  Polarization is the next frontier of CMB analysis, but its signal is
dominated over much of the sky by foregrounds which must be carefully removed.
To determine the efficacy of this cleaning it is necessary to have sensitive
tests for residual foreground contamination in polarization sky maps. The
dominant Galactic foregrounds introduce a large-scale anisotropy on to the sky,
so it makes sense to use a statistic sensitive to overall directionality for
this purpose. Here we adapt the rapidly computable D statistic of Bunn and
Scott to polarization data, and demonstrate its utility as a foreground monitor
by applying it to the low resolution WMAP 3-yr sky maps. With a thorough
simulation of the maps' noise properties, we find no evidence for contamination
in the foreground cleaned sky maps.
