3 July 2000 Full-sampling array feeds for radio telescopes
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Proceedings Volume 4015, Radio Telescopes; (2000); doi: 10.1117/12.390425
Event: Astronomical Telescopes and Instrumentation, 2000, Munich, Germany
Abstract
Phased array feeds offer the possibility of more efficient use of large radio astronomy reflector antennas by providing more closely spaced beams over a wide field of view and higher aperture efficiency in each beam than have been realized with horn feeds. This paper examines the array design constraints imposed by complete sampling of the fields near the reflector focus. In particular, array element spacing must be less than 1 (lambda) for large F/D reflectors and less than about 0.7 (lambda) for F/D < 0.5. This rules out conventional horns as array elements and sets a limit on the array bandwidth. The receive-only case of radio astronomy permits the use of number of signal combining techniques that do not degrade system sensitivity. Because practical arrays are of finite extent, and unwanted noise from the antenna surroundings is largely coherent between the elements, neither field conjugate nor maximal-ratio diversity methods of array weight optimization can be used. A modified form of field matching is a good starting approximation, however. Correction of reflector errors is examined briefly.
© (2000) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
J. Richard Fisher, Richard F. Bradley, "Full-sampling array feeds for radio telescopes", Proc. SPIE 4015, Radio Telescopes, (3 July 2000); doi: 10.1117/12.390425; https://doi.org/10.1117/12.390425
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KEYWORDS
Reflectors

Antennas

Phased arrays

Radio astronomy

Monochromatic aberrations

Signal processing

Convolution

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