Solar coronal magnetic fields derived using seismology techniques applied to omnipresent sunspot waves

Jess, D.B., Reznikova, V.E., Ryans, R.S.I. et al. (9 more authors) (2016) Solar coronal magnetic fields derived using seismology techniques applied to omnipresent sunspot waves. Nature Physics, 12 (2). pp. 179-185. ISSN 1745-2473

Abstract

Metadata

Authors/Creators:
  • Jess, D.B.
  • Reznikova, V.E.
  • Ryans, R.S.I.
  • Christian, D.J.
  • Keys, P.H.
  • Mathioudakis, M.
  • Mackay, D.H.
  • Krishna Prasad, S.
  • Banerjee, D.
  • Grant, S.D.T.
  • Yau, S.
  • Diamond, C.
Copyright, Publisher and Additional Information: © 2015 Macmillan Publishers
Keywords: Solar physics; Stars
Dates:
  • Published: 2 February 2016
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: 19 Feb 2016 14:26
Last Modified: 19 Feb 2016 14:26
Published Version: https://dx.doi.org/10.1038/nphys3544
Status: Published
Publisher: Nature Publishing Group
Refereed: Yes
Identification Number: https://doi.org/10.1038/nphys3544

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