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Symplectic mappings

Published online by Cambridge University Press:  25 May 2016

John D. Hadjidemetriou
John D. Hadjidemetriou*
Affiliation:
University of Thessaloniki, Department of Physics GR-540 06 Thessaloniki, Greece e-mail: hadjidem@olymp.ccf.auth.gr

Abstract

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This paper reviews the main methods for constructing mapping models for Hamiltonian systems, for the study of motion in the Solar System. The emphasis is given to the relation between the various mapping techniques, the methods to check how close is a mapping model to the original system and the effects of an incomplete model on the evolution of the system.

Information

Type
Part VII - The Calculus of Perturbations
Information
Symposium - International Astronomical Union , Volume 172: Dynamics, Ephemerides and Astrometry of the Solar System , 1996, pp. 255 - 266
Copyright
Copyright © Kluwer 1996 

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