Using Fermat's principle, we analyze the effects of very long waveleng
th gravitational waves upon the images of a gravitationally lensed qua
sar. We show that the lens equation in the presence of gravity waves i
s equivalent to that of a lens with a different alignment between sour
ce, deflector, and observer in the absence of gravity waves. Contrary
to a recent claim, we conclude that measurements of time delays in gra
vitational lenses cannot serve as a method to detect or constrain a st
ochastic background of gravitational waves of cosmological wavelengths
, because the wave-induced time delay is observationally indistinguish
able from an intrinsic time delay due to the lens geometry.