In this paper we discuss the application of correlated k-distribution metho
ds for the computation of radiative transfer through the atmosphere in the
visible, near IR, and IR spectral regions. Whereas the correlated k-distrib
ution is a good approximation overall to line-by-line calculations, it is i
naccurate in regions of strong absorber overlap. Several approaches (band s
plitting, strength-based splitting, double and triple correlated k) are pro
posed to modify the conventional correlated k-distribution and improve its
predictions in these regions of absorber line overlap. A comparison with li
ne-by-line computations in the infrared spectral region demonstrates that a
combination of these methods produces brightness temperatures within less
than 0.25 K of those obtained from line-by-line computations at significant
ly less computation costs. In the visible and near IR, when atmospheric sca
ttering is included, the new treatment of overlapping mixed gases also prod
uces excellent agreement with the line-by-line model. (C) 1999 Elsevier Sci
ence Ltd. All rights reserved.