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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. 21 — Jupiter limb spectra in the 600 GHz (top) and 1200 GHz (bottom) bands probed by SWI, with the main observable molecular lines. Spectra are computed at the limb for a tangential height of 200 km above the 1-bar level and are convolved by the instrument beam and to a spectral resolution of 1 MHz