Initiation of coalescence in a cumulus cloud: A beneficial influence of entrainment and mixing

Although rain has been observed to form in warm cumulus clouds within about twenty minutes, calculations that represent condensation and coalescence accurately in such clouds have had difficulty producing rainfall in such a short time except via processes involving giant cloud condensation nuclei (with diameters larger than 2 Îźm). This model-based study explores a different possible mechanism for accelerating the production of warm rain, one that depends on the variability in droplet trajectories arriving at a given location and time in a cumulus cloud. In the presence of entrainment such droplets experience different growth histories, and the result is broadening of the droplet size distribution. That broadening favours coalescence, leading to embryos that grow to raindrops. These calculations do lead to production of rain that is within the lower range of observations for clouds of Florida, USA, the location on which the input conditions were based. The process emphasized in this study, the formation of drizzle via collisions among droplets in the main peak of the droplet size distribution, complements the growth of precipitation on giant nuclei, which is also an important source of the first rain in the case studied. The results indicate that the mechanism developed here should be considered an important influence on the formation of rain in warm clouds.

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Copyright Author(s) 2011. This work is distributed under the Creative Commons Attribution 3.0 License


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Author Cooper, William
Lasher-Trapp, S.
Blyth, A.
Publisher UCAR/NCAR - Library
Publication Date 2011-04-05T00:00:00
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Topic Category geoscientificInformation
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Metadata Date 2023-08-18T18:26:08.366508
Metadata Record Identifier edu.ucar.opensky::articles:17390
Metadata Language eng; USA
Suggested Citation Cooper, William, Lasher-Trapp, S., Blyth, A.. (2011). Initiation of coalescence in a cumulus cloud: A beneficial influence of entrainment and mixing. UCAR/NCAR - Library. http://n2t.net/ark:/85065/d7fn17g8. Accessed 28 June 2025.

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