A theoretical and numerical investigation of the systematic phase errors in
phase-shifting speckle interferometry is presented. The theoretical invest
igation analyzes the behavior of some systematic error induced by intensity
variations in two cases of data-computing techniques. The first case deals
with the technique in which the phase change is computed, unwrapped, and t
hen linearly filtered; the second case deals with the technique in which th
e data are linearly filtered before the arctangent calculation and then unw
rapped. With the first filtering technique it is shown that it is preferabl
e when the phase change is of relatively low spatial frequency, leading to
a particularly accurate method. With the second case it is demonstrated tha
t an important parameter of speckle interferometry is the modulation factor
of the interference frame that induces phase errors when the data are filt
ered before the arctangent calculation. We show that this technique is bett
er than the first when the phase change is composed of high-spatial-frequen
cy variations. The theoretical investigation of the two techniques is compa
red with numerical simulations, considering the frequency characteristics o
f the phase change, and this shows a good match between theory and simulati
ons. (C) 2001 Optical Society of America.