Radial expansion of the magnetohydrodynamic equations for axially symmetric configurations

DOI10.1080/03091928908218530zbMath0687.76110OpenAlexW2053294249MaRDI QIDQ4206521

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Publication date: 1989

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

Full work available at URL: https://doi.org/10.1080/03091928908218530

zbMATH Keywords

boundary conditionsmagnetohydrodynamic equationsaxially symmetric, time-dependent problemsexpanded magnetofluid equationsmagnetic field concentrations in stellar atmospheres

Mathematics Subject Classification ID

Magnetohydrodynamics and electrohydrodynamics (76W05) Galactic and stellar structure (85A15) Geodesy, mapping problems (86A30) Ionized gas flow in electromagnetic fields; plasmic flow (76X05)

Related Items (1)

Shock wave propagation in a magnetic flux tube

Cites Work

• Unnamed Item
• Instability of a thin magnetic tube in the solar atmosphere
• Solitary waves in a magnetic flux tube
• Nonlinear flows along magnetic flux tubes: Mathematical structure and exact simple wave solutions
• The structure of untwisted magnetic flux tubes

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