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  2. Astronomical optical interferometry - Wikipedia

    en.wikipedia.org/wiki/Astronomical_optical...

    A simple two-element optical interferometer. Light from two small telescopes (shown as lenses) is combined using beam splitters at detectors 1, 2, 3 and 4. The elements create a 1/4 wave delay in the light, allowing the phase and amplitude of the interference visibility to be measured, thus giving information about the shape of the light source.

  3. Interferometry - Wikipedia

    en.wikipedia.org/wiki/Interferometry

    Interferometry is a technique which uses the interference of superimposed waves to extract information. [1] Interferometry typically uses electromagnetic waves and is an important investigative technique in the fields of astronomy, fiber optics, engineering metrology, optical metrology, oceanography, seismology, spectroscopy (and its ...

  4. Rayleigh interferometer - Wikipedia

    en.wikipedia.org/wiki/Rayleigh_interferometer

    Rayleigh interferometer at the National Bureau of Standards. In optics, a Rayleigh interferometer is a type of interferometer which employs two beams of light from a single source.

  5. Astronomical interferometer - Wikipedia

    en.wikipedia.org/wiki/Astronomical_interferometer

    When using interferometry, a complex system of mirrors brings the light from the different telescopes to the astronomical instruments where it is combined and processed. This is technically demanding as the light paths must be kept equal to within 1/1000 mm (the same order as the wavelength of light) over distances of a few hundred metres.

  6. Michelson interferometer - Wikipedia

    en.wikipedia.org/wiki/Michelson_interferometer

    As shown in Fig. 3a and 3b, the observer has a direct view of mirror M 1 seen through the beam splitter, and sees a reflected image M' 2 of mirror M 2. The fringes can be interpreted as the result of interference between light coming from the two virtual images S' 1 and S' 2 of the original source S. The characteristics of the interference ...

  7. Common-path interferometer - Wikipedia

    en.wikipedia.org/wiki/Common-path_interferometer

    Lateral shearing interferometry is a self-referencing method of wavefront sensing. Instead of comparing a wavefront with a separate path reference wavefront, lateral shearing interferometry interferes a wavefront with a shifted version of itself. As a result, it is sensitive to the slope of a wavefront, not the wavefront shape per se. The ...

  8. SU (1,1) interferometry - Wikipedia

    en.wikipedia.org/wiki/SU(1,1)_interferometry

    SU(1,1) interferometry is a technique that uses parametric amplification for splitting and mixing of electromagnetic waves for precise estimation of phase change and achieves the Heisenberg limit of sensitivity with fewer optical elements than conventional interferometric techniques.

  9. Category:Interferometry - Wikipedia

    en.wikipedia.org/wiki/Category:Interferometry

    Seismic interferometry; Self-mixing interferometry; Single-shot multi-contrast X-ray imaging; Speckle interferometry; Spectral interferometry; Spectral phase interferometry for direct electric-field reconstruction; SU(1,1) interferometry