Wright, A. N. and Elsden, T. (2020) Simulations of MHD wave propagation and coupling in a 3‐D magnetosphere. Journal of Geophysical Research: Space Physics, 125(2), 027589. (doi: 10.1029/2019ja027589)
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Abstract
A novel simulation grid is devised that is optimized for studying magnetohydrodynamic (MHD) wave coupling and phase mixing in a dipole-like magnetic field. The model also includes flaring on the dawn and dusk flanks. The location of the magnetopause is quite general. In particular, it does not have to coincide with a coordinate surface. Simulations indicate the central role of global fast waveguide modes. These switch from being azimuthally standing in nature at noon, to propagating antisunward on the flanks. The field line resonances (FLRs) seen in the simulation results are three dimensional and not strictly azimuthally polarized. When a plume is present, the FLRs cross a range of 2 in urn:x-wiley:jgra:media:jgra55535:jgra55535-math-0001 shell, and have a polarization that is midway between toroidal and poloidal.
Item Type: | Articles |
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Additional Information: | A. N. W. was partially funded by STFC(ST/N000609/1) and the LeverhulmeTrust (RPG-2016-071). T. E. wasfunded by the Leverhulme Trust(RPG-2016-071) and a LeverhulmeTrust Early Career Fellowship(ECF-2019-155). |
Status: | Published |
Refereed: | Yes |
Glasgow Author(s) Enlighten ID: | Elsden, Dr Thomas |
Authors: | Wright, A. N., and Elsden, T. |
College/School: | College of Science and Engineering > School of Mathematics and Statistics > Mathematics |
Journal Name: | Journal of Geophysical Research: Space Physics |
Publisher: | Wiley |
ISSN: | 2169-9380 |
ISSN (Online): | 2169-9402 |
Published Online: | 06 February 2020 |
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