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西北工业大学
收稿日期:2011-03-22,
修回日期:2011-05-10,
网络出版日期:2011-12-06,
纸质出版日期:2011-12-26
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孙瑾秋,周军,张臻,张永鹏. 基于能量累加的空间目标星象质心定位方法[J]. 光学精密工程, 2011, 19(12): 0-0.
XUN Jin-Qiu,ZHOU Jun,ZHANG Zhen,ZHANG Yong-Peng. Space Target Centroid Location based on Energy Accumulate Method[J]. Editorial Office of Optics and Precision Engineering, 2011, 19(12): 0-0.
为了有效的提高目标星象的天文定位精度,CCD观测图像的亚象素级高精度质心定位技术的研究至关重要。本文首先系统的分析了影响定位精度的主要因素,如图像噪声、离散化采样误差及定位窗口选择等;在此基础上,通过结合CCD弥散斑的成像特性,提出了一种基于能量累加的空间目标星象质心定位方法。该方法通过插值方式降低离散采样点和实际感光区域光线照度的不一致性,并通过弥散斑能量累加自适应确定目标星象的有效窗口,通过对目标星象灰度优化消除随机噪声影响的基础上,采用平方加权质心定位方法进行质心计算。实验结果表明,该方法具有较强的抗干扰能力和稳定性,定位精度可达到0.01像元,可适用于低信噪比条件下的质心定位计算。
In order to effectively improve the precision of the astronomical determination of space target
sub-pixel positioning technology research is very important for CCD exploration images. This article firstly systematic analysis of the main factors which affect the positioning accuracy
such as image noise
discrete sampling error and window selection etc.. Combining with the CCD imaging characteristics
a target centroid location method which based on energy accumulation is proposed. This method using interpolation technique to reduce the inconsistency which caused by the difference between the actual sensitive area light intensity and discrete sample points
and then by energy accumulation of diffuse plaque to adaptive selection the correct target window
by gray optimizing for the target to reducing random noise effect
finally using squared weighted centroid localization method to get the high precision position. Experimental results show that the method has strong anti-interference ability and stability
positioning accuracy can reach 0.01 pixels. It is suitable for low SNR condition.
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