  We perform direct numerical simulations of three-dimensional freely decaying
magnetohydrodynamic (MHD) turbulence. For helical magnetic fields an inverse
cascade effect is observed in which power is transfered from smaller scales to
larger scales. The magnetic field reaches a scaling regime with self-similar
evolution, and power law behavior at high wavenumbers. We also find power law
decay in the magnetic and kinematic energies, and power law growth in the
characteristic length scale of the magnetic field.
