摘要
运用数字天顶仪进行天文定位时,需采用最小二乘算法建立电荷耦合元件图像坐标系和天球切平面坐标系之间的映射关系。针对最小二乘算法只考虑了观测量中的误差,没有顾及系数矩阵中的误差和数据中可能存在的粗大误差问题,为了提高数字天顶仪进行天文定位时的解算精度,将最小二乘算法与总体最小二乘算法进行有效结合构成了混合最小二乘算法,该算法能够同时顾及坐标转换中系数矩阵和观测量中的误差。为了消除识别恒星数据中可能存在的粗大误差对天文解算的影响,对所提算法进行了稳健加权,并结合星等设置合理的权阵。数据分析的结果证明,稳健加权混合最小二乘算法在进行天文解算时具有较高的精度。
It is necessary to use the least square algorithm to establish the mapping relationship between the charge-coupled device(CCD)image coordinate system and the celestial tangent plane coordinate system when using the digital zenith camera for astronomical positioning.The least squares algorithm only considers the errors in the observation,but does not consider the errors in the coefficient matrix and the possible gross errors in the data.In order to improve the accuracy of the digital zenith camera in astronomical positioning,the least squares algorithm and the total least squares algorithm are effectively combined to form a mixed least squares algorithm,which can take into account the errors of the coefficient matrix and observation in coordinate transformation.In order to eliminate the influence of the possible gross errors in star recognition data on astronomical solution,the proposed algorithm is weighted robustly,and a reasonable weight matrix is set combined with magnitude.The results of data analysis show that the robust weighted mixed least squares algorithm has high accuracy in astronomical solution.
作者
黄坤阳
刘先一
张志利
HUANG Kunyang;LIU Xianyi;ZHANG Zhili(Institute of Missile Engineering,Rocket Force University of Engineering,Xi’an 710025,China;Unit 96901 of the PLA,Beijing 100080,China)
出处
《系统工程与电子技术》
EI
CSCD
北大核心
2021年第6期1659-1663,共5页
Systems Engineering and Electronics
基金
国家自然科学基金(41174162)资助课题。
关键词
数字天顶仪
坐标转换
混合最小二乘
稳健加权
digital zenith camera
shift between coordinates
mixed least squares
robust weighting
