  We present an analysis comparing the bulk--flow measurements for six recent
peculiar velocity surveys, namely, ENEAR, SFI, RFGC, SBF and the Mark III
singles and group catalogs. We study whether the direction of the bulk--flow
estimates are consistent with each other and construct the full three
dimensional bulk--flow vectors for each survey. We show that although the
surveys differ in their geometry, galaxy morphologies, distance measures and
measurement errors, their bulk flow vectors are expected to be highly
correlated and in fact show impressive agreement in all cases. We found a
combined weighted mean bulk motion of 330 km s$^{-1}$ $\pm 101$ km s$^{-1}$
toward $l= 234^{\degree}\pm 11^{\degree}$ and $b=12^{\degree}\pm 9^{\degree}$
in a sphere with an effective depth of $\sim4000$ km s$^{-1}$.
