EDP Sciences
Free access
Volume 461, Number 3, January III 2007
Page(s) 1149 - 1154
Section The Sun
DOI http://dx.doi.org/10.1051/0004-6361:20065986

A&A 461, 1149-1154 (2007)
DOI: 10.1051/0004-6361:20065986

Sausage oscillations of coronal loops

D. J. Pascoe, V. M. Nakariakov, and T. D. Arber

Physics Department, University of Warwick, Coventry, CV4 7AL, UK
    e-mail: D.J.Pascoe@warwick.ac.uk

(Received 6 July 2006 / Accepted 29 September 2006 )

Aims.Analytical theory predicts the existence of trapped global (or fundamental) sausage fast magnetoacoustic modes in thick and dense coronal loops only, with the periods estimated as the ratio of double the loop length and the Alfvén speed outside the loop. We extend this study to the leaking regime, considering global sausage modes of long loops with small density contrasts.
Methods.Anti-symmetric fast magnetoacoustic perturbations (sausage, or m=0 modes) of a low $\beta$ plasma slab with the symmetric Epstein profile of plasma density are modelled numerically.
Results.It was found that long loops with sufficiently small density contrast can support global sausage leaky modes of detectable quality. The periods of the leaky modes are found to be approximately determined by the loop length and the external Alfvén speed. If the loop length can be estimated from imaging observations, the observed period of this mode provides us with the information about the Alfvén speed outside the loop. For typical flaring coronal loops, the estimated periods of the global sausage modes are about 5-60 s.

Key words: Sun: corona -- Sun: oscillations -- Sun: flares -- magnetohydrodynamics (MHD)

© ESO 2007

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