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arXiv · 2002.09404

Rayleigh-B\'{e}nard Convection in Strong Vertical Magnetic Field: Flow Structure and Verification of Numerical Method

Ruslan Akhmedagaev·Oleg Zikanov·Dmitry Krasnov·Joerg Schumacher
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Abstract

Direct numerical simulations are performed to study turbulent Rayleigh-B\'{e}nard convection in a vertical cylindrical cavity with uniform axial magnetic field. Flows at high Hartmann and Rayleigh numbers are considered. The calculations reveal that, similarly to the behavior observed in Rayleigh-B\'{e}nard convection with strong rotation, flows at strong magnetic field develop a central vortex, while the heat transfer is suppressed.

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Ruslan Akhmedagaev, Oleg Zikanov, Dmitry Krasnov, Joerg Schumacher. 2020-02-21. Rayleigh-B\'{e}nard Convection in Strong Vertical Magnetic Field: Flow Structure and Verification of Numerical Method. https://arxiv.org/abs/2002.09404

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