Magnetohydrodynamics of solar coronal plasmas in cylindrical geometry

DOI10.1006/jcph.1998.5841zbMath0906.76096OpenAlexW2052708262MaRDI QIDQ1387897

Zoran Mikić, Roberto Lionello, Dalton D. Schnack

Publication date: 31 January 1999

Published in: Journal of Computational Physics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1006/jcph.1998.5841

zbMATH Keywords

iterative methodsmomentum equationsemi-implicit schemesolar magnetic fieldskink instabilitysolar coronal heatingtwisted flux tube

Mathematics Subject Classification ID

Finite difference methods applied to problems in fluid mechanics (76M20) Magnetohydrodynamics and electrohydrodynamics (76W05) Planetary atmospheres (85A20) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30)

Related Items (2)

Invariant finite-difference schemes for cylindrical one-dimensional MHD flows with conservation laws preservation ⋮ Stability of algorithms for waves with large flows

Cites Work

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• A pseudospectral algorithm for three-dimensional magnetohydrodynamic simulation
• An alternating direction implicit scheme for parabolic systems of partial differential equations
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• Semi-implicit method for three-dimensional compressible magnetohydrodynamic simulation
• Semi-implicit method for long time scale magnetohydrodynamic computations in three dimensions
• The use of a preconditioned bi-conjugate gradient method for hybrid plasma stability analysis
• A new semi-implicit method for MHD computations
• Semi-implicit magnetohydrodynamic calculations
• Critical conditions for magnetic instabilities in force-free coronal loops

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