Fourier analysis of local Lyapunov characteristic exponents for satellite-type motions

Details Fourier analysis of local Lyapunov characteristic exponents for satellite-type motions Fourier analysis of local Lyapunov characteristic exponents for satellite-type motions

Oct 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993cemda..57..369l&link_type=abstract

Celestial Mechanics and Dynamical Astronomy (ISSN 0923-2958), vol. 57, no. 1-2, p. 369-372

Astronomy and Astrophysics

Astronomy

2

Binary Stars, Fourier Analysis, Liapunov Functions, Orbit Calculation, Stellar Models, Stellar Orbits, Stochastic Processes, Three Body Problem, Chaos, Mathematical Models

Scientific paper

For a binary star system with equal masses the transition from regular to stochastic motion has been determined by means of the Lyapunov Characteristic Numbers (LCN) in a paper of Gonczi and Froeschle (1981), where the initial distance of the massless body to the second primary was used as parameter of integration. This time we analyse the Fourier spectra of the local LCNs (alphaik of this system for different intervals of time.

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