Magnetohydrodynamic simulation of coronal magnetic fields

DOI10.1016/0010-4655(90)90153-RzbMath0875.76679OpenAlexW2045070434MaRDI QIDQ1366161

G. Van Hoven, D. C. Barnes, Zoran Mikić, Dalton D. Schnack

Publication date: 11 November 1997

Published in: Computer Physics Communications (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1016/0010-4655(90)90153-r

zbMATH Keywords

supercomputersforce-free equilibrianonlinear magnetohydrodynamic systems

Mathematics Subject Classification ID

Magnetohydrodynamics and electrohydrodynamics (76W05)

Cites Work

• Unnamed Item
• An implicit algorithm for compressible three-dimensional magnetohydrodynamic calculations
• Semi-implicit method for three-dimensional compressible magnetohydrodynamic simulation
• Semi-implicit method for long time scale magnetohydrodynamic computations in three dimensions
• Semi-implicit magnetohydrodynamic calculations
• Force free fields and coronal heating part I. The formation of current sheets
• The energetics of steady—state flows in the solar corona

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