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  2. Interferometry - Wikipedia

    en.wikipedia.org/wiki/Interferometry

    Interferometry is used in radio astronomy, with timing offsets of D sin θ. In physics, one of the most important experiments of the late 19th century was the famous "failed experiment" of Michelson and Morley which provided evidence for special relativity.

  3. Astronomical interferometer - Wikipedia

    en.wikipedia.org/wiki/Astronomical_interferometer

    An astronomical interferometer or telescope array is a set of separate telescopes, mirror segments, or radio telescope antennas that work together as a single telescope to provide higher resolution images of astronomical objects such as stars, nebulas and galaxies by means of interferometry.

  4. Astronomical optical interferometry - Wikipedia

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

    In optical astronomy, interferometry is used to combine signals from two or more telescopes to obtain measurements with higher resolution than could be obtained with either telescopes individually. This technique is the basis for astronomical interferometer arrays, which can make measurements of very small astronomical objects if the telescopes ...

  5. Michelson interferometer - Wikipedia

    en.wikipedia.org/wiki/Michelson_interferometer

    Fig. 7 illustrates use of a Michelson interferometer as a tunable narrow band filter to create dopplergrams of the Sun's surface. When used as a tunable narrow band filter, Michelson interferometers exhibit a number of advantages and disadvantages when compared with competing technologies such as Fabry–Pérot interferometers or Lyot filters ...

  6. Very-long-baseline interferometry - Wikipedia

    en.wikipedia.org/wiki/Very-long-baseline...

    Very-long-baseline interferometry (VLBI) is a type of astronomical interferometry used in radio astronomy. In VLBI a signal from an astronomical radio source, such as a quasar, is collected at multiple radio telescopes on Earth or in space. The distance between the radio telescopes is then calculated using the time difference between the ...

  7. 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]

  8. Astrometry - Wikipedia

    en.wikipedia.org/wiki/Astrometry

    Illustration of the use of interferometry in the optical wavelength range to determine precise positions of stars. Courtesy NASA/JPL-Caltech. Astrometry is a branch of astronomy that involves precise measurements of the positions and movements of stars and other celestial bodies.

  9. List of types of interferometers - Wikipedia

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

    An interferometer is a device for extracting information from the superposition of multiple waves. Field and linear interferometers. Air-wedge shearing interferometer;