Bibcode
Belluzzi, L.; Trujillo Bueno, J.; Landi Degl’Innocenti, E.
Referencia bibliográfica
The Astrophysical Journal, Volume 814, Issue 2, article id. 116, 14 pp. (2015).
Fecha de publicación:
12
2015
Revista
Número de citas
13
Número de citas referidas
10
Descripción
The modeling of the peculiar scattering polarization signals observed in
some diagnostically important solar resonance lines requires the
consideration of the detailed spectral structure of the incident
radiation field as well as the possibility of ground level polarization,
along with the atom's hyperfine structure and quantum interference
between hyperfine F-levels pertaining either to the same fine structure
J-level, or to different J-levels of the same term. Here we present a
theoretical and numerical approach suitable for solving this complex
non-LTE radiative transfer problem. This approach is based on the
density-matrix metalevel theory (where each level is viewed as a
continuous distribution of sublevels) and on accurate formal solvers of
the transfer equations and efficient iterative methods. We show an
application to the D-lines of Na i, with emphasis on the enigmatic
D1 line, pointing out the observable signatures of the
various physical mechanisms considered. We demonstrate that the linear
polarization observed in the core of the D1 line may be
explained by the effect that one gets when the detailed spectral
structure of the anisotropic radiation responsible for the optical
pumping is taken into account. This physical ingredient is capable of
introducing significant scattering polarization in the core of the Na i
D1 line without the need for ground-level polarization.
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