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Magneto-Acoustic Waves in Compressible Magnetically Twisted Flux Tubes
Erdélyi, Robert; Fedun, Viktor
AA(Solar Physics and Space Plasma Research Centre (SP²RC), Department of Applied Mathematics, University of Sheffield, Sheffield, UK), AB(Solar Physics and Space Plasma Research Centre (SP²RC), Department of Applied Mathematics, University of Sheffield, Sheffield, UK)
Solar Physics, Volume 263, Issue 1-2, pp. 63-85 (SoPh Homepage)
Publication Date:
Twisted magnetic flux tube, MHD waves, Solar atmosphere, Magneto-seismology
Abstract Copyright:
(c) 2010: Springer Science+Business Media B.V.
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The oscillatory modes of a magnetically twisted compressible flux tube embedded in a compressible magnetic environment are investigated in cylindrical geometry. Solutions to the governing equations to linear wave perturbations are derived in terms of Whittaker's functions. A general dispersion equation is obtained in terms of Kummer's functions for the approximation of weak and uniform internal twist, which is a good initial working model for flux tubes in solar applications. The sausage, kink and fluting modes are examined by means of the derived exact dispersion equation. The solutions of this general dispersion equation are found numerically under plasma conditions representative of the solar photosphere and corona. Solutions for the phase speed of the allowed eigenmodes are obtained for a range of wavenumbers and varying magnetic twist. Our results generalise previous classical and widely applied studies of MHD waves and oscillations in magnetic loops without a magnetic twist. Potential applications to solar magneto-seismology are discussed.
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