most citedNonlinear Instability of kink oscillations due to shear motions

183 citations · 547 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph2008183 cited

Nonlinear Instability of kink oscillations due to shear motions

J. Terradas, J. Andries, M. Goossens +3

First results from a high-resolution three-dimensional nonlinear numerical study of the kink oscillation are presented. We show in detail the development of a shear instability in…

astro-ph200884 cited

Damping of Fast Magnetohydrodynamic Oscillations in Quiescent Filament Threads

Inigo Arregui, Jaume Terradas, Ramon Oliver +1

High-resolution observations provide evidence about the existence of small-amplitude transverse oscillations in solar filament fine structures. These oscillations are believed to r…

astro-ph2008116 cited

Analytic approximate seismology of transversely oscillating coronal loops

M. Goossens, I. Arregui, J. L. Ballester +1

We present an analytic approximate seismic inversion scheme for damped transverse coronal loop oscillations based on the thin tube and thin boundary approximation for computing the…

astro-ph200827 cited

On the scaling of the damping time for resonantly damped oscillations in coronal loops

Inigo Arregui, Jose Luis Ballester, Marcel Goossens

There is not as yet full agreement on the mechanism that causes the rapid damping of the oscillations observed by TRACE in coronal loops. It has been suggested that the variation o…

astro-ph200896 cited

Resonant absorption in complicated plasma configurations: applications to multi-stranded coronal loop oscillations

J. Terradas, I. Arregui, R. Oliver +3

We study the excitation and damping of transverse oscillations in a multi-stranded model of a straight line-tied coronal loop. The transverse geometry of our equilibrium configurat…

astro-ph200727 cited

Resonantly damped surface and body MHD waves in a solar coronal slab with oblique propagation

I. Arregui, J. Terradas, R. Oliver +1

The theory of magnetohydrodynamic (MHD) waves in solar coronal slabs in a zero- configuration and for parallel propagation of waves does not allow the existence of surface waves…