[1] [1] Zhang Jingxu. Structure types and design principles of ground-based telescope enclosures [J]. Chinese Optics, 2012, 5(2): 126-132.

[2] [2] Yao Zhengqiu, Zhou Fang. Progress in modern enclosure[J]. Progress in Astronomy, 2003, 21(3): 206-218.

[3] [3] Hammerschlag R H, Kommers J N M, Leverink S J, et al.. Mechanical design of a completely open-foldable dome for EST[C]. SPIE, 2010, 7733: 77330J.

[4] [4] M Riva. A partially foldable light weighted dome for fast pointing 3 m-class telescopes[C]. SPIE, 2010, 7733: 77333W.

[5] [5] MacMartin D G, Konstantinos Vogiatzis. Unsteady wind loads for TMT: replacing parametric models with CFD[C]. SPIE, 2014, 9150: 91500Q.

[6] [6] Loewen N, Breckenridge C, Vasiljevic A. Enclosure design for Thirty Meter Telescope[C]. SPIE, 2008, 7012: 70121D.

[7] [7] Schneermann M, G Marchiori, F Dimichino. The VLT enclosures: design and construction[C]. SPIE, 1997, 2781: 650-656.

[8] [8] Shu Xinling, Zhou Dai, Wang Yongfang. Review and prospect on measurement and simulation techniques of wind load[J]. Journal of Vibration and Shock, 2002, 21(3): 6-10, 25.

[9] [9] Yang Dehua, Xu Lingzhe, Xu Xinqi. Wind disturbance study on large astronomical telescopes[J]. Optical Technique, 2009, 35(3): 342-346.

[10] [10] Wu Lin, Fang Jiancheng, Yang Zhaohua. Study on aero-optical distortion simulation of high refraction index gradient regions in hypersonic turbulent flow[J]. Acta Optica Sinica, 2009, 29(11): 2952-2957.

[11] [11] Zhang Shijie, Li Junshan, Sun Lihui, et al.. Aero-optical imaging deviation under the small-incidence-angle condition[J]. Acta Optica Sinica, 2012, 32(10): 1001002.

[12] [12] Du Qiang, Tan San, Liu Ning. Comparison for computational methods to structures of wind loads in atmospheric boundary layer[J]. Computer and Modernization, 2012, 9: 137-139, 142.

[13] [13] Li Huafeng, Ma Jun, Zhou Dai, et al.. The numerical simulation for the wind fields and wind loads around spatial structures[J]. Journal of Shanghai Jiaotong University, 2006, 40(12): 2112-2117.

[14] [14] Liu Guangqian, Yang Lei, Deng Linhua, et al.. Influence of atmospheric turbulence on the accuracy of astronomical telescope autoguiding system[J]. Acta Optica Sinica, 2013, 33(1): 0101002.

[15] [15] Hao Weina. Experiment Research and Computation Analysis of LAMOST Dome Seeing[D]. Nanjing: Nanjing Institute of Astronomical Optics & Technology, Chinese Academy of Sciences, 2004: 5.

[16] [16] Zhang Jun, Xian Hao, He Yuanxing, et al.. Theoretical calculation of telescope primary mirror’s thermal field and seeing analysis of primary mirror[J]. Acta Optica Sinica, 2012, 32(10): 1022001.

[17] [17] Zhang Jun, Xian Hao, Zhang Cheng, et al.. Telescope primary mirror seeing and air knife effect analysis based on theoretical calculation of temperature field[J]. Acta Optica Sinica, 2013, 33(8): 0811005.

[18] [18] Ban Blanco. Estimating local seeing at the DCT facility[C]. SPIE, 2008, 7012: 70123V.

[19] [19] South B J, Soukup I M, Worthington M S, et al.. Wind loading analysis and strategy for deflection reduction on HET wide field upgrade[C]. SPIE, 2010, 7733: 77333Z.