activity
20082024
most citedObservation of a Large-scale Anisotropy in the Arrival Directions of Cosmic Rays above eV

409 citations · 3.2k across the 48 of their papers we have counts for

collaborators
Showing 2019Show all

9 papers · 1 filter

astro-ph.SR2019★ 7 cited

Continuum enhancements, line profiles and magnetic field evolution during consecutive flares

Francesca Zuccarello, Salvo L. Guglielmino, Vincenzo Capparelli +5

During solar flares, magnetic energy can be converted into electromagnetic radiation from radio waves to rays. Enhancements in the continuum at visible wavelengths give rise to…

astro-ph.SR2019★ 6 cited

Science Requirement Document (SRD) for the European Solar Telescope (EST) (3rd Edition, December 2025)

Rolf Schlichenmaier, Luis R. Bellot Rubio, Manuel Collados Vera +31

The European Strategy Forum on Research Infrastructures (ESFRI) included the European Solar Telescope (EST) as an ESFRI Project in its 2016 Roadmap and confirmed this status in 202…

astro-ph.HE2019★ 108 cited

Probing the origin of ultra-high-energy cosmic rays with neutrinos in the EeV energy range using the Pierre Auger Observatory

The Pierre Auger Collaboration, A. Aab, P. Abreu +389

Neutrinos with energies above eV are detectable with the Surface Detector Array of the Pierre Auger Observatory. The identification is efficiently performed for neutrinos…

astro-ph.HE2019★ 54 cited

Limits on point-like sources of ultra-high-energy neutrinos with the Pierre Auger Observatory

The Pierre Auger Collaboration, A. Aab, P. Abreu +389

With the Surface Detector array (SD) of the Pierre Auger Observatory we can detect neutrinos with energy between eV and eV from point-like sources across the…

astro-ph.SR2019★ 16 cited

Properties of the Umbral Filament Observed in Active Region NOAA 12529

S. L. Guglielmino, P. Romano, B. Ruiz Cobo +2

Recent observations of the solar photosphere revealed the presence of elongated filamentary bright structures inside sunspot umbrae, called umbral filaments (UFs). These features d…

astro-ph.SR2019

Recent insights on the penumbra formation process

M. Murabito, P. Romano, F. Zuccarello +1

Using high-resolution spectropolarimetric data acquired by \textit{IBIS}, as well as \textit{SDO}/HMI observations, we studied the penumbra formation in AR NOAA 11490 and in a samp…

astro-ph.SR2019

Continuum emission enhancements and penumbral changes observed during flares by IRIS, ROSA, and Hinode

F. Zuccarello, S. L. Guglielmino, V. Capparelli +6

In this paper we describe observations acquired by satellite instruments (Hinode/SOT and IRIS) and ground-based telescopes (ROSA@DST) during two consecutive C7.0 and X1.6 flares oc…

astro-ph.SR2019

Satellite observations of reconnection between emerging and pre-existing small-scale magnetic fields

S. L. Guglielmino, F. Zuccarello, P. R. Young +2

We report multi-wavelength ultraviolet observations taken with the IRIS satellite, concerning the emergence phase in the upper chromosphere and transition region of an emerging flu…

astro-ph.SR2019★ 1 cited

Long-term optical monitoring of the solar atmosphere in Italy

S. L. Guglielmino, I. Ermolli, P. Romano +8

Probably, the long-term monitoring of the solar atmosphere started in Italy with the first telescopic observations of the Sun made by Galileo Galilei in the early $17^{\mathrm{th}}…