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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 , traveling in a medium with refractive index and converging to a spot with half-angle will have a minimum resolvable distance of

  3. Dawes' limit - Wikipedia

    en.wikipedia.org/wiki/Dawes'_limit

    diffraction pattern matching Dawes' limit. Dawes' limit is a formula to express the maximum resolving power of a microscope or telescope. [1] It is so named after its discoverer, William Rutter Dawes, [2] although it is also credited to Lord Rayleigh. The formula takes different forms depending on the units.

  4. Scherzer's theorem - Wikipedia

    en.wikipedia.org/wiki/Scherzer's_theorem

    Due to the inevitability of spherical aberration, there is a practical, but not a fundamental, limit to the resolving power of the electron microscope." [ 1 ] The resolution limit provided by Scherzer's theorem can be overcome by breaking one of the above mentioned three conditions.

  5. Optical resolution - Wikipedia

    en.wikipedia.org/wiki/Optical_resolution

    Also common in the microscopy literature is a formula for resolution that treats the above-mentioned concerns about contrast differently. [2] The resolution predicted by this formula is proportional to the Rayleigh-based formula, differing by about 20%. For estimating theoretical resolution, it may be adequate.

  6. Spatial cutoff frequency - Wikipedia

    en.wikipedia.org/wiki/Spatial_cutoff_frequency

    High-resolution black-and-white film is capable of resolving details on the film as small as 3 micrometers or smaller, thus its cutoff frequency is about 150 cycles/millimeter. So, the telescope's optical resolution is about twice that of high-resolution film, and a crisp, sharp picture would result (provided focus is perfect and atmospheric ...

  7. Aberration-Corrected Transmission Electron Microscopy

    en.wikipedia.org/wiki/Aberration-Corrected...

    He investigated the need for a brighter electron source in the microscope, positing that cold field emission guns would be feasible. [9] Through this and other iterations, Crewe was able to improve the resolution of the STEM from 30 Ångstroms (Å) down to 2.5 Å. [10] Crewe's work made it possible to visualize individual atoms for the first ...

  8. Contrast transfer function - Wikipedia

    en.wikipedia.org/wiki/Contrast_transfer_function

    The first time the function crosses the x-axis is called the point resolution; To maximize phase signal, it is generally better to use imaging conditions that push the point resolution to higher spatial frequencies; When the function is negative, that represents positive phase contrast, leading to a bright background, with dark atomic features

  9. Angular resolution - Wikipedia

    en.wikipedia.org/wiki/Angular_resolution

    In a dry objective or condenser, this gives a maximum NA of 0.95. In a high-resolution oil immersion lens, the maximum NA is typically 1.45, when using immersion oil with a refractive index of 1.52. Due to these limitations, the resolution limit of a light microscope using visible light is about 200 nm.