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. 2021 Oct 28;217(8):80. doi: 10.1007/s11214-021-00855-2

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© The Author(s) 2021

Open Access This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons licence, and indicate if changes were made. The images or other third party material in this article are included in the article’s Creative Commons licence, unless indicated otherwise in a credit line to the material. If material is not included in the article’s Creative Commons licence and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this licence, visit http://creativecommons.org/licenses/by/4.0/.

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Fig. 11 — Comparison of the main rate (MR) and high-rate (HR) data products from the LOW-A unit. (a) Raw angular distributions (in local pitch angle, $α_{L}$ ) obtained over one full spacecraft spin ( $\sim 11 sec$ ) for $\sim 33 keV$ (left) and $\sim 54 keV$ electrons (right). (b) & (c) The same $\sim 11 sec$ of data but now plotted versus time, for $\sim 33 keV$ and $\sim 54 keV$ , respectively