activity
20152021
most citedBroad Non-Gaussian Fe XXIV Line Profiles in the Impulsive Phase of the 2017 September 10 X8.3 class Flare Observed by Hinode/EIS

65 citations · 166 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.SR2021★ 9 cited

Saddle-shaped solar flare arcades

Juraj Lörinčík, Jaroslav Dudík, Guillaume Aulanier

Arcades of flare loops form as a consequence of magnetic reconnection powering solar flares and eruptions. We analyse the morphology and evolution of flare arcades that formed duri…

astro-ph.SR2021★ 5 cited

Flare Expansion to a Magnetic Rope Accompanied by Rare Radio Bursts

Alena Zemanová, Marian Karlický, Jana Kašparová +1

We present multispectral analysis (radio, H, UV/EUV, and hard X-ray) of a confined flare from 2015 March 12. This flare started within the active region NOAA 12 297 and then it…

astro-ph.SR2020

Plasma Diagnostics From Active Region and Quiet Sun Spectra Observed by Hinode/EIS: Quantifying the Departures from a Maxwellian Distribution

Juraj Lörinčík, Jaroslav Dudík, Giulio del Zanna +2

We perform plasma diagnostics, including that of the non-Maxwellian -distributions, in several structures observed in the solar corona by the Extreme-Ultraviolet Imaging Spectro…

astro-ph.SR2019★ 24 cited

Velocities of flare kernels and the mapping norm of field line connectivity

Juraj Lörinčík, Guillaume Aulanier, Jaroslav Dudík +2

We report on observations of flare ribbon kernels during the 2012 August 31 filament eruption. In the 1600\,Å and 304\,Å channels of the Atmospheric Imaging Assembly, flare kernels…

astro-ph.SR2018★ 65 cited

Broad Non-Gaussian Fe XXIV Line Profiles in the Impulsive Phase of the 2017 September 10 X8.3 class Flare Observed by Hinode/EIS

Vanessa Polito, Jaroslav Dudík, Jana Kašparová +4

We analyze the spectra of high temperature \fexxiv~lines observed by \emph{Hinode}/EIS during the impulsive phase of the X8.3--class flare on September 10, 2017. The line profiles…

astro-ph.SR2015★ 63 cited

KAPPA: A Package for Synthesis of optically thin spectra for the non-Maxwellian kappa-distributions based on the CHIANTI database

Elena Dzifčáková, Jaroslav Dudík, Pavel Kotrč +2

The non-Maxwellian -distributions have been detected in the solar transition region and flares. These distributions are characterized by a high-energy tail and a near-Maxwellian…