The phenomenon of quasi-periodic pulsations (QPPs) in solar and stellar flares has been
known for over 50 years and significant progress has been made in this research area. It has …

Abstract 'Pulsations' include a wide range of phenomena from strictly sinusoidal oscillations
up to quasiperiodic fine structures, observed in the radio, microwave and X-ray frequency …

We report here, for the first time, on spatial oscillations of coronal loops, which were detected
in extreme-ultraviolet wavelengths (171 Å) with the Transition Region and Coronal Explorer …

Pulsations in radio emission from the solar coronal plasma have been detected for over a
decade1–9. The oscillations are quasiperiodic, with periods of typically a second or so …

We examine observational evidence concerning energy release in solar flares. We propose
that different processes may be operative on four different time scales:(a) on the sub-second …

In the present discussion of the Hinotori satellite's solar flare X-ray observations, attention is
given to complex flare variety in X-ray temporal profiles, spectra, and morphology. The …

Solar burst emission data at shorter millimetre wavelengths have been based on a few
events measured with low sensitivity and relatively poor time resolution1–9. We present …

An analysis of the May 21, 1984 fast pulse solar burst detected by the Solar Maximum
Mission satellite associates the observed mm-wave emission with a synchrotron component …

Energy release in solar flares occurs during the impulsive phase, which is a period of a few
to about ten minutes, during which energy is injected into the flare region in bursts with …

Oscillatory reconnection is a process that has been suggested to underlie several solar and
stellar phenomena, and is likely to play an important role in transient events such as flares …