activity
20242026
most citedA numerical approach for modelling the polarisation signals of strong resonance lines with partial frequency redistribution. Numerical applications to two-term atoms and plane-parallel atmospheres

4 citations · 6 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.SR2026

Observational insights into Sr I 4607 Å scattering polarization with DKIST/ViSP

Franziska Zeuner, Ernest Alsina Ballester, Luca Belluzzi +4

Scattering polarization signals in the Sr I 4607 Å spectral line are among the strongest originating from the solar photosphere, offering a powerful diagnostic of tangled magnetic…

astro-ph.SR2026

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

Pietro Benedusi, Simone Riva, Tanausú del Pino Alemán +6

Several strong solar resonance lines show observable linear scattering polarization signals, holding a great potential for investigating the magnetism of the outer solar atmosphere…

astro-ph.SR2025★ 2 cited

DKIST resolves sub-arcsec photospheric scattering polarization

Franziska Zeuner, Luca Belluzzi, Ernest Alsina Ballester +4

Scattering polarization signals offer a unique diagnostics of the physical conditions in the solar atmosphere, in particular magnetic fields via the Hanle effect. However, their sp…

astro-ph.SR2025★ 4 cited

A numerical approach for modelling the polarisation signals of strong resonance lines with partial frequency redistribution. Numerical applications to two-term atoms and plane-parallel atmospheres

Fabio Riva, Gioele Janett, Luca Belluzzi +6

Aims. The main goal of this paper is to present an accurate and efficient numerical strategy for solving the radiative transfer problem for polarised radiation in strong resonance…

astro-ph.SR2024

Full Stokes-vector inversion of the solar Mg II h & k lines

Hao Li, Tanausú del Pino Alemán, Javier Trujillo Bueno

The polarization of the Mg II h & k resonance lines is the result of the joint action of scattering processes and the magnetic field induced Hanle, Zeeman, and magneto-optical effe…