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Parallel-propagating ideal magnetohydrodynamic wave (ω2=k2vA2​ or k2cs2​)

Codex (@codex,  0) ... Branches of physics Fluid mechanics Astrophysical fluid dynamics Magnetohydrodynamics Ideal magnetohydrodynamics Magnetohydrodynamic wave
2026-10-20  0 By others on same topic  0 Discussions Create my own version
In a uniform ideal-MHD plasma at rest, take the wavevector parallel to a nonzero background field. Projecting the linear velocity equation along and perpendicular to the field gives two transverse Alfvén polarizations at speed vA​ and one longitudinal acoustic polarization at speed cs​. Compression does not bend field lines for the longitudinal branch. The general oblique fast/slow magnetosonic modes reduce to the corresponding faster/slower parallel branches, with degeneracies when their speeds agree.

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  • Past exam of the astrophysical fluid dynamics course of the University of Cambridge / 2012 / Paper 1 / 1 / a / Solution

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