Abstract
Multidimensional upwind residual distribution schemes for the numerical solution of the ideal magnetohydrodynamics equations have been extended to three spatial dimensions. The schemes operate on unstructured grids composed of tetrahedra. Both the two and the three dimensional schemes have been implemented into a multipurpose parallel implicit solver. The code is used to investigate a complex interacting shock structure, involving intermediate shock segments appearing in a bow shock flow in space physics.
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