The effects of longwave radiation in a small cumulus cloud are investi
gated by a combination of a three-dimensional radiative transfer model
as well as a slab-symmetric cloud dynamics model. The calculations in
dicate that longwave radiative cooling substantially enhances the maxi
mum cloud water content. For a run in an environment without wind shea
r, the maximum increase reaches 96%. The total cloud water content was
also increased somewhat (maximum 20%). The effects of longwave coolin
g at different stages of development of the simulated cloud were furth
er examined and analyzed. In the initial stage of the development, the
augmentation of cloud water content near the cloud top and sides is t
raced mainly to the direct effect of longwave radiative cooling on clo
ud microphysics (i.e., radiative cooling reduces the local temperature
and hence the saturation water vapor pressure, which leads to additio
nal condensation). In the mature stage of the cloud, the increase of t
otal cloud water content arises from a combination of the effects of r
adiation on microphysics and dynamics. The cooling from radiation and
evaporation produces additional downward motion at the sides of the cl
oud. The enhanced low-level convergence invigorates the updraft to pro
mote further cloud development. In the decaying stage, the negative bu
oyancy produced by cloud top radiative cooling and a higher liquid wat
er load speeds up the decay process. The effect of wind shear was also
studied. It was shown that, similar to the case of a calm environment
, longwave cooling strengthens the secondary circulation and the cloud
water content. However, shear suppresses convection and the cloud bec
omes weaker. Longwave cooling also enhances the asymmetric characteris
tics of the simulated cloud. In conjunction with horizontal momentum t
ransport, radiative cooling results in a more negative temperature per
turbation and a stronger downdraft on the downshear flank relative to
the upshear side.