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Some features of the thermally concentrated convective motion of a hardening binary melt and the impurity distribution

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Abstract

Some features of the thermally concentrated convective motion of a binary melt, hardening in a closed rectangular region with movable boundaries, and the impurity distribution are investigated numerically.

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Abbreviations

x0 :

characteristic dimension

xi (i=1, 2):

a dimensional coordinate

li (i=1, 2):

height and width of the crystallizer cavity

ri, ei (i=1, 2):

dimensional coordinates of the phase transition in the Ox1x2 coordinate system

T, T0, and TK :

current temperature, initial temperature, and melt crystallization temperature

ρ :

density of the melt

P, Pmax, and Pmin :

current pressure, maximum pressure, and minimum pressure in the system

c, c0 :

current and initial impurity concentration

e2 :

unit vector having the same direction as the direction as the force of gravity

¯g:

acceleration due to gravity

β :

coefficient of thermal expansion

γ :

diffusion broadening coefficient

¯u:

velocity of convective motion

ν :

kinematic viscosity

k:

equilibrium impurity distribution coefficient

t:

current time

D:

diffusion coefficient

a :

thermal diffusivity

ΔT=t0-tK :

initial overheating of the melt

η i=Xi/x0 (i=1, 2):

dimensionless coordinate

ι i=L1/x0 (i=1, 2):

relative height and width of the crystallizer cavity in the coordinate system Oη 1 η 2

Ri=ri/x0, εii/x0 :

dimensionless coordinates of the phase-transition boundary in the Oν 1 η 2 coordinate system

Ū=ū/u0 :

dimensionless velocity of convective motion

Gr=¦¯g¦βΔTx 30 /ν 2 :

Grashof hydrodynamic number

GrD=¦¯g¦γc0X 30 2 :

Grashof diffusion number

Fo=Dt x 20 ):

dimensionless time, Sm=ν/D, Schmidt number

Lu=D/a:

Lewis number

Literature cited

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Translated from Inzhenerno-Fizicheskii Zhurnal, Vol. 39, No. 1, pp. 118–125, July, 1980.

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Zavgorodnii, P.F. Some features of the thermally concentrated convective motion of a hardening binary melt and the impurity distribution. Journal of Engineering Physics 39, 797–803 (1980). https://doi.org/10.1007/BF00821839

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  • DOI: https://doi.org/10.1007/BF00821839

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