Abstract
Estimates of the vertical mass eddy diffusion coefficient K are necessary to understand the dynamics and photochemistry of a planetary atmosphere. Most previous estimates for the atmosphere of Venus1–10, pertain to the upper atmosphere. In the lower atmosphere (≲80 km), information on small-scale (≲1 km) temperature fluctuations has been provided by radio scintillations observed during radio occultation by the atmosphere11–18. Here we relate the vertical mass eddy diffusion coefficient to these radio scintillation observations so that reliable estimates can be obtained near the tropopause level of 60 km for the first time. Using the recent Pioneer Venus radio occultation measurements16, and assuming that the turbulence is generated by shear instability, we find that K = 4 × 104 cm2 s−1, the energy dissipation rate ɛ = 20 cm2 s−1, and the dissipation rate of temperature fluctuations Nθ = 10−3 K2 s−1. These results indicate that small-scale turbulence probably plays a major part in vertical transport near the tropopause of Venus.
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Woo, R., Ishimaru, A. Eddy diffusion coefficient for the atmosphere of Venus from radio scintillation measurements. Nature 289, 383–384 (1981). https://doi.org/10.1038/289383a0
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DOI: https://doi.org/10.1038/289383a0
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