Write and wavenumber . The pupil Fourier transform, normalized by pupil area, gives the Fraunhofer diffraction wave amplitude. In pupil polar coordinates,
The angular average is because . The Bessel function of the first kind identity then reduces the radial integral to . Taking the squared magnitude yields the Airy disk light intensity profile.[ref]
The apparent division by zero is removable. The power series
gives and . At the centre, every pupil contribution has the same wave phase, so their normalized sum is one. The first dark ring instead corresponds to with , rather than to the removable zero of at the origin.

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