Two scientists from the French National Centre for Scientific Research in Paris have built a computer model that simulates the atmosphere on Titan, one of Saturn’s sixty two moons, and as a result now believe that Titan has two different atmospheric boundary layers, the lower of which appears to impact the formation of methane clouds, dune movement on the surface and wind patterns. The researchers, Benjamin Charnay and Sébastien Lebonnois have published their findings in Nature Geoscience.

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