Airydisk calculator

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As the Separation Distance slider is adjusted to move the Airy patterns closer together in the tutorial, they eventually reach the Rayleigh criteria distance, which is noted by a pop-up in the tutorial window. Upon even closer approach, the Sparrow limit is reached, also noted by a pop-up.

To operate the tutorial, use the Wavelength slider on the left to adjust the wavelength of illumination. As this value is decreased, note how the Airy disk size decreases (and resolution (r) increases). The Numerical Aperture slider can also be used to adjust Airy pattern size by changing the numerical aperture of a virtual microscope objective. As the Airy patterns approach each other, by adjustment of the Separation Distance slider, they eventually reach the Rayleigh Criterion limit of separation (discussed below), followed by the Sparrow limit. This tutorial assumes that virtual objective lenses are completely free of aberrations, that the Airy patterns are of identical brightness, and that the unit diffraction pattern generated by the specimen through a circular aperture is in fact an Airy disk. Airy patterns are modified to alternative diffraction patterns by lens aberrations or non-standard aperture conditions.

Airy patterncalculator

In the ideal case, when the objective is aberration-free and provides a uniform circular aperture, two adjacent points are just resolved when the centers of their Airy disks are separated by r (the central Airy disk radius). When the objective numerical aperture matches that of the substage condenser, r is determined from the equation:

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Airydisc diffraction

Airy diffraction pattern sizes and their corresponding radial intensity distribution functions are sensitive to the combination of objective and condenser numerical apertures as well as the wavelength of illuminating light (when monochromatic light is used to illuminate the specimen). For a well-corrected objective with a uniform circular aperture, two adjacent points are just resolved when the centers of their Airy patterns are separated by a minimum distance (D) equal to the radius (r) of the central disk in the Airy pattern.

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Figure 1 illustrates the calculated impact of condenser numerical aperture on resolution and includes values where the objective numerical aperture is less than that of the condenser. This figure plots the ratio of the numerical apertures of the condenser and objective versus the minimum resolved distance between Airy patterns (Rayleigh criterion) in units of wavelength divided by the objective aperture.

Airydisk formula

where n is the refractive index of the medium separating the objective front lens and the specimen, and is the half-cone of light captured by the objective. If the specimen is not self-luminous or when the objective and condenser numerical apertures do not match, the equation for r is given by:

AiryDisk telescope

In cases where two adjacent Airy patterns become closer to each other than in the Rayleigh criterion, the separation is known as the Sparrow limit, which is given by the equation:

where λ is the wavelength of light with air as the immersion medium and NA(obj) is the numerical aperture of the objective (and condenser). According to Abbe diffraction theory, the objective numerical aperture is determined by:

This tutorial explores how Airy disk sizes, at the limit of optical resolution, vary with changes in objective numerical aperture (NA) and illumination wavelength, and how these changes affect the resolution (r) of the objective (lower values for r indicate increasing resolution). The tutorial initializes with the Wavelength slider set to 528 nanometers in the green color region of the visible light spectrum. Also upon initialization, the virtual Numerical Aperture slider is set to a value of 0.16 and the two Airy patterns are separated by a distance (D) of 4.3 micrometers. Beneath the sliders is real-time calculation of the resolution according to Abbe diffraction theory that changes with adjustments to the sliders. Above the sliders is a simulated illumination cone that becomes wider or narrower as the numerical aperture is changed. The light cone size will increase with numerical aperture (at fixed wavelength) and produce a corresponding decrease in the size of the Airy disks (and an increase in resolution). A decrease in wavelength at fixed numerical aperture will result in a decrease in Airy pattern size.

Objects in the optical microscope that are either self-luminous or illuminated by a large-angle cone of light form Airy patterns at the intermediate image plane that are incoherent and do not interfere with each other. This allows the determination of the minimum separation distance between adjacent Airy patterns by examination of the total intensity distribution (the sum of intensities) when these patterns are closely spaced or overlapping. In the case of Airy patterns produced by coherent illumination, the minimum separation distance must be ascertained by adding the pattern amplitudes rather than their intensities.

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When the separation distance (D) between adjacent Airy patterns is greater than the central disk radius (r), the sum of the intensities yields two individual peaks. As the disks approach each other, the separation distance will reach a value equal to the central disk radius, a condition known as the Rayleigh criterion. At even closer approach, the separation distance is less than the central disk radius and the sum of the two peaks merges into a single peak. In the latter instance, the two Airy patterns are said not to be resolved.