Fig. 2: Saturation of the no-cosines flow

Total magnetic, kinetic and thermal energy as functions of time for cases with Rem = 100 and Re = 50 (left) and Rem = 100 and Re = 400 (right). Line styles are the same as in Fig. 1.

From the paper "On the Saturation of Astrophysical Dynamos: Numerical Experiments with the No-Cosines Flow" by S. B. F. DorchV. Archontis.

Published in: Solar Physics October 2004.