首页 | 官方网站   微博 | 高级检索  
     

基于光斑高斯拟合的大视场星相机定焦方法
引用本文:邸晶晶,王伟之,任宇宁,于艳波,宗云花,贾永丹,王妍.基于光斑高斯拟合的大视场星相机定焦方法[J].半导体光电,2019,40(2):261-265.
作者姓名:邸晶晶  王伟之  任宇宁  于艳波  宗云花  贾永丹  王妍
作者单位:北京空间机电研究所,北京,100094;北京空间机电研究所,北京,100094;北京空间机电研究所,北京,100094;北京空间机电研究所,北京,100094;北京空间机电研究所,北京,100094;北京空间机电研究所,北京,100094;北京空间机电研究所,北京,100094
基金项目:国家重点研发计划地球观测与导航重点专项项目(2016YFB0500802).
摘    要:针对高精度立体测绘任务对星相机的使用要求,提出了一种基于光斑高斯拟合的星相机焦面定焦方法。首先,搭建了基于星点靶标和平行光管的定焦系统,通过移动靶标在中心和边缘视场获取多幅不同程度的离焦图像;其次,采用基于平方加权的质心定位算法计算各视场靶标点像的精确位置用于像面拟合;然后,采用Gibbs采样/马尔可夫蒙特卡洛法对每个光斑进行高斯曲面拟合,获取星点的高斯半径,通过对各视场的最佳焦面位置进行最小二乘拟合,得到最佳像面。对上述定焦方法进行了试验验证,结果表明星相机在各视场的能量集中度测量值与设计值符合,星相机在轨拍摄的星点图像满足要求。

关 键 词:星相机  定焦方法  高斯拟合  大视场
收稿时间:2018/11/17 0:00:00

Focus Locating Method on Guassian Fitting of Light Spot for Wide Field Star Camera
DI Jingjing,WANG Weizhi,REN Yuning,YU Yanbo,ZONG Yunhu,JIA Yongdan and WANG Yan.Focus Locating Method on Guassian Fitting of Light Spot for Wide Field Star Camera[J].Semiconductor Optoelectronics,2019,40(2):261-265.
Authors:DI Jingjing  WANG Weizhi  REN Yuning  YU Yanbo  ZONG Yunhu  JIA Yongdan and WANG Yan
Affiliation:Beijing Institute of Space Mechanics & Electricity, Beijing 100094, CHN,Beijing Institute of Space Mechanics & Electricity, Beijing 100094, CHN,Beijing Institute of Space Mechanics & Electricity, Beijing 100094, CHN,Beijing Institute of Space Mechanics & Electricity, Beijing 100094, CHN,Beijing Institute of Space Mechanics & Electricity, Beijing 100094, CHN,Beijing Institute of Space Mechanics & Electricity, Beijing 100094, CHN and Beijing Institute of Space Mechanics & Electricity, Beijing 100094, CHN
Abstract:Aiming at the requirements of star camera for high precision stereo mapping, a focus locating method based on Guassian fitting of light spot is introduced. Firstly, a focus locating system was built with a point target and a collimator. Several defocused photos were taken by moving the target in central and fringe fields of view. Secondly, an algorithm of centroid locating on squared weighting method was used to calculate the precise location in each field of view to fit the image surface, and an algorithm of Gibbs sampling and Markov Chain Monte Carlo was applied to each light spot to make Guassian curve fitting, to get the Guassian radius of each light spot. Then, the best focal plane was acquired by least squares fitting of the optimum focal planes in each field of view. Tests verify that the enegy focusability in each field of view agrees with the design value, and the pictures taken on orbit meet requirements.
Keywords:star camera  focus locating  Guassian fitting  wide field of view
本文献已被 万方数据 等数据库收录!
点击此处可从《半导体光电》浏览原始摘要信息
点击此处可从《半导体光电》下载全文
设为首页 | 免责声明 | 关于勤云 | 加入收藏

Copyright©北京勤云科技发展有限公司    京ICP备09084417号-23

京公网安备 11010802026262号