Modeling the scattering polarization in the solar Ca I 4227Å line with angle-dependent PRD effects and bulk velocities
N. Guerreiro,
G. Janett,
S. Riva
et al.
Abstract:Modeling the scattering polarization signals of strong chromospheric lines requires solving the radiative transfer (RT) problem for polarized radiation, out of local thermodynamic equilibrium, taking partial frequency redistribution (PRD) effects into account.
This problem is extremely challenging from a computational standpoint and, so far, most studies have been carried out by either modeling PRD effects under the angle-average approximation or by considering academic models of the solar atmosphere.
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