Spectral line shapes provide a powerful tool for characterizing strongly co
upled plasmas that have become experimentally more accessible in recent yea
rs. Line shape calculations in turn require as input the electric microfiel
d distribution at the emitting atom or ion. The APEX approximation for micr
ofield distributions is computationally fast and suited for weakly as well
as strongly coupled plasmas. The currently available APEX program, however,
contains computationally difficulties that restrict its range of applicabi
lity. Consequently, the code has been improved removing many of its shortco
mings. An important new feature is the incorporation of the HNC integral eq
uation solution to the radial distribution functions necessary for the APEX
approximation. Published by Elsevier Science Ltd.