English: "The present-day atmosphere of Venus. Starting in the 1960s, several probes made in situ measurements of temperature and wind speeds in the Venusian atmosphere. Missions also determined the size distribution(s) of aerosol particles in the cloud and haze layers. Black curves show an equatorial temperature profile from the Venus International Reference Atmosphere (solid) and zonal wind speeds from four Pioneer Venus entry probes (dashed)"[1]
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↑O’Rourke, Joseph G. (2023). "Venus, the Planet: Introduction to the Evolution of Earth’s Sister Planet". Space Science Reviews219 (1). Springer Science and Business Media LLC. DOI:10.1007/s11214-023-00956-0. ISSN0038-6308.
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