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. 2023 Sep 20;219(7):53. doi: 10.1007/s11214-023-00996-6

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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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Fig. 19 — (Top) Expected coverage of Jupiter’s disk by MAJIS on 2032-Sep-24, near perijove #12. Different colours present the coverage of four cubes acquired at time intervals of 1 h 10 m. (Bottom) Expected coverage of Jupiter’s auroras by MAJIS on 2032-Sep-25, a few hours after perijove #12. Different colours present the coverage of four cubes acquired at time intervals of 46 m