When a large aperture is used to collect light propagated through the
atmosphere, it performs an average operation on the irradiance fluctua
tions, resulting in collected-power fluctuations that are not as large
as those that could be obtained from a point receiver. We present an
expression for the aperture-averaging factor of optical scintillation
using multiaperture architectures on the receiver configuration. That
expression is used to assess the decrease in the total collected power
fluctuations for several multiaperture receiver configurations. (C) 1
996 Society of Photo-Optical instrumentation Engineers.