NASA NTRS · 19900035656
The energetic ion substorm injection boundary
Abstract
In this paper, 167 dispersionless energetic ion injections which were observed by AMPTE CCE are identified. The radial and local time distribution of the events as a function of kp is qualitatively similar to that envisioned in the injection boundary model of Mauk and McIlwain (1974). It is argued that particles observed during dispersionless injections are locally energized during the disruption of the cross-tail current sheet. Therefore, the injection boundary is identified as derived from the spatial distribution of dispersionless injections, with the earthward edge of the region of the magnetotail which undergoes current sheet disruption during the substorm expansion phase. It is shown that this qualitative model for the generation of the injection boundary can provide an explanation for the dispersionless nature, the double spiral shape, and the Kp dependence of the boundary.
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Lopez, R. E., Sibeck, D. G., Mcentire, R. W., Krimigis, S. M.. 1990-01-01. The energetic ion substorm injection boundary. https://ntrs.nasa.gov/citations/19900035656
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