宇航计测技术

• 论文 • 上一篇    下一篇

星载立体测绘相机立方镜间姿态标定

黄桂平1； 钦桂勤2；马开锋1   

  1. 1、华北水利水电大学，郑州 450001；
    2、信息工程大学，郑州 450052
  • 出版日期:2013-08-15 发布日期:2013-08-15
  • 作者简介:黄桂平（1973-），男，博士、副教授，主要研究方向：大尺寸三维测量、精密工程测量和工业摄影测量等方向的研究。
  • 基金资助:
    国家863计划（2008AA042410），国家科技重大专项（2009ZX04014-093）

Attitude Calibration on Three-line Array CCD Camera of Space Stereo Mapping

HUANG Gui-ping1；Qin Gui-qin2；MA Kai-feng1   

  1. 1、North China University of Water Resources and Electric Power, Zhengzhou 450011;
    2、Institute of Geomatics，Information Engineering University, Zhengzhou 450052
  • Online:2013-08-15 Published:2013-08-15

PDF (PC)

524

摘要： 介绍了测绘相机立方镜与星敏感器立方镜间坐标系转换关系的标定方法。采用4台自准直经纬仪分别对两个立方镜进行准直测量，建立立方镜坐标系，并推导了基于准直测量角度的立方镜坐标系的旋转矩阵公式；利用经纬仪间短边互瞄方法实现两个立方镜间姿态的传递。标定试验表明，该方法可以标定出两立方镜坐标轴间夹角以及测绘相机间的姿态关系，满足了相机研制要求。

关键词: 三线阵CCD相机, 立体测绘, 姿态标定, 立方镜, 准直测量

Abstract: One method for calibrating the transformation matrix of cubic prism coordinate system between stereo mapping camera and star sensor was adopted. Autocollimation on two cubic prisms was finished using 4 theodolites. After that, the cubic prism coordinate system was set up. And the detailed equations of rotation matrix were deduced too. The attitude between two cubic prisms was calibrated by azimuth transmission. Tests indicate that the calibration error of angle between two cubic prism coordinate system axes is less than 1.5″(1δ）. The error of final attitude calibration of the stereo mapping camera is less than 5″（1δ）.

Key words: Three-line array CCD camera, Stereo mapping, Attitude calibration, Cubic prism, Collimation measurement

京ICP备09048426号-4　 京公网安备 11010602060144号　版权所有 © 《宇航计测技术》编辑部