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Geophysical & Astrophysical Fluid Dynamics Volume 114, 2020 - Issue 1-2: On the Physics and Algorithms of the Pencil Code
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Articles

Driving solar coronal MHD simulations on high-performance computers

Philippe-A. BourdinSpace Research Institute, Austrian Academy of Sciences, Graz, AustriaCorrespondence[email protected]
ORCID Iconhttps://orcid.org/0000-0002-6793-601X
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Pages 235-260 | Received 30 Aug 2018, Accepted 11 Jul 2019, Published online: 29 Jul 2019

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A. Brandenburg, S. Candelaresi & F. A. Gent. (2020) Introduction. Geophysical & Astrophysical Fluid Dynamics 114:1-2, pages 1-7.
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Articles from other publishers (4)

P. Vemareddy, Jörn Warnecke & Ph. A. Bourdin. (2024) Data-driven Simulations of Magnetic Field Evolution in Active Region 11429: Magneto-frictional Method Using PENCIL CODE. Research in Astronomy and Astrophysics 24:2, pages 025007.
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Jörn Warnecke, Maarit J. Korpi-Lagg, Frederick A. Gent & Matthias Rheinhardt. (2023) Numerical evidence for a small-scale dynamo approaching solar magnetic Prandtl numbers. Nature Astronomy 7:6, pages 662-668.
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Xiang-Yu Li & Lars Mattsson. (2021) Coagulation of inertial particles in supersonic turbulence. Astronomy & Astrophysics 648, pages A52.
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Xiang-Yu 宇 Li 李翔 & Lars Mattsson. (2020) Dust Growth by Accretion of Molecules in Supersonic Interstellar Turbulence. The Astrophysical Journal 903:2, pages 148.
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