Computer Science
Scientific paper
Apr 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003eaeja....14246p&link_type=abstract
EGS - AGU - EUG Joint Assembly, Abstracts from the meeting held in Nice, France, 6 - 11 April 2003, abstract #14246
Computer Science
Scientific paper
In this work for the first time we test the chaos hypothesis for the dynamics of the inner magnetosphere of Jupiter as this dynamics is appeared in energetic populations. For this we study geometrical and dynamical characteristics of Jovian energetic ion time series in the reconstructed phase space by using the SVD extended chaotic analysis. The null hypothesis is applied for the SVD reconstructed signals reveals a strong stochastic and high dimensional external component, as well as an internal low dimensional, nonlinear and chaotic deterministic component. The results of this study indicate the existence of a low dimensional strange attractor underlying the Jovian magnetospheric dynamics which produces the observed quasiperiodic phenomena.
Anagnostopoulos G. C.
Athanasiu M. A.
Pavlos G. P.
Sarris Emmanuel T.
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