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NASA NTRS · 19890049333

Polar cap deflation during magnetospheric substorms

Abstract

The expanding/contracting polar cap model has been used to simulate DE-2 ion drift data during substorms as determined using the AL index. Of the 39 cases modeled, 57 percent required the opening of a nightside gap which maps to where reconnection occurs in the tail; 75 percent of the 16 recovery phase cases required a nightside gap, while only 29 percent of the 17 expansion phase cases required a nightside gap. On the basis of this result, it is concluded that if a nightside gap implies tail reconnection, then reconnection probably occurs after expansion phase onset and continues throughout most of the recovery phase of a substorm.

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BibTeXRIS

Moses, J. J., Siscoe, G. L., Heelis, R. A., Winningham, J. D.. 1989-04-01. Polar cap deflation during magnetospheric substorms. https://ntrs.nasa.gov/citations/19890049333

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