We present the radio light curves of lensed images of the gravitational len
s B1422+231. The observations have been carried out using the VLA at 8.4 an
d 15 GHz over a period of 197 d. We describe a method to estimate the time
delay from the observed light curves. Using this method, our cross-correlat
ion analysis shows that the time delay between images B and A is 1.5 +/- 1.
4 d, that between A and C is 7.6 +/- 2.5 d, and that between B and C is 8.2
+/- 2.0 d. When applied to other lensed systems with measured time delays
our new method gives comparable results.