“…A significant advance in the existing knowledge of MHD flows has been achieved by experiments (Lykoudis and Brouillette, 1968;Moresco and Alboussière, 2004) and by direct numerical simulations (DNS) in homogeneous turbulence (Zikanov and Thess, 1998;Kassinos et al, 2006Kassinos et al, , 2007, in turbulent channel (Lee and Choi, 2001;Boeck et al, 2007;Shatrov and Gerbeth, 2007;Krasnov et al, 2008) or pipe flows (Satake et al, 2002), and in natural convection in cylindrical cavities (Kakarantzas et al, 2009;Sarris et al, 2010) at low magnetic Reynolds numbers. A summary of related studies is provided by Knaepen and Moreau (2008).…”