  I outline the prospects for performing weak lensing studies with the new
generation of radio telescopes that are coming online now and in the future. I
include a description of a proposed technique to use polarization observations
in radio weak lensing analyses which could prove extremely useful for removing
a contaminating signal from intrinsic alignments. Ultimately, the Square
Kilometre Array promises to be an exceptional instrument for performing weak
lensing studies due to the high resolution, large area surveys which it will
perform. In the nearer term, the e-MERLIN instrument in the UK offers the high
sensitivity and sub-arcsec resolution required to prove weak lensing techniques
in the radio band. I describe the SuperCLASS survey -- a recently accepted
e-MERLIN legacy programme which will perform a pioneering radio weak lensing
analysis of a supercluster of galaxies.
