Abstract

Abstract. Although typically associated with precipitating cumuli, cold pools also form under shallower stratocumulus. This study presents cold-pool observations as sampled by the NSF/NCAR C-130, which made cloud and boundary-layer measurements over the southeast Pacific stratocumulus region at an altitude of approximately 150 m during the VOCALS Regional Experiment. Ninety edges of cold pools are found in the C-130 measurements by identifying step-like changes in the potential temperature. Examination of their mesoscale environment shows that the observed cold pools tend to form under heavier precipitation, thicker clouds, and in cleaner environments. Cold pools are also found to form under clouds with high LWP values over the night of or before sampling. When they form, cold pools often form in clusters or on top of each other, rather than as separate, individual entities. Their sizes range from 2 km to 16 km (middle 50th percentile), where the largest of cold pools are associated with the greatest drops in temperature. Composites of various observed thermodynamic and chemical variables along the cold-pool edges indicate increased humidity, equivalent potential temperature, coarse-mode aerosol, and dimethyl sulfide concentration inside cold pools. The enhancements inside cold pools are consistent with increased static stability that traps fluxes from the ocean surface in the lowest levels of the boundary layer. By using pressure perturbations, the average cold pool is estimated to be approximately 300 m deep. The temperature depression in cold pools also leads to density-driven flows that drive convergence of horizontal winds and measurable, mechanically driven vertical wind velocity at the edges of cold pools.

Highlights

  • The formation of pools of cold, relatively high-density air at the surface, or cold pools, represents one key way in which precipitation from convective clouds organizes cloud fields

  • Cloud top height (m) temporal evolution of cloud field TB using forward trajectories calculated from European Centre for Medium Range Weather Forecasting (ECMWF) wind fields (George et al, 2013), we find no indication that cold-pool formation preferentially leads to clouds breaking up, suggesting that cold-pool formation does not necessarily lead to cloud breakup

  • We examine whether the same changes in cloud and precipitation properties occur across the cold-pool edges at the 1 km scale, using retrievals from the Wyoming Cloud Lidar (WCL), Wyoming Cloud Radar (WCR), and the G-band Radiometer Probe (GVR)

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Summary

Introduction

The formation of pools of cold, relatively high-density air at the surface, or cold pools, represents one key way in which precipitation from convective clouds organizes cloud fields. Elevated θe is not always associated with cold pools forming under precipitating clouds In their observational study of cold pools under precipitating trade cumuli, Zuidema et al (2012a) found reduced θe in cold pools and showed how this is achieved by precipitationdriven downdrafts that pull down drier air from aloft. The rate at which precipitation falls from stratocumulus clouds is largely controlled by the liquid water path (LWP), or alternatively cloud thickness, and the cloud droplet number concentration (Geoffroy et al, 2008; Wood, 2012) The latter is closely related to the accumulation mode aerosol concentration in marine environments (Martin et al, 1994), and this is the case over the southeastern Pacific (SEP, Terai et al, 2012).

Data and methods
Identifying cold pools in the data
Atmospheric conditions when cold pools are observed
Location
Boundary-layer characteristics
Satellite derived cloud field
Thermodynamics
Dynamics
Cloud and precipitation
Aerosols and DMS
Two box model
Findings
Discussion and conclusions
Full Text
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