Reduction of velocity fluctuations in a turbulent flow of gallium by an   external magnetic field
  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. 
Michael Berhanu, Basile Gallet, Nicolas Mordant, Stephan Fauve