were performed, and all of them showed good agreement
with the theories. 相似文献