On the design of a correlator supersynthesis array

Details On the design of a correlator supersynthesis array On the design of a correlator supersynthesis array

Sep 1968

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1968apsi.conf...34m&link_type=abstract

1968 Antennas and Propagation Society International Symposium 6: p. 34-38

Astronomy and Astrophysics

Astronomy

Scientific paper

Recent developments in radio astronomy have pointed to the need of higher resolution and greater sensitivity in radio telescopes. Interferometers provide the easiest way to achieve high resolution. A variable-baseline two-element interferometer can measure all the spatial frequency components of the brightness distribution of a source, but the process is very slow. The process can be greatly speeded up by using a large number of antennas, connected in pairs as interferometers, and allowing the antennas to track the source as it moves. Such an array is called a correlator supersynthesis array.

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