Physics
Scientific paper
Jul 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988p%26ss...36..715s&link_type=abstract
Planetary and Space Science (ISSN 0032-0633), vol. 36, July 1988, p. 715-723, 725-732.
Physics
10
Atmospheric Electricity, Atmospheric Models, Auroral Arcs, Current Sheets, Magnetic Storms, Temporal Resolution, Atmospheric Boundary Layer, Auroral Zones, Eiscat Radar System (Europe), Kelvin-Helmholtz Instability
Scientific paper
Observations of auroral disturbances such as westward-traveling surges, omega bands, and auroral folds are by necessity usually made when the luminous features have acquired their characteristic geometry; i.e., after the actual formation process. An event in which the initial brightening of an arc develops into a series of auroral spirals and finally into a westward-traveling surge is demonstrated. Two intervals of spiral formation were observed, but only the second of these generated a surgelike feature. Since the surge formation occurred on a time-scale of a few seconds, this type of observation can only be made with high-time-resolution imaging devices. The auroral developments took place in the zenith above Kiruna, where they were recorded by ground-based monochromatic imagers. The subsequent poleward expansion of the activity was observed by the EISCAT incoherent scatter radar 200 km to the north of the initial activation. These observations are discussed in the light of existing substorm theories, and it is proposed that the instability responsible for the final break-up of the arc is self-destructive.
Collis P. N.
Steen Å.
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