activity
20192025
most citedWave excitation by energetic ring-distributed electron beams in the solar corona

21 citations · 37 across the 5 of their papers we have counts for

collaborators

5 papers

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.SR2023

Weak Solar Radio Bursts from the Solar Wind Acceleration Region Observed by Parker Solar Probe and Its Probable Emission Mechanism

Ling Chen, Bing Ma, Dejin Wu +7

The Parker Solar Probe (PSP) provides us the unprecedentedly close approach observation to the Sun, and hence the possibility of directly understanding the "elementary process" whi…

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…

physics.plasm-ph2020★ 9 cited

The effects of density inhomogeneities on the radio wave emission in electron beam plasmas

Xin Yao, Patricio A. Muñoz, Jörg Büchner +2

Type III radio bursts are radio emissions associated with solar flares. They are considered to be caused by electron beams traveling from the solar corona to the solar wind. Magnet…

physics.plasm-ph2019★ 21 cited

Wave excitation by energetic ring-distributed electron beams in the solar corona

X. Zhou, P. A. Muñoz, J. Büchner +1

We analyzed properties of waves excited by mildly relativistic electron beams propagating along magnetic field with a ring-shape perpendicular momentum distribution in neutral and…