Abstract

Katabatic winds are very frequent but poorly understood or simulated over steep slopes. This study focuses on a katabatic jet above a steep alpine slope. We assess the buoyancy terms in both the turbulence kinetic energy (TKE) and the Reynolds shear-stress budget equations. We specifically focus on the contribution of the slope-normal and along-slope turbulent sensible heat fluxes to these terms. Four levels of measurements below and above the maximum wind-speed height enable analysis of the buoyancy effect along the vertical profile as follow: (i) buoyancy tends to destroy TKE, as expected in stable conditions, and the turbulent momentum flux in the inner-layer region of the jet below the maximum wind-speed height $$z_j$$ ; (ii) results also suggest buoyancy contributes to the production of TKE in the outer-layer shear region of the jet (well above $$z_j$$ ) while consumption of the turbulent momentum flux is observed in the same region; (iii) In the region around the maximum wind speed where mechanical shear production is marginal, buoyancy tends to destroy TKE and our results suggest it tends to increase the momentum flux. The present study also provides an analytical condition for the limit between production and consumption of the turbulent momentum flux due to buoyancy as a function of the slope angle, similar to the condition already proposed for TKE. We reintroduce the stress Richardson number, which is the equivalent of the flux Richardson number for the Reynolds shear-stress budget. We point out that the flux Richardson number and the stress Richardson number are complementary stability parameters for characterizing the katabatic flow apart from the region around the maximum wind-speed height.

Highlights

  • Katabatic winds are gravity flows that develop over sloping terrain due to radiative cooling at the surface

  • We presently focus on the flux Richardson number R f, defined in Eq 6 (Stull 1988) because it represents the ratio between the buoyancy and the mechanical shear terms that serve as source or sink in the turbulence kinetic energy (TKE) budget (Eq 1), Rf

  • The dataset obtained over a steep slope of more than 20◦ with four levels of turbulent measurements up to a height of 6.31 m allowed us to investigate the impact of buoyancy on TKE following in the footsteps of Grachev et al (2016) and Oldroyd et al (2016a)

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Summary

Introduction

Katabatic winds are gravity flows that develop over sloping terrain due to radiative cooling at the surface. They generally are responsible for night circulation near the surface and bring cold air down the valleys, thereby enhancing the temperature inversion and trapping pollutants (Whiteman 2000). For steep slopes of more than 20◦, the maximum wind-speed height can be as low as 1 m (Horst and Doran 1988; Oldroyd et al 2014). Such flows are inadequately represented in most meteorological models, with poor resolution close to the surface. Extending our understanding of katabatic flows is a major challenge to improving mountain weather forecasts and mitigating the risk of this type of pollution for public health

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