Solar coronal loop oscillations: theory of resonantly damped oscillations and comparison with observations
One of the proposed damping mechanisms of coronal transverse loop oscillations in the kink mode is resonant absorption as a result of the spatial variation of the Alfvén velocity in the equilibrium configuration. Analytical expressions for the period and the damping time exist for 1-D cylindrical equilibrium models with thin non-uniform
Goossens, M. et al.
Fecha de publicación:
9
2005