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A Proposed Correlator Backend for the Culgoora Radioheliograph

  • D. J. McLean (a1), M. Beard (a1) and A. Bos (a1)

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The Culgoora radioheliograph was designed in the early 1960s and commissioned in 1967. Since then there have been dramatic increases in the speed and versatility of digital integrated-circuit devices, and also a marked fall in their cost. It is now possible to replace the original signal processing electronics with equipment, based on modern digital technology, which will significantly enhance the performance of this radio telescope for solar and cosmic radio observations at metre wavelengths.

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References

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Frater, R.H., Astron. Astrophys., 68, 397 (1978).
Frater, R.H., and Skellern, D.J., Astron. Astrophys., 68, 391 (1978).
McLean, D.J., A proposed correlator back-end for the Culgoora radioheliograph. Proc. IAU/URSI Colloquium ‘Formation of images from spatial coherence functions in astronomy’, held Groningen, Aug. 1978.
Read, R.B., Astrophys. J., 138, 1 (1963).
Sheridan, K.V., Labrum, N.R., and Payten, W.J., Proc. IEEE, 61, 1312 (1973).
Swenson, G.W. Jr., and Mathur, N.C., Proc. Inst. Radio Electron. Eng. (Aust.), 28, 370 (1967).
Wild, J.P. (Ed.), Proc. Inst. Radio Electron. Eng. (Aust.), 28, 277 (1967).

A Proposed Correlator Backend for the Culgoora Radioheliograph

  • D. J. McLean (a1), M. Beard (a1) and A. Bos (a1)

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