Role of uniform horizontal magnetic field on convective flow
Pinaki Pal, Krishna Kumar

TL;DR
This study investigates how a uniform horizontal magnetic field influences convective flow patterns in low-Prandtl-number fluids, revealing that it suppresses chaos, aligns rolls, and affects secondary instability thresholds without altering primary instability onset.
Contribution
It introduces a low-dimensional model to analyze the effects of horizontal magnetic fields on Rayleigh-Bénard convection, highlighting the magnetic field's role in stabilizing and orienting convective flows.
Findings
Magnetic field aligns convective rolls along its direction.
It inhibits the secondary wavy instability and chaos.
The critical Rayleigh number for wavy instability increases with magnetic field strength.
Abstract
The effect of uniform magnetic field applied along a fixed horizontal direction in Rayleigh-B\'enard convection in low-Prandtl-number fluids has been studied using a low dimensional model. The model shows the onset of convection (primary instability) in the form of two dimensional stationary rolls in the absence of magnetic field, when the Rayleigh number is raised above a critical value . The flow becomes three dimensional at slightly higher values of Rayleigh number via wavy instability. These wavy rolls become chaotic for slightly higher values of in low-Prandtl-number () fluids. A uniform magnetic field along horizontal plane strongly affects all kinds of convective flows observed at higher values of in its absence. As the magnetic field is raised above certain value, it orients the convective rolls in its own direction. Although the horizontal magnetic field…
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