Modelling the connection between propagating disturbances and solar spicules

Skirvin, S.J. orcid.org/0000-0002-3814-4232, Samanta, T. orcid.org/0000-0002-9667-6392 and Van Doorsselaere, T. orcid.org/0000-0001-9628-4113 (2024) Modelling the connection between propagating disturbances and solar spicules. Astronomy & Astrophysics, 689. A135. 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: Sun: chromosphere; Sun: corona; Sun: oscillations; solar wind; Sun: transition region
Dates:
  • Published: September 2024
  • Published (online): 6 September 2024
  • Accepted: 18 June 2024
Institution: The University of Sheffield
Academic Units: The University of Sheffield > Faculty of Engineering (Sheffield) > School of Electrical and Electronic Engineering
Depositing User: Symplectic Sheffield
Date Deposited: 10 Oct 2024 15:38
Last Modified: 10 Oct 2024 15:38
Published Version: http://dx.doi.org/10.1051/0004-6361/202450186
Status: Published
Publisher: EDP Sciences
Refereed: Yes
Identification Number: 10.1051/0004-6361/202450186
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