A novel approach to identify resonant MHD wave modes in solar pores and sunspot umbrae : B  −  ω analysis

Stangalini, M., Jess, D.B., Verth, G. et al. (12 more authors) (2021) A novel approach to identify resonant MHD wave modes in solar pores and sunspot umbrae : B  −  ω analysis. Astronomy and Astrophysics, 649. A169. ISSN 0004-6361

Abstract

Metadata

Authors/Creators:
  • Stangalini, M.
  • Jess, D.B.
  • Verth, G.
  • Fedun, V. ORCID logo https://orcid.org/0000-0002-0893-7346
  • Fleck, B.
  • Jafarzadeh, S.
  • Keys, P.H.
  • Murabito, M.
  • Calchetti, D.
  • Aldhafeeri, A.A.
  • Berrilli, F.
  • Moro, D.D.
  • Jefferies, S.M.
  • Terradas, J.
  • Soler, R.
Copyright, Publisher and Additional Information: © 2021 ESO. This is an author-produced version of a paper subsequently published in Astronomy and Astrophysics. Uploaded in accordance with the publisher's self-archiving policy.
Keywords: Sun: atmosphere; Sun: oscillations; Sun: magnetic fields; Sun: photosphere
Dates:
  • Accepted: 9 March 2021
  • Published (online): 2 June 2021
  • Published: 2 June 2021
Institution: The University of Sheffield
Academic Units: The University of Sheffield > Faculty of Engineering (Sheffield) > Department of Automatic Control and Systems Engineering (Sheffield)
The University of Sheffield > Faculty of Science (Sheffield) > School of Mathematics and Statistics (Sheffield)
Depositing User: Symplectic Sheffield
Date Deposited: 24 May 2021 13:54
Last Modified: 07 Jun 2021 07:18
Status: Published
Publisher: EDP Sciences
Refereed: Yes
Identification Number: https://doi.org/10.1051/0004-6361/202140429
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