Hostname: page-component-78c5997874-t5tsf Total loading time: 0 Render date: 2024-11-18T01:22:34.231Z Has data issue: false hasContentIssue false

A Proposed Correlator Backend for the Culgoora Radioheliograph

Published online by Cambridge University Press:  25 April 2016

D. J. McLean
Affiliation:
Division of Radiopnysics, CSIRO, Sydney
M. Beard
Affiliation:
Division of Radiopnysics, CSIRO, Sydney
A. Bos
Affiliation:
Division of Radiopnysics, CSIRO, Sydney

Extract

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.

Type
Contributions
Copyright
Copyright © Astronomical Society of Australia 1979

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

Frater, R.H., Astron. Astrophys., 68, 397 (1978).Google Scholar
Frater, R.H., and Skellern, D.J., Astron. Astrophys., 68, 391 (1978).Google Scholar
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.Google Scholar
Read, R.B., Astrophys. J., 138, 1 (1963).CrossRefGoogle Scholar
Sheridan, K.V., Labrum, N.R., and Payten, W.J., Proc. IEEE, 61, 1312 (1973).Google Scholar
Swenson, G.W. Jr., and Mathur, N.C., Proc. Inst. Radio Electron. Eng. (Aust.), 28, 370 (1967).Google Scholar
Wild, J.P. (Ed.), Proc. Inst. Radio Electron. Eng. (Aust.), 28, 277 (1967).Google Scholar