The angular asymmetries and relative separations of the hotspots of Fa
naroff-Riley II (FRII) radio sources in a complete sample of 3CR sourc
es have been used to study the effects of misalignment of the directio
ns of ejection and the velocities of the hotspots. It is found that th
e observed distribution of asymmetry angles is consistent with unified
schemes for radio galaxies and radio quasars and with the source comp
onents being ejected uniformly within an angle phi(max) of 6 degrees-7
degrees about the source axis. The separation quotients of the hotspo
ts are also consistent with unified schemes, if the velocities of the
hotspots have a broad distribution about a mean of 0.2 c, with values
extending at least up to 0.4 c.