Jc. Petch et al., A COMPARISON OF 2 BULK MICROPHYSICAL SCHEMES AND THEIR EFFECTS ON RADIATIVE-TRANSFER USING A SINGLE-COLUMN MODEL, Quarterly Journal of the Royal Meteorological Society, 123(542), 1997, pp. 1561-1580
Increasingly, numerical models in climate studies are using prognostic
bulk microphysical schemes to predict grid-scale cloud cover and prop
erties. These schemes provide information which can lead to improved c
alculations of radiative transfer, and a better understanding of the i
nteraction of radiation with cloud microphysics on the large scale. In
this study a one-dimensional, hydrostatic column model with fixed ver
tical velocities includes two different bulk microphysical schemes to
investigate how the type of scheme influences the hydrometeor content
in a cloud, and the effect of this on the radiative heating rates thro
ugh the cloud. Two test cases are performed, one representing the stra
tiform region of a tropical cloud cluster, the other a dissipating tro
pical cirrus cloud, Each test is first performed using a microphysical
scheme that carries only one variable for solid water (MS1), and then
using a scheme that separates solid water into ice crystals, snow, an
d graupel (MS2). Further sensitivity tests are made using MS2 to exami
ne the effects of excluding graupel, and of allowing the ice crystals
to fall. The influence of these modifications on the hydrometeor conte
nts of the clouds and the corresponding radiative heating rates is con
sidered. In a simulation of the stratiform region of a tropical cloud
cluster, MS1 is shown to produce significantly larger hydrometeor cont
ents than MS2. However, in the simulation of a dissipating cirrus clou
d, the ice content predicted by MS2 remains much larger than the ice c
ontent predicted by MS1, throughout a 24-hour integration. This is bec
ause there is a non-precipitating ice category in MS2 which is very sl
ow to convert to snow at low ice-water contents. The use of a non-prec
ipitating ice variable is shown to have a major impact on both the sol
ar and the infrared radiative heating rates at the cloud top, and in s
ome cases to give unrealistic predictions of cloud ice contents.