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. 2020 Feb 26;10:3448. doi: 10.1038/s41598-020-59278-8

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© The Author(s) 2020

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 license, and indicate if changes were made. The images or other third party material in this article are included in the article’s Creative Commons license, unless indicated otherwise in a credit line to the material. If material is not included in the article’s Creative Commons license 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 license, visit http://creativecommons.org/licenses/by/4.0/.

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Local time–latitude distribution of radio occultation measurements made on Venus Express (dots) and Akatsuki (crosses) missions. An observation point is defined as the tangential point of the straight line connecting the spacecraft and tracking station at the moment that the spacecraft is occulted by the 50-km-altitude surface.