  We report on low resolution (R~3000) spectropolarimetry of the A0 supergiant
star HD 92207. This star is well-known for significant spectral variability.
The source was observed on seven different nights spanning approximately 3
months in time. With a rotation period of approximately 1 year, our data covers
approximately a quarter of the star's rotational phase. Variability in the
continuum polarization level is observed over this period of time. The
polarization across the Halpha line on any given night is typically different
from the degree and position angle of the polarization in the continuum.
Interestingly, Hbeta is not in emission and does not show polarimetric
variability. We associate the changes at Halpha as arising in the wind, which
is in accord with the observed changes in the profile shape and equivalent
width of Halpha along with the polarimetric variability. For the continuum
polarization, we explore a spiral shaped wind density enhancement in the
equatorial plane of the star, in keeping with the suggestion of Kaufer etal
(1997). Variable polarization signatures across Halpha are too complex to be
explained by this simple model and will require a more intensive polarimetric
follow-up study to interpret properly.
