A new turbulent mixing scheme, described in Part I of this paper, is tested
in the climate and mesoscale configurations of the U.K. Met. Office's Unif
ied Model (UM). In climate configuration, the scheme is implemented along w
ith increased vertical resolution below 700 hPa (the same as that in the me
soscale model), in order to allow the different boundary layer types and pr
ocesses to be identified and treated properly. In both configurations, the
new boundary layer (PBL-N) mixing scheme produces some improvement over the
current boundary layer (PBL-C) scheme. The PBL-N scheme is able to diagnos
e different boundary layer types that appear to be consistent with the obse
rved conditions, and the boundary layer structure is improved in comparison
with observations. In the climate model, the boundary layer and cloud stru
cture in the semipermanent stratocumulus regions of the eastern subtropical
oceans are noticeably improved with the PBL-N scheme. The deepening and de
coupling of the boundary layer toward the trade cumulus regime is also simu
lated more realistically. However, the cloud amounts in the stratocumulus r
egions, which were underestimated with the PBL-C scheme, are reduced furthe
r when the PBL-N scheme is included. Tests of the PBL-N scheme in the UM si
ngle-column model and in a development version of the UM, where the dynamic
s, time stepping, and vertical grid are different from the standard version
. both show that realistic stratocumulus cloud amounts can be achieved. Thu
s, it is thought that the performance of the PBL-N scheme in the standard U
M may be bring Limited by other aspects of that model. In the mesoscale mod
el, improvements in the simulation of a convective case are achieved with t
he PBL-N scheme through reductions in layer cloud amount, while the simulat
ion of a stratocumulus case is improved through better representation of th
e cloud and boundary layer structure. Other mesoscale model case studies sh
ow that there is a consistent improvement in fog probabilities and forecast
s of cloud-base height. The root-mean-square errors in screen-level tempera
ture are also reduced slightly. The weak daytime bias in wind strength is i
mproved greatly through a systematic increase In the IO-m wind speed in uns
table conditions. As a result of these trials, the scheme has been implemen
ted operationally in the mesoscale model.