Abstract:
Using a shell model of turbulence, we have investigated a long-time
evolution of magnetic and velocity fields in the MHD turbulence with
various types of initial states. For each kind of these
states, 24 realizations of the process with random noise in the initial
states were modeled simultaneously with the help of a parallel computer cluster at the
Research Computing Center of Moscow State University. For
most realizations, a coherent state with high alignment
between the magnetic and velocity fields has been developed. In the case of
establishment of the coherent state, the dissipation rate of energy is found
to be substantially reduced. At the same time, there exist few realizations
that behave in another manner: they are characterized by a lower level of
cross-helicity or an essentially faster energy decay.
Keywords:shell models, MHD turbulence, magnetic fields, parallel algorithms, energy dissipation.