April, 2026 - CESRA: Community of European Solar Radio Astronomers

Signatures of Large-scale Magnetic Field Disturbances and Switchbacks in Interplanetary Type III Radio Bursts by Daniel L. Clarkson et al.

April 30, 2026

Solar radio bursts are intrinsically linked to the motion of their emitting source through the coronal and heliospheric plasma. Electron transport is mostly confined to magnetic field lines. These electrons move at a substantial fraction of the speed of light and often generate radio emission via the plasma emission process. The resulting radio bursts, such as type III bursts from electrons streaming along open field lines, are an excellent diagnostic […]

Dataset for Recognition and Detection Based on Solar Radio Spectrogram Data by Yan et al

April 14, 2026

Solar radio bursts and their fine spectral structures contain key physical information related to plasma instabilities, high-energy particle acceleration, and other important processes. They therefore serve as an important observational means for studying solar activity and space weather. With the increasing volume of solar radio spectrogram observation data, deep learning-based recognition and detection of solar radio bursts have become a key research direction. However, most studies on meter-wave solar radio […]