We study the influence of kinetic-scale Alfvénic turbulence on the generation of plasma radio
emission in the solar coronal regions where the ratio β \upbeta of plasma to magnetic …

Narrowband radio bursts with durations of the order of milliseconds, called spikes, are
known to be associated with solar flares. In order to understand the particle beams …

Electrons accelerated in the corona during solar activity give rise to radio emission events
that can be observed over a wide range of frequencies. Among different finer-scale …

Fast Radio Bursts (FRBs) are ultra-brief, ultra-powerful bursts of energy of unknown source
that seem to be originating in distant galaxies. Here, we propose that they could be …

La dinámica en las regiones activas del sol está fuertemente dominada por las erupciones
solares, como evidencia de ello las observaciones actuales, las cuales muestran que las …