Condensation rate-mass flux correlation: implications for
supersaturation in shallow cumulus clouds
Abstract
The system of trade wind cumulus clouds observed during the RICO field
project was simulated by an LES model over a domain size of a mesoscale
model grid. More than 2000 clouds were analyzed by stratifying them by
their size/stage of maturity. The investigation was focused on phase
transition rates, which in warm tropical clouds are represented by the
processes of condensation/evaporation. Data from LES simulations of
shallow cumulus clouds demonstrated a nearly perfect correlation between
condensation rate (CR) and upward (positive) mass flux (MFP). This
strong correlation is explained using the condensation theory. The
strong CR-MFP correlation implies that supersaturation in clouds varies
within a few percent of its quasi-steady value. Calculating the slope of
the CR-MFP linear fit from concurrent measurements of temperature and
vertical velocity, and comparing it with the corresponding slope based
on the quasi-steady supersaturation assumption, may provide a method for
estimating the supersaturation in clouds. The strong dependence of
condensation rates on vertical velocity may indicate the direction for
development of SGS latent heat release parameterization.