Simulating Radiating and Magnetized Flows in Multiple Dimensions with ZEUS-MP
This paper describes ZEUS-MP, a multiphysics, massively parallel, message-passing implementation of the ZEUS code. ZEUS-MP differs significantly from the thoroughly documented ZEUS-2D code, the completely undocumented (in peer-reviewed literature) ZEUS-3D code, and a marginally documented "vers...
Gespeichert in:
Veröffentlicht in: | The Astrophysical journal. Supplement series 2006-07, Vol.165 (1), p.188-228 |
---|---|
Hauptverfasser: | , , , , , , , |
Format: | Artikel |
Sprache: | eng |
Online-Zugang: | Volltext bestellen |
Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
container_end_page | 228 |
---|---|
container_issue | 1 |
container_start_page | 188 |
container_title | The Astrophysical journal. Supplement series |
container_volume | 165 |
creator | Hayes, John C Norman, Michael L Fiedler, Robert A Bordner, James O Li, Pak Shing Clark, Stephen E ud-Doula, Asif Mac Low, Mordecai-Mark |
description | This paper describes ZEUS-MP, a multiphysics, massively parallel, message-passing implementation of the ZEUS code. ZEUS-MP differs significantly from the thoroughly documented ZEUS-2D code, the completely undocumented (in peer-reviewed literature) ZEUS-3D code, and a marginally documented "version 1" of ZEUS-MP first distributed publicly in 1999. ZEUS-MP offers an MHD algorithm that is better suited for multidimensional flows than the ZEUS-2D module by virtue of modifications to the method of characteristics scheme first suggested by Hawley & Stone. This MHD module is shown to compare quite favorably to the TVD scheme described by Ryu et al. ZEUS-MP is the first publicly available ZEUS code to allow the advection of multiple chemical (or nuclear) species. Radiation hydrodynamic simulations are enabled via an implicit flux-limited radiation diffusion (FLD) module. The hydrodynamic, MHD, and FLD modules can be used, singly or in concert, in one, two, or three space dimensions. In addition, so-called 1.5D and 2.5D grids, in which the "half-D" denotes a symmetry axis along which a constant but nonzero value of velocity or magnetic field is evolved, are supported. Self-gravity can be included either through the assumption of a GM/r potential or through a solution of Poisson's equation using one of three linear solver packages (conjugate gradient, multigrid, and FFT) provided for that purpose. Point-mass potentials are also supported. Because ZEUS-MP is designed for large simulations on parallel computing platforms, considerable attention is paid to the parallel performance characteristics of each module in the code. Strong-scaling tests involving pure hydrodynamics (with and without self-gravity), MHD, and RHD are performed in which large problems (256 super(3) zones) are distributed among as many as 1024 processors of an IBM SP3. Parallel efficiency is a strong function of the amount of communication required between processors in a given algorithm, but all modules are shown to scale well on up to 1024 processors for the chosen fixed problem size. |
doi_str_mv | 10.1086/504594 |
format | Article |
fullrecord | <record><control><sourceid>proquest_O3W</sourceid><recordid>TN_cdi_crossref_primary_10_1086_504594</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>743455915</sourcerecordid><originalsourceid>FETCH-LOGICAL-c379t-bec5dd6fee2117b16496ea911ee9854c0d1b952fb02f759d3209a3e83e9ebce43</originalsourceid><addsrcrecordid>eNp90E9LwzAYx_EgCs6pr6FeFITqkyZpm6PMTYUVxbmLl5A2T2ek_2xahr56NyoKCp6e5_Dhd_gSckzhgkIcXgrgQvIdMqKCxT5nodglI4Aw8gG43CcHzr0CQCSYHJFkYcu-0J2tVt6jNnb4dGW8RK8q7OwHGm9W1Gvn2cpL-qKzTYHetS2xcraunLe23Yv3PF0u_OThkOzlunB49HXHZDmbPk1u_fn9zd3kau5nLJKdn2ImjAlzxIDSKKUhlyFqSSmijAXPwNBUiiBPIcgjIQ0LQGqGMUOJaYacjcnZsNu09VuPrlOldRkWha6w7p2KOONCyE2AMTn9VwbABKPAf2DW1s61mKumtaVu3xUFte2qhq4beD5AWzffZptXbfMqGgpFFY1j1Zh8g0_-4l-DnyESgIA</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>20353104</pqid></control><display><type>article</type><title>Simulating Radiating and