We analyze intensity variations, as measured by the Atmospheric Imaging Assembly in the 171 Å passband, in two coronal loops embedded within a single coronal magnetic arcade. We detect oscillations in the fundamental mode with periods of roughly 2 minutes and decay times of 5 minutes. The oscillations were initiated by interaction of the arcade with a large wavefront issuing from a flare site. Further, the power spectra of the oscillations evince signatures consistent with oblique propagation to the field lines and for the existence of a two-dimensional waveguide instead of a one-dimensional one
Coronal loops exist ubiquitously in the solar atmosphere. These loops puzzle astronomers over half a...
Quasi-periodical oscillations of positions of coronal loops were observed in the extreme- ultraviole...
High cadence, 171 Angstrom, TRACE observations show that outward propagating intensity disturbances ...
Images of the solar corona by extreme-ultraviolet (EUV) telescopes reveal elegant arches of glowing ...
We study intensity variations, as measured by the Atmospheric Imaging Assembly on board the Solar Dy...
We present an alternative model of coronal-loop oscillations, which considers that the waves are tra...
Context: Transverse loop oscillations and loop contractions are commonly associated with solar flare...
We report decaying quasi-periodic intensity oscillations in the X-ray (6–12 keV) and extreme-ultravi...
Context. Kink oscillations in coronal loops are ubiquitous, and we apply the observed parameters of ...
Context. Magnetic arcades in the solar atmosphere, or coronal loops, are common structures known to ...
Loops of hot plasma trace the invisible magnetic field lines of the Sun's dynamic corona. These stru...
High cadence, 171 Å, TRACE observations show that outward propagating intensity disturbances are a c...
Copyright © 2012 ESO / EDP SciencesAims. We report and analyse the first observation of a transverse...
Aims. We report and analyse the first observation of a transverse oscillation in a hot coronal loop ...
We present measurements of periodicity for transverse loop oscillations during the periods of activi...
Coronal loops exist ubiquitously in the solar atmosphere. These loops puzzle astronomers over half a...
Quasi-periodical oscillations of positions of coronal loops were observed in the extreme- ultraviole...
High cadence, 171 Angstrom, TRACE observations show that outward propagating intensity disturbances ...
Images of the solar corona by extreme-ultraviolet (EUV) telescopes reveal elegant arches of glowing ...
We study intensity variations, as measured by the Atmospheric Imaging Assembly on board the Solar Dy...
We present an alternative model of coronal-loop oscillations, which considers that the waves are tra...
Context: Transverse loop oscillations and loop contractions are commonly associated with solar flare...
We report decaying quasi-periodic intensity oscillations in the X-ray (6–12 keV) and extreme-ultravi...
Context. Kink oscillations in coronal loops are ubiquitous, and we apply the observed parameters of ...
Context. Magnetic arcades in the solar atmosphere, or coronal loops, are common structures known to ...
Loops of hot plasma trace the invisible magnetic field lines of the Sun's dynamic corona. These stru...
High cadence, 171 Å, TRACE observations show that outward propagating intensity disturbances are a c...
Copyright © 2012 ESO / EDP SciencesAims. We report and analyse the first observation of a transverse...
Aims. We report and analyse the first observation of a transverse oscillation in a hot coronal loop ...
We present measurements of periodicity for transverse loop oscillations during the periods of activi...
Coronal loops exist ubiquitously in the solar atmosphere. These loops puzzle astronomers over half a...
Quasi-periodical oscillations of positions of coronal loops were observed in the extreme- ultraviole...
High cadence, 171 Angstrom, TRACE observations show that outward propagating intensity disturbances ...