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Power spectra obtained from cloud brightness distribution in Galileo violet images are used as a proxy of the kinetic energy power spectra in order to study the atmospheric turbulence in Venus. Interpretation based on a review of predicted regimes from classical laws is made, in addition to comparing Venus results with the ones obtained in Earth.
Turbulence, Planets, Planetary Atmospheres, Solar System
Turbulence, Planets, Planetary Atmospheres, Solar System
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