Magnetized Flows in Multiple Dimensions with ZEUS-MP</title><source>IOP Publishing Free Content</source><creator>Hayes, John C ; Norman, Michael L ; Fiedler, Robert A ; Bordner, James O ; Li, Pak Shing ; Clark, Stephen E ; ud-Doula, Asif ; Mac Low, Mordecai-Mark</creator><creatorcontrib>Hayes, John C ; Norman, Michael L ; Fiedler, Robert A ; Bordner, James O ; Li, Pak Shing ; Clark, Stephen E ; ud-Doula, Asif ; Mac Low, Mordecai-Mark</creatorcontrib><description>This paper describes ZEUS-MP, a multiphysics, massively parallel, message-passing implementation of the ZEUS code. ZEUS-MP differs significantly from the thoroughly documented ZEUS-2D code, the completely undocumented (in peer-reviewed literature) ZEUS-3D code, and a marginally documented "version 1" of ZEUS-MP first distributed publicly in 1999. ZEUS-MP offers an MHD algorithm that is better suited for multidimensional flows than the ZEUS-2D module by virtue of modifications to the method of characteristics scheme first suggested by Hawley & Stone. This MHD module is shown to compare quite favorably to the TVD scheme described by Ryu et al. ZEUS-MP is the first publicly available ZEUS code to allow the advection of multiple chemical (or nuclear) species. Radiation hydrodynamic simulations are enabled via an implicit flux-limited radiation diffusion (FLD) module. The hydrodynamic, MHD, and FLD modules can be used, singly or in concert, in one, two, or three space dimensions. In addition, so-called 1.5D and 2.5D grids, in which the "half-D" denotes a symmetry axis along which a constant but nonzero value of velocity or magnetic field is evolved, are supported. Self-gravity can be included either through the assumption of a GM/r potential or through a solution of Poisson's equation using one of three linear solver packages (conjugate gradient, multigrid, and FFT) provided for that purpose. Point-mass potentials are also supported. Because ZEUS-MP is designed for large simulations on parallel computing platforms, considerable attention is paid to the parallel performance characteristics of each module in the code. Strong-scaling tests involving pure hydrodynamics (with and without self-gravity), MHD, and RHD are performed in which large problems (256 super(3) zones) are distributed among as many as 1024 processors of an IBM SP3. Parallel efficiency is a strong function of the amount of communication required between processors in a given algorithm, but all modules are shown to scale well on up to 1024 processors for the chosen fixed problem size.</description><identifier>ISSN: 0067-0049</identifier><identifier>EISSN: 1538-4365</identifier><identifier>DOI: 10.1086/504594</identifier><language>eng</language><publisher>IOP Publishing</publisher><ispartof>The Astrophysical journal. Supplement series, 2006-07, Vol.165 (1), p.188-228</ispartof><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c379t-bec5dd6fee2117b16496ea911ee9854c0d1b952fb02f759d3209a3e83e9ebce43</citedby><cites>FETCH-LOGICAL-c379t-bec5dd6fee2117b16496ea911ee9854c0d1b952fb02f759d3209a3e83e9ebce43</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://iopscience.iop.org/article/10.1086/504594/pdf$$EPDF$$P50$$Giop$$H</linktopdf><link.rule.ids>314,778,782,27615,27911,27912,53918</link.rule.ids><linktorsrc>$$Uhttp://iopscience.iop.org/0067-0049/165/1/188$$EView_record_in_IOP_Publishing$$FView_record_in_$$GIOP_Publishing</linktorsrc></links><search><creatorcontrib>Hayes, John C</creatorcontrib><creatorcontrib>Norman, Michael L</creatorcontrib><creatorcontrib>Fiedler, Robert A</creatorcontrib><creatorcontrib>Bordner, James O</creatorcontrib><creatorcontrib>Li, Pak Shing</creatorcontrib><creatorcontrib>Clark, Stephen E</creatorcontrib><creatorcontrib>ud-Doula, Asif</creatorcontrib><creatorcontrib>Mac Low, Mordecai-Mark</creatorcontrib><title>Simulating Radiating and Magnetized Flows in Multiple Dimensions with ZEUS-MP</title><title>The Astrophysical journal. Supplement series</title><description>This paper describes ZEUS-MP, a multiphysics, massively parallel, message-passing implementation of the ZEUS code. ZEUS-MP differs significantly from the thoroughly documented ZEUS-2D code, the completely undocumented (in peer-reviewed literature) ZEUS-3D code, and a marginally documented "version 1" of ZEUS-MP first distributed publicly in 1999. ZEUS-MP offers an MHD algorithm that is better suited for multidimensional flows than the ZEUS-2D module by virtue of modifications to the method of characteristics scheme first suggested by Hawley & Stone. This MHD module is shown to compare quite favorably to the TVD scheme described by Ryu et al. ZEUS-MP is the first publicly available ZEUS code to allow the advection of multiple chemical (or nuclear) species. Radiation hydrodynamic simulations are enabled via an implicit flux-limited radiation diffusion (FLD) module. The hydrodynamic, MHD, and FLD modules can be used, singly or in concert, in one, two, or three space dimensions. In addition, so-called 1.5D and 2.5D grids, in which the "half-D" denotes a symmetry axis along which a constant but nonzero value of velocity or magnetic field is evolved, are supported. Self-gravity can be included either through the assumption of a GM/r potential or through a solution of Poisson's equation using one of three linear solver packages (conjugate gradient, multigrid, and FFT) provided for that purpose. Point-mass potentials are also supported. Because ZEUS-MP is designed for large simulations on parallel computing platforms, considerable attention is paid to the parallel performance characteristics of each module in the code. Strong-scaling tests involving pure hydrodynamics (with and without self-gravity), MHD, and RHD are performed in which large problems (256 super(3) zones) are distributed among as many as 1024 processors of an IBM SP3. Parallel efficiency is a strong function of the amount of communication required between processors in a given algorithm, but all modules are shown to scale well on up to 1024 processors for the chosen fixed problem size.</description><issn>0067-0049</issn><issn>1538-4365</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2006</creationdate><recordtype>article</recordtype><recordid>eNp90E9LwzAYx_EgCs6pr6FeFITqkyZpm6PMTYUVxbmLl5A2T2ek_2xahr56NyoKCp6e5_Dhd_gSckzhgkIcXgrgQvIdMqKCxT5nodglI4Aw8gG43CcHzr0CQCSYHJFkYcu-0J2tVt6jNnb4dGW8RK8q7OwHGm9W1Gvn2cpL-qKzTYHetS2xcraunLe23Yv3PF0u_OThkOzlunB49HXHZDmbPk1u_fn9zd3kau5nLJKdn2ImjAlzxIDSKKUhlyFqSSmijAXPwNBUiiBPIcgjIQ0LQGqGMUOJaYacjcnZsNu09VuPrlOldRkWha6w7p2KOONCyE2AMTn9VwbABKPAf2DW1s61mKumtaVu3xUFte2qhq4beD5AWzffZptXbfMqGgpFFY1j1Zh8g0_-4l-DnyESgIA</recordid><startdate>20060701</startdate><enddate>20060701</enddate><creator>Hayes, John C</creator><creator>Norman, Michael L</creator><creator>Fiedler, Robert A</creator><creator>Bordner, James O</creator><creator>Li, Pak Shing</creator><creator>Clark, Stephen E</creator><creator>ud-Doula, Asif</creator><creator>Mac Low, Mordecai-Mark</creator><general>IOP Publishing</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>KL.</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope></search><sort><creationdate>20060701</creationdate><title>Simulating Radiating and Magnetized Flows in Multiple Dimensions with ZEUS-MP</title><author>Hayes, John C ; Norman, Michael L ; Fiedler, Robert A ; Bordner, James O ; Li, Pak Shing ; Clark, Stephen E ; ud-Doula, Asif ; Mac Low, Mordecai-Mark</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c379t-bec5dd6fee2117b16496ea911ee9854c0d1b952fb02f759d3209a3e83e9ebce43</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2006</creationdate><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Hayes, John C</creatorcontrib><creatorcontrib>Norman, Michael L</creatorcontrib><creatorcontrib>Fiedler, Robert A</creatorcontrib><creatorcontrib>Bordner, James O</creatorcontrib><creatorcontrib>Li, Pak Shing</creatorcontrib><creatorcontrib>Clark, Stephen E</creatorcontrib><creatorcontrib>ud-Doula, Asif</creatorcontrib><creatorcontrib>Mac