中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
机构
采集方式
内容类型
发表日期
学科主题
筛选

浏览/检索结果: 共10条,第1-10条 帮助

条数/页: 排序方式:
SG-SRNs: Superpixel-Guided Scene Representation Networks 期刊论文  OAI收割
IEEE SIGNAL PROCESSING LETTERS, 2022, 卷号: 29, 页码: 2038-2042
作者:  
Liu, Qiang;  Lu, Xiao;  Dong, Qiulei;  Zhang, Yangyong;  Wang, Haixia
  |  收藏  |  浏览/下载:38/0  |  提交时间:2022/11/14
Image Retargetability 期刊论文  OAI收割
IEEE TRANSACTIONS ON MULTIMEDIA, 2020, 卷号: 22, 期号: 3, 页码: 641-654
作者:  
Tang, Fan;  Dong, Weiming;  Meng, Yiping;  Ma, Chongyang;  Wu, Fuzhang
  |  收藏  |  浏览/下载:36/0  |  提交时间:2020/06/02
Misalignment Measurement of Orbital Angular Momentum Signal Based on Spectrum Analysis and Image Processing 期刊论文  OAI收割
IEEE TRANSACTIONS ON ANTENNAS AND PROPAGATION, 2020, 卷号: 68, 期号: 1, 页码: 521-526
作者:  
Gao, Xinlu;  Song, Xiyao;  Zheng, Zhennan;  Xie, Mutong;  Huang, Shanguo
  |  收藏  |  浏览/下载:30/0  |  提交时间:2020/12/10
Secure Face Unlock: Spoof Detection on Smartphones 期刊论文  OAI收割
IEEE TRANSACTIONS ON INFORMATION FORENSICS AND SECURITY, 2016, 卷号: 11, 期号: 10, 页码: 2268-2283
作者:  
Patel, Keyurkumar;  Han, Hu;  Jain, Anil K.
  |  收藏  |  浏览/下载:38/0  |  提交时间:2019/12/13
Crowd density estimation based on statistical analysis of local intra-crowd motions for public area surveillance 期刊论文  OAI收割
Optical Engineering, 2012, 卷号: 51, 期号: 4, 页码: 1-14
作者:  
Zhaoxiang Zhang;  Min Li
  |  收藏  |  浏览/下载:16/0  |  提交时间:2017/02/09
Design and simulation of CMOS star sensor lens with large relative aperture and wide field (EI CONFERENCE) 会议论文  OAI收割
2011 International Conference on Electronic and Mechanical Engineering and Information Technology, EMEIT 2011, August 12, 2011 - August 14, 2011, Harbin, China
Zhong X.; Jin G.
收藏  |  浏览/下载:65/0  |  提交时间:2013/03/25
A 50mm focal length  F/1.25  Gaussian type optical system is designed in this paper  which has 20field of view. Actual star image adding optical cross-talk effect of CMOS(Complementary Metal Oxide Semiconductor)  detector is simulated by non-sequential ray tracing in ZEMAX optical design and analysis software to evaluate its performance. The distortion relative to image spot centriod is introduced and calculated by simulated star images  which is less than 0.03% of lens in this paper. Thermal adaptability is discussed by opt-mechanic thermal analysis  which shows the RMS spot radius of marginal filed changes less than 0.7m under 10C temperature gradient  and changes less than 1m during homogeneous temperature changing from 40C to 40C. The results of analyses and simulations show the design of this lens can achieve the requirement of high precision CMOS star sensor well. 2011 IEEE.  
Equivalent lenses of supersonic seeker's outflow refractive index field obtained by simulation and experiment (EI CONFERENCE) 会议论文  OAI收割
2008 International Conference on Optical Instruments and Technology: Optical Systems and Optoelectronic Instruments, November 16, 2008 - November 19, 2008, Beijing, China
Qun W.; Hongguang J.; Ming X.
收藏  |  浏览/下载:30/0  |  提交时间:2013/03/25
图像与视频拼接算法研究 学位论文  OAI收割
工学博士, 中国科学院自动化研究所: 中国科学院研究生院, 2007
作者:  
苗立刚
收藏  |  浏览/下载:88/0  |  提交时间:2015/09/02
Design and analysis of large spaceborne light-weighted primary mirror and its support system (EI CONFERENCE) 会议论文  OAI收割
3rd International Symposium on Advanced Optical Manufacturing and Testing Technologies, AOMATT 2007: Large Mirrors and Telescopes, July 8, 2007 - July 12, 2007, Chengdu, China
Yan Y.; Jin G.; Yang H.-B.
收藏  |  浏览/下载:23/0  |  提交时间:2013/03/25
With the development of the resolution of spaceborne remote sensor  the diameter of the primary mirror of spaceborne telescope becomes larger and larger. The distortion of primary mirror which is influenced by the mirror material  structure  self-weight  support system and temperature environment affects optical image quality finally. In this paper  an on-axis TMA high-resolution Cassegrain optical payload with a primary mirror whose diameter is 650mm was designed and the effects of the influence factors of the distortion acts on the on-axis TMA optical system primary mirror had been analyzed by means of Finite Element Analysis. During work  the technology of the primary mirror design had been summarized and general consideration of the primary mirror design technology also had been described at the same time. Considering the telescope manufacture and work station  a reasonable and optimal structure of the primary mirror sub-assembly is taken finally. In the end  the distortion of the primary mirror during its fabrication station and work station had been analyzed by integrated Finite Element Analysis Method. The results implicated the synthesis profile error (P-V value) for the primary mirror is less than /10 and all the indexes of the primary mirror satisfy the requirements of the optical system.  
Practical method of shadow detection and removal for high spatial resolution remote sensing image 会议论文  OAI收割
MIPPR 2007: Remote Sensing and GIS Data Processing and Applications; and Innovative Multispectral Technology and Applications, Wuhan, China, November 15, 2007 - November 17,2007
Ru, Li; Bing, Zhang; Xia, Zhang; Zhengchao, Chen; Zheng, Wei; Lanfen, Zheng
收藏  |  浏览/下载:22/0  |  提交时间:2014/12/07