BAS-RBM simulations of ultra-relativistic electron acceleration in Earth's radiation belts using a coupled plasma density model

The data set contains electron flux measurements from the Van Allen Probes A and B satellites, from the REPT, MagEIS and HOPE instruments for the period 2014-10-18 to 2014-10-28, a set of BAS-RBM simulations covering the same time period, and plasma density dependent chorus diffusion coefficients used to drive the BAS-RBM. The output of a coupled-density model is also included. When coupled with the density model, the density dependent chorus diffusion coefficients improve the BAS-RBM reproduction of ultra-relativistic electron acceleration. Funding: This material is based upon work supported by the Air Force Office of Scientific Research under award number FA9550-19-1-7039. Richard Horne and Sarah Glauert were also supported by the Natural Environment Research Council (NERC) grant NE/V00249X/1 (Sat-Risk) and National and Public Good activity grant NE/R016445/1. Giulio Del Zanna acknowledges support from STFC (UK) via the consolidated grant to the astrophysics group at DAMTP, University of Cambridge (ST/T000481/1). Jay Albert acknowledges support from NASA Grant No. 80NSSC20K1270.