Identification of the Structures for Low Reynolds Number Flow in the Strong Magnetic Field
Autor: | Elzbieta Fornalik-Wajs, Łukasz Pleskacz |
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Rok vydání: | 2019 |
Předmět: |
Graetz–Brinkman problem
020209 energy Prandtl number magnetic field computational fluid dynamics 02 engineering and technology lcsh:Thermodynamics Computational fluid dynamics Physics::Fluid Dynamics symbols.namesake flow structure 020401 chemical engineering lcsh:QC310.15-319 0202 electrical engineering electronic engineering information engineering Astrophysics::Solar and Stellar Astrophysics 0204 chemical engineering Physics::Atmospheric and Oceanic Physics forced convection lcsh:QC120-168.85 Fluid Flow and Transfer Processes Physics business.industry Mechanical Engineering Reynolds number Mechanics Thermomagnetic convection Solver Condensed Matter Physics Forced convection Magnetic field Flow (mathematics) symbols lcsh:Descriptive and experimental mechanics business |
Zdroj: | Fluids, Vol 4, Iss 1, p 36 (2019) Fluids Volume 4 Issue 1 |
ISSN: | 2311-5521 |
DOI: | 10.3390/fluids4010036 |
Popis: | Thermomagnetic convection is still a phenomenon which generates interest among researchers. The authors decided to focus their attention on the magnetic field influence on forced convection and analyze the extended Graetz&ndash Brinkman problem. A numerical model based on a commonly available solver implemented with user-defined functions was used. The results exhibited the variety of possible flow structures depending on the dimensionless parameters, namely Prandtl and Reynolds numbers. Three flow structure classes were distinguished, and they provide a platform for further research. |
Databáze: | OpenAIRE |
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