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The nucleation, growth and settling of crystals from a turbulently convecting fluid

Published online by Cambridge University Press:  26 April 2006

Richard A. Jarvis  and
Andrew W. Woods
Richard A. Jarvis
Affiliation:
Department of Geology and Geophysics, Yale University, New Haven, CT 06511, USA Present address: Laboratoire de Dynamique des Systèmes Géologiques, Institut de Physique du Globe, 4 place Jussieu, 75252 Paris Cedex 05, France
Andrew W. Woods
Affiliation:
Institute Theoretical Geophysics, Department of Applied Mathematics and Theoretical Physics, University of Cambridge, Silver Street, Cambridge CB3 9EW, UK
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Abstract

We present a new model to describe the thermal and compositional evolution of a binary alloy which is cooled from above. Explicit account is taken of the nucleation of crystals in the cold upper thermal boundary layer, the growth of crystals in the turbulently convecting interior, and their subsequent gravitational settling to the floor of the chamber. The crystallization of one solid phase only is considered. When the residence time of a typical crystal within the convecting bulk is short compared with the overall cooling time of the fluid, the crystal size distribution loses memory of earlier conditions in the fluid and the number density simply decays exponentially with the cube of the crystal size. A quasi-steady state exists in which the rate of crystal production is balanced by the rate of sedimentation at the floor, allowing the volume fraction of suspended crystals to remain small until convection ceases to be vigorous.

We focus on the situation in which the latent heat released by solidification would far exceed the heat flux extracted through convection if the melt undercooling were maintained equal to the initial temperature difference applied at the cold upper boundary. In this case, either the growth or nucleation of crystals must be limited in order that the fluid continues to cool. Both the growth-limited and nucleation-limited regimes may develop during the cooling of an individual fluid body, depending upon the thermal boundary condition at the upper boundary of the convecting portion of the fluid.

We calculate how the mean crystal size within the sedimented crystal pile evolves as the fluid cools. During the growth-limited regime, the mean crystal size in the crystal pile typically decreases with height, owing to the decrease in the extracted heat flux and the greater efficiency of crystal settling as the fluid layer becomes shallower. In contrast, during the nucleation-limited regime, the fluid undercooling may increase significantly as the fluid cools, and inverse grading (large crystals over small) is possible. We discuss the possible application of our theory to the cooling of large igneous intrusions.

Type
Research Article
Information
Journal of Fluid Mechanics , Volume 273 , 25 August 1994 , pp. 83 - 107
Copyright
© 1994 Cambridge University Press

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