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Polarized Light Scattering with the Paschen-Back Effect, Level-crossing of Fine Structure States, and Partial Frequency Redistribution

  • Authors: K. Sowmya, K. N. Nagendra, M. Sampoorna, and J. O. Stenflo

Sowmya et al. 2014 The Astrophysical Journal 793 71.

  • Provider: AAS Journals

Caption: Figure 4.

Stokes profiles computed using the PB-FS code by including the contribution from the polarized continuum. The line types and the orientation of the magnetic field are indicated in the intensity panel. The vertical dotted lines in all the panels correspond to the line center wavelength of the L = 0 → 1 → 0 transition in the reference isotope 7Li; see text for more details.

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