The need for new techniques to identify the high-frequency MHD waves of an oscillating coronal loop

Allian, F. orcid.org/0000-0002-4569-0370 and Jain, R. orcid.org/0000-0002-0080-5445 (2021) The need for new techniques to identify the high-frequency MHD waves of an oscillating coronal loop. Astronomy and Astrophysics, 650. A91. ISSN 0004-6361

Abstract

Metadata

Authors/Creators:
Copyright, Publisher and Additional Information: © 2021 ESO. Reproduced in accordance with the publisher's self-archiving policy.
Keywords: Sun: oscillations; Sun: activity; Sun: corona; Sun: flares; Sun: magnetic fields
Dates:
  • Accepted: 1 May 2021
  • Published (online): 11 June 2021
  • Published: June 2021
Institution: The University of Sheffield
Academic Units: The University of Sheffield > Faculty of Science (Sheffield) > School of Mathematics and Statistics (Sheffield)
Funding Information:
FunderGrant number
Science and Technology Facilities Council1949553
Depositing User: Symplectic Sheffield
Date Deposited: 14 Jun 2021 09:31
Last Modified: 14 Jun 2021 09:31
Status: Published
Publisher: EDP Sciences
Refereed: Yes
Identification Number: https://doi.org/10.1051/0004-6361/202039763
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