地基大口径望远镜系统结构技术综述 -

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地基大口径望远镜系统结构技术综述

doi:10.3788/CO.20120504.0327

张景旭^,

中国科学院长春光学精密机械与物理研究所, 吉林长春 130033

详细信息

通讯作者:
张景旭

中图分类号:TH751
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- 文章访问数:3811
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- 被引次数:0
出版历程
- 收稿日期:2012-03-21
- 修回日期:2012-05-23
- 刊出日期:2012-08-10

Overview of structure technologies of large aperture ground-based telescopes

ZHANG Jing-xu^,

Changchun Institute of Optics, Fine Mechanics and Physics, Chinese Academy of Sciences, Changchun 130033, China

摘要

摘要:概述了地基大口径望远镜的发展状况,阐述了口径变大的意义及实现的关键技术途径。概括了当前大口径望远镜的应用价值。介绍了国外5种典型的大口径望远镜系统,它们代表了当前地基大口径望远镜发展的最高技术水平。从跟踪架、主望远镜筒、主镜支撑及次镜支撑调整几个方面论述了大口径望远镜的结构特点及关键技术。最后,总结了大口径望远镜系统的发展趋势,指出其光学系统已从同轴系统向离轴系统发展并极具应用前景。
- 地基望远镜/
- 大口径望远镜/
- 跟踪架/
- 主镜/
- 次镜
Abstract:The developing status of large aperture ground-based telescopes is reviewed in this paper. The significance of bigger apertures for telescopes and their main technological approaches are expatiated and the summary on appliance values of modern large aperture telescopes is given. Then, it introduces five kinds of modern typical large telescope systems, which represent the topmost technological level. The key structures and technologies of large telescopes about mount, telescope tubes, primary mirror supports and secondary mirror assemblies are disscussed. Finally, it summarizes the developing trends of the large aperture ground-based telescopes and points out that some of the optical systems in the telescopes have been changed from coaxial systems to off-axial systems, while they are better application prospects.
- ground-based telescope/
- large aperture telescope/
- tracking mount/
- primary mirror/
- secondary mirror

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[1] BELY P Y.The Design and Construction of Large Optical Telescopes[M]. Berlin:Springer-verlag,2002. [2] 夏坚白.实用天文学[M]. 武汉:武汉大学出版社,2007. XIA J B.Practical Astronomy[M]. Wuhan:Wuhan University Publishing House,2007.(in Chinese) [3] CUI X Q. Progress and prospect of LAMOST project[J].SPIE,2006,6267:626703. [4] CUI X Q. The optical performance of LAMOST telescope[J].SPIE,2010,7733:773303. [5] CUI X Q. Preparing the first light of LAMOST[J].SPIE,2008,7012:701203. [6] 苏定强.2.16 m天文望远镜工程文集[M]. 北京:中国科学技术出版社,2001. SU D Q.2.16 m Astronomical Telescope Process Corpus[M]. Beijing:China Science & Technology,2001.( in Chinese) [7] KOEHLER B,FLEBUS C. VLTI auxiliary telescopes[J].SPIE,2000,4006:13-24. [8] 李东源. 国外的地基对空间目标光电探测系统浅析[J]. 光电对抗与无源干扰 ,2003,69(1):9-11. LI D Y. Overview on photoelectric detection for ground base to space target aboard[J].Photoelectricity Antagonize and Passive Disturb,2003,69(1):9-11.(in Chinese) [9] 孔建业. 美国空间目标监视系统概况[J]. 863先进防御技术通讯(A类) ,2000,8. KONG J Y. Overview of supervisory system in America for space target[J].863 Advanced Defensive Technology Communication(Class A),2000,8.(in Chinese) [10] 李颖. 空间目标监视系统发展现状及展望[J]. 国际太空 ,2004(6):28-32. LI Y. Present status and prospect of supervisory system for space target[J].International Space,2004(6):28-32.(in Chinese) [11] VIGIL M L,DAVID J. Sensor suite for the Advanced Electro-Optical System(AEOS) 3.6 m telescope[J].SPIE,1996,2819:151-169. [12] KIMBRELL J E. AEOS 3.67 m telescope primary mirror active control system[J].SPIE,1998,3352:400-411. [13] HOUCHARD J. Orbital debris detection program highlights from the air force mauii optical station[J].SPIE,1994,2214:7-20. [14] LIPINSKI R J. Laser beaming demonstrations at the starfire optical range[J].SPIE,1995,2376:219-230. [15] FUGATE R Q. The starfire optical range 3.5 m adaptive optical telescope[J].SPIE,2003,4837:934-943. [16] FUGATE R Q. The VLT enclosure design and construction[J].SPIE,1997,2871:650. [17] 崔向群. 采用主动光学的大口径单块薄镜面的支撑系统 .南京:中科院南京紫金山天文台,1995. CUI X Q. Supporting system of large aperture thin monolithic primary mirror with active optics . Nanjing:Nanjing observatory,Chinese Academy of Sciences,1995.(in Chinese) [18] WILSON R N.Reflecting Telescope OpticsⅡ[M]. Berlin:Springer-verlag,2001. [19] ARCIDIACONO C. The opto-mechanical alignment procedure[J].SPIE,2010,7733:773357. [20] ROBERTS S. Optical performance analysis and optimization of large telescope structural designs[J].SPIE,2005,5867:58670O. [21] SZETO K,ROBERTS S,SUN S,et al.. TMT telescope structure system:design and development[J].SPIE,2008,7012:70122G. [22] ROBERTS S. Systems engineering of the TMT through integrated opto-mechanical analysis[J].SPIE,2010,7738:773818. [23] MARCHIORI G. New solutions for innovative ELT[J].SPIE,2006,6148:614806. [24] ANDERSON T. An integrated model of the E-ELT[J].SPIE,2008,7017:70170S. [25] MURGA G. Detail design and construction plans for a dome for the E-ELT[J].SPIE,2010,7733:773324. [26] 程景全.天文望远镜原理和设计[M]. 北京:中国科学技术出版社,2002. CHENG J Q.Principle and Design of Astronical Telescope[M]. Beijing:China Science & Technology,2003.(in Chinese) [27] RAY F B. Active optics technology-an overview[J].SPIE,1991,1532:188-206. [28] IYE M,NOGUCHI T. Active optics experiments with a 62 cm thin mirror[J].SPIE,1990,1236:929-939. [29] 苏定强,崔向群. 主动光学—新一代大望远镜的关键技术[J]. 天文学进展 ,1999(17):1-13. SU D Q,CUI X Q. Active Optics—Pivotal technology of new Large aperture telescope[J].Development in Astronomy,1999(17):1-13.(in Chinese) [30] YODER P R.Opto-Mechanical Systems Design[M]. New York:Marcel Dekker,Inc.,1993. [31] 程景全,李国平. 四翼梁式十字形中心支撑的力学特性[J]. 天文仪器与技术 ,1988(1):5-10. CHENG J Q,LI G P. Mechanical properties of crossed-vane type supporting structure[J].Astronomical Instruments and Technology,1988(1):5-10.(in Chinese) [32] VAN BELLE G T. The scaling relationship between telescope cost and aperture size for very large telescopes[J].SPIE,2004,5489:563.

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