Physics
Scientific paper
Dec 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992itps...20..715s&link_type=abstract
IEEE Transactions on Plasma Science (ISSN 0093-3813), vol. 20, no. 6, p. 715-725.
Physics
Auroral Zones, Kelvin-Helmholtz Instability, Magnetopause, Magnetosphere-Ionosphere Coupling, Solar Terrestrial Interactions, Space Plasmas, Field Aligned Currents, Interplanetary Magnetic Fields, Transient Response
Scientific paper
A specific category of auroral events occurring predominantly during a southward-directed IMF is examined. Coordinated observations from the ground and satellites in polar orbit are used to study the temporal/spatial development of the events in relation to the background patterns of particle precipitation and ionospheric convection as well as the field-aligned current and ion drift characteristics of the individual events. The auroral phenomenon is characterized by a sequence of elongated forms moving laterally into the polar cap after forming near the persistent cusp/cleft arc. It is suggested that the motion pattern is regulated by the IMF orientation. Both prenoon and postnoon sector events are reported.
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