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From the 1 of 5 linked papers with an AI index.

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5 papers

astro-ph.SR2026

Magnetic Field Stratification in Active-Region Plage from Ca II K and Ca II 8542 Ã Spectropolarimetry

Iñigo Juanikorena Berasategi, Ernest Alsina Ballester, Javier Trujillo Bueno +31

The study measures how the line‑of‑sight magnetic field strength changes from the photosphere to the upper chromosphere in solar active‑region plage using Ca II K and Ca II 8542 Å…

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.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

Spectropolarimetric synthesis of forbidden lines in MHD models of coronal bright points

Ernest Alsina Ballester, Daniel Nóbrega-Siverio, Fernando Moreno-Insertis +1

The inference of the magnetic field vector from spectropolarimetric observations is crucial for understanding the physical processes governing the solar corona. We investigate whic…

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…