Trans-sonic cusped shaped, periodic waves and solitary waves of the electrostatic ion-cyclotron type

J. F. Mckenzie (1, 2, 3) , T. B. Doyle (2)

1 MPS - Max-Planck-Institut für Sonnensystemforschung = Max Planck Institute for Solar System Research
2 School of Physics & School of Mathematical and Statistical Sciences
3 Department of Physics

By adopting an essentially fluid dynamic viewpoint we derive the wave structure equation for stationary, fully nonlinear, electrostatic, ion-cyclotron waves. The existence of two fundamental constants of the motion, namely, conservation of momentum flux parallel to the ambient magnetic field, and energy flux parallel to the direction of wave propagation, enables the wave structure equation to be reduced to a first order differential equation, which has solutions that are physically transparent. The analysis shows that sufficiently oblique waves, propagating at sub-ion acoustic speeds, form soliton pulse-like solutions whose amplitudes are greatest for perpendicular propagation. Waves that propagate supersonically have periodic cnoidal waveforms, which are asymmetric about the compressive and rarefactive phases of the wave. It is also shown that there exist critical driver fields for which the end point of the compressive phase goes sonic (in the wave frame), with the consequence that the wave form develops a cusp. It is possible that this trans-sonic, choked flow feature provides a mechanism for the "spiky" waveforms observed in auroral electric field measurements.

Domaines: Cosmologie et astrophysique extra-galactique [astro-ph.CO]; Astrophysique [astro-ph]; Sciences de la Terre

J. F. Mckenzie, T. B. Doyle. Trans-sonic cusped shaped, periodic waves and solitary waves of the electrostatic ion-cyclotron type. Nonlinear Processes in Geophysics, 2004, 11 (4), pp.421-425. ⟨hal-00302361⟩