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Origin of Spatial Variations of Scattering Polarization in the Wings of the Ca I 4227 Å Line

  • Authors: M. Sampoorna, J. O. Stenflo, K. N. Nagendra, M. Bianda, R. Ramelli, and L. S. Anusha

SAMPOORNA et al. 2009 The Astrophysical Journal 699 1650.

  • Provider: AAS Journals

Caption: Figure 7.

Attempt to model the ( Q/ I, U/ I) wing signatures. The observations (dotted lines) shown here correspond to the "magnetic observations" presented in Figure  2. In the Q/ I panel the heavy solid line represents the magnetic model profile, the thin solid line the nonmagnetic model profile, and the dashed line their difference. In the U/ I panel, the solid line represents the magnetic model profile. The parameters used are (Γ B , thetav B , phiv B ; Γ ER) = (10, 90°, 135°; 10).

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