On the differences in the periodic behavior of magnetic helicity flux in flaring active regions with and without X-class events

Soós, S., Korsós, M.B., Morgan, H. et al. (1 more author) (2022) On the differences in the periodic behavior of magnetic helicity flux in flaring active regions with and without X-class events. Astrophysical Journal, 925 (2). 129. ISSN 0004-637X

Abstract

Metadata

Item Type: Article
Authors/Creators:
  • Soós, S.
  • Korsós, M.B.
  • Morgan, H.
  • Erdélyi, R.
Copyright, Publisher and Additional Information:

© 2022. The Author(s). Published by the American Astronomical Society. Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence (http://creativecommons.org/licenses/by/4.0/). Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.

Keywords: Solar activity; Solar flares; Sunspots; Solar active regions; Solar active region magnetic fields; Space weather
Dates:
  • Published: 1 February 2022
  • Published (online): 1 February 2022
  • Accepted: 14 December 2021
Institution: The University of Sheffield
Academic Units: The University of Sheffield > Faculty of Science (Sheffield) > School of Mathematics and Statistics (Sheffield)
Funding Information:
Funder
Grant number
Science and Technology Facilities Council
ST/M000826/1
The Royal Society
IE161153
Depositing User: Symplectic Sheffield
Date Deposited: 15 Dec 2021 08:09
Last Modified: 22 Feb 2022 16:51
Status: Published
Publisher: American Astronomical Society
Refereed: Yes
Identification Number: 10.3847/1538-4357/ac4094
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Open Archives Initiative ID (OAI ID):

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