Rayleigh criterion 2026-10-14
The Rayleigh criterion calls two equal, mutually incoherent optical point sources just resolved when one circular-pupil Airy disk's centre coincides with the other's first zero. It is a specified discrimination convention, distinct from full width at half maximum and from precision in estimating one source's position.
For this circular optical pupil, the Rayleigh criterion uses angular separation , or in the paraxial approximation to the focal plane. The point spread functions still overlap.[ref]
For the Airy disk design example with , and , the angular convention gives , or about arcseconds, and the image-plane separation is . Two equally bright, mutually incoherent optical point sources at separations , and times this scale would have image separations , and respectively. These calculated cases are compared in incoherent two-source Airy profile.
The Rayleigh criterion is useful because it ties an easily recognized two-peak convention to a predictable optical scale. It does not assert that all information vanishes below that separation. Inferring two unknown positions also depends on photon shot noise, background, unequal brightness and uncertainty in the point spread function; locating a single isolated source is a different task. A theoretical analysis shows that alternative optical measurements can estimate the separation of two incoherent optical point sources below this scale.[ref]
The mutual optical coherence condition is essential. In incoherent imaging, time-averaged light intensities add. In coherent imaging, wave amplitudes add before squaring, leaving a wave interference term controlled by relative wave phase. Two holes illuminated by the same coherent laser therefore do not implement the equal-incoherent-source convention merely because their individual patterns resemble Airy disks. The coherent single-aperture laboratory test establishes the response of each aperture; it does not establish the pair's mutual incoherence.