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星敏数据转换为参考系欧拉角姿态的方法

淡鹏 王丹 郭延臣

电讯技术2016,Vol.56Issue(12):1340-1345,6.
电讯技术2016,Vol.56Issue(12):1340-1345,6.DOI:10.3969/j.issn.1001-893x.2016.12.007

星敏数据转换为参考系欧拉角姿态的方法

Method for Transferring Star Sensor Attitude to Reference Coordinate Euler Angle

淡鹏 1王丹 2郭延臣3

作者信息

  • 1. 宇航动力学国家重点实验室,西安710043
  • 2. 西安卫星测控中心,西安710043
  • 3. 西安卫星测控中心,西安710043
  • 折叠

摘要

Abstract

The measurement data of star sensor for three-axis stabilized satellites' attitude often need to be converted to the Euler angle in a reference coordinate system. In view of this,the conversion methods are summarized,including the conversion from star sensor data to attitude matrix and conversion from attitude matrix to the Euler angles. From the programming point of view,a way to calculate full-scale Euler angle is also given under 312&321 transform orders which are often used in project. Then some error factors are an-alyzed,and the transform order suggested for geostationary satellite is also provided according to analysis. The results indicate that the method is correct and useful for the attitude calculation and error analysis of three-axis stabilized satellites.

关键词

三轴稳定卫星/卫星姿态控制/星敏感器/欧拉角解算

Key words

three-axis stabilized satellite/satellite attitude control/star sensor/Euler angle calculation

分类

航空航天

引用本文复制引用

淡鹏,王丹,郭延臣..星敏数据转换为参考系欧拉角姿态的方法[J].电讯技术,2016,56(12):1340-1345,6.

电讯技术

OA北大核心CSTPCD

1001-893X

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