[1] URS Corporation. Site-Specific Seismic Hazard Assessment of Proposed Thirty Meter Telescope Site, Mauna Kea, Hawaii [OL]. http://tmt.org/sites/default/files/documents/application/pdf/urs_report_2-4-10.pdf.[2013-09-06].
[2] TMT Group. Design Requirements Document for Tertiary Mirror System (M3S) [Z].TMT. OPT. DRD.07.006.REL29. 2012.
[3] F W Kan, J Antebi. Seismic hazard: analysis and design of large ground based telescopes [C]. SPIE, 2008, 7012: 70122E.
[4] F KOCH. Analysis concepts for large telescope structures under earthquake load [C]. SPIE, 1997, 2871: 117-126.
[5] D Tsang, G Austin, M Gedig, et al.. TMT telescope structure system-seismic analysis and design [C]. SPIE, 2008, 7012: 07124J.
[6] D R Neill, M Warmer, J Sebag, et al.. Seismic design accelerations for the LSST telescope [C]. SPIE, 2012, 8444: 84440R.
[8] Li Jie, Li Guoqiang. Earthquake Engineer Introduction [M]. Beijing: Earthquake Press, 1984.
[9] Chen Yongqi, Liu Xiquan, Gong Sili. Artificial seismic wave fitting standard response spectrum [J]. Engineer Mechanics, 1994, 12(3): 31-42.
[10] Yang Fei, Ming Ming, Chen Baogang, et al.. Influence of diversification of elevation to the opto-mechanical system of 1.23 m telescope [J]. Laser & Optoelectronics Progress, 2012, 49(3): 032201.
[12] Hu Yuxian, He Xun. Artificial seismic response spectrum fitting with phase spectrum considered [J]. Earthquake Engineer and Engineer Vibration, 1986, 6(2): 37-51.
[13] Chen Wei. Direction method research on seismic acceleration response spectrum fitting [J]. Engineer Mechanics, 2000, 17(1): 83-87.
[15] Wang Xinmin. Ansys Engineer Structure Numerical Analysis [M]. Beijing: China Communications Press, 2007.