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A Pegasus computer programme for the improvement of the orbital parameters of an earth-satellite

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Book cover Dynamics of Satellites / Dynamique des Satellites

Part of the book series: IUTAM Symposia ((IUTAM))

Abstract

The dynamic model adopted for the motion of a satellite includes the first order short–period and secular perturbations of the orbital elements due to earth’s oblateness and other perturbations of the elements are represented by polynomials in time up to the third degree.

The values of the six basic elements at a given time, together with such polynomial coefficients as are required, are determined from a set of observations by a differential correction technique. In this procedure the observation times and angles are weighted according to a priori estimates of their accuracy. In addition to the estimates of the orbital parameters, estimates of their variances and covariances are also determined.

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References

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Maurice Roy

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© 1963 Springer-Verlag Berlin Heidelberg

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Merson, R.H. (1963). A Pegasus computer programme for the improvement of the orbital parameters of an earth-satellite. In: Roy, M. (eds) Dynamics of Satellites / Dynamique des Satellites. IUTAM Symposia. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-48130-7_9

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  • DOI: https://doi.org/10.1007/978-3-642-48130-7_9

  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-642-48132-1

  • Online ISBN: 978-3-642-48130-7

  • eBook Packages: Springer Book Archive

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