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BAS-RBM simulations of ultra-relativistic electron acceleration in Earth's radiation belts using a coupled plasma density model
GB/NERC/BAS/PDC/01929

Summary

Abstract:
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.

Keywords:
BAS-RBM, VAP, magnetosphere, plasma density, radiation belts

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Citation

Daggitt, T., Horne, R., Glauert, S., & Del Zanna, G. (2024). BAS-RBM simulations of ultra-relativistic electron acceleration in Earth's radiation belts using a coupled plasma density model (Version 1.0) [Data set]. NERC EDS UK Polar Data Centre. https://doi.org/10.5285/ea37228a-5b4d-4db2-8d97-53fff2c43f3f

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