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Dissipation of buoyancy waves and turbulence in the atmosphere of venus
DOI: 10.1134/S0038094610060018 Bibcode: 2010SoSyR..44..475I

Izakov, M. N.

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 charac…

2010 Solar System Research
VenusExpress 6
Venus Express: The presence of turbulence in the mesosphere of venus is confirmed
DOI: 10.1134/S0038094610020012 Bibcode: 2010SoSyR..44...87I

Izakov, M. N.

Among the numerous and valuable results obtained from the Venus Express spacecraft, information from several instruments suggests that turbulence is present in the mesosphere. In this paper, the results of these experiments are interpreted with the use of the available data on turbulence in planetary atmospheres. Accounting for turbulence is neces…

2010 Solar System Research
VenusExpress 4