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. 2016 Jan 28;121(1):397–412. doi: 10.1002/2015JA021569

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©2015. The Authors.

This is an open access article under the terms of the Creative Commons Attribution‐NonCommercial‐NoDerivs License, which permits use and distribution in any medium, provided the original work is properly cited, the use is non‐commercial and no modifications or adaptations are made.

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HOPE electron fluxes from 1 to 50 keV (<1 keV HOPE data are not considered in this study) and background‐corrected MagEIS data from 50 keV to 4 MeV plotted as a function of energy and L shell. This shows on pass through the radiation belts during quiet times: the inbound leg of RBSP‐A orbit 485 (11:14 to 15:43 UT on 27 February).