Airy Diffraction Pattern from a Circular Aperture
What you are seeing: if you shine a perfectly collimated monochromatic light beam through a small round hole and catch the light on a screen far away, you do not get a sharp shadow of the hole. You get a bright central spot surrounded by faint concentric rings: the Airy pattern. It is one of the most fundamental diffraction phenomena and sets the resolution limit of every telescope and microscope.
For a circular aperture of radius , the intensity in the Fraunhofer far field is where is the first Bessel function of the first kind. The first dark ring sits at , corresponding to angular radius with the diameter. This is the Rayleigh resolution criterion.
Below: 2D intensity heatmap on the left (use the gamma slider to bring out faint rings), 1D radial intensity profile on the right with the first five zeros marked.
WHAT TO TRY
- Widen the aperture D: the Airy disk and its rings shrink as 1.22 lambda over D, so a bigger lens resolves finer detail. The first-null angle in the readout sets the diffraction limit.
- Add RMS wavefront error sigma: the Strehl ratio drops, light bleeds out of the central disk into the rings, and the radial profile loses its clean peak. That is how aberrations blur an image.
- Change the wavelength: longer light spreads the pattern wider for the same aperture, since diffraction scales with lambda. The Bessel-zero nulls mark each dark ring.