Refilling of the slot region between the inner and outer electron radiation belts during geomagnetic storms

TitleRefilling of the slot region between the inner and outer electron radiation belts during geomagnetic storms
Publication TypeJournal Article
Year of Publication2007
AuthorsThorne, RM, Shprits, YY, Meredith, NP, Horne, RB, Li, W, Lyons, LR
JournalJournal of Geophysical Research
Volume112
Date Published06/2007
ISSN0148-0227
KeywordsShock-Induced Transport. Slot Refilling and Formation of New Belts.
Abstract[1] Energetic electrons (≥50 keV) are injected into the slot region (2 < L < 4) between the inner and outer radiation belts during the early recovery phase of geomagnetic storms. Enhanced convection from the plasma sheet can account for the storm-time injection at lower energies but does not explain the rapid appearance of higher-energy electrons (≥150 keV). The effectiveness of either radial diffusion (driven by enhanced ULF waves) or local acceleration (during interactions with enhanced whistler mode chorus emissions), as a potential source for refilling the slot at higher energies, is analyzed for observed conditions during the early recovery phase of the 10 October 1990 storm. We demonstrate that local acceleration, driven by observed chorus emissions, can account for the rapid enhancement in 200–700 keV electrons in the outer slot region near L = 3.3. Radial diffusion is much less effective but may partially contribute to the flux enhancement at lower L. Subsequent outward expansion of the plasmapause during the storm recovery phase effectively terminates local wave acceleration in the slot and prevents acceleration to energies higher than ∼700 keV. A statistical analysis of energetic electron flux enhancements and wave and plasma properties over the entire CRRES mission supports the concept of local wave acceleration as a dominant process for refilling the slot during the main and early recovery phase of storms. For moderate storms, the injection process naturally becomes less effective at energies ≥1 MeV, due to the longer wave acceleration times and additional precipitation loss from scattering by electromagnetic ion cyclotron waves. However, during extreme events when the plasmapause remains compressed for several days, conditions may occur to allow wave acceleration to multi-MeV energies at locations normally associated with the slot.
URLhttp://onlinelibrary.wiley.com/doi/10.1029/2006JA012176/abstract
DOI10.1029/2006JA012176


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