Physics – Fluid Dynamics
Scientific paper
2008-06-24
Physics
Fluid Dynamics
accepted for Physical Review E
Scientific paper
10.1103/PhysRevE.78.015302
The magnetic field of planets or stars is generated by the motion of a conducting fluid through a dynamo instability. The saturation of the magnetic field occurs through the reaction of the Lorentz force on the flow. In relation to this phenomenon, we study the effect of a magnetic field on a turbulent flow of liquid Gallium. The measurement of electric potential differences provides a signal related to the local velocity fluctuations. We observe a reduction of velocity fluctuations at all frequencies in the spectrum when the magnetic field is increased.
Berhanu Michael
Fauve Stéphan
Gallet Basile
Mordant Nicolas
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