This is a simulation of Pm=50, so Rm is pretty much pushed to the limit. The data files var.dat in the proc0-127 directory tree is at t=882. This is at a time where magnetic and kinetic energies are approximately in equipartition. At t=558.86 the field had been rescaled by a factor of 100, so as to reach equipartition faster.

  • Other parameters: ν=10-3, η=2×10-5
  • Foring amplitude: f0=0.02
  • Average foring wavenumber: kf=1.5

    Further details and discussions of this run can be found on pp. 57-59 of Brandenburg & Subramanian (2005).

    Reference:

    Brandenburg, A., & Subramanian, K.: 2005, ``Astrophysical magnetic fields and nonlinear dynamo theory,'' Phys. Rep. 417, 1-209 (astro-ph/0405052, ADS, PDF)

    $Date: 2006/06/09 17:53:20 $, $Author: brandenb $, $Revision: 1.2 $