activity
20162025
most citedThe European Solar Telescope

99 citations · 309 across the 25 of their papers we have counts for

collaborators

25 papers

astro-ph.SR2025★ 2 cited

The magnetic sensitivity of the Ca II resonance and subordinate lines in the solar atmosphere

I. Juanikorena Berasategi, E. Alsina Ballester, T. del Pino Alemán +1

Aims: The polarization of the Ca II resonant doublet (H and K lines) and the subordinate infrared triplet lines are key observables for diagnosing solar chromospheric magnetism. It…

astro-ph.SR2025★ 4 cited

Determining the Magnetic Field in the Atmosphere of a Solar Active Region Observed by the CLASP2.1 Sounding Rocket Experiment

Ryohko Ishikawa, Javier Trujillo Bueno, David E. McKenzie +17

We determine magnetic fields from the photosphere to the upper chromosphere combining data from the Hinode satellite and the CLASP2.1 sounding rocket experiment. CLASP2.1 provided…

astro-ph.SR2025★ 2 cited

The uncertainty of magnetic fields in 3D non-local thermodynamic equilibrium inversions

Jiri Stepan, Tanausu del Pino Aleman, Andres Vicente Arevalo

We describe our approach to solve the problem of ensuring the solenoidality of the magnetic field vector in three-dimensional (3D) inversions, as well as the estimation of the unce…

astro-ph.SR2024

Mapping the longitudinal magnetic field in the atmosphere of an active region plage from the inversion of the near-ultraviolet CLASP2.1 spectropolarimetric data

Hao Li, Tanausú del Pino Alemán, Javier Trujillo Bueno +10

We apply the HanleRT Tenerife Inversion Code to the spectro-polarimetric observations obtained by the Chromospheric LAyer SpectroPolarimeter. This suborbital space experiment measu…

astro-ph.SR2024★ 4 cited

Magnetic field diagnostics of prominences with the Mg II k line: 3D Stokes inversions versus traditional methods

Jiří Štěpán, Tanausú del Pino Alemán, Javier Trujillo Bueno

The Mg II k resonance line is commonly used for diagnosing the solar chromosphere. We theoretically investigated its intensity and polarization in solar prominences, taking 3D radi…

astro-ph.SR2024

Accurate PRD modeling of the forward-scattering Hanle effect in the chromospheric CaI 4227 Å line

Luca Belluzzi, Simone Riva, Gioele Janett +7

Measurable linear scattering polarization signals have been predicted and detected at the solar disk center in the core of chromospheric lines. These forward-scattering polarizatio…