Structure and evolution of the solar coronal magnetic field

DOI10.1080/03091920701495320zbMath1505.85002OpenAlexW2023110963MaRDI QIDQ5060763

Tahar Amari, J. J. Aly

Publication date: 11 January 2023

Published in: Geophysical & Astrophysical Fluid Dynamics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1080/03091920701495320

zbMATH Keywords

numerical simulationsmagnetohydrodynamicssolar coronaforce-free magnetic fieldseruptive events

Mathematics Subject Classification ID

Magnetohydrodynamics and electrohydrodynamics (76W05) Galactic and stellar structure (85A15) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30)

Cites Work

• Unnamed Item
• Quasi-static evolution of a force-free magnetic field
• On the existence of force-free magnetic fields with small nonconstant \(\alpha\) in exterior domains
• Well posed reconstruction of the solar coronal magnetic field
• A uniqueness result for a simple force-free magnetic field submitted to a topological constraint
• Equilibrium and observational properties of line-tied twisted flux tubes
• A Preconditioned Semi-Implicit Method for Magnetohydrodynamics Equations
• An Iterative Method for Solving Non-Linear Hydromagnetic Equations
• Transport of Magnetic Fields on the Sun.
• On the existence of force‐free magnetic fields
• On the existence of non-linear force-free fields in three-dimensional domains

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