Spiral defect chaos in a model of Rayleigh-Benard convection

Nonlinear Sciences – Pattern Formation and Solitons

Scientific paper

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LaTeX. 4 PostScript figures. Appended

Scientific paper

10.1103/PhysRevLett.71.2030

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 $\epsilon=0.25$. The power spectrum of the state is isotropic, and the spatial correlation function decays exponentially, with an estimated decay length $\xi \approx 2.5 \lambda_{c}$, where $\lambda_{c}$ 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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