Type of trajectory instability for a movable disk model of the lithosphere

Details Type of trajectory instability for a movable disk model of the lithosphere Type of trajectory instability for a movable disk model of the lithosphere

Mar 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999pepi..111..305p&link_type=abstract

Physics of the Earth and Planetary Interiors, Volume 111, Issue 3-4, p. 305-315.

Physics

1

Scientific paper

A toy model of seismicity, based on a system of movable interacting disks, was used to evaluate the velocity of chaotization process in coordinate phase space. This paper pursues two major goals: to demonstrate that the model reproduces some important features of seismicity in terms of similarity of energy dissipation processes in the model and in the lithosphere; and to show that the simple measure of trajectory separation increases with time, not as a standard Lyapunov exponent, but rather obeying the power law, resulting in a `weak chaos' situation.

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