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作 者:何鑫 姜翔[1,2] 顾伯忠[1,2] 叶宇[1,2] 乐中宇[1,2] He Xin;Jiang Xiang;Gu Bozhong;Ye Yu;Yue Zhongyu(National Astronomical Observatories/Nanjing Institute of Astronomical Optics&Technology,Chinese Academy of Sciences,Nanjing 210042,China;CAS Key Laboratory of Astronomical Optics&Technology,Nanjing Institute of Astronomical Optics&Technology,Nanjing 210042,China;University of Chinese Academy of Sciences,Beijing 100049,China)
机构地区:[1]中国科学院国家天文台南京天文光学技术研究所,江苏南京210042 [2]中国科学院天文光学技术重点实验室(南京天文光学技术研究所),江苏南京210042 [3]中国科学院大学,北京100049
出 处:《红外与激光工程》2022年第5期364-372,共9页Infrared and Laser Engineering
基 金:国家自然科学基金(11703057)。
摘 要:针对丽江2.4 m望远镜耐焦与卡焦不能自动切换的现状,设计了一套M3切换系统,实现焦点间快速切换,进一步提高望远镜的观测能力。首先对切换系统进行结构设计,介绍了系统的组成和实现方法,然后进行了精度分析及有限元分析,最后通过实验进行了标定和测试。有限元分析结果表明,在重力作用下反射镜的面形精度RMS<λ/60(λ=632.8 nm),切换系统的一阶模态达到了34.71 Hz,整个系统具有较好的刚度。实验测试表明,方位轴系和俯仰轴系的重复定位精度优于0.5″,平移机构的重复定位精度为1μm。该切换系统的性能指标达到了设计要求,并已装调于该望远镜且投入观测使用,同时也为类似望远镜的设计提供了参考。In order to solve the situation that the 2.4-meter telescope cannot switch Nasmyth focus and Cassgrain focus intelligently,a switching system was designed to switch focuses rapidly to improve the observation ability.Firstly,a M3 switching system model was built,the composition and implementation of the system were discussed in detail.Then precision analysis and finite element analysis were performed to optimize design.Finally,the calibration and test were carried out through experiment.Finite element analysis shows that under the action of gravity,the mirror surface shape RMS<λ/60(λ=632.8 nm).The first-order modal of system reaches 34.71 Hz,the system has good stiffness.Experimental measurement shows that azimuth structure and altitude structure repetition precision are superior to 0.5″,translation stage repetition precision is 1μm.The switching system meets the performance requirements and has been installed in the telescope,which has been used for observation.It also provides a reference for the design of other telescopes.
关 键 词:2.4 m望远镜 三镜系统 精度分析 有限元分析
分 类 号:TH751[机械工程—仪器科学与技术]
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