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大口径主镜的侧向定位系统

原帅 张景旭 王富国 刘祥意

光学精密工程2017,Vol.25Issue(10):2564-2571,8.
光学精密工程2017,Vol.25Issue(10):2564-2571,8.DOI:10.3788/OPE.20172510.2564

大口径主镜的侧向定位系统

Lateral positioning system for large aperture primary mirror

原帅 1张景旭 2王富国 1刘祥意1

作者信息

  • 1. 中国科学院长春光学精密机械与物理研究所,吉林长春130033
  • 2. 中国科学院大学,北京100049
  • 折叠

摘要

Abstract

To locate accurately a large aperture primary mirror with balance weight support and Whif-fletree support in the primary mirror cell ,a lateral positioning method for the large aperture primary mirror was proposed based on the kinematic constraint .The principle of kinematic constraint was in-troduced ,a design scheme of lateral positioning system for the primary mirror was proposed including the selection of location points and the design of flexure hinges and location bases ,and then a lateral positioning system was implemented .With finite element method ,the influences of the lateral positio-ning system on the large aperture primary mirror system was analyzed in several aspects ,such as sys-tem location ,resonant frequency and mirror surface profile .As the results ,it shows that the resonant frequency of the primary mirror reaches 13 .6 Hz ,the average displacement of the primary mirror is-355 .863 nm along the Y-axis direction , and the primary mirror surface profile is uninfluenced .These parameters all meet the design requirements of this lateral positioning system .Experimental re-sults verify the engineering signification of proposed lateral positioning system on the design of sup-port and position systems of primary mirror in large aperture telescopes in the future .

关键词

大口径主镜/定位/运动学约束/谐振频率/面形精度

Key words

large aperture primary mirror/positioning/kinematic constraint/resonant frequency/sur-face profile

分类

机械制造

引用本文复制引用

原帅,张景旭,王富国,刘祥意..大口径主镜的侧向定位系统[J].光学精密工程,2017,25(10):2564-2571,8.

基金项目

国家自然科学基金资助项目(No.11403023) (No.11403023)

光学精密工程

OA北大核心CSCDCSTPCD

1004-924X

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