Night-side radiation belt electron precipitation bursts are common during storms, have exponential spectra with E0 around 100 keV, and likely result from ducted whistler-mode waves.
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Night-Side Relativistic Electron Precipitation Bursts in the Outer Radiation Belt: Insights from ELFIN and THEMIS
Night-side radiation belt electron precipitation bursts are common during storms, have exponential spectra with E0 around 100 keV, and likely result from ducted whistler-mode waves.