Abstract
The range of existence and the properties of two essentially different chaotic attractors found in a model of nonlinear convection-driven dynamos in rotating spherical shells are investigated. A hysteretic transition between these attractors is established as a function of the rotation parameter t. The width of the basins of attraction is also estimated.
Original language | English |
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Article number | 018409 |
Journal | Physica Scripta |
Volume | 86 |
Issue number | 1 |
DOIs | |
Publication status | Published - Jul 2012 |