Spiral defect chaos in a model of Rayleigh-Benard convection
arXiv:patt-sol/9305004 · doi:10.1103/PhysRevLett.71.2030
Abstract
A numerical solution of a generalized Swift-Hohenberg equation in two dimensions reveals the existence of a spatio-temporal chaotic state comprised of a large number of rotating spirals. This state is observed for a reduced Rayleigh number . The power spectrum of the state is isotropic, and the spatial correlation function decays exponentially, with an estimated decay length , where is the critical wavelength near the onset of convection. Our study suggests that this spiral defect state occurs for low Prandtl numbers and large aspect ratios.
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References in corpus (4)
- Spiral Defect Chaos in Large Aspect Ratio Rayleigh-Benard Convection
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Cited by in corpus (20)
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- Lyapunov spectral analysis of a nonequilibrium Ising-like transition
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- Mean flow in hexagonal convection: stability and nonlinear dynamics
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- Grain boundary dynamics in stripe phases of non potential systems
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- Nature of Roll to Spiral-Defect-Chaos Transition
- Pattern Formation Near Onset of a Convecting Fluid In an Annulus
- Skew-Varicose Instability in Two Dimensional Generalized Swift-Hohenberg Equations
- Spiral Dynamics in Pattern-Forming Systems: Mean Flow Effects
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- Spiral defect chaos in Rayleigh-Bénard convection: Asymptotic and numerical studies of azimuthal flows induced by rotating spirals