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1. 中国科学院 长春光学精密机械与物理研究所,吉林 长春,中国,130033
2. 中国科学院大学 北京,中国,100049
收稿日期:2012-06-17,
修回日期:2012-08-03,
纸质出版日期:2012-10-10
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范磊, 张景旭, 吴小霞, 王富国, 陈夫林, 杨洪波. 大口径轻量化主镜边缘侧向支撑的优化设计[J]. 光学精密工程, 2012,20(10): 2207-2213
FAN Lei, ZHANG Jing-xu, WU Xiao-xia, WANG Fu-guo, CHEN Fu-lin, YANG Hong-bo. Optimum design of edge-lateral support for large-aperture lightweight primary mirror[J]. Editorial Office of Optics and Precision Engineering, 2012,20(10): 2207-2213
范磊, 张景旭, 吴小霞, 王富国, 陈夫林, 杨洪波. 大口径轻量化主镜边缘侧向支撑的优化设计[J]. 光学精密工程, 2012,20(10): 2207-2213 DOI: 10.3788/OPE.20122010.2207.
FAN Lei, ZHANG Jing-xu, WU Xiao-xia, WANG Fu-guo, CHEN Fu-lin, YANG Hong-bo. Optimum design of edge-lateral support for large-aperture lightweight primary mirror[J]. Editorial Office of Optics and Precision Engineering, 2012,20(10): 2207-2213 DOI: 10.3788/OPE.20122010.2207.
对大口径主镜的侧向支撑结构进行了优化
以便最大限度地降低重力作用下的镜面变形。首先
从理论上给出了一种优化主镜边缘侧支撑结构的判据和思路
然后
引入边缘切向剪切侧支撑原理
阐述了这种支撑形式的优化思想和优势。以口径为2060 mm的扇形轻量化主镜作为分析实例
采用16个边缘离散支撑点
优化设计等角间距侧向支撑
并针对轻量化主镜的结构特点和等角间距支撑下支撑力值相差较大的缺点
将等角间距改为不等角间距侧向支撑
分析推导了相应的支撑力公式。结果显示
改进后的支撑形式提高了系统的支撑刚度
镜面变形由原来的1.723 nm降为1.633 nm。所研究的边缘切向剪切支撑方式很大程度上保证了主镜镜面面形
对不同口径的扇形孔轻量化主镜的设计有普适性。
The lateral support structure of a large aperture primary mirror was researched and optimized to effectively reduce the deformation of the primary mirror under the gravity. First
an idea and criterion to optimize the edge-lateral support structure was provided theoretically.Then
on the basis of the tangential shearing support principle
the optimization procedure of the support structure and its merit were explained. Based on the principle
a lightweight mirror with a diameter of 2 060 mm was taken as an example
and an equal-angle lateral support was optimized by using 16 discrete points. According to the characteristic of the lightweight mirror
the original supporting structure was improved to be the no-equal-angle lateral support to avoid the disadvantage that the gap between the support forces was large in previous structure. The results indicate that the supporting stiffness of the system has been enhanced and the mirror deformation is reduced from 1.723 nm to 1.633 nm. It concludes that the edge tangential shearing support structure which is fit to the lightweight mirror with sector hole can keep the mirror surface figure to a large extent. So this method provides a new option for the lateral support of large-aperture lightweight mirror.
王富国,杨洪波,赵文兴,等. 1.2 m SiC主镜轻量化设计与分析[J]. 光学 精密工程, 2009, 17(1):85-91. WANG F G, YANG H B, ZHAO W X, et al.. Lightweight design and analysis of 1.2 m SiC primary mirror [J]. Opts. Precision Eng., 2009,17(1):85-91. (in Chinese)[2] 王洋,张景旭,杨飞. 大口径望远镜主镜支撑系统结构研究[J]. 红外与激光工程, 2006,35(增刊):31-33. WANG Y, ZHANG J X, YANG F. Support structure of large-aperture telescope primary mirror [J].Infrared and Laser Engineering, 2006,35(supp):31-33. (in Chinese)[3] 程景全.天文望远镜原理和设计[M]. 北京:中国科学技术出版社, 2003. CHENG J Q. Principles of Astronomical Telescope Design [M].Beijing: China Science & Technology Press, 2003. (in Chinese)[4] WEST S C,NAGEL R H, HARVEY D, et al.. Progress at vatican advanced technology telescope [J]. SPIE, 1997,2871:73-84.[5] PAUL R.YOUDER. Opto-mechanical System Design [M].Washington: CRC Press, 2006.[6] DAVID S A, JONATHAN K, JOHN M H, et al.. The large binocular telescope primary mirror support control system description and current performance results [J]. SPIE, 2008, 7018:4C1-12.[7] SCHWESINGER G. Lateral support of very large telescope mirrors by edge forces only [J]. Journal of Modern Optics, 1991,38(8):1507-1516.[8] 王洋,张景旭. 大口径望远镜主镜支撑优化分析[J]. 光电工程, 2009, 36(1):108-113. WANG Y, ZHANG J X. Optimization and analysis for the support of the large aperture telescope primary mirror structure of large-aperture telescope primary mirror [J].Opto-Electronic Engineering, 2009, 36(1):108-113. (in Chinese)[9] 闫勇,贾继强,金光. 新型轻质大口径空间反射镜支撑设计[J]. 光学 精密工程,2008, 16(8):1534-1539. YAN Y, JIA J Q, JIN G.Design of new type spaceborne lightweighted primary mirror support [J].Opt. Precision Eng., 2008,16(8):1534-1539. (in Chinese)[10] 郭疆,何欣. 大口径空间遥感相机主反射镜支撑设计[J]. 光学 精密工程,2008, 16(9):1642-1647. GUO J, HE X. Design of support for primary mirror of space remote sensing camera [J].Opt. Precision Eng., 2008, 16(9): 1642-1647. (in Chinese)[11] 崔向群.采用主动光学的大口径单块薄镜面支撑系统. 中科院南京紫金山天文台博士毕业论文,1995. CUI X Q. Support System of Large Aperture Thin Primary Mirror with Active Optics. Najing:Dissertation of doctoral degree, Nanjing observatory, Chinese Academy of Sciences, 1995. (in Chinese)
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