中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Structural Analysis of the Reflecting Surface System of a Large Astronomical Telescope

文献类型:期刊论文

作者Yang Dehua; Cui Xiangqun; Gu Bozhong
刊名Chinese Journal of Mechanical Engineering
出版日期2004-03
卷号17期号:3页码:415-419
关键词Astronomical telescope Finite element method Seismic response spectrum
英文摘要The reflecting Schmidt plate system of the large sky area multi-object fiber spectroscopic telescope (LAMOST) serves active optical correction with a reflecting surface of segmented mirror. An azimuth-altitude mounting is adopted with two self-aligning ball bearings for altitude axis and hydrostatic bearings for azimuth. With static and modal analyses, finite element modeling of the full Schmidt plate system is discussed. Conventional seismic response spectrum has been adapted for particular application for telescope engineering before a seismic response spectrum analysis is performed, and results have confirmed that the design of the reflecting Schmidt plate manifests good performance and can survive the seismic intensity of up to 7 magnitude specified by technical requirements. 
学科主题郭守敬望远镜(LAMOST) ; 有限元分析
公开日期2013-12-23
源URL[http://ir.niaot.ac.cn/handle/114a32/389]  
专题期刊论文
推荐引用方式
GB/T 7714
Yang Dehua,Cui Xiangqun,Gu Bozhong. Structural Analysis of the Reflecting Surface System of a Large Astronomical Telescope[J]. Chinese Journal of Mechanical Engineering,2004,17(3):415-419.
APA Yang Dehua,Cui Xiangqun,&Gu Bozhong.(2004).Structural Analysis of the Reflecting Surface System of a Large Astronomical Telescope.Chinese Journal of Mechanical Engineering,17(3),415-419.
MLA Yang Dehua,et al."Structural Analysis of the Reflecting Surface System of a Large Astronomical Telescope".Chinese Journal of Mechanical Engineering 17.3(2004):415-419.

入库方式: OAI收割

来源:南京天文光学技术研究所

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