  The parsec scale properties of low power radio galaxies are reviewed here,
using the available data on 12 FR I galaxies. The most frequent radio structure
is an asymmetric parsec-scale morphology, i.e. core and one-sided jet. It is
shared by 9 (possibly 10) of the 12 mapped radio galaxies. One (possibly 2) of
the other galaxies has (have) a two-sided jet emission. Two sources are known
from published data to show a proper motion; we present here evidence for
proper motion in two more galaxies. Therefore, in the present sample we have 4
radio galaxies with a measured proper motion. One of these has a very symmetric
structure and therefore should be in the plane of the sky. The results
discussed here are in agreement with the predictions of the unified scheme
models. Moreover, the present data indicate that the parsec scale structure in
low and high power radio galaxies is essentially the same.
