Techniques for retrieving column water vapor from Sun radiometer measuremen
ts involving the 940-nm water vapor absorption band have been around for th
e better part of a century. Arguably, the best method to use for this retri
eval is the modified Langley technique. However, to apply this method one m
ust obtain the instrument response at the top of the atmosphere using modif
ied Langley plots on clear days with a very stable water vapor column. Usin
g subsequent measurements in this filter, ratioed to the top-of-the-atmosph
ere response allows one to determine the transmission in the 940-nm water b
and. In this paper, we present an approach that does not require an absolut
e knowledge of the extraterrestrial instrument response. The method discuss
ed here relies, instead, on relative measurements of a calibration lamp and
the extraterrestrial spectral irradiance within and just outside the 940nm
absorption band. We execute these retrievals for the rotating shadowband s
pectroradiometer (RSS) on 3 days during the Department of Energy's Atmosphe
ric Radiation Measurement program's 1997 Water Vapor Intensive Observation
Period. We compare the results to those retrieved from a colocated multifil
ter rotating shadowband radiometer (MFRSR) that uses an empirical calibrati
on and from a colocated microwave radiometer. Since our optical method of r
etrieving column water vapor from RSS measurements does not depend on a cal
ibration performed against another water vapor measurement, it contributes
an independent estimate in the search for absolute accuracy. The major cont
ributors to the uncertainty of this retrieval are the water vapor band stre
ngth calculations, the difference in aerosol extinction in and near the wat
er vapor band, the relative spectral irradiance output of the calibration l
amp and the Sun at the nonabsorbing and band-centered wavelengths, and the
stability of the spectral response of the instrument, which will be discuss
ed in detail.