Fig. 5
From: The competition between Lorentz and Coriolis forces in planetary dynamos
Comparison of predicted and calculated Elsasser numbers as a function of the relative strengths of buoyancy and Coriolis forces. Ratio of \(\Lambda _{d} / \Lambda _{d}^{*}\) plotted versus the convective Rossby number, \({Ro}_{c}=\sqrt {Ra E^{2}/Pr}\)