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. 2020 Jun 10;11:2942. doi: 10.1038/s41467-020-16660-4

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© The Author(s) 2020

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 license, and indicate if changes were made. The images or other third party material in this article are included in the article’s Creative Commons license, unless indicated otherwise in a credit line to the material. If material is not included in the article’s Creative Commons license 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 license, visit http://creativecommons.org/licenses/by/4.0/.

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Fig. 7 — a Magnetic field observed by MMS4 along the bow shock crossing. b–m Electron distribution functions at the peaks and the corresponding valleys of magnetic fluctuations along the bow shock crossing are plotted. The distributions with the colored borders are the distributions taken at the magnetic peaks at the times denoted by the colored lines in a. The adjacent distributions are taken at the associated valleys denoted by the adjacent dashed lines in a.