Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
519474 | Journal of Computational Physics | 2011 | 19 Pages |
Abstract
A finite volume numerical technique is proposed to solve the compressible ideal MHD equations for steady and unsteady problems based on a quasi-Newton implicit time integration strategy. The solenoidal constraint is handled by a hyperbolic divergence cleaning approach allowing its satisfaction up to machine accuracy. The conservation of the magnetic flux is computed in a consistent way using the numerical flux of the finite volume discretization. For the unsteady problem, the time accuracy is obtained by a Newton subiteration at each physical timestep thereby converging the solenoidal constraint to steady state. We perform extensive numerical experiments to validate and demonstrate the capabilities of the proposed numerical technique.
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Authors
M.S. Yalim, D. Vanden Abeele, A. Lani, T. Quintino, H. Deconinck,