The design of a three-channel solar radiometer used to determine total
columnar atmospheric water-vapor amounts is presented. The main chann
el is located in the 0.94-mum water-vapor band, and two other channels
are located in adjacent nonabsorption regions of the solar spectrum a
nd are used to remove scattering effects from the main channel. Water-
vapor transmittance is determined by means of a modified Langley appro
ach, and these transmittances are converted to columnar water vapor by
means of a band model developed at the University of Arizona. Several
cases are presented in which columnar water-vapor amounts are determi
ned through the use of the instrument and method described here. These
results are compared with sounding-balloon results. Tests of the meth
od indicate that columnar water vapor may be retrieved with an uncerta
inty of less than 10%.