Philip H. Austin

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Constraints on droplet growth in radiatively cooled stratocumulus clouds
Philip H. Austin, Steven Siems and Yinong Wang
Journal of the Geophysical Research, 1 July 1995, 100, No. D7, pages 14231-14243.

Abstract


Radiative cooling near the top of a layer cloud plays a dominant role in droplet condensation growth. The impact of this cooling on the evolution of small droplets and the formation of precipitation-sized drops is calculated using a microphysical model that includes radiatively-driven condensation and coalescence. The cloud top radiative environment used for these calculations is determined using a mixed-layer model of a marine stratocumulus cloud with a subsiding, radiatively cooled inversion. Calculations of the radiatively-driven equilibrium supersaturation show that net long-wave emission by cloud droplets produces supersaturations below 0.04\% for typical nocturnal conditions. While supersaturations as low as this will force evaporation for droplets smaller than $\approx$ 5 $\mu m$, radiatively enhanced growth for larger droplets can reduce the time required to produce precipitation-sized particles by a factor of 2-4, compared with droplets in a quiescent cloud without flux divergence. The impact of this radiative enhancement on the acceleration of coalescence is equivalent to that produced in updrafts of 0.1 - 0.5 $m\,s^{-1}$, and varies linearly with the total emitted flux (the ``radiative exchange'').

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