Optics and Precision Engineering, Volume. 25, Issue 10, 2614(2017)
Secondary mirror supporting structure for 1.2 m telescope
[1] [1] SANDERS G H. The thirty meter telescope (TMT): an international observatory[J]. Journal of Astrophysics and Astronomy, 2013, 34(2): 81-86.
[2] [2] WILSON R N. Reflecting Telescope Optics II: Manufacture, Testing, Alignment, Modern Techniques[M]. New York: Springer, 2013.
[3] [3] CHENG J Q. Principles of Astronomical Telescope Design[M]. Beijing: Science and Technology of China Press, 2003. (in Chinese)
[4] [4] WANG S Q, WEI K, ZHENG W J, et al.. First light on an adaptive optics system using a non-modulation pyramid wavefront sensor for a 1.8 m telescope[J]. Chinese Optics Letters, 2016, 14(10): 100101.
[9] [9] YANG T Y, WIEBE R. Experimental Study on the Effect of Large Axial Tensile Force on the Natural Frequency of a Fixed-Fixed Steel Beam[M]//KERSCHEN G. Nonlinear Dynamics, Volume 1, Springer, 2017: 127-134.
[10] [10] XIONG H X, ZHANG Y T. Theoretical analysis of natural frequency of externally prestressed concrete beam based on rigidity correction[J]. Academic of Xi’an Jiaotong University, 2009, 21(1): 31-35.
[11] [11] SHI H M. Vibration Systems—Analyzing Testing Modeling Controlling[M]. 2nd ed.. Wuhan: Huazhong University of Science and Technology Press, 2004: 91-124. (in Chinese)
[12] [12] HUANG B K, HUANG P H. Finite element and wavefront error analysis of the primary mirror of an experimental telescope with reverse engineering[J].SPIE, 2016, 9953: 99530T.
Get Citation
Copy Citation Text
ZHAO Hong-chao, ZHANG Jing-xu, YANG Fei, AN Qi-chang. Secondary mirror supporting structure for 1.2 m telescope[J]. Optics and Precision Engineering, 2017, 25(10): 2614
Category:
Received: Jun. 1, 2017
Accepted: --
Published Online: Nov. 24, 2017
The Author Email: Hong-chao ZHAO (zhaohcciomp@163.com)