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A method to image random three-dimensional source distributions is proposed. We show that, by using a Michelson stellar interferometer in a prescribed fashion, one is able to measure a special form of a threedimensional degree of coherence. The inverse Fourier transform of this coherence function yields the threedimensional intensity distribution of the source as seen from the paraxial far zone.
Rosen et al. (1996) studied this question.