Abstract
The structure of turbulence in an inversion layer and in an homogeneous convective field of the planetary boundary layer is described. In the first part of the paper, we validate the sodar estimates of turbulent dissipation, by using measurements with an hot-wire anemometric system in situ. Limitations of an ε measurement technique using structure function calculations are given, taking account of atmospheric properties and acoustic Doppler instrumental effects.
By comparison between isopleths of backscattering intensity and of turbulent dissipation rates, we observe that in the early morning, turbulence is advected by mechanical turbulence generated by wind shear. The same mechanism seems to be operating in the case of an inversion layer capping thermal instability, when the convective activity is not too greatly developed.
A turbulent kinetic energy budget is examined using aircraft, sodar, and tower measurements. This indicates a constant turbulent dissipation profile through a deep convective layer.
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Weill, A., Baudin, F., Goutorbe, J.P. et al. Turbulence structure in temperature inversions and in convection fields as observed by doppler sodar. Boundary-Layer Meteorol 15, 375–390 (1978). https://doi.org/10.1007/BF02652609
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DOI: https://doi.org/10.1007/BF02652609