Front propagation in a chaotic flow field

C. O. Mehrvarzi and M. R. Paul
Phys. Rev. E 90, 012905 – Published 21 July 2014

Abstract

We investigate numerically the dynamics of a propagating front in the presence of a spatiotemporally chaotic flow field. The flow field is the three-dimensional time-dependent state of spiral defect chaos generated by Rayleigh-Bénard convection in a spatially extended domain. Using large-scale parallel numerical simulations, we simultaneously solve the Boussinesq equations and a reaction-advection-diffusion equation with a Fischer-Kolmogorov-Petrovskii-Piskunov reaction for the transport of the scalar species in a large-aspect-ratio cylindrical domain for experimentally accessible conditions. We explore the front dynamics and geometry in the low-Damköhler-number regime, where the effect of the flow field is significant. Our results show that the chaotic flow field enhances the front propagation when compared with a purely cellular flow field. We quantify this enhancement by computing the spreading rate of the reaction products for a range of parameters. We use our results to quantify the complexity of the three-dimensional front geometry for a range of chaotic flow conditions.

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  • Received 4 April 2014

DOI:https://doi.org/10.1103/PhysRevE.90.012905

©2014 American Physical Society

Authors & Affiliations

C. O. Mehrvarzi and M. R. Paul*

  • Department of Mechanical Engineering, Virginia Polytechnic Institute and State University, Blacksburg, Virginia 24061, USA

  • *Corresponding author: mrp@vt.edu

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Vol. 90, Iss. 1 — July 2014

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