Bibcode
Luna, M.; Terradas, J.; Oliver, R.; Ballester, J. L.
Bibliographical reference
Astronomy and Astrophysics, Volume 457, Issue 3, October III 2006, pp.1071-1079
Advertised on:
10
2006
Journal
Citations
18
Refereed citations
16
Description
Aims.We study fast magnetohydrodynamic waves in a system of two coronal
loops modeled as smoothed, dense plasma slabs in a uniform magnetic
field. This allows us to analyse in a simple configuration the
collective behaviour of the structure due to the interaction between the
slabs. Methods: .We first calculate the normal modes of the system
and find analytical expressions for the dispersion relation of the
two-slab configuration. Next, we study the time-dependent problem of the
excitation of slab oscillations by numerically solving the initial value
problem. We investigate the behaviour of the system for several shapes
of the initial disturbances. Results: .The symmetric mode respect
to the centre of the structure is the only trapped mode for all
distances between the slabs while the antisymmetric mode is leaky for
small slab separations. Nevertheless, there is a wide range of slab
separations for which the fundamental symmetric and antisymmetric
trapped modes are allowed and have very close frequencies. These modes
are excited according to the parity of the initial perturbation.
Conclusions: .We find that for any initial disturbance the slabs
oscillate with the normal modes of the coupled slab system, which are
different from the modes of the individual slabs. We show that it is
possible to excite the symmetric and antisymmetric trapped modes at the
same time. This kind of excitation can produce the beating phenomenon,
characterised by a continuous exchange of energy between the individual
slabs.