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An innovative, highly sensitive receiver system for the Square Kilometre Array Mid radio telescope

Tan, G. H. (author)
Lehmensiek, R. (author)
Billade, Bhushan, 1982 (author)
Chalmers tekniska högskola,Chalmers University of Technology
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Caputa, Krzysztof (author)
National Research Council Canada
Gauffre, S. (author)
Université de Bordeaux,University of Bordeaux,Centre national de la recherche scientifique (CNRS)
Theron, I. P. (author)
Pantaleev, Miroslav, 1970 (author)
Chalmers tekniska högskola,Chalmers University of Technology
Ljusic, Z. (author)
National Research Council Canada
Quertier, B. (author)
Centre national de la recherche scientifique (CNRS),Université de Bordeaux,University of Bordeaux
Peens-Hough, A. (author)
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 (creator_code:org_t)
SPIE, 2018
2018
English.
In: Proceedings of SPIE - The International Society for Optical Engineering. - : SPIE. - 0277-786X .- 1996-756X. ; 9906
  • Conference paper (peer-reviewed)
Abstract Subject headings
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  • The Square Kilometre Array (SKA) Project is a global science and engineering project realizing the next-generation radio telescopes operating in the metre and centimetre wavelengths regions. This paper addresses design concepts of the broadband, exceptionally sensitive receivers and reflector antennas deployed in the SKA1-Mid radio telescope to be located in South Africa. SKA1-Mid (350 MHz -13.8 GHz with an option for an upper limit of similar to 24 GHz) will consist of 133 reflector antennas using an unblocked aperture, offset Gregorian configuration with an effective diameter of 15 m. Details on the unblocked aperture Gregorian antennas, low noise front ends and advanced direct digitization receivers, are provided from a system design perspective. The unblocked aperture results in increased aperture efficiency and lower side-lobe levels compared to a traditional on-axis configuration. The low side-lobe level reduces the noise contribution due to ground pick-up but also makes the antenna less susceptible to ground-based RFI sources. The addition of extra shielding on the sub-reflector provides a further reduction of ground pick-up. The optical design of the SKA1-Mid reflector antenna has been tweaked using advanced EM simulation tools in combination with sophisticated models for sky, atmospheric and ground noise contributions. This optimal antenna design in combination with very low noise, partially cryogenic, receivers and wide instantaneous bandwidth provide excellent receiving sensitivity in combination with instrumental flexibility to accommodate a wide range of astronomical observation modes.

Subject headings

TEKNIK OCH TEKNOLOGIER  -- Elektroteknik och elektronik -- Telekommunikation (hsv//swe)
ENGINEERING AND TECHNOLOGY  -- Electrical Engineering, Electronic Engineering, Information Engineering -- Telecommunications (hsv//eng)

Keyword

Square Kilometre Array
reflector antenna
receiver
optimisation methods
SKA
radio astronomy
radio telescope

Publication and Content Type

kon (subject category)
ref (subject category)

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