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Owens Valley Solar Array : ウィキペディア英語版 | Owens Valley Solar Array
The Owens Valley Solar Array (OVSA) is an astronomical radio telescope array with main interests in studying the physics of the Sun. The instruments of the observatory are designed and employed specifically for studying the activities and phenomena of our solar system's sun. Other solar dedicated instruments operated on the site include the Solar Radio Burst Locator (SRBL), the FASR Subsystem Testbed (FST), and the Korean SRBL (KSRBL). The OVSA is operated by the New Jersey Institute of Technology (NJIT), which also operates the Big Bear Solar Observatory. The OVSA is located at Owens Valley Radio Observatory (OVRO), near Big Pine, California. ==About the radio telescope array==
The facility was built by the California Institute of Technology in 1982. Management of the observatory was transferred to NJIT in 1997. At the time of transfer the site had 5 antennas including two 27-m antennas (originally used to study radio galaxies), and three 1.8-m antennas. Two more 1.8-m antennas were added later. Funding comes from the National Science Foundation and NASA.
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