首页 | 本学科首页   官方微博 | 高级检索  
     检索      

?????????????????????????????
引用本文:陈俊平,王解先.?????????????????????????????[J].大地测量与地球动力学,2007,27(4):57-61.
作者姓名:陈俊平  王解先
作者单位:1. 同济大学测量与国土信息工程系,上海,200092;GeoForschungsZentrum Potsdam,14473,Potsdam,Germany
2. 同济大学测量与国土信息工程系,上海,200092;现代工程测量国家测绘局重点实验室,上海,200092
基金项目:国家自然基金重点项目(40234039)
摘    要:????????λPPP?????????????????ù???????????????????????????? ???????????????????????????????????????????????????????????????????????????????????????о????н??????? ????????????CHAMP??RACE????????????????????ο?????????????CHAMP???????????ο??????XYZ3?????????????????????0.22 m??0.22 m??0.25 m???????????????0.41 m??GRACE??A??????????????ο??????XYZ 3?????????????????????0.27 m??0.23 m??0.29 m???????????????0.45 m??

关 键 词:GPS  CHAMP  GRACE  ???????  ???????????  
文章编号:1671-5942(2007)04-0057-06
修稿时间:2007-02-05

KINEMATIC PRECISE ORBIT DETERMINATION OF LOW EARTH ORBITER BASED ON EPOCH-DIFFERENCE STRATEGY
Chen Junping,Wang Jiexian.KINEMATIC PRECISE ORBIT DETERMINATION OF LOW EARTH ORBITER BASED ON EPOCH-DIFFERENCE STRATEGY[J].Journal of Geodesy and Geodynamics,2007,27(4):57-61.
Authors:Chen Junping  Wang Jiexian
Institution:1. Department of Surveying and Geomatics , Tongji University, Shanghai 200092 ; 2. GeoForschungsZentrum Potsdam, 14473, Potsdam, Germany; 3.Key Laboratory of Modern Engineering Surveying, State Bureau of Surveying and Mapping, Shanghai 20092
Abstract:On the basis of the theory of Precise Point Positioning (PPP), a kinematic algorithm ——POD(Precise Orbiter Determination) based on an epoch wise processing of the code observations combined with an epoch-differece processing of the phase observations is introduced. The method allows recovering the trajectory of the LEO without making use of any a priori dynamic perturbation, e.g., gravity field information and air drag, it may be very useful for gravity field recovery. Experiments with CHAMP and GRACE observations over a period of 2 weeks show that kinematic orbits of CHAMP have an average 3D RMS about 0.41m comparing to reference orbits, while the average 3D RMS of GRACE is 0.45 m,the average RMS of the 3 axes component (0.22,0.22,0.25) m are of CHAMP and (0.27,0.23,0.29) m of GRACE.
Keywords:GPS  CHAMP  GRACE  low earth orbiter  kinematic POD(Precise Orbiter Determination)
本文献已被 CNKI 维普 万方数据 等数据库收录!
点击此处可从《大地测量与地球动力学》浏览原始摘要信息
点击此处可从《大地测量与地球动力学》下载免费的PDF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