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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 aa, the intensity in the Fraunhofer far field is I(θ)/I0=[2J1(x)x]2,x=2πaλsinθ,I(\theta) / I_0 = \left[\frac{2 J_1(x)}{x}\right]^2,\quad x = \frac{2\pi a}{\lambda}\sin\theta, where J1J_1 is the first Bessel function of the first kind. The first dark ring sits at x13.8317x_1 \approx 3.8317, corresponding to angular radius θ1=1.22λ/D\theta_1 = 1.22\,\lambda / D with D=2aD = 2 a 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 I(x)I(x) on the right with the first five J1J_1 zeros marked.

Figure 1. Airy diffraction pattern, exact closed form on a 256 x 256 grid. Right panel: I(x) on linear scale with first five J_1 zeros marked.
wavelength550
aperture D1.0
sigma_RMS0.000
gamma0.30

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.