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 …

Quasi-periodic, fast-mode propagating (QFP) wave trains in the corona have been studied
intensively over the last decade, thanks to the full-disk, high spatio-temporal resolution, and …

Context. We present a new event of quasi-periodic wave trains observed in EUV wavebands
that rapidly propagate away from an active region after a flare. Aims. We measured the …

Context. Fast magneto-acoustic waves are highly dispersive in waveguides, so they can
generate quasi-periodic wave trains if a localised, impulsive driver is applied. Such wave …

Context. Rapidly propagating coronal EUV disturbances recently discovered in the solar
corona are interpreted in terms of guided fast magnetoacoustic waves. Fast …

Aims. To obtain diagnostics tools for solar flare current sheets, we numerically studied
impulsively generated magnetoacoustic waves in the Harris current sheet. Methods. We …

We report a detailed observational study of two quasi-periodic fast-propagating (QFP)
magnetosonic wave events that occurred on 2011 March 9 and 10, respectively …

Aims. We numerically studied evolution of impulsively generated magnetoacoustic waves in
the vertical flare current-sheet that is embedded in the gravitationally stratified solar …

Impulsively generated fast magnetoacoustic wave trains in a solar coronal loop are
numerically studied. The problem is considered as 2-D in space, and for the description, the …

The digital, decimetric (950–2500MHz) Brazilian Solar Spectroscope (BSS, Sawant, HS,
Subramanian, KR, Faria, C., et al. Brazilian Solar Spectroscope (BSS). Solar Phys. 200, 167 …