4.7 Article

Van Allen Probes observation of localized drift resonance between poloidal mode ultra-low frequency waves and 60 keV electrons

Journal

GEOPHYSICAL RESEARCH LETTERS
Volume 40, Issue 17, Pages 4491-4497

Publisher

AMER GEOPHYSICAL UNION
DOI: 10.1002/grl.50901

Keywords

drift-resonance; ultra-low frequency; radiation belt electron; radial diffusion; inner magnetosphere

Funding

  1. JHU/APL [967399, 921647]
  2. NASA' [NAS5-01072]
  3. NASA [NNX10AK93G]
  4. Canadian Space Agency
  5. Monitoring, Analyzing and Assessing Radiation Belt Loss and Energization (MAARBLE) consortium
  6. European Community [284520]
  7. Canadian NSERC
  8. NASA [NNX10AK93G, 130412] Funding Source: Federal RePORTER

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We present NASA Van Allen Probes observations of wave-particle interactions between magnetospheric ultra-low frequency (ULF) waves and energetic electrons (20-500 keV) on 31 October 2012. The ULF waves are identified as the fundamental poloidal mode oscillation and are excited following an interplanetary shock impact on the magnetosphere. Large amplitude modulations in energetic electron flux are observed at the same period (approximate to 3 min) as the ULF waves and are consistent with a drift-resonant interaction. The azimuthal mode number of the interacting wave is estimated from the electron measurements to be similar to 40, based on an assumed symmetric drift resonance. The drift-resonant interaction is observed to be localized and occur over 5-6 wave cycles, demonstrating peak electron flux modulations at energies similar to 60 keV. Our observation clearly shows electron drift resonance with the fundamental poloidal mode, the energy dependence of the amplitude and phase of the electron flux modulations providing strong evidence for such an interaction. Significantly, the observation highlights the importance of localized wave-particle interactions for understanding energetic particle dynamics in the inner magnetosphere, through the intermediary of ULF waves.

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