1990
DOI: 10.1088/0951-7715/3/1/008
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A low-order model of the shear instability of convection: chaos and the effect of noise

Abstract: We consider a third-order system of ordinary differential equations aimed at modelling the shear instability of tall thin cells as found, for example, in thermohaline convection. The nonlinear interactions between the zeroth and first harmonics of the convective cells (A and B) fuel the growth of a horizontal shear (C) which, in turn, becomes of sufficient magnitude to destabilise the convective motions. The most interesting feature of the model is that in certain parameter regimes a small amount of random noi… Show more

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Cited by 42 publications
(43 citation statements)
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“…Note that the system we consider serves only as a prototype of this behavior and it is not derived from the convection problem. On the other hand, a 3D model with similar behavior was systematically derived for a homogeneous thermohaline convection problem directly from the partial differential equations [10]. Here we aim to capture the central qualitative features in a two dimensional model.…”
Section: Introductionmentioning
confidence: 99%
“…Note that the system we consider serves only as a prototype of this behavior and it is not derived from the convection problem. On the other hand, a 3D model with similar behavior was systematically derived for a homogeneous thermohaline convection problem directly from the partial differential equations [10]. Here we aim to capture the central qualitative features in a two dimensional model.…”
Section: Introductionmentioning
confidence: 99%
“…The phenomenon has been reported in a one-dimensional map [5], in repeated passage through a saddle-node bifurcation [13], and in ordinary differential equations describing the resonant interaction of wave modes [6,10], the intermittent destabilization of convection by shear [7,11], pulsating laser oscillations [9] and plane Poiseuille flow [14]. Numerical evidence for similar behavior has been found in a set of partial differential equations describing the shear instability of thermohaline convection [8].…”
Section: Introductionmentioning
confidence: 69%
“…Successive maxima are independent, depending only the realization of the noise in the slow phase leading up to it. This is the key to the simplification of the dynamics produced by noise [6,7,10,11]. We shall calculate the density of maxima of |a a a t (0)| as follows.…”
Section: Calculation Of Density Of Maximamentioning
confidence: 99%
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