Radio interferometry is a mature, well understood field that has historically benefited from
of the application of mathematical analysis, coupled with adequate computing power. However,
a new generation of telescopes strain both analysis and computing. The problem arises from
the expansion of the field of view to a regime where a simple two-dimensional Fourier transform
relationship between measured coherence and unknown sky brightness fails. I will review
existing techniques for overcoming these limitations and indicate areas where more sophisticated
mathematical analysis is needed.