Correlators ( Backend System )

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Presentation transcript:

Correlators ( Backend System ) ATNF Synthesis Imaging Workshop Correlators ( Backend System ) Warwick Wilson, ATNF.

An Aperture Synthesis Array Radiotelescope A collection of simple interferometers An array of N antennas Processed in pairs N(N-1)/2 pairs or baselines

- u,v in wavelengths

Complex Correlator Measures visibility or cross power ( complex ) Band limiting filter Cosine correlator 90 degree phase shift Sine correlator

Base-band Correlator - with fringe rotation Common Local Oscillator

Digital Correlator Sampler/digitiser - with fine delay control

Advantages of measuring the Cross Power Spectrum Reduces the effects of frequency smearing and provides more independent measurements on the u,v plane. (MFS) Allows measurement of any frequency dependence in the source, e.g. spectral lines. Provides an easy method of delay calibration. Provides means of removing interference.

Spectro-Correlator

Visibility / Cross Power Cross Power Spectrum -- Cross Correlation Function

Cross-correlation Spectro-Correlator Digital Cross-correlator Measure over a range of (positive and negative) delays

The ATCA Correlator A digital cross-correlator Bandwidths - 128 MHz to 4MHz Maximum sample rate - 256 Msamples/sec Processing elements - 8 Msamples/sec Parallel processing Large number of simple processing elements 2 bit quantisation

Parallel Processing in the ATCA Correlator Correlation function window in the lag domain - for maximum bandwidth

00 10 01 11 V=0

Samplers with coarse quantisation Bits Levels Efficiency 1 2 0.64 2 4 0.88