Zonal averages of annual and seasonal averages of ozone amounts from Nimbus
7/TOMS (1979-1992) have been examined to estimate the systematic interannu
al variability of UV-B (390-320 nm) exposure to solar radiation between +/-
60 degrees latitude. As shown from statistical modeling, clear-sky interann
ual UV-B changes can be ascribed mainly to the quasi-biennial oscillation (
QBO) driven by stratospheric winds. The QBO oscillations can cause interann
ual changes in UV-B exposure of +/-15% at 300 nm and +/-5% at 310 nm at the
equator and at middle latitudes. In addition to QBO effects, there are lar
ger interannual changes in ozone and UV-B associated with dynamical effects
at higher latitudes. When UV-B attenuation from clouds is included, the ge
neral latitudinal structure of the interannual variability is maintained. A
t the equator the interannual variability of ozone amounts and UV exposure
caused by the combination of the 2.3 year QBO and annual cycles implies tha
t there is about a 5 year periodicity in UV-B variability caused by dynamic
al effects. At higher latitudes the appearance of the interannual UV-B maxi
mum is predicted by the QBO but without the regular periodicity. The QBO ef
fects on UV-B irradiance are larger than the long-term changes caused by th
e decrease in ozone amounts.