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New Observational Techniques and Precise Orbit Determination of Artificial Satellites

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Dynamics and Astrometry of Natural and Artificial Celestial Bodies
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Abstract

Modern observational techniques using ground-based and space-based instrumentation have enabled the measurement of the distance between the instrument and satellite to better than one centimeter. Such high precision instrumentation has fostered applications with centimeter-level requirements for satellite position knowledge. The determination of the satellite position to such accuracy requires a comparable modeling of the forces experienced by the satellite, especially when classical orbit determination methods are used. Geodetic satellites, such as Lageos, in conjunction with high precision ground-based laser ranging, have been used to improve for modeling of forces experienced by the satellite. Space-based techniques, such as Global Positioning System (GPS), offer alternatives, including kinematic techniques which require no modeling of the satellite forces, or only rudimentary models. This paper will describe the various techniques and illustrate the accuracies achieved with current satellites, such as TOPEX/POSEIDON, GPS/MET and the expectations for some future satellites.

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© 1997 Springer Science+Business Media Dordrecht

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Schutz, B.E. (1997). New Observational Techniques and Precise Orbit Determination of Artificial Satellites. In: Wytrzyszczak, I.M., Lieske, J.H., Feldman, R.A. (eds) Dynamics and Astrometry of Natural and Artificial Celestial Bodies. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-5534-2_9

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  • DOI: https://doi.org/10.1007/978-94-011-5534-2_9

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-6330-2

  • Online ISBN: 978-94-011-5534-2

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