基于Kittler最小误差分割算法的小视场星图分割  

Segmentation of Small-Field-of-Viewstar Images Based on Kittler Minimum Error Algorithm

作　　者：时春霖 杨培章 张超[1] 杜兰[1,4] 叶凯 范承啸 李建 祖安然 SHI Chunlin;YANG Peizhang;ZHANG Chao;DU Lan;YE Kai;FAN Chengxiao;LI Jian;ZU Anran(Geospatial Information Academy,Information Engineering University,Zhengzhou 450001,China;The PLA Troop 61206,Beijing 100042,China;The PLA Air Force Political Work Department,Beijing 100843,China;Beijing Satellite Navigation Center,Beijing 100094;Beijing Aerospace Flight Control Center,Beijing 100089,China)

机构地区：[1]信息工程大学地理空间信息学院,河南郑州450001 [2]中国人民解放军61206部队,北京100042 [3]中国人民解放军空军政治工作部,北京100843 [4]北京卫星导航中心,北京100094 [5]北京航天飞行控制中心,北京100089

出　　处：《西南交通大学学报》2021年第1期168-175,共8页Journal of Southwest Jiaotong University

基　　金：国家自然科学基金(41604011,41774038,41804034,41704006)。

摘　　要：小视场星图易受光照不均和噪声影响,常用阈值分割算法存在处理效果不佳或效率较低的不足.针对星图灰度的高斯分布特征,基于贝叶斯最小误差理论,提出利用Kittler最小误差分割算法处理小视场星图.以视频测量机器人为测量平台,以"优度法"、区域一致性、区域对比度和时间复杂度为评价指标,对比了常用的阈值分割算法和一维最大熵法,验证了Kittler算法在确保星图良好分割的同时,星图处理效率可以提高70%左右.基于半仿真星图和真实星图的室内试验表明,Kittler算法可以准确提取星点质心坐标,水平和垂直方向均方根误差分别为0.025像素和0.019像素;采用该算法的野外天文定位实测表明,经纬度内符合平均精度分别优于0.015 s和0.22″,外符合精度分别优于0.025 s和0.35″,可以满足一等天文测量的精度要求.Compared with conventional images,small-field-of-view star images are more susceptible to the impacts of uneven illumination and measurement noises.Meanwhile,the traditional threshold segmentation algorithm has poor processing effect or efficiency.In terms of the Gaussian distribution of star image gray,the Kittler minimum error segmentation algorithm was used to process star images on the basis of Bayesian minimum error theory.By the use of the video measuring robot,several commonly-used threshold segmentation algorithms and one-dimensional maximum entropy algorithm are compared and analyzed in terms of goodness methods,regional consistency,regional contrast ratio and time complexity.It is indicated that the Kittler minimum error segmentation algorithm can achieve a satisfied segmentation of the small-field-of-view star images,and improves astronomical data processing efficiency significantly withthe average computation timereduced by about 70%.Laboratory experiments for semi-simulation star map and real star mapshow that the proposed algorithm can extract star points and obtain centroid coordinates accurately,whose horizontal and vertical root mean square errors are 0.025 and 0.019 pixels,respectively.Furthermore,extensive field experiments show that the astronomical longitude and latitude calculated by the proposed algorithm can meet first-class astronomical survey accuracy requirements,whose average internal accordant accuracy is better than 0.015 s and 0.22″respectively,and external accordant accuracy is better than 0.025 s and 0.35″respectively.

关 键 词：天文测量 高斯分布 图像分割 Kittler最小误差法 小视场星图 

分 类 号：P114[天文地球—天文学] TP751[自动化与计算机技术—检测技术与自动化装置]