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Analysis and optimization of a 2.5m telescope mount
Guomin Wang; Zhiyong Zhang; Bozhong Gu
2008-07-14
Source PublicationAdvanced Optical and Mechanical Technologies in Telescopes and Instrumentation
Volume7018
Issue7018
PagesVol.7018 47-1-10
Conference Date2008-6-23
Conference PlaceMarseille, France
Funding OrganizationThe International Society for Optical Engineering
PublisherSPIE
Abstract
For an astronomical telescope mount, having a high stiffness to support the mirror cell and instruments is its basic function. Traditionally, the mount is composed of azimuth base, azimuth axis, fork, altitude axis, tube, top-ring, etc. On the other hand, telescope will be driven to track the observing objects during operation. So, for the mechanical structure
design engineer, finding a high stiffness-to-weight ratio mount is the main task. Finite element method (FEM) is a powerful tool to help structure design engineer to achieve this goal. ANSYS is one of these kinds of finite element method software. In this paper, with the help of ANSYS, the static and dynamic analysis, calculation and optimization of  a 2.5m telescope mount will be given. The FEM results show that the structure, designed for 2.5m telescope, is feasible and reliable and have a high stiffness-to-weight ratio to meet the optical demands.
KeywordTelescope Structure Design Fem Optimization
Subject Area天文技术与方法
Document Type会议论文
Identifierhttp://ir.niaot.ac.cn/handle/114a32/543
Collection中国科学院南京天文光学技术研究所_会议论文
望远镜新技术研究室_会议论文
Recommended Citation
GB/T 7714
Guomin Wang,Zhiyong Zhang,Bozhong Gu. Analysis and optimization of a 2.5m telescope mount[C]:SPIE,2008:Vol.7018 47-1-10.
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