Radiation belt electron acceleration by chorus waves during the 17 March 2013 storm

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Electron losses from the radiation belts caused by EMIC waves (2014, result): “We note that our results are less sensitive to the choice of the upper cutoff due to the fact that the peak helium band frequency determined here is lower than that used in Li et al. [2014] and hence further from the helium ion cyclotron frequency.”
Particle Dynamics in the Earth's Radiation Belts: Review of Current Research and Open Questions (2020, methodology): “D diffusion code (e.g., Tao et al., 2011; Li et al., 2014; Li, Ma, et al., 2016; Ma et al., 2015, 2016, 2016, Ma et al., 2017 that incorporates the (UCLA) Full Diffusion Code (e.g., Ni et al., 2008, Ni et al., 2011; Shprits & Ni, 2009) in order to compute diffusion coefficients (similarly to VERB 3‐”
Space Weather Effects in the Earth’s Radiation Belts (2018, background): “The driving of magnetospheric processes by the solar wind has also been shown to be critical in radiation belt electron dynamics (e.g., Baker et al. 1990; Reeves 1998; Reeves et al. 2003; Li et al. 2009; Zhao and Li 2013; Jaynes et al. 2015).”