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

collaborators

21 papers

astro-ph.HE2026

Fast Radio Bursts from Monster Shocks and Flares of Inspiraling Binary Neutron Stars: A Kinetic Model for Double Pulsar

Jan Benáček, Benoît Cerutti, Martin Pohl +2

The coalescence of binary neutron star systems offers unprecedented possibilities for multimessenger observations, including the detection of gravitational waves, gamma-ray bursts,…

astro-ph.HE2026

Understanding Pulsar Magnetospheres with the SKAO

L. S. Oswald, A. Basu, M. Chakraborty +21

The SKA telescopes will bring unparalleled sensitivity across a broad radio band, a wide field of view across the Southern sky, and the capacity for sub-arraying, all of which make…

astro-ph.HE2025

Understanding pulsar magnetospheres with the SKAO

L. S. Oswald, A. Basu, M. Chakraborty +22

The SKA telescopes will bring unparalleled sensitivity across a broad radio band, a wide field of view across the Southern sky, and the capacity for sub-arraying, all of which make…

astro-ph.HE2025★ 1 cited

A broadband study of FRB20240114A with the Effelsberg 100-m radio telescope

P. Limaye, L. G. Spitler, N. Manaswini +5

We present Effelsberg 100-m telescope observations of the hyperactive repeating fast radio burst source FRB 20240110A, discovered by CHIME/FRB in January 2024. Using the Ultra Broa…

physics.plasm-ph2025

Electromagnetic field solver for QED polarization in super-strong magnetic fields of magnetar and laser plasmas

Mahmoud Alawashra, Jan Benáček, Martin Pohl +1

Super-strongly magnetized plasmas play a crucial role in extreme environments of magnetar and laboratory laser experiments, demanding comprehensive understanding of how quantum ele…

astro-ph.SR2025

Small-scale inhomogeneity effects on coherent solar radio emission

Xiaowei Zhou, Patricio Munoz, Jan Benacek +5

Coherent radio emission mechanism of solar radio bursts is one of the most complicated and controversial topics in solar physics. To clarify the mechanism(s) of different types of…

astro-ph.HE2024★ 2 cited

Dispersion properties of neutron star magnetospheric plasmas with relativistic kappa distribution

M. Mousavi, J. Benáček

The various distribution functions can encompass the diverse characteristics of the magnetospheric plasma of surrounding neutron stars in both hot and cold environments; however, t…

astro-ph.SR2022★ 2 cited

Zebra stripes with high gyro-harmonic numbers

Jan Benáček, Marian Karlický

Solar radio zebras are used in the determination of the plasma density and magnetic field in solar flare plasmas. Analyzing observed zebra stripes and assuming their generation by…

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.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…

astro-ph.HE2020★ 13 cited

Refining pulsar radio emission due to streaming instabilities: Linear theory and PIC simulations in a wide parameter range

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

Several important mechanisms that explain the coherent pulsar radio emission rely on streaming (or beam) instabilities of the relativistic pair plasma in a pulsar magnetosphere. Ho…

astro-ph.SR2019★ 3 cited

Growth Rates of the Upper-hybrid Waves for Power-law and Kappa Distributions with a Loss-cone Anisotropy

Leonid V. Yasnov, Jan Benáček, Marian Karlický

Fine structures of radio bursts play an important role in diagnostics of the solar flare plasma. Among them the zebras, which are prevalently assumed to be generated by the double…

physics.plasm-ph2019★ 11 cited

Growth rates of the electrostatic waves in radio zebra models

Jan Benáček, Marian Karlický

Zebras were observed not only in the solar radio emission but also in radio emissions of Jupiter and Crab Nebula pulsar. In their models, growth rates of the electrostatic waves pl…

physics.plasm-ph2017★ 15 cited

Double plasma resonance instability as a source of solar zebra emission

Jan Benáček, Marian Karlický

The double plasma resonance (DPR) instability plays a basic role in the generation of solar radio zebras. In the plasma, consisting of the loss-cone type distribution of hot electr…

astro-ph.SR2017★ 8 cited

Brightness Temperature of Radio Zebras and Wave Energy Densities in Their Sources

Leonid V. Yasnov, Jan Benáček, Marian Karlický

We estimated the brightness temperature of radio zebras (zebra pattern -- ZP), considering that ZPs are generated in loops having an exponential density profile in their cross-sect…

astro-ph.SR2017★ 22 cited

Temperature dependent growth rates of the upper-hybrid waves and solar radio zebra patterns

Jan Benáček, Marian Karlický, Leonid V. Yasnov

Context. The zebra patterns observed in solar radio emission are very important for are plasma diagnostics. The most promising model of these patterns is based on double plasma res…