Aims. We use multi-spacecraft observations of individual type III radio bursts to calculate the
directivity of the radio emission. We compare these data to the results of ray-tracing …

Interplanetary solar radio type III bursts provide the means to remotely study and track
energetic electrons propagating in the interplanetary medium. Due to the lack of direct radio …

Context. Metrewave solar type-III radio bursts offer a unique means to study the properties of
turbulence across coronal heights. Theoretical models have shown that the apparent …

Context. The Sun is the source of different types of radio bursts that are associated with solar
flares, for example. Among the most frequently observed phenomena are type III solar …

Solar radio spikes are short duration and narrow bandwidth fine structures in dynamic
spectra observed from the GHz to tens of MHz range. Their very short duration and narrow …

Understanding electron acceleration associated with magnetic energy release at subsecond
scales presents major challenges in solar physics. Solar radio spikes observed as …

Type II radio bursts are thought to be produced by shock waves in the solar atmosphere.
However, what magnetic conditions are needed for the generation of type II radio bursts is …

Multiple pieces of evidence have revealed the important role of turbulence in physical
processes in solar eruptions, from particle acceleration to the suppression of conductive …

Radio observations from space allow to characterize solar radio bursts below the
ionospheric cutoff, which are otherwise inaccessible, but suffer from low, insufficient …

Polarization of electromagnetic waves carries a large amount of information about their
astrophysical emitters and the media they passed through, and hence is crucial in various …