activity
20052024
most citedDeducing Electron Properties From Hard X-Ray Observations

171 citations · 832 across the 24 of their papers we have counts for

collaborators

24 papers

astro-ph.SR2024

Slowly positively drifting bursts generated by large-scale magnetic reconnection

Alena Zemanová, Marian Karlický, Jana Kašparová +2

The slowly positively drifting bursts (SPDBs) are rarely observed in radio emission of solar flares. To understand how the SPDBs are generated, we studied the radio observations at…

astro-ph.SR2023★ 40 cited

The F-CHROMA grid of 1D RADYN flare models

Mats Carlsson, Lyndsay Fletcher, Joel Allred +6

Context: Solar flares are the result of the sudden release of magnetic energy in the corona. Much of this energy goes into accelerating charged particles to high velocity. These pa…

astro-ph.SR2022★ 7 cited

Filament Leg--Leg Reconnection as a Source of Prominent Supra-Arcade Downflows

Jaroslav Dudik, Guillaume Aulanier, Jana Kasparova +4

We report on interaction of the legs of the erupting filament of 2012 August 31 and associated prominent supra-arcade downflows (P-SADs) as observed by the Atmospheric Imaging Asse…

astro-ph.SR2022

Narrowband spikes observed during the 13 June 2012 flare in the 800-2000 MHz range

M. Karlicky, J. Rybak, J. Benacek +1

Narrowband (~5 MHz) and short-lived (~0.01 s) spikes with three different distributions on the 800-2000 MHz radio spectrum of the 13 June 2012 flare are detected and analyzed. We d…

astro-ph.SR2021★ 6 cited

On the Importance of Ca II Photoionisation by the Hydrogen Lyman Transitions in Solar Flare Models

Christopher M. J. Osborne, Petr Heinzel, Jana Kašparová +1

The forward fitting of solar flare observations with radiation-hydrodynamic simulations is a common technique for learning about energy deposition and atmospheric evolution during…

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…