The effect of data-driving and relaxation models on magnetic flux rope evolution and stability

Wagner, A. orcid.org/0000-0002-5349-6308, Price, D.J. orcid.org/0000-0002-8065-2847, Bourgeois, S. orcid.org/0000-0002-3776-7024 et al. (7 more authors) (2024) The effect of data-driving and relaxation models on magnetic flux rope evolution and stability. Astronomy & Astrophysics, 692. A74. ISSN 0004-6361

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Item Type: Article
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© 2024 The Authors. This is an Open Access article distributed under the terms of the Creative Commons Attribution Licence (https://creativecommons.org/licenses/by/4.0/), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.

Keywords: magnetohydrodynamics (MHD); methods: data analysis; Sun: corona; Sun: coronal mass ejections (CMEs); Sun: magnetic fields
Dates:
  • Published: December 2024
  • Published (online): 2 December 2024
  • Accepted: 22 October 2024
Institution: The University of Sheffield
Academic Units: The University of Sheffield > Faculty of Science (Sheffield) > School of Mathematical and Physical Sciences
Depositing User: Symplectic Sheffield
Date Deposited: 02 Jan 2025 10:47
Last Modified: 02 Jan 2025 10:47
Published Version: https://doi.org/10.1051/0004-6361/202450577
Status: Published
Publisher: EDP Sciences
Refereed: Yes
Identification Number: 10.1051/0004-6361/202450577
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