The latitudinal morphology of 10-eV to 10-keV electron fluxes during magnetically quiet and disturbed times in the 2100-0300 MLT sector
摘要：
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 21000300 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.
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关键词：
Experimental/ atmospheric electron precipitation magnetic storms magnetosphere/ latitudinal morphology electron fluxes auroral particle fluxes substorm time 10 eV to 10 keV Isis satellites 2100 to 0300 magnetic local time period electron precipitation/ A9430 Magnetosphere
DOI：
10.1029/JA080i022p03148
被引量：
年份：
1975
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