[1] Gao Yanlong. Study on wind characteristics simulation method of antennae[D]. Xi′an: University of Electronic Science and Technology of China, 2009. (in Chinese)
[2] De Young, Vogiatzis K. Numerical simulations of airflow in verylarge telescope enclosures[C]//SPIE, Second Backaskog Workshop on Extremely Large Telescopes, 2004, 5382: 379-387.
[3] Y Chen, G A Kopp, D Surry. Prediction of pressure coefficients on roofs of low buildings using artificial neural networks[J]. Wind Eng Ind Aerodyn, 2003, 91: 423-441.
[4] GB50009-2001. Load code for the design of building structures[S]. Beijing: China Architecture & Building Press, 2006. (in Chinese)
[5] Zhang Xiangting. Handbook of Computational Wind Engineering Design[M]. Beijing: Chinese Architectural Press, 1998.(in Chinese)
[6] GB50011-2010. Code for seismic design of buildings[S]. Beijing: China Architecture & Building Press, 2010. (in Chinese)
[7] Qian Hongliang, Liu Yan, Fan Feng. Surface precision analysis on main reflector of 65 m antenna structure[J]. Infrared and Laser Engineering, 2012, 41(11): 3027-3033. (in Chinese)
[8] Bremer M, Penalver J. FE model based interpretation of telescope temperature variations[C]//SPIE, 2002, 4757: 186.
[9] Bremer M, Greve A, van′t Klooster K, et al. Front and rear Perspective heated prototype panels for the IRAM 15–m telescopes[C]//28th ESA Antenna Workshop on Space Antenna Systems and Technologies, ESTEC, 2005: 943.
[10] Chamberlin R A. Temperature meaurements on the Leighton telescope[J]. Surface Memo, 2003, 5: 124-130.
[11] Cheng J. Principles of Astronomical Telescope Design [M]. New York: Springer, Heidelberg, 2009.