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Statistics of Whistler‐Mode Waves in the Near‐Earth Plasma Sheet
Journal article   Peer reviewed

Statistics of Whistler‐Mode Waves in the Near‐Earth Plasma Sheet

L. Gao, D. Vainchtein, A. V. Artemyev and X.‐J. Zhang
Journal of geophysical research. Space physics, v 127(8), pn/a
Aug 2022

Abstract

plasma sheet wave‐particle resonances whistler‐mode waves
Electromagnetic whistler‐mode waves are among the wave modes mainly responsible for energetic electron scattering and acceleration in the inner magnetosphere and near‐Earth plasma sheet. Although whistler‐driven electron precipitation significantly contributes to diffuse aurora at large L‐shells of ∼9–13, all existing empirical models of whistler‐mode waves are limited to the inner magnetosphere, at L < 9. This study aims to utilize more than 10 years of Time History of Events and Macroscale Interactions during Substorms observations to investigate main properties of whistler‐mode waves in the near‐Earth plasma sheet. We reveal relations between wave intensity Bw2 $\left({B}_{w}^{2}\right)$ and characteristics of the anisotropic electron population. We showed that in 99% of whistler wave events, the observed Bw2 ${B}_{w}^{2}$, mean wave frequency 〈f〉, and wave spectrum width Δf are consistent with expectations from the quasi‐linear theory of wave‐particle resonant interactions. Based on these statistics, we built an empirical model of Bw2 ${B}_{w}^{2}$, 〈f〉, and Δf as a function of L‐shell and MLT. This model extends existing inner magnetosphere models to a higher L‐shell range. Key Points We have constructed an empirical model of whistler‐mode waves in the quiet near‐Earth plasma sheet 99% of observed waves resonate with electrons in the quasi‐linear regime Whistler wave intensity correlates with the linear growth rate of unstable electrons

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Astronomy & Astrophysics
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