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Chinese Academy of Sciences Institutional Repositories Grid
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浏览/检索结果: 共17条,第1-10条 帮助

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Self-organized voids revisited: Experimental verification of the formation mechanism 期刊论文  OAI收割
chin. phys. b, 2014, 卷号: 23, 期号: 7, 页码: 77901
作者:  
Song Juan;  Ye Jun-Yi;  Qian Meng-Di;  Luo Fang-Fang;  Lin Xian
收藏  |  浏览/下载:108/0  |  提交时间:2016/11/28
Self-organized voids revisited: Experimental verification of the formation mechanism 期刊论文  OAI收割
chin. phys. b, 2014, 卷号: 23, 期号: 7, 页码: 77901
作者:  
Song Juan;  Ye Jun-Yi;  Qian Meng-Di;  Luo Fang-Fang;  Lin Xian
收藏  |  浏览/下载:29/0  |  提交时间:2016/11/28
Simulation of a low energy beam transport line 期刊论文  OAI收割
NUCLEAR SCIENCE AND TECHNIQUES, 2012, 卷号: 23, 页码: 83-89
作者:  
Yao, Z (reprint author), Lanzhou Univ, Sch Nucl Sci & Technol, Lanzhou 730000, Peoples R China.;  Yang, Y;  Liu, ZW;  Zhang, WH;  Ma, HY
  |  收藏  |  浏览/下载:24/0  |  提交时间:2017/04/17
High accuracy star image locating and imaging calibration for star sensor technology (EI CONFERENCE) 会议论文  OAI收割
6th International Symposium on Precision Engineering Measurements and Instrumentation, August 8, 2010 - August 11, 2010, Hangzhou, China
作者:  
Wang Y.;  Wang Y.;  Wang Y.;  Wang Y.
收藏  |  浏览/下载:21/0  |  提交时间:2013/03/25
Today aircraft attitude measurement technology plays an important role in an aircraft system because it can provide orientation for aircraft in action. Lately star sensor technology used in aircraft attitude measurement has become more and more popular because of its high accuracy  light weight  without attitude accumulation errors and other advantages. There are three main steps for star sensor to measure aircraft attitude  star image locating  star identification and attitude tracking. The latter two steps are based on the accuracy of star image locating. So it's critical to make efforts to advance the accuracy of star image locating. Some imaging errors  such as spherical aberration or coma aberration  also have negative effect on the accuracy of star image locating  of which the effect is necessarily reduced as well. At the beginning of this article  the structure of star sensor hardware is introduced. Secondly three methods for star image locating are described specifically  which are traditional centroid method  Gauss quadric fitting method and improved Gauss quadric fitting method. Subsequently an imaging calibration method is described for the purpose of reducing the effect of imaging errors. Finally the experiment shows that the accuracy of the star sensor is 2-arc-second. 2010 SPIE.  
Expansion of interatomic distances in platinum catalyst nanoparticles 期刊论文  OAI收割
Acta Materialia, 2010, 卷号: 58, 期号: 3, 页码: 836-845
K. Du; F. Emst; M. C. Pelsozy; J. Barthel; K. Tillmann
收藏  |  浏览/下载:96/0  |  提交时间:2012/04/13
Structural characterization of interfaces in epitaxial Fe/MgO/Fe magnetic tunnel junctions by transmission electron microscopy 期刊论文  OAI收割
PHYSICAL REVIEW B, 2010, 卷号: 82, 期号: 2
Wang, C; Kohn, A; Wang, SG; Chang, LY; Choi, SY; Kirkland, AI; Petford-Long, AK; Ward, RCC
收藏  |  浏览/下载:17/0  |  提交时间:2013/09/24
Effects of Monochromatic Aberration on Visual Acuity Using Adaptive Optics 期刊论文  OAI收割
OPTOMETRY AND VISION SCIENCE, 2009, 卷号: 86, 期号: 7, 页码: 868-874
作者:  
Li, Shiming;  Xiong, Ying;  Li, Jing;  Wang, Ningli;  Dai, Yun
收藏  |  浏览/下载:18/0  |  提交时间:2015/09/21
The first observation of titanate nanotubes by spherical aberration corrected high-resolution transmission electron microscopy 期刊论文  OAI收割
superlattices and microstructures, 2009, 卷号: 46, 期号: 1-2, 页码: 357-364
作者:  
Miao, L.;  Tanemura, S.;  Jiang, T.;  Tanemura, M.;  Yoshida, K.
收藏  |  浏览/下载:24/0  |  提交时间:2016/10/27
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:25/0  |  提交时间:2013/03/25
A spherical catadioptric telescope system based on Cooke corrector group (EI CONFERENCE) 会议论文  OAI收割
Novel Optical Systems Design and Optimization XII, August 3, 2009 - August 4, 2009, San Diego, CA, United states
作者:  
Zhang J.;  Liu W.;  Zhang J.;  Zhang J.
收藏  |  浏览/下载:31/0  |  提交时间:2013/03/25
To obtain a number of advantages in fabrication  testing and alignment  many designs in which spherical mirrors replace classical Cassegrain-form aspheric mirrors are present in the literature. However  spherical mirrors suffer from substantial spherical aberration and thereby require some form of corrector group. But in this case  the question encountered is that of making the basic optical configuration more complex. In this paper  a new design based on Cooke corrector group is presented for eliminating spherical aberration  which is believed to provide higher performance with less complexity than previous approaches. Besides  the cost and fabrication period will be extremely decreased. The telescope system using corrector group here can achieve good optical performance with f# of 10  full field of 0.5  obscuration of 1/3 and MTF (Modulation Transfer Function) of 0.48 corresponding to 50@lp/mm. 2009 Copyright SPIE - The International Society for Optical Engineering.