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The Cambridge Interferometer was a radio t … The Cambridge Interferometer was a radio telescope interferometer built by Martin Ryle and Antony Hewish in the early 1950s to the west of Cambridge (between the Grange Road football ground and the current Cavendish Laboratory). The interferometer consisted of an array of 4 fixed elements to survey the sky. It produced the two Cambridge catalogues of radio sources (the 2C catalogue of radio sources at 81.5 MHz, and the 3C catalogue of radio sources at 159 MHz, building on the work of the Preliminary survey of the radio stars in the Northern Hemisphere at 45 MHz - 214 MHz using the 2-element Long Michelson Interferometer), discovering some of the most interesting astronomical objects known. The telescope was operated by the Radio Astronomy Group of Cambridge University. Martin Ryle and Antony Hewish received the Nobel Prize for Physics in 1974 for this and other related work.s in 1974 for this and other related work.
, 劍橋干涉儀是由馬丁·賴爾和安東尼·休伊什在1950年代早期於劍橋西區（在現在的格蘭奇 … 劍橋干涉儀是由馬丁·賴爾和安東尼·休伊什在1950年代早期於劍橋西區（在現在的格蘭奇道足球場與卡文迪許實驗室之間）建造的電波望遠鏡。這個干涉儀是包含4個固定元件的巡天陣列，它產生了兩份劍橋的無線電原目錄（以81.5MHz編製的2C無線電源表，和以159MHz編製的3C無線電源表。建築在45MHz-214MHz，使用2個元件的北半球電波星的初步調查（页面存档备份，存于互联网档案馆）），發現一些最有趣且有名的天體。這架望遠鏡由劍橋大學的操作。 馬丁·賴爾和安東尼·休伊什因為這件事和其他的工作獲得1974年的諾貝爾物理獎。作。 馬丁·賴爾和安東尼·休伊什因為這件事和其他的工作獲得1974年的諾貝爾物理獎。
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劍橋干涉儀是由馬丁·賴爾和安東尼·休伊什在1950年代早期於劍橋西區（在現在的格蘭奇 … 劍橋干涉儀是由馬丁·賴爾和安東尼·休伊什在1950年代早期於劍橋西區（在現在的格蘭奇道足球場與卡文迪許實驗室之間）建造的電波望遠鏡。這個干涉儀是包含4個固定元件的巡天陣列，它產生了兩份劍橋的無線電原目錄（以81.5MHz編製的2C無線電源表，和以159MHz編製的3C無線電源表。建築在45MHz-214MHz，使用2個元件的北半球電波星的初步調查（页面存档备份，存于互联网档案馆）），發現一些最有趣且有名的天體。這架望遠鏡由劍橋大學的操作。 馬丁·賴爾和安東尼·休伊什因為這件事和其他的工作獲得1974年的諾貝爾物理獎。作。 馬丁·賴爾和安東尼·休伊什因為這件事和其他的工作獲得1974年的諾貝爾物理獎。
, The Cambridge Interferometer was a radio t … The Cambridge Interferometer was a radio telescope interferometer built by Martin Ryle and Antony Hewish in the early 1950s to the west of Cambridge (between the Grange Road football ground and the current Cavendish Laboratory). The interferometer consisted of an array of 4 fixed elements to survey the sky. It produced the two Cambridge catalogues of radio sources (the 2C catalogue of radio sources at 81.5 MHz, and the 3C catalogue of radio sources at 159 MHz, building on the work of the Preliminary survey of the radio stars in the Northern Hemisphere at 45 MHz - 214 MHz using the 2-element Long Michelson Interferometer), discovering some of the most interesting astronomical objects known. The telescope was operated by the Radio Astronomy Group of Cambridge University.o Astronomy Group of Cambridge University.
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劍橋干涉儀
, Cambridge Interferometer
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