MacTaggart, David, Elsheikh, Abdulaziz, McLaughlin, James and Simitev, Radostin (2013) Non-symmetric magnetohydrostatic equilibria: a multigrid approach. Astronomy & Astrophysics, 556. A40. ISSN 0004-6361
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Abstract
Aims: Linear magnetohydrostatic (MHS) models of solar magnetic fields balance plasma pressure gradients, gravity and Lorentz forces where the current density is composed of a linear force-free component and a cross-field component that depends on gravitational stratification. In this paper, we investigate an efficient numerical procedure for calculating such equilibria.
Methods: The MHS equations are reduced to two scalar elliptic equations – one on the lower boundary and the other within the interior of the computational domain. The normal component of the magnetic field is prescribed on the lower boundary and a multigrid method is applied on both this boundary and within the domain to find the poloidal scalar potential. Once solved to a desired accuracy, the magnetic field, plasma pressure and density are found using a finite difference method.
Results: We investigate the effects of the cross-field currents on the linear MHS equilibria. Force-free and non-force-free examples are given to demonstrate the numerical scheme and an analysis of speed-up due to parallelization on a graphics processing unit (GPU) is presented. It is shown that speed-ups of ×30 are readily achievable.
Item Type: | Article |
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Additional Information: | magnetic fields, magnetohydrodynamics (MHD), methods: numerical |
Subjects: | F300 Physics F500 Astronomy F800 Physical and Terrestrial Geographical and Environmental Sciences G100 Mathematics |
Department: | Faculties > Engineering and Environment > Mathematics, Physics and Electrical Engineering |
Depositing User: | Prof James McLaughlin |
Date Deposited: | 04 Oct 2013 08:09 |
Last Modified: | 17 Dec 2023 14:36 |
URI: | https://nrl.northumbria.ac.uk/id/eprint/13792 |
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