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Electron and proton data from Isis 1 and 2 have been used to examine the change in the latitudinal morphology of auroral particle fluxes as a function of substorm time in the 2100–0300 dipole magnetic local time period. Clear and repeatable systematics in the latitudinal morphology were observed during the various phases of a substorm, allowing one to identify the substorm phase based on particle data alone. Based on this study, a new phenomenological substorm model is presented that relates particle precipitation from various parts of the magnetotail to auroral oval morphology.
Winningham et al. (Fri,) studied this question.
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