Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
10695042 | Advances in Space Research | 2005 | 7 Pages |
Abstract
Bénard-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.
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Space and Planetary Science
Authors
Thomas Boeck,