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Simulation and optimization for a computer-controlled large-tool polisher 计算机控制的大型刀具抛光机的仿真与优化
Pub Date : 1900-01-01 DOI: 10.1364/oft.1998.omd.2
J. Burge
Large aspheric mirrors are ground and polished at the Steward Observatory Mirror Lab (SOML) using stressed-lap polishers under computer control.1,2 Stressed-lap polishing uses large stiff circular polishing tools, which are actively deformed under computer control forcing the lap to continually fit the aspheric mirror surface. The size of the tool is typically one-third to one-sixth the diameter of the minor. As the lap is translated across the rotating minor, the lap's horizontal speed and rotation rate, the total force on the lap, and applied moments to the lap are all dynamically controlled. In order to take full advantage of these many degrees of freedom, computer simulation and optimization software has been developed. The simulation is based on Preston's relation (local removal rate proportional to pressure and relative velocity) but allows the inclusion of non-linear effects based on measured results. The optimization of polishing parameters is accomplished by a damped least squares optimization algorithm which varies the polishing parameters to obtain a desired simulated removal profile. This software has been successfully used at SOML to guide grinding and polishing of numerous large primary and secondary telescope mirrors.3 The software was developed for the stressed lap polishers at the University of Arizona, but it can be used with equal effectiveness for other types of polishers.
大型非球面镜面在Steward天文台镜面实验室(SOML)使用计算机控制下的应力lap抛光机进行研磨和抛光。1,2应力搭接抛光采用大型刚性圆形抛光工具,在计算机控制下进行主动变形,迫使搭接连续贴合非球面镜面。工具的尺寸通常是小管柱直径的三分之一到六分之一。当圈圈在旋转的小赛道上平移时,圈圈的水平速度和旋转速率、圈圈上的总力以及圈圈上的力矩都是动态控制的。为了充分利用这众多的自由度,人们开发了计算机仿真和优化软件。模拟基于Preston关系(局部去除率与压力和相对速度成正比),但允许包含基于测量结果的非线性效应。抛光参数的优化是通过阻尼最小二乘优化算法来实现的,该算法通过改变抛光参数来获得所需的模拟去除轮廓。该软件已成功应用于SOML,指导了许多大型望远镜主镜和副镜的研磨和抛光该软件是为亚利桑那大学的应力搭接抛光机开发的,但它也可以用于其他类型的抛光机。
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引用次数: 0
New NC Data Generating Method Including Tool Wear Compensation in ELID (Electrolytic In-Process Dressing) Grinding 电解加工中刀具磨损补偿的数控数据生成新方法
Pub Date : 1900-01-01 DOI: 10.1364/FTA.1999.GA2
S. Moriyasu, Y. Yamagata, H. Ohmori
Recent demands for ultraprecision machining has been for higher precision. The ELID grinding technique is widely known as a method which produces high precision ground surfaces in a short period of time.1) Aspherical optics, one typical example of super precision parts, require not only good mirror surface finish but also high form accuracy.2) But it involves considerable difficulty to achieve both good mirror surface finish and high form accuracy. The authors have proposed a new form control system for achieving high form accuracy regularly and efficiently in aspherical ELID grinding, and successful results could be obtained through some experiments3),4). But there had been some conditions, under which the profile errors could not converge because the radius of the grinding wheel decreased by the wear. This paper proposes a new form compensation method which can be applied to the condition under which the grinding wheel is much worn.
最近对超精密加工的要求是更高的精度。ELID磨削技术是一种在短时间内获得高精度磨削表面的方法。1)非球面光学器件是超精密零件的典型代表,它不仅要求镜面光洁度好,而且要求形状精度高。2)镜面光洁度好,形状精度高,但要同时实现镜面光洁度好和形状精度高,难度很大。作者提出了一种新的形状控制系统,可以在非球面ELID磨削中实现有规律、高效的高形状精度,并通过一些实验获得了成功的结果(3),4)。但在一定条件下,由于磨耗使砂轮半径减小,使齿形误差不能收敛。本文提出了一种新的形式补偿方法,适用于砂轮磨损严重的情况。
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引用次数: 0
Image Acquisition for High Accuracy Interferometry 高精度干涉测量的图像采集
Pub Date : 1900-01-01 DOI: 10.1364/oft.1998.owc.2
G. Campbell, G. Sommargren, B. Truax
In phase shifting interferometry, the image acquisition electronics have largely been ignored, because the overall measurement accuracy has generally been limited by the quality of the reference wave. A recently developed interferometer, the phase shifting diffraction interferometer,[1] provides a high quality reference wave, which has been measured to be better than λ/8000 rms. With such a reference wave, the interferometer accuracy then becomes limited by systematic errors in the image acquisition electronics. This paper presents a variety of issues that arise when using image acquisition electronics of the sort commonly used in commercial interferometers. A basic fiber interferometer that isolates electronics issues is described, as are simple solutions to some of the errors.
