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High-order magnetohydrodynamics for astrophysics with an adaptive mesh refinement discontinuous Galerkin scheme

Abstract. Modern astrophysical simulations aim to accurately model an ever-growing array of physical processes, including the interaction of fluids with magnet

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Bibliographic Details
Main Authors: Guillet, Thomas (Author) , Pakmor, Rüdiger (Author) , Springel, Volker (Author)
Format: Article (Journal)
Language:English
Published: 2019 January 30
In: Monthly notices of the Royal Astronomical Society
Year: 2019, Volume: 485, Issue: 3, Pages: 4209-4246
ISSN:1365-2966
DOI:10.1093/mnras/stz314
Online Access:Verlag, Volltext: https://doi.org/10.1093/mnras/stz314
Verlag, Volltext: https://academic.oup.com/mnras/article/485/3/4209/5304629
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Author Notes:Thomas Guillet, Rüdiger Pakmor, Volker Springel, Praveen Chandrashekar and Christian Klingenberg
Description
Summary:Abstract. Modern astrophysical simulations aim to accurately model an ever-growing array of physical processes, including the interaction of fluids with magnet
Item Description:Gesehen am 27.05.2019
Physical Description:Online Resource
ISSN:1365-2966
DOI:10.1093/mnras/stz314

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