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  2. List of radio telescopes - Wikipedia

    en.wikipedia.org/wiki/List_of_radio_telescopes

    38-element radio telescope interferometer working in the frequency range of 1.2–6.0 GHz. The final baseline will be 2.27 km in the East-West and 1.17 km in the South directions, respectively. This instrument will obtain radio images from the sun with a spatial resolution ≈4x6 arc seconds.

  3. AN/APG-78 Longbow - Wikipedia

    en.wikipedia.org/wiki/AN/APG-78_Longbow

    The AN/APG-78 Longbow is a millimeter-wave fire-control radar (FCR) target acquisition system and the Radar Frequency Interferometer (RFI), which are housed in a dome located above the main rotor. [4] [5] The radome's raised position enables target detection while the helicopter is behind obstacles (e.g. terrain, trees or buildings). The APG-78 ...

  4. Martin Ryle - Wikipedia

    en.wikipedia.org/wiki/Martin_Ryle

    In 1946 Ryle built the first multi-element astronomical radio interferometer. [10] Ryle guided the Cambridge radio astronomy group in the production of several important radio source catalogues. One such catalogue, the Third Cambridge Catalogue of Radio Sources (3C) in 1959 helped lead to the discovery of the first quasi-stellar object .

  5. List of military electronics of the United States - Wikipedia

    en.wikipedia.org/wiki/List_of_military...

    Rifleman Radio is a handheld, intra-squad tactical radio: Thales Group, General Dynamics: AN/PRC-155: Joint Tactical Radio System (JTRS) Handheld, Manpack & Small Form Fit (HMS) General Dynamics: AN/PRC-158: Falcon® IV Multi-channel Manpack (MCMP) radio: L3Harris Technologies: AN/PRC-159: Falcon® III wideband team radio: L3Harris Technologies ...

  6. Arcminute Microkelvin Imager - Wikipedia

    en.wikipedia.org/wiki/Arcminute_Microkelvin_Imager

    The Arcminute Microkelvin Imager (AMI) consists of a pair of interferometric radio telescopes - the Small and Large Arrays - located at the Mullard Radio Astronomy Observatory near Cambridge. AMI was designed, built and is operated by the Cavendish Astrophysics Group .

  7. 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 ...

  8. Zygo Corporation - Wikipedia

    en.wikipedia.org/wiki/Zygo_Corporation

    Zygo Corporation, or simply Zygo, is a manufacturer headquartered at Middlefield, Connecticut, that specializes in optical systems and equipment.Their metrology product lines include 3D measuring microscopes using coherence scanning interferometry, laser Fizeau interferometers for testing optical components, laser displacement interferometers, and heterodyne optical encoders for stage position ...

  9. 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.