  This paper explores the effects of large-scale magnetic fields in hot
accretion flows for asymmetric configurations with respect to the equatorial
plane. The solutions that we have found show that the large-scale asymmetric
magnetic field can significantly affect the dynamics of the flow and also cause
notable outflows in the outer parts. Previously, we treated a viscous resistive
accreting disc in the presence of an odd symmetric $\textbf{B-}$ field about
the equatorial plane. Now we extend our earlier work by taking into account
another configuration of large-scale magnetic field which is no longer
symmetric. We provide asymmetric field structures with small deviations from
even and odd symmetric $\textbf{B-}$field. Our results show that the disc's
dynamics and appearance become different above and below the equatorial plane.
The set of solutions also predicts that even a small deviation in a symmetric
field causes the disc to compress on one side and expand on the other. In some
cases, our solution represents a very strong outflow from just one side of the
disc. Therefore, the solution may potentially explain the origin of one-sided
jets in radio galaxies.
