activity
20172026
most citedTemperature dependent growth rates of the upper-hybrid waves and solar radio zebra patterns

22 citations · 116 across the 19 of their papers we have counts for

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Showing 2021Show all

6 papers · 1 filter

astro-ph.HE2021★ 7 cited

Linear acceleration emission of pulsar relativistic streaming instability and interacting plasma bunches

Jan Benáček, Patricio A. Muñoz, Jörg Büchner +1

Linear acceleration emission is one of the mechanisms that might explain intense coherent emissions of radio pulsars. This mechanism is not well understood, however, because the ef…

astro-ph.GA2021★ 4 cited

A Survey of Novae in M83

A. W. Shafter, K. Hornoch, J. Benáček +14

The results of the first synoptic survey of novae in the barred spiral and starburst galaxy, M83 (NGC 5236), are presented. A total of 19 novae and one background supernova were di…

astro-ph.SR2021★ 7 cited

Wave emission of non-thermal electron beams generated by magnetic reconnection

Xin Yao, Patricio Muñoz, Jörg Büchner +3

Magnetic reconnection in solar flares can efficiently generate non-thermal electron beams. The energetic electrons can, in turn, cause radio waves through microscopic plasma instab…

astro-ph.HE2021★ 1 cited

Bunch Expansion as a cause for Pulsar Radio Emissions

Jan Benáček, Patricio A. Muñoz, Jörg Büchner

Electromagnetic waves due to electron-positron clouds (bunches), created by cascading processes in pulsar magnetospheres, have been proposed to explain the pulsar radio emission. I…

astro-ph.SR2021★ 7 cited

Narrowband Spikes Observed during the 2013 November 7 Flare

Marian Karlický, Jan Benáček, Ján Rybák

Narrowband spikes are observed in solar flares for several decades. However, their exact origin is still discussed. To contribute to understanding of these spikes, we analyze the n…

astro-ph.HE2021★ 13 cited

Radio Emission by Soliton Formation in Relativistically Hot Streaming Pulsar Pair Plasmas

Jan Benáček, Patricio A. Muñoz, Alina C. Manthei +1

A number of possible pulsar radio emission mechanisms are based on streaming instabilities in relativistically hot electron-positron pair plasmas. At saturation the unstable waves…