Kopsavilkums
We present a computational model of 3D turbulent melt convection in Czochralski Si-crystal growth systems, based on the hybridization of Reynolds-averaged approach and large eddy simulation. The effect of superimposed magnetic field action on the melt flow is introduced in the model to account for the suppression of turbulent melt fluctuations. The model has been verified using experimental data for temperature in the melt and along the melt-crucible surface. Effects of axial magnetic field on the change in melt convection are studied in an industrial configuration.
| Oriģinālvaloda | Angļu |
|---|---|
| Lapas (no-līdz) | 1757-1761 |
| Lapu skaits | 5 |
| Žurnāls | Journal of Crystal Growth |
| Sējums | 237-239 |
| Izdevuma numurs | 1-4 |
| DOIs | |
| Publikācijas statuss | Publicēts - apr. 2002 |
| Ārēji publicēts | Jā |
Nospiedums
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