Abstract
In order to reduce the error propagation in the numerical calculation of orbits two methods of stabilization of the differential equations of the perturbed Keplerian motion are offered: (1) a nonconservative method by asymptotical stabilization of the energy relation, (2) a conservative method by manipulation of the Hamiltonian. In both methods the stabilization is combined with the introduction of a new independent variable in order to achieve an analytic step size adaption.
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References
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© 1976 D. Reidel Publishing Company, Dordrecht-Holland
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Baumgarte, J. (1976). Stabilization, Manipulation and Analytic Step Adaption. In: Szebehely, V., Tapley, B.D. (eds) Long-Time Predictions in Dynamics. NATO Advanced Study Institutes Series, vol 26. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-1493-9_11
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DOI: https://doi.org/10.1007/978-94-010-1493-9_11
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