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1
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5344276720
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C. Gebrogi, E. Ott, S. Pelikan and J. A. Yorke, Physica D 13, 261 (1984).
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(1984)
Physica D
, vol.13
, pp. 261
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Gebrogi, C.1
Ott, E.2
Pelikan, S.3
Yorke, J.A.4
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2
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0000435339
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A. Bondeson, E. Ott and T. M. Antonsen, Jr., , Phys. Rev. Lett. 55, 2103 (1985).
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(1985)
Phys. Rev. Lett.
, vol.55
, pp. 2103
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Bondeson, A.1
Ott, E.2
Antonsen, T.M.3
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4
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0000419939
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F. J. Romeiras, A. Bondeson, E. Ott, T. M. Antonsen, Jr., and C. Grebogi, Physica D 26, 277 (1987).
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(1987)
Physica D
, vol.26
, pp. 277
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Romeiras, F.J.1
Bondeson, A.2
Ott, E.3
Antonsen, T.M.4
Grebogi, C.5
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11
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0000374456
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W. L. Ditto, M. L. Spano, H. T. Savage, S. N. Rauseo, J. F. Heagy and E. Ott, Phys. Rev. Lett. 65, 533 (1990).
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(1990)
Phys. Rev. Lett.
, vol.65
, pp. 533
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Ditto, W.L.1
Spano, M.L.2
Savage, H.T.3
Rauseo, S.N.4
Heagy, J.F.5
Ott, E.6
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13
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85035202647
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The quasiperiodically forced pendulum has two nontrivial Lyapunov exponents LAMBDA and Λ prime that satisfy Λ prime = - ( p + Λ ), where p is the damping rate in Eq. (10). This can be seen by noting that Eq. (10) is actually a time-dependent flow of the form d φ / d t = v and d v / d t = - p ( v - cos φ ) + f (t). Taking the divergence of this flow, we obtain ( partial / partial v ) ( d v / d t ) + ( partial / partial φ ) ( d φ / d t ) = - p. Since this divergence is also the sum of the Lyapunov exponents, Eq. (13) holds. For large values of p, both LAMBDA and Λ prime are negative. The exponent Λ prime can be viewed as the exponential rate at which orbits in the three-dimensional phase space ( φ , v , z ) are attracted to the torus. For large p the rate is large, rendering the torus stable and difficult to destroy. As p decreases, - Λ prime becomes smaller. For p
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The quasiperiodically forced pendulum has two nontrivial Lyapunov exponents LAMBDA and Λ prime that satisfy Λ prime = - ( p + Λ ), where p is the damping rate in Eq. (10). This can be seen by noting that Eq. (10) is actually a time-dependent flow of the form d φ / d t = v and d v / d t = - p ( v - cos φ ) + f (t). Taking the divergence of this flow, we obtain ( partial / partial v ) ( d v / d t ) + ( partial / partial φ ) ( d φ / d t ) = - p. Since this divergence is also the sum of the Lyapunov exponents, Eq. (13) holds. For large values of p, both LAMBDA and Λ prime are negative. The exponent Λ prime can be viewed as the exponential rate at which orbits in the three-dimensional phase space ( φ , v , z ) are attracted to the torus. For large p the rate is large, rendering the torus stable and difficult to destroy. As p decreases, - Λ prime becomes smaller. For p
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23
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6144267833
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J. C. Sommerer, W. L. Ditto, C. Grebogi, E. Ott and M. L. Spano, Phys. Lett. A 153, 105 (1991).
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(1991)
Phys. Lett. A
, vol.153
, pp. 105
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Sommerer, J.C.1
Ditto, W.L.2
Grebogi, C.3
Ott, E.4
Spano, M.L.5
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24
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85035233220
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Transition to chaos characterized by a linearly passing through zero of the Lyapunov exponent has also been identified in random maps.
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Transition to chaos characterized by a linearly passing through zero of the Lyapunov exponent has also been identified in random maps.
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