Photonica

Airy disk

The diffraction pattern formed in the focal plane of an ideal lens or telescope from a uniformly-illuminated circular aperture. A central bright disk surrounded by concentric rings of decreasing intensity, setting the resolution limit of imaging systems.

The Airy disk is the diffraction pattern produced in the focal plane of an ideal converging lens (or far-field of an aperture) when light from a point source passes through a circular aperture. The pattern was first described by George Biddell Airy in 1835 and consists of a bright central disk surrounded by alternating dark and bright concentric rings.

Intensity distribution. The radial intensity profile of the Airy pattern:

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-order Bessel function, aa is the aperture radius, and θ\theta is the angle from the optical axis.

Positions of the dark rings. The dark rings occur at the zeros of J1(x)J_1(x):

RingZero of J1J_1Angular position θ\thetaLinear position at focal length ff
1st dark ringx=3.832x = 3.832sinθ=1.22λ/D\sin\theta = 1.22 \lambda / Dr1=1.22λf/Dr_1 = 1.22 \lambda f / D
2nd dark ringx=7.016x = 7.016sinθ=2.23λ/D\sin\theta = 2.23 \lambda / Dr2=2.23λf/Dr_2 = 2.23 \lambda f / D
3rd dark ringx=10.173x = 10.173sinθ=3.24λ/D\sin\theta = 3.24 \lambda / Dr3=3.24λf/Dr_3 = 3.24 \lambda f / D

The diameter of the central Airy disk (between the two first dark rings) is d=2.44λf/Dd = 2.44 \lambda f / D.

Power distribution. The fraction of total beam power enclosed within each ring:

Ring inclusionFraction of total power
Central disk only (within first dark ring)83.8%
Through 1st bright ring91.0%
Through 2nd bright ring93.8%
Through 3rd bright ring95.3%

This is why the central Airy disk is the conceptual "spot size" of an imaging system: it contains nearly all the power even though the rings extend to infinity.

Diffraction-limited spot size. For a focusing system with numerical aperture NA, the Airy disk diameter is:

dAiry  =  1.22λNA  =  1.22λfD,d_\text{Airy} \;=\; 1.22 \, \frac{\lambda}{\text{NA}} \;=\; 1.22 \, \frac{\lambda f}{D},

where the second form uses NA=D/(2f)\text{NA} = D/(2f) for small NA (paraxial approximation). This is the absolute lower limit of focused-spot size — no aberration-free lens can produce a smaller spot.

Examples for typical systems.

Systemλ\lambdaNA or f/#f/\#Airy disk diameter
Microscope objective 100×/1.4 oil550 nm1.4480 nm
Microscope objective 40×/0.65550 nm0.651.0 μm
Camera lens, f/4550 nm0.1255.4 μm
Telescope, 8-inch f/10550 nm0.0513.4 μm
Photolithography stepper193 nm0.95250 nm
Optical disc drive (Blu-ray)405 nm0.85580 nm
HeNe focused by 100 mm f/2 lens633 nm0.253.1 μm
Telecom DFB into single-mode fiber1550 nm0.1413.5 μm

Rayleigh resolution criterion. Two point sources are "just resolved" when the central Airy disk of one falls on the first dark ring of the other. This separation in image space is the Airy radius:

δRayleigh  =  1.22λfD  =  1.22λ2NA.\delta_\text{Rayleigh} \;=\; 1.22 \, \frac{\lambda f}{D} \;=\; 1.22 \, \frac{\lambda}{2 \text{NA}}.

Below this separation, two point sources merge into a single elongated blob and cannot be reliably resolved.

Sparrow criterion. A slightly tighter resolution definition: two point sources are "just resolved" when the combined intensity profile no longer has a central dip between them. The Sparrow criterion gives:

δSparrow    0.94λ2NA,\delta_\text{Sparrow} \;\approx\; 0.94 \, \frac{\lambda}{2 \text{NA}},

about 25% smaller than Rayleigh. Modern resolution standards typically use Rayleigh, but Sparrow is sometimes cited in imaging literature.

Abbe limit (microscopy). For incoherent illumination at the focal plane of a microscope:

dAbbe  =  λ2NA,d_\text{Abbe} \;=\; \frac{\lambda}{2 \text{NA}},

approximately 22% smaller than the Rayleigh-limited diffraction spot. The Abbe limit is the most commonly cited resolution limit in microscopy.

Beyond the Airy disk. Several techniques achieve sub-Airy-disk resolution:

  • Structured illumination microscopy (SIM): extracts spatial frequency components beyond the cutoff via interference patterns; resolution ~2× better than Abbe
  • Stimulated emission depletion (STED): depletes outer parts of the Airy disk by stimulated emission; effective resolution down to ~30 nm
  • PALM/STORM: localizes individual fluorophores to ~10 nm precision via Gaussian fitting of their (still-diffraction-limited) PSFs
  • Near-field scanning optical microscopy (NSOM): uses sub-wavelength probes, bypassing diffraction
  • Photoactivated localization: similar to PALM/STORM

References: Saleh & Teich, Fundamentals of Photonics (3rd ed., 2019), Ch. 4 (Fourier optics, diffraction); Born & Wolf, Principles of Optics (7th ed.), Ch. 8 for the rigorous derivation; Goodman, Introduction to Fourier Optics (3rd ed., 2005), Ch. 6.