  In this study, we investigate preferences of dipolar magnetic structure from
a seed magnetic field in the rapidly rotating spherical shell dynamo models. In
this study, we set up a realistic model to show the effect of the Lorentz force
in the polarity selection. The important results that has come out from our
study is that the magnetic field acts on the flow much before the saturation.
Our study suggests that the growth of the magnetic field is not a kinematic
effect as one might think off, rather a dynamic effect. This dynamic effect
grows as the field generated with time and finally brings the saturation to the
dynamo action. Previous studies show that Lorentz force effect the flow when
Elsasser number more or less 1 and the studies were focused on the saturation
by looking at the time-averaged quantities. However, in this study, we show a
clear effect of the Lorentz force even at Elsasser number of $0.3-0.4$. To show
the effect of the Lorentz force, we did two different simulations, one is a
nonlinear model and another is kinematic model and shows that how a magnetic
field can change the flow structure and by doing that the generated field
changes, while this kind of behavior is not observed in kinematic dynamo
models. This study shows a scale dependent behaviour of the kinetic helicity at
two different spectral range.
