Solar type III radio bursts are the most common impulsive radio signatures from the Sun,
stimulated by electron beams traveling through the solar corona and solar wind. Type III …

Solar Orbiter's four in situ instruments have recorded numerous energetic electron events at
heliocentric distances between 0.5 and 1 au. We analyze energetic electron fluxes, spectra …

Context. Radio U-bursts and J-bursts are signatures of electron beams propagating along
magnetic loops confined to the corona. The more commonly observed type III radio bursts …

Context. Solar type III radio bursts contain a wealth of information about the dynamics of
electron beams in the solar corona and the inner heliosphere; this information is currently …

Continuous plasma coherent emission is maintained by repetitive Langmuir collapse driven
by the nonlinear evolution of a strong electron two-stream instability. The Langmuir waves …

Solar radio type III bursts are believed to be the most sensitive signatures of near-relativistic
electron beam propagation in the corona. A solar radio type IIIb-III pair burst with fine …

A component of space weather, electron beams are routinely accelerated in the solar
atmosphere and propagate through interplanetary space. Electron beams interact with …

Plasma emission (PE), ie, electromagnetic radiation at the plasma frequency and its second
harmonic, is a general process occurring in both astrophysical and laboratory plasmas. The …

In this paper we study how efficiently electromagnetic radiation can be generated by a
relativistic electron beam with a gigawatt power level during its injection into a thin …

Solar accelerated electron beams, a component of space weather, are emitted by eruptive
events at the Sun. They interact with the ambient plasma to grow Langmuir waves, which …