Volume 43 Issue 9
Oct.  2014
Turn off MathJax
Article Contents

Liao Yufu, Zhong Jianyong, Chen Dong. Estimation of degradation parameters of smearing star image based on motion trajectory of star’s centroid[J]. Infrared and Laser Engineering, 2014, 43(9): 3162-3167.
Citation: Liao Yufu, Zhong Jianyong, Chen Dong. Estimation of degradation parameters of smearing star image based on motion trajectory of star’s centroid[J]. Infrared and Laser Engineering, 2014, 43(9): 3162-3167.

Estimation of degradation parameters of smearing star image based on motion trajectory of star’s centroid

  • Received Date: 2014-01-10
  • Rev Recd Date: 2014-02-25
  • Publish Date: 2014-09-25
  • Star' s gray intensity wouldn' t follow 2-D Gaussian distribution when the rotational velocity exceeded the highest rotational velocity which would affect the processing precision of centroid of star spot. The analytical solution of motion trajectory of star' s centroid was simplified considering that the exposure time was short enough, and then the precision of the linear approximation was analyzed through simulation. The character of gray intensity of smearing star was analyzed based on the simplified trajectory, then a novel algorithm was proposed to estimate the degradation parameters of smearing star image. Through simulation and experiment, the validity of the proposed algorithm has been testified, the largest error of estimated blur length is around 0.8 of a pixel, while error of the estimated blur direction is about 2, feasibility of the proposed method has also been validated through simulations.
  • [1] Liebe C C. Accuracy performance of star tracks-a tutorial[J].Aerospace and Electronical System, 2002, 38(2): 587-599.
    [2]
    [3] Wang Haiyong, Zhou Wenrui, Cheng Xuan, et al. Imagesmearing modeling and verification for strapdown star sensor[J]. Chinese Journal of Aeronautics, 2012, 25(1): 115-123.
    [4]
    [5]
    [6] Samaan M A, Pollock T C, Junkins J L. Predictivecentroiding for star trackers with the effect of imagesmearing [J]. The Journal of Astronautical Sciences, 2002,50(1): 1-14.
    [7] Zhang Weina, Quan Wei, Guo Lei. Blurred star imageprocessing for star sensor under dynamic conditions [J].Sensor, 2012, 12(5): 6712-6726.
    [8]
    [9] Wu Xiaojuan, Wang Xinlong. Multiple blur of star imageand the restoration under dynamic conditions [J]. ActaAstronautica, 2011, 68(11-12): 1903-1913.
    [10]
    [11]
    [12] Irwan R, Lane R G. Analysis of optimal centroid estimationapplied to Shack-Hartman sensing [J]. Applied Optics, 1999,38(32): 6737-6743.
    [13] Arines J, Ares J. Minimum variance centroid thresholding[J]. Optics Letters, 2002, 27(7): 497-499.
    [14]
    [15]
    [16] Anup Bharat Katake. Modeling, image processing and attitudeestimation of high speed star sensors [D]. US: Texas AMUniversity, 2006: 91-93.
    [17]
    [18] Samaan M A. Toward faster and more accurate star sensorsusing recursive centroiding and star identification [D].US:Texas AM University, 2003: 95-97.
    [19] Yitzhaky Y, Mor I, Lantzman A, et al. Direct method forrestoration of motion-blurred images [J]. Journal of theOptical Society of America A: Optics, Image Science, 1998,15: 1512-1519.
    [20]
    [21] Levin A. Blind motion deblurring using image statistics [C]//NIPS, 2007: 841-848.
  • 加载中
通讯作者: 陈斌, bchen63@163.com
  • 1. 

    沈阳化工大学材料科学与工程学院 沈阳 110142

  1. 本站搜索
  2. 百度学术搜索
  3. 万方数据库搜索
  4. CNKI搜索

Article Metrics

Article views(855) PDF downloads(131) Cited by()

Related
Proportional views

Estimation of degradation parameters of smearing star image based on motion trajectory of star’s centroid

  • 1. Institute of Optics and Electronics,Chinese Academy of Sciences,Chengdu 610200,China;
  • 2. University of Chinese Academy of Sciences,Beijing 100049,China

Abstract: Star' s gray intensity wouldn' t follow 2-D Gaussian distribution when the rotational velocity exceeded the highest rotational velocity which would affect the processing precision of centroid of star spot. The analytical solution of motion trajectory of star' s centroid was simplified considering that the exposure time was short enough, and then the precision of the linear approximation was analyzed through simulation. The character of gray intensity of smearing star was analyzed based on the simplified trajectory, then a novel algorithm was proposed to estimate the degradation parameters of smearing star image. Through simulation and experiment, the validity of the proposed algorithm has been testified, the largest error of estimated blur length is around 0.8 of a pixel, while error of the estimated blur direction is about 2, feasibility of the proposed method has also been validated through simulations.

Reference (21)

Catalog

    /

    DownLoad:  Full-Size Img  PowerPoint
    Return
    Return