Initial conditions for turbulent mixing simulations
In the context of the classical Rayleigh-Taylor hydrodynamical instability, we examine the much debated question of models for initial conditions and the possible influence of unrecorded long wave length contributions to the instability growth rate α.
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| Datum: | 2010 |
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| Hauptverfasser: | , , |
| Format: | Artikel |
| Sprache: | English |
| Veröffentlicht: |
Інститут фізики конденсованих систем НАН України
2010
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| Schriftenreihe: | Condensed Matter Physics |
| Online Zugang: | http://dspace.nbuv.gov.ua/handle/123456789/32125 |
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| Назва журналу: | Digital Library of Periodicals of National Academy of Sciences of Ukraine |
| Zitieren: | Initial conditions for turbulent mixing simulations / T. Kaman, J. Glimm, D.H. Sharp // Condensed Matter Physics. — 2010. — Т. 13, № 4. — С. 43401:1-7. — Бібліогр.: 15 назв. — англ. |