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NASA NTRS · 19910069094

Dayside auroral particle acceleration mechanisms derived from Dynamics Explorer data

Abstract

The characteristics of dayside electron acceleration regions, or inverted V's, and the nature of the field-aligned currents flowing in their vicinity are studied by using data from Dynamics Explorer hot-plasma and magnetic-field instruments. It is shown that dayside inverted-V events are common features of the mid-altitude extension of the boundary layer, which lies equatorward of the cusp. Upward-accelerated ionospheric electron beams are found to be carriers of downward region-1 currents even in regions of downward electron acceleration. It is not clear, however, how the upward-accelerated cold electron beams can exist above an apparent upward parallel electric field, since such a potential different would tend to confine the cold ionospheric electrons to low altitudes.

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BibTeXRIS

Burch, J. L., Menietti, J. D., Slavin, J. A.. 1990-01-01. Dayside auroral particle acceleration mechanisms derived from Dynamics Explorer data. https://ntrs.nasa.gov/citations/19910069094

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