在相移干涉测量中,由于整体测量精度通常受到参考波质量的限制,图像采集电子在很大程度上被忽略了。最近开发的一种干涉仪,相移衍射干涉仪[1]提供了高质量的参考波,测量结果优于λ/8000 rms。有了这样一个参考波,干涉仪的精度就会受到图像采集电子系统误差的限制。本文介绍了在使用商业干涉仪中常用的那种图像采集电子器件时出现的各种问题。描述了一种隔离电子问题的基本光纤干涉仪,以及一些误差的简单解决方案。
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引用次数: 0
Fabrication of Deep Concave Glass Micro Lens by ELID Grinding ELID磨削加工深凹玻璃微透镜
Pub Date : 1900-01-01 DOI: 10.1364/oft.1998.omc.4
Yutaka Yamgata, S. Moriyasu, S. Morita, H. Ohmori, T. Higuchi
Due to the progress in fiber optics, optical storage systems and portable information devices, fabrication technologies for micro optical components becomes more and more important. The fabrication process of micro optical componets especially deep concave glass micro lens is facing a number of diffculties: (1)Since the diameter of the micro optical component is very small and the depth of the surface is large, the grinding wheel must have even samller diameter. (2)In order to obtain optimum cicumference speed, the rotation speed of the grinding wheel becomes extremely high. In order to overcome those problems, inclined grinding wheel can be used to cut the deep concave surface. This method solves the first problem but still extremely high rotation speed is necessary. The authors present a new resolution to those problems using ELID (ElectroLytic In-process Drssing) grinding method. Using ELID grinding, the grinding wheel is continuously dressed during the machininig process and always kept sharpened. This results in a very high quality surface finish even under low circumference speed. Fabrication example of glass micro concave lens (radius:4.6mm) is carried out with small grinding wheel (diameter 5mm) at relatively low rotation speed of 20,000 rpm, which is equivalent to 300m/min circumference speed. Surface roughness of 40nmp-ν and profile accuracy of approximately 1μm was obtained.
随着光纤、光存储系统和便携式信息器件的发展,微光器件的制造技术变得越来越重要。微光学元件特别是深凹玻璃微透镜的制造工艺面临着诸多困难:(1)由于微光学元件的直径很小,表面深度又很大,因此砂轮的直径必须更小。(2)为了获得最佳的周长速度,砂轮的转速变得极高。为了克服这些问题,可以采用倾斜砂轮切割深凹面。这种方法解决了第一个问题,但仍然需要极高的旋转速度。作者提出了一种新的解决这些问题的方法,即ELID (electrotic In-process dressing)磨削法。采用ELID磨削,使砂轮在加工过程中不断修整,始终保持锋利。这导致一个非常高质量的表面光洁度,即使在低周长速度。利用直径5mm的小砂轮,以相对较低的转速20000转/分,相当于300米/分钟的圆周速度,进行了玻璃微凹透镜(半径4.6mm)的加工实例。获得了40nmp-ν的表面粗糙度和约1μm的轮廓精度。
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引用次数: 0
A New Ion Exchange Technique for Fabricating Radial GI lenses 一种制备径向GI透镜的离子交换新技术
Pub Date : 1900-01-01 DOI: 10.1364/oft.1988.fb4
Yoshikazu Kaite, M. Toyama, I. Kitano
The ion exchange technique is widely used to produce radial gradient-index lenses, however, has a disadvantage for fabricating much larger ones. It probably takes hundreds days to make the lenses with 20 mm in diameter using this technique. In large scale imaging systems, such large radial gradient-index lenses are required.
