A numerical model to estimate spectral and broadband ultraviolet irradiance
(290 to 325 nm) for Canadian conditions is described and validated with Br
ewer spectroradiometer measurements at four stations. The model applies the
delta-Eddington algorithm to a 50-level, 100-km, plane-parallel atmosphere
with cloud inserted between 2 and 3 km. It requires measured total atmosph
eric ozone depth and hourly observations of cloud amount. In the absence of
ozone soundings, model ozone profiles are scaled by the ratio of measured
(from the Brewer instrument) to model total atmospheric ozone depths. In th
e model calculations, SUSIM ATLAS 3 extraterrestrial irradiance measurement
s are averaged for each nanometer of wavelength to mimic the triangular fil
ter used by the Brewer instrument. Ozone absorption is calculated from the
temperature-dependent coefficients of Pauer and Bass(1985), Rayleigh optica
l depths after Elterman (1968), and aerosol optical properties from MODTRAN
. Surface albedo is a function of snow depth and 0.05 for snow-free ground.
Model and measured spectral irradiances for cloudless skies agree well, bu
t model values are smaller than measurements for wavelengths below about 30
5 nm because of enhancement of the Brewer signal by stray light. Model valu
es of daily cloudless sky irradiance using lidar aerosol optical depth meas
urements from York University after the Mt. Pinatubo eruption in 1991 agree
well with measurements. Cloud optical depths were calculated iteratively f
or overcast conditions. A fixed optical depth of 45 was used to calculate c
loudy sky irradiances at the four stations. These agree well with measureme
nts. Mean bias error (MBE) is less than 5% of the mean measured daily irrad
iance and Foot mean square error (RMSE) less than 25%, decreasing to below
12% for 10-day averages. Agreement between mean daily measured and calculat
ed spectral irradiances over a month is also good.