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. 2022 Jun 8;606(7915):674–677. doi: 10.1038/s41586-022-04728-8

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© The Author(s) 2022

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. 1 — a, The plot shows EUV brightness distribution (image) in the context of the hand-drawn magnetic field lines outlining closed, post-reconnection loops, cusp region including a so-called Y-point and the vertical plasma sheet. ROI1 and ROI2 used in the analysis are also shown. b, Distribution of the median values of the thermal plasma density, log scale, obtained from the microwave data using MCMC simulations; see Methods. Strong depletion of the thermal number density is apparent inside ROI1.