activity
20072009
most citedDamping of filament thread oscillations: effect of the slow continuum

66 citations · 178 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.SR200966 cited

Damping of filament thread oscillations: effect of the slow continuum

R. Soler, R. Oliver, J. L. Ballester +1

Transverse oscillations of small amplitude are commonly seen in high-resolution observations of filament threads, i.e. the fine-structures of solar filaments/prominences, and are t…

astro-ph200860 cited

Non-adiabatic magnetohydrodynamic waves in a cylindrical prominence thread with mass flow

R. Soler, R. Oliver, J. L. Ballester

High-resolution observations show that oscillations and waves in prominence threads are common and that they are attenuated in a few periods. In addition, observers have also repor…

astro-ph200813 cited

Attenuation of small-amplitude oscillations in a prominence-corona model with a transverse magnetic field

R. Soler, R. Oliver, J. L. Ballester

Small-amplitude prominence oscillations are usually damped after a few periods. We study the attenuation of non-adiabatic magnetoacoustic waves in a slab prominence embedded in the…

astro-ph20078 cited

Oscillatory Modes of a Prominence-PCTR-Corona Slab Model

R. Soler, R. Oliver, J. L. Ballester

Oscillations of magnetic structures in the solar corona have often been interpreted in terms of magnetohydrodynamic waves. We study the adiabatic magnetoacoustic modes of a promine…

astro-ph200731 cited

The effect of the solar corona on the attenuation of small-amplitude prominence oscillations. I. Longitudinal magnetic field

R. Soler, R. Oliver, J. L. Ballester

Context. One of the typical features shown by observations of solar prominence oscillations is that they are damped in time and that the values of the damping times are usually bet…