北京航空航天大学学报 ›› 2011, Vol. 37 ›› Issue (10): 1271-1276.doi: CNKI:11-2625/V.20111020.1127.013

• 论文 • 上一篇    下一篇

顾及星像点分布的恒星相机在轨检校

谢俊峰1, 江万寿2, 龚健雅2   

  1. 1. 国家测绘局 卫星测绘应用中心, 北京 100830;
    2. 武汉大学 测绘遥感国家重点实验室, 武汉 430079
  • 收稿日期:2010-05-24 出版日期:2011-10-30 发布日期:2011-11-03
  • 作者简介:谢俊峰(1981-),男,湖北天门人,助理研究员,junfengxie@gmail.com.
  • 基金资助:

    国家973计划资助项目(2006CB701300-G)

On-orbit calibration of stellar camera considering distribution of star image points

Xie Junfeng1, Jiang Wanshou2, Gong Jianya2   

  1. 1. The Satellite Mapping Application Center, State Bureau of Surveying and Mapping, Beijing 100830, China;
    2. State Key Laboratory of Information Engineering in Surveying, Mapping and Remote Sensing, Wuhan University, Wuhan 430079, China
  • Received:2010-05-24 Online:2011-10-30 Published:2011-11-03

摘要: 由于卫星发射前后以及在轨运行过程中,环境因素的变化都可能引起恒星相机参数发生改变,从而导致星敏感器姿态测量精度下降.将多片空间后方交会方法应用于恒星相机的在轨检校.在利用该方法检校时,实验发现检校结果的精度受到参与检校的恒星影像上星像点分布的影响,由此进一步提出了凸包面积百分比准则,该方法自动选取分布较好的影像用于检校,有助于提高检校精度.实验结果证明:基于后方交会进行恒星相机在轨检校时,利用凸包法选取的影像片进行检校的精度明显优于未选片时检校的结果.

Abstract: Although the parameters of the stellar camera are accurate by the ground calibration in advance, they will change due to the intense vibration in the process of the satellite launch or the change of space environmental factors such as the temperature, the atmospheric pressure, etc. The on-orbit calibration method based on the spatial resection with multi-images was applied to the stellar camera. The percentage of the convex hull area out of the star image was employed to choose the stellar image with good distribution since the calibration accuracy is related to the distribution of the star image points. The experiment result indicates that the calibration accuracy based on the selected images is better than that based on all the stellar images.

中图分类号: 


版权所有 © 《北京航空航天大学学报》编辑部
通讯地址:北京市海淀区学院路37号 北京航空航天大学学报编辑部 邮编:100191 E-mail:jbuaa@buaa.edu.cn
本系统由北京玛格泰克科技发展有限公司设计开发