Tsunami in the Skies: Unraveling the Mysteries of Atmospheric Acceleration on Venus

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Experts from the Universities of Seville and of the Basque Country believe that discontinuity may be playing a very significant role in the acceleration of this planet’s atmosphere. A group of scientists from the University of Seville, in collaboration with experts from the University of the Basq

A false-color image of the sulfurous Venusian cloud cover was produced using two ultraviolet channels from Akatsuki, the Japanese PLANET-C, and Venus Climate Orbiter, which highlights the convective turbulence of the planet’s tropical regions, in contrast with the clear, smoother polar regions. Credit: Daimia Bouic/JAXA/ISAS/DARTS

Examples of discontinuity events during 2022. The discontinuity was apparent on the nightside lower clouds with 2.26 μm images from IRTF/SpeX taken on February 4, and at the dayside middle clouds as observed in images by amateur observers taken with filters covering wavelengths 700–900 nm from May to July 2022. During June 14, Akatsuki/UVI images at 365 nm suggest that the discontinuity was propagating simultaneously at the upper and middle clouds .

 

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