activity
20242026
collaborators

8 papers

astro-ph.SR2026

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

Franziska Zeuner, Ernest Alsina Ballester, Luca Belluzzi +4

Scattering polarization signals in the Sr I 4607 Ã 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 Ã 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

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

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.SR2025

Multi-wavelength spectropolarimetric observations of AR13724 performed by GRIS

C. Quintero Noda, J. C. Trelles Arjona, T. del Pino Alemán +10

Multi-line spectropolarimetric observations allow for the simultaneous inference of the magnetic field at different layers of the solar atmosphere and provide insight into how thes…

astro-ph.SR2024

Non-Local Thermodynamic Equilibrium inversions of the Si I 10827 A spectral line

C. Quintero Noda, N. G. Shchukina, A. Asensio Ramos +4

Inferring the coupling of different atmospheric layers requires observing spectral lines sensitive to the atmospheric parameters, particularly the magnetic field vector, at various…