Two-dimensional simulations of beam-driven turbulence in the auroral ionosp
here have shown the formation and instability of phase-space tubes. These t
ubes are a generalization of electron phase-space holes in a one-dimensiona
l plasma. In a strongly magnetized plasma, such tubes vibrate at frequencie
s below the bounce frequency of the trapping potential. A theory for these
vibrations yields quantitative agreement with kinetic simulations. Furtherm
ore, the theory predicts that the vibrations can become unstable when reson
antly coupled to electrostatic whistlers-also in agreement with simulations
.