  Recently completed H-Alpha surveys of large portions of the sky can be used
to create maps of the free-free intensity distribution at high Galactic
latitude that are independent of the spectral fits to the CMB data. This
provides an opportunity to test the accuracy of the spectral fitting procedures
and to search for other sources of Galactic forground contamination that could
be confused spectrally with the free-free, such as spinning dust grains. The
Wisconsin H-Alpha Mapper (WHAM) survey has sampled the sky north of declination
-30 deg at about one degree angular resolution and has revealed that, except
for a few isolated regions of enhanced emission, \Delta T_{ff} (30 GHz) < 30
micro-K at Galactic latitudes near 15 deg, decreasing to \Delta T_{ff} (30 GHz)
< 4 mircro-K at latitudes above 50 deg. Also in progress are H-Alpha surveys
that sample the sky at higher angular resolution.
