Fig. 10
Modeling of an equatorial, electron-filled, fragmented scattering disk with a half-opening angle θ0 = 80°. The fraction F/F∗ of the central flux (upper panel) and the spatially integrated polarization P (lower panel) are seen at different viewing inclinations, i, integrated over 2000 to 8000 Å. We note the change in scale between the polarizations of the four models.
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