An analytical model of the Kelvin–Helmholtz instability of transverse coronal loop oscillations

Barbulescu, M. orcid.org/0000-0001-9569-8306, Ruderman, M.S. orcid.org/0000-0003-2324-8466, Doorsselaere, T.V. et al. (1 more author) (2019) An analytical model of the Kelvin–Helmholtz instability of transverse coronal loop oscillations. The Astrophysical Journal, 870 (2). 108. ISSN 0004-637X

Abstract

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Authors/Creators:
Copyright, Publisher and Additional Information: © 2019 The American Astronomical Society. Reproduced in accordance with the publisher's self-archiving policy.
Keywords: instabilities; magnetohydrodynamics (MHD); plasmas; Sun: corona; Sun: magnetic fields; Sun: oscillations
Dates:
  • Accepted: 25 November 2018
  • Published (online): 15 January 2019
  • Published: 10 January 2019
Institution: The University of Sheffield
Academic Units: The University of Sheffield > Faculty of Science (Sheffield) > School of Mathematics and Statistics (Sheffield)
Depositing User: Symplectic Sheffield
Date Deposited: 28 Nov 2019 10:16
Last Modified: 28 Nov 2019 20:50
Status: Published
Publisher: American Astronomical Society
Refereed: Yes
Identification Number: https://doi.org/10.3847/1538-4357/aaf506
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