Bibcode
Díaz, A. J.
Referencia bibliográfica
Astronomy and Astrophysics, Volume 456, Issue 2, September III 2006, pp.737-746
Fecha de publicación:
9
2006
Revista
Número de citas
22
Número de citas referidas
21
Descripción
Aims.A model of a elliptically shaped coronal arcade with piecewise
constant density is discussed to explore the effects of curvature on
radially polarised fast modes. It is important to test whether the main
results in the straight and cylindrical geometries can be extrapolated
to these more complex equilibria. Methods: .An equilibrium model
for a force-free, line-tied elliptical arcade is introduced and a
partial differential equation is derived for the velocity perturbation
of the fast modes, which is solved analytically. The properties of the
modes are studied in terms of the dispersion relation, which depends on
the eccentricity, the arcade width, and the density contrast.
Results: .Modes mainly contained in the cavity below the arcade are also
present, and have avoided crossings with the modes of the arcade. Even
the fundamental mode becomes leaky due to curvature. Approximated
relations are deduced for the frequency of the modes and the spatial
structure is discussed, focusing on the different families through which
a rich mode spectrum can be classified. Conclusions: .The
different types of modes of the spectrum are described and its relevance
to observations is discussed. The periods obtained in Cartesian geometry
provide a reasonable approximation, but this geometry lacks some other
key ingredients: the damping rates are different and some types of modes
present in the elliptical geometry are not sustained in the straight
slab.