Abstract

Abstract. The misrepresentation of the diurnal cycle of boundary layer clouds by large-scale models strongly impacts the modeled regional energy balance in southern West Africa. In particular, recognizing the processes involved in the maintenance and transition of the nighttime stratocumulus to diurnal shallow cumulus over land remains a challenge. This is due to the fact that over vegetation, surface fluxes exhibit a much larger magnitude and variability than on the more researched marine stratocumulus transitions. An improved understanding of the interactions between surface and atmosphere is thus necessary to improve its representation. To this end, the Dynamics-aerosol-chemistry-cloud interactions in West Africa (DACCIWA) measurement campaign gathered a unique dataset of observations of the frequent stratocumulus-to-cumulus transition in southern West Africa. Inspired and constrained by these observations, we perform a series of numerical experiments using large eddy simulation. The experiments include interactive radiation and surface schemes where we explicitly resolve, quantify and describe the physical processes driving such transition. Focusing on the local processes, we quantify the transition in terms of dynamics, radiation, cloud properties, surface processes and the evolution of dynamically relevant layers such as subcloud layer, cloud layer and inversion layer. We further quantify the processes driving the stratocumulus thinning and the subsequent transition initiation by using a liquid water path budget. Finally, we study the impact of mean wind and wind shear at the cloud top through two additional numerical experiments. We find that the sequence starts with a nighttime well-mixed layer from the surface to the cloud top, in terms of temperature and humidity, and transitions to a prototypical convective boundary layer by the afternoon. We identify radiative cooling as the largest factor for the maintenance leading to a net thickening of the cloud layer of about 18 g m−2 h−1 before sunrise. Four hours after sunrise, the cloud layer decouples from the surface through a growing negative buoyancy flux at the cloud base. After sunrise, the increasing impact of entrainment leads to a progressive thinning of the cloud layer. While the effect of wind on the stratocumulus layer during nighttime is limited, after sunrise we find shear at the cloud top to have the largest impact: the local turbulence generated by shear enhances the boundary layer growth and entrainment aided by the increased surface fluxes. As a consequence, wind shear at the cloud top accelerates the breakup and transition by about 2 h. The quantification of the transition and its driving factors presented here sets the path for an improved representation by larger-scale models.

Highlights

  • Stratocumulus (Sc) clouds play a critical role in the radiative balance of the planet given their high albedo (Hartmann et al, 1992; Chen et al, 2000) and extensive cover worldwide (Eastman and Warren, 2014; Eastman et al, 2014)

  • We systematically focus on the following processes and the role played in the maintenance of the Sc and its transition to cumulus clouds: radiation, entrainment and the land surface fluxes

  • Based on observations of the Dynamics-aerosol-chemistry-cloud interactions in West Africa (DACCIWA) project in southern West Africa we designed a numerical experiment to reproduce the transition from nighttime stratocumulus to daytime cumulus clouds over land

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Summary

Introduction

Stratocumulus (Sc) clouds play a critical role in the radiative balance of the planet given their high albedo (Hartmann et al, 1992; Chen et al, 2000) and extensive cover worldwide (Eastman and Warren, 2014; Eastman et al, 2014). The arrival of the cooler, but not necessarily moister, mass of air more than a 100 km inland facilitates the onset of Sc clouds over land (Adler et al, 2019; Babicet al., 2019; Dione et al, 2019) The fact that this mass of air is characterized by cloudless conditions when over the sea reveals the importance of the land and other local factors for the cloud formation and maintenance (Adler et al, 2019; Babicet al., 2019; Lohou et al, 2019). Lohou et al (2019) extended the previous work and summarized the four phases leading from cloud formation to dissipation: stable phase, jet phase, stratus phase and convective phase They described three observed scenarios for the breakup and dissipation of the Sc deck throughout the day.

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