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近红外星图质心检测C样条插值法和高斯方法比较
引用本文:陆斌,郭少军,王铎.近红外星图质心检测C样条插值法和高斯方法比较[J].光电技术应用,2011(5):59-63.
作者姓名:陆斌  郭少军  王铎
作者单位:海军航空工程学院;
基金项目:国家自然科学基金(2010AAJ140)
摘    要:可见光CCD拍摄的星空图像中目标点的质心求取已经有了很多种方法,可见光中的恒星质心求取方法在近红外星图中同样适用,常用的方法有Gauss拟合法,矩方法(包括修正矩方法)和寻导法等。介绍了质心求取方法中的Gauss拟合法,分析其优劣性,并以这种方法为基础,根据近红外星图导航的实际情况提出了一种较为实用的方法,并验证比较其...

关 键 词:质心求取  C样条差值  高斯拟合  近红外星图

Centroid Detection of Targets on Near Infrared Stellar Map Based on C Spline Method and Gauss Method Comprision
LU Bin,GUO Shao-jun,WANG Duo.Centroid Detection of Targets on Near Infrared Stellar Map Based on C Spline Method and Gauss Method Comprision[J].Electro-Optic Technology Application,2011(5):59-63.
Authors:LU Bin  GUO Shao-jun  WANG Duo
Affiliation:LU Bin,GUO Shao-jun,WANG Duo(Naval Aeronautical and Astronautical University,Yantai 264001,China)
Abstract:The centroid of the visible light CCD image targets can be derived by using lots of methods,these algorithms are also suitable for the near infrared stellar map.The common methods are: Gauss fitting method,method of moments,derivative search and so on.The Gauss fitting method is introduced and analyzed its advantages and disadvantages.According to this method,a more practical method is proposed based on the near infrared stellar map navigation,verified and compared its accuracy and feasibility.
Keywords:centroid derivation  C spline interpolation  Gauss fitting  near infrared stellar map  
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