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Area of Science:

  • Space Physics
  • Atmospheric Science
  • Plasma Physics

Background:

  • Auroral substorms are dynamic upper-atmosphere phenomena driven by solar wind energy release from the magnetosphere.
  • Pulsating aurorae are characterized by quasiperiodic, blinking patches caused by precipitating energetic electrons.
  • The interaction between magnetospheric electrons and whistler-mode chorus waves is a hypothesized cause of this precipitation.

Purpose of the Study:

  • To provide direct observational evidence of energetic electron scattering by chorus waves.
  • To confirm the mechanism responsible for generating pulsating aurorae.

Main Methods:

  • Observations using a magnetospheric spacecraft equipped with electron sensors and electromagnetic field instruments in March 2017.
  • Analysis of quasiperiodic precipitating electron flux.
  • Simultaneous observation by a ground auroral imager.

Main Results:

  • Directly observed energetic electrons being scattered by chorus waves.
  • Measured precipitating electron flux intense enough to generate pulsating aurora.
  • Confirmed simultaneous observation of pulsating aurora from the ground.

Conclusions:

  • The study provides the first direct observational evidence linking chorus waves to energetic electron precipitation and pulsating aurora.
  • This finding validates a crucial mechanism in space physics responsible for auroral phenomena.