Quasi-periodic pulsations (QPP) are a common feature of flaring energy releases in the
solar atmosphere, observed in all bands, from radio to hard X-ray. In this review we …

Characterized by cyclic axisymmetric perturbations to both the magnetic and fluid
parameters, magnetohydrodynamic fast sausage modes (FSMs) have proven useful for …

Abstract The Atacama Large Millimeter/submillimeter Array (ALMA) is a new powerful tool for
observing the Sun at high spatial, temporal, and spectral resolution. These capabilities can …

Magnetic reconnection plays a crucial role in powering solar flares, production of energetic
particles, and plasma heating. However, where the magnetic reconnections occur, how and …

Global extreme-ultraviolet (EUV) waves are spectacular traveling disturbances in the solar
corona associated with energetic eruptions such as coronal mass ejections (CMEs) and …

Solar flares often display pulsating and oscillatory signatures in the emission, known as
quasi-periodic pulsations (QPP). QPP are typically identified during the impulsive phase of …

This review discusses the complementary relationship between radio and hard X-ray
observations of the Sun using primarily results from the era of the Reuven Ramaty High …

Quasi-periodic pulsations (QPP) of microwave emission generated in single flaring loops
observed with the Nobeyama Radioheliograph (NoRH) and Nobeyama Radio Polarimeters …

Context. Quasi-periodic pulsations (QPP) of the electromagnetic radiation emitted in solar
and stellar flares are often detected in microwave, white light, X-ray, and gamma-ray bands …

Heliophysics is a fast-developing scientific discipline that integrates studies of the Sun's
variability, the surrounding heliosphere, and the environment and climate of planets. The …