Numerical solutions of the three-dimensional magnetohydrodynamic alpha model.
We present direct numerical simulations and alpha -model simulations of four familiar three-dimensional magnetohydrodynamic (MHD) turbulence effects: selective decay, dynamic alignment, inverse cascade of magnetic helicity, and the helical dynamo effect. The MHD alpha model is shown to capture the long-wavelength spectra in all these problems, allowing for a significant reduction of computer time and memory at the same kinetic and magnetic Reynolds numbers. In the helical dynamo, not only does the alpha model correctly reproduce the growth rate of magnetic energy during the kinematic regime, it also captures the nonlinear saturation level and the late generation of a large scale magnetic field by the helical turbulence.
Mininni
Pablo D
PD
Advanced Study Program, National Center for Atmospheric Research, P. O. Box 3000, Boulder, Colorado 80307, USA.
Montgomery
David C
DC
Pouquet
Annick
A