  We use Vector Spectromagnetograph (VSM) chromospheric full-disk magnetograms,
from the Synoptic Optical Long-term Investigations of the Sun (SOLIS) project,
to study the distribution of magnetic field flux concentrations within the
polar caps. We find that magnetic flux elements preferentially appear toward
lower latitudes within the polar caps away from the poles. This has
implications on numerous solar phenomena such as the formation and evolution of
fine polar coronal structures (i.e., polar plumes). Our results also have
implications for the processes carrying the magnetic flux from low to high
latitudes (e.g., meridional circulation).
