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The damping of coronal loop oscillations

Ruderman, M.S. and Roberts, B. (2002) The damping of coronal loop oscillations. Astrophysical Journal, 577 (1). pp. 475-486. ISSN 1538-4365

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Abstract

Motivated by recent Transition Region and Coronal Explorer (TRACE) observations of damped oscillations in coronal loops, we consider analytically the motion of an inhomogeneous coronal magnetic tube of radius a in a zero-beta plasma. An initially perturbed tube may vibrate in its kink mode of oscillation, but those vibrations are damped. The damping is due to resonant absorption, acting in the inhomogeneous regions of the tube, which leads to a transfer of energy from the kink mode to Alfven (azimuthal) oscillations within the inhomogeneous layer. We determine explicitly the decrement gamma (decay time gamma(-1)) for a coronal flux tube whose plasma density varies only in a thin layer of thickness l on the tube boundary. The effect of viscosity is also considered. We show that, in general, the problem involves two distinct timescales, gamma(-1) and omega(k)(-1)R(1/3), where R is the Reynolds number and omega(k) is the frequency of the kink mode. Under coronal conditions (when gamma(-1) << omega(k)(-1) R-1/3), the characteristic damping time of global oscillations is gamma(-1). During this time, most of the energy in the initial perturbation is transferred into a resonant absorption layer of thickness of order l(2)/a, with motions in this layer having an amplitude of order a/l times the initial amplitude. We apply our results to the observations, suggesting that loop oscillations decay principally because of inhomogeneities in the loop. Our theory suggests that only those loops with density inhomogeneities on a small scale (confined to within a thin layer of order agamma/omega(k) in thickness) are able to support coherent oscillations for any length of time and so be observable. Loops with a more gradual density variation, on the scale of the tube radius a, do not exhibit pronounced oscillations.

Item Type: Article
Copyright, Publisher and Additional Information: © 2002 The American Astronomical Society. Reproduced in accordance with the publisher's self-archiving policy.
Keywords: MHD, plasmas, Sun : corona, waves
Academic Units: The University of Sheffield > Faculty of Science (Sheffield) > School of Mathematics and Statistics (Sheffield)
Depositing User: Repository Officer
Date Deposited: 27 Oct 2006
Last Modified: 08 Feb 2013 16:50
Published Version: http://dx.doi.org/10.1086/342130
Status: Published
Publisher: University of Chicago Press
Refereed: Yes
Identification Number: 10.1086/342130
URI: http://eprints.whiterose.ac.uk/id/eprint/1657

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