Abstract
We seek the conditions in which Alfvén waves (AW) can be produced in laboratory-scale liquid metal experiments, i.e. at low magnetic Reynolds Number (Rm). Alfvén waves are incompressible waves propagating along magnetic fields typically found in geophysical and astrophysical systems. Despite the high values of Rm in these flows, AW can undergo high dissipation in thin regions, for example in the solar corona where anomalous heating occurs (Davila, Astrophys. J., vol. 317, 1987, p. 514; Singh & Subramanian, Sol. Phys., vol. 243, 2007, pp. 163–169). Understanding how AW dissipate energy and studying their nonlinear regime in controlled laboratory conditions may thus offer a convenient alternative to observations to understand these mechanisms at a fundamental level. Until now, however, only linear waves have been experimentally produced in liquid metals because of the large magnetic dissipation they undergo when Rm ≪ 1 and the conditions of their existence at low Rm are not understood. To address these questions, we force AW with an alternating electric current in a liquid metal in a transverse magnetic field. We provide the first mathematical derivation of a wave-bearing extension of the usual low-Rm magnetohydrodynamics (MHD) approximation to identify two linear regimes: the purely diffusive regime exists when Nω, the ratio of the oscillation period to the time scale of diffusive two-dimensionalisation by the Lorentz force, is small; the propagative regime is governed by the ratio of the forcing period to the AW propagation time scale, which we call the Jameson number Ja after (Jameson, J. Fluid Mech., vol. 19, issue 4, 1964, pp. 513–527). In this regime, AW are dissipative and dispersive as they propagate more slowly where transverse velocity gradients are higher. Both regimes are recovered in the FlowCube experiment (Pothérat & Klein, J. Fluid Mech., vol. 761, 2014, pp. 168–205), in excellent agreement with the model up to Ja ≲ 0.85 but near the Ja = 1 resonance, high amplitude waves become clearly nonlinear. Hence, in electrically driving AW, we identified the purely diffusive MHD regime, the regime where linear, dispersive AW propagate, and the regime of nonlinear propagation.
Original language | English |
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Article number | A19 |
Number of pages | 42 |
Journal | Journal of Fluid Mechanics |
Volume | 1003 |
DOIs | |
Publication status | Published - 16 Jan 2025 |
Bibliographical note
This is an Open Access article, distributed under the terms of the Creative Commons Attribution licence (http://creativecommons.org/licenses/by/4.0), which permits unrestricted re-use, distribution and reproduction, provided the original article is properly cited.Funding
The authors would also like to thank the IDEX of Université Grenoble Alpes for its substantial contribution to the funding of Samy Lalloz's doctoral scholarship through the International Strategic Partnerships (ISP) program. The SIMaP laboratory is part of the LabEx Tec 21 (Investissements d'Avenir, grant agreement no. ANR-11-LABX-0030). The UK subscription to EMFL for access to the magnets at LNCMI-Grenoble is funded by EPSRC grant NS/A000060/1.
Funders | Funder number |
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Université Grenoble Alpes | ANR-11-LABX-0030 |
Engineering and Physical Sciences Research Council | NS/A000060/1 |
Keywords
- high-Hartmann-number flows