Alfvén‐Fast Wave Coupling in a 2D Nonuniform Medium

Abstract A 2D Cartesian simulation is presented and used to solve the ideal, low‐beta, linear magnetohydrodynamics equations. A simulation is used to investigate the propagation of Alfvén waves through inhomogeneities in Alfvén speed and density. In particular, the loss of Alfvén wave energy through...

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Main Authors: R. Davies, A. N. Wright
Format: Article
Language:English
Published: American Geophysical Union (AGU) 2023-10-01
Series:Earth and Space Science
Subjects:
Online Access:https://doi.org/10.1029/2023EA003167
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author R. Davies
A. N. Wright
author_facet R. Davies
A. N. Wright
author_sort R. Davies
collection DOAJ
description Abstract A 2D Cartesian simulation is presented and used to solve the ideal, low‐beta, linear magnetohydrodynamics equations. A simulation is used to investigate the propagation of Alfvén waves through inhomogeneities in Alfvén speed and density. In particular, the loss of Alfvén wave energy through coupling to the fast wave, and also the form of the Alfvén wave as it emerges from the inhomogeneous region is studied. Potential applications of this include the magnetospheres of both Jupiter and the Earth. The results show that Alfvén waves can be significantly distorted by a nonuniformity and still propagate through the region efficiently, with relatively small amounts of Alfvén wave energy lost through mode conversion and reflection.
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spelling doaj.art-7efd6a088dd74dca9f9af6e0693db3c72023-10-27T17:48:33ZengAmerican Geophysical Union (AGU)Earth and Space Science2333-50842023-10-011010n/an/a10.1029/2023EA003167Alfvén‐Fast Wave Coupling in a 2D Nonuniform MediumR. Davies0A. N. Wright1School of Mathematics and Statistics University of St Andrews St Andrews UKSchool of Mathematics and Statistics University of St Andrews St Andrews UKAbstract A 2D Cartesian simulation is presented and used to solve the ideal, low‐beta, linear magnetohydrodynamics equations. A simulation is used to investigate the propagation of Alfvén waves through inhomogeneities in Alfvén speed and density. In particular, the loss of Alfvén wave energy through coupling to the fast wave, and also the form of the Alfvén wave as it emerges from the inhomogeneous region is studied. Potential applications of this include the magnetospheres of both Jupiter and the Earth. The results show that Alfvén waves can be significantly distorted by a nonuniformity and still propagate through the region efficiently, with relatively small amounts of Alfvén wave energy lost through mode conversion and reflection.https://doi.org/10.1029/2023EA003167magnetohydrodynamicswave mode couplingAlfven wavesmagnetospheric physics
spellingShingle R. Davies
A. N. Wright
Alfvén‐Fast Wave Coupling in a 2D Nonuniform Medium
Earth and Space Science
magnetohydrodynamics
wave mode coupling
Alfven waves
magnetospheric physics
title Alfvén‐Fast Wave Coupling in a 2D Nonuniform Medium
title_full Alfvén‐Fast Wave Coupling in a 2D Nonuniform Medium
title_fullStr Alfvén‐Fast Wave Coupling in a 2D Nonuniform Medium
title_full_unstemmed Alfvén‐Fast Wave Coupling in a 2D Nonuniform Medium
title_short Alfvén‐Fast Wave Coupling in a 2D Nonuniform Medium
title_sort alfven fast wave coupling in a 2d nonuniform medium
topic magnetohydrodynamics
wave mode coupling
Alfven waves
magnetospheric physics
url https://doi.org/10.1029/2023EA003167
work_keys_str_mv AT rdavies alfvenfastwavecouplingina2dnonuniformmedium
AT anwright alfvenfastwavecouplingina2dnonuniformmedium