Calculation of Path-integrated Growth of Whistler-mode Chorus Waves With the HOTRAY Code Based on CRRES Observation

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2483 Wave/Particle Interactions (7867), 2716 Energetic Particles: Precipitating, 2730 Magnetosphere: Inner, 2753 Numerical Modeling, 2774 Radiation Belts

Scientific paper

Whistler-mode chorus waves are excited in the low-density region outside the plasmapause by the injection of plasmasheet electrons into the inner magnetosphere. During substorm injection, electron anisotropy increases as electrons move from the plasmasheet to lower L shells conserving the first adiabatic invariant. On the other hand, electron scattering by chorus waves reduces the electron anisotropy. We fit 5 minute-averaged CRRES data of the electron phase space density (PSD) at different equatorial pitch-angles for various energy channels (between 0.1 keV and 20 keV) with an analytical distribution function to calculate the hot electron density and anisotropy. The path-integrated growth of chorus waves is simulated with the HOTRAY code by tracing chorus waves in a hot magnetized plasma. The results show that substorm-injected electrons are responsible for the intensification of the whistler-mode chorus and higher electron anisotropy than that obtained from the 5 minute- averaged electron PSD data is needed to reproduce the observed wave intensity by CRRES during a substorm injection event. We also suggest that the electron anisotropy is reduced due to pitch-angle scattering by the enhanced chorus waves within the 5 minutes interval over which the CRRES data are analyzed.

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