[astro-ph.EP] We investigate the thermal structure of the Venusian middle atmosphere between 45 and 80 km using radio occultation (RO) measurements from Venus Express and Akatsuki spanning 2006-2024.
![Global Temperature contour maps of Venus with VEX RO serving as the primary reference dataset. The data binning is the same as in Figure 4. -- [astro-ph.EP]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/08/Study-on.png?resize=1200%2C720&ssl=1)
[astro-ph.EP] We investigate the thermal structure of the Venusian middle atmosphere between 45 and 80 km using radio occultation (RO) measurements from Venus Express and Akatsuki spanning 2006-2024.