Plasma injection at synchronous orbit and spatial and temporal auroral morphology

Details Plasma injection at synchronous orbit and spatial and temporal auroral morphology Plasma injection at synchronous orbit and spatial and temporal auroral morphology

Jun 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976jgr....81.2805e&link_type=abstract

Journal of Geophysical Research, vol. 81, June 1, 1976, p. 2805-2824. Research supported by the Lockheed Independent Research P

Physics

8

Ats 5, Auroral Spectroscopy, Ground Stations, Plasma Layers, Satellite-Borne Instruments, Synchronous Satellites, Geomagnetic Tail, Magnetically Trapped Particles, Nocturnal Variations, Photometry, Plasma-Particle Interactions

Scientific paper

Analysis of ATS 5 particle spectrograms and simultaneous meridian-scanning photometer data obtained at the base of the ATS field line has revealed systematic relationships between temporal and spatial auroral morphology and particle-injection events. The details of these relationships depend on previous injection events, the local time of the observatory with respect to current-injection events, and the extent and magnitude of current injections. A persistent zone of weak aurora is related to steady plasma-sheet drizzle, and the equatorward edge of this aurora delineates field lines threading the inner edge of the plasma sheet. Auroras associated with injection events superimpose on this preexisting pattern, with the lowest latitude of new precipitation depending on local time. In general, plasma energization is not required between the equatorial plane and the ionosphere to account for observed auroral intensities. The data indicate occasional occurrence of enhanced loss-cone fluxes, suggesting low-altitude field-aligned acceleration. A summary figure shows how various characteristic auroral-precipitation regions are related to the shape, extent, and orientation of the substorm injection boundary and to the subsequent drift paths of injected plasma.

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