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Driving solar coronal MHD simulations on high-performance computers
DOI: 10.1080/03091929.2019.1643849 Bibcode: 2020GApFD.114..235B

Bourdin, Philippe-A.

The quality of today's research is often tightly limited to the available computing power and scalability of codes to many processors. For example, tackling the problem of heating the solar corona requires a most realistic description of the plasma dynamics and the magnetic field. Numerically solving such a magneto-hydrodynamical (MHD) description…

2020 Geophysical and Astrophysical Fluid Dynamics
Hinode 8