A microphysical model attributes color changes in Jupiter's Oval BA to variations in tropospheric downwelling velocities of order 10^{-4} to 10^{-3} m s^{-1}.
The Astrophysical Journal , author=
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Tholins formed at 0.125 torr have threefold lower production rate but higher density and nanoindentation hardness than those at 1 torr, while particle size, morphology, surface energy, and Young's modulus remain similar.
citing papers explorer
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Colour changes of Jupiter's Oval BA through microphysical modelling
A microphysical model attributes color changes in Jupiter's Oval BA to variations in tropospheric downwelling velocities of order 10^{-4} to 10^{-3} m s^{-1}.
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Feeling the Pressure: Effects of Formation Pressure on the Physical Properties of Titan Haze Analogs
Tholins formed at 0.125 torr have threefold lower production rate but higher density and nanoindentation hardness than those at 1 torr, while particle size, morphology, surface energy, and Young's modulus remain similar.