  The diverse polarization properties in pulsars are in conflict with applying
a unique emission mechanism to the population. The polarization position angle
(PPA) traverse in most pulsars shows a S-shaped curve that can be interpreted
using the rotating vector model (RVM) as the radio emission being directed
either parallel or perpendicular to the divergent magnetic field lines and
argues for a coherent curvature radiation mechanism from charge bunches in a
strongly magnetized pair plasma. However, in a subset of pulsars the radio
emission is significantly depolarized and the PPA shows a complex pattern which
cannot be explained using RVM. We propose that even in such cases the highly
polarized time samples in the single pulses should follow the RVM with possibly
two parallel tracks separated by 90\degr. We have investigated PSR
J1645$-$0317, with complex PPA traverse, and demonstrated for the first time
that considering only the highly polarized time samples in the single pulses,
the PPA distribution clearly follows the RVM. We conclude that this strongly
favour the coherent curvature radiation mechanism to be universally applicable
in the pulsar population.
