The proper motions of the H2O masers in W49N have been measured with multie
poch very long baseline interferometry (VLBI) by Gwinn, Moran, & Reid. The
number of motions derived is large (105), and the spatial coverage of the s
ource by maser spots is excellent, making W49N a natural candidate for anal
ytic tools based on diagonalization of the velocity variance-covariance mat
rix (VVCM). The velocity dispersions (or internal relative velocities) used
in VVCM analysis are the quantities directly determined by VLBI proper mot
ion experiments, which lack an absolute phase reference. I apply the VVCM d
iagonalization procedure to the H2O masers in W49N, deriving in an objectiv
e, model-independent way the kinematic axes of the outflow. I then compare
these local axes with various geometrical axes suggested by the morphology
of an apparent "ring" of H II regions that accompany the one containing H2O
masers, and with the axis of the large-scale outflow seen in molecular emi
ssion. I also present kinematic evidence not revealed by previous modeling
for pronounced asymmetry of the collimating mechanism that channels the mas
er outflow, and propose an explanation in terms of magnetic drag.