AZEuS: an adaptive zone Eulerian scheme for computational magnetohydrodynamics
A new adaptive mesh refinement (AMR) version of the ZEUS-3D astrophysical magnetohydrodynamical fluid code, AZEuS , is described. The AMR module in AZEuS has been completely adapted to the staggered mesh that characterizes the ZEUS family of codes on which scalar quantities are zone-centered and vec...
Gespeichert in:
| Hauptverfasser: | , , |
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
2012 February 29
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| In: |
The astrophysical journal. Supplement series
Year: 2012, Jahrgang: 199, Heft: 1 |
| ISSN: | 1538-4365 |
| DOI: | 10.1088/0067-0049/199/1/13 |
| Online-Zugang: | Verlag, Volltext: http://dx.doi.org/10.1088/0067-0049/199/1/13 Verlag, Volltext: http://stacks.iop.org/0067-0049/199/i=1/a=13 
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| Verfasserangaben: | Jon P. Ramsey, David A. Clarke, Alexander B. Men'shchikov |
MARC
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| 520 | |a A new adaptive mesh refinement (AMR) version of the ZEUS-3D astrophysical magnetohydrodynamical fluid code, AZEuS , is described. The AMR module in AZEuS has been completely adapted to the staggered mesh that characterizes the ZEUS family of codes on which scalar quantities are zone-centered and vector components are face-centered. In addition, for applications using static grids, it is necessary to use higher-order interpolations for prolongation to minimize the errors caused by waves crossing from a grid of one resolution to another. Finally, solutions to test problems in one, two, and three dimensions in both Cartesian and spherical coordinates are presented. | ||
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