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Title: Auroral electrodynamics at the cusp/cleft poleward boundary during northward interplanetary magnetic field

Journal Article · · Geophysical Research Letters (American Geophysical Union); (United States)
DOI:https://doi.org/10.1029/91GL00849· OSTI ID:5221360

Combined latitude profiles of optical aurora, magnetic disturbances, particle precipitation and field-aligned currents are used to investigate the electrodynamics of the cusp/cleft ionosphere during northward interplanetary magnetic field. An active zone of strong azimuthal plasma convection, manifested by the Svalgaard-Mansurov effect in ground magnetic deflections and auroral structure at the poleward boundary of the cusp/cleft is observed within {approximately}1,030-1,230 MLT. Contrary to the typical cusp/cleft auroral activity during negative IMF B{sub z} the discrete auroral forms in the present case move into the cusp/cleft arc, from the poleward edge. Both the optical observations and the inferred field-aligned current/plasma flow pattern indicate a generator mechanism poleward of the cusp/cleft, giving rise to strong momentum transfer and discrete electron precipitation within a {approximately}200 km wide latitudinal zone at the cusp/cleft poleward boundary, at the time of a poleward moving cusp/cleft arc. From this and other similar studies of the cusp/cleft ionosphere, the author concludes that a qualitatively similar mode of solar wind-magnetosphere interaction is operating both during northward and southward IMF.

OSTI ID:
5221360
Journal Information:
Geophysical Research Letters (American Geophysical Union); (United States), Vol. 18:5; ISSN 0094-8276
Country of Publication:
United States
Language:
English