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. 2023 Jun 14;298(6):78. doi: 10.1007/s11207-023-02170-1

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© The Author(s) 2023

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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Different views of the middle corona, observed on 29 April 2021, in EUV from SUVI (top in 17.1 nm, and middle panel in 19.5 nm) and visible light from K-Cor (bottom left) and LASCO (bottom right; with SUVI superimposed). Images are in camera coordinates and not necessarily co-aligned, although solar North is generally upwards in each frame.