At optical wavelengths, geometrical optics holds that the extinction e
fficiency of raindrops is equal to two. This approximation yields a wa
velength-independent extinction coefficient that, however, can hardly
be used to predict accurately rain extinction measured in optical tran
smissions. Actually, in addition to the extinct direct incoming light,
a significant part of the power scattered by the rain particles reach
es the receiver. This leads to a reduced apparent extinction that depe
nds on both rain characteristics and link parameters. A simple method
is proposed to evaluate this apparent extinction. It accounts for the
additional scattered power that enters the receiver when one considers
the forward-scattering pattern of the raindrops as well as the multip
le-scattering effects using, respectively, the Fraunhofer diffraction
and Twersky theory. It results in a direct analytical formula that ena
bles a quick and accurate estimation of the rain apparent extinction a
nd highlights the influence of the link parameters. Predictions of app
arent extinction through rain are found in excellent agreement with me
asurements in the visible and IR regions. (C) 1996 Optical Society of
America.