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Chinese Academy of Sciences Institutional Repositories Grid
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浏览/检索结果: 共24条,第1-10条 帮助

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Post Optical Freeform Compensation Technique for Machining Errors of Large-Aperture Primary Mirror 期刊论文  OAI收割
PHOTONICS, 2023, 卷号: 10, 期号: 7
作者:  
Huang, Cheng;  Li, Jinpeng;  Cai, Zhaohan;  Yu, Jiadong;  Xie, Yongjun
  |  收藏  |  浏览/下载:16/0  |  提交时间:2023/08/18
Microstress bonding design of low-distortion mirror assembly 期刊论文  OAI收割
OPTICAL ENGINEERING, 2022, 卷号: 61, 期号: 10
作者:  
Sun, Lijun;  Wu, Weichao;  Chen, Wencong;  Li, Siyuan;  Zhang, Zhaohui
  |  收藏  |  浏览/下载:37/0  |  提交时间:2022/11/30
Design and optimization research of phi 1.6m space mirror and its supporting structure 会议论文  OAI收割
ELECTR NETWORK, 2022-11-24
作者:  
Wei De Jing;  Wang Wei;  Hu Bin;  Lin Shang Min;  Cheng Peng Fei
  |  收藏  |  浏览/下载:9/0  |  提交时间:2023/06/19
Applications and development of micro- or nano-metric multi degree of freedom adjusting displacement scaling mechanisms for primary mirror 会议论文  OAI收割
Xian, PEOPLES R CHINA, 2020-10-15
作者:  
Hu, Bin;  Li, Chuang;  Zhu, Qing;  Ye, Jing
  |  收藏  |  浏览/下载:33/0  |  提交时间:2021/07/23
Design and Test of Flexible Support Structure for Large Aperture Lightweight Mirror 会议论文  OAI收割
Beijing, PEOPLES R CHINA, 2020-11-30
作者:  
Sun Li Jun;  Liu Zhen;  Zhang Zhao Hui;  Li Li Bo;  Li Si Yuan
  |  收藏  |  浏览/下载:20/0  |  提交时间:2021/06/04
Topology optimization design of large aperture mirror for the vt system of svom 会议论文  OAI收割
Beijing, China, 2020-11-30
作者:  
Lin, Feng;  Wang, Wei;  Zhang, Jian;  Fan, Xuewu;  Xu, Wenjing
  |  收藏  |  浏览/下载:25/0  |  提交时间:2020/12/29
A method based on exact constraint for supporting space-based large mirror with a diameter of 2.8m 期刊论文  OAI收割
Optik, 2019, 卷号: 179, 页码: 499-504
作者:  
Z.S.Wang;  J.X.Zhang;  J.X.Wang;  X.He;  L.T.Fu
  |  收藏  |  浏览/下载:25/0  |  提交时间:2020/08/24
A Review of Large Aperture Schlieren Photography Technique 会议论文  OAI收割
photoelectronic-technology-committee conference, peoples r china, 2016-11-15
作者:  
Xu Song-bo;  Xie Yong-jun;  Chen Lei
收藏  |  浏览/下载:36/0  |  提交时间:2016/10/18
Structural design of primary mirror subassembly for space telescope (EI CONFERENCE) 会议论文  OAI收割
2nd International Conference on Mechatronics and Applied Mechanics, ICMAM 2012, December 8, 2012 - December 9, 2012, Taiwan
作者:  
Xu H.
收藏  |  浏览/下载:62/0  |  提交时间:2013/03/25
In order to design a large aperture primary mirror with the diameter of 1150 mm  the parameters impacting on gravity deformation of the mirror were analyzed and discussed in detail  including material selection  diameter-thickness ratio  the number of the support points  location selection and lightweight structure  etc. A novel space mirror structure system was put forward  and its back was opened and supported by six points on back. The dynamic and static and thermal characteristics were analyzed based on the finite element method. Analysis results showed the surface figure accuracy reached to RMS 14.5nm under the action of gravity load along the optical axis direction and the first-order natural frequency was 214Hz which met to the designed indexes requirements. (2013) Trans Tech Publications  Switzerland.  
Structural design of large aperture rectangular mirror for space telescope (EI CONFERENCE) 会议论文  OAI收割
2nd International Conference on Civil Engineering and Transportation, ICCET 2012, October 27, 2012 - October 28, 2012, Guilin, China
作者:  
Li Z.;  Li Z.
收藏  |  浏览/下载:42/0  |  提交时间:2013/03/25
Structural design of large aperture mirror is one of the key technologies for space telescope development. To meet the requirements of high stiffness  strength and thermal dimensional stability  some factors such as support scheme  materials selection  lightweight design and flexible support design were taken into account. The three supports location of the mirror was determined according to the modal analytical solution. By adjusting the parameters of flexure hinge  influences of gravity  assembly stress and thermal stress on the mirror were reduced obviously. Finite element analysis (FEA) results indicate that the surface accuracy reach to rms10.2nm and 10.8nm under the gravity along optical axis direction and 5C uniform temperature rise respectively  the fundamental frequency of the mirror component is 268Hz. Dynamics test shows that the first order natural frequency is 256Hz  which shows an error less than 5% compared to FEA results. (2013) Trans Tech Publications  Switzerland.