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Van Allen Probes observations of prompt MeV radiation belt electron acceleration in nonlinear interactions with VLF chorus

J. C. FosterHaystack Observatory Massachusetts Institute of Technology Westford Massachusetts USAP. J. EricksonHaystack Observatory Massachusetts Institute of Technology Westford Massachusetts USAYoshiharu OmuraResearch Institute for Sustainable Humanosphere Kyoto University Kyoto JapanD. N. BakerLaboratory for Atmospheric and Space Physics University of Colorado, Boulder Boulder Colorado USAC. A. KletzingDepartment of Physics and Astronomy University of Iowa Iowa City Iowa USAS. G. ClaudepierreAerospace Corporation Los Angeles California USA
2016en
ABI

Аннотация

Abstract Prompt recovery of MeV (millions of electron Volts) electron populations in the poststorm core of the outer terrestrial radiation belt involves local acceleration of a seed population of energetic electrons in interactions with VLF chorus waves. Electron interactions during the generation of VLF rising tones are strongly nonlinear, such that a fraction of the relativistic electrons at resonant energies are trapped by waves, leading to significant nonadiabatic energy exchange. Through detailed examination of VLF chorus and electron fluxes observed by Van Allen Probes, we investigate the efficiency of nonlinear processes for acceleration of electrons to MeV energies. We find through subpacket analysis of chorus waveforms that electrons with initial energy of hundreds of keV to 3 MeV can be accelerated by 50 keV–200 keV in resonant interactions with a single VLF rising tone on a time scale of 10–100 ms.

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