Physics
Scientific paper
Mar 2004
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004georl..3105804m&link_type=abstract
Geophysical Research Letters, Volume 31, Issue 5, CiteID L05804
Physics
3
Magnetospheric Physics: Plasma Sheet, Magnetospheric Physics: Electric Fields (2411), Magnetospheric Physics: Auroral Phenomena (2407)
Scientific paper
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.
André Martial
Balogh André
Buchert Stephan C.
Dandouras Iannis
David Winningham J.
No associations
LandOfFree
Cluster observations of ULF waves with pulsating electron beams above the high latitude dusk-side auroral region does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Cluster observations of ULF waves with pulsating electron beams above the high latitude dusk-side auroral region, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Cluster observations of ULF waves with pulsating electron beams above the high latitude dusk-side auroral region will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1133875