AZEuS: An Adaptive Zone Eulerian Scheme for Computational MHD

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dc.creator Ramsey, Jon P.
dc.creator Clarke, David C.
dc.creator Men'Shchikov, Alexander B.
dc.date.accessioned 2024-09-11T14:46:43Z
dc.date.available 2024-09-11T14:46:43Z
dc.date.issued 2012-03
dc.identifier.issn 2331-8422
dc.identifier.uri https://dx.doi.org/10.1088/0067-0049/199/1/13
dc.identifier.uri http://library2.smu.ca/xmlui/handle/01/32006
dc.description Published version en_CA
dc.description.abstract A new adaptive mesh refinement (AMR) version of the ZEUS-3D astrophysical magnetohydrodynamical (MHD) fluid code, AZEuS, is described. The AMR module in AZEuS has been completely adapted to the staggered mesh that characterises the ZEUS family of codes, on which scalar quantities are zone-centred and vector components are face-centred. In addition, for applications using static grids, it is necessary to use higher-order interpolations for prolongation to minimise the errors caused by waves crossing from a grid of one resolution to another. Finally, solutions to test problems in 1-, 2-, and 3-dimensions in both Cartesian and spherical coordinates are presented. en_CA
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dc.description.provenance Made available in DSpace on 2024-09-11T14:46:43Z (GMT). No. of bitstreams: 1 Ramsey_Jon_P._2012.pdf: 2459471 bytes, checksum: 69573c6a97143b078614517f5e8b1264 (MD5) Previous issue date: 2012-03 en
dc.language.iso en en_CA
dc.publisher Cornell University Library, arXiv.org en_CA
dc.title AZEuS: An Adaptive Zone Eulerian Scheme for Computational MHD en_CA
dc.type Text en_CA
dcterms.bibliographicCitation The Astrophysical Journal Supplement Series, 199 (13). (2012) en_CA
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