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A simple model of high Prandtl and high Rayleigh number convection bounded by thin low-viscosity layers
F. H. Busse 1 , M. A. Richards 2 and A. Lenardic 3
  1 Institute of Physics, University of Bayreuth, D-95440 Bayreuth, Germany. E-mail: Friedrich.Busse@uni-bayreuth.de   2 Department Earth Planet. Science, University of California, Berkeley, CA 94720, USA   3 Department Earth Science, Rice University, Houston, Texas, USA
Copyright 2005 The Authors Journal compilation © 2005 RAS
KEYWORDS
low-viscosity layer • mantle convection

ABSTRACT

Motivated by recent numerical results on convection in the Earth's mantle in the presence of a low-viscosity zone, an analytical model is derived for 2-D steady convection with symmetric low-viscosity layers at the upper and lower boundaries. The asymptotic limits of high Rayleigh and high Prandtl number are assumed. The low- viscosity layers carry with minimal dissipation most of the horizontal component of the convection flow and thereby increase the efficiency of the convective heat transport. A Nusselt number (Nu)–Rayleigh number (R) relationship of the form  NuR1/3 (ℓ/δ)2/3  is obtained for an aspect ratio 2ℓ of the convection cell of order unity or less. Here δ denotes the fraction of the layer depth occupied by each of the low-viscosity channels. For large ℓ and  τ∼ℓ6δ−3 , where τ denotes the ratio between the viscosity of the interior and that of the thin low-viscosity layers, Nu reaches a maximum value of the order  (Rτ2/3)1/3  at  ℓ= (τδ3/9)1/6π/2 . This result suggests that the aspect ratio of convection increases with viscosity contrast.


Accepted 2005 October 7. Received 2005 September 30; in original form 2004 June 18

DIGITAL OBJECT IDENTIFIER (DOI)
10.1111/j.1365-246X.2005.02836.x About DOI

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