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

Solar flare emission is detected in all EM bands and variations in flux density of solar
energetic particles. Often the EM radiation generated in solar and stellar flares shows a …

Quasi-periodic pulsations (or QPPs) are periodic intensity variations in the flare emission
that occur across all wavelength bands. In this article, we review the observational 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 …

We explore the quasi-periodic pulsations (QPPs) in a solar flare observed by Fermi Gamma-
ray Burst Monitor, Solar Dynamics Observatory, Solar Terrestrial Relations Observatory, and …

The dependence of the period of sausage oscillations of coronal loops on length together
with the depth and steepness of the radial profile are determined. We performed a …

In this paper, we report our multiwavelength observations of the C3. 1 circular-ribbon flare
SOL2015-10-16T10: 20 in active region (AR) 12434. The flare consisted of a circular flare …

An observation from the Interface Region Imaging Spectrograph reveals coherent
oscillations in the loops of an M1. 6 flare on 2015 March 12. Both the intensity and Doppler …

Context. Diagnostics of magnetohydrodynamic (MHD) waves in the solar atmosphere is a
topic that often encounters interpretation problems, partly because of the high complexity of …

Kink oscillations of coronal loops are often influenced by external events and this results in
various changes of the oscillations. Studying the changes can provide valuable information …