Convective Instability of a Mushy Layer - I: Uniform Permeability

Details Convective Instability of a Mushy Layer - I: Uniform Permeability Convective Instability of a Mushy Layer - I: Uniform Permeability

Feb 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003gapfd..97...97r&link_type=abstract

Geophysical and Astrophysical Fluid Dynamics, vol. 97, Issue 2, p.97-134

Physics

Fluid Dynamics

2

Scientific paper

Mushy layers arise and are significant in a number of geophysical contexts, including freezing of sea ice, solidification of magma chambers and inner-core solidification. A mushy layer is a region of solid and liquid in phase equilibrium which commonly forms between the liquid and solid regions of a solidifying system composed of two or more constituents. We consider the convective instability of a plane mushy layer which advances steadily upwards as heat is withdrawn at a uniform rate from the bottom of a eutectic binary alloy. The solid which forms is assumed to be composed entirely of the denser constituent, making the residual liquid within the mush compositionally buoyant and thus prone to convective motion. In this article we focus on the large-scale mush mode of instability, arguing that the 'boundary-layer' mode is not amenable to the standard stability analysis, because convective motions occur on that scale for any non-zero value of the Rayleigh number. We quantify the minimum critical Rayleigh number and determine the structure of the convective modes of motion within the mush and the associated deflections of the mush-melt and mush-solid boundaries. This study of convective perturbations differs from previous analyses in two ways; the inhibition of motion and deformation of the mush-melt interface by the stable stratification of the overlying melt is properly quantified and deformation of the mush-solid interface is permitted and quantified. We find that the mush-melt interface is almost unaffected by convection while significant deformation of the mush-solid interface occurs. We show that each of these effects causes significant (unit-order) changes in the predicted critical Rayleigh number. The marginal modes depend on three dimensionless parameters: a scaled eutectic temperature, e (which characterizes the eutectic temperature relative to the depression of the liquidus), a scaled superheat, (which measures the amount by which the temperature of the incoming melt exceeds the liquidus temperature) and the Stefan number, S (which measures the latent heat of crystallization). To survey parameter space, we focus on seven cases, a standard case having S = = = 1, and six others in which one of the parameters is either large or small compared with unity: a nearly pure case (e = 100; having little of the light constituent), the large superheat limit (&), a case of large latent heat (S = 100), the near eutectic limit (e 0), a case of small superheat ( = 0.01) and the case of zero latent heat (S = 0). The critical Rayleigh number and the associated wavelength of the convection pattern are determined in each case. The eigenvector for each case is presented in terms of the streamlines and the isolines of the perturbation temperature and solid fraction.

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