Use a two-element radio interferometer: couple two small dishes coherently and align the projected baseline along the angular separation of the neighbouring satellites. Each dish's broad antenna response should include both satellites. Match the electronic delays so that the desired satellite arrives in phase at the combiner. For baseline length perpendicular to the central line of sight, a small angular displacement produces geometric path difference and phase difference
For equal signal amplitudes from one source, the output wave intensity is . Put one satellite on a maximum and its neighbour on the first null: . The smallest useful projected baseline is therefore
The angles here are measured near the normal to the baseline. At a general pointing angle , replace in the small-separation estimate by . Longer odd-half-fringe baselines can also null the neighbour but create more angular ambiguity. This arrangement provides discrimination along one direction; two collectors alone have repeated interference fringes and do not produce an unambiguous full image.

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