Dissipation of buoyancy waves and turbulence in the atmosphere of venus

Details Dissipation of buoyancy waves and turbulence in the atmosphere of venus Dissipation of buoyancy waves and turbulence in the atmosphere of venus

Dec 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010sosyr..44..475i&link_type=abstract

Solar System Research, Volume 44, Issue 6, pp.475-486

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Scientific paper

The turbulent energy dissipation rate and the coefficients of turbulent diffusion and viscosity caused by breaking buoyancy waves (BWs) have been calculated. From the comparison of these values with other data, the contribution of BWs to the generation of turbulence has been determined. The comparison confirms the validity of the turbulence characteristics of the Venusian troposphere previously calculated from experimental data.

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