Cluster observations of ULF waves with pulsating electron beams above the high latitude dusk-side auroral region
Winningham, J. D.; Balogh, A.; Dandouras, I.; Wahlund, J. -E.; Lavraud, B.; Fazakerley, A. N.; André, M.; Rème, H.; Morooka, M.; Buchert, S. C.; Igenbergs, K.
Abstract
We report observations by the four Cluster satellites of particle acceleration associated with ULF (Alfvén) waves at an altitude of 6RE above the dusk-side auroral region. All satellites observed upward accelerated ions and upgoing electron beams, which coincided with the upward field-aligned current around the plasmasheet boundary region. Here we study in detail one region of Alfvénic ULF waves observed together with upward electron beams, both having a quasi-periodicity of about 2 minutes. The ULF waves have a downward Poynting flux. Comparing data from different spacecraft, the observed electron beams are likely caused by the ULF waves in localized (0.5° latitude extension) flux tubes in the plasmasheet boundary region. The high-energy keV plasmasheet dispersive ion signatures showed similar periodicity, which suggests that the generation region of the ULF Alfvén waves is near the magnetospheric flank, and in turn induce time-varying particle energization.