Abstract
Different types of GPS clock and orbit data provided by the International GPS Service (IGS) have been used to assess the accuracy of rapid orbit determination for satellites in low Earth orbit (LEO) using spaceborne GPS measurements. To avoid the need for reference measurements from ground-based reference receivers, the analysis is based on an undifferenced processing of GPS code and carrier-phase measurements. Special attention is therefore given to the quality of GPS clock data that directly affects the resulting orbit determination accuracy. Interpolation of clock data from the available 15 min grid points is identified as a limiting factor in the use of IGS ultra-rapid ephemerides. Despite this restriction, a 10-cm orbit determination accuracy can be obtained with these products data as demonstrated for the GRACE-B spacecraft during selected data arcs between 2002 and 2004. This performance may be compared with a 5-cm orbit determination accuracy achievable with IGS rapid and final products using 5 min clock samples. For improved accuracy, high-rate (30 s) clock solutions are recommended that are presently only available from individual IGS centers. Likewise, a reduced latency and more frequent updates of IGS ultra-rapid ephemerides are desirable to meet the requirements of upcoming satellite missions for near real-time and precise orbit determination.
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Acknowledgments
The present study makes use of GRACE GPS observations and reference orbits that have been made available by the Jet Propulsion Laboratory (JPL), Pasadena, on behalf of the GRACE project. GPS orbit and clock solutions have been obtained from the International GPS Service (IGS) and the Center for Orbit Determination in Europe (CODE). Selected samples of real-time generated GPS ephemerides have, furthermore, been provided by JPL for use in this analysis. The authors gratefully acknowledge these contributions.
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Montenbruck, O., Gill, E. & Kroes, R. Rapid orbit determination of LEO satellites using IGS clock and ephemeris products. GPS Solut 9, 226–235 (2005). https://doi.org/10.1007/s10291-005-0131-0
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DOI: https://doi.org/10.1007/s10291-005-0131-0