  We present an analysis of the velocity space of a sample of globular clusters
(GC) with absolute proper motions. The vertical component of the velocity is
found to be correlated with luminosity and galactocentric radius. We divided
the sample into two luminosity groups above and below the peak of the
luminosity function (LF), MV=-7.5, for Galactic GCs. The two groups display
different kinematic behaviour according to the first and second statitical
moments of the velocity distribution as well as distinct velocity ellipsoids.
The velocity ellipsoid of the high luminosity clusters is aligned with the
symmetry axes of the Galaxy, whereas the minor axis of the Low Luminosity group
is strongly inclined relative to the Galactic rotation axis.
