The latitudinal morphology of 10-eV to 10-keV electron fluxes during magnetically quiet and disturbed times in the 2100-0300 MLT sector

Mathematics – Logic

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Auroral Zones, Electron Precipitation, Latitude, Polar Substorms, Proton Precipitation, Time Dependence, Electron Flux Density, Geomagnetism, Magnetic Disturbances, Spatial Distribution, Spectrograms, Universal Time

Scientific paper

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 dipole magnetic local time period from 2100 to 0300. Clear and repeatable systematics in the latitudinal morphology were observed during the various phases of a substorm, allowing the substorm phase to be identified on the basis of particle data alone. Based on this study, a new phenomenological substorm model is presented which relates particle precipitation from various parts of the magnetotail to auroral oval morphology.

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