Exact nonlinear solutions for three-dimensional Alfvén-wave packets in relativistic magnetohydrodynamics

Abstract

We show that large-amplitude, non-planar, Alfvén wave (AW) packets are exact nonlinear solutions of the relativistic MHD equations when the total magnetic-field strength in the local fluid rest frame ($b$) is a constant. We derive analytic expressions relating the components of the fluctuating velocity and magnetic field. We also show that these constant-$b$ AWs propagate without distortion at the relativistic Alfvén velocity and never steepen into shocks. These findings and the observed abundance of large-amplitude, constant-$b$ AWs in the solar wind suggest that such waves may be present in relativistic outflows around compact astrophysical objects.

5 pages

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Cited by in corpus (3)

• New Observations of Solar Wind 1/f Turbulence Spectrum from Parker Solar Probe
• Turbulence and particle acceleration in a relativistic plasma
• Solitary Alfvén Waves