A new method for correcting the wavelength misalignment in measured UV spec
tra is presented. It is based on a comparison between measured irradiances
and irradiances computed from a radiative transfer code for a set of given
atmospheric and solar conditions (250 < Dobson units < 450, 30 degrees < so
lar zenith angle < 75 degrees). Results of tests run with spectra recorded
on a clear-sky day by two spectroradiometers in a French UV spectral networ
k station are analyzed. Applying the method once reduces shift to less than
0.05 nm. The smoothing included in the method enables detection of aberran
t irradiance values and then completion of an initial quality control of me
asured spectra. A technique for assessing the instruments' slit function is
also presented. The key algorithms needed to build a computer code based o
n this method are given. (C) 2001 Optical Society of America.