How Does a Circular Aperture Affect Light Diffraction?

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SUMMARY

The discussion focuses on the diffraction of light through a circular aperture, specifically detailing the mathematical framework governing this phenomenon. The power per area (irradiance) is defined by the equation I(θ) = I(0) (2 J1(k r sinθ) / (k r sinθ))^2, where the angular radii of the first four dark rings are determined by specific values of k r sinθ. The Airy disk, which represents the central bright spot in the diffraction pattern, is characterized by the angular radius θAiry = 1.22 λ/d, linking the wavelength λ and the aperture diameter d. This entry provides essential insights into the behavior of light as it interacts with circular apertures.

PREREQUISITES
  • Understanding of Fraunhofer diffraction principles
  • Familiarity with Bessel functions, specifically J1
  • Knowledge of optical systems, including focal length and aperture diameter
  • Basic grasp of wave optics and irradiance calculations
NEXT STEPS
  • Study the applications of Bessel functions in optics
  • Explore the impact of aperture shape on diffraction patterns
  • Learn about the design and optimization of imaging systems using the f/number concept
  • Investigate the relationship between wavelength and diffraction in various materials
USEFUL FOR

Optical engineers, physicists, and students studying wave optics will benefit from this discussion, particularly those interested in the effects of circular apertures on light diffraction and imaging system design.

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Definition/Summary

This entry describes diffraction of a wave when it passes through a circular aperture.

Equations

The far-field (Fraunhofer) diffraction pattern for a circular aperture of radius r has a power per area (irradiance) given by:

<br /> I(\theta) = I(0) \left( \frac{2 J_1(k \ r \ \sin\theta)}{k \ r \ \sin\theta} \right)^2 <br />The angular radii of the first 4 dark rings in the diffraction pattern occur at

<br /> k \ r \ \sin\theta \ \approx \ 3.8317, \ \ 7.0156, \ \ 10.173, \ \ 13.324 <br />

where the numbers are the zeros of J_1

Equivalently, in terms of wavelength the zeroes are at

<br /> \sin\theta \ \approx \frac{\lambda}{r} \ \cdot \ 0.610, \ \ 1.12, \ \ 1.62, \ \ 2.12, \ \ 2.62, \ \ . . .<br />

Angular radius (angle between the central axis and the 1st dark ring) of Airy disk:

<br /> \theta_{Airy} \ = \ 1.22 \ \frac{\lambda}{d} <br />Airy disk radius for an imaging system:

<br /> r_{Airy} \ = \ 1.22 \ \lambda \ \frac{f}{d}<br />

Extended explanation

Definitions of terms
I = Power per area (irradiance) of the wave, with SI units of W/m2
I(0) = the irradiance at θ=0
r = the aperture radius
d = 2r = diameter of the aperture, lens, or mirror
λ = the wavelength of the wave
k = 2π/λ
θ = the angle at which the irradiance is evaluated
J1 = Bessel function of the first kind​

The Airy disk is the central bright spot of the diffraction pattern, within the 1st dark ring.

f and d are the focal length and diameter, respectively, of the lens or mirror in an imaging system.

The ratio f/d is the f/number of a lens or mirror. For example, an f/4 lens has f/d=4.

* This entry is from our old Library feature, and was originally created by Redbelly98.
 
Last edited by a moderator:
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Thanks for the overview on circular apeture
 

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