activity
20042025
most citedStar-planet interactions: II. Is planet engulfment the origin of fast rotating red giants?

77 citations · 457 across the 35 of their papers we have counts for

collaborators

37 papers

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.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.SR2021★ 14 cited

Velocity difference of ions and neutrals in solar prominences

Eberhard Wiehr, Goetz Stellmacher, Horst Balthasar +1

Marked velocity excesses of ions relative to neutrals are obtained from two time series of the neighboring emission lines He I 5015 and Fe II 5018 in a quiescent prominence. Their…

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…

astro-ph.SR2019★ 11 cited

Observations on spatial variations of the Sr~{\sc i} 4607~Å~scattering polarization signals at different limb distances with ZIMPOL

Sajal Kumar Dhara, Emilia Capozzi, Daniel Gisler +5

The Sr~{\sc i} 4607~Å spectral line shows one of the strongest scattering polarization signals in the visible solar spectrum. The amplitude of this polarization signal is expected…