中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
The active support system of LAMOST reflecting Schmidt plate

文献类型:会议论文

作者Dehua Yang; Guoping Li; Xiangqun Cui; Yuefei Wang; Yeping Li; Zhengqiu Yao; Xiaoyu Ni
出版日期2003-02-01
会议日期2002-8-22
会议地点Hawaii USA
关键词Astronomical Telescope Active optics Mirror support system Mirror cell
卷号4837
期号4837
页码Vol.4837 628-636
英文摘要
The reflecting Schmidt plate MA of LAMOST is with 5.7m x 4.4m reflecting area and consists of 24 segmented hexagonal sub-mirrors. Each sub-mirror is 25mm in thickness and 1.1m in diagonal. To correct the spherical aberration of the primary mirror, during observation, the aspherical shape of MA should be changed in every 1.5 minutes. To achieve the good image during observation, the active support system of MA will not only create the correct off-axis aspherical shape on each sub-mirror, but also maintain the co-focus for all 24 sub-mirrors.

This paper presents the studying design with finite element analysis and experiments on the active support system of MA, including its axial and lateral supports, force actuators, optimization of the stiffness of the force actuator, sub-mirror cell, the mirror support structure etc. There are 30 force actuators and three position actuators, which support each sub-mirror and connected by sub-mirror cell. Total 24 sub-mirror cells located on the top of the MA main support structure. All force actuators work as both active and passive supports for each sub-mirror. It showed that the support system is complex but should work properly within the optical requirement.
会议主办者The International Society for Optical Engineering
会议录Large Ground-based Telescopes
会议录出版者SPIE
学科主题郭守敬望远镜(LAMOST) ; 主动光学
源URL[http://ir.niaot.ac.cn/handle/114a32/362]  
专题会议论文
推荐引用方式
GB/T 7714
Dehua Yang,Guoping Li,Xiangqun Cui,et al. The active support system of LAMOST reflecting Schmidt plate[C]. 见:. Hawaii USA. 2002-8-22.

入库方式: OAI收割

来源:南京天文光学技术研究所

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