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Title: Access of energetic particles to storm time ring current through enhanced radial diffusion

Journal Article · · Journal of Geophysical Research; (USA)
;  [1]
  1. Aerospace Corp., Los Angeles, CA (USA)

Magnetic storms are distinguishable from other periods of geomagnetic activity by the injection of trapped electrons and ions to the 2{approx lt} L {approx lt} 4 region. It has been proposed previously that this injection results from an inward displacement of the preexisting trapped-particle population by enhanced storm time electric fields. However, high-energy ({approx gt} 40 keV) ring-current particles have drift periods that are typically shorter than the time of the main-phase development, and so the direct radial transport of these particles is restricted. The authors propose here that the transport of {approx gt} 40 keV particles into the storm time ring current can result from enhanced stochastic radial transport driven by fluctuating electric fields during a storm's main phase. They estimate the effects of such electric fields by applying radial-diffusion theory, assuming a preexisting trapped-particle population as the initial conditions, and they demonstrate the feasibility of explaining observed flux increases of {approx gt} 40-keV particles at L{approx lt} 4 by enhanced radial diffusion. It is necessary that new particles be injected near the outer boundary of the trapping region so as to maintain the fluxes there as an outer boundary condition, and they estimate that the {approx gt} 40-keV portion of the storm time ring current at L {approximately} 3 consists of about 50% preexisting and about 50% new particles. They thus find that formation of the storm time ring current may be explainable via a combination of direct radial transport at energies {approx lt} 40 keV and diffusive radial transport at higher energies.

OSTI ID:
5831304
Journal Information:
Journal of Geophysical Research; (USA), Vol. 94:A5; ISSN 0148-0227
Country of Publication:
United States
Language:
English