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Abstrakty
In the this paper our results on the natural convection in an enclosed rotating cavity are presented. We have focused our attention on the influence of the Rayleigh and Taylor numbers on the flow structure. DNS computations have been performed for the geometry of aspect ratio L=9 and curvature parameter Rm=1.5.
Słowa kluczowe
Wydawca
Rocznik
Tom
Strony
267--272
Opis fizyczny
Bibliogr. 14 poz., rys.
Twórcy
autor
autor
- Poznan University of Technology, Chair of Thermal Engineering, Piotrowo 3, 60-965 Poznan, Poland, ojciech.majchrowski@doctorate.put.poznan.pl
Bibliografia
- [1] Rossby H T 1969 J. Fluid Mech. 36 309
- [2] Siggia E D 1994 Annu. Rev. Fluid Mech. 26 137
- [3] Chandrasekhar S 1953 Proc. R. Soc. Lond. A217 306
- [4] Chandrasekhar S 1961 Hydrodynamic and Hydromagnetic Stability, Oxford University Press
- [5] Nagakawa Y and Frenzen P 1955 Tellus 7 1
- [6] Boubnov B M and Golistyn G S 1986 J. Fluid Mech. 167 503
- [7] Zhong F, Ecke R and Steinberg V 1993 J. Fluid Mech. 249 135
- [8] Kunnen R P J, Geurts B J and Clercx H J H 2006 Direct Numerical Simulation of Turbulent Rotating Rayleigh-Benard Convection, Direct Large-Eddy Simulation VI
- [9] Serre E and Pulicani J P 2001 Computers and Fluids 30 491
- [10] Tuliszka-Sznitko E and Zieliński A 2006 J. Theor. Appl. Mech. 44 (3) 405
- [11] Fernando H J S, Chen R-R and Boyer D L 1991 J. Fluid Mech. 228 513
- [12] Julien K, Legg S, McWilliams J and Werne J 1996 J. Fluid Mech. 322 243
- [13] Vorobieff P and Ecke R E 2002 J. Fluid Mech. 458 191
- [14] Zhao A X, Moates F C and Narayanan R 1995 Phys. Fluids 7 1576
Typ dokumentu
Bibliografia
Identyfikator YADDA
bwmeta1.element.baztech-article-BPG8-0009-0027