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  2. Diffraction-limited system - Wikipedia

    en.wikipedia.org/wiki/Diffraction-limited_system

    The observation of sub-wavelength structures with microscopes is difficult because of the Abbe diffraction limit. Ernst Abbe found in 1873, [ 2 ] and expressed as a formula in 1882, [ 3 ] that light with wavelength λ {\displaystyle \lambda } , traveling in a medium with refractive index n {\displaystyle n} and converging to a spot with half ...

  3. Angular resolution - Wikipedia

    en.wikipedia.org/wiki/Angular_resolution

    The result, θ = 4.56/D, with D in inches and θ in arcseconds, is slightly narrower than calculated with the Rayleigh criterion. A calculation using Airy discs as point spread function shows that at Dawes' limit there is a 5% dip between the two maxima, whereas at Rayleigh's criterion there is a 26.3% dip. [3]

  4. Rayleigh criterion - Wikipedia

    en.wikipedia.org/wiki/Rayleigh_criterion

    Rayleigh criterion may refer to: Angular resolution § The Rayleigh criterion, optical angular resolution; Taylor–Couette flow § Rayleigh's criterion, instability ...

  5. Sparrow's resolution limit - Wikipedia

    en.wikipedia.org/wiki/Sparrow's_resolution_limit

    Sparrow's resolution limit is nearly equivalent to the theoretical diffraction limit of resolution, the wavelength of light divided by the aperture diameter, and about 20% smaller than the Rayleigh limit. For example, in a 200 mm (eight-inch) telescope, Rayleigh's resolution limit is 0.69 arc seconds, Sparrow's resolution limit is 0.54 arc seconds.

  6. Optical resolution - Wikipedia

    en.wikipedia.org/wiki/Optical_resolution

    The ability of a lens to resolve detail is usually determined by the quality of the lens, but is ultimately limited by diffraction.Light coming from a point source in the object diffracts through the lens aperture such that it forms a diffraction pattern in the image, which has a central spot and surrounding bright rings, separated by dark nulls; this pattern is known as an Airy pattern, and ...

  7. Airy disk - Wikipedia

    en.wikipedia.org/wiki/Airy_disk

    The Rayleigh criterion for barely resolving two objects that are point sources of light, such as stars seen through a telescope, is that the center of the Airy disk for the first object occurs at the first minimum of the Airy disk of the second. This means that the angular resolution of a diffraction-limited system is given by the same formulae.

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  9. Near-field scanning optical microscope - Wikipedia

    en.wikipedia.org/wiki/Near-field_scanning...

    Thus, the resolution limit is usually around λ 0 /2 for conventional optical microscopy. [17] This treatment takes into account only the light diffracted into the far-field that propagates without any restrictions. NSOM makes use of evanescent or non propagating fields that exist only near the surface of the object.