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Research on mirror lateral support of large astronomical telescope
Xuefei Gong; Xiangqun Cui
2006-05-30
会议录名称Advanced Optical Manufacturing and Testing Technologies: Large Mirrors and Telescopes
卷号6148
期号6148
页码Vol.6148 0Y-1-6
会议日期2005-11-2
会议地点Xian, China
会议主办者The International Society for Optical Engineering
出版者SPIE
摘要
Mirror support system of astronomical telescope is composed of axial support and lateral support. In traditional telescope, because the contribution of lateral support to surface distortion is less than axial support, there are usually few lateral support methods such as lever counterweight, hydrostatic pressure and steel strap in the past. With increase of
diameter to thickness ratio and use of strongly concave mirrors, lateral support is becoming more complicated and important than before. At the same time, application of segmented mirror make it impossible to support periphery of mirror, so, some new schemes have been designed to meet requirement of large segmented-mirror telescope. This paper introduces some classic and recent methods of lateral support for large telescope and gives some results of finite element analysis.
关键词Astronomical Telescope Mirror Lateral Support Finite Element Analysis
学科领域天文技术与方法
文献类型会议论文
条目标识符http://ir.niaot.ac.cn/handle/114a32/452
专题会议论文
推荐引用方式
GB/T 7714
Xuefei Gong,Xiangqun Cui. Research on mirror lateral support of large astronomical telescope[C]:SPIE,2006:Vol.6148 0Y-1-6.
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