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Mirror Instabilities in the Inner Magnetosphere and Their Potential for Localized ULF Wave Generation.

M B Cooper1, A J Gerrard1, L J Lanzerotti1

  • 1Center for Solar-Terrestrial Research New Jersey Institute of Technology Newark NJ USA.

Journal of Geophysical Research. Space Physics
|March 8, 2021
PubMed
Summary
This summary is machine-generated.

NASA Van Allen Probes data reveal mirror/drift-mirror unstable plasma regions in the night-side inner magnetosphere. These findings identify the source of storm time Pc5 ULF waves, suggesting a new generation mechanism.

Keywords:
ULF wavesinner magnetospheremagnetotail injectionsmirror mode unstable plasma

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Area of Science:

  • Space Physics
  • Plasma Physics
  • Magnetospheric Physics

Background:

  • Observations show mirror/drift-mirror (M/D-M) unstable plasma regions in the night-side inner magnetosphere.
  • These regions exist on the kinetic-frozen-in plasma threshold, favoring M/D-M mode formation and ultralow frequency (ULF) wave signatures.

Purpose of the Study:

  • To perform a climatological analysis of plasma anisotropy (gamma) and beta in the inner magnetosphere.
  • To identify the conditions and most likely regions for M/D-M instability.
  • To investigate the source region of storm time Pc5 ULF waves.

Main Methods:

  • Analysis of plasma anisotropy (gamma) and total plasma beta.
  • Application of bi-Maxwellian distribution assumptions to assess instability conditions.
  • Climatological study of M/D-M unstable plasma regions using Van Allen Probes data.

Main Results:

  • A strong preference for M/D-M unstable plasmas was found in the premidnight sector of the night-side magnetosphere.
  • Observed events ranged from half-minute to several-hour durations.
  • The statistical distribution explicitly identifies the source region for storm time Pc5 ULF waves.

Conclusions:

  • The premidnight inner magnetosphere is a key region for M/D-M instability.
  • These findings suggest an alternative generation mechanism for storm time Pc5 ULF waves.
  • The study enhances understanding of magnetospheric plasma dynamics and ULF wave generation.