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2009 MAGNETO-SCIENCELarge Alfvén Waves in liquid sodiumAlfvén waves are hydromagnetic waves involving fluid velocityand magnetic field. They are a key ph<strong>en</strong>om<strong>en</strong>onin many geophysical and astrophysical area, such as theEarth’s liquid core, the magnetosphere, solar wind and interstellarplasma dynamics. They are difficult to observe inexperim<strong>en</strong>ts but it would be useful to reach a state of interactingAlfvén waves as a key example of weak turbul<strong>en</strong>ce.Here, we use liquid sodium (figure 154). Compared togalinstan (gallium/indium/tin liquid metal alloy) it is a betterelectrical conductor (ohmic dissipation of Alfvén wavesis reduced) and its d<strong>en</strong>sity is much less (h<strong>en</strong>ce Alfvénwaves are faster). The geometry of the liquid sodium cavityis a cylinder of diameter 10 cm and of l<strong>en</strong>gth 20 cm.This was inserted in an available diameter of 16 cm witha maximum value of 16 T. 7 coils are placed around thiscylinder at regular intervals along the l<strong>en</strong>gth. In addition, aso-called ‘emission’ coil is placed at one <strong>en</strong>d of the cylinderto provide a magnetic excitation of Alfvén waves. This is ashort electrical pulse curr<strong>en</strong>t producing a poloïdal magneticfield. The Alfvén wave can th<strong>en</strong> be observed on the signalof the 7 measuring coils. The characteristic dim<strong>en</strong>sionlessLundquist number (propagation time divided by dissipationtime) changed from a maximum of 60 with galinstanto around 500 with liquid sodium. H<strong>en</strong>ce we expect to observeAlfvén waves very clearly. In figure 155, the arrivalof an Alfvén wave is recorded at the <strong>en</strong>d of the cylindricalcavity, while it was produced at the other <strong>en</strong>d by a pulsein a coil. On the left-hand side, one can see the electricalpulse (black curve) followed by the arrival of a main oscillationwith a shorter delay wh<strong>en</strong> the applied B is stronger,according to the Alfvén propagation time. On the righthandside, time is made dim<strong>en</strong>sionless using the theoreticaltime of propagation of an Alfvén wave from one <strong>en</strong>d of thecylinder to the other: all arrivals collapse around a dim<strong>en</strong>sionlesstime of unity. In figure 156, the 7 measured signalsare shown. It is possible to follow the signal from the <strong>en</strong>dwhere it was created to the other <strong>en</strong>d. There is however anadditional compon<strong>en</strong>t to the signal which is the signatureof structural vibrations. The linearity of the response signal(figure 157) shows however that the excitation is not yetlarge <strong>en</strong>ough to reach a turbul<strong>en</strong>t state.Figure 155: Propagation of an Alfvén wave recorded on the coilfarthest from the ‘emission’ coil for differ<strong>en</strong>t int<strong>en</strong>sities of magneticfield. Same plot using the dim<strong>en</strong>sionless time scale based ontheoretical Alfvén speed.Figure 156:a pulse.The 7 signals of the 7 coils are plotted together, afterFigure 154: These photographs show the process of filling thecontainer with sodium, the bare setup and finally the setup withinits thermal insulator equipped with pressure and temperature s<strong>en</strong>sors.Figure 157: Linear response of electromotive force with respectto the int<strong>en</strong>sity of the excitation pulse. Energy losses during reflections.F. DebrayTh. Alboussiere, P. Cardin, P. La Rizza, J.P. Masson, H.C. Nataf, F. Plunian, N. Schaeffer, D. Schmitt(LGIT/CNRS/OSUG/UJF, Gr<strong>en</strong>oble)109

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