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Magnetic modulation of flow reversals in liquid metal thermal convection

Yan-Wu Cao, Ming-Zhu Ai, Long Chen, Juan-Cheng Yang, Ming-Jiu Ni

TL;DR

This study addresses the rarity of flow reversals in low-$Pr$ liquid-metal convection by demonstrating that a transverse magnetic field can induce reversals in a quasi-two-dimensional cell. It combines GaInSn experiments across ranges of $Ra$ and $Ha$ with a theoretical framework that accounts for magnetic-field effects to predict reversal frequencies. The results reveal two linear thresholds in $(Ra/Ha)$ that separate stable-LSC, periodic-reversal, and stochastic-reversal regimes, and they validate an extended Ni-based model predicting reversal frequencies that closely match observations. The work shows that magnetic fields can controllably modulate reversal dynamics in low-$Pr$ convection by increasing an effective viscosity and $Pr^*$, offering a practical framework for studying MHD-reversal phenomena.

Abstract

Flow reversals are rarely observed in low-Prandtl-number liquid metal convection due to the fluid's exceptionally high thermal diffusivity. Here, we demonstrate that an external transverse magnetic field can induce such reversals in a quasi-two-dimensional (Q2D) rectangular cell with an aspect ratio ($\itΓ$) of $0.2$. Our experimental observations reveal that the system initially exhibits periodic dynamics at the onset of reversals before transitioning to stochastic behavior as the ratio of Rayleigh number ($Ra$) to Hartmann number ($Ha$) increases. This transition is governed by the competition between buoyancy and Lorentz forces, with experimental data showing a linear scaling relationship between $Ra$ and $Ha$ at critical points. We develop a theoretical model that incorporates magnetic field effects in low-Prandtl-number convection to predict the reversal frequencies. These findings provide new insights into how magnetic fields can modulate flow regimes in low-Prandtl-number convection, establishing a controlled framework for investigating reversal dynamics in magnetohydrodynamic systems.

Magnetic modulation of flow reversals in liquid metal thermal convection

TL;DR

This study addresses the rarity of flow reversals in low- liquid-metal convection by demonstrating that a transverse magnetic field can induce reversals in a quasi-two-dimensional cell. It combines GaInSn experiments across ranges of and with a theoretical framework that accounts for magnetic-field effects to predict reversal frequencies. The results reveal two linear thresholds in that separate stable-LSC, periodic-reversal, and stochastic-reversal regimes, and they validate an extended Ni-based model predicting reversal frequencies that closely match observations. The work shows that magnetic fields can controllably modulate reversal dynamics in low- convection by increasing an effective viscosity and , offering a practical framework for studying MHD-reversal phenomena.

Abstract

Flow reversals are rarely observed in low-Prandtl-number liquid metal convection due to the fluid's exceptionally high thermal diffusivity. Here, we demonstrate that an external transverse magnetic field can induce such reversals in a quasi-two-dimensional (Q2D) rectangular cell with an aspect ratio () of . Our experimental observations reveal that the system initially exhibits periodic dynamics at the onset of reversals before transitioning to stochastic behavior as the ratio of Rayleigh number () to Hartmann number () increases. This transition is governed by the competition between buoyancy and Lorentz forces, with experimental data showing a linear scaling relationship between and at critical points. We develop a theoretical model that incorporates magnetic field effects in low-Prandtl-number convection to predict the reversal frequencies. These findings provide new insights into how magnetic fields can modulate flow regimes in low-Prandtl-number convection, establishing a controlled framework for investigating reversal dynamics in magnetohydrodynamic systems.

Paper Structure

This paper contains 3 sections, 9 equations, 5 figures.

Figures (5)

  • Figure 1: Probe arrangement and velocity distribution without magnetic field. (a) Arrangement of temperature and ultrasonic probes in the experimental setup. (b) Measured $Nu$ and $Re$: black squares for $Nu$, blue triangles for $Re$, with the dotted line showing the fit and the red line indicating GL theory. (c) Time evolution of velocity at $Ra = 4.54 \times 10^6$, normalized by the free-fall time $\tau_{ff} = \sqrt{H/(\alpha g \Delta T)}$, showing a clear LSC with red and blue denoting opposite flow directions.
  • Figure 2: Typical flow reversal at $Ha=705.39$, $Ra=7.20\times10^6$ from experiment. (a) Spatiotemporal velocity distribution: red indicates flow in the positive $x$-direction (away from the probe), blue indicates the opposite. (b) Time series of temperature difference $\Delta T_{top} = T_1 - T_4$. (c) Instantaneous Nusselt number ($Nu$), synchronized with the velocity field; time is normalized by the free-fall time $\tau_{ff}$. The black box highlights a full reversal cycle, with dashed lines marking $\tau_r/4$, $\tau_r/2$, and $3\tau_r/4$. (d)-(g) Cartoons of flow structures at four typical moments within a cycle. Arrows represent velocity vectors derived from MPUDV, with color and size scaled by the instantaneous velocity normalized by $u_{max}$. The $x$ and $y$ axes correspond to directions defined in figure \ref{['fig:Fig_1']}(a).
  • Figure 3: Heat transfer in liquid metal convection. The scaling of $Nu$ versus $Ra$ is shown. Our data are compared with previous work, as indicated in the legend. The dashed line represents fitted results for $Ha=0$. The solid data points correspond to cases where a magnetic field is applied. For clarity, the $Nu$ values for $Ha =$ 554.23, 705.39, 857.11, 1158.85 and 1461.16 have been vertically shifted by +8, +6, +4, and +2 units, respectively. These artificial vertical shifts are illustrated in the inset plot.
  • Figure 4: The reversal characteristics in different regions. (a) and (b) are $\Delta T_{top}$ and its PSD for $Ra=2.86\times10^6$, $Ha=1461.16$ (white region in figure \ref{['fig:Fig_5']} (a)). (c) and (d) for $Ra=4.54\times10^6$, $Ha=554.23$ (orange region in figure \ref{['fig:Fig_5']} (a)). (e) and (f) for $Ra=2.28\times10^7$, $Ha=1158.85$ (blue region in figure \ref{['fig:Fig_5']} (a)). Red squares and green diamonds mark the start and end of reversals.
  • Figure 5: The statistical characteristics of flow reversal. (a) Phase diagram with three regimes divided by $(Ra/Ha)_{c1} \simeq 5250$ and $(Ra/Ha)_{c2} \simeq 16750$: Region I (stable LSC, inverted triangles), Region II (periodic reversals, squares), Region III (stochastic reversals, upright triangles). The marker color shows normalized $Nu$. Dimensionless reversal frequency with error bars. The error bar originates from the statistics of the reversals. Regions and vertical lines match figure \ref{['fig:Fig_5']} (a).