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We quantitatively investigate the role of gravity wave drag in the SBL over realistic (i.e. non idealized) terrain. We use a high resolution column model for the SBL that includes a first order turbulence closure, a broadband longwave radiation scheme, and has a full coupling with the land surface. The model has been validated for Cabauw and CASES99 observations before. This model is has been coupled with a module that analyzes the vertical profiles of wave drag from wind and temperature profiles. The innovative aspect of this module is that the contributions of the individual Fourier mode of the terrain to the wave drag are considered for each wind sector. Also it allows for analyzing critical levels, and wave stress divergence, which might trigger flow acceleration, and turbulence.
We run the model for 23 nights of the CASES99 experimental campaign. For weak wind nights, a substantial amount of wave drag is found, especially relative to the turbulent drag. The wave drag seems of intermittent nature, in certain nights, but during other nights the contribution is more continuous. As such, the simulations suggest that wave drag can be important and need to be parameterized in large-scale models.