Magnetopause ripples going against the flow form azimuthally stationary surface waves
M. O. Archer, M. D. Hartinger, F. Plaschke, D. J. Southwood, L., Rastaetter

TL;DR
This study reveals that certain magnetopause surface waves are stationary and propagate against the flow, challenging the traditional view of tailward wave propagation, with implications for space weather dynamics.
Contribution
It demonstrates through observations, simulations, and theory that impulsively-excited magnetopause surface waves can be stationary and oppose the flow, contrary to previous assumptions.
Findings
Waves are stationary and oppose flow outside the boundary.
Poynting flux balances flow advection, leading to no net energy flux.
Waves seed fluctuations that grow via Kelvin-Helmholtz instability.
Abstract
Surface waves process the turbulent disturbances which drive dynamics in many space, astrophysical and laboratory plasma systems, with the outer boundary of Earth's magnetosphere, the magnetopause, providing an accessible environment to study them. Like waves on water, magnetopause surface waves are thought to travel in the direction of the driving solar wind, hence a paradigm in global magnetospheric dynamics of tailward propagation has been well-established. Here we show through multi-spacecraft observations, global simulations, and analytic theory that the lowest-frequency impulsively-excited magnetopause surface waves, with standing structure along the terrestrial magnetic field, propagate against the flow outside the boundary. Across a wide local time range (09-15h) the waves' Poynting flux exactly balances the flow's advective effect, leading to no net energy flux and thus…
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