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Oscillatory convection and chaos in a Lorenz-type model of a rotating fluid

Journal Article · · Journal of Statistical Physics; (USA)
DOI:https://doi.org/10.1007/BF01016782· OSTI ID:6196356
 [1]
  1. Univ. of Manchester (England)

A four-mode model of convection in a rotating fluid layer is studied. The model is an extension of the Lorenz model of Rayleigh-Benard convection, the extra mode accounting for the regeneration of vorticity by rotation. Perturbation theory is applied to show that the Hopf bifurcations from conductive and steady convective solutions can be either supercritical or subcritical. Perturbation theory is also used at large Rayleigh numbers r to predict novel behavior. Supercritical oscillatory convection of finite amplitude is found by numerical integration of the governing equations. The general picture is of a series of oscillatory solutions stable over large r intervals, interspersed by short bursts of chaos.

OSTI ID:
6196356
Journal Information:
Journal of Statistical Physics; (USA), Journal Name: Journal of Statistical Physics; (USA) Vol. 56:5-6; ISSN 0022-4715; ISSN JSTPB
Country of Publication:
United States
Language:
English