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Effective drag in rotating, poorly conducting plasma turbulence

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Benavides, Santiago J., Burns, Keaton J., Gallet, Basile and Flierl, Glenn R. (2022) Effective drag in rotating, poorly conducting plasma turbulence. The Astrophysical Journal, 938 (2). 92. doi:10.3847/1538-4357/ac9137 ISSN 1538-4357.

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Official URL: https://doi.org/10.3847/1538-4357/ac9137

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Abstract

Despite the increasing sophistication of numerical models of hot Jupiter atmospheres, the large timescale separation required in simulating the wide range in electrical conductivity between the dayside and nightside has made it difficult to run fully consistent magnetohydrodynamic (MHD) models. This has led to many studies that resort to drag parameterizations of MHD. In this study, we revisit the question of the Lorentz force as an effective drag by running a series of direct numerical simulations of a weakly rotating, poorly conducting flow in the presence of a misaligned, strong background magnetic field. We find that the drag parameterization fails once the timescale associated with the Lorentz force becomes shorter than the dynamical timescale in the system, beyond which the effective drag coefficient remains roughly constant, despite orders-of-magnitude variation in the Lorentz (magnetic) timescale. We offer an improvement to the drag parameterization by considering the relevant asymptotic limit of low conductivity and strong background magnetic field, known as the quasi-static MHD approximation of the Lorentz force. This approximation removes the fast timescale associated with magnetic diffusion, but retains a more complex version of the Lorentz force, which could be utilized in future numerical models of hot Jupiter atmospheric circulation.

Item Type: Journal Article
Subjects: Q Science > QB Astronomy
Q Science > QC Physics
Divisions: Faculty of Science, Engineering and Medicine > Science > Mathematics
SWORD Depositor: Library Publications Router
Library of Congress Subject Headings (LCSH): Extrasolar planets -- Atmopsheres, Astrophysics, Fluid Dynamics, Magnetohydrodynamics
Journal or Publication Title: The Astrophysical Journal
Publisher: The American Astronomical Society
ISSN: 1538-4357
Official Date: 20 October 2022
Dates:
DateEvent
20 October 2022Published
17 October 2022Available
10 September 2022Accepted
Volume: 938
Number: 2
Number of Pages: 8
Article Number: 92
DOI: 10.3847/1538-4357/ac9137
Status: Peer Reviewed
Publication Status: Published
Access rights to Published version: Open Access (Creative Commons)
Date of first compliant deposit: 8 November 2022
Date of first compliant Open Access: 8 November 2022
RIOXX Funder/Project Grant:
Project/Grant IDRIOXX Funder NameFunder ID
80NSSC20K1367[NASA] National Aeronautics and Space Administrationhttp://dx.doi.org/10.13039/100000104

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