An efficient algorithm of evaluating absorption coefficients line-by-line f
or the purpose of integrating the radiative transfer equation with emphasis
on the Earth's atmosphere is presented. The main problems associated with
such an algorithm are concerned with line shape, the treatment of lines out
side the spectral range of interest, and the way in which spectral sampling
is performed. These are considered together with methods improving speed o
f computation in general. Results and intercomparisons from applications of
the algorithm are presented. (C) 1999 Elsevier Science Ltd. All rights res
erved.