Modeling radiation belt electron dynamics during GEM challenge intervals with the DREAM3D diffusion model

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Particle Dynamics in the Earth's Radiation Belts: Review of Current Research and Open Questions (2020, background): “D codes (Camporeale et al., 2013a, 2013b; Cunningham, 2016; Cunningham et al., 2018; Tu et al., 2013), the Commissariat à l'Energie Atomique (CEA) CEVA code (Réveillé, 1997; Ripoll & Mourenas, 2012; Ripoll, Chen, et al., 2014, Ripoll, Reeves, et al., 2016, Ripoll et al., 2017, 2019), and the STEERB…”
The Challenge of Machine Learning in Space Weather: Nowcasting and Forecasting (2019, methodology): “For instance, diffusion coefficients in radiation belt quasi-linear models are often parameterized in terms of Kp (see, e.g., Tu et al., 2013).”
Event‐specific chorus wave and electron seed population models in DREAM3D using the Van Allen Probes (2014, methodology): “In our previous work [Tu et al., 2013] and the run in Figure 1d, the electron seed population, or low-energy boundary at Emin = 100 keV, is first set by the initial condition.”