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The nonlinear dynamics of a bundle of magnetic flux ropes driven bystationary fluid motions at their endpoints is studied, by performing numericalsimulations of the magnetohydrodynamic (MHD) equations. The development of MHDturbulence is shown, where the system reaches a state that is characterized bythe ratio between the Alfven time (the time for incompressible MHD waves totravel along the field lines) and the convective time scale of the drivingmotions. This ratio of time scales determines the energy spectra and therelaxation toward different regimes ranging from weak to strong turbulence. Aconnection is made with phenomenological theories for the energy spectra in MHDturbulence.Comment: Published in Physics of Plasma

Energy spectrum of turbulent fluctuations in boundary driven reduced magnetohydrodynamics