Mechanisms of extensive spatiotemporal chaos in Rayleigh-Bernard convection

被引:124
作者
Egolf, DA [1 ]
Melnikov, IV
Pesch, W
Ecke, RE
机构
[1] Univ Calif Los Alamos Natl Lab, Ctr Nonlinear Studies, Div Theoret, Los Alamos, NM 87545 USA
[2] Univ Bayreuth, Inst Phys, D-95440 Bayreuth, Germany
关键词
D O I
10.1038/35008013
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
Spatially extended dynamical systems exhibit complex behaviour in both space and time-spatiotemporal chaos(1,2). Analysis of dynamical quantities (such as fractal dimensions and Lyapunov exponents(3)) 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(1,4,5). 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(6-8) (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(5,9) in Rayleigh-Benard convection, in which we rnd 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 rnd that the mechanism for the generation of chaotic disorder is spatially and temporally localized to events associated with the creation and annihilation of defects.
引用
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页码:733 / 736
页数:5
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