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  2. File:LIGO schematic (multilang).svg - Wikipedia

    en.wikipedia.org/wiki/File:LIGO_schematic_(multi...

    English: Concept of LIGO: A schematic diagram of a laser interferometer with light storage arms. ... This image is a derivative work of the following images:

  3. LIGO - Wikipedia

    en.wikipedia.org/wiki/LIGO

    The Laser Interferometer Gravitational-Wave Observatory (LIGO) is a large-scale physics experiment and observatory designed to detect cosmic gravitational waves and to develop gravitational-wave observations as an astronomical tool. [1]

  4. Interferometry - Wikipedia

    en.wikipedia.org/wiki/Interferometry

    The Laser Interferometer Gravitational-Wave Observatory (LIGO) uses two 4-km Michelson–Fabry–Pérot interferometers for the detection of gravitational waves. [38] In this application, the Fabry–Pérot cavity is used to store photons for almost a millisecond while they bounce up and down between the mirrors.

  5. Electronic speckle pattern interferometry - Wikipedia

    en.wikipedia.org/wiki/Electronic_speckle_pattern...

    Electronic speckle pattern interferometry (ESPI), [1] also known as TV holography, is a technique that uses laser light, together with video detection, recording and processing, to visualise static and dynamic displacements of components with optically rough surfaces. The visualisation is in the form of fringes on the image, where each fringe ...

  6. Michelson interferometer - Wikipedia

    en.wikipedia.org/wiki/Michelson_interferometer

    The "LUPI" is a Twyman–Green interferometer that uses a coherent laser light source. The high coherence length of a laser allows unequal path lengths in the test and reference arms and permits economical use of the Twyman–Green configuration in testing large optical components. A similar scheme has been used by Tajammal M in his PhD thesis ...

  7. Sagnac effect - Wikipedia

    en.wikipedia.org/wiki/Sagnac_effect

    The result is an interferometer that exhibits the stability of the Sagnac topology while being insensitive to rotation. [46] The Laser Interferometer Gravitational-Wave Observatory (LIGO) consisted of two 4-km Michelson–Fabry–Pérot interferometers, and operated at a power level of about 100 watts of laser power at the beam splitter. After ...

  8. N-slit interferometer - Wikipedia

    en.wikipedia.org/wiki/N-slit_interferometer

    The original application of the N-slit laser interferometer was interferometric imaging. [ 6 ] [ 10 ] [ 14 ] In particular, the one dimensionally expanded laser beam (with a cross section 25-50 mm wide by 10-25 μm high) was used to illuminate imaging surfaces (such as silver-halide films) to measure the microscopic density of the illuminated ...

  9. List of types of interferometers - Wikipedia

    en.wikipedia.org/wiki/List_of_types_of...

    Bath interferometer (common path) Cyclic interferometer; Diffraction-grating interferometer (white light) Double-slit interferometer; Dual-polarization interferometry; Fabry–Pérot interferometer; Fizeau interferometer; Fourier-transform interferometer; Fresnel interferometer (e.g. Fresnel biprism, Fresnel mirror or Lloyd's mirror)