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. 2023 May 31;620(7973):292–298. doi: 10.1038/s41586-023-06230-1

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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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Extended Data Fig. 7 — a, GCM light curves compared against the data and the best-fitting eclipse-mapping model. b, Data and the GCM light curves with the eclipse-mapping model subtracted. The GCMs with strong atmospheric drag (RM-GCM B = 20 G and SPARC/MITgcm τ_drag = 10³ s) match the data better than their counterparts that have little to no drag.

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