The Spatio-Temporal Structure of Spiral-Defect Chaos
  We present a study of the recently discovered spatially-extended chaotic state known as spiral-defect chaos, which occurs in low-Prandtl-number, large-aspect-ratio Rayleigh-Benard convection. We employ the modulus squared of the space-time Fourier transform of time series of two-dimensional shadowgraph images to construct the structure factor ${S}({\vec k},\omega )$.   This analysis is used to characterize the average spatial and temporal scales of the chaotic state. We find that the correlation length and time can be described by power-law dependences on the reduced Rayleigh number ${\epsilon}$. These power laws have as yet no theoretical explanation. 
Stephen W. Morris (U. Toronto), Eberhard Bodenschatz (Cornell), David   S. Cannell and Guenter Ahlers (UCSB and CNLS)