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. 2019 Feb 4;124(2):934–951. doi: 10.1029/2018JA026349

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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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jgra54747-fig-0005 — Same format as Figure 3 but for 1.01‐MeV electrons from pixel 0 on the HIGH unit (HIGH‐P0). We draw attention to the middle panel (CORR‐STD), where a newly formed inner belt appears following the June 2015 storm, as detailed in Claudepierre et al. (2017). The inner belt structure is highlighted with a red polygon, which is also shown for comparison in the bottom panel, where the alternative background correction algorithm is used in the inner zone. It is clear that the alternative correction algorithm is able to resolve the 1‐MeV inner electron belt with much greater accuracy than is obtained with the standard algorithm.