Physics
Scientific paper
Dec 2011
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011agufmsm33a2139k&link_type=abstract
American Geophysical Union, Fall Meeting 2011, abstract #SM33A-2139
Physics
[2704] Magnetospheric Physics / Auroral Phenomena, [2721] Magnetospheric Physics / Field-Aligned Currents And Current Systems
Scientific paper
We present CHAMP observations of intense transverse magnetic field fluctuations (10-20 nT amplitude) at frequencies of 1-15 Hz as the satellite crosses visible auroral arcs seen by the THEMIS ground-based camera array. Fluctuations in this frequency range are caused by small-scale FACs and they are consistent with published observations of auroral flicker observed both by ground-based cameras and in-situ. While the THEMIS cameras are not able to resolve the flicker itself, they allow us to associate the magnetic oscillations observed in-situ with strong, northward expanding, multiple auroral arcs. In two cases, the oscillations occur within quasi-static upward FAC channels tens of km wide and with amplitudes of 2-5 μ A/m2. In a third example, the magnetic fluctuations detected by CHAMP show no low-frequency component, indicating no quasi-static ("DC") upward FAC associated with the arc. In fact CHAMP detects a strong downward current within or near the arc, suggesting that all of the visible emission observed by the cameras is due entirely to oscillating fields with no static component. An additional new aspect of these magnetic observations is the presence of strong harmonics at multiples of the ˜3 Hz fundamental oscillation.
Donovan Eric
Kabirzadeh R.
Knudsen David J.
Lühr Hermann
Spanswick E. L.
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