Characterising Jupiter's dynamo radius using its magnetic energy spectrum

Tsang, Y-K and Jones, CA orcid.org/0000-0002-1105-3920 (2020) Characterising Jupiter's dynamo radius using its magnetic energy spectrum. Earth and Planetary Science Letters, 530. 115879. ISSN 0012-821X

Abstract

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Authors/Creators:
Copyright, Publisher and Additional Information: Crown Copyright © 2019 Published by Elsevier B.V. This is an open access article under the CC BY license (http://creativecommons.org/licenses/by/4.0/).
Keywords: Jupiter; dynamo region; anelastic convection; magnetic energy spectrum; Lowes–Mauersberger spectrum
Dates:
  • Accepted: 2 October 2019
  • Published (online): 22 October 2019
  • Published: January 2020
Institution: The University of Leeds
Academic Units: The University of Leeds > Faculty of Engineering & Physical Sciences (Leeds) > School of Mathematics (Leeds) > Applied Mathematics (Leeds)
Depositing User: Symplectic Publications
Date Deposited: 22 Jul 2020 12:13
Last Modified: 22 Jul 2020 12:13
Status: Published
Publisher: Elsevier
Identification Number: https://doi.org/10.1016/j.epsl.2019.115879
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