S.M. Sadjadi, S. Chen, et al.
TAPIA 2009
A procedure is described for the numerical solution of the time-dependent equations governing the flow in a crystal-growth crucible. The molten crystal material is taken to be a Newtonian fluid with constant viscosity. The Boussinesq approximation is employed, i.e. compressibility is neglected except insofar as thermal expansion modifies the gravitational body force. Crucible rotation is the main driving force, but a series of numerical experiments suggests that buoyancy effects can modify appreciably the impurity-blending estimates obtained from an isothermal study. © 1977.
S.M. Sadjadi, S. Chen, et al.
TAPIA 2009
Yao Qi, Raja Das, et al.
ISSTA 2009
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Dianli Xitong Zidonghua/Automation of Electric Power Systems
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WOSP/SIPEW 2010