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长春光学精密机械与物... [4]
清华大学 [1]
北京大学 [1]
国家天文台 [1]
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会议论文 [5]
期刊论文 [2]
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2016 [1]
2010 [5]
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Hierarchical classification for the topography analysis of Asteroid (4179) Toutatis from the Chang'E-2 images
期刊论文
ICARUS, 2016, 卷号: 278, 页码: 119-127
作者:
Zheng, Chen
;
Ping, Jinsong
;
Wang, Mingyuan
收藏
  |  
浏览/下载:69/0
  |  
提交时间:2017/02/15
Asteroids
surfaces
Image processing
Satellites of asteroids
一种CCD星图星点快速定位算法
期刊论文
2010, 2010
王兆魁
;
张育林
;
WANG Zhaokui
;
ZHANG Yulin
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  |  
浏览/下载:5/0
High Accuracy Star Image Locating and Imaging Calibration for Star Sensor Technology
会议论文
2010
Zhang S. D.
;
Zhang Z. J.
;
Sun H. H.
;
Wang Y. J.
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  |  
浏览/下载:4/0
  |  
提交时间:2013/03/28
High accuracy star image locating and imaging calibration for star sensor technology (EI CONFERENCE)
会议论文
6th International Symposium on Precision Engineering Measurements and Instrumentation, August 8, 2010 - August 11, 2010, Hangzhou, China
Zhang S.
;
Zhang Z.
;
Sun H.
;
Wang Y.
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  |  
浏览/下载:13/0
  |  
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
2010 International Conference on Computer, Mechatronics, Control and Electronic Engineering, CMCE 2010, August 24, 2010 - August 26, 2010, Changchun, China
Zhang S.
;
Sun H.
;
Wang Y.
;
Jia X.
;
Chen H.
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浏览/下载:51/0
  |  
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.
High-precision algorithm for centroid location of star pattern recognition
会议论文
Xu, Wencong
;
Chu, Tianguang
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  |  
浏览/下载:3/0
  |  
提交时间:2015/11/13
Active pixel sensor geometrical characteristic effects on star image subdivided locating accuracy for star tracker (EI CONFERENCE)
会议论文
ICO20: Remote Sensing and Infrared Devices and Systems, August 21, 2005 - August 26, 2005, Changchun, China
Li J.
;
Liu J.
;
Hao Z.
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浏览/下载:21/0
  |  
提交时间:2013/03/25
Active pixel sensor (APS) star tracker becomes an investigated hotspot because of its technical advantages. And centroid algorithm is a subpixel method proper to star position calculation because of its high accuracy and simplicity. When centroid algorithm is applied on APS star tracker
APS pixel geometrical characteristics might effect on star image position accuracy. Because the amplifier circuit and other function circuits inter pixel of APS take up some pixel area
the Fill Factor is less than 100%. Moreover
the active sensitive area has a certain geometrical shape
such as square
rectangle and L shape. The Fill Factor of pixel influences on star image subdivided locating accuracy when using centioid algorithm. In this paper
we have analyzed all pixel geometrical characteristics influence on the star position accuracy. From simulation experiments
we can conclude that Fill factor and pixel geometric shape influence on star position accuracy. The star locating error increased when Fill Factor decreased
and different geometrical shape of active sensitive area of pixel can make different influence on star location accuracy
the symmetrical sensitive area in x or y axis have symmetrical location error in the same axis.
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