Abstract
Experimental and numerical observations of oscillatory instability of melt flow in a Czochralski model are compared, and a disagreement observed at small crystal dummy rotation rates is addressed. To exclude uncertainties connected with flow along the free surface, the latter is covered by a no-slip thermally insulating ring. Experiments reveal an appearance of oscillations at temperature differences smaller than the numerically predicted critical ones. At the same time, a steep increase of the oscillations amplitude is observed just beyond the computed threshold values. By increasing thedummy rotation gradually, we are able to qualitatively confirm the numerically predicted flow destabilization. A good quantitative comparison is reached only with a rather strong rotation of the crystal dummy. Focusing on thedisagreement in the non-rotating case, we argue that the experimentally observed instability is triggered by an external excitation that results from low-amplitude temperature oscillations in thermostatic baths. This argumentis supported by a numerical simulation of the parametrically excited model.
Original language | English |
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Pages (from-to) | 209-234 |
Number of pages | 26 |
Journal | Fluid Dynamics and Materials Processing |
Volume | 9 |
Issue number | 3 |
DOIs | |
State | Published - 2013 |
Keywords
- Convection
- Czochralski growth
- Oscillatory instability
- Rotating flows