Detection of ordered and chaotic motion using the dynamical spectra

Citation
N. Voglis et al., Detection of ordered and chaotic motion using the dynamical spectra, CEL MEC DYN, 73(1-4), 1999, pp. 211-220
Citations number
21
Categorie Soggetti
Space Sciences
Journal title
CELESTIAL MECHANICS & DYNAMICAL ASTRONOMY
ISSN journal
09232958 → ACNP
Volume
73
Issue
1-4
Year of publication
1999
Pages
211 - 220
Database
ISI
SICI code
0923-2958(1999)73:1-4<211:DOOACM>2.0.ZU;2-9
Abstract
Two simple and efficient numerical methods to explore the phase space struc ture are presented, based on the properties of the "dynamical spectra". 1) We calculate a "spectral distance" D of the dynamical spectra for two diffe rent initial deviation vectors. D --> 0 in the case of chaotic orbits, whil e D --> const not equal 0 in the case of ordered orbits. This method is by orders of magnitude faster than the method of the Lyapunov Characteristic N umber (LCN). 2) We define a sensitive indicator called ROTOR (ROtational TO ri Recongnizer) for 2D maps. The ROTOR remains zero in time on a rotational torus, while it tends to infinity at a rate proportional to N = number of iterations, in any case other than a rotational torus. We use this method t o locate the last KAM torus of an island of stability, as well as the most important cantori causing stickiness near it.