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 |
|---|---|
| Article number | 018409 |
| Journal | Physica Scripta |
| Volume | 86 |
| Issue number | 1 |
| DOIs | |
| Publication status | Published - Jul 2012 |
Bibliographical note
© 2012 The Royal Swedish Academy of SciencesFingerprint
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