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20012026
most citedAlfven Waves in the Lower Solar Atmosphere

443 citations · 3.8k across the 97 of their papers we have counts for

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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.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★ 10 cited

Hydrogen Emission in Type II White-light Solar Flares

Ondřej Procházka, Aaron Reid, Mihalis Mathioudakis

Type II WLFs have weak Balmer line emission and no Balmer jump. We carried out a set of radiative hydrodynamic simulations to understand how the hydrogen radiative losses vary with…

astro-ph.SR2019★ 14 cited

The Chromospheric Response to the Sunquake generated by the X9.3 Flare of NOAA 12673

Sean Quinn, Aaron Reid, Mihalis Mathioudakis +3

Active region NOAA 12673 was extremely volatile in 2017 September, producing many solar flares, including the largest of solar cycle 24, an X9.3 flare of 06 September 2017. It has…

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…