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In Wisniewski et al. 2010, paper I, we analyzed 15 years of spectroscopic andspectropolarimetric data from the Ritter and Pine Bluff Observatories of 2 Bestars, 60 Cygni and {\pi} Aquarii, when a transition from Be to B staroccurred. Here we anaylize the intrinsic polarization, where we observeloop-like structures caused by the rise and fall of the polarization BalmerJump and continuum V-band polarization being mismatched temporally withpolarimetric outbursts. We also see polarization angle deviations from themean, reported in paper I, which may be indicative of warps in the disk, blobsinjected at an inclined orbit, or spiral density waves. We show our ongoingefforts to model time dependent behavior of the disk to constrain thephenomena, using 3D Monte Carlo radiative transfer codes.

Disk-Loss and Disk Renewal Phases in Classical Be Stars II. Detailed Analysis of Spectropolarimetric Data