On the storm‐time evolution of relativistic electron phase space density in Earth's outer radiation belt

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Fine structure of large‐amplitude chorus wave packets (2014, background): “The role of whistler mode chorus waves in the dynamics of Earth’s radiation belts has been demonstrated for both losses [e.g., Tsurutani et al., 2009] and local acceleration of relativistic electrons by wave-particle interactions [e.g., Turner et al., 2013].”
Particle Dynamics in the Earth's Radiation Belts: Review of Current Research and Open Questions (2020, background): “This is even more complicated when considering the complex PSD structures that arise during storms (e.g., Turner et al., 2012, 2013).”
Radiation belt electron acceleration by chorus waves during the 17 March 2013 storm (2014, background): “Outer radiation belt electron fluxes are highly variable during geomagnetic storms due to a competition between various loss and acceleration processes [Reeves et al., 2003; Bortnik and Thorne, 2007; Li et al., 2006; Li et al., 2007; Xiao et al., 2009; Thorne, 2010; Turner et al., 2013].”
Evolution and slow decay of an unusual narrow ring of relativistic electrons near L ~ 3.2 following the September 2012 magnetic storm (2013, background): “This rebuilding of the outer belt was most rapid at lower energies and occurred in the region outside the plasmapause over the range of L-shells where chorus emissions were observed to be strong, consistent with local wave acceleration [e.g., Horne and Thorne, 2003; Horne et al., 2005; Turner et al.”