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Cryogenic 1.2 to 11...
Cryogenic 1.2 to 116 GHz Receiver for Large Arrays
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- Weinreb, Sander (författare)
- California Institute of Technology (Caltech)
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- Mani, Hamdi (författare)
- Arizona State University
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- Zhong, Weiye (författare)
- Shanghai Astronomical Observatory. Chinese Academy of Sciences,Shanghai Astronomical Observatory Chinese Academy of Sciences
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- Flygare, Jonas, 1988 (författare)
- Chalmers tekniska högskola,Chalmers University of Technology
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- Billade, Bhushan, 1982 (författare)
- Chalmers tekniska högskola,Chalmers University of Technology
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- Akgiray, Ahmed (författare)
- Özyeğin Üniversitesi,Özyeğin University
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Dong, Li (författare)
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(creator_code:org_t)
- Institution of Engineering and Technology, 2018
- 2018
- Engelska.
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Ingår i: IET Conference Publications. - : Institution of Engineering and Technology. ; 2018:CP741
- Relaterad länk:
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https://doi.org/10.1...
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https://research.cha...
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https://research.cha...
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Abstract
Ämnesord
Stäng
- Current and future large arrays for radio astronomy are compared and the Next Generation Very Large Array, ngVLA, is introduced. Receiver requirements are described and a 4-feed system covering 1.2 to 116 GHz, in a single vacuum cryogenic enclosure is presented followed by description of the reflector optics, the wide-band feeds, and the expected system performance
Ämnesord
- TEKNIK OCH TEKNOLOGIER -- Elektroteknik och elektronik -- Kommunikationssystem (hsv//swe)
- ENGINEERING AND TECHNOLOGY -- Electrical Engineering, Electronic Engineering, Information Engineering -- Communication Systems (hsv//eng)
- TEKNIK OCH TEKNOLOGIER -- Elektroteknik och elektronik (hsv//swe)
- ENGINEERING AND TECHNOLOGY -- Electrical Engineering, Electronic Engineering, Information Engineering (hsv//eng)
Nyckelord
- cryogenic
- radio astronomy
- low noise amplifiers
- QRFH
Publikations- och innehållstyp
- kon (ämneskategori)
- ref (ämneskategori)