Abstract
This paper presents a transient model for tfopant segregation during semiconductor crystal growth in space With a steady transverse residual acceleration and with a steady magnetic field. Crystals are being gttnvn in the presence of magnetic fields in space in an attempt to eliminate buoyant convection. Unfortunately, magnetically damped buoyant convection created by a residual acceleration in space is large enough to drive convectivc mass transport, which produces non-Uniformities in the concentration in both the melt and the crystal.
| Original language | English |
|---|---|
| Pages (from-to) | 234-239 |
| Number of pages | 6 |
| Journal | Magnetohydrodynamics |
| Volume | 36 |
| Issue number | 3 |
| DOIs | |
| State | Published - 2000 |
| Externally published | Yes |
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