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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. Very Long Baseline Array - Wikipedia

    en.wikipedia.org/wiki/Very_Long_Baseline_Array

    These ten radio antennas work together as an array that forms the longest system in the world that uses very long baseline interferometry. The longest baseline available in this interferometer is about 8,611 kilometers (5,351 mi). [2] The construction of the VLBA began in February 1986 and it was completed in May 1993.

  4. Very Large Array - Wikipedia

    en.wikipedia.org/wiki/Very_Large_Array

    The VLA comprises twenty-eight 25-meter radio telescopes (twenty-seven of which are operational while one is always rotating through maintenance) deployed in a Y-shaped array and all the equipment, instrumentation, and computing power to function as an interferometer.

  5. Northern Extended Millimeter Array - Wikipedia

    en.wikipedia.org/wiki/Northern_Extended...

    The Northern Extended Millimeter Array (NOEMA) is one of the largest astronomical facilities on European ground and the most powerful radio telescope in the Northern Hemisphere operating at millimeter wavelengths. It consists of a large array of twelve 15-meter antennas that can spread over distances of up to 1.7 kilometers, working together as ...

  6. Owens Valley Solar Array - Wikipedia

    en.wikipedia.org/wiki/Owens_Valley_Solar_Array

    The radio interferometer continued to be expanded with larger and better radio telescopes. In 1979, the two dishes were retired from the radio interferometer and were repurposed to be used as an array dedicated to solar observation. The Owens Valley Solar Array was established with the two dish interferometer under the direction of professor ...

  7. 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 .

  8. Green Bank Observatory - Wikipedia

    en.wikipedia.org/wiki/Green_Bank_Observatory

    The Green Bank Observatory (previously National Radio Astronomy Observatory, Green Bank) is an astronomical observatory located in the National Radio Quiet Zone in Green Bank, West Virginia, U.S. It is the operator of the Robert C. Byrd Green Bank Telescope , the world's largest fully steerable radio telescope .

  9. Green Bank Telescope - Wikipedia

    en.wikipedia.org/wiki/Green_Bank_Telescope

    The Robert C. Byrd Green Bank Telescope (GBT) in Green Bank, West Virginia, US is the world's largest fully steerable radio telescope, [1] surpassing the Effelsberg 100-m Radio Telescope in Germany. [2] The Green Bank site was part of the National Radio Astronomy Observatory (NRAO) until September 30, 2016.