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. 2019 Apr 10;124(4):2588–2602. doi: 10.1029/2018JA026259

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©2019. The Authors.

This is an open access article under the terms of the http://creativecommons.org/licenses/by-nc-nd/4.0/ 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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(a–d) Spin‐averaged fluxes of electrons with energies of 1.8, 2.6, 4.2, and 6.3 MeV from 1 February to 1 May 2013, using data from both Van Allen Probes. (e–h) One‐hour solar wind speed, IMF B, IMF B _z, and VB _z during the same period. RBSP = Radiation Belt Storm Probes; REPT = Relativistic Electron‐Proton Telescope.