Solar flares are observed at all wavelengths from decameter radio waves to gamma-rays
beyond 1 GeV. This review focuses on recent observations in EUV, soft and hard X-rays …

Abstract Solar Energetic Particles (SEPs) are an important component of Space Weather,
including radiation hazard to humans and electronic equipment, and the ionisation of the …

Context. The origin of coronal type II radio bursts and the nature of their band splitting are
still not fully understood, though a number of scenarios have been proposed to explain …

Coronal mass ejections (CMEs) are large eruptions of plasma and magnetic field from the
low solar corona into the heliosphere. These eruptions are often associated with energetic …

Even small solar flares can display a surprising level of complexity regarding their
morphology and temporal evolution. Many of their properties, such as energy release and …

Context. The highest energies of solar energetic nucleons detected in space or through
gamma-ray emission in the solar atmosphere are in the GeV range. Where and how the …

Aims. We analyse particle, radio, and X-ray observations during the first relativistic proton
event of solar cycle 25 detected on Earth. The aim is to gain insight into the relationship …

Solar flares often involve the acceleration of particles to relativistic energies and the
generation of high-intensity bursts of radio emission. In some cases, the radio bursts can …

ABSTRACT A quantitative study of the observable radio signatures of the sausage, kink, and
torsional magnetohydrodynamic (MHD) oscillation modes in flaring coronal loops is …

We analyze the 26 November 2005 solar radio event observed interferometrically at
frequencies of 244 and 611 MHz by the Giant Metrewave Radio Telescope (GMRT) in Pune …