共查询到19条相似文献,搜索用时 453 毫秒
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基于Hwey-Lan Liou人眼生理模型,采用光线追迹的方法,分析了相同孔径下具有不同球差的人工晶体(IOL)在眼内的倾斜和偏心对人眼视功能的影响.IOL在眼内无倾斜和偏心时,负球差IOL对人眼视功能的改善优于无球差IOL和传统的正球差IOL;当IOL在眼内倾斜,偏心程度一定时,负球差IOL球差值越大,其倾斜和偏心对人眼视功能的降低越明显;植入无球差IOL的眼的视功能受其倾斜和偏心的影响较小,在IOL偏心1.0 mm,倾斜10°已使人眼有明显视觉不适的情况下,仍能表现出良好的光学性能,对人眼视功能的改善不仅优于正球差IOL,而且优于负球差IOL. 相似文献
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随着航天遥感需求的不断提高,光学遥感器的口径越来越大,光学元件的支撑和重力变形对光学系统的影响难以消除,因此需要在轨调整光学元件位置变量,来补偿主镜面形误差引起的系统光学性能的下降。以一个大口径同轴三反射式光学系统为例,在理论上分析了次镜的倾斜、偏心和轴向位置引起的初级像差的变化,得出次镜的在轨补偿能力。利用Zernike多项式模拟主镜面形误差,通过调整次镜的位置自由度,分别补偿主镜的球差、彗差和像散,给出了仿真结果,并进行了工程可实现性分析。结果表明,次镜的位置自由度调整能够补偿主镜的彗差,并能够补偿一定量的像散,但是只能补偿小量球差。 相似文献
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<正> 经典的朗奇测试曾广泛地用于光学检验。以往这种技术都作为定性的测量,这主要是因为朗奇图形用解析处理比较困难。现在采用光栅干涉的观点,可以得到象差的测量表示式。对朗奇图上为数很少的几个特征值进行测量,就可以求出球差和彗差的波差值。朗奇体系本 相似文献
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《中国光学与应用光学文摘》2005,(1)
TH703 2005010039 偏心和倾斜光学系统初级像差理论的研究=Study on the primary aberration theory of decentered and tilted optical system[刊,中]/樊学武(中科院西安光机所空间光学室. 陕西,西安(710068)),陈荣利…∥光子学报.-2004,33 (4).-494-496 在共轴光学系统波像差的基础上,推导出了光学元件的偏心和倾斜分别对主要像差的影响。得出了除了球差 相似文献
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《物理学报》2020,(1)
利用涡旋光束作为空间光通信载波可以大大提高数据传输的容量,因此,研究涡旋光束在大气湍流中的传输具有重要意义.涡旋光束在大气湍流中传输时会产生光束漂移,进而影响通信系统的性能.本文基于多相位屏和傅里叶变换的方法,研究了带有彗差和球差的涡旋光束在大气湍流中传输时的光束漂移特性.结果表明,涡旋光束在大气湍流中传输时,随着传输距离的增大,彗差和球差对光束漂移特性的影响均明显增强.传输天顶角及彗差系数越大,涡旋光束的光束漂移量越大,而球差系数的增大,将会降低光束漂移量.当天顶角和传输距离相同时,涡旋光束的漂移量都会随着拓扑荷数的增大而减小.相对而言,彗差对涡旋光束的光束漂移特性影响比球差更大. 相似文献
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本文叙述了菲涅尔透镜的一种新型象差——线彗差及这种象差的特性和其他象差的关系。薄平菲涅尔透镜是一步彩虹全息中较理想的成象透镜。 相似文献
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The aberration field of an optical system with a tilted pupil is explored through expanding the vector expressions of the third-order wavefront aberrations. First, the vector forms of the wavefront aberrations are modified to obtain the aberration expressions with the pupil tilted; full field displays of coma and astigmatism in this situation are given. Then, the third-order aberration formulas with the pupil decentered and tilted simultaneously are derived and discussed. Finally, an example is taken to certify the validity of aberration distribution properties. 相似文献
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折射率失配对双光子三维光存储中像差的影响 总被引:5,自引:3,他引:2
双光子吸收三维光信息存储是实现高密度光存储的重要方法。三维数据写入过程中光束需经过两层不同的介质(如空气和存储材料),对像差和存储效果产生很大的影响,因此在理论和实验上分析系统各项光学参量对折射率失配引起的像差和存储效果的影响具有很大的意义。首先建立光学存储系统模型,在平行平板条件下,利用波像差函数推导展开,获得五项初级(赛德耳)像差,即球差、彗差、像散、场曲、畸变,然后对于存储材料在水平和倾斜两种情况下对初级像差进行模拟计算与分析,理论模拟与实验表明:物镜的数值孔径越大,像差随着存储深度增加而增大的速度就越快。 相似文献
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根据波像差理论,推导了光学合成孔径成像系统单个子孔径存在各种像差时波面方差与子孔径数(N)的关系。推导结果表明,piston误差对系统的影响最大,其次是离焦误差、倾斜误差、球差、彗差和像散。运用离焦误差对piston误差、球差和像散进行像差平衡,其效果显著,特别是球差引起的波面方差下降90%。系统各项像差系数随子孔径数的增加而降低;当子孔径数大于6时,各像差系数变化缓慢。根据瑞利判据,计算N(N≤6)个子孔径合成系统的像差允限和相应的3孔径系统的斯特列尔比。 相似文献