离子交换技术被广泛用于制造径向梯度折射率透镜,然而,它在制造更大的透镜时有一个缺点。使用这种技术制造直径20毫米的镜片可能需要数百天。在大尺度成像系统中,需要如此大的径向梯度折射率透镜。
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引用次数: 0
Fabrication of an Optical Heterodyne Profilometer 光学外差轮廓仪的研制
Pub Date : 1900-01-01 DOI: 10.1364/oft.1988.tha5
M. George, H. Jagannath, B. R. Reddy, G. Perera, P. Venkateswarlu
An optical heterodyne profilometer was fabricated for the measurement of surface roughness. Briefly, when two beams of slightly different frequencies are reflected from two different points on the surface, the phase of the resulting sinusoidal interference signal is related to the height difference between the two points, whose absolute value is estimated by comparing it with the phase of a reference signal, but no reference surface is involved.1
制作了一种测量表面粗糙度的光学外差轮廓仪。简而言之,当两束频率略有不同的波束从表面上的两个不同点反射时,得到的正弦干涉信号的相位与两点之间的高度差有关,通过与参考信号的相位比较来估计其绝对值,但不涉及参考表面
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引用次数: 0
Measurement of the homogeneity of optical materials 光学材料均匀性的测量
Pub Date : 1900-01-01 DOI: 10.1364/oft.1990.othb4
G. C. Hunter, L. J. Sutton
The measurement of the homogeneity of optical materials is discussed. Methods and equipment for evaluation of both polished and unpolished material samples are described.
讨论了光学材料均匀性的测量方法。描述了评估抛光和未抛光材料样品的方法和设备。
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引用次数: 1
The Importance of Standards for the U.S. Optics Industry 标准对美国光学工业的重要性
Pub Date : 1900-01-01 DOI: 10.1364/oft.1996.owb.1
Gene Kohlenberg
The Optics and Electro-Optics Standards Council (OEOSC) has been formed to help the U.S. take a more active role in the development, maintenance, and administration of U.S. optics and electro-optics standards, and participate in international standards activities under ISO (International Organization for Standardization). Optics and electro-optics standards activities in the U.S. are in a time of crisis. Without support from U.S. optics and electro-optics companies, these communities will be unable to participate in the world market, and will find it progressively more difficult to engage in domestic production and sales.
光学和电光标准委员会(OEOSC)的成立是为了帮助美国在发展、维护和管理美国光学和电光标准方面发挥更积极的作用,并参与ISO(国际标准化组织)下的国际标准活动。美国的光学和电光标准活动正处于危机时期。如果没有美国光学和光电公司的支持,这些社区将无法参与世界市场,并将发现越来越难以从事国内生产和销售。
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引用次数: 0
Null correctors for 6.5-m f/1.25 paraboloidal mirrors 用于6.5 m f/1.25抛物面镜的零校正器
Pub Date : 1900-01-01 DOI: 10.1364/FTA.1999.FT5
J. Burge, L. Dettmann, S. West
The instruments used to interferometrically measure the optical surfaces of the 6.5-m f/1.25 primary mirrors for the University of Arizona telescope projects must compensate over 800 μm surface departure from the best fitting sphere. The errors in the optical test must not contribute more than 0.04 arc seconds FWHM to the final image and the conic constant must be held to 0.01%. This paper presents an overview of the instruments used to measure these giant mirrors to such high accuracy.
亚利桑那大学望远镜项目中用于干涉测量6.5 m f/1.25主镜光学表面的仪器必须补偿与最佳拟合球的表面偏差超过800 μm。光学测试中的误差对最终图像的贡献不得超过0.04角秒FWHM,并且圆锥常数必须保持在0.01%。本文概述了用于测量这些巨镜的仪器,以达到如此高的精度。
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引用次数: 10
Innovative Optics for Giant Telescopes 巨型望远镜的创新光学
Pub Date : 1900-01-01 DOI: 10.1364/FTA.1999.FT4
H. Martin
The present decade is an unprecedented period of expansion in the collective power of ground-based optical and infrared telescopes worldwide. No fewer than 13 telescopes between 6.5 m and 10 m in diameter--all larger than the most powerful telescope available before 1990--will be completed by roughly the year 2000. Some of these telescopes are designed with specific scientific goals in mind, such as high-resolution infrared imaging and spectroscopy, while others are multi-purpose instruments designed to serve the needs of an astronomical community whose observations have been limited by collecting area and resolving power for several decades. The projects are listed below.
目前的十年是全球地面光学和红外望远镜集体力量空前扩张的时期。不少于13架直径在6.5米到10米之间的望远镜——都比1990年以前最强大的望远镜要大——将在大约2000年完工。其中一些望远镜是为特定的科学目标而设计的,比如高分辨率红外成像和光谱,而另一些则是多用途仪器,旨在满足天文团体的需要,这些天文团体的观测几十年来一直受到收集面积和分辨率的限制。项目列表如下。
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Optical Fabrication and Testing
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