1998
DOI: 10.1016/s1364-6826(98)00003-0
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Pulsations of precipitating energetic electrons: ACTIVE satellite data

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“…High temporal resolution allowed with using SPE-1 to observe the high frequency energetic electron (~20 to ~300 keV) pulsations in middle latitudes, in subauroral and auroral regions and to identify differences at different pitch angles close to the equatorial loss cone. While strong, short time and/or small scale size pulsations of energetic electrons in different energy ranges in 20-300 keV within the loss cone have been observed during the recovery phase of a substorm in the morningside auroral and subauroral regions, simultaneous measurements outside the local loss cone did not exhibit such structure [4]. The dependence of durations of the spikes on L as well as relations to VLF emissions were found.…”
Section: Earlier Activities Spe-1 On Activementioning
confidence: 80%
“…High temporal resolution allowed with using SPE-1 to observe the high frequency energetic electron (~20 to ~300 keV) pulsations in middle latitudes, in subauroral and auroral regions and to identify differences at different pitch angles close to the equatorial loss cone. While strong, short time and/or small scale size pulsations of energetic electrons in different energy ranges in 20-300 keV within the loss cone have been observed during the recovery phase of a substorm in the morningside auroral and subauroral regions, simultaneous measurements outside the local loss cone did not exhibit such structure [4]. The dependence of durations of the spikes on L as well as relations to VLF emissions were found.…”
Section: Earlier Activities Spe-1 On Activementioning
confidence: 80%