Long period longitudinal oscillations of a flaring coronal loop are studied numerically. In the
recent work of Nakariakov et al.(2004) it has been shown that the time dependence of …

Evolution of a coronal loop in response to an impulsive energy release is numerically
modelled. It is shown that the loop density evolution curves exhibit quasi-periodic …

Context. Flaring coronal loops are often observed in microwave and sometimes in soft X-
rays, as extended structures of variable cross-section or width. The quasi-periodic pulsations …

Aims. Using temporal series image data from the Coronal Diagnostic Spectrometer (CDS)
on SOHO, we study oscillations found in intensity (radiance) measurements from the …

Rapidly decaying oscillations of the thermal emission detected in the decay phase of solar
and stellar flares are usually interpreted as standing or sloshing (reflecting) slow …

Standing long-period (with periods longer than several minutes) oscillations in large, hot
(with a temperature higher than 3 MK) coronal loops have been observed as the quasi …

Aims. We aim to study the influence of radiative cooling on the standing kink oscillations of a
coronal loop. Methods. Using the FLASH code, we solved the 3D ideal …

High cadence Transition Region and Coronal Explorer (TRACE) observations show that
outward propagating intensity disturbances are a common feature in large, quiescent …

Aims. We determine the dependence of the observed properties of fast magnetoacoustic
axisymmetric oscillations (the sausage mode) of a thick and dense flaring coronal loop …

Context. A detailed understanding of the physical processes that determine the damping
timescales of magneto-acoustic waves is essential to interpret diagnostic results from the …