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Spatiotemporal chaos in Rayleigh-Benard convection

Citation

Chiam, Keng-Hwee (2004) Spatiotemporal chaos in Rayleigh-Benard convection. Dissertation (Ph.D.), California Institute of Technology. http://resolver.caltech.edu/CaltechETD:etd-08062003-162208

Abstract

Spatiotemporal chaos, or disorder in both the space and time coordinates, is studied in direct numerical simulations of Rayleigh-B?rd convection. In particular, the following investigations pertaining to spiral defect chaos are discussed.

First, in the absence of the mean flow, spiral defect chaos is found to collapse to a stationary pattern comprising textures of stripes with angular bends. The quenched patterns are characterized by mean wave numbers that approach those uniquely selected by focus-type singularities, which, in the absence of the mean flow, lie at the zig zag instability boundary. In addition, mean flow is shown to contribute to the phenomenon of rolls terminating perpendicularly into lateral walls. In the absence of the mean flow, rolls begin to terminate into lateral walls at an oblique angle. This obliqueness increases with the Rayleigh number.

Second, the transport of passive tracers in the presence of advection by spiral defect chaos is found to be characterized by normal diffusion. The enhancement in the tracer diffusivity follows two regimes. When the molecular diffusivity of the tracer concentration is small, the enhancement is proportional to the P?et number. When the molecular diffusivity is large, the enhancement is proportional to the square root of the P?et number. This difference is explained in terms of the dependence of the transport on the local wave numbers. It is found that tracer concentrations with small molecular diffusivity experience enhanced longitudinal diffusion and suppressed lateral diffusion at regions of the flow occupied by defects.

Third, perturbations in spiral defect chaos are found to propagate in a localized manner. In particular, they nucleate around the defect structures in the flow. In addition, an oscillatory instability at the spiral core is discovered. Finally, the propagation in pre-chaotic stripe textures is explained in terms of the diffusion of the phase variable of the stripe state.

Item Type:Thesis (Dissertation (Ph.D.))
Subject Keywords:nonlinear dynamics; Rayleigh-B?rd convection; spatiotemporal chaos; statistical physics
Degree Grantor:California Institute of Technology
Division:Physics, Mathematics and Astronomy
Major Option:Physics
Thesis Availability:Public (worldwide access)
Research Advisor(s):
  • Cross, Michael Clifford
Thesis Committee:
  • Cross, Michael Clifford (chair)
  • Meiron, Daniel I.
  • Libbrecht, Kenneth George
  • Leonard, Anthony
Defense Date:1 August 2003
Author Email:ChiamKH (AT) MailAPS.ORG
Record Number:CaltechETD:etd-08062003-162208
Persistent URL:http://resolver.caltech.edu/CaltechETD:etd-08062003-162208
Default Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:3020
Collection:CaltechTHESIS
Deposited By: Imported from ETD-db
Deposited On:15 Aug 2003
Last Modified:26 Dec 2012 02:56

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