Presented is a parameterization of the liquid water droplet optical propert
ies for the solar spectrum. Two models are provided: a 4-band model for use
in general circulation models and a 31-band model for use in higher spectr
al resolution investigations. The form of the parameterization is a simple
extension of Slingo [1989], and the subdivision of wavelengths into bands i
s almost identical. The parameterization scheme is for all of the optical p
roperties needed to perform 2- and 4-stream calculations. The 4-band model
has the same spectral divisions as Slingo [1989], whereas the 31-band model
has finer resolution of the absorbing bands in the near infrared. The para
meterized single-scattering optical properties are accurate to within 0.5%
compared to exact Mie calculations for both band models over the r(eff) ran
ge from 5 to 40 mu m. The layer radiative properties, from both two- and fo
ur-stream methods, are almost always within 1% accuracy compared to calcula
tions using exact optical properties as inputs. Also, it is shown that usin
g the Henyey-Greenstein phase function to obtain the higher-order moments,
used in four-stream calculations, results in substantial error in the layer
radiative properties compared to using exact Mie inputs.