[1]
[2] Tang Jinlong. The support optimum of honeycomb light-weight primary mirror and the study of pneumatic actuator[D]. Chengdu: The Institute of Optics and Electronics the Chinese Academy of Sciences, 2012. (in Chinese)
[3] Pietro Schipani, Massimo Capaccioli, Sergio D'Orsi, et al. The VST active primary mirror support system[C]//SPIE，2010, 7739, 31.
[4]
[5]
[6] Chen Fulin, Zhang Jingxu, Wu Xiaoxia, et al. Supporting structure of 620 mm thin primary mirror and its active surface correction[J]. Optics and Precision Engineering, 2011, 19(5): 1022-1029. (in Chinese)
[7] Yao Pin. The control study of Thin-mirror active optics[D]. Chengdu: The Institute of Optics and Electronics the Chinese Academy of Sciences, 2012. (in Chinese)
[8]
[9]
[10] Shi Zhenguang, Sui Yongxin, Liu Zhenyu, et al. Mathematical construction and perturbation analysis of Zernike discrete orthogonal points[J]. Applied Optics, 2012, 51 (18): 4210-4214. (in Chinese)
[11] Wilson R N, Rranza F, Noethe L, et al. A system for optimizing the optical quality and reducing the costs of large telescopes[J]. Journal of Modern Optics, 1987, 34(4): 485-509.
[12]
[13] Ernst-Dieter Knohl, CARL ZEISS Oberkochen, VLT Primary Support system[C]//SPIE, 1994, 2199: 271.
[14]
[15]
[16] Stephane Guisard, Lothar Noethe, Jason Spyromilio. Performance of active optics at the VLT[C]//SPIE, 2000, 4003.
[17] Noethe L. Use of minimum-energy modes for modal-active optics correction[J]. Journal of Modern Optics, 1991, 38(6): 1043-1066.