Physics
Scientific paper
Jul 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006georl..3313106s&link_type=abstract
Geophysical Research Letters, Volume 33, Issue 13, CiteID L13106
Physics
14
Magnetospheric Physics: Auroral Phenomena (2407), Ionosphere: Wave/Particle Interactions (7867), Magnetospheric Physics: Energetic Particles: Precipitating, Ionosphere: Plasma Waves And Instabilities (2772), Magnetospheric Physics: Magnetosphere/Ionosphere Interactions (2431)
Scientific paper
The two-fluid theory of inertial Alfvén waves predicts that wave energy spreads azimuthally across the background magnetic field, and that phase- and group- velocities in the B$\perp$ plane are oppositely directed. These features have been observed in laboratory plasmas but have yet to be identified in the natural auroral plasma. Using narrow-field video recorded at 50 images/s, we have identified a time dependent morphology that is consistent with these predictions. The aurora at issue is best modeled as an expanding amplitude envelope within which periodic auroral structure evolves. If luminous structure is interpreted as a projection of the parallel wave electric field into the B$\perp$ plane, then successive images reveal the cross-sectional structure of the resonant cone at increasing distance from the wave source. Phase- and group-velocities extracted under this interpretation were found to be consistent with theoretical predictions for a dispersing inertial Alfvén wave packet.
Blixt Erik Mårten
Semeter Joshua
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