Linear Alfvén wave equations
ID: linear-alfven-wave-equations
Take a static uniform fluid of mass density , constant gas pressure, and background magnetic field with . Use SI units, vacuum permeability , zero electrical resistivity and zero viscosity. Write and , with both disturbances perpendicular to . Retain only linear order in their amplitudes. There is no background fluid flow, so the linear material derivative is .
The continuity equation has , hence ; choosing no initial mass density fluctuation gives . For this shear mode the gas pressure fluctuation is also zero. In the ideal magnetohydrodynamic momentum equation, the Lorentz force density can be writtenBecause , the perturbed magnetic pressure starts at quadratic order. The surviving transverse magnetic tension gives the first equation below. Expanding the ideal magnetohydrodynamic induction equation gives the second:Differentiate the first in time and substitute the second. Both velocity and magnetic field disturbances obey the one-dimensional wave equation:For a plane wave proportional to , this gives , or . The magnetic and velocity amplitudes satisfy : they have opposite signs for propagation along and equal signs for propagation along . The general uniform-background shear polarization of waves, perpendicular to both and , gives the same dispersion relation with . Its group velocity is , whereas its phase velocity normal to an oblique wavefront has magnitude .
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