  With the resonant magnetic perturbations (RMPs) consolidating as an important
tool to control the transport barrier relaxation, the mechanism on how they
work is still a subject to be clearly understood. In this work we investigate
the equilibrium states in the presence of RMPs for a reduced MHD model using 3D
electromagnetic fluid numerical code (EMEDGE3D) with a single harmonic RMP
(single magnetic island chain) and multiple harmonics RMPs in cylindrical and
toroidal geometry. Two different equilibrium states were found in the presence
of the RMPs with different characteristics for each of the geometries used. For
the cylindrical geometry in the presence of a single RMP, the equilibrium state
is characterized by a strong convective radial thermal flux and the generation
of a mean poloidal velocity shear. In contrast, for toroidal geometry the
thermal flux is dominated by the magnetic flutter. For multiple RMPs, the high
amplitude of the convective flux and poloidal rotation are basically the same
in cylindrical geometry, but in toroidal geometry the convective thermal flux
and the poloidal rotation appear only with the islands overlapping of the
linear coupling between neighbouring poloidal wavenumbers $m$, $m-1$, $m+1$.
