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CAS IR Grid
机构
长春光学精密机械与物... [4]
高能物理研究所 [2]
上海光学精密机械研究... [2]
南京天文光学技术研究... [1]
半导体研究所 [1]
紫金山天文台 [1]
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OAI收割 [9]
iSwitch采集 [2]
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期刊论文 [7]
会议论文 [4]
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Physics, M... [1]
天文技术与方法::主... [1]
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Computation of misalignment and primary mirror astigmatism figure error of two-mirror telescopes
期刊论文
OAI收割
Journal of Astronomical Telescopes Instruments and Systems, 2018, 卷号: 4, 期号: 1, 页码: 10
作者:
Gu, Z. Y.
;
Wang, Y.
;
Ju, G. H.
;
Yan, C. X.
  |  
收藏
  |  
浏览/下载:162/0
  |  
提交时间:2019/09/17
active optics
alignment
misalignments
astigmatic figure error
nodal
aberration theory
two-mirror telescope
5th-order optical aberrations
rotational symmetry
wave-front
systems
collimation
Engineering
Instruments & Instrumentation
Optics
Motion of photons in a gravitational wave background
期刊论文
iSwitch采集
Chinese physics c, 2017, 卷号: 41, 期号: 9, 页码: 9
作者:
Chang, Zhe
;
Huang, Chao-Guang
;
Zhao, Zhi-Chao
收藏
  |  
浏览/下载:27/0
  |  
提交时间:2019/04/23
Fermat principle
Modified maxwell equations
Time variation
Frequency dependency
Gravitational wave vs mirror swing
Motion of photons in a gravitational wave background
期刊论文
OAI收割
CHINESE PHYSICS C中国物理. C, 2017, 卷号: 41, 期号: 9, 页码: 93108
作者:
Chang, Z
;
Huang, CG
;
Chang Z(常哲)
;
Zhao ZC(赵志超)
;
Zhao, ZC
  |  
收藏
  |  
浏览/下载:28/0
  |  
提交时间:2019/08/27
Fermat principle
modified Maxwell equations
time variation
frequency dependency
gravitational wave vs mirror swing
Wavefront correction of Ti:sapphire terawatt laser with varying precision of phase conjugation between deformable mirror and wavefront sensor
期刊论文
OAI收割
chinese physic b, 2012, 卷号: 21, 期号: 1, 页码: 014201
Yu LH(於亮红)
收藏
  |  
浏览/下载:17/0
  |  
提交时间:2013/09/10
adaptive optics, wave front correction, phase conjugation, deformable mirror
Research on automatic Hartmann test of membrane mirror (EI CONFERENCE)
会议论文
OAI收割
5th International Symposium on Advanced Optical Manufacturing and Testing Technologies: Optical Test and Measurement Technology and Equipment, April 26, 2010 - April 29, 2010, Dalian, China
作者:
Zhang P.
收藏
  |  
浏览/下载:41/0
  |  
提交时间:2013/03/25
Electrostatic membrane mirror is ultra-lightweight and easy to acquire a large diameter comparing with traditional optical elements
so its development and usage is the trend of future large mirrors. In order to research the control method of the static stretching membrane mirror
the surface configuration must be tested. However
membrane mirror's shape is always changed by variable voltages on the electrodes
and the optical properties of membrane materials using in our experiment are poor
so it is difficult to test membrane mirror by interferometer and null compensator method. To solve this problem
an automatic optical test procedure for membrane mirror is designed based on Hartmann screen method. The optical path includes point light source
CCD camera
splitter and diffuse transmittance screen. The spots' positions on the diffuse transmittance screen are pictured by CCD camera connected with computer
and image segmentation and centroid solving is auto processed. The CCD camera's lens distortion is measured
and fixing coefficients are given to eliminate the spots' positions recording error caused by lens distortion. To process the low sampling Hartmann test results
Zernike polynomial fitting method is applied to smooth the wave front. So low frequency error of the membrane mirror can be measured then. Errors affecting the test accuracy are also analyzed in this paper. The method proposed in this paper provides a reference for surface shape detection in membrane mirror research. 2010 Copyright SPIE - The International Society for Optical Engineering.
Application of precision harmonic gear drive in focusing mechanism of space camera (EI CONFERENCE)
会议论文
OAI收割
5th International Symposium on Advanced Optical Manufacturing and Testing Technologies: Smart Structures and Materials in Manufacturing and Testing, April 26, 2010 - April 29, 2010, Dalian, China
作者:
Zhang X.
;
Zhang X.
;
Zhang X.
收藏
  |  
浏览/下载:31/0
  |  
提交时间:2013/03/25
A kind of precision harmonic gear drive in the focusing mechanism of space camera is studied
which adopt external meshing complex wave transmission mode. Wave generator is combined with an elliptic cam and a flexible bearing around it. Flexspline is a structure of single wave with the same teeth. The output shaft is supported by a single cross-roller bearing. Ball screws connected the output shaft translate the rotational motion to the linear motion
and drive the focusing mirror repeated moving along the linear guide. The output rigid wheel is connected with absolute encoder to detect displacement of focusing movement. It has the characteristics of big transmission ratio
high precision
compact structure
high efficiency and smooth running etc. According to the practical application of this harmonic gear drive in the space camera
the location relationship between the displacement of focusing structure and the focal plane movement is derived
and the system error is analyzed
its accuracy is tested with the open-loop control method. Experimental results show that transmission ratio of the instrument is 1:70
repeated positional accuracy is 2m
which meet the requirements for use. 2010 SPIE.
Degenerate four-wave mixing based all-optical wavelength conversion in a semiconductor optical amplifier and highly-nonlinear photonic crystal fiber parametric loop mirror
期刊论文
iSwitch采集
Optics communications, 2008, 卷号: 281, 期号: 21, 页码: 5415-5419
作者:
Liu, Jianguo
;
Cheng, Tee Hiang
;
Yeo, Yong kee
;
Wang, Yixin
;
Xue, Lifang
收藏
  |  
浏览/下载:34/0
  |  
提交时间:2019/05/12
Degenerate four-wave mixing
Wavelength conversion
Semiconductor optical amplifier
Highly-nonlinear photonic crystal fiber
Parameter loop mirror
Based on Householder transform of the Zernike polynomial wave front fitting method to solve active optics correction force (EI CONFERENCE)
会议论文
OAI收割
Infrared Materials, Devices, and Applications, November 12, 2007 - November 15, 2007, Beijing, China
作者:
Wu X.-X.
收藏
  |  
浏览/下载:30/0
  |  
提交时间:2013/03/25
Corrective force solving is a critical technology of the active optics. A method to solve active optics corrective force is introduced
which is based on Householder transform of Zernike polynomial wave front fitting
this method is different from the traditional least square method and Gram-Schmid orthogonal method
because it does not bring ill-conditioned polynomial without constructing normal equation
so it can avoid calculation error
wave front fitting is precision. Based on the coefficient of the Zernike polynomial and the response function of the each actuator
the stiffness matrix of the primary mirror is built
and then adopting the damp least square method to calculate corrective force. Based on this method
cp400m test mirror is simulated many times
the calculation result approve: if the Householder transform is adopted
wave front fitting is precision
the result is stabilization and corrective effectiveness is better.
大型光学镜子热弹性变形的有限元分析
期刊论文
OAI收割
激光与光电子学进展, 2005, 卷号: 42, 期号: 1, 页码: 28, 31
张德江
;
刘立人
;
徐荣伟
;
李大汕
收藏
  |  
浏览/下载:1216/188
  |  
提交时间:2009/09/18
光学
optical mirror
一般方法
thermoelastic deformation
镜子
finite element analysis
实用技巧
wave aberration
过程
透镜
简述
热弹性
ANSYS软件
Experiment system of LAMOST active optics
会议论文
OAI收割
Glasgow, Scotland, 2004-6-21
作者:
Guoping Li
;
Zhengcao Zhang
;
Xiangqun Cui
;
Zhengqiu Yao
;
Ding-qiang Su
收藏
  |  
浏览/下载:35/0
  |  
提交时间:2013/12/23
Astronomical telescope
Active optics
Force actuator
Wave front test
Mirror support