Modeling and Analysis of LAMOST Primary Mirror Support Structure
Xuefei Gong ; Xiangqun Cui
2002-07-30
会议日期2002-5-2
会议地点Lund, Sweden
关键词Astronomical Telescope Structural Analysis Mirror Support Structure
卷号4757
期号4757
页码Vol.4757 138-144
英文摘要
The Large Sky Area Multi-object Fiber Spectroscopic Telescope (LAMOST) is a national large scientific project in China at the beginning of this century. It is an unconventional designed modern optical telescope and has the both large field of view and large aperture. The spherical primary mirror MB in LAMOST is a segmented mirror with 37 sub-mirrors. The MB will be supported by a very stable truss structure and the mirror surface will be kept in a high optical accuracy.

This paper presents the work on the finite element model of the truss structure of MB and gives the results of static and dynamic analysis with this model especially for the optimization ofthe higher stiffness and the lighter weight.
会议主办者Society of Photo-Optical Instrumentation Engineers
会议录Integrated Modeling of Telescopes
会议录出版者SPIE
学科主题郭守敬望远镜(LAMOST) ; 天文技术与方法
内容类型会议论文
源URL[http://ir.niaot.ac.cn/handle/114a32/343]  
专题南京天文光学技术研究所_中科院南京天光所知识成果_会议论文
南京天文光学技术研究所_望远镜新技术研究室_会议论文
推荐引用方式
GB/T 7714
Xuefei Gong,Xiangqun Cui. Modeling and Analysis of LAMOST Primary Mirror Support Structure[C]. 见:. Lund, Sweden. 2002-5-2.
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