Formation of polarized spectral lines in atmospheres with horizontal inhomogeneities
We study the problem of the generation and transfer of spectral line intensity and polarization in models of stellar atmospheres with horizontal plasma inhomogeneities. We solve the non-LTE radiative transfer problem in full 3D geometry taking into account resonant scattering polarization and its modification by magnetic fields via the Hanle effect
Tichý, A. et al.
Advertised on:
10
2015