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2
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85036220223
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See, e.g., D.N. Subarev, Statistische Thermodynamik des Nichtgleichgewichts (Akademie-Verlag, Berlin, 1976), and references therein
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See, e.g., D.N. Subarev, Statistische Thermodynamik des Nichtgleichgewichts (Akademie-Verlag, Berlin, 1976), and references therein.
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J. Guckenheimer and P. Holmes, Nonlinear Oscillations, Dynamical Systems, and Bifurcation of Vector Fields, Applied Mathematical Sciences Vol. 42 (Springer, New York, 1983).
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R. Abraham and J.E. Marsden, Foundations of Mechanics (Benjamin, Reading, MA, 1978).
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85036271420
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C. Sparrow, The Lorenz Equations (Springer, New York, 1982)
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C. Sparrow, The Lorenz Equations (Springer, New York, 1982).
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W. Breymann and H. Thomas, in From Phase Transitions to Chaos, edited by G. Györgyi, I. Kondor, L. Sasvary, and T. Tel (World Scientific, Singapore, 1992)
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W. Breymann and H. Thomas, in From Phase Transitions to Chaos, edited by G. Györgyi, I. Kondor, L. Sasvary, and T. Tel (World Scientific, Singapore, 1992).
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R. Kubo, M. Toda, and N. Hashitsume, Statistical Physics II (Springer, Berlin, 1985), pp. 196–199.
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31
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85036158716
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Similar results as those presented here have also been obtained for (Formula presented), where the Lorenz system is also chaotic
-
Similar results as those presented here have also been obtained for (Formula presented), where the Lorenz system is also chaotic.
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32
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85036255444
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All integrations of the Lorenz system were done with a fourth order Runge-Kutta integration scheme with time step (Formula presented)
-
All integrations of the Lorenz system were done with a fourth order Runge-Kutta integration scheme with time step (Formula presented).
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33
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85036336604
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For frequencies around (Formula presented) very long integration times T (up to (Formula presented) are needed to see the beginning of the plateau. The reason for this is that in this range of “internal frequencies” the chaotic background (Formula presented) is very large so that the first term in Eq. (2.10) gives considerable contributions for smaller T
-
For frequencies around (Formula presented) very long integration times T (up to (Formula presented) are needed to see the beginning of the plateau. The reason for this is that in this range of “internal frequencies” the chaotic background (Formula presented) is very large so that the first term in Eq. (2.10) gives considerable contributions for smaller T.
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34
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85036401297
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Why for small values of (Formula presented) the phase (Formula presented) seems to lock to (Formula presented) or (Formula presented) has not further been analyzed; for the present purpose only the stabilization at sufficiently large (Formula presented) is of interest
-
Why for small values of (Formula presented) the phase (Formula presented) seems to lock to (Formula presented) or (Formula presented) has not further been analyzed; for the present purpose only the stabilization at sufficiently large (Formula presented) is of interest.
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37
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0025554311
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M.Y. Li, Tin Win, C.O. Weiss, and N.R. Heckenberg, Opt. Commun. 80, 119 (1990), and references therein.
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(1990)
Opt. Commun.
, vol.80
, pp. 119
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Li, M.Y.1
Win, T.2
Weiss, C.O.3
Heckenberg, N.R.4
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