Dynamics of the Earth's Radiation Belts and Inner Magnetosphere

By C. Schultz. 2013

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Gradual diffusion and punctuated phase space density enhancements of highly relativistic electrons: Van Allen Probes observations (2014, background): “These particle populations wax and wane in absolute flux on a wide range of timescales having both to do with internal magnetospheric physical processes and with external driving effects imposed by the solar wind [e.g., Baker and Blake, 2012].”
Space Weather Effects in the Earth’s Radiation Belts (2018, background): “From the first realization that the terrestrial magnetic field could “trap” high-energy particles, we have come today to a much more sophisticated understanding of what are appropriately often dubbed the “Van Allen Radiation Zones” (see Summers et al. 2012).”
The Challenge of Machine Learning in Space Weather: Nowcasting and Forecasting (2019, unknown): “10.1029/2018SW002061 Camporeale, 2015; Reeves et al., 2013; Ukhorskiy & Sitnov, 2012).”
Source and seed populations for relativistic electrons: Their roles in radiation belt changes (2015, background): “These seed electrons can be pumped up in energy by large factors on characteristic time scales of minutes to hours [Summers et al., 2002; Horne et al., 2005; Thorne et al., 2013b; Summers et al., 2012].”