G_283.mp4

You can access the full paper and its associated media through the .

The article explores how the brightness of Venus is affected by planetary-scale waves in its atmosphere, rather than the rotation of the planet itself. Source: Nature Communications g_283.mp4

Observations from the Akatsuki spacecraft showing brightness modulations at 283, 365, and 2020 nm wavelengths. You can access the full paper and its

The "283" in the filename likely refers to the (ultraviolet) data discussed in the paper. Videos with this naming convention in academic journals are typically Supplemental Materials that show: Time-lapse imagery of atmospheric motion. Visualizations of the super-rotating winds. Data plots showing the modulation periods over time. g_283.mp4