1970
DOI: 10.1049/piee.1970.0284
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Wideband multiplier correlator

Abstract: Apparatus to measure the correlation between two wideband (10-100 MHz) noise signals has been developed for the stellar intensity interferometer at the Narrabri observatory. This instrument is used to measure the angular diameters of stars in the range 0 • 01 -0• 000\" of arc, with an accuracy within about 5 % To achieve this precision with the low signal/noise ratio of an intensity interferometer, it is necessary to integrate and average the data for periods up to lOOh, which may involve observations spread o… Show more

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Cited by 5 publications
(3 citation statements)
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“…For delays up to about 1 s, lengths of coaxial cable or optical fiber have been used. The design of analog multiplying circuits for correlators has been discussed by Allen and Frater (1970). An example of a broadband analog correlator is described by Padin (1994).…”
Section: Delay and Correlator Subsystemsmentioning
confidence: 99%
“…For delays up to about 1 s, lengths of coaxial cable or optical fiber have been used. The design of analog multiplying circuits for correlators has been discussed by Allen and Frater (1970). An example of a broadband analog correlator is described by Padin (1994).…”
Section: Delay and Correlator Subsystemsmentioning
confidence: 99%
“…In particular, a transistorized version of the linear multiplier, a key component of the correlator, was developed by L.R. Allen and R.H. Frater (Allen & Frater 1970). The resulting improvement in the stability of the correlator was vital for the observations of fainter stars towards the end of the stellar programme.…”
Section: The Stellar Programmementioning
confidence: 99%
“…Hanbury Brown and Twiss [7] and later by Allen and Frater [8]. We adopted their approach with newer electronics and detectors to obtain better stability and greater bandwidth.…”
Section: Construction Of the Interferometermentioning
confidence: 99%