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Specific type of energetic electron\udprecipitation accompanied by a sharp increase in trapped energetic electron flux\udare found in the data obtained from low-altitude NOAA satellites. These strongly\udlocalized variations of the trapped and precipitated energetic electron flux\udhave been observed in the evening sector near the plasmapause during recovery\udphase of magnetic storms. Statistical characteristics of these structures as\udwell as the results of comparison with proton precipitation are described. We\uddemonstrate the spatial coincidence of localized electron precipitation with\udcold plasma gradient and whistler wave intensification measured on board the\udDE-1 and Aureol-3 satellites. A simultaneous localized sharp increase in both\udtrapped and precipitating electron flux could be a result of significant\udpitch-angle isotropization of drifting electrons due to their interaction via\udcyclotron instability with the region of sharp increase in background plasma\uddensity.  <b>Key words.</b> Ionosphere (particle precipitation;\udwave-particle interaction) Magnetospheric Physics (plasmasphere

Strong localized variations of the low-altitude energetic electron fluxes in the evening sector near the plasmapause