南极小望远镜阵的抗振设计分析与测试
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摘要
南极Dome A被认为是地球上最好的天文观测台址,研制一台用于测光和台址测量的南极小望远镜的课题由此产生。CSTAR(Chinese Small Telescope ARray)于2006年8月提出,用时一年研制成功,并于2007年11月启程运往南极。文章运用振动理论并辅以ANSYS有限元分析软件,设计了该望远镜的抗振运输箱并通过实验加以验证。
Dome A in Antarctic plateau is considered to be the best astronomical observatory site in the world.In August 2006,a scheme which was about to build an optical telescope for site selection and testing in Dome A was proposed.CSTAR(Chinese Small Telescope Array)was successfully accomplished in August 2007 and has been shipping to Dome A in November 2007.The anti-vibration design of CSTAR was analyzed by ANSYS and proved to be suitable through experiments based on vibration theory.
引文
1J.W.V.Storey.Introduction to the Antarctic Plateau[A].Proceedings of Conference on Wide Field Survey Telescope at DOME C and A,held on3-4June2005,Beijing,China:10~12
    2LI Yuansheng.Introduction to Chinese Dome A Inland Traverse2004/2005[A].Proceedings of Conference on Wide Field Survey Telescope at DOME C and A,held on3-4June2005,Beijing,China:13~17
    3倪振华.振动力学[M].西安:西安交通大学出版社,1990
    4李建丰,徐鸿,王楠等.设备地震响应的频谱分析法[J].北京化工大学学报,2003,30(1):57~60

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