Convection with Misaligned Gravity and Rotation: Simulations and Rotating Mixing Length Theory

Currie, L, Barker, A orcid.org/0000-0003-4397-7332, Lithwick, Y et al. (1 more author) (2020) Convection with Misaligned Gravity and Rotation: Simulations and Rotating Mixing Length Theory. Monthly Notices of the Royal Astronomical Society. ISSN 0035-8711

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Copyright, Publisher and Additional Information: This article is protected by copyright. This is an author produced version of a paper accepted for publication in Monthly Notices of the Royal Astronomical Society. Uploaded in accordance with the publisher's self-archiving policy.
Keywords: Convection, hydrodynamics, stars: interiors, stars: rotation, Sun: interior, planets and satellites: interiors
Dates:
  • Accepted: 4 February 2020
  • Published (online): 10 February 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)
Funding Information:
FunderGrant number
Leverhulme TrustECF-2014-216
Science & Technology Facilities Council (STFC)ST/R00059X/1
Science & Technology Facilities Council (STFC)ST/S000275/1
Depositing User: Symplectic Publications
Date Deposited: 11 Feb 2020 12:37
Last Modified: 11 Feb 2020 12:46
Status: Published online
Publisher: Oxford University Press
Identification Number: https://doi.org/10.1093/mnras/staa372

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