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Expressions for third-order aberration in the reconstructed wave front of point objects are established by Meier. But Smith,
Neil Mohon, Sweatt independently reported that their results differ from that of Meier. We found that coefficients for spherical
aberration, astigmatism, tally with Meier’s while coefficients for distortion and coma differ. 相似文献
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Imaging by two concentric spheres is studied by geometrical method. As the system is symmetric with respect to the common center of curvature, peripheral aberrations, namely coma, astigmatism, and distortion, do not appear. The imaging surface is a sphere that shares the center of curvature with two mirrors. As we solve the zero spherical aberration condition for imaging of an object at infinite distance, the golden section number appears as the ratio of the distance between two mirrors and the radius of the primary mirror. For imaging of an object at finite distance, we have to increase the radius of the second mirror. This system also has no peripheral aberrations. Making the object surface spherical, we can obtain a flat image surface. As the spherical aberration is zero in the original system, spherical aberration, coma, and astigmatism remain zero when the object surface is curved. 相似文献
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According to the structural characteristics of aspheric off-axis two-mirror optical system, the imaging characteristics of the system were analyzed by using primary aberration theory. Based on the characteristics of different aspheric surfaces, the vector expression of system aberrations was derived. Using the Seidel coefficients, the primary wave aberration of systems were expanded and values of system aberration for different aspheric surface shapes were specifically calculated. After the evaluation index of the off-axis structure was determined, the imaging qualities of different surface shape combinations were compared. Then the optimal surface shape selection method was analyzed by quantitative comparison results. The results show that compared with other reflector combination methods, the spherical aberration, coma and astigmatism of the off-axis double paraboloid system are all 0, the wavefront RMS is much better than λ/14 (λ=0.587 6 μm), and the Strehl ratio is greater than 0.8. According to the calculation results, it not only has a stronger ability to suppress multiple primary aberrations, but also can effectively compress the volume of the system. Copyright ©2022 Journal of Applied Optics. All rights reserved. 相似文献
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红外热成像鱼眼镜头设计中若干特殊问题的处理 总被引:7,自引:1,他引:7
提出鱼眼镜头光阑球差的级数表达式及其基于有限差分的近似计算方法,解决了通常的光阑倒追方法面临的难题;讨论孔径光阑与入瞳的特殊"共轭"关系,分析了光阑彗差和像差渐晕;运用Aitkin插值技术填补"溢出"光线在像面上的落点,以保证像质函数定义的一致性,维持自动优化持续进展,从而克服频繁的光线"溢出"造成的严重困难;提出充分利用像差渐晕改善像面照度均匀性的方法;论述标定轴外光束边界的逐次渐近过程和运用入瞳距离变量实现孔径光阑位置全域优化的技术. 相似文献