基于星间光学测量的多星联合定轨  

Multi-satellite joint orbit determination based on inter-satellite optical measurement

作　　者：周凤岐[1] 张轲[1] 叶修松[2] 薛嘉[2] 

机构地区：[1]西北工业大学航天学院,陕西西安710072 [2]中国西安卫星测控中心,陕西西安710043

出　　处：《西北大学学报（自然科学版）》2013年第1期27-32,共6页Journal of Northwest University（Natural Science Edition）

基　　金：国家自然科学基金资助项目(40774031)

摘　　要：目的为了节约测控资源。方法采用天地基测量的卫星星座联合轨道确定,同时阐述了基于星间光学测量的多星精密轨道确定的关键技术,给出了星间光学测量模型及对应的偏导数计算公式,分析了多星联合定轨所面临的主要问题及应对的解决方案。结果实现了真正的多星同步轨道积分。结论对天基监测的非合作目标卫星轨道确定进行了计算分析,为天地基一体化联合多星定轨提供了基础。Aim To save TT＆C resource. Methods Satellite constellation joint orbit was determined based on space-based and ground-based measurement data. The key technologies of multi-satellite precise orbit determination was described based on inter-satellite optimal measurement data, the inter-satellite optimal measurement model and the corresponding partial derivatives calculation formula was provided, the main problems of tile multi-satellite joint orbit determination analyzed. Results The real multi-satellite synchronous integration was obtained. Conclusion The non-cooperative satellite orbit determination was analyzed based on space-based monitoring data, which set the foundation for the space-based and ground-based joint multi-satellite orbit determination.

关 键 词：监视卫星 联合定轨 天基监测 

分 类 号：TP43[自动化与计算机技术]