AbstractBénard–Marangoni convection at large Marangoni and low Prandtl numbers can be efficiently simulated using spectral numerical methods. Previous two-dimensional simulations indicate power-law scaling over a significant range of Marangoni numbers for both laminar and turbulent convection. We summarize these numerical results and describe corresponding phenomenological models. New three-dimensional simulations support the scaling results obtained in the turbulent two-dimensional case.
Bénard–Marangoni convection at large Marangoni numbers: Results of numerical simulations
Advances in Space Research ; 36 , 1 ; 4-10
2005-02-26
7 pages
Article (Journal)
Electronic Resource
English
Bénard#8211Marangoni convection at large Marangoni numbers: Results of numerical simulations
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