Natural-convection flow in the presence of a magnetic field in an enclosure heated from bottom and cooled from top is considered. The fluid (molten sodium) properties are function of temperature. To solve the governing non-linear differential equations (mass, momentum and energy) a finite volume code based on PATANKAR’s SIMPLER method is utilized. The results for different Rayleigh and Hartmann numbers show that the strength of the magnetic field has significant effects on the flow and temperature fields. The convection becomes stronger as the Rayleigh number increases while the magnetic field suppresses the convective flow and the heat transfer rate. When the magnetic field is weak and the Rayleigh number is high, the convection is dominant.
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ASME 2009 Heat Transfer Summer Conference collocated with the InterPACK09 and 3rd Energy Sustainability Conferences
July 19–23, 2009
San Francisco, California, USA
Conference Sponsors:
- Heat Transfer Division
ISBN:
978-0-7918-4357-4
PROCEEDINGS PAPER
Numerical Simulation of Magneto-Convection in an Enclosure
M. Ghassemi,
M. Ghassemi
K. N. Toosi University of Technology, Tehran, Iran
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M. Pirmohammadi
M. Pirmohammadi
K. N. Toosi University of Technology, Tehran, Iran
Search for other works by this author on:
M. Ghassemi
K. N. Toosi University of Technology, Tehran, Iran
M. Pirmohammadi
K. N. Toosi University of Technology, Tehran, Iran
Paper No:
HT2009-88433, pp. 883-888; 6 pages
Published Online:
March 12, 2010
Citation
Ghassemi, M, & Pirmohammadi, M. "Numerical Simulation of Magneto-Convection in an Enclosure." Proceedings of the ASME 2009 Heat Transfer Summer Conference collocated with the InterPACK09 and 3rd Energy Sustainability Conferences. Volume 2: Theory and Fundamental Research; Aerospace Heat Transfer; Gas Turbine Heat Transfer; Computational Heat Transfer. San Francisco, California, USA. July 19–23, 2009. pp. 883-888. ASME. https://doi.org/10.1115/HT2009-88433
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