A Coscaling Grid for Athena++. II. Magnetohydrodynamics
We extend the coscaling formalism of Habegger & Heitsch implemented in Athena++ to magnetohydrodynamics. The formalism relies on flow symmetries in astrophysical problems involving expansion, contraction, and center-of-mass motion. The formalism is fully consistent with the upwind constrained tr...
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Language: | English |
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IOP Publishing
2025-01-01
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Series: | The Astrophysical Journal Supplement Series |
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Online Access: | https://doi.org/10.3847/1538-4365/ada289 |
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author | Fabian Heitsch Roark Habegger |
author_facet | Fabian Heitsch Roark Habegger |
author_sort | Fabian Heitsch |
collection | DOAJ |
description | We extend the coscaling formalism of Habegger & Heitsch implemented in Athena++ to magnetohydrodynamics. The formalism relies on flow symmetries in astrophysical problems involving expansion, contraction, and center-of-mass motion. The formalism is fully consistent with the upwind constrained transport method implemented in Athena++ and is accurate to second order in space. Applying our implementation to standard magnetohydrodynamic test cases leads to improved results and higher efficiency, compared to the fixed-grid solutions. |
format | Article |
id | doaj-art-7ca9ecc179614ac6b9ceeaa0ef75c197 |
institution | Kabale University |
issn | 0067-0049 |
language | English |
publishDate | 2025-01-01 |
publisher | IOP Publishing |
record_format | Article |
series | The Astrophysical Journal Supplement Series |
spelling | doaj-art-7ca9ecc179614ac6b9ceeaa0ef75c1972025-01-31T09:19:42ZengIOP PublishingThe Astrophysical Journal Supplement Series0067-00492025-01-0127626110.3847/1538-4365/ada289A Coscaling Grid for Athena++. II. MagnetohydrodynamicsFabian Heitsch0https://orcid.org/0000-0002-4775-039XRoark Habegger1https://orcid.org/0000-0003-4776-940XUniversity of North Carolina at Chapel Hill , Department of Physics and Astronomy, Chapel Hill, NC 27599, USA ; fheitsch@unc.eduUniversity of Wisconsin-Madison , Astronomy Department, Madison, WI 53703, USA ; rhabegger@wisc.eduWe extend the coscaling formalism of Habegger & Heitsch implemented in Athena++ to magnetohydrodynamics. The formalism relies on flow symmetries in astrophysical problems involving expansion, contraction, and center-of-mass motion. The formalism is fully consistent with the upwind constrained transport method implemented in Athena++ and is accurate to second order in space. Applying our implementation to standard magnetohydrodynamic test cases leads to improved results and higher efficiency, compared to the fixed-grid solutions.https://doi.org/10.3847/1538-4365/ada289Computational methodsMagnetohydrodynamical simulationsAstronomical simulations |
spellingShingle | Fabian Heitsch Roark Habegger A Coscaling Grid for Athena++. II. Magnetohydrodynamics The Astrophysical Journal Supplement Series Computational methods Magnetohydrodynamical simulations Astronomical simulations |
title | A Coscaling Grid for Athena++. II. Magnetohydrodynamics |
title_full | A Coscaling Grid for Athena++. II. Magnetohydrodynamics |
title_fullStr | A Coscaling Grid for Athena++. II. Magnetohydrodynamics |
title_full_unstemmed | A Coscaling Grid for Athena++. II. Magnetohydrodynamics |
title_short | A Coscaling Grid for Athena++. II. Magnetohydrodynamics |
title_sort | coscaling grid for athena ii magnetohydrodynamics |
topic | Computational methods Magnetohydrodynamical simulations Astronomical simulations |
url | https://doi.org/10.3847/1538-4365/ada289 |
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