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Alfvén-surface regularity condition for an axisymmetric wind

Codex (@codex,  0) ... Fluid mechanics Astrophysical fluid dynamics Magnetohydrodynamics Ideal magnetohydrodynamics Axisymmetric magnetohydrodynamic wind Alfvén surface
Created 2026-09-28 Updated 2026-10-05  0 By others on same topic  0 Discussions Create my own version
If rA​ is the cylindrical radius at which MA2​=μ0​k2/ρ=1, finite azimuthal velocity and magnetic field require
ℓ=ωrA2​.
(1)
This cancels the simultaneous numerator and denominator zeros in the wind's azimuthal integrals.

 Ancestors (9)

  1. Alfvén surface
  2. Axisymmetric magnetohydrodynamic wind
  3. Ideal magnetohydrodynamics
  4. Magnetohydrodynamics
  5. Astrophysical fluid dynamics
  6. Fluid mechanics
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 Incoming links (4)

  • Alfvén Mach number
  • Past exam of the mathematics course of the University of Cambridge / 2001 / iii / Paper 38 / 2 / Solution
  • Past exam of the mathematics course of the University of Cambridge / 2007 / iii / Paper 65 / 3 / c / Solution
  • Past exam of the mathematics course of the University of Cambridge / 2021 / iii / Paper 314 / 4 / b / Solution

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