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. 2024 Aug 8;220(5):59. doi: 10.1007/s11214-024-01089-8

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© The Author(s) 2024

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. 10 — Acquisition sequence of MAJIS during the first flyby of Europa (flyby 7E1). Colours are related to the spatial resolutions achievable by MAJIS in the different observing sections, indicated by the side colour bar. Surface area shaded in dark khaki colour represents Europa’s nightside hemisphere. The observing sections composing the sequence are as follows. a. inbound dayside global scans at low-mid resolution (3–5 km/px). b. inbound dayside regional scans at mid-high res (0.5–3 km/px). c. Pushbroom dayside local scans at very high resolution (0.06–0.5 km/px). d. (1, 2, 3) outbound sequences of limb scans for the exosphere at variable resolution (1–2 km/px for d1, 5–7 km/px for d2, 8–9 km/px for d3). e. outbound nightside global scans for hotspots search at mid resolution (∼3–5 km/px)