Abstract
In this Keynote lecture, we review the main known features of MHD Turbulence at Low Magnetic Reynolds number, that is when the flow isn’t intense enough to disturb an externally applied magnetic field. The emphasis is deliberately placed on the very specific physical mechanisms of this type of flows, rather than their numerical modelling. We also focus on homogeneous magnetic fields which have received most attention. We stress in particular that the tendency to two-dimensionality observed in these flows casts the boundaries of the domain into a leading role.
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