activity
20042026
most citedAbsence of linear polarization in Halpha emission of solar flares

31 citations · 279 across the 30 of their papers we have counts for

collaborators

31 papers

astro-ph.SR2026

ZIMPOL detects scattering polarization in He I D during a solar flare

Francesco Vitali, Andrea Francesco Battaglia, Luca Belluzzi +5

Spectropolarimetric observations of solar flares in the He I D line at 5876 Å are extremely rare, and their diagnostic potential remains largely unexplored. We report the first…

astro-ph.SR2025

Study of an active region prominence using spectropolarimetric data in the He I D3 multiplet

S. Esteban Pozuelo, A. Asensio Ramos, J. Trujillo Bueno +3

Prominences are cool overdensities of plasma supported by magnetic fields that levitate in the solar corona. The physical characterization of these structures is key for understand…

astro-ph.SR2023★ 10 cited

Reconstruction of the Sunspot Number Source Database and the 1947 Zurich Discontinuity

Frédéric Clette, Laure Lefèvre, Sabrina Bechet +2

The recalibration of the sunspot number series, the primary long-term record of the solar cycle, requires the recovery of the entire collection of raw sunspot counts collected by t…

astro-ph.SR2022★ 9 cited

Hanle rotation signatures in Sr I 4607 Å

Franziska Zeuner, Luca Belluzzi, Nuno Guerreiro +2

Observations of scattering polarization and the Hanle effect in various spectral lines are increasingly used to complement traditional solar magnetic field determination techniques…

astro-ph.SR2022★ 4 cited

Spectropolarimetric observations of the solar atmosphere in the H 6563 Å line

J. Jaume Bestard, J. Trujillo Bueno, M. Bianda +2

We present novel spectropolarimetric observations of the hydrogen H line taken with the Zürich Imaging Polarimeter (ZIMPOL) at the Gregory Coudé Telescope of the Istituto Ricerc…

astro-ph.SR2020★ 9 cited

Observational indications of magneto-optical effects in the scattering polarization wings of the Ca I 4227 Å line

E. Capozzi, E. Alsina Ballester, L. Belluzzi +3

Several strong resonance lines, such as H I Ly-, Mg II k, Ca II K, Ca I 4227 Å\, which are characterized by deep and broad absorption profiles in the solar intensity spectrum, s…