  We present new radio observations of the brighter region of the northern lobe
(the Northern Middle Lobe, NML) of Centaurus A obtained at 20 cm with the
Australia Telescope Compact Array. The angular resolutions are ~50 and ~130
arcsec, therefore much higher than for the previously available radio images of
this region. The most interesting feature detected is a large-scale jet that
connects the inner radio lobe and the NML and that is imaged for the first
time. The NML itself appears as diffuse emission with a relatively bright ridge
on the eastern side. The radio morphology of Centaurus A and, in particular,
its NML could be the result of a precessing jet that has undergone a strong
interaction with the environment at least in the northern side. The very big
drop in intensity between the inner jet and the large-scale jet can be
explained with a sequence of bursts of activity at different epochs in the life
of the source. Alternatively (or additionally) a ``bursting bubble'' model is
proposed which could also explain the good collimation of the large-scale jet.
In this model, the plasma accumulated in the inner lobe would be able to
``burst'' out only through one nozzle that would be the region where the
large-scale jet forms. From the comparison between the radio emission and the
regions of ionized gas we find that the inner optical filament falls about 2
arcmin (~2 kpc) away from the large-scale radio jet. Thus, this filament does
not seem to have experienced a direct interaction with the radio plasma. The
outer filaments appear to be, in projection, closer to the radio emission,
arguing for a direct interaction with the radio jet. However, also in this case
a more complicated interaction than assumed so far has to be occuring.
