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A Radiation Accumulation Based Detection Algorithm for Rectilinear-Motion Infrared Dim Target with Constant Acceleration 会议论文  OAI收割
1st International Conference on Multimedia and Image Processing, ICMIP 2016, Bandar Seri Begawan, Brunei, June 1-3, 2016
作者:  
Ma TL(马天磊);  Shi ZL(史泽林);  Xu BS(徐保树);  Yin J(尹健);  Liu YP(刘云鹏)
收藏  |  浏览/下载:19/0  |  提交时间:2016/11/06
Multi-type sweeping for improving the efficiency of flow accumulation calculation 会议论文  OAI收割
2012 20th International Conference on, 香港, 2012-6-15~17
Yuanzhi Yao(姚远志); Heping Tao(陶和平); Xun Shi(施迅)
收藏  |  浏览/下载:9/0  |  提交时间:2012/12/26
Loosen solid materials discrimination at debris flow source area-Take Dujiangyan Guojuanyan gully as an example 会议论文  OAI收割
2012 2nd International Conference on Remote Sensing, Environment and Transportation Engineering, 中国南京, 2012-6-1
作者:  
Jun Wang;  Guoqiang Ou;  Huali Pan
收藏  |  浏览/下载:11/0  |  提交时间:2012/12/26
Electron cooling experiments in CSR 会议论文  OAI收割
作者:  
Yang XiaoDong;  Li Jie;  Mao LiJun;  Li GuoHong;  Ma XiaoMing
  |  收藏  |  浏览/下载:96/0  |  提交时间:2018/08/20
Electron cooling experiments in CSR 会议论文  OAI收割
作者:  
Yang XiaoDong;  Li Jie;  Mao LiJun;  Li GuoHong;  Ma XiaoMing
  |  收藏  |  浏览/下载:95/0  |  提交时间:2018/08/20
SGCMG design and time accumulation error analysis (EI CONFERENCE) 会议论文  OAI收割
2011 International Conference on Mechatronic Science, Electric Engineering and Computer, MEC 2011, August 19, 2011 - August 22, 2011, Jilin, China
Xu W.
收藏  |  浏览/下载:15/0  |  提交时间:2013/03/25
Electronic system design of ultraviolet ozone vertical profile probe for aerography satellite (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
Song K.; Wang S.
收藏  |  浏览/下载:15/0  |  提交时间:2013/03/25
The design of ultraviolet ozone vertical profile probe is illustrated and the electronic system is introduced in detail. The device is a compact  high precision  ultraviolet-vacuum  ultraviolet spectral radiometer  and is used to measure atmospheric solar backscattering spectral radiance and solar spectral irradiance. Noise of the system is analyzed and Numeric accumulation and synchronous demodulation was used to decrease the noise and the zero-drift of the instrument. The solar irradiance at altitude 830 km in 160-400 nm and the backscattering solar spectral radiance in the ultraviolet ozone absorption band at 12 wavelengths from 250 nm to 340 nm are obtained. Test results on orbit show that all the requested function is met successfully and the performance is stable. 2011 IEEE.  
Influence of debris flow on channel evolution 会议论文  OAI收割
Padua, 2011
作者:  
Liu, Jiankang;  Cheng, Zunlan;  Zhang, Xiaogang
  |  收藏  |  浏览/下载:22/0  |  提交时间:2018/11/08
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:12/0  |  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.  
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.
收藏  |  浏览/下载:50/0  |  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.