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Title: Radial transport of radiation belt electrons in kinetic field-line resonances

Journal Article · · Geophysical Research Letters
DOI:https://doi.org/10.1002/2017GL074587· OSTI ID:1402654

A representative case study from the Van Allen Probes during a geomagnetic storm recovery phase reveals enhanced electron fluxes at intermediate pitch angles over energies from ~100 keV to 5 MeV coincident with broadband low-frequency electromagnetic waves. The statistical properties of these waves are used to build a model for radial diffusion via drift-bounce resonances in kinetic Alfvén eigenmodes/kinetic field-line resonances. Estimated diffusion coefficients indicate timescales for radial transport on the order of hours in storm time events at energies from <100 keV to MeVs over equatorial pitch angles from the edge of the loss cone to nearly perpendicular to the geomagnetic field. In conclusion, the correlation of kinetic resonances with electron depletions and enhancements during storm main phase and recovery, and the rapid diffusion these waves drive, suggests that they may modulate the outer radiation belt.

Research Organization:
Los Alamos National Laboratory (LANL), Los Alamos, NM (United States)
Sponsoring Organization:
National Aeronautics and Space Administration (NASA); USDOE
Grant/Contract Number:
AC52-06NA25396
OSTI ID:
1402654
Report Number(s):
LA-UR-17-28035; TRN: US1702889
Journal Information:
Geophysical Research Letters, Vol. 44, Issue 16; ISSN 0094-8276
Publisher:
American Geophysical UnionCopyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 16 works
Citation information provided by
Web of Science

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Cited By (3)

A Census of Plasma Waves and Structures Associated With an Injection Front in the Inner Magnetosphere: BOUNDARY WAVE CASE STUDY journal April 2018
Earth's Van Allen Radiation Belts: From Discovery to the Van Allen Probes Era journal November 2019
Impact of Significant Time‐Integrated Geomagnetic Activity on 2‐MeV Electron Flux journal June 2019

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