Rayleigh optical depths that were calculated by Bucholtz represent an
improvement over previous calculations (from 1.4% to 20%) because an u
pdated depolarization factor that varied with the wavelength was used.
These optical depths were obtained by integrating standard atmospheri
c model temperature and pressure profiles over height. This integratio
n is a valid method for obtaining an estimate of the column density an
d therefore the Rayleigh optical depth, given that small errors (less
than 0.7%) will be introduced because of quadrature and inaccuracies i
n any given model. (C) 1998 Optical Society of America.