An analysis of the wide area differential method of geostationary orbit satellites

This work aims to obtain a wide area differential method for geostationary orbit (GEO) constellation. A comparison between the dilution of precision (DOP) of four-dimensional (4D) calculation including sa- tellite clock errors and ephemeris errors and that of three-dimensional (3D) calculation only...

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Bibliographic Details
Published inScience China. Physics, mechanics & astronomy Vol. 52; no. 2; pp. 310 - 314
Main Authors Cai, ChengLin, Li, XiaoHui, Wu, HaiTao
Format Journal Article
LanguageEnglish
Published Heidelberg SP Science in China Press 01.02.2009
Springer Nature B.V
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Summary:This work aims to obtain a wide area differential method for geostationary orbit (GEO) constellation. A comparison between the dilution of precision (DOP) of four-dimensional (4D) calculation including sa- tellite clock errors and ephemeris errors and that of three-dimensional (3D) calculation only including ephemeris errors with the inverse positioning theory of GPS shows the conclusion that all the 3D PDOPs are greatly reduced. Based on this, a basic idea of correcting satellite clock errors and ephem- eris errors apart is put forward, and moreover, a specific method of separation is proposed. Satellite clock errors are separated in a master station with time synchronization, and all the remaining pseu- do-range errors after the satellite clock errors have been deducted are used to work out ephemeris corrections of all GEO satellites. By a comparative analysis of user positioning accuracy before and after differential, the wide area differential method is verified to be quite valid for GEO constellation.
Bibliography:11-5000/N
CAI ChengLin1,2,3?, LI XiaoHui1 & WU HaiTao1 1 National Time Service Center, Chinese Academy of Sciences, Lintong 710600, China; 2 Hunan Institute of Humanities, Science and Technology, Loudi 417000, China; 3 Graduate University of Chinese Academy of Sciences, Beijing 100049, China
ObjectType-Article-2
SourceType-Scholarly Journals-1
ObjectType-Feature-1
content type line 23
ISSN:1674-7348
1672-1799
1869-1927
1862-2844
DOI:10.1007/s11433-009-0036-y