Mechanisms of extensive spatiotemporal chaos in Rayleigh–Bénard convection

Spatially extended dynamical systems exhibit complex behaviour in both space and time—spatiotemporal chaos. Analysis of dynamical quantities (such as fractal dimensions and Lyapunov exponents) has provided insights into low-dimensional systems; but it has proven more difficult to understand spatiotemporal chaos in high-dimensional systems, despite abundant data describing its statistical properties. Initial attempts have been made to extend the dynamical approach to higher-dimensional systems, demonstrating numerically that the spatiotemporal chaos in several simple models is extensive (the number of dynamical degrees of freedom scales with the system volume). Here we report a computational investigation of a phenomenon found in nature, ‘spiral defect’ chaos in Rayleigh–Bénard convection, in which we find that the spatiotemporal chaos in this state is extensive and characterized by about a hundred dynamical degrees of freedom. By studying the detailed space–time evolution of the dynamical degrees of freedom, we find that the mechanism for the generation of chaotic disorder is spatially and temporally localized to events associated with the creation and annihilation of defects.

[1]  The spatio-temporal structure of spiral-defect chaos , 1996, chao-dyn/9604013.

[2]  Eberhard Bodenschatz,et al.  Recent Developments in Rayleigh-Bénard Convection , 2000 .

[3]  Eberhard Bodenschatz,et al.  Importance of Local Pattern Properties in Spiral Defect Chaos , 1998 .

[4]  J. Gollub,et al.  Order and disorder in fluid motion. , 1995, Proceedings of the National Academy of Sciences of the United States of America.

[5]  R. M. Clever,et al.  Instabilities of convection rolls in a fluid of moderate Prandtl number , 1979, Journal of Fluid Mechanics.

[6]  Department of Physics,et al.  Extensive scaling and nonuniformity of the Karhunen-Loève decomposition for the spiral-defect chaos state , 1998, chao-dyn/9808006.

[7]  Morris,et al.  Spiral defect chaos in large aspect ratio Rayleigh-Bénard convection. , 1993, Physical review letters.

[8]  J. Davies,et al.  Dust outflows from starburst galaxies , 1999 .

[9]  Lyapunov Analysis of Spatiotemporal Intermittency , 1993 .

[10]  G. Ahlers,et al.  Apparatus for the study of Rayleigh–Bénard convection in gases under pressure , 1996 .

[11]  D. Ruelle Large volume limit of the distribution of characteristic exponents in turbulence , 1982 .

[12]  Ronnie Mainieri,et al.  Excitation of Spirals and Chiral Symmetry Breaking in Rayleigh-B�nard Convection , 1995, Science.

[13]  Cross,et al.  Defect dynamics for spiral chaos in Rayleigh-Bénard convection. , 1995, Physical review letters.

[14]  Henry S. Greenside,et al.  Relation between fractal dimension and spatial correlation length for extensive chaos , 1994, Nature.

[15]  David A. Egolf Dynamical Dimension of Defects in Spatiotemporal Chaos , 1998 .

[16]  M. Cross,et al.  Pattern formation outside of equilibrium , 1993 .

[17]  Victor Steinberg,et al.  Transition between spiral and target states in Rayleigh–Bénard convection , 1994, Nature.

[18]  Mark Dragovan,et al.  The Shapes and Alignment Properties of Interstellar Dust Grains , 1995 .

[19]  D. Ruelle,et al.  Ergodic theory of chaos and strange attractors , 1985 .

[20]  D. Sokoloff,et al.  Galactic Magnetism: Recent developments and perspectives , 1996 .

[21]  Weber,et al.  Spiral defect chaos in Rayleigh-Bénard convection. , 1994, Physical Review Letters.