Transition from steady to oscillating convection rolls in Rayleigh-B\'enard convection under the influence of a horizontal magnetic field

TL;DR

This study investigates how a horizontal magnetic field influences Rayleigh-Bénard convection in a liquid metal, revealing a transition from steady to oscillating and then to three-dimensional turbulent flow as the magnetic influence varies.

Contribution

It provides experimental evidence on the transition from steady to oscillatory convection in a magnetic field, extending understanding of the Busse balloon in liquid metal convection.

Findings

Magnetic field extends the steady convection regime to higher Rayleigh numbers.

Transition to oscillatory flow occurs at a critical Q/Ra ratio, with initial two-dimensional oscillations.

Further decrease in Q/Ra leads to three-dimensional structures and turbulence.

Abstract

In this study we consider the effect of a horizontal magnetic field on the Rayleigh-B\'enard convection in a finite liquid metal layer contained in a cuboid vessel (200 \times 200 \times 40 mm^3). Laboratory experiments are performed for measuring temperature and flow field in the alloy GaInSn at Prandtl number Pr = 0.03 and in a Rayleigh number range 2.3 \times 10^4 < Ra < 2.6 \times 10^5. The field strength is varied up to a maximum value of 320 mT (Ha = 2470, Q = 6.11 \times 10^6). The magnetic field forces the flow to form two-dimensional rolls parallel to the direction of the field lines. The experiments confirm the predictions made by Busse and Clever (J. M\'ecanique Th\'eorique et Appliqu\'ee, 1983) who showed that the application of the horizontal magnetic field extends the range in which steady two-dimensional roll structures exist (Busse balloon) towards higher Ra numbers. A transition from the steady to a time-dependent oscillatory flow occurs when Ra exceeds a critical value for a given Chandrasekhar number Q, which is also equivalent to a reduction of the ratio Q/Ra. Our measurements reveal that the first developing oscillations are clearly of two-dimensional nature, in particular a mutual increase and decrease in the size of adjacent convection rolls is observed without the formation of any detectable gradients in the velocity field along the magnetic field direction. At a ratio of Q/Ra = 1, the first 3D structures appear, which initially manifest themselves in a slight inclination of the rolls with respect to the magnetic field direction. Immediately in the course of this, there arise also disturbances in the spaces between adjacent convection rolls, which are advected along the rolls due to the secondary flow driven by Ekman pumping. The transition to fully-developed three-dimensional structures and then to a turbulent regime takes place with further lowering Q/Ra.