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Reactive Rayleigh–Taylor turbulence

Published online by Cambridge University Press:  25 August 2009

M. CHERTKOV ,
V. LEBEDEV  and
N. VLADIMIROVA
M. CHERTKOV
Affiliation:
Theoretical Division and Center for Nonlinear Studies, Los Alamos National Laboratory, Los Alamos, NM 87545, USA
V. LEBEDEV
Affiliation:
Theoretical Division and Center for Nonlinear Studies, Los Alamos National Laboratory, Los Alamos, NM 87545, USA Landau Institute for Theoretical Physics, Russian Academy of Sciences, Chernogolovka, Russia
N. VLADIMIROVA*
Affiliation:
Theoretical Division and Center for Nonlinear Studies, Los Alamos National Laboratory, Los Alamos, NM 87545, USA Department of Mathematics and Statistics, University of New Mexico, Albuquerque, NM 87131, USA ASC Flash Center, University of Chicago, 5640 S Ellis Avenue, Chicago, IL 60637, USA
*
†Email address for correspondence: nata@flash.uchicago.edu
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Abstract

The Rayleigh–Taylor (RT) instability develops and leads to turbulence when a heavy fluid falls under the action of gravity through a light one. We consider a model in which the RT instability is accompanied by a reactive transformation between the fluids. We study the model using direct numerical simulations (DNSs), focusing on the effect of the reaction (flame) on the turbulent mixing. We discuss ‘slow’ reactions in which the characteristic reaction time exceeds the temporal scale of the RT instability, τ ≫ tinst. In the early turbulent stage, tinst ≲ t ≲ τ, effects of the flame are distributed over a maturing mixing zone, whose development is weakly influenced by the reaction. At t ≳ τ, the fully mixed zone transforms into a conglomerate of pure-fluid patches of sizes proportional to the mixing zone width. In this ‘stirred flame’ regime, temperature fluctuations are consumed by reactions in the regions separating the pure-fluid patches. This DNS-based qualitative description is followed by a phenomenology suggesting that thin turbulent flame is of a single-fractal character, and thus distribution of the temperature field is strongly intermittent.

Type
Papers
Information
Journal of Fluid Mechanics , Volume 633 , 25 August 2009 , pp. 1 - 16
Copyright
Copyright © Cambridge University Press 2009

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