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  2. Interferometry - Wikipedia

    en.wikipedia.org/wiki/Interferometry

    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 applications to chemistry), quantum mechanics, nuclear and particle physics, plasma physics, biomolecular interactions ...

  3. LIGO - Wikipedia

    en.wikipedia.org/wiki/LIGO

    In 1962, M. E. Gertsenshtein and V. I. Pustovoit published the very first paper describing the principles for using interferometers for the detection of very long wavelength gravitational waves. [63] The authors argued that by using interferometers the sensitivity can be 10 7 to 10 10 times better than by using electromechanical experiments.

  4. 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 ...

  5. 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. Македонски: Шема на ласерскиот интеферометар LIGO за забележување на гравитациски бранови .

  6. Fourier-transform infrared spectroscopy - Wikipedia

    en.wikipedia.org/wiki/Fourier-transform_infrared...

    Although instrument design has become more sophisticated, the basic principles remain the same. Nowadays, the moving mirror of the interferometer moves at a constant velocity, and sampling of the interferogram is triggered by finding zero-crossings in the fringes of a secondary interferometer lit by a helium–neon laser.

  7. Fabry–Pérot interferometer - Wikipedia

    en.wikipedia.org/wiki/Fabry–Pérot_interferometer

    This principle is used by detectors such as LIGO and Virgo, which consist of a Michelson interferometer with a Fabry–Pérot cavity with a length of several kilometers in both arms. Smaller cavities, usually called mode cleaners , are used for spatial filtering and frequency stabilization of the main laser.

  8. Fizeau interferometer - Wikipedia

    en.wikipedia.org/wiki/Fizeau_interferometer

    Fizeau interferometers are commonly used for measuring the shape of an optical surface: Typically, a fabricated lens or mirror is compared to a reference piece having the desired shape. In Fig. 1, the Fizeau interferometer is shown as it might be set up to test an optical flat. A precisely figured reference flat is placed on top of the flat ...

  9. Laser Doppler vibrometer - Wikipedia

    en.wikipedia.org/wiki/Laser_Doppler_vibrometer

    A vibrometer is generally a two beam laser interferometer that measures the frequency (or phase) difference between an internal reference beam and a test beam. The most common type of laser in an LDV is the helium–neon laser, although laser diodes, fiber lasers, and Nd:YAG lasers are also used.