activity
20092026
most citedSlipping magnetic reconnection during an X-class solar flare observed by SDO/AIA

146 citations · 202 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.SR2026

Kinetic Processes to Radio Burst: First Observational-driven Study in Coronal Loops

Mehdi Yousefzadeh, Marian Karlicky, Artem Koval +3

Understanding the origin of coherent solar radio bursts requires linking macroscopic coronal structures with the kinetic processes responsible for wave generation. We investigate e…

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

Radio bursts observed during solar eruptive flares and their schematic summary

Marian Karlický

In this review we summarize results of our analysis of the observations of solar eruptive flares made by the Ondřejov radiospectrograph for more than twenty years. We also present…

astro-ph.SR2015★ 5 cited

SSALMON - The Solar Simulations for the Atacama Large Millimeter Observatory Network

S. Wedemeyer, T. Bastian, R. Brajsa +27

The Solar Simulations for the Atacama Large Millimeter Observatory Network (SSALMON) was initiated in 2014 in connection with two ALMA development studies. The Atacama Large Millim…

astro-ph.SR2014★ 146 cited

Slipping magnetic reconnection during an X-class solar flare observed by SDO/AIA

Jaroslav Dudík, Miho Janvier, Guillaume Aulanier +4

We present SDO/AIA observations of an eruptive X-class flare of July 12, 2012, and compare its evolution with the predictions of a 3D numerical simulation. We focus on the dynamics…

astro-ph.SR2009★ 51 cited

Response of optical hydrogen lines to beam heating: I. Electron beams

J. Kasparova, M. Varady, P. Heinzel +2

We investigate the role of non-thermal electrons in the formation regions of Halpha, Hbeta, and Hgamma lines in order to unfold their influence on the formation of these lines. We…