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CORC

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Design and Thermal Stability Analysis of Swing Micro-Mirror Structure for Gravitational Wave Observatory in Space 期刊论文
machines, 2021, 卷号: 9, 期号: 5, 页码: 104-127
作者:  Zheng KY(郑焜耀);  Xu MM(许明明)
收藏  |  浏览/下载：3/0  |  提交时间：2022/04/01
Study on plasma cleaning of the large-scale first mirror of the charge exchange recombination spectroscopy diagnostic on EAST 期刊论文
PLASMA SCIENCE & TECHNOLOGY, 2020, 卷号: 22
作者:  Peng, Jiao;  Yan, Rong;  Chen, Junling;  Ding, Rui;  Li, Yingying
收藏  |  浏览/下载：17/0  |  提交时间：2020/11/26
Real-Time 2-D Optical Polarization Properties of the Fusion Reactor First Mirror Based on Active Polarized Beams 期刊论文
IEEE TRANSACTIONS ON PLASMA SCIENCE, 2018, 卷号: 46, 期号: 5, 页码: 1186-1190
作者:  Qi, Junli;  Wang, Weihua;  Pan, Baoguo;  Zhang, Hui;  Yang, Jinhong
收藏  |  浏览/下载：47/0  |  提交时间：2019/06/10
Plasma cleaning of ITER first mirrors 期刊论文
PHYSICA SCRIPTA, 2017, 卷号: T170, 期号: 无, 页码: 7
作者:  Moser, L.;  Marot, L.;  Steiner, R.;  Reichle, R.;  Leipold, F.
收藏  |  浏览/下载：24/0  |  提交时间：2019/06/17
Repetitive cleaning of a stainless steel first mirror using radio frequency plasma 期刊论文
PLASMA SCIENCE & TECHNOLOGY, 2017, 卷号: 19, 期号: 10
作者:  Peng, Jiao;  Yan, Rong;  Ding, Rui;  Chen, Junling;  Zhu, Dahuan
收藏  |  浏览/下载：16/0  |  提交时间：2018/08/16
Comparative investigations of stainless steel and molybdenum first mirrors cleaning using radio frequency plasma 期刊论文
FUSION ENGINEERING AND DESIGN, 2016, 卷号: 112, 期号: 无, 页码: 317-323
作者:  Peng, J.;  Chen, L. W.;  Yan, R.;  Chen, J. L.;  Zhu, D. H.
收藏  |  浏览/下载：15/0  |  提交时间：2017/07/17
Hybrid optimization methodology of variable densities mesh model for the axial supporting design of wide-field survey telescope 期刊论文
OPTICAL ENGINEERING, 2016, 卷号: 55, 期号: 3
作者:  Wang, Hairen;  Lou, Zheng;  Qian, Yuan;  Zheng, Xianzhong;  Zuo, Yingxi
收藏  |  浏览/下载：13/0  |  提交时间：2016/09/27
Structural design of primary mirror subassembly for space telescope (EI CONFERENCE) 会议论文
2nd International Conference on Mechatronics and Applied Mechanics, ICMAM 2012, December 8, 2012 - December 9, 2012, Taiwan
Xu H.
收藏  |  浏览/下载：43/0  |  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
2nd International Conference on Civil Engineering and Transportation, ICCET 2012, October 27, 2012 - October 28, 2012, Guilin, China
Li Z.
收藏  |  浏览/下载：27/0  |  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.  
Advanced astigmatism-corrected tandem Wadsworth mounting for small-scale spectral broadband imaging spectrometer (EI CONFERENCE) 会议论文
Lei Y.; Lin G.-Y.
收藏  |  浏览/下载：29/0  |  提交时间：2013/03/25
Tandem gratings of double-dispersion mount make it possible to design an imaging spectrometer for the weak light observation with high spatial resolution  high spectral resolution  and high optical transmission efficiency. The traditional tandem Wadsworth mounting is originally designed to match the coaxial telescope and large-scale imaging spectrometer. When it is used to connect the off-axis telescope such as off-axis parabolic mirror  it presents lower imaging quality than to connect the coaxial telescope. It may also introduce interference among the detector and the optical elements as it is applied to the short focal length and small-scale spectrometer in a close volume by satellite. An advanced tandem Wadsworth mounting has been investigated to deal with the situation. The Wadsworth astigmatism-corrected mounting condition for which is expressed as the distance between the second concave grating and the imaging plane is calculated. Then the optimum arrangement for the first plane grating and the second concave grating  which make the anterior Wadsworth condition fulfilling each wavelength  is analyzed by the geometric and first order differential calculation. These two arrangements comprise the advanced Wadsworth mounting condition. The spectral resolution has also been calculated by these conditions. An example designed by the optimum theory proves that the advanced tandem Wadsworth mounting performs excellently in spectral broadband. 2012 Optical Society of America.  

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