[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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