Wavefront Aberrometry, Adaptive Optics, Retinal Metrology & Point Spread Function • 15 min read

Point Spread Function (PSF), Strehl Ratio & Airy Disc: Maréchal's Criterion & Optical Diffraction Limits

EXECUTIVE CLINICAL SUMMARY
In an optically perfect system, an infinitely small point source of light does not focus to an infinitesimal point on the retina; diffraction through the circular pupil spreads the light into a central bright core surrounded by concentric rings known as the Airy disc. The intensity distribution of this image is the Point Spread Function (PSF). Optical aberrations scatter energy out of the core into broad flare skirts, quantified by the Strehl ratio and Maréchal's criterion.
ELLASUV Wavefront Biophysics Laboratory Advanced Optical Wavefront Metrology & Adaptive Optics Group
ISO 8980-3 / ANSI Z80.1 Metrology Updated: 2026-09-07 ✓ Peer-Reviewed

Diffraction Limits: The Airy Disc & The Fraunhofer Integral

For a circular entrance pupil of diameter DD and focal length ff' in a medium of refractive index nn', Fraunhofer diffraction yields the radial intensity distribution of the Airy Pattern:

I(θ)=I0(2J1(πDsinθ/λ)πDsinθ/λ)2    dAiry=2.44λfDI(\theta) = I_0 \left( \frac{2 J_1(\pi D \sin\theta / \lambda)}{\pi D \sin\theta / \lambda} \right)^2 \implies d_{\text{Airy}} = 2.44 \cdot \frac{\lambda \cdot f'}{D}

For the human eye (f17 mmf' \approx 17\ \text{mm}) under green light (λ=555 nm\lambda = 555\ \text{nm}):

  • At D=2.0 mmD = 2.0\ \text{mm}: dAiry=2.440.000555×172.011.5 μmd_{\text{Airy}} = 2.44 \cdot \frac{0.000555 \times 17}{2.0} \approx \mathbf{11.5\ \mu\text{m}} (Diffraction dominates; exceeds foveal cone diameter).
  • At D=6.0 mmD = 6.0\ \text{mm}: dAiry3.8 μmd_{\text{Airy}} \approx \mathbf{3.8\ \mu\text{m}} (Theoretical diffraction core is smaller than foveal cones; however, higher-order aberrations explode!).

The Strehl Ratio & Maréchal's Criterion

The Strehl Ratio (SS) is the ratio of peak on-axis intensity of the aberrated PSF compared to that of an unaberrated, diffraction-limited PSF:

S=Iaberrated(0,0)Idiffraction(0,0)eσϕ21(2πλRMS)2S = \frac{I_{\text{aberrated}}(0, 0)}{I_{\text{diffraction}}(0, 0)} \approx e^{-\sigma_\phi^2} \approx 1 - \left( \frac{2\pi}{\lambda} \cdot RMS \right)^2

According to Maréchal's Criterion, an optical system is deemed 'diffraction-limited' (essentially optically perfect) if:

S0.80    RMSwavefrontλ140.040 μm\mathbf{S \ge 0.80} \iff RMS_{\text{wavefront}} \le \frac{\lambda}{14} \approx 0.040\ \mu\text{m}

Most young human eyes achieve a Strehl ratio of only 0.10 to 0.350.10\text{ to } 0.35 under a dilated 6 mm6\ \text{mm} pupil, illustrating how heavily human vision is limited by natural aberrations rather than pure diffraction.

PSF Convolution & Real-World Visual Perception

Any real-world scene O(x,y)O(x, y) perceived by a patient is the mathematical 2D convolution of the object with the ocular PSF: I(x,y)=O(x,y)PSF(x,y)I(x, y) = O(x, y) \otimes PSF(x, y). Asymmetric PSFs with coma wings generate the ghosted letter shadows seen in keratoconus and post-LASIK decentration.

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FREQUENTLY ASKED CLINICAL QUESTIONS

Expert Answers

What is a Point Spread Function (PSF) in simple terms?
The PSF is a picture of what a single pinpoint star of light actually looks like when focused onto your retina. If your eye has aberrations, that tiny point spreads out into a blurry blob, starburst, or comet-shaped smudge.
What is a good Strehl ratio for human eyes?
A perfect, flawless telescope achieves a Strehl ratio of 1.0 (or 0.80+ for diffraction-limited optics). Normal human eyes with a 6 mm pupil typically score between 0.15 and 0.30 due to natural cornea and lens aberrations.
Why do my eyes see sharper through a tiny pinhole?
A tiny pinhole (1.5 to 2 mm) blocks all peripheral aberrated light rays from your cornea and lens, creating an almost purely diffraction-limited image on your retina, instantly clearing refractive blur.
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