  The complex 10-component gravitational lens B1933+503 has been monitored with
the VLA during the period February to June 1998. Here we present the results of
this A-configuration 8.4 GHz monitoring campaign. The 37 epochs of observations
have an average spacing of 3 days. The data have yielded light curves for the
four flat-spectrum radio components (components 1, 3, 4 and 6). We find no
significant flux density changes in any of the four flat spectrum components.
