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DESIGN OF UNOBSCURED REFLECTIVE OPTICAL SYSTEMS WITH GENERAL SURFACES.

机译:具有一般表面的模糊光学系统的设计。

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摘要

Unobscured reflective optical systems can be more transmissive and of higher diffraction quality than classical systems. Unobscured systems are generated by decentering symmetric systems, tilting elements to correct coma or astigmatism along a real ray, or by cross-tilting elements to control astigmatism. Such a system of relatively high quality may be further corrected with a general spline surface. For spline surfaces, optical aberration coefficients are undefined. This study developed real ray analysis and design techniques for general optical systems. A decentered symmetric system with a field correcting spline surface was designed. The optical design program ACCOS V was used for most design and analysis tasks. Design and analysis of general systems are considered first. Basic system quantities of image location, scaling, and irradiation are defined with real rays. Spline surfaces are discussed with special emphasis on features important in optical design. Real ray analytical techniques of composite spot diagrams across the image, footprints on spline surfaces, wavefront aperture maps, and spline surface maps are described. The use of these tools in general system design procedures is discussed. Standard telescope objectives of f/8.5 were considered as base designs for systems with spline surfaces. A spline surface was added to the decentered Schmidt-Cassegrain. Optimization yielded diffraction-limited performance across a 0.85 degree square field. The spline system was compared to the Galileo spacecraft narrow angle lens and a three-mirror decentered design. It had a far wider field than the Galileo but at a lower quality. Diffraction quality was better than that of the three-mirror system. Simple tolerances were considered for the spline system. The allowable effect of a thermal gradient was estimated by bending the reference axis. Decentration and figure tolerances for the spline were commensurate with classical surfaces. Techniques presented were shown to be useful for design and analysis of general systems. Spline surfaces were found to be useful in optimization of such systems. This work was supported by the Director's Discretionary Fund, Jet Propulsion Laboratory, California Institute of Technology.
机译:与经典系统相比,无遮挡的反射光学系统可以更具透射性并且具有更高的衍射质量。通过使对称系统偏心,倾斜元素以校正沿真实光线的彗差或像散,或通过交叉倾斜元素以控制像散,可以生成不模糊的系统。可以用普通的花键表面进一步校正这种质量较高的系统。对于样条曲面,光学像差系数不确定。这项研究开发了用于通用光学系统的真实射线分析和设计技术。设计了具有场校正样条曲面的偏心对称系统。光学设计程序ACCOS V用于大多数设计和分析任务。首先考虑一般系统的设计和分析。图像位置,缩放和辐照的基本系统数量由实际光线定义。讨论样条曲面时特别强调了光学设计中重要的功能。描述了跨图像的合成点图,样条表面上的足迹,波前孔径图和样条表面图的实线分析技术。讨论了这些工具在一般系统设计过程中的使用。 f / 8.5的标准望远镜物镜被认为是具有花键表面的系统的基础设计。将样条曲面添加到偏心的Schmidt-Cassegrain。优化产生了在0.85度方波​​场上衍射受限的性能。样条系统与伽利略航天器窄角镜头和三镜偏心设计进行了比较。它的范围比伽利略大得多,但质量较低。衍射质量优于三镜系统。花键系统考虑了简单的公差。通过弯曲参考轴来估算热梯度的允许效果。花键的偏心度和图形公差与经典曲面相当。所展示的技术被证明对通用系统的设计和分析很有用。发现样条曲面可用于优化此类系统。这项工作得到了加州理工学院喷气推进实验室主任的酌处基金的支持。

著录项

  • 作者

    STACY JOHN ERIC.;

  • 作者单位
  • 年度 1983
  • 总页数
  • 原文格式 PDF
  • 正文语种 en
  • 中图分类

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