Modeling compact tori (left: uniform-density model; right: clumpy torus) with θ₀ = 45° measured relative to the symmetry axis. In the case of the fragmented torus, the filling factor is equal to 0.25 and the optical thickness per clump is 50 in the V-band. The fraction F/F_∗ of the central flux (upper figures) and the spatially integrated polarization P (lower figures) are seen at different viewing inclinations, i, from 2000 to 8000 Å. We note the change in scale between the polarization spectra of the two models.