4.5 Article

A Census of Plasma Waves and Structures Associated With an Injection Front in the Inner Magnetosphere

Journal

JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS
Volume 123, Issue 4, Pages 2566-2587

Publisher

AMER GEOPHYSICAL UNION
DOI: 10.1002/2017JA025005

Keywords

inner magnetosphere; electron injection; plasma waves; kinetic structures; plasma boundaries; radiation belts

Funding

  1. NASA [NNX17AB81G]
  2. Van Allen Probes team
  3. EFW team
  4. EMFISIS team
  5. ECT team
  6. NASA [NNX17AB81G, 1003777] Funding Source: Federal RePORTER

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Now that observations have conclusively established that the inner magnetosphere is abundantly populated with kinetic electric field structures and nonlinear waves, attention has turned to quantifying the ability of these structures and waves to scatter and accelerate inner magnetospheric plasma populations. A necessary step in that quantification is determining the distribution of observed structure and wave properties (e.g., occurrence rates, amplitudes, and spatial scales). Kinetic structures and nonlinear waves have broadband signatures in frequency space, and consequently, high-resolution time domain electric and magnetic field data are required to uniquely identify such structures and waves as well as determine their properties. However, most high-resolution fields data are collected with a strong bias toward high-amplitude signals in a preselected frequency range, strongly biasing observations of structure and wave properties. In this study, an similar to 45 min unbroken interval of 16,384 samples/s field burst data, encompassing an electron injection event, is examined. This data set enables an unbiased census of the kinetic structures and nonlinear waves driven by this electron injection, as well as determination of their typical properties. It is found that the properties determined using this unbiased burst data are considerably different than those inferred from amplitude-biased burst data, with significant implications for wave-particle interactions due to kinetic structures and nonlinear waves in the inner magnetosphere.

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