  We consider electromagnetic fields and charged particle dynamics around
non-singular black holes in conformal gravity immersed in an external,
asymptotically uniform magnetic field. First, we obtain analytic solutions of
the electromagnetic field equation around rotating non-singular black holes in
conformal gravity. We show that the radial components of the electric and
magnetic fields increase with the increase of the parameters $L$ and $N$ of the
black hole solution. Second, we study the dynamics of charged particles. We
show that the increase of the values of the parameters $L$ and $N$ and of
magnetic field causes a decrease in the radius of the innermost stable circular
orbits (ISCO) and the magnetic coupling parameter can mimic the effect of
conformal gravity giving the same ISCO radius up to $\omega_{\rm B}\leq 0.07$
when $N=3$.
