Geostatsionaarse orbiidi läheduses täheldatud elektronivoog kujutab endast voo järsu vähenemise ja suurenemise mustrit, mis tekib siis, kui geomagnetiline väli taastub pärast päikese aktiivsuse häirimist.
The electron flux observed in the vicinity of a geostationary orbit presents a pattern of sudden decrease and increase in the flux, which occurs when the geomagnetic field is restored after being disturbed by solar activity.
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