Field-aligned particle currents near an auroral arc

A Nike-Tomahawk rocket equipped to measure electric and magnetic fields and charged particles from a few ev to several hundred kev energy was flown into an auroral band from Fort Churchill on April 11, 1970. The particle detectors were oriented so as to measure net field-aligned currents. Electrons from a few to several kev were responsible for the auroral luminosity and represented a positive current away from the atmosphere of the order of 5×10−7 amp m−2. Changes in the fluxes of these particles are observed to be the cause of luminosity variations. Enhancements in the transverse electric field magnitude are correlated with auroral motions and increases in the over-all luminosity. The E×B drift imposed on the primary beam can account for auroral motions observed. North of the auroral luminosity, an intense current sheet was measured by the particle detectors. The precipitating electrons responsible for the current sheet had an energy of the order of a few hundred ev and resulted in a field-aligned current about an order of magnitude greater than that produced by the more energetic electrons responsible for the luminosity. The current sheet separated the region of hard spectra magnetically tied to the aurora from that characterized by soft spectra north of the luminosity. The spectrum of particles north of the aurora was very soft, having a shape and intensity similar to that consistently seen in the tail of the magnetosphere by the Vela spacecraft. The implication of this is that perhaps the northern edge of the luminosity is a line of demarcation beyond which field lines commence to thread the plasma sheet. When intense field-aligned currents were observed, the direction of the electric field in the ionosphere pointed westward or southwestward. Outside of the region of luminosity and when the substorm was recovering, the electric field switched to an eastward direction as the magnitude of the field-aligned currents decreased. This correlation appears to be a spatial effect, although it could be interpreted temporally as a characteristic of magnetosphere tail fields during the substorm recovery. A correlation of particle fluxes measured by the rocket detectors and those seen simultaneously at 6.6 RE by the ATS 5 spacecraft is discussed.

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