Driving solar coronal MHD simulations on high-performance computers-Reference-Cited by-同舟云学术

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Driving solar coronal MHD simulations on high-performance computers

Published:2019-07-29 Issue:1-2 Volume:114 Page:235-260
ISSN:0309-1929
Container-title:Geophysical & Astrophysical Fluid Dynamics
language:en
Short-container-title:Geophysical & Astrophysical Fluid Dynamics

Author:

Bourdin Philippe-A.¹^ORCID

Affiliation:

1. Space Research Institute, Austrian Academy of Sciences, Graz, Austria

Publisher

Informa UK Limited

Subject

Geochemistry and Petrology,Mechanics of Materials,Geophysics,Astronomy and Astrophysics,Computational Mechanics

Link

https://www.tandfonline.com/doi/pdf/10.1080/03091929.2019.1643849

Reference35 articles.

1. On the nature of coronal loops above the quiet sun network

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1. Data-driven Simulations of Magnetic Field Evolution in Active Region 11429: Magneto-frictional Method Using PENCIL CODE;Research in Astronomy and Astrophysics;2024-01-31

2. Numerical evidence for a small-scale dynamo approaching solar magnetic Prandtl numbers;Nature Astronomy;2023-05-18

3. Coagulation of inertial particles in supersonic turbulence;Astronomy & Astrophysics;2021-04

4. Dust Growth by Accretion of Molecules in Supersonic Interstellar Turbulence;The Astrophysical Journal;2020-11-01

5. Introduction;Geophysical & Astrophysical Fluid Dynamics;2019-12-13

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