  A Newtonian model of non-conductive, charged, perfect fluid tori orbiting in
combined spherical gravitational and dipolar magnetic fields is presented and
stationary, axisymmetric toroidal structures are analyzed. Matter in such tori
exhibits a purely circulatory motion and the resulting convection carries
charges into permanent rotation around the symmetry axis. As a main result, we
demonstrate the possible existence of off-equatorial charged tori and
equatorial tori with cusps enabling outflows of matter from the torus also in
the Newtonian regime. These phenomena represent qualitatively a new consequence
of the interplay between gravity and electromagnetism. From an astrophysical
point of view, our investigation can provide insight into processes that
determine the vertical structure of dusty tori surrounding accretion disks.
