  We study the ionised gas kinematics of 293 Active Galactic Nuclei (AGN) hosts
as compared to that of 485 control galaxies from the MaNGA-SDSS survey using
measurements of the [OIII]$\lambda$5007\AA emission-line profiles, presenting
flux, velocity and W$_{80}$ maps. In 45% of the AGN, a broad component was
needed to fit the line profiles wings within the inner few kpc, that we have
identified with an outflow. But in most AGN, the profiles are broader than that
of their controls over a much more extended region, identified as the
"kinematically disturbed regions" (KDRs). We find a positive correlation
between the mean $\langle$W$_{80}\rangle$ and L[OIII], supporting that the KDR
is due to heating and turbulence of the ISM by outflows and radiation from the
AGN. The extent R$_{KDR}$ reaches up to 24kpc, with a mean ratio to that of the
ENLR of 57%. We estimate ionised gas mass flow rates ($\dot{M}_{\rm out}$) and
kinetic powers ($\dot{E}_{\rm out}$) both from the AGN broad components and
from the W$_{80}$ values, that can be obtained for the whole AGN sample. We
find values for $\dot{M}_{\rm out}$ and $\dot{E}_{\rm out}$ that correlate with
the AGN luminosity $L_{bol}$, populating the low luminosity end of these known
correlations. The mean coupling efficiency between $\dot{E}_{\rm out}$ and AGN
luminosity is $\approx$ 0.02% from the W$_{80}$ values and lower from the broad
component. But the large extent of the KDR shows that even low-luminosity AGN
can impact the host galaxy along several kpc in a "maintenance mode" feedback.
