1994
DOI: 10.1016/0022-0248(94)90969-5
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Experimental observation and numerical simulation of wave patterns in a Czochralski silicon melt

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Cited by 60 publications
(27 citation statements)
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“…Contrarily, Seidl et al [20] observed that the azimuthal m-folded (m=2, 3, 4, … ) waves propagated in a direction opposite to the crucible at higher crucible rotation rates, both by experiments and numerical simulations. With the higher crucible rotation rate, the wave number is larger and the phase velocity of the wave is faster, but always lower than the crucible rotation rate [21].…”
Section: Introductionmentioning
confidence: 96%
“…Contrarily, Seidl et al [20] observed that the azimuthal m-folded (m=2, 3, 4, … ) waves propagated in a direction opposite to the crucible at higher crucible rotation rates, both by experiments and numerical simulations. With the higher crucible rotation rate, the wave number is larger and the phase velocity of the wave is faster, but always lower than the crucible rotation rate [21].…”
Section: Introductionmentioning
confidence: 96%
“…Ristorcelli et al [9] summarized many possible flow instabilities in the melt of the Czochralski cystal growing system. Among the instabilities, researchers thought that the rotating RayleighBenard instability [10] or the baroclinic [11] instability might be the origin of the asymmetric profile.…”
Section: Results Of the Calcula~ons And Discussionmentioning
confidence: 99%
“…[45] Die periodischen Oszillationen werden durch konvektive Instabilitäten bewirkt, [49] wenn in rotierenden Flüssigkeiten dominante, vertikale Temperaturgradienten auftreten. [50] Schaltet man das Cusp-Magnetfeld aus (Ha = 0), so verlieren die Oszillationen im beschriebenen Modell ihre Periodizität. Bei Z (Abbildung 11, oben) liegt Ein Cusp-Magnetfeld wirkt sich auch sehr güns-tig auf die Temperaturverteilung in der Siliciumschmelze und an der Grenzfläche zum CZ-Siliciumeinkristall aus.…”
Section: Numerische Simulation Des Kristallziehensunclassified