Published January 1, 2007
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Atmospheric Turbulence in the Clouds of Venus
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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.
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- Book: 10.1007/978-1-4020-6000-7 (DOI)