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The effect analysis of conic coefficient error based on data measured from Talysurf and simulation of Zernike coefficients

机译:基于塔尔郡测量的数据的锥形系数误差与Zernike系数模拟的影响分析

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Derivation of the conic coefficient error of practical aspheric optic surface is quite significant to aspheric machining accuracy, optical system imaging quality analysis and decomposition analysis of optical lenses. The primary mirror of R-c telescope system was tested by Taylor Hobson Talysurf. The practical surface was fitted using Zernike polynomials based on the date measured from Talysurf. Though taking the Zernike coefficients into the optical system, the effect of the aberration which was brought by optical machining to the optical system imaging quality was obtained. The analysis shows that the spherical aberration was brought into the optical system because of the figure error of the primary mirror. And the value of the spherical aberration was same to the practical alignment result. Then the conicoid aspherical degree of the primary mirror was tested by the Talysurf. The machining deviation of the conic coefficient was gotten though comparing the conicoid aspherical degree of the practical primary mirror with that of the perfect primary mirror. The practical conic coefficient was calculated by the deviation. Taking the practical conic coefficient into the R-c telescope system, the degradation of the optical system imaging quality was known. Also the spherical aberration was brought into the optical system. Experimental results show that the value of the spherical aberration analyzed by the two methods is same and consist with the practical alignment result. That is to say that the conic coefficient changed due to machining error of the conicoid aspherical degree. Because of the change the spherical aberration was attached to primary mirror. And which caused the optical system imaging quality declined. Finally, corrector was designed to balance the spherical aberration of the primary mirror. Ensure that the optical system imaging quality meet the requirement.
机译:实际球面光学表面的圆锥系数误差的衍生对于非球面加工精度,光学系统成像质量分析和光学镜片分解分析非常重要。 R-C望远镜系统的主要镜子由Taylor Hobson Talysurf测试。使用基于Talysurf测量的日期,使用Zernike多项式拟合实际表面。虽然将Zernike系数取入光学系统,但是获得了通过光学加工到光学系统成像质量的像差的效果。分析表明,由于主镜的图形误差,球面像差被带入光学系统。球面像差的值与实际对准结果相同。然后通过Talysurf测试初级镜的果皮非球面度。虽然将实用初级镜的与完美初级镜子的Conicoid非球面相比,所以已经获得了圆锥系数的加工偏差。通过偏差计算实际圆锥系数。采用实际圆锥系数进入R-C望远镜系统,已知光学系统成像质量的劣化。也将球形像差进入光学系统。实验结果表明,通过两种方法分析的球面像差的值是相同的,并且由实际对准结果组成。也就是说,由于多半藻非球面度的加工误差,圆锥系数发生变化。由于改变,球面像差与初级镜子连接。并且导致光学系统成像质量下降。最后,校正器旨在平衡主镜的球面像差。确保光学系统成像质量满足要求。

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