The transfer of resonance line polarization with partial frequency redistribution and J-state interference. Theoretical approach and numerical methods
The linear polarization signals produced by scattering processes in strong resonance lines are rich in information on the magnetic and thermal structure of the chromosphere and transition region of the Sun and of other stars. A correct modeling of these signals requires accounting for partial frequency redistribution effects, as well as for the
Belluzzi, L. et al.
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2014