Liquid water path variability in unbroken marine stratocumulus clouds is ex
amined using a simple adiabatic model and both ground-based and airborne ob
servations. Observations from FIRE suggest that fluctuations in liquid wate
r path at scales smaller than around 60 km can be modelled reasonably well
as a function of fluctuations in cloud-base height. A simple adiabatic mode
l of cloud liquid water content with a normally distributed cloud base and
constant inversion height results in liquid water path distributions that c
ompare favourably with observations. Further, it is shown how cloud-base he
ight fluctuations can be predicted from the sub-cloud turbulent fluctuation
s of temperature, specific humidity and their covariance. The relative impo
rtance of these three contributing terms is assessed. Aircraft observations
of these fluctuating variables are used to predict the widths of liquid wa
ter path distributions observed radiometrically, The observations also sugg
est that the standard deviation of cloud-base height and hence liquid water
path variability increases with increasing boundary-layer depth. The model
liquid water path distributions could be used to derive plane-parallel alb
edo biases and offer a possible framework for future parametrizations of su
bgrid-scale variability in general circulation models.