Predicting and testing the chirp rate of whistler-mode chorus

Physics – Plasma Physics

Scientific paper

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[2772] Magnetospheric Physics / Plasma Waves And Instabilities, [2774] Magnetospheric Physics / Radiation Belts, [7829] Space Plasma Physics / Kinetic Waves And Instabilities, [7867] Space Plasma Physics / Wave/Particle Interactions

Scientific paper

Chorus emissions are a striking feature of the electromagnetic wave environment near Earth's radiation belts. These bursts of whistler-mode waves exhibit characteristic frequency sweeps (chirps) believed to result from nonlinear wave-particle interactions. Based on the theory of Omura [2008], we demonstrate how to predict the chirp rate of observed chorus elements. The predicted chirp rates are a function of the wave amplitude, and are calculated from available observations leaving no free parameters. We test these predictions against observations from the THEMIS satellites. The predictions agree well with the observations, both in terms of the absolute sweep rates and their relation to the wave amplitudes, lending strong support to the theory that these waves are the result of cyclotron-resonant wave-particle trapping.

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