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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 5.

Role of PRD. The heavy solid and dotted lines are the same as in Figure  4. The dashed line is the model profile computed with frequency coherent scattering (CS), while the dot-dashed line is computed assuming CRD. The thin solid line is the model profile with R II- AA , while the heavy solid line has been computed with R II- AD .

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