Damping Mechanisms for Oscillations in Solar Prominences
Small amplitude oscillations are a commonly observed feature in prominences/filaments. These oscillations appear to be of local nature, are associated to the fine structure of prominence plasmas, and simultaneous flows and counterflows are also present. The existing observational evidence reveals that small amplitude oscillations, after excited
Arregui, Iñigo et al.
Fecha de publicación:
7
2011