Physics
Scientific paper
Dec 2002
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002agufmsm21b0541l&link_type=abstract
American Geophysical Union, Fall Meeting 2002, abstract #SM21B-0541
Physics
2409 Current Systems (2708), 2431 Ionosphere/Magnetosphere Interactions (2736), 2455 Particle Precipitation, 2471 Plasma Waves And Instabilities, 2475 Polar Cap Ionosphere
Scientific paper
Where currents are carried by a plasma, these currents tend to be bursty and to focus into discrete channels, often with a filamented structure. This situation is very common in nature and in the laboratory. Here we present evidence of bursty and filamentary structures in the terrestrial aurora, observed through the enhancements of radar echoes produced by plasma instability in the filaments. By recording the raw time series from the radar directly, we have resolved the time development of the observed phenomena and we find significant variations on sub-second time scales. Using an interferometric technique to attain sub-beam spatial resolution, we have estimated the horizontal scale size of the structures, and find it to be comparable to the smallest known scale size of optical aurora, which despite extensive theoretical attempts remain little understood (e.g., Borovsky, JGR 98, 6101-6138, 1993). Enhanced radar echoes of this type have been observed previously at several Incoherent Scattering Radar observatories. One of the suggested explanations would enhance only one shoulder. Hence, temporal or spatial averaging of short-lived or spatially small structure was hypothesized to explain simultaneous enhancement of both shoulders. Our time/space resolved observations let us test this
hypothesis with the result that time averaging is ruled out, whereas the enhancement of both shoulders appears to occur in the same volume.
Blixt M.
Brekke Asgeir
Grydeland Tom
Hagfors Tor
La Hoz Cesar
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