  We have obtained Tully-Fisher (TF) measurements for some 3000 late-type
galaxies in the field and in 76 clusters distributed throughout the sky between
10 and 200\h Mpc. The cluster data are applied to the construction of an I band
TF template, resulting in a relation with a scatter of 0.35 magnitudes and a
zero-point accurate to 0.02 magnitudes. Peculiar motions are computed by
referral to the template relation, and the distribution of line-of-sight
cluster peculiar motions is presented.
  The dipole of the reflex motion of the Local Group of galaxies with respect
to galaxies with measured peculiar velocity converges to the CMB dipole within
less than 6000 km/s. The progression of this convergence is well illustrated
when the reflex motion is referred to a well-distributed sample of field
galaxies, and it is maintained when the reflex motion is referred to the
reference frame constituted by the distant clusters in our sample. The field
and cluster samples exhibit bulk motion amplitudes of order 200 km/s or
smaller.
  Finally, we apply our sample of cluster peculiar velocities to a test of the
putative Hubble bubble recently claimed by Zehavi and coworkers. In contrast to
their findings, our data support a relatively quiescent Hubble flow beyond 35\h
Mpc.