Low, Mordecai-Mark</creatorcontrib><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>The Astrophysical journal. Supplement series</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Hayes, John C</au><au>Norman, Michael L</au><au>Fiedler, Robert A</au><au>Bordner, James O</au><au>Li, Pak Shing</au><au>Clark, Stephen E</au><au>ud-Doula, Asif</au><au>Mac Low, Mordecai-Mark</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Simulating Radiating and Magnetized Flows in Multiple Dimensions with ZEUS-MP</atitle><jtitle>The Astrophysical journal. Supplement series</jtitle><date>2006-07-01</date><risdate>2006</risdate><volume>165</volume><issue>1</issue><spage>188</spage><epage>228</epage><pages>188-228</pages><issn>0067-0049</issn><eissn>1538-4365</eissn><abstract>This paper describes ZEUS-MP, a multiphysics, massively parallel, message-passing implementation of the ZEUS code. ZEUS-MP differs significantly from the thoroughly documented ZEUS-2D code, the completely undocumented (in peer-reviewed literature) ZEUS-3D code, and a marginally documented "version 1" of ZEUS-MP first distributed publicly in 1999. ZEUS-MP offers an MHD algorithm that is better suited for multidimensional flows than the ZEUS-2D module by virtue of modifications to the method of characteristics scheme first suggested by Hawley & Stone. This MHD module is shown to compare quite favorably to the TVD scheme described by Ryu et al. ZEUS-MP is the first publicly available ZEUS code to allow the advection of multiple chemical (or nuclear) species. Radiation hydrodynamic simulations are enabled via an implicit flux-limited radiation diffusion (FLD) module. The hydrodynamic, MHD, and FLD modules can be used, singly or in concert, in one, two, or three space dimensions. In addition, so-called 1.5D and 2.5D grids, in which the "half-D" denotes a symmetry axis along which a constant but nonzero value of velocity or magnetic field is evolved, are supported. Self-gravity can be included either through the assumption of a GM/r potential or through a solution of Poisson's equation using one of three linear solver packages (conjugate gradient, multigrid, and FFT) provided for that purpose. Point-mass potentials are also supported. Because ZEUS-MP is designed for large simulations on parallel computing platforms, considerable attention is paid to the parallel performance characteristics of each module in the code. Strong-scaling tests involving pure hydrodynamics (with and without self-gravity), MHD, and RHD are performed in which large problems (256 super(3) zones) are distributed among as many as 1024 processors of an IBM SP3. Parallel efficiency is a strong function of the amount of communication required between processors in a given algorithm, but all modules are shown to scale well on up to 1024 processors for the chosen fixed problem size.</abstract><pub>IOP Publishing</pub><doi>10.1086/504594</doi><tpages>41</tpages><oa>free_for_read</oa></addata></record> |
fulltext | fulltext_linktorsrc |
identifier | ISSN: 0067-0049 |
ispartof | The Astrophysical journal. Supplement series, 2006-07, Vol.165 (1), p.188-228 |
issn | 0067-0049 1538-4365 |
language | eng |
recordid | cdi_crossref_primary_10_1086_504594 |
source | IOP Publishing Free Content |
title | Simulating Radiating and Magnetized Flows in Multiple Dimensions with ZEUS-MP |
url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-15T18%3A13%3A47IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_O3W&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Simulating%20Radiating%20and%20Magnetized%20Flows%20in%20Multiple%20Dimensions%20with%20ZEUS-MP&rft.jtitle=The%20Astrophysical%20journal.%20Supplement%20series&rft.au=Hayes,%20John%20C&rft.date=2006-07-01&rft.volume=165&rft.issue=1&rft.spage=188&rft.epage=228&rft.pages=188-228&rft.issn=0067-0049&rft.eissn=1538-4365&rft_id=info:doi/10.1086/504594&rft_dat=%3Cproquest_O3W%3E743455915%3C/proquest_O3W%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=20353104&rft_id=info:pmid/&rfr_iscdi=true |