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A pressure‐based method with AUSM‐type fluxes for MHD flows at arbitrary Mach numbers
Author(s) -
Xisto C.M.,
Páscoa J.C.,
Oliveira P.J.
Publication year - 2013
Publication title -
international journal for numerical methods in fluids
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.938
H-Index - 112
eISSN - 1097-0363
pISSN - 0271-2091
DOI - 10.1002/fld.3781
Subject(s) - magnetohydrodynamics , euler equations , mach number , classification of discontinuities , euler's formula , shock (circulatory) , supersonic speed , physics , riemann problem , mathematics , classical mechanics , mathematical analysis , mechanics , riemann hypothesis , magnetic field , medicine , quantum mechanics
SUMMARY In this paper, we propose an extension of a PISO method, previously developed to solve the Euler equations, and which is here extended to the ideal magnetohydrodynamic (MHD) equations. By following a pressure‐based approach, we make use of the flexibility given by pressure equation for calculating flows at arbitrary Mach numbers. To handle MHD discontinuities, we have adapted the MHD‐Advection Upstream Splitting Method for our pressure‐based formulation. With the purpose of validation, four sets of test cases are presented and discussed. We start with the circularly polarized Alfvén waves that serves as a smooth flow validation. The second case is the 1‐D Riemann problem that is calculated using both 1‐D and 2‐D formulation of the MHD equations. The third and fourth problems are the Orszag–Tang vortex and the supersonic low‐ β cylinder allowing validation of the method in complex 2‐D MHD shock interaction. Copyright © 2013 John Wiley & Sons, Ltd.