activity
20102026
most citedVorticity in the solar photosphere

127 citations · 1.6k across the 51 of their papers we have counts for

collaborators
Showing 2019Show all

5 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

High-resolution spectropolarimetric observations of the temporal evolution of magnetic fields in photospheric bright points

Peter H. Keys, Aaron Reid, Mihalis Mathioudakis +7

Context. Magnetic bright points (MBPs) are dynamic, small-scale magnetic elements often found with field strengths of the order of a kilogauss within intergranular lanes in the pho…

astro-ph.SR2019★ 17 cited

The magnetic properties of photospheric magnetic bright points with high resolution spectropolarimetry

Peter H. Keys, Aaron Reid, Mihalis Mathioudakis +7

Magnetic bright points are small-scale magnetic elements ubiquitous across the solar disk, with the prevailing theory suggesting that they form due to the process of convective col…

astro-ph.SR2019★ 5 cited

A Search for High-Frequency Coronal Brightness Variations in the 21 August 2017 Total Solar Eclipse

P. Rudawy, K. Radziszewski, A. Berlicki +4

We report on a search for short-period intensity variations in the green-line FeXIV 530.3 nm emission from the solar corona during the 21 August 2017 total eclipse viewed from Idah…

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…