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Chinese Academy of Sciences Institutional Repositories Grid
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浏览/检索结果: 共12条,第1-10条 帮助

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Research on cylindrical labels unfolding algorithm based on machine vision 会议论文  OAI收割
Chongqing, China, March 12-14, 2021
作者:  
Zhang ZL(张泽鲁);  Xu M(许敏);  Chen S(陈帅)
  |  收藏  |  浏览/下载:28/0  |  提交时间:2021/05/10
Femtosecond streak tube with large work area and small size for 3D imaging lidar 会议论文  OAI收割
Xi'an, China, 2019-08-06
作者:  
Liu, Rong;  Tian, Jinshou;  Hui, Dandan;  Xue, Qihang;  Zheng, Kaiwen
  |  收藏  |  浏览/下载:75/0  |  提交时间:2020/03/04
Design and optimization of resistive anode for a two-dimensional imaging GEM detector 期刊论文  OAI收割
CHINESE PHYSICS C, 2016, 卷号: 40, 期号: 8
作者:  
Ju XD(鞠旭东);  Dong MY(董明义);  Zhou CX(周传兴);  Ou YQ(欧阳群);  Ju, XD
  |  收藏  |  浏览/下载:25/0  |  提交时间:2017/07/27
The effect of inhomogeneous water on seismic imaging in deepwater areas of the South China Sea 期刊论文  OAI收割
CHINESE SCIENCE BULLETIN, 2013, 卷号: 58, 期号: 35, 页码: 4443-4449
作者:  
Ji LL(姬莉莉);  Lin M(林缅);  Hao TY(郝天珧)
收藏  |  浏览/下载:31/0  |  提交时间:2013/12/16
中尺度涡影响下目的层地震成像的畸变与影响因素分析 期刊论文  OAI收割
地球物理学报=Chinese Journal of Geophysics- Chinese Edition, 2013, 卷号: 56, 期号: 1, 页码: 195-203
作者:  
姬莉莉;  林缅
收藏  |  浏览/下载:29/0  |  提交时间:2013/03/04
Laboratory test of a polarimetry imaging subtraction system for the high-contrast imaging 会议论文  OAI收割
Amsterdam, Netherlands, 2012-7-1
作者:  
Jiangpei Dou;  Yongtian Zhu;  Xi Zhang;  Rong Li;  Deqing Ren
收藏  |  浏览/下载:29/0  |  提交时间:2014/01/10
Self-calibration of hybrid central catadioptric and perspective cameras 期刊论文  OAI收割
COMPUTER VISION AND IMAGE UNDERSTANDING, 2012, 卷号: 116, 期号: 6, 页码: 715-729
作者:  
Deng, Xiaoming;  Wu, Fuchao;  Wu, Yihong;  Duan, Fuqing;  Chang, Liang
收藏  |  浏览/下载:35/0  |  提交时间:2015/08/12
A dual-channel imaging polarimetry system 会议论文  OAI收割
Beijing, China, 2011-11-6
作者:  
Jiangpei Dou;  Yongtian Zhu;  Xi Zhang;  Deqing Ren;  Xue Wang
收藏  |  浏览/下载:49/0  |  提交时间:2014/01/07
Imaging system effects on the measuring accuracy of the optical surface in interferometer (EI CONFERENCE) 会议论文  OAI收割
3rd International Conference on Measuring Technology and Mechatronics Automation, ICMTMA 2011, January 6, 2011 - January 7, 2011, Shanghai, China
Yang W.; Liu M.; Xu W.
收藏  |  浏览/下载:27/0  |  提交时间:2013/03/25
In order to measure high accuracy or mid spatial frequency optical surfaces  this study investigated imaging system in Fizeau interferometer. Interferometer is a transferring phase information system. General transfer function can't evaluate the ability of imaging system in interferometer that transfers the phase information of the optical surface. So this paper deduced instrument transfer function (ITF) and used ITF to evaluate the phase information transfer ability of interferometer. We obtained some results about ITF of imaging system by numerical simulation when there are different aberrations in imaging system or measuring optical surfaces were different. Our results indicate that ITF can evaluate the ability of transferring phase information in interferometer and the distortion of imaging system evidently affects the accuracy of interferometric measurements. 2010 IEEE.  
Design of high precision star image locating method used in star sensor technology (EI CONFERENCE) 会议论文  OAI收割
2010 International Conference on Computer, Mechatronics, Control and Electronic Engineering, CMCE 2010, August 24, 2010 - August 26, 2010, Changchun, China
作者:  
Sun H.;  Wang Y.;  Wang Y.;  Wang Y.;  Wang Y.
收藏  |  浏览/下载:55/0  |  提交时间:2013/03/25
Nowadays star sensor technology used in aircraft attitude measurement has become more and more popular for its high precision  light weight  without attitude accumulation errors and other advantages. In order to enhance the accuracy of star sensor  it is critical to make efforts to promote the precision of star image locating. High precision star image locating method mentioned in this article includes two aspects. One is sub-pixel dividing algorithm used to acquire the coordinate of stars. The other one is imaging calibration method used to weaken the effect caused by imaging distortion. This method is finally realized in some type of star sensor system. Then an experiment is designed to verify the precision of the method. The result of the experiment shows that the precision of the method is 2" in the experimental environment. 2010 IEEE.