Linear MHD stability of infinitely long coronal flux tubes

DOI10.1007/BF00648384zbMath0661.76041OpenAlexW1983983656MaRDI QIDQ1113754

I. J. D. Craig, A. D. Sneyd

Publication date: 1989

Published in: Astrophysics and Space Science (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/bf00648384

zbMATH Keywords

eigenvaluescoronal loopshelical kink modesTwisted magnetic flux

Mathematics Subject Classification ID

Stability and instability of magnetohydrodynamic and electrohydrodynamic flows (76E25) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30) Ionized gas flow in electromagnetic fields; plasmic flow (76X05)

Related Items (3)

The acceleration of matrix power methods by cyclic variations of the shift parameter ⋮ The kink instability in infinite cylindrical flux tubes: Eigenvalues for power-law twist profiles ⋮ An alternating direction implicit scheme for parabolic systems of partial differential equations

Cites Work

• An energy principle for hydromagnetic stability problems
• Critical conditions for magnetic instabilities in force-free coronal loops
• Magnetostatic equilibria and analogous Euler flows of arbitrarily complex topology. Part 1. Fundamentals

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