Left: intensity spectra of the 2008 spectropolarimetry with the contribution of the secondary star subtracted. The mean spectra of two orbits are shown twice for visual continuity. Two systems of cyclotron lines are visible that originate near two poles of similar field strength. Center: circular polarization spectra with white indicating positive and black negative polarization. Right: maxima of the cyclotron lines of both poles (circles, triangles), extrema of the circular polarization (plus signs, crosses), and best-fit line positions as functions of orbital phase (red curves).