Bibcode
Luna, M.; Terradas, J.; Oliver, R.; Ballester, J. L.
Referencia bibliográfica
The Astrophysical Journal, Volume 716, Issue 2, pp. 1371-1380 (2010).
Fecha de publicación:
6
2010
Revista
Número de citas
30
Número de citas referidas
30
Descripción
We investigate the transverse oscillations of a line-tied multi-stranded
coronal loop composed of several parallel cylindrical strands. First,
the collective fast normal modes of the loop are found with the T-matrix
theory. There is a huge quantity of normal modes with very different
frequencies and a complex structure of the associated magnetic pressure
perturbation and velocity field. The modes can be classified as bottom,
middle, and top according to their frequencies and spatial structure.
Second, the temporal evolution of the velocity and magnetic pressure
perturbation after an initial disturbance are analyzed. We find complex
motions of the strands. The frequency analysis reveals that these
motions are a combination of low and high frequency modes. The
complexity of the strand motions produces a strong modulation of the
whole tube movement. We conclude that the presumed internal fine
structure of a loop influences its transverse oscillations and so its
transverse dynamics cannot be properly described by those of an
equivalent monolithic loop.