T. del Pino Alemán

3D radiative transfer modeling of scattering polarization with partial frequency redistribution. I. Verification and disk-center results for the solar Ca i line at 4227,Å

Several strong solar resonance lines show observable linear scattering polarization signals, holding a great potential for investigating the magnetism of the outer solar atmosphere. Accurately modeling these signals requires consideration of the detailed 3D structure of the solar atmosphere and accounting for partial f...