Auroral intensification structure and dynamics in the double oval: Substorm of December 26, 2000

Details Auroral intensification structure and dynamics in the double oval: Substorm of December 26, 2000 Auroral intensification structure and dynamics in the double oval: Substorm of December 26, 2000

Jul 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006ge%26ae..46..450k&link_type=abstract

Geomagnetism and Aeronomy, Volume 46, Issue 4, pp.450-456

Physics

3

Auroral Phenomena In Magnetosphere

Scientific paper

Based on results of the simultaneous TV observations at Barentsburg high-latitude observatory and Lovozero auroral observatory and using the IMAGE auroral luminosity images, the auroral fine structure and dynamics has been studied during the substorm of December 26, 2000, when the auroral luminosity distribution represented a double oval. It has been indicated that the interaction between the processes proceeding in different magnetospheric regions, the projections of which are the poleward and equatorward edges of the double oval, is observed in auroras in the process of substorm development